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The Project Gutenberg eBook of Geology, Vol. 1 [of 3]
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Title: Geology, Vol. 1 [of 3]
Geologic processes and their results
Author: Thomas C. Chamberlin
Rollin D. Salisbury
Release date: August 27, 2024 [eBook #74316]
Language: English
Original publication: New York: Henry Holt and Company, 1906
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Credits: Peter Becker, Robert Tonsing, and the Online Distributed
Proofreading Team at https://www.pgdp.net (This file was
produced from images generously made available by The
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*** START OF THE PROJECT GUTENBERG EBOOK GEOLOGY,
VOL. 1 [OF 3] ***
This eBook is for the use of anyone anywhere in the United States and
most other parts of the world at no cost and with almost no restrictions
whatsoever. You may copy it, give it away or re-use it under the terms
of the Project Gutenberg License included with this eBook or online at
www.gutenberg.org. If you are not located in the United States, you
will have to check the laws of the country where you are located
before using this eBook.
Title: Geology, Vol. 1 [of 3]
Geologic processes and their results
Author: Thomas C. Chamberlin
Rollin D. Salisbury
Release date: August 27, 2024 [eBook #74316]
Language: English
Original publication: New York: Henry Holt and Company, 1906
Other information and formats: www.gutenberg.org/ebooks/74316
Credits: Peter Becker, Robert Tonsing, and the Online Distributed
Proofreading Team at https://www.pgdp.net (This file was
produced from images generously made available by The
Internet Archive)
*** START OF THE PROJECT GUTENBERG EBOOK GEOLOGY,
VOL. 1 [OF 3] ***
Page 4
AMERICAN SCIENCE SERIES—ADVANCED COURSE
GEOLOGY
BY
THOMAS C. CHAMBERLIN AND ROLLIN D. SALISBURY
Heads of the Departments of Geology and Geography, University of Chicago
Members of the United States Geological Survey
Editors of the Journal of Geology
IN THREE VOLUMES
VOL. I.—GEOLOGIC PROCESSES AND THEIR RESULTS
SECOND EDITION, REVISED
NEW YORK
HENRY HOLT AND COMPANY
1909
GEOLOGY
BY
THOMAS C. CHAMBERLIN AND ROLLIN D. SALISBURY
Heads of the Departments of Geology and Geography, University of Chicago
Members of the United States Geological Survey
Editors of the Journal of Geology
IN THREE VOLUMES
VOL. I.—GEOLOGIC PROCESSES AND THEIR RESULTS
SECOND EDITION, REVISED
NEW YORK
HENRY HOLT AND COMPANY
1909
Page 5
Copyright, 1904,
BY
HENRY HOLT AND COMPANY
PRINTED IN THE U. S. A.
BY
HENRY HOLT AND COMPANY
PRINTED IN THE U. S. A.
Page 6
PREFACE.
In the preparation of this work it has been the purpose of the authors to
present an outline of the salient features of geology, as now developed,
encumbered as little as possible by technicalities and details whose bearings
on the general theme are unimportant. In common with most writers of text-
books on geology, the authors believe that the subject is best approached by
a study of the forces and processes now in operation, and of the results
which these forces and processes are now bringing about. Such study
necessarily involves a consideration of the principles which govern the
activities of geologic agencies. These topics are presented in Volume I, and
prepare the way for the study of the history of past ages, which is outlined
in Volume II.
The general plan of the work has been determined by the experience of
the authors as instructors. Little emphasis is laid on the commonly
recognized subdivisions of the science, such as dynamic geology,
stratigraphic geology, physiographic geology, etc. The treatment proceeds
rather from the point of view that the science is a unit, that its one theme is
the history of the earth, and that the discussions of dynamic geology,
physiographic geology, etc., apart from their historical bearing, lose much
of their significance and interest. The effort has, therefore, been to
emphasize the historical element, even in the discussion of special themes,
such as the work of rivers, the work of snow and ice, and the origin and
descent of rocks. This does not mean that phases of geology other than
historical have been neglected, but it means that an effort has been made to
give a historical cast to all phases of the subject, so far as the topics permit.
Throughout the work the central purpose has been not merely to set forth
the present status of knowledge, but to present it in such a way that the
student will be introduced to the methods and spirit of the science, led to a
sympathetic interest in its progress, and prepared to receive intelligently,
and to welcome cordially, its future advances. Where practicable, the text
has been so shaped that the student may follow the steps which have led to
In the preparation of this work it has been the purpose of the authors to
present an outline of the salient features of geology, as now developed,
encumbered as little as possible by technicalities and details whose bearings
on the general theme are unimportant. In common with most writers of text-
books on geology, the authors believe that the subject is best approached by
a study of the forces and processes now in operation, and of the results
which these forces and processes are now bringing about. Such study
necessarily involves a consideration of the principles which govern the
activities of geologic agencies. These topics are presented in Volume I, and
prepare the way for the study of the history of past ages, which is outlined
in Volume II.
The general plan of the work has been determined by the experience of
the authors as instructors. Little emphasis is laid on the commonly
recognized subdivisions of the science, such as dynamic geology,
stratigraphic geology, physiographic geology, etc. The treatment proceeds
rather from the point of view that the science is a unit, that its one theme is
the history of the earth, and that the discussions of dynamic geology,
physiographic geology, etc., apart from their historical bearing, lose much
of their significance and interest. The effort has, therefore, been to
emphasize the historical element, even in the discussion of special themes,
such as the work of rivers, the work of snow and ice, and the origin and
descent of rocks. This does not mean that phases of geology other than
historical have been neglected, but it means that an effort has been made to
give a historical cast to all phases of the subject, so far as the topics permit.
Throughout the work the central purpose has been not merely to set forth
the present status of knowledge, but to present it in such a way that the
student will be introduced to the methods and spirit of the science, led to a
sympathetic interest in its progress, and prepared to receive intelligently,
and to welcome cordially, its future advances. Where practicable, the text
has been so shaped that the student may follow the steps which have led to
Page 7
present conclusions. To this end the working methods of the practical
geologist have been implied as frequently as practicable. To this end also
there has been frankness of statement relative to the limitations of
knowledge and the uncertainty of many tentative conclusions. In these and
in other respects, the purpose has been to take the student into the fraternity
of geologists, and to reveal to him the true state of the development of the
science, giving an accurate and proportionate view of the positive
knowledge attained, of the problems yet unsolved, or but partially solved,
and of solutions still to be attained.
The theoretical and interpretative elements which enter into the general
conceptions of geology have been freely used, because they are regarded as
an essential part of the evolution of the science, because they often help to
clear and complete conceptions, and because they stimulate thought. The
aim has been, however, to characterize hypothetical elements as such, and
to avoid confusing the interpretations based on hypothesis, with the
statements of fact and established doctrines. Especial care has been taken to
recognize the uncertain nature of prevalent interpretations when they are
dependent on unverified hypotheses, especially if this dependence is likely
to be overlooked. If this shall seem to give prominence to the hypothetical
element, it should also be regarded as giving so much the more emphasis to
that which is really trustworthy, in that it sets forth more frankly that which
is doubtful. Hypothetical and unsolved problems have been treated, so far
as practicable, on the multiple basis; that is, alternative hypotheses and
alternative interpretations are frequently presented where knowledge does
not warrant positive conclusions.
In many cases the topics discussed will be found to be presented in ways
differing widely from those which have become familiar. In some cases,
fundamentally new conceptions of familiar subjects are involved; in others,
topics not usually discussed in text-books are stated with some fullness; and
in still others, the emphasis is laid on points which have not commonly
been brought into prominence. Whether the authors have been wise in
departing to this extent from beaten paths, the users of the volumes must
decide.
The work is intended primarily for mature students, and is designed to
furnish the basis for a year’s work in the later part of the college course. By
judicious selection of material to be presented and omitted, the volumes
geologist have been implied as frequently as practicable. To this end also
there has been frankness of statement relative to the limitations of
knowledge and the uncertainty of many tentative conclusions. In these and
in other respects, the purpose has been to take the student into the fraternity
of geologists, and to reveal to him the true state of the development of the
science, giving an accurate and proportionate view of the positive
knowledge attained, of the problems yet unsolved, or but partially solved,
and of solutions still to be attained.
The theoretical and interpretative elements which enter into the general
conceptions of geology have been freely used, because they are regarded as
an essential part of the evolution of the science, because they often help to
clear and complete conceptions, and because they stimulate thought. The
aim has been, however, to characterize hypothetical elements as such, and
to avoid confusing the interpretations based on hypothesis, with the
statements of fact and established doctrines. Especial care has been taken to
recognize the uncertain nature of prevalent interpretations when they are
dependent on unverified hypotheses, especially if this dependence is likely
to be overlooked. If this shall seem to give prominence to the hypothetical
element, it should also be regarded as giving so much the more emphasis to
that which is really trustworthy, in that it sets forth more frankly that which
is doubtful. Hypothetical and unsolved problems have been treated, so far
as practicable, on the multiple basis; that is, alternative hypotheses and
alternative interpretations are frequently presented where knowledge does
not warrant positive conclusions.
In many cases the topics discussed will be found to be presented in ways
differing widely from those which have become familiar. In some cases,
fundamentally new conceptions of familiar subjects are involved; in others,
topics not usually discussed in text-books are stated with some fullness; and
in still others, the emphasis is laid on points which have not commonly
been brought into prominence. Whether the authors have been wise in
departing to this extent from beaten paths, the users of the volumes must
decide.
The work is intended primarily for mature students, and is designed to
furnish the basis for a year’s work in the later part of the college course. By
judicious selection of material to be presented and omitted, the volumes
Page 8
will be found useful for briefer courses, and by the use of the numerous
references to the fuller discussions of special treatises, they may be made
the basis for more extended courses than are commonly given in
undergraduate work. The attempt has also been made to make the volumes
readable, in the belief that many persons not in colleges or universities will
be interested in following a connected account of the earth’s history, and of
the means by which that history is recorded and read. Antecedent
elementary courses in geology will not be necessary to the use of these
volumes, though such courses may be helpful.
The arrangement of themes adopted is such as to bring to the fore
processes with which all students are immediately in contact, and which are
available for study at all seats of learning. The commoner geologic agents,
such as the atmosphere and running water, have been elaborated somewhat
more fully than is customary, and the common rather than the exceptional
phases of the work of these agents have been emphasized, both because of
their greater importance and their universal availability. The text has been
so shaped as to suggest field work in connection with these topics
especially, since work of this sort is everywhere possible.
After the preliminary outline, which is intended to give some idea of the
scope of the science, and of its salient features, and to show the relations of
the special subjects which follow, the order of treatment is such as to pass
from the commoner and more readily apprehended portions of the subject to
those which are less readily accessible and more obscure. Following the
same general conception, the treatment of the topics is somewhat graded,
the earlier chapters being developed with greater simplicity and fullness,
while the later are somewhat more condensed.
Many acknowledgments are made in the text and foot-notes, but it is
impossible to adequately acknowledge all the sources which have been
drawn upon, since the whole body of literature has been laid under
contribution. The authors especially acknowledge the generous assistance
of Professor J. P. Iddings in connection with the chapter on The Origin and
Descent of Rocks; of Dr. F. R. Moulton, Professor C. S. Slichter, Professor
L. M. Hoskins, Mr. A. C. Lunn, and Mr. W. H. Emmons in connection with
mathematical problems; of Professor C. R. Barnes in connection with the
geologic functions of life; and of Professor Julius Stieglitz in connection
with chemical subjects.
references to the fuller discussions of special treatises, they may be made
the basis for more extended courses than are commonly given in
undergraduate work. The attempt has also been made to make the volumes
readable, in the belief that many persons not in colleges or universities will
be interested in following a connected account of the earth’s history, and of
the means by which that history is recorded and read. Antecedent
elementary courses in geology will not be necessary to the use of these
volumes, though such courses may be helpful.
The arrangement of themes adopted is such as to bring to the fore
processes with which all students are immediately in contact, and which are
available for study at all seats of learning. The commoner geologic agents,
such as the atmosphere and running water, have been elaborated somewhat
more fully than is customary, and the common rather than the exceptional
phases of the work of these agents have been emphasized, both because of
their greater importance and their universal availability. The text has been
so shaped as to suggest field work in connection with these topics
especially, since work of this sort is everywhere possible.
After the preliminary outline, which is intended to give some idea of the
scope of the science, and of its salient features, and to show the relations of
the special subjects which follow, the order of treatment is such as to pass
from the commoner and more readily apprehended portions of the subject to
those which are less readily accessible and more obscure. Following the
same general conception, the treatment of the topics is somewhat graded,
the earlier chapters being developed with greater simplicity and fullness,
while the later are somewhat more condensed.
Many acknowledgments are made in the text and foot-notes, but it is
impossible to adequately acknowledge all the sources which have been
drawn upon, since the whole body of literature has been laid under
contribution. The authors especially acknowledge the generous assistance
of Professor J. P. Iddings in connection with the chapter on The Origin and
Descent of Rocks; of Dr. F. R. Moulton, Professor C. S. Slichter, Professor
L. M. Hoskins, Mr. A. C. Lunn, and Mr. W. H. Emmons in connection with
mathematical problems; of Professor C. R. Barnes in connection with the
geologic functions of life; and of Professor Julius Stieglitz in connection
with chemical subjects.
Page 9
The illustrations have been selected from numerous sources, which are
usually acknowledged in the text. Especial acknowledgment is due to the
U. S. Geological Survey for the use of numerous photographs and maps,
and to Mr. G. A. Johnson, who has made many of the drawings reproduced
in Volume I. The authors are under even larger obligations for assistance in
the preparation of Volume II, for which acknowledgment will be made in
the proper place.
University of Chicago, January, 1904.
usually acknowledged in the text. Especial acknowledgment is due to the
U. S. Geological Survey for the use of numerous photographs and maps,
and to Mr. G. A. Johnson, who has made many of the drawings reproduced
in Volume I. The authors are under even larger obligations for assistance in
the preparation of Volume II, for which acknowledgment will be made in
the proper place.
University of Chicago, January, 1904.
Page 10
CONTENTS.
VOLUME I.
CHAPTER I.
PRELIMINARY OUTLINE.
Subdivisions, 1. Dominant processes, 2.
PAGE
Astronomic Geology 2
The earth as a planet, 2. Its satellite, 3. Dependence on
the sun, 4. Meteorites, 4.
Geognosy 5
I. The Atmosphere 5
Mass and extent, 6. Geologic activity, 6. A thermal
blanket, 7.
II. The Hydrosphere 7
Oceanic dimensions, 8. Geologic activity, 8. Chief
horizons of activity, 9.
III. The Lithosphere 9
Irregularities, 10. Epicontinental seas, 11. Diversities of
surface, 12. The surface mantle of the lithosphere, 12. The
crust of the lithosphere, 13. The interior, 14. Varieties of
rock in crust, 14. Stratified rocks, 14. Conformability, 15.
Relative ages, 15. The crystalline rocks, 16. Four great
sedimentary eras, 17. The Archean complex, 18.
General Table of Geologic Divisions 19
CHAPTER II.
VOLUME I.
CHAPTER I.
PRELIMINARY OUTLINE.
Subdivisions, 1. Dominant processes, 2.
PAGE
Astronomic Geology 2
The earth as a planet, 2. Its satellite, 3. Dependence on
the sun, 4. Meteorites, 4.
Geognosy 5
I. The Atmosphere 5
Mass and extent, 6. Geologic activity, 6. A thermal
blanket, 7.
II. The Hydrosphere 7
Oceanic dimensions, 8. Geologic activity, 8. Chief
horizons of activity, 9.
III. The Lithosphere 9
Irregularities, 10. Epicontinental seas, 11. Diversities of
surface, 12. The surface mantle of the lithosphere, 12. The
crust of the lithosphere, 13. The interior, 14. Varieties of
rock in crust, 14. Stratified rocks, 14. Conformability, 15.
Relative ages, 15. The crystalline rocks, 16. Four great
sedimentary eras, 17. The Archean complex, 18.
General Table of Geologic Divisions 19
CHAPTER II.
Page 11
THE ATMOSPHERE AS A GEOLOGICAL AGENT.
The Atmosphere as a Direct Agency 21
I. Mechanical Work 21
Transportation and deposition of dust, 22. Transportation
and deposition of sand, 25. Formation of dunes, 26. Shapes
of dunes, 26. The topographic map, 30. Topography of dune
areas, 32. Migration of dunes, 33. Distribution of dunes,
35. Wind ripples, 37. Abrasion by the wind, 38. Effects of
wind on plants, 40. Indirect effects of the wind, 41.
II. Chemical Work 41
Precipitation from solution, 41. Oxidation, 42.
Carbonation, 43. Other chemical changes, 43. Conditions
favorable for chemical changes, 43.
The Atmosphere as a Conditioning Agency 43
I. Temperature Effects 44
II. Evaporation and Precipitation 50
III. Effects of Electricity. 52
Summary 54
CHAPTER III.
THE WORK OF RUNNING WATER.
Rain and River Erosion 57
Subaërial Erosion without Valleys 58
The Development of Valleys 63
By the growth of gullies, 63. Limits of growth, 67. The
permanent stream, 70. Other modes of valley development,
73. Structural valleys, 77. The courses of valleys, 77. The
development of tributaries, 78.
A Cycle of Erosion. Its Stages 80
General Characteristics of Topography Developed by River
92
Erosion
The Atmosphere as a Direct Agency 21
I. Mechanical Work 21
Transportation and deposition of dust, 22. Transportation
and deposition of sand, 25. Formation of dunes, 26. Shapes
of dunes, 26. The topographic map, 30. Topography of dune
areas, 32. Migration of dunes, 33. Distribution of dunes,
35. Wind ripples, 37. Abrasion by the wind, 38. Effects of
wind on plants, 40. Indirect effects of the wind, 41.
II. Chemical Work 41
Precipitation from solution, 41. Oxidation, 42.
Carbonation, 43. Other chemical changes, 43. Conditions
favorable for chemical changes, 43.
The Atmosphere as a Conditioning Agency 43
I. Temperature Effects 44
II. Evaporation and Precipitation 50
III. Effects of Electricity. 52
Summary 54
CHAPTER III.
THE WORK OF RUNNING WATER.
Rain and River Erosion 57
Subaërial Erosion without Valleys 58
The Development of Valleys 63
By the growth of gullies, 63. Limits of growth, 67. The
permanent stream, 70. Other modes of valley development,
73. Structural valleys, 77. The courses of valleys, 77. The
development of tributaries, 78.
A Cycle of Erosion. Its Stages 80
General Characteristics of Topography Developed by River
92
Erosion
Page 12
Special Features Resulting from Special Conditions of Erosion 92
Bad-land topography, 93. Special forms of valleys;
canyons, 94.
The Struggle for Existence Among Valleys and Streams 100
Piracy, 103.
Rate of Degradation 105
Material in solution in river water. 107.
Economic Considerations 108
Analysis of Erosion 110
Weathering 110
Transportation 115
Transporting power and velocity, 115. How sediment is
carried, 116.
Corrasion 119
Abrasion, 119. Solution, 122.
Conditions Affecting the Rate of Erosion 123
The Influence of Declivity 123
The Influence of Rock 124
Physical constitution, 124. Chemical composition, 124.
Structure, 125.
The Influence of Climate 110
Effects of Unequal Hardness 132
Rapids and falls, 132. Rock terraces, 140. Narrows,
141. Other effects on topography, 142. Adjustment of
streams to rock structures, 146.
Influence of Joints and Folds 150
Joints, 150. Folds, 154.
Effect of Changes of Level 132
Rise, 161. Sinking, 170. Differential movement,
warping, 171.
The Aggradational Work of Running Water 177
Principles involved, 177.
Bad-land topography, 93. Special forms of valleys;
canyons, 94.
The Struggle for Existence Among Valleys and Streams 100
Piracy, 103.
Rate of Degradation 105
Material in solution in river water. 107.
Economic Considerations 108
Analysis of Erosion 110
Weathering 110
Transportation 115
Transporting power and velocity, 115. How sediment is
carried, 116.
Corrasion 119
Abrasion, 119. Solution, 122.
Conditions Affecting the Rate of Erosion 123
The Influence of Declivity 123
The Influence of Rock 124
Physical constitution, 124. Chemical composition, 124.
Structure, 125.
The Influence of Climate 110
Effects of Unequal Hardness 132
Rapids and falls, 132. Rock terraces, 140. Narrows,
141. Other effects on topography, 142. Adjustment of
streams to rock structures, 146.
Influence of Joints and Folds 150
Joints, 150. Folds, 154.
Effect of Changes of Level 132
Rise, 161. Sinking, 170. Differential movement,
warping, 171.
The Aggradational Work of Running Water 177
Principles involved, 177.
Page 13
The Deposits 181
Types, 181. Alluvial fans and cones, 181. Ill-defined
alluvium, 183. Alluvial plains, 184. Flood-plains due to
alluviation, 186. Flood-plains due to obstructions, 188.
Levees, 188. Flood-plain meanders, cut-and-fill, 190.
Scour-and-fill, 194. Materials of the flood-plain, 196.
Topography of the flood-plain, 196. Topographic adjustment
of tributaries, 197. River-lakes, 198. Deltas, 198. Delta
lakes, 204.
Stream Terraces 204
Due to inequalities of hardness, 204. Normal flood-plain
terraces, 205. Flood-plain terraces due to other causes, 208.
Discontinuity of terraces, 209. Termini of terraces, 210.
CHAPTER IV.
THE WORK OF GROUND (UNDERGROUND) WATER.
Conditions influencing descent of rain-water, 213.
Supply of ground-water not altogether dependent on local
rainfall, 215. Ground-water surface—water table, 215.
Depth to which ground-water sinks, 216. Movement of
ground-water, 220. Amount of ground-water, 221. Fate of
ground-water, 221.
The Work of Ground-water 222
Chemical Work 222
Quantitative importance of solution, 223. Deposition of
mineral matter from solution, 225.
Mechanical Work 226
Results of the Work of Ground-water 226
Weathering, 226. Caverns, 227. Creep, slumps, and
landslides, 231.
Summary 232
Springs and Flowing Wells 234
Types, 181. Alluvial fans and cones, 181. Ill-defined
alluvium, 183. Alluvial plains, 184. Flood-plains due to
alluviation, 186. Flood-plains due to obstructions, 188.
Levees, 188. Flood-plain meanders, cut-and-fill, 190.
Scour-and-fill, 194. Materials of the flood-plain, 196.
Topography of the flood-plain, 196. Topographic adjustment
of tributaries, 197. River-lakes, 198. Deltas, 198. Delta
lakes, 204.
Stream Terraces 204
Due to inequalities of hardness, 204. Normal flood-plain
terraces, 205. Flood-plain terraces due to other causes, 208.
Discontinuity of terraces, 209. Termini of terraces, 210.
CHAPTER IV.
THE WORK OF GROUND (UNDERGROUND) WATER.
Conditions influencing descent of rain-water, 213.
Supply of ground-water not altogether dependent on local
rainfall, 215. Ground-water surface—water table, 215.
Depth to which ground-water sinks, 216. Movement of
ground-water, 220. Amount of ground-water, 221. Fate of
ground-water, 221.
The Work of Ground-water 222
Chemical Work 222
Quantitative importance of solution, 223. Deposition of
mineral matter from solution, 225.
Mechanical Work 226
Results of the Work of Ground-water 226
Weathering, 226. Caverns, 227. Creep, slumps, and
landslides, 231.
Summary 232
Springs and Flowing Wells 234
Page 14
Mineral matter in solution, 235. Geysers, 236. Artesian
wells, 242.
CHAPTER V.
THE WORK OF SNOW AND ICE.
Snow- and Ice-fields 244
The passage of snow into névé and ice, 246. Structure of
the ice, 247. Texture, 247. Inauguration of movement, 248.
Types of Glaciers 251
The General Phenomena of Glaciers 256
Dimensions, 256. Limits, 258. Movement, 259.
Conditions affecting rate of movement, 261. Likenesses and
unlikenesses of glaciers and rivers, 262.
Surface Features 266
Topography, 266. Surface moraines, 266. Relief due to
surface débris, 268. Dust-wells, 269. Débris below the
surface, 272.
Temperature, Waste, and Drainage 273
The winter wave, 274. The summer wave, 276. The
temperature of the bottom, 276. Temperature of the interior
of the ice, 277. Compression and friction as causes of heat,
278. Summary, 279. Movement under low temperature,
279. Evaporation, 279. Drainage, 280.
The Work of Glaciers 281
Erosion and Transportation 281
Getting load, 282. Conditions influencing rate of
erosion, 283. Summary, 286. Varied nature of glacial débris,
286. The topographic effects of glacial erosion, 287. Fiords,
290. The positions in which débris is carried, 290. Transfers
of load, 292. Wear of drift in transit, 298.
Deposition of the Drift 298
Beneath the body of the ice, 298. At ends and edges of
glaciers, 299.
wells, 242.
CHAPTER V.
THE WORK OF SNOW AND ICE.
Snow- and Ice-fields 244
The passage of snow into névé and ice, 246. Structure of
the ice, 247. Texture, 247. Inauguration of movement, 248.
Types of Glaciers 251
The General Phenomena of Glaciers 256
Dimensions, 256. Limits, 258. Movement, 259.
Conditions affecting rate of movement, 261. Likenesses and
unlikenesses of glaciers and rivers, 262.
Surface Features 266
Topography, 266. Surface moraines, 266. Relief due to
surface débris, 268. Dust-wells, 269. Débris below the
surface, 272.
Temperature, Waste, and Drainage 273
The winter wave, 274. The summer wave, 276. The
temperature of the bottom, 276. Temperature of the interior
of the ice, 277. Compression and friction as causes of heat,
278. Summary, 279. Movement under low temperature,
279. Evaporation, 279. Drainage, 280.
The Work of Glaciers 281
Erosion and Transportation 281
Getting load, 282. Conditions influencing rate of
erosion, 283. Summary, 286. Varied nature of glacial débris,
286. The topographic effects of glacial erosion, 287. Fiords,
290. The positions in which débris is carried, 290. Transfers
of load, 292. Wear of drift in transit, 298.
Deposition of the Drift 298
Beneath the body of the ice, 298. At ends and edges of
glaciers, 299.
Page 15
Types of Moraines 301
The terminal moraine, 301. The ground moraine, 301.
The lateral moraines, 302. Distinctive nature of glacial
deposits, 304. Glaciated rock surfaces, 304.
Glacio-Fluvial Work 305
Icebergs 307
The Intimate Structure and the Movement of Glaciers 308
The growth and constitution of a glacier, 308. The
arrangement of the crystal axes, 312.
The Probable Fundamental Element in Glacial Motion 313
Melting and freezing, 313. Accumulated motion in the
terminal part of a glacier, 316.
Auxiliary Elements 317
Shearing, 317. High temperature and water, 318.
Applications, 319.
Corroborative Phenomena 320
Other Views of Glacier Motion 321
CHAPTER VI.
THE WORK OF THE OCEAN.
Volume and composition, 324. Topography of bed, 326.
Distribution of marine life, 328.
Processes in Operation in the Sea 329
Diastrophism, 329. Vulcanism, 332. Gradation, 333.
Movements of the Sea-water 334
Differences in density and their results, 335. Differences
in level and their results. 335. Movements generated by
winds, 336. Movements generated by attraction, 322.
Aperiodic movements, 338. Summary, 339.
Waves 339
Wave-motion, 339.
Work of the Waves 342
The terminal moraine, 301. The ground moraine, 301.
The lateral moraines, 302. Distinctive nature of glacial
deposits, 304. Glaciated rock surfaces, 304.
Glacio-Fluvial Work 305
Icebergs 307
The Intimate Structure and the Movement of Glaciers 308
The growth and constitution of a glacier, 308. The
arrangement of the crystal axes, 312.
The Probable Fundamental Element in Glacial Motion 313
Melting and freezing, 313. Accumulated motion in the
terminal part of a glacier, 316.
Auxiliary Elements 317
Shearing, 317. High temperature and water, 318.
Applications, 319.
Corroborative Phenomena 320
Other Views of Glacier Motion 321
CHAPTER VI.
THE WORK OF THE OCEAN.
Volume and composition, 324. Topography of bed, 326.
Distribution of marine life, 328.
Processes in Operation in the Sea 329
Diastrophism, 329. Vulcanism, 332. Gradation, 333.
Movements of the Sea-water 334
Differences in density and their results, 335. Differences
in level and their results. 335. Movements generated by
winds, 336. Movements generated by attraction, 322.
Aperiodic movements, 338. Summary, 339.
Waves 339
Wave-motion, 339.
Work of the Waves 342
Page 16
Erosion 342
By waves and undertow, 342.
Topographic Features Developed by Wave Erosion 349
The sea-cliff, 349. Chimney rocks, etc., 350. Sea caves,
350. The wave-cut terrace, 351. Wave erosion and
horizontal configuration, 353.
Transportation by Waves 354
Deposition by Waves, Undertow, and Shore Currents 355
The beach, 355. The barrier, 356. The spit, the bar, and
the loop, 357. Wave-built terraces, 363.
Effect of Shore Deposition on Coastal Configuration 363
Summary of Coastal Irregularities 364
The Work of Ocean-currents 366
Deposits of the Ocean-bed 368
Shallow-water Deposits 369
Littoral deposits, 369. Non-littoral, mechanical deposits
in shallow water, 369. Characteristics of shallow-water
deposits, 373. Topography of shallow-water deposits, 374.
Chemical and organic deposits, 375. Limestone, 378.
Deep-sea Deposits 378
Contrasted with shallow-water deposits, 378. Sources,
380. Mechanical inorganic deposits, 380. Organic
constituents of pelagic deposits, 382. Chemical deposits,
383.
Lakes 386
Changes taking place in lakes, 387. Lacustrine deposits,
388. Extinct lakes, 388. Lake ice, 389. Saline lakes, 391.
Indirect effects of lakes, 392. Composition of lake waters,
392.
CHAPTER VII.
THE ORIGIN AND DESCENT OF ROCKS.
By waves and undertow, 342.
Topographic Features Developed by Wave Erosion 349
The sea-cliff, 349. Chimney rocks, etc., 350. Sea caves,
350. The wave-cut terrace, 351. Wave erosion and
horizontal configuration, 353.
Transportation by Waves 354
Deposition by Waves, Undertow, and Shore Currents 355
The beach, 355. The barrier, 356. The spit, the bar, and
the loop, 357. Wave-built terraces, 363.
Effect of Shore Deposition on Coastal Configuration 363
Summary of Coastal Irregularities 364
The Work of Ocean-currents 366
Deposits of the Ocean-bed 368
Shallow-water Deposits 369
Littoral deposits, 369. Non-littoral, mechanical deposits
in shallow water, 369. Characteristics of shallow-water
deposits, 373. Topography of shallow-water deposits, 374.
Chemical and organic deposits, 375. Limestone, 378.
Deep-sea Deposits 378
Contrasted with shallow-water deposits, 378. Sources,
380. Mechanical inorganic deposits, 380. Organic
constituents of pelagic deposits, 382. Chemical deposits,
383.
Lakes 386
Changes taking place in lakes, 387. Lacustrine deposits,
388. Extinct lakes, 388. Lake ice, 389. Saline lakes, 391.
Indirect effects of lakes, 392. Composition of lake waters,
392.
CHAPTER VII.
THE ORIGIN AND DESCENT OF ROCKS.
Page 17
Composition of Igneous Rocks 395
Leading elements, 396. Union of elements, 397.
Formation of minerals, 397. Sources of complexity, 398.
The leading minerals of igneous rocks, 399. The feldspathic
minerals, 400. The ferromagnesian minerals, 400. Summary
of salient facts, 401.
The Nature of Molten Magmas 401
Time required in crystallization, 402. Successive stages
of crystallization, 403.
The Fragmental Products of Sudden Cooling 404
Pyroclastic rocks, 404.
The Glassy Rocks 406
The solid glasses. 406. The first stages of crystallization,
407. The obsidians, 407.
Special Structures 410
Flow structure, 410. Amygdaloids, 411.
The Porphyritic Rocks 411
The Phanerocrystalline Rocks 412
The phanerites, 412. The granites, 413. The syenites,
415. The diorites, 416. The gabbros, 416. The peridotites,
416. The basalts, 417. The dolerites, 417. General names,
418.
Derivation of Secondary Rocks 420
Regolith, 422. Disrupted products: arkose and wacke,
422. Disintegrated products, 422.
Classes of Sedimentary Rocks 422
Shales, sandstones, and conglomerates, 422. Limestones
and dolomites, 424. Precipitates, 424. Iron-ore beds, 425.
Silicious deposits, 425. Organic rocks, 426.
Internal Alterations of Rocks 426
Oxidation and deoxidation, 427. Solution and
deposition, 427. Hydration and dehydration, 428.
Carbonation and decarbonation, 429. Molecular
rearrangements, 431.
Leading elements, 396. Union of elements, 397.
Formation of minerals, 397. Sources of complexity, 398.
The leading minerals of igneous rocks, 399. The feldspathic
minerals, 400. The ferromagnesian minerals, 400. Summary
of salient facts, 401.
The Nature of Molten Magmas 401
Time required in crystallization, 402. Successive stages
of crystallization, 403.
The Fragmental Products of Sudden Cooling 404
Pyroclastic rocks, 404.
The Glassy Rocks 406
The solid glasses. 406. The first stages of crystallization,
407. The obsidians, 407.
Special Structures 410
Flow structure, 410. Amygdaloids, 411.
The Porphyritic Rocks 411
The Phanerocrystalline Rocks 412
The phanerites, 412. The granites, 413. The syenites,
415. The diorites, 416. The gabbros, 416. The peridotites,
416. The basalts, 417. The dolerites, 417. General names,
418.
Derivation of Secondary Rocks 420
Regolith, 422. Disrupted products: arkose and wacke,
422. Disintegrated products, 422.
Classes of Sedimentary Rocks 422
Shales, sandstones, and conglomerates, 422. Limestones
and dolomites, 424. Precipitates, 424. Iron-ore beds, 425.
Silicious deposits, 425. Organic rocks, 426.
Internal Alterations of Rocks 426
Oxidation and deoxidation, 427. Solution and
deposition, 427. Hydration and dehydration, 428.
Carbonation and decarbonation, 429. Molecular
rearrangements, 431.
Page 18
The Salient Features of Rock Descent 431
The Reascensional Process 432
Induration under ordinary pressures and temperatures,
432. Cavity filling, 436. Fissure filling; veins, 437.
Solution as well as deposition, 437. Concretions, 438.
Replacements and pseudomorphs, 439. Incipient
crystallization, 439.
Reconstruction under Exceptional Conditions 440
Slaty structure, 441. Foliation, schistosity, 443.
Metamorphism by heat, 446. Metamorphism by heat and
lateral pressure, 448. Deep-seated metamorphism, 449.
Completion of the rock cycle, 449.
Various Classifications and Nomenclatures 449
New System of Classification and Nomenclature 451
The Proposed Field System 451
The phanerites, 451. The aphanites, 452.
The Proposed Quantitative System 454
Reference List of the More Common Minerals 460
Reference List of the More Common Rocks 467
Ore Deposits 474
Concentration, 474. Exceptional and doubtful cases,
474. Original distribution, 475. Magmatic segregation, 475.
Marine segregation and dispersion, 476. Origin of ore
regions, 477. Surface residual concentration, 478.
Purification and concentration, 478. Concentration by
solution and reprecipitation, 479. Location of greatest
solvent action, 480. Short-course action, 481. Long-course
action, 481. Summary, 483. The influence of contacts, 484.
The effect of igneous intrusions, 484. The influence of rock
walls, 484.
CHAPTER VIII.
STRUCTURAL (GEOTECTONIC) GEOLOGY.
The Reascensional Process 432
Induration under ordinary pressures and temperatures,
432. Cavity filling, 436. Fissure filling; veins, 437.
Solution as well as deposition, 437. Concretions, 438.
Replacements and pseudomorphs, 439. Incipient
crystallization, 439.
Reconstruction under Exceptional Conditions 440
Slaty structure, 441. Foliation, schistosity, 443.
Metamorphism by heat, 446. Metamorphism by heat and
lateral pressure, 448. Deep-seated metamorphism, 449.
Completion of the rock cycle, 449.
Various Classifications and Nomenclatures 449
New System of Classification and Nomenclature 451
The Proposed Field System 451
The phanerites, 451. The aphanites, 452.
The Proposed Quantitative System 454
Reference List of the More Common Minerals 460
Reference List of the More Common Rocks 467
Ore Deposits 474
Concentration, 474. Exceptional and doubtful cases,
474. Original distribution, 475. Magmatic segregation, 475.
Marine segregation and dispersion, 476. Origin of ore
regions, 477. Surface residual concentration, 478.
Purification and concentration, 478. Concentration by
solution and reprecipitation, 479. Location of greatest
solvent action, 480. Short-course action, 481. Long-course
action, 481. Summary, 483. The influence of contacts, 484.
The effect of igneous intrusions, 484. The influence of rock
walls, 484.
CHAPTER VIII.
STRUCTURAL (GEOTECTONIC) GEOLOGY.
Page 19
The structural phases which rocks assume, 486.
Structural Features of Sedimentary Rocks 486
Stratification, 486. Lateral graduation, 488. Special
markings, 489. Concretionary structure, 490. Secretions,
497.
Structural Features of Igneous Rocks 498
Structural Features Arising From Disturbance 500
Inclination and folding of strata, 500. Joints, 510.
Sandstone dikes, 514. Faults, 514. The significance of
faults, 521. Effect of faulting on outcrops, 522.
CHAPTER IX.
THE MOVEMENTS AND DEFORMATIONS OF THE
EARTH’S BODY (DIASTROPHISM).
Minute and Rapid Movements 526
Earthquakes 527
Points of origin, foci, 527. The amplitude of the
vibrations, 529. Destructive effects, 530. Direction of throw,
531. Rate of propagation, 532. Sequences of vibrations,
533. Gaseous emanations, 533. Distribution of earthquakes,
533.
The Geologic Effects of Earthquakes 534
Fracturing of rock, 534. Changes of surface, 534.
Effects on drainage, 535. Effects on standing water, 535.
Changes of level, 536.
Slow Massive Movements 537
Present movements, 538. Fundamental conceptions, 539.
Nearly Constant Small Movements 540
Reciprocal features, 541.
The Great Periodic Movements 542
Mountain-forming movements, 542. Distribution of
folded ranges, 543. Plateau-forming movements, 543.
Structural Features of Sedimentary Rocks 486
Stratification, 486. Lateral graduation, 488. Special
markings, 489. Concretionary structure, 490. Secretions,
497.
Structural Features of Igneous Rocks 498
Structural Features Arising From Disturbance 500
Inclination and folding of strata, 500. Joints, 510.
Sandstone dikes, 514. Faults, 514. The significance of
faults, 521. Effect of faulting on outcrops, 522.
CHAPTER IX.
THE MOVEMENTS AND DEFORMATIONS OF THE
EARTH’S BODY (DIASTROPHISM).
Minute and Rapid Movements 526
Earthquakes 527
Points of origin, foci, 527. The amplitude of the
vibrations, 529. Destructive effects, 530. Direction of throw,
531. Rate of propagation, 532. Sequences of vibrations,
533. Gaseous emanations, 533. Distribution of earthquakes,
533.
The Geologic Effects of Earthquakes 534
Fracturing of rock, 534. Changes of surface, 534.
Effects on drainage, 535. Effects on standing water, 535.
Changes of level, 536.
Slow Massive Movements 537
Present movements, 538. Fundamental conceptions, 539.
Nearly Constant Small Movements 540
Reciprocal features, 541.
The Great Periodic Movements 542
Mountain-forming movements, 542. Distribution of
folded ranges, 543. Plateau-forming movements, 543.
Page 20
Continent-forming movements, 544. Relations of these
movements in time, 545. Relations of vertical to horizontal
movements, 545. The squeezed segments, 546. The
depressed or master segments, 546. The differential extent
of crustal movements, 548.
The Causes of Movement 551
General Considerations 551
1. The centripetal agencies 552
Gravity, 552. Molecular and sub-molecular
attractions, 554. Cohesion and crystallization, 554.
Diffusion, 555. Chemical combination, 556. Sub-atomic
forces 556.
2. The resisting agencies 557
Heat, 557. All resistance perhaps due to motion, 558.
Alternative Views of Original Heat Distribution 559
Thermal distribution on the convection hypothesis, 559.
Level of no stress, 561. Thermal distribution on the
hypothesis of central solidification, 562. Thermal
distribution under the accretion hypothesis, 564.
Computed Pressures, Densities, and Temperatures within the
564
Earth Based on Laplace’s Law
Recombination of material, 568. Comparison of the
hypotheses, 568.
Observed Temperatures in Excavations 569
Explanations of varying increment, 570. The permeation
and circulation of water, 570. Chemical action, 570.
Differences in the conductivity of rock, 571. Compression,
571. Gradients projected, 571. The amount of loss of heat,
572. The amount of shrinkage from loss of heat, 572.
Other Sources of Deformation 574
Transfer of internal heat, 574. Denser aggregation of
matter, 574. Extravasation of lavas, 574. Change in the rate
of rotation, 575. Distribution of rigidity, 578.
Sphericity as a Factor in Deformation 580
movements in time, 545. Relations of vertical to horizontal
movements, 545. The squeezed segments, 546. The
depressed or master segments, 546. The differential extent
of crustal movements, 548.
The Causes of Movement 551
General Considerations 551
1. The centripetal agencies 552
Gravity, 552. Molecular and sub-molecular
attractions, 554. Cohesion and crystallization, 554.
Diffusion, 555. Chemical combination, 556. Sub-atomic
forces 556.
2. The resisting agencies 557
Heat, 557. All resistance perhaps due to motion, 558.
Alternative Views of Original Heat Distribution 559
Thermal distribution on the convection hypothesis, 559.
Level of no stress, 561. Thermal distribution on the
hypothesis of central solidification, 562. Thermal
distribution under the accretion hypothesis, 564.
Computed Pressures, Densities, and Temperatures within the
564
Earth Based on Laplace’s Law
Recombination of material, 568. Comparison of the
hypotheses, 568.
Observed Temperatures in Excavations 569
Explanations of varying increment, 570. The permeation
and circulation of water, 570. Chemical action, 570.
Differences in the conductivity of rock, 571. Compression,
571. Gradients projected, 571. The amount of loss of heat,
572. The amount of shrinkage from loss of heat, 572.
Other Sources of Deformation 574
Transfer of internal heat, 574. Denser aggregation of
matter, 574. Extravasation of lavas, 574. Change in the rate
of rotation, 575. Distribution of rigidity, 578.
Sphericity as a Factor in Deformation 580
Page 21
The influence of the domed form of the surface, 581.
Theoretical strength of domes of earth-dimensions, 581.
Stress-accumulation independent of sphericity, 583. The
actual configuration of the surface, 584. Concave tracts,
584. General conclusion, 588.
CHAPTER X.
THE EXTRUSIVE PROCESSES.
Outward movements, 590.
Vulcanism 590
Phases of vulcanism, 591.
1. Intrusions 591
The heating action, 592.
2. Extrusions 592
Fissure eruptions, 593. Volcanic eruptions, 594.
Intermediate phenomena, 596. Lunar craters, 598.
Volcanoes 599
Number of, 599.
Distribution of Volcanoes 599
In time, 599. Relative to land and sea, 599. Relative to
crustal deformations, 601. In latitude, 603. In curved lines,
603.
Relations of Volcanoes 604
Relations to rising and sinking surfaces, 604. Relations
to one another, 605. Unimportant coincidences, 606.
Periodicity, 607.
Formation of Cones 608
Lava-cones, 608. Cinder-cones, 608. Subordinate cones,
610. Composite cones, 610. Extra-cone distribution, 610.
Lavas 612
Their nature, 612. Consanguinity and succession of
lavas, 614. Temperature of lavas, 615. Depth of source, 616.
Theoretical strength of domes of earth-dimensions, 581.
Stress-accumulation independent of sphericity, 583. The
actual configuration of the surface, 584. Concave tracts,
584. General conclusion, 588.
CHAPTER X.
THE EXTRUSIVE PROCESSES.
Outward movements, 590.
Vulcanism 590
Phases of vulcanism, 591.
1. Intrusions 591
The heating action, 592.
2. Extrusions 592
Fissure eruptions, 593. Volcanic eruptions, 594.
Intermediate phenomena, 596. Lunar craters, 598.
Volcanoes 599
Number of, 599.
Distribution of Volcanoes 599
In time, 599. Relative to land and sea, 599. Relative to
crustal deformations, 601. In latitude, 603. In curved lines,
603.
Relations of Volcanoes 604
Relations to rising and sinking surfaces, 604. Relations
to one another, 605. Unimportant coincidences, 606.
Periodicity, 607.
Formation of Cones 608
Lava-cones, 608. Cinder-cones, 608. Subordinate cones,
610. Composite cones, 610. Extra-cone distribution, 610.
Lavas 612
Their nature, 612. Consanguinity and succession of
lavas, 614. Temperature of lavas, 615. Depth of source, 616.
Page 22
Volcanic Gases 617
Differences in gas action, 617. Spasmodic action, 618.
Kinds of gases, 618. Residual gases in volcanic rock, 619.
The source of the gases, 621.
The Cause of Vulcanism 623
I. On the Assumption that the Lavas are Original 623
Lava outflows from a molten interior, 624. Lavas
assigned to molten reservoirs, 624.
II. On the Assumption that the Lavas are Secondary 625
Lavas assigned to the reaction of water and air
penetrating to hot rocks, 625. Lavas assigned to relief of
pressure, 627. Lavas assigned to melting by crushing, 628.
Lavas assigned to melting by depression, 629. Vulcanism
assigned to the outflow of deep-seated heat, 629.
Modes of Reaching the Surface 631
Additional Considerations Relative to the Gases 633
Thermal Considerations 635
CHAPTER XI.
THE GEOLOGIC FUNCTIONS OF LIFE.
I. The Distinctive Features of Organic Processes 638
The Chemical Work of Life 638
Life material chiefly atmospheric, 638. The non-
atmospheric factors, 639.
(1) Changes in the composition of the atmosphere 639
The consumption and restoration of carbon dioxide,
640. The freezing and consumption of oxygen, 640. The
organic residue, 640. The meaning of the organic residue,
641. The more inert factor, 642. Probable fluctuations of
atmospheric composition, 642. The climatic effects of
organic action, 643.
(2) Aid and hindrance to inorganic action 644
Differences in gas action, 617. Spasmodic action, 618.
Kinds of gases, 618. Residual gases in volcanic rock, 619.
The source of the gases, 621.
The Cause of Vulcanism 623
I. On the Assumption that the Lavas are Original 623
Lava outflows from a molten interior, 624. Lavas
assigned to molten reservoirs, 624.
II. On the Assumption that the Lavas are Secondary 625
Lavas assigned to the reaction of water and air
penetrating to hot rocks, 625. Lavas assigned to relief of
pressure, 627. Lavas assigned to melting by crushing, 628.
Lavas assigned to melting by depression, 629. Vulcanism
assigned to the outflow of deep-seated heat, 629.
Modes of Reaching the Surface 631
Additional Considerations Relative to the Gases 633
Thermal Considerations 635
CHAPTER XI.
THE GEOLOGIC FUNCTIONS OF LIFE.
I. The Distinctive Features of Organic Processes 638
The Chemical Work of Life 638
Life material chiefly atmospheric, 638. The non-
atmospheric factors, 639.
(1) Changes in the composition of the atmosphere 639
The consumption and restoration of carbon dioxide,
640. The freezing and consumption of oxygen, 640. The
organic residue, 640. The meaning of the organic residue,
641. The more inert factor, 642. Probable fluctuations of
atmospheric composition, 642. The climatic effects of
organic action, 643.
(2) Aid and hindrance to inorganic action 644
Page 23
The promotion of disintegration, 644. Protection
against erosion, 644. The influence of land vegetation on
the character of the sediments, 645.
(3) Distinctive deposits 646
Organic rocks, 646. Inorganic rocks due to life, 646.
Fossils 646
The general order of life succession determined by
stratigraphy, 647. Fossils as means of correlation, 647.
Special Modes of Aggregation and of Movement 648
The Mental Element 649
(1) The material effects of the mental element, 649.
Human modification of the animal and vegetal kingdoms,
650. (2) The psychological factors as such, 651.
II. Special Contributions of the Organic Kingdoms 652
Contributions of the Plant Kingdom 652
Reference table of the principal groups of plants, 653.
The contribution of the Thallophytes, 653. The contribution
of the Bryophytes, 656. The contribution of the
Pteridophytes, 657. The contribution of the Spermatophytes,
657. Plant life terrestrial rather than marine, 658.
Contributions of the Animal Kingdom 658
Reference table of the principal groups of animals, 659.
The contribution of the Protozoa, 660. The contribution of
the Cœlenterata, 661. The contribution of the
Echinodermata, 661. The contribution of the Vermes, 662.
The contribution of the Molluscoidea, 662. The contribution
of the Mollusca, 662. The contribution of the Arthropoda,
662. The contribution of the Vertebrata, 663.
III. The Associations and Ecological Relations of Life 663
The Basis of Floras and Faunas 663
Assemblages Influenced by the Mutual Relations of Organisms 664
Food relations, 664. Adaptive relations, 665.
Competitive relations, 665. Offensive and defensive
relations, 665. Implied forms of life, 666.
against erosion, 644. The influence of land vegetation on
the character of the sediments, 645.
(3) Distinctive deposits 646
Organic rocks, 646. Inorganic rocks due to life, 646.
Fossils 646
The general order of life succession determined by
stratigraphy, 647. Fossils as means of correlation, 647.
Special Modes of Aggregation and of Movement 648
The Mental Element 649
(1) The material effects of the mental element, 649.
Human modification of the animal and vegetal kingdoms,
650. (2) The psychological factors as such, 651.
II. Special Contributions of the Organic Kingdoms 652
Contributions of the Plant Kingdom 652
Reference table of the principal groups of plants, 653.
The contribution of the Thallophytes, 653. The contribution
of the Bryophytes, 656. The contribution of the
Pteridophytes, 657. The contribution of the Spermatophytes,
657. Plant life terrestrial rather than marine, 658.
Contributions of the Animal Kingdom 658
Reference table of the principal groups of animals, 659.
The contribution of the Protozoa, 660. The contribution of
the Cœlenterata, 661. The contribution of the
Echinodermata, 661. The contribution of the Vermes, 662.
The contribution of the Molluscoidea, 662. The contribution
of the Mollusca, 662. The contribution of the Arthropoda,
662. The contribution of the Vertebrata, 663.
III. The Associations and Ecological Relations of Life 663
The Basis of Floras and Faunas 663
Assemblages Influenced by the Mutual Relations of Organisms 664
Food relations, 664. Adaptive relations, 665.
Competitive relations, 665. Offensive and defensive
relations, 665. Implied forms of life, 666.
Page 24
Assemblages Influenced by Environment 666
Plant societies, 667.
The Influence of Geographic Conditions on the Evolution of
668
Floras and Faunas
The development of provincial and cosmopolitan faunas,
668. Restrictive and expansional evolution, 672.
Plant societies, 667.
The Influence of Geographic Conditions on the Evolution of
668
Floras and Faunas
The development of provincial and cosmopolitan faunas,
668. Restrictive and expansional evolution, 672.
Page 25
PLATES.
PLATE FACE PAGE
I. Bathymetrical Chart of the Oceans 10
II. Fig. 1. New Jersey. Fig. 2. Kansas. Fig. 3. Indiana. Fig. 4.
Nebraska 39
III. Fig. 1. Kansas. Fig. 2. Nevada 72
IV. Fig. 1. Illinois. Fig. 2. North Dakota 73
V. Fig. 1. Kentucky. Fig. 2. Virginia 85
VI. Parts of Los Angeles and San Bernardino Counties,
California 87
VII. Kansas 90
VIII. About 16 Miles Southwest of St. Louis, Mo. 91
IX. Niagara Falls 100
X. Fig. 1. Yellowstone Park. Fig. 2. Arizona 101
XI. Part of the Catskills, N. Y. 106
XII. Fig. 1. New Mexico. Fig. 2. Virginia, West Virginia, and
Maryland 107
XIII. Fig. 1. Colorado. Fig. 2. Kansas 162
XIV. Fig. 1. Pennsylvania. Fig. 2. California 163
XV. Near Hahnville, Louisiana 188
XVI. Missouri 189
XVII. Fig. 1. Hunterdon County, N. J. Fig. 2. Near Pikeville,
Tenn. 232
XVII
Fig. 1. Washington. Fig. 2. California
I. 233
XIX. Part of the Big Horn Range, Wyoming 286
XX. Section of the California Coast near San Mateo, Cal. 287
XXI. New Jersey 356
PLATE FACE PAGE
I. Bathymetrical Chart of the Oceans 10
II. Fig. 1. New Jersey. Fig. 2. Kansas. Fig. 3. Indiana. Fig. 4.
Nebraska 39
III. Fig. 1. Kansas. Fig. 2. Nevada 72
IV. Fig. 1. Illinois. Fig. 2. North Dakota 73
V. Fig. 1. Kentucky. Fig. 2. Virginia 85
VI. Parts of Los Angeles and San Bernardino Counties,
California 87
VII. Kansas 90
VIII. About 16 Miles Southwest of St. Louis, Mo. 91
IX. Niagara Falls 100
X. Fig. 1. Yellowstone Park. Fig. 2. Arizona 101
XI. Part of the Catskills, N. Y. 106
XII. Fig. 1. New Mexico. Fig. 2. Virginia, West Virginia, and
Maryland 107
XIII. Fig. 1. Colorado. Fig. 2. Kansas 162
XIV. Fig. 1. Pennsylvania. Fig. 2. California 163
XV. Near Hahnville, Louisiana 188
XVI. Missouri 189
XVII. Fig. 1. Hunterdon County, N. J. Fig. 2. Near Pikeville,
Tenn. 232
XVII
Fig. 1. Washington. Fig. 2. California
I. 233
XIX. Part of the Big Horn Range, Wyoming 286
XX. Section of the California Coast near San Mateo, Cal. 287
XXI. New Jersey 356
Page 26
PLATE FACE PAGE
XXII. Fig. 1. Portion of South Coast of Martha’s Vineyard,
Mass. Fig. 2. Portion of the California Coast near
Tamalpais 357
XXII
Fig. 1. Massachusetts. Fig. 2. Maine
I. 364
XXI
Portion of the Coast of Maine
V. 365
XXII. Fig. 1. Portion of South Coast of Martha’s Vineyard,
Mass. Fig. 2. Portion of the California Coast near
Tamalpais 357
XXII
Fig. 1. Massachusetts. Fig. 2. Maine
I. 364
XXI
Portion of the Coast of Maine
V. 365
Page 27
TABLES.
Analyses of American River-waters 106
Analyses of American Spring-waters 236
Analyses of the Waters of Inclosed Lakes 392
Analyses of American River-waters 106
Analyses of American Spring-waters 236
Analyses of the Waters of Inclosed Lakes 392
Page 28
GEOLOGY
Page 29
CHAPTER I.
PRELIMINARY OUTLINE.
Geology treats of the structure of the earth, of the various stages through
which it has passed, and of the living beings that have dwelt upon it,
together with the agencies and processes involved in the changes it has
undergone. Geology is essentially a history of the earth and its inhabitants.
It is one of the broadest of the sciences, and brings under consideration
certain phases of nearly all the other sciences, particularly those of
astronomy, physics, chemistry, zoology, and botany. It also embraces the
earlier expressions of mental development and of life-relationships, chiefly
as found in the lower animals.
Subdivisions.—Naturally so broad a science has many special aspects
which constitute subdivisions, in a sense, though they are rather dominant
phases than independent sections. That phase which treats of the outer
relations of the earth is Cosmic or Astronomic geology; that which treats of
the constituent parts of the earth and its material is Geognosy, of which the
most important branch is Petrology, the science of rocks. That branch which
investigates the structural arrangement of the material, or “the architecture
of the earth,” is Geotectonic, or Structural geology; while that which deals
with the surface changes and topographic forms, that is, with the face of the
earth, is Physiographic geology. The study of the fossils that have been
preserved in the rocks, and of the faunas and floras that these imply,
constitutes Paleontologic geology, or Paleontology. The treatment of the
succession of events forms Historical geology. This is chiefly worked out
by the succession of beds laid down in the progress of the ages, which
constitutes Stratigraphic geology. The treatment of causes, agencies, and
processes is the function of Dynamic or Philosophic geology.
Besides these there are special applications which give occasion for other
terms, as Economic geology, which is concerned with the industrial
applications of geologic knowledge; Mining geology, which is a sub-section
of economic geology, relating to the application of geologic facts and
principles to mining operations; Atmospheric geology, Glacial geology, and
PRELIMINARY OUTLINE.
Geology treats of the structure of the earth, of the various stages through
which it has passed, and of the living beings that have dwelt upon it,
together with the agencies and processes involved in the changes it has
undergone. Geology is essentially a history of the earth and its inhabitants.
It is one of the broadest of the sciences, and brings under consideration
certain phases of nearly all the other sciences, particularly those of
astronomy, physics, chemistry, zoology, and botany. It also embraces the
earlier expressions of mental development and of life-relationships, chiefly
as found in the lower animals.
Subdivisions.—Naturally so broad a science has many special aspects
which constitute subdivisions, in a sense, though they are rather dominant
phases than independent sections. That phase which treats of the outer
relations of the earth is Cosmic or Astronomic geology; that which treats of
the constituent parts of the earth and its material is Geognosy, of which the
most important branch is Petrology, the science of rocks. That branch which
investigates the structural arrangement of the material, or “the architecture
of the earth,” is Geotectonic, or Structural geology; while that which deals
with the surface changes and topographic forms, that is, with the face of the
earth, is Physiographic geology. The study of the fossils that have been
preserved in the rocks, and of the faunas and floras that these imply,
constitutes Paleontologic geology, or Paleontology. The treatment of the
succession of events forms Historical geology. This is chiefly worked out
by the succession of beds laid down in the progress of the ages, which
constitutes Stratigraphic geology. The treatment of causes, agencies, and
processes is the function of Dynamic or Philosophic geology.
Besides these there are special applications which give occasion for other
terms, as Economic geology, which is concerned with the industrial
applications of geologic knowledge; Mining geology, which is a sub-section
of economic geology, relating to the application of geologic facts and
principles to mining operations; Atmospheric geology, Glacial geology, and
Page 30
others that define themselves, and are for the greater part but limited aspects
of the broad science.
Dominant processes.—Three sets of processes, now in operation on the
surface of the lithosphere, have given rise to most of the details of its
configuration, and even many of its larger features. These processes have
been designated diastrophism, vulcanism, and gradation. Diastrophism
includes all crustal movements, whether slow or rapid, gentle or violent,
slight or extensive. Many parts of the land, especially along coasts, are
known to be slowly sinking relative to the sea-level, while other parts are
known to be rising. The fact that rocks originally formed beneath the sea
now exist at great elevations, and the further fact that areas which were
once land are now beneath the sea, are sufficient evidence that similar
changes have taken place in the past. Vulcanism includes all processes
connected with the extrusion of lava and other volcanic products, and with
the rise of lava from lower to higher levels, even if not extruded. Vulcanism
and diastrophism may be closely associated, for local movements at least
are often associated with volcanic eruptions, and more considerable
movements may be connected with the movements of subsurface lavas,
even when the connection is not demonstrable. Gradation includes all those
processes which tend to bring the surface of the lithosphere to a common
level. Gradational processes belong to two categories—those which level
down, degradation, and those which level up, aggradation. The
transportation of material from the land, whether by rain, rivers, glaciers,
waves, or winds, is degradation and the deposition of material, whether on
the land or in the sea, is aggradation. Degradation affects primarily the
protuberances of the lithosphere, while aggradation affects primarily its
depressions.
Astronomic Geology.
The earth as a planet.—Though supremely important to us, the earth is
but one of the minor planets attendant upon the sun, and is in no very
special way distinguished as a planetary body. Of the eight planets, four,
Jupiter, Saturn, Uranus, and Neptune, are much larger than the earth, while
three, Mars, Venus, and Mercury, are smaller. There are a host of asteroids,
but all together they do not equal the mass of the smallest planet. The
of the broad science.
Dominant processes.—Three sets of processes, now in operation on the
surface of the lithosphere, have given rise to most of the details of its
configuration, and even many of its larger features. These processes have
been designated diastrophism, vulcanism, and gradation. Diastrophism
includes all crustal movements, whether slow or rapid, gentle or violent,
slight or extensive. Many parts of the land, especially along coasts, are
known to be slowly sinking relative to the sea-level, while other parts are
known to be rising. The fact that rocks originally formed beneath the sea
now exist at great elevations, and the further fact that areas which were
once land are now beneath the sea, are sufficient evidence that similar
changes have taken place in the past. Vulcanism includes all processes
connected with the extrusion of lava and other volcanic products, and with
the rise of lava from lower to higher levels, even if not extruded. Vulcanism
and diastrophism may be closely associated, for local movements at least
are often associated with volcanic eruptions, and more considerable
movements may be connected with the movements of subsurface lavas,
even when the connection is not demonstrable. Gradation includes all those
processes which tend to bring the surface of the lithosphere to a common
level. Gradational processes belong to two categories—those which level
down, degradation, and those which level up, aggradation. The
transportation of material from the land, whether by rain, rivers, glaciers,
waves, or winds, is degradation and the deposition of material, whether on
the land or in the sea, is aggradation. Degradation affects primarily the
protuberances of the lithosphere, while aggradation affects primarily its
depressions.
Astronomic Geology.
The earth as a planet.—Though supremely important to us, the earth is
but one of the minor planets attendant upon the sun, and is in no very
special way distinguished as a planetary body. Of the eight planets, four,
Jupiter, Saturn, Uranus, and Neptune, are much larger than the earth, while
three, Mars, Venus, and Mercury, are smaller. There are a host of asteroids,
but all together they do not equal the mass of the smallest planet. The
Page 31
average mass of the eight planets is more than fifty times that of the earth,
while the largest, Jupiter, is more than three hundred times as massive as the
earth. The earth’s position in the group is in no sense distinguished. It is
neither the outer nor the inner, nor even the middle planet. Even in the
minor group to which it belongs, it is neither the outermost nor the
innermost member, though in this group it is the largest. Its average
distance from the sun is about 92.9 million miles, and this fixes its
revolution at 365¼ days, for its period of revolution is directly dependent
on its distance from the sun, and is necessarily longer than the revolutions
of the inner planets and shorter than those of the outer planets. Its rotation
in twenty-four hours is not far different from that of its neighbor Mars, but
is much slower than the more distant and larger planets, Jupiter and Saturn,
which rotate in about ten hours. Comparison cannot be made with the
innermost and outermost planets, because their rotations are not yet
satisfactorily determined. The plane of the earth’s revolution lies near the
common plane of the whole system, but this is not peculiar, as all of the
planets revolve in nearly the same plane. Only a few of the small asteroids
depart notably from this common plane. This has an important bearing on
theories of the origin of the system, since this close coincidence of the
planes of the orbits is not consistent with any haphazard aggregation of the
material. Of similar importance is the fact that all of the planets revolve in
the same direction and in ellipses that do not depart widely from circles.
The eccentricity of the earth’s orbit is only about ¹⁄₆₀. This eccentricity
varies somewhat, due to the disturbing influences of the other planets, and
this variation has been regarded by some geologists as an influential cause
of climatic changes, but its adequacy to produce great effects has been
doubted by others. The inclination of the earth’s axis, now about 23½°,
holds an intermediate position, some of the planets having axes more
inclined, as Saturn, 26 ⅚ °, and others less inclined, as Jupiter, 3°. The
inclination of the axis is subject to trivial variations at present, and in the
long periods of the past has possibly changed more notably. This possible
change has also been thought to be a cause of climatic variation, but its
efficiency has not been demonstrated.
Its satellite.—The earth is peculiar in having one unusually large
satellite, which has a mass ¹⁄₈₁ of its own. The great planets have several
satellites whose combined mass exceeds that of the moon, and perhaps in
while the largest, Jupiter, is more than three hundred times as massive as the
earth. The earth’s position in the group is in no sense distinguished. It is
neither the outer nor the inner, nor even the middle planet. Even in the
minor group to which it belongs, it is neither the outermost nor the
innermost member, though in this group it is the largest. Its average
distance from the sun is about 92.9 million miles, and this fixes its
revolution at 365¼ days, for its period of revolution is directly dependent
on its distance from the sun, and is necessarily longer than the revolutions
of the inner planets and shorter than those of the outer planets. Its rotation
in twenty-four hours is not far different from that of its neighbor Mars, but
is much slower than the more distant and larger planets, Jupiter and Saturn,
which rotate in about ten hours. Comparison cannot be made with the
innermost and outermost planets, because their rotations are not yet
satisfactorily determined. The plane of the earth’s revolution lies near the
common plane of the whole system, but this is not peculiar, as all of the
planets revolve in nearly the same plane. Only a few of the small asteroids
depart notably from this common plane. This has an important bearing on
theories of the origin of the system, since this close coincidence of the
planes of the orbits is not consistent with any haphazard aggregation of the
material. Of similar importance is the fact that all of the planets revolve in
the same direction and in ellipses that do not depart widely from circles.
The eccentricity of the earth’s orbit is only about ¹⁄₆₀. This eccentricity
varies somewhat, due to the disturbing influences of the other planets, and
this variation has been regarded by some geologists as an influential cause
of climatic changes, but its adequacy to produce great effects has been
doubted by others. The inclination of the earth’s axis, now about 23½°,
holds an intermediate position, some of the planets having axes more
inclined, as Saturn, 26 ⅚ °, and others less inclined, as Jupiter, 3°. The
inclination of the axis is subject to trivial variations at present, and in the
long periods of the past has possibly changed more notably. This possible
change has also been thought to be a cause of climatic variation, but its
efficiency has not been demonstrated.
Its satellite.—The earth is peculiar in having one unusually large
satellite, which has a mass ¹⁄₈₁ of its own. The great planets have several
satellites whose combined mass exceeds that of the moon, and perhaps in
Page 32
some few cases the individual satellites may be larger than the moon, but
they do not sustain so large a ratio to their planets, for Titan, probably the
largest, is only ¹⁄₄₆₀₀ of the mass of Saturn. There is little doubt that the
moon has played an important part in the history of the earth. It is the chief
agency in developing oceanic tides, and it possibly also develops a body
tide in the earth itself. These tides act as a brake on the rotation of the earth
and tend to reduce its rate, and thereby to lengthen the day. While this may
have been counteracted in some measure by the shrinkage of the earth,
which tends to increase its rate of rotation, it has been held by eminent
physicists and geologists that the rotation of the earth has been greatly
lessened during its history, and that a long train of important consequences
has resulted. If the contraction of the earth has been sufficient to offset this
lessening, the tidal brake must be credited with the prevention of the
excessive speed of rotation which would otherwise have been developed.
The tides are efficient agencies in the shore wear of the oceans, and in the
distribution of marine sediments, and these, it will be seen later, are
important elements in the formation of strata.
Dependence on the sun.—By far the most important external relation of
the earth, however, is its dependence on the sun. The earth is a mere
satellite of the sun, less than ¹⁄₃₀₀₀₀₀ of its mass, and hence under its full
gravitative control. The earth is dependent on the sun for nearly all its heat
and light, and, through these, for nearly all of the activities that have given
character to its history. It is too much to say that all activities on the surface
of the earth are solely dependent on those of the sun, for a certain measure
of heat and light and other energy is derived from other bodies, and a
certain not inconsiderable source of energy is found in the interior of the
earth itself; yet all of these are so far subordinate to that great flood of
energy which comes from the sun that they are quite inconsequential. The
history of the earth in the past has been intimately dependent upon that of
the sun, and its future is locked up with the destiny of that great luminary.
Geology in its broadest phases can therefore scarcely be separated from the
study of the sun, but this falls within the function of the astronomer rather
than the geologist.
Meteorites.—There are a multitude of small bodies passing through
space in varying directions and with varying velocities and occasionally
encountering the earth, to which they add their substance. Some of these
they do not sustain so large a ratio to their planets, for Titan, probably the
largest, is only ¹⁄₄₆₀₀ of the mass of Saturn. There is little doubt that the
moon has played an important part in the history of the earth. It is the chief
agency in developing oceanic tides, and it possibly also develops a body
tide in the earth itself. These tides act as a brake on the rotation of the earth
and tend to reduce its rate, and thereby to lengthen the day. While this may
have been counteracted in some measure by the shrinkage of the earth,
which tends to increase its rate of rotation, it has been held by eminent
physicists and geologists that the rotation of the earth has been greatly
lessened during its history, and that a long train of important consequences
has resulted. If the contraction of the earth has been sufficient to offset this
lessening, the tidal brake must be credited with the prevention of the
excessive speed of rotation which would otherwise have been developed.
The tides are efficient agencies in the shore wear of the oceans, and in the
distribution of marine sediments, and these, it will be seen later, are
important elements in the formation of strata.
Dependence on the sun.—By far the most important external relation of
the earth, however, is its dependence on the sun. The earth is a mere
satellite of the sun, less than ¹⁄₃₀₀₀₀₀ of its mass, and hence under its full
gravitative control. The earth is dependent on the sun for nearly all its heat
and light, and, through these, for nearly all of the activities that have given
character to its history. It is too much to say that all activities on the surface
of the earth are solely dependent on those of the sun, for a certain measure
of heat and light and other energy is derived from other bodies, and a
certain not inconsiderable source of energy is found in the interior of the
earth itself; yet all of these are so far subordinate to that great flood of
energy which comes from the sun that they are quite inconsequential. The
history of the earth in the past has been intimately dependent upon that of
the sun, and its future is locked up with the destiny of that great luminary.
Geology in its broadest phases can therefore scarcely be separated from the
study of the sun, but this falls within the function of the astronomer rather
than the geologist.
Meteorites.—There are a multitude of small bodies passing through
space in varying directions and with varying velocities and occasionally
encountering the earth, to which they add their substance. Some of these
Page 33
meteorites revolve about the sun much as if they were minute planets, but
some of them come from such directions and with such velocities as to
show that they do not belong to the solar family. Some consist almost
wholly of metal, chiefly iron alloyed with a small percent. of nickel
(holosiderites); some consist of metal and rock intimately mixed
(syssiderites and sporadosiderites); and some consist wholly of rock
(asiderites). The rock is usually composed of the heavier basic minerals,
though some meteorites consist largely of carbonaceous material. Besides
meteorites, there is little doubt that wandering gaseous particles strike the
earth, but this is beyond the reach of present demonstration. The amount of
substance added to the earth by these meteorites and gases in recent times is
relatively slight compared with the whole body of the earth. What
contribution may have come to the earth in earlier times from such sources
is a matter of hypothesis which will be discussed later.
Geognosy.
The constitution of the earth.—Turning from its external relations to
the earth itself, a natural threefold division is presented: (1) the atmosphere,
(2) the hydrosphere, and (3) the lithosphere.
I. The Atmosphere.
The atmosphere is an intimate mixture of (1) all those substances that
cannot take a liquid or solid state at the temperatures and pressures which
prevail at the earth’s surface, together with (2) such transient vapors as the
various substances of the earth throw off. The first class form the permanent
gases of the atmosphere, and consist of nitrogen about 79 parts, oxygen
about 21 parts, carbon dioxide about .03 part, together with small quantities
of argon, neon, xenon, krypton, helium, and other rare constituents. The
second class are the transient and fluctuating constituents of the
atmosphere, chief among which is aqueous vapor, which varies greatly in
amount according to temperature, pressure, and other conditions. To this are
to be added volcanic emanations and a great variety of volatile organic
substances. Theoretically, every substance, however solid, discharges
particles which may transiently become constituents of the atmosphere.
Practically, only a few of these exist in such quantity as to be appreciable.
some of them come from such directions and with such velocities as to
show that they do not belong to the solar family. Some consist almost
wholly of metal, chiefly iron alloyed with a small percent. of nickel
(holosiderites); some consist of metal and rock intimately mixed
(syssiderites and sporadosiderites); and some consist wholly of rock
(asiderites). The rock is usually composed of the heavier basic minerals,
though some meteorites consist largely of carbonaceous material. Besides
meteorites, there is little doubt that wandering gaseous particles strike the
earth, but this is beyond the reach of present demonstration. The amount of
substance added to the earth by these meteorites and gases in recent times is
relatively slight compared with the whole body of the earth. What
contribution may have come to the earth in earlier times from such sources
is a matter of hypothesis which will be discussed later.
Geognosy.
The constitution of the earth.—Turning from its external relations to
the earth itself, a natural threefold division is presented: (1) the atmosphere,
(2) the hydrosphere, and (3) the lithosphere.
I. The Atmosphere.
The atmosphere is an intimate mixture of (1) all those substances that
cannot take a liquid or solid state at the temperatures and pressures which
prevail at the earth’s surface, together with (2) such transient vapors as the
various substances of the earth throw off. The first class form the permanent
gases of the atmosphere, and consist of nitrogen about 79 parts, oxygen
about 21 parts, carbon dioxide about .03 part, together with small quantities
of argon, neon, xenon, krypton, helium, and other rare constituents. The
second class are the transient and fluctuating constituents of the
atmosphere, chief among which is aqueous vapor, which varies greatly in
amount according to temperature, pressure, and other conditions. To this are
to be added volcanic emanations and a great variety of volatile organic
substances. Theoretically, every substance, however solid, discharges
particles which may transiently become constituents of the atmosphere.
Practically, only a few of these exist in such quantity as to be appreciable.
Page 34
Dust and other suspended matter are usually regarded as impurities rather
than constituents of the atmosphere, but they play a not unimportant part by
affecting its temperature and luminosity, and by facilitating the
condensation of moisture.
Mass and extent.—The total mass of the atmosphere is estimated at five
quadrillion tons, or ¹⁄₁₂₀₀₀₀₀ of the mass of the earth. It is relatively dense at
the surface of the earth and decreases in density outwards in a manner
difficult of absolute determination, so that the actual height of the
appreciable atmosphere is not positively known. The true conception of the
atmosphere is perhaps that of a tenuous envelope exerting a pressure of
about fifteen pounds per square inch at the sea-level, and thinning gradually
upwards until it reaches a tenuity which is inappreciable, but perhaps not
ceasing absolutely until the sphere of gravitative control of the earth is
passed, about 620,000 miles from the lithosphere. In the lower portion,
according to the kinetic theory of gases, the molecules fly to and fro,
colliding with each other with almost inconceivable frequency, and with
very short paths between successive collisions, but in the upper rare portion
some of the molecules bound outwards, and do not strike other molecules,
and hence pursue long elliptical paths until the gravity of the earth
overcomes their momentum, when they return, perhaps to bound off again
or to force other molecules to do so. This fountain-like nature of the outer
part of the atmosphere makes any sharp definition of its limit impracticable.
Some molecules are believed to be shot away at such speed that they do not
return. Beyond about 620,000 miles from the surface of the lithosphere, the
differential attraction of the sun is greater than that of the earth, and if the
attraction of the earth does not turn the molecules back before reaching this
distance, they are almost certain to be lost to the earth.
The measurement of heights by the aneroid barometer, which is much
used in practical geology, is dependent on the lessening of pressure as the
instrument is carried upward.
Geologic activity.—The atmosphere is the most mobile and active of the
three great subdivisions of the earth, and when its indirect effects through
the agency of water, as well as its direct effects, are considered, it is to be
regarded as one of the most effective agencies of change. It acts chemically
upon the rock substance of the earth, causing induration in some instances,
but more often inducing disintegration and change of composition by means
than constituents of the atmosphere, but they play a not unimportant part by
affecting its temperature and luminosity, and by facilitating the
condensation of moisture.
Mass and extent.—The total mass of the atmosphere is estimated at five
quadrillion tons, or ¹⁄₁₂₀₀₀₀₀ of the mass of the earth. It is relatively dense at
the surface of the earth and decreases in density outwards in a manner
difficult of absolute determination, so that the actual height of the
appreciable atmosphere is not positively known. The true conception of the
atmosphere is perhaps that of a tenuous envelope exerting a pressure of
about fifteen pounds per square inch at the sea-level, and thinning gradually
upwards until it reaches a tenuity which is inappreciable, but perhaps not
ceasing absolutely until the sphere of gravitative control of the earth is
passed, about 620,000 miles from the lithosphere. In the lower portion,
according to the kinetic theory of gases, the molecules fly to and fro,
colliding with each other with almost inconceivable frequency, and with
very short paths between successive collisions, but in the upper rare portion
some of the molecules bound outwards, and do not strike other molecules,
and hence pursue long elliptical paths until the gravity of the earth
overcomes their momentum, when they return, perhaps to bound off again
or to force other molecules to do so. This fountain-like nature of the outer
part of the atmosphere makes any sharp definition of its limit impracticable.
Some molecules are believed to be shot away at such speed that they do not
return. Beyond about 620,000 miles from the surface of the lithosphere, the
differential attraction of the sun is greater than that of the earth, and if the
attraction of the earth does not turn the molecules back before reaching this
distance, they are almost certain to be lost to the earth.
The measurement of heights by the aneroid barometer, which is much
used in practical geology, is dependent on the lessening of pressure as the
instrument is carried upward.
Geologic activity.—The atmosphere is the most mobile and active of the
three great subdivisions of the earth, and when its indirect effects through
the agency of water, as well as its direct effects, are considered, it is to be
regarded as one of the most effective agencies of change. It acts chemically
upon the rock substance of the earth, causing induration in some instances,
but more often inducing disintegration and change of composition by means
Page 35
of which rock is reduced to soil, or soil-like material, and rendered
susceptible of easy removal by winds and waters. When in motion the
atmosphere acts mechanically on the surface of the earth, transporting dust
and sand, and by the friction of these it abrades the surface. It is chiefly
effective, however, in furnishing the conditions for water action. Partly by
its mechanical aid, but chiefly by securing the right temperature, it is a
necessary factor in the action of rains, streams, glaciers, and the various
forms of moving water upon land. So also, on the ocean, wave action is
essentially dependent on the winds. In the absence of atmospheric
propulsion, wave action would be chiefly confined to the tides and to
occasional earthquake impulses, and would lose nearly all its efficiency.
Stream action and wave action, which are the most declared of the
geological agencies, are therefore to be credited as much to the atmosphere
as to the hydrosphere, since the action is a joint one to which both
envelopes are essential.
A thermal blanket.—A function of the atmosphere of supreme
importance is the thermal blanketing of the earth. In its absence the heat of
the sun would reach the surface with full intensity, and would be radiated
back from the surface almost as rapidly as received, and only a transient
heating would result. During the night an intensity of cold would intervene
scarcely less severe than the temperature of space. In penetrating the
atmosphere certain portions of the radiant energy of the sun are absorbed.
Of the remainder which reaches the surface of the earth, a part is
transformed into vibrations of lower intensity, which are then more
effectively retained by the atmosphere. The air thus distributes and
equalizes the temperature. The two constituents of the atmosphere which
are most efficient in this work are aqueous vapor and carbon dioxide, and
the climate of the earth is believed to have been very greatly affected by the
varying amounts of these constituents in the atmosphere, as well as by the
total mass of the atmosphere.
The function of the atmosphere in sustaining life and promoting all that
depends on life is too obvious to need comment.
The special geological action of the atmosphere will be discussed in the
next chapter.
II. The Hydrosphere.
susceptible of easy removal by winds and waters. When in motion the
atmosphere acts mechanically on the surface of the earth, transporting dust
and sand, and by the friction of these it abrades the surface. It is chiefly
effective, however, in furnishing the conditions for water action. Partly by
its mechanical aid, but chiefly by securing the right temperature, it is a
necessary factor in the action of rains, streams, glaciers, and the various
forms of moving water upon land. So also, on the ocean, wave action is
essentially dependent on the winds. In the absence of atmospheric
propulsion, wave action would be chiefly confined to the tides and to
occasional earthquake impulses, and would lose nearly all its efficiency.
Stream action and wave action, which are the most declared of the
geological agencies, are therefore to be credited as much to the atmosphere
as to the hydrosphere, since the action is a joint one to which both
envelopes are essential.
A thermal blanket.—A function of the atmosphere of supreme
importance is the thermal blanketing of the earth. In its absence the heat of
the sun would reach the surface with full intensity, and would be radiated
back from the surface almost as rapidly as received, and only a transient
heating would result. During the night an intensity of cold would intervene
scarcely less severe than the temperature of space. In penetrating the
atmosphere certain portions of the radiant energy of the sun are absorbed.
Of the remainder which reaches the surface of the earth, a part is
transformed into vibrations of lower intensity, which are then more
effectively retained by the atmosphere. The air thus distributes and
equalizes the temperature. The two constituents of the atmosphere which
are most efficient in this work are aqueous vapor and carbon dioxide, and
the climate of the earth is believed to have been very greatly affected by the
varying amounts of these constituents in the atmosphere, as well as by the
total mass of the atmosphere.
The function of the atmosphere in sustaining life and promoting all that
depends on life is too obvious to need comment.
The special geological action of the atmosphere will be discussed in the
next chapter.
II. The Hydrosphere.
Page 36
About 1300 quadrillion tons of water lie upon the surface of the solid
earth. This equals about ¹⁄₄₅₄₀ part of the earth’s mass. Were the surface of
the solid earth perfectly spheroidal, this would constitute a universal ocean
somewhat less than two miles deep. Owing to the inequalities of the rock
surface, the water is chiefly gathered into a series of great basins or troughs
occupying about three-fourths (72%) of the earth’s surface. These basins are
all connected with each other and act as a unit, so that anything which
changes the level of the water in one changes the level of all. This helps to
make a common record of all great movements of the earth’s body, for the
level of the ocean determines where the detritus from the land shall lodge,
and hence where the edge of the marine beds shall be formed. This will
appear more clearly when the formation of marine strata is discussed.
Oceanic dimensions.—The surface area of the ocean is estimated by
Murray at 143,259,300 square miles. Of this, somewhat more than
10,000,000 square miles lie on the continental shelf, i.e., lap up on the
borders of the continental platforms. This shows that the great basins are
somewhat more than full. If about 600 feet of the upper part of the ocean
were removed, the true ocean basins would be just full, and the surfaces of
the true continental platforms would be dry land. The area of the true
oceanic basins is about 133,000,000 square miles, and that of the true
continental platforms about 64,000,000 square miles. Under about 20% of
the ocean area, the bottom sinks to depths between 6000 and 12,000 feet;
under about 53% it sinks to depths between 12,000 and 18,000 feet; and
under the remaining 4% it ranges from 18,000 feet down to about 30,000.
The last includes those singular sunken areas known as “deeps,” and
sometimes called anti-plateaus, as they extend downward from the general
ocean bottom much as the plateaus protrude upwards from the general land
surface.
Besides the ocean, the hydrosphere includes all the water which
constitutes the surface streams and lakes, together with that which
permeates the pores and fissures of the outer part of the solid earth; but
altogether these are small in amount compared with the great ocean mass.
Geologic activity.—Of all geological agencies water is the most obvious
and apparently the greatest, though its efficiency is conditioned upon the
presence of the atmosphere, upon the relief of the land, and upon the radiant
energy of the sun. Through the agency of rainfall, of surface streams, of
earth. This equals about ¹⁄₄₅₄₀ part of the earth’s mass. Were the surface of
the solid earth perfectly spheroidal, this would constitute a universal ocean
somewhat less than two miles deep. Owing to the inequalities of the rock
surface, the water is chiefly gathered into a series of great basins or troughs
occupying about three-fourths (72%) of the earth’s surface. These basins are
all connected with each other and act as a unit, so that anything which
changes the level of the water in one changes the level of all. This helps to
make a common record of all great movements of the earth’s body, for the
level of the ocean determines where the detritus from the land shall lodge,
and hence where the edge of the marine beds shall be formed. This will
appear more clearly when the formation of marine strata is discussed.
Oceanic dimensions.—The surface area of the ocean is estimated by
Murray at 143,259,300 square miles. Of this, somewhat more than
10,000,000 square miles lie on the continental shelf, i.e., lap up on the
borders of the continental platforms. This shows that the great basins are
somewhat more than full. If about 600 feet of the upper part of the ocean
were removed, the true ocean basins would be just full, and the surfaces of
the true continental platforms would be dry land. The area of the true
oceanic basins is about 133,000,000 square miles, and that of the true
continental platforms about 64,000,000 square miles. Under about 20% of
the ocean area, the bottom sinks to depths between 6000 and 12,000 feet;
under about 53% it sinks to depths between 12,000 and 18,000 feet; and
under the remaining 4% it ranges from 18,000 feet down to about 30,000.
The last includes those singular sunken areas known as “deeps,” and
sometimes called anti-plateaus, as they extend downward from the general
ocean bottom much as the plateaus protrude upwards from the general land
surface.
Besides the ocean, the hydrosphere includes all the water which
constitutes the surface streams and lakes, together with that which
permeates the pores and fissures of the outer part of the solid earth; but
altogether these are small in amount compared with the great ocean mass.
Geologic activity.—Of all geological agencies water is the most obvious
and apparently the greatest, though its efficiency is conditioned upon the
presence of the atmosphere, upon the relief of the land, and upon the radiant
energy of the sun. Through the agency of rainfall, of surface streams, of
Page 37
underground waters, and of wave action, the hydrosphere is constantly
modifying the surface of the lithosphere, while at the same time it is bearing
into the various basins the wash of the land and depositing it in stratified
beds. It thereby becomes the great agency for the degradation of the land
and the building up of the basin bottoms. It works upon the land partly by
dissolving soluble portions of the rock substance, and partly by mechanical
action. The solution of the soluble part usually loosens the insoluble, and
renders it an easy prey of the surface waters. These transport the loosened
material to the valleys and at length to the great basins, meanwhile rolling
and grinding it and thus reducing it to rounder forms and a finer state, until
at length it reaches the still waters or the low gradients of the basins and
comes to rest. The hydrosphere is therefore both destructive and
constructive in its action. As the beds of sediment which it lays down
follow one another in orderly succession, each later one lying above each
earlier one, they form a time record. And as relics of the life of each age
become more or less imbedded in these sediments, they furnish the means
of following the history of life from age to age. The historical record of
geology is therefore very largely dependent upon the fact that the waters
have thus buried in systematic order the successive life of the ages. Aside
from this, the means of determining the order of events of the earth’s
history are limited and more or less uncertain.
The special processes of the hydrosphere in its various phases will be the
subject of discussion hereafter (Chaps. III, IV, VI). Suffice it here to
recognize its great function in the constant degradation of the land, and in
the deposition of the derived material in orderly succession in the basins.
Chief horizons of activity.—The great horizons of geological activity
are (1) the contact zone between the atmosphere and the hydrosphere,
chiefly the surface of the ocean, (2) the contact zone between the
hydrosphere and the lithosphere, chiefly the shore belts, and (3) the contact
zone of the atmosphere and surface waters, with the face of the continents.
It is in these three zones that the greatest external work is being done and
has been done in all the known ages.
III. The Lithosphere.
The atmosphere and hydrosphere are rather envelopes or shells than true
spheres, though in some degree both penetrate the lithosphere. The
modifying the surface of the lithosphere, while at the same time it is bearing
into the various basins the wash of the land and depositing it in stratified
beds. It thereby becomes the great agency for the degradation of the land
and the building up of the basin bottoms. It works upon the land partly by
dissolving soluble portions of the rock substance, and partly by mechanical
action. The solution of the soluble part usually loosens the insoluble, and
renders it an easy prey of the surface waters. These transport the loosened
material to the valleys and at length to the great basins, meanwhile rolling
and grinding it and thus reducing it to rounder forms and a finer state, until
at length it reaches the still waters or the low gradients of the basins and
comes to rest. The hydrosphere is therefore both destructive and
constructive in its action. As the beds of sediment which it lays down
follow one another in orderly succession, each later one lying above each
earlier one, they form a time record. And as relics of the life of each age
become more or less imbedded in these sediments, they furnish the means
of following the history of life from age to age. The historical record of
geology is therefore very largely dependent upon the fact that the waters
have thus buried in systematic order the successive life of the ages. Aside
from this, the means of determining the order of events of the earth’s
history are limited and more or less uncertain.
The special processes of the hydrosphere in its various phases will be the
subject of discussion hereafter (Chaps. III, IV, VI). Suffice it here to
recognize its great function in the constant degradation of the land, and in
the deposition of the derived material in orderly succession in the basins.
Chief horizons of activity.—The great horizons of geological activity
are (1) the contact zone between the atmosphere and the hydrosphere,
chiefly the surface of the ocean, (2) the contact zone between the
hydrosphere and the lithosphere, chiefly the shore belts, and (3) the contact
zone of the atmosphere and surface waters, with the face of the continents.
It is in these three zones that the greatest external work is being done and
has been done in all the known ages.
III. The Lithosphere.
The atmosphere and hydrosphere are rather envelopes or shells than true
spheres, though in some degree both penetrate the lithosphere. The
Page 38
lithosphere, on the other hand, is a nearly perfect oblate spheroid with a
polar diameter of 7899.7 miles, and an equatorial diameter of about 26.8
miles more. Its equatorial circumference is 24,902 miles, its meridional
circumference 24,860 miles, its surface area 196,940,700 square miles, its
volume 260,000,000,000 cubic miles, and its average specific gravity about
5.57. The oblateness of the spheroid is an accommodation to the rotation of
the earth, the centrifugal force at the equator being sufficient to cause the
specified amount of bulging there. Computations seem to indicate that the
accommodation is very nearly what would take place if the earth were in a
liquid condition, from which the inference has been drawn that it must have
been in that condition when it assumed this form, and must have continued
essentially liquid until it attained its present rate of rotation, since, if the
earth once rotated at a much higher speed, the flattening at the poles and the
bulging at the equator must have been correspondingly greater. It is thought
by others, however, that the plasticity of the earth is such that it would at all
times assume a close degree of approximation to the demands of rotation,
even if the interior were in a solid condition. By still others it is thought that
the contraction of the earth has tended to accelerate the rotation about as
much as the tides have tended to retard it, and that it has undergone little
change of form.
Irregularities.—It is only in a general view, however, that there is a
close approximation to a perfect spheroidal surface. In detail there are very
notable variations from it. Geodetic surveys seem to have shown that the
equatorial diameters are not all equal, even when the measurements are
reduced to sea-level, but research along this line has not reached a sufficient
stage of completeness to permit satisfactory discussion. It is, however,
highly probable that the ocean surface as well as the average land surface is
warped out of the perfect spheroidal form to some notable degree. This is
very likely due to inequalities in the density of the earth’s interior. The fact
that the larger portion of the water is gathered on one side of the globe,
while the land chiefly protrudes on the opposite side, is very possibly due to
unequal specific gravity in the interior of the earth.
The most obvious departure from a spheroidal form is found in the
protrusion of the continents and in the sinking away of the earth surface
under the oceans. As these inequalities present themselves to-day, they are
known as continental platforms and ocean basins. These do not correspond
polar diameter of 7899.7 miles, and an equatorial diameter of about 26.8
miles more. Its equatorial circumference is 24,902 miles, its meridional
circumference 24,860 miles, its surface area 196,940,700 square miles, its
volume 260,000,000,000 cubic miles, and its average specific gravity about
5.57. The oblateness of the spheroid is an accommodation to the rotation of
the earth, the centrifugal force at the equator being sufficient to cause the
specified amount of bulging there. Computations seem to indicate that the
accommodation is very nearly what would take place if the earth were in a
liquid condition, from which the inference has been drawn that it must have
been in that condition when it assumed this form, and must have continued
essentially liquid until it attained its present rate of rotation, since, if the
earth once rotated at a much higher speed, the flattening at the poles and the
bulging at the equator must have been correspondingly greater. It is thought
by others, however, that the plasticity of the earth is such that it would at all
times assume a close degree of approximation to the demands of rotation,
even if the interior were in a solid condition. By still others it is thought that
the contraction of the earth has tended to accelerate the rotation about as
much as the tides have tended to retard it, and that it has undergone little
change of form.
Irregularities.—It is only in a general view, however, that there is a
close approximation to a perfect spheroidal surface. In detail there are very
notable variations from it. Geodetic surveys seem to have shown that the
equatorial diameters are not all equal, even when the measurements are
reduced to sea-level, but research along this line has not reached a sufficient
stage of completeness to permit satisfactory discussion. It is, however,
highly probable that the ocean surface as well as the average land surface is
warped out of the perfect spheroidal form to some notable degree. This is
very likely due to inequalities in the density of the earth’s interior. The fact
that the larger portion of the water is gathered on one side of the globe,
while the land chiefly protrudes on the opposite side, is very possibly due to
unequal specific gravity in the interior of the earth.
The most obvious departure from a spheroidal form is found in the
protrusion of the continents and in the sinking away of the earth surface
under the oceans. As these inequalities present themselves to-day, they are
known as continental platforms and ocean basins. These do not correspond
Page 39
accurately with the present land and water surfaces. About the continental
lands there is a submerged border extending some distance out from the
shore, and constituting a sea-shelf beyond which the surface descends
rapidly to the great depths of the ocean. This slightly submerged portion,
known as the continental shelf, belongs as properly to the continent as the
adjacent low lands which are not submerged. The submergence of the edge
of this shelf at present is usually about 100 fathoms, so that if the upper 600
feet of the ocean were removed, the outlines of the land would correspond
quite closely with the border of the true continental platform.
BATHYMETRICAL CHART OF THE OCEANS
SHOWING THE “DEEPS” ACCORDING TO SIR JOHN MURRAY
It is customary to look upon the protrusions of the continents as the great
features of the earth’s surface, but in reality the oceanic depressions are the
master phenomena. In breadth, depth, and capacity they much exceed the
continental protrusions, and if the earth be regarded as a shrunken body, the
settling of the ocean bottoms has doubtless constituted its greatest surface
movement. From the estimates of Murray, Gilbert has derived the following
tables, showing the relative areas of the lithosphere above, below, and
between certain levels.[1]
lands there is a submerged border extending some distance out from the
shore, and constituting a sea-shelf beyond which the surface descends
rapidly to the great depths of the ocean. This slightly submerged portion,
known as the continental shelf, belongs as properly to the continent as the
adjacent low lands which are not submerged. The submergence of the edge
of this shelf at present is usually about 100 fathoms, so that if the upper 600
feet of the ocean were removed, the outlines of the land would correspond
quite closely with the border of the true continental platform.
BATHYMETRICAL CHART OF THE OCEANS
SHOWING THE “DEEPS” ACCORDING TO SIR JOHN MURRAY
It is customary to look upon the protrusions of the continents as the great
features of the earth’s surface, but in reality the oceanic depressions are the
master phenomena. In breadth, depth, and capacity they much exceed the
continental protrusions, and if the earth be regarded as a shrunken body, the
settling of the ocean bottoms has doubtless constituted its greatest surface
movement. From the estimates of Murray, Gilbert has derived the following
tables, showing the relative areas of the lithosphere above, below, and
between certain levels.[1]
Page 40
From these estimates it appears that if the surface were graded to a
common level by cutting away the continental platforms and dumping the
matter in the abysmal basins, the average plane would lie somewhere near
9000 feet below the sea-level. The continental platform may be conceived
as rising from this common plane rather than from the sea-level.
Percent. of Surface Percent. of Surface
Contours.
above. below.
Contour 24,000 feet above sea-level 0.004 99.996
“ 18,000 “ “ “ 0.09 99.91
“ 12,000 “ “ “ 0.7 99.3
“ 6,000 “ “ “ 2.3 97.7
Sea level 27.7 72.3
Contour 6,000 feet below sea-level 42.5 57.5
“ 12,000 “ “ “ 57.3 42.7
“ 18,000 “ “ “ 96.8 3.2
“ 24,000 “ “ “ 99.93 0.07
Percent.
More than 6000 feet above sea-level 2.3
Between sea-level and 6000 feet above 25.5
Between sea-level and 6000 feet below 14.8
Between 6000 and 12,000 feet below sea-level 14.8
Between 12,000 and 18,000 feet below sea-level 39.4
Between 18,000 feet and 24,000 feet 3.1
Epicontinental seas.—Those shallow portions of the sea which lie upon
the continental shelf, and those portions which extend into the interior of
the continent with like shallow depths, such as the Baltic Sea and the
Hudson Bay, may be called epicontinental seas, for they really lie upon the
continent, or at least upon the continental platform; while those other
detached bodies of water which occupy deep depressions in the surface are
to be regarded as true abysmal seas, as, for example, the Mediterranean and
Caribbean seas and the Gulf of Mexico, whose bottoms are as profound as
many parts of the true ocean basin itself.
Diversities of surface.—The bottoms of the oceanic basins are
diversified by broad undulations which range through many thousands of
feet, but they are not carved into the diversified forms that give variety to
land surfaces. The ocean bottoms are also diversified by volcanic peaks,
many of which rise to the surface and constitute isolated islands. Some of
them have notable platforms at or near the surface, cut by the waves or built
common level by cutting away the continental platforms and dumping the
matter in the abysmal basins, the average plane would lie somewhere near
9000 feet below the sea-level. The continental platform may be conceived
as rising from this common plane rather than from the sea-level.
Percent. of Surface Percent. of Surface
Contours.
above. below.
Contour 24,000 feet above sea-level 0.004 99.996
“ 18,000 “ “ “ 0.09 99.91
“ 12,000 “ “ “ 0.7 99.3
“ 6,000 “ “ “ 2.3 97.7
Sea level 27.7 72.3
Contour 6,000 feet below sea-level 42.5 57.5
“ 12,000 “ “ “ 57.3 42.7
“ 18,000 “ “ “ 96.8 3.2
“ 24,000 “ “ “ 99.93 0.07
Percent.
More than 6000 feet above sea-level 2.3
Between sea-level and 6000 feet above 25.5
Between sea-level and 6000 feet below 14.8
Between 6000 and 12,000 feet below sea-level 14.8
Between 12,000 and 18,000 feet below sea-level 39.4
Between 18,000 feet and 24,000 feet 3.1
Epicontinental seas.—Those shallow portions of the sea which lie upon
the continental shelf, and those portions which extend into the interior of
the continent with like shallow depths, such as the Baltic Sea and the
Hudson Bay, may be called epicontinental seas, for they really lie upon the
continent, or at least upon the continental platform; while those other
detached bodies of water which occupy deep depressions in the surface are
to be regarded as true abysmal seas, as, for example, the Mediterranean and
Caribbean seas and the Gulf of Mexico, whose bottoms are as profound as
many parts of the true ocean basin itself.
Diversities of surface.—The bottoms of the oceanic basins are
diversified by broad undulations which range through many thousands of
feet, but they are not carved into the diversified forms that give variety to
land surfaces. The ocean bottoms are also diversified by volcanic peaks,
many of which rise to the surface and constitute isolated islands. Some of
them have notable platforms at or near the surface, cut by the waves or built
Page 41
up by the accumulation of sediment and of coralline and other growths
about them. Aside from these encircling platforms, the solid surface usually
shelves rapidly down to abysmal depths, so that the islands constitute peaks
whose heights and slopes would seem extraordinary if the ocean were
removed.
The surface of the land is diversified in a similar way by broad
undulations and volcanic peaks, and also by narrower wrinklings and
foldings of the crust; but all of these irregularities have been carved into
diversified and picturesque forms by subaërial erosion. In this respect the
surface of the land differs radically from the bed of the sea. The agencies
which have produced the continental platforms and abysmal basins, and the
great undulations and foldings, as well as the volcanic extrusions that mark
them, are yet subjects of debate. Here lie some of the most difficult
problems of geology, but these cannot be stated with sufficient brevity to
find a place here.
The surface mantle of the lithosphere.—The surface of the lithosphere
is very generally mantled by a layer of loose material composed of soil,
clay, sand, gravel, and broken rock. This loose material is sometimes known
as mantle rock, and sometimes as rock waste. On the land, mantle rock is
often composed of the disintegrated products of underlying rock
formations. It represents the results of the recent action of the atmosphere,
of water, of changes of temperature, and of other physical agencies acting
on the outer part of the rock sphere. The surface of this mantle is being
constantly removed by wind and water, but as constantly renewed by
continued decomposition of the rock below. In some areas, especially in the
northern part of North America and the northwestern part of Europe, the
soil graduates down into an irregular sheet of mixed clay, sand, gravel, and
bowlders, known as drift. From this and other evidence it is inferred that at
a time not greatly antedating our own, ice, chiefly in the form of glaciers,
spread extensively over the high latitudes of the northern hemisphere. In
some parts of the earth the surface is still covered by fields of snow and ice,
comparable to those which formed the drift. In still other places, especially
along the flood plains of streams, the mantle rock consists of deposits made
by streams which were unable to carry their loads of sediment to the sea.
The crust of the lithosphere.—Much of the detritus washed down from
the land finds its way to bodies of standing water, and beneath lakes and
about them. Aside from these encircling platforms, the solid surface usually
shelves rapidly down to abysmal depths, so that the islands constitute peaks
whose heights and slopes would seem extraordinary if the ocean were
removed.
The surface of the land is diversified in a similar way by broad
undulations and volcanic peaks, and also by narrower wrinklings and
foldings of the crust; but all of these irregularities have been carved into
diversified and picturesque forms by subaërial erosion. In this respect the
surface of the land differs radically from the bed of the sea. The agencies
which have produced the continental platforms and abysmal basins, and the
great undulations and foldings, as well as the volcanic extrusions that mark
them, are yet subjects of debate. Here lie some of the most difficult
problems of geology, but these cannot be stated with sufficient brevity to
find a place here.
The surface mantle of the lithosphere.—The surface of the lithosphere
is very generally mantled by a layer of loose material composed of soil,
clay, sand, gravel, and broken rock. This loose material is sometimes known
as mantle rock, and sometimes as rock waste. On the land, mantle rock is
often composed of the disintegrated products of underlying rock
formations. It represents the results of the recent action of the atmosphere,
of water, of changes of temperature, and of other physical agencies acting
on the outer part of the rock sphere. The surface of this mantle is being
constantly removed by wind and water, but as constantly renewed by
continued decomposition of the rock below. In some areas, especially in the
northern part of North America and the northwestern part of Europe, the
soil graduates down into an irregular sheet of mixed clay, sand, gravel, and
bowlders, known as drift. From this and other evidence it is inferred that at
a time not greatly antedating our own, ice, chiefly in the form of glaciers,
spread extensively over the high latitudes of the northern hemisphere. In
some parts of the earth the surface is still covered by fields of snow and ice,
comparable to those which formed the drift. In still other places, especially
along the flood plains of streams, the mantle rock consists of deposits made
by streams which were unable to carry their loads of sediment to the sea.
The crust of the lithosphere.—Much of the detritus washed down from
the land finds its way to bodies of standing water, and beneath lakes and
Page 42
seas the mantle of loose material is made up largely of the gravel, sand, and
mud derived from the land. Before deposition these materials are more or
less assorted and arranged in layers by waves and currents. When
consolidated they constitute rock. The weathering of the rocks of the land,
the wearing away of the resulting detritus, and its deposition beneath
standing water, are among the most important processes of geologic change.
On the land, the mantle of loose material is sometimes absent, and in
such places the surface of solid rock of the crust appears. Bare surfaces of
rock are most commonly seen where the topography is rough, especially on
the slopes of steep-sided valleys and mountains, and on the slopes of cliffs
which face seas or lakes. Solid rock, without covering of soil or loose
material of any sort, is also frequently seen in the channels of streams,
especially where there are falls or rapids.
We have but to note the effects of a vigorous shower on a steep slope, or
of a swift stream on its channel, or of waves on the cliffs which face lakes
and seas, to understand at least one of the reasons why loose materials are
frequently absent from steep slopes. The very general exposure of solid
rock where conditions favor surface erosion suggests that rock is
everywhere present beneath the soil or subsoil. Fortunately there is an easy
way of testing the universality of the crust beneath the mantle. In all lands
inhabited by civilized peoples there are numerous wells and other
excavations ranging from a few feet to several hundred feet in depth, and
occasional wells and mine-shafts reach depths of several thousand feet.
Even in shallow excavations rock is often encountered, and in most regions
excavations as much as two or three hundred feet deep usually reach rock,
and no really deep boring has ever failed to find it. It may, therefore, be
accepted as a fact that the upper surface of the solid rock is nowhere far
below the surface.
Concerning the thickness of the crust, if there be any true crust at all,
little is known by direct observation. The deepest valleys, such as the
canyon of the Colorado, and the shafts and borings of the deepest mines and
wells, give knowledge of nothing but rock. The deepest excavations extend
rarely more than a mile below the surface. It is certain that rock of known
kinds extends to far greater depths.
mud derived from the land. Before deposition these materials are more or
less assorted and arranged in layers by waves and currents. When
consolidated they constitute rock. The weathering of the rocks of the land,
the wearing away of the resulting detritus, and its deposition beneath
standing water, are among the most important processes of geologic change.
On the land, the mantle of loose material is sometimes absent, and in
such places the surface of solid rock of the crust appears. Bare surfaces of
rock are most commonly seen where the topography is rough, especially on
the slopes of steep-sided valleys and mountains, and on the slopes of cliffs
which face seas or lakes. Solid rock, without covering of soil or loose
material of any sort, is also frequently seen in the channels of streams,
especially where there are falls or rapids.
We have but to note the effects of a vigorous shower on a steep slope, or
of a swift stream on its channel, or of waves on the cliffs which face lakes
and seas, to understand at least one of the reasons why loose materials are
frequently absent from steep slopes. The very general exposure of solid
rock where conditions favor surface erosion suggests that rock is
everywhere present beneath the soil or subsoil. Fortunately there is an easy
way of testing the universality of the crust beneath the mantle. In all lands
inhabited by civilized peoples there are numerous wells and other
excavations ranging from a few feet to several hundred feet in depth, and
occasional wells and mine-shafts reach depths of several thousand feet.
Even in shallow excavations rock is often encountered, and in most regions
excavations as much as two or three hundred feet deep usually reach rock,
and no really deep boring has ever failed to find it. It may, therefore, be
accepted as a fact that the upper surface of the solid rock is nowhere far
below the surface.
Concerning the thickness of the crust, if there be any true crust at all,
little is known by direct observation. The deepest valleys, such as the
canyon of the Colorado, and the shafts and borings of the deepest mines and
wells, give knowledge of nothing but rock. The deepest excavations extend
rarely more than a mile below the surface. It is certain that rock of known
kinds extends to far greater depths.
Page 43
The interior.—Concerning the great interior of the earth, little is known
except by inference. From the weight of the earth,[2] it is inferred that its
interior is much more dense than its surface. From its behavior under the
attraction of other bodies, it is believed to be at least as rigid as steel, and its
interior cannot, therefore, be liquid, in the usual sense of that term. From
the phenomena of volcanoes, and from observations on temperature in deep
borings, it is inferred that its interior is very hot. Further inferences
concerning its character are less simply stated, and will be referred to later.
The solid part of the earth is therefore composed of (1) a thin layer of
unconsolidated or earthy material, a few feet to a few hundred feet in
thickness, covering (2) a layer or zone many thousands of feet, and
probably many miles, thick, composed of solid rock comparable to that
exposed at numerous points on the surface, and (3) a central mass, to which
the preceding layers are but a shell, composed of hot, dense, and rigid rock,
the real nature of which is not known by observation.
Varieties of rock in crust.—If the mantle of soil, subsoil, and glacial
rubbish were stripped from the land, the surface beneath would be found to
be made up of a great variety of rocks, all of which may be grouped into
two great classes. About four-fifths of the land surface would be of rock
arranged in layers, and the other fifth would be of crystalline rock,
generally without distinct stratification, and often bearing evidence of the
effects of high temperature.
Stratified rocks.—The composition of most stratified rocks corresponds
somewhat closely with the composition of sediments now being carried
from the land and being deposited in the sea. Their arrangement in layers is
the same, and the markings on the surfaces of the layers, such as ripple-
marks, rill-marks, wave-marks, etc., are identical. Furthermore, the
stratified rocks of the land, like the recent sediments of the sea, frequently
contain the shells and skeletons of animals, and sometimes the impressions
of plants. Most of the relics of life found in the stratified rocks belonged to
animals or plants which lived in salt water. Because of their structure, their
composition, their distinctive markings, and the remains of life which they
contain, it is confidently inferred that most of the stratified rocks which lie
beneath the mantle rock of the land were originally laid down in beds
beneath the sea, and that the familiar processes of the present time furnish
the key to their history.
except by inference. From the weight of the earth,[2] it is inferred that its
interior is much more dense than its surface. From its behavior under the
attraction of other bodies, it is believed to be at least as rigid as steel, and its
interior cannot, therefore, be liquid, in the usual sense of that term. From
the phenomena of volcanoes, and from observations on temperature in deep
borings, it is inferred that its interior is very hot. Further inferences
concerning its character are less simply stated, and will be referred to later.
The solid part of the earth is therefore composed of (1) a thin layer of
unconsolidated or earthy material, a few feet to a few hundred feet in
thickness, covering (2) a layer or zone many thousands of feet, and
probably many miles, thick, composed of solid rock comparable to that
exposed at numerous points on the surface, and (3) a central mass, to which
the preceding layers are but a shell, composed of hot, dense, and rigid rock,
the real nature of which is not known by observation.
Varieties of rock in crust.—If the mantle of soil, subsoil, and glacial
rubbish were stripped from the land, the surface beneath would be found to
be made up of a great variety of rocks, all of which may be grouped into
two great classes. About four-fifths of the land surface would be of rock
arranged in layers, and the other fifth would be of crystalline rock,
generally without distinct stratification, and often bearing evidence of the
effects of high temperature.
Stratified rocks.—The composition of most stratified rocks corresponds
somewhat closely with the composition of sediments now being carried
from the land and being deposited in the sea. Their arrangement in layers is
the same, and the markings on the surfaces of the layers, such as ripple-
marks, rill-marks, wave-marks, etc., are identical. Furthermore, the
stratified rocks of the land, like the recent sediments of the sea, frequently
contain the shells and skeletons of animals, and sometimes the impressions
of plants. Most of the relics of life found in the stratified rocks belonged to
animals or plants which lived in salt water. Because of their structure, their
composition, their distinctive markings, and the remains of life which they
contain, it is confidently inferred that most of the stratified rocks which lie
beneath the mantle rock of the land were originally laid down in beds
beneath the sea, and that the familiar processes of the present time furnish
the key to their history.
Page 44
Fig. 1.—Beds of (Cambrian) sandstone, a, are conformable with one another, but
unconformable on beds of (Huronian) quartzite, b, Near Ableman, Wis.
Conformability.—When the stratified rocks exposed by the removal of
the mantle rock are examined, the successive beds are sometimes found to
lie on one another in regular succession, showing that they were laid down
one after another, without change in the attitude of the surface on which
they were deposited. Such rocks are conformable (the beds of series a, Fig.
1). In other cases it would be seen that certain beds overlie the worn
surfaces of lower beds, the layers of which may have a different angle of
inclination (series a, Fig. 1, is unconformable on series b). Such relations
show that the lower series of beds was disturbed and eroded before the
overlying beds were deposited on them. Such series of rocks are
unconformable.
Relative ages.—The structure and relations of rocks lead to inferences as
to their relative ages. In the case of stratified rocks it is obvious that
overlying beds were deposited later than those below, and where there is
unconformity it is evident that an interval of time elapsed between the
deposition of the unconformable series. Another and in some respects more
important means of telling their order of formation is found in the remains
of life entrapped in the water-laid sediments. Whatever life existed in the
waters in which the sediments were deposited was liable to burial, and if it
was possessed of hard parts, such as bones, teeth, shells, hard integuments,
etc., these parts, or at least their impressions, were likely to be preserved in
the sediments. Even tracks and imprints of perishable parts are sometimes
preserved. All these relics, which we call fossils, give indications of the
unconformable on beds of (Huronian) quartzite, b, Near Ableman, Wis.
Conformability.—When the stratified rocks exposed by the removal of
the mantle rock are examined, the successive beds are sometimes found to
lie on one another in regular succession, showing that they were laid down
one after another, without change in the attitude of the surface on which
they were deposited. Such rocks are conformable (the beds of series a, Fig.
1). In other cases it would be seen that certain beds overlie the worn
surfaces of lower beds, the layers of which may have a different angle of
inclination (series a, Fig. 1, is unconformable on series b). Such relations
show that the lower series of beds was disturbed and eroded before the
overlying beds were deposited on them. Such series of rocks are
unconformable.
Relative ages.—The structure and relations of rocks lead to inferences as
to their relative ages. In the case of stratified rocks it is obvious that
overlying beds were deposited later than those below, and where there is
unconformity it is evident that an interval of time elapsed between the
deposition of the unconformable series. Another and in some respects more
important means of telling their order of formation is found in the remains
of life entrapped in the water-laid sediments. Whatever life existed in the
waters in which the sediments were deposited was liable to burial, and if it
was possessed of hard parts, such as bones, teeth, shells, hard integuments,
etc., these parts, or at least their impressions, were likely to be preserved in
the sediments. Even tracks and imprints of perishable parts are sometimes
preserved. All these relics, which we call fossils, give indications of the
Page 45
kinds of life which existed when the beds were formed. The fossils of the
youngest beds show that the life which existed when they were deposited
was quite like that of the present time. The fossils of the next older and
lower beds show greater departure from present types. This series of
changes continues downward as lower and lower beds are studied, until
beds at considerable depths contain no relics of existing species but, in lieu
thereof, forms of more primitive types. Some of these earlier types are
clearly the ancestors of more modern forms, while others seem to have no
living descendants. Going still deeper, the fossils indicate life of more and
more primitive types, until they depart very widely from the living forms,
and seem to be but remotely ancestral. So the beds may be followed
downward until the lowest, which contain distinct evidences of life, are
reached.
It should be understood that it is not possible to proceed directly
downward through the whole succession of bedded rocks, but that the edges
of the various beds may be found here and there where they have been
brought to the surface by warpings or tiltings, or exposed by the wearing
away of the beds which once overlay them. The full series of strata is made
out only by putting together the data gathered throughout all lands, and
even when this is done an absolutely complete series cannot yet be made
out or, at least, has not been.
The crystalline rocks.—The crystalline rocks which would appear if the
mantle rock were removed are of two types, igneous and metamorphic.
Igneous rocks may be loosely defined as hardened lavas. Metamorphic
rocks are those which are greatly changed from their original condition.
Either stratified or igneous rocks may become metamorphic.
Igneous rocks sustain various relations to the stratified rocks, as
illustrated by Fig. 2. From these relations it is possible to tell something of
the order of their formation. Where the stratified rocks are broken through
by lavas, it is obvious that the stratified rocks were formed first, and the
lavas intruded later. Lava sheets intruded between beds of stratified rock
can be told from those which flowed out on the surface and were
subsequently buried, for in the former case the sedimentary rocks, both
above and below the igneous rock, were affected by the heat, while in the
latter case only those below were so affected.
youngest beds show that the life which existed when they were deposited
was quite like that of the present time. The fossils of the next older and
lower beds show greater departure from present types. This series of
changes continues downward as lower and lower beds are studied, until
beds at considerable depths contain no relics of existing species but, in lieu
thereof, forms of more primitive types. Some of these earlier types are
clearly the ancestors of more modern forms, while others seem to have no
living descendants. Going still deeper, the fossils indicate life of more and
more primitive types, until they depart very widely from the living forms,
and seem to be but remotely ancestral. So the beds may be followed
downward until the lowest, which contain distinct evidences of life, are
reached.
It should be understood that it is not possible to proceed directly
downward through the whole succession of bedded rocks, but that the edges
of the various beds may be found here and there where they have been
brought to the surface by warpings or tiltings, or exposed by the wearing
away of the beds which once overlay them. The full series of strata is made
out only by putting together the data gathered throughout all lands, and
even when this is done an absolutely complete series cannot yet be made
out or, at least, has not been.
The crystalline rocks.—The crystalline rocks which would appear if the
mantle rock were removed are of two types, igneous and metamorphic.
Igneous rocks may be loosely defined as hardened lavas. Metamorphic
rocks are those which are greatly changed from their original condition.
Either stratified or igneous rocks may become metamorphic.
Igneous rocks sustain various relations to the stratified rocks, as
illustrated by Fig. 2. From these relations it is possible to tell something of
the order of their formation. Where the stratified rocks are broken through
by lavas, it is obvious that the stratified rocks were formed first, and the
lavas intruded later. Lava sheets intruded between beds of stratified rock
can be told from those which flowed out on the surface and were
subsequently buried, for in the former case the sedimentary rocks, both
above and below the igneous rock, were affected by the heat, while in the
latter case only those below were so affected.
Page 46
Fig. 2.—Diagrammatic representation of the relations of igneous rock to stratified rock.
The igneous rocks, represented in black, have been forced up from beneath.
More commonly than otherwise the metamorphic rocks (Fig. 3) lie
beneath the sedimentary beds and are often broken through by the igneous
rocks. From their position in many places their great age may be inferred,
but locally, especially where dynamic action has been severe, relatively
young rocks are metamorphic.
Fig. 3. The figure represents a section of the earth about 1000 miles Long. The unequally
thick black line at the top represents on something like its proper scale the depth of the
stratified rock. The area below represents crystalline rock, largely metamorphic.
Four great sedimentary eras.—The water-laid series represents four
great eras in the history of the earth, as shown by the relics of life imbedded
in them. Beginning with the latest, these are the Cenozoic (recent life),
during which the life took on its modern aspect; the Mesozoic (middle life),
during which the life bore a mediæval aspect; the Paleozoic (ancient life),
during which the life belonged to older types; and the Proterozoic (earlier
life), during which it is inferred that much life prevailed, though its record
is very imperfect. It may safely be assumed to have been more primitive
than that of the Paleozoic, as it was earlier. Each of these great divisions
embraced several lesser periods or epochs, and these again are subdivided
more and more closely according to the degrees of refinement to which
studies are carried. The chief of these subdivisions are given in the table on
page 19, and others will come under consideration in the historical chapters.
In these four great series of sedimentary rocks there are, here and there,
intrusions of igneous rocks, and in some places the sedimentary beds have
been metamorphosed into crystalline rocks by heat and pressure. This is
particularly true in the lowest of these series, the Proterozoic, where a large
The igneous rocks, represented in black, have been forced up from beneath.
More commonly than otherwise the metamorphic rocks (Fig. 3) lie
beneath the sedimentary beds and are often broken through by the igneous
rocks. From their position in many places their great age may be inferred,
but locally, especially where dynamic action has been severe, relatively
young rocks are metamorphic.
Fig. 3. The figure represents a section of the earth about 1000 miles Long. The unequally
thick black line at the top represents on something like its proper scale the depth of the
stratified rock. The area below represents crystalline rock, largely metamorphic.
Four great sedimentary eras.—The water-laid series represents four
great eras in the history of the earth, as shown by the relics of life imbedded
in them. Beginning with the latest, these are the Cenozoic (recent life),
during which the life took on its modern aspect; the Mesozoic (middle life),
during which the life bore a mediæval aspect; the Paleozoic (ancient life),
during which the life belonged to older types; and the Proterozoic (earlier
life), during which it is inferred that much life prevailed, though its record
is very imperfect. It may safely be assumed to have been more primitive
than that of the Paleozoic, as it was earlier. Each of these great divisions
embraced several lesser periods or epochs, and these again are subdivided
more and more closely according to the degrees of refinement to which
studies are carried. The chief of these subdivisions are given in the table on
page 19, and others will come under consideration in the historical chapters.
In these four great series of sedimentary rocks there are, here and there,
intrusions of igneous rocks, and in some places the sedimentary beds have
been metamorphosed into crystalline rocks by heat and pressure. This is
particularly true in the lowest of these series, the Proterozoic, where a large
Page 47
part of the sediment is metamorphosed, and where there is much igneous
rock, but it is still clear that the main portion of this series was originally
water-laid sediment, and so it belongs to the sedimentary series rather than
the Archean, in which the sediments are the minor rather than the main
factor. It has, however, usually been classed with the Archean, and it is
certainly not always easy to draw the dividing line. In a sense it may be
regarded as a transition series.
The Archean complex.—Beneath the dominantly sedimentary but partly
metamorphic and igneous series there is a very complex group of rocks
largely of metamorphosed igneous origin, though containing some
metamorphosed sediments. These extend downwards to unknown depths.
While all the great formations are occasionally bent and broken, these
lowest ones are almost everywhere warped, folded, and contorted, often in
the most intricate way. They have been very generally mashed and sheared
by enormous pressure, so that they have become foliated, and their original
character is much masked. They therefore form a series of great obscurity
and complexity. As they are at the bottom of the known series, they have
been called the “Fundamental gneiss” and the “Basement complex,” but as
the part which we see is not the true base nor the true foundation, it is safer
to call them simply the Archean (very ancient) complex. As life appears to
have been present during a part at least of the period of its formation is
referred to the Archeozoic era.
Fig. 4.—Diagram to illustrate the relations of the five great groups of formations.
AR = Archean, Pr = Proterozoic, P = Paleozoic, M = Mesozoic, C = Cenozoic.
Beyond and below this series, the structure of the earth is a matter of
inference. Vast as are the preceding series, they together form relatively but
a thin shell on the outer surface of the globe.
The foregoing series are diagrammatically expressed in Fig. 4, and
systematically presented to the eye in the following table.
GENERAL TABLE OF GEOLOGIC DIVISIONS.
Cenozoic Present.
rock, but it is still clear that the main portion of this series was originally
water-laid sediment, and so it belongs to the sedimentary series rather than
the Archean, in which the sediments are the minor rather than the main
factor. It has, however, usually been classed with the Archean, and it is
certainly not always easy to draw the dividing line. In a sense it may be
regarded as a transition series.
The Archean complex.—Beneath the dominantly sedimentary but partly
metamorphic and igneous series there is a very complex group of rocks
largely of metamorphosed igneous origin, though containing some
metamorphosed sediments. These extend downwards to unknown depths.
While all the great formations are occasionally bent and broken, these
lowest ones are almost everywhere warped, folded, and contorted, often in
the most intricate way. They have been very generally mashed and sheared
by enormous pressure, so that they have become foliated, and their original
character is much masked. They therefore form a series of great obscurity
and complexity. As they are at the bottom of the known series, they have
been called the “Fundamental gneiss” and the “Basement complex,” but as
the part which we see is not the true base nor the true foundation, it is safer
to call them simply the Archean (very ancient) complex. As life appears to
have been present during a part at least of the period of its formation is
referred to the Archeozoic era.
Fig. 4.—Diagram to illustrate the relations of the five great groups of formations.
AR = Archean, Pr = Proterozoic, P = Paleozoic, M = Mesozoic, C = Cenozoic.
Beyond and below this series, the structure of the earth is a matter of
inference. Vast as are the preceding series, they together form relatively but
a thin shell on the outer surface of the globe.
The foregoing series are diagrammatically expressed in Fig. 4, and
systematically presented to the eye in the following table.
GENERAL TABLE OF GEOLOGIC DIVISIONS.
Cenozoic Present.
Page 48
Pleistocene.
Pliocene.
Miocene.
Oligocene.
Eocene.
Transition (Arapahoe and Denver).
Upper Cretaceous.
Lower Cretaceous (Comanche or Shastan).
Mesozoic
Jurassic.
Triassic.
Permian.
Coal Measures or Pennsylvanian.
Subcarboniferous, or Mississippian.
Paleozoic Silurian.
Devonian.
Ordovician.
Cambrian.
Great interval.
Keweenawan.
Interval.
Animikean or Penokean.
Proterozoic
(Upper Huronian of some authors).
Interval.
Huronian.
Great interval.
Archeozoic Archean Great Granitoid Series.
Complex. (Intrusive in the main,
Laurentian.)
Great Schist Series.
(Mona, Kitchi, Lower Keewatin,
Pliocene.
Miocene.
Oligocene.
Eocene.
Transition (Arapahoe and Denver).
Upper Cretaceous.
Lower Cretaceous (Comanche or Shastan).
Mesozoic
Jurassic.
Triassic.
Permian.
Coal Measures or Pennsylvanian.
Subcarboniferous, or Mississippian.
Paleozoic Silurian.
Devonian.
Ordovician.
Cambrian.
Great interval.
Keweenawan.
Interval.
Animikean or Penokean.
Proterozoic
(Upper Huronian of some authors).
Interval.
Huronian.
Great interval.
Archeozoic Archean Great Granitoid Series.
Complex. (Intrusive in the main,
Laurentian.)
Great Schist Series.
(Mona, Kitchi, Lower Keewatin,
Page 49
Coutchiching, Lower Huronian of
some authors.)
The purpose of this general survey is to bring the salient features of the
earth’s structure into view preparatory to entering in more detail into the
study of particular processes and special formations and to lay a foundation
for the fuller apprehension of the successive stages of the history of the
earth, which constitutes the chief purpose of geological study. It is now
advisable to turn to the detailed consideration of individual processes and
specific structures. The complexity of the actions involved in the history of
the earth is so great that such separate consideration at the outset is helpful.
some authors.)
The purpose of this general survey is to bring the salient features of the
earth’s structure into view preparatory to entering in more detail into the
study of particular processes and special formations and to lay a foundation
for the fuller apprehension of the successive stages of the history of the
earth, which constitutes the chief purpose of geological study. It is now
advisable to turn to the detailed consideration of individual processes and
specific structures. The complexity of the actions involved in the history of
the earth is so great that such separate consideration at the outset is helpful.
Page 50
CHAPTER II.
THE ATMOSPHERE AS A GEOLOGICAL AGENT.
While it is convenient to regard the lithosphere as the earth proper, and
the atmosphere as its envelope, the latter is as truly a part of the planet as
the former, and its activities and its history are as truly subjects of
geological study as the formation of the rocks. This view is in no way
vitiated by the fact that the special study of the atmosphere is set apart
under the name Meteorology, for in the same way the special study of rocks
is set apart under the name Petrology, that of ancient life under the name
Paleontology, and that of other phases of the subject under other names.
The atmosphere is one of the three great formations of the earth, and as a
geological factor takes its place beside the hydrosphere and the lithosphere.
It has played a part in the history of the earth comparable to that of the
water, though its mass is less and its record more elusive. Unsubstantial as
the atmosphere seems when contrasted with the liquid and solid portions of
the earth, its extreme mobility and its chemical activity compensate for its
lightness and tenuity, and give it a function of the first order of importance.
The atmosphere plays a direct part as (1) a mechanical and (2) a chemical
agent, and at the same time serves an indirect function in furnishing
favorable conditions under which (3) solar radiation produces temperature
effects, and (4) evaporation gives origin to precipitation and stream effects,
and furnishes the necessary conditions for land plants and animals, and the
important influences that spring from them.
This chapter is devoted to the work of the atmosphere in these and some
less notable phases. The consideration of the origin and history of the
atmosphere will receive attention later.
A. THE ATMOSPHERE AS A DIRECT AGENCY.
I. Mechanical Work.
THE ATMOSPHERE AS A GEOLOGICAL AGENT.
While it is convenient to regard the lithosphere as the earth proper, and
the atmosphere as its envelope, the latter is as truly a part of the planet as
the former, and its activities and its history are as truly subjects of
geological study as the formation of the rocks. This view is in no way
vitiated by the fact that the special study of the atmosphere is set apart
under the name Meteorology, for in the same way the special study of rocks
is set apart under the name Petrology, that of ancient life under the name
Paleontology, and that of other phases of the subject under other names.
The atmosphere is one of the three great formations of the earth, and as a
geological factor takes its place beside the hydrosphere and the lithosphere.
It has played a part in the history of the earth comparable to that of the
water, though its mass is less and its record more elusive. Unsubstantial as
the atmosphere seems when contrasted with the liquid and solid portions of
the earth, its extreme mobility and its chemical activity compensate for its
lightness and tenuity, and give it a function of the first order of importance.
The atmosphere plays a direct part as (1) a mechanical and (2) a chemical
agent, and at the same time serves an indirect function in furnishing
favorable conditions under which (3) solar radiation produces temperature
effects, and (4) evaporation gives origin to precipitation and stream effects,
and furnishes the necessary conditions for land plants and animals, and the
important influences that spring from them.
This chapter is devoted to the work of the atmosphere in these and some
less notable phases. The consideration of the origin and history of the
atmosphere will receive attention later.
A. THE ATMOSPHERE AS A DIRECT AGENCY.
I. Mechanical Work.
Page 51
The mechanical work of the atmosphere is accomplished chiefly through
its movement. A feeble breeze is competent to move particles of dust, and
winds of moderate velocity to shift sand. Exceptionally strong winds
sometimes move small pebbles, but winds of sufficient force to move larger
pieces of rock are rare. It follows, therefore, that the impact of the wind has
little direct effect except on surfaces covered with dust and dry sand.
The transportation of material by the wind is limited by the size of the
particles to which it has access. Dust particles expose more surface to the
wind relative to their mass than sand grains. Winds which are unable to
carry sand may still carry dust, and winds which are able to shift sand no
more than a trivial distance may blow dust great distances.
The common conception of wind as a horizontal movement of some part
of the atmosphere is not altogether accurate. Every obstacle against which
wind blows causes deflections of its currents, and some of these deflections
are upward. Furthermore, there are exceptional winds, in which the vertical
element predominates. Particles of dust are often involved in these upward
currents, and by them carried to great heights, and in the upper air are
transported great distances.
Transportation and deposition of dust.[3]—The universality of the
transportation of dust by the wind is well known. No house, no room, and
scarcely a drawer can be so tightly closed but that dust enters it, and the
movements of dust in the open must be much more considerable. The
visible dustiness of the atmosphere in dry regions during wind-storms is
adequate and familiar proof of the efficiency of the wind as a transporter of
dust.
Under special circumstances, opportunity is afforded for rough
determinations of the distance and height to which wind-blown dust is
transported. Snow taken from snow-fields in high mountain regions is
found to contain a small amount of earthy matter. Its particles are often
found to be in part volcanic, even when the place whence the snow was
taken is scores or even hundreds of miles from the nearest volcano. There is
probably no snow-field so high, or so far from volcanoes, but that volcanic
dust reaches it. If this be true of all snow-fields, it is probably true of all
land surfaces. In the great Krakatoa[4] eruptions of 1883 large quantities of
volcanic ash (pulverized lava) were projected to great heights into the
its movement. A feeble breeze is competent to move particles of dust, and
winds of moderate velocity to shift sand. Exceptionally strong winds
sometimes move small pebbles, but winds of sufficient force to move larger
pieces of rock are rare. It follows, therefore, that the impact of the wind has
little direct effect except on surfaces covered with dust and dry sand.
The transportation of material by the wind is limited by the size of the
particles to which it has access. Dust particles expose more surface to the
wind relative to their mass than sand grains. Winds which are unable to
carry sand may still carry dust, and winds which are able to shift sand no
more than a trivial distance may blow dust great distances.
The common conception of wind as a horizontal movement of some part
of the atmosphere is not altogether accurate. Every obstacle against which
wind blows causes deflections of its currents, and some of these deflections
are upward. Furthermore, there are exceptional winds, in which the vertical
element predominates. Particles of dust are often involved in these upward
currents, and by them carried to great heights, and in the upper air are
transported great distances.
Transportation and deposition of dust.[3]—The universality of the
transportation of dust by the wind is well known. No house, no room, and
scarcely a drawer can be so tightly closed but that dust enters it, and the
movements of dust in the open must be much more considerable. The
visible dustiness of the atmosphere in dry regions during wind-storms is
adequate and familiar proof of the efficiency of the wind as a transporter of
dust.
Under special circumstances, opportunity is afforded for rough
determinations of the distance and height to which wind-blown dust is
transported. Snow taken from snow-fields in high mountain regions is
found to contain a small amount of earthy matter. Its particles are often
found to be in part volcanic, even when the place whence the snow was
taken is scores or even hundreds of miles from the nearest volcano. There is
probably no snow-field so high, or so far from volcanoes, but that volcanic
dust reaches it. If this be true of all snow-fields, it is probably true of all
land surfaces. In the great Krakatoa[4] eruptions of 1883 large quantities of
volcanic ash (pulverized lava) were projected to great heights into the
Page 52
atmosphere. The coarser particles soon settled; but, caught by the currents
of the upper atmosphere, many of the finer particles were transported
incredible distances. Through all their long journey, the particles of dust
were gradually settling from the atmosphere, but not until the dust had
traveled repeatedly round the earth did its amount become so small as to
cease to make its influence felt in the historic red sunsets which it
occasioned.[5] Some of this dust completed the circuit of the earth in 15
days.
In various parts of Kansas and Nebraska[6] there are very considerable
beds of volcanic dust, locally as much as 30 feet thick, which must have
been transported from volcanic vents by the wind, though there are no
known centers of volcanic action, past or present, within some hundreds of
miles of some of the localities where the dust occurs. These beds of
volcanic dust, so far from its source, may serve as an illustration of the
importance of atmospheric movements as a geological force.
Volcanic dust is shot into the atmosphere rather than picked up by it. Dust
picked up by the wind is perhaps transported not less widely than volcanic
dust, but, after settling, its point of origin is less readily determined. It
would perhaps be an exaggeration to say that every square mile of land
surface contains particles of dust brought to it by the wind from every other
square mile, but such a statement would probably involve much less
exaggeration than might at first be supposed.
Examples of extensive deposits of dust other than volcanic are also
known. In China there is an extensive earthy formation, the loess,
sometimes reaching 1,000 feet in thickness, which von Richtofen believes
to have been deposited by the wind.[7] This conclusion has, however, not
passed unchallenged.[8] The loess of some other regions has been referred to
the same origin, and some of it is quite certainly eolian.[9]
The transportation of dust is important wherever strong winds blow over
dry surfaces, free or nearly free of vegetation, and composed of earthy
matter. Its effects may be seen in such regions as the sage-brush plains of
western North America. The roots of the sage-brush hold the soil
immediately about them, but between the clumps of brush, where there is
little other vegetation, the wind has often blown away the soil to such an
extent that each clump of brush stands up several inches, or even a foot or
of the upper atmosphere, many of the finer particles were transported
incredible distances. Through all their long journey, the particles of dust
were gradually settling from the atmosphere, but not until the dust had
traveled repeatedly round the earth did its amount become so small as to
cease to make its influence felt in the historic red sunsets which it
occasioned.[5] Some of this dust completed the circuit of the earth in 15
days.
In various parts of Kansas and Nebraska[6] there are very considerable
beds of volcanic dust, locally as much as 30 feet thick, which must have
been transported from volcanic vents by the wind, though there are no
known centers of volcanic action, past or present, within some hundreds of
miles of some of the localities where the dust occurs. These beds of
volcanic dust, so far from its source, may serve as an illustration of the
importance of atmospheric movements as a geological force.
Volcanic dust is shot into the atmosphere rather than picked up by it. Dust
picked up by the wind is perhaps transported not less widely than volcanic
dust, but, after settling, its point of origin is less readily determined. It
would perhaps be an exaggeration to say that every square mile of land
surface contains particles of dust brought to it by the wind from every other
square mile, but such a statement would probably involve much less
exaggeration than might at first be supposed.
Examples of extensive deposits of dust other than volcanic are also
known. In China there is an extensive earthy formation, the loess,
sometimes reaching 1,000 feet in thickness, which von Richtofen believes
to have been deposited by the wind.[7] This conclusion has, however, not
passed unchallenged.[8] The loess of some other regions has been referred to
the same origin, and some of it is quite certainly eolian.[9]
The transportation of dust is important wherever strong winds blow over
dry surfaces, free or nearly free of vegetation, and composed of earthy
matter. Its effects may be seen in such regions as the sage-brush plains of
western North America. The roots of the sage-brush hold the soil
immediately about them, but between the clumps of brush, where there is
little other vegetation, the wind has often blown away the soil to such an
extent that each clump of brush stands up several inches, or even a foot or
Page 53
two, above its surroundings (Fig. 5). Such mounds are often partly due to
the lodgment of dust about the bushes.
Fig. 5.—This figure shows the effect of sage-brush or other similar vegetation in holding
sand or earth, or in causing its lodgment, in dry regions.
Where the earthy matter is moist, the cohesion of the particles is great,
and the wind cannot pick them up. Furthermore, if the surface is generally
moist, it is likely to be covered with vegetation which protects it against the
wind. But even where vegetation is prevalent the wind finds many a
vulnerable point. Thus on the edges of plains or plateaus facing abrupt
valleys, the wind attacks the soil from the side, and in such situations all
earthy matter may be stripped from the underlying rock for considerable
distances from the edge of the cliff (Fig. 6). This may be seen at numerous
points on the lava plateaus of Washington.
Fig. 6.—Diagram to illustrate the way in which the wind sometimes strips the soil from the
edge of a bluff. This phenomenon is not rare in the basin of the Columbia River in
Washington.
the lodgment of dust about the bushes.
Fig. 5.—This figure shows the effect of sage-brush or other similar vegetation in holding
sand or earth, or in causing its lodgment, in dry regions.
Where the earthy matter is moist, the cohesion of the particles is great,
and the wind cannot pick them up. Furthermore, if the surface is generally
moist, it is likely to be covered with vegetation which protects it against the
wind. But even where vegetation is prevalent the wind finds many a
vulnerable point. Thus on the edges of plains or plateaus facing abrupt
valleys, the wind attacks the soil from the side, and in such situations all
earthy matter may be stripped from the underlying rock for considerable
distances from the edge of the cliff (Fig. 6). This may be seen at numerous
points on the lava plateaus of Washington.
Fig. 6.—Diagram to illustrate the way in which the wind sometimes strips the soil from the
edge of a bluff. This phenomenon is not rare in the basin of the Columbia River in
Washington.
Page 54
The presence of dust in the upper atmosphere during a rain-storm is
sometimes the occasion of phenomena which are often misinterpreted. If
there be abundant dust in the atmosphere through which rain-drops or
snowflakes fall, much of it is gathered up by them, and the water is thereby
rendered turbid and the snow discolored. Here is to be found the
explanation of “mud-rain,” “blood-rain” (red dust), etc.
Since dust is carried to a considerable extent in the upper atmosphere, its
movements and its deposition are little affected by obstacles on the surface
of the land. A building or a hedge can only affect the lodgment of that part
of the atmospheric dust which comes in contact with it or is swept into its
lee. Since most obstacles on the surface of the solid part of the earth reach
up but slight distances into the atmosphere, the dust of the greater part of
the air settles without especial reference to them, and is spread more or less
uniformly over the surface on which it falls.
Fig. 7.—Diagram to illustrate the effect of an obstacle on the transportation and deposition
of sand. The direction of the wind is indicated by the upper arrow. The lower arrows
represent the direction of eddies in the air occasioned by the obstacle. If the surface in
which the obstacle was set was originally flat (dotted line), the sand would tend to be
piled up on either side at a little distance from the obstacle, but more to leeward. At the
same time, depressions would be hollowed out near the obstacle itself (see full line).
(After Cornish.)
Much of the dust transported by the wind is carried out over seas or lakes
and falls into them. By this means, sedimentation is doubtless going on at
the bottom of the whole ocean, and at the bottoms of all lakes. While means
of determining the amount of dust blown into the sea are not at hand, it is
safe to say that, were such determinations possible, the result, if stated in
terms of weight, would be surprising.
Transportation and deposition of sand.—In its transportation by the
wind, sand is not commonly lifted far above the surface of the land, and its
movement is therefore more generally interfered with by surface obstacles
than is the movement of dust. A shrub, a tree, a fence, a building, or even a
sometimes the occasion of phenomena which are often misinterpreted. If
there be abundant dust in the atmosphere through which rain-drops or
snowflakes fall, much of it is gathered up by them, and the water is thereby
rendered turbid and the snow discolored. Here is to be found the
explanation of “mud-rain,” “blood-rain” (red dust), etc.
Since dust is carried to a considerable extent in the upper atmosphere, its
movements and its deposition are little affected by obstacles on the surface
of the land. A building or a hedge can only affect the lodgment of that part
of the atmospheric dust which comes in contact with it or is swept into its
lee. Since most obstacles on the surface of the solid part of the earth reach
up but slight distances into the atmosphere, the dust of the greater part of
the air settles without especial reference to them, and is spread more or less
uniformly over the surface on which it falls.
Fig. 7.—Diagram to illustrate the effect of an obstacle on the transportation and deposition
of sand. The direction of the wind is indicated by the upper arrow. The lower arrows
represent the direction of eddies in the air occasioned by the obstacle. If the surface in
which the obstacle was set was originally flat (dotted line), the sand would tend to be
piled up on either side at a little distance from the obstacle, but more to leeward. At the
same time, depressions would be hollowed out near the obstacle itself (see full line).
(After Cornish.)
Much of the dust transported by the wind is carried out over seas or lakes
and falls into them. By this means, sedimentation is doubtless going on at
the bottom of the whole ocean, and at the bottoms of all lakes. While means
of determining the amount of dust blown into the sea are not at hand, it is
safe to say that, were such determinations possible, the result, if stated in
terms of weight, would be surprising.
Transportation and deposition of sand.—In its transportation by the
wind, sand is not commonly lifted far above the surface of the land, and its
movement is therefore more generally interfered with by surface obstacles
than is the movement of dust. A shrub, a tree, a fence, a building, or even a
Page 55
stone may occasion the lodgment of sand in considerable quantity, though it
has little effect on the lodgment of dust. The effect of obstacles is illustrated
by Fig. 7 (see also Fig. 5). If the obstacle which occasions the lodgment of
sand presents a surface which the wind cannot penetrate, such as a wall,
sand is dropped abundantly on its windward side as well as on the leeward;
but if it be penetrable, like an open fence, the lodgment takes place chiefly
on its leeward side. In cultivated regions cases are known where, in a few
weeks of dry weather, sand has been drifted into lanes in the lee of hedges
to the depth of two or three feet, making them nearly impassable to
vehicles.
Formation of dunes.—In contrast with dust deposited from the
atmosphere, wind-blown sand is commonly aggregated into mounds and
ridges in the process of lodgment. These mounds and ridges are dunes.
Once a dune is started, it occasions the further lodgment of sand, and is a
cause of its own growth. Dunes sometimes reach heights of 200 or 300 feet,
but they are much more commonly no more than 10 or 20 feet in height. On
plane surfaces, there is a limit in height above which they do not rise,
though the limit is different under different conditions. The velocity of wind
at the bottom of the air is not so great as that higher up, and as a dune is
built up, a level is presently reached where the stronger upper winds sweep
away as much sand as is brought to the top. The very even crests of many
dune ridges are probably to be accounted for in this way. Wind-blown or
eolian sand, not piled up in heaps or ridges, is somewhat widespread, but
does not constitute dunes.
Shapes of dunes.[10]—Dunes may assume the form of ridges or of
hillocks. The ridges may be transverse to the direction of the prevailing
wind or parallel with it. Where dunes assume the form of hillocks rather
than ridges, a group of them may be elongate in a direction parallel to the
dominant wind, or at right angles thereto. The shape assumed by a dune or a
group of dunes depends on the abundance of the sand, the strength and
direction of the wind, and the shape of the obstacle which occasions the
lodgment.
has little effect on the lodgment of dust. The effect of obstacles is illustrated
by Fig. 7 (see also Fig. 5). If the obstacle which occasions the lodgment of
sand presents a surface which the wind cannot penetrate, such as a wall,
sand is dropped abundantly on its windward side as well as on the leeward;
but if it be penetrable, like an open fence, the lodgment takes place chiefly
on its leeward side. In cultivated regions cases are known where, in a few
weeks of dry weather, sand has been drifted into lanes in the lee of hedges
to the depth of two or three feet, making them nearly impassable to
vehicles.
Formation of dunes.—In contrast with dust deposited from the
atmosphere, wind-blown sand is commonly aggregated into mounds and
ridges in the process of lodgment. These mounds and ridges are dunes.
Once a dune is started, it occasions the further lodgment of sand, and is a
cause of its own growth. Dunes sometimes reach heights of 200 or 300 feet,
but they are much more commonly no more than 10 or 20 feet in height. On
plane surfaces, there is a limit in height above which they do not rise,
though the limit is different under different conditions. The velocity of wind
at the bottom of the air is not so great as that higher up, and as a dune is
built up, a level is presently reached where the stronger upper winds sweep
away as much sand as is brought to the top. The very even crests of many
dune ridges are probably to be accounted for in this way. Wind-blown or
eolian sand, not piled up in heaps or ridges, is somewhat widespread, but
does not constitute dunes.
Shapes of dunes.[10]—Dunes may assume the form of ridges or of
hillocks. The ridges may be transverse to the direction of the prevailing
wind or parallel with it. Where dunes assume the form of hillocks rather
than ridges, a group of them may be elongate in a direction parallel to the
dominant wind, or at right angles thereto. The shape assumed by a dune or a
group of dunes depends on the abundance of the sand, the strength and
direction of the wind, and the shape of the obstacle which occasions the
lodgment.
Page 56
Fig. 8.—Dune ridges parallel to the direction of the wind. Southwest part of India. Scale
about 3 miles to the inch. (Cornish.)
Fig. 9.—Dune ridges transverse to the direction of the wind. Scale about 3 miles to the inch.
(Cornish.)
The incipient stages of dune formation are readily seen in many dry,
sandy regions. The dune is likely to start in the lee of some obstacle, and to
be elongate in the direction of the wind, especially if the wind be strong
about 3 miles to the inch. (Cornish.)
Fig. 9.—Dune ridges transverse to the direction of the wind. Scale about 3 miles to the inch.
(Cornish.)
The incipient stages of dune formation are readily seen in many dry,
sandy regions. The dune is likely to start in the lee of some obstacle, and to
be elongate in the direction of the wind, especially if the wind be strong
Page 57
relative to the supply of sand. This shape is permanently preserved if the
proper relations between the supply of sand and strength and direction of
wind are preserved. In the dune region of the Indian desert[11] the prevailing
winds are alternately the southwest and northeast monsoons, the former
being the stronger. The supply of sand comes from the southwest. Near the
southwest coast the dune ridges are parallel to the direction of the wind
(Fig. 8); in the interior, where the winds are less strong, the dunes are
transverse to it (Fig. 9); while between the districts where these two types
prevail intermediate forms occur. The transverse dune ridges (Fig. 9) are
said to be the result of the lateral growth and erosion of longitudinal dunes.
[12]
In regions of changeable winds the shape of the dunes is subject to great
variation. Dunes are sometimes crescentic, the convexity facing the wind
(Fig. 10).
Fig. 10.—Crescentic dunes in ground-plan, the convexities facing the wind. (Bokhara.)
(Walther.)
proper relations between the supply of sand and strength and direction of
wind are preserved. In the dune region of the Indian desert[11] the prevailing
winds are alternately the southwest and northeast monsoons, the former
being the stronger. The supply of sand comes from the southwest. Near the
southwest coast the dune ridges are parallel to the direction of the wind
(Fig. 8); in the interior, where the winds are less strong, the dunes are
transverse to it (Fig. 9); while between the districts where these two types
prevail intermediate forms occur. The transverse dune ridges (Fig. 9) are
said to be the result of the lateral growth and erosion of longitudinal dunes.
[12]
In regions of changeable winds the shape of the dunes is subject to great
variation. Dunes are sometimes crescentic, the convexity facing the wind
(Fig. 10).
Fig. 10.—Crescentic dunes in ground-plan, the convexities facing the wind. (Bokhara.)
(Walther.)
Page 58
Along coasts, dune ridges are often transverse to the wind, and groups of
dune hillocks are frequently elongate in the same direction. Here the source
of supply of the sand is itself an elongate belt, often transverse to the
dominant wind, and the resulting dunes often have great length transverse
to the wind. Where the wind has strong mastery over the sand, the
longitudinal tendency is seen, even along coasts.[13]
Fig. 11.—Section of a dune showing, by the dotted line, the steep leeward (bc) and gentler
windward (ab) slope. By reversal of the wind the cross-section may be altered to the form
shown by the line adc. (Cornish.)
The shapes of dunes in section, like
the shapes in ground-plan, depend on
Fig. 12.—Cross-section of a dune the relative strength and constancy of
showing the profiles developed by the winds and the supply of sand. With
scour of the wind on both flanks. constant winds and abundant drifting
(Cornish.)
sand, dunes are steep on the lee side
(bc, Fig. 11), where the angle of slope is the angle of rest for the sand. It
rarely exceeds 23° or 24°.[14] Under the same conditions the windward slope
is relatively gentle (ab, Fig. 11). If the winds be variable so that the
windward slope of one period becomes the leeward slope of another, and
vice versa, this form is not preserved. Thus, by reversal of the wind, the
section abc, Fig. 11, may be changed to adc. If the winds and the supply of
sand be equal, on the average, from opposite directions, the slopes should,
on the average, be equal, though perhaps unequal after any particular storm.
The steep slopes of new-made dunes are lost after the sand has ceased to be
blown. At some points where the winds erode (scour) more than they
deposit, new profiles are developed (Figs. 12 and 13). The erosion profiles
may be very irregular if the dunes are partially covered with vegetation. The
effect of vegetation in restraining wind erosion is shown in Fig. 14, where
plants have preserved a remnant of a dune.
The topographic map.—Since dunes as well as other
topographic features are conveniently represented on contour
maps, and since such maps will be used frequently in the
dune hillocks are frequently elongate in the same direction. Here the source
of supply of the sand is itself an elongate belt, often transverse to the
dominant wind, and the resulting dunes often have great length transverse
to the wind. Where the wind has strong mastery over the sand, the
longitudinal tendency is seen, even along coasts.[13]
Fig. 11.—Section of a dune showing, by the dotted line, the steep leeward (bc) and gentler
windward (ab) slope. By reversal of the wind the cross-section may be altered to the form
shown by the line adc. (Cornish.)
The shapes of dunes in section, like
the shapes in ground-plan, depend on
Fig. 12.—Cross-section of a dune the relative strength and constancy of
showing the profiles developed by the winds and the supply of sand. With
scour of the wind on both flanks. constant winds and abundant drifting
(Cornish.)
sand, dunes are steep on the lee side
(bc, Fig. 11), where the angle of slope is the angle of rest for the sand. It
rarely exceeds 23° or 24°.[14] Under the same conditions the windward slope
is relatively gentle (ab, Fig. 11). If the winds be variable so that the
windward slope of one period becomes the leeward slope of another, and
vice versa, this form is not preserved. Thus, by reversal of the wind, the
section abc, Fig. 11, may be changed to adc. If the winds and the supply of
sand be equal, on the average, from opposite directions, the slopes should,
on the average, be equal, though perhaps unequal after any particular storm.
The steep slopes of new-made dunes are lost after the sand has ceased to be
blown. At some points where the winds erode (scour) more than they
deposit, new profiles are developed (Figs. 12 and 13). The erosion profiles
may be very irregular if the dunes are partially covered with vegetation. The
effect of vegetation in restraining wind erosion is shown in Fig. 14, where
plants have preserved a remnant of a dune.
The topographic map.—Since dunes as well as other
topographic features are conveniently represented on contour
maps, and since such maps will be used frequently in the
Page 59
following pages, a general explanation of them is here
introduced.
“The features represented on the topographic map are of three
distinct kinds: (1) inequalities of surface, called relief, as plains,
plateaus, valleys, hills, and mountains; (2) distribution of water,
called drainage, as streams, lakes, and swamps; (3) the works of
man, called culture, as roads, railroads, boundaries, villages, and
cities.
Fig. 13.—Diagram showing the outline of dunes in process of destruction.
Seven Mile Beach, N. J. (N. J. Geol. Surv.)
Fig. 14.—Illustrates the protective effect of vegetation against wind erosion.
Dune Park, Ind. (Cowles)
Relief.—All elevations are measured from mean sea-level.
The heights of many points are accurately determined, and those
which are most important are given on the map in figures. It is
desirable, however, to give the elevation of all parts of the area
introduced.
“The features represented on the topographic map are of three
distinct kinds: (1) inequalities of surface, called relief, as plains,
plateaus, valleys, hills, and mountains; (2) distribution of water,
called drainage, as streams, lakes, and swamps; (3) the works of
man, called culture, as roads, railroads, boundaries, villages, and
cities.
Fig. 13.—Diagram showing the outline of dunes in process of destruction.
Seven Mile Beach, N. J. (N. J. Geol. Surv.)
Fig. 14.—Illustrates the protective effect of vegetation against wind erosion.
Dune Park, Ind. (Cowles)
Relief.—All elevations are measured from mean sea-level.
The heights of many points are accurately determined, and those
which are most important are given on the map in figures. It is
desirable, however, to give the elevation of all parts of the area
Page 60
mapped, to delineate the horizontal outline, or contour, of all
slopes, and to indicate their grade or degree of steepness. This is
done by lines connecting points of equal elevation above mean
sea-level, the lines being drawn at regular vertical intervals.
These lines are called contours, and the uniform vertical space
between each two contours is called the contour interval. On the
maps of the United States Geological Survey the contours and
elevations are printed in brown (see Plate II).
Fig. 15.—Sketch and map of the same area to illustrate the representation of
topography by means of contour lines (U. S. Geol. Surv.)
The manner in which contours express elevation, form, and
grade is shown in the following sketch and corresponding
contour map, Fig. 15.
The sketch represents a river valley between two hills. In the
foreground is the sea, with a bay which is partly closed by a
hooked sand bar. On each side of the valley is a terrace. From
the terrace on the right a hill rises gradually, while from that on
slopes, and to indicate their grade or degree of steepness. This is
done by lines connecting points of equal elevation above mean
sea-level, the lines being drawn at regular vertical intervals.
These lines are called contours, and the uniform vertical space
between each two contours is called the contour interval. On the
maps of the United States Geological Survey the contours and
elevations are printed in brown (see Plate II).
Fig. 15.—Sketch and map of the same area to illustrate the representation of
topography by means of contour lines (U. S. Geol. Surv.)
The manner in which contours express elevation, form, and
grade is shown in the following sketch and corresponding
contour map, Fig. 15.
The sketch represents a river valley between two hills. In the
foreground is the sea, with a bay which is partly closed by a
hooked sand bar. On each side of the valley is a terrace. From
the terrace on the right a hill rises gradually, while from that on
Page 61
the left the ground ascends steeply in a precipice. Contrasted
with this precipice is the gentle descent of the slope at the left.
In the map each of these features is indicated, directly beneath
its position in the sketch, by contours. The following
explanation may make clearer the manner in which contours
delineate elevation, form, and grade:
1. A contour indicates approximately a certain height above
sea-level. In this illustration the contour interval is 50 feet;
therefore the contours are drawn at 50, 100, 150, 200 feet, and
so on, above sea-level. Along the contour at 250 feet lie all
points of the surface 250 feet above sea; and similarly with any
other contour. In the space between any two contours are found
all elevations above the lower and below the higher contour.
Thus the contour at 150 feet falls just below the edge of the
terrace, while that at 200 feet lies above the terrace; therefore all
points on the terrace are shown to be more than 150 but less
than 200 feet above sea. The summit of the higher hill is stated
to be 670 feet above sea; accordingly the contour at 650 feet
surrounds it. In this illustration nearly all the contours are
numbered. Where this is not possible, certain contours—say
every fifth one—are accentuated and numbered; the heights of
others may then be ascertained by counting up or down from a
numbered contour.
2. Contours define the forms of slopes. Since contours are
continuous horizontal lines conforming to the surface of the
ground, they wind smoothly about smooth surfaces, recede into
all reëntrant angles of ravines, and project in passing about
prominences. The relations of contour curves and angles to
forms of the landscape can be traced in the map and sketch.
3. Contours show the approximate grade of any slope. The
vertical space between two contours is the same, whether they
lie along a cliff or on a gentle slope; but to rise a given height on
a gentle slope one must go farther than on a steep slope, and
therefore contours are far apart on gentle slopes and near
together on steep ones.
with this precipice is the gentle descent of the slope at the left.
In the map each of these features is indicated, directly beneath
its position in the sketch, by contours. The following
explanation may make clearer the manner in which contours
delineate elevation, form, and grade:
1. A contour indicates approximately a certain height above
sea-level. In this illustration the contour interval is 50 feet;
therefore the contours are drawn at 50, 100, 150, 200 feet, and
so on, above sea-level. Along the contour at 250 feet lie all
points of the surface 250 feet above sea; and similarly with any
other contour. In the space between any two contours are found
all elevations above the lower and below the higher contour.
Thus the contour at 150 feet falls just below the edge of the
terrace, while that at 200 feet lies above the terrace; therefore all
points on the terrace are shown to be more than 150 but less
than 200 feet above sea. The summit of the higher hill is stated
to be 670 feet above sea; accordingly the contour at 650 feet
surrounds it. In this illustration nearly all the contours are
numbered. Where this is not possible, certain contours—say
every fifth one—are accentuated and numbered; the heights of
others may then be ascertained by counting up or down from a
numbered contour.
2. Contours define the forms of slopes. Since contours are
continuous horizontal lines conforming to the surface of the
ground, they wind smoothly about smooth surfaces, recede into
all reëntrant angles of ravines, and project in passing about
prominences. The relations of contour curves and angles to
forms of the landscape can be traced in the map and sketch.
3. Contours show the approximate grade of any slope. The
vertical space between two contours is the same, whether they
lie along a cliff or on a gentle slope; but to rise a given height on
a gentle slope one must go farther than on a steep slope, and
therefore contours are far apart on gentle slopes and near
together on steep ones.
Page 62
For a flat or gently undulating country a small contour
interval is used; for a steep or mountainous country a large
interval is necessary. The smallest interval used on the atlas
sheets of the Geological Survey is 5 feet. This is used for
regions like the Mississippi delta and the Dismal Swamp. In
mapping great mountain masses, like those in Colorado, the
interval may be 250 feet. For intermediate relief contour
intervals of 10, 20, 25, 50, and 100 feet are used.
Drainage.—Watercourses are indicated by blue lines. If the
streams flow the year round the line is drawn unbroken, but if
the channel is dry a part of the year the line is broken or dotted.
Where a stream sinks and reappears at the surface, the supposed
underground course is shown by a broken blue line. Lakes,
marshes, and other bodies of water are also shown in blue, by
appropriate conventional signs.
Culture.—The works of man, such as road, railroads, and
towns, together with boundaries of townships, counties and
states, and artificial details, are printed in black.”[15]
Topography of dune areas.—From what has been said, it is clear that
the topography of dune regions may vary widely, but it is always
distinctive. Where the dunes take the form of ridges (Fig. 1, Pl. II), the
ridges are often of essentially uniform height and width for considerable
distances. If there are parallel ridges, they are often separated by trough-like
depressions. Where dunes assume the form of hillocks (Figs. 2 and 3, Pl.
II), rather than ridges, the topography is even more distinctive. In some
regions, depressions (basins) are associated with the dune hillocks.
Occasionally they are hardly less notable than the dunes themselves. A
somewhat similar association of hillocks and basins is locally developed by
other means, but dunes are made up of sand and usually of sand only, while
the composition of similarly shaped hillocks and depressions shaped by
other agencies is notably different.
In Fig. 1, Plate II (Five Mile Beach, 8 miles northeast of Cape
May, N. J.), the contour interval is 10 feet. There is here but one
contour line (the 10-foot contour), though this appears in several
interval is used; for a steep or mountainous country a large
interval is necessary. The smallest interval used on the atlas
sheets of the Geological Survey is 5 feet. This is used for
regions like the Mississippi delta and the Dismal Swamp. In
mapping great mountain masses, like those in Colorado, the
interval may be 250 feet. For intermediate relief contour
intervals of 10, 20, 25, 50, and 100 feet are used.
Drainage.—Watercourses are indicated by blue lines. If the
streams flow the year round the line is drawn unbroken, but if
the channel is dry a part of the year the line is broken or dotted.
Where a stream sinks and reappears at the surface, the supposed
underground course is shown by a broken blue line. Lakes,
marshes, and other bodies of water are also shown in blue, by
appropriate conventional signs.
Culture.—The works of man, such as road, railroads, and
towns, together with boundaries of townships, counties and
states, and artificial details, are printed in black.”[15]
Topography of dune areas.—From what has been said, it is clear that
the topography of dune regions may vary widely, but it is always
distinctive. Where the dunes take the form of ridges (Fig. 1, Pl. II), the
ridges are often of essentially uniform height and width for considerable
distances. If there are parallel ridges, they are often separated by trough-like
depressions. Where dunes assume the form of hillocks (Figs. 2 and 3, Pl.
II), rather than ridges, the topography is even more distinctive. In some
regions, depressions (basins) are associated with the dune hillocks.
Occasionally they are hardly less notable than the dunes themselves. A
somewhat similar association of hillocks and basins is locally developed by
other means, but dunes are made up of sand and usually of sand only, while
the composition of similarly shaped hillocks and depressions shaped by
other agencies is notably different.
In Fig. 1, Plate II (Five Mile Beach, 8 miles northeast of Cape
May, N. J.), the contour interval is 10 feet. There is here but one
contour line (the 10-foot contour), though this appears in several
Page 63
places. Since this line connects places 10 feet above sea-level,
all places between it and the sea (or marsh) are less than 10 feet
above the water, while all places within the lines have an
elevation of more than 10 feet. None of them reaches an
elevation of 20 feet, since a 20-foot contour does not appear. It
will be seen that some of the elevations in Fig. 1 are elongate,
while others have the form of mounds.
Fig. 2 (Pl. II) shows dune topography along the Arkansas
River in Kansas (near Larned); Fig. 4, dune topography in
Nebraska (Lat. 42°, Long. 103°), not in immediate association
with a valley or shore; and Fig. 3 shows irregular ridge-like
dunes at the head of Lake Michigan. In Fig. 2 the contour
interval is 20 feet. All the small hillocks southeast of the river
are dunes. Some of them are represented by one contour and
some by two. The altitude of the region is considerable, the
heavy contour representing an elevation of 2100 feet; but the
dunes themselves are rarely more than 20 feet above their
surroundings. In Fig. 4, where the contour interval is also 20
feet, there are, besides the numerous hillocks, several
depressions (basins). These are represented by hachures inside
the contour lines. In some cases there are intermittent lakes
(blue) in the depressions. The heavy contour at Spring Lakes in
this figure is the contour of 4300 feet. There are two depression
contours (4280 and 4260) below it. The bottom of the
depression is therefore lower than 4260, but not so low as 4240.
In Fig. 3 the contour interval is 10 feet, and the dune ridges
north of Miller are more than 50 feet high. The dune ridges here
have helped to determine the position of this branch of the
Calumet River, and have blocked its former outlet. The present
drainage is to the westward.
Migration of dunes.—By the continual transfer of sand from its
windward to its leeward side, a dune may be moved from one place to
another, though continuing to be made up, in large part, of the same sand. In
their migration dunes sometimes invade fertile lands, causing so great loss
that means are devised for stopping them. The simplest method (employed
in France and Holland) is to help vegetation to get a foothold in the sand.
all places between it and the sea (or marsh) are less than 10 feet
above the water, while all places within the lines have an
elevation of more than 10 feet. None of them reaches an
elevation of 20 feet, since a 20-foot contour does not appear. It
will be seen that some of the elevations in Fig. 1 are elongate,
while others have the form of mounds.
Fig. 2 (Pl. II) shows dune topography along the Arkansas
River in Kansas (near Larned); Fig. 4, dune topography in
Nebraska (Lat. 42°, Long. 103°), not in immediate association
with a valley or shore; and Fig. 3 shows irregular ridge-like
dunes at the head of Lake Michigan. In Fig. 2 the contour
interval is 20 feet. All the small hillocks southeast of the river
are dunes. Some of them are represented by one contour and
some by two. The altitude of the region is considerable, the
heavy contour representing an elevation of 2100 feet; but the
dunes themselves are rarely more than 20 feet above their
surroundings. In Fig. 4, where the contour interval is also 20
feet, there are, besides the numerous hillocks, several
depressions (basins). These are represented by hachures inside
the contour lines. In some cases there are intermittent lakes
(blue) in the depressions. The heavy contour at Spring Lakes in
this figure is the contour of 4300 feet. There are two depression
contours (4280 and 4260) below it. The bottom of the
depression is therefore lower than 4260, but not so low as 4240.
In Fig. 3 the contour interval is 10 feet, and the dune ridges
north of Miller are more than 50 feet high. The dune ridges here
have helped to determine the position of this branch of the
Calumet River, and have blocked its former outlet. The present
drainage is to the westward.
Migration of dunes.—By the continual transfer of sand from its
windward to its leeward side, a dune may be moved from one place to
another, though continuing to be made up, in large part, of the same sand. In
their migration dunes sometimes invade fertile lands, causing so great loss
that means are devised for stopping them. The simplest method (employed
in France and Holland) is to help vegetation to get a foothold in the sand.
Page 64
The effect of the vegetation is to pin the sand down. As a dune ridge along a
coast travels inland, another may be formed behind it. Successions of dune
ridges are thus sometimes formed.
Fig. 16.—Diagram illustrating the migration of dunes on the Kurische Nehrung. (Credner.)
A remarkable instance of the migration of a sand dune is recorded on the
Kurische Nehrung on the north coast of Germany. The Nehrung consists of
a long narrow neck of land composed of sand, lying off the main coast. At
the beginning of this century there was a notable dune ridge on one side.
Since that time it has migrated a considerable distance, and in its migration
it has been brought into the relationships illustrated in the accompanying
diagrams (Fig. 16). In 1800 the dune ridge was on one side of a church,
which was then in use. In 1839 the ridge had been so far shifted to the
leeward as to completely bury the church, and in 1869, its migration had
progressed so far as to again discover the building.[16]
coast travels inland, another may be formed behind it. Successions of dune
ridges are thus sometimes formed.
Fig. 16.—Diagram illustrating the migration of dunes on the Kurische Nehrung. (Credner.)
A remarkable instance of the migration of a sand dune is recorded on the
Kurische Nehrung on the north coast of Germany. The Nehrung consists of
a long narrow neck of land composed of sand, lying off the main coast. At
the beginning of this century there was a notable dune ridge on one side.
Since that time it has migrated a considerable distance, and in its migration
it has been brought into the relationships illustrated in the accompanying
diagrams (Fig. 16). In 1800 the dune ridge was on one side of a church,
which was then in use. In 1839 the ridge had been so far shifted to the
leeward as to completely bury the church, and in 1869, its migration had
progressed so far as to again discover the building.[16]
Page 65
Fig. 17.—Migration of dunes into a timbered region. Dune Park, Ind. Head of Lake
Michigan. (Meyers.)
When dunes migrate into a timbered region they bury and kill the trees
(Fig. 17). In one instance on the coast of Prussia a tall pine forest, covering
hundreds of acres, was destroyed during the brief period between 1804 and
1827.[17] At some points in New Jersey orchards have been so far buried
within the lifetime of their owners that only the tops of the highest trees are
exposed. Trees and other objects once buried may be again discovered by
farther migration of the sand (Figs. 18 and 19).[18]
Michigan. (Meyers.)
When dunes migrate into a timbered region they bury and kill the trees
(Fig. 17). In one instance on the coast of Prussia a tall pine forest, covering
hundreds of acres, was destroyed during the brief period between 1804 and
1827.[17] At some points in New Jersey orchards have been so far buried
within the lifetime of their owners that only the tops of the highest trees are
exposed. Trees and other objects once buried may be again discovered by
farther migration of the sand (Figs. 18 and 19).[18]
Page 66
Fig. 18.—A resurrected forest. The dune sand after burying and killing the timber has
been shifted beyond it. Dune Park. Ind. (Meyers.)
Eolian sand, not aggregated into distinct dunes, is often destructive. Even
valleys and cities are sometimes buried by it. Drifting sands had so
completely buried Nineveh two centuries after its destruction that its site
was unknown.
Distribution of dunes.—Dunes are likely to be developed wherever dry
sand is exposed to the wind. Their favorite situations are the dry and sandy
shores of lakes and seas, sandy valleys, and arid sandy plains.
Along coasts, dunes are likely to be extensively developed only where
the prevailing winds are on shore. Thus about Lake Michigan, where the
prevailing winds are from the west, dunes are abundant and large on the
east shore, and but few and small on the west. In shallow water, shore
currents and storm waves often build up a reef of sand a little above the
normal level of the water. When the waves subside, the sand dries and the
wind heaps it up into dunes. This sequence of events is in progress at many
points on the Atlantic Coast. Sandy Hook, New Jersey, and the “beaches”
farther south started as barrier ridges. When the waves had built them above
normal water-level, the wind re-worked the sand, piling it up into mounds
and hillocks (Fig. 1, Pl. II). Such dune belts a little off shore are sometimes
turned to good account. They are usually separated from the mainland by a
shallow lagoon. Where land is valuable, the lagoon is sometimes filled in,
making new land, thus anticipating the result which nature would achieve
been shifted beyond it. Dune Park. Ind. (Meyers.)
Eolian sand, not aggregated into distinct dunes, is often destructive. Even
valleys and cities are sometimes buried by it. Drifting sands had so
completely buried Nineveh two centuries after its destruction that its site
was unknown.
Distribution of dunes.—Dunes are likely to be developed wherever dry
sand is exposed to the wind. Their favorite situations are the dry and sandy
shores of lakes and seas, sandy valleys, and arid sandy plains.
Along coasts, dunes are likely to be extensively developed only where
the prevailing winds are on shore. Thus about Lake Michigan, where the
prevailing winds are from the west, dunes are abundant and large on the
east shore, and but few and small on the west. In shallow water, shore
currents and storm waves often build up a reef of sand a little above the
normal level of the water. When the waves subside, the sand dries and the
wind heaps it up into dunes. This sequence of events is in progress at many
points on the Atlantic Coast. Sandy Hook, New Jersey, and the “beaches”
farther south started as barrier ridges. When the waves had built them above
normal water-level, the wind re-worked the sand, piling it up into mounds
and hillocks (Fig. 1, Pl. II). Such dune belts a little off shore are sometimes
turned to good account. They are usually separated from the mainland by a
shallow lagoon. Where land is valuable, the lagoon is sometimes filled in,
making new land, thus anticipating the result which nature would achieve
Page 67
more slowly. This has been done at some points on the western coast of
Europe.
Fig. 19.—Migration of dune sand exposing bones in a cemetery. Hatteras Island, N. C.
(Collier Cobb.)
Dunes are likely to occur along stream valleys (Fig. 2, Pl. II), if their
bottoms or slopes are of sand, and not covered by vegetation. Dunes along
valleys are usually on the side toward which the prevailing winds blow.
Thus they are more common on the east side of the Mississippi than on the
west. Dunes may be formed in the valley bottoms, but the sand is often
blown up out of the valley and lodged on the bluffs above.
Apart from these special classes of situations, any sandy region the
surface of which is dry is likely to have its surface material shifted by the
wind and piled up into dune ridges or hillocks (Fig. 4, Pl. II). Dunes
probably reach their greatest development in the Sahara, where some of
them take the form of hillocks, and some the form of ridges. Travelers in
that region report that dune ridges are sometimes encountered the faces of
which are so high and steep as to be difficult of ascent, and that parties have
been obliged to travel miles along their bases before finding a break where
crossing was practicable.
Europe.
Fig. 19.—Migration of dune sand exposing bones in a cemetery. Hatteras Island, N. C.
(Collier Cobb.)
Dunes are likely to occur along stream valleys (Fig. 2, Pl. II), if their
bottoms or slopes are of sand, and not covered by vegetation. Dunes along
valleys are usually on the side toward which the prevailing winds blow.
Thus they are more common on the east side of the Mississippi than on the
west. Dunes may be formed in the valley bottoms, but the sand is often
blown up out of the valley and lodged on the bluffs above.
Apart from these special classes of situations, any sandy region the
surface of which is dry is likely to have its surface material shifted by the
wind and piled up into dune ridges or hillocks (Fig. 4, Pl. II). Dunes
probably reach their greatest development in the Sahara, where some of
them take the form of hillocks, and some the form of ridges. Travelers in
that region report that dune ridges are sometimes encountered the faces of
which are so high and steep as to be difficult of ascent, and that parties have
been obliged to travel miles along their bases before finding a break where
crossing was practicable.
Page 68
Fig. 20.—Wind-ripples. (Cross, U. S. Geol. Surv.)
Wind-ripples.—The surface of the dry sand over which the wind has
blown for a few hours is likely to be marked with ripples (Fig. 20) similar
to those made on a sandy bottom beneath shallow water, under the influence
of waves. Like ripple marks made by the water, wind-ripples have one side
(the lee) steeper than the other. While the ripples are, as a rule, but a
fraction of an inch high, they throw much light on the origin of the great
dune ridges. If the ripples be watched closely during the progress of a wind-
storm, they are found gradually to shift their position. Sand is blown up the
gentler windward slope to the crest of the ridge and falls down on the other
side. The moment it falls below the crest of the ridge to leeward, it is
protected against the wind, and is likely to lodge. Wear on the windward
side is about equal to deposition on the leeward, and the result is the orderly
progression of the ripples in the direction in which the wind is blowing, just
as in the case of dune ridges.
Abrasion by the wind.—While the effect of the wind on sandy and
dusty surfaces may be considerable, its effect on solid rock is relatively
slight and accomplished, not by its own impact, but by that of the material it
Wind-ripples.—The surface of the dry sand over which the wind has
blown for a few hours is likely to be marked with ripples (Fig. 20) similar
to those made on a sandy bottom beneath shallow water, under the influence
of waves. Like ripple marks made by the water, wind-ripples have one side
(the lee) steeper than the other. While the ripples are, as a rule, but a
fraction of an inch high, they throw much light on the origin of the great
dune ridges. If the ripples be watched closely during the progress of a wind-
storm, they are found gradually to shift their position. Sand is blown up the
gentler windward slope to the crest of the ridge and falls down on the other
side. The moment it falls below the crest of the ridge to leeward, it is
protected against the wind, and is likely to lodge. Wear on the windward
side is about equal to deposition on the leeward, and the result is the orderly
progression of the ripples in the direction in which the wind is blowing, just
as in the case of dune ridges.
Abrasion by the wind.—While the effect of the wind on sandy and
dusty surfaces may be considerable, its effect on solid rock is relatively
slight and accomplished, not by its own impact, but by that of the material it
Page 69
carries. The effect of blown sand on rock surfaces over and against which it
is driven is perhaps best understood by recalling the effects of artificial
sand-blasts, by means of which glass is etched. In a region where sand is
blowing, exposed surfaces of rock suffer from a multitude of blows struck
by the sand grains in transit. The result is that such rock surfaces are worn,
and worn in a way peculiar to the agency accomplishing the work. If the
rock be made up of laminæ which are of unequal hardness, the blown sand
digs out the softer ones, leaving the harder projecting as ridges between
them. Adjacent masses of harder and softer rock of whatever thickness are
similarly affected. The sculpturing thus effected on projecting masses of
rock is often picturesque and striking (Figs. 21 and 22), and is most
common in arid regions. Details of wind-carving are shown in Fig. 23.
Fig. 21.—Wind-carved rock. (Green.)
PLATE II.
is driven is perhaps best understood by recalling the effects of artificial
sand-blasts, by means of which glass is etched. In a region where sand is
blowing, exposed surfaces of rock suffer from a multitude of blows struck
by the sand grains in transit. The result is that such rock surfaces are worn,
and worn in a way peculiar to the agency accomplishing the work. If the
rock be made up of laminæ which are of unequal hardness, the blown sand
digs out the softer ones, leaving the harder projecting as ridges between
them. Adjacent masses of harder and softer rock of whatever thickness are
similarly affected. The sculpturing thus effected on projecting masses of
rock is often picturesque and striking (Figs. 21 and 22), and is most
common in arid regions. Details of wind-carving are shown in Fig. 23.
Fig. 21.—Wind-carved rock. (Green.)
PLATE II.
Page 70
U. S. Geol. Surv. Fig. 1. NEW Scale, 1+ mile per inch.
JERSEY.
U. S. Geol. Surv. Fig. 3.
INDI Scale, 1+ mile per inch.
U. S. Geol. Surv. Fig. 2. KANSAS. Scale, 2+ mile per inch. ANA.
JERSEY.
U. S. Geol. Surv. Fig. 3.
INDI Scale, 1+ mile per inch.
U. S. Geol. Surv. Fig. 2. KANSAS. Scale, 2+ mile per inch. ANA.
Page 71
U. S. Geol. Surv. Fig. 4. NEBRASKA. Scale, 2+ mile per inch.
Sand drifted over loose stones lying on the surface often develops flat or
flattish faces or facets on them. These facets are likely to be three in
number, and the exposed portion of the stone is likely to develop a sort of
pyramidal shape, the three flattish surfaces being mutually limited by
tolerably well-defined lines (Fig. 24). Thus arise the three-faceted stones
(Dreikanter of the Germans) commonly seen where sands have been long in
movement.
Sand drifted over loose stones lying on the surface often develops flat or
flattish faces or facets on them. These facets are likely to be three in
number, and the exposed portion of the stone is likely to develop a sort of
pyramidal shape, the three flattish surfaces being mutually limited by
tolerably well-defined lines (Fig. 24). Thus arise the three-faceted stones
(Dreikanter of the Germans) commonly seen where sands have been long in
movement.
Page 72
Fig. 22.—Wind-carved hillock of cross-bedded sandstone. Missouri River, Montana.
(Calhoun, U. S. G. S.)
Not only does the drifting sand wear the surface over which it passes and
against which it strikes, but the grains themselves are worn in the process.
They are liable to be broken as they strike rock surfaces, and they are likely
to strike one another in the atmosphere. In both cases they are subject to
wear, and so to reduction to a finer and finer state.
The erosion accomplished by the wind is therefore of various sorts. The
impact of the wind itself picks up the fine materials which are already
loosened, thus wearing down the surface from which they are removed; the
materials picked up wear the rock surfaces against which they are blown,
and the transported materials themselves suffer reduction in transit.
Effects of wind on plants.—Another effect of wind work is seen in the
uprooting of trees (Fig. 25). The uprooting disturbs the surface in such a
way as to make loose earth more readily accessible to wind and water. The
uprooting of trees on steep slopes often causes the descent of considerable
quantities of loose rock and soil. Again, organisms of various sorts (certain
types of seeds, germs, etc.), as well as dust and sand, are extensively
transported by the wind. While this is important biologically its geological
effects are remote.
(Calhoun, U. S. G. S.)
Not only does the drifting sand wear the surface over which it passes and
against which it strikes, but the grains themselves are worn in the process.
They are liable to be broken as they strike rock surfaces, and they are likely
to strike one another in the atmosphere. In both cases they are subject to
wear, and so to reduction to a finer and finer state.
The erosion accomplished by the wind is therefore of various sorts. The
impact of the wind itself picks up the fine materials which are already
loosened, thus wearing down the surface from which they are removed; the
materials picked up wear the rock surfaces against which they are blown,
and the transported materials themselves suffer reduction in transit.
Effects of wind on plants.—Another effect of wind work is seen in the
uprooting of trees (Fig. 25). The uprooting disturbs the surface in such a
way as to make loose earth more readily accessible to wind and water. The
uprooting of trees on steep slopes often causes the descent of considerable
quantities of loose rock and soil. Again, organisms of various sorts (certain
types of seeds, germs, etc.), as well as dust and sand, are extensively
transported by the wind. While this is important biologically its geological
effects are remote.
Page 73
Fig. 23.—Figure showing details of wind-carving on rock surface (rhyolite). Mono Valley,
California.
California.
Page 74
Fig. 24.—Wind-worn stones (Dreikanter).
Fig. 25.—Shows the disturbance of surface earth and rocks by upturning of trees. (Darton,
U. S. Geol. Surv.)
Indirect effects of the wind.—Other dynamic processes are called into
being or stimulated by the atmosphere. Winds generate both waves and
Fig. 25.—Shows the disturbance of surface earth and rocks by upturning of trees. (Darton,
U. S. Geol. Surv.)
Indirect effects of the wind.—Other dynamic processes are called into
being or stimulated by the atmosphere. Winds generate both waves and
Page 75
currents, and both are effective agents in geological work. The results of
their activities are discussed elsewhere.
II. The Chemical Work of the Atmosphere.
The chemical work of the atmosphere (including solution and
precipitation from solution) is principally accomplished in connection with
water, a dry atmosphere having relatively little direct chemical effect on
rock or soils.
Precipitation from solution.—The water in the soil is constantly
evaporating. Such substances as it contains in solution are deposited where
the water evaporates, and where evaporation is long continued without re-
solution of the substances deposited, the surface becomes coated with an
efflorescence of mineral matter. Conspicuous examples are found in the
alkali plains of certain areas in the western part of the United States. Since
the alkaline efflorescence is the result of evaporation it is connected with
the atmosphere, but the material of the efflorescence was brought to its
present position by water. The principle involved is illustrated by the white
efflorescence which frequently appears on brick walls during the dry days
which follow a drenching rain. The water penetrates the brick and mortar
and dissolves something of their substance, and when it is evaporated from
the surface the material in solution is left behind.
In arid regions the deposition of substances other than alkali is common.
The percolating waters dissolve whatever is soluble, and when they
evaporate their mineral content is left. The pebbles and stones of the arid
plains have in many places become heavily coated with mineral matter
deposited in this way, and not infrequently cemented into conglomerate.
One of the commonest mineral substances found in such situations is lime
carbonate. In some cases it was doubtless derived by solution from
limestone beds beneath the surface, but this is not always the case. It often
encrusts the bits of lava on lava plains where it can hardly have been
derived from limestone. The faces of cliffs of granite or gneiss, hundreds
and even thousands of feet above all other sorts of rock,[19] are sometimes
spotted with patches of lime carbonate. In the first case the lime carbonate
was derived by chemical change from the lava, and in the second, from the
granite or gneiss (see Carbonation below), but its present position is the
result of evaporation.
their activities are discussed elsewhere.
II. The Chemical Work of the Atmosphere.
The chemical work of the atmosphere (including solution and
precipitation from solution) is principally accomplished in connection with
water, a dry atmosphere having relatively little direct chemical effect on
rock or soils.
Precipitation from solution.—The water in the soil is constantly
evaporating. Such substances as it contains in solution are deposited where
the water evaporates, and where evaporation is long continued without re-
solution of the substances deposited, the surface becomes coated with an
efflorescence of mineral matter. Conspicuous examples are found in the
alkali plains of certain areas in the western part of the United States. Since
the alkaline efflorescence is the result of evaporation it is connected with
the atmosphere, but the material of the efflorescence was brought to its
present position by water. The principle involved is illustrated by the white
efflorescence which frequently appears on brick walls during the dry days
which follow a drenching rain. The water penetrates the brick and mortar
and dissolves something of their substance, and when it is evaporated from
the surface the material in solution is left behind.
In arid regions the deposition of substances other than alkali is common.
The percolating waters dissolve whatever is soluble, and when they
evaporate their mineral content is left. The pebbles and stones of the arid
plains have in many places become heavily coated with mineral matter
deposited in this way, and not infrequently cemented into conglomerate.
One of the commonest mineral substances found in such situations is lime
carbonate. In some cases it was doubtless derived by solution from
limestone beds beneath the surface, but this is not always the case. It often
encrusts the bits of lava on lava plains where it can hardly have been
derived from limestone. The faces of cliffs of granite or gneiss, hundreds
and even thousands of feet above all other sorts of rock,[19] are sometimes
spotted with patches of lime carbonate. In the first case the lime carbonate
was derived by chemical change from the lava, and in the second, from the
granite or gneiss (see Carbonation below), but its present position is the
result of evaporation.
Page 76
Oxidation.—In the presence of moisture the oxygen of the air enters into
combination with various elements of the soil and rocks. This is oxidation.
No other common mineral substance shows the results of oxidation so
quickly and so distinctly as iron. The oxidized portion is loose and friable,
and a mass of iron exposed to a moist atmosphere will ultimately crumble
away. This change is comparable to other less obvious changes taking place
in many minerals at and below the surface. Oxidation generally involves the
disintegration of the rock concerned. Its effects in this direction will be
referred to in other connections.
Carbonation.—The production of lime carbonate from rock containing
calcium compounds, but not in the form of carbonates, is known as
carbonation, and is one of the important chemical changes effected by the
carbon dioxide of the atmosphere in coöperation with water. In the process
of carbonation the original minerals of complex composition are
decomposed and simpler ones usually formed. Volumetric changes are
involved, which often lead to the disruption of the rock (see Ground water).
Furthermore, carbonates are among the more soluble minerals, and their
production therefore brings some of the rock materials into a soluble
condition, and their extraction through solution tends still further to
disintegrate the rock. The carbonation of crystalline rocks is therefore a
disintegrating process, and will be considered further in its many concrete
applications.
Other chemical changes.—A third chemical process which often
accompanies oxidation and carbonation is hydration. This is effected by
water rather than by air, and will be considered in that connection. In
general it leads to the disintegration of the minerals and rocks affected. The
chemical effects of nitric acid, etc., developed through the agency of
atmospheric electricity, and the corresponding effects of the gases and
vapors which issue from volcanoes, many of them chemically active, are to
be mentioned in this connection.
Conditions favorable for chemical changes.—Conditions are not
everywhere equally favorable for the chemical work of the atmosphere. In
general, high temperatures facilitate chemical action, and, other things
being equal, rocks are more readily decomposed by atmospheric action in
warm than in cold regions. Chemical activity is probably greater where the
climate is continuously warm than where there are great changes of
combination with various elements of the soil and rocks. This is oxidation.
No other common mineral substance shows the results of oxidation so
quickly and so distinctly as iron. The oxidized portion is loose and friable,
and a mass of iron exposed to a moist atmosphere will ultimately crumble
away. This change is comparable to other less obvious changes taking place
in many minerals at and below the surface. Oxidation generally involves the
disintegration of the rock concerned. Its effects in this direction will be
referred to in other connections.
Carbonation.—The production of lime carbonate from rock containing
calcium compounds, but not in the form of carbonates, is known as
carbonation, and is one of the important chemical changes effected by the
carbon dioxide of the atmosphere in coöperation with water. In the process
of carbonation the original minerals of complex composition are
decomposed and simpler ones usually formed. Volumetric changes are
involved, which often lead to the disruption of the rock (see Ground water).
Furthermore, carbonates are among the more soluble minerals, and their
production therefore brings some of the rock materials into a soluble
condition, and their extraction through solution tends still further to
disintegrate the rock. The carbonation of crystalline rocks is therefore a
disintegrating process, and will be considered further in its many concrete
applications.
Other chemical changes.—A third chemical process which often
accompanies oxidation and carbonation is hydration. This is effected by
water rather than by air, and will be considered in that connection. In
general it leads to the disintegration of the minerals and rocks affected. The
chemical effects of nitric acid, etc., developed through the agency of
atmospheric electricity, and the corresponding effects of the gases and
vapors which issue from volcanoes, many of them chemically active, are to
be mentioned in this connection.
Conditions favorable for chemical changes.—Conditions are not
everywhere equally favorable for the chemical work of the atmosphere. In
general, high temperatures facilitate chemical action, and, other things
being equal, rocks are more readily decomposed by atmospheric action in
warm than in cold regions. Chemical activity is probably greater where the
climate is continuously warm than where there are great changes of
Page 77
temperature. Changes of temperature, on the other hand, tend to disrupt
rock, and thus increase the amount of surface exposed to chemical change.
Since nearly all the chemical changes worked by the atmosphere on the
rocks are increased by the presence of moisture, the chemical activity of the
atmosphere is greater in moist than in dry regions.
B. THE ATMOSPHERE AS A CONDITIONING AGENCY.
The most obvious mechanical work of the atmosphere is effected by the
wind, but mechanical results of great importance, conditioned by the
atmosphere, are also effected when the air is still.
I. Temperature Effects.
When the sun shines on bare rock its surface is heated and expanded, and
the expanded particles crowd one another with great force. Since rock is a
poor conductor of heat its surface is heated and expanded notably more than
parts beneath the surface. It follows that strains are set up between the
expanded outer portion and the cooler and less expanded parts within. In the
cooling of the same rock mass it is the outermost portion which cools first
and fastest, and, contracting as it cools, strains are again set up between the
outer part, which is cooled more, and the inner part, which is cooled less.
The result may be illustrated by the effect of cold water on hot glass, or of
hot water on cold glass. In either case the fracture is the result of the sudden
and considerable differential expansion or contraction. Since the heating
and cooling of rock are much slower than the heating and cooling of glass
under the conditions mentioned, the rupturing effects are less conspicuous,
but none the less real. The actual effects of temperature changes are
illustrated by familiar phenomena. The surface portions of bowlders
exposed to the sun are frequently seen to be shelling off (Fig. 26). The
loosened concentric shells may be a fraction of an inch, or sometimes even
several inches in thickness. This process of exfoliation affects not only
bowlders, but bare rock surfaces wherever exposed to the sun (Figs. 27, 28).
It is often conspicuous on the faces of cliffs.
rock, and thus increase the amount of surface exposed to chemical change.
Since nearly all the chemical changes worked by the atmosphere on the
rocks are increased by the presence of moisture, the chemical activity of the
atmosphere is greater in moist than in dry regions.
B. THE ATMOSPHERE AS A CONDITIONING AGENCY.
The most obvious mechanical work of the atmosphere is effected by the
wind, but mechanical results of great importance, conditioned by the
atmosphere, are also effected when the air is still.
I. Temperature Effects.
When the sun shines on bare rock its surface is heated and expanded, and
the expanded particles crowd one another with great force. Since rock is a
poor conductor of heat its surface is heated and expanded notably more than
parts beneath the surface. It follows that strains are set up between the
expanded outer portion and the cooler and less expanded parts within. In the
cooling of the same rock mass it is the outermost portion which cools first
and fastest, and, contracting as it cools, strains are again set up between the
outer part, which is cooled more, and the inner part, which is cooled less.
The result may be illustrated by the effect of cold water on hot glass, or of
hot water on cold glass. In either case the fracture is the result of the sudden
and considerable differential expansion or contraction. Since the heating
and cooling of rock are much slower than the heating and cooling of glass
under the conditions mentioned, the rupturing effects are less conspicuous,
but none the less real. The actual effects of temperature changes are
illustrated by familiar phenomena. The surface portions of bowlders
exposed to the sun are frequently seen to be shelling off (Fig. 26). The
loosened concentric shells may be a fraction of an inch, or sometimes even
several inches in thickness. This process of exfoliation affects not only
bowlders, but bare rock surfaces wherever exposed to the sun (Figs. 27, 28).
It is often conspicuous on the faces of cliffs.
Page 78
Fig. 26.—Exfoliation. A bowlder of weathering, the rock being granite. Wichita Mountains,
Oklahoma.
Fig. 27.—A weathered summit of granite in the Wichita Mountains. Oklahoma. (Willis,
U. S. Geol. Surv.)
Several conditions, some of which are connected with the atmosphere
and some with the rock, determine the efficiency of this process. Since the
breaking of the rock results from the expansion and contraction due to its
changes of temperature, it follows that, other things being equal, the greater
the change, the greater the breaking; but the suddenness of the temperature
change is even more important than its amount. It follows that great daily,
rather than great annual, changes of temperature[20] favor rock-breaking,
Oklahoma.
Fig. 27.—A weathered summit of granite in the Wichita Mountains. Oklahoma. (Willis,
U. S. Geol. Surv.)
Several conditions, some of which are connected with the atmosphere
and some with the rock, determine the efficiency of this process. Since the
breaking of the rock results from the expansion and contraction due to its
changes of temperature, it follows that, other things being equal, the greater
the change, the greater the breaking; but the suddenness of the temperature
change is even more important than its amount. It follows that great daily,
rather than great annual, changes of temperature[20] favor rock-breaking,
Page 79
though with changes of a given frequency their effectiveness is greater the
greater their range. A partial exception to this generalization should be
noted. If abundant moisture is present in the pores and cracks of the rock a
change of temperature from 45° to 35° (Fahr.) might be far less effective in
breaking the rock than a change from 35° to 25° in the same time, for in the
latter case the sudden and very considerable expansion (about one-tenth)
which water undergoes on freezing is brought into play. This may be called
the wedge-work of ice. The daily range of temperature is influenced
especially by latitude, altitude, and humidity. Other things being equal, the
greatest daily ranges of temperature occur in high-temperate latitudes,
though to this general statement there are local exceptions, depending on
other conditions. High altitudes favor great daily ranges of temperature, so
far as the rock surface is concerned (see Figs. 29, 30), for though the rock
becomes heated during the sunny day, the thinness and dryness of the
atmosphere allow its heat to radiate rapidly at night. Here, too, the daily
range of temperature is likely to bring the wedge-work of ice into play.
Since the south side of a mountain (in the northern hemisphere) is heated
more than the north, it is subject to the greater daily range of temperature,
and the rock on this side suffers the greater disruption. Similarly, rock
surfaces on which the sun shines daily are subject to greater disruption than
those much shielded by clouds. Isolated peaks, because of their greater
exposure, are subject to rather greater daily ranges of temperature than
plateaus of the same elevation.
greater their range. A partial exception to this generalization should be
noted. If abundant moisture is present in the pores and cracks of the rock a
change of temperature from 45° to 35° (Fahr.) might be far less effective in
breaking the rock than a change from 35° to 25° in the same time, for in the
latter case the sudden and very considerable expansion (about one-tenth)
which water undergoes on freezing is brought into play. This may be called
the wedge-work of ice. The daily range of temperature is influenced
especially by latitude, altitude, and humidity. Other things being equal, the
greatest daily ranges of temperature occur in high-temperate latitudes,
though to this general statement there are local exceptions, depending on
other conditions. High altitudes favor great daily ranges of temperature, so
far as the rock surface is concerned (see Figs. 29, 30), for though the rock
becomes heated during the sunny day, the thinness and dryness of the
atmosphere allow its heat to radiate rapidly at night. Here, too, the daily
range of temperature is likely to bring the wedge-work of ice into play.
Since the south side of a mountain (in the northern hemisphere) is heated
more than the north, it is subject to the greater daily range of temperature,
and the rock on this side suffers the greater disruption. Similarly, rock
surfaces on which the sun shines daily are subject to greater disruption than
those much shielded by clouds. Isolated peaks, because of their greater
exposure, are subject to rather greater daily ranges of temperature than
plateaus of the same elevation.
Page 80
Fig. 28.—Exfoliation on a mountain slope. Mt. Starr-King (Cal.) from the north.
The daily range of temperature is also influenced by humidity. Because
of the effect of water vapor in the atmosphere on insolation and radiation, a
rock surface becomes hotter in the day and cooler at night beneath a dry
atmosphere than beneath a moist one. Aridity therefore favors the disruption
of rock by changing temperatures.
Turning from the conditions of the atmosphere which affect the
disruption of rock to the conditions of the rock which influence the same
process, several points are to be noted. In the first place, the disrupting
effects of changes of temperature are slight or nil where the solid rock is
protected by soil, clay, sand, gravel, snow, or other incoherent material. If
the constituent parts of the loose material are coarse, like bowlders, their
surfaces are affected like those of larger bodies of rock. The color of rock,
its texture and its composition, also influence its range of daily temperature
by influencing absorption and conduction. Dark-colored rocks absorb more
heat than light-colored ones, and compact rocks are better conductors than
porous ones. Great absorption and slow conduction favor disruption. A
given range of temperature is unequally effective on rocks of different
mineral composition. In general crystalline rocks (igneous and
The daily range of temperature is also influenced by humidity. Because
of the effect of water vapor in the atmosphere on insolation and radiation, a
rock surface becomes hotter in the day and cooler at night beneath a dry
atmosphere than beneath a moist one. Aridity therefore favors the disruption
of rock by changing temperatures.
Turning from the conditions of the atmosphere which affect the
disruption of rock to the conditions of the rock which influence the same
process, several points are to be noted. In the first place, the disrupting
effects of changes of temperature are slight or nil where the solid rock is
protected by soil, clay, sand, gravel, snow, or other incoherent material. If
the constituent parts of the loose material are coarse, like bowlders, their
surfaces are affected like those of larger bodies of rock. The color of rock,
its texture and its composition, also influence its range of daily temperature
by influencing absorption and conduction. Dark-colored rocks absorb more
heat than light-colored ones, and compact rocks are better conductors than
porous ones. Great absorption and slow conduction favor disruption. A
given range of temperature is unequally effective on rocks of different
mineral composition. In general crystalline rocks (igneous and
Page 81
metamorphic) are more subject to disruption by this means than
sedimentary rocks, partly because they are more compact, but especially
because they are made up of aggregates of crystals of different minerals
which, under changes of temperature, expand and contract at different rates,
while the common sedimentary rocks are made up largely of numerous
particles of one mineral.
Fig. 29.—Top of Notch Peak, Bighorn Mountains, Wyo. Shows the thoroughly broken
character of the rock on the summit, the absence of soil, vegetation, etc. (Kümmel.)
Fig. 30.—A detail from Fig. 29 showing the size of the rock blocks. (Kümmel.)
sedimentary rocks, partly because they are more compact, but especially
because they are made up of aggregates of crystals of different minerals
which, under changes of temperature, expand and contract at different rates,
while the common sedimentary rocks are made up largely of numerous
particles of one mineral.
Fig. 29.—Top of Notch Peak, Bighorn Mountains, Wyo. Shows the thoroughly broken
character of the rock on the summit, the absence of soil, vegetation, etc. (Kümmel.)
Fig. 30.—A detail from Fig. 29 showing the size of the rock blocks. (Kümmel.)
Page 82
Fig. 31.—Peak north of Kearsarge Pass, the Sierras. Shows the way in which serrate peaks
break up into angular blocks.
The freezing of water in the pores of rock is effective in disrupting them
only when the pores are essentially full at the time of freezing. Otherwise
there is room for the expansion attending the freezing. If the pores of the
rock are large, the expansion on freezing may force out sufficient water to
balance the increase of volume, even though the rock was completely
saturated. If the pores be very small the water passes out less readily, and if
the rock is saturated, freezing is more likely to be attended with disruption.
[21]
In view of these considerations the breaking of rock by changes of
temperature should be greatest on the bare slopes of isolated elevations of
crystalline rock, where the temperature conditions of temperate latitudes
prevail, and where the atmosphere is relatively free from moisture. All these
conditions are not often found in one place, but the disrupting effects of
changing temperatures are best seen where several of them are associated
(Figs. 29, 30, and 31).
The importance of this method of rock-breaking has rarely been
appreciated except by those who have worked in high and dry regions.
Climbers of high mountains know that almost every high peak is covered
break up into angular blocks.
The freezing of water in the pores of rock is effective in disrupting them
only when the pores are essentially full at the time of freezing. Otherwise
there is room for the expansion attending the freezing. If the pores of the
rock are large, the expansion on freezing may force out sufficient water to
balance the increase of volume, even though the rock was completely
saturated. If the pores be very small the water passes out less readily, and if
the rock is saturated, freezing is more likely to be attended with disruption.
[21]
In view of these considerations the breaking of rock by changes of
temperature should be greatest on the bare slopes of isolated elevations of
crystalline rock, where the temperature conditions of temperate latitudes
prevail, and where the atmosphere is relatively free from moisture. All these
conditions are not often found in one place, but the disrupting effects of
changing temperatures are best seen where several of them are associated
(Figs. 29, 30, and 31).
The importance of this method of rock-breaking has rarely been
appreciated except by those who have worked in high and dry regions.
Climbers of high mountains know that almost every high peak is covered
Page 83
with broken rock to such an extent as to make its ascent dangerous to the
uninitiated. High serrate peaks, especially of crystalline rock, are, as a rule,
literally crumbling to pieces (Fig. 31). The piles of talus which lie at the
bases of steep mountain slopes are often hundreds of feet in height, and
their materials are often in large part the result of the process here under
discussion. In mountain regions where atmospheric conditions favor sudden
changes of temperature, the sharp reports of the disruption of rock masses
are often heard. Masses of rock, scores and even hundreds of pounds in
weight, are frequently thus detached and started on their downward course.
[22]
Small pieces of rock are of course much more commonly broken off than
large ones. The disruption of rock by changes of temperature is not usually
the result of a single change of temperature, but rather of many successive
expansions and contractions.
The sharp needle-like peaks which mark the summits of most high
mountain ranges (Fig. 32) are largely developed by the process here
outlined. The altitude at which the serrate topography appears varies with
the latitude, being, as a rule, higher in low latitudes and lower in high. But
even in the same latitude it varies notably with the isolation of the
mountains and with the aridity of the climate. Thus within the United States
the sharply serrate summits appear in some places, as in Washington and
Oregon, at altitudes of 6000 to 10,000 feet, while in the isolated Wichita
range of Oklahoma, much farther south, but in a much drier climate, the
same sort of topography is developed at altitudes of 2500 to 3000 feet.
Even in low latitudes and moist climates the effects of temperature
changes are often seen. Thin beds of limestone at the bottom of quarries are
sometimes so expanded by the heat of the sun as to arch up and break.[23] In
desert and arid regions,[24] whatever the altitude, the effects of temperature
changes are often striking.
uninitiated. High serrate peaks, especially of crystalline rock, are, as a rule,
literally crumbling to pieces (Fig. 31). The piles of talus which lie at the
bases of steep mountain slopes are often hundreds of feet in height, and
their materials are often in large part the result of the process here under
discussion. In mountain regions where atmospheric conditions favor sudden
changes of temperature, the sharp reports of the disruption of rock masses
are often heard. Masses of rock, scores and even hundreds of pounds in
weight, are frequently thus detached and started on their downward course.
[22]
Small pieces of rock are of course much more commonly broken off than
large ones. The disruption of rock by changes of temperature is not usually
the result of a single change of temperature, but rather of many successive
expansions and contractions.
The sharp needle-like peaks which mark the summits of most high
mountain ranges (Fig. 32) are largely developed by the process here
outlined. The altitude at which the serrate topography appears varies with
the latitude, being, as a rule, higher in low latitudes and lower in high. But
even in the same latitude it varies notably with the isolation of the
mountains and with the aridity of the climate. Thus within the United States
the sharply serrate summits appear in some places, as in Washington and
Oregon, at altitudes of 6000 to 10,000 feet, while in the isolated Wichita
range of Oklahoma, much farther south, but in a much drier climate, the
same sort of topography is developed at altitudes of 2500 to 3000 feet.
Even in low latitudes and moist climates the effects of temperature
changes are often seen. Thin beds of limestone at the bottom of quarries are
sometimes so expanded by the heat of the sun as to arch up and break.[23] In
desert and arid regions,[24] whatever the altitude, the effects of temperature
changes are often striking.
Page 84
Fig. 32.—Serrate peaks of granitic rock in Black Hills. (Darton, U. S. Geol. Surv.)
The disruption of rock by changes of temperature is one phase of
weathering. It tends to the formation of a mantle of rock waste, which, were
it not removed, would soon completely cover the solid rock beneath and
protect it from further disruption by heating and cooling; but the loose
material thus produced becomes an easy prey to running water, so that the
work of the atmosphere prepares the way for that of other eroding agencies.
II. Evaporation and Precipitation.
Perhaps the most important work of the atmosphere as a dynamic agent
lies in its function as the medium for the circulation and distribution of
water. Atmospheric temperature is the primary factor governing
evaporation, an important factor in the circulation of the vapor after it is
formed, and controls its condensation and precipitation.
The average amount of annual precipitation on the land is variously
estimated at from forty to sixty inches, the lesser figure being probably
more nearly correct. Since much of this water falls at high altitudes, the
work which it accomplishes in getting back to the sea is great. The water
which falls on the land, if withdrawn wholly from the ocean, would exhaust
The disruption of rock by changes of temperature is one phase of
weathering. It tends to the formation of a mantle of rock waste, which, were
it not removed, would soon completely cover the solid rock beneath and
protect it from further disruption by heating and cooling; but the loose
material thus produced becomes an easy prey to running water, so that the
work of the atmosphere prepares the way for that of other eroding agencies.
II. Evaporation and Precipitation.
Perhaps the most important work of the atmosphere as a dynamic agent
lies in its function as the medium for the circulation and distribution of
water. Atmospheric temperature is the primary factor governing
evaporation, an important factor in the circulation of the vapor after it is
formed, and controls its condensation and precipitation.
The average amount of annual precipitation on the land is variously
estimated at from forty to sixty inches, the lesser figure being probably
more nearly correct. Since much of this water falls at high altitudes, the
work which it accomplishes in getting back to the sea is great. The water
which falls on the land, if withdrawn wholly from the ocean, would exhaust
Page 85
that body of water in 10,000 to 15,000 years if none of it returned. The
work of evaporation is of course not done by the atmosphere, though the
atmosphere determines the effect of the solar energy which does the work.
[25]
The precipitation is distributed with great inequality, and this inequality
affects both the rain and the snow. Some regions have heavy precipitation
and some light; some regions have much rain and little snow; others have
much snow and little rain; others have rain and no snow, and still others
have snow and little or no rain. The amount and distribution of rain and
snow determine the size and distribution of streams and glaciers, and
streams and glaciers are the most important agencies modifying the surface
of the land.
It is impossible to separate sharply the geologic work of the water of the
atmosphere from that of other waters; but so long as moisture is in the
atmosphere (including the time of its precipitation) its effects are best
considered in connection with the atmosphere.
The mechanical work of the rain.—In falling the rain washes the
atmosphere, taking from it much of the dust, spores, etc., which the winds
have lifted from the surface of the dry land. Not only this, but in passing
through the atmosphere the water dissolves some of its gases, and perhaps
particles of soluble solid matter. When therefore the falling water reaches
the surface of the land it is no longer pure, and some of the gases it has
taken up in its descent enable it to dissolve various mineral matters on
which pure water has little effect.
As it falls on the surface of the land the rain produces various effects of a
mechanical nature. In the first place, it leaves on the surface the solid matter
taken from the air. The amount of material, thus added to any given region
in any particular shower is trivial, but in the course of long periods of time
the total amount of material washed out of the air must be very great.
Every rain-drop strikes a blow. If the drops fall on vegetation, they have
little effect, but if they fall on sand or unprotected earthy matter they cause
movements of the particles on one another, and this movement involves
friction and wear. While the results thus effected are inconsiderable in any
brief period of time, they are not so insignificant when the long periods of
the earth’s history are considered.
work of evaporation is of course not done by the atmosphere, though the
atmosphere determines the effect of the solar energy which does the work.
[25]
The precipitation is distributed with great inequality, and this inequality
affects both the rain and the snow. Some regions have heavy precipitation
and some light; some regions have much rain and little snow; others have
much snow and little rain; others have rain and no snow, and still others
have snow and little or no rain. The amount and distribution of rain and
snow determine the size and distribution of streams and glaciers, and
streams and glaciers are the most important agencies modifying the surface
of the land.
It is impossible to separate sharply the geologic work of the water of the
atmosphere from that of other waters; but so long as moisture is in the
atmosphere (including the time of its precipitation) its effects are best
considered in connection with the atmosphere.
The mechanical work of the rain.—In falling the rain washes the
atmosphere, taking from it much of the dust, spores, etc., which the winds
have lifted from the surface of the dry land. Not only this, but in passing
through the atmosphere the water dissolves some of its gases, and perhaps
particles of soluble solid matter. When therefore the falling water reaches
the surface of the land it is no longer pure, and some of the gases it has
taken up in its descent enable it to dissolve various mineral matters on
which pure water has little effect.
As it falls on the surface of the land the rain produces various effects of a
mechanical nature. In the first place, it leaves on the surface the solid matter
taken from the air. The amount of material, thus added to any given region
in any particular shower is trivial, but in the course of long periods of time
the total amount of material washed out of the air must be very great.
Every rain-drop strikes a blow. If the drops fall on vegetation, they have
little effect, but if they fall on sand or unprotected earthy matter they cause
movements of the particles on one another, and this movement involves
friction and wear. While the results thus effected are inconsiderable in any
brief period of time, they are not so insignificant when the long periods of
the earth’s history are considered.
Page 86
Clayey soils contract and often crack on drying. Falling on such a soil
when it is dry the rain causes it to expand, and the cracks are healed by
lateral swelling. The same soils are baked under the influence of the sun,
and when in this condition are softened and made more mobile by the
falling of rain. Under the influence of the expansion and contraction
occasioned by wetting and drying, the soils and earths on slopes creep
slowly downward. When rain falls on dry sand or dust the cohesion is at
once increased, and shifting by the wind is temporarily stopped.
After the water has fallen on the land its further work cannot be looked
upon as a part of the work of the atmosphere; but any conception of the
geological work of the atmosphere which did not recognize the fact that the
waters of the land have come through the atmosphere would be inadequate.
The work of the water after it has been precipitated from the atmosphere
must be considered in another chapter.
III. Effects of Electricity.
Another dynamic effect conditioned by the atmosphere is that produced
by lightning. In the aggregate this result is inconsequential; yet instances
are known where large bodies of rock have been fractured by a stroke of
lightning, and masses many tons in weight have sometimes been moved
appreciable distances. Incipient fusion in very limited spots is also known
to have been induced by lightning. Where it strikes sand it often fuses the
sand for a short distance, and, on cooling, the partially fused material is
consolidated, forming a little tube or irregular rod (a fulgurite) of partially
glassy matter. Fulgurites are usually only a few inches in length, and more
commonly than otherwise a fraction of an inch in diameter. Strictly
speaking these results are the effect of the electricity of the atmosphere
rather than of the atmosphere itself, but they are best mentioned in this
connection.
Allusion has already been made to the chemical changes in the
atmosphere occasioned by electric discharges.
when it is dry the rain causes it to expand, and the cracks are healed by
lateral swelling. The same soils are baked under the influence of the sun,
and when in this condition are softened and made more mobile by the
falling of rain. Under the influence of the expansion and contraction
occasioned by wetting and drying, the soils and earths on slopes creep
slowly downward. When rain falls on dry sand or dust the cohesion is at
once increased, and shifting by the wind is temporarily stopped.
After the water has fallen on the land its further work cannot be looked
upon as a part of the work of the atmosphere; but any conception of the
geological work of the atmosphere which did not recognize the fact that the
waters of the land have come through the atmosphere would be inadequate.
The work of the water after it has been precipitated from the atmosphere
must be considered in another chapter.
III. Effects of Electricity.
Another dynamic effect conditioned by the atmosphere is that produced
by lightning. In the aggregate this result is inconsequential; yet instances
are known where large bodies of rock have been fractured by a stroke of
lightning, and masses many tons in weight have sometimes been moved
appreciable distances. Incipient fusion in very limited spots is also known
to have been induced by lightning. Where it strikes sand it often fuses the
sand for a short distance, and, on cooling, the partially fused material is
consolidated, forming a little tube or irregular rod (a fulgurite) of partially
glassy matter. Fulgurites are usually only a few inches in length, and more
commonly than otherwise a fraction of an inch in diameter. Strictly
speaking these results are the effect of the electricity of the atmosphere
rather than of the atmosphere itself, but they are best mentioned in this
connection.
Allusion has already been made to the chemical changes in the
atmosphere occasioned by electric discharges.
Page 87
Fig. 33.—Stratified jointed rock in process of weathering. (Cross, U. S. Geol. Surv.)
Page 88
Fig. 34.—Represents a later stage of the processes illustrated by Fig. 33. (Darton, U. S.
Geol. Surv.)
SUMMARY.
Weathering.—The result of all atmospheric processes, whether physical
or chemical, by which surface rock is disrupted, decomposed or in any way
loosened, is weathering. This convenient term also includes similar results
effected by ground water, plants, etc. The tendency of weathering is to
produce a mantle of residuary earth over solid rock. Weathering by
mechanical means tends to produce material which, though in a finer state
of division, is still like the original rock in chemical composition.
Weathering by chemical means tends to produce a mantle made up chiefly
of the less soluble parts of the rock from which it was derived. All processes
of weathering prepare material for transportation by wind and water.
Geol. Surv.)
SUMMARY.
Weathering.—The result of all atmospheric processes, whether physical
or chemical, by which surface rock is disrupted, decomposed or in any way
loosened, is weathering. This convenient term also includes similar results
effected by ground water, plants, etc. The tendency of weathering is to
produce a mantle of residuary earth over solid rock. Weathering by
mechanical means tends to produce material which, though in a finer state
of division, is still like the original rock in chemical composition.
Weathering by chemical means tends to produce a mantle made up chiefly
of the less soluble parts of the rock from which it was derived. All processes
of weathering prepare material for transportation by wind and water.
Page 89
Fig. 35.—Details of a weathered rock surface, due partly to wind work and partly to
solution. The particular phase of weathering illustrated by this figure is known as
“honeycomb” weathering. (Gilbert, U. S. Geol. Surv.)
Many considerations determine the thickness which the mantle of
weathered rock (mantle rock) attains. Some of these considerations have to
do with the atmosphere, and some with drainage. Since the latter are, on the
whole, more important, this matter will be discussed in connection with the
work of water (Chapters III and IV).
solution. The particular phase of weathering illustrated by this figure is known as
“honeycomb” weathering. (Gilbert, U. S. Geol. Surv.)
Many considerations determine the thickness which the mantle of
weathered rock (mantle rock) attains. Some of these considerations have to
do with the atmosphere, and some with drainage. Since the latter are, on the
whole, more important, this matter will be discussed in connection with the
work of water (Chapters III and IV).
Page 90
CHAPTER III.
THE WORK OF RUNNING WATER.
Familiar phenomena, both of land and sea, reveal the constant activity and
importance of water as a geologic agent. Even when there is no precipitation the
moisture in the air influences its activity in certain ways. Just as iron “rusts” more
readily in moist air than in dry, so changes in other mineral substances are
influenced by atmospheric humidity. Where precipitation takes place the results are
more obvious. The passing shower works changes in the surface of the land,
striking in proportion to the rate and amount of precipitation. The rains feed the
streams, and every stream is modifying its bed, and with increasing rapidity as its
current is swollen. Even the moisture which is precipitated as snow works its
appropriate results. Before it melts it protects the surface against other agents of
change; but if it accumulates in sufficient quantity in appropriate situations, it may
give rise to avalanches and glaciers, which, like running water, degrade the surface
over which they pass.
A part of the water which falls as rain, and a part of that which results from the
melting of snow and ice, sinks into the soil and into the rock below, becoming
ground water. It is this ground water which especially justifies the name
hydrosphere, often applied to the waters of the earth, for it literally forms a
spherical layer in the outer portion of the solid part of the earth. During the stay of
the water beneath the surface it effects changes in the rocks through which it
passes, dissolving mineral matter here and depositing it there, substituting one
substance for another in this place, and effecting new chemical combinations in
that. Slow as these processes are, they have worked wondrous changes in the
course of the earth’s history.
When the waters are gathered together in ponds, lakes, and oceans, they are still
active, and the results of their activity are seen along the shores, where winds and
waves produce their chiefest effects. Even the ocean currents, far from land, and the
processes of the deep sea, are not without their effect on the course of geological
history.
The work of the surface waters, ground (underground) waters, standing waters,
and ice will be considered in order.
THE WORK OF RUNNING WATER.
Familiar phenomena, both of land and sea, reveal the constant activity and
importance of water as a geologic agent. Even when there is no precipitation the
moisture in the air influences its activity in certain ways. Just as iron “rusts” more
readily in moist air than in dry, so changes in other mineral substances are
influenced by atmospheric humidity. Where precipitation takes place the results are
more obvious. The passing shower works changes in the surface of the land,
striking in proportion to the rate and amount of precipitation. The rains feed the
streams, and every stream is modifying its bed, and with increasing rapidity as its
current is swollen. Even the moisture which is precipitated as snow works its
appropriate results. Before it melts it protects the surface against other agents of
change; but if it accumulates in sufficient quantity in appropriate situations, it may
give rise to avalanches and glaciers, which, like running water, degrade the surface
over which they pass.
A part of the water which falls as rain, and a part of that which results from the
melting of snow and ice, sinks into the soil and into the rock below, becoming
ground water. It is this ground water which especially justifies the name
hydrosphere, often applied to the waters of the earth, for it literally forms a
spherical layer in the outer portion of the solid part of the earth. During the stay of
the water beneath the surface it effects changes in the rocks through which it
passes, dissolving mineral matter here and depositing it there, substituting one
substance for another in this place, and effecting new chemical combinations in
that. Slow as these processes are, they have worked wondrous changes in the
course of the earth’s history.
When the waters are gathered together in ponds, lakes, and oceans, they are still
active, and the results of their activity are seen along the shores, where winds and
waves produce their chiefest effects. Even the ocean currents, far from land, and the
processes of the deep sea, are not without their effect on the course of geological
history.
The work of the surface waters, ground (underground) waters, standing waters,
and ice will be considered in order.
Page 91
RAIN AND RIVER EROSION.
Rain and river erosion began when the first rains fell on land surfaces. Neither
the location nor the nature of the first land surface is known. There is little reason
to believe that the ocean was ever universal, but there is reason to believe that most
land areas have at some time or other been covered by the sea. The prevalent
conception that land areas which were once submerged came into existence by
being elevated above sea-level, should be supplemented by the alternative
conception that submerged areas may have become land by the depression of the
ocean basins, thus drawing off the water from the areas where it was shallow. Thus
in Fig. 36 the sinking of the sea-bottom from a to b would lower the surface of the
water from cc′, to dd′, and draw off the water from the surfaces cd and c′d′.
Fig. 36.—Diagram to illustrate the origin of lands by the lowering of the sea-level due to depression
of the sea bottom. If the bottom is depressed from a to b the surface will be drawn down from cc′
to dd′, and the surfaces cd and c′d′ will become land.
Without attempting to picture the character of the original land our study of
subaërial erosion may begin with an area which has just been changed from sea
bottom to land. What is the nature of such a land surface? Of what material is it
composed, and what is the character of its topography? Concerning its constitution
something may be inferred from the nature of the deposits now found at the bottom
of the sea. Near the shore and in shallow water they often consist of gravel and
sand, though other materials are not wanting. Far from shore and in deep water they
consist for the most part of fine sediments, some of which were washed or blown
from the land, some of which came from the shells and other secretions of marine
animals, some from volcanoes, and some from various other sources. The
topography of the newly emerged land may have had some likeness to the
topography of the sea bottom. The numerous soundings which have been made
over large areas of the sea have shown that its bottom is, as a rule, free from the
numerous small irregularities which affect the surface of the land. They seem to
show that a large part of the ocean bottom is so nearly flat that, if the water were
removed, the eye would hardly detect irregularities in the surface. This statement
does not lose sight of the fact that the ocean bottom is, in certain places, markedly
irregular. Volcanic peaks and striking irregularities of other sorts abound in some
places. Nevertheless if the bottom of the sea could be seen as the land is, its most
striking feature, taken as a whole, would be its apparent flatness.
Rain and river erosion began when the first rains fell on land surfaces. Neither
the location nor the nature of the first land surface is known. There is little reason
to believe that the ocean was ever universal, but there is reason to believe that most
land areas have at some time or other been covered by the sea. The prevalent
conception that land areas which were once submerged came into existence by
being elevated above sea-level, should be supplemented by the alternative
conception that submerged areas may have become land by the depression of the
ocean basins, thus drawing off the water from the areas where it was shallow. Thus
in Fig. 36 the sinking of the sea-bottom from a to b would lower the surface of the
water from cc′, to dd′, and draw off the water from the surfaces cd and c′d′.
Fig. 36.—Diagram to illustrate the origin of lands by the lowering of the sea-level due to depression
of the sea bottom. If the bottom is depressed from a to b the surface will be drawn down from cc′
to dd′, and the surfaces cd and c′d′ will become land.
Without attempting to picture the character of the original land our study of
subaërial erosion may begin with an area which has just been changed from sea
bottom to land. What is the nature of such a land surface? Of what material is it
composed, and what is the character of its topography? Concerning its constitution
something may be inferred from the nature of the deposits now found at the bottom
of the sea. Near the shore and in shallow water they often consist of gravel and
sand, though other materials are not wanting. Far from shore and in deep water they
consist for the most part of fine sediments, some of which were washed or blown
from the land, some of which came from the shells and other secretions of marine
animals, some from volcanoes, and some from various other sources. The
topography of the newly emerged land may have had some likeness to the
topography of the sea bottom. The numerous soundings which have been made
over large areas of the sea have shown that its bottom is, as a rule, free from the
numerous small irregularities which affect the surface of the land. They seem to
show that a large part of the ocean bottom is so nearly flat that, if the water were
removed, the eye would hardly detect irregularities in the surface. This statement
does not lose sight of the fact that the ocean bottom is, in certain places, markedly
irregular. Volcanic peaks and striking irregularities of other sorts abound in some
places. Nevertheless if the bottom of the sea could be seen as the land is, its most
striking feature, taken as a whole, would be its apparent flatness.
Page 92
With the topography of the sea bottom the topography of the land is, in its
details, in sharp contrast. In order to get at the history of the latter, we may study
the sequence of events which would follow the emergence of a portion of the
former.
Subaërial Erosion without Valleys.
For the sake of emphasizing the fundamental principles involved in the work of
running water, a hypothetical case will first be studied in some detail, even at the
risk of elaborating processes already understood. The principles themselves will
find application later in relations which are much less simple.
Let it be assumed that the area of newly emerged land is a circular dome-shaped
island. The simplest possible condition is represented by assuming its slope to be
the same in all directions from the center, and its materials to be absolutely
homogeneous. Such an island would be subject to all the forces ordinarily operating
on land surfaces. The chief agency tending to modify land surfaces is atmospheric
precipitation. It will be assumed that the rain falls on the surface of the island with
absolute equality at all points, and that all other forces which affect it operate
equally everywhere.
The rain falling on a land area disappears in various ways; part of it evaporates,
part of it sinks, and part of it runs off over the surface. If the island be composed of
fine and unconsolidated materials, such as clay, the water which runs off over the
surface will carry sediment down to the sea. If the island be composed of solid rock
instead, exposure to the air will cause it to decay, and the products of decay, such as
sand and mud, will suffer a like fate.
For the sake of a clear understanding of the processes involved, two cases may
be postulated; one in which the waters of the sea remove the sediment washed
down from the hypothetical island as fast as it reaches the shore, and one in which
they allow it to accumulate without let or hindrance. In both cases the wear of the
waves will be neglected.
1. In the first case the water flowing off over the surface (the run-off) will
descend equally in all directions. It will constitute a continuous sheet of surface-
water, and both its volume and its velocity will be the same at all points equally
distant from the summit. Erosion accomplished by sheets of running water, as
distinct from streams, is sheet (or sheet-flood) erosion.[26] Since the material of the
surface is homogeneous, the wear effected by the water will be equal at all points
where its velocity and volume are equal. For obvious reasons the depth of the run-
off will increase from summit to base. The gradient (slope) also increases in the
same direction, and the increase of volume and of gradient conspire to augment the
details, in sharp contrast. In order to get at the history of the latter, we may study
the sequence of events which would follow the emergence of a portion of the
former.
Subaërial Erosion without Valleys.
For the sake of emphasizing the fundamental principles involved in the work of
running water, a hypothetical case will first be studied in some detail, even at the
risk of elaborating processes already understood. The principles themselves will
find application later in relations which are much less simple.
Let it be assumed that the area of newly emerged land is a circular dome-shaped
island. The simplest possible condition is represented by assuming its slope to be
the same in all directions from the center, and its materials to be absolutely
homogeneous. Such an island would be subject to all the forces ordinarily operating
on land surfaces. The chief agency tending to modify land surfaces is atmospheric
precipitation. It will be assumed that the rain falls on the surface of the island with
absolute equality at all points, and that all other forces which affect it operate
equally everywhere.
The rain falling on a land area disappears in various ways; part of it evaporates,
part of it sinks, and part of it runs off over the surface. If the island be composed of
fine and unconsolidated materials, such as clay, the water which runs off over the
surface will carry sediment down to the sea. If the island be composed of solid rock
instead, exposure to the air will cause it to decay, and the products of decay, such as
sand and mud, will suffer a like fate.
For the sake of a clear understanding of the processes involved, two cases may
be postulated; one in which the waters of the sea remove the sediment washed
down from the hypothetical island as fast as it reaches the shore, and one in which
they allow it to accumulate without let or hindrance. In both cases the wear of the
waves will be neglected.
1. In the first case the water flowing off over the surface (the run-off) will
descend equally in all directions. It will constitute a continuous sheet of surface-
water, and both its volume and its velocity will be the same at all points equally
distant from the summit. Erosion accomplished by sheets of running water, as
distinct from streams, is sheet (or sheet-flood) erosion.[26] Since the material of the
surface is homogeneous, the wear effected by the water will be equal at all points
where its velocity and volume are equal. For obvious reasons the depth of the run-
off will increase from summit to base. The gradient (slope) also increases in the
same direction, and the increase of volume and of gradient conspire to augment the
Page 93
velocity of the water, and therefore of the wear effected by it. If the thin sheet of
water starting from the top of the island with relatively low velocity be able to wash
off even a little fine material from the surface, the thicker sheet farther down the
slope, moving with greater velocity, will be able to carry away more of the same
sort of material, and the increase will be progressive from summit to base. It
follows, therefore, that the surface will be worn equally at points equally distant
from the summit, but unequally at points unequally distant from it. The first shower
which falls on the island may be conceived to wash off from its surface a very thin
sheet of material, but a sheet which increases in thickness from top to bottom. The
run-off will not be stopped immediately on reaching the sea, but will displace the
sea-water to some slight depth, and wear the surface some trivial distance below
the normal level of the sea. The result of successive showers working in the same
way through a long period of time will be to diminish the area of the island and to
steepen its slopes. The results of a considerable period of erosion under these
conditions are shown diagrammatically in Fig. 37, which illustrates both the
diminution in area which the island has suffered, and the increase in the angle of its
slopes. Immediately about it, at the stage represented by aa, Fig. 37, there is a
narrow marginal platform, or submerged terrace, in place of the land area which
has been worn away at or just below the level of the sea. Long successions of rains
working in the same way will give the island steeper slopes, a smaller area, and a
wider marginal terrace. Successive stages are shown by the lines bb and cc, Fig. 37.
Fig. 37.—Diagram to illustrate the effect of rain erosion on an island where there is no deposition or
wave erosion about its borders. The uppermost curve represents the original surface, while aa, bb,
and cc represent successive surfaces developed by sheet erosion, on the supposition that no
material is deposited along the shores.
If rain falls on such an island until it completes the work which it is possible for
running water to do, the island will be reduced essentially to the level of the sea,
and in its place there will be a plain, the area of which will be equal to that of the
original island. Its central point will be at the level of the sea, and its borders a
trifling distance below it (Fig. 38). The island is gone, and in its place there is a
plain as low as running water can wear it. Other agencies might come in to defeat
the result just outlined, but if the island did not rise or sink after its formation, rain
falling upon it would, under the conditions specified, finally bring about the result
which has been sketched. The plain (Fig. 38) which succeeds the island is a base-
level of erosion, though this term is also used in other ways. Under these conditions
the slope of the land would remain convex at all stages, but the convex erosion
profile of the land would meet a nearly straight line just below sea-level. The
relative lengths of these two elements of the profile, the curve above and the
water starting from the top of the island with relatively low velocity be able to wash
off even a little fine material from the surface, the thicker sheet farther down the
slope, moving with greater velocity, will be able to carry away more of the same
sort of material, and the increase will be progressive from summit to base. It
follows, therefore, that the surface will be worn equally at points equally distant
from the summit, but unequally at points unequally distant from it. The first shower
which falls on the island may be conceived to wash off from its surface a very thin
sheet of material, but a sheet which increases in thickness from top to bottom. The
run-off will not be stopped immediately on reaching the sea, but will displace the
sea-water to some slight depth, and wear the surface some trivial distance below
the normal level of the sea. The result of successive showers working in the same
way through a long period of time will be to diminish the area of the island and to
steepen its slopes. The results of a considerable period of erosion under these
conditions are shown diagrammatically in Fig. 37, which illustrates both the
diminution in area which the island has suffered, and the increase in the angle of its
slopes. Immediately about it, at the stage represented by aa, Fig. 37, there is a
narrow marginal platform, or submerged terrace, in place of the land area which
has been worn away at or just below the level of the sea. Long successions of rains
working in the same way will give the island steeper slopes, a smaller area, and a
wider marginal terrace. Successive stages are shown by the lines bb and cc, Fig. 37.
Fig. 37.—Diagram to illustrate the effect of rain erosion on an island where there is no deposition or
wave erosion about its borders. The uppermost curve represents the original surface, while aa, bb,
and cc represent successive surfaces developed by sheet erosion, on the supposition that no
material is deposited along the shores.
If rain falls on such an island until it completes the work which it is possible for
running water to do, the island will be reduced essentially to the level of the sea,
and in its place there will be a plain, the area of which will be equal to that of the
original island. Its central point will be at the level of the sea, and its borders a
trifling distance below it (Fig. 38). The island is gone, and in its place there is a
plain as low as running water can wear it. Other agencies might come in to defeat
the result just outlined, but if the island did not rise or sink after its formation, rain
falling upon it would, under the conditions specified, finally bring about the result
which has been sketched. The plain (Fig. 38) which succeeds the island is a base-
level of erosion, though this term is also used in other ways. Under these conditions
the slope of the land would remain convex at all stages, but the convex erosion
profile of the land would meet a nearly straight line just below sea-level. The
relative lengths of these two elements of the profile, the curve above and the
Page 94
straight line below, vary as erosion progresses, the convex portion becoming
shorter and the other longer, The two parts of the profile taken together are concave
upward at the lower end all the time, and for a greater distance from its lower end
in all the advanced stages of erosion (Fig. 37).
Fig. 38.—Diagram to illustrate the final effect of rain erosion under the conditions specified in the
text. The diagram expresses the final result of the processes suggested by Fig. 37.
In the destruction of the land under these conditions neither valleys nor hills
would be developed, nor would the topography of the land be fashioned to
correspond with the surfaces with which we are familiar.
It is to be distinctly borne in mind that the foregoing is a hypothetical case; it is
not probable that such an island ever existed, or ever will; but that does not
diminish the value of the illustration, since the principles involved are operating on
every land mass, though in less simple relations.
2. The second case differs from the first in that the sediment washed down from
the land is deposited about its borders. This results in the building up of a marginal
platform, as shown in Figs. 39–41. As erosion goes on more sediment is washed
down and deposited, partly on the narrow marginal shelf which has already been
developed, and partly on its outer slope, as shown in the figures. The marginal flat
is thus extended beyond the original shores of the island on the one hand, and
toward its center on the other. As it develops, its inner portion, and indeed all
except its outer edge (ab, Figs. 40 and 41), will be gradually built up above the
level of the water. This marginal lowland is developed at a level as low as running
water, under the conditions then and there present, can reduce the land. Such a
surface may be said to be at grade, since running water neither wears it down nor
builds it up. Its angle of slope is a function of (1) the volume of the water running
over it, and (2) of the load which the water carries.
shorter and the other longer, The two parts of the profile taken together are concave
upward at the lower end all the time, and for a greater distance from its lower end
in all the advanced stages of erosion (Fig. 37).
Fig. 38.—Diagram to illustrate the final effect of rain erosion under the conditions specified in the
text. The diagram expresses the final result of the processes suggested by Fig. 37.
In the destruction of the land under these conditions neither valleys nor hills
would be developed, nor would the topography of the land be fashioned to
correspond with the surfaces with which we are familiar.
It is to be distinctly borne in mind that the foregoing is a hypothetical case; it is
not probable that such an island ever existed, or ever will; but that does not
diminish the value of the illustration, since the principles involved are operating on
every land mass, though in less simple relations.
2. The second case differs from the first in that the sediment washed down from
the land is deposited about its borders. This results in the building up of a marginal
platform, as shown in Figs. 39–41. As erosion goes on more sediment is washed
down and deposited, partly on the narrow marginal shelf which has already been
developed, and partly on its outer slope, as shown in the figures. The marginal flat
is thus extended beyond the original shores of the island on the one hand, and
toward its center on the other. As it develops, its inner portion, and indeed all
except its outer edge (ab, Figs. 40 and 41), will be gradually built up above the
level of the water. This marginal lowland is developed at a level as low as running
water, under the conditions then and there present, can reduce the land. Such a
surface may be said to be at grade, since running water neither wears it down nor
builds it up. Its angle of slope is a function of (1) the volume of the water running
over it, and (2) of the load which the water carries.
Page 95
Fig. 39–41.—Diagrams to illustrate the effect of rain erosion on an island when all the eroded
material is deposited about the shore. The black portions represent deposition. The dotted lines
represent the original surface. The several diagrams represent successive stages in the process.
Since the marginal plain of the above illustration extends beyond the original
shore of the island, the area of land is increased, though both its average elevation
and its mass (above water) are reduced. In case destructive processes did not
operate on the marginal graded plain the spreading and lowering suggested by Figs.
39 and 40 would go on until the central mass of the island was brought down to a
gradient in harmony with that of the gently sloping border, as shown in Fig. 41.
When this had been accomplished there would be a relatively large land area with
low slopes (Fig. 41) in place of the smaller area with steeper ones (compare Figs.
39 and 40). The basal part of the larger island from the center to the original margin
would be made up of the original material in its original position (unshaded part of
Fig. 41). Its surface would be covered, least deeply near its center and most deeply
near the original margin, with débris gradually shifted from higher levels, as shown
in Fig. 41.
Were such an island as that shown in Fig. 41 once formed, the rain falling on it,
and flowing off over its surface, would carry off its surface soil and spread it about
the shores. Though the surface of the marginal flat of Fig. 40 was as low as running
water could bring it at the time it was developed, the conditions of erosion have
changed by the time the land reaches the conditions shown in Fig. 41, and the same
amount of rainfall may now be effective in erosion. In the first case (Fig. 40) the
water descending from the higher part of the land brought down sediment and
started across the flat with a load. Its energy was consumed in transporting what it
had, not in getting new material. In the second case (Fig. 41) the water flowing
over the gently sloping surface has no initial load, and its energy is therefore
available for erosion. Under continued rainfall, the area of the land shown in Fig.
41 would be increased as before by successive marginal deposits (see Fig. 42), and
at the same time its average height would be reduced. The lowering and enlarging
of the island would continue until the whole surface was brought so nearly to the
level of the sea that water would cease to run over it with sufficient velocity to
material is deposited about the shore. The black portions represent deposition. The dotted lines
represent the original surface. The several diagrams represent successive stages in the process.
Since the marginal plain of the above illustration extends beyond the original
shore of the island, the area of land is increased, though both its average elevation
and its mass (above water) are reduced. In case destructive processes did not
operate on the marginal graded plain the spreading and lowering suggested by Figs.
39 and 40 would go on until the central mass of the island was brought down to a
gradient in harmony with that of the gently sloping border, as shown in Fig. 41.
When this had been accomplished there would be a relatively large land area with
low slopes (Fig. 41) in place of the smaller area with steeper ones (compare Figs.
39 and 40). The basal part of the larger island from the center to the original margin
would be made up of the original material in its original position (unshaded part of
Fig. 41). Its surface would be covered, least deeply near its center and most deeply
near the original margin, with débris gradually shifted from higher levels, as shown
in Fig. 41.
Were such an island as that shown in Fig. 41 once formed, the rain falling on it,
and flowing off over its surface, would carry off its surface soil and spread it about
the shores. Though the surface of the marginal flat of Fig. 40 was as low as running
water could bring it at the time it was developed, the conditions of erosion have
changed by the time the land reaches the conditions shown in Fig. 41, and the same
amount of rainfall may now be effective in erosion. In the first case (Fig. 40) the
water descending from the higher part of the land brought down sediment and
started across the flat with a load. Its energy was consumed in transporting what it
had, not in getting new material. In the second case (Fig. 41) the water flowing
over the gently sloping surface has no initial load, and its energy is therefore
available for erosion. Under continued rainfall, the area of the land shown in Fig.
41 would be increased as before by successive marginal deposits (see Fig. 42), and
at the same time its average height would be reduced. The lowering and enlarging
of the island would continue until the whole surface was brought so nearly to the
level of the sea that water would cease to run over it with sufficient velocity to
Page 96
carry away even the fine material of its surface. Such a surface, brought down as
low as running water can degrade it, is also (see p. 57) a base-level. It will be seen
from the foregoing illustrations that a graded surface may pass into a base-level,
with no sharper line of demarkation than that which separates a mature man from
an old one. In this case, as in the preceding, the island has been base-leveled, but
still without the formation of valleys or hills.
Fig. 42.—Diagram to illustrate the result of the continuation of the processes shown in Figs. 39–41.
Both the preceding hypothetical cases make it clear that, from the point of view
of erosion, every drop of water which runs off over the surface of the land has for
its mission the getting of the land into the sea. Under ordinary conditions surface
drainage must fail to bring a land area altogether to sea-level, the absolute base-
level of subaërial forces; but it is not simply the water which runs off over the
surface which degrades the land. That which sinks beneath the surface contributes
to the same end by slowly dissolving mineral matter below the surface, and finally
carrying it to the sea. In this way the reduction of land areas to sea-level may be
completed.
The rain-water which evaporates from the surface without sinking beneath it
does not effect much wear; but the water thus evaporated is subject to
reprecipitation, so that, in the long run, it may assist in the work which has been
sketched. Thus it is not simply the waters which run off over the surface of the
land, but all which fall upon it, which unite to compass its destruction.
The Development of Valleys.
By the growth of gullies.—Had the slopes of the hypothetical island not been
absolutely uniform the processes of erosion would have been different. Let the
departure from uniformity be supposed to consist of a single slight meridional
depression near the base of the island (Fig. 43). As the rain falls it will no longer
run off equally in all directions. A greater volume will flow through the depression
than over other parts of the surface having the same altitude, and the greater
volume of water along this line will give greater velocity, greater velocity will
occasion greater erosion, and greater erosion will deepen the depression. The
immediate result is a gully or wash (Fig. 44). So soon as the gully is started it tends
still further to concentrate drainage in itself, and is thereby enlarged. The water
which enters it from the sides widens it; that which enters at its head lengthens it by
causing its upper end to recede; and all which flows through it, so long as its
bottom is above base-level, deepens it. The enlarged gully will gather more water
low as running water can degrade it, is also (see p. 57) a base-level. It will be seen
from the foregoing illustrations that a graded surface may pass into a base-level,
with no sharper line of demarkation than that which separates a mature man from
an old one. In this case, as in the preceding, the island has been base-leveled, but
still without the formation of valleys or hills.
Fig. 42.—Diagram to illustrate the result of the continuation of the processes shown in Figs. 39–41.
Both the preceding hypothetical cases make it clear that, from the point of view
of erosion, every drop of water which runs off over the surface of the land has for
its mission the getting of the land into the sea. Under ordinary conditions surface
drainage must fail to bring a land area altogether to sea-level, the absolute base-
level of subaërial forces; but it is not simply the water which runs off over the
surface which degrades the land. That which sinks beneath the surface contributes
to the same end by slowly dissolving mineral matter below the surface, and finally
carrying it to the sea. In this way the reduction of land areas to sea-level may be
completed.
The rain-water which evaporates from the surface without sinking beneath it
does not effect much wear; but the water thus evaporated is subject to
reprecipitation, so that, in the long run, it may assist in the work which has been
sketched. Thus it is not simply the waters which run off over the surface of the
land, but all which fall upon it, which unite to compass its destruction.
The Development of Valleys.
By the growth of gullies.—Had the slopes of the hypothetical island not been
absolutely uniform the processes of erosion would have been different. Let the
departure from uniformity be supposed to consist of a single slight meridional
depression near the base of the island (Fig. 43). As the rain falls it will no longer
run off equally in all directions. A greater volume will flow through the depression
than over other parts of the surface having the same altitude, and the greater
volume of water along this line will give greater velocity, greater velocity will
occasion greater erosion, and greater erosion will deepen the depression. The
immediate result is a gully or wash (Fig. 44). So soon as the gully is started it tends
still further to concentrate drainage in itself, and is thereby enlarged. The water
which enters it from the sides widens it; that which enters at its head lengthens it by
causing its upper end to recede; and all which flows through it, so long as its
bottom is above base-level, deepens it. The enlarged gully will gather more water
Page 97
to itself, and, as before, increased volume means increased velocity, and increased
velocity increased erosion. As the gully grows, therefore, its increased size
becomes the occasion of still further enlargement.
Fig. 43.—Diagram showing a slight meridional depression in the surface of an otherwise even-sloped
island.
Continued growth transforms the gully into a ravine, though between a gully and
a ravine there is no distinct line of demarkation. But growth does not stop with
ravine-hood. Water from every shower gathers in the ravine, and, flowing through
it, increases its length, width, and depth, until it reaches such proportions that the
term ravine is laid aside, as childhood names are, and the depression becomes a
valley.
Fig. 44.—Diagram illustrating the development of a gully, starting from the condition shown in Fig.
43.
It was assumed in the preceding paragraphs that the single depression in the
slope was meridional and low on the slope, but almost any sort of depression in
almost any position would bring about a similar result, since it would lead to
concentration of the run-off. Had the original surface been interrupted by ridges
instead of depressions, the effect on valley development would have been much the
same, for a ridge, like a depression, would, in almost any position, occasion the
concentration of the run-off, and so the development of valleys. Under the
conditions represented in Fig. 44 the lengthening of the drainage depression is
effected chiefly at its upper end, the head of the valley working its way farther and
farther back into the land. This method of elongation is known as head erosion. But
the lengthening of the valley is not always wholly by head erosion. The gully
normally begins where concentration of run-off begins, and if this were not at sea-
level, the gully might be lengthening at both ends at the same time. This would
have been the case, for example, had the original depression of Fig. 43 been half-
way up the slope of the island.
If while the slopes of the island were absolutely uniform its surface material
failed of homogeneity, the result would be much the same as if the slopes were
unequal. If the material lying along a certain meridian of the island be slightly
softer than that over the rest of the surface, the run-off, which would at the outset
velocity increased erosion. As the gully grows, therefore, its increased size
becomes the occasion of still further enlargement.
Fig. 43.—Diagram showing a slight meridional depression in the surface of an otherwise even-sloped
island.
Continued growth transforms the gully into a ravine, though between a gully and
a ravine there is no distinct line of demarkation. But growth does not stop with
ravine-hood. Water from every shower gathers in the ravine, and, flowing through
it, increases its length, width, and depth, until it reaches such proportions that the
term ravine is laid aside, as childhood names are, and the depression becomes a
valley.
Fig. 44.—Diagram illustrating the development of a gully, starting from the condition shown in Fig.
43.
It was assumed in the preceding paragraphs that the single depression in the
slope was meridional and low on the slope, but almost any sort of depression in
almost any position would bring about a similar result, since it would lead to
concentration of the run-off. Had the original surface been interrupted by ridges
instead of depressions, the effect on valley development would have been much the
same, for a ridge, like a depression, would, in almost any position, occasion the
concentration of the run-off, and so the development of valleys. Under the
conditions represented in Fig. 44 the lengthening of the drainage depression is
effected chiefly at its upper end, the head of the valley working its way farther and
farther back into the land. This method of elongation is known as head erosion. But
the lengthening of the valley is not always wholly by head erosion. The gully
normally begins where concentration of run-off begins, and if this were not at sea-
level, the gully might be lengthening at both ends at the same time. This would
have been the case, for example, had the original depression of Fig. 43 been half-
way up the slope of the island.
If while the slopes of the island were absolutely uniform its surface material
failed of homogeneity, the result would be much the same as if the slopes were
unequal. If the material lying along a certain meridian of the island be slightly
softer than that over the rest of the surface, the run-off, which would at the outset
Page 98
be equal on all sides, would effect more erosion along the line of the less resistant
material than elsewhere. The result would be a depression along this line, and, once
started, the depression would be a cause of its own growth. If the soft material were
disposed in any way other than that indicated, the final result would be much the
same, for it would quickly give origin to a depression which would lead to the
concentration of the surface-waters, and this is the condition for the development of
a gully, a ravine, and finally a valley.
In the presence of sufficient rainfall,
either heterogeneity of slope or of material
will therefore occasion the development of
valleys. If the lack of uniformity appears at
but a single point there will be but a single
valley. If it appears at many points the
number of valleys will be large. Since it is
incredible that a land mass of perfectly
homogeneous material and of absolutely
uniform slopes ever existed, it is believed
that every land mass, affected for any
considerable length of time by rain, has had
valleys developed in it. The degree of
heterogeneity of material and slope is
usually so great as to lead to the Fig. 45.—Diagram to illustrate the effect of
development of many valleys, even on sheet and stream erosion on the outline of
an island when no deposition takes place
areas which are not large; but for the sake about its borders. The dotted line
of emphasizing the simpler elements of the represents the original outline of the
island, the full line its border at a later
complex processes of stream work, the time. The stream develops a reëntrant
hypothetical case of an island with but a (bay) in the outline.
single valley, and that without tributaries,
may first be studied. Under these conditions two cases may be considered, the one
where there is no deposition about the island, and the other where deposition takes
place.
1. If all the material eroded from the surface of such an island, both in and out of
the valley, were carried well beyond the borders of the land before being deposited,
the edge of the island would recede from its original position toward the center, as
illustrated by Figs. 37 and 45; but the recession would be most rapid where the
valley joins the sea (Fig. 45). At this point therefore a reëntrant would be developed
(a, Fig. 45), and the island would lose its circular outline. Continued erosion would
cause the shore-line to retreat on all sides, but fastest at the lower end of the valley,
and the final result would be a base-level differing from that developed under the
material than elsewhere. The result would be a depression along this line, and, once
started, the depression would be a cause of its own growth. If the soft material were
disposed in any way other than that indicated, the final result would be much the
same, for it would quickly give origin to a depression which would lead to the
concentration of the surface-waters, and this is the condition for the development of
a gully, a ravine, and finally a valley.
In the presence of sufficient rainfall,
either heterogeneity of slope or of material
will therefore occasion the development of
valleys. If the lack of uniformity appears at
but a single point there will be but a single
valley. If it appears at many points the
number of valleys will be large. Since it is
incredible that a land mass of perfectly
homogeneous material and of absolutely
uniform slopes ever existed, it is believed
that every land mass, affected for any
considerable length of time by rain, has had
valleys developed in it. The degree of
heterogeneity of material and slope is
usually so great as to lead to the Fig. 45.—Diagram to illustrate the effect of
development of many valleys, even on sheet and stream erosion on the outline of
an island when no deposition takes place
areas which are not large; but for the sake about its borders. The dotted line
of emphasizing the simpler elements of the represents the original outline of the
island, the full line its border at a later
complex processes of stream work, the time. The stream develops a reëntrant
hypothetical case of an island with but a (bay) in the outline.
single valley, and that without tributaries,
may first be studied. Under these conditions two cases may be considered, the one
where there is no deposition about the island, and the other where deposition takes
place.
1. If all the material eroded from the surface of such an island, both in and out of
the valley, were carried well beyond the borders of the land before being deposited,
the edge of the island would recede from its original position toward the center, as
illustrated by Figs. 37 and 45; but the recession would be most rapid where the
valley joins the sea (Fig. 45). At this point therefore a reëntrant would be developed
(a, Fig. 45), and the island would lose its circular outline. Continued erosion would
cause the shore-line to retreat on all sides, but fastest at the lower end of the valley,
and the final result would be a base-level differing from that developed under the
Page 99
conditions specified on p. 60, in that the last part to be brought low would not be
the center of the original island.
Under the foregoing conditions the
profile of that part of the valley which is
above sea-level (cb) would be convex,
following the analogy of sheet erosion on a
hypothetical island of uniform slopes and
homogeneous material with no marginal
deposition. Its side slopes, likewise
developed under the influence of running
water augmented in volume from top to
bottom, would also be convex.
2. If the sediment washed down from the
land is deposited about its borders, both the
outline of the island and the profile of the
valley will be altered. Deposition at the
debouchure of the valley follows the same
Fig. 46.—Diagram showing the outline of an principles as deposition elsewhere; but if all
island as modified by sheet and stream the sediment brought to the sea be
erosion where eroded material is deposited
at the shore. The dotted line represents the
deposited at the shore, the seaward
original outline; the full line, a later one. extension of the land by deposition would
The excess of deposition at the end of the be more rapid opposite the valley than
valley causes a projection of land into the
sea. elsewhere, and the island would lose its
circular outline, and develop some such
form as is shown in Fig. 46. In this case the profile of the upper end of the valley,
and the upper parts of its side slopes, as well as the upper parts of the extra-valley
slopes of the island, are convex (compare Figs. 39 and 40); but the convexity above
is exchanged for concavity below, the change beginning at the point where
downward erosion of the descending waters is checked. As a valley lengthens, the
larger part of its profile becomes concave (compare the profiles of Figs. 39 to 41),
but the extreme upper end still remains convex. Since the side slopes of a valley are
much shorter than its lengthwise slope, a larger proportion remains convex. Under
the conditions here discussed the change from convexity above to concavity below
would begin at about the point where deposition begins.[27]
the center of the original island.
Under the foregoing conditions the
profile of that part of the valley which is
above sea-level (cb) would be convex,
following the analogy of sheet erosion on a
hypothetical island of uniform slopes and
homogeneous material with no marginal
deposition. Its side slopes, likewise
developed under the influence of running
water augmented in volume from top to
bottom, would also be convex.
2. If the sediment washed down from the
land is deposited about its borders, both the
outline of the island and the profile of the
valley will be altered. Deposition at the
debouchure of the valley follows the same
Fig. 46.—Diagram showing the outline of an principles as deposition elsewhere; but if all
island as modified by sheet and stream the sediment brought to the sea be
erosion where eroded material is deposited
at the shore. The dotted line represents the
deposited at the shore, the seaward
original outline; the full line, a later one. extension of the land by deposition would
The excess of deposition at the end of the be more rapid opposite the valley than
valley causes a projection of land into the
sea. elsewhere, and the island would lose its
circular outline, and develop some such
form as is shown in Fig. 46. In this case the profile of the upper end of the valley,
and the upper parts of its side slopes, as well as the upper parts of the extra-valley
slopes of the island, are convex (compare Figs. 39 and 40); but the convexity above
is exchanged for concavity below, the change beginning at the point where
downward erosion of the descending waters is checked. As a valley lengthens, the
larger part of its profile becomes concave (compare the profiles of Figs. 39 to 41),
but the extreme upper end still remains convex. Since the side slopes of a valley are
much shorter than its lengthwise slope, a larger proportion remains convex. Under
the conditions here discussed the change from convexity above to concavity below
would begin at about the point where deposition begins.[27]
Page 100
Fig. 47.—Diagram representing several meridional valleys developing in a circular island. The
valleys are all young and narrow. All are making deposits at their debouchures.
The deposition at the debouchure of the valley, and later above the debouchure,
will follow the same course as about the island under the conditions already
discussed (pp. 61, 62).
Limits of growth.—In all cases there are limits in depth, length, and width,
beyond which a valley may not grow. In depth it may reach base-level. At the coast,
base-level is sea-level,[28] but inland it rises by a gentle gradient. In length, the
valley will grow as long as its head continues to work inland. In the case
represented by Figs. 45 and 46 the head of the valley would not cease to advance
when the center of the island was reached, though beyond that point head erosion
would not be more rapid than lateral erosion on either side. If but a single valley
affected a land area the limit toward which it would tend, and beyond which it
could never pass, would be the length of the land area in the direction of the
valley’s axis. In width, a valley is increased by the side cutting of the stream, by the
wash of the rain which falls on its slopes, and by the action of gravity which tends
to carry down to the bottom of the slope the material which is loosened above by
any process whatsoever. If there be but one valley in a land area its limiting width
is scarcely less than the width of the land itself.
valleys are all young and narrow. All are making deposits at their debouchures.
The deposition at the debouchure of the valley, and later above the debouchure,
will follow the same course as about the island under the conditions already
discussed (pp. 61, 62).
Limits of growth.—In all cases there are limits in depth, length, and width,
beyond which a valley may not grow. In depth it may reach base-level. At the coast,
base-level is sea-level,[28] but inland it rises by a gentle gradient. In length, the
valley will grow as long as its head continues to work inland. In the case
represented by Figs. 45 and 46 the head of the valley would not cease to advance
when the center of the island was reached, though beyond that point head erosion
would not be more rapid than lateral erosion on either side. If but a single valley
affected a land area the limit toward which it would tend, and beyond which it
could never pass, would be the length of the land area in the direction of the
valley’s axis. In width, a valley is increased by the side cutting of the stream, by the
wash of the rain which falls on its slopes, and by the action of gravity which tends
to carry down to the bottom of the slope the material which is loosened above by
any process whatsoever. If there be but one valley in a land area its limiting width
is scarcely less than the width of the land itself.
Page 101
Fig. 48.—Same as Fig. 47, with the valleys more developed. The dotted line represents the original
outline of the island. Its area is being extended by deposition everywhere, but most at the
debouchures of the streams.
Fig. 49.—A later stage of the island shown in Fig. 48.
outline of the island. Its area is being extended by deposition everywhere, but most at the
debouchures of the streams.
Fig. 49.—A later stage of the island shown in Fig. 48.
Page 102
Had there been several initial meridional
depressions instead of one in the island, or
had there been several meridional belts
where the material of the surface was less
Fig. 50.—Diagram to illustrate the lowering
resistant than elsewhere, several valleys of a divide without shifting it. The crest of
would have been developed, converging the divide is at a, b, and c successively. If
toward the center (Fig. 47). If the erosion were unequal on the two sides, the
divide would be shifted.
conditions were such as to allow of the
equal development of valleys on all sides of the island, each would be lengthened
by head erosion until it reached the center of the island, where the permanent divide
between their heads would be established. Each would be widened by all the
processes which widen valleys, and their widening would narrow the intervening
areas (Figs. 48 and 49). Under conditions of equal erosion the limits of width for
each valley would be the centers of the ridges on either side, and here the divides
between them would be permanently established. Though erosion would continue
even after the crest of the ridge had been narrowed to a line, the permanence of the
divide would follow from the fact that erosion would be equal on both sides of this
line, and its effect would be to lower the divide, but not to shift it horizontally (Fig.
50). The limits in length and width are therefore not the same where there are
several valleys as where there is but one. The limit in depth, however, remains the
same, and the final result of erosion, proceeding along these lines, would be the
base-leveling of the land, leaving a plain but slightly above sea-level. The plain
would not be absolutely flat, though its relief would be very slight, and the higher
parts would be along the lines of the divides between the streams (Fig. 51.
Compare also Fig. 42). Many valleys would occasion more rapid degradation than
few, and the period of base-leveling would be correspondingly shortened.
Had the initial depressions which gave origin to the valleys had positions other
than meridional, the valleys would have had other and less regularly radial courses,
but the final result of their development would have been the same.
It is not to be inferred that the method of valley development which has been
sketched is the only one. The processes of valley development are complex, and the
history of some valleys has run a different course; yet the processes outlined above
are in operation in all cases, and they were probably the most important ones in the
development of the first drainage system on any land surface. As will be seen in the
sequel the history of valleys is subject to serious accidents, and they are often of
such a nature as to mask the simplicity of the more normal processes.
depressions instead of one in the island, or
had there been several meridional belts
where the material of the surface was less
Fig. 50.—Diagram to illustrate the lowering
resistant than elsewhere, several valleys of a divide without shifting it. The crest of
would have been developed, converging the divide is at a, b, and c successively. If
toward the center (Fig. 47). If the erosion were unequal on the two sides, the
divide would be shifted.
conditions were such as to allow of the
equal development of valleys on all sides of the island, each would be lengthened
by head erosion until it reached the center of the island, where the permanent divide
between their heads would be established. Each would be widened by all the
processes which widen valleys, and their widening would narrow the intervening
areas (Figs. 48 and 49). Under conditions of equal erosion the limits of width for
each valley would be the centers of the ridges on either side, and here the divides
between them would be permanently established. Though erosion would continue
even after the crest of the ridge had been narrowed to a line, the permanence of the
divide would follow from the fact that erosion would be equal on both sides of this
line, and its effect would be to lower the divide, but not to shift it horizontally (Fig.
50). The limits in length and width are therefore not the same where there are
several valleys as where there is but one. The limit in depth, however, remains the
same, and the final result of erosion, proceeding along these lines, would be the
base-leveling of the land, leaving a plain but slightly above sea-level. The plain
would not be absolutely flat, though its relief would be very slight, and the higher
parts would be along the lines of the divides between the streams (Fig. 51.
Compare also Fig. 42). Many valleys would occasion more rapid degradation than
few, and the period of base-leveling would be correspondingly shortened.
Had the initial depressions which gave origin to the valleys had positions other
than meridional, the valleys would have had other and less regularly radial courses,
but the final result of their development would have been the same.
It is not to be inferred that the method of valley development which has been
sketched is the only one. The processes of valley development are complex, and the
history of some valleys has run a different course; yet the processes outlined above
are in operation in all cases, and they were probably the most important ones in the
development of the first drainage system on any land surface. As will be seen in the
sequel the history of valleys is subject to serious accidents, and they are often of
such a nature as to mask the simplicity of the more normal processes.
Page 103
Fig. 51.—Diagram illustrating the further development of Fig. 49. The land here has been reduced
greatly, though not yet to base-level.
The permanent stream.—From the foregoing discussion, it is seen that a valley
may be developed by the run-off of successive showers. If supplied only from this
source surface streams would cease to flow soon after the rain ceased to fall, and a
valley might attain considerable size without possessing a permanent stream. How
does the valley developed by the run-off of successive showers come to have a
permanent stream? The answer to this question involves a brief consideration of
that part of the rainfall which sinks beneath the surface.
If wells be sunk in a flat region of uniform structure and composition the water
in them is generally found to stand at a nearly common level. The meaning of this
fact is not far to seek. If a hole 60 feet deep fills with water up to a point 20 feet
from the surface, it is because the material in which the well is sunk is full of water
up to that level. When the well is dug the water leaks into it, filling the hole up to
the level to which the rock (or subsoil) is itself full. This level, below which the
rock and subsoil (down to unknown depths) are full of water, is known as the
ground-water level, ground-water surface, or water-table.
The ground-water level fluctuates. In a wet season it rises, because more water
has fallen and sunk beneath the soil; but several processes at once conspire to bring
greatly, though not yet to base-level.
The permanent stream.—From the foregoing discussion, it is seen that a valley
may be developed by the run-off of successive showers. If supplied only from this
source surface streams would cease to flow soon after the rain ceased to fall, and a
valley might attain considerable size without possessing a permanent stream. How
does the valley developed by the run-off of successive showers come to have a
permanent stream? The answer to this question involves a brief consideration of
that part of the rainfall which sinks beneath the surface.
If wells be sunk in a flat region of uniform structure and composition the water
in them is generally found to stand at a nearly common level. The meaning of this
fact is not far to seek. If a hole 60 feet deep fills with water up to a point 20 feet
from the surface, it is because the material in which the well is sunk is full of water
up to that level. When the well is dug the water leaks into it, filling the hole up to
the level to which the rock (or subsoil) is itself full. This level, below which the
rock and subsoil (down to unknown depths) are full of water, is known as the
ground-water level, ground-water surface, or water-table.
The ground-water level fluctuates. In a wet season it rises, because more water
has fallen and sunk beneath the soil; but several processes at once conspire to bring
Page 104
it down again. Where there is growing vegetation its roots draw up water from
beneath, and evaporation also goes on independently of vegetation. The water is
drawn out through wells and runs out through openings. It may also flow
underground from one region to another where the ground-water surface is lower.
All these processes depress the ground-water surface.
A well sunk to such a level as to be
supplied with abundant water in a wet
season may go dry during a period of
drought because the ground-water level is
depressed below its bottom. Thus either
well shown in Fig. 52 will have water
during a wet season when the water-level is Fig. 52.—Diagram illustrating the
at a; but well No. 1 will go dry when the fluctuation of a ground-water surface. a =
wet-weather ground-water level; b =
water surface is depressed to b. ground-water level during drought. Well
No. 1 will contain water during the wet
The principles applicable to wells are season, but will go dry in times of drought.
applicable to valleys. When a valley has Well No. 2 will be permanent.
been deepened until its bottom reaches below the ground-water level, water seeps
or flows into it from the sides. The valley is then no longer dependent on the run-
off of showers for a stream. It will be readily seen that at some stage in its
development, the bottom of a valley may be below the ground-water level of a wet
season without being below that of a dry one. Thus the valley represented in cross-
section by the line 2–2, in Fig. 53, will have a stream when the ground-water level
is at aa, but none when this level is depressed to bb. If the rainfall of the year were
concentrated in a single wet season, the intermittent stream would flow not only
during that season, but for so long a time afterward as the ground-water level
remained well above the valley bottom. In regions subject to frequent and short
periods of heavy precipitation, alternating with droughts, the periods of intermittent
flow may be many and short. Since the precipitation of many regions varies greatly
from year to year, it follows that a stream may flow continuously one year and be
intermittent the next. Many valleys in various parts of the earth are now in the stage
of development where their streams are intermittent.
As a valley containing an intermittent stream becomes deeper, the periods when
it is dry become shorter, and when it has been sunk below the lowest ground-water
level, it will have a permanent stream (3, Fig. 53). Since a valley normally develops
headward, its lower and older portion is likely to acquire a permanent stream, while
its upper and younger part has only an intermittent one (Fig. 47 and Fig. 1, Pl. III,
near Anthony, Kan. The intermittent part of the stream is indicated by the dotted
blue line). For the same reason the head of a stream is likely to be farther up the
valley in wet weather than in dry. So soon as a valley gets a permanent stream, the
beneath, and evaporation also goes on independently of vegetation. The water is
drawn out through wells and runs out through openings. It may also flow
underground from one region to another where the ground-water surface is lower.
All these processes depress the ground-water surface.
A well sunk to such a level as to be
supplied with abundant water in a wet
season may go dry during a period of
drought because the ground-water level is
depressed below its bottom. Thus either
well shown in Fig. 52 will have water
during a wet season when the water-level is Fig. 52.—Diagram illustrating the
at a; but well No. 1 will go dry when the fluctuation of a ground-water surface. a =
wet-weather ground-water level; b =
water surface is depressed to b. ground-water level during drought. Well
No. 1 will contain water during the wet
The principles applicable to wells are season, but will go dry in times of drought.
applicable to valleys. When a valley has Well No. 2 will be permanent.
been deepened until its bottom reaches below the ground-water level, water seeps
or flows into it from the sides. The valley is then no longer dependent on the run-
off of showers for a stream. It will be readily seen that at some stage in its
development, the bottom of a valley may be below the ground-water level of a wet
season without being below that of a dry one. Thus the valley represented in cross-
section by the line 2–2, in Fig. 53, will have a stream when the ground-water level
is at aa, but none when this level is depressed to bb. If the rainfall of the year were
concentrated in a single wet season, the intermittent stream would flow not only
during that season, but for so long a time afterward as the ground-water level
remained well above the valley bottom. In regions subject to frequent and short
periods of heavy precipitation, alternating with droughts, the periods of intermittent
flow may be many and short. Since the precipitation of many regions varies greatly
from year to year, it follows that a stream may flow continuously one year and be
intermittent the next. Many valleys in various parts of the earth are now in the stage
of development where their streams are intermittent.
As a valley containing an intermittent stream becomes deeper, the periods when
it is dry become shorter, and when it has been sunk below the lowest ground-water
level, it will have a permanent stream (3, Fig. 53). Since a valley normally develops
headward, its lower and older portion is likely to acquire a permanent stream, while
its upper and younger part has only an intermittent one (Fig. 47 and Fig. 1, Pl. III,
near Anthony, Kan. The intermittent part of the stream is indicated by the dotted
blue line). For the same reason the head of a stream is likely to be farther up the
valley in wet weather than in dry. So soon as a valley gets a permanent stream, the
Page 105
process of enlargement goes on without the interruption to which it was subject
when the supply of water was intermittent.
Fig. 53.—Diagram to illustrate the intermittency of streams due to fluctuations of the ground-water
level. The water level aa would be depressed next the valley 2–2 by the flow of the water into the
valley. The profile of the ground-water surface would therefore be aca rather than aa.
In general a permanent stream at one point in a valley means a continuous stream
from that point to the sea or lake which the valley joins; but to this rule there are
many exceptions. They are likely to arise where a stream heads in a region of
abundant precipitation, and flows thence through an arid tract where the ground-
water level is low, and evaporation great. In such cases, evaporation and absorption
may dissipate the water gathered above, and the stream disappears (Fig. 2, Pl. III,
near Paradise, Nev.).
PLATE III.
when the supply of water was intermittent.
Fig. 53.—Diagram to illustrate the intermittency of streams due to fluctuations of the ground-water
level. The water level aa would be depressed next the valley 2–2 by the flow of the water into the
valley. The profile of the ground-water surface would therefore be aca rather than aa.
In general a permanent stream at one point in a valley means a continuous stream
from that point to the sea or lake which the valley joins; but to this rule there are
many exceptions. They are likely to arise where a stream heads in a region of
abundant precipitation, and flows thence through an arid tract where the ground-
water level is low, and evaporation great. In such cases, evaporation and absorption
may dissipate the water gathered above, and the stream disappears (Fig. 2, Pl. III,
near Paradise, Nev.).
PLATE III.
Page 106
U. S. Geol. Surv. Fig. 1.
KANSA Scale, 2+ mile per inch.
S. U. S. Geol. Surv. Fig. 2. NEVADA. Scale, 4+ mile per inch.
KANSA Scale, 2+ mile per inch.
S. U. S. Geol. Surv. Fig. 2. NEVADA. Scale, 4+ mile per inch.
Page 107
PLATE IV.
U. S. Geol. Surv. Fig. 1. ILLINOIS. Scale, 1+ mile per inch.
U. S. Geol. Surv. Fig. 1. ILLINOIS. Scale, 1+ mile per inch.
Page 108
U. S. Geol. Surv. Fig. 2. NORTH DAKOTA. Scale, 2+ mile per inch.
Other modes of valley development.—If as a new area of land emerges from
the sea its surface has a depression without an outlet, and such an assumption is by
no means improbable, the depression would be filled with sea-water. The inflowing
water from the surrounding land might fill the basin to overflowing, and the
outflow, finding exit at the lowest point in the rim of the basin, would flow thence
toward the sea. Such a stream would develop a valley, the history of which would
be somewhat different from that which has been sketched. Instead of developing
headward from the sea, the valley would be in process of excavation all the way
from the initial basin to the sea at the same time (Fig. 54). The upper end of the
valley might ultimately be cut to the level of the bottom of the basin, when the lake
would disappear. The head of the valley might then work back across the former
site of the lake into the territory beyond. Valleys might have developed above the
lake before it was drained, and after this event, such valleys would make
connections with the valley below (Fig. 55). A valley developed in this manner is
not simply a gully grown big by head erosion, and the valley would not precede the
stream.
Other modes of valley development.—If as a new area of land emerges from
the sea its surface has a depression without an outlet, and such an assumption is by
no means improbable, the depression would be filled with sea-water. The inflowing
water from the surrounding land might fill the basin to overflowing, and the
outflow, finding exit at the lowest point in the rim of the basin, would flow thence
toward the sea. Such a stream would develop a valley, the history of which would
be somewhat different from that which has been sketched. Instead of developing
headward from the sea, the valley would be in process of excavation all the way
from the initial basin to the sea at the same time (Fig. 54). The upper end of the
valley might ultimately be cut to the level of the bottom of the basin, when the lake
would disappear. The head of the valley might then work back across the former
site of the lake into the territory beyond. Valleys might have developed above the
lake before it was drained, and after this event, such valleys would make
connections with the valley below (Fig. 55). A valley developed in this manner is
not simply a gully grown big by head erosion, and the valley would not precede the
stream.
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Fig. 54.—Diagram to show how a valley may be developing all the way from a water-filled basin
(lake) to the sea at the same time. Small valleys leading to the lake are also developing. The black
area = the sea.
(lake) to the sea at the same time. Small valleys leading to the lake are also developing. The black
area = the sea.
Page 110
Fig. 55.—The stream leading out from the lake (Fig. 54) has drained the lake, and the valleys above
and below the site of the former lake have united.
If a surface of land were notably irregular before valleys were developed in it,
there might be many lakes, and the flow from a higher lake might pass to a lower. If
the lakes were ultimately drained, the several sections of the valley would be joined
to one another without intervening basins. In certain regions, especially those
which have been affected by continental ice-sheets, this has been a common
method of valley development in post-glacial time. In this case also the stream
precedes its valley, and not the valley its stream. Many post-glacial valleys, on the
other hand, antedated their permanent streams, as in the cases first described.
and below the site of the former lake have united.
If a surface of land were notably irregular before valleys were developed in it,
there might be many lakes, and the flow from a higher lake might pass to a lower. If
the lakes were ultimately drained, the several sections of the valley would be joined
to one another without intervening basins. In certain regions, especially those
which have been affected by continental ice-sheets, this has been a common
method of valley development in post-glacial time. In this case also the stream
precedes its valley, and not the valley its stream. Many post-glacial valleys, on the
other hand, antedated their permanent streams, as in the cases first described.
Page 111
Fig. 56.—Diagram showing the phases of valley development described in the text.
If the gradient of a slope on which valleys are to develop is notably unequal,
though without basins, the development of valleys may follow somewhat different
lines. If on emergence the seaward part of a new land area assumes the form of a
plain, bordered landward by a steeper slope (Fig. 56), the most notable early
growth of the valleys would be on the latter. The run-off would develop gullies on
the steep slope, but on reaching the plain below the velocity of the water would be
checked, and it would drop much of the detritus washed down from above. This
deposition would build up (aggrade) the surface, and much or even all the water
might sink into and seep through the débris thus deposited, and disappear altogether
from the surface, as at b, Fig. 56. This would be most likely to occur where the
débris is abundant and coarse, and the precipitation slight. If the water disappears at
the base of the mountain (see Fig. 2, Pl. III), the early growth of the valley may be
confined to the steep slope remote from the sea (ab, Fig. 56); but on the slope
where the valley is growing there will be headward lengthening, as in the general
case already considered. If the surface drainage does not disappear at the base of
the steep slope, the run-off will find its way over the plain along the lowest
accessible route to the sea (de, Fig. 56). In this case the valley may be growing
throughout its length at the same time.
If the gradient of a slope on which valleys are to develop is notably unequal,
though without basins, the development of valleys may follow somewhat different
lines. If on emergence the seaward part of a new land area assumes the form of a
plain, bordered landward by a steeper slope (Fig. 56), the most notable early
growth of the valleys would be on the latter. The run-off would develop gullies on
the steep slope, but on reaching the plain below the velocity of the water would be
checked, and it would drop much of the detritus washed down from above. This
deposition would build up (aggrade) the surface, and much or even all the water
might sink into and seep through the débris thus deposited, and disappear altogether
from the surface, as at b, Fig. 56. This would be most likely to occur where the
débris is abundant and coarse, and the precipitation slight. If the water disappears at
the base of the mountain (see Fig. 2, Pl. III), the early growth of the valley may be
confined to the steep slope remote from the sea (ab, Fig. 56); but on the slope
where the valley is growing there will be headward lengthening, as in the general
case already considered. If the surface drainage does not disappear at the base of
the steep slope, the run-off will find its way over the plain along the lowest
accessible route to the sea (de, Fig. 56). In this case the valley may be growing
throughout its length at the same time.
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The conditions represented by ab, Fig. 56, may
be no more than temporary. Sooner or later a valley
developing headward across the plain (hi, Fig. 56)
may provide a channel for the water descending
from the higher land beyond. In this case the valley
develops in sections, the one on the slope above,
the other on the plain below, and their union
(compare fghi, Fig. 56, with Fig. 57) results from
their growth.
The principles here sketched have been in
operation wherever land areas were so elevated as
to give rise to unequal slopes, and this has perhaps
been the rule rather than the exception. The results
effected by the operation of these principles would
of course be dependent on the varieties of slope, on
the abruptness with which a slope of one gradient
gave place to another, on the texture of the rock,
the amount and distribution of precipitation, etc.,
etc.
Fig. 57.—Diagram representing the In the preceding paragraphs the lengthening of a
further development of the valley at its upper end by head erosion has been
valleys fg and hi in Fig. 56. The
repeatedly referred to. If all valleys began their
head of the latter (Fig. 56) has
worked back until it has reacheddevelopment at the sea and lengthened headward, it
the lower end of the former. might seem that their seaward ends should be their
oldest parts; but since the development of valleys is begun somewhat promptly
after the land appears above the sea, and since the emergence is generally gradual,
that part of a valley which is at the seashore at one time may be far inland a little
later, because the land has been extended seaward. On an emerging land area
therefore the normal growth of a valley involves its lengthening at its lower end as
well as at its upper. The lengthening of a valley, or at least the lengthening of a
stream, also takes place at its lower end if the land in which it lies is being extended
seaward by deposition.
Structural valleys.—In mountain regions valleys are sometimes formed by the
uplift of parallel mountain folds, leaving a depression between (Fig. 58). Drainage
will appropriate such a valley so that it becomes in some sense a river valley. But it
is not a river valley in the sense in which the term has been used in the preceding
pages. It is rather a structural valley. In its bottom a river valley may be developed
(a, Fig. 58).
be no more than temporary. Sooner or later a valley
developing headward across the plain (hi, Fig. 56)
may provide a channel for the water descending
from the higher land beyond. In this case the valley
develops in sections, the one on the slope above,
the other on the plain below, and their union
(compare fghi, Fig. 56, with Fig. 57) results from
their growth.
The principles here sketched have been in
operation wherever land areas were so elevated as
to give rise to unequal slopes, and this has perhaps
been the rule rather than the exception. The results
effected by the operation of these principles would
of course be dependent on the varieties of slope, on
the abruptness with which a slope of one gradient
gave place to another, on the texture of the rock,
the amount and distribution of precipitation, etc.,
etc.
Fig. 57.—Diagram representing the In the preceding paragraphs the lengthening of a
further development of the valley at its upper end by head erosion has been
valleys fg and hi in Fig. 56. The
repeatedly referred to. If all valleys began their
head of the latter (Fig. 56) has
worked back until it has reacheddevelopment at the sea and lengthened headward, it
the lower end of the former. might seem that their seaward ends should be their
oldest parts; but since the development of valleys is begun somewhat promptly
after the land appears above the sea, and since the emergence is generally gradual,
that part of a valley which is at the seashore at one time may be far inland a little
later, because the land has been extended seaward. On an emerging land area
therefore the normal growth of a valley involves its lengthening at its lower end as
well as at its upper. The lengthening of a valley, or at least the lengthening of a
stream, also takes place at its lower end if the land in which it lies is being extended
seaward by deposition.
Structural valleys.—In mountain regions valleys are sometimes formed by the
uplift of parallel mountain folds, leaving a depression between (Fig. 58). Drainage
will appropriate such a valley so that it becomes in some sense a river valley. But it
is not a river valley in the sense in which the term has been used in the preceding
pages. It is rather a structural valley. In its bottom a river valley may be developed
(a, Fig. 58).
Page 113
Fig. 58.—Structural valley with a river valley developing its bottom.
The foregoing illustrations by no means exhaust the list of conditions under
which valleys develop, but they suffice for the present.
The courses of valleys.—River valleys
are rarely straight. To understand why they
are crooked it is only necessary to
understand the methods by which they
grow. In so far as a river valley is a gully
grown big, that is, in so far as its length is
the result of head erosion, its course was
determined by the course of the antecedent Fig. 59. Fig. 60.
gully. If in the case shown in Fig. 59 the Figures to show why the head of a gully (and
therefore a valley) departs from a direct
slope of the surface above the head of the course.
gully is uniform, its material homogeneous,
and the rainfall everywhere equal, more water will come into the gully from the
direction a than from any other. In this case there would be more wear in the direct
line of its extension than elsewhere, and the head would advance in a straight line.
But if there be inequalities of slope about the head of a gully at any stage of its
development more water may come in from some direction other than that in the
direct line of its extension. In Fig. 59, for example, more water may enter from the
direction of b than from that of a. Since most wear is likely to be affected along the
line of greatest inflow, the head of the gully will be turned in that direction (Fig.
60). Started in this course it will continue in the new direction so long as erosion in
this line is greater than that elsewhere; but whenever the configuration of the
surface causes more water to enter the head of the gully from some direction other
than that in which it is headed, the line of axial growth is again changed, as toward
c, Fig. 60. Since new land surfaces are probably more or less undulatory,
crookedness should be the rule among valleys developed from gullies by head
erosion. Streams and valleys the courses of which are determined by the original
slope of the land are said to be consequent.
Inequalities of material, leading to unequal rates of erosion, effect the same
result, in the absence of inequalities of slope. If at any stage of a valley’s
The foregoing illustrations by no means exhaust the list of conditions under
which valleys develop, but they suffice for the present.
The courses of valleys.—River valleys
are rarely straight. To understand why they
are crooked it is only necessary to
understand the methods by which they
grow. In so far as a river valley is a gully
grown big, that is, in so far as its length is
the result of head erosion, its course was
determined by the course of the antecedent Fig. 59. Fig. 60.
gully. If in the case shown in Fig. 59 the Figures to show why the head of a gully (and
therefore a valley) departs from a direct
slope of the surface above the head of the course.
gully is uniform, its material homogeneous,
and the rainfall everywhere equal, more water will come into the gully from the
direction a than from any other. In this case there would be more wear in the direct
line of its extension than elsewhere, and the head would advance in a straight line.
But if there be inequalities of slope about the head of a gully at any stage of its
development more water may come in from some direction other than that in the
direct line of its extension. In Fig. 59, for example, more water may enter from the
direction of b than from that of a. Since most wear is likely to be affected along the
line of greatest inflow, the head of the gully will be turned in that direction (Fig.
60). Started in this course it will continue in the new direction so long as erosion in
this line is greater than that elsewhere; but whenever the configuration of the
surface causes more water to enter the head of the gully from some direction other
than that in which it is headed, the line of axial growth is again changed, as toward
c, Fig. 60. Since new land surfaces are probably more or less undulatory,
crookedness should be the rule among valleys developed from gullies by head
erosion. Streams and valleys the courses of which are determined by the original
slope of the land are said to be consequent.
Inequalities of material, leading to unequal rates of erosion, effect the same
result, in the absence of inequalities of slope. If at any stage of a valley’s
Page 114
development erosion were equal in two
directions at its head, and at the same time
greater than at points between, two gullies
would result (Fig. 61) diverging from the
point in question.
In the case of a valley developed by
overflow from a lake its course is
determined by the lowest line of flow to
Fig. 61.—Diagram illustrating the
development of two equal gullies from the which the water has access. If this line be
head of one. straight the valley will be straight; if it is
crooked, as it generally is, the valley is crooked also.
The development of tributaries.—Thus far valleys leading immediately to the
sea have been considered, and no account taken of tributaries. As a matter of fact
most considerable valleys have numerous tributaries. It is now in order to inquire
into their mode of development.
So soon as a gully is started, the water flowing into it from either side wears back
the slopes. The least inequality of slope, or the least variation in the character of the
material, is sufficient to make the lateral erosion unequal at different points, and
unequal erosion in the slopes results in the development of tributary gullies. The
oldest tributaries may be nearly as old as the main which they join, and from which
they developed, for the possibilities of unequal side erosion exist as soon as a gully
is opened. While the main gully is developing into a ravine, and the ravine into a
valley, the tributary gullies are likewise developing into maturer stages. Tributary to
a young valley, therefore, there may be gullies near its head, ravines in its middle
course, and small valleys along its oldest portion. It is not to be understood,
however, that the oldest tributaries are necessarily the largest, for because of more
favorable conditions for growth the younger tributaries often outstrip the older.
The position of tributaries with reference to their mains is worthy of note. The
water flowing down a slope follows the line of steepest descent. A gully is usually
wider at its lower end, and narrower at its upper. Wherever this is true the line of
steepest descent down its side is not a line perpendicular to its axis, but a line
slightly oblique to it (ef, Fig. 62), and oblique in such a direction that it meets the
axis with an obtuse angle below and an acute angle above. It is in the direction
corresponding to this line that tributary gullies tend to develop. Thus at the
inception of its history a tributary gully is likely to join its main with an angle
slightly acute on the up-stream side. If the tributary did not begin until after its
main was farther advanced this tendency would be less and less pronounced.
Inequalities of material or slope would often counteract this tendency, which, at
directions at its head, and at the same time
greater than at points between, two gullies
would result (Fig. 61) diverging from the
point in question.
In the case of a valley developed by
overflow from a lake its course is
determined by the lowest line of flow to
Fig. 61.—Diagram illustrating the
development of two equal gullies from the which the water has access. If this line be
head of one. straight the valley will be straight; if it is
crooked, as it generally is, the valley is crooked also.
The development of tributaries.—Thus far valleys leading immediately to the
sea have been considered, and no account taken of tributaries. As a matter of fact
most considerable valleys have numerous tributaries. It is now in order to inquire
into their mode of development.
So soon as a gully is started, the water flowing into it from either side wears back
the slopes. The least inequality of slope, or the least variation in the character of the
material, is sufficient to make the lateral erosion unequal at different points, and
unequal erosion in the slopes results in the development of tributary gullies. The
oldest tributaries may be nearly as old as the main which they join, and from which
they developed, for the possibilities of unequal side erosion exist as soon as a gully
is opened. While the main gully is developing into a ravine, and the ravine into a
valley, the tributary gullies are likewise developing into maturer stages. Tributary to
a young valley, therefore, there may be gullies near its head, ravines in its middle
course, and small valleys along its oldest portion. It is not to be understood,
however, that the oldest tributaries are necessarily the largest, for because of more
favorable conditions for growth the younger tributaries often outstrip the older.
The position of tributaries with reference to their mains is worthy of note. The
water flowing down a slope follows the line of steepest descent. A gully is usually
wider at its lower end, and narrower at its upper. Wherever this is true the line of
steepest descent down its side is not a line perpendicular to its axis, but a line
slightly oblique to it (ef, Fig. 62), and oblique in such a direction that it meets the
axis with an obtuse angle below and an acute angle above. It is in the direction
corresponding to this line that tributary gullies tend to develop. Thus at the
inception of its history a tributary gully is likely to join its main with an angle
slightly acute on the up-stream side. If the tributary did not begin until after its
main was farther advanced this tendency would be less and less pronounced.
Inequalities of material or slope would often counteract this tendency, which, at
Page 115
best, would cause the courses of tributaries to depart but
little from perpendicularity to their mains.
After the head of a tributary has worked back from the
immediate slope of its main every condition which
determines the course of a gully is likely to affect it, and
it is by no means certain that it will continue to lengthen
in the direction in which it started. Since the general
slope of the surface into which the tributary works is
likely to be seaward, more water is likely to enter from
the landward than from the seaward side of its head, so
that, except where there are notable irregularities of
slope, its tendency will be to turn more and more toward Fig. 62.—Diagram to
the direction of its main (efg, Fig. 62). illustrate the oblique
position of a tributary
In depth the tributary is always limited by its main. gully at its inception, and
its later normal change of
The principles which determine the length and width of a direction.
main valley determine also the length and width of a
tributary (see p. 67 et seq.).
A CYCLE OF EROSION. ITS STAGES.
From what has preceded it is clear that the topography of a region undergoing
erosion will change greatly from time to time. The first effect of erosion is to
roughen the surface by cutting out valleys, leaving ridges and hills. The final effect
is to make it smooth again by cutting the ridges and hills down to the level of the
valleys.
Fig. 63.—Diagram showing three parallel valleys in a land surface.
little from perpendicularity to their mains.
After the head of a tributary has worked back from the
immediate slope of its main every condition which
determines the course of a gully is likely to affect it, and
it is by no means certain that it will continue to lengthen
in the direction in which it started. Since the general
slope of the surface into which the tributary works is
likely to be seaward, more water is likely to enter from
the landward than from the seaward side of its head, so
that, except where there are notable irregularities of
slope, its tendency will be to turn more and more toward Fig. 62.—Diagram to
the direction of its main (efg, Fig. 62). illustrate the oblique
position of a tributary
In depth the tributary is always limited by its main. gully at its inception, and
its later normal change of
The principles which determine the length and width of a direction.
main valley determine also the length and width of a
tributary (see p. 67 et seq.).
A CYCLE OF EROSION. ITS STAGES.
From what has preceded it is clear that the topography of a region undergoing
erosion will change greatly from time to time. The first effect of erosion is to
roughen the surface by cutting out valleys, leaving ridges and hills. The final effect
is to make it smooth again by cutting the ridges and hills down to the level of the
valleys.
Fig. 63.—Diagram showing three parallel valleys in a land surface.
Page 116
Fig. 64.—Diagram to illustrate the lowering of the surface by valley erosion. The successive cross
profiles of the valleys are represented by the lines 1–1, 1–1′, 2–2, 2–2′, etc.
The base-level of erosion has already been defined; but the mode of its
development may now be illustrated in the light of the preceding discussion.
Suppose a land surface affected by a series of parallel young valleys without
tributaries (Fig. 63). Between them there is a series of upland plateaus. The profile
of the surface between two adjacent valleys is represented in section by the
uppermost line in Fig. 64. As the valleys are widened from 1–1 and 1,′–1′, to 2–2
and 2′–2′, the intervening plateau is correspondingly narrowed. When the valleys
have attained the form represented by 3–3 and 3′–3′, the intervening upland has
been narrowed to a ridge, a, and the valley flats have become wide. With continued
erosion the ridge will be lowered (to b and below), and in time the surface will
approach a plain. In this condition it is known as a peneplain (an “almost-plain”).
Finally, when running water has done its utmost, the ridges will be essentially
obliterated and a base-leveled plain (e, e′, e″) results. The figure expresses the fact
that the base-level develops laterally from the axis of the valley. It also develops
headward from the seaward end of the valley. Similarly, taking into account all the
valleys which affect it, the seaward margin of a base-leveled plain is developed
first, and thence it extends itself inland.
Fig. 65.—Diagram showing the dissection of the upland shown in Fig. 64 by tributary valleys.
Tributaries are tolerably sure to develop along each main valley. The heads of the
tributaries work back across the uplands between the main valleys, dissecting them
into secondary ridges (Fig. 65). Tributaries will develop on the tributaries, and
these tertiary valleys dissect the secondary ridges into those of a lower order. This
profiles of the valleys are represented by the lines 1–1, 1–1′, 2–2, 2–2′, etc.
The base-level of erosion has already been defined; but the mode of its
development may now be illustrated in the light of the preceding discussion.
Suppose a land surface affected by a series of parallel young valleys without
tributaries (Fig. 63). Between them there is a series of upland plateaus. The profile
of the surface between two adjacent valleys is represented in section by the
uppermost line in Fig. 64. As the valleys are widened from 1–1 and 1,′–1′, to 2–2
and 2′–2′, the intervening plateau is correspondingly narrowed. When the valleys
have attained the form represented by 3–3 and 3′–3′, the intervening upland has
been narrowed to a ridge, a, and the valley flats have become wide. With continued
erosion the ridge will be lowered (to b and below), and in time the surface will
approach a plain. In this condition it is known as a peneplain (an “almost-plain”).
Finally, when running water has done its utmost, the ridges will be essentially
obliterated and a base-leveled plain (e, e′, e″) results. The figure expresses the fact
that the base-level develops laterally from the axis of the valley. It also develops
headward from the seaward end of the valley. Similarly, taking into account all the
valleys which affect it, the seaward margin of a base-leveled plain is developed
first, and thence it extends itself inland.
Fig. 65.—Diagram showing the dissection of the upland shown in Fig. 64 by tributary valleys.
Tributaries are tolerably sure to develop along each main valley. The heads of the
tributaries work back across the uplands between the main valleys, dissecting them
into secondary ridges (Fig. 65). Tributaries will develop on the tributaries, and
these tertiary valleys dissect the secondary ridges into those of a lower order. This
Page 117
process of tributary development goes on until drainage lines of the fourth, fifth,
sixth, and higher orders are formed (Fig. 66). Since the process of valley
development under such circumstances is also the process of ridge dissection, a
stage is presently reached where the ridges are cut into such short sections that they
cease to be ridges, and become hills instead. Even then the processes of erosion do
not stop, for the rain-water falling on the hills washes the loose material from their
surfaces, and starts it on its seaward journey. Thus the “everlasting hills”
themselves are lowered, and, given time enough, will be carried to the sea. Under
these conditions, as under those already discussed, the final result of stream erosion
is the reduction of the land to base-level. The base-leveled surface, as before, would
not be absolutely flat. The area reduced by each stream will have a slight gradient
down-stream, and from each lateral divide toward the axis of the valley. The crests
of the scarcely perceptible elevations which remain will be in the position of the
former divides, and these will be highest where most distant from the sea by the
course which this part of the drainage took. Even the insensible divides between
streams flowing in a common direction may disappear, for when valleys have
reached their limits in depth, their streams do not cease to cut laterally. Meandering
in their flat-bottomed valleys, they often reach and undercut the divides (Pl. VII),
whether they be high or low. By lateral planation, therefore, the divides between
streams may be entirely eaten away.
Fig. 66.—Diagram showing tributaries of several orders developed from the conditions sketched in
the text.
It has now been seen that by whatever method erosion by running water
proceeds, whether there be many valleys, or few or none, the final result of
subaërial erosion must be the production of a base-level. It has also been seen that
the base-level is first developed at the lower ends of the main streams, and that it
extends itself systematically up the main valleys and up all tributaries. The time
involved in the reduction of a land area to base-level is a cycle of erosion.
sixth, and higher orders are formed (Fig. 66). Since the process of valley
development under such circumstances is also the process of ridge dissection, a
stage is presently reached where the ridges are cut into such short sections that they
cease to be ridges, and become hills instead. Even then the processes of erosion do
not stop, for the rain-water falling on the hills washes the loose material from their
surfaces, and starts it on its seaward journey. Thus the “everlasting hills”
themselves are lowered, and, given time enough, will be carried to the sea. Under
these conditions, as under those already discussed, the final result of stream erosion
is the reduction of the land to base-level. The base-leveled surface, as before, would
not be absolutely flat. The area reduced by each stream will have a slight gradient
down-stream, and from each lateral divide toward the axis of the valley. The crests
of the scarcely perceptible elevations which remain will be in the position of the
former divides, and these will be highest where most distant from the sea by the
course which this part of the drainage took. Even the insensible divides between
streams flowing in a common direction may disappear, for when valleys have
reached their limits in depth, their streams do not cease to cut laterally. Meandering
in their flat-bottomed valleys, they often reach and undercut the divides (Pl. VII),
whether they be high or low. By lateral planation, therefore, the divides between
streams may be entirely eaten away.
Fig. 66.—Diagram showing tributaries of several orders developed from the conditions sketched in
the text.
It has now been seen that by whatever method erosion by running water
proceeds, whether there be many valleys, or few or none, the final result of
subaërial erosion must be the production of a base-level. It has also been seen that
the base-level is first developed at the lower ends of the main streams, and that it
extends itself systematically up the main valleys and up all tributaries. The time
involved in the reduction of a land area to base-level is a cycle of erosion.
Page 118
It will have been evident from the preceding pages that the terms “grade,”
“graded plain,” and “base-level” and “base-leveled plain,” are somewhat variously,
and therefore somewhat confusingly, used. “Grade is a condition of essential
balance between corrasion and deposition.”[29] A graded valley is one in which
deposition and corrasion are, in the vertical sense, balanced. Its angle of slope is
most variable, and is dependent on the capacity of the stream for work, and on the
work it has to do. A weak river must have a higher gradient than a strong one; a
stream with much sediment must have a higher gradient than one with little, and a
stream with a load of coarse material must have a higher gradient than one with a
load of fine. Thus the graded valley of the lower Mississippi has an inappreciable
angle of slope, but the graded valleys of many of its tributaries have slopes of
hundreds of feet per mile. Since both the size of the stream and the amount and
coarseness of its load at a given place vary from time to time, it is clear that the
inclination of a graded valley must vary also, and further, that it must be in process
of continual readjustment. With the changing conditions of advancing years the
slope of a graded valley normally decreases. The same principles apply to graded
surfaces outside of valleys.
In the continual readjustment of grades incident to a river’s normal history the
land is brought nearer and nearer to sea-level without ceasing to be at grade. When
the inclination of a graded surface becomes so low that it is sensibly flat, the
surface may be said to be at base-level, although this does not mean that the surface
can never be degraded further. If the term be used in this way, it is clear that there is
no sharp line of distinction between a graded surface and a base-leveled surface,
and as the terms are now commonly applied no such distinction exists.
If the term base-level were made synonymous with sea-level, as has been
proposed,[30] the term might as well be discarded, for sea-level could always be
used in its stead. Furthermore, streams often erode below sea-level. The bottom of
the channel of the Mississippi is below sea-level for some 400 miles above its
debouchure, and locally (Fort Jackson) it is nearly 250 feet below. This deep
channel is the result of the erosive activity of the stream, not of subsidence. Again,
the sea-level is itself inconstant. The extent of its changes cannot now be measured,
but they have probably been more considerable in the course of geological history
than has been commonly recognized. It is true that they take place slowly, as far as
known, but it is also true that the duration of an erosion cycle is sufficiently long
for even very slow changes to reach great magnitude. The sea-level, therefore, can
hardly be accepted as the absolute base-level, unless (1) the absolute base-level is a
variable, and unless (2) the absolute base-level be a surface below which rivers
may cut to the extent of at least 250 feet.
“graded plain,” and “base-level” and “base-leveled plain,” are somewhat variously,
and therefore somewhat confusingly, used. “Grade is a condition of essential
balance between corrasion and deposition.”[29] A graded valley is one in which
deposition and corrasion are, in the vertical sense, balanced. Its angle of slope is
most variable, and is dependent on the capacity of the stream for work, and on the
work it has to do. A weak river must have a higher gradient than a strong one; a
stream with much sediment must have a higher gradient than one with little, and a
stream with a load of coarse material must have a higher gradient than one with a
load of fine. Thus the graded valley of the lower Mississippi has an inappreciable
angle of slope, but the graded valleys of many of its tributaries have slopes of
hundreds of feet per mile. Since both the size of the stream and the amount and
coarseness of its load at a given place vary from time to time, it is clear that the
inclination of a graded valley must vary also, and further, that it must be in process
of continual readjustment. With the changing conditions of advancing years the
slope of a graded valley normally decreases. The same principles apply to graded
surfaces outside of valleys.
In the continual readjustment of grades incident to a river’s normal history the
land is brought nearer and nearer to sea-level without ceasing to be at grade. When
the inclination of a graded surface becomes so low that it is sensibly flat, the
surface may be said to be at base-level, although this does not mean that the surface
can never be degraded further. If the term be used in this way, it is clear that there is
no sharp line of distinction between a graded surface and a base-leveled surface,
and as the terms are now commonly applied no such distinction exists.
If the term base-level were made synonymous with sea-level, as has been
proposed,[30] the term might as well be discarded, for sea-level could always be
used in its stead. Furthermore, streams often erode below sea-level. The bottom of
the channel of the Mississippi is below sea-level for some 400 miles above its
debouchure, and locally (Fort Jackson) it is nearly 250 feet below. This deep
channel is the result of the erosive activity of the stream, not of subsidence. Again,
the sea-level is itself inconstant. The extent of its changes cannot now be measured,
but they have probably been more considerable in the course of geological history
than has been commonly recognized. It is true that they take place slowly, as far as
known, but it is also true that the duration of an erosion cycle is sufficiently long
for even very slow changes to reach great magnitude. The sea-level, therefore, can
hardly be accepted as the absolute base-level, unless (1) the absolute base-level is a
variable, and unless (2) the absolute base-level be a surface below which rivers
may cut to the extent of at least 250 feet.
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The ocean may be looked upon as a barrier which in a general way limits the
down-cutting of running water; for only very large streams cut much below its
level. Other barriers, such as lakes, and the outcrops of hard rock in a stream’s bed,
have a comparable, though more temporary, effect on the development of valley
plains above. Plains thus developed have been called temporary base-levels. They
differ from other graded plains in being controlled primarily by a barrier below,
rather than by conditions which exist above.
Since river valleys have a beginning and pass through various stages of
development before the country they drain is base-leveled, it is important to
recognize their various stages of advancement. Nor is this difficult. An old valley
and a young one have different characteristics, and the one would no more be
mistaken for the other by those who have learned to interpret them, than the face of
an aged man would be mistaken for that of a child.
Fig. 67.—A gully developed by a single shower. (Blackwelder.)
The cycle begins with the beginning of valley development, and at that stage
drainage is in its infancy. The type of the infant valley is the gully or ravine (Figs.
67 and 68). It has steep slopes and a narrow bottom. Fig. 1 of Plate IV represents
similar, or rather older, ravines in contour (shore of Lake Michigan, just north of
Chicago). With age, the valley widens, lengthens, and deepens, and passes from
infancy to youth. In this stage also the valleys are relatively narrow, and the divides
between them broad. They may be deep or shallow, according to the height of the
land in which they are cut, and the fall of the water flowing through them; but in
any case the streams flowing through them have done but a small part of the work
down-cutting of running water; for only very large streams cut much below its
level. Other barriers, such as lakes, and the outcrops of hard rock in a stream’s bed,
have a comparable, though more temporary, effect on the development of valley
plains above. Plains thus developed have been called temporary base-levels. They
differ from other graded plains in being controlled primarily by a barrier below,
rather than by conditions which exist above.
Since river valleys have a beginning and pass through various stages of
development before the country they drain is base-leveled, it is important to
recognize their various stages of advancement. Nor is this difficult. An old valley
and a young one have different characteristics, and the one would no more be
mistaken for the other by those who have learned to interpret them, than the face of
an aged man would be mistaken for that of a child.
Fig. 67.—A gully developed by a single shower. (Blackwelder.)
The cycle begins with the beginning of valley development, and at that stage
drainage is in its infancy. The type of the infant valley is the gully or ravine (Figs.
67 and 68). It has steep slopes and a narrow bottom. Fig. 1 of Plate IV represents
similar, or rather older, ravines in contour (shore of Lake Michigan, just north of
Chicago). With age, the valley widens, lengthens, and deepens, and passes from
infancy to youth. In this stage also the valleys are relatively narrow, and the divides
between them broad. They may be deep or shallow, according to the height of the
land in which they are cut, and the fall of the water flowing through them; but in
any case the streams flowing through them have done but a small part of the work
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they are to do before the country they drain is base-leveled. Figs. 69 and 70,
respectively, represent youthful valleys in regions of moderate and great relief. Fig.
2, Plate IV, shows a youthful valley in a region of slight relief (near Casselton, N.
D., Lat. 46° 40′, Long. 97° 25′). The uppermost line in Fig. 64 likewise represents
topographic youth, as shown in cross-profile.
Fig. 68.—A gully somewhat older than that shown in Fig. 67. (Alden.)
respectively, represent youthful valleys in regions of moderate and great relief. Fig.
2, Plate IV, shows a youthful valley in a region of slight relief (near Casselton, N.
D., Lat. 46° 40′, Long. 97° 25′). The uppermost line in Fig. 64 likewise represents
topographic youth, as shown in cross-profile.
Fig. 68.—A gully somewhat older than that shown in Fig. 67. (Alden.)
Page 121
Fig. 69.—A young valley in a region of slight relief.
Not only are narrow valleys said to be young, but the territory affected by them
is said to be in its topographic youth, since but a small part of the time necessary to
reduce it to base-level has elapsed. An area is in its topographic youth when
considerable portions of it are still unaffected by valleys. Thus the areas (as a
whole), as well as the valleys, represented on Plate IV, are in their topographic
youth. It is often convenient to recognize various sub-stages, such as early, middle,
and late, within the youthful stage of valleys or topographies. The different parts of
the areas shown on Plate IV, for example, represent different stages of youth.
Youthful streams, as well as youthful topographies, have their distinctive
characteristics. They are usually swift; their cutting is mainly at the bottom rather
than at the sides, and their courses are often marked by rapids and falls.
As valleys approach base-level they develop flats. As the valleys and their flats
widen, and as their tributaries increase in numbers and size, a stage of erosion is
presently reached where but little of the original upland surface remains. The
country is largely reduced to slopes. In this condition the drainage and the
topography which it has determined are said to be mature. Mature topography is
shown in contours in the figures of Plate V, and in the northern part of Plate VI,
where slopes, rather than upland or valley flats, predominate. Fig. 1 of Plate V
represents an area in southeastern Kentucky (Lat. 37° 12′, Long. 83° 10′); Fig. 2, an
area in western Virginia. Plate VI represents an area in southern California,
somewhat west of San Bernardino. The three areas are alike in representing mature
drainage, though not of equal stages of advancement. The striking differences of
Not only are narrow valleys said to be young, but the territory affected by them
is said to be in its topographic youth, since but a small part of the time necessary to
reduce it to base-level has elapsed. An area is in its topographic youth when
considerable portions of it are still unaffected by valleys. Thus the areas (as a
whole), as well as the valleys, represented on Plate IV, are in their topographic
youth. It is often convenient to recognize various sub-stages, such as early, middle,
and late, within the youthful stage of valleys or topographies. The different parts of
the areas shown on Plate IV, for example, represent different stages of youth.
Youthful streams, as well as youthful topographies, have their distinctive
characteristics. They are usually swift; their cutting is mainly at the bottom rather
than at the sides, and their courses are often marked by rapids and falls.
As valleys approach base-level they develop flats. As the valleys and their flats
widen, and as their tributaries increase in numbers and size, a stage of erosion is
presently reached where but little of the original upland surface remains. The
country is largely reduced to slopes. In this condition the drainage and the
topography which it has determined are said to be mature. Mature topography is
shown in contours in the figures of Plate V, and in the northern part of Plate VI,
where slopes, rather than upland or valley flats, predominate. Fig. 1 of Plate V
represents an area in southeastern Kentucky (Lat. 37° 12′, Long. 83° 10′); Fig. 2, an
area in western Virginia. Plate VI represents an area in southern California,
somewhat west of San Bernardino. The three areas are alike in representing mature
drainage, though not of equal stages of advancement. The striking differences of
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topography of the three areas are the result of differences in rock structure and
altitude, and will be considered later. Mature topography is also shown in Fig. 71,
where the relief is moderate, and in Figs. 72 and 73, where it is great. Figs. 72 and
73 illustrate clearly the universal tendency of rivers in regions of notable relief to
develop new flats well below the old surface of the region. At the same time that
these low-lying flats are developing, tributary drainage is dissecting and
roughening the upper surfaces. This process is well shown in Fig. 73. In both Figs.
72 and 73 the summits of the mountains on either side of the valleys appear to have
had about the same elevation. The new flat is therefore developed at the expense of
the old flat. As will be seen in the sequel, the first flat which a stream develops
along its course is usually somewhat above base-level. It is a graded flat.
PLATE V.
U. S. Geol. Surv. Fig. 1. KENTUCKY. Scale, 2+ mile per inch.
altitude, and will be considered later. Mature topography is also shown in Fig. 71,
where the relief is moderate, and in Figs. 72 and 73, where it is great. Figs. 72 and
73 illustrate clearly the universal tendency of rivers in regions of notable relief to
develop new flats well below the old surface of the region. At the same time that
these low-lying flats are developing, tributary drainage is dissecting and
roughening the upper surfaces. This process is well shown in Fig. 73. In both Figs.
72 and 73 the summits of the mountains on either side of the valleys appear to have
had about the same elevation. The new flat is therefore developed at the expense of
the old flat. As will be seen in the sequel, the first flat which a stream develops
along its course is usually somewhat above base-level. It is a graded flat.
PLATE V.
U. S. Geol. Surv. Fig. 1. KENTUCKY. Scale, 2+ mile per inch.
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U. S. Geol. Surv. Fig. 2. VIRGINIA. Scale, 2+ mile per inch.
Page 124
PLATE VI.
U. S. Geol. Surv. Scale, 1+ mile per inch.
PARTS OF LOS ANGELES AND SAN BERNARDINO
COUNTIES, CALIFORNIA.
U. S. Geol. Surv. Scale, 1+ mile per inch.
PARTS OF LOS ANGELES AND SAN BERNARDINO
COUNTIES, CALIFORNIA.
Page 125
Fig. 70.—The valley (canyon) of the Yellowstone. A young valley in an elevated region.
Page 126
Fig. 71.—Mature erosion topography in a region of slight relief, Iowa. (Calvin.)
Fig. 72.—Mature erosion in a mountain region. From mouth of Gray Copper Gulch, Silverton,
Colo., quadrangle. (Cross, U. S. Geol. Surv.)
The same processes which have made young valleys mature will in time work
further changes. When the gradients of the valleys have become low and their
bottoms wide, and when the intervening ridges and hills have become narrow and
small, the drainage and the drainage topography have reached old age, and the
streams are in a condition of senility. This is illustrated by Fig. 1, Plate VII (central
Kansas), and in section by the third and lower lines in Fig. 64. Topographic old age
sometimes has a different expression; this is shown in Fig. 74, where most of the
surface has been brought low. The elevations which rise above the general plain are
small in area, but have abrupt slopes. This phase of old-age topography is usually
the result of the unequal resistance of the rock degraded. The effects of unequal
rock-resistance will be considered later.
Fig. 72.—Mature erosion in a mountain region. From mouth of Gray Copper Gulch, Silverton,
Colo., quadrangle. (Cross, U. S. Geol. Surv.)
The same processes which have made young valleys mature will in time work
further changes. When the gradients of the valleys have become low and their
bottoms wide, and when the intervening ridges and hills have become narrow and
small, the drainage and the drainage topography have reached old age, and the
streams are in a condition of senility. This is illustrated by Fig. 1, Plate VII (central
Kansas), and in section by the third and lower lines in Fig. 64. Topographic old age
sometimes has a different expression; this is shown in Fig. 74, where most of the
surface has been brought low. The elevations which rise above the general plain are
small in area, but have abrupt slopes. This phase of old-age topography is usually
the result of the unequal resistance of the rock degraded. The effects of unequal
rock-resistance will be considered later.
Page 127
Fig. 73.—Mature erosion in a mountain region. Silverton, Colo. (Cross, U. S. Geol. Surv.)
The marks of old streams are as characteristic as those of young ones. They have
low gradients and are sluggish. Instead of lowering their channels steadily they cut
them down in flood, and fill them up when their currents are not swollen. They
meander widely in their flat-bottomed valleys (Fig. 1, Pl. VII, Central Kansas) and
their erosion, except in time of flood, is largely lateral.
If the processes of degradation were to continue until the land surface was
brought to sea-level, and this might be done by solution though not by mechanical
erosion of running water, the rivers would no longer flow, and the drainage system
would have reached the end of its history—death.
Not only do valleys normally pass from birth to youth, from youth to maturity,
and from maturity to old age, but a single river system may show these various
stages of development in its various parts. Thus in the area shown in Fig. 2, Plate
VII (north central Kansas), there is a tract (extreme southwest) where the erosion
history is scarcely begun. The zone of land a little farther northeast, and just
reached by the heads of the valleys (same figure), is in its youth. The well-drained
and uneven tract southwest of the flat of the Solomon River is in maturity, while
the flat of the main valley has the general characteristics of old age.
The marks of old streams are as characteristic as those of young ones. They have
low gradients and are sluggish. Instead of lowering their channels steadily they cut
them down in flood, and fill them up when their currents are not swollen. They
meander widely in their flat-bottomed valleys (Fig. 1, Pl. VII, Central Kansas) and
their erosion, except in time of flood, is largely lateral.
If the processes of degradation were to continue until the land surface was
brought to sea-level, and this might be done by solution though not by mechanical
erosion of running water, the rivers would no longer flow, and the drainage system
would have reached the end of its history—death.
Not only do valleys normally pass from birth to youth, from youth to maturity,
and from maturity to old age, but a single river system may show these various
stages of development in its various parts. Thus in the area shown in Fig. 2, Plate
VII (north central Kansas), there is a tract (extreme southwest) where the erosion
history is scarcely begun. The zone of land a little farther northeast, and just
reached by the heads of the valleys (same figure), is in its youth. The well-drained
and uneven tract southwest of the flat of the Solomon River is in maturity, while
the flat of the main valley has the general characteristics of old age.
Page 128
Fig. 74.—A peneplained surface where the elevations are small but steep-sided. Near Camp Douglas,
Wis. (Atwood.)
The age of valleys in terms of erosion is also expressed more or less perfectly by
their cross-sections. The line 1–1 (and 1′–1′) of Fig. 64 represents in cross-section a
narrow V-shaped valley. Such a section is always indicative of youth. The stream
which developed it cut chiefly at its bottom, not at its sides. It was therefore rapid,
and rapid streams are young. The line 2–2, (2′–2′) (Fig. 64) shows the same valley
at a later and maturer stage when downward cutting has nearly ceased. The
widening of the valley by slope wash has become relatively more important than
before, and the stream has so far lost velocity as the result of diminished gradient as
to be unable to carry away all the detritus washed down from the sides. As a result
of deposition at the bases of the side slopes, a concave curve has been developed.
Up the valley from the point where such a section as is represented by 2–2 occurs,
the valley may still have a section similar to that represented by 1–1.
Wis. (Atwood.)
The age of valleys in terms of erosion is also expressed more or less perfectly by
their cross-sections. The line 1–1 (and 1′–1′) of Fig. 64 represents in cross-section a
narrow V-shaped valley. Such a section is always indicative of youth. The stream
which developed it cut chiefly at its bottom, not at its sides. It was therefore rapid,
and rapid streams are young. The line 2–2, (2′–2′) (Fig. 64) shows the same valley
at a later and maturer stage when downward cutting has nearly ceased. The
widening of the valley by slope wash has become relatively more important than
before, and the stream has so far lost velocity as the result of diminished gradient as
to be unable to carry away all the detritus washed down from the sides. As a result
of deposition at the bases of the side slopes, a concave curve has been developed.
Up the valley from the point where such a section as is represented by 2–2 occurs,
the valley may still have a section similar to that represented by 1–1.
Page 129
PLATE VII.
U. S. Geol. Surv. Fig. 1. KANSAS. Scale, 2+ mile per inch.
U. S. Geol. Surv. Fig. 1. KANSAS. Scale, 2+ mile per inch.
Page 130
U. S. Geol. Surv. Fig. 2. KANSAS. Scale, 2+ mile per inch.
Page 131
PLATE VIII.
U. S. Geol. Surv. ABOUT 15 MILES SOUTHWEST OF ST. Scale, 1+ mile per inch.
LOUIS, MISSOURI.
Still later stages of development are represented by the cross-sections 3–3 and 4–
4. Not only has the valley become larger, but the stream has deposited detritus (not
shown in the figure) in the bottom of its valley, developing an alluvial flat. On this
flat the stream meanders, and the valley may be widened by the undercutting of the
bluffs wherever the stream in its wanderings reaches them (Pl. VIII, near St. Louis).
A valley might possess the characteristics shown by the cross-sections 3–3, 2–2,
and 1–1, Fig. 64, in its lower, middle, and upper courses, respectively.
U. S. Geol. Surv. ABOUT 15 MILES SOUTHWEST OF ST. Scale, 1+ mile per inch.
LOUIS, MISSOURI.
Still later stages of development are represented by the cross-sections 3–3 and 4–
4. Not only has the valley become larger, but the stream has deposited detritus (not
shown in the figure) in the bottom of its valley, developing an alluvial flat. On this
flat the stream meanders, and the valley may be widened by the undercutting of the
bluffs wherever the stream in its wanderings reaches them (Pl. VIII, near St. Louis).
A valley might possess the characteristics shown by the cross-sections 3–3, 2–2,
and 1–1, Fig. 64, in its lower, middle, and upper courses, respectively.
Page 132
The preceding discussion, and the illustrations which accompany it, give some
idea of the topography which characterizes an area in various stages of its erosion
history. Whether the valleys are deep or shallow, and the intervening ridges high or
low, depends on the original height of the land and its distance from the sea. The
higher the land, and the nearer it is to the sea, the greater the relief developed by
erosion. A plateau near the sea may become mountainous in the mature stage of its
erosion history, while a plain in the same situation would only become hilly. A
plateau in the heart of a continent would have less relief in its maturity than one of
equal elevation near the sea, since the grade-plain in the former position is higher
than in the latter. Plates IV and IX show youthful topography where the relief is
relatively slight, and Plate X shows youthful topography where the relief is great.
Similarly, Plates V and VI show mature topography where the relief is great, and
Fig. 1, Plate III, shows mature topography where the relief is relatively slight.
Topographic youth, topographic maturity, and topographic old age are also
indicated in other ways, and especially by the presence of features which rivers
tend to destroy. If, for example, the surface of the land, well above the valley
bottoms, is marked by numerous ponds and marshes, it is clear that drainage has
not yet progressed beyond its early stages, for, unless the lakes be very deep,
valleys working back into the land will find and drain them before topographic
maturity has been reached. Their presence is evidence that the region where they
occur has not yet been thoroughly dissected by erosion lines, and therefore has not
reached maturity. Still other marks of topographic youth, such as rapids, falls, etc.,
as well as marks of topographic maturity and old age, will be mentioned in the
following pages.
GENERAL CHARACTERISTICS OF TOPOGRAPHIES
DEVELOPED BY RIVER EROSION.
With the characteristics of river valleys and the methods by which they grow
clearly in mind it is easy to say whether rivers have been the chief agents in the
development of a given topography. River valleys are distinguished from other
depressions on land surfaces by their linear form and, leaving out of consideration
the relatively insignificant inequalities in a stream’s channel, by the fact that any
point in the bottom of a river valley is lower than any other point farther up the
stream in the same valley, and higher than any point farther down the stream. The
second point might be otherwise stated by saying that every valley excavated by
erosion leads to a lower valley, or to the sea, or an inland basin. Streams which dry
up, or otherwise disappear as they flow, constitute partial exceptions. If, therefore,
the depressions on a land surface are linear, lead to other and deeper valleys, and
idea of the topography which characterizes an area in various stages of its erosion
history. Whether the valleys are deep or shallow, and the intervening ridges high or
low, depends on the original height of the land and its distance from the sea. The
higher the land, and the nearer it is to the sea, the greater the relief developed by
erosion. A plateau near the sea may become mountainous in the mature stage of its
erosion history, while a plain in the same situation would only become hilly. A
plateau in the heart of a continent would have less relief in its maturity than one of
equal elevation near the sea, since the grade-plain in the former position is higher
than in the latter. Plates IV and IX show youthful topography where the relief is
relatively slight, and Plate X shows youthful topography where the relief is great.
Similarly, Plates V and VI show mature topography where the relief is great, and
Fig. 1, Plate III, shows mature topography where the relief is relatively slight.
Topographic youth, topographic maturity, and topographic old age are also
indicated in other ways, and especially by the presence of features which rivers
tend to destroy. If, for example, the surface of the land, well above the valley
bottoms, is marked by numerous ponds and marshes, it is clear that drainage has
not yet progressed beyond its early stages, for, unless the lakes be very deep,
valleys working back into the land will find and drain them before topographic
maturity has been reached. Their presence is evidence that the region where they
occur has not yet been thoroughly dissected by erosion lines, and therefore has not
reached maturity. Still other marks of topographic youth, such as rapids, falls, etc.,
as well as marks of topographic maturity and old age, will be mentioned in the
following pages.
GENERAL CHARACTERISTICS OF TOPOGRAPHIES
DEVELOPED BY RIVER EROSION.
With the characteristics of river valleys and the methods by which they grow
clearly in mind it is easy to say whether rivers have been the chief agents in the
development of a given topography. River valleys are distinguished from other
depressions on land surfaces by their linear form and, leaving out of consideration
the relatively insignificant inequalities in a stream’s channel, by the fact that any
point in the bottom of a river valley is lower than any other point farther up the
stream in the same valley, and higher than any point farther down the stream. The
second point might be otherwise stated by saying that every valley excavated by
erosion leads to a lower valley, or to the sea, or an inland basin. Streams which dry
up, or otherwise disappear as they flow, constitute partial exceptions. If, therefore,
the depressions on a land surface are linear, lead to other and deeper valleys, and
Page 133
finally to an inland basin, or the sea, and if the elevations between these valleys are
such as might have been left by the excavation of the valleys, it is generally clear
that rain and rivers have been the chief factors in the development of the
topography. If, on the other hand, a surface is characterized by topographic features
which streams cannot develop, such as enclosed depressions, or hills and ridges
whose arrangement is independent of drainage lines, other agents besides rain and
surface streams have been concerned in its development.
SPECIAL FEATURES RESULTING FROM SPECIAL
CONDITIONS OF EROSION.
Many striking topographic and scenic features result from rain and river erosion.
Some of them depend primarily on the conditions of erosion, such as climate,
altitude, etc., while others depend largely on the structure and resistance of the
rock. Between these two classes there is no sharp line of demarkation. Illustrations
of two types, dependent largely but by no means wholly on conditions independent
of the rock, are cited at this point. Others will be mentioned in other connections.
such as might have been left by the excavation of the valleys, it is generally clear
that rain and rivers have been the chief factors in the development of the
topography. If, on the other hand, a surface is characterized by topographic features
which streams cannot develop, such as enclosed depressions, or hills and ridges
whose arrangement is independent of drainage lines, other agents besides rain and
surface streams have been concerned in its development.
SPECIAL FEATURES RESULTING FROM SPECIAL
CONDITIONS OF EROSION.
Many striking topographic and scenic features result from rain and river erosion.
Some of them depend primarily on the conditions of erosion, such as climate,
altitude, etc., while others depend largely on the structure and resistance of the
rock. Between these two classes there is no sharp line of demarkation. Illustrations
of two types, dependent largely but by no means wholly on conditions independent
of the rock, are cited at this point. Others will be mentioned in other connections.
Page 134
Fig. 75.—Bad-land topography. North of Scott’s Bluff, Neb. (Darton, U. S. Geol. Surv.)
Bad-land topography.—To a type of topography developed in early maturity in
certain high regions where the rock is but slightly, though unequally, resistant, a
special name is sometimes given. Such regions are termed bad lands. Some idea of
bad-land topography is gained from Figs. 75 to 78. Bad-land topography is found in
various localities in the West, but especially in western Nebraska and Wyoming,
and the western parts of the Dakotas. The formations here are often beds of
sandstone or shale, alternating with unindurated beds of clay. Climatic factors are
also concerned in the development of bad-land topography. A semi-arid climate,
where the precipitation is much concentrated, seems to be most favorable for its
development. The bad-land topography is most striking in early maturity.
Bad-land topography.—To a type of topography developed in early maturity in
certain high regions where the rock is but slightly, though unequally, resistant, a
special name is sometimes given. Such regions are termed bad lands. Some idea of
bad-land topography is gained from Figs. 75 to 78. Bad-land topography is found in
various localities in the West, but especially in western Nebraska and Wyoming,
and the western parts of the Dakotas. The formations here are often beds of
sandstone or shale, alternating with unindurated beds of clay. Climatic factors are
also concerned in the development of bad-land topography. A semi-arid climate,
where the precipitation is much concentrated, seems to be most favorable for its
development. The bad-land topography is most striking in early maturity.
Page 135
Fig. 76.—Toadstool Park, Sioux Co., Neb. The peculiar topography is the result of erosion working
on jointed rocks of unequal hardness in an arid region of considerable elevation where rainfall is
unequally distributed. (Darton, U. S. Geol. Surv.)
Special forms of valleys; canyons.—Various conditions influence the size and
shape of valleys, especially in the early stage of their development. If the altitude of
the land be great, the gradient of the streams at this stage will be high. A high
gradient means a swift stream, and a swift stream erodes chiefly at its bottom. High
altitudes therefore favor the development of deep valleys. Such valleys will be
narrow if the conditions which determine widening are absent or unfavorable.
Since slope wash is one of the main factors in the widening of valleys, an arid
climate favors the development of narrow valleys, if there be sufficient water to
maintain a vigorous stream. Narrowness and steepness of slopes will also be
favored if the valley is cut in rock which is capable of standing with steep faces.
Thus a stream may develop a narrow valley in indurated rock where it would not do
so in loose gravel, and, other things being equal, it will develop a narrower valley
in rock which is horizontally bedded than in rock the beds of which are inclined.
Aridity, high altitude, and the proper sort of rock structure therefore favor the
development of canyons, and many of the young valleys in the western part of the
United States where these conditions prevail, belong to this class.
on jointed rocks of unequal hardness in an arid region of considerable elevation where rainfall is
unequally distributed. (Darton, U. S. Geol. Surv.)
Special forms of valleys; canyons.—Various conditions influence the size and
shape of valleys, especially in the early stage of their development. If the altitude of
the land be great, the gradient of the streams at this stage will be high. A high
gradient means a swift stream, and a swift stream erodes chiefly at its bottom. High
altitudes therefore favor the development of deep valleys. Such valleys will be
narrow if the conditions which determine widening are absent or unfavorable.
Since slope wash is one of the main factors in the widening of valleys, an arid
climate favors the development of narrow valleys, if there be sufficient water to
maintain a vigorous stream. Narrowness and steepness of slopes will also be
favored if the valley is cut in rock which is capable of standing with steep faces.
Thus a stream may develop a narrow valley in indurated rock where it would not do
so in loose gravel, and, other things being equal, it will develop a narrower valley
in rock which is horizontally bedded than in rock the beds of which are inclined.
Aridity, high altitude, and the proper sort of rock structure therefore favor the
development of canyons, and many of the young valleys in the western part of the
United States where these conditions prevail, belong to this class.
Page 136
Fig. 77.—Detail of bad-land topography. Head of Indian Draw, Washington Co., S. D. Protoceras
sandstone on Oreodon clay. (Darton, U. S. Geol. Surv.)
sandstone on Oreodon clay. (Darton, U. S. Geol. Surv.)
Page 137
Fig. 78.—Detail of bad-land topography. Southwest foot of Mesa Verde, Colo. (Matthes, U. S. Geol.
Surv.)
Fig. 79.—Grand Canyon of the Colorado. (Peabody.)
Surv.)
Fig. 79.—Grand Canyon of the Colorado. (Peabody.)
Page 138
Fig. 80.—Grand Canyon of the Colorado. (Peabody.)
While all canyons are valleys, most valleys are not
canyons. The distinction between a canyon and a valley
which is not a canyon is not sharp. The canyon depends Fig. 81.—Diagram showing
the relations of depth and
for its distinctive character on the relation of depth, width of a valley, the
width, and angle of slope to one another; but any width of which is eight
definition of the depth, width, and angle of slope times the depth.
[31]
necessary to constitute a valley a canyon is arbitrary. In popular usage the rule
seems to be that if a valley is sufficiently deep, narrow, and steep-sided to be
distinctly striking, it is called a canyon in regions where that term is in use.
Whether a valley is deep, narrow, and steep-sided enough to be striking clearly
depends on the observer. The Colorado Canyon (Figs. 79 and 80) is the greatest
canyon known, but it is rarely more than a mile deep, and where its depth
approaches this figure it is often eight, ten, or even twelve miles wide from rim to
rim. Its width at bottom is little more than the width of the stream; that is, a few
hundred feet. Its cross-profile throughout much of its course is therefore not in
keeping with the conventional idea of a canyon. With a depth of one mile and a
width of eight, the slope, if uniform, would have an angle of less than 15°. Such a
valley is represented in Fig. 81. As a matter of fact the slopes of a canyon are not
commonly uniform. The slopes represented in Fig. 82 correspond more nearly than
those of Fig. 81, to the actual slopes of the Colorado Canyon. The inequalities of
slope are occasioned by the inequalities of hardness. It is perhaps needless to say
While all canyons are valleys, most valleys are not
canyons. The distinction between a canyon and a valley
which is not a canyon is not sharp. The canyon depends Fig. 81.—Diagram showing
the relations of depth and
for its distinctive character on the relation of depth, width of a valley, the
width, and angle of slope to one another; but any width of which is eight
definition of the depth, width, and angle of slope times the depth.
[31]
necessary to constitute a valley a canyon is arbitrary. In popular usage the rule
seems to be that if a valley is sufficiently deep, narrow, and steep-sided to be
distinctly striking, it is called a canyon in regions where that term is in use.
Whether a valley is deep, narrow, and steep-sided enough to be striking clearly
depends on the observer. The Colorado Canyon (Figs. 79 and 80) is the greatest
canyon known, but it is rarely more than a mile deep, and where its depth
approaches this figure it is often eight, ten, or even twelve miles wide from rim to
rim. Its width at bottom is little more than the width of the stream; that is, a few
hundred feet. Its cross-profile throughout much of its course is therefore not in
keeping with the conventional idea of a canyon. With a depth of one mile and a
width of eight, the slope, if uniform, would have an angle of less than 15°. Such a
valley is represented in Fig. 81. As a matter of fact the slopes of a canyon are not
commonly uniform. The slopes represented in Fig. 82 correspond more nearly than
those of Fig. 81, to the actual slopes of the Colorado Canyon. The inequalities of
slope are occasioned by the inequalities of hardness. It is perhaps needless to say
Page 139
that to an observer on the rim of the canyon the slopes seem several times as steep
as those shown in the diagrams.
Like all valleys which are narrow relative to their depth, the Colorado Canyon,
great as it is, is a young valley; for it represents but a small part of the work which
the stream must do to bring its drainage basin to base-level.
While aridity and altitude are conditions which favor the development of
canyons, as shown by the fact that most canyons are high and dry regions, they are
not indispensable. Niagara River has a canyon below its falls (Pl. IX), and the
surrounding region is neither high nor arid. The narrow part of the valley has been
developed by the recession of the falls, and is so young that side erosion has not yet
widened the valley or lowered its angle of slope to such an extent as to destroy its
canyon character. This canyon is often called a gorge, a term frequently applied to
small valleys of the canyon type.
Fig. 82.—Cross-section of the Colorado Canyon. (After Gilbert and Brigham.)
as those shown in the diagrams.
Like all valleys which are narrow relative to their depth, the Colorado Canyon,
great as it is, is a young valley; for it represents but a small part of the work which
the stream must do to bring its drainage basin to base-level.
While aridity and altitude are conditions which favor the development of
canyons, as shown by the fact that most canyons are high and dry regions, they are
not indispensable. Niagara River has a canyon below its falls (Pl. IX), and the
surrounding region is neither high nor arid. The narrow part of the valley has been
developed by the recession of the falls, and is so young that side erosion has not yet
widened the valley or lowered its angle of slope to such an extent as to destroy its
canyon character. This canyon is often called a gorge, a term frequently applied to
small valleys of the canyon type.
Fig. 82.—Cross-section of the Colorado Canyon. (After Gilbert and Brigham.)
Page 140
Fig. 83.—Detail of erosion in the Grand Canyon. The inequalities of slope are the result of unequal
hardness. The vertical planes which give the architectural effect are the result of joints. (Holmes.)
Plate X shows portions of the canyons of the Yellowstone and the Colorado
rivers respectively. In the first the contour interval is 100 feet, and in the second,
250 feet. The horizontal scale is ¹⁄₁₂₅₀₀₀ (about 2 miles to the inch) in the first, and
¹⁄₂₅₀₀₀₀ in the second. These scales should be borne in mind in interpreting the map.
Falls, rapids, narrows, and other peculiar features, due primarily to inequalities in
the hardness of the rock affected by erosion, will be considered later.
hardness. The vertical planes which give the architectural effect are the result of joints. (Holmes.)
Plate X shows portions of the canyons of the Yellowstone and the Colorado
rivers respectively. In the first the contour interval is 100 feet, and in the second,
250 feet. The horizontal scale is ¹⁄₁₂₅₀₀₀ (about 2 miles to the inch) in the first, and
¹⁄₂₅₀₀₀₀ in the second. These scales should be borne in mind in interpreting the map.
Falls, rapids, narrows, and other peculiar features, due primarily to inequalities in
the hardness of the rock affected by erosion, will be considered later.
Page 141
Fig. 84.—A surface illustrating the struggle for existence among gullies. Most of the smaller gullies
shown on the slope can have but little growth before being absorbed by their larger neighbors. A
type of erosion surface common in the Bad Lands. Scott’s Bluff, Neb. (Darton, U. S. Geol. Surv.)
THE STRUGGLE FOR EXISTENCE AMONG VALLEYS AND
STREAMS.
It is not to be inferred that every gully becomes a valley, nor that every small
valley becomes a large one. Among valleys, as among living things, there is a
struggle for existence, and fitness determines growth and survival. At an early stage
of its erosion history the number of small valleys in a given area is often great,
while at a later stage the number is less and the size of the survivors greater.
shown on the slope can have but little growth before being absorbed by their larger neighbors. A
type of erosion surface common in the Bad Lands. Scott’s Bluff, Neb. (Darton, U. S. Geol. Surv.)
THE STRUGGLE FOR EXISTENCE AMONG VALLEYS AND
STREAMS.
It is not to be inferred that every gully becomes a valley, nor that every small
valley becomes a large one. Among valleys, as among living things, there is a
struggle for existence, and fitness determines growth and survival. At an early stage
of its erosion history the number of small valleys in a given area is often great,
while at a later stage the number is less and the size of the survivors greater.
Page 142
PLATE IX.
U. S. Geol. Surv. NIAGARA FALLS. Scale, 1+ mile per inch.
U. S. Geol. Surv. NIAGARA FALLS. Scale, 1+ mile per inch.
Page 143
PLATE X.
U. S. Geol. Surv. Fig. 1. YELLOWSTONE PARK. Scale, 2+ mile per inch.
U. S. Geol. Surv. Fig. 1. YELLOWSTONE PARK. Scale, 2+ mile per inch.
Page 144
U. S. Geol. Surv. Fig. 2. ARIZONA. Scale, 2+ mile per inch.
One phase of the struggle for existence is often well
illustrated on a freshly exposed slope of clay. The
number of miniature gullies which develop on such a
Fig. 85.—Diagram slope, even in a single shower, may be very large (Fig.
illustrating the absorption
of one gully by another by
84); but the history of many of them is ephemeral. If two
lateral erosion. The adjacent ones are of unequal depth the widening of the
successive lines represent deeper narrows and finally eliminates the divide between
successive cross-sections.
them, and the two become one (Fig. 85).
Another phase of the struggle for existence is shown in other situations.
Examination of a good map of the north shore of Lake Superior or the west shore
of Lake Michigan shows a large number of small streams and gullies (Fig. 1, Pl.
IV). The valleys are short and narrow, and between and beyond them are
One phase of the struggle for existence is often well
illustrated on a freshly exposed slope of clay. The
number of miniature gullies which develop on such a
Fig. 85.—Diagram slope, even in a single shower, may be very large (Fig.
illustrating the absorption
of one gully by another by
84); but the history of many of them is ephemeral. If two
lateral erosion. The adjacent ones are of unequal depth the widening of the
successive lines represent deeper narrows and finally eliminates the divide between
successive cross-sections.
them, and the two become one (Fig. 85).
Another phase of the struggle for existence is shown in other situations.
Examination of a good map of the north shore of Lake Superior or the west shore
of Lake Michigan shows a large number of small streams and gullies (Fig. 1, Pl.
IV). The valleys are short and narrow, and between and beyond them are
Page 145
considerable areas untouched by erosion. The drainage near the lake is therefore
young, and each of the small valleys is growing. This condition of things is perhaps
typical of that which has been, is, or will be along the average coast at a certain
stage in its erosion history. No equal stretch of coast-line where erosion is far
advanced can boast of a number of large rivers comparable to that of the many
small ones along the coasts mentioned. It therefore seems evident that of these
many small streams a few only will attain considerable size.
Some of the methods by which the growth of the many is arrested are easily
understood. Some of the young valleys on a given coast will work their heads back
into the land faster than others because of inequalities of slope and material. This
will be true of the tributaries no less than of their mains. If valleys develop in ways
other than by head erosion (see p. 73) the chances are also against their equality of
growth. If two streams, such as a and c, Fig. 86, develop faster than the
intermediate stream b, it is clear that their tributaries may work back into the
territory which at the outset drained into b, so as to cut off the supply of water from
the latter stream (compare a′b′c′, Fig. 87). As a result, the growth of b will be
checked, and ultimately stopped. Similarly other valleys, such as f, will get the
better of their neighbors, and many of the competitors, as b, d, e, and g will soon
drop out of the race. Between the stronger streams competition still goes on. If a′
and f′ develop faster than c′ its prospective drainage territory will be preëmpted by
its rivals (compare Figs. 87 and 88). Thus as the result of the unequal rate at which
valleys are lengthened, the larger number of those which come into existence are
arrested in their development. As a result of growth in the manner indicated, the
basins of even the large streams remain narrow at their lower ends while they
expand above. This is the usual form of a drainage basin the development of which
has been normal.
young, and each of the small valleys is growing. This condition of things is perhaps
typical of that which has been, is, or will be along the average coast at a certain
stage in its erosion history. No equal stretch of coast-line where erosion is far
advanced can boast of a number of large rivers comparable to that of the many
small ones along the coasts mentioned. It therefore seems evident that of these
many small streams a few only will attain considerable size.
Some of the methods by which the growth of the many is arrested are easily
understood. Some of the young valleys on a given coast will work their heads back
into the land faster than others because of inequalities of slope and material. This
will be true of the tributaries no less than of their mains. If valleys develop in ways
other than by head erosion (see p. 73) the chances are also against their equality of
growth. If two streams, such as a and c, Fig. 86, develop faster than the
intermediate stream b, it is clear that their tributaries may work back into the
territory which at the outset drained into b, so as to cut off the supply of water from
the latter stream (compare a′b′c′, Fig. 87). As a result, the growth of b will be
checked, and ultimately stopped. Similarly other valleys, such as f, will get the
better of their neighbors, and many of the competitors, as b, d, e, and g will soon
drop out of the race. Between the stronger streams competition still goes on. If a′
and f′ develop faster than c′ its prospective drainage territory will be preëmpted by
its rivals (compare Figs. 87 and 88). Thus as the result of the unequal rate at which
valleys are lengthened, the larger number of those which come into existence are
arrested in their development. As a result of growth in the manner indicated, the
basins of even the large streams remain narrow at their lower ends while they
expand above. This is the usual form of a drainage basin the development of which
has been normal.
Page 146
Fig. 86–88.—Diagrams to illustrate successive stages in the struggle for existence and dominion
among streams.
Did valleys grow in length only, competition would not destroy the small ones; it
would simply limit them. But valleys widen as well as lengthen, and by widening,
adjacent valleys may eliminate the divide between them and become one. The
elimination of the intervening ridge may be by lateral planation (p. 82), or, if the
valleys be of unequal depth, by slope wash (see Fig. 85). By these and other
processes many young valleys are dwarfed, and many others are destroyed.
Piracy.—Streams do not always hold the courses which they establish for
themselves at the outset. If the valley occupied by the stream a, Fig. 89, is
deepened more rapidly than the valley occupied by b, a tributary from the former,
among streams.
Did valleys grow in length only, competition would not destroy the small ones; it
would simply limit them. But valleys widen as well as lengthen, and by widening,
adjacent valleys may eliminate the divide between them and become one. The
elimination of the intervening ridge may be by lateral planation (p. 82), or, if the
valleys be of unequal depth, by slope wash (see Fig. 85). By these and other
processes many young valleys are dwarfed, and many others are destroyed.
Piracy.—Streams do not always hold the courses which they establish for
themselves at the outset. If the valley occupied by the stream a, Fig. 89, is
deepened more rapidly than the valley occupied by b, a tributary from the former,
Page 147
c, may work back across the inter-stream area to e and steal the head waters of that
stream (Fig. 90). The tributary which does the stealing is known as a pirate. Stream
f (Fig. 90) is said to be beheaded, and its upper portion, de, diverted. The beheaded
stream is diminished in volume; or if its total supply of water came in above the
point of tapping it would disappear altogether.
Fig. 89 and 90.—Diagrams to illustrate piracy.
The process may not end even here. If after the diversion of de the point in the
channel to the left is lowered faster than the channel of the beheaded stream f, the
divide between dg and the head of f (Fig. 90) will be shifted down the valley of the
latter, as shown in Fig. 91. The shifting will go on until the divide reaches a
position of stability, that is, until erosion on its opposite sides is equal.
stream (Fig. 90). The tributary which does the stealing is known as a pirate. Stream
f (Fig. 90) is said to be beheaded, and its upper portion, de, diverted. The beheaded
stream is diminished in volume; or if its total supply of water came in above the
point of tapping it would disappear altogether.
Fig. 89 and 90.—Diagrams to illustrate piracy.
The process may not end even here. If after the diversion of de the point in the
channel to the left is lowered faster than the channel of the beheaded stream f, the
divide between dg and the head of f (Fig. 90) will be shifted down the valley of the
latter, as shown in Fig. 91. The shifting will go on until the divide reaches a
position of stability, that is, until erosion on its opposite sides is equal.
Page 148
Fig. 91.—Diagram showing the shifting of a divide after piracy.
The foregoing case may be called foreign piracy because the valleys of different
systems are concerned. Domestic piracy may also take place, as illustrated in the
accompanying diagrams (Figs. 92 and 93). Here a tributary to a crooked river may
develop, working back until it taps the main at a higher point, thus straightening the
course of the stream. The change takes place only when the highest point in the
tributary valley is brought below the surface of the water in the main stream at the
point where the tapping takes place. This would be likely to occur only after the
main stream had attained a low gradient, for so long as it is deepening its channel
notably, the small amount of water flowing through the tributary valley would not
be likely to bring it down to the level of the main. In any case the flow of water
from the main stream through the new valley would be likely to be started during
flood, and at such time the erosion in the new channel would be great. The
complete and final diversion of the stream through the new channel might be a
slow process.
Piracy may occur where the material in which the valleys are cut is
homogeneous; but, as will be seen later, heterogeneity of material, by determining
unequal rates of erosion, stimulates the piratical proclivities of streams.
An actual case of piracy is shown on Plate XI. North and South Lakes formerly
drained westward to the Schoharie Creek, the present head of which is in the
extreme northwest corner of the map. The head of Kaaterskill Creek, which had a
much higher gradient, worked back and captured the head of the westward-flowing
stream, diverting the drainage from North and South Lakes to itself. Schoharie
Creek was thus beheaded.
Plaatekill Creek, near the south limit of the map, appears to have beheaded the
creek flowing west and northwest, similarly diverting its head waters. The Dells,
The foregoing case may be called foreign piracy because the valleys of different
systems are concerned. Domestic piracy may also take place, as illustrated in the
accompanying diagrams (Figs. 92 and 93). Here a tributary to a crooked river may
develop, working back until it taps the main at a higher point, thus straightening the
course of the stream. The change takes place only when the highest point in the
tributary valley is brought below the surface of the water in the main stream at the
point where the tapping takes place. This would be likely to occur only after the
main stream had attained a low gradient, for so long as it is deepening its channel
notably, the small amount of water flowing through the tributary valley would not
be likely to bring it down to the level of the main. In any case the flow of water
from the main stream through the new valley would be likely to be started during
flood, and at such time the erosion in the new channel would be great. The
complete and final diversion of the stream through the new channel might be a
slow process.
Piracy may occur where the material in which the valleys are cut is
homogeneous; but, as will be seen later, heterogeneity of material, by determining
unequal rates of erosion, stimulates the piratical proclivities of streams.
An actual case of piracy is shown on Plate XI. North and South Lakes formerly
drained westward to the Schoharie Creek, the present head of which is in the
extreme northwest corner of the map. The head of Kaaterskill Creek, which had a
much higher gradient, worked back and captured the head of the westward-flowing
stream, diverting the drainage from North and South Lakes to itself. Schoharie
Creek was thus beheaded.
Plaatekill Creek, near the south limit of the map, appears to have beheaded the
creek flowing west and northwest, similarly diverting its head waters. The Dells,
Page 149
Wis., quadrangle (U. S. Geol. Surv.)
affords an illustration of domestic
piracy.
Fig. 92 and 93.—Domestic piracy. The tributary, a of
Fig. 92, develops headward until it taps the main
stream at b, giving the result shown in Fig. 93.
RATE OF DEGRADATION.
The amount of mechanical sediment which the Mississippi River carries to the
Gulf of Mexico is estimated to represent a rate of degradation for the Mississippi
basin of about one foot in 5000 years. But the mechanical sediment carried to the
Gulf does not really represent the total degradation of the basin, for the water which
sinks beneath the surface is dissolving more or less rock substance, especially lime
carbonate. This material is carried to the sea in solution, and does not appear in the
sediment on which the above estimate is based. Taking into account the matter
dissolved by the water and carried to the sea in solution, the average rate of
degradation for the Mississippi basin is estimated at one foot in 3000 to 4000 years.
It is not to be inferred that this rate is uniform, or even that erosion at any rate
whatsoever is taking place in all parts of the basin. Such is not the fact. On the
whole the rate of erosion is doubtless greatest toward the margins of the basins
where the land is in its topographic youth or early maturity. It is notably less in the
middle courses of the valleys, and erosion is locally exceeded by deposition along
the lower courses of the Mississippi and some of its main tributaries.
The average elevation of North America is not accurately known, but it is
probably not far from 2000 feet. If the present rate of degradation, say one foot in
3500 years, were to continue, it would take something like 7,000,000 years to bring
the continent to sea-level. But this rate of degradation could not continue to the
affords an illustration of domestic
piracy.
Fig. 92 and 93.—Domestic piracy. The tributary, a of
Fig. 92, develops headward until it taps the main
stream at b, giving the result shown in Fig. 93.
RATE OF DEGRADATION.
The amount of mechanical sediment which the Mississippi River carries to the
Gulf of Mexico is estimated to represent a rate of degradation for the Mississippi
basin of about one foot in 5000 years. But the mechanical sediment carried to the
Gulf does not really represent the total degradation of the basin, for the water which
sinks beneath the surface is dissolving more or less rock substance, especially lime
carbonate. This material is carried to the sea in solution, and does not appear in the
sediment on which the above estimate is based. Taking into account the matter
dissolved by the water and carried to the sea in solution, the average rate of
degradation for the Mississippi basin is estimated at one foot in 3000 to 4000 years.
It is not to be inferred that this rate is uniform, or even that erosion at any rate
whatsoever is taking place in all parts of the basin. Such is not the fact. On the
whole the rate of erosion is doubtless greatest toward the margins of the basins
where the land is in its topographic youth or early maturity. It is notably less in the
middle courses of the valleys, and erosion is locally exceeded by deposition along
the lower courses of the Mississippi and some of its main tributaries.
The average elevation of North America is not accurately known, but it is
probably not far from 2000 feet. If the present rate of degradation, say one foot in
3500 years, were to continue, it would take something like 7,000,000 years to bring
the continent to sea-level. But this rate of degradation could not continue to the
Page 150
end, for as the continent became lower streams would become sluggish and erosion
less rapid. Long before the continent reached base-level the rate of degradation, so
far as dependent on mechanical erosion, would become so slow that the time
necessary to bring the continent to sea-level would be almost inconceivably
prolonged. Furthermore, it is quite possible that the land is suffering, or is liable to
suffer, uplift, relative or absolute. If the rate of rise were equal to the rate of
degradation the average height of the continent would of course not be affected.
The amount of sediment carried by streams in suspension varies
notably according to the stage of the water. During a year when the
stream was under careful study the Mississippi at Carrollton (Miss.)
was found to carry ¹⁄₆₈₁ of its weight of sediment during the high-water
stage of June, and ¹⁄₆₃₈₃ during the low-water of October, the average
for the year being ¹⁄₁₈₀₈. The average of a greater number of records
gives about ¹⁄₁₅₀₀ as the average ratio between the weight of the
sediment and the weight of the water. This corresponds to about ¹⁄₂₉₀₀
by volume, the average specific gravity being about 1.9. The amount
of material carried in the upper part of the water was notably less than
that carried at greater depths, but that carried midway between top and
bottom was about the same as that carried at the bottom.[32]
The discharge of the Mississippi River is about 19,500,000,000,000
cubic feet of water per year, and the sediment it carries in suspension is
estimated to weigh about 812,500,000,000 pounds. This is equivalent
to about 6,714,694,400 cubic feet. It is estimated that about
750,000,000 cubic feet of sediment is rolled along the bottom, giving a
total of 7,468,694,400 cubic feet as the aggregate annual load carried
to the Gulf by the river. This would be adequate to cover an area one
square mile in extent to the depth of 268 feet per year.
less rapid. Long before the continent reached base-level the rate of degradation, so
far as dependent on mechanical erosion, would become so slow that the time
necessary to bring the continent to sea-level would be almost inconceivably
prolonged. Furthermore, it is quite possible that the land is suffering, or is liable to
suffer, uplift, relative or absolute. If the rate of rise were equal to the rate of
degradation the average height of the continent would of course not be affected.
The amount of sediment carried by streams in suspension varies
notably according to the stage of the water. During a year when the
stream was under careful study the Mississippi at Carrollton (Miss.)
was found to carry ¹⁄₆₈₁ of its weight of sediment during the high-water
stage of June, and ¹⁄₆₃₈₃ during the low-water of October, the average
for the year being ¹⁄₁₈₀₈. The average of a greater number of records
gives about ¹⁄₁₅₀₀ as the average ratio between the weight of the
sediment and the weight of the water. This corresponds to about ¹⁄₂₉₀₀
by volume, the average specific gravity being about 1.9. The amount
of material carried in the upper part of the water was notably less than
that carried at greater depths, but that carried midway between top and
bottom was about the same as that carried at the bottom.[32]
The discharge of the Mississippi River is about 19,500,000,000,000
cubic feet of water per year, and the sediment it carries in suspension is
estimated to weigh about 812,500,000,000 pounds. This is equivalent
to about 6,714,694,400 cubic feet. It is estimated that about
750,000,000 cubic feet of sediment is rolled along the bottom, giving a
total of 7,468,694,400 cubic feet as the aggregate annual load carried
to the Gulf by the river. This would be adequate to cover an area one
square mile in extent to the depth of 268 feet per year.
Page 151
PLATE XI.
U. S. Geol. Surv. PART OF THE Scale, 2+ mile per inch.
CATSKILLS, NEW
YORK.
U. S. Geol. Surv. PART OF THE Scale, 2+ mile per inch.
CATSKILLS, NEW
YORK.
Page 152
PLATE XII.
U. S. Geol. Surv. Fig. 1. NEW MEXICO. Scale, 2+ mile per inch.
U. S. Geol. Surv. Fig. 1. NEW MEXICO. Scale, 2+ mile per inch.
Page 153
U. S. Geol. Surv. Fig. 2. VIRGINIA, WEST VIRGINIA AND MARYLAND. Scale, 1+ mile per inch.
ANALYSES OF AMERICAN RIVER-WATERS.[33]
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
Hudson,
Name of river Bear Croton Cumberland Delaware James
N. Y.
Collected at Evanston, Reservoir, New Reservoir at Reservoir Richmond
Wy. York City Nashville, at Water
............
Tenn. Trenton, Works, Va.
N. J.
Date Dec., 1873 1881 Oct. 24. 1876,
............ ............ ............ after light
rain
Analyst F. W. Clarke E. Waller N. T. Lupton H. Wurtz C. F. W. H. Taylor
Chandler
Reference Bulletin No. Water supply Am. Chemist, Geol. of Public Health Ann. Rept.
9, U. S. of New York July 16, N. J., Papers, Board of
Geol. Surv., City, 1881 1876, p. 16 1868, p. Vol. I, Am. Health,
p. 30 702 Pub. Health Richmond,
Ass. Va., 1876
ANALYSES OF AMERICAN RIVER-WATERS.[33]
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
Hudson,
Name of river Bear Croton Cumberland Delaware James
N. Y.
Collected at Evanston, Reservoir, New Reservoir at Reservoir Richmond
Wy. York City Nashville, at Water
............
Tenn. Trenton, Works, Va.
N. J.
Date Dec., 1873 1881 Oct. 24. 1876,
............ ............ ............ after light
rain
Analyst F. W. Clarke E. Waller N. T. Lupton H. Wurtz C. F. W. H. Taylor
Chandler
Reference Bulletin No. Water supply Am. Chemist, Geol. of Public Health Ann. Rept.
9, U. S. of New York July 16, N. J., Papers, Board of
Geol. Surv., City, 1881 1876, p. 16 1868, p. Vol. I, Am. Health,
p. 30 702 Pub. Health Richmond,
Ass. Va., 1876
Page 154
Hudson,
Name of river Bear Croton Cumberland Delaware James
N. Y.
Sodium, Na .0082 [34] .01032 .00072 .00244 .00234
.00298
Potassium, K ...... .00154 .00050 .00178 .00058 .00251
Calcium, Ca .0432 .00905 .02987 .01104 .02220 .01284
Magnesium, Mg .0125 .00336 .00280 .00435 .00465 .00377
Chlorine, Cl .0049 .00213 .00299 .00121 .00581 .00105
Carbonic acid, [35] [34]
CO2 .0982 .02248 .05727 .02552 .07278 .02954
Sulphuric acid,
SO3 .0105 .00441 .00563 .00175 .01257 .00363
Phosphoric acid,
H3PO ...... .00172 Trace
Nitric acid,
HNO3 ...... ...... .00511 ...... ...... .00231
Silica, SiO2 .0070 .03360 Trace .00852 .00698 .01024
Alumina, Al2O3 .00041
Sesquioxide of .00047
iron, Fe2O3 ...... ...... ......
Sesquioxides of
iron and
alumina, Fe2O3 ...... .00078 .00671 ...... .00120 ......
and Al2O3
Sesquioxides of
iron and
manganese, .00072
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese,
FeCO3 and
MnCO3
Oxide of iron,
......
FeO
Oxide of
manganese, Trace ......
MnO
Hydrogen in
.00121
bicarbonates, H
Chloride and
sulphate of
sodium, NaCl, ......
and Na2SO4
Ammonia, NH4 ...... ...... ...... .00001
.01087
Organic matter .00400 .01666 .01197 .00299
Carbonates and ...... ...... ...... ...... ...... ......
sulphates of
Name of river Bear Croton Cumberland Delaware James
N. Y.
Sodium, Na .0082 [34] .01032 .00072 .00244 .00234
.00298
Potassium, K ...... .00154 .00050 .00178 .00058 .00251
Calcium, Ca .0432 .00905 .02987 .01104 .02220 .01284
Magnesium, Mg .0125 .00336 .00280 .00435 .00465 .00377
Chlorine, Cl .0049 .00213 .00299 .00121 .00581 .00105
Carbonic acid, [35] [34]
CO2 .0982 .02248 .05727 .02552 .07278 .02954
Sulphuric acid,
SO3 .0105 .00441 .00563 .00175 .01257 .00363
Phosphoric acid,
H3PO ...... .00172 Trace
Nitric acid,
HNO3 ...... ...... .00511 ...... ...... .00231
Silica, SiO2 .0070 .03360 Trace .00852 .00698 .01024
Alumina, Al2O3 .00041
Sesquioxide of .00047
iron, Fe2O3 ...... ...... ......
Sesquioxides of
iron and
alumina, Fe2O3 ...... .00078 .00671 ...... .00120 ......
and Al2O3
Sesquioxides of
iron and
manganese, .00072
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese,
FeCO3 and
MnCO3
Oxide of iron,
......
FeO
Oxide of
manganese, Trace ......
MnO
Hydrogen in
.00121
bicarbonates, H
Chloride and
sulphate of
sodium, NaCl, ......
and Na2SO4
Ammonia, NH4 ...... ...... ...... .00001
.01087
Organic matter .00400 .01666 .01197 .00299
Carbonates and ...... ...... ...... ...... ...... ......
sulphates of
Page 155
Hudson,
Name of river Bear Croton Cumberland Delaware James
N. Y.
Na, K, and Mg
.1845 .08433 .13786 .06795 .14238 .07246
ANALYSES OF AMERICAN RIVER-WATERS (continued).
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
Rio
Los Maumee,
Name of river Mississippi Ottawa Passaic
Grande del Sacramento
Angeles O.
Norte
Collected at Hydrant, St. Ann’s 4 miles Fort Hydrant, Hydrant at
City ater Lock, above Craig, Sacramento, Los
Works, Montreal, Newark, New Cal. Angeles,
............
New Can. N. J. Mexico Cal.
Orleans,
La.
Date Sept. 8, Mar. 9, 1851 1873 Sept., 1878
............ ............
1878 1854
Analyst W. J. Jones C. F. W. J. Jones T. S. Hunt E. N. O. Loew W. J. Jones
Chandler Horsford
Reference Rept. Cal. Report of Rept. La. Geol. of Geol. of N. J., U. S. Geog. Rept. Cal.
State Toledo State Canada, 1868, p. 708 Surv. State
Board of Water Board of 1863, p. west of Board of
Health, Works, Health, 567 100th M., Health,
1878 1881 1882, p. Vol. III. 1878
370 p. 576
Sodium, Na .02968 .00162 .0310 .00239 .02357 .03220 .00200
Potassium, K ...... .00309 ...... .00139 .00163 .00063 ......
Calcium, Ca .01750 .02645 .0372 .00992 .01459 .01633 .01279
Magnesium,
.02097 .00443 ...... .00161 .00404 .00123 .00121
Mg
Chlorine, Cl .01044 .00250 .0480 .00076 .03192 .03604 ......
Carbonic acid,
CO2 .05635 .04438 .0383 .02255 .02634 .01025 .00887
Sulphuric acid,
SO3 .05724 .01401 .00194 .01716 .04700 .00397
Phosphoric
acid, H3PO .02638 Trace Faint trace .0179
Nitric acid,
HNO3 ...... ...... ...... Trace ......
Silica, SiO2 .02005 .00724 .02060 Trace .03167
Alumina, Al2O3 .00171 ...... Trace Trace .00120 Trace
.01342
Sesquioxide of
iron, Fe2O3 .00100
Sesquioxides of ...... ......
iron and
alumina,
Name of river Bear Croton Cumberland Delaware James
N. Y.
Na, K, and Mg
.1845 .08433 .13786 .06795 .14238 .07246
ANALYSES OF AMERICAN RIVER-WATERS (continued).
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
Rio
Los Maumee,
Name of river Mississippi Ottawa Passaic
Grande del Sacramento
Angeles O.
Norte
Collected at Hydrant, St. Ann’s 4 miles Fort Hydrant, Hydrant at
City ater Lock, above Craig, Sacramento, Los
Works, Montreal, Newark, New Cal. Angeles,
............
New Can. N. J. Mexico Cal.
Orleans,
La.
Date Sept. 8, Mar. 9, 1851 1873 Sept., 1878
............ ............
1878 1854
Analyst W. J. Jones C. F. W. J. Jones T. S. Hunt E. N. O. Loew W. J. Jones
Chandler Horsford
Reference Rept. Cal. Report of Rept. La. Geol. of Geol. of N. J., U. S. Geog. Rept. Cal.
State Toledo State Canada, 1868, p. 708 Surv. State
Board of Water Board of 1863, p. west of Board of
Health, Works, Health, 567 100th M., Health,
1878 1881 1882, p. Vol. III. 1878
370 p. 576
Sodium, Na .02968 .00162 .0310 .00239 .02357 .03220 .00200
Potassium, K ...... .00309 ...... .00139 .00163 .00063 ......
Calcium, Ca .01750 .02645 .0372 .00992 .01459 .01633 .01279
Magnesium,
.02097 .00443 ...... .00161 .00404 .00123 .00121
Mg
Chlorine, Cl .01044 .00250 .0480 .00076 .03192 .03604 ......
Carbonic acid,
CO2 .05635 .04438 .0383 .02255 .02634 .01025 .00887
Sulphuric acid,
SO3 .05724 .01401 .00194 .01716 .04700 .00397
Phosphoric
acid, H3PO .02638 Trace Faint trace .0179
Nitric acid,
HNO3 ...... ...... ...... Trace ......
Silica, SiO2 .02005 .00724 .02060 Trace .03167
Alumina, Al2O3 .00171 ...... Trace Trace .00120 Trace
.01342
Sesquioxide of
iron, Fe2O3 .00100
Sesquioxides of ...... ......
iron and
alumina,
Page 156
Rio
Los Maumee,
Name of river Mississippi Ottawa Passaic Grande del Sacramento
Angeles O.
Norte
Fe2O3 and
Al2O3
Sesquioxides of
iron and
manganese, ...... ......
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese, .00443 ...... ...... .01088
FeCO3 and
MnCO3
Oxide of iron,
Trace Trace
FeO
Oxide of
manganese, Trace
MnO
Hydrogen in
bicarbonates, ......
H
Chloride and
sulphate of
sodium, ...... .02431
NaCl, and
Na2SO4
Ammonia, NH4 ...... Trace
Organic matter .00499 ...... .01392
Carbonates and
sulphates of
...... ...... .0154 ...... ...... ...... ......
Na, K, and
Mg
.24475 .10971 .1699 .06116 .13287 .15760 .11484
ANALYSES OF AMERICAN RIVER-WATERS (continued).
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
St.
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
South side Collected Battle Mt., Lake Tahoe, Mason Utah Utica, N. Y. Rochester,
Point des at Nev. Nev. Valley, Lake N. Y.
Cascades Nev.
Date Mar. 30, Dec., 1872 Oct., 1872 Oct., 1872 Nov.,
1863 1873
Analyst T. S. T. M. F. W. Clarke F. W. Clarke F. W. C. F. C. F.
Hunt Chatard Clarke Chandler Chandler
Reference Geol. of U. S. Geol. U. S. Geol. U. S. Geol. Bulletin Johnson’s Johnson’s
Canada, Surv., Surv., Surv., No. 9, Cyclopedia, Cyclopedia,
Los Maumee,
Name of river Mississippi Ottawa Passaic Grande del Sacramento
Angeles O.
Norte
Fe2O3 and
Al2O3
Sesquioxides of
iron and
manganese, ...... ......
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese, .00443 ...... ...... .01088
FeCO3 and
MnCO3
Oxide of iron,
Trace Trace
FeO
Oxide of
manganese, Trace
MnO
Hydrogen in
bicarbonates, ......
H
Chloride and
sulphate of
sodium, ...... .02431
NaCl, and
Na2SO4
Ammonia, NH4 ...... Trace
Organic matter .00499 ...... .01392
Carbonates and
sulphates of
...... ...... .0154 ...... ...... ...... ......
Na, K, and
Mg
.24475 .10971 .1699 .06116 .13287 .15760 .11484
ANALYSES OF AMERICAN RIVER-WATERS (continued).
[Reduced to Parts per 1000 by Dr. H. J. Van Hoesen.]
St.
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
South side Collected Battle Mt., Lake Tahoe, Mason Utah Utica, N. Y. Rochester,
Point des at Nev. Nev. Valley, Lake N. Y.
Cascades Nev.
Date Mar. 30, Dec., 1872 Oct., 1872 Oct., 1872 Nov.,
1863 1873
Analyst T. S. T. M. F. W. Clarke F. W. Clarke F. W. C. F. C. F.
Hunt Chatard Clarke Chandler Chandler
Reference Geol. of U. S. Geol. U. S. Geol. U. S. Geol. Bulletin Johnson’s Johnson’s
Canada, Surv., Surv., Surv., No. 9, Cyclopedia, Cyclopedia,
Page 157
St.
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
1863, p. Monograph Monograph Monograph U. S. Vol. IV Vol. IV
567 XI, p. 41 XI, p. 42 XI, p. 40 Geol.
Surv.,
p. 29
Sodium, Na .00513 .0467 .0073 .0318 .0178 .0036 .0044
Potassium, K .00115 .0100 .0033 Trace ...... .0009 .0023
Calcium, Ca .03233 .0489 .0093 .0228 .0558 .0318 .0417
Magnesium,
.00585 .0124 .0030 .0038 .0186 .0069 .00896
Mg
Chlorine, Cl .00242 .0075 .0023 .0131 .0124 .0023 .0024
Carbonic acid, [35] [35] [35]
CO2 .06836 .1544 .0287 .0576 .0608 .0569 .0646
Sulphuric acid,
SO3 .00831 .0477 .0054 .0284 .1306 .0187 .0431
Phosphoric
acid, H3PO Trace ......
Nitric acid,
HNO3 ...... ...... ...... ...... ...... ......
Silica, SiO2 .03700 .0326 .0137 0.225 .0100 .0067 .0014
Alumina,
Al2O3 .0013
Sesquioxide of
iron, Fe2O3 ...... ......
Sesquioxides
of iron and
alumina, .0013 .0014
Fe2O3 and
Al2O3
Sesquioxides
of iron and
manganese,
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese, ......
FeCO3 and
MnCO3
Oxide of iron,
Trace ......
FeO
Oxide of
manganese, Trace ...... ......
MnO
Hydrogen in
bicarbonates, ...... ...... ......
H
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
1863, p. Monograph Monograph Monograph U. S. Vol. IV Vol. IV
567 XI, p. 41 XI, p. 42 XI, p. 40 Geol.
Surv.,
p. 29
Sodium, Na .00513 .0467 .0073 .0318 .0178 .0036 .0044
Potassium, K .00115 .0100 .0033 Trace ...... .0009 .0023
Calcium, Ca .03233 .0489 .0093 .0228 .0558 .0318 .0417
Magnesium,
.00585 .0124 .0030 .0038 .0186 .0069 .00896
Mg
Chlorine, Cl .00242 .0075 .0023 .0131 .0124 .0023 .0024
Carbonic acid, [35] [35] [35]
CO2 .06836 .1544 .0287 .0576 .0608 .0569 .0646
Sulphuric acid,
SO3 .00831 .0477 .0054 .0284 .1306 .0187 .0431
Phosphoric
acid, H3PO Trace ......
Nitric acid,
HNO3 ...... ...... ...... ...... ...... ......
Silica, SiO2 .03700 .0326 .0137 0.225 .0100 .0067 .0014
Alumina,
Al2O3 .0013
Sesquioxide of
iron, Fe2O3 ...... ......
Sesquioxides
of iron and
alumina, .0013 .0014
Fe2O3 and
Al2O3
Sesquioxides
of iron and
manganese,
Fe2O3 and
Mn2O3
Carbonates of
iron and
manganese, ......
FeCO3 and
MnCO3
Oxide of iron,
Trace ......
FeO
Oxide of
manganese, Trace ...... ......
MnO
Hydrogen in
bicarbonates, ...... ...... ......
H
Page 158
St.
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
Chloride and
sulphate of
sodium, ...... ...... ......
NaCl, and
Na2SO4
Ammonia,
NH4 ...... ...... ......
Organic matter ...... ...... .0234 .0250
Carbonates
and
sulphates of ...... ...... ...... ...... ...... ...... ......
Na, K, and
Mg
.16055 .3615 .0730 .1800 .3060 .1525 019526
The following table[36] gives the percentage of material carried in suspension by
various rivers:
Height in Feet of Thickness of
Drainage Mean Annual Ratio of
Column of Sediment in
Areas in Discharge (in Total Tons Sediment to
River. Sediment with a Inches if Spread
Square Cubic Feet.) Annually. Water by
Base of One over Drainage
Miles. per Second. Weight.
Square Mile. Area.
Potomac 11,043 20,160 5,557,250 1 : 3,575 4.0 .00433
Mississippi 1,244,000 610,000 406,250,000 1 : 1,500 241.4 .00223
Rio
30,000 1,700 3,830,000 1: 291 2.8 .00116
Grande
Uruguay 150,000 150,000 14,782,500 1 : 10,000 10.6 .00085
Rhone 34,800 65,850 36,000,000 1 : 1,775 31.1 .01075
Po 27,100 62,200 67,000,000 1: 900 59.0 .01139
Danube 320,300 315,200 108,000,000 1 : 2,880 93.2 .00354
Nile 1,100,000 113,000 54,000,000 1 : 2,050 38.8 .00042
Irrawaddy 125,000 475,000 291,430,000 1 : 1,610 209.0 .02005
Mean 334,693 201,468 109,649,972 1 : 2,731 76.65 .00614
The composition of rain-water falling near London, as determined by analysis,
was as follows:[37]
Organic carbon .99 part in 1,000,000 of water.
Organic nitrogen .22 “ “ “ “ “
Ammonia .50 “ “ “ “ “
Nitrogen as nitrates and nitrites .07 “ “ “ “ “
Chlorine 6.30 parts in “ “ “
Total solids 39.50 “ “ “ “ “
Name of river Humboldt Truckee Walker Jordan Mohawk Genesee
Lawrence
Chloride and
sulphate of
sodium, ...... ...... ......
NaCl, and
Na2SO4
Ammonia,
NH4 ...... ...... ......
Organic matter ...... ...... .0234 .0250
Carbonates
and
sulphates of ...... ...... ...... ...... ...... ...... ......
Na, K, and
Mg
.16055 .3615 .0730 .1800 .3060 .1525 019526
The following table[36] gives the percentage of material carried in suspension by
various rivers:
Height in Feet of Thickness of
Drainage Mean Annual Ratio of
Column of Sediment in
Areas in Discharge (in Total Tons Sediment to
River. Sediment with a Inches if Spread
Square Cubic Feet.) Annually. Water by
Base of One over Drainage
Miles. per Second. Weight.
Square Mile. Area.
Potomac 11,043 20,160 5,557,250 1 : 3,575 4.0 .00433
Mississippi 1,244,000 610,000 406,250,000 1 : 1,500 241.4 .00223
Rio
30,000 1,700 3,830,000 1: 291 2.8 .00116
Grande
Uruguay 150,000 150,000 14,782,500 1 : 10,000 10.6 .00085
Rhone 34,800 65,850 36,000,000 1 : 1,775 31.1 .01075
Po 27,100 62,200 67,000,000 1: 900 59.0 .01139
Danube 320,300 315,200 108,000,000 1 : 2,880 93.2 .00354
Nile 1,100,000 113,000 54,000,000 1 : 2,050 38.8 .00042
Irrawaddy 125,000 475,000 291,430,000 1 : 1,610 209.0 .02005
Mean 334,693 201,468 109,649,972 1 : 2,731 76.65 .00614
The composition of rain-water falling near London, as determined by analysis,
was as follows:[37]
Organic carbon .99 part in 1,000,000 of water.
Organic nitrogen .22 “ “ “ “ “
Ammonia .50 “ “ “ “ “
Nitrogen as nitrates and nitrites .07 “ “ “ “ “
Chlorine 6.30 parts in “ “ “
Total solids 39.50 “ “ “ “ “
Page 159
A comparison of the composition of rain-water with that of springs and rivers
gives some idea of the solvent work of water. From a study of the water of nineteen
of the principal rivers of the world Murray has compiled the following table[38]
showing the amount of mineral matter in average river water:
MATERIAL IN SOLUTION IN ONE CUBIC
MILE OF AVERAGE RIVER WATER.[39]
Constituents. Tons in a Cubic Mile.
Calcium carbonate (CaCO3) 326,710
Magnesium carbonate (MgCO3) 112,870
Calcium phosphate (Ca3P2O8) 2,913
Calcium sulphate (CaSO4) 34,361
Sodium sulphate (Na2SO4) 31,805
Potassium sulphate (K2SO4) 20,358
Sodium nitrate (NaNO3) 26,800
Sodium chloride (NaCl) 16,657
Lithium chloride (LiCl) 2,462
Ammonium chloride (NH4Cl) 1,030
Silica (SiO2) 74,577
Ferric oxide (Fe2O3) 13,006
Alumina (Al2O3) 14,315
Manganese oxide (Mn2O3) 5,703
Organic matter 79,020
Total dissolved matter 762,587
Murray also estimates that the aggregate amount of water flowing into the sea
annually is about 6528 cubic miles, which, on the above basis, would carry about
4,975,000,000 tons of mineral matter in solution.
A large number of analyses of waters of rivers from the United States and
Canada give an average of about .15,044 part in a thousand of mineral matter in
solution, more than one-third being CaCO3. The average amount of mineral matter
in solution in 48 European streams cited by Bischoff[40] is .2127 part in a thousand,
of which CaCO3 is rather more than half. The average mineral matter in solution in
36 rivers cited by Roth[41] (including some of those tabulated by Bischoff) is .2033
part in a thousand, of which CaCO3 is slightly less than one-half.
gives some idea of the solvent work of water. From a study of the water of nineteen
of the principal rivers of the world Murray has compiled the following table[38]
showing the amount of mineral matter in average river water:
MATERIAL IN SOLUTION IN ONE CUBIC
MILE OF AVERAGE RIVER WATER.[39]
Constituents. Tons in a Cubic Mile.
Calcium carbonate (CaCO3) 326,710
Magnesium carbonate (MgCO3) 112,870
Calcium phosphate (Ca3P2O8) 2,913
Calcium sulphate (CaSO4) 34,361
Sodium sulphate (Na2SO4) 31,805
Potassium sulphate (K2SO4) 20,358
Sodium nitrate (NaNO3) 26,800
Sodium chloride (NaCl) 16,657
Lithium chloride (LiCl) 2,462
Ammonium chloride (NH4Cl) 1,030
Silica (SiO2) 74,577
Ferric oxide (Fe2O3) 13,006
Alumina (Al2O3) 14,315
Manganese oxide (Mn2O3) 5,703
Organic matter 79,020
Total dissolved matter 762,587
Murray also estimates that the aggregate amount of water flowing into the sea
annually is about 6528 cubic miles, which, on the above basis, would carry about
4,975,000,000 tons of mineral matter in solution.
A large number of analyses of waters of rivers from the United States and
Canada give an average of about .15,044 part in a thousand of mineral matter in
solution, more than one-third being CaCO3. The average amount of mineral matter
in solution in 48 European streams cited by Bischoff[40] is .2127 part in a thousand,
of which CaCO3 is rather more than half. The average mineral matter in solution in
36 rivers cited by Roth[41] (including some of those tabulated by Bischoff) is .2033
part in a thousand, of which CaCO3 is slightly less than one-half.
Page 160
An average for American and European rivers, so far as determinable from data
at hand, is about .1888 part in a thousand in solution, of which CaCO3 is slightly
less than one-half. These last figures are probably not very far from an average for
river water in general.
The following table shows the total amount of solids carried in solution by the
rivers indicated:[42]
Rhine 5,816,805 tons per year.
Rhone 8,290,464 “ “ “
Danube 22,521,434 “ “ “
Thames 613,930 “ “ “
Nile 16,950,000 “ “ “
Croton 66,795 “ “ “
Hudson 438,000 “ “ “
Mississippi 112,832,171 “ “ “
ECONOMIC CONSIDERATIONS.
Certain considerations of human interest in connection with river erosion are
worthy of note. When a drainage system has reached its mature stage its basin has
the roughest topography which it will have at any time during that cycle of erosion.
At that stage, therefore, road construction is relatively difficult. If the relief be
great, roads must follow the valleys, or the crests of the ridges between them, if
they would avoid heavy grades. In such regions roads are usually few and crooked.
The stage of development of valleys has an influence on the navigability of their
streams. Streams well advanced in life are much more readily navigable than young
ones, because their grades are lower and their volumes of water greater. Old
streams, on the other hand, are sometimes depositing sand or silt along their lower
courses to such an extent as to interfere with navigation.
At certain stages of their development the power of streams is more easily
utilized than at others. Young streams, depending as they do for their supply on the
rainfall of a limited area, are likely to be fitful in their flow, and therefore unreliable
as a source of power. This is especially true where the precipitation is unequally
distributed, and where the slopes are steep and free from forests. Because of their
great volume, old and large streams, though sluggish, have great power, but it is
less easily controlled. Where streams are large enough to be navigable industrial
considerations often prevent the utilization of their power, the streams being more
serviceable as highways than as sources of power. Other things being equal, it
at hand, is about .1888 part in a thousand in solution, of which CaCO3 is slightly
less than one-half. These last figures are probably not very far from an average for
river water in general.
The following table shows the total amount of solids carried in solution by the
rivers indicated:[42]
Rhine 5,816,805 tons per year.
Rhone 8,290,464 “ “ “
Danube 22,521,434 “ “ “
Thames 613,930 “ “ “
Nile 16,950,000 “ “ “
Croton 66,795 “ “ “
Hudson 438,000 “ “ “
Mississippi 112,832,171 “ “ “
ECONOMIC CONSIDERATIONS.
Certain considerations of human interest in connection with river erosion are
worthy of note. When a drainage system has reached its mature stage its basin has
the roughest topography which it will have at any time during that cycle of erosion.
At that stage, therefore, road construction is relatively difficult. If the relief be
great, roads must follow the valleys, or the crests of the ridges between them, if
they would avoid heavy grades. In such regions roads are usually few and crooked.
The stage of development of valleys has an influence on the navigability of their
streams. Streams well advanced in life are much more readily navigable than young
ones, because their grades are lower and their volumes of water greater. Old
streams, on the other hand, are sometimes depositing sand or silt along their lower
courses to such an extent as to interfere with navigation.
At certain stages of their development the power of streams is more easily
utilized than at others. Young streams, depending as they do for their supply on the
rainfall of a limited area, are likely to be fitful in their flow, and therefore unreliable
as a source of power. This is especially true where the precipitation is unequally
distributed, and where the slopes are steep and free from forests. Because of their
great volume, old and large streams, though sluggish, have great power, but it is
less easily controlled. Where streams are large enough to be navigable industrial
considerations often prevent the utilization of their power, the streams being more
serviceable as highways than as sources of power. Other things being equal, it
Page 161
follows that streams are most available for water-power when they are large enough
to have a moderately steady flow, and not so large as to be beyond ready control, or
to be valuable for purposes of navigation.
Streams are subject to more disastrous floods in some stages of their
development than in others. Floods resulting from heavy rains are likely to be
greatest where the slopes above the drainage lines are on the whole greatest, for this
is the condition under which the water is most quickly gathered into the drainage
channels. The most disastrous floods, humanly speaking, are those which affect
wide-bottomed valleys, where the flats are settled. In such cases a relatively slight
rise may flood very extensive areas. In such valleys the most disastrous floods are
generally in the spring, when the waters from the melting snows of the preceding
winter are being discharged.[43] Many other considerations enter into the problem of
floods. The presence of forests and other forms of vegetation on the slopes retards
the flow of water into the valleys, and so tends to prevent floods, or at any rate to
make them less severe. Porous soil and subsoil, or in their absence porous rock,
absorb the rainfall, and prevent its prompt descent into the valleys and so tends to
prevent or diminish floods.
The acreage of arable land within a given area stands in some relation to its
drainage development. At an early stage in its erosion history, before an upland has
been dissected by valleys, nearly all of it may be arable. Later, when drainage is at
its maturity, and when hillsides and ridge slopes constitute a large part of the area,
there is probably the least acreage of arable land. This is especially true if the
slopes are so steep as to allow the soil to be readily washed away. At a still later
stage, when the valley bottoms have become wide and the slopes of the ridges and
hills so reduced as to be available, the area of cultivable land is again increased.
Marshes, ponds, and lakes have some bearing on the resources and industries of
a region, and they stand in a more or less definite relation to the stage of erosion in
which a region finds itself. In its youth ponds and lakes may occupy much of the
surface; in its maturity they will have been largely drained.
These suggestions are sufficient to show that the topography of a region, even in
so far as shaped by erosion, touches human interests at many points.
ANALYSIS OF EROSION.[44]
Erosion is the term applied to all the processes by which earthy matter or rock is
loosened and removed from one place to another. It consists of three sub-processes,
namely, weathering, transportation, and corrasion.
to have a moderately steady flow, and not so large as to be beyond ready control, or
to be valuable for purposes of navigation.
Streams are subject to more disastrous floods in some stages of their
development than in others. Floods resulting from heavy rains are likely to be
greatest where the slopes above the drainage lines are on the whole greatest, for this
is the condition under which the water is most quickly gathered into the drainage
channels. The most disastrous floods, humanly speaking, are those which affect
wide-bottomed valleys, where the flats are settled. In such cases a relatively slight
rise may flood very extensive areas. In such valleys the most disastrous floods are
generally in the spring, when the waters from the melting snows of the preceding
winter are being discharged.[43] Many other considerations enter into the problem of
floods. The presence of forests and other forms of vegetation on the slopes retards
the flow of water into the valleys, and so tends to prevent floods, or at any rate to
make them less severe. Porous soil and subsoil, or in their absence porous rock,
absorb the rainfall, and prevent its prompt descent into the valleys and so tends to
prevent or diminish floods.
The acreage of arable land within a given area stands in some relation to its
drainage development. At an early stage in its erosion history, before an upland has
been dissected by valleys, nearly all of it may be arable. Later, when drainage is at
its maturity, and when hillsides and ridge slopes constitute a large part of the area,
there is probably the least acreage of arable land. This is especially true if the
slopes are so steep as to allow the soil to be readily washed away. At a still later
stage, when the valley bottoms have become wide and the slopes of the ridges and
hills so reduced as to be available, the area of cultivable land is again increased.
Marshes, ponds, and lakes have some bearing on the resources and industries of
a region, and they stand in a more or less definite relation to the stage of erosion in
which a region finds itself. In its youth ponds and lakes may occupy much of the
surface; in its maturity they will have been largely drained.
These suggestions are sufficient to show that the topography of a region, even in
so far as shaped by erosion, touches human interests at many points.
ANALYSIS OF EROSION.[44]
Erosion is the term applied to all the processes by which earthy matter or rock is
loosened and removed from one place to another. It consists of three sub-processes,
namely, weathering, transportation, and corrasion.
Page 162
Weathering.
The term weathering is applied to nearly all those natural processes which tend
to loosen or change the exposed surfaces of rock. The lettering of inscriptions on
exposed marble becomes fainter and fainter as time goes by, and finally disappears,
because the rock in which the letters were cut has weathered away. Some of it has
crumbled off as the result of the expansion and contraction induced by changes of
temperature, and some of it has been dissolved by the rain which has fallen upon it.
In this case the weathering is effected partly by the atmosphere and partly by water.
These are the chief, but not the only agents concerned in the general processes of
weathering. Those phases of weathering which are the result of the activities of the
atmosphere, whether physical or chemical, have been discussed in connection with
the atmosphere (pp. 42 and 54).
The rain which falls upon the surface of exposed rock, and that which sinks
through the soil to the solid rock below, dissolves, even if slowly, some of the rock
constituents. Each constituent of a rock composed of several minerals may be
looked upon as a binding material for the others. When one is dissolved the rock
crumbles, much as mortar does when the lime which cements the sand is dissolved.
The solution of mineral matter by ground water, as well as the other chemical
changes it effects, is greatly augmented by the impurities, especially carbonic and
other organic gases, dissolved by the water from the atmosphere and the soil. The
commonest chemical changes effected by the joint action of water and air,
oxidation and carbonation, have been referred to in Chapter II. Hydration is more
exclusively the work of water, and is one of the commonest processes of rock
change, and often of rock disintegration. Numerous other less simple chemical
changes resulting from the activities of ground water are constantly in progress, and
in so far as they lead to the disintegration of rock are processes of weathering.
Many chemical changes involve notable changes in volume of the mineral matter
concerned. Merrill has calculated that in the conversion of the granitic rock of the
vicinity of Washington, D. C., into soil, its volume has been increased 88 percent.,
largely as the result of hydration.[45] Even when the chemical changes do not
themselves directly involve the disintegration of the rock, the accompanying
increase of volume is sometimes sufficient to cause its physical disruption. This
also may be regarded as a phase of weathering.
The weathering accomplished by water, or under its influence, proceeds at rates
which vary with the composition of the rock, the amount and composition of the
water, the temperature, and certain other factors less susceptible of brief statement.
The weathering effected by ground water has a wider range both in area and depth
than that due to changes of temperature, for while the latter is effective only where
The term weathering is applied to nearly all those natural processes which tend
to loosen or change the exposed surfaces of rock. The lettering of inscriptions on
exposed marble becomes fainter and fainter as time goes by, and finally disappears,
because the rock in which the letters were cut has weathered away. Some of it has
crumbled off as the result of the expansion and contraction induced by changes of
temperature, and some of it has been dissolved by the rain which has fallen upon it.
In this case the weathering is effected partly by the atmosphere and partly by water.
These are the chief, but not the only agents concerned in the general processes of
weathering. Those phases of weathering which are the result of the activities of the
atmosphere, whether physical or chemical, have been discussed in connection with
the atmosphere (pp. 42 and 54).
The rain which falls upon the surface of exposed rock, and that which sinks
through the soil to the solid rock below, dissolves, even if slowly, some of the rock
constituents. Each constituent of a rock composed of several minerals may be
looked upon as a binding material for the others. When one is dissolved the rock
crumbles, much as mortar does when the lime which cements the sand is dissolved.
The solution of mineral matter by ground water, as well as the other chemical
changes it effects, is greatly augmented by the impurities, especially carbonic and
other organic gases, dissolved by the water from the atmosphere and the soil. The
commonest chemical changes effected by the joint action of water and air,
oxidation and carbonation, have been referred to in Chapter II. Hydration is more
exclusively the work of water, and is one of the commonest processes of rock
change, and often of rock disintegration. Numerous other less simple chemical
changes resulting from the activities of ground water are constantly in progress, and
in so far as they lead to the disintegration of rock are processes of weathering.
Many chemical changes involve notable changes in volume of the mineral matter
concerned. Merrill has calculated that in the conversion of the granitic rock of the
vicinity of Washington, D. C., into soil, its volume has been increased 88 percent.,
largely as the result of hydration.[45] Even when the chemical changes do not
themselves directly involve the disintegration of the rock, the accompanying
increase of volume is sometimes sufficient to cause its physical disruption. This
also may be regarded as a phase of weathering.
The weathering accomplished by water, or under its influence, proceeds at rates
which vary with the composition of the rock, the amount and composition of the
water, the temperature, and certain other factors less susceptible of brief statement.
The weathering effected by ground water has a wider range both in area and depth
than that due to changes of temperature, for while the latter is effective only where
Page 163
temperature changes are considerable, and where coherent material lies at the
surface (p. 45), the former is operative to all depths to which water sinks.
Fig. 94.—Talus accumulation at the base of a steep bluff. Weber Canyon, Uinta Mountains, Utah.
The talus has accumulated since the last glaciation of the valley and is therefore of very recent
origin. (Church.)
There are other processes of weathering not due directly either to the atmosphere
or to water. The roots of trees and smaller plants frequently grow into cracks of
rocks, and, increasing in size, act much like freezing water (p. 45) in similar
situations. This wedge-work of roots is a phase of weathering.
From the faces of steep cliffs masses of rock frequently fall. However dislodged,
their descent is effected by gravity. The quantities of débris at the bases of many
cliffs, forming slopes of talus (Fig. 94), testify to the importance of the action of
gravity in getting material from higher to lower levels. Another phase of gravity-
work is shown in Fig. 95. Here, under the influence of gravity and expansion and
contraction, due to freezing and thawing and wetting and drying, the surface
material is creeping down slope. In the process the rock is being broken. The
process illustrated by the figure involves weathering as well as other factors.
The foregoing are among the commoner processes of weathering, although they
do not exhaust the list. The more active and tangible processes by which surface
rocks are broken up, such as wave wear, river wear and glacier wear, are processes
of corrasion. The mechanical wear effected by wind-driven sand might be
surface (p. 45), the former is operative to all depths to which water sinks.
Fig. 94.—Talus accumulation at the base of a steep bluff. Weber Canyon, Uinta Mountains, Utah.
The talus has accumulated since the last glaciation of the valley and is therefore of very recent
origin. (Church.)
There are other processes of weathering not due directly either to the atmosphere
or to water. The roots of trees and smaller plants frequently grow into cracks of
rocks, and, increasing in size, act much like freezing water (p. 45) in similar
situations. This wedge-work of roots is a phase of weathering.
From the faces of steep cliffs masses of rock frequently fall. However dislodged,
their descent is effected by gravity. The quantities of débris at the bases of many
cliffs, forming slopes of talus (Fig. 94), testify to the importance of the action of
gravity in getting material from higher to lower levels. Another phase of gravity-
work is shown in Fig. 95. Here, under the influence of gravity and expansion and
contraction, due to freezing and thawing and wetting and drying, the surface
material is creeping down slope. In the process the rock is being broken. The
process illustrated by the figure involves weathering as well as other factors.
The foregoing are among the commoner processes of weathering, although they
do not exhaust the list. The more active and tangible processes by which surface
rocks are broken up, such as wave wear, river wear and glacier wear, are processes
of corrasion. The mechanical wear effected by wind-driven sand might be
Page 164
considered either as corrasion or as weathering. It is more likely to be regarded as
corrasion if the amount of wear is considerable enough to be obvious. Rock is
sometimes decomposed by the chemical action of hot vapors, gases, and waters
rising to the surface from considerable depths. This is often seen in volcanic
regions. A conspicuous illustration is seen in the canyon of the Yellowstone in the
National Park. Decay of this sort is perhaps not properly weathering, but is not
always readily distinguished from it.
Fig. 95.—Shows the downward creep of soil and slaty rock under the influence of gravity.
The importance of weathering in the general processes of erosion is shown in
many ways. In regions where the mantle rock is the product of the decay of the
solid rock beneath, and such regions constitute a large portion of the earth’s
surface, the soil and subsoil represent the excess of weathering over transportation.
Since most of the earth’s surface is covered with soil to a greater or less depth, it is
clear that, on the whole, weathering keeps ahead of transportation. Again, it is clear
that the loosening of rock by weathering greatly increases the erosion which a
given amount of moving water can accomplish. Not only this, but weathering plays
a much more important rôle in the development of valleys than is commonly
realized. This is best illustrated by the valleys of young swift streams. The valley
corrasion if the amount of wear is considerable enough to be obvious. Rock is
sometimes decomposed by the chemical action of hot vapors, gases, and waters
rising to the surface from considerable depths. This is often seen in volcanic
regions. A conspicuous illustration is seen in the canyon of the Yellowstone in the
National Park. Decay of this sort is perhaps not properly weathering, but is not
always readily distinguished from it.
Fig. 95.—Shows the downward creep of soil and slaty rock under the influence of gravity.
The importance of weathering in the general processes of erosion is shown in
many ways. In regions where the mantle rock is the product of the decay of the
solid rock beneath, and such regions constitute a large portion of the earth’s
surface, the soil and subsoil represent the excess of weathering over transportation.
Since most of the earth’s surface is covered with soil to a greater or less depth, it is
clear that, on the whole, weathering keeps ahead of transportation. Again, it is clear
that the loosening of rock by weathering greatly increases the erosion which a
given amount of moving water can accomplish. Not only this, but weathering plays
a much more important rôle in the development of valleys than is commonly
realized. This is best illustrated by the valleys of young swift streams. The valley
Page 165
which is not at its top ten times as wide as its stream is rare. The stream which has
such a canyon has been cutting chiefly at its bottom. Ignoring its lateral corrasion,
which is slight, the valley which it would cut would have a width equal to its own.
This is illustrated by Fig. 96. Weathering in its broadest sense is largely responsible
for the width of such a valley, in so far as it exceeds the width of the stream. The
work of weathering, slope wash, etc., has been to get the material which originally
lay between a, b, and c down to the stream. The stream has then carried it away.
The above illustration would not apply to old and sluggish streams, for they, by
their meandering, widen their valleys independently of weathering.
Fig. 96.—Diagram of a valley the top of which is ten times the width of the stream.
Weathering is a part of erosion, but only a part. In so far as it is effected by
solution the process involves the transportation of that which is dissolved to some
other point. Transportation is also involved to some extent in the other processes of
weathering, but the central idea of the processes embraced under this term is the
loosening and disrupting of rock by which it is prepared for transportation.
Transportation.
The second element of erosion is transportation. The transportation of
mechanical sediment is to be distinguished from the transportation of materials in
solution. In so far as mineral matter is dissolved it becomes, so far as flowage is
concerned, a part of the stream. If the quantity dissolved were large it might
influence the mobility of the water, but the amount is usually too slight to influence
the flow sensibly.
The sediment transported by a stream is either rolled along its bottom or carried
in suspension at some higher level. The coarser materials (gravel and sand) are
carried chiefly in the former position, and the finer (silt and mud) largely in the
latter.
Transporting power and velocity.—The transporting power of running water
depends on its velocity. The formula expressing the relations between them is as
follows: Transporting power, t, varies as the sixth power of velocity, v, (tαv6); that
is, doubling the velocity of the stream increases its transporting power 64-fold.
Strictly speaking, this means that if a stream of given velocity is just able to move a
stone of a given size, a stream with double that velocity will be just able to move a
stone of the same shape 64 times as large as the first. This may be graphically
illustrated as follows: Let a current be supposed just able to move the cube a (Fig.
such a canyon has been cutting chiefly at its bottom. Ignoring its lateral corrasion,
which is slight, the valley which it would cut would have a width equal to its own.
This is illustrated by Fig. 96. Weathering in its broadest sense is largely responsible
for the width of such a valley, in so far as it exceeds the width of the stream. The
work of weathering, slope wash, etc., has been to get the material which originally
lay between a, b, and c down to the stream. The stream has then carried it away.
The above illustration would not apply to old and sluggish streams, for they, by
their meandering, widen their valleys independently of weathering.
Fig. 96.—Diagram of a valley the top of which is ten times the width of the stream.
Weathering is a part of erosion, but only a part. In so far as it is effected by
solution the process involves the transportation of that which is dissolved to some
other point. Transportation is also involved to some extent in the other processes of
weathering, but the central idea of the processes embraced under this term is the
loosening and disrupting of rock by which it is prepared for transportation.
Transportation.
The second element of erosion is transportation. The transportation of
mechanical sediment is to be distinguished from the transportation of materials in
solution. In so far as mineral matter is dissolved it becomes, so far as flowage is
concerned, a part of the stream. If the quantity dissolved were large it might
influence the mobility of the water, but the amount is usually too slight to influence
the flow sensibly.
The sediment transported by a stream is either rolled along its bottom or carried
in suspension at some higher level. The coarser materials (gravel and sand) are
carried chiefly in the former position, and the finer (silt and mud) largely in the
latter.
Transporting power and velocity.—The transporting power of running water
depends on its velocity. The formula expressing the relations between them is as
follows: Transporting power, t, varies as the sixth power of velocity, v, (tαv6); that
is, doubling the velocity of the stream increases its transporting power 64-fold.
Strictly speaking, this means that if a stream of given velocity is just able to move a
stone of a given size, a stream with double that velocity will be just able to move a
stone of the same shape 64 times as large as the first. This may be graphically
illustrated as follows: Let a current be supposed just able to move the cube a (Fig.
Page 166
97). If the current be doubled, twice as much water will strike the same surface
with twice the force in the same time; that is, the force exerted on the cube a will be
quadrupled. It will, therefore, be able not only to move the one cube, but it will be
able to move three other cubes (b, c, and d) besides (Fig. 98). The same current
against any other equal surface would also be able to move four small cubes, and
there are sixteen such surfaces on the face of the large cube (Fig. 99). It follows that
the dimension of the cube which the stream with the doubled velocity can move is
four times as great as that of the cube which the original current could move, and
the cubical contents of such a cube is 64 times as great as that of the first (64 = 26)
(Fig. 99). Swift streams, therefore, have enormously greater power of
transportation than sluggish ones. It does not necessarily follow that transportation
keeps pace with transporting power; that depends on the accessibility of materials
suitable for transportation. A stream of great transporting power, like the Niagara at
its rapids, may carry little sediment, because there is little to be had.
The velocity of a stream depends chiefly on three elements—its gradient, its
volume, and its load, (i.e., the sediment it is moving). The higher the gradient the
greater the volume, and the less the load the greater the velocity. The relation
between gradient and velocity is evident; that between volume and velocity is
illustrated by every stream in time of flood, when its rate of flow is greatly
increased. The relation between velocity and load is less obvious, but none the less
definite. Every particle of sediment carried by a stream makes a draught on its
energy, and energy expended in this way reduces the velocity. The draught on a
stream’s energy of a particle carried in suspension is measured by its mass into the
distance it would fall in a unit of time in still water. It follows that a large particle
makes a stronger draught on a stream’s energy than the same amount of material in
smaller pieces. It follows also that the comminution of sediment facilitates
transportation in much more than a simple ratio, for not only can a given amount of
energy carry more fine material than coarse, but a larger proportion of a stream’s
energy can be utilized in the transportation of the fine.
Fig. 97–99.—Diagrammatic representation of the effect of increased velocity on transporting power.
with twice the force in the same time; that is, the force exerted on the cube a will be
quadrupled. It will, therefore, be able not only to move the one cube, but it will be
able to move three other cubes (b, c, and d) besides (Fig. 98). The same current
against any other equal surface would also be able to move four small cubes, and
there are sixteen such surfaces on the face of the large cube (Fig. 99). It follows that
the dimension of the cube which the stream with the doubled velocity can move is
four times as great as that of the cube which the original current could move, and
the cubical contents of such a cube is 64 times as great as that of the first (64 = 26)
(Fig. 99). Swift streams, therefore, have enormously greater power of
transportation than sluggish ones. It does not necessarily follow that transportation
keeps pace with transporting power; that depends on the accessibility of materials
suitable for transportation. A stream of great transporting power, like the Niagara at
its rapids, may carry little sediment, because there is little to be had.
The velocity of a stream depends chiefly on three elements—its gradient, its
volume, and its load, (i.e., the sediment it is moving). The higher the gradient the
greater the volume, and the less the load the greater the velocity. The relation
between gradient and velocity is evident; that between volume and velocity is
illustrated by every stream in time of flood, when its rate of flow is greatly
increased. The relation between velocity and load is less obvious, but none the less
definite. Every particle of sediment carried by a stream makes a draught on its
energy, and energy expended in this way reduces the velocity. The draught on a
stream’s energy of a particle carried in suspension is measured by its mass into the
distance it would fall in a unit of time in still water. It follows that a large particle
makes a stronger draught on a stream’s energy than the same amount of material in
smaller pieces. It follows also that the comminution of sediment facilitates
transportation in much more than a simple ratio, for not only can a given amount of
energy carry more fine material than coarse, but a larger proportion of a stream’s
energy can be utilized in the transportation of the fine.
Fig. 97–99.—Diagrammatic representation of the effect of increased velocity on transporting power.
Page 167
How sediment is carried.—Coarse materials, such as gravel stones, are rolled
along the bottoms of the swift streams which carry them. Their movement is
effected by the impact of water. The same is true to a large extent of sand grains,
especially if they be coarse. So far as concerns the material rolled along the bottom
it is to be noted that a stream’s transporting power is dependent on the velocity of
the water at its bottom. This is much less than the surface, or even the average
velocity. The particles of fine sediments, such as silt and mud, are frequently
carried by streams quite above their bottoms, as shown by the roiliness of many
streams. A particle of mud is usually a small bit of mineral matter, the specific
gravity of which is two or three times that of water. Why does it not sink through
the water and come to rest at the bottom of the stream, or suffer transportation as
the gravel does?
A particle of sediment in running water
is obviously subject to two forces, that of
the current which tends to move it nearly
horizontally down-stream, and that of
gravity which tends to carry it to the bed
of the stream. In Fig. 100, the arrows ab
and ac represent respectively the relative
force of gravity and a current of 5 miles
per hour. As a result of these two forces Fig. 100.—Diagram to illustrate the relative
the particle would tend to descend in the strength of the two forces acting on a
particle in suspension. The arrows represent
general direction of ad, a line which the relative strength of the two forces when
represents the resultant of these forces, the stream’s velocity is 5 miles per hour. No
though not the exact path which a particle account is taken in the diagram of the
viscosity of the water, or of the acceleration
acted on by them would take in water. If a of velocity of fall.
river were the simple straightforward
current which it is popularly thought to be, a particle in suspension would reach its
bottom in the time it would take to sink through an equal depth of still water, for
the descent would be none the less certain and none the less prompt because of the
forward movement of the water. The current would simply be a factor in
determining the position of the particle when it reached the bottom, not the time of
reaching it. Very fine particles, like those of clay, though having the same specific
gravity as grains of sand, would sink less readily than coarser ones, because they
expose larger surfaces, relative to their mass, to the water through which they sink.
But even such particles, unless of extraordinary fineness, would presently reach the
bottom if acted on only by a horizontal current and gravity. Since even sediment
which is not of exceeding fineness is kept in suspension it is clear that some other
factor is involved. This is found, in part at least, in the subordinate upward currents
in a stream.
along the bottoms of the swift streams which carry them. Their movement is
effected by the impact of water. The same is true to a large extent of sand grains,
especially if they be coarse. So far as concerns the material rolled along the bottom
it is to be noted that a stream’s transporting power is dependent on the velocity of
the water at its bottom. This is much less than the surface, or even the average
velocity. The particles of fine sediments, such as silt and mud, are frequently
carried by streams quite above their bottoms, as shown by the roiliness of many
streams. A particle of mud is usually a small bit of mineral matter, the specific
gravity of which is two or three times that of water. Why does it not sink through
the water and come to rest at the bottom of the stream, or suffer transportation as
the gravel does?
A particle of sediment in running water
is obviously subject to two forces, that of
the current which tends to move it nearly
horizontally down-stream, and that of
gravity which tends to carry it to the bed
of the stream. In Fig. 100, the arrows ab
and ac represent respectively the relative
force of gravity and a current of 5 miles
per hour. As a result of these two forces Fig. 100.—Diagram to illustrate the relative
the particle would tend to descend in the strength of the two forces acting on a
particle in suspension. The arrows represent
general direction of ad, a line which the relative strength of the two forces when
represents the resultant of these forces, the stream’s velocity is 5 miles per hour. No
though not the exact path which a particle account is taken in the diagram of the
viscosity of the water, or of the acceleration
acted on by them would take in water. If a of velocity of fall.
river were the simple straightforward
current which it is popularly thought to be, a particle in suspension would reach its
bottom in the time it would take to sink through an equal depth of still water, for
the descent would be none the less certain and none the less prompt because of the
forward movement of the water. The current would simply be a factor in
determining the position of the particle when it reached the bottom, not the time of
reaching it. Very fine particles, like those of clay, though having the same specific
gravity as grains of sand, would sink less readily than coarser ones, because they
expose larger surfaces, relative to their mass, to the water through which they sink.
But even such particles, unless of extraordinary fineness, would presently reach the
bottom if acted on only by a horizontal current and gravity. Since even sediment
which is not of exceeding fineness is kept in suspension it is clear that some other
factor is involved. This is found, in part at least, in the subordinate upward currents
in a stream.
Page 168
Where a bowlder occurs in the bed of a stream (Fig. 101) the water which strikes
it is in part forced up over it. If there be many bowlders the process is frequently
repeated, and the number of upward currents is great. Any roughness will serve the
same purpose, and every stream’s bed is rough to a greater or less extent. Where
there are roughnesses at the sides of a channel, currents are started which flow from
them toward the center. The varying velocities of the different parts of a stream
serve a similar purpose. The curves in a river tend to give the water a rotatory
movement. A river is therefore to be looked upon not as a single straightforward
current, but as a multitude of currents, some rising from the bottom toward the top,
some descending from top to bottom, some diverging from the center toward the
sides, and some converging from the sides toward the center. The existence of these
subordinate currents is often evident from the boiling and eddying readily seen in
many streams. It is, of course, true that the sum of the upward currents is always
less than the sum of the downward, so that the aggregate motion of the water is
down slope; but it is also true that minor upward currents are common. Sediment in
suspension is held up chiefly by such currents, which, locally and temporarily,
overcome the effect of gravity. The particles in suspension are constantly tending to
fall, and frequently falling; but before they reach the bottom many of them are
seized and carried upward by the subordinate currents, only to sink and be carried
up again. Even if they reach the bottom, as they frequently do, they may be picked
up again. It is probable that every particle of sediment of such size that it would
sink readily in still water is dropped and picked up many times in the course of any
long river journey, and its periods of rest often exceed its periods of movement.
Fig. 101.—Diagram to illustrate the effect of bowlders, a and b, in a stream’s bed on the currents of
water impinging against them.
Independently of the subordinate currents, the different velocities of the different
parts of a stream tend to keep materials in suspension by exerting different
pressures on the different sides of suspended particles.[46]
River ice sometimes facilitates the transportation of débris which the water alone
could not carry. The ice freezes to bowlders in the banks of the streams, to those
which are partially submerged, and sometimes to those altogether submerged
beneath slight depths of water. When the ice breaks up in the spring such bowlders,
buoyed up by the ice, may be floated far down the stream. The influence of ice in
this connection is most considerable in high latitudes, but it is of consequence as far
south as Virginia, where the river deposits sometimes contain bowlders which the
it is in part forced up over it. If there be many bowlders the process is frequently
repeated, and the number of upward currents is great. Any roughness will serve the
same purpose, and every stream’s bed is rough to a greater or less extent. Where
there are roughnesses at the sides of a channel, currents are started which flow from
them toward the center. The varying velocities of the different parts of a stream
serve a similar purpose. The curves in a river tend to give the water a rotatory
movement. A river is therefore to be looked upon not as a single straightforward
current, but as a multitude of currents, some rising from the bottom toward the top,
some descending from top to bottom, some diverging from the center toward the
sides, and some converging from the sides toward the center. The existence of these
subordinate currents is often evident from the boiling and eddying readily seen in
many streams. It is, of course, true that the sum of the upward currents is always
less than the sum of the downward, so that the aggregate motion of the water is
down slope; but it is also true that minor upward currents are common. Sediment in
suspension is held up chiefly by such currents, which, locally and temporarily,
overcome the effect of gravity. The particles in suspension are constantly tending to
fall, and frequently falling; but before they reach the bottom many of them are
seized and carried upward by the subordinate currents, only to sink and be carried
up again. Even if they reach the bottom, as they frequently do, they may be picked
up again. It is probable that every particle of sediment of such size that it would
sink readily in still water is dropped and picked up many times in the course of any
long river journey, and its periods of rest often exceed its periods of movement.
Fig. 101.—Diagram to illustrate the effect of bowlders, a and b, in a stream’s bed on the currents of
water impinging against them.
Independently of the subordinate currents, the different velocities of the different
parts of a stream tend to keep materials in suspension by exerting different
pressures on the different sides of suspended particles.[46]
River ice sometimes facilitates the transportation of débris which the water alone
could not carry. The ice freezes to bowlders in the banks of the streams, to those
which are partially submerged, and sometimes to those altogether submerged
beneath slight depths of water. When the ice breaks up in the spring such bowlders,
buoyed up by the ice, may be floated far down the stream. The influence of ice in
this connection is most considerable in high latitudes, but it is of consequence as far
south as Virginia, where the river deposits sometimes contain bowlders which the
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unaided streams could not have carried. Ground ice sometimes forms about
bowlders in the bottoms of streams, especially in the quiet pools of turbulent rivers,
and floats them to the surface before the surface itself is frozen.[47] In the floods of
spring rivers often spread their ice widely over their flood-plains. It is sometimes
massed in constricted portions of valleys so as to form great dams, the breaking of
which is attended with great destruction.
Corrasion.
Abrasion.—The wear effected by running water is corrasion. So long as the
materials to be carried away are incoherent it is easy to see how running water
picks them up and carries them forward. The water which gathers in the
depressions on the slope of a cultivated field gathers earthy matter from the surface
over which it passes, even before it is concentrated into rills, and the rills continue
the process. Thus the loose materials of the surface are gathered at the very sources
of the streams, and the amount of sediment in the water after a heavy shower, even
at the head of the stream, may be great. The run-off from the slopes of any valley in
any part of its course likewise brings sediment to the stream, which gathers more
from its bed whereever it flows with sufficient velocity over incoherent material.
Streams also undercut their banks, and receive new load from the fall of the
overhanging material.
By far the larger part of the sediment acquired by a normal stream is made up of
material loosened in advance by the processes of weathering. The stream, or the
waters which get together to make the stream, find them ready-made; but rivers
frequently wear rock which is not weathered, for the principal valleys of the earth’s
surface are cut in solid rock, and many of them in rock of exceeding hardness. How
does the stream wear the solid rock?
When a stream flows over a rock bed, the wear which it accomplishes depends
chiefly on the character of the rock, the velocity of the stream, and the load it
carries. If the rock be stratified and in thin layers, and if these thin layers be broken
by numerous joints at high angles to the stratification planes, the impact of the
water of a clear stream of even moderate strength may be effective in dislodging
bits of the rock. This condition of things is often seen where streams run on beds of
shale or slate. If the rock be hard and without bedding-planes and joints, or if its
layers be thick and its joints few, clear water will be much less effective. If the
surface of the rock be rough, the mechanical action of a swift stream of clear water
might still produce some effect on it; but if massive hard rock presents a smooth
surface to a clear stream, the mechanical effect of even a swift current is slight.
This general principle is illustrated by the Niagara River. Just above the falls the
current is swift. When the river is essentially free from sediment, the surface of the
bowlders in the bottoms of streams, especially in the quiet pools of turbulent rivers,
and floats them to the surface before the surface itself is frozen.[47] In the floods of
spring rivers often spread their ice widely over their flood-plains. It is sometimes
massed in constricted portions of valleys so as to form great dams, the breaking of
which is attended with great destruction.
Corrasion.
Abrasion.—The wear effected by running water is corrasion. So long as the
materials to be carried away are incoherent it is easy to see how running water
picks them up and carries them forward. The water which gathers in the
depressions on the slope of a cultivated field gathers earthy matter from the surface
over which it passes, even before it is concentrated into rills, and the rills continue
the process. Thus the loose materials of the surface are gathered at the very sources
of the streams, and the amount of sediment in the water after a heavy shower, even
at the head of the stream, may be great. The run-off from the slopes of any valley in
any part of its course likewise brings sediment to the stream, which gathers more
from its bed whereever it flows with sufficient velocity over incoherent material.
Streams also undercut their banks, and receive new load from the fall of the
overhanging material.
By far the larger part of the sediment acquired by a normal stream is made up of
material loosened in advance by the processes of weathering. The stream, or the
waters which get together to make the stream, find them ready-made; but rivers
frequently wear rock which is not weathered, for the principal valleys of the earth’s
surface are cut in solid rock, and many of them in rock of exceeding hardness. How
does the stream wear the solid rock?
When a stream flows over a rock bed, the wear which it accomplishes depends
chiefly on the character of the rock, the velocity of the stream, and the load it
carries. If the rock be stratified and in thin layers, and if these thin layers be broken
by numerous joints at high angles to the stratification planes, the impact of the
water of a clear stream of even moderate strength may be effective in dislodging
bits of the rock. This condition of things is often seen where streams run on beds of
shale or slate. If the rock be hard and without bedding-planes and joints, or if its
layers be thick and its joints few, clear water will be much less effective. If the
surface of the rock be rough, the mechanical action of a swift stream of clear water
might still produce some effect on it; but if massive hard rock presents a smooth
surface to a clear stream, the mechanical effect of even a swift current is slight.
This general principle is illustrated by the Niagara River. Just above the falls the
current is swift. When the river is essentially free from sediment, the surface of the
Page 170
limestone near the bank beneath it is sometimes distinctly green from the presence
of the one-celled plants (fresh-water algæ) which grow upon it. The whole force of
the mighty torrent is not able to sweep them from their moorings. Were the stream
supplied with a tithe of the sand which it is capable of carrying, it would not take
many hours, and perhaps not many minutes, to remove the last trace of vegetation.
This illustration furnishes a clue to the method by which the erosion of solid rock in
a stream’s bed is effected.
It has been seen that the ingathering waters which make a stream often have
abundant sediment before they reach well-defined stream channels, and that the
streams continue to gather sediment whereever their beds are composed of material
which is readily detached. The sediments which the stream carries are the tools
with which it works. Without them it is relatively impotent, so far as the abrasion of
solid rock is concerned; with them, it may wear any rock over which it passes (Fig.
102).
We have next to inquire the methods by which running water uses its tools in the
excavation of valleys. When gravel is rolled along in the channel of a stream there
is friction between it and the bed over which it moves. If the pebbles be as hard as
the bed over which they are rolled their movement must result in its wear, and even
if they be softer more or less wear takes place. As the moving stones wear the rock
of the stream’s bed they are themselves worn by impact with it and with one
another. In all cases the softer material suffers the more rapid wear. The first effect
of wear on materials in transportation is the reduction of their rugosities of surface.
The projecting points and sharp angles are worn off, and the stones are reduced to
rounded water-worn forms. The particles broken off make grains of sand, or, if very
fine, particles of silt or mud. Even after a stone has been rounded it is subject to
further wear and reduction, and in the course of time may be literally worn out.
The sediment carried in suspension, as well as that rolled along the bottom, may
wear the rock bed of a stream. When a grain of sand in suspension escapes from an
upward moving current it may not sink quietly. If it be caught by a downward
current it may be made to strike a blow on the bed of the stream, and the effect of
the blow is to wear the surface which receives it. The larger the grain and the
stronger the current the greater the wear.
of the one-celled plants (fresh-water algæ) which grow upon it. The whole force of
the mighty torrent is not able to sweep them from their moorings. Were the stream
supplied with a tithe of the sand which it is capable of carrying, it would not take
many hours, and perhaps not many minutes, to remove the last trace of vegetation.
This illustration furnishes a clue to the method by which the erosion of solid rock in
a stream’s bed is effected.
It has been seen that the ingathering waters which make a stream often have
abundant sediment before they reach well-defined stream channels, and that the
streams continue to gather sediment whereever their beds are composed of material
which is readily detached. The sediments which the stream carries are the tools
with which it works. Without them it is relatively impotent, so far as the abrasion of
solid rock is concerned; with them, it may wear any rock over which it passes (Fig.
102).
We have next to inquire the methods by which running water uses its tools in the
excavation of valleys. When gravel is rolled along in the channel of a stream there
is friction between it and the bed over which it moves. If the pebbles be as hard as
the bed over which they are rolled their movement must result in its wear, and even
if they be softer more or less wear takes place. As the moving stones wear the rock
of the stream’s bed they are themselves worn by impact with it and with one
another. In all cases the softer material suffers the more rapid wear. The first effect
of wear on materials in transportation is the reduction of their rugosities of surface.
The projecting points and sharp angles are worn off, and the stones are reduced to
rounded water-worn forms. The particles broken off make grains of sand, or, if very
fine, particles of silt or mud. Even after a stone has been rounded it is subject to
further wear and reduction, and in the course of time may be literally worn out.
The sediment carried in suspension, as well as that rolled along the bottom, may
wear the rock bed of a stream. When a grain of sand in suspension escapes from an
upward moving current it may not sink quietly. If it be caught by a downward
current it may be made to strike a blow on the bed of the stream, and the effect of
the blow is to wear the surface which receives it. The larger the grain and the
stronger the current the greater the wear.
Page 171
Fig. 102.—Some of the tools with which a stream works. The cobbles and bowlders have been shifted
by the stream in its flow. Other stones and bowlders now in transit cause the ripples in the stream.
The Chelan River, Wash., just above its junction with the Columbia. (Willis, U. S. Geol. Surv.)
The ceaseless repetition of the blows struck by the material in suspension, or
rolled on its bottom, hour after hour, day after day, and year after year, will
accomplish sensible results. In the long course of the ages this process has
excavated deep valleys. Concomitant processes are largely concerned in making
valleys wide, but the depth of valleys cut in solid rock is chiefly the result of the
impact and friction of the sediment in transportation.
The wear effected in this way is not proportional to the number of blows struck.
Since every pebble and every grain of sand carried diminishes the velocity of a
stream, and since with diminished velocity the force of the blows struck is
diminished, it follows that the blows may become so weak, as the result of their
multiplication, as to be ineffective. The larger the load, therefore, which the stream
carries, the more the tools with which it has to work, but the less effectively can it
use them; and the load may be so far increased as to destroy its corrasive power
altogether. On the other hand, the smaller the load of the stream the greater its
velocity and the more effectively will its tools be used; but their number may be so
far reduced that their aggregate effect is slight. To accomplish the greatest results
on a bed of solid rock a stream must have tools to work with, but must not be so
heavily burdened as to interfere with its effective use of them.
Whatever the cause of their unequal velocities swift and slow streams corrade
their valleys differently. The erosion of a swift stream is chiefly at the bottom of its
by the stream in its flow. Other stones and bowlders now in transit cause the ripples in the stream.
The Chelan River, Wash., just above its junction with the Columbia. (Willis, U. S. Geol. Surv.)
The ceaseless repetition of the blows struck by the material in suspension, or
rolled on its bottom, hour after hour, day after day, and year after year, will
accomplish sensible results. In the long course of the ages this process has
excavated deep valleys. Concomitant processes are largely concerned in making
valleys wide, but the depth of valleys cut in solid rock is chiefly the result of the
impact and friction of the sediment in transportation.
The wear effected in this way is not proportional to the number of blows struck.
Since every pebble and every grain of sand carried diminishes the velocity of a
stream, and since with diminished velocity the force of the blows struck is
diminished, it follows that the blows may become so weak, as the result of their
multiplication, as to be ineffective. The larger the load, therefore, which the stream
carries, the more the tools with which it has to work, but the less effectively can it
use them; and the load may be so far increased as to destroy its corrasive power
altogether. On the other hand, the smaller the load of the stream the greater its
velocity and the more effectively will its tools be used; but their number may be so
far reduced that their aggregate effect is slight. To accomplish the greatest results
on a bed of solid rock a stream must have tools to work with, but must not be so
heavily burdened as to interfere with its effective use of them.
Whatever the cause of their unequal velocities swift and slow streams corrade
their valleys differently. The erosion of a swift stream is chiefly at the bottom of its
Page 172
channel. The sluggish stream lowers its channel less rapidly, while lateral erosion is
relatively more important. The result is that slow streams increase the width of their
valleys more than the depth, while swift streams increase the depth more than the
width. It follows that slow streams develop flats, while swift ones do not. Not only
is a slow stream more likely to have a flat, and therefore a better chance to
meander, but it is more likely to take advantage of opportunities in this line, for a
slow stream gets out of the way for such obstacles as it may encounter, while a
swift stream is much more likely to get obstacles out of its way.
Special phases of corrasion are introduced where waterfalls and other
peculiarities dependent on inequalities of rock resistance occur.
Solution.—In most cases the solution effected by a stream is much less
important than its mechanical work. Only when conditions are unfavorable to the
latter, is solution the chief factor in the excavation of a valley. This may be the case
where a stream’s bed is over soluble rock, such as limestone, and where the stream
is clear, or its gradient so low that its current is sluggish. The solvent power of
water is not influenced by the presence of sediment, though the presence of
sediment offers the water a greater surface on which to work.
relatively more important. The result is that slow streams increase the width of their
valleys more than the depth, while swift streams increase the depth more than the
width. It follows that slow streams develop flats, while swift ones do not. Not only
is a slow stream more likely to have a flat, and therefore a better chance to
meander, but it is more likely to take advantage of opportunities in this line, for a
slow stream gets out of the way for such obstacles as it may encounter, while a
swift stream is much more likely to get obstacles out of its way.
Special phases of corrasion are introduced where waterfalls and other
peculiarities dependent on inequalities of rock resistance occur.
Solution.—In most cases the solution effected by a stream is much less
important than its mechanical work. Only when conditions are unfavorable to the
latter, is solution the chief factor in the excavation of a valley. This may be the case
where a stream’s bed is over soluble rock, such as limestone, and where the stream
is clear, or its gradient so low that its current is sluggish. The solvent power of
water is not influenced by the presence of sediment, though the presence of
sediment offers the water a greater surface on which to work.
Page 173
CONDITIONS AFFECTING THE RATE OF EROSION.
In considering the rate of erosion, both the work of the stream in its
valley and that of the general run-off are to be considered. The conditions
which favor the most rapid erosion in a stream’s channel are not necessarily
those which determine most rapid degradation in the basin outside of the
valley.
The Influence of Declivity.
In general the greater the declivity the more rapid the rate of erosion,
whether in the stream’s channel or on the slopes above it. The truth of this
conclusion is illustrated by the great erosive power of swift streams as
compared with slow ones.
It does not follow, however, that high declivity favors each element of
erosion. The effect of declivity on weathering is far from simple. For
example, great declivity, by allowing more of the rainfall to flow off over
the surface, and by causing it to flow off more promptly, restricts the work
of solution, and therefore of decomposition, both at the surface and beneath
it. High declivity is also unfavorable to the growth of vegetation, and so to
the wedge-work of roots. On the other hand, a given amount of wedge-work
of roots and ice is more effective where the slope is steep than where it is
gentle, for such materials as are loosened descend the slopes more readily.
The prompt removal of weathered materials, by exposing fresh surfaces of
rock, accelerates weathering. The total amount of weathering may therefore
not be diminished by the increase of slope, even though certain of its
processes are hindered.
The effect of high declivity on transportation, the second element of
erosion, is too patent to need explanation.
Corrasion likewise is favored by high declivity, for the abrasive power of
a stream increases as the square of its velocity. With corrasive power
increased, corrasion will also be increased if the water has tools to work
with. Since high declivity greatly increases both the transporting and the
corrasive power of running water, and favors certain elements of
weathering, it is clear that the aggregate effect of high declivity is to favor
In considering the rate of erosion, both the work of the stream in its
valley and that of the general run-off are to be considered. The conditions
which favor the most rapid erosion in a stream’s channel are not necessarily
those which determine most rapid degradation in the basin outside of the
valley.
The Influence of Declivity.
In general the greater the declivity the more rapid the rate of erosion,
whether in the stream’s channel or on the slopes above it. The truth of this
conclusion is illustrated by the great erosive power of swift streams as
compared with slow ones.
It does not follow, however, that high declivity favors each element of
erosion. The effect of declivity on weathering is far from simple. For
example, great declivity, by allowing more of the rainfall to flow off over
the surface, and by causing it to flow off more promptly, restricts the work
of solution, and therefore of decomposition, both at the surface and beneath
it. High declivity is also unfavorable to the growth of vegetation, and so to
the wedge-work of roots. On the other hand, a given amount of wedge-work
of roots and ice is more effective where the slope is steep than where it is
gentle, for such materials as are loosened descend the slopes more readily.
The prompt removal of weathered materials, by exposing fresh surfaces of
rock, accelerates weathering. The total amount of weathering may therefore
not be diminished by the increase of slope, even though certain of its
processes are hindered.
The effect of high declivity on transportation, the second element of
erosion, is too patent to need explanation.
Corrasion likewise is favored by high declivity, for the abrasive power of
a stream increases as the square of its velocity. With corrasive power
increased, corrasion will also be increased if the water has tools to work
with. Since high declivity greatly increases both the transporting and the
corrasive power of running water, and favors certain elements of
weathering, it is clear that the aggregate effect of high declivity is to favor
Page 174
erosion, whether in the channel of the stream or on the general surface of its
drainage basin.
The Influence of Rock.
The physical constitution, the chemical composition, and the stratigraphy
of a rock formation, influence the rate at which it may be broken up and
carried away. Clastic or fragmental rocks are usually stratified and made up
of cemented pebbles (conglomerate), sand grains (sandstone), or particles of
mud (shale). Igneous rocks, such as granite, are massive instead of
stratified, and are usually made up of great numbers of interlocking crystals
which bind one another together. Some crystalline rocks, such as schists,
though not stratified, possess cleavage, which has much the effect of
stratification, so far as erosion is concerned. All rocks are affected by
systems of more or less nearly vertical cracks called joints. All these
structures have their influence upon the rate of degradation.
Physical constitution.—Clastic rocks may be firmly cemented, or their
constituents may be loosely bound together. The less the coherence the
more ready the disintegration, and the finer the particles the more easily are
they carried away. When the particles in transportation are angular they
effect more wear on the bed over which they move, and on one another,
than when they are round. The difference is great where the particles are
large, and little where they are very small. If the materials carried be harder
than the bed over which they pass, corrasion of the latter is favored.
Chemical composition.—Something also depends on the chemical
composition of the rock, since this affects its solubility, and therefore its
rate of decomposition. The more soluble the rock the larger the proportion
of it which will be taken away in solution; but it does not follow that the
most soluble rock will be most rapidly eroded, since the rate of erosion
depends on abrasion as well as solution, and a rock which is readily soluble,
as rocks go, may be less easily abraded than a rock which is made of
discrete and insoluble particles bound together by a soluble cement. In such
rocks, for example a sandstone in which the grains are cemented together
by lime carbonate, the solution of the cement sets free a considerable
quantity of sand, so that a small amount of solution prepares a large amount
of sediment for removal. A stream might cut its valley much more rapidly in
such a sandstone than in a compact limestone, though the latter is, as a
drainage basin.
The Influence of Rock.
The physical constitution, the chemical composition, and the stratigraphy
of a rock formation, influence the rate at which it may be broken up and
carried away. Clastic or fragmental rocks are usually stratified and made up
of cemented pebbles (conglomerate), sand grains (sandstone), or particles of
mud (shale). Igneous rocks, such as granite, are massive instead of
stratified, and are usually made up of great numbers of interlocking crystals
which bind one another together. Some crystalline rocks, such as schists,
though not stratified, possess cleavage, which has much the effect of
stratification, so far as erosion is concerned. All rocks are affected by
systems of more or less nearly vertical cracks called joints. All these
structures have their influence upon the rate of degradation.
Physical constitution.—Clastic rocks may be firmly cemented, or their
constituents may be loosely bound together. The less the coherence the
more ready the disintegration, and the finer the particles the more easily are
they carried away. When the particles in transportation are angular they
effect more wear on the bed over which they move, and on one another,
than when they are round. The difference is great where the particles are
large, and little where they are very small. If the materials carried be harder
than the bed over which they pass, corrasion of the latter is favored.
Chemical composition.—Something also depends on the chemical
composition of the rock, since this affects its solubility, and therefore its
rate of decomposition. The more soluble the rock the larger the proportion
of it which will be taken away in solution; but it does not follow that the
most soluble rock will be most rapidly eroded, since the rate of erosion
depends on abrasion as well as solution, and a rock which is readily soluble,
as rocks go, may be less easily abraded than a rock which is made of
discrete and insoluble particles bound together by a soluble cement. In such
rocks, for example a sandstone in which the grains are cemented together
by lime carbonate, the solution of the cement sets free a considerable
quantity of sand, so that a small amount of solution prepares a large amount
of sediment for removal. A stream might cut its valley much more rapidly in
such a sandstone than in a compact limestone, though the latter is, as a
Page 175
whole, the more soluble. The constituent minerals of crystalline rocks resist
solution and decay unequally, and when any one is dissolved or
decomposed the rock crumbles and the less soluble constituents are ready
for removal by mechanical means. So long as the material loosened by
disintegration is removed, chemical heterogeneity favors erosion; but if the
loosened débris is not removed erosion is not favored by chemical
heterogeneity. In such a case erosion would be most rapid where the rock
was most soluble.
Structure.—The structure of the rock has much to do with the rate of its
erosion. Other things being equal, stratified rock is more readily eroded
than massive rock, since stratification-planes are planes of cleavage, and
therefore of weakness. Taking advantage of these planes the water has less
breaking to perform to reduce the material to a transportable condition. For
the same reason a thin-bedded formation is more easily eroded than a thick-
bedded one.
Fig. 103 and 104.—Diagrams to illustrate the fact that a stream crosses many more
cleavage-planes when the beds of rock are inclined than when they are horizontal.
The beds of stratified rock may be horizontal, vertical, or inclined, and
inclined strata may stand at any angle between horizontality and verticality.
In indurated formations the rate of erosion is influenced both by the
position of the strata and by the relation of the direction of the flowing
water to their dip and strike. On the whole the strata which are horizontal,
or but slightly inclined, are probably less favorable for rapid erosion than
those which are vertical or inclined at considerable angles. This is at least
true where the layers are of uniform hardness and the joints infrequent.
Horizontal strata expose fewer cleavage planes to the water flowing over
them than strata in any other position. In Fig. 103 the stream which has the
profile ad crosses bedding-planes at b and c. In Fig. 104, where the beds dip
up-stream, many more division-planes are crossed in the same distance.
Since bedding-planes are planes of weakness, it follows that horizontal and
solution and decay unequally, and when any one is dissolved or
decomposed the rock crumbles and the less soluble constituents are ready
for removal by mechanical means. So long as the material loosened by
disintegration is removed, chemical heterogeneity favors erosion; but if the
loosened débris is not removed erosion is not favored by chemical
heterogeneity. In such a case erosion would be most rapid where the rock
was most soluble.
Structure.—The structure of the rock has much to do with the rate of its
erosion. Other things being equal, stratified rock is more readily eroded
than massive rock, since stratification-planes are planes of cleavage, and
therefore of weakness. Taking advantage of these planes the water has less
breaking to perform to reduce the material to a transportable condition. For
the same reason a thin-bedded formation is more easily eroded than a thick-
bedded one.
Fig. 103 and 104.—Diagrams to illustrate the fact that a stream crosses many more
cleavage-planes when the beds of rock are inclined than when they are horizontal.
The beds of stratified rock may be horizontal, vertical, or inclined, and
inclined strata may stand at any angle between horizontality and verticality.
In indurated formations the rate of erosion is influenced both by the
position of the strata and by the relation of the direction of the flowing
water to their dip and strike. On the whole the strata which are horizontal,
or but slightly inclined, are probably less favorable for rapid erosion than
those which are vertical or inclined at considerable angles. This is at least
true where the layers are of uniform hardness and the joints infrequent.
Horizontal strata expose fewer cleavage planes to the water flowing over
them than strata in any other position. In Fig. 103 the stream which has the
profile ad crosses bedding-planes at b and c. In Fig. 104, where the beds dip
up-stream, many more division-planes are crossed in the same distance.
Since bedding-planes are planes of weakness, it follows that horizontal and
Page 176
nearly horizontal strata are not, under ordinary conditions of erosion, in a
position favorable for most rapid wear. When strata are horizontal, it makes
no difference which way the stream runs, for the current sustains the same
relation to the cleavage-planes whatever its course.
In the case of incoherent material the position of the beds, or even their
existence, has little influence on the rate of erosion. Such formations are
weak in all directions, not simply along bedding-planes.
When the strata are vertical,
three distinct cases may arise (Fig.
105). The stream may flow (1)
with the strike (aa); (2) at right
angles to the strike (bb); or (3)
oblique to it (cc) at any angle
whatsoever. It is perhaps not
possible to say which of these
positions is most favorable for
erosion, for the character of the
rock, the thickness of its layers, its
Fig. 105.—Diagram to illustrate the various
relations a stream may sustain to the outcrop
ability to stand with steep slopes,
of vertical layers of rock. and the strength of the currents
concerned, would influence the
result. A stream which flows at right angles to the strike (bb, Fig. 105)
would cross more cleavage-planes in a given distance than a stream flowing
in any other direction, and would strike the outcropping edges of layers at
the angle of greatest advantage. A stream flowing along the strike (aa), on
the other hand, has better opportunity to sink its channel on cleavage-
planes, and the current oblique to the strike (cc), has some of the advantages
of each of the others.
When the strata are inclined five cases may arise. (1) The stream may be
parallel to the strike (aa, Fig. 106), when it makes no difference which way
the current flows; it may be at right angles to the strike (bb′), and (2)
flowing with the dip (toward b′), or (3) against it (toward b); it may be
oblique to the strike, and flowing (4) in the general direction of dip (toward
c′); or (5) in the opposite direction (toward c). As before, the stream flowing
at right angles to the strike would cross the largest number of layers in a
given distance, and so have an opportunity to take advantage of more
position favorable for most rapid wear. When strata are horizontal, it makes
no difference which way the stream runs, for the current sustains the same
relation to the cleavage-planes whatever its course.
In the case of incoherent material the position of the beds, or even their
existence, has little influence on the rate of erosion. Such formations are
weak in all directions, not simply along bedding-planes.
When the strata are vertical,
three distinct cases may arise (Fig.
105). The stream may flow (1)
with the strike (aa); (2) at right
angles to the strike (bb); or (3)
oblique to it (cc) at any angle
whatsoever. It is perhaps not
possible to say which of these
positions is most favorable for
erosion, for the character of the
rock, the thickness of its layers, its
Fig. 105.—Diagram to illustrate the various
relations a stream may sustain to the outcrop
ability to stand with steep slopes,
of vertical layers of rock. and the strength of the currents
concerned, would influence the
result. A stream which flows at right angles to the strike (bb, Fig. 105)
would cross more cleavage-planes in a given distance than a stream flowing
in any other direction, and would strike the outcropping edges of layers at
the angle of greatest advantage. A stream flowing along the strike (aa), on
the other hand, has better opportunity to sink its channel on cleavage-
planes, and the current oblique to the strike (cc), has some of the advantages
of each of the others.
When the strata are inclined five cases may arise. (1) The stream may be
parallel to the strike (aa, Fig. 106), when it makes no difference which way
the current flows; it may be at right angles to the strike (bb′), and (2)
flowing with the dip (toward b′), or (3) against it (toward b); it may be
oblique to the strike, and flowing (4) in the general direction of dip (toward
c′); or (5) in the opposite direction (toward c). As before, the stream flowing
at right angles to the strike would cross the largest number of layers in a
given distance, and so have an opportunity to take advantage of more
Page 177
cleavage-planes than a stream in
any other position. But in the case
of inclined strata a new element
enters into the problem. When the
stream flows parallel to the strike,
the valley which is in process of
deepening is not sunk vertically,
but is shifted more or less in the
direction of the dip (Fig. 107).
This is called monoclinal shifting.
The result is that there is a
constant tendency to undermine Fig. 106.—Diagram to illustrate the various
relations a stream may sustain to the
(sap) the valley bluff on the down- outcrops of inclined layers of rock.
dip side, and this process of
sapping will, according to its rate, accelerate the growth of the valley,
especially in width. Monoclinal shifting is favored by the presence of a hard
layer (H), as shown in Fig. 107, if this stratum is the bed of the stream.
In the second and third cases
mentioned above, the only difference is
in the angle at which the current strikes
the outcropping edges of layers and
laminæ. The mechanical advantage is
with the stream which flows with the
Fig. 107.—Diagram to illustrate
monoclinal shifting. The valley abc, as
dip. In the fourth and fifth cases
seen in cross-section, becomes deb, as something will depend on the angle
the stream lowers its channel. which the stream’s course makes with
the strike. In all these cases, as in those where the strata are vertical, much
will depend on the thickness and resistance of the layers and on the strength
of the currents concerned.
The Influence of Climate.
Climate has both a direct and an indirect effect on erosion. Its direct
influence is through precipitation, evaporation, changes of temperature, and
wind; its indirect, through vegetation. Like declivity and rock structure,
climate does not affect all elements of erosion equally.
any other position. But in the case
of inclined strata a new element
enters into the problem. When the
stream flows parallel to the strike,
the valley which is in process of
deepening is not sunk vertically,
but is shifted more or less in the
direction of the dip (Fig. 107).
This is called monoclinal shifting.
The result is that there is a
constant tendency to undermine Fig. 106.—Diagram to illustrate the various
relations a stream may sustain to the
(sap) the valley bluff on the down- outcrops of inclined layers of rock.
dip side, and this process of
sapping will, according to its rate, accelerate the growth of the valley,
especially in width. Monoclinal shifting is favored by the presence of a hard
layer (H), as shown in Fig. 107, if this stratum is the bed of the stream.
In the second and third cases
mentioned above, the only difference is
in the angle at which the current strikes
the outcropping edges of layers and
laminæ. The mechanical advantage is
with the stream which flows with the
Fig. 107.—Diagram to illustrate
monoclinal shifting. The valley abc, as
dip. In the fourth and fifth cases
seen in cross-section, becomes deb, as something will depend on the angle
the stream lowers its channel. which the stream’s course makes with
the strike. In all these cases, as in those where the strata are vertical, much
will depend on the thickness and resistance of the layers and on the strength
of the currents concerned.
The Influence of Climate.
Climate has both a direct and an indirect effect on erosion. Its direct
influence is through precipitation, evaporation, changes of temperature, and
wind; its indirect, through vegetation. Like declivity and rock structure,
climate does not affect all elements of erosion equally.
Page 178
The chief elements of climate are temperature, moisture, and atmospheric
movements; the principal factors which influence it are latitude, altitude,
distance from the sea, direction of prevailing winds, and topographic
relations.
The effects of variations in temperature on rock weathering have already
been discussed (p. 43). They are chiefly mechanical, and are seen at their
best where the daily range is great.
High temperature favors chemical action, and the weathering of rock by
decomposition is at its best in the presence of abundant moisture in regions
where the temperature is uniformly high. Furthermore, a warm moist
climate favors the growth of vegetation, the decay of which supplies the
water with organic acids which greatly increase its solvent power. The
climatic conditions favoring mechanical weathering are therefore different
from those favoring chemical weathering. High temperature and abundant
moisture and vegetation are found in many tropical regions, and here the
rock is often decomposed to greater depths, on the whole, than in high
latitudes. How far this is the result of rapid weathering, and how far of slow
removal, due in part to the protective influence of the plants, cannot be
affirmed. If the weathered material is not removed, it will presently become
a mantle thick enough to retard the processes which brought it into
existence.
So long as the water of the surface and that in the soil remains unfrozen,
temperature affects neither corrasion nor transportation. But in middle and
high latitudes the surface is frozen for some part of each year. During this
time corrasion is at a minimum, for although the streams continue to flow
there is relatively little water running over the surface outside the drainage
channels, and that little is relatively ineffective. Under some conditions,
therefore, temperature affects both corrasion and transportation.
The humidity of the atmosphere has an influence even more important
than that of temperature on the rate of erosion, and its influence is exerted
on each of the elements of that complex process. A moist atmosphere favors
oxidation, carbonation, hydration, and the growth of vegetation, all of
which promote certain phases of rock weathering. On the other hand,
humidity tends to prevent sudden and considerable variations in
temperature, thus checking the weathering effected by this means.
movements; the principal factors which influence it are latitude, altitude,
distance from the sea, direction of prevailing winds, and topographic
relations.
The effects of variations in temperature on rock weathering have already
been discussed (p. 43). They are chiefly mechanical, and are seen at their
best where the daily range is great.
High temperature favors chemical action, and the weathering of rock by
decomposition is at its best in the presence of abundant moisture in regions
where the temperature is uniformly high. Furthermore, a warm moist
climate favors the growth of vegetation, the decay of which supplies the
water with organic acids which greatly increase its solvent power. The
climatic conditions favoring mechanical weathering are therefore different
from those favoring chemical weathering. High temperature and abundant
moisture and vegetation are found in many tropical regions, and here the
rock is often decomposed to greater depths, on the whole, than in high
latitudes. How far this is the result of rapid weathering, and how far of slow
removal, due in part to the protective influence of the plants, cannot be
affirmed. If the weathered material is not removed, it will presently become
a mantle thick enough to retard the processes which brought it into
existence.
So long as the water of the surface and that in the soil remains unfrozen,
temperature affects neither corrasion nor transportation. But in middle and
high latitudes the surface is frozen for some part of each year. During this
time corrasion is at a minimum, for although the streams continue to flow
there is relatively little water running over the surface outside the drainage
channels, and that little is relatively ineffective. Under some conditions,
therefore, temperature affects both corrasion and transportation.
The humidity of the atmosphere has an influence even more important
than that of temperature on the rate of erosion, and its influence is exerted
on each of the elements of that complex process. A moist atmosphere favors
oxidation, carbonation, hydration, and the growth of vegetation, all of
which promote certain phases of rock weathering. On the other hand,
humidity tends to prevent sudden and considerable variations in
temperature, thus checking the weathering effected by this means.
Page 179
Precipitation, the most important single factor in determining the rate of
erosion, is dependent on atmospheric humidity. Its amount, its kind (rain or
snow), and its distribution in time, are the elements which determine its
effectiveness in any given place.
Other things being equal the greater the amount of precipitation the more
rapid the corrasion and transportation. Much, however, depends on its
distribution in time. A given amount of rainfall may be distributed equally
through the year, or it may fall during a wet season only. The maximum
inequality of distribution would occur if all the rainfall of a given period
were concentrated in a single shower. With such concentration the volume
of water flowing off over the surface immediately after the down-pour
would be greater than under any other conditions of precipitation, and since
velocity is increased with volume, and erosive power with velocity, it
follows that the erosive power of a given amount of water would be greater
under these circumstances than under any other. Furthermore, a larger
proportion of the precipitation would run off over the surface under these
circumstances than under any other, for less of it would sink beneath the
surface and less would be evaporated. If erosive power and rate of erosion
were equal terms, this would therefore be the condition for greatest erosion;
but erosive power and rate of erosion do not always correspond. If the water
falling in this way could get hold of all the material it could carry, extreme
concentration of precipitation would be the condition favorable for most
rapid erosion. But if the amount of available material for transportation is
slight, a large part of the force of the water could not be utilized in erosion.
It follows that if there were a large amount of disintegrated material on the
surface, erosion would be greater the greater the concentration of
precipitation. If, on the other hand, there were but little disintegrated
material on the surface, frequent showers, with intervening periods when
conditions were favorable for weathering, that is, for preparing material for
transportation, might be more favorable for rapid erosion. While the total
energy of running water available for erosion under these conditions would
be less than before, there might in the long run be more material for
transport; for weathering in the presence of moisture, and all that goes with
it, might be more effective in preparing material for transportation, than
weathering during the long periods of drought which would occur if the
precipitation were concentrated to its maximum. Temperature favoring, the
uniform distribution of moisture through the year would allow the growth
erosion, is dependent on atmospheric humidity. Its amount, its kind (rain or
snow), and its distribution in time, are the elements which determine its
effectiveness in any given place.
Other things being equal the greater the amount of precipitation the more
rapid the corrasion and transportation. Much, however, depends on its
distribution in time. A given amount of rainfall may be distributed equally
through the year, or it may fall during a wet season only. The maximum
inequality of distribution would occur if all the rainfall of a given period
were concentrated in a single shower. With such concentration the volume
of water flowing off over the surface immediately after the down-pour
would be greater than under any other conditions of precipitation, and since
velocity is increased with volume, and erosive power with velocity, it
follows that the erosive power of a given amount of water would be greater
under these circumstances than under any other. Furthermore, a larger
proportion of the precipitation would run off over the surface under these
circumstances than under any other, for less of it would sink beneath the
surface and less would be evaporated. If erosive power and rate of erosion
were equal terms, this would therefore be the condition for greatest erosion;
but erosive power and rate of erosion do not always correspond. If the water
falling in this way could get hold of all the material it could carry, extreme
concentration of precipitation would be the condition favorable for most
rapid erosion. But if the amount of available material for transportation is
slight, a large part of the force of the water could not be utilized in erosion.
It follows that if there were a large amount of disintegrated material on the
surface, erosion would be greater the greater the concentration of
precipitation. If, on the other hand, there were but little disintegrated
material on the surface, frequent showers, with intervening periods when
conditions were favorable for weathering, that is, for preparing material for
transportation, might be more favorable for rapid erosion. While the total
energy of running water available for erosion under these conditions would
be less than before, there might in the long run be more material for
transport; for weathering in the presence of moisture, and all that goes with
it, might be more effective in preparing material for transportation, than
weathering during the long periods of drought which would occur if the
precipitation were concentrated to its maximum. Temperature favoring, the
uniform distribution of moisture through the year would allow the growth
Page 180
of vegetation, which, although favoring some processes of weathering,
retards erosion in general. While therefore it is not possible to say what
distribution of rainfall favors most rapid erosion without knowing the
nature of the surface on which it is to fall, enough has been said to show
that the problem is by no means a simple one. Some of the most striking
phases of topography developed by erosion, such as those of the Bad Lands
(Figs. 75 to 78, and 108), are developed where the rainfall is unequally
distributed in time, and too slight or too infrequent to support abundant
vegetation.
Fig. 108.—Bad-land topography developed under conditions of aridity and unequal
distribution of rainfall. Slope of Pinal Mountains, Ariz. (Ransome, U. S. Geol. Surv.)
During its fall, and immediately after, rain is more effective than an equal
amount of snow; but the snow may be accumulated through a considerable
period of the year, and then melted rapidly, when it has an effect
comparable to that which would be produced by the concentration of the
rainfall into a limited period of the year. If the ground beneath be frozen
when the snow melts (and this is often the case) the erosion accomplished
by the resulting water will be diminished.
Except in dry regions, where wind-work sometimes exceeds water-work,
the movements of the atmosphere are of less importance directly than
precipitation in determining the rate of erosion. But even in regions which
are not arid the winds have much to do with the rate of evaporation and the
distribution of rainfall, so that their indirect effect is great. Even their direct
effects in moist climates are not to be lost sight of, for even here the surface
retards erosion in general. While therefore it is not possible to say what
distribution of rainfall favors most rapid erosion without knowing the
nature of the surface on which it is to fall, enough has been said to show
that the problem is by no means a simple one. Some of the most striking
phases of topography developed by erosion, such as those of the Bad Lands
(Figs. 75 to 78, and 108), are developed where the rainfall is unequally
distributed in time, and too slight or too infrequent to support abundant
vegetation.
Fig. 108.—Bad-land topography developed under conditions of aridity and unequal
distribution of rainfall. Slope of Pinal Mountains, Ariz. (Ransome, U. S. Geol. Surv.)
During its fall, and immediately after, rain is more effective than an equal
amount of snow; but the snow may be accumulated through a considerable
period of the year, and then melted rapidly, when it has an effect
comparable to that which would be produced by the concentration of the
rainfall into a limited period of the year. If the ground beneath be frozen
when the snow melts (and this is often the case) the erosion accomplished
by the resulting water will be diminished.
Except in dry regions, where wind-work sometimes exceeds water-work,
the movements of the atmosphere are of less importance directly than
precipitation in determining the rate of erosion. But even in regions which
are not arid the winds have much to do with the rate of evaporation and the
distribution of rainfall, so that their indirect effect is great. Even their direct
effects in moist climates are not to be lost sight of, for even here the surface
Page 181
is sometimes dry enough to yield dust and sand, and the uprooting of trees
so disturbs the surface as to make earthy débris more accessible to wind and
water. Where trees gain precarious footholds on steep slopes, as they often
do, they are likely to be overturned as soon as they are large enough to offer
considerable resistance to the wind, and in the overturning, large quantities
of rock are sometimes loosened and carried down the slope by gravity. This
phase of destructive work is seen at its best on the walls of gorges, where
trees often flourish until their tops project above the rim of the valley.
Through vegetation, climate influences erosion in ways which are easily
defined qualitatively, but not quantitatively. Both by its growth (wedge-
work of roots) and by its decay (supplying CO2, etc., to descending waters)
it favors certain phases of weathering; but, on the other hand, it retards
corrasion and transportation both by wind and water. This is well shown
along the banks of streams and on the faces of cliffs, in clay, sand, etc. Its
aggregate effect is probably unfavorable to erosion by mechanical means,
and favorable to that by chemical processes.
Fig. 109.—Characteristic cliffs of high arid regions. Right wall of Snake River canyon,
nearly opposite the mouth of Salmon River, Id. Two spring-formed coves, with “Castle
Rock” between. (Russell, U. S. Geol. Surv.)
Erosion in high arid regions differs from that in regions of abundant
rainfall in several ways. It is obvious that the valleys will develop more
slowly in the former, that they will remain young longer, that the period
necessary for the dissection of the surface is greater, that the watercourses
will be less numerous, and that fewer of them will have permanent streams.
There are certain other differences which are less obvious. If the arid region
so disturbs the surface as to make earthy débris more accessible to wind and
water. Where trees gain precarious footholds on steep slopes, as they often
do, they are likely to be overturned as soon as they are large enough to offer
considerable resistance to the wind, and in the overturning, large quantities
of rock are sometimes loosened and carried down the slope by gravity. This
phase of destructive work is seen at its best on the walls of gorges, where
trees often flourish until their tops project above the rim of the valley.
Through vegetation, climate influences erosion in ways which are easily
defined qualitatively, but not quantitatively. Both by its growth (wedge-
work of roots) and by its decay (supplying CO2, etc., to descending waters)
it favors certain phases of weathering; but, on the other hand, it retards
corrasion and transportation both by wind and water. This is well shown
along the banks of streams and on the faces of cliffs, in clay, sand, etc. Its
aggregate effect is probably unfavorable to erosion by mechanical means,
and favorable to that by chemical processes.
Fig. 109.—Characteristic cliffs of high arid regions. Right wall of Snake River canyon,
nearly opposite the mouth of Salmon River, Id. Two spring-formed coves, with “Castle
Rock” between. (Russell, U. S. Geol. Surv.)
Erosion in high arid regions differs from that in regions of abundant
rainfall in several ways. It is obvious that the valleys will develop more
slowly in the former, that they will remain young longer, that the period
necessary for the dissection of the surface is greater, that the watercourses
will be less numerous, and that fewer of them will have permanent streams.
There are certain other differences which are less obvious. If the arid region
Page 182
be high and composed of heterogeneous strata, the topography which
erosion develops is more angular (Fig. 83) than that of the humid region.
This is because there is less rock decay, and less vegetation to hold the
products of decay. The more resistant beds of rock therefore come into
greater prominence, especially on slopes, where they develop cliffs (Figs.
109 and 110). These general principles find abundant illustration in the
plateaus of the western part of the United States,[48] where the cliffs are by
no means confined to the immediate valleys of the streams (Fig. 1, Pl. XII).
Fig. 110.—A Butte. A characteristic feature of the arid plateau region of the West. (Dutton,
Mono. II, U. S. Geol. Surv.)
EFFECTS OF UNEQUAL HARDNESS.
In the preceding pages incidental reference has been made to the results
of inequalities of rock resistance. This topic will now be considered more
fully.
Rapids and falls.—Returning for a moment to the hypothetical island
with which our study of erosion began, let a horizontal layer of hard rock be
erosion develops is more angular (Fig. 83) than that of the humid region.
This is because there is less rock decay, and less vegetation to hold the
products of decay. The more resistant beds of rock therefore come into
greater prominence, especially on slopes, where they develop cliffs (Figs.
109 and 110). These general principles find abundant illustration in the
plateaus of the western part of the United States,[48] where the cliffs are by
no means confined to the immediate valleys of the streams (Fig. 1, Pl. XII).
Fig. 110.—A Butte. A characteristic feature of the arid plateau region of the West. (Dutton,
Mono. II, U. S. Geol. Surv.)
EFFECTS OF UNEQUAL HARDNESS.
In the preceding pages incidental reference has been made to the results
of inequalities of rock resistance. This topic will now be considered more
fully.
Rapids and falls.—Returning for a moment to the hypothetical island
with which our study of erosion began, let a horizontal layer of hard rock be
Page 183
assumed to run through it (H, Fig. 111). As the rain falls on the land and
runs off over it, wear will be less rapid where the hard layer comes to the
surface than at the higher or lower levels. As a result, the slope will become
steeper at and below the outcrop of the hard layer, and less steep
immediately above it, as shown by ab in Fig. 111. Under these conditions
the water passing over the hard ledge constitutes rapids. The increased
erosion which accompanies the increased velocity makes the rapids more
rapid. The process may continue until the water falls, rather than flows over
the hard layer (cd, Fig. 111). With continued rainfall the edges of the hard
layer, together with the slopes above and below, would continue to recede
toward the center of the island. Under conditions of absolute homogeneity
of material, save for the hard layer specified, no valley would be developed,
and therefore no stream.
If the surface was so changed as to allow of the development of a valley
(p. 63) the same principles would be applicable. As an active stream passes
from a hard layer to one less resistant, the greater wear on the latter gives
origin to rapids. At first the rapids would be slight (a, Fig. 112), but would
become more considerable (b) as time and erosion go on. When the bed of
the rapids becomes sufficiently steep, the rapids become falls[49] (cd). When
the water falls rather than flows over the rock surface below the hard layer,
erosion assumes a new phase. The hard layer is then undermined, and the
undermining causes the falls to recede. This phase of erosion is sometimes
called sapping.
Fig. 111.—Diagram representing a horizontal layer of hard rock in an island, and its effects
on erosion.
Fig. 112.—Diagram illustrating the development of a fall where the hard layer dips gently
up-stream.
runs off over it, wear will be less rapid where the hard layer comes to the
surface than at the higher or lower levels. As a result, the slope will become
steeper at and below the outcrop of the hard layer, and less steep
immediately above it, as shown by ab in Fig. 111. Under these conditions
the water passing over the hard ledge constitutes rapids. The increased
erosion which accompanies the increased velocity makes the rapids more
rapid. The process may continue until the water falls, rather than flows over
the hard layer (cd, Fig. 111). With continued rainfall the edges of the hard
layer, together with the slopes above and below, would continue to recede
toward the center of the island. Under conditions of absolute homogeneity
of material, save for the hard layer specified, no valley would be developed,
and therefore no stream.
If the surface was so changed as to allow of the development of a valley
(p. 63) the same principles would be applicable. As an active stream passes
from a hard layer to one less resistant, the greater wear on the latter gives
origin to rapids. At first the rapids would be slight (a, Fig. 112), but would
become more considerable (b) as time and erosion go on. When the bed of
the rapids becomes sufficiently steep, the rapids become falls[49] (cd). When
the water falls rather than flows over the rock surface below the hard layer,
erosion assumes a new phase. The hard layer is then undermined, and the
undermining causes the falls to recede. This phase of erosion is sometimes
called sapping.
Fig. 111.—Diagram representing a horizontal layer of hard rock in an island, and its effects
on erosion.
Fig. 112.—Diagram illustrating the development of a fall where the hard layer dips gently
up-stream.
Page 184
If the hard layer which occasions a
fall dips up-stream (Fig. 112), its
outcrop in the stream’s bed becomes
lower as the fall recedes (e). When it
has become so low that the water
passing over it no longer reacts
effectively against the less resistant
material beneath (f), sapping ceases,
and the point of greatest erosion may be
shifted from the soft material beneath
the fall to the hard layer itself. The Fig. 113.—Diagram illustrating the
actual rate of erosion at this point may conditions which exist at Niagara
Falls. (Gilbert.)
be no greater than before, though the
relative rate is. Under these circumstances the vertical edge of the hard
layer will presently be converted into an incline (f), and as this takes place
the fall becomes rapids. The conversion of the falls into the rapids begins
about the time the lower edge of the hard stratum in the channel reaches
grade. By continuation of the process which transformed the falls into
rapids, the rapids become less rapid, and when the upper edge of the hard
layer has been brought to grade, the rapids disappear (h, Fig. 112). The
history of rapids which succeed falls is the reverse of that which preceded.
The later rapids are steepest at the beginning of their history, the earlier at
their end. Stated in other terms, rapids are steepest when nearest falls in
time. Slight differences in hardness in successive layers often occasion
successive falls or rapids (Fig. 114).
If the hard layer which occasions the falls be horizontal, instead of
dipping up-stream, the general result would be the same; but, other things
being equal, the duration of the falls developed under these conditions
would be greater, since they must recede farther before becoming rapids.
If the layers of unequal hardness in a stream’s bed be vertical and the
course of the stream at right angles to the strike, rapids, and perhaps falls,
will develop (Fig. 115). The chances for falls are greater, the greater the
difference in hardness. Falls developed under these conditions, as well as
the rapids preceding and following, would remain constant in position until
the resistant layer was brought to grade, but they would ultimately
disappear as in the preceding cases. Falls are not likely to develop where
fall dips up-stream (Fig. 112), its
outcrop in the stream’s bed becomes
lower as the fall recedes (e). When it
has become so low that the water
passing over it no longer reacts
effectively against the less resistant
material beneath (f), sapping ceases,
and the point of greatest erosion may be
shifted from the soft material beneath
the fall to the hard layer itself. The Fig. 113.—Diagram illustrating the
actual rate of erosion at this point may conditions which exist at Niagara
Falls. (Gilbert.)
be no greater than before, though the
relative rate is. Under these circumstances the vertical edge of the hard
layer will presently be converted into an incline (f), and as this takes place
the fall becomes rapids. The conversion of the falls into the rapids begins
about the time the lower edge of the hard stratum in the channel reaches
grade. By continuation of the process which transformed the falls into
rapids, the rapids become less rapid, and when the upper edge of the hard
layer has been brought to grade, the rapids disappear (h, Fig. 112). The
history of rapids which succeed falls is the reverse of that which preceded.
The later rapids are steepest at the beginning of their history, the earlier at
their end. Stated in other terms, rapids are steepest when nearest falls in
time. Slight differences in hardness in successive layers often occasion
successive falls or rapids (Fig. 114).
If the hard layer which occasions the falls be horizontal, instead of
dipping up-stream, the general result would be the same; but, other things
being equal, the duration of the falls developed under these conditions
would be greater, since they must recede farther before becoming rapids.
If the layers of unequal hardness in a stream’s bed be vertical and the
course of the stream at right angles to the strike, rapids, and perhaps falls,
will develop (Fig. 115). The chances for falls are greater, the greater the
difference in hardness. Falls developed under these conditions, as well as
the rapids preceding and following, would remain constant in position until
the resistant layer was brought to grade, but they would ultimately
disappear as in the preceding cases. Falls are not likely to develop where
Page 185
the strata of the stream’s bed dip down-stream, though they may develop
even under these conditions if the gradient of the stream is greater than the
dip of the strata (Fig. 116).
Fig. 114.—Falls in Utica shale, Canajoharie, N. Y. (Darton, U. S. Geol. Surv.)
The inequality of resistance in the rock which occasions a fall may be
original or secondary. In the case of Niagara Falls[50] (Fig. 113) relatively
resistant limestone overlies relatively weak shale. At the Falls of St.
Anthony (Minneapolis) limestone overlies friable sandstone. The falls of
the Yellowstone and the Shoshone Falls of the Snake River (Idaho), are in
igneous rock. In the former case the unequal resistance is occasioned by
unequal decay of the rock, due perhaps to the rise of hot vapors which have
decomposed the rock along the lines of their ascent; in the latter, a more
resistant sort of igneous rock overlies a less resistant.
even under these conditions if the gradient of the stream is greater than the
dip of the strata (Fig. 116).
Fig. 114.—Falls in Utica shale, Canajoharie, N. Y. (Darton, U. S. Geol. Surv.)
The inequality of resistance in the rock which occasions a fall may be
original or secondary. In the case of Niagara Falls[50] (Fig. 113) relatively
resistant limestone overlies relatively weak shale. At the Falls of St.
Anthony (Minneapolis) limestone overlies friable sandstone. The falls of
the Yellowstone and the Shoshone Falls of the Snake River (Idaho), are in
igneous rock. In the former case the unequal resistance is occasioned by
unequal decay of the rock, due perhaps to the rise of hot vapors which have
decomposed the rock along the lines of their ascent; in the latter, a more
resistant sort of igneous rock overlies a less resistant.
Page 186
Structural features, such as jointing, sometimes give rise to falls, or
determine their distinctive features (Fig. 117), even where the formations
involved are of uniform hardness. A joint plane has the effect of a weak
vertical or highly inclined bed. If an open joint is discovered in a stream’s
bed, the water enters it. If it finds an outlet below, a channel is worn along
the new line of flow, with rapids or falls where the water descends. Rock
originally homogeneous may be much fractured in some parts, while it
remains unbroken in others. Where a stream passes from the solid to the
broken portion rapids, or even falls, may develop.
Fig. 115.—Diagram illustrating the development of falls over a vertical hard layer.
Fig. 116.—Diagram illustrating the possibility of falls where the beds dip down-stream.
Falls may originate in still other ways. If for any reason a stream is
forced out of its valley, it may in its flow find entrance to another valley, or
to another part of its own valley, over a steep slope. If the structure of the
slope favors, a fall may speedily develop. The Falls of St. Anthony are an
example, the Mississippi having been turned out of its earlier course by
deposits of glacial drift. Again, if an obstruction of any sort, such as a flow
of lava, dams a stream, rapids or falls are developed where the water
overflows the dam. When a main valley is notably deepened by glaciation
the drainage from tributary valleys may fall into it, if the tributaries were
not equally deepened. Falls which originated in this way are common in the
western mountains of the United States, as well as in most mountain regions
recently affected by local glaciers (Fig. 118).
One waterfall often breeds others. Thus where a fall recedes beyond the
mouth of a tributary stream, the tributary falls. The Falls of Minnehaha, on
a small tributary to the Mississippi, near Minneapolis, may serve as an
illustration. In such cases the falls may not develop from rapids. Once in
determine their distinctive features (Fig. 117), even where the formations
involved are of uniform hardness. A joint plane has the effect of a weak
vertical or highly inclined bed. If an open joint is discovered in a stream’s
bed, the water enters it. If it finds an outlet below, a channel is worn along
the new line of flow, with rapids or falls where the water descends. Rock
originally homogeneous may be much fractured in some parts, while it
remains unbroken in others. Where a stream passes from the solid to the
broken portion rapids, or even falls, may develop.
Fig. 115.—Diagram illustrating the development of falls over a vertical hard layer.
Fig. 116.—Diagram illustrating the possibility of falls where the beds dip down-stream.
Falls may originate in still other ways. If for any reason a stream is
forced out of its valley, it may in its flow find entrance to another valley, or
to another part of its own valley, over a steep slope. If the structure of the
slope favors, a fall may speedily develop. The Falls of St. Anthony are an
example, the Mississippi having been turned out of its earlier course by
deposits of glacial drift. Again, if an obstruction of any sort, such as a flow
of lava, dams a stream, rapids or falls are developed where the water
overflows the dam. When a main valley is notably deepened by glaciation
the drainage from tributary valleys may fall into it, if the tributaries were
not equally deepened. Falls which originated in this way are common in the
western mountains of the United States, as well as in most mountain regions
recently affected by local glaciers (Fig. 118).
One waterfall often breeds others. Thus where a fall recedes beyond the
mouth of a tributary stream, the tributary falls. The Falls of Minnehaha, on
a small tributary to the Mississippi, near Minneapolis, may serve as an
illustration. In such cases the falls may not develop from rapids. Once in
Page 187
existence, the fall of a tributary follows the same history as that of a main
stream.
Fig. 117.—Kepler’s Cascade, in the Yellowstone Park. The jointed and fractured character
of the igneous rocks occasions a series of falls and rapids. (Iddings, U. S. Geol. Surv.)
Streams which have falls are relatively clear.[51] If a stream favorably
situated for the development of a fall carried a heavy load, deposition would
take place below the rapids, and the tendency would be to aggrade the
channel at that point and so to prevent the development of the fall. Falls
occur only on streams which have relatively high gradients. This means that
the streams which have falls are well above base-level, and streams well
above base-level are young. Falls therefore are a mark of topographic
youth.
stream.
Fig. 117.—Kepler’s Cascade, in the Yellowstone Park. The jointed and fractured character
of the igneous rocks occasions a series of falls and rapids. (Iddings, U. S. Geol. Surv.)
Streams which have falls are relatively clear.[51] If a stream favorably
situated for the development of a fall carried a heavy load, deposition would
take place below the rapids, and the tendency would be to aggrade the
channel at that point and so to prevent the development of the fall. Falls
occur only on streams which have relatively high gradients. This means that
the streams which have falls are well above base-level, and streams well
above base-level are young. Falls therefore are a mark of topographic
youth.
Page 188
Fig. 118.—The Upper Yosemite Falls.
The fall of the Niagara[52] (Pl. IX) is one of the most remarkable known,
both because of its large volume of water and its great descent, between 160
and 170 feet. The rate at which the fall is receding is a matter of interest not
only in itself, but because, once determined, it may be made to serve as a
unit of measurement for certain important events in geological history. It
was formerly conjectured that this fall was receding at the rate of one to
three feet per century, but it was not until recent years that its actual rate of
recession was approximately fixed. By surveys executed in 1842 and 1890
it has been determined that its average rate of recession between those dates
The fall of the Niagara[52] (Pl. IX) is one of the most remarkable known,
both because of its large volume of water and its great descent, between 160
and 170 feet. The rate at which the fall is receding is a matter of interest not
only in itself, but because, once determined, it may be made to serve as a
unit of measurement for certain important events in geological history. It
was formerly conjectured that this fall was receding at the rate of one to
three feet per century, but it was not until recent years that its actual rate of
recession was approximately fixed. By surveys executed in 1842 and 1890
it has been determined that its average rate of recession between those dates
Page 189
was something like 4½ feet per year, or about 150 times as great as the
highest estimate stated above. It is to be noted that this is the average rate
of recession, for all parts of the ledge over which the water falls are not
receding at the same rate. The point of the “Horseshoe” has, during the
same time, gone back at more than twice this rate.[53]
Fig. 119.—A group of pot-holes. (Turner, U. S. Geol. Surv.)
Rapids and falls sometimes occasion the development of pot-holes (Fig.
119), a peculiar rather than important erosion feature. The holes are
excavated in part by the falling and eddying of silt-charged water, but
chiefly by stones which the eddies move. Pot-holes which are not now in
highest estimate stated above. It is to be noted that this is the average rate
of recession, for all parts of the ledge over which the water falls are not
receding at the same rate. The point of the “Horseshoe” has, during the
same time, gone back at more than twice this rate.[53]
Fig. 119.—A group of pot-holes. (Turner, U. S. Geol. Surv.)
Rapids and falls sometimes occasion the development of pot-holes (Fig.
119), a peculiar rather than important erosion feature. The holes are
excavated in part by the falling and eddying of silt-charged water, but
chiefly by stones which the eddies move. Pot-holes which are not now in
Page 190
immediate association with rapids or falls often point to the former
existence of rapids or falls.
Rock terraces.—The tendency to sapping shown in many waterfalls is
also shown in the weathering and erosion of the sides of a valley where a
hard layer outcrops above the bottom, and the profile of the side slopes of
the valley simulates that of the stream; that is, the slope becomes gentle just
above the hard layer, and steep, or even vertical, at and below its outcrop.
This is illustrated by Fig. 120, where the hard layer through which the
stream has sunk its valley stands out as a rock terrace on either side of the
valley. Such terraces are not rare and are popularly believed to be old
“water-lines”; that is, to represent the height at which the water once stood.
In one sense this interpretation is correct, since a river has stood at all levels
between that of the surface in which its valley started, and its present
channel, but the shelf of hard rock does not mean that the river, after
attaining its present channel, was ever so large as to fill the valley to the
level of the terrace. Rock terraces may also result from changes of level.
Fig. 120.—Diagram to illustrate the development of rock terraces.
Narrows.—Inequalities in hardness occasion another peculiarity
common to valleys. If a stream crosses vertical or highly inclined strata of
unequal hardness, its valley is usually constricted at the crossing of the
harder layers. If such a constriction be notable it is called a narrows, or
sometimes a water-gap (Figs. 121, 159, and Fig. 2, Pl. XII). The
Appalachian Mountains afford numerous examples. The constriction arises
because the processes which widen the valley are less effective on the hard
layer than on the less resistant ones on either hand. Though most narrows
are due to the superior resistance of the rock where they occur, they are
sometimes the result of other causes.
existence of rapids or falls.
Rock terraces.—The tendency to sapping shown in many waterfalls is
also shown in the weathering and erosion of the sides of a valley where a
hard layer outcrops above the bottom, and the profile of the side slopes of
the valley simulates that of the stream; that is, the slope becomes gentle just
above the hard layer, and steep, or even vertical, at and below its outcrop.
This is illustrated by Fig. 120, where the hard layer through which the
stream has sunk its valley stands out as a rock terrace on either side of the
valley. Such terraces are not rare and are popularly believed to be old
“water-lines”; that is, to represent the height at which the water once stood.
In one sense this interpretation is correct, since a river has stood at all levels
between that of the surface in which its valley started, and its present
channel, but the shelf of hard rock does not mean that the river, after
attaining its present channel, was ever so large as to fill the valley to the
level of the terrace. Rock terraces may also result from changes of level.
Fig. 120.—Diagram to illustrate the development of rock terraces.
Narrows.—Inequalities in hardness occasion another peculiarity
common to valleys. If a stream crosses vertical or highly inclined strata of
unequal hardness, its valley is usually constricted at the crossing of the
harder layers. If such a constriction be notable it is called a narrows, or
sometimes a water-gap (Figs. 121, 159, and Fig. 2, Pl. XII). The
Appalachian Mountains afford numerous examples. The constriction arises
because the processes which widen the valley are less effective on the hard
layer than on the less resistant ones on either hand. Though most narrows
are due to the superior resistance of the rock where they occur, they are
sometimes the result of other causes.
Page 191
Fig. 121.—Lower narrows of the Baraboo River, Wis. The even-crested ridge is Huronian
quartzite. The surroundings are of Cambrian sandstone. (Atwood.)
Fig. 122.—A hog-back, Jura-Trias. Colorado City, Colo. (Russell, U. S. Geol. Surv.)
Narrows are much more conspicuous in certain stages of erosion than in
others. While a valley is still so young as to be narrow at all points, no
narrows will be conspicuous; but at a later stage in its history, when the
valley is otherwise wide, narrows are more pronounced. At a still later
stage, when the hard strata themselves approach base-level, the narrows
again become inconspicuous.
From what has preceded it is clear that rapids or falls are likely to occur
at narrows, especially in the early part of their history.
Other effects on topography.—Inequalities in the hardness of rock
develop certain peculiarities of topography other than those of valleys. The
quartzite. The surroundings are of Cambrian sandstone. (Atwood.)
Fig. 122.—A hog-back, Jura-Trias. Colorado City, Colo. (Russell, U. S. Geol. Surv.)
Narrows are much more conspicuous in certain stages of erosion than in
others. While a valley is still so young as to be narrow at all points, no
narrows will be conspicuous; but at a later stage in its history, when the
valley is otherwise wide, narrows are more pronounced. At a still later
stage, when the hard strata themselves approach base-level, the narrows
again become inconspicuous.
From what has preceded it is clear that rapids or falls are likely to occur
at narrows, especially in the early part of their history.
Other effects on topography.—Inequalities in the hardness of rock
develop certain peculiarities of topography other than those of valleys. The
Page 192
less resistant portions of a land area more or less distant from streams are
worn down more readily than those which are more resistant. If great areas
of high land be capped with hard rock they are likely to remain as plateaus
after surrounding areas of less resistance are brought low. If the hard
capping affects a small area instead of a large one, the elevation is a butte, a
hill, or a mountain, instead of a plateau (Fig. 110). Many buttes and small
mesas are but remnants of former plateaus (Mesa Lauriano, N. M., Fig. 1,
Pl. XII). A feature of buttes and mesas capped by hard rock is the steep
slope or cliff corresponding to the edge of the hard bed (Figs. 78 and 109).
Fig. 123.—A ridge due to the outcropping edge of hard Jurassic rock. Wyoming.
If the rock of a region be stratified and the layers tilted, the removal of
the softer beds leaves the harder ones projecting above the general level in
the form of ridges or “hog-backs” (Figs. 122 and 123). Dikes of igneous
rock, harder than the beds which they intersect, likewise become ridges
after the degradation of their surroundings. The plugs of old volcanic vents
and other igneous intrusions of limited area often constitute conspicuous
hills or mountains after erosion has removed their less resistant
surroundings (Fig. 124). Inequalities of hardness are therefore responsible
for many hills and ridges. In the isolation of the hills and ridges picturesque
coves are developed, where the attitude and distribution of the weak and
strong rocks are propitious. The bottoms of the coves are located on the
weak rocks, and above them rise the precipitous slopes of the resistant ones.
worn down more readily than those which are more resistant. If great areas
of high land be capped with hard rock they are likely to remain as plateaus
after surrounding areas of less resistance are brought low. If the hard
capping affects a small area instead of a large one, the elevation is a butte, a
hill, or a mountain, instead of a plateau (Fig. 110). Many buttes and small
mesas are but remnants of former plateaus (Mesa Lauriano, N. M., Fig. 1,
Pl. XII). A feature of buttes and mesas capped by hard rock is the steep
slope or cliff corresponding to the edge of the hard bed (Figs. 78 and 109).
Fig. 123.—A ridge due to the outcropping edge of hard Jurassic rock. Wyoming.
If the rock of a region be stratified and the layers tilted, the removal of
the softer beds leaves the harder ones projecting above the general level in
the form of ridges or “hog-backs” (Figs. 122 and 123). Dikes of igneous
rock, harder than the beds which they intersect, likewise become ridges
after the degradation of their surroundings. The plugs of old volcanic vents
and other igneous intrusions of limited area often constitute conspicuous
hills or mountains after erosion has removed their less resistant
surroundings (Fig. 124). Inequalities of hardness are therefore responsible
for many hills and ridges. In the isolation of the hills and ridges picturesque
coves are developed, where the attitude and distribution of the weak and
strong rocks are propitious. The bottoms of the coves are located on the
weak rocks, and above them rise the precipitous slopes of the resistant ones.
Page 193
Round valley (Fig. 1, Pl. XVII, High Bridge, N. J., quadrangle, U. S. Geol.
Surv.) and the coves about the head of Hiawassee River (Dahlonega, Ga.,
quadrangle) are examples.
Fig. 124.—Matteo tepee, Wyo. Mass of igneous rock exposed by erosion, and preserved
because of its superior resistance. (Detroit Photo. Co.)
Ridges and hills resulting from the unequal degradation of unequally
resistant terranes are not equally prominent at all stages in an erosion cycle.
In early youth the material surrounding the hard bodies of rock has not been
removed; in early maturity considerable portions of their surroundings still
remain about them; but in late maturity or early old age the outcropping
masses of hard rock have been more perfectly isolated and are most
conspicuous. Most of the even-crested ridges of the Appalachian system, as
well as many others which might be mentioned, became ridges in this way.
In the final stages of an erosion cycle the ridges of hard rock are themselves
brought low. Isolated remnants of hard rock which remain distinctly above
their surroundings in the late stages of an erosion cycle (Fig. 124) are
known as Monadnocks, the name being derived from Mount Monadnock,
N. H., an elevation of this sort developed in a cycle antedating the present.
Surv.) and the coves about the head of Hiawassee River (Dahlonega, Ga.,
quadrangle) are examples.
Fig. 124.—Matteo tepee, Wyo. Mass of igneous rock exposed by erosion, and preserved
because of its superior resistance. (Detroit Photo. Co.)
Ridges and hills resulting from the unequal degradation of unequally
resistant terranes are not equally prominent at all stages in an erosion cycle.
In early youth the material surrounding the hard bodies of rock has not been
removed; in early maturity considerable portions of their surroundings still
remain about them; but in late maturity or early old age the outcropping
masses of hard rock have been more perfectly isolated and are most
conspicuous. Most of the even-crested ridges of the Appalachian system, as
well as many others which might be mentioned, became ridges in this way.
In the final stages of an erosion cycle the ridges of hard rock are themselves
brought low. Isolated remnants of hard rock which remain distinctly above
their surroundings in the late stages of an erosion cycle (Fig. 124) are
known as Monadnocks, the name being derived from Mount Monadnock,
N. H., an elevation of this sort developed in a cycle antedating the present.
Page 194
Fig. 125–27.—Diagrams illustrating piracy, where the stream which does not flow over rock
of superior hardness captures those which do. Fig. 126 represents a further development
of the drainage shown in Fig. 125, and Fig. 127 represents a still later stage.
of superior hardness captures those which do. Fig. 126 represents a further development
of the drainage shown in Fig. 125, and Fig. 127 represents a still later stage.
Page 195
Fig. 128–30.—Diagrams to illustrate piracy, where the competing streams all cross a hard
layer. The diagrams represent successive stages of development.
Adjustment of streams to rock structures.—Valleys (gullies) locate
themselves at the outset without immediate regard to the hardness and
softness of their beds. It is primarily the slope about the head of a gully
which determines its line of growth, though relative hardness often
determines the details of slope, even in the early stages of an erosion cycle.
Once established, streams tend to hold their courses, even if this involves
the crossing of resistant layers.
layer. The diagrams represent successive stages of development.
Adjustment of streams to rock structures.—Valleys (gullies) locate
themselves at the outset without immediate regard to the hardness and
softness of their beds. It is primarily the slope about the head of a gully
which determines its line of growth, though relative hardness often
determines the details of slope, even in the early stages of an erosion cycle.
Once established, streams tend to hold their courses, even if this involves
the crossing of resistant layers.
Page 196
While a region where more and less resistant layers of rock come to the
surface is in a youthful stage of erosion, some of the valleys (and therefore
the streams) are likely to be located on the less resistant rock, some on the
more resistant, and some partly on the one and partly on the other. The
streams on the weaker rock will deepen their valleys more rapidly than the
others, and those which flow across stronger and weaker rocks alternately
will deepen their valleys more rapidly than those which run on hard rock all
the time. The former conclusion is self-evident. The latter appears from the
fact that rapids will be likely to develop at the crossing of each hard layer,
thus accelerating erosion at those points. Such a stream therefore not only
has less hard rock to erode than one which flows on resistant rock all the
time, but it erodes that which it does cross much faster.
Fig. 131, 132.—The capture of the head of Beaverdam Creek by the Shenandoah Va.-W. Va.
(After Willis.)
Streams which do not cross hard layers therefore have an advantage over
those which do, and the tributaries to such streams, since they join deeper
mains, have an advantage over the tributaries to the others. The valleys of
the former may lengthen until their heads reach the latter, and capture their
streams. This sequence of events is illustrated in the accompanying
surface is in a youthful stage of erosion, some of the valleys (and therefore
the streams) are likely to be located on the less resistant rock, some on the
more resistant, and some partly on the one and partly on the other. The
streams on the weaker rock will deepen their valleys more rapidly than the
others, and those which flow across stronger and weaker rocks alternately
will deepen their valleys more rapidly than those which run on hard rock all
the time. The former conclusion is self-evident. The latter appears from the
fact that rapids will be likely to develop at the crossing of each hard layer,
thus accelerating erosion at those points. Such a stream therefore not only
has less hard rock to erode than one which flows on resistant rock all the
time, but it erodes that which it does cross much faster.
Fig. 131, 132.—The capture of the head of Beaverdam Creek by the Shenandoah Va.-W. Va.
(After Willis.)
Streams which do not cross hard layers therefore have an advantage over
those which do, and the tributaries to such streams, since they join deeper
mains, have an advantage over the tributaries to the others. The valleys of
the former may lengthen until their heads reach the latter, and capture their
streams. This sequence of events is illustrated in the accompanying
Page 197
diagrams (Figs. 125–27). Even where several streams cross the same
resistant bed, piracy is likely to take place among them, for some are sure to
deepen their valleys faster than others, because of inequalities of volume,
load, or hardness. This is illustrated by Figs. 128–30. An actual case is
shown in Figs. 131, 132. Though piracy may take place when streams do
not flow over rock of unequal hardness (p. 103), it is much more common
where unequal resistance of the rock puts one stream at a disadvantage as
compared with another.
The changes in the courses of streams, by means of which they come to
sustain definite and stable relations to the rock structure beneath, are known
as processes of adjustment.[54] Since streams and valleys adjust themselves
to other conditions as well, this phase of adjustment may be called
structural adjustment. Structural adjustment is not uncommon among rivers
flowing over strata which are vertical or highly inclined, since in these
positions the hard and soft strata are most likely to come to the surface in
frequent alternation. The smaller streams suffer capture and adjustment
first, since, as a rule, they have shallower valleys. It often happens that main
streams, because of their deeper valleys, hold courses not in adjustment
with structure (the Delaware, the Susquehanna, etc.), while tributary
streams are captured, diverted, and adjusted. The capture of a tributary,
however, leads both to the diminution of its main and to the increase of its
captor, and the weakened stream may ultimately fall a prey to the one which
is strengthened.
The processes of adjustment go on until the streams flow as much as
possible on the weaker beds, and as little as possible on the stronger, when
adjustment is complete. This amounts to the same thing as saying that the
outcrops of the hard layers tend to become divides. In many cases an area is
so situated that there is no escape for its drainage except across resistant
rock. In this case its drainage is completely adjusted when as few streams as
possible cross the resistant rock, and these by the shortest routes.
Adjustment has been carried to a high degree of perfection in most parts
of the Appalachian system. Here, as in all other mountains of similar
structure, strata of unequal hardness were folded into ridges. In this case,
the folds have been truncated by erosion, exposing the more and the less
resistant beds (H and S respectively) in alternate belts along the flanks of
the truncated folds (ab and cd, Fig. 133). The streams, especially the lesser
resistant bed, piracy is likely to take place among them, for some are sure to
deepen their valleys faster than others, because of inequalities of volume,
load, or hardness. This is illustrated by Figs. 128–30. An actual case is
shown in Figs. 131, 132. Though piracy may take place when streams do
not flow over rock of unequal hardness (p. 103), it is much more common
where unequal resistance of the rock puts one stream at a disadvantage as
compared with another.
The changes in the courses of streams, by means of which they come to
sustain definite and stable relations to the rock structure beneath, are known
as processes of adjustment.[54] Since streams and valleys adjust themselves
to other conditions as well, this phase of adjustment may be called
structural adjustment. Structural adjustment is not uncommon among rivers
flowing over strata which are vertical or highly inclined, since in these
positions the hard and soft strata are most likely to come to the surface in
frequent alternation. The smaller streams suffer capture and adjustment
first, since, as a rule, they have shallower valleys. It often happens that main
streams, because of their deeper valleys, hold courses not in adjustment
with structure (the Delaware, the Susquehanna, etc.), while tributary
streams are captured, diverted, and adjusted. The capture of a tributary,
however, leads both to the diminution of its main and to the increase of its
captor, and the weakened stream may ultimately fall a prey to the one which
is strengthened.
The processes of adjustment go on until the streams flow as much as
possible on the weaker beds, and as little as possible on the stronger, when
adjustment is complete. This amounts to the same thing as saying that the
outcrops of the hard layers tend to become divides. In many cases an area is
so situated that there is no escape for its drainage except across resistant
rock. In this case its drainage is completely adjusted when as few streams as
possible cross the resistant rock, and these by the shortest routes.
Adjustment has been carried to a high degree of perfection in most parts
of the Appalachian system. Here, as in all other mountains of similar
structure, strata of unequal hardness were folded into ridges. In this case,
the folds have been truncated by erosion, exposing the more and the less
resistant beds (H and S respectively) in alternate belts along the flanks of
the truncated folds (ab and cd, Fig. 133). The streams, especially the lesser
Page 198
ones, now flow along the strike of the softer beds much more commonly
than elsewhere, and where they cross the hard layers it is usually at right
angles to the strike. This is shown in Fig. 134, where the arrows indicate the
direction of strike. In the history of these rivers, however, a factor is
involved which has not yet been considered, and these streams will be
referred to later.
Fig. 133.—Diagram showing the outcrops of hard layers on the flanks of a truncated fold.
cd represents th/e present surface; dotted lines above, earlier surfaces.
than elsewhere, and where they cross the hard layers it is usually at right
angles to the strike. This is shown in Fig. 134, where the arrows indicate the
direction of strike. In the history of these rivers, however, a factor is
involved which has not yet been considered, and these streams will be
referred to later.
Fig. 133.—Diagram showing the outcrops of hard layers on the flanks of a truncated fold.
cd represents th/e present surface; dotted lines above, earlier surfaces.
Page 199
Fig. 134.—Example of adjusted drainage in a region of folded rocks, Va.-W. Va.
Page 200
Fig. 135.—Diagram to illustrate readjustment of drainage, as base-level is approached.
Fig. 136.—Diagram to illustrate superimposition. The consequent stream on the upper
formation is superimposed on the underlying structures when the upper bed has been cut
through.
As base-level is approached, the outcrops of hard rock are brought low.
When they have been reduced to the level of their surroundings, the streams
may flow without regard to the resistance of the rock beneath, for
downward cutting has ceased. As this stage of erosion is approached, a
readjustment of the drainage may take place, and the waters which had
Fig. 136.—Diagram to illustrate superimposition. The consequent stream on the upper
formation is superimposed on the underlying structures when the upper bed has been cut
through.
As base-level is approached, the outcrops of hard rock are brought low.
When they have been reduced to the level of their surroundings, the streams
may flow without regard to the resistance of the rock beneath, for
downward cutting has ceased. As this stage of erosion is approached, a
readjustment of the drainage may take place, and the waters which had
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taken long and circuitous courses to avoid hard rock, may change their
courses to more direct ones (compare Figs. 130 and 135). Adjustment is,
therefore, a relative term, and streams which are adjusted at one stage of
erosion, are not necessarily adjusted at another.
It sometimes happens that rocks of unequal resistance are covered by
beds of uniform hardness. A consequent stream developed on the latter may
find itself out of structural adjustment when it has cut its channel down to
the level of the heterogeneous beds below. Such a stream is said to be
superimposed (Fig. 136) on the underlying structure. Structural adjustment
is likely to follow.
INFLUENCE OF JOINTS AND FOLDS.
Joints.—Various structural features of rock other than hardness influence
its erosion. Apart from the stratification planes, most rock formations are
affected by joints or fissures. The joints are often, but not always, nearly
vertical. Two sets are generally present, and sometimes more. If but two,
they usually meet at a large angle; if more than two, two are likely to be
nearly perpendicular to each other, while the third and fourth sets have such
directions as to cut the others at large angles. These joints allow the ingress
of water, roots, etc., which help to weather and disrupt rocks. Occasionally
there is notable sag of the beds of rock along joint planes, but this effect is
usually superficial only (Fig. 137). Where the jointage planes are frequent
and open, the columns bounded by them sometimes topple over on cliff
faces, either by undercutting, or by the wedge-work of roots or ice.
The effect of joints on erosion may often be seen along a stream which
flows in a rock gorge. In such situations, the outlines of the banks are
sometimes angular, and sometimes crenate (Fig. 138), the reëntrants being
located at the joints. By working into and widening joints, running water
sometimes isolates masses of rock as islands (Fig. 139). In a region free
from mantle rock, or where the mantle rock is meagre, joints often
determine the courses of valleys by directing the course of surface drainage.
This is shown in many parts of the arid west. In regions where the rocks are
notably faulted, the courses of the streams are sometimes controlled by the
courses of the fault planes. This is the case, for example, in central
Washington.[55]
courses to more direct ones (compare Figs. 130 and 135). Adjustment is,
therefore, a relative term, and streams which are adjusted at one stage of
erosion, are not necessarily adjusted at another.
It sometimes happens that rocks of unequal resistance are covered by
beds of uniform hardness. A consequent stream developed on the latter may
find itself out of structural adjustment when it has cut its channel down to
the level of the heterogeneous beds below. Such a stream is said to be
superimposed (Fig. 136) on the underlying structure. Structural adjustment
is likely to follow.
INFLUENCE OF JOINTS AND FOLDS.
Joints.—Various structural features of rock other than hardness influence
its erosion. Apart from the stratification planes, most rock formations are
affected by joints or fissures. The joints are often, but not always, nearly
vertical. Two sets are generally present, and sometimes more. If but two,
they usually meet at a large angle; if more than two, two are likely to be
nearly perpendicular to each other, while the third and fourth sets have such
directions as to cut the others at large angles. These joints allow the ingress
of water, roots, etc., which help to weather and disrupt rocks. Occasionally
there is notable sag of the beds of rock along joint planes, but this effect is
usually superficial only (Fig. 137). Where the jointage planes are frequent
and open, the columns bounded by them sometimes topple over on cliff
faces, either by undercutting, or by the wedge-work of roots or ice.
The effect of joints on erosion may often be seen along a stream which
flows in a rock gorge. In such situations, the outlines of the banks are
sometimes angular, and sometimes crenate (Fig. 138), the reëntrants being
located at the joints. By working into and widening joints, running water
sometimes isolates masses of rock as islands (Fig. 139). In a region free
from mantle rock, or where the mantle rock is meagre, joints often
determine the courses of valleys by directing the course of surface drainage.
This is shown in many parts of the arid west. In regions where the rocks are
notably faulted, the courses of the streams are sometimes controlled by the
courses of the fault planes. This is the case, for example, in central
Washington.[55]
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Fig. 137.—Shows the sagging of beds along joints. The disturbance does not extend far
below the surface. Cook’s quarry (Niagara limestone) near La Salle, Niagara Co., N. Y.
(Gilbert, U. S. Geol. Surv.)
The jointing of rocks often shows itself distinctly in the weathered faces
of cliffs (Figs. 140 and 141), especially in arid and semi-arid regions, or
where the slope is too steep for the accumulation of soil and rock-waste on
its surface.
If a stream flowing over jointed rock has falls, the conditions are
sometimes afforded for the development of an exceptional and striking
scenic feature. If above Niagara Falls, for example, there were an open joint
in the bed of the stream (as at b, Fig. 142), some portion of the water would
descend through it. After reaching a lower level it might find or make a
passage through the rock to the river below the falls. If even a little water
took such a course, the flow would enlarge its channel, making a
passageway between the joint through which the water descended and the
valley below the falls (bcde, Fig. 142). This passageway might become
large enough to accommodate all the water of the river. In this case, the
entire fall would be transferred from the position which it previously
below the surface. Cook’s quarry (Niagara limestone) near La Salle, Niagara Co., N. Y.
(Gilbert, U. S. Geol. Surv.)
The jointing of rocks often shows itself distinctly in the weathered faces
of cliffs (Figs. 140 and 141), especially in arid and semi-arid regions, or
where the slope is too steep for the accumulation of soil and rock-waste on
its surface.
If a stream flowing over jointed rock has falls, the conditions are
sometimes afforded for the development of an exceptional and striking
scenic feature. If above Niagara Falls, for example, there were an open joint
in the bed of the stream (as at b, Fig. 142), some portion of the water would
descend through it. After reaching a lower level it might find or make a
passage through the rock to the river below the falls. If even a little water
took such a course, the flow would enlarge its channel, making a
passageway between the joint through which the water descended and the
valley below the falls (bcde, Fig. 142). This passageway might become
large enough to accommodate all the water of the river. In this case, the
entire fall would be transferred from the position which it previously
Page 203
occupied (f) to the position of the enlarged joint (b). The fall would then
recede. The underground channel between the old falls and the new would
be bridged by rock (bf″ and f‴, Fig. 143), making a natural bridge. The
natural bridge near Lexington, Va. (Fig. 144), almost 200 feet above the
stream which flows beneath it, is believed to have been developed in this
way. A similar bridge is now in process of development in Two Medicine
River in northwestern Montana (Fig. 145). Once in existence, a natural
bridge will slowly weather away.
Fig. 138.—Figure showing crenate river bank, the reëntrants being determined by joints.
Dells of the Wisconsin River, near Kilbourn, Wis. (Atwood.)
recede. The underground channel between the old falls and the new would
be bridged by rock (bf″ and f‴, Fig. 143), making a natural bridge. The
natural bridge near Lexington, Va. (Fig. 144), almost 200 feet above the
stream which flows beneath it, is believed to have been developed in this
way. A similar bridge is now in process of development in Two Medicine
River in northwestern Montana (Fig. 145). Once in existence, a natural
bridge will slowly weather away.
Fig. 138.—Figure showing crenate river bank, the reëntrants being determined by joints.
Dells of the Wisconsin River, near Kilbourn, Wis. (Atwood.)
Page 204
Fig. 139.—Lone Rock. An island isolated by the notable widening of a series of joints. The
joints in the rock of the island have themselves been so widened that a rowboat may be
taken through it in two directions. Lower Dells of the Wisconsin. (Meyers.)
joints in the rock of the island have themselves been so widened that a rowboat may be
taken through it in two directions. Lower Dells of the Wisconsin. (Meyers.)
Page 205
Fig. 140.—Effect of columnar structure on weathering. Material unconsolidated. Spur of
south end of Sheep Mountain. (Lippincott, U. S. Geol. Surv.)
It is not to be understood that all natural bridges have had this history.
They are sometimes developed from underground caves when parts of their
roofs are destroyed, as well as in various other ways.
south end of Sheep Mountain. (Lippincott, U. S. Geol. Surv.)
It is not to be understood that all natural bridges have had this history.
They are sometimes developed from underground caves when parts of their
roofs are destroyed, as well as in various other ways.
Page 206
Fig. 141.—Effect of columnar structure on weathering. Big Bad Lands, S. D. (Darton, U. S.
Geol. Surv.)
Folds.—The erosion of folded strata (anticlines and synclines) leads to
the development of distinctive topographic features. So soon as a fold
begins to be lifted, it is, by reason of its position, subject to more rapid
erosion than its surroundings. For the same reason the crest of the fold is
likely to be degraded more rapidly than its lower slopes, and must suffer
more degradation before it is brought to base-level. Folds are usually
composed of beds of unequal resistance, and as the degradation of a fold
proceeds, successive layers are worn from the top, and the alternating hard
and soft layers composing it are exposed. So soon as this is accomplished,
adjustment of the streams is likely to begin, and the watercourses, and later
the valley plains, come to be located on the outcrops of the less resistant
layers, while the outcrops of the harder beds become ridges.
If the axis of an eroded anticline were horizontal, a given hard layer, the
arch of which has been cut off, would, after erosion, outcrop on both sides
of the axis. When the topography was mature these outcrops would
Geol. Surv.)
Folds.—The erosion of folded strata (anticlines and synclines) leads to
the development of distinctive topographic features. So soon as a fold
begins to be lifted, it is, by reason of its position, subject to more rapid
erosion than its surroundings. For the same reason the crest of the fold is
likely to be degraded more rapidly than its lower slopes, and must suffer
more degradation before it is brought to base-level. Folds are usually
composed of beds of unequal resistance, and as the degradation of a fold
proceeds, successive layers are worn from the top, and the alternating hard
and soft layers composing it are exposed. So soon as this is accomplished,
adjustment of the streams is likely to begin, and the watercourses, and later
the valley plains, come to be located on the outcrops of the less resistant
layers, while the outcrops of the harder beds become ridges.
If the axis of an eroded anticline were horizontal, a given hard layer, the
arch of which has been cut off, would, after erosion, outcrop on both sides
of the axis. When the topography was mature these outcrops would
Page 207
constitute parallel ridges, or parallel lines of hills; when the region had been
base-leveled, the outcrops would be in parallel belts, though no longer
ridges or hills. The lower the plane of truncation, the farther apart would the
outcrops be in the anticline, and the nearer together in the syncline
(compare ab and cd, Fig. 133).
Fig. 142.—A natural bridge in process of development; longitudinal section at the left;
transverse section, looking toward e, at the right.
Fig. 143.—The same as Fig. 142 at a later stage of development.
If, on the other hand, the axis of the anticline or syncline to be eroded
was not horizontal, that is, if it plunged, the topographic result would be
somewhat different. Suppose a plunging anticline to be truncated at base-
level. If either end of the fold plunged below the plane of truncation, the
outcrops of a given layer on opposite sides of the axis would converge in
the direction of plunge, and come together at the end. At a stage of erosion
antedating planation (say late maturity) there would have been a ridge, or a
succession of hills, in the position corresponding to the outcrop of a hard
layer, with a canoe-shaped valley within. If two hard layers were involved,
instead of one, there would be two encircling ridges, with a curved valley
between them, and a canoe-shaped valley within the innermost (Fig. 146).
If the anticline plunged both ways, the valley enclosed by the hard-layer
ridge would be canoe-shaped at both ends (Fig. 147). In such a case there
would be likely to be a low gap (water-gap) in the rim of the valley through
which the drainage which degraded the surface escaped, but there would be
likely to be but one, for if two or more streams had drained the area of the
valley at an early stage of erosion, one would be likely to have captured the
others (see p. 138) before late maturity. A succession of doubly-plunging
anticlines and synclines might give rise to a very complex series of ridges
base-leveled, the outcrops would be in parallel belts, though no longer
ridges or hills. The lower the plane of truncation, the farther apart would the
outcrops be in the anticline, and the nearer together in the syncline
(compare ab and cd, Fig. 133).
Fig. 142.—A natural bridge in process of development; longitudinal section at the left;
transverse section, looking toward e, at the right.
Fig. 143.—The same as Fig. 142 at a later stage of development.
If, on the other hand, the axis of the anticline or syncline to be eroded
was not horizontal, that is, if it plunged, the topographic result would be
somewhat different. Suppose a plunging anticline to be truncated at base-
level. If either end of the fold plunged below the plane of truncation, the
outcrops of a given layer on opposite sides of the axis would converge in
the direction of plunge, and come together at the end. At a stage of erosion
antedating planation (say late maturity) there would have been a ridge, or a
succession of hills, in the position corresponding to the outcrop of a hard
layer, with a canoe-shaped valley within. If two hard layers were involved,
instead of one, there would be two encircling ridges, with a curved valley
between them, and a canoe-shaped valley within the innermost (Fig. 146).
If the anticline plunged both ways, the valley enclosed by the hard-layer
ridge would be canoe-shaped at both ends (Fig. 147). In such a case there
would be likely to be a low gap (water-gap) in the rim of the valley through
which the drainage which degraded the surface escaped, but there would be
likely to be but one, for if two or more streams had drained the area of the
valley at an early stage of erosion, one would be likely to have captured the
others (see p. 138) before late maturity. A succession of doubly-plunging
anticlines and synclines might give rise to a very complex series of ridges
Page 208
and valleys. Illustrations of the above phenomena are found at various
points in the Appalachian Mountains, especially in eastern Pennsylvania.[56]
Fig. 144.—The Natural Bridge of Virginia, from the southeast (Walcott, U. S. Geol. Surv.)
points in the Appalachian Mountains, especially in eastern Pennsylvania.[56]
Fig. 144.—The Natural Bridge of Virginia, from the southeast (Walcott, U. S. Geol. Surv.)
Page 209
Fig. 145.—A natural bridge in development. Two Medicine River, Mont. Corresponds to
the stage represented by Fig. 142, and the view corresponds to that shown
diagrammatically at the right-hand end of the figure. (Whitney.)
In the structural adjustment which goes with the erosion of folds, it often
happens that the valleys come to be located on the anticlines, while the
outcrops of the hard layers on the flanks of the anticlines, or even in the
original synclines, become the mountains. The adjustments by which
valleys come to be located on anticlines are somewhat as follows:[57] Fig.
148 represents two doubly-plunging anticlines with a syncline between, the
relative elevations being shown by contour lines. At the outset, the drainage
of such a region must have followed the structural valley, and its initial
course, consequent on the slope, must have been down the axial trough.
Drainage from the anticlines into the synclines would have promptly
developed valleys, and the valleys would soon have acquired streams.
the stage represented by Fig. 142, and the view corresponds to that shown
diagrammatically at the right-hand end of the figure. (Whitney.)
In the structural adjustment which goes with the erosion of folds, it often
happens that the valleys come to be located on the anticlines, while the
outcrops of the hard layers on the flanks of the anticlines, or even in the
original synclines, become the mountains. The adjustments by which
valleys come to be located on anticlines are somewhat as follows:[57] Fig.
148 represents two doubly-plunging anticlines with a syncline between, the
relative elevations being shown by contour lines. At the outset, the drainage
of such a region must have followed the structural valley, and its initial
course, consequent on the slope, must have been down the axial trough.
Drainage from the anticlines into the synclines would have promptly
developed valleys, and the valleys would soon have acquired streams.
Page 210
Fig. 146.—A canoe-shaped valley bordered by a ridge formed by the outcrop of a hard
layer in a plunging syncline. The ridge bounding the canoe-valley is separated from an
outer ridge by a curved valley underlain by relatively weak rock. (After Willis.)
Fig. 147.—A diagram to illustrate the effects of erosion on a doubly-plunging anticline
made up of beds of unequal hardness.
layer in a plunging syncline. The ridge bounding the canoe-valley is separated from an
outer ridge by a curved valley underlain by relatively weak rock. (After Willis.)
Fig. 147.—A diagram to illustrate the effects of erosion on a doubly-plunging anticline
made up of beds of unequal hardness.
Page 211
Fig. 148–51.—Diagrams to illustrate the shifting of rivers from a synclinal to an anticlinal
position. (After Davis.)
The anticlines and synclines under consideration are assumed to have a
thick hard layer at the surface, and softer beds below. This is shown in the
cross-section introduced in the figure, the upper hard stratum (m) being
indicated by the dots, while the softer one (n) is white. The line oo
represents base-level, which is below the hard layer both in the syncline and
anticline, but much farther below in the latter position than in the former.
Because of their higher gradients, and because of the greater fracturing to
which the region they drain was presumably subject at the time of folding,
the tributary streams might cut through the hard layer sooner than the main
stream which they join. This done, they would enlarge their valleys rapidly
in the softer rock beneath, and secondary tributaries would be developed
(Fig. 149). When the condition of things represented in Fig. 149 is reached,
the streams c and d, tributary to the synclinal stream, come into
competition. The former has the advantage over the latter, because it joins
the main stream at a lower level. Stream c will therefore be likely to capture
d. The incipient stages of the capture are stealthy, and the later bold. At first
the divide between their head waters is shifted northward inch by inch,
position. (After Davis.)
The anticlines and synclines under consideration are assumed to have a
thick hard layer at the surface, and softer beds below. This is shown in the
cross-section introduced in the figure, the upper hard stratum (m) being
indicated by the dots, while the softer one (n) is white. The line oo
represents base-level, which is below the hard layer both in the syncline and
anticline, but much farther below in the latter position than in the former.
Because of their higher gradients, and because of the greater fracturing to
which the region they drain was presumably subject at the time of folding,
the tributary streams might cut through the hard layer sooner than the main
stream which they join. This done, they would enlarge their valleys rapidly
in the softer rock beneath, and secondary tributaries would be developed
(Fig. 149). When the condition of things represented in Fig. 149 is reached,
the streams c and d, tributary to the synclinal stream, come into
competition. The former has the advantage over the latter, because it joins
the main stream at a lower level. Stream c will therefore be likely to capture
d. The incipient stages of the capture are stealthy, and the later bold. At first
the divide between their head waters is shifted northward inch by inch,
Page 212
because the gradient toward g is higher than that toward e. The capture of
the head waters of e is as slow as the migration of the divide, until the
divide reaches the point where e joins f. The stream f is then diverted
promptly into the valley of g, and is at once led away to c (see Fig. 150).
Strengthened by its increased volume, the stream c (Fig. 150) lowers its
valley across the hard layer more rapidly than before, and so holds the
advantage it has gained. Not only this, but the beheaded stream d (Fig. 150),
because of its diminished volume, sinks its valley into the hard layer less
rapidly than before, and its decrease in power also works to the advantage
of the stream leading to c. The result is that the divide between fg and d
does not remain constant, but is driven back step by step toward a.
Similarly a tributary to the main stream at b (Fig. 150), may by means of
its tributary h, capture the waters of fg, and lead them to the synclinal valley
at b (compare Figs. 150 and 151). Deprived of its main source of supply (at
c) the synclinal stream is greatly diminished above b, and cuts more and
more slowly, while the stream fgh (Fig. 151), having greater volume and
working mainly in softer rock, sinks its channel faster than the stream in the
synclinal axis. Under these circumstances, the stream at f may cut its valley
below the valley in the synclinal axis a (Fig. 150). In this event, the divide
between f and a (Fig. 150) may be pushed back until the synclinal stream is
beheaded at a and carried out of the syncline and over into the anticlinal
valley (Fig. 151). Thus, the old anticlinal axis comes to be the course of the
main stream. Similarly the stream entering the syncline at b (Fig. 151)
might later be captured by i, thus lengthening its anticlinal course.
It is not to be understood that this sequence of events will take place in
the degradation of every anticline, but the principles here set forth will
always be operative. The result specified will be accomplished wherever
hard and soft layers have the relations indicated in the diagrams; that is,
where the stream in the syncline finds itself on a resistant layer as it
approaches base-level, while at the same time the (original) tributary
streams are working in softer beds. It is not to be understood, therefore, that
streams migrate from synclines to anticlines for the sake of getting out of
the former positions into the latter. If they shift their courses it is to find
easier ones.
That these changes are not fanciful is shown by the fact that the
adjustment described corresponds with that shown in many parts of the
the head waters of e is as slow as the migration of the divide, until the
divide reaches the point where e joins f. The stream f is then diverted
promptly into the valley of g, and is at once led away to c (see Fig. 150).
Strengthened by its increased volume, the stream c (Fig. 150) lowers its
valley across the hard layer more rapidly than before, and so holds the
advantage it has gained. Not only this, but the beheaded stream d (Fig. 150),
because of its diminished volume, sinks its valley into the hard layer less
rapidly than before, and its decrease in power also works to the advantage
of the stream leading to c. The result is that the divide between fg and d
does not remain constant, but is driven back step by step toward a.
Similarly a tributary to the main stream at b (Fig. 150), may by means of
its tributary h, capture the waters of fg, and lead them to the synclinal valley
at b (compare Figs. 150 and 151). Deprived of its main source of supply (at
c) the synclinal stream is greatly diminished above b, and cuts more and
more slowly, while the stream fgh (Fig. 151), having greater volume and
working mainly in softer rock, sinks its channel faster than the stream in the
synclinal axis. Under these circumstances, the stream at f may cut its valley
below the valley in the synclinal axis a (Fig. 150). In this event, the divide
between f and a (Fig. 150) may be pushed back until the synclinal stream is
beheaded at a and carried out of the syncline and over into the anticlinal
valley (Fig. 151). Thus, the old anticlinal axis comes to be the course of the
main stream. Similarly the stream entering the syncline at b (Fig. 151)
might later be captured by i, thus lengthening its anticlinal course.
It is not to be understood that this sequence of events will take place in
the degradation of every anticline, but the principles here set forth will
always be operative. The result specified will be accomplished wherever
hard and soft layers have the relations indicated in the diagrams; that is,
where the stream in the syncline finds itself on a resistant layer as it
approaches base-level, while at the same time the (original) tributary
streams are working in softer beds. It is not to be understood, therefore, that
streams migrate from synclines to anticlines for the sake of getting out of
the former positions into the latter. If they shift their courses it is to find
easier ones.
That these changes are not fanciful is shown by the fact that the
adjustment described corresponds with that shown in many parts of the
Page 213
Appalachian Mountains, and in other mountains of similar structure.
If in a later stage of its history, the new main stream, fh, were to cut its
bed down to a lower hard layer, while the original stream, ab, reached a
softer bed beneath the hard one above, the latter would again have an
advantage, and a new series of adjustments would be inaugurated which
might result in re-establishing the main stream in its original synclinal
position.
EFFECT OF CHANGES OF LEVEL.
Rise.—If after being base-leveled, or notably reduced by erosion, a
region is uplifted so as to increase the gradients and therefore the velocities
of the streams which drain it, the streams are said to be rejuvenated, and a
new cycle of erosion is begun. If the rise of the area were equal everywhere,
while the coast line remained constant in position, there would be an
immediate increase in velocity only at the debouchures of the streams
flowing directly into the sea. At the debouchures of such streams there
would be rapids or falls. Each rapids or falls would promptly recede, and
with the recession, the acceleration of velocity resulting from the uplift
would be felt farther and farther up-stream, and ultimately to its source. The
rejuvenated streams would cut new valleys in the bottoms of their old ones
(Figs. 152 and 153). The new valleys would begin where the increase in
velocity was first felt, and they would be lengthened by head erosion just as
valleys of the first cycle were lengthened.
Fig. 152.—Cross-section of a wide valley, ab, in the bottom of which a younger valley, cd,
has been excavated as the result of uplift.
If in a later stage of its history, the new main stream, fh, were to cut its
bed down to a lower hard layer, while the original stream, ab, reached a
softer bed beneath the hard one above, the latter would again have an
advantage, and a new series of adjustments would be inaugurated which
might result in re-establishing the main stream in its original synclinal
position.
EFFECT OF CHANGES OF LEVEL.
Rise.—If after being base-leveled, or notably reduced by erosion, a
region is uplifted so as to increase the gradients and therefore the velocities
of the streams which drain it, the streams are said to be rejuvenated, and a
new cycle of erosion is begun. If the rise of the area were equal everywhere,
while the coast line remained constant in position, there would be an
immediate increase in velocity only at the debouchures of the streams
flowing directly into the sea. At the debouchures of such streams there
would be rapids or falls. Each rapids or falls would promptly recede, and
with the recession, the acceleration of velocity resulting from the uplift
would be felt farther and farther up-stream, and ultimately to its source. The
rejuvenated streams would cut new valleys in the bottoms of their old ones
(Figs. 152 and 153). The new valleys would begin where the increase in
velocity was first felt, and they would be lengthened by head erosion just as
valleys of the first cycle were lengthened.
Fig. 152.—Cross-section of a wide valley, ab, in the bottom of which a younger valley, cd,
has been excavated as the result of uplift.
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Fig. 153.—Diagram to illustrate in ground plan an ideal case of rejuvenation as the result
of uplift.
When the head of the new part of a valley of a rejuvenated stream
recedes past the mouth of a tributary adjusted[58] to the gradient of the main
stream before rejuvenation, the velocity of the tributary is accelerated at its
debouchure, and it begins to excavate a new valley in the bottom of its old
one. The new valley commences at the lower end of the old one, and
develops headward (a and b, Fig. 153). Good illustrations are furnished by
the streams in the west central part of New Jersey. The Delaware has here a
sharply defined valley, and its tributaries are essentially as deep as their
main at the point of junction. Above this point they have high gradients for
a short distance (three to six miles), beyond which they wind sluggishly in
wide valleys with low gradients across a relatively high plateau. Their
of uplift.
When the head of the new part of a valley of a rejuvenated stream
recedes past the mouth of a tributary adjusted[58] to the gradient of the main
stream before rejuvenation, the velocity of the tributary is accelerated at its
debouchure, and it begins to excavate a new valley in the bottom of its old
one. The new valley commences at the lower end of the old one, and
develops headward (a and b, Fig. 153). Good illustrations are furnished by
the streams in the west central part of New Jersey. The Delaware has here a
sharply defined valley, and its tributaries are essentially as deep as their
main at the point of junction. Above this point they have high gradients for
a short distance (three to six miles), beyond which they wind sluggishly in
wide valleys with low gradients across a relatively high plateau. Their
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profiles are illustrated by Fig. 154. The flat, though high, surface in which
their upper courses lie, appears to have been nearly base-leveled in an
earlier cycle, and then to have been elevated. The date of the elevation is
fixed, in terms of erosion, by the time necessary for the excavation of the
Delaware gorge, and the narrow gorges along the lower courses of its
tributaries. It was so recent that the effects of rejuvenation, proceeding from
the debouchures of the tributaries toward their heads, have not yet advanced
far from the Delaware. Similar relations are found elsewhere (Fig. 1, Pl.
XIII, s. c. Col.). Another peculiarity of rejuvenated drainage is shown in
Fig. 2, Plate XIII (s. Kan.). Here Elm Creek flows at a level 200 feet below
that of Sand Creek, 4 miles distant. The valley of the former appears to have
entered upon a new cycle as the result of uplift, while that of the latter, in
the area shown on the map, is still unrejuvenated. Farther down-stream, the
valley of Sand Creek shows signs of rejuvenation. It may be noted that a
tributary of Amber Creek has good opportunity to capture Sand Creek, for
the latter flows about 25 miles before reaching the level of Amber Creek at
its junction with Elm Creek.
their upper courses lie, appears to have been nearly base-leveled in an
earlier cycle, and then to have been elevated. The date of the elevation is
fixed, in terms of erosion, by the time necessary for the excavation of the
Delaware gorge, and the narrow gorges along the lower courses of its
tributaries. It was so recent that the effects of rejuvenation, proceeding from
the debouchures of the tributaries toward their heads, have not yet advanced
far from the Delaware. Similar relations are found elsewhere (Fig. 1, Pl.
XIII, s. c. Col.). Another peculiarity of rejuvenated drainage is shown in
Fig. 2, Plate XIII (s. Kan.). Here Elm Creek flows at a level 200 feet below
that of Sand Creek, 4 miles distant. The valley of the former appears to have
entered upon a new cycle as the result of uplift, while that of the latter, in
the area shown on the map, is still unrejuvenated. Farther down-stream, the
valley of Sand Creek shows signs of rejuvenation. It may be noted that a
tributary of Amber Creek has good opportunity to capture Sand Creek, for
the latter flows about 25 miles before reaching the level of Amber Creek at
its junction with Elm Creek.
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PLATE XIII.
U. S. Geol. Surv. Fig. 1. COLORADO. Scale, 2+ mile per inch.
U. S. Geol. Surv. Fig. 1. COLORADO. Scale, 2+ mile per inch.
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U. S. Geol. Surv. Fig. 2. KANSAS. Scale, 2+ mile per inch.
PLATE XIV.
U. S. Geol. Surv. Fig. 1. PENNSYLVANIA. Scale, 1+ mile per inch.
PLATE XIV.
U. S. Geol. Surv. Fig. 1. PENNSYLVANIA. Scale, 1+ mile per inch.
Page 218
U. S. Geol. Surv. Fig. 2. CALIFORNIA. Scale, 1+ mile per inch.
Fig. 154.—Profile of a rejuvenated stream. The Lockatong River (N. J.) to the head of Mud
Run.
Should the lower end of a tributary valley fail to be degraded as fast as
the valley of the main at the point of junction, the tributary is out of
topographic adjustment with its main. Falls or rapids may result. When the
lower end of a tributary valley is distinctly above the level of its main, the
former is called a hanging valley. Hanging valleys developed by stream
erosion alone are not common except just after the recession of a falls past
the mouth of a tributary. Hanging valleys, as well as the characters and
relations illustrated by Figs. 152–154 are criteria of rejuvenation, but they
Fig. 154.—Profile of a rejuvenated stream. The Lockatong River (N. J.) to the head of Mud
Run.
Should the lower end of a tributary valley fail to be degraded as fast as
the valley of the main at the point of junction, the tributary is out of
topographic adjustment with its main. Falls or rapids may result. When the
lower end of a tributary valley is distinctly above the level of its main, the
former is called a hanging valley. Hanging valleys developed by stream
erosion alone are not common except just after the recession of a falls past
the mouth of a tributary. Hanging valleys, as well as the characters and
relations illustrated by Figs. 152–154 are criteria of rejuvenation, but they
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must be applied with discretion. Such profiles, for example, as that shown
in Fig. 154 may be developed when the rock of a stream’s bed is unequally
resistant, and hanging valleys are generally a result of glaciation (see
Chapter V).
Rejuvenated streams sometimes inherit certain peculiarities from their
aged ancestors. Thus a rejuvenated stream may intrench the meanders
possessed by the old stream which preceded (see Fig. 1, Pl. XIV, near
Harrisburg, Pa.), and intrenched meanders are one of the marks of
rejuvenated streams. They are not uncommon in the Appalachian Mountain
regions, and are known in other parts of the world. The Seine and the
Moselle furnish further illustrations.[59]
The history of the new cycle of erosion inaugurated by the uplift would
differ from that of the preceding cycle in that the new one would begin with
a drainage system already developed. Other things being equal, therefore,
the reduction of the land would proceed more rapidly in a subsequent cycle
than in the first.
The recognition of different cycles of erosion, separated by uplifts, is
often easy. The principles involved are illustrated by Fig. 155 which
represents an ideal profile of considerable length (say 50 miles). The points
a, a′, and a″ reach a common level. Below them there are areas b, b′, and b″
which have a nearly common elevation, below which are the sharp valleys
d, d′, and d″. The points a, a′, and a″ represent the cross-sections of ridges
formed by the outcrops of layers of hard rock. If the crests of the ridges are
level, the points a, a′, and a″ must represent remnants of an old base-level,
since at no time after a ridge of hard rock becomes deeply notched does it
acquire an even crest, until it is base-leveled.[60] At all earlier stages its crest
is uneven. After the cycle represented by the remnants a, a′, and a″ was
completed, the region suffered uplift. A new cycle represented by the plain
b, b′, and b″ was well advanced, though not completed, when the region
was again elevated, and the rejuvenated streams began to cut their valleys d,
d′, and d″ in the plain of the previous incomplete cycle. The elevations, c
and c′ (intermediate in elevation between a, a′, and a″, and b, b′, and b″)
may represent either remnants of the first base-level plain which were
lowered, but not obliterated, while the plane b, b′, b″ was developing; or
they may represent a cycle intermediate between that during which a, a′, a″
and b, b′, b″ were developed. If the intermediate elevations (c, c′) have a
in Fig. 154 may be developed when the rock of a stream’s bed is unequally
resistant, and hanging valleys are generally a result of glaciation (see
Chapter V).
Rejuvenated streams sometimes inherit certain peculiarities from their
aged ancestors. Thus a rejuvenated stream may intrench the meanders
possessed by the old stream which preceded (see Fig. 1, Pl. XIV, near
Harrisburg, Pa.), and intrenched meanders are one of the marks of
rejuvenated streams. They are not uncommon in the Appalachian Mountain
regions, and are known in other parts of the world. The Seine and the
Moselle furnish further illustrations.[59]
The history of the new cycle of erosion inaugurated by the uplift would
differ from that of the preceding cycle in that the new one would begin with
a drainage system already developed. Other things being equal, therefore,
the reduction of the land would proceed more rapidly in a subsequent cycle
than in the first.
The recognition of different cycles of erosion, separated by uplifts, is
often easy. The principles involved are illustrated by Fig. 155 which
represents an ideal profile of considerable length (say 50 miles). The points
a, a′, and a″ reach a common level. Below them there are areas b, b′, and b″
which have a nearly common elevation, below which are the sharp valleys
d, d′, and d″. The points a, a′, and a″ represent the cross-sections of ridges
formed by the outcrops of layers of hard rock. If the crests of the ridges are
level, the points a, a′, and a″ must represent remnants of an old base-level,
since at no time after a ridge of hard rock becomes deeply notched does it
acquire an even crest, until it is base-leveled.[60] At all earlier stages its crest
is uneven. After the cycle represented by the remnants a, a′, and a″ was
completed, the region suffered uplift. A new cycle represented by the plain
b, b′, and b″ was well advanced, though not completed, when the region
was again elevated, and the rejuvenated streams began to cut their valleys d,
d′, and d″ in the plain of the previous incomplete cycle. The elevations, c
and c′ (intermediate in elevation between a, a′, and a″, and b, b′, and b″)
may represent either remnants of the first base-level plain which were
lowered, but not obliterated, while the plane b, b′, b″ was developing; or
they may represent a cycle intermediate between that during which a, a′, a″
and b, b′, b″ were developed. If the intermediate elevations (c, c′) have a
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common height and level crests, the presumption would be in favor of the
latter interpretation. If they be numerous and of varying heights, as is
possible, they may in the field obscure the planes (a, a′, a″ and b, b′, b″)
developed in the different cycles, which, in the figure, are distinct.
Fig. 155.—Diagram to illustrate cycles of erosion where the beds are tilted.
If the strata involved be horizontal the determination of cycles is
sometimes less easy. Thus in Fig. 156, it is not possible to say whether a
and a′ represent remnants of an old base-level, or whether they represent the
original surface from which degradation started. So, too, the various
benches below a, such as b, b′, and b″ may readily be the result of the
superior hardness of the beds at this level. For the determination of
successive uplifts in the field it is necessary to consider areas of
considerable size, and to eliminate the topographic effects of inequalities of
hardness, and of certain other factors to be mentioned presently.
Fig. 156.—Diagram to illustrate cycles of erosion where the beds are horizontal.
The inequalities in the depths of the young valleys in Figs. 155 and 156
may be explained on the supposition that the deeper ones belong to main
streams, and the shallower ones to tributaries. Such a valley as that shown
at e, Fig. 155, suggests rejuvenation at this point; but farther up the stream
which occupies this valley, rejuvenation might not be apparent. In this case,
the main streams might be flowing in new valleys, d, d′, etc., while the
heads of their tributaries are still flowing in the older valleys of the
preceding cycle (compare Fig. 154 and Fig. 1, Pl. XIII).
It is by the application of the preceding principles that it is known that
the Appalachian Mountains, after being folded, were reduced to a peneplain
(p. 76), throughout their whole extent from the Hudson River to Alabama.
The peneplain level is indicated by the level crests of the Appalachian
ridges, shown in cross profile by the high points of Fig. 157. The system
latter interpretation. If they be numerous and of varying heights, as is
possible, they may in the field obscure the planes (a, a′, a″ and b, b′, b″)
developed in the different cycles, which, in the figure, are distinct.
Fig. 155.—Diagram to illustrate cycles of erosion where the beds are tilted.
If the strata involved be horizontal the determination of cycles is
sometimes less easy. Thus in Fig. 156, it is not possible to say whether a
and a′ represent remnants of an old base-level, or whether they represent the
original surface from which degradation started. So, too, the various
benches below a, such as b, b′, and b″ may readily be the result of the
superior hardness of the beds at this level. For the determination of
successive uplifts in the field it is necessary to consider areas of
considerable size, and to eliminate the topographic effects of inequalities of
hardness, and of certain other factors to be mentioned presently.
Fig. 156.—Diagram to illustrate cycles of erosion where the beds are horizontal.
The inequalities in the depths of the young valleys in Figs. 155 and 156
may be explained on the supposition that the deeper ones belong to main
streams, and the shallower ones to tributaries. Such a valley as that shown
at e, Fig. 155, suggests rejuvenation at this point; but farther up the stream
which occupies this valley, rejuvenation might not be apparent. In this case,
the main streams might be flowing in new valleys, d, d′, etc., while the
heads of their tributaries are still flowing in the older valleys of the
preceding cycle (compare Fig. 154 and Fig. 1, Pl. XIII).
It is by the application of the preceding principles that it is known that
the Appalachian Mountains, after being folded, were reduced to a peneplain
(p. 76), throughout their whole extent from the Hudson River to Alabama.
The peneplain level is indicated by the level crests of the Appalachian
ridges, shown in cross profile by the high points of Fig. 157. The system
Page 221
was then uplifted, and in the cycle of erosion which followed, broad plains
were developed at a new and lower level, corresponding in a general way to
the plains b, b′, and b″ of Fig. 155. The plains were located, for the most
part, where the less resistant strata come to the surface. Above them rose
even-crested ridges, the outcrops of the resistant layers, which had been
isolated by the degradation of the softer beds between. They constitute the
present mountain ridges (the high points of Fig. 157). The evenness of their
crests, testifying to the completeness of the first peneplanation, is shown in
Fig. 158, which represents, diagrammatically, a longitudinal profile of an
Appalachian Mountain ridge. The evenness of the crest is interrupted by (1)
notches (b, c, etc., Fig. 158) cut by the streams in later cycles, and (2) by
occasional elevations above the common level (monadnocks, a, a′, Fig.
158). The monadnocks are generally rather inconspicuous, but there is a
notable group of them in North Carolina and Tennessee. Mount Mitchell
and Roane Mountain are examples. When long distances are considered, the
ridge crests depart somewhat from horizontality. This is believed to be due,
in part at least, to deformations of the old peneplain during the uplift which
inaugurated the second cycle of erosion.
Fig. 157.—Cross-section of a portion of the Appalachian Mountains to illustrate the
phenomena of erosion cycles. (After Rogers.)
Fig. 158.—A diagrammatic longitudinal profile of an Appalachian Mountain ridge.
The extent to which the second cycle of erosion recorded in the present
topography had proceeded before its interruption by uplift, is indicated by
the extent of the valley plains (Fig. 157) below the mountain ridges. While
these plains were being developed on the weak rocks, narrow valleys only
(Fig. 158) were cut in the resistant rocks which now stood out as ridges. In
Fig. 158 some of these valleys are shallow (c, c′, c″, etc.), and but one of
them deep. The former may be either (1) the valleys of streams which
crossed the hard layer at the beginning of the cycle, and which were
diverted before their valleys became deep; or (2) they may represent the
heads of valleys now working back into the ridges. The deep valley (b)
represents the work of a stream which has held its course across the hard
were developed at a new and lower level, corresponding in a general way to
the plains b, b′, and b″ of Fig. 155. The plains were located, for the most
part, where the less resistant strata come to the surface. Above them rose
even-crested ridges, the outcrops of the resistant layers, which had been
isolated by the degradation of the softer beds between. They constitute the
present mountain ridges (the high points of Fig. 157). The evenness of their
crests, testifying to the completeness of the first peneplanation, is shown in
Fig. 158, which represents, diagrammatically, a longitudinal profile of an
Appalachian Mountain ridge. The evenness of the crest is interrupted by (1)
notches (b, c, etc., Fig. 158) cut by the streams in later cycles, and (2) by
occasional elevations above the common level (monadnocks, a, a′, Fig.
158). The monadnocks are generally rather inconspicuous, but there is a
notable group of them in North Carolina and Tennessee. Mount Mitchell
and Roane Mountain are examples. When long distances are considered, the
ridge crests depart somewhat from horizontality. This is believed to be due,
in part at least, to deformations of the old peneplain during the uplift which
inaugurated the second cycle of erosion.
Fig. 157.—Cross-section of a portion of the Appalachian Mountains to illustrate the
phenomena of erosion cycles. (After Rogers.)
Fig. 158.—A diagrammatic longitudinal profile of an Appalachian Mountain ridge.
The extent to which the second cycle of erosion recorded in the present
topography had proceeded before its interruption by uplift, is indicated by
the extent of the valley plains (Fig. 157) below the mountain ridges. While
these plains were being developed on the weak rocks, narrow valleys only
(Fig. 158) were cut in the resistant rocks which now stood out as ridges. In
Fig. 158 some of these valleys are shallow (c, c′, c″, etc.), and but one of
them deep. The former may be either (1) the valleys of streams which
crossed the hard layer at the beginning of the cycle, and which were
diverted before their valleys became deep; or (2) they may represent the
heads of valleys now working back into the ridges. The deep valley (b)
represents the work of a stream which has held its course across the hard
Page 222
layer while the latter was being isolated as a mountain ridge (compare Figs.
131 and 132). Deep narrows of this sort are often called water-gaps. Similar
valleys, whether shallow or deep, from which drainage has been diverted,
are sometimes called wind-gaps. The second cycle of erosion, while still far
from complete, was interrupted by uplift (relative or absolute), and a new
cycle inaugurated. This event was so recent that the new (third) cycle has
not yet advanced far.
Fig. 159.—The Kittatinny Mountains and Delaware Water-Gap from Manunka Chunk.
(N. J. Geol. Surv.)
Recently it has been urged that another cycle, intermediate between the
first and second, is to be recognized.[61]
Some of the features just described are illustrated by Fig. 159. The even
mountain crest in the background is the Kittatinny Mountain of New Jersey
and its continuation in Pennsylvania. In common with other corresponding
crests it represents the oldest recorded base-level (or peneplain) of the
region. The great gap in the mountain is the Delaware Water-Gap. Below
the mountain crest there is another plain, developed in a subsequent cycle of
erosion, while the valley plain in the foreground represents the work of a
still later cycle.
131 and 132). Deep narrows of this sort are often called water-gaps. Similar
valleys, whether shallow or deep, from which drainage has been diverted,
are sometimes called wind-gaps. The second cycle of erosion, while still far
from complete, was interrupted by uplift (relative or absolute), and a new
cycle inaugurated. This event was so recent that the new (third) cycle has
not yet advanced far.
Fig. 159.—The Kittatinny Mountains and Delaware Water-Gap from Manunka Chunk.
(N. J. Geol. Surv.)
Recently it has been urged that another cycle, intermediate between the
first and second, is to be recognized.[61]
Some of the features just described are illustrated by Fig. 159. The even
mountain crest in the background is the Kittatinny Mountain of New Jersey
and its continuation in Pennsylvania. In common with other corresponding
crests it represents the oldest recorded base-level (or peneplain) of the
region. The great gap in the mountain is the Delaware Water-Gap. Below
the mountain crest there is another plain, developed in a subsequent cycle of
erosion, while the valley plain in the foreground represents the work of a
still later cycle.
Page 223
Fig. 160.—Showing certain peculiarities of Appalachian drainage. 1 = the Susquehanna; 2
= the Potomac; 3 = the James; 4 = the Roanoke; 5 = the Coosa; 6 = the Tennessee; 7 = the
Kanawha; 8 = head of New River; 9 = head of the French Broad.
The oldest erosion plain of the Appalachian Mountains, the results of
which are seen in the even-crested ridges so characteristic of the system, is
sometimes called the Kittatinny base-level.[62] It was completed early in the
Cretaceous period, and hence is sometimes known as the Cretaceous base-
level. The next lower plain, imperfectly developed, has been called the
Shenandoah Plain,[62a] from the Shenandoah Valley where it is well seen
(Fig. 132 and Fig. 2, Pl. XII). It is to be noted that the terms base-level and
peneplain have both been used in connection with these old plains. Graded
plain is equally applicable. The truth is that the topographic types
= the Potomac; 3 = the James; 4 = the Roanoke; 5 = the Coosa; 6 = the Tennessee; 7 = the
Kanawha; 8 = head of New River; 9 = head of the French Broad.
The oldest erosion plain of the Appalachian Mountains, the results of
which are seen in the even-crested ridges so characteristic of the system, is
sometimes called the Kittatinny base-level.[62] It was completed early in the
Cretaceous period, and hence is sometimes known as the Cretaceous base-
level. The next lower plain, imperfectly developed, has been called the
Shenandoah Plain,[62a] from the Shenandoah Valley where it is well seen
(Fig. 132 and Fig. 2, Pl. XII). It is to be noted that the terms base-level and
peneplain have both been used in connection with these old plains. Graded
plain is equally applicable. The truth is that the topographic types
Page 224
represented by these three terms grade into one another. It may be
questioned whether definitions should be insisted on which differentiate
these types more sharply than Nature has.
Many of the peculiarities of the drainage of the Appalachian Mountain
system are intimately connected with the history just outlined. Thus three
great rivers, the Delaware, the Susquehanna, and the Potomac, have their
sources west of the Appalachians proper, cross the system in apparent
disregard of the structure, and flow into the Atlantic. The James and
Roanoke head far to the west, although not beyond the mountain system,
and flow eastward, while the New River (leading to the Kanawha) farther
south, heads east of the mountain-folds, and flows northwestward across the
alternating hard and soft beds of the whole Appalachian system, to the Ohio
(Fig. 160). The French Broad, a tributary to the Tennessee, has a similar
course. Such streams are clearly not in structural adjustment, and afford
good opportunities for piracy. Their courses were apparently assumed
during the time of the Kittatinny base-level, when the streams had so low a
gradient as not to be affected by the structure (p. 150). Elevation
rejuvenated them, and they have held their courses in succeeding cycles
across beds of unequal resistance, though smaller streams have become
somewhat thoroughly adjusted. Crustal deformations have also helped them
to hold their courses, for the Cretaceous peneplain seems to have been tilted
to the southeast at its northern end, and to the southwest at its southern,
when the succeeding cycle began.
Streams which hold their early courses in spite of changes which have
taken place since their courses were assumed are said to be antecedent.
They antedate the crustal movements which, but for pre-existent streams,
would have given origin to a different arrangement of river courses. As a
result of crustal movements, therefore, a consequent stream may become
antecedent. Master streams are more likely to hold their courses, and
therefore to become antecedent, than subordinate ones.
The uplift of base-leveled beds, especially if the beds are tilted so as to
bring layers of unequal resistance to the surface at frequent intervals,
affords conditions favorable for extensive adjustment. The numerous wind-
gaps in the mountain ridges, representing the abandoned courses of minor
streams, and the less numerous water-gaps, which indicate the resistance of
large streams to structural adjustment, are instructive witnesses of the extent
questioned whether definitions should be insisted on which differentiate
these types more sharply than Nature has.
Many of the peculiarities of the drainage of the Appalachian Mountain
system are intimately connected with the history just outlined. Thus three
great rivers, the Delaware, the Susquehanna, and the Potomac, have their
sources west of the Appalachians proper, cross the system in apparent
disregard of the structure, and flow into the Atlantic. The James and
Roanoke head far to the west, although not beyond the mountain system,
and flow eastward, while the New River (leading to the Kanawha) farther
south, heads east of the mountain-folds, and flows northwestward across the
alternating hard and soft beds of the whole Appalachian system, to the Ohio
(Fig. 160). The French Broad, a tributary to the Tennessee, has a similar
course. Such streams are clearly not in structural adjustment, and afford
good opportunities for piracy. Their courses were apparently assumed
during the time of the Kittatinny base-level, when the streams had so low a
gradient as not to be affected by the structure (p. 150). Elevation
rejuvenated them, and they have held their courses in succeeding cycles
across beds of unequal resistance, though smaller streams have become
somewhat thoroughly adjusted. Crustal deformations have also helped them
to hold their courses, for the Cretaceous peneplain seems to have been tilted
to the southeast at its northern end, and to the southwest at its southern,
when the succeeding cycle began.
Streams which hold their early courses in spite of changes which have
taken place since their courses were assumed are said to be antecedent.
They antedate the crustal movements which, but for pre-existent streams,
would have given origin to a different arrangement of river courses. As a
result of crustal movements, therefore, a consequent stream may become
antecedent. Master streams are more likely to hold their courses, and
therefore to become antecedent, than subordinate ones.
The uplift of base-leveled beds, especially if the beds are tilted so as to
bring layers of unequal resistance to the surface at frequent intervals,
affords conditions favorable for extensive adjustment. The numerous wind-
gaps in the mountain ridges, representing the abandoned courses of minor
streams, and the less numerous water-gaps, which indicate the resistance of
large streams to structural adjustment, are instructive witnesses of the extent
Page 225
to which adjustment has gone. So extensive has been the adjustment among
the streams of the Appalachian Mountains that there is probably no
considerable stream in the whole system which has not gained or lost
through its own or its neighbors’ piracy. The history of the rivers of the
Appalachian Mountains has been further complicated by a considerable
amount of warping during the periods of uplift.[63]
Fig. 161, 162.—Diagrams to illustrate the effect of crustal warping on stream erosion. The
dotted lines represent the profiles of the streams before deformation; the full lines, after.
Erosion will be stimulated between a and b in each case, and between c and d in Fig. 162.
Below b, Fig. 161, the stream will be drowned, and erosion therefore stopped. Erosion
will also be stopped or retarded above a, between b and c, and below d in Fig. 162.
Sinking.—The land on which a river system is developed may be
depressed relative to sea-level. In this case the sea would occupy the lower
ends of valleys, converting them into bays and estuaries. A stream in this
condition is said to be drowned. Of drowned rivers there are many
examples along the Atlantic coast. Thus the St. Lawrence River is drowned
up to Montreal, and the Hudson up to Albany. If the drowned portion of the
latter valley were not so narrow, it would be a bay. Delaware and
Chesapeake Bays, as well as many smaller ones, both north and south, are
likewise the drowned ends of river valleys (see figures, Chapter VI). If all
parts of a drainage basin sank equally, the velocities of the streams above
the limit of drowning would not be changed, for the gradients would remain
the same as before. The fact that a river’s channel is below sea-level is not
to be taken as proof that the valley is drowned. Thus the bottom of the
channel of the Mississippi is as much as 100 feet below the level of the
Gulf, some 20 miles above New Orleans.[64]
the streams of the Appalachian Mountains that there is probably no
considerable stream in the whole system which has not gained or lost
through its own or its neighbors’ piracy. The history of the rivers of the
Appalachian Mountains has been further complicated by a considerable
amount of warping during the periods of uplift.[63]
Fig. 161, 162.—Diagrams to illustrate the effect of crustal warping on stream erosion. The
dotted lines represent the profiles of the streams before deformation; the full lines, after.
Erosion will be stimulated between a and b in each case, and between c and d in Fig. 162.
Below b, Fig. 161, the stream will be drowned, and erosion therefore stopped. Erosion
will also be stopped or retarded above a, between b and c, and below d in Fig. 162.
Sinking.—The land on which a river system is developed may be
depressed relative to sea-level. In this case the sea would occupy the lower
ends of valleys, converting them into bays and estuaries. A stream in this
condition is said to be drowned. Of drowned rivers there are many
examples along the Atlantic coast. Thus the St. Lawrence River is drowned
up to Montreal, and the Hudson up to Albany. If the drowned portion of the
latter valley were not so narrow, it would be a bay. Delaware and
Chesapeake Bays, as well as many smaller ones, both north and south, are
likewise the drowned ends of river valleys (see figures, Chapter VI). If all
parts of a drainage basin sank equally, the velocities of the streams above
the limit of drowning would not be changed, for the gradients would remain
the same as before. The fact that a river’s channel is below sea-level is not
to be taken as proof that the valley is drowned. Thus the bottom of the
channel of the Mississippi is as much as 100 feet below the level of the
Gulf, some 20 miles above New Orleans.[64]
Page 226
Differential movement. Warping.—Where a land surface on which a
river system is established suffers warping, some parts going up and others
down, the opposite movements being either absolute or relative, various
phenomena would result. This may be illustrated by the accompanying
diagrams (Figs. 161 and 162), where the profiles of the streams are
represented as warped from the positions represented by the dotted lines, to
the positions shown by the full lines. The velocity will be accelerated below
the points of differential elevation (between a and b, Fig. 161, and between
a and b, and c and d, Fig. 162), but checked above (above a, and between b
and c, Fig. 162). Above an elevation which notably checks its flow, a stream
is ponded. If the ponding is slight, a marsh may develop above the
obstruction; if more considerable, a lake is formed. Lakes of this class are
likely to be short-lived, since the ponded waters are likely to soon overflow
and lower their outlet so as to drain the lake. The elevation which ponds the
stream may be great enough and rapid enough so that the resulting lake
finds an outlet by some course other than that originally followed by the
stream. Where a stream holds its course across an uplift athwart its valley,
either with or without ponding, it becomes an antecedent stream (see p.
169), since it has a course assumed before the latest deformation of the
crust and in apparent disregard of present surface configuration. Thus the
Columbia River holds its antecedent course across areas which have been
uplifted (differentially) hundreds and even thousands of feet.[65] Some of the
striking scenic features of this noble valley are the result of these changes in
the country through which it flows. A lesser stream would have been
diverted, as many of its tributaries have been. Even its course across the
Cascade ranges is believed to be antecedent.[66]
river system is established suffers warping, some parts going up and others
down, the opposite movements being either absolute or relative, various
phenomena would result. This may be illustrated by the accompanying
diagrams (Figs. 161 and 162), where the profiles of the streams are
represented as warped from the positions represented by the dotted lines, to
the positions shown by the full lines. The velocity will be accelerated below
the points of differential elevation (between a and b, Fig. 161, and between
a and b, and c and d, Fig. 162), but checked above (above a, and between b
and c, Fig. 162). Above an elevation which notably checks its flow, a stream
is ponded. If the ponding is slight, a marsh may develop above the
obstruction; if more considerable, a lake is formed. Lakes of this class are
likely to be short-lived, since the ponded waters are likely to soon overflow
and lower their outlet so as to drain the lake. The elevation which ponds the
stream may be great enough and rapid enough so that the resulting lake
finds an outlet by some course other than that originally followed by the
stream. Where a stream holds its course across an uplift athwart its valley,
either with or without ponding, it becomes an antecedent stream (see p.
169), since it has a course assumed before the latest deformation of the
crust and in apparent disregard of present surface configuration. Thus the
Columbia River holds its antecedent course across areas which have been
uplifted (differentially) hundreds and even thousands of feet.[65] Some of the
striking scenic features of this noble valley are the result of these changes in
the country through which it flows. A lesser stream would have been
diverted, as many of its tributaries have been. Even its course across the
Cascade ranges is believed to be antecedent.[66]
Page 227
Fig. 163, 164.—Piracy stimulated by warping. Uplift along axis 1–2.
Another peculiarity of valleys and streams resulting from changes of
level is illustrated in Fig. 2, Pl. XIV (southern California). The main valleys
of this part of the coast were developed when the land stood considerably
higher than now. Later the subsidence of the coast converted the lower ends
of the valleys into bays or fiords. The bays were then transformed into
lagoons by deposition. Subsequent rise of the land or depression of the sea
allowed the drainage from the old lagoons to cut across the deposits which
had converted the bays into lagoons. The result is an old, wide valley above,
suggested by a young one below.
Another peculiarity of valleys and streams resulting from changes of
level is illustrated in Fig. 2, Pl. XIV (southern California). The main valleys
of this part of the coast were developed when the land stood considerably
higher than now. Later the subsidence of the coast converted the lower ends
of the valleys into bays or fiords. The bays were then transformed into
lagoons by deposition. Subsequent rise of the land or depression of the sea
allowed the drainage from the old lagoons to cut across the deposits which
had converted the bays into lagoons. The result is an old, wide valley above,
suggested by a young one below.
Page 228
If the warpings were considerable, much more decisive changes in
drainage would result. Suppose the drainage of a given region to be
represented by the streams in Fig. 163. If there is uplift along the axis 1–2,
that part of ac above the axis of uplift would be ponded, or at least have its
velocity checked, while the flow of some of the tributaries of d would be
accelerated, and might work back and capture the other stream (Fig. 164).
Crustal warping was one of the conditions under which the Tennessee
achieved its present anomalous course, and its history[67] is illustrative of the
complex changes which drainage suffers when warping affects the area
where the rock structures are of unequal resistance. At the close of the
Cretaceous cycle of erosion, when the Appalachian Mountains had been
reduced to a peneplain, the waters falling in the area now drained by the
upper course of the Tennessee flowed south-south-west to the Gulf in a
stream (the Appalachian River, a, Fig. 165) the lower part of which had the
general position of the Coosa and the Alabama.
To the west of the Appalachian River, shorter streams flowed west and
southwest into the Mississippi embayment (Fig. 165) by courses which are
not now definitely known. The succeeding cycle of erosion was inaugurated
by uplift and deformation of the peneplain. The axis of greatest elevation
(AB, Fig. 166) was nearly parallel to the Appalachian River, and the effect
of the differential uplift was to impose a greater task on this river (a, Fig.
166), which flowed along the axis of uplift, than upon the rivers which
flowed westward and southwestward to the Mississippi embayment. The
result was that the strongest of the southwesterly flowing streams worked
its head back into the drainage basin of the Appalachian River, and
captured, one by one, the head-waters of its westerly tributaries,
establishing some such drainage relations as are shown in Fig. 166. Still
later, after the land area of the region had been considerably extended by
the withdrawal of the sea, the Appalachian River itself was reached by the
invading stream, and its waters carried away to the Mississippi Bay by a
course the lower part of which is thought to have corresponded
approximately with the course of the present Black River (b, Fig. 167).
drainage would result. Suppose the drainage of a given region to be
represented by the streams in Fig. 163. If there is uplift along the axis 1–2,
that part of ac above the axis of uplift would be ponded, or at least have its
velocity checked, while the flow of some of the tributaries of d would be
accelerated, and might work back and capture the other stream (Fig. 164).
Crustal warping was one of the conditions under which the Tennessee
achieved its present anomalous course, and its history[67] is illustrative of the
complex changes which drainage suffers when warping affects the area
where the rock structures are of unequal resistance. At the close of the
Cretaceous cycle of erosion, when the Appalachian Mountains had been
reduced to a peneplain, the waters falling in the area now drained by the
upper course of the Tennessee flowed south-south-west to the Gulf in a
stream (the Appalachian River, a, Fig. 165) the lower part of which had the
general position of the Coosa and the Alabama.
To the west of the Appalachian River, shorter streams flowed west and
southwest into the Mississippi embayment (Fig. 165) by courses which are
not now definitely known. The succeeding cycle of erosion was inaugurated
by uplift and deformation of the peneplain. The axis of greatest elevation
(AB, Fig. 166) was nearly parallel to the Appalachian River, and the effect
of the differential uplift was to impose a greater task on this river (a, Fig.
166), which flowed along the axis of uplift, than upon the rivers which
flowed westward and southwestward to the Mississippi embayment. The
result was that the strongest of the southwesterly flowing streams worked
its head back into the drainage basin of the Appalachian River, and
captured, one by one, the head-waters of its westerly tributaries,
establishing some such drainage relations as are shown in Fig. 166. Still
later, after the land area of the region had been considerably extended by
the withdrawal of the sea, the Appalachian River itself was reached by the
invading stream, and its waters carried away to the Mississippi Bay by a
course the lower part of which is thought to have corresponded
approximately with the course of the present Black River (b, Fig. 167).
Page 229
Fig. 165.—Shows the general position of the main drainage lines in the southern
Appalachians at the close of the Cretaceous cycle of erosion. The lower part of stream b is
made to follow the course of a portion of the present Tennessee.
Appalachians at the close of the Cretaceous cycle of erosion. The lower part of stream b is
made to follow the course of a portion of the present Tennessee.
Page 230
Fig. 166.—Shows the general position of the main drainage lines in the southern
Appalachians, after the capture of the westerly tributaries of the Appalachian River by
stream b. Compare Fig. 165.
Appalachians, after the capture of the westerly tributaries of the Appalachian River by
stream b. Compare Fig. 165.
Page 231
Fig. 167.—A stage later than that shown in Fig. 166. The sea is represented as having
withdrawn from a considerable area which was submerged at earlier stages (Figs. 165,
166).
withdrawn from a considerable area which was submerged at earlier stages (Figs. 165,
166).
Page 232
Fig. 168.—Shows the final change which resulted in the present course of the Tennessee.
The land is represented as somewhat higher than now.[68]
Still later there was further deformation which caused additional changes
in the drainage. The whole region was uplifted, relatively if not absolutely,
but the uplift was differential, being greatest along the axis represented by
AB, Fig. 167. The effect of the deformation was to stimulate the tributaries
of the Ohio flowing north from this axis. Their growth was further
accelerated by the weakness of the strata over which they ran. At the same
time, the uplift to the south led the southwesterly flowing stream (b, Fig.
167) to discover relatively hard beds of rock in its lower course, and these
The land is represented as somewhat higher than now.[68]
Still later there was further deformation which caused additional changes
in the drainage. The whole region was uplifted, relatively if not absolutely,
but the uplift was differential, being greatest along the axis represented by
AB, Fig. 167. The effect of the deformation was to stimulate the tributaries
of the Ohio flowing north from this axis. Their growth was further
accelerated by the weakness of the strata over which they ran. At the same
time, the uplift to the south led the southwesterly flowing stream (b, Fig.
167) to discover relatively hard beds of rock in its lower course, and these
Page 233
beds retarded its down-cutting. The result was that a tributary of the Ohio
(a, Fig. 167) finally tapped the main stream flowing to the southwest (b,
Fig. 167) and carried its upper part over to the Ohio (Fig. 168). This was the
beginning of the present Tennessee.
THE AGGRADATIONAL WORK OF RUNNING WATER.
Principles involved.—Since deposition results from the failure of
transportation, the factors which control transportation also influence
deposition. Transportation by streams is determined largely by velocity, and
the most important factors influencing velocity are slope, volume, and load
(p. 115). Of these the first two are usually of greater importance than the
third.
A stream is said to be loaded when it has all the sediment it can carry; it
is loaded with fine material when it has all the fine material it can carry, and
with coarse material when it has all the coarse it can transport. A stream
loaded with coarse material flows more swiftly than one loaded with fine,
for a larger percentage of a stream’s energy can be utilized in carrying fine
material than coarse, and hence a larger percentage of the energy of a
stream which carries a load of the latter will express itself in velocity.
Deposition takes place whenever a stream finds itself with more load
than it can carry, and is an expression of the stream’s refusal to remain
overloaded. A stream may become overloaded in various ways. It might at
first seem unnecessary to inquire whether a stream may be overloaded at its
source, but the question is not necessarily to be answered in the negative.
The source of a stream is not always a definite point. In a general way it
may be said that the source of the normal stream is at that point in its valley
where the bottom is as low as the ground-water level of the region. But
since the ground-water level is not constant (p. 71) the source of a stream is
likely to be farther up its valley in a wet season than in a dry one (p. 72).
After a heavy shower, the run-off descends to the axis of the valley from the
slopes on all sides, and temporarily the stream begins above the point which
marks even its wet-season source. If under such circumstances the slopes
about the head of the valley are notably steeper than the slope of the valley
itself, as they frequently are, the water flowing down them may gather an
amount of material which it cannot carry after it reaches the bottom of the
(a, Fig. 167) finally tapped the main stream flowing to the southwest (b,
Fig. 167) and carried its upper part over to the Ohio (Fig. 168). This was the
beginning of the present Tennessee.
THE AGGRADATIONAL WORK OF RUNNING WATER.
Principles involved.—Since deposition results from the failure of
transportation, the factors which control transportation also influence
deposition. Transportation by streams is determined largely by velocity, and
the most important factors influencing velocity are slope, volume, and load
(p. 115). Of these the first two are usually of greater importance than the
third.
A stream is said to be loaded when it has all the sediment it can carry; it
is loaded with fine material when it has all the fine material it can carry, and
with coarse material when it has all the coarse it can transport. A stream
loaded with coarse material flows more swiftly than one loaded with fine,
for a larger percentage of a stream’s energy can be utilized in carrying fine
material than coarse, and hence a larger percentage of the energy of a
stream which carries a load of the latter will express itself in velocity.
Deposition takes place whenever a stream finds itself with more load
than it can carry, and is an expression of the stream’s refusal to remain
overloaded. A stream may become overloaded in various ways. It might at
first seem unnecessary to inquire whether a stream may be overloaded at its
source, but the question is not necessarily to be answered in the negative.
The source of a stream is not always a definite point. In a general way it
may be said that the source of the normal stream is at that point in its valley
where the bottom is as low as the ground-water level of the region. But
since the ground-water level is not constant (p. 71) the source of a stream is
likely to be farther up its valley in a wet season than in a dry one (p. 72).
After a heavy shower, the run-off descends to the axis of the valley from the
slopes on all sides, and temporarily the stream begins above the point which
marks even its wet-season source. If under such circumstances the slopes
about the head of the valley are notably steeper than the slope of the valley
itself, as they frequently are, the water flowing down them may gather an
amount of material which it cannot carry after it reaches the bottom of the
Page 234
valley. This may be the case at, or even above, the point which marks the
source of the permanent stream. It is, therefore, possible for a stream to be
overloaded at its source, if we take the source to be the point whence the
water permanently flows. Deposition may, therefore, be taking place in a
valley at the head of its permanent stream, or temporarily even in the valley
above it.
Streams issuing from glaciers sometimes have more load than they can
carry after they escape from the ice. If the stream be regarded as beginning
at the point where it issues from beneath the ice it may be overloaded at its
source.[69]
Under certain circumstances, a stream may overload itself. Thus if a
stream loaded with coarse detritus reaches a portion of its valley where fine
material is accessible in abundance, some of the velocity which is helping
to carry the coarse may be used in picking up and carrying the fine. This
reduces the velocity, and since the stream already had all the coarse material
it could carry, reduction of velocity must result in deposition. It follows that
when a stream fully loaded with coarse material picks up fine, it becomes
overloaded, so far as the coarse material is concerned.
Again, tributaries may overload their mains. While tributaries are usually
smaller than their mains, they frequently have higher gradients, and the
smaller stream of higher gradient may bring to the larger stream of lower
gradient more material than the latter can carry away. Thus deposition may
take place at the point of junction of tributaries with their mains. This may
go so far as to pond the latter enough to cause its expansion into a river-
lake. Lake Pepin, in the Mississippi River at the mouth of the Chippewa (in
Wis.), is an example.
Streams may become overloaded by losing velocity or volume, or both.
Decrease in velocity is brought about either by decrease in declivity or in
volume. In general, streams have lower gradients and greater volumes in
their lower courses than in their upper, and these two elements affect
velocity in different ways. If the increase in volume be not enough to
counterbalance the decrease in declivity, as is often the case, a stream which
is loaded in its upper course will deposit in its lower. The decrease of
velocity at the debouchure of a stream almost always leads to deposition.
source of the permanent stream. It is, therefore, possible for a stream to be
overloaded at its source, if we take the source to be the point whence the
water permanently flows. Deposition may, therefore, be taking place in a
valley at the head of its permanent stream, or temporarily even in the valley
above it.
Streams issuing from glaciers sometimes have more load than they can
carry after they escape from the ice. If the stream be regarded as beginning
at the point where it issues from beneath the ice it may be overloaded at its
source.[69]
Under certain circumstances, a stream may overload itself. Thus if a
stream loaded with coarse detritus reaches a portion of its valley where fine
material is accessible in abundance, some of the velocity which is helping
to carry the coarse may be used in picking up and carrying the fine. This
reduces the velocity, and since the stream already had all the coarse material
it could carry, reduction of velocity must result in deposition. It follows that
when a stream fully loaded with coarse material picks up fine, it becomes
overloaded, so far as the coarse material is concerned.
Again, tributaries may overload their mains. While tributaries are usually
smaller than their mains, they frequently have higher gradients, and the
smaller stream of higher gradient may bring to the larger stream of lower
gradient more material than the latter can carry away. Thus deposition may
take place at the point of junction of tributaries with their mains. This may
go so far as to pond the latter enough to cause its expansion into a river-
lake. Lake Pepin, in the Mississippi River at the mouth of the Chippewa (in
Wis.), is an example.
Streams may become overloaded by losing velocity or volume, or both.
Decrease in velocity is brought about either by decrease in declivity or in
volume. In general, streams have lower gradients and greater volumes in
their lower courses than in their upper, and these two elements affect
velocity in different ways. If the increase in volume be not enough to
counterbalance the decrease in declivity, as is often the case, a stream which
is loaded in its upper course will deposit in its lower. The decrease of
velocity at the debouchure of a stream almost always leads to deposition.
Page 235
Decrease in velocity as the result of decrease in volume is less common.
When decrease in volume occurs, it may be the result of (1) evaporation, (2)
the absorption of water into the bed of the stream, or (3) branching—the
giving off of distributaries. While evaporation is going on everywhere, the
diminution of a stream by this means is usually more than balanced by the
increase from tributaries, rainfall, and springs; but in arid regions a very
different condition of things sometimes exists. If mountains in an arid
region be capped with snow, its melting supplies the streams during the
melting season. As the streams flow out from the mountains through dry
regions, they receive little or no increment from rainfall, tributaries, or
springs, and evaporation reduces the volume of water, or even dissipates it
altogether. Absorption of water into the bed of the stream often
accompanies evaporation. Reduction of volume by evaporation and by
absorption is especially common in arid regions. Wherever loaded streams
are reduced in volume, whether by evaporation or absorption, deposition
takes place.
The third way by which velocity is decreased as the result of decreasing
volume is illustrated at the debouchures of many streams. Near the Gulf, for
example, the Mississippi branches repeatedly (see Fig. 190). The same
phenomena are often seen where one stream joins another (Fig. 169).
Individually the distributaries are much smaller than the main stream before
they separated from it, and because they are smaller their combined
surfaces are greater, and the amount of energy consumed in the friction of
flow is increased. The velocity of the water and its carrying power are,
therefore, reduced. Thus the branching of streams gives rise to deposition,
and where deposition takes place the gradient of the stream is reduced, and
this occasions still further deposition. The sediment which fills up the
channel and checks the flow finally compels the stream, or some part of it,
to transgress its banks. Deposition, therefore, favors the development of
distributaries, and the development of distributaries in turn favors
deposition.
When decrease in volume occurs, it may be the result of (1) evaporation, (2)
the absorption of water into the bed of the stream, or (3) branching—the
giving off of distributaries. While evaporation is going on everywhere, the
diminution of a stream by this means is usually more than balanced by the
increase from tributaries, rainfall, and springs; but in arid regions a very
different condition of things sometimes exists. If mountains in an arid
region be capped with snow, its melting supplies the streams during the
melting season. As the streams flow out from the mountains through dry
regions, they receive little or no increment from rainfall, tributaries, or
springs, and evaporation reduces the volume of water, or even dissipates it
altogether. Absorption of water into the bed of the stream often
accompanies evaporation. Reduction of volume by evaporation and by
absorption is especially common in arid regions. Wherever loaded streams
are reduced in volume, whether by evaporation or absorption, deposition
takes place.
The third way by which velocity is decreased as the result of decreasing
volume is illustrated at the debouchures of many streams. Near the Gulf, for
example, the Mississippi branches repeatedly (see Fig. 190). The same
phenomena are often seen where one stream joins another (Fig. 169).
Individually the distributaries are much smaller than the main stream before
they separated from it, and because they are smaller their combined
surfaces are greater, and the amount of energy consumed in the friction of
flow is increased. The velocity of the water and its carrying power are,
therefore, reduced. Thus the branching of streams gives rise to deposition,
and where deposition takes place the gradient of the stream is reduced, and
this occasions still further deposition. The sediment which fills up the
channel and checks the flow finally compels the stream, or some part of it,
to transgress its banks. Deposition, therefore, favors the development of
distributaries, and the development of distributaries in turn favors
deposition.
Page 236
Fig. 169.—Delta of the Chelan River at its junction with the Columbia. Shows the tendency
of streams to distribute where active deposition is in progress. (Willis, U. S. Geol. Surv.
The foregoing statements make it clear that a stream may be eroding in
one part of its valley while it is depositing in another, and that erosion may
alternate with deposition in the same place, on account of fluctuations in
volume, and, therefore, in velocity of the stream. It will be seen in the
sequel that erosion and deposition may be taking place at the same time in
the same part of the valley. The activities of a river are so nicely balanced
that slight disturbance at one point causes disturbance at all points below.
The deposits.
Types.—Turning from the principles which underlie river deposition to
the deposits themselves, they are found to occur in various situations.
Running water usually descends from steeper slopes above to gentler slopes
below, and ends at the sea, or in a lake or inland basin. Wherever there is a
sudden decrease in its gradient, as at the base of a hill, ridge, or mountain,
running water is likely to leave a large part of its load, building an alluvial
fan or cone (Figs. 67, 68, and Pl. VI). Even where there is no sudden
decrease in the gradient of a stream, there is likely to be a gradual one, and
in spite of the fact that the increased volume of a stream in its lower course
tends to overcome the effect of diminished gradient on velocity, deposition
is likely to take place as the gradient is reduced. Deposits occasioned by the
gradual reduction of a stream’s velocity often have great extent in the
of streams to distribute where active deposition is in progress. (Willis, U. S. Geol. Surv.
The foregoing statements make it clear that a stream may be eroding in
one part of its valley while it is depositing in another, and that erosion may
alternate with deposition in the same place, on account of fluctuations in
volume, and, therefore, in velocity of the stream. It will be seen in the
sequel that erosion and deposition may be taking place at the same time in
the same part of the valley. The activities of a river are so nicely balanced
that slight disturbance at one point causes disturbance at all points below.
The deposits.
Types.—Turning from the principles which underlie river deposition to
the deposits themselves, they are found to occur in various situations.
Running water usually descends from steeper slopes above to gentler slopes
below, and ends at the sea, or in a lake or inland basin. Wherever there is a
sudden decrease in its gradient, as at the base of a hill, ridge, or mountain,
running water is likely to leave a large part of its load, building an alluvial
fan or cone (Figs. 67, 68, and Pl. VI). Even where there is no sudden
decrease in the gradient of a stream, there is likely to be a gradual one, and
in spite of the fact that the increased volume of a stream in its lower course
tends to overcome the effect of diminished gradient on velocity, deposition
is likely to take place as the gradient is reduced. Deposits occasioned by the
gradual reduction of a stream’s velocity often have great extent in the
Page 237
direction of a stream’s flow. They cover the flood plains of streams, making
them alluvial plains (Fig. 73). When a stream reaches the sea or a lake its
current is destroyed and its load dropped, unless taken in charge by the
waves and currents of the standing water. Sediment accumulated in quantity
at the debouchures of streams gives rise to deltas (Figs. 169, 187). Alluvial
cones and fans, alluvial plains, and deltas, are the principal types of river
deposits. Apart from these well-defined types there are bars in the channels
of depositing streams, and much ill-defined alluvium which does not allow
of ready classification.
Alluvial fans and cones.—The only distinction between the alluvial fan
and the alluvial cone is one of slope, the cones (they are but half-cones at
best) being steeper than the fans. Alluvial fans and cones have their most
striking development where temporary torrents, occasioned by showers or
the rapid melting of snow, issue from mountain ravines. Such streams
usually carry heavy loads of detritus, the coarser part of which is likely to
be deposited at the base of the mountain slope. Cones and fans built by such
streams have a periodic rather than a steady growth.
At the beginning of its development the material of the alluvial cone is
deposited much as in a talus cone (compare Fig. 170 with Figs. 67 and 68).
Its deposition chokes the channel of the stream, and some of the water then
seeks new courses to right and left of the apex of the deposit. This expands
the area of deposition to right and left, while the water which flows over it
lengthens it in the direction of flow.
The course and behavior of the water after reaching an alluvial cone is
instructive. As its velocity is checked, deposition often takes place in the
channel, diminishing its capacity. As the channel is filled up, the water
tends to overflow on either side. The overflowing water, being shallow, has
so little velocity that much of its load is dropped on either margin of the
channel, building up levees. The water ever and anon breaks through the
levees, giving rise to distributary streams, each of which aggrades its
channel and builds its own miniature levees (Fig. 171). Not rarely this
process of channel-filling and levee-building goes on until the channels of
the little rivulets are above the general level of the cone on which they rest.
The rivulet then runs in a groove on the crest of a little ridge. The channels
on the surfaces of fans and cones are fewest and deepest at their heads, and
more numerous and shallower below. In some cases the surface-water
them alluvial plains (Fig. 73). When a stream reaches the sea or a lake its
current is destroyed and its load dropped, unless taken in charge by the
waves and currents of the standing water. Sediment accumulated in quantity
at the debouchures of streams gives rise to deltas (Figs. 169, 187). Alluvial
cones and fans, alluvial plains, and deltas, are the principal types of river
deposits. Apart from these well-defined types there are bars in the channels
of depositing streams, and much ill-defined alluvium which does not allow
of ready classification.
Alluvial fans and cones.—The only distinction between the alluvial fan
and the alluvial cone is one of slope, the cones (they are but half-cones at
best) being steeper than the fans. Alluvial fans and cones have their most
striking development where temporary torrents, occasioned by showers or
the rapid melting of snow, issue from mountain ravines. Such streams
usually carry heavy loads of detritus, the coarser part of which is likely to
be deposited at the base of the mountain slope. Cones and fans built by such
streams have a periodic rather than a steady growth.
At the beginning of its development the material of the alluvial cone is
deposited much as in a talus cone (compare Fig. 170 with Figs. 67 and 68).
Its deposition chokes the channel of the stream, and some of the water then
seeks new courses to right and left of the apex of the deposit. This expands
the area of deposition to right and left, while the water which flows over it
lengthens it in the direction of flow.
The course and behavior of the water after reaching an alluvial cone is
instructive. As its velocity is checked, deposition often takes place in the
channel, diminishing its capacity. As the channel is filled up, the water
tends to overflow on either side. The overflowing water, being shallow, has
so little velocity that much of its load is dropped on either margin of the
channel, building up levees. The water ever and anon breaks through the
levees, giving rise to distributary streams, each of which aggrades its
channel and builds its own miniature levees (Fig. 171). Not rarely this
process of channel-filling and levee-building goes on until the channels of
the little rivulets are above the general level of the cone on which they rest.
The rivulet then runs in a groove on the crest of a little ridge. The channels
on the surfaces of fans and cones are fewest and deepest at their heads, and
more numerous and shallower below. In some cases the surface-water
Page 238
disappears altogether before the outer border of the fan is reached, by
sinking into the débris.
Fig. 170.—A talus cone. North Greenland Coast. The talus cone reaches the sea-level.
Drawn from photograph.
Alluvial fans and cones have various forms, and often attain considerable
dimensions. Their angles of slope depend on the amount of reduction of
velocity which the depositing water suffers, and the amount and kind of
load which it carries. The maximum slope of the cone is the angle at which
the loose material involved will lie. The minimum slope of the fan, on the
other hand, approaches horizontality. If many alluvial fans develop in
proximity to one another, as at the base of a mountain range, they may
expand laterally until they merge. A long succession of them may thus give
rise to an extensive alluvial piedmont plain, or a compound alluvial fan.
The lower edge of such a fan is often somewhat lobate. Such plains exist
along the bases of many mountain ranges (Pl. VI), and may be seen in
miniature even along low ridges.
sinking into the débris.
Fig. 170.—A talus cone. North Greenland Coast. The talus cone reaches the sea-level.
Drawn from photograph.
Alluvial fans and cones have various forms, and often attain considerable
dimensions. Their angles of slope depend on the amount of reduction of
velocity which the depositing water suffers, and the amount and kind of
load which it carries. The maximum slope of the cone is the angle at which
the loose material involved will lie. The minimum slope of the fan, on the
other hand, approaches horizontality. If many alluvial fans develop in
proximity to one another, as at the base of a mountain range, they may
expand laterally until they merge. A long succession of them may thus give
rise to an extensive alluvial piedmont plain, or a compound alluvial fan.
The lower edge of such a fan is often somewhat lobate. Such plains exist
along the bases of many mountain ranges (Pl. VI), and may be seen in
miniature even along low ridges.
Page 239
Fig. 171.—Miniature levees on an alluvial cone. Slope of Gray Peak, Colo. (R. T.
Chamberlin.)
A permanent stream, as well as a temporary one, may develop an alluvial
fan at the base of a mountain slope; but since the mountain course of the
former is likely to be less steep than that of the latter, its waters suffer a
correspondingly less reduction of velocity at any one point. The fan of the
permanent stream is therefore likely to be relatively flat, and to stretch far
down the valley. Such fans grade into valley plains. From the general
principles already discussed, it is clear that well-developed fans go with
relatively youthful stages of erosion, and belong normally to the upper parts
of drainage lines.
Ill-defined alluvium.—There is a widespread mantle of alluvial material
deposited by running water which was not organized into distinct streams.
The water which runs down smooth slopes in sheets during showers carries
fine earthy matter, as well as some that is coarser. These materials are
largely deposited at the bases of the slopes, forming basal accumulations of
greater or less extent, comparable in origin to alluvial fans. A relatively
small amount of the slope wash is carried far out from the base of the
declivities. It is not easy to realize the extent to which this process is taking
place. There is hardly a slope without loose material, and there is hardly an
acre of low land below a slope on which running water has not deposited
Chamberlin.)
A permanent stream, as well as a temporary one, may develop an alluvial
fan at the base of a mountain slope; but since the mountain course of the
former is likely to be less steep than that of the latter, its waters suffer a
correspondingly less reduction of velocity at any one point. The fan of the
permanent stream is therefore likely to be relatively flat, and to stretch far
down the valley. Such fans grade into valley plains. From the general
principles already discussed, it is clear that well-developed fans go with
relatively youthful stages of erosion, and belong normally to the upper parts
of drainage lines.
Ill-defined alluvium.—There is a widespread mantle of alluvial material
deposited by running water which was not organized into distinct streams.
The water which runs down smooth slopes in sheets during showers carries
fine earthy matter, as well as some that is coarser. These materials are
largely deposited at the bases of the slopes, forming basal accumulations of
greater or less extent, comparable in origin to alluvial fans. A relatively
small amount of the slope wash is carried far out from the base of the
declivities. It is not easy to realize the extent to which this process is taking
place. There is hardly a slope without loose material, and there is hardly an
acre of low land below a slope on which running water has not deposited
Page 240
sediment washed down from above. When it is remembered that this is as
true of gentle slopes and their surroundings as of steep slopes, though
perhaps not to the same extent, and that a very large part of the earth’s
surface is made up of sensible slopes, or of flats at their bases, some idea of
the aggregate effect may be gained.
There is another way of looking at the same question. Earthy matter is
being continually transferred from land to sea, and chiefly from high land.
Rarely does it start from any point distant from the shore and move
uninterruptedly to it. It is transported a short distance and lodged, to be
again picked up, carried forward another step in its journey, and lodged
again. For a very large part of the earth’s surface it would be true to say that
its mantle rock is material in transit from higher land to the sea.
Alluvial plains.—Most streams, whether heading in mountains or not,
have gentler gradients in their lower courses than in their upper, and in spite
of increasing volume are usually unable to carry to their debouchures all the
material gathered above. The excess of load is dropped chiefly on the flood-
plains of the streams and constitutes them alluvial plains.
The making of an alluvial plain usually involves both erosion and
deposition. When a stream has cut its channel to grade, downward erosion
ceases, or more exactly, downward cutting is, on the average,
counterbalanced by deposition. So long as a stream is cutting downward
rapidly, it carries away whatever débris descends the side slopes. When it
approaches grade, the débris which descends the side slopes tends to
accumulate at their bases, and the V-shaped cross-section of the valley
becomes U-shaped (see Fig. 172). At about the same time the stream begins
to meander, for, having lost something of its former velocity, it is more
easily turned from side to side. As it begins to meander, it widens the
bottom of its valley. This is the initial stage in the development of the valley
flat (2 and 3, Fig. 172). In its meandering the stream encroaches on the talus
accumulations at the bases of its valley’s slopes. The side-cutting may
remove all the loose débris and even undercut the bluff as at a, Fig. 173.
The stream’s meanders shift their positions from time to time so that the
valley flat is successively widened at different points. By lateral planation,
therefore, a stream tends to develop a flat as soon as it reaches grade. This
is the initial part of erosion in the making of a river flat, but a flat developed
by erosion alone is not an alluvial plain.
true of gentle slopes and their surroundings as of steep slopes, though
perhaps not to the same extent, and that a very large part of the earth’s
surface is made up of sensible slopes, or of flats at their bases, some idea of
the aggregate effect may be gained.
There is another way of looking at the same question. Earthy matter is
being continually transferred from land to sea, and chiefly from high land.
Rarely does it start from any point distant from the shore and move
uninterruptedly to it. It is transported a short distance and lodged, to be
again picked up, carried forward another step in its journey, and lodged
again. For a very large part of the earth’s surface it would be true to say that
its mantle rock is material in transit from higher land to the sea.
Alluvial plains.—Most streams, whether heading in mountains or not,
have gentler gradients in their lower courses than in their upper, and in spite
of increasing volume are usually unable to carry to their debouchures all the
material gathered above. The excess of load is dropped chiefly on the flood-
plains of the streams and constitutes them alluvial plains.
The making of an alluvial plain usually involves both erosion and
deposition. When a stream has cut its channel to grade, downward erosion
ceases, or more exactly, downward cutting is, on the average,
counterbalanced by deposition. So long as a stream is cutting downward
rapidly, it carries away whatever débris descends the side slopes. When it
approaches grade, the débris which descends the side slopes tends to
accumulate at their bases, and the V-shaped cross-section of the valley
becomes U-shaped (see Fig. 172). At about the same time the stream begins
to meander, for, having lost something of its former velocity, it is more
easily turned from side to side. As it begins to meander, it widens the
bottom of its valley. This is the initial stage in the development of the valley
flat (2 and 3, Fig. 172). In its meandering the stream encroaches on the talus
accumulations at the bases of its valley’s slopes. The side-cutting may
remove all the loose débris and even undercut the bluff as at a, Fig. 173.
The stream’s meanders shift their positions from time to time so that the
valley flat is successively widened at different points. By lateral planation,
therefore, a stream tends to develop a flat as soon as it reaches grade. This
is the initial part of erosion in the making of a river flat, but a flat developed
by erosion alone is not an alluvial plain.
Page 241
So soon as the flat developed by a stream exceeds the width of its
channel, the water (except in times of flood) does not cover it all at the
same time. On any part which it temporarily abandons, some débris
(alluvium) is likely to be left. This deposit of alluvium constitutes the valley
flat an alluvial plain (Fig. 174). It will be seen that the valley flat is
commonly an alluvial plain from the beginning.
Fig. 172.—Diagram illustrating the transformation of a V-shaped valley into a U-shaped
valley.
Fig. 173.—Diagram to illustrate the widening of a valley flat by erosion. Compare 3, Fig.
172.
Once the valley flat and alluvial plain are begun, their further
development is easily followed. The stream in flood overflows the banks of
its channel. The velocity of the overflowing water is reduced, and if it has
much load a part of it will be dropped and the plain aggraded. Meantime
meandering and lateral planation continue. Thus the flood-plain is widened
by erosion, and aggraded by alluviation, the two processes going on
simultaneously.
Fig. 174.—An alluvial plain. The diagram suggests the relative importance of lateral
planation and alluviation in the development of the flat.
Flood-plains, chiefly the result of planation, but partly of aggradation, are
a normal feature of river valleys, after a certain stage of development has
been reached. This stage is that at which downward erosion becomes slight
in comparison with lateral erosion. It follows that an alluvial plain normally
begins its development where the valley is first brought to grade, that is, in
channel, the water (except in times of flood) does not cover it all at the
same time. On any part which it temporarily abandons, some débris
(alluvium) is likely to be left. This deposit of alluvium constitutes the valley
flat an alluvial plain (Fig. 174). It will be seen that the valley flat is
commonly an alluvial plain from the beginning.
Fig. 172.—Diagram illustrating the transformation of a V-shaped valley into a U-shaped
valley.
Fig. 173.—Diagram to illustrate the widening of a valley flat by erosion. Compare 3, Fig.
172.
Once the valley flat and alluvial plain are begun, their further
development is easily followed. The stream in flood overflows the banks of
its channel. The velocity of the overflowing water is reduced, and if it has
much load a part of it will be dropped and the plain aggraded. Meantime
meandering and lateral planation continue. Thus the flood-plain is widened
by erosion, and aggraded by alluviation, the two processes going on
simultaneously.
Fig. 174.—An alluvial plain. The diagram suggests the relative importance of lateral
planation and alluviation in the development of the flat.
Flood-plains, chiefly the result of planation, but partly of aggradation, are
a normal feature of river valleys, after a certain stage of development has
been reached. This stage is that at which downward erosion becomes slight
in comparison with lateral erosion. It follows that an alluvial plain normally
begins its development where the valley is first brought to grade, that is, in
Page 242
its lower course. As the development of the valley goes on, the head of the
flood-plain advances up-stream, and at the same time its older parts become
wider.
Flood-plains due to alluviation
only.—Exceptionally, an alluvial plain
is developed by deposition only. Thus if
a stream becomes overloaded while its
valley is still narrow, as sometimes
happens, deposition follows, and, as
aggradation proceeds, the narrow valley Fig. 175.—Diagrammatic representation
acquires a progressively wider bottom of a flood plain developed by
(Fig. 175). Wide valley plains are alluviation only.
sometimes developed in this way. Flood plains developed wholly by
alluviation are sometimes formed under conditions which are independent
of the stage of a valley’s development. Thus if a stream suddenly acquires
an exceptional supply of detritus in its upper course, the development of an
alluvial plain begins immediately below the point of overloading.
The overload might be acquired in various ways. (1) If a stream taps
another (piracy) which carries a large quantity of sediment, carrying off
both water and sediment to a channel with a lower gradient, deposition may
take place where, under the earlier conditions, there was none. (2) Again,
when a stream cuts through a barrier near its head waters, its velocity, and,
therefore, its eroding power, may be so increased in its upper course that
sediment enough is acquired to occasion deposition below, where none took
place before. (3) In working back through formations of varying degrees of
resistance, a stream’s head may presently reach a formation or a region
which yields abundant sediment, even though there was no especial barrier
below. (4) If an advancing glacier should reach the head waters of a stream,
its discharge to the stream would greatly increase the load of the latter, and,
although its volume would be augmented at the same time, deposition
might result. As a matter of fact, streams carrying glacial drainage are
usually aggrading streams. In general, anything which greatly increases the
load of a stream near its head is likely to cause deposition, and so the
development of a flood plain, at some point farther down the valley.
flood-plain advances up-stream, and at the same time its older parts become
wider.
Flood-plains due to alluviation
only.—Exceptionally, an alluvial plain
is developed by deposition only. Thus if
a stream becomes overloaded while its
valley is still narrow, as sometimes
happens, deposition follows, and, as
aggradation proceeds, the narrow valley Fig. 175.—Diagrammatic representation
acquires a progressively wider bottom of a flood plain developed by
(Fig. 175). Wide valley plains are alluviation only.
sometimes developed in this way. Flood plains developed wholly by
alluviation are sometimes formed under conditions which are independent
of the stage of a valley’s development. Thus if a stream suddenly acquires
an exceptional supply of detritus in its upper course, the development of an
alluvial plain begins immediately below the point of overloading.
The overload might be acquired in various ways. (1) If a stream taps
another (piracy) which carries a large quantity of sediment, carrying off
both water and sediment to a channel with a lower gradient, deposition may
take place where, under the earlier conditions, there was none. (2) Again,
when a stream cuts through a barrier near its head waters, its velocity, and,
therefore, its eroding power, may be so increased in its upper course that
sediment enough is acquired to occasion deposition below, where none took
place before. (3) In working back through formations of varying degrees of
resistance, a stream’s head may presently reach a formation or a region
which yields abundant sediment, even though there was no especial barrier
below. (4) If an advancing glacier should reach the head waters of a stream,
its discharge to the stream would greatly increase the load of the latter, and,
although its volume would be augmented at the same time, deposition
might result. As a matter of fact, streams carrying glacial drainage are
usually aggrading streams. In general, anything which greatly increases the
load of a stream near its head is likely to cause deposition, and so the
development of a flood plain, at some point farther down the valley.
Page 243
Fig. 176.—Anastomosing of a depositing stream. Yahtse River, Alaska. (Russell, U. S. Geol.
Surv.)
Streams which are actively aggrading their valleys are likely to
anastomose (Figs. 176, 177). This results from the filling of the channels
until they are too small to accommodate all the water. The latter then breaks
out of the channel at few or many points. The new channels thus established
suffer the same fate.
Fig. 177.—Anastomosing of the Platte River, Dawson Co., Neb. (U. S. Geol. Surv.)
Surv.)
Streams which are actively aggrading their valleys are likely to
anastomose (Figs. 176, 177). This results from the filling of the channels
until they are too small to accommodate all the water. The latter then breaks
out of the channel at few or many points. The new channels thus established
suffer the same fate.
Fig. 177.—Anastomosing of the Platte River, Dawson Co., Neb. (U. S. Geol. Surv.)
Page 244
Flood-plains due to obstructions.—Again, any obstacle in a stream’s
course is likely to cause deposition above. Thus dams built across rivers
entail the deposition of sediment above. Where a stream flows over the
outcropping edges of strata of different strength, the more resistant serve, in
some sense, as dams. Above them the stream cuts its bed to a low gradient,
and, becoming sluggish, drops more or less of the detritus brought down
from above. Obstacles of any sort across a stream’s channel, therefore,
favor the development of alluvial plains.
Fig. 178.—The levees of the Mississippi in cross-section, 4 miles north of Donaldsonville,
⨉
La. Vertical scale 50. The horizontal line in the diagram represents sea-level. The
bottom of the channel at this point is far below sea-level.
Levees.—As the stream in flood escapes its channel and overspreads its
plain, its immediate banks are the site of active deposition, for it is here that
the velocity of the overflowing water is first notably checked. On the banks
of the channel, therefore, low alluvial ridges, called natural levees, are built
up (Fig. 178, and Pl. XV). They may be narrow, or hundreds of feet in
width, and are often several feet above the plains behind them, giving the
latter a slope away from the channel of the stream. They are sometimes high
enough to control the courses of tributary streams, as shown by numerous
tributaries to the Mississippi below the Ohio. The Yazoo, for example,
flows some 200 miles on the flood-plain of the Mississippi before it joins
that river near Vicksburg. The levees even become divides, directing
drainage away from the streams they guard (Pl. XV). Streams sometimes
build levees faster than their tributaries aggrade their channels. The latter
are then ponded, giving rise to lakes. The lakes on the lower courses of the
tributaries to the Red River of Louisiana are examples.[70] They are
sometimes built up above their natural level and kept in repair by human
agency so as to confine the streams in time of flood. This is a source of
danger unless they be steadily maintained, for the breaking of such levees
often occasions great destruction. A case in point is the breaking of the
levees of the Mississippi near New Orleans in 1890. The water broke
through the levees at the Nita and Martinez crevasses (Fig. 187) and flowed
eastward (from the former) with a current of 15 miles per hour, spreading
destruction in its path. The water flowed eastward through Lakes
Pontchartrain and Borgne, and entered Mobile Bay with such volume,
course is likely to cause deposition above. Thus dams built across rivers
entail the deposition of sediment above. Where a stream flows over the
outcropping edges of strata of different strength, the more resistant serve, in
some sense, as dams. Above them the stream cuts its bed to a low gradient,
and, becoming sluggish, drops more or less of the detritus brought down
from above. Obstacles of any sort across a stream’s channel, therefore,
favor the development of alluvial plains.
Fig. 178.—The levees of the Mississippi in cross-section, 4 miles north of Donaldsonville,
⨉
La. Vertical scale 50. The horizontal line in the diagram represents sea-level. The
bottom of the channel at this point is far below sea-level.
Levees.—As the stream in flood escapes its channel and overspreads its
plain, its immediate banks are the site of active deposition, for it is here that
the velocity of the overflowing water is first notably checked. On the banks
of the channel, therefore, low alluvial ridges, called natural levees, are built
up (Fig. 178, and Pl. XV). They may be narrow, or hundreds of feet in
width, and are often several feet above the plains behind them, giving the
latter a slope away from the channel of the stream. They are sometimes high
enough to control the courses of tributary streams, as shown by numerous
tributaries to the Mississippi below the Ohio. The Yazoo, for example,
flows some 200 miles on the flood-plain of the Mississippi before it joins
that river near Vicksburg. The levees even become divides, directing
drainage away from the streams they guard (Pl. XV). Streams sometimes
build levees faster than their tributaries aggrade their channels. The latter
are then ponded, giving rise to lakes. The lakes on the lower courses of the
tributaries to the Red River of Louisiana are examples.[70] They are
sometimes built up above their natural level and kept in repair by human
agency so as to confine the streams in time of flood. This is a source of
danger unless they be steadily maintained, for the breaking of such levees
often occasions great destruction. A case in point is the breaking of the
levees of the Mississippi near New Orleans in 1890. The water broke
through the levees at the Nita and Martinez crevasses (Fig. 187) and flowed
eastward (from the former) with a current of 15 miles per hour, spreading
destruction in its path. The water flowed eastward through Lakes
Pontchartrain and Borgne, and entered Mobile Bay with such volume,
Page 245
velocity, and load of mud, as to destroy for a time the oyster and fish
industries of that locality.[71]
PLATE XV.
U. S. Geol. Surv. NEAR HAHNVILLE, Scale, 1+ mile per inch.
LOUISIANA.
industries of that locality.[71]
PLATE XV.
U. S. Geol. Surv. NEAR HAHNVILLE, Scale, 1+ mile per inch.
LOUISIANA.
Page 246
PLATE XVI.
U. S. Geol. Surv. Fig. 1. Scale, 2+ miles per inch.
MISSOURI U. S. Geol. Surv. Scale, 2 miles per inch.
. Fig. 2. MISSOURI.
U. S. Geol. Surv. Fig. 1. Scale, 2+ miles per inch.
MISSOURI U. S. Geol. Surv. Scale, 2 miles per inch.
. Fig. 2. MISSOURI.
Page 247
U. S. Geol. Surv. Fig. 3. MISSOURI. Scale, 2+ miles per inch.
Page 248
Fig. 179.—Flood-plain of the Mississippi River south of the mouth of the Ohio. (From
charts of the Miss. Riv. Commission.)
Flood-plain meanders. Cut-and-fill.—A stream with an alluvial plain is
likely to meander widely (Pl. XVI). In general terms this may be said to be
the result of low velocity, which allows it to be easily turned aside. Were the
course of such a stream made straight, it would soon become crooked again.
The manner of change is illustrated by Figs. 180 and 181. If the banks be
less resistant at some points than at others, as is always the case, the stream
will cut in at those points. If the configuration of the channel is such as to
direct a current against a given point, a (Fig. 180), the result is the same,
even without inequality of material. Once a curve in the bank is started, it is
charts of the Miss. Riv. Commission.)
Flood-plain meanders. Cut-and-fill.—A stream with an alluvial plain is
likely to meander widely (Pl. XVI). In general terms this may be said to be
the result of low velocity, which allows it to be easily turned aside. Were the
course of such a stream made straight, it would soon become crooked again.
The manner of change is illustrated by Figs. 180 and 181. If the banks be
less resistant at some points than at others, as is always the case, the stream
will cut in at those points. If the configuration of the channel is such as to
direct a current against a given point, a (Fig. 180), the result is the same,
even without inequality of material. Once a curve in the bank is started, it is
Page 249
increased by the current which is directed
into it. Furthermore, as the current issues
from the curve, it impinges against the
opposite bank and develops a curve at that
point. The water issuing from this curve
develops another, and so on.
Once started, the curves or meanders tend
to become more and more pronounced
(compare Figs. 180 and 181). In the case
represented by Fig. 1, Plate XVI (Missouri
River near Brunswick, Mo.) the narrow neck
of land between curves is almost cut through.
When this is accomplished, the stream will
abandon its wide curve. A later stage in the
process is shown in Fig. 2, Plate XVI (the
Osage River near Schell, Mo.).
The straightening of the channel is often
accomplished in another way. Even before
the meanders reach the stage represented by
Fig. 1, Plate XVI, the position of the channel
becomes unstable. In time of flood, the
whole flat is covered with flowing water.
Fig. 180.—Diagram illustrating an
early stage in the development The greater depth of water in the channel
of meanders. The shaded part tends to give it a velocity greater than that of
represents the area over which the water on the flat outside. But the distance
the stream has worked.
from a to c via b (Fig. 181) is much greater
than that in a direct line. It follows that the slope from a to c direct is
greater than that by way of b. If the current between a and c in time of flood
be strong enough to erode, it may deepen its bed, and thereby increase the
volume of water following this course. The increased volume gives
increased velocity, and the result may be the opening of a channel between
a and c direct. The channel may be worn so deep that when the flood
subsides, the stream will follow it. So long as the abandoned channel-curve
remains unfilled with sediment, it is often called a cut-off. If it contains
standing water and has the proper form, it is called an ox-bow lake (Fig.
182), or sometimes a bayou. The water-filled portions are not always bows
into it. Furthermore, as the current issues
from the curve, it impinges against the
opposite bank and develops a curve at that
point. The water issuing from this curve
develops another, and so on.
Once started, the curves or meanders tend
to become more and more pronounced
(compare Figs. 180 and 181). In the case
represented by Fig. 1, Plate XVI (Missouri
River near Brunswick, Mo.) the narrow neck
of land between curves is almost cut through.
When this is accomplished, the stream will
abandon its wide curve. A later stage in the
process is shown in Fig. 2, Plate XVI (the
Osage River near Schell, Mo.).
The straightening of the channel is often
accomplished in another way. Even before
the meanders reach the stage represented by
Fig. 1, Plate XVI, the position of the channel
becomes unstable. In time of flood, the
whole flat is covered with flowing water.
Fig. 180.—Diagram illustrating an
early stage in the development The greater depth of water in the channel
of meanders. The shaded part tends to give it a velocity greater than that of
represents the area over which the water on the flat outside. But the distance
the stream has worked.
from a to c via b (Fig. 181) is much greater
than that in a direct line. It follows that the slope from a to c direct is
greater than that by way of b. If the current between a and c in time of flood
be strong enough to erode, it may deepen its bed, and thereby increase the
volume of water following this course. The increased volume gives
increased velocity, and the result may be the opening of a channel between
a and c direct. The channel may be worn so deep that when the flood
subsides, the stream will follow it. So long as the abandoned channel-curve
remains unfilled with sediment, it is often called a cut-off. If it contains
standing water and has the proper form, it is called an ox-bow lake (Fig.
182), or sometimes a bayou. The water-filled portions are not always bows
Page 250
(Fig. 183, Osage River, near Butler, Mo.). Cut-offs, with or without
standing water, are of common occurrence along most rivers with wide
plains. Meandering is not confined to streams which are near sea-level.
Even small creeks at high altitudes may meander, if so situated as to have
slight velocity. Trout Creek in the Yellowstone Park (Fig. 184) is an
example.
Fig. 181.—Diagram illustrating later stages in the development of meanders.
standing water, are of common occurrence along most rivers with wide
plains. Meandering is not confined to streams which are near sea-level.
Even small creeks at high altitudes may meander, if so situated as to have
slight velocity. Trout Creek in the Yellowstone Park (Fig. 184) is an
example.
Fig. 181.—Diagram illustrating later stages in the development of meanders.
Page 251
Fig. 182.—Meanders and cut-offs (ox-bow lakes) in the Mississippi Valley a little below
Vicksburg. The figure also shows the migration of meanders down-stream, and their
tendency to increase themselves. (From charts Nos. 18 and 19, Mississippi River
Commission.)
There seems to be some relation between the width of the belt within
which a stream meanders, and the width of the stream itself. Recently it has
been estimated that the ratio between them is 18:1.[72]
During the development of the meanders it is to be noted that lateral
planation on the one side of a stream is accompanied by deposition on the
other. This is cut-and-fill. The sediment eroded from the curve which is
concave toward the stream is shifted down-stream, while that deposited in
Vicksburg. The figure also shows the migration of meanders down-stream, and their
tendency to increase themselves. (From charts Nos. 18 and 19, Mississippi River
Commission.)
There seems to be some relation between the width of the belt within
which a stream meanders, and the width of the stream itself. Recently it has
been estimated that the ratio between them is 18:1.[72]
During the development of the meanders it is to be noted that lateral
planation on the one side of a stream is accompanied by deposition on the
other. This is cut-and-fill. The sediment eroded from the curve which is
concave toward the stream is shifted down-stream, while that deposited in
Page 252
the curve which is convex toward the
stream is brought down from above.
Thus even in the development of
meanders, the material which is
dislodged is shifted down-stream.
Since the current directed against the
down-stream side of a growing
meander is on the average stronger
than that directed against the opposite
side, the meander itself has a tendency
to migrate down-stream (Fig. 182).
In their evolution, the curves of a
stream’s channel often reach and
undermine the valley bluff (Pl. VII).
Since the meanders are, on the
average, shifted down-stream
individually, and since meanders are
frequently developed in new places, it Fig. 183.—Bayou Lakes, Osage River, near
Butler, Mo.
follows that a meandering stream
tends to widen its valley throughout. Widening is also effected in other
ways, for a stream with a flood-plain sometimes abandons its channel
altogether for miles at a stretch, and the new course chosen may be against
one of the bluffs of the valley. Such changes are most likely to take place
where deposition along channel and levees has brought the part of the
flood-plain (though not necessarily the bottom of the channel) adjacent to
the stream above the level of that farther from it (Fig. 178). The change is
likely to be effected in time of flood.
Flood-plains often attain great size. That of the Mississippi below the
Ohio (Fig. 179) has a width ranging from rather more than 20 miles at
Helena (Ark.), to something like 80 miles in the latitude of Greenville
(Miss.).[73] Below the Ohio its area is something like 30,000 square miles,
and its entire area has been estimated at about 50,000 square miles.[74]
Theoretically, the rotation of the earth should affect the erosion of
streams, increasing it on the one bank (the right in the northern hemisphere
and the left in the southern) and decreasing it on the other.[75] The streams
doubtless accommodate themselves to the rotation of the earth in the
stream is brought down from above.
Thus even in the development of
meanders, the material which is
dislodged is shifted down-stream.
Since the current directed against the
down-stream side of a growing
meander is on the average stronger
than that directed against the opposite
side, the meander itself has a tendency
to migrate down-stream (Fig. 182).
In their evolution, the curves of a
stream’s channel often reach and
undermine the valley bluff (Pl. VII).
Since the meanders are, on the
average, shifted down-stream
individually, and since meanders are
frequently developed in new places, it Fig. 183.—Bayou Lakes, Osage River, near
Butler, Mo.
follows that a meandering stream
tends to widen its valley throughout. Widening is also effected in other
ways, for a stream with a flood-plain sometimes abandons its channel
altogether for miles at a stretch, and the new course chosen may be against
one of the bluffs of the valley. Such changes are most likely to take place
where deposition along channel and levees has brought the part of the
flood-plain (though not necessarily the bottom of the channel) adjacent to
the stream above the level of that farther from it (Fig. 178). The change is
likely to be effected in time of flood.
Flood-plains often attain great size. That of the Mississippi below the
Ohio (Fig. 179) has a width ranging from rather more than 20 miles at
Helena (Ark.), to something like 80 miles in the latitude of Greenville
(Miss.).[73] Below the Ohio its area is something like 30,000 square miles,
and its entire area has been estimated at about 50,000 square miles.[74]
Theoretically, the rotation of the earth should affect the erosion of
streams, increasing it on the one bank (the right in the northern hemisphere
and the left in the southern) and decreasing it on the other.[75] The streams
doubtless accommodate themselves to the rotation of the earth in the
Page 253
original development of their gradation-plains and flood-plains, and the
later effects of rotation are usually inconspicuous.
Fig. 184.—Meanders of Trout Creek, Yellowstone Park. (Walcott, U. S. Geol. Surv.)
Scour-and-fill.—It has already been shown that aggrading streams cut
laterally at the same time that they build up their plains. It is now to be
added that they periodically deepen their channels to a notable extent, and
that the deepening of the channel takes place at the very time when the
flood-plain is being aggraded. In other words, the stream in flood aggrades
its plain, and degrades its channel. This follows from the fact that the
current is sluggish in the former position, where the water is shallow, and
rapid in the latter, where it is deep. When the flood subsides, the channel,
deepened while the current was torrential, is filled again by the feebler
current which follows. This alternate deepening and filling is known as
scour-and-fill. It is well illustrated by the Missouri River. At Nebraska City,
scour is believed to occasionally reach depths of 70 to 90 feet.[76] At Blair,
about 25 miles above Omaha, the same river is believed to cut to bed-rock
(about 40 feet below the bottom of the channel in low water) twice a year,
that is, during floods.[77] Fig. 185 shows the changes recorded in the channel
of the river at this point during the year 1883. It shows that the scour-and-
later effects of rotation are usually inconspicuous.
Fig. 184.—Meanders of Trout Creek, Yellowstone Park. (Walcott, U. S. Geol. Surv.)
Scour-and-fill.—It has already been shown that aggrading streams cut
laterally at the same time that they build up their plains. It is now to be
added that they periodically deepen their channels to a notable extent, and
that the deepening of the channel takes place at the very time when the
flood-plain is being aggraded. In other words, the stream in flood aggrades
its plain, and degrades its channel. This follows from the fact that the
current is sluggish in the former position, where the water is shallow, and
rapid in the latter, where it is deep. When the flood subsides, the channel,
deepened while the current was torrential, is filled again by the feebler
current which follows. This alternate deepening and filling is known as
scour-and-fill. It is well illustrated by the Missouri River. At Nebraska City,
scour is believed to occasionally reach depths of 70 to 90 feet.[76] At Blair,
about 25 miles above Omaha, the same river is believed to cut to bed-rock
(about 40 feet below the bottom of the channel in low water) twice a year,
that is, during floods.[77] Fig. 185 shows the changes recorded in the channel
of the river at this point during the year 1883. It shows that the scour-and-
Page 254
fill during this year amounted to almost 40 feet. All streams similarly
situated do a like work. The material thus eroded is shifted down-stream,
some of it for short distances only, and some of it to the sea. Even an
aggrading stream therefore is not without erosive activity; it is a stream
whose fill exceeds its scour, not one which has ceased to erode.
Fig. 185.—Diagram illustrating scour and fill in the Missouri River. A record of soundings
at Blair Bridge (near Omaha), 1883. Shows also the cross-sections of the river at various
rates. (Todd, Bull. 158, U. S. Geol. Surv.)
Materials of the flood-plain.—As a result of its varying velocities in
flood and low water, a stream may deposit coarse material at one time and
fine at another. A similar sequence of deposits takes place in the flood-plain
of a meandering stream, irrespective of floods. Flood-plain deposits are
often therefore very heterogeneous, as shown in Fig. 186, which represents
the constitution of the alluvium of the Missouri River at Omaha. The
deposits of the streams range from the finest clay, through sand to gravel,
and even bowlders. In general they become finer down-stream. In a given
plain, they are usually coarser below and finer above.
situated do a like work. The material thus eroded is shifted down-stream,
some of it for short distances only, and some of it to the sea. Even an
aggrading stream therefore is not without erosive activity; it is a stream
whose fill exceeds its scour, not one which has ceased to erode.
Fig. 185.—Diagram illustrating scour and fill in the Missouri River. A record of soundings
at Blair Bridge (near Omaha), 1883. Shows also the cross-sections of the river at various
rates. (Todd, Bull. 158, U. S. Geol. Surv.)
Materials of the flood-plain.—As a result of its varying velocities in
flood and low water, a stream may deposit coarse material at one time and
fine at another. A similar sequence of deposits takes place in the flood-plain
of a meandering stream, irrespective of floods. Flood-plain deposits are
often therefore very heterogeneous, as shown in Fig. 186, which represents
the constitution of the alluvium of the Missouri River at Omaha. The
deposits of the streams range from the finest clay, through sand to gravel,
and even bowlders. In general they become finer down-stream. In a given
plain, they are usually coarser below and finer above.
Page 255
Fig. 186.—Diagram to show the heterogeneous character of alluvial deposits. (Todd, Bull.
158, U. S. Geol. Surv.)
Topography of the flood-plain.—The flood-plain is nearly, but not
altogether, flat. It has a gentle slope down-stream, and often for a distance
from the sides toward the center (Fig. 174). This latter slope is the result of
deposition by waters descending to the plain from the sides. It is destroyed
wherever a meandering stream reaches its bluffs. When levees are well
developed, there is a slope from them toward the sides of the valley (Fig.
178), but it rarely continues to the limiting bluffs. Since a stream with a
well-developed flat frequently shifts its course, old levees and abandoned
channels lend variety to the topography of the flood-plain.
The topographic adjustment of tributaries.[78]—The meandering and
shifting of a main stream affects its tributaries. If a main stream swings
against the bluff through which a tributary enters, the latter brings its
channel into topographic adjustment by lowering its end to the level of the
main. If now the main stream opposite the tributary swings to the other side
of its valley, the tributary must make its way across the flat with a very low
gradient. Not only this, but the flat of the main valley through which the
tributary must flow is likely to be aggraded by the main in time of flood.
The result is that the tributary stream becomes an aggrading stream at its
debouchure, and topographic adjustment is not established until it has filled
up the lower end of its valley to some notable extent. The filling of the
lower end of the tributary likewise affects the lower ends of its lower
tributaries.
158, U. S. Geol. Surv.)
Topography of the flood-plain.—The flood-plain is nearly, but not
altogether, flat. It has a gentle slope down-stream, and often for a distance
from the sides toward the center (Fig. 174). This latter slope is the result of
deposition by waters descending to the plain from the sides. It is destroyed
wherever a meandering stream reaches its bluffs. When levees are well
developed, there is a slope from them toward the sides of the valley (Fig.
178), but it rarely continues to the limiting bluffs. Since a stream with a
well-developed flat frequently shifts its course, old levees and abandoned
channels lend variety to the topography of the flood-plain.
The topographic adjustment of tributaries.[78]—The meandering and
shifting of a main stream affects its tributaries. If a main stream swings
against the bluff through which a tributary enters, the latter brings its
channel into topographic adjustment by lowering its end to the level of the
main. If now the main stream opposite the tributary swings to the other side
of its valley, the tributary must make its way across the flat with a very low
gradient. Not only this, but the flat of the main valley through which the
tributary must flow is likely to be aggraded by the main in time of flood.
The result is that the tributary stream becomes an aggrading stream at its
debouchure, and topographic adjustment is not established until it has filled
up the lower end of its valley to some notable extent. The filling of the
lower end of the tributary likewise affects the lower ends of its lower
tributaries.
Page 256
Fig. 187.—A general view of the Mississippi delta.
If the main stream again swings over to the point where the tributary
issues from its valley, the tributary stream and all its affected tributaries
again become eroding streams. Thus scour-and-fill are not confined to the
valley of the main stream.
River-lakes.—While rivers are in general hostile to lakes, they
sometimes give origin to them. Oxbow lakes (Fig. 182 and Pl. XVI), due to
the cut-offs of meandering streams, have already been referred to. Lakes
formed in the same way have other forms (Pl. XVI and Fig. 183). Rivers
also give rise to lakes through the deposits they make. If a main stream
obstructs its tributaries by deposition at their debouchures, their lower
courses are ponded and converted into lakes. The lakes along the tributaries
to the Red River of Louisiana have already been cited as examples. If a
tributary brings more load to its main than the latter can carry away, the
detritus constitutes a partial dam, ponding the river and causing it to expand
into a lake above. Such is the origin of Lake Pepin already referred to. In
mountain regions, the alluvial cones of tributary valleys sometimes pond
their mains.
If the main stream again swings over to the point where the tributary
issues from its valley, the tributary stream and all its affected tributaries
again become eroding streams. Thus scour-and-fill are not confined to the
valley of the main stream.
River-lakes.—While rivers are in general hostile to lakes, they
sometimes give origin to them. Oxbow lakes (Fig. 182 and Pl. XVI), due to
the cut-offs of meandering streams, have already been referred to. Lakes
formed in the same way have other forms (Pl. XVI and Fig. 183). Rivers
also give rise to lakes through the deposits they make. If a main stream
obstructs its tributaries by deposition at their debouchures, their lower
courses are ponded and converted into lakes. The lakes along the tributaries
to the Red River of Louisiana have already been cited as examples. If a
tributary brings more load to its main than the latter can carry away, the
detritus constitutes a partial dam, ponding the river and causing it to expand
into a lake above. Such is the origin of Lake Pepin already referred to. In
mountain regions, the alluvial cones of tributary valleys sometimes pond
their mains.
Page 257
Fig. 188.—Longitudinal section of an incipient delta made of coarse material.
Rivers may be dammed in other ways, as by lava flows, by landslides, by
glacial drift, etc. In all such cases, lakes may come into existence, but they
are not due primarily to the activity of the river itself.
Deltas.[79]—Where a stream enters standing water, or a slower stream, a
special form of plain, the delta, is sometimes built up (Figs. 169, 187, and
188). Deltas and alluvial fans have much in common, and their only notable
differences are those imposed by the differences in the conditions of
deposition. The current of the stream is checked, but not altogether stopped,
at its immediate debouchure. If it carries abundant sediment, much of it will
be promptly dropped where the decrease in velocity is first felt. Such flow
as there is beyond the debouchure is not confined to a definite channel, and
the deposits made are therefore spread more or less on either side of the line
which represents the continuation of the stream’s course.
As the depth of the water into which the stream flows increases, the
current diminishes. Out to the point where the depth of the standing water is
less than the depth of the current, the latter affects the bottom, and the
surface of the deposits made slopes gently seaward; but where the depth of
the standing water is such that the projected stream current is ineffective at
the bottom, all the load rolled along the bottom is dropped, and a
depositional slope is established (Fig. 188), its upper edge being below sea-
level by an amount corresponding roughly to the depth of the current which
brings the detritus. The outer slope is relatively steep and well-defined
where the detritus is coarse, and relatively gentle and ill-defined where it is
fine. Thus the stream tends to construct a sort of platform in the water just
beyond its debouchure. The successive deposits on the outer abrupt slope
will dip conformably with its surface (Fig. 189). The finest sediment will be
carried beyond the steep slope, and conform to the topography of the
bottom beyond (c, Fig. 189).
Rivers may be dammed in other ways, as by lava flows, by landslides, by
glacial drift, etc. In all such cases, lakes may come into existence, but they
are not due primarily to the activity of the river itself.
Deltas.[79]—Where a stream enters standing water, or a slower stream, a
special form of plain, the delta, is sometimes built up (Figs. 169, 187, and
188). Deltas and alluvial fans have much in common, and their only notable
differences are those imposed by the differences in the conditions of
deposition. The current of the stream is checked, but not altogether stopped,
at its immediate debouchure. If it carries abundant sediment, much of it will
be promptly dropped where the decrease in velocity is first felt. Such flow
as there is beyond the debouchure is not confined to a definite channel, and
the deposits made are therefore spread more or less on either side of the line
which represents the continuation of the stream’s course.
As the depth of the water into which the stream flows increases, the
current diminishes. Out to the point where the depth of the standing water is
less than the depth of the current, the latter affects the bottom, and the
surface of the deposits made slopes gently seaward; but where the depth of
the standing water is such that the projected stream current is ineffective at
the bottom, all the load rolled along the bottom is dropped, and a
depositional slope is established (Fig. 188), its upper edge being below sea-
level by an amount corresponding roughly to the depth of the current which
brings the detritus. The outer slope is relatively steep and well-defined
where the detritus is coarse, and relatively gentle and ill-defined where it is
fine. Thus the stream tends to construct a sort of platform in the water just
beyond its debouchure. The successive deposits on the outer abrupt slope
will dip conformably with its surface (Fig. 189). The finest sediment will be
carried beyond the steep slope, and conform to the topography of the
bottom beyond (c, Fig. 189).
Page 258
At the beginning, the top of the delta platform is at the level of the
bottom of the stream’s channel at the point of debouchure, but it is
gradually aggraded as water continues to flow over it. Its landward margin
is presently built up to sea-level and then above it, and as the delta grows
the delta-land is extended seaward (compare Figs. 188 and 189). At the
same time the channel of the stream above the original head of the delta is
aggraded, for the current there is checked by the aggradation of the delta.
Thus alluvial deposits continuous with the delta are extended landward.
Fig. 189.—Longitudinal section of the delta at a later stage of development.
The projection of the direction of the lower end of the stream may be said
to be the axis of the extra-debouchure current. From this axis, where the
flow is strongest, the movement diverges more or less to right and left.
Since the velocity of the diverging water is reduced more rapidly than that
of the water which follows the axis of flow, deposition is likely to take
place faster on either side of the axis than along the axis itself. The result is
that the extra-debouchure current tends to build up levee-like ridges on
either side, making a sort of sluice-way for itself. This sluice-way is
gradually extended seaward, and at the same time gradually filled. As its
capacity is reduced, more and more of the water flows over its sides.
Presently the escape of the water over the little side-levees will develop a
break at some point, and a line of distinct flow then diverges from the main
current. This distributary repeats the history of its main. Thus the processes
of levee-building, channel-filling, and levee-breaking follow one another,
until some such system of currents as shown in Fig. 190 is developed. The
result is that a delta’s growth is not simply in the line of extension of the
main stream, but in a more or less semicircular area, the center of the circle
being a point slightly below the position of the debouchure of the stream
when the delta began. At any stage in its development the margin of the
delta is more or less crenate (Fig. 191), or characterized by delta fingers
(Fig. 190), the projections corresponding to the positions of the
debouchures of the latest streams flowing across it. The extreme ends of the
bottom of the stream’s channel at the point of debouchure, but it is
gradually aggraded as water continues to flow over it. Its landward margin
is presently built up to sea-level and then above it, and as the delta grows
the delta-land is extended seaward (compare Figs. 188 and 189). At the
same time the channel of the stream above the original head of the delta is
aggraded, for the current there is checked by the aggradation of the delta.
Thus alluvial deposits continuous with the delta are extended landward.
Fig. 189.—Longitudinal section of the delta at a later stage of development.
The projection of the direction of the lower end of the stream may be said
to be the axis of the extra-debouchure current. From this axis, where the
flow is strongest, the movement diverges more or less to right and left.
Since the velocity of the diverging water is reduced more rapidly than that
of the water which follows the axis of flow, deposition is likely to take
place faster on either side of the axis than along the axis itself. The result is
that the extra-debouchure current tends to build up levee-like ridges on
either side, making a sort of sluice-way for itself. This sluice-way is
gradually extended seaward, and at the same time gradually filled. As its
capacity is reduced, more and more of the water flows over its sides.
Presently the escape of the water over the little side-levees will develop a
break at some point, and a line of distinct flow then diverges from the main
current. This distributary repeats the history of its main. Thus the processes
of levee-building, channel-filling, and levee-breaking follow one another,
until some such system of currents as shown in Fig. 190 is developed. The
result is that a delta’s growth is not simply in the line of extension of the
main stream, but in a more or less semicircular area, the center of the circle
being a point slightly below the position of the debouchure of the stream
when the delta began. At any stage in its development the margin of the
delta is more or less crenate (Fig. 191), or characterized by delta fingers
(Fig. 190), the projections corresponding to the positions of the
debouchures of the latest streams flowing across it. The extreme ends of the
Page 259
delta lobes (Fig. 190), and of groups of the delta fingers, often have
something of the shape of the Greek letter from which the name originated,
but the resemblance in form between a well-developed delta and the Greek
letter is not striking. Deltas are sometimes built in bays, and in such cases
their forms are predetermined on all sides but one. The head of a delta is
sometimes arbitrarily located at the point where the first distributaries are
given off. Since this point shifts widely with time, the definition can hardly
be accepted. On this basis the head of the Mississippi delta is about 200
miles above its lower end. In reality it is much farther north.
Fig. 190.—The terminus of the delta of the Mississippi. (C. and G. Survey.)
something of the shape of the Greek letter from which the name originated,
but the resemblance in form between a well-developed delta and the Greek
letter is not striking. Deltas are sometimes built in bays, and in such cases
their forms are predetermined on all sides but one. The head of a delta is
sometimes arbitrarily located at the point where the first distributaries are
given off. Since this point shifts widely with time, the definition can hardly
be accepted. On this basis the head of the Mississippi delta is about 200
miles above its lower end. In reality it is much farther north.
Fig. 190.—The terminus of the delta of the Mississippi. (C. and G. Survey.)
Page 260
Fig. 191.—A miniature delta.
The structure of a delta, shown in Fig. 189, shows its history. At any
stage in its growth the river discharges its sediment across that part of the
platform already built. The sediment rolled at the bottom of the current is
dumped on reaching the steep slope, and constitutes the inclined fore-set
beds shown in Fig. 189. The material in suspension is carried farther, settles
more gradually, and constitutes the bottom-set beds (c, Fig. 189). In time
the bottom-set beds, originally deposited some distance beyond the
debouchure, may come to be overlain by the fore-set beds, deposited at a
later time. While the fore-set beds are being deposited on the steep slopes of
the delta, and the bottom-set beds beyond, deposition is also taking place on
the top of the delta. These top-set beds are laid down in a nearly horizontal
position, and their seaward margin is gradually extended. Thus the delta
comes to have the threefold structure shown in Fig. 189.
That part of the delta which is above the abrupt slope of its front
corresponds in all essentials to an alluvial fan; but the delta as a whole
differs from the fan in its abrupt and crenate or digitate margin.
It is to be noted that the delta is not wholly the product of a stream’s
activity. The stream supplies the material, but the lake or sea renders at least
passive assistance in its disposition. Not all rivers opening into the sea build
deltas, and their failure is often the result of waves or shore currents which
carry off the river sediment. Deltas are, however, sometimes formed in tidal
seas, as at the debouchures of the Yukon; the Mackenzie, where the tidal
The structure of a delta, shown in Fig. 189, shows its history. At any
stage in its growth the river discharges its sediment across that part of the
platform already built. The sediment rolled at the bottom of the current is
dumped on reaching the steep slope, and constitutes the inclined fore-set
beds shown in Fig. 189. The material in suspension is carried farther, settles
more gradually, and constitutes the bottom-set beds (c, Fig. 189). In time
the bottom-set beds, originally deposited some distance beyond the
debouchure, may come to be overlain by the fore-set beds, deposited at a
later time. While the fore-set beds are being deposited on the steep slopes of
the delta, and the bottom-set beds beyond, deposition is also taking place on
the top of the delta. These top-set beds are laid down in a nearly horizontal
position, and their seaward margin is gradually extended. Thus the delta
comes to have the threefold structure shown in Fig. 189.
That part of the delta which is above the abrupt slope of its front
corresponds in all essentials to an alluvial fan; but the delta as a whole
differs from the fan in its abrupt and crenate or digitate margin.
It is to be noted that the delta is not wholly the product of a stream’s
activity. The stream supplies the material, but the lake or sea renders at least
passive assistance in its disposition. Not all rivers opening into the sea build
deltas, and their failure is often the result of waves or shore currents which
carry off the river sediment. Deltas are, however, sometimes formed in tidal
seas, as at the debouchures of the Yukon; the Mackenzie, where the tidal
Page 261
range is three feet; the Niger, where the range is four feet; the Hoang-Ho,
where the range is eight feet; and the Brahmaputra and Ganges, where the
range is sixteen feet.[80] Since lakes, bays, gulfs, and inland seas have
weaker waves and currents than the open sea, they are more favorable than
the latter for the growth of deltas. Hence occur such deltas as those of the
Mississippi, the Nile, the Po, and the Danube.
Deltas are likely to be absent, or confined to the heads of bays, on coasts
which have recently sunk. Their general absence on the Atlantic coast of the
United States is a case in point.
The following figures give some idea of the extent of deltas, and of their
importance in land building. The Mississippi delta is advancing into the
Gulf at the rate of about 100 yards per year, or a mile in 16 or 17 years. Its
length is more than 200 miles, its area more than 12,000 square miles, and
its depth at New Orleans has been estimated at 700[81] to 1000[82] feet. This
great depth is believed to be the result of subsidence, and so of the
superposition of one delta on another.[83] The delta of the Yukon has a sea
margin of 70 miles, and extends more than 100 miles inland. The delta of
the Rhône has also had a remarkable growth, considering the size and the
history of the stream. Arles, near the debouchure of the stream, was 14 to 16
miles inland in the fourth century b.c., and is now 30 miles inland.[84] The
Rhône has also built a great delta in Lake Geneva, and its lower delta is
built of sediment gathered below the lake. The Po has built a delta 14 miles
beyond Adria, the port which gave its name to the Adriatic Sea. The
extension of this delta has been at the average rate of about 50 feet per year,
but recently, on account of artificial embankments, the rate has been much
more rapid.[85] The Ganges and Brahmaputra together have made a delta of
great size. Its area is sometimes estimated to be as high as 50,000 or 60,000
square miles, and its head is more than 200 miles from the sea.[86] The head
of the Nile delta is 90 miles from the sea, and it has a coastal border of 180
miles. The head of the delta of the Hoang-Ho is about 300 miles from the
coast, and its seaward border has a length of about 400 miles, though with
some highland interruptions.[87]
After a delta has been built into a lake, the lake may disappear, leaving
the delta out of water. Such “fossil” deltas, if so recently exposed that
erosion has not destroyed their distinctive features, are readily recognized
by their flat tops, their abrupt and lobate fronts, and their characteristic
where the range is eight feet; and the Brahmaputra and Ganges, where the
range is sixteen feet.[80] Since lakes, bays, gulfs, and inland seas have
weaker waves and currents than the open sea, they are more favorable than
the latter for the growth of deltas. Hence occur such deltas as those of the
Mississippi, the Nile, the Po, and the Danube.
Deltas are likely to be absent, or confined to the heads of bays, on coasts
which have recently sunk. Their general absence on the Atlantic coast of the
United States is a case in point.
The following figures give some idea of the extent of deltas, and of their
importance in land building. The Mississippi delta is advancing into the
Gulf at the rate of about 100 yards per year, or a mile in 16 or 17 years. Its
length is more than 200 miles, its area more than 12,000 square miles, and
its depth at New Orleans has been estimated at 700[81] to 1000[82] feet. This
great depth is believed to be the result of subsidence, and so of the
superposition of one delta on another.[83] The delta of the Yukon has a sea
margin of 70 miles, and extends more than 100 miles inland. The delta of
the Rhône has also had a remarkable growth, considering the size and the
history of the stream. Arles, near the debouchure of the stream, was 14 to 16
miles inland in the fourth century b.c., and is now 30 miles inland.[84] The
Rhône has also built a great delta in Lake Geneva, and its lower delta is
built of sediment gathered below the lake. The Po has built a delta 14 miles
beyond Adria, the port which gave its name to the Adriatic Sea. The
extension of this delta has been at the average rate of about 50 feet per year,
but recently, on account of artificial embankments, the rate has been much
more rapid.[85] The Ganges and Brahmaputra together have made a delta of
great size. Its area is sometimes estimated to be as high as 50,000 or 60,000
square miles, and its head is more than 200 miles from the sea.[86] The head
of the Nile delta is 90 miles from the sea, and it has a coastal border of 180
miles. The head of the delta of the Hoang-Ho is about 300 miles from the
coast, and its seaward border has a length of about 400 miles, though with
some highland interruptions.[87]
After a delta has been built into a lake, the lake may disappear, leaving
the delta out of water. Such “fossil” deltas, if so recently exposed that
erosion has not destroyed their distinctive features, are readily recognized
by their flat tops, their abrupt and lobate fronts, and their characteristic
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structure. They are often a means of determining the former existence of
extinct lakes,[88] or the former higher levels of lakes which still exist.[89]
Elevated deltas on seashores show either a rise of the land or a depression
of the sea-level.
The material which is carried along the coasts or shores from the mouths
of rivers may take on various and peculiar forms, according to the strength,
direction, and relations of waves and currents. The consideration of these
forms belongs more properly to the work of the sea than to that of rivers,
since rivers are not concerned in their construction except in supplying
material.
Delta lakes.—Delta-building streams sometimes help to form lakes by
throwing their deposits around an area which fails to be aggraded to sea-
level. Lake Pontchartrain, and other lakes in the delta of the Mississippi are
examples (Fig. 187).
Fig. 192.—Terraces of the Frazier River at Lillooet, B. C. (Calvin.)
STREAM TERRACES.
Stream terraces[90] are bench-like flats or narrow plains along the sides of
valleys (Fig. 192). They are usually narrow, but sometimes have great
extinct lakes,[88] or the former higher levels of lakes which still exist.[89]
Elevated deltas on seashores show either a rise of the land or a depression
of the sea-level.
The material which is carried along the coasts or shores from the mouths
of rivers may take on various and peculiar forms, according to the strength,
direction, and relations of waves and currents. The consideration of these
forms belongs more properly to the work of the sea than to that of rivers,
since rivers are not concerned in their construction except in supplying
material.
Delta lakes.—Delta-building streams sometimes help to form lakes by
throwing their deposits around an area which fails to be aggraded to sea-
level. Lake Pontchartrain, and other lakes in the delta of the Mississippi are
examples (Fig. 187).
Fig. 192.—Terraces of the Frazier River at Lillooet, B. C. (Calvin.)
STREAM TERRACES.
Stream terraces[90] are bench-like flats or narrow plains along the sides of
valleys (Fig. 192). They are usually narrow, but sometimes have great
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length in the direction of the axis of the valley. They originate in various
ways.
Due to inequalities of hardness.—Reference has already been made (p.
140) to the effect of hard horizontal layers in the development of terraces
and terraciform projections on the sides of valleys (Fig. 120). Such terraces
are the result of differential degradation, and the upper surface of the hard
layer marks the lower limit of the terrace, which commonly has a distinct
slope toward the stream. Except where interrupted by tributary valleys, such
terraces are likely to be continuous in a valley so long as the structure
remains the same and the stream sustains the same relation to it. Such
terraces would first show themselves in the older part of the valley. The
effect of inclination of the hard stratum on the development of such terraces
will be readily inferred. Terraces and benches of this sort are not equally
distinct at all stages of a valley’s history. For great distinctness, the hard
layer should have been exposed long enough to allow the general processes
of erosion to have effected considerable differential wear, but not long
enough to allow the topographic effects of unequal resistance to be
obliterated.
Fig. 193.—Diagram illustrating a distinct terrace and a “second bottom (b),” which may be
regarded as a low terrace.
Normal flood-plain terraces.—It has been seen that deposition in a river
valley stands in more or less definite relationship to the stage of its
development, and that the deposition which leads to the development of an
alluvial plain is likely to take place where the higher gradient of the upper
course gives place to the gentler gradient of the lower. It has also been seen
that as a stream’s history advances, the stretch where the gradient is high
recedes up-stream, and that the point which marks the head of active
deposition follows. It follows that a river flat or flood-plain normally begins
in the lower part of a valley, and works progressively headward, its upper
end following, at some considerable distance, the head of the valley itself.
The commoner river terraces are remnants of former flood-plains, below
which the streams which made them have cut their channels. It has already
ways.
Due to inequalities of hardness.—Reference has already been made (p.
140) to the effect of hard horizontal layers in the development of terraces
and terraciform projections on the sides of valleys (Fig. 120). Such terraces
are the result of differential degradation, and the upper surface of the hard
layer marks the lower limit of the terrace, which commonly has a distinct
slope toward the stream. Except where interrupted by tributary valleys, such
terraces are likely to be continuous in a valley so long as the structure
remains the same and the stream sustains the same relation to it. Such
terraces would first show themselves in the older part of the valley. The
effect of inclination of the hard stratum on the development of such terraces
will be readily inferred. Terraces and benches of this sort are not equally
distinct at all stages of a valley’s history. For great distinctness, the hard
layer should have been exposed long enough to allow the general processes
of erosion to have effected considerable differential wear, but not long
enough to allow the topographic effects of unequal resistance to be
obliterated.
Fig. 193.—Diagram illustrating a distinct terrace and a “second bottom (b),” which may be
regarded as a low terrace.
Normal flood-plain terraces.—It has been seen that deposition in a river
valley stands in more or less definite relationship to the stage of its
development, and that the deposition which leads to the development of an
alluvial plain is likely to take place where the higher gradient of the upper
course gives place to the gentler gradient of the lower. It has also been seen
that as a stream’s history advances, the stretch where the gradient is high
recedes up-stream, and that the point which marks the head of active
deposition follows. It follows that a river flat or flood-plain normally begins
in the lower part of a valley, and works progressively headward, its upper
end following, at some considerable distance, the head of the valley itself.
The commoner river terraces are remnants of former flood-plains, below
which the streams which made them have cut their channels. It has already
Page 264
been pointed out (p. 184) that processes of erosion and deposition work
together in the development of flood-plains, and that some flood-plains
have but little alluvium (Fig. 174), while others owe their origin wholly to
stream deposits (Fig. 175). It follows that terraces developed from flood-
plains may be of rock, of alluvium, or of rock covered with alluvium.
The amount which a river channel must be deepened in order to change
the remnants of its flood-plain to terraces cannot be definitely stated. When
a channel is so deep that the remnants of a former flood-plain are no longer
flooded, they would be called terraces, especially if a lower flood-plain has
been developed. Even though not above the reach of floods, they are often
called terraces if they are notably above the channel and separated from it
by a lower plain. Thus the flat at b, Fig. 193, would be called a terrace, even
though covered by water in exceptional floods; but the flat at c, but slightly
above the channel, would hardly be called a terrace.
Fig. 194.—Diagram illustrating the beginning of the development of a terrace from a flood-
plain.
The question now arises why a stream, having once developed a flood-
plain, should sink its channel to a lower level, leaving parts of the old flood-
plain as terraces. This may be brought about by the operation of various
causes.
(1) In the first place, the head of the valley-plain where the first notable
deposition takes place normally advances up-stream. After the advance has
been considerable, the descending stream may, on reaching the head of its
valley-plain, lose so much of its load as to be able to sink its channel into
the flood-plain farther down the valley (Fig. 194).
together in the development of flood-plains, and that some flood-plains
have but little alluvium (Fig. 174), while others owe their origin wholly to
stream deposits (Fig. 175). It follows that terraces developed from flood-
plains may be of rock, of alluvium, or of rock covered with alluvium.
The amount which a river channel must be deepened in order to change
the remnants of its flood-plain to terraces cannot be definitely stated. When
a channel is so deep that the remnants of a former flood-plain are no longer
flooded, they would be called terraces, especially if a lower flood-plain has
been developed. Even though not above the reach of floods, they are often
called terraces if they are notably above the channel and separated from it
by a lower plain. Thus the flat at b, Fig. 193, would be called a terrace, even
though covered by water in exceptional floods; but the flat at c, but slightly
above the channel, would hardly be called a terrace.
Fig. 194.—Diagram illustrating the beginning of the development of a terrace from a flood-
plain.
The question now arises why a stream, having once developed a flood-
plain, should sink its channel to a lower level, leaving parts of the old flood-
plain as terraces. This may be brought about by the operation of various
causes.
(1) In the first place, the head of the valley-plain where the first notable
deposition takes place normally advances up-stream. After the advance has
been considerable, the descending stream may, on reaching the head of its
valley-plain, lose so much of its load as to be able to sink its channel into
the flood-plain farther down the valley (Fig. 194).
Page 265
(2) Ordinarily a stream does not drop all its load at the head of its plain,
but only its excess; but it will always drop coarse sediment to take fine, if
fine be available. For a relatively small amount of coarse material dropped,
a relatively large amount of fine may be taken up (p. 179). Other things
being equal, it follows that when a stream drops coarse material to take fine,
its channel is degraded unless there is at the same time a great reduction in
the stream’s energy. Such reduction is likely to go with the decreasing
declivity down-stream; but this is partly, or sometimes wholly,
counterbalanced by the increasing volume of water. By the exchange of
load, therefore, a stream may ultimately sink its channel below the flood-
plain which the earlier and perhaps smaller stream had developed.
Fig. 195.—Diagram to illustrate the development of river terraces by the widening of a
channel or meander belt. The valley flat above might not be called a terrace; but the
same plain below, where the meander belt has some width, would be called a terrace.
(3) Again, so long as a stream is actively eroding at its head, there is
likely to be some aggradation below. At a later stage in the stream’s history,
when active erosion at the head has ceased because of the reduction of the
surface, less material will be carried from the upper part of the valley, and
the stream on the flood-plain below, formerly loaded with material from up
the valley, is now free to take up and carry away material temporarily left
on the flood-plain. The result is a deepening of the channel.
(4) Any stream which has reached the flood-plain stage is likely to
meander. After the flood-plain has become wide, the width of the belt
within which the stream meanders is less than the width of its plain. In the
Lower Mississippi, for example, the meander belt is often no more than a
third to a tenth of the width of the flood-plain. It has already been pointed
but only its excess; but it will always drop coarse sediment to take fine, if
fine be available. For a relatively small amount of coarse material dropped,
a relatively large amount of fine may be taken up (p. 179). Other things
being equal, it follows that when a stream drops coarse material to take fine,
its channel is degraded unless there is at the same time a great reduction in
the stream’s energy. Such reduction is likely to go with the decreasing
declivity down-stream; but this is partly, or sometimes wholly,
counterbalanced by the increasing volume of water. By the exchange of
load, therefore, a stream may ultimately sink its channel below the flood-
plain which the earlier and perhaps smaller stream had developed.
Fig. 195.—Diagram to illustrate the development of river terraces by the widening of a
channel or meander belt. The valley flat above might not be called a terrace; but the
same plain below, where the meander belt has some width, would be called a terrace.
(3) Again, so long as a stream is actively eroding at its head, there is
likely to be some aggradation below. At a later stage in the stream’s history,
when active erosion at the head has ceased because of the reduction of the
surface, less material will be carried from the upper part of the valley, and
the stream on the flood-plain below, formerly loaded with material from up
the valley, is now free to take up and carry away material temporarily left
on the flood-plain. The result is a deepening of the channel.
(4) Any stream which has reached the flood-plain stage is likely to
meander. After the flood-plain has become wide, the width of the belt
within which the stream meanders is less than the width of its plain. In the
Lower Mississippi, for example, the meander belt is often no more than a
third to a tenth of the width of the flood-plain. It has already been pointed
Page 266
out that the meanders migrate down the valley. In so doing they depress the
meander belt, the tendency being to reduce it to the level of the channel,
and, therefore, below the level of the flood-plain. As the meander belt
widens, the depression which it develops becomes more and more
capacious. Presently it may attain such dimensions as to hold the water of
ordinary floods. At this stage, or even before, such parts of the earlier flood-
plain as remain, are terraces.
These several tendencies conspire to partially destroy river flood-plains,
and to transform such parts as remain into terraces in the normal course of a
river’s history. They appear first in the lower part of the valley, and migrate
headward, following the course of nearly every other phase of activity in a
stream’s history. The heads of the terraces follow, at a respectful distance,
the head of the flood-plain, just as the head of the flood-plain follows at a
distance the head of the valley. The second and subsequent flood-plains and
the terraces to which they give origin follow the same course.
Terraces developed by the normal activities of a stream are always low,
and it is improbable that they would ordinarily be conspicuous. The vertical
distance between the first (highest) and second is greater than that between
the second and third. The principles developed on page 65 et seq., in
connection with the erosion of the hypothetical island, are applicable here.
Flood-plain terraces due to other causes.—Certain other causes,
accidental rather than normal to a stream, result in the development of
terraces from flood-plains. (1) If there be uplift in a region where the rivers
have flats, the streams are rejuvenated, and the remnants of their former
flood-plains become terraces. (2) If an alluvial flood-plain has been built as
the result of an excessive supply of sediment (p. 186), the exhaustion or
withdrawal of the excessive supply would leave the stream again relatively
clear, and free to erode where it had been depositing. It would forthwith set
to work to carry away the material which it had temporarily unloaded on the
plain. The plains built up in many valleys in the northern part of our
continent during the glacial period, when the drainage from the ice coursed
through them, have subsequently been partially destroyed by erosion, and
their remnants have become terraces. A notable reduction in the amount of
available sediment, even when the earlier supply was not excessive,
produces a similar result. (3) A notable increase in the volume of a stream,
without corresponding increase in load, as when one stream captures
meander belt, the tendency being to reduce it to the level of the channel,
and, therefore, below the level of the flood-plain. As the meander belt
widens, the depression which it develops becomes more and more
capacious. Presently it may attain such dimensions as to hold the water of
ordinary floods. At this stage, or even before, such parts of the earlier flood-
plain as remain, are terraces.
These several tendencies conspire to partially destroy river flood-plains,
and to transform such parts as remain into terraces in the normal course of a
river’s history. They appear first in the lower part of the valley, and migrate
headward, following the course of nearly every other phase of activity in a
stream’s history. The heads of the terraces follow, at a respectful distance,
the head of the flood-plain, just as the head of the flood-plain follows at a
distance the head of the valley. The second and subsequent flood-plains and
the terraces to which they give origin follow the same course.
Terraces developed by the normal activities of a stream are always low,
and it is improbable that they would ordinarily be conspicuous. The vertical
distance between the first (highest) and second is greater than that between
the second and third. The principles developed on page 65 et seq., in
connection with the erosion of the hypothetical island, are applicable here.
Flood-plain terraces due to other causes.—Certain other causes,
accidental rather than normal to a stream, result in the development of
terraces from flood-plains. (1) If there be uplift in a region where the rivers
have flats, the streams are rejuvenated, and the remnants of their former
flood-plains become terraces. (2) If an alluvial flood-plain has been built as
the result of an excessive supply of sediment (p. 186), the exhaustion or
withdrawal of the excessive supply would leave the stream again relatively
clear, and free to erode where it had been depositing. It would forthwith set
to work to carry away the material which it had temporarily unloaded on the
plain. The plains built up in many valleys in the northern part of our
continent during the glacial period, when the drainage from the ice coursed
through them, have subsequently been partially destroyed by erosion, and
their remnants have become terraces. A notable reduction in the amount of
available sediment, even when the earlier supply was not excessive,
produces a similar result. (3) A notable increase in the volume of a stream,
without corresponding increase in load, as when one stream captures
Page 267
another, may occasion the development of terraces by allowing the stream
to deepen its channel. (4) Above any barrier which dams a stream, a flood-
plain is likely to be developed. When the barrier is removed the stream will
cut more or less deeply into the plain above, leaving terraces. (5) The
recession of a falls through a flood-plain converts such parts of it as remain,
into terraces.
In conclusion, it may be stated that many river terraces, mostly very low,
are normal features of valley development, coming into existence at definite
stages in a valley’s history. They are generally composed, in large part, of
river alluvium. Others result from more or less accidental causes, working
singly or in conjunction, and to this class belong all of the more
conspicuous terraces developed from flood-plains. The structure of a terrace
often affords some clue to its origin (Fig. 196).
Fig. 196.—Terraces partly of rock and partly of alluvium. Such terraces indicate successive
uplifts, or some other change which had a similar effect on the stream which made the
valley.
Discontinuity of terraces.—When a stream sinks its channel into its
flood-plain, it does not follow that a terrace remains on each side. Where
the stream’s deepened channel is in the middle of its flood-plain, there is,
temporarily, a terrace on either side; but wherever the deepened channel is
at one margin of its flood-plain, a terrace remains on the other side only.
Even where continuous at the outset, terraces soon become discontinuous,
for all processes of subaërial erosion conspire to destroy them. A stream is
likely to meander on its second and later flood-plains, as on its first and
highest one. Wherever the meanders on its second flood-plain reach the
borders of the first flood-plain, the terrace at that point disappears, and
since the meanders are continually migrating, terraces are continually
disappearing. The same would be true of the second terrace, if a second
were developed. The removal of portions of a terrace by the sweep of
meanders is likely to leave the remnants cuspate toward the stream.[91]
Again, tributary streams, in bringing their channels into topographic
adjustment with their mains, cut through the terraces of the latter. New
gullies develop on the faces of the terraces and their heads work back across
them, dissecting them still further. At the same time, sheet erosion and other
to deepen its channel. (4) Above any barrier which dams a stream, a flood-
plain is likely to be developed. When the barrier is removed the stream will
cut more or less deeply into the plain above, leaving terraces. (5) The
recession of a falls through a flood-plain converts such parts of it as remain,
into terraces.
In conclusion, it may be stated that many river terraces, mostly very low,
are normal features of valley development, coming into existence at definite
stages in a valley’s history. They are generally composed, in large part, of
river alluvium. Others result from more or less accidental causes, working
singly or in conjunction, and to this class belong all of the more
conspicuous terraces developed from flood-plains. The structure of a terrace
often affords some clue to its origin (Fig. 196).
Fig. 196.—Terraces partly of rock and partly of alluvium. Such terraces indicate successive
uplifts, or some other change which had a similar effect on the stream which made the
valley.
Discontinuity of terraces.—When a stream sinks its channel into its
flood-plain, it does not follow that a terrace remains on each side. Where
the stream’s deepened channel is in the middle of its flood-plain, there is,
temporarily, a terrace on either side; but wherever the deepened channel is
at one margin of its flood-plain, a terrace remains on the other side only.
Even where continuous at the outset, terraces soon become discontinuous,
for all processes of subaërial erosion conspire to destroy them. A stream is
likely to meander on its second and later flood-plains, as on its first and
highest one. Wherever the meanders on its second flood-plain reach the
borders of the first flood-plain, the terrace at that point disappears, and
since the meanders are continually migrating, terraces are continually
disappearing. The same would be true of the second terrace, if a second
were developed. The removal of portions of a terrace by the sweep of
meanders is likely to leave the remnants cuspate toward the stream.[91]
Again, tributary streams, in bringing their channels into topographic
adjustment with their mains, cut through the terraces of the latter. New
gullies develop on the faces of the terraces and their heads work back across
them, dissecting them still further. At the same time, sheet erosion and other
Page 268
phases of slope wash tend to drive the scarps of the terraces back toward the
bluff beyond. By the time a second series of terraces is well developed, no
more than meagre remnants of the first may remain.
From the foregoing considerations it is clear that the extent to which river
terraces once developed, now remain, is dependent in part on the length of
time which has elapsed since the river sank its channel below them. Other
things being equal, the greater their age the more meagre their remnants.
Terraces developed from river plains formed chiefly by alluviation stand
a better chance of long life than most other alluvial terraces. This is because
of the configuration of the original valley, the aggradation of which gave
origin to the plain. The principle involved is illustrated by Fig. 197. In
developing the second flood-plain the river encounters the rock wall of the
valley. This greatly retards lateral erosion, and the terrace above,
defended[92] by the rock, is likely to be long-lived.
Fig. 197.—Diagram to show why certain terraces are longer lived than others.
Alluvial terraces, like rock shelves, are popularly thought to mark “old
levels of the river.” In one sense this is true, but not in the sense in which
the expression is commonly used. Every level, from the crest of the
bounding bluffs to the bottom of a valley, is a level at which water ran for a
longer or shorter time; but the terrace does not mean that the river was once
so much larger than now as to fill the valley from its present channel to the
level of the terraces.
Termini of terraces.—From the mode of development of terraces it will
be seen that, traced up-stream, each terrace should theoretically grade into a
flood-plain at its upper end (Fig. 194), and that the upper end of the second
(from the top) terrace, where there are two, would not be so far up-stream
as the upper end of the first (highest). This is represented diagrammatically
in Fig. 198.
The down-stream termini of terraces are rarely distinct. This is partly
because the notable meandering of the streams in their lower courses is
antagonistic to the preservation of terraces. If all terraces once developed
remained, and if delta-building proceeded without interruption from waves,
bluff beyond. By the time a second series of terraces is well developed, no
more than meagre remnants of the first may remain.
From the foregoing considerations it is clear that the extent to which river
terraces once developed, now remain, is dependent in part on the length of
time which has elapsed since the river sank its channel below them. Other
things being equal, the greater their age the more meagre their remnants.
Terraces developed from river plains formed chiefly by alluviation stand
a better chance of long life than most other alluvial terraces. This is because
of the configuration of the original valley, the aggradation of which gave
origin to the plain. The principle involved is illustrated by Fig. 197. In
developing the second flood-plain the river encounters the rock wall of the
valley. This greatly retards lateral erosion, and the terrace above,
defended[92] by the rock, is likely to be long-lived.
Fig. 197.—Diagram to show why certain terraces are longer lived than others.
Alluvial terraces, like rock shelves, are popularly thought to mark “old
levels of the river.” In one sense this is true, but not in the sense in which
the expression is commonly used. Every level, from the crest of the
bounding bluffs to the bottom of a valley, is a level at which water ran for a
longer or shorter time; but the terrace does not mean that the river was once
so much larger than now as to fill the valley from its present channel to the
level of the terraces.
Termini of terraces.—From the mode of development of terraces it will
be seen that, traced up-stream, each terrace should theoretically grade into a
flood-plain at its upper end (Fig. 194), and that the upper end of the second
(from the top) terrace, where there are two, would not be so far up-stream
as the upper end of the first (highest). This is represented diagrammatically
in Fig. 198.
The down-stream termini of terraces are rarely distinct. This is partly
because the notable meandering of the streams in their lower courses is
antagonistic to the preservation of terraces. If all terraces once developed
remained, and if delta-building proceeded without interruption from waves,
Page 269
the relations should be somewhat as follows: Traced down-stream, the cliff
between the oldest (highest) terrace and the next younger becomes
gradually lower until it finally disappears, and the continuation of the two is
found in a common plain. The cliff between the second and third terraces
should disappear in the same way, and below its disappearance the plain
representing their continuation is continuous with that representing the
continuation of the first and second. The cliff between the second and third
terraces may or may not continue farther down-stream than that between the
first and second. The plains below the terraces finally become continuous
with the lowest flood-plain and with the delta. These relations can rarely be
seen because of the destruction of the older terraces, and because of the
erosion by waves along shore.
Fig. 198.—Diagram looking up the valley, showing two terraces below, one in the middle,
and none above. The relations are purely diagrammatic.
The topography of terraces is similar to that of flood-plains, except in so
far as modified by erosion. While flat in general, the terrace may slope
either toward or from the valley bluff, and its surface may be marked by all
the minor irregularities which characterize a flood-plain.
between the oldest (highest) terrace and the next younger becomes
gradually lower until it finally disappears, and the continuation of the two is
found in a common plain. The cliff between the second and third terraces
should disappear in the same way, and below its disappearance the plain
representing their continuation is continuous with that representing the
continuation of the first and second. The cliff between the second and third
terraces may or may not continue farther down-stream than that between the
first and second. The plains below the terraces finally become continuous
with the lowest flood-plain and with the delta. These relations can rarely be
seen because of the destruction of the older terraces, and because of the
erosion by waves along shore.
Fig. 198.—Diagram looking up the valley, showing two terraces below, one in the middle,
and none above. The relations are purely diagrammatic.
The topography of terraces is similar to that of flood-plains, except in so
far as modified by erosion. While flat in general, the terrace may slope
either toward or from the valley bluff, and its surface may be marked by all
the minor irregularities which characterize a flood-plain.
Page 270
CHAPTER IV.
THE WORK OF GROUND- (UNDERGROUND) WATER.
Many familiar facts demonstrate the general presence of abundant water beneath the surface of the land. The
thousands of wells in regions peopled by civilized races, and the countless springs which issue from the sides of
mountains and valleys are a sufficient proof both of the wide distribution of ground-water and of its great
abundance.
Certain well-known facts make it clear that ground-water is intimately connected with rainfall. In a dry season
the level of the water in wells commonly sinks, and after a heavy rain it rises (p. 71); and the amount of sinking
is greater when the drought is long, and the rise is most notable when the rainfall is heavy. Many springs which
discharge large quantities of water during a wet season flow with reduced volume, or cease to flow altogether in
periods of drought. Furthermore, the water of springs and wells has the properties which rain-water would
possess after sinking beneath the surface and dissolving mineral substances. Rain-water is seen to sink beneath
the surface with every shower, and since this source seems altogether adequate for ground-water, and since no
other source is known whence any considerable amount of ground-water might come, it is concluded that
atmospheric precipitation is its chief source.
Water gets beneath the surface by processes which are readily seen. Wherever the soil is porous some of the
rain which falls upon it is absorbed. Sinking through the soil to the solid rock it finds cracks and pores through
which it descends to great depths. Nowhere are the rocks beneath the mantle rock so compact and so free from
cracks, when any considerable area is considered, as to prevent the percolation of water through them.
Conditions influencing descent of rain-water.—There are several conditions which influence not only the
amount of water which sinks beneath the surface in a given area, but the proportion of the precipitation which
follows this course. These are as follows: (1) Amount of precipitation.—In a general way it is true that the
greater the amount of precipitation the greater the amount of water which will sink beneath the surface. Other
things being equal, a region of heavy precipitation is a region where wells are easily obtained and springs
common. (2) Rate of precipitation.—A given amount of precipitation may be concentrated in a short interval, or
distributed through a considerable period of time. In the latter case more of the water sinks beneath the surface;
in the former, a larger proportion runs off over the surface. The reason is readily seen. Water passes through
small spaces, such as those of soil, slowly, and its rate of passage decreases rapidly with decreasing size of the
passageways. When rain falls rapidly on a surface of even moderately close texture, the uppermost layer of soil
is promptly filled with water, and since the water passes downward slowly, the uppermost saturated part of the
soil becomes virtually impervious. While in this condition, the water which falls on it will run off if there be
slope, and stand if there be none. In the latter case it will sink slowly as the water in the soil passes down to
lower levels. If precipitation takes place no faster than the water can sink through the soil, all the water may
become ground-water. (3) The topography of the surface has much to do with determining the proportion of
rainfall which becomes ground-water. If the surface be flat, more will sink in; if it be sloping, more of it will run
off before it has time to sink. Other things being equal, the steeper the slope the larger the proportion of the
rainfall which will run off over it. (4) The texture of the soil, or other material on which the rain falls, helps to
determine what proportion of it sinks beneath the surface. If the surface materials be porous, the water sinks
readily; if of close texture, it finds less ready ingress. Other things being equal, the closer the texture of the soil
the less the proportion of the rainfall which will enter it. (5) The texture and structure of the rock beneath the
surface have some influence on the amount of ground-water. The rock may be stratified or massive; it may be
abundantly or sparsely jointed; it may be porous or compact. On the whole, stratified rock is more favorable for
the entrance of water than unstratified, partly because of its greater average porosity, and partly because the
planes of division between beds often allow the passage of water. If the beds of stratified rock are vertical or
inclined, water finds its way into them more readily than if they are horizontal, in so far as it descends along
THE WORK OF GROUND- (UNDERGROUND) WATER.
Many familiar facts demonstrate the general presence of abundant water beneath the surface of the land. The
thousands of wells in regions peopled by civilized races, and the countless springs which issue from the sides of
mountains and valleys are a sufficient proof both of the wide distribution of ground-water and of its great
abundance.
Certain well-known facts make it clear that ground-water is intimately connected with rainfall. In a dry season
the level of the water in wells commonly sinks, and after a heavy rain it rises (p. 71); and the amount of sinking
is greater when the drought is long, and the rise is most notable when the rainfall is heavy. Many springs which
discharge large quantities of water during a wet season flow with reduced volume, or cease to flow altogether in
periods of drought. Furthermore, the water of springs and wells has the properties which rain-water would
possess after sinking beneath the surface and dissolving mineral substances. Rain-water is seen to sink beneath
the surface with every shower, and since this source seems altogether adequate for ground-water, and since no
other source is known whence any considerable amount of ground-water might come, it is concluded that
atmospheric precipitation is its chief source.
Water gets beneath the surface by processes which are readily seen. Wherever the soil is porous some of the
rain which falls upon it is absorbed. Sinking through the soil to the solid rock it finds cracks and pores through
which it descends to great depths. Nowhere are the rocks beneath the mantle rock so compact and so free from
cracks, when any considerable area is considered, as to prevent the percolation of water through them.
Conditions influencing descent of rain-water.—There are several conditions which influence not only the
amount of water which sinks beneath the surface in a given area, but the proportion of the precipitation which
follows this course. These are as follows: (1) Amount of precipitation.—In a general way it is true that the
greater the amount of precipitation the greater the amount of water which will sink beneath the surface. Other
things being equal, a region of heavy precipitation is a region where wells are easily obtained and springs
common. (2) Rate of precipitation.—A given amount of precipitation may be concentrated in a short interval, or
distributed through a considerable period of time. In the latter case more of the water sinks beneath the surface;
in the former, a larger proportion runs off over the surface. The reason is readily seen. Water passes through
small spaces, such as those of soil, slowly, and its rate of passage decreases rapidly with decreasing size of the
passageways. When rain falls rapidly on a surface of even moderately close texture, the uppermost layer of soil
is promptly filled with water, and since the water passes downward slowly, the uppermost saturated part of the
soil becomes virtually impervious. While in this condition, the water which falls on it will run off if there be
slope, and stand if there be none. In the latter case it will sink slowly as the water in the soil passes down to
lower levels. If precipitation takes place no faster than the water can sink through the soil, all the water may
become ground-water. (3) The topography of the surface has much to do with determining the proportion of
rainfall which becomes ground-water. If the surface be flat, more will sink in; if it be sloping, more of it will run
off before it has time to sink. Other things being equal, the steeper the slope the larger the proportion of the
rainfall which will run off over it. (4) The texture of the soil, or other material on which the rain falls, helps to
determine what proportion of it sinks beneath the surface. If the surface materials be porous, the water sinks
readily; if of close texture, it finds less ready ingress. Other things being equal, the closer the texture of the soil
the less the proportion of the rainfall which will enter it. (5) The texture and structure of the rock beneath the
surface have some influence on the amount of ground-water. The rock may be stratified or massive; it may be
abundantly or sparsely jointed; it may be porous or compact. On the whole, stratified rock is more favorable for
the entrance of water than unstratified, partly because of its greater average porosity, and partly because the
planes of division between beds often allow the passage of water. If the beds of stratified rock are vertical or
inclined, water finds its way into them more readily than if they are horizontal, in so far as it descends along
Page 271
stratification planes. Horizontally bedded rock, or rock which is not bedded at all, may be so much jointed, and
the joints so open, as to allow the water to enter readily.
The conditions favorable to the sinking of abundant water below the surface are therefore heavy precipitation,
falling slowly on a surface with little relief, a soil of open texture underlain by rock which is porous, or affected
by vertical or highly inclined planes of cleavage. The annual discharge of water by rivers is estimated to be
about 22 percent. of the rainfall on the land.[93]
Supply of ground-water not altogether dependent on local rainfall.—The amount of ground-water in a
given region is not always entirely dependent on the local rainfall. Ground-water is in constant movement, and
entering the soil or rock at one point it may, after a long subterranean journey, reach a point far from that at
which it entered. Thus beneath the Great Plains of the West there is much subterranean water which fell on the
eastern slopes of the mountains to the west. It has flowed beneath the surface to the Plains, where some of it is
now withdrawn for the purposes of irrigation in regions where rainfall is deficient. The accompanying diagram
(Fig. 199) illustrates the flow here described.
Fig. 199.—Diagram illustrating the general point that ground-water is not dependent entirely upon local supply.
Fig. 200.—Diagram illustrating the position of the ground-water surface (the dotted line) in a region of undulatory topography.
The ground-water surface. Water table.—The water table has already been defined (p. 71) as the upper
surface of the ground-water. In a flat region of uniform structure the ground-water surface is essentially level,
but rises and falls with the rainfall. Where the topography of a region is not flat, the ground-water surface is not
level. As a rule it is higher, though farther below the surface, under an elevation than under surrounding
lowlands, as illustrated by Fig. 200. The explanation is not far to seek. If a hill of sand be exposed to rainfall,
most of the water falling on its porous surface will sink into it. If the precipitation continues long enough, as in a
protracted rain, the hill of sand will be filled with water, the water occupying the interstices between the grains.
If the sand of the hill could be removed, leaving the water which it contains on the same area, it would constitute
a mound perhaps a third or a fourth as high as the hill itself. If unsupported, this mound of water would spread
promptly in all directions until its surface was level. While the sand remains, the water in it constitutes a mound,
and has a tendency to spread. It does in fact spread, but since the process involves great friction the spreading is
slow. With the spreading the surface of the water in the sand sinks, and sinks fastest at the center where it is
highest (b, Fig. 201). If the process were not interrupted the surface of the water in the hill would, in time, sink
approximately to the level of the water in the surrounding land (d, Fig. 201); but at every stage preceding the
last, the surface of the water would be higher beneath the summit of the hill than elsewhere, though farther from
the surface. In regions of even moderate precipitation the water surface beneath the hills rarely sinks to the level
of that in the lowlands adjacent, before being raised by further rains.
Fig. 201.—Diagram to illustrate the relations of ground-water to the surface.
The water-level beneath the lowlands also sinks. Some of it finds its way into valleys, some of it sinks to
greater depths, and some of it evaporates; but since the water surface beneath the elevation sinks more rapidly
the joints so open, as to allow the water to enter readily.
The conditions favorable to the sinking of abundant water below the surface are therefore heavy precipitation,
falling slowly on a surface with little relief, a soil of open texture underlain by rock which is porous, or affected
by vertical or highly inclined planes of cleavage. The annual discharge of water by rivers is estimated to be
about 22 percent. of the rainfall on the land.[93]
Supply of ground-water not altogether dependent on local rainfall.—The amount of ground-water in a
given region is not always entirely dependent on the local rainfall. Ground-water is in constant movement, and
entering the soil or rock at one point it may, after a long subterranean journey, reach a point far from that at
which it entered. Thus beneath the Great Plains of the West there is much subterranean water which fell on the
eastern slopes of the mountains to the west. It has flowed beneath the surface to the Plains, where some of it is
now withdrawn for the purposes of irrigation in regions where rainfall is deficient. The accompanying diagram
(Fig. 199) illustrates the flow here described.
Fig. 199.—Diagram illustrating the general point that ground-water is not dependent entirely upon local supply.
Fig. 200.—Diagram illustrating the position of the ground-water surface (the dotted line) in a region of undulatory topography.
The ground-water surface. Water table.—The water table has already been defined (p. 71) as the upper
surface of the ground-water. In a flat region of uniform structure the ground-water surface is essentially level,
but rises and falls with the rainfall. Where the topography of a region is not flat, the ground-water surface is not
level. As a rule it is higher, though farther below the surface, under an elevation than under surrounding
lowlands, as illustrated by Fig. 200. The explanation is not far to seek. If a hill of sand be exposed to rainfall,
most of the water falling on its porous surface will sink into it. If the precipitation continues long enough, as in a
protracted rain, the hill of sand will be filled with water, the water occupying the interstices between the grains.
If the sand of the hill could be removed, leaving the water which it contains on the same area, it would constitute
a mound perhaps a third or a fourth as high as the hill itself. If unsupported, this mound of water would spread
promptly in all directions until its surface was level. While the sand remains, the water in it constitutes a mound,
and has a tendency to spread. It does in fact spread, but since the process involves great friction the spreading is
slow. With the spreading the surface of the water in the sand sinks, and sinks fastest at the center where it is
highest (b, Fig. 201). If the process were not interrupted the surface of the water in the hill would, in time, sink
approximately to the level of the water in the surrounding land (d, Fig. 201); but at every stage preceding the
last, the surface of the water would be higher beneath the summit of the hill than elsewhere, though farther from
the surface. In regions of even moderate precipitation the water surface beneath the hills rarely sinks to the level
of that in the lowlands adjacent, before being raised by further rains.
Fig. 201.—Diagram to illustrate the relations of ground-water to the surface.
The water-level beneath the lowlands also sinks. Some of it finds its way into valleys, some of it sinks to
greater depths, and some of it evaporates; but since the water surface beneath the elevation sinks more rapidly
Page 272
than that beneath the lowland, the two approach a common level. Their difference will be least at the end of a
drought, and greatest just after heavy rains.
Depth to which ground-water sinks.—The depth to which ground-water penetrates has not been determined
empirically. No borings or excavations of any sort have been made to such depths as to indicate that its limit was
being approached, though some of them are a mile or more deep. There is a popular belief that water sinks until
it reaches a temperature sufficient to convert it into steam, but except for special localities where hot lava lies
near the surface, this belief is not well founded. In the first place, it is not known at what temperature water
below the surface would be converted into steam. While water boils at sea-level at a temperature of 212° (Fahr.)
a higher temperature would be necessary below that level.
Assuming the temperature of water sinking beneath the surface to be 50° Fahr., its temperature must be raised
162° to bring it to the temperature at which it would boil at sea-level. On the above assumption of initial
temperature, the following table shows the depths at which water would reach a temperature of 212° Fahr. under
various assumptions as to the rate of increase of temperature. It shows also the pressure in atmospheres which
would exist at these several depths if the overlying rock were full of water.
Depth at which
Rate of Increase Equivalent Pressure
Temperature of 212°
of Temperature. in Atmospheres.
would be reached.
1° for 50 feet 8,100 feet 238 (approximately)
1° for 60 “ 9,720 “ 285 “
1° for 70 “ 11,340 “ 333 “
With an initial temperature of 80°, corresponding to that of the warmer parts of the earth’s surface, instead of
50°, the table would be as follows:
1° for 50 feet 6,600 feet 194 (approximately)
1° for 60 “ 7,920 “ 214 “
1° for 70 “ 9,240 “ 272 “
The temperature at which water boils increases with the pressure. A pressure of about 200 atmospheres is the
critical pressure for water; that is, the pressure which, if increased, will prevent boiling altogether. The depth at
which a pressure of 200 atmospheres would be reached, supposing the upper rock to be full of water, is about
6800 feet. The temperature of the water at this depth, under various assumptions as to initial temperature and
rate of increase of heat, is shown in the following table:
Rate of Increase Temperature at a
Initial Temperature.
of Temperature. Depth of 6,800 Feet.
50° 1° for 50 feet 186° Fahr.
50° 1° for 60 “ 163° “
50° 1° for 70 “ 147° “
80° 1° for 50 “ 216° “
80° 1° for 60 “ 193° “
80° 1° for 70 “ 177° “
Only one of these temperatures reaches the boiling-point of water at sea-level. It is therefore clear that at this
depth water has not even closely approached the boiling temperature for this depth, and since this is the depth of
the critical pressure, it is clear that it cannot boil at any greater depth. The descent of water is therefore not
stopped, under normal conditions of crustal temperature, because it reaches its boiling-point. Locally, as in the
vicinity of active or recently extinct volcanoes, the case may be different.
It is conceivable that water may descend until it reaches its critical temperature (somewhere between 610° and
635° Fahr.). The depth at which the critical temperature would be reached, under various assumptions, is shown
in the following table:
Rate of Increase
Initial Temperature. Depth of Critical Temperature.
of Temperature.
50° 1° for 50 feet 28,000 to 29,250 feet
50° 1° for 60 “ 33,600 to 35,100 “
50° 1° for 70 “ 39,200 to 40,950 “
80° 1° for 50 “ 26,500 to 27,750 “
80° 1° for 60 “ 31,800 to 33,300 “
80° 1° for 70 “ 37,100 to 38,850 “
drought, and greatest just after heavy rains.
Depth to which ground-water sinks.—The depth to which ground-water penetrates has not been determined
empirically. No borings or excavations of any sort have been made to such depths as to indicate that its limit was
being approached, though some of them are a mile or more deep. There is a popular belief that water sinks until
it reaches a temperature sufficient to convert it into steam, but except for special localities where hot lava lies
near the surface, this belief is not well founded. In the first place, it is not known at what temperature water
below the surface would be converted into steam. While water boils at sea-level at a temperature of 212° (Fahr.)
a higher temperature would be necessary below that level.
Assuming the temperature of water sinking beneath the surface to be 50° Fahr., its temperature must be raised
162° to bring it to the temperature at which it would boil at sea-level. On the above assumption of initial
temperature, the following table shows the depths at which water would reach a temperature of 212° Fahr. under
various assumptions as to the rate of increase of temperature. It shows also the pressure in atmospheres which
would exist at these several depths if the overlying rock were full of water.
Depth at which
Rate of Increase Equivalent Pressure
Temperature of 212°
of Temperature. in Atmospheres.
would be reached.
1° for 50 feet 8,100 feet 238 (approximately)
1° for 60 “ 9,720 “ 285 “
1° for 70 “ 11,340 “ 333 “
With an initial temperature of 80°, corresponding to that of the warmer parts of the earth’s surface, instead of
50°, the table would be as follows:
1° for 50 feet 6,600 feet 194 (approximately)
1° for 60 “ 7,920 “ 214 “
1° for 70 “ 9,240 “ 272 “
The temperature at which water boils increases with the pressure. A pressure of about 200 atmospheres is the
critical pressure for water; that is, the pressure which, if increased, will prevent boiling altogether. The depth at
which a pressure of 200 atmospheres would be reached, supposing the upper rock to be full of water, is about
6800 feet. The temperature of the water at this depth, under various assumptions as to initial temperature and
rate of increase of heat, is shown in the following table:
Rate of Increase Temperature at a
Initial Temperature.
of Temperature. Depth of 6,800 Feet.
50° 1° for 50 feet 186° Fahr.
50° 1° for 60 “ 163° “
50° 1° for 70 “ 147° “
80° 1° for 50 “ 216° “
80° 1° for 60 “ 193° “
80° 1° for 70 “ 177° “
Only one of these temperatures reaches the boiling-point of water at sea-level. It is therefore clear that at this
depth water has not even closely approached the boiling temperature for this depth, and since this is the depth of
the critical pressure, it is clear that it cannot boil at any greater depth. The descent of water is therefore not
stopped, under normal conditions of crustal temperature, because it reaches its boiling-point. Locally, as in the
vicinity of active or recently extinct volcanoes, the case may be different.
It is conceivable that water may descend until it reaches its critical temperature (somewhere between 610° and
635° Fahr.). The depth at which the critical temperature would be reached, under various assumptions, is shown
in the following table:
Rate of Increase
Initial Temperature. Depth of Critical Temperature.
of Temperature.
50° 1° for 50 feet 28,000 to 29,250 feet
50° 1° for 60 “ 33,600 to 35,100 “
50° 1° for 70 “ 39,200 to 40,950 “
80° 1° for 50 “ 26,500 to 27,750 “
80° 1° for 60 “ 31,800 to 33,300 “
80° 1° for 70 “ 37,100 to 38,850 “
Page 273
There is good reason, in the increasing density beneath the surface, for believing that the rate of increase of
temperature decreases with depth, and therefore that the rate of 1° for 50 feet for the depths concerned is too
high. The greater depths of the table above are therefore believed to more nearly represent the truth than the
lesser ones. (See discussion of underground temperature in Chapter XI.)
If descending water attained its critical temperature, the extent to which the resulting water-gas might be
absorbed is not known. So far as limited by temperature, therefore, it is not possible to assign a limit to the
descent of water under average conditions of crustal temperature.
Other considerations seem to place a limit to the descent of water. Rock, solid and unyielding as it seems, is
yet plastic when under sufficiently great pressure. The cracks and cavities affecting it are believed to descend a
distance which is but slight in comparison with the radius of the earth. Even if openings were once formed at
greater depths, they could not persist, for the adjacent rock, under the pressure which there exists, would “flow”
in, in effect (though perhaps not in principle) much as stiff liquid might, and close them. The outer zone of the
earth where cavities may exist is known as the zone of fracture.[94] The depth of the zone of fracture differs for
different rocks, but is not believed to extend below some such depth as five or six miles, even for the most
resistant.[95] It is to be noted that these depths are less than those at which the critical temperature of water would
be reached under most of the conditions, including all the more probable ones, specified in the above table.
Let it be assumed that water descends through openings in the rock to a depth of six miles. At this depth it
would, under the various assumptions specified in the first and second columns of the following table, have the
temperature indicated in the third column:
Rate of Increase Temperature at
Initial Temperature.
of Temperature. Depth of Six Miles.
50° 1° for 50 feet 683° Fahr.
50° 1° for 60 “ 578° “
50° 1° for 70 “ 502° “
80° 1° for 50 “ 713° “
80° 1° for 60 “ 608° “
80° 1° for 70 “ 532° “
In two of these cases, namely, those in which the assumed rate of increase of temperature is highest, the
temperature of the water at the assumed lower limit of the zone of fracture is above the critical temperature of
water. If the assumptions involved in these two cases be correct, water might descend to the point where it
would be converted into water-gas, and in this condition it might be occluded by the hot rock. In the other cases,
involving the more probable assumptions, the critical temperature is not reached at a depth of six miles. If pores
and cracks do not extend to greater depths, liquid water could not; and since the water at this depth has probably
not reached its critical temperature, it cannot exist as water-gas. If it does not exist in the form of water-gas, its
occlusion by the hot rock substance would not be probable. It would seem, therefore, that the descent of water
under ordinary conditions is much more likely to be limited by the zone of fracture, than by temperature.
Movement of ground-water.[96]—Ground-water is in more or less continual movement. If all the water be
pumped out of a well it soon fills up again to its normal level by inflow from all sides. Springs and flowing
wells also demonstrate the movement of ground-water. Near the surface the movement of ground-water is
primarily downward if the medium through which it passes is equally permeable in all directions; but so soon as
the descending water reaches the water surface, its descent is checked and its movement is partly lateral.
The commonest sort of movement of ground-water is that exemplified as the water sinks beneath the surface,
namely, slow percolation through the pores and cracks of the soil and rock. Ground-water is not generally
organized into definite streams, though underground streams, mostly small, are sometimes seen in caves and
crevices, and sometimes issue as springs. Most underground streams which issue as springs probably have
definite channels for short distances only before they issue. It is probable that ground-water frequently flows in
considerable quantity along somewhat definite planes, without having open channels. Thus every porous bed of
rock is likely to serve as the pathway along which subterranean drainage passes. This is especially true where
the porous bed is underlain by an impervious one. The “reservoirs” from which artesian wells draw their supply
are not usually streams or lakes, but porous beds of rock through which abundant water passes. As the supply is
drawn off at one point, it is renewed by water entering elsewhere. Since the freedom of movement of ground-
water is notably influenced by the porosity of the rock, and since the rock is, on the average, most porous and
the pores largest near the surface, the movement of ground-water is, on the average, greatest near the surface,
temperature decreases with depth, and therefore that the rate of 1° for 50 feet for the depths concerned is too
high. The greater depths of the table above are therefore believed to more nearly represent the truth than the
lesser ones. (See discussion of underground temperature in Chapter XI.)
If descending water attained its critical temperature, the extent to which the resulting water-gas might be
absorbed is not known. So far as limited by temperature, therefore, it is not possible to assign a limit to the
descent of water under average conditions of crustal temperature.
Other considerations seem to place a limit to the descent of water. Rock, solid and unyielding as it seems, is
yet plastic when under sufficiently great pressure. The cracks and cavities affecting it are believed to descend a
distance which is but slight in comparison with the radius of the earth. Even if openings were once formed at
greater depths, they could not persist, for the adjacent rock, under the pressure which there exists, would “flow”
in, in effect (though perhaps not in principle) much as stiff liquid might, and close them. The outer zone of the
earth where cavities may exist is known as the zone of fracture.[94] The depth of the zone of fracture differs for
different rocks, but is not believed to extend below some such depth as five or six miles, even for the most
resistant.[95] It is to be noted that these depths are less than those at which the critical temperature of water would
be reached under most of the conditions, including all the more probable ones, specified in the above table.
Let it be assumed that water descends through openings in the rock to a depth of six miles. At this depth it
would, under the various assumptions specified in the first and second columns of the following table, have the
temperature indicated in the third column:
Rate of Increase Temperature at
Initial Temperature.
of Temperature. Depth of Six Miles.
50° 1° for 50 feet 683° Fahr.
50° 1° for 60 “ 578° “
50° 1° for 70 “ 502° “
80° 1° for 50 “ 713° “
80° 1° for 60 “ 608° “
80° 1° for 70 “ 532° “
In two of these cases, namely, those in which the assumed rate of increase of temperature is highest, the
temperature of the water at the assumed lower limit of the zone of fracture is above the critical temperature of
water. If the assumptions involved in these two cases be correct, water might descend to the point where it
would be converted into water-gas, and in this condition it might be occluded by the hot rock. In the other cases,
involving the more probable assumptions, the critical temperature is not reached at a depth of six miles. If pores
and cracks do not extend to greater depths, liquid water could not; and since the water at this depth has probably
not reached its critical temperature, it cannot exist as water-gas. If it does not exist in the form of water-gas, its
occlusion by the hot rock substance would not be probable. It would seem, therefore, that the descent of water
under ordinary conditions is much more likely to be limited by the zone of fracture, than by temperature.
Movement of ground-water.[96]—Ground-water is in more or less continual movement. If all the water be
pumped out of a well it soon fills up again to its normal level by inflow from all sides. Springs and flowing
wells also demonstrate the movement of ground-water. Near the surface the movement of ground-water is
primarily downward if the medium through which it passes is equally permeable in all directions; but so soon as
the descending water reaches the water surface, its descent is checked and its movement is partly lateral.
The commonest sort of movement of ground-water is that exemplified as the water sinks beneath the surface,
namely, slow percolation through the pores and cracks of the soil and rock. Ground-water is not generally
organized into definite streams, though underground streams, mostly small, are sometimes seen in caves and
crevices, and sometimes issue as springs. Most underground streams which issue as springs probably have
definite channels for short distances only before they issue. It is probable that ground-water frequently flows in
considerable quantity along somewhat definite planes, without having open channels. Thus every porous bed of
rock is likely to serve as the pathway along which subterranean drainage passes. This is especially true where
the porous bed is underlain by an impervious one. The “reservoirs” from which artesian wells draw their supply
are not usually streams or lakes, but porous beds of rock through which abundant water passes. As the supply is
drawn off at one point, it is renewed by water entering elsewhere. Since the freedom of movement of ground-
water is notably influenced by the porosity of the rock, and since the rock is, on the average, most porous and
the pores largest near the surface, the movement of ground-water is, on the average, greatest near the surface,
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and least at its lower limit. In general the decrease of movement is much more rapid than the decrease in the size
of the pores. It follows that while the upper part of the ground-water, especially that above ground-water level,
moves somewhat freely, the lower part moves much more slowly. It is probable, indeed, that the movement in
the lower part of the subterranean hydrosphere is extremely slight.
The amount of ground-water.—The porosity of surface rocks varies widely, and the porosity of but few has
been determined.[97] Such determinations as have been made are chiefly on building stones, in which the range of
porosity varies from a fraction of one percent., in the case of granite, to nearly 30 percent. in the case of some
sandstones. Building stone is perhaps more dense than the average surface rock. Furthermore, such tests as have
been made do not take account of the larger cracks and openings of rock, for these would not appear in the
specimens tested; nor of the mantle rock, which generally contains a large amount of water. From such
determinations as have been made it is estimated that the average porosity of the outer part of the lithosphere is
somewhere between 5 and 10 percent. If the porosity diminishes regularly to a depth of six miles, where it
becomes zero, the average porosity to this depth would be half the surface porosity.[98] An average porosity of
two and one-half percent. would mean that the rock contains enough water to form a layer nearly 800 feet deep.
With an average porosity of 5 percent., this figure would be doubled.[99] While these figures are not to be
regarded as measurements, they perhaps give some idea of the amount of ground-water. It is this sphere of
ground-water which justifies the term hydrosphere, as applied to the waters of the earth.
Fate of ground-water.—Most of the water which sinks into the earth reaches the surface again after a longer
or shorter journey. Some of it is evaporated from the surface directly; some of it is taken up by plants and is
passed by them into the atmosphere; some of it issues in the form of springs; some of it seeps out; some of it is
drawn out through wells; and much of the remainder finds its way underground to the sea or to lakes, issuing as
springs beneath them. A small portion of the descending waters enters into permanent combination with mineral
matter. Many minerals are known to take up water, being changed thereby from an anhydrous to a hydrous
condition. It does not necessarily follow, however, that the total supply of water is thereby decreasing. Minerals
once hydrated may be dehydrated subsequently, the water being set free. Furthermore, considerable quantities of
water in the form of vapor issue from volcanoes, and volcanic vents often continue to steam long after volcanic
action proper has ceased. It is probable that some, and perhaps much of the water issuing from these vents has
never been at the surface before, and it is not now possible to affirm that the supply from this source does not
offset, or even surpass, the depletion of the hydrosphere resulting from mineral hydration.
THE WORK OF GROUND-WATER.
Ground-water effects very considerable results in the course of its history. These results are partly chemical
and partly mechanical, the former being far more important than the latter.
Chemical Work.
The results of the chemical and chemico-physical action of water may be grouped in several more or less
distinct categories.
1. The simplest effect is the subtraction of soluble mineral matter. Pure water is in itself a solvent of certain
minerals; but the carbonic-acid gas extracted from the atmosphere, and the products of organic decay extracted
from the soil make ground-water a much more efficient solvent. Something of the results which it achieves is
shown by its composition. All ground-water, whether issuing as springs or drawn out through wells, contains
much more mineral matter than the water which falls as rain, and the excess is acquired in its underground
course.
The subtraction of soluble matter from rock renders it porous. The amount of material dissolved from a given
place may be trivial or considerable, according to the character of the rock, the readiness with which water has
access to it, and the character of the water. Locally, the subtraction of mineral matter may be the chief, or even
the only appreciable, effect of the ground-water.
2. It sometimes happens that ground-water with certain mineral substances in solution exchanges them for
other substances extracted from the rock. Thus the process of substitution is effected. By this process the lime
carbonate of a shell imbedded in rock may be removed, molecule by molecule, and some other substance, such
of the pores. It follows that while the upper part of the ground-water, especially that above ground-water level,
moves somewhat freely, the lower part moves much more slowly. It is probable, indeed, that the movement in
the lower part of the subterranean hydrosphere is extremely slight.
The amount of ground-water.—The porosity of surface rocks varies widely, and the porosity of but few has
been determined.[97] Such determinations as have been made are chiefly on building stones, in which the range of
porosity varies from a fraction of one percent., in the case of granite, to nearly 30 percent. in the case of some
sandstones. Building stone is perhaps more dense than the average surface rock. Furthermore, such tests as have
been made do not take account of the larger cracks and openings of rock, for these would not appear in the
specimens tested; nor of the mantle rock, which generally contains a large amount of water. From such
determinations as have been made it is estimated that the average porosity of the outer part of the lithosphere is
somewhere between 5 and 10 percent. If the porosity diminishes regularly to a depth of six miles, where it
becomes zero, the average porosity to this depth would be half the surface porosity.[98] An average porosity of
two and one-half percent. would mean that the rock contains enough water to form a layer nearly 800 feet deep.
With an average porosity of 5 percent., this figure would be doubled.[99] While these figures are not to be
regarded as measurements, they perhaps give some idea of the amount of ground-water. It is this sphere of
ground-water which justifies the term hydrosphere, as applied to the waters of the earth.
Fate of ground-water.—Most of the water which sinks into the earth reaches the surface again after a longer
or shorter journey. Some of it is evaporated from the surface directly; some of it is taken up by plants and is
passed by them into the atmosphere; some of it issues in the form of springs; some of it seeps out; some of it is
drawn out through wells; and much of the remainder finds its way underground to the sea or to lakes, issuing as
springs beneath them. A small portion of the descending waters enters into permanent combination with mineral
matter. Many minerals are known to take up water, being changed thereby from an anhydrous to a hydrous
condition. It does not necessarily follow, however, that the total supply of water is thereby decreasing. Minerals
once hydrated may be dehydrated subsequently, the water being set free. Furthermore, considerable quantities of
water in the form of vapor issue from volcanoes, and volcanic vents often continue to steam long after volcanic
action proper has ceased. It is probable that some, and perhaps much of the water issuing from these vents has
never been at the surface before, and it is not now possible to affirm that the supply from this source does not
offset, or even surpass, the depletion of the hydrosphere resulting from mineral hydration.
THE WORK OF GROUND-WATER.
Ground-water effects very considerable results in the course of its history. These results are partly chemical
and partly mechanical, the former being far more important than the latter.
Chemical Work.
The results of the chemical and chemico-physical action of water may be grouped in several more or less
distinct categories.
1. The simplest effect is the subtraction of soluble mineral matter. Pure water is in itself a solvent of certain
minerals; but the carbonic-acid gas extracted from the atmosphere, and the products of organic decay extracted
from the soil make ground-water a much more efficient solvent. Something of the results which it achieves is
shown by its composition. All ground-water, whether issuing as springs or drawn out through wells, contains
much more mineral matter than the water which falls as rain, and the excess is acquired in its underground
course.
The subtraction of soluble matter from rock renders it porous. The amount of material dissolved from a given
place may be trivial or considerable, according to the character of the rock, the readiness with which water has
access to it, and the character of the water. Locally, the subtraction of mineral matter may be the chief, or even
the only appreciable, effect of the ground-water.
2. It sometimes happens that ground-water with certain mineral substances in solution exchanges them for
other substances extracted from the rock. Thus the process of substitution is effected. By this process the lime
carbonate of a shell imbedded in rock may be removed, molecule by molecule, and some other substance, such
Page 275
as silica, left in its place. When the process is complete, the substance of the shell has been completely removed,
though its form and structure are still preserved in the new material which has taken the place of the old. Buried
logs are sometimes converted into stone by the substitution of mineral matter for the vegetable tissue. This is
petrification. Petrification is altogether distinct from incrustation, which simply means the coating of an object
with mineral matter. A bird’s nest may be incrusted with lime carbonate, but it is not thereby petrified. Solution
is a necessary antecedent of substitution.
3. The materials which are subtracted from the rock at one point may be added to other rock elsewhere. Thus
a third type of change, addition, is effected. Rock may at one time and place be rendered porous by the
subtraction of some of its substance, and the openings thus formed may subsequently become the receptacles of
deposits from solution. This is exemplified in the stalactitic deposits of many caves. Not uncommonly cracks
and fissures are filled with mineral matter deposited by the waters which pass through them. Thus arise veins
which, for the most part, are nothing more than cracks and crevices filled by mineral matter brought to them in
solution, and precipitated on their walls. Most veins of metallic ores have originated in this way.
4. A further series of changes is effected by ground-water when it, or the mineral matter it contains, enters into
combination with the mineral matter through which it passes. One of the commonest processes of this sort,
hydration, has already been referred to (pp. 43 and 428); but in the development of many of the commoner
hydrous minerals changes other than hydration are involved. These changes result in new mineral combinations,
the new minerals being developed out of the old, usually with some additions or subtractions. In the long course
of time changes of this sort may be very great, so great indeed that large bodies of rock are radically changed,
both chemically and physically. Much of the old substance may remain, but it has entered into new and more
stable combinations with the materials which the water has brought to it.
Quantitative importance of solution.—In general, solution is probably most effective at a relatively slight
distance below the surface. In the outermost zone of mantle rock the materials are usually less soluble than
below, for they often represent the residuum after the soluble parts of the formation from which they originated
were dissolved out. Below this zone the rock contains more soluble matter, and the water, charged with organic
matter in its descent through the soil, is in condition to dissolve it. At greater depths the water has become
saturated to some extent, and, so far forth, less active. Here, too, the movement is less free. The increased
pressure at considerable depths, on the other hand, facilitates solution, which must be understood to take place
under proper circumstances in any zone reached by the water.
Calculations have been made which illustrate the quantitative importance of the solution effected by ground-
water. The springs of Leuk (Switzerland) bring to the surface annually more than 2000 tons of calcium sulphate
(gypsum) in solution, and in the same time the springs of Bath (England) bring up an amount of mineral matter
in solution sufficient to make a column 9 feet in diameter, and 140 feet high.[100]
The amount of mineral matter in solution in streams is also significant, for while stream-water is not all
derived from ground-water, much of it had such an origin. In the case of several streams, among them the
Thames and the Elbe, careful estimates of the amount of dissolved mineral matter have been made. Though the
Thames drains an area only about one-tenth as large as the State of New York, it is estimated to carry about 1500
tons of mineral matter in solution to the sea daily.[101]
From the uppermost 20,000 square miles of its drainage basin the Elbe is estimated to carry yearly about
1,370,000 tons of mineral matter in solution. Estimates of the amounts of material carried to the sea in solution
by several rivers are given on pp. 102 and 103. Much of this matter was brought to the rivers by waters which
had been underground before reaching the streams.
From these figures it is clear that we have to reckon here with a very considerable factor in the lowering of
land surfaces. From the amount of lime carbonate carried by the Thames it has been estimated that the average
amount of this material dissolved from the limestone area drained by this stream is 143[102] tons per square mile
per year. It is estimated that, on the average, something like one-third as much matter is carried to the sea in
solution as in the form of sediment, and that by this process alone land areas would be lowered something like
one foot in 13,000 years.[103]
Deposition of mineral matter from solution.—The deposition of material from solution is effected in
several ways. (1) It is sometimes deposited by evaporation. This is well shown where water seeps out on arid
lands. The same process is illustrated when water is boiled. (2) Reduction of temperature often occasions
though its form and structure are still preserved in the new material which has taken the place of the old. Buried
logs are sometimes converted into stone by the substitution of mineral matter for the vegetable tissue. This is
petrification. Petrification is altogether distinct from incrustation, which simply means the coating of an object
with mineral matter. A bird’s nest may be incrusted with lime carbonate, but it is not thereby petrified. Solution
is a necessary antecedent of substitution.
3. The materials which are subtracted from the rock at one point may be added to other rock elsewhere. Thus
a third type of change, addition, is effected. Rock may at one time and place be rendered porous by the
subtraction of some of its substance, and the openings thus formed may subsequently become the receptacles of
deposits from solution. This is exemplified in the stalactitic deposits of many caves. Not uncommonly cracks
and fissures are filled with mineral matter deposited by the waters which pass through them. Thus arise veins
which, for the most part, are nothing more than cracks and crevices filled by mineral matter brought to them in
solution, and precipitated on their walls. Most veins of metallic ores have originated in this way.
4. A further series of changes is effected by ground-water when it, or the mineral matter it contains, enters into
combination with the mineral matter through which it passes. One of the commonest processes of this sort,
hydration, has already been referred to (pp. 43 and 428); but in the development of many of the commoner
hydrous minerals changes other than hydration are involved. These changes result in new mineral combinations,
the new minerals being developed out of the old, usually with some additions or subtractions. In the long course
of time changes of this sort may be very great, so great indeed that large bodies of rock are radically changed,
both chemically and physically. Much of the old substance may remain, but it has entered into new and more
stable combinations with the materials which the water has brought to it.
Quantitative importance of solution.—In general, solution is probably most effective at a relatively slight
distance below the surface. In the outermost zone of mantle rock the materials are usually less soluble than
below, for they often represent the residuum after the soluble parts of the formation from which they originated
were dissolved out. Below this zone the rock contains more soluble matter, and the water, charged with organic
matter in its descent through the soil, is in condition to dissolve it. At greater depths the water has become
saturated to some extent, and, so far forth, less active. Here, too, the movement is less free. The increased
pressure at considerable depths, on the other hand, facilitates solution, which must be understood to take place
under proper circumstances in any zone reached by the water.
Calculations have been made which illustrate the quantitative importance of the solution effected by ground-
water. The springs of Leuk (Switzerland) bring to the surface annually more than 2000 tons of calcium sulphate
(gypsum) in solution, and in the same time the springs of Bath (England) bring up an amount of mineral matter
in solution sufficient to make a column 9 feet in diameter, and 140 feet high.[100]
The amount of mineral matter in solution in streams is also significant, for while stream-water is not all
derived from ground-water, much of it had such an origin. In the case of several streams, among them the
Thames and the Elbe, careful estimates of the amount of dissolved mineral matter have been made. Though the
Thames drains an area only about one-tenth as large as the State of New York, it is estimated to carry about 1500
tons of mineral matter in solution to the sea daily.[101]
From the uppermost 20,000 square miles of its drainage basin the Elbe is estimated to carry yearly about
1,370,000 tons of mineral matter in solution. Estimates of the amounts of material carried to the sea in solution
by several rivers are given on pp. 102 and 103. Much of this matter was brought to the rivers by waters which
had been underground before reaching the streams.
From these figures it is clear that we have to reckon here with a very considerable factor in the lowering of
land surfaces. From the amount of lime carbonate carried by the Thames it has been estimated that the average
amount of this material dissolved from the limestone area drained by this stream is 143[102] tons per square mile
per year. It is estimated that, on the average, something like one-third as much matter is carried to the sea in
solution as in the form of sediment, and that by this process alone land areas would be lowered something like
one foot in 13,000 years.[103]
Deposition of mineral matter from solution.—The deposition of material from solution is effected in
several ways. (1) It is sometimes deposited by evaporation. This is well shown where water seeps out on arid
lands. The same process is illustrated when water is boiled. (2) Reduction of temperature often occasions
Page 276
deposition. In general, hot water is a better solvent of mineral matter than cold,[104] and if it issues with abundant
mineral matter in solution the precipitation of some of it is likely to take place. (3) Plants sometimes cause the
precipitation of mineral matter from solution. About some hot springs, even where the temperature of the water
is very high small plants of low type (algæ) grow in profusion. In ways which are not perfectly understood these
algæ extract the mineral matter from the hot water. They are now thought to be a chief factor in the deposits
about the hot springs of the Yellowstone Park.[105] The influence of organisms on precipitation from solution is
not confined to the waters of hot springs. (4) A fourth factor involved in the deposition of mineral matter from
solution is pressure. Pressure increases the solvent power of water with respect to minerals directly; it produces
the same effect indirectly by its effect on the solution of gases. As water charged with gas comes to the surface,
the pressure is relieved and some of the gas escapes. Such mineral matter as was held in solution by the help of
the gas which escapes is then precipitated. (5) Precipitation is also sometimes effected by the mingling of waters
containing different mineral substances in solution. Such mingling of solutions would be most common along
lines of ready subterranean flow, and while each portion of the water entering a crevice or porous bed may be
able to keep its own mineral matter in solution, their mingling may involve chemical changes resulting in the
formation of insoluble compounds, and therefore in deposition. This principle has probably been involved in the
filling of many fissures and crevices, converting them into veins. (6) The escape of gases from water, whether
from increase of temperature or by the disturbance of water, sometimes causes the deposition of mineral matter
held in solution.
The deposition of material held in solution is most notable at two zones, one below that of most active
solution, and the other at the surface, where evaporation is active. Under proper conditions, however, deposition
may take place at any level reached by water.
Mechanical Work.
The mechanical work of ground-water is relatively unimportant. Wherever it is organized into definite
streams, the channels through which it flows are likely to be increased by mechanical erosion as well as by
solution. Either beneath the surface, or after the streams issue, the mechanical sediment carried will be
deposited.
Fig. 202.—Diagram to illustrate the general form and relations of caves developed by solution. The black portions represent the cavern
spaces. Some limestone sinks are represented on the surface above.
RESULTS OF THE WORK OF GROUND-WATER.
Weathering.—Where the solution effected by ground-water in any locality is slight and equally distributed,
the result is to make the rock porous. If, for example, some of the cement of sandstone is dissolved, the texture
of the rock becomes more open; but if all the cement be removed the rock is changed from sandstone to sand. If
a complex crystalline rock contains among its many minerals some one which is more soluble than the others,
that one may be dissolved. This has the effect of breaking up the rock, since each mineral acts as a binder for the
rest. It might happen that no one of the minerals is dissolved completely, but that some one of them is
decomposed by water, and certain of its constituents removed. Such change would be likely to cause the mineral
so affected to crumble, and with its crumbling, if it be an important constituent of the rock, the integrity of the
mineral matter in solution the precipitation of some of it is likely to take place. (3) Plants sometimes cause the
precipitation of mineral matter from solution. About some hot springs, even where the temperature of the water
is very high small plants of low type (algæ) grow in profusion. In ways which are not perfectly understood these
algæ extract the mineral matter from the hot water. They are now thought to be a chief factor in the deposits
about the hot springs of the Yellowstone Park.[105] The influence of organisms on precipitation from solution is
not confined to the waters of hot springs. (4) A fourth factor involved in the deposition of mineral matter from
solution is pressure. Pressure increases the solvent power of water with respect to minerals directly; it produces
the same effect indirectly by its effect on the solution of gases. As water charged with gas comes to the surface,
the pressure is relieved and some of the gas escapes. Such mineral matter as was held in solution by the help of
the gas which escapes is then precipitated. (5) Precipitation is also sometimes effected by the mingling of waters
containing different mineral substances in solution. Such mingling of solutions would be most common along
lines of ready subterranean flow, and while each portion of the water entering a crevice or porous bed may be
able to keep its own mineral matter in solution, their mingling may involve chemical changes resulting in the
formation of insoluble compounds, and therefore in deposition. This principle has probably been involved in the
filling of many fissures and crevices, converting them into veins. (6) The escape of gases from water, whether
from increase of temperature or by the disturbance of water, sometimes causes the deposition of mineral matter
held in solution.
The deposition of material held in solution is most notable at two zones, one below that of most active
solution, and the other at the surface, where evaporation is active. Under proper conditions, however, deposition
may take place at any level reached by water.
Mechanical Work.
The mechanical work of ground-water is relatively unimportant. Wherever it is organized into definite
streams, the channels through which it flows are likely to be increased by mechanical erosion as well as by
solution. Either beneath the surface, or after the streams issue, the mechanical sediment carried will be
deposited.
Fig. 202.—Diagram to illustrate the general form and relations of caves developed by solution. The black portions represent the cavern
spaces. Some limestone sinks are represented on the surface above.
RESULTS OF THE WORK OF GROUND-WATER.
Weathering.—Where the solution effected by ground-water in any locality is slight and equally distributed,
the result is to make the rock porous. If, for example, some of the cement of sandstone is dissolved, the texture
of the rock becomes more open; but if all the cement be removed the rock is changed from sandstone to sand. If
a complex crystalline rock contains among its many minerals some one which is more soluble than the others,
that one may be dissolved. This has the effect of breaking up the rock, since each mineral acts as a binder for the
rest. It might happen that no one of the minerals is dissolved completely, but that some one of them is
decomposed by water, and certain of its constituents removed. Such change would be likely to cause the mineral
so affected to crumble, and with its crumbling, if it be an important constituent of the rock, the integrity of the
Page 277
rock is destroyed. Where considerable chemical changes, especially
subtractions, are going on, the rock is likely to crumble. The increase in
volume attendant on hydration, etc., sometimes leads to the disruption of
rock. These are phases of weathering. (For other phases of weathering see pp.
54 and 110.)
Caverns.[106]—Where local solution is very great results of another sort
may be effected. In formations like limestone, which are relatively soluble,
considerable quantities of material are frequently dissolved from a given
place. Instead of making the rock porous, in the usual sense of the term, large
caverns may be developed (Fig. 202). In their production, solution may be
abetted by the mechanical action of the water passing through the openings
which solution has developed. Considerable caves are found chiefly in
limestone. They were probably developed when the surface relief was slight,
and surface drainage therefore poor. Regions where caves were developed
under these conditions may subsequently acquire relief, so that caves are not
now confined to flat regions.
One of the best known regions of caves is in the basin of the Ohio in
Kentucky and southern Indiana, where the number of caves is large, and the
size of some of them, such as Mammoth and Wyandotte, very great. A
ground-plan of Wyandotte (Ind.) Cave is shown in Fig. 203. The aggregate
length of the passageways is about 23½ miles.
Fig. 203.—Ground-plan of Wyandotte
Cave. The unshaded areas represent
the passageways. (21st Ann. Rept.,
Ind. Geol. Surv.)
subtractions, are going on, the rock is likely to crumble. The increase in
volume attendant on hydration, etc., sometimes leads to the disruption of
rock. These are phases of weathering. (For other phases of weathering see pp.
54 and 110.)
Caverns.[106]—Where local solution is very great results of another sort
may be effected. In formations like limestone, which are relatively soluble,
considerable quantities of material are frequently dissolved from a given
place. Instead of making the rock porous, in the usual sense of the term, large
caverns may be developed (Fig. 202). In their production, solution may be
abetted by the mechanical action of the water passing through the openings
which solution has developed. Considerable caves are found chiefly in
limestone. They were probably developed when the surface relief was slight,
and surface drainage therefore poor. Regions where caves were developed
under these conditions may subsequently acquire relief, so that caves are not
now confined to flat regions.
One of the best known regions of caves is in the basin of the Ohio in
Kentucky and southern Indiana, where the number of caves is large, and the
size of some of them, such as Mammoth and Wyandotte, very great. A
ground-plan of Wyandotte (Ind.) Cave is shown in Fig. 203. The aggregate
length of the passageways is about 23½ miles.
Fig. 203.—Ground-plan of Wyandotte
Cave. The unshaded areas represent
the passageways. (21st Ann. Rept.,
Ind. Geol. Surv.)
Page 278
Fig. 204.—Deposits in Wyandotte (Ind.) Cave. (Hains.)
Fig. 205.—Deposits in Wyandotte Cave. (Hains.)
Fig. 205.—Deposits in Wyandotte Cave. (Hains.)
Page 279
Deposition often takes place in caves after they are formed (Figs. 204 and 205). It may even go on at the same
time that the cave is being excavated. Here are formed the well-known stalactites and stalagmites. A stalactite
may start from a drop of water leaking through the roof of the cave. Evaporation, or the escape of some of the
carbonic gas in solution, results in the deposition of some of the lime carbonate about the margin of the drop, in
the form of a ring. Successive drops make successive deposits on the lower edge of the ring, which grows
downward into a hollow tube through which descending water passes, making its chief deposits at the end.
Deposition in the tube may ultimately close it, while deposition on the outside, due to water trickling down in
that position, may greatly enlarge it.
Fig. 206.—A limestone sink-hole, east-northeast of Cambria, Wyo., exceptional for its steep sides. Minnekahta limestone. (Darton, U. S.
Geol. Surv.)
Underground caves sometimes give rise to topographic features which are of local importance. When the
solution of material in a cavern has gone so far that its roof becomes thin and weak, it may collapse, giving rise
to a sink or depression in the surface over the site of the original cave. This is so common that regions of
limestone caves are often affected by frequent sinks formed in this way. They are a conspicuous feature of the
landscape in the cave region of Kentucky, and are well known in many other limestone districts. They are known
as limestone sinks. (Fig. 206 and Fig. 2, Pl. XVII.)
time that the cave is being excavated. Here are formed the well-known stalactites and stalagmites. A stalactite
may start from a drop of water leaking through the roof of the cave. Evaporation, or the escape of some of the
carbonic gas in solution, results in the deposition of some of the lime carbonate about the margin of the drop, in
the form of a ring. Successive drops make successive deposits on the lower edge of the ring, which grows
downward into a hollow tube through which descending water passes, making its chief deposits at the end.
Deposition in the tube may ultimately close it, while deposition on the outside, due to water trickling down in
that position, may greatly enlarge it.
Fig. 206.—A limestone sink-hole, east-northeast of Cambria, Wyo., exceptional for its steep sides. Minnekahta limestone. (Darton, U. S.
Geol. Surv.)
Underground caves sometimes give rise to topographic features which are of local importance. When the
solution of material in a cavern has gone so far that its roof becomes thin and weak, it may collapse, giving rise
to a sink or depression in the surface over the site of the original cave. This is so common that regions of
limestone caves are often affected by frequent sinks formed in this way. They are a conspicuous feature of the
landscape in the cave region of Kentucky, and are well known in many other limestone districts. They are known
as limestone sinks. (Fig. 206 and Fig. 2, Pl. XVII.)
Page 280
Fig. 207.—A fresh landslide near Medicine Lake, Mont. The bare space shows the position from which the slide started. (Whitney.)
Fig. 208.—Landslide topography. The protruding mass on the right has slumped down from the mountain to the left. South face of
Landslip Mountain, Colo., seen from the west; Rico quadrangle. (Cross, U. S. Geol. Surv.)
Fig. 208.—Landslide topography. The protruding mass on the right has slumped down from the mountain to the left. South face of
Landslip Mountain, Colo., seen from the west; Rico quadrangle. (Cross, U. S. Geol. Surv.)
Page 281
Under certain circumstances caves may give rise to striking features of another sort. If for any reason the roof
is destroyed at the two ends of a cave, remaining intact over the middle, the latter part constitutes a natural
bridge. Natural bridges also originate in other ways (pp. 151, 153).
Fig. 209.—Landslide topography on Badger Mountain, Washington. The slumping material in this case is basalt.
Creep, slumps, and landslides.—When the soil and subsoil on a slope become charged with water they tend
to move downward. When the movement is too slow to be sensible it is called creep. The common downward
inclination of trees growing in such situations, the result of the more rapid creep of the surface as compared with
the deeper part of the soil, is both an expression of the movement and of its slowness. Other factors besides
ground-water are involved in creep (see p. 112).
When the movement is rapid enough to be sensible the material is said to slump or slide. This may happen
when the slope on which water-charged mantle rock lies is steep (Fig. 207). Great landslides of this sort have
been recorded, and some of them have done great damage. Where a stream’s banks are high, and of unindurated
material, such as clay, considerable masses sometimes slump from the bank or bluff into the river, or settle away
slowly from their former positions. This is a common phenomenon along streams which have cut valleys in
drift, and along shores on which waves are encroaching. The same phenomenon is common on a larger scale on
the slopes of steep mountains.[107] Considerable terraces are sometimes developed on their slopes in this way, but
they are usually irregular and discontinuous (Figs. 208, and 209). The loose débris on steep slopes sometimes
assumes a sort of flowing motion and descends the slope with some such form and at some such rate as a glacier.
Such bodies of débris are sometimes called “talus glaciers” (Fig. 210). In many such cases, snow and ice have
had some part in their development.
In creep and in landslides gravity is the force involved, and the ground-water only a condition which makes
gravity effective. Gravity alone accomplishes similar results, as illustrated by Fig. 211.
Summary.
All in all, ground-water is to be looked upon as a most important geological agent. When it is remembered
that a very large part of all the water which falls on the surface of the earth, either in the form of rain or snow,
sinks beneath the surface; that much of it sinks to a great depth; that much of it has a long underground course
before it reappears at the surface; that it is everywhere and always active, either in subtracting from the rock
through which it passes, in adding to it, in effecting the substitution of one mineral substance for another, or in
is destroyed at the two ends of a cave, remaining intact over the middle, the latter part constitutes a natural
bridge. Natural bridges also originate in other ways (pp. 151, 153).
Fig. 209.—Landslide topography on Badger Mountain, Washington. The slumping material in this case is basalt.
Creep, slumps, and landslides.—When the soil and subsoil on a slope become charged with water they tend
to move downward. When the movement is too slow to be sensible it is called creep. The common downward
inclination of trees growing in such situations, the result of the more rapid creep of the surface as compared with
the deeper part of the soil, is both an expression of the movement and of its slowness. Other factors besides
ground-water are involved in creep (see p. 112).
When the movement is rapid enough to be sensible the material is said to slump or slide. This may happen
when the slope on which water-charged mantle rock lies is steep (Fig. 207). Great landslides of this sort have
been recorded, and some of them have done great damage. Where a stream’s banks are high, and of unindurated
material, such as clay, considerable masses sometimes slump from the bank or bluff into the river, or settle away
slowly from their former positions. This is a common phenomenon along streams which have cut valleys in
drift, and along shores on which waves are encroaching. The same phenomenon is common on a larger scale on
the slopes of steep mountains.[107] Considerable terraces are sometimes developed on their slopes in this way, but
they are usually irregular and discontinuous (Figs. 208, and 209). The loose débris on steep slopes sometimes
assumes a sort of flowing motion and descends the slope with some such form and at some such rate as a glacier.
Such bodies of débris are sometimes called “talus glaciers” (Fig. 210). In many such cases, snow and ice have
had some part in their development.
In creep and in landslides gravity is the force involved, and the ground-water only a condition which makes
gravity effective. Gravity alone accomplishes similar results, as illustrated by Fig. 211.
Summary.
All in all, ground-water is to be looked upon as a most important geological agent. When it is remembered
that a very large part of all the water which falls on the surface of the earth, either in the form of rain or snow,
sinks beneath the surface; that much of it sinks to a great depth; that much of it has a long underground course
before it reappears at the surface; that it is everywhere and always active, either in subtracting from the rock
through which it passes, in adding to it, in effecting the substitution of one mineral substance for another, or in
Page 282
bringing about new chemical combinations; and when it is remembered that this process has been going on for
untold millions of years, it will be seen that the total result accomplished must be stupendous. The rock
formations of the earth to the depths to which ground-water penetrates are to be looked upon as a sort of
chemical laboratory through which waters are circulating in all directions, charged with all sorts of mineral
substances. Some of the substances in solution are deposited beneath the surface, and some are brought to the
surface where the waters issue. Much of the material brought to the surface in solution is carried to the sea and
utilized by marine organisms in the making of shells. Without the mineral matter brought to the sea by springs
and rivers, many shell-bearing animals of great importance, geologically, would perish. Biologically, therefore,
as well as geologically, ground-water is of great importance.
PLATE XVII.
U. S. Geol. Surv. Fig. 1. HUNTERDON COUNTY, NEW JERSEY. Scale, 1+ miles per inch.
untold millions of years, it will be seen that the total result accomplished must be stupendous. The rock
formations of the earth to the depths to which ground-water penetrates are to be looked upon as a sort of
chemical laboratory through which waters are circulating in all directions, charged with all sorts of mineral
substances. Some of the substances in solution are deposited beneath the surface, and some are brought to the
surface where the waters issue. Much of the material brought to the surface in solution is carried to the sea and
utilized by marine organisms in the making of shells. Without the mineral matter brought to the sea by springs
and rivers, many shell-bearing animals of great importance, geologically, would perish. Biologically, therefore,
as well as geologically, ground-water is of great importance.
PLATE XVII.
U. S. Geol. Surv. Fig. 1. HUNTERDON COUNTY, NEW JERSEY. Scale, 1+ miles per inch.
Page 283
U. S. Geol. Surv. Fig. 2. NEAR PIKEVILLE, TENNESSEE. Scale, 1+ miles per inch.
Page 284
PLATE XVIII.
U. S. Geol. Surv. Fig. 1. WASHINGTON. Scale, 2+ miles per inch.
U. S. Geol. Surv. Fig. 1. WASHINGTON. Scale, 2+ miles per inch.
Page 285
U. S. Geol. Surv. Fig. 2. CALIFORNIA. Scale, 2+ miles per inch.
Page 286
Fig. 210.—A “talus glacier,” in Silver Basin, near Silverton, Colo. (Cross, U. S. Geol. Surv.)
Fig. 211.—A huge mass of rock settling into the Canyon of the Colorado. A result of gravity action. (Atwood.)
SPRINGS AND FLOWING WELLS.
Fig. 211.—A huge mass of rock settling into the Canyon of the Colorado. A result of gravity action. (Atwood.)
SPRINGS AND FLOWING WELLS.
Page 287
The term spring is applied to any water which issues from beneath the surface with sufficient volume to cause
a distinct current. If the water issues so slowly as to merely keep the surface moist, it is not called a spring, but
seepage. The spring from which water issues with a strong current, especially if it be upward, is comparable to a
flowing well, while the spring from which water issues with little force, and without upward movement, is
comparable to the flow of water into a common well.
Springs often issue from the sides of valleys (Fig. 212), the bottoms of which are below ground-water level.
They are especially likely to issue at the surface of relatively impervious layers, and where the valley slopes cut
joints, porous beds, or other structures which allow free flow of ground-water.
Fig. 212.—Diagram illustrating positions, a and b, favorable for springs.
Springs are classified in various ways, and these several classifications suggest characteristics worthy of note.
They are sometimes said to be deep and shallow. The “deep” spring, as the term is ordinarily used, is one which
issues with great force, and with something of upward movement, and the “shallow” spring, one which issues
with little force, and without upward movement; but the spring which issues with force is not necessarily deep,
nor is the one which issues with little force necessarily shallow. The idea involved in this grouping would be
better expressed by strong and feeble. Springs are also classified as cold and thermal, the latter term meaning
simply that the temperature is such as to make the springs seem warm or hot. The temperature of thermal springs
ranges up to the boiling-point of water. Between deep springs and shallow ones, and between cold springs and
thermal, respectively, there is no sharp line of demarkation. Again, some springs are continuous in their flow,
while others are intermittent. Most intermittent springs flow after periods of precipitation, but dry up during
droughts (see p. 202). Springs are also classified as mineral and common. Mineral springs, in the popular sense
of the term, are of two types: (1) Those which contain an unusual amount of mineral matter, and (2) those which
contain some unusual mineral. Springs are especially likely to be called mineral if the substances which they
contain, have, or are supposed to have, some medicinal property. All springs which are not “mineral” are
“common.” This classification is not altogether rational, for all springs contain more or less mineral matter, and
many springs which are “common,” contain more mineral matter than some springs that are “mineral.” Mineral
springs are themselves classified according to the kind and amount of mineral matter they contain. Thus saline
springs contain salt; sulphur springs contain compounds (especially gaseous) of sulphur; chalybeate springs
contain iron compounds, especially the sulphate; calcareous springs contain abundant lime carbonate, etc. These
various mineral substances are extracted from the rock, sometimes by simple solution, and sometimes by
solution resulting from other chemical change. The salt of saline springs is usually extracted from beds of salt
beneath the surface. Lime carbonate, one of the commonest substances in solution in ground-water, is dissolved
from limestone, or derived by chemical change from rocks containing other calcium compounds. Thus lime
feldspars, by carbonation, give rise to lime carbonate. The chalybeate waters often arise from the oxidation of
iron sulphide, a mineral which is common in many sedimentary rocks. The iron sulphate is itself subject to
change in the presence of the ubiquitous lime carbonate. From this change iron carbonate results, and this is
usually quickly altered to iron oxide, which, being relatively insoluble, is precipitated. About chalybeate springs,
therefore, iron oxide is frequently being deposited. Medicinal springs are those which contain some substance or
substances which have, or are supposed to have, curative properties.
Mineral matter in solution.—The number and variety of mineral substances in spring water is very great,
and the amount of solid matter in solution varies widely. Some of the hot springs of the Yellowstone Park
contain nearly three grams (2.8733) of mineral matter per kilogram.[108]
The composition of various spring and well waters is shown in the accompanying table, which gives some
idea of the range of mineral substances commonly in solution in ground-water.
a distinct current. If the water issues so slowly as to merely keep the surface moist, it is not called a spring, but
seepage. The spring from which water issues with a strong current, especially if it be upward, is comparable to a
flowing well, while the spring from which water issues with little force, and without upward movement, is
comparable to the flow of water into a common well.
Springs often issue from the sides of valleys (Fig. 212), the bottoms of which are below ground-water level.
They are especially likely to issue at the surface of relatively impervious layers, and where the valley slopes cut
joints, porous beds, or other structures which allow free flow of ground-water.
Fig. 212.—Diagram illustrating positions, a and b, favorable for springs.
Springs are classified in various ways, and these several classifications suggest characteristics worthy of note.
They are sometimes said to be deep and shallow. The “deep” spring, as the term is ordinarily used, is one which
issues with great force, and with something of upward movement, and the “shallow” spring, one which issues
with little force, and without upward movement; but the spring which issues with force is not necessarily deep,
nor is the one which issues with little force necessarily shallow. The idea involved in this grouping would be
better expressed by strong and feeble. Springs are also classified as cold and thermal, the latter term meaning
simply that the temperature is such as to make the springs seem warm or hot. The temperature of thermal springs
ranges up to the boiling-point of water. Between deep springs and shallow ones, and between cold springs and
thermal, respectively, there is no sharp line of demarkation. Again, some springs are continuous in their flow,
while others are intermittent. Most intermittent springs flow after periods of precipitation, but dry up during
droughts (see p. 202). Springs are also classified as mineral and common. Mineral springs, in the popular sense
of the term, are of two types: (1) Those which contain an unusual amount of mineral matter, and (2) those which
contain some unusual mineral. Springs are especially likely to be called mineral if the substances which they
contain, have, or are supposed to have, some medicinal property. All springs which are not “mineral” are
“common.” This classification is not altogether rational, for all springs contain more or less mineral matter, and
many springs which are “common,” contain more mineral matter than some springs that are “mineral.” Mineral
springs are themselves classified according to the kind and amount of mineral matter they contain. Thus saline
springs contain salt; sulphur springs contain compounds (especially gaseous) of sulphur; chalybeate springs
contain iron compounds, especially the sulphate; calcareous springs contain abundant lime carbonate, etc. These
various mineral substances are extracted from the rock, sometimes by simple solution, and sometimes by
solution resulting from other chemical change. The salt of saline springs is usually extracted from beds of salt
beneath the surface. Lime carbonate, one of the commonest substances in solution in ground-water, is dissolved
from limestone, or derived by chemical change from rocks containing other calcium compounds. Thus lime
feldspars, by carbonation, give rise to lime carbonate. The chalybeate waters often arise from the oxidation of
iron sulphide, a mineral which is common in many sedimentary rocks. The iron sulphate is itself subject to
change in the presence of the ubiquitous lime carbonate. From this change iron carbonate results, and this is
usually quickly altered to iron oxide, which, being relatively insoluble, is precipitated. About chalybeate springs,
therefore, iron oxide is frequently being deposited. Medicinal springs are those which contain some substance or
substances which have, or are supposed to have, curative properties.
Mineral matter in solution.—The number and variety of mineral substances in spring water is very great,
and the amount of solid matter in solution varies widely. Some of the hot springs of the Yellowstone Park
contain nearly three grams (2.8733) of mineral matter per kilogram.[108]
The composition of various spring and well waters is shown in the accompanying table, which gives some
idea of the range of mineral substances commonly in solution in ground-water.
Page 288
Geysers.—Geysers are intermittently eruptive hot springs. They occur only in volcanic regions (past or
present) and in but few of them. Active geysers are virtually confined to the Yellowstone Park and Iceland,
though they formerly existed at other places. Those of New Zealand have but recently become extinct. The great
geyser region of the world is the Yellowstone Park, where there are said to be more than sixty active geysers.
The cause of the eruption is steam. The surface-water sinks down until, at some unknown depth, it comes into
contact with rock sufficiently hot to boil it. The source of the heat is not open to inspection, but it is believed to
be the uncooled part of an extrusive lava flow, or of an intrusive lava mass. From what was said on pp. 216 and
217 it is clear that geysers do not have their origin in water which sinks down to the zone of great heat, where
the increment of heat is normal.
The water of a geyser issues through a tube of unknown length. Whether the tube is open down to the source
of the heat is not determinable, but water from such a source finds its way to the tube. Water may enter the tube
from all sides and at various levels from top to bottom. The heating may precede or follow its entrance into the
tube, or both. So far as the water is heated after it enters the tube, the point of most rapid heating may be at the
bottom of the tube or at some point above. If the temperature of the source of heat were high enough to convert
the descending water into steam as fast as it enters the tube, the steam would escape continuously, though there
would be no geyser; but if the rock is only hot enough to bring the water to the boiling-point after some lapse of
time, and after some water has accumulated, an eruption is possible.
ANALYSES OF AMERICAN SPRING-WATERS.[109]
[Reduced to Parts per 1000 by Dr H. J. Van Hoesen.]
Waters Artesian Artesian Artesian Manitou Opal Spring Sulphur Spring Hot Hot Boiling Warm
well well well[110] Spring Spring Spring Spring Spring
“Glacier
Spouting
Spring”
Location Lexington, Saratoga, Sheboygan, Manitou, Col. Yellowstone Los Angeles, Hot Sp. Ward’s Shaffer’s Warm
Ky. N. Y. Wis. National Cal. Station, Ranch, Ranch, Spring
Park C. P. R. base of Honey Sta. B.
R. Granite Lake & B. R.
Mts., Valley, Mono
Nev. Cal. Basin
Date ...... 1872 Feb. 1876 ...... ...... ...... ...... ...... ...... ......
Analyst R. Peters F. A. C. F. Oscar Loew H. Leffman Oscar Loew T. M. T. M. T. M. T. M.
Cairns Chandler Chatard Chatard Chatard Chatard
and C. F.
Chandler
References Ky. Geol. Am. Am. U. S. G. S. W., U. S. Geol. An. Rep. Ante, p. Ante, p. Ante, p. Bulletin
Surv., N. Chemist, Chemist, 100th M.. & Geog. U. S. G. S. W., 49 53 51 No. 9,
S., Vol. Nov. 1876, p. Vol. III, p. Surv. Id., 100th M., U. S.
V, p. 189 1872, p. 370 618 Wyo. 1876, p. 195 Geol.
164 Ter., Survey,
1878, p. p. 27
393
Sodium, Na .09227 4.72640 2.0398 .45164 .4615 .10424 .7743 .3554 .3040 .6116
Potassium,
.00919 .35806 .1285 .05980 ...... Trace .0669 .0191 .0094 .0630
K
Calcium, Ca .02136 .94050 1.0739 .44400 .0344 .0305 .0367 .0121 .0589
Magnesium, .50600[111]
.01805 .53470 .2352 .05860 ...... .0010 .0034 .0004 .0604
Mg
Barium, Ba ...... .01848 Trace
Strontium,
Sr Trace[112] .00057
Lithium, Li Trace .01078 .0003 .00039 ...... Trace
Iron, Fe Trace[113] .00341 .0027 Trace[114] ...... Trace
Manganese,
...... ...... .0009 ...... ...... Trace
Mn
Chlorine, Cl .07465 7.47400 4.2730 .24850 .7496 Trace[115] .9697 .2396 .2070 .2272
Bromine, Br .04661 .0025
Iodine, I .00060 Trace
Fluorine, Fl ...... Trace[116]
Carbonic
acid, CO2 .12160 5.82603 .1792 1.11001 ...... .03516 ...... Trace ...... .5787
present) and in but few of them. Active geysers are virtually confined to the Yellowstone Park and Iceland,
though they formerly existed at other places. Those of New Zealand have but recently become extinct. The great
geyser region of the world is the Yellowstone Park, where there are said to be more than sixty active geysers.
The cause of the eruption is steam. The surface-water sinks down until, at some unknown depth, it comes into
contact with rock sufficiently hot to boil it. The source of the heat is not open to inspection, but it is believed to
be the uncooled part of an extrusive lava flow, or of an intrusive lava mass. From what was said on pp. 216 and
217 it is clear that geysers do not have their origin in water which sinks down to the zone of great heat, where
the increment of heat is normal.
The water of a geyser issues through a tube of unknown length. Whether the tube is open down to the source
of the heat is not determinable, but water from such a source finds its way to the tube. Water may enter the tube
from all sides and at various levels from top to bottom. The heating may precede or follow its entrance into the
tube, or both. So far as the water is heated after it enters the tube, the point of most rapid heating may be at the
bottom of the tube or at some point above. If the temperature of the source of heat were high enough to convert
the descending water into steam as fast as it enters the tube, the steam would escape continuously, though there
would be no geyser; but if the rock is only hot enough to bring the water to the boiling-point after some lapse of
time, and after some water has accumulated, an eruption is possible.
ANALYSES OF AMERICAN SPRING-WATERS.[109]
[Reduced to Parts per 1000 by Dr H. J. Van Hoesen.]
Waters Artesian Artesian Artesian Manitou Opal Spring Sulphur Spring Hot Hot Boiling Warm
well well well[110] Spring Spring Spring Spring Spring
“Glacier
Spouting
Spring”
Location Lexington, Saratoga, Sheboygan, Manitou, Col. Yellowstone Los Angeles, Hot Sp. Ward’s Shaffer’s Warm
Ky. N. Y. Wis. National Cal. Station, Ranch, Ranch, Spring
Park C. P. R. base of Honey Sta. B.
R. Granite Lake & B. R.
Mts., Valley, Mono
Nev. Cal. Basin
Date ...... 1872 Feb. 1876 ...... ...... ...... ...... ...... ...... ......
Analyst R. Peters F. A. C. F. Oscar Loew H. Leffman Oscar Loew T. M. T. M. T. M. T. M.
Cairns Chandler Chatard Chatard Chatard Chatard
and C. F.
Chandler
References Ky. Geol. Am. Am. U. S. G. S. W., U. S. Geol. An. Rep. Ante, p. Ante, p. Ante, p. Bulletin
Surv., N. Chemist, Chemist, 100th M.. & Geog. U. S. G. S. W., 49 53 51 No. 9,
S., Vol. Nov. 1876, p. Vol. III, p. Surv. Id., 100th M., U. S.
V, p. 189 1872, p. 370 618 Wyo. 1876, p. 195 Geol.
164 Ter., Survey,
1878, p. p. 27
393
Sodium, Na .09227 4.72640 2.0398 .45164 .4615 .10424 .7743 .3554 .3040 .6116
Potassium,
.00919 .35806 .1285 .05980 ...... Trace .0669 .0191 .0094 .0630
K
Calcium, Ca .02136 .94050 1.0739 .44400 .0344 .0305 .0367 .0121 .0589
Magnesium, .50600[111]
.01805 .53470 .2352 .05860 ...... .0010 .0034 .0004 .0604
Mg
Barium, Ba ...... .01848 Trace
Strontium,
Sr Trace[112] .00057
Lithium, Li Trace .01078 .0003 .00039 ...... Trace
Iron, Fe Trace[113] .00341 .0027 Trace[114] ...... Trace
Manganese,
...... ...... .0009 ...... ...... Trace
Mn
Chlorine, Cl .07465 7.47400 4.2730 .24850 .7496 Trace[115] .9697 .2396 .2070 .2272
Bromine, Br .04661 .0025
Iodine, I .00060 Trace
Fluorine, Fl ...... Trace[116]
Carbonic
acid, CO2 .12160 5.82603 .1792 1.11001 ...... .03516 ...... Trace ...... .5787
Page 289
Sulphuric
acid, H2SO4 .03218 .00234 2.0318 .20696 .0325 .16140 .3555 .3901 .3492 .3131
Phosphoric
acid, H3PO4 Trace .00005 .0004 ...... ...... Trace
Boracic acid,
H3BO3 Trace Trace
Alumina,
Al2O3 ...... .00770 .0022 ...... ...... Trace .0010 ...... ...... .0018
Silica, SiO2 .00940 .01174 .0080 .02010 .7680 Trace .2788 .1136 .1310 .1220
Hydrogen in
bicarbonates, ...... .09713 .0030
H
Organic
Trace Trace Trace ...... ...... Trace
substances
Oxygen, O ...... ...... ...... ...... ...... ...... .0194[117] .0255[117] .0080[117] .0325[117]
.37870 20.05910 9.9814 2.60000 2.0460 .80680 2.4953 1.1834 1.0211 2.0692
Carbonic
acid, CO2 ...... 2.015[118] ...... ...... ...... In excess Trace
Sulphuretted
hydrogen, ...... ...... ...... ...... ...... 0.5000
H2S
The exact sequence of events which leads up to an
eruption is not known, but a definite conception of the
principles involved may perhaps be secured by a definite
case. Suppose a geyser-tube filled with water, and heated at
its lower end. As the water is heated below, convection
tends to distribute the heat throughout the column of water
above. If convection were free, and the tube short, the result
would be a boiling spring; but if the tube is long, and
especially if convection is impeded, the water at some level
below the surface may be brought to the boiling-point
earlier than that at the top. Under these circumstances if
even a little water in the lower part of the tube is converted
into steam, the steam will raise the column of water above,
and it will overflow. The overflow relieves the pressure on
all parts of the column of water below the surface. If before
the overflow there was any considerable volume of water
essentially ready to boil, the relief of pressure following the
overflow might allow it to be converted into steam
suddenly, and the sudden conversion of any considerable
quantity of water into steam would cause the eruption of all
the water above it (Figs. 213 and 214). The height to which
the water would be thrown would depend upon the amount
of steam, the size and straightness of the tube, etc.
It is clear that everything which impedes convection in
the geyser tube will hasten the period of eruption, since
impeded circulation will have the effect of holding the heat
down, and so of bringing the water at some level below the
top more quickly to the boiling-point. It follows that
anything which chokes up the tube, or which increases the
viscosity of the water, or its surface tension, would hasten
an eruption.[119] Fig. 213.—“Old Faithful” in eruption.
Geysers often build up crater-like basins or cones (Figs. 214 to 217) about themselves, the cone being of
material deposited from solution. In the Yellowstone Park the precipitation of the matter in solution (chiefly
silica) is partly due to cooling and partly to the algæ which abound even in the boiling water, and the brilliant
colors of the deposits about the springs are attributable to these plants. When the water from any geyser or hot
acid, H2SO4 .03218 .00234 2.0318 .20696 .0325 .16140 .3555 .3901 .3492 .3131
Phosphoric
acid, H3PO4 Trace .00005 .0004 ...... ...... Trace
Boracic acid,
H3BO3 Trace Trace
Alumina,
Al2O3 ...... .00770 .0022 ...... ...... Trace .0010 ...... ...... .0018
Silica, SiO2 .00940 .01174 .0080 .02010 .7680 Trace .2788 .1136 .1310 .1220
Hydrogen in
bicarbonates, ...... .09713 .0030
H
Organic
Trace Trace Trace ...... ...... Trace
substances
Oxygen, O ...... ...... ...... ...... ...... ...... .0194[117] .0255[117] .0080[117] .0325[117]
.37870 20.05910 9.9814 2.60000 2.0460 .80680 2.4953 1.1834 1.0211 2.0692
Carbonic
acid, CO2 ...... 2.015[118] ...... ...... ...... In excess Trace
Sulphuretted
hydrogen, ...... ...... ...... ...... ...... 0.5000
H2S
The exact sequence of events which leads up to an
eruption is not known, but a definite conception of the
principles involved may perhaps be secured by a definite
case. Suppose a geyser-tube filled with water, and heated at
its lower end. As the water is heated below, convection
tends to distribute the heat throughout the column of water
above. If convection were free, and the tube short, the result
would be a boiling spring; but if the tube is long, and
especially if convection is impeded, the water at some level
below the surface may be brought to the boiling-point
earlier than that at the top. Under these circumstances if
even a little water in the lower part of the tube is converted
into steam, the steam will raise the column of water above,
and it will overflow. The overflow relieves the pressure on
all parts of the column of water below the surface. If before
the overflow there was any considerable volume of water
essentially ready to boil, the relief of pressure following the
overflow might allow it to be converted into steam
suddenly, and the sudden conversion of any considerable
quantity of water into steam would cause the eruption of all
the water above it (Figs. 213 and 214). The height to which
the water would be thrown would depend upon the amount
of steam, the size and straightness of the tube, etc.
It is clear that everything which impedes convection in
the geyser tube will hasten the period of eruption, since
impeded circulation will have the effect of holding the heat
down, and so of bringing the water at some level below the
top more quickly to the boiling-point. It follows that
anything which chokes up the tube, or which increases the
viscosity of the water, or its surface tension, would hasten
an eruption.[119] Fig. 213.—“Old Faithful” in eruption.
Geysers often build up crater-like basins or cones (Figs. 214 to 217) about themselves, the cone being of
material deposited from solution. In the Yellowstone Park the precipitation of the matter in solution (chiefly
silica) is partly due to cooling and partly to the algæ which abound even in the boiling water, and the brilliant
colors of the deposits about the springs are attributable to these plants. When the water from any geyser or hot
Page 290
spring ceases to flow the plants die and the colors disappear. The details of the surface of the deposits about
geysers and hot springs are often complicated, and frequently very beautiful (Fig. 218).
Fig. 214.—“Giant” Geyser, Yellowstone Park, in eruption. Shows also the cone. (Wineman.)
geysers and hot springs are often complicated, and frequently very beautiful (Fig. 218).
Fig. 214.—“Giant” Geyser, Yellowstone Park, in eruption. Shows also the cone. (Wineman.)
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Fig. 215.—Cone (or crater) of Castle Geyser, Yellowstone Park. (Detroit Photo. Co.)
Fig. 216.—Cone (or crater) of Grotto Geyser, Yellowstone Park. (Detroit Photo. Co.)
The heating of geyser and hot-spring water must cool the lava or other source of heat below. As this takes
place, the time between eruptions becomes longer and longer. In the course of time, therefore, the geyser must
cease to be eruptive, and when this change is brought about the geyser becomes a hot spring. Within historic
times several geysers have ceased to erupt and new ones have been developed. In the Yellowstone Park, where
Fig. 216.—Cone (or crater) of Grotto Geyser, Yellowstone Park. (Detroit Photo. Co.)
The heating of geyser and hot-spring water must cool the lava or other source of heat below. As this takes
place, the time between eruptions becomes longer and longer. In the course of time, therefore, the geyser must
cease to be eruptive, and when this change is brought about the geyser becomes a hot spring. Within historic
times several geysers have ceased to erupt and new ones have been developed. In the Yellowstone Park, where
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there are said to be something like 3000 vents of all sorts,
hot springs which are not eruptive greatly outnumber the
geysers. From many of the vents but little steam issues, and
from some, little else.
Fig. 217.—Cone of Giant Geyser, Yellowstone Park.
(Wineman.)
hot springs which are not eruptive greatly outnumber the
geysers. From many of the vents but little steam issues, and
from some, little else.
Fig. 217.—Cone of Giant Geyser, Yellowstone Park.
(Wineman.)
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Fig. 218.—Hot springs deposits. Terraces of Mammoth Hot Springs, Yellowstone Park.
A few geysers have somewhat definite periods of eruption. Of such “Old Faithful” is the type; but even this
geyser, which formerly erupted at regular intervals of about an hour, is losing the reputation on which its name is
based. Not only is its period of eruption lengthening, but it is becoming irregular, and the irregularity appears to
be increasing. In the short time during which this geyser has been under observation its period has changed from
a regular one of sixty minutes, or a little less, to an irregular one of seventy to ninety minutes. In the case of
some geysers years elapse between eruptions, and in some the date of the last eruption is so distant that it is
uncertain whether the vent should be looked upon as a geyser or merely a hot spring.
In the Yellowstone Park[120] the geysers are mainly in the bottoms of valleys (Fig. 219), but the deposits
characteristic of geysers are found in not a few places well above the present bottoms. These deposits record the
fact that in earlier times the geysers were at higher levels than now. It is probable that they have been, at all
stages in their history, near the bottoms of the valleys, and that, as the valleys have been deepened the ground-
water has found lower and lower points of issue. In this respect the geysers have probably had the same history
as other springs.
A few geysers have somewhat definite periods of eruption. Of such “Old Faithful” is the type; but even this
geyser, which formerly erupted at regular intervals of about an hour, is losing the reputation on which its name is
based. Not only is its period of eruption lengthening, but it is becoming irregular, and the irregularity appears to
be increasing. In the short time during which this geyser has been under observation its period has changed from
a regular one of sixty minutes, or a little less, to an irregular one of seventy to ninety minutes. In the case of
some geysers years elapse between eruptions, and in some the date of the last eruption is so distant that it is
uncertain whether the vent should be looked upon as a geyser or merely a hot spring.
In the Yellowstone Park[120] the geysers are mainly in the bottoms of valleys (Fig. 219), but the deposits
characteristic of geysers are found in not a few places well above the present bottoms. These deposits record the
fact that in earlier times the geysers were at higher levels than now. It is probable that they have been, at all
stages in their history, near the bottoms of the valleys, and that, as the valleys have been deepened the ground-
water has found lower and lower points of issue. In this respect the geysers have probably had the same history
as other springs.
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Fig. 219.—Hot springs and geysers. Norris Geyser basin, Yellowstone Park.
Unless new intrusions of lava occur, or unless heat is otherwise renewed at the proper points, it is probable
that all existing geysers will become extinct within a time which is, geologically, short. New geyser regions may,
however, develop as old ones disappear.
Artesian wells.—Originally the terms artesian wells and flowing wells were synonymous; but at the present
time any notably deep well is called artesian, especially if it descends to considerable depths below the mantle
rock. The artesian well which does not flow, does not differ from common wells in principle; but being deeper,
the water which it affords is often more thoroughly filtered and frequently more highly mineralized than that of
other wells. The flowing well is really a gushing spring, the opening of which was made by man.
Flowing wells[121] depend upon certain relations of rock structure, water supply, and elevation. Generally
speaking a flowing well is possible in any place underlain by any considerable bed of porous rock, if such rock
outcrops at a sufficiently higher level in a region of adequate rainfall, and is covered by a layer or bed of
impervious, or relatively impervious rock. This statement involves four conditions, all of which are illustrated
by Fig. 199, where a is the bed of porous rock. It is not necessary that the beds of rock form a structural basin,
nor is it usually necessary to take account of the character of the rock beneath the porous bed which contains the
water.
The bed of porous rock is the “reservoir” of the flowing well. Formations of sand or sandstone, and of gravel
or conglomerate, most commonly serve as the reservoirs. In order that it may contain abundant water it must
have some thickness, and its outcropping edge must be so situated that the water may enter freely and be
replenished, chiefly by rain, as the water flows out at the well.
A relatively impervious layer of rock above the reservoir (b, Fig. 199) is most important; otherwise the water
in the reservoir will leak out, and there will be little or no “head” at the well site. Thus if the rock overlying
stratum a (Fig. 199) were badly broken, the fractures extending up to the surface, the conditions would be
unfavorable for flowing wells. Under such conditions, wells in the positions of those shown in Fig. 199 might
Unless new intrusions of lava occur, or unless heat is otherwise renewed at the proper points, it is probable
that all existing geysers will become extinct within a time which is, geologically, short. New geyser regions may,
however, develop as old ones disappear.
Artesian wells.—Originally the terms artesian wells and flowing wells were synonymous; but at the present
time any notably deep well is called artesian, especially if it descends to considerable depths below the mantle
rock. The artesian well which does not flow, does not differ from common wells in principle; but being deeper,
the water which it affords is often more thoroughly filtered and frequently more highly mineralized than that of
other wells. The flowing well is really a gushing spring, the opening of which was made by man.
Flowing wells[121] depend upon certain relations of rock structure, water supply, and elevation. Generally
speaking a flowing well is possible in any place underlain by any considerable bed of porous rock, if such rock
outcrops at a sufficiently higher level in a region of adequate rainfall, and is covered by a layer or bed of
impervious, or relatively impervious rock. This statement involves four conditions, all of which are illustrated
by Fig. 199, where a is the bed of porous rock. It is not necessary that the beds of rock form a structural basin,
nor is it usually necessary to take account of the character of the rock beneath the porous bed which contains the
water.
The bed of porous rock is the “reservoir” of the flowing well. Formations of sand or sandstone, and of gravel
or conglomerate, most commonly serve as the reservoirs. In order that it may contain abundant water it must
have some thickness, and its outcropping edge must be so situated that the water may enter freely and be
replenished, chiefly by rain, as the water flows out at the well.
A relatively impervious layer of rock above the reservoir (b, Fig. 199) is most important; otherwise the water
in the reservoir will leak out, and there will be little or no “head” at the well site. Thus if the rock overlying
stratum a (Fig. 199) were badly broken, the fractures extending up to the surface, the conditions would be
unfavorable for flowing wells. Under such conditions, wells in the positions of those shown in Fig. 199 might
Page 295
get abundant water, but they would not be likely to flow. If the stratum next below the reservoir is not
impervious, some lower one probably is. No layer of rock is more impervious than one which is full of water,
and the substructure of any bed which might serve as a reservoir is usually full of water, even if the rock be
porous.
If the outcrop of the reservoir be notably above the site of the well, and if it be kept full by frequent rains, the
“head” will be strong, though the water at the well will not rise to the level of the outcrop of the reservoir.
Experience has shown that an allowance of about one foot per mile of subterranean flow should be made. Thus
if the site of the well be 100 miles from the outcrop of the water-bearing stratum, and 200 feet below it, the
water will rise something like 100 feet above the surface at the well. This rule is, however, not applicable
everywhere. The failure of the water to rise to the level of its head is due to the adhesion and the friction of flow
through the rock. The more porous the rock the less the reduction of head by friction. The height of the flow is
also influenced by the number of wells drawing on the same reservoir, on the degree of imperviousness of the
confining bed above, etc.
Flowing wells, often relatively shallow, are frequently obtained from unconsolidated drift. Some such
relations as suggested by Fig. 220 would afford the conditions for flowing wells in such a formation.
Fig. 220.—Figure illustrating the principle of artesian wells in drift.
impervious, some lower one probably is. No layer of rock is more impervious than one which is full of water,
and the substructure of any bed which might serve as a reservoir is usually full of water, even if the rock be
porous.
If the outcrop of the reservoir be notably above the site of the well, and if it be kept full by frequent rains, the
“head” will be strong, though the water at the well will not rise to the level of the outcrop of the reservoir.
Experience has shown that an allowance of about one foot per mile of subterranean flow should be made. Thus
if the site of the well be 100 miles from the outcrop of the water-bearing stratum, and 200 feet below it, the
water will rise something like 100 feet above the surface at the well. This rule is, however, not applicable
everywhere. The failure of the water to rise to the level of its head is due to the adhesion and the friction of flow
through the rock. The more porous the rock the less the reduction of head by friction. The height of the flow is
also influenced by the number of wells drawing on the same reservoir, on the degree of imperviousness of the
confining bed above, etc.
Flowing wells, often relatively shallow, are frequently obtained from unconsolidated drift. Some such
relations as suggested by Fig. 220 would afford the conditions for flowing wells in such a formation.
Fig. 220.—Figure illustrating the principle of artesian wells in drift.
Page 296
CHAPTER V.
THE WORK OF SNOW AND ICE.
A part of the atmospheric precipitation falls as snow, and this, like the
rain, does its appropriate work in degrading the land. Over the larger part of
the land surface the snow of the winter does not endure through the
succeeding summer, and when it melts it follows the same course as the
precipitation which falls as rain; but in cold regions where the fall of snow
is heavy some of it remains unmelted and constitutes perennial snow-fields.
SNOW- AND ICE-FIELDS.
Snow-fields.—Mountain heights and polar lands are the most common
habitats of snow-fields, though they are not confined to these situations. In
North America there are numerous small snow-fields in the western
mountains, from Mexico on the south to Alaska on the north, their number
and size increasing in the latter direction. In the United States there are few
snow-fields south of the parallel of 36° 30′, and most of the many hundreds
north of that latitude (excluding Alaska) are small (Pl. XVIII, Fig. 1,
Washington, Lat. 48° 5′, Long. 121° 5′; Fig. 2, Lat. 41° 25′, Long. 122° 12′.
From Glacier Peak and Shasta Special Quadrangles, U. S. Geol. Surv.).
Farther north, especially in Alaska, the snow-fields of the western
mountains attain much greater size. In Europe snow-fields comparable to
those of the northwestern part of the United States and British Columbia
occur in the Alps (Fig. 221), the Pyrenees, the Caucasus, and the
Scandinavian mountains. In Asia snow-fields occur in the Himalayas and in
many of the high mountains farther north, from Turkestan on the southwest
nearly to the coast on the northeast. In South America there are snow-fields
of small size even in equatorial latitudes, and farther south in the Chilean
Andes there are some of considerable size. Small snow-fields occur on the
highest peaks of tropical Africa, and in the mountains of New Zealand. For
THE WORK OF SNOW AND ICE.
A part of the atmospheric precipitation falls as snow, and this, like the
rain, does its appropriate work in degrading the land. Over the larger part of
the land surface the snow of the winter does not endure through the
succeeding summer, and when it melts it follows the same course as the
precipitation which falls as rain; but in cold regions where the fall of snow
is heavy some of it remains unmelted and constitutes perennial snow-fields.
SNOW- AND ICE-FIELDS.
Snow-fields.—Mountain heights and polar lands are the most common
habitats of snow-fields, though they are not confined to these situations. In
North America there are numerous small snow-fields in the western
mountains, from Mexico on the south to Alaska on the north, their number
and size increasing in the latter direction. In the United States there are few
snow-fields south of the parallel of 36° 30′, and most of the many hundreds
north of that latitude (excluding Alaska) are small (Pl. XVIII, Fig. 1,
Washington, Lat. 48° 5′, Long. 121° 5′; Fig. 2, Lat. 41° 25′, Long. 122° 12′.
From Glacier Peak and Shasta Special Quadrangles, U. S. Geol. Surv.).
Farther north, especially in Alaska, the snow-fields of the western
mountains attain much greater size. In Europe snow-fields comparable to
those of the northwestern part of the United States and British Columbia
occur in the Alps (Fig. 221), the Pyrenees, the Caucasus, and the
Scandinavian mountains. In Asia snow-fields occur in the Himalayas and in
many of the high mountains farther north, from Turkestan on the southwest
nearly to the coast on the northeast. In South America there are snow-fields
of small size even in equatorial latitudes, and farther south in the Chilean
Andes there are some of considerable size. Small snow-fields occur on the
highest peaks of tropical Africa, and in the mountains of New Zealand. For
Page 297
reasons which will appear later, much of every considerable snow-field is
really ice.
In addition to these limited fields of snow in mountain regions, there are
fields of much greater extent covering wide expanses of plain and plateau in
the polar regions. The greater part of the island of Greenland is covered
with a single field of ice and snow, the size of which is variously estimated
at 300,000 to 400,000 square miles (Fig. 222)—an area 400 to 600 times as
large as the snow-and-ice-covered area of Switzerland. Numerous islands to
the west of North Greenland are also partly covered with snow, the areas of
the snow-fields far exceeding those of most mountain regions. In Antarctica
there is believed to be a still larger field, the largest of the earth. Its area is
not even approximately known, but such data as are at hand indicate that it
may have an extent of 3,000,000 or 4,000,000 square miles.
Fig. 221.—An alpine snow-field.
really ice.
In addition to these limited fields of snow in mountain regions, there are
fields of much greater extent covering wide expanses of plain and plateau in
the polar regions. The greater part of the island of Greenland is covered
with a single field of ice and snow, the size of which is variously estimated
at 300,000 to 400,000 square miles (Fig. 222)—an area 400 to 600 times as
large as the snow-and-ice-covered area of Switzerland. Numerous islands to
the west of North Greenland are also partly covered with snow, the areas of
the snow-fields far exceeding those of most mountain regions. In Antarctica
there is believed to be a still larger field, the largest of the earth. Its area is
not even approximately known, but such data as are at hand indicate that it
may have an extent of 3,000,000 or 4,000,000 square miles.
Fig. 221.—An alpine snow-field.
Page 298
The only condition necessary
for a snow-field is an excess of
snowfall over snow waste. The
lower edge of a snow-field, the
snow-line, is dependent chiefly on
temperature and snowfall. In
general it does not depart much
from the summer isotherm of 32°,
though it may be well above this
isotherm where the snowfall is
light. That the snow-line is not a
function of temperature only is
shown by its position in various
places. In the equatorial portion of
the Andes, for example, the snow-
line has an altitude of about
16,000 feet on the east side of the
mountains, where the precipitation
is heavier, and of about 18,500
feet on the west side, where it is
lighter. For the same reason the
snow-line in the Himalayas is
3000 or 4000 feet lower on the
south side than on the north.
While in equatorial regions the
Fig. 222.—Map of Greenland. The borders snow-line has an altitude of
only are free from ice. (Stieler.) 15,000 to 18,000 feet, it
approaches or even reaches sea-level in the latitude of Antarctica and North
Greenland. In intermediate latitudes it has an intermediate position.
While temperature and snowfall are the most important factors
controlling the position of the snow-line, both humidity and the movements
of the air are of some importance, since both affect the rate of evaporation
of snow and ice.
The passage of snow into névé and ice.—The snow does not lie on the
surface long before it undergoes obvious change. The light flakes soon
begin to be transformed into granules, and the snow becomes “coarse-
for a snow-field is an excess of
snowfall over snow waste. The
lower edge of a snow-field, the
snow-line, is dependent chiefly on
temperature and snowfall. In
general it does not depart much
from the summer isotherm of 32°,
though it may be well above this
isotherm where the snowfall is
light. That the snow-line is not a
function of temperature only is
shown by its position in various
places. In the equatorial portion of
the Andes, for example, the snow-
line has an altitude of about
16,000 feet on the east side of the
mountains, where the precipitation
is heavier, and of about 18,500
feet on the west side, where it is
lighter. For the same reason the
snow-line in the Himalayas is
3000 or 4000 feet lower on the
south side than on the north.
While in equatorial regions the
Fig. 222.—Map of Greenland. The borders snow-line has an altitude of
only are free from ice. (Stieler.) 15,000 to 18,000 feet, it
approaches or even reaches sea-level in the latitude of Antarctica and North
Greenland. In intermediate latitudes it has an intermediate position.
While temperature and snowfall are the most important factors
controlling the position of the snow-line, both humidity and the movements
of the air are of some importance, since both affect the rate of evaporation
of snow and ice.
The passage of snow into névé and ice.—The snow does not lie on the
surface long before it undergoes obvious change. The light flakes soon
begin to be transformed into granules, and the snow becomes “coarse-
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grained.” The granular character, so pronounced in the snow of the last
banks which remain in the spring in temperate latitudes, is even more
distinct in perennial snow-fields, either at the surface or just beneath it. This
granular snow is called névé, or firn. Still deeper beneath the surface, where
the thickness of the snow is great, the névé becomes more compact and
finally coherent, and grades into porous ice. This gradation is accomplished
at no great depth, though the thicknesses of snow and névé are by no means
constant.
Structure of the ice.—Ice formed beneath a snow-field is in some sense
stratified. It is made up of successive falls of snow which tend to retain the
form of layers. This follows from two or three conditions. The snow of one
season, or of one period of precipitation, may have been considerably
changed before the succeeding fall of snow. So also the surface of the
snow-field at the end of the melting season is often covered with a visible
amount of earthy matter, some of which was blown up and dropped on the
surface during the melting season, and some of which was concentrated in
that position by the melting of the snow in which it was originally
imbedded. The amount of earthy matter is often sufficient to define snows
of successive years, or perhaps of minor periods of precipitation, and makes
distinct the stratification which would otherwise remain obscure. The
snowfall of successive years has been estimated by this means[122] where the
snow is exposed in crevices in the snow-field.
In addition to its rude stratification, the ice of the deeper portions often
acquires a stratiform structure which may perhaps best be called foliation to
distinguish it from the stratification which arises from deposition. The
foliation appears to result mainly from the shearing of one part over another
in the course of the movements to which the ice is subjected, as will be
illustrated presently.
Texture.—The ice derived from the snow is formed of interlocking
crystalline grains. The crystalline character is present from the beginning,
for it is assumed by the snowflakes when they form, and the subsequent
changes seem only to modify the original crystals by building up some and
destroying others. By the time the snow is converted into névé, the granules
have become coarse, and wherever the ice derived from the névé has been
examined, the granular crystalline texture is present. The individual crystals
in the ice are usually larger than those of the névé, and more closely grown
banks which remain in the spring in temperate latitudes, is even more
distinct in perennial snow-fields, either at the surface or just beneath it. This
granular snow is called névé, or firn. Still deeper beneath the surface, where
the thickness of the snow is great, the névé becomes more compact and
finally coherent, and grades into porous ice. This gradation is accomplished
at no great depth, though the thicknesses of snow and névé are by no means
constant.
Structure of the ice.—Ice formed beneath a snow-field is in some sense
stratified. It is made up of successive falls of snow which tend to retain the
form of layers. This follows from two or three conditions. The snow of one
season, or of one period of precipitation, may have been considerably
changed before the succeeding fall of snow. So also the surface of the
snow-field at the end of the melting season is often covered with a visible
amount of earthy matter, some of which was blown up and dropped on the
surface during the melting season, and some of which was concentrated in
that position by the melting of the snow in which it was originally
imbedded. The amount of earthy matter is often sufficient to define snows
of successive years, or perhaps of minor periods of precipitation, and makes
distinct the stratification which would otherwise remain obscure. The
snowfall of successive years has been estimated by this means[122] where the
snow is exposed in crevices in the snow-field.
In addition to its rude stratification, the ice of the deeper portions often
acquires a stratiform structure which may perhaps best be called foliation to
distinguish it from the stratification which arises from deposition. The
foliation appears to result mainly from the shearing of one part over another
in the course of the movements to which the ice is subjected, as will be
illustrated presently.
Texture.—The ice derived from the snow is formed of interlocking
crystalline grains. The crystalline character is present from the beginning,
for it is assumed by the snowflakes when they form, and the subsequent
changes seem only to modify the original crystals by building up some and
destroying others. By the time the snow is converted into névé, the granules
have become coarse, and wherever the ice derived from the névé has been
examined, the granular crystalline texture is present. The individual crystals
in the ice are usually larger than those of the névé, and more closely grown
Page 300
together. In the fresh unexposed ice the crystals are so intimately
interlocked that they are not readily seen except under a polarizing
microscope, but when the ice has been honeycombed by partial melting, the
granules become partially separated and may be easily seen. Fig. 223 shows
quantities of them which have been washed down from the surface, and
disposed as cones at its base. While a given mass of snow in a great snow-
and ice-field cannot be followed consecutively through its whole history,
yet since (1) the granular texture is pronounced in the névé stage where the
granules show evidences of growth, and since (2) the same texture is also
pronounced in the last stages of the ice when it is undergoing dissolution, as
well as at all observed intermediate stages, and since (3) the crystals are, on
the average, larger in proportion to the lateness of the stage of their history,
while (4) experiment has shown that granules grow under the conditions
which exist in snow-fields, and (5) that they persist under very considerable
pressure, it is legitimate to assume that a granular crystalline condition
persists throughout all stages, and is a feature of progressive growth.
Fig. 223.—Figure showing cones of granules of ice which have been washed down the front
of the glacier by streamlets, and accumulated after the manner of talus or alluvial cones.
North Greenland.
Inauguration of movement.—Eventually the increase in depth of snow
and ice in a snow-field gives rise to motion. The exact nature of the motion
has not yet been demonstrated to the satisfaction of all investigators. Brittle
interlocked that they are not readily seen except under a polarizing
microscope, but when the ice has been honeycombed by partial melting, the
granules become partially separated and may be easily seen. Fig. 223 shows
quantities of them which have been washed down from the surface, and
disposed as cones at its base. While a given mass of snow in a great snow-
and ice-field cannot be followed consecutively through its whole history,
yet since (1) the granular texture is pronounced in the névé stage where the
granules show evidences of growth, and since (2) the same texture is also
pronounced in the last stages of the ice when it is undergoing dissolution, as
well as at all observed intermediate stages, and since (3) the crystals are, on
the average, larger in proportion to the lateness of the stage of their history,
while (4) experiment has shown that granules grow under the conditions
which exist in snow-fields, and (5) that they persist under very considerable
pressure, it is legitimate to assume that a granular crystalline condition
persists throughout all stages, and is a feature of progressive growth.
Fig. 223.—Figure showing cones of granules of ice which have been washed down the front
of the glacier by streamlets, and accumulated after the manner of talus or alluvial cones.
North Greenland.
Inauguration of movement.—Eventually the increase in depth of snow
and ice in a snow-field gives rise to motion. The exact nature of the motion
has not yet been demonstrated to the satisfaction of all investigators. Brittle
Page 301
and resistant as ice seems, it exhibits, under proper conditions, some of the
outward characteristics of a plastic substance. Thus it may be made to
change its form, and may even be moulded into almost any desired shape if
carefully subjected to sufficient pressure, steadily applied through long
intervals of time.[123] These changes may be brought about without visible
fracture, and have been thought to point to a viscous condition of the ice.
There is much reason, however, as will be seen later, to question this
interpretation of the ultimate nature of the movement. Whatever this may
be, the mass result of the movement in a field of ice is comparable, in a
superficial way at least, to that which would be brought about if the ice
were capable of moving like a viscous liquid, the motion taking place with
extreme slowness. This slow motion of ice in an ice-field is glacier motion,
and ice thus moving is glacier ice.
Fig. 224.—Ice-caps of small size. The figure also shows some valley glaciers extending out
from the main ice-sheet and from the local ice-caps. A portion of the North Greenland
coast, north of Inglefield Gulf. Lat. about 78°. (Peary.)
outward characteristics of a plastic substance. Thus it may be made to
change its form, and may even be moulded into almost any desired shape if
carefully subjected to sufficient pressure, steadily applied through long
intervals of time.[123] These changes may be brought about without visible
fracture, and have been thought to point to a viscous condition of the ice.
There is much reason, however, as will be seen later, to question this
interpretation of the ultimate nature of the movement. Whatever this may
be, the mass result of the movement in a field of ice is comparable, in a
superficial way at least, to that which would be brought about if the ice
were capable of moving like a viscous liquid, the motion taking place with
extreme slowness. This slow motion of ice in an ice-field is glacier motion,
and ice thus moving is glacier ice.
Fig. 224.—Ice-caps of small size. The figure also shows some valley glaciers extending out
from the main ice-sheet and from the local ice-caps. A portion of the North Greenland
coast, north of Inglefield Gulf. Lat. about 78°. (Peary.)
Page 302
Fig. 225.—Small ice-caps in the northwestern part of Iceland. (Thoraddsen’s geological
map of Iceland.)
Fig. 226.—A glacial lobe, midway between an ice-cap and a valley glacier. A protrusion
from a local ice-cap east of Cape York, Greenland.
If both the surface on which the ice-sheet develops and its surroundings
be essentially plane, as may happen in high latitudes, and if the snow- and
ice-field be symmetrical in shape, the outward movement will be
approximately equal in all directions, and the area covered by the spreading
ice-field will remain more or less circular. If the ice-field rests on a steeply
inclined surface, like a mountain slope, the movement becomes one-sided
map of Iceland.)
Fig. 226.—A glacial lobe, midway between an ice-cap and a valley glacier. A protrusion
from a local ice-cap east of Cape York, Greenland.
If both the surface on which the ice-sheet develops and its surroundings
be essentially plane, as may happen in high latitudes, and if the snow- and
ice-field be symmetrical in shape, the outward movement will be
approximately equal in all directions, and the area covered by the spreading
ice-field will remain more or less circular. If the ice-field rests on a steeply
inclined surface, like a mountain slope, the movement becomes one-sided
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in conformity to the slope. If the surface, otherwise plane, be affected by
valleys parallel to the direction of movement, the ice in the valleys will be
deeper than that on the divides between them, and its movement stronger. In
the valleys, therefore, the ice will advance farther than elsewhere before
being melted, and the outline of the ice will become lobate, the lobes
occupying the depressions. These general relations are shown in Figs. 224
and 225. If the depressions be wide and shallow, the lobes will be broad and
short (Fig. 226); if the depressions be narrow and deep, the lobes will be
relatively narrow and Long. If the snow and ice rest on a surface consisting
chiefly of steep valleys and sharp ridges, as is common on mountain slopes,
the snow and ice are chiefly gathered in the valleys, and take a linear form.
TYPES OF GLACIERS.
These different forms give rise to different terms. The ice which spreads
with some approach to equality in all directions from a center is a glacier, is
indeed the type of the greatest glaciers, but is commonly called an ice-cap.
The same name is applied to any glacier in which there is movement in all
directions from the center, even though its shape departs widely from a
circle. The glacier covering the larger part of Greenland (Fig. 222) is a good
example of a large ice-cap, and the glaciers on some of the flat-topped
peninsular promontories of the same island are good examples of small
ones (Fig. 224). If ice-caps cover a large part of a continent, as some of
those of the past have done, they are often called continental glaciers.
valleys parallel to the direction of movement, the ice in the valleys will be
deeper than that on the divides between them, and its movement stronger. In
the valleys, therefore, the ice will advance farther than elsewhere before
being melted, and the outline of the ice will become lobate, the lobes
occupying the depressions. These general relations are shown in Figs. 224
and 225. If the depressions be wide and shallow, the lobes will be broad and
short (Fig. 226); if the depressions be narrow and deep, the lobes will be
relatively narrow and Long. If the snow and ice rest on a surface consisting
chiefly of steep valleys and sharp ridges, as is common on mountain slopes,
the snow and ice are chiefly gathered in the valleys, and take a linear form.
TYPES OF GLACIERS.
These different forms give rise to different terms. The ice which spreads
with some approach to equality in all directions from a center is a glacier, is
indeed the type of the greatest glaciers, but is commonly called an ice-cap.
The same name is applied to any glacier in which there is movement in all
directions from the center, even though its shape departs widely from a
circle. The glacier covering the larger part of Greenland (Fig. 222) is a good
example of a large ice-cap, and the glaciers on some of the flat-topped
peninsular promontories of the same island are good examples of small
ones (Fig. 224). If ice-caps cover a large part of a continent, as some of
those of the past have done, they are often called continental glaciers.
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Fig. 227.—Characteristic end of a North Greenland (Bryant) glacier.
Fig. 228.—The Rhône glacier. (Reid.)
Fig. 228.—The Rhône glacier. (Reid.)
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Fig. 229.—Characteristic end of a North Greenland glacier. North side of Herbert Island,
Inglefield Gulf.
Inglefield Gulf.
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Fig. 230.—The end of an alpine (Forno, Switzerland) glacier. (Reid.)
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Fig. 231.—Deploying end of a North Greenland glacier.
Where ice-caps are developed on plateaus whose borders are trenched by
valleys, ice-tongues from the edge of the ice-cap often extend down into the
valleys and give rise to one type of valley glacier (Figs. 224 and 227). A
second and more familiar type of valley glacier occupies mountain valleys,
and is the offspring of mountain snow-fields (Fig. 228). The former are
confined chiefly to high latitudes, and are distinguished as polar or high-
latitude glaciers (Figs. 227 and 229); the latter are known as alpine glaciers
(Figs. 228 and 230). The end and side slopes of polar glaciers are, as a rule,
much steeper than those of alpine glaciers. When a valley glacier descends
through its valley to the plain beyond, its end deploys, forming a fan (Fig.
231). The deploying ends of adjacent glaciers sometimes merge, and the
resulting body of ice constitutes a piedmont glacier (Fig. 232). At the
present time, piedmont glaciers are confined to high latitudes. In some cases
the snow-field that gives rise to a glacier is restricted to a relatively small
depression in the side of a mountain, or in the escarpment of a plateau. In
such cases the snow-field and glacier are hardly distinguishable, and the
latter descends but little below the snow-line. In many cases it does not
even enter the narrow valley which leads out from the depression occupied
by the snow-field. Such a glacier is nestled in the face of a cliff, and may
therefore be called a cliff glacier[124] (Figs. 233 and 234). The snow-field of
a cliff glacier is sometimes no more than a great snowdrift, accumulated
Where ice-caps are developed on plateaus whose borders are trenched by
valleys, ice-tongues from the edge of the ice-cap often extend down into the
valleys and give rise to one type of valley glacier (Figs. 224 and 227). A
second and more familiar type of valley glacier occupies mountain valleys,
and is the offspring of mountain snow-fields (Fig. 228). The former are
confined chiefly to high latitudes, and are distinguished as polar or high-
latitude glaciers (Figs. 227 and 229); the latter are known as alpine glaciers
(Figs. 228 and 230). The end and side slopes of polar glaciers are, as a rule,
much steeper than those of alpine glaciers. When a valley glacier descends
through its valley to the plain beyond, its end deploys, forming a fan (Fig.
231). The deploying ends of adjacent glaciers sometimes merge, and the
resulting body of ice constitutes a piedmont glacier (Fig. 232). At the
present time, piedmont glaciers are confined to high latitudes. In some cases
the snow-field that gives rise to a glacier is restricted to a relatively small
depression in the side of a mountain, or in the escarpment of a plateau. In
such cases the snow-field and glacier are hardly distinguishable, and the
latter descends but little below the snow-line. In many cases it does not
even enter the narrow valley which leads out from the depression occupied
by the snow-field. Such a glacier is nestled in the face of a cliff, and may
therefore be called a cliff glacier[124] (Figs. 233 and 234). The snow-field of
a cliff glacier is sometimes no more than a great snowdrift, accumulated
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through successive years. Cliff glaciers are often as wide as long, and are
always small, and between them and valley glaciers there are all gradations
(Fig. 235). Occasionally the end of a valley glacier, or the edge of an ice-
sheet reaches a precipitous cliff, and the end or edge of the ice breaks off
and accumulates like talus below. The ice fragments may then again
become a coherent mass by regelation, and the whole may resume motion.
Such a glacier is called a reconstructed glacier. The precipitous cliffs of the
Greenland coast furnish illustrations.
Fig. 232.—The Malaspina glacier, Alaska; the best known example of a piedmont glacier.
(Russell.)
always small, and between them and valley glaciers there are all gradations
(Fig. 235). Occasionally the end of a valley glacier, or the edge of an ice-
sheet reaches a precipitous cliff, and the end or edge of the ice breaks off
and accumulates like talus below. The ice fragments may then again
become a coherent mass by regelation, and the whole may resume motion.
Such a glacier is called a reconstructed glacier. The precipitous cliffs of the
Greenland coast furnish illustrations.
Fig. 232.—The Malaspina glacier, Alaska; the best known example of a piedmont glacier.
(Russell.)
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Fig. 233.—A cliff glacier. North Greenland type. North side of Herbert Island, Inglefield
Gulf. The lower half of the white area is snow, and snow talus. So also are the white
patches to the right. The height of the cliff is perhaps 2000 feet. The water in the
foreground is the sea.
Gulf. The lower half of the white area is snow, and snow talus. So also are the white
patches to the right. The height of the cliff is perhaps 2000 feet. The water in the
foreground is the sea.
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Fig. 234.—Chancy glacier; a cliff glacier of the Montana type. (Shepard.)
Of the foregoing types of glaciers, the ice-caps far exceed all others both
in size and importance, while the valley glaciers out-rank, in the same
respects, the other types; but since the valley glaciers are the most familiar
type, the general phenomena of glaciers will be discussed with primary
reference to them.
THE GENERAL PHENOMENA OF GLACIERS.[125]
Dimensions.—Glaciers which occupy valleys leading down from snow-
fields sometimes reach the upper parts of the valleys only, sometimes
extend through them, and sometimes push out on the plain beyond. In
length they range from a fraction of a mile to many miles, and though their
width is usually much less than their length, the reverse is sometimes the
case (Figs. 233, 234, and 235). Their thickness is usually measured by
Of the foregoing types of glaciers, the ice-caps far exceed all others both
in size and importance, while the valley glaciers out-rank, in the same
respects, the other types; but since the valley glaciers are the most familiar
type, the general phenomena of glaciers will be discussed with primary
reference to them.
THE GENERAL PHENOMENA OF GLACIERS.[125]
Dimensions.—Glaciers which occupy valleys leading down from snow-
fields sometimes reach the upper parts of the valleys only, sometimes
extend through them, and sometimes push out on the plain beyond. In
length they range from a fraction of a mile to many miles, and though their
width is usually much less than their length, the reverse is sometimes the
case (Figs. 233, 234, and 235). Their thickness is usually measured by
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hundreds of feet rather than by denominations of other orders, but the
variation is great, and exact measurements are almost wholly wanting. The
minimum thickness is that necessary to cause movement, and this varies
with the slope, the temperature, and other conditions. There is also much
variation in the thickness in different parts of a glacier. As a rule, it is
thinnest in its terminal portion, and thickest at some point intermediate
between this and its source, but nearer the latter than the former. Cliff and
reconstructed glaciers are comparable in size to the smaller valley glaciers.
Piedmont glaciers may attain greater size.
variation is great, and exact measurements are almost wholly wanting. The
minimum thickness is that necessary to cause movement, and this varies
with the slope, the temperature, and other conditions. There is also much
variation in the thickness in different parts of a glacier. As a rule, it is
thinnest in its terminal portion, and thickest at some point intermediate
between this and its source, but nearer the latter than the former. Cliff and
reconstructed glaciers are comparable in size to the smaller valley glaciers.
Piedmont glaciers may attain greater size.
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Fig. 235.—A glacier in the Cascades near Cascade Pass, Wash. A glacier intermediate
between a cliff glacier and a valley glacier. (Willis, U. S. Geol. Surv.)
An ice-cap is theoretically thickest at its center and thins away to its
borders, but its actual dimensions are influenced by the topography on
which it is developed. The Greenland ice-cap is known to rise about 9000
feet above the sea, and it probably reaches considerably higher than this in
the unexplored center of its broad dome. The height of the land surface
beneath is unknown, but it is unlikely that it averages half this amount, and
hence the ice is probably 5000 feet or more thick in the center. There is
reason to think that it is much thicker in Antarctica.
between a cliff glacier and a valley glacier. (Willis, U. S. Geol. Surv.)
An ice-cap is theoretically thickest at its center and thins away to its
borders, but its actual dimensions are influenced by the topography on
which it is developed. The Greenland ice-cap is known to rise about 9000
feet above the sea, and it probably reaches considerably higher than this in
the unexplored center of its broad dome. The height of the land surface
beneath is unknown, but it is unlikely that it averages half this amount, and
hence the ice is probably 5000 feet or more thick in the center. There is
reason to think that it is much thicker in Antarctica.
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Limits.—The ice of a glacier is always moving forward (neglecting
temporary halts), but the end of a glacier may be retreating, advancing or
remaining stationary, according as the rate of wastage is greater, less, or just
equal to the forward movement of the ice. The position of the lower end of
the glacier is therefore determined by the ratio of movement to wastage. Its
upper end is generally ill-defined. In a superficial sense, it is the point
where the ice emerges from the snow-field; but the lower limit of the snow-
field is often ill-defined, and in any case is not the true upper limit of the
glacier, since there must be movement from the granular mass of ice
beneath the snow to make up for the waste below, and the moving ice
beneath the snow-field which feeds the tongue of ice in the valley is just as
really a part of the glacier as the more consolidated portion in the valley
below. If a definite upper limit for an alpine glacier is to be named, it should
probably be the Bergschrund, a gaping crevasse, or series of crevasses
which sometimes open near the precipitous slope of the peak or cliff where
the snow-field lies. The Bergschrund is formed by the moving of the lower
part of the snow-field away from the portion above.
The lower end of a glacier is usually free from snow and névé in summer,
but, traced toward its source, it first becomes covered with névé, then with
snow, and finally merges into the snow-field without having ceased to be a
glacier. The term glacier is, however, commonly used to mean merely the
more solid portion outside (below) the névé.
Movement.—The fact of glacier movement is established in various
ways, the most obvious being by the advance of its lower end. Such
advance is too slow to be seen from day to day, and is only detected when
the lower end of the glacier overrides or overturns objects in front of it, or
moves out over ground previously unoccupied. But even when the end of a
glacier is not advancing, the movement of the ice may be established by
means of stakes or other marks set on the surface. If the positions of these
marks relative to fixed points on the sides of the valley be determined, they
are found after a time to have moved down the valley. Rows of stakes or
lines of stones set across a glacier in the upper, middle and lower portions
have revealed many facts concerning the movement of the ice.
Generally speaking, the middle of a valley glacier moves more rapidly
than its sides (Fig. 236), but in some cases, especially in large glaciers,
there are found to be two or more main lines of movement, with belts of
temporary halts), but the end of a glacier may be retreating, advancing or
remaining stationary, according as the rate of wastage is greater, less, or just
equal to the forward movement of the ice. The position of the lower end of
the glacier is therefore determined by the ratio of movement to wastage. Its
upper end is generally ill-defined. In a superficial sense, it is the point
where the ice emerges from the snow-field; but the lower limit of the snow-
field is often ill-defined, and in any case is not the true upper limit of the
glacier, since there must be movement from the granular mass of ice
beneath the snow to make up for the waste below, and the moving ice
beneath the snow-field which feeds the tongue of ice in the valley is just as
really a part of the glacier as the more consolidated portion in the valley
below. If a definite upper limit for an alpine glacier is to be named, it should
probably be the Bergschrund, a gaping crevasse, or series of crevasses
which sometimes open near the precipitous slope of the peak or cliff where
the snow-field lies. The Bergschrund is formed by the moving of the lower
part of the snow-field away from the portion above.
The lower end of a glacier is usually free from snow and névé in summer,
but, traced toward its source, it first becomes covered with névé, then with
snow, and finally merges into the snow-field without having ceased to be a
glacier. The term glacier is, however, commonly used to mean merely the
more solid portion outside (below) the névé.
Movement.—The fact of glacier movement is established in various
ways, the most obvious being by the advance of its lower end. Such
advance is too slow to be seen from day to day, and is only detected when
the lower end of the glacier overrides or overturns objects in front of it, or
moves out over ground previously unoccupied. But even when the end of a
glacier is not advancing, the movement of the ice may be established by
means of stakes or other marks set on the surface. If the positions of these
marks relative to fixed points on the sides of the valley be determined, they
are found after a time to have moved down the valley. Rows of stakes or
lines of stones set across a glacier in the upper, middle and lower portions
have revealed many facts concerning the movement of the ice.
Generally speaking, the middle of a valley glacier moves more rapidly
than its sides (Fig. 236), but in some cases, especially in large glaciers,
there are found to be two or more main lines of movement, with belts of
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lesser movement between. The top of a glacier moves, on the whole, more
rapidly than the bottom, though the observations made do not show that the
rate of movement diminishes regularly downward, and it probably does not
so diminish in many cases. In Switzerland, where the glaciers have been
studied more carefully than elsewhere, the determined rates of movement
range from one or two inches to four feet or more per day. Some of the
larger glaciers in other regions move more rapidly, but it does not follow
that large glaciers always move faster than small ones. The Muir glacier of
Alaska has been found to move seven feet or more per day,[126] and some of
the glaciers of Greenland have been found to move, in the summer time, 50,
60, or even more feet per day. A single estimate as high as 100 feet per day
has been made; but these high rates have been observed only where the ice
of a large inland area crowds down into a comparatively narrow fjord, and
debouches into the sea, and then only in the summer. In the case of the
glacier with the highest recorded rate of summer movement, 100 feet per
day, the advance was only 34 feet at about the same place in April.
rapidly than the bottom, though the observations made do not show that the
rate of movement diminishes regularly downward, and it probably does not
so diminish in many cases. In Switzerland, where the glaciers have been
studied more carefully than elsewhere, the determined rates of movement
range from one or two inches to four feet or more per day. Some of the
larger glaciers in other regions move more rapidly, but it does not follow
that large glaciers always move faster than small ones. The Muir glacier of
Alaska has been found to move seven feet or more per day,[126] and some of
the glaciers of Greenland have been found to move, in the summer time, 50,
60, or even more feet per day. A single estimate as high as 100 feet per day
has been made; but these high rates have been observed only where the ice
of a large inland area crowds down into a comparatively narrow fjord, and
debouches into the sea, and then only in the summer. In the case of the
glacier with the highest recorded rate of summer movement, 100 feet per
day, the advance was only 34 feet at about the same place in April.
Page 315
Fig. 236.—Diagram to show the rate of movement of the Rhone Glacier at various points in
its course at centre and sides. It also shows the fluctuations in the positions of the end of
the glacier between 1874 and 1882, and the profile of the ice. (Heim.)
The average movement of the border of the inland ice of Greenland is
very small. Rink says that “between 62° and 68° 30′, the edge of the inland
ice is almost stationary for a remarkably long distance.”[127] The
observations of the authors between 77° and 78° were of like import.
Probably the average movement of the border of the Greenland ice-cap is
less than one foot a week.
its course at centre and sides. It also shows the fluctuations in the positions of the end of
the glacier between 1874 and 1882, and the profile of the ice. (Heim.)
The average movement of the border of the inland ice of Greenland is
very small. Rink says that “between 62° and 68° 30′, the edge of the inland
ice is almost stationary for a remarkably long distance.”[127] The
observations of the authors between 77° and 78° were of like import.
Probably the average movement of the border of the Greenland ice-cap is
less than one foot a week.
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Conditions affecting rate of movement.—The rate of glacier movement
appears to depend on (1) the depth of the moving ice; (2) the slope of the
surface over which it moves; (3) the slope of the upper surface of the ice;
(4) the topography of the bed over which it passes; (5) the temperature; and
(6) the amount of water which falls upon it or is carried to it by the drainage
of its surroundings, in addition to that produced by the melting of the
glacier itself. Great thickness, a steep slope, much water, smoothness of
bed, and a high (for ice) temperature favor rapid movement. Since some of
these conditions, notably temperature and amount of water, vary with the
season, the rate of movement for any given glacier is not constant
throughout the year. Other conditions, especially the first of those
mentioned above, vary through longer periods of time, and occasion
periodic variations in the rate of movement.
Since the volume of ice concerned influences the rate of movement,
anything which changes the volume affects the rate. An excess of snowfall
with favorable conditions for its preservation for a period of years,
increases the volume of ice, and tends to accelerate its movement. A
deficiency in snowfall, or in its preservation, as from high average
temperature or from aridity, diminishes the quantity of ice, and so retards
the movement. An acceleration of velocity causes the ice to move down the
valley farther before being melted, that is, causes the end of the glacier to
advance, while a decrease of velocity produces the opposite effect. As a
matter of fact, the lower ends of glaciers advance for a period of years and
then retreat, to advance again at a later time.[128] Observation has shown that
the periods of advance follow a succession of years when the snowfall has
been heavy and the temperature low, while the periods of retreat follow a
succession of years when the snowfall has been light and the temperature
above the average. The periods of advance and retreat lag behind the
periods of heavy and light snowfall respectively, by some years, and a long
glacier responds less promptly than a short one. Present knowledge seems
to point to a period of 35 to 40 years as the time within which a cycle of
fluctuation, that is, an advance and a retreat, takes place.
A declining upper surface is essential to glacier motion. There are short
stretches where this is not the case, and indeed there are particular places
where the upper surface slopes backward.[129] This may occur where the ice
is pushed up over a swell in its bed, or is crowded up against any
appears to depend on (1) the depth of the moving ice; (2) the slope of the
surface over which it moves; (3) the slope of the upper surface of the ice;
(4) the topography of the bed over which it passes; (5) the temperature; and
(6) the amount of water which falls upon it or is carried to it by the drainage
of its surroundings, in addition to that produced by the melting of the
glacier itself. Great thickness, a steep slope, much water, smoothness of
bed, and a high (for ice) temperature favor rapid movement. Since some of
these conditions, notably temperature and amount of water, vary with the
season, the rate of movement for any given glacier is not constant
throughout the year. Other conditions, especially the first of those
mentioned above, vary through longer periods of time, and occasion
periodic variations in the rate of movement.
Since the volume of ice concerned influences the rate of movement,
anything which changes the volume affects the rate. An excess of snowfall
with favorable conditions for its preservation for a period of years,
increases the volume of ice, and tends to accelerate its movement. A
deficiency in snowfall, or in its preservation, as from high average
temperature or from aridity, diminishes the quantity of ice, and so retards
the movement. An acceleration of velocity causes the ice to move down the
valley farther before being melted, that is, causes the end of the glacier to
advance, while a decrease of velocity produces the opposite effect. As a
matter of fact, the lower ends of glaciers advance for a period of years and
then retreat, to advance again at a later time.[128] Observation has shown that
the periods of advance follow a succession of years when the snowfall has
been heavy and the temperature low, while the periods of retreat follow a
succession of years when the snowfall has been light and the temperature
above the average. The periods of advance and retreat lag behind the
periods of heavy and light snowfall respectively, by some years, and a long
glacier responds less promptly than a short one. Present knowledge seems
to point to a period of 35 to 40 years as the time within which a cycle of
fluctuation, that is, an advance and a retreat, takes place.
A declining upper surface is essential to glacier motion. There are short
stretches where this is not the case, and indeed there are particular places
where the upper surface slopes backward.[129] This may occur where the ice
is pushed up over a swell in its bed, or is crowded up against any
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considerable obstacle; but such cases are no more than local exceptions, and
do not militate against the truth of the general statement that the upper
surface of a glacier declines in the direction of motion. A declining lower
surface is less necessary. In the case of valley glaciers, the bed does, as a
rule, decline in the direction of motion, but that there are local exceptions is
shown by the deep basins in rock which such glaciers often leave behind
them when they retreat. In the great continental glaciers of recent geologic
times, the ice frequently moved up slopes for scores, and even hundreds of
miles; but in all such cases, the upper surface must have declined in the
direction of movement. With a given thickness of ice, the greater the
decline of its lower surface in the direction of motion, the more rapid its
progress. A rough bed, or a crooked course retards the motion of a glacier,
while a smooth bottom and a straight course facilitate it.
Slope, roughness of bed, and volume affect the movement of glaciers
somewhat as they affect the movement of rivers. The temperature of the
water, on the other hand, has little effect on the flow of a river so long as it
remains unfrozen; but the effect of temperature on the motion of ice is most
important. In many cases, indeed, the temperature, together with the water
that is incidental to it, seems to be the chief factor in determining the rate of
movement. The way in which its effects are felt will be discussed later.
Likenesses and unlikenesses of glaciers and rivers.—Many of the
characteristics of a valley glacier may be understood from the study of the
accompanying figure (Fig. 237) of the White (Alaska) glacier. From this
figure it will be seen that the glacier is an elongate river-like body,
following the curves of the valley in stream-like fashion. It has its origin in
the snows collected on the mountain heights seen in the distance, and it
works its way down the valley in a manner which, in the aggregate, is
similar to the movement of a stiff liquid. The likeness to a river extends to
many details. Not only does the center move faster than the sides, and the
upper part faster than the bottom, as in the case of streams, but the
movement is more rapid in constricted portions of the valley and slower in
the broader parts. These and other likenesses, some of which are apparent
rather than real, have given origin to the view that glacier ice moves like a
stiff viscous liquid.
do not militate against the truth of the general statement that the upper
surface of a glacier declines in the direction of motion. A declining lower
surface is less necessary. In the case of valley glaciers, the bed does, as a
rule, decline in the direction of motion, but that there are local exceptions is
shown by the deep basins in rock which such glaciers often leave behind
them when they retreat. In the great continental glaciers of recent geologic
times, the ice frequently moved up slopes for scores, and even hundreds of
miles; but in all such cases, the upper surface must have declined in the
direction of movement. With a given thickness of ice, the greater the
decline of its lower surface in the direction of motion, the more rapid its
progress. A rough bed, or a crooked course retards the motion of a glacier,
while a smooth bottom and a straight course facilitate it.
Slope, roughness of bed, and volume affect the movement of glaciers
somewhat as they affect the movement of rivers. The temperature of the
water, on the other hand, has little effect on the flow of a river so long as it
remains unfrozen; but the effect of temperature on the motion of ice is most
important. In many cases, indeed, the temperature, together with the water
that is incidental to it, seems to be the chief factor in determining the rate of
movement. The way in which its effects are felt will be discussed later.
Likenesses and unlikenesses of glaciers and rivers.—Many of the
characteristics of a valley glacier may be understood from the study of the
accompanying figure (Fig. 237) of the White (Alaska) glacier. From this
figure it will be seen that the glacier is an elongate river-like body,
following the curves of the valley in stream-like fashion. It has its origin in
the snows collected on the mountain heights seen in the distance, and it
works its way down the valley in a manner which, in the aggregate, is
similar to the movement of a stiff liquid. The likeness to a river extends to
many details. Not only does the center move faster than the sides, and the
upper part faster than the bottom, as in the case of streams, but the
movement is more rapid in constricted portions of the valley and slower in
the broader parts. These and other likenesses, some of which are apparent
rather than real, have given origin to the view that glacier ice moves like a
stiff viscous liquid.
Page 318
Fig. 237.—White glacier (central background) joining a larger glacier (foreground), Alaska.
(Reid.)
But while the points of likeness between glaciers and rivers are several,
their differences are at least equally numerous and significant. The trains of
débris on the surface (the dark bands in the illustration), like the central
currents of streams, pass nearer the projecting points of the valley walls and
farther from the receding bends; but beyond this point the analogy fails, for
the trains of débris on the ice do not conform in detail to the courses of the
currents of a winding stream, nor is there evidence of the rotatory motion
that characterizes river water. Furthermore, the glacier is readily fractured,
as the numerous gaping crevices on many glaciers show. The crevasses are
sometimes longitudinal, sometimes transverse, and sometimes oblique. In
the case of Arctic glaciers, longitudinal crevassing is especially
conspicuous.
(Reid.)
But while the points of likeness between glaciers and rivers are several,
their differences are at least equally numerous and significant. The trains of
débris on the surface (the dark bands in the illustration), like the central
currents of streams, pass nearer the projecting points of the valley walls and
farther from the receding bends; but beyond this point the analogy fails, for
the trains of débris on the ice do not conform in detail to the courses of the
currents of a winding stream, nor is there evidence of the rotatory motion
that characterizes river water. Furthermore, the glacier is readily fractured,
as the numerous gaping crevices on many glaciers show. The crevasses are
sometimes longitudinal, sometimes transverse, and sometimes oblique. In
the case of Arctic glaciers, longitudinal crevassing is especially
conspicuous.
Page 319
Fig. 238.—Cracking of glacier due to change in grade of bed. A North Greenland glacier
overriding a mound of moraine-stuff.
Crevasses appear to be developed wherever there is appreciable tension,
and the causes of this tension are many. An obvious cause is an abrupt
increase of gradient in the bed (Fig. 238). If the change of gradient be
considerable, an ice-fall or cascade results, and the ice may be greatly riven
(Fig. 228). Below the cascade, the surface may bristle with wedges and
pinnacles of ice (séracs, Fig. 239). Transverse crevices at the margin
sometimes appear to be the result of the tension developed on a curve.
Oblique crevices on the surface near the sides are commonly ascribed to the
tension between the faster-moving center and the slower-moving margins,
and in like manner crevasses that rise obliquely from the bottoms are
attributed to the tension between the faster-moving portions above and the
slower-moving portions below. All these crevasses indicate strains to which
a liquid, whose pressures are equal in all directions, does not offer a close
analogy. Longitudinal crevasses may affect both the river-like part of a
glacier and its deploying end, and are the result of tension developed by
movement within the ice itself, to which, again, rivers offer no analogy.
overriding a mound of moraine-stuff.
Crevasses appear to be developed wherever there is appreciable tension,
and the causes of this tension are many. An obvious cause is an abrupt
increase of gradient in the bed (Fig. 238). If the change of gradient be
considerable, an ice-fall or cascade results, and the ice may be greatly riven
(Fig. 228). Below the cascade, the surface may bristle with wedges and
pinnacles of ice (séracs, Fig. 239). Transverse crevices at the margin
sometimes appear to be the result of the tension developed on a curve.
Oblique crevices on the surface near the sides are commonly ascribed to the
tension between the faster-moving center and the slower-moving margins,
and in like manner crevasses that rise obliquely from the bottoms are
attributed to the tension between the faster-moving portions above and the
slower-moving portions below. All these crevasses indicate strains to which
a liquid, whose pressures are equal in all directions, does not offer a close
analogy. Longitudinal crevasses may affect both the river-like part of a
glacier and its deploying end, and are the result of tension developed by
movement within the ice itself, to which, again, rivers offer no analogy.
Page 320
Somewhat similar cracks develop in the outer crust of asphalt, when a mass
of it is allowed to stand and spread; but in this case there is evaporation of
the volatile ingredients, giving to the outer part relative rigidity and
brittleness, while the inner part remains more fluent. The analogy is
therefore not perfect and probably not really illustrative. The crevices may
be narrow or wide, and both narrow and wide may be found in the same
glacier. The narrow crevices that never open much are the most significant,
as they show that very little stretching is needed to satisfy the tension. The
opening of a gaping crevice is sometimes the work of weeks, and, in the
slow-moving glaciers of high latitudes, sometimes the work of successive
seasons. All this shows that the glacier is a very brittle body, incapable of
resisting even very moderate strains brought to bear upon it very slowly.
Had the ice even moderate ductility, it would adapt itself to tension brought
to bear upon it so slowly as are many of the tensions which produce
crevassing. In its behavior under tension therefore a glacier is notably
unlike a river.
of it is allowed to stand and spread; but in this case there is evaporation of
the volatile ingredients, giving to the outer part relative rigidity and
brittleness, while the inner part remains more fluent. The analogy is
therefore not perfect and probably not really illustrative. The crevices may
be narrow or wide, and both narrow and wide may be found in the same
glacier. The narrow crevices that never open much are the most significant,
as they show that very little stretching is needed to satisfy the tension. The
opening of a gaping crevice is sometimes the work of weeks, and, in the
slow-moving glaciers of high latitudes, sometimes the work of successive
seasons. All this shows that the glacier is a very brittle body, incapable of
resisting even very moderate strains brought to bear upon it very slowly.
Had the ice even moderate ductility, it would adapt itself to tension brought
to bear upon it so slowly as are many of the tensions which produce
crevassing. In its behavior under tension therefore a glacier is notably
unlike a river.
Page 321
Fig. 239.—Séracs of glacier. (Reid.)
SURFACE FEATURES.
Topography.—Many of the minor irregularities of the surface of a
glacier are the result of crevassing. After the ice is crevassed, the sun’s rays
and the air which has been warmed by them penetrate the openings and
melt the ice. The melting is most rapid at the top, and decreases downward.
The result is that the sections of ice between adjacent crevasses are
narrowed into wedges. If there be cross-crevassing, as is common, points
instead of wedges result. As the sort of surface shown in Fig. 239 develops,
any débris which was on the ice slides into the crevices, and the upper
surface becomes clean.
Where ice is crevassed transversely, and where melting is not rapid, the
crevasses may close as the ice moves forward, and the regelation of
adjoining faces heals the rents in the surface. Even in this case, however,
SURFACE FEATURES.
Topography.—Many of the minor irregularities of the surface of a
glacier are the result of crevassing. After the ice is crevassed, the sun’s rays
and the air which has been warmed by them penetrate the openings and
melt the ice. The melting is most rapid at the top, and decreases downward.
The result is that the sections of ice between adjacent crevasses are
narrowed into wedges. If there be cross-crevassing, as is common, points
instead of wedges result. As the sort of surface shown in Fig. 239 develops,
any débris which was on the ice slides into the crevices, and the upper
surface becomes clean.
Where ice is crevassed transversely, and where melting is not rapid, the
crevasses may close as the ice moves forward, and the regelation of
adjoining faces heals the rents in the surface. Even in this case, however,
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the surface is likely to be more or less undulating because of the waste on
the sides of the crevices before they are closed. After regelation, surface
ablation tends to obliterate the protuberances.
The topography of the surface of the ice is affected by other conditions.
All parts of the surface of the ice are not equally compact, and the least
compact portions melt most rapidly, giving rise to depressions, while the
more solid parts occasion protuberances. Both depressions and
protuberances may be regular or irregular in form (Figs. 240 and 241).
Undulations of the bed often show themselves in the surface of the ice as
suggested by Fig. 242. In such cases, ponds or lakelets sometimes
accumulate on the surface of the ice. The topography of the ice in such
cases seems to show that the ice is forced up slope.
Surface moraines.—The surface of a glacier is often affected by débris
of one sort or another, and this also influences its topography. The débris is
sometimes disposed in the form of belts or moraines (Figs. 237, 243). The
surface moraines may be lateral, medial, or terminal. A lateral moraine is
any considerable accumulation of débris in a belt on the side of a glacier. A
medial moraine is a similar accumulation at some distance from the
margins, but not necessarily in or near the middle. There may be several
medial moraines on one glacier, in which case some of them may be far
from the center. In alpine glaciers, the surface terminal moraine is less well-
defined; in polar glaciers it often connects two lateral moraines, making a
loop roughly concentric with the terminus of the glacier.
the sides of the crevices before they are closed. After regelation, surface
ablation tends to obliterate the protuberances.
The topography of the surface of the ice is affected by other conditions.
All parts of the surface of the ice are not equally compact, and the least
compact portions melt most rapidly, giving rise to depressions, while the
more solid parts occasion protuberances. Both depressions and
protuberances may be regular or irregular in form (Figs. 240 and 241).
Undulations of the bed often show themselves in the surface of the ice as
suggested by Fig. 242. In such cases, ponds or lakelets sometimes
accumulate on the surface of the ice. The topography of the ice in such
cases seems to show that the ice is forced up slope.
Surface moraines.—The surface of a glacier is often affected by débris
of one sort or another, and this also influences its topography. The débris is
sometimes disposed in the form of belts or moraines (Figs. 237, 243). The
surface moraines may be lateral, medial, or terminal. A lateral moraine is
any considerable accumulation of débris in a belt on the side of a glacier. A
medial moraine is a similar accumulation at some distance from the
margins, but not necessarily in or near the middle. There may be several
medial moraines on one glacier, in which case some of them may be far
from the center. In alpine glaciers, the surface terminal moraine is less well-
defined; in polar glaciers it often connects two lateral moraines, making a
loop roughly concentric with the terminus of the glacier.
Page 323
Fig. 240.—End of Mount Dana glacier, Cal. Shows irregularities of surface due to
crevassing farther up the glacier, and to unequal melting.
Fig. 241.—Shows irregularities due to unequal melting of veined ice. End of small glacier
south of Forno hut, Engadine, Switzerland. (Reid.)
crevassing farther up the glacier, and to unequal melting.
Fig. 241.—Shows irregularities due to unequal melting of veined ice. End of small glacier
south of Forno hut, Engadine, Switzerland. (Reid.)
Page 324
Besides the surface moraines, which represent belted aggregations of
débris, there may be scattered bowlders and bits of rock of various sizes on
the ice, and, in addition to the coarse material, there is often some dust
which has been blown upon the ice.
Relief due to surface débris.—The débris on the ice affects its
topography by influencing the melting of the subjacent and adjacent ice.
The rock débris absorbs heat more readily than the ice. A small and thin
piece of stone lying on the ice is warmed through by the sun’s rays, and,
melting the ice beneath, sinks, just as a piece of black cloth on snow will
sink because of the increased melting beneath it. Though a good absorber of
heat, rock is a poor conductor, and so the lower surface of a large mass of
stone is not notably warmed. The ice beneath it is protected from the direct
rays of the sun, and is therefore melted more slowly than that around it. The
result is that the bowlder presently stands on a protuberance of ice (Fig.
244). When its pedestal becomes high, the oblique rays of the sun and the
warm air surrounding it cause it to waste away, and the capping bowlder
falls. In high latitudes, the great obliquity of the rays sometimes allows
them to strike under isolated bowlders. In this case, they are warmed from
below, and thus aid rather than hinder the melting of the ice.
Fig. 242.—Irregular surface due to uneven bottom. Bowdoin glacier, Inglefield Gulf, North
Greenland. The dark patches near the left margin of the glacier are lakelets in basins
produced by the upward bending of the ice as it overrides an elevation in its bed. The
figure also shows a depressed medial moraine.
The same principles apply to the moraines. A thin bowlder moraine in
high latitudes is sometimes sunk below the surface (Fig. 242). Usually,
however, a medial moraine protects the ice beneath from melting, and
débris, there may be scattered bowlders and bits of rock of various sizes on
the ice, and, in addition to the coarse material, there is often some dust
which has been blown upon the ice.
Relief due to surface débris.—The débris on the ice affects its
topography by influencing the melting of the subjacent and adjacent ice.
The rock débris absorbs heat more readily than the ice. A small and thin
piece of stone lying on the ice is warmed through by the sun’s rays, and,
melting the ice beneath, sinks, just as a piece of black cloth on snow will
sink because of the increased melting beneath it. Though a good absorber of
heat, rock is a poor conductor, and so the lower surface of a large mass of
stone is not notably warmed. The ice beneath it is protected from the direct
rays of the sun, and is therefore melted more slowly than that around it. The
result is that the bowlder presently stands on a protuberance of ice (Fig.
244). When its pedestal becomes high, the oblique rays of the sun and the
warm air surrounding it cause it to waste away, and the capping bowlder
falls. In high latitudes, the great obliquity of the rays sometimes allows
them to strike under isolated bowlders. In this case, they are warmed from
below, and thus aid rather than hinder the melting of the ice.
Fig. 242.—Irregular surface due to uneven bottom. Bowdoin glacier, Inglefield Gulf, North
Greenland. The dark patches near the left margin of the glacier are lakelets in basins
produced by the upward bending of the ice as it overrides an elevation in its bed. The
figure also shows a depressed medial moraine.
The same principles apply to the moraines. A thin bowlder moraine in
high latitudes is sometimes sunk below the surface (Fig. 242). Usually,
however, a medial moraine protects the ice beneath from melting, and
Page 325
occasions the development of a ridge of ice beneath itself. As the ice on
either side is then lowered by ablation, the moraine matter of the medial
belt tends to slide down on either hand. The same is true of the lateral
moraines. So far does this spreading go, that in some cases the lower end of
a glacier is completely covered with the débris which has spread from the
medial and lateral moraines. Examples of this may be seen in almost any
region of abundant, long, alpine glaciers.
Fig. 243.—A Swiss glacier, showing surface moraines, characteristic profile, etc.
Dust-wells.—The wind-blown dust sometimes gives rise to peculiar
topographic features of small size. The dust is not distributed by the wind
with absolute equality, and the surface drainage of the ice tends to aggregate
it. Every dust particle acts like a small stone, and where aggregations of
dust occur, they melt their way down into the ice, developing holes or
“dust-wells” (Fig. 245). These wells rarely reach a depth of more than a few
inches, but they may be so numerous that the pedestrian is obliged to watch
his steps. This is especially true near the edge of the large ice-caps. It is
either side is then lowered by ablation, the moraine matter of the medial
belt tends to slide down on either hand. The same is true of the lateral
moraines. So far does this spreading go, that in some cases the lower end of
a glacier is completely covered with the débris which has spread from the
medial and lateral moraines. Examples of this may be seen in almost any
region of abundant, long, alpine glaciers.
Fig. 243.—A Swiss glacier, showing surface moraines, characteristic profile, etc.
Dust-wells.—The wind-blown dust sometimes gives rise to peculiar
topographic features of small size. The dust is not distributed by the wind
with absolute equality, and the surface drainage of the ice tends to aggregate
it. Every dust particle acts like a small stone, and where aggregations of
dust occur, they melt their way down into the ice, developing holes or
“dust-wells” (Fig. 245). These wells rarely reach a depth of more than a few
inches, but they may be so numerous that the pedestrian is obliged to watch
his steps. This is especially true near the edge of the large ice-caps. It is
Page 326
evident that the depth of these dust wells must be slight, for so soon as they
are deep enough to cut off the sun’s rays from the dust at the bottom, the
deepening ceases. Other things being equal, they are deeper in low latitudes
than in high.
Fig. 244.—Bowlder on ice pinnacle. Forno glacier, Switzerland. (Reid.)
are deep enough to cut off the sun’s rays from the dust at the bottom, the
deepening ceases. Other things being equal, they are deeper in low latitudes
than in high.
Fig. 244.—Bowlder on ice pinnacle. Forno glacier, Switzerland. (Reid.)
Page 327
Fig. 245.—Dust-wells. Igloodahomyne glacier, North Greenland.
Fig. 246.—Disposition of débris in ice. North Greenland glacier. (Libbey.)
Fig. 246.—Disposition of débris in ice. North Greenland glacier. (Libbey.)
Page 328
Débris below the surface.—
The lower part of a glacier, as well
as the upper, carries rock débris.
This débris is sometimes so
abundant, especially near the ends
and edges of the ice, that it is
difficult to locate the bottom of
the glacier; for between the
moving ice which is full of débris,
and the stationary débris which is
full of ice, there seems to be a
nearly complete gradation. The
débris in the lower part of arctic
glaciers, and to some extent of
others, is often disposed in thin
sheets sandwiched in between
layers of clean ice. These débris
sheets are often numerous and
usually discontinuous, though
groups of such sheets often persist
for considerable distances. Débris
also occurs to some extent in the
ice well above its base. It is
sometimes in belts, as seen in
section, and sometimes in
bunches. These various relations
are illustrated by Figs. 227, 229,
Fig. 247.—Profile of the lower part of the
and 246–249. lateral margin of a glacier. Southeast side of
McCormick Bay, North Greenland.
Another characteristic of the
basal débris-laden part of some glaciers is the foliation of the ice (Figs. 248,
249, etc.). This is especially well shown in the arctic glaciers, the ends and
sides of which have steep or vertical faces. The foliation is best developed
in the débris zone, though often shown above. The foliation is sometimes
minute, consisting of layers of clean ice, an inch or less in thickness,
separated by mere films of earthy matter. In extreme cases there are a score
or more of laminæ within a foot. Locally, and especially where débris is
The lower part of a glacier, as well
as the upper, carries rock débris.
This débris is sometimes so
abundant, especially near the ends
and edges of the ice, that it is
difficult to locate the bottom of
the glacier; for between the
moving ice which is full of débris,
and the stationary débris which is
full of ice, there seems to be a
nearly complete gradation. The
débris in the lower part of arctic
glaciers, and to some extent of
others, is often disposed in thin
sheets sandwiched in between
layers of clean ice. These débris
sheets are often numerous and
usually discontinuous, though
groups of such sheets often persist
for considerable distances. Débris
also occurs to some extent in the
ice well above its base. It is
sometimes in belts, as seen in
section, and sometimes in
bunches. These various relations
are illustrated by Figs. 227, 229,
Fig. 247.—Profile of the lower part of the
and 246–249. lateral margin of a glacier. Southeast side of
McCormick Bay, North Greenland.
Another characteristic of the
basal débris-laden part of some glaciers is the foliation of the ice (Figs. 248,
249, etc.). This is especially well shown in the arctic glaciers, the ends and
sides of which have steep or vertical faces. The foliation is best developed
in the débris zone, though often shown above. The foliation is sometimes
minute, consisting of layers of clean ice, an inch or less in thickness,
separated by mere films of earthy matter. In extreme cases there are a score
or more of laminæ within a foot. Locally, and especially where débris is
Page 329
abundant, the laminæ are much contorted. This is seen both in section (Figs.
248 and 249) and on the surface (Fig. 250).
TEMPERATURE, WASTE, AND DRAINAGE.
The temperature of glacier ice may range downward from the freezing
point of water much as other solid portions of the earth’s surface, but it has
a fixed upper limit at 32° Fahr. (0° C.) because all the heat it receives
tending to raise its temperature above that point, is converted into the latent
form by the melting of the ice. The range of temperature is greatest at the
surface, where it varies from 32° in the summer, to the coldest temperature
of the region where the ice occurs. Beneath the surface the range of
temperature is more restricted, and increasingly so with increasing depth.
Fig. 248.—Side view of end of glacier. Southeast side of McCormick Bay, North Greenland.
Shows structure of ice as well as position of débris.
248 and 249) and on the surface (Fig. 250).
TEMPERATURE, WASTE, AND DRAINAGE.
The temperature of glacier ice may range downward from the freezing
point of water much as other solid portions of the earth’s surface, but it has
a fixed upper limit at 32° Fahr. (0° C.) because all the heat it receives
tending to raise its temperature above that point, is converted into the latent
form by the melting of the ice. The range of temperature is greatest at the
surface, where it varies from 32° in the summer, to the coldest temperature
of the region where the ice occurs. Beneath the surface the range of
temperature is more restricted, and increasingly so with increasing depth.
Fig. 248.—Side view of end of glacier. Southeast side of McCormick Bay, North Greenland.
Shows structure of ice as well as position of débris.
Page 330
The variation of temperature at the surface is due primarily to the varying
temperature of the air. During the cold season, a wave of low temperature
(the winter wave), starting at the surface, penetrates the ice, and during the
warm season a wave of higher temperature (the summer wave) takes the
same course. The day and night waves and other minor variables are, for
present purposes, negligible.
Fig. 249.—Side view of a North Greenland glacier (East glacier), showing position of débris
and structure of the ice.
The winter wave.—There are but few observations on the internal
temperatures of glaciers during the winter season, but it seems certain that
the winter wave diminishes rapidly downward and dies out below, much as
does the winter wave which affects land surfaces not covered with ice.
Conduction alone considered, the temperature of the ice where the cold
wave dies out, should correspond, approximately, to the mean annual
temperature of the air. During the cold season, a wave of low temperature
(the winter wave), starting at the surface, penetrates the ice, and during the
warm season a wave of higher temperature (the summer wave) takes the
same course. The day and night waves and other minor variables are, for
present purposes, negligible.
Fig. 249.—Side view of a North Greenland glacier (East glacier), showing position of débris
and structure of the ice.
The winter wave.—There are but few observations on the internal
temperatures of glaciers during the winter season, but it seems certain that
the winter wave diminishes rapidly downward and dies out below, much as
does the winter wave which affects land surfaces not covered with ice.
Conduction alone considered, the temperature of the ice where the cold
wave dies out, should correspond, approximately, to the mean annual
Page 331
temperature of the region, provided that temperature is below the melting
point of ice.
Assuming that in the high altitudes and high latitudes where glaciers
abound, the temperature of the surface may average about −12° Fahr. (about
−25° C.) for the winter half of the year, which is about the case for north
Greenland, Spitzbergen, and Franz Josef Land, and that the conductivity of
the ice in the C. G. S.[130] system is .005, the temperature would be lowered
appreciably only about 40 feet below the surface at the close of the winter
period, conduction only being considered. How far the internal temperature
may be influenced by air forced through the ice by winds and by variations
of the barometer is not known and cannot well be estimated. The wave of
low temperature descending from the surface in winter would probably
become inappreciable before reaching a depth of 60 feet. At this depth the
temperature should be about 15° Fahr.—the mean annual temperature of the
region.
point of ice.
Assuming that in the high altitudes and high latitudes where glaciers
abound, the temperature of the surface may average about −12° Fahr. (about
−25° C.) for the winter half of the year, which is about the case for north
Greenland, Spitzbergen, and Franz Josef Land, and that the conductivity of
the ice in the C. G. S.[130] system is .005, the temperature would be lowered
appreciably only about 40 feet below the surface at the close of the winter
period, conduction only being considered. How far the internal temperature
may be influenced by air forced through the ice by winds and by variations
of the barometer is not known and cannot well be estimated. The wave of
low temperature descending from the surface in winter would probably
become inappreciable before reaching a depth of 60 feet. At this depth the
temperature should be about 15° Fahr.—the mean annual temperature of the
region.
Page 332
Fig. 250.—Contorted lamination shown at the surface. A small glacier south of Forno hut,
Engadine, Switzerland. (Reid.)
The summer wave.—The warm wave follows the analogy of the
summer wave of ice-free land surfaces much less closely. This is because of
the low melting temperature of ice as compared with other forms of solid
earth-matter. On this account the summer wave is bi-fold. The one part
travels downward by conduction, the other by the descent of water; the one
has to do primarily with the temperature before the melting-point of ice is
reached; the other, with the temperature after that point is reached; the first
conforms measurably to the warm wave affecting other solid earth-matter,
while the second is governed by special laws. After the surface portion of
the ice is brought to the melting temperature, the additional heat which it
receives melts the ice and is transformed from sensible into potential heat.
Ice charged with water is potentially, but not sensibly, warmer than ice
which has just reached the melting temperature.
Engadine, Switzerland. (Reid.)
The summer wave.—The warm wave follows the analogy of the
summer wave of ice-free land surfaces much less closely. This is because of
the low melting temperature of ice as compared with other forms of solid
earth-matter. On this account the summer wave is bi-fold. The one part
travels downward by conduction, the other by the descent of water; the one
has to do primarily with the temperature before the melting-point of ice is
reached; the other, with the temperature after that point is reached; the first
conforms measurably to the warm wave affecting other solid earth-matter,
while the second is governed by special laws. After the surface portion of
the ice is brought to the melting temperature, the additional heat which it
receives melts the ice and is transformed from sensible into potential heat.
Ice charged with water is potentially, but not sensibly, warmer than ice
which has just reached the melting temperature.
Page 333
The warm wave of conduction dies out below like the cold wave. The
warm wave descending by the flow of water stops where the freezing
temperature of water is reached. In regions where the average temperature
is below freezing, the water-wave does not descend so far as the wave of
conduction, since the latter descends below the zone where the melting
temperature is found.
The foregoing considerations warrant the generalization that glaciers
normally consist of two zones (1) an outer or upper zone of fluctuating
temperature, and (2) an under zone of nearly constant temperature. The
under zone obviously does not exist where the thickness of the ice is less
than the thickness of the zone of fluctuating temperature. This may be the
case in very thin glaciers in very cold regions, and in the thin ends and
edges of all glaciers.
The temperature of the bottom.—The internal heat of the earth is
slowly conducted to the base of a glacier where it melts the ice at the
estimated average rate of about one-fourth of an inch per year. The
temperature of melting is a little below 32° Fahr. since pressure lowers the
melting-point at the rate of .0133° Fahr. (.0075° C.) for one atmosphere of
pressure. At the bottom of a mile of ice therefore the melting temperature is
about 30.2° Fahr. (−1° C.) It is probable that in all thick glaciers the
temperature of the bottom is constantly maintained at the melting-point.
This may be indicated by the streams which issue from beneath glaciers
during the winter, though this criterion is hardly decisive since the issuing
waters may be derived partly or wholly from the rock beneath. In glaciers
or in parts of glaciers so thin as to lie wholly within the zone of fluctuating
temperature, the temperature of the bottom is obviously not constant.
Temperature of the interior of the ice.—The variation of temperature
of the surface of a glacier has already been shown to lie between a
maximum of 32° Fahr. and the minimum temperature of the region where
the glacier occurs. Lower, in the zone of fluctuating temperature, the
variation is less, and where the zone of fluctuating temperature passes into
the zone of constant temperature, variation ceases. The thickness of the
zone of fluctuating temperature varies with the temperature of the region
where the glacier occurs, being greatest where the winters are coldest. In
the case of all glaciers except thin ones in very cold regions, the
temperatures within the zone of constant temperature range from the mean
warm wave descending by the flow of water stops where the freezing
temperature of water is reached. In regions where the average temperature
is below freezing, the water-wave does not descend so far as the wave of
conduction, since the latter descends below the zone where the melting
temperature is found.
The foregoing considerations warrant the generalization that glaciers
normally consist of two zones (1) an outer or upper zone of fluctuating
temperature, and (2) an under zone of nearly constant temperature. The
under zone obviously does not exist where the thickness of the ice is less
than the thickness of the zone of fluctuating temperature. This may be the
case in very thin glaciers in very cold regions, and in the thin ends and
edges of all glaciers.
The temperature of the bottom.—The internal heat of the earth is
slowly conducted to the base of a glacier where it melts the ice at the
estimated average rate of about one-fourth of an inch per year. The
temperature of melting is a little below 32° Fahr. since pressure lowers the
melting-point at the rate of .0133° Fahr. (.0075° C.) for one atmosphere of
pressure. At the bottom of a mile of ice therefore the melting temperature is
about 30.2° Fahr. (−1° C.) It is probable that in all thick glaciers the
temperature of the bottom is constantly maintained at the melting-point.
This may be indicated by the streams which issue from beneath glaciers
during the winter, though this criterion is hardly decisive since the issuing
waters may be derived partly or wholly from the rock beneath. In glaciers
or in parts of glaciers so thin as to lie wholly within the zone of fluctuating
temperature, the temperature of the bottom is obviously not constant.
Temperature of the interior of the ice.—The variation of temperature
of the surface of a glacier has already been shown to lie between a
maximum of 32° Fahr. and the minimum temperature of the region where
the glacier occurs. Lower, in the zone of fluctuating temperature, the
variation is less, and where the zone of fluctuating temperature passes into
the zone of constant temperature, variation ceases. The thickness of the
zone of fluctuating temperature varies with the temperature of the region
where the glacier occurs, being greatest where the winters are coldest. In
the case of all glaciers except thin ones in very cold regions, the
temperatures within the zone of constant temperature range from the mean
Page 334
annual temperature of the region at the top of the zone (provided this is not
above the melting-point of ice at this depth) to the melting temperature of
the ice at the bottom. Within these limits the range may be great or slight.
If we consider only the effects of the external seasonal temperatures and
the internal heat of the earth, it appears that all the ice in the zone of
constant temperature in the lower end of a typical alpine glacier should
have a constant melting temperature, for the average temperature of regions
where the ends of such glaciers occur is usually above 32° Fahr., and this
determines a temperature of 32° Fahr. (or a little less) at the top of the zone,
while a melting temperature is maintained at the bottom by the earth’s
interior heat. In thin glaciers of very cold regions, where the zone of
constant temperature has relatively slight thickness, the low temperature
descending from the surface may so far overcome the effect of internal heat
as to keep the bottom of the ice at a freezing temperature. In all other cases,
the ice at the bottom of the under zone has a melting temperature, while that
above is probably colder.
In the higher altitudes and in the polar latitudes where glaciers are chiefly
generated, the mean annual temperature of the surface is usually below the
melting-point of ice. Here the temperature of the ice between the top and
bottom of the zone of constant temperature must, on the average, be below
the melting-point, unless heat enough is generated in the interior of the ice
to offset the effect of the temperature above. For example, where the mean
annual temperature is 20° Fahr. or lower, as in middle Greenland,
Spitzbergen, and Franz Josef Land, and at certain high altitudes in more
southerly latitudes, the mean temperature in the zone of constant
temperature should range from 20° Fahr. at the top to 32° Fahr. (or a little
less) below; i.e., it should average about 6° below the melting-point. Under
these conditions, all the ice in the zone of constant temperature, except that
at its bottom, must be permanently below the melting-point, but it is
perhaps worthy of especial note that much of it is but little below. In alpine
glaciers the part of the ice affected by this constant low temperature (below
freezing) is presumed to be chiefly that which lies beneath the snow-fields.
In polar glaciers the low temperature probably prevails beneath the surface,
not only throughout the great ice-caps, but also in the marginal glaciers
which descend from them.
above the melting-point of ice at this depth) to the melting temperature of
the ice at the bottom. Within these limits the range may be great or slight.
If we consider only the effects of the external seasonal temperatures and
the internal heat of the earth, it appears that all the ice in the zone of
constant temperature in the lower end of a typical alpine glacier should
have a constant melting temperature, for the average temperature of regions
where the ends of such glaciers occur is usually above 32° Fahr., and this
determines a temperature of 32° Fahr. (or a little less) at the top of the zone,
while a melting temperature is maintained at the bottom by the earth’s
interior heat. In thin glaciers of very cold regions, where the zone of
constant temperature has relatively slight thickness, the low temperature
descending from the surface may so far overcome the effect of internal heat
as to keep the bottom of the ice at a freezing temperature. In all other cases,
the ice at the bottom of the under zone has a melting temperature, while that
above is probably colder.
In the higher altitudes and in the polar latitudes where glaciers are chiefly
generated, the mean annual temperature of the surface is usually below the
melting-point of ice. Here the temperature of the ice between the top and
bottom of the zone of constant temperature must, on the average, be below
the melting-point, unless heat enough is generated in the interior of the ice
to offset the effect of the temperature above. For example, where the mean
annual temperature is 20° Fahr. or lower, as in middle Greenland,
Spitzbergen, and Franz Josef Land, and at certain high altitudes in more
southerly latitudes, the mean temperature in the zone of constant
temperature should range from 20° Fahr. at the top to 32° Fahr. (or a little
less) below; i.e., it should average about 6° below the melting-point. Under
these conditions, all the ice in the zone of constant temperature, except that
at its bottom, must be permanently below the melting-point, but it is
perhaps worthy of especial note that much of it is but little below. In alpine
glaciers the part of the ice affected by this constant low temperature (below
freezing) is presumed to be chiefly that which lies beneath the snow-fields.
In polar glaciers the low temperature probably prevails beneath the surface,
not only throughout the great ice-caps, but also in the marginal glaciers
which descend from them.
Page 335
From these theoretical considerations we may deduce the generalization
that in the zone of constant temperature within the area of glacial growth,
the temperature of the ice is generally below the melting-point, while within
the area of wastage, the temperature of the corresponding zone is generally
at the melting-point.
Compression and friction as causes of heat.—The foregoing
conclusions are somewhat modified by dynamic sources of heat. The
compression arising from gravity, and the friction developed where there is
motion, are causes of heat. Since friction occurs only when motion takes
place, the heat which it generates is secondary and may, for present
purposes, be neglected. Compression not only lowers the melting-point
slightly, but it produces heat at the point of compression. Where the ice is
granular, the compression, due to weight, takes place at the contacts of the
grains. At intermediate points the pressure tends to cause them to bulge, and
this has the effect of lowering the temperature of the bulging points. If
therefore the compression be considerable, the granules may be warmed to
the melting-point where they press each other, while at other points their
temperature may be lower. In this case melting will take place at the points
of compression, and the moisture so produced will be transferred to the
adjacent parts of the granule and immediately refrozen. Melting at the
points of compression would result in some yielding of the mass, and in
some shifting of the pressure to new points where compression and melting
would again take place. Thus the melting, the refreezing, and the attendant
movement might go on until the limits of the power of gravity in this
direction were reached. From considerations already adduced, it appears
that the temperature in some parts of every considerable body of ice must
be such as to permit these changes. The heat due to depression and friction
may modify the theoretical deductions drawn above from atmospheric and
internal influences.
Summary.—If the foregoing generalizations be correct, (1) the surface
of a glacier is likely to be melted during the summer, (2) its immediate
bottom is slowly melting all the time (unless the thickness of the ice be less
than the thickness of the zone of annual variation or of permanent freezing
temperature); (3) its subsurface portion in the zone of waste is generally
melting, owing to descending water, compression, and friction; while (4) its
subsurface portion in the zone of growth is probably below the melting-
that in the zone of constant temperature within the area of glacial growth,
the temperature of the ice is generally below the melting-point, while within
the area of wastage, the temperature of the corresponding zone is generally
at the melting-point.
Compression and friction as causes of heat.—The foregoing
conclusions are somewhat modified by dynamic sources of heat. The
compression arising from gravity, and the friction developed where there is
motion, are causes of heat. Since friction occurs only when motion takes
place, the heat which it generates is secondary and may, for present
purposes, be neglected. Compression not only lowers the melting-point
slightly, but it produces heat at the point of compression. Where the ice is
granular, the compression, due to weight, takes place at the contacts of the
grains. At intermediate points the pressure tends to cause them to bulge, and
this has the effect of lowering the temperature of the bulging points. If
therefore the compression be considerable, the granules may be warmed to
the melting-point where they press each other, while at other points their
temperature may be lower. In this case melting will take place at the points
of compression, and the moisture so produced will be transferred to the
adjacent parts of the granule and immediately refrozen. Melting at the
points of compression would result in some yielding of the mass, and in
some shifting of the pressure to new points where compression and melting
would again take place. Thus the melting, the refreezing, and the attendant
movement might go on until the limits of the power of gravity in this
direction were reached. From considerations already adduced, it appears
that the temperature in some parts of every considerable body of ice must
be such as to permit these changes. The heat due to depression and friction
may modify the theoretical deductions drawn above from atmospheric and
internal influences.
Summary.—If the foregoing generalizations be correct, (1) the surface
of a glacier is likely to be melted during the summer, (2) its immediate
bottom is slowly melting all the time (unless the thickness of the ice be less
than the thickness of the zone of annual variation or of permanent freezing
temperature); (3) its subsurface portion in the zone of waste is generally
melting, owing to descending water, compression, and friction; while (4) its
subsurface portion in the zone of growth is probably below the melting-
Page 336
point except as locally brought to that temperature by compression, friction,
and descending water, and at the bottom by conduction from the rock
beneath.
Movement under low temperature.—Glacier motion will not be
discussed at this point, but one of the bearings of the preceding conclusions
on glacier motion may be pointed out. Since there must be motion in the
area of growth to supply the loss in the area of waste, the fundamental cause
of motion must be operative in bodies of ice the mean temperature of which
is below the melting-point, unless the dynamic sources of heat are
considerable. This fundamental cause does not exclude the coöperation of
causes that work only (1) at the melting temperature, or (2) where the ice is
bathed with water, or (3) in the plane of contact between wet ice above and
dry ice below. These may be auxiliary causes which abet the fundamental
one in producing the more rapid movement of warm seasons, or in bringing
about the especially rapid movement in situations where there is abundant
water, or in inducing the shearing which is such a remarkable feature of
arctic glaciers.
Evaporation.—The ice wastes by evaporation as well as by melting, and
while the former process is far less important than the latter, its results are
probably larger than is commonly apprehended. One of the most
remarkable features of some of the deposits of ancient glaciers is the slight
evidence they afford of escaping waters. The most plausible explanation
seems to lie in the supposition that the ice was largely wasted by
evaporation. This conclusion finds support in many places in the presence
of a mantle of fine silt over the drift, the silt being apparently composed of
dust blown upon the ice. It is supposed to imply aridity in the region about
the ice. If a sufficient mantle of dust were spread over the border zone of
the ice, and if the air were very dry, nearly all the water melted on the
surface of the ice might be held back by the dust-wells until the water was
evaporated or absorbed.
and descending water, and at the bottom by conduction from the rock
beneath.
Movement under low temperature.—Glacier motion will not be
discussed at this point, but one of the bearings of the preceding conclusions
on glacier motion may be pointed out. Since there must be motion in the
area of growth to supply the loss in the area of waste, the fundamental cause
of motion must be operative in bodies of ice the mean temperature of which
is below the melting-point, unless the dynamic sources of heat are
considerable. This fundamental cause does not exclude the coöperation of
causes that work only (1) at the melting temperature, or (2) where the ice is
bathed with water, or (3) in the plane of contact between wet ice above and
dry ice below. These may be auxiliary causes which abet the fundamental
one in producing the more rapid movement of warm seasons, or in bringing
about the especially rapid movement in situations where there is abundant
water, or in inducing the shearing which is such a remarkable feature of
arctic glaciers.
Evaporation.—The ice wastes by evaporation as well as by melting, and
while the former process is far less important than the latter, its results are
probably larger than is commonly apprehended. One of the most
remarkable features of some of the deposits of ancient glaciers is the slight
evidence they afford of escaping waters. The most plausible explanation
seems to lie in the supposition that the ice was largely wasted by
evaporation. This conclusion finds support in many places in the presence
of a mantle of fine silt over the drift, the silt being apparently composed of
dust blown upon the ice. It is supposed to imply aridity in the region about
the ice. If a sufficient mantle of dust were spread over the border zone of
the ice, and if the air were very dry, nearly all the water melted on the
surface of the ice might be held back by the dust-wells until the water was
evaporated or absorbed.
Page 337
Fig. 251.—Spouting stream. Glacier south side of Olriks Bay, North Greenland.
Drainage.—Some of the water produced by surface melting forms little
streams on the ice. Sooner or later they plunge into crevasses or over the
sides and ends of the glacier. In the former case, they may melt or wear out
well-like passages (moulins) in the ice, and even in the rock beneath. Much
of the surface water sinks into the ice. Its ready penetration is aided by the
“dust-wells” which mark the surface of many glaciers. In north Greenland
wells which contain six or eight inches of water at the end of a warm day
are often dry in the morning. The water has leaked out and passed to lower
levels. From these and other harmonious observations it is inferred that the
superficial part of a glacier at least is readily penetrated by water. The depth
to which surface water penetrates is undetermined, but it doubtless varies
greatly, not only in different glaciers, but in different parts of the same
glacier, and in the same part at different times. Above the line of perennial
snow there is little water either from melting or from rain, and hence
relatively slight penetration. Below the line of perennial snow there is much
melting and much rain, and here it is probable that the water sometimes,
Drainage.—Some of the water produced by surface melting forms little
streams on the ice. Sooner or later they plunge into crevasses or over the
sides and ends of the glacier. In the former case, they may melt or wear out
well-like passages (moulins) in the ice, and even in the rock beneath. Much
of the surface water sinks into the ice. Its ready penetration is aided by the
“dust-wells” which mark the surface of many glaciers. In north Greenland
wells which contain six or eight inches of water at the end of a warm day
are often dry in the morning. The water has leaked out and passed to lower
levels. From these and other harmonious observations it is inferred that the
superficial part of a glacier at least is readily penetrated by water. The depth
to which surface water penetrates is undetermined, but it doubtless varies
greatly, not only in different glaciers, but in different parts of the same
glacier, and in the same part at different times. Above the line of perennial
snow there is little water either from melting or from rain, and hence
relatively slight penetration. Below the line of perennial snow there is much
melting and much rain, and here it is probable that the water sometimes,
Page 338
perhaps usually, penetrates to the bottom of the ice during the melting
season, even independently of crevasses.
Once within the glacier, the course of the water is variable. Exceptionally
it follows definite englacial channels, as shown by springs or streams
issuing from the ice at some point above its bottom (Fig. 251). Oftener it
descends or moves forward through the irregular openings which the
accidents of motion have developed. If it reaches a level where the
temperature is below its freezing-point, it congeals. Otherwise it remains in
cavities or descends to the bottom. The water produced by melting within
the glacier probably follows a similar course. So far as these waters descend
to the bottom, they join those produced by basal melting and issue from the
glacier with them. In alpine glaciers the waters beneath the ice often unite
in a common stream in the axis of the valley, and hollow out a tunnel. Thus
the Rhone is already a considerable stream where it issues from beneath the
Rhone glacier. In the glaciers of high latitudes, subglacial tunnels are less
common and the drainage is in streams along the sides of the glaciers or
through the débris beneath and about them.
At the end of the glacier, all waters, whether they have been superglacial,
englacial or subglacial, unite to bear away the silt, sand, gravel, and even
small bowlders set free from the ice, and to spread them in belts along the
border of the ice or in trains stretching down the valleys below. These are
the most common of the glacio-fluvial deposits.
THE WORK OF GLACIERS.
Erosion and transportation.
The work accomplished by glaciers is distinctive, for while like rivers,
they abrade the valleys through which they pass, carry forward the material
which they remove from the surface, and wear, grind, and ultimately
deposit it, and while their work therefore includes erosion, transportation,
and deposition, their method is peculiar.
Getting load.—If the surface on which the snow-field which is to
become a glacier accumulates be rough and covered with abundant rock
débris, as such surfaces usually are, the glacier already has a basal load
when its movement begins, for the snow covers, surrounds, and includes
season, even independently of crevasses.
Once within the glacier, the course of the water is variable. Exceptionally
it follows definite englacial channels, as shown by springs or streams
issuing from the ice at some point above its bottom (Fig. 251). Oftener it
descends or moves forward through the irregular openings which the
accidents of motion have developed. If it reaches a level where the
temperature is below its freezing-point, it congeals. Otherwise it remains in
cavities or descends to the bottom. The water produced by melting within
the glacier probably follows a similar course. So far as these waters descend
to the bottom, they join those produced by basal melting and issue from the
glacier with them. In alpine glaciers the waters beneath the ice often unite
in a common stream in the axis of the valley, and hollow out a tunnel. Thus
the Rhone is already a considerable stream where it issues from beneath the
Rhone glacier. In the glaciers of high latitudes, subglacial tunnels are less
common and the drainage is in streams along the sides of the glaciers or
through the débris beneath and about them.
At the end of the glacier, all waters, whether they have been superglacial,
englacial or subglacial, unite to bear away the silt, sand, gravel, and even
small bowlders set free from the ice, and to spread them in belts along the
border of the ice or in trains stretching down the valleys below. These are
the most common of the glacio-fluvial deposits.
THE WORK OF GLACIERS.
Erosion and transportation.
The work accomplished by glaciers is distinctive, for while like rivers,
they abrade the valleys through which they pass, carry forward the material
which they remove from the surface, and wear, grind, and ultimately
deposit it, and while their work therefore includes erosion, transportation,
and deposition, their method is peculiar.
Getting load.—If the surface on which the snow-field which is to
become a glacier accumulates be rough and covered with abundant rock
débris, as such surfaces usually are, the glacier already has a basal load
when its movement begins, for the snow covers, surrounds, and includes
Page 339
such loose blocks of rock as project above the general surface and envelops
all projecting points of rock within its field. When the snow becomes ice
and the ice begins to move, it carries forward the loose rock already
imbedded in it, and tears off the weak points of the enveloped rock-
projections. It may perhaps also move some of the soil and mantle rock of
the original surface to which it is frozen. In addition to the subglacial load
which the glacier thus has at the outset, there may be a surface load which
has fallen on the snow or ice from cliffs above. This is especially true of
mountain-valley glaciers. If this has been buried by snow and ice it is
englacial; if it lies on the surface it is superglacial.
Once in movement, the ice carries away the débris to which it was
originally attached, and at the same time gathers new load from the same
area. The new load is acquired partly by the rasping effect of the rock-shod
ice on its bed, and partly by its rending power which, under favorable
circumstances, may quarry out considerable blocks of rock. This “plucking”
process is at its best where the ice passes over cliffs of jointed rock or steep-
sloped hills.
As the ice advances into new territory it acquires additional basal load,
partly by rasping, partly by plucking, partly by freezing to it, and partly in
other ways. One of these ways may be illustrated by the sequence of events
when the end of a glacier advances on a very large bowlder. As the ice
approaches it, the reflection of heat from it melts the adjacent edge of the
ice, making a slight reëntrant. With farther advance, the ice closes in against
and around the bowlder, and finally carries it along in the bottom of the
moving mass. In some cases, especially when its advance is rapid, the ice
may push débris in front of itself. Even where this is the case, the amount of
material pushed forward is generally slight, partly because the extreme edge
of the ice often fails to rest on the land in summer, when the movement is
greatest, being melted from below by the heat of the surface over which it is
spreading (see Fig. 252), and partly because the earth in front of the glacier
is frozen during a large part of the year. In this condition, the earthy matter
has greater resistance than the ice, and the latter rides over it. Superglacial
material may be acquired during movement by the fall of débris from cliffs,
or by the descent of avalanches.
Conditions influencing rate of erosion.—An obstructive attitude of the
surface toward the movement of the ice is as necessary for effective erosion
all projecting points of rock within its field. When the snow becomes ice
and the ice begins to move, it carries forward the loose rock already
imbedded in it, and tears off the weak points of the enveloped rock-
projections. It may perhaps also move some of the soil and mantle rock of
the original surface to which it is frozen. In addition to the subglacial load
which the glacier thus has at the outset, there may be a surface load which
has fallen on the snow or ice from cliffs above. This is especially true of
mountain-valley glaciers. If this has been buried by snow and ice it is
englacial; if it lies on the surface it is superglacial.
Once in movement, the ice carries away the débris to which it was
originally attached, and at the same time gathers new load from the same
area. The new load is acquired partly by the rasping effect of the rock-shod
ice on its bed, and partly by its rending power which, under favorable
circumstances, may quarry out considerable blocks of rock. This “plucking”
process is at its best where the ice passes over cliffs of jointed rock or steep-
sloped hills.
As the ice advances into new territory it acquires additional basal load,
partly by rasping, partly by plucking, partly by freezing to it, and partly in
other ways. One of these ways may be illustrated by the sequence of events
when the end of a glacier advances on a very large bowlder. As the ice
approaches it, the reflection of heat from it melts the adjacent edge of the
ice, making a slight reëntrant. With farther advance, the ice closes in against
and around the bowlder, and finally carries it along in the bottom of the
moving mass. In some cases, especially when its advance is rapid, the ice
may push débris in front of itself. Even where this is the case, the amount of
material pushed forward is generally slight, partly because the extreme edge
of the ice often fails to rest on the land in summer, when the movement is
greatest, being melted from below by the heat of the surface over which it is
spreading (see Fig. 252), and partly because the earth in front of the glacier
is frozen during a large part of the year. In this condition, the earthy matter
has greater resistance than the ice, and the latter rides over it. Superglacial
material may be acquired during movement by the fall of débris from cliffs,
or by the descent of avalanches.
Conditions influencing rate of erosion.—An obstructive attitude of the
surface toward the movement of the ice is as necessary for effective erosion
Page 340
as the movement of the ice itself.
Advancing over a flat surface, ice
ordinarily inflicts but little wear,
since there is little for it to get
hold of. So slight is the abrasive
power of ice under these
conditions that it frequently
overrides and buries the soil with
more or less of its herbaceous Figthe . 252.—Diagram showing lack of contact of
edge of the ice with its bed.
vegetation. But while a certain
measure of roughness of surface is favorable for glacial erosion, the
topography may be so uneven as to seriously impede the ice. Erosion is
probably at its maximum, so far as influenced by topography, when the
roughness of the surface is such as to offer notable catchment for the basal
ice, but not such as to impede its motion very seriously. The amount of
relief favorable for the greatest erosion increases with increasing thickness
of the ice.
Other conditions which influence erosion by ice are (1) the amount of
loose or slightly attached débris on the surface, (2) the resistance of the
rock, (3) the slope of the surface, (4) the thickness of the ice, (5) the rate of
movement, and (6) the abundance and character of the débris which the ice
has to work with. The effect of the first five of these conditions is evident.
The effect of the last is less simple. Clean ice passing over a smooth surface
of solid rock has little effect upon it; but a rock-shod glacier will abrade the
same surface notably. The effect of this abrasion is shown in the grooves
and scratches (striæ) which the stones in the bottom of the ice inflict on the
surface of the rock over which they pass (Figs. 253, 255, and 256). At the
same time the stones in the ice are themselves worn both by abrasion with
the bottom, and with one another (Fig. 254). It does not follow, however,
that the more material in the bottom of the ice the greater the erosion it
effects; for with increase of débris there may be decrease of motion[131] and,
beyond a certain point, the decrease of motion seriously interferes with the
efficiency of erosion. When any considerable thickness of ice at the bottom
of the glacier is full of débris, this loaded basal portion may approach
stagnancy, and the lower limit of considerable movement may lie between
the loaded ice below and the relatively clean ice above. A moderate, but not
an excessive load of débris is, therefore, favorable for great erosion.
Advancing over a flat surface, ice
ordinarily inflicts but little wear,
since there is little for it to get
hold of. So slight is the abrasive
power of ice under these
conditions that it frequently
overrides and buries the soil with
more or less of its herbaceous Figthe . 252.—Diagram showing lack of contact of
edge of the ice with its bed.
vegetation. But while a certain
measure of roughness of surface is favorable for glacial erosion, the
topography may be so uneven as to seriously impede the ice. Erosion is
probably at its maximum, so far as influenced by topography, when the
roughness of the surface is such as to offer notable catchment for the basal
ice, but not such as to impede its motion very seriously. The amount of
relief favorable for the greatest erosion increases with increasing thickness
of the ice.
Other conditions which influence erosion by ice are (1) the amount of
loose or slightly attached débris on the surface, (2) the resistance of the
rock, (3) the slope of the surface, (4) the thickness of the ice, (5) the rate of
movement, and (6) the abundance and character of the débris which the ice
has to work with. The effect of the first five of these conditions is evident.
The effect of the last is less simple. Clean ice passing over a smooth surface
of solid rock has little effect upon it; but a rock-shod glacier will abrade the
same surface notably. The effect of this abrasion is shown in the grooves
and scratches (striæ) which the stones in the bottom of the ice inflict on the
surface of the rock over which they pass (Figs. 253, 255, and 256). At the
same time the stones in the ice are themselves worn both by abrasion with
the bottom, and with one another (Fig. 254). It does not follow, however,
that the more material in the bottom of the ice the greater the erosion it
effects; for with increase of débris there may be decrease of motion[131] and,
beyond a certain point, the decrease of motion seriously interferes with the
efficiency of erosion. When any considerable thickness of ice at the bottom
of the glacier is full of débris, this loaded basal portion may approach
stagnancy, and the lower limit of considerable movement may lie between
the loaded ice below and the relatively clean ice above. A moderate, but not
an excessive load of débris is, therefore, favorable for great erosion.
Page 341
Something depends, too, on the character of the load. Coarse, hard, and
angular débris is a more effective instrument of erosion than fine, soft, or
rounded material. The adverse influence of the overloading of the ice on its
motion has been likened to the stiffening of a viscous liquid by the addition
of foreign matter, but it may better perhaps be referred to the destruction of
the granular-crystalline continuity on which glacier motion probably
depends.
Fig. 253.—Glacial striæ and bruises. The block to the right shows two sets of striæ: that to
the left shows the peculiar curved fractures known as Chatter Marks.
angular débris is a more effective instrument of erosion than fine, soft, or
rounded material. The adverse influence of the overloading of the ice on its
motion has been likened to the stiffening of a viscous liquid by the addition
of foreign matter, but it may better perhaps be referred to the destruction of
the granular-crystalline continuity on which glacier motion probably
depends.
Fig. 253.—Glacial striæ and bruises. The block to the right shows two sets of striæ: that to
the left shows the peculiar curved fractures known as Chatter Marks.
Page 342
Fig. 254.—Bowlders showing glacial striation. (Drawn by Miss Matz.)
Fig. 255.—Striæ on bed rock, Kingston, Des Moines Co., Ia. (Iowa Geol. Surv.)
From the preceding statement, it is evident that erosion is not equally
effective at all points beneath a glacier. So far as concerns the ice itself,
erosion is not most effective at the end of a valley glacier, or at the edge of
an ice sheet, for here the strength of movement is too slight and the load too
Fig. 255.—Striæ on bed rock, Kingston, Des Moines Co., Ia. (Iowa Geol. Surv.)
From the preceding statement, it is evident that erosion is not equally
effective at all points beneath a glacier. So far as concerns the ice itself,
erosion is not most effective at the end of a valley glacier, or at the edge of
an ice sheet, for here the strength of movement is too slight and the load too
Page 343
great; nor is the most effective erosion at the source or near it, for though
the ice may here be thick, the movement is slow and the load likely to be
slight. Ice conditions only being considered, erosion is most effective
somewhere between the source and the terminus, and probably much nearer
the latter than the former. The conditions of the surface over which the ice
passes may be such as to vary the place of greatest erosion widely. Thus in
an Alpine glacier, erosion may be most effective at the Bergschrund
because the slope here favors “plucking.” Here, notable amphitheatres
(cirques) are sometimes excavated. After the glacier disappears, the bottom
of the cirque is often seen to contain rock basins (Fig. 257). Glacial cirques
abound in mountains where glaciers once existed, but from which they have
now disappeared. The cirques of the Bighorn mountains of Wyoming (Pl.
XIX) are examples.
Fig. 256.—Striæ, grooves, etc., in a canyon tributary to Big Cottonwood Canyon, Wasatch
Mountains. (Church.)
Summary.—In summary it may be said that rapidly moving ice of
sufficient thickness to be working under goodly pressure, shod with a
sufficient but not excessive quantity of hard-rock material, passing over
incoherent or soft formations possessing a topography of sufficient relief to
the ice may here be thick, the movement is slow and the load likely to be
slight. Ice conditions only being considered, erosion is most effective
somewhere between the source and the terminus, and probably much nearer
the latter than the former. The conditions of the surface over which the ice
passes may be such as to vary the place of greatest erosion widely. Thus in
an Alpine glacier, erosion may be most effective at the Bergschrund
because the slope here favors “plucking.” Here, notable amphitheatres
(cirques) are sometimes excavated. After the glacier disappears, the bottom
of the cirque is often seen to contain rock basins (Fig. 257). Glacial cirques
abound in mountains where glaciers once existed, but from which they have
now disappeared. The cirques of the Bighorn mountains of Wyoming (Pl.
XIX) are examples.
Fig. 256.—Striæ, grooves, etc., in a canyon tributary to Big Cottonwood Canyon, Wasatch
Mountains. (Church.)
Summary.—In summary it may be said that rapidly moving ice of
sufficient thickness to be working under goodly pressure, shod with a
sufficient but not excessive quantity of hard-rock material, passing over
incoherent or soft formations possessing a topography of sufficient relief to
Page 344
offer some resistance, and yet too little to retard seriously the progress of
the ice, will erode most effectively.
Varied nature of glacial débris.—From its mode of erosion it will
readily be seen that the bottom of a glacier may be charged with various
sorts of material. There may be (1) bowlders which the ice has picked up
from the surface, or which it has broken off from projecting points of rock
over which it has passed; (2) smaller pieces of rock of the size of cobbles,
pebbles, etc., either picked up by the ice from its bed or broken off from
larger masses; (3) the fine products (rock-flour) produced by the grinding of
the débris in the ice on the rock-bed over which it passes, and similar
products resulting from the rubbing of stones in the ice against one another;
and (4) sand, clay, soil, vegetation, etc., derived from the surface
overridden. Thus the materials which the ice carries (drift) are of all grades
of coarseness and fineness, from large bowlders to fine clay. The coarser
material may be angular or round at the outset, and its form may be changed
and its surface striated as it is moved forward. Whether one sort of material
or another predominates, depends primarily on the nature of the surface
overridden.
the ice, will erode most effectively.
Varied nature of glacial débris.—From its mode of erosion it will
readily be seen that the bottom of a glacier may be charged with various
sorts of material. There may be (1) bowlders which the ice has picked up
from the surface, or which it has broken off from projecting points of rock
over which it has passed; (2) smaller pieces of rock of the size of cobbles,
pebbles, etc., either picked up by the ice from its bed or broken off from
larger masses; (3) the fine products (rock-flour) produced by the grinding of
the débris in the ice on the rock-bed over which it passes, and similar
products resulting from the rubbing of stones in the ice against one another;
and (4) sand, clay, soil, vegetation, etc., derived from the surface
overridden. Thus the materials which the ice carries (drift) are of all grades
of coarseness and fineness, from large bowlders to fine clay. The coarser
material may be angular or round at the outset, and its form may be changed
and its surface striated as it is moved forward. Whether one sort of material
or another predominates, depends primarily on the nature of the surface
overridden.
Page 345
PLATE XIX.
U. S. Geol. Surv.
PART OF THE Scale, 2+ miles per inch.
BIGHORN
MOUNTAIN RANGE, WYOMING.
U. S. Geol. Surv.
PART OF THE Scale, 2+ miles per inch.
BIGHORN
MOUNTAIN RANGE, WYOMING.
Page 346
PLATE XX.
U. S. Geol. Surv. Scale, 1+ miles per inch.
A SECTION OF THE CALIFORNIA
COAST NEAR SAN MATEO,
CALIFORNIA.
U. S. Geol. Surv. Scale, 1+ miles per inch.
A SECTION OF THE CALIFORNIA
COAST NEAR SAN MATEO,
CALIFORNIA.
Page 347
Fig. 257.—A glacial cirque. The lake occupies a rock basin, produced by glacier erosion.
Head of Little Timber Creek, Montana.
The topographic effects of glacial erosion.—In passing through its
valley, an alpine glacier deepens and widens its bottom and smooths its
slopes up to the upper limit of the ice. It tends to change a V-shaped valley
(Fig. 258) into a U-shaped one (Fig. 259). The change in topography at the
upper limit of glaciation is often marked (Figs. 260 and 261).
Head of Little Timber Creek, Montana.
The topographic effects of glacial erosion.—In passing through its
valley, an alpine glacier deepens and widens its bottom and smooths its
slopes up to the upper limit of the ice. It tends to change a V-shaped valley
(Fig. 258) into a U-shaped one (Fig. 259). The change in topography at the
upper limit of glaciation is often marked (Figs. 260 and 261).
Page 348
Fig. 258.—The Valley of the American Fork. A V-shaped non-glaciated valley in the
Wasatch Mountains of Utah. Compare Fig. 259. (Church.)
Fig. 259.—U-shaped valley resulting from glaciation. Little Cottonwood Canyon, Wasatch
Mountains. (Church.)
Wasatch Mountains of Utah. Compare Fig. 259. (Church.)
Fig. 259.—U-shaped valley resulting from glaciation. Little Cottonwood Canyon, Wasatch
Mountains. (Church.)
Page 349
Fig. 260.—Contrast between glaciated topography below and non-glaciated topography
above. The minarets in the Sierras, Cal.
above. The minarets in the Sierras, Cal.
Page 350
Fig. 261.—Contrast between glaciated topography below, and non-glaciated topography
above. Needles Mountains, from slope west of Hidden Lake. (Cross, U. S. Geol. Surv.)
The deepening of a valley by glacial erosion may throw its tributaries out
of topographic adjustment. Thus if a main valley is lowered 100 feet by
glacial erosion while its tributary is not deepened, the lower end of the latter
will be 100 feet above the former when the ice disappears. Such a valley is
called a hanging valley (Figs. 262 and 263). Such valleys are of common
occurrence in regions recently glaciated, but now ice-free. Examples are
common in the western mountains of North America and elsewhere.
Ice-caps which overspread the surface irrespective of valleys and hills,
tend to reduce the angularities of the surface. Hills and ridges are cut down
and smoothed (Figs. 264 and 265); but since valleys parallel to the direction
of movement are deepened at the same time, it is doubtful if the relief of the
surface is commonly reduced by the erosion of an ice-cap.
above. Needles Mountains, from slope west of Hidden Lake. (Cross, U. S. Geol. Surv.)
The deepening of a valley by glacial erosion may throw its tributaries out
of topographic adjustment. Thus if a main valley is lowered 100 feet by
glacial erosion while its tributary is not deepened, the lower end of the latter
will be 100 feet above the former when the ice disappears. Such a valley is
called a hanging valley (Figs. 262 and 263). Such valleys are of common
occurrence in regions recently glaciated, but now ice-free. Examples are
common in the western mountains of North America and elsewhere.
Ice-caps which overspread the surface irrespective of valleys and hills,
tend to reduce the angularities of the surface. Hills and ridges are cut down
and smoothed (Figs. 264 and 265); but since valleys parallel to the direction
of movement are deepened at the same time, it is doubtful if the relief of the
surface is commonly reduced by the erosion of an ice-cap.
Page 351
Fig. 262.—A hanging valley. East side of Lake Kootenai, B. C. All except the highest
summits glaciated. (Atwood.)
Fiords.—A glacier descending into the head of a narrow bay may gouge
out the bay to a very considerable depth, causing its head to recede. When
the ice finally melts, the bay may be a fiord. Thus have arisen the glacial
features of many of the fiords of high-latitude coasts, and many of the
glaciers of those coasts are now making fiords (Fig. 266). Fiords also arise
in other ways. Coasts indented by fiords are likely to be bordered by
islands.
The positions in which débris is carried.—As a result of the methods
by which a glacier becomes loaded, there are three positions in which the
débris is carried: (1) the basal or subglacial, (2) the englacial, and (3) the
superglacial. The material picked up or rubbed off from the surface over
which the ice moves is normally carried forward in the base of the ice;
while that which falls on the surface is usually carried in the form of surface
moraines. In the former position the drift is basal; in the latter, superglacial.
It is doubtful if much débris is moved along beneath (that is, strictly below
the bottom of) the ice, though the movement of the latter would have a
tendency to drag or urge along with it the loose material of its bed. If drift
were carried forward in such positions, it would be strictly subglacial.
summits glaciated. (Atwood.)
Fiords.—A glacier descending into the head of a narrow bay may gouge
out the bay to a very considerable depth, causing its head to recede. When
the ice finally melts, the bay may be a fiord. Thus have arisen the glacial
features of many of the fiords of high-latitude coasts, and many of the
glaciers of those coasts are now making fiords (Fig. 266). Fiords also arise
in other ways. Coasts indented by fiords are likely to be bordered by
islands.
The positions in which débris is carried.—As a result of the methods
by which a glacier becomes loaded, there are three positions in which the
débris is carried: (1) the basal or subglacial, (2) the englacial, and (3) the
superglacial. The material picked up or rubbed off from the surface over
which the ice moves is normally carried forward in the base of the ice;
while that which falls on the surface is usually carried in the form of surface
moraines. In the former position the drift is basal; in the latter, superglacial.
It is doubtful if much débris is moved along beneath (that is, strictly below
the bottom of) the ice, though the movement of the latter would have a
tendency to drag or urge along with it the loose material of its bed. If drift
were carried forward in such positions, it would be strictly subglacial.
Page 352
Fig. 263.—A hanging valley. The water falls (Bridal Veil) from a hanging valley.
(Wineman.)
The basal load of a glacier is constantly being mixed with new accessions
derived from ground over which the ice is passing, and this admixture tells
the story of the work done by the bottom of the ice. The englacial and
superglacial material, on the other hand, is normally borne from the place of
origin to the place of deposition without such intermixture. It is a case of
“local” versus “through” transportation.
Transfers of load.—While the origin of the load usually determines its
position, exceptions and complications arise from the transfer of load from
one position to another, and from the gradation of one horizon into another.
(Wineman.)
The basal load of a glacier is constantly being mixed with new accessions
derived from ground over which the ice is passing, and this admixture tells
the story of the work done by the bottom of the ice. The englacial and
superglacial material, on the other hand, is normally borne from the place of
origin to the place of deposition without such intermixture. It is a case of
“local” versus “through” transportation.
Transfers of load.—While the origin of the load usually determines its
position, exceptions and complications arise from the transfer of load from
one position to another, and from the gradation of one horizon into another.
Page 353
Fig. 264.—A non-glaciated hill. Dalrymple Island. North Greenland.
Fig. 265.—A glaciated hill. Southeastern Carey Island. About 30 miles west-northwest of
Dalrymple Island.
Most of the débris gathered by ice is acquired at its bottom. While such
material is basal at the outset, some of it may find itself above the bottom a
little later. Thus when ice passes over a hill (Fig. 267) the bottom of the ice
rends débris from the top of the hill. When it descends from one level to
another there is a similar result (Fig. 268). To the lee of the hill the ice from
Fig. 265.—A glaciated hill. Southeastern Carey Island. About 30 miles west-northwest of
Dalrymple Island.
Most of the débris gathered by ice is acquired at its bottom. While such
material is basal at the outset, some of it may find itself above the bottom a
little later. Thus when ice passes over a hill (Fig. 267) the bottom of the ice
rends débris from the top of the hill. When it descends from one level to
another there is a similar result (Fig. 268). To the lee of the hill the ice from
Page 354
either side may close in under that which came over the top, in which case
the débris derived from the top of the hill by the bottom of the overriding
ice will be well up in the ice. It has passed from an initial basal to a
subsequent englacial position. The change does not usually involve an
actual rise of the material, but rather a decline. If carried upward at all, the
upward movement is temporary only, and incident to the passage of the ice
over the hill, or to other local causes. The englacial débris may be little or
much above the basal zone according to the height of the elevation
overridden.
Fig. 266.—Alaskan fiords. The shaded areas represent land. (From charts of the C. & G.
Surv.)
the débris derived from the top of the hill by the bottom of the overriding
ice will be well up in the ice. It has passed from an initial basal to a
subsequent englacial position. The change does not usually involve an
actual rise of the material, but rather a decline. If carried upward at all, the
upward movement is temporary only, and incident to the passage of the ice
over the hill, or to other local causes. The englacial débris may be little or
much above the basal zone according to the height of the elevation
overridden.
Fig. 266.—Alaskan fiords. The shaded areas represent land. (From charts of the C. & G.
Surv.)
Page 355
Fig. 267.—Diagram to illustrate the taking of débris from a hill-top. It also illustrates how
englacial débris may become superglacial as the result of surface ablation.
Fig. 268.—Taking débris from a protuberance of the bed.
Superglacial débris may obviously become englacial by falling into
crevasses or by being carried down by descending waters. Either
superglacial or englacial débris may become basal by the same means.
From their form and position, there is less ice-free land in immediate
association with ice-caps than with valley glaciers. Furthermore, the ice-
free land about the borders of an ice-cap is less likely to be in the form of
cliffs above it. As a result, the surfaces of ice-caps are comparatively clean,
except at their edges where the ice is thin.
englacial débris may become superglacial as the result of surface ablation.
Fig. 268.—Taking débris from a protuberance of the bed.
Superglacial débris may obviously become englacial by falling into
crevasses or by being carried down by descending waters. Either
superglacial or englacial débris may become basal by the same means.
From their form and position, there is less ice-free land in immediate
association with ice-caps than with valley glaciers. Furthermore, the ice-
free land about the borders of an ice-cap is less likely to be in the form of
cliffs above it. As a result, the surfaces of ice-caps are comparatively clean,
except at their edges where the ice is thin.
Page 356
Fig. 269.—Side view of end of a glacier on the south side of Olriks Bay, North Greenland.
Fig. 270.—Closer view of a part of the ice shown in Fig. 269.
Englacial material may become superglacial by surface ablation. In this
case the drift does not rise, but melting brings the surface of the ice down to
its level. This occurs chiefly at the end or edge of the ice, where the surface
melting is greatest. Englacial débris, especially that near the bottom, may
also become basal by the melting of the bottom of the ice.
Fig. 270.—Closer view of a part of the ice shown in Fig. 269.
Englacial material may become superglacial by surface ablation. In this
case the drift does not rise, but melting brings the surface of the ice down to
its level. This occurs chiefly at the end or edge of the ice, where the surface
melting is greatest. Englacial débris, especially that near the bottom, may
also become basal by the melting of the bottom of the ice.
Page 357
Englacial material plucked or rasped from an elevation over which the
ice has passed is liable to be disposed in a longitudinal belt in the ice in the
lee of the elevation itself. By surface ablation this material may reach the
surface at some point below its source, and be disposed as a medial
moraine. Such a moraine has an origin very different from that of a medial
moraine formed by the junction of two lateral moraines of superglacial
origin.
Much less in the natural order of things is the transfer of material from a
basal to an englacial and from an englacial to a superglacial position by
upward movement of the débris itself. Such transfer is remarkable because
the specific gravity of rock is from two and a half to three times as great as
that of ice, so that its normal tendency is to sink.
Fig. 271.—Surface terminal moraines due to upturning. Edge of the ice-sheet, North
Greenland.
In arctic glaciers, and probably in others, some material which has been
basal becomes englacial by being sheared forward over ice in front of it. So
far as observed this takes place chiefly where the ice in front of the plane of
shearing lies at a lower level than that behind, as where the surface of an
upland falls off into a valley, or where a boss of rock shelters the ice in its
lee from the thrust of the overriding ice (Fig. 268).
At the borders of arctic glaciers the
lower layers are not infrequently
upturned, as shown in Figs. 269 to
Fig. 272.—Diagram illustrating the
272. Where the layers turn up at the upturning of the layers of ice at the end
end of a glacier (Figs. 269 and 270), of an arctic glacier as seen in end-
basal and englacial débris is carried to section. The bottom line represents sea
level.
the surface by actual upward
ice has passed is liable to be disposed in a longitudinal belt in the ice in the
lee of the elevation itself. By surface ablation this material may reach the
surface at some point below its source, and be disposed as a medial
moraine. Such a moraine has an origin very different from that of a medial
moraine formed by the junction of two lateral moraines of superglacial
origin.
Much less in the natural order of things is the transfer of material from a
basal to an englacial and from an englacial to a superglacial position by
upward movement of the débris itself. Such transfer is remarkable because
the specific gravity of rock is from two and a half to three times as great as
that of ice, so that its normal tendency is to sink.
Fig. 271.—Surface terminal moraines due to upturning. Edge of the ice-sheet, North
Greenland.
In arctic glaciers, and probably in others, some material which has been
basal becomes englacial by being sheared forward over ice in front of it. So
far as observed this takes place chiefly where the ice in front of the plane of
shearing lies at a lower level than that behind, as where the surface of an
upland falls off into a valley, or where a boss of rock shelters the ice in its
lee from the thrust of the overriding ice (Fig. 268).
At the borders of arctic glaciers the
lower layers are not infrequently
upturned, as shown in Figs. 269 to
Fig. 272.—Diagram illustrating the
272. Where the layers turn up at the upturning of the layers of ice at the end
end of a glacier (Figs. 269 and 270), of an arctic glacier as seen in end-
basal and englacial débris is carried to section. The bottom line represents sea
level.
the surface by actual upward
Page 358
movement, and a terminal moraine or a series of terminal moraines
sometimes aggregated where the upturned layers of ice outcrop at the
surface (Fig. 271). That the material of these moraines was originally basal
is abundantly demonstrated by the bruised and scratched condition of the
bowlders and pebbles, and sometimes by the nature of the material itself.
For example, in two cases in North Greenland where glaciers descend into
the heads of shallow bays and move forward on their bottoms, moraines
formed by the upturning of the layers were seen to contain abundant
molluscan shells derived from the bottom of the bay. The upturning
sometimes affects the side-edges of ice-tongues (Fig. 272) as well as their
ends, and the material thus brought to the surface gives origin to lateral
moraines altogether different in origin from the lateral moraines formed by
the falling of débris upon the glaciers. Sometimes also there is an upturning
of the ice along a longitudinal zone well back from the lateral margins (Fig.
273), and the material so borne to the surface in such a zone gives rise to a
moraine resembling the medial moraine formed by the union of lateral
moraines, but of wholly different origin.
Fig. 273.—Diagram illustrating the same point as 272, where the structure is more
complex. The bottom line of the figure represents sea level.
The phenomenon of upturning here referred to has been observed only at
or near the terminus of the ice, and is perhaps due in most part to the
resistance of frozen morainic or other material beneath and in front of the
edge. To this should probably be added the effect of the increased rigidity of
the ice at its borders, due to the low external temperature during the larger
part of the year, while the interior, with its higher temperature, remains
more fluent. But even this probably leaves the explanation inadequate. In
not a few instances the upturning is associated with a notable thickening of
the layers toward their edges (Fig. 274). This suggests that perhaps there is
an exceptional growth of the granular crystals of the ice near the edge of the
layers, owing to the penetration of the surface-waters which are much more
abundant at the borders than elsewhere, and which in the arctic glaciers
probably do not penetrate deeply before they reach a freezing temperature.
sometimes aggregated where the upturned layers of ice outcrop at the
surface (Fig. 271). That the material of these moraines was originally basal
is abundantly demonstrated by the bruised and scratched condition of the
bowlders and pebbles, and sometimes by the nature of the material itself.
For example, in two cases in North Greenland where glaciers descend into
the heads of shallow bays and move forward on their bottoms, moraines
formed by the upturning of the layers were seen to contain abundant
molluscan shells derived from the bottom of the bay. The upturning
sometimes affects the side-edges of ice-tongues (Fig. 272) as well as their
ends, and the material thus brought to the surface gives origin to lateral
moraines altogether different in origin from the lateral moraines formed by
the falling of débris upon the glaciers. Sometimes also there is an upturning
of the ice along a longitudinal zone well back from the lateral margins (Fig.
273), and the material so borne to the surface in such a zone gives rise to a
moraine resembling the medial moraine formed by the union of lateral
moraines, but of wholly different origin.
Fig. 273.—Diagram illustrating the same point as 272, where the structure is more
complex. The bottom line of the figure represents sea level.
The phenomenon of upturning here referred to has been observed only at
or near the terminus of the ice, and is perhaps due in most part to the
resistance of frozen morainic or other material beneath and in front of the
edge. To this should probably be added the effect of the increased rigidity of
the ice at its borders, due to the low external temperature during the larger
part of the year, while the interior, with its higher temperature, remains
more fluent. But even this probably leaves the explanation inadequate. In
not a few instances the upturning is associated with a notable thickening of
the layers toward their edges (Fig. 274). This suggests that perhaps there is
an exceptional growth of the granular crystals of the ice near the edge of the
layers, owing to the penetration of the surface-waters which are much more
abundant at the borders than elsewhere, and which in the arctic glaciers
probably do not penetrate deeply before they reach a freezing temperature.
Page 359
Wear of drift in transit.—Drift carried at the bottom of the ice is subject
to notable wear. The materials in transportation abrade one another and are
abraded by the bed over which they pass. Englacial drift is subject to less
wear because it is commonly more scattered. Superglacial drift is worn little
or none while it lies on the surface of the ice; but in so far as superglacial or
englacial drift is derived from the basal load, it may show the same
evidences of wear as the basal drift itself. Superglacial drift often reveals its
history in this way.
Fig. 274.—Thickening of the upturned layers of ice.
Deposition of the Drift.
1. Beneath the body of the ice.—During the advance of a glacier,
deposition may take place both beneath the body of the ice and beneath its
end and edges. Deposition beneath the body of the ice is liable to take place
wherever the topography favors lodgment, or wherever the ice is
overloaded. The topography favoring deposition is much the same as that
favoring erosion, but the two processes are not favored at the same point.
Erosion is greatest on the “stoss” side of an obstruction (the side against
which the ice advances), and deposition on the lee side. The ice is likely to
be overloaded (1) just beyond a place where conditions have favored the
to notable wear. The materials in transportation abrade one another and are
abraded by the bed over which they pass. Englacial drift is subject to less
wear because it is commonly more scattered. Superglacial drift is worn little
or none while it lies on the surface of the ice; but in so far as superglacial or
englacial drift is derived from the basal load, it may show the same
evidences of wear as the basal drift itself. Superglacial drift often reveals its
history in this way.
Fig. 274.—Thickening of the upturned layers of ice.
Deposition of the Drift.
1. Beneath the body of the ice.—During the advance of a glacier,
deposition may take place both beneath the body of the ice and beneath its
end and edges. Deposition beneath the body of the ice is liable to take place
wherever the topography favors lodgment, or wherever the ice is
overloaded. The topography favoring deposition is much the same as that
favoring erosion, but the two processes are not favored at the same point.
Erosion is greatest on the “stoss” side of an obstruction (the side against
which the ice advances), and deposition on the lee side. The ice is likely to
be overloaded (1) just beyond a place where conditions have favored the
Page 360
gathering of a heavy load, and (2) where the ice is rapidly thinning. On the
whole, however, the deposition of material beneath the main body of a
glacier is much more than balanced by erosion in the same position.
Fig. 275.—Glacier building an embankment. Southeast side of McCormick Bay, North
Greenland.
2. At ends and edges of glaciers.—At and near the end of a glacier the
conditions of deposition are somewhat different. Here deposition beneath
the ice goes on faster than elsewhere, chiefly because of the more rapid
melting and the more rapid thinning and weakening of the ice. If the end of
the glacier be stationary in position, drift is being continually brought to it
and left there, for though the end is stationary, the ice continues to move. If
the glacier moves forward 500 feet per year, and if its end is melted at the
same rate, all the débris in the 500 feet of ice which has been melted has
been deposited, and all except that which has been washed away has been
deposited at and beneath the end of the glacier. If the end of the glacier is
retreating, the retreat means that the waste at the end exceeds the forward
movement. If the ice advances 300 feet per year, and is melted back 500
feet in the same time, all the débris carried by the 500 feet which has been
melted has been deposited, and largely in the narrow zone (200 feet) from
which the ice has receded. Even in this case, therefore, there is a notable
whole, however, the deposition of material beneath the main body of a
glacier is much more than balanced by erosion in the same position.
Fig. 275.—Glacier building an embankment. Southeast side of McCormick Bay, North
Greenland.
2. At ends and edges of glaciers.—At and near the end of a glacier the
conditions of deposition are somewhat different. Here deposition beneath
the ice goes on faster than elsewhere, chiefly because of the more rapid
melting and the more rapid thinning and weakening of the ice. If the end of
the glacier be stationary in position, drift is being continually brought to it
and left there, for though the end is stationary, the ice continues to move. If
the glacier moves forward 500 feet per year, and if its end is melted at the
same rate, all the débris in the 500 feet of ice which has been melted has
been deposited, and all except that which has been washed away has been
deposited at and beneath the end of the glacier. If the end of the glacier is
retreating, the retreat means that the waste at the end exceeds the forward
movement. If the ice advances 300 feet per year, and is melted back 500
feet in the same time, all the débris carried by the 500 feet which has been
melted has been deposited, and largely in the narrow zone (200 feet) from
which the ice has receded. Even in this case, therefore, there is a notable
Page 361
tendency to marginal accumulation. If the end of the glacier is advancing
500 feet per year while it is being melted but 300 feet, all the drift in the
300 feet melted has been deposited, and chiefly at or beneath the immediate
margin of the ice. To the marginal and sub-marginal accumulations made in
this way, the material carried on the ice is added whenever the ice is melted
from beneath it. This addition is sometimes considerable and sometimes
meagre. If the edge of the ice is without much fluctuation in position, the
material dumped over its end may take the form of a narrow ridge or
bowlder-wall (Geschiebe-wall). If a glacier pushes material in front of it,
this, too, becomes a part of the general terminal aggregation of drift.
Fig. 276.—Embankment completed. Near the last.
TYPES OF MORAINES.
The terminal moraine.—The thick accumulation of drift made at the
end of a glacier or at the edge of an ice sheet, especially where its end or
edge is stationary, or nearly stationary, for a considerable time, is the
terminal moraine. That part of the aggregation deposited beneath the ice is
sometimes called the lodge moraine (Figs. 275 and 276; see also Fig. 235);
that carried on the ice and dropped at its edge, the dump moraine; and that
500 feet per year while it is being melted but 300 feet, all the drift in the
300 feet melted has been deposited, and chiefly at or beneath the immediate
margin of the ice. To the marginal and sub-marginal accumulations made in
this way, the material carried on the ice is added whenever the ice is melted
from beneath it. This addition is sometimes considerable and sometimes
meagre. If the edge of the ice is without much fluctuation in position, the
material dumped over its end may take the form of a narrow ridge or
bowlder-wall (Geschiebe-wall). If a glacier pushes material in front of it,
this, too, becomes a part of the general terminal aggregation of drift.
Fig. 276.—Embankment completed. Near the last.
TYPES OF MORAINES.
The terminal moraine.—The thick accumulation of drift made at the
end of a glacier or at the edge of an ice sheet, especially where its end or
edge is stationary, or nearly stationary, for a considerable time, is the
terminal moraine. That part of the aggregation deposited beneath the ice is
sometimes called the lodge moraine (Figs. 275 and 276; see also Fig. 235);
that carried on the ice and dropped at its edge, the dump moraine; and that
Page 362
pushed before the ice, the push moraine. Many moraines marginal to the ice
appear to be push moraines, when they are really lodge moraines from
which the ice has withdrawn (Fig. 277). The push moraine can rarely be
distinguished, and the dump moraine by no means always, after the
disappearance of the ice.
Fig. 277.—End of a glacier a few miles west of Kaslo on Lake Kootenai, B. C. A lodge
moraine from which the ice has withdrawn, giving it the appearance of a push moraine.
It is possible that the lodge moraine material has been pushed up a little by re-advance of
the ice. (Atwood.)
The ground moraine.—When a glacier disappears by melting, all its
débris is deposited. All the drift deposited beneath the advancing ice and all
deposited from the base of the ice during its dissolution constitutes the
ground moraine. The thickness of the ground moraine is notably unequal. In
general, it is thicker toward the terminus of the glacier and thinner toward
its source, but considerable portions of a glacier’s bed are often left without
débris when the ice melts. In general, the terminal moraine is not only
thicker, but more irregularly disposed than the ground moraine.
appear to be push moraines, when they are really lodge moraines from
which the ice has withdrawn (Fig. 277). The push moraine can rarely be
distinguished, and the dump moraine by no means always, after the
disappearance of the ice.
Fig. 277.—End of a glacier a few miles west of Kaslo on Lake Kootenai, B. C. A lodge
moraine from which the ice has withdrawn, giving it the appearance of a push moraine.
It is possible that the lodge moraine material has been pushed up a little by re-advance of
the ice. (Atwood.)
The ground moraine.—When a glacier disappears by melting, all its
débris is deposited. All the drift deposited beneath the advancing ice and all
deposited from the base of the ice during its dissolution constitutes the
ground moraine. The thickness of the ground moraine is notably unequal. In
general, it is thicker toward the terminus of the glacier and thinner toward
its source, but considerable portions of a glacier’s bed are often left without
débris when the ice melts. In general, the terminal moraine is not only
thicker, but more irregularly disposed than the ground moraine.
Page 363
The lateral moraines.—The surface lateral moraines of valley glaciers
are let down on the surface beneath when the ice melts out from under
them; but the lateral moraines in a valley from which the ice has melted are
not merely the lateral moraines which were on the glacier at a given time.
They are often far more massive than any which ever existed on the ice
itself at any one time (Fig. 278). As a glacier retreats, its lateral moraine
material is more or less bunched. Thus if the ice advances 200 feet while its
end is being melted back 300 feet, the lateral moraines on the 300 feet
melted are concentrated into 100 feet, as they are delivered on to the land
by the melting of the ice from beneath. If the retreat of the end of a glacier
be very slow, the bunching may be great. But even this cannot explain the
massiveness of some lateral moraines. Furthermore, the materials of which
many lateral moraines are composed are nearly as well worn as those of the
ground moraine. The massive lateral moraines of which this is true are often
made up chiefly of the drift accumulated beneath the lateral margins of the
glaciers. This accumulation is the result of the lateral motion of the ice from
center to side. Such sublateral accumulations are akin to terminal moraines.
Some of the lateral moraines of ancient valley glaciers, such as those of the
Uinta, Wasatch, and Bighorn mountains are several hundred feet high, and
in one case about 1000 feet. In northern Italy lateral moraines are said to be
1500 to 2000 feet high.[132]
Fig. 278.—A lateral moraine from which the ice has retreated. Bighorn Mountains, Wyo.
(Blackwelder.)
are let down on the surface beneath when the ice melts out from under
them; but the lateral moraines in a valley from which the ice has melted are
not merely the lateral moraines which were on the glacier at a given time.
They are often far more massive than any which ever existed on the ice
itself at any one time (Fig. 278). As a glacier retreats, its lateral moraine
material is more or less bunched. Thus if the ice advances 200 feet while its
end is being melted back 300 feet, the lateral moraines on the 300 feet
melted are concentrated into 100 feet, as they are delivered on to the land
by the melting of the ice from beneath. If the retreat of the end of a glacier
be very slow, the bunching may be great. But even this cannot explain the
massiveness of some lateral moraines. Furthermore, the materials of which
many lateral moraines are composed are nearly as well worn as those of the
ground moraine. The massive lateral moraines of which this is true are often
made up chiefly of the drift accumulated beneath the lateral margins of the
glaciers. This accumulation is the result of the lateral motion of the ice from
center to side. Such sublateral accumulations are akin to terminal moraines.
Some of the lateral moraines of ancient valley glaciers, such as those of the
Uinta, Wasatch, and Bighorn mountains are several hundred feet high, and
in one case about 1000 feet. In northern Italy lateral moraines are said to be
1500 to 2000 feet high.[132]
Fig. 278.—A lateral moraine from which the ice has retreated. Bighorn Mountains, Wyo.
(Blackwelder.)
Page 364
Fig. 279.—Glacial drift, coarse and fine together. (Geol. Surv. of N. J.)
Most of the material which was englacial during the transportation
becomes either subglacial or superglacial before deposition, for it ordinarily
reaches the bottom or the top of the ice before being deposited. Where the
ends or edges of a glacier are vertical or nearly so, as in the high arctic
regions, deposition may take place from the englacial position directly.
Distinctive nature of glacial deposits.—The deposits made by glaciers
are distinctive. In the first place the ice does not assort its material, and
bowlders, cobbles, pebbles, sand, and clay are confusedly commingled (Fig.
279). In this respect, the deposits of ice differ notably from those of water.
Furthermore, many stones of the drift show the peculiar type of wear which
glaciers inflict. They are not rounded as the stones carried by rivers, though
they are notably worn. Many of them have subangular forms with planed
and beveled faces, the planes being striated and bruised (Fig. 254). The
Most of the material which was englacial during the transportation
becomes either subglacial or superglacial before deposition, for it ordinarily
reaches the bottom or the top of the ice before being deposited. Where the
ends or edges of a glacier are vertical or nearly so, as in the high arctic
regions, deposition may take place from the englacial position directly.
Distinctive nature of glacial deposits.—The deposits made by glaciers
are distinctive. In the first place the ice does not assort its material, and
bowlders, cobbles, pebbles, sand, and clay are confusedly commingled (Fig.
279). In this respect, the deposits of ice differ notably from those of water.
Furthermore, many stones of the drift show the peculiar type of wear which
glaciers inflict. They are not rounded as the stones carried by rivers, though
they are notably worn. Many of them have subangular forms with planed
and beveled faces, the planes being striated and bruised (Fig. 254). The
Page 365
absence of stratification, the physical heterogeneity, and the striation of at
least a part of the stones are among the most distinctive characteristics of
glacial drift. A not less real though less obvious characteristic is the
constitution of the fine material, for it is in general not the product of rock
decay, but of rock grinding. The fine material handled by streams (except
glacial streams) on the other hand, is usually the product of rock decay.
Fig. 280.—Roche moutonnée, Victoria Harbor, B. C.
Glaciated rock surfaces.—Another distinctive mark which a glacier
leaves behind it is the character of the surface of the rock on which the drift
rests. This is generally smoothed by the severe abrasion to which it has been
subjected, and the smoothed surfaces are marked by grooves and striæ,
similar to those on the stones of the drift (Figs. 255 and 256). Other
distinctive features of a glaciated area are the rounded bosses of rock
(roches moutonnées, Fig. 280; see also surface about the lakes, Fig. 261),
the rock basins, the lakes (Fig. 261), ponds, and marshes, and the peculiar
topographies resulting from the unequal erosion, and the still more unequal
deposition of the drift. Surface bowlders, often unlike the underlying
formations of rock, and sometimes in peculiar and apparently unstable
positions, are still another mark of a glaciated area.
GLACIO-FLUVIAL WORK.
least a part of the stones are among the most distinctive characteristics of
glacial drift. A not less real though less obvious characteristic is the
constitution of the fine material, for it is in general not the product of rock
decay, but of rock grinding. The fine material handled by streams (except
glacial streams) on the other hand, is usually the product of rock decay.
Fig. 280.—Roche moutonnée, Victoria Harbor, B. C.
Glaciated rock surfaces.—Another distinctive mark which a glacier
leaves behind it is the character of the surface of the rock on which the drift
rests. This is generally smoothed by the severe abrasion to which it has been
subjected, and the smoothed surfaces are marked by grooves and striæ,
similar to those on the stones of the drift (Figs. 255 and 256). Other
distinctive features of a glaciated area are the rounded bosses of rock
(roches moutonnées, Fig. 280; see also surface about the lakes, Fig. 261),
the rock basins, the lakes (Fig. 261), ponds, and marshes, and the peculiar
topographies resulting from the unequal erosion, and the still more unequal
deposition of the drift. Surface bowlders, often unlike the underlying
formations of rock, and sometimes in peculiar and apparently unstable
positions, are still another mark of a glaciated area.
GLACIO-FLUVIAL WORK.
Page 366
The constant but unequal waste of glaciers has already been referred to.
The streams to which this gives rise are usually laden with gravel, sand and
silt derived from the ice. Since the mud is often light-colored, the streams
are sometimes described as “milky.” Where the amount of material carried
is great, much of it is dropped at a slight distance from the ice, the coarsest
being dropped first. Glacial streams are, as a rule, aggrading streams, and
therefore develop alluvial plains, called valley trains (Fig. 281 and 282), or
where they enter lakes (Fig. 283), bays, or other streams, deltas. In its
transportation, the river-borne drift is assorted; after its deposition, it is
stratified. True glacial deposits in the upper part of a mountain valley are,
therefore, often continued below by glacio-fluvial deposits derived from the
same source.
Fig. 281.—Alluviation by glacial stream: Nicolai Creek, Alaska. (Schrader, U. S. Geol.
Surv.)
The most common form of such deposit is a valley train (Fig. 281) of
glacial wash stretching indefinitely down the valley. The silt, sand, and
gravel of such trains can usually be distinguished from valley deposits of
non-glacial origin by the character of the material, as much of it is the
product of grinding, crushing, and fracture, rather than of ordinary surface
decay. Its materials are, therefore, fresh and often include rock material
which, if long exposed at the surface, would be decomposed or dissolved.
The streams to which this gives rise are usually laden with gravel, sand and
silt derived from the ice. Since the mud is often light-colored, the streams
are sometimes described as “milky.” Where the amount of material carried
is great, much of it is dropped at a slight distance from the ice, the coarsest
being dropped first. Glacial streams are, as a rule, aggrading streams, and
therefore develop alluvial plains, called valley trains (Fig. 281 and 282), or
where they enter lakes (Fig. 283), bays, or other streams, deltas. In its
transportation, the river-borne drift is assorted; after its deposition, it is
stratified. True glacial deposits in the upper part of a mountain valley are,
therefore, often continued below by glacio-fluvial deposits derived from the
same source.
Fig. 281.—Alluviation by glacial stream: Nicolai Creek, Alaska. (Schrader, U. S. Geol.
Surv.)
The most common form of such deposit is a valley train (Fig. 281) of
glacial wash stretching indefinitely down the valley. The silt, sand, and
gravel of such trains can usually be distinguished from valley deposits of
non-glacial origin by the character of the material, as much of it is the
product of grinding, crushing, and fracture, rather than of ordinary surface
decay. Its materials are, therefore, fresh and often include rock material
which, if long exposed at the surface, would be decomposed or dissolved.
Page 367
Fig. 282.—Alluviation by glacial stream below Hidden glacier, Alaska. (Gilbert, U. S. Geol.
Surv.)
Where an ice sheet ends in a broad face, as did the ancient continental
glaciers, numerous streams flow from it and spread their débris in front of
the terminal moraine, forming a broad fringing sheet or “apron” (outwash
plain) along it. Where streams of considerable size form tunnels under or in
the ice, these may become more or less filled with wash, and when the ice
melts the aggraded channels appear as long ridges of gravel and sand
known as eskers (osars and serpentine kames and kames of authors. See
chapter on glacial period). It has been thought that similar ridges are
sometimes formed in valleys cut in the ice from top to bottom, and even
that they arise from gravel and sand lodged in superglacial channels. The
latter at least is probably rare, as the surface streams usually have high
gradients, swift currents, and smooth bottoms, and hence give little
opportunity for lodgment. In the case of ice-sheets, too, in connection with
which eskers are chiefly developed, there is usually no surface material
except at the immediate edge, where the ice is thin and its layers upturned.
At the mouths of ice-tunnels or ice-channels, especially where they end
against terminal moraines, sands and gravels are liable to be bunched in
quantity, giving rise, after the adjacent ice has melted, to peculiar hills and
hollows of the knob-and-basin type. The hills and short ridges are known as
kames (see glacial period). Subglacial streams may leave washed and
Surv.)
Where an ice sheet ends in a broad face, as did the ancient continental
glaciers, numerous streams flow from it and spread their débris in front of
the terminal moraine, forming a broad fringing sheet or “apron” (outwash
plain) along it. Where streams of considerable size form tunnels under or in
the ice, these may become more or less filled with wash, and when the ice
melts the aggraded channels appear as long ridges of gravel and sand
known as eskers (osars and serpentine kames and kames of authors. See
chapter on glacial period). It has been thought that similar ridges are
sometimes formed in valleys cut in the ice from top to bottom, and even
that they arise from gravel and sand lodged in superglacial channels. The
latter at least is probably rare, as the surface streams usually have high
gradients, swift currents, and smooth bottoms, and hence give little
opportunity for lodgment. In the case of ice-sheets, too, in connection with
which eskers are chiefly developed, there is usually no surface material
except at the immediate edge, where the ice is thin and its layers upturned.
At the mouths of ice-tunnels or ice-channels, especially where they end
against terminal moraines, sands and gravels are liable to be bunched in
quantity, giving rise, after the adjacent ice has melted, to peculiar hills and
hollows of the knob-and-basin type. The hills and short ridges are known as
kames (see glacial period). Subglacial streams may leave washed and
Page 368
assorted material in their tracks under the ice, and this is sometimes buried
under deposits made by the ice itself, so that glacio-fluvial and glacial
deposits are interbedded.
Fig. 283.—Delta at Isola, Lake of Sils, Engadine, Switzerland. (Reid.)
ICEBERGS.
When glaciers advance into water, the depth of which approaches their
thickness, their ends are broken off (Fig. 284), and the detached masses
float away as icebergs (Fig. 285). Many of the bergs are overturned, or at
least tilted, as they set sail. If this does not happen at the outset, it is likely
to occur later as the result of the melting and wave-cutting which disturb
their equilibrium. The great majority of bergs do not travel far before losing
all trace of stony and earthy débris, but the finding of glacial material in
dredgings far south of all glaciers shows that they occasionally carry stones
far from land.
under deposits made by the ice itself, so that glacio-fluvial and glacial
deposits are interbedded.
Fig. 283.—Delta at Isola, Lake of Sils, Engadine, Switzerland. (Reid.)
ICEBERGS.
When glaciers advance into water, the depth of which approaches their
thickness, their ends are broken off (Fig. 284), and the detached masses
float away as icebergs (Fig. 285). Many of the bergs are overturned, or at
least tilted, as they set sail. If this does not happen at the outset, it is likely
to occur later as the result of the melting and wave-cutting which disturb
their equilibrium. The great majority of bergs do not travel far before losing
all trace of stony and earthy débris, but the finding of glacial material in
dredgings far south of all glaciers shows that they occasionally carry stones
far from land.
Page 369
Fig. 284.—End of Muir glacier, Alaska. (Reid.)
THE INTIMATE STRUCTURE AND THE MOVEMENT OF
GLACIERS.
With the preceding account of glaciers in mind, we may return to a closer
study of their origin, their intimate structure, and their mode of motion. The
key to this study is the thesis that a glacier is a mass of crystalline rock—the
purest and simplest type of crystalline rock known—since it is made up of a
single mineral of simple composition and rare purity, which never appears
in a solid state except in the crystalline form.
The growth and constitution of a glacier.—The origin and history of a
glacier is little more than the origin and aggregate history of the crystals
that compose it. The fundamental conception of a glacier is therefore best
obtained by tracing the growth of its constituent crystals. A basal fact ever
to be kept in mind is that water in the solid form is always controlled by
crystalline forces. When it solidifies from the vapor of the atmosphere it
takes the form of separate crystals (Figs. 286–291). Perfect forms are
developed only when the flakes fall quietly through a saturated atmosphere
which allows them to grow as they descend. Under other conditions, the
crystals are imperfect in growth and are mutilated by impact. But however
modified, they are always crystals. The molecules are arranged on the
hexagonal plan, and, as the expansive power of freezing water shows, the
arrangement is controlled by a strong force. Once the definite crystalline
arrangement is established, the molecules can be displaced only by
relatively great force.
THE INTIMATE STRUCTURE AND THE MOVEMENT OF
GLACIERS.
With the preceding account of glaciers in mind, we may return to a closer
study of their origin, their intimate structure, and their mode of motion. The
key to this study is the thesis that a glacier is a mass of crystalline rock—the
purest and simplest type of crystalline rock known—since it is made up of a
single mineral of simple composition and rare purity, which never appears
in a solid state except in the crystalline form.
The growth and constitution of a glacier.—The origin and history of a
glacier is little more than the origin and aggregate history of the crystals
that compose it. The fundamental conception of a glacier is therefore best
obtained by tracing the growth of its constituent crystals. A basal fact ever
to be kept in mind is that water in the solid form is always controlled by
crystalline forces. When it solidifies from the vapor of the atmosphere it
takes the form of separate crystals (Figs. 286–291). Perfect forms are
developed only when the flakes fall quietly through a saturated atmosphere
which allows them to grow as they descend. Under other conditions, the
crystals are imperfect in growth and are mutilated by impact. But however
modified, they are always crystals. The molecules are arranged on the
hexagonal plan, and, as the expansive power of freezing water shows, the
arrangement is controlled by a strong force. Once the definite crystalline
arrangement is established, the molecules can be displaced only by
relatively great force.
Page 370
Fig. 285.—An iceberg, west coast of Greenland.
Snow crystals often continue to grow so long as they are in the
atmosphere; but if they pass through an under-saturated stratum of air or a
stratum whose temperature is above 32° Fahr., they suffer from evaporation
or melting. When they reach the ground, the processes of growth and
decadence continue, and the crystals grow or diminish according to
circumstances.
A glacier is a colossal aggregation of crystals grown from snowflakes to
granules of much greater sizes. The microscopic study of new-fallen snow
reveals the mode of change from flakes to granules. The slender points and
angles of the former yield to melting and evaporation more than the more
massive central portions, and this change probably illustrates a law of vital
importance. It may often be seen that the water melted from the periphery
of a flake gathers about its center, and if the temperature be right, it freezes
there. This is a first step toward the pronounced granulation of snow which
has lain for some time on the ground. If measured systematically from day
to day, the larger granules taken from beneath the surface of this coarse-
grained snow are found to be growing. In a series of experiments[133] to
determine the law of growth it was found that when the temperature of the
atmosphere was above the melting-point the growth was appreciably more
rapid than when the air was colder, but there was, on the average, an
increase under all conditions of temperature. A portion of this average
increase of the larger granules appears to come from the diminution and
destruction of the smaller ones, for the total number of granules steadily
Snow crystals often continue to grow so long as they are in the
atmosphere; but if they pass through an under-saturated stratum of air or a
stratum whose temperature is above 32° Fahr., they suffer from evaporation
or melting. When they reach the ground, the processes of growth and
decadence continue, and the crystals grow or diminish according to
circumstances.
A glacier is a colossal aggregation of crystals grown from snowflakes to
granules of much greater sizes. The microscopic study of new-fallen snow
reveals the mode of change from flakes to granules. The slender points and
angles of the former yield to melting and evaporation more than the more
massive central portions, and this change probably illustrates a law of vital
importance. It may often be seen that the water melted from the periphery
of a flake gathers about its center, and if the temperature be right, it freezes
there. This is a first step toward the pronounced granulation of snow which
has lain for some time on the ground. If measured systematically from day
to day, the larger granules taken from beneath the surface of this coarse-
grained snow are found to be growing. In a series of experiments[133] to
determine the law of growth it was found that when the temperature of the
atmosphere was above the melting-point the growth was appreciably more
rapid than when the air was colder, but there was, on the average, an
increase under all conditions of temperature. A portion of this average
increase of the larger granules appears to come from the diminution and
destruction of the smaller ones, for the total number of granules steadily
Page 371
diminishes. A portion of the growth doubtless comes from the moisture of
the atmosphere which penetrates the snow and another portion from the
moisture derived from surface melting; but beneath the surface of a large
body of snow the growth of the large granules is probably chiefly at the
expense of the small ones. To follow the process it should be noted that the
free surface of every granule is constantly throwing off particles of water-
vapor (evaporation); that the rate at which the particles are thrown off is
dependent, among other things, on the curvature of the surface, being
greater the sharper the curve; that the surfaces of the granules are at the
same time liable to receive and retain molecules thrown from other
granules, and that, other things being equal, the retention of particles also
depends on the curvature of the surface, the less curved surface retaining
more than the sharply curved one. Under these laws, it is obvious that the
larger granules of smaller curvature will lose less and gain more, on the
average, than the smaller granules of greater curvature. It follows that the
larger granules will grow at the expense of the smaller. It is also to be noted
that, other things being equal, small granules melt more readily than large
ones, and that where the temperature is nicely adjusted between melting and
freezing, the smaller may lose while the larger gain.
the atmosphere which penetrates the snow and another portion from the
moisture derived from surface melting; but beneath the surface of a large
body of snow the growth of the large granules is probably chiefly at the
expense of the small ones. To follow the process it should be noted that the
free surface of every granule is constantly throwing off particles of water-
vapor (evaporation); that the rate at which the particles are thrown off is
dependent, among other things, on the curvature of the surface, being
greater the sharper the curve; that the surfaces of the granules are at the
same time liable to receive and retain molecules thrown from other
granules, and that, other things being equal, the retention of particles also
depends on the curvature of the surface, the less curved surface retaining
more than the sharply curved one. Under these laws, it is obvious that the
larger granules of smaller curvature will lose less and gain more, on the
average, than the smaller granules of greater curvature. It follows that the
larger granules will grow at the expense of the smaller. It is also to be noted
that, other things being equal, small granules melt more readily than large
ones, and that where the temperature is nicely adjusted between melting and
freezing, the smaller may lose while the larger gain.
Page 372
Figs. 286–91.—Snowflakes. (Photographed by W. A. Bentley.)
Another factor that enters into the process is that of pressure and tension.
The granules are compressed at the points of contact and put under tension
at points not in contact, and the pressure and tension are, on the average,
likely to be relatively greatest for the smallest granules. Tension increases
the tendency to evaporation and adds its effects to curvature, and the
capillary spaces adjoining the points of contact probably favor
condensation. Ice expands in crystallizing and pressure reduces the melting-
point, while tension raises it. The effect of this is slight (p. 276), and it
probably plays little part in glacial action, but it is to be correlated with the
much more important fact that compression produces heat which may raise
the temperature of the ice to the melting-point, while tension may reduce
the temperature to or below freezing. There is therefore a tendency for the
ice to melt at the points of contact and compression, and for the water so
produced to refreeze at adjacent points where the surface is under tension.
Another factor that enters into the process is that of pressure and tension.
The granules are compressed at the points of contact and put under tension
at points not in contact, and the pressure and tension are, on the average,
likely to be relatively greatest for the smallest granules. Tension increases
the tendency to evaporation and adds its effects to curvature, and the
capillary spaces adjoining the points of contact probably favor
condensation. Ice expands in crystallizing and pressure reduces the melting-
point, while tension raises it. The effect of this is slight (p. 276), and it
probably plays little part in glacial action, but it is to be correlated with the
much more important fact that compression produces heat which may raise
the temperature of the ice to the melting-point, while tension may reduce
the temperature to or below freezing. There is therefore a tendency for the
ice to melt at the points of contact and compression, and for the water so
produced to refreeze at adjacent points where the surface is under tension.
Page 373
This process becomes effective beneath a considerable body of snow, and
here the granules gradually lose the spheroidal form assumed in the early
stages of granulation and become irregular polyhedrons interlocked into a
more or less solid mass.
A third factor is also to be recognized, though its effectiveness is
unknown. Under severe wind pressure, air penetrates porous bodies with
appreciable facility. The “breathing” of soils and the curious phenomena of
“blowing-wells” and “blowing-caves” teach us of the effective penetration
and extrusion of the air under variations of barometric pressure. In the
snow-fields, and in the more granular portions of glaciers near their heads,
the porosity is doubtless sufficient to allow of the appreciable penetration of
the atmosphere. During a part of the time, the probable effect is the
condensation within the ice of moisture from the air, and during another
part, evaporation from the ice. These alternating processes are attended by
oscillations of temperature. While the balance between loss and gain of
substance may be immaterial, the oscillating nature of the process and the
fluctuations of temperature are probably favorable to granular change.
Whether these processes furnish an adequate explanation of the changes
or not, the observed fact is that there are all gradations from snowflakes and
pellets into granular névé, and thence into glacier granules
(Gletscherkörner), varying in size up to that of filberts and walnuts, and
even beyond. In coherence, these aggregations may vary from the early
slightly coherent granular stage, where the grains are small and spheroidal,
to the ice stage, where the cohesion has become strong through the
interlocking growths of the large granules. Even when the mass has become
seemingly solid ice, sufficient space is usually left between the granules to
give the dispersive reflection to light which imparts to glacier ice its
distinctive whitish color.
The arrangement of the crystal axes.—The most radical difference
between glacier ice and ice formed directly from water is in the
arrangement (orientation) of the crystals. In the ice formed on undisturbed
water, the bases of the crystals are at the surface and their principal axes are
vertical, as shown by Mügge.[134] As they grow, the crystal prisms extend
downwards. This gives a columnar or prismatic structure to the ice, well
seen when it is “honeycombed” by partial melting. In the glacier, on the
other hand, the crystals, starting from snowflakes, have their axes turned in
here the granules gradually lose the spheroidal form assumed in the early
stages of granulation and become irregular polyhedrons interlocked into a
more or less solid mass.
A third factor is also to be recognized, though its effectiveness is
unknown. Under severe wind pressure, air penetrates porous bodies with
appreciable facility. The “breathing” of soils and the curious phenomena of
“blowing-wells” and “blowing-caves” teach us of the effective penetration
and extrusion of the air under variations of barometric pressure. In the
snow-fields, and in the more granular portions of glaciers near their heads,
the porosity is doubtless sufficient to allow of the appreciable penetration of
the atmosphere. During a part of the time, the probable effect is the
condensation within the ice of moisture from the air, and during another
part, evaporation from the ice. These alternating processes are attended by
oscillations of temperature. While the balance between loss and gain of
substance may be immaterial, the oscillating nature of the process and the
fluctuations of temperature are probably favorable to granular change.
Whether these processes furnish an adequate explanation of the changes
or not, the observed fact is that there are all gradations from snowflakes and
pellets into granular névé, and thence into glacier granules
(Gletscherkörner), varying in size up to that of filberts and walnuts, and
even beyond. In coherence, these aggregations may vary from the early
slightly coherent granular stage, where the grains are small and spheroidal,
to the ice stage, where the cohesion has become strong through the
interlocking growths of the large granules. Even when the mass has become
seemingly solid ice, sufficient space is usually left between the granules to
give the dispersive reflection to light which imparts to glacier ice its
distinctive whitish color.
The arrangement of the crystal axes.—The most radical difference
between glacier ice and ice formed directly from water is in the
arrangement (orientation) of the crystals. In the ice formed on undisturbed
water, the bases of the crystals are at the surface and their principal axes are
vertical, as shown by Mügge.[134] As they grow, the crystal prisms extend
downwards. This gives a columnar or prismatic structure to the ice, well
seen when it is “honeycombed” by partial melting. In the glacier, on the
other hand, the crystals, starting from snowflakes, have their axes turned in
Page 374
various directions according to the accidents of their fall; and as the snow
develops into ice, the principal axes of the crystals continue to lie in all
directions. Hence glacier ice, unlike pond ice, cannot usually be split along
definite planes, except where cleavage planes are subsequently developed
by extraneous agencies.
Figures to illustrate the method of deformation of ice crystals.
While the crystals of a glacier usually have their principal axes in various
directions, there appears to be a tendency for them to approach parallelism
in certain positions, especially in the basal parts of a glacier near its
terminus. Observations on this point are not so full and critical as could be
desired, but it is probable that the parallel orientation is partly general, and
due to the vertical pressure of the ice, and partly special and local, and
connected with the shearing planes and foliation.
The bearing of this partial parallelism of the crystals on shearing and
foliation is supposed to reside in the fact that a crystal of ice is made up of a
series of plates arranged at right angles to the principal axis of the crystal.
These plates may be likened to a pile of cards, the principal axis being
represented by a line vertical to them. If a cube be cut from a large crystal
of ice, it will behave much like a cube cut from the pile of cards. If the cube
be so placed that its plates are horizontal (Fig. 291a), and if it be rested on
supports at two edges and heavily weighted in the middle, it will sag, the
plates sliding slightly over one another so as to give oblique ends, but in
this case the cube offers considerable resistance to deformation. If the cube
be so placed that the plates stand on edge, each reaching from support to
support (Fig. 291b), it will offer very great resistance to deformation; but if
the plates be vertical and transverse to the line joining the supports, as in
Fig. 291c, the middle portion will sag under very moderate weighting by
develops into ice, the principal axes of the crystals continue to lie in all
directions. Hence glacier ice, unlike pond ice, cannot usually be split along
definite planes, except where cleavage planes are subsequently developed
by extraneous agencies.
Figures to illustrate the method of deformation of ice crystals.
While the crystals of a glacier usually have their principal axes in various
directions, there appears to be a tendency for them to approach parallelism
in certain positions, especially in the basal parts of a glacier near its
terminus. Observations on this point are not so full and critical as could be
desired, but it is probable that the parallel orientation is partly general, and
due to the vertical pressure of the ice, and partly special and local, and
connected with the shearing planes and foliation.
The bearing of this partial parallelism of the crystals on shearing and
foliation is supposed to reside in the fact that a crystal of ice is made up of a
series of plates arranged at right angles to the principal axis of the crystal.
These plates may be likened to a pile of cards, the principal axis being
represented by a line vertical to them. If a cube be cut from a large crystal
of ice, it will behave much like a cube cut from the pile of cards. If the cube
be so placed that its plates are horizontal (Fig. 291a), and if it be rested on
supports at two edges and heavily weighted in the middle, it will sag, the
plates sliding slightly over one another so as to give oblique ends, but in
this case the cube offers considerable resistance to deformation. If the cube
be so placed that the plates stand on edge, each reaching from support to
support (Fig. 291b), it will offer very great resistance to deformation; but if
the plates be vertical and transverse to the line joining the supports, as in
Fig. 291c, the middle portion will sag under very moderate weighting by
Page 375
the sliding of the plates on one another, and in a comparatively short time
the middle portion may be pushed entirely out, dividing the cube. These
properties have been demonstrated by McConnel[135] and Mügge, and they
appear to throw light on certain phases of the action of glaciers that are
most pronounced in their basal parts, and are best illustrated in arctic
glaciers.
The Probable Fundamental Element in Glacial Motion.
Melting and freezing.—It has already been shown (p. 279) that the
initial or fundamental cause of glacial motion must be operative at the
heads of glaciers where the temperature is lowest and the material most
loosely granular. In this condition, there is reason to believe that motion
takes place between the grains, rather than by their distortion through the
displacement of their laminæ. The fact that the granular structure is not
destroyed, as it would be by the indefinite sliding of the crystal plates over
each other, sustains this view. The inference is that the gliding planes play a
notable rôle in glacial movement only in the basal parts of the lower ends of
glaciers, where the greatest thrusts are developed, and where the granules
have become largest and most completely interlocked. At the heads of
glaciers, where motion is initiated, there may be great downward pressure,
but not vigorous thrusts from behind, and probably only moderate thrusts
developed within the body itself. There seems therefore no escape from the
conclusion that the primal cause of glacial motion is one which may operate
even under the relatively low temperatures, the relatively dry conditions,
and the relatively granular textures which affect the heads of glaciers. These
considerations lead to the view that movement takes place by the minute
individual movements of the grains upon one another. While they are in the
spheroidal form, as in the névé, this would not seem to be at all difficult.
They may rotate and slide over each other as the weight of the snow
increases; but as they become interlocked by growth, both rotation and
sliding must apparently encounter more resistance. The amount of rotary
motion required of an individual granule is, however, surprisingly small,
and the meltings and refreezings incident to shifting pressures and tensions,
and to the growth of the granules, seem adequate to meet the requirements.
In order to account for a movement of three feet per day in a glacier six
miles long, the mean motion of the average granule relative to its neighbor
the middle portion may be pushed entirely out, dividing the cube. These
properties have been demonstrated by McConnel[135] and Mügge, and they
appear to throw light on certain phases of the action of glaciers that are
most pronounced in their basal parts, and are best illustrated in arctic
glaciers.
The Probable Fundamental Element in Glacial Motion.
Melting and freezing.—It has already been shown (p. 279) that the
initial or fundamental cause of glacial motion must be operative at the
heads of glaciers where the temperature is lowest and the material most
loosely granular. In this condition, there is reason to believe that motion
takes place between the grains, rather than by their distortion through the
displacement of their laminæ. The fact that the granular structure is not
destroyed, as it would be by the indefinite sliding of the crystal plates over
each other, sustains this view. The inference is that the gliding planes play a
notable rôle in glacial movement only in the basal parts of the lower ends of
glaciers, where the greatest thrusts are developed, and where the granules
have become largest and most completely interlocked. At the heads of
glaciers, where motion is initiated, there may be great downward pressure,
but not vigorous thrusts from behind, and probably only moderate thrusts
developed within the body itself. There seems therefore no escape from the
conclusion that the primal cause of glacial motion is one which may operate
even under the relatively low temperatures, the relatively dry conditions,
and the relatively granular textures which affect the heads of glaciers. These
considerations lead to the view that movement takes place by the minute
individual movements of the grains upon one another. While they are in the
spheroidal form, as in the névé, this would not seem to be at all difficult.
They may rotate and slide over each other as the weight of the snow
increases; but as they become interlocked by growth, both rotation and
sliding must apparently encounter more resistance. The amount of rotary
motion required of an individual granule is, however, surprisingly small,
and the meltings and refreezings incident to shifting pressures and tensions,
and to the growth of the granules, seem adequate to meet the requirements.
In order to account for a movement of three feet per day in a glacier six
miles long, the mean motion of the average granule relative to its neighbor
Page 376
would be, roundly, ¹⁄₁₀₀₀₀ of its own diameter per day, or one diameter in
10,000 days; in other words, it would change its relations to its neighbors
to the extent of its diameter in about thirty years. A change of so great
slowness under the conditions of granular alteration can scarcely be thought
incredible, or even improbable, in spite of the interlocking which the
granules may develop. The movement is supposed to be permitted chiefly
by the temporary passage of minute portions of the granules into the fluid
form at the points of greatest compression, the transfer of the moisture to
adjoining points, and its resolidification. The points of greatest compression
are obviously just those whose yielding most promotes motion, and a
successive yielding of the points that come in succession to oppose motion
most (and thus to receive the greatest stresses) permits continuous motion.
It is merely necessary to assume that the gravity of the accumulated mass is
sufficient to produce the minute temporary liquefaction at the points of
greatest stress, the result being accomplished not so much by the lowering
of the melting-point as by the development of heat by pressure.
Fig. 292.—Portion of the east face of Bowdoin glacier, North Greenland, showing oblique
upward thrust, with shear.
10,000 days; in other words, it would change its relations to its neighbors
to the extent of its diameter in about thirty years. A change of so great
slowness under the conditions of granular alteration can scarcely be thought
incredible, or even improbable, in spite of the interlocking which the
granules may develop. The movement is supposed to be permitted chiefly
by the temporary passage of minute portions of the granules into the fluid
form at the points of greatest compression, the transfer of the moisture to
adjoining points, and its resolidification. The points of greatest compression
are obviously just those whose yielding most promotes motion, and a
successive yielding of the points that come in succession to oppose motion
most (and thus to receive the greatest stresses) permits continuous motion.
It is merely necessary to assume that the gravity of the accumulated mass is
sufficient to produce the minute temporary liquefaction at the points of
greatest stress, the result being accomplished not so much by the lowering
of the melting-point as by the development of heat by pressure.
Fig. 292.—Portion of the east face of Bowdoin glacier, North Greenland, showing oblique
upward thrust, with shear.
Page 377
This conception of glacial “flowage” involves only the momentary
liquefaction of minute portions of the mass, while the ice as a whole
remains rigid, as its crystalline nature requires. Instead of assigning a slow
viscous fluidity like that of asphalt to the whole mass, which seems
inconsistent with its crystalline character, it assigns a free fluidity to a
succession of particles that form only a minute fraction of the whole at any
instant.
This conception is consistent with the retention of the granular condition
of the ice, with the heterogeneous (in the main) orientation of the crystals,
with the rigidity and brittleness of the ice, and with its strictly crystalline
character, a character which a viscous liquid does not possess however
much its high viscosity may make it resemble a rigid body.
Accumulated motion in the terminal part of a glacier.—However
slight the relative motion of one granule on its neighbor, the granules in any
part of a glacier partake in the accumulated motion of all parts nearer the
source, and hence all are thrust forward. Herein appears to lie the distinctive
nature of glacial movement. Each part of a stream of water feels the
hydrostatic pressure of neighboring parts (theoretically equal in all
directions) and the momentum of motion, but not the rigid thrust of the
mass behind. Lava streams are good types of viscous fluids flowing in
masses comparable to those of glaciers and on similar slopes, and, in their
last stages, at similar rates, but their special modes of flow and their effects
on the sides and bottoms of their paths are radically different from those of
glaciers. Forceful abrasion, and particularly the rigid holding of imbedded
stones while they score and groove the rock beneath, is unknown in lava
streams and is scarcely conceivable. There is, so far as we know, no
experimental or natural evidence that any typical viscous body in flowing
over a rugose bottom detaches and picks up fragments and holds them as
graving tools in its base so fixedly as to cut deep, long, straight grooves in
the hard bottom over which it flows. It would seem that competency to do
this peculiar class of work, which is distinctive of glaciers, should be
demonstrated before the viscous theory of glacial movement is accepted as
even a good working hypothesis. Somewhat in contrast with viscous
movement, it is conceived that a glacier is thrust forward rigidly by internal
elongation, shears forcibly over its sides and bottoms, and leaves its
distinctive marks upon them.
liquefaction of minute portions of the mass, while the ice as a whole
remains rigid, as its crystalline nature requires. Instead of assigning a slow
viscous fluidity like that of asphalt to the whole mass, which seems
inconsistent with its crystalline character, it assigns a free fluidity to a
succession of particles that form only a minute fraction of the whole at any
instant.
This conception is consistent with the retention of the granular condition
of the ice, with the heterogeneous (in the main) orientation of the crystals,
with the rigidity and brittleness of the ice, and with its strictly crystalline
character, a character which a viscous liquid does not possess however
much its high viscosity may make it resemble a rigid body.
Accumulated motion in the terminal part of a glacier.—However
slight the relative motion of one granule on its neighbor, the granules in any
part of a glacier partake in the accumulated motion of all parts nearer the
source, and hence all are thrust forward. Herein appears to lie the distinctive
nature of glacial movement. Each part of a stream of water feels the
hydrostatic pressure of neighboring parts (theoretically equal in all
directions) and the momentum of motion, but not the rigid thrust of the
mass behind. Lava streams are good types of viscous fluids flowing in
masses comparable to those of glaciers and on similar slopes, and, in their
last stages, at similar rates, but their special modes of flow and their effects
on the sides and bottoms of their paths are radically different from those of
glaciers. Forceful abrasion, and particularly the rigid holding of imbedded
stones while they score and groove the rock beneath, is unknown in lava
streams and is scarcely conceivable. There is, so far as we know, no
experimental or natural evidence that any typical viscous body in flowing
over a rugose bottom detaches and picks up fragments and holds them as
graving tools in its base so fixedly as to cut deep, long, straight grooves in
the hard bottom over which it flows. It would seem that competency to do
this peculiar class of work, which is distinctive of glaciers, should be
demonstrated before the viscous theory of glacial movement is accepted as
even a good working hypothesis. Somewhat in contrast with viscous
movement, it is conceived that a glacier is thrust forward rigidly by internal
elongation, shears forcibly over its sides and bottoms, and leaves its
distinctive marks upon them.
Page 378
Fig. 293.—Shearing plane well defined. A Spitsbergen glacier. (Hamberg.)
Auxiliary Elements.
Shearing.—In the lower portion of a glacier where normally the thrusts
are greatest, the granules fewest, and their interlocking most intimate,
shearing takes place within the ice itself. This is illustrated by the
accompanying Figs., 292–295. The shearing results in the foliation of the
ice and in the forcing of débris between the sheared layers. Thus the ice
becomes loaded in a special englacial or baso-englacial fashion, as
previously mentioned and illustrated in Fig. 268.
Within the zone of shearing, it is probable that the gliding planes of the
crystals come into effective function. It is thought that the combined effect
of the vertical pressure, the forward thrust, and the basal drag of the ice,
may be to increase the number of granules whose gliding planes are parallel
to the glacier’s bottom. At any rate, Drygalski reports[136] that there is a
tendency to such an arrangement in the basal portion of the Greenland
glaciers at their borders. It is conceived that where strong thrusts are
brought to bear upon such a mass of granules, those whose gliding planes
Auxiliary Elements.
Shearing.—In the lower portion of a glacier where normally the thrusts
are greatest, the granules fewest, and their interlocking most intimate,
shearing takes place within the ice itself. This is illustrated by the
accompanying Figs., 292–295. The shearing results in the foliation of the
ice and in the forcing of débris between the sheared layers. Thus the ice
becomes loaded in a special englacial or baso-englacial fashion, as
previously mentioned and illustrated in Fig. 268.
Within the zone of shearing, it is probable that the gliding planes of the
crystals come into effective function. It is thought that the combined effect
of the vertical pressure, the forward thrust, and the basal drag of the ice,
may be to increase the number of granules whose gliding planes are parallel
to the glacier’s bottom. At any rate, Drygalski reports[136] that there is a
tendency to such an arrangement in the basal portion of the Greenland
glaciers at their borders. It is conceived that where strong thrusts are
brought to bear upon such a mass of granules, those whose gliding planes
Page 379
are parallel to the direction of thrust are strained with sufficient intensity to
cause the plates to slide over each other, while those which are not parallel
to the direction of thrust are either rotated into parallelism—when they also
yield—or are pressed aside out of the plane of shear. As previously noted,
shearing is observed to occur chiefly where the ice below the plane of
shearing is protected more or less from the force of the thrust. It perhaps
also occurs where the basal ice becomes so overloaded with débris that it is
incapable of ready movement.
It is also probable that sharp
differential strain and shearing are
developed at the level where the
surface-water of the warm season,
descending into the ice, reaches
the zone of freezing. The
expanding of the freezing water at
the upper limit of the cold zone
may cause the layer expanded by
it to shear over that below. As the
level of freezing is lowered with
the advance of the warm season,
the zone of shearing also sinks.
This may be regarded as an
auxiliary agency of shearing, of
application to a special horizon.
High temperature and water.
—In the zone of waste, a higher
temperature and more water lend
their aid to the fundamental
agencies of movement, and there
Fig. 294.—Portion of the lateral margin of a is need for these aids to promote a
North Greenland glacier. Shows upturning of
the layers at the base, the cleanness of the ice proportionate movement, for here
above the bottom, and, possibly, shearing. the granules are more intimately
interlocked and the ice more compact and inherently more solid and rigid.
The average temperature is, however, near the melting-point (p. 276), and
during the warm season the ice is bathed in water so that the necessary
changes in the crystals are facilitated, and movement apparently takes place
cause the plates to slide over each other, while those which are not parallel
to the direction of thrust are either rotated into parallelism—when they also
yield—or are pressed aside out of the plane of shear. As previously noted,
shearing is observed to occur chiefly where the ice below the plane of
shearing is protected more or less from the force of the thrust. It perhaps
also occurs where the basal ice becomes so overloaded with débris that it is
incapable of ready movement.
It is also probable that sharp
differential strain and shearing are
developed at the level where the
surface-water of the warm season,
descending into the ice, reaches
the zone of freezing. The
expanding of the freezing water at
the upper limit of the cold zone
may cause the layer expanded by
it to shear over that below. As the
level of freezing is lowered with
the advance of the warm season,
the zone of shearing also sinks.
This may be regarded as an
auxiliary agency of shearing, of
application to a special horizon.
High temperature and water.
—In the zone of waste, a higher
temperature and more water lend
their aid to the fundamental
agencies of movement, and there
Fig. 294.—Portion of the lateral margin of a is need for these aids to promote a
North Greenland glacier. Shows upturning of
the layers at the base, the cleanness of the ice proportionate movement, for here
above the bottom, and, possibly, shearing. the granules are more intimately
interlocked and the ice more compact and inherently more solid and rigid.
The average temperature is, however, near the melting-point (p. 276), and
during the warm season the ice is bathed in water so that the necessary
changes in the crystals are facilitated, and movement apparently takes place
Page 380
even more readily than in the more open granular portion of lower
temperature and dryer state. The extraordinary movements of certain
tongues of ice in some of the great fiords of Greenland are probably due to
the convergence of very thick slow-moving ice from the interior into basins
leading down to the fiords. Into the same basins a large amount of surface-
water is concentrated at the same time, with the result that the thick ice,
bathed with water and having a high gradient, develops unusual velocity
during the warm season.
Fig. 295.—Lateral margin of a North Greenland glacier, Inglefield Gulf region. The
overhanging edges of the successive layers are not altogether the result of shear. They are
due in part at least to differential melting along the lines where débris comes to the
surface. The débris planes may be shear planes.
Applications.—By a studious consideration of the coöperation of the
auxiliary agencies with the fundamental ones, the peculiarities of glacial
movement may apparently be explained. In regions of intense cold, where a
dry state and low temperature prevail, as in the heart of Greenland, the
snow-ice mass may accumulate to extraordinary thicknesses, for the burden
temperature and dryer state. The extraordinary movements of certain
tongues of ice in some of the great fiords of Greenland are probably due to
the convergence of very thick slow-moving ice from the interior into basins
leading down to the fiords. Into the same basins a large amount of surface-
water is concentrated at the same time, with the result that the thick ice,
bathed with water and having a high gradient, develops unusual velocity
during the warm season.
Fig. 295.—Lateral margin of a North Greenland glacier, Inglefield Gulf region. The
overhanging edges of the successive layers are not altogether the result of shear. They are
due in part at least to differential melting along the lines where débris comes to the
surface. The débris planes may be shear planes.
Applications.—By a studious consideration of the coöperation of the
auxiliary agencies with the fundamental ones, the peculiarities of glacial
movement may apparently be explained. In regions of intense cold, where a
dry state and low temperature prevail, as in the heart of Greenland, the
snow-ice mass may accumulate to extraordinary thicknesses, for the burden
Page 381
of movement seems to be thrown almost wholly upon compression, with
the slight aid of molecular changes due to internal evaporation and allied
inefficient processes. Since the temperature in the upper part of the ice is
very adverse (see p. 277), the compression must be great before it becomes
effective in melting the ice, and hence the great thickness of the mass
antecedent to much motion. Similar conditions more or less affect the heads
of alpine glaciers, though here the high gradients favor motion with lesser
thicknesses of ice; but in the lower reaches of alpine glaciers, where the
temperatures are near the melting-point, and the ice is bathed in water,
movement may take place in ice which is thin and compact.
If the views here presented are correct, there is also, near the end or edge
of a glacier, the coöperation of rigid thrust from behind with the tendency of
the mass to move on its own account. The latter is controlled by gravity, and
conforms in its results to laws of liquid flow. The former is a derived factor,
and is a mechanical thrust. This thrust is different from the pressure of the
upper part of a liquid stream on the lower part, because it is transmitted
through a body whose rigidity is effective, while the latter is transmitted on
the hydrostatic principle of equal pressure in all directions.
Corroborative Phenomena.
The conception of the glacier and its movement here presented explains
some of the anomalies that otherwise seem paradoxical. While a glacier in a
sense flows over a surface, it often cuts long, deep furrows in firm rock. It
is difficult to explain this if the ice be so yielding as to flow under its own
weight on a surface which is almost flat. If the mass is really viscous, its
hold on its imbedded débris should also be viscous, and a bowlder in the
bottom should be rotated in the yielding mass when its lower point catches
on the rock beneath, instead of being firmly held while a deep groove is cut.
This is more to the point since viscous fluids flow by a partially rotary
movement. If, on the other hand, the ice is always a rigid body which yields
only as its interlocking granules change their form by loss and gain, a rigid
hold on the imbedded rock at some times, and a yielding hold at others, is
intelligible, for on this view the nature of its hold is dependent on the
temperature and dryness of the ice. Stones in the base of a glacier may be
held with very great rigidity when the ice is dry, scoring the bottom with
much force, while they may be rotated with relative ease when the ice is
the slight aid of molecular changes due to internal evaporation and allied
inefficient processes. Since the temperature in the upper part of the ice is
very adverse (see p. 277), the compression must be great before it becomes
effective in melting the ice, and hence the great thickness of the mass
antecedent to much motion. Similar conditions more or less affect the heads
of alpine glaciers, though here the high gradients favor motion with lesser
thicknesses of ice; but in the lower reaches of alpine glaciers, where the
temperatures are near the melting-point, and the ice is bathed in water,
movement may take place in ice which is thin and compact.
If the views here presented are correct, there is also, near the end or edge
of a glacier, the coöperation of rigid thrust from behind with the tendency of
the mass to move on its own account. The latter is controlled by gravity, and
conforms in its results to laws of liquid flow. The former is a derived factor,
and is a mechanical thrust. This thrust is different from the pressure of the
upper part of a liquid stream on the lower part, because it is transmitted
through a body whose rigidity is effective, while the latter is transmitted on
the hydrostatic principle of equal pressure in all directions.
Corroborative Phenomena.
The conception of the glacier and its movement here presented explains
some of the anomalies that otherwise seem paradoxical. While a glacier in a
sense flows over a surface, it often cuts long, deep furrows in firm rock. It
is difficult to explain this if the ice be so yielding as to flow under its own
weight on a surface which is almost flat. If the mass is really viscous, its
hold on its imbedded débris should also be viscous, and a bowlder in the
bottom should be rotated in the yielding mass when its lower point catches
on the rock beneath, instead of being firmly held while a deep groove is cut.
This is more to the point since viscous fluids flow by a partially rotary
movement. If, on the other hand, the ice is always a rigid body which yields
only as its interlocking granules change their form by loss and gain, a rigid
hold on the imbedded rock at some times, and a yielding hold at others, is
intelligible, for on this view the nature of its hold is dependent on the
temperature and dryness of the ice. Stones in the base of a glacier may be
held with very great rigidity when the ice is dry, scoring the bottom with
much force, while they may be rotated with relative ease when the ice is
Page 382
wet. In short, the relation of the ice to the bowlders in its bottom varies
radically according to its dryness and temperature. A dry glacier is a rigid
glacier. A dry glacier is necessarily cold, and a cold glacier is necessarily
dry.
On the view here presented, a glacier should be more rigid in winter than
in summer, and the whole thickness of the glacier should experience this
rigidity chiefly at the ends and edges, where the relative thinness of the ice
permits the low temperature to reach its bottom. The motion in these parts
during the winter is, therefore, very small.
In this view may also be found an explanation of the movement of
glaciers for considerable distances on upward slopes, even when the surface
as well as the base is inclined backwards. So far does this go that
superglacial streams sometimes run for some distance backwards, i.e.
toward the heads of the glaciers, while in other places surface-waters are
collected into ponds and lakelets. Such a slope of the surface of ice is not
difficult to understand if the movement be due to thrust from behind, or if it
be occasioned by internal crystalline changes acting upon a rigid body; but
it must be regarded as very remarkable if the movement be that of a fluid
body, no matter how viscous, for the length of the acclivity is sometimes
several times the thickness of the ice. Crevassing and other evidences of
brittleness and rigidity find a ready elucidation under the view that the ice is
a really solid body at all times, and that its apparent fluency is due to the
momentary fluidity of small portions of the mass assumed in succession as
compression demands.
In addition to the considerations already adduced, it may be urged that a
glacier does not flow as a stiff liquid because its granules are not habitually
drawn out into elongated forms, as are cavities in lavas and plastic lumps in
viscous bodies. Flowage lines comparable to those in lavas are unknown in
glaciers.
All this is strictly consistent with our primary thesis, that a glacier is a
crystalline rock of the purest and simplest type, and that it never has other
than the crystalline state. This strictly crystalline character is incompatible
with viscous liquidity.
Other Views of Glacier Motion.[137]
radically according to its dryness and temperature. A dry glacier is a rigid
glacier. A dry glacier is necessarily cold, and a cold glacier is necessarily
dry.
On the view here presented, a glacier should be more rigid in winter than
in summer, and the whole thickness of the glacier should experience this
rigidity chiefly at the ends and edges, where the relative thinness of the ice
permits the low temperature to reach its bottom. The motion in these parts
during the winter is, therefore, very small.
In this view may also be found an explanation of the movement of
glaciers for considerable distances on upward slopes, even when the surface
as well as the base is inclined backwards. So far does this go that
superglacial streams sometimes run for some distance backwards, i.e.
toward the heads of the glaciers, while in other places surface-waters are
collected into ponds and lakelets. Such a slope of the surface of ice is not
difficult to understand if the movement be due to thrust from behind, or if it
be occasioned by internal crystalline changes acting upon a rigid body; but
it must be regarded as very remarkable if the movement be that of a fluid
body, no matter how viscous, for the length of the acclivity is sometimes
several times the thickness of the ice. Crevassing and other evidences of
brittleness and rigidity find a ready elucidation under the view that the ice is
a really solid body at all times, and that its apparent fluency is due to the
momentary fluidity of small portions of the mass assumed in succession as
compression demands.
In addition to the considerations already adduced, it may be urged that a
glacier does not flow as a stiff liquid because its granules are not habitually
drawn out into elongated forms, as are cavities in lavas and plastic lumps in
viscous bodies. Flowage lines comparable to those in lavas are unknown in
glaciers.
All this is strictly consistent with our primary thesis, that a glacier is a
crystalline rock of the purest and simplest type, and that it never has other
than the crystalline state. This strictly crystalline character is incompatible
with viscous liquidity.
Other Views of Glacier Motion.[137]
Page 383
While these views of glacial motion seem to us to best accord with the
known facts, they are not to be regarded as established in scientific opinion,
or as the views most commonly held. The mode of glacial motion has long
been a mooted question, and is still so regarded. The main alternative
interpretations that have been entertained are the following:
(1) In the early days of glacial studies De Saussure thought that glaciers
slid bodily on their beds;
(2) Charpentier and Agassiz referred the movement to the expansion of
descending water freezing within the glacier;
(3) Rendu and Forbes, followed by many, perhaps most, modern writers,
believed ice to be viscous, and that in sufficiently large masses it flows
under the influence of its own weight, like pitch or asphalt;
(4) Others, realizing the fundamental difference between crystalline ice
and a true viscous body, have fallen back on a vague notion of plasticity
which scarcely amounts to a definite hypothesis at all;
(5) Tyndall urged that the movement was accomplished by minute
repeated fracturing and regelation, appealing to the fact that broken pieces
of ice slightly pressed together at melting temperatures freeze together, but
neglecting the fact that this would destroy the integrity of the crystals;
(6) Moseley assigned the movement to a bodily expansion and
contraction of the glacier, analogous to the creeping of a mass of lead on a
roof;
(7) James Thompson demonstrated that pressure lowers the melting-
point, and while this effect is so small as probably to be ineffectual, it is
correlated with the very important fact that compression may cause melting,
which is not the case in most other rocks. He recognized that under pressure
partial liquefaction took place, that the water so liberated might be refrozen
as it escaped from pressure, and appears to have regarded this as a vital
factor;
(8) Croll held that the movement was due to a consecutive series of
molecular changes somewhat like the chain of chemical combinations in
electrolysis;
known facts, they are not to be regarded as established in scientific opinion,
or as the views most commonly held. The mode of glacial motion has long
been a mooted question, and is still so regarded. The main alternative
interpretations that have been entertained are the following:
(1) In the early days of glacial studies De Saussure thought that glaciers
slid bodily on their beds;
(2) Charpentier and Agassiz referred the movement to the expansion of
descending water freezing within the glacier;
(3) Rendu and Forbes, followed by many, perhaps most, modern writers,
believed ice to be viscous, and that in sufficiently large masses it flows
under the influence of its own weight, like pitch or asphalt;
(4) Others, realizing the fundamental difference between crystalline ice
and a true viscous body, have fallen back on a vague notion of plasticity
which scarcely amounts to a definite hypothesis at all;
(5) Tyndall urged that the movement was accomplished by minute
repeated fracturing and regelation, appealing to the fact that broken pieces
of ice slightly pressed together at melting temperatures freeze together, but
neglecting the fact that this would destroy the integrity of the crystals;
(6) Moseley assigned the movement to a bodily expansion and
contraction of the glacier, analogous to the creeping of a mass of lead on a
roof;
(7) James Thompson demonstrated that pressure lowers the melting-
point, and while this effect is so small as probably to be ineffectual, it is
correlated with the very important fact that compression may cause melting,
which is not the case in most other rocks. He recognized that under pressure
partial liquefaction took place, that the water so liberated might be refrozen
as it escaped from pressure, and appears to have regarded this as a vital
factor;
(8) Croll held that the movement was due to a consecutive series of
molecular changes somewhat like the chain of chemical combinations in
electrolysis;
Page 384
(9) Hugi, Eli de Beaumont, Bertin, Forel, and others thought that the
growth of the granules was the leading factor in the ice movement;
(10) McConnel and Mügge have made the gliding planes of the ice
crystals serve an important function in glacial movement.
It will be seen that the principle of partial liquefaction for which
Thompson laid the basis, the crystallization of descending water, urged by
Charpentier and Agassiz, and the granular growth on which Hugi,
Beaumont, Forel, and others founded their hypotheses, are incorporated in
the view already presented. Probably the agencies on which some of the
other views are based may also be participants in producing glacial motion,
sometimes as incidental factors, and sometimes perhaps as important ones,
for under different conditions, different agencies may play rôles of varying
importance. For example, in going over the brinks of precipices of
sufficient height, glaciers break into fragments which are re-cemented
below, and the “reconstructed” glacier moves on as before. Here fracture
and regelation are evident. The movement of the gliding planes of the ice
crystals over each other, which has been looked upon as a special kind of
viscoid movement, probably plays a large part in the shearing movements in
certain cases. But neither of these is probably a large factor in ordinary
glacial movement, and it seems highly improbable that any of them are
essential factors in the primary movements in the snow-fields where glacial
action begins.
growth of the granules was the leading factor in the ice movement;
(10) McConnel and Mügge have made the gliding planes of the ice
crystals serve an important function in glacial movement.
It will be seen that the principle of partial liquefaction for which
Thompson laid the basis, the crystallization of descending water, urged by
Charpentier and Agassiz, and the granular growth on which Hugi,
Beaumont, Forel, and others founded their hypotheses, are incorporated in
the view already presented. Probably the agencies on which some of the
other views are based may also be participants in producing glacial motion,
sometimes as incidental factors, and sometimes perhaps as important ones,
for under different conditions, different agencies may play rôles of varying
importance. For example, in going over the brinks of precipices of
sufficient height, glaciers break into fragments which are re-cemented
below, and the “reconstructed” glacier moves on as before. Here fracture
and regelation are evident. The movement of the gliding planes of the ice
crystals over each other, which has been looked upon as a special kind of
viscoid movement, probably plays a large part in the shearing movements in
certain cases. But neither of these is probably a large factor in ordinary
glacial movement, and it seems highly improbable that any of them are
essential factors in the primary movements in the snow-fields where glacial
action begins.
Page 385
CHAPTER VI.
THE WORK OF THE OCEAN.
The general facts concerning the depth of the ocean and the distribution
of its water have been given on a preceding page (p. 8), and the origin of
the ocean and the ocean basins is discussed in the second volume. This
chapter has to do primarily with the processes now going on in the sea and
its borders, in so far as they are of importance in the interpretation of
geologic history. The study of these processes is prefaced by a few words
concerning the amount and composition of the sea-water, the life of the
ocean, and the topography of its bed.[138]
Volume and composition.—Every 1000 parts of sea-water contain about
34.40 parts by weight of mineral matter in solution. The principal solids,
acids, and bases, combined according to the principles laid down by
Dittmar, are shown in the following table:[2]
Chloride of sodium 77.758
Chloride of magnesium 10.878
Sulphate of magnesium 4.737
Sulphate of calcium 3.600
Sulphate of potassium 2.465
Bromide of magnesium 0.217
Carbonate of calcium 0.345
————
Total salts 100.000
Expressed in terms of tons per cubic mile of sea-water, the composition
is as follows:[139]
Tons per Cubic Mile.
Chloride of sodium (NaCl) 117,434,000
Chloride of magnesium (MgCl2) 16,428,000
Sulphate of magnesium (MgSO4) 7,154,000
Sulphate of calcium (CaSO4) 5,437,000
THE WORK OF THE OCEAN.
The general facts concerning the depth of the ocean and the distribution
of its water have been given on a preceding page (p. 8), and the origin of
the ocean and the ocean basins is discussed in the second volume. This
chapter has to do primarily with the processes now going on in the sea and
its borders, in so far as they are of importance in the interpretation of
geologic history. The study of these processes is prefaced by a few words
concerning the amount and composition of the sea-water, the life of the
ocean, and the topography of its bed.[138]
Volume and composition.—Every 1000 parts of sea-water contain about
34.40 parts by weight of mineral matter in solution. The principal solids,
acids, and bases, combined according to the principles laid down by
Dittmar, are shown in the following table:[2]
Chloride of sodium 77.758
Chloride of magnesium 10.878
Sulphate of magnesium 4.737
Sulphate of calcium 3.600
Sulphate of potassium 2.465
Bromide of magnesium 0.217
Carbonate of calcium 0.345
————
Total salts 100.000
Expressed in terms of tons per cubic mile of sea-water, the composition
is as follows:[139]
Tons per Cubic Mile.
Chloride of sodium (NaCl) 117,434,000
Chloride of magnesium (MgCl2) 16,428,000
Sulphate of magnesium (MgSO4) 7,154,000
Sulphate of calcium (CaSO4) 5,437,000
Page 386
Tons per Cubic Mile.
Sulphate of potassium (K2SO4) 3,723,000
Bromide of magnesium (MgBr2) 328,000
Carbonate of calcium (CaCO3) 521,000
—————
For sea-water, total dissolved matter 151,025,000
Aside from the ingredients shown in the above tables, the presence of the
following has been proved: iodine, fluorine, phosphorus, silicon, boron,
silver, lead, copper, zinc, cobalt, nickel, iron, manganese, aluminum,
barium, strontium, arsenic, lithium, cæsium, rubidium, and gold. Oxygen,
nitrogen, and carbonic acid gas are also present in quantity. The amount of
carbonic acid is estimated to be 18 times as great as in the atmosphere.[140]
The amount of sea-water is estimated by Murray at 323,722,150 cubic
miles,[141] or about 15 times the volume of the land above sea-level. The
volume and composition of the sea-water being known, the amount of
mineral matter which it contains may be readily calculated. Assuming the
average specific gravity of the mineral matter in solution to be 2.5, the 3.5%
by weight becomes 1.4% by volume, and 1.4% of 323,722,150 cubic miles
is 4,532,110 cubic miles. This then represents the aggregate volume of
mineral matter in the sea if it were precipitated and compacted so as to have
an average specific gravity of 2.5. Assuming the average depth of the sea to
be 2076 fathoms (12,456 feet), as given by Murray, the mineral matter in
solution, if precipitated, would cover the ocean bottom to a depth of about
175 feet. Assuming the area of the land to be to that of the sea as 28 to 72,
this amount of mineral matter would make a layer about 450 feet deep over
the land. Its amount is equal to about 20% of that of all lands above sea-
level, and it falls but little short of that in all lands below 600 feet in
altitude. If it were precipitated and concentrated in the shallow waters about
the borders of the lands, it would fill the sea out to the depth of about 4000
feet, and would diminish its area by some 19,000,000 to 20,000,000 square
miles, an area which is more than ⅓ of the present land surface. In other
words, if the mineral matter in the sea-water were precipitated and
concentrated in the shallow waters about the lands, it would restore the
continental shelves to the land areas, and add an almost equal area beyond.
These comparisons may perhaps help to give some idea of the amount of
mineral matter in solution in the sea, but they give no more than a hint of
Sulphate of potassium (K2SO4) 3,723,000
Bromide of magnesium (MgBr2) 328,000
Carbonate of calcium (CaCO3) 521,000
—————
For sea-water, total dissolved matter 151,025,000
Aside from the ingredients shown in the above tables, the presence of the
following has been proved: iodine, fluorine, phosphorus, silicon, boron,
silver, lead, copper, zinc, cobalt, nickel, iron, manganese, aluminum,
barium, strontium, arsenic, lithium, cæsium, rubidium, and gold. Oxygen,
nitrogen, and carbonic acid gas are also present in quantity. The amount of
carbonic acid is estimated to be 18 times as great as in the atmosphere.[140]
The amount of sea-water is estimated by Murray at 323,722,150 cubic
miles,[141] or about 15 times the volume of the land above sea-level. The
volume and composition of the sea-water being known, the amount of
mineral matter which it contains may be readily calculated. Assuming the
average specific gravity of the mineral matter in solution to be 2.5, the 3.5%
by weight becomes 1.4% by volume, and 1.4% of 323,722,150 cubic miles
is 4,532,110 cubic miles. This then represents the aggregate volume of
mineral matter in the sea if it were precipitated and compacted so as to have
an average specific gravity of 2.5. Assuming the average depth of the sea to
be 2076 fathoms (12,456 feet), as given by Murray, the mineral matter in
solution, if precipitated, would cover the ocean bottom to a depth of about
175 feet. Assuming the area of the land to be to that of the sea as 28 to 72,
this amount of mineral matter would make a layer about 450 feet deep over
the land. Its amount is equal to about 20% of that of all lands above sea-
level, and it falls but little short of that in all lands below 600 feet in
altitude. If it were precipitated and concentrated in the shallow waters about
the borders of the lands, it would fill the sea out to the depth of about 4000
feet, and would diminish its area by some 19,000,000 to 20,000,000 square
miles, an area which is more than ⅓ of the present land surface. In other
words, if the mineral matter in the sea-water were precipitated and
concentrated in the shallow waters about the lands, it would restore the
continental shelves to the land areas, and add an almost equal area beyond.
These comparisons may perhaps help to give some idea of the amount of
mineral matter in solution in the sea, but they give no more than a hint of
Page 387
the importance of the solvent power of water in the general processes of
rock decay, for most of the substances carried to the sea in solution by
rivers are extracted from the water about as rapidly as they are supplied.
Thus calcium carbonate is about twenty times as abundant as sodium
chloride in river-water,[142] but is only ¹⁄₁₂₅ as abundant in sea-water.
The total river discharge into the sea is estimated at 6524 cubic miles of
water per year.[143] This water is estimated to carry to the sea annually about
half a cubic mile of mineral matter in solution. At this rate it would take
about 9,000,000 years for the streams to bring to the sea an amount of
mineral matter equal to that it now contains, but the proportions of the
ingredients would be very different.
The sodium chloride makes up about 2.4% of the mineral matter in river-
water and nearly 78% of the mineral matter of the sea. At this rate it would
take nearly 300,000,000 years for the salt of the sea to have been
contributed by the rivers. It is not to be understood, however, that this figure
indicates the age of the ocean. The salt is not all brought in by the rivers;
the rivers have probably not always contributed at the present rate; and
much salt once in the sea has been precipitated. Nevertheless the above
figure gives some suggestion as to the order of magnitude of the figures
which represent the age of the ocean.
In contrast with the salt, the amount of calcium carbonate in the sea is so
small that at their present rate of contribution, it would be brought to the sea
by rivers in about 62,000 years.
Topography of bed.—The general relations of ocean basins to
continents are suggested by Fig. 296. The borders of the continental
platforms are covered by the epicontinental sea, while the abysmal sea
occupies the ocean basins proper. From the figure it is seen that an ocean
basin is pronouncedly convex upward, and so departs as widely as may be
from the current notion of the homely utensil from which it is named. Only
when it is remembered that a level surface (on the earth) is one which has
the mean curvature of the earth, and that the deeper parts of the ocean basin
are well below the mean sphere level, does the current name seem justified.
[144]
The figure also shows that the depth of an ocean basin is slight
compared with the radius of the earth.
rock decay, for most of the substances carried to the sea in solution by
rivers are extracted from the water about as rapidly as they are supplied.
Thus calcium carbonate is about twenty times as abundant as sodium
chloride in river-water,[142] but is only ¹⁄₁₂₅ as abundant in sea-water.
The total river discharge into the sea is estimated at 6524 cubic miles of
water per year.[143] This water is estimated to carry to the sea annually about
half a cubic mile of mineral matter in solution. At this rate it would take
about 9,000,000 years for the streams to bring to the sea an amount of
mineral matter equal to that it now contains, but the proportions of the
ingredients would be very different.
The sodium chloride makes up about 2.4% of the mineral matter in river-
water and nearly 78% of the mineral matter of the sea. At this rate it would
take nearly 300,000,000 years for the salt of the sea to have been
contributed by the rivers. It is not to be understood, however, that this figure
indicates the age of the ocean. The salt is not all brought in by the rivers;
the rivers have probably not always contributed at the present rate; and
much salt once in the sea has been precipitated. Nevertheless the above
figure gives some suggestion as to the order of magnitude of the figures
which represent the age of the ocean.
In contrast with the salt, the amount of calcium carbonate in the sea is so
small that at their present rate of contribution, it would be brought to the sea
by rivers in about 62,000 years.
Topography of bed.—The general relations of ocean basins to
continents are suggested by Fig. 296. The borders of the continental
platforms are covered by the epicontinental sea, while the abysmal sea
occupies the ocean basins proper. From the figure it is seen that an ocean
basin is pronouncedly convex upward, and so departs as widely as may be
from the current notion of the homely utensil from which it is named. Only
when it is remembered that a level surface (on the earth) is one which has
the mean curvature of the earth, and that the deeper parts of the ocean basin
are well below the mean sphere level, does the current name seem justified.
[144]
The figure also shows that the depth of an ocean basin is slight
compared with the radius of the earth.
Page 388
The bed of the ocean, like the face of the land, is affected by elevations
and depressions, and its deepest points are about as far below its surface as
the highest mountains are above it. There are areas of the sea bottom which,
as a whole, may be compared to the plains of the land, and others which
may be likened to plateaus, and the lines of gradation between them are as
indistinct as they often are on the land. There are mountain peaks, chiefly of
volcanic origin, and depressions comparable to the great basins on the land.
But apart from these general features, there is little in common between the
topography of the sea bottom and that of the land. Mountain systems are,
for the most part, absent, though certain islands, like Cuba and some of its
associates, may be regarded as the crests of systems which are chiefly
submerged. If the water were drawn off from the ocean’s bed so that it
could be seen as the land is, its most impressive feature would be its
monotony. The familiar hills and valleys which, in all their multitudinous
forms, give the land surface its most characteristic features are essentially
absent. A large part of its surface would be found to be so nearly flat that
the eye would not detect its departure from planeness.
and depressions, and its deepest points are about as far below its surface as
the highest mountains are above it. There are areas of the sea bottom which,
as a whole, may be compared to the plains of the land, and others which
may be likened to plateaus, and the lines of gradation between them are as
indistinct as they often are on the land. There are mountain peaks, chiefly of
volcanic origin, and depressions comparable to the great basins on the land.
But apart from these general features, there is little in common between the
topography of the sea bottom and that of the land. Mountain systems are,
for the most part, absent, though certain islands, like Cuba and some of its
associates, may be regarded as the crests of systems which are chiefly
submerged. If the water were drawn off from the ocean’s bed so that it
could be seen as the land is, its most impressive feature would be its
monotony. The familiar hills and valleys which, in all their multitudinous
forms, give the land surface its most characteristic features are essentially
absent. A large part of its surface would be found to be so nearly flat that
the eye would not detect its departure from planeness.
Page 389
Fig. 296.—General relations of ocean basins to the lithosphere. Lat. 20° S. Depth of the
water (black) and height of land exaggerated ten times. (Data from Murray, Scot. Geogr.
Mag., Vol. XV, 1899.)
The reason for this profound difference is readily found. On the land, the
dominant processes which shape the details of the surface are degradational,
and though the final result of degradation is flatness (base-level), the
immediate result is relief, and, most commonly, relief of the hill-and-valley
type. In the sea, the dominant processes are aggradational, and tend to
monotonous planeness.
water (black) and height of land exaggerated ten times. (Data from Murray, Scot. Geogr.
Mag., Vol. XV, 1899.)
The reason for this profound difference is readily found. On the land, the
dominant processes which shape the details of the surface are degradational,
and though the final result of degradation is flatness (base-level), the
immediate result is relief, and, most commonly, relief of the hill-and-valley
type. In the sea, the dominant processes are aggradational, and tend to
monotonous planeness.
Page 390
Distribution of marine life.—Marine life has been of such importance
in the history of the earth that the elementary facts concerning its
distribution and the principles which control it are here recalled. The
distribution of marine life is influenced by many factors, chief among
which are temperature and depth of water. Not only is life more abundant in
the warmer parts of the ocean than in the colder, but the species inhabiting
cold waters are different from those in warm, and few species range through
great variations. Many forms of life are restricted to shallow water. Many
more, especially those which do not live on the bottom, swim about freely
without reference to the depth of the water beneath them, while relatively
few are restricted to great depths. Many species are also influenced by the
salinity of the water, which varies notably along coasts where the fresh
waters from the land are discharged; by the character of the sediment at the
bottom, some species preferring mud, others sand, and others gravel; by the
movement of the waters, some species preferring still waters and others
rough; and some species by the abundance and nature of the food-supply,
and by rival and hostile species.
Subject to the exceptions determined by temperature, etc., plant life
abounds in shallow water out to depths of 100 fathoms or so, and is found
in abundance at the surface where the depth is much greater. Animal life
abounds in shallow water, both at the bottom and above it, out to depths of
200 or 300 fathoms, and occurs in great profusion in the surface-waters of
temperate and tropical regions without regard to the depth. The great body
of the ocean water lying below a depth of some few hundred fathoms is
nearly tenantless, though life reappears sparingly at the bottom, even where
the depth is great. For further discussion of this topic, see Chapter XI.
PROCESSES IN OPERATION IN THE SEA.
Within the area of the sea, as on the area of the land, three sets of
processes are at work—diastrophism, vulcanism, and gradation.
Diastrophism (p. 2) affects the sea-bottom as the land, but the results are
notably different in certain respects. So far as the lithosphere is concerned,
the sea-level may be said to be the critical level. At and above it, many
processes are in operation which do not appear below, and below it, many
which do not take place above. Changes of level which do not involve the
submergence of areas which were land, or the emergence of areas which
in the history of the earth that the elementary facts concerning its
distribution and the principles which control it are here recalled. The
distribution of marine life is influenced by many factors, chief among
which are temperature and depth of water. Not only is life more abundant in
the warmer parts of the ocean than in the colder, but the species inhabiting
cold waters are different from those in warm, and few species range through
great variations. Many forms of life are restricted to shallow water. Many
more, especially those which do not live on the bottom, swim about freely
without reference to the depth of the water beneath them, while relatively
few are restricted to great depths. Many species are also influenced by the
salinity of the water, which varies notably along coasts where the fresh
waters from the land are discharged; by the character of the sediment at the
bottom, some species preferring mud, others sand, and others gravel; by the
movement of the waters, some species preferring still waters and others
rough; and some species by the abundance and nature of the food-supply,
and by rival and hostile species.
Subject to the exceptions determined by temperature, etc., plant life
abounds in shallow water out to depths of 100 fathoms or so, and is found
in abundance at the surface where the depth is much greater. Animal life
abounds in shallow water, both at the bottom and above it, out to depths of
200 or 300 fathoms, and occurs in great profusion in the surface-waters of
temperate and tropical regions without regard to the depth. The great body
of the ocean water lying below a depth of some few hundred fathoms is
nearly tenantless, though life reappears sparingly at the bottom, even where
the depth is great. For further discussion of this topic, see Chapter XI.
PROCESSES IN OPERATION IN THE SEA.
Within the area of the sea, as on the area of the land, three sets of
processes are at work—diastrophism, vulcanism, and gradation.
Diastrophism (p. 2) affects the sea-bottom as the land, but the results are
notably different in certain respects. So far as the lithosphere is concerned,
the sea-level may be said to be the critical level. At and above it, many
processes are in operation which do not appear below, and below it, many
which do not take place above. Changes of level which do not involve the
submergence of areas which were land, or the emergence of areas which
Page 391
were under water, are relatively unimportant, compared with those which
effect such changes. The rise of the bottom of the sea from a depth of 500
fathoms to a depth of 200 fathoms would not lead to important
consequences, so far as the area itself is concerned, while an equal rise of
the bottom beneath 200 fathoms of water, or an equal subsidence of land
500 feet high, would be attended by more striking consequences. It follows
that the changes effected by diastrophism are much more obvious along
coasts than in the deep seas. Emergence or submergence shifts the zones of
aggradation and degradation, shifts the zone of contact of ocean and land,
and changes the region concerned from one appropriate for sea life to one
appropriate for terrestrial forms, or vice versa.
Over the continental shelves the water is shallow and the bottom
relatively smooth. If a coastal region be elevated evenly, or if the sea-level
be drawn down, the new shore-line on the smooth surface of the former
submerged shelf will be relatively regular, even though the coast was
notably irregular before the change. Thus in Fig. 297 the coast-line is
notably irregular. A sea-withdrawal or a land-uplift of 120 feet would
change the coast-line to the position of the 20-fathom line, when it would
be notably less irregular than now. If it were shifted to the 100-fathom line,
few irregularities would remain. In so far as new coast-lines formed by the
lowering of the sea (or rise of the crust) depart from straightness, it is
usually by broad, smooth curves. Local uplifts of coastal lands, and
especially uplifts along axes normal to the trend of the coast, would give
rise to projections of land, and so to coastal irregularities; but such uplifts
are rarely so localized as to give origin to minor projections. It follows that
rising coasts, and those which have recently risen, or more likely, coasts
along which the sea-level is sinking or has recently sunk, are likely to be
regular so far as details of outline are concerned. Subsidence of a coast-line
(or rise of the sea-level) tends to the opposite results, for in this case the sea
advances on a surface which has more or less relief, and the water takes
possession of every depression brought to its level. The lower parts of the
valleys are converted into bays, the length and width of which depend on
the slope and width of the valleys drowned. The numerous bays at the
debouchures of the streams along the Atlantic coast of the United States,
from Long Island Sound to Carolina, such as the Delaware, Chesapeake,
(Fig. 297) and numerous smaller bays, are the results of recent sinking,
which has allowed the sea to invade the lower ends of river valleys. The
effect such changes. The rise of the bottom of the sea from a depth of 500
fathoms to a depth of 200 fathoms would not lead to important
consequences, so far as the area itself is concerned, while an equal rise of
the bottom beneath 200 fathoms of water, or an equal subsidence of land
500 feet high, would be attended by more striking consequences. It follows
that the changes effected by diastrophism are much more obvious along
coasts than in the deep seas. Emergence or submergence shifts the zones of
aggradation and degradation, shifts the zone of contact of ocean and land,
and changes the region concerned from one appropriate for sea life to one
appropriate for terrestrial forms, or vice versa.
Over the continental shelves the water is shallow and the bottom
relatively smooth. If a coastal region be elevated evenly, or if the sea-level
be drawn down, the new shore-line on the smooth surface of the former
submerged shelf will be relatively regular, even though the coast was
notably irregular before the change. Thus in Fig. 297 the coast-line is
notably irregular. A sea-withdrawal or a land-uplift of 120 feet would
change the coast-line to the position of the 20-fathom line, when it would
be notably less irregular than now. If it were shifted to the 100-fathom line,
few irregularities would remain. In so far as new coast-lines formed by the
lowering of the sea (or rise of the crust) depart from straightness, it is
usually by broad, smooth curves. Local uplifts of coastal lands, and
especially uplifts along axes normal to the trend of the coast, would give
rise to projections of land, and so to coastal irregularities; but such uplifts
are rarely so localized as to give origin to minor projections. It follows that
rising coasts, and those which have recently risen, or more likely, coasts
along which the sea-level is sinking or has recently sunk, are likely to be
regular so far as details of outline are concerned. Subsidence of a coast-line
(or rise of the sea-level) tends to the opposite results, for in this case the sea
advances on a surface which has more or less relief, and the water takes
possession of every depression brought to its level. The lower parts of the
valleys are converted into bays, the length and width of which depend on
the slope and width of the valleys drowned. The numerous bays at the
debouchures of the streams along the Atlantic coast of the United States,
from Long Island Sound to Carolina, such as the Delaware, Chesapeake,
(Fig. 297) and numerous smaller bays, are the results of recent sinking,
which has allowed the sea to invade the lower ends of river valleys. The
Page 392
ragged coast of Maine is another example, though glaciation as well as
subsidence has been operative here. From the present configuration of
coast-lines, it has been inferred that the present is, on the whole, an era of
continental depression.[145] River valleys, the lower ends of which are
embayed, are sometimes found to be continuous with submerged valleys
beyond the coast-line (Fig. 298). Submerged river valleys show that the
surface in which they lie was once land.
Fig. 297.—Sketch of the eastern coast of the United States from Cape May to Cape Henry,
showing coastal irregularities. The figures represent the depths of water in fathoms.
(From charts of C. and G. Surv.)
subsidence has been operative here. From the present configuration of
coast-lines, it has been inferred that the present is, on the whole, an era of
continental depression.[145] River valleys, the lower ends of which are
embayed, are sometimes found to be continuous with submerged valleys
beyond the coast-line (Fig. 298). Submerged river valleys show that the
surface in which they lie was once land.
Fig. 297.—Sketch of the eastern coast of the United States from Cape May to Cape Henry,
showing coastal irregularities. The figures represent the depths of water in fathoms.
(From charts of C. and G. Surv.)
Page 393
Fig. 298.—Sketch of Carmel Bay, Cal. The contours below sea-level show a deep
submerged channel. (From charts of C. and G. Surv.)
Bays may be developed by local subsidence as well as by the submerging
of valleys, though decisive examples are not readily cited. Bays may also be
produced by uplift of the surface on either side of an area which does not
change its level. For example, uplift on either side of the Gulf of California
has probably been one element, though probably not the only one, in the
development of this indentation. The general outline of a great bay
produced by coastal warping might be regular, though it would be likely to
be marked by small irregularities where the streams enter. It is not to be
understood that all, or even most, bays are due to local diastrophism.
Diastrophism, then, as it affects the ocean-bottoms and the ocean-
borders, may make the water of any ocean shallower or deeper; it may
cause the emergence or submergence of land; it may make coast-lines
regular or irregular; it may shift the habitat of life, and through these
changes may greatly influence the processes of gradation, which are
especially active along the contact of sea and land.
submerged channel. (From charts of C. and G. Surv.)
Bays may be developed by local subsidence as well as by the submerging
of valleys, though decisive examples are not readily cited. Bays may also be
produced by uplift of the surface on either side of an area which does not
change its level. For example, uplift on either side of the Gulf of California
has probably been one element, though probably not the only one, in the
development of this indentation. The general outline of a great bay
produced by coastal warping might be regular, though it would be likely to
be marked by small irregularities where the streams enter. It is not to be
understood that all, or even most, bays are due to local diastrophism.
Diastrophism, then, as it affects the ocean-bottoms and the ocean-
borders, may make the water of any ocean shallower or deeper; it may
cause the emergence or submergence of land; it may make coast-lines
regular or irregular; it may shift the habitat of life, and through these
changes may greatly influence the processes of gradation, which are
especially active along the contact of sea and land.
Page 394
Vulcanism affects the sea-bottom much as it affects the land. At the
volcanic centers, where the great body of extruded matter accumulates,
mounds and mountains are built up. Most of the mountain peaks of the sea-
bottom, whether their crests are islands, or whether they are wholly
submerged, have had a volcanic origin. The rock material ejected from
submarine vents is probably less widely distributed than that from vents on
land, and so far forth, the volcanic cones in the oceans are steeper than
those on land. Where volcanic cones are built up near the surface of the sea,
they often furnish a home for shallow-water life, such as polyps. Wherever
built up so as to be within the reach of waves, gradational processes are
stimulated.
The processes of vulcanism do not commonly influence coasts of
continents directly, for few volcanoes lie immediately on coasts. In places,
however, as at various points in and about Italy, the configuration of the
coast is influenced by the building of volcanoes. Indirectly, vulcanism
influences the shape of coast-lines, for the resistance of igneous rock is
often different from that of the rock with which it is associated, and under
the influences of the forces of gradation it may come to form projecting
points or reëntrants, as the case may be.
The number of active volcanoes on islands is about 200, or about two-
thirds of all now known. Since the area of the sea is about three times that
of the land, the known active volcanoes in the sea are rather less numerous
per unit area than those on the land. The number of active vents beneath the
sea is altogether unknown. A few submarine eruptions have been observed,
and those observed are probably but a small percentage of those which have
taken place in historic time. Slight eruptions in deep water might not
manifest themselves at the surface in an unequivocal way, even were
observers stationed near them. Volcanic cones which fail to reach the
surface are known, and the forms of many sea-bottom mountain peaks are
such as to make it probable that they are volcanic. These phenomena, as
well as the numerous volcanic islands, give some indication of the
importance of submarine eruptions in past time.
Ocean volcanoes, and especially submarine volcanoes, affect both the
temperature and the composition of the sea-water. Both the increase of
temperature and the solution of volcanic gases increase the capacity of the
water for mineral matter, and both the change in temperature and
volcanic centers, where the great body of extruded matter accumulates,
mounds and mountains are built up. Most of the mountain peaks of the sea-
bottom, whether their crests are islands, or whether they are wholly
submerged, have had a volcanic origin. The rock material ejected from
submarine vents is probably less widely distributed than that from vents on
land, and so far forth, the volcanic cones in the oceans are steeper than
those on land. Where volcanic cones are built up near the surface of the sea,
they often furnish a home for shallow-water life, such as polyps. Wherever
built up so as to be within the reach of waves, gradational processes are
stimulated.
The processes of vulcanism do not commonly influence coasts of
continents directly, for few volcanoes lie immediately on coasts. In places,
however, as at various points in and about Italy, the configuration of the
coast is influenced by the building of volcanoes. Indirectly, vulcanism
influences the shape of coast-lines, for the resistance of igneous rock is
often different from that of the rock with which it is associated, and under
the influences of the forces of gradation it may come to form projecting
points or reëntrants, as the case may be.
The number of active volcanoes on islands is about 200, or about two-
thirds of all now known. Since the area of the sea is about three times that
of the land, the known active volcanoes in the sea are rather less numerous
per unit area than those on the land. The number of active vents beneath the
sea is altogether unknown. A few submarine eruptions have been observed,
and those observed are probably but a small percentage of those which have
taken place in historic time. Slight eruptions in deep water might not
manifest themselves at the surface in an unequivocal way, even were
observers stationed near them. Volcanic cones which fail to reach the
surface are known, and the forms of many sea-bottom mountain peaks are
such as to make it probable that they are volcanic. These phenomena, as
well as the numerous volcanic islands, give some indication of the
importance of submarine eruptions in past time.
Ocean volcanoes, and especially submarine volcanoes, affect both the
temperature and the composition of the sea-water. Both the increase of
temperature and the solution of volcanic gases increase the capacity of the
water for mineral matter, and both the change in temperature and
Page 395
composition affect the life of the adjacent waters. The destruction of life
during eruptions occasions the generation of the products of organic
decomposition, and these stimulate further chemical changes. The diffusion
of affected waters occasions chemical changes wherever they go. The
effects of oceanic volcanoes on the sea-water are, therefore, appreciable,
when long periods of time are considered. The deposition of the finer parts
of volcanic discharges will be considered in connection with the deposits of
the deep sea.
Gradation.—The gradational processes of the land and the sea are in
striking contrast. On the land, degradation predominates, and aggradation is
subordinate. In the sea, aggradation predominates, and degradation is
subordinate. On the land, degradation is, on the whole, greatest where the
land is highest, while aggradation is of consequence only where the land is
low, or where steep slopes give place to gentle ones. In the sea, degradation
is virtually confined to shallow water, or to what might be called the
highlands of the sea, while aggradation is nearly universal, but most
considerable in shallow water, or where shallow water gives place to deep.
Both the degradational and aggradational work of the sea are greatest near
its shores. Opposed as the gradational work of the land and sea are, they yet
tend to a common end—the leveling of the surface of the lithosphere.
The gradational processes which affect the sea-bottom may be divided
into three categories: (1) Those effected by mechanical means, (2) those
effected by chemical means, and (3) those effected by organic agencies.
The mechanical work of gradation in the sea is effected chiefly by the
movements of the water, and, very subordinately, by the movements of the
ice which the water carries. The results of these movements may be
degradational wherever the water is sufficiently shallow for the motion to
affect the bottom. Elsewhere it is aggradational.
The direct gradational work effected by chemical means is likewise
partly degradational and partly aggradational. If at any time or place the
water becomes supersaturated with any mineral substance, precipitation
takes place, and the precipitate accumulates as sediment on the bottom. This
sometimes happens in lagoons and other small inclosures, and perhaps in
open water. On the other hand, wherever solution is effected, degradation is
during eruptions occasions the generation of the products of organic
decomposition, and these stimulate further chemical changes. The diffusion
of affected waters occasions chemical changes wherever they go. The
effects of oceanic volcanoes on the sea-water are, therefore, appreciable,
when long periods of time are considered. The deposition of the finer parts
of volcanic discharges will be considered in connection with the deposits of
the deep sea.
Gradation.—The gradational processes of the land and the sea are in
striking contrast. On the land, degradation predominates, and aggradation is
subordinate. In the sea, aggradation predominates, and degradation is
subordinate. On the land, degradation is, on the whole, greatest where the
land is highest, while aggradation is of consequence only where the land is
low, or where steep slopes give place to gentle ones. In the sea, degradation
is virtually confined to shallow water, or to what might be called the
highlands of the sea, while aggradation is nearly universal, but most
considerable in shallow water, or where shallow water gives place to deep.
Both the degradational and aggradational work of the sea are greatest near
its shores. Opposed as the gradational work of the land and sea are, they yet
tend to a common end—the leveling of the surface of the lithosphere.
The gradational processes which affect the sea-bottom may be divided
into three categories: (1) Those effected by mechanical means, (2) those
effected by chemical means, and (3) those effected by organic agencies.
The mechanical work of gradation in the sea is effected chiefly by the
movements of the water, and, very subordinately, by the movements of the
ice which the water carries. The results of these movements may be
degradational wherever the water is sufficiently shallow for the motion to
affect the bottom. Elsewhere it is aggradational.
The direct gradational work effected by chemical means is likewise
partly degradational and partly aggradational. If at any time or place the
water becomes supersaturated with any mineral substance, precipitation
takes place, and the precipitate accumulates as sediment on the bottom. This
sometimes happens in lagoons and other small inclosures, and perhaps in
open water. On the other hand, wherever solution is effected, degradation is
Page 396
the result. Solution is most important where the bottom consists of
relatively soluble rock, such as lime carbonate.
Organic agencies are, on the whole, aggradational. Accumulations of
coral, coral débris, shells, etc., help to build up the sea-bottom, and most
rapidly in shallow water where the proper forms of life are most abundant.
Here also should be mentioned the accumulations of carbonaceous matter,
especially in the form of plant bodies. In the aggradation effected directly
by organic agencies, the sea is passive. Its only part is to support the life
which gives rise to the solid matter, and incidentally to float a part of it in
its currents.
MOVEMENTS OF THE SEA-WATER.
The movements of the sea-water fall into several categories. There is (1)
a general circulation of sea-water, determined chiefly by three factors:
differences in density in the sea-water, differences of level, and the general
movements of the atmosphere; (2) periodic movements which are not
primarily circulatory, brought about by the attraction of the sun and moon;
and (3) aperiodic movements, due to occasional causes, such as
earthquakes, volcanic explosions, landslides, etc., which determine local
and temporary movements, often of exceptional strength.
Differences in density and their results.—Differences in density result
from differences in temperature and salinity. Temperature alone considered,
water would be densest where it is coldest, namely in the polar regions.
Differences in salinity result from differences in evaporation and from
inequalities in the supply of fresh water. Evaporation alone considered, the
sea-water should be densest where evaporation is greatest; but the
equatorial region, where evaporation is greatest, is also a region where
precipitation is heavy, and precipitation, by freshening the water, opposes
the effect of great evaporation. The greatest differences in density due to the
unequal supply of fresh water are to be found near the borders of
continents, where the precipitation on the land is discharged into the sea. In
the polar regions, the great supply of fresh water, especially during the
season when the ice is melting, opposes the effect of the low temperature,
so far as the density of the water is concerned. The result of the operation of
these factors affecting the density of the sea-water is to insure a general
relatively soluble rock, such as lime carbonate.
Organic agencies are, on the whole, aggradational. Accumulations of
coral, coral débris, shells, etc., help to build up the sea-bottom, and most
rapidly in shallow water where the proper forms of life are most abundant.
Here also should be mentioned the accumulations of carbonaceous matter,
especially in the form of plant bodies. In the aggradation effected directly
by organic agencies, the sea is passive. Its only part is to support the life
which gives rise to the solid matter, and incidentally to float a part of it in
its currents.
MOVEMENTS OF THE SEA-WATER.
The movements of the sea-water fall into several categories. There is (1)
a general circulation of sea-water, determined chiefly by three factors:
differences in density in the sea-water, differences of level, and the general
movements of the atmosphere; (2) periodic movements which are not
primarily circulatory, brought about by the attraction of the sun and moon;
and (3) aperiodic movements, due to occasional causes, such as
earthquakes, volcanic explosions, landslides, etc., which determine local
and temporary movements, often of exceptional strength.
Differences in density and their results.—Differences in density result
from differences in temperature and salinity. Temperature alone considered,
water would be densest where it is coldest, namely in the polar regions.
Differences in salinity result from differences in evaporation and from
inequalities in the supply of fresh water. Evaporation alone considered, the
sea-water should be densest where evaporation is greatest; but the
equatorial region, where evaporation is greatest, is also a region where
precipitation is heavy, and precipitation, by freshening the water, opposes
the effect of great evaporation. The greatest differences in density due to the
unequal supply of fresh water are to be found near the borders of
continents, where the precipitation on the land is discharged into the sea. In
the polar regions, the great supply of fresh water, especially during the
season when the ice is melting, opposes the effect of the low temperature,
so far as the density of the water is concerned. The result of the operation of
these factors affecting the density of the sea-water is to insure a general
Page 397
circulation, directed to the end of equalizing the densities; and since the
disturbing factors are constantly in operation, equilibrium is never
established, and the movements of the water are perpetual.
The pressure gradients resulting from differences of density are so slight
that the resulting movements are scarcely more than a creep of the waters.
In general they are far too slow to be of importance in gradational work; but
the earth’s rotation deflects the creeping waters and tends to concentrate the
equator-ward movement into currents on the east sides of the continents,
and the pole-ward movement on the west sides. In favorable situations these
currents may be competent to produce sensible mechanical results. Even
where this is not the case the circulation helps to equalize the temperatures
of the sea, and so of the air above and of the land about. Indirectly,
therefore, the circulation of the ocean-waters affects every geological
process which is sensitive to climate.
Differences in level and their results.—While the surface of the ocean
is the common datum plane to which elevations and depressions are
referred, it is to be remembered that the sea has “a very complicated
undulating surface in consequence of the attraction which the
heterogeneous and elevated portions of the lithosphere exercise on the
liquid hydrosphere. In the opinion of geodesists, the geoid may in some
places depart from the figure of the spheroid by 1000 feet.”[146] These
variations in level would, however, not occasion circulation. The
differences in level which determine circulation are much more trivial.
Every stream which pours fresh water into the sea tends to raise the level of
the water where it enters. The waters brought to the ocean by the Amazon,
the Mississippi, and other great rivers would appreciably change the level
of the sea at their debouchures, if the excess did not promptly flow away.
The ready mobility of the water, however, prevents its accumulation, and
the discharge of every stream generates widespread movement. This
movement is strongest at the debouchure, and weakens with increasing
distance from it, though in the case of great streams, such as the Amazon,
the movement is traceable, by means of the sediment which the water
carries, hundreds of miles out to sea.
Changes of level are also brought about by the winds, which pile up
water along the shore against which they blow. The level of the water is
said to have risen 24 feet at Calcutta on October 5, 1864, as the result of a
disturbing factors are constantly in operation, equilibrium is never
established, and the movements of the water are perpetual.
The pressure gradients resulting from differences of density are so slight
that the resulting movements are scarcely more than a creep of the waters.
In general they are far too slow to be of importance in gradational work; but
the earth’s rotation deflects the creeping waters and tends to concentrate the
equator-ward movement into currents on the east sides of the continents,
and the pole-ward movement on the west sides. In favorable situations these
currents may be competent to produce sensible mechanical results. Even
where this is not the case the circulation helps to equalize the temperatures
of the sea, and so of the air above and of the land about. Indirectly,
therefore, the circulation of the ocean-waters affects every geological
process which is sensitive to climate.
Differences in level and their results.—While the surface of the ocean
is the common datum plane to which elevations and depressions are
referred, it is to be remembered that the sea has “a very complicated
undulating surface in consequence of the attraction which the
heterogeneous and elevated portions of the lithosphere exercise on the
liquid hydrosphere. In the opinion of geodesists, the geoid may in some
places depart from the figure of the spheroid by 1000 feet.”[146] These
variations in level would, however, not occasion circulation. The
differences in level which determine circulation are much more trivial.
Every stream which pours fresh water into the sea tends to raise the level of
the water where it enters. The waters brought to the ocean by the Amazon,
the Mississippi, and other great rivers would appreciably change the level
of the sea at their debouchures, if the excess did not promptly flow away.
The ready mobility of the water, however, prevents its accumulation, and
the discharge of every stream generates widespread movement. This
movement is strongest at the debouchure, and weakens with increasing
distance from it, though in the case of great streams, such as the Amazon,
the movement is traceable, by means of the sediment which the water
carries, hundreds of miles out to sea.
Changes of level are also brought about by the winds, which pile up
water along the shore against which they blow. The level of the water is
said to have risen 24 feet at Calcutta on October 5, 1864, as the result of a
Page 398
severe storm. While this is exceptional, a rise of 2 feet is not rare. This
piling up of the waters along shore insures a compensating movement
(undertow, littoral currents, etc.) in some other direction. Unequal
evaporation and precipitation likewise disturb the level of the sea and
occasion movement. In the open sea the movements generated by
differences of level, like those generated by differences of density, are
chiefly slow, creeping movements, but movements which never cease. In
bays and gulfs, on the other hand, the surface of the water may be so raised,
either as the result of wind, river discharge, or heavy precipitation, as to
give rise to strong outward currents. There is little doubt at the present time
that the Gulf Stream owes its origin primarily to the difference of level
between the Gulf of Mexico and the Atlantic.[147]
Movements generated by winds.—The circulation resulting from the
tendency of the winds to change the level of the sea-water has already been
mentioned, but the wind also works in other ways. Where the winds have a
somewhat constant direction and are at the same time strong, they
determine a general movement of the surface-waters in their own direction,
the surface-water being dragged along at a rate somewhat less than that of
the wind itself. The constant trades appear to be the chief generators of the
equatorial ocean-currents. Once generated, these currents may be
concentrated and their courses modified. The currents generated by trades
are turned north and south when directed against a continent; they are
modified by the configuration of the bottom if the water be shallow, and
always and everywhere, except, at the equator, they are deflected by the
rotation of the earth, in the northern hemisphere to the right, and in the
southern to the left. The pole-ward currents generated in the equatorial
region by the trades, and directed by the winds, the lands, the configuration
of the bottom, and the rotation of the earth, determine compensating
currents from high latitudes to low, and the same influences which control
the course of the former direct the latter as well.
Since the atmospheric movements are so far constant that there is a
prevailing direction of winds in all latitudes, the winds, as well as
differences of density and differences of level, insure a general and
continual circulation of sea-water. The geological effects of this circulation
are direct and indirect; direct, by gradation of the bottom over which they
flow, and indirect, by the modifications of climate they produce. Since
piling up of the waters along shore insures a compensating movement
(undertow, littoral currents, etc.) in some other direction. Unequal
evaporation and precipitation likewise disturb the level of the sea and
occasion movement. In the open sea the movements generated by
differences of level, like those generated by differences of density, are
chiefly slow, creeping movements, but movements which never cease. In
bays and gulfs, on the other hand, the surface of the water may be so raised,
either as the result of wind, river discharge, or heavy precipitation, as to
give rise to strong outward currents. There is little doubt at the present time
that the Gulf Stream owes its origin primarily to the difference of level
between the Gulf of Mexico and the Atlantic.[147]
Movements generated by winds.—The circulation resulting from the
tendency of the winds to change the level of the sea-water has already been
mentioned, but the wind also works in other ways. Where the winds have a
somewhat constant direction and are at the same time strong, they
determine a general movement of the surface-waters in their own direction,
the surface-water being dragged along at a rate somewhat less than that of
the wind itself. The constant trades appear to be the chief generators of the
equatorial ocean-currents. Once generated, these currents may be
concentrated and their courses modified. The currents generated by trades
are turned north and south when directed against a continent; they are
modified by the configuration of the bottom if the water be shallow, and
always and everywhere, except, at the equator, they are deflected by the
rotation of the earth, in the northern hemisphere to the right, and in the
southern to the left. The pole-ward currents generated in the equatorial
region by the trades, and directed by the winds, the lands, the configuration
of the bottom, and the rotation of the earth, determine compensating
currents from high latitudes to low, and the same influences which control
the course of the former direct the latter as well.
Since the atmospheric movements are so far constant that there is a
prevailing direction of winds in all latitudes, the winds, as well as
differences of density and differences of level, insure a general and
continual circulation of sea-water. The geological effects of this circulation
are direct and indirect; direct, by gradation of the bottom over which they
flow, and indirect, by the modifications of climate they produce. Since
Page 399
rotation deflects the pole-ward currents to the east sides of the oceans (west
sides of the continents) and the equator-ward movements to the west sides
of the oceans (east sides of the continents), the east shores of the oceans are
warmer than the west in corresponding latitudes, and the west sides of the
continents are both warmer and moister[148] than the east sides.
The most obvious disturbance of sea-water resulting from the winds is
the generation of waves. Waves are not primarily parts of the general
oceanic circulation. Since they are generated in other ways than by winds,
and since the gradational effects of waves are independent of their origin,
the effects of wind-waves will not be considered separately.
Movements generated by attraction.—One of the movements of the
sea-water which is not primarily circulatory results from the attraction of
the moon and sun. The tide is really the result of the inequalities of the
attraction of these bodies on different parts of the earth. The lunar tide is
more important than the solar, not because the attraction of the moon is
greater, for it is not, but because its differential attraction, the result of its
lesser distance, is greater.
The distance of the moon from the earth is about 240,000 miles. If this be
taken as the distance from the center of the moon to the center of the earth,
236,000 and 244,000 miles respectively are the distances from the center of
the moon to the nearest and most distant points on the earth. The distance of
the sun from the earth is about 93,000,000 miles. If this be taken as the
distance between the centers of these bodies, then the distances from the
center of the sun to the nearest and most distant points on the earth’s surface
are 92,996,000 and 93,004,000 miles respectively. The ratio of 4000 to
236,000 or to 244,000 is much greater than the ratio of 4000 to 92,996,000
or to 93,004,000. Hence the tide-producing force of the moon is greater
than that of the sun.
The tides show themselves along shores in the form of waves which, in
shallow water, become translatory. They differ from the wind-waves in their
periodicity, and locally in their greater height. The effects of the tidal waves
on the shores of the sea, and on the bottom in shallow water, are the same as
the effect of wind-waves of equal strength, and need not be separately
considered in connection with the gradation of the sea-bottom. In passing
through narrow straits or narrow passes of any sort, the tidal movement
sides of the continents) and the equator-ward movements to the west sides
of the oceans (east sides of the continents), the east shores of the oceans are
warmer than the west in corresponding latitudes, and the west sides of the
continents are both warmer and moister[148] than the east sides.
The most obvious disturbance of sea-water resulting from the winds is
the generation of waves. Waves are not primarily parts of the general
oceanic circulation. Since they are generated in other ways than by winds,
and since the gradational effects of waves are independent of their origin,
the effects of wind-waves will not be considered separately.
Movements generated by attraction.—One of the movements of the
sea-water which is not primarily circulatory results from the attraction of
the moon and sun. The tide is really the result of the inequalities of the
attraction of these bodies on different parts of the earth. The lunar tide is
more important than the solar, not because the attraction of the moon is
greater, for it is not, but because its differential attraction, the result of its
lesser distance, is greater.
The distance of the moon from the earth is about 240,000 miles. If this be
taken as the distance from the center of the moon to the center of the earth,
236,000 and 244,000 miles respectively are the distances from the center of
the moon to the nearest and most distant points on the earth. The distance of
the sun from the earth is about 93,000,000 miles. If this be taken as the
distance between the centers of these bodies, then the distances from the
center of the sun to the nearest and most distant points on the earth’s surface
are 92,996,000 and 93,004,000 miles respectively. The ratio of 4000 to
236,000 or to 244,000 is much greater than the ratio of 4000 to 92,996,000
or to 93,004,000. Hence the tide-producing force of the moon is greater
than that of the sun.
The tides show themselves along shores in the form of waves which, in
shallow water, become translatory. They differ from the wind-waves in their
periodicity, and locally in their greater height. The effects of the tidal waves
on the shores of the sea, and on the bottom in shallow water, are the same as
the effect of wind-waves of equal strength, and need not be separately
considered in connection with the gradation of the sea-bottom. In passing
through narrow straits or narrow passes of any sort, the tidal movement
Page 400
becomes a current which, under favorable conditions, abrades or “scours”
the bottom effectively. The tidal currents in the narrow passes about New
York harbor may serve as an illustration.
Aperiodic movements.—In addition to the wind-waves which are
essentially constant and universal, and to the tidal waves, which are
periodic, there are accidental waves which are locally and temporarily of
importance. Such are earthquake-waves, which are sometimes extremely
destructive. Thus an earthquake-wave on the coast of Peru in 1746 swept a
frigate several miles inland and deluged Lima, seven miles from the shore.
The havoc of most earthquakes affecting coasts, such as that of Lisbon in
1755, is greatly aggravated by accompanying sea-waves. Earthquake-waves
differ from ordinary waves in being translatory, and so in being more
effective on the bottom in deep water. Their greatest force, however, is felt
in shallow water and on shores. Volcanic eruptions likewise give rise to
exceptional aperiodic waves. The same is true of landslides where they
affect the coast or any part of the sea-bottom. The fall of glacier ends and
the capsizing of icebergs likewise generate strong waves. To the category of
exceptional waves also belong those generated by the winds of exceptional
storms, such as that which devastated Galveston in 1900.[149]
Summary.—From the point of view of their direct geological results in
shallow water, all movements of the sea-water may be grouped into two
main classes—(1) waves, with the undertow and the littoral currents they
generate, and (2) ocean-currents.[150]
WAVES.
Wave-motion.[151]—The most common waves, and from the present point
of view the most important, are those generated by winds. During the
passage of a wave, each particle affected by it rises and falls, and moves
forward and backward describing an orbit in a vertical plane. If the passing
wave is a swell, the orbit of the particle is closed and is either a circle or an
ellipse; but in the case of a wind-wave the orbit is not closed. In such a
wave two things move forward, the undulation and the water. The velocity
of the undulation is relatively rapid; that of the water, slow and rhythmic.
On the crest of the wind-wave each particle of water moves forward, and in
the trough it moves less rapidly backward, and the excess of the forward
the bottom effectively. The tidal currents in the narrow passes about New
York harbor may serve as an illustration.
Aperiodic movements.—In addition to the wind-waves which are
essentially constant and universal, and to the tidal waves, which are
periodic, there are accidental waves which are locally and temporarily of
importance. Such are earthquake-waves, which are sometimes extremely
destructive. Thus an earthquake-wave on the coast of Peru in 1746 swept a
frigate several miles inland and deluged Lima, seven miles from the shore.
The havoc of most earthquakes affecting coasts, such as that of Lisbon in
1755, is greatly aggravated by accompanying sea-waves. Earthquake-waves
differ from ordinary waves in being translatory, and so in being more
effective on the bottom in deep water. Their greatest force, however, is felt
in shallow water and on shores. Volcanic eruptions likewise give rise to
exceptional aperiodic waves. The same is true of landslides where they
affect the coast or any part of the sea-bottom. The fall of glacier ends and
the capsizing of icebergs likewise generate strong waves. To the category of
exceptional waves also belong those generated by the winds of exceptional
storms, such as that which devastated Galveston in 1900.[149]
Summary.—From the point of view of their direct geological results in
shallow water, all movements of the sea-water may be grouped into two
main classes—(1) waves, with the undertow and the littoral currents they
generate, and (2) ocean-currents.[150]
WAVES.
Wave-motion.[151]—The most common waves, and from the present point
of view the most important, are those generated by winds. During the
passage of a wave, each particle affected by it rises and falls, and moves
forward and backward describing an orbit in a vertical plane. If the passing
wave is a swell, the orbit of the particle is closed and is either a circle or an
ellipse; but in the case of a wind-wave the orbit is not closed. In such a
wave two things move forward, the undulation and the water. The velocity
of the undulation is relatively rapid; that of the water, slow and rhythmic.
On the crest of the wind-wave each particle of water moves forward, and in
the trough it moves less rapidly backward, and the excess of the forward
Page 401
movement over the backward gives it a slight residual advance. This
residual advance is the initiatory element of current. By virtue of it, the
upper layer of water is carried forward with reference to the layer below, in
the direction toward which the wind blows. The waves of any considerable
or long-continued wind, therefore, generate a current tending in the same
direction as the wind.
The agitation of which waves are the superficial manifestation is not
restricted to the surface, but is propagated indefinitely downward. Near the
surface the amount of motion diminishes rapidly with increasing depth (Fig.
299), but the rate of diminution itself diminishes, and there seems no
theoretic reason for assigning any definite limit to the downward
propagation of the oscillation.
Fig. 299.—Figure illustrating the decrease in the amount of wave-movement with increase
of depth. (Fenneman.)
At the surface, the radius of the circular orbit which a particle of water in
a wave tends to describe is half the height of the wave. At a depth equal to
one wave-length, the radius of the circle described by a particle is ¹⁄₅₃₅ as
great as at the surface, and at a depth equal to two wave-lengths, ¹⁄₃₀₀₀₀₀. If
the height of a wave be 43 feet, the radius of the circle described by a
surface particle is 21½ feet. If the length of the wave be 300 feet, the radius
of a particle at a depth of 300 feet is only about ⁴⁄₁₀ of an inch, and at 600
feet ¹⁄₁₂₀₀ of an inch.[152] These figures make it clear that effective agitation
of the water does not extend to great depths.
residual advance is the initiatory element of current. By virtue of it, the
upper layer of water is carried forward with reference to the layer below, in
the direction toward which the wind blows. The waves of any considerable
or long-continued wind, therefore, generate a current tending in the same
direction as the wind.
The agitation of which waves are the superficial manifestation is not
restricted to the surface, but is propagated indefinitely downward. Near the
surface the amount of motion diminishes rapidly with increasing depth (Fig.
299), but the rate of diminution itself diminishes, and there seems no
theoretic reason for assigning any definite limit to the downward
propagation of the oscillation.
Fig. 299.—Figure illustrating the decrease in the amount of wave-movement with increase
of depth. (Fenneman.)
At the surface, the radius of the circular orbit which a particle of water in
a wave tends to describe is half the height of the wave. At a depth equal to
one wave-length, the radius of the circle described by a particle is ¹⁄₅₃₅ as
great as at the surface, and at a depth equal to two wave-lengths, ¹⁄₃₀₀₀₀₀. If
the height of a wave be 43 feet, the radius of the circle described by a
surface particle is 21½ feet. If the length of the wave be 300 feet, the radius
of a particle at a depth of 300 feet is only about ⁴⁄₁₀ of an inch, and at 600
feet ¹⁄₁₂₀₀ of an inch.[152] These figures make it clear that effective agitation
of the water does not extend to great depths.
Page 402
So long as the velocity of the wind remains constant, the velocity of the
current which the wind-waves generate is less than that of the wind, and
there is always a differential movement of the water, each layer moving
faster than the one beneath. The friction is thus distributed through the
whole vertical column of the water in movement, and is even borne in part
by the sea-bottom if the movement extends so far down. The greater the
depth, the smaller the share of the friction each layer of water is called upon
to bear, and the greater the velocity of the current generated by a given
wind. But while the wave-motion extends indefinitely downward, the lower
limit of agitation effective in erosion is soon reached. Engineering
operations have shown that submarine structures are little disturbed at
depths of five meters in the Mediterranean and eight meters in the Atlantic.
[153]
On the other hand, débris as coarse as gravel, which is transported by
rolling on the bottom, is not infrequently carried out to depths of 50 feet,
and sometimes even to 150 feet. Fine sediment, like silt, is disturbed at still
greater depths, for ripple-marks, which indicate agitation of the water, are
said to have been found at depths of 100 fathoms.[154]
When a wave approaches a shelving shore, its habit is changed. The
velocity of the undulation is diminished, while the velocity of the advancing
particle of water in the crest is increased; the wave-length, measured from
trough to trough, is diminished, and the wave-height is increased; the crest
becomes acute, with the front steeper than the back, and these changes
culminate in the breaking of the crest, when the undulation proper ceases.
Waves of a given height break in about the same depth of water, and the
line along which incoming waves break is the line of breakers. The line of
breakers is in deeper water and farther from shore when the waves are
strong than when they are weak. Waves are reported to have broken in 100
fathoms of water,[155] but this must be regarded as very exceptional. The
return of the water thrown forward in the crests of waves is accomplished
by a current along the bottom called the undertow. The undertow is sensibly
normal to the coast when uninfluenced by oblique waves, and is efficient in
removing the products of erosion.
Since the incoming wave affects water which is at the same time under
the influence of the undertow, it gives to that current a pulsating character,
for the wave-motion sometimes supports and sometimes opposes the
undertow, and thus endows it with a higher transporting power than belongs
current which the wind-waves generate is less than that of the wind, and
there is always a differential movement of the water, each layer moving
faster than the one beneath. The friction is thus distributed through the
whole vertical column of the water in movement, and is even borne in part
by the sea-bottom if the movement extends so far down. The greater the
depth, the smaller the share of the friction each layer of water is called upon
to bear, and the greater the velocity of the current generated by a given
wind. But while the wave-motion extends indefinitely downward, the lower
limit of agitation effective in erosion is soon reached. Engineering
operations have shown that submarine structures are little disturbed at
depths of five meters in the Mediterranean and eight meters in the Atlantic.
[153]
On the other hand, débris as coarse as gravel, which is transported by
rolling on the bottom, is not infrequently carried out to depths of 50 feet,
and sometimes even to 150 feet. Fine sediment, like silt, is disturbed at still
greater depths, for ripple-marks, which indicate agitation of the water, are
said to have been found at depths of 100 fathoms.[154]
When a wave approaches a shelving shore, its habit is changed. The
velocity of the undulation is diminished, while the velocity of the advancing
particle of water in the crest is increased; the wave-length, measured from
trough to trough, is diminished, and the wave-height is increased; the crest
becomes acute, with the front steeper than the back, and these changes
culminate in the breaking of the crest, when the undulation proper ceases.
Waves of a given height break in about the same depth of water, and the
line along which incoming waves break is the line of breakers. The line of
breakers is in deeper water and farther from shore when the waves are
strong than when they are weak. Waves are reported to have broken in 100
fathoms of water,[155] but this must be regarded as very exceptional. The
return of the water thrown forward in the crests of waves is accomplished
by a current along the bottom called the undertow. The undertow is sensibly
normal to the coast when uninfluenced by oblique waves, and is efficient in
removing the products of erosion.
Since the incoming wave affects water which is at the same time under
the influence of the undertow, it gives to that current a pulsating character,
for the wave-motion sometimes supports and sometimes opposes the
undertow, and thus endows it with a higher transporting power than belongs
Page 403
to its mean velocity. Near the breaker-line, the oscillations communicated
by the wave may momentarily overcome and even reverse the movement of
the undertow. Inside the breaker-line, irregular oscillation only is
communicated. The broken wave-crest, dashing forward, overcomes the
undertow and throws it back, and the water returns as a simple current
descending a slope. The power of the undertow diminishes rapidly from the
breaker-line outward as the depth of the water increases.
When waves advance on the shore obliquely, a
shore-current is developed as illustrated by Fig.
300, where ab represents the direction of the
incoming wave, bc the direction of the littoral
current, and bd the direction of the undertow.
Where they strike the borders of land, the wind-
waves, therefore, generate two other movements,
the undertow and the littoral current. Any
particle of water near shore may be affected by
any two or by all three of these movements at
the same moment. The effect of littoral current
and undertow is to give a particle of water on
which both are working a direction between the
Fig. 300.—Diagram showing
relative directions of wave, two, as be. The effect of other combinations can
undertow, and shore- be readily inferred. These various combinations
current. are of consequence in the transportation of
débris.
WORK OF THE WAVES.
Erosion.
The general effects of the waves and the other movements to which they
give rise along shores are (1) the wear of the shores; (2) the transportation
for greater or less distances of the products of wear; and (3) the deposition
of the transported materials.
By waves and undertow.—In the dash of the waves against the shore,
the chief wear is effected by the impact of the water and of the débris which
the water carries. Lesser results are accomplished in other ways.
by the wave may momentarily overcome and even reverse the movement of
the undertow. Inside the breaker-line, irregular oscillation only is
communicated. The broken wave-crest, dashing forward, overcomes the
undertow and throws it back, and the water returns as a simple current
descending a slope. The power of the undertow diminishes rapidly from the
breaker-line outward as the depth of the water increases.
When waves advance on the shore obliquely, a
shore-current is developed as illustrated by Fig.
300, where ab represents the direction of the
incoming wave, bc the direction of the littoral
current, and bd the direction of the undertow.
Where they strike the borders of land, the wind-
waves, therefore, generate two other movements,
the undertow and the littoral current. Any
particle of water near shore may be affected by
any two or by all three of these movements at
the same moment. The effect of littoral current
and undertow is to give a particle of water on
which both are working a direction between the
Fig. 300.—Diagram showing
relative directions of wave, two, as be. The effect of other combinations can
undertow, and shore- be readily inferred. These various combinations
current. are of consequence in the transportation of
débris.
WORK OF THE WAVES.
Erosion.
The general effects of the waves and the other movements to which they
give rise along shores are (1) the wear of the shores; (2) the transportation
for greater or less distances of the products of wear; and (3) the deposition
of the transported materials.
By waves and undertow.—In the dash of the waves against the shore,
the chief wear is effected by the impact of the water and of the débris which
the water carries. Lesser results are accomplished in other ways.
Page 404
When the land at the margin of the water consists of unconsolidated
material, or of fragmental material but slightly cemented, the impact of the
water is sufficient to displace or erode it. If weak rock be associated with
resistant rock within the zone of wave-work, the removal of the former may
lead to the disruption and fall of the latter, especially when weak rock is
washed out from beneath the strong. The impact of the water is competent
also to break up and remove rock which was once resistant, but which has
been superficially weakened by changes of temperature. Rock affected by
numerous open joints is likewise attacked with success, for by the dash of
the waves the blocks between the joints may be loosened and literally
quarried out. It may, however, be doubted whether the dash of waves of
clear water, even when their force is many tons to the square foot, has any
appreciable power to wear rock which is thoroughly solid.
material, or of fragmental material but slightly cemented, the impact of the
water is sufficient to displace or erode it. If weak rock be associated with
resistant rock within the zone of wave-work, the removal of the former may
lead to the disruption and fall of the latter, especially when weak rock is
washed out from beneath the strong. The impact of the water is competent
also to break up and remove rock which was once resistant, but which has
been superficially weakened by changes of temperature. Rock affected by
numerous open joints is likewise attacked with success, for by the dash of
the waves the blocks between the joints may be loosened and literally
quarried out. It may, however, be doubted whether the dash of waves of
clear water, even when their force is many tons to the square foot, has any
appreciable power to wear rock which is thoroughly solid.
Page 405
Fig. 301.—Angular blocks of rock which have fallen from the cliff above, as a result of
undercutting by the waves. Grand Island, Lake Champlain. The rock is Black River
limestone. Although from the shore of a lake instead of the sea, the principles illustrated
are the same. (Perry.)
The impact of the waves is generally reinforced and made effective by
the impact of the detritus they carry. The sand, the pebbles, and such stones
as the waves can move are used as weapons of attack, being turned against
one another and against the shore. Masses of rock too large for the waves to
move (Fig. 301) are worn by the detritus
driven back and forth over them, and in time reduced to movable
dimensions (Fig. 302). They then become the tools of the waves, and in use,
are reduced to smaller and smaller size. Thus bowlders are reduced to
cobbles, cobbles to pebbles, pebbles to sand, and sand to silt. The silt is
readily held in suspension in agitated water, and thus is carried out beyond
the range of breakers, and settles in water so deep as not to be effectively
agitated to its bottom. Thus one generation of bowlders after another is
undercutting by the waves. Grand Island, Lake Champlain. The rock is Black River
limestone. Although from the shore of a lake instead of the sea, the principles illustrated
are the same. (Perry.)
The impact of the waves is generally reinforced and made effective by
the impact of the detritus they carry. The sand, the pebbles, and such stones
as the waves can move are used as weapons of attack, being turned against
one another and against the shore. Masses of rock too large for the waves to
move (Fig. 301) are worn by the detritus
driven back and forth over them, and in time reduced to movable
dimensions (Fig. 302). They then become the tools of the waves, and in use,
are reduced to smaller and smaller size. Thus bowlders are reduced to
cobbles, cobbles to pebbles, pebbles to sand, and sand to silt. The silt is
readily held in suspension in agitated water, and thus is carried out beyond
the range of breakers, and settles in water so deep as not to be effectively
agitated to its bottom. Thus one generation of bowlders after another is
Page 406
worn out, and the comminuted products are carried out from the immediate
shore and deposited in deeper water.
The effectiveness of waves, whether they work by impact of water alone,
or by impact of water and detritus, is dependent on their strength and on the
concentration of their blows.[156] The strength of waves is dependent on the
strength of the winds (or other generating cause) and the depth and expanse
of the water, and the concentration of their blows is conditioned by the
slope against which they break. On exposed ocean-coasts the fetch of the
waves is always great. The winds are variable. For a given coast they have
an average strength, but the effectiveness of wave-erosion is determined
less by the average strength of waves than by the strength of the storm-
waves. This is often very great. On the Atlantic and North Sea coasts of
Britain, winter breakers which exert a pressure of three tons per square foot
are not infrequent.[157] So great is the force of exceptional storm-waves that
blocks of rock exceeding 100 tons in weight are known to have been moved
by them. Ground-swells, “even when no wind is blowing, often cover the
cliffs of north Scotland with sheets of water and foam up to heights of 100
or even nearly 200 feet. During northeasterly gales the windows of the
Dunnet Head lighthouse, at a height of upwards of 300 feet above high-
water mark, are said to be sometimes broken by stones swept up the cliffs
by sheets of sea-water.”[158] The average force of waves on the Atlantic coast
of Britain has been found to be 611 lbs. per square foot in summer, and
2086 lbs. in winter.[159]
Where deep water extends up to the shore, the force of the wave is almost
wholly expended near the water line; where shallow water borders the land,
the force of the waves is expended over a greater area. Waves are, therefore,
most efficient on bold coasts bordered by broad expanses of deep water.
The less familiar phases of wave-work are accomplished by hydraulic
pressure, compressed air, the use of ice, etc. When the water of a wave is
driven into an open joint or a cave, the hydraulic pressure is great, and if the
structure be weak, the rock may be broken. When water is driven with force
into a cave, the compression of the air may be great if the wave be high
enough to close the entrance. When the water runs out of a cave, the air
within may be greatly rarefied, while that above exerts its normal pressure.
In either case the roof of the cave, if it be weak, may be broken. At certain
seasons of the year, especially during the spring, waves make destructive
shore and deposited in deeper water.
The effectiveness of waves, whether they work by impact of water alone,
or by impact of water and detritus, is dependent on their strength and on the
concentration of their blows.[156] The strength of waves is dependent on the
strength of the winds (or other generating cause) and the depth and expanse
of the water, and the concentration of their blows is conditioned by the
slope against which they break. On exposed ocean-coasts the fetch of the
waves is always great. The winds are variable. For a given coast they have
an average strength, but the effectiveness of wave-erosion is determined
less by the average strength of waves than by the strength of the storm-
waves. This is often very great. On the Atlantic and North Sea coasts of
Britain, winter breakers which exert a pressure of three tons per square foot
are not infrequent.[157] So great is the force of exceptional storm-waves that
blocks of rock exceeding 100 tons in weight are known to have been moved
by them. Ground-swells, “even when no wind is blowing, often cover the
cliffs of north Scotland with sheets of water and foam up to heights of 100
or even nearly 200 feet. During northeasterly gales the windows of the
Dunnet Head lighthouse, at a height of upwards of 300 feet above high-
water mark, are said to be sometimes broken by stones swept up the cliffs
by sheets of sea-water.”[158] The average force of waves on the Atlantic coast
of Britain has been found to be 611 lbs. per square foot in summer, and
2086 lbs. in winter.[159]
Where deep water extends up to the shore, the force of the wave is almost
wholly expended near the water line; where shallow water borders the land,
the force of the waves is expended over a greater area. Waves are, therefore,
most efficient on bold coasts bordered by broad expanses of deep water.
The less familiar phases of wave-work are accomplished by hydraulic
pressure, compressed air, the use of ice, etc. When the water of a wave is
driven into an open joint or a cave, the hydraulic pressure is great, and if the
structure be weak, the rock may be broken. When water is driven with force
into a cave, the compression of the air may be great if the wave be high
enough to close the entrance. When the water runs out of a cave, the air
within may be greatly rarefied, while that above exerts its normal pressure.
In either case the roof of the cave, if it be weak, may be broken. At certain
seasons of the year, especially during the spring, waves make destructive
Page 407
use of the ice which is then breaking up, but it is only in high latitudes that
sea-ice is of consequence in this way. In general, the effect of its presence in
keeping down waves overbalances its effect as an agent of erosion.
Fig. 302.—Showing blocks similar to those of Fig. 306, reduced and rounded by wave-
action. Shore of Lake Champlain. The rock is Utica shale. (Perry.)
The direct effect of wave-erosion is restricted to a zone which is narrow
both horizontally and vertically. There is no impact of breakers at levels
lower than the troughs of the waves, though erosion may extend down to
the limit of effective agitation (p. 341). The efficient impact of waves is
limited upward by the level of the wave-crests, although the dash of the
water produces feebler blows at higher levels. The rise and fall of the water
during the flow and ebb of the tides gives the waves a greater vertical range
than wind-waves alone would have. The vertical zone of direct wave-work
sea-ice is of consequence in this way. In general, the effect of its presence in
keeping down waves overbalances its effect as an agent of erosion.
Fig. 302.—Showing blocks similar to those of Fig. 306, reduced and rounded by wave-
action. Shore of Lake Champlain. The rock is Utica shale. (Perry.)
The direct effect of wave-erosion is restricted to a zone which is narrow
both horizontally and vertically. There is no impact of breakers at levels
lower than the troughs of the waves, though erosion may extend down to
the limit of effective agitation (p. 341). The efficient impact of waves is
limited upward by the level of the wave-crests, although the dash of the
water produces feebler blows at higher levels. The rise and fall of the water
during the flow and ebb of the tides gives the waves a greater vertical range
than wind-waves alone would have. The vertical zone of direct wave-work
Page 408
is therefore limited above by the level of wave-crests, and below by the
depth of wave-troughs (nearly). The indirect work of waves is limited only
by the height of the shore, for as the zone of excavation is carried landward,
masses higher up the slope are undermined and fall. The fallen rock
temporarily protects the shore against the waves, but are themselves
eventually broken up.
Fig. 303.—Diagram illustrating high sea-cliffs. It also shows a submerged terrace, due
partly to wave-cutting (wave-cut terrace), and partly to building (wave-built terrace).
(Gilbert.)
Fig. 304.—Diagram showing a low sea-cliff. (Gilbert.)
The pulsating current of the undertow (p. 341) has both an erosive and a
transporting function. It carries the detritus of the shore to and fro, and
dragging it over the bottom, continues downward the erosion initiated by
the breakers. This downward erosion is the necessary concomitant of the
shoreward progress of wave-erosion; for, if the land were merely planed
away to the level of the wave-troughs, the incoming waves would break
where shoal water was first reached, and become ineffective at the water
margin. The rate of erosion by the undertow becomes less and less as the
surface it affects is lowered. Littoral currents do little erosive work beyond
that inflicted on the material which they transport.
The general result of wave-erosion is the advance of the sea on the land,
the rate of advance being determined chiefly by the nature of the material
depth of wave-troughs (nearly). The indirect work of waves is limited only
by the height of the shore, for as the zone of excavation is carried landward,
masses higher up the slope are undermined and fall. The fallen rock
temporarily protects the shore against the waves, but are themselves
eventually broken up.
Fig. 303.—Diagram illustrating high sea-cliffs. It also shows a submerged terrace, due
partly to wave-cutting (wave-cut terrace), and partly to building (wave-built terrace).
(Gilbert.)
Fig. 304.—Diagram showing a low sea-cliff. (Gilbert.)
The pulsating current of the undertow (p. 341) has both an erosive and a
transporting function. It carries the detritus of the shore to and fro, and
dragging it over the bottom, continues downward the erosion initiated by
the breakers. This downward erosion is the necessary concomitant of the
shoreward progress of wave-erosion; for, if the land were merely planed
away to the level of the wave-troughs, the incoming waves would break
where shoal water was first reached, and become ineffective at the water
margin. The rate of erosion by the undertow becomes less and less as the
surface it affects is lowered. Littoral currents do little erosive work beyond
that inflicted on the material which they transport.
The general result of wave-erosion is the advance of the sea on the land,
the rate of advance being determined chiefly by the nature of the material
Page 409
attacked and the strength of the waves. Numerous as examples are of the
retreat of coast-lines before the advance of the sea, it is not to be understood
that the advance of the sea on the land is universal or uninterrupted.
Numerous instances may be cited of the encroachment of the land on the
sea. At Long Branch the advance of the sea, in spite of elaborate
breakwaters, has been so rapid in recent years as to menace important
buildings, while a few miles to the north and south, the land is advancing in
the face of the waves. The low coast of the Middle Netherlands has
retreated two miles or more in historic times,[160] but the opposite tendency
is shown at other points in the same region. On the coast of England the
sites of villages have disappeared by the advance of the sea within historic
times,[161] but the coast of the same island affords illustrations of land
advance. On the south side of Nantucket island, the sea-cliff has been
known to retreat before the waves as much as six feet in a single year.[162]
Almost every considerable stretch of coast affords illustrations both of the
advance of the sea on the land and of land on the sea; but in the long run,
the former must exceed the latter, diastrophic movements aside.
retreat of coast-lines before the advance of the sea, it is not to be understood
that the advance of the sea on the land is universal or uninterrupted.
Numerous instances may be cited of the encroachment of the land on the
sea. At Long Branch the advance of the sea, in spite of elaborate
breakwaters, has been so rapid in recent years as to menace important
buildings, while a few miles to the north and south, the land is advancing in
the face of the waves. The low coast of the Middle Netherlands has
retreated two miles or more in historic times,[160] but the opposite tendency
is shown at other points in the same region. On the coast of England the
sites of villages have disappeared by the advance of the sea within historic
times,[161] but the coast of the same island affords illustrations of land
advance. On the south side of Nantucket island, the sea-cliff has been
known to retreat before the waves as much as six feet in a single year.[162]
Almost every considerable stretch of coast affords illustrations both of the
advance of the sea on the land and of land on the sea; but in the long run,
the former must exceed the latter, diastrophic movements aside.
Page 410
Fig. 305.—Steep cliff developed by waves. Allen Point, Grand Island, Lake Champlain.
(Perry.)
(Perry.)
Page 411
Fig. 306.—Cliff in unconsolidated material (bowlder clay), with lake-beach in foreground.
South Manitou Island, Lake Michigan. (Russell, U. S. Geol. Surv.)
South Manitou Island, Lake Michigan. (Russell, U. S. Geol. Surv.)
Page 412
Fig. 307.—Steep cliff in unconsolidated material, the result of rapid cutting. Southeast
extremity of Grove Point, Md.
Topographic Features Developed by Wave-erosion.
extremity of Grove Point, Md.
Topographic Features Developed by Wave-erosion.
Page 413
Fig. 308.—Standing Rock. A wave-erosion monument. West shore of Random Sound, south
of Clarenville, N. F. (Walcott, U. S. Geol. Surv.)
The sea-cliff.—The action of the waves, cutting as they do along a
definite horizontal zone, has been compared to the action of a horizontal
saw. As the waves cut into the shore at and near the water-level, the material
above, being unsupported, falls, leaving a steep face above the line of
cutting. This steep face is known as the sea-cliff (Figs. 301 to 306). The
same term is sometimes applied to the cliffs of lakes. The principles
involved in the development of the sea-cliff are applicable to any broad
stretch of water.
The height of the cliff depends on the height of the land on which the sea
is advancing. Its slope may be steep or gentle (compare Figs. 303 to 306),
according to the nature of the material of which it is composed and the
rapidity of the cutting. Rapid cutting tends to produce steep cliffs and slow
cutting gentle ones, for in the latter case weathering is more important
relative to the cutting, and at sea-level (low altitudes) weathering generally
tends to reduce the angle of slope. In general, the more resistant the material
the steeper the slope of the cliff. Incoherent materials, such as sand and
clay, are not likely to form steep cliffs; but if the cutting be very rapid, bold
faces may be developed even in such materials (Fig. 307). If beds of slight
resistance at sea-level underlie beds of greater resistance, the development
of steep cliffs is favored. The structure of the cliff-rock also has an
influence on the slope. The rock may be massive or bedded. If bedded, the
beds may be horizontal, or they may dip at any angle, in any direction. The
of Clarenville, N. F. (Walcott, U. S. Geol. Surv.)
The sea-cliff.—The action of the waves, cutting as they do along a
definite horizontal zone, has been compared to the action of a horizontal
saw. As the waves cut into the shore at and near the water-level, the material
above, being unsupported, falls, leaving a steep face above the line of
cutting. This steep face is known as the sea-cliff (Figs. 301 to 306). The
same term is sometimes applied to the cliffs of lakes. The principles
involved in the development of the sea-cliff are applicable to any broad
stretch of water.
The height of the cliff depends on the height of the land on which the sea
is advancing. Its slope may be steep or gentle (compare Figs. 303 to 306),
according to the nature of the material of which it is composed and the
rapidity of the cutting. Rapid cutting tends to produce steep cliffs and slow
cutting gentle ones, for in the latter case weathering is more important
relative to the cutting, and at sea-level (low altitudes) weathering generally
tends to reduce the angle of slope. In general, the more resistant the material
the steeper the slope of the cliff. Incoherent materials, such as sand and
clay, are not likely to form steep cliffs; but if the cutting be very rapid, bold
faces may be developed even in such materials (Fig. 307). If beds of slight
resistance at sea-level underlie beds of greater resistance, the development
of steep cliffs is favored. The structure of the cliff-rock also has an
influence on the slope. The rock may be massive or bedded. If bedded, the
beds may be horizontal, or they may dip at any angle, in any direction. The
Page 414
rock, whether stratified or not, may be abundantly or sparsely jointed. All
these structures influence the slope and configuration of the sea-cliff (see
Figs. 305 to 308).
Chimney-rocks, etc.—By working in
along the joints of the rock, widening them
and quarrying out the intervening blocks,
pillars of rock (“chimney-rocks,” “pulpit-
rocks”) or even considerable islets are
sometimes isolated by the waves. This is
most readily accomplished where the joints
converge back from the shore. A well-known
example of this sort is the “Old Man of Hoy”
(Fig. 309) on the coast of the Orkneys. A
pulpit-rock or other island, or any jutting
point of rock may be pierced, giving an arch
or bridge. La Roche Percée, a steep-faced
Fig. 309.—“Old Man of Hoy.” isle near Gaspé Harbor, is an example.
(Geikie.)
Sea-caves.—Waves sometimes excavate
caves at the bases of cliffs. This is especially likely to occur where the rock
is much jointed and where the joints are not continued to the surface in a
single plane. The bottom and roof of a sea-cave usually have a pronounced
inclination landward. If the cliff be low, the cave may be extended landward
until its roof is pierced. Through such an opening in the top of the cliff the
water of the incoming waves may be forced in the form of spray. On the
New England coast such holes are sometimes known as “spouting horns.”
Similar openings may be made, as already pointed out, by the compression
or rarefaction of the air in the cave as the wave enters or retreats. If the roof
of the cave be partially destroyed, the portion which remains may form an
arch or bridge. Such a bridge occurs on Santa Cruz Island, California (Fig.
310).
these structures influence the slope and configuration of the sea-cliff (see
Figs. 305 to 308).
Chimney-rocks, etc.—By working in
along the joints of the rock, widening them
and quarrying out the intervening blocks,
pillars of rock (“chimney-rocks,” “pulpit-
rocks”) or even considerable islets are
sometimes isolated by the waves. This is
most readily accomplished where the joints
converge back from the shore. A well-known
example of this sort is the “Old Man of Hoy”
(Fig. 309) on the coast of the Orkneys. A
pulpit-rock or other island, or any jutting
point of rock may be pierced, giving an arch
or bridge. La Roche Percée, a steep-faced
Fig. 309.—“Old Man of Hoy.” isle near Gaspé Harbor, is an example.
(Geikie.)
Sea-caves.—Waves sometimes excavate
caves at the bases of cliffs. This is especially likely to occur where the rock
is much jointed and where the joints are not continued to the surface in a
single plane. The bottom and roof of a sea-cave usually have a pronounced
inclination landward. If the cliff be low, the cave may be extended landward
until its roof is pierced. Through such an opening in the top of the cliff the
water of the incoming waves may be forced in the form of spray. On the
New England coast such holes are sometimes known as “spouting horns.”
Similar openings may be made, as already pointed out, by the compression
or rarefaction of the air in the cave as the wave enters or retreats. If the roof
of the cave be partially destroyed, the portion which remains may form an
arch or bridge. Such a bridge occurs on Santa Cruz Island, California (Fig.
310).
Page 415
Fig. 310.—An arch developed by waves. Santa Cruz Island, Cal. (Law.)
The cave, the “spouting horn,” the “bridge,” the “pulpit-rock,” and other
isolated islets, are all closely associated with the sea-cliff in origin.
The wave-cut terrace.—The bottom of the sea-cliff is bordered by a
submerged platform over which the water is shallow. This platform, or at
any rate its landward portion, represents the area over which the water has
advanced as the result of wave-cutting, and is, therefore, known as the
wave-cut terrace. From the method of cliff development it will be seen that
the wave-cut terrace is its necessary accompaniment. Such a terrace has a
gentle slope to seaward, for its outer and older edge has been degraded
longer and more. Its slope is influenced by the strength of the waves, being
greater where they are stronger. The outer edge of the wave-cut terrace is
often marked by an abrupt descent. Fig. 303 represents the wave-cut terrace
in its relation to the sea-cliff above.
The cave, the “spouting horn,” the “bridge,” the “pulpit-rock,” and other
isolated islets, are all closely associated with the sea-cliff in origin.
The wave-cut terrace.—The bottom of the sea-cliff is bordered by a
submerged platform over which the water is shallow. This platform, or at
any rate its landward portion, represents the area over which the water has
advanced as the result of wave-cutting, and is, therefore, known as the
wave-cut terrace. From the method of cliff development it will be seen that
the wave-cut terrace is its necessary accompaniment. Such a terrace has a
gentle slope to seaward, for its outer and older edge has been degraded
longer and more. Its slope is influenced by the strength of the waves, being
greater where they are stronger. The outer edge of the wave-cut terrace is
often marked by an abrupt descent. Fig. 303 represents the wave-cut terrace
in its relation to the sea-cliff above.
Page 416
Fig. 311.—An elevated cliff above Great Salt Lake. In this case the water-level has been
lowered. (Gilbert, U. S. Geol. Surv.)
So long as wave-cut terraces are submerged, they do not appear on
topographic maps of the land, though they appear on the charts of the
coasts; but if a coastal tract with wave-cut terraces be elevated, or if the sea-
level be drawn down, the terraces become land. Elevated sea-cliffs and
wave-cut terraces are among the best evidences of change of relative level
between water and land (Fig. 311).
Wave-erosion and horizontal configuration.—The structure of the rock
along shore has as much to do with the horizontal configuration of the
lowered. (Gilbert, U. S. Geol. Surv.)
So long as wave-cut terraces are submerged, they do not appear on
topographic maps of the land, though they appear on the charts of the
coasts; but if a coastal tract with wave-cut terraces be elevated, or if the sea-
level be drawn down, the terraces become land. Elevated sea-cliffs and
wave-cut terraces are among the best evidences of change of relative level
between water and land (Fig. 311).
Wave-erosion and horizontal configuration.—The structure of the rock
along shore has as much to do with the horizontal configuration of the
Page 417
wave-shaped coast, as with its relief. In general, waves develop reëntrants
in the less resistant portions of the shore, leaving the more resistant parts as
headlands (San Pedro Point and Devil’s Slide, Pl. XX, Coast of California).
It is to be noted that the resistance of rock to wave-erosion is not
determined by its hardness alone. Every division plane, whether due to
bedding, to jointing, or to irregular fracture, is a source of weakness to the
rock, and rock of great hardness may be so broken as to offer relatively
little resistance. Inequalities of resistance, whatever their cause, give origin
to inequalities of coastal configuration where wave-erosion is in progress.
Given a coast of marked regularity and equal exposure, but composed of
unequally resistant material, the waves will make it irregular by cutting
most where the material is least resistant. A regular coast of uniform
material, but unequal exposure, will be made irregular by the greater cutting
at the points of greater exposure. A coast of marked irregularity and
homogeneous material will be made more regular by the cutting off of the
projecting points, because they are most exposed. With a given set of
conditions, waves tend to develop a certain sort of shore-line which, so far
as its horizontal form is concerned, is relatively stable. Such a shore-line
may be said to be mature[163] so far as wave-erosion is concerned. Since
coastal lands are, in general, both heterogeneous and unequally exposed, a
mature coast-line is somewhat irregular. Its maturity is attained when the
lesser exposure in the reëntrants developed in the less resistant parts,
balances the superior exposure of the projections of the more resistant
portions.
Since the conditions of erosion along coasts are constantly, even if
slowly, changing, maturity is constantly being approached, but rarely
reached. Other forces and processes, such as those of aggradation,
vulcanism, and diastrophism, are in operation along coasts, and their results
are sometimes antagonistic to those of the waves. The horizontal
configuration of coasts is, therefore, the result of many coöperating forces,
of which waves are but one. It is, nevertheless, important to note the goal to
which the waves are working, even though they are continually defeated in
their attempt to reach it. Their immediate goal is an equilibrium of erosion-
rate and maturity of configuration; their final goal is the destruction of the
land and the deposition of its substance in the sea, that is, in a position
nearer the center of gravity of the earth.
in the less resistant portions of the shore, leaving the more resistant parts as
headlands (San Pedro Point and Devil’s Slide, Pl. XX, Coast of California).
It is to be noted that the resistance of rock to wave-erosion is not
determined by its hardness alone. Every division plane, whether due to
bedding, to jointing, or to irregular fracture, is a source of weakness to the
rock, and rock of great hardness may be so broken as to offer relatively
little resistance. Inequalities of resistance, whatever their cause, give origin
to inequalities of coastal configuration where wave-erosion is in progress.
Given a coast of marked regularity and equal exposure, but composed of
unequally resistant material, the waves will make it irregular by cutting
most where the material is least resistant. A regular coast of uniform
material, but unequal exposure, will be made irregular by the greater cutting
at the points of greater exposure. A coast of marked irregularity and
homogeneous material will be made more regular by the cutting off of the
projecting points, because they are most exposed. With a given set of
conditions, waves tend to develop a certain sort of shore-line which, so far
as its horizontal form is concerned, is relatively stable. Such a shore-line
may be said to be mature[163] so far as wave-erosion is concerned. Since
coastal lands are, in general, both heterogeneous and unequally exposed, a
mature coast-line is somewhat irregular. Its maturity is attained when the
lesser exposure in the reëntrants developed in the less resistant parts,
balances the superior exposure of the projections of the more resistant
portions.
Since the conditions of erosion along coasts are constantly, even if
slowly, changing, maturity is constantly being approached, but rarely
reached. Other forces and processes, such as those of aggradation,
vulcanism, and diastrophism, are in operation along coasts, and their results
are sometimes antagonistic to those of the waves. The horizontal
configuration of coasts is, therefore, the result of many coöperating forces,
of which waves are but one. It is, nevertheless, important to note the goal to
which the waves are working, even though they are continually defeated in
their attempt to reach it. Their immediate goal is an equilibrium of erosion-
rate and maturity of configuration; their final goal is the destruction of the
land and the deposition of its substance in the sea, that is, in a position
nearer the center of gravity of the earth.
Page 418
Transportation by Waves.
The material eroded from the shore by the waves in the shaping of the
cliff and terrace is carried away by the joint action of the waves, undertow,
and shore-currents.
The in-coming wave begins to shift material where it begins to drag
bottom, that is, a little outside the line of breakers. From the line where
transportation begins, to the line of breakers, bottom detritus is shifted
shoreward by the waves, while the undertow tends to carry it back again.
Between the breakers and the shore there is also a tendency for the on-shore
movement to carry débris to the water’s edge, and for the ebbing wave to
carry it back again. The result of these opposed tendencies is to keep
sediment in transit between the shore and the line of breakers. If the in-
coming waves have a direction normal to the shore, the advance and recoil
of the water move particles toward and from the shore, but effect no transfer
along the shore; but the results which waves normal to the shore would
achieve are always modified by other waves and by littoral currents.
If the in-coming wave is oblique to the shore, it shifts material in its own
direction. The transfer by undertow, taken alone, would be sensibly normal
to the shore, but the effect of the oblique waves is to slightly modify this
direction. There is thus a slow transportation along shore, even in the
absence of steady currents. A great amount of transportation would be
effected in this way, though it would be carried on at a slow rate. Oblique
waves also tend to develop a definite shore-current (p. 342) which affects
both the amount and direction of the transportation. Any particle in
suspension, or in motion on the bottom as the result of the wave or
undertow, is shifted along shore by the littoral current, which affects the
same water (Fig. 300). By the coöperation of wave- and shore-current, more
and heavier material can be moved than by either alone, and the direction of
movement is more nearly parallel to the shore than that of the wave.
Similarly, by the coöperation of undertow and shore-current, more and
heavier material can be moved than by either alone. The direction of
movement is readily inferred from Fig. 300. The direction in which débris is
shifted by wave- and shore-current is modified by the undertow, and the
direction which would result from undertow and current is modified by the
wave. It is often the waves of storms, rather than those of the prevailing
winds, which determine the direction of greatest shore transportation.
The material eroded from the shore by the waves in the shaping of the
cliff and terrace is carried away by the joint action of the waves, undertow,
and shore-currents.
The in-coming wave begins to shift material where it begins to drag
bottom, that is, a little outside the line of breakers. From the line where
transportation begins, to the line of breakers, bottom detritus is shifted
shoreward by the waves, while the undertow tends to carry it back again.
Between the breakers and the shore there is also a tendency for the on-shore
movement to carry débris to the water’s edge, and for the ebbing wave to
carry it back again. The result of these opposed tendencies is to keep
sediment in transit between the shore and the line of breakers. If the in-
coming waves have a direction normal to the shore, the advance and recoil
of the water move particles toward and from the shore, but effect no transfer
along the shore; but the results which waves normal to the shore would
achieve are always modified by other waves and by littoral currents.
If the in-coming wave is oblique to the shore, it shifts material in its own
direction. The transfer by undertow, taken alone, would be sensibly normal
to the shore, but the effect of the oblique waves is to slightly modify this
direction. There is thus a slow transportation along shore, even in the
absence of steady currents. A great amount of transportation would be
effected in this way, though it would be carried on at a slow rate. Oblique
waves also tend to develop a definite shore-current (p. 342) which affects
both the amount and direction of the transportation. Any particle in
suspension, or in motion on the bottom as the result of the wave or
undertow, is shifted along shore by the littoral current, which affects the
same water (Fig. 300). By the coöperation of wave- and shore-current, more
and heavier material can be moved than by either alone, and the direction of
movement is more nearly parallel to the shore than that of the wave.
Similarly, by the coöperation of undertow and shore-current, more and
heavier material can be moved than by either alone. The direction of
movement is readily inferred from Fig. 300. The direction in which débris is
shifted by wave- and shore-current is modified by the undertow, and the
direction which would result from undertow and current is modified by the
wave. It is often the waves of storms, rather than those of the prevailing
winds, which determine the direction of greatest shore transportation.
Page 419
The waves, the undertow, and the littoral currents work together in
assorting the detritus of the shore. The coarsest parts may be beyond the
power of all but the strongest waves. They accumulate where agitation is
great. Less coarse parts are shifted farther from the site of greatest agitation,
but no materials which are classed as coarse are carried beyond the depth of
sensible movement. The coarse material which covers the bottom where the
agitation of the water at the bottom is effective, constitutes shore drift.
Shore drift is not all derived from the shore by the cutting of the waves.
A part of it is brought to the sea by streams and mingled with that eroded
from the cliffs. The material which is fine enough to be held in suspension
is measurably independent of depth. This is shown during storms when the
water becomes turbid far beyond the line of breakers, and clears only after
the waves have died away.
This sorting of shore drift, effected while it is in transportation, is often
very perfect. The conditions favoring assortment are (1) vigorous wave-
action, (2) prolonged transportation, and (3) a moderate volume of
sediment.[164] The effect of these several conditions will be readily
understood.
Extensive transportation of shore drift of a given degree of coarseness is
favored by (1) strong waves and undertow, (2) continuous currents, and (3)
shallow water, deepening but gradually off shore.
Deposition by Waves, Undertow, and Shore-currents.[165]
The beach.—The zone
occupied by the shore drift in
transit is the beach. The lower
margin is beneath the water, a
little beyond the line where the
great storm-waves break. Its upper Fig. 312.—Cross-section of the beach.
margin is at the level reached by (Gilbert.)
storm-waves, and is usually a few feet above the level of still water. To the
beach, material is brought from seaward by the in-coming waves, and from
it detritus is carried out by the undertow. The cross-section of a beach is
shown in Fig. 312. In horizontal position the beach follows the general
boundary between water and land, though it does not conform to its minor
assorting the detritus of the shore. The coarsest parts may be beyond the
power of all but the strongest waves. They accumulate where agitation is
great. Less coarse parts are shifted farther from the site of greatest agitation,
but no materials which are classed as coarse are carried beyond the depth of
sensible movement. The coarse material which covers the bottom where the
agitation of the water at the bottom is effective, constitutes shore drift.
Shore drift is not all derived from the shore by the cutting of the waves.
A part of it is brought to the sea by streams and mingled with that eroded
from the cliffs. The material which is fine enough to be held in suspension
is measurably independent of depth. This is shown during storms when the
water becomes turbid far beyond the line of breakers, and clears only after
the waves have died away.
This sorting of shore drift, effected while it is in transportation, is often
very perfect. The conditions favoring assortment are (1) vigorous wave-
action, (2) prolonged transportation, and (3) a moderate volume of
sediment.[164] The effect of these several conditions will be readily
understood.
Extensive transportation of shore drift of a given degree of coarseness is
favored by (1) strong waves and undertow, (2) continuous currents, and (3)
shallow water, deepening but gradually off shore.
Deposition by Waves, Undertow, and Shore-currents.[165]
The beach.—The zone
occupied by the shore drift in
transit is the beach. The lower
margin is beneath the water, a
little beyond the line where the
great storm-waves break. Its upper Fig. 312.—Cross-section of the beach.
margin is at the level reached by (Gilbert.)
storm-waves, and is usually a few feet above the level of still water. To the
beach, material is brought from seaward by the in-coming waves, and from
it detritus is carried out by the undertow. The cross-section of a beach is
shown in Fig. 312. In horizontal position the beach follows the general
boundary between water and land, though it does not conform to its minor
Page 420
irregularities (Fig. 313). The beach or barrier ridge often causes the
deflection of the lower courses of streams descending to it (Pl. XXI).
Fig. 313.—A lake-beach (barrier); Griffin’s Bay, Lake Ontario.
deflection of the lower courses of streams descending to it (Pl. XXI).
Fig. 313.—A lake-beach (barrier); Griffin’s Bay, Lake Ontario.
Page 421
PLATE XXI.
U. S. Geol. Surv. NEW JERSEY. Scale, 1 mile per inch.
U. S. Geol. Surv. NEW JERSEY. Scale, 1 mile per inch.
Page 422
PLATE XXII.
U. S. Geol. Surv. Fig. 1. PORTION OF SOUTH COAST OF MARTHAS Scale, 1 mile per inch.
VINEYARD, MASSACHUSETTS.
U. S. Geol. Surv. Fig. 1. PORTION OF SOUTH COAST OF MARTHAS Scale, 1 mile per inch.
VINEYARD, MASSACHUSETTS.
Page 423
U. S. Geol. Surv. Fig. 2. PORTION OF THE CALIFORNIA COAST NEAR Scale, 1 mile per inch.
TAMALPAIS.
The barrier.—When the agitation
of the water along shore becomes
insufficient to carry the material, it is
Fig. 314.—Section of a barrier. (Gilbert.)
dropped. In its deposition it assumes
various forms. Where the bottom of the lake or sea near shore has a very
gentle inclination, the in-coming waves break some distance from the
shore-line, and it is here that the most violent agitation occurs when the
waves are strong. To this line of breakers, material is shifted from both
directions: from shore by undertow, and from seaward by the waves.
Accumulating here, it builds up a low ridge. This is a barrier (Fig. 314). If
it is built up above the surface of the water by storm-waves, it may shut in a
lagoon behind it, and this may ultimately be filled by sediment washed
down from the land. At one stage in the filling, the lagoon becomes a
marsh.[166] In the part which the barrier plays in the history of a coast, it is
identical with the beach.
TAMALPAIS.
The barrier.—When the agitation
of the water along shore becomes
insufficient to carry the material, it is
Fig. 314.—Section of a barrier. (Gilbert.)
dropped. In its deposition it assumes
various forms. Where the bottom of the lake or sea near shore has a very
gentle inclination, the in-coming waves break some distance from the
shore-line, and it is here that the most violent agitation occurs when the
waves are strong. To this line of breakers, material is shifted from both
directions: from shore by undertow, and from seaward by the waves.
Accumulating here, it builds up a low ridge. This is a barrier (Fig. 314). If
it is built up above the surface of the water by storm-waves, it may shut in a
lagoon behind it, and this may ultimately be filled by sediment washed
down from the land. At one stage in the filling, the lagoon becomes a
marsh.[166] In the part which the barrier plays in the history of a coast, it is
identical with the beach.
Page 424
Fig. 315.—A recurved spit. Dutch Point, Grand Traverse Bay, Lake Michigan.
The spit, the bar, and the loop.—
The disposition of shore-deposits
depends largely on the currents at and
near shore. If the coast-line is deeply
indented, the littoral current usually Fig. 316.—Cross-section of a bar.
fails to follow the reëntrants. In (Gilbert.)
holding its course across the mouth of
a small bay, a shore-current usually passes into deeper water. Here its
velocity is checked because its motion is communicated to the water
beneath it, and a larger amount of water being involved in the motion, the
motion of each part is diminished. If sediment was being moved along its
bottom before the current was checked, some part of it is dropped when and
where the current is slackened. It follows that deposition commonly takes
place beneath a littoral current as it crosses the mouth of a bay. The belt of
deposition is often narrow, and the result is the construction of a ridge
beneath the water in the direction of the current. The current would never
build the embankment up to the water-level, but when its surface
approaches the level of effective agitation, the waves may begin to work on
it, as on a barrier, and may build it up to, and even above, the surface of the
water. So long as the end of such an embankment is free, it is a spit (Fig.
315 and Pl. XXI). If the spit be lengthened until it crosses, or nearly
crosses, the bay, shutting it off from the open water, it becomes a bar. Bars
have shut in lakes (ponds) on the coast of Martha’s Vineyard, Mass. (Fig. 1,
Pl. XXII), and lakes and lagoons at numerous points both on the Atlantic
and the Pacific coasts (Fig. 2, Pl. XXII, Rodeo lagoon). The same
phenomena are to be seen along many lake shores. Bars sometimes tie
islands to the mainland (Pl. XXIII, Fig. 1, Nahant, Mass.; Fig. 2, near
The spit, the bar, and the loop.—
The disposition of shore-deposits
depends largely on the currents at and
near shore. If the coast-line is deeply
indented, the littoral current usually Fig. 316.—Cross-section of a bar.
fails to follow the reëntrants. In (Gilbert.)
holding its course across the mouth of
a small bay, a shore-current usually passes into deeper water. Here its
velocity is checked because its motion is communicated to the water
beneath it, and a larger amount of water being involved in the motion, the
motion of each part is diminished. If sediment was being moved along its
bottom before the current was checked, some part of it is dropped when and
where the current is slackened. It follows that deposition commonly takes
place beneath a littoral current as it crosses the mouth of a bay. The belt of
deposition is often narrow, and the result is the construction of a ridge
beneath the water in the direction of the current. The current would never
build the embankment up to the water-level, but when its surface
approaches the level of effective agitation, the waves may begin to work on
it, as on a barrier, and may build it up to, and even above, the surface of the
water. So long as the end of such an embankment is free, it is a spit (Fig.
315 and Pl. XXI). If the spit be lengthened until it crosses, or nearly
crosses, the bay, shutting it off from the open water, it becomes a bar. Bars
have shut in lakes (ponds) on the coast of Martha’s Vineyard, Mass. (Fig. 1,
Pl. XXII), and lakes and lagoons at numerous points both on the Atlantic
and the Pacific coasts (Fig. 2, Pl. XXII, Rodeo lagoon). The same
phenomena are to be seen along many lake shores. Bars sometimes tie
islands to the mainland (Pl. XXIII, Fig. 1, Nahant, Mass.; Fig. 2, near
Page 425
Biddeford, Me.). The structure of a bar as seen in cross-section is shown in
Fig. 316.
The construction of a spit has been aptly compared to the construction of
a railway embankment across a depression. The material is first carried out
from the bordering upland (shallow water) and dumped where the slope to
the depression (deep water) begins. The embankment thus begun is
extended by the carrying out of new material, which is left at the end of the
dump already made.
If the bay across which the bar is built receives abundant drainage from
the land, the outflow from the bay may be sufficient to prevent the
completion of the bar (Fig. 2, Pl. XXII), for when the growth of the spit has
sufficiently narrowed the outlet of the bay, the sediment brought to the end
of the spit by the littoral current will be swept out beyond the spit by the
current setting out from the bay.
The completion of a bar may be interfered with by tidal currents, even
without land-drainage. Currents generated by the tides may sweep in or out
of the bay with increased force as the entrance is narrowed, carrying in or
out the sediment which the littoral current would have left at the end of the
spit. The scour of the tides often insures deep entrances (inlets) to bays, and
maintains definite channels or “thorofares” in the lagoon marshes behind
barriers and spits. The sediment brought down from the land, as well as that
washed in by tidal currents and waves, tends to fill up the lagoon behind a
barrier, a spit, or a bar, converting it into land (Fig. 317).
Fig. 316.
The construction of a spit has been aptly compared to the construction of
a railway embankment across a depression. The material is first carried out
from the bordering upland (shallow water) and dumped where the slope to
the depression (deep water) begins. The embankment thus begun is
extended by the carrying out of new material, which is left at the end of the
dump already made.
If the bay across which the bar is built receives abundant drainage from
the land, the outflow from the bay may be sufficient to prevent the
completion of the bar (Fig. 2, Pl. XXII), for when the growth of the spit has
sufficiently narrowed the outlet of the bay, the sediment brought to the end
of the spit by the littoral current will be swept out beyond the spit by the
current setting out from the bay.
The completion of a bar may be interfered with by tidal currents, even
without land-drainage. Currents generated by the tides may sweep in or out
of the bay with increased force as the entrance is narrowed, carrying in or
out the sediment which the littoral current would have left at the end of the
spit. The scour of the tides often insures deep entrances (inlets) to bays, and
maintains definite channels or “thorofares” in the lagoon marshes behind
barriers and spits. The sediment brought down from the land, as well as that
washed in by tidal currents and waves, tends to fill up the lagoon behind a
barrier, a spit, or a bar, converting it into land (Fig. 317).
Page 426
Fig. 317.—Sketch of a portion of the New Jersey coast. The dotted belt next the sea is the
barrier, modified by the wind. The area marked by the diagonal lines is the mainland. In
the marshy area between, there are numerous channels or “thorofares” kept open by the
currents. The figures show the depths of water in feet. Scale about ⅜ inch = 1 mile.
Since spits and bars are built only where there is shore-drift in transit,
they are always built out from a beach or barrier. The distal end of the bar
may also join a beach or barrier. Traced back to its source, the beach from
which a spit leads out is often found to terminate in the cliff from which the
material of the beach and the spit were derived (Pl. XX and Fig. 2, Pl.
XXII). In such cases the sediment of the beach has been shifted but a short
distance; but in other cases it has traveled far.
barrier, modified by the wind. The area marked by the diagonal lines is the mainland. In
the marshy area between, there are numerous channels or “thorofares” kept open by the
currents. The figures show the depths of water in feet. Scale about ⅜ inch = 1 mile.
Since spits and bars are built only where there is shore-drift in transit,
they are always built out from a beach or barrier. The distal end of the bar
may also join a beach or barrier. Traced back to its source, the beach from
which a spit leads out is often found to terminate in the cliff from which the
material of the beach and the spit were derived (Pl. XX and Fig. 2, Pl.
XXII). In such cases the sediment of the beach has been shifted but a short
distance; but in other cases it has traveled far.
Page 427
Fig. 318.—Map of shore-terraces, largely wave-built. Lake Bonneville. (Gilbert.)
Page 428
Fig. 319.—A portion of the Texas coast showing the tendency of shore-deposition to
simplify the coast-line. The deposits (the narrow necks of land parallel to the coast) shut
in the bays. (From chart of C. and G. Surv.)
simplify the coast-line. The deposits (the narrow necks of land parallel to the coast) shut
in the bays. (From chart of C. and G. Surv.)
Page 429
Fig. 320.—Map showing that in the early stages of the simplification of a shore-line the
irregularities are increased. The numbers indicate the depth of water in fathoms. (From
chart of C. and G. Surv.)
The spit is usually either straight or in conformity with the general course
of the shore-current, but since the littoral current itself is subject to
alteration as the result of shifting winds, the spit may depart from
straightness. Winds which simply reverse the direction of the littoral current
retard its construction, but may not otherwise affect it; but if a strong
current be made to flow past the end of a spit, it may cut away its extremity
and rebuild the materials into a smaller spit, joining the main one at an
angle. This gives rise to a hook (Fig. 315). Successive storms may develop
irregularities are increased. The numbers indicate the depth of water in fathoms. (From
chart of C. and G. Surv.)
The spit is usually either straight or in conformity with the general course
of the shore-current, but since the littoral current itself is subject to
alteration as the result of shifting winds, the spit may depart from
straightness. Winds which simply reverse the direction of the littoral current
retard its construction, but may not otherwise affect it; but if a strong
current be made to flow past the end of a spit, it may cut away its extremity
and rebuild the materials into a smaller spit, joining the main one at an
angle. This gives rise to a hook (Fig. 315). Successive storms may develop
Page 430
successive hooks along the side of a growing spit. The end of a hook may
be so extended as to join the mainland, when it becomes a loop.
Wave-built terraces.—Under the influence of off-shore currents, littoral
currents may be drawn from the coast-line. If such a current continues as a
well-defined surface-current, it builds a spit, but if it spreads, it tends to
build a terrace. The accumulation then is not at the end of a beach, as in the
case of a spit, but on its side, and the result of the deposition is to carry the
beach seaward. The undertow abets the process. The widened beach is a
wave-built terrace. The wave-built terrace often borders the wave-cut
terrace along its seaward margin (Figs. 303 and 318). With the help of
waves, the surface of the terrace may be built up into land by the expansion
of the crest of the beach. Terrace-cutting and terrace-building are both
involved in the development of the continental shelves.
Beach ridges, spits, bars, etc., like sea-cliffs and wave-cut terraces, are
often preserved after the relative level of sea and land has changed. If the
shore has risen, relatively or absolutely, these features are relied on as
evidences of the change. If shore features be submerged instead of elevated,
they furnish less accessible, though not less real, evidence of the change of
level. Similar features about lakes have a like significance, but in this case it
is often demonstrable that it is the water rather than the land which has
changed its level.
Effect of Shore-deposition on Coastal Configuration.
The tendency of shore-deposition is to cut off bays and to straighten and
simplify the shore-lines. This is abundantly illustrated along the Atlantic
and Gulf coasts of the United States (see Fig. 319 and Pl. XXII). It is to be
noted, however, that in the simplification of the shore-line through
deposition, the initial stages often result in great irregularity (Fig. 320 and
Pl. XXIII). In some cases, the irregularities are not temporary. Thus deltas
(p. 198), though not wholly the work of sea- (or lake-) water, often
constitute irregularities of a more or less permanent nature. This is the case
where they project beyond the general trend of the coast-line. Where, on the
other hand, they are built at the heads of bays, they tend to simplify the
coast-line by obliterating the indentation. The delta at the head of the Gulf
of California is an example. So too is the delta of the Mississippi, the real
head of which is far above the present debouchure of the stream. The form
be so extended as to join the mainland, when it becomes a loop.
Wave-built terraces.—Under the influence of off-shore currents, littoral
currents may be drawn from the coast-line. If such a current continues as a
well-defined surface-current, it builds a spit, but if it spreads, it tends to
build a terrace. The accumulation then is not at the end of a beach, as in the
case of a spit, but on its side, and the result of the deposition is to carry the
beach seaward. The undertow abets the process. The widened beach is a
wave-built terrace. The wave-built terrace often borders the wave-cut
terrace along its seaward margin (Figs. 303 and 318). With the help of
waves, the surface of the terrace may be built up into land by the expansion
of the crest of the beach. Terrace-cutting and terrace-building are both
involved in the development of the continental shelves.
Beach ridges, spits, bars, etc., like sea-cliffs and wave-cut terraces, are
often preserved after the relative level of sea and land has changed. If the
shore has risen, relatively or absolutely, these features are relied on as
evidences of the change. If shore features be submerged instead of elevated,
they furnish less accessible, though not less real, evidence of the change of
level. Similar features about lakes have a like significance, but in this case it
is often demonstrable that it is the water rather than the land which has
changed its level.
Effect of Shore-deposition on Coastal Configuration.
The tendency of shore-deposition is to cut off bays and to straighten and
simplify the shore-lines. This is abundantly illustrated along the Atlantic
and Gulf coasts of the United States (see Fig. 319 and Pl. XXII). It is to be
noted, however, that in the simplification of the shore-line through
deposition, the initial stages often result in great irregularity (Fig. 320 and
Pl. XXIII). In some cases, the irregularities are not temporary. Thus deltas
(p. 198), though not wholly the work of sea- (or lake-) water, often
constitute irregularities of a more or less permanent nature. This is the case
where they project beyond the general trend of the coast-line. Where, on the
other hand, they are built at the heads of bays, they tend to simplify the
coast-line by obliterating the indentation. The delta at the head of the Gulf
of California is an example. So too is the delta of the Mississippi, the real
head of which is far above the present debouchure of the stream. The form
Page 431
of the delta in ground-plan depends on the horizontal configuration of the
coast where it is developed, on the strength of the waves and shore-currents,
and on their relation to the amount of detritus contributed by the stream
concerned. Good illustrations are furnished by the Gulf of Mexico where
the deltas of the Mississippi and Rio Grande are in contrast.
So far as concerns the vertical configuration of coasts, erosion and
deposition are in contrast, for while the former tends to develop steep,
irregular, and often high slopes (p. 349) from the land to the sea, the latter
tends to develop gentle, regular, and low ones. A partial exception to the
latter part of this general statement comes about through the building of
dunes, the material for which is furnished by the waves.
SUMMARY OF COASTAL IRREGULARITIES.
The horizontal irregularities of coasts are both large and small. Some of
them, like Florida, Sandy Hook, etc., consist primarily of projections of
land into the sea; others, like Chesapeake Bay, the Gulf of Mexico, and
Puget Sound, are projections of the sea into the land; while still others, like
the Gulf of California and its associated peninsula, cannot readily be put in
either of the foregoing classes. Some of the irregularities of the land border,
such as Yucatan, are more or less nearly normal to the general trend of the
coast which they affect, while others, such as the “beaches” along the
Atlantic and Gulf coasts of the United States (Figs. 319 and 320), are more
or less nearly parallel with it. Some of the irregularities, especially some of
the small ones, are more or less angular in their outline (Pl. XX and parts of
Fig. 2, Pl. XXII), while others are bounded by curves instead.
In many cases more than one factor has been involved in the
development of irregularities. In the case of great irregularities,
diastrophism has generally been the dominant factor. The Gulf of Mexico
and the Mediterranean Sea perhaps represent differential subsidence, while
Florida and the Iberian peninsula represent differential uplift (relative,
though perhaps not absolute). The narrow bays which indent many coasts
generally represent the subsidence of a region previously affected by
valleys (Fig. 297). Many of them, such as Narragansett, Delaware, and
Chesapeake Bays, are primarily the drowned ends of river valleys, while
others, such as Puget Sound,[167] are primarily structural valleys (synclines).
coast where it is developed, on the strength of the waves and shore-currents,
and on their relation to the amount of detritus contributed by the stream
concerned. Good illustrations are furnished by the Gulf of Mexico where
the deltas of the Mississippi and Rio Grande are in contrast.
So far as concerns the vertical configuration of coasts, erosion and
deposition are in contrast, for while the former tends to develop steep,
irregular, and often high slopes (p. 349) from the land to the sea, the latter
tends to develop gentle, regular, and low ones. A partial exception to the
latter part of this general statement comes about through the building of
dunes, the material for which is furnished by the waves.
SUMMARY OF COASTAL IRREGULARITIES.
The horizontal irregularities of coasts are both large and small. Some of
them, like Florida, Sandy Hook, etc., consist primarily of projections of
land into the sea; others, like Chesapeake Bay, the Gulf of Mexico, and
Puget Sound, are projections of the sea into the land; while still others, like
the Gulf of California and its associated peninsula, cannot readily be put in
either of the foregoing classes. Some of the irregularities of the land border,
such as Yucatan, are more or less nearly normal to the general trend of the
coast which they affect, while others, such as the “beaches” along the
Atlantic and Gulf coasts of the United States (Figs. 319 and 320), are more
or less nearly parallel with it. Some of the irregularities, especially some of
the small ones, are more or less angular in their outline (Pl. XX and parts of
Fig. 2, Pl. XXII), while others are bounded by curves instead.
In many cases more than one factor has been involved in the
development of irregularities. In the case of great irregularities,
diastrophism has generally been the dominant factor. The Gulf of Mexico
and the Mediterranean Sea perhaps represent differential subsidence, while
Florida and the Iberian peninsula represent differential uplift (relative,
though perhaps not absolute). The narrow bays which indent many coasts
generally represent the subsidence of a region previously affected by
valleys (Fig. 297). Many of them, such as Narragansett, Delaware, and
Chesapeake Bays, are primarily the drowned ends of river valleys, while
others, such as Puget Sound,[167] are primarily structural valleys (synclines).
Page 432
Many of the long and narrow bays or fiords common in the high latitudes of
North America and Europe (Fig. 266, p. 293) appear to be the drowned ends
of valleys previously deepened by glaciers. The drowned ends of river
canyons, and the submerged parts of valleys excavated (not sunk) beneath
the sea by glaciers, would also be fiords.
PLATE XXIII.
U. S. Geol. Surv. Fig. 1. Scale, 1+ mile per inch.
MASSACHUSET
TS.
North America and Europe (Fig. 266, p. 293) appear to be the drowned ends
of valleys previously deepened by glaciers. The drowned ends of river
canyons, and the submerged parts of valleys excavated (not sunk) beneath
the sea by glaciers, would also be fiords.
PLATE XXIII.
U. S. Geol. Surv. Fig. 1. Scale, 1+ mile per inch.
MASSACHUSET
TS.
Page 433
U. S. Geol. Surv. Fig. 2. MAINE. Scale, 1+ mile per inch.
Page 434
PLATE XXIV.
U. S. Geol. Surv. PORTION OF THE Scale, 1+ mile per inch.
COAST OF MAINE.
The processes which develop coastal indentations, together with the
antecedent subaërial and the subsequent wave gradation, account for most
of the islands which affect indented coasts. Some of them are high and
some low for reasons which will be readily understood. The long narrow
belts of land constituting irregularities parallel to the general trend of the
coast (Figs. 319 and 320) are usually the result of deposition in shallow
water. They are usually sand or coral reefs, built up above water-level by
waves. The deposits at the debouchures of streams give rise to projecting
U. S. Geol. Surv. PORTION OF THE Scale, 1+ mile per inch.
COAST OF MAINE.
The processes which develop coastal indentations, together with the
antecedent subaërial and the subsequent wave gradation, account for most
of the islands which affect indented coasts. Some of them are high and
some low for reasons which will be readily understood. The long narrow
belts of land constituting irregularities parallel to the general trend of the
coast (Figs. 319 and 320) are usually the result of deposition in shallow
water. They are usually sand or coral reefs, built up above water-level by
waves. The deposits at the debouchures of streams give rise to projecting
Page 435
deltas. Most small irregularities of angular form, especially if high (Pl. XX),
indicate wave-erosion, and their details of form are determined by the
structure of the rock along shore, while most irregularities of curved outline
involve something of shore-deposition, if not due wholly to it. Glaciation,
or glaciation and subsidence, may also give rise to peninsulas, capes, and
islands of curved outlines (Pl. XXIV, coast of Maine). Curving outlines
may, however, be developed by erosion alone in weak rock structures. This
is illustrated by the weak rock structures (clay, sand, etc.) of most of the
Atlantic coastal plain. Thus inspection of the horizontal configuration of
coasts will often indicate the processes which have been dominant there in
recent times. On the other hand, the interpretations of many coastal
irregularities, such as Hudson Bay, Puget Sound, the Gulf of California, the
Baltic Sea, etc., are not to be read from the map. In such cases, diastrophism
and gradation have usually coöperated, but the relative importance of the
two processes can only be determined by detailed study in the field. When it
is remembered that the tendency of shore-erosion is to reduce great
irregularities of horizontal configuration, though not to obliterate small ones
if the coast be heterogeneous in composition (p. 353), and that the tendency
of shore-deposition is also to regularity, it is clear that the great
irregularities of coast-lines are due neither to shore-erosion nor to shore-
deposition, though minor ones may be due to either.
THE WORK OF OCEAN-CURRENTS.
As agents of erosion, ocean-currents are not, in general, of great
importance. Currents which reach the bottom are comparable, in their
effects, to rivers of the same velocity and volume; but most ocean-currents
do not touch bottom, and, therefore, do not erode it. Where the current
agitates the bottom sensibly, as it often does in shallow water, the bottom is
abraded, and in the lee of such places it is doubtless aggraded. Since ocean-
currents do not, for the most part, flow in shallow water, their erosive work
is, on the whole, relatively slight; but where they are forced through narrow
and shallow passageways, their abrasive work may be considerable. Thus
the Gulf Stream, where it issues from the Gulf, has a velocity of four or five
miles per hour, and its shallow and narrow channel is current-swept.
indicate wave-erosion, and their details of form are determined by the
structure of the rock along shore, while most irregularities of curved outline
involve something of shore-deposition, if not due wholly to it. Glaciation,
or glaciation and subsidence, may also give rise to peninsulas, capes, and
islands of curved outlines (Pl. XXIV, coast of Maine). Curving outlines
may, however, be developed by erosion alone in weak rock structures. This
is illustrated by the weak rock structures (clay, sand, etc.) of most of the
Atlantic coastal plain. Thus inspection of the horizontal configuration of
coasts will often indicate the processes which have been dominant there in
recent times. On the other hand, the interpretations of many coastal
irregularities, such as Hudson Bay, Puget Sound, the Gulf of California, the
Baltic Sea, etc., are not to be read from the map. In such cases, diastrophism
and gradation have usually coöperated, but the relative importance of the
two processes can only be determined by detailed study in the field. When it
is remembered that the tendency of shore-erosion is to reduce great
irregularities of horizontal configuration, though not to obliterate small ones
if the coast be heterogeneous in composition (p. 353), and that the tendency
of shore-deposition is also to regularity, it is clear that the great
irregularities of coast-lines are due neither to shore-erosion nor to shore-
deposition, though minor ones may be due to either.
THE WORK OF OCEAN-CURRENTS.
As agents of erosion, ocean-currents are not, in general, of great
importance. Currents which reach the bottom are comparable, in their
effects, to rivers of the same velocity and volume; but most ocean-currents
do not touch bottom, and, therefore, do not erode it. Where the current
agitates the bottom sensibly, as it often does in shallow water, the bottom is
abraded, and in the lee of such places it is doubtless aggraded. Since ocean-
currents do not, for the most part, flow in shallow water, their erosive work
is, on the whole, relatively slight; but where they are forced through narrow
and shallow passageways, their abrasive work may be considerable. Thus
the Gulf Stream, where it issues from the Gulf, has a velocity of four or five
miles per hour, and its shallow and narrow channel is current-swept.
Page 436
A rough test of the abrasive work of an ocean-current is found in the
nature of the bottom beneath it. If this be hard, it indicates that the loose
sediment on the floor of the ocean has been swept away, while the presence
of fine detritus indicates that the current is not wearing. Thus the abrasive
power of the Gulf Stream is known to continue somewhat beyond its
narrow channel, for on the Blake plateau (between the Bahamas and Cape
Hatteras), where the water is 600 fathoms and less in depth, “the bottom of
the Gulf Stream ... is swept clean of lime and ooze and is nearly barren of
animal life.”[168] Other illustrations of the erosive power of currents have
been noted near Gibraltar in water 500 fathoms deep, and between the
Canary Islands at depths of 1000 fathoms.[169] In spite of these examples,
and of many others which probably exist in similar situations, it yet remains
true that ocean-currents are on the whole but feeble agents of erosion.
As agents of transportation, ocean-currents are scarcely more important
than as agents of corrasion, for they transport only what they erode, if the
life which inhabits them be left out of consideration. This phase of their
work has probably been exaggerated through a confusion of transporting
energy and actual transportation. Ocean-currents which do not touch bottom
roll no sediment and carry only what may be held in suspension. A river’s
power of transporting sediment in suspension is due largely to the cross-
currents occasioned by the unevenness of its resistant bottom (p. 117). If a
particle of mud in suspension in a river drops to the bottom, as it frequently
does, it may be picked up again and carried forward. If, on the other hand, a
particle in suspension in an ocean-current once escapes the moving water
by settling through it, the current which does not drag bottom has no chance
to pick it up again. Very fine sediment may be carried by an ocean-current
far beyond the point where it was acquired, but currents which do not touch
bottom are rarely strong enough to hold any but the finest material for any
considerable length of time. As transporters of sediment, therefore, ocean-
currents are at a great disadvantage as compared with rivers.
How readily particles of extreme fineness may be kept in suspension, and
how little agitation is necessary to keep them from sinking, is shown by the
experiments of Sorby, who showed that while a sand grain ¹⁄₁₀₀ of an inch in
diameter will settle one foot per second in still water, fine particles of clay
require days to sink through the same distance. The Challenger found fine
sediment derived from the land 400 miles from the coast of Africa, and that
nature of the bottom beneath it. If this be hard, it indicates that the loose
sediment on the floor of the ocean has been swept away, while the presence
of fine detritus indicates that the current is not wearing. Thus the abrasive
power of the Gulf Stream is known to continue somewhat beyond its
narrow channel, for on the Blake plateau (between the Bahamas and Cape
Hatteras), where the water is 600 fathoms and less in depth, “the bottom of
the Gulf Stream ... is swept clean of lime and ooze and is nearly barren of
animal life.”[168] Other illustrations of the erosive power of currents have
been noted near Gibraltar in water 500 fathoms deep, and between the
Canary Islands at depths of 1000 fathoms.[169] In spite of these examples,
and of many others which probably exist in similar situations, it yet remains
true that ocean-currents are on the whole but feeble agents of erosion.
As agents of transportation, ocean-currents are scarcely more important
than as agents of corrasion, for they transport only what they erode, if the
life which inhabits them be left out of consideration. This phase of their
work has probably been exaggerated through a confusion of transporting
energy and actual transportation. Ocean-currents which do not touch bottom
roll no sediment and carry only what may be held in suspension. A river’s
power of transporting sediment in suspension is due largely to the cross-
currents occasioned by the unevenness of its resistant bottom (p. 117). If a
particle of mud in suspension in a river drops to the bottom, as it frequently
does, it may be picked up again and carried forward. If, on the other hand, a
particle in suspension in an ocean-current once escapes the moving water
by settling through it, the current which does not drag bottom has no chance
to pick it up again. Very fine sediment may be carried by an ocean-current
far beyond the point where it was acquired, but currents which do not touch
bottom are rarely strong enough to hold any but the finest material for any
considerable length of time. As transporters of sediment, therefore, ocean-
currents are at a great disadvantage as compared with rivers.
How readily particles of extreme fineness may be kept in suspension, and
how little agitation is necessary to keep them from sinking, is shown by the
experiments of Sorby, who showed that while a sand grain ¹⁄₁₀₀ of an inch in
diameter will settle one foot per second in still water, fine particles of clay
require days to sink through the same distance. The Challenger found fine
sediment derived from the land 400 miles from the coast of Africa, and that
Page 437
not opposite the debouchure of any large river. Sediment settles more
readily in salt water than in fresh, despite the fact that the former is heavier.
This is presumably because the salt diminishes the cohesion of the water.
Deposition by ocean-currents is limited by their transportation. Only
where they erode their bottoms do they gather coarse materials, and only in
the lee of such places are their deposits coarse. Since the material which
they carry is generally fine, it is widely distributed before deposition.
Ocean-currents have little influence on the configuration of coast-lines.
DEPOSITS ON THE OCEAN-BED.
Something has already been said concerning the sediments which
accumulate in the shallow waters along shores; but the area of marine
sedimentation is as extensive as the ocean itself, and the deposits must now
be reviewed from another point of view.
Oceanic deposits may be conveniently divided into two chief groups,
dependent on the depth of the water in which they are made.[170] These
groups are (1) shallow-water deposits, made in water less than some such
depth as 100 fathoms, and (2) deep-sea deposits, laid down in water of
greater depth. The selection of the 100-fathom line as the dividing depth is
less arbitrary than it seems, for passing outward from the shore, it is at
about this depth that the bottom ceases to be commonly disturbed by the
action of currents and waves; that sunlight and vegetable life cease to be
important at the bottom; and that the coarser sediments which predominate
along shore give place, as a rule, to muds and oozes. Furthermore, the 100-
fathom line (or some line very near it) is an important one in the physical
relief of the globe, for it appears to mark, approximately, the junction of
continental plateaus and ocean-basins. Only because the latter are a little
over-full does the water run over their rims, covering about 10,000,000
square miles of the borders of the continents, converting them from land
into epicontinental seas.
Aside from the deposits made by organisms, shallow-water deposits are
divisible into two groups—(a) those immediately along the shore, the
littoral deposits, and (b) those made between the littoral zone and the 100-
fathom line. Both are terrigenous. The deep-sea deposits likewise are
readily in salt water than in fresh, despite the fact that the former is heavier.
This is presumably because the salt diminishes the cohesion of the water.
Deposition by ocean-currents is limited by their transportation. Only
where they erode their bottoms do they gather coarse materials, and only in
the lee of such places are their deposits coarse. Since the material which
they carry is generally fine, it is widely distributed before deposition.
Ocean-currents have little influence on the configuration of coast-lines.
DEPOSITS ON THE OCEAN-BED.
Something has already been said concerning the sediments which
accumulate in the shallow waters along shores; but the area of marine
sedimentation is as extensive as the ocean itself, and the deposits must now
be reviewed from another point of view.
Oceanic deposits may be conveniently divided into two chief groups,
dependent on the depth of the water in which they are made.[170] These
groups are (1) shallow-water deposits, made in water less than some such
depth as 100 fathoms, and (2) deep-sea deposits, laid down in water of
greater depth. The selection of the 100-fathom line as the dividing depth is
less arbitrary than it seems, for passing outward from the shore, it is at
about this depth that the bottom ceases to be commonly disturbed by the
action of currents and waves; that sunlight and vegetable life cease to be
important at the bottom; and that the coarser sediments which predominate
along shore give place, as a rule, to muds and oozes. Furthermore, the 100-
fathom line (or some line very near it) is an important one in the physical
relief of the globe, for it appears to mark, approximately, the junction of
continental plateaus and ocean-basins. Only because the latter are a little
over-full does the water run over their rims, covering about 10,000,000
square miles of the borders of the continents, converting them from land
into epicontinental seas.
Aside from the deposits made by organisms, shallow-water deposits are
divisible into two groups—(a) those immediately along the shore, the
littoral deposits, and (b) those made between the littoral zone and the 100-
fathom line. Both are terrigenous. The deep-sea deposits likewise are
Page 438
divisible into two groups, (a) terrigenous deposits formed close to land, and
made up chiefly of materials derived immediately from the disintegration of
land formations; and (b) the pelagic deposits, made up chiefly of the
remains of pelagic organisms and the ultimate products arising from the
decomposition of rocks and minerals. The former predominate in the less
deep waters relatively near shore; the latter in the deeper water far from
land. The shallow- and deep-water deposits grade into each other in a belt
along the 100-fathom line.
Shallow-water Deposits.
Littoral deposits.—The littoral zone is the zone between high- and low-
water marks. It is the zone in which bowlders, gravels, sands, and all
coarser materials accumulate, though muds are occasionally met with in
sheltered estuaries. Generally speaking, the nature of these deposits is
determined by the character of the adjoining lands and the nature of the
local organisms. “The heavier materials brought by rivers from high
terrestrial regions, or thrown up by the tides and waves of the sea, are here
arranged with great diversity of stratification through the alternate play of
the winds and waves. Twice in the twenty-four hours the littoral zone is
covered by water and exposed to the direct rays of the sun or the cooling
effects of the night. There is a great range of temperature; mechanical
agencies produce their maximum effects,”[171] and physical conditions in
general are most varied. Still greater diversity is introduced by the fact that
the zone is inhabited by both marine and terrestrial organisms, while the
evaporation of the sea-water which flows over tidal marshes and lagoons
leads to the formation of saline deposits. If the length of the coast-lines of
the world be taken at 125,000 miles (about 200,000 kilometers), and the
average width of this zone at half a mile, these deposits are now forming
over an area of 62,500 square miles (about 160,000 square kilometers) of
the earth’s surface.
Non-littoral, mechanical deposits in shallow water.—These deposits
are laid down in the zone of the ocean between low-water mark and the
100-fathom line. They cover about 10,000,000 square miles.[172] Their
composition is much the same as that of the littoral deposits, with which
they are continuous, though on the whole they are finer. At their lower limit
they pass insensibly into the fine deposits of the deep sea. Coarse material,
made up chiefly of materials derived immediately from the disintegration of
land formations; and (b) the pelagic deposits, made up chiefly of the
remains of pelagic organisms and the ultimate products arising from the
decomposition of rocks and minerals. The former predominate in the less
deep waters relatively near shore; the latter in the deeper water far from
land. The shallow- and deep-water deposits grade into each other in a belt
along the 100-fathom line.
Shallow-water Deposits.
Littoral deposits.—The littoral zone is the zone between high- and low-
water marks. It is the zone in which bowlders, gravels, sands, and all
coarser materials accumulate, though muds are occasionally met with in
sheltered estuaries. Generally speaking, the nature of these deposits is
determined by the character of the adjoining lands and the nature of the
local organisms. “The heavier materials brought by rivers from high
terrestrial regions, or thrown up by the tides and waves of the sea, are here
arranged with great diversity of stratification through the alternate play of
the winds and waves. Twice in the twenty-four hours the littoral zone is
covered by water and exposed to the direct rays of the sun or the cooling
effects of the night. There is a great range of temperature; mechanical
agencies produce their maximum effects,”[171] and physical conditions in
general are most varied. Still greater diversity is introduced by the fact that
the zone is inhabited by both marine and terrestrial organisms, while the
evaporation of the sea-water which flows over tidal marshes and lagoons
leads to the formation of saline deposits. If the length of the coast-lines of
the world be taken at 125,000 miles (about 200,000 kilometers), and the
average width of this zone at half a mile, these deposits are now forming
over an area of 62,500 square miles (about 160,000 square kilometers) of
the earth’s surface.
Non-littoral, mechanical deposits in shallow water.—These deposits
are laid down in the zone of the ocean between low-water mark and the
100-fathom line. They cover about 10,000,000 square miles.[172] Their
composition is much the same as that of the littoral deposits, with which
they are continuous, though on the whole they are finer. At their lower limit
they pass insensibly into the fine deposits of the deep sea. Coarse material,
Page 439
such as gravel and sand, prevails, though in special situations, such as
depressions and inclosed basins, muddy deposits are found. While some of
the deposits are wholly composed of inorganic débris, organic remains are
freely mingled with others. The mechanical effects of tides, currents, and
waves are everywhere present, but become less and less well marked as the
100-fathom line is approached. The forms of vegetable and animal life are
numerous, though the former decrease as depths which exclude the sunlight
are approached.
Both littoral deposits and deposits in shallow water outside the littoral
zone have already been referred to in connection with the work of waves
and currents (pp. 355–66). A few additional points only need here be added.
Figs. 321 and 322.—Diagrams showing how shallow-water deposits may attain considerable
depth by the shifting of the zone of deposition seaward.
Fig. 323.—Diagram showing the interwedging of gravel-, sand-, and mud-beds.
In general the coarser sediments are lodged near shore and those farther
from the land become progressively finer. Even the coarser part of the
material carried in suspension by the undertow is partly left in the shallow
water. On the other hand, waves of exceptional strength may carry coarse
material into water of some depth. Thus coarse shingle (gravel) and even
bowlders have been found at depths of 10 fathoms.[173] Coarse deposits may
extend far out from land if the waves are strong, and especially if the water
is shallow, and since the zone of shallow water may be extended seaward
by the aggradation of the bottom, shallow-water deposits may cover
extensive areas. They may become deep at the same time, for as the outer
depressions and inclosed basins, muddy deposits are found. While some of
the deposits are wholly composed of inorganic débris, organic remains are
freely mingled with others. The mechanical effects of tides, currents, and
waves are everywhere present, but become less and less well marked as the
100-fathom line is approached. The forms of vegetable and animal life are
numerous, though the former decrease as depths which exclude the sunlight
are approached.
Both littoral deposits and deposits in shallow water outside the littoral
zone have already been referred to in connection with the work of waves
and currents (pp. 355–66). A few additional points only need here be added.
Figs. 321 and 322.—Diagrams showing how shallow-water deposits may attain considerable
depth by the shifting of the zone of deposition seaward.
Fig. 323.—Diagram showing the interwedging of gravel-, sand-, and mud-beds.
In general the coarser sediments are lodged near shore and those farther
from the land become progressively finer. Even the coarser part of the
material carried in suspension by the undertow is partly left in the shallow
water. On the other hand, waves of exceptional strength may carry coarse
material into water of some depth. Thus coarse shingle (gravel) and even
bowlders have been found at depths of 10 fathoms.[173] Coarse deposits may
extend far out from land if the waves are strong, and especially if the water
is shallow, and since the zone of shallow water may be extended seaward
by the aggradation of the bottom, shallow-water deposits may cover
extensive areas. They may become deep at the same time, for as the outer
Page 440
border of the shallow-water zone is shifted seaward by aggradation, the
vertical space to be filled becomes greater (compare Figs. 321 and 322).
Again, if the coast be sinking, new deposits of coarse material may be made
on older ones. In this way also great thicknesses of sediment may be
accumulated, all parts of which were deposited in shallow water. The great
thickness of some of the conglomerate beds of the past shows how far this
process may go.
Fig. 324.—Ripple-marks.
vertical space to be filled becomes greater (compare Figs. 321 and 322).
Again, if the coast be sinking, new deposits of coarse material may be made
on older ones. In this way also great thicknesses of sediment may be
accumulated, all parts of which were deposited in shallow water. The great
thickness of some of the conglomerate beds of the past shows how far this
process may go.
Fig. 324.—Ripple-marks.
Page 441
Fig. 325.—Rill-marks resembling impressions of seaweeds. Beach at Noyes Point, R. I.
(Walcott, U. S. Geol. Surv.)
(Walcott, U. S. Geol. Surv.)
Page 442
Fig. 326.—Rill-marks. Same locality as 325. (Walcott.)
As a rule, no definite line marks the seaward terminus of the coarse
detritus, since coarse material is carried farther out when the waves run high
(and the undertow is strong) than when they are feeble. In calm weather,
therefore, fine sediment may be deposited where coarse had been laid down
in the preceding storm, only to be covered in turn by other deposits of a
different character. Thus gravel grades off into sand, with more or less
overlapping or interwedging, and sand grades off into silt in the same way.
This is diagrammatically illustrated by Fig. 323.
Characteristics of shallow-water deposits.—Clastic sediments laid
down in shallow water have several distinctive characteristics. While they
are, in the aggregate, coarse, they are characterized by frequent variations in
coarseness. The surfaces of successive beds are likely to be ripple- and rill-
marked (Figs. 324, 325, 326), and cross-bedding (Fig. 327) is of common
As a rule, no definite line marks the seaward terminus of the coarse
detritus, since coarse material is carried farther out when the waves run high
(and the undertow is strong) than when they are feeble. In calm weather,
therefore, fine sediment may be deposited where coarse had been laid down
in the preceding storm, only to be covered in turn by other deposits of a
different character. Thus gravel grades off into sand, with more or less
overlapping or interwedging, and sand grades off into silt in the same way.
This is diagrammatically illustrated by Fig. 323.
Characteristics of shallow-water deposits.—Clastic sediments laid
down in shallow water have several distinctive characteristics. While they
are, in the aggregate, coarse, they are characterized by frequent variations in
coarseness. The surfaces of successive beds are likely to be ripple- and rill-
marked (Figs. 324, 325, 326), and cross-bedding (Fig. 327) is of common
Page 443
occurrence. Clayey sediments accumulated between high and low water are
often sun-cracked (Fig. 328), and the tracks of land animals are sometimes
preserved on their surfaces. Shallow-water deposits often contain fossils of
organisms which live in waters of slight depth. These characteristics are
sufficient to differentiate sedimentary formations made in shallow water
from those made in deep water, even after they have been converted into
solid rock and after the rock has emerged from the sea. Many of these
characteristics are, however, shared by deposits made by streams on the
land. Subaërial and lacustrine sediments are usually distinguishable from
those made in the sea by their fossils, and sometimes by their distribution.
Fig. 327.—Cross-bedding. (Gilbert.)
Fig. 328.—Sun-cracks. These cracks were on the mud-flats of the Missouri a few miles
above Kansas City, but the sun-cracks on shore-deposits are not essentially different.
(Calvin.)
Topography of shallow-water deposits.—The shallow-water deposits
have, on the whole, a rather plane surface, though there are some notable
departures from flatness. The steep slopes of the delta fronts and of wave-
built terraces have already been spoken of. Barriers often shut in
depressions, and the disposition of the material deposited is sometimes
often sun-cracked (Fig. 328), and the tracks of land animals are sometimes
preserved on their surfaces. Shallow-water deposits often contain fossils of
organisms which live in waters of slight depth. These characteristics are
sufficient to differentiate sedimentary formations made in shallow water
from those made in deep water, even after they have been converted into
solid rock and after the rock has emerged from the sea. Many of these
characteristics are, however, shared by deposits made by streams on the
land. Subaërial and lacustrine sediments are usually distinguishable from
those made in the sea by their fossils, and sometimes by their distribution.
Fig. 327.—Cross-bedding. (Gilbert.)
Fig. 328.—Sun-cracks. These cracks were on the mud-flats of the Missouri a few miles
above Kansas City, but the sun-cracks on shore-deposits are not essentially different.
(Calvin.)
Topography of shallow-water deposits.—The shallow-water deposits
have, on the whole, a rather plane surface, though there are some notable
departures from flatness. The steep slopes of the delta fronts and of wave-
built terraces have already been spoken of. Barriers often shut in
depressions, and the disposition of the material deposited is sometimes
Page 444
uneven, owing to shore and tidal currents. The result is that the surface of
the shallow-water deposits is often affected by low elevations and by
shallow depressions. The elevations and depressions may be elongate,
circular, or irregular in form. These general facts are shown in Figs. 319,
320, and 329. This topography is sometimes preserved on newly emerged
lands, as at various points on the Coastal Plain of the United States.
Fig. 329.—Irregularities of topography of shallow-water deposits. The depths of the water
are shown in fathoms. (Chart of C. and G. Surv.)
Chemical and organic deposits.—There is no sharp line of distinction
between the deposits usually classed as chemical and those regarded as
organic. The latter are chemical in the broader sense of the term, but as they
are immediately associated with life and are dependent upon it, it is a matter
the shallow-water deposits is often affected by low elevations and by
shallow depressions. The elevations and depressions may be elongate,
circular, or irregular in form. These general facts are shown in Figs. 319,
320, and 329. This topography is sometimes preserved on newly emerged
lands, as at various points on the Coastal Plain of the United States.
Fig. 329.—Irregularities of topography of shallow-water deposits. The depths of the water
are shown in fathoms. (Chart of C. and G. Surv.)
Chemical and organic deposits.—There is no sharp line of distinction
between the deposits usually classed as chemical and those regarded as
organic. The latter are chemical in the broader sense of the term, but as they
are immediately associated with life and are dependent upon it, it is a matter
Page 445
of practical convenience to separate them. Aside from the organic deposits,
the chemical deposits made in shallow sea-water embrace (1) those due to
reactions between constituents so brought together that new and insoluble
compounds are formed and precipitated, and (2) those due to evaporation.
The points of saturation for the various substances dissolved in sea-water
are reached at different stages, and hence they are deposited more or less in
succession.
The chemical deposits made in the shallow water of the sea, or in shallow
bodies of water isolated from the sea, are chiefly simple precipitates
resulting from evaporation; but new combinations are sometimes made in
the process of concentration and precipitation. All substances in solution are
necessarily precipitated on complete evaporation, but since the sea-water is
in general far from saturation, so far as all its leading salts are concerned,
only a few are thrown down in quantity sufficient to have geological
importance where evaporation is incomplete. The leading deposits are lime
carbonate (CaCO3), lime sulphate (gypsum, CaSO4,2H2O), common salt
(rock-salt, NaCl), and the magnesium salts, usually the chlorides and
sulphates, which are later changed to carbonates. In investigations on
Mediterranean water[174] which had an initial density of 1.02, no deposit
took place until concentration by evaporation had brought the water to a
specific gravity of 1.05. Between this density and that of 1.13, lime
carbonate and some iron oxide were deposited. Between 1.13 and 1.22, lime
sulphate was the most abundant precipitate, while between 1.22 and 1.31,
95% of the deposit was common salt. With still further concentration, the
remaining substances in solution, especially the magnesium salts, were
thrown down.
While there is somewhat more than ten times as much lime sulphate as
lime carbonate in the ocean (p. 324), the deposits of the carbonate
(including the organic) have been very much greater than those of the
sulphate. This is due partly to the fact that the sulphate is much more
soluble in natural waters than the carbonate. Rivers bring much more
carbonate than sulphate to the sea, so that the point of saturation for the
sulphate would normally be reached much later than that of the carbonate.
The more important fact, however, is that marine plants and animals use
lime carbonate freely for skeletal and housing purposes. It is held by some
that they get their lime from the sulphate, but if so they convert it into
the chemical deposits made in shallow sea-water embrace (1) those due to
reactions between constituents so brought together that new and insoluble
compounds are formed and precipitated, and (2) those due to evaporation.
The points of saturation for the various substances dissolved in sea-water
are reached at different stages, and hence they are deposited more or less in
succession.
The chemical deposits made in the shallow water of the sea, or in shallow
bodies of water isolated from the sea, are chiefly simple precipitates
resulting from evaporation; but new combinations are sometimes made in
the process of concentration and precipitation. All substances in solution are
necessarily precipitated on complete evaporation, but since the sea-water is
in general far from saturation, so far as all its leading salts are concerned,
only a few are thrown down in quantity sufficient to have geological
importance where evaporation is incomplete. The leading deposits are lime
carbonate (CaCO3), lime sulphate (gypsum, CaSO4,2H2O), common salt
(rock-salt, NaCl), and the magnesium salts, usually the chlorides and
sulphates, which are later changed to carbonates. In investigations on
Mediterranean water[174] which had an initial density of 1.02, no deposit
took place until concentration by evaporation had brought the water to a
specific gravity of 1.05. Between this density and that of 1.13, lime
carbonate and some iron oxide were deposited. Between 1.13 and 1.22, lime
sulphate was the most abundant precipitate, while between 1.22 and 1.31,
95% of the deposit was common salt. With still further concentration, the
remaining substances in solution, especially the magnesium salts, were
thrown down.
While there is somewhat more than ten times as much lime sulphate as
lime carbonate in the ocean (p. 324), the deposits of the carbonate
(including the organic) have been very much greater than those of the
sulphate. This is due partly to the fact that the sulphate is much more
soluble in natural waters than the carbonate. Rivers bring much more
carbonate than sulphate to the sea, so that the point of saturation for the
sulphate would normally be reached much later than that of the carbonate.
The more important fact, however, is that marine plants and animals use
lime carbonate freely for skeletal and housing purposes. It is held by some
that they get their lime from the sulphate, but if so they convert it into
Page 446
carbonate before it takes the form of shells, coral, etc., the sulphuric acid set
free in the process reproducing, directly or indirectly, more sulphate. The
secretion of lime carbonate by organisms is not dependent on the saturation
of the water, but may be carried on when the amount in solution is very
small.
There can be little doubt that the chief deposits of lime carbonate have
been and are being made through the agency of plants and animals in the
form of shells, coral, bones, teeth, and other devices for supporting,
stiffening, housing, protecting, and arming themselves; but while it is
agreed that the larger part of the lime carbonate deposited in the open sea is
of organic origin, it is equally clear that in closed seas subject to
concentration from evaporation, simple precipitation takes place freely.
There is some difference of opinion as to the importance of these two
classes of deposits, past and present. The debated point is whether simple
precipitation takes place in any appreciable degree under the usual oceanic
conditions. There is much more evidence of solution by sea-water than of
precipitation from it. The ocean appears to be under-saturated with lime
carbonate on the whole, though it is still possible that deposition may take
place in favorable situations, as, for example, where the very calcareous
waters of rivers are spread out in thin sheets on the surface of the heavier
salt water, and thus exposed to exceptional evaporation, or where there is
very exceptional agitation and aëration.[175]
Gypsum appears to be deposited in quantity only in the closed basins of
arid regions where concentration reaches an advanced state.
Since normal sea-water is far from saturation with common salt, the latter
is precipitated only in lagoons, closed seas, or other situations favorable to
great concentration. This is usually achieved only in notably arid regions,
and in basins that receive little or no drainage from the land.
Deposits of salt usually, therefore, signify highly arid conditions, and
where they occur over wide ranges in latitude and longitude, as in certain
periods of the past, unusual aridity is inferred. Where confined to limited
areas, their climatic significance is less, for topographic conditions may
determine local aridity. The total area where salt is now being precipitated
is small, though on the whole the present is probably to be regarded as a
rather arid period of the earth’s history. On the other hand, ancient deposits
free in the process reproducing, directly or indirectly, more sulphate. The
secretion of lime carbonate by organisms is not dependent on the saturation
of the water, but may be carried on when the amount in solution is very
small.
There can be little doubt that the chief deposits of lime carbonate have
been and are being made through the agency of plants and animals in the
form of shells, coral, bones, teeth, and other devices for supporting,
stiffening, housing, protecting, and arming themselves; but while it is
agreed that the larger part of the lime carbonate deposited in the open sea is
of organic origin, it is equally clear that in closed seas subject to
concentration from evaporation, simple precipitation takes place freely.
There is some difference of opinion as to the importance of these two
classes of deposits, past and present. The debated point is whether simple
precipitation takes place in any appreciable degree under the usual oceanic
conditions. There is much more evidence of solution by sea-water than of
precipitation from it. The ocean appears to be under-saturated with lime
carbonate on the whole, though it is still possible that deposition may take
place in favorable situations, as, for example, where the very calcareous
waters of rivers are spread out in thin sheets on the surface of the heavier
salt water, and thus exposed to exceptional evaporation, or where there is
very exceptional agitation and aëration.[175]
Gypsum appears to be deposited in quantity only in the closed basins of
arid regions where concentration reaches an advanced state.
Since normal sea-water is far from saturation with common salt, the latter
is precipitated only in lagoons, closed seas, or other situations favorable to
great concentration. This is usually achieved only in notably arid regions,
and in basins that receive little or no drainage from the land.
Deposits of salt usually, therefore, signify highly arid conditions, and
where they occur over wide ranges in latitude and longitude, as in certain
periods of the past, unusual aridity is inferred. Where confined to limited
areas, their climatic significance is less, for topographic conditions may
determine local aridity. The total area where salt is now being precipitated
is small, though on the whole the present is probably to be regarded as a
rather arid period of the earth’s history. On the other hand, ancient deposits
Page 447
of salt preserved in the sedimentary strata show that the area of salt
deposition has been much more considerable than now at one time and
another in the earth’s history. The salt and gypsum deposits of the past
seem, therefore, to tell an interesting tale of the climates of the past.
The magnesium salts are among the last to be thrown down as the sea-
water is evaporated, and they most commonly take the form of sulphates
and chlorides. They often form double salts with potassium, a relatively
small and soluble constituent of sea-water. In the artificial evaporation of
salt water to obtain common salt, the process is usually stopped before the
saturation-point for the magnesium salts is reached, and the residue, the
“mother-liquor,” or “bittern,” is drawn off to prevent these “bitter” salts
from mixing with the common salt. The magnesium salts are among the last
to be precipitated, not only because they are readily soluble, but because
their quantity is small; yet in the original rock from which all the sea-salts
came, there is at least as much magnesium as sodium, while in the sea there
is about five times as much sodium as magnesium. Just what becomes of
the remaining magnesium is not yet well understood. It has a notable
disposition to form double salts with some other constituent, as noted
above. In the earlier marine strata, dolomite, that is, limestone composed
partly or wholly of the double carbonate of lime and magnesia, (CaMg)CO3,
abounds. This appears to have been formed by a gradual substitution of
molecules of magnesium for those of calcium, but just how and when and
why it was done has not been fully worked out. It appears to be a case
where the saline matter of the sea made its contribution to the sedimentary
deposits by chemical reaction upon them, rather than by precipitation
because of saturation.
The relatively small amount of potash in the sea-water is probably due to
its disposition to remain united with the clays and earths of the mantle rock
and of the shaley deposits.
To some extent the salts in solution act directly on the earthy matter
brought down into the sea by rivers, but where sedimentation is rapid, as it
often is in shallow water, this action is limited and obscure. In the main, the
ocean-waters protect the sediments from weathering and similar changes,
except as organic matter buried with them induces change.
deposition has been much more considerable than now at one time and
another in the earth’s history. The salt and gypsum deposits of the past
seem, therefore, to tell an interesting tale of the climates of the past.
The magnesium salts are among the last to be thrown down as the sea-
water is evaporated, and they most commonly take the form of sulphates
and chlorides. They often form double salts with potassium, a relatively
small and soluble constituent of sea-water. In the artificial evaporation of
salt water to obtain common salt, the process is usually stopped before the
saturation-point for the magnesium salts is reached, and the residue, the
“mother-liquor,” or “bittern,” is drawn off to prevent these “bitter” salts
from mixing with the common salt. The magnesium salts are among the last
to be precipitated, not only because they are readily soluble, but because
their quantity is small; yet in the original rock from which all the sea-salts
came, there is at least as much magnesium as sodium, while in the sea there
is about five times as much sodium as magnesium. Just what becomes of
the remaining magnesium is not yet well understood. It has a notable
disposition to form double salts with some other constituent, as noted
above. In the earlier marine strata, dolomite, that is, limestone composed
partly or wholly of the double carbonate of lime and magnesia, (CaMg)CO3,
abounds. This appears to have been formed by a gradual substitution of
molecules of magnesium for those of calcium, but just how and when and
why it was done has not been fully worked out. It appears to be a case
where the saline matter of the sea made its contribution to the sedimentary
deposits by chemical reaction upon them, rather than by precipitation
because of saturation.
The relatively small amount of potash in the sea-water is probably due to
its disposition to remain united with the clays and earths of the mantle rock
and of the shaley deposits.
To some extent the salts in solution act directly on the earthy matter
brought down into the sea by rivers, but where sedimentation is rapid, as it
often is in shallow water, this action is limited and obscure. In the main, the
ocean-waters protect the sediments from weathering and similar changes,
except as organic matter buried with them induces change.
Page 448
While the lime deposits are by far the greatest of the chemical and
organic deposits of the sea, plants and animals also secrete notable
quantities of silica. Silica deposits of organic origin are relatively much
more important in the deep sea than in shallow water, and will be
mentioned in that connection.
Limestone.—Something concerning the origin of limestone has already
been given in the preceding paragraphs, but because of the importance of
this formation, it may be added by way of summary that shallow seas free,
or nearly free, from terrigenous sediment, and abounding in lime-secreting
life, furnish the conditions for nearly pure deposits of limestone, and that
most of the limestone within the areas of the present continents appears to
have originated under such conditions. The common notion that limestone
is normally a deep-water formation is a serious error. Although limestones
are formed in deep as well as in shallow waters, by far the more important
classes of lime-secreting organisms are photobathic, i.e. are limited to the
depths to which light penetrates. In the shallow waters, these plants and
animals are in part free and in part attached. Within the areas of deep water
they are free and at the surface, and their remains drop to the bottom, if not
sooner dissolved. But few forms live on the deep, dark, cold bottoms of
abysmal depths. Clear waters, free from abundant terrigenous sediments
and abounding in lime-secreting life, rather than deep waters, are, therefore,
the most favorable conditions for the origin of limestone.
The purely chemical deposits of limestone are probably all of shallow-
water origin. Once made, they are subject to solution, redeposition, and
other mutations like other deposits. As a result, they often lose many of
their original characteristics, but enough usually remain to tell the story of
their origin.
Deep-sea Deposits.
Contrasted with shallow-water deposits.—The deep-sea deposits cover
the ocean-bottom below the 100-fathom line. Their area is considerably
more than half the earth’s surface. The characteristic deposits are muds,
organic oozes, and clays, which in their physical characteristics are
remarkably uniform. In regions of floating ice, greater diversity is
introduced from the varied nature of the materials which the ice transports,
but gravels and sands, comparable to those of shallow water, are rarely
organic deposits of the sea, plants and animals also secrete notable
quantities of silica. Silica deposits of organic origin are relatively much
more important in the deep sea than in shallow water, and will be
mentioned in that connection.
Limestone.—Something concerning the origin of limestone has already
been given in the preceding paragraphs, but because of the importance of
this formation, it may be added by way of summary that shallow seas free,
or nearly free, from terrigenous sediment, and abounding in lime-secreting
life, furnish the conditions for nearly pure deposits of limestone, and that
most of the limestone within the areas of the present continents appears to
have originated under such conditions. The common notion that limestone
is normally a deep-water formation is a serious error. Although limestones
are formed in deep as well as in shallow waters, by far the more important
classes of lime-secreting organisms are photobathic, i.e. are limited to the
depths to which light penetrates. In the shallow waters, these plants and
animals are in part free and in part attached. Within the areas of deep water
they are free and at the surface, and their remains drop to the bottom, if not
sooner dissolved. But few forms live on the deep, dark, cold bottoms of
abysmal depths. Clear waters, free from abundant terrigenous sediments
and abounding in lime-secreting life, rather than deep waters, are, therefore,
the most favorable conditions for the origin of limestone.
The purely chemical deposits of limestone are probably all of shallow-
water origin. Once made, they are subject to solution, redeposition, and
other mutations like other deposits. As a result, they often lose many of
their original characteristics, but enough usually remain to tell the story of
their origin.
Deep-sea Deposits.
Contrasted with shallow-water deposits.—The deep-sea deposits cover
the ocean-bottom below the 100-fathom line. Their area is considerably
more than half the earth’s surface. The characteristic deposits are muds,
organic oozes, and clays, which in their physical characteristics are
remarkably uniform. In regions of floating ice, greater diversity is
introduced from the varied nature of the materials which the ice transports,
but gravels and sands, comparable to those of shallow water, are rarely
Page 449
found. “Tides, currents, and waves produce some mechanical effects at the
upper limits of the deep-sea region, but on the whole there is an absence of
the phenomena of erosion, and mechanical action would appear to be absent
except in the case of submarine eruptions. The depth is too great for
sunlight to penetrate, and vegetable life is limited to the upper zone. Animal
life is present in the same zone and on the bottom, but absent or nearly so in
the middle depths. The temperature (at the bottom) is below 40° Fahr.
throughout the larger part of the area, and if subject to variation with
latitude or change of season, these changes affect only the depths
immediately beyond the 100-fathom line. Throughout the whole region
there is a very uniform set of conditions. In the shallow-water and littoral
zones, owing to the rapid accumulation and the mechanical effects of
transportation and erosion, the effects of chemical modification are not very
apparent in the deposits; but in deep-sea deposits, in consequence of the less
rapid rate of accumulation, absence of transport, the nature and small size
of the particles, many evident chemical reactions have taken place, resulting
in the formation in situ of glauconite, phosphatic and manganese nodules,
zeolites, and other secondary products.”[176] With increasing depth and
distance from the shore, the character of the deposits undergoes a change.
There is less and less material derived directly from the land, and more
“amorphous matter arising from the ultimate decomposition of minerals and
rocks, and accompanied, in all moderate depths, by an increase [relative] of
the remains of pelagic organisms. We thus pass insensibly from those deep-
sea deposits of a terrestrial origin, which we call ‘terrigenous,’ to those
deep-sea deposits denominated ‘pelagic,’ in which the remains of
calcareous and siliceous organisms, clays and other substances of secondary
origin play the principal rôle.”[176]
The following table[177] shows the relations of the various groups of
marine deposits.
1. Deep-sea deposits beyond Red clay
100 fathoms Radiolarian ooze
Diatom ooze I. Pelagic deposits formed in deep
Globigerina water removed from land.
ooze
Pteropod ooze
Blue mud II. Terrigenous deposits formed in
deep and shallow water, mostly
Red mud close to land.
upper limits of the deep-sea region, but on the whole there is an absence of
the phenomena of erosion, and mechanical action would appear to be absent
except in the case of submarine eruptions. The depth is too great for
sunlight to penetrate, and vegetable life is limited to the upper zone. Animal
life is present in the same zone and on the bottom, but absent or nearly so in
the middle depths. The temperature (at the bottom) is below 40° Fahr.
throughout the larger part of the area, and if subject to variation with
latitude or change of season, these changes affect only the depths
immediately beyond the 100-fathom line. Throughout the whole region
there is a very uniform set of conditions. In the shallow-water and littoral
zones, owing to the rapid accumulation and the mechanical effects of
transportation and erosion, the effects of chemical modification are not very
apparent in the deposits; but in deep-sea deposits, in consequence of the less
rapid rate of accumulation, absence of transport, the nature and small size
of the particles, many evident chemical reactions have taken place, resulting
in the formation in situ of glauconite, phosphatic and manganese nodules,
zeolites, and other secondary products.”[176] With increasing depth and
distance from the shore, the character of the deposits undergoes a change.
There is less and less material derived directly from the land, and more
“amorphous matter arising from the ultimate decomposition of minerals and
rocks, and accompanied, in all moderate depths, by an increase [relative] of
the remains of pelagic organisms. We thus pass insensibly from those deep-
sea deposits of a terrestrial origin, which we call ‘terrigenous,’ to those
deep-sea deposits denominated ‘pelagic,’ in which the remains of
calcareous and siliceous organisms, clays and other substances of secondary
origin play the principal rôle.”[176]
The following table[177] shows the relations of the various groups of
marine deposits.
1. Deep-sea deposits beyond Red clay
100 fathoms Radiolarian ooze
Diatom ooze I. Pelagic deposits formed in deep
Globigerina water removed from land.
ooze
Pteropod ooze
Blue mud II. Terrigenous deposits formed in
deep and shallow water, mostly
Red mud close to land.
Page 450
Green mud
Volcanic mud
Coral mud
2. Shallow-water deposits
Sands, gravels,
between low-water mark and
muds, etc.
100 fathoms
3. Littoral deposits between Sands, gravels,
high- and low-water marks muds, etc.
Sources.—The pelagic deposits are made up in part of materials of
organic origin, and in part of materials of inorganic origin. The inorganic
materials may be of mechanical or chemical origin. Mechanical pelagic
deposits originate in various ways. They may come (1) from the land by the
ordinary processes of gradation, (2) from volcanic vents, or (3) from extra-
terrestrial sources. Chemical deposits may be formed (1) in situ by the
chemical interaction of substances in the sea-water on materials of organic
and inorganic origin, and (2) by direct precipitation from the sea-water.
Mechanical inorganic deposits.—The terrigenous materials which reach
the deep sea are, as a rule, only the finest products of land decay, and are
carried out by movements of water or by the winds. They are not commonly
recognized in the dredgings more than 200 miles from the shore, but
opposite the mouths of great rivers they extend much farther,—1000 miles
in the case of the Amazon. They are especially abundant on the slopes of
the continental shelves. Here occur the blue, green, and red muds, with
which are associated volcanic and coral muds. The color of these various
muds is dependent in part on the changes which they have undergone since
their deposition. The green muds usually contain enough glauconite to give
them their color, and are most commonly found off bold coasts where
sedimentation is not rapid. The blue muds indicate lack of oxidation, or
perhaps deoxidation. Red muds are not common, though they have been
found in some situations. In general, these deposits are analogous to certain
shales, marls, etc., found within the continents.
Though coarse materials derived from the land are occasionally found in
the deep-sea deposits, their presence must be looked upon as in some sense
accidental. Occasional pebbles, or even bowlders, are carried out into the
ocean entangled in the roots of floating trees. Within limits, too, icebergs
have carried out land débris, though it is probable that transportation by this
Volcanic mud
Coral mud
2. Shallow-water deposits
Sands, gravels,
between low-water mark and
muds, etc.
100 fathoms
3. Littoral deposits between Sands, gravels,
high- and low-water marks muds, etc.
Sources.—The pelagic deposits are made up in part of materials of
organic origin, and in part of materials of inorganic origin. The inorganic
materials may be of mechanical or chemical origin. Mechanical pelagic
deposits originate in various ways. They may come (1) from the land by the
ordinary processes of gradation, (2) from volcanic vents, or (3) from extra-
terrestrial sources. Chemical deposits may be formed (1) in situ by the
chemical interaction of substances in the sea-water on materials of organic
and inorganic origin, and (2) by direct precipitation from the sea-water.
Mechanical inorganic deposits.—The terrigenous materials which reach
the deep sea are, as a rule, only the finest products of land decay, and are
carried out by movements of water or by the winds. They are not commonly
recognized in the dredgings more than 200 miles from the shore, but
opposite the mouths of great rivers they extend much farther,—1000 miles
in the case of the Amazon. They are especially abundant on the slopes of
the continental shelves. Here occur the blue, green, and red muds, with
which are associated volcanic and coral muds. The color of these various
muds is dependent in part on the changes which they have undergone since
their deposition. The green muds usually contain enough glauconite to give
them their color, and are most commonly found off bold coasts where
sedimentation is not rapid. The blue muds indicate lack of oxidation, or
perhaps deoxidation. Red muds are not common, though they have been
found in some situations. In general, these deposits are analogous to certain
shales, marls, etc., found within the continents.
Though coarse materials derived from the land are occasionally found in
the deep-sea deposits, their presence must be looked upon as in some sense
accidental. Occasional pebbles, or even bowlders, are carried out into the
ocean entangled in the roots of floating trees. Within limits, too, icebergs
have carried out land débris, though it is probable that transportation by this
Page 451
means has been exaggerated. The amount which icebergs might carry, if
fully loaded, is far greater than the amount which they do carry.
Of the identifiable inorganic materials in the deep sea, the most abundant
are of volcanic origin, and among these the most common is pumice, which
is frequently so light that it floats readily until it becomes water-logged.
Pieces of pumice brought up by the Challenger and thoroughly dried were
found to float for months in sea-water before settling even through the
depth of water contained in the vessel in which the experiment was
performed.[178] The next most abundant substance of volcanic origin in
pelagic deposits is volcanic glass. This ranges from pieces of the size of a
walnut down to the smallest fragments, which often serve as centers for
concretions. Lapilli (cinders) and volcanic ash also are abundant in parts of
the deep sea. The distribution of these volcanic products is essentially
universal, though by no means uniform. Some of them are probably from
submarine volcanoes.
The study of the deep sea deposits has revealed the presence of many
nodules and grains which are believed to be of extra-terrestrial origin. Many
of them are magnetic.[179] The dust of countless meteors which enter the
atmosphere daily settles on land and sea alike, and enters into the sediment
of the bottom of the latter. It is probably no more abundant in deep water
than in shallow, but it is relatively more important, since other
sedimentation is more meager. The number of meteorites which enter the
atmosphere daily has been estimated at from 15,000,000 to 20,000,000.[180]
If on the average the meteorites weigh ten grains each, probably a rather
high estimate, the total amount of extra-terrestrial matter reaching the earth
yearly would be 5,000 to 7,000 tons, and something like three-fourths of
this must, on the average, fall into the sea. But even at this rate it would
take some fifty billion years to cover the sea-bottom with a layer one foot in
thickness.
Organic constituents of pelagic deposits.—With increasing distance
from shores, and especially with increasing depth of water, terrigenous
deposits become less and less abundant, and sediments derived from pelagic
life increase in relative importance. Beyond the upper part of the outer
slopes of the continental shelves, the pelagic deposits are largely made up
of shells and skeletons of marine organisms which live in the surface-
waters. Pelagic molluscs, foraminifera, and algæ secrete shells of lime
fully loaded, is far greater than the amount which they do carry.
Of the identifiable inorganic materials in the deep sea, the most abundant
are of volcanic origin, and among these the most common is pumice, which
is frequently so light that it floats readily until it becomes water-logged.
Pieces of pumice brought up by the Challenger and thoroughly dried were
found to float for months in sea-water before settling even through the
depth of water contained in the vessel in which the experiment was
performed.[178] The next most abundant substance of volcanic origin in
pelagic deposits is volcanic glass. This ranges from pieces of the size of a
walnut down to the smallest fragments, which often serve as centers for
concretions. Lapilli (cinders) and volcanic ash also are abundant in parts of
the deep sea. The distribution of these volcanic products is essentially
universal, though by no means uniform. Some of them are probably from
submarine volcanoes.
The study of the deep sea deposits has revealed the presence of many
nodules and grains which are believed to be of extra-terrestrial origin. Many
of them are magnetic.[179] The dust of countless meteors which enter the
atmosphere daily settles on land and sea alike, and enters into the sediment
of the bottom of the latter. It is probably no more abundant in deep water
than in shallow, but it is relatively more important, since other
sedimentation is more meager. The number of meteorites which enter the
atmosphere daily has been estimated at from 15,000,000 to 20,000,000.[180]
If on the average the meteorites weigh ten grains each, probably a rather
high estimate, the total amount of extra-terrestrial matter reaching the earth
yearly would be 5,000 to 7,000 tons, and something like three-fourths of
this must, on the average, fall into the sea. But even at this rate it would
take some fifty billion years to cover the sea-bottom with a layer one foot in
thickness.
Organic constituents of pelagic deposits.—With increasing distance
from shores, and especially with increasing depth of water, terrigenous
deposits become less and less abundant, and sediments derived from pelagic
life increase in relative importance. Beyond the upper part of the outer
slopes of the continental shelves, the pelagic deposits are largely made up
of shells and skeletons of marine organisms which live in the surface-
waters. Pelagic molluscs, foraminifera, and algæ secrete shells of lime
Page 452
carbonate, while diatoms and radiolarians secrete shells of silica. When the
organisms die, they sink to the bottom with their shells, and these mineral
matters of organic origin are mingled with the volcanic products which are
universal over the sea-floor. Pelagic deposits of organic origin are named
according to their characteristic constituents. Thus there are pteropod oozes,
globigerina oozes, diatom oozes, radiolarian oozes, etc.[181] It is not to be
understood that these oozes are made up exclusively of the shells which
give them their names. Diatom ooze is an ooze in which diatom shells are
abundant, not an ooze made up wholly of diatom shells; and globigerina
ooze is an ooze in which globigerina shells are abundant, though in many
cases they do not make up even the bulk of the matter. While samples of
these various oozes might be selected which are thoroughly distinct from
one another, there are all gradations between them, since pelagic life does
not recognize boundary-lines.
It is a significant fact that with increasing depth the proportion of lime
carbonate in the ooze decreases. Thus in tropical regions remote from land
where the depths are less than 600 fathoms, the carbonate of lime of the
shells of pelagic organisms may constitute 80% or 90% of the deposit. With
the same surface conditions, but with increasing depth, the percentage of
lime carbonate decreases, until at 2000 fathoms it is less than 60%; at 2400
fathoms, 30%, and at 2600 fathoms, 10%. Beyond this depth there are
usually no more than traces of carbonate of lime. The data at hand show
that the percentage of lime carbonate falls off below 2200 fathoms more
rapidly than at lesser depths.
When the percentage of lime carbonate becomes very low, the calcareous
oozes grade off into the red clay with which the sea-floor below 2400 to
2600 fathoms is covered.
Chemical deposits.—The chemical deposits of the deep sea are chiefly
the alteration products of sediments which reach the sea-bottom by
mechanical means. All sediment deposited in the sea undergoes more or less
chemical change, but it is only when the change is very considerable that
the product is referred to this class. Where sedimentation is rapid and the
sediment coarse, the chemical change is relatively slight; but where the
sedimentation is slow and the sediment fine, the chemical change is
relatively great; for the longer exposure to the sea-water and the greater
proportion of surface exposed to attack, both favor change. Both the area
organisms die, they sink to the bottom with their shells, and these mineral
matters of organic origin are mingled with the volcanic products which are
universal over the sea-floor. Pelagic deposits of organic origin are named
according to their characteristic constituents. Thus there are pteropod oozes,
globigerina oozes, diatom oozes, radiolarian oozes, etc.[181] It is not to be
understood that these oozes are made up exclusively of the shells which
give them their names. Diatom ooze is an ooze in which diatom shells are
abundant, not an ooze made up wholly of diatom shells; and globigerina
ooze is an ooze in which globigerina shells are abundant, though in many
cases they do not make up even the bulk of the matter. While samples of
these various oozes might be selected which are thoroughly distinct from
one another, there are all gradations between them, since pelagic life does
not recognize boundary-lines.
It is a significant fact that with increasing depth the proportion of lime
carbonate in the ooze decreases. Thus in tropical regions remote from land
where the depths are less than 600 fathoms, the carbonate of lime of the
shells of pelagic organisms may constitute 80% or 90% of the deposit. With
the same surface conditions, but with increasing depth, the percentage of
lime carbonate decreases, until at 2000 fathoms it is less than 60%; at 2400
fathoms, 30%, and at 2600 fathoms, 10%. Beyond this depth there are
usually no more than traces of carbonate of lime. The data at hand show
that the percentage of lime carbonate falls off below 2200 fathoms more
rapidly than at lesser depths.
When the percentage of lime carbonate becomes very low, the calcareous
oozes grade off into the red clay with which the sea-floor below 2400 to
2600 fathoms is covered.
Chemical deposits.—The chemical deposits of the deep sea are chiefly
the alteration products of sediments which reach the sea-bottom by
mechanical means. All sediment deposited in the sea undergoes more or less
chemical change, but it is only when the change is very considerable that
the product is referred to this class. Where sedimentation is rapid and the
sediment coarse, the chemical change is relatively slight; but where the
sedimentation is slow and the sediment fine, the chemical change is
relatively great; for the longer exposure to the sea-water and the greater
proportion of surface exposed to attack, both favor change. Both the area
Page 453
and the mass of sea-bottom sediment radically changed in this way are
large, but most of the deposit does not correspond to any formation known
on the land.
The red clay already referred to belongs to this class of deposits. Its
origin has been the subject of much discussion. It contains much volcanic
débris, various concretions, bones of mammals, zeolitic crystals, and extra-
terrestrial spherules, and doubtless the insoluble products of the shells of
pelagic life; but it is still a mooted question how far the clay itself is the
product of decomposed shells, and how far the altered product of pulverized
pumice, volcanic ash, dust, etc. Pelagic life does not seem to be less
abundant at the surface where the water is deep than where it is shallow,
and it would appear that the shells must sink in such situations as
elsewhere. If the lime carbonate of globigerina ooze be removed by dilute
acid, the inorganic residue is similar to the red clay in the ocean-bottom.
This suggests that owing to the more complete solution in the very deep
water, the lime carbonate of the shells has been dissolved, leaving the red
clay as a residuum. The more complete solution at the bottom might be the
result either of the greater pressure, or of a greater percentage of CO2 in the
water due to emanations from the sea-floor, or to both; but the suddenness
of the transition from oozes to red clay, with increasing depth, does not
seem to be fully explained by these assumptions. The study of the dredgings
has inclined the students of these materials to the conclusion that volcanic
materials, rather than shells, are the principal source of the red clay.[182] The
volcanic materials are thought to have accumulated slowly and to have been
long exposed to the action of sea-water. The various nodules and crystals in
the clay are believed to be secondary products, the materials for which were
derived from the decomposition of the same materials. Eolian dust may be a
notable constituent of the red clay.
Various specific products of chemical change may be briefly referred to.
The decomposition of certain mineral particles, such as feldspar, gives rise
to kaolin, and kaolin is a very considerable constituent of most of the clayey
deposits of the ocean-bottom. The kaolinization of feldspar may take place
both on land and in the sea. Manganiferous deposits are widespread in the
ocean-bottom, occurring both as coatings on grains of mechanical
sediments, shells, etc., and as concretions ranging in sizes from minute
particles to nodules an inch or more in diameter. The concretions are
large, but most of the deposit does not correspond to any formation known
on the land.
The red clay already referred to belongs to this class of deposits. Its
origin has been the subject of much discussion. It contains much volcanic
débris, various concretions, bones of mammals, zeolitic crystals, and extra-
terrestrial spherules, and doubtless the insoluble products of the shells of
pelagic life; but it is still a mooted question how far the clay itself is the
product of decomposed shells, and how far the altered product of pulverized
pumice, volcanic ash, dust, etc. Pelagic life does not seem to be less
abundant at the surface where the water is deep than where it is shallow,
and it would appear that the shells must sink in such situations as
elsewhere. If the lime carbonate of globigerina ooze be removed by dilute
acid, the inorganic residue is similar to the red clay in the ocean-bottom.
This suggests that owing to the more complete solution in the very deep
water, the lime carbonate of the shells has been dissolved, leaving the red
clay as a residuum. The more complete solution at the bottom might be the
result either of the greater pressure, or of a greater percentage of CO2 in the
water due to emanations from the sea-floor, or to both; but the suddenness
of the transition from oozes to red clay, with increasing depth, does not
seem to be fully explained by these assumptions. The study of the dredgings
has inclined the students of these materials to the conclusion that volcanic
materials, rather than shells, are the principal source of the red clay.[182] The
volcanic materials are thought to have accumulated slowly and to have been
long exposed to the action of sea-water. The various nodules and crystals in
the clay are believed to be secondary products, the materials for which were
derived from the decomposition of the same materials. Eolian dust may be a
notable constituent of the red clay.
Various specific products of chemical change may be briefly referred to.
The decomposition of certain mineral particles, such as feldspar, gives rise
to kaolin, and kaolin is a very considerable constituent of most of the clayey
deposits of the ocean-bottom. The kaolinization of feldspar may take place
both on land and in the sea. Manganiferous deposits are widespread in the
ocean-bottom, occurring both as coatings on grains of mechanical
sediments, shells, etc., and as concretions ranging in sizes from minute
particles to nodules an inch or more in diameter. The concretions are
Page 454
sometimes approximately spheroidal, but often botryoidal. These
manganiferous nodules are believed to have arisen from the decay of
fragments of volcanic rocks. In their decay, the manganese and iron are
believed to have been first changed to carbonates, and subsequently to
oxides. After manganese oxide, iron oxide and silica are by far the most
abundant constituents, but many other substances enter into their
composition in minor quantities.
Another substance somewhat widely distributed in the sea-bed, though
by no means universal, is glauconite, a complex silicate of alumina, iron,
potassium, etc. Glauconite is, on the whole, most abundant along the edges
of the continental shelves, though it is by no means universal in this
position. It is not commonly found in deep water, nor very near the shore,
but approximately at the “mud-line.” The glauconite grains begin to form,
as a rule, in tiny shells, chiefly the shells of foraminifera. After filling the
shell, the shell itself may disappear, while the glauconite goes on
accumulating around the core already formed, until the grain attains
considerable size. Glauconite is believed to be an alteration product of
certain sorts of mechanical sediment, the change being effected under the
influence of the decaying organic matter in the shells.[183] It does not occur
where sedimentation is rapid, and its formation appears to be favored by
considerable changes of temperature. Glauconite deposits occur on the land
and are commonly known as green sand marl. Glauconite also occurs
sparingly in many other sedimentary rocks.
manganiferous nodules are believed to have arisen from the decay of
fragments of volcanic rocks. In their decay, the manganese and iron are
believed to have been first changed to carbonates, and subsequently to
oxides. After manganese oxide, iron oxide and silica are by far the most
abundant constituents, but many other substances enter into their
composition in minor quantities.
Another substance somewhat widely distributed in the sea-bed, though
by no means universal, is glauconite, a complex silicate of alumina, iron,
potassium, etc. Glauconite is, on the whole, most abundant along the edges
of the continental shelves, though it is by no means universal in this
position. It is not commonly found in deep water, nor very near the shore,
but approximately at the “mud-line.” The glauconite grains begin to form,
as a rule, in tiny shells, chiefly the shells of foraminifera. After filling the
shell, the shell itself may disappear, while the glauconite goes on
accumulating around the core already formed, until the grain attains
considerable size. Glauconite is believed to be an alteration product of
certain sorts of mechanical sediment, the change being effected under the
influence of the decaying organic matter in the shells.[183] It does not occur
where sedimentation is rapid, and its formation appears to be favored by
considerable changes of temperature. Glauconite deposits occur on the land
and are commonly known as green sand marl. Glauconite also occurs
sparingly in many other sedimentary rocks.
Page 455
Fig. 330.—Distribution of various sorts of deep-sea deposits. (Murray. Challenger Reports.)
Another substance which is somewhat widespread in the ocean-bottom is
phosphate of lime, which occurs in various sorts of oozes, in the
manganiferous nodules, in glauconite, and in independent nodules. Like the
grains of glauconite, the grains of phosphate of lime appear to have started
as concretions in shells, and to be the result of the reaction of organic matter
on the contents of sea-water. The immediate source of the lime phosphate in
the water appears to have been the shells or bones of the numerous animals
living in the sea.
Secondary minerals made from the constituents of volcanic matter which
has been decomposed occur not uncommonly in the bottom of the sea.
These minerals belong to the general class of zeolites, phillipsite being the
most abundant. Their distribution is somewhat wide, but their quantity is
slight.
Unfortunately, knowledge of the deep-sea deposits is limited to their
superficial layers. Soundings do not usually penetrate more than a few
inches, or at most a foot or two.
Unlike shallow-water deposits, those of the really deep sea seem to find
no correlatives in the known rock formations of the land.
Another substance which is somewhat widespread in the ocean-bottom is
phosphate of lime, which occurs in various sorts of oozes, in the
manganiferous nodules, in glauconite, and in independent nodules. Like the
grains of glauconite, the grains of phosphate of lime appear to have started
as concretions in shells, and to be the result of the reaction of organic matter
on the contents of sea-water. The immediate source of the lime phosphate in
the water appears to have been the shells or bones of the numerous animals
living in the sea.
Secondary minerals made from the constituents of volcanic matter which
has been decomposed occur not uncommonly in the bottom of the sea.
These minerals belong to the general class of zeolites, phillipsite being the
most abundant. Their distribution is somewhat wide, but their quantity is
slight.
Unfortunately, knowledge of the deep-sea deposits is limited to their
superficial layers. Soundings do not usually penetrate more than a few
inches, or at most a foot or two.
Unlike shallow-water deposits, those of the really deep sea seem to find
no correlatives in the known rock formations of the land.
Page 456
LAKES.
Most of the phenomena of the ocean are repeated on a smaller scale in
lakes. The waves of lakes and their attendant undertows and littoral currents
are governed by the same laws and do the same sort of work as the
corresponding movements of the ocean. Tides are absent, or insignificant,
but slight changes of level, known as seiches,[184] have been observed in
many lakes. They are probably caused by sudden changes in atmospheric
pressure. While they are generally very slight, they frequently amount to as
much as a foot, and occasionally to several feet. The seiches are oscillatory
movements, and their period is influenced by the length and depth of the
lake. They have been studied most carefully in Switzerland. Currents
corresponding to those of the ocean are slight or wanting in lakes, but since
most lakes have inlets and outlets, their waters are in constant movement
toward the latter. In most cases this movement is too slow to be readily
noted, or to do effective work either in corrasion or transportation. The
work of the ice, on the other hand, is relatively more important in lakes than
in the sea.
Changes taking place in lakes.—The processes in operation in lakes are
easily observed and readily understood. (1) The waves wear the shores, and
the material thus derived is transported, assorted, and deposited as in the
sea, and all the topographic forms resulting from erosion or deposition
along the seacoast are reproduced on their appropriate scale in lakes. (2)
Streams bear their burden of gravel, sand, and mud into lakes and leave it
there. (3) The winds blow dust and sand into the lakes, and in some places
pile the sand up into dunes along the shores. (4) Animals of various sorts
live in the lakes, and their shells and bones give rise to deposits comparable
to the animal deposits in the sea. (5) Abundant plants grow in the shallow
water about the borders of many ponds and lakes, and as they die, their
substance accumulates on the bottom. (6) At the outlet the water is
constantly lowering its channel. The lowering of the outlet is often slow,
especially if the rock be coherent, for the outflowing water is usually clear,
and therefore inefficient in corrasive work. These six processes are
essentially universal, and all conspire against the perpetuity of the lakes. (7)
In lakes where the temperature is low enough for ice to be formed, it
crowds on the shores and develops phenomena peculiar to itself. The ice of
Most of the phenomena of the ocean are repeated on a smaller scale in
lakes. The waves of lakes and their attendant undertows and littoral currents
are governed by the same laws and do the same sort of work as the
corresponding movements of the ocean. Tides are absent, or insignificant,
but slight changes of level, known as seiches,[184] have been observed in
many lakes. They are probably caused by sudden changes in atmospheric
pressure. While they are generally very slight, they frequently amount to as
much as a foot, and occasionally to several feet. The seiches are oscillatory
movements, and their period is influenced by the length and depth of the
lake. They have been studied most carefully in Switzerland. Currents
corresponding to those of the ocean are slight or wanting in lakes, but since
most lakes have inlets and outlets, their waters are in constant movement
toward the latter. In most cases this movement is too slow to be readily
noted, or to do effective work either in corrasion or transportation. The
work of the ice, on the other hand, is relatively more important in lakes than
in the sea.
Changes taking place in lakes.—The processes in operation in lakes are
easily observed and readily understood. (1) The waves wear the shores, and
the material thus derived is transported, assorted, and deposited as in the
sea, and all the topographic forms resulting from erosion or deposition
along the seacoast are reproduced on their appropriate scale in lakes. (2)
Streams bear their burden of gravel, sand, and mud into lakes and leave it
there. (3) The winds blow dust and sand into the lakes, and in some places
pile the sand up into dunes along the shores. (4) Animals of various sorts
live in the lakes, and their shells and bones give rise to deposits comparable
to the animal deposits in the sea. (5) Abundant plants grow in the shallow
water about the borders of many ponds and lakes, and as they die, their
substance accumulates on the bottom. (6) At the outlet the water is
constantly lowering its channel. The lowering of the outlet is often slow,
especially if the rock be coherent, for the outflowing water is usually clear,
and therefore inefficient in corrasive work. These six processes are
essentially universal, and all conspire against the perpetuity of the lakes. (7)
In lakes where the temperature is low enough for ice to be formed, it
crowds on the shores and develops phenomena peculiar to itself. The ice of
Page 457
the sea may work in similar ways, but its work is restricted to high latitudes.
(8) In lakes in arid regions, deposits are often made by precipitation from
solution. The first five and the last of these processes are filling the basins
of the lakes. As the sediment is deposited, a corresponding volume of water
is displaced, and, if there be outlets, forced out of the basins; the sixth
process is equally antagonistic to the lakes, while the seventh has little
influence on their permanence. Given time enough, these processes must
bring the history of any lake to an end. The lowering of the outlet will alone
accomplish this result if the bottom of the basin is above base-level. Many
lakes have already become extinct, either through the filling or draining of
their basins, or through both combined. The antagonism of rivers and lakes
long ago led to the epigram “Rivers are the mortal enemies of lakes.” True
as this statement is, it does not follow that lakes will ever cease to exist, for
the causes which produce new lakes may be in operation
contemporaneously with those which bring lakes now in existence to an
end.
Lacustrine deposits.—The beds of sediment deposited in lakes are
similar in kind, in structure, and in disposition to beds of sediment laid
down in the sea, but river-borne sediment is more commonly concentrated
into deltas, since waves and shore-currents are less effective. Even the
limestone of the sea has its correlative in some lakes. Some of it was made
of the shells of fresh-water animals which throve where the inwash of
terrigenous sediment was slight, some of it from the calcareous secretions
of plants,[185] and some of it was precipitated from solution.[186] Salt and
iron-ore[187] deposits are also sometimes made in lakes.
Extinct lakes.—The former existence of lakes where none now exist
may be known in various ways. If the lake basin was filled, its former area
is a flat, the beds of which bear evidence, in their composition, their
structure, and often in their fossil contents, of their origin in standing water.
Such a flat is commonly so situated topographically that the basin would be
reproduced if the lacustrine deposits were removed. To this general rule
there might be exceptions, as where a glacier formed one side of the basin
when it was filled. If the lake was destroyed by the reduction of its outlet, or
by the removal of some other barrier, such as glacier ice, or by desiccation,
shore phenomena, such as beaches, spits, etc., may be found. In time such
(8) In lakes in arid regions, deposits are often made by precipitation from
solution. The first five and the last of these processes are filling the basins
of the lakes. As the sediment is deposited, a corresponding volume of water
is displaced, and, if there be outlets, forced out of the basins; the sixth
process is equally antagonistic to the lakes, while the seventh has little
influence on their permanence. Given time enough, these processes must
bring the history of any lake to an end. The lowering of the outlet will alone
accomplish this result if the bottom of the basin is above base-level. Many
lakes have already become extinct, either through the filling or draining of
their basins, or through both combined. The antagonism of rivers and lakes
long ago led to the epigram “Rivers are the mortal enemies of lakes.” True
as this statement is, it does not follow that lakes will ever cease to exist, for
the causes which produce new lakes may be in operation
contemporaneously with those which bring lakes now in existence to an
end.
Lacustrine deposits.—The beds of sediment deposited in lakes are
similar in kind, in structure, and in disposition to beds of sediment laid
down in the sea, but river-borne sediment is more commonly concentrated
into deltas, since waves and shore-currents are less effective. Even the
limestone of the sea has its correlative in some lakes. Some of it was made
of the shells of fresh-water animals which throve where the inwash of
terrigenous sediment was slight, some of it from the calcareous secretions
of plants,[185] and some of it was precipitated from solution.[186] Salt and
iron-ore[187] deposits are also sometimes made in lakes.
Extinct lakes.—The former existence of lakes where none now exist
may be known in various ways. If the lake basin was filled, its former area
is a flat, the beds of which bear evidence, in their composition, their
structure, and often in their fossil contents, of their origin in standing water.
Such a flat is commonly so situated topographically that the basin would be
reproduced if the lacustrine deposits were removed. To this general rule
there might be exceptions, as where a glacier formed one side of the basin
when it was filled. If the lake was destroyed by the reduction of its outlet, or
by the removal of some other barrier, such as glacier ice, or by desiccation,
shore phenomena, such as beaches, spits, etc., may be found. In time such
Page 458
evidences are destroyed by subaërial erosion, so that they are most distinct
soon after the lake becomes extinct.
Many lakes, some of them large[188] and many of them small, are known
to have become extinct, while many others are now in their last stages,
namely, marshes. Many others have been greatly reduced in size. Such
reductions are often obvious where deltas are built into lakes. Thus the delta
built by the Rhone into Lake Geneva is several miles in length, and has
been lengthened nearly two miles since the time of the Roman occupation.
The end of Seneca (N. Y.) lake has been crowded northward some two
miles by deposition at its head. Similar changes have taken place and are
now in progress in many other lakes.
Lake ice.[189]—Since fresh water is densest at 39° Fahr., ice does not
commonly form on the surface until the temperature from top to bottom is
reduced to this point. Cooled below this temperature, the surface-water fails
to sink, and with sufficient reduction freezes. If the lake be small, and
especially if it be shallow, it is likely to freeze over completely in any
region where the temperature is notably below the freezing-point for fresh
water for any considerable period of time. It is under these circumstances
that the ice becomes most effective.
Fig. 331.—Ice crowding upon low shore. Clear Lake, Ia. (Calvin.)
Suppose a lake in temperate latitudes, where the range of temperature is
considerable, to be frozen over when the temperature is 20° Fahr. If now the
temperature be suddenly lowered to −10°, and such change of temperature
is not uncommon in the northern part of the United States, the ice contracts
notably. In contracting, it either pulls away from the shores or cracks. If the
soon after the lake becomes extinct.
Many lakes, some of them large[188] and many of them small, are known
to have become extinct, while many others are now in their last stages,
namely, marshes. Many others have been greatly reduced in size. Such
reductions are often obvious where deltas are built into lakes. Thus the delta
built by the Rhone into Lake Geneva is several miles in length, and has
been lengthened nearly two miles since the time of the Roman occupation.
The end of Seneca (N. Y.) lake has been crowded northward some two
miles by deposition at its head. Similar changes have taken place and are
now in progress in many other lakes.
Lake ice.[189]—Since fresh water is densest at 39° Fahr., ice does not
commonly form on the surface until the temperature from top to bottom is
reduced to this point. Cooled below this temperature, the surface-water fails
to sink, and with sufficient reduction freezes. If the lake be small, and
especially if it be shallow, it is likely to freeze over completely in any
region where the temperature is notably below the freezing-point for fresh
water for any considerable period of time. It is under these circumstances
that the ice becomes most effective.
Fig. 331.—Ice crowding upon low shore. Clear Lake, Ia. (Calvin.)
Suppose a lake in temperate latitudes, where the range of temperature is
considerable, to be frozen over when the temperature is 20° Fahr. If now the
temperature be suddenly lowered to −10°, and such change of temperature
is not uncommon in the northern part of the United States, the ice contracts
notably. In contracting, it either pulls away from the shores or cracks. If the
Page 459
former, the water from which the ice is withdrawn quickly freezes; if the
latter, water rises in the cracks and freezes there. In either case, the ice-
cover of the lake is again complete. If the temperature now rises to 20° the
ice expands. The cover is now too large for the lake, and it must either
crowd up on the shores (Fig. 331) or arch up (wrinkle) elsewhere. It follows
the one course or the other, or both, according to the resistance offered by
the shore.
If the water near the shore is very shallow, the ice freezes to the sand,
gravel, and bowlders at the bottom. If the adjacent land is low, the ice in
expanding may shove up over it, carrying the débris frozen in its bottom. It
may even push up loose gravel and sand in front of its edge if they be
present on the shore. Where bowlders are frozen to the bottom of the ice,
the shoreward thrust in expanding has the effect of shifting them in the
same direction, and even of lifting them a little above the normal water-
level. This constant process of concentrating bowlders at the shore-line
gives rise to the “walled” lakes, which are not uncommon in the northern
part of the United States. The “wall” does not commonly extend entirely
around a lake, though it exists at various points on the shores of many lakes.
In making the walls, the ice shoved up by winds, especially in the spring
when the ice is breaking up, coöperates.
latter, water rises in the cracks and freezes there. In either case, the ice-
cover of the lake is again complete. If the temperature now rises to 20° the
ice expands. The cover is now too large for the lake, and it must either
crowd up on the shores (Fig. 331) or arch up (wrinkle) elsewhere. It follows
the one course or the other, or both, according to the resistance offered by
the shore.
If the water near the shore is very shallow, the ice freezes to the sand,
gravel, and bowlders at the bottom. If the adjacent land is low, the ice in
expanding may shove up over it, carrying the débris frozen in its bottom. It
may even push up loose gravel and sand in front of its edge if they be
present on the shore. Where bowlders are frozen to the bottom of the ice,
the shoreward thrust in expanding has the effect of shifting them in the
same direction, and even of lifting them a little above the normal water-
level. This constant process of concentrating bowlders at the shore-line
gives rise to the “walled” lakes, which are not uncommon in the northern
part of the United States. The “wall” does not commonly extend entirely
around a lake, though it exists at various points on the shores of many lakes.
In making the walls, the ice shoved up by winds, especially in the spring
when the ice is breaking up, coöperates.
Page 460
Fig. 333.—Calcareous tufa domes. Pyramid Lake, Nev. (Russell.)
If the lake be bordered by a low marsh, the ice and frozen earth of the
latter are really continuous with the ice of the lake, and the push of the latter
sometimes arches up the former into distinct anticlines, the frozen part only
being involved in the deformation. A succession of colder and less cold
periods may give rise to a succession of such anticlines.[190] If the shore be
steep and of non-resistant material, the crowding of the ice produces
different but not less striking results. Where the thrust of the ice is against a
low cliff of yielding material, such as clay, it disturbs all above the shore-
line. Where the cliff is sufficiently resistant, it withstands the push of the
ice, and the ice itself is warped and broken.
Saline lakes.—A few lakes, especially in arid or semi-arid regions, are
salt, and others are “bitter.” Beside sodium chloride, salt lakes usually
If the lake be bordered by a low marsh, the ice and frozen earth of the
latter are really continuous with the ice of the lake, and the push of the latter
sometimes arches up the former into distinct anticlines, the frozen part only
being involved in the deformation. A succession of colder and less cold
periods may give rise to a succession of such anticlines.[190] If the shore be
steep and of non-resistant material, the crowding of the ice produces
different but not less striking results. Where the thrust of the ice is against a
low cliff of yielding material, such as clay, it disturbs all above the shore-
line. Where the cliff is sufficiently resistant, it withstands the push of the
ice, and the ice itself is warped and broken.
Saline lakes.—A few lakes, especially in arid or semi-arid regions, are
salt, and others are “bitter.” Beside sodium chloride, salt lakes usually
Page 461
contain magnesium chloride, and magnesium and calcium sulphates.
“Bitter” lakes usually contain much sodium carbonate, as well as some
sodium chloride and sulphate, and sometimes borax. The degrees of saltness
and bitterness vary from freshness on the one hand to saturation on the
other. The water of the Caspian Sea (lake) contains, on the average, less salt
than that of the sea; that of Great Salt Lake contains about 18%; that of the
Dead Sea, about 24%; and that of Lake Van (eastern Turkestan), the densest
body of water known, about 33%. See accompanying table.
Many salt lakes, such as the Dead Sea and Great Salt Lake, are
descended from fresh-water ancestors, while others, like the Caspian and
Aral Seas, are probably isolated portions of the ocean. Lakes of the former
class have usually become salt through a decrease in the humidity of the
region where they occur. The water begins to be salt when the aridity is
such that evaporation from the lake exceeds its inflow. In this case the
inflowing waters bring in small amounts of saline and alkaline matter,
which is concentrated as evaporation takes place. The concentration may go
on until the point of saturation is reached, or until chemical reactions cause
precipitation. In general the least soluble minerals are precipitated first.
Thus gypsum begins to be deposited from sea-water when 37% of it has
been evaporated; but the saturation-point for salt is not reached until 93% of
the water has been evaporated (see p. 375). The relations in lakes are
similar, and gypsum deposits often underlie those of salt. Deposits of salt
and other mineral matters once in solution are making in some salt lakes at
the present time, and considerable formations of the same sort have been so
made in the past. Buried beneath sediments of other sorts, beds of common
salt or of other precipitates are preserved for ages. Lime carbonate has been
precipitated in quantity from some extinct lakes (Fig. 333).
The lakes which originate by the isolation of portions of the sea are salt
at the outset. If inflow exceeds evaporation, they become fresher and may
ultimately become fresh; otherwise they remain salt. If evaporation exceeds
inflow they diminish in size and their waters become more and more salt or
bitter.
Indirect effects of lakes.—Lakes tend to modify the climate of the
region where they occur, both by increasing its humidity and by decreasing
its range of temperature. They act as reservoirs for surface-waters, and so
tend to restrain floods and to promote regularity of stream flow. They purify
“Bitter” lakes usually contain much sodium carbonate, as well as some
sodium chloride and sulphate, and sometimes borax. The degrees of saltness
and bitterness vary from freshness on the one hand to saturation on the
other. The water of the Caspian Sea (lake) contains, on the average, less salt
than that of the sea; that of Great Salt Lake contains about 18%; that of the
Dead Sea, about 24%; and that of Lake Van (eastern Turkestan), the densest
body of water known, about 33%. See accompanying table.
Many salt lakes, such as the Dead Sea and Great Salt Lake, are
descended from fresh-water ancestors, while others, like the Caspian and
Aral Seas, are probably isolated portions of the ocean. Lakes of the former
class have usually become salt through a decrease in the humidity of the
region where they occur. The water begins to be salt when the aridity is
such that evaporation from the lake exceeds its inflow. In this case the
inflowing waters bring in small amounts of saline and alkaline matter,
which is concentrated as evaporation takes place. The concentration may go
on until the point of saturation is reached, or until chemical reactions cause
precipitation. In general the least soluble minerals are precipitated first.
Thus gypsum begins to be deposited from sea-water when 37% of it has
been evaporated; but the saturation-point for salt is not reached until 93% of
the water has been evaporated (see p. 375). The relations in lakes are
similar, and gypsum deposits often underlie those of salt. Deposits of salt
and other mineral matters once in solution are making in some salt lakes at
the present time, and considerable formations of the same sort have been so
made in the past. Buried beneath sediments of other sorts, beds of common
salt or of other precipitates are preserved for ages. Lime carbonate has been
precipitated in quantity from some extinct lakes (Fig. 333).
The lakes which originate by the isolation of portions of the sea are salt
at the outset. If inflow exceeds evaporation, they become fresher and may
ultimately become fresh; otherwise they remain salt. If evaporation exceeds
inflow they diminish in size and their waters become more and more salt or
bitter.
Indirect effects of lakes.—Lakes tend to modify the climate of the
region where they occur, both by increasing its humidity and by decreasing
its range of temperature. They act as reservoirs for surface-waters, and so
tend to restrain floods and to promote regularity of stream flow. They purify
Page 462
the waters which enter them by allowing their sediments to settle, and so
influence the work and the life of the waters below.
Composition of lake-waters.—The accompanying table[191] shows the
composition of various inclosed lake-waters, and gives some idea of the
wide range, both in kind and quantity, of the mineral matter held in solution
by them. It is to be noted that the table shows the composition of the waters
of exceptional, rather than common, lakes. The waters of fresh lakes do not
depart widely from those of rivers (p. 107).
TABLE—ANALYSES OF THE WATERS OF INCLOSED
LAKES.
[Reduced to Parts per 1000 by Dr. H. J. Van Housen.]
Locality Abert Lake, Bogdo Caspian Sea. 2° Caspian Sea, Dead Sea,
Oregon Lake W. S. W. of near mouth Ras Dale,
Pischina, at 15 of the surface
feet depth, Volga
wind, W. S. W.
Specific ...... ...... ......
1023.17 1.0216
gravity
Date May 3, 1883 ...... ...... ...... Mar. 20, 1864
Analyst F. W. Gobel Gobel H. Rose
Terreil
Taylor
Reference Lartet Fourth Lariet Geological Bischof’s Bischof’s
Geological Ann. Rep. Exploration of Chemical Chemical
Exploration of U. S. Dead Sea, p. Geology, Geology,
Dead Sea, p. Geol. 284 Vol. I, p. 89 Vol. I, p. 89
278 Survey, p.
454
Sodium, Na 2.838 74.700 1.4440 .3081 .885
Potassium, K 10.880 1.041 .0398 .474
Rubidium, Rb ...... ...... ...... ......
Calcium, Ca ...... 3.647 .1854 .1238 2.150
Magnesium,
.002 13.777 .4095 .0728 4.197
Mg
Lithium, Li ......
Iron, Fe ...... ...... ...... ...... Trace
Chlorine, Cl 8.410 163.344 2.7376 .4576 17.628
Bromine, br2 ...... .043 Trace ...... .167
Carbonic acid
gas, CO2 4.653 ...... .1382 .3746 Trace
influence the work and the life of the waters below.
Composition of lake-waters.—The accompanying table[191] shows the
composition of various inclosed lake-waters, and gives some idea of the
wide range, both in kind and quantity, of the mineral matter held in solution
by them. It is to be noted that the table shows the composition of the waters
of exceptional, rather than common, lakes. The waters of fresh lakes do not
depart widely from those of rivers (p. 107).
TABLE—ANALYSES OF THE WATERS OF INCLOSED
LAKES.
[Reduced to Parts per 1000 by Dr. H. J. Van Housen.]
Locality Abert Lake, Bogdo Caspian Sea. 2° Caspian Sea, Dead Sea,
Oregon Lake W. S. W. of near mouth Ras Dale,
Pischina, at 15 of the surface
feet depth, Volga
wind, W. S. W.
Specific ...... ...... ......
1023.17 1.0216
gravity
Date May 3, 1883 ...... ...... ...... Mar. 20, 1864
Analyst F. W. Gobel Gobel H. Rose
Terreil
Taylor
Reference Lartet Fourth Lariet Geological Bischof’s Bischof’s
Geological Ann. Rep. Exploration of Chemical Chemical
Exploration of U. S. Dead Sea, p. Geology, Geology,
Dead Sea, p. Geol. 284 Vol. I, p. 89 Vol. I, p. 89
278 Survey, p.
454
Sodium, Na 2.838 74.700 1.4440 .3081 .885
Potassium, K 10.880 1.041 .0398 .474
Rubidium, Rb ...... ...... ...... ......
Calcium, Ca ...... 3.647 .1854 .1238 2.150
Magnesium,
.002 13.777 .4095 .0728 4.197
Mg
Lithium, Li ......
Iron, Fe ...... ...... ...... ...... Trace
Chlorine, Cl 8.410 163.344 2.7376 .4576 17.628
Bromine, br2 ...... .043 Trace ...... .167
Carbonic acid
gas, CO2 4.653 ...... .1382 .3746 Trace
Page 463
Sulphuric
acid, H2SO4 .509 .198 1.3372 .3109 .202
Phosphoric
acid, HPO4
Nitric acid,
NO3
Boracic acid,
H3BO3 ...... ......
Silica, SiO2 .064 .006
Alumina,
Al2O3 ...... ...... ...... Trace
Hydrogen in
bicarbonates, .0023 .0062 ......
H
Ammonium,
NH4 ...... Trace
Organic
...... ...... ...... ...... Trace
matter
27.357 256.750 6.2940 1.6540 25.709
Locality Dead Sea, near Dead Sea, at Dead Sea, at Elton Lake Elton Lake
the Island, 393 ft., 656 ft.,
surface between Ras between Ras
Feschkak and Feschkak and
Ras Zerka Ras Zerka
Specific
1.1647 1.2225 1.2300 ...... ......
gravity
Date Apr. 7, 1864 Mar. 15, 1804 Mar. 15, 1864 April August
Analyst Terreil Terreil Terreil Gobel Erdman
Reference Lartet Lartet Lartet Bischof’s Bischof’s
Geological Geological Geological Chemical Chemical
Exploration Exploration Exploration Geology, Geology,
of Dead Sea, of Dead Sea, of Dead Sea, Vol. I, p. Vol. I, p.
p. 278 p. 278 p. 278 403–405 403–405
Sodium, Na 22.400 25.071 25.107 51.590 29.300
Potassium, K 3.547 3.990 4.503 1.162
Rubidium,
...... ...... ...... ......
Rb
Calcium, Ca 9.094 3.704 4.218 ...... .106
Magnesium,
25.529 41.306 42.006 29.971 45.598
Mg
Lithium, Li ...... ...... ......
Iron, Fe Trace Trace Trace ...... ......
Chlorine, Cl 126.521 166.340 170.425 159.498 166.890
Bromine, br2 4.568 4.870 4.385 .059 ......
acid, H2SO4 .509 .198 1.3372 .3109 .202
Phosphoric
acid, HPO4
Nitric acid,
NO3
Boracic acid,
H3BO3 ...... ......
Silica, SiO2 .064 .006
Alumina,
Al2O3 ...... ...... ...... Trace
Hydrogen in
bicarbonates, .0023 .0062 ......
H
Ammonium,
NH4 ...... Trace
Organic
...... ...... ...... ...... Trace
matter
27.357 256.750 6.2940 1.6540 25.709
Locality Dead Sea, near Dead Sea, at Dead Sea, at Elton Lake Elton Lake
the Island, 393 ft., 656 ft.,
surface between Ras between Ras
Feschkak and Feschkak and
Ras Zerka Ras Zerka
Specific
1.1647 1.2225 1.2300 ...... ......
gravity
Date Apr. 7, 1864 Mar. 15, 1804 Mar. 15, 1864 April August
Analyst Terreil Terreil Terreil Gobel Erdman
Reference Lartet Lartet Lartet Bischof’s Bischof’s
Geological Geological Geological Chemical Chemical
Exploration Exploration Exploration Geology, Geology,
of Dead Sea, of Dead Sea, of Dead Sea, Vol. I, p. Vol. I, p.
p. 278 p. 278 p. 278 403–405 403–405
Sodium, Na 22.400 25.071 25.107 51.590 29.300
Potassium, K 3.547 3.990 4.503 1.162
Rubidium,
...... ...... ...... ......
Rb
Calcium, Ca 9.094 3.704 4.218 ...... .106
Magnesium,
25.529 41.306 42.006 29.971 45.598
Mg
Lithium, Li ...... ...... ......
Iron, Fe Trace Trace Trace ...... ......
Chlorine, Cl 126.521 166.340 170.425 159.498 166.890
Bromine, br2 4.568 4.870 4.385 .059 ......
Page 464
Carbonic acid
gas, CO2 Trace Trace Trace ...... .272
Sulphuric
acid, H2SO4 .494 .451 .459 13.320 17.734
Phosphoric
acid, HPO4
Nitric acid,
NO3
Boracic acid,
H3BO3 ...... ...... ......
Silica, SiO2 Trace Trace Trace
Alumina,
Al2O3 Trace Trace Trace
Hydrogen in
bicarbonates, ...... ...... ......
H
Ammonium,
NH4 Trace Trace Trace ...... ......
Organic
Trace Trace Trace Trace 5.080
matter
192.153 245.732 251.103 255.600 264.980
Locality Great Salt Great Salt Great Salt Humboldt[192] Indevak
Elton Lake
Lake Lake Lake Lake Lake
Specific
1.27288 1.170 2.4 1.102 1.007 ......
gravity
Date October 1850 1869 Aug., 1873 ...... ......
Analyst H. Rose L. D. Gale O. D. Allen H. Bassett O. D. Allen Gobel
Reference Bischof’s Stambury’s U. S. Amer. U. S. Expl. Lartet
Chemical Expedition Geological Chemist, 40th par. Expl.
Geology. to Great Expl. 40th 1874, p. 1877, Vol. I, of
Vol. I, p. Salt Lake, par. 1877, 395 p. 528 Dead
403–405 p. 410 Vol. II, p. Sea, p.
435 284
Sodium, Na 15.060 85.330 49.690 38.3 .27842 94.050
Potassium, K 1.204 2.407 9.9 .06083 .529
Rubidium,
...... ...... ...... ...... ......
Rb
Calcium, Ca ...... Trace[196] .255 .6 .01257 .123
Magnesium,
60.540 .636 3.780 3.0 .01648 5.076
Mg
Lithium, Li Trace Trace
Iron, Fe ...... ...... ...... ...... ...... ......
Chlorine, Cl 171.936 124.454 83.946 73.6 .29545 158.687
gas, CO2 Trace Trace Trace ...... .272
Sulphuric
acid, H2SO4 .494 .451 .459 13.320 17.734
Phosphoric
acid, HPO4
Nitric acid,
NO3
Boracic acid,
H3BO3 ...... ...... ......
Silica, SiO2 Trace Trace Trace
Alumina,
Al2O3 Trace Trace Trace
Hydrogen in
bicarbonates, ...... ...... ......
H
Ammonium,
NH4 Trace Trace Trace ...... ......
Organic
Trace Trace Trace Trace 5.080
matter
192.153 245.732 251.103 255.600 264.980
Locality Great Salt Great Salt Great Salt Humboldt[192] Indevak
Elton Lake
Lake Lake Lake Lake Lake
Specific
1.27288 1.170 2.4 1.102 1.007 ......
gravity
Date October 1850 1869 Aug., 1873 ...... ......
Analyst H. Rose L. D. Gale O. D. Allen H. Bassett O. D. Allen Gobel
Reference Bischof’s Stambury’s U. S. Amer. U. S. Expl. Lartet
Chemical Expedition Geological Chemist, 40th par. Expl.
Geology. to Great Expl. 40th 1874, p. 1877, Vol. I, of
Vol. I, p. Salt Lake, par. 1877, 395 p. 528 Dead
403–405 p. 410 Vol. II, p. Sea, p.
435 284
Sodium, Na 15.060 85.330 49.690 38.3 .27842 94.050
Potassium, K 1.204 2.407 9.9 .06083 .529
Rubidium,
...... ...... ...... ...... ......
Rb
Calcium, Ca ...... Trace[196] .255 .6 .01257 .123
Magnesium,
60.540 .636 3.780 3.0 .01648 5.076
Mg
Lithium, Li Trace Trace
Iron, Fe ...... ...... ...... ...... ...... ......
Chlorine, Cl 171.936 124.454 83.946 73.6 .29545 158.687
Page 465
Bromine, br2 Trace ......
Carbonic
acid gas, ...... ...... ...... ...... .20126 ......
CO2
Sulphuric
acid, H2SO4 42.560 12.400 9.858 8.8 .03040 3.065
Phosphoric
acid, HPO4 .00069
Nitric acid,
NO3 ...... .03250
Boracic acid,
H3BO3 Trace Trace
Silica, SiO2 ...... .03250
Alumina,
Al2O3
Hydrogen in
bicarbonates,
H
Ammonium,
NH4 ......
Organic
Trace ...... ...... ...... ...... .....
matter
291.300 222.820 149.936 134.2 .92800 261.530
Locality Soda Lake,
Soda Lake, Mono Lake,
near Ragtown,
near Ragtown, Cal., at 1 foot Owen’s Lake,
Nev., at 100 Urmiah Lake
Nev., at 1 foot below Cal.
feet below
below surface surface
surface
Specific
1.101 1.101 1.048 1.155 1.051
gravity
Date ...... ...... July 16, 1883 ...... ......
Analyst T. M.
T. M. Chatard T. M. Chatard Hitchcock O. Loew
Chatard
Reference Lartet Appendix JJ
Bulletin No. Geological Ann. Rep.
Ante, p. 70 Ante, p. 70 9. U. S. Exploration of Chief
Survey, p. 26 Dead Sea, p. Engineers,
284 1876 p. 190
Sodium, Na 41.632 40.206 18.100 74.890 21.650
Potassium, K 2.290 2.425 1.111 2.751
Rubidium, Rb ...... ...... ......
Calcium, Ca ...... ...... .278 .529 Trace
Magnesium,
.245 .245 .125 2.914 Trace
Mg
Carbonic
acid gas, ...... ...... ...... ...... .20126 ......
CO2
Sulphuric
acid, H2SO4 42.560 12.400 9.858 8.8 .03040 3.065
Phosphoric
acid, HPO4 .00069
Nitric acid,
NO3 ...... .03250
Boracic acid,
H3BO3 Trace Trace
Silica, SiO2 ...... .03250
Alumina,
Al2O3
Hydrogen in
bicarbonates,
H
Ammonium,
NH4 ......
Organic
Trace ...... ...... ...... ...... .....
matter
291.300 222.820 149.936 134.2 .92800 261.530
Locality Soda Lake,
Soda Lake, Mono Lake,
near Ragtown,
near Ragtown, Cal., at 1 foot Owen’s Lake,
Nev., at 100 Urmiah Lake
Nev., at 1 foot below Cal.
feet below
below surface surface
surface
Specific
1.101 1.101 1.048 1.155 1.051
gravity
Date ...... ...... July 16, 1883 ...... ......
Analyst T. M.
T. M. Chatard T. M. Chatard Hitchcock O. Loew
Chatard
Reference Lartet Appendix JJ
Bulletin No. Geological Ann. Rep.
Ante, p. 70 Ante, p. 70 9. U. S. Exploration of Chief
Survey, p. 26 Dead Sea, p. Engineers,
284 1876 p. 190
Sodium, Na 41.632 40.206 18.100 74.890 21.650
Potassium, K 2.290 2.425 1.111 2.751
Rubidium, Rb ...... ...... ......
Calcium, Ca ...... ...... .278 .529 Trace
Magnesium,
.245 .245 .125 2.914 Trace
Mg
Page 466
Lithium, Li ...... Trace
Iron, Fe ...... ...... ...... ...... ......
Chlorine, Cl 41.496 40.206 11.610 119.496 13.440
Bromine, br2 ...... ...... ...... ......
Carbonic acid
gas, CO2 15.650[7] 18.058[7] 14.465[7] ...... 13.140
Sulphuric
acid, H2SO4 11.771 11.943 6.520 7.671 9.362
Phosphoric
acid, HPO4 ...... ......
Nitric acid,
NO3 ...... ...... ...... Trace
Boracic acid,
H3BO3 .285 .287 .153 Trace
Silica, SiO2 .275 .281 .268 .164
Alumina,
Al2O3 ...... Trace
Hydrogen in
bicarbonates, ......
H
Ammonium,
NH4 ......
Organic matter ...... ...... ...... ...... Trace
113.644 113.651 49.630 205.500 60.507
Locality Pyramid Walker
Sevier Winnemucca
Lake,[193] Lake, Utah Lake,[194] Lake, Nev. Van Lake Aral Sea
Nev. Nev.
Specific
...... ...... 1.003 1.001 ...... ......
gravity
Date Aug.
1872 Sept., 1882 Aug., 1882 ...... ......
1882
Analyst F. W. F. W.
O. Loew F. W. Clarke Chancourtois ......
Clarke Clarke
Reference U. S. Ante, p. 70 Ante, p. 63 Bischof’s Roth
Survey, Chemical Chemical
Ante, pp. W. 100 Geology, Geology,
57 and 58 M., Vol. Vol. I, p. 94 p. 465
III, p.
144
Sodium, Na 1.1796 28.840 .85535 1.2970 8.502[4] 2.4512
Potassium, K .0733 Trace .0686 .246 .0584
Rubidium, Rb ...... ...... ...... ...... .0022
Calcium, Ca .0089 .118 .02215 .0196 ...... .4581
Iron, Fe ...... ...... ...... ...... ......
Chlorine, Cl 41.496 40.206 11.610 119.496 13.440
Bromine, br2 ...... ...... ...... ......
Carbonic acid
gas, CO2 15.650[7] 18.058[7] 14.465[7] ...... 13.140
Sulphuric
acid, H2SO4 11.771 11.943 6.520 7.671 9.362
Phosphoric
acid, HPO4 ...... ......
Nitric acid,
NO3 ...... ...... ...... Trace
Boracic acid,
H3BO3 .285 .287 .153 Trace
Silica, SiO2 .275 .281 .268 .164
Alumina,
Al2O3 ...... Trace
Hydrogen in
bicarbonates, ......
H
Ammonium,
NH4 ......
Organic matter ...... ...... ...... ...... Trace
113.644 113.651 49.630 205.500 60.507
Locality Pyramid Walker
Sevier Winnemucca
Lake,[193] Lake, Utah Lake,[194] Lake, Nev. Van Lake Aral Sea
Nev. Nev.
Specific
...... ...... 1.003 1.001 ...... ......
gravity
Date Aug.
1872 Sept., 1882 Aug., 1882 ...... ......
1882
Analyst F. W. F. W.
O. Loew F. W. Clarke Chancourtois ......
Clarke Clarke
Reference U. S. Ante, p. 70 Ante, p. 63 Bischof’s Roth
Survey, Chemical Chemical
Ante, pp. W. 100 Geology, Geology,
57 and 58 M., Vol. Vol. I, p. 94 p. 465
III, p.
144
Sodium, Na 1.1796 28.840 .85535 1.2970 8.502[4] 2.4512
Potassium, K .0733 Trace .0686 .246 .0584
Rubidium, Rb ...... ...... ...... ...... .0022
Calcium, Ca .0089 .118 .02215 .0196 ...... .4581
Page 467
Magnesium,
Mg
.0797 2.000 .03830 .0173 .157[197] .5965
Lithium, Li ...... .....
Iron, Fe ...... ...... ...... ..... [197] .0008
Trace
Chlorine, Cl 1.4300 45.500 .58375 1.6934 5.693 3.8386
Bromine, br2 ...... ...... ...... ...... .0029
Carbonic acid
gas, CO2 .4900[7] ...... .47445[198] .3458[198] 5.267[195] .0918
Sulphuric
acid, H2SO4 .1822 9.345 .52000 .1333 2.555 3.3368
Phosphoric
acid, HPO4 ...... .0011
Nitric acid,
NO3 Trace
Boracic acid,
H3BO3 ...... ...... ...... ......
Silica, SiO2 .0334 .00750 .0275 .180 .0032
Alumina,
Al2O3 ...... ...... ......
Hydrogen in
bicarbonates, ......
H
Ammonium,
NH4 Trace
Organic
...... ...... ...... ...... ...... Trace
matter
3.4861 86.403 2.50150 3.6025 22.600 10.8416
Mg
.0797 2.000 .03830 .0173 .157[197] .5965
Lithium, Li ...... .....
Iron, Fe ...... ...... ...... ..... [197] .0008
Trace
Chlorine, Cl 1.4300 45.500 .58375 1.6934 5.693 3.8386
Bromine, br2 ...... ...... ...... ...... .0029
Carbonic acid
gas, CO2 .4900[7] ...... .47445[198] .3458[198] 5.267[195] .0918
Sulphuric
acid, H2SO4 .1822 9.345 .52000 .1333 2.555 3.3368
Phosphoric
acid, HPO4 ...... .0011
Nitric acid,
NO3 Trace
Boracic acid,
H3BO3 ...... ...... ...... ......
Silica, SiO2 .0334 .00750 .0275 .180 .0032
Alumina,
Al2O3 ...... ...... ......
Hydrogen in
bicarbonates, ......
H
Ammonium,
NH4 Trace
Organic
...... ...... ...... ...... ...... Trace
matter
3.4861 86.403 2.50150 3.6025 22.600 10.8416
Page 468
CHAPTER VII.
THE ORIGIN AND DESCENT OF ROCKS.
It has been the current opinion that the earth was once in a molten state,
and thence cooled to a solid condition, and hence that all the primitive rocks
were igneous. Even those who think that the earth may never have passed
through a molten state agree that the oldest known rocks are either true
igneous rocks, or rocks of very similar nature. A molten magma may,
therefore, be taken as the mother state of the rocks. Starting with this
conception, the natural order of events suggests the inquiries (1) how rocks
are formed from molten magmas, (2) what natures they assume, (3) how
other rocks are derived from them, (4) how still other rocks are derived
from these derivatives, and so on. To answer these inquiries is to trace out
the generations of rocks and learn the general history of rock-formation.
(1) The process by which igneous rocks are formed from lavas is actually
taking place in existing volcanoes. As these are widely scattered over the
face of the earth, the material poured out by them represents different parts
of the interior and varies in nature accordingly. This affords the means of
studying the differences that arise from differences of material. This is a
radical consideration, for variations in composition give rise to the most
fundamental distinctions between rocks, though by no means the only ones.
Rocks which have the same composition often differ greatly in texture or
structure, owing to the varying conditions under which they were formed.
In the solidification of rocks from the molten state, the rate of cooling
causes many differences. A means of studying this is afforded by the
various lava flows that are now being poured out on the surface under
different conditions; but a more important means is afforded by extinct
volcanoes, especially by those which have been deeply cut open by erosion.
In certain very ancient volcanoes, not only have the solidified lava streams
of the surface been cut across by erosion, but the lava that remained in the
crater, or in the neck that led up from below, is laid bare for inspection.
Exposures of even more profound nature have been made by the great
THE ORIGIN AND DESCENT OF ROCKS.
It has been the current opinion that the earth was once in a molten state,
and thence cooled to a solid condition, and hence that all the primitive rocks
were igneous. Even those who think that the earth may never have passed
through a molten state agree that the oldest known rocks are either true
igneous rocks, or rocks of very similar nature. A molten magma may,
therefore, be taken as the mother state of the rocks. Starting with this
conception, the natural order of events suggests the inquiries (1) how rocks
are formed from molten magmas, (2) what natures they assume, (3) how
other rocks are derived from them, (4) how still other rocks are derived
from these derivatives, and so on. To answer these inquiries is to trace out
the generations of rocks and learn the general history of rock-formation.
(1) The process by which igneous rocks are formed from lavas is actually
taking place in existing volcanoes. As these are widely scattered over the
face of the earth, the material poured out by them represents different parts
of the interior and varies in nature accordingly. This affords the means of
studying the differences that arise from differences of material. This is a
radical consideration, for variations in composition give rise to the most
fundamental distinctions between rocks, though by no means the only ones.
Rocks which have the same composition often differ greatly in texture or
structure, owing to the varying conditions under which they were formed.
In the solidification of rocks from the molten state, the rate of cooling
causes many differences. A means of studying this is afforded by the
various lava flows that are now being poured out on the surface under
different conditions; but a more important means is afforded by extinct
volcanoes, especially by those which have been deeply cut open by erosion.
In certain very ancient volcanoes, not only have the solidified lava streams
of the surface been cut across by erosion, but the lava that remained in the
crater, or in the neck that led up from below, is laid bare for inspection.
Exposures of even more profound nature have been made by the great
Page 469
disruptions which the outer part of the crust has suffered. In certain tracts
there have been profound fractures, and the formations on one side of these
have settled down and on the other side have been pushed up (faulted), so
as to expose parts that were once much below the surface. Sometimes also
the crust has been folded and crumpled, and the wrinkles thus formed have
afterwards been worn away or cut open by deep valleys, and rocks that
were once deeply buried have been laid bare. By the revelations made in
these and other ways, it has been learned that at various times in the history
of the earth molten matter has been thrust into fissures or intruded between
layers of the crust and cooled there, without coming to the surface.
Sometimes the lava appears to have forced its way into the rocks, and
sometimes to have lifted the upper beds and formed great subterranean
layers or tumor-like aggregates, called bathyliths and laccoliths (Fig. 334).
Such intruded bodies of molten rock, solidifying under the varying
conditions of such subterranean situations, are a fruitful source of
instruction respecting the influence of varying rates and modes of cooling,
as well as of other attendant conditions.
Fig. 334.—Diagram of a laccolith. (Gilbert.)
It will thus be readily seen that the rate of cooling of the various molten
rocks must have differed very greatly. In the portions poured out upon the
surface there were sometimes narrow streams and thin sheets, giving large
exposure in proportion to the mass (Fig. 335), and sometimes thick flows
and deep pondings in basins and choked valleys, giving massive bodies
with relatively small surface exposure. There were explosions of the lava
into minute particles with almost instantaneous cooling, and there were
eruptions beneath the sea the peculiar effects of which are rather matters of
inference than of positive knowledge. In the portions underground there
were insinuations into thin fissures, on the one hand, and in-thrustings of
there have been profound fractures, and the formations on one side of these
have settled down and on the other side have been pushed up (faulted), so
as to expose parts that were once much below the surface. Sometimes also
the crust has been folded and crumpled, and the wrinkles thus formed have
afterwards been worn away or cut open by deep valleys, and rocks that
were once deeply buried have been laid bare. By the revelations made in
these and other ways, it has been learned that at various times in the history
of the earth molten matter has been thrust into fissures or intruded between
layers of the crust and cooled there, without coming to the surface.
Sometimes the lava appears to have forced its way into the rocks, and
sometimes to have lifted the upper beds and formed great subterranean
layers or tumor-like aggregates, called bathyliths and laccoliths (Fig. 334).
Such intruded bodies of molten rock, solidifying under the varying
conditions of such subterranean situations, are a fruitful source of
instruction respecting the influence of varying rates and modes of cooling,
as well as of other attendant conditions.
Fig. 334.—Diagram of a laccolith. (Gilbert.)
It will thus be readily seen that the rate of cooling of the various molten
rocks must have differed very greatly. In the portions poured out upon the
surface there were sometimes narrow streams and thin sheets, giving large
exposure in proportion to the mass (Fig. 335), and sometimes thick flows
and deep pondings in basins and choked valleys, giving massive bodies
with relatively small surface exposure. There were explosions of the lava
into minute particles with almost instantaneous cooling, and there were
eruptions beneath the sea the peculiar effects of which are rather matters of
inference than of positive knowledge. In the portions underground there
were insinuations into thin fissures, on the one hand, and in-thrustings of
Page 470
thick bodies, on the other. Some intrusions entered the upper part of the
crust where the rocks were cold and wet, and some were thrust into the
deeper portions where the rocks were warmer and less penetrated by water.
Sometimes the lava rose rapidly and was little cooled in passage, sometimes
slowly with more cooling en route, and sometimes there were long halts
between eruptions, with much opportunity to cool. An almost infinite
variety of conditions is thus presented, and with it a rich field for the study
of the modes of solidification.
Fig. 335.—Fresh lava flow, with large surface exposure. Holemaumau, Hawaii. (Libbey.)
In the underground intrusions the additional factor of high pressure was
also present, and this is the third important condition in determining the
nature of igneous rocks.
The three factors, composition, rate of cooling, and degree of pressure,
require special consideration.
Composition of Igneous Rocks.
All or nearly all the chemical elements known on the earth are found in
greater or less amounts in igneous rocks, and in a broad sense are
constituents of them. If there are any exceptions, they are most likely to be
found in the rarer elements in the atmosphere. Oxygen, nitrogen, hydrogen,
aqueous vapor, and carbonic acid, which make up the mass of the present
crust where the rocks were cold and wet, and some were thrust into the
deeper portions where the rocks were warmer and less penetrated by water.
Sometimes the lava rose rapidly and was little cooled in passage, sometimes
slowly with more cooling en route, and sometimes there were long halts
between eruptions, with much opportunity to cool. An almost infinite
variety of conditions is thus presented, and with it a rich field for the study
of the modes of solidification.
Fig. 335.—Fresh lava flow, with large surface exposure. Holemaumau, Hawaii. (Libbey.)
In the underground intrusions the additional factor of high pressure was
also present, and this is the third important condition in determining the
nature of igneous rocks.
The three factors, composition, rate of cooling, and degree of pressure,
require special consideration.
Composition of Igneous Rocks.
All or nearly all the chemical elements known on the earth are found in
greater or less amounts in igneous rocks, and in a broad sense are
constituents of them. If there are any exceptions, they are most likely to be
found in the rarer elements in the atmosphere. Oxygen, nitrogen, hydrogen,
aqueous vapor, and carbonic acid, which make up the mass of the present
Page 471
atmosphere, are all found in lavas and in their cooled products. Probably all
the rarer elements also occur in igneous rocks. Helium is known to be given
forth by springs.
Leading elements.—But although nearly or quite all the known
chemical elements enter into the igneous rocks, only a few of them are
abundant. These are regarded as normal or essential constituents, while the
rarer substances are regarded as incidental. By combining a large number of
the most trustworthy analyses of rocks of all sorts, F. W. Clarke[199] has
estimated the relative amounts of the more abundant elements in the crust
of the earth with the following result:
Percent. in
Element. Symbol.
the Solid Crust.
Oxygen (O) 47.02
Silicon (Si) 28.06
Aluminum (Al) 8.16
Iron (Fe) 4.64
Calcium (Ca) 3.50
Magnesium (Mg) 2.62
Sodium (Na) 2.63
Potassium (K) 2.32
Titanium (Ti) .41
Hydrogen (H) .17
Carbon (C) .12
Phosphorus (P) .09
Manganese (Mn) .07
Sulphur (S) .07
Barium (Ba) .05
Strontium (Sr) .02
Chromium (Cr) .01
Nickel (Ni) .01
Lithium (Li) .01
Chlorine (Cl) .01
Fluorine (Fl) .01
———
100.00
It will be seen that only eight of the elements hold a high rank in
quantity. Many that are of the utmost importance in the history of the earth
and the affairs of men are low in the list, or do not even appear in it at all,
the rarer elements also occur in igneous rocks. Helium is known to be given
forth by springs.
Leading elements.—But although nearly or quite all the known
chemical elements enter into the igneous rocks, only a few of them are
abundant. These are regarded as normal or essential constituents, while the
rarer substances are regarded as incidental. By combining a large number of
the most trustworthy analyses of rocks of all sorts, F. W. Clarke[199] has
estimated the relative amounts of the more abundant elements in the crust
of the earth with the following result:
Percent. in
Element. Symbol.
the Solid Crust.
Oxygen (O) 47.02
Silicon (Si) 28.06
Aluminum (Al) 8.16
Iron (Fe) 4.64
Calcium (Ca) 3.50
Magnesium (Mg) 2.62
Sodium (Na) 2.63
Potassium (K) 2.32
Titanium (Ti) .41
Hydrogen (H) .17
Carbon (C) .12
Phosphorus (P) .09
Manganese (Mn) .07
Sulphur (S) .07
Barium (Ba) .05
Strontium (Sr) .02
Chromium (Cr) .01
Nickel (Ni) .01
Lithium (Li) .01
Chlorine (Cl) .01
Fluorine (Fl) .01
———
100.00
It will be seen that only eight of the elements hold a high rank in
quantity. Many that are of the utmost importance in the history of the earth
and the affairs of men are low in the list, or do not even appear in it at all,
Page 472
because their quantity is too small to be estimated in percentages. The
precious metals, and even some of the more common metals, as lead, zinc,
and copper, are too scarce to form an appreciable percentage.
Union of elements.—In a general study of the igneous rocks we may for
the present neglect all but the first eight of these elements. Out of these
elements spring various chemical combinations, and out of these
combinations spring the various minerals, and out of the combinations of
minerals come the various rocks. The union of oxygen with the other seven
elements may be taken as a fundamental step in this series of combinations.
The result is the following oxides: Silica (SiO2), alumina (Al2O3), ferrous,
ferric, and magnetic oxide (FeO, Fe2O3, and Fe3O4), magnesia (MgO),
calcium oxide or lime (CaO), soda (Na2O), and potash (K2O). The oxygen
sometimes unites in proportions different from those here given, but such
exceptions may be neglected in a general study. We thus have nine leading
oxides. Of these, silica acts as an acid, or more strictly according to the
newer chemical view, as an acid anhydride. All the rest, except the magnetic
oxide of iron, and sometimes the oxide of aluminum, act as basic oxides.
In the older chemical philosophy these oxides were supposed to combine
by the simple union of an acid oxide with a basic oxide, and to remain as
oxide joined to oxide; thus silica (SiO2) and lime (CaO) formed silicate of
lime (CaO,Si2). The symbols express the idea better than the words. This
method is used in the older geological works and in some of the later. But in
the newer chemical doctrine, the oxides are not believed to remain so
distinct after their union, and the symbols are written CaSiO3, and the
compound is named calcium silicate. According to the modern doctrine of
solution, some of the calcium, silicon, and oxygen may exist as free ions in
molten rock. The precise way in which the elements are related to each
other in these compounds can scarcely be said to be known. For the general
purposes of geology it is most convenient to think of these oxides as uniting
in the simple fashion first named, and this involves no apparent geological
error in general studies, since they are oxides when they enter the
compound, and if the compound is decomposed they usually come forth
again as oxides; but in closer studies more complex unions, attended by
dissociations (ionization), must be recognized.
precious metals, and even some of the more common metals, as lead, zinc,
and copper, are too scarce to form an appreciable percentage.
Union of elements.—In a general study of the igneous rocks we may for
the present neglect all but the first eight of these elements. Out of these
elements spring various chemical combinations, and out of these
combinations spring the various minerals, and out of the combinations of
minerals come the various rocks. The union of oxygen with the other seven
elements may be taken as a fundamental step in this series of combinations.
The result is the following oxides: Silica (SiO2), alumina (Al2O3), ferrous,
ferric, and magnetic oxide (FeO, Fe2O3, and Fe3O4), magnesia (MgO),
calcium oxide or lime (CaO), soda (Na2O), and potash (K2O). The oxygen
sometimes unites in proportions different from those here given, but such
exceptions may be neglected in a general study. We thus have nine leading
oxides. Of these, silica acts as an acid, or more strictly according to the
newer chemical view, as an acid anhydride. All the rest, except the magnetic
oxide of iron, and sometimes the oxide of aluminum, act as basic oxides.
In the older chemical philosophy these oxides were supposed to combine
by the simple union of an acid oxide with a basic oxide, and to remain as
oxide joined to oxide; thus silica (SiO2) and lime (CaO) formed silicate of
lime (CaO,Si2). The symbols express the idea better than the words. This
method is used in the older geological works and in some of the later. But in
the newer chemical doctrine, the oxides are not believed to remain so
distinct after their union, and the symbols are written CaSiO3, and the
compound is named calcium silicate. According to the modern doctrine of
solution, some of the calcium, silicon, and oxygen may exist as free ions in
molten rock. The precise way in which the elements are related to each
other in these compounds can scarcely be said to be known. For the general
purposes of geology it is most convenient to think of these oxides as uniting
in the simple fashion first named, and this involves no apparent geological
error in general studies, since they are oxides when they enter the
compound, and if the compound is decomposed they usually come forth
again as oxides; but in closer studies more complex unions, attended by
dissociations (ionization), must be recognized.
Page 473
Formation of minerals.—As but one of the leading oxides that abound
in an average magma plays the part of an acid, the silica, a very simple
conception of the general nature of igneous rocks may be reached by noting
that they are mostly silicates of the seven leading basic oxides—alumina,
potash, soda, lime, magnesia, and the iron oxides. This general idea is a
very useful one and represents a most important truth; but in its use we
must not forget that there are many exceptions. Sulphur, phosphorus,
chlorine, and other elements unite with the bases to form sulphates,
sulphides, phosphates, phosphides, chlorides, etc. So also there are many
minor bases that form silicates; and these minor bases unite with the minor
acids to form many more or less rare minerals. Again, there are native
metals in some igneous rocks. But altogether these hardly reach more than
one or two percent. of the whole.
There are, however, two exceptions of more importance. In the molten
magma the acid and basic elements are not always evenly matched. When
there is an excess of silica, a portion remains free and takes the form of
quartz (SiO2). If there is an excess of the basic oxides, the weakest one is
usually left out of the combination. This is commonly the iron oxide, which
then usually takes the form of magnetite (Fe3O4). It is a singular fact that
quartz often forms when there is no excess of silica, and magnetite when
there is no excess of base. Quartz (free acid anhydride) and magnetite (free
basic oxide) sometimes occur in the same rock. The explanation for this is
yet to be found. These form rather important exceptions to the
generalization that the igneous rocks are mostly made up of silicates, but,
thus qualified, it expresses the essential truth, and has the merit of
embodying the central chemical fact relative to these rocks.
Sources of complexity.—But here simplicity ends. As we pass on to the
specific silicates that are formed, we encounter several sources of
complexity. In the first place, the silica unites with the bases in different
ratios and thus gives rise to unisilicates or orthosilicates (ratio of oxygen of
bases to oxygen of silica, 1:1), subsilicates (ratio more than 1), bisilicates
(ratio 1:2), trisilicates or polysilicates (ratio 1:3 or higher), and
combinations of these. All the bases are not known to combine in all these
ways, but many do in more than one of them. Still, if the silica were content
to unite with each of the bases by itself alone, the results would remain
comparatively simple; but instead of this it unites with two or more at the
in an average magma plays the part of an acid, the silica, a very simple
conception of the general nature of igneous rocks may be reached by noting
that they are mostly silicates of the seven leading basic oxides—alumina,
potash, soda, lime, magnesia, and the iron oxides. This general idea is a
very useful one and represents a most important truth; but in its use we
must not forget that there are many exceptions. Sulphur, phosphorus,
chlorine, and other elements unite with the bases to form sulphates,
sulphides, phosphates, phosphides, chlorides, etc. So also there are many
minor bases that form silicates; and these minor bases unite with the minor
acids to form many more or less rare minerals. Again, there are native
metals in some igneous rocks. But altogether these hardly reach more than
one or two percent. of the whole.
There are, however, two exceptions of more importance. In the molten
magma the acid and basic elements are not always evenly matched. When
there is an excess of silica, a portion remains free and takes the form of
quartz (SiO2). If there is an excess of the basic oxides, the weakest one is
usually left out of the combination. This is commonly the iron oxide, which
then usually takes the form of magnetite (Fe3O4). It is a singular fact that
quartz often forms when there is no excess of silica, and magnetite when
there is no excess of base. Quartz (free acid anhydride) and magnetite (free
basic oxide) sometimes occur in the same rock. The explanation for this is
yet to be found. These form rather important exceptions to the
generalization that the igneous rocks are mostly made up of silicates, but,
thus qualified, it expresses the essential truth, and has the merit of
embodying the central chemical fact relative to these rocks.
Sources of complexity.—But here simplicity ends. As we pass on to the
specific silicates that are formed, we encounter several sources of
complexity. In the first place, the silica unites with the bases in different
ratios and thus gives rise to unisilicates or orthosilicates (ratio of oxygen of
bases to oxygen of silica, 1:1), subsilicates (ratio more than 1), bisilicates
(ratio 1:2), trisilicates or polysilicates (ratio 1:3 or higher), and
combinations of these. All the bases are not known to combine in all these
ways, but many do in more than one of them. Still, if the silica were content
to unite with each of the bases by itself alone, the results would remain
comparatively simple; but instead of this it unites with two or more at the
Page 474
same time; and, more than that, it unites with them in varying amounts. The
case would still remain measurably simple if these chemical compounds
always crystallized out by themselves, each compound forming one
mineral, and but one; but the different silicates have the confusing habit of
crystallizing together in the same mineral. A crystal may thus sometimes be
seen, under the microscope, to be made up of alternating layers of different
silicates; e.g., a microscopic layer of an aluminum-calcium silicate may be
overlain by a microscopic layer of an aluminum-sodium silicate, and the
alternation may be repeated throughout the crystal, giving it a banded
structure. There is reason to believe that this is true in many cases where the
microscope fails to detect it, and that less symmetrical comminglings of
silicates may take place. As such alternations or mixtures are not governed
by any known mathematical law, as is the case in chemical compounds,
there is no determinate limit to the number of combinations that may arise.
As a matter of fact, new ones are still being discovered in the progress of
research, and the total number that may ultimately be found can scarcely be
prophesied.
As a result of all this fertility of combination, the total number of
silicious minerals in igneous rocks is large. It is the function of the
mineralogist to treat of these minerals as such. The geologist deals with
them as constituents of the earth and as factors in its history. Only a few of
them are so abundant as to require special individual notice in a general
study of the earth. It may be remarked also that only a few of them can be
identified by simple inspection as they occur in the rocks, partly because of
the delicacy of the distinctions between many of them, and partly because
of their minuteness and intricate intermixture. The resources of the
polarizing microscope are necessary for safe determination in most cases.
The student need not feel embarrassment or discouragement if he is often
unable to recognize the constituents of the intimately crystalline rocks.
Their determination has grown to be a profession by itself.
The leading minerals of igneous rocks.—Fortunately for the simplicity
of geological study, a few minerals make up the great mass of the igneous
rocks. These few are quartz, the feldspathic minerals, the ferromagnesian
minerals, and the iron oxides. Quartz (silica, SiO2) is the free acid already
mentioned. The feldspathic and ferromagnesian minerals are the leading
silicates of the earth’s crust, and vastly surpass all others in abundance. The
case would still remain measurably simple if these chemical compounds
always crystallized out by themselves, each compound forming one
mineral, and but one; but the different silicates have the confusing habit of
crystallizing together in the same mineral. A crystal may thus sometimes be
seen, under the microscope, to be made up of alternating layers of different
silicates; e.g., a microscopic layer of an aluminum-calcium silicate may be
overlain by a microscopic layer of an aluminum-sodium silicate, and the
alternation may be repeated throughout the crystal, giving it a banded
structure. There is reason to believe that this is true in many cases where the
microscope fails to detect it, and that less symmetrical comminglings of
silicates may take place. As such alternations or mixtures are not governed
by any known mathematical law, as is the case in chemical compounds,
there is no determinate limit to the number of combinations that may arise.
As a matter of fact, new ones are still being discovered in the progress of
research, and the total number that may ultimately be found can scarcely be
prophesied.
As a result of all this fertility of combination, the total number of
silicious minerals in igneous rocks is large. It is the function of the
mineralogist to treat of these minerals as such. The geologist deals with
them as constituents of the earth and as factors in its history. Only a few of
them are so abundant as to require special individual notice in a general
study of the earth. It may be remarked also that only a few of them can be
identified by simple inspection as they occur in the rocks, partly because of
the delicacy of the distinctions between many of them, and partly because
of their minuteness and intricate intermixture. The resources of the
polarizing microscope are necessary for safe determination in most cases.
The student need not feel embarrassment or discouragement if he is often
unable to recognize the constituents of the intimately crystalline rocks.
Their determination has grown to be a profession by itself.
The leading minerals of igneous rocks.—Fortunately for the simplicity
of geological study, a few minerals make up the great mass of the igneous
rocks. These few are quartz, the feldspathic minerals, the ferromagnesian
minerals, and the iron oxides. Quartz (silica, SiO2) is the free acid already
mentioned. The feldspathic and ferromagnesian minerals are the leading
silicates of the earth’s crust, and vastly surpass all others in abundance. The
Page 475
feldspathic group embraces minerals formed by silica in union with
alumina, together with either potash, soda, or lime, or two or more of these
together. The ferromagnesian group embraces minerals formed by the union
of silica with iron, magnesia, and lime, together with more or less of the
other basic oxides. These statements are only true in a very general sense.
Admixtures, replacements, and impurities are so frequent as to break down
all sharp, simple definitions. The feldspathic minerals are normally light in
color, ranging from white to red or gray. The ferromagnesian minerals are
normally dark (commonly greenish) from the presence of iron, the great
coloring element of rocks. But these color distinctions do not hold good in
detail and cannot be much trusted as a means of identification.
The feldspathic minerals (p. 462) embrace the potash feldspars,
orthoclase and microcline; the soda feldspar, albite; the lime feldspar,
anorthite; and the mixed feldspars intermediate between albite and
anorthite, viz., the soda-lime feldspar, oligoclase, the lime-soda feldspar,
andesine, in which lime and soda are nearly equal, and the lime-soda
feldspar, labradorite, in which the lime predominates; together with leucite,
a potash silicate higher in alkali than orthoclase, and nephelite, a soda
silicate higher in soda than albite. Leucite and nephelite are usually
classified as feldspathoids, not as feldspars. It is to be understood that
alumina is normally present in all these. Additional details respecting these
minerals may be found in the reference list, p. 460.
Among the ferromagnesian minerals the most important are the
pyroxenes, the amphiboles, and the biotite type of mica. Olivine is of
subordinate importance. The pyroxenes (p. 465) and amphiboles (p. 460)
have nearly the same chemical composition, but differ in crystallization and
physical properties. Hornblende (an amphibole) has been melted, and on
cooling under proper conditions found to take on the form of augite (a
pyroxene). Pyroxene is sometimes altered into uralite, one of the
amphiboles. The pyroxenes and amphiboles are the most abundant of the
dark minerals in crystalline rocks. The leading members of the pyroxene
group are augite, diallage, hypersthene, enstatite, and soda pyroxene. The
chief members of the amphibole group are hornblende and the soda
amphiboles. All are essentially silicates of magnesia and iron oxide, with or
without the addition of lime, soda, and alumina. Details respecting these
may be found in the reference list.
alumina, together with either potash, soda, or lime, or two or more of these
together. The ferromagnesian group embraces minerals formed by the union
of silica with iron, magnesia, and lime, together with more or less of the
other basic oxides. These statements are only true in a very general sense.
Admixtures, replacements, and impurities are so frequent as to break down
all sharp, simple definitions. The feldspathic minerals are normally light in
color, ranging from white to red or gray. The ferromagnesian minerals are
normally dark (commonly greenish) from the presence of iron, the great
coloring element of rocks. But these color distinctions do not hold good in
detail and cannot be much trusted as a means of identification.
The feldspathic minerals (p. 462) embrace the potash feldspars,
orthoclase and microcline; the soda feldspar, albite; the lime feldspar,
anorthite; and the mixed feldspars intermediate between albite and
anorthite, viz., the soda-lime feldspar, oligoclase, the lime-soda feldspar,
andesine, in which lime and soda are nearly equal, and the lime-soda
feldspar, labradorite, in which the lime predominates; together with leucite,
a potash silicate higher in alkali than orthoclase, and nephelite, a soda
silicate higher in soda than albite. Leucite and nephelite are usually
classified as feldspathoids, not as feldspars. It is to be understood that
alumina is normally present in all these. Additional details respecting these
minerals may be found in the reference list, p. 460.
Among the ferromagnesian minerals the most important are the
pyroxenes, the amphiboles, and the biotite type of mica. Olivine is of
subordinate importance. The pyroxenes (p. 465) and amphiboles (p. 460)
have nearly the same chemical composition, but differ in crystallization and
physical properties. Hornblende (an amphibole) has been melted, and on
cooling under proper conditions found to take on the form of augite (a
pyroxene). Pyroxene is sometimes altered into uralite, one of the
amphiboles. The pyroxenes and amphiboles are the most abundant of the
dark minerals in crystalline rocks. The leading members of the pyroxene
group are augite, diallage, hypersthene, enstatite, and soda pyroxene. The
chief members of the amphibole group are hornblende and the soda
amphiboles. All are essentially silicates of magnesia and iron oxide, with or
without the addition of lime, soda, and alumina. Details respecting these
may be found in the reference list.
Page 476
The two leading micas are the iron-magnesia mica, biotite, and the
potash mica, muscovite, the familiar “isinglass” of the stove-door.
Chemically, muscovite should go with the potash feldspars, but it is
distinguished from them by its crystalline habit and physical properties. The
biotite should go chemically with the pyroxenes and amphiboles, which it
closely resembles except in its crystalline properties. Details respecting the
micas may be found in the reference list, p. 464.
Two iron oxides, magnetite (Fe3O4) and hematite (Fe2O3) are widely
disseminated in igneous rocks. They constitute the free bases already
mentioned.
Summary of salient facts.—The salient facts are, therefore, (1) that out
of the seventy-odd chemical elements in the earth, eight form the chief part
of it; (2) that one of these elements uniting with the rest forms nine leading
oxides; (3) that one of these oxides acts as an acid and the rest as bases; (4)
that by their combination they form a series of silicates of which a few are
easily chief; (5) that these silicates crystallize into a multitude of minerals
of which again a few are chief; and (6) that these minerals are aggregated in
various ways to form rocks. Possessed of these leading ideas, we are
prepared to turn to the consideration of some of the conditions under which
these combinations take place in the formation of rocks from molten
magmas.
THE NATURE OF MOLTEN MAGMAS.
We easily fall into the habit of thinking of molten rock as we think of a
molten metal, merely as a substance which has passed from the solid to the
liquid condition because of high temperature. With the return of low
temperature a molten metal returns to the solid state usually in the same
molecular condition which it possessed before. The point of fusion and the
point of solidification are the same and are rigidly fixed. If this were true of
the constituents of a rock, a definite order for the solidification of the
several minerals might be anticipated. As a matter of fact, the order is not
the same under all conditions, and, what is especially significant, the order
is far from being that in which the constituents would fuse or would solidify
separately. For instance, in a granite composed chiefly of quartz, feldspar,
and mica, the quartz is often the last to take form, although it is more
potash mica, muscovite, the familiar “isinglass” of the stove-door.
Chemically, muscovite should go with the potash feldspars, but it is
distinguished from them by its crystalline habit and physical properties. The
biotite should go chemically with the pyroxenes and amphiboles, which it
closely resembles except in its crystalline properties. Details respecting the
micas may be found in the reference list, p. 464.
Two iron oxides, magnetite (Fe3O4) and hematite (Fe2O3) are widely
disseminated in igneous rocks. They constitute the free bases already
mentioned.
Summary of salient facts.—The salient facts are, therefore, (1) that out
of the seventy-odd chemical elements in the earth, eight form the chief part
of it; (2) that one of these elements uniting with the rest forms nine leading
oxides; (3) that one of these oxides acts as an acid and the rest as bases; (4)
that by their combination they form a series of silicates of which a few are
easily chief; (5) that these silicates crystallize into a multitude of minerals
of which again a few are chief; and (6) that these minerals are aggregated in
various ways to form rocks. Possessed of these leading ideas, we are
prepared to turn to the consideration of some of the conditions under which
these combinations take place in the formation of rocks from molten
magmas.
THE NATURE OF MOLTEN MAGMAS.
We easily fall into the habit of thinking of molten rock as we think of a
molten metal, merely as a substance which has passed from the solid to the
liquid condition because of high temperature. With the return of low
temperature a molten metal returns to the solid state usually in the same
molecular condition which it possessed before. The point of fusion and the
point of solidification are the same and are rigidly fixed. If this were true of
the constituents of a rock, a definite order for the solidification of the
several minerals might be anticipated. As a matter of fact, the order is not
the same under all conditions, and, what is especially significant, the order
is far from being that in which the constituents would fuse or would solidify
separately. For instance, in a granite composed chiefly of quartz, feldspar,
and mica, the quartz is often the last to take form, although it is more
Page 477
infusible than the feldspar or the mica. This and other phenomena show that
a molten magma is not to be viewed simply as a fused substance, but rather
as a solution of one silicate in another, or as a solution of several silicates in
one another mutually. The high temperature is to be regarded merely as a
condition prerequisite to solution, or as the condition of fusion of some one
constituent which then dissolves the others. If crystals of snow, sugar, and
salt be mixed at a low temperature and compacted, the mass may be
regarded as an artificial rock. On raising the temperature, all will pass into
solution while the temperature is still somewhat below the melting-point of
the snow, the most fusible, and while it is much below that of either the
sugar or the salt. This particular case is instructive because the ice is not
simply fused by temperature; the affinity of the salt plays a part. If the
temperature were again lowered, the sugar and salt would not crystallize out
at their fusing-points, but would remain in solution down to and even below
the normal freezing-point of water; in other words, they would remain in
solution until the water crystallized out and forced them to take the solid
state. This holds good when the amounts of the sugar and salt are small
relative to the water. If, on the contrary, their quantity is large relatively,
crystallization will take place at higher temperatures and before the water
crystallizes to ice. From this it appears that the salt and sugar might
crystallize either before the water or after it, according to the degree of
concentration. The behavior of mixtures of minerals in passing into and out
of the molten condition appears to be quite analogous to this, and hence a
great variety of results attend the process, dependent upon the number, the
nature, and the relative quantities of the ingredients. The approved
conception of the genesis of a rock from a molten magma (when ample time
is given) is that one compound after another crystallizes out as the
temperature falls and its point of saturation for each is reached, until the
whole has been solidified. The modes of combination of the elements in the
molten magma are not necessarily the same as those in the derivative
crystals; indeed, the combinations doubtless change as the process
proceeds; certain constituents being taken out, the remaining ones probably
rearrange themselves.
Time required in crystallization.—The liquid magma of igneous rocks
is essentially a fluid glass or slag. It is analogous to common glass, which is
a silicate of potash, soda, or other base, except that usually common glass is
relatively free from iron and other coloring substances, while these abound
a molten magma is not to be viewed simply as a fused substance, but rather
as a solution of one silicate in another, or as a solution of several silicates in
one another mutually. The high temperature is to be regarded merely as a
condition prerequisite to solution, or as the condition of fusion of some one
constituent which then dissolves the others. If crystals of snow, sugar, and
salt be mixed at a low temperature and compacted, the mass may be
regarded as an artificial rock. On raising the temperature, all will pass into
solution while the temperature is still somewhat below the melting-point of
the snow, the most fusible, and while it is much below that of either the
sugar or the salt. This particular case is instructive because the ice is not
simply fused by temperature; the affinity of the salt plays a part. If the
temperature were again lowered, the sugar and salt would not crystallize out
at their fusing-points, but would remain in solution down to and even below
the normal freezing-point of water; in other words, they would remain in
solution until the water crystallized out and forced them to take the solid
state. This holds good when the amounts of the sugar and salt are small
relative to the water. If, on the contrary, their quantity is large relatively,
crystallization will take place at higher temperatures and before the water
crystallizes to ice. From this it appears that the salt and sugar might
crystallize either before the water or after it, according to the degree of
concentration. The behavior of mixtures of minerals in passing into and out
of the molten condition appears to be quite analogous to this, and hence a
great variety of results attend the process, dependent upon the number, the
nature, and the relative quantities of the ingredients. The approved
conception of the genesis of a rock from a molten magma (when ample time
is given) is that one compound after another crystallizes out as the
temperature falls and its point of saturation for each is reached, until the
whole has been solidified. The modes of combination of the elements in the
molten magma are not necessarily the same as those in the derivative
crystals; indeed, the combinations doubtless change as the process
proceeds; certain constituents being taken out, the remaining ones probably
rearrange themselves.
Time required in crystallization.—The liquid magma of igneous rocks
is essentially a fluid glass or slag. It is analogous to common glass, which is
a silicate of potash, soda, or other base, except that usually common glass is
relatively free from iron and other coloring substances, while these abound
Page 478
in the natural magmas and render them dark and more or less opaque; but
the fundamental nature is the same, except that the natural lavas are usually
mixtures of several silicates, while the artificial glasses consist of only one,
or at most a few. Furnace slag is essentially an artificial lava.
When a lava is cooled quickly, the commingled silicates solidify in the
diffused condition essentially as they were in the liquid; for there is no time
for the silicate molecules of a like kind to come together, particle by
particle, in regular systematic order, as required in crystallization. The
essential feature of crystallization is this systematic arrangement of the
molecules according to a definite plan, giving a specific crystal form, as a
cube, a hexagonal prism, etc.
There are six (sometimes made seven) fundamental systems of
crystallization, and a multitude of variations of special form in each system.
The treatment of these forms belongs to mineralogy.
In a thick viscid liquid, this systematic arrangement of molecules into
definite crystal forms takes place slowly, for the crystalline force in the
silicates is far less energetic than that in water, which crystallizes into ice
with much rapidity and with great force. Because of this slowness, the
solidification of the lava may catch the process of crystallization at any
stage. If the lava is cooled quickly, the result is a glass; if less quickly, part
glass and part crystals; if slowly enough, all becomes crystalline. In general
the slower the growth the larger the crystals. The solidification product may,
therefore, range from a glass to a mass of crystals; i.e., it may be (1) wholly
glass, (2) a glassy matrix with a few small crystals scattered through it, (3) a
less abundant glassy matrix with more and larger crystals, (4) a mere
remnant of glass in a mass of crystals, or (5) a mass of crystals with no
glass.
Successive stages of crystallization.—Since eruptions take place
intermittently, it is obvious that cooling of the lava may be in progress in its
hidden reservoir during the quiescent intervals between eruptions. After a
certain stage of partial crystallization has been reached during such time of
quiet, a renewal of eruption may take place and the whole mass of lava be
shifted into quite new conditions, and a second phase of solidification may
be superposed on the one already started. The rock will then show two
phases of crystallization: (1) large crystals of the kind or kinds most prone
the fundamental nature is the same, except that the natural lavas are usually
mixtures of several silicates, while the artificial glasses consist of only one,
or at most a few. Furnace slag is essentially an artificial lava.
When a lava is cooled quickly, the commingled silicates solidify in the
diffused condition essentially as they were in the liquid; for there is no time
for the silicate molecules of a like kind to come together, particle by
particle, in regular systematic order, as required in crystallization. The
essential feature of crystallization is this systematic arrangement of the
molecules according to a definite plan, giving a specific crystal form, as a
cube, a hexagonal prism, etc.
There are six (sometimes made seven) fundamental systems of
crystallization, and a multitude of variations of special form in each system.
The treatment of these forms belongs to mineralogy.
In a thick viscid liquid, this systematic arrangement of molecules into
definite crystal forms takes place slowly, for the crystalline force in the
silicates is far less energetic than that in water, which crystallizes into ice
with much rapidity and with great force. Because of this slowness, the
solidification of the lava may catch the process of crystallization at any
stage. If the lava is cooled quickly, the result is a glass; if less quickly, part
glass and part crystals; if slowly enough, all becomes crystalline. In general
the slower the growth the larger the crystals. The solidification product may,
therefore, range from a glass to a mass of crystals; i.e., it may be (1) wholly
glass, (2) a glassy matrix with a few small crystals scattered through it, (3) a
less abundant glassy matrix with more and larger crystals, (4) a mere
remnant of glass in a mass of crystals, or (5) a mass of crystals with no
glass.
Successive stages of crystallization.—Since eruptions take place
intermittently, it is obvious that cooling of the lava may be in progress in its
hidden reservoir during the quiescent intervals between eruptions. After a
certain stage of partial crystallization has been reached during such time of
quiet, a renewal of eruption may take place and the whole mass of lava be
shifted into quite new conditions, and a second phase of solidification may
be superposed on the one already started. The rock will then show two
phases of crystallization: (1) large crystals of the kind or kinds most prone
Page 479
to develop in the given lava may have grown during the first long stage of
slow subterranean cooling, while the greater part of the lava still remained
liquid; and (2) small crystals or glass may have developed when the more
rapid cooling under the new conditions took place. The result would be
large crystals set in a matrix of small crystals or of glass, a combination
styled porphyritic. In such cases the lava, in its later stages, carries the large
crystals floating throughout its mass, and is not a simple liquid.
THE FRAGMENTAL PRODUCTS OF SUDDEN COOLING.
Pyroclastic rocks.—The extreme example of sudden cooling is
presented when lavas are violently exploded into the air and solidify almost
instantly. The resulting glassy particles or filaments, if small, constitute
volcanic ash. The explosion appears to be due to steam and other gases
which are held in the deeper lava under great pressure, but which, as they
rise toward the surface of the lava where the pressure is relieved, expand
with explosive violence. It is probably also due in part to progressive
crystallization, which forces the gases out from the part that crystallizes and
overcharges the rest. Sometimes the projected particles draw after
themselves long filaments like the threads of spun glass, and sometimes
while in the air they divide and draw apart, spinning a filament of viscid
lava between them. A variety of this kind at the volcano of Kilauea in
Hawaii is known as “Pele’s hair.” These light filaments drift with the wind
and lodge on the lee side of the volcano, covering the surface “like mown
grass” (Dana).
slow subterranean cooling, while the greater part of the lava still remained
liquid; and (2) small crystals or glass may have developed when the more
rapid cooling under the new conditions took place. The result would be
large crystals set in a matrix of small crystals or of glass, a combination
styled porphyritic. In such cases the lava, in its later stages, carries the large
crystals floating throughout its mass, and is not a simple liquid.
THE FRAGMENTAL PRODUCTS OF SUDDEN COOLING.
Pyroclastic rocks.—The extreme example of sudden cooling is
presented when lavas are violently exploded into the air and solidify almost
instantly. The resulting glassy particles or filaments, if small, constitute
volcanic ash. The explosion appears to be due to steam and other gases
which are held in the deeper lava under great pressure, but which, as they
rise toward the surface of the lava where the pressure is relieved, expand
with explosive violence. It is probably also due in part to progressive
crystallization, which forces the gases out from the part that crystallizes and
overcharges the rest. Sometimes the projected particles draw after
themselves long filaments like the threads of spun glass, and sometimes
while in the air they divide and draw apart, spinning a filament of viscid
lava between them. A variety of this kind at the volcano of Kilauea in
Hawaii is known as “Pele’s hair.” These light filaments drift with the wind
and lodge on the lee side of the volcano, covering the surface “like mown
grass” (Dana).
Page 480
Fig. 336.—Volcanic bomb. About half natural size. (Photo. by Church.)
When the exploded fragments are coarser they fall about the volcanic
vent and form the tuffs (tufa) of which most steep volcanic cones are chiefly
built. In these larger fragments, crystals are not infrequently found, and the
same is even true of the volcanic ash. These crystals are undoubtedly such
as had already been formed in the lava before it exploded, and their
formation, as suggested above, may have contributed to the explosion.
Fragments too large to be borne far away by the air, but still small, are
known as lapilli, especially if they are somewhat rounded and gravel-like. A
finer variety, of the nature of sand, much used in making Portland cement,
is locally known as puzzolana.
When the exploded fragments are coarser they fall about the volcanic
vent and form the tuffs (tufa) of which most steep volcanic cones are chiefly
built. In these larger fragments, crystals are not infrequently found, and the
same is even true of the volcanic ash. These crystals are undoubtedly such
as had already been formed in the lava before it exploded, and their
formation, as suggested above, may have contributed to the explosion.
Fragments too large to be borne far away by the air, but still small, are
known as lapilli, especially if they are somewhat rounded and gravel-like. A
finer variety, of the nature of sand, much used in making Portland cement,
is locally known as puzzolana.
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Fig. 337.—Volcanic bomb of unusual form, 13 foot Long. Cinder Buttes, Idaho. (Russell,
U. S. Geol. Surv.)
The rougher, irregular fragments of a clinker-like nature ejected by
volcanoes are known as scoriæ or cinders. They are more or less distended
by gas-bubbles and are hence light and pumiceous.
The larger masses of lava ejected into the air are often caused to rotate by
the unequal force of the projection, or by the unequal friction of the air, and
to assume spheroidal forms, the internal gases at the same time often
expanding and rendering the mass vesicular. These rounded projectiles are
known as volcanic bombs (Figs. 336 and 337). Balls of lava that have
originated in rolling movements of the seething mass, or in other ways, are
also styled bombs. Usage is not altogether harmonious or consistent in the
application of the term.
The larger masses that are projected into the air are more or less vesicular
from the expansion of included gases, as already noted, and so the
fragmental products of volcanic action grade into the vesicular. The type of
this class is pumice, in which the gas cavities make up by far the larger part
U. S. Geol. Surv.)
The rougher, irregular fragments of a clinker-like nature ejected by
volcanoes are known as scoriæ or cinders. They are more or less distended
by gas-bubbles and are hence light and pumiceous.
The larger masses of lava ejected into the air are often caused to rotate by
the unequal force of the projection, or by the unequal friction of the air, and
to assume spheroidal forms, the internal gases at the same time often
expanding and rendering the mass vesicular. These rounded projectiles are
known as volcanic bombs (Figs. 336 and 337). Balls of lava that have
originated in rolling movements of the seething mass, or in other ways, are
also styled bombs. Usage is not altogether harmonious or consistent in the
application of the term.
The larger masses that are projected into the air are more or less vesicular
from the expansion of included gases, as already noted, and so the
fragmental products of volcanic action grade into the vesicular. The type of
this class is pumice, in which the gas cavities make up by far the larger part
Page 482
of the volume of the whole mass, and the whole is reduced to the condition
of a solidified froth or foam. So thin are the dividing films of glassy
material in some cases that the whole is pure white, though the same
material in solid mass would be dark. This solidified glassy froth is often
lighter than water and floats freely on the sea until it becomes “water-
logged” and sinks. Dredgings of the deep sea show that much pumice has
accumulated there, and being far from the land has escaped burial by the
sediments borne in by the rivers.
All of these fragmental rocks produced by volcanic action are known as
pyroclastic (fire-fragmented) rocks, a general term of much convenience in
distinguishing them from lava-flows, on the one hand, and from the
fragmental rocks produced by air and water (ordinary clastics), on the other.
THE GLASSY ROCKS.
The solid glasses.—The quick cooling of lava-flows into solid glasses is
chiefly dependent on their exposure at the surface. Hence it is often the case
that the exterior of a lava-flow is glassy in greater or lesser degree, while
the interior is more or less crystalline. Quick cooling is sometimes also due
to the intrusion of the lava in thin sheets into fissures in cold rocks. When
massive bodies of lavas penetrate solid rocks, the lava does not usually cool
so fast as to prevent some degree of crystallization, and the crystallization
may even become complete; but if the intruded lava sheet be very thin, the
lava is liable to be cooled to a nearly perfect glass. The glassy condition is,
therefore, subject to indefinite gradations. As a rule, the acid lavas are
stiffer at the same temperature than the basic ones, and crystallize more
slowly, so that acid glasses are more common than basic ones. The basic
rocks usually crystallize pretty thoroughly, except on the immediate surface
of the flows.
The first stages of crystallization.—The microscopic study of the
volcanic glasses reveals great numbers of minute forms known as
crystallites, microlites, globulites, etc., that appear to be first steps in
crystallization, though many of them do not take definite geometrical
shapes and some do not show the optical characters of crystals. There are
minute globules (globulites), needles, and hair-like bodies (trichites) of
of a solidified froth or foam. So thin are the dividing films of glassy
material in some cases that the whole is pure white, though the same
material in solid mass would be dark. This solidified glassy froth is often
lighter than water and floats freely on the sea until it becomes “water-
logged” and sinks. Dredgings of the deep sea show that much pumice has
accumulated there, and being far from the land has escaped burial by the
sediments borne in by the rivers.
All of these fragmental rocks produced by volcanic action are known as
pyroclastic (fire-fragmented) rocks, a general term of much convenience in
distinguishing them from lava-flows, on the one hand, and from the
fragmental rocks produced by air and water (ordinary clastics), on the other.
THE GLASSY ROCKS.
The solid glasses.—The quick cooling of lava-flows into solid glasses is
chiefly dependent on their exposure at the surface. Hence it is often the case
that the exterior of a lava-flow is glassy in greater or lesser degree, while
the interior is more or less crystalline. Quick cooling is sometimes also due
to the intrusion of the lava in thin sheets into fissures in cold rocks. When
massive bodies of lavas penetrate solid rocks, the lava does not usually cool
so fast as to prevent some degree of crystallization, and the crystallization
may even become complete; but if the intruded lava sheet be very thin, the
lava is liable to be cooled to a nearly perfect glass. The glassy condition is,
therefore, subject to indefinite gradations. As a rule, the acid lavas are
stiffer at the same temperature than the basic ones, and crystallize more
slowly, so that acid glasses are more common than basic ones. The basic
rocks usually crystallize pretty thoroughly, except on the immediate surface
of the flows.
The first stages of crystallization.—The microscopic study of the
volcanic glasses reveals great numbers of minute forms known as
crystallites, microlites, globulites, etc., that appear to be first steps in
crystallization, though many of them do not take definite geometrical
shapes and some do not show the optical characters of crystals. There are
minute globules (globulites), needles, and hair-like bodies (trichites) of
Page 483
more or less indeterminate nature, together with other forms that can be
seen to be certainly the initial forms of well-known minerals.
Fig. 338.—Flow structure in rhyolite. Nearly natural size. (Photo. by Church.)
The obsidians.—Of the compact glassy rocks, obsidian is the best type.
It is essentially a natural glass, formed usually of acid silicates. It has the
close texture, conchoidal fracture, and other qualities of glass. It is usually
black, but sometimes red, brown, purple, bluish, or gray. While chiefly of
glass, it usually contains more or less of the incipient crystals above
described, showing that even here the first step in the gradation to the next
or the crystalline stage has been taken. These incipient crystals sometimes
become so abundant as to change the texture from the vitreous to the stony
order. In some cases, the stony texture seems to have been developed in the
obsidian after it was formed, the change being a part of a subsequent
seen to be certainly the initial forms of well-known minerals.
Fig. 338.—Flow structure in rhyolite. Nearly natural size. (Photo. by Church.)
The obsidians.—Of the compact glassy rocks, obsidian is the best type.
It is essentially a natural glass, formed usually of acid silicates. It has the
close texture, conchoidal fracture, and other qualities of glass. It is usually
black, but sometimes red, brown, purple, bluish, or gray. While chiefly of
glass, it usually contains more or less of the incipient crystals above
described, showing that even here the first step in the gradation to the next
or the crystalline stage has been taken. These incipient crystals sometimes
become so abundant as to change the texture from the vitreous to the stony
order. In some cases, the stony texture seems to have been developed in the
obsidian after it was formed, the change being a part of a subsequent
Page 484
process of devitrification, but in other cases the crystals seem to be original.
Besides these, there are often small globular bodies known as spherulites.
Varieties of glassy rock in which the embryo crystals are more numerous
and the glassy texture less perfect, are known as pitchstones. The fresh
surfaces of these have rather the aspect of pitch or resin than that of true
glass; hence their name. Like the obsidians, they are usually dark, but they
take on greenish, brownish, yellowish, and light-colored hues as well.
Sometimes glassy rock fractures in small spheroidal forms like pearls, and
is known as perlite. Basic glasses are relatively rare, and while usually
included under the term obsidian, are sometimes given special names.
Fig. 339.—Flow structure in volcanic glass. About half natural size. (Photo. by Church.)
Besides these, there are often small globular bodies known as spherulites.
Varieties of glassy rock in which the embryo crystals are more numerous
and the glassy texture less perfect, are known as pitchstones. The fresh
surfaces of these have rather the aspect of pitch or resin than that of true
glass; hence their name. Like the obsidians, they are usually dark, but they
take on greenish, brownish, yellowish, and light-colored hues as well.
Sometimes glassy rock fractures in small spheroidal forms like pearls, and
is known as perlite. Basic glasses are relatively rare, and while usually
included under the term obsidian, are sometimes given special names.
Fig. 339.—Flow structure in volcanic glass. About half natural size. (Photo. by Church.)
Page 485
Fig. 340.—Flow structure in porphyry, shown by the position of the large crystals. About
two-thirds natural size. (Photo. by Church.)
two-thirds natural size. (Photo. by Church.)
Page 486
Fig. 341.—Scoriaceous texture. About four-fifths natural size. (Photo. by Church.)
SPECIAL STRUCTURES.
Flow structure.—Lavas that cool into glassy rocks frequently contain
gas cavities, colored spots and variations of texture which, together with the
hair-like embryo crystals, are drawn out into lines, streaks, and parallel belts
by the flow of the viscous mass, giving rise to rhyolitic or flow structure
(Figs. 338 and 339). Rocks in which this is the most pronounced feature
were formerly known as rhyolites, though the term has drifted away from
this original meaning and has been applied to a class of acidic rocks. The
obsidians and pitchstones may be more or less rhyolitic under the
microscope, though to the naked eye they may appear only as a glassy or
resinous mass. The rhyolites generally have but an imperfect glassy texture,
since the crystals and the cavities sometimes make up a notable part of the
mass, the glassy portion being scarcely more than a matrix in which the
SPECIAL STRUCTURES.
Flow structure.—Lavas that cool into glassy rocks frequently contain
gas cavities, colored spots and variations of texture which, together with the
hair-like embryo crystals, are drawn out into lines, streaks, and parallel belts
by the flow of the viscous mass, giving rise to rhyolitic or flow structure
(Figs. 338 and 339). Rocks in which this is the most pronounced feature
were formerly known as rhyolites, though the term has drifted away from
this original meaning and has been applied to a class of acidic rocks. The
obsidians and pitchstones may be more or less rhyolitic under the
microscope, though to the naked eye they may appear only as a glassy or
resinous mass. The rhyolites generally have but an imperfect glassy texture,
since the crystals and the cavities sometimes make up a notable part of the
mass, the glassy portion being scarcely more than a matrix in which the
Page 487
crystals, spherulites, and cavities are carried. By an increase of the crystals
in number and size, the rock passes by gradations into porphyry or
phanerite.
Fig. 342.—Porphyritic texture. Two-thirds natural size. (Photo. by Church.)
Amygdaloids.—In lava-flows the included steam often collects in
bubbles near the surface as the lava cools and forms a vesicular portion with
a scoriaceous texture (Fig. 341). In its upper part, the vapor bubbles may be
numerous, while below they become more and more scattered until they
disappear. Similar bubbles are also often found near the bottom of a sheet of
lava. This is perhaps due to the rolling under of the frontal surface of the
lava-stream as it flows. Later, these cavities often become filled with
minerals deposited from solution and the rock then becomes an amygdaloid,
but this filling is a secondary action.
in number and size, the rock passes by gradations into porphyry or
phanerite.
Fig. 342.—Porphyritic texture. Two-thirds natural size. (Photo. by Church.)
Amygdaloids.—In lava-flows the included steam often collects in
bubbles near the surface as the lava cools and forms a vesicular portion with
a scoriaceous texture (Fig. 341). In its upper part, the vapor bubbles may be
numerous, while below they become more and more scattered until they
disappear. Similar bubbles are also often found near the bottom of a sheet of
lava. This is perhaps due to the rolling under of the frontal surface of the
lava-stream as it flows. Later, these cavities often become filled with
minerals deposited from solution and the rock then becomes an amygdaloid,
but this filling is a secondary action.
Page 488
Fig. 343.—Porphyritic texture. Natural size. (Photo. by Church.)
THE PORPHYRITIC ROCKS.
When the conditions are such that after a part of the magma has formed
distinct crystals floating in the remaining liquid lava, there is a change
which causes the rest to solidify as a glass or as a mass of small crystals, the
structure is known as porphyritic, and the rocks possessing it are called
porphyries. This differentiation into distinct crystals set in a ground-mass of
minute crystals or of glass often gives a mottled or variegated aspect to the
rock, especially if the matrix of glass or minute crystals differs in color
from the distinct crystals. This structure is much oftener developed in acidic
rocks than in basic ones, because the latter crystallize more readily. The
most common porphyritic crystals are feldspar and quartz, though they are
by no means the only ones. The matrix is also usually felsitic or quartzose,
but not necessarily so. The character is a structural one, and is not
THE PORPHYRITIC ROCKS.
When the conditions are such that after a part of the magma has formed
distinct crystals floating in the remaining liquid lava, there is a change
which causes the rest to solidify as a glass or as a mass of small crystals, the
structure is known as porphyritic, and the rocks possessing it are called
porphyries. This differentiation into distinct crystals set in a ground-mass of
minute crystals or of glass often gives a mottled or variegated aspect to the
rock, especially if the matrix of glass or minute crystals differs in color
from the distinct crystals. This structure is much oftener developed in acidic
rocks than in basic ones, because the latter crystallize more readily. The
most common porphyritic crystals are feldspar and quartz, though they are
by no means the only ones. The matrix is also usually felsitic or quartzose,
but not necessarily so. The character is a structural one, and is not
Page 489
dependent upon any special chemical or mineralogical constitution. The
distinct crystals are known as phenocrysts, and the varieties of porphyries
are named from the characteristic phenocryst, e.g., quartzophyre (quartz-
porphyry) if the conspicuous crystals are quartz, orthophyre if orthoclase,
augitophyre if augite, etc. A convenient classification has recently been
proposed[200] into (1) leucophyre (white porphyries), which have a light-
colored ground-mass set with phenocrysts of any kind, and (2) melaphyres
(black porphyries), which have a dark-colored ground-mass, with
phenocrysts of any kind. While it is to be hoped this usage will prevail, it is
to be noted that these terms, especially the latter, have been used in a
different sense. (See reference list of rocks, p. 445.)
In many cases the ground-mass itself becomes minutely crystalline and
the porphyritic aspect is due simply to large distinct crystals set in a mass of
minute obscure ones. The rock is then really holocrystalline, but the term
porphyry is applied to it. In other rocks the crystals of the ground-mass
become more and more distinct, the porphyritic aspect gradually disappears,
and there is a graduation into the next class.
THE PHANEROCRYSTALLINE ROCKS.
The phanerites.—When time enough is given for the cooling process the
molten magma becomes completely crystalline. The holocrystalline rocks
hence include a large series, ranging from the most acid to the most basic.
In this class the differentiation of the rock material and the formation of
distinct minerals reach a high stage, and as a natural result the varieties of
rock are numerous. Taken as a group they are phanerites. If they are to be
more particularly characterized, it is usually done on the basis of the
minerals of which they are composed. The following are the leading types,
beginning with those which are rich in silica and poor in basic oxides, and
ending with those which are rich in basic oxides and poor in silica.
distinct crystals are known as phenocrysts, and the varieties of porphyries
are named from the characteristic phenocryst, e.g., quartzophyre (quartz-
porphyry) if the conspicuous crystals are quartz, orthophyre if orthoclase,
augitophyre if augite, etc. A convenient classification has recently been
proposed[200] into (1) leucophyre (white porphyries), which have a light-
colored ground-mass set with phenocrysts of any kind, and (2) melaphyres
(black porphyries), which have a dark-colored ground-mass, with
phenocrysts of any kind. While it is to be hoped this usage will prevail, it is
to be noted that these terms, especially the latter, have been used in a
different sense. (See reference list of rocks, p. 445.)
In many cases the ground-mass itself becomes minutely crystalline and
the porphyritic aspect is due simply to large distinct crystals set in a mass of
minute obscure ones. The rock is then really holocrystalline, but the term
porphyry is applied to it. In other rocks the crystals of the ground-mass
become more and more distinct, the porphyritic aspect gradually disappears,
and there is a graduation into the next class.
THE PHANEROCRYSTALLINE ROCKS.
The phanerites.—When time enough is given for the cooling process the
molten magma becomes completely crystalline. The holocrystalline rocks
hence include a large series, ranging from the most acid to the most basic.
In this class the differentiation of the rock material and the formation of
distinct minerals reach a high stage, and as a natural result the varieties of
rock are numerous. Taken as a group they are phanerites. If they are to be
more particularly characterized, it is usually done on the basis of the
minerals of which they are composed. The following are the leading types,
beginning with those which are rich in silica and poor in basic oxides, and
ending with those which are rich in basic oxides and poor in silica.
Page 490
Fig. 344.—Granitic texture. About half natural size. (Photo. by Church.)
The granites.—The term granite was originally used to designate a
granular, i.e., a distinctly crystalline, rock, and it is still popularly and
properly so used. In scientific treatises it has usually been confined to a
special aggregate of crystals of quartz, feldspar, and mica. It has recently
been proposed to give it again a more general application, though not quite
its original one, by including under it all holocrystalline rocks composed of
dominant quartz and feldspar of any kind, with mica, hornblende, or other
minerals in subordinate amount. In scientific literature as it now stands,
granite consists of quartz, feldspar, and mica, the feldspar being of the
alkali-potash or soda variety (orthoclase, microcline, or albite), and the
mica, either muscovite or biotite. In the type form the crystals are distinct
and sometimes large (Fig. 344). They are intimately mingled with one
another, and in growing, interfered more or less with each other and so
The granites.—The term granite was originally used to designate a
granular, i.e., a distinctly crystalline, rock, and it is still popularly and
properly so used. In scientific treatises it has usually been confined to a
special aggregate of crystals of quartz, feldspar, and mica. It has recently
been proposed to give it again a more general application, though not quite
its original one, by including under it all holocrystalline rocks composed of
dominant quartz and feldspar of any kind, with mica, hornblende, or other
minerals in subordinate amount. In scientific literature as it now stands,
granite consists of quartz, feldspar, and mica, the feldspar being of the
alkali-potash or soda variety (orthoclase, microcline, or albite), and the
mica, either muscovite or biotite. In the type form the crystals are distinct
and sometimes large (Fig. 344). They are intimately mingled with one
another, and in growing, interfered more or less with each other and so
Page 491
became interlocked. The granites are among the most common and easily
recognized of the holocrystalline rocks. Their color is mainly dependent
upon the feldspar, the red and pink varieties of the mineral giving rise to red
granite, and the white varieties to gray granite.
Fig. 345.—Graphic granitic (or pegmatitic) texture. Nearly natural size. (Photo. by
Church.)
Very few granites conform strictly to the type. They vary by the addition
and substitution of other minerals, and these sometimes become as
prominent as the type minerals. The soda-lime feldspars sometimes take the
place of the orthoclase, or accompany it; hornblende and other minerals
take the place of the biotite, or occur with it; and so on. Whenever one of
these replacing or accessory minerals is notable in quantity, its name is
recognized of the holocrystalline rocks. Their color is mainly dependent
upon the feldspar, the red and pink varieties of the mineral giving rise to red
granite, and the white varieties to gray granite.
Fig. 345.—Graphic granitic (or pegmatitic) texture. Nearly natural size. (Photo. by
Church.)
Very few granites conform strictly to the type. They vary by the addition
and substitution of other minerals, and these sometimes become as
prominent as the type minerals. The soda-lime feldspars sometimes take the
place of the orthoclase, or accompany it; hornblende and other minerals
take the place of the biotite, or occur with it; and so on. Whenever one of
these replacing or accessory minerals is notable in quantity, its name is
Page 492
often prefixed, as hornblende-granite, oligoclase-granite, zircon-granite, etc.
In this way the rock grades almost insensibly into the syenites, diorites, etc.
Variations also arise from the absence of one of the three leading minerals.
If mica is absent, the rock is termed an aplite (quartz and feldspar). If the
feldspar is absent, it is called a greisen (quartz and mica). If quartz is
absent, it is termed a minette (feldspar and mica). These varietal terms are
neither universally nor always consistently used, and it is to be hoped they
will be replaced by the systematic nomenclature recently proposed and
outlined later (p. 451).
The granites were formed from a magma rich in silica, alumina, potash,
and soda, but generally poor in lime, iron, and magnesia. Incidentally other
substances were present. The alumina, potash, and other bases united with
so much of the silica as was required to form the feldspars and micas, and
the remaining silica crystallized into quartz.
Granite is normally a massive rock without foliation or banding. If it
takes on these characters, it becomes a gneiss, and passes into the foliated
or schistose class of rocks, to be discussed later. The texture of graphic
granite (see pegmatite) is notably peculiar, due to the simultaneous
crystallization of the quartz and feldspar (Fig. 345).
The syenites.—When the mica of a granite is replaced by hornblende,
the rock is now commonly known as a hornblende-granite, but it was
formerly called syenite, because found at Syene on the Nile. The term
syenite is now applied to a rock consisting essentially of feldspar and
hornblende or mica, but there is a complete gradation from the granites to
the syenites. The magma of the syenites was richer in iron and magnesium
than the typical granitic magma. The syenites also grade into other classes,
as do the granites, and are named by similar prefixes, as augite-syenite, etc.,
and some of these varieties have special names. The syenites are red or
gray, according to the color of the feldspar, and are usually darker than the
granites. The texture of syenite is like that of granite. In the scheme of field
names recently proposed, syenite is made to include all holocrystalline
rocks composed mainly of feldspar of any kind, with subordinate amounts
of mica, hornblende, pyroxene, and other minerals, but without a noticeable
amount of quartz.
In this way the rock grades almost insensibly into the syenites, diorites, etc.
Variations also arise from the absence of one of the three leading minerals.
If mica is absent, the rock is termed an aplite (quartz and feldspar). If the
feldspar is absent, it is called a greisen (quartz and mica). If quartz is
absent, it is termed a minette (feldspar and mica). These varietal terms are
neither universally nor always consistently used, and it is to be hoped they
will be replaced by the systematic nomenclature recently proposed and
outlined later (p. 451).
The granites were formed from a magma rich in silica, alumina, potash,
and soda, but generally poor in lime, iron, and magnesia. Incidentally other
substances were present. The alumina, potash, and other bases united with
so much of the silica as was required to form the feldspars and micas, and
the remaining silica crystallized into quartz.
Granite is normally a massive rock without foliation or banding. If it
takes on these characters, it becomes a gneiss, and passes into the foliated
or schistose class of rocks, to be discussed later. The texture of graphic
granite (see pegmatite) is notably peculiar, due to the simultaneous
crystallization of the quartz and feldspar (Fig. 345).
The syenites.—When the mica of a granite is replaced by hornblende,
the rock is now commonly known as a hornblende-granite, but it was
formerly called syenite, because found at Syene on the Nile. The term
syenite is now applied to a rock consisting essentially of feldspar and
hornblende or mica, but there is a complete gradation from the granites to
the syenites. The magma of the syenites was richer in iron and magnesium
than the typical granitic magma. The syenites also grade into other classes,
as do the granites, and are named by similar prefixes, as augite-syenite, etc.,
and some of these varieties have special names. The syenites are red or
gray, according to the color of the feldspar, and are usually darker than the
granites. The texture of syenite is like that of granite. In the scheme of field
names recently proposed, syenite is made to include all holocrystalline
rocks composed mainly of feldspar of any kind, with subordinate amounts
of mica, hornblende, pyroxene, and other minerals, but without a noticeable
amount of quartz.
Page 493
The diorites.—These embrace rocks which were crystallized from a
magma still poorer in silica and the alkalies, and richer in the earthy bases.
In composition they closely approach the ideal average rock, but usually
fall a little below it in silica and the alkalies, and rise a little above it in the
earthy bases. In current usage, diorite is defined as an intimate mixture of
crystals of hornblende and a plagioclase feldspar. It differs from the syenite
in having plagioclase feldspar instead of orthoclase. By substitutions and
the addition of accessory minerals, the diorites graduate toward the granites
and syenites on the one hand, as already noted, and into gabbros on the
other.
In the scheme recently proposed, all holocrystalline rocks in which
hornblende is dominant and feldspar subordinate are classed as diorites.
The gabbros.—The name gabbro was formerly applied to a coarse-
grained basic rock consisting of labradorite and diallage, but the name has
been gradually extended until it embraces a large group of rocks that have
essentially the same composition as the dolerites mentioned below, but are
coarser in crystallization, and the crystals do not embrace one another (i.e.,
are not ophitic). The principal minerals are plagioclase (normally
labradorite) and pyroxene (normally diallage) with magnetite or ilmenite.
They are usually dark, heavy rocks. The pearly luster of the cleavage faces
of the diallage, when present, gives a peculiar sheen to a fresh surface of the
rock. In the recently proposed field names, gabbro is made to include all
phanerocrystalline rocks in which pyroxene predominates, attended by
feldspar of any kind in subordinate quantity, with or without hornblende or
mica.
The peridotites.—These stand at the basic end of the series, having been
formed from a magma in which the silica was low (39–45 per cent.), as
were also the alumina, lime, and alkalies, but in which the magnesia was
relatively very high, ranging from 35 to 48 per cent. The rock consists very
largely of olivine associated with pyroxene, magnetite, and other very basic
minerals. Little or no feldspar is present. The peridotites are much less
abundant than the preceding classes and represent a very distinctive phase
of the magma in which the magnesia was greatly concentrated.
Closely allied to the peridotites are rocks which are made up largely of a
single basic mineral, as augitite, pyroxenite, hornblendite, rocks essentially
magma still poorer in silica and the alkalies, and richer in the earthy bases.
In composition they closely approach the ideal average rock, but usually
fall a little below it in silica and the alkalies, and rise a little above it in the
earthy bases. In current usage, diorite is defined as an intimate mixture of
crystals of hornblende and a plagioclase feldspar. It differs from the syenite
in having plagioclase feldspar instead of orthoclase. By substitutions and
the addition of accessory minerals, the diorites graduate toward the granites
and syenites on the one hand, as already noted, and into gabbros on the
other.
In the scheme recently proposed, all holocrystalline rocks in which
hornblende is dominant and feldspar subordinate are classed as diorites.
The gabbros.—The name gabbro was formerly applied to a coarse-
grained basic rock consisting of labradorite and diallage, but the name has
been gradually extended until it embraces a large group of rocks that have
essentially the same composition as the dolerites mentioned below, but are
coarser in crystallization, and the crystals do not embrace one another (i.e.,
are not ophitic). The principal minerals are plagioclase (normally
labradorite) and pyroxene (normally diallage) with magnetite or ilmenite.
They are usually dark, heavy rocks. The pearly luster of the cleavage faces
of the diallage, when present, gives a peculiar sheen to a fresh surface of the
rock. In the recently proposed field names, gabbro is made to include all
phanerocrystalline rocks in which pyroxene predominates, attended by
feldspar of any kind in subordinate quantity, with or without hornblende or
mica.
The peridotites.—These stand at the basic end of the series, having been
formed from a magma in which the silica was low (39–45 per cent.), as
were also the alumina, lime, and alkalies, but in which the magnesia was
relatively very high, ranging from 35 to 48 per cent. The rock consists very
largely of olivine associated with pyroxene, magnetite, and other very basic
minerals. Little or no feldspar is present. The peridotites are much less
abundant than the preceding classes and represent a very distinctive phase
of the magma in which the magnesia was greatly concentrated.
Closely allied to the peridotites are rocks which are made up largely of a
single basic mineral, as augitite, pyroxenite, hornblendite, rocks essentially
Page 494
formed of the minerals augite, pyroxene, and hornblende respectively. It
will be noted that in these rocks the magma became quite simple in nature,
just as at the acid end of the series certain rocks become comparatively
simple from the concentration of the acid element, as in certain acidic
granites, felsites, etc. (See pp. 523–524.)
The basalts.—The term basalt is used in a somewhat comprehensive
way to embrace dark, compact, igneous rocks that appear to be nearly
homogeneous, owing to the minuteness of the crystals, which are usually so
small as to be identifiable only under the microscope. In some cases the
crystals are scattered throughout a ground-mass after the porphyritic
fashion. In some of these cases there is a true glassy base, and in such cases
the rock does not strictly belong in the holocrystalline group. In the more
typical cases the constituent minerals are very minutely crystallized and
intimately intermixed. The leading minerals are plagioclase (usually
labradorite or anorthite) and pyroxene (usually augite), with olivine and
magnetite or ilmenite usually present. There is a considerable range in
chemical nature, but the basalts are relatively poor in silica, usually also
low in potash and soda, but rich in lime, magnesia, and the iron oxides.
They are classed as basic and are sometimes highly so. The magmas of the
basalts are especially fluid, and when poured forth upon the surface easily
spread out in thin sheets. In cooling they are prone to take on a columnar or
basaltic structure, the columns standing at right angles to the surfaces
exposed to cooling. The columns are sometimes curved, owing to the
peculiar attitude of the cooling surface. The columns of Giant’s Causeway
and Fingal’s Cave are familiar examples.
The dolerites.—The basalts graduate insensibly into the dolerites; indeed
the dolerites may be regarded simply as basalts of coarser crystallization.
The minerals are evident to the eye and range up to medium size. The more
abundant minerals are plagioclase feldspar (labradorite or anorthite), with
one or more of the ferromagnesian minerals (augite, olivine, or biotite), and
magnetite or ilmenite. In the growth of the minerals one crystal frequently
embraces others, giving an ophitic structure. The dolerites have many
varieties, due either to accessory minerals or to the development of some of
the constituents more amply than the rest. The type may be said to consist
of plagioclase and augite, the other minerals being regarded as accessories.
Magnetite or ilmenite is almost universally present. The varieties are
will be noted that in these rocks the magma became quite simple in nature,
just as at the acid end of the series certain rocks become comparatively
simple from the concentration of the acid element, as in certain acidic
granites, felsites, etc. (See pp. 523–524.)
The basalts.—The term basalt is used in a somewhat comprehensive
way to embrace dark, compact, igneous rocks that appear to be nearly
homogeneous, owing to the minuteness of the crystals, which are usually so
small as to be identifiable only under the microscope. In some cases the
crystals are scattered throughout a ground-mass after the porphyritic
fashion. In some of these cases there is a true glassy base, and in such cases
the rock does not strictly belong in the holocrystalline group. In the more
typical cases the constituent minerals are very minutely crystallized and
intimately intermixed. The leading minerals are plagioclase (usually
labradorite or anorthite) and pyroxene (usually augite), with olivine and
magnetite or ilmenite usually present. There is a considerable range in
chemical nature, but the basalts are relatively poor in silica, usually also
low in potash and soda, but rich in lime, magnesia, and the iron oxides.
They are classed as basic and are sometimes highly so. The magmas of the
basalts are especially fluid, and when poured forth upon the surface easily
spread out in thin sheets. In cooling they are prone to take on a columnar or
basaltic structure, the columns standing at right angles to the surfaces
exposed to cooling. The columns are sometimes curved, owing to the
peculiar attitude of the cooling surface. The columns of Giant’s Causeway
and Fingal’s Cave are familiar examples.
The dolerites.—The basalts graduate insensibly into the dolerites; indeed
the dolerites may be regarded simply as basalts of coarser crystallization.
The minerals are evident to the eye and range up to medium size. The more
abundant minerals are plagioclase feldspar (labradorite or anorthite), with
one or more of the ferromagnesian minerals (augite, olivine, or biotite), and
magnetite or ilmenite. In the growth of the minerals one crystal frequently
embraces others, giving an ophitic structure. The dolerites have many
varieties, due either to accessory minerals or to the development of some of
the constituents more amply than the rest. The type may be said to consist
of plagioclase and augite, the other minerals being regarded as accessories.
Magnetite or ilmenite is almost universally present. The varieties are
Page 495
usually designated by prefixes, as olivine-dolerite, enstatite-dolerite, etc.,
but special names are also used for some of these.
Fig. 346.—Conglomerate, Carboniferous series. Bancroft Place, Newport, R. I. (Walcott,
U. S. Geol. Surv.)
The ancient dolerites have usually undergone internal changes and such
rocks are often called diabases. While the use of the term has not been
uniform, it accords with the better practice to regard the diabases simply as
partially altered dolerites and basalts. In general, therefore, the diabases are
but ancient dolerites.
General names.
The difficulty of distinguishing many of the foregoing rocks from each
other by any means available in the field, owing to the minuteness of the
crystals, and to the gradation of one type of rock into another, makes it
desirable to employ certain general names which will correctly express the
leading character of the rock without implying a knowledge of the precise
but special names are also used for some of these.
Fig. 346.—Conglomerate, Carboniferous series. Bancroft Place, Newport, R. I. (Walcott,
U. S. Geol. Surv.)
The ancient dolerites have usually undergone internal changes and such
rocks are often called diabases. While the use of the term has not been
uniform, it accords with the better practice to regard the diabases simply as
partially altered dolerites and basalts. In general, therefore, the diabases are
but ancient dolerites.
General names.
The difficulty of distinguishing many of the foregoing rocks from each
other by any means available in the field, owing to the minuteness of the
crystals, and to the gradation of one type of rock into another, makes it
desirable to employ certain general names which will correctly express the
leading character of the rock without implying a knowledge of the precise
Page 496
mineral composition. A convenient term of this kind is greenstone, which
merely indicates that the ferromagnesian minerals are prominent and
usually give a greenish or dark cast to the rock. The greenstones embrace
the diorites, dolerites, some of the gabbros and the basalts, and may even
extend to the peridotites and some of the more hornblendic of the granitoid
rocks. Another convenient name is trap, which may be used for any dark,
heavy igneous rock. The name (from trappe, stairs) refers to the step-like
arrangement which the edges of the superimposed sheets of lava often take,
especially when the lava is of the free-flowing, basaltic kind.
merely indicates that the ferromagnesian minerals are prominent and
usually give a greenish or dark cast to the rock. The greenstones embrace
the diorites, dolerites, some of the gabbros and the basalts, and may even
extend to the peridotites and some of the more hornblendic of the granitoid
rocks. Another convenient name is trap, which may be used for any dark,
heavy igneous rock. The name (from trappe, stairs) refers to the step-like
arrangement which the edges of the superimposed sheets of lava often take,
especially when the lava is of the free-flowing, basaltic kind.
Page 497
Fig. 347.—Brecciated limestone, Calciferous formation. One mile south of Highgate Falls,
Vt.
The term basalt is sometimes used to embrace any of the very fine-
grained dark igneous rocks. In such cases, it covers the very fine-grained
dolerites, diorites, peridotites, etc. The term granite was used originally for
any coarse-grained crystalline rock, and there is a tendency to revive this
early use. In general descriptions, some of our best petrographers call any
coarsely crystalline rock (e.g., coarse-grained syenites, diorites, gabbros,
etc.) granite. The term granitoids may be used with strict propriety to cover
all rocks of this class.
Vt.
The term basalt is sometimes used to embrace any of the very fine-
grained dark igneous rocks. In such cases, it covers the very fine-grained
dolerites, diorites, peridotites, etc. The term granite was used originally for
any coarse-grained crystalline rock, and there is a tendency to revive this
early use. In general descriptions, some of our best petrographers call any
coarsely crystalline rock (e.g., coarse-grained syenites, diorites, gabbros,
etc.) granite. The term granitoids may be used with strict propriety to cover
all rocks of this class.
Page 498
DERIVATION OF SECONDARY ROCKS.
Rocks, though commonly made the symbol of the abiding, are subject to
constant slow changes. Through these changes newer rocks have been
derived from older ones, and still others in turn from these derivatives, and
so on in an endless chain. All derived rocks are conveniently termed
secondary, though they may be several generations removed from the
primitive rocks, and even the primitive rocks, as we now understand them,
may be themselves derived. The ordinary changes of rock are most active at
or near the surface, and the processes of such change have already been
discussed in part under the titles “Weathering” (pp. 54 and 110), “Erosion”
(pp. 119–123 and 342–349), “Transportation” (pp. 115–119 and 354–355),
and “Deposition” (pp. 177–204 and 355–363).
Fig. 348.—Quartzitic breccia. About one-third natural size. (Photo. by Church.)
Rocks, though commonly made the symbol of the abiding, are subject to
constant slow changes. Through these changes newer rocks have been
derived from older ones, and still others in turn from these derivatives, and
so on in an endless chain. All derived rocks are conveniently termed
secondary, though they may be several generations removed from the
primitive rocks, and even the primitive rocks, as we now understand them,
may be themselves derived. The ordinary changes of rock are most active at
or near the surface, and the processes of such change have already been
discussed in part under the titles “Weathering” (pp. 54 and 110), “Erosion”
(pp. 119–123 and 342–349), “Transportation” (pp. 115–119 and 354–355),
and “Deposition” (pp. 177–204 and 355–363).
Fig. 348.—Quartzitic breccia. About one-third natural size. (Photo. by Church.)
Page 499
Fig. 349.—Section of limestone showing abundant fossils imbedded in a matrix made up of
comminuted shell matter. About two-thirds natural size. (Photo. by Church.)
comminuted shell matter. About two-thirds natural size. (Photo. by Church.)
Page 500
Fig. 350.—Limestone composed chiefly of shells. About three-fourths natural size. (Photo.
by Church.)
Regolith.—The first great product of the surface changes is mantle-rock
(regolith), which comprehends all the loose matter that springs from rock
decay, wear, fracture, and other forms of disintegration. It lies in an
unconsolidated sheet on the face of the land, whether as soil, sand, clay,
earth, gravel, or loose rock.
Disrupted products: arkose and wacke.—In dry regions, in cold
regions, on mountain heights and precipitous slopes, and under other
conditions where sudden changes of temperature and frost action work
efficiently, rocks are broken down into fine fragments without much
chemical decomposition. Such disaggregated rather than decomposed
matter, if derived from granitic and similar crystalline rocks, is termed
arkose, or arkose sand, and consists of fragments of quartz, feldspar, mica,
etc. Common sand consists essentially of quartz grains. If the fine
fragments are derived from the darker igneous rocks, and consist mainly of
by Church.)
Regolith.—The first great product of the surface changes is mantle-rock
(regolith), which comprehends all the loose matter that springs from rock
decay, wear, fracture, and other forms of disintegration. It lies in an
unconsolidated sheet on the face of the land, whether as soil, sand, clay,
earth, gravel, or loose rock.
Disrupted products: arkose and wacke.—In dry regions, in cold
regions, on mountain heights and precipitous slopes, and under other
conditions where sudden changes of temperature and frost action work
efficiently, rocks are broken down into fine fragments without much
chemical decomposition. Such disaggregated rather than decomposed
matter, if derived from granitic and similar crystalline rocks, is termed
arkose, or arkose sand, and consists of fragments of quartz, feldspar, mica,
etc. Common sand consists essentially of quartz grains. If the fine
fragments are derived from the darker igneous rocks, and consist mainly of
Page 501
grains of plagioclase feldspar, and ferromagnesian minerals, it is sometimes
called wacke. This term is not widely used in just this sense, but there seems
to be an important place for it, and it will be so employed in this work.
These disaggregated sands are but special phases of the mantle-rock.
Disintegrated products.—When the surface-rock is chemically
decomposed, the residual material is confined mainly to the insoluble
portions, i.e., the silicious and clayey parts; while the lime, magnesia, soda,
potash, and similar substances are largely dissolved and borne to the ocean.
The potash is somewhat more disposed to remain with the clays than the
soda, lime, or magnesia; but residues of all are usually present.
Classes of Sedimentary Rocks.
Shales, sandstones, and conglomerates.—As already shown in the
discussion of the atmosphere and surface-waters, the mantle-rock is
constantly being borne away and redeposited in lodgment spots on the land
or in the basins of the sea, while it is constantly being renewed below. It is
an evanescent but ever-renewed derivative mantle. In this process of
renewal, removal, and redeposition, the mantle material is usually assorted
into mud, sand, and gravel; and these several classes of material are laid
down more or less separately, and usually take the stratified form, because
their deposition depends on different degrees of motion of the transporting
waters or wind. When these several classes of material become cemented or
otherwise hardened, they give rise to shales (cemented muds), sandstones
(cemented sands), and conglomerates (or pudding-stones, cemented gravel,
Fig. 346). If the coarse material remains angular, they form breccia instead
of conglomerates (Figs. 347 and 348). For the most part, the deposits of
mud, sand, and gravel are made under the sea or in lakes and estuaries, but
they are also formed on the land in lodgment basins, in low-gradient
valleys, and on base-plains. The deposits of sediment on land have received
less recognition than they deserve. When formed under the sea or in other
life-sustaining waters, shells and other organic material are liable to be
entrapped and to form a part of the rock. These organic remains, or fossils,
greatly aid in interpreting the deposits in which they occur. Fossils are less
liable to be preserved in sedimentary deposits formed on land. There is,
therefore, some ground to suspect that great series of sandstones and shales
which do not contain marine or fresh-water fossils were formed in lodgment
called wacke. This term is not widely used in just this sense, but there seems
to be an important place for it, and it will be so employed in this work.
These disaggregated sands are but special phases of the mantle-rock.
Disintegrated products.—When the surface-rock is chemically
decomposed, the residual material is confined mainly to the insoluble
portions, i.e., the silicious and clayey parts; while the lime, magnesia, soda,
potash, and similar substances are largely dissolved and borne to the ocean.
The potash is somewhat more disposed to remain with the clays than the
soda, lime, or magnesia; but residues of all are usually present.
Classes of Sedimentary Rocks.
Shales, sandstones, and conglomerates.—As already shown in the
discussion of the atmosphere and surface-waters, the mantle-rock is
constantly being borne away and redeposited in lodgment spots on the land
or in the basins of the sea, while it is constantly being renewed below. It is
an evanescent but ever-renewed derivative mantle. In this process of
renewal, removal, and redeposition, the mantle material is usually assorted
into mud, sand, and gravel; and these several classes of material are laid
down more or less separately, and usually take the stratified form, because
their deposition depends on different degrees of motion of the transporting
waters or wind. When these several classes of material become cemented or
otherwise hardened, they give rise to shales (cemented muds), sandstones
(cemented sands), and conglomerates (or pudding-stones, cemented gravel,
Fig. 346). If the coarse material remains angular, they form breccia instead
of conglomerates (Figs. 347 and 348). For the most part, the deposits of
mud, sand, and gravel are made under the sea or in lakes and estuaries, but
they are also formed on the land in lodgment basins, in low-gradient
valleys, and on base-plains. The deposits of sediment on land have received
less recognition than they deserve. When formed under the sea or in other
life-sustaining waters, shells and other organic material are liable to be
entrapped and to form a part of the rock. These organic remains, or fossils,
greatly aid in interpreting the deposits in which they occur. Fossils are less
liable to be preserved in sedimentary deposits formed on land. There is,
therefore, some ground to suspect that great series of sandstones and shales
which do not contain marine or fresh-water fossils were formed in lodgment
Page 502
basins on land, though the absence of fossils cannot be regarded as proof of
such origin.
Fig. 351. Fig. 352.
Fig. 351.—Globigerina ooze. Magnified 20 times. (Murray and Renard.)
Fig. 352.—Pteropod ooze. Magnified 4 times. (Murray and Renard.)
Limestones and dolomites.—Of the lime, magnesia, soda, and potash
leached out of the surface-rocks and carried to the ocean in solution, the
lime is largely extracted to form the shells, skeletons, teeth, armor, and
other hard parts of sea-animals and sea-plants. These limy parts are at
length left on the floor of the ocean and become more or less disintegrated
and help to form beds of lime-mud and lime-sand which in time are
cemented into limestone (Figs. 349, 350, 351, and 352). A larger proportion
of the magnesia remains in solution in the sea-water, but in ways not yet
well understood, the magnesia sometimes unites with the lime to form
dolomite, a double carbonate of lime and magnesia (Ca,Mg)CO3. This
such origin.
Fig. 351. Fig. 352.
Fig. 351.—Globigerina ooze. Magnified 20 times. (Murray and Renard.)
Fig. 352.—Pteropod ooze. Magnified 4 times. (Murray and Renard.)
Limestones and dolomites.—Of the lime, magnesia, soda, and potash
leached out of the surface-rocks and carried to the ocean in solution, the
lime is largely extracted to form the shells, skeletons, teeth, armor, and
other hard parts of sea-animals and sea-plants. These limy parts are at
length left on the floor of the ocean and become more or less disintegrated
and help to form beds of lime-mud and lime-sand which in time are
cemented into limestone (Figs. 349, 350, 351, and 352). A larger proportion
of the magnesia remains in solution in the sea-water, but in ways not yet
well understood, the magnesia sometimes unites with the lime to form
dolomite, a double carbonate of lime and magnesia (Ca,Mg)CO3. This
Page 503
change is sometimes local, and sometimes affects great series of beds, more
commonly the ancient ones than the modern. Sometimes the dolomization
appears to have taken place long after the original limestone was formed
and probably sometimes after it was lifted out of the sea, while in other
cases it seems to have taken place while the sediment was accumulating, or
at least before the next overlying beds were laid down. The potash in
solution is to some large extent taken up by the land- and sea-plants or is
retained in the clays, and through them becomes again incorporated in the
sediments. The soda largely remains in solution in the sea-water.
Precipitates.—When a portion of the ocean-water is isolated in a region
where evaporation from the surface of the water is greater than the rainfall
on it, and the inflow from the tributary basin, the lime, magnesia, soda,
potash, and other dissolved substances (solutes) are concentrated until the
water becomes saturated. The solutes are then precipitated in the order in
which they reach the point of saturation. This order, when taken in strict and
full detail, gives a very complex series, but the leading deposits are calcium
carbonate (limestone), calcium sulphate (gypsum), and sodium chloride
(halite or rock salt) (see p. 375). Isolated lakes in arid regions may give rise
to similar deposits. It has sometimes been thought that the ancient
limestones were produced largely by precipitation from concentrated sea-
water. While this is probably the case in some instances and to some degree,
it has not been demonstrated that the great limestone formations were made
to any large extent in this way. The more accepted view is that the
limestones in the main were made from organic remains. The lime in
solution in the ocean is chiefly in the form of the sulphate.
Iron Ore-beds.—In a somewhat different way iron ore-deposits are
formed by the precipitation of iron oxide or iron carbonate from solutions
of ferrous compounds. The ferrous compounds in solution were leached
from iron-bearing rocks by percolating waters. The most familiar case is
that of iron-bearing springs. On exposure to the air, the iron compounds in
solution undergo change, and ferric oxide is thrown down, usually forming
limonite (Fe2O3,3H2O), but sometimes hematite (Fe2O3). This change is
common in marshes and gives origin to “bog-ore.” Similar deposits take
place in certain shallow lakes, and hence are known as “lake ore.” Iron ore
sometimes also forms at the bottom of a peaty bed or in muddy soil. In
connection with the great coal formations, beds of iron carbonate (siderite)
commonly the ancient ones than the modern. Sometimes the dolomization
appears to have taken place long after the original limestone was formed
and probably sometimes after it was lifted out of the sea, while in other
cases it seems to have taken place while the sediment was accumulating, or
at least before the next overlying beds were laid down. The potash in
solution is to some large extent taken up by the land- and sea-plants or is
retained in the clays, and through them becomes again incorporated in the
sediments. The soda largely remains in solution in the sea-water.
Precipitates.—When a portion of the ocean-water is isolated in a region
where evaporation from the surface of the water is greater than the rainfall
on it, and the inflow from the tributary basin, the lime, magnesia, soda,
potash, and other dissolved substances (solutes) are concentrated until the
water becomes saturated. The solutes are then precipitated in the order in
which they reach the point of saturation. This order, when taken in strict and
full detail, gives a very complex series, but the leading deposits are calcium
carbonate (limestone), calcium sulphate (gypsum), and sodium chloride
(halite or rock salt) (see p. 375). Isolated lakes in arid regions may give rise
to similar deposits. It has sometimes been thought that the ancient
limestones were produced largely by precipitation from concentrated sea-
water. While this is probably the case in some instances and to some degree,
it has not been demonstrated that the great limestone formations were made
to any large extent in this way. The more accepted view is that the
limestones in the main were made from organic remains. The lime in
solution in the ocean is chiefly in the form of the sulphate.
Iron Ore-beds.—In a somewhat different way iron ore-deposits are
formed by the precipitation of iron oxide or iron carbonate from solutions
of ferrous compounds. The ferrous compounds in solution were leached
from iron-bearing rocks by percolating waters. The most familiar case is
that of iron-bearing springs. On exposure to the air, the iron compounds in
solution undergo change, and ferric oxide is thrown down, usually forming
limonite (Fe2O3,3H2O), but sometimes hematite (Fe2O3). This change is
common in marshes and gives origin to “bog-ore.” Similar deposits take
place in certain shallow lakes, and hence are known as “lake ore.” Iron ore
sometimes also forms at the bottom of a peaty bed or in muddy soil. In
connection with the great coal formations, beds of iron carbonate (siderite)
Page 504
occur. Organic matter seems to play a great part
both in the original solution and the later
deposition of these ores. From certain soils and
clay-beds on which the ancient coal-producing
forests grew, the iron has been almost
completely removed, either by the action of the
roots, or more probably by organic acids arising
from their decay and from the decaying
vegetation on the surface. On flowing into
shallow bodies of water or into marshes, the
waters containing such dissolved iron
Fig. 353.—Diatom ooze.
Magnified 150 times. compounds usually throw down their iron
(Murray.) content either as a carbonate (siderite), or as a
hydrous ferric oxide (limonite). The siderite is formed where decaying
vegetation is present to furnish abundant carbon dioxide and to partially
protect the iron solution from oxidation, and the limonite where free
oxidation takes place. Sand, silt, clay, or calcium carbonate often
accumulates with the iron precipitate, and the result is an impure deposit
which becomes an ironstone. Such deposits often become segregated into
nodules, as will be explained later. It is thought that diatoms sometimes aid
in the deposit of iron ore in shallow waters.
Silicious deposits.—In the decomposition of igneous rocks, a certain
portion of the silica, as well as of the bases, is dissolved and carried away in
solution. Certain organisms extract this from solution for their skeletons,
just as others extract calcium carbonate. The accumulation of these silicious
skeletons often forms silicious rocks. The diatom, radiolarian, and other
oozes (Fig. 353) of the deep sea are the great examples. Sometimes layers
of infusorial earth, tripolite, arise from the shells of diatoms and other
aquatic organisms secreting silica. The waters in which such earths
accumulate are rather shallow, and either fresh or salt. The most familiar
examples of indurated rocks formed in this general method are the flints and
cherts (impure flints) that occur in limestone and chalk, chiefly as nodules,
but sometimes in distinct beds.
Organic rocks.—While most limestones, chalks, flints, cherts, and the
silicious and calcareous oozes are formed through the agency of organisms,
they are not themselves strictly organic. There is, however, a small but
both in the original solution and the later
deposition of these ores. From certain soils and
clay-beds on which the ancient coal-producing
forests grew, the iron has been almost
completely removed, either by the action of the
roots, or more probably by organic acids arising
from their decay and from the decaying
vegetation on the surface. On flowing into
shallow bodies of water or into marshes, the
waters containing such dissolved iron
Fig. 353.—Diatom ooze.
Magnified 150 times. compounds usually throw down their iron
(Murray.) content either as a carbonate (siderite), or as a
hydrous ferric oxide (limonite). The siderite is formed where decaying
vegetation is present to furnish abundant carbon dioxide and to partially
protect the iron solution from oxidation, and the limonite where free
oxidation takes place. Sand, silt, clay, or calcium carbonate often
accumulates with the iron precipitate, and the result is an impure deposit
which becomes an ironstone. Such deposits often become segregated into
nodules, as will be explained later. It is thought that diatoms sometimes aid
in the deposit of iron ore in shallow waters.
Silicious deposits.—In the decomposition of igneous rocks, a certain
portion of the silica, as well as of the bases, is dissolved and carried away in
solution. Certain organisms extract this from solution for their skeletons,
just as others extract calcium carbonate. The accumulation of these silicious
skeletons often forms silicious rocks. The diatom, radiolarian, and other
oozes (Fig. 353) of the deep sea are the great examples. Sometimes layers
of infusorial earth, tripolite, arise from the shells of diatoms and other
aquatic organisms secreting silica. The waters in which such earths
accumulate are rather shallow, and either fresh or salt. The most familiar
examples of indurated rocks formed in this general method are the flints and
cherts (impure flints) that occur in limestone and chalk, chiefly as nodules,
but sometimes in distinct beds.
Organic rocks.—While most limestones, chalks, flints, cherts, and the
silicious and calcareous oozes are formed through the agency of organisms,
they are not themselves strictly organic. There is, however, a small but
Page 505
important group of rocks formed directly from organic matter. In favorable
situations the woody parts of plants, falling into water, are so far preserved
from decay that they accumulate in beds, and by slow changes pass into
peat, lignite, bituminous coal, anthracite, and graphite. The first of these is
composed essentially of carbohydrates and hydrocarbons much as plants
are, while the last two are mainly carbon, and the intermediate members
represent stages of passage from the first to the last. They are all derived
from the strictly organic part of the plants, and spring essentially from the
atmosphere and hydrosphere. They are only indirectly associated with the
evolutions of the inorganic series.
INTERNAL ALTERATIONS OF ROCKS.
Besides the extreme alterations of rocks at the surface of the earth by
which they pass into solution and into residual mantle-rock, and at length
by transportation and re-sedimentation become stratified rocks, as just
described, those rocks which are not at the surface are subject to changes
that give rise to several varieties of altered rocks. These changes are taking
place constantly under ordinary conditions, though usually very slowly.
Under great pressure and heat the changes are relatively rapid and intense,
and lead to results not reached under other conditions. These more profound
changes are termed metamorphism, and will be considered later. It is,
however, important to recognize the great fact that the outer part of the
earth, for perhaps 20,000 or 30,000 feet, is more or less fractured and
permeated by water containing in solution various substances dissolved
from the atmosphere, the soil, and the rocks through which it has already
passed, and that this permeating and circulating water is now, and for long
ages has been, working changes in the rocks, partly by dissolving matter out
of them, partly by depositing matter in them, and partly by furnishing a
medium through which new combinations of their constituents may take
place. This outer fractured portion of the lithosphere has been called the
zone of fracture.[201]
Oxidation and deoxidation.—At and above the surface of the
underground water, where the rocks are easily reached by atmospheric
waters carrying much free oxygen, and by the air itself, oxidation prevails.
Through oxidation the ferrous oxides are changed to ferric oxides, a change
situations the woody parts of plants, falling into water, are so far preserved
from decay that they accumulate in beds, and by slow changes pass into
peat, lignite, bituminous coal, anthracite, and graphite. The first of these is
composed essentially of carbohydrates and hydrocarbons much as plants
are, while the last two are mainly carbon, and the intermediate members
represent stages of passage from the first to the last. They are all derived
from the strictly organic part of the plants, and spring essentially from the
atmosphere and hydrosphere. They are only indirectly associated with the
evolutions of the inorganic series.
INTERNAL ALTERATIONS OF ROCKS.
Besides the extreme alterations of rocks at the surface of the earth by
which they pass into solution and into residual mantle-rock, and at length
by transportation and re-sedimentation become stratified rocks, as just
described, those rocks which are not at the surface are subject to changes
that give rise to several varieties of altered rocks. These changes are taking
place constantly under ordinary conditions, though usually very slowly.
Under great pressure and heat the changes are relatively rapid and intense,
and lead to results not reached under other conditions. These more profound
changes are termed metamorphism, and will be considered later. It is,
however, important to recognize the great fact that the outer part of the
earth, for perhaps 20,000 or 30,000 feet, is more or less fractured and
permeated by water containing in solution various substances dissolved
from the atmosphere, the soil, and the rocks through which it has already
passed, and that this permeating and circulating water is now, and for long
ages has been, working changes in the rocks, partly by dissolving matter out
of them, partly by depositing matter in them, and partly by furnishing a
medium through which new combinations of their constituents may take
place. This outer fractured portion of the lithosphere has been called the
zone of fracture.[201]
Oxidation and deoxidation.—At and above the surface of the
underground water, where the rocks are easily reached by atmospheric
waters carrying much free oxygen, and by the air itself, oxidation prevails.
Through oxidation the ferrous oxides are changed to ferric oxides, a change
Page 506
which is usually manifested by a transition from a gray, green, or blue color,
to buff, brown, yellow, or red. The partial progress of such oxidation is
often shown in a fractured block or bowlder whose exterior shows the latter
colors, while the interior shows the former. The sulphides, of which
common pyrites (FeS2) is the most familiar, are oxidized into sulphates, and
then sometimes pass on into the higher oxides and other compounds. Thus
copperas (FeSO4) arises from pyrites (FeS2) by direct oxidation of both Fe
and S. The sulphuric acid of this compound, uniting with some base
stronger than the ferrous oxide, gives rise to further oxidation and results in
hematite (Fe2O3) and limonite (Fe2O3,3H2O). In general, the mineral
constituents of the rocks in this upper zone take on their maximum states of
oxidation. This oxidation affects more or less profoundly the character of
the rock as a whole. Deeper in the earth oxidation is less prevalent, and the
action is sometimes reversed and deoxidation takes place. So also wherever
organic matter is undergoing decomposition deoxidation is likely to occur.
Solution and deposition.—Solution preponderates in the upper part of
the zone of fracture, but deposition is prevalent in its deeper parts. The
calcium carbonate and silica dissolved near the surface are often deposited
below as calcite and quartz. The sulphates and other sulphur compounds
that are formed and dissolved near the surface are apt to be changed into
sulphides lower down by deoxidation. The soluble oxides and other
compounds formed near the surface are often likewise precipitated below.
This is particularly true where the descending waters encounter
decomposing organic matter, and where they mingle with waters that have
followed other routes and have become charged with different solutes. On
coming together, reaction between the constituents takes place, resulting
sometimes in new solutions and sometimes in precipitation.
If these lower deposits of calcite, quartz, sulphides, etc., are made in the
pores of the rock, they change its texture and composition. If they are made
in fissures they constitute veins, and if a sufficient percentage of the vein
matter consists of valuable metallic compounds, they constitute ores.
As the waters descend they suffer greater and greater pressure and some
increase of temperature, and these changes modify their power to hold
substances in solution. In general, the waters increase in solvent power, but
the effect is different for different mineral substances, and hence as a rule
to buff, brown, yellow, or red. The partial progress of such oxidation is
often shown in a fractured block or bowlder whose exterior shows the latter
colors, while the interior shows the former. The sulphides, of which
common pyrites (FeS2) is the most familiar, are oxidized into sulphates, and
then sometimes pass on into the higher oxides and other compounds. Thus
copperas (FeSO4) arises from pyrites (FeS2) by direct oxidation of both Fe
and S. The sulphuric acid of this compound, uniting with some base
stronger than the ferrous oxide, gives rise to further oxidation and results in
hematite (Fe2O3) and limonite (Fe2O3,3H2O). In general, the mineral
constituents of the rocks in this upper zone take on their maximum states of
oxidation. This oxidation affects more or less profoundly the character of
the rock as a whole. Deeper in the earth oxidation is less prevalent, and the
action is sometimes reversed and deoxidation takes place. So also wherever
organic matter is undergoing decomposition deoxidation is likely to occur.
Solution and deposition.—Solution preponderates in the upper part of
the zone of fracture, but deposition is prevalent in its deeper parts. The
calcium carbonate and silica dissolved near the surface are often deposited
below as calcite and quartz. The sulphates and other sulphur compounds
that are formed and dissolved near the surface are apt to be changed into
sulphides lower down by deoxidation. The soluble oxides and other
compounds formed near the surface are often likewise precipitated below.
This is particularly true where the descending waters encounter
decomposing organic matter, and where they mingle with waters that have
followed other routes and have become charged with different solutes. On
coming together, reaction between the constituents takes place, resulting
sometimes in new solutions and sometimes in precipitation.
If these lower deposits of calcite, quartz, sulphides, etc., are made in the
pores of the rock, they change its texture and composition. If they are made
in fissures they constitute veins, and if a sufficient percentage of the vein
matter consists of valuable metallic compounds, they constitute ores.
As the waters descend they suffer greater and greater pressure and some
increase of temperature, and these changes modify their power to hold
substances in solution. In general, the waters increase in solvent power, but
the effect is different for different mineral substances, and hence as a rule
Page 507
the waters are taking up some substances and laying down others as they
proceed. After penetrating to greater or less depths, the waters may come
again to the surface, either because they are pushed up by the higher head of
the waters behind, or because they become warmer and thus lighter, and are
forced up by the heavier cold waters above, or else they pass up by
diffusion through the descending waters. In any case, the deep, warm
waters, usually rather highly charged with material dissolved in their
previous courses, are apt to deposit some of their burden as they ascend to
horizons of lower pressures and temperatures. They are particularly liable to
make deposits where they commingle with other waters differently charged
with solutes. Thus internal changes in the body of the rocks are, and for
ages have been, taking place. In the upper part of the depositing zone,
calcite is the dominant mineral deposited, while in the lower, quartz is more
common; but much depends on local conditions and other influences, and
no rigid rule holds good.
Hydration and dehydration.—Water sometimes unites directly with
some of the constituents of a rock and produces hydrated minerals, i.e.,
minerals that have water as an element of their constitution, not simply
water absorbed into their pores. A large class of minerals known as zeolites,
because they swell up and undergo life-like contortions when their basic
water is driven off by heat, are examples of hydrous products. A more
familiar example is limonite (Fe2O3,3H2O), of which yellow ocher is a
variety, which on heating sufficiently gives off its water and becomes
hematite (Fe2O3) or red ocher. The turning of yellow clay to red brick on
burning is a familiar example of dehydration. The general tendency in the
upper zones penetrated by water is toward hydration. In the lower zones,
where the pressure is great, Van Hise holds that there is a tendency toward
dehydration, if the rocks have been previously hydrated. This may be the
case if rocks have once been near the surface and later deeply buried by the
accumulation of sediments on them. If the principle holds, rocks subjected
to intense lateral pressure may be dehydrated.
Carbonation and decarbonation.—The igneous rocks are largely
silicates. The carbonic acid of the surface-waters and of the air acting upon
them, converts them, in part, into carbonates. In this way has arisen most of
the original supply of calcium and magnesium carbonates. Original
carbonates formed in this way are precipitated and redissolved again and
proceed. After penetrating to greater or less depths, the waters may come
again to the surface, either because they are pushed up by the higher head of
the waters behind, or because they become warmer and thus lighter, and are
forced up by the heavier cold waters above, or else they pass up by
diffusion through the descending waters. In any case, the deep, warm
waters, usually rather highly charged with material dissolved in their
previous courses, are apt to deposit some of their burden as they ascend to
horizons of lower pressures and temperatures. They are particularly liable to
make deposits where they commingle with other waters differently charged
with solutes. Thus internal changes in the body of the rocks are, and for
ages have been, taking place. In the upper part of the depositing zone,
calcite is the dominant mineral deposited, while in the lower, quartz is more
common; but much depends on local conditions and other influences, and
no rigid rule holds good.
Hydration and dehydration.—Water sometimes unites directly with
some of the constituents of a rock and produces hydrated minerals, i.e.,
minerals that have water as an element of their constitution, not simply
water absorbed into their pores. A large class of minerals known as zeolites,
because they swell up and undergo life-like contortions when their basic
water is driven off by heat, are examples of hydrous products. A more
familiar example is limonite (Fe2O3,3H2O), of which yellow ocher is a
variety, which on heating sufficiently gives off its water and becomes
hematite (Fe2O3) or red ocher. The turning of yellow clay to red brick on
burning is a familiar example of dehydration. The general tendency in the
upper zones penetrated by water is toward hydration. In the lower zones,
where the pressure is great, Van Hise holds that there is a tendency toward
dehydration, if the rocks have been previously hydrated. This may be the
case if rocks have once been near the surface and later deeply buried by the
accumulation of sediments on them. If the principle holds, rocks subjected
to intense lateral pressure may be dehydrated.
Carbonation and decarbonation.—The igneous rocks are largely
silicates. The carbonic acid of the surface-waters and of the air acting upon
them, converts them, in part, into carbonates. In this way has arisen most of
the original supply of calcium and magnesium carbonates. Original
carbonates formed in this way are precipitated and redissolved again and
Page 508
again. The carbonates in river-waters are much more largely solutions of
previously solid carbonates than original carbonates formed from the
silicates. The potassium and sodium of the silicates also form carbonates,
but by preference they unite with the sulphur and chlorine, and hence
appear more largely as sulphates and chlorides.
Carbonation is usually accompanied by oxidation and hydration. These
several processes break up the complex and relatively unstable silicates into
simpler and more stable silicates, carbonates, and oxides. This is illustrated
by the following formulas illustrative of the changes undergone by augite
and labradorite, two common rock-forming minerals.
The composition of augite may be represented by the formula
CaO.(Mg,Fe)O.2SiO2
(Mg,Fe)O.(Al,Fe)2O3.SiO2.
Assuming Mg and Fe to be equal in amount in the first half of the above
formula, and Mg and Fe to be equal in the first part of the second half, and
Al and Fe to be equal in the last part of the second half, doubling the whole
and allowing it to be acted on by CO2 and H2O, we have
2CaO.2MgO.2FeO.Al2O3.Fe2O3.6SiO2 + 6CO2 + 2H2O
= 2CaCO3 + 2MgCO3 + 2H2O.Al2O3.2SiO2 + 2FeCO3 + Fe2O3
+ 4SiO2.
The hydrous silicate of the last part of the equation is kaolin.
The composition of labradorite is represented by the formula
CaO.Al2O3.2SiO2
Na2O.Al2O3.6SiO2.
Assuming the two molecules represented by this formula to be equally
abundant, and allowing the whole to be acted on by H2O and CO2, we have
CaO.Na2O.2Al2O3.8SiO2 + 4H2O + 2CO2
= CaCO3 + Na2CO3 + 2(2H2O.Al2O3.2SiO2) + 4SiO2.
When waters charged with carbonates descend into the earth they are
likely to precipitate a portion of their burden, forming calcite and other
previously solid carbonates than original carbonates formed from the
silicates. The potassium and sodium of the silicates also form carbonates,
but by preference they unite with the sulphur and chlorine, and hence
appear more largely as sulphates and chlorides.
Carbonation is usually accompanied by oxidation and hydration. These
several processes break up the complex and relatively unstable silicates into
simpler and more stable silicates, carbonates, and oxides. This is illustrated
by the following formulas illustrative of the changes undergone by augite
and labradorite, two common rock-forming minerals.
The composition of augite may be represented by the formula
CaO.(Mg,Fe)O.2SiO2
(Mg,Fe)O.(Al,Fe)2O3.SiO2.
Assuming Mg and Fe to be equal in amount in the first half of the above
formula, and Mg and Fe to be equal in the first part of the second half, and
Al and Fe to be equal in the last part of the second half, doubling the whole
and allowing it to be acted on by CO2 and H2O, we have
2CaO.2MgO.2FeO.Al2O3.Fe2O3.6SiO2 + 6CO2 + 2H2O
= 2CaCO3 + 2MgCO3 + 2H2O.Al2O3.2SiO2 + 2FeCO3 + Fe2O3
+ 4SiO2.
The hydrous silicate of the last part of the equation is kaolin.
The composition of labradorite is represented by the formula
CaO.Al2O3.2SiO2
Na2O.Al2O3.6SiO2.
Assuming the two molecules represented by this formula to be equally
abundant, and allowing the whole to be acted on by H2O and CO2, we have
CaO.Na2O.2Al2O3.8SiO2 + 4H2O + 2CO2
= CaCO3 + Na2CO3 + 2(2H2O.Al2O3.2SiO2) + 4SiO2.
When waters charged with carbonates descend into the earth they are
likely to precipitate a portion of their burden, forming calcite and other
Page 509
crystalline carbonates, and hence these are among the most common
minerals found in veins and rock cavities. Carbonates are also deposited
when carbonate-charged waters come to the surface and evaporate or lose a
part of their carbon dioxide.
Decarbonation also takes place, but it is, at least at the surface, a much
less common process, and its conditions are less well understood.
Sufficiently high heat will drive off the carbon dioxide, as in the artificial
process of burning lime, but this is rarely observed in nature. Even lava
intrusions do not usually reduce limestone to caustic lime at any appreciable
distance from the contact. It is believed, however, that in the deeper zones,
where high pressure and heat prevail, carbonates are changed into silicates,
thus in a way reversing the process that prevails at the surface, and setting
free again a portion of the carbon dioxide that had become locked up in the
formation of the carbonates. To this action some of the carbon dioxide of
deep-seated thermal springs is assigned.
The carbonation of the silicates takes place at the expense of the carbon
dioxide of the atmosphere and hydrosphere, and hence in proportion as the
igneous rocks are changed into carbonates, the atmosphere and hydrosphere
are depleted of carbon dioxide, new supplies being neglected. As plants are
dependent on carbon dioxide for their principal food, and as animals are
dependent on plants for their food, directly or indirectly, the process of
carbonation has a profound bearing on the life-history of the earth, and will
often invite attention in the historical chapters. It is sufficient here to note
that carbonation is one of the chief processes in the alteration of igneous
rocks and furnishes, directly and indirectly, a larger percentage of the
mineral substances dissolved in the waters that flow from the land, than any
other single process.
Molecular rearrangements.—Besides these and similar changes that
involve additions and subtractions through the agency of percolating water,
the molecules of some of the rock constituents rearrange themselves, or the
elements enter into new chemical relations; thus, pyroxene may pass into
hornblende by a change of the crystalline arrangement of the molecules.
The change may sometimes be caught in progress, the outer part of the
crystal being hornblende (which when thus formed is called uralite), while
the heart of the crystal remains pyroxene. So aragonite may pass into
calcite.
minerals found in veins and rock cavities. Carbonates are also deposited
when carbonate-charged waters come to the surface and evaporate or lose a
part of their carbon dioxide.
Decarbonation also takes place, but it is, at least at the surface, a much
less common process, and its conditions are less well understood.
Sufficiently high heat will drive off the carbon dioxide, as in the artificial
process of burning lime, but this is rarely observed in nature. Even lava
intrusions do not usually reduce limestone to caustic lime at any appreciable
distance from the contact. It is believed, however, that in the deeper zones,
where high pressure and heat prevail, carbonates are changed into silicates,
thus in a way reversing the process that prevails at the surface, and setting
free again a portion of the carbon dioxide that had become locked up in the
formation of the carbonates. To this action some of the carbon dioxide of
deep-seated thermal springs is assigned.
The carbonation of the silicates takes place at the expense of the carbon
dioxide of the atmosphere and hydrosphere, and hence in proportion as the
igneous rocks are changed into carbonates, the atmosphere and hydrosphere
are depleted of carbon dioxide, new supplies being neglected. As plants are
dependent on carbon dioxide for their principal food, and as animals are
dependent on plants for their food, directly or indirectly, the process of
carbonation has a profound bearing on the life-history of the earth, and will
often invite attention in the historical chapters. It is sufficient here to note
that carbonation is one of the chief processes in the alteration of igneous
rocks and furnishes, directly and indirectly, a larger percentage of the
mineral substances dissolved in the waters that flow from the land, than any
other single process.
Molecular rearrangements.—Besides these and similar changes that
involve additions and subtractions through the agency of percolating water,
the molecules of some of the rock constituents rearrange themselves, or the
elements enter into new chemical relations; thus, pyroxene may pass into
hornblende by a change of the crystalline arrangement of the molecules.
The change may sometimes be caught in progress, the outer part of the
crystal being hornblende (which when thus formed is called uralite), while
the heart of the crystal remains pyroxene. So aragonite may pass into
calcite.
Page 510
By changes of the foregoing kinds, many crystalline rocks are much
altered. Some become chloritic from the development of the soft, green
hydrated mineral, chlorite, derived from the pyroxene, amphibole, biotite,
and perhaps other silicates of the original rock. Others become talcose from
the development of talc, a very soft, unctuous, hydrous magnesian silicate
developed from the magnesian minerals of the original rock. Soapstone or
steatite is a rock composed essentially of such secondary material.
Serpentine is a rock made up of a similar secondary mineral (serpentine)
apparently derived from chrysolite (olivine) and other magnesian minerals.
Epidote, a complex lime-iron-alumina silicate, often recognizable by its
peculiar pistachio-green color, is derived from other silicates, and is rather
common in many varieties of crystalline rocks. Melaphyre is a name
applied rather loosely and variously to certain altered basic rocks of the
basalt family. Diabase is essentially an altered dolerite. Nearly all the very
ancient basaltic rocks show notable degrees of alteration, even though they
appear to have escaped unusual dynamic conditions since their original
formation, and hence their alteration seems to have resulted chiefly from
the operation of unobtrusive agencies, chief among which is the circulation
of water.
The Salient Features of Rock Descent.
The foregoing processes by which primitive or igneous rocks are
disintegrated and their constituents converted into fragmental material may
be said to constitute the descent of rocks in its fuller sense. Viewed
chemically, the great features of the process are (1) the breaking down of
the complex silicates, and (2) the gathering of the resultant simpler silicates
(mainly aluminum silicates) into the silt and clay beds, (3) the assembling
of a large part of the free acidic element (the quartz) into the sand and
gravel beds, and (4) the concentration of a large part of the earthy basic
element (the calcium, magnesium, and iron oxides) into the calcareous,
magnesian, and iron deposits, while (5) a large part of the alkaline basic
remainder (the sodium, and potassium oxides) is dissolved and held in the
sea-water. Physically, the great features are (1) the disaggregation of the
antecedent rock, and (2) the separation from one another of products which
are physically unlike, that is, the coarser from the finer, and the heavier
from the lighter, and (3) the aggregation of these diverse materials in more
altered. Some become chloritic from the development of the soft, green
hydrated mineral, chlorite, derived from the pyroxene, amphibole, biotite,
and perhaps other silicates of the original rock. Others become talcose from
the development of talc, a very soft, unctuous, hydrous magnesian silicate
developed from the magnesian minerals of the original rock. Soapstone or
steatite is a rock composed essentially of such secondary material.
Serpentine is a rock made up of a similar secondary mineral (serpentine)
apparently derived from chrysolite (olivine) and other magnesian minerals.
Epidote, a complex lime-iron-alumina silicate, often recognizable by its
peculiar pistachio-green color, is derived from other silicates, and is rather
common in many varieties of crystalline rocks. Melaphyre is a name
applied rather loosely and variously to certain altered basic rocks of the
basalt family. Diabase is essentially an altered dolerite. Nearly all the very
ancient basaltic rocks show notable degrees of alteration, even though they
appear to have escaped unusual dynamic conditions since their original
formation, and hence their alteration seems to have resulted chiefly from
the operation of unobtrusive agencies, chief among which is the circulation
of water.
The Salient Features of Rock Descent.
The foregoing processes by which primitive or igneous rocks are
disintegrated and their constituents converted into fragmental material may
be said to constitute the descent of rocks in its fuller sense. Viewed
chemically, the great features of the process are (1) the breaking down of
the complex silicates, and (2) the gathering of the resultant simpler silicates
(mainly aluminum silicates) into the silt and clay beds, (3) the assembling
of a large part of the free acidic element (the quartz) into the sand and
gravel beds, and (4) the concentration of a large part of the earthy basic
element (the calcium, magnesium, and iron oxides) into the calcareous,
magnesian, and iron deposits, while (5) a large part of the alkaline basic
remainder (the sodium, and potassium oxides) is dissolved and held in the
sea-water. Physically, the great features are (1) the disaggregation of the
antecedent rock, and (2) the separation from one another of products which
are physically unlike, that is, the coarser from the finer, and the heavier
from the lighter, and (3) the aggregation of these diverse materials in more
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or less distinct beds. It is to be noted that while the rearrangement of the
sediments is made on the basis of their physical characters, it results in
chemical differentiation as well, for the products of rock decay, which are
physically diverse, are often chemically diverse as well. The physical
assortment and the stratification are to be looked upon as a step in the
direction of a simpler grouping of the material. On the whole, the process is
descensional in character.
THE REASCENSIONAL PROCESS.
Running hand in hand with this descensional process, there has always
been a reascensional process by which the coherence, the crystallization,
and in some measure the complex composition of the rocks are restored.
This is partially due to external mechanical agencies, but chiefly to internal
chemical and molecular forces.
Two general phases of this reconstructional work are recognized. The
first, simplest and most universal, is that by which the incoherent materials
produced by the descensional processes, i.e., the muds, sands, and clastic
materials generally, are hardened into firm, coherent shales, sandstones, and
limestones, and incidentally more or less changed in composition and
molecular arrangement. The second is that by which more profound
changes of induration and of composition are wrought, bringing the rock
back to a state resembling its original crystalline character. This is known as
metamorphism. Often, however, it is but an extension and intensification of
the more common processes of the first class. Metamorphism is essentially
reconstruction.
Induration under ordinary pressures and temperatures.—All kinds
of loose fragmental material, whether soils, earths, clays, sands, gravels,
volcanic ashes, cinders, or other forms of clastic or pyroclastic material,
may become hardened into firm rock either by pressure, or by cementation,
or by both. Pressure and cementation commonly act together and aid each
other. The ordinary pressures arise from the weight of the overlying
material, and these of course increase with depth. Extraordinary pressures
arise from the shrinkage of the earth and perhaps from other sources. The
fragments of the clastic material, on being pressed together for long periods,
weld more or less at the points of contact. If they are irregular, angular, or
sediments is made on the basis of their physical characters, it results in
chemical differentiation as well, for the products of rock decay, which are
physically diverse, are often chemically diverse as well. The physical
assortment and the stratification are to be looked upon as a step in the
direction of a simpler grouping of the material. On the whole, the process is
descensional in character.
THE REASCENSIONAL PROCESS.
Running hand in hand with this descensional process, there has always
been a reascensional process by which the coherence, the crystallization,
and in some measure the complex composition of the rocks are restored.
This is partially due to external mechanical agencies, but chiefly to internal
chemical and molecular forces.
Two general phases of this reconstructional work are recognized. The
first, simplest and most universal, is that by which the incoherent materials
produced by the descensional processes, i.e., the muds, sands, and clastic
materials generally, are hardened into firm, coherent shales, sandstones, and
limestones, and incidentally more or less changed in composition and
molecular arrangement. The second is that by which more profound
changes of induration and of composition are wrought, bringing the rock
back to a state resembling its original crystalline character. This is known as
metamorphism. Often, however, it is but an extension and intensification of
the more common processes of the first class. Metamorphism is essentially
reconstruction.
Induration under ordinary pressures and temperatures.—All kinds
of loose fragmental material, whether soils, earths, clays, sands, gravels,
volcanic ashes, cinders, or other forms of clastic or pyroclastic material,
may become hardened into firm rock either by pressure, or by cementation,
or by both. Pressure and cementation commonly act together and aid each
other. The ordinary pressures arise from the weight of the overlying
material, and these of course increase with depth. Extraordinary pressures
arise from the shrinkage of the earth and perhaps from other sources. The
fragments of the clastic material, on being pressed together for long periods,
weld more or less at the points of contact. If they are irregular, angular, or
Page 512
elongate, they come to interlock more or less like the fragments of
macadam, and this coöperates with the welding. The process is greatly
aided by water-bearing solutions of lime, silica, etc. which are deposited at
the points where the fragments press upon each other. It is here that the
capillary spaces are most minute and deposition is most liable to take place.
Sometimes a film of mineral matter is laid down over the surfaces of the
fragments and serves to bind them together. This process goes on wherever
the ground-waters are in a depositing condition, just as the opposite process
of disintegration takes place wherever the waters are in a solvent state. At
and near the surface of the land, the waters are usually in the latter
condition and disintegration is in progress, as already noted, but this is not
always so. At times and places, the water from within the rock-mass may
come to the surface and evaporate, and in so doing leave all its dissolved
material on the surface, or within the outer pores of the mass, as cementing
material. The exterior thus becomes firmly bound together, “case-
hardened,” as it is termed. This may be seen in the drying of a lump of mud,
the exterior of which often becomes quite firm. It is seen in quarry-rock,
especially sandstone, which is sometimes soft and easily worked when
taken wet from the earth, but which hardens as the water—the “sap” of the
quarrymen—dries out and deposits its solutes in the capillary spaces of the
grains of the surface. It is obvious that it is the very last of the “sap” which
contains the most concentrated solutes, and that this last remnant is held in
the minute capillary spaces where the grains touch each other, and hence the
last stage of drying leaves the cement at the points where it is most
effective. In natural exposures of sandstone, the pores of the outer shell
sometimes become almost completely filled in this way with silicious
deposits, and the sandstone is changed into a quartzite.
In the sea, and in the deep water underground, the common habit of the
water is to deposit more than to dissolve, though it is doing more or less of
both. As a rule, therefore, loose material in these situations becomes bound
more or less firmly into rock, and hence what were originally loose sand
beds become sandstones; what were soft muds become shales or limestone,
according to composition; what was gravel becomes conglomerate; what
was chipstone becomes breccia; what were volcanic ashes, cinders, and
lapilli become tuffs; and what were masses of volcanic blocks and coarse
fragments become agglomerates.
macadam, and this coöperates with the welding. The process is greatly
aided by water-bearing solutions of lime, silica, etc. which are deposited at
the points where the fragments press upon each other. It is here that the
capillary spaces are most minute and deposition is most liable to take place.
Sometimes a film of mineral matter is laid down over the surfaces of the
fragments and serves to bind them together. This process goes on wherever
the ground-waters are in a depositing condition, just as the opposite process
of disintegration takes place wherever the waters are in a solvent state. At
and near the surface of the land, the waters are usually in the latter
condition and disintegration is in progress, as already noted, but this is not
always so. At times and places, the water from within the rock-mass may
come to the surface and evaporate, and in so doing leave all its dissolved
material on the surface, or within the outer pores of the mass, as cementing
material. The exterior thus becomes firmly bound together, “case-
hardened,” as it is termed. This may be seen in the drying of a lump of mud,
the exterior of which often becomes quite firm. It is seen in quarry-rock,
especially sandstone, which is sometimes soft and easily worked when
taken wet from the earth, but which hardens as the water—the “sap” of the
quarrymen—dries out and deposits its solutes in the capillary spaces of the
grains of the surface. It is obvious that it is the very last of the “sap” which
contains the most concentrated solutes, and that this last remnant is held in
the minute capillary spaces where the grains touch each other, and hence the
last stage of drying leaves the cement at the points where it is most
effective. In natural exposures of sandstone, the pores of the outer shell
sometimes become almost completely filled in this way with silicious
deposits, and the sandstone is changed into a quartzite.
In the sea, and in the deep water underground, the common habit of the
water is to deposit more than to dissolve, though it is doing more or less of
both. As a rule, therefore, loose material in these situations becomes bound
more or less firmly into rock, and hence what were originally loose sand
beds become sandstones; what were soft muds become shales or limestone,
according to composition; what was gravel becomes conglomerate; what
was chipstone becomes breccia; what were volcanic ashes, cinders, and
lapilli become tuffs; and what were masses of volcanic blocks and coarse
fragments become agglomerates.
Page 513
Fig. 354. Fig. 355.
Fig. 354.—Quartz crystal enlarged by secondary growth. The shaded outline
represents the outline of the sand grain; the solid lines, the outline after
secondary growth. Magnified 67 diameters. (Van Hise.)
Fig. 355.—Sandstone and quartzite texture. The shaded outlines represent the
surfaces of the sand grains before growth, the intervening white portions, the
added quartz, and the black portions, unfilled spaces. Open spaces
characterize sandstone. When the spaces are filled with quartz, the rock
becomes quartzite. Magnified 35 diameters. (Van Hise.)
The cementing process works at times in specially interesting ways. In
quartz sandstones, the grains are worn fragments of quartz crystals, formed
originally in quartz-bearing rock. The crystalline force in these remnants
controls the arrangement of the new molecules of silica deposited about
them. The result is that the new deposits tend to build up the original forms
of the crystals from which the sand grains were derived (Fig. 354).
Fig. 354.—Quartz crystal enlarged by secondary growth. The shaded outline
represents the outline of the sand grain; the solid lines, the outline after
secondary growth. Magnified 67 diameters. (Van Hise.)
Fig. 355.—Sandstone and quartzite texture. The shaded outlines represent the
surfaces of the sand grains before growth, the intervening white portions, the
added quartz, and the black portions, unfilled spaces. Open spaces
characterize sandstone. When the spaces are filled with quartz, the rock
becomes quartzite. Magnified 35 diameters. (Van Hise.)
The cementing process works at times in specially interesting ways. In
quartz sandstones, the grains are worn fragments of quartz crystals, formed
originally in quartz-bearing rock. The crystalline force in these remnants
controls the arrangement of the new molecules of silica deposited about
them. The result is that the new deposits tend to build up the original forms
of the crystals from which the sand grains were derived (Fig. 354).
Page 514
Sometimes a film of iron oxide has formed about the grain of sand before
the addition of the new silica. This, or some difference of color, may clearly
distinguish the original grain from subsequent additions. Sometimes the
adjacent grains of sandstone are rebuilt in this way until the interstices are
completely filled. When this has been accomplished, the sandstone becomes
a quartzite (Fig. 355). Most quartzites indeed appear to have been formed in
this way, but mainly under special conditions that promote the deposition of
silica. Grains of other minerals, such as feldspar, are subject to similar
secondary enlargement (Fig. 356).
Fig. 356.—Feldspar crystals enlarged by secondary growth. Magnified 50 diameters. AA =
original grains; BB = enlargements; D = unfilled spaces. (Van Hise.)
Sometimes the new material is deposited in the form of concentric shells
about the particles of sediment, building them up into little spheres. Rock
formed of such spherules is known as oolite, from the resemblance of the
grains to the roe of fish (Fig. 357). Sometimes the nuclei of the concretions
are grains of quartz sand, and the added concentric layers are of calcium
carbonate. In this case the structure is quite obvious; but perhaps more
frequently the nuclei are minute and difficult to identify, and the concentric
shells make up the main mass of the grains. Certain formations, as the
the addition of the new silica. This, or some difference of color, may clearly
distinguish the original grain from subsequent additions. Sometimes the
adjacent grains of sandstone are rebuilt in this way until the interstices are
completely filled. When this has been accomplished, the sandstone becomes
a quartzite (Fig. 355). Most quartzites indeed appear to have been formed in
this way, but mainly under special conditions that promote the deposition of
silica. Grains of other minerals, such as feldspar, are subject to similar
secondary enlargement (Fig. 356).
Fig. 356.—Feldspar crystals enlarged by secondary growth. Magnified 50 diameters. AA =
original grains; BB = enlargements; D = unfilled spaces. (Van Hise.)
Sometimes the new material is deposited in the form of concentric shells
about the particles of sediment, building them up into little spheres. Rock
formed of such spherules is known as oolite, from the resemblance of the
grains to the roe of fish (Fig. 357). Sometimes the nuclei of the concretions
are grains of quartz sand, and the added concentric layers are of calcium
carbonate. In this case the structure is quite obvious; but perhaps more
frequently the nuclei are minute and difficult to identify, and the concentric
shells make up the main mass of the grains. Certain formations, as the
Page 515
oolitic limestone of Indiana and elsewhere, and the Upper and Lower
Oolites of England, are characterized by this structure. In most cases these
accretions probably grew in depositing waters that gently rolled the grains
while layers were being added. They thus do not fall under the head of
cementation after the beds were formed; but concentric additions to the
grains appear sometimes to have taken place after they were formed into
beds.
Fig. 358.—Agate structure. The cavity was
first coated with mineral matter deposited
from solution. The contracted cavity was
then nearly filled with the same sort of
material deposited in layers, apparently
Fig. 357.—Oolitic texture. About natural over the bottom, until the cavity was
size. (Photo. by Church.) nearly obliterated.
Cavity filling.—When cavities of some size occur in rocks and the
percolating waters are in a depositing state, the interiors of the cavities are
sometimes lined with concentric layers of deposit. Here, instead of building
out from a nucleus, the waters build in from the walls of the cavity. The
agate structure (Fig. 358) is a case of this kind, in which the successive
layers are commonly silica in the form of chalcedony and differ from each
other in color and texture. Often before the cavity is entirely filled, the
deposit changes from chalcedony, to crystals of quartz, which grow with
Oolites of England, are characterized by this structure. In most cases these
accretions probably grew in depositing waters that gently rolled the grains
while layers were being added. They thus do not fall under the head of
cementation after the beds were formed; but concentric additions to the
grains appear sometimes to have taken place after they were formed into
beds.
Fig. 358.—Agate structure. The cavity was
first coated with mineral matter deposited
from solution. The contracted cavity was
then nearly filled with the same sort of
material deposited in layers, apparently
Fig. 357.—Oolitic texture. About natural over the bottom, until the cavity was
size. (Photo. by Church.) nearly obliterated.
Cavity filling.—When cavities of some size occur in rocks and the
percolating waters are in a depositing state, the interiors of the cavities are
sometimes lined with concentric layers of deposit. Here, instead of building
out from a nucleus, the waters build in from the walls of the cavity. The
agate structure (Fig. 358) is a case of this kind, in which the successive
layers are commonly silica in the form of chalcedony and differ from each
other in color and texture. Often before the cavity is entirely filled, the
deposit changes from chalcedony, to crystals of quartz, which grow with
Page 516
their bases on the walls and their pyramidal points toward the center of the
cavity. Geodes are examples of a similar process in which the cavity is but
partially filled with crystals which have their bases set on the walls of the
cavity and their points directed inwards (Fig. 359). The crystals of geodes
are most commonly quartz or calcite, but they may be any other mineral
that the waters are capable of depositing. Very large cavities lined in this
way are known to miners as vuggs, and these grade on into caves lined with
crystals and with stalactite and stalagmite. These are the largest expression
of the solidifying process by means of internal deposition.
Fissure-filling; veins.—Cracks, crevices, and fissures filled by
deposition in a similar way give rise to veins (Fig. 360). Here the filling
grows from the walls toward the center, and hence often has a banded
appearance. By this filling of cracks and crevices, the circulating water
heals the breaks in the rocks. Frequently a crushed zone is thus restored to a
solid state. When the fissures are deep and wide and traverse different
formations, conditions are afforded for very complex deposits, and for the
concentration of rare and valuable material originally dispersed through a
great mass of rock. Ore deposition in such veins is usually treated as a
theme by itself, but it is really but a declared expression of the work which
the percolating waters are doing throughout all the rocks which they
penetrate. Most of the fine crystals that grace mineralogical collections
were formed in cavities and fissures by deposition from circulating
mineralized waters.
cavity. Geodes are examples of a similar process in which the cavity is but
partially filled with crystals which have their bases set on the walls of the
cavity and their points directed inwards (Fig. 359). The crystals of geodes
are most commonly quartz or calcite, but they may be any other mineral
that the waters are capable of depositing. Very large cavities lined in this
way are known to miners as vuggs, and these grade on into caves lined with
crystals and with stalactite and stalagmite. These are the largest expression
of the solidifying process by means of internal deposition.
Fissure-filling; veins.—Cracks, crevices, and fissures filled by
deposition in a similar way give rise to veins (Fig. 360). Here the filling
grows from the walls toward the center, and hence often has a banded
appearance. By this filling of cracks and crevices, the circulating water
heals the breaks in the rocks. Frequently a crushed zone is thus restored to a
solid state. When the fissures are deep and wide and traverse different
formations, conditions are afforded for very complex deposits, and for the
concentration of rare and valuable material originally dispersed through a
great mass of rock. Ore deposition in such veins is usually treated as a
theme by itself, but it is really but a declared expression of the work which
the percolating waters are doing throughout all the rocks which they
penetrate. Most of the fine crystals that grace mineralogical collections
were formed in cavities and fissures by deposition from circulating
mineralized waters.
Page 517
Fig. 359.—A geode. About half natural size. (Photo. by Church.)
Solution as well as deposition.—A further phase of the process needs
attention. The percolating waters are constantly taking up matter as well as
throwing it down, and so, while they are cementing fragments together and
healing fractures, they are also removing material, and a rock may be
growing porous and cavernous at the same time that its fragments are being
united. Cavities may be formed at one stage and filled at another; matter
may be taken up at one point and put down at another, and so an internal
reconstruction is in slow progress.
Solution as well as deposition.—A further phase of the process needs
attention. The percolating waters are constantly taking up matter as well as
throwing it down, and so, while they are cementing fragments together and
healing fractures, they are also removing material, and a rock may be
growing porous and cavernous at the same time that its fragments are being
united. Cavities may be formed at one stage and filled at another; matter
may be taken up at one point and put down at another, and so an internal
reconstruction is in slow progress.
Page 518
Fig. 360.—Veins of calcite in limestone. Calciferous formation near Highgate Springs, Vt.
(Walcott, U. S. Geol. Surv.)
Concretions.—A notable phase of this internal reconstruction is the
assembling together of like kinds of matter. For instance, silica that was
probably deposited in the form of the silicious shells and spicules of plants
and animals, and was disseminated through the sediments as originally
formed, is aggregated into nodules of chert or flint (Fig. 361); similarly,
concretions of ferrous carbonate or calcium carbonate grow in sands, silts,
or muds; clusters of crystals of pyrite (FeS2), of sphalerite (ZnS), and
galenite (PbS) are formed in clayey layers, pressing the clay back as they
grow; and in many other cases, kind comes to kind. Some concretions
probably form during the accumulation of the beds in which they lie.
Replacements and pseudomorphs.—So also there are replacements,
sometimes resulting in imitative or false forms. Frequently the calcium
carbonate of corals, molluscan shells, etc., is replaced by silica, and this
substitution is brought about so gradually, particle by particle, that the
(Walcott, U. S. Geol. Surv.)
Concretions.—A notable phase of this internal reconstruction is the
assembling together of like kinds of matter. For instance, silica that was
probably deposited in the form of the silicious shells and spicules of plants
and animals, and was disseminated through the sediments as originally
formed, is aggregated into nodules of chert or flint (Fig. 361); similarly,
concretions of ferrous carbonate or calcium carbonate grow in sands, silts,
or muds; clusters of crystals of pyrite (FeS2), of sphalerite (ZnS), and
galenite (PbS) are formed in clayey layers, pressing the clay back as they
grow; and in many other cases, kind comes to kind. Some concretions
probably form during the accumulation of the beds in which they lie.
Replacements and pseudomorphs.—So also there are replacements,
sometimes resulting in imitative or false forms. Frequently the calcium
carbonate of corals, molluscan shells, etc., is replaced by silica, and this
substitution is brought about so gradually, particle by particle, that the
Page 519
minutest details of structure are sometimes fully preserved. This is often of
great service in their study, since the limestone in which they are imbedded
may often be dissolved away, while the silicified fossil is unaffected. So
woody matter is sometimes replaced by silica, forming silicified wood.
Similarly, the molecules of one crystal are sometimes replaced by different
material, as the molecules of calcite by zinc carbonate, giving a
pseudomorph of zinc carbonate after calcite.
Fig. 361.—Nodule of chert. About half natural size. (Photo. by Church.)
Incipient crystallization.—A more general change is incipient
crystallization. Some common limestones and dolomites are now largely
made up of small crystals, though the mass was originally a calcareous mud
or ooze. Incipient crystals are formed in shales and other sediments. This
process, like the preceding, is a kind of incipient metamorphism or
reconstruction, but it is a pervasive process, taking place under ordinary
conditions of heat and pressure, and through the agency of circulating
ground-waters.
By these and similar processes the fragmental deposits are solidified into
firm rock and undergo internal changes which more or less reorganize the
matter of which they are composed. The process is a very slow one usually.
Some of the sands and muds of very early geologic ages are yet imperfectly
solidified; e.g., much of the St. Peter’s sandstone, a very ancient formation,
is yet so incoherent as to break down into sand in being dug out, and is used
for mortar sand much more than for building stone. Some of the Hudson
River shales of scarcely less age are more nearly clay than hard rock. But
these are examples of excessive slowness and slightness of change. In
great service in their study, since the limestone in which they are imbedded
may often be dissolved away, while the silicified fossil is unaffected. So
woody matter is sometimes replaced by silica, forming silicified wood.
Similarly, the molecules of one crystal are sometimes replaced by different
material, as the molecules of calcite by zinc carbonate, giving a
pseudomorph of zinc carbonate after calcite.
Fig. 361.—Nodule of chert. About half natural size. (Photo. by Church.)
Incipient crystallization.—A more general change is incipient
crystallization. Some common limestones and dolomites are now largely
made up of small crystals, though the mass was originally a calcareous mud
or ooze. Incipient crystals are formed in shales and other sediments. This
process, like the preceding, is a kind of incipient metamorphism or
reconstruction, but it is a pervasive process, taking place under ordinary
conditions of heat and pressure, and through the agency of circulating
ground-waters.
By these and similar processes the fragmental deposits are solidified into
firm rock and undergo internal changes which more or less reorganize the
matter of which they are composed. The process is a very slow one usually.
Some of the sands and muds of very early geologic ages are yet imperfectly
solidified; e.g., much of the St. Peter’s sandstone, a very ancient formation,
is yet so incoherent as to break down into sand in being dug out, and is used
for mortar sand much more than for building stone. Some of the Hudson
River shales of scarcely less age are more nearly clay than hard rock. But
these are examples of excessive slowness and slightness of change. In
Page 520
general, all but the most recent deposits show notable progress in
reconstruction.
Fig. 362.—Figure showing the elongation of pebbles resulting from pressure. Carboniferous
formation, Bancroft Place, Newport, R. I. (Walcott, U. S. Geol. Surv.)
Reconstruction under Exceptional Conditions.
Two special conditions greatly influence changes in rocks, viz., pressure
and heat. Their action gives rise to three general cases, but these blend
indefinitely: (1) exceptional pressure without great heat, (2) great heat
without exceptional pressure, and (3) great heat and great pressure
conjoined. Exceptional pressure may arise from the weight of overlying
rocks, or from lateral thrust due to the shrinkage of the globe, and
occasionally from other causes. Exceptional heat may arise from pressure,
from the intrusion of hot lavas, and occasionally from other sources. In the
case of intruded lavas there may or may not be exceptional pressure. Thrust
reconstruction.
Fig. 362.—Figure showing the elongation of pebbles resulting from pressure. Carboniferous
formation, Bancroft Place, Newport, R. I. (Walcott, U. S. Geol. Surv.)
Reconstruction under Exceptional Conditions.
Two special conditions greatly influence changes in rocks, viz., pressure
and heat. Their action gives rise to three general cases, but these blend
indefinitely: (1) exceptional pressure without great heat, (2) great heat
without exceptional pressure, and (3) great heat and great pressure
conjoined. Exceptional pressure may arise from the weight of overlying
rocks, or from lateral thrust due to the shrinkage of the globe, and
occasionally from other causes. Exceptional heat may arise from pressure,
from the intrusion of hot lavas, and occasionally from other sources. In the
case of intruded lavas there may or may not be exceptional pressure. Thrust
Page 521
usually gives heat as well as pressure, but if lateral thrust acts on rocks near
the surface, they may be mashed into new forms without becoming very
exceptionally heated, though some rise of temperature is inevitable.
Fig. 363.—Pre-Cambrian fossiliferous slate. Deep Creek Canyon, 16 miles southeast of
Townsend, Mont. (Walcott, U. S. Geol. Surv.])
(1) Slaty structure.—When rocks made up of clastic particles are
compressed in a given direction and are relatively free to expand at right
angles to the direction of pressure, the particles that are already elongated
tend to take positions with their longer axes at right angles to the direction
the surface, they may be mashed into new forms without becoming very
exceptionally heated, though some rise of temperature is inevitable.
Fig. 363.—Pre-Cambrian fossiliferous slate. Deep Creek Canyon, 16 miles southeast of
Townsend, Mont. (Walcott, U. S. Geol. Surv.])
(1) Slaty structure.—When rocks made up of clastic particles are
compressed in a given direction and are relatively free to expand at right
angles to the direction of pressure, the particles that are already elongated
tend to take positions with their longer axes at right angles to the direction
Page 522
of pressure, and all particles, whether elongate or not, are more or less
flattened in a plane transverse to the direction of pressure. This may be
readily seen where the particles are large (Fig. 362). As a result of the
orientation and flattening of their particles, rocks so affected split more
readily between the elongate and flattened particles than across them. In
other words, the rocks cleave along planes normal to the direction of
compression, and break with difficulty and with rough fracture across the
planes of cleavage. The condition thus induced is known as slaty structure
(Fig. 363), and is best illustrated by roofing-slate, which was originally a
mud, later a shale, and finally assumed the slaty condition under strong
compression. Sometimes the original bedding may still be seen running
across the induced cleavage planes (Fig. 364). As the original mud beds
were horizontal or nearly so, and as the thrust is usually horizontal or nearly
so, the induced cleavage commonly crosses the bedding planes at a high
angle (Fig. 364); but after the beds are tilted or bent, the lines of pressure
take new directions relative to the bedding planes, and the angles between
the original bedding and the slaty cleavages usually become smaller, and
may even disappear in exceptional cases. Limestones, sandstones, and
conglomerates are not so easily compressed as mudstones, and they usually
take on only an imperfect cleavage normal to the direction of pressure.
Often they merely show some little compacting, while the shaly strata
between them are converted into slate. Obviously the direction of slaty
cleavage may be used to determine the direction of the compressing force,
and is thus serviceable in dynamic studies.
flattened in a plane transverse to the direction of pressure. This may be
readily seen where the particles are large (Fig. 362). As a result of the
orientation and flattening of their particles, rocks so affected split more
readily between the elongate and flattened particles than across them. In
other words, the rocks cleave along planes normal to the direction of
compression, and break with difficulty and with rough fracture across the
planes of cleavage. The condition thus induced is known as slaty structure
(Fig. 363), and is best illustrated by roofing-slate, which was originally a
mud, later a shale, and finally assumed the slaty condition under strong
compression. Sometimes the original bedding may still be seen running
across the induced cleavage planes (Fig. 364). As the original mud beds
were horizontal or nearly so, and as the thrust is usually horizontal or nearly
so, the induced cleavage commonly crosses the bedding planes at a high
angle (Fig. 364); but after the beds are tilted or bent, the lines of pressure
take new directions relative to the bedding planes, and the angles between
the original bedding and the slaty cleavages usually become smaller, and
may even disappear in exceptional cases. Limestones, sandstones, and
conglomerates are not so easily compressed as mudstones, and they usually
take on only an imperfect cleavage normal to the direction of pressure.
Often they merely show some little compacting, while the shaly strata
between them are converted into slate. Obviously the direction of slaty
cleavage may be used to determine the direction of the compressing force,
and is thus serviceable in dynamic studies.
Page 523
Fig. 364.—Slaty structure and its relation to bedding planes. Two miles south of Walland,
Tenn. (Keith, U. S. Geol. Surv.)
Tenn. (Keith, U. S. Geol. Surv.)
Page 524
Fig. 365.—Foliated rock. (Ells, Can. Geol. Surv.)
Foliation, schistosity.—A more intense application of pressure in a given
direction is capable of breaking down and deforming the most resistant
rock. This must necessarily be attended with the evolution of much heat,
and thermal effects are mingled with pressure effects, but the thermal
effects may be neglected for the moment. The first stage of the mechanical
effect of the compression may be to crush the rock more or less. It thus
becomes granular or fragmental, and is really a peculiar species of clastic
rock (autoclastic). At a further stage, the fragmented material may be
pressed into layers or leaves, much as in the development of slaty cleavage,
but as a result of the nature of the material, the cleavage is less perfect. This
is often attended by more or less shearing of the material upon itself, and
thus a rude fissility and foliation is developed. The result, including the
attendant metamorphism about to be described, is a foliated or schistose
structure (Figs. 365 and 366). Even the most massive rocks may be reduced
to the foliated form by this process; thus, a granite may be mashed into a
Foliation, schistosity.—A more intense application of pressure in a given
direction is capable of breaking down and deforming the most resistant
rock. This must necessarily be attended with the evolution of much heat,
and thermal effects are mingled with pressure effects, but the thermal
effects may be neglected for the moment. The first stage of the mechanical
effect of the compression may be to crush the rock more or less. It thus
becomes granular or fragmental, and is really a peculiar species of clastic
rock (autoclastic). At a further stage, the fragmented material may be
pressed into layers or leaves, much as in the development of slaty cleavage,
but as a result of the nature of the material, the cleavage is less perfect. This
is often attended by more or less shearing of the material upon itself, and
thus a rude fissility and foliation is developed. The result, including the
attendant metamorphism about to be described, is a foliated or schistose
structure (Figs. 365 and 366). Even the most massive rocks may be reduced
to the foliated form by this process; thus, a granite may be mashed into a
Page 525
gneiss—which is a granite in composition, but has a foliated structure—or a
basalt may be converted into a schist, a common term for foliated
crystalline rocks. Porphyritic rock rendered schistose by pressure is shown
in Fig. 366. When massive rocks like granite or basalt are thus crushed
down into the foliated form, the process is in a sense degradational. It is a
kind of katamorphism or downward change. It is often difficult to
differentiate the schists thus derived by degrading massive rocks, from
those developed by ascensional processes from clastic formations
(anamorphism). The action of heat is important in the evolution of schists
of both classes, but the effects of heat may best be taken up where it acts
measurably alone.
basalt may be converted into a schist, a common term for foliated
crystalline rocks. Porphyritic rock rendered schistose by pressure is shown
in Fig. 366. When massive rocks like granite or basalt are thus crushed
down into the foliated form, the process is in a sense degradational. It is a
kind of katamorphism or downward change. It is often difficult to
differentiate the schists thus derived by degrading massive rocks, from
those developed by ascensional processes from clastic formations
(anamorphism). The action of heat is important in the evolution of schists
of both classes, but the effects of heat may best be taken up where it acts
measurably alone.
Page 526
Fig. 366.—Porphyry rendered schistose by pressure. Near Green Park, Caldwell Co., N. C.
(Keith, U. S. Geol. Surv.)
(Keith, U. S. Geol. Surv.)
Page 527
Fig. 367.—Schistose structure developed by pressure shown in the left half of the figure,
while it is wanting in the right half. The vertical line is a bedding plane. The layer to the
left was of sufficiently different composition or subject to sufficiently different movement
to develop schistosity, while that to the right was broken (brecciated) instead. The rock at
the left would be called quartz schist, while that at the right is quartzite. Huronian
formation near Ableman, Wis. (Atwood.)
Metamorphism by heat.—When a mass of lava is poured out upon the
surface, it bakes the mantle-rock which it overruns, in greater or less
degree, depending on the mass and temperature. The nature of the effect is
much the same as in the process of brick-making, a dehydration of the
material, a hardening of the loose matter by the partial welding of the
particles, and sometimes the partial fusion of the surface and the
while it is wanting in the right half. The vertical line is a bedding plane. The layer to the
left was of sufficiently different composition or subject to sufficiently different movement
to develop schistosity, while that to the right was broken (brecciated) instead. The rock at
the left would be called quartz schist, while that at the right is quartzite. Huronian
formation near Ableman, Wis. (Atwood.)
Metamorphism by heat.—When a mass of lava is poured out upon the
surface, it bakes the mantle-rock which it overruns, in greater or less
degree, depending on the mass and temperature. The nature of the effect is
much the same as in the process of brick-making, a dehydration of the
material, a hardening of the loose matter by the partial welding of the
particles, and sometimes the partial fusion of the surface and the
Page 528
development of new compounds, usually glassy, but sometimes partially
crystalline. In both the natural and the artificial process, the time element is
short, the pressure trivial, and the water action limited. If the heat were to
become sufficiently intense, the result would be fusion, i.e., a lava which
would solidify into a glass. In such a case, the rock cycle would be carried
back to the initial molten state and a new cycle instituted, but this does not
usually take place when lava merely overflows the surface.
If lavas, instead of rising to the surface, wedge in between layers of rock
and form sills, or interstratified sheets, the surface above as well as that
below is baked, and as the excess of heat of the lava can only escape
through the neighboring rock, the effects for a given mass of lava are more
considerable, and as the time element and the water action (and sometimes
the pressure) are usually greater than in the case of extruded lavas, the
effects tend rather toward chemical and crystalline change than to simple
baking. This tendency increases with increase in the mass of the lava and in
its temperature. Sometimes enormous masses of very hot lava are thrust in
between or among the strata that lie beneath the surface, and bring to bear
upon them intense heat for a long period. So also, when a vent or fissure is
the passageway for lavas that continue to come to the surface for long
periods, as in the case of persistent volcanoes, the rocks which form the
walls of the vent or fissure are heated for a long time, and this gives rise to
metamorphism through heat, without very unusual pressure, but usually
with the free aid of water. In these cases the chief effect is chemical
recombination and crystallization. In the limestones and sandstones it is
simple; in the shales more complex. In pure limestones and dolomites little
chemical change takes place, but the molecules are rearranged into larger
and more perfect crystals, and marble is the result. The coarseness of the
crystals is, in a general way, a measure of the length of time during which
the heat acts, and of its intensity, but much depends on the freedom of the
attendant water circulation. Crystals an inch or two across are sometimes
formed in the contact zone, where the attendant water action is important. If
impurities, as silica, alumina, iron, etc., are present, various minerals, such
as tremolite and actinolite, may be formed in the marble. In pure quartzose
sandstones, the effect is to cause the building up of the quartz grains until
the interspaces are essentially filled and the whole becomes a massive
quartzite. Here, as in the marbles, impurities form adventitious crystals, a
crystalline. In both the natural and the artificial process, the time element is
short, the pressure trivial, and the water action limited. If the heat were to
become sufficiently intense, the result would be fusion, i.e., a lava which
would solidify into a glass. In such a case, the rock cycle would be carried
back to the initial molten state and a new cycle instituted, but this does not
usually take place when lava merely overflows the surface.
If lavas, instead of rising to the surface, wedge in between layers of rock
and form sills, or interstratified sheets, the surface above as well as that
below is baked, and as the excess of heat of the lava can only escape
through the neighboring rock, the effects for a given mass of lava are more
considerable, and as the time element and the water action (and sometimes
the pressure) are usually greater than in the case of extruded lavas, the
effects tend rather toward chemical and crystalline change than to simple
baking. This tendency increases with increase in the mass of the lava and in
its temperature. Sometimes enormous masses of very hot lava are thrust in
between or among the strata that lie beneath the surface, and bring to bear
upon them intense heat for a long period. So also, when a vent or fissure is
the passageway for lavas that continue to come to the surface for long
periods, as in the case of persistent volcanoes, the rocks which form the
walls of the vent or fissure are heated for a long time, and this gives rise to
metamorphism through heat, without very unusual pressure, but usually
with the free aid of water. In these cases the chief effect is chemical
recombination and crystallization. In the limestones and sandstones it is
simple; in the shales more complex. In pure limestones and dolomites little
chemical change takes place, but the molecules are rearranged into larger
and more perfect crystals, and marble is the result. The coarseness of the
crystals is, in a general way, a measure of the length of time during which
the heat acts, and of its intensity, but much depends on the freedom of the
attendant water circulation. Crystals an inch or two across are sometimes
formed in the contact zone, where the attendant water action is important. If
impurities, as silica, alumina, iron, etc., are present, various minerals, such
as tremolite and actinolite, may be formed in the marble. In pure quartzose
sandstones, the effect is to cause the building up of the quartz grains until
the interspaces are essentially filled and the whole becomes a massive
quartzite. Here, as in the marbles, impurities form adventitious crystals, a
Page 529
very common one being hematite, formed from the segregation of the ferric
oxide of the sandstone.
In the shales, the material to be acted upon is more complex, for, while
the main mass is an aluminum silicate, there is usually much free quartz,
not a little potash and iron, and more or less of lime, magnesia, soda, and
other ingredients, for the muds from which the shales arose contained not
only the fully decomposed matter of the original crystalline rocks, but the
fine matter worn from them by wind and water without decomposition.
When this mixed matter is acted upon by high heat and moisture, it tends to
return to its original crystalline state, so far as its changed constitution
permits. The potash chiefly unites with alumina and silica, and forms potash
feldspar (orthoclase chiefly) and potash mica (muscovite). The iron often
unites with magnesia, alumina, and silica to form biotite or one of the
ferromagnesian minerals, chiefly an amphibole. The lime usually aids in the
formation of other silicates of either the feldspar or the ferromagnesian
group, while the surplus silica crystallizes into quartz. There is usually a
predisposition to form mica in preference to other silicates if the proper
constituents are present, and the result is that mica schists and gneisses, in
which mica abounds, are common products of the metamorphism of shales
by contact with bodies of lava. Mica schists and micaceous gneisses are
also formed in other ways, and other schists, dependent on the composition
of the shales, are formed about intrusions of igneous rock. In all such cases
pressure probably attends the heat and is a factor in the development of the
schists. When the change induced by the heat is less considerable, the shale
is baked, with incipient recrystallization, and often takes the form of
argillite, a compact, massive sort of shale.
Beds of hydrous iron oxide (limonite) or of iron carbonate (siderite) are
usually converted by heat into hematite or magnetite. Beds of peat, lignite,
and bituminous coal are converted into anthracite by the driving off of the
volatile hydrocarbons. If the process goes to the extreme, graphite is the
result.
Metamorphism by heat and lateral pressure.—As already indicated,
the more common intense pressures experienced by rocks at and near the
surface are those that come from lateral thrusts arising from the shrinkage
of the earth. These affect one dimension of the rock-mass, while they permit
it to expand in one or both of the other dimensions. This produces a strain in
oxide of the sandstone.
In the shales, the material to be acted upon is more complex, for, while
the main mass is an aluminum silicate, there is usually much free quartz,
not a little potash and iron, and more or less of lime, magnesia, soda, and
other ingredients, for the muds from which the shales arose contained not
only the fully decomposed matter of the original crystalline rocks, but the
fine matter worn from them by wind and water without decomposition.
When this mixed matter is acted upon by high heat and moisture, it tends to
return to its original crystalline state, so far as its changed constitution
permits. The potash chiefly unites with alumina and silica, and forms potash
feldspar (orthoclase chiefly) and potash mica (muscovite). The iron often
unites with magnesia, alumina, and silica to form biotite or one of the
ferromagnesian minerals, chiefly an amphibole. The lime usually aids in the
formation of other silicates of either the feldspar or the ferromagnesian
group, while the surplus silica crystallizes into quartz. There is usually a
predisposition to form mica in preference to other silicates if the proper
constituents are present, and the result is that mica schists and gneisses, in
which mica abounds, are common products of the metamorphism of shales
by contact with bodies of lava. Mica schists and micaceous gneisses are
also formed in other ways, and other schists, dependent on the composition
of the shales, are formed about intrusions of igneous rock. In all such cases
pressure probably attends the heat and is a factor in the development of the
schists. When the change induced by the heat is less considerable, the shale
is baked, with incipient recrystallization, and often takes the form of
argillite, a compact, massive sort of shale.
Beds of hydrous iron oxide (limonite) or of iron carbonate (siderite) are
usually converted by heat into hematite or magnetite. Beds of peat, lignite,
and bituminous coal are converted into anthracite by the driving off of the
volatile hydrocarbons. If the process goes to the extreme, graphite is the
result.
Metamorphism by heat and lateral pressure.—As already indicated,
the more common intense pressures experienced by rocks at and near the
surface are those that come from lateral thrusts arising from the shrinkage
of the earth. These affect one dimension of the rock-mass, while they permit
it to expand in one or both of the other dimensions. This produces a strain in
Page 530
all the constituent particles of the rock, and under such strain they pass
more readily into solution than when free from strain, and more readily
rearrange their molecules internally into positions of less strain. The
crystals grow most freely along the planes of least stress, i.e., at right angles
to the pressure.[202] As a consequence, where unidimensional pressure and
high heat resulting from the compression unite their influence, the
metamorphic changes are not only facilitated, but the rearrangement is
controlled by the pressure and results in a parallel arrangement of the
constituent crystals, giving a foliated or schistose character to the new rock.
The changes themselves are much the same as those produced by heat and
water without exceptional pressure, though some distinctions may be noted.
It is to be observed, however, that two kinds of work are embraced here: the
metamorphism of clastic rocks into crystalline schists, which may be
regarded as an upbuilding process, anamorphism, and the mashing down of
massive crystalline rocks into schists, which may be regarded as a
degradational process, katamorphism. In both cases, however, there is
solution and rearrangement of the molecules. The katamorphism of basalts
and other basic rocks gives basic schists; that of granitic and similar rocks
gives gneisses. The anamorphism of basic pyroclastic tuffs and wackes
gives basic schists, while that of acid pyroclastics and most shales gives
gneisses, mica schists, or similar acidic schists. It is obvious that ordinary
shales cannot usually become basic schists, because in producing the
original muds, the bases were generally removed; but when shales are
highly calcareous and magnesian, as when they grade toward the limestones
and dolomites, they may become basic schists by metamorphism, e.g.,
certain hornblendic schists. It is even more obvious that the limestone and
sandstone formations must largely retain their distinct composition. It is
thus seen that, in general, a sedimentary series anamorphosed must differ
from a crystalline series katamorphosed, though both give rise to foliated or
schistose rocks.
Deep-seated metamorphism.—When the exceptional pressure arises
from the weight of rocks felt at great depth, it is practically equal in all
directions and the crystallization probably develops normally and is not
forced into the parallel or foliated form. Rocks metamorphosed under these
conditions probably tend to take the massive form rather than the schistose
form, but this conclusion is theoretical rather than observational, for little or
nothing is known of the history of such rocks.
more readily into solution than when free from strain, and more readily
rearrange their molecules internally into positions of less strain. The
crystals grow most freely along the planes of least stress, i.e., at right angles
to the pressure.[202] As a consequence, where unidimensional pressure and
high heat resulting from the compression unite their influence, the
metamorphic changes are not only facilitated, but the rearrangement is
controlled by the pressure and results in a parallel arrangement of the
constituent crystals, giving a foliated or schistose character to the new rock.
The changes themselves are much the same as those produced by heat and
water without exceptional pressure, though some distinctions may be noted.
It is to be observed, however, that two kinds of work are embraced here: the
metamorphism of clastic rocks into crystalline schists, which may be
regarded as an upbuilding process, anamorphism, and the mashing down of
massive crystalline rocks into schists, which may be regarded as a
degradational process, katamorphism. In both cases, however, there is
solution and rearrangement of the molecules. The katamorphism of basalts
and other basic rocks gives basic schists; that of granitic and similar rocks
gives gneisses. The anamorphism of basic pyroclastic tuffs and wackes
gives basic schists, while that of acid pyroclastics and most shales gives
gneisses, mica schists, or similar acidic schists. It is obvious that ordinary
shales cannot usually become basic schists, because in producing the
original muds, the bases were generally removed; but when shales are
highly calcareous and magnesian, as when they grade toward the limestones
and dolomites, they may become basic schists by metamorphism, e.g.,
certain hornblendic schists. It is even more obvious that the limestone and
sandstone formations must largely retain their distinct composition. It is
thus seen that, in general, a sedimentary series anamorphosed must differ
from a crystalline series katamorphosed, though both give rise to foliated or
schistose rocks.
Deep-seated metamorphism.—When the exceptional pressure arises
from the weight of rocks felt at great depth, it is practically equal in all
directions and the crystallization probably develops normally and is not
forced into the parallel or foliated form. Rocks metamorphosed under these
conditions probably tend to take the massive form rather than the schistose
form, but this conclusion is theoretical rather than observational, for little or
nothing is known of the history of such rocks.
Page 531
Completion of the rock cycle.—The crystallizing processes of
metamorphism are fundamentally similar to the processes by which rocks
crystallize out of magmas, only in the first case the work is done chiefly by
the aid of an aqueous solution, while in the second it is done through a
mutual solution of the constituents in themselves, where water was but an
incident. If the heat factor in metamorphism be sufficiently increased,
aqueous solution may actually grade into magmatic solution through
various degrees of softening and melting, and the cycle of changes be
closed in upon itself.
VARIOUS CLASSIFICATIONS AND NOMENCLATURES.
From the foregoing sketch of the processes of rock-making it may easily
be inferred that the varieties of rocks may be almost unlimited, and that
they may be defined, named, and classified on many different bases; for
example.
(1) If the mode of origin is chiefly in mind, rocks may be classed as
igneous (lavas, tuffs, etc.); metamorphic (schists, gneisses, anthracite,
magnetite, etc.); aqueous (water-laid sediments, stalactites, travertine, etc.);
eolian (dunes, loess in part); glacial (till, moraines); clastic (mantle-rock,
sandstone, conglomerate, etc.); organic (peat, lignite, coal, etc., and
indirectly, limestone, chalk, infusorial earth, etc.); and so on.
(2) If the textural or structural characters are in mind, rocks are
designated vesicular (pumice, scoria, etc.); rhyolitic (flow-structure rocks);
glassy (obsidian, tachylite); porphyritic (distinct crystals in obscure matrix);
granitic (well-grained); compact, porous, earthy, arenaceous (sandy),
schistose, etc.
(3) If the chemical composition is chiefly regarded, they may be classed
as silicious, calcareous, carbonaceous, ferruginous, etc.; or, if the chemical
nature is considered, they are grouped as acidic, basic, or neutral.
(4) If the crystalline character is made the basis, they are designated
phanerocrystalline (distinctly crystallized), microcrystalline (minutely
crystallized), cryptocrystalline (hiddenly crystallized), and amorphous (non-
crystalline).
metamorphism are fundamentally similar to the processes by which rocks
crystallize out of magmas, only in the first case the work is done chiefly by
the aid of an aqueous solution, while in the second it is done through a
mutual solution of the constituents in themselves, where water was but an
incident. If the heat factor in metamorphism be sufficiently increased,
aqueous solution may actually grade into magmatic solution through
various degrees of softening and melting, and the cycle of changes be
closed in upon itself.
VARIOUS CLASSIFICATIONS AND NOMENCLATURES.
From the foregoing sketch of the processes of rock-making it may easily
be inferred that the varieties of rocks may be almost unlimited, and that
they may be defined, named, and classified on many different bases; for
example.
(1) If the mode of origin is chiefly in mind, rocks may be classed as
igneous (lavas, tuffs, etc.); metamorphic (schists, gneisses, anthracite,
magnetite, etc.); aqueous (water-laid sediments, stalactites, travertine, etc.);
eolian (dunes, loess in part); glacial (till, moraines); clastic (mantle-rock,
sandstone, conglomerate, etc.); organic (peat, lignite, coal, etc., and
indirectly, limestone, chalk, infusorial earth, etc.); and so on.
(2) If the textural or structural characters are in mind, rocks are
designated vesicular (pumice, scoria, etc.); rhyolitic (flow-structure rocks);
glassy (obsidian, tachylite); porphyritic (distinct crystals in obscure matrix);
granitic (well-grained); compact, porous, earthy, arenaceous (sandy),
schistose, etc.
(3) If the chemical composition is chiefly regarded, they may be classed
as silicious, calcareous, carbonaceous, ferruginous, etc.; or, if the chemical
nature is considered, they are grouped as acidic, basic, or neutral.
(4) If the crystalline character is made the basis, they are designated
phanerocrystalline (distinctly crystallized), microcrystalline (minutely
crystallized), cryptocrystalline (hiddenly crystallized), and amorphous (non-
crystalline).
Page 532
(5) If attention is fastened on certain ingredients, rocks are characterized
as quartzose, micaceous, chloritic, talcose, pyritiferous, garnetiferous, etc.
(6) When rocks are regarded as mineral aggregates, if (a) the aggregates
are simple, they are named from the dominant minerals, as dolomite,
hornblendite, garnetite, anorthite, etc.; and if (b) the aggregates are complex
they take special names, as syenite (orthoclase and hornblende), gabbro
(plagioclase feldspar and pyroxene), etc.
(7) When the point of view is structure of the mass, they are classed as
massive, stratified, shaly, laminated, slaty, foliated, schistose, etc.
(8) When physical state or genesis is considered, they are grouped as
clastic, fragmental, or detrital (conglomeratic, brecciated, arenaceous,
argillaceous, etc.); or pyroclastic (tufaceous, scoriaceous, agglomeratic); or
massive, in a sense slightly different from that above (7).
As sometimes one of these characteristics and sometimes another is most
important in a given rock, or in a given study, no one classification is
satisfactory in all cases, yet each has its advantages in particular cases.
New System of Classification and Nomenclature.
The present systems of classifying and naming rocks have grown up
gradually out of earlier and cruder methods, many of which were inherited
from popular usage. Most of the names and definitions came into use before
microscopical and other modern means of study were adopted. These
systems, therefore, retain many inherited crudities and inconsistencies, and
lack adaptation to present needs. They are too complex and difficult for
field use and for general discussions, while not sufficiently exact and
systematic for the more rigorous petrological discussions. A more adaptive
and consistent practice has been earnestly sought by petrologists, and a new
system of classification of igneous rocks has been offered by a group of
leading American petrologists, an outline of which is here given.[203] To
some extent this may be extended to the metamorphic crystalline rocks with
necessary modifications and additions. The classification and nomenclature
of the secondary rocks must probably always remain variable and plastic to
express the various points of view which it is desirable to take. During the
transition to this or some other new system, which seems inevitable, the
appended alphabetical reference lists of the most common minerals and
as quartzose, micaceous, chloritic, talcose, pyritiferous, garnetiferous, etc.
(6) When rocks are regarded as mineral aggregates, if (a) the aggregates
are simple, they are named from the dominant minerals, as dolomite,
hornblendite, garnetite, anorthite, etc.; and if (b) the aggregates are complex
they take special names, as syenite (orthoclase and hornblende), gabbro
(plagioclase feldspar and pyroxene), etc.
(7) When the point of view is structure of the mass, they are classed as
massive, stratified, shaly, laminated, slaty, foliated, schistose, etc.
(8) When physical state or genesis is considered, they are grouped as
clastic, fragmental, or detrital (conglomeratic, brecciated, arenaceous,
argillaceous, etc.); or pyroclastic (tufaceous, scoriaceous, agglomeratic); or
massive, in a sense slightly different from that above (7).
As sometimes one of these characteristics and sometimes another is most
important in a given rock, or in a given study, no one classification is
satisfactory in all cases, yet each has its advantages in particular cases.
New System of Classification and Nomenclature.
The present systems of classifying and naming rocks have grown up
gradually out of earlier and cruder methods, many of which were inherited
from popular usage. Most of the names and definitions came into use before
microscopical and other modern means of study were adopted. These
systems, therefore, retain many inherited crudities and inconsistencies, and
lack adaptation to present needs. They are too complex and difficult for
field use and for general discussions, while not sufficiently exact and
systematic for the more rigorous petrological discussions. A more adaptive
and consistent practice has been earnestly sought by petrologists, and a new
system of classification of igneous rocks has been offered by a group of
leading American petrologists, an outline of which is here given.[203] To
some extent this may be extended to the metamorphic crystalline rocks with
necessary modifications and additions. The classification and nomenclature
of the secondary rocks must probably always remain variable and plastic to
express the various points of view which it is desirable to take. During the
transition to this or some other new system, which seems inevitable, the
appended alphabetical reference lists of the most common minerals and
Page 533
rocks, with brief definitions in accordance with current usage, will be found
serviceable. The proposed system includes two parts, a field system and a
quantitative system, the one applicable to rocks on casual inspection, and
the other, only after detailed study.
The proposed field system.
The proposed field names are based largely on texture and color. The
mineral constituents are used for subdivisions when they can be
determined; otherwise they are neglected.
Classifying chiefly on the basis of texture and crystalline state, there are
three groups: Phanerites, in which all the leading mineral constituents can
be seen megascopically; aphanites, in which all, or at least an appreciable
part, of the constituent minerals cannot be distinguished megascopically;
and glasses, in which the material is wholly or largely vitreous.
I. The Phanerites may be further classified by their chief mineral
constituents as follows:
1. Granites (f.n.),[204] consisting largely of quartz and feldspar of any
kind, with or without mica, hornblende, pyroxene, or other minerals. This
differs from the present common use in not regarding mica as an essential
constituent, and in not distinguishing between alkali feldspars and calcic
feldspars, thus broadening the class.
2. Syenites (f.n.), consisting predominantly of feldspar of any kind, with
subordinate amounts of hornblende, mica, or pyroxene, but with little or no
quartz. This differs from the common use in giving hornblende a
subordinate place, and in embracing rocks with calcic feldspars, thus
broadening the class.
3. Diorites (f.n.), consisting predominantly of hornblende and
subordinately of feldspar of any kind, with which there may be mica,
pyroxene, or other minerals. This is nearly the present use except that any
kind of feldspar may form the subordinate element.
4. Gabbros (f.n.), consisting predominantly of pyroxene and
subordinately of feldspar of any kind, with or without other minerals. This
nearly coincides with one of the various present uses of the term except that
the range of the feldspar is increased.
serviceable. The proposed system includes two parts, a field system and a
quantitative system, the one applicable to rocks on casual inspection, and
the other, only after detailed study.
The proposed field system.
The proposed field names are based largely on texture and color. The
mineral constituents are used for subdivisions when they can be
determined; otherwise they are neglected.
Classifying chiefly on the basis of texture and crystalline state, there are
three groups: Phanerites, in which all the leading mineral constituents can
be seen megascopically; aphanites, in which all, or at least an appreciable
part, of the constituent minerals cannot be distinguished megascopically;
and glasses, in which the material is wholly or largely vitreous.
I. The Phanerites may be further classified by their chief mineral
constituents as follows:
1. Granites (f.n.),[204] consisting largely of quartz and feldspar of any
kind, with or without mica, hornblende, pyroxene, or other minerals. This
differs from the present common use in not regarding mica as an essential
constituent, and in not distinguishing between alkali feldspars and calcic
feldspars, thus broadening the class.
2. Syenites (f.n.), consisting predominantly of feldspar of any kind, with
subordinate amounts of hornblende, mica, or pyroxene, but with little or no
quartz. This differs from the common use in giving hornblende a
subordinate place, and in embracing rocks with calcic feldspars, thus
broadening the class.
3. Diorites (f.n.), consisting predominantly of hornblende and
subordinately of feldspar of any kind, with which there may be mica,
pyroxene, or other minerals. This is nearly the present use except that any
kind of feldspar may form the subordinate element.
4. Gabbros (f.n.), consisting predominantly of pyroxene and
subordinately of feldspar of any kind, with or without other minerals. This
nearly coincides with one of the various present uses of the term except that
the range of the feldspar is increased.
Page 534
5. Dolerites[205] (f.n.), consisting predominantly of any ferromagnesian
mineral not distinguishable as hornblende or pyroxene, with subordinate
elements of feldspar of any kind, and with or without other accessory
minerals. A name to be used when the dominant mineral is clearly
ferromagnesian, but cannot be satisfactorily identified as either hornblende
or pyroxene, although it may probably be one of these. In other words, the
dolerites (deceptive) embrace the whole diorite-gabbro group when too
obscure for separation.
6. Peridotites, consisting predominantly of olivine and ferromagnesian
minerals, without feldspar, or with very little.
7. Pyroxenite, consisting essentially of pyroxene without feldspar or
olivine.
8. Hornblendite, consisting essentially of hornblende without feldspar or
olivine.
II. The Aphanites may be non-porphyritic or porphyritic.
(a) Non-porphyritic aphanites when light-colored may be classed as
felsites; when dark-colored, as basalts.
(b) The porphyritic aphanites or porphyries, when light-colored, are
leucophyres; when dark-colored, are melaphyres (f.n.). They may be
classified further, according to the kind of phenocryst imbedded in the
aphanitic ground-mass, as
Quartz-porphyries, or quartzophyres;
Feldspar-porphyries, or feldspaphyres (not felsophyres);
Hornblende-porphyries, or hornblendophyres; and so on.
These may be subclassed by color, as
Quartz-leucophyres, light-colored quartz-porphyries;
Quartz-melaphyres, dark-colored quartz-porphyries;
Feldspar-leucophyres;
Feldspar-melaphyres; and so on.
III. The glasses are classified, according to color and luster, into
obsidians or pitchstones when dark and lustrous; perlites, when a spheroidal
fracture gives them a pearly appearance; and pumice when greatly inflated
by included gases.
mineral not distinguishable as hornblende or pyroxene, with subordinate
elements of feldspar of any kind, and with or without other accessory
minerals. A name to be used when the dominant mineral is clearly
ferromagnesian, but cannot be satisfactorily identified as either hornblende
or pyroxene, although it may probably be one of these. In other words, the
dolerites (deceptive) embrace the whole diorite-gabbro group when too
obscure for separation.
6. Peridotites, consisting predominantly of olivine and ferromagnesian
minerals, without feldspar, or with very little.
7. Pyroxenite, consisting essentially of pyroxene without feldspar or
olivine.
8. Hornblendite, consisting essentially of hornblende without feldspar or
olivine.
II. The Aphanites may be non-porphyritic or porphyritic.
(a) Non-porphyritic aphanites when light-colored may be classed as
felsites; when dark-colored, as basalts.
(b) The porphyritic aphanites or porphyries, when light-colored, are
leucophyres; when dark-colored, are melaphyres (f.n.). They may be
classified further, according to the kind of phenocryst imbedded in the
aphanitic ground-mass, as
Quartz-porphyries, or quartzophyres;
Feldspar-porphyries, or feldspaphyres (not felsophyres);
Hornblende-porphyries, or hornblendophyres; and so on.
These may be subclassed by color, as
Quartz-leucophyres, light-colored quartz-porphyries;
Quartz-melaphyres, dark-colored quartz-porphyries;
Feldspar-leucophyres;
Feldspar-melaphyres; and so on.
III. The glasses are classified, according to color and luster, into
obsidians or pitchstones when dark and lustrous; perlites, when a spheroidal
fracture gives them a pearly appearance; and pumice when greatly inflated
by included gases.
Page 535
In general discussions, it is regarded as serviceable to use the term
granitoids in a broad generic sense, to include all crystalline rocks of the
general granitoid type, including the granites, syenites, gneisses, etc. In a
similar broad way, the term gabbroids may be used to include the dark
crystalline rocks in which the ferromagnesian minerals predominate, as the
diorites, gabbros, dolerites, peridotites, etc. In this convenient and
comprehensive way, two contrasted groups of igneous rocks may be
designated. As the granitoids are usually acidic and the gabbroids usually
basic, the grouping represents a broad fact of importance.
THE PROPOSED QUANTITATIVE SYSTEM.
The distinguishing characteristic of the more rigorous system designed to
meet the needs of scientific petrology is its quantitative chemical character.
All igneous rocks are classified primarily according to their chemical
composition and only secondarily according to their mineral constituents,
texture, and other characters. The rigorous application of the system
requires chemical analyses of the rocks, but as these are not available in
many cases, the authors of the system have devised a method of optical
mineral analysis by which the nearly exact proportions of all the constituent
minerals can be determined, and by knowledge of their chemical nature the
results may be converted, by computation, into chemical terms. This can
only be done for holocrystalline rocks whose crystals are large enough to be
measured under the microscope, but aphanitic rocks may often be
approximately classified by comparison with similar rocks already
accurately determined. To facilitate this method of chemical analysis by
measuring the minerals, the chemical composition of certain common rock-
making minerals is expressed in proportional parts and tabulated, and is
used somewhat as molecular weight is in ordinary chemical analysis.
Certain of these are selected as standard minerals, the selection being such
that the standard minerals embrace all the essential elements that enter into
the composition of rocks. All other minerals are converted into their
chemical equivalents in terms of these standard minerals by the use of the
tables. All the mineral constituents being thus reduced to standard minerals,
the classification is built up systematically on these standard (or
standardized) minerals.
granitoids in a broad generic sense, to include all crystalline rocks of the
general granitoid type, including the granites, syenites, gneisses, etc. In a
similar broad way, the term gabbroids may be used to include the dark
crystalline rocks in which the ferromagnesian minerals predominate, as the
diorites, gabbros, dolerites, peridotites, etc. In this convenient and
comprehensive way, two contrasted groups of igneous rocks may be
designated. As the granitoids are usually acidic and the gabbroids usually
basic, the grouping represents a broad fact of importance.
THE PROPOSED QUANTITATIVE SYSTEM.
The distinguishing characteristic of the more rigorous system designed to
meet the needs of scientific petrology is its quantitative chemical character.
All igneous rocks are classified primarily according to their chemical
composition and only secondarily according to their mineral constituents,
texture, and other characters. The rigorous application of the system
requires chemical analyses of the rocks, but as these are not available in
many cases, the authors of the system have devised a method of optical
mineral analysis by which the nearly exact proportions of all the constituent
minerals can be determined, and by knowledge of their chemical nature the
results may be converted, by computation, into chemical terms. This can
only be done for holocrystalline rocks whose crystals are large enough to be
measured under the microscope, but aphanitic rocks may often be
approximately classified by comparison with similar rocks already
accurately determined. To facilitate this method of chemical analysis by
measuring the minerals, the chemical composition of certain common rock-
making minerals is expressed in proportional parts and tabulated, and is
used somewhat as molecular weight is in ordinary chemical analysis.
Certain of these are selected as standard minerals, the selection being such
that the standard minerals embrace all the essential elements that enter into
the composition of rocks. All other minerals are converted into their
chemical equivalents in terms of these standard minerals by the use of the
tables. All the mineral constituents being thus reduced to standard minerals,
the classification is built up systematically on these standard (or
standardized) minerals.
Page 536
A new system of names is required, and these have been very skillfully
formed by selecting significant letters from the names of the leading
minerals or from words signifying their preponderance, so that short terms
which carry their meaning in their forms, are secured, and this has been
done so that these are usually euphonious, however strange they may seem
to our preoccupied senses. For example, minerals composed chiefly of
silica and alumina are called salic; those of ferromagnesian minerals, femic;
those of aluminous ferromagnesian minerals, alferric, etc. When in a
combination of salic and femic minerals, the salic are extremely abundant,
the rock is persalic; if notably dominant, dosalic; if the salic and femic
minerals are nearly equal, salfemic; if the femic are dominant, dofemic; if
extremely abundant, perfemic, and so on, the system being mnemonic. This
method of deriving names is applicable only to a portion of the necessary
divisions. For the rest, a series of roots derived from geographic names,
with a system of terminations, has been employed.
All standard minerals are divided into two groups of primary importance:
one of minerals characterized by alumina, as the feldspars,—orthoclase,
albite, anorthite,—leucite, nephelite, sodalite, noselite, and corundum, to
which are added the closely associated minerals, quartz and zircon. This is
called the salic group. The second group contains minerals characterized by
iron and magnesia with no alumina, as hypersthene (enstatite), acmite,
olivine, magnetite, hematite, and ilmenite, to which are added the closely
associated minerals, titanite, perofskite, rutile, apatite, and all other rock-
making minerals except those containing alumina together with iron and
magnesia. The second group is called femic.
Aluminous ferromagnesian minerals, such as hornblende, augite, mica,
etc.; are called alferric, and are not classed as standard minerals, because
their complexity of composition makes it better to treat them as though
made up of the simpler minerals of the standard list.
The composition of all igneous rocks can be expressed in terms of the
relative proportions of the two groups of the standard minerals, salic and
femic. By subdividing these groups successively on a mineral and chemical
basis, a series of classificatory divisions of greater and greater precision has
been formed. In each stage of the series, two factors only are compared, and
a simple set of ratios has been selected to limit the divisions. Assuming the
possibility of a continuous range of variable mixtures of the two factors (A
formed by selecting significant letters from the names of the leading
minerals or from words signifying their preponderance, so that short terms
which carry their meaning in their forms, are secured, and this has been
done so that these are usually euphonious, however strange they may seem
to our preoccupied senses. For example, minerals composed chiefly of
silica and alumina are called salic; those of ferromagnesian minerals, femic;
those of aluminous ferromagnesian minerals, alferric, etc. When in a
combination of salic and femic minerals, the salic are extremely abundant,
the rock is persalic; if notably dominant, dosalic; if the salic and femic
minerals are nearly equal, salfemic; if the femic are dominant, dofemic; if
extremely abundant, perfemic, and so on, the system being mnemonic. This
method of deriving names is applicable only to a portion of the necessary
divisions. For the rest, a series of roots derived from geographic names,
with a system of terminations, has been employed.
All standard minerals are divided into two groups of primary importance:
one of minerals characterized by alumina, as the feldspars,—orthoclase,
albite, anorthite,—leucite, nephelite, sodalite, noselite, and corundum, to
which are added the closely associated minerals, quartz and zircon. This is
called the salic group. The second group contains minerals characterized by
iron and magnesia with no alumina, as hypersthene (enstatite), acmite,
olivine, magnetite, hematite, and ilmenite, to which are added the closely
associated minerals, titanite, perofskite, rutile, apatite, and all other rock-
making minerals except those containing alumina together with iron and
magnesia. The second group is called femic.
Aluminous ferromagnesian minerals, such as hornblende, augite, mica,
etc.; are called alferric, and are not classed as standard minerals, because
their complexity of composition makes it better to treat them as though
made up of the simpler minerals of the standard list.
The composition of all igneous rocks can be expressed in terms of the
relative proportions of the two groups of the standard minerals, salic and
femic. By subdividing these groups successively on a mineral and chemical
basis, a series of classificatory divisions of greater and greater precision has
been formed. In each stage of the series, two factors only are compared, and
a simple set of ratios has been selected to limit the divisions. Assuming the
possibility of a continuous range of variable mixtures of the two factors (A
Page 537
and B) from an extreme composed wholly of one (A), and an extreme
composed wholly of the other (B), five ideal cases have been chosen as
types or centerpoints about which variation in mixture may take place.
These are:
composed wholly of the other (B), five ideal cases have been chosen as
types or centerpoints about which variation in mixture may take place.
These are:
Page 538
A 1 A 3 A 1 A 1 A 0
— = —, — = —, — = —, — = —, — = —,
B 0 B 1 B 1 B 3 B 1
Division lines half-way between these points occur as the following ratios:
A 7 A 7 5 A 5 3 A 3 1 A 1
(1) — > —, (2) — < — > —, (3) — < — > —, (4) — < — > —, (5) — < —.
B 1 B 1 3 B 3 5 B 5 7 B 7
These ratios are used throughout the system. In (1) A is extreme; in (5) B is extreme; in (2) A
dominates over B; in (4) B dominates over A; in (3) A and B are equal or nearly equal.
All igneous rocks are grouped in five (5) primary divisions called Classes on a basis of the
proportions of the salic and femic minerals, thus:
Sal 7
Class I. —— > —, extremely rich in salic minerals, called persalane.
Fem 1
Sal 7 5
II. —— < — > —, with dominant salic minerals, called dosalane.
Fem 1 3
Sal 5 3
III. —— < — > —, salic and femic minerals, equal or nearly equal, called salfemane.
Fem 3 5
Sal 3 1
IV. —— < — > —, with dominant femic minerals, called dofemane.
Fem 5 7
Sal 1
V. —— < —, extremely rich in femic minerals, called perfemane.
Fem 7
Each of these classes is divided into two subclasses according to the proportions of two
subgroups of the preponderant group of standard minerals. Of salic minerals one subgroup
includes quartz, feldspars, and the feldspathoids; the other includes corundum and zircon. Of
femic minerals one subgroup includes the silicates with magnetite, ilmenite, hematite, and rutile;
the other contains apatite and the remaining minerals of this group. Most known igneous rocks fall
into the first subclass of each class.
The classes are further divided into orders according to the proportions of certain minerals in
the preponderant subgroups. Thus Classes I, II, and III are each divided into nine orders on a basis
of the proportions of quartz and the feldspars, and of the feldspars and the feldspathoids, quartz
and feldspathoids not occurring together. The orders may be described in the same terms for each
of the first three classes as follows:
Q 7
Order I. — > —, extremely rich in quartz, perquaric.
F 1
— = —, — = —, — = —, — = —, — = —,
B 0 B 1 B 1 B 3 B 1
Division lines half-way between these points occur as the following ratios:
A 7 A 7 5 A 5 3 A 3 1 A 1
(1) — > —, (2) — < — > —, (3) — < — > —, (4) — < — > —, (5) — < —.
B 1 B 1 3 B 3 5 B 5 7 B 7
These ratios are used throughout the system. In (1) A is extreme; in (5) B is extreme; in (2) A
dominates over B; in (4) B dominates over A; in (3) A and B are equal or nearly equal.
All igneous rocks are grouped in five (5) primary divisions called Classes on a basis of the
proportions of the salic and femic minerals, thus:
Sal 7
Class I. —— > —, extremely rich in salic minerals, called persalane.
Fem 1
Sal 7 5
II. —— < — > —, with dominant salic minerals, called dosalane.
Fem 1 3
Sal 5 3
III. —— < — > —, salic and femic minerals, equal or nearly equal, called salfemane.
Fem 3 5
Sal 3 1
IV. —— < — > —, with dominant femic minerals, called dofemane.
Fem 5 7
Sal 1
V. —— < —, extremely rich in femic minerals, called perfemane.
Fem 7
Each of these classes is divided into two subclasses according to the proportions of two
subgroups of the preponderant group of standard minerals. Of salic minerals one subgroup
includes quartz, feldspars, and the feldspathoids; the other includes corundum and zircon. Of
femic minerals one subgroup includes the silicates with magnetite, ilmenite, hematite, and rutile;
the other contains apatite and the remaining minerals of this group. Most known igneous rocks fall
into the first subclass of each class.
The classes are further divided into orders according to the proportions of certain minerals in
the preponderant subgroups. Thus Classes I, II, and III are each divided into nine orders on a basis
of the proportions of quartz and the feldspars, and of the feldspars and the feldspathoids, quartz
and feldspathoids not occurring together. The orders may be described in the same terms for each
of the first three classes as follows:
Q 7
Order I. — > —, extremely rich in quartz, perquaric.
F 1
Page 539
Q 7 5
II. — < — > —, quartz dominant over feldspar, doquaric.
F 1 3
Q 5 3
III. — < — > —, quartz and feldspar equal or nearly equal, quarfelic.
F 3 5
Q 3 1
IV. — < — > —, feldspar dominant over quartz, quardofelic.
F 5 7
Q or L 1
V. ——— < —, extremely rich in feldspar, perfelic.
F 7
L 5 3
VII. — < — > —, feldspar and lenads equal or nearly equal, lenfelic.
F 3 5
L 7 5
VIII. — < — > —, lenads dominant over feldspars, dolenic.
F 1 3
L 7
IX. — > —, extremely rich in lenads, perlenic.
F 1
In classes IV and V the preponderant minerals are femic, and in subclass 1 they are silicates,
titanates, and ferrates, with hematite and rutile. These are subdivided as follows:
Silicates—pyroxenes and olivine with akermanite in one subgroup; the other minerals,
magnetite, hematite, ilmenite, titanite, perofskite, rutile, in the second subgroup. This first group is
called polic, mnemonic of pyroxene and olivine; the second group is called mitic, mnemonic of
magnetite, ilmenite, titanite.
There are five orders in each of these classes, as follows:
PO 7
Order I. — > —, extremely rich in pyroxene or olivine, perpolic.
M 1
PO 7 5
II. — < — > —, dominant pyroxene or olivine, dopolic.
M 1 3
PO 5 3
—, pyroxene or olivine, equal or nearly equal to the mitic minerals,
III. — < — >
polmitic.
M 3 5
II. — < — > —, quartz dominant over feldspar, doquaric.
F 1 3
Q 5 3
III. — < — > —, quartz and feldspar equal or nearly equal, quarfelic.
F 3 5
Q 3 1
IV. — < — > —, feldspar dominant over quartz, quardofelic.
F 5 7
Q or L 1
V. ——— < —, extremely rich in feldspar, perfelic.
F 7
L 5 3
VII. — < — > —, feldspar and lenads equal or nearly equal, lenfelic.
F 3 5
L 7 5
VIII. — < — > —, lenads dominant over feldspars, dolenic.
F 1 3
L 7
IX. — > —, extremely rich in lenads, perlenic.
F 1
In classes IV and V the preponderant minerals are femic, and in subclass 1 they are silicates,
titanates, and ferrates, with hematite and rutile. These are subdivided as follows:
Silicates—pyroxenes and olivine with akermanite in one subgroup; the other minerals,
magnetite, hematite, ilmenite, titanite, perofskite, rutile, in the second subgroup. This first group is
called polic, mnemonic of pyroxene and olivine; the second group is called mitic, mnemonic of
magnetite, ilmenite, titanite.
There are five orders in each of these classes, as follows:
PO 7
Order I. — > —, extremely rich in pyroxene or olivine, perpolic.
M 1
PO 7 5
II. — < — > —, dominant pyroxene or olivine, dopolic.
M 1 3
PO 5 3
—, pyroxene or olivine, equal or nearly equal to the mitic minerals,
III. — < — >
polmitic.
M 3 5
Page 540
PO 3 1
IV. — < — > —, dominant mitic minerals, domitic.
M 5 7
PO 1
V. — < —, extremely rich in mitic minerals, permitic.
M 7
In the first three orders a distinction between pyroxene and olivine is recognized by sections,
five in number:
P 7
Section 1. — > —, extremely rich in pyroxene, perpyric.
O 1
P 7 5
2. — < — > —, dominant pyroxene, dopyric.
O 1 3
P 5 3
3. — < — > —, pyroxene and olivine, equal or nearly equal, pyrolic.
O 3 5
P 3 1
4. — < — > —, dominant olivine, domolic.
O 5 7
P 1
5. — < —, extremely rich in olivine, perolic.
O 7
In the last two orders a distinction between the preponderant mitic minerals is recognized by
suborders, five in number. The minerals containing Fe2O3 are compared with those containing
TiO2. The former, magnetite and hematite, are called hemic, mnemonic of hematite; the latter
subgroup, titanite, ilmenite, perofskite, rutile, are called tilic, mnemonic of titanite and ilmenite.
Of orders 4 and 5, there are
H 7
Suborder 1. — > —, hemic minerals extreme, perhemic.
T 1
H 7 5
2. — < — > —, dominant hemic minerals, dohemic.
T 1 3
H 5 3
3. — < — > —, hemic and tilic minerals equal or nearly equal, tilhemic.
T 3 5
IV. — < — > —, dominant mitic minerals, domitic.
M 5 7
PO 1
V. — < —, extremely rich in mitic minerals, permitic.
M 7
In the first three orders a distinction between pyroxene and olivine is recognized by sections,
five in number:
P 7
Section 1. — > —, extremely rich in pyroxene, perpyric.
O 1
P 7 5
2. — < — > —, dominant pyroxene, dopyric.
O 1 3
P 5 3
3. — < — > —, pyroxene and olivine, equal or nearly equal, pyrolic.
O 3 5
P 3 1
4. — < — > —, dominant olivine, domolic.
O 5 7
P 1
5. — < —, extremely rich in olivine, perolic.
O 7
In the last two orders a distinction between the preponderant mitic minerals is recognized by
suborders, five in number. The minerals containing Fe2O3 are compared with those containing
TiO2. The former, magnetite and hematite, are called hemic, mnemonic of hematite; the latter
subgroup, titanite, ilmenite, perofskite, rutile, are called tilic, mnemonic of titanite and ilmenite.
Of orders 4 and 5, there are
H 7
Suborder 1. — > —, hemic minerals extreme, perhemic.
T 1
H 7 5
2. — < — > —, dominant hemic minerals, dohemic.
T 1 3
H 5 3
3. — < — > —, hemic and tilic minerals equal or nearly equal, tilhemic.
T 3 5
Page 541
H 3 1
4. — < — > —, dominant tilic minerals, dotilic.
T 5 7
H 1
5. — < —, tilic minerals extreme, pertilic.
T 7
Further subdivision, producing rangs and subrangs, is made on the character of the chemical
bases in the standard minerals used in forming orders and is expressed in terms of the molecular
proportions of certain oxides. For the salic minerals, forming orders in the first three classes, the
bases are alkalies—K2O and Na2O—and lime, CaO. For the femic minerals, forming orders in the
last two classes, the bases are MgO, FeO, CaO and alkalies, K2O, Na2O. In classes I, II, and III
rangs are formed by comparing salic alkalies, K2O′ + Na2O′, with salic lime, CaO′; and subrangs
are formed by comparing K2O′ with Na2O′.
K2O′ + Na2O′ 7
Rang 1. —————— > —, alkalies extreme, peralkalic.
CaO′ 1
7 5
2. “ < — > —, alkalies dominant, domalkalic.
1 3
5 3
3. “ < — > —, alkalies and lime equal or nearly so, alkalicalcic.
3 5
3 1
4. “ < — > —, lime dominant, docalcic.
5 7
1
5. “ < —, lime extreme, percalcic.
7
K2O′ 7
Subrang 1. ——— > —, potash extreme, perpotassic.
Na2O′ 1
7 5
2. “ < — > —, potash dominant, dopotassic.
1 3
5 3
3. “ < — > —, potash and soda equal, sodipotassic.
3 5
4. — < — > —, dominant tilic minerals, dotilic.
T 5 7
H 1
5. — < —, tilic minerals extreme, pertilic.
T 7
Further subdivision, producing rangs and subrangs, is made on the character of the chemical
bases in the standard minerals used in forming orders and is expressed in terms of the molecular
proportions of certain oxides. For the salic minerals, forming orders in the first three classes, the
bases are alkalies—K2O and Na2O—and lime, CaO. For the femic minerals, forming orders in the
last two classes, the bases are MgO, FeO, CaO and alkalies, K2O, Na2O. In classes I, II, and III
rangs are formed by comparing salic alkalies, K2O′ + Na2O′, with salic lime, CaO′; and subrangs
are formed by comparing K2O′ with Na2O′.
K2O′ + Na2O′ 7
Rang 1. —————— > —, alkalies extreme, peralkalic.
CaO′ 1
7 5
2. “ < — > —, alkalies dominant, domalkalic.
1 3
5 3
3. “ < — > —, alkalies and lime equal or nearly so, alkalicalcic.
3 5
3 1
4. “ < — > —, lime dominant, docalcic.
5 7
1
5. “ < —, lime extreme, percalcic.
7
K2O′ 7
Subrang 1. ——— > —, potash extreme, perpotassic.
Na2O′ 1
7 5
2. “ < — > —, potash dominant, dopotassic.
1 3
5 3
3. “ < — > —, potash and soda equal, sodipotassic.
3 5
Page 542
3 1
4. “ < — > —, soda dominant, dosodic.
5 7
1
5. “ < —, soda extreme, persodic.
7
In classes IV and V rangs are formed by comparing femic MgO + FeO + CaO″ with femic
alkalies K2O″ + Na2O″.
Minerals containing magnesia, iron, and lime are called mirlic.
MgO + FeO + CaO″ 7
Rang 1. ———————— > —, extremely mirlic, permirlic.
K2O″ + Na2O″ 1
7 5
2. “ < — > —, dominantly mirlic, domirlic.
1 3
5 3
3. “ < — > —, equally mirlic and alkalic, alkalimirlic.
3 5
3 1
4. “ < — > —, dominantly alkalic, domalkalic.
5 7
1
5. “ < —, extremely alkalic, peralkalic.
7
Sections of rangs distinguish between MgO + FeO and CaO″. Minerals with MgO + FeO are
called miric.
MgO + FeO 7
Section 1. ————— > —, extremely mirlic, permirlic.
CaO″ 1
7 5
2. “ < — > —, dominantly miric, domiric.
1 3
5 3
3. “ < — > —, equally miric and calcic, calcimiric.
3 5
3 1
4. “ < — > —, dominantly calcic, docalcic.
5 7
4. “ < — > —, soda dominant, dosodic.
5 7
1
5. “ < —, soda extreme, persodic.
7
In classes IV and V rangs are formed by comparing femic MgO + FeO + CaO″ with femic
alkalies K2O″ + Na2O″.
Minerals containing magnesia, iron, and lime are called mirlic.
MgO + FeO + CaO″ 7
Rang 1. ———————— > —, extremely mirlic, permirlic.
K2O″ + Na2O″ 1
7 5
2. “ < — > —, dominantly mirlic, domirlic.
1 3
5 3
3. “ < — > —, equally mirlic and alkalic, alkalimirlic.
3 5
3 1
4. “ < — > —, dominantly alkalic, domalkalic.
5 7
1
5. “ < —, extremely alkalic, peralkalic.
7
Sections of rangs distinguish between MgO + FeO and CaO″. Minerals with MgO + FeO are
called miric.
MgO + FeO 7
Section 1. ————— > —, extremely mirlic, permirlic.
CaO″ 1
7 5
2. “ < — > —, dominantly miric, domiric.
1 3
5 3
3. “ < — > —, equally miric and calcic, calcimiric.
3 5
3 1
4. “ < — > —, dominantly calcic, docalcic.
5 7
Page 543
1
5. “ < —, extremely calcic, percalcic.
7
Subrangs distinguish between MgO and FeO, thus:
MgO 7
Subrang 1. —— > —, extremely magnesic, permagnesic.
FeO 1
7 5
2. “ < — > —, dominantly magnesic, domagnesic.
1 3
5 3
3. “ < — > —, equally magnesic and ferrous, magnesiferrous.
3 5
3 1
4. “ < — > —, dominantly ferrous, doferrous.
5 7
1
5. “ < —, extremely ferrous, perferrous.
7
Finally a recognition of the character of the subordinate standard minerals leads to further
subdivisions known as grads and subgrads. They only occur in classes II, III, and IV, because
these are the only ones in which the subordinate minerals are in notable amounts. Grads are
formed in a manner similar to that employed to produce orders. Thus grads in classes II and III
correspond to orders in class IV and the reverse. Subgrads are the same in form as rangs when the
difference in the treatment of salic and femic minerals is borne in mind. The names given to these
divisions, which in fact recognize only the character of the magma, are derived from geographical
localities and embrace many of those already in use, except that the names of orders are taken
from countries or nations. Specific terminations indicate the place in the series of divisions:
ane for class, one for subclass.
are for order, ore for suborder.
ase for rang, ose for subrang.
ate for grad, ote for subgrad.
This may be illustrated as follows:
Class I. persalane, all rocks extremely salic.
Order 4. britannare, feldspar dominant over quartz, quardofelic. Many rocks of granitic
composition whether crystalline or glassy.
Rang 1. liparase, peralkalic, rocks in which the potential feldspars are extremely alkalic,
orthoclase, or albite.
5. “ < —, extremely calcic, percalcic.
7
Subrangs distinguish between MgO and FeO, thus:
MgO 7
Subrang 1. —— > —, extremely magnesic, permagnesic.
FeO 1
7 5
2. “ < — > —, dominantly magnesic, domagnesic.
1 3
5 3
3. “ < — > —, equally magnesic and ferrous, magnesiferrous.
3 5
3 1
4. “ < — > —, dominantly ferrous, doferrous.
5 7
1
5. “ < —, extremely ferrous, perferrous.
7
Finally a recognition of the character of the subordinate standard minerals leads to further
subdivisions known as grads and subgrads. They only occur in classes II, III, and IV, because
these are the only ones in which the subordinate minerals are in notable amounts. Grads are
formed in a manner similar to that employed to produce orders. Thus grads in classes II and III
correspond to orders in class IV and the reverse. Subgrads are the same in form as rangs when the
difference in the treatment of salic and femic minerals is borne in mind. The names given to these
divisions, which in fact recognize only the character of the magma, are derived from geographical
localities and embrace many of those already in use, except that the names of orders are taken
from countries or nations. Specific terminations indicate the place in the series of divisions:
ane for class, one for subclass.
are for order, ore for suborder.
ase for rang, ose for subrang.
ate for grad, ote for subgrad.
This may be illustrated as follows:
Class I. persalane, all rocks extremely salic.
Order 4. britannare, feldspar dominant over quartz, quardofelic. Many rocks of granitic
composition whether crystalline or glassy.
Rang 1. liparase, peralkalic, rocks in which the potential feldspars are extremely alkalic,
orthoclase, or albite.
Page 544
Subrang 2. Omeose, dopotassic, rocks in which the extremely alkali feldspars are dominantly
potassic, orthoclase, with subordinate albite. Examples of omeose are: granite from Omeo,
Victoria, Australia, and rhyolite from Silver Cliff, Colorado.
The presence of distinctive minerals not indicated in the standard mineral composition of norm
is expressed by qualifying the magmatic name by the name of the distinctive mineral; as, a
hornblende-monzonose.
The precise texture of the rock is expressed by qualifying the magmatic name by a textural
adjective; as, a grano-monzonose, a vitro-monzonose, a phyro-monzonose, etc.
REFERENCE LIST OF THE MORE COMMON MINERALS.
Actinolite—a magnesium-calcium-iron amphibole (q.v.); commonly bright green to grayish
green; crystals usually slender or fibrous.
Agate—a banded or variegated chalcedony (quartz, q.v.).
Alabaster—a fine-grained variety of gypsum (q.v.), either white or delicately colored.
Albite—a soda feldspar (q.v.), an aluminum-sodium silicate; H. 5–6; cleavage perfect in two
planes; luster vitreous or pearly white; occasionally bluish gray, reddish, greenish; sometimes
opalescent.
Amethyst—a variety of quartz of purple or bluish-violet color, due probably to manganese.
Amphibole—the type of an important group of rock-forming minerals known as the amphibole
or hornblende group; a ferromagnesian silicate, monoclinic, H. 5–6; luster vitreous to pearly;
fibrous varieties often silky; black, ranging through various shades of green to light colors;
embraces the magnesium-calcium varieties, tremolite and nephrite; the magnesium-calcium-iron
variety actinolite; the aluminous-magnesium-iron-calcium variety hornblende, and others.
Analcite—analcine, one of the zeolites; a hydrous aluminum-sodium silicate; luster vitreous,
colorless, white; occasionally grayish, greenish, yellowish, reddish, transparent to opaque.
Andesine—a plagioclase feldspar (q.v.); a sodium-calcium-aluminum silicate, intermediate in
composition between albite and anorthite; H. 5–6; white, gray, grayish, yellowish, flesh red; luster
subvitreous, inclining to pearly.
Andalusite—an aluminum silicate; luster vitreous; whitish, rose red, flesh red, variety pearly
gray, reddish brown, olive-green; H. 7.5, infusible; impurities sometimes so arranged in the
interior as to exhibit a colored, crossed, or tesselated appearance in cross-section (chiastolite).
Anhydrite—a calcium sulphate; H. 3–3.5; luster pearly to vitreous; white, sometimes bluish or
reddish; differs from gypsum in absence of water and in its greater hardness.
Anorthite—a plagioclase feldspar (q.v.); a calcium-aluminum silicate; varies much by
impurities and admixtures; H. 6–6.5; pearly or vitreous luster; white, grayish, reddish.
Anthracite—hard coal; hydrocarbon with impurities; supposed to be derived from bituminous
coal by metamorphism.
Antimony—a native metal, tin-white, brittle; rather rare in native form.
potassic, orthoclase, with subordinate albite. Examples of omeose are: granite from Omeo,
Victoria, Australia, and rhyolite from Silver Cliff, Colorado.
The presence of distinctive minerals not indicated in the standard mineral composition of norm
is expressed by qualifying the magmatic name by the name of the distinctive mineral; as, a
hornblende-monzonose.
The precise texture of the rock is expressed by qualifying the magmatic name by a textural
adjective; as, a grano-monzonose, a vitro-monzonose, a phyro-monzonose, etc.
REFERENCE LIST OF THE MORE COMMON MINERALS.
Actinolite—a magnesium-calcium-iron amphibole (q.v.); commonly bright green to grayish
green; crystals usually slender or fibrous.
Agate—a banded or variegated chalcedony (quartz, q.v.).
Alabaster—a fine-grained variety of gypsum (q.v.), either white or delicately colored.
Albite—a soda feldspar (q.v.), an aluminum-sodium silicate; H. 5–6; cleavage perfect in two
planes; luster vitreous or pearly white; occasionally bluish gray, reddish, greenish; sometimes
opalescent.
Amethyst—a variety of quartz of purple or bluish-violet color, due probably to manganese.
Amphibole—the type of an important group of rock-forming minerals known as the amphibole
or hornblende group; a ferromagnesian silicate, monoclinic, H. 5–6; luster vitreous to pearly;
fibrous varieties often silky; black, ranging through various shades of green to light colors;
embraces the magnesium-calcium varieties, tremolite and nephrite; the magnesium-calcium-iron
variety actinolite; the aluminous-magnesium-iron-calcium variety hornblende, and others.
Analcite—analcine, one of the zeolites; a hydrous aluminum-sodium silicate; luster vitreous,
colorless, white; occasionally grayish, greenish, yellowish, reddish, transparent to opaque.
Andesine—a plagioclase feldspar (q.v.); a sodium-calcium-aluminum silicate, intermediate in
composition between albite and anorthite; H. 5–6; white, gray, grayish, yellowish, flesh red; luster
subvitreous, inclining to pearly.
Andalusite—an aluminum silicate; luster vitreous; whitish, rose red, flesh red, variety pearly
gray, reddish brown, olive-green; H. 7.5, infusible; impurities sometimes so arranged in the
interior as to exhibit a colored, crossed, or tesselated appearance in cross-section (chiastolite).
Anhydrite—a calcium sulphate; H. 3–3.5; luster pearly to vitreous; white, sometimes bluish or
reddish; differs from gypsum in absence of water and in its greater hardness.
Anorthite—a plagioclase feldspar (q.v.); a calcium-aluminum silicate; varies much by
impurities and admixtures; H. 6–6.5; pearly or vitreous luster; white, grayish, reddish.
Anthracite—hard coal; hydrocarbon with impurities; supposed to be derived from bituminous
coal by metamorphism.
Antimony—a native metal, tin-white, brittle; rather rare in native form.
Page 545
Apatite—essentially calcium phosphate with chlorine or fluorine; hexagonal; H. 5; luster
vitreous or subresinous; colors usually greenish to bluish, characterized by a hexagonal form.
Aragonite—a calcium carbonate; differs from calcite in cleavage, and in being orthorhombic;
H. 3.5–4; luster vitreous or resinous; white, also gray, yellow, green, and violet.
Asphaltum—asphalt; mineral pitch, bitumen; a natural mixture of different hydrocarbons; odor
bituminous; melts at 90 to 100 degrees C.; burns with a bright flame; graduates into mineral tars
and through these into petroleum; probably the residue of the latter.
Augite—one of the pyroxenes (q.v.); an aluminum-calcium-magnesium-iron silicate; H. 5–6;
monoclinic, crystals usually thick and stout; sometimes lamellar; also granular; black, greenish
black, deep green; an important rock-forming mineral.
Beauxite—essentially hydrated alumina; occurs in concretionary grains of clay-like form,
whitish to brown; valuable as a source of aluminum.
Beryl—a beryllium-aluminum silicate; hexagonal; prismatic; H. 8; luster vitreous or resinous;
marl-green, pale passing into whitish; closely resembles apatite, but distinguished by superior
hardness and in composition.
Barite—barites, heavy-spar, barium sulphate; orthorhombic, H. 3–3.5; luster vitreous to
resinous, sometimes pearly; white, inclining to yellow, gray, blue, red, or brown; very heavy, sp.
sr. 4.3–4.7.
Biotite—black mica, a potash-aluminum-magnesium-iron silicate; monoclinic; easy basal
cleavage into thin laminæ; sometimes occurs as a massive aggregation of cleavable scales; H. 2.5–
3; luster splendent on cleavage surface; black to dark green; cleavage surfaces smooth and
shining; a very common constituent of crystalline rocks.
Bitumen—the same as asphaltum (q.v.).
Bismuth—a metal of whitish color and rather brittle nature; occurring occasionally native,
usually as an ore.
Bronzite—a variety of enstatite (q.v.); grayish green to olive-green and brown with luster on
cleavage surface often adamantine, pearly or bronze-like and submetallic.
Calcite—calcspar; calcium carbonate; rhombohedral, perfect rhombohedral cleavage; often
taking the forms known as dogtooth spar, nail-head spar; frequently stalactitic and stalagmitic; H.
2.5–3.5; luster vitreous; white, occasionally pale shades of gray, red, green, blue, violet, yellow,
brown; strong double refraction; embraces variety called Iceland spar; a very common mineral;
the essential basis of limestone.
Cassiterite—tin stone; an oxide of tin; tetragonal; luster adamantine, usually splendent; brown
or black, sometimes red, gray, white, or yellow; an important source of tin.
Catlinite—essentially a hardened red clay, rather a rock than a mineral; much prized by Indians
for pipes.
Chalcedony—a cryptocrystalline variety of quartz having a wax-like luster, either transparent
or translucent; white, grayish, pale brown to dark brown, black, sometimes delicate blue,
occasionally other shades; frequently occurs as the lining or filling of cavities, taking on a
botryoidal or mamillary form.
Chiastolite—andalusite (q.v.).
vitreous or subresinous; colors usually greenish to bluish, characterized by a hexagonal form.
Aragonite—a calcium carbonate; differs from calcite in cleavage, and in being orthorhombic;
H. 3.5–4; luster vitreous or resinous; white, also gray, yellow, green, and violet.
Asphaltum—asphalt; mineral pitch, bitumen; a natural mixture of different hydrocarbons; odor
bituminous; melts at 90 to 100 degrees C.; burns with a bright flame; graduates into mineral tars
and through these into petroleum; probably the residue of the latter.
Augite—one of the pyroxenes (q.v.); an aluminum-calcium-magnesium-iron silicate; H. 5–6;
monoclinic, crystals usually thick and stout; sometimes lamellar; also granular; black, greenish
black, deep green; an important rock-forming mineral.
Beauxite—essentially hydrated alumina; occurs in concretionary grains of clay-like form,
whitish to brown; valuable as a source of aluminum.
Beryl—a beryllium-aluminum silicate; hexagonal; prismatic; H. 8; luster vitreous or resinous;
marl-green, pale passing into whitish; closely resembles apatite, but distinguished by superior
hardness and in composition.
Barite—barites, heavy-spar, barium sulphate; orthorhombic, H. 3–3.5; luster vitreous to
resinous, sometimes pearly; white, inclining to yellow, gray, blue, red, or brown; very heavy, sp.
sr. 4.3–4.7.
Biotite—black mica, a potash-aluminum-magnesium-iron silicate; monoclinic; easy basal
cleavage into thin laminæ; sometimes occurs as a massive aggregation of cleavable scales; H. 2.5–
3; luster splendent on cleavage surface; black to dark green; cleavage surfaces smooth and
shining; a very common constituent of crystalline rocks.
Bitumen—the same as asphaltum (q.v.).
Bismuth—a metal of whitish color and rather brittle nature; occurring occasionally native,
usually as an ore.
Bronzite—a variety of enstatite (q.v.); grayish green to olive-green and brown with luster on
cleavage surface often adamantine, pearly or bronze-like and submetallic.
Calcite—calcspar; calcium carbonate; rhombohedral, perfect rhombohedral cleavage; often
taking the forms known as dogtooth spar, nail-head spar; frequently stalactitic and stalagmitic; H.
2.5–3.5; luster vitreous; white, occasionally pale shades of gray, red, green, blue, violet, yellow,
brown; strong double refraction; embraces variety called Iceland spar; a very common mineral;
the essential basis of limestone.
Cassiterite—tin stone; an oxide of tin; tetragonal; luster adamantine, usually splendent; brown
or black, sometimes red, gray, white, or yellow; an important source of tin.
Catlinite—essentially a hardened red clay, rather a rock than a mineral; much prized by Indians
for pipes.
Chalcedony—a cryptocrystalline variety of quartz having a wax-like luster, either transparent
or translucent; white, grayish, pale brown to dark brown, black, sometimes delicate blue,
occasionally other shades; frequently occurs as the lining or filling of cavities, taking on a
botryoidal or mamillary form.
Chiastolite—andalusite (q.v.).
Page 546
Chlorite—the type of an important group of secondary minerals usually characterized by a
green color, softness and smoothness or unctuousness of feeling; they are usually aluminum-
magnesium-iron silicates, with chemically combined water; derived from several other species, as
pyroxene, amphibole, biotite, garnet, etc.; embraces a number of species, among which are
clinochlore, penninite, prochlorite, and delessite.
Chromite—chromic iron; essentially an iron chromate; isometric; luster submetallic; iron black
to brownish black; opaque; sometimes magnetic; resembles magnetite.
Chrysolite—olivine; essentially a magnesium-iron silicate; orthorhombic; H. 6–7; luster
vitreous; green, commonly olive-green, sometimes yellow, brownish, grayish green; highly
infusible; a common constituent of certain basic igneous rocks; the name olivine is more
commonly used by geologists.
Chrysotile—a delicately fibrous variety of serpentine (q.v.).
Corundum—alumina; an oxide of aluminum; H. 9; rhombohedral; large crystals usually rough;
luster vitreous; color blue, red, yellow, gray, and nearly white; purer forms of fine colors are
sapphires; the red variety is ruby, the yellow, oriental topaz, the green, emerald, and the purple,
amethyst; dark colors, with iron oxide, emery.
Delessite—a ferruginous chlorite, usually olive-green or blackish green; occurring commonly
in the cavities of amygdaloids.
Diallage—a variety of pyroxene (q.v.); H. 4; characterized by thin foliæ; usually grayish green
to grass-green, or deep green; luster on cleavage surface pearly, sometimes metalloid or brassy; an
essential mineral in the gabbros, as sometimes defined.
Elæolite—a variety of nephelite (q.v.); occurring in large coarse crystals or massive, with
greasy luster, from which the name is derived; a characteristic constituent of elæolite syenite.
Enstatite—one of the pyroxenes; essentially a magnesium silicate; orthorhombic; H. 5.5; luster
a little pearly on cleavage surface; metalloidal in the bronze variety (bronzite); grayish white,
yellowish white, greenish white to olive-green and brown; very infusible; a common mineral in
certain basic crystalline rocks.
Epidote—a complex aluminum-calcium-iron silicate of varying composition; monoclinic; H.
6–7; luster vitreous, pearly, or resinous; color usually pistachio-green, or yellowish green to
brownish green; can usually be detected by its peculiar pistachio hue, which is seldom found in
other minerals; common in many crystalline rocks, usually as a secondary product.
Feldspar—a group of minerals of the first importance in rock formation, embracing orthoclase,
microcline, albite, oligoclase, andesine, labradorite, anorthite, and numerous variations; aluminum
silicates, with either potassium, sodium, or calcium or two or more of these; crystallizes in both
the monoclinic and triclinic systems; possesses very distinct cleavage in two directions; H. 6–6.5;
range in color from white through pale yellow, red, or green, and occasionally dark; triclinic
feldspars frequently called plagioclase (see individual feldspars).
Fluorite—fluorspar; calcium fluoride; isometric, usually cubic; H. 4; luster vitreous, sometimes
splendent; white, yellow, green, rose, crimson red, violet, sky-blue, and brown; yellow, greenish,
and violet most common; occurs usually in veins or cavities in beautiful crystalline form.
Galenite—galena; lead sulphide; isometric, usually cubic; perfect cubic cleavage; luster
metallic; lead-gray; a common ore of lead; occurs in veins and layers, also as linings of cavities.
green color, softness and smoothness or unctuousness of feeling; they are usually aluminum-
magnesium-iron silicates, with chemically combined water; derived from several other species, as
pyroxene, amphibole, biotite, garnet, etc.; embraces a number of species, among which are
clinochlore, penninite, prochlorite, and delessite.
Chromite—chromic iron; essentially an iron chromate; isometric; luster submetallic; iron black
to brownish black; opaque; sometimes magnetic; resembles magnetite.
Chrysolite—olivine; essentially a magnesium-iron silicate; orthorhombic; H. 6–7; luster
vitreous; green, commonly olive-green, sometimes yellow, brownish, grayish green; highly
infusible; a common constituent of certain basic igneous rocks; the name olivine is more
commonly used by geologists.
Chrysotile—a delicately fibrous variety of serpentine (q.v.).
Corundum—alumina; an oxide of aluminum; H. 9; rhombohedral; large crystals usually rough;
luster vitreous; color blue, red, yellow, gray, and nearly white; purer forms of fine colors are
sapphires; the red variety is ruby, the yellow, oriental topaz, the green, emerald, and the purple,
amethyst; dark colors, with iron oxide, emery.
Delessite—a ferruginous chlorite, usually olive-green or blackish green; occurring commonly
in the cavities of amygdaloids.
Diallage—a variety of pyroxene (q.v.); H. 4; characterized by thin foliæ; usually grayish green
to grass-green, or deep green; luster on cleavage surface pearly, sometimes metalloid or brassy; an
essential mineral in the gabbros, as sometimes defined.
Elæolite—a variety of nephelite (q.v.); occurring in large coarse crystals or massive, with
greasy luster, from which the name is derived; a characteristic constituent of elæolite syenite.
Enstatite—one of the pyroxenes; essentially a magnesium silicate; orthorhombic; H. 5.5; luster
a little pearly on cleavage surface; metalloidal in the bronze variety (bronzite); grayish white,
yellowish white, greenish white to olive-green and brown; very infusible; a common mineral in
certain basic crystalline rocks.
Epidote—a complex aluminum-calcium-iron silicate of varying composition; monoclinic; H.
6–7; luster vitreous, pearly, or resinous; color usually pistachio-green, or yellowish green to
brownish green; can usually be detected by its peculiar pistachio hue, which is seldom found in
other minerals; common in many crystalline rocks, usually as a secondary product.
Feldspar—a group of minerals of the first importance in rock formation, embracing orthoclase,
microcline, albite, oligoclase, andesine, labradorite, anorthite, and numerous variations; aluminum
silicates, with either potassium, sodium, or calcium or two or more of these; crystallizes in both
the monoclinic and triclinic systems; possesses very distinct cleavage in two directions; H. 6–6.5;
range in color from white through pale yellow, red, or green, and occasionally dark; triclinic
feldspars frequently called plagioclase (see individual feldspars).
Fluorite—fluorspar; calcium fluoride; isometric, usually cubic; H. 4; luster vitreous, sometimes
splendent; white, yellow, green, rose, crimson red, violet, sky-blue, and brown; yellow, greenish,
and violet most common; occurs usually in veins or cavities in beautiful crystalline form.
Galenite—galena; lead sulphide; isometric, usually cubic; perfect cubic cleavage; luster
metallic; lead-gray; a common ore of lead; occurs in veins and layers, also as linings of cavities.
Page 547
Garnet—a complex silicate of varying composition, embracing aluminum, calcium,
magnesium, chromium, iron, and manganese, but usually only two or three of these are present in
abundance, and the varieties are characterized by the leading constituent; isometric, usually in
dodecahedrons or trapezohedrons; H. 6.5–7.5; luster vitreous to resinous; commonly red or brown,
sometimes yellow, white to blue, green or black; common in mica schist, gneiss, hornblende
schist; also in granite, syenite, and metamorphosed limestone.
Geyserite—a concretionary deposit of silica in the opal condition; formed about geysers; white
or grayish.
Glauconite—green-sand, a hydrous potassium-iron silicate usually impure, amorphous, or
earthy; dull olive-green or blackish, yellowish, or grayish green; opaque, commonly occurs as
grains or small aggregations.
Graphite—plumbago, black lead; a form of carbon, usually impure; rhombohedral, but rarely
appearing as a crystal; more often as thin laminæ of greasy feel; yields a black adhesive powder;
hence its common use for lead pencils; occurs in granite, gneiss, mica schist, crystalline limestone;
sometimes results from alteration of coal by heat; occasionally occurs in basaltic rocks and
meteorites.
Gypsum—a hydrous calcium sulphate; monoclinic; perfect cleavage into smooth polished
plates; occurs in a variety of forms, including fibrous and granular; H. 1.5–2; luster pearly and
shiny; white, sometimes gray, flesh-red, yellowish, and blue; impure varieties dark; crystallized
varieties include selenite, satinspar, alabaster, etc.; easily recognized by its softness and want of
effervescence with acids; occurs in beds; calcined and ground constitutes plaster of Paris.
Haüynite—a complex sodium-aluminum silicate and calcium sulphate; crystals
dodecahedrons; luster vitreous or somewhat greasy; bright blue, sky-blue, or greenish blue, or
green; occurs in certain igneous rocks, commonly associated with nephelite and leucite.
Hematite—ferric oxide, Fe2O3, iron-sesquioxide; rhombohedral, more commonly columnar,
granular, botryoidal, or stalactitic; luster metallic, sometimes earthy; iron-black, dark steel-gray,
red when earthy; gives red streak or powder; a leading iron ore, 70 percent. metallic iron when
pure; the chief source of the red color of soils and rocks generally.
Hornblende—an amphibole; name sometimes used as a synonym for amphibole; sometimes to
designate a variety under amphibole (q.v.).
Hyalite—a variety of silica in the opal condition; clear and colorless like glass, consisting of
globular concretions or crusts.
Hypersthene—one of the pyroxenes; a ferromagnesian silicate; orthorhombic; H. 5–6; luster
somewhat pearly on cleavage; surface often iridescent; dark brownish green, grayish, or greenish
black and brown; a frequent constituent of crystalline rocks.
Iceland spar—a form of transparent calcite (q.v.).
Ilmenite—menaccanite; a titanium iron oxide; rhombohedral; resembles hematite; luster
submetallic; iron-black; powder black or brownish red; occurs frequently in crystalline rocks
associated with magnetite.
Iron pyrites—pyrite (q.v.).
Kaolin—kaolinite; essentially a hydrous aluminum silicate; usually in clay-like or earthy form;
white or grayish white; often tinged with impurities; commonly arises from decomposition of
magnesium, chromium, iron, and manganese, but usually only two or three of these are present in
abundance, and the varieties are characterized by the leading constituent; isometric, usually in
dodecahedrons or trapezohedrons; H. 6.5–7.5; luster vitreous to resinous; commonly red or brown,
sometimes yellow, white to blue, green or black; common in mica schist, gneiss, hornblende
schist; also in granite, syenite, and metamorphosed limestone.
Geyserite—a concretionary deposit of silica in the opal condition; formed about geysers; white
or grayish.
Glauconite—green-sand, a hydrous potassium-iron silicate usually impure, amorphous, or
earthy; dull olive-green or blackish, yellowish, or grayish green; opaque, commonly occurs as
grains or small aggregations.
Graphite—plumbago, black lead; a form of carbon, usually impure; rhombohedral, but rarely
appearing as a crystal; more often as thin laminæ of greasy feel; yields a black adhesive powder;
hence its common use for lead pencils; occurs in granite, gneiss, mica schist, crystalline limestone;
sometimes results from alteration of coal by heat; occasionally occurs in basaltic rocks and
meteorites.
Gypsum—a hydrous calcium sulphate; monoclinic; perfect cleavage into smooth polished
plates; occurs in a variety of forms, including fibrous and granular; H. 1.5–2; luster pearly and
shiny; white, sometimes gray, flesh-red, yellowish, and blue; impure varieties dark; crystallized
varieties include selenite, satinspar, alabaster, etc.; easily recognized by its softness and want of
effervescence with acids; occurs in beds; calcined and ground constitutes plaster of Paris.
Haüynite—a complex sodium-aluminum silicate and calcium sulphate; crystals
dodecahedrons; luster vitreous or somewhat greasy; bright blue, sky-blue, or greenish blue, or
green; occurs in certain igneous rocks, commonly associated with nephelite and leucite.
Hematite—ferric oxide, Fe2O3, iron-sesquioxide; rhombohedral, more commonly columnar,
granular, botryoidal, or stalactitic; luster metallic, sometimes earthy; iron-black, dark steel-gray,
red when earthy; gives red streak or powder; a leading iron ore, 70 percent. metallic iron when
pure; the chief source of the red color of soils and rocks generally.
Hornblende—an amphibole; name sometimes used as a synonym for amphibole; sometimes to
designate a variety under amphibole (q.v.).
Hyalite—a variety of silica in the opal condition; clear and colorless like glass, consisting of
globular concretions or crusts.
Hypersthene—one of the pyroxenes; a ferromagnesian silicate; orthorhombic; H. 5–6; luster
somewhat pearly on cleavage; surface often iridescent; dark brownish green, grayish, or greenish
black and brown; a frequent constituent of crystalline rocks.
Iceland spar—a form of transparent calcite (q.v.).
Ilmenite—menaccanite; a titanium iron oxide; rhombohedral; resembles hematite; luster
submetallic; iron-black; powder black or brownish red; occurs frequently in crystalline rocks
associated with magnetite.
Iron pyrites—pyrite (q.v.).
Kaolin—kaolinite; essentially a hydrous aluminum silicate; usually in clay-like or earthy form;
white or grayish white; often tinged with impurities; commonly arises from decomposition of
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aluminous silicates, especially the feldspars; basis of pottery and china.
Labradorite—a plagioclase feldspar; essentially an aluminum-calcium-sodium silicate;
composition intermediate between that of albite and anorthite; triclinic; H. 6; luster pearly or
vitreous, gray, brown, or greenish; sometimes colorless or white; frequently shows play of colors;
important constituent of various crystalline rocks, especially of the basic class; usually associated
with a pyroxene or amphibole.
Lepidolite—lithia mica; essentially like muscovite (q.v.) except that potash is replaced by
lithia.
Leucite—essentially an aluminum-potassium silicate, allied to the feldspars; H. 5–6; luster
vitreous, white, ash-gray, or smoke-gray; occurs in certain volcanic rocks, particularly lavas of
Vesuvius.
Limonite—brown hematite, ocher;—a hydrous iron oxide; commonly earthy; also
concretionary, stalactitic, botryoidal, and mamillary, with fibrous structure; H. 5–5.5; luster silky,
sometimes submetallic, but commonly dull and earthy; brown, ocherous yellow; streak and
powder yellowish brown; constitutes ocher, bog-ore, ironstone, etc.; is the chief source of the
yellow color of soils and rocks; arises from the alteration of other iron ores.
Magnesite—magnesium carbonate; rhombohedral; white, yellowish, grayish white to brown;
fibrous, earthy, or massive; found in altered magnesium rocks.
Magnetite—magnetic iron ore; iron oxide, Fe3O4; octahedral or dodecahedral; strongly
magnetic; H. 5.5–6.5; abounds in igneous and metamorphic rocks.
Marcasite—white iron pyrites; iron sulphide; same composition as pyrite, which it closely
resembles; H. 6–6.5; luster metallic, pale gray, bronze, or yellow; prone to decomposition;
disseminated through various rocks, particularly plastic clays containing organic matter.
Martite—iron sesquioxide; originally magnetite, which by oxidation has assumed the
composition of hematite.
Mica—the type of an important group of rock-forming minerals well known for their perfect
cleavage into thin elastic laminæ; among the leading varieties are the common potassium mica
(muscovite), the sodium mica (paragonite), the lithium mica (lepidolite), the magnesium-iron mica
(biotite), the magnesium mica (phlogopite), and the iron-potash mica (lepidomelane).
Menaccanite—ilmenite; titanium iron ore (q.v.).
Microcline—a triclinic feldspar, closely resembling orthoclase in appearance and having the
same composition.
Muscovite—common or potash mica; essentially an aluminum-potassium silicate; H. 2–2.5;
monoclinic; remarkable for its basal cleavage; splits easily into exceedingly thin, flexible, elastic
laminæ; luster vitreous, more or less pearly or silky; colorless or variously tinged brown, green, or
violet; a common mineral in crystalline rocks, particularly in the granites or gneisses.
Nephelite—nepheline; essentially an aluminum-sodium silicate with potash; allied to the soda-
feldspars; hexagonal; usually in thick prisms; H. 5.5–6; luster vitreous to greasy, white or
yellowish, varying to greenish, bluish, and red; occurs in volcanic rocks; the variety elæolite
characterizes the elæolite syenite.
Nosite—nosean; a complex sodium-aluminum silicate and sulphate, like haüynite, but with
little calcium; common in phonolites.
Labradorite—a plagioclase feldspar; essentially an aluminum-calcium-sodium silicate;
composition intermediate between that of albite and anorthite; triclinic; H. 6; luster pearly or
vitreous, gray, brown, or greenish; sometimes colorless or white; frequently shows play of colors;
important constituent of various crystalline rocks, especially of the basic class; usually associated
with a pyroxene or amphibole.
Lepidolite—lithia mica; essentially like muscovite (q.v.) except that potash is replaced by
lithia.
Leucite—essentially an aluminum-potassium silicate, allied to the feldspars; H. 5–6; luster
vitreous, white, ash-gray, or smoke-gray; occurs in certain volcanic rocks, particularly lavas of
Vesuvius.
Limonite—brown hematite, ocher;—a hydrous iron oxide; commonly earthy; also
concretionary, stalactitic, botryoidal, and mamillary, with fibrous structure; H. 5–5.5; luster silky,
sometimes submetallic, but commonly dull and earthy; brown, ocherous yellow; streak and
powder yellowish brown; constitutes ocher, bog-ore, ironstone, etc.; is the chief source of the
yellow color of soils and rocks; arises from the alteration of other iron ores.
Magnesite—magnesium carbonate; rhombohedral; white, yellowish, grayish white to brown;
fibrous, earthy, or massive; found in altered magnesium rocks.
Magnetite—magnetic iron ore; iron oxide, Fe3O4; octahedral or dodecahedral; strongly
magnetic; H. 5.5–6.5; abounds in igneous and metamorphic rocks.
Marcasite—white iron pyrites; iron sulphide; same composition as pyrite, which it closely
resembles; H. 6–6.5; luster metallic, pale gray, bronze, or yellow; prone to decomposition;
disseminated through various rocks, particularly plastic clays containing organic matter.
Martite—iron sesquioxide; originally magnetite, which by oxidation has assumed the
composition of hematite.
Mica—the type of an important group of rock-forming minerals well known for their perfect
cleavage into thin elastic laminæ; among the leading varieties are the common potassium mica
(muscovite), the sodium mica (paragonite), the lithium mica (lepidolite), the magnesium-iron mica
(biotite), the magnesium mica (phlogopite), and the iron-potash mica (lepidomelane).
Menaccanite—ilmenite; titanium iron ore (q.v.).
Microcline—a triclinic feldspar, closely resembling orthoclase in appearance and having the
same composition.
Muscovite—common or potash mica; essentially an aluminum-potassium silicate; H. 2–2.5;
monoclinic; remarkable for its basal cleavage; splits easily into exceedingly thin, flexible, elastic
laminæ; luster vitreous, more or less pearly or silky; colorless or variously tinged brown, green, or
violet; a common mineral in crystalline rocks, particularly in the granites or gneisses.
Nephelite—nepheline; essentially an aluminum-sodium silicate with potash; allied to the soda-
feldspars; hexagonal; usually in thick prisms; H. 5.5–6; luster vitreous to greasy, white or
yellowish, varying to greenish, bluish, and red; occurs in volcanic rocks; the variety elæolite
characterizes the elæolite syenite.
Nosite—nosean; a complex sodium-aluminum silicate and sulphate, like haüynite, but with
little calcium; common in phonolites.
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Oligoclase—a plagioclase feldspar; essentially an aluminum-calcium-sodium silicate which
may be regarded as a mixture of albite and a small amount of anorthite; triclinic; luster vitreous,
pearly, or waxy; whitish grading into greenish and reddish; H. 6–7; common in crystalline rocks.
Orthoclase—a potash feldspar; essentially a potassium-aluminum silicate; varying by the
replacement of the potassium by sodium and less frequently by other substitutions; monoclinic;
occurring in distinct crystals and also in cryptocrystalline forms; cleavage planes perfect with
pearly luster on cleavage surface; white, gray, and flesh-red, occasionally varying to greenish
white and bright green; H. 6–6.5; difficultly fusible; sanidine a glassy variety; felsite a
cryptocrystalline form; a very common mineral, especially in the granites and gneisses.
Olivine—chrysolite (q.v.).
Omphacite—a variety of pyroxene of grass-green color and silky to fibrous luster; allied to
diallage.
Opal—silica with a varying amount of water; differs from quartz in a lack of crystallization and
in lower degree of hardness; amorphous, massive; sometimes reniform, stalactitic, or tuberous;
also earthy; H. 5.5–6.5; luster vitreous, inclining to resinous; white, yellow, red, brown, green,
gray, blue, generally pale; colors arise from admixtures; sometimes play of colors as in precious
opal.
Ozocerite—a native paraffine, mineral wax.
Petroleum—naphtha; a native mineral oil; a hydrocarbon, commonly believed to arise from
organic matter, both animal and vegetable, but held by some to be due to deep-seated chemical
and thermal action.
Pictotite—a variety of spinel, containing chromium.
Pisolite—a concretionary variety of calcite.
Picrolite—a variety of serpentine.
Piedmontite—a manganese epidote.
Plagioclase—a general term embracing the triclinic feldspars whose two cleavages are oblique
to each other; embracing albite, oligoclase, andesine, labradorite, and anorthite (q.v.).
Plumbago—graphite (q.v.).
Psilomelane—essentially a hydrous manganese oxide occurring in massive, botryoidal,
reniform, and stalactitic forms; luster submetallic; iron-black, passing into dark steel-gray; H. 5–6;
the common ore of manganese.
Pseudomorph—a false form, i.e., having the form of one mineral and the composition of
another; usually arises from the replacement of a mineral, particle by particle, by a solution of
another substance, leaving the original form unchanged.
Pyrite—iron pyrites, fool’s gold, iron sulphide; isometric; commonly in cubes; H. 6–6.5; luster
metallic, splendent, or glistening; pale brass-yellow; occurs widely disseminated throughout a
large class of rocks; usually harder and lighter in color than copper pyrites, and deeper in color
than marcasite, which has the same composition.
Pyroxene—the type of a large and important group of rock-forming ferromagnesian minerals;
varies in composition and embraces a large number of varieties; usually a magnesium-iron-
calcium silicate; crystals usually thick and stout, but varying greatly; sometimes lamellar and
may be regarded as a mixture of albite and a small amount of anorthite; triclinic; luster vitreous,
pearly, or waxy; whitish grading into greenish and reddish; H. 6–7; common in crystalline rocks.
Orthoclase—a potash feldspar; essentially a potassium-aluminum silicate; varying by the
replacement of the potassium by sodium and less frequently by other substitutions; monoclinic;
occurring in distinct crystals and also in cryptocrystalline forms; cleavage planes perfect with
pearly luster on cleavage surface; white, gray, and flesh-red, occasionally varying to greenish
white and bright green; H. 6–6.5; difficultly fusible; sanidine a glassy variety; felsite a
cryptocrystalline form; a very common mineral, especially in the granites and gneisses.
Olivine—chrysolite (q.v.).
Omphacite—a variety of pyroxene of grass-green color and silky to fibrous luster; allied to
diallage.
Opal—silica with a varying amount of water; differs from quartz in a lack of crystallization and
in lower degree of hardness; amorphous, massive; sometimes reniform, stalactitic, or tuberous;
also earthy; H. 5.5–6.5; luster vitreous, inclining to resinous; white, yellow, red, brown, green,
gray, blue, generally pale; colors arise from admixtures; sometimes play of colors as in precious
opal.
Ozocerite—a native paraffine, mineral wax.
Petroleum—naphtha; a native mineral oil; a hydrocarbon, commonly believed to arise from
organic matter, both animal and vegetable, but held by some to be due to deep-seated chemical
and thermal action.
Pictotite—a variety of spinel, containing chromium.
Pisolite—a concretionary variety of calcite.
Picrolite—a variety of serpentine.
Piedmontite—a manganese epidote.
Plagioclase—a general term embracing the triclinic feldspars whose two cleavages are oblique
to each other; embracing albite, oligoclase, andesine, labradorite, and anorthite (q.v.).
Plumbago—graphite (q.v.).
Psilomelane—essentially a hydrous manganese oxide occurring in massive, botryoidal,
reniform, and stalactitic forms; luster submetallic; iron-black, passing into dark steel-gray; H. 5–6;
the common ore of manganese.
Pseudomorph—a false form, i.e., having the form of one mineral and the composition of
another; usually arises from the replacement of a mineral, particle by particle, by a solution of
another substance, leaving the original form unchanged.
Pyrite—iron pyrites, fool’s gold, iron sulphide; isometric; commonly in cubes; H. 6–6.5; luster
metallic, splendent, or glistening; pale brass-yellow; occurs widely disseminated throughout a
large class of rocks; usually harder and lighter in color than copper pyrites, and deeper in color
than marcasite, which has the same composition.
Pyroxene—the type of a large and important group of rock-forming ferromagnesian minerals;
varies in composition and embraces a large number of varieties; usually a magnesium-iron-
calcium silicate; crystals usually thick and stout, but varying greatly; sometimes lamellar and
Page 550
fibrous; H. 5–6; luster vitreous inclining to resinous; green of various shades verging towards light
colors, occasionally more often to browns and blacks; among the minerals belonging to the
pyroxene group are augite, bronzite, diallage, diopside, enstatite, hypersthene, and others.
Quartz—crystallized silica; rhombohedral; crystals commonly six-sided prisms capped by six-
sided pyramids; without cleavage; H. 7; scratches glass; usually transparent, glassy, colorless
when pure, shaded by impurities to yellow, red, brown, green, blue, and black; varieties, amethyst,
purple, or violet; false topaz, yellow, rose-quartz, smoky, milky, cat’s eye, opalescent; aventurine,
spangled with scales of mica; chalcedony is a cryptocrystalline variety; carnelian, a red
chalcedony; chrysoprase, an apple-green chalcedony; prase, a leek-green variety; agate, a
variegated or banded chalcedony; moss-agate, a chalcedony containing moss-like or dendritic
crystallizations of iron or manganese oxide; onyx, a chalcedony in layers; sardonyx, like onyx in
structure, but includes layers of sard (carnelian); jasper, an opaque-colored quartz, usually red or
brown; flint, an opaque impure chalcedony; chert, an ill-defined term applied to an impure flinty
rock; hornstone, a translucent, brittle, flinty rock.
Rutile—titanium oxide; tetragonal, crystals commonly in prisms; H. 6–6.5; luster metallic,
adamantine; reddish brown, passing to red; sometimes yellowish, bluish, violet, and black; occurs
in crystalline rocks and is a common secondary product in the form of microlites.
Sanidine—a glassy variety of orthoclase feldspar.
Satinspar—a variety of selenite or gypsum.
Selenite—a distinctly crystallized transparent form of gypsum.
Serpentine—a hydrous magnesium silicate; usually in pseudomorph forms; also fibrous,
granular, cryptocrystalline, and amorphous; H. 2.5–4; luster subresinous to greasy, pearly or
earthy, resinous or wax-like; feel, smooth and somewhat greasy; leek-green to blackish green and
siskin green verging into brownish and other colors; apparently derived most commonly from
chrysolite or olivine and also from other magnesian minerals; sometimes constitutes the bulk of
rock masses.
Siderite—iron carbonate; rhombohedral; H. 3.5–4.5; luster vitreous, more or less pearly, ash-
gray, yellowish or greenish, also brownish; occurs as extensive iron deposits and in crystalline
rocks.
Smaragdite—a form of amphibole or hornblende (q.v.).
Spherosiderite—a globular form of siderite.
Spinel—a magnesium-aluminum oxide; crystals, octahedrons; red of various shades, passing
into other colors; spinel-ruby is a variety.
Staurolite—a complex hydrous iron-magnesium-aluminum silicate; orthorhombic; disposed to
cruciform shapes; occurs in schists and gneisses.
Steatite—soapstone, a variety of talc (q.v.); a hydrous magnesium silicate.
Sulphur—a well-known element occurring native in volcanic regions; also formed by the
decomposition of sulphides, particularly pyrites.
Talc—a hydrous magnesium silicate; usually in foliæ; granular or fibrous forms; also compact;
easy cleavage into thin flexible laminaæ, but not elastic; feel greasy; luster pearly on cleavage
surface; apple-green to silvery white; H. 1–2; a secondary product from the alteration of
colors, occasionally more often to browns and blacks; among the minerals belonging to the
pyroxene group are augite, bronzite, diallage, diopside, enstatite, hypersthene, and others.
Quartz—crystallized silica; rhombohedral; crystals commonly six-sided prisms capped by six-
sided pyramids; without cleavage; H. 7; scratches glass; usually transparent, glassy, colorless
when pure, shaded by impurities to yellow, red, brown, green, blue, and black; varieties, amethyst,
purple, or violet; false topaz, yellow, rose-quartz, smoky, milky, cat’s eye, opalescent; aventurine,
spangled with scales of mica; chalcedony is a cryptocrystalline variety; carnelian, a red
chalcedony; chrysoprase, an apple-green chalcedony; prase, a leek-green variety; agate, a
variegated or banded chalcedony; moss-agate, a chalcedony containing moss-like or dendritic
crystallizations of iron or manganese oxide; onyx, a chalcedony in layers; sardonyx, like onyx in
structure, but includes layers of sard (carnelian); jasper, an opaque-colored quartz, usually red or
brown; flint, an opaque impure chalcedony; chert, an ill-defined term applied to an impure flinty
rock; hornstone, a translucent, brittle, flinty rock.
Rutile—titanium oxide; tetragonal, crystals commonly in prisms; H. 6–6.5; luster metallic,
adamantine; reddish brown, passing to red; sometimes yellowish, bluish, violet, and black; occurs
in crystalline rocks and is a common secondary product in the form of microlites.
Sanidine—a glassy variety of orthoclase feldspar.
Satinspar—a variety of selenite or gypsum.
Selenite—a distinctly crystallized transparent form of gypsum.
Serpentine—a hydrous magnesium silicate; usually in pseudomorph forms; also fibrous,
granular, cryptocrystalline, and amorphous; H. 2.5–4; luster subresinous to greasy, pearly or
earthy, resinous or wax-like; feel, smooth and somewhat greasy; leek-green to blackish green and
siskin green verging into brownish and other colors; apparently derived most commonly from
chrysolite or olivine and also from other magnesian minerals; sometimes constitutes the bulk of
rock masses.
Siderite—iron carbonate; rhombohedral; H. 3.5–4.5; luster vitreous, more or less pearly, ash-
gray, yellowish or greenish, also brownish; occurs as extensive iron deposits and in crystalline
rocks.
Smaragdite—a form of amphibole or hornblende (q.v.).
Spherosiderite—a globular form of siderite.
Spinel—a magnesium-aluminum oxide; crystals, octahedrons; red of various shades, passing
into other colors; spinel-ruby is a variety.
Staurolite—a complex hydrous iron-magnesium-aluminum silicate; orthorhombic; disposed to
cruciform shapes; occurs in schists and gneisses.
Steatite—soapstone, a variety of talc (q.v.); a hydrous magnesium silicate.
Sulphur—a well-known element occurring native in volcanic regions; also formed by the
decomposition of sulphides, particularly pyrites.
Talc—a hydrous magnesium silicate; usually in foliæ; granular or fibrous forms; also compact;
easy cleavage into thin flexible laminaæ, but not elastic; feel greasy; luster pearly on cleavage
surface; apple-green to silvery white; H. 1–2; a secondary product from the alteration of
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magnesian minerals; distinguished by its soft, soapy feel, soapstone being one variety; whitish
form is known as French chalk.
Titanite—calcium-titano-silicate; monoclinic; luster adamantine to resinous; brown, gray,
yellow, green, and black; H. 5–5.5; occurs in various crystalline rocks.
Topaz—an aluminum silicate, with part of the oxygen replaced by fluorine; orthorhombic; H.
8; luster vitreous; colorless, straw-yellow verging to various pale shades, grayish, greenish, bluish,
and reddish; distinguished by its hardness and infusibility; occurs in crystalline rock.
Tremolite—a calcium-magnesium amphibole; a common constituent of certain crystalline
rocks.
Viridite—a general term used for green products of rock alteration, usually hydrous silicates of
iron and magnesia; mainly chlorite.
Wad—bog manganese; a variety of psilomelane (q.v.).
Zeolite—a group of minerals derived from the alteration of various aluminous silicates.
Zircon—zirconium silicate; H. 7.5; luster adamantine; pale yellowish, grayish, yellowish green,
brownish yellow, and reddish brown; infusible; occurs characteristically in square prismatic
forms; found in crystalline rocks and granular limestone.
REFERENCE LIST OF THE MORE COMMON ROCKS.[206]
Adobe—a fine silty or loamy deposit formed by gentle wash from slopes and subsequent
lodgment on flats; especially applied to silty accumulations in the basins and on the plains of the
western dry region.
Agglomerate—an aggregate of irregular, angular, or subangular blocks of varying sizes,
usually of volcanic origin, distinguished from conglomerate in which the constituents are rounded.
Alluvium—sediment deposited by streams.
Amygdaloid—a vesicular igneous rock whose cavities have become filled with minerals; the
fillings are called amygdules, because sometimes almond-like in form.
Andesite—an aphanitic igneous rock consisting essentially of the plagioclase feldspar andesine
(sometimes oligoclase) and pyroxene (or some related ferromagnesian mineral); sometimes
cellular, porphyritic, or even glassy; usually rich in feldspar microlites.
Anorthosite—a rock consisting mainly of the feldspar labradorite.
Aphanite—a rock whose constituents are so minute as to be indistinguishable to the naked eye;
rather a condition of various rocks than of any specific rock.
Aqueous rocks—a general term applied to rocks deposited through the agency of water.
Arenaceous rocks—either those which are mainly sand or those in which sand is a notable
accessory.
Argillite—a clayey rock; usually applied to hard varieties only.
Arkose—a sand or sandstone formed of disaggregated granite or similar rock in which a
notable part of the grains are feldspar or other silicate; sand when undefined, is understood to be
quartzose.
form is known as French chalk.
Titanite—calcium-titano-silicate; monoclinic; luster adamantine to resinous; brown, gray,
yellow, green, and black; H. 5–5.5; occurs in various crystalline rocks.
Topaz—an aluminum silicate, with part of the oxygen replaced by fluorine; orthorhombic; H.
8; luster vitreous; colorless, straw-yellow verging to various pale shades, grayish, greenish, bluish,
and reddish; distinguished by its hardness and infusibility; occurs in crystalline rock.
Tremolite—a calcium-magnesium amphibole; a common constituent of certain crystalline
rocks.
Viridite—a general term used for green products of rock alteration, usually hydrous silicates of
iron and magnesia; mainly chlorite.
Wad—bog manganese; a variety of psilomelane (q.v.).
Zeolite—a group of minerals derived from the alteration of various aluminous silicates.
Zircon—zirconium silicate; H. 7.5; luster adamantine; pale yellowish, grayish, yellowish green,
brownish yellow, and reddish brown; infusible; occurs characteristically in square prismatic
forms; found in crystalline rocks and granular limestone.
REFERENCE LIST OF THE MORE COMMON ROCKS.[206]
Adobe—a fine silty or loamy deposit formed by gentle wash from slopes and subsequent
lodgment on flats; especially applied to silty accumulations in the basins and on the plains of the
western dry region.
Agglomerate—an aggregate of irregular, angular, or subangular blocks of varying sizes,
usually of volcanic origin, distinguished from conglomerate in which the constituents are rounded.
Alluvium—sediment deposited by streams.
Amygdaloid—a vesicular igneous rock whose cavities have become filled with minerals; the
fillings are called amygdules, because sometimes almond-like in form.
Andesite—an aphanitic igneous rock consisting essentially of the plagioclase feldspar andesine
(sometimes oligoclase) and pyroxene (or some related ferromagnesian mineral); sometimes
cellular, porphyritic, or even glassy; usually rich in feldspar microlites.
Anorthosite—a rock consisting mainly of the feldspar labradorite.
Aphanite—a rock whose constituents are so minute as to be indistinguishable to the naked eye;
rather a condition of various rocks than of any specific rock.
Aqueous rocks—a general term applied to rocks deposited through the agency of water.
Arenaceous rocks—either those which are mainly sand or those in which sand is a notable
accessory.
Argillite—a clayey rock; usually applied to hard varieties only.
Arkose—a sand or sandstone formed of disaggregated granite or similar rock in which a
notable part of the grains are feldspar or other silicate; sand when undefined, is understood to be
quartzose.
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Augitite—a rock mainly made up of augite.
Basalt—a dark, compact basic igneous rock consisting of a mass of minute crystals sometimes
with more or less glassy base, often containing also visible crystals; composed of plagioclase and
pyroxene, with olivine, magnetite, or titaniferous iron as common accessories; a basic lava in
which the crystallization has taken place rapidly; usually rich in crystallites or microlites;
graduates into dolerite and basic andesite.
Bituminous coal—common soft coal, intermediate between lignite and anthracite; contains
much bituminous matter, i.e., hydrocarbons.
Bowlders—rounded masses of rock, particularly those that have been shaped by glaciers.
Breccia—a rock composed of angular fragments, contrasted with pudding-stone or
conglomerate, in which the fragments are rounded.
Buhrstone—a compact, flint-like silicious rock full of small cavities, so named from use as
millstones.
Calc-sinter (calcareous tufa)—a loose cellular deposit of calcium carbonate made by springs;
travertine is the better term, as tufa should be left for volcanic elastics.
Cannel coal—a very fine-grained homogeneous bituminous coal, giving off much gas and
burning with a candle-like flame.
Chalk—a fine-grained soft rock composed essentially of calcium carbonate derived from
minute marine organisms.
Chlorite schist—a schistose rock in which chlorite is a predominant mineral; usually greenish,
whence the name.
Clastic rock—formed from the débris of broken-down rocks; the same as fragmental or detrital
rock.
Clay—a term commonly applied to any soft, unctuous, adhesive deposit, but in strict use
confined to material composed of aluminum silicate; many so-called clays are chiefly silicious
silts or loams.
Clay ironstone—a clayey rock heavily charged with iron oxide, usually limonite; commonly in
concretionary form.
Clinkstone—a name applied to phonolite because of its metallic clinking sound when struck;
composed of orthoclase, with nephelite and one or more of the ferromagnesian minerals as
accessories.
Chert—an impure flint, usually of light color, occurring abundantly in concretionary form as
nodules in certain limestones.
Coal—a carbonaceous deposit formed from the remains of plants by partial decomposition.
Concretions—aggregates of rounded outlines formed about a nucleus; the material is various:
clay, iron ore, calcite, silica, etc.
Conglomerate (pudding-stone)—a rock formed from rounded pebbles, consolidated gravel.
Coquina—a rock formed almost wholly of small and broken shells; especially applied to a
shell limestone of Florida.
Dacite (quartz-andesite)—an andesite (q.v.) with quartz.
Basalt—a dark, compact basic igneous rock consisting of a mass of minute crystals sometimes
with more or less glassy base, often containing also visible crystals; composed of plagioclase and
pyroxene, with olivine, magnetite, or titaniferous iron as common accessories; a basic lava in
which the crystallization has taken place rapidly; usually rich in crystallites or microlites;
graduates into dolerite and basic andesite.
Bituminous coal—common soft coal, intermediate between lignite and anthracite; contains
much bituminous matter, i.e., hydrocarbons.
Bowlders—rounded masses of rock, particularly those that have been shaped by glaciers.
Breccia—a rock composed of angular fragments, contrasted with pudding-stone or
conglomerate, in which the fragments are rounded.
Buhrstone—a compact, flint-like silicious rock full of small cavities, so named from use as
millstones.
Calc-sinter (calcareous tufa)—a loose cellular deposit of calcium carbonate made by springs;
travertine is the better term, as tufa should be left for volcanic elastics.
Cannel coal—a very fine-grained homogeneous bituminous coal, giving off much gas and
burning with a candle-like flame.
Chalk—a fine-grained soft rock composed essentially of calcium carbonate derived from
minute marine organisms.
Chlorite schist—a schistose rock in which chlorite is a predominant mineral; usually greenish,
whence the name.
Clastic rock—formed from the débris of broken-down rocks; the same as fragmental or detrital
rock.
Clay—a term commonly applied to any soft, unctuous, adhesive deposit, but in strict use
confined to material composed of aluminum silicate; many so-called clays are chiefly silicious
silts or loams.
Clay ironstone—a clayey rock heavily charged with iron oxide, usually limonite; commonly in
concretionary form.
Clinkstone—a name applied to phonolite because of its metallic clinking sound when struck;
composed of orthoclase, with nephelite and one or more of the ferromagnesian minerals as
accessories.
Chert—an impure flint, usually of light color, occurring abundantly in concretionary form as
nodules in certain limestones.
Coal—a carbonaceous deposit formed from the remains of plants by partial decomposition.
Concretions—aggregates of rounded outlines formed about a nucleus; the material is various:
clay, iron ore, calcite, silica, etc.
Conglomerate (pudding-stone)—a rock formed from rounded pebbles, consolidated gravel.
Coquina—a rock formed almost wholly of small and broken shells; especially applied to a
shell limestone of Florida.
Dacite (quartz-andesite)—an andesite (q.v.) with quartz.
Page 553
Diabase—a dolerite (q.v.) which has undergone alteration; consists essentially of plagioclase
feldspar and augite, with magnetite or titaniferous iron as a common accessory; one of the
greenstones.
Diatom ooze—a soft silicious deposit found on the bottom of the deep sea, made largely or
partly of the shells of diatoms; similar deposits are formed from the shells of radiolaria.
Diorite—an igneous rock usually of dark-greenish color, consisting of plagioclase feldspar and
hornblende; often speckled from the commingling of light feldspar and dark hornblende.
Dolerite—a fine-grained igneous rock composed of plagioclase feldspar (labradorite or
anorthite) and augite (or related ferromagnesian mineral, as enstatite, olivine, or biotite), with
magnetic or titaniferous iron as common accessories; crystals usually of medium size, assuming
the ophitic structure; embraces many of the greenstones; graduates into basalt on the one hand and
gabbro on the other.
Dolomite—a magnesian limestone.
Drift—in common American usage, a mixture of clay, sand, gravel, and bowlders formed by
glacial agencies.
Eolian rocks—deposits formed by wind, embracing especially dunes and one variety of loess.
Felsite (felstone)—a light-colored aphanitic rock composed of feldspar often with quartz, in
which the crystallization is very imperfect or obscure, giving a close-grained texture with
conchoidal fracture and flinty aspect; certain varieties are called petrosilex and hälleflinta.
Flint—a compact dark chalcedonic or lithoid form of quartz.
Freestone—a sandstone of uniform grain without special tendency to split in any direction.
Fulgurites—glassy tubes, produced through fusion by lightning in penetrating sand, earth, or
rock.
Gabbro (euphotide)—a crystalline rock composed of the plagioclase feldspar, labradorite (or
anorthite), and diallage (or a related ferromagnesian mineral), with magnetite or titaniferous iron
as a common accessory.
Gangue—a term applied to the crystalline material in which ores are imbedded.
Gannister—essentially a quartz silt or pulverized quartz used for lining iron furnaces.
Garnetite—a rock composed largely of garnets.
Geest—residual earth or clay left by the decomposition of rocks, especially limestones.
Geyserite—the silicious sinter deposited about hot springs.
Globulites—minute spherical bodies embraced in volcanic glass.
Gneiss—a foliated granite, consisting typically of quartz, feldspar, and mica; the feldspar
typically orthoclase.
Granite—a granular crystalline aggregate of quartz, feldspar, and mica; the feldspar typically
orthoclase; popularly and properly used for any distinctly granular crystalline rock.
Granitell—a name used to designate a quartz-feldspar rock.
Granitite—a biotite granite with quartz.
feldspar and augite, with magnetite or titaniferous iron as a common accessory; one of the
greenstones.
Diatom ooze—a soft silicious deposit found on the bottom of the deep sea, made largely or
partly of the shells of diatoms; similar deposits are formed from the shells of radiolaria.
Diorite—an igneous rock usually of dark-greenish color, consisting of plagioclase feldspar and
hornblende; often speckled from the commingling of light feldspar and dark hornblende.
Dolerite—a fine-grained igneous rock composed of plagioclase feldspar (labradorite or
anorthite) and augite (or related ferromagnesian mineral, as enstatite, olivine, or biotite), with
magnetic or titaniferous iron as common accessories; crystals usually of medium size, assuming
the ophitic structure; embraces many of the greenstones; graduates into basalt on the one hand and
gabbro on the other.
Dolomite—a magnesian limestone.
Drift—in common American usage, a mixture of clay, sand, gravel, and bowlders formed by
glacial agencies.
Eolian rocks—deposits formed by wind, embracing especially dunes and one variety of loess.
Felsite (felstone)—a light-colored aphanitic rock composed of feldspar often with quartz, in
which the crystallization is very imperfect or obscure, giving a close-grained texture with
conchoidal fracture and flinty aspect; certain varieties are called petrosilex and hälleflinta.
Flint—a compact dark chalcedonic or lithoid form of quartz.
Freestone—a sandstone of uniform grain without special tendency to split in any direction.
Fulgurites—glassy tubes, produced through fusion by lightning in penetrating sand, earth, or
rock.
Gabbro (euphotide)—a crystalline rock composed of the plagioclase feldspar, labradorite (or
anorthite), and diallage (or a related ferromagnesian mineral), with magnetite or titaniferous iron
as a common accessory.
Gangue—a term applied to the crystalline material in which ores are imbedded.
Gannister—essentially a quartz silt or pulverized quartz used for lining iron furnaces.
Garnetite—a rock composed largely of garnets.
Geest—residual earth or clay left by the decomposition of rocks, especially limestones.
Geyserite—the silicious sinter deposited about hot springs.
Globulites—minute spherical bodies embraced in volcanic glass.
Gneiss—a foliated granite, consisting typically of quartz, feldspar, and mica; the feldspar
typically orthoclase.
Granite—a granular crystalline aggregate of quartz, feldspar, and mica; the feldspar typically
orthoclase; popularly and properly used for any distinctly granular crystalline rock.
Granitell—a name used to designate a quartz-feldspar rock.
Granitite—a biotite granite with quartz.
Page 554
Granulite—a fine-grained granite with little or no mica.
Greensand—a sand or sandstone containing a notable percentage of grains of glauconite.
Greenstone—a comprehensive term used to designate igneous and metamorphic crystalline
rocks of greenish hue and of intricate and often minute crystallization; they are mostly dolerites,
diabases, and diorites; a convenient term for field use where the constituents cannot be
determined, and for general use when the variety is unimportant.
Greisen—an aggregate of quartz and mica, i.e., a granite without feldspar.
Greywacke—a sand rock in which the grains are basic silicates instead of quartz.
Hälleflinta—a compact flint-like felsitic rock.
Hornblendite—a rock essentially composed of hornblende.
Hornstone—a very compact, silicious rock of horn-like texture, allied to flint; term also
applied to flinty forms of felsite.
Hypogene rocks—those formed deep within the earth under the influence of heat and pressure.
Ironstone—a rock composed largely of iron, usually applied to clayey rocks having a large iron
content.
Infusorial earth (tripolite)—an earthy or silt deposit consisting chiefly of the silicious shells of
diatoms.
Itacolumite—a flexible sandstone whose pliability is due to an open arrangement of sand
grains which are held together by scales of mica.
Jasper—a reddish variety of chalcedonic quartz.
Keratophyre—a felsite with a large percentage of soda.
Kersantite—a mica dolerite consisting chiefly of plagioclase, augite, and biotite.
Lapilli—small fragments of lava ejected from volcanoes; volcanic cinders.
Laterite—a red, porous, ferruginous residual earth of India and other tropical countries.
Lava—a molten rock, especially applied to flows upon the surface, whether from vents or from
fissures; also applied to the solidified product.
Lignite (brown coal)—a soft, brown, impure coal.
Limburgite—a compact basic igneous rock of the basaltic class, composed essentially of augite
and olivine, with magnetite iron and apatite as common accessories.
Limestone—a rock composed primarily of calcium carbonate, though magnesium sometimes
replaces a part of the calcium. (See dolomite and marble.)
Liparite (rhyolite)—an acidic igneous rock of aphanitic or glassy texture, characterized by
flowage lines and various microscopic crystals; rhyolite is the more common American name.
Loess—a very fine porous silicious silt containing some calcareous material which often
collects in nodules (Löss Kindchen) or in vertical tubules; characterized by a peculiar competency
to stand in vertical walls; held by some to be eolian, by others to be fluvial or lacustrine, and by
still others to be partly eolian and partly aqueous.
Greensand—a sand or sandstone containing a notable percentage of grains of glauconite.
Greenstone—a comprehensive term used to designate igneous and metamorphic crystalline
rocks of greenish hue and of intricate and often minute crystallization; they are mostly dolerites,
diabases, and diorites; a convenient term for field use where the constituents cannot be
determined, and for general use when the variety is unimportant.
Greisen—an aggregate of quartz and mica, i.e., a granite without feldspar.
Greywacke—a sand rock in which the grains are basic silicates instead of quartz.
Hälleflinta—a compact flint-like felsitic rock.
Hornblendite—a rock essentially composed of hornblende.
Hornstone—a very compact, silicious rock of horn-like texture, allied to flint; term also
applied to flinty forms of felsite.
Hypogene rocks—those formed deep within the earth under the influence of heat and pressure.
Ironstone—a rock composed largely of iron, usually applied to clayey rocks having a large iron
content.
Infusorial earth (tripolite)—an earthy or silt deposit consisting chiefly of the silicious shells of
diatoms.
Itacolumite—a flexible sandstone whose pliability is due to an open arrangement of sand
grains which are held together by scales of mica.
Jasper—a reddish variety of chalcedonic quartz.
Keratophyre—a felsite with a large percentage of soda.
Kersantite—a mica dolerite consisting chiefly of plagioclase, augite, and biotite.
Lapilli—small fragments of lava ejected from volcanoes; volcanic cinders.
Laterite—a red, porous, ferruginous residual earth of India and other tropical countries.
Lava—a molten rock, especially applied to flows upon the surface, whether from vents or from
fissures; also applied to the solidified product.
Lignite (brown coal)—a soft, brown, impure coal.
Limburgite—a compact basic igneous rock of the basaltic class, composed essentially of augite
and olivine, with magnetite iron and apatite as common accessories.
Limestone—a rock composed primarily of calcium carbonate, though magnesium sometimes
replaces a part of the calcium. (See dolomite and marble.)
Liparite (rhyolite)—an acidic igneous rock of aphanitic or glassy texture, characterized by
flowage lines and various microscopic crystals; rhyolite is the more common American name.
Loess—a very fine porous silicious silt containing some calcareous material which often
collects in nodules (Löss Kindchen) or in vertical tubules; characterized by a peculiar competency
to stand in vertical walls; held by some to be eolian, by others to be fluvial or lacustrine, and by
still others to be partly eolian and partly aqueous.
Page 555
Marble—typically a granular crystalline limestone or dolomite produced by metamorphic
action; but the term is variously applied to calcareous and even to other rocks that are colored
ornamentally and susceptible of polish.
Marl—an earth formed largely of calcium carbonate, usually derived from the disintegration of
shells; or the calcareous accretions of plants, notably the stoneworts; term also sometimes applied
to glauconitic and other fertilizing earths.
Melaphyre—a term of varying usage; most commonly applied perhaps to an altered basalt
(q.v.), especially an olivine-bearing variety.
Meta-diabase—a term sometimes used for a metamorphic diabase; in like manner meta is
prefixed to dolerite, syenite, etc.; not in general use.
Meta-igneous rock—a metamorphosed igneous rock.
Metamorphic rock—a rock which has been altered, particularly one which has been rendered
crystalline, or recrystallized by heat and pressure.
Meta-sedimentary rock—a metamorphosed sedimentary rock.
Microgranite—a very fine-grained granite.
Microlites—incipient crystals found in glassy lavas; usually needle-shaped, or rod-like;
occurring singly and in aggregates.
Millstone—see buhrstone.
Minette (mica-syenite)—a rock consisting essentially of orthoclase and mica, or a syenite in
which mica replaces hornblende or predominates over it.
Monzonite—a granitic rock composed of orthoclase and plagioclase in nearly equal
proportions, with ferromagnesian minerals; a rock intermediate between syenite and diorite.
Mudstone—solidified mud or silt, shale.
Nephelinite—a rock composed essentially of nepheline and augite, with magnetite and other
accessories.
Nevadite—a variety of rhyolite of granitoid aspect due to an abundance of porphyritic crystals.
Nodules—concretionary aggregations of rounded form.
Norite—a fine-grained rock consisting of plagioclase and hypersthene.
Novaculite (honestone, oilstone)—a very fine-grained, hard sandstone or silt-stone, used for
whetstones.
Obsidian—a typical form of volcanic glass usually of the acidic class.
Onyx—a variety of chalcedonic quartz having colored bands alternating with white; the
“Mexican onyx” is a crystalline calcium carbonate, variegated with delicate colors due to iron and
manganese.
Oolite—a limestone or dolomite composed of small concretions resembling the roe of fish.
Ooze—an exceedingly soft watery deposit of the deep sea; characterized usually by
microscopic shells from which it is mainly derived, as diatom ooze, globigerina ooze, etc.
action; but the term is variously applied to calcareous and even to other rocks that are colored
ornamentally and susceptible of polish.
Marl—an earth formed largely of calcium carbonate, usually derived from the disintegration of
shells; or the calcareous accretions of plants, notably the stoneworts; term also sometimes applied
to glauconitic and other fertilizing earths.
Melaphyre—a term of varying usage; most commonly applied perhaps to an altered basalt
(q.v.), especially an olivine-bearing variety.
Meta-diabase—a term sometimes used for a metamorphic diabase; in like manner meta is
prefixed to dolerite, syenite, etc.; not in general use.
Meta-igneous rock—a metamorphosed igneous rock.
Metamorphic rock—a rock which has been altered, particularly one which has been rendered
crystalline, or recrystallized by heat and pressure.
Meta-sedimentary rock—a metamorphosed sedimentary rock.
Microgranite—a very fine-grained granite.
Microlites—incipient crystals found in glassy lavas; usually needle-shaped, or rod-like;
occurring singly and in aggregates.
Millstone—see buhrstone.
Minette (mica-syenite)—a rock consisting essentially of orthoclase and mica, or a syenite in
which mica replaces hornblende or predominates over it.
Monzonite—a granitic rock composed of orthoclase and plagioclase in nearly equal
proportions, with ferromagnesian minerals; a rock intermediate between syenite and diorite.
Mudstone—solidified mud or silt, shale.
Nephelinite—a rock composed essentially of nepheline and augite, with magnetite and other
accessories.
Nevadite—a variety of rhyolite of granitoid aspect due to an abundance of porphyritic crystals.
Nodules—concretionary aggregations of rounded form.
Norite—a fine-grained rock consisting of plagioclase and hypersthene.
Novaculite (honestone, oilstone)—a very fine-grained, hard sandstone or silt-stone, used for
whetstones.
Obsidian—a typical form of volcanic glass usually of the acidic class.
Onyx—a variety of chalcedonic quartz having colored bands alternating with white; the
“Mexican onyx” is a crystalline calcium carbonate, variegated with delicate colors due to iron and
manganese.
Oolite—a limestone or dolomite composed of small concretions resembling the roe of fish.
Ooze—an exceedingly soft watery deposit of the deep sea; characterized usually by
microscopic shells from which it is mainly derived, as diatom ooze, globigerina ooze, etc.
Page 556
Orthophyre (orthoclase porphyry)—a rock consisting of crystals of orthoclase in an aphanitic
base.
Peastone (pisolite)—a very coarse variety of oolite.
Peat—the dark brown or black residuum arising from the partial decomposition of mosses and
vegetable tissue in marshes and wet places.
Pegmatite—a term of ill-defined usage applied to rocks whose grain varies from coarser to
finer, and often takes on peculiar aspects due to the simultaneous crystallization and mutual
intergrowths of the crystals; graphic granite is a distinct type of pegmatite in which quartz and
orthoclase crystals grew together along parallel axes so that cross-sections give figures resembling
certain Semitic letters (Fig. 345).
Peridotite—a very basic igneous rock composed chiefly of olivine with augite or related
ferromagnesian minerals, with magnetite and chromite as accessories.
Pelites—a general term embracing clay rocks.
Perlite (pearlstone)—a form of glassy lava made up in part of small spheroids formed of
concentric layers which have a lustrous appearance like pearls.
Petrosilex—an old name for felsite or hälleflinta.
Phonolite (nephelite-trachyte, clinkstone)—a compact resonant igneous rock formed of
sanidine and nephelite with accessories.
Phyllite (argillite)—a variety of indurated, partly metamorphosed, clay silt in which finely
disseminated micaceous scales are abundant and lustrous; intermediate between typical clay slate
and mica-schist.
Pitchstone—a dark vitreous, acid, igneous rock of less perfect glassy texture than obsidian and
more resinous and pitch-like.
Plutonic rocks—igneous rocks formed deep within the earth under the influence of high heat
and pressure; hypogene rocks; distinguished from eruptive rocks formed at the surface.
Porphyrite—a term sometimes used for an altered form of andesite, usually porphyritic in
structure.
Porphyry—a rock consisting of distinct crystals embedded in an aphanitic ground-mass.
Propylite—an altered form of andesite and similar igneous rocks.
Protogine—a hydrated micaceous or chloritic variety of granite or gneiss.
Pumice—a glassy form of lava rendered very vesicular through inflation by steam.
Pyroclastic rocks—fragmental or clastic rocks produced through igneous agencies, embracing
volcanic ashes, tuffs, agglomerates, etc.
Pyroxenite—an igneous rock consisting essentially of pyroxene.
Quartzite—a rock consisting essentially of quartz, usually formed from quartzose sandstone by
cementation or metamorphic action.
Regolith—a name recently suggested by Merrill to embrace the earthy mantle that covers
indurated rocks, chiefly residuary earths; mantle-rock.
base.
Peastone (pisolite)—a very coarse variety of oolite.
Peat—the dark brown or black residuum arising from the partial decomposition of mosses and
vegetable tissue in marshes and wet places.
Pegmatite—a term of ill-defined usage applied to rocks whose grain varies from coarser to
finer, and often takes on peculiar aspects due to the simultaneous crystallization and mutual
intergrowths of the crystals; graphic granite is a distinct type of pegmatite in which quartz and
orthoclase crystals grew together along parallel axes so that cross-sections give figures resembling
certain Semitic letters (Fig. 345).
Peridotite—a very basic igneous rock composed chiefly of olivine with augite or related
ferromagnesian minerals, with magnetite and chromite as accessories.
Pelites—a general term embracing clay rocks.
Perlite (pearlstone)—a form of glassy lava made up in part of small spheroids formed of
concentric layers which have a lustrous appearance like pearls.
Petrosilex—an old name for felsite or hälleflinta.
Phonolite (nephelite-trachyte, clinkstone)—a compact resonant igneous rock formed of
sanidine and nephelite with accessories.
Phyllite (argillite)—a variety of indurated, partly metamorphosed, clay silt in which finely
disseminated micaceous scales are abundant and lustrous; intermediate between typical clay slate
and mica-schist.
Pitchstone—a dark vitreous, acid, igneous rock of less perfect glassy texture than obsidian and
more resinous and pitch-like.
Plutonic rocks—igneous rocks formed deep within the earth under the influence of high heat
and pressure; hypogene rocks; distinguished from eruptive rocks formed at the surface.
Porphyrite—a term sometimes used for an altered form of andesite, usually porphyritic in
structure.
Porphyry—a rock consisting of distinct crystals embedded in an aphanitic ground-mass.
Propylite—an altered form of andesite and similar igneous rocks.
Protogine—a hydrated micaceous or chloritic variety of granite or gneiss.
Pumice—a glassy form of lava rendered very vesicular through inflation by steam.
Pyroclastic rocks—fragmental or clastic rocks produced through igneous agencies, embracing
volcanic ashes, tuffs, agglomerates, etc.
Pyroxenite—an igneous rock consisting essentially of pyroxene.
Quartzite—a rock consisting essentially of quartz, usually formed from quartzose sandstone by
cementation or metamorphic action.
Regolith—a name recently suggested by Merrill to embrace the earthy mantle that covers
indurated rocks, chiefly residuary earths; mantle-rock.
Page 557
Rhyolite—an aphanitic or glassy igneous rock showing flowage lines, usually applied only to
the acidic varieties.
Sandstone—indurated sand usually composed of grains of quartz, but not necessarily so;
sometimes formed of calcareous grains or of grains of the various silicates.
Schist—a crystalline rock having a foliated or parallel structure, splitting easily into slabs or
flakes, less uniform than slate; they are mainly composed of the silicate minerals.
Scoriæ—light, cellular fragments of volcanic rock, coarser than pumice; cinders.
Septaria—concretions the interior of which have parted, and the gaping cracks become filled
with calcite or other mineral deposited from solution (Figs. 375–77).
Serpentine—a rock consisting largely of serpentine; derived in most cases by alteration from
magnesian silicate rocks.
Shale—a more or less laminated rock, consisting of indurated muds, silts, or clays.
Slate—an argillaceous rock which is finely laminated and fissile, either due to very uniform
sedimentation or (more properly) to compression at right angles to the cleavage planes; e.g.,
common roofing-slate (Fig. 362).
Soapstone (steatite)—a soft unctuous rock, composed mainly of talc.
Stalactites—pendant icicle-like forms of calcium carbonate deposited from dripping water.
Stalagmite—the complement of stalactites formed by calcareous waters dripping upon the
floors of caverns.
Steatite—see soapstone.
Syenite—a granitoid rock composed of orthoclase and hornblende, or other ferromagnesian
mineral; the name was formerly applied to a granitoid aggregate of quartz, feldspar, and
hornblende.
Tachylite (hyalomelane, basaltic glass)—a black glass of basaltic nature corresponding to the
acidic glasses, obsidian and pitchstone.
Till (bowlder clay)—a stony or bowldery clay or rock rubbish formed by glaciers.
Trachyte—a name formerly applied to a rock possessing a peculiar roughness due to its cellular
structure; but at present mainly confined to a compact, usually porphyritic igneous rock,
consisting mainly of sanidine associated with varying amounts of triclinic feldspar, augite,
hornblende, and biotite.
Trap—a general term for igneous rocks of the darker basaltic types.
Travertine—a limestone deposited from calcareous waters, chiefly springs; usually soft and
cellular, and hence also called calcareous tufa, calc sinter.
Tuff (tufa)—a term including certain porous granular or cellular rocks of diverse origins; the
volcanic tuffs embrace the finer kinds of pyroclastic detritus, as ashes, cinders, etc.; the calcareous
tufa embrace the granular and cellular deposits of springs; the better usage limits the term to
volcanic clastics.
Water-lime—an impure argillaceous limestone possessing hydraulic properties.
the acidic varieties.
Sandstone—indurated sand usually composed of grains of quartz, but not necessarily so;
sometimes formed of calcareous grains or of grains of the various silicates.
Schist—a crystalline rock having a foliated or parallel structure, splitting easily into slabs or
flakes, less uniform than slate; they are mainly composed of the silicate minerals.
Scoriæ—light, cellular fragments of volcanic rock, coarser than pumice; cinders.
Septaria—concretions the interior of which have parted, and the gaping cracks become filled
with calcite or other mineral deposited from solution (Figs. 375–77).
Serpentine—a rock consisting largely of serpentine; derived in most cases by alteration from
magnesian silicate rocks.
Shale—a more or less laminated rock, consisting of indurated muds, silts, or clays.
Slate—an argillaceous rock which is finely laminated and fissile, either due to very uniform
sedimentation or (more properly) to compression at right angles to the cleavage planes; e.g.,
common roofing-slate (Fig. 362).
Soapstone (steatite)—a soft unctuous rock, composed mainly of talc.
Stalactites—pendant icicle-like forms of calcium carbonate deposited from dripping water.
Stalagmite—the complement of stalactites formed by calcareous waters dripping upon the
floors of caverns.
Steatite—see soapstone.
Syenite—a granitoid rock composed of orthoclase and hornblende, or other ferromagnesian
mineral; the name was formerly applied to a granitoid aggregate of quartz, feldspar, and
hornblende.
Tachylite (hyalomelane, basaltic glass)—a black glass of basaltic nature corresponding to the
acidic glasses, obsidian and pitchstone.
Till (bowlder clay)—a stony or bowldery clay or rock rubbish formed by glaciers.
Trachyte—a name formerly applied to a rock possessing a peculiar roughness due to its cellular
structure; but at present mainly confined to a compact, usually porphyritic igneous rock,
consisting mainly of sanidine associated with varying amounts of triclinic feldspar, augite,
hornblende, and biotite.
Trap—a general term for igneous rocks of the darker basaltic types.
Travertine—a limestone deposited from calcareous waters, chiefly springs; usually soft and
cellular, and hence also called calcareous tufa, calc sinter.
Tuff (tufa)—a term including certain porous granular or cellular rocks of diverse origins; the
volcanic tuffs embrace the finer kinds of pyroclastic detritus, as ashes, cinders, etc.; the calcareous
tufa embrace the granular and cellular deposits of springs; the better usage limits the term to
volcanic clastics.
Water-lime—an impure argillaceous limestone possessing hydraulic properties.
Page 558
Wacke—a dark earthy or granular deposit formed from basic tuffs or from the disaggregation
of basaltic and similar rocks; a term which may well come into more general use to distinguish the
silicate sands that arise from the disaggregation, but only partial decomposition, of basic rocks, as
arkose does, the like products of the acidic or granitoid rocks, and as sandstone does, the granular
products of complete chemical decomposition.
ORE-DEPOSITS.[207]
Ore-deposits are but a special phase of the rock-forming processes already discussed. They have
peculiar interest because of their industrial value. An ore is simply a rock that contains a metal that
can be profitably extracted, though for convenience the term is used more broadly to include
unworkable lean ores and ore material. The metal need not preponderate or form any fixed
percentage of the whole, for the criterion is solely economic and not petrologic. A gold ore rarely
contains more than a very small fraction of one percent. of the precious metal, while high-grade
iron ore yields sixty-odd percent. of the metal. In iron ore, the metallic oxide or carbonate makes
up nearly the whole rock; in gold ore, the metal is the merest incidental constituent, from the
petrologic point of view.
Concentration.—The essential fact in the formation of ores is the unusual concentration of the
metal. There are vast quantities of all the metals disseminated through the rock substance of the
earth and even throughout the hydrosphere, but they do not constitute ores because they have no
economic value. They become ores when concentrated in accessible places to a workable richness.
The degree of concentration required is measured by the value of the metal. The essential elements
for consideration are, therefore, (1) the original distribution of the metallic materials through the
rocks, (2) their solution by circulating waters (or, rarely, by other means), (3) their transportation
in solution to the place of deposit, (4) their precipitation in concentrated form, and (5) perhaps
their further concentration and purification by subsequent processes.
Exceptional and doubtful cases.—There are a few cases where ore-deposits are made by
volcanic fumes or vapors, but these may be neglected here. Formerly, ores were often attributed to
vapors supposed to arise from the hot interior, but this mode of origin seems incompatible with
physical conditions. Ores have been attributed to water originally contained as steam in lavas, and
to waters escaping from the interior of the earth, these waters being supposed to be especially
mineralized. Direct evidence on this point is obviously beyond reach. Segregation in the molten
state is recognized as a source of ores, but its function is probably confined chiefly to partial
enrichment as stated below. There are other occasional methods, but the chief process of
concentration, immeasurably surpassing all others, consists in the leaching out of ore materials
disseminated through the country rock and their redeposition in segregated forms, as an incident
of the recognized system of water circulation.
Original distribution.—The original distribution of ore material through the primitive rocks is
beyond the ken of present science, for even the nature of the true primitive rocks is unknown. For
present purposes it is sufficient to regard all rocks concerned in ore-deposition as either igneous or
sedimentary, and to inquire, as a first step, how far ordinary igneous and sedimentary processes
contribute to the segregation of ore material, leaving for a second stage of inquiry the subsequent
processes of concentration.
Magmatic segregation.—In a few instances workable masses of ore seem to have arisen from
lavas by direct segregation in the molten state, without the aid of subsequent concentration by
of basaltic and similar rocks; a term which may well come into more general use to distinguish the
silicate sands that arise from the disaggregation, but only partial decomposition, of basic rocks, as
arkose does, the like products of the acidic or granitoid rocks, and as sandstone does, the granular
products of complete chemical decomposition.
ORE-DEPOSITS.[207]
Ore-deposits are but a special phase of the rock-forming processes already discussed. They have
peculiar interest because of their industrial value. An ore is simply a rock that contains a metal that
can be profitably extracted, though for convenience the term is used more broadly to include
unworkable lean ores and ore material. The metal need not preponderate or form any fixed
percentage of the whole, for the criterion is solely economic and not petrologic. A gold ore rarely
contains more than a very small fraction of one percent. of the precious metal, while high-grade
iron ore yields sixty-odd percent. of the metal. In iron ore, the metallic oxide or carbonate makes
up nearly the whole rock; in gold ore, the metal is the merest incidental constituent, from the
petrologic point of view.
Concentration.—The essential fact in the formation of ores is the unusual concentration of the
metal. There are vast quantities of all the metals disseminated through the rock substance of the
earth and even throughout the hydrosphere, but they do not constitute ores because they have no
economic value. They become ores when concentrated in accessible places to a workable richness.
The degree of concentration required is measured by the value of the metal. The essential elements
for consideration are, therefore, (1) the original distribution of the metallic materials through the
rocks, (2) their solution by circulating waters (or, rarely, by other means), (3) their transportation
in solution to the place of deposit, (4) their precipitation in concentrated form, and (5) perhaps
their further concentration and purification by subsequent processes.
Exceptional and doubtful cases.—There are a few cases where ore-deposits are made by
volcanic fumes or vapors, but these may be neglected here. Formerly, ores were often attributed to
vapors supposed to arise from the hot interior, but this mode of origin seems incompatible with
physical conditions. Ores have been attributed to water originally contained as steam in lavas, and
to waters escaping from the interior of the earth, these waters being supposed to be especially
mineralized. Direct evidence on this point is obviously beyond reach. Segregation in the molten
state is recognized as a source of ores, but its function is probably confined chiefly to partial
enrichment as stated below. There are other occasional methods, but the chief process of
concentration, immeasurably surpassing all others, consists in the leaching out of ore materials
disseminated through the country rock and their redeposition in segregated forms, as an incident
of the recognized system of water circulation.
Original distribution.—The original distribution of ore material through the primitive rocks is
beyond the ken of present science, for even the nature of the true primitive rocks is unknown. For
present purposes it is sufficient to regard all rocks concerned in ore-deposition as either igneous or
sedimentary, and to inquire, as a first step, how far ordinary igneous and sedimentary processes
contribute to the segregation of ore material, leaving for a second stage of inquiry the subsequent
processes of concentration.
Magmatic segregation.—In a few instances workable masses of ore seem to have arisen from
lavas by direct segregation in the molten state, without the aid of subsequent concentration by
Page 559
water action, on which most ores are dependent. It is not improbable that the segregation of
metallic iron and nickel, and perhaps other metals, in the deeper parts of the earth may be a
prevalent process, giving rise to masses like the native iron found in basalt in Greenland. This iron
closely resembles the nickel-irons of meteorites, which may be illustrations of similar action in
small planetary bodies that have been disrupted. Metallic masses so segregated presumably
gravitate toward the planetary center and hence, whatever their inherent interest, have little
relation to a subject whose basal criterion is economic. It is not at all improbable, however, that in
the magmatic differentiation of the lavas that come to the surface, there is some metallic
segregation that may make the enriched parts effective ground for the concentrating processes of
water circulation, and so determine the location of ore-deposits. Igneous rocks are not equally the
seats of ore-deposits, even when the circulatory conditions seem to be equally favorable. These
conditions may not really be equally favorable, but there is good ground to believe that some
igneous masses constitute a richer field for concentration than others. No definite rule, however,
for distinguishing rich varieties of rock from lean ones has been determined. The basic igneous
rocks are, on the whole, perhaps somewhat richer in ores than the acidic class, but there is no
established law. Many acidic rocks bear more and richer ores than many basic ones. The view here
entertained is that both classes are subject to regional enrichment through conditions connected
with their origin, as yet little known.
Marine segregation and dispersion.—In the formation of the sedimentary rocks from the
primitive and igneous rocks there was notable metallic concentration in some cases, and even
more notable depletion in others. The ground-waters of the land, after their subterranean circuits,
carried into the water-basins various metallic substances in solution. These were either
precipitated early in the marine or lacustrine drift of the waters, or became diffused throughout the
oceanic body. In the main they appear to have been widely diffused, and either to have remained
long in solution, or to have been very sparsely deposited through the marine or lacustrine
sediments. As a rule, these sediments seem to contain less of valuable ore material than igneous
rocks, and this is rational, for, as we shall see, the ground-water circulation of the land tends to
concentrate and hold back a part of the metallic content of the land rocks so that only a residue
reaches the sea. But there are important exceptions to this general rule of sedimentary leanness.
The iron-ore beds of Clinton age ranging from New York to Alabama, and appearing also in
Wisconsin and Nova Scotia, form a stratum in the midst of the ordinary sediments, and contain
marine fossils. The great ore beds of Lake Superior were originally of similar type, and so are
most other important iron deposits. It cannot be said, in most cases, that these iron deposits are
marine as distinguished from lacustrine or lodgment deposits, but they are at least sedimentary.
The ferruginous material was originally disseminated widely through antecedent land rocks, but
was concentrated in the course of the sedimentary processes.
Limestone appears to have been sometimes enriched locally in lead and zinc, and more rarely in
copper, in the course of its sedimentation. The lead and zinc regions of the Mississippi basin have
been regarded as dependent on such regional enrichment as a primary condition. This localized
enrichment has been attributed to solutions brought into the sea from neighboring metal-bearing
lands and precipitated by organic action in the sea-water,[208] this organic action being more
effective in some areas than in others because of the unequal distribution of life and the
concentration of its decaying products. It is assumed that such precipitates were at first too diffuse
to be of value, and further concentration was required to bring them together into workable
deposits; but the further processes appear to have been effective only where the preliminary
enrichment had taken place. At any rate, the workable deposits are singularly localized, while the
concentrative processes are very general.
metallic iron and nickel, and perhaps other metals, in the deeper parts of the earth may be a
prevalent process, giving rise to masses like the native iron found in basalt in Greenland. This iron
closely resembles the nickel-irons of meteorites, which may be illustrations of similar action in
small planetary bodies that have been disrupted. Metallic masses so segregated presumably
gravitate toward the planetary center and hence, whatever their inherent interest, have little
relation to a subject whose basal criterion is economic. It is not at all improbable, however, that in
the magmatic differentiation of the lavas that come to the surface, there is some metallic
segregation that may make the enriched parts effective ground for the concentrating processes of
water circulation, and so determine the location of ore-deposits. Igneous rocks are not equally the
seats of ore-deposits, even when the circulatory conditions seem to be equally favorable. These
conditions may not really be equally favorable, but there is good ground to believe that some
igneous masses constitute a richer field for concentration than others. No definite rule, however,
for distinguishing rich varieties of rock from lean ones has been determined. The basic igneous
rocks are, on the whole, perhaps somewhat richer in ores than the acidic class, but there is no
established law. Many acidic rocks bear more and richer ores than many basic ones. The view here
entertained is that both classes are subject to regional enrichment through conditions connected
with their origin, as yet little known.
Marine segregation and dispersion.—In the formation of the sedimentary rocks from the
primitive and igneous rocks there was notable metallic concentration in some cases, and even
more notable depletion in others. The ground-waters of the land, after their subterranean circuits,
carried into the water-basins various metallic substances in solution. These were either
precipitated early in the marine or lacustrine drift of the waters, or became diffused throughout the
oceanic body. In the main they appear to have been widely diffused, and either to have remained
long in solution, or to have been very sparsely deposited through the marine or lacustrine
sediments. As a rule, these sediments seem to contain less of valuable ore material than igneous
rocks, and this is rational, for, as we shall see, the ground-water circulation of the land tends to
concentrate and hold back a part of the metallic content of the land rocks so that only a residue
reaches the sea. But there are important exceptions to this general rule of sedimentary leanness.
The iron-ore beds of Clinton age ranging from New York to Alabama, and appearing also in
Wisconsin and Nova Scotia, form a stratum in the midst of the ordinary sediments, and contain
marine fossils. The great ore beds of Lake Superior were originally of similar type, and so are
most other important iron deposits. It cannot be said, in most cases, that these iron deposits are
marine as distinguished from lacustrine or lodgment deposits, but they are at least sedimentary.
The ferruginous material was originally disseminated widely through antecedent land rocks, but
was concentrated in the course of the sedimentary processes.
Limestone appears to have been sometimes enriched locally in lead and zinc, and more rarely in
copper, in the course of its sedimentation. The lead and zinc regions of the Mississippi basin have
been regarded as dependent on such regional enrichment as a primary condition. This localized
enrichment has been attributed to solutions brought into the sea from neighboring metal-bearing
lands and precipitated by organic action in the sea-water,[208] this organic action being more
effective in some areas than in others because of the unequal distribution of life and the
concentration of its decaying products. It is assumed that such precipitates were at first too diffuse
to be of value, and further concentration was required to bring them together into workable
deposits; but the further processes appear to have been effective only where the preliminary
enrichment had taken place. At any rate, the workable deposits are singularly localized, while the
concentrative processes are very general.
Page 560
Metallic material is sometimes partially concentrated in sandstones and shales in the process of
sedimentation, though more rarely. The copper-bearing shale (Kupferschiefer) of the Zechstein
group in Germany, so extensively worked along the flanks of the Harz Mountains, is a striking
example.
It is in every way reasonable to suppose that land-waters, on reaching the margins of the water-
basins, must occasionally find conditions favorable for the precipitation of their metallic contents,
and that the ratio of these precipitates to other material might be relatively high in the more
favorable situations, and that this enrichment of the country rock may be a condition precedent to
a sufficient subsequent concentration to yield workable accumulations.
It is, therefore, inferred that while the processes of sedimentation tended on the whole to
leanness, they gave rise to (1) some very important ore-deposits, notably the chief iron ores, the
greatest of all ores in quantity and in real industrial value, and (2) a diffuse enrichment of certain
other areas which made them productive under subsequent concentrative processes, while the
sedimentary formations in general were left barren.
Origin of ore regions.—From these considerations it appears that for the fundamental
explanation of “mining regions” we must look mainly (1) to magmatic differentiation, so far as the
country rock is igneous, and (2) to sedimentary enrichment, so far as the rock is secondary. The
determining conditions in both cases are obscure and unpredictable, but the recognition of such
regions, and of the function of preliminary diffuse regional enrichment, contributes to a
comprehensive view of the complex processes of ore concentration. The subsequent processes
consist in the further concentration of the ore material into sheets, lodes, veins, and similar
aggregations by ground-water circulation, or else in the purification of the ores by the removal of
useless or deleterious material, or in both combined.
Surface residual concentration.—The simplest of all modes of concentration takes place in
the formation of mantle-rock. An insoluble or slightly soluble metallic substance sparsely
distributed through a rock may be concentrated to working value by the decay and removal of the
main rock material, leaving the metallic material in the residuary mantle. The tin ores of the Malay
peninsula[209] are especially good examples. The crystals of tin oxide were originally scattered
sparsely through granite and limestone, but by their decay and partial removal it has accumulated
in workable quantities. Certain gold fields and certain iron ores have acquired higher values in the
same way. Such residuary material may be further concentrated by wash into gulches or alluvial
flats, in the course of which the lighter parts of the mantle-rock are largely carried away, and the
heavier, including the metal or its compounds, are mainly left behind. Gold placers are the best
example. The mining of placers by hydraulic processes is but a further extension of the natural
process of concentration.
Such concentrates in past ages have in some cases been buried by later deposits, and hence
certain ancient sandstones, conglomerates, and mantle-rocks have become ore-bearing horizons.
The Rand of South Africa appears to be of this type.
Purification and concentration.—A somewhat different mode of concentration and
purification has affected certain of the great iron deposits. As already explained, the iron
compounds were originally dissolved from the iron-bearing constituents of the primitive or of
igneous rocks, or their derivatives, and were deposited in beds as chemical stratiform deposits. In
some cases they were sufficiently pure, as first precipitated, to be worked profitably, but in most
cases they were seriously affected by undesirable mineral associates. When, however, such impure
deposits are subjected for long periods to the percolation of waters from the surface under
sedimentation, though more rarely. The copper-bearing shale (Kupferschiefer) of the Zechstein
group in Germany, so extensively worked along the flanks of the Harz Mountains, is a striking
example.
It is in every way reasonable to suppose that land-waters, on reaching the margins of the water-
basins, must occasionally find conditions favorable for the precipitation of their metallic contents,
and that the ratio of these precipitates to other material might be relatively high in the more
favorable situations, and that this enrichment of the country rock may be a condition precedent to
a sufficient subsequent concentration to yield workable accumulations.
It is, therefore, inferred that while the processes of sedimentation tended on the whole to
leanness, they gave rise to (1) some very important ore-deposits, notably the chief iron ores, the
greatest of all ores in quantity and in real industrial value, and (2) a diffuse enrichment of certain
other areas which made them productive under subsequent concentrative processes, while the
sedimentary formations in general were left barren.
Origin of ore regions.—From these considerations it appears that for the fundamental
explanation of “mining regions” we must look mainly (1) to magmatic differentiation, so far as the
country rock is igneous, and (2) to sedimentary enrichment, so far as the rock is secondary. The
determining conditions in both cases are obscure and unpredictable, but the recognition of such
regions, and of the function of preliminary diffuse regional enrichment, contributes to a
comprehensive view of the complex processes of ore concentration. The subsequent processes
consist in the further concentration of the ore material into sheets, lodes, veins, and similar
aggregations by ground-water circulation, or else in the purification of the ores by the removal of
useless or deleterious material, or in both combined.
Surface residual concentration.—The simplest of all modes of concentration takes place in
the formation of mantle-rock. An insoluble or slightly soluble metallic substance sparsely
distributed through a rock may be concentrated to working value by the decay and removal of the
main rock material, leaving the metallic material in the residuary mantle. The tin ores of the Malay
peninsula[209] are especially good examples. The crystals of tin oxide were originally scattered
sparsely through granite and limestone, but by their decay and partial removal it has accumulated
in workable quantities. Certain gold fields and certain iron ores have acquired higher values in the
same way. Such residuary material may be further concentrated by wash into gulches or alluvial
flats, in the course of which the lighter parts of the mantle-rock are largely carried away, and the
heavier, including the metal or its compounds, are mainly left behind. Gold placers are the best
example. The mining of placers by hydraulic processes is but a further extension of the natural
process of concentration.
Such concentrates in past ages have in some cases been buried by later deposits, and hence
certain ancient sandstones, conglomerates, and mantle-rocks have become ore-bearing horizons.
The Rand of South Africa appears to be of this type.
Purification and concentration.—A somewhat different mode of concentration and
purification has affected certain of the great iron deposits. As already explained, the iron
compounds were originally dissolved from the iron-bearing constituents of the primitive or of
igneous rocks, or their derivatives, and were deposited in beds as chemical stratiform deposits. In
some cases they were sufficiently pure, as first precipitated, to be worked profitably, but in most
cases they were seriously affected by undesirable mineral associates. When, however, such impure
deposits are subjected for long periods to the percolation of waters from the surface under
Page 561
favorable conditions, the impurities are often dissolved and the ores concentrated. The great
Bessemer ore-deposits of Lake Superior are examples. Originally impure carbonates or silicates,
they have been converted into rich and phenomenally pure ferric oxides along certain lines of
ground-water circulation, and in certain areas of free leaching. Van Hise has shown the definite
relation between the water circulation and the production of the high-grade ores.[210] Vast quantities
of unconcentrated lean ores lie in the tracts not thus purified and enriched by circulating waters.
This does not appear to be simply residual concentration. The waters seem to have added ferric
oxide brought from above, while they carried away the “impurities,” silica, carbon dioxide, etc.
Perhaps this is an instance of mass action in which the ore present aided in causing additions to
itself.
Concentration by solution and reprecipitation.—By a process almost the opposite of residual
concentration, ore material is often leached out of the surface-rock by water circulating slowly
through its pores, cleavage planes, and minute crevices, and is carried on with the circulation until
it reaches some substance which causes a reaction that precipitates the ore material. This
substance may be a constituent of some rock which the circulating water encounters, such as
organic matter. More commonly, the precipitation seems to be due to the mingling of waters
charged with different mineral substances, the mingling inducing reaction and the precipitation of
the ore. Precipitation, however, does not necessarily follow such commingling. The junctions of
underground waterways are sometimes characterized by barrenness instead of richness. In the
expressive phraseology of the miners, a tributary current sometimes “makes” and sometimes “cuts
out.” In chemical phrase, when the mingling waters reduce the solubility of the appropriate
substance sufficiently, an ore-deposit is formed; when they increase its solubility, they promote
barrenness. Changes of pressure and temperature may enter into the process, and mass action may
lend its aid when once a deposit is started.
More concretely stated, the general process of underground ore formation appears to be this: the
permeating waters dissolve the ore material disseminated through the rock and carry it thence into
the main channels of circulation, usually the fissures, broken tracts, porous belts, or cavernous
spaces. If precipitating conditions are found there, deposition takes place. The precipitating
conditions may be merely changes of physical state, such as cooling or relief of pressure, but
probably much more generally they consist in the commingling and mutual reaction of waters that
have pursued different courses and become differently mineralized, as implied above. In these
cases the metal-bearing current may be scarcely more important than the precipitating current.
Since the solvent action is a condition precedent to deposition, the location of the greatest
solvent action first invites attention. At present it must be treated in general terms, for it is not
known what solutions must be formed beyond the fact that they must include the ore material.
Probably they must include much besides. Furthermore, it is not known that deep-seated rocks
carry more ore material than similar rocks at or near the surface or at any other horizon. Fantastic
conceptions of deep-seated metallic richness are to be shunned as quite beyond practical
consideration. The water circulation is probably very slight below a depth of two or three miles at
most, and above that depth there is little ground to suppose that the rocks of one horizon are
inherently more metalliferous than others of their kind. There is no assignable reason why the
igneous rocks at the surface are not as rich in ore material as the igneous rocks two or three miles
below, since all are probably eruptive and of much the same nature on the whole, being in many
cases parts of the same eruptions.
Location of greatest solvent action.—Solvent action is probably most intense where the
temperature and pressure are highest, that is, in the deeper reaches of water circulation; but the
Bessemer ore-deposits of Lake Superior are examples. Originally impure carbonates or silicates,
they have been converted into rich and phenomenally pure ferric oxides along certain lines of
ground-water circulation, and in certain areas of free leaching. Van Hise has shown the definite
relation between the water circulation and the production of the high-grade ores.[210] Vast quantities
of unconcentrated lean ores lie in the tracts not thus purified and enriched by circulating waters.
This does not appear to be simply residual concentration. The waters seem to have added ferric
oxide brought from above, while they carried away the “impurities,” silica, carbon dioxide, etc.
Perhaps this is an instance of mass action in which the ore present aided in causing additions to
itself.
Concentration by solution and reprecipitation.—By a process almost the opposite of residual
concentration, ore material is often leached out of the surface-rock by water circulating slowly
through its pores, cleavage planes, and minute crevices, and is carried on with the circulation until
it reaches some substance which causes a reaction that precipitates the ore material. This
substance may be a constituent of some rock which the circulating water encounters, such as
organic matter. More commonly, the precipitation seems to be due to the mingling of waters
charged with different mineral substances, the mingling inducing reaction and the precipitation of
the ore. Precipitation, however, does not necessarily follow such commingling. The junctions of
underground waterways are sometimes characterized by barrenness instead of richness. In the
expressive phraseology of the miners, a tributary current sometimes “makes” and sometimes “cuts
out.” In chemical phrase, when the mingling waters reduce the solubility of the appropriate
substance sufficiently, an ore-deposit is formed; when they increase its solubility, they promote
barrenness. Changes of pressure and temperature may enter into the process, and mass action may
lend its aid when once a deposit is started.
More concretely stated, the general process of underground ore formation appears to be this: the
permeating waters dissolve the ore material disseminated through the rock and carry it thence into
the main channels of circulation, usually the fissures, broken tracts, porous belts, or cavernous
spaces. If precipitating conditions are found there, deposition takes place. The precipitating
conditions may be merely changes of physical state, such as cooling or relief of pressure, but
probably much more generally they consist in the commingling and mutual reaction of waters that
have pursued different courses and become differently mineralized, as implied above. In these
cases the metal-bearing current may be scarcely more important than the precipitating current.
Since the solvent action is a condition precedent to deposition, the location of the greatest
solvent action first invites attention. At present it must be treated in general terms, for it is not
known what solutions must be formed beyond the fact that they must include the ore material.
Probably they must include much besides. Furthermore, it is not known that deep-seated rocks
carry more ore material than similar rocks at or near the surface or at any other horizon. Fantastic
conceptions of deep-seated metallic richness are to be shunned as quite beyond practical
consideration. The water circulation is probably very slight below a depth of two or three miles at
most, and above that depth there is little ground to suppose that the rocks of one horizon are
inherently more metalliferous than others of their kind. There is no assignable reason why the
igneous rocks at the surface are not as rich in ore material as the igneous rocks two or three miles
below, since all are probably eruptive and of much the same nature on the whole, being in many
cases parts of the same eruptions.
Location of greatest solvent action.—Solvent action is probably most intense where the
temperature and pressure are highest, that is, in the deeper reaches of water circulation; but the
Page 562
amount of water passing in and out of the deeper zone is but a small fraction of that which courses
through the upper horizons, and the total solvent action is quite certainly much greater in the upper
zone than in the lower. At the same time the solutions in the upper zone are quite certainly more
dilute than those below. The horizon of greatest solution lies between the surface and a level
slightly below the ground-water surface, or, in other words, in the zone where atmosphere and
hydrosphere coöperate. Surface-waters are charged with atmospheric and organic acids and other
solvents, and their general effect upon the rocks is markedly solvent down to or often below the
permanent water-level. In this zone concentration by residual accumulation may take place, as
already noted, if the metallic compounds resist solution; otherwise this zone is depleted of its ore
material by solution, and preparation is made for deposition elsewhere.
Solution also continues to take place varyingly as the water descends below this zone of
dominant solution, and extends probably to the full depth of water circulation, but in the deeper
circuit, precipitation also takes place and the action becomes complex. With the waters taking up
and throwing down material at the same time, it is difficult to estimate the balance of results.
When waters that have been mineralized near the surface descend, they often take on a
precipitating phase at no great depth below the upper level of the ground-water; thus sulphides
that were oxidized and dissolved near the surface are reprecipitated, often at horizons not greatly
below the permanent water-level. Waters that dissolve metallic substances in the upper levels often
become charged with sulphuretted hydrogen and other precipitants within a few scores or a few
hundreds of feet of the surface, as deep wells abundantly prove. The freshness of surface which
metallic sulphides often exhibit at these levels is fair ground for inferring recency of deposition
and absence of solvent action. Actual demonstrations of depositions in progress are not wanting.
Short-course action.—The concentration which thus takes place by solution in the upper zone,
followed closely by reprecipitation within a few score or a few hundred feet, may well be termed
the short-course mode of ore concentration. It finds its most important illustration in what is
commonly known as the “secondary enrichment” of ore-deposits. The ores in the outcropping
edge of the vein or lode are dissolved by the surface-waters, carried a short distance down the ore
tract and redeposited, causing enrichment at that point. This is only a special case of what takes
place generally at this horizon. It is effective in this case because it has a previous partial
concentration to work upon. Secondary enrichments of this kind often contain most or all the
workable values of the ore tract. If instead of a previous concentration in a vein, lode, or similar
ore tract, there had been partial concentration in the country rock by sedimentation, as in the case
of iron-ore beds and perhaps lead-, zinc-, and copper-impregnated sediments, the short-course
method may give working values not before possessed. In some of the more obscure cases of
previous partial concentration in the crystalline and other rocks, it is probably this short-course
action that brings the concentration up to working value. It is probably effective also in
concentrating the metallic contents of certain igneous rocks that were rich in metallic material
when extruded. How far this is true has been, and still remains, a mooted question.
Long-course action.—After the surface-waters have once passed through a cycle of dissolving
and precipitating action, as they are apt to do within the first few hundred feet of their courses
below the water-level, they are liable to pass through a succession of dissolving and depositing
stages, each reaction resulting in a state that makes a new reaction possible. This is especially true
if the waters pursue deep courses. Strictly speaking, the precipitations usually concern only a part
of the substances dissolved. New substances are often taken up in the very act of throwing down
those already held, and the way thus prepared for further changes. If the water pursues a deep and
devious course, it may receive additions by solution and suffer losses by precipitation at many
through the upper horizons, and the total solvent action is quite certainly much greater in the upper
zone than in the lower. At the same time the solutions in the upper zone are quite certainly more
dilute than those below. The horizon of greatest solution lies between the surface and a level
slightly below the ground-water surface, or, in other words, in the zone where atmosphere and
hydrosphere coöperate. Surface-waters are charged with atmospheric and organic acids and other
solvents, and their general effect upon the rocks is markedly solvent down to or often below the
permanent water-level. In this zone concentration by residual accumulation may take place, as
already noted, if the metallic compounds resist solution; otherwise this zone is depleted of its ore
material by solution, and preparation is made for deposition elsewhere.
Solution also continues to take place varyingly as the water descends below this zone of
dominant solution, and extends probably to the full depth of water circulation, but in the deeper
circuit, precipitation also takes place and the action becomes complex. With the waters taking up
and throwing down material at the same time, it is difficult to estimate the balance of results.
When waters that have been mineralized near the surface descend, they often take on a
precipitating phase at no great depth below the upper level of the ground-water; thus sulphides
that were oxidized and dissolved near the surface are reprecipitated, often at horizons not greatly
below the permanent water-level. Waters that dissolve metallic substances in the upper levels often
become charged with sulphuretted hydrogen and other precipitants within a few scores or a few
hundreds of feet of the surface, as deep wells abundantly prove. The freshness of surface which
metallic sulphides often exhibit at these levels is fair ground for inferring recency of deposition
and absence of solvent action. Actual demonstrations of depositions in progress are not wanting.
Short-course action.—The concentration which thus takes place by solution in the upper zone,
followed closely by reprecipitation within a few score or a few hundred feet, may well be termed
the short-course mode of ore concentration. It finds its most important illustration in what is
commonly known as the “secondary enrichment” of ore-deposits. The ores in the outcropping
edge of the vein or lode are dissolved by the surface-waters, carried a short distance down the ore
tract and redeposited, causing enrichment at that point. This is only a special case of what takes
place generally at this horizon. It is effective in this case because it has a previous partial
concentration to work upon. Secondary enrichments of this kind often contain most or all the
workable values of the ore tract. If instead of a previous concentration in a vein, lode, or similar
ore tract, there had been partial concentration in the country rock by sedimentation, as in the case
of iron-ore beds and perhaps lead-, zinc-, and copper-impregnated sediments, the short-course
method may give working values not before possessed. In some of the more obscure cases of
previous partial concentration in the crystalline and other rocks, it is probably this short-course
action that brings the concentration up to working value. It is probably effective also in
concentrating the metallic contents of certain igneous rocks that were rich in metallic material
when extruded. How far this is true has been, and still remains, a mooted question.
Long-course action.—After the surface-waters have once passed through a cycle of dissolving
and precipitating action, as they are apt to do within the first few hundred feet of their courses
below the water-level, they are liable to pass through a succession of dissolving and depositing
stages, each reaction resulting in a state that makes a new reaction possible. This is especially true
if the waters pursue deep courses. Strictly speaking, the precipitations usually concern only a part
of the substances dissolved. New substances are often taken up in the very act of throwing down
those already held, and the way thus prepared for further changes. If the water pursues a deep and
devious course, it may receive additions by solution and suffer losses by precipitation at many
Page 563
points in its course, both descending and ascending. The changes are very complex, and in the
case of a deep or long circuit where various rocks, pressures, and temperatures are encountered,
the history becomes one long succession of complexities, the full nature of which is not yet
revealed.
In the deeper circuits, each individual current usually takes on a descending, a lateral, and
ascending phase, the three being necessary to complete a circuit. The chemical conditions of the
waters in the three phases are probably not sharply distinguished from one another, and hence
there seems to be no defined horizon of concentration comparable to that near the water-level
already described. The chief distinctions in the deeper regions relate to pressure, temperature,
length or depth of penetration, and duration of contact. It seems safe to assume, as a general truth,
that, other things being equal, the solutions become more complex and more nearly reach general
saturation the farther and the deeper the waters penetrate.
It has long been a mooted question whether ore-deposits are due chiefly to descending, to
lateral, or to ascending currents. The question in its usual form is too undiscriminating for
advantageous discussion, but if the ore-deposits due to surface or short-course concentrations and
reconcentrations be set aside, as in some sense a separate class, the relative functions of the
descending, the lateral, and the ascending portions of the deeper circulations become a measurably
definite question. Two great working factors enter into the comparison: (1) much greater
circulation in the upper zone, where lateral movement most prevails; (2) much greater heat and
pressure in the lower zone, where the circulation must be chiefly vertical.
Heat and pressure in general favor solution, and hence so far as this factor goes, descending
water is likely to be increasing its mineral content, rather than diminishing it by deposition. But
this is only general; particular elements of the solution may be deposited. In ascending, as the
same water must later, it is predisposed to deposition from loss of solvent power through reduction
of pressure and temperature. The theoretical balance is here clearly in favor of preponderant
deposition by the ascending portion of the current. So far as precipitation is dependent on the
mingling of differently mineralized waters, descending and ascending currents seem to be situated
much alike, in general, for both are subject to accessions and mutual unions.
The amount of water that circulates in the deeper horizons is much less than that nearer the
surface. Allowing a few hundred, or at most one or two thousand feet for the special short-circuit
zone next below the water-level (it is known to reach 1000 to 1500 feet in some cases), the water
circulating through the next 1000 or 2000 feet is probably several times greater than all that
circulates at greater depths, and this greater circulation above doubtless offsets, in greater or less
measure, the intensified action of the deeper circulation. Much of the upper and more rapid
circulation is lateral, being actuated by the sloping surface of the ground-water, which in turn is
determined by topography, precipitation, and other surface conditions. Theoretical considerations,
therefore, favor the view that lateral flow is an important factor in the concentration of ore
material. But as descending and lateral currents almost inevitably meet and mingle with ascending
currents, it is difficult to distinguish, in the ore-deposits, the special functions of each phase of
action. It is even more difficult to determine whether the different phases are not alike essential to
the mutual reactions on which the deposition depends. It may be as necessary to have a precipitant
as to have a metallic constituent in solution to be precipitated, and what is more, this precipitating
agency may be a substance of no economic value in itself and of no obvious relations to the
substances that form the ores. If the deposition is due solely to a physical state, as relief of
pressure or lowering of temperature, these considerations do not hold.
case of a deep or long circuit where various rocks, pressures, and temperatures are encountered,
the history becomes one long succession of complexities, the full nature of which is not yet
revealed.
In the deeper circuits, each individual current usually takes on a descending, a lateral, and
ascending phase, the three being necessary to complete a circuit. The chemical conditions of the
waters in the three phases are probably not sharply distinguished from one another, and hence
there seems to be no defined horizon of concentration comparable to that near the water-level
already described. The chief distinctions in the deeper regions relate to pressure, temperature,
length or depth of penetration, and duration of contact. It seems safe to assume, as a general truth,
that, other things being equal, the solutions become more complex and more nearly reach general
saturation the farther and the deeper the waters penetrate.
It has long been a mooted question whether ore-deposits are due chiefly to descending, to
lateral, or to ascending currents. The question in its usual form is too undiscriminating for
advantageous discussion, but if the ore-deposits due to surface or short-course concentrations and
reconcentrations be set aside, as in some sense a separate class, the relative functions of the
descending, the lateral, and the ascending portions of the deeper circulations become a measurably
definite question. Two great working factors enter into the comparison: (1) much greater
circulation in the upper zone, where lateral movement most prevails; (2) much greater heat and
pressure in the lower zone, where the circulation must be chiefly vertical.
Heat and pressure in general favor solution, and hence so far as this factor goes, descending
water is likely to be increasing its mineral content, rather than diminishing it by deposition. But
this is only general; particular elements of the solution may be deposited. In ascending, as the
same water must later, it is predisposed to deposition from loss of solvent power through reduction
of pressure and temperature. The theoretical balance is here clearly in favor of preponderant
deposition by the ascending portion of the current. So far as precipitation is dependent on the
mingling of differently mineralized waters, descending and ascending currents seem to be situated
much alike, in general, for both are subject to accessions and mutual unions.
The amount of water that circulates in the deeper horizons is much less than that nearer the
surface. Allowing a few hundred, or at most one or two thousand feet for the special short-circuit
zone next below the water-level (it is known to reach 1000 to 1500 feet in some cases), the water
circulating through the next 1000 or 2000 feet is probably several times greater than all that
circulates at greater depths, and this greater circulation above doubtless offsets, in greater or less
measure, the intensified action of the deeper circulation. Much of the upper and more rapid
circulation is lateral, being actuated by the sloping surface of the ground-water, which in turn is
determined by topography, precipitation, and other surface conditions. Theoretical considerations,
therefore, favor the view that lateral flow is an important factor in the concentration of ore
material. But as descending and lateral currents almost inevitably meet and mingle with ascending
currents, it is difficult to distinguish, in the ore-deposits, the special functions of each phase of
action. It is even more difficult to determine whether the different phases are not alike essential to
the mutual reactions on which the deposition depends. It may be as necessary to have a precipitant
as to have a metallic constituent in solution to be precipitated, and what is more, this precipitating
agency may be a substance of no economic value in itself and of no obvious relations to the
substances that form the ores. If the deposition is due solely to a physical state, as relief of
pressure or lowering of temperature, these considerations do not hold.
Page 564
Summary.—The general results are probably these: In the deeper circuits, more ore material is
brought upward and deposited than is carried downward and deposited, so that metallic values are
shifted toward accessible horizons. In the lateral currents, more metallic values are shifted toward
the trunk-lines of circulation—the great crevices and other waterways—than are carried from
these into the rock and distributed, and lateral segregation results. At the same time the
atmospheric waters acting at or near the surface concentrate ore values downwards. The sum total
of these processes is to promote the development of the higher ore values in accessible horizons,
and along the main lines of circulation.
The influence of contacts.—As ore-deposits depend on a dissolving state followed by a
depositing state of the waters, and perhaps on a complex succession of these alterations, it is
obvious that conditions which favor changes of state and the commingling of different kinds of
water are apt to be favorable to ore production. At any rate it is observed that many important ore-
deposits occur at the contact between formations of different character. The contact of igneous
rock with limestone is a rather notable instance. It is not to be inferred that such contacts are
generally accompanied by workable ore-deposits, but merely that a notable proportion of
workable ore-deposits occur at such junctions. It is rational to suppose that where the chemical
nature of the two formations is in contrast, the waters that percolate through the one are likely to
be mineralized very differently from those that course through the other, and hence that on
mingling at the contact, reactions are specially liable to take place, and that when a valuable
metallic substance is present it is liable to be involved and by chance to suffer precipitation.
Reactions are the more probable because the contact is likely to be a plane of crustal movement,
and hence more or less open and accompanied by fractures, zones of crushed rock and other
conditions that facilitate circulation and offer suitable places for ore formation.
The effect of igneous intrusions.—A special case of much importance arises when lavas are
intruded into sediments that have previously been partially enriched in the ways above described.
The igneous intrusion not only introduces new contact zones, and more or less fracturing, but it
brings into play hot waters with their intensified solvent work, their more active circulation, and
the reaction between waters of different temperatures. The special efficiency of these agencies is
believed to be the determining factor in many cases.
The influence of rock walls.—The rock walls themselves are thought sometimes to be a factor
in ore-precipitating reactions. By mass action, they may withdraw a constituent of the solution and
destroy its equilibrium in such a way as to cause the precipitation of the metallic constituent. Once
deposited on the walls ores aid, by mass action, the further accretion of ores.
The special forms which ores assume in deposition, as beds, veins, lodes, stockworks,
disseminations, segregations, etc., are chiefly incidental to the local situation in which the
essential chemical or physical change takes place.
brought upward and deposited than is carried downward and deposited, so that metallic values are
shifted toward accessible horizons. In the lateral currents, more metallic values are shifted toward
the trunk-lines of circulation—the great crevices and other waterways—than are carried from
these into the rock and distributed, and lateral segregation results. At the same time the
atmospheric waters acting at or near the surface concentrate ore values downwards. The sum total
of these processes is to promote the development of the higher ore values in accessible horizons,
and along the main lines of circulation.
The influence of contacts.—As ore-deposits depend on a dissolving state followed by a
depositing state of the waters, and perhaps on a complex succession of these alterations, it is
obvious that conditions which favor changes of state and the commingling of different kinds of
water are apt to be favorable to ore production. At any rate it is observed that many important ore-
deposits occur at the contact between formations of different character. The contact of igneous
rock with limestone is a rather notable instance. It is not to be inferred that such contacts are
generally accompanied by workable ore-deposits, but merely that a notable proportion of
workable ore-deposits occur at such junctions. It is rational to suppose that where the chemical
nature of the two formations is in contrast, the waters that percolate through the one are likely to
be mineralized very differently from those that course through the other, and hence that on
mingling at the contact, reactions are specially liable to take place, and that when a valuable
metallic substance is present it is liable to be involved and by chance to suffer precipitation.
Reactions are the more probable because the contact is likely to be a plane of crustal movement,
and hence more or less open and accompanied by fractures, zones of crushed rock and other
conditions that facilitate circulation and offer suitable places for ore formation.
The effect of igneous intrusions.—A special case of much importance arises when lavas are
intruded into sediments that have previously been partially enriched in the ways above described.
The igneous intrusion not only introduces new contact zones, and more or less fracturing, but it
brings into play hot waters with their intensified solvent work, their more active circulation, and
the reaction between waters of different temperatures. The special efficiency of these agencies is
believed to be the determining factor in many cases.
The influence of rock walls.—The rock walls themselves are thought sometimes to be a factor
in ore-precipitating reactions. By mass action, they may withdraw a constituent of the solution and
destroy its equilibrium in such a way as to cause the precipitation of the metallic constituent. Once
deposited on the walls ores aid, by mass action, the further accretion of ores.
The special forms which ores assume in deposition, as beds, veins, lodes, stockworks,
disseminations, segregations, etc., are chiefly incidental to the local situation in which the
essential chemical or physical change takes place.
Page 565
CHAPTER VIII.
STRUCTURAL (GEOTECTONIC) GEOLOGY.
The structural phases which rocks assume.—In the previous chapters,
the general method by which rocks are formed has been set forth, and many
of their structural features have been touched upon incidentally. It remains
to assemble the structural features already mentioned, and to consider
certain additional structural phases which rocks assume.
STRUCTURAL FEATURES OF SEDIMENTARY ROCKS.
In the deposition of sediments in the sea, or in other bodies of standing
water, the coarser portion of the material is usually deposited in the shallow
water near the shore where the wave-action is strongest, and the less coarse
of various grades is deposited at greater and greater distances from the land,
while only extremely fine silt is usually carried out to abysmal depths (see
p. 380). To this general law of distribution there are important exceptions.
Fine sediments are sometimes deposited near the shore, and where currents,
tidal agitation, or floating ice are effective, coarse deposits are occasionally
carried far out from the shore.
Stratification.—Sedimentary rocks are usually arranged in more or less
distinct layers; that is, they are stratified. The stratification consists
primarily in the superposition of layers of different constitution or different
compactness on one another. Layers of like constitution or compactness are
often separated by films of different material which cause the partings
between them. The bedded arrangement of stratified rocks is due to various
causes, but primarily to the varying agitation of the waters in which the
sediment was laid down. Where the depositing waters are agitated to the
bottom, coarse sediment is likely to be deposited. Where the waters are
quiet at the bottom, fine sediment is the rule. Since the agitation of the
waters is subject to frequent change, it follows that coarser material
STRUCTURAL (GEOTECTONIC) GEOLOGY.
The structural phases which rocks assume.—In the previous chapters,
the general method by which rocks are formed has been set forth, and many
of their structural features have been touched upon incidentally. It remains
to assemble the structural features already mentioned, and to consider
certain additional structural phases which rocks assume.
STRUCTURAL FEATURES OF SEDIMENTARY ROCKS.
In the deposition of sediments in the sea, or in other bodies of standing
water, the coarser portion of the material is usually deposited in the shallow
water near the shore where the wave-action is strongest, and the less coarse
of various grades is deposited at greater and greater distances from the land,
while only extremely fine silt is usually carried out to abysmal depths (see
p. 380). To this general law of distribution there are important exceptions.
Fine sediments are sometimes deposited near the shore, and where currents,
tidal agitation, or floating ice are effective, coarse deposits are occasionally
carried far out from the shore.
Stratification.—Sedimentary rocks are usually arranged in more or less
distinct layers; that is, they are stratified. The stratification consists
primarily in the superposition of layers of different constitution or different
compactness on one another. Layers of like constitution or compactness are
often separated by films of different material which cause the partings
between them. The bedded arrangement of stratified rocks is due to various
causes, but primarily to the varying agitation of the waters in which the
sediment was laid down. Where the depositing waters are agitated to the
bottom, coarse sediment is likely to be deposited. Where the waters are
quiet at the bottom, fine sediment is the rule. Since the agitation of the
waters is subject to frequent change, it follows that coarser material
Page 566
succeeds finer, and finer coarser, in the same place. Hence arise beds,
layers, and laminæ. The terms layer and bed are generally used as
synonyms, while laminæ are thinner divisions of the same sort. The term
stratum is sometimes applied to one layer and sometimes to all the
consecutive layers of the same sort of rock. For the latter meaning the term
formation is often used. Sometimes bedding seems to have been determined
by strong currents which temporarily not only prevented deposition over a
given area, but even cut away the loose surface of deposits already made,
giving a firm surface from which succeeding deposits are distinct. This
sequence of events is sometimes shown by the truncation of laminæ, and by
other signs of erosion. The commoner sorts of bedded rock are limestones,
shales, sandstones, and conglomerates.
The bedding of limestones is often caused by the introduction of thin
films of clayey material which interrupt the continuity of the lime
accumulation and cause natural partings. Sometimes, however, bedding
arises from variations in the physical condition of the lime sediment itself.
Lamination is not usually conspicuous in pure limestone, though it may be
well developed in the shaly phases of this rock. Shales are normally
laminated as well as bedded, and the lamination is often more notable than
the thicker bedding. Bedding in shale may arise from the introduction of
sandy laminæ, or by notable changes in the texture of the shale material.
Similarly, sandstones are sometimes divided into beds by shaly (clayey)
partings, but more often by variations in the coarseness of the sand itself, or
by the presence of laminæ that are less coherent than those above and
below. Sometimes the layers appear to be determined by the compacting of
the surface of sand already accumulated before it was buried by later
deposits. Sandstones may be thick- or thin-bedded, and their bedding passes
insensibly into lamination.
Sand deposits usually take place in relatively shallow water, and the sand
is subjected to much shifting before it finds a permanent lodgment. In the
course of this shifting, bars are formed which usually have a rather steep
face in the direction in which they are being shifted. The sand carried over
the top of the bar finds lodgment on the sloping terrace face. The inclined
laminæ thus formed constitute a kind of bedding, but since its planes do not
conform to the general horizontal attitude of the formation as a whole, it is
called false- or cross-bedding or, more accurately, cross-lamination (see
layers, and laminæ. The terms layer and bed are generally used as
synonyms, while laminæ are thinner divisions of the same sort. The term
stratum is sometimes applied to one layer and sometimes to all the
consecutive layers of the same sort of rock. For the latter meaning the term
formation is often used. Sometimes bedding seems to have been determined
by strong currents which temporarily not only prevented deposition over a
given area, but even cut away the loose surface of deposits already made,
giving a firm surface from which succeeding deposits are distinct. This
sequence of events is sometimes shown by the truncation of laminæ, and by
other signs of erosion. The commoner sorts of bedded rock are limestones,
shales, sandstones, and conglomerates.
The bedding of limestones is often caused by the introduction of thin
films of clayey material which interrupt the continuity of the lime
accumulation and cause natural partings. Sometimes, however, bedding
arises from variations in the physical condition of the lime sediment itself.
Lamination is not usually conspicuous in pure limestone, though it may be
well developed in the shaly phases of this rock. Shales are normally
laminated as well as bedded, and the lamination is often more notable than
the thicker bedding. Bedding in shale may arise from the introduction of
sandy laminæ, or by notable changes in the texture of the shale material.
Similarly, sandstones are sometimes divided into beds by shaly (clayey)
partings, but more often by variations in the coarseness of the sand itself, or
by the presence of laminæ that are less coherent than those above and
below. Sometimes the layers appear to be determined by the compacting of
the surface of sand already accumulated before it was buried by later
deposits. Sandstones may be thick- or thin-bedded, and their bedding passes
insensibly into lamination.
Sand deposits usually take place in relatively shallow water, and the sand
is subjected to much shifting before it finds a permanent lodgment. In the
course of this shifting, bars are formed which usually have a rather steep
face in the direction in which they are being shifted. The sand carried over
the top of the bar finds lodgment on the sloping terrace face. The inclined
laminæ thus formed constitute a kind of bedding, but since its planes do not
conform to the general horizontal attitude of the formation as a whole, it is
called false- or cross-bedding or, more accurately, cross-lamination (see
Page 567
Fig. 368). The same structure is developed on delta fronts and generally in
water shallow enough to be subject to frequent agitation at the bottom.
Sandstone is cross-bedded more commonly than other sorts of sedimentary
rock.
The bedding of conglomerate is due chiefly to variations in coarseness.
Laminæ or thicker layers of sand are frequently found between layers of
coarser material. Conglomerate is likely to be thick-bedded, and cross-
bedding is common.
Lateral gradation.—When the varying nature of the agitation of the sea
at different depths and along the different parts of the coast-border, and
during different phases of the sea-currents, is considered, it will be readily
understood that sedimentary beds are affected by many irregularities, and
that deposits of one kind grade into others horizontally with great freedom.
Thus a bed of conglomerate (gravel) may grade laterally into sandstone, and
this into shale or limestone. It is indeed rather more remarkable that the
sedimentary strata should be as regular and persistent as they are, than that
they sometimes grade into one another.
water shallow enough to be subject to frequent agitation at the bottom.
Sandstone is cross-bedded more commonly than other sorts of sedimentary
rock.
The bedding of conglomerate is due chiefly to variations in coarseness.
Laminæ or thicker layers of sand are frequently found between layers of
coarser material. Conglomerate is likely to be thick-bedded, and cross-
bedding is common.
Lateral gradation.—When the varying nature of the agitation of the sea
at different depths and along the different parts of the coast-border, and
during different phases of the sea-currents, is considered, it will be readily
understood that sedimentary beds are affected by many irregularities, and
that deposits of one kind grade into others horizontally with great freedom.
Thus a bed of conglomerate (gravel) may grade laterally into sandstone, and
this into shale or limestone. It is indeed rather more remarkable that the
sedimentary strata should be as regular and persistent as they are, than that
they sometimes grade into one another.
Page 568
Fig. 368.—Cross-bedding in sandstone. Dells of the Wisconsin near Kilbourn, Wis.
(Bennett.)
Special markings.—The rhythmical action of waves gives rise to
undulatory lodgment, known as ripple-marks (Fig. 324). They are usually
not the direct product of the surface-waves, since they are much too small.
They are produced mainly by the vibratory movement of the undertow, but
they apparently result from various other phases of vibratory agitation of
the bottom waters. They are sometimes made by streams and stream-like
currents. Ripple-marks are apparently preserved indefinitely under proper
circumstances. They are sometimes found, for example, on very ancient
quartzites. Ripples are also made by wind (p. 37). Ripple-marks are usually
(Bennett.)
Special markings.—The rhythmical action of waves gives rise to
undulatory lodgment, known as ripple-marks (Fig. 324). They are usually
not the direct product of the surface-waves, since they are much too small.
They are produced mainly by the vibratory movement of the undertow, but
they apparently result from various other phases of vibratory agitation of
the bottom waters. They are sometimes made by streams and stream-like
currents. Ripple-marks are apparently preserved indefinitely under proper
circumstances. They are sometimes found, for example, on very ancient
quartzites. Ripples are also made by wind (p. 37). Ripple-marks are usually
Page 569
only an inch or two from crest to crest, but in rare instances they attain
much greater size. Examples of ripple-marks 30 feet across are known.[211]
Occasional ridges and depressions of much greater dimensions are
produced which are attributable to the formation of successive bars, or to
the building of wave-cusps.[212] Rill-marks are not infrequently produced by
the undertow and other currents passing over pebbles, shells, etc. (Figs. 325
and 326).
Fig. 369.—Mud-cracks in Brunswick Shale, N. J. (Kümmel.)
Sediments are sometimes exposed between tides, or under other
circumstances, for periods long enough to permit drying and cracking at the
surface. On the return of the waters, the cracks may be filled and
permanently preserved. These are known as sun-cracks or mud-cracks
(Figs. 328 and 369). They chiefly affect shales, but are occasionally seen in
limestones and fine-grained sandstones. During the exposure of the
sediments a shower may pass and rain-drop impressions (Fig. 370) be made
which are subsequently filled by fine sediment and preserved. The size and
depth of rain-drop impressions give some hint as to the meteorological
conditions of far-off ages. Wave-marks, which consist of the faint line-
ridges developed on a sandy beach at the limit of the incoming wave, are
much greater size. Examples of ripple-marks 30 feet across are known.[211]
Occasional ridges and depressions of much greater dimensions are
produced which are attributable to the formation of successive bars, or to
the building of wave-cusps.[212] Rill-marks are not infrequently produced by
the undertow and other currents passing over pebbles, shells, etc. (Figs. 325
and 326).
Fig. 369.—Mud-cracks in Brunswick Shale, N. J. (Kümmel.)
Sediments are sometimes exposed between tides, or under other
circumstances, for periods long enough to permit drying and cracking at the
surface. On the return of the waters, the cracks may be filled and
permanently preserved. These are known as sun-cracks or mud-cracks
(Figs. 328 and 369). They chiefly affect shales, but are occasionally seen in
limestones and fine-grained sandstones. During the exposure of the
sediments a shower may pass and rain-drop impressions (Fig. 370) be made
which are subsequently filled by fine sediment and preserved. The size and
depth of rain-drop impressions give some hint as to the meteorological
conditions of far-off ages. Wave-marks, which consist of the faint line-
ridges developed on a sandy beach at the limit of the incoming wave, are
Page 570
sometimes preserved and may be seen occasionally on layers of rock
deposited millions of years ago.
Fig. 370.—Rain-drop impressions. (Brigham.)
Concretionary structure.—Various sedimentary formations contain
nodules or irregularly shaped masses of mineral matter unlike the rock in
which they occur. When these nodules consist of matter aggregated about
some center, they are called concretions. They are common in sedimentary
rocks, and here it may sometimes be seen that the aggregation has taken
place about a shell, a leaf, or some other organic relic. The nuclei are,
however, not always organic. The material of the concretion may have
come from the immediately surrounding rock, having been first dissolved
by water and then deposited about the nucleus, or it may have been
introduced from without, likewise by the agency of water. In the first case,
the mineral matter of the concretion is usually one of the minor constituents
of the rock. Thus the commonest concretions in limestone are composed of
impure silica (chert, Fig. 361); in shale, of lime carbonate or iron sulphide;
in sandstone, of iron oxide. The concretion may be made up almost wholly
of concentrated matter, in which case the matter originally in the place of
the concretion has been crowded aside; or it may involve much of the
material of the imbedding rock. Thus the concretion of lime carbonate in
shale may be nearly pure, or it may involve much of the earthy matter of the
deposited millions of years ago.
Fig. 370.—Rain-drop impressions. (Brigham.)
Concretionary structure.—Various sedimentary formations contain
nodules or irregularly shaped masses of mineral matter unlike the rock in
which they occur. When these nodules consist of matter aggregated about
some center, they are called concretions. They are common in sedimentary
rocks, and here it may sometimes be seen that the aggregation has taken
place about a shell, a leaf, or some other organic relic. The nuclei are,
however, not always organic. The material of the concretion may have
come from the immediately surrounding rock, having been first dissolved
by water and then deposited about the nucleus, or it may have been
introduced from without, likewise by the agency of water. In the first case,
the mineral matter of the concretion is usually one of the minor constituents
of the rock. Thus the commonest concretions in limestone are composed of
impure silica (chert, Fig. 361); in shale, of lime carbonate or iron sulphide;
in sandstone, of iron oxide. The concretion may be made up almost wholly
of concentrated matter, in which case the matter originally in the place of
the concretion has been crowded aside; or it may involve much of the
material of the imbedding rock. Thus the concretion of lime carbonate in
shale may be nearly pure, or it may involve much of the earthy matter of the
Page 571
shale, while the concretion of iron oxide in sandstone commonly includes
much sand. In extreme cases, indeed, the concentrated matter of the
concretion merely cements the material involved into distinct nodules.
Occasionally the rock substance itself takes on a concretionary form, all or
most of its material being involved.
Fig. 371.—Discoid calcareous concretions from post-glacial clays. Ryegate, Vt. (Photo. by
Church.)
much sand. In extreme cases, indeed, the concentrated matter of the
concretion merely cements the material involved into distinct nodules.
Occasionally the rock substance itself takes on a concretionary form, all or
most of its material being involved.
Fig. 371.—Discoid calcareous concretions from post-glacial clays. Ryegate, Vt. (Photo. by
Church.)
Page 572
Fig. 372.—Irregular calcareous concretions. Ryegate, Vt. (Photo. by Church.)
Page 573
Fig. 373.—Calcareous concretions, some of them showing bilateral symmetry. Ryegate, Vt.
(Photo. by Church.)
(Photo. by Church.)
Page 574
Fig. 374.—Irregular tubular silicious concretions in Arikaree clays. Northwest of Wildcat
Mountain, Banner Co., Neb. (Darton, U. S. Geol. Surv.)
In size, concretions may vary from microscopic dimensions to huge
masses, 8, 10, or even more feet in diameter. The variations in shape are
also great. They may be spherical, elliptical, discoid, or they may assume
more irregular and complex forms (Figs. 371 and 372). The conditions of
growth have much to do with the form. Thus a concretion which starts as a
sphere may find growth easier in one plane than another, when it becomes
discoid. Two or more concretions sometimes grow together, giving rise to
complicated forms. Some of the most complex and fantastic forms are
perhaps to be explained in this way. Concretions sometimes take the form
of tubes. Some minute tubular concretions were formed about rootlets, but
the larger ones appear to owe their form to other influences (Fig. 374).
Mountain, Banner Co., Neb. (Darton, U. S. Geol. Surv.)
In size, concretions may vary from microscopic dimensions to huge
masses, 8, 10, or even more feet in diameter. The variations in shape are
also great. They may be spherical, elliptical, discoid, or they may assume
more irregular and complex forms (Figs. 371 and 372). The conditions of
growth have much to do with the form. Thus a concretion which starts as a
sphere may find growth easier in one plane than another, when it becomes
discoid. Two or more concretions sometimes grow together, giving rise to
complicated forms. Some of the most complex and fantastic forms are
perhaps to be explained in this way. Concretions sometimes take the form
of tubes. Some minute tubular concretions were formed about rootlets, but
the larger ones appear to owe their form to other influences (Fig. 374).
Page 575
Fig. 375.—Section of a concretion (septarium) the cracks of which have been filled by
matter deposited from solution. About half natural size. (Photo. by Church.)
matter deposited from solution. About half natural size. (Photo. by Church.)
Page 576
Fig. 376.—Section of a concretion, the cracks in which have been filled by deposition from
solution. The filling appears to have wedged the parts of the original concretion apart.
The fillings are veins. Some of them show that the vein-material was deposited on both
walls. About half natural size. (Photo. by Church.)
One of the most extraordinary features of some concretions of complex
form is their symmetry. This may be of various phases; in exceptional cases
there is a bilateral symmetry almost as perfect as in the higher types of
animals. This is especially true of certain calcareous concretions developed
in plastic clays (Fig. 373).
solution. The filling appears to have wedged the parts of the original concretion apart.
The fillings are veins. Some of them show that the vein-material was deposited on both
walls. About half natural size. (Photo. by Church.)
One of the most extraordinary features of some concretions of complex
form is their symmetry. This may be of various phases; in exceptional cases
there is a bilateral symmetry almost as perfect as in the higher types of
animals. This is especially true of certain calcareous concretions developed
in plastic clays (Fig. 373).
Page 577
Fig. 377.—Septarium from Cretaceous clays near the east base of the Rocky Mountains in
Montana. (Photo. by Church.)
Concretions sometimes develop cracks within themselves, and these may
then be filled with mineral matter differing in composition or color from
that of the original concretions (Figs. 375 and 376). Concretions the cracks
of which have been filled by deposition from solution, are called septaria.
They are especially abundant in some of the Cretaceous shales and clays. In
not a few cases the filling of the cracks appears to have wedged segments of
the original concretion farther and farther apart, until the outer surface of
the septarium is made up more largely of vein-matter than of the original
concretion (Fig. 377). Such concretions are often popularly known as
“petrified turtles.”
Montana. (Photo. by Church.)
Concretions sometimes develop cracks within themselves, and these may
then be filled with mineral matter differing in composition or color from
that of the original concretions (Figs. 375 and 376). Concretions the cracks
of which have been filled by deposition from solution, are called septaria.
They are especially abundant in some of the Cretaceous shales and clays. In
not a few cases the filling of the cracks appears to have wedged segments of
the original concretion farther and farther apart, until the outer surface of
the septarium is made up more largely of vein-matter than of the original
concretion (Fig. 377). Such concretions are often popularly known as
“petrified turtles.”
Page 578
Concretions of the sort indicated above often develop after the enclosing
sedimentary rock was deposited. This is shown, among other things, by the
fact that numerous planes of lamination may sometimes be traced through
the concretions.
Concretions also form in water during the deposition of sedimentary
rock. Exceptionally, sedimentary rock is made up chiefly of concretions.
The chemical precipitates from the concentrated waters of certain enclosed
lakes sometimes take the form of minute spherules which resemble the roe
of fish. From this resemblance the resulting rock is called oolite (Fig. 357).
Oolite is now forming about some coral reefs, presumably from the
precipitation of the lime carbonate which was temporarily in solution.
Considerable beds of limestone are sometimes oolitic. The calcium
carbonate of such rock may be subsequently replaced by silica, so that the
oolitic structure is sometimes found in silicious rock. If the concretions
become larger, say as large as peas, the rock is called pisolite instead of
oolite (Fig. 378).
Fig. 378.—Pisolite. Half natural size. (Photo. by Church.)
sedimentary rock was deposited. This is shown, among other things, by the
fact that numerous planes of lamination may sometimes be traced through
the concretions.
Concretions also form in water during the deposition of sedimentary
rock. Exceptionally, sedimentary rock is made up chiefly of concretions.
The chemical precipitates from the concentrated waters of certain enclosed
lakes sometimes take the form of minute spherules which resemble the roe
of fish. From this resemblance the resulting rock is called oolite (Fig. 357).
Oolite is now forming about some coral reefs, presumably from the
precipitation of the lime carbonate which was temporarily in solution.
Considerable beds of limestone are sometimes oolitic. The calcium
carbonate of such rock may be subsequently replaced by silica, so that the
oolitic structure is sometimes found in silicious rock. If the concretions
become larger, say as large as peas, the rock is called pisolite instead of
oolite (Fig. 378).
Fig. 378.—Pisolite. Half natural size. (Photo. by Church.)
Page 579
Fig. 379.—Columnar structure, “Devil’s Post Pile.” Upper San Joaquin Canyon, Sierra
Nevada Mountains.
Beds of iron ore are likewise sometimes concretionary. Thus in the
Clinton formation there are widespread beds of “flaxseed” ore made up of
concretions of iron oxide which, individually, resemble the seed which has
given the ore its name. The nucleus in this case is usually too small for
identification.
Secretions.—When cavities in rock are filled by material deposited from
solution, the result is sometimes called a secretion. Secretions therefore
grow from without toward a center, while concretions follow the opposite
order. Crystal-lined cavities (geodes, Fig. 359) and agates (Fig. 358) are
examples of secretions. Crystal-lined cavities and veins are the same in
principle.
STRUCTURAL FEATURES OF IGNEOUS ROCKS.
Nevada Mountains.
Beds of iron ore are likewise sometimes concretionary. Thus in the
Clinton formation there are widespread beds of “flaxseed” ore made up of
concretions of iron oxide which, individually, resemble the seed which has
given the ore its name. The nucleus in this case is usually too small for
identification.
Secretions.—When cavities in rock are filled by material deposited from
solution, the result is sometimes called a secretion. Secretions therefore
grow from without toward a center, while concretions follow the opposite
order. Crystal-lined cavities (geodes, Fig. 359) and agates (Fig. 358) are
examples of secretions. Crystal-lined cavities and veins are the same in
principle.
STRUCTURAL FEATURES OF IGNEOUS ROCKS.
Page 580
Certain structural features of igneous rocks have been mentioned in
treating of their origin in the previous chapter. When a great flow of lava
spreads out upon the surface, there is no internal lamination or stratification,
and the resulting rock is usually classified as massive rather than stratified;
but when a succession of flows occur, each individual flow forms a layer,
and the series as a whole becomes stratiform. The successive flows are not
usually coextensive. If the later flows of the closing stages of a period of
vulcanism fail to reach as far as the earlier ones, a terraced or step-like
aspect is given to the region, whence the name trap-rock (trappe, steps) is
derived. Such lava sheets, especially if of basalt, often assume a columnar
structure in cooling, the columns being rude six-sided prisms standing at
right angles to the cooling surfaces (Figs. 379 and 380). This phenomenon
is usually best developed where the sheet is intruded between layers of
preexisting rock in the form of sills. The formation of the columns is
sometimes regarded as a variety of concretionary action, but more
commonly as a result of contraction. The former is suggested by the ball-
and-socket ends of the sections of some columns (Fig. 382). The
development of the columns by contraction may be explained as follows:
The surface of the homogeneous lava contracts about equally in all
directions on cooling. The contractile force may be thought of as centering
about equidistant points. About a given point, the least number of cracks
which will relieve the tension in all directions is three (Fig. 383). If these
radiate symmetrically from the point, the angle between any two is 120°,
the angle of the hexagonal prism. Similar radiating cracks from other
centers complete the columns (Fig. 384). A five-sided column would arise
from the failure of the cracks to develop about some one of the points (Fig.
385).
treating of their origin in the previous chapter. When a great flow of lava
spreads out upon the surface, there is no internal lamination or stratification,
and the resulting rock is usually classified as massive rather than stratified;
but when a succession of flows occur, each individual flow forms a layer,
and the series as a whole becomes stratiform. The successive flows are not
usually coextensive. If the later flows of the closing stages of a period of
vulcanism fail to reach as far as the earlier ones, a terraced or step-like
aspect is given to the region, whence the name trap-rock (trappe, steps) is
derived. Such lava sheets, especially if of basalt, often assume a columnar
structure in cooling, the columns being rude six-sided prisms standing at
right angles to the cooling surfaces (Figs. 379 and 380). This phenomenon
is usually best developed where the sheet is intruded between layers of
preexisting rock in the form of sills. The formation of the columns is
sometimes regarded as a variety of concretionary action, but more
commonly as a result of contraction. The former is suggested by the ball-
and-socket ends of the sections of some columns (Fig. 382). The
development of the columns by contraction may be explained as follows:
The surface of the homogeneous lava contracts about equally in all
directions on cooling. The contractile force may be thought of as centering
about equidistant points. About a given point, the least number of cracks
which will relieve the tension in all directions is three (Fig. 383). If these
radiate symmetrically from the point, the angle between any two is 120°,
the angle of the hexagonal prism. Similar radiating cracks from other
centers complete the columns (Fig. 384). A five-sided column would arise
from the failure of the cracks to develop about some one of the points (Fig.
385).
Page 581
Fig. 380.—Columnar structure, obsidian cliff, Yellowstone Park. (Iddings, U. S. Geol.
Surv.)
When lava is forced into crevices or rises to the surface through fissures,
and the residual portion solidifies in them, it gives rise to dikes, as
illustrated in Figs. 2 and 417 (not a true dike). Dikes are sometimes affected
by columnar structure. In this case, as in all others, the columns are likely to
be at right angles to the cooling surface. Lava solidifying in the passageway
leading from the interior of a volcano gives rise to a neck or plug. If the lava
is forced between beds of rock in the form of a sheet, and solidifies there, it
is called a sill. If, after rising to a certain point in the strata, the lava arches
Surv.)
When lava is forced into crevices or rises to the surface through fissures,
and the residual portion solidifies in them, it gives rise to dikes, as
illustrated in Figs. 2 and 417 (not a true dike). Dikes are sometimes affected
by columnar structure. In this case, as in all others, the columns are likely to
be at right angles to the cooling surface. Lava solidifying in the passageway
leading from the interior of a volcano gives rise to a neck or plug. If the lava
is forced between beds of rock in the form of a sheet, and solidifies there, it
is called a sill. If, after rising to a certain point in the strata, the lava arches
Page 582
the beds above into a dome, and forms a great lens-like or cistern-like mass,
it constitutes a laccolith (Fig. 334). If an intrusion of the laccolithic type
faults the overlying beds instead of arching them, and especially if the
vertical dimension of the intruded mass be great in comparison with its
lateral dimensions, its shape is more like that of a plug or core. Such an
intruded core is a bysmalith[213] (Fig. 124). Between the bysmalith and the
laccolith there are various gradations, just as between the laccolith and the
sill. When lava forces aside the rocks at considerable depths or absorbs
them by solution or by “stoping,” and then solidifies in great masses of
irregular or undetermined forms, these masses are called batholiths.
Fig. 381. Fig. 382. Fig. 383.
Fig. 381.—Sections of columns from Giant’s Causeway, coast of Ireland.
Fig. 382.—Ball-and-socket joints in columns of basalt. (Scrope.)
Fig. 383.—Diagram to illustrate the first stages in the formation of hexagonal
columns by contraction.
Fig. 384. Fig. 385.
it constitutes a laccolith (Fig. 334). If an intrusion of the laccolithic type
faults the overlying beds instead of arching them, and especially if the
vertical dimension of the intruded mass be great in comparison with its
lateral dimensions, its shape is more like that of a plug or core. Such an
intruded core is a bysmalith[213] (Fig. 124). Between the bysmalith and the
laccolith there are various gradations, just as between the laccolith and the
sill. When lava forces aside the rocks at considerable depths or absorbs
them by solution or by “stoping,” and then solidifies in great masses of
irregular or undetermined forms, these masses are called batholiths.
Fig. 381. Fig. 382. Fig. 383.
Fig. 381.—Sections of columns from Giant’s Causeway, coast of Ireland.
Fig. 382.—Ball-and-socket joints in columns of basalt. (Scrope.)
Fig. 383.—Diagram to illustrate the first stages in the formation of hexagonal
columns by contraction.
Fig. 384. Fig. 385.
Page 583
Fig. 384.—The completion of the hexagonal columns.
Fig. 385.—Diagram to illustrate the development of five-sided columns.
Volcanic cones are familiar structures built up about the vents of active
volcanoes, and will be discussed under vulcanism.
STRUCTURAL FEATURES ARISING FROM
DISTURBANCE.
Inclination and folding of strata.—The original attitude of beds,
whether formed by water or by lava-flows, is normally horizontal, or nearly
so. Both kinds of deposits, however, occasionally take place on
considerable slopes. Modifications of the original attitude result from earth
movements, and the measurement of these modifications is an important
feature of field study. It is recorded in terms of dip and strike. The dip is the
inclination of the beds referred to a horizontal plane, as illustrated in Fig.
386, and is usually measured by a clinometer, the principle of which is
shown in Fig. 387. In measuring the dip, the maximum angle is always
taken. In Fig. 386, for example, the angle would be less if the direction
were either to the right or left of that indicated by the arrow. The direction
as well as the amount of the dip is always to be noted. This must be
determined by the compass, to which the clinometer may be conveniently
attached. Dip 40°, S. 20° W. gives the full record of the position of the bed
of rock under consideration. The strike is the direction of the horizontal
edge of dipping beds, or more generally, the direction of a horizontal line on
the surface of the beds. This is illustrated in Fig. 386. Since the strike is
always at right angles to the dip, the strike need not be recorded if the
direction of the dip is. Thus dip 40°, S. 20° W. is the same as dip 40°, strike
N. 70° W.
Fig. 385.—Diagram to illustrate the development of five-sided columns.
Volcanic cones are familiar structures built up about the vents of active
volcanoes, and will be discussed under vulcanism.
STRUCTURAL FEATURES ARISING FROM
DISTURBANCE.
Inclination and folding of strata.—The original attitude of beds,
whether formed by water or by lava-flows, is normally horizontal, or nearly
so. Both kinds of deposits, however, occasionally take place on
considerable slopes. Modifications of the original attitude result from earth
movements, and the measurement of these modifications is an important
feature of field study. It is recorded in terms of dip and strike. The dip is the
inclination of the beds referred to a horizontal plane, as illustrated in Fig.
386, and is usually measured by a clinometer, the principle of which is
shown in Fig. 387. In measuring the dip, the maximum angle is always
taken. In Fig. 386, for example, the angle would be less if the direction
were either to the right or left of that indicated by the arrow. The direction
as well as the amount of the dip is always to be noted. This must be
determined by the compass, to which the clinometer may be conveniently
attached. Dip 40°, S. 20° W. gives the full record of the position of the bed
of rock under consideration. The strike is the direction of the horizontal
edge of dipping beds, or more generally, the direction of a horizontal line on
the surface of the beds. This is illustrated in Fig. 386. Since the strike is
always at right angles to the dip, the strike need not be recorded if the
direction of the dip is. Thus dip 40°, S. 20° W. is the same as dip 40°, strike
N. 70° W.
Page 584
Fig. 386.—Diagram illustrating dip and strike. (Geikie.)
Fig. 387.—The clinometer.
Fig. 387.—The clinometer.
Page 585
Fig. 388.—Open anticline, near Hancock, Md. (Russell, U. S. Geol. Surv.)
Page 586
Fig. 389.—Closed anticline, near Levis Station, Quebec. (Walcott, U. S. Geol. Surv.)
Fig. 390.—Inclined anticline. (Van Hise, U. S. Geol. Surv.)
Fig. 390.—Inclined anticline. (Van Hise, U. S. Geol. Surv.)
Page 587
Fig. 391.—Recumbent anticline. (Van Hise, U. S. Geol. Surv.)
Fig. 392.—Syncline, C. & O. canal, 3 miles west of Hancock, Md. The beds are shale and
sandstone near base of the Silurian. (Walcott, U. S. Geol. Surv.)
When the beds incline in a single direction, they form a monocline. When
beds are arched so as to incline away from one another, they form an up-
fold or anticline (Figs. 388 to 391). The anticline may depart from its
simple form, as shown in Figs. 390 and 391. When beds are curved
Fig. 392.—Syncline, C. & O. canal, 3 miles west of Hancock, Md. The beds are shale and
sandstone near base of the Silurian. (Walcott, U. S. Geol. Surv.)
When the beds incline in a single direction, they form a monocline. When
beds are arched so as to incline away from one another, they form an up-
fold or anticline (Figs. 388 to 391). The anticline may depart from its
simple form, as shown in Figs. 390 and 391. When beds are curved
Page 588
downward so as to incline towards one another, they form a syncline (Fig.
392). When beds assume the position shown in Fig. 393, the folds are said
to be isoclinal. When they are arched so as to form a cone or dome, and
incline in all directions from a central point, they are said to have a
quaquaversal dip. When considerable tracts are bent so as to form great
arches or great troughs with many minor undulations on the flanks of the
larger, they are designated as geanticlines, or anticlinoria (Figs. 394 and
395), and geosynclines or synclinoria (Figs. 396 and 397). Folding is often
accompanied by the development of slaty cleavage (p. 440).
Fig. 393.—Isocline. (Van Hise, U. S. Geol. Surv.)
Fig. 394.—Anticlinorium: diagrammatic. (Van Hise, U. S. Geol. Surv.)
Fig. 395.—Anticlinorium. General section in the central massif of the Alps. (Heim.)
392). When beds assume the position shown in Fig. 393, the folds are said
to be isoclinal. When they are arched so as to form a cone or dome, and
incline in all directions from a central point, they are said to have a
quaquaversal dip. When considerable tracts are bent so as to form great
arches or great troughs with many minor undulations on the flanks of the
larger, they are designated as geanticlines, or anticlinoria (Figs. 394 and
395), and geosynclines or synclinoria (Figs. 396 and 397). Folding is often
accompanied by the development of slaty cleavage (p. 440).
Fig. 393.—Isocline. (Van Hise, U. S. Geol. Surv.)
Fig. 394.—Anticlinorium: diagrammatic. (Van Hise, U. S. Geol. Surv.)
Fig. 395.—Anticlinorium. General section in the central massif of the Alps. (Heim.)
Page 589
Fig. 396.—Synclinorium: diagrammatic. (Van Hise, U. S. Geol. Surv.)
Fig. 397.—Synclinorium, Mt. Greylock, Mass. (Dale, U. S. Geol. Surv.)
Fig. 398.—A series of diagrams illustrating actual field relations in regions of folded strata.
Westchester Co., N. Y. (Dana.)
Fig. 397.—Synclinorium, Mt. Greylock, Mass. (Dale, U. S. Geol. Surv.)
Fig. 398.—A series of diagrams illustrating actual field relations in regions of folded strata.
Westchester Co., N. Y. (Dana.)
Page 590
Fig. 399. Fig. 400.
Fig. 399.—Diagram to show how dip and strike are recorded.
Fig. 400.—Map record of dip and strike, showing synclinal structure.
Fig. 401. Fig. 402.
Fig. 401.—Map record of dip and strike showing anticlinal structure.
Fig. 402.—The structure of the area shown in Fig. 401, in cross-section.
As found in the field, folds are usually much eroded, and often
completely truncated (Fig. 398). The determination of anticlinal or synclinal
structure is then not based on topography, or even on such sections as
shown in Figs. 394 to 397, for such sections are relatively rare. The
structure is determined by a careful record of dips and strikes. On the field
map, the record may be made as shown in Figs. 399 to 401, where the free
ends of the lines with but one free end point in the direction of dip, while
the other lines represent the directions of strike. Applying this method, the
structure shown in Fig. 400 represents a syncline, and that in Fig. 401 an
anticline. In cross-section, the structure presented by Fig. 401 would appear
as in Fig. 402. Fig. 403 shows a doubly plunging anticline; that is, an
anticline the axis of which dips down at either end. Fig. 404 shows a
combination of synclines and anticlines, and Fig. 405 a cross-section along
the line ab of Fig. 404. The outcrops of rock where the dip and strike may
be determined may be few and far between, but when they are sufficiently
Fig. 399.—Diagram to show how dip and strike are recorded.
Fig. 400.—Map record of dip and strike, showing synclinal structure.
Fig. 401. Fig. 402.
Fig. 401.—Map record of dip and strike showing anticlinal structure.
Fig. 402.—The structure of the area shown in Fig. 401, in cross-section.
As found in the field, folds are usually much eroded, and often
completely truncated (Fig. 398). The determination of anticlinal or synclinal
structure is then not based on topography, or even on such sections as
shown in Figs. 394 to 397, for such sections are relatively rare. The
structure is determined by a careful record of dips and strikes. On the field
map, the record may be made as shown in Figs. 399 to 401, where the free
ends of the lines with but one free end point in the direction of dip, while
the other lines represent the directions of strike. Applying this method, the
structure shown in Fig. 400 represents a syncline, and that in Fig. 401 an
anticline. In cross-section, the structure presented by Fig. 401 would appear
as in Fig. 402. Fig. 403 shows a doubly plunging anticline; that is, an
anticline the axis of which dips down at either end. Fig. 404 shows a
combination of synclines and anticlines, and Fig. 405 a cross-section along
the line ab of Fig. 404. The outcrops of rock where the dip and strike may
be determined may be few and far between, but when they are sufficiently
Page 591
near one another, the structure of the rock, as shown in
Fig. 405, may be worked out, even though the surface
be flat.
Fig. 403.—Map
record of dip and
strike showing
plunging (dipping
down at ends)
anticline.
Fig. 404.—Map record of dip and strike showing complex structure.
Fig. 405, may be worked out, even though the surface
be flat.
Fig. 403.—Map
record of dip and
strike showing
plunging (dipping
down at ends)
anticline.
Fig. 404.—Map record of dip and strike showing complex structure.
Page 592
Fig. 405.—Cross-section of Fig. 404 along the line ab.
Fig. 406.—Complex folding. Section across the Alps from the neighborhood of Zürich
toward Como: about 110 miles. (Heim and Prestwich.)
Fig. 407.—Generalized fan fold of the central massif of the Alps. (Heim.)
Fig. 406.—Complex folding. Section across the Alps from the neighborhood of Zürich
toward Como: about 110 miles. (Heim and Prestwich.)
Fig. 407.—Generalized fan fold of the central massif of the Alps. (Heim.)
Page 593
Fig. 408.—Intimate crumpling of beds near head of Sperry glacier, Mont. (Meyers.)
Fig. 409.—Intimate crumpling in detail, accompanied by faulting. Jasper Hill, Ishpeming,
Mich. (Meyers.)
Fig. 409.—Intimate crumpling in detail, accompanied by faulting. Jasper Hill, Ishpeming,
Mich. (Meyers.)
Page 594
Much the larger portion of the earth’s surface is occupied by beds that
retain nearly their original horizontal attitude; but in mountainous regions
the beds have usually suffered bending, folding, crumpling, and crushing, in
various degrees, in the course of the deformations that gave rise to the
mountains. Distortion is on the whole most intense and characteristic in the
most ancient rocks known, the Archean, in which a distorted condition is
nearly universal, so far as observation goes. Distortion is assigned chiefly to
lateral thrust arising from the shrinkage of the earth, as explained in the
chapter on Earth Movements. The simpler, and some rather complex forms
of deformation, are shown in the preceding figures, but the folding is
sometimes much more complex (Fig. 406), the folds sometimes “fan” (Fig.
407), and the beds of which they are composed are sometimes intricately
crumpled (Figs. 408 to 410). Among these various phases of deformation
there are all gradations and combinations. Overturned folds reverse the
order of the strata in the under limb of the fold. After such folds have been
greatly eroded, so that their outer form is lost and their relations have
become obscure, the reversed beds are likely to be interpreted as though
they lay in natural order. In such a case as that represented in Fig. 411, a
complex structure may be interpreted as a simple one. Thus the strata of
Fig. 411 may have the structure shown in Fig. 412, 413, or 414, so far as
dip and strike show.
retain nearly their original horizontal attitude; but in mountainous regions
the beds have usually suffered bending, folding, crumpling, and crushing, in
various degrees, in the course of the deformations that gave rise to the
mountains. Distortion is on the whole most intense and characteristic in the
most ancient rocks known, the Archean, in which a distorted condition is
nearly universal, so far as observation goes. Distortion is assigned chiefly to
lateral thrust arising from the shrinkage of the earth, as explained in the
chapter on Earth Movements. The simpler, and some rather complex forms
of deformation, are shown in the preceding figures, but the folding is
sometimes much more complex (Fig. 406), the folds sometimes “fan” (Fig.
407), and the beds of which they are composed are sometimes intricately
crumpled (Figs. 408 to 410). Among these various phases of deformation
there are all gradations and combinations. Overturned folds reverse the
order of the strata in the under limb of the fold. After such folds have been
greatly eroded, so that their outer form is lost and their relations have
become obscure, the reversed beds are likely to be interpreted as though
they lay in natural order. In such a case as that represented in Fig. 411, a
complex structure may be interpreted as a simple one. Thus the strata of
Fig. 411 may have the structure shown in Fig. 412, 413, or 414, so far as
dip and strike show.
Page 595
Fig. 410.—Plicated layers of thin-bedded chert in limestone, etched by erosion. Lower
Cambrian (?), two miles southwest of Big Pine, Inyo Co., Cal. (Walcott, U. S. Geol. Surv.)
Joints.—The surface rocks of the earth are almost universally traversed
by deep cracks called joints (Figs. 415, 138 and 140). In most regions there
are at least two systems of joints, the crevices of each system being roughly
parallel to one another, while those of the two systems, where there are two,
are approximately at right angles. In regions of great disturbance, the
number of sets of joints is often three, four, or even more. The joints of each
set may be many yards apart, or in exceptional cases, but a few inches, or
even a fraction of an inch.
Generally speaking, there are more systems of joints, and more frequent
joints in each system, where the rocks are much deformed than where they
have been but little disturbed. In undisturbed rocks the joints approach
verticality, but in regions where the rocks have been notably deformed, the
joint planes may have any position. Not rarely they simulate bedding
Cambrian (?), two miles southwest of Big Pine, Inyo Co., Cal. (Walcott, U. S. Geol. Surv.)
Joints.—The surface rocks of the earth are almost universally traversed
by deep cracks called joints (Figs. 415, 138 and 140). In most regions there
are at least two systems of joints, the crevices of each system being roughly
parallel to one another, while those of the two systems, where there are two,
are approximately at right angles. In regions of great disturbance, the
number of sets of joints is often three, four, or even more. The joints of each
set may be many yards apart, or in exceptional cases, but a few inches, or
even a fraction of an inch.
Generally speaking, there are more systems of joints, and more frequent
joints in each system, where the rocks are much deformed than where they
have been but little disturbed. In undisturbed rocks the joints approach
verticality, but in regions where the rocks have been notably deformed, the
joint planes may have any position. Not rarely they simulate bedding
Page 596
planes, especially in igneous and metamorphic rocks (Fig. 416). In the latter
case especially, the cleavage due to jointing is often mistaken for bedding.
They do not ordinarily show themselves at the surface in regions where
there is much mantle rock, but they are readily seen in the faces of cliffs, in
quarries, and, in general, wherever rock is exposed (Figs. 138 and 140).
Though some of them extend to greater depths than rock has ever been
penetrated, joints are, after all, superficial phenomena. They must be limited
to the zone of fracture, and most of them are probably much more narrowly
limited. Joints frequently end at the plane of contact of two sorts of rock.
Thus a joint extending down through limestone may end where shale is
reached. Joints are frequently offset at the contact of layers or formations,
and a single joint sometimes gives place to many smaller ones. All these
phenomena are to be explained on the basis of the different constitution and
elasticity of various sorts of rock. Generally speaking, rigid rock is more
readily jointed than that which is more yielding.
Joints may remain closed, or they may gap. In the latter case, they may
be widened by solution, weathering, etc., but they are quite as likely to be
filled by detritus from above, or by material deposited from solution
(veins). It is along joint-planes that many rich ore-veins are developed (pp.
478–484).
Fig. 411.—This diagram might represent either isoclinal or monoclinal structure. In the
former case the strata might have the structure shown in any one of the following
Figures, 412 to 414, so far as dip and strike show. (Dana.)
Fig. 412. Fig. 413. Fig. 414.
Fig. 412.—A possible interpretation of Fig. 411. (Dana.)
Fig. 413.—A possible interpretation of Fig. 411. (Dana.)
Fig. 414.—A possible interpretation of Fig. 411. (Dana.) ]
case especially, the cleavage due to jointing is often mistaken for bedding.
They do not ordinarily show themselves at the surface in regions where
there is much mantle rock, but they are readily seen in the faces of cliffs, in
quarries, and, in general, wherever rock is exposed (Figs. 138 and 140).
Though some of them extend to greater depths than rock has ever been
penetrated, joints are, after all, superficial phenomena. They must be limited
to the zone of fracture, and most of them are probably much more narrowly
limited. Joints frequently end at the plane of contact of two sorts of rock.
Thus a joint extending down through limestone may end where shale is
reached. Joints are frequently offset at the contact of layers or formations,
and a single joint sometimes gives place to many smaller ones. All these
phenomena are to be explained on the basis of the different constitution and
elasticity of various sorts of rock. Generally speaking, rigid rock is more
readily jointed than that which is more yielding.
Joints may remain closed, or they may gap. In the latter case, they may
be widened by solution, weathering, etc., but they are quite as likely to be
filled by detritus from above, or by material deposited from solution
(veins). It is along joint-planes that many rich ore-veins are developed (pp.
478–484).
Fig. 411.—This diagram might represent either isoclinal or monoclinal structure. In the
former case the strata might have the structure shown in any one of the following
Figures, 412 to 414, so far as dip and strike show. (Dana.)
Fig. 412. Fig. 413. Fig. 414.
Fig. 412.—A possible interpretation of Fig. 411. (Dana.)
Fig. 413.—A possible interpretation of Fig. 411. (Dana.)
Fig. 414.—A possible interpretation of Fig. 411. (Dana.) ]
Page 597
Fig. 415.—Jointed rocks. Cayuga Lake, N. Y. (Hall.)
Joints have been referred to various causes, among which tension,
torsion,[214] earthquakes,[215] and shearing[216] are the most important. Most of
them may probably be referred to the tension or compression developed
during crustal movements.[217] In the formation of a simple fold, for
example, tension-joints parallel with the fold will be developed, if tension
goes beyond the limit of elasticity of the rock involved. If the axis of a fold
is not horizontal, that is, if it “plunges,” as it commonly does, a second set
of joints roughly perpendicular to the first will be developed. If the uplift be
dome-shaped and sufficient to develop joints, they will radiate from the
center. It is true that joints affect regions where the rocks have not been
folded, and where they have been deformed but little, but deformation to
some extent is well-nigh universal.
Joints have been referred to various causes, among which tension,
torsion,[214] earthquakes,[215] and shearing[216] are the most important. Most of
them may probably be referred to the tension or compression developed
during crustal movements.[217] In the formation of a simple fold, for
example, tension-joints parallel with the fold will be developed, if tension
goes beyond the limit of elasticity of the rock involved. If the axis of a fold
is not horizontal, that is, if it “plunges,” as it commonly does, a second set
of joints roughly perpendicular to the first will be developed. If the uplift be
dome-shaped and sufficient to develop joints, they will radiate from the
center. It is true that joints affect regions where the rocks have not been
folded, and where they have been deformed but little, but deformation to
some extent is well-nigh universal.
Page 598
Fig. 416.—Jointing in granite. The surface of the rock is a joint plane. Northwest boundary
of the United States. The edges of other joint planes normal to the surface are also shown.
(Ransome, U. S. Geol. Surv.)
of the United States. The edges of other joint planes normal to the surface are also shown.
(Ransome, U. S. Geol. Surv.)
Page 599
Fig. 417.—Sandstone dike. Northern California. (Diller, U. S. Geol. Surv.)
A minor cause of tension-jointing is shrinkage, due (1) to cooling, as in
the development of the columnar structure of certain lavas, and (2) to
dessication, as shown by the cracks developed in mud when it dries. These
causes, however, are not believed to affect rock structures to any
considerable depth. Torsional joints and joints due to earthquake vibrations
appear to be special phases of tension-joints.
Two or more sets of joints may also be produced by compression, the
number being dependent on the complexity of the folding. Many
A minor cause of tension-jointing is shrinkage, due (1) to cooling, as in
the development of the columnar structure of certain lavas, and (2) to
dessication, as shown by the cracks developed in mud when it dries. These
causes, however, are not believed to affect rock structures to any
considerable depth. Torsional joints and joints due to earthquake vibrations
appear to be special phases of tension-joints.
Two or more sets of joints may also be produced by compression, the
number being dependent on the complexity of the folding. Many
Page 600
compression-joints correspond in direction with planes of shearing. They
are often associated with minor faulting and with slaty cleavage.
Tension-joints appear to be much more widely distributed than
compression-joints.
Sandstone dikes.—Exceptionally, open joints are filled by the intrusion
of sedimentary material from beneath. Thus have arisen the remarkable
sandstone dikes[218] of the West, especially of California (Fig. 417). Such
dikes are sometimes several miles (nine at least) in length. The sand of
these dikes was forced up from beneath either by earthquake movements or
by hydrostatic pressure.
Faults.—The beds on one side of a
joint-plane or fissure are sometimes
elevated or depressed relative to those
on the opposite side, and the
displacement is known as a fault
(Figs. 418 and 419). The joint-planes
may have any position, and hence
fault-planes may vary from verticality
Fig. 418.—Diagram of a normal fault. to approximate horizontality. The
angle by which the fault-plane departs from a vertical position is known as
the hade (bac, Fig. 418). The vertical displacement (ac) is the throw and the
horizontal displacement (bc) the heave. The heave and the throw are to be
distinguished from the displacement, which is the amount of movement
along the fault-plane (ab, Fig. 418).
The cliff above the edge of the downthrow side is a fault-scarp. In many,
probably in most cases, the scarp has been destroyed, or at any rate greatly
obscured by erosion; but occasionally fault-scarps of mountainous heights,
as along the east face of the Sierras and along many of the basin ranges of
Utah, Nevada, etc., are found though much modified by erosion (Fig. 419).
Faults sometimes arise from over-intense folding (Fig. 420). A
deformation which at one point results merely in a bending of the beds, may
occasion a fault at another. Faults may pass into folds either vertically (Figs.
421 and 422) or horizontally (Fig. 423). In such cases, thickening and
thinning, and stretching and shortening of the beds is often involved (see
are often associated with minor faulting and with slaty cleavage.
Tension-joints appear to be much more widely distributed than
compression-joints.
Sandstone dikes.—Exceptionally, open joints are filled by the intrusion
of sedimentary material from beneath. Thus have arisen the remarkable
sandstone dikes[218] of the West, especially of California (Fig. 417). Such
dikes are sometimes several miles (nine at least) in length. The sand of
these dikes was forced up from beneath either by earthquake movements or
by hydrostatic pressure.
Faults.—The beds on one side of a
joint-plane or fissure are sometimes
elevated or depressed relative to those
on the opposite side, and the
displacement is known as a fault
(Figs. 418 and 419). The joint-planes
may have any position, and hence
fault-planes may vary from verticality
Fig. 418.—Diagram of a normal fault. to approximate horizontality. The
angle by which the fault-plane departs from a vertical position is known as
the hade (bac, Fig. 418). The vertical displacement (ac) is the throw and the
horizontal displacement (bc) the heave. The heave and the throw are to be
distinguished from the displacement, which is the amount of movement
along the fault-plane (ab, Fig. 418).
The cliff above the edge of the downthrow side is a fault-scarp. In many,
probably in most cases, the scarp has been destroyed, or at any rate greatly
obscured by erosion; but occasionally fault-scarps of mountainous heights,
as along the east face of the Sierras and along many of the basin ranges of
Utah, Nevada, etc., are found though much modified by erosion (Fig. 419).
Faults sometimes arise from over-intense folding (Fig. 420). A
deformation which at one point results merely in a bending of the beds, may
occasion a fault at another. Faults may pass into folds either vertically (Figs.
421 and 422) or horizontally (Fig. 423). In such cases, thickening and
thinning, and stretching and shortening of the beds is often involved (see
Page 601
Figs. 421 and 422). Faults are often due to the greater settling of the beds on
one side of a fissure than on the other, without special disposition to fold.
Fig. 419.—A fault-scarp; the triangular faces rising abruptly above the plain at the ends of
the spurs. (Davis.)
Fig. 420.—Diagrams showing relations of faults and folds.
Fig. 421. Fig. 422.
one side of a fissure than on the other, without special disposition to fold.
Fig. 419.—A fault-scarp; the triangular faces rising abruptly above the plain at the ends of
the spurs. (Davis.)
Fig. 420.—Diagrams showing relations of faults and folds.
Fig. 421. Fig. 422.
Page 602
Fig. 421.—The fault above grades into a fold below. Thickening and thinning of
layers next the fault-plane evident. Based on experimental results of Willis
(13th Ann. Rept., U. S. Geol. Surv.)
Fig. 422.—Fault below grading into fold above. Stretching and thinning, and
shortening and thickening of beds under pressure is involved. Based on
experimental results of Willis.
Fig. 423.—Diagram showing a fault grading into a monocline horizontally.
Fig. 424.—Slickenside surface. (Prestwich.)
The rock on either side of a fault-plane is often smoothed as the result of
the friction of movement. Such surfaces are slickensides (Fig. 424). A
slickenside surface has some resemblance to a glaciated surface, but
generally gives evidence of greater rigidity between the moving surfaces.
layers next the fault-plane evident. Based on experimental results of Willis
(13th Ann. Rept., U. S. Geol. Surv.)
Fig. 422.—Fault below grading into fold above. Stretching and thinning, and
shortening and thickening of beds under pressure is involved. Based on
experimental results of Willis.
Fig. 423.—Diagram showing a fault grading into a monocline horizontally.
Fig. 424.—Slickenside surface. (Prestwich.)
The rock on either side of a fault-plane is often smoothed as the result of
the friction of movement. Such surfaces are slickensides (Fig. 424). A
slickenside surface has some resemblance to a glaciated surface, but
generally gives evidence of greater rigidity between the moving surfaces.
Page 603
Faults are of two general classes, normal and reversed. In the normal
fault (Fig. 418) the overhanging side is the downthrow side, i.e., the
downthrow is on the side towards which the fault-plane inclines, as though
the overhanging beds had slidden down the slope. Normal faults, as a rule,
indicate an extension of strata, this being necessary to permit the dissevered
blocks to settle downwards. In the reversed fault, the overhanging beds
appear to have moved up the slope of the fault-plane, as though the
displacement took place under lateral pressure. This is clearly shown to be
the case where an overfold passes into a reversed fault (Fig. 420). Reversed
faults are further illustrated by Figs. 425, 426, and 427. Where the plane of
the reversed fault approaches horizontality, the fault is often called a thrust-
fault, or an overthrust. In such cases the throw is to be distinguished from
the stratigraphic throw (see Fig. 426). In thrust-faults, the heave is often
great. The eastern face of the Rocky Mountains near the boundary-line
between the United States and Canada has been pushed over the strata of
the bordering plains to a distance of at least eight miles.[219] Overthrusts of
like gigantic displacement have been detected in British Columbia,[220]
Scotland,[221] and elsewhere.
fault (Fig. 418) the overhanging side is the downthrow side, i.e., the
downthrow is on the side towards which the fault-plane inclines, as though
the overhanging beds had slidden down the slope. Normal faults, as a rule,
indicate an extension of strata, this being necessary to permit the dissevered
blocks to settle downwards. In the reversed fault, the overhanging beds
appear to have moved up the slope of the fault-plane, as though the
displacement took place under lateral pressure. This is clearly shown to be
the case where an overfold passes into a reversed fault (Fig. 420). Reversed
faults are further illustrated by Figs. 425, 426, and 427. Where the plane of
the reversed fault approaches horizontality, the fault is often called a thrust-
fault, or an overthrust. In such cases the throw is to be distinguished from
the stratigraphic throw (see Fig. 426). In thrust-faults, the heave is often
great. The eastern face of the Rocky Mountains near the boundary-line
between the United States and Canada has been pushed over the strata of
the bordering plains to a distance of at least eight miles.[219] Overthrusts of
like gigantic displacement have been detected in British Columbia,[220]
Scotland,[221] and elsewhere.
Page 604
Fig. 425.—Perspective view and vertical section of a thrust-fault. (Willis, U. S. Geol. Surv.)
Fig. 426.—Diagram of a thrust-fault illustrating the several terms used in describing faults.
The distinctions between heave and displacement, and between throw and stratigraphic
throw, are to be especially noted. (Willis, U. S. Geol. Surv.)
Fig. 426.—Diagram of a thrust-fault illustrating the several terms used in describing faults.
The distinctions between heave and displacement, and between throw and stratigraphic
throw, are to be especially noted. (Willis, U. S. Geol. Surv.)
Page 605
Fig. 427.—Step-fold showing (in 1) break in the massive limestone bed which determines
the plane of the break-thrust along which the displacement shown in 2 takes place.
(Willis, U. S. Geol. Surv.)
Sometimes a fault branches (Fig. 428) and sometimes the faulting is
distributed among a series of parallel planes at short distances from one
another,[222] instead of being concentrated along a single plane, thus giving
rise to a distributive fault (Fig. 429). This is perhaps more common in
normal than in reversed faulting.
Fig. 428. Fig. 429.
Fig. 428.—Branching-fault. (Powell.)
Fig. 429.—Diagram showing a series of small faults—distributive faulting.
the plane of the break-thrust along which the displacement shown in 2 takes place.
(Willis, U. S. Geol. Surv.)
Sometimes a fault branches (Fig. 428) and sometimes the faulting is
distributed among a series of parallel planes at short distances from one
another,[222] instead of being concentrated along a single plane, thus giving
rise to a distributive fault (Fig. 429). This is perhaps more common in
normal than in reversed faulting.
Fig. 428. Fig. 429.
Fig. 428.—Branching-fault. (Powell.)
Fig. 429.—Diagram showing a series of small faults—distributive faulting.
Page 606
Fig. 430.—Fault in Gering series. Near Rutland Siding, near Crawford, Neb. (Darton, U. S.
Geol. Surv.)
The amount of throw occasionally reaches several thousand feet.
Occasionally faults of incredible dimensions are reported, but these are
perhaps misinterpretations. Faults are observed to die out gradually when
traced horizontally, sometimes by passing into monoclinal folds, and
sometimes without connection with folding. In depth they probably die out
in similar ways in most cases. Where the throw is great, they probably give
place to folds below (Fig. 421). Other phenomena of faulting are illustrated
by Figs. 430–435. A fault of thousands, or even hundreds of feet is probably
the sum of numerous smaller slippings distributed through long intervals of
time. Faulting is probably one of the common causes of earthquakes.
Geol. Surv.)
The amount of throw occasionally reaches several thousand feet.
Occasionally faults of incredible dimensions are reported, but these are
perhaps misinterpretations. Faults are observed to die out gradually when
traced horizontally, sometimes by passing into monoclinal folds, and
sometimes without connection with folding. In depth they probably die out
in similar ways in most cases. Where the throw is great, they probably give
place to folds below (Fig. 421). Other phenomena of faulting are illustrated
by Figs. 430–435. A fault of thousands, or even hundreds of feet is probably
the sum of numerous smaller slippings distributed through long intervals of
time. Faulting is probably one of the common causes of earthquakes.
Page 607
Fig. 431.—Contorted and faulted laminated rock. Cook Inlet. (Gilbert, U. S. Geol. Surv.)
Fig. 432.—Faulting shown in a cobblestone. The fault-planes have become veins by
deposition from solution. The figure shows how the relative ages of crossing-faults may
be determined. (Schrader, U. S. Geol. Surv.)
Fig. 432.—Faulting shown in a cobblestone. The fault-planes have become veins by
deposition from solution. The figure shows how the relative ages of crossing-faults may
be determined. (Schrader, U. S. Geol. Surv.)
Page 608
Fig. 433.—Figure showing minute faulting. The length of the specimen is 8 inches. The
number of faults is nearly 100. (Photo. by Church.)
Fig. 434. Fig. 435.
Fig. 434.—Diagram illustrating common phenomena of a faulted region. (Dana.)
Fig. 435.—Diagram showing a fault, the plane of which forms an open fissure
and has been filled with débris from above. (Powell.)
The significance of faults.[223]—Faults afford a valuable indication of the
conditions of stress to which a region has been subjected, but some caution
must be exercised in their interpretation. Normal faults usually indicate an
extension of the surface sufficient to permit the fault-blocks to settle down
unequally. Reversed faults usually signify a compression of the surface
which requires the blocks to overlap one another more than they did before
the faulting. In other words, normal faulting usually implies tensional stress,
and reversed faulting compressional stress. It is not difficult to see,
however, that in an intensely compressed and folded region there might be
cases of normal faulting on the crests of folds where local stretching took
place, and that reversed faults might occur even in regions of tension. But
such cases must usually be local, and capable of detection and elimination
number of faults is nearly 100. (Photo. by Church.)
Fig. 434. Fig. 435.
Fig. 434.—Diagram illustrating common phenomena of a faulted region. (Dana.)
Fig. 435.—Diagram showing a fault, the plane of which forms an open fissure
and has been filled with débris from above. (Powell.)
The significance of faults.[223]—Faults afford a valuable indication of the
conditions of stress to which a region has been subjected, but some caution
must be exercised in their interpretation. Normal faults usually indicate an
extension of the surface sufficient to permit the fault-blocks to settle down
unequally. Reversed faults usually signify a compression of the surface
which requires the blocks to overlap one another more than they did before
the faulting. In other words, normal faulting usually implies tensional stress,
and reversed faulting compressional stress. It is not difficult to see,
however, that in an intensely compressed and folded region there might be
cases of normal faulting on the crests of folds where local stretching took
place, and that reversed faults might occur even in regions of tension. But
such cases must usually be local, and capable of detection and elimination
Page 609
by a study of the phenomena of the surrounding region. These exceptional
cases aside, the general inference from prevailing normal faults is that the
regions where they occur have undergone stretching, while the inference
from the less widely distributed reversed faults is that the surface where
they occur has undergone compression.
In view of the current opinion that the crust of the earth has been
subjected to great lateral thrust as a result of cooling, it is well to make
especial note of the fact that the faults which imply stretching are called
normal because they are the more abundant; and that the faults which imply
thrust are less common, and are styled reversed. The numerical ratio of
normal to reversed faults has never been closely determined, but normal
faults very greatly preponderate, and are estimated by some writers to
embrace 90-odd per cent. of the whole. The testimony of normal faults is
supported by the prevalence of gaping crevices, and of veins which are but
crevices that stood open until they were filled by deposition. All these
phenomena seem to testify to a stretched condition of the larger part of the
surface of the continents. This will again claim attention in the study of
Earth Movements.
Effect of faulting on outcrops.—
Faulting may bring about numerous
complications in the outcrop of rock
formations. In a series of formations having
a monoclinal structure (Fig. 436), many
changes may be introduced. Let it be
supposed in the following cases that, after
faulting, the surface has been reduced to
Fig. 436.—Diagram showing an planeness by erosion. If the fault-plane be
area of rock with monoclinal
structure. One layer notably
parallel to the strike of the beds (ab, Fig.
unlike the others. 436), and hence a strike fault, the outcrop
of a given layer may be duplicated (H, Fig.
437), or it may be eliminated altogether (Fig. 438). If the fault-plane be
parallel to the direction of dip (cd, Fig. 436), a dip fault, the layer H will
outcrop, as in Fig. 439, if the downthrow was on the far side, or as in Fig.
440 if the downthrow was on the opposite side. In both cases the outcrop H
is offset, the amount of the offset decreasing with increasing angle of dip
and increasing with increasing throw of the fault. If the fault be oblique to
cases aside, the general inference from prevailing normal faults is that the
regions where they occur have undergone stretching, while the inference
from the less widely distributed reversed faults is that the surface where
they occur has undergone compression.
In view of the current opinion that the crust of the earth has been
subjected to great lateral thrust as a result of cooling, it is well to make
especial note of the fact that the faults which imply stretching are called
normal because they are the more abundant; and that the faults which imply
thrust are less common, and are styled reversed. The numerical ratio of
normal to reversed faults has never been closely determined, but normal
faults very greatly preponderate, and are estimated by some writers to
embrace 90-odd per cent. of the whole. The testimony of normal faults is
supported by the prevalence of gaping crevices, and of veins which are but
crevices that stood open until they were filled by deposition. All these
phenomena seem to testify to a stretched condition of the larger part of the
surface of the continents. This will again claim attention in the study of
Earth Movements.
Effect of faulting on outcrops.—
Faulting may bring about numerous
complications in the outcrop of rock
formations. In a series of formations having
a monoclinal structure (Fig. 436), many
changes may be introduced. Let it be
supposed in the following cases that, after
faulting, the surface has been reduced to
Fig. 436.—Diagram showing an planeness by erosion. If the fault-plane be
area of rock with monoclinal
structure. One layer notably
parallel to the strike of the beds (ab, Fig.
unlike the others. 436), and hence a strike fault, the outcrop
of a given layer may be duplicated (H, Fig.
437), or it may be eliminated altogether (Fig. 438). If the fault-plane be
parallel to the direction of dip (cd, Fig. 436), a dip fault, the layer H will
outcrop, as in Fig. 439, if the downthrow was on the far side, or as in Fig.
440 if the downthrow was on the opposite side. In both cases the outcrop H
is offset, the amount of the offset decreasing with increasing angle of dip
and increasing with increasing throw of the fault. If the fault be oblique to
Page 610
the direction of dip and strike (ef, Fig. 436), an oblique fault, the outcrop of
such a layer as H will have the relations shown in Fig. 441 if the
downthrow was to the left, and that shown in Fig. 442 if the downthrow
was to the right. In the former case, it is said that there is offset with
overlap; in the latter, offset with gap. The amount of the overlap and gap,
respectively, increases with the increase of throw and hade, and decreases
with increase of dip. In all cases the outcrop (after the degradation of the
upthrow side) is shifted down dip.
Fig. 437.—Same as Fig. 436, after (1) displacement by a strike fault and (2) base-leveling.
The outcrops of certain beds are repeated.
Fig. 438.—Diagram illustrating how a strike fault in such a structure as that shown in Fig.
436 may cause the outcrop of certain beds to disappear.
Fig. 439.—Diagram illustrating how a dip fault in the structure shown in Fig. 436 affects
the outcrop when the downthrow was on the farther side of the fault-plane.
such a layer as H will have the relations shown in Fig. 441 if the
downthrow was to the left, and that shown in Fig. 442 if the downthrow
was to the right. In the former case, it is said that there is offset with
overlap; in the latter, offset with gap. The amount of the overlap and gap,
respectively, increases with the increase of throw and hade, and decreases
with increase of dip. In all cases the outcrop (after the degradation of the
upthrow side) is shifted down dip.
Fig. 437.—Same as Fig. 436, after (1) displacement by a strike fault and (2) base-leveling.
The outcrops of certain beds are repeated.
Fig. 438.—Diagram illustrating how a strike fault in such a structure as that shown in Fig.
436 may cause the outcrop of certain beds to disappear.
Fig. 439.—Diagram illustrating how a dip fault in the structure shown in Fig. 436 affects
the outcrop when the downthrow was on the farther side of the fault-plane.
Page 611
Fig. 440.—Same as Fig. 439, except that the downthrow was on the opposite side.
Fig. 441.—Oblique fault in the structure shown in Fig. 436. The downthrow was on the left
side. The outcrop of layer H is offset with overlap.
Fig. 442.—Same as Fig. 441, except that the downthrow was on the right side, and the offset
is with a gap instead of an overlap.
Fig. 443.—Diagram showing effect of faulting on the outcrops of synclinal beds.
Fig. 441.—Oblique fault in the structure shown in Fig. 436. The downthrow was on the left
side. The outcrop of layer H is offset with overlap.
Fig. 442.—Same as Fig. 441, except that the downthrow was on the right side, and the offset
is with a gap instead of an overlap.
Fig. 443.—Diagram showing effect of faulting on the outcrops of synclinal beds.
Page 612
Fig. 444.—Diagram showing effect of faulting on outcrops of anticlinal beds.
Fig. 445.—Diagram illustrating the effect of diminishing throw on outcrops in regions of
folded rocks.
If a fault crosses folds at right angles to their axes, the effect is to change
the distance between the outcrops of a given bed on opposite sides of the
fault, after the truncation of the folded beds. The distance is decreased on
the upthrow side of a syncline (Fig. 443) and increased on the upthrow side
of an anticline (Fig. 444). If the throw of a fault in tilted beds diminishes in
one direction, it may cause beds to outcrop, as shown in Fig. 445. Various
other complications arise under other circumstances. Since faults rarely
show themselves in the topography of the surface, except under special
circumstances (see p. 151), their detection and measurement is usually
based on the study of the relations of the beds involved, as illustrated by
Figs. 436–445.
Fig. 445.—Diagram illustrating the effect of diminishing throw on outcrops in regions of
folded rocks.
If a fault crosses folds at right angles to their axes, the effect is to change
the distance between the outcrops of a given bed on opposite sides of the
fault, after the truncation of the folded beds. The distance is decreased on
the upthrow side of a syncline (Fig. 443) and increased on the upthrow side
of an anticline (Fig. 444). If the throw of a fault in tilted beds diminishes in
one direction, it may cause beds to outcrop, as shown in Fig. 445. Various
other complications arise under other circumstances. Since faults rarely
show themselves in the topography of the surface, except under special
circumstances (see p. 151), their detection and measurement is usually
based on the study of the relations of the beds involved, as illustrated by
Figs. 436–445.
Page 613
CHAPTER IX.
THE MOVEMENTS AND DEFORMATIONS OF THE EARTH’S BODY
(DIASTROPHISM).
The body of the earth is subject to an infinite variety of movements,
ranging from the almost inconceivably rapid to the almost imperceptibly
slow, and from the almost immeasurably minute to the enormously massive;
but, for practical treatment, they fall mainly into two couplets: (1) the
minute and rapid, and (2) the slow and massive. Sudden movements of
local masses, giving rise to intense vibrations, are put in the first class.
There are innumerable minute and slow movements, but unless they rise to
appreciable magnitude by long continuance, they are neglected.
MINUTE AND RAPID MOVEMENTS.
The crust of the earth is in a state of perpetual tremor. For the most part,
these tremors are too minute to be sensible, but are revealed by delicate
instrumental devices. Some of them are but the declining stages of sensible
vibrations, but others are minute from their inception. Many of them spring
from the ordinary incidents of the surface, and claim attention chiefly as
obstacles to the study of more significant oscillations. Winds, waves,
waterfalls, the tread of animals, the rumble of traffic, the blasts of mines,
the changes of temperature, the variations in atmospheric pressure, the
weighting of rainfall and the lightening of evaporation, the rupture of rock
or ice or frozen earth, and many other processes, make their contributions to
local and minute movements. For the greater part, these vibrations are
superficial in origin, and are soon damped beyond recognition by dispersal
and by the inelastic and discontinuous nature of the looser material of the
surface. When a temporary rigid crust is formed by freezing, as in winter,
these surface vibrations are transmitted with much less loss, and the
distances at which the rumble of winter traffic is heard, is a good illustration
of the function of continuity and solidity in the conveyance of vibrations.
THE MOVEMENTS AND DEFORMATIONS OF THE EARTH’S BODY
(DIASTROPHISM).
The body of the earth is subject to an infinite variety of movements,
ranging from the almost inconceivably rapid to the almost imperceptibly
slow, and from the almost immeasurably minute to the enormously massive;
but, for practical treatment, they fall mainly into two couplets: (1) the
minute and rapid, and (2) the slow and massive. Sudden movements of
local masses, giving rise to intense vibrations, are put in the first class.
There are innumerable minute and slow movements, but unless they rise to
appreciable magnitude by long continuance, they are neglected.
MINUTE AND RAPID MOVEMENTS.
The crust of the earth is in a state of perpetual tremor. For the most part,
these tremors are too minute to be sensible, but are revealed by delicate
instrumental devices. Some of them are but the declining stages of sensible
vibrations, but others are minute from their inception. Many of them spring
from the ordinary incidents of the surface, and claim attention chiefly as
obstacles to the study of more significant oscillations. Winds, waves,
waterfalls, the tread of animals, the rumble of traffic, the blasts of mines,
the changes of temperature, the variations in atmospheric pressure, the
weighting of rainfall and the lightening of evaporation, the rupture of rock
or ice or frozen earth, and many other processes, make their contributions to
local and minute movements. For the greater part, these vibrations are
superficial in origin, and are soon damped beyond recognition by dispersal
and by the inelastic and discontinuous nature of the looser material of the
surface. When a temporary rigid crust is formed by freezing, as in winter,
these surface vibrations are transmitted with much less loss, and the
distances at which the rumble of winter traffic is heard, is a good illustration
of the function of continuity and solidity in the conveyance of vibrations.
Page 614
Earthquakes.
When the tremors spring from sources within the earth itself and are of
appreciable violence, they are recognized as earthquakes. The sources of
earthquake tremors are various. The most prevalent is probably the fracture
of rocks and the slipping of strata on each other in the process of faulting.
The interpretation of movements of this class has now been so far perfected
that the length and depth of the fault, the amount of the slip, and the
direction of the hade are capable of approximate estimation.[224] To the same
class belong the movements due to slumping. They are illustrated by the
sliding and arrest of great masses of sediment along the steep fronts of
deltas, and of the accumulations of deep-sea oozes on steep submarine
slopes. Such slumping is, in reality, superficial faulting. Seismic tremors
often attend volcanic eruptions, and are then probably attributable to the
sudden fracture and displacement of rock by the penetration of lava, or by
rapid and unequal heating. They are perhaps also due sometimes to the
sudden generation or cooling of steam in underground conduits, crevices,
and caverns, the action possibly being in some cases of the “water-hammer”
type. In rare instances, probably, the bursting of beds overlying pent-up
non-volcanic gases may give origin to earthquakes. A more superficial
source of earthquake vibrations is the collapse of the roofs of subterranean
caverns.
Seismic vibrations seem to be in part compressional, in part distortional,
in part (on the surface) undulatory, and in part irregular. The distortional are
especially significant, as they seem to imply a solid medium of
transmission.
Points of origin, foci.—It is probable that nearly or quite all earthquake
movements start within the upper ten miles of the crust, and most of them
within the upper five. Some of the earlier estimates indeed placed the points
of origin as deep as 20 or 30 miles, but in these cases the necessary
corrections, discussed below, were neglected. Most of the recent and more
accurate estimates fall within the limits given.
The method of estimating the depth of the centers of disturbance consists
in observing the directions of throw or thrust of bodies at the surface, and in
regarding these as representing the lines of emergence of the earthquake-
waves. By plotting these lines of emergence, and projecting them
When the tremors spring from sources within the earth itself and are of
appreciable violence, they are recognized as earthquakes. The sources of
earthquake tremors are various. The most prevalent is probably the fracture
of rocks and the slipping of strata on each other in the process of faulting.
The interpretation of movements of this class has now been so far perfected
that the length and depth of the fault, the amount of the slip, and the
direction of the hade are capable of approximate estimation.[224] To the same
class belong the movements due to slumping. They are illustrated by the
sliding and arrest of great masses of sediment along the steep fronts of
deltas, and of the accumulations of deep-sea oozes on steep submarine
slopes. Such slumping is, in reality, superficial faulting. Seismic tremors
often attend volcanic eruptions, and are then probably attributable to the
sudden fracture and displacement of rock by the penetration of lava, or by
rapid and unequal heating. They are perhaps also due sometimes to the
sudden generation or cooling of steam in underground conduits, crevices,
and caverns, the action possibly being in some cases of the “water-hammer”
type. In rare instances, probably, the bursting of beds overlying pent-up
non-volcanic gases may give origin to earthquakes. A more superficial
source of earthquake vibrations is the collapse of the roofs of subterranean
caverns.
Seismic vibrations seem to be in part compressional, in part distortional,
in part (on the surface) undulatory, and in part irregular. The distortional are
especially significant, as they seem to imply a solid medium of
transmission.
Points of origin, foci.—It is probable that nearly or quite all earthquake
movements start within the upper ten miles of the crust, and most of them
within the upper five. Some of the earlier estimates indeed placed the points
of origin as deep as 20 or 30 miles, but in these cases the necessary
corrections, discussed below, were neglected. Most of the recent and more
accurate estimates fall within the limits given.
The method of estimating the depth of the centers of disturbance consists
in observing the directions of throw or thrust of bodies at the surface, and in
regarding these as representing the lines of emergence of the earthquake-
waves. By plotting these lines of emergence, and projecting them
Page 615
backwards to their underground crossings, a first approximation to the
location of the focus is reached (the lines EF′, Fig. 446). From the nature of
the case, the observations of the angles of emergence cannot be very
accurate, but an effort is made to limit the error by making the number of
observations great.
Two systematic corrections are to be applied to all such estimates, the
one for varying elasticity and density, and the other for varying continuity.
Both reduce the estimated depth. In making the correction for varying
elasticity, it must be noted that the velocity of vibrations varies directly as
the square root of the elasticity, and inversely as the square root of the
density. The velocity is also accelerated by increase of temperature. The
elasticity, temperature, and density all increase with depth. Theoretically,
the increase of velocity due to the increasing elasticity and temperature of
increasing depths, overbalances the retardation due to increasing density,
and recent observations on the transmission of seismic waves through deep
chords of the earth have confirmed this conclusion. The path of the
vibration will, therefore, be curved toward the surface, as pointed out by
Schmidt and illustrated in Fig. 446, taken from his discussion.[225] From this
it is clear that the focus is not so deep as implied by the simple backward
projection of the lines of emergence.
location of the focus is reached (the lines EF′, Fig. 446). From the nature of
the case, the observations of the angles of emergence cannot be very
accurate, but an effort is made to limit the error by making the number of
observations great.
Two systematic corrections are to be applied to all such estimates, the
one for varying elasticity and density, and the other for varying continuity.
Both reduce the estimated depth. In making the correction for varying
elasticity, it must be noted that the velocity of vibrations varies directly as
the square root of the elasticity, and inversely as the square root of the
density. The velocity is also accelerated by increase of temperature. The
elasticity, temperature, and density all increase with depth. Theoretically,
the increase of velocity due to the increasing elasticity and temperature of
increasing depths, overbalances the retardation due to increasing density,
and recent observations on the transmission of seismic waves through deep
chords of the earth have confirmed this conclusion. The path of the
vibration will, therefore, be curved toward the surface, as pointed out by
Schmidt and illustrated in Fig. 446, taken from his discussion.[225] From this
it is clear that the focus is not so deep as implied by the simple backward
projection of the lines of emergence.
Page 616
Fig. 446.—Diagram illustrating by closed curves the different rates of propagation of
seismic tremors from a focus F, and, by lines normal to these, the changing directions of
propagation of the wave-front. It will be seen that the paths of propagation curve
upwards in approaching the surface. If the lines of emergence, as at E and E, be
projected backwards, as to F′, the points of crossing will be below the true focus.
A second correction must be made for the differences of continuity of the
upper rock in the vertical and horizontal directions. In the outer part of the
earth, the continuity in horizontal directions is interrupted by vertical
fissures. Were these not usually filled with water, they would soon kill the
horizontal component of the seismic wave, and the residual portion would
be directed almost vertically to the surface, for the width of the fissures is
almost always greater than the amplitude of the seismic vibrations. The
water restores the continuity, in a measure, but not perfectly, for the
elasticity of water is much less than that of rock. It is clear that in horizontal
movement there must be a constant transfer from rock to water and from
water to rock, and this must retard, as well as partially destroy, the
vibrations. In a vertical direction, however, the rocks rest firmly upon one
another, and this gives measurable continuity, the only change being from
one layer or kind of rock to another. It seems certain, therefore, that the
vertical component of the seismic wave will be less damped and less
retarded in transmission than the horizontal. It will, therefore, reach the
surface sooner and will have the greater effect on bodies at the surface, not
only for the reasons given, but also because it emerges more nearly in the
line of least resistance and of freest projection. On this account, a second
seismic tremors from a focus F, and, by lines normal to these, the changing directions of
propagation of the wave-front. It will be seen that the paths of propagation curve
upwards in approaching the surface. If the lines of emergence, as at E and E, be
projected backwards, as to F′, the points of crossing will be below the true focus.
A second correction must be made for the differences of continuity of the
upper rock in the vertical and horizontal directions. In the outer part of the
earth, the continuity in horizontal directions is interrupted by vertical
fissures. Were these not usually filled with water, they would soon kill the
horizontal component of the seismic wave, and the residual portion would
be directed almost vertically to the surface, for the width of the fissures is
almost always greater than the amplitude of the seismic vibrations. The
water restores the continuity, in a measure, but not perfectly, for the
elasticity of water is much less than that of rock. It is clear that in horizontal
movement there must be a constant transfer from rock to water and from
water to rock, and this must retard, as well as partially destroy, the
vibrations. In a vertical direction, however, the rocks rest firmly upon one
another, and this gives measurable continuity, the only change being from
one layer or kind of rock to another. It seems certain, therefore, that the
vertical component of the seismic wave will be less damped and less
retarded in transmission than the horizontal. It will, therefore, reach the
surface sooner and will have the greater effect on bodies at the surface, not
only for the reasons given, but also because it emerges more nearly in the
line of least resistance and of freest projection. On this account, a second
Page 617
correction must be added to the correction for elasticity, and this must
further reduce appreciably the first estimate of the depth of the focus.
Observation shows that in some way a seismic wave becomes separated
in transmission into portions of different natures and speeds, but their
interpretation is yet uncertain. These separated portions probably consist of
the compressional, the distortional, and the undulatory waves, and perhaps
of refractions and reflections of these (see Fig. 448).
A most important recent achievement is the detection and investigation of
seismic tremors that appear to have come through the earth. The
transmission of such waves promises to reveal much relative to the nature
of the deep interior, when enough data are gathered to warrant conclusions.
The rate of propagation in the central parts is found to be greater than in the
outer parts, implying high elasticity within.
The amplitude of the vibrations.—From the very disastrous effects of
severe earthquakes, it is natural to infer that the distinctive oscillations must
have large amplitude, but in fact it is the suddenness of the vibration, rather
than its length, that is effective. Instrumental investigations indicate that the
oscillations, after they have left their points of origin, are usually only a
fraction of a millimeter in amplitude; at most they seldom exceed a few
millimeters. A sudden shock with an amplitude of 5 or 6 millimeters is
sufficient to shatter a chimney. It is true that estimates assigning amplitudes
of a foot or more have been made, but their correctness is open to serious
doubt. It should be understood that it is the length of oscillation of the
particles of the subsurface rock transmitting the vibrations that is referred
to, not the movement of the free surface, or of objects on the surface. The
throw at and on the surface is much greater. Just as a slight, quick tap of a
hammer on a floor is sufficient to make a marble lying on it bound several
inches, so a sufficiently sudden rise of the surface of the earth, though but a
fraction of an inch, may project loose bodies many feet.
further reduce appreciably the first estimate of the depth of the focus.
Observation shows that in some way a seismic wave becomes separated
in transmission into portions of different natures and speeds, but their
interpretation is yet uncertain. These separated portions probably consist of
the compressional, the distortional, and the undulatory waves, and perhaps
of refractions and reflections of these (see Fig. 448).
A most important recent achievement is the detection and investigation of
seismic tremors that appear to have come through the earth. The
transmission of such waves promises to reveal much relative to the nature
of the deep interior, when enough data are gathered to warrant conclusions.
The rate of propagation in the central parts is found to be greater than in the
outer parts, implying high elasticity within.
The amplitude of the vibrations.—From the very disastrous effects of
severe earthquakes, it is natural to infer that the distinctive oscillations must
have large amplitude, but in fact it is the suddenness of the vibration, rather
than its length, that is effective. Instrumental investigations indicate that the
oscillations, after they have left their points of origin, are usually only a
fraction of a millimeter in amplitude; at most they seldom exceed a few
millimeters. A sudden shock with an amplitude of 5 or 6 millimeters is
sufficient to shatter a chimney. It is true that estimates assigning amplitudes
of a foot or more have been made, but their correctness is open to serious
doubt. It should be understood that it is the length of oscillation of the
particles of the subsurface rock transmitting the vibrations that is referred
to, not the movement of the free surface, or of objects on the surface. The
throw at and on the surface is much greater. Just as a slight, quick tap of a
hammer on a floor is sufficient to make a marble lying on it bound several
inches, so a sufficiently sudden rise of the surface of the earth, though but a
fraction of an inch, may project loose bodies many feet.
Page 618
Fig. 447.—Illustration of the destructive effects of the Charleston earthquake, showing
definite direction of throw. (W. J. McGee.)
Destructive effects.—The interpretation of the disastrous results of
earthquake shocks has, therefore, its key in the suddenness and strength of
rather minute vibrations of the earth-matter, but it is also dependent on the
freedom of motion of the bodies affected. The rocks of the deeper zones,
where the matter is sensibly continuous, transmit the seismic vibrations
without appreciable disruptive effect, so far as known, though the origin of
crevices has been assigned to this cause; but bodies at the surface are
fractured, overturned, and hurled from their places. The reason is doubtless
this: Within a great mass firmly held in place by cohesion and pressure on
all sides, the forward motion of a particle develops an equal elastic
resistance, and it is quickly thrown back again and the wave passes on. At
the surface, where bodies are freer to move, the stroke of the vibration
projects the body, and so, instead of vibratory resilience, the chief energy is
converted into mass-motion. The tap of a hammer sends an almost
imperceptible vibration along the floor, but this vibration may throw a glass
definite direction of throw. (W. J. McGee.)
Destructive effects.—The interpretation of the disastrous results of
earthquake shocks has, therefore, its key in the suddenness and strength of
rather minute vibrations of the earth-matter, but it is also dependent on the
freedom of motion of the bodies affected. The rocks of the deeper zones,
where the matter is sensibly continuous, transmit the seismic vibrations
without appreciable disruptive effect, so far as known, though the origin of
crevices has been assigned to this cause; but bodies at the surface are
fractured, overturned, and hurled from their places. The reason is doubtless
this: Within a great mass firmly held in place by cohesion and pressure on
all sides, the forward motion of a particle develops an equal elastic
resistance, and it is quickly thrown back again and the wave passes on. At
the surface, where bodies are freer to move, the stroke of the vibration
projects the body, and so, instead of vibratory resilience, the chief energy is
converted into mass-motion. The tap of a hammer sends an almost
imperceptible vibration along the floor, but this vibration may throw a glass
Page 619
ball, beneath which it runs, into the air. So the minute vibrations of earth-
matter may travel miles from their origin through continuous substance
with little result, and then so suddenly thrust a loose body on the surface, or
the base of a column, or the foundation of a house, as to rack it with
differential strains, or even to hurl it to destruction. So, too, earth-waves
striking the sea-border may thrust the waters off shore by their sudden
impact, and the reaction may develop a wave which overwhelms the coast.
Such waves may doubtless arise from a sudden stroke of seismic vibrations
on the sea-bottom. The great gaping fissures that sometimes open during
earthquakes occur oftenest where the surface on one side is less well
supported than on the other, as on a slope, or near a bluff-face or a river-
channel. When in such situations the earth is once suddenly forced in the
direction of least resistance, it is not always met by sufficient elastic
resistance to throw it back. Sometimes, however, there is an elastic return,
and the fissure closes forcibly an instant after it is opened.
Direction of throw.—Immediately above the point of origin, technically
the epicentrum or epi-focal point, bodies are projected upwards. When
crushing takes place in such a case, it is due to the upthrust or to the return
downfall. At one side of the epicentrum the thrust is oblique in various
degrees, and is usually more destructive, if not too far from the epicentrum.
The destructiveness commonly increases for a certain distance from the epi-
focal point, and then diminishes. Under ideal conditions, the greatest effects
are found where the vibration emerges at an angle of about 45°, but various
influences modify this result. Lines drawn through points of equal effect
(isoseismals) are not usually regular circles or ellipses about the
epicentrum, as they would be under ideal conditions. The various
divergencies represent differences of effective elasticity, of surface, and of
other influences. As most earthquakes originate from lines, planes, or
masses, rather than points, there are doubtless differences of intensity of
vibration at different points on the lines, planes, or areas of origin, and these
differences introduce inequalities in propagation and in surface effects.
matter may travel miles from their origin through continuous substance
with little result, and then so suddenly thrust a loose body on the surface, or
the base of a column, or the foundation of a house, as to rack it with
differential strains, or even to hurl it to destruction. So, too, earth-waves
striking the sea-border may thrust the waters off shore by their sudden
impact, and the reaction may develop a wave which overwhelms the coast.
Such waves may doubtless arise from a sudden stroke of seismic vibrations
on the sea-bottom. The great gaping fissures that sometimes open during
earthquakes occur oftenest where the surface on one side is less well
supported than on the other, as on a slope, or near a bluff-face or a river-
channel. When in such situations the earth is once suddenly forced in the
direction of least resistance, it is not always met by sufficient elastic
resistance to throw it back. Sometimes, however, there is an elastic return,
and the fissure closes forcibly an instant after it is opened.
Direction of throw.—Immediately above the point of origin, technically
the epicentrum or epi-focal point, bodies are projected upwards. When
crushing takes place in such a case, it is due to the upthrust or to the return
downfall. At one side of the epicentrum the thrust is oblique in various
degrees, and is usually more destructive, if not too far from the epicentrum.
The destructiveness commonly increases for a certain distance from the epi-
focal point, and then diminishes. Under ideal conditions, the greatest effects
are found where the vibration emerges at an angle of about 45°, but various
influences modify this result. Lines drawn through points of equal effect
(isoseismals) are not usually regular circles or ellipses about the
epicentrum, as they would be under ideal conditions. The various
divergencies represent differences of effective elasticity, of surface, and of
other influences. As most earthquakes originate from lines, planes, or
masses, rather than points, there are doubtless differences of intensity of
vibration at different points on the lines, planes, or areas of origin, and these
differences introduce inequalities in propagation and in surface effects.
Page 620
Fig. 448.—Illustrations of the records made by earthquake tremors after distant
transmission through the earth. The four diagrams represent the same set of tremors as
received at Shide, Kew, Bidston, and Edinburgh in Great Britain. The movement was
from left to right. (Milne.)
Rate of propagation.—The progress of a seismic wave varies very
greatly. Both experimental tests and natural observations give very
discordant results. At present, they justify only the broad statement that the
velocity of propagation varies from several hundreds to several thousands
of feet per second at the surface. The rate seems to be greater for strong
vibrations than for weak ones, and hence it is faster near the origin than
farther away. The strength of a vibration dies away, theoretically, according
to the inverse square of the distance from the point of origin. Practically
there is to be added to this the partial destruction of the vibrations by
conversion into other forms of motion.
Sequences of vibrations.—Near the source, the main shocks are apt to
come suddenly and to be followed by minor tremors. At a distance there are
usually “preliminary” vibrations followed by the main tremors, and these by
others of gradually diminishing value. This development is assigned to
different rates of propagation, and to refractions and reflections not unlike
the prolongation of thunder (see Fig. 448). This deployment of the
vibrations is notably developed in the shocks that pass long distances
transmission through the earth. The four diagrams represent the same set of tremors as
received at Shide, Kew, Bidston, and Edinburgh in Great Britain. The movement was
from left to right. (Milne.)
Rate of propagation.—The progress of a seismic wave varies very
greatly. Both experimental tests and natural observations give very
discordant results. At present, they justify only the broad statement that the
velocity of propagation varies from several hundreds to several thousands
of feet per second at the surface. The rate seems to be greater for strong
vibrations than for weak ones, and hence it is faster near the origin than
farther away. The strength of a vibration dies away, theoretically, according
to the inverse square of the distance from the point of origin. Practically
there is to be added to this the partial destruction of the vibrations by
conversion into other forms of motion.
Sequences of vibrations.—Near the source, the main shocks are apt to
come suddenly and to be followed by minor tremors. At a distance there are
usually “preliminary” vibrations followed by the main tremors, and these by
others of gradually diminishing value. This development is assigned to
different rates of propagation, and to refractions and reflections not unlike
the prolongation of thunder (see Fig. 448). This deployment of the
vibrations is notably developed in the shocks that pass long distances
Page 621
through the earth. The vibrations of the first phase are regarded as
compressional, those of the second as distortional, while the largest
oscillations which arise still later perhaps come around the surface, and may
be undulatory, though their nature is not yet determined.
There is often, however, a true succession of original shocks caused by a
succession of slips or ruptures at the source. Sometimes these are
exceedingly persistent, running through days, weeks, or even months. In
such cases a slow faulting is probably in progress, and little slips and stops
follow in close succession. In one instance as many as 600 shocks in ten
days have been reported.[226]
Gaseous emanations.—Vapors and gas frequently issue from earthquake
rents, and are popularly made to serve as causes, but they are usually
merely the earth gases that are permitted to escape by the rending of the
ground, or are forced out by readjustment of the shaken beds. Like other
subterranean gases, they are often sulphurous, and they are sometimes hot,
especially in volcanic regions. Where the shocks are connected with
eruptions, the gases may be truly volcanic.
Distribution of earthquakes.—Over large portions of the globe, severe
earthquakes are exceedingly rare, but in certain regions they are
unfortunately frequent. For the most part, these are volcanic districts, but
this is by no means a universal relation. Earthquakes and volcanoes are only
in part associates. In general, it may be said that earthquakes are frequent
where geologic changes are in rapid progress, as along belts of young
mountains, where the stresses are not yet adjusted, or at the mouths of great
streams, where deltas are accumulating, or about volcanoes, where
temperatures and strains are changing, or on the great slopes, particularly
the submarine slopes, where readjustments in response to inequalities of
surface stress are in progress. Not a few, however, occur where the special
occasion is not at all obvious.
The Geologic Effects of Earthquakes.
Earthquakes are of much less importance, geologically, than many
gentler movements and activities. Disastrous as they sometimes are to
human affairs, they leave few distinct and readily identifiable marks which
are more than temporary.
compressional, those of the second as distortional, while the largest
oscillations which arise still later perhaps come around the surface, and may
be undulatory, though their nature is not yet determined.
There is often, however, a true succession of original shocks caused by a
succession of slips or ruptures at the source. Sometimes these are
exceedingly persistent, running through days, weeks, or even months. In
such cases a slow faulting is probably in progress, and little slips and stops
follow in close succession. In one instance as many as 600 shocks in ten
days have been reported.[226]
Gaseous emanations.—Vapors and gas frequently issue from earthquake
rents, and are popularly made to serve as causes, but they are usually
merely the earth gases that are permitted to escape by the rending of the
ground, or are forced out by readjustment of the shaken beds. Like other
subterranean gases, they are often sulphurous, and they are sometimes hot,
especially in volcanic regions. Where the shocks are connected with
eruptions, the gases may be truly volcanic.
Distribution of earthquakes.—Over large portions of the globe, severe
earthquakes are exceedingly rare, but in certain regions they are
unfortunately frequent. For the most part, these are volcanic districts, but
this is by no means a universal relation. Earthquakes and volcanoes are only
in part associates. In general, it may be said that earthquakes are frequent
where geologic changes are in rapid progress, as along belts of young
mountains, where the stresses are not yet adjusted, or at the mouths of great
streams, where deltas are accumulating, or about volcanoes, where
temperatures and strains are changing, or on the great slopes, particularly
the submarine slopes, where readjustments in response to inequalities of
surface stress are in progress. Not a few, however, occur where the special
occasion is not at all obvious.
The Geologic Effects of Earthquakes.
Earthquakes are of much less importance, geologically, than many
gentler movements and activities. Disastrous as they sometimes are to
human affairs, they leave few distinct and readily identifiable marks which
are more than temporary.
Page 622
Fracturing of rock.—During the passage of notable earthquake waves,
the solid rock is probably often fractured (see p. 509), though where it is
covered by deep soil the fractures are rarely observable at the surface.
Elsewhere the crevices are readily seen, especially if they gape. In a few
instances surface-rock has been seen to be thoroughly shattered after the
passage of an earthquake, as in the Concepcion earthquake of 1835.[227]
Joints which were before closed are often opened during an earthquake.
Thus in northern Arizona, not far from Canyon Diablo, there is a crevice
traceable for a considerable distance, which is said to have been opened
during an earthquake. Locally, it gaps several feet. Other notable earthquake
fissures have been recorded in India,[228] Japan, and New Zealand. During an
earthquake which shook the South Island of New Zealand in 1848, “a
fissure was formed averaging 18 inches in width, and traceable for a
distance of 60 miles, parallel to the axis of the adjacent mountain chain.”[229]
The development of fractures or the opening of joints is sometimes
accompanied by faulting. This was the case in Japan during the earthquake
of October 28, 1891, when the surface on one side of a fissure, which could
be traced for 40 miles, sank 2 to 20 feet. In this case there was also notable
horizontal displacement, the east wall of the fissure being thrust locally as
much as 13 feet to the north.[230]
Changes of surface.—Circular surface openings or basins are sometimes
developed during earthquakes. This was the case during the Charleston
earthquake of 1886,[231] and similar effects have been noted elsewhere.
These openings often serve as avenues of escape for ground-water, gases,
and vapor. They are commonly supposed to be the result of the collapse of
caverns, or other subterranean openings, the collapse often causing the
forcible ejection of water. Such openings are likely to be formed only where
the surface material is incoherent. Sandstone dikes (p. 514) may perhaps be
associated in origin with earthquakes.
Earthquakes are likely to dislodge masses of rock in unstable positions,
as on slopes or cliffs. They may also occasion slumps and landslides.[232]
Effects on drainage.—The fracturing of the rock may interfere with the
movement of ground-water. After new cracks are developed, or old ones
opened or closed, the movement of ground-water adapts itself to the new
conditions. It follows that springs sometimes cease to flow after an
earthquake, while new ones break out where there had been none before.
the solid rock is probably often fractured (see p. 509), though where it is
covered by deep soil the fractures are rarely observable at the surface.
Elsewhere the crevices are readily seen, especially if they gape. In a few
instances surface-rock has been seen to be thoroughly shattered after the
passage of an earthquake, as in the Concepcion earthquake of 1835.[227]
Joints which were before closed are often opened during an earthquake.
Thus in northern Arizona, not far from Canyon Diablo, there is a crevice
traceable for a considerable distance, which is said to have been opened
during an earthquake. Locally, it gaps several feet. Other notable earthquake
fissures have been recorded in India,[228] Japan, and New Zealand. During an
earthquake which shook the South Island of New Zealand in 1848, “a
fissure was formed averaging 18 inches in width, and traceable for a
distance of 60 miles, parallel to the axis of the adjacent mountain chain.”[229]
The development of fractures or the opening of joints is sometimes
accompanied by faulting. This was the case in Japan during the earthquake
of October 28, 1891, when the surface on one side of a fissure, which could
be traced for 40 miles, sank 2 to 20 feet. In this case there was also notable
horizontal displacement, the east wall of the fissure being thrust locally as
much as 13 feet to the north.[230]
Changes of surface.—Circular surface openings or basins are sometimes
developed during earthquakes. This was the case during the Charleston
earthquake of 1886,[231] and similar effects have been noted elsewhere.
These openings often serve as avenues of escape for ground-water, gases,
and vapor. They are commonly supposed to be the result of the collapse of
caverns, or other subterranean openings, the collapse often causing the
forcible ejection of water. Such openings are likely to be formed only where
the surface material is incoherent. Sandstone dikes (p. 514) may perhaps be
associated in origin with earthquakes.
Earthquakes are likely to dislodge masses of rock in unstable positions,
as on slopes or cliffs. They may also occasion slumps and landslides.[232]
Effects on drainage.—The fracturing of the rock may interfere with the
movement of ground-water. After new cracks are developed, or old ones
opened or closed, the movement of ground-water adapts itself to the new
conditions. It follows that springs sometimes cease to flow after an
earthquake, while new ones break out where there had been none before.
Page 623
The character of the water of springs is sometimes changed, presumably
because it comes from different sources after the earthquake. Joints may be
so widened as to intercept rivulets, and the waters thus intercepted may
cause the further enlargement of the opening. Illustrations of this sort are
furnished by the earthquakes of the Mississippi valley (Lat. 36° to 38°) in
1811–12. Where faults accompany earthquakes, they occasion ponds or
falls where they cross streams. Illustrations of both were furnished by the
Chedrang River of India after the earthquake of 1897.[233]
Effects on standing water.—Some of the most destructive effects of
earthquakes are felt along the borders of the sea. Thus the great sea-wave of
the Lisbon earthquake (1755) and that of the earthquake which affected the
coasts of Ecuador and Peru in 1868 are examples. Such waves have been
known to advance on the land as walls of water 60 feet in height. They are
most destructive along low coasts, for here the water may sweep much
more extensively over the land. The great loss of life during an earthquake
has usually been the direct result of the great waves. Lakes are also affected
by earthquakes, their waters sometimes rising and falling for several hours
after the initial disturbance, but lake-waves are much feebler than those of
the sea, and are not often destructive.
Earthquake shocks are sometimes remarkably destructive to the life of
lakes and seas. Thus during the Indian earthquake of 1897, “fishes were
killed in myriads as by the explosion of a dynamite cartridge ... and for days
after the earthquake, the river (Sumesari) was choked with thousands of
dead fish ... and two floating carcasses of Gangetic dolphins were seen
which had been killed by the shock.”[234] This wholesale destruction of life
is of interest, since the surfaces of layers of rock, often of great age, are
sometimes covered with fossils of fish or other animal forms, so numerous
and so preserved as to indicate that the animals were killed suddenly and in
great numbers, and their bodies quickly buried. It has been suggested that
such rock surfaces may be memorials of ancient earthquake shocks.[235]
Changes of level.—Permanent changes of level sometimes accompany
an earthquake. Thus after the earthquake of 1822 “the coast of Chili for a
long distance was said to have risen 3 or 4 feet.”[236] Similar results have
occurred on the same coast at other times, and on other coasts at various
times. Depression of the surface is perhaps even more common than
elevation. Thus on the coast of India all except the higher parts of an area
because it comes from different sources after the earthquake. Joints may be
so widened as to intercept rivulets, and the waters thus intercepted may
cause the further enlargement of the opening. Illustrations of this sort are
furnished by the earthquakes of the Mississippi valley (Lat. 36° to 38°) in
1811–12. Where faults accompany earthquakes, they occasion ponds or
falls where they cross streams. Illustrations of both were furnished by the
Chedrang River of India after the earthquake of 1897.[233]
Effects on standing water.—Some of the most destructive effects of
earthquakes are felt along the borders of the sea. Thus the great sea-wave of
the Lisbon earthquake (1755) and that of the earthquake which affected the
coasts of Ecuador and Peru in 1868 are examples. Such waves have been
known to advance on the land as walls of water 60 feet in height. They are
most destructive along low coasts, for here the water may sweep much
more extensively over the land. The great loss of life during an earthquake
has usually been the direct result of the great waves. Lakes are also affected
by earthquakes, their waters sometimes rising and falling for several hours
after the initial disturbance, but lake-waves are much feebler than those of
the sea, and are not often destructive.
Earthquake shocks are sometimes remarkably destructive to the life of
lakes and seas. Thus during the Indian earthquake of 1897, “fishes were
killed in myriads as by the explosion of a dynamite cartridge ... and for days
after the earthquake, the river (Sumesari) was choked with thousands of
dead fish ... and two floating carcasses of Gangetic dolphins were seen
which had been killed by the shock.”[234] This wholesale destruction of life
is of interest, since the surfaces of layers of rock, often of great age, are
sometimes covered with fossils of fish or other animal forms, so numerous
and so preserved as to indicate that the animals were killed suddenly and in
great numbers, and their bodies quickly buried. It has been suggested that
such rock surfaces may be memorials of ancient earthquake shocks.[235]
Changes of level.—Permanent changes of level sometimes accompany
an earthquake. Thus after the earthquake of 1822 “the coast of Chili for a
long distance was said to have risen 3 or 4 feet.”[236] Similar results have
occurred on the same coast at other times, and on other coasts at various
times. Depression of the surface is perhaps even more common than
elevation. Thus on the coast of India all except the higher parts of an area
Page 624
60 square miles in extent were sunk below the sea during an earthquake in
1762. Widespread depression in the vicinity of the Mississippi in Missouri,
Arkansas, Kentucky, and Tennessee accompanied the earthquakes of 1811
and 1812. Some of the depressed areas were converted into marshes, while
others became the sites of permanent lakes. Reelfoot Lake, mainly in
Tennessee, is an example. Change of level is involved wherever there is
faulting, and faulting is probably rather common in connection with
earthquakes.
Changes of level are not confined to the land. Where earthquake
disturbances affect the sea-bottom in regions of telegraph cables, the cables
are often broken. In such cases notable changes have sometimes been
discovered and recorded when the cables were repaired. Striking examples
are furnished by the region about Greece.[237] In one instance (1873) the
repairing vessel found about 2000 feet of water where about 1400 feet
existed when the cable was laid. In another instance (1878) the bottom was
“so irregular and uneven for a distance of about two miles, that a detour was
made and the cable lengthened by five or six miles.” In still another case
(1885) the repairing vessel found a “difference of 1500 feet between the
bow and stern soundings.” These records point to sea-bottom faulting on a
large scale.
It is probably no nearer the truth to say that changes of level result from
earthquakes than to say that earthquakes result from changes of level. The
two classes of phenomena are probably to be referred to a common cause.
[238]
SLOW MASSIVE MOVEMENTS.
It is a far cry from the intense and inconceivably rapid oscillations of the
earthquake, to the excessively slow subsidences of continents, or even the
slow wrinkling of mountain folds. Not infrequently rivers wear down their
channels across a mountain range as fast as it rises athwart them. The
movements of continents are even more deliberate. But, far apart as these
contrasted movements are, in rate and method, they are associated in
ultimate causation, and the earthquake shock is often merely an incident in
the formation of a mountain range or in the subsidence of a continent.
1762. Widespread depression in the vicinity of the Mississippi in Missouri,
Arkansas, Kentucky, and Tennessee accompanied the earthquakes of 1811
and 1812. Some of the depressed areas were converted into marshes, while
others became the sites of permanent lakes. Reelfoot Lake, mainly in
Tennessee, is an example. Change of level is involved wherever there is
faulting, and faulting is probably rather common in connection with
earthquakes.
Changes of level are not confined to the land. Where earthquake
disturbances affect the sea-bottom in regions of telegraph cables, the cables
are often broken. In such cases notable changes have sometimes been
discovered and recorded when the cables were repaired. Striking examples
are furnished by the region about Greece.[237] In one instance (1873) the
repairing vessel found about 2000 feet of water where about 1400 feet
existed when the cable was laid. In another instance (1878) the bottom was
“so irregular and uneven for a distance of about two miles, that a detour was
made and the cable lengthened by five or six miles.” In still another case
(1885) the repairing vessel found a “difference of 1500 feet between the
bow and stern soundings.” These records point to sea-bottom faulting on a
large scale.
It is probably no nearer the truth to say that changes of level result from
earthquakes than to say that earthquakes result from changes of level. The
two classes of phenomena are probably to be referred to a common cause.
[238]
SLOW MASSIVE MOVEMENTS.
It is a far cry from the intense and inconceivably rapid oscillations of the
earthquake, to the excessively slow subsidences of continents, or even the
slow wrinkling of mountain folds. Not infrequently rivers wear down their
channels across a mountain range as fast as it rises athwart them. The
movements of continents are even more deliberate. But, far apart as these
contrasted movements are, in rate and method, they are associated in
ultimate causation, and the earthquake shock is often merely an incident in
the formation of a mountain range or in the subsidence of a continent.
Page 625
The great movements are usually classed (1) as continent-making
(epeirogenic) and (2) mountain-making (orogenic). They may also be
classed as (1) vertical movements and (2) horizontal movements, and
dynamically, as (1) thrust movements and (2) stretching movements. It is to
be understood that these distinctions are little more than analytical
conveniences, for continental movements are often at the same time
mountain-making movements; vertical movements are usually involved in
horizontal movements, and stretching usually takes part in the processes in
which thrust predominates, and vice versa. But where one phase greatly
preponderates, it may conveniently give name to the whole.
Present movements.—Critical observations on seacoasts show that some
shores are slowly rising and some slowly sinking relative to the ocean-level.
We do not certainly know what their movements are relative to the center of
the earth; very possibly all may be sinking, one set faster than the other, the
ocean-surface also going down at an intermediate rate. Theoretically, all
might possibly be rising, one set faster than the other, the ocean also rising
at an intermediate rate, though this is extremely improbable. One set may
be actually rising relative to the center of the earth, and the other sinking,
while the ocean-level is stationary, or nearly so. This is the way in which we
are accustomed to interpret them. A general shrinkage of the earth, however,
is probably going on, carrying down land-surface and sea-surface. It has
been urged by Suess[239] that the general shrinkage is so great that the local
upward warpings and foldings never equal it, and that the real movements
are all downward, though in different degrees. This is probably the general
fact at least. Over against this is the popular disposition to regard earth
movements generally as “upheavals.” There is also a predilection for
regarding the rigid land as moving and the mobile sea-level as fixed. In
reality, the sea is an extremely adaptive body that settles into the irregular
hollows of the lithosphere, and is shifted about with every warping of the
latter. Whatever change affects the capacity of its depressions affects also
the sea-level. If they are increased, the sea settles more deeply into them; if
they are decreased, the sea spreads out more widely on the borders of the
land. The one thing that gives a measure of stability to the sea-level is the
fact that all the great basins are connected, and so an average is maintained.
A warping down in one part of the sea-bottom may be offset by an upward
warping somewhere else in the 72% of the earth’s surface covered by the
ocean, and so it is only the sum total of all changes in the sea-bottoms and
(epeirogenic) and (2) mountain-making (orogenic). They may also be
classed as (1) vertical movements and (2) horizontal movements, and
dynamically, as (1) thrust movements and (2) stretching movements. It is to
be understood that these distinctions are little more than analytical
conveniences, for continental movements are often at the same time
mountain-making movements; vertical movements are usually involved in
horizontal movements, and stretching usually takes part in the processes in
which thrust predominates, and vice versa. But where one phase greatly
preponderates, it may conveniently give name to the whole.
Present movements.—Critical observations on seacoasts show that some
shores are slowly rising and some slowly sinking relative to the ocean-level.
We do not certainly know what their movements are relative to the center of
the earth; very possibly all may be sinking, one set faster than the other, the
ocean-surface also going down at an intermediate rate. Theoretically, all
might possibly be rising, one set faster than the other, the ocean also rising
at an intermediate rate, though this is extremely improbable. One set may
be actually rising relative to the center of the earth, and the other sinking,
while the ocean-level is stationary, or nearly so. This is the way in which we
are accustomed to interpret them. A general shrinkage of the earth, however,
is probably going on, carrying down land-surface and sea-surface. It has
been urged by Suess[239] that the general shrinkage is so great that the local
upward warpings and foldings never equal it, and that the real movements
are all downward, though in different degrees. This is probably the general
fact at least. Over against this is the popular disposition to regard earth
movements generally as “upheavals.” There is also a predilection for
regarding the rigid land as moving and the mobile sea-level as fixed. In
reality, the sea is an extremely adaptive body that settles into the irregular
hollows of the lithosphere, and is shifted about with every warping of the
latter. Whatever change affects the capacity of its depressions affects also
the sea-level. If they are increased, the sea settles more deeply into them; if
they are decreased, the sea spreads out more widely on the borders of the
land. The one thing that gives a measure of stability to the sea-level is the
fact that all the great basins are connected, and so an average is maintained.
A warping down in one part of the sea-bottom may be offset by an upward
warping somewhere else in the 72% of the earth’s surface covered by the
ocean, and so it is only the sum total of all changes in the sea-bottoms and
Page 626
borders that effects the common level. Thus it happens that,
notwithstanding its instability and its complete subordination to the
lithosphere, the sea-level is the most convenient basis of reference, and has
become the accepted datum-plane. If there were some available mode of
measuring the distance of points from the center of the earth, it would give
absolute data and absolute terms, and would reveal much that is now
uncertain respecting the real movements of the surface. For convenience,
however, since absolute terms are impracticable, the ordinary language of
geology, which represents movements as upward and downward, according
to their relations to the sea-level or to the average surface, will be
employed. Notwithstanding this concession to convenience in the use of
terms, it is of the greatest importance to form, and to constantly retain, true
fundamental views.
Fundamental conceptions.—The existence of any land at all is
dependent on the inequalities of the surface and of the density of the
lithosphere, for if it were perfectly spheroidal and equidense, the
hydrosphere would cover it completely to a depth of about two miles. Not
only are inequalities necessary to the existence of land, but these
inequalities must be renewed from time to time, or the land area would soon,
geologically speaking, be covered by the sea. The renewal has been made
again and again in geological history by movements that have increased the
inequalities in the surface of the lithosphere. With each such movement,
apparently, the oceans have withdrawn more completely within the basins,
and the continents have stood forth more broadly and relatively higher, until
again worn down. This renewal of inequalities appears to have been, in its
great features, a periodic movement, recurring at long intervals. In the
intervening times, the sea has crept out over the lower parts of the
continents, moving on steadily and slowly toward their complete
submersion, which would inevitably have been attained if no interruption
had checked and reversed the process. These are the great movements of the
earth, and in them lies, we believe, the soul of geologic history and the basis
for its grand divisions. The reasons for this will appear as the history is
followed, and its most potential agencies are seen unfolding themselves. At
the same time, there have been numerous minor surface movements in
almost constant progress. While these two classes of movements have been
associated, and are perhaps due in the main to the same causes, they are
notwithstanding its instability and its complete subordination to the
lithosphere, the sea-level is the most convenient basis of reference, and has
become the accepted datum-plane. If there were some available mode of
measuring the distance of points from the center of the earth, it would give
absolute data and absolute terms, and would reveal much that is now
uncertain respecting the real movements of the surface. For convenience,
however, since absolute terms are impracticable, the ordinary language of
geology, which represents movements as upward and downward, according
to their relations to the sea-level or to the average surface, will be
employed. Notwithstanding this concession to convenience in the use of
terms, it is of the greatest importance to form, and to constantly retain, true
fundamental views.
Fundamental conceptions.—The existence of any land at all is
dependent on the inequalities of the surface and of the density of the
lithosphere, for if it were perfectly spheroidal and equidense, the
hydrosphere would cover it completely to a depth of about two miles. Not
only are inequalities necessary to the existence of land, but these
inequalities must be renewed from time to time, or the land area would soon,
geologically speaking, be covered by the sea. The renewal has been made
again and again in geological history by movements that have increased the
inequalities in the surface of the lithosphere. With each such movement,
apparently, the oceans have withdrawn more completely within the basins,
and the continents have stood forth more broadly and relatively higher, until
again worn down. This renewal of inequalities appears to have been, in its
great features, a periodic movement, recurring at long intervals. In the
intervening times, the sea has crept out over the lower parts of the
continents, moving on steadily and slowly toward their complete
submersion, which would inevitably have been attained if no interruption
had checked and reversed the process. These are the great movements of the
earth, and in them lies, we believe, the soul of geologic history and the basis
for its grand divisions. The reasons for this will appear as the history is
followed, and its most potential agencies are seen unfolding themselves. At
the same time, there have been numerous minor surface movements in
almost constant progress. While these two classes of movements have been
associated, and are perhaps due in the main to the same causes, they are
Page 627
sufficiently different in some of their dynamic aspects to be separated in
treatment.
Nearly Constant Small Movements.
Innumerable gentle warpings have affected nearly every portion of the
surface of the globe at nearly all stages of its history. Not only during the
periods of great movements were there countless minor and gentler
movements, but at times of relative quiescence there were slow swellings
and saggings of the surface of the lithosphere. They sometimes affected
small areas and sometimes large ones, and they were sometimes of upward
phase and sometimes of downward. They were the immediate agencies in
locating and controlling the deposition of stratified rocks, though they rest
back on the great movements for their working conditions. Very slow
sinkings of sea-borders have permitted deposition to go on in shallow water
for long periods without being interrupted by the local filling of the sea.
Very slow swellings of land tracts, relative or absolute, have permitted
erosion to supply material for such sedimentation for long periods without
exhausting the sources. Very slow upward warpings in one region and
downward warpings in another have shifted the borders of the land and sea,
and with them the areas of erosion and deposition. Thus have arisen
overlaps and unconformities of strata and diversities in their distribution
from stage to stage. Such movements may have amounted to a few inches,
or a few feet, or a few fathoms per century. Downward movements have
sometimes affected a considerable section of a continent, letting in a
shallow epicontinental sea upon it, such, for example, as the North Sea
upon the northwestern border of the continent of Europe, and Hudson Bay
upon the northeastern part of North America. Similar movements seem to
have extended the seas even more widely upon the surface of the land in
times past, as attested by the great transgressions of the ocean-borders and
the great epicontinental spread of strata. Notwithstanding their great
breadths, the epicontinental seas were generally shallow. Similar gentle
warpings of upward phase rescued the bottoms of shallow seas from
submersion, and inaugurated erosion; or they bowed base-leveled lands
upward, and rejuvenated their streams and inaugurated a new cycle of
denudation. Often they connected continents previously separated by
treatment.
Nearly Constant Small Movements.
Innumerable gentle warpings have affected nearly every portion of the
surface of the globe at nearly all stages of its history. Not only during the
periods of great movements were there countless minor and gentler
movements, but at times of relative quiescence there were slow swellings
and saggings of the surface of the lithosphere. They sometimes affected
small areas and sometimes large ones, and they were sometimes of upward
phase and sometimes of downward. They were the immediate agencies in
locating and controlling the deposition of stratified rocks, though they rest
back on the great movements for their working conditions. Very slow
sinkings of sea-borders have permitted deposition to go on in shallow water
for long periods without being interrupted by the local filling of the sea.
Very slow swellings of land tracts, relative or absolute, have permitted
erosion to supply material for such sedimentation for long periods without
exhausting the sources. Very slow upward warpings in one region and
downward warpings in another have shifted the borders of the land and sea,
and with them the areas of erosion and deposition. Thus have arisen
overlaps and unconformities of strata and diversities in their distribution
from stage to stage. Such movements may have amounted to a few inches,
or a few feet, or a few fathoms per century. Downward movements have
sometimes affected a considerable section of a continent, letting in a
shallow epicontinental sea upon it, such, for example, as the North Sea
upon the northwestern border of the continent of Europe, and Hudson Bay
upon the northeastern part of North America. Similar movements seem to
have extended the seas even more widely upon the surface of the land in
times past, as attested by the great transgressions of the ocean-borders and
the great epicontinental spread of strata. Notwithstanding their great
breadths, the epicontinental seas were generally shallow. Similar gentle
warpings of upward phase rescued the bottoms of shallow seas from
submersion, and inaugurated erosion; or they bowed base-leveled lands
upward, and rejuvenated their streams and inaugurated a new cycle of
denudation. Often they connected continents previously separated by
Page 628
shallow straits, and thus inaugurated inter-continental migrations of land
life, while they stopped inter-oceanic migration.
The gentleness and frequency of these movements is attested by the
character of the sediments and by their relations to one another, as will be
seen in the study of the sedimentary series.
Reciprocal features.—These minor warpings show a notable tendency
to be reciprocal. If one area is bowed up, another near by is bowed down. If
the continents settle, the oceans rise on their borders. If the land is cut
down, the sea is filled up. There is an important phase of this deserving
especial note. Certain tracts have been slowly bowed upwards into long
land swells, the streams being rejuvenated and degradation hastened.
Adjacent tracts have been slowly bowed downwards into long parallel
troughs which received the wash from the adjacent swells, and thus became
tracts of exceptional sedimentation. Such a tract of parallel swell and sag, if
our interpretation be correct, developed along the Atlantic border of North
America in the Paleozoic era. By the slow upward warping of the swells,
the feeding-grounds of the streams were maintained, and the sags were
filled about as fast as they sank. Thus a great depth of sediment was laid
down in the course of an era measured by millions of years. So in other
regions, especially near the borders of the continents, there have been
similar reciprocal movements, giving at once feeding-grounds for the
streams and lodgment-grounds for the sediments, side by side in parallel
belts. It is a common view that these belts of deep sedimentation were the
forerunners of mountain formation, and that they determined the formation
of the mountains. In view of the grounds for doubting the efficiency of so
superficial an agency in mountain formation, which will appear as we go
on, it may be well to hold this view in abeyance, and to dwell on the
reciprocal nature of the action, in which the upward bowing that gave the
feeding-grounds is as vital a factor as the sagging that accommodated the
sedimentation. It is important to recognize that in so far as the crust was
weak enough to yield to these gentler forces, it was not strong enough to
accumulate the great stresses necessary to form mountain ranges, and
further, that in so far as the stresses were eased by the gentle warping, they
could not be accumulated for the later work of mountain-folding. It is
nevertheless probable that the conditions which located the gentle swelling
and sagging also located the mountain-folding.
life, while they stopped inter-oceanic migration.
The gentleness and frequency of these movements is attested by the
character of the sediments and by their relations to one another, as will be
seen in the study of the sedimentary series.
Reciprocal features.—These minor warpings show a notable tendency
to be reciprocal. If one area is bowed up, another near by is bowed down. If
the continents settle, the oceans rise on their borders. If the land is cut
down, the sea is filled up. There is an important phase of this deserving
especial note. Certain tracts have been slowly bowed upwards into long
land swells, the streams being rejuvenated and degradation hastened.
Adjacent tracts have been slowly bowed downwards into long parallel
troughs which received the wash from the adjacent swells, and thus became
tracts of exceptional sedimentation. Such a tract of parallel swell and sag, if
our interpretation be correct, developed along the Atlantic border of North
America in the Paleozoic era. By the slow upward warping of the swells,
the feeding-grounds of the streams were maintained, and the sags were
filled about as fast as they sank. Thus a great depth of sediment was laid
down in the course of an era measured by millions of years. So in other
regions, especially near the borders of the continents, there have been
similar reciprocal movements, giving at once feeding-grounds for the
streams and lodgment-grounds for the sediments, side by side in parallel
belts. It is a common view that these belts of deep sedimentation were the
forerunners of mountain formation, and that they determined the formation
of the mountains. In view of the grounds for doubting the efficiency of so
superficial an agency in mountain formation, which will appear as we go
on, it may be well to hold this view in abeyance, and to dwell on the
reciprocal nature of the action, in which the upward bowing that gave the
feeding-grounds is as vital a factor as the sagging that accommodated the
sedimentation. It is important to recognize that in so far as the crust was
weak enough to yield to these gentler forces, it was not strong enough to
accumulate the great stresses necessary to form mountain ranges, and
further, that in so far as the stresses were eased by the gentle warping, they
could not be accumulated for the later work of mountain-folding. It is
nevertheless probable that the conditions which located the gentle swelling
and sagging also located the mountain-folding.
Page 629
The Great Periodic Movements.
Mountain-forming movements.—Along certain tracts, usually near the
borders of the continents, and at certain times, usually separated by long
intervals, the crust was folded into gigantic wrinkles, and these constitute
the chief type of mountains, though not the only type. The characteristic
force in this folding was lateral thrust. The strata were not only arched, but
often closely folded, and sometimes intensely crumpled. In extreme cases,
like the Alps, the folds flared out above, giving overturn dips and reversed
strata, as illustrated in the chapter on Structural Geology, pp. 501–511. In
these cases there was an upward as well as a horizontal movement, for the
folds themselves were lifted; but the horizontal thrust so much
preponderated, and was so much the more remarkable, that the upward
movement was overshadowed. It is well to note, however, that these
mountain ranges are crumpled outward and not inward, as might be
expected if they resulted simply from the shrinkage of the under side of a
thin shell. The folds are sometimes nearly upright and symmetrical, and
sometimes inclined and asymmetrical, as illustrated in the chapter referred
to. Where the folds lean, the inference has been drawn that the active thrust
came from the side of the gentler slope, the folds being pushed over toward
the resisting side, and this seems to be commonly true. The original attitude
of the beds, however, has much to do with the character of the folds.[240] By
a slight change in the mode of thrust, sheets of paper may be so pushed as
to lean forward or backward at pleasure. The leaning of the folds seems,
therefore, a doubtful criterion for determining the direction of the active
movement. Mountains of the thrust type usually consist of a series of folds
nearly parallel to each other, the whole forming an anticlinorium.
Mountain-forming movements.—Along certain tracts, usually near the
borders of the continents, and at certain times, usually separated by long
intervals, the crust was folded into gigantic wrinkles, and these constitute
the chief type of mountains, though not the only type. The characteristic
force in this folding was lateral thrust. The strata were not only arched, but
often closely folded, and sometimes intensely crumpled. In extreme cases,
like the Alps, the folds flared out above, giving overturn dips and reversed
strata, as illustrated in the chapter on Structural Geology, pp. 501–511. In
these cases there was an upward as well as a horizontal movement, for the
folds themselves were lifted; but the horizontal thrust so much
preponderated, and was so much the more remarkable, that the upward
movement was overshadowed. It is well to note, however, that these
mountain ranges are crumpled outward and not inward, as might be
expected if they resulted simply from the shrinkage of the under side of a
thin shell. The folds are sometimes nearly upright and symmetrical, and
sometimes inclined and asymmetrical, as illustrated in the chapter referred
to. Where the folds lean, the inference has been drawn that the active thrust
came from the side of the gentler slope, the folds being pushed over toward
the resisting side, and this seems to be commonly true. The original attitude
of the beds, however, has much to do with the character of the folds.[240] By
a slight change in the mode of thrust, sheets of paper may be so pushed as
to lean forward or backward at pleasure. The leaning of the folds seems,
therefore, a doubtful criterion for determining the direction of the active
movement. Mountains of the thrust type usually consist of a series of folds
nearly parallel to each other, the whole forming an anticlinorium.
Page 630
Fig. 449.—The great Eurasian mountain tract. Jones Relief Globe. (Photo. by R. T.
Chamberlin.)
Distribution of folded ranges.—The prevailing location of this class of
mountains is so generally near the borders of the continents that the relation
is probably significant. Dana[241] long ago called attention to the fact that the
greatest mountain ranges stand opposite the greatest ocean-basins, and he
connected the elevation of the one with the depression of the other. One of
the most notable exceptions to this relation is the complex system of
southern Europe, from the Pyrenees to the Caucasus, and another is the
Altai and connected ranges (Fig. 449). The Urals and not a few minor
ranges are also exceptions. It is probably better to regard the crumpled
tracts as lying on the borders of great segments of the earth that acted
Chamberlin.)
Distribution of folded ranges.—The prevailing location of this class of
mountains is so generally near the borders of the continents that the relation
is probably significant. Dana[241] long ago called attention to the fact that the
greatest mountain ranges stand opposite the greatest ocean-basins, and he
connected the elevation of the one with the depression of the other. One of
the most notable exceptions to this relation is the complex system of
southern Europe, from the Pyrenees to the Caucasus, and another is the
Altai and connected ranges (Fig. 449). The Urals and not a few minor
ranges are also exceptions. It is probably better to regard the crumpled
tracts as lying on the borders of great segments of the earth that acted
Page 631
essentially as units, and to regard the relationship to the sea as a
coincidence that is only in part causal.[242]
Plateau-forming movements.—Another leading phase of crustal
movement is the settling or rising of great blocks of the crust, as though by
vertical rather than horizontal force. The western plateau of North America
and the great plateau of Thibet are gigantic examples. The American plateau
embraces numerous blocks which, while they have been elevated together,
are individually tilted in their own fashion. At the surface, they are
separated by fault-planes, but below, some of them, and perhaps most of
them, pass into flexures. Most of these flexures are of the monoclinal type
(p. 516), which dynamically means much the same as a fault; but some of
them may be of the compressive type, without inconsistency with vertical
fault-relief above. Research has not yet covered thoroughly any great
plateau, and knowledge of this class of movements is less complete than
that of folding by lateral thrust, and it has a less ample place in the literature
of the subject. The plateau-forming movements are, however, much more
massive than the mountain-folding movements, and stand next in
magnitude to the continent-forming movements. Plateaus may be regarded
as smaller platforms superposed on the continental platforms.
In the ocean-basins, there appear to be raised platforms of the plateau
type, and there are remarkable “deeps” that have the aspect of anti-plateaus.
Continent-forming movements.—True continent-forming movements
appear to have antedated the earliest known sediments. As far back as we
can read the sedimentary record, the continents seem to have been well
established, and there is little evidence that they have since been
fundamentally changed. It is true that some very eminent geologists have
rather freely connected formations on one continent with formations having
similar faunas on an opposite continent, by a hypothetical conversion of the
intervening ocean-bottoms into land or shallow water; but most such faunal
relations can be explained almost equally well by migration around the
coasts, or at most by mere ridge-connections. The paucity, if not total
absence, of abysmal deposits in the strata of the continents, taken with the
persistence of terrestrial and coastal faunas, leaves little room for assigning
an interchange of position between abysmal depths and continental
elevations, and vice versa. Dynamic considerations also offer grave
difficulties. The doctrine of the persistence of continents probably ought not
coincidence that is only in part causal.[242]
Plateau-forming movements.—Another leading phase of crustal
movement is the settling or rising of great blocks of the crust, as though by
vertical rather than horizontal force. The western plateau of North America
and the great plateau of Thibet are gigantic examples. The American plateau
embraces numerous blocks which, while they have been elevated together,
are individually tilted in their own fashion. At the surface, they are
separated by fault-planes, but below, some of them, and perhaps most of
them, pass into flexures. Most of these flexures are of the monoclinal type
(p. 516), which dynamically means much the same as a fault; but some of
them may be of the compressive type, without inconsistency with vertical
fault-relief above. Research has not yet covered thoroughly any great
plateau, and knowledge of this class of movements is less complete than
that of folding by lateral thrust, and it has a less ample place in the literature
of the subject. The plateau-forming movements are, however, much more
massive than the mountain-folding movements, and stand next in
magnitude to the continent-forming movements. Plateaus may be regarded
as smaller platforms superposed on the continental platforms.
In the ocean-basins, there appear to be raised platforms of the plateau
type, and there are remarkable “deeps” that have the aspect of anti-plateaus.
Continent-forming movements.—True continent-forming movements
appear to have antedated the earliest known sediments. As far back as we
can read the sedimentary record, the continents seem to have been well
established, and there is little evidence that they have since been
fundamentally changed. It is true that some very eminent geologists have
rather freely connected formations on one continent with formations having
similar faunas on an opposite continent, by a hypothetical conversion of the
intervening ocean-bottoms into land or shallow water; but most such faunal
relations can be explained almost equally well by migration around the
coasts, or at most by mere ridge-connections. The paucity, if not total
absence, of abysmal deposits in the strata of the continents, taken with the
persistence of terrestrial and coastal faunas, leaves little room for assigning
an interchange of position between abysmal depths and continental
elevations, and vice versa. Dynamic considerations also offer grave
difficulties. The doctrine of the persistence of continents probably ought not
Page 632
to be pushed so far as to exclude shallow water, or even land, connections
between South America, Antarctica, Australia, India, and South Africa,
directly or indirectly, at certain stages of geological history. Without
forming final conclusions as to the measure of the change which the
continents have suffered during known geological history, it is safe to
conclude that the continents and ocean-basins were in the main formed very
early in the earth’s history, and that subsequent changes have consisted
chiefly in the further sinking of the basins and the further protrusion of the
land, save as the latter has been cut down by erosion. Incidentally, the
ocean-basins have probably been extended and the continents restricted. On
the other hand, the continents have been built out on their borders by wash
from the land, and the waters of the ocean have been somewhat lifted by the
deposition of sediment in their basins. It is estimated that the cutting away
of the present continents, and the deposition of the material in the ocean-
basins, would raise the sea-level about 650 feet. (R. D. George.)
Relations of these movements in time.—The folding movements seem
to have had extraordinary prevalence in the earliest ages, for the Archean
rocks are almost universally crumpled, and often in the most intricate
fashion. There is no sign that the folding was then limited to the borders of
the continents; it seems rather to have affected the whole continental
surface. After the beginning of the well-known sedimentary series,
crumpling appears to have taken place chiefly at long intervals, thus
marking off great time-divisions, and to have been confined at any given
stage to certain tracts, chiefly on the borders of great segments of the earth’s
crust.
Concerning the plateau-forming movements in the past, knowledge is
very meager, as the detection of plateaus of ancient times is more difficult
than the detection of folds. Gentle warpings have apparently been in
progress at all times.
Relations of vertical to horizontal movements.—The downward
movements are unquestionably the primary ones, and the horizontal ones
are secondary and incidental. The fundamental feature is doubtless central
condensation actuated by gravity, and the master movements are the
sinkings of the ocean-basins. The great periodic movements that made
mountains and plateaus, and changed the capacity of the ocean-basins,
probably started with the sinking of part or all of the ocean-bottoms. In the
between South America, Antarctica, Australia, India, and South Africa,
directly or indirectly, at certain stages of geological history. Without
forming final conclusions as to the measure of the change which the
continents have suffered during known geological history, it is safe to
conclude that the continents and ocean-basins were in the main formed very
early in the earth’s history, and that subsequent changes have consisted
chiefly in the further sinking of the basins and the further protrusion of the
land, save as the latter has been cut down by erosion. Incidentally, the
ocean-basins have probably been extended and the continents restricted. On
the other hand, the continents have been built out on their borders by wash
from the land, and the waters of the ocean have been somewhat lifted by the
deposition of sediment in their basins. It is estimated that the cutting away
of the present continents, and the deposition of the material in the ocean-
basins, would raise the sea-level about 650 feet. (R. D. George.)
Relations of these movements in time.—The folding movements seem
to have had extraordinary prevalence in the earliest ages, for the Archean
rocks are almost universally crumpled, and often in the most intricate
fashion. There is no sign that the folding was then limited to the borders of
the continents; it seems rather to have affected the whole continental
surface. After the beginning of the well-known sedimentary series,
crumpling appears to have taken place chiefly at long intervals, thus
marking off great time-divisions, and to have been confined at any given
stage to certain tracts, chiefly on the borders of great segments of the earth’s
crust.
Concerning the plateau-forming movements in the past, knowledge is
very meager, as the detection of plateaus of ancient times is more difficult
than the detection of folds. Gentle warpings have apparently been in
progress at all times.
Relations of vertical to horizontal movements.—The downward
movements are unquestionably the primary ones, and the horizontal ones
are secondary and incidental. The fundamental feature is doubtless central
condensation actuated by gravity, and the master movements are the
sinkings of the ocean-basins. The great periodic movements that made
mountains and plateaus, and changed the capacity of the ocean-basins,
probably started with the sinking of part or all of the ocean-bottoms. In the
Page 633
greater periodic movements, probably all the basins participated more or
less, but some seem to have been more active than others. For example, in
the last great mountain-making period, the Pacific basin seems to have been
more active than the Atlantic, while in the similar great event at the close of
the Paleozoic, the opposite seems to have been true. The squeezing up of
the continents doubtless took place simultaneously with the settling of the
basins. The true conception is perhaps that the ocean-basins and continental
platforms are but the surface forms of great segments of the lithosphere, all
of which crowd toward the center, the stronger and heavier segments taking
precedence and squeezing the weaker and lighter ones between them. The
area of the more depressed or master segments is almost exactly twice that
of the protruding or squeezed ones. This estimate includes in the latter
about 10,000,000 square miles now covered with shallow water. The
volume of the hydrosphere is a little too great for the true basins, and it runs
over, covering the borders of the continents. The amount of the overflow
fluctuates from time to time, and may be neglected in a study of the
movements and deformations of the lithosphere.
The squeezed segments.—The great protruding segments show a
tendency toward rude triangularity. They are (1) the Eurasian, now strongly
ridged on the south and east, and relatively flat on the northwest; (2) the
African, rather strongly ridged on the east, but less abruptly elevated on the
west and north; (3) the North American, now strongly ridged on the west,
more gently on the east, and relatively flat at the north and in the interior;
(4) the South American, strongly ridged on the west and somewhat on the
northeast and southeast.
The foregoing form the major group. The minor group embraces (5) the
Antarctic segment, not as yet sufficiently known to be well defined, and (6)
the Australian, broadly reniform rather than triangular. To these are perhaps
to be added (7) the largely submerged platform that stretches from Sumatra
and Java on the southwest to the Philippines on the northeast, and is
attached to India on the northwest; and (8) Greenland, which, though
closely associated with North America, is partially separated by a rather
deep depression.
The depressed or master segments.—The great sunken segments show
a tendency to assume roughly polygonal, rather than triangular, forms. This
accords with the primary place assigned them, since, in a spherical surface
less, but some seem to have been more active than others. For example, in
the last great mountain-making period, the Pacific basin seems to have been
more active than the Atlantic, while in the similar great event at the close of
the Paleozoic, the opposite seems to have been true. The squeezing up of
the continents doubtless took place simultaneously with the settling of the
basins. The true conception is perhaps that the ocean-basins and continental
platforms are but the surface forms of great segments of the lithosphere, all
of which crowd toward the center, the stronger and heavier segments taking
precedence and squeezing the weaker and lighter ones between them. The
area of the more depressed or master segments is almost exactly twice that
of the protruding or squeezed ones. This estimate includes in the latter
about 10,000,000 square miles now covered with shallow water. The
volume of the hydrosphere is a little too great for the true basins, and it runs
over, covering the borders of the continents. The amount of the overflow
fluctuates from time to time, and may be neglected in a study of the
movements and deformations of the lithosphere.
The squeezed segments.—The great protruding segments show a
tendency toward rude triangularity. They are (1) the Eurasian, now strongly
ridged on the south and east, and relatively flat on the northwest; (2) the
African, rather strongly ridged on the east, but less abruptly elevated on the
west and north; (3) the North American, now strongly ridged on the west,
more gently on the east, and relatively flat at the north and in the interior;
(4) the South American, strongly ridged on the west and somewhat on the
northeast and southeast.
The foregoing form the major group. The minor group embraces (5) the
Antarctic segment, not as yet sufficiently known to be well defined, and (6)
the Australian, broadly reniform rather than triangular. To these are perhaps
to be added (7) the largely submerged platform that stretches from Sumatra
and Java on the southwest to the Philippines on the northeast, and is
attached to India on the northwest; and (8) Greenland, which, though
closely associated with North America, is partially separated by a rather
deep depression.
The depressed or master segments.—The great sunken segments show
a tendency to assume roughly polygonal, rather than triangular, forms. This
accords with the primary place assigned them, since, in a spherical surface
Page 634
divided into larger and smaller segments, the major parts should be
polygonal while the minor residual segments are more likely to be
triangular. The major segments are (1) the Pacific, (2) the Indian, (3) the
North Atlantic, and (4) the South Atlantic. These form the principal group,
while (5) the Arctic deeps (not including the shallow epicontinental
portions), (6) the Mediterranean, (7) the Caribbean, and (8) the chain of
deep pits between the Philippine ridge and the Bornean platform, constitute
a subordinate group.
Each member of the minor group is an irregular chain of depressed pits
rather than a single continuous deep, unless the Arctic depression, of which
little is now known, proves an exception. They lie between the greater
segments at what may be conceived to be points of critical working
relations, and are accompanied by small elevated blocks. The Caribbean,
the Mediterranean, and the Bornean regions are the seats of the greatest
present volcanic and related activities.
In a general view, there are then four great sunken quadrilaterals and four
great elevated triangles, with minor attendants in each class. Lest fondness
for simplicity and symmetry lead too far, we must hasten to observe that the
dimensions are not alike in either class. The Pacific segment is more than
twice the size of any other basin segment, and four times that of the North
Atlantic. The Eurasian triangle is more than twice the average size of the
other land segments, and nearly three times that of the South American. Nor
is there any large common divisor of approximate accuracy. This is not at
all strange if the earth be regarded as a body of somewhat heterogeneous
composition which naturally shrank in rather irregular segments. On the
other hand, this irregularity is somewhat strange if the earth has evolved
from a very homogeneous and symmetrical, primitive, fluid state. It is also
a serious consideration in any theory that appeals to crystalline form, or
analogy, as in the doctrine of a tetrahedral earth.
Roughly approximated in millions of square miles, the major depressed
segments are as follows: the Pacific, 60, the Indian, 27, the South Atlantic,
24, and the North Atlantic, 14, leaving 8 for minor depressions. The
elevated segments are Eurasian, 24, African, 12, North American, 10, and
South American, 9, leaving 10 for the minor blocks.
polygonal while the minor residual segments are more likely to be
triangular. The major segments are (1) the Pacific, (2) the Indian, (3) the
North Atlantic, and (4) the South Atlantic. These form the principal group,
while (5) the Arctic deeps (not including the shallow epicontinental
portions), (6) the Mediterranean, (7) the Caribbean, and (8) the chain of
deep pits between the Philippine ridge and the Bornean platform, constitute
a subordinate group.
Each member of the minor group is an irregular chain of depressed pits
rather than a single continuous deep, unless the Arctic depression, of which
little is now known, proves an exception. They lie between the greater
segments at what may be conceived to be points of critical working
relations, and are accompanied by small elevated blocks. The Caribbean,
the Mediterranean, and the Bornean regions are the seats of the greatest
present volcanic and related activities.
In a general view, there are then four great sunken quadrilaterals and four
great elevated triangles, with minor attendants in each class. Lest fondness
for simplicity and symmetry lead too far, we must hasten to observe that the
dimensions are not alike in either class. The Pacific segment is more than
twice the size of any other basin segment, and four times that of the North
Atlantic. The Eurasian triangle is more than twice the average size of the
other land segments, and nearly three times that of the South American. Nor
is there any large common divisor of approximate accuracy. This is not at
all strange if the earth be regarded as a body of somewhat heterogeneous
composition which naturally shrank in rather irregular segments. On the
other hand, this irregularity is somewhat strange if the earth has evolved
from a very homogeneous and symmetrical, primitive, fluid state. It is also
a serious consideration in any theory that appeals to crystalline form, or
analogy, as in the doctrine of a tetrahedral earth.
Roughly approximated in millions of square miles, the major depressed
segments are as follows: the Pacific, 60, the Indian, 27, the South Atlantic,
24, and the North Atlantic, 14, leaving 8 for minor depressions. The
elevated segments are Eurasian, 24, African, 12, North American, 10, and
South American, 9, leaving 10 for the minor blocks.
Page 635
If these segments be regarded as the great integers of body-movement,
two-thirds of them taking precedence in sinking and the other third in
suffering distortion, it is easy to pass to the conception of sub-segments,
moving somewhat differently from the main segments, so as to aid in their
adjustment to one another, and thus to the conception of plateaus and deeps.
It is easy also to pass to the conception of mutual crowding and crumpling
at the edges of these segments, accompanied by fracture and slipping. These
conceptions perhaps represent the true relations between the massive
movements of the abysmal and continental segments, as well as the less
massive plateau-forming movements and the mountain-forming distortions.
The mountains and plateaus are probably the incidental results of the great
abysmal and continental readjustments.
The great movements are probably to be attributed to stresses that
gradually accumulated until they overcame the rigidity of the thick massive
segments involved, and forced a readjustment. In accumulating these
stresses, some local yielding on weak lines and at special points was an
inevitable incident in distributing more equably the accumulating stresses.
So, also, the first great readjustments probably left many local strains and
unequal stresses which gradually eased themselves by warpings, minor
faultings, etc., so that some minor movements were a natural sequence of
the great movements. But there were doubtless many local and superficial
causes, such as irregular gains and losses of heat, regional loading and
unloading, solution, hydration, etc., that have caused local or regional
movement, and which have little to do with the great deformations of the
earth’s body. As implied above, the gentle, nearly constant movements
probably fall mainly into a different category from the great periodic
movements. Both will be considered further.
The differential extent of the movements.—Between the highest
elevation of the land and the lowest depth of the ocean, there is a vertical
range of nearly twelve miles. There may have been higher elevations,
relatively, in past times, but probably not deeper depressions; and so, if we
assume that the surface was once perfectly spheroidal, this may be taken as
a maximum expression of differential movement, not absolute vertical
movement. From the Thibetan plateau, where a considerable area exceeds
three miles in height, to the Tuscarora deep, where a notable tract exceeds
five miles in depth, the range is eight miles, which may fairly represent the
two-thirds of them taking precedence in sinking and the other third in
suffering distortion, it is easy to pass to the conception of sub-segments,
moving somewhat differently from the main segments, so as to aid in their
adjustment to one another, and thus to the conception of plateaus and deeps.
It is easy also to pass to the conception of mutual crowding and crumpling
at the edges of these segments, accompanied by fracture and slipping. These
conceptions perhaps represent the true relations between the massive
movements of the abysmal and continental segments, as well as the less
massive plateau-forming movements and the mountain-forming distortions.
The mountains and plateaus are probably the incidental results of the great
abysmal and continental readjustments.
The great movements are probably to be attributed to stresses that
gradually accumulated until they overcame the rigidity of the thick massive
segments involved, and forced a readjustment. In accumulating these
stresses, some local yielding on weak lines and at special points was an
inevitable incident in distributing more equably the accumulating stresses.
So, also, the first great readjustments probably left many local strains and
unequal stresses which gradually eased themselves by warpings, minor
faultings, etc., so that some minor movements were a natural sequence of
the great movements. But there were doubtless many local and superficial
causes, such as irregular gains and losses of heat, regional loading and
unloading, solution, hydration, etc., that have caused local or regional
movement, and which have little to do with the great deformations of the
earth’s body. As implied above, the gentle, nearly constant movements
probably fall mainly into a different category from the great periodic
movements. Both will be considered further.
The differential extent of the movements.—Between the highest
elevation of the land and the lowest depth of the ocean, there is a vertical
range of nearly twelve miles. There may have been higher elevations,
relatively, in past times, but probably not deeper depressions; and so, if we
assume that the surface was once perfectly spheroidal, this may be taken as
a maximum expression of differential movement, not absolute vertical
movement. From the Thibetan plateau, where a considerable area exceeds
three miles in height, to the Tuscarora deep, where a notable tract exceeds
five miles in depth, the range is eight miles, which may fairly represent the
Page 636
vertical range of rather massive differential movement. From the average
height of the continents to the average abysmal bottoms of the oceans the
range is nearly three miles, which may be taken as the differential
movement of the great segments. Under certain hypotheses of the origin
and early history of the earth, to be sketched later, the surface is not
assumed to have been perfectly spheroidal originally, and hence the present
irregularities do not necessarily imply so great differential movement.
If the protruding portions of the lithosphere were graded down and the
basins graded up to a common level, this level would lie about 9000 feet
below the ocean-surface. This equated level is the best basis of reference for
relative segmental movements. Referred to this datum plane, the continents,
having an area about half as great as that of the ocean depths, have been
squeezed up relatively about two miles, and the basins have sunk about one
mile from the ideal common plane. The total downward movement,
representing the total shrinkage of the earth, is quite unknown from
observation. It is probably very much greater than the differential
movement, as will appear from theoretical considerations as we go on.
The extent of the lateral movements has a peculiar interest, for it bears
theoretically on the shrinkage of the earth. Every mile of descent of the
crust represents 6 miles (6.28) shortening of the circumference. If the
vertical movements were limited to the relative ones just named, the mile of
basin descent would give but little more than 6 miles of surplus
circumference for lateral thrust and crumpling. How far does this go in
explaining the known facts? By measuring the folds of the Alps, Heim has
estimated the shortening represented by them to be 74 miles.[243] Claypole
estimated the shortening for the Appalachians in Pennsylvania, not
including the crystalline belt on the east, at 46 miles;[244] McConnel placed
that of the Laramide range in British America at 25 miles,[245] and LeConte
that of the Coast range in California at 9 to 12 miles.[246] These estimates
must be corrected for the thickening and thinning of the beds in the process
of folding, for the composite character of the folds, and for the effects of
shearing and faulting. These will in part tend to increase and in part to
decrease the estimates. The first effect of horizontal thrust is to close up all
crevices and compact the beds as much as they will stand without bending.
A part of the unusual thickness which the beds of folded regions commonly
show is probably due to this edgewise compression. In experiments on
height of the continents to the average abysmal bottoms of the oceans the
range is nearly three miles, which may be taken as the differential
movement of the great segments. Under certain hypotheses of the origin
and early history of the earth, to be sketched later, the surface is not
assumed to have been perfectly spheroidal originally, and hence the present
irregularities do not necessarily imply so great differential movement.
If the protruding portions of the lithosphere were graded down and the
basins graded up to a common level, this level would lie about 9000 feet
below the ocean-surface. This equated level is the best basis of reference for
relative segmental movements. Referred to this datum plane, the continents,
having an area about half as great as that of the ocean depths, have been
squeezed up relatively about two miles, and the basins have sunk about one
mile from the ideal common plane. The total downward movement,
representing the total shrinkage of the earth, is quite unknown from
observation. It is probably very much greater than the differential
movement, as will appear from theoretical considerations as we go on.
The extent of the lateral movements has a peculiar interest, for it bears
theoretically on the shrinkage of the earth. Every mile of descent of the
crust represents 6 miles (6.28) shortening of the circumference. If the
vertical movements were limited to the relative ones just named, the mile of
basin descent would give but little more than 6 miles of surplus
circumference for lateral thrust and crumpling. How far does this go in
explaining the known facts? By measuring the folds of the Alps, Heim has
estimated the shortening represented by them to be 74 miles.[243] Claypole
estimated the shortening for the Appalachians in Pennsylvania, not
including the crystalline belt on the east, at 46 miles;[244] McConnel placed
that of the Laramide range in British America at 25 miles,[245] and LeConte
that of the Coast range in California at 9 to 12 miles.[246] These estimates
must be corrected for the thickening and thinning of the beds in the process
of folding, for the composite character of the folds, and for the effects of
shearing and faulting. These will in part tend to increase and in part to
decrease the estimates. The first effect of horizontal thrust is to close up all
crevices and compact the beds as much as they will stand without bending.
A part of the unusual thickness which the beds of folded regions commonly
show is probably due to this edgewise compression. In experiments on
Page 637
artificial strata made to illustrate foldings (Fig. 449a), the thickening of the
layers is a very appreciable part of the process, though probably natural
beds do not thicken in equal proportion. After the beds have been closely
folded and the thrust is athwart them, they are thinned and stretched on the
limbs of the fold. How far this and other causes of extension offset initial
compression is undetermined, and is differently estimated. It seems highly
probable from the nature of the case that the edgewise compression which
resulted from sustaining the full stress before the beds bent, was much
greater than the crosswise compression on the limbs of the folds, which
came into action only after the stress had been largely satisfied by folding.
Fig. 449a.—Illustrations of Willis’ experiments in the artificial representation of mountain
folding. The sections were formed of layers of wax of different colors, and were
mechanically compressed from the right. The upper section shows the original state, and
the offsets of the succeeding sections at the right indicate the amount of shortening.
(Thirteenth Ann. Rep. U. S. Geol. Surv.)
layers is a very appreciable part of the process, though probably natural
beds do not thicken in equal proportion. After the beds have been closely
folded and the thrust is athwart them, they are thinned and stretched on the
limbs of the fold. How far this and other causes of extension offset initial
compression is undetermined, and is differently estimated. It seems highly
probable from the nature of the case that the edgewise compression which
resulted from sustaining the full stress before the beds bent, was much
greater than the crosswise compression on the limbs of the folds, which
came into action only after the stress had been largely satisfied by folding.
Fig. 449a.—Illustrations of Willis’ experiments in the artificial representation of mountain
folding. The sections were formed of layers of wax of different colors, and were
mechanically compressed from the right. The upper section shows the original state, and
the offsets of the succeeding sections at the right indicate the amount of shortening.
(Thirteenth Ann. Rep. U. S. Geol. Surv.)
Page 638
Whatever the correction, and whatever the probable errors of the above
estimates, the amount of shortening involved in folding is large. The
estimates given are merely those for certain periods of folding, and
represent only that portion of the compression of the circumference which
was concentrated in a given mountain range. The whole shortening of a
circumference is to be found by adding together all the transverse foldings
on a given great circle, following it about the globe at right angles to a
given folded tract. In so doing, it will be seen that the belt does not usually
cross more than one or two strongly folded tracts of the same age, from
which it is inferred that the shortening on each great circle was largely
concentrated in a few tracts running at large angles to each other, to
accommodate the shrinkage of the globe in all directions. If the folding in a
main range crossing any great circle is doubled, it will probably represent
roughly the shortening for that entire circle for that age. If one is disposed
to minimize the amount of folding, the estimate may perhaps be put roundly
at 50 miles, on an entire circumference, for each of the great mountain-
making periods. If, on the other hand, one is disposed to give the estimates
a generous figure so as to put explanations to the severest test, he may
perhaps fairly place the shortening at 100 miles, or even more. For the
whole shortening since Cambrian times, perhaps twice these amounts might
suffice, for while there have been several mountain-making periods, only
three are perhaps entitled to be put in the first order, that at the close of the
Paleozoic, that at the close of the Mesozoic, and that in the late Tertiary.
The shortening in the Proterozoic period was considerable, but is
imperfectly known. The Archean rocks suffered great compression in their
own times, and probably shared in that of all later periods, and if their
shortening could be estimated closely, it might be taken as covering the
whole. Assuming the circumferential shortening to have been 50 miles
during a given great mountain-folding period, the appropriate radial
shrinkage is 8 miles. For the more generous estimate of 100 miles, it is 16
miles. If these estimates be doubled for the whole of the Paleozoic and later
eras, the radial shortening becomes 16 and 32 miles, respectively.
THE CAUSES OF MOVEMENT.
General Considerations.
estimates, the amount of shortening involved in folding is large. The
estimates given are merely those for certain periods of folding, and
represent only that portion of the compression of the circumference which
was concentrated in a given mountain range. The whole shortening of a
circumference is to be found by adding together all the transverse foldings
on a given great circle, following it about the globe at right angles to a
given folded tract. In so doing, it will be seen that the belt does not usually
cross more than one or two strongly folded tracts of the same age, from
which it is inferred that the shortening on each great circle was largely
concentrated in a few tracts running at large angles to each other, to
accommodate the shrinkage of the globe in all directions. If the folding in a
main range crossing any great circle is doubled, it will probably represent
roughly the shortening for that entire circle for that age. If one is disposed
to minimize the amount of folding, the estimate may perhaps be put roundly
at 50 miles, on an entire circumference, for each of the great mountain-
making periods. If, on the other hand, one is disposed to give the estimates
a generous figure so as to put explanations to the severest test, he may
perhaps fairly place the shortening at 100 miles, or even more. For the
whole shortening since Cambrian times, perhaps twice these amounts might
suffice, for while there have been several mountain-making periods, only
three are perhaps entitled to be put in the first order, that at the close of the
Paleozoic, that at the close of the Mesozoic, and that in the late Tertiary.
The shortening in the Proterozoic period was considerable, but is
imperfectly known. The Archean rocks suffered great compression in their
own times, and probably shared in that of all later periods, and if their
shortening could be estimated closely, it might be taken as covering the
whole. Assuming the circumferential shortening to have been 50 miles
during a given great mountain-folding period, the appropriate radial
shrinkage is 8 miles. For the more generous estimate of 100 miles, it is 16
miles. If these estimates be doubled for the whole of the Paleozoic and later
eras, the radial shortening becomes 16 and 32 miles, respectively.
THE CAUSES OF MOVEMENT.
General Considerations.
Page 639
The volume of the earth is at all times dependent on two sets of
antagonistic forces, (1) the attractive or centripetal, consisting of gravity
and the molecular and sub-molecular attractions, and (2) the resistant forces
—which are not necessarily centrifugal—consisting of heat and the resistant
molecular and sub-molecular forces.
1. The centripetal agencies.
Gravity.—The most obvious of the concentrating forces is gravity, and
in most questions relating to great segmental movements, it has been
thought sufficient to consider gravity alone, but it is by no means certain
that this does not lead to serious error. In studying the causes and effects of
earth movements, it is necessary to consider both gravitational energy and
gravitational force. Gravitational energy is greatest when the mass is most
widely dispersed, and least when most concentrated. Gravitational force is
greatest when the mass is most concentrated, and least when most
dispersed. The gravitational energy of the earth matter was at its maximum
when it was most widely diffused in the supposed nebulous condition. It
will perhaps reach its minimum at some future period when the shrinkage
shall reach its limit. In passing from an expanded condition to a more
concentrated condition, potential energy, or energy of position, is
transformed into other forms of energy, chiefly heat. The heat thus
developed is an important factor in the earth’s dynamics. The total amount
of gravitational energy involved in the earth’s evolution is unknown, for
neither the maximum dispersion of the earliest state, nor the ultimate
condensation, is known. It is not difficult, however, to compute the amount
of transformation of gravitational energy into heat, or other forms of energy,
during a given degree of condensation. If a mass equal to that of the earth
were originally infinitely scattered, the gravitational energy given up by it
in condensing into a homogeneous sphere of the earth’s present size would,
if all transformed into heat, suffice to raise the temperature of an equal mass
of water 8900° C. (Hoskins), or an equal mass of rock (specific heat of .2),
44,500° C. If the mass were more condensed toward the center, as is the
actual case, the heat would be considerably greater. If the condensation
toward the center followed the Laplacian law (p. 564), the heat would be
sufficient to raise the earth mass 48,900° C., assuming its specific heat to be
.2, which is about the average specific heat of rock at the surface (Lunn). A
antagonistic forces, (1) the attractive or centripetal, consisting of gravity
and the molecular and sub-molecular attractions, and (2) the resistant forces
—which are not necessarily centrifugal—consisting of heat and the resistant
molecular and sub-molecular forces.
1. The centripetal agencies.
Gravity.—The most obvious of the concentrating forces is gravity, and
in most questions relating to great segmental movements, it has been
thought sufficient to consider gravity alone, but it is by no means certain
that this does not lead to serious error. In studying the causes and effects of
earth movements, it is necessary to consider both gravitational energy and
gravitational force. Gravitational energy is greatest when the mass is most
widely dispersed, and least when most concentrated. Gravitational force is
greatest when the mass is most concentrated, and least when most
dispersed. The gravitational energy of the earth matter was at its maximum
when it was most widely diffused in the supposed nebulous condition. It
will perhaps reach its minimum at some future period when the shrinkage
shall reach its limit. In passing from an expanded condition to a more
concentrated condition, potential energy, or energy of position, is
transformed into other forms of energy, chiefly heat. The heat thus
developed is an important factor in the earth’s dynamics. The total amount
of gravitational energy involved in the earth’s evolution is unknown, for
neither the maximum dispersion of the earliest state, nor the ultimate
condensation, is known. It is not difficult, however, to compute the amount
of transformation of gravitational energy into heat, or other forms of energy,
during a given degree of condensation. If a mass equal to that of the earth
were originally infinitely scattered, the gravitational energy given up by it
in condensing into a homogeneous sphere of the earth’s present size would,
if all transformed into heat, suffice to raise the temperature of an equal mass
of water 8900° C. (Hoskins), or an equal mass of rock (specific heat of .2),
44,500° C. If the mass were more condensed toward the center, as is the
actual case, the heat would be considerably greater. If the condensation
toward the center followed the Laplacian law (p. 564), the heat would be
sufficient to raise the earth mass 48,900° C., assuming its specific heat to be
.2, which is about the average specific heat of rock at the surface (Lunn). A
Page 640
further shrinkage of one mile would transform an additional amount of
gravitational energy into heat about equal in amount to Tait’s estimate of the
loss of heat from the surface of the earth in 100,000,000 years (see p. 572).
If the radial shrinkage has been 32 miles, or even 16 miles, the amount of
heat generated is very much greater than the estimated loss from the
surface.
How much gravitational energy can possibly be transformed into heat
and other forms of energy in the future, can only be computed by making
assumptions as to the possible extent of further contraction, and that
involves hypotheses as to the atomic and sub-atomic constitution of the
earth’s matter, and its behavior under the prodigious pressures of the earth’s
interior. All shrinkage develops added gravitational force and further
tendency to shrinkage, which follows when the heat generated by the
shrinkage is lost; and where the process may end, in a body of the
dimensions of the earth, is beyond present determination. If there were no
limit to the density that might be attained, it would be impossible to assign
any limit to the energy that might be transformed. It has usually been
assumed that contraction could not go on indefinitely because the atoms
would come into actual contact, and prevent further increase of density.
This conception rests on the recently prevalent hypothesis of the atomic
constitution of matter; but the more recent hypotheses that substitute
multitudes of revolving corpuscles or electrons for irreducible atoms, do not
carry the same presumption of a rigorous limit to condensation. It is not
therefore prudent to try to set such a limit, or to make it a feature in the
dynamical doctrines of the earth. It is even less prudent to try to measure
the limit of future conversion of the gravitational energy of the sun into
heat, and so to set a limit to the habitability of the earth.
The force of gravity may be defined as the effort of gravitational energy
to change into other forms of energy. It is most familiarly expressed in
terms of weight, which is the resultant of the gravitational force of the
whole earth upon a given portion. Weight is determined by the distances
and directions of the given portion from all parts of the attracting mass, the
amount of the attraction being directly as the mass and inversely as the
square of the distance, modified by the direction. It is greatest about 610
miles below the surface, where it is 1.0392 times that at the surface. Below
this point it declines, and at the center it is zero. The sum total of the earth’s
gravitational energy into heat about equal in amount to Tait’s estimate of the
loss of heat from the surface of the earth in 100,000,000 years (see p. 572).
If the radial shrinkage has been 32 miles, or even 16 miles, the amount of
heat generated is very much greater than the estimated loss from the
surface.
How much gravitational energy can possibly be transformed into heat
and other forms of energy in the future, can only be computed by making
assumptions as to the possible extent of further contraction, and that
involves hypotheses as to the atomic and sub-atomic constitution of the
earth’s matter, and its behavior under the prodigious pressures of the earth’s
interior. All shrinkage develops added gravitational force and further
tendency to shrinkage, which follows when the heat generated by the
shrinkage is lost; and where the process may end, in a body of the
dimensions of the earth, is beyond present determination. If there were no
limit to the density that might be attained, it would be impossible to assign
any limit to the energy that might be transformed. It has usually been
assumed that contraction could not go on indefinitely because the atoms
would come into actual contact, and prevent further increase of density.
This conception rests on the recently prevalent hypothesis of the atomic
constitution of matter; but the more recent hypotheses that substitute
multitudes of revolving corpuscles or electrons for irreducible atoms, do not
carry the same presumption of a rigorous limit to condensation. It is not
therefore prudent to try to set such a limit, or to make it a feature in the
dynamical doctrines of the earth. It is even less prudent to try to measure
the limit of future conversion of the gravitational energy of the sun into
heat, and so to set a limit to the habitability of the earth.
The force of gravity may be defined as the effort of gravitational energy
to change into other forms of energy. It is most familiarly expressed in
terms of weight, which is the resultant of the gravitational force of the
whole earth upon a given portion. Weight is determined by the distances
and directions of the given portion from all parts of the attracting mass, the
amount of the attraction being directly as the mass and inversely as the
square of the distance, modified by the direction. It is greatest about 610
miles below the surface, where it is 1.0392 times that at the surface. Below
this point it declines, and at the center it is zero. The sum total of the earth’s
Page 641
gravitative force at the present time is equivalent to about 6 × 1021 tons.
This gives rise to a pressure of about 3,000,000 atmospheres at the center of
the earth.
Gravitational force is also expressed in terms of the earth’s ability to
accelerate the velocity of falling bodies at its surface, which is now
approximately 32 feet per second. For certain purposes, the force of gravity
may be better pictured by means of the velocity required to overbalance it,
which is 6.9 miles per second; e.g. a body shot away from the surface at a
speed exceeding 6.9 miles per second, would escape from the control of the
earth if the influence of the atmosphere and other bodies is neglected; while
a body shot away at less than this speed would return to the earth.
Molecular and sub-molecular attractions.—In addition to gravity,
there are at least three additional classes of attractive agencies whose laws
appear to differ from those of gravity, viz. cohesion, chemical affinity, and
sub-atomic attraction, using these terms in their comprehensive generic
senses. The thought has been entertained that these might be reducible to
forms of gravity in ulterior analysis, but it does not appear from existing
evidence that the laws of their attractions are conformable to the Newtonian
law of the inverse square of the distance, to which gravity conforms.
Apparently the forces of the molecular, atomic, and sub-atomic attractions
increase at higher rates, and have individual peculiarities of action quite
different from gravity. It would be of the utmost service to geological
philosophy if these laws of molecular and sub-molecular attractions were
firmly established, and could be applied to the conditions of heat and
pressure under which the matter of the interior of the earth exists. In the
absence of such determinations, we can do little more than recognize that
the matter of the interior of the earth tends to condense itself by the aid of
molecular and sub-molecular attractions, supplemental to the attraction of
gravity.
Cohesion and crystallization.—The force of gravity between small
bodies is exceedingly feeble, but it is cumulative, every particle in a mass
attracting every other particle, so that in great masses the force becomes
enormous. In cohesion, and probably in the other molecular and sub-
molecular attractions, the particles attract very strongly the particles with
which they are in close relations, but beyond minute distances their effects
are insensible. The force of crystallization is felt for a very short distance
This gives rise to a pressure of about 3,000,000 atmospheres at the center of
the earth.
Gravitational force is also expressed in terms of the earth’s ability to
accelerate the velocity of falling bodies at its surface, which is now
approximately 32 feet per second. For certain purposes, the force of gravity
may be better pictured by means of the velocity required to overbalance it,
which is 6.9 miles per second; e.g. a body shot away from the surface at a
speed exceeding 6.9 miles per second, would escape from the control of the
earth if the influence of the atmosphere and other bodies is neglected; while
a body shot away at less than this speed would return to the earth.
Molecular and sub-molecular attractions.—In addition to gravity,
there are at least three additional classes of attractive agencies whose laws
appear to differ from those of gravity, viz. cohesion, chemical affinity, and
sub-atomic attraction, using these terms in their comprehensive generic
senses. The thought has been entertained that these might be reducible to
forms of gravity in ulterior analysis, but it does not appear from existing
evidence that the laws of their attractions are conformable to the Newtonian
law of the inverse square of the distance, to which gravity conforms.
Apparently the forces of the molecular, atomic, and sub-atomic attractions
increase at higher rates, and have individual peculiarities of action quite
different from gravity. It would be of the utmost service to geological
philosophy if these laws of molecular and sub-molecular attractions were
firmly established, and could be applied to the conditions of heat and
pressure under which the matter of the interior of the earth exists. In the
absence of such determinations, we can do little more than recognize that
the matter of the interior of the earth tends to condense itself by the aid of
molecular and sub-molecular attractions, supplemental to the attraction of
gravity.
Cohesion and crystallization.—The force of gravity between small
bodies is exceedingly feeble, but it is cumulative, every particle in a mass
attracting every other particle, so that in great masses the force becomes
enormous. In cohesion, and probably in the other molecular and sub-
molecular attractions, the particles attract very strongly the particles with
which they are in close relations, but beyond minute distances their effects
are insensible. The force of crystallization is felt for a very short distance
Page 642
from the crystal, and “mass action” is probably dependent on a function of
similar kind, acting at a very small distance, but the range of these forces is
very limited in comparison with that of gravity.
Rock matter, as a rule, tends to become crystalline by the assembling of
like molecules in systematic order. The general effect is condensation,
though this is not universally the case, for in some instances the crystalline
arrangement results in expansion. The crystallizing force may be regarded
as a specialized variety of cohesion which usually coöperates with gravity
to produce increased density. In cases of expansion it seems clear that the
organizing force does not act according to the law of gravity. The intensity
of the force exhibited in the formation of ice illustrates the superiority of the
molecular force over the gravitative force in small masses; but in a planet of
ice of very moderate dimensions, the internal pressure of gravity would
overcome the crystalline force, which illustrates the superiority of gravity in
large masses.
While the crystalline force may thus in exceptional cases operate against
gravity, it is known that in most cases it not only operates with it, but is
controlled by it, in this sense—that where a substance has two forms of
crystallization, it will take the denser one when the pressure is great. The
inference is that if the less dense form of crystallization takes place under
slight pressure, and subsequently the pressure is greatly increased, the form
of crystallization will change from the less to the more dense.[247] It is
probable that in general those forms of molecular arrangement will be
assumed in the deep zones which give the greatest density, and this
probably includes concretionary, colloidal, and other forms of aggregation,
as well as crystallization.
Diffusion.—The same law probably holds relative to diffusion, though in
a molecular sense diffusion is the opposite of crystallization, for in
crystallization, like comes to like, while in diffusion the molecules
distribute themselves among those of unlike nature. Diffusive action, quite
familiar in gases and liquids, takes place to some extent in solids. The
molecules of plates of gold and lead brought into intimate contact under
pressure mutually diffuse among one another. So gases seem to be very
generally diffused or “occluded” in rocks, though the nature of this relation
is imperfectly determined. It is known that pressure upon gases promotes
their diffusion through liquids and solids. It is inferred that pressure upon a
similar kind, acting at a very small distance, but the range of these forces is
very limited in comparison with that of gravity.
Rock matter, as a rule, tends to become crystalline by the assembling of
like molecules in systematic order. The general effect is condensation,
though this is not universally the case, for in some instances the crystalline
arrangement results in expansion. The crystallizing force may be regarded
as a specialized variety of cohesion which usually coöperates with gravity
to produce increased density. In cases of expansion it seems clear that the
organizing force does not act according to the law of gravity. The intensity
of the force exhibited in the formation of ice illustrates the superiority of the
molecular force over the gravitative force in small masses; but in a planet of
ice of very moderate dimensions, the internal pressure of gravity would
overcome the crystalline force, which illustrates the superiority of gravity in
large masses.
While the crystalline force may thus in exceptional cases operate against
gravity, it is known that in most cases it not only operates with it, but is
controlled by it, in this sense—that where a substance has two forms of
crystallization, it will take the denser one when the pressure is great. The
inference is that if the less dense form of crystallization takes place under
slight pressure, and subsequently the pressure is greatly increased, the form
of crystallization will change from the less to the more dense.[247] It is
probable that in general those forms of molecular arrangement will be
assumed in the deep zones which give the greatest density, and this
probably includes concretionary, colloidal, and other forms of aggregation,
as well as crystallization.
Diffusion.—The same law probably holds relative to diffusion, though in
a molecular sense diffusion is the opposite of crystallization, for in
crystallization, like comes to like, while in diffusion the molecules
distribute themselves among those of unlike nature. Diffusive action, quite
familiar in gases and liquids, takes place to some extent in solids. The
molecules of plates of gold and lead brought into intimate contact under
pressure mutually diffuse among one another. So gases seem to be very
generally diffused or “occluded” in rocks, though the nature of this relation
is imperfectly determined. It is known that pressure upon gases promotes
their diffusion through liquids and solids. It is inferred that pressure upon a
Page 643
solid tends to the diffusion of the entrapped gases within it, but it is not to
be inferred from this that pressure upon rock promotes the absorption of
gases into it, but rather the opposite. It is probable that great pressure with
high heat promotes the diffusion of entrapped gases or other diffusible
substances through the rock-mass, and at the same time tends to their
extrusion along lines of least resistance; but this is an inference rather than a
demonstration.
Chemical combination.—The general effect of chemical combination
under pressure is greater density. In reversible reactions capable of
conditions of chemical or physical equilibrium, pressure invariably favors
the formation of the denser of any possible products.
Sub-atomic forces.—Recent investigation has made it probable that
atoms are composite, embracing many exceedingly minute bodies—
corpuscles or electrons—in a state of extremely high activity and possessed
of marvelous energy notwithstanding their minuteness. This discovery
possesses deep interest to the geologist because it seems to reveal sources
of energy of almost incalculable potency, some portions of which at least
are being constantly freed and added to the previously recognized supplies
of energy. Attempts have been made during the past few decades to limit the
habitable age of the earth, both retrospectively and prospectively, by the
smallness of the sum total of energy derivable from gravity. In these
estimates slight recognition has been given to the resources of molecular
and atomic energy, and none at all to the possibilities of sub-atomic energy.
It would be going quite too far to assume that these sub-atomic energies are
all available for the perpetuation of habitable conditions on the earth or in
the solar system, but we are doubtless justified in appealing to them as an
offset to all dicta restricting the period of the earth’s habitability by
supposed insufficiencies of energy deduced merely from the estimated
resources of gravity. The banishment of the idea of the atom as a minute,
incompressible, undecomposable sphere takes away the theoretical limit of
compressibility, and by so doing cuts away the groundwork for assigning
definite limits even to the resources of gravity, since, as already indicated,
unlimited condensation gives theoretically unlimited transformation of the
potential energy of gravity.
While we must await with such patience as we can command the
development of fuller knowledge concerning the nature and laws of the
be inferred from this that pressure upon rock promotes the absorption of
gases into it, but rather the opposite. It is probable that great pressure with
high heat promotes the diffusion of entrapped gases or other diffusible
substances through the rock-mass, and at the same time tends to their
extrusion along lines of least resistance; but this is an inference rather than a
demonstration.
Chemical combination.—The general effect of chemical combination
under pressure is greater density. In reversible reactions capable of
conditions of chemical or physical equilibrium, pressure invariably favors
the formation of the denser of any possible products.
Sub-atomic forces.—Recent investigation has made it probable that
atoms are composite, embracing many exceedingly minute bodies—
corpuscles or electrons—in a state of extremely high activity and possessed
of marvelous energy notwithstanding their minuteness. This discovery
possesses deep interest to the geologist because it seems to reveal sources
of energy of almost incalculable potency, some portions of which at least
are being constantly freed and added to the previously recognized supplies
of energy. Attempts have been made during the past few decades to limit the
habitable age of the earth, both retrospectively and prospectively, by the
smallness of the sum total of energy derivable from gravity. In these
estimates slight recognition has been given to the resources of molecular
and atomic energy, and none at all to the possibilities of sub-atomic energy.
It would be going quite too far to assume that these sub-atomic energies are
all available for the perpetuation of habitable conditions on the earth or in
the solar system, but we are doubtless justified in appealing to them as an
offset to all dicta restricting the period of the earth’s habitability by
supposed insufficiencies of energy deduced merely from the estimated
resources of gravity. The banishment of the idea of the atom as a minute,
incompressible, undecomposable sphere takes away the theoretical limit of
compressibility, and by so doing cuts away the groundwork for assigning
definite limits even to the resources of gravity, since, as already indicated,
unlimited condensation gives theoretically unlimited transformation of the
potential energy of gravity.
While we must await with such patience as we can command the
development of fuller knowledge concerning the nature and laws of the
Page 644
molecular, atomic, and sub-atomic energies, and their applicability to the
activities resident in the interior of the earth, it is permissible even now to
assume that, besides the simple compressive action of gravity, there are at
work varied forms of molecular aggregation, of atomic combination, and
perhaps of sub-atomic change, tending toward increased density, and that
the ulterior limit of these processes is quite undetermined. The
condensational forces are now restrained at certain temporary limits by the
antagonistic resistant forces, some of which, such as heat, are the products
of the condensational forces, and are gradually being dissipated, permitting
further condensation. Where the process may ultimately end, we dare not
attempt to say. On the other hand, we are not compelled to accept assigned
limits that seem to be inconsistent with the phenomena which the earth
actually presents.
2. The resisting agencies.
Heat.—The most familiar of the active agencies that resist condensation
is heat. Upon this the existing volume of the earth is immediately
dependent, in some large part at least. As this heat is dissipated, the earth
shrinks. This shrinkage increases the force of gravity, and hence the internal
pressure increases, and, if further compression takes place as the result of
this increased pressure, additional heat is developed, which checks further
condensation until it is dissipated. It is this kind of creative and self-
checking action that determines the volume of great gaseous bodies like the
sun. Though their matter is far from its ultimate density, and their self-
gravity is enormous, they condense slowly, because, with every stage of
condensation, heat is generated which antagonizes gravity and checks
condensation, until at least a part of the heat is radiated away. As the force
of gravity increases with every stage of condensation, the heat developed to
hold it in check must increase, and hence the famous law of Lane, that a
gaseous body like the sun grows hotter as it condenses. This law holds good
while the body remains in a gaseous state in which the maintenance of the
volume is essentially dependent on heat. When a body becomes liquid or
solid, its volume is dependent in part on forms of resistance other than heat,
and the force of the law is abated, though the principle still holds good. In
small solids, the principle has little application, since the force of self-
gravity is slight compared to the resisting forces, and very little new heat is
activities resident in the interior of the earth, it is permissible even now to
assume that, besides the simple compressive action of gravity, there are at
work varied forms of molecular aggregation, of atomic combination, and
perhaps of sub-atomic change, tending toward increased density, and that
the ulterior limit of these processes is quite undetermined. The
condensational forces are now restrained at certain temporary limits by the
antagonistic resistant forces, some of which, such as heat, are the products
of the condensational forces, and are gradually being dissipated, permitting
further condensation. Where the process may ultimately end, we dare not
attempt to say. On the other hand, we are not compelled to accept assigned
limits that seem to be inconsistent with the phenomena which the earth
actually presents.
2. The resisting agencies.
Heat.—The most familiar of the active agencies that resist condensation
is heat. Upon this the existing volume of the earth is immediately
dependent, in some large part at least. As this heat is dissipated, the earth
shrinks. This shrinkage increases the force of gravity, and hence the internal
pressure increases, and, if further compression takes place as the result of
this increased pressure, additional heat is developed, which checks further
condensation until it is dissipated. It is this kind of creative and self-
checking action that determines the volume of great gaseous bodies like the
sun. Though their matter is far from its ultimate density, and their self-
gravity is enormous, they condense slowly, because, with every stage of
condensation, heat is generated which antagonizes gravity and checks
condensation, until at least a part of the heat is radiated away. As the force
of gravity increases with every stage of condensation, the heat developed to
hold it in check must increase, and hence the famous law of Lane, that a
gaseous body like the sun grows hotter as it condenses. This law holds good
while the body remains in a gaseous state in which the maintenance of the
volume is essentially dependent on heat. When a body becomes liquid or
solid, its volume is dependent in part on forms of resistance other than heat,
and the force of the law is abated, though the principle still holds good. In
small solids, the principle has little application, since the force of self-
gravity is slight compared to the resisting forces, and very little new heat is
Page 645
generated as the body loses that which it has; but in large bodies, like the
earth, where the condensational forces are enormous and the internal
temperature is very high, it is not improbable that the heat generated at
every stage of condensation is relatively large. It has been inferred by some
students of the phenomena that the conditions in the interior of the earth are
essentially those of gaseous matter, so far as molecular relations are
concerned, because the temperatures are thought to be above the critical
temperatures of the substances composing it. If this be true, the new heat
generated with each stage of condensation is large. However this may be, it
seems safe to infer that in so far as the volume of the interior mass is
dependent on heat resistance, the loss of existing heat leads to the
generation of new heat. The amount of this new heat must be enough,
together with the residual heat and the other forces of resistance, to match
the new condensational forces. The molecular and sub-molecular forces of
resistance other than heat, are probably responsible for some large part of
the resistance to the increased condensational force, but how much is not
determined.
All resistance perhaps due to motion.—As now interpreted, the force
of resistance of heat is due to the impact of the flying particles of the heated
matter. The other forms of resistance to compression have not usually been
interpreted in this way, but the tendency of recent investigation is to place
them in the same dynamic class. A cold solid body offers resistance to
compression that is in no obvious way dependent on heat motion. In small
bodies this resistance is immeasurably greater than the self-gravity of the
body. It is so great that it can only be partially overcome by any force which
human ingenuity can bring to bear upon it. This form of resistance has thus,
not unnaturally, come to be regarded as approximately immeasurable, and
perhaps as grading into actual immeasurability, and as resting back upon the
actual contact of irreducible atoms. But the recent researches which have
developed grounds for the conception that even the atoms are composite,
lead to the further conception that their resistance to compression is
dependent on the movement of their constituent corpuscles or electrons.
This encourages the broad conception that the whole of the resistance to
compression arises from molecular, atomic, and sub-atomic motions, of
which heat is merely one form.
earth, where the condensational forces are enormous and the internal
temperature is very high, it is not improbable that the heat generated at
every stage of condensation is relatively large. It has been inferred by some
students of the phenomena that the conditions in the interior of the earth are
essentially those of gaseous matter, so far as molecular relations are
concerned, because the temperatures are thought to be above the critical
temperatures of the substances composing it. If this be true, the new heat
generated with each stage of condensation is large. However this may be, it
seems safe to infer that in so far as the volume of the interior mass is
dependent on heat resistance, the loss of existing heat leads to the
generation of new heat. The amount of this new heat must be enough,
together with the residual heat and the other forces of resistance, to match
the new condensational forces. The molecular and sub-molecular forces of
resistance other than heat, are probably responsible for some large part of
the resistance to the increased condensational force, but how much is not
determined.
All resistance perhaps due to motion.—As now interpreted, the force
of resistance of heat is due to the impact of the flying particles of the heated
matter. The other forms of resistance to compression have not usually been
interpreted in this way, but the tendency of recent investigation is to place
them in the same dynamic class. A cold solid body offers resistance to
compression that is in no obvious way dependent on heat motion. In small
bodies this resistance is immeasurably greater than the self-gravity of the
body. It is so great that it can only be partially overcome by any force which
human ingenuity can bring to bear upon it. This form of resistance has thus,
not unnaturally, come to be regarded as approximately immeasurable, and
perhaps as grading into actual immeasurability, and as resting back upon the
actual contact of irreducible atoms. But the recent researches which have
developed grounds for the conception that even the atoms are composite,
lead to the further conception that their resistance to compression is
dependent on the movement of their constituent corpuscles or electrons.
This encourages the broad conception that the whole of the resistance to
compression arises from molecular, atomic, and sub-atomic motions, of
which heat is merely one form.
Page 646
While all this is yet on the frontier of physical progress, these
conceptions may well be recognized in framing interpretations of the
agencies which determine the volume of the earth, and which control the
changes that take place in it from age to age. The result of their combined
action at any stage is a state of temporary equilibrium between gravity,
aided by the molecular, atomic, and sub-atomic attractions, on the one hand,
and heat, aided by the molecular, atomic, and sub-atomic resistances, on the
other. The vital problem is to ascertain the original condition of balance
between these antagonistic forces, and the changes which have affected that
balance since. The original state of balance is necessarily a matter of
hypothesis, and the best that can be done at present is to picture as clearly
as possible the different hypotheses that have been entertained, and the
different consequences that logically flow from them. The most important
factor in the case is the original amount and distribution of internal heat.
ALTERNATIVE VIEWS OF ORIGINAL HEAT
DISTRIBUTION.
The hypothetical modes of origin of the earth will be treated in the
historical section. Suffice it here to say that one view is that the earth was
once gaseous, passed thence into a liquid, and later into a solid state. Under
this view, there are two hypotheses as to the original distribution of internal
heat, dependent on the mode of solidification. According to the one,
solidification began at the surface after convection had brought the
temperature of the whole mass down nearly to the point of congelation;
according to the other, solidification began at the center at a high
temperature, because of pressure, and proceeded thence outwards. The
former only has been much developed in the literature of the subject,
though the latter is now generally regarded as the more probable.
Another view of the globe’s origin is that the earth was built up gradually
by the infall of matter, bit by bit, at such a rate that though each little mass
became hot as a result of its fall, it cooled off before others fell on the same
spot, the rain of matter not being fast enough to heat up the whole mass to
the melting-point. Under this view, the internal heat arose chiefly from
compression due to the earth’s gravity.
conceptions may well be recognized in framing interpretations of the
agencies which determine the volume of the earth, and which control the
changes that take place in it from age to age. The result of their combined
action at any stage is a state of temporary equilibrium between gravity,
aided by the molecular, atomic, and sub-atomic attractions, on the one hand,
and heat, aided by the molecular, atomic, and sub-atomic resistances, on the
other. The vital problem is to ascertain the original condition of balance
between these antagonistic forces, and the changes which have affected that
balance since. The original state of balance is necessarily a matter of
hypothesis, and the best that can be done at present is to picture as clearly
as possible the different hypotheses that have been entertained, and the
different consequences that logically flow from them. The most important
factor in the case is the original amount and distribution of internal heat.
ALTERNATIVE VIEWS OF ORIGINAL HEAT
DISTRIBUTION.
The hypothetical modes of origin of the earth will be treated in the
historical section. Suffice it here to say that one view is that the earth was
once gaseous, passed thence into a liquid, and later into a solid state. Under
this view, there are two hypotheses as to the original distribution of internal
heat, dependent on the mode of solidification. According to the one,
solidification began at the surface after convection had brought the
temperature of the whole mass down nearly to the point of congelation;
according to the other, solidification began at the center at a high
temperature, because of pressure, and proceeded thence outwards. The
former only has been much developed in the literature of the subject,
though the latter is now generally regarded as the more probable.
Another view of the globe’s origin is that the earth was built up gradually
by the infall of matter, bit by bit, at such a rate that though each little mass
became hot as a result of its fall, it cooled off before others fell on the same
spot, the rain of matter not being fast enough to heat up the whole mass to
the melting-point. Under this view, the internal heat arose chiefly from
compression due to the earth’s gravity.
Page 647
A clear conception of the three hypotheses of thermal distribution which
rest on these two views of the origin of the earth is important to the further
discussion.
1. Thermal distribution on the convection hypothesis.—It was
formerly the prevailing opinion that the molten condition of the earth
persisted in the interior until after the crust had formed, and that
solidification proceeded from the surface downwards. It was a natural
corollary of this view that, previous to the beginning of solidification,
convection stirred the liquid mass from center to circumference and
equalized the temperature so that the whole mass cooled down equably until
it approached the point of solidification and became too viscous for ready
convection. The temperature should, therefore, have been nearly the same
from center to surface at the stage just preceding incipient solidification.
This conception forms the basis of most discussions involving internal
temperatures.[248] The famous studies of Lord Kelvin are based on the
assumption of a uniform initial temperature of 7000° Fahr.[249] Other
temperatures have been assumed in similar studies by others, but the results
do not differ materially. On this hypothesis there would be no deep-seated
change of temperature until a temperature-gradient, extending to the deeper
horizons, had been developed by surface cooling. In the earliest eras, the
loss of heat would be felt solely in the outer zone. By surface cooling, a
temperature gradient would be slowly developed, and gradually changed
from age to age, as shown by the curved lines in Fig. 450, each of which
shows the temperature at the successive stages stated in the legend. The
computations for these curves were based on the methods and assumptions
of Lord Kelvin. The two lower curves represent greater periods than those
usually assigned by geologists to the whole history of the earth. It will be
seen that the modification of the original temperature line extends only
about 160 miles below the surface for the 100,000,000-year period, only
about 240 miles for the 237,000,000-year period, and only about 320 miles
for the excessive period of 600,000,000 years. The superficial nature of the
whole thermal problem under this hypothesis is thus made clear and
impressive.
rest on these two views of the origin of the earth is important to the further
discussion.
1. Thermal distribution on the convection hypothesis.—It was
formerly the prevailing opinion that the molten condition of the earth
persisted in the interior until after the crust had formed, and that
solidification proceeded from the surface downwards. It was a natural
corollary of this view that, previous to the beginning of solidification,
convection stirred the liquid mass from center to circumference and
equalized the temperature so that the whole mass cooled down equably until
it approached the point of solidification and became too viscous for ready
convection. The temperature should, therefore, have been nearly the same
from center to surface at the stage just preceding incipient solidification.
This conception forms the basis of most discussions involving internal
temperatures.[248] The famous studies of Lord Kelvin are based on the
assumption of a uniform initial temperature of 7000° Fahr.[249] Other
temperatures have been assumed in similar studies by others, but the results
do not differ materially. On this hypothesis there would be no deep-seated
change of temperature until a temperature-gradient, extending to the deeper
horizons, had been developed by surface cooling. In the earliest eras, the
loss of heat would be felt solely in the outer zone. By surface cooling, a
temperature gradient would be slowly developed, and gradually changed
from age to age, as shown by the curved lines in Fig. 450, each of which
shows the temperature at the successive stages stated in the legend. The
computations for these curves were based on the methods and assumptions
of Lord Kelvin. The two lower curves represent greater periods than those
usually assigned by geologists to the whole history of the earth. It will be
seen that the modification of the original temperature line extends only
about 160 miles below the surface for the 100,000,000-year period, only
about 240 miles for the 237,000,000-year period, and only about 320 miles
for the excessive period of 600,000,000 years. The superficial nature of the
whole thermal problem under this hypothesis is thus made clear and
impressive.
Page 648
Fig. 450.—Diagram showing the original distribution of heat assumed by the convection
hypothesis and the modifications of this distribution near the surface in successive long
periods. The base-line of the figure represents divisions of the earth-radius with center at
the left and surface at the right. The vertical lines represent temperatures ranging from
0° C. to 5000° C. The assumed initial temperature 3900° C. (7000° F.) is represented by
the horizontal line TC, full at the left and dotted at the right to indicate the original
extension of the initial temperature to the surface. The upper curve at the right shows
how much the temperature will have been modified at the end of 100,000,000 years,
computed according to the method of Lord Kelvin. The middle curve shows the change
at the end of 237,000,000 years, and the lower curve the change at the end of 600,000,000
years. Similar curves may be found in an article by Clarence King, Am. Jour. of Sci.,
XLV, 1893, p. 16.
After the outer shell had cooled so as to be in approximate equilibrium
with the environment of the earth, it suffered practically no contraction.
So also it appears from the diagram that there was practically no
contraction below 160 miles up to the end of the 100,000,000-year period,
because cooling had not yet reached that depth. Between these two non-
contracting horizons the greatest rate of contraction at the close of the
100,000,000-year period lay about 60 miles below the surface. The
contraction of this middle zone, while the outermost shell and the interior
body remained constant, is held to have developed a state of horizontal
thrust in the outer shell, because this shell, being too large for the shrinking
subcrust, tended to settle, and to crowd upon itself horizontally. The
wrinkling and other modes of deformation of the outer part of the earth are
referred, under this view, to the thrust so developed. This is the view which
has been most generally accepted.
Level of no stress.—As the outer shell is thus held to be in a state of
thrust while the zone below is in a state of shrinkage, there must be,
between these two zones, a level of no stress, where there is neither
compression nor stretching. Above this level, the thrust increases to the
surface, and below it, the stretching increases to the depth of most rapid
change of temperature, below which it decreases and finally vanishes at the
lower limit of temperature change. In the earliest stages of cooling, the level
of no stress must have been near the surface, and must have descended
gradually as the cooling proceeded. The depth of this level has been
repeatedly computed on the basis of assumed times and rates of cooling.
hypothesis and the modifications of this distribution near the surface in successive long
periods. The base-line of the figure represents divisions of the earth-radius with center at
the left and surface at the right. The vertical lines represent temperatures ranging from
0° C. to 5000° C. The assumed initial temperature 3900° C. (7000° F.) is represented by
the horizontal line TC, full at the left and dotted at the right to indicate the original
extension of the initial temperature to the surface. The upper curve at the right shows
how much the temperature will have been modified at the end of 100,000,000 years,
computed according to the method of Lord Kelvin. The middle curve shows the change
at the end of 237,000,000 years, and the lower curve the change at the end of 600,000,000
years. Similar curves may be found in an article by Clarence King, Am. Jour. of Sci.,
XLV, 1893, p. 16.
After the outer shell had cooled so as to be in approximate equilibrium
with the environment of the earth, it suffered practically no contraction.
So also it appears from the diagram that there was practically no
contraction below 160 miles up to the end of the 100,000,000-year period,
because cooling had not yet reached that depth. Between these two non-
contracting horizons the greatest rate of contraction at the close of the
100,000,000-year period lay about 60 miles below the surface. The
contraction of this middle zone, while the outermost shell and the interior
body remained constant, is held to have developed a state of horizontal
thrust in the outer shell, because this shell, being too large for the shrinking
subcrust, tended to settle, and to crowd upon itself horizontally. The
wrinkling and other modes of deformation of the outer part of the earth are
referred, under this view, to the thrust so developed. This is the view which
has been most generally accepted.
Level of no stress.—As the outer shell is thus held to be in a state of
thrust while the zone below is in a state of shrinkage, there must be,
between these two zones, a level of no stress, where there is neither
compression nor stretching. Above this level, the thrust increases to the
surface, and below it, the stretching increases to the depth of most rapid
change of temperature, below which it decreases and finally vanishes at the
lower limit of temperature change. In the earliest stages of cooling, the level
of no stress must have been near the surface, and must have descended
gradually as the cooling proceeded. The depth of this level has been
repeatedly computed on the basis of assumed times and rates of cooling.
Page 649
Fisher, assuming the temperature of solidification to have been 4000° Fahr.
and the period of cooling 33,000,000 years, computed its depth at only ⁷⁄₁₀
of a mile below the surface.[250] T. Mellard Reade, with somewhat different
assumptions, placed it at 2 miles after 100,000,000 years of cooling.[251]
Davison (1897) placed it at 2.17 miles,[252] and G. H. Darwin at 2 miles after
the same period.[252] In a later computation, based on the assumption that the
coefficient of dilatation increases with the temperature, Davison placed the
level of no stress at 7.79 miles, and stated that if the coefficient of
conductivity and the initial heat also increased down wards, the zone would
lie still deeper. To suppose the initial heat to increase downwards, however,
is to abandon the hypothesis we are now considering. These computations
seem to show that, at the very utmost, the level of no stress, under this
hypothesis, lies at a very slight depth, and that the thrust zone above is,
therefore, very shallow. This should be kept constantly in mind in all
deductions drawn from this hypothesis. If the thickness of the thrust zone be
taken at 8 or 10 miles, it will apparently be conceding to the view all that
can legitimately be claimed for it.
and the period of cooling 33,000,000 years, computed its depth at only ⁷⁄₁₀
of a mile below the surface.[250] T. Mellard Reade, with somewhat different
assumptions, placed it at 2 miles after 100,000,000 years of cooling.[251]
Davison (1897) placed it at 2.17 miles,[252] and G. H. Darwin at 2 miles after
the same period.[252] In a later computation, based on the assumption that the
coefficient of dilatation increases with the temperature, Davison placed the
level of no stress at 7.79 miles, and stated that if the coefficient of
conductivity and the initial heat also increased down wards, the zone would
lie still deeper. To suppose the initial heat to increase downwards, however,
is to abandon the hypothesis we are now considering. These computations
seem to show that, at the very utmost, the level of no stress, under this
hypothesis, lies at a very slight depth, and that the thrust zone above is,
therefore, very shallow. This should be kept constantly in mind in all
deductions drawn from this hypothesis. If the thickness of the thrust zone be
taken at 8 or 10 miles, it will apparently be conceding to the view all that
can legitimately be claimed for it.
Page 650
Fig. 451.—Diagram illustrating the internal temperatures of the earth when it first became
solid, under the hypothesis that it solidified from the center outward, and assuming that
the fusing-point rose directly as the pressure, in accordance with Barus’ experiments
with diabase. The divisions of the base-line represent fractions of the earth’s radius. The
divisions of the vertical lines represent pressures in atmospheres at the left, and
temperatures in degrees C. at the right. The lower curve, PC, represents the interior
pressures, ranging from one atmosphere at the surface to 3,000,000 atmospheres at the
center, derived from Laplace’s law of density. The upper curve, FC, represents the
fusion-points of diabase at the various depths and pressures, and hence the temperatures
at which the interior would become solid at the various depths, or, in other words, the
initial temperatures of the solid earth. The lower curve is derived from Slichter; the
upper is formed by directly plotting the temperatures given by Barus (Am. Jour. Sci.,
1893, p. 7).
2. Thermal distribution on the hypothesis of central solidification.—
When the previous conception was first formed, the effect of pressure on
the melting-points of lavas was neglected, as little or nothing was known on
the subject. Experiment, however, has shown that pressure, as a rule, raises
the melting-points of lavas, and out of this has grown the doctrine that the
earth solidified first at the center, where the pressure was greatest, and
gradually congealed outwards. Barus has shown that the melting-point of
diabase,[253] selected as a representative rock, rises directly with the
solid, under the hypothesis that it solidified from the center outward, and assuming that
the fusing-point rose directly as the pressure, in accordance with Barus’ experiments
with diabase. The divisions of the base-line represent fractions of the earth’s radius. The
divisions of the vertical lines represent pressures in atmospheres at the left, and
temperatures in degrees C. at the right. The lower curve, PC, represents the interior
pressures, ranging from one atmosphere at the surface to 3,000,000 atmospheres at the
center, derived from Laplace’s law of density. The upper curve, FC, represents the
fusion-points of diabase at the various depths and pressures, and hence the temperatures
at which the interior would become solid at the various depths, or, in other words, the
initial temperatures of the solid earth. The lower curve is derived from Slichter; the
upper is formed by directly plotting the temperatures given by Barus (Am. Jour. Sci.,
1893, p. 7).
2. Thermal distribution on the hypothesis of central solidification.—
When the previous conception was first formed, the effect of pressure on
the melting-points of lavas was neglected, as little or nothing was known on
the subject. Experiment, however, has shown that pressure, as a rule, raises
the melting-points of lavas, and out of this has grown the doctrine that the
earth solidified first at the center, where the pressure was greatest, and
gradually congealed outwards. Barus has shown that the melting-point of
diabase,[253] selected as a representative rock, rises directly with the
Page 651
pressure. If this rate holds good to the center of the earth, the melting
temperature of diabase there would be 76,000° C. (136,800°F.). The range
of the experiment is, however, very small compared with the range of the
application, and little confidence can be felt in the special numerical result
reached. The rate of rise of the fusion-point may be much changed as the
extraordinary conditions of the deep interior are invaded. Still there is good
ground for the hypothesis that solidification took place at some very high
temperature at the center, because of the very great pressure there. The
inference then is that when the temperature of the center of the supposed
molten globe reached the appropriate point, solidification began there, and
that it took place at lesser depths in succession as the appropriate
temperatures were reached. This view excludes convection in the successive
zones from the center outward after the time when their temperatures of
solidification were reached, or after these were approached sufficiently near
to develop prohibitive viscosity. Some loss of heat from these horizons
would be suffered while the outer parts were solidifying, but on account of
the exceedingly slow conductivity of rock, it is improbable that the amount
of loss would be sufficient to change the general character of the internal
distribution of heat previous to solidification at the surface, the time when
the existing phase of the earth’s history by hypothesis began. Fig. 451
shows the theoretical distribution of heat under this view. The consequences
of this assumption are very important to geological theory and, carried out
to their logical consequences, lead to the conclusion that cooling and
shrinkage affected the deep interior of the earth, for the high central heat
must have been constantly passing out toward the surface. Instead,
therefore, of the contraction being concentrated in and limited to the outer
200 miles or so, as under the preceding hypothesis, it was deeply
distributed. The contraction within the outer zone would be less than under
the preceding view, because the flow of heat from within would partially
offset the flow outwards, and a corresponding part of the contraction would
be distributed below.
COMPUTED PRESSURES, DENSITIES, AND
TEMPERATURES WITHIN THE EARTH BASED
ON LAPLACE’s LAW.
temperature of diabase there would be 76,000° C. (136,800°F.). The range
of the experiment is, however, very small compared with the range of the
application, and little confidence can be felt in the special numerical result
reached. The rate of rise of the fusion-point may be much changed as the
extraordinary conditions of the deep interior are invaded. Still there is good
ground for the hypothesis that solidification took place at some very high
temperature at the center, because of the very great pressure there. The
inference then is that when the temperature of the center of the supposed
molten globe reached the appropriate point, solidification began there, and
that it took place at lesser depths in succession as the appropriate
temperatures were reached. This view excludes convection in the successive
zones from the center outward after the time when their temperatures of
solidification were reached, or after these were approached sufficiently near
to develop prohibitive viscosity. Some loss of heat from these horizons
would be suffered while the outer parts were solidifying, but on account of
the exceedingly slow conductivity of rock, it is improbable that the amount
of loss would be sufficient to change the general character of the internal
distribution of heat previous to solidification at the surface, the time when
the existing phase of the earth’s history by hypothesis began. Fig. 451
shows the theoretical distribution of heat under this view. The consequences
of this assumption are very important to geological theory and, carried out
to their logical consequences, lead to the conclusion that cooling and
shrinkage affected the deep interior of the earth, for the high central heat
must have been constantly passing out toward the surface. Instead,
therefore, of the contraction being concentrated in and limited to the outer
200 miles or so, as under the preceding hypothesis, it was deeply
distributed. The contraction within the outer zone would be less than under
the preceding view, because the flow of heat from within would partially
offset the flow outwards, and a corresponding part of the contraction would
be distributed below.
COMPUTED PRESSURES, DENSITIES, AND
TEMPERATURES WITHIN THE EARTH BASED
ON LAPLACE’s LAW.
Page 652
Distance from Pressure in
Temperature
center in terms megadynes Density.
in degrees C.
of radius. per sq. cm.[254]
1.00 0 2.80 0
.95 97,000 3.37 320
.90 215,000 3.95 1,110
.85 353,000 4.54 2,190
.80 510,000 5.13 3,470
.75 684,000 5.71 4,880
.70 874,000 6.28 6,350
.65 1,077,000 6.84 7,860
.60 1,289,000 7.38 9,360
.55 1,507,000 7.90 10,830
.50 1,727,000 8.39 12,250
.45 1,944,000 8.84 13,590
.40 2,154,000 9.26 14,840
.35 2,353,000 9.64 15,980
.30 2,535,000 9.98 17,000
.25 2,698,000 10.27 17,880
.20 2,836,000 10.51 18,610
.15 2,947,000 10.70 19,190
.10 3,029,000 10.84 19,610
.05 3,078,000 10.92 19,870
.00 3,095,000 10.95 19,950
3. Thermal distribution under the accretion hypothesis.—The
accretion hypothesis assumes that the internal heat was gradually developed
from the center outwards as the earth grew and the internal compression
was progressively developed. The heat, therefore, continued to rise at the
center as long as compression continued, or at least as long as the
compression was sufficient to generate heat faster than it was conducted
outwards. As the conduction of heat through rock is exceedingly slow, the
central heat may be assumed to have continued to rise so long as the infall
of matter caused appreciable compression. In the same way, heat was
generated progressively in the less central parts, and these parts also
received the heat that passed out from beneath. It is assumed under this
Temperature
center in terms megadynes Density.
in degrees C.
of radius. per sq. cm.[254]
1.00 0 2.80 0
.95 97,000 3.37 320
.90 215,000 3.95 1,110
.85 353,000 4.54 2,190
.80 510,000 5.13 3,470
.75 684,000 5.71 4,880
.70 874,000 6.28 6,350
.65 1,077,000 6.84 7,860
.60 1,289,000 7.38 9,360
.55 1,507,000 7.90 10,830
.50 1,727,000 8.39 12,250
.45 1,944,000 8.84 13,590
.40 2,154,000 9.26 14,840
.35 2,353,000 9.64 15,980
.30 2,535,000 9.98 17,000
.25 2,698,000 10.27 17,880
.20 2,836,000 10.51 18,610
.15 2,947,000 10.70 19,190
.10 3,029,000 10.84 19,610
.05 3,078,000 10.92 19,870
.00 3,095,000 10.95 19,950
3. Thermal distribution under the accretion hypothesis.—The
accretion hypothesis assumes that the internal heat was gradually developed
from the center outwards as the earth grew and the internal compression
was progressively developed. The heat, therefore, continued to rise at the
center as long as compression continued, or at least as long as the
compression was sufficient to generate heat faster than it was conducted
outwards. As the conduction of heat through rock is exceedingly slow, the
central heat may be assumed to have continued to rise so long as the infall
of matter caused appreciable compression. In the same way, heat was
generated progressively in the less central parts, and these parts also
received the heat that passed out from beneath. It is assumed under this
Page 653
hypothesis that the degree of interior compression stands in close relation to
interior density, for while there would probably be some segregation of
heavier matter toward the center and of lighter toward the surface by means
of volcanic action and internal rearrangement under stress differences, the
interior density is regarded as due mainly to compression. The distribution
of internal pressure and density generally accepted is that of Laplace, who
assumed that the increase of the density varies as the square root of the
increase of the pressure. This law gives a distribution of density that
accords fairly well with the phenomena of precession of the equinoxes,
which require that the higher densities of the interior shall be distributed in
certain proportions between the center and the equatorial protuberance
whose attraction by the sun and moon causes precession. The increases in
pressure, density, and temperature have been computed as follows by Mr. A.
C. Lunn,[255] the average specific gravity of the earth being taken at 5.6, the
surface specific gravity at 2.8, and the specific heat at .2.
The temperatures are shown graphically in Fig. 452, in which the curves
of pressure and density are also given. The nature of the curve of
temperature is such that, if the thermometric conductivity of the material is
uniform at all depths, the temperature will fall in the deeper portions and
rise in the outer ones, excluding the surface portions subject to outside
cooling. The curve indicates that the rising temperature would affect
somewhat more than 800 miles of the outer part of the spheroid, or about
half its volume, i.e. the inner half during the initial period had a falling
temperature and the outer half, except the immediate surface, a rising
temperature. This introduces a very singular feature into the problem, for
the outer zone must shrink to fit the inner portion that is losing heat, while
its own material is expanding because of its increase of temperature. A
double distortional effect must result.[256] If the conductivity of the dense
interior is greater than that of the outer parts, the effect is intensified. The
redistribution of heat resulting from this unequal flowage would in time
change the curve so that more nearly equal flowage would result. It would
probably take a very long period for this to be effected, on account of the
very slow conductivity of rock.
The accretion hypothesis assumes that, during the growth of the earth,
large amounts of heat were carried by volcanic action from deeper horizons
to higher ones and to the surface, and that this still continues at a
interior density, for while there would probably be some segregation of
heavier matter toward the center and of lighter toward the surface by means
of volcanic action and internal rearrangement under stress differences, the
interior density is regarded as due mainly to compression. The distribution
of internal pressure and density generally accepted is that of Laplace, who
assumed that the increase of the density varies as the square root of the
increase of the pressure. This law gives a distribution of density that
accords fairly well with the phenomena of precession of the equinoxes,
which require that the higher densities of the interior shall be distributed in
certain proportions between the center and the equatorial protuberance
whose attraction by the sun and moon causes precession. The increases in
pressure, density, and temperature have been computed as follows by Mr. A.
C. Lunn,[255] the average specific gravity of the earth being taken at 5.6, the
surface specific gravity at 2.8, and the specific heat at .2.
The temperatures are shown graphically in Fig. 452, in which the curves
of pressure and density are also given. The nature of the curve of
temperature is such that, if the thermometric conductivity of the material is
uniform at all depths, the temperature will fall in the deeper portions and
rise in the outer ones, excluding the surface portions subject to outside
cooling. The curve indicates that the rising temperature would affect
somewhat more than 800 miles of the outer part of the spheroid, or about
half its volume, i.e. the inner half during the initial period had a falling
temperature and the outer half, except the immediate surface, a rising
temperature. This introduces a very singular feature into the problem, for
the outer zone must shrink to fit the inner portion that is losing heat, while
its own material is expanding because of its increase of temperature. A
double distortional effect must result.[256] If the conductivity of the dense
interior is greater than that of the outer parts, the effect is intensified. The
redistribution of heat resulting from this unequal flowage would in time
change the curve so that more nearly equal flowage would result. It would
probably take a very long period for this to be effected, on account of the
very slow conductivity of rock.
The accretion hypothesis assumes that, during the growth of the earth,
large amounts of heat were carried by volcanic action from deeper horizons
to higher ones and to the surface, and that this still continues at a
Page 654
diminished rate. It assumes that whenever the interior heat raised any
constituent of the interior matter above its fusing-point under the local
pressure, it passed into the liquid state, and was forced outwards by the
stress differences to which it was subjected, unless its specific gravity was
sufficiently high to counterbalance them. It is conceived that the more
fusible portions were liquefied first, and that in so doing they absorbed the
necessary heat of liquefaction and began to work their way outward,
carrying their heat into higher horizons and temporarily checking the
development of more intense stresses in the lower horizons. They thus
served to keep the temperature there below the fusion-point of the
remaining more refractory substances. Meanwhile the extruded portions
were raising the temperatures of the higher horizons into which they were
intruded or through which they were forced to pass. There was thus, it is
thought, an automatic action that tended to reduce the heat-curve to the
fusion-curve. The actual curve of internal temperature may, therefore, be
practically the fusion-curve. This is identical with the curve supposed to
arise from solidification by pressure from the center outward under the
molten hypothesis, except so far as the two would vary as the result of
variations in the distribution of matter, which would not be quite the same
under the two hypotheses. The curve of fusion deduced by an extension of
the results of Barus’ experiment has been given. It is necessary to recognize
that the rate of rise of the fusion-point may, and very likely does, change in
the deep interior. The curve given represents much higher temperatures in
the central parts than those given by Lunn’s computations from
compression, which seem inherently more probable than the higher ones.
constituent of the interior matter above its fusing-point under the local
pressure, it passed into the liquid state, and was forced outwards by the
stress differences to which it was subjected, unless its specific gravity was
sufficiently high to counterbalance them. It is conceived that the more
fusible portions were liquefied first, and that in so doing they absorbed the
necessary heat of liquefaction and began to work their way outward,
carrying their heat into higher horizons and temporarily checking the
development of more intense stresses in the lower horizons. They thus
served to keep the temperature there below the fusion-point of the
remaining more refractory substances. Meanwhile the extruded portions
were raising the temperatures of the higher horizons into which they were
intruded or through which they were forced to pass. There was thus, it is
thought, an automatic action that tended to reduce the heat-curve to the
fusion-curve. The actual curve of internal temperature may, therefore, be
practically the fusion-curve. This is identical with the curve supposed to
arise from solidification by pressure from the center outward under the
molten hypothesis, except so far as the two would vary as the result of
variations in the distribution of matter, which would not be quite the same
under the two hypotheses. The curve of fusion deduced by an extension of
the results of Barus’ experiment has been given. It is necessary to recognize
that the rate of rise of the fusion-point may, and very likely does, change in
the deep interior. The curve given represents much higher temperatures in
the central parts than those given by Lunn’s computations from
compression, which seem inherently more probable than the higher ones.
Page 655
Fig. 452.—Diagram illustrating the distribution of temperature under the accretion
hypothesis (neglecting the heat from infall and other external sources). The divisions of
the base-line represent fractions of the earth’s radius. The vertical divisions represent
both pressure in megadynes per sq. cm., nearly the same as atmospheres per sq. in., at
the left, and temperatures in degrees C. at the right. It is to be noted that the temperature
scale is 2000° C. per division, while that of Fig. 451 is 5000° C. per division. The upper
curve at the left, PC, is the pressure curve. The middle curve, DC, is the density curve,
beginning at 2.8 at the surface and reaching nearly 11 at the center. The lower curve, TC,
is the temperature curve, rising from the surface temperature, 0° C., at the right, to
20,000° C. at the center. It is to be noted that the portion of this curve at the left
representing the deeper part of the earth is convex upwards, while the portion at the
right is concave. It will be seen that the gradient increases from the center to a point
between .6 and .7 radius, and then decreases, and that between .8 radius and the surface,
a distance of about 800 miles, the decrease is notable. This means that with an equal
coefficient of conductivity the flow from the center outward to .6 or .7 radius will be
faster than the flow from .8 radius to the surface, neglecting the immediate surface
effects of external cooling. These curves were worked out by Mr. Lunn.
As astronomical and seismic evidences strongly favor the view that the
earth is rigid throughout, they lend support to the view that the interior
retains its rigidity by the extrusion of liquid matter practically as fast as it is
formed, and that this progressive extrusion adjusts the temperature to that
which is consistent with solidity.
hypothesis (neglecting the heat from infall and other external sources). The divisions of
the base-line represent fractions of the earth’s radius. The vertical divisions represent
both pressure in megadynes per sq. cm., nearly the same as atmospheres per sq. in., at
the left, and temperatures in degrees C. at the right. It is to be noted that the temperature
scale is 2000° C. per division, while that of Fig. 451 is 5000° C. per division. The upper
curve at the left, PC, is the pressure curve. The middle curve, DC, is the density curve,
beginning at 2.8 at the surface and reaching nearly 11 at the center. The lower curve, TC,
is the temperature curve, rising from the surface temperature, 0° C., at the right, to
20,000° C. at the center. It is to be noted that the portion of this curve at the left
representing the deeper part of the earth is convex upwards, while the portion at the
right is concave. It will be seen that the gradient increases from the center to a point
between .6 and .7 radius, and then decreases, and that between .8 radius and the surface,
a distance of about 800 miles, the decrease is notable. This means that with an equal
coefficient of conductivity the flow from the center outward to .6 or .7 radius will be
faster than the flow from .8 radius to the surface, neglecting the immediate surface
effects of external cooling. These curves were worked out by Mr. Lunn.
As astronomical and seismic evidences strongly favor the view that the
earth is rigid throughout, they lend support to the view that the interior
retains its rigidity by the extrusion of liquid matter practically as fast as it is
formed, and that this progressive extrusion adjusts the temperature to that
which is consistent with solidity.
Page 656
The bearing of this conception becomes evident on consideration. The
shrinkage of the earth from loss of heat by conduction and by the extrusion
of molten rock, affects the deep interior as well as the more superficial
zones. It is even possible that the shrinkage may originate chiefly in the
deeper zones. The postulated transfer of fluid rock from the deeper parts to
the more superficial ones lessens the heat in the former, and adds to that in
the latter. The postulated greater flow of heat from the deeper half to the
outer half, than from the latter outward, gives a concordant result. If the
conductivity of the deeper and denser material is appreciably greater than
that of the more superficial and less dense material, as seems probable, this
effect is intensified. The distribution of compressibility at the existing state
of condensation may possibly be such that more new heat is generated by
shrinkage in the outer parts than in the inner. Neither of these conceptions
can be affirmed as actually taking place. They merely lie within the range of
reasonable hypothesis in the present state of experimental data. What the
real truth is must be left to further research. Present effort may be regarded
as temporarily successful if it forms consistent conceptions of the
applicable hypotheses, and of their consequences.
Recombination of material.—One other peculiarity of the accretion
hypothesis must be recalled here. The incoming bodies must probably be
assumed to have fallen in promiscuous order, and hence to have been
indiscriminately mingled in the growing earth. As they became buried
deeper and deeper and their temperatures and pressures were raised, much
recombination, chemical and physical, may be presumed to have followed.
As already noted, these changes would probably give increased density in
the main. The material being, however, in a solid state, the rearrangement
would be slow and its persistence in time indeterminate, and it may yet be
far from complete. It is not improbable, therefore, under this hypothesis,
that some notable part of the recent shrinkage of the earth has been due to
the continued rearrangement of its heterogeneous internal matter. This
would not be equally so in an earth derived from a molten mass, for the
required adjustments of the material should have taken place while in the
fluid state before solidification.
Comparison of the hypotheses.—By comparing the three hypotheses of
the early states of the earth’s temperature, it will be seen that there is a
radical difference, thermally, between the first and the last two. The first
shrinkage of the earth from loss of heat by conduction and by the extrusion
of molten rock, affects the deep interior as well as the more superficial
zones. It is even possible that the shrinkage may originate chiefly in the
deeper zones. The postulated transfer of fluid rock from the deeper parts to
the more superficial ones lessens the heat in the former, and adds to that in
the latter. The postulated greater flow of heat from the deeper half to the
outer half, than from the latter outward, gives a concordant result. If the
conductivity of the deeper and denser material is appreciably greater than
that of the more superficial and less dense material, as seems probable, this
effect is intensified. The distribution of compressibility at the existing state
of condensation may possibly be such that more new heat is generated by
shrinkage in the outer parts than in the inner. Neither of these conceptions
can be affirmed as actually taking place. They merely lie within the range of
reasonable hypothesis in the present state of experimental data. What the
real truth is must be left to further research. Present effort may be regarded
as temporarily successful if it forms consistent conceptions of the
applicable hypotheses, and of their consequences.
Recombination of material.—One other peculiarity of the accretion
hypothesis must be recalled here. The incoming bodies must probably be
assumed to have fallen in promiscuous order, and hence to have been
indiscriminately mingled in the growing earth. As they became buried
deeper and deeper and their temperatures and pressures were raised, much
recombination, chemical and physical, may be presumed to have followed.
As already noted, these changes would probably give increased density in
the main. The material being, however, in a solid state, the rearrangement
would be slow and its persistence in time indeterminate, and it may yet be
far from complete. It is not improbable, therefore, under this hypothesis,
that some notable part of the recent shrinkage of the earth has been due to
the continued rearrangement of its heterogeneous internal matter. This
would not be equally so in an earth derived from a molten mass, for the
required adjustments of the material should have taken place while in the
fluid state before solidification.
Comparison of the hypotheses.—By comparing the three hypotheses of
the early states of the earth’s temperature, it will be seen that there is a
radical difference, thermally, between the first and the last two. The first
Page 657
assumes a nearly uniform distribution of internal temperature, and hence,
owing to the exceedingly slow rate of conduction, limits the movements
and deformations of the crust, so far as dependent on heat, to very
superficial horizons. The second and third views agree in postulating
changes of temperature in the deep portions, as well as in the superficial,
and hence involve the central portion of the earth in the great movements
and deformations. It is not to be supposed that this of itself necessarily
increases the sum-total of the effects of contraction, for, given a certain loss
of heat from the surface, it may be relatively immaterial whether this loss
arose from a large reduction of temperature in a shallow zone, or a small
reduction of temperature in a deep zone, for, except as the coefficient of
expansion varies, the total shrinkage would be the same. But the difference
in distribution makes a radical difference in the resulting movements, for, in
the first case, the movements are in a weak superficial shell that cannot
accumulate great stresses, and hence must yield practically as fast as the
stresses arise, while, in the second case, the stress-accumulating power of
the thick segments may be great, and the stresses may gather for long
periods and give rise to great cumulative results at long intervals. In this
respect the last two views have much in common, though they differ in
other important particulars.
With this general background of hypothesis, we may now turn to the
direct evidences of the distribution of internal temperature which
observations near the surface afford. Unfortunately they are limited to a
mere film, as it were, little more than ¹⁄₄₀₀₀ of the radius of the earth.
OBSERVED TEMPERATURES IN EXCAVATIONS.
As the earth is penetrated below the zone of seasonal changes by wells,
mines, tunnels, and other excavations, the temperature is almost invariably
found to rise. The rate of rise, however, is far from uniform. If we set aside
as exceptional the unusually rapid rise near volcanoes and in other localities
of obvious igneous influence, the highest rates are still six times the lowest.
A large number of records have been collated by the Committee on
Underground Temperatures, of the British Association for the Advancement
of Science. These range from 1° F. in less than 20 feet to 1° F. in 130 feet,
with an average of 1° F. in 50 to 60 feet, which has usually been taken as
owing to the exceedingly slow rate of conduction, limits the movements
and deformations of the crust, so far as dependent on heat, to very
superficial horizons. The second and third views agree in postulating
changes of temperature in the deep portions, as well as in the superficial,
and hence involve the central portion of the earth in the great movements
and deformations. It is not to be supposed that this of itself necessarily
increases the sum-total of the effects of contraction, for, given a certain loss
of heat from the surface, it may be relatively immaterial whether this loss
arose from a large reduction of temperature in a shallow zone, or a small
reduction of temperature in a deep zone, for, except as the coefficient of
expansion varies, the total shrinkage would be the same. But the difference
in distribution makes a radical difference in the resulting movements, for, in
the first case, the movements are in a weak superficial shell that cannot
accumulate great stresses, and hence must yield practically as fast as the
stresses arise, while, in the second case, the stress-accumulating power of
the thick segments may be great, and the stresses may gather for long
periods and give rise to great cumulative results at long intervals. In this
respect the last two views have much in common, though they differ in
other important particulars.
With this general background of hypothesis, we may now turn to the
direct evidences of the distribution of internal temperature which
observations near the surface afford. Unfortunately they are limited to a
mere film, as it were, little more than ¹⁄₄₀₀₀ of the radius of the earth.
OBSERVED TEMPERATURES IN EXCAVATIONS.
As the earth is penetrated below the zone of seasonal changes by wells,
mines, tunnels, and other excavations, the temperature is almost invariably
found to rise. The rate of rise, however, is far from uniform. If we set aside
as exceptional the unusually rapid rise near volcanoes and in other localities
of obvious igneous influence, the highest rates are still six times the lowest.
A large number of records have been collated by the Committee on
Underground Temperatures, of the British Association for the Advancement
of Science. These range from 1° F. in less than 20 feet to 1° F. in 130 feet,
with an average of 1° F. in 50 to 60 feet, which has usually been taken as
Page 658
representative. The more recent deep borings that have been carefully
measured with due regard to sources of error indicate a slower rate of rise.
Some of the more notable records are as follows:[257]
Depth. Rate of rise.
Sperenberg bore (Germany) 3492 feet. 1° F. in 51.5 feet.
Schladeback bore (Germany) 5630 “ 1° F. in 67.1 “
Cremorne bore (N. S. Wales) 2929 “ 1° F. in 80 “
Paruschowitz bore (Upper Silesia) 6408 “ 1° F. in 62.2 “
Wheeling well (W. Va.) 4462 “ 1° F. in 74.1 “
St. Gothard tunnel (Italy-Switzerland) 5578 “ 1° F. in 82 “
Mt. Cenis tunnel (France-Italy) 5280 “ 1° F. in 79 “
Tamarack mine (N. Mich.) 4450 “ 1° F. in 100 “[257]
Calumet and Hecla mine (N. Mich.) 4939 “ 1° F. in 103 “[257]
Ditto, between 3324 feet and 4837 feet 1° F. in 93.4 “
It is to be noted that even these selected records vary a hundred per cent.
Very notable variations are found in the same mine or well, and often much
difference is found in adjacent records, especially those of artesian wells.
Some of these are explainable, but the full meaning of other variations is
yet to be found.
Explanations of varying increment.—Certain apparent variations are
merely due to inequalities of topography. The isogeotherms, or planes of
equal underground temperature, do not normally rise and fall with every
local irregularity of the surface, but more nearly strike an average. A well
on a bluff 500 feet high would probably reach nearly the same temperature
at 1000 feet, as a well 500 feet deep in the adjacent valley, giving a gradient
twice as great in the one case as in the other.
In interpreting the temperatures of artesian flows, regard must be had to
the depths of rock under which the waters have passed, as well as the
depths at the location of the wells. Darton has found[258] unusually high and
varying temperatures in the artesian wells of the Dakotas, some part of
which may be due to this cause, though a full explanation of their singular
variations is not yet reached.
The permeation and circulation of water affect the temperature in two
important ways: (1) wet rocks are better conductors than dry ones, and (2)
the convective movement of water is a means of conveying heat from lower
to higher horizons. As the circulation of underground water is very unequal,
measured with due regard to sources of error indicate a slower rate of rise.
Some of the more notable records are as follows:[257]
Depth. Rate of rise.
Sperenberg bore (Germany) 3492 feet. 1° F. in 51.5 feet.
Schladeback bore (Germany) 5630 “ 1° F. in 67.1 “
Cremorne bore (N. S. Wales) 2929 “ 1° F. in 80 “
Paruschowitz bore (Upper Silesia) 6408 “ 1° F. in 62.2 “
Wheeling well (W. Va.) 4462 “ 1° F. in 74.1 “
St. Gothard tunnel (Italy-Switzerland) 5578 “ 1° F. in 82 “
Mt. Cenis tunnel (France-Italy) 5280 “ 1° F. in 79 “
Tamarack mine (N. Mich.) 4450 “ 1° F. in 100 “[257]
Calumet and Hecla mine (N. Mich.) 4939 “ 1° F. in 103 “[257]
Ditto, between 3324 feet and 4837 feet 1° F. in 93.4 “
It is to be noted that even these selected records vary a hundred per cent.
Very notable variations are found in the same mine or well, and often much
difference is found in adjacent records, especially those of artesian wells.
Some of these are explainable, but the full meaning of other variations is
yet to be found.
Explanations of varying increment.—Certain apparent variations are
merely due to inequalities of topography. The isogeotherms, or planes of
equal underground temperature, do not normally rise and fall with every
local irregularity of the surface, but more nearly strike an average. A well
on a bluff 500 feet high would probably reach nearly the same temperature
at 1000 feet, as a well 500 feet deep in the adjacent valley, giving a gradient
twice as great in the one case as in the other.
In interpreting the temperatures of artesian flows, regard must be had to
the depths of rock under which the waters have passed, as well as the
depths at the location of the wells. Darton has found[258] unusually high and
varying temperatures in the artesian wells of the Dakotas, some part of
which may be due to this cause, though a full explanation of their singular
variations is not yet reached.
The permeation and circulation of water affect the temperature in two
important ways: (1) wet rocks are better conductors than dry ones, and (2)
the convective movement of water is a means of conveying heat from lower
to higher horizons. As the circulation of underground water is very unequal,
Page 659
much irregularity of thermal distribution in the upper zones probably arises
from this source. The general effect of water circulation is to reduce the
thermal gradient where the circulation is relatively rapid, as it is near the
surface and in the main thoroughfares of circulation, and hence to cause a
relatively rapid rise in the gradient just below the zone of effective water
influence. Some records conform to this theoretical deduction, but in
general it is masked by other influences.
Chemical action, especially oxidation, carbonation, hydration, solution,
and precipitation, modify the normal temperature gradient, but how
effectively is not well determined. With little doubt the first three mentioned
above raise the temperature, while solution and precipitation in some large
measure offset each other.[259] The sum-total is probably an appreciable rise
in temperature. It has even been conjectured that the heat of volcanic action
is due to chemical combination in the lower reaches of water circulation,
but this is obviously an over-estimate.
Differences in the conductivity of rock are an obvious source of
varying underground temperature gradients. If an outer formation conducts
heat more freely than those below, it tends to lower the gradient within
itself and to cause a relative rise in the gradient just below. If a lower
formation is more conductive than that above, it tends to lower the gradient
within itself, and to raise it in the one above, because it carries heat to the
outer one faster than the latter carries it away.
The compression to which rocks have been subjected affects their
temperature. At the surface the variation from this source is chiefly
dependent on the lateral thrust suffered.
When allowances are made for all these and other known causes of local
variation of temperature, it is still not clear that a uniform average gradient
remains as the true conception. If the earth were once a molten spheroid,
there would be a strong presumption that, aside from local variations, there
would be a normal curve applicable to all regions. On the other hand, if the
internal heat has arisen chiefly from compression, and if the compression
has varied in different regions, as the inequalities of the surface render
probable, there would be no such definite normal curve in the accessible
zone of the earth, but rather a varying rate in different regions. In either
from this source. The general effect of water circulation is to reduce the
thermal gradient where the circulation is relatively rapid, as it is near the
surface and in the main thoroughfares of circulation, and hence to cause a
relatively rapid rise in the gradient just below the zone of effective water
influence. Some records conform to this theoretical deduction, but in
general it is masked by other influences.
Chemical action, especially oxidation, carbonation, hydration, solution,
and precipitation, modify the normal temperature gradient, but how
effectively is not well determined. With little doubt the first three mentioned
above raise the temperature, while solution and precipitation in some large
measure offset each other.[259] The sum-total is probably an appreciable rise
in temperature. It has even been conjectured that the heat of volcanic action
is due to chemical combination in the lower reaches of water circulation,
but this is obviously an over-estimate.
Differences in the conductivity of rock are an obvious source of
varying underground temperature gradients. If an outer formation conducts
heat more freely than those below, it tends to lower the gradient within
itself and to cause a relative rise in the gradient just below. If a lower
formation is more conductive than that above, it tends to lower the gradient
within itself, and to raise it in the one above, because it carries heat to the
outer one faster than the latter carries it away.
The compression to which rocks have been subjected affects their
temperature. At the surface the variation from this source is chiefly
dependent on the lateral thrust suffered.
When allowances are made for all these and other known causes of local
variation of temperature, it is still not clear that a uniform average gradient
remains as the true conception. If the earth were once a molten spheroid,
there would be a strong presumption that, aside from local variations, there
would be a normal curve applicable to all regions. On the other hand, if the
internal heat has arisen chiefly from compression, and if the compression
has varied in different regions, as the inequalities of the surface render
probable, there would be no such definite normal curve in the accessible
zone of the earth, but rather a varying rate in different regions. In either
Page 660
case, the later movements, compressions and strains of the crust, must
modify the original thermal gradients.
Gradients projected.—It is not probable that these gradients, even when
corrected for local variations, continue unmodified to the center of the
earth. If they did, 1° F. in 60 feet continued to the earth’s center would give
348,000° F., and 1° F. in 100 feet would give 209,000° F. It is much more
probable that the rates of rise fall away below the superficial zone. If water
circulation in the fracture zone is the most efficient agency cooperating with
conductivity in the outward conveyance of heat, as seems probable, the
gradient in that zone should rise at an abnormal rate, and hence the average
gradient in the deeper portions not affected by this circulation should be
lower. It will be recalled that the central temperature deduced from an
extension of Barus’ fusion curve is 136,800° F. (76,000° C.), which, high as
it is, gives a lower average gradient than the surface observations. The
computations from compression by Lunn, giving a central temperature of
36,000° F. (20,000° C.), imply a still lower average rate, while the
convection hypothesis postulates no sensible increase at all below 200 or
300 miles.
Average material of Mineral
Norm minerals
crust (Clarke’s tables). equivalent Linear Volume
calculated from Axis.
[260] (C.I.P.W. expansion. expansion.
Clarke’s average.
system).
SiO2 58.59 Quartz 11.4 Quartz +.00001206 .00003618
Al2O3 15.04 Orthoclase 17.2 a +.00001906
Fe2O3 3.94 Albite 27.3 Anorthite b −.000002035
FeO 3.48 Anorthite 17.8 c −.000001495 .00001553
CaO 5.29 Diopside 6.8 a +.000008125
MgO 4.49 Hypersthene 10.2 Diopside b +.000016963 .0000234
K2O 2.90 Magnetite and c −.000001707
Na2O 3.20 Ilmenite 6.8 Augite a +.000013856
TiO2 .55 Minor (used for
constituents hypersthene)
Minor
constituents omitted 2.5
omitted ——— b +.00000272 .0000245
2.52 100.00 Magnetite c +.00000791
——— +.000009540 .00002862
100.00
The amount of loss of heat.—The amount of loss of interior heat which
the earth suffers may be estimated by that which is observed to be passing
modify the original thermal gradients.
Gradients projected.—It is not probable that these gradients, even when
corrected for local variations, continue unmodified to the center of the
earth. If they did, 1° F. in 60 feet continued to the earth’s center would give
348,000° F., and 1° F. in 100 feet would give 209,000° F. It is much more
probable that the rates of rise fall away below the superficial zone. If water
circulation in the fracture zone is the most efficient agency cooperating with
conductivity in the outward conveyance of heat, as seems probable, the
gradient in that zone should rise at an abnormal rate, and hence the average
gradient in the deeper portions not affected by this circulation should be
lower. It will be recalled that the central temperature deduced from an
extension of Barus’ fusion curve is 136,800° F. (76,000° C.), which, high as
it is, gives a lower average gradient than the surface observations. The
computations from compression by Lunn, giving a central temperature of
36,000° F. (20,000° C.), imply a still lower average rate, while the
convection hypothesis postulates no sensible increase at all below 200 or
300 miles.
Average material of Mineral
Norm minerals
crust (Clarke’s tables). equivalent Linear Volume
calculated from Axis.
[260] (C.I.P.W. expansion. expansion.
Clarke’s average.
system).
SiO2 58.59 Quartz 11.4 Quartz +.00001206 .00003618
Al2O3 15.04 Orthoclase 17.2 a +.00001906
Fe2O3 3.94 Albite 27.3 Anorthite b −.000002035
FeO 3.48 Anorthite 17.8 c −.000001495 .00001553
CaO 5.29 Diopside 6.8 a +.000008125
MgO 4.49 Hypersthene 10.2 Diopside b +.000016963 .0000234
K2O 2.90 Magnetite and c −.000001707
Na2O 3.20 Ilmenite 6.8 Augite a +.000013856
TiO2 .55 Minor (used for
constituents hypersthene)
Minor
constituents omitted 2.5
omitted ——— b +.00000272 .0000245
2.52 100.00 Magnetite c +.00000791
——— +.000009540 .00002862
100.00
The amount of loss of heat.—The amount of loss of interior heat which
the earth suffers may be estimated by that which is observed to be passing
Page 661
outward through the rock, or by computing the amount which should be
conveyed outwards with the estimated gradients and with the conductivity
of rock as determined by experiment. The latter method is usually employed
in general problems. Taking the mean thermometric conductivity of rock as
0.0045, the gradient as 1° C. in 30 meters, the average specific heat of rock
as 0.5 small calories per cubic centimeter, it is computed that in
100,000,000 years the loss of heat would amount to 45° C. (81° F.) for the
whole body of the earth.[261] Tait makes the more conservative estimate of
10° C. (18° F.) in the same period.[262] This is an exceedingly small result,
and emphasizes the low conductivity of rock.
The amount of shrinkage from loss of heat.—To compute the amount
of shrinkage for a given amount of cooling, the average coefficient of
expansion of rock is required. This has been experimentally determined by
several investigators. By combining the determinations of others with his
own, T. Mellard Reade found the linear coefficient to be .000005257 per 1°
F., equivalent to .00002838 per 1° C. per volume. In this the proportions of
the different rocks in the crust were roughly estimated. To secure an
independent result from the best available estimate of what constitutes the
average rock, W. H. Emmons has reduced Clarke’s average of the chemical
constituents of the crust to the norm minerals under the new system of
Cross, Iddings, Pirsson, and Washington (see p. 454) and made a weighted
average of the conductivities of these, as shown in the following table:
Volume
Percentages Volume
Sp. Gr. of proportions
of norm proportions
norm minerals. of temp.
minerals. of norm minerals.
1° C. higher.
Quartz 11.4 2.66 4.28 4.2801548504
Feldspars[263] 62.3 2.7 23.07 23.0703582771
Diopside 6.8 3.3 2.06 2.0600482040
Hypersthene 10.2 3.45 2.95 2.9500722750
Magnetite 6.8 5.17 1.3 1.3000372060
—— ——— ———————
Total 97.5 33.66 33.6606708125
Subtracting the stated volume from the volume at a temperature of 1° C.
higher, the difference is found to be .0006708125, which divided by the
volume gives .0000199, which is the coefficient of expansion of the
theoretical, average, surface rock of the earth.
conveyed outwards with the estimated gradients and with the conductivity
of rock as determined by experiment. The latter method is usually employed
in general problems. Taking the mean thermometric conductivity of rock as
0.0045, the gradient as 1° C. in 30 meters, the average specific heat of rock
as 0.5 small calories per cubic centimeter, it is computed that in
100,000,000 years the loss of heat would amount to 45° C. (81° F.) for the
whole body of the earth.[261] Tait makes the more conservative estimate of
10° C. (18° F.) in the same period.[262] This is an exceedingly small result,
and emphasizes the low conductivity of rock.
The amount of shrinkage from loss of heat.—To compute the amount
of shrinkage for a given amount of cooling, the average coefficient of
expansion of rock is required. This has been experimentally determined by
several investigators. By combining the determinations of others with his
own, T. Mellard Reade found the linear coefficient to be .000005257 per 1°
F., equivalent to .00002838 per 1° C. per volume. In this the proportions of
the different rocks in the crust were roughly estimated. To secure an
independent result from the best available estimate of what constitutes the
average rock, W. H. Emmons has reduced Clarke’s average of the chemical
constituents of the crust to the norm minerals under the new system of
Cross, Iddings, Pirsson, and Washington (see p. 454) and made a weighted
average of the conductivities of these, as shown in the following table:
Volume
Percentages Volume
Sp. Gr. of proportions
of norm proportions
norm minerals. of temp.
minerals. of norm minerals.
1° C. higher.
Quartz 11.4 2.66 4.28 4.2801548504
Feldspars[263] 62.3 2.7 23.07 23.0703582771
Diopside 6.8 3.3 2.06 2.0600482040
Hypersthene 10.2 3.45 2.95 2.9500722750
Magnetite 6.8 5.17 1.3 1.3000372060
—— ——— ———————
Total 97.5 33.66 33.6606708125
Subtracting the stated volume from the volume at a temperature of 1° C.
higher, the difference is found to be .0006708125, which divided by the
volume gives .0000199, which is the coefficient of expansion of the
theoretical, average, surface rock of the earth.
Page 662
With this coefficient, the radial shrinkage resulting from an average loss
of 10° C. (18° F.), (Tait’s estimate), is a little over a quarter of a mile
(.2572); and for a loss of 45° C. (81° F.), (estimate of Daniell’s Physics), a
little over a mile (1.1574). The shortening of the circumference for 10° C.
loss is 1.6 miles, and for 45° C., 7.27 miles. Computations based on the
coefficient of expansion adopted by Reade give 2.35 miles circumferential
shortening for a loss of 10° C. and 10.5 miles for a loss of 45° C. In both
these cases, the whole contraction is assumed to take a vertical direction,
and hence these are maximum results. They are exceedingly small.
Unless there is a very serious error in the estimated rate of thermal loss,
or in the coefficients of expansion, cooling would seem to be a very
inadequate cause for the shrinkage which the mountain foldings, overthrust
faults, and other deformations imply. This inadequacy has been strongly
urged by Fisher[264] and by Dutton.[265] In view of the apparent incompetency
of external loss of heat, the possibilities of distortion from other causes
invite consideration.
OTHER SOURCES OF DEFORMATION.
Transfer of internal heat.—It is theoretically possible that deformation
of the subcrust may result from the internal transfer of heat without regard
to external loss. It has already been shown (p. 539) that under certain
possible conditions more heat would flow from the inner parts to higher
horizons than would be conveyed through these latter to the surface and
there lost, and that, as a result, the temperatures of the inner parts might be
falling, while those of the outer parts (except the surface) might be rising.
With the more conservative coefficient of expansion previously given, a
lowering of the average temperature of the inner half of the earth 500° C.
and the raising, by transfer, of the outer half to an equal amount would give
a lateral thrust of about 83 miles, which is about the order of magnitude
thought to be needed. It is not affirmed that this takes place, but some
transfer of this kind is among the theoretical possibilities under the
accretion hypothesis. The process could not continue indefinitely; but, for
aught that can now be affirmed, it may still be in progress.
Denser aggregation of matter.—As already noted, matter under intense
pressure tends to aggregate itself in the forms that give the greatest density.
of 10° C. (18° F.), (Tait’s estimate), is a little over a quarter of a mile
(.2572); and for a loss of 45° C. (81° F.), (estimate of Daniell’s Physics), a
little over a mile (1.1574). The shortening of the circumference for 10° C.
loss is 1.6 miles, and for 45° C., 7.27 miles. Computations based on the
coefficient of expansion adopted by Reade give 2.35 miles circumferential
shortening for a loss of 10° C. and 10.5 miles for a loss of 45° C. In both
these cases, the whole contraction is assumed to take a vertical direction,
and hence these are maximum results. They are exceedingly small.
Unless there is a very serious error in the estimated rate of thermal loss,
or in the coefficients of expansion, cooling would seem to be a very
inadequate cause for the shrinkage which the mountain foldings, overthrust
faults, and other deformations imply. This inadequacy has been strongly
urged by Fisher[264] and by Dutton.[265] In view of the apparent incompetency
of external loss of heat, the possibilities of distortion from other causes
invite consideration.
OTHER SOURCES OF DEFORMATION.
Transfer of internal heat.—It is theoretically possible that deformation
of the subcrust may result from the internal transfer of heat without regard
to external loss. It has already been shown (p. 539) that under certain
possible conditions more heat would flow from the inner parts to higher
horizons than would be conveyed through these latter to the surface and
there lost, and that, as a result, the temperatures of the inner parts might be
falling, while those of the outer parts (except the surface) might be rising.
With the more conservative coefficient of expansion previously given, a
lowering of the average temperature of the inner half of the earth 500° C.
and the raising, by transfer, of the outer half to an equal amount would give
a lateral thrust of about 83 miles, which is about the order of magnitude
thought to be needed. It is not affirmed that this takes place, but some
transfer of this kind is among the theoretical possibilities under the
accretion hypothesis. The process could not continue indefinitely; but, for
aught that can now be affirmed, it may still be in progress.
Denser aggregation of matter.—As already noted, matter under intense
pressure tends to aggregate itself in the forms that give the greatest density.
Page 663
If the earth were built up of heterogeneous matter arranged at haphazard,
the material would probably readjust itself more or less, as time went on,
into combinations of greater and greater density. This process may be one
of the important sources of shrinkage, for an average change of density of 1
percent., affecting the matter of the whole globe, would probably meet all
the demands of deformation since the beginning of the Paleozoic period.
Extravasation of lavas.—It is obvious that if lavas are forced out from
beneath the crust and spread upon it, a compensating sinking of the crust
will follow. This, however, is rather a mode than an ulterior cause, for a
cause must be found for the extrusion of the lavas, and this cause may be
one of the other agencies recognized, such as a transfer of heat, a
reorganization of matter, or a change of pressure. The more practical
question, however, relates to its competency. Can the amount of lava that
has been extruded have had any very appreciable effect on the descent of
the crust? The great Deccan flow is credited with an area of 200,000 square
miles, and a thickness of 4000 to 6000 feet. Vast as this is for a lava-flow, it
would form a layer only about 5 feet thick when spread over the whole
surface of the globe, and hence the sinking to replace it would cause a
lateral thrust, on any great circle, of about 31 feet only. It requires a very
generous estimate of the lavas poured out between any two great mountain-
making periods since the beginning of the well-known stratigraphic series
to cause a horizontal thrust of any appreciable part of that involved in
mountain-making. The case is different, however, if we go back to the
Archean era, in which the proportion of extrusive and intrusive rocks is
very high. Very notable distortion may then be assigned to the extravasation
of lavas. The outward movement of lava must also be credited with some
transfer of heat from lower to higher horizons, and this is probably one of
the agencies that have produced the relatively high underground
temperatures in the outer part of the earth.
If lavas are thrust into crevices of the crust they contribute to its
extension, but causes for the crevices and for the intrusion must be found,
and these are probably only expressions of one or another of the more
general agencies.
Change in the rate of rotation.—As previously noted, the tide acts as a
brake on the rotation of the earth. The oblateness of the present earth is
accommodated to its present rate of rotation. It is assumed that such
the material would probably readjust itself more or less, as time went on,
into combinations of greater and greater density. This process may be one
of the important sources of shrinkage, for an average change of density of 1
percent., affecting the matter of the whole globe, would probably meet all
the demands of deformation since the beginning of the Paleozoic period.
Extravasation of lavas.—It is obvious that if lavas are forced out from
beneath the crust and spread upon it, a compensating sinking of the crust
will follow. This, however, is rather a mode than an ulterior cause, for a
cause must be found for the extrusion of the lavas, and this cause may be
one of the other agencies recognized, such as a transfer of heat, a
reorganization of matter, or a change of pressure. The more practical
question, however, relates to its competency. Can the amount of lava that
has been extruded have had any very appreciable effect on the descent of
the crust? The great Deccan flow is credited with an area of 200,000 square
miles, and a thickness of 4000 to 6000 feet. Vast as this is for a lava-flow, it
would form a layer only about 5 feet thick when spread over the whole
surface of the globe, and hence the sinking to replace it would cause a
lateral thrust, on any great circle, of about 31 feet only. It requires a very
generous estimate of the lavas poured out between any two great mountain-
making periods since the beginning of the well-known stratigraphic series
to cause a horizontal thrust of any appreciable part of that involved in
mountain-making. The case is different, however, if we go back to the
Archean era, in which the proportion of extrusive and intrusive rocks is
very high. Very notable distortion may then be assigned to the extravasation
of lavas. The outward movement of lava must also be credited with some
transfer of heat from lower to higher horizons, and this is probably one of
the agencies that have produced the relatively high underground
temperatures in the outer part of the earth.
If lavas are thrust into crevices of the crust they contribute to its
extension, but causes for the crevices and for the intrusion must be found,
and these are probably only expressions of one or another of the more
general agencies.
Change in the rate of rotation.—As previously noted, the tide acts as a
brake on the rotation of the earth. The oblateness of the present earth is
accommodated to its present rate of rotation. It is assumed that such
Page 664
accommodation has always obtained, and that if the rotation has changed,
the form of the earth has changed also. Now, the more oblate the spheroid,
the larger its surface shell and the less the total force of gravity. Hence if the
earth’s rotation has diminished, its crust must have shrunk, because the
form of the spheroid has become more compact, and the increase of gravity
has increased its density. There is at present a water-tide chiefly generated
in the southern ocean, and irregularly distributed to more northerly waters.
This irregularity interferes with its systematic action as a brake, and its
average effects are difficult of estimation. The water-tides of past ages are
still more uncertain, as they must have depended on the configuration and
continuity of the oceans. There are geological grounds for the belief that the
southern ocean was interrupted by land during portions of the past at least,
and it is unknown whether there were elsewhere ocean-belts well suited to
the generation of large tides. The ocean-tide, therefore, furnishes a very
uncertain basis for estimating the retardation of rotation.[266] The theoretical
case rests largely on the assumption of an effective body-tide. The earth
doubtless has some body-tide, but whether it is sufficiently great to be
effective, and whether its position, which depends on its promptness in
yielding and in resilience, is favorable to the retardation of rotation, are yet
open questions. The existence of an appreciable body-tide has not yet been
proved by observation.
G. H. Darwin, assuming that the earth is viscous enough to give a body-
tide of appreciable value and of effective position, has deduced a series of
former rates of rotation of the earth and has computed the corresponding
distances of the moon.[267] C. S. Slichter has shown that the lessening of the
area of the surface and the increase of the force of gravity corresponding to
these assigned changes of rotation are large, and that if the changes were
actually experienced they must have involved much distortion of the crust.
[268]
These distortions would, however, be of a peculiar nature, and should
thereby be detectible, if they were realized; for in passing from a more
oblate to a less oblate spheroid, the equatorial belt shrinks, and the polar
tracts rise and become more convex. Wrinkles should, therefore, mark the
equatorial belts, and tension the high latitudes. Slichter has computed that in
a change from a rotation period of 3.82 hours to the present one, the
equatorial belt must shorten 1131 miles and the meridional circles lengthen
495 miles. If we take Heim’s estimate of the crust-shortening involved in
forming the Alps—74 miles—as a standard, the 1131 miles of equatorial
the form of the earth has changed also. Now, the more oblate the spheroid,
the larger its surface shell and the less the total force of gravity. Hence if the
earth’s rotation has diminished, its crust must have shrunk, because the
form of the spheroid has become more compact, and the increase of gravity
has increased its density. There is at present a water-tide chiefly generated
in the southern ocean, and irregularly distributed to more northerly waters.
This irregularity interferes with its systematic action as a brake, and its
average effects are difficult of estimation. The water-tides of past ages are
still more uncertain, as they must have depended on the configuration and
continuity of the oceans. There are geological grounds for the belief that the
southern ocean was interrupted by land during portions of the past at least,
and it is unknown whether there were elsewhere ocean-belts well suited to
the generation of large tides. The ocean-tide, therefore, furnishes a very
uncertain basis for estimating the retardation of rotation.[266] The theoretical
case rests largely on the assumption of an effective body-tide. The earth
doubtless has some body-tide, but whether it is sufficiently great to be
effective, and whether its position, which depends on its promptness in
yielding and in resilience, is favorable to the retardation of rotation, are yet
open questions. The existence of an appreciable body-tide has not yet been
proved by observation.
G. H. Darwin, assuming that the earth is viscous enough to give a body-
tide of appreciable value and of effective position, has deduced a series of
former rates of rotation of the earth and has computed the corresponding
distances of the moon.[267] C. S. Slichter has shown that the lessening of the
area of the surface and the increase of the force of gravity corresponding to
these assigned changes of rotation are large, and that if the changes were
actually experienced they must have involved much distortion of the crust.
[268]
These distortions would, however, be of a peculiar nature, and should
thereby be detectible, if they were realized; for in passing from a more
oblate to a less oblate spheroid, the equatorial belt shrinks, and the polar
tracts rise and become more convex. Wrinkles should, therefore, mark the
equatorial belts, and tension the high latitudes. Slichter has computed that in
a change from a rotation period of 3.82 hours to the present one, the
equatorial belt must shorten 1131 miles and the meridional circles lengthen
495 miles. If we take Heim’s estimate of the crust-shortening involved in
forming the Alps—74 miles—as a standard, the 1131 miles of equatorial
Page 665
shortening would be sufficient for the formation of 15 mountain ranges of
Alpine magnitude. If, as some geologists urge, the estimate of mountain
folding is too great, the quotient would be still larger. These ranges should
run across the equator and be limited to about 33° N. and S. latitude. The
high-latitude tension would be sufficient to cause the earth to gape more
than two hundred miles at the poles, if there were simple ideal shrinkage.
The amounts and the distribution of thrust and shrinkage are shown in Fig.
453. If the change of rotation were no more than from 14 hours to the
present rate, there would still be 52 miles of thrust in the equatorial belt,
and 40 miles of shortage in the meridional circles. There are no clear signs
of such a remarkable distribution of thrust and tension as this hypothesis
requires. Mountains are about as abundant and as strong north of 33°, the
neutral line, as south of it, and they extend to high latitudes. The Archean
rocks, in which this agency should have been most effective because of
their early formation, are crumpled and crushed in the high latitudes much
the same as in low latitudes. Furthermore, if there had been appreciable
change in the form of the earth to accommodate itself to a slower rotation,
the water on the surface, being the most mobile element, should have
gathered toward the poles, and the less mobile solid earth should have
protruded about the equator, but the distribution of land and water, present
and past, gives no clear evidence of this. The equatorial belt contains a less
percentage of land than the area north of it and more than that south of it. It
varies but slightly from the average for the whole globe.
Alpine magnitude. If, as some geologists urge, the estimate of mountain
folding is too great, the quotient would be still larger. These ranges should
run across the equator and be limited to about 33° N. and S. latitude. The
high-latitude tension would be sufficient to cause the earth to gape more
than two hundred miles at the poles, if there were simple ideal shrinkage.
The amounts and the distribution of thrust and shrinkage are shown in Fig.
453. If the change of rotation were no more than from 14 hours to the
present rate, there would still be 52 miles of thrust in the equatorial belt,
and 40 miles of shortage in the meridional circles. There are no clear signs
of such a remarkable distribution of thrust and tension as this hypothesis
requires. Mountains are about as abundant and as strong north of 33°, the
neutral line, as south of it, and they extend to high latitudes. The Archean
rocks, in which this agency should have been most effective because of
their early formation, are crumpled and crushed in the high latitudes much
the same as in low latitudes. Furthermore, if there had been appreciable
change in the form of the earth to accommodate itself to a slower rotation,
the water on the surface, being the most mobile element, should have
gathered toward the poles, and the less mobile solid earth should have
protruded about the equator, but the distribution of land and water, present
and past, gives no clear evidence of this. The equatorial belt contains a less
percentage of land than the area north of it and more than that south of it. It
varies but slightly from the average for the whole globe.
Page 666
Fig. 453.—Polar projection of the earth’s hemisphere showing the theoretical high-latitude
tension and low-latitude compression involved in a change of rotation from 3.82 hours to
the present rate. The figure is drawn to true scale as seen from a point above the pole,
and in consequence the equatorial tract is foreshortened. The black triangles show
compression reduced in length by foreshortening; the white show tension in essentially
true proportions to the high-latitude areas. The neutral line between the areas of
compression and of stretching lies at 33° 20′ latitude.
While the doctrine of tidal retardation is theoretically sound, and while
the relations of the moon to the earth have probably been appreciably
affected by tidal action, geological evidence indicates that it has not been
sufficiently effective in producing crustal deformations to be clearly
detected by its own distinctive results. This may be due (1) to the fact that
there are compensating agencies that tend to acceleration of rotation, and
(2) to the probable fact that the central rigidity of the earth is too high to
give a very effective body-tide. Hence the process of retardation may have
been too slow to have been geologically appreciable in the known period.
The recent estimates of the effective rigidity of the earth are greater than
former ones, and they may need to be modified yet further in the same
direction.
tension and low-latitude compression involved in a change of rotation from 3.82 hours to
the present rate. The figure is drawn to true scale as seen from a point above the pole,
and in consequence the equatorial tract is foreshortened. The black triangles show
compression reduced in length by foreshortening; the white show tension in essentially
true proportions to the high-latitude areas. The neutral line between the areas of
compression and of stretching lies at 33° 20′ latitude.
While the doctrine of tidal retardation is theoretically sound, and while
the relations of the moon to the earth have probably been appreciably
affected by tidal action, geological evidence indicates that it has not been
sufficiently effective in producing crustal deformations to be clearly
detected by its own distinctive results. This may be due (1) to the fact that
there are compensating agencies that tend to acceleration of rotation, and
(2) to the probable fact that the central rigidity of the earth is too high to
give a very effective body-tide. Hence the process of retardation may have
been too slow to have been geologically appreciable in the known period.
The recent estimates of the effective rigidity of the earth are greater than
former ones, and they may need to be modified yet further in the same
direction.
Page 667
Distribution of rigidity.—An important consideration in this connection
is the distribution of interior rigidity. It is certain that the rigidity of the
outermost part, taken as a mass, is somewhat less than that of rock of an
average surface type, for it is fissured, and there is no reason to suppose that
the rigidity of the rock next below the fissure zone rises at once to the
rigidity of steel, and hence if the average rigidity of the whole earth is equal
to that of steel, a portion of the interior must have a rigidity much higher
than steel. There is probably some law of increase from surface to center,
and there are theoretical grounds for thinking that it is in some way
connected with the laws of pressure, density, compressibility, and
temperature. All of these factors probably affect rigidity, but in different
ways. The modulus of rigidity of steel is about 770 × 106 grms. per sq. cm.
Milne and Gray[269] found that of granite to be 128 × 106. The ratio of the
rigidity of steel to that of rock is, therefore, about 6 : 1. If it be assumed that
the rigidity increases in depth directly as the density, the rigidity will
nowhere reach that of steel, being only about two-thirds as much at the
center. If it be assumed that the rigidity increases as the squares of the
density ratios, the following values are obtained:
Distances from
Densities under Density ratios
center in terms Density ratios. Deduced rigidities.
Laplace’s law. squared.
of radius.
1.00 2.8 1 1 0.16 Steel
.75 5.7 2 4 0.6 ”
.50 8.39 3 9 1.5 ”
.25 10.27 3.7 13.7 2.3 ”
.00 10.95 3.9 15.2 2.5 ”
These values seem fairly consistent with the apparent requirements of the
case.
If the distribution of rigidity were of this nature, the average rigidity
would be much less than that of steel, for more than half the volume lies in
the outer division, between 1.00 and .75 radius, and yet the effective
resistance to tidal deformation would be high, for, according to G. H.
Darwin,[270] the tidal stress-differences are eight times as great in the center
as at the surface. The rigidity would, therefore, be distributed so as to be
much more effective in resistance than if it were uniform. The suggestion
arises here that the tidal stresses and other analogous stresses arising from
astronomical sources may be in themselves the causes of some such
is the distribution of interior rigidity. It is certain that the rigidity of the
outermost part, taken as a mass, is somewhat less than that of rock of an
average surface type, for it is fissured, and there is no reason to suppose that
the rigidity of the rock next below the fissure zone rises at once to the
rigidity of steel, and hence if the average rigidity of the whole earth is equal
to that of steel, a portion of the interior must have a rigidity much higher
than steel. There is probably some law of increase from surface to center,
and there are theoretical grounds for thinking that it is in some way
connected with the laws of pressure, density, compressibility, and
temperature. All of these factors probably affect rigidity, but in different
ways. The modulus of rigidity of steel is about 770 × 106 grms. per sq. cm.
Milne and Gray[269] found that of granite to be 128 × 106. The ratio of the
rigidity of steel to that of rock is, therefore, about 6 : 1. If it be assumed that
the rigidity increases in depth directly as the density, the rigidity will
nowhere reach that of steel, being only about two-thirds as much at the
center. If it be assumed that the rigidity increases as the squares of the
density ratios, the following values are obtained:
Distances from
Densities under Density ratios
center in terms Density ratios. Deduced rigidities.
Laplace’s law. squared.
of radius.
1.00 2.8 1 1 0.16 Steel
.75 5.7 2 4 0.6 ”
.50 8.39 3 9 1.5 ”
.25 10.27 3.7 13.7 2.3 ”
.00 10.95 3.9 15.2 2.5 ”
These values seem fairly consistent with the apparent requirements of the
case.
If the distribution of rigidity were of this nature, the average rigidity
would be much less than that of steel, for more than half the volume lies in
the outer division, between 1.00 and .75 radius, and yet the effective
resistance to tidal deformation would be high, for, according to G. H.
Darwin,[270] the tidal stress-differences are eight times as great in the center
as at the surface. The rigidity would, therefore, be distributed so as to be
much more effective in resistance than if it were uniform. The suggestion
arises here that the tidal stresses and other analogous stresses arising from
astronomical sources may be in themselves the causes of some such
Page 668
distribution of rigidity as this. The tidal stresses are rhythmical and give rise
to a kind of kneading of the body of the earth, small in measure to be sure,
but persistent and rapidly recurrent. Since these stress-differences at the
center are eight times those at the surface, and since also the gravitative
stress at the center is 3,000,000 times that at the surface, there is a series of
persistently recurring stress-differences, greatest at the center and declining
outwards, superposed on enormous static stresses, also intensest at the
center and declining outwards. Now, if the earth material were once made
up of a mixture of minerals of different fusibility, some of which became
more mobile (whether fluid or viscous) than others under the rising
temperature of the interior, it seems that the more mobile portion must have
tended to move from the regions of greater stress-differences to those of
lesser stress-differences. The persistence and the rhythmical nature of the
tidal stress-differences seem well suited to aid the mobile parts in gradually
working their way outwards. At the same time the more solid and resistant
portions should remain behind, and thus come to constitute the dominant
material of the central regions where stress-differences were greatest, and
so, as it were, concentrate rigidity there. The process may still be in action.
If it be assumed that the rhythmical stresses have thus developed a
resistance to deformation proportional to their intensity, we may combine
this with density to form the basis of another hypothetical distribution of
rigidity, as follows:
Distances
from Densities
Density Ratios adjusted to stress- Deduced
center in under
ratios. differences. 1:8) rigidities.
terms Laplace’s law.
of radius.
1.00 2.8 1 1 0.16 Steel
.75 5.7 2 3.5 0.58 ”
.50 8.39 3 5.4 0.90 ”
.25 10.27 3.7 7 1.16 ”
.00 10.95 3.9 8 1.33 ”
The average rigidity is here also much less than that of steel, but its
distribution is such as to render it ideally fitted to resist tidal distortion.
These hypothetical distributions of rigidity have no claims to special
value in themselves, for the grounds on which they are based are quite
inadequate, but they are not without importance in giving tangible form to
to a kind of kneading of the body of the earth, small in measure to be sure,
but persistent and rapidly recurrent. Since these stress-differences at the
center are eight times those at the surface, and since also the gravitative
stress at the center is 3,000,000 times that at the surface, there is a series of
persistently recurring stress-differences, greatest at the center and declining
outwards, superposed on enormous static stresses, also intensest at the
center and declining outwards. Now, if the earth material were once made
up of a mixture of minerals of different fusibility, some of which became
more mobile (whether fluid or viscous) than others under the rising
temperature of the interior, it seems that the more mobile portion must have
tended to move from the regions of greater stress-differences to those of
lesser stress-differences. The persistence and the rhythmical nature of the
tidal stress-differences seem well suited to aid the mobile parts in gradually
working their way outwards. At the same time the more solid and resistant
portions should remain behind, and thus come to constitute the dominant
material of the central regions where stress-differences were greatest, and
so, as it were, concentrate rigidity there. The process may still be in action.
If it be assumed that the rhythmical stresses have thus developed a
resistance to deformation proportional to their intensity, we may combine
this with density to form the basis of another hypothetical distribution of
rigidity, as follows:
Distances
from Densities
Density Ratios adjusted to stress- Deduced
center in under
ratios. differences. 1:8) rigidities.
terms Laplace’s law.
of radius.
1.00 2.8 1 1 0.16 Steel
.75 5.7 2 3.5 0.58 ”
.50 8.39 3 5.4 0.90 ”
.25 10.27 3.7 7 1.16 ”
.00 10.95 3.9 8 1.33 ”
The average rigidity is here also much less than that of steel, but its
distribution is such as to render it ideally fitted to resist tidal distortion.
These hypothetical distributions of rigidity have no claims to special
value in themselves, for the grounds on which they are based are quite
inadequate, but they are not without importance in giving tangible form to
Page 669
considerations that bear vitally not only on tidal problems, but on many
others connected with the internal constitution and dynamics of the earth.
Sphericity as a factor in deformation.
It is obvious that if the earth shrinks, its crust must become too large for
the reduced spheroid, and must be compressed or distorted to fit the new
form. The amount of distortion required for any given shrinkage is easily
computed from the ratio of the radius to the circumference of a sphere,
which is approximately 1 : 6.28. If, for example, the radius shortens 5
miles, each great circle must on the average be compressed, wrinkled, or
otherwise distorted to the extent of about 31 miles, or, in reversed
application, if the mountain foldings on any great circle together show a
shortening of 100 miles, the appropriate radial shortening is 16 miles. The
ratio of 1 : 6+ furnishes a convenient check on hypotheses that assign
specific thrusts to specific sinkings of adjacent segments. A segment 3000
miles across, for example, such as the bottom of the North Atlantic basin,
sinking three miles, about the full depth of the basin, would give a lateral
thrust of about 2.2 miles, a little over a mile on each side, a trivial amount
compared with the foldings on the adjacent continental borders.
The influence of the domed form of the surface.—Because of the
spheroidal form of the earth, each portion of the crust is ideally an arch or
dome. When broad areas like the continents are considered, it is the dome
rather than the arch that is involved, and in this the thrust is ideally toward
all parts of the periphery. It is probably for this reason that mountain ranges
so often follow curved or angulated lines, or outline rude triangles or
polygons. The sigmoidal courses of the ranges of southern Europe, the
looped chains of the eastern border of Asia, and the curved ranges of the
Antillean region, are notable examples. The border ranges of the Americas,
of the Thibetan plateau, and of other great segments, illustrate the polygonal
tendency. The general distribution of the great ranges is such that a nearly
equal portion of crustal crumpling is thrown across each great circle, as
theory demands. The common generalization that mountain ranges run
chiefly in oblique directions, as northeast-southwest, northwest-southeast, is
but a partial view of the more general fact that the lines of distortion must
lie in all directions to accommodate the old crust to the new geoid, if there
be equable contraction in all parts.
others connected with the internal constitution and dynamics of the earth.
Sphericity as a factor in deformation.
It is obvious that if the earth shrinks, its crust must become too large for
the reduced spheroid, and must be compressed or distorted to fit the new
form. The amount of distortion required for any given shrinkage is easily
computed from the ratio of the radius to the circumference of a sphere,
which is approximately 1 : 6.28. If, for example, the radius shortens 5
miles, each great circle must on the average be compressed, wrinkled, or
otherwise distorted to the extent of about 31 miles, or, in reversed
application, if the mountain foldings on any great circle together show a
shortening of 100 miles, the appropriate radial shortening is 16 miles. The
ratio of 1 : 6+ furnishes a convenient check on hypotheses that assign
specific thrusts to specific sinkings of adjacent segments. A segment 3000
miles across, for example, such as the bottom of the North Atlantic basin,
sinking three miles, about the full depth of the basin, would give a lateral
thrust of about 2.2 miles, a little over a mile on each side, a trivial amount
compared with the foldings on the adjacent continental borders.
The influence of the domed form of the surface.—Because of the
spheroidal form of the earth, each portion of the crust is ideally an arch or
dome. When broad areas like the continents are considered, it is the dome
rather than the arch that is involved, and in this the thrust is ideally toward
all parts of the periphery. It is probably for this reason that mountain ranges
so often follow curved or angulated lines, or outline rude triangles or
polygons. The sigmoidal courses of the ranges of southern Europe, the
looped chains of the eastern border of Asia, and the curved ranges of the
Antillean region, are notable examples. The border ranges of the Americas,
of the Thibetan plateau, and of other great segments, illustrate the polygonal
tendency. The general distribution of the great ranges is such that a nearly
equal portion of crustal crumpling is thrown across each great circle, as
theory demands. The common generalization that mountain ranges run
chiefly in oblique directions, as northeast-southwest, northwest-southeast, is
but a partial view of the more general fact that the lines of distortion must
lie in all directions to accommodate the old crust to the new geoid, if there
be equable contraction in all parts.
Page 670
THEORETICAL STRENGTH OF IDEAL DOMES ARCHED TWO
MILES ABOVE THE AVERAGE SURFACE OF THE SPHERE.
Diameter of given Multiplier of 1/525 Proportion of its own
dome arched i.e. the supporting weight sustained by
2 miles above proportion of a given dome arched
sphere. spherical dome. 2 miles above sphere.
3,000 miles 1.006 1/522
400 ” 1.396 1/376
240 ” 2.11 1/249
160 ” 3.49 1/150
80 ” 10.97 1/48
From this table it will be seen that for domes of continental dimensions
the supporting strength equals only a very small fraction of the dome’s own
weight. Increasing the thickness of the shell increases its actual supporting
power, but the proportion is somewhat less when the whole sphere is
concerned. The problem has not been worked out for domes of limited
extent. For rough estimates, where the dimensions of the dome are of
continental magnitude, each mile of thickness may be taken as supporting a
layer of about 10 feet of its own material. If the hypothetical level of no
stress be placed at 8 miles depth, the shell above this, by reason of its
domed shape, could relieve its own pressure on that below to an amount
equal only to the weight of about 80 feet of rock over its surface, even if its
form and structure were ideal. If the shell were thick enough (817 miles) to
embrace one-half the volume of the earth, its supporting power would be a
little more than the weight of one and one-half miles of rock. As the radius
of the earth is less than 4000 miles, the extreme supporting power reckoned
on this basis would be only about 8 miles of rock-depth. It is interesting, if
not significant, to observe that this depth barely reaches the minimum
shrinkage that will serve, according to current estimates, to account for the
crustal shortening of the great mountain-making periods. It is as if the
shrinkage stresses accumulated to the full extent of the stress-resisting
power of the whole sphere, and then collapsed. It is not safe, however, to
give much weight to this coincidence, for higher densities and probably
higher resistances to distortion come into play in the deeper horizons. If
these resistances are proportional to the higher densities of the interior, the
deductions would remain the same. If the effective rigidity of the earth as a
whole is that of steel, as deduced by Kelvin and Darwin from tidal and
other observations, or twice that of steel, as inferred by Milne from the
MILES ABOVE THE AVERAGE SURFACE OF THE SPHERE.
Diameter of given Multiplier of 1/525 Proportion of its own
dome arched i.e. the supporting weight sustained by
2 miles above proportion of a given dome arched
sphere. spherical dome. 2 miles above sphere.
3,000 miles 1.006 1/522
400 ” 1.396 1/376
240 ” 2.11 1/249
160 ” 3.49 1/150
80 ” 10.97 1/48
From this table it will be seen that for domes of continental dimensions
the supporting strength equals only a very small fraction of the dome’s own
weight. Increasing the thickness of the shell increases its actual supporting
power, but the proportion is somewhat less when the whole sphere is
concerned. The problem has not been worked out for domes of limited
extent. For rough estimates, where the dimensions of the dome are of
continental magnitude, each mile of thickness may be taken as supporting a
layer of about 10 feet of its own material. If the hypothetical level of no
stress be placed at 8 miles depth, the shell above this, by reason of its
domed shape, could relieve its own pressure on that below to an amount
equal only to the weight of about 80 feet of rock over its surface, even if its
form and structure were ideal. If the shell were thick enough (817 miles) to
embrace one-half the volume of the earth, its supporting power would be a
little more than the weight of one and one-half miles of rock. As the radius
of the earth is less than 4000 miles, the extreme supporting power reckoned
on this basis would be only about 8 miles of rock-depth. It is interesting, if
not significant, to observe that this depth barely reaches the minimum
shrinkage that will serve, according to current estimates, to account for the
crustal shortening of the great mountain-making periods. It is as if the
shrinkage stresses accumulated to the full extent of the stress-resisting
power of the whole sphere, and then collapsed. It is not safe, however, to
give much weight to this coincidence, for higher densities and probably
higher resistances to distortion come into play in the deeper horizons. If
these resistances are proportional to the higher densities of the interior, the
deductions would remain the same. If the effective rigidity of the earth as a
whole is that of steel, as deduced by Kelvin and Darwin from tidal and
other observations, or twice that of steel, as inferred by Milne from the
Page 671
transmission of seismic vibrations, the supporting power of the body of the
earth dependent on its sphericity would be appreciably higher.
It would seem clear from the foregoing considerations that something
more than the mere crust of the earth has been involved in the great
deformations. Indeed it is not clear that the fullest resources of stress-
accumulation which the spheroidal form of the earth affords are sufficient
to meet the demands of the problem, unless the rigidity of the earth be taken
at a much higher value than that of surface-rock, and this is perhaps an
additional argument for the high rigidities inferred from tides and seismic
waves.
In view of the doubtful competency of even the thickest segments to
accumulate the requisite stresses, there is need to consider modes of
differential stress-accumulation other than those dependent on sphericity.
Stress-accumulation independent of sphericity.—The principle of the
dome is brought into play whenever an interior shell shrinks away, or tends
to shrink away, from an outer one which does not shrink. In this case, there
is a free outer surface and a more or less unsupported under surface toward
which motion is possible. The dome may, therefore, yield by crushing or by
contortion. The computations given above are for cases of this kind. But
where the thickness becomes great and the dome involves a large part or
even all of a sector of the earth, freedom of motion beneath is small, and to
readjust the matter to a new form, strains must be developed widely
throughout the sector, and must involve regions where the pressure is
extremely great on all sides, and crushing in the usual sense impossible.
Assuming the correctness of the modern doctrine that such pressure
increases rigidity, instead of the older doctrine that it gives plasticity, it
becomes reasonable to assume that stress-differences would be distributed
throughout the mass, and bring into play a large portion of its stress-
accumulating competency. When the mass yielded, it would not be by
crushing, but by “flowage,” which would be more or less general
throughout the mass. It might, however, be partially concentrated, as, for
example, on the borders of sectors of different specific gravity.
Stress-differences may arise from physical changes within the rock itself.
Whenever there is a re-aggregation of matter, or a change of any kind which
involves change of volume, a change of stress is liable to be involved. It
earth dependent on its sphericity would be appreciably higher.
It would seem clear from the foregoing considerations that something
more than the mere crust of the earth has been involved in the great
deformations. Indeed it is not clear that the fullest resources of stress-
accumulation which the spheroidal form of the earth affords are sufficient
to meet the demands of the problem, unless the rigidity of the earth be taken
at a much higher value than that of surface-rock, and this is perhaps an
additional argument for the high rigidities inferred from tides and seismic
waves.
In view of the doubtful competency of even the thickest segments to
accumulate the requisite stresses, there is need to consider modes of
differential stress-accumulation other than those dependent on sphericity.
Stress-accumulation independent of sphericity.—The principle of the
dome is brought into play whenever an interior shell shrinks away, or tends
to shrink away, from an outer one which does not shrink. In this case, there
is a free outer surface and a more or less unsupported under surface toward
which motion is possible. The dome may, therefore, yield by crushing or by
contortion. The computations given above are for cases of this kind. But
where the thickness becomes great and the dome involves a large part or
even all of a sector of the earth, freedom of motion beneath is small, and to
readjust the matter to a new form, strains must be developed widely
throughout the sector, and must involve regions where the pressure is
extremely great on all sides, and crushing in the usual sense impossible.
Assuming the correctness of the modern doctrine that such pressure
increases rigidity, instead of the older doctrine that it gives plasticity, it
becomes reasonable to assume that stress-differences would be distributed
throughout the mass, and bring into play a large portion of its stress-
accumulating competency. When the mass yielded, it would not be by
crushing, but by “flowage,” which would be more or less general
throughout the mass. It might, however, be partially concentrated, as, for
example, on the borders of sectors of different specific gravity.
Stress-differences may arise from physical changes within the rock itself.
Whenever there is a re-aggregation of matter, or a change of any kind which
involves change of volume, a change of stress is liable to be involved. It
Page 672
may be of the nature of relief or of intensification. In an earth built up by
the haphazard infall of matter, a very heterogeneous mass must result, and
the subsequent changes may be supposed to be intimately distributed
through the mass, being slight at any point, but present at innumerable
points. An immeasurable number of small stress-differences may, therefore,
be developed throughout the mass. Until these overmatch the effective
strength of the mass, they may continue to accumulate. These are not
necessarily connected with stresses that arise from sphericity, and may work
more or less independently of them. It is not improbable that the great
stress-accumulating power of the globe finds an essential part of its
explanation in supplemental considerations of this kind, and not wholly in
its spheroidal form.
The actual configuration of the surface.—The foregoing computations
relative to the power of shells of the earth to sustain pressures are based on
ideal forms and structures that are not realized in fact. How far the earth
fails to conform to these conditions must now be considered. When
compared with the earth as a whole, the inequalities of its surface are trivial.
If the great dynamic forces acted through the whole or the larger part of the
body of the earth, the configuration of the surface can be supposed to have
done little more than influence the location of the surface deformations and
their special phases. But if the forces were limited to a crust of moderate
thickness, the configuration of the surface is a matter of radical importance.
Concave tracts.—There is need, therefore, to inquire if any considerable
breadth of the crust is outwardly plane or concave, for the principle of the
dome is obviously not applicable to a plane or concave surface. To be a
source of fatal weakness, the concavity must be broad enough to cause the
planes of equal cooling, the isogeotherms, to be concave to considerable
depths. For example, if the hypothetical level of no stress is eight miles
below the surface, as computed on certain assumptions, the concave portion
must be so broad that the isogeotherms will also be concave outward at
something near that depth; in other words, the main part of the zone of
thrust must be concave. A narrow concavity at the surface, such as an
ordinary valley in a portion of the crust that has the average convexity,
would not seriously depress the isogeotherms, or affect the zone of thrust,
but a valley several times eight miles (level of no stress) in breadth would.
For inspecting the surface of the earth in this regard, it is convenient to
the haphazard infall of matter, a very heterogeneous mass must result, and
the subsequent changes may be supposed to be intimately distributed
through the mass, being slight at any point, but present at innumerable
points. An immeasurable number of small stress-differences may, therefore,
be developed throughout the mass. Until these overmatch the effective
strength of the mass, they may continue to accumulate. These are not
necessarily connected with stresses that arise from sphericity, and may work
more or less independently of them. It is not improbable that the great
stress-accumulating power of the globe finds an essential part of its
explanation in supplemental considerations of this kind, and not wholly in
its spheroidal form.
The actual configuration of the surface.—The foregoing computations
relative to the power of shells of the earth to sustain pressures are based on
ideal forms and structures that are not realized in fact. How far the earth
fails to conform to these conditions must now be considered. When
compared with the earth as a whole, the inequalities of its surface are trivial.
If the great dynamic forces acted through the whole or the larger part of the
body of the earth, the configuration of the surface can be supposed to have
done little more than influence the location of the surface deformations and
their special phases. But if the forces were limited to a crust of moderate
thickness, the configuration of the surface is a matter of radical importance.
Concave tracts.—There is need, therefore, to inquire if any considerable
breadth of the crust is outwardly plane or concave, for the principle of the
dome is obviously not applicable to a plane or concave surface. To be a
source of fatal weakness, the concavity must be broad enough to cause the
planes of equal cooling, the isogeotherms, to be concave to considerable
depths. For example, if the hypothetical level of no stress is eight miles
below the surface, as computed on certain assumptions, the concave portion
must be so broad that the isogeotherms will also be concave outward at
something near that depth; in other words, the main part of the zone of
thrust must be concave. A narrow concavity at the surface, such as an
ordinary valley in a portion of the crust that has the average convexity,
would not seriously depress the isogeotherms, or affect the zone of thrust,
but a valley several times eight miles (level of no stress) in breadth would.
For inspecting the surface of the earth in this regard, it is convenient to
Page 673
know what amounts of fall below the level surface give a true plane for
given distances. These are shown in the following table:[274]
Average fall of
Length of normal to chord true plane from
Length of arc at middle point in level plane per
in miles. mile, in feet.
Greater fall
Feet. Fathoms.
gives concavity.
25 100.3 16.7 8.
50 432. 72. 17.3
75 913.4 152.2 24.3
100 1,684. 280.7 33.7
150 3,748.8 624.8 49.9
200 6,674. 1,112.3 66.7
250 10,369.9 1,728.3 82.9
300 14,942. 2,490.3 99.6
400 26,664. 4,444. 133.3
500 41,659. 6,943. 166.6
Applying these criteria to the surface of the lithosphere, it is found that
concave tracts from 100 to 300 miles in breadth are not uncommon. The
more notable of these are shown in black on the accompanying map, Fig.
454, and two typical ones are shown in cross-section in Figs. 455 and 456.
It is to be observed that concave tracts border the continents very generally.
They are connected with the descent from the continental shelf to the
abysmal basins, and are unsymmetrical. Notable concavities are found in
some of the great valleys on the continental platforms. The basins of Lake
Superior, Michigan, Huron, and Ontario are in part concave; so are Puget
Sound, the Adriatic, and the Dead Sea; so also are the valleys of California,
of the Po, and of the Ganges, when the adjacent mountains are included.
Some of the “deeps” of the bottom of the ocean are notably concave. Fig.
455, a cross-section of the Challenger Deep, drawn to true scale and
convexity, shows the nature of the phenomenon. The breadth is here 300
miles, and the depression below a true plane is 11,400 feet. The lower line
of the figure shows the approximate position and form of the normal
isogeotherm about ten miles below the surface. Assuming equal
conductivity in all parts, it is clear that the isogeotherms must be concave
upwards for a considerable distance below ten miles. Unless the shell of
thrust is much more than ten miles thick, these concave portions should
given distances. These are shown in the following table:[274]
Average fall of
Length of normal to chord true plane from
Length of arc at middle point in level plane per
in miles. mile, in feet.
Greater fall
Feet. Fathoms.
gives concavity.
25 100.3 16.7 8.
50 432. 72. 17.3
75 913.4 152.2 24.3
100 1,684. 280.7 33.7
150 3,748.8 624.8 49.9
200 6,674. 1,112.3 66.7
250 10,369.9 1,728.3 82.9
300 14,942. 2,490.3 99.6
400 26,664. 4,444. 133.3
500 41,659. 6,943. 166.6
Applying these criteria to the surface of the lithosphere, it is found that
concave tracts from 100 to 300 miles in breadth are not uncommon. The
more notable of these are shown in black on the accompanying map, Fig.
454, and two typical ones are shown in cross-section in Figs. 455 and 456.
It is to be observed that concave tracts border the continents very generally.
They are connected with the descent from the continental shelf to the
abysmal basins, and are unsymmetrical. Notable concavities are found in
some of the great valleys on the continental platforms. The basins of Lake
Superior, Michigan, Huron, and Ontario are in part concave; so are Puget
Sound, the Adriatic, and the Dead Sea; so also are the valleys of California,
of the Po, and of the Ganges, when the adjacent mountains are included.
Some of the “deeps” of the bottom of the ocean are notably concave. Fig.
455, a cross-section of the Challenger Deep, drawn to true scale and
convexity, shows the nature of the phenomenon. The breadth is here 300
miles, and the depression below a true plane is 11,400 feet. The lower line
of the figure shows the approximate position and form of the normal
isogeotherm about ten miles below the surface. Assuming equal
conductivity in all parts, it is clear that the isogeotherms must be concave
upwards for a considerable distance below ten miles. Unless the shell of
thrust is much more than ten miles thick, these concave portions should
Page 674
yield as fast as cooling below them permits, and no stresses arising from
convexity could be accumulated.
Fig. 454.—Map of the world, showing in black the chief submarine concavities of the
lithosphere. (Prepared by W. H. Emmons.)
Fig. 455.—Section of the Challenger Deep from an island on the Caroline plateau, a, to an
island on the Ladrone plateau, b, drawn to a true scale, showing the real concavity of the
surface of the lithosphere for a breadth of 300 miles. The upper line represents the sea
surface, a natural level. The next line below represents a true plane, eliminating the
curvature of the sea surface. The third line represents the bottom of the deep. By
comparison with the line above, its true concavity may be seen. The lowest line represents
an isogeotherm at about 10 miles below the surface; i.e. appreciably below “the level of
no stress,” as usually computed, showing that the whole thrust zone is concave outwards,
if it is limited to surface cooling as usually computed. (Prepared by W. H. Emmons.)
Fig. 456.—Section through the Atlantic coastal plain, the continental shelf, and a portion of
the abysmal bottom, drawn to a true scale, showing that the surface of the lithosphere
drops below a true plane tangent to the continental shelf and the ocean-bottom. The
upper line represents the surface of the coastal plain at the left and of the ocean at the
right. The lower line represents the sea-bottom, and the middle line a true plane tangent
to the shelf and the sea-bottom. The breadth of the concave tract varies from 100 to 150
miles. (Prepared by W. H. Emmons.)
convexity could be accumulated.
Fig. 454.—Map of the world, showing in black the chief submarine concavities of the
lithosphere. (Prepared by W. H. Emmons.)
Fig. 455.—Section of the Challenger Deep from an island on the Caroline plateau, a, to an
island on the Ladrone plateau, b, drawn to a true scale, showing the real concavity of the
surface of the lithosphere for a breadth of 300 miles. The upper line represents the sea
surface, a natural level. The next line below represents a true plane, eliminating the
curvature of the sea surface. The third line represents the bottom of the deep. By
comparison with the line above, its true concavity may be seen. The lowest line represents
an isogeotherm at about 10 miles below the surface; i.e. appreciably below “the level of
no stress,” as usually computed, showing that the whole thrust zone is concave outwards,
if it is limited to surface cooling as usually computed. (Prepared by W. H. Emmons.)
Fig. 456.—Section through the Atlantic coastal plain, the continental shelf, and a portion of
the abysmal bottom, drawn to a true scale, showing that the surface of the lithosphere
drops below a true plane tangent to the continental shelf and the ocean-bottom. The
upper line represents the surface of the coastal plain at the left and of the ocean at the
right. The lower line represents the sea-bottom, and the middle line a true plane tangent
to the shelf and the sea-bottom. The breadth of the concave tract varies from 100 to 150
miles. (Prepared by W. H. Emmons.)
Page 675
These concavities of surface are so extensive and so widely distributed
over the globe that no part of the outer shell can be supposed to be capable
of accumulating notable stresses unless rigidly attached to the earth-body
below. In other words, so far as sphericity is concerned, the crust must ease
all its stresses nearly as fast as they accumulate, if, as usually assumed, it
rests on a contracting or mobile substratum.
Surface cooling under these conditions should give only feeble thrusts,
developed and eased nearly constantly. Such movements should be
admirably adapted to give those gentle, nearly constant subsidences that
furnish the nice adjustments of water-depth required for the accumulation of
thick strata in shallow water, and those slow upward warpings that renew
the feeding-grounds of erosion, the necessary complement of the
deposition. These gentle, nearly constant movements mark every stage of
geological history, and constitute one of its greatest though least obtrusive
features. But if superficial stresses arising in this way are eased in
producing these effects, they cannot accumulate to cause the great periodic
movements.
Even where the crust is not concave, it is so warped and so traversed by
folds and fault-planes that its resistance to thrust is relatively low, and it
should, therefore, warp easily and at many points, if the thrust be confined
to a superficial crust.
General conclusion.—When to the weakness of the crust, as computed
under ideal conditions, there is added the weakness inherent in these
concave and warped tracts, the conclusion seems imperative that while the
crust is the pliant subject of minor and nearly constant warpings, such as are
everywhere implied in the stratigraphic series, it is wholly incompetent to
be the medium of those great deformations which occur at long intervals
and mark off the great eras of geologic history. These great deformations
apparently involve the whole, or a large part, of the body of the earth, and
seem to require a very high state of effective rigidity.
General references on crustal movements.—Babbage, Jour.
Geol. Soc., Vol. III (1834), p. 206 Lyell, Principles of Geology,
Vol. II, p. 235; Mallet, Phil. Trans. (1873), p. 205; Reade, Origin
of Mountain Ranges, and Evolution of Earth Structure; Fisher,
Physics of the Earth’s Crust; Dutton, Greater Problems of
over the globe that no part of the outer shell can be supposed to be capable
of accumulating notable stresses unless rigidly attached to the earth-body
below. In other words, so far as sphericity is concerned, the crust must ease
all its stresses nearly as fast as they accumulate, if, as usually assumed, it
rests on a contracting or mobile substratum.
Surface cooling under these conditions should give only feeble thrusts,
developed and eased nearly constantly. Such movements should be
admirably adapted to give those gentle, nearly constant subsidences that
furnish the nice adjustments of water-depth required for the accumulation of
thick strata in shallow water, and those slow upward warpings that renew
the feeding-grounds of erosion, the necessary complement of the
deposition. These gentle, nearly constant movements mark every stage of
geological history, and constitute one of its greatest though least obtrusive
features. But if superficial stresses arising in this way are eased in
producing these effects, they cannot accumulate to cause the great periodic
movements.
Even where the crust is not concave, it is so warped and so traversed by
folds and fault-planes that its resistance to thrust is relatively low, and it
should, therefore, warp easily and at many points, if the thrust be confined
to a superficial crust.
General conclusion.—When to the weakness of the crust, as computed
under ideal conditions, there is added the weakness inherent in these
concave and warped tracts, the conclusion seems imperative that while the
crust is the pliant subject of minor and nearly constant warpings, such as are
everywhere implied in the stratigraphic series, it is wholly incompetent to
be the medium of those great deformations which occur at long intervals
and mark off the great eras of geologic history. These great deformations
apparently involve the whole, or a large part, of the body of the earth, and
seem to require a very high state of effective rigidity.
General references on crustal movements.—Babbage, Jour.
Geol. Soc., Vol. III (1834), p. 206 Lyell, Principles of Geology,
Vol. II, p. 235; Mallet, Phil. Trans. (1873), p. 205; Reade, Origin
of Mountain Ranges, and Evolution of Earth Structure; Fisher,
Physics of the Earth’s Crust; Dutton, Greater Problems of
Page 676
Physical Geology, Bull. Phil. Soc. of Washington, Vol. XI, p. 52,
also Amer. Jour. of Sci., Vol. VIII (1874), p. 121, and Geology
of the High Plateaus of Utah (1880); Jamieson, Quar. Jour. Geol.
Soc. (1882), and Geol. Mag. (1882), pp. 400 and 526; Heim,
Mechanismus der Gebirgsbildung; Marjerie and Heim, Les
Dislocations de l’Écorce terrestre (1888); Shaler, Proc. Boston
Soc. Nat. Hist., Vol. XVII, p. 288; Dana, Manual of Geol., 4th
ed., p. 345 et seq.; Woodward, Mathematical Theories of the
Earth, Smithsonian Rept. for 1890, p. 196; Willis, The
Mechanics of the Appalachian Structures, 13th Ann. Rept. U. S.
Geol. Surv., Pt. II (1893), pp. 211–282; LeConte, Theories of
Mountain Origin, Jour. Geol. Vol. I (1893), p. 542; Gilbert, Jour.
Geol., Vol. III (1895), p. 333, and Bull. Phil. Soc. of
Washington, Vol. XIII (1895), p. 31; Van Hise, Earth
Movements, Trans. Wis. Acad. Sci., Arts and Let., Vol. II
(1898), pp. 512–514; Estimates and Causes of Crustal
Shortening, Jour. Geol., Vol. VI (1898), pp. 29–31; Relations of
Rock Flowage to Mountain Making, Mon. XLVII, U. S. Geol.
Surv. (1904), pp. 924–931; A. Geikie, Text-book of Geology, 4th
ed., pp. 672–702.
also Amer. Jour. of Sci., Vol. VIII (1874), p. 121, and Geology
of the High Plateaus of Utah (1880); Jamieson, Quar. Jour. Geol.
Soc. (1882), and Geol. Mag. (1882), pp. 400 and 526; Heim,
Mechanismus der Gebirgsbildung; Marjerie and Heim, Les
Dislocations de l’Écorce terrestre (1888); Shaler, Proc. Boston
Soc. Nat. Hist., Vol. XVII, p. 288; Dana, Manual of Geol., 4th
ed., p. 345 et seq.; Woodward, Mathematical Theories of the
Earth, Smithsonian Rept. for 1890, p. 196; Willis, The
Mechanics of the Appalachian Structures, 13th Ann. Rept. U. S.
Geol. Surv., Pt. II (1893), pp. 211–282; LeConte, Theories of
Mountain Origin, Jour. Geol. Vol. I (1893), p. 542; Gilbert, Jour.
Geol., Vol. III (1895), p. 333, and Bull. Phil. Soc. of
Washington, Vol. XIII (1895), p. 31; Van Hise, Earth
Movements, Trans. Wis. Acad. Sci., Arts and Let., Vol. II
(1898), pp. 512–514; Estimates and Causes of Crustal
Shortening, Jour. Geol., Vol. VI (1898), pp. 29–31; Relations of
Rock Flowage to Mountain Making, Mon. XLVII, U. S. Geol.
Surv. (1904), pp. 924–931; A. Geikie, Text-book of Geology, 4th
ed., pp. 672–702.
Page 677
CHAPTER X.
THE EXTRUSIVE PROCESSES.
Outward movements.—In the preceding chapters movements toward
the center have been considered. The complementary processes of outward
movement now invite attention. Without doubt these are mainly but a
resultant of the centripetal actions. For each pound of material moved
outwards an equivalent is quite surely moved inwards. Notwithstanding
this, the outward movements have a peculiar nature of their own, and serve
a function of radical importance in the economy of the globe. Some minor
phases have been incidentally considered, such as the upward flow of
springs and deep-seated waters, but here the descending and ascending
factors are alike, and are closely and obviously connected.
VULCANISM.
The great example of ascensive action is the movement of fluid rock
from the interior outwards. The term vulcanism will be used to embrace not
only volcanic phenomena in the narrower sense, but all outward forcing of
molten material, whether strictly extrusive or merely ascensive.
The philosophy of this ascensive action, taken as a whole, is simple. In
the effort at concentration under the powerful action of the earth’s gravity,
the material of high specific gravity is urged more strongly toward the
center, volume for volume, than that of less specific gravity, and as gravity
is perpetually active, it follows that whenever any movement, molecular or
molar, takes place which permits a readjustment of the positions of the two
kinds of matter, the heavier sinks toward the center and the lighter rises, or
at least tends to do so. So also where there are stress-differences, the mobile
matter tends to flow from the regions of greater stress toward those of lesser
stress. In so far as any portion of the interior becomes liquid, it is free to
move up or down according to the balance of stress brought to bear upon it,
THE EXTRUSIVE PROCESSES.
Outward movements.—In the preceding chapters movements toward
the center have been considered. The complementary processes of outward
movement now invite attention. Without doubt these are mainly but a
resultant of the centripetal actions. For each pound of material moved
outwards an equivalent is quite surely moved inwards. Notwithstanding
this, the outward movements have a peculiar nature of their own, and serve
a function of radical importance in the economy of the globe. Some minor
phases have been incidentally considered, such as the upward flow of
springs and deep-seated waters, but here the descending and ascending
factors are alike, and are closely and obviously connected.
VULCANISM.
The great example of ascensive action is the movement of fluid rock
from the interior outwards. The term vulcanism will be used to embrace not
only volcanic phenomena in the narrower sense, but all outward forcing of
molten material, whether strictly extrusive or merely ascensive.
The philosophy of this ascensive action, taken as a whole, is simple. In
the effort at concentration under the powerful action of the earth’s gravity,
the material of high specific gravity is urged more strongly toward the
center, volume for volume, than that of less specific gravity, and as gravity
is perpetually active, it follows that whenever any movement, molecular or
molar, takes place which permits a readjustment of the positions of the two
kinds of matter, the heavier sinks toward the center and the lighter rises, or
at least tends to do so. So also where there are stress-differences, the mobile
matter tends to flow from the regions of greater stress toward those of lesser
stress. In so far as any portion of the interior becomes liquid, it is free to
move up or down according to the balance of stress brought to bear upon it,
Page 678
and adapts itself to any line of least resistance available to it. As a natural
result, therefore, the portion of the interior which becomes fluid most
largely participates in the outward movement. In so far as molecular action
permits a readjustment of material, there is a tendency, even in the solid
state, for the lighter material to move upwards and the heavier downwards,
and for the more stressed portions to move toward points of less stress; but
this takes place with extreme slowness. In so far as the materials of the
interior diffuse themselves through each other, the same laws hold good, but
they are modified by the special principles that control diffusion. The
outward diffusion of interior gases may be a factor of appreciable
importance, but this cannot be affirmed at present.
Phases of vulcanism.—The forcing of fluid rock outward assumes two
general phases, which, however, merge into each other; and these main
phases take on various sub-phases. The first phase embraces those outward
movements of fluid rock which do not reach the surface. The lavas, after
ascending to the vicinity of the surface, intrude themselves into the outer
formations of the earth and congeal underground (plutonic). The second
phase embraces those outward movements in which the fluid rock reaches
the surface and gives rise to eruptive phenomena (volcanic). The first is
intrusive, the second extrusive; the first constitutes irruptions, the second
eruptions.[275] The fundamental nature of the two is the same, but the
extrusions usually take on special phases because of the relief of pressure at
the surface of the earth, and because of the action of surface-waters in
contact with the heated lavas. Just where the lavas come from, and how
they find their way through the deep-lying compact zone below the zone of
fracture, may better be considered later. When they reach the zone of
fracture, they usually either take advantage of fissures already formed, or
force passageways for themselves by fracture. There is little evidence that
they bore their way through the rocks by melting, though they appear to
round out their channels in some way into pipes, ducts, and other tubular
forms when they flow through them for long periods of time.
1. Intrusions.
Fluid rock forced into fissures and solidified there forms dikes; forced
into chimney-like passages, it forms pipes or plugs; insinuated between
beds, it forms sills; bunched under strata so as to arch them upwards, it
result, therefore, the portion of the interior which becomes fluid most
largely participates in the outward movement. In so far as molecular action
permits a readjustment of material, there is a tendency, even in the solid
state, for the lighter material to move upwards and the heavier downwards,
and for the more stressed portions to move toward points of less stress; but
this takes place with extreme slowness. In so far as the materials of the
interior diffuse themselves through each other, the same laws hold good, but
they are modified by the special principles that control diffusion. The
outward diffusion of interior gases may be a factor of appreciable
importance, but this cannot be affirmed at present.
Phases of vulcanism.—The forcing of fluid rock outward assumes two
general phases, which, however, merge into each other; and these main
phases take on various sub-phases. The first phase embraces those outward
movements of fluid rock which do not reach the surface. The lavas, after
ascending to the vicinity of the surface, intrude themselves into the outer
formations of the earth and congeal underground (plutonic). The second
phase embraces those outward movements in which the fluid rock reaches
the surface and gives rise to eruptive phenomena (volcanic). The first is
intrusive, the second extrusive; the first constitutes irruptions, the second
eruptions.[275] The fundamental nature of the two is the same, but the
extrusions usually take on special phases because of the relief of pressure at
the surface of the earth, and because of the action of surface-waters in
contact with the heated lavas. Just where the lavas come from, and how
they find their way through the deep-lying compact zone below the zone of
fracture, may better be considered later. When they reach the zone of
fracture, they usually either take advantage of fissures already formed, or
force passageways for themselves by fracture. There is little evidence that
they bore their way through the rocks by melting, though they appear to
round out their channels in some way into pipes, ducts, and other tubular
forms when they flow through them for long periods of time.
1. Intrusions.
Fluid rock forced into fissures and solidified there forms dikes; forced
into chimney-like passages, it forms pipes or plugs; insinuated between
beds, it forms sills; bunched under strata so as to arch them upwards, it
Page 679
forms laccoliths; massed in great aggregations underground, it constitutes
batholiths, as already described (pp. 394 and 500). Lavas sometimes crowd
aside the adjacent rocks so far as to cause them to take a concentric form
about the intruded mass. This is not uncommon in the oldest formations,
and is probably not infrequent in the deeper horizons where the pressures
are very great. Some part of this may, however, be due to later
deformations. Nearer the surface, usually, the beds are merely lifted as in
forming the sills, or are bowed upwards, as in the laccoliths, or faulted as in
bysmaliths (p. 500).
The heating action on the adjacent rock varies greatly with the mass and
temperature of the intruded lava. Thin dikes and sills often produce little
effect, while greater and hotter masses notably metamorphose the adjacent
rock. In some cases marked effects are due to a thin stream of lava flowing
through a fissure for a long period, and so maintaining a high temperature.
In the least effective cases, the adjacent rock usually shows some signs of
baking. In the marked cases, there is more or less new crystallization. The
surrounding rock commonly shows some evidence of material derived from
the lavas; less often the lava shows some evidence of having received
material from the adjacent rock. But since the lavas do not usually bore
their way through the strata in the zone of fracture, nor melt the adjacent
rock, the constitution of the lavas is not appreciably changed by the kinds of
rock which they penetrate. On the other hand, the intrusions often show the
effects of rather rapid cooling by contact with the adjacent rock, (a) by a
less coarse crystallization near the rock-walls, and sometimes (b) in a
segregation of the material.
2. Extrusions.
When molten rock is forced to the surface it gives rise to the most intense
and impressive of all geological phenomena. The energies acquired in the
interior under great compression here find sudden relief. Occluded gases
often expand with extreme violence, hurling portions of the lavas to great
heights and shattering them into fragments constituting “smoke,” ash,
cinders, bombs, and other pyroclastic material. Much of the explosive
violence of volcanoes has been attributed to the contact of surface-waters
with the hot rising lava, but the function of this kind of action has probably
been exaggerated.
batholiths, as already described (pp. 394 and 500). Lavas sometimes crowd
aside the adjacent rocks so far as to cause them to take a concentric form
about the intruded mass. This is not uncommon in the oldest formations,
and is probably not infrequent in the deeper horizons where the pressures
are very great. Some part of this may, however, be due to later
deformations. Nearer the surface, usually, the beds are merely lifted as in
forming the sills, or are bowed upwards, as in the laccoliths, or faulted as in
bysmaliths (p. 500).
The heating action on the adjacent rock varies greatly with the mass and
temperature of the intruded lava. Thin dikes and sills often produce little
effect, while greater and hotter masses notably metamorphose the adjacent
rock. In some cases marked effects are due to a thin stream of lava flowing
through a fissure for a long period, and so maintaining a high temperature.
In the least effective cases, the adjacent rock usually shows some signs of
baking. In the marked cases, there is more or less new crystallization. The
surrounding rock commonly shows some evidence of material derived from
the lavas; less often the lava shows some evidence of having received
material from the adjacent rock. But since the lavas do not usually bore
their way through the strata in the zone of fracture, nor melt the adjacent
rock, the constitution of the lavas is not appreciably changed by the kinds of
rock which they penetrate. On the other hand, the intrusions often show the
effects of rather rapid cooling by contact with the adjacent rock, (a) by a
less coarse crystallization near the rock-walls, and sometimes (b) in a
segregation of the material.
2. Extrusions.
When molten rock is forced to the surface it gives rise to the most intense
and impressive of all geological phenomena. The energies acquired in the
interior under great compression here find sudden relief. Occluded gases
often expand with extreme violence, hurling portions of the lavas to great
heights and shattering them into fragments constituting “smoke,” ash,
cinders, bombs, and other pyroclastic material. Much of the explosive
violence of volcanoes has been attributed to the contact of surface-waters
with the hot rising lava, but the function of this kind of action has probably
been exaggerated.
Page 680
There are two phases of extrusion often quite strongly contrasted. The
one is explosive ejection, often attended with great violence; the other, a
quiet out-welling of the lava, with little more than ebullition. More or less
closely related to these differences are two classes of conduits, (a) the one,
great fissures, out of which the lava pours in great volume and spreads forth
over wide tracts, often in broad thin sheets; (b) the other, restricted
openings, often pipes, ducts, or limited fissures, from which the extrusion is
usually much less abundant, and hence it more largely congeals near the
orifice, forming cones. Flows from the former constitute massive eruptions;
those from the latter, the more familiar volcanic eruptions. There is no
radical difference between them, and the two classes blend. The extent of
the spreading of lava into thin sheets is due more to the mass and the
fluidity than to the form of the outlet. The stupendous outflows of certain
geologic periods appear to have issued mainly from extended fissures,
doubtless because these better accommodated the outbursting floods.
a. Fissure eruptions.—The chief known fissure eruptions of recent times
are the vast basaltic floods of Iceland. Most of the eruptions of historic
times are of the volcanic type; but at certain times in the past there were
prodigious outpourings, flow following flow until layers thousands of feet
thick covering thousands of square miles were built up. One of these
occurred in Tertiary times in Idaho, Oregon, and Washington, where some
200,000 square miles were covered with sheets of lava, aggregating in
places 2000 feet or more in thickness. Earlier than this, in Cretaceous times,
there were enormous flows on the Deccan plateau of India, covering a like
area to a depth of 4000 to 6000 feet. Still earlier than this, in Keweenawan
times, an even more prolonged succession of lava-flows covered nearly all
the area of the Lake Superior basin, and extended beyond it, and built up a
series of almost incredible thickness, the estimates reaching 15,000 to
25,000 feet. In these cases there is little evidence of explosive or other
violent action. There are few beds of ash, cinders, and similar pyroclastic
material. The inference is, therefore, that the lavas welled out rather quietly
and spread themselves rather fluently over the surrounding country. For the
most part these wide-spreading flows are composed of basic material,
which is more easily fusible and more highly fluent at a given temperature
than the acidic lavas. The latter are more disposed to form thick
embossments near the point of extrusion.
one is explosive ejection, often attended with great violence; the other, a
quiet out-welling of the lava, with little more than ebullition. More or less
closely related to these differences are two classes of conduits, (a) the one,
great fissures, out of which the lava pours in great volume and spreads forth
over wide tracts, often in broad thin sheets; (b) the other, restricted
openings, often pipes, ducts, or limited fissures, from which the extrusion is
usually much less abundant, and hence it more largely congeals near the
orifice, forming cones. Flows from the former constitute massive eruptions;
those from the latter, the more familiar volcanic eruptions. There is no
radical difference between them, and the two classes blend. The extent of
the spreading of lava into thin sheets is due more to the mass and the
fluidity than to the form of the outlet. The stupendous outflows of certain
geologic periods appear to have issued mainly from extended fissures,
doubtless because these better accommodated the outbursting floods.
a. Fissure eruptions.—The chief known fissure eruptions of recent times
are the vast basaltic floods of Iceland. Most of the eruptions of historic
times are of the volcanic type; but at certain times in the past there were
prodigious outpourings, flow following flow until layers thousands of feet
thick covering thousands of square miles were built up. One of these
occurred in Tertiary times in Idaho, Oregon, and Washington, where some
200,000 square miles were covered with sheets of lava, aggregating in
places 2000 feet or more in thickness. Earlier than this, in Cretaceous times,
there were enormous flows on the Deccan plateau of India, covering a like
area to a depth of 4000 to 6000 feet. Still earlier than this, in Keweenawan
times, an even more prolonged succession of lava-flows covered nearly all
the area of the Lake Superior basin, and extended beyond it, and built up a
series of almost incredible thickness, the estimates reaching 15,000 to
25,000 feet. In these cases there is little evidence of explosive or other
violent action. There are few beds of ash, cinders, and similar pyroclastic
material. The inference is, therefore, that the lavas welled out rather quietly
and spread themselves rather fluently over the surrounding country. For the
most part these wide-spreading flows are composed of basic material,
which is more easily fusible and more highly fluent at a given temperature
than the acidic lavas. The latter are more disposed to form thick
embossments near the point of extrusion.
Page 681
Massive outflows of this class constitute by far the greatest phenomena
of the extrusive type, though they are not now the dominant type. It has
been sometimes thought that the more local volcanic type of extrusion
followed the more massive fissure type as a phase of decline; but this has
not been substantiated.
Fig. 457.—Lava-flow near the Jordan craters, Malheur Co., Oregon. Though not of the
gigantic order, it illustrates the general aspect of massive lava-flows. (Russell, U. S. Geol.
Surv.)
b. Volcanic eruptions.—In the types of eruption prevailing at the present
time, the lavas are forced out through ducts or perhaps short fissures or
sections of fissures, and build up cones about the vents, the eruptive action
maintaining craters in the centers of the cones. The essential feature of a
volcano is the issuance of hot rock and gas from a local vent. A mountain is
the usual result, but the mountain is secondary and not usually present in
of the extrusive type, though they are not now the dominant type. It has
been sometimes thought that the more local volcanic type of extrusion
followed the more massive fissure type as a phase of decline; but this has
not been substantiated.
Fig. 457.—Lava-flow near the Jordan craters, Malheur Co., Oregon. Though not of the
gigantic order, it illustrates the general aspect of massive lava-flows. (Russell, U. S. Geol.
Surv.)
b. Volcanic eruptions.—In the types of eruption prevailing at the present
time, the lavas are forced out through ducts or perhaps short fissures or
sections of fissures, and build up cones about the vents, the eruptive action
maintaining craters in the centers of the cones. The essential feature of a
volcano is the issuance of hot rock and gas from a local vent. A mountain is
the usual result, but the mountain is secondary and not usually present in
Page 682
the first stages; the localized eruption is the primary and necessary factor.
The amount of rock matter ejected is not necessarily great. Compared to the
massive extrusions of fissure eruptions, it is usually rather trivial; but the
volcano makes up in demonstrativeness what it lacks in massiveness of
product.
Fig. 458.—The volcano Colima, Mexico, in eruption. March 24, 1903. (José Maria Arreola,
per Frederick Starr.)
c. Intermediate phenomena.—On the border-line between the intrusive
and the extrusive phenomena there are special cases of interest. There
appear to be certain instances in which the intrusion comes so near the
The amount of rock matter ejected is not necessarily great. Compared to the
massive extrusions of fissure eruptions, it is usually rather trivial; but the
volcano makes up in demonstrativeness what it lacks in massiveness of
product.
Fig. 458.—The volcano Colima, Mexico, in eruption. March 24, 1903. (José Maria Arreola,
per Frederick Starr.)
c. Intermediate phenomena.—On the border-line between the intrusive
and the extrusive phenomena there are special cases of interest. There
appear to be certain instances in which the intrusion comes so near the
Page 683
surface as to develop explosive phenomena without the extrusion of lava.
From the nature of the case this is an interpretation rather than a
demonstration. It is certain, however, that occasional violent explosions
take place where no lava comes in sight. This sometimes occurs in old
volcanic formations, and sometimes in regions of undisturbed horizontal
strata. In the former case the phenomena may be due to the intrusion of a
fresh tongue of lava below, or it may be due to the penetration of surface-
waters to hot rocks that have remained uncooled from previous volcanic
action, and the development, by such contact, of a volume of confined
steam sufficient to produce the explosion. A case of this doubtful kind
occurred at Bandai-San in Japan in 1888, where there was a sudden and
violent explosion which blew away a considerable part of the side of a
volcanic mountain which had not been in eruption for at least a thousand
years. The mass and violence of the exploded material was such as to fill
the air with ashes and débris in a fashion altogether similar to a typical
volcanic eruption. A large tract of adjacent country was devastated, and
many lives lost. The whole action, however, was concentrated in the initial
explosion, and within a few hours the cloud of ashes had disappeared and
the phenomenon was ended. An examination of the disrupted area revealed
no signs of liquid lava.
An example of the latter class is Coon Butte in Arizona.[276] This consists
of a rim of fragmental material encircling a crater-like pit from which the
fragments were obviously forced by violent explosion. The pit is in ordinary
sedimentary strata, and the material of the rim is composed of the disrupted
fragments of the sedimentary rock ejected from the pit. There are no signs
of igneous material, but there was igneous action in the vicinity. Fragments
of a meteorite were found on the rim and in the vicinity, but this association
appears to be accidental. Computation shows that the volume of the
material of the rim closely matches the size of the pit. The source of the
explosion is not demonstrable, and it may be an error to connect it with an
intrusion of lava below; but since intrusions rise to various degrees of
nearness to the surface, and in innumerable cases reach the surface, there is
every reason to entertain the conception of a class of intrusions which
develop explosive phenomena by close approach to the surface, without
actually reaching it.
From the nature of the case this is an interpretation rather than a
demonstration. It is certain, however, that occasional violent explosions
take place where no lava comes in sight. This sometimes occurs in old
volcanic formations, and sometimes in regions of undisturbed horizontal
strata. In the former case the phenomena may be due to the intrusion of a
fresh tongue of lava below, or it may be due to the penetration of surface-
waters to hot rocks that have remained uncooled from previous volcanic
action, and the development, by such contact, of a volume of confined
steam sufficient to produce the explosion. A case of this doubtful kind
occurred at Bandai-San in Japan in 1888, where there was a sudden and
violent explosion which blew away a considerable part of the side of a
volcanic mountain which had not been in eruption for at least a thousand
years. The mass and violence of the exploded material was such as to fill
the air with ashes and débris in a fashion altogether similar to a typical
volcanic eruption. A large tract of adjacent country was devastated, and
many lives lost. The whole action, however, was concentrated in the initial
explosion, and within a few hours the cloud of ashes had disappeared and
the phenomenon was ended. An examination of the disrupted area revealed
no signs of liquid lava.
An example of the latter class is Coon Butte in Arizona.[276] This consists
of a rim of fragmental material encircling a crater-like pit from which the
fragments were obviously forced by violent explosion. The pit is in ordinary
sedimentary strata, and the material of the rim is composed of the disrupted
fragments of the sedimentary rock ejected from the pit. There are no signs
of igneous material, but there was igneous action in the vicinity. Fragments
of a meteorite were found on the rim and in the vicinity, but this association
appears to be accidental. Computation shows that the volume of the
material of the rim closely matches the size of the pit. The source of the
explosion is not demonstrable, and it may be an error to connect it with an
intrusion of lava below; but since intrusions rise to various degrees of
nearness to the surface, and in innumerable cases reach the surface, there is
every reason to entertain the conception of a class of intrusions which
develop explosive phenomena by close approach to the surface, without
actually reaching it.
Page 684
Fig. 459.—Photograph of a portion of the moon taken at Lick Observatory.
Lunar craters.—There are grounds for thinking that the remarkable
craters of the moon, assuming that they are truly volcanic,[277] may belong to
this class, for they are very similar to the Coon Butte pit. The capacities of
the lunar craters, so far as they can be estimated, seem to equal, if they do
not in many cases exceed, the volume of matter in their rims. They do not
appear usually to be great cones of accumulated material with relatively
small craters, like the typical products of terrestrial volcanoes. Besides,
there are no clear evidences of lava-streams. The radiating tracts once
interpreted as such have been shown by increased telescopic power and the
Lunar craters.—There are grounds for thinking that the remarkable
craters of the moon, assuming that they are truly volcanic,[277] may belong to
this class, for they are very similar to the Coon Butte pit. The capacities of
the lunar craters, so far as they can be estimated, seem to equal, if they do
not in many cases exceed, the volume of matter in their rims. They do not
appear usually to be great cones of accumulated material with relatively
small craters, like the typical products of terrestrial volcanoes. Besides,
there are no clear evidences of lava-streams. The radiating tracts once
interpreted as such have been shown by increased telescopic power and the
Page 685
resources of photography to be at least something other than lava-streams.
They are vaguely defined tracts which run over heights and depths
indifferently, and are plausibly interpreted as lines of débris projected to
extraordinary distances because of the absence of a lunar atmosphere, and
because of the low force of the moon’s gravity. Since the moon now has no
appreciable atmosphere or surface-waters, and since it is doubtful whether it
ever possessed either on account of its probable inability to hold
atmospheric gases or the vapor of water in the form of an envelope about it,
owing to its low gravity, there is reason to suppose that the external matter
of the moon derived from the explosions of the multitude of lunar
volcanoes would remain in a loose, incoherent condition, from the absence
of dissolving and cementing agencies. It is reasonable to suppose that lava-
tongues arising from the deeper interior would have a higher specific
gravity, even in their heated condition, than this porous covering of the
moon, and that therefore they would almost universally become intrusions
rather than extrusions, or at most they would not rise beyond the bottom of
the craters they had produced by explosion. This seems to furnish at least a
plausible explanation of the prevailing differences between the large lunar
craters encircled by mere rims and the much smaller terrestrial craters
seated in relatively large cones.
VOLCANOES.
Number of volcanoes.—It is impracticable to state exactly the number
of volcanoes that are active at the present time, because most volcanoes are
periodic, and become active at more or less distant periods, and it is
impossible to say whether a given volcano that may be now quiescent has
really become extinct or is only enjoying its customary period of rest. It is
quite safe to include at least 300 in the active list, and the number may
reach 350 or more. The numbers that have been active so recently that their
cones have not been entirely worn away is several times as great.
Distribution of Volcanoes.
1. In time.—In the earliest known ages igneous action appears to have
been very general, if not practically universal. No area of the earliest
(Archean) rocks is now known which is not formed chiefly of rocks that
They are vaguely defined tracts which run over heights and depths
indifferently, and are plausibly interpreted as lines of débris projected to
extraordinary distances because of the absence of a lunar atmosphere, and
because of the low force of the moon’s gravity. Since the moon now has no
appreciable atmosphere or surface-waters, and since it is doubtful whether it
ever possessed either on account of its probable inability to hold
atmospheric gases or the vapor of water in the form of an envelope about it,
owing to its low gravity, there is reason to suppose that the external matter
of the moon derived from the explosions of the multitude of lunar
volcanoes would remain in a loose, incoherent condition, from the absence
of dissolving and cementing agencies. It is reasonable to suppose that lava-
tongues arising from the deeper interior would have a higher specific
gravity, even in their heated condition, than this porous covering of the
moon, and that therefore they would almost universally become intrusions
rather than extrusions, or at most they would not rise beyond the bottom of
the craters they had produced by explosion. This seems to furnish at least a
plausible explanation of the prevailing differences between the large lunar
craters encircled by mere rims and the much smaller terrestrial craters
seated in relatively large cones.
VOLCANOES.
Number of volcanoes.—It is impracticable to state exactly the number
of volcanoes that are active at the present time, because most volcanoes are
periodic, and become active at more or less distant periods, and it is
impossible to say whether a given volcano that may be now quiescent has
really become extinct or is only enjoying its customary period of rest. It is
quite safe to include at least 300 in the active list, and the number may
reach 350 or more. The numbers that have been active so recently that their
cones have not been entirely worn away is several times as great.
Distribution of Volcanoes.
1. In time.—In the earliest known ages igneous action appears to have
been very general, if not practically universal. No area of the earliest
(Archean) rocks is now known which is not formed chiefly of rocks that
Page 686
appear to have been either intruded or extruded. Rocks which can
reasonably be assigned to the hypothetical molten globe, if there be such,
are not here included. It is probable that the surface of the early earth was as
thickly occupied with points of extrusion as the surface of the moon appears
to be. In the ages between the Archean and the present, the distribution of
volcanic action over the surface seems to have been in a general way much
what it is to-day; that is, certain areas were volcanically active at times,
while other and larger areas were measurably free from any outward
expressions of igneous action. This is not equally true of all ages, as will be
seen in the historical studies that follow. There were periods when volcanic
activity seems to have been widespread and energetic, and others when it
was limited both in amount and distribution. The known facts do not
indicate a steady decline in volcanic activity, but rather a periodicity; at
least this is so for the portion of the globe that is now well enough known
geologically to warrant conclusions. One of the greatest of the volcanic
periods falls within the Cenozoic era, just preceding the present geological
period, and the volcanic activity of the present is perhaps but a declining
phase of that time.
2. Relative to land and sea.—At present the active volcanoes are chiefly
distributed about the borders of the continents, and, less notably, within the
great oceanic basins. On this account the sea has often been supposed to
have some connection with volcanic action, and the presence of chlorine in
the volcanic emanations has been cited in support of this position. When
critically examined, however, the argument from distribution is not very
strong; for the volcanoes are not distributed equally or proportionately
about the several oceans, as if dependent on them. Volcanoes are especially
numerous around and within the Pacific, the greatest of the oceans, and this
might seem a favorable instance, but they are also numerous around and
within the Mediterranean, a relatively small body of water. Volcanoes are
not especially abundant in or about the margins of the Atlantic.
reasonably be assigned to the hypothetical molten globe, if there be such,
are not here included. It is probable that the surface of the early earth was as
thickly occupied with points of extrusion as the surface of the moon appears
to be. In the ages between the Archean and the present, the distribution of
volcanic action over the surface seems to have been in a general way much
what it is to-day; that is, certain areas were volcanically active at times,
while other and larger areas were measurably free from any outward
expressions of igneous action. This is not equally true of all ages, as will be
seen in the historical studies that follow. There were periods when volcanic
activity seems to have been widespread and energetic, and others when it
was limited both in amount and distribution. The known facts do not
indicate a steady decline in volcanic activity, but rather a periodicity; at
least this is so for the portion of the globe that is now well enough known
geologically to warrant conclusions. One of the greatest of the volcanic
periods falls within the Cenozoic era, just preceding the present geological
period, and the volcanic activity of the present is perhaps but a declining
phase of that time.
2. Relative to land and sea.—At present the active volcanoes are chiefly
distributed about the borders of the continents, and, less notably, within the
great oceanic basins. On this account the sea has often been supposed to
have some connection with volcanic action, and the presence of chlorine in
the volcanic emanations has been cited in support of this position. When
critically examined, however, the argument from distribution is not very
strong; for the volcanoes are not distributed equally or proportionately
about the several oceans, as if dependent on them. Volcanoes are especially
numerous around and within the Pacific, the greatest of the oceans, and this
might seem a favorable instance, but they are also numerous around and
within the Mediterranean, a relatively small body of water. Volcanoes are
not especially abundant in or about the margins of the Atlantic.
Page 687
Fig. 460.—Volcanoes in the Pacific. Jones Relief Globe. (Photo. by R. T. Chamberlin.)
If volcanoes were dependent upon proximity to the sea, the relation
should be close in the past as well as in the present, but this does not seem
to be true. There has recently been much volcanic activity in the plateau
region of western America at long distances from the Pacific basin. Even on
the plains east of the Rocky Mountains notable volcanic action took place.
There were also volcanoes in the interior of Asia and of Africa.
3. Relative to crustal deformations.—The distribution of present and
recent volcanoes is much more suggestively associated with those portions
of the crust that have undergone notable changes in position in
comparatively recent times. The great “world-ridge” stretching from Cape
Horn to Alaska and thence onwards along the east coast of Asia is a striking
instance, for it is dotted throughout with active and recently extinct
volcanoes. The tortuous zone of mountainous wrinkles that borders the
Mediterranean and stretches thence eastward to the Polynesian Islands is
another notable volcanic tract. These two belts include the greater number
If volcanoes were dependent upon proximity to the sea, the relation
should be close in the past as well as in the present, but this does not seem
to be true. There has recently been much volcanic activity in the plateau
region of western America at long distances from the Pacific basin. Even on
the plains east of the Rocky Mountains notable volcanic action took place.
There were also volcanoes in the interior of Asia and of Africa.
3. Relative to crustal deformations.—The distribution of present and
recent volcanoes is much more suggestively associated with those portions
of the crust that have undergone notable changes in position in
comparatively recent times. The great “world-ridge” stretching from Cape
Horn to Alaska and thence onwards along the east coast of Asia is a striking
instance, for it is dotted throughout with active and recently extinct
volcanoes. The tortuous zone of mountainous wrinkles that borders the
Mediterranean and stretches thence eastward to the Polynesian Islands is
another notable volcanic tract. These two belts include the greater number
Page 688
of existing and recent volcanoes on the land, while the great basins
associated with them embrace the chief oceanic volcanoes.
Fig. 461.—Active volcanic area at the junction of the continental segments of North and
South America, and of the abysmal segments of the Atlantic and Pacific. Jones Relief
Globe. (Photo. by R. T. Chamberlin.)
There is perhaps some significance in the fact that the most active
regions of vulcanism to-day lie at the angular junctions of the great earth-
segments. The Antillean and Central American volcanic region, that has
recently been so demonstrative, lies where the southern angle of the North
American continental block joins the northern angle of the South American
continental block, and where the western angle of the North Atlantic
abysmal segment closely approaches one of the eastern angles of the great
Pacific abysmal segment. The complex and very active Java-Philippine
volcanic region lies where the southeastern angle of the great Asian
segment projects toward the Australian block, and where the western angle
associated with them embrace the chief oceanic volcanoes.
Fig. 461.—Active volcanic area at the junction of the continental segments of North and
South America, and of the abysmal segments of the Atlantic and Pacific. Jones Relief
Globe. (Photo. by R. T. Chamberlin.)
There is perhaps some significance in the fact that the most active
regions of vulcanism to-day lie at the angular junctions of the great earth-
segments. The Antillean and Central American volcanic region, that has
recently been so demonstrative, lies where the southern angle of the North
American continental block joins the northern angle of the South American
continental block, and where the western angle of the North Atlantic
abysmal segment closely approaches one of the eastern angles of the great
Pacific abysmal segment. The complex and very active Java-Philippine
volcanic region lies where the southeastern angle of the great Asian
segment projects toward the Australian block, and where the western angle
Page 689
of the Pacific block approaches the northeastern angle of the Indian oceanic
segment. The active Alaskan volcanic area lies at the angles of the North
American, Asian, Pacific, and Arctic segments. The Mediterranean volcanic
area falls less notably under this generalization, but it lies where the
continental blocks of Europe and Africa come into peculiar relations to each
other on either side of the remarkable Mediterranean trough. The eastern
angle of the North Atlantic segment is near by, but not in very close
relations. The Icelandic region, small but vigorous, lies near the junction of
the North American, European, North Atlantic, and Arctic segments, and
the New Zealand volcanic region is somewhat less closely related to the
approach of the Australian, Antarctic, Pacific, and Southern oceanic
segments. Nearly all of these angular conjunctions involve two depressed
segments joining two relatively elevated segments. This relationship
suggests a causal connection between the intensified movements at these
angular conjunctions and the intensified volcanic action of these regions.
There are enough volcanoes, however, that do not fall into these groups, or
apparently into any other grouping, to suggest that the development of
volcanoes is not wholly dependent on any surface relationship, but that it is
connected with deep-seated causes that are indeed modified, but not wholly
controlled, by surface conditions, or even by the movements of the master
segments of the earth’s crust.
segment. The active Alaskan volcanic area lies at the angles of the North
American, Asian, Pacific, and Arctic segments. The Mediterranean volcanic
area falls less notably under this generalization, but it lies where the
continental blocks of Europe and Africa come into peculiar relations to each
other on either side of the remarkable Mediterranean trough. The eastern
angle of the North Atlantic segment is near by, but not in very close
relations. The Icelandic region, small but vigorous, lies near the junction of
the North American, European, North Atlantic, and Arctic segments, and
the New Zealand volcanic region is somewhat less closely related to the
approach of the Australian, Antarctic, Pacific, and Southern oceanic
segments. Nearly all of these angular conjunctions involve two depressed
segments joining two relatively elevated segments. This relationship
suggests a causal connection between the intensified movements at these
angular conjunctions and the intensified volcanic action of these regions.
There are enough volcanoes, however, that do not fall into these groups, or
apparently into any other grouping, to suggest that the development of
volcanoes is not wholly dependent on any surface relationship, but that it is
connected with deep-seated causes that are indeed modified, but not wholly
controlled, by surface conditions, or even by the movements of the master
segments of the earth’s crust.
Page 690
Fig. 462.—Active volcanic area at the junction of the continental segments of Asia and
Australia, and the abysmal segments of the Pacific and Indian oceans. Jones Relief
Globe. (Photo. by R. T. Chamberlin.)
4. In latitude.—The distribution of volcanoes appears to have no
specific relation to latitude. Mounts Erebus and Terror, amid the ice-mantle
of Antarctica, and Mount Hecla in Iceland, as well as the numerous
volcanoes of the Aleutian chain, give no ground for supposing that
volcanoes shun the frigid zones. On the other hand, the numerous volcanoes
of the equatorial zone do not imply that they avoid the torrid belt. Their
distribution appears to be independent of latitude. This is not cited because
of any supposed effects of external temperature, for that must be trivial, but
because it bears on the question whether strains are now arising from the
supposed slackening of the earth’s rotation, which have any connection
with volcanic action. If the oblateness of the earth is decreasing, the
equatorial belt must be sinking and growing shorter, and hence must be
under lateral pressure, while the polar caps must be rising, and increasing
their curvatures, and should be under tension. These conditions, if real,
might be supposed to have something to do with the extrusion of lava.
Australia, and the abysmal segments of the Pacific and Indian oceans. Jones Relief
Globe. (Photo. by R. T. Chamberlin.)
4. In latitude.—The distribution of volcanoes appears to have no
specific relation to latitude. Mounts Erebus and Terror, amid the ice-mantle
of Antarctica, and Mount Hecla in Iceland, as well as the numerous
volcanoes of the Aleutian chain, give no ground for supposing that
volcanoes shun the frigid zones. On the other hand, the numerous volcanoes
of the equatorial zone do not imply that they avoid the torrid belt. Their
distribution appears to be independent of latitude. This is not cited because
of any supposed effects of external temperature, for that must be trivial, but
because it bears on the question whether strains are now arising from the
supposed slackening of the earth’s rotation, which have any connection
with volcanic action. If the oblateness of the earth is decreasing, the
equatorial belt must be sinking and growing shorter, and hence must be
under lateral pressure, while the polar caps must be rising, and increasing
their curvatures, and should be under tension. These conditions, if real,
might be supposed to have something to do with the extrusion of lava.
Page 691
Nothing in the present or the past distribution of igneous action seems to
afford much support to this hypothetical inference.
5. In curved lines.—In the Antilles, the Aleutian Islands, the Kurile
Islands, and in other instances, there is a notable linear arrangement of
volcanoes with appreciable curvature. It has been noted that the convexity
of the curves is turned toward the adjacent ocean. In some cases, however,
there is a notable linear arrangement without appreciable curvature, as in
the Hawaiian range, in the recently extinct line of cones of the Cascade
Range, and in others. Less often, volcanoes are bunched irregularly, as in
some of the groups of volcanic islands of the Pacific (Fig. 460).
Relations of Volcanoes.
1. Relations to rising and sinking surfaces.—So far as observations
cover this point, the area immediately adjacent to active volcanoes is rising
(Dutton). This is shown by raised beaches, terraces, coral deposits, etc.
Whether this is wholly due to the expansional effect of the heating of the
subterrane by the rising lava, or whether it has a wider significance, is not
known. If a broader view is taken, it does not appear that there are sufficient
data to connect volcanic action exclusively with either the rising or the
sinking of the general surface. It is certain that the great mountain ranges
and plateaus in which so much of the more recent volcanic action has taken
place have been recently elevated relatively, but they have also undergone
more or less of oscillation, involving some relative depression. The question
whether the Pacific basin as a whole has been relatively elevated or
depressed in modern times is a mooted one. Darwin[278] and Dana,[279] as the
result of their early studies on its coral deposits and on other phenomena,
concluded that the Pacific was a sinking area, but this view has been
recently challenged by Murray[280] and Agassiz[281] with at least some
measure of success. From the fiords on the borders of the Pacific and other
physical phenomena, the inference has been drawn that relative sinking of
the land has recently taken place. Raised beaches on the coasts are
interpreted as indicating a relative rise of the land or a sinking of some
ocean basin, for the withdrawal of the waters can only be the result of
increasing the capacity of the oceanic basin as a whole. The most probable
view is that the general areas of present and recent volcanic action are
partly rising areas and partly sinking areas, and that movement of either
afford much support to this hypothetical inference.
5. In curved lines.—In the Antilles, the Aleutian Islands, the Kurile
Islands, and in other instances, there is a notable linear arrangement of
volcanoes with appreciable curvature. It has been noted that the convexity
of the curves is turned toward the adjacent ocean. In some cases, however,
there is a notable linear arrangement without appreciable curvature, as in
the Hawaiian range, in the recently extinct line of cones of the Cascade
Range, and in others. Less often, volcanoes are bunched irregularly, as in
some of the groups of volcanic islands of the Pacific (Fig. 460).
Relations of Volcanoes.
1. Relations to rising and sinking surfaces.—So far as observations
cover this point, the area immediately adjacent to active volcanoes is rising
(Dutton). This is shown by raised beaches, terraces, coral deposits, etc.
Whether this is wholly due to the expansional effect of the heating of the
subterrane by the rising lava, or whether it has a wider significance, is not
known. If a broader view is taken, it does not appear that there are sufficient
data to connect volcanic action exclusively with either the rising or the
sinking of the general surface. It is certain that the great mountain ranges
and plateaus in which so much of the more recent volcanic action has taken
place have been recently elevated relatively, but they have also undergone
more or less of oscillation, involving some relative depression. The question
whether the Pacific basin as a whole has been relatively elevated or
depressed in modern times is a mooted one. Darwin[278] and Dana,[279] as the
result of their early studies on its coral deposits and on other phenomena,
concluded that the Pacific was a sinking area, but this view has been
recently challenged by Murray[280] and Agassiz[281] with at least some
measure of success. From the fiords on the borders of the Pacific and other
physical phenomena, the inference has been drawn that relative sinking of
the land has recently taken place. Raised beaches on the coasts are
interpreted as indicating a relative rise of the land or a sinking of some
ocean basin, for the withdrawal of the waters can only be the result of
increasing the capacity of the oceanic basin as a whole. The most probable
view is that the general areas of present and recent volcanic action are
partly rising areas and partly sinking areas, and that movement of either
Page 692
kind may be connected with the extrusion of the lavas. The rising and
sinking are but complementary phases of a deformation of the earth’s body,
and involve a readjustment of stresses within the body of the earth. These
stresses are possibly an essential factor in eruptions.
2. Relations to one another.—A most significant feature of volcanic
action is the degree of concurrence or of independence of action in adjacent
volcanoes. In some instances they act as though in sympathy, as in the
recent outburst in Martinique and Saint Vincent, and the concurrent
symptoms of activity in other places. On the other hand, the independence
of neighboring vents is sometimes extraordinary. The group of volcanoes
near the center of the Mediterranean, of which Vesuvius and Etna are the
most conspicuous examples, usually act with measurable independence of
one another, an eruption in the one not being habitually coincident with an
eruption in the others. But the most conspicuous instance of independence
is found in the great craters of Mauna Loa and Kilauea in Hawaii. They are
only about twenty miles apart, the one on the top and the other on the side
of the same great mountain mass. The crater of Mauna Loa is about 10,000
feet higher than the crater of Kilauea, and yet, while the latter has been in
constant activity as far back as its history is known, the former is periodic.
The case is the more remarkable because of the greatness of the ejections.
The outflow of Mauna Loa in 1885 formed a stream from three to ten miles
in width, and forty-five miles in length, with a probable average thickness
of 100 feet, and some of its other outflows were of nearly equal greatness;
indeed its outflows are among the most massive that have issued from
volcanoes in recent times. Besides this massiveness there have been
extraordinary movements of the lava within the crater, if the testimony of
witnesses may be trusted. But throughout these great movements in the
higher crater, the lava-column of Kilauea, 10,000 feet lower, continued its
quiet action without sensible effects from its boisterous neighbor. The
bearing of such extraordinary independence upon the sources of volcanic
action is very cogent, for the lavas are of the same type, both being basalts,
that of Mauna Loa being notably basic and probably as high in specific
gravity as that in Kilauea. No difference in specific gravity that could at all
account for a difference in height of 10,000 feet can be presumed, unless
their ducts remain separate to extraordinary depths. Nor does it appear
possible that a superior amount of gas within the column of Mauna Loa
could account for such an extraordinary difference in height, for the
sinking are but complementary phases of a deformation of the earth’s body,
and involve a readjustment of stresses within the body of the earth. These
stresses are possibly an essential factor in eruptions.
2. Relations to one another.—A most significant feature of volcanic
action is the degree of concurrence or of independence of action in adjacent
volcanoes. In some instances they act as though in sympathy, as in the
recent outburst in Martinique and Saint Vincent, and the concurrent
symptoms of activity in other places. On the other hand, the independence
of neighboring vents is sometimes extraordinary. The group of volcanoes
near the center of the Mediterranean, of which Vesuvius and Etna are the
most conspicuous examples, usually act with measurable independence of
one another, an eruption in the one not being habitually coincident with an
eruption in the others. But the most conspicuous instance of independence
is found in the great craters of Mauna Loa and Kilauea in Hawaii. They are
only about twenty miles apart, the one on the top and the other on the side
of the same great mountain mass. The crater of Mauna Loa is about 10,000
feet higher than the crater of Kilauea, and yet, while the latter has been in
constant activity as far back as its history is known, the former is periodic.
The case is the more remarkable because of the greatness of the ejections.
The outflow of Mauna Loa in 1885 formed a stream from three to ten miles
in width, and forty-five miles in length, with a probable average thickness
of 100 feet, and some of its other outflows were of nearly equal greatness;
indeed its outflows are among the most massive that have issued from
volcanoes in recent times. Besides this massiveness there have been
extraordinary movements of the lava within the crater, if the testimony of
witnesses may be trusted. But throughout these great movements in the
higher crater, the lava-column of Kilauea, 10,000 feet lower, continued its
quiet action without sensible effects from its boisterous neighbor. The
bearing of such extraordinary independence upon the sources of volcanic
action is very cogent, for the lavas are of the same type, both being basalts,
that of Mauna Loa being notably basic and probably as high in specific
gravity as that in Kilauea. No difference in specific gravity that could at all
account for a difference in height of 10,000 feet can be presumed, unless
their ducts remain separate to extraordinary depths. Nor does it appear
possible that a superior amount of gas within the column of Mauna Loa
could account for such an extraordinary difference in height, for the
Page 693
hydrostatic pressure of such a column is not far from 10,000 pounds to the
square inch. Even if the difference in the heights of the columns could be
explained by differences in specific gravity, the agitation of the one should
be communicated to the other, and an outflow of the one, particularly an
outflow by a breakage through its walls sufficient to lower its surface
hundreds of feet, as has repeatedly occurred in Kilauea, should change the
surface of the other proportionately, if they were in hydrostatic equilibrium.
It seems a necessary inference, therefore, that the two lava-columns have no
connection with each other or with a common reservoir. The tops of some
lava-columns stand about 20,000 feet above the sea, while others emerge on
the sea-bottom far below sea-level. The total vertical range is, therefore,
probably between 30,000 and 40,000 feet, a difference which tells its own
story as to their relative independence.
Fig. 463.—Surface of lava-flow of 1881, from Mauna Loa, as seen back of Hilo, Hawaii.
(Photo. by Calvin.)
square inch. Even if the difference in the heights of the columns could be
explained by differences in specific gravity, the agitation of the one should
be communicated to the other, and an outflow of the one, particularly an
outflow by a breakage through its walls sufficient to lower its surface
hundreds of feet, as has repeatedly occurred in Kilauea, should change the
surface of the other proportionately, if they were in hydrostatic equilibrium.
It seems a necessary inference, therefore, that the two lava-columns have no
connection with each other or with a common reservoir. The tops of some
lava-columns stand about 20,000 feet above the sea, while others emerge on
the sea-bottom far below sea-level. The total vertical range is, therefore,
probably between 30,000 and 40,000 feet, a difference which tells its own
story as to their relative independence.
Fig. 463.—Surface of lava-flow of 1881, from Mauna Loa, as seen back of Hilo, Hawaii.
(Photo. by Calvin.)
Page 694
3. Unimportant coincidences.—Eruptions seem to be somewhat more
liable to occur at times of high atmospheric pressure than at low, doubtless
because the increased atmospheric weight on a large area of the adjacent
crust aids in forcing out the lava or the volcanic gases. This can only be
effective when other forces have almost accomplished the result, and would
doubtless have completed it a little later had not the atmospheric wave
supplied the little remaining pressure needed. Eruption seems also to be
more common when the tidal strains favor it, for like reasons. In the same
class are probably to be put the effects of heavy rains, whether they act by
gravity or by giving rise to steam. Such agencies are to be regarded as mere
incidents of no moment in the real causation of vulcanism, but of some
value in determining the precise moment of action. This is not to be
understood as inconsistent with the view that the periodic stresses of the
body-tides of the earth are important factors in vulcanism, as elsewhere
explained, but merely that the special time of surface-eruption is only
incidentally connected with the water-tides.
Fig. 464.—Crater of Kilauea.
Periodicity.—Most volcanoes are periodic in their stages of action. Long
dormant periods intervene between eruptive periods. Volcanoes supposed to
be extinct occasionally awaken with terrific violence. Sometimes also they
awaken quietly. This larger periodicity yet awaits an explanation, but it very
liable to occur at times of high atmospheric pressure than at low, doubtless
because the increased atmospheric weight on a large area of the adjacent
crust aids in forcing out the lava or the volcanic gases. This can only be
effective when other forces have almost accomplished the result, and would
doubtless have completed it a little later had not the atmospheric wave
supplied the little remaining pressure needed. Eruption seems also to be
more common when the tidal strains favor it, for like reasons. In the same
class are probably to be put the effects of heavy rains, whether they act by
gravity or by giving rise to steam. Such agencies are to be regarded as mere
incidents of no moment in the real causation of vulcanism, but of some
value in determining the precise moment of action. This is not to be
understood as inconsistent with the view that the periodic stresses of the
body-tides of the earth are important factors in vulcanism, as elsewhere
explained, but merely that the special time of surface-eruption is only
incidentally connected with the water-tides.
Fig. 464.—Crater of Kilauea.
Periodicity.—Most volcanoes are periodic in their stages of action. Long
dormant periods intervene between eruptive periods. Volcanoes supposed to
be extinct occasionally awaken with terrific violence. Sometimes also they
awaken quietly. This larger periodicity yet awaits an explanation, but it very
Page 695
likely means a temporary exhaustion of the supply of gas or of lava, or of
both, to which the active stage is due.
Formation of Cones.
Lava-cones.—The lava usually flows away from the vent in short
streams which solidify before running far. As the lava-streams flow in
different directions at different times, the total effect is a low cone formed
of radiating tongues surrounding the point of exit. Occasionally the streams
run a dozen or a score of miles, but such cases, except in the gigantic
volcanoes of Hawaii and a few others, are rare. Often the streams congeal
before they reach much beyond the base of the cone, and quite often while
they are yet on its slope. So far, therefore, as the volcanic cone is formed of
lava, it has a radiate structure made up of a succession of congealed lava-
streams. In these cases the slopes are low, because the fluidity of the lava
prevents the development of high gradients. It is, however, rather the
exception than the rule, that the cone is made up mainly of lava-streams,
though the great Hawaiian volcanoes are of this class.
Fig. 465.—Typical cinder-cone, Clayton valley, Cal. (Turner, U. S. Geol. Surv.)
Cinder-cones.—The larger portion of the lava blown into the air by the
expanding gas-bubbles falls back in the immediate vicinity of the vent and
both, to which the active stage is due.
Formation of Cones.
Lava-cones.—The lava usually flows away from the vent in short
streams which solidify before running far. As the lava-streams flow in
different directions at different times, the total effect is a low cone formed
of radiating tongues surrounding the point of exit. Occasionally the streams
run a dozen or a score of miles, but such cases, except in the gigantic
volcanoes of Hawaii and a few others, are rare. Often the streams congeal
before they reach much beyond the base of the cone, and quite often while
they are yet on its slope. So far, therefore, as the volcanic cone is formed of
lava, it has a radiate structure made up of a succession of congealed lava-
streams. In these cases the slopes are low, because the fluidity of the lava
prevents the development of high gradients. It is, however, rather the
exception than the rule, that the cone is made up mainly of lava-streams,
though the great Hawaiian volcanoes are of this class.
Fig. 465.—Typical cinder-cone, Clayton valley, Cal. (Turner, U. S. Geol. Surv.)
Cinder-cones.—The larger portion of the lava blown into the air by the
expanding gas-bubbles falls back in the immediate vicinity of the vent and
Page 696
builds up a cinder-cone. From the nature of the case, this often takes on a
beautiful symmetry and assumes a steep slope (Fig. 465). The ragged
cinders lend themselves readily to the formation of an acute cone, quite
different from the flatter cone formed by lavas. Sometimes the cinders are
still plastic when they fall, and weld themselves together and hold their
places even on very steep slopes, but usually they have already hardened
before they reach the surface.
Fig. 466.—Spatter-cone and cavern. Kilauea, Hawaii. (Photo. by Libbey.)
beautiful symmetry and assumes a steep slope (Fig. 465). The ragged
cinders lend themselves readily to the formation of an acute cone, quite
different from the flatter cone formed by lavas. Sometimes the cinders are
still plastic when they fall, and weld themselves together and hold their
places even on very steep slopes, but usually they have already hardened
before they reach the surface.
Fig. 466.—Spatter-cone and cavern. Kilauea, Hawaii. (Photo. by Libbey.)
Page 697
Fig. 467.—Hollow spatter-cone. Oregon. (Russell, U. S. Geol. Surv.)
Subordinate cones.—Small or temporary vents formed as offshoots
from the main vents often give rise to secondary or “parasitic” cones. These
are sometimes numerous, as in the case of Etna, and they may be so
important that the mountain becomes a compound cone. A still more
subordinate variety consists of “spatter-cones” formed by small mildly
explosive vents that spatter forth little dabs of lava which form chimneys, or
cones, and sometimes completely curved domes over vents (Figs. 466 and
467). Spatter-cones often arise from the lava-flows themselves.
Composite cones.—From most existing volcanoes there issue both lava-
flows and fragmental ejecta, and the resulting cones are composite in
material. The lava more frequently breaks through the side of the cone than
overflows its summit, and this gives rise to irregularities of form and
structure. The cones are also subject to partial destruction both by the
outbursts of lava and by the explosions, and perhaps also by migration of
the vents. As a result, many volcanic regions show old, partially destroyed
craters, together with new and more perfect ones, and the history of
Subordinate cones.—Small or temporary vents formed as offshoots
from the main vents often give rise to secondary or “parasitic” cones. These
are sometimes numerous, as in the case of Etna, and they may be so
important that the mountain becomes a compound cone. A still more
subordinate variety consists of “spatter-cones” formed by small mildly
explosive vents that spatter forth little dabs of lava which form chimneys, or
cones, and sometimes completely curved domes over vents (Figs. 466 and
467). Spatter-cones often arise from the lava-flows themselves.
Composite cones.—From most existing volcanoes there issue both lava-
flows and fragmental ejecta, and the resulting cones are composite in
material. The lava more frequently breaks through the side of the cone than
overflows its summit, and this gives rise to irregularities of form and
structure. The cones are also subject to partial destruction both by the
outbursts of lava and by the explosions, and perhaps also by migration of
the vents. As a result, many volcanic regions show old, partially destroyed
craters, together with new and more perfect ones, and the history of
Page 698
volcanic action in a region may often be read in the succession of cone
formations.
The form of the cone, when composed chiefly of lava, is also affected by
the mass of the outflow and by its fluidity. The larger the outflow at a given
time, other things being equal, the wider it distributes itself and the flatter is
the cone. As a rule, the basic lavas are more fluid than the acidic, and the
cones of basic lavas are flatter than the cones of acidic lavas.
Extra-cone distribution.—In violent eruptions, the steam, accompanied
with much ash, is shot up to great heights, often rolling outwards in
cumulus or cauliflower-like forms (Fig. 458). In the more violent
explosions these columns are projected several miles. In the phenomenal
case of Krakatoa the projection was estimated at seventeen miles. The
steam, by reason of its great expansion and its contact with the colder
regions of the upper air, is quickly condensed, and prodigious floods of rain
frequently accompany the eruption. This rain, carrying down a portion of
the ash and gathering up much that had previously fallen, gives rise to mud-
flows, which in some cases constitute a large part of the final deposit. These
mud-flows chiefly lodge on the lower slopes of the volcano or adjacent to
its base, and give rise to rather flat cones, sometimes designated as tufa-
cones to distinguish them from cinder-cones formed by the direct fall of
fragmental material. Mud-flows appear also to be formed by the ejection of
mud and water that had gathered in quiescent craters during intervals
between stages of eruption.
A portion of the finer exploded material floats away in the air to greater
or less distances, and forms widespread tufa-deposits. In. some cases beds
of volcanic ash of appreciable thickness (as those of Nebraska)[282] are found
far from any known volcanic center. The extremely fine ash from the great
explosion of Krakatoa floated several times around the earth in the
equatorial belt and spread northward into the temperate zones.
formations.
The form of the cone, when composed chiefly of lava, is also affected by
the mass of the outflow and by its fluidity. The larger the outflow at a given
time, other things being equal, the wider it distributes itself and the flatter is
the cone. As a rule, the basic lavas are more fluid than the acidic, and the
cones of basic lavas are flatter than the cones of acidic lavas.
Extra-cone distribution.—In violent eruptions, the steam, accompanied
with much ash, is shot up to great heights, often rolling outwards in
cumulus or cauliflower-like forms (Fig. 458). In the more violent
explosions these columns are projected several miles. In the phenomenal
case of Krakatoa the projection was estimated at seventeen miles. The
steam, by reason of its great expansion and its contact with the colder
regions of the upper air, is quickly condensed, and prodigious floods of rain
frequently accompany the eruption. This rain, carrying down a portion of
the ash and gathering up much that had previously fallen, gives rise to mud-
flows, which in some cases constitute a large part of the final deposit. These
mud-flows chiefly lodge on the lower slopes of the volcano or adjacent to
its base, and give rise to rather flat cones, sometimes designated as tufa-
cones to distinguish them from cinder-cones formed by the direct fall of
fragmental material. Mud-flows appear also to be formed by the ejection of
mud and water that had gathered in quiescent craters during intervals
between stages of eruption.
A portion of the finer exploded material floats away in the air to greater
or less distances, and forms widespread tufa-deposits. In. some cases beds
of volcanic ash of appreciable thickness (as those of Nebraska)[282] are found
far from any known volcanic center. The extremely fine ash from the great
explosion of Krakatoa floated several times around the earth in the
equatorial belt and spread northward into the temperate zones.
Page 699
Fig. 468.—Mt. Shasta, a typical extinct cone, furrowed by erosion, but retaining its general
form. (Diller, U. S. Geol. Surv.)
LAVAS.
Their nature.—In the chapter on the Origin and Descent of Rocks, the
nature of lavas and of the rocks derived from them has been discussed
(Chapter VII). In view of prevalent misconceptions, it may be repeated, for
the sake of emphasis, that lavas are mutual solutions of mineral matter in
mineral matter, rather than simply melted rock. Into this mutual solution
there enter not only rock materials, but gases. The distinction between
mutual solutions and simple molten rock cannot be rigorously made, but it
is at least essential to know that the minerals do not necessarily crystallize
from lavas in the order of their melting temperatures, or in any uniform
order, but rather in the order in which saturation of the several mineral
constituents happens to be reached in the given mutual solution. Thus
quartz, which has a very high melting-point, is often one of the last minerals
to crystallize. The mutual solutions are exceedingly complex, embracing a
form. (Diller, U. S. Geol. Surv.)
LAVAS.
Their nature.—In the chapter on the Origin and Descent of Rocks, the
nature of lavas and of the rocks derived from them has been discussed
(Chapter VII). In view of prevalent misconceptions, it may be repeated, for
the sake of emphasis, that lavas are mutual solutions of mineral matter in
mineral matter, rather than simply melted rock. Into this mutual solution
there enter not only rock materials, but gases. The distinction between
mutual solutions and simple molten rock cannot be rigorously made, but it
is at least essential to know that the minerals do not necessarily crystallize
from lavas in the order of their melting temperatures, or in any uniform
order, but rather in the order in which saturation of the several mineral
constituents happens to be reached in the given mutual solution. Thus
quartz, which has a very high melting-point, is often one of the last minerals
to crystallize. The mutual solutions are exceedingly complex, embracing a
Page 700
wide range of chemical substances, but the chief of them, as already stated,
are silicates of aluminum, potassium, sodium, calcium, magnesium, and
iron, with minor ingredients of nearly all known substances, in greater or
less proportion. The old idea of lavas as simply melted rock is not, however,
wholly to be abandoned. The mode of solidifying is often simply that of
molten matter freezing. If lava be suddenly cooled, the congelation is
essentially the solidification of a melted substance. The result is a glassy
body, every part of which has essentially the same composition that the
liquid had. Usually, however, even in this case, the gases escape in part. If
the cooling is slower, the various substances in the mixture crystallize out
into minerals in the order in which they severally reach saturation. This
involves the principle that solubility is dependent on temperature, and that
as the temperature sinks the degree of solubility declines, and the
saturation-point for some constituents of the solution is reached earlier than
for others. With sufficiently slow cooling, all the material will pass into the
solid state by the crystallizing of the several minerals in succession. This
does not mean that two or more minerals may not be forming at the same
time, for crystals often interfere with each other’s growth. It does, however,
involve the doctrine that some substances may complete their crystallization
while the surrounding material is yet in the fluid condition. In most igneous
rocks nearly perfect crystals of certain minerals are common, while other
minerals, crystallizing later, are compelled to adapt themselves to the space
left. This conception is supported by the fact that lavas, while still in the
fluid condition, often contain well-formed crystals, and these crystals
sometimes make up a considerable percent. of the flowing mass, just as
water in certain conditions may be filled with crystals of ice. So also
crystals after having been formed may be redissolved in part, doubtless
because of changes in the nature of the magma due to undetermined
conditions which may arise in the process of crystallization, or from the
accession of gas, or from new material dissolved from the walls of the
passageway.
are silicates of aluminum, potassium, sodium, calcium, magnesium, and
iron, with minor ingredients of nearly all known substances, in greater or
less proportion. The old idea of lavas as simply melted rock is not, however,
wholly to be abandoned. The mode of solidifying is often simply that of
molten matter freezing. If lava be suddenly cooled, the congelation is
essentially the solidification of a melted substance. The result is a glassy
body, every part of which has essentially the same composition that the
liquid had. Usually, however, even in this case, the gases escape in part. If
the cooling is slower, the various substances in the mixture crystallize out
into minerals in the order in which they severally reach saturation. This
involves the principle that solubility is dependent on temperature, and that
as the temperature sinks the degree of solubility declines, and the
saturation-point for some constituents of the solution is reached earlier than
for others. With sufficiently slow cooling, all the material will pass into the
solid state by the crystallizing of the several minerals in succession. This
does not mean that two or more minerals may not be forming at the same
time, for crystals often interfere with each other’s growth. It does, however,
involve the doctrine that some substances may complete their crystallization
while the surrounding material is yet in the fluid condition. In most igneous
rocks nearly perfect crystals of certain minerals are common, while other
minerals, crystallizing later, are compelled to adapt themselves to the space
left. This conception is supported by the fact that lavas, while still in the
fluid condition, often contain well-formed crystals, and these crystals
sometimes make up a considerable percent. of the flowing mass, just as
water in certain conditions may be filled with crystals of ice. So also
crystals after having been formed may be redissolved in part, doubtless
because of changes in the nature of the magma due to undetermined
conditions which may arise in the process of crystallization, or from the
accession of gas, or from new material dissolved from the walls of the
passageway.
Page 701
Fig. 469.—Lobular form of lava-flow, “Pahoehoe.” (Dutton, U. S. Geol. Surv.)
Page 702
Fig. 470.—Terminal portion of a rough lava-flow, “aa.” Cinder Buttes, Idaho. (Russell,
U. S. Geol. Surv.)
U. S. Geol. Surv.)
Page 703
Fig. 471.—Lava flowing over a precipice near Hilo, Hawaiian Islands.
Consanguinity and succession of lavas.—The lavas that are poured
forth at different stages in the succession of eruptions of a given region are
usually not the same, as might naturally be expected, but form a curious
series the members of which are related to one another. Iddings has called
this relation consanguinity.[283] No universal law of succession has yet been
established, and perhaps none exists; but Richthofen[284] many years ago
announced a definite order for the Tertiary flows of western America which
seems to hold fairly well in its general aspects, though not everywhere
completely realized, so far as surface observation goes. Richthofen’s order
is: (1) lavas of neutral types, (2) lavas of acid types, (3) lavas of basic types,
(4) lavas of more acid types, and (5) lavas of more basic types. The special
varieties of rock vary, and even the general order is often apparently
defective. The defects are sometimes assigned to the concealment of some
of the outflows. While this may be true in some cases, it is not unlikely that
in others there is a real failure of the sequence. At any rate, the sequence
can only be regarded as a rough generalization. It is supposed to be due to
magmatic differentiation caused by the differences of temperature to which
the different parts are subjected underground, by differences of specific
gravity and fluidity which result from changes of temperature, and probably
by other causes.
Consanguinity and succession of lavas.—The lavas that are poured
forth at different stages in the succession of eruptions of a given region are
usually not the same, as might naturally be expected, but form a curious
series the members of which are related to one another. Iddings has called
this relation consanguinity.[283] No universal law of succession has yet been
established, and perhaps none exists; but Richthofen[284] many years ago
announced a definite order for the Tertiary flows of western America which
seems to hold fairly well in its general aspects, though not everywhere
completely realized, so far as surface observation goes. Richthofen’s order
is: (1) lavas of neutral types, (2) lavas of acid types, (3) lavas of basic types,
(4) lavas of more acid types, and (5) lavas of more basic types. The special
varieties of rock vary, and even the general order is often apparently
defective. The defects are sometimes assigned to the concealment of some
of the outflows. While this may be true in some cases, it is not unlikely that
in others there is a real failure of the sequence. At any rate, the sequence
can only be regarded as a rough generalization. It is supposed to be due to
magmatic differentiation caused by the differences of temperature to which
the different parts are subjected underground, by differences of specific
gravity and fluidity which result from changes of temperature, and probably
by other causes.
Page 704
Temperatures of lavas.—Accurate determinations of the temperatures in
the center of the lava-columns, where they have been least reduced by
contact with the rock-walls, have not yet been made, but it is clear from the
whiteness of the lavas that their temperatures are often appreciably above
the melting-point. This is also a necessary inference from the length of time
they remain fluid, notwithstanding the great surface contact of the column
in its miles of ascent, the conversion of contact water into steam, and the
expansion and escape of the gases. In cases where determination has been
practicable (and they certainly do not represent the maximum temperatures)
it has been found that the melting-points of silver, about 960° C., and of
copper, about 1060° C., are reached. In connection with overflows, it has
been found that brass is decomposed into its component metals, the copper
actually crystallizing. Silver has been sublimed, and made to redeposit itself
in crystalline form. This implies much more than the bare melting
temperatures. Even the fine edges of flints have been fused. It is, therefore,
probably safe to assume that the original temperatures of the lavas as they
rise to the surface sometimes reach considerably beyond 2000° Fahr. (1093°
C.), and may perhaps even attain 3000° Fahr. or more. Even these
temperatures must be somewhat below the original subterranean
temperatures of the lavas, because some heat must necessarily be lost in
rising, partly by contact with the walls of the colder rocks through which
they pass, probably for as much as a score of miles at least, and partly from
the expansion of the gases within them. If any considerable part of these
gases is derived from waters which joined the lava in its upward course in
the fracture zone, the energy consumed in raising the water to the high
temperatures of the lavas must be subtracted from the original heat, and
must be a further source of reduction of temperature. It is important to
emphasize this point in view of its bearing upon the origin of the lavas. It
has been suggested that lavas may be due to an aqueo-igneous fusion, a
kind of fusion which may take place at comparatively moderate
temperatures. It seems obvious, however, from the phenomena themselves,
that temperatures as high as ordinary dry fusion, and perhaps even higher,
are attained. It is clear also that the maintenance of the liquid condition in a
constant state of ebullition for a long period of time implies a large surplus
of heat above that necessary for liquefaction simply. This is especially true
if the ebullition comes from surface-waters penetrating to and becoming
absorbed in the lava-column below. This process must tend rapidly to
the center of the lava-columns, where they have been least reduced by
contact with the rock-walls, have not yet been made, but it is clear from the
whiteness of the lavas that their temperatures are often appreciably above
the melting-point. This is also a necessary inference from the length of time
they remain fluid, notwithstanding the great surface contact of the column
in its miles of ascent, the conversion of contact water into steam, and the
expansion and escape of the gases. In cases where determination has been
practicable (and they certainly do not represent the maximum temperatures)
it has been found that the melting-points of silver, about 960° C., and of
copper, about 1060° C., are reached. In connection with overflows, it has
been found that brass is decomposed into its component metals, the copper
actually crystallizing. Silver has been sublimed, and made to redeposit itself
in crystalline form. This implies much more than the bare melting
temperatures. Even the fine edges of flints have been fused. It is, therefore,
probably safe to assume that the original temperatures of the lavas as they
rise to the surface sometimes reach considerably beyond 2000° Fahr. (1093°
C.), and may perhaps even attain 3000° Fahr. or more. Even these
temperatures must be somewhat below the original subterranean
temperatures of the lavas, because some heat must necessarily be lost in
rising, partly by contact with the walls of the colder rocks through which
they pass, probably for as much as a score of miles at least, and partly from
the expansion of the gases within them. If any considerable part of these
gases is derived from waters which joined the lava in its upward course in
the fracture zone, the energy consumed in raising the water to the high
temperatures of the lavas must be subtracted from the original heat, and
must be a further source of reduction of temperature. It is important to
emphasize this point in view of its bearing upon the origin of the lavas. It
has been suggested that lavas may be due to an aqueo-igneous fusion, a
kind of fusion which may take place at comparatively moderate
temperatures. It seems obvious, however, from the phenomena themselves,
that temperatures as high as ordinary dry fusion, and perhaps even higher,
are attained. It is clear also that the maintenance of the liquid condition in a
constant state of ebullition for a long period of time implies a large surplus
of heat above that necessary for liquefaction simply. This is especially true
if the ebullition comes from surface-waters penetrating to and becoming
absorbed in the lava-column below. This process must tend rapidly to
Page 705
exhaust the heat in the column of lava. If, on the other hand, the gases are
derived from the deep interior, and the ebullition at the surface is due to
their escape, they may bring up new supplies of heat to counteract the
cooling effects of their expansion.
Depth of source.—Attempts have been made to ascertain the depth from
which lavas rise, by means of the earthquake tremors that accompany
eruptions. The estimates have ranged from seven or eight to thirty miles.
The mode of estimate is that discussed under earthquakes, and is subject to
the corrections there indicated. If these could be perfectly applied, the
estimates might probably all fall within ten miles, and not improbably all
within six miles of the surface. But in any case the method really tells very
little as to the true point of origin of the lava. At most it probably only tells
where the ascending lava begins to rupture the rock through which it
passes, and rupture may not be possible below the zone of fracture, which is
probably not more than six miles deep. In the zone of flowage below, where
the pressure is too great to permit fracture, the lava not improbably makes
its way by some boring or fluxing process, which might not, because of its
nature, be capable of giving rise to seismic tremors. The behavior of the
tremors perhaps forces us to locate the origin of lava movement at least as
low as the bottom of the fracture zone, but it probably offers no sufficient
ground for limiting the lava’s origin to this or any other specific depth.
VOLCANIC GASES.
The most distinctive feature of volcanoes is the explosive action arising
from the gases and vapors pent up in the lava. There is not a little explosive
action of a secondary character arising from the mere outer contact of
surface-waters with lavas or with the hot rocks of the crater walls, or with
the hot ashes and rocks thrown out; but these are incidental, not essential,
features.
The precise nature of the occlusion or absorption of gases and vapors has
not yet been determined. It is thought that lava spontaneously absorbs such
gases when at high temperatures, and especially when the gases are under
great pressure, and that as the pressure is relieved and the lava is cooled and
solidified, the larger part of the gases escapes. In those cases in which the
eruption is quiet, the escape of the gases is but partial while the lava is in
derived from the deep interior, and the ebullition at the surface is due to
their escape, they may bring up new supplies of heat to counteract the
cooling effects of their expansion.
Depth of source.—Attempts have been made to ascertain the depth from
which lavas rise, by means of the earthquake tremors that accompany
eruptions. The estimates have ranged from seven or eight to thirty miles.
The mode of estimate is that discussed under earthquakes, and is subject to
the corrections there indicated. If these could be perfectly applied, the
estimates might probably all fall within ten miles, and not improbably all
within six miles of the surface. But in any case the method really tells very
little as to the true point of origin of the lava. At most it probably only tells
where the ascending lava begins to rupture the rock through which it
passes, and rupture may not be possible below the zone of fracture, which is
probably not more than six miles deep. In the zone of flowage below, where
the pressure is too great to permit fracture, the lava not improbably makes
its way by some boring or fluxing process, which might not, because of its
nature, be capable of giving rise to seismic tremors. The behavior of the
tremors perhaps forces us to locate the origin of lava movement at least as
low as the bottom of the fracture zone, but it probably offers no sufficient
ground for limiting the lava’s origin to this or any other specific depth.
VOLCANIC GASES.
The most distinctive feature of volcanoes is the explosive action arising
from the gases and vapors pent up in the lava. There is not a little explosive
action of a secondary character arising from the mere outer contact of
surface-waters with lavas or with the hot rocks of the crater walls, or with
the hot ashes and rocks thrown out; but these are incidental, not essential,
features.
The precise nature of the occlusion or absorption of gases and vapors has
not yet been determined. It is thought that lava spontaneously absorbs such
gases when at high temperatures, and especially when the gases are under
great pressure, and that as the pressure is relieved and the lava is cooled and
solidified, the larger part of the gases escapes. In those cases in which the
eruption is quiet, the escape of the gases is but partial while the lava is in
Page 706
the crater, and much gas remains to be given out from the molten material
after it has been extruded and is about to congeal. The gases are then given
off with relative slowness and quietness. If, however, the lavas are
surcharged with gases, and if these are restrained from free escape by the
viscosity of the lavas, the gases gather in large vesicles in the lava in the
throat of the volcano, and on coming to the surface explode, hurling the
enveloping lava upwards and outwards, often to great distances. The
violence of projection reduces a portion of the lava to a finely divided state
constituting the “ash” and “smoke” of the volcano. Other portions less
divided are inflated by the gases disseminated through them, and form
“pumice” and “scoria,” according to the degree of inflation, while masses of
lava that have already solidified into more or less rounded masses in the
crater are hurled forth as “bombs”; not infrequently portions of the walls of
the crater or of the duct below are also disrupted and shot forth.
Differences in gas action.—The causes of the differences of gas action
in different volcanoes are undetermined, but the following suggestions may
point to a part of the truth: (1) Doubtless some lavas contain more gases
than others, and hence are predisposed to be more explosive; (2) some are
more viscous than others and hence hold the gases more tenaciously until
they accumulate and acquire explosive force, while the more liquid lavas
allow their gases to escape more freely and easily; (3) some are hotter than
others, and hence hold their gases until after they have escaped from the
crater, when they give them off from their expanded surfaces in the open
air, where there is no restraint to develop explosiveness; (4) some flows are
so massive that they cool to the chief gas-discharging point only after they
are spread out on the surface, when quiet escape is possible; (5) probably a
main occasion of the very violent explosions lies in the fact that the lavas
have begun to crystallize while yet in the duct of the volcano. The crystals,
in forming in the magma, exclude the gases from themselves, and this
excluded portion overcharges the remaining portion of the lava. This
process continues as the lava rises and grows cooler until the gases acquire
great volume and explosive force. This view is sustained by the fact that the
pumice and ash of such extraordinarily explosive eruptions as those of
Krakatoa and Pelée contain many small crystals which had certainly formed
before the explosive inflation took place. Incipient crystallization does not,
however, appear to be a universal accompaniment of explosive action.
after it has been extruded and is about to congeal. The gases are then given
off with relative slowness and quietness. If, however, the lavas are
surcharged with gases, and if these are restrained from free escape by the
viscosity of the lavas, the gases gather in large vesicles in the lava in the
throat of the volcano, and on coming to the surface explode, hurling the
enveloping lava upwards and outwards, often to great distances. The
violence of projection reduces a portion of the lava to a finely divided state
constituting the “ash” and “smoke” of the volcano. Other portions less
divided are inflated by the gases disseminated through them, and form
“pumice” and “scoria,” according to the degree of inflation, while masses of
lava that have already solidified into more or less rounded masses in the
crater are hurled forth as “bombs”; not infrequently portions of the walls of
the crater or of the duct below are also disrupted and shot forth.
Differences in gas action.—The causes of the differences of gas action
in different volcanoes are undetermined, but the following suggestions may
point to a part of the truth: (1) Doubtless some lavas contain more gases
than others, and hence are predisposed to be more explosive; (2) some are
more viscous than others and hence hold the gases more tenaciously until
they accumulate and acquire explosive force, while the more liquid lavas
allow their gases to escape more freely and easily; (3) some are hotter than
others, and hence hold their gases until after they have escaped from the
crater, when they give them off from their expanded surfaces in the open
air, where there is no restraint to develop explosiveness; (4) some flows are
so massive that they cool to the chief gas-discharging point only after they
are spread out on the surface, when quiet escape is possible; (5) probably a
main occasion of the very violent explosions lies in the fact that the lavas
have begun to crystallize while yet in the duct of the volcano. The crystals,
in forming in the magma, exclude the gases from themselves, and this
excluded portion overcharges the remaining portion of the lava. This
process continues as the lava rises and grows cooler until the gases acquire
great volume and explosive force. This view is sustained by the fact that the
pumice and ash of such extraordinarily explosive eruptions as those of
Krakatoa and Pelée contain many small crystals which had certainly formed
before the explosive inflation took place. Incipient crystallization does not,
however, appear to be a universal accompaniment of explosive action.
Page 707
Spasmodic action.—The discharge of the gases is spasmodic, and
usually consists of a succession of distinct explosions. Sometimes these
succeed one another at rather constant and frequent intervals, as in
Stromboli, where the explosions follow one another at intervals of three to
ten or more minutes. In many others the outbursts are rhythmic, while in
others the spasms are distant and irregular.
Kinds of gases.—Steam is the chief volcanic gas. Its constituents,
hydrogen and oxygen, are also present in the free state, and are perhaps the
result of the dissociation of the steam at the very high temperatures of the
lavas. Carbon dioxide is probably next in abundance. No positive statement
as to the relative amounts of the subordinate gases can be made because of
the obvious difficulties of obtaining anything like a representative analysis
of the gases concerned in the great volcanic eruptions. The materials for the
analyses which have been made were derived chiefly from little secondary
or “parasitic” vents, or from side-wall crevices, through which the volcanic
gases rise. Such vents probably derive their gases from the very border of
the main mass, where it is most subject to the influence of waters and gases
from the adjacent walls, and it is uncertain how far they are truly
representative of the gases in the interior of the lava itself. The data now at
command seem to indicate that carbon dioxide increases greatly in relative
abundance as volcanic action dies away. Great quantities of this gas are
often given forth long after all signs of active vulcanism have disappeared.
Such gases have been attributed to the action of the lavas on buried beds of
limestone or other carbonates, but in many cases the geology of the region
offers no special support to this hypothesis. It does not seem inherently
probable that the heat of the lava would be sufficient to decompose
limestone at a period very long after the active eruption. An alternative
suggestion is that the stronger volcanic acids mentioned below are
gradually conveyed into the adjacent rocks and there act on limestones or
on partially carbonated crystalline rocks, setting free carbon dioxide.
Whatever may be true with regard to secondary gases of this kind, it is quite
certain that the lavas themselves contain large quantities of carbon dioxide,
and also of carbon monoxide, doubtless reduced from the dioxide. Sulphur
gases are very common accompaniments of volcanic eruptions. They take
the forms of sulphuretted hydrogen and sulphurous acid and perhaps of
sublimated sulphur, all of which are liable to pass by oxidation and
hydration into sulphuric acid. Chlorine and hydrochloric gases are also
usually consists of a succession of distinct explosions. Sometimes these
succeed one another at rather constant and frequent intervals, as in
Stromboli, where the explosions follow one another at intervals of three to
ten or more minutes. In many others the outbursts are rhythmic, while in
others the spasms are distant and irregular.
Kinds of gases.—Steam is the chief volcanic gas. Its constituents,
hydrogen and oxygen, are also present in the free state, and are perhaps the
result of the dissociation of the steam at the very high temperatures of the
lavas. Carbon dioxide is probably next in abundance. No positive statement
as to the relative amounts of the subordinate gases can be made because of
the obvious difficulties of obtaining anything like a representative analysis
of the gases concerned in the great volcanic eruptions. The materials for the
analyses which have been made were derived chiefly from little secondary
or “parasitic” vents, or from side-wall crevices, through which the volcanic
gases rise. Such vents probably derive their gases from the very border of
the main mass, where it is most subject to the influence of waters and gases
from the adjacent walls, and it is uncertain how far they are truly
representative of the gases in the interior of the lava itself. The data now at
command seem to indicate that carbon dioxide increases greatly in relative
abundance as volcanic action dies away. Great quantities of this gas are
often given forth long after all signs of active vulcanism have disappeared.
Such gases have been attributed to the action of the lavas on buried beds of
limestone or other carbonates, but in many cases the geology of the region
offers no special support to this hypothesis. It does not seem inherently
probable that the heat of the lava would be sufficient to decompose
limestone at a period very long after the active eruption. An alternative
suggestion is that the stronger volcanic acids mentioned below are
gradually conveyed into the adjacent rocks and there act on limestones or
on partially carbonated crystalline rocks, setting free carbon dioxide.
Whatever may be true with regard to secondary gases of this kind, it is quite
certain that the lavas themselves contain large quantities of carbon dioxide,
and also of carbon monoxide, doubtless reduced from the dioxide. Sulphur
gases are very common accompaniments of volcanic eruptions. They take
the forms of sulphuretted hydrogen and sulphurous acid and perhaps of
sublimated sulphur, all of which are liable to pass by oxidation and
hydration into sulphuric acid. Chlorine and hydrochloric gases are also
Page 708
common, particularly at high temperatures. Fluorine and other gases are
occasionally present. Certain gases, such as hydrogen and chlorine, are
especially associated with high temperatures and energetic action, and are
probably dependent on them. Hydrochloric acid and the sulphurous gases
are also mainly associated with high temperatures, while sulphuretted
hydrogen is commoner at lower temperatures. Oxygen, nitrogen, and
probably carbon dioxide or carbon monoxide are present throughout all
ranges of temperature. Nitrogen is a rather frequent but not very abundant
constituent of the volcanic gases. How far it results from admixture of the
atmosphere and how far it is original, is not determined. It is, however, one
of the gases found in volcanic rocks after they have cooled, and is
presumably original in part. A large series of secondary vapors naturally
arise from the volatilization of substances contained in the lavas, such as the
oxides, chlorides, and sulphides of the metals, etc.
Residual gases in volcanic rocks.—Some light upon the vital question
of the original, as distinguished from the secondary gases of lavas may be
found in the analyses of the gases that remain in the lavas after they are
solidified. When the lavas lodged underground without free communication
with the surface, there is reason to think that they retained a larger
percentage of their original gases in solidification than in cases of free
exposure at the surface; at any rate, such rocks contain notable quantities of
gases occluded in some way within themselves. Recent surface-lavas also
contain gases of similar kinds, but not in equal degree, so far as available
analyses show. The gases are in part held in numerous small cavities within
the constituent minerals, especially in the quartz. This is perhaps due to the
fact that quartz usually crystallizes late in the process of solidification, and
its mother-material becomes crowded with gases excluded by the previous
crystallization of other minerals. Analyses of twenty-five crystalline rocks
of various kinds from many typical localities by Tilden,[285] gave an average
volume of gas, under ordinary atmospheric pressure, four and a half times
that of the containing rock. This shows the condensed condition in which
the gases are held. Of these gases, the chief is hydrogen, which much
exceeds all the rest. Next in order of abundance is carbon dioxide, followed
by carbon monoxide, marsh gas (CH4), and nitrogen. Water is frequently
present and free oxygen almost universally absent. The average ratio of
hydrogen to carbon dioxide by volume in these analyses is about 70 : 30.
occasionally present. Certain gases, such as hydrogen and chlorine, are
especially associated with high temperatures and energetic action, and are
probably dependent on them. Hydrochloric acid and the sulphurous gases
are also mainly associated with high temperatures, while sulphuretted
hydrogen is commoner at lower temperatures. Oxygen, nitrogen, and
probably carbon dioxide or carbon monoxide are present throughout all
ranges of temperature. Nitrogen is a rather frequent but not very abundant
constituent of the volcanic gases. How far it results from admixture of the
atmosphere and how far it is original, is not determined. It is, however, one
of the gases found in volcanic rocks after they have cooled, and is
presumably original in part. A large series of secondary vapors naturally
arise from the volatilization of substances contained in the lavas, such as the
oxides, chlorides, and sulphides of the metals, etc.
Residual gases in volcanic rocks.—Some light upon the vital question
of the original, as distinguished from the secondary gases of lavas may be
found in the analyses of the gases that remain in the lavas after they are
solidified. When the lavas lodged underground without free communication
with the surface, there is reason to think that they retained a larger
percentage of their original gases in solidification than in cases of free
exposure at the surface; at any rate, such rocks contain notable quantities of
gases occluded in some way within themselves. Recent surface-lavas also
contain gases of similar kinds, but not in equal degree, so far as available
analyses show. The gases are in part held in numerous small cavities within
the constituent minerals, especially in the quartz. This is perhaps due to the
fact that quartz usually crystallizes late in the process of solidification, and
its mother-material becomes crowded with gases excluded by the previous
crystallization of other minerals. Analyses of twenty-five crystalline rocks
of various kinds from many typical localities by Tilden,[285] gave an average
volume of gas, under ordinary atmospheric pressure, four and a half times
that of the containing rock. This shows the condensed condition in which
the gases are held. Of these gases, the chief is hydrogen, which much
exceeds all the rest. Next in order of abundance is carbon dioxide, followed
by carbon monoxide, marsh gas (CH4), and nitrogen. Water is frequently
present and free oxygen almost universally absent. The average ratio of
hydrogen to carbon dioxide by volume in these analyses is about 70 : 30.
Page 709
Five complete analyses gave the following averages: H2, 52.134; CO2,
34.104; CO, 8.422; CH4, 3.224; N2, 2.072. It will be seen that the gases
contained in these rocks are in proportions radically different from those of
the atmosphere, and it is doubtful whether they can be reasonably assigned
to any other source than the lavas from which the rocks were formed. It is
to be noted, however, that some sedimentary and meta-sedimentary rocks,
such as quartzite and quartz-schist, contain similar gases, but this may be
because the granules of the original rock retain them, notwithstanding the
secondary processes through which they have passed. Analyses of
meteorites show essentially the same gases in much the same proportions. If
evidence of this kind can be trusted, the standard original gases of lavas are
the elements or compounds of hydrogen, carbon, and nitrogen, in the order
named, while the chlorine and sulphur gases are to be regarded as
accessory. Because of their intensely energetic and noxious character, these
latter gases make themselves disproportionately manifest in the vicinity of
active volcanoes. That they are really not preponderant seems to be implied
by the fact that the volcanic rains, which are extremely copious, are usually
fresh, and only in rare cases is the presence of the hydrochloric or
sulphurous elements sufficient to produce noxious effects. Volcanic and
meteoric data seem to indicate that steam is held less tenaciously than the
other gases in the magmas as they solidify into rocks.
The source of the gases.—As already noted, it is one of the outstanding
problems of geology to determine (a) how far the gases of lavas were
possessed by them from their origin, whatever that may be, and (b) how far
they have been acquired in the lava’s ascent to the surface. It is recognized
that lavas have the power of absorbing gases, and one of the views
entertained is that surface-waters, percolating through the rocks and coming
in contact with the ascending column of lava, are converted into steam,
which is absorbed into the lava and rises with it to the surface. There are
two phases of this view. (1) The more conservative one supposes that the
water merely penetrates the fracture zone of the surface of the earth through
the ordinary means of passage of underground-waters, and so makes a
comparatively short circuit. Under this view, the steam and other gases
given forth are not a contribution to the atmosphere and hydrosphere, but
merely a restoration to them of water and dissolved gases previously carried
down from the surface. An even narrower view is sometimes entertained
34.104; CO, 8.422; CH4, 3.224; N2, 2.072. It will be seen that the gases
contained in these rocks are in proportions radically different from those of
the atmosphere, and it is doubtful whether they can be reasonably assigned
to any other source than the lavas from which the rocks were formed. It is
to be noted, however, that some sedimentary and meta-sedimentary rocks,
such as quartzite and quartz-schist, contain similar gases, but this may be
because the granules of the original rock retain them, notwithstanding the
secondary processes through which they have passed. Analyses of
meteorites show essentially the same gases in much the same proportions. If
evidence of this kind can be trusted, the standard original gases of lavas are
the elements or compounds of hydrogen, carbon, and nitrogen, in the order
named, while the chlorine and sulphur gases are to be regarded as
accessory. Because of their intensely energetic and noxious character, these
latter gases make themselves disproportionately manifest in the vicinity of
active volcanoes. That they are really not preponderant seems to be implied
by the fact that the volcanic rains, which are extremely copious, are usually
fresh, and only in rare cases is the presence of the hydrochloric or
sulphurous elements sufficient to produce noxious effects. Volcanic and
meteoric data seem to indicate that steam is held less tenaciously than the
other gases in the magmas as they solidify into rocks.
The source of the gases.—As already noted, it is one of the outstanding
problems of geology to determine (a) how far the gases of lavas were
possessed by them from their origin, whatever that may be, and (b) how far
they have been acquired in the lava’s ascent to the surface. It is recognized
that lavas have the power of absorbing gases, and one of the views
entertained is that surface-waters, percolating through the rocks and coming
in contact with the ascending column of lava, are converted into steam,
which is absorbed into the lava and rises with it to the surface. There are
two phases of this view. (1) The more conservative one supposes that the
water merely penetrates the fracture zone of the surface of the earth through
the ordinary means of passage of underground-waters, and so makes a
comparatively short circuit. Under this view, the steam and other gases
given forth are not a contribution to the atmosphere and hydrosphere, but
merely a restoration to them of water and dissolved gases previously carried
down from the surface. An even narrower view is sometimes entertained
Page 710
which supposes that the larger part of the water descends through the
volcanic cone itself, or immediately about its base. The presence of chlorine
gases in the volcanic emanations and the nearness of most existing
volcanoes to the sea have been the basis for the idea that sea-water,
penetrating to the lava, is a chief source of the volcanic gases. (2) The
broader phase of the view assumes that the waters penetrate not only the
outer fracture zone of the earth, which is probably limited to five or six
miles in depth, but that they diffuse themselves through the continuous
unfractured zone down to depths where temperatures of fusion prevail, and
that they there enter into combination with the lavas or with hot rock to
form lavas. It is well known that aqueous vapor facilitates the fusion, or
more accurately, the mutual solution of the minerals. This view is a part of
one of the hypotheses concerning the origin of the lavas themselves.
The opposing view supposes that the gases were in the main original. Of
this view there are two phases: (1) One supposes that the lavas are remnants
of an original molten globe which absorbed gases from the primitive
atmosphere and retained them till the time of their eruption. The possible
absorption of steam and air into the supposed molten globe has been much
neglected in current conceptions of early conditions. If the lavas of the
supposed molten globe absorbed proportionately as much water-vapor as
the volcanic lavas often contain, it would probably take forty or fifty times
the present ocean and atmosphere to supply them. Any remnants of these
original lavas might well be supposed to hold gases. Even rocks derived
from them by deep-seated solidification might retain much gas. (2) The
other phase of the view assumes that the gases were entrapped when the
globe was built up of meteoroidal or planetesimal matter, as assumed in the
accretion hypothesis.
Under either of the last two views the gases may be said to be primary,
and genetically connected with the origin of the lavas themselves. Such
gases would be a contribution to the atmosphere and the hydrosphere. This
view does not exclude the idea that as the lava rises through the surface-
rocks, other gases are formed by contact, and that they may be absorbed
into the rising column. On the contrary, the view recognizes the possibility
that a tongue of lava rising into the upper formations may encounter bodies
of water, or masses of thoroughly water-soaked rock, from which great
quantities of steam may be generated, and that this accessory steam may be
volcanic cone itself, or immediately about its base. The presence of chlorine
gases in the volcanic emanations and the nearness of most existing
volcanoes to the sea have been the basis for the idea that sea-water,
penetrating to the lava, is a chief source of the volcanic gases. (2) The
broader phase of the view assumes that the waters penetrate not only the
outer fracture zone of the earth, which is probably limited to five or six
miles in depth, but that they diffuse themselves through the continuous
unfractured zone down to depths where temperatures of fusion prevail, and
that they there enter into combination with the lavas or with hot rock to
form lavas. It is well known that aqueous vapor facilitates the fusion, or
more accurately, the mutual solution of the minerals. This view is a part of
one of the hypotheses concerning the origin of the lavas themselves.
The opposing view supposes that the gases were in the main original. Of
this view there are two phases: (1) One supposes that the lavas are remnants
of an original molten globe which absorbed gases from the primitive
atmosphere and retained them till the time of their eruption. The possible
absorption of steam and air into the supposed molten globe has been much
neglected in current conceptions of early conditions. If the lavas of the
supposed molten globe absorbed proportionately as much water-vapor as
the volcanic lavas often contain, it would probably take forty or fifty times
the present ocean and atmosphere to supply them. Any remnants of these
original lavas might well be supposed to hold gases. Even rocks derived
from them by deep-seated solidification might retain much gas. (2) The
other phase of the view assumes that the gases were entrapped when the
globe was built up of meteoroidal or planetesimal matter, as assumed in the
accretion hypothesis.
Under either of the last two views the gases may be said to be primary,
and genetically connected with the origin of the lavas themselves. Such
gases would be a contribution to the atmosphere and the hydrosphere. This
view does not exclude the idea that as the lava rises through the surface-
rocks, other gases are formed by contact, and that they may be absorbed
into the rising column. On the contrary, the view recognizes the possibility
that a tongue of lava rising into the upper formations may encounter bodies
of water, or masses of thoroughly water-soaked rock, from which great
quantities of steam may be generated, and that this accessory steam may be
Page 711
a large factor in the initial explosion which often accompanies the
development of a new volcano, or the new eruption of an old one after a
long period of quiescence.
A decision on the vital question whether the volcanic gases are largely
primary, or are essentially secondary, has not yet been reached; but it will
doubtless be reached when a sufficient number of really representative
analyses of volcanic gases have been made, and when the phenomena of the
gases occluded in igneous rocks have been thoroughly investigated.
The peculiar proportions of the rock-gases, in which hydrogen and
carbon dioxide so greatly preponderate, seem to imply that they are not
derived from the atmosphere; at least if they were so derived, there must
have been a selective absorption of a most remarkable kind, because
hydrogen is present in the atmosphere in exceedingly small quantities,
while carbon dioxide is a very minor constituent. At the same time, as
already remarked, no free oxygen is usually found in these absorbed gases.
The question as to whether the larger part of the volcanic gases is original
or is merely a special form of convective circulation, has an important
bearing on the supply of the atmosphere, which is constantly being depleted
by the oxidation of the rocks and by the formation of carbonates and
carbonaceous deposits. This vital phase of the subject will receive further
consideration. While recognizing the lack of decisive proof, it would seem
that the preponderance of evidence lies in favor of the view that a notable
portion, at least, of gaseous volcanic emanations is derived from the interior
of the earth, and is really a contribution to the atmosphere and the
hydrosphere. The hydrogen, on coming in contact with the atmosphere,
ignites and adds itself to the hydrosphere. The carbon dioxide is in part
decomposed by plants, and adds to the supply of atmospheric oxygen. The
nitrogen, being comparatively inert, doubtless gradually accumulates in the
air and has thus come to be its preponderant constituent.
THE CAUSE OF VULCANISM.
The extraordinary facts involved in volcanic phenomena cannot well be
discussed fully until the origin of the earth is considered, and the great
agencies, as well as the peculiar conditions, which the earth inherited from
development of a new volcano, or the new eruption of an old one after a
long period of quiescence.
A decision on the vital question whether the volcanic gases are largely
primary, or are essentially secondary, has not yet been reached; but it will
doubtless be reached when a sufficient number of really representative
analyses of volcanic gases have been made, and when the phenomena of the
gases occluded in igneous rocks have been thoroughly investigated.
The peculiar proportions of the rock-gases, in which hydrogen and
carbon dioxide so greatly preponderate, seem to imply that they are not
derived from the atmosphere; at least if they were so derived, there must
have been a selective absorption of a most remarkable kind, because
hydrogen is present in the atmosphere in exceedingly small quantities,
while carbon dioxide is a very minor constituent. At the same time, as
already remarked, no free oxygen is usually found in these absorbed gases.
The question as to whether the larger part of the volcanic gases is original
or is merely a special form of convective circulation, has an important
bearing on the supply of the atmosphere, which is constantly being depleted
by the oxidation of the rocks and by the formation of carbonates and
carbonaceous deposits. This vital phase of the subject will receive further
consideration. While recognizing the lack of decisive proof, it would seem
that the preponderance of evidence lies in favor of the view that a notable
portion, at least, of gaseous volcanic emanations is derived from the interior
of the earth, and is really a contribution to the atmosphere and the
hydrosphere. The hydrogen, on coming in contact with the atmosphere,
ignites and adds itself to the hydrosphere. The carbon dioxide is in part
decomposed by plants, and adds to the supply of atmospheric oxygen. The
nitrogen, being comparatively inert, doubtless gradually accumulates in the
air and has thus come to be its preponderant constituent.
THE CAUSE OF VULCANISM.
The extraordinary facts involved in volcanic phenomena cannot well be
discussed fully until the origin of the earth is considered, and the great
agencies, as well as the peculiar conditions, which the earth inherited from
Page 712
its birth, are duly weighed, for these were, with little doubt, the true causal
antecedents of vulcanism. We shall return to the subject after a sketch of the
early conditions of the earth, but the views that have been entertained may
be reviewed here while the phenomena are fresh in mind.
The explanation of vulcanism involves two essential elements. These are
(1) the origin of the lavas, which involves a consideration of the necessary
temperatures, pressures, and other conditions, and (2) the forces by which
the lavas are expelled.
Nearly all current explanations of vulcanism are founded upon conditions
supposed to be derived from a molten globe, and fall under two general
classes: (I) those which assume that the lavas are residual portions of the
original molten mass, and (II) those which assign the lavas to the local
melting of rock.
I. On the Assumption that the Lavas are Original.
In this case it is not necessary to assume any special accession of heat,
but merely to account for extrusion. There are two phases of this view, (1)
the one postulating a general molten interior, (2) the other limiting the
molten matter to local reservoirs.
Hypothesis I. Lava outflows from a molten interior.—In the early days
of geology, when the earth was supposed to have a thin crust and a molten
interior, it was very naturally assumed that volcanoes were but pipes
leading down to the molten mass within. This view has been essentially
abandoned. The independence of adjacent vents is in itself almost a fatal
objection, when it is recalled that the height of recent volcanic craters
ranges from nearly 20,000 feet above the sea, to 10,000 to 20,000 feet
below. The view would involve the conception of lava-columns connected
with a common reservoir varying possibly 30,000 to 40,000 feet in altitude,
and certainly more than half that much, simultaneously. The lower outlets
should as certainly be selected for the outflow of the great interior sea of
fluid rock, as the lowest sag in the rim of a lake for its outflow, for no great
differences in specific gravity are presumable under this hypothesis. An
equally grave objection arises from tidal strain. If the earth were liquid
within and merely crusted over by a shell of rock of moderate thickness, it
would yield appreciably to tidal stresses, and this yielding would change the
antecedents of vulcanism. We shall return to the subject after a sketch of the
early conditions of the earth, but the views that have been entertained may
be reviewed here while the phenomena are fresh in mind.
The explanation of vulcanism involves two essential elements. These are
(1) the origin of the lavas, which involves a consideration of the necessary
temperatures, pressures, and other conditions, and (2) the forces by which
the lavas are expelled.
Nearly all current explanations of vulcanism are founded upon conditions
supposed to be derived from a molten globe, and fall under two general
classes: (I) those which assume that the lavas are residual portions of the
original molten mass, and (II) those which assign the lavas to the local
melting of rock.
I. On the Assumption that the Lavas are Original.
In this case it is not necessary to assume any special accession of heat,
but merely to account for extrusion. There are two phases of this view, (1)
the one postulating a general molten interior, (2) the other limiting the
molten matter to local reservoirs.
Hypothesis I. Lava outflows from a molten interior.—In the early days
of geology, when the earth was supposed to have a thin crust and a molten
interior, it was very naturally assumed that volcanoes were but pipes
leading down to the molten mass within. This view has been essentially
abandoned. The independence of adjacent vents is in itself almost a fatal
objection, when it is recalled that the height of recent volcanic craters
ranges from nearly 20,000 feet above the sea, to 10,000 to 20,000 feet
below. The view would involve the conception of lava-columns connected
with a common reservoir varying possibly 30,000 to 40,000 feet in altitude,
and certainly more than half that much, simultaneously. The lower outlets
should as certainly be selected for the outflow of the great interior sea of
fluid rock, as the lowest sag in the rim of a lake for its outflow, for no great
differences in specific gravity are presumable under this hypothesis. An
equally grave objection arises from tidal strain. If the earth were liquid
within and merely crusted over by a shell of rock of moderate thickness, it
would yield appreciably to tidal stresses, and this yielding would change the
Page 713
capacity of the interior so that with every distortion of the spheroid a
portion of its fluid interior would be forced to the outside, and with every
return to the more spheroidal form there would either be a re-flow to the
interior or a shrinking of the crust. In any case a very demonstrative
response to tidal influence would tell the story of interior fluidity. No such
effects are observed. The tidal strains may perhaps have a slight effect in
hastening a given eruption when the forces are approaching a delicate
balance and an eruption is imminent, but the very triviality of this influence
implies not only the absence of a general liquid interior, but also of
extensive reservoirs.
Hypothesis 2. Lavas assigned to molten reservoirs.—A modification
of the preceding view has been made to escape the difficulties involved in
the hypothesis as stated above. It is supposed that while nearly all the
subcrust solidified, numerous liquid spots were left scattered through it.
This honeycombed substratum is supposed to connect the continuous outer
crust with a central solid body, solidified because of pressure in spite of its
high temperature. This hypothesis escapes only a portion of the objections.
For instance, the lavas in Mauna Loa and Kilauea in Hawaii differ nearly
10,000 feet in height, and hence cannot well be supposed to connect with
the same reservoir, but they are both on the same vast cone, which implies
at least an equally large molten reservoir as its source. If there were two
distinct reservoirs of the required magnitude, they must be singularly placed
to supply vents so near and yet so independent. The difficulty grows greater
when the whole Hawaiian chain is considered, for the points of eruption
seem to have migrated from the northwesterly islands, where the volcanoes
are old, to the southeastern end, where volcanic activity is now in progress.
It would be natural under this view to suppose that these residuary
lakelets of liquid rock should be gradually exhausted as time goes on, and
that vulcanism should be a declining phenomenon. It is not clear that this is
the case. The great number of existing volcanoes in regions where great
extrusions took place in earlier ages does not seem to be in harmony with
the hypothesis.
II. On the Assumption that the Lavas are Secondary.
The serious difficulties that arise in interpreting volcanic lavas as
remnants of an original molten mass, and the strong arguments of recent
portion of its fluid interior would be forced to the outside, and with every
return to the more spheroidal form there would either be a re-flow to the
interior or a shrinking of the crust. In any case a very demonstrative
response to tidal influence would tell the story of interior fluidity. No such
effects are observed. The tidal strains may perhaps have a slight effect in
hastening a given eruption when the forces are approaching a delicate
balance and an eruption is imminent, but the very triviality of this influence
implies not only the absence of a general liquid interior, but also of
extensive reservoirs.
Hypothesis 2. Lavas assigned to molten reservoirs.—A modification
of the preceding view has been made to escape the difficulties involved in
the hypothesis as stated above. It is supposed that while nearly all the
subcrust solidified, numerous liquid spots were left scattered through it.
This honeycombed substratum is supposed to connect the continuous outer
crust with a central solid body, solidified because of pressure in spite of its
high temperature. This hypothesis escapes only a portion of the objections.
For instance, the lavas in Mauna Loa and Kilauea in Hawaii differ nearly
10,000 feet in height, and hence cannot well be supposed to connect with
the same reservoir, but they are both on the same vast cone, which implies
at least an equally large molten reservoir as its source. If there were two
distinct reservoirs of the required magnitude, they must be singularly placed
to supply vents so near and yet so independent. The difficulty grows greater
when the whole Hawaiian chain is considered, for the points of eruption
seem to have migrated from the northwesterly islands, where the volcanoes
are old, to the southeastern end, where volcanic activity is now in progress.
It would be natural under this view to suppose that these residuary
lakelets of liquid rock should be gradually exhausted as time goes on, and
that vulcanism should be a declining phenomenon. It is not clear that this is
the case. The great number of existing volcanoes in regions where great
extrusions took place in earlier ages does not seem to be in harmony with
the hypothesis.
II. On the Assumption that the Lavas are Secondary.
The serious difficulties that arise in interpreting volcanic lavas as
remnants of an original molten mass, and the strong arguments of recent
Page 714
years for a very solid earth, have turned inquiry chiefly toward the second
class of hypotheses, which refer the origin of lavas to the local melting of
deep-seated rock. These differ widely among themselves. One group seeks
for a cause of the melting in the penetration of surface air and water;
another, in the relief of pressure; a third, in crushing and shearing; a fourth,
in the depression of sediments into the heated interior zone; and a fifth, in
the outward flow of deep-seated heat.
Hypothesis 3. Lavas assigned to the reaction of water and air
penetrating to hot rocks.—As steam is one of the great factors in the
explosions of volcanoes, and as water reduces the melting-point of rocks, it
is a natural and simple view that water penetrating through the fissures and
pores of the outer crust and coming into contact with the heated rocks
below, is absorbed into them and renders them liquid, and that then, being
rendered swollen and lighter by the process, they ascend and discharge
quietly or explosively according to the special conditions of the case.
Naturally the suggestion arises that the waters would be converted into
steam long before they could reach rock hot enough to be melted, and that
this steam would be forced back along its own track, as the line of least
resistance, rather than force itself into the rock material and rise in the lava-
column; but to this it is answered that an experiment of Daubree’s has
shown that water will penetrate the capillaries of sandstone against high
steam pressure and add itself to the steam within. The fact is also cited that
certain substances, when highly heated, absorb gases which they give out
when they cool. The absorption of hydrogen by platinum, and of oxygen by
molten silver, are illustrations. It is certain that the lavas do contain large
quantities of absorbed gases, and that these are partly, and in most cases
largely, given out in cooling, when the cooling takes place at the surface.
The presumption is that the lavas would take the gases up again on
remelting under similar conditions. If the lavas of actual volcanoes had the
temperatures of aqueo-igneous fusion (700°–1000° Fahr.) only, it would
strengthen this view; but as temperatures of lavas often exceed 2000° Fahr.,
and probably sometimes reach 2500° Fahr., and perhaps 3000° Fahr., it is
not easy to account for such temperatures under this hypothesis, because
they would only be reached at levels far below those at which aqueo-
igneous fusion might be presumed to take place. Perhaps this could be met
by invoking pressure which might prevent even aqueo-igneous fusion from
class of hypotheses, which refer the origin of lavas to the local melting of
deep-seated rock. These differ widely among themselves. One group seeks
for a cause of the melting in the penetration of surface air and water;
another, in the relief of pressure; a third, in crushing and shearing; a fourth,
in the depression of sediments into the heated interior zone; and a fifth, in
the outward flow of deep-seated heat.
Hypothesis 3. Lavas assigned to the reaction of water and air
penetrating to hot rocks.—As steam is one of the great factors in the
explosions of volcanoes, and as water reduces the melting-point of rocks, it
is a natural and simple view that water penetrating through the fissures and
pores of the outer crust and coming into contact with the heated rocks
below, is absorbed into them and renders them liquid, and that then, being
rendered swollen and lighter by the process, they ascend and discharge
quietly or explosively according to the special conditions of the case.
Naturally the suggestion arises that the waters would be converted into
steam long before they could reach rock hot enough to be melted, and that
this steam would be forced back along its own track, as the line of least
resistance, rather than force itself into the rock material and rise in the lava-
column; but to this it is answered that an experiment of Daubree’s has
shown that water will penetrate the capillaries of sandstone against high
steam pressure and add itself to the steam within. The fact is also cited that
certain substances, when highly heated, absorb gases which they give out
when they cool. The absorption of hydrogen by platinum, and of oxygen by
molten silver, are illustrations. It is certain that the lavas do contain large
quantities of absorbed gases, and that these are partly, and in most cases
largely, given out in cooling, when the cooling takes place at the surface.
The presumption is that the lavas would take the gases up again on
remelting under similar conditions. If the lavas of actual volcanoes had the
temperatures of aqueo-igneous fusion (700°–1000° Fahr.) only, it would
strengthen this view; but as temperatures of lavas often exceed 2000° Fahr.,
and probably sometimes reach 2500° Fahr., and perhaps 3000° Fahr., it is
not easy to account for such temperatures under this hypothesis, because
they would only be reached at levels far below those at which aqueo-
igneous fusion might be presumed to take place. Perhaps this could be met
by invoking pressure which might prevent even aqueo-igneous fusion from
Page 715
taking place until these temperatures were reached, but pressure brings in a
grave difficulty in another line, as we shall presently see.
There is a phase of the water-penetration hypothesis which seeks to
account for an accession of heat. It is affirmed that the outer rocks are
oxidized, while the inner ones were not originally, or at least not completely
oxidized, and that air and water from the surface, reaching the unoxidized
zone, enter into combination and generate the necessary heat. This view
was pardonable before the development of modern thermo-chemistry, but is
now quite untenable, as may be shown by working out the reactions
thermally.
All views which assign the penetration of surface air or water as a cause
meet with a grave, if not insuperable, difficulty in the condition of the lower
part of the earth’s crust (see p. 218). The fractured condition of the crust,
which permits a ready penetration of water, is a very superficial
phenomenon. Below the first few thousand feet the crevices and porosities
of the rock are rapidly closed by the pressure of overlying rock, and all
appreciable crevices and pores probably disappear at a depth of five or six
miles. The effective function of fissures is, therefore, limited to the upper
few miles of the crust, and even here to certain portions only. The great
pressures in gas- and oil-wells show that in many quite superficial beds,
even when arched, there are no fissures or pores capable of letting even gas
escape effectively. The depths at which the temperatures of lavas are
reached are usually estimated, from the downward increase of temperature,
at 20 to 30 miles. This leaves from 14 to 24 miles of the compressed zone
between the lowest assignable limit of the fissured zone, and the highest
assignable zone for the origin of lavas. This thick zone of dense rock must
be reckoned with in all hypotheses that involve the penetration of air and
water from without, and, as well, the extrusion of lavas from within. In
addition to the difficulties of the penetration of ground-water, the
limitations of its heat, at penetrable depths, also bear adversely (see p. 219),
on the descent of air and water.
Hypothesis 4. Lavas assigned to relief of pressure.—It seems to be
demonstrated that pressure raises the melting-point of average rock, and
hence at twenty or thirty miles’ depth there may be rocks hot enough to melt
at the surface, but still solid because of high pressure. If this pressure were
in some way relieved they would become liquid. Pressure may be locally
grave difficulty in another line, as we shall presently see.
There is a phase of the water-penetration hypothesis which seeks to
account for an accession of heat. It is affirmed that the outer rocks are
oxidized, while the inner ones were not originally, or at least not completely
oxidized, and that air and water from the surface, reaching the unoxidized
zone, enter into combination and generate the necessary heat. This view
was pardonable before the development of modern thermo-chemistry, but is
now quite untenable, as may be shown by working out the reactions
thermally.
All views which assign the penetration of surface air or water as a cause
meet with a grave, if not insuperable, difficulty in the condition of the lower
part of the earth’s crust (see p. 218). The fractured condition of the crust,
which permits a ready penetration of water, is a very superficial
phenomenon. Below the first few thousand feet the crevices and porosities
of the rock are rapidly closed by the pressure of overlying rock, and all
appreciable crevices and pores probably disappear at a depth of five or six
miles. The effective function of fissures is, therefore, limited to the upper
few miles of the crust, and even here to certain portions only. The great
pressures in gas- and oil-wells show that in many quite superficial beds,
even when arched, there are no fissures or pores capable of letting even gas
escape effectively. The depths at which the temperatures of lavas are
reached are usually estimated, from the downward increase of temperature,
at 20 to 30 miles. This leaves from 14 to 24 miles of the compressed zone
between the lowest assignable limit of the fissured zone, and the highest
assignable zone for the origin of lavas. This thick zone of dense rock must
be reckoned with in all hypotheses that involve the penetration of air and
water from without, and, as well, the extrusion of lavas from within. In
addition to the difficulties of the penetration of ground-water, the
limitations of its heat, at penetrable depths, also bear adversely (see p. 219),
on the descent of air and water.
Hypothesis 4. Lavas assigned to relief of pressure.—It seems to be
demonstrated that pressure raises the melting-point of average rock, and
hence at twenty or thirty miles’ depth there may be rocks hot enough to melt
at the surface, but still solid because of high pressure. If this pressure were
in some way relieved they would become liquid. Pressure may be locally
Page 716
relieved somewhat (1) by denudation, (2) by certain phases of faulting, (3)
by anticlinal arches, and (4) by continental deformation.
(1) In most cases of denudation, cooling below probably keeps pace with
loss above. At any rate, many volcanoes rise from the bottoms of the oceans
where no denudation takes place, and this phase of the hypothesis is not
workable there.
(2) The theory of relief by faulting finds encouragement in the fact that
many volcanoes occur on fault-lines. There is no evidence, however, that
this is a universal or necessary relation. Computation as to the amount of
lowering of the melting-point that might arise from the faulting associated
with volcanoes indicates that it is necessary to suppose that the rocks were
already very close to the melting-point when the faulting took place, to
make the doctrine applicable. It is to be observed that in faulting the relief
of pressure on one side of the fault-line is likely to be balanced by increased
pressure on the other side, and that this difference in pressure may be lost
by distribution at a depth of 20 or 30 miles, where, at the nearest, this
delicate relation between solidity and liquidity, on which the theory is
dependent, may perhaps be reached.
(3) Immediately under an anticlinal arch there may doubtless be some
relief of pressure within the limits of strength of the arch, which is not great
(p. 582). The pressure under the arch as a whole is greater than before it
was bowed up by lateral thrust, and in depth this excess becomes distributed
so as to obliterate the local relief under the center of the arch, and so adds
the effects of folding to the average pressure of the crust. Besides, as a
matter of fact, volcanoes do not appear to be especially associated with
mountain folds where arching reaches its best expression.
(4) The same general considerations bear on the assignment of
liquefaction to relief of pressure in connection with the more general
deformation of the earth’s body. Besides, while relief of pressure might
account for liquefaction, it leaves the extrusion without an obvious cause;
indeed, it would seem to furnish a condition opposed to extrusion, and if
pressure were subsequently added to force the liquid out, it would tend to
restore the solid condition.
Hypothesis 5. Lavas assigned to melting by crushing.—Mallet[286] and
others have attributed melting to the crushing of rock. Crushing, in the
by anticlinal arches, and (4) by continental deformation.
(1) In most cases of denudation, cooling below probably keeps pace with
loss above. At any rate, many volcanoes rise from the bottoms of the oceans
where no denudation takes place, and this phase of the hypothesis is not
workable there.
(2) The theory of relief by faulting finds encouragement in the fact that
many volcanoes occur on fault-lines. There is no evidence, however, that
this is a universal or necessary relation. Computation as to the amount of
lowering of the melting-point that might arise from the faulting associated
with volcanoes indicates that it is necessary to suppose that the rocks were
already very close to the melting-point when the faulting took place, to
make the doctrine applicable. It is to be observed that in faulting the relief
of pressure on one side of the fault-line is likely to be balanced by increased
pressure on the other side, and that this difference in pressure may be lost
by distribution at a depth of 20 or 30 miles, where, at the nearest, this
delicate relation between solidity and liquidity, on which the theory is
dependent, may perhaps be reached.
(3) Immediately under an anticlinal arch there may doubtless be some
relief of pressure within the limits of strength of the arch, which is not great
(p. 582). The pressure under the arch as a whole is greater than before it
was bowed up by lateral thrust, and in depth this excess becomes distributed
so as to obliterate the local relief under the center of the arch, and so adds
the effects of folding to the average pressure of the crust. Besides, as a
matter of fact, volcanoes do not appear to be especially associated with
mountain folds where arching reaches its best expression.
(4) The same general considerations bear on the assignment of
liquefaction to relief of pressure in connection with the more general
deformation of the earth’s body. Besides, while relief of pressure might
account for liquefaction, it leaves the extrusion without an obvious cause;
indeed, it would seem to furnish a condition opposed to extrusion, and if
pressure were subsequently added to force the liquid out, it would tend to
restore the solid condition.
Hypothesis 5. Lavas assigned to melting by crushing.—Mallet[286] and
others have attributed melting to the crushing of rock. Crushing, in the
Page 717
ordinary sense of the term, can only take place in the zone of fracture, and
that is apparently too shallow to meet the requirements of the case. Below
this zone, the pressure on all sides is too great to permit any separation of
fragments, and a solid mass can only change its form by what is called
“solid flowage.” The rock under these conditions may be compressed, and
this compression must give rise to heat, but at the same time the melting-
point is raised, according to all experiments. It seems improbable that
melting can be produced in this way. If great pressure could be brought to
bear upon a tract of rock so as to heat it by compression, and if then the
pressure were relaxed before the heat generated could be distributed by
conduction, and if re-expansion did not follow, possibly melting could be
effected, but this makes the process complicated and apparently
inapplicable. It is scarcely possible that such a sequence of events can have
affected all the tracts that are now volcanic, much less all those that have
been such throughout geologic history. As noted in the preceding case,
relaxation would seem to be unfavorable to expulsion. Besides, volcanoes
do not seem to be confined to tracts that show signs of great crumpling and
crushing, as the Alps, the Appalachians, and the closely folded ranges
generally. Extrusions seem rather more common with faulted ranges where
crushing is less notable and where surface tension replaces compression.
Hypothesis 6. Lavas assigned to melting by depression.—It is
observed that in certain regions great thicknesses of sediments have
accumulated by the slow settling of the crust below, and as these sediments
obstruct the outward flow of heat while the lower beds settle nearer to the
interior source of heat, it is conceived that they become heated below and,
being saturated with water, take on aqueo-igneous fusion and rise as lavas,
well supplied with internal gas and steam from the water and volatile
constituents that were entrapped and carried down with them. The question
obviously arises whether such depression is sufficient to give the
temperatures the lavas show, and whether volcanic action is confined to
such areas of depression and deep sedimentation. At the highest credible
estimates—which are none the less to be taken with reserve—the post-
Archean sediments rarely reach five or six miles in thickness at any given
point, and probably never exceed ten or twelve, while twenty or thirty miles
is the computed depth required for the acquisition of the temperatures the
lavas actually possess. If the Archean terranes be included among the
sedimentaries, the thickness may be adequate, but what then of the Archean
that is apparently too shallow to meet the requirements of the case. Below
this zone, the pressure on all sides is too great to permit any separation of
fragments, and a solid mass can only change its form by what is called
“solid flowage.” The rock under these conditions may be compressed, and
this compression must give rise to heat, but at the same time the melting-
point is raised, according to all experiments. It seems improbable that
melting can be produced in this way. If great pressure could be brought to
bear upon a tract of rock so as to heat it by compression, and if then the
pressure were relaxed before the heat generated could be distributed by
conduction, and if re-expansion did not follow, possibly melting could be
effected, but this makes the process complicated and apparently
inapplicable. It is scarcely possible that such a sequence of events can have
affected all the tracts that are now volcanic, much less all those that have
been such throughout geologic history. As noted in the preceding case,
relaxation would seem to be unfavorable to expulsion. Besides, volcanoes
do not seem to be confined to tracts that show signs of great crumpling and
crushing, as the Alps, the Appalachians, and the closely folded ranges
generally. Extrusions seem rather more common with faulted ranges where
crushing is less notable and where surface tension replaces compression.
Hypothesis 6. Lavas assigned to melting by depression.—It is
observed that in certain regions great thicknesses of sediments have
accumulated by the slow settling of the crust below, and as these sediments
obstruct the outward flow of heat while the lower beds settle nearer to the
interior source of heat, it is conceived that they become heated below and,
being saturated with water, take on aqueo-igneous fusion and rise as lavas,
well supplied with internal gas and steam from the water and volatile
constituents that were entrapped and carried down with them. The question
obviously arises whether such depression is sufficient to give the
temperatures the lavas show, and whether volcanic action is confined to
such areas of depression and deep sedimentation. At the highest credible
estimates—which are none the less to be taken with reserve—the post-
Archean sediments rarely reach five or six miles in thickness at any given
point, and probably never exceed ten or twelve, while twenty or thirty miles
is the computed depth required for the acquisition of the temperatures the
lavas actually possess. If the Archean terranes be included among the
sedimentaries, the thickness may be adequate, but what then of the Archean
Page 718
vulcanism, which much surpasses that of later times, and the other early
extrusions before the sediments were thick; and what of the moon, where
there are probably no sediments at all?
Besides, it is not at all clear that the distribution of vulcanism is specially
related to that of thick sediments, as it should be if this hypothesis were the
true one. There are many volcanoes in the heart of the great oceans where
sedimentation is now inappreciable, and probably has been in all past
periods.
Hypothesis 7. Vulcanism assigned to the outflow of deep-seated heat.
—If the earth grew up by slow accessions of meteoroidal or planetesimal
matter, in a manner to be more fully set forth in the discussion of the origin
of the earth, and if its interior heat be due chiefly to compression by its own
gravity, the internal temperature would be originally distributed according
to the degree of compression, and this would depend on the intensity of the
internal pressure. This can be approximately computed, and is shown in the
diagram on page 563, where this subject has been treated. On not
improbable assumptions regarding the thermometric conductivity, the flow
of heat from the deep interior to the middle zone would be greater than the
loss of this zone to the superficial zone. This middle zone should, under this
view, experience a rising temperature. By hypothesis, this zone is composed
of various kinds of matter mixed as they happened to fall in. Hence as the
temperature rises, the fusion-points of some of these constituents will be
reached before those of others. More strictly, the temperatures at which
some of these constituents will mutually dissolve one another will be
reached, while other constituents remain undissolved, and thus a partial and
distributed liquefaction will arise. The gases and volatile constituents in the
mixed material would naturally enter largely into the liquefied portion. It is
assumed that with a continued rise of temperature, the partial liquefactions
would increase until the liquefied parts found means of uniting, and the
lighter portions, embracing the gaseous contingent, were able to work their
way toward the surface. As they rose by fusing or fluxing their way, the
pressure upon them became less and less, and hence the temperature
necessary for liquefaction gradually fell, leaving them a constantly renewed
margin of temperature available for melting their way through the upper
horizons. Thus it is conceived that these fusible and fluxing selections from
the middle zone might thread their ways up to the zone of fracture and
extrusions before the sediments were thick; and what of the moon, where
there are probably no sediments at all?
Besides, it is not at all clear that the distribution of vulcanism is specially
related to that of thick sediments, as it should be if this hypothesis were the
true one. There are many volcanoes in the heart of the great oceans where
sedimentation is now inappreciable, and probably has been in all past
periods.
Hypothesis 7. Vulcanism assigned to the outflow of deep-seated heat.
—If the earth grew up by slow accessions of meteoroidal or planetesimal
matter, in a manner to be more fully set forth in the discussion of the origin
of the earth, and if its interior heat be due chiefly to compression by its own
gravity, the internal temperature would be originally distributed according
to the degree of compression, and this would depend on the intensity of the
internal pressure. This can be approximately computed, and is shown in the
diagram on page 563, where this subject has been treated. On not
improbable assumptions regarding the thermometric conductivity, the flow
of heat from the deep interior to the middle zone would be greater than the
loss of this zone to the superficial zone. This middle zone should, under this
view, experience a rising temperature. By hypothesis, this zone is composed
of various kinds of matter mixed as they happened to fall in. Hence as the
temperature rises, the fusion-points of some of these constituents will be
reached before those of others. More strictly, the temperatures at which
some of these constituents will mutually dissolve one another will be
reached, while other constituents remain undissolved, and thus a partial and
distributed liquefaction will arise. The gases and volatile constituents in the
mixed material would naturally enter largely into the liquefied portion. It is
assumed that with a continued rise of temperature, the partial liquefactions
would increase until the liquefied parts found means of uniting, and the
lighter portions, embracing the gaseous contingent, were able to work their
way toward the surface. As they rose by fusing or fluxing their way, the
pressure upon them became less and less, and hence the temperature
necessary for liquefaction gradually fell, leaving them a constantly renewed
margin of temperature available for melting their way through the upper
horizons. Thus it is conceived that these fusible and fluxing selections from
the middle zone might thread their ways up to the zone of fracture and
Page 719
thence, taking advantage of fissures and fractures, reach the surface. It is
conceived that such liquefaction and extrusion would carry out from the
middle zone the excess of temperature received from the deeper interior,
and thus regulate its temperature and forestall general liquefaction, the zone
as a whole remaining always solid. The independence of volcanoes is
assigned to the independence of the liquid threads that worked their way to
the surface. Nothing like a reservoir or molten lake enters into the
conception. The prolonged action of volcanoes is attributed to the slow
feeding of the liquid threads from the locally fused middle zone. The
frequent pauses in action are assigned to temporary deficiencies of supply;
the renewals to the gathering of new supplies after a sufficient period of
accumulation. The distribution of volcanoes in essentially all latitudes and
longitudes is assigned to the general nature of the cause. The special surface
distributions are assumed to be influenced, though not altogether controlled,
by the favorable or unfavorable conditions for escape presented by the
crustal segments of the earth. The persistence of volcanic action in time is
attributed to the magnitude of the interior source, to its deep-seated
location, and to the slowness of conduction of heat in the earth’s interior.
The force of expulsion is found in the stress-differences in the interior,
particularly the periodic tidal and other astronomic stresses (see p. 580), and
in the slow pressure brought to bear on the slender threads of liquid by the
creep of the adjacent rock. The violent expulsions are due to the included
gases, of which steam is chief. Little efficiency is assigned to surface-
waters, and that little is regarded as wholly secondary and incidental. The
true volcanic gases are regarded as coming from the deep interior and as
being true accessions to the atmosphere and hydrosphere. The standing of
the lavas in volcanic ducts for hundreds and even thousands of years with
only small outflows, as in some of the best-known volcanoes, is regarded as
an exhibition of an approximate equilibrium between the hydrostatic
pressure of the deep-penetrating column of lava, and the flowage-tendency
of the rock-walls, the outflow being, of course, also conditioned on the slow
rate of supply below, and the periodic stress-differences of the interior.
For the present these hypotheses must be left to work out their own
destiny, serving in the mean time as stimulants of research. All but the last
have been for some time under the consideration of geologists, and are set
forth in the literature of the subject (p. 636).
conceived that such liquefaction and extrusion would carry out from the
middle zone the excess of temperature received from the deeper interior,
and thus regulate its temperature and forestall general liquefaction, the zone
as a whole remaining always solid. The independence of volcanoes is
assigned to the independence of the liquid threads that worked their way to
the surface. Nothing like a reservoir or molten lake enters into the
conception. The prolonged action of volcanoes is attributed to the slow
feeding of the liquid threads from the locally fused middle zone. The
frequent pauses in action are assigned to temporary deficiencies of supply;
the renewals to the gathering of new supplies after a sufficient period of
accumulation. The distribution of volcanoes in essentially all latitudes and
longitudes is assigned to the general nature of the cause. The special surface
distributions are assumed to be influenced, though not altogether controlled,
by the favorable or unfavorable conditions for escape presented by the
crustal segments of the earth. The persistence of volcanic action in time is
attributed to the magnitude of the interior source, to its deep-seated
location, and to the slowness of conduction of heat in the earth’s interior.
The force of expulsion is found in the stress-differences in the interior,
particularly the periodic tidal and other astronomic stresses (see p. 580), and
in the slow pressure brought to bear on the slender threads of liquid by the
creep of the adjacent rock. The violent expulsions are due to the included
gases, of which steam is chief. Little efficiency is assigned to surface-
waters, and that little is regarded as wholly secondary and incidental. The
true volcanic gases are regarded as coming from the deep interior and as
being true accessions to the atmosphere and hydrosphere. The standing of
the lavas in volcanic ducts for hundreds and even thousands of years with
only small outflows, as in some of the best-known volcanoes, is regarded as
an exhibition of an approximate equilibrium between the hydrostatic
pressure of the deep-penetrating column of lava, and the flowage-tendency
of the rock-walls, the outflow being, of course, also conditioned on the slow
rate of supply below, and the periodic stress-differences of the interior.
For the present these hypotheses must be left to work out their own
destiny, serving in the mean time as stimulants of research. All but the last
have been for some time under the consideration of geologists, and are set
forth in the literature of the subject (p. 636).
Page 720
A few special phases of the problem need further discussion, though they
have been incidentally touched upon.
Modes of Reaching the Surface.
All of the views that locate the origin of the lavas deep in the earth must
face the difficulties of the passage through the dense portion of the sphere
below the fracture zone. Near the surface, the lavas usually take advantage
of fissures or bedding-planes already existing or made by themselves. There
is little evidence that they bore their way by melting, though they round out
their ducts into pipes as they use them, much as streamlets on glaciers
falling into crevices round out moulins. But this use of fissures and
bedding-planes for passage is probably merely a matter of least resistance
where the lavas are relatively cool, and their capacity for melting is low or
perhaps even gone. Daly has recently urged that lavas work out reservoirs
and enlarge passageways for themselves by detaching masses of rock from
the roofs and sides of the spaces already occupied by them, these masses
either melting and mingling with the lava, or else sinking to lower positions
in the column. This process he designates stoping.[287]
In the denser and warmer zone below, the alternatives seem to be (1)
melting or fluxing, or (2) mechanical penetration without fracture. As rocks
“flow” in this zone by differential pressure without rupture, an included
liquid mass may be forced to flow through the zone by sufficient
differential pressure. If local differential pressures at the surface be
neglected as probably incompetent, there only remain the stress-differences
of the interior and the differences of hydrostatic pressure between the lava-
column and the surrounding solid columns. The latter would not be great
until a column of liquid of much depth was formed, and the former would
probably not be concentrated on the liquid in such a way as to force it
bodily through the solid rock. Probably fusing or fluxing its way with the
aid of stress-differences is the chief resource of the lava in the initial stages.
In this it may be supposed to be assisted by its gases, by its selective fusible
and fluxing nature, by its very high temperature if it comes from very great
depths, as held in the seventh hypothesis, and by the stress-differences
which prevail in the deep interior, as shown in the last chapter. In ascending
from lower to higher horizons, the lava would be constantly invading
regions of lower melting-point because of less pressure. It would thus
have been incidentally touched upon.
Modes of Reaching the Surface.
All of the views that locate the origin of the lavas deep in the earth must
face the difficulties of the passage through the dense portion of the sphere
below the fracture zone. Near the surface, the lavas usually take advantage
of fissures or bedding-planes already existing or made by themselves. There
is little evidence that they bore their way by melting, though they round out
their ducts into pipes as they use them, much as streamlets on glaciers
falling into crevices round out moulins. But this use of fissures and
bedding-planes for passage is probably merely a matter of least resistance
where the lavas are relatively cool, and their capacity for melting is low or
perhaps even gone. Daly has recently urged that lavas work out reservoirs
and enlarge passageways for themselves by detaching masses of rock from
the roofs and sides of the spaces already occupied by them, these masses
either melting and mingling with the lava, or else sinking to lower positions
in the column. This process he designates stoping.[287]
In the denser and warmer zone below, the alternatives seem to be (1)
melting or fluxing, or (2) mechanical penetration without fracture. As rocks
“flow” in this zone by differential pressure without rupture, an included
liquid mass may be forced to flow through the zone by sufficient
differential pressure. If local differential pressures at the surface be
neglected as probably incompetent, there only remain the stress-differences
of the interior and the differences of hydrostatic pressure between the lava-
column and the surrounding solid columns. The latter would not be great
until a column of liquid of much depth was formed, and the former would
probably not be concentrated on the liquid in such a way as to force it
bodily through the solid rock. Probably fusing or fluxing its way with the
aid of stress-differences is the chief resource of the lava in the initial stages.
In this it may be supposed to be assisted by its gases, by its selective fusible
and fluxing nature, by its very high temperature if it comes from very great
depths, as held in the seventh hypothesis, and by the stress-differences
which prevail in the deep interior, as shown in the last chapter. In ascending
from lower to higher horizons, the lava would be constantly invading
regions of lower melting-point because of less pressure. It would thus
Page 721
always have an excess of heat above the local melting temperature until it
invaded the external, cool zone, where the regional temperature is below the
melting-point of surface pressure. From that point on it must constantly lose
portions of its excess of temperature by contact with cooler rocks, and
probably in the process of fluxing its way in the compact zone. If this
excess is insufficient to enable it to reach the zone of fracture, the ascending
column is arrested and becomes merely a plutonic pipe or mass. If it
suffices to reach the zone of fracture, advantage may be taken thereafter of
fissures and of rupturing, and the problem of further ascent probably
becomes chiefly one of hydrostatic pressure, in which the ascent of the
lava-column is favored by its high temperature and its included gases. The
hydrostatic contest is here between the lava-column, measured to its
extreme base, and the adjacent rock-columns, measured to the same extreme
depth. The result is, therefore, not necessarily dependent on the flowage of
the outer rocks, but may be essentially or wholly dependent on the deep-
seated flowage of the rock of the lower horizons. The ascending column
may reach hydrostatic equilibrium before it reaches the surface, and may
then form underground intrusions of various sorts without superficial
eruption, or it may only find equilibrium by coming to the surface and
pouring out a portion of its substance and discharging its gases.
Additional Considerations Relative to the Gases.
The question whether the volcanic gases are a contribution to the
atmosphere and hydrosphere is so important in its bearings on the whole
history of the atmosphere as to merit additional consideration here. As
already noted, if the volcanic gases arise from water and absorbed air that
have previously passed down through the strata, there is no real
contribution to the hydrosphere and atmosphere, but merely circulation. If
the gases are chiefly derived from the deep interior, they are an important
accession to the atmosphere and hydrosphere.
Most views are more or less intermediate, assigning a part of the gases to
the interior and a part to the exterior. No one will question that some part at
least of the steam is due to the contact between the ground-waters and the
hot lava, and probably no one will question that some gas comes from the
interior if the lavas originate there. The vital question is, whence comes the
major portion? Are the constant ebullitions of some volcanoes and the
invaded the external, cool zone, where the regional temperature is below the
melting-point of surface pressure. From that point on it must constantly lose
portions of its excess of temperature by contact with cooler rocks, and
probably in the process of fluxing its way in the compact zone. If this
excess is insufficient to enable it to reach the zone of fracture, the ascending
column is arrested and becomes merely a plutonic pipe or mass. If it
suffices to reach the zone of fracture, advantage may be taken thereafter of
fissures and of rupturing, and the problem of further ascent probably
becomes chiefly one of hydrostatic pressure, in which the ascent of the
lava-column is favored by its high temperature and its included gases. The
hydrostatic contest is here between the lava-column, measured to its
extreme base, and the adjacent rock-columns, measured to the same extreme
depth. The result is, therefore, not necessarily dependent on the flowage of
the outer rocks, but may be essentially or wholly dependent on the deep-
seated flowage of the rock of the lower horizons. The ascending column
may reach hydrostatic equilibrium before it reaches the surface, and may
then form underground intrusions of various sorts without superficial
eruption, or it may only find equilibrium by coming to the surface and
pouring out a portion of its substance and discharging its gases.
Additional Considerations Relative to the Gases.
The question whether the volcanic gases are a contribution to the
atmosphere and hydrosphere is so important in its bearings on the whole
history of the atmosphere as to merit additional consideration here. As
already noted, if the volcanic gases arise from water and absorbed air that
have previously passed down through the strata, there is no real
contribution to the hydrosphere and atmosphere, but merely circulation. If
the gases are chiefly derived from the deep interior, they are an important
accession to the atmosphere and hydrosphere.
Most views are more or less intermediate, assigning a part of the gases to
the interior and a part to the exterior. No one will question that some part at
least of the steam is due to the contact between the ground-waters and the
hot lava, and probably no one will question that some gas comes from the
interior if the lavas originate there. The vital question is, whence comes the
major portion? Are the constant ebullitions of some volcanoes and the
Page 722
terrific explosions of others due mainly to surface-waters, or to interior
gases?
It seems to be certain that in most cases the gases are diffused through the
substance of the lava, and are not simply in contact with the walls of the
column or with its summit. Without doubt steam is generated around the
lava-column by external contact, and perhaps some explosions are due to
the entrance of the rising lava upon a crevice or cavern filled with water, or
to the invasion of a lake gathered in an old crater; but it still remains a
question whether the importance of such explosions has not been
exaggerated. Such action does not seem competent to produce inflated
lavas, but merely shattered ones. Water thus “suddenly flashed into steam”
could scarcely diffuse itself intimately through the lava, for the process of
diffusion is exceedingly slow. But inflated lavas, pumice, scoriæ, and
cinders are the typical products of explosive vulcanism. Not only in the
ordinary Vesuvian type, but in the extraordinary Krakatoan type, inflated
lavas are the dominant product. Prodigious quantities of this covered the sea
about Krakatoa after its tremendous explosion in 1883. Judd estimates that
the volume of included steam involved in the inflation of the pumice
examined by him, was from three to five times that of the rock, and that the
amount involved in exploding the lava into the fine dust that floated in the
upper atmosphere for months, was presumably much greater.
If the sudden flashing into steam of bodies of water in external contact
with hot lava be rejected as only an incidental source of explosion, it
remains to be considered whether waters permeating the rock and becoming
converted into steam may not be absorbed into the rising lava, become
diffused through it, and ascending with it, explode at the surface. So far as
access through fissures and cavities large enough to be entered by lava are
concerned, it may safely be concluded that since the hydrostatic pressure of
the lava must be greater than that of the water in the fissures, or else it could
not rise, the lava will enter them, forcing back the water or the steam
generated from it, and, having penetrated as far as accessible, will solidify
as a dike, and plug up the avenue of contact between the ground-water and
the portion of the lava still remaining molten. The numerous dikes that
attend volcanic necks testify to the prevalence of this action. The capillary
pores of the wall-rock, which cannot be thus bodily occupied by the lava,
must doubtless become filled with steam, and this, following the principles
gases?
It seems to be certain that in most cases the gases are diffused through the
substance of the lava, and are not simply in contact with the walls of the
column or with its summit. Without doubt steam is generated around the
lava-column by external contact, and perhaps some explosions are due to
the entrance of the rising lava upon a crevice or cavern filled with water, or
to the invasion of a lake gathered in an old crater; but it still remains a
question whether the importance of such explosions has not been
exaggerated. Such action does not seem competent to produce inflated
lavas, but merely shattered ones. Water thus “suddenly flashed into steam”
could scarcely diffuse itself intimately through the lava, for the process of
diffusion is exceedingly slow. But inflated lavas, pumice, scoriæ, and
cinders are the typical products of explosive vulcanism. Not only in the
ordinary Vesuvian type, but in the extraordinary Krakatoan type, inflated
lavas are the dominant product. Prodigious quantities of this covered the sea
about Krakatoa after its tremendous explosion in 1883. Judd estimates that
the volume of included steam involved in the inflation of the pumice
examined by him, was from three to five times that of the rock, and that the
amount involved in exploding the lava into the fine dust that floated in the
upper atmosphere for months, was presumably much greater.
If the sudden flashing into steam of bodies of water in external contact
with hot lava be rejected as only an incidental source of explosion, it
remains to be considered whether waters permeating the rock and becoming
converted into steam may not be absorbed into the rising lava, become
diffused through it, and ascending with it, explode at the surface. So far as
access through fissures and cavities large enough to be entered by lava are
concerned, it may safely be concluded that since the hydrostatic pressure of
the lava must be greater than that of the water in the fissures, or else it could
not rise, the lava will enter them, forcing back the water or the steam
generated from it, and, having penetrated as far as accessible, will solidify
as a dike, and plug up the avenue of contact between the ground-water and
the portion of the lava still remaining molten. The numerous dikes that
attend volcanic necks testify to the prevalence of this action. The capillary
pores of the wall-rock, which cannot be thus bodily occupied by the lava,
must doubtless become filled with steam, and this, following the principles
Page 723
of Daubree’s experiment, will force itself into contact with the lava and be
absorbed by it, but whether this will be in sufficient quantity, and will
become sufficiently diffused through the body of the lava-column to
produce the observed effects, is an open question. The increasing testimony
of deep mining is that relatively little water flows through the deeper
horizons. It is urged that the water remaining in solidified lavas is very
unequal in distribution, as though due to unequal access and partial
diffusion. The argument seems strong, but to make it thoroughly good, it
must be shown that this inequality is not due to irregularity of discharge of
the gases during and after eruption, rather than to irregularity of original
accession. There is, perhaps, as much ground for assigning differences in
the degree of parting with the included gases, as in acquiring them.
Doubtless those lavas that boiled and seethed for a long period in the
caldron were more fully deprived of their gases than those that were more
promptly disgorged and cooled with less convection and surface exposure.
Thermal considerations.—Probably the most important consideration
relates to the heat effects. If underground-waters enter the lava-column and
come forth as steam, great quantities of heat are consumed in the process.
Has the lava a sufficient excess of heat to stand this? Can ebullition be
maintained for the observed periods if the steam comes from ground-
waters?
Many lavas probably do not carry a very large excess of heat above that
necessary for liquefaction, for not a few of them contain crystals already
forming, which shows that they are within the range of the temperatures of
solidification of their constituents. The same conclusion is indicated by the
limited fusing effects shown by the walls of dikes and sills. On the other
hand, as already remarked, dikes and sills often show the effects of a rather
rapid cooling from the walls. The method of flow often implies the same
condition for the acidic lavas, since they usually behave as stiff, pasty
masses of limited liquidity. On the other hand, the basic lavas, whose
fusion-point is much lower, often flow freely and reach great distances
before solidifying. The facts taken altogether imply that the average
temperature of the lavas is not much above the fusing-point of the acidic
lavas, while it may probably be very considerably above the fusing-point of
basalt. For a rough estimate, with no pretensions to accuracy, it may be
assumed that in an average case there are 500° Fahr. excess, but probably
absorbed by it, but whether this will be in sufficient quantity, and will
become sufficiently diffused through the body of the lava-column to
produce the observed effects, is an open question. The increasing testimony
of deep mining is that relatively little water flows through the deeper
horizons. It is urged that the water remaining in solidified lavas is very
unequal in distribution, as though due to unequal access and partial
diffusion. The argument seems strong, but to make it thoroughly good, it
must be shown that this inequality is not due to irregularity of discharge of
the gases during and after eruption, rather than to irregularity of original
accession. There is, perhaps, as much ground for assigning differences in
the degree of parting with the included gases, as in acquiring them.
Doubtless those lavas that boiled and seethed for a long period in the
caldron were more fully deprived of their gases than those that were more
promptly disgorged and cooled with less convection and surface exposure.
Thermal considerations.—Probably the most important consideration
relates to the heat effects. If underground-waters enter the lava-column and
come forth as steam, great quantities of heat are consumed in the process.
Has the lava a sufficient excess of heat to stand this? Can ebullition be
maintained for the observed periods if the steam comes from ground-
waters?
Many lavas probably do not carry a very large excess of heat above that
necessary for liquefaction, for not a few of them contain crystals already
forming, which shows that they are within the range of the temperatures of
solidification of their constituents. The same conclusion is indicated by the
limited fusing effects shown by the walls of dikes and sills. On the other
hand, as already remarked, dikes and sills often show the effects of a rather
rapid cooling from the walls. The method of flow often implies the same
condition for the acidic lavas, since they usually behave as stiff, pasty
masses of limited liquidity. On the other hand, the basic lavas, whose
fusion-point is much lower, often flow freely and reach great distances
before solidifying. The facts taken altogether imply that the average
temperature of the lavas is not much above the fusing-point of the acidic
lavas, while it may probably be very considerably above the fusing-point of
basalt. For a rough estimate, with no pretensions to accuracy, it may be
assumed that in an average case there are 500° Fahr. excess, but probably
Page 724
not 1000° Fahr. A computation based on even so rough an estimate as this
may, by showing the order of magnitude of the thermal considerations,
indicate their radical bearing. The average temperature of the ground-water
of the upper two or three miles of the crust—the only portion through which
water probably penetrates with sufficient freedom to be effective in this
case—is probably less than 200° Fahr. The specific heat of rock appears to
average somewhat less than 0.2. The temperature of the lava may be taken
at 3000° Fahr. as a sufficiently high average. From these data it follows that
if an amount of ground-water equal to five percent. of the volume of the
lava entered the lava and was brought up to its temperature and then
discharged, the temperature of the whole mass would be lowered 550° Fahr.
It is therefore evident that only a small percentage of surface-water can pass
through the lava consistently with its continued fluidity.
M. Fouqué estimated that the discharge of steam from a merely parasitic
cone of Etna during 100 days was equal to 2,100,000 cubic meters of water.
If this were ground-water, and the lava from which it issued had an excess
of 500° Fahr. above the fusion-point, the formation of this steam would
congeal a column 400 feet in diameter and 3000 feet deep in the time given.
If this case is typical, and if Fouqué’s estimate is not greatly exaggerated or
very exceptional, the view that any large portion of the steam from
volcanoes comes from surface-waters seems to be incompatible with the
persistence of ebullition and explosion which many of them exhibit.
Stromboli has been in constant eruption as far back as the history of the
region runs. It is now exploding every three to ten minutes, and yet the
mass of lava seems to be small and its outflow inconsiderable. Is it possible
that a current of steam, given out with this activity for so long a period, was
derived from adjacent ground-waters, and has not yet solidified the lava?
The problem takes on a very different aspect if the steam, or at least some
large part of it, rises from great depths and brings thence an excess of heat.
It then becomes an agency for the maintenance of the liquidity of the lava,
for giving it convective motion, and for promoting explosive action, so long
as it continues to rise.
For these and other reasons the balance of present evidence seems to us
to favor the view that most of the steam and other gases come with the lava
from its original source deep in the earth.
may, by showing the order of magnitude of the thermal considerations,
indicate their radical bearing. The average temperature of the ground-water
of the upper two or three miles of the crust—the only portion through which
water probably penetrates with sufficient freedom to be effective in this
case—is probably less than 200° Fahr. The specific heat of rock appears to
average somewhat less than 0.2. The temperature of the lava may be taken
at 3000° Fahr. as a sufficiently high average. From these data it follows that
if an amount of ground-water equal to five percent. of the volume of the
lava entered the lava and was brought up to its temperature and then
discharged, the temperature of the whole mass would be lowered 550° Fahr.
It is therefore evident that only a small percentage of surface-water can pass
through the lava consistently with its continued fluidity.
M. Fouqué estimated that the discharge of steam from a merely parasitic
cone of Etna during 100 days was equal to 2,100,000 cubic meters of water.
If this were ground-water, and the lava from which it issued had an excess
of 500° Fahr. above the fusion-point, the formation of this steam would
congeal a column 400 feet in diameter and 3000 feet deep in the time given.
If this case is typical, and if Fouqué’s estimate is not greatly exaggerated or
very exceptional, the view that any large portion of the steam from
volcanoes comes from surface-waters seems to be incompatible with the
persistence of ebullition and explosion which many of them exhibit.
Stromboli has been in constant eruption as far back as the history of the
region runs. It is now exploding every three to ten minutes, and yet the
mass of lava seems to be small and its outflow inconsiderable. Is it possible
that a current of steam, given out with this activity for so long a period, was
derived from adjacent ground-waters, and has not yet solidified the lava?
The problem takes on a very different aspect if the steam, or at least some
large part of it, rises from great depths and brings thence an excess of heat.
It then becomes an agency for the maintenance of the liquidity of the lava,
for giving it convective motion, and for promoting explosive action, so long
as it continues to rise.
For these and other reasons the balance of present evidence seems to us
to favor the view that most of the steam and other gases come with the lava
from its original source deep in the earth.
Page 725
References on vulcanism.—G. P. Scrope, Volcanoes, London,
1872. R. Mallet, on Volcanic Energy, Phil. Trans., 1873. C.
Darwin, Geological Observations on Volcanic Islands, London,
1876. E. Reyer, Beitrag zur Physik der Eruptionen, Vienna,
1877; Theoretische Geologie, 1888. Fouqué, Santorin et ses
Éruptions, Paris, 1879, Sartoris von Waltershausen and A. von
Lasaulx, Der Aetna, Leipzig, 1880. C. E. Dutton, Geology of the
High Plateaus of Utah, U. S. Geog. and Geol. Surv., 1880; The
Hawaiian Volcanoes, Fourth Ann. Rept. U. S. Geol. Surv., 1883.
Judd, Volcanoes, 1881; The Eruption of Krakatoa (Com. of the
Roy. Soc.), 1888. J. D. Dana, Characteristics of Volcanoes,
1890. H. J. Johnston-Lavis, The South Italian Volcanoes,
Naples, 1891. E. Hull, Volcanoes, Past and Present, 1892. Milne
and Burton, The Volcanoes of Japan, 1892. J. P. Iddings, The
Origin of Igneous Rocks, Bull. Phil. Soc., Washington, Vol. XII,
1892. A. C. Lane, Geologic Activity of the Earth’s Originally
Absorbed Gases, Bull. Geol. Soc. Am., Vol. V, 1894. A. Geikie,
Ancient Volcanoes of Great Britain, London, 1897. I. C. Russell,
Volcanoes of North America, 1897. T. G. Bonney, Volcanoes,
Their Structure and Significance, New York (and London),
1899. F. Miron, Étude des Phénomènes Volcaniques, Paris,
1903. G. C. Curtis, Secondary Phenomena of the West Indian
Volcanic Eruptions of 1902, Jour. Geol., Vol. XI, No. 2, 1903. A.
Heilprin, Mont Pelée and the Tragedy of Martinique,
Philadelphia (and London), 1903. Robert T. Hill, Report on the
Volcanic Disturbances in the West Indies, Nat’l Geog. Mag.,
Vol. XIII, No. 7, 1902. I. C. Russell, The Recent Volcanic
Eruptions in the West Indies, Nat’l Geog. Mag., Vol. XIII, No. 7,
1902; Volcanic Eruptions on Martinique and St. Vincent, Nat’l
Geog. Mag., Vol. XIII, No. 12, 1902. J. S. Diller, Volcanic
Rocks of Martinique and St. Vincent, Nat’l Geog. Mag., Vol.
XIII, No. 7, 1902. W. F. Hillebrand, Chemical Discussion of
Analyses of Volcanic Ejecta from Martinique and St. Vincent,
Nat’l Geog. Mag., Vol. XIII, No. 7, 1902. E. O. Hovey, The
Eruptions of La Soufrière, St. Vincent, in May, 1902, Nat’l
Geog. Mag., Vol. XIII, No. 12, 1902.
1872. R. Mallet, on Volcanic Energy, Phil. Trans., 1873. C.
Darwin, Geological Observations on Volcanic Islands, London,
1876. E. Reyer, Beitrag zur Physik der Eruptionen, Vienna,
1877; Theoretische Geologie, 1888. Fouqué, Santorin et ses
Éruptions, Paris, 1879, Sartoris von Waltershausen and A. von
Lasaulx, Der Aetna, Leipzig, 1880. C. E. Dutton, Geology of the
High Plateaus of Utah, U. S. Geog. and Geol. Surv., 1880; The
Hawaiian Volcanoes, Fourth Ann. Rept. U. S. Geol. Surv., 1883.
Judd, Volcanoes, 1881; The Eruption of Krakatoa (Com. of the
Roy. Soc.), 1888. J. D. Dana, Characteristics of Volcanoes,
1890. H. J. Johnston-Lavis, The South Italian Volcanoes,
Naples, 1891. E. Hull, Volcanoes, Past and Present, 1892. Milne
and Burton, The Volcanoes of Japan, 1892. J. P. Iddings, The
Origin of Igneous Rocks, Bull. Phil. Soc., Washington, Vol. XII,
1892. A. C. Lane, Geologic Activity of the Earth’s Originally
Absorbed Gases, Bull. Geol. Soc. Am., Vol. V, 1894. A. Geikie,
Ancient Volcanoes of Great Britain, London, 1897. I. C. Russell,
Volcanoes of North America, 1897. T. G. Bonney, Volcanoes,
Their Structure and Significance, New York (and London),
1899. F. Miron, Étude des Phénomènes Volcaniques, Paris,
1903. G. C. Curtis, Secondary Phenomena of the West Indian
Volcanic Eruptions of 1902, Jour. Geol., Vol. XI, No. 2, 1903. A.
Heilprin, Mont Pelée and the Tragedy of Martinique,
Philadelphia (and London), 1903. Robert T. Hill, Report on the
Volcanic Disturbances in the West Indies, Nat’l Geog. Mag.,
Vol. XIII, No. 7, 1902. I. C. Russell, The Recent Volcanic
Eruptions in the West Indies, Nat’l Geog. Mag., Vol. XIII, No. 7,
1902; Volcanic Eruptions on Martinique and St. Vincent, Nat’l
Geog. Mag., Vol. XIII, No. 12, 1902. J. S. Diller, Volcanic
Rocks of Martinique and St. Vincent, Nat’l Geog. Mag., Vol.
XIII, No. 7, 1902. W. F. Hillebrand, Chemical Discussion of
Analyses of Volcanic Ejecta from Martinique and St. Vincent,
Nat’l Geog. Mag., Vol. XIII, No. 7, 1902. E. O. Hovey, The
Eruptions of La Soufrière, St. Vincent, in May, 1902, Nat’l
Geog. Mag., Vol. XIII, No. 12, 1902.
Page 726
CHAPTER XI.
THE GEOLOGIC FUNCTIONS OF LIFE.
I. THE DISTINCTIVE FEATURES OF ORGANIC PROCESSES.
There is no reason to suppose that life processes, as we know them, were
in operation in the earliest stages of the earth’s history. They were
introduced and developed gradually during its progress. With life there
came into the processes of the earth’s development three distinctive factors:
A. Certain chemical actions giving rise to compounds that are not known
to occur independently of life.
B. Certain modes of aggregation of material, and certain kinds of bodily
movements, not known except in association with life.
C. The mental element, under the direction of which certain new
processes were inaugurated, and certain previous processes were modified
and controlled.
A. The Chemical Work of Life.
The peculiar chemical phenomena connected with life chiefly concern
the carbon compounds. In the inorganic world the carbon compounds are
few and simple. In the organic world they become extremely numerous and
complicated. These compounds are very unstable, for the greater part, and
their partial decomposition gives rise to many additional compounds. Some
of the true organic compounds and some of their decomposition products
have the power of combining with inorganic substances, and so produce an
additional series of semi-organic combinations. The total number of the
compounds thus directly and indirectly connected with life greatly exceeds
that of all inorganic compounds. Their mass, however, is very greatly
inferior.
THE GEOLOGIC FUNCTIONS OF LIFE.
I. THE DISTINCTIVE FEATURES OF ORGANIC PROCESSES.
There is no reason to suppose that life processes, as we know them, were
in operation in the earliest stages of the earth’s history. They were
introduced and developed gradually during its progress. With life there
came into the processes of the earth’s development three distinctive factors:
A. Certain chemical actions giving rise to compounds that are not known
to occur independently of life.
B. Certain modes of aggregation of material, and certain kinds of bodily
movements, not known except in association with life.
C. The mental element, under the direction of which certain new
processes were inaugurated, and certain previous processes were modified
and controlled.
A. The Chemical Work of Life.
The peculiar chemical phenomena connected with life chiefly concern
the carbon compounds. In the inorganic world the carbon compounds are
few and simple. In the organic world they become extremely numerous and
complicated. These compounds are very unstable, for the greater part, and
their partial decomposition gives rise to many additional compounds. Some
of the true organic compounds and some of their decomposition products
have the power of combining with inorganic substances, and so produce an
additional series of semi-organic combinations. The total number of the
compounds thus directly and indirectly connected with life greatly exceeds
that of all inorganic compounds. Their mass, however, is very greatly
inferior.
Page 727
Life material chiefly atmospheric.—In the building up of the organic
compounds, a necessary step is the decomposition of certain inorganic
compounds. The chief of these is the carbon dioxide of the atmosphere and
hydrosphere, the decomposition of which furnishes the carbon needed for
the organic compounds. On this account carbon dioxide may be regarded as
in some sense the basal material or the fundamental food of the organic
kingdom, and hence it plays a radical rôle in the life-history of the earth.
Water, and the constituents of water, oxygen and hydrogen, play a larger
part quantitatively, but a less distinctive part.
Nitrogen is also an essential element, and usually stands next to carbon,
oxygen, and hydrogen in quantity.
These, it will be noted, are all atmospheric constituents, and the material
of life is, therefore, dominantly atmospheric. This is even true of aquatic
life, for it lives largely on the atmospheric constituents dissolved in the
water. The function of life, considered from the material point of view, is
not only fundamentally concerned with the atmosphere, and intimately
dependent on its conditions, but its most important material effects appear
to lie in its modification of the constitution of the atmosphere.
The non-atmospheric factors.—The atmospheric constituents are not,
however, the only elements intimately connected with the life function.
Compounds of sulphur, phosphorus, potassium, sodium, chlorine, iron,
calcium, magnesium, silicon, and other elements are more or less essential
to the life of many organisms, or are employed by them for their skeletons,
coverings, etc. Incidentally, nearly all the common elements become
intimately related to living organisms either in the relations of active
elements in their physiological functions, or of passive elements in their
structure or in their auxiliary parts.
Three Classes of Effects.
Out of life processes grow three rather distinct classes of results: (1)
changes in the amounts and proportions of the constituents of the
atmosphere and, to some slight extent, of the hydrosphere and lithosphere;
(2) aid or hindrance to inorganic processes, such as disintegration, erosion,
and deposition; and (3) distinctive products, either (a) of organic matter that
compounds, a necessary step is the decomposition of certain inorganic
compounds. The chief of these is the carbon dioxide of the atmosphere and
hydrosphere, the decomposition of which furnishes the carbon needed for
the organic compounds. On this account carbon dioxide may be regarded as
in some sense the basal material or the fundamental food of the organic
kingdom, and hence it plays a radical rôle in the life-history of the earth.
Water, and the constituents of water, oxygen and hydrogen, play a larger
part quantitatively, but a less distinctive part.
Nitrogen is also an essential element, and usually stands next to carbon,
oxygen, and hydrogen in quantity.
These, it will be noted, are all atmospheric constituents, and the material
of life is, therefore, dominantly atmospheric. This is even true of aquatic
life, for it lives largely on the atmospheric constituents dissolved in the
water. The function of life, considered from the material point of view, is
not only fundamentally concerned with the atmosphere, and intimately
dependent on its conditions, but its most important material effects appear
to lie in its modification of the constitution of the atmosphere.
The non-atmospheric factors.—The atmospheric constituents are not,
however, the only elements intimately connected with the life function.
Compounds of sulphur, phosphorus, potassium, sodium, chlorine, iron,
calcium, magnesium, silicon, and other elements are more or less essential
to the life of many organisms, or are employed by them for their skeletons,
coverings, etc. Incidentally, nearly all the common elements become
intimately related to living organisms either in the relations of active
elements in their physiological functions, or of passive elements in their
structure or in their auxiliary parts.
Three Classes of Effects.
Out of life processes grow three rather distinct classes of results: (1)
changes in the amounts and proportions of the constituents of the
atmosphere and, to some slight extent, of the hydrosphere and lithosphere;
(2) aid or hindrance to inorganic processes, such as disintegration, erosion,
and deposition; and (3) distinctive products, either (a) of organic matter that
Page 728
would not have come into the existing combination but for life, such as
peat, lignite, amber, etc., or (b) of special forms of inorganic matter that
would not have arisen but for life, such as coral deposits, shell-marl, diatom
ooze, etc.
(1) Changes in the composition of the atmosphere.
The succession of modifications which the atmosphere has undergone
from time to time through the action of life will be discussed as the earth’s
history is followed in the second volume. It may suffice here to note briefly
the chief ways in which the atmosphere has probably been modified by the
agency of life, not only as regards its quantity but also as regards the
proportions of its constituents.
The consumption and restoration of carbon dioxide.—As the
fundamental food of the organic world, carbon dioxide has suffered
enormous consumption in the course of the geological ages, and is now
reduced to the very small proportion of .0004 or .0003 of the whole. At the
outset it was probably one of the most abundant constituents; possibly even
the chief one. It has been partially restored, concurrently with its
consumption, by animal respiration, by certain classes of plant action, and
by combustion and other forms of inorganic combination. This restorative
action has been incomplete at all known stages of the earth’s history, and
hence there has been constant loss of carbon dioxide. The inorganic
processes which have also profoundly affected both the consumption and
restoration of carbon dioxide are here neglected and discussed elsewhere.
The freeing and consumption of oxygen.—The oxygen of the
atmosphere is actively consumed by animals and by plants, but on the other
hand, it is set free abundantly by green plants, and hence its amount has
probably fluctuated from time to time according to the state of balance
between the organic processes of its production, and those of its
consumption. The consumption of oxygen by organic processes is, however,
little more than a reversal of the previous process by which it was set free;
for instance, green plants in forming their food set free the oxygen of the
carbon dioxide used for the purpose. When the organic substance so formed
is ultimately consumed through plant or animal action or by inorganic
means, an equivalent amount of oxygen reunites with the carbon to again
peat, lignite, amber, etc., or (b) of special forms of inorganic matter that
would not have arisen but for life, such as coral deposits, shell-marl, diatom
ooze, etc.
(1) Changes in the composition of the atmosphere.
The succession of modifications which the atmosphere has undergone
from time to time through the action of life will be discussed as the earth’s
history is followed in the second volume. It may suffice here to note briefly
the chief ways in which the atmosphere has probably been modified by the
agency of life, not only as regards its quantity but also as regards the
proportions of its constituents.
The consumption and restoration of carbon dioxide.—As the
fundamental food of the organic world, carbon dioxide has suffered
enormous consumption in the course of the geological ages, and is now
reduced to the very small proportion of .0004 or .0003 of the whole. At the
outset it was probably one of the most abundant constituents; possibly even
the chief one. It has been partially restored, concurrently with its
consumption, by animal respiration, by certain classes of plant action, and
by combustion and other forms of inorganic combination. This restorative
action has been incomplete at all known stages of the earth’s history, and
hence there has been constant loss of carbon dioxide. The inorganic
processes which have also profoundly affected both the consumption and
restoration of carbon dioxide are here neglected and discussed elsewhere.
The freeing and consumption of oxygen.—The oxygen of the
atmosphere is actively consumed by animals and by plants, but on the other
hand, it is set free abundantly by green plants, and hence its amount has
probably fluctuated from time to time according to the state of balance
between the organic processes of its production, and those of its
consumption. The consumption of oxygen by organic processes is, however,
little more than a reversal of the previous process by which it was set free;
for instance, green plants in forming their food set free the oxygen of the
carbon dioxide used for the purpose. When the organic substance so formed
is ultimately consumed through plant or animal action or by inorganic
means, an equivalent amount of oxygen reunites with the carbon to again
Page 729
form carbon dioxide. And so if the whole of the organic matter is returned
to the inorganic state, no more oxygen is consumed than had been before set
free in the process of forming the organic matter. But, as a matter of fact, a
large amount of organic matter has not gone back completely to the
inorganic state, and this residue constitutes a factor of no small importance
in the geological record.
The organic residue.—There is a certain portion of vegetation that is not
consumed by animals or by other plants, and that escapes combustion and
all kinds of ordinary decay, and this constitutes a part of the organic residue.
Animals never completely oxidize all the organic matter they take into their
systems; their bodies never entirely consume themselves. A like statement
may be made respecting those plants that feed on organic matter. That
which animals and plants leave unoxidized is indeed more or less preyed
upon by other animals and plants, and relatively little escapes final
reoxidation, but there is a remnant, and this constitutes another part of the
organic residue. The more conspicuous forms of the organic residue are
found in the mucks, peats, lignites, coals, organic oils, and gases, but in
addition there is not a little disseminated organic matter in nearly all the
sedimentary rocks; in the aggregate, this probably amounts to more than the
distinct organic deposits.
The meaning of the organic residue.—All the unoxidized, or
incompletely oxidized, carbon in the organic residue implies that oxygen
has previously been separated from this residual carbon by plants and given
to the atmosphere, and hence has been a source of atmospheric enrichment
in oxygen. The amount thus contributed is equal to that which is required to
restore the residual carbon to its original state of oxidation. So, in a similar
way, the unoxidized hydrogen in the organic hydrocarbons and like
compounds implies that oxygen has been separated from the hydrogen of
water and given to the atmosphere, and hence this also is a source of
atmospheric enrichment in oxygen. It seems safe, therefore, to conclude that
the action of life, taken as a whole, has increased the free oxygen of the
atmosphere.
While not here under consideration, it is not to be forgotten that inorganic
processes involving the same atmospheric constituents have been in
operation concurrently with the organic processes, and that they have also
affected the amounts and proportions of the atmospheric constituents.
to the inorganic state, no more oxygen is consumed than had been before set
free in the process of forming the organic matter. But, as a matter of fact, a
large amount of organic matter has not gone back completely to the
inorganic state, and this residue constitutes a factor of no small importance
in the geological record.
The organic residue.—There is a certain portion of vegetation that is not
consumed by animals or by other plants, and that escapes combustion and
all kinds of ordinary decay, and this constitutes a part of the organic residue.
Animals never completely oxidize all the organic matter they take into their
systems; their bodies never entirely consume themselves. A like statement
may be made respecting those plants that feed on organic matter. That
which animals and plants leave unoxidized is indeed more or less preyed
upon by other animals and plants, and relatively little escapes final
reoxidation, but there is a remnant, and this constitutes another part of the
organic residue. The more conspicuous forms of the organic residue are
found in the mucks, peats, lignites, coals, organic oils, and gases, but in
addition there is not a little disseminated organic matter in nearly all the
sedimentary rocks; in the aggregate, this probably amounts to more than the
distinct organic deposits.
The meaning of the organic residue.—All the unoxidized, or
incompletely oxidized, carbon in the organic residue implies that oxygen
has previously been separated from this residual carbon by plants and given
to the atmosphere, and hence has been a source of atmospheric enrichment
in oxygen. The amount thus contributed is equal to that which is required to
restore the residual carbon to its original state of oxidation. So, in a similar
way, the unoxidized hydrogen in the organic hydrocarbons and like
compounds implies that oxygen has been separated from the hydrogen of
water and given to the atmosphere, and hence this also is a source of
atmospheric enrichment in oxygen. It seems safe, therefore, to conclude that
the action of life, taken as a whole, has increased the free oxygen of the
atmosphere.
While not here under consideration, it is not to be forgotten that inorganic
processes involving the same atmospheric constituents have been in
operation concurrently with the organic processes, and that they have also
affected the amounts and proportions of the atmospheric constituents.
Page 730
Rocks have been oxidized in greater or less measure at the expense of the
atmospheric oxygen, and hence when the total atmospheric problem is
considered, there arises the question whether the amount of oxygen in the
atmosphere has been increased or diminished during geological history,
when the balance is struck between the inorganic and the organic actions.
The probabilities seem to us to strongly favor the view that organic action
has preponderated, and that the oxygen has been increased beyond its
primitive amount, but that it has fluctuated during known geological
history. The reasons for this view will appear in the historical chapters.
The disintegration of the crystalline rocks and the solution of limestone
have consumed much carbon dioxide, and this is to be added to the loss
through organic action. On the other hand, there are inorganic processes
that supply carbon dioxide, and hence when the larger problem of the
atmosphere is raised, the factors become so complicated that their
consideration is best deferred to the historical chapters. This passing
reference may stand us in good part lest we forget, for the moment, the
inorganic factors in the atmospheric problem.
The more inert factor.—Nitrogen in the free state is relatively inert
chemically, and it does not appear that it can be used directly by the higher
plants and animals in appreciable amounts. Certain bacteria, and perhaps
certain algæ[288] and other low forms of plants, have the power of using free
nitrogen, and this is a principal way in which it is put within the reach of
higher plants. Nitrogen is also combined in small quantity in the
atmosphere by electric action, and thus made available for plants. On
account of the inertness of nitrogen and of the relatively limited amount
required for organic purposes, the nitrogen of the atmosphere has been less
consumed than the carbon dioxide. Besides this, the nitrogen compounds
are very decomposable, and are very generally and completely returned to
their original state. Deposits of nitrates or other nitrogenous compounds are
relatively rare.
It is obvious that if there is any considerable source of supply concurrent
with this slight loss, the amount of nitrogen in the atmosphere must have
been increasing. We have seen that volcanoes give forth considerable
quantities of nitrogen, and that this may be a real addition to the
atmosphere, and not merely a return of the atmospheric nitrogen that had
been carried down previously by underground-water. It has also been noted
atmospheric oxygen, and hence when the total atmospheric problem is
considered, there arises the question whether the amount of oxygen in the
atmosphere has been increased or diminished during geological history,
when the balance is struck between the inorganic and the organic actions.
The probabilities seem to us to strongly favor the view that organic action
has preponderated, and that the oxygen has been increased beyond its
primitive amount, but that it has fluctuated during known geological
history. The reasons for this view will appear in the historical chapters.
The disintegration of the crystalline rocks and the solution of limestone
have consumed much carbon dioxide, and this is to be added to the loss
through organic action. On the other hand, there are inorganic processes
that supply carbon dioxide, and hence when the larger problem of the
atmosphere is raised, the factors become so complicated that their
consideration is best deferred to the historical chapters. This passing
reference may stand us in good part lest we forget, for the moment, the
inorganic factors in the atmospheric problem.
The more inert factor.—Nitrogen in the free state is relatively inert
chemically, and it does not appear that it can be used directly by the higher
plants and animals in appreciable amounts. Certain bacteria, and perhaps
certain algæ[288] and other low forms of plants, have the power of using free
nitrogen, and this is a principal way in which it is put within the reach of
higher plants. Nitrogen is also combined in small quantity in the
atmosphere by electric action, and thus made available for plants. On
account of the inertness of nitrogen and of the relatively limited amount
required for organic purposes, the nitrogen of the atmosphere has been less
consumed than the carbon dioxide. Besides this, the nitrogen compounds
are very decomposable, and are very generally and completely returned to
their original state. Deposits of nitrates or other nitrogenous compounds are
relatively rare.
It is obvious that if there is any considerable source of supply concurrent
with this slight loss, the amount of nitrogen in the atmosphere must have
been increasing. We have seen that volcanoes give forth considerable
quantities of nitrogen, and that this may be a real addition to the
atmosphere, and not merely a return of the atmospheric nitrogen that had
been carried down previously by underground-water. It has also been noted
Page 731
that crystalline rocks contain occluded nitrogen, which is doubtless freed by
their disintegration. It is, therefore, not improbable that the nitrogen of the
atmosphere has been increasing, both actually and relatively.
Probable fluctuations of atmospheric composition.—With this general
sketch of the interplay of the atmospheric elements under organic influence,
we are prepared for the further conception that if one or another of these
actions was relatively more vigorous than usual for a period, it would bring
about a variation in the proportions of the atmospheric constituents. If, for
example, vegetation flourished luxuriantly for a long period, but was
measurably protected from the organisms that preyed upon it and from
inorganic decomposition, as by falling into water or by prompt burial under
sediment, the atmosphere might be growing richer in oxygen. If, on the
other hand, vegetation were being relatively reduced, as perhaps it is being
reduced now by man, and if previous organic products were being
reoxidized at an unusual rate, as they are now in the burning of timber, coal,
natural oil and gas, the carbon dioxide of the atmosphere might be relatively
increasing, while the oxygen might be relatively diminishing. The possible
fluctuations of the atmosphere as the result of organic action are, therefore,
matters of vital importance, and invite attention in the historical study of the
earth and in the outlook into its future.
The climatic effects of organic action.—Interest does not, however, rest
at this point. The researches of physicists have made it probable, if they
have not altogether demonstrated, that the composition of the atmosphere
has much to do with the climatic conditions at the surface of the earth. The
atmosphere blankets the earth and equalizes its temperature. Acting as a
screen, it subdues in some measure the intensity of the sun’s rays by day,
while it retards the radiation of the earth’s acquired heat at night. This is in
some measure the function of all the constituents of the atmosphere, but by
no means of all equally. The oxygen and nitrogen are relatively
diathermous, letting the sun’s rays pass in freely, and the earth’s rays pass
out freely; but carbon dioxide and the vapor of water are much less
diathermous, particularly to rays of low intensity, such as are thrown out by
non-luminous bodies like the earth. It follows that while the solar rays come
in rather freely and heat the surface of the earth, the dark rays which the
earth radiates back are measurably arrested by the carbon dioxide and vapor
of water, and serve to keep the air warm. The influence of the vapor of
their disintegration. It is, therefore, not improbable that the nitrogen of the
atmosphere has been increasing, both actually and relatively.
Probable fluctuations of atmospheric composition.—With this general
sketch of the interplay of the atmospheric elements under organic influence,
we are prepared for the further conception that if one or another of these
actions was relatively more vigorous than usual for a period, it would bring
about a variation in the proportions of the atmospheric constituents. If, for
example, vegetation flourished luxuriantly for a long period, but was
measurably protected from the organisms that preyed upon it and from
inorganic decomposition, as by falling into water or by prompt burial under
sediment, the atmosphere might be growing richer in oxygen. If, on the
other hand, vegetation were being relatively reduced, as perhaps it is being
reduced now by man, and if previous organic products were being
reoxidized at an unusual rate, as they are now in the burning of timber, coal,
natural oil and gas, the carbon dioxide of the atmosphere might be relatively
increasing, while the oxygen might be relatively diminishing. The possible
fluctuations of the atmosphere as the result of organic action are, therefore,
matters of vital importance, and invite attention in the historical study of the
earth and in the outlook into its future.
The climatic effects of organic action.—Interest does not, however, rest
at this point. The researches of physicists have made it probable, if they
have not altogether demonstrated, that the composition of the atmosphere
has much to do with the climatic conditions at the surface of the earth. The
atmosphere blankets the earth and equalizes its temperature. Acting as a
screen, it subdues in some measure the intensity of the sun’s rays by day,
while it retards the radiation of the earth’s acquired heat at night. This is in
some measure the function of all the constituents of the atmosphere, but by
no means of all equally. The oxygen and nitrogen are relatively
diathermous, letting the sun’s rays pass in freely, and the earth’s rays pass
out freely; but carbon dioxide and the vapor of water are much less
diathermous, particularly to rays of low intensity, such as are thrown out by
non-luminous bodies like the earth. It follows that while the solar rays come
in rather freely and heat the surface of the earth, the dark rays which the
earth radiates back are measurably arrested by the carbon dioxide and vapor
of water, and serve to keep the air warm. The influence of the vapor of
Page 732
water is vividly shown in the different degrees to which cooling takes place
at night in a dry and in a moist atmosphere, respectively, where other
conditions are the same. Ice is said to form at night in desert regions where
the air is extremely dry, even within the tropics, while in humid regions of
the same latitude and altitude oppressively hot nights are common. The
influence of the carbon dioxide is not thus familiarly demonstrated, since its
amount varies but slightly in different localities, but physical experiment
indicates that it has a similar function.
If the amount of carbon dioxide in the atmosphere varies from age to age,
the climate of the earth must apparently vary accordingly, and on this is
built one of the hypotheses of climatic variation subsequently to be
considered. We shall find that there have been great changes in the climate
of the earth during its history. There is good evidence of former glaciation,
not only in the northern United States and in England, Germany, and central
Russia, but in India, Australia, and South Africa. At other times, figs and
magnolias grew in Greenland and Spitzbergen, and corals flourished in the
Arctic seas. There is good evidence of arid periods where humidity now
prevails, and of humid periods where aridity now prevails. It is not assumed
that the influence of organic action on the atmosphere has been the sole, or
perhaps even the main, cause of these great climatic changes, but it is
believed that it has been an important contributing factor. It is even possible
that the climate of the future is much dependent on the agency of man, as
implied above, however little ground there may be to suppose that he will,
with altruistic purpose, control his action with a view to its bearing on the
generations that may live tens of thousands of years hence.
(2) Aid and hindrance to inorganic action.
The promotion of disintegration.—While the influence of organic
action on the lithosphere is quite superficial, and far less radical than that on
the atmosphere, it is still important. Plants promote both disintegration and
disaggregation under certain conditions, and hinder them under others, as
already set forth. Chemical action of a decomposing and solvent nature
takes place in connection with the roots of plants, while their growth
sometimes rends rocks into whose crevices they have insinuated
themselves. The acids and other products of organic growth and of organic
at night in a dry and in a moist atmosphere, respectively, where other
conditions are the same. Ice is said to form at night in desert regions where
the air is extremely dry, even within the tropics, while in humid regions of
the same latitude and altitude oppressively hot nights are common. The
influence of the carbon dioxide is not thus familiarly demonstrated, since its
amount varies but slightly in different localities, but physical experiment
indicates that it has a similar function.
If the amount of carbon dioxide in the atmosphere varies from age to age,
the climate of the earth must apparently vary accordingly, and on this is
built one of the hypotheses of climatic variation subsequently to be
considered. We shall find that there have been great changes in the climate
of the earth during its history. There is good evidence of former glaciation,
not only in the northern United States and in England, Germany, and central
Russia, but in India, Australia, and South Africa. At other times, figs and
magnolias grew in Greenland and Spitzbergen, and corals flourished in the
Arctic seas. There is good evidence of arid periods where humidity now
prevails, and of humid periods where aridity now prevails. It is not assumed
that the influence of organic action on the atmosphere has been the sole, or
perhaps even the main, cause of these great climatic changes, but it is
believed that it has been an important contributing factor. It is even possible
that the climate of the future is much dependent on the agency of man, as
implied above, however little ground there may be to suppose that he will,
with altruistic purpose, control his action with a view to its bearing on the
generations that may live tens of thousands of years hence.
(2) Aid and hindrance to inorganic action.
The promotion of disintegration.—While the influence of organic
action on the lithosphere is quite superficial, and far less radical than that on
the atmosphere, it is still important. Plants promote both disintegration and
disaggregation under certain conditions, and hinder them under others, as
already set forth. Chemical action of a decomposing and solvent nature
takes place in connection with the roots of plants, while their growth
sometimes rends rocks into whose crevices they have insinuated
themselves. The acids and other products of organic growth and of organic
Page 733
decomposition attack some of the constituents of the rocks and contribute to
their solution and disintegration. On the other hand, organic matter
entrapped in the sediments, and so introduced into the strata at various
depths, often acts as a reducing agency, causing the deposit of substances
carried in solution in the underground-waters. Ores are sometimes thus
formed, as explained in the discussion of ore-deposits (p. 476). Organic
action on the whole promotes solution and disintegration at the surface, and
prepares the way for deposition below.
Protection against erosion.—Another important function of vegetation
is the protection of the land surface against erosion, as already noted in the
discussion of erosion. A mantle of grass, especially if it forms a turf, or a
carpet of leaves protected by bush and forest, greatly retards surface wash.
It does this not only because it directly covers the soil, but because it holds
back the run-off and tends to prevent those violent floods which give to
erosion its greatest intensity. There is a marked difference between the
erosive work which a given amount of water will do if, in the one case, it
runs off gradually, and in the other, precipitately. By way of offset, it is to
be noted that the disintegrating action of vegetation prepares the rock
material for easy erosion, and to this extent helps in its removal by the
drainage; but on the average this is greatly overbalanced by the protection
afforded by the vegetal covering, though this is not true in every instance.
The influence of land vegetation on the character of the sediments.—
The presence or absence of a vegetal covering influences the kind of
deposit which is derived from the land, particularly if the surface be
occupied by crystalline rocks. If the surface be well clothed with vegetation,
the crystals of the complex silicates, such as the feldspars, micas, and
ferromagnesian minerals, are usually disintegrated into clayey products
before they are removed, so that, when borne away and deposited, the result
is common shale. Concurrently, the relatively undecomposable quartz-
grains are rounded into sand, and deposited as common quartzose
sandstone, while the calcareous material is borne away in solution and
deposited as limestone. But if the surface be bare of vegetation, the
crystalline rocks are usually disaggregated before they are decomposed, for
destructive action works best at the junctions of crystals, and along
cleavage lines, and hence the crystals are usually separated from one
another before they are fully decomposed. In the absence of a covering to
their solution and disintegration. On the other hand, organic matter
entrapped in the sediments, and so introduced into the strata at various
depths, often acts as a reducing agency, causing the deposit of substances
carried in solution in the underground-waters. Ores are sometimes thus
formed, as explained in the discussion of ore-deposits (p. 476). Organic
action on the whole promotes solution and disintegration at the surface, and
prepares the way for deposition below.
Protection against erosion.—Another important function of vegetation
is the protection of the land surface against erosion, as already noted in the
discussion of erosion. A mantle of grass, especially if it forms a turf, or a
carpet of leaves protected by bush and forest, greatly retards surface wash.
It does this not only because it directly covers the soil, but because it holds
back the run-off and tends to prevent those violent floods which give to
erosion its greatest intensity. There is a marked difference between the
erosive work which a given amount of water will do if, in the one case, it
runs off gradually, and in the other, precipitately. By way of offset, it is to
be noted that the disintegrating action of vegetation prepares the rock
material for easy erosion, and to this extent helps in its removal by the
drainage; but on the average this is greatly overbalanced by the protection
afforded by the vegetal covering, though this is not true in every instance.
The influence of land vegetation on the character of the sediments.—
The presence or absence of a vegetal covering influences the kind of
deposit which is derived from the land, particularly if the surface be
occupied by crystalline rocks. If the surface be well clothed with vegetation,
the crystals of the complex silicates, such as the feldspars, micas, and
ferromagnesian minerals, are usually disintegrated into clayey products
before they are removed, so that, when borne away and deposited, the result
is common shale. Concurrently, the relatively undecomposable quartz-
grains are rounded into sand, and deposited as common quartzose
sandstone, while the calcareous material is borne away in solution and
deposited as limestone. But if the surface be bare of vegetation, the
crystalline rocks are usually disaggregated before they are decomposed, for
destructive action works best at the junctions of crystals, and along
cleavage lines, and hence the crystals are usually separated from one
another before they are fully decomposed. In the absence of a covering to
Page 734
hold them in place until they are decomposed, they are apt to be washed
away, and the resulting deposit consists in considerable part of grains of
feldspar, mica, hornblende, and other minerals, which do not usually occur
in well-decomposed sediments. The deposits are, therefore, of the nature of
arkose, if the original rocks are granitic, or of the nature of wacke, as the
term is used in this book, if they are of the basic type. On this is based the
inference that a vegetal covering of the land extended as far back in the
history of the earth as clay shales, quartzose sandstones, and limestones
form the prevailing sediments.
(3) Distinctive deposits.
Organic rocks.—In the chapter on the origin and descent of rocks, a
group of rocks formed directly from organic matter is recognized and
described. The chief of these are peat, lignite, bituminous coal, anthracite,
and graphite. It is the belief of many geologists that natural gases, oils, and
asphalts are also mainly derived from animal and vegetal remains. An
alternative view, advocated by Mendelejeff and Moissan, assigns the oils,
gases, etc., in part at least, to deep-seated carbides to which water has
gained access and developed hydrocarbons, after the analogy of acetylene.
[289]
Whatever may be the truth relative to inorganic action, it is clear from
geological conditions that some of the natural gases and oils are organic
products. Besides the more common organic deposits, there is a long list of
minor products, among which are amber, copalite, paraffine, ozocerite,
camphene, etc. Guano and coprolites represent the excrementitious class.
Inorganic rocks due to life.—Besides these deposits of organic matter,
or of its decomposition products, there is a large class formed from the
inorganic matter that served auxiliary functions in the economy of life, such
as shells, skeletons, etc. For the greater part these are composed of calcium
carbonate, and give rise to limestones, marls, chalk, etc. Not a few,
however, are silicious, and give rise to flints, cherts, and silicious earths.
Some are formed of calcium phosphate, and a few of other inorganic
material. The deposits formed in these ways have been defined in the
chapter on rocks.
away, and the resulting deposit consists in considerable part of grains of
feldspar, mica, hornblende, and other minerals, which do not usually occur
in well-decomposed sediments. The deposits are, therefore, of the nature of
arkose, if the original rocks are granitic, or of the nature of wacke, as the
term is used in this book, if they are of the basic type. On this is based the
inference that a vegetal covering of the land extended as far back in the
history of the earth as clay shales, quartzose sandstones, and limestones
form the prevailing sediments.
(3) Distinctive deposits.
Organic rocks.—In the chapter on the origin and descent of rocks, a
group of rocks formed directly from organic matter is recognized and
described. The chief of these are peat, lignite, bituminous coal, anthracite,
and graphite. It is the belief of many geologists that natural gases, oils, and
asphalts are also mainly derived from animal and vegetal remains. An
alternative view, advocated by Mendelejeff and Moissan, assigns the oils,
gases, etc., in part at least, to deep-seated carbides to which water has
gained access and developed hydrocarbons, after the analogy of acetylene.
[289]
Whatever may be the truth relative to inorganic action, it is clear from
geological conditions that some of the natural gases and oils are organic
products. Besides the more common organic deposits, there is a long list of
minor products, among which are amber, copalite, paraffine, ozocerite,
camphene, etc. Guano and coprolites represent the excrementitious class.
Inorganic rocks due to life.—Besides these deposits of organic matter,
or of its decomposition products, there is a large class formed from the
inorganic matter that served auxiliary functions in the economy of life, such
as shells, skeletons, etc. For the greater part these are composed of calcium
carbonate, and give rise to limestones, marls, chalk, etc. Not a few,
however, are silicious, and give rise to flints, cherts, and silicious earths.
Some are formed of calcium phosphate, and a few of other inorganic
material. The deposits formed in these ways have been defined in the
chapter on rocks.
Page 735
Fossils.
The term fossil is used so comprehensively as to include not only the
remains of plants and animals themselves, but their tracks, impressions,
casts, replacements, and all other distinct traces. It also embraces nests,
borings, implements, and other distinctive products. These enter into the
formation of the two classes of rocks just considered, but they have an
independent function. They constitute the specific record of life, and their
study not only reveals much of the past history of plants and animals, but
furnishes one of the most important means by which the ages of formations
are determined. In the early development of the science it was found that
the uppermost and hence the latest beds of rock contain fossil forms either
identical with those now living, or closely similar to them; that beds below
these bear life relics that depart somewhat more from the living forms, and
are somewhat less highly developed; that beds still lower bear fossils that
depart still more from the living types, and are more primitive in general,
and so on down as far as fossils are found.
The general order of life succession determined by stratigraphy.—
Thus it appeared from the evidence of the strata that there was a general
order of life succession. It was also found that this was, in its main features,
the same for all the continents. By continued and close studies, the
particulars of the succession were worked out more and more fully, and the
work is still being pushed forward to greater and greater degrees of
refinement. At the same time, it was found that there were different faunas
and floras in different parts of the world in past times, much as there are
now; that there were shiftings and migrations as now; that given species
were increasing in some regions and dying out in others, and that
innumerable variations and complications entered into the evolution and
distribution of the life forms. But under and through all these there run a
sufficient number of common features to show beyond reasonable question
the order of succession of life.
Throughout all this study, the chief guide was the actual order in which
the fossils were found in the succession of strata, because there is no
evidence so conclusive of the order of events as the superposition of the
sedimentary beds when they are normal and undisturbed. By the study of
the fossils in the successive beds, it was found that there was a more or less
progressive evolution of plants and animals brought about by modifications
The term fossil is used so comprehensively as to include not only the
remains of plants and animals themselves, but their tracks, impressions,
casts, replacements, and all other distinct traces. It also embraces nests,
borings, implements, and other distinctive products. These enter into the
formation of the two classes of rocks just considered, but they have an
independent function. They constitute the specific record of life, and their
study not only reveals much of the past history of plants and animals, but
furnishes one of the most important means by which the ages of formations
are determined. In the early development of the science it was found that
the uppermost and hence the latest beds of rock contain fossil forms either
identical with those now living, or closely similar to them; that beds below
these bear life relics that depart somewhat more from the living forms, and
are somewhat less highly developed; that beds still lower bear fossils that
depart still more from the living types, and are more primitive in general,
and so on down as far as fossils are found.
The general order of life succession determined by stratigraphy.—
Thus it appeared from the evidence of the strata that there was a general
order of life succession. It was also found that this was, in its main features,
the same for all the continents. By continued and close studies, the
particulars of the succession were worked out more and more fully, and the
work is still being pushed forward to greater and greater degrees of
refinement. At the same time, it was found that there were different faunas
and floras in different parts of the world in past times, much as there are
now; that there were shiftings and migrations as now; that given species
were increasing in some regions and dying out in others, and that
innumerable variations and complications entered into the evolution and
distribution of the life forms. But under and through all these there run a
sufficient number of common features to show beyond reasonable question
the order of succession of life.
Throughout all this study, the chief guide was the actual order in which
the fossils were found in the succession of strata, because there is no
evidence so conclusive of the order of events as the superposition of the
sedimentary beds when they are normal and undisturbed. By the study of
the fossils in the successive beds, it was found that there was a more or less
progressive evolution of plants and animals brought about by modifications
Page 736
of their forms, and that these modifications assisted in determining the
order of succession when the evidence of the strata was defective; and so
the biological and stratigraphical factors reacted helpfully on each other.
Fossils as means of correlation.—While stratigraphy was thus, in the
earliest stages, the main reliance in determining the order of events, and
biology was the chief gainer, in the end stratigraphy received ample
compensation, if indeed it did not become the greater beneficiary; for at no
known and accessible place is there a complete succession of sedimentary
beds. There are great series here and there, but their connections with one
another are more or less concealed by surface formations or water-bodies.
So also at many places the stratified series has been broken up by
deformation, or cut away by erosion. Hence there was need for some
reliable means of matching the beds of separated series, and of making up a
complete ideal series. This means is found in the fossils they contain. While
the variations of the faunas and floras in different regions, and their
migrations, introduce some minor difficulties, the relations of the
fossiliferous beds of one region to those of another can be determined with
great satisfaction, and often with great precision. This is particularly so
when abundant floating or free-swimming species lived in the seas and
were freely fossilized, for they were deposited on the coasts of all the
continents at practically the same time, and no uncertainties from migration
or local differences in rate of evolution intervened to throw doubt upon the
correlation. Without the aid of fossils, the correlation of the deposits on the
separate continents would be attended with grave obstacles and much
uncertainty, if not with quite prohibitive difficulties.
B. Special Modes of Aggregation and of Movement.
Inorganic solid matter is chiefly crystalloidal; organic matter is chiefly
colloidal; but there are colloidal states of inorganic matter and there are
crystalloids among the organic products. In the inorganic world, solids very
generally tend to organize in the form of crystals; in the organic world, they
as generally tend to organize in the form of cells. Neither tendency is
complete or exclusive, but each is dominant in its own sphere.
Still more distinctive than the formation of cells is the growth of complex
organized bodies, the differentiated members of which perform special
order of succession when the evidence of the strata was defective; and so
the biological and stratigraphical factors reacted helpfully on each other.
Fossils as means of correlation.—While stratigraphy was thus, in the
earliest stages, the main reliance in determining the order of events, and
biology was the chief gainer, in the end stratigraphy received ample
compensation, if indeed it did not become the greater beneficiary; for at no
known and accessible place is there a complete succession of sedimentary
beds. There are great series here and there, but their connections with one
another are more or less concealed by surface formations or water-bodies.
So also at many places the stratified series has been broken up by
deformation, or cut away by erosion. Hence there was need for some
reliable means of matching the beds of separated series, and of making up a
complete ideal series. This means is found in the fossils they contain. While
the variations of the faunas and floras in different regions, and their
migrations, introduce some minor difficulties, the relations of the
fossiliferous beds of one region to those of another can be determined with
great satisfaction, and often with great precision. This is particularly so
when abundant floating or free-swimming species lived in the seas and
were freely fossilized, for they were deposited on the coasts of all the
continents at practically the same time, and no uncertainties from migration
or local differences in rate of evolution intervened to throw doubt upon the
correlation. Without the aid of fossils, the correlation of the deposits on the
separate continents would be attended with grave obstacles and much
uncertainty, if not with quite prohibitive difficulties.
B. Special Modes of Aggregation and of Movement.
Inorganic solid matter is chiefly crystalloidal; organic matter is chiefly
colloidal; but there are colloidal states of inorganic matter and there are
crystalloids among the organic products. In the inorganic world, solids very
generally tend to organize in the form of crystals; in the organic world, they
as generally tend to organize in the form of cells. Neither tendency is
complete or exclusive, but each is dominant in its own sphere.
Still more distinctive than the formation of cells is the growth of complex
organized bodies, the differentiated members of which perform special
Page 737
functions for one another, and are mutually dependent on one another. This
is a profound departure from the habitual modes of the inorganic world.
Still more so is the power of voluntary motion in more or less disregard
of outside physical influences. Through this power, distribution may take
place contrary to current and wind, and to gravitation itself. From the view-
point of past geologic transportation, this is perhaps more singular than
important, for no great mass of matter has been transported contrary to the
influences of gravity, wind, and current, by the exercise of this peculiar
power of animals, but it is not without geologic importance in the
migrations and in the redistributions of organic influences that arise from
migrations. When the influence of man is included, the geologic effects
require consideration, but here the third distinctive factor, the mental
element, comes into effective play, and we pass to its consideration.
C. The Mental Element.
Current opinion does not recognize a mental element as residing in the
plant world, and it is divided as to the degree of its development in the
lower animal kingdom, but its influential presence in the higher animal
orders and in man is beyond legitimate question. Two phases are to be
recognized: (1) the material work done under the stimulus and direction of
mental impulses, as, for example, excavations, transportations, changes of
drainage, removal of forests, cultivation of soil, etc., and (2) the intellectual
work of the faculties themselves irrespective of material changes. In one
view, geology is a purely material science concerned solely with the
formation of the earth and with the physical development and relations of
its inhabitants. In another, geology is a comprehensive historical science
concerned with every phase of the world’s history, and certainly not least
with the higher forms of life development, with their psychological,
sociological, and other phases of mental attainments, since these are the
highest output of the earth’s evolution. The latter seems to us the more
comprehensive view.
(1) The material effects of the mental element.—Lyell long since urged
that the direct work of man in changing the face of the earth was slight
compared with that of the contemporaneous inorganic agencies. He called
attention to the relative insignificance of the quarries, pits, cellars, and other
is a profound departure from the habitual modes of the inorganic world.
Still more so is the power of voluntary motion in more or less disregard
of outside physical influences. Through this power, distribution may take
place contrary to current and wind, and to gravitation itself. From the view-
point of past geologic transportation, this is perhaps more singular than
important, for no great mass of matter has been transported contrary to the
influences of gravity, wind, and current, by the exercise of this peculiar
power of animals, but it is not without geologic importance in the
migrations and in the redistributions of organic influences that arise from
migrations. When the influence of man is included, the geologic effects
require consideration, but here the third distinctive factor, the mental
element, comes into effective play, and we pass to its consideration.
C. The Mental Element.
Current opinion does not recognize a mental element as residing in the
plant world, and it is divided as to the degree of its development in the
lower animal kingdom, but its influential presence in the higher animal
orders and in man is beyond legitimate question. Two phases are to be
recognized: (1) the material work done under the stimulus and direction of
mental impulses, as, for example, excavations, transportations, changes of
drainage, removal of forests, cultivation of soil, etc., and (2) the intellectual
work of the faculties themselves irrespective of material changes. In one
view, geology is a purely material science concerned solely with the
formation of the earth and with the physical development and relations of
its inhabitants. In another, geology is a comprehensive historical science
concerned with every phase of the world’s history, and certainly not least
with the higher forms of life development, with their psychological,
sociological, and other phases of mental attainments, since these are the
highest output of the earth’s evolution. The latter seems to us the more
comprehensive view.
(1) The material effects of the mental element.—Lyell long since urged
that the direct work of man in changing the face of the earth was slight
compared with that of the contemporaneous inorganic agencies. He called
attention to the relative insignificance of the quarries, pits, cellars, and other
Page 738
excavations of man, compared with the work of streams, waves, and other
inorganic agencies. There is justness in this view, but it needs qualification.
It is to be observed that the mental era has but just begun, and that its
effects are increasing with a rapidity quite phenomenal when measured by
the slow pace of most geologic events. The excavations and transportations
of material to-day show an enormous advance on those of Lyell’s day,
which was, geologically speaking, but a moment ago. The mile-tons of
industrial freightage in the Mississippi basin are to-day not wholly
incomparable with the drainage transportation of the same area a century
ago. A century ago is named, because the surface was then covered with
natural vegetation, and the normal effect of surface erosion, independent of
man, was then experienced. At present the indirect effects of man’s action
are mingled with those of natural processes, and these indirect effects are
probably much more important than the direct ones. The removal of the
native vegetation and the cultivation of the soil expose the surface to wash
to a degree far beyond that prevalent when the surface was prairie sod, or
leaf-carpeted forest, and denudation and transportation have been greatly
multiplied in consequence. Not only has this cultivation increased the
exposure to erosion, but, by increasing the rate of run-off, it has added to
the erosive power of the streams. The ditching of swamps and other tracts
of retarded drainage has contributed to this acceleration. The naked, soil-
less uplands of some of the once populous kingdoms of the Orient, notably
portions of Syria and Greece, are sad witnesses of the accelerated erosion
that attends cultivation. The erosion of certain southern fields of the United
States in the last forty years is another striking illustration. It is doubtful
whether some parts of this region suffered as much erosion in the preceding
five centuries as they have during the last one. On the other hand, some
compensation is found in the reservoirs established for water-power, and in
artificial devices for retarding and steadying stream flow.
In the light of considerations such as these, man may well be regarded
not only as a potent geological agent, but as dangerously so to himself. The
hope is that the intelligence that has wrought a change of surface conditions
serviceable for the present, but dangerous to the future, will be so enlarged
as to inspire a still more intelligent control of surface conditions which shall
compass the future welfare as well as transient benefit.
inorganic agencies. There is justness in this view, but it needs qualification.
It is to be observed that the mental era has but just begun, and that its
effects are increasing with a rapidity quite phenomenal when measured by
the slow pace of most geologic events. The excavations and transportations
of material to-day show an enormous advance on those of Lyell’s day,
which was, geologically speaking, but a moment ago. The mile-tons of
industrial freightage in the Mississippi basin are to-day not wholly
incomparable with the drainage transportation of the same area a century
ago. A century ago is named, because the surface was then covered with
natural vegetation, and the normal effect of surface erosion, independent of
man, was then experienced. At present the indirect effects of man’s action
are mingled with those of natural processes, and these indirect effects are
probably much more important than the direct ones. The removal of the
native vegetation and the cultivation of the soil expose the surface to wash
to a degree far beyond that prevalent when the surface was prairie sod, or
leaf-carpeted forest, and denudation and transportation have been greatly
multiplied in consequence. Not only has this cultivation increased the
exposure to erosion, but, by increasing the rate of run-off, it has added to
the erosive power of the streams. The ditching of swamps and other tracts
of retarded drainage has contributed to this acceleration. The naked, soil-
less uplands of some of the once populous kingdoms of the Orient, notably
portions of Syria and Greece, are sad witnesses of the accelerated erosion
that attends cultivation. The erosion of certain southern fields of the United
States in the last forty years is another striking illustration. It is doubtful
whether some parts of this region suffered as much erosion in the preceding
five centuries as they have during the last one. On the other hand, some
compensation is found in the reservoirs established for water-power, and in
artificial devices for retarding and steadying stream flow.
In the light of considerations such as these, man may well be regarded
not only as a potent geological agent, but as dangerously so to himself. The
hope is that the intelligence that has wrought a change of surface conditions
serviceable for the present, but dangerous to the future, will be so enlarged
as to inspire a still more intelligent control of surface conditions which shall
compass the future welfare as well as transient benefit.
Page 739
Human modification of the animal and vegetal kingdoms.—Man’s
agency is also coming to be felt powerfully in the modification of the plant
and animal life of the land and even to some extent of the sea. The larger
animals that are not propagated by man are fast approaching extinction. At
the present rate of extension of man’s dominion, a century or so will see the
disappearance of nearly every large mammal and reptile that he does not
choose to protect or propagate. By way of compensation, certain selected
animals are increasing and will doubtless continue to increase. The result is,
therefore, likely to be a peculiar assemblage of animal life dependent
strictly on the choice of a dominant type, a state of things that has
apparently never occurred in an equal degree in the past history of the earth.
How far the minor forms of life, especially the insect life, and the denizens
of the sea, may be brought under this monopolistic control may not be
predicted so easily.
A similar profound transition in vegetation is being forced by man. The
native vegetation is rapidly being replaced by selected varieties, and by
varieties that take advantage of conditions furnished by man. As the
agricultural control of the earth becomes more complete and effective, a
result toward which very rapid progress is being made, a new flora of man’s
selection will very generally prevail over the whole land surface of the
globe. It is doubtful whether at any time in the history of the earth changes
of flora and of fauna, and of surface, have been more rapid than those that
are now taking place under the accelerating influence of man’s action, and
this accelerating influence springs not mainly from automatic or instinctive
reaction, but from conscious impulse and intelligent direction.
(2) The psychological factors as such.—Are the introduction and the
evolution of the psychological factors themselves to be regarded as subjects
of geological study? We shall find that, at the outset, the geologic record is
a complete blank so far as clear evidence of terrestrial organisms actuated
by their own intelligence is concerned; that later, organisms with some
apparent consciousness and intelligence appeared, and that the mental
element increased apace unto its present attainment. We know that
relationships of a sociological nature arose in apparent feebleness, and
gradually evolved into more definite, higher, and more complex forms. By
sociological factors we mean merely those conscious relations which one
organism bears to another, of which the parental and the gregarious
agency is also coming to be felt powerfully in the modification of the plant
and animal life of the land and even to some extent of the sea. The larger
animals that are not propagated by man are fast approaching extinction. At
the present rate of extension of man’s dominion, a century or so will see the
disappearance of nearly every large mammal and reptile that he does not
choose to protect or propagate. By way of compensation, certain selected
animals are increasing and will doubtless continue to increase. The result is,
therefore, likely to be a peculiar assemblage of animal life dependent
strictly on the choice of a dominant type, a state of things that has
apparently never occurred in an equal degree in the past history of the earth.
How far the minor forms of life, especially the insect life, and the denizens
of the sea, may be brought under this monopolistic control may not be
predicted so easily.
A similar profound transition in vegetation is being forced by man. The
native vegetation is rapidly being replaced by selected varieties, and by
varieties that take advantage of conditions furnished by man. As the
agricultural control of the earth becomes more complete and effective, a
result toward which very rapid progress is being made, a new flora of man’s
selection will very generally prevail over the whole land surface of the
globe. It is doubtful whether at any time in the history of the earth changes
of flora and of fauna, and of surface, have been more rapid than those that
are now taking place under the accelerating influence of man’s action, and
this accelerating influence springs not mainly from automatic or instinctive
reaction, but from conscious impulse and intelligent direction.
(2) The psychological factors as such.—Are the introduction and the
evolution of the psychological factors themselves to be regarded as subjects
of geological study? We shall find that, at the outset, the geologic record is
a complete blank so far as clear evidence of terrestrial organisms actuated
by their own intelligence is concerned; that later, organisms with some
apparent consciousness and intelligence appeared, and that the mental
element increased apace unto its present attainment. We know that
relationships of a sociological nature arose in apparent feebleness, and
gradually evolved into more definite, higher, and more complex forms. By
sociological factors we mean merely those conscious relations which one
organism bears to another, of which the parental and the gregarious
Page 740
impulses are two fundamental expressions. For manifest reasons, the
introduction and evolution of the psychological and sociological factors
themselves have received little direct recognition as a portion of geological
studies. The record of such factors in the fossils of past ages is necessarily
obscure and imperfect, and the interpretation of what there is lacks certainty
and precision. None the less, this psychological record, with all its
imperfections, is beyond valuation, and must, we think, come to be an
indispensable factor in the study of psychological and sociological
evolution, for it shows, what nothing else can show equally well, the
extremely prolonged history of that evolution, and it gives hints of modes
and means which no study of existing stages can equally reveal. The
organization of the Cambrian trilobites, for example, implies no small
development of the senses and of the coordinating faculties even at that
early stage, and a study of the relations of these to their fellow creatures
opens up the first known chapter in the sociological record of the earth’s
inhabitants. From this stage onward the progress in the development of the
higher faculties, and of the sociological relations of the leading forms, is
one of the most instructive phases of the great history. Such a study reveals
the fact that many questions, narrowly supposed to be purely human, have
had their prototypes in the earlier experiences of the animal kingdom. Some
of these questions have found solutions, temporary or permanent, which
passed under the test of ages to whose length human experience affords no
parallel, and have received the sanction or disapproval of such tests
according as they were well or ill adapted to the actual conditions involved.
If one seeks the lessons of history in the largest sense, he cannot wisely
neglect the prolonged record of the great biological family.
II. SPECIAL CONTRIBUTIONS OF THE ORGANIC
KINGDOMS.
An essential part of the historical chapters of the second volume will
consist of the description and illustration of the life progress of the
successive periods. It will suffice here to give a preliminary synopsis of the
kinds of record made by the several groups of plants and animals.
A. Contributions of the Plant Kingdom.[290]
introduction and evolution of the psychological and sociological factors
themselves have received little direct recognition as a portion of geological
studies. The record of such factors in the fossils of past ages is necessarily
obscure and imperfect, and the interpretation of what there is lacks certainty
and precision. None the less, this psychological record, with all its
imperfections, is beyond valuation, and must, we think, come to be an
indispensable factor in the study of psychological and sociological
evolution, for it shows, what nothing else can show equally well, the
extremely prolonged history of that evolution, and it gives hints of modes
and means which no study of existing stages can equally reveal. The
organization of the Cambrian trilobites, for example, implies no small
development of the senses and of the coordinating faculties even at that
early stage, and a study of the relations of these to their fellow creatures
opens up the first known chapter in the sociological record of the earth’s
inhabitants. From this stage onward the progress in the development of the
higher faculties, and of the sociological relations of the leading forms, is
one of the most instructive phases of the great history. Such a study reveals
the fact that many questions, narrowly supposed to be purely human, have
had their prototypes in the earlier experiences of the animal kingdom. Some
of these questions have found solutions, temporary or permanent, which
passed under the test of ages to whose length human experience affords no
parallel, and have received the sanction or disapproval of such tests
according as they were well or ill adapted to the actual conditions involved.
If one seeks the lessons of history in the largest sense, he cannot wisely
neglect the prolonged record of the great biological family.
II. SPECIAL CONTRIBUTIONS OF THE ORGANIC
KINGDOMS.
An essential part of the historical chapters of the second volume will
consist of the description and illustration of the life progress of the
successive periods. It will suffice here to give a preliminary synopsis of the
kinds of record made by the several groups of plants and animals.
A. Contributions of the Plant Kingdom.[290]
Page 741
The record of plants in the early geological ages is extremely imperfect.
In the very earliest times the conditions seem to have been wholly unsuited
to the preservation of any relics of life; but even after animal remains were
abundantly preserved in the sea sediments, the plant record was still very
meager for a long period. This was probably due in the main to two chief
causes: (1) the probable softness and perishability of the early types of
vegetation, and (2) the fact that vegetation is preponderantly terrestrial. At
no time has marine vegetation reached a high development. Land conditions
favor decomposition, transportation, and erosion, and through these,
destruction; and only under rather occasional and exceptional conditions did
the old lands leave a good record of their life. Nevertheless all the great
groups of plants, viz. the Thallophytes (algæ, fungi), the Bryophytes
(mosses, liverworts), the Pteridophytes (ferns, horsetails, lycopods), and the
Spermatophytes (gymnosperms, angiosperms) have left some record.
REFERENCE TABLE OF THE PRINCIPAL GROUPS OF PLANTS.
Cyanophyceæ, blue-green algæ.
Chlorophyceæ, green algæ.
Rhodophyceæ, red algæ.
Phæophyceæ, brown algæ.
Algæ and algoid forms
Diatomaceæ, diatoms.
Coccospheres
Pelagic algæ(?).
Rhabdospheres
Thallophytes
Charophyta, stoneworts.
(Thallus
plants) Phycomycetes, algæ-fungi, water-molds.
Ascomycetes, ascus-fungi, mildews.
Basidiomycetes, basidium-fungi,
Fungi and fungoid forms mushrooms.
Æcidiomycetes, æcidium-fungi, “rusts.”
Schizomycetes, “fission-fungi,” bacteria.
Myxomycetes, “animal fungi,” slime-molds.
Lichens Symbiont algæ and fungi.
Bryophytes Hepaticæ, liverworts.
(Moss plants) Musci, mosses.
Filices, true ferns.
Filicales
Cycadofilices, cycad-ferns.
Equisetæ, scouring-rushes, horsetails.
Equisetales
Pteridophytes Calamites.
(Fern plants) Sphenophyllales.
Lycopodiaceæ, club-mosses.
Lycopodiales Lepidodendra.
Sigillaria and stigmaria.
In the very earliest times the conditions seem to have been wholly unsuited
to the preservation of any relics of life; but even after animal remains were
abundantly preserved in the sea sediments, the plant record was still very
meager for a long period. This was probably due in the main to two chief
causes: (1) the probable softness and perishability of the early types of
vegetation, and (2) the fact that vegetation is preponderantly terrestrial. At
no time has marine vegetation reached a high development. Land conditions
favor decomposition, transportation, and erosion, and through these,
destruction; and only under rather occasional and exceptional conditions did
the old lands leave a good record of their life. Nevertheless all the great
groups of plants, viz. the Thallophytes (algæ, fungi), the Bryophytes
(mosses, liverworts), the Pteridophytes (ferns, horsetails, lycopods), and the
Spermatophytes (gymnosperms, angiosperms) have left some record.
REFERENCE TABLE OF THE PRINCIPAL GROUPS OF PLANTS.
Cyanophyceæ, blue-green algæ.
Chlorophyceæ, green algæ.
Rhodophyceæ, red algæ.
Phæophyceæ, brown algæ.
Algæ and algoid forms
Diatomaceæ, diatoms.
Coccospheres
Pelagic algæ(?).
Rhabdospheres
Thallophytes
Charophyta, stoneworts.
(Thallus
plants) Phycomycetes, algæ-fungi, water-molds.
Ascomycetes, ascus-fungi, mildews.
Basidiomycetes, basidium-fungi,
Fungi and fungoid forms mushrooms.
Æcidiomycetes, æcidium-fungi, “rusts.”
Schizomycetes, “fission-fungi,” bacteria.
Myxomycetes, “animal fungi,” slime-molds.
Lichens Symbiont algæ and fungi.
Bryophytes Hepaticæ, liverworts.
(Moss plants) Musci, mosses.
Filices, true ferns.
Filicales
Cycadofilices, cycad-ferns.
Equisetæ, scouring-rushes, horsetails.
Equisetales
Pteridophytes Calamites.
(Fern plants) Sphenophyllales.
Lycopodiaceæ, club-mosses.
Lycopodiales Lepidodendra.
Sigillaria and stigmaria.
Page 742
Cordaiteæ, cordaites.
Bennettiteæ.
Gymnospermæ Cycadales (cycads)
Cycadaceæ.
(Naked seed)
Coniferæ, evergreens.
Spermatophytes
(Seed plants) Ginkgoaceæ, ginkgo.
Monocotyledoneæ, cereals, grasses, etc.
Angiospermæ
(one-leafed seed).
(Covered Seed) (Flowering
plants) Dicotyledoneæ, oaks, poplars, peas, etc.
(two-leafed seed).
The contribution of the Thallophytes (algæ, fungi, bacteria).—The
Thallophytes embrace the simplest types of plants, and are probably the
nearest present representatives of the ancestral forms. Some of them are
minute one-celled organisms, as simple as an organism can well be
conceived to be. The simple blue-green algæ of our fresh waters well
represent this class. The most are, however, multicellular, and some (as the
great seaweeds) rise to a degree of complexity and of a bodily segmentation
resembling that of the higher plants. The various species are adapted to an
extremely wide range of conditions; some live in hot springs at 170° Fahr.,
and some in Arctic seas at the freezing-point; some flourish in fresh water,
some in brackish, some in salt water, and some even out of the water. This
wide adaptation implies an ancient and plastic type. The fact that they
flourish in waters so hot and sometimes also so sulphurous as to be fatal to
most plants, suggests the possibility of their introduction during the very
early volcanic stages of the earth, while conditions were yet uncongenial for
other plants.
The geologic work of the thermal algæ is well shown in the beautiful
travertine and sinter deposits of the Yellowstone Park (Figs. 215 and 218).
At the Mammoth Hot Springs the deposits are calcareous, while at most of
the other hot springs silicious deposits are formed, in both cases partly, but
not wholly, by the aid of algæ. The beautiful yellows, reds, browns, and
greens of these springs are not mineral coloring, but living plants.[291] In the
calcareous waters, the algæ are believed to cause the deposition of calcium
carbonate from calcium bicarbonate by consuming the second equivalent of
carbon dioxide that rendered the carbonate soluble.[292] In the silicious
waters, the process of deposition is not understood. Similar deposits by the
aid of algæ take place in the geyser regions of Iceland and of New Zealand,
in the hot springs of Carlsbad, where they have been well studied by Cohn,
[292]
and in most other hot springs. The same, or very similar, forms of algæ
Bennettiteæ.
Gymnospermæ Cycadales (cycads)
Cycadaceæ.
(Naked seed)
Coniferæ, evergreens.
Spermatophytes
(Seed plants) Ginkgoaceæ, ginkgo.
Monocotyledoneæ, cereals, grasses, etc.
Angiospermæ
(one-leafed seed).
(Covered Seed) (Flowering
plants) Dicotyledoneæ, oaks, poplars, peas, etc.
(two-leafed seed).
The contribution of the Thallophytes (algæ, fungi, bacteria).—The
Thallophytes embrace the simplest types of plants, and are probably the
nearest present representatives of the ancestral forms. Some of them are
minute one-celled organisms, as simple as an organism can well be
conceived to be. The simple blue-green algæ of our fresh waters well
represent this class. The most are, however, multicellular, and some (as the
great seaweeds) rise to a degree of complexity and of a bodily segmentation
resembling that of the higher plants. The various species are adapted to an
extremely wide range of conditions; some live in hot springs at 170° Fahr.,
and some in Arctic seas at the freezing-point; some flourish in fresh water,
some in brackish, some in salt water, and some even out of the water. This
wide adaptation implies an ancient and plastic type. The fact that they
flourish in waters so hot and sometimes also so sulphurous as to be fatal to
most plants, suggests the possibility of their introduction during the very
early volcanic stages of the earth, while conditions were yet uncongenial for
other plants.
The geologic work of the thermal algæ is well shown in the beautiful
travertine and sinter deposits of the Yellowstone Park (Figs. 215 and 218).
At the Mammoth Hot Springs the deposits are calcareous, while at most of
the other hot springs silicious deposits are formed, in both cases partly, but
not wholly, by the aid of algæ. The beautiful yellows, reds, browns, and
greens of these springs are not mineral coloring, but living plants.[291] In the
calcareous waters, the algæ are believed to cause the deposition of calcium
carbonate from calcium bicarbonate by consuming the second equivalent of
carbon dioxide that rendered the carbonate soluble.[292] In the silicious
waters, the process of deposition is not understood. Similar deposits by the
aid of algæ take place in the geyser regions of Iceland and of New Zealand,
in the hot springs of Carlsbad, where they have been well studied by Cohn,
[292]
and in most other hot springs. The same, or very similar, forms of algæ
Page 743
abound in nearly all waters, fresh and salt, but the question whether they
make calcareous and silicious deposits in notable quantity appears not to
have received as yet the critical investigation its importance deserves,
except in a few special cases. It is clear, however, that in the cool waters
such deposits do not reach the conspicuous amounts that they attain in the
thermal springs. In the shallow waters of the ocean, especially in the
warmer regions, lime-secreting algæ are abundant and make large
contributions to the lime deposits.
Among the higher algæ are the lime-secreting corallines or nullipores
(Rhodophyceæ, red algæ), once regarded as animals, which contribute a
notable part of the calcareous substance of coral reefs. They are important
geologic agents in the temperate and tropical seas, and have been traced as
far back in time as the early Paleozoic era.
The Challenger reports[293] describe two forms of minute calcareous
spherical organisms, Rhabdospheres and Coccospheres, as very abundant in
the surface-waters of the temperate and tropical seas, and as important in
contributing to the calcareous deposits of the sea-bottoms. The affinities of
these bodies are in doubt, but they are regarded by Murray as probably
pelagic algæ.
The stoneworts (Characeæ), an aberrant group of algæ inhabiting fresh
and brackish water, secrete notable quantities of calcium carbonate in and
around their tissues, and the accumulation of these gives rise to marl or
limestone. It has recently been urged that our so-called shell-marls are
mainly due to Charæ,[294] the molluscan shells being incidental rather than
essential constituents.
In very ancient and also in some of the later strata, there are limestones
that do not carry any visible fossils, and their origin is, therefore, debatable.
There are also not a few limestones that are made up of a fine-grained base
through which are scattered molluscan shells, corals, etc., in a fine state of
preservation. The condition of these fossils bears rather adversely on the
view that shells, etc., have been powdered in sufficient numbers and to a
sufficient degree to form the compact base. In all these cases the usual
explanations leave something to be desired. It is worth considering whether
low forms of plants may not be among the undemonstrated agents in
forming these apparently unfossiliferous limestones or parts of limestones.
make calcareous and silicious deposits in notable quantity appears not to
have received as yet the critical investigation its importance deserves,
except in a few special cases. It is clear, however, that in the cool waters
such deposits do not reach the conspicuous amounts that they attain in the
thermal springs. In the shallow waters of the ocean, especially in the
warmer regions, lime-secreting algæ are abundant and make large
contributions to the lime deposits.
Among the higher algæ are the lime-secreting corallines or nullipores
(Rhodophyceæ, red algæ), once regarded as animals, which contribute a
notable part of the calcareous substance of coral reefs. They are important
geologic agents in the temperate and tropical seas, and have been traced as
far back in time as the early Paleozoic era.
The Challenger reports[293] describe two forms of minute calcareous
spherical organisms, Rhabdospheres and Coccospheres, as very abundant in
the surface-waters of the temperate and tropical seas, and as important in
contributing to the calcareous deposits of the sea-bottoms. The affinities of
these bodies are in doubt, but they are regarded by Murray as probably
pelagic algæ.
The stoneworts (Characeæ), an aberrant group of algæ inhabiting fresh
and brackish water, secrete notable quantities of calcium carbonate in and
around their tissues, and the accumulation of these gives rise to marl or
limestone. It has recently been urged that our so-called shell-marls are
mainly due to Charæ,[294] the molluscan shells being incidental rather than
essential constituents.
In very ancient and also in some of the later strata, there are limestones
that do not carry any visible fossils, and their origin is, therefore, debatable.
There are also not a few limestones that are made up of a fine-grained base
through which are scattered molluscan shells, corals, etc., in a fine state of
preservation. The condition of these fossils bears rather adversely on the
view that shells, etc., have been powdered in sufficient numbers and to a
sufficient degree to form the compact base. In all these cases the usual
explanations leave something to be desired. It is worth considering whether
low forms of plants may not be among the undemonstrated agents in
forming these apparently unfossiliferous limestones or parts of limestones.
Page 744
The calcium carbonate deposited by the algæ is in minute and delicate form,
and is usually crystalline while yet in the living tissues. It is, therefore,
easily subject to comminution and to such further crystallization as would
obscure the minute features that constitute the evidences of algal origin.
The more complex and conspicuous algæ, the seaweeds, have left
impressions of their stems and fronds on the marine beds of most of the
periods, but they are usually obscure. Seaweeds are perhaps the source of
the vegetal matter in certain carbonaceous shales and limestones. As
seaweeds extract bromine and iodine and certain metallic ingredients from
the sea-water, some of the iodine and bromine springs issuing from ancient
marine deposits, and certain ores, may owe their origin to ancient seaweeds.
Diatoms, minute plants of the Thallophyte group, secrete a delicate
framework of silica which becomes a contribution to the silicious deposits.
Diatoms have sometimes contributed the material for very considerable
beds, such as those of the ooze-bogs now forming in the marshes of the
geyser basins of the Yellowstone Park,[295] and the diatom oozes of the deep
sea (Fig. 353, p. 425).
Fungi, for obvious reasons, have left but scant traces of themselves.
Bacteria are believed to be recognizable as far back as the Paleozoic era.
They are now the chief agents in the decomposition of organic matter, and
may be regarded as the prime enemies of the fossil record. It is probable
that similar decomposition took place actively in the earliest ages, for
otherwise the remains of the ancient organisms should be more abundant.
There is hence a theoretical probability that bacteria flourished as far back
as the stratigraphic record goes. Not unlikely they were originally simple
algæ that turned from the primitive habit of making their own food, to
living on other organisms or their remains, and in so doing lost their power
of manufacturing chlorophyll and of using inorganic carbon compounds.
Their remarkable adaptation to the most varied conditions, and their
extraordinary ability to endure the greatest vicissitudes of environment,
support the view that they are a very ancient and plastic form.
At present certain bacteria are important to higher vegetation because of
their ability to use the free nitrogen of the atmosphere and to combine it
into forms available for the higher plants. It is not improbable that they
have subserved this important function through all the known ages. Some
and is usually crystalline while yet in the living tissues. It is, therefore,
easily subject to comminution and to such further crystallization as would
obscure the minute features that constitute the evidences of algal origin.
The more complex and conspicuous algæ, the seaweeds, have left
impressions of their stems and fronds on the marine beds of most of the
periods, but they are usually obscure. Seaweeds are perhaps the source of
the vegetal matter in certain carbonaceous shales and limestones. As
seaweeds extract bromine and iodine and certain metallic ingredients from
the sea-water, some of the iodine and bromine springs issuing from ancient
marine deposits, and certain ores, may owe their origin to ancient seaweeds.
Diatoms, minute plants of the Thallophyte group, secrete a delicate
framework of silica which becomes a contribution to the silicious deposits.
Diatoms have sometimes contributed the material for very considerable
beds, such as those of the ooze-bogs now forming in the marshes of the
geyser basins of the Yellowstone Park,[295] and the diatom oozes of the deep
sea (Fig. 353, p. 425).
Fungi, for obvious reasons, have left but scant traces of themselves.
Bacteria are believed to be recognizable as far back as the Paleozoic era.
They are now the chief agents in the decomposition of organic matter, and
may be regarded as the prime enemies of the fossil record. It is probable
that similar decomposition took place actively in the earliest ages, for
otherwise the remains of the ancient organisms should be more abundant.
There is hence a theoretical probability that bacteria flourished as far back
as the stratigraphic record goes. Not unlikely they were originally simple
algæ that turned from the primitive habit of making their own food, to
living on other organisms or their remains, and in so doing lost their power
of manufacturing chlorophyll and of using inorganic carbon compounds.
Their remarkable adaptation to the most varied conditions, and their
extraordinary ability to endure the greatest vicissitudes of environment,
support the view that they are a very ancient and plastic form.
At present certain bacteria are important to higher vegetation because of
their ability to use the free nitrogen of the atmosphere and to combine it
into forms available for the higher plants. It is not improbable that they
have subserved this important function through all the known ages. Some
Page 745
experiments seem to show that certain of the existing algæ have this power,
and possibly the ancestral forms of plants possessed it. The bacteria, being a
derived and not an original form, could not have performed the function for
the first plants. It is possible, of course, that the inorganic supply of nitrogen
compounds was sufficient for plant life at the outset.
The contribution of the Bryophytes (liverworts, mosses).—The
mosses and liverworts have left no certain record of their work in the earlier
and middle geologic eras, and, if they existed at all, their contributions were
unimportant. Although low forms of plant life, they are not primitive ones,
as they are characterized by a definite alternation of generations implying a
considerable time antecedent to the attainment of their present forms; hence
there are no very cogent theoretical reasons for assigning them a place in
early geologic history, though their absence cannot be affirmed. Some
botanists think the Pteridophytes were derived from some ancestral form of
liverwort, which, if true, would require the presence of the latter in an early
geologic period; but the negative geological evidence relative to their
presence favors the alternative view that the Pteridophytes were derived
from some form of the Thallophytes by an independent line. In recent times,
certain of the mosses, especially the sphagnum mosses, have played a
notable part in the formation of peat accumulations. For this, their habit of
growing in bogs, and of dying below while they continue to grow above
admirably fits them.
The contribution of the Pteridophytes (ferns, horsetails, lycopods,
Sphenophyllum).—The Pteridophytes include the most important fossil
plants of the earlier and middle geologic eras. To them we owe chiefly the
great carbonaceous deposits of the Coal Measures and probably most of the
disseminated carbons of the early and middle eras; perhaps also much of the
natural oil and gas. Their special work is so conspicuous that it will be
noted at length in the chapters on the Devonian and Carboniferous periods,
and hence may be passed here with brevity. The ferns, now known more for
their beauty than their importance, are the representative type of the group,
and are really a wonderful family, having preserved their characteristic leaf-
forms with a persistence attained by no other group of plants. The Paleozoic
ferns are recognizable as such by every one, irrespective of botanical
knowledge; indeed it is the detection of the differences, rather than the
resemblances, between the ancient and modern forms, that requires expert
and possibly the ancestral forms of plants possessed it. The bacteria, being a
derived and not an original form, could not have performed the function for
the first plants. It is possible, of course, that the inorganic supply of nitrogen
compounds was sufficient for plant life at the outset.
The contribution of the Bryophytes (liverworts, mosses).—The
mosses and liverworts have left no certain record of their work in the earlier
and middle geologic eras, and, if they existed at all, their contributions were
unimportant. Although low forms of plant life, they are not primitive ones,
as they are characterized by a definite alternation of generations implying a
considerable time antecedent to the attainment of their present forms; hence
there are no very cogent theoretical reasons for assigning them a place in
early geologic history, though their absence cannot be affirmed. Some
botanists think the Pteridophytes were derived from some ancestral form of
liverwort, which, if true, would require the presence of the latter in an early
geologic period; but the negative geological evidence relative to their
presence favors the alternative view that the Pteridophytes were derived
from some form of the Thallophytes by an independent line. In recent times,
certain of the mosses, especially the sphagnum mosses, have played a
notable part in the formation of peat accumulations. For this, their habit of
growing in bogs, and of dying below while they continue to grow above
admirably fits them.
The contribution of the Pteridophytes (ferns, horsetails, lycopods,
Sphenophyllum).—The Pteridophytes include the most important fossil
plants of the earlier and middle geologic eras. To them we owe chiefly the
great carbonaceous deposits of the Coal Measures and probably most of the
disseminated carbons of the early and middle eras; perhaps also much of the
natural oil and gas. Their special work is so conspicuous that it will be
noted at length in the chapters on the Devonian and Carboniferous periods,
and hence may be passed here with brevity. The ferns, now known more for
their beauty than their importance, are the representative type of the group,
and are really a wonderful family, having preserved their characteristic leaf-
forms with a persistence attained by no other group of plants. The Paleozoic
ferns are recognizable as such by every one, irrespective of botanical
knowledge; indeed it is the detection of the differences, rather than the
resemblances, between the ancient and modern forms, that requires expert
Page 746
knowledge. This continuity shows that since their introduction the changes
of climate have never been so great as to prevent their propagation, without
radical modification, in some part of the globe, and this fact rather narrowly
limits the range of surface temperatures, and of other climatic vicissitudes.
The persistence of the Equisetæ (horsetails, scouring-rushes) and the
lycopods (club-mosses) bears like testimony, as does the persistence of life
in general; but the rather delicate ferns are perhaps more obviously
significant than most organisms.
The contribution of the Spermatophytes (seed plants, including
gymnosperms or “evergreens” and angiosperms or “flowering plants”).
—The angiosperms, the dominant group to-day, make their appearance in
the record in the latter part of the Mesozoic era, and their contribution is,
therefore, relatively modern. They contributed to the coals, lignites, oils,
and organic gases of the late geological periods, as did the Pteridophytes in
the earlier periods, the latter participating, however, in the late deposits.
Perhaps the most important function of the Spermatophytes lay in their
superior serviceability as food for the higher land animals, by virtue of their
seeds, fruits, and foliage. Neither the Thallophytes, Bryophytes, nor
Pteridophytes, nor all combined, approach the Spermatophytes in food
value for the higher types of animal life, and it is doubtful whether the
higher evolution of the land animals could have taken place without the
previous introduction of the seed plants. It will be noted in the historical
narrative that the great placental group of mammals came in and deployed
with marvelous rapidity, as geological progress goes, soon after the
Spermatophytes became the dominant form of vegetation.
Plant life terrestrial rather than marine.—It is to be noticed that the
chief development of all the great groups of plants took place on the land,
or in the land-waters, rather than in the sea. This is preeminently true of the
higher types, and appears also to be true of even the Thallophytes, although
the number of individual algæ and their total mass is very much greater in
the sea than on the land and in the land-waters. But the fresh-water algæ
appear to possess in a higher degree than the marine forms those plastic and
germinal characters from which new forms spring, and are probably to be
regarded as the parental type. These are facts to be pondered on, since it has
been the current opinion of geologists that life arose in the sea and was
propagated thence to the land. The alternative view that life developed
of climate have never been so great as to prevent their propagation, without
radical modification, in some part of the globe, and this fact rather narrowly
limits the range of surface temperatures, and of other climatic vicissitudes.
The persistence of the Equisetæ (horsetails, scouring-rushes) and the
lycopods (club-mosses) bears like testimony, as does the persistence of life
in general; but the rather delicate ferns are perhaps more obviously
significant than most organisms.
The contribution of the Spermatophytes (seed plants, including
gymnosperms or “evergreens” and angiosperms or “flowering plants”).
—The angiosperms, the dominant group to-day, make their appearance in
the record in the latter part of the Mesozoic era, and their contribution is,
therefore, relatively modern. They contributed to the coals, lignites, oils,
and organic gases of the late geological periods, as did the Pteridophytes in
the earlier periods, the latter participating, however, in the late deposits.
Perhaps the most important function of the Spermatophytes lay in their
superior serviceability as food for the higher land animals, by virtue of their
seeds, fruits, and foliage. Neither the Thallophytes, Bryophytes, nor
Pteridophytes, nor all combined, approach the Spermatophytes in food
value for the higher types of animal life, and it is doubtful whether the
higher evolution of the land animals could have taken place without the
previous introduction of the seed plants. It will be noted in the historical
narrative that the great placental group of mammals came in and deployed
with marvelous rapidity, as geological progress goes, soon after the
Spermatophytes became the dominant form of vegetation.
Plant life terrestrial rather than marine.—It is to be noticed that the
chief development of all the great groups of plants took place on the land,
or in the land-waters, rather than in the sea. This is preeminently true of the
higher types, and appears also to be true of even the Thallophytes, although
the number of individual algæ and their total mass is very much greater in
the sea than on the land and in the land-waters. But the fresh-water algæ
appear to possess in a higher degree than the marine forms those plastic and
germinal characters from which new forms spring, and are probably to be
regarded as the parental type. These are facts to be pondered on, since it has
been the current opinion of geologists that life arose in the sea and was
propagated thence to the land. The alternative view that life developed
Page 747
primarily on the land and in the land-waters and migrated to the sea is not,
however, without its support in the plant world, as we thus see, and the
plant world was the primitive one; the dependent animal world necessarily
followed its development. The hypothesis of a terrestrial origin of life
throws a very suggestive cross-light on many geological problems, as will
be seen later, and it may well be entertained as an alternative working
hypothesis until the facts are more fully developed.
B. Contributions of the Animal Kingdom.[296]
As already noted, animal life is dependent on the decomposition of
matter organized by green plants, and the conversion of its potential energy
into active forms. Animals are, therefore, dynamic rather than constructive
agencies. Nevertheless they transform organic vegetal matter into organic
animal matter, and this is sometimes really an advance in organization. The
organized animal matter is subject to preservation in some small degree,
though it usually perishes. Some contribution is, therefore, made to the
organic deposits, chiefly in the form of hydrocarbons. It is the view of some
geologists that the natural oils and gases have an animal origin in the main.
REFERENCE TABLE OF THE PRINCIPAL GROUPS OF ANIMALS.[297]
Foraminifera.
Rhizopoda
Radiolaria.
Protozoa
Flagellata
The simplest animals)
Infusoria Unknown in fossil state.
Gregarina
Calcareous sponges.
Porifera Spongiæ
Cœlenterata Silicious sponges.
(Sponges, corals, jellyfishes) Anthozoa, coral polyps.
Cnidaria
Hydrozoa, hydroids and medusæ.
Cystoidea, cystids.
Pelmatozoa Crinoidea, stone lilies.
Echinodermata Blastoidea, blastids.
(Crinoids, starfishes, sea- Ophiuroidea, brittle-stars
Asterozoa
urchins) Asteroidea, starfishes.
Echinoidea, sea-urchins.
Echinozoa
Holothuroidea, sea-cucumbers.
Vermes Platyhelminthes
(Worms) Rotifera
Rare as fossils.
Nemathelminthes
Gephyrea
however, without its support in the plant world, as we thus see, and the
plant world was the primitive one; the dependent animal world necessarily
followed its development. The hypothesis of a terrestrial origin of life
throws a very suggestive cross-light on many geological problems, as will
be seen later, and it may well be entertained as an alternative working
hypothesis until the facts are more fully developed.
B. Contributions of the Animal Kingdom.[296]
As already noted, animal life is dependent on the decomposition of
matter organized by green plants, and the conversion of its potential energy
into active forms. Animals are, therefore, dynamic rather than constructive
agencies. Nevertheless they transform organic vegetal matter into organic
animal matter, and this is sometimes really an advance in organization. The
organized animal matter is subject to preservation in some small degree,
though it usually perishes. Some contribution is, therefore, made to the
organic deposits, chiefly in the form of hydrocarbons. It is the view of some
geologists that the natural oils and gases have an animal origin in the main.
REFERENCE TABLE OF THE PRINCIPAL GROUPS OF ANIMALS.[297]
Foraminifera.
Rhizopoda
Radiolaria.
Protozoa
Flagellata
The simplest animals)
Infusoria Unknown in fossil state.
Gregarina
Calcareous sponges.
Porifera Spongiæ
Cœlenterata Silicious sponges.
(Sponges, corals, jellyfishes) Anthozoa, coral polyps.
Cnidaria
Hydrozoa, hydroids and medusæ.
Cystoidea, cystids.
Pelmatozoa Crinoidea, stone lilies.
Echinodermata Blastoidea, blastids.
(Crinoids, starfishes, sea- Ophiuroidea, brittle-stars
Asterozoa
urchins) Asteroidea, starfishes.
Echinoidea, sea-urchins.
Echinozoa
Holothuroidea, sea-cucumbers.
Vermes Platyhelminthes
(Worms) Rotifera
Rare as fossils.
Nemathelminthes
Gephyrea
Page 748
Annelida, sea-worms.
Molluscoidea Bryozoa, sea-mosses.
(Mollusc-like forms) Brachiopoda, lamp-shells.
Pelecypoda, lamellibranchs, bivalves.
Scaphopoda, tusk-shells.
Mollusca
Amphineura, chiton.
(Molluscs)
Gastropoda, univalves, snails, etc.
Cephalopoda, nautilus, cuttlefish.
Crustacea.
Trilobita, trilobites.
Branchiata Gigantostraca, horse-shoe crabs.
Arthropoda Entomostraca, ostracoids, barnacles.
(The articulates) Malacostraca, lobsters, crabs.
Myriapoda, centipedes.
Tracheata Arachnoidea, spiders, scorpions.
Insecta, insects.
Cyclostomata, lampreys.
Selachii, sharks.
Holocephali, spook-fishes.
Pisces Dipnoi, lung-fishes.
(fishes) Teleostomi, ganoids and
teleosus.
Vertebrata (common fishes).
Amphibia, amphibians, batrachians.
Reptilia, reptiles.
Aves, birds.
Prototheria, monotremes.
Mammalia
Metatheria, marsupials.
(mammals)
Eutheria, placentals.
As dynamic organisms animals have need for supporting- and working-
frames, for protective covering or housing, and for offensive and defensive
weapons, and these have been constructed chiefly out of inorganic matter,
and subordinately of indurated organic matter. It is through these that
animals have made their chief contribution to the material of the geologic
record. Skeletons and other hard parts to give internal stiffness or firmness;
shells, plates, indurated integuments, and various other forms of external
protection; teeth, spines, horns, and other means of gathering and
masticating food, and of attack and defense, contribute material to the
deposits, and form a record of the life activities and of the physiographic
environment. All of the eight groups of animals, viz. Protozoa, Cœlenterata,
Echinodermata, Vermes, Molluscoidea, Mollusca, Arthropoda, and
Vertebrata, have left some record, but it is in all cases a very imperfect one.
Molluscoidea Bryozoa, sea-mosses.
(Mollusc-like forms) Brachiopoda, lamp-shells.
Pelecypoda, lamellibranchs, bivalves.
Scaphopoda, tusk-shells.
Mollusca
Amphineura, chiton.
(Molluscs)
Gastropoda, univalves, snails, etc.
Cephalopoda, nautilus, cuttlefish.
Crustacea.
Trilobita, trilobites.
Branchiata Gigantostraca, horse-shoe crabs.
Arthropoda Entomostraca, ostracoids, barnacles.
(The articulates) Malacostraca, lobsters, crabs.
Myriapoda, centipedes.
Tracheata Arachnoidea, spiders, scorpions.
Insecta, insects.
Cyclostomata, lampreys.
Selachii, sharks.
Holocephali, spook-fishes.
Pisces Dipnoi, lung-fishes.
(fishes) Teleostomi, ganoids and
teleosus.
Vertebrata (common fishes).
Amphibia, amphibians, batrachians.
Reptilia, reptiles.
Aves, birds.
Prototheria, monotremes.
Mammalia
Metatheria, marsupials.
(mammals)
Eutheria, placentals.
As dynamic organisms animals have need for supporting- and working-
frames, for protective covering or housing, and for offensive and defensive
weapons, and these have been constructed chiefly out of inorganic matter,
and subordinately of indurated organic matter. It is through these that
animals have made their chief contribution to the material of the geologic
record. Skeletons and other hard parts to give internal stiffness or firmness;
shells, plates, indurated integuments, and various other forms of external
protection; teeth, spines, horns, and other means of gathering and
masticating food, and of attack and defense, contribute material to the
deposits, and form a record of the life activities and of the physiographic
environment. All of the eight groups of animals, viz. Protozoa, Cœlenterata,
Echinodermata, Vermes, Molluscoidea, Mollusca, Arthropoda, and
Vertebrata, have left some record, but it is in all cases a very imperfect one.
Page 749
The contribution of the Protozoa.—The Protozoa are related to the
animal kingdom much as the Thallophytes are to the vegetable, and the two
bear a close structural resemblance to one another. So near, indeed, do the
Protozoa and the Thallophytes approach one another in their minuteness
and simplicity, that the place of not a few organisms is in doubt, and the two
kingdoms, in general so different, seem here to blend in the group
Flagellata. The Protozoa are usually very minute one-celled organisms with
very little differentiation of tissue or organs. Of the four classes of Protozoa,
only one, the Rhizopoda, is found in the fossil state. The rhizopods secrete
silicious skeletons, and calcareous, silicious, and chitinous tests of a great
variety of forms, and this gives them geologic importance. The deep-sea
oozes and the chalk deposits are their best-known contributions at present.
They have probably played a more important rôle in the formation of
ordinary limestones and silicious silts than can be demonstrated, because of
the delicacy of their relics and the ease with which these are pulverized by
wave-action in the shallow seas, or changed by recrystallization or by
concretionary aggregation. The globigerina oozes are formed largely from
the calcareous shells of Foraminifera (Fig. 351), one of the orders of
rhizopods, among which the genus Globigerina is a leading form. Those
forms which make the deep-sea oozes live, not on the bottom, but near the
surface of the open sea, and on the death of the organisms, the shells, tests,
and skeletons sink to the bottom. Chalk is formed in a similar way from
calcareous Foraminifera, but not necessarily in very deep water.
Foraminifera live in shallow water as well as in the open sea, and in this
case they sometimes creep on the bottom or are attached to algæ, but their
deposits in shallow water are usually much obscured by other kinds of
deposition and by destructive action. Some of the foraminiferal shells are
divided into chambers and assume various spiral forms, of which the
Nummulites, named from their resemblance to coins, are notable examples.
These formed an important part of the nummulitic limestone of the Eocene
period.
The radiolarian ooze is characterized by the silicious tests of various
members of the silica-bearing order, Radiolaria. The “Barbadoes earth” and
“Tripoli” are notable deposits of fossil radiolarians.
The contribution of the Cœlenterata.—The Cœlenterata embrace the
sponges, the coral polyps (Anthozoa), and the hydroids and medusæ
animal kingdom much as the Thallophytes are to the vegetable, and the two
bear a close structural resemblance to one another. So near, indeed, do the
Protozoa and the Thallophytes approach one another in their minuteness
and simplicity, that the place of not a few organisms is in doubt, and the two
kingdoms, in general so different, seem here to blend in the group
Flagellata. The Protozoa are usually very minute one-celled organisms with
very little differentiation of tissue or organs. Of the four classes of Protozoa,
only one, the Rhizopoda, is found in the fossil state. The rhizopods secrete
silicious skeletons, and calcareous, silicious, and chitinous tests of a great
variety of forms, and this gives them geologic importance. The deep-sea
oozes and the chalk deposits are their best-known contributions at present.
They have probably played a more important rôle in the formation of
ordinary limestones and silicious silts than can be demonstrated, because of
the delicacy of their relics and the ease with which these are pulverized by
wave-action in the shallow seas, or changed by recrystallization or by
concretionary aggregation. The globigerina oozes are formed largely from
the calcareous shells of Foraminifera (Fig. 351), one of the orders of
rhizopods, among which the genus Globigerina is a leading form. Those
forms which make the deep-sea oozes live, not on the bottom, but near the
surface of the open sea, and on the death of the organisms, the shells, tests,
and skeletons sink to the bottom. Chalk is formed in a similar way from
calcareous Foraminifera, but not necessarily in very deep water.
Foraminifera live in shallow water as well as in the open sea, and in this
case they sometimes creep on the bottom or are attached to algæ, but their
deposits in shallow water are usually much obscured by other kinds of
deposition and by destructive action. Some of the foraminiferal shells are
divided into chambers and assume various spiral forms, of which the
Nummulites, named from their resemblance to coins, are notable examples.
These formed an important part of the nummulitic limestone of the Eocene
period.
The radiolarian ooze is characterized by the silicious tests of various
members of the silica-bearing order, Radiolaria. The “Barbadoes earth” and
“Tripoli” are notable deposits of fossil radiolarians.
The contribution of the Cœlenterata.—The Cœlenterata embrace the
sponges, the coral polyps (Anthozoa), and the hydroids and medusæ
Page 750
(Hydrozoa). The contribution of coral polyps to the formation of limestone
is most important, and is too familiar to require elaboration here. The corals
range throughout nearly the whole fossiliferous series, and their
development will be followed and illustrated in the historical chapters.
The sponges are widely represented by their spicules, and not
uncommonly their aggregate form is preserved even in very ancient strata.
Their contribution is largely silicious, but is partly calcareous. The hydroids
and medusæ have left little trace of themselves in the rocks, although
impressions supposed to represent medusæ are found in strata as early as
the Cambrian. Certain coral-like forms, as the Millepores, Tubularia, and
Stromatopora, are classed as Hydrozoa. The graptolites, delicate leaf-like
floating forms, very serviceable in marking exact horizons on different
continents because of their free distribution, are also classed here.
The contribution of the Echinodermata.—Under the echinoderms are
grouped the crinoids (sea-lilies), cystoids, blastoids, ophiuroids (brittle
stars), asteroids (starfishes), echinoids (sea-urchins), and holothuroids (sea-
cucumbers). This is one of the marked groups of ancient as well as modern
life, and its beautiful fossils grace every period in which life relics are well
preserved. The cystoids and crinoids, and later the blastoids, were
prominent in the Paleozoic ages, while the remaining forms were more
conspicuous later, though early introduced. All divisions, except the
holothuroids, whose softness prevented, have left a good record, as fossil
records go. Their relics are chiefly calcareous, and they most abound in the
limestones, some of which are largely made up of their remains, as the
encrinital limestone (Fig. 349). They will be subjects of frequent comment
and illustration in the historical chapters.
The contribution of the Vermes.—Most of the worms are ill adapted to
fossilization and are not known in the fossil form. The segmental worms of
the sea, the annelids, however, left some traces of themselves in tubes and
borings and in tracks and sometimes by fossil jaws and teeth. They range
from the earliest fossil-marked horizons onward, but seem to have always
been an inferior group.
The contribution of the Molluscoidea.—This group includes the
bryozoans, whose fossil products closely resemble the minute-celled corals,
and the brachiopods, whose shells closely resemble those of the molluscs.
is most important, and is too familiar to require elaboration here. The corals
range throughout nearly the whole fossiliferous series, and their
development will be followed and illustrated in the historical chapters.
The sponges are widely represented by their spicules, and not
uncommonly their aggregate form is preserved even in very ancient strata.
Their contribution is largely silicious, but is partly calcareous. The hydroids
and medusæ have left little trace of themselves in the rocks, although
impressions supposed to represent medusæ are found in strata as early as
the Cambrian. Certain coral-like forms, as the Millepores, Tubularia, and
Stromatopora, are classed as Hydrozoa. The graptolites, delicate leaf-like
floating forms, very serviceable in marking exact horizons on different
continents because of their free distribution, are also classed here.
The contribution of the Echinodermata.—Under the echinoderms are
grouped the crinoids (sea-lilies), cystoids, blastoids, ophiuroids (brittle
stars), asteroids (starfishes), echinoids (sea-urchins), and holothuroids (sea-
cucumbers). This is one of the marked groups of ancient as well as modern
life, and its beautiful fossils grace every period in which life relics are well
preserved. The cystoids and crinoids, and later the blastoids, were
prominent in the Paleozoic ages, while the remaining forms were more
conspicuous later, though early introduced. All divisions, except the
holothuroids, whose softness prevented, have left a good record, as fossil
records go. Their relics are chiefly calcareous, and they most abound in the
limestones, some of which are largely made up of their remains, as the
encrinital limestone (Fig. 349). They will be subjects of frequent comment
and illustration in the historical chapters.
The contribution of the Vermes.—Most of the worms are ill adapted to
fossilization and are not known in the fossil form. The segmental worms of
the sea, the annelids, however, left some traces of themselves in tubes and
borings and in tracks and sometimes by fossil jaws and teeth. They range
from the earliest fossil-marked horizons onward, but seem to have always
been an inferior group.
The contribution of the Molluscoidea.—This group includes the
bryozoans, whose fossil products closely resemble the minute-celled corals,
and the brachiopods, whose shells closely resemble those of the molluscs.
Page 751
Both are calcareous and make important contributions to the formation of
limestone (Fig. 350). A few brachiopods secrete calcium phosphate instead
of calcium carbonate. Both classes have a great geologic range and their
fossils are valuable aids in identifying and correlating formations. Probably
the brachiopods are more utilized for this purpose than any other single
class. They are the symbol of conservatism and persistence, ranging from
the Cambrian to the present time, and embracing some forms that have
scarcely changed to the extent of generic difference in that time.
The contribution of the Mollusca.—The molluscs have also ranged
from the earliest well-recorded times, and some divisions, as the pelecypods
(lamellibranchs, embracing clams, oysters, etc.) and gastropods (snails,
etc.), have undergone no very marked change beyond a rather ample and
progressive development; but others, as the cephalopods (nautilus, squids,
cuttlefish, etc.), mark out the progress of the ages by distinct and striking
changes of form. Their shells are chiefly calcareous and they have
contributed materially to the formation of limestone. Muddy and sandy
bottoms are, however, more congenial to the pelecypods and gastropods
than to the corals, crinoids, and many other limestone-forming types, and
hence fossils of these molluscs frequently abound in shales and sandstones
and give them a calcareous element. In sandstones, however, the calcareous
matter is often dissolved out and only the casts of the shells remain. The
molluscs will be much cited and illustrated in the historical chapters.
The contribution of the Arthropoda.—This group embraces the
crustaceans, myriopods, spiders, and insects. The hard parts of their bodies
are mainly horny or chitinous forms of organic matter, and hence their relics
differ notably from the inorganic calcareous and silicious remains of most
of the preceding forms. The Arthropoda did not at any time form a notable
stratum of rock. Their geologic value lies chiefly in what they teach of the
progress of life and its relations, and the aid they render in correlation and
identification. In these respects the group is a notable one. It was
represented in the early fossiliferous strata by the trilobites, one of the most
interesting of all types of fossils. These were probably the most highly
developed organisms of their times and give the clearest hints of the stage
of psychological and sociological development that had been reached when
first the record of life is opened to us. The record of the myriopods, spiders,
limestone (Fig. 350). A few brachiopods secrete calcium phosphate instead
of calcium carbonate. Both classes have a great geologic range and their
fossils are valuable aids in identifying and correlating formations. Probably
the brachiopods are more utilized for this purpose than any other single
class. They are the symbol of conservatism and persistence, ranging from
the Cambrian to the present time, and embracing some forms that have
scarcely changed to the extent of generic difference in that time.
The contribution of the Mollusca.—The molluscs have also ranged
from the earliest well-recorded times, and some divisions, as the pelecypods
(lamellibranchs, embracing clams, oysters, etc.) and gastropods (snails,
etc.), have undergone no very marked change beyond a rather ample and
progressive development; but others, as the cephalopods (nautilus, squids,
cuttlefish, etc.), mark out the progress of the ages by distinct and striking
changes of form. Their shells are chiefly calcareous and they have
contributed materially to the formation of limestone. Muddy and sandy
bottoms are, however, more congenial to the pelecypods and gastropods
than to the corals, crinoids, and many other limestone-forming types, and
hence fossils of these molluscs frequently abound in shales and sandstones
and give them a calcareous element. In sandstones, however, the calcareous
matter is often dissolved out and only the casts of the shells remain. The
molluscs will be much cited and illustrated in the historical chapters.
The contribution of the Arthropoda.—This group embraces the
crustaceans, myriopods, spiders, and insects. The hard parts of their bodies
are mainly horny or chitinous forms of organic matter, and hence their relics
differ notably from the inorganic calcareous and silicious remains of most
of the preceding forms. The Arthropoda did not at any time form a notable
stratum of rock. Their geologic value lies chiefly in what they teach of the
progress of life and its relations, and the aid they render in correlation and
identification. In these respects the group is a notable one. It was
represented in the early fossiliferous strata by the trilobites, one of the most
interesting of all types of fossils. These were probably the most highly
developed organisms of their times and give the clearest hints of the stage
of psychological and sociological development that had been reached when
first the record of life is opened to us. The record of the myriopods, spiders,
Page 752
and insects dates from the middle Paleozoic, and gives the first clear hints
of animal life on the land.
The contribution of the Vertebrata.—In the vertebrates the dynamic or
working organism may be said to reach its highest expression, unless it be
in the flying insects, and their inorganic residue becomes relatively
unimportant in rock formation. Although the greatest of all animal types in
most respects, it has never formed more than trivial beds of rocks. There are
occasional “bone beds,” but they are thin and limited in extent, and only
partially formed of vertebrate matter. The geological importance of the
vertebrates lies in the higher field of life evolution and in its mental
accompaniment. Fishes excepted, the vertebrates are mainly land types, and
have for their chief colleagues plants and insects. The other groups of
animals are mainly, though not wholly, marine. The vertebrates have little
place in the Paleozoic record, except near its close, but they dominate the
Mesozoic and Cenozoic eras, and are conspicuously the master type to day.
III. THE ASSOCIATIONS AND ECOLOGICAL RELATIONS
OF LIFE.
A. The Basis of Floras and Faunas.
Geologic interest is not confined to the kinds of plants and animals that
have lived and the contributions they have made to the deposits, but
embraces also their assemblage into floras and faunas, and the relations of
these assemblages to the prevailing physiographic features. These
assemblages and relationships are among the most suggestive factors of the
earth’s evolution, and are the most instructive for purposes of comparison
with human history, and for forecasting the future of man and of the whole
biological kingdom. Moreover, floras and faunas, as such, are used in the
correlation of formations, and in this application they give surer results than
correlations by individual species. A particular species may live far beyond
the usual period of a species, and if fossilized in one region in its early
history and in another in its late history, the two formations might be
referred erroneously to the same stage. This is far less likely to happen with
a whole assemblage of forms. There is a similar liability to error in
interpreting migrations on the basis of a single or a few species, for a single
of animal life on the land.
The contribution of the Vertebrata.—In the vertebrates the dynamic or
working organism may be said to reach its highest expression, unless it be
in the flying insects, and their inorganic residue becomes relatively
unimportant in rock formation. Although the greatest of all animal types in
most respects, it has never formed more than trivial beds of rocks. There are
occasional “bone beds,” but they are thin and limited in extent, and only
partially formed of vertebrate matter. The geological importance of the
vertebrates lies in the higher field of life evolution and in its mental
accompaniment. Fishes excepted, the vertebrates are mainly land types, and
have for their chief colleagues plants and insects. The other groups of
animals are mainly, though not wholly, marine. The vertebrates have little
place in the Paleozoic record, except near its close, but they dominate the
Mesozoic and Cenozoic eras, and are conspicuously the master type to day.
III. THE ASSOCIATIONS AND ECOLOGICAL RELATIONS
OF LIFE.
A. The Basis of Floras and Faunas.
Geologic interest is not confined to the kinds of plants and animals that
have lived and the contributions they have made to the deposits, but
embraces also their assemblage into floras and faunas, and the relations of
these assemblages to the prevailing physiographic features. These
assemblages and relationships are among the most suggestive factors of the
earth’s evolution, and are the most instructive for purposes of comparison
with human history, and for forecasting the future of man and of the whole
biological kingdom. Moreover, floras and faunas, as such, are used in the
correlation of formations, and in this application they give surer results than
correlations by individual species. A particular species may live far beyond
the usual period of a species, and if fossilized in one region in its early
history and in another in its late history, the two formations might be
referred erroneously to the same stage. This is far less likely to happen with
a whole assemblage of forms. There is a similar liability to error in
interpreting migrations on the basis of a single or a few species, for a single
Page 753
species or a few species may be transported by unusual or accidental means,
so to speak, when there is no normal pathway for general migration, and
when no systematic migration takes place. In most of the great questions
that arise concerning the connections and disseverances of the continents,
and concerning the unions and separations of the oceans, which are the
fundamental causes of the migrations and of the isolations of plants and
animals, typical floras and faunas are to be studied, rather than isolated
species or sporadic forms. A brief sketch of the leading causes and
consequences of these special assemblages of plants and animals may aid in
appreciating the underlying significance of floras and faunas, and in
interpreting their meaning as they are met in the study of the strata. A part
of these grow out of the relations of the organisms to one another, and a part
out of the relations of the organisms to their environment.
(1) Assemblages Influenced by the Mutual Relations of Organisms.
(a) Food relations.—The relations of food-supply are among the most
obvious reasons for assemblages. As animals are dependent directly or
indirectly on plants for their food, they must gather where the plants grow,
or in the currents in which the plant products are borne. Whatever
determines an assemblage of plants also causes, or at least invites, an
assemblage of animals. Whatever causes an assemblage of particular plants,
invites an assemblage of the particular animals that use these plants.
Animals that feed on plants are in turn preyed upon by other animals, and
these in turn by others. A whole train of organisms may, therefore, be
gathered into a region by the conditions that foster a certain kind of
vegetation there. In interpreting the physical significance of such a train, it
is obvious that the head of the train carries the fundamental meaning. The
dependent creatures that follow the primary forms may be only incidentally,
and perhaps very slightly, adapted to the physical environment.
(b) Adaptive relations.—Organisms depending on other organisms for
food or other necessary conditions of life, present many forms of adaptation
the better to secure their food and to use it. These adaptations are the
consequences and the signs of the assemblage, and are of the greatest
service in interpreting the place and significance of the organisms in the
assemblage. Teeth usually reveal the food of their possessors, and hence
teeth are among the most significant of fossils. Fortunately their functions
so to speak, when there is no normal pathway for general migration, and
when no systematic migration takes place. In most of the great questions
that arise concerning the connections and disseverances of the continents,
and concerning the unions and separations of the oceans, which are the
fundamental causes of the migrations and of the isolations of plants and
animals, typical floras and faunas are to be studied, rather than isolated
species or sporadic forms. A brief sketch of the leading causes and
consequences of these special assemblages of plants and animals may aid in
appreciating the underlying significance of floras and faunas, and in
interpreting their meaning as they are met in the study of the strata. A part
of these grow out of the relations of the organisms to one another, and a part
out of the relations of the organisms to their environment.
(1) Assemblages Influenced by the Mutual Relations of Organisms.
(a) Food relations.—The relations of food-supply are among the most
obvious reasons for assemblages. As animals are dependent directly or
indirectly on plants for their food, they must gather where the plants grow,
or in the currents in which the plant products are borne. Whatever
determines an assemblage of plants also causes, or at least invites, an
assemblage of animals. Whatever causes an assemblage of particular plants,
invites an assemblage of the particular animals that use these plants.
Animals that feed on plants are in turn preyed upon by other animals, and
these in turn by others. A whole train of organisms may, therefore, be
gathered into a region by the conditions that foster a certain kind of
vegetation there. In interpreting the physical significance of such a train, it
is obvious that the head of the train carries the fundamental meaning. The
dependent creatures that follow the primary forms may be only incidentally,
and perhaps very slightly, adapted to the physical environment.
(b) Adaptive relations.—Organisms depending on other organisms for
food or other necessary conditions of life, present many forms of adaptation
the better to secure their food and to use it. These adaptations are the
consequences and the signs of the assemblage, and are of the greatest
service in interpreting the place and significance of the organisms in the
assemblage. Teeth usually reveal the food of their possessors, and hence
teeth are among the most significant of fossils. Fortunately their functions
Page 754
require them to be hard and durable, and hence well suited to fossilization.
The growth of low plants into trees forced a notable series of adaptations in
the animals that fed upon them in the matter of height, of reaching
members, of climbing, and probably at length of parachuting and flying. In
these and similar ways the floras and faunas took on special phases because
of the mutual relations of their members.
(c) Competitive relations.—The assembling of plants and animals, with
their prodigious possibilities of multiplication, brought competition, and
with it a struggle for food which often became a struggle for existence, and
out of this grew innumerable modifications of form and habit. These have
become so familiar since the great awakening caused by the doctrines of
Darwin and Wallace that they need no elaboration here.
(d) Offensive and defensive relations.—Within limits, plants are
benefited by the feeding of animals and respond by developing seeds and
fruits that especially invite such action, their compensation being found in
planting and distribution. It is obvious that, on the whole, the continued
growth of plants is largely dependent on the renewal of a supply of carbon
dioxide through the agency of animals and some plants, bacteria in
particular. Otherwise the supply would become so reduced as to greatly
limit plant life. It has been estimated[298] that the whole of the present supply
of carbon dioxide would be consumed by plants in one hundred years if the
consumption continued at the present rate and no carbon dioxide was
returned. It is now well known that the so-called decay by which carbon
dioxide is freed is due more to microscopic organisms than to inorganic
processes. It seems clear, therefore, that the continued activity of plants is
largely due to their consumption by animals and other plants. But still,
though the larger good of plants is conserved by the predaceous action of
animals, and of certain parasitic and saprophytic plants, their individual
preservation is often conserved by defensive devices, such as thorns,
poisons, bitter compounds, etc. This is notably true in desert regions where
the conditions are hard and the total extinction of plants would be
threatened if animals were permitted to feed freely upon them. Within the
animal world, the preying of one form upon another is the main source of
that great struggle for existence which has characterized the whole known
history of life, and has been one of the influential factors in shaping the
The growth of low plants into trees forced a notable series of adaptations in
the animals that fed upon them in the matter of height, of reaching
members, of climbing, and probably at length of parachuting and flying. In
these and similar ways the floras and faunas took on special phases because
of the mutual relations of their members.
(c) Competitive relations.—The assembling of plants and animals, with
their prodigious possibilities of multiplication, brought competition, and
with it a struggle for food which often became a struggle for existence, and
out of this grew innumerable modifications of form and habit. These have
become so familiar since the great awakening caused by the doctrines of
Darwin and Wallace that they need no elaboration here.
(d) Offensive and defensive relations.—Within limits, plants are
benefited by the feeding of animals and respond by developing seeds and
fruits that especially invite such action, their compensation being found in
planting and distribution. It is obvious that, on the whole, the continued
growth of plants is largely dependent on the renewal of a supply of carbon
dioxide through the agency of animals and some plants, bacteria in
particular. Otherwise the supply would become so reduced as to greatly
limit plant life. It has been estimated[298] that the whole of the present supply
of carbon dioxide would be consumed by plants in one hundred years if the
consumption continued at the present rate and no carbon dioxide was
returned. It is now well known that the so-called decay by which carbon
dioxide is freed is due more to microscopic organisms than to inorganic
processes. It seems clear, therefore, that the continued activity of plants is
largely due to their consumption by animals and other plants. But still,
though the larger good of plants is conserved by the predaceous action of
animals, and of certain parasitic and saprophytic plants, their individual
preservation is often conserved by defensive devices, such as thorns,
poisons, bitter compounds, etc. This is notably true in desert regions where
the conditions are hard and the total extinction of plants would be
threatened if animals were permitted to feed freely upon them. Within the
animal world, the preying of one form upon another is the main source of
that great struggle for existence which has characterized the whole known
history of life, and has been one of the influential factors in shaping the
Page 755
evolution of life and in modifying the special aspects assumed by the floras
and faunas of each period.
Implied forms of life.—The full meaning of the fossils of any period can
only be gathered by duly considering these relationships in their
interpretation. The existence of animals implies the existence of plants in
supporting abundance, whether the record contains their relics or not; an
animal with a protective covering implies an enemy; a tooth of a specific
kind implies the appropriate class of food, etc. While inferences of this kind
are subject to error, they are at present the only means by which the faunas
and floras of most ages can be rounded out into a rational assemblage of
organisms, that is, an assemblage that affords the necessary food for its
members and an adequate function for the offensive and defensive devices
which its members present. Only a small part of the life that lived was
fossilized, and only a small part of the fossils actually carried in the strata
have been collected, because only a small part of the strata are exposed at
the surface. The direct record now accessible is, therefore, very incomplete
and hence the need—and in the need the excuse—for adding the forms that
are implied by the character of the known fossils.
(2) Assemblages Influenced by Environment.
It has been noted that some animals depend for existence on other
animals; that ultimately all animals depend on plants, and that green plants
alone can make food directly from inorganic material. Green plants,
therefore, head the train of dependencies, and their relations to the physical
conditions that surround them are the primal relations.
Plant societies.[299]—The control of physical conditions has been
sufficient to develop special associations or societies of plants by fostering
those adapted to these conditions and eliminating those that are not. Among
these are (1) the hydrophytes (“water plants”), embracing those that grow in
water or in very wet situations; (2) xerophytes (“drought plants”),
embracing the opposite class, which are adapted to very dry situations; (3)
mesophytes, including those suited to conditions lying between these
extremes, the great middle class to which the prevailing upland vegetation
belongs; and (4) the halophytes (“salt plants”), which are dependent on the
presence of certain salts, and embrace such plants as are found on the
and faunas of each period.
Implied forms of life.—The full meaning of the fossils of any period can
only be gathered by duly considering these relationships in their
interpretation. The existence of animals implies the existence of plants in
supporting abundance, whether the record contains their relics or not; an
animal with a protective covering implies an enemy; a tooth of a specific
kind implies the appropriate class of food, etc. While inferences of this kind
are subject to error, they are at present the only means by which the faunas
and floras of most ages can be rounded out into a rational assemblage of
organisms, that is, an assemblage that affords the necessary food for its
members and an adequate function for the offensive and defensive devices
which its members present. Only a small part of the life that lived was
fossilized, and only a small part of the fossils actually carried in the strata
have been collected, because only a small part of the strata are exposed at
the surface. The direct record now accessible is, therefore, very incomplete
and hence the need—and in the need the excuse—for adding the forms that
are implied by the character of the known fossils.
(2) Assemblages Influenced by Environment.
It has been noted that some animals depend for existence on other
animals; that ultimately all animals depend on plants, and that green plants
alone can make food directly from inorganic material. Green plants,
therefore, head the train of dependencies, and their relations to the physical
conditions that surround them are the primal relations.
Plant societies.[299]—The control of physical conditions has been
sufficient to develop special associations or societies of plants by fostering
those adapted to these conditions and eliminating those that are not. Among
these are (1) the hydrophytes (“water plants”), embracing those that grow in
water or in very wet situations; (2) xerophytes (“drought plants”),
embracing the opposite class, which are adapted to very dry situations; (3)
mesophytes, including those suited to conditions lying between these
extremes, the great middle class to which the prevailing upland vegetation
belongs; and (4) the halophytes (“salt plants”), which are dependent on the
presence of certain salts, and embrace such plants as are found on the
Page 756
seacoast, around salt springs, on alkaline flats, etc. The characters which
distinguish the xerophytes from the hydrophytes and mesophytes have
special geological interest, as they aid in determining the climatic
conditions, a feature whose interest increases as the variability of the
ancient climates is more fully recognized.
Within these greater groups there are special minor associations
determined by soil, temperature, topography, subjacent strata, and by the
relations of the plants to one another.[300] These natural groups are valuable
indications of the agricultural capabilities of the districts occupied by them.
They may be regarded as the outcome of Nature’s experiments in crop-
raising, running consecutively through thousands of years. They are natural
correlations of compatible members into communities of plants. Some
members of the society are obviously dependent on others, as certain forms
of undergrowth on the shadowing of the upper growth, as of vines upon
supporting-trees, etc. There is probably a more occult relation in some
cases, the effects of certain plants on the soil being sometimes advantageous
to other plants, and sometimes harmful, as illustrated in the conditions that
require a rotation of crops.
The chief point of geologic interest lies in the fact that floras are not mere
miscellaneous mixtures of plants that happen to live in a given area at a
given period, but are organized communities, in a more or less definite
sense. They therefore imply more or less definitely the physical conditions
which are congenial to them, and thus furnish the basis for interpreting such
conditions in the past, so far as the floras are well preserved. The faunas,
especially the land faunas, being primarily dependent on the floras, furnish
a basis for interpretations of like import.
B. The Influence of Geographic Conditions on the Evolution of
Floras and Faunas.
The geographic features of the earth impose on organisms a complex
series of influences which modify the evolution of life and produce faunal
and floral variation on a large scale. The larger assemblages of life, which
inhabit a continent or dwell in a great sea, are designated faunas and floras,
as well as the smaller assemblages just discussed, but obviously in a
broader and in a different sense. The disseverance of the land by the sea, or
of the sea by the land, isolates the life and forces independent development.
distinguish the xerophytes from the hydrophytes and mesophytes have
special geological interest, as they aid in determining the climatic
conditions, a feature whose interest increases as the variability of the
ancient climates is more fully recognized.
Within these greater groups there are special minor associations
determined by soil, temperature, topography, subjacent strata, and by the
relations of the plants to one another.[300] These natural groups are valuable
indications of the agricultural capabilities of the districts occupied by them.
They may be regarded as the outcome of Nature’s experiments in crop-
raising, running consecutively through thousands of years. They are natural
correlations of compatible members into communities of plants. Some
members of the society are obviously dependent on others, as certain forms
of undergrowth on the shadowing of the upper growth, as of vines upon
supporting-trees, etc. There is probably a more occult relation in some
cases, the effects of certain plants on the soil being sometimes advantageous
to other plants, and sometimes harmful, as illustrated in the conditions that
require a rotation of crops.
The chief point of geologic interest lies in the fact that floras are not mere
miscellaneous mixtures of plants that happen to live in a given area at a
given period, but are organized communities, in a more or less definite
sense. They therefore imply more or less definitely the physical conditions
which are congenial to them, and thus furnish the basis for interpreting such
conditions in the past, so far as the floras are well preserved. The faunas,
especially the land faunas, being primarily dependent on the floras, furnish
a basis for interpretations of like import.
B. The Influence of Geographic Conditions on the Evolution of
Floras and Faunas.
The geographic features of the earth impose on organisms a complex
series of influences which modify the evolution of life and produce faunal
and floral variation on a large scale. The larger assemblages of life, which
inhabit a continent or dwell in a great sea, are designated faunas and floras,
as well as the smaller assemblages just discussed, but obviously in a
broader and in a different sense. The disseverance of the land by the sea, or
of the sea by the land, isolates the life and forces independent development.
Page 757
The introduction of cold zones, desert tracts, or other potent climatic belts
has somewhat the same effect. So, measurably, does the raising of a
mountain range or a plateau, or the sinking of critical portions of the sea-
bottom.
The development of provincial and cosmopolitan faunas.[301]—If a
region is isolated from other regions by the cutting off of all ready means of
intermigration, as by the formation of an island from what had been a
peninsula, or of an inland sea from what had been a bay, the flora and fauna
are developed by themselves without much influx of other forms, and hence
become local or provincial. This is usually more marked in the case of the
fauna than of the flora, because the latter has more ample means of
dispersion, on the whole, and so the fauna may for convenience be taken as
the type. A good illustration is the native fauna of Australia which was once
connected with Asia, but has long been separated from it. Previous to
importations by man, this continent had a very peculiar and distinct fauna,
descended from its Mesozoic inhabitants. Most of the isolated islands have
peculiar faunas, but in many cases they were isolated from the beginning,
having been built up by volcanic action from the bottom of the sea, and
their faunas are due to the accidents of transportation and to the
development of these sporadic forms in isolation.[302]
It is evident that whenever any geographic change introduces a barrier to
migration, the faunas of the dissevered portions will, in all probability,
develop along different lines, and will diverge into provincial faunas. On
the other hand, any geographic change that unites areas and leads to
intermigration, tends to a community of fauna or to cosmopolitanism. These
tendencies have been markedly felt all through the geologic ages, and
constitute one of the most vital features of their history. When continents
are connected, their faunas intermingle and the exchange gives rise to
common forms. They tend to blend into one great fauna except so far as the
local differences develop those minor assemblages previously discussed.
When continents are separated, they tend to develop peculiar faunas, as do
islands, but on a larger scale. This is very obvious in the case of the land
life, but needs more special statement for the oceans.
The oceans constitute a single body of water with ample connections and
stirred by a system of constant circulation. Probably this has been true for
most of known geologic time. A single cosmopolitan fauna of the largest
has somewhat the same effect. So, measurably, does the raising of a
mountain range or a plateau, or the sinking of critical portions of the sea-
bottom.
The development of provincial and cosmopolitan faunas.[301]—If a
region is isolated from other regions by the cutting off of all ready means of
intermigration, as by the formation of an island from what had been a
peninsula, or of an inland sea from what had been a bay, the flora and fauna
are developed by themselves without much influx of other forms, and hence
become local or provincial. This is usually more marked in the case of the
fauna than of the flora, because the latter has more ample means of
dispersion, on the whole, and so the fauna may for convenience be taken as
the type. A good illustration is the native fauna of Australia which was once
connected with Asia, but has long been separated from it. Previous to
importations by man, this continent had a very peculiar and distinct fauna,
descended from its Mesozoic inhabitants. Most of the isolated islands have
peculiar faunas, but in many cases they were isolated from the beginning,
having been built up by volcanic action from the bottom of the sea, and
their faunas are due to the accidents of transportation and to the
development of these sporadic forms in isolation.[302]
It is evident that whenever any geographic change introduces a barrier to
migration, the faunas of the dissevered portions will, in all probability,
develop along different lines, and will diverge into provincial faunas. On
the other hand, any geographic change that unites areas and leads to
intermigration, tends to a community of fauna or to cosmopolitanism. These
tendencies have been markedly felt all through the geologic ages, and
constitute one of the most vital features of their history. When continents
are connected, their faunas intermingle and the exchange gives rise to
common forms. They tend to blend into one great fauna except so far as the
local differences develop those minor assemblages previously discussed.
When continents are separated, they tend to develop peculiar faunas, as do
islands, but on a larger scale. This is very obvious in the case of the land
life, but needs more special statement for the oceans.
The oceans constitute a single body of water with ample connections and
stirred by a system of constant circulation. Probably this has been true for
most of known geologic time. A single cosmopolitan fauna of the largest
Page 758
type might be expected. This is in a measure realized in the pelagic fauna of
the open ocean, though this is somewhat modified by the climatic zones.
But the marine faunas that are fossilized in the known strata, and have most
geologic interest, are, with rare exceptions, not those of the open ocean, but
those of the shore zones and of the shallow seas. Now, although these shore
belts and shallow seas are broadly connected with the great ocean body, and
are usually regarded as a part of it, they are singularly separated from it, or
rather they are singularly separated by it, so far as the life dependent on
shallow-water conditions is concerned. To this life, the deep sea is a barrier
not quite as effective as the land, but still a barrier. The key to this
important fact may be found in a consideration of the vertical distribution
of life.
The great horizon of life is at or near the contact zone of the atmosphere
with the hydrosphere and lithosphere. Life declines with increasing altitude,
partly because of the lowering temperature, and partly because of the
increasing tenuity of the atmosphere. The successive changes of plant and
animal life with the ascent of mountains and plateaus is familiar. Life
declines in descent into the sea chiefly from lack of light, and secondarily
from the lowering of temperature. Light is essential to the formation of
chlorophyll and, through it, of all other organic compounds. The
chlorophyll-forming plants are, therefore, limited to such depths as are
penetrated by the rays necessary for the photosynthesis of organic matter.
Vision is cut off within 200 to 300 feet, and most plant growth takes place
above that depth. Photographic effects become feeble or inappreciable at
1000 to 1200 feet.[303] The photosynthesis of plants is chiefly aided by the
lower and middle part of the spectrum, while the ordinary photographic
work is chiefly done by the upper end, so that the photographic limit is
below the photosynthetic limit. Microscopic plants are sometimes found
lower than these limits, but they may have been carried below their working
limits by currents or other incidental agencies. For all general purposes, the
limiting depth of living carbon-compounding plants may be set at 100
fathoms, as a generous figure—about the average depth of the border of the
continental shelf—while the vast majority flourish only in the upper third of
this depth.
Life does not cease here, for the products of this surface-life sink to
greater depths and are fed upon by forms of sea animals that have become
the open ocean, though this is somewhat modified by the climatic zones.
But the marine faunas that are fossilized in the known strata, and have most
geologic interest, are, with rare exceptions, not those of the open ocean, but
those of the shore zones and of the shallow seas. Now, although these shore
belts and shallow seas are broadly connected with the great ocean body, and
are usually regarded as a part of it, they are singularly separated from it, or
rather they are singularly separated by it, so far as the life dependent on
shallow-water conditions is concerned. To this life, the deep sea is a barrier
not quite as effective as the land, but still a barrier. The key to this
important fact may be found in a consideration of the vertical distribution
of life.
The great horizon of life is at or near the contact zone of the atmosphere
with the hydrosphere and lithosphere. Life declines with increasing altitude,
partly because of the lowering temperature, and partly because of the
increasing tenuity of the atmosphere. The successive changes of plant and
animal life with the ascent of mountains and plateaus is familiar. Life
declines in descent into the sea chiefly from lack of light, and secondarily
from the lowering of temperature. Light is essential to the formation of
chlorophyll and, through it, of all other organic compounds. The
chlorophyll-forming plants are, therefore, limited to such depths as are
penetrated by the rays necessary for the photosynthesis of organic matter.
Vision is cut off within 200 to 300 feet, and most plant growth takes place
above that depth. Photographic effects become feeble or inappreciable at
1000 to 1200 feet.[303] The photosynthesis of plants is chiefly aided by the
lower and middle part of the spectrum, while the ordinary photographic
work is chiefly done by the upper end, so that the photographic limit is
below the photosynthetic limit. Microscopic plants are sometimes found
lower than these limits, but they may have been carried below their working
limits by currents or other incidental agencies. For all general purposes, the
limiting depth of living carbon-compounding plants may be set at 100
fathoms, as a generous figure—about the average depth of the border of the
continental shelf—while the vast majority flourish only in the upper third of
this depth.
Life does not cease here, for the products of this surface-life sink to
greater depths and are fed upon by forms of sea animals that have become
Page 759
adapted to the dark and cold abyss of the ocean. Obviously, these deep-sea
forms are a very distinct type of life, and constitute a fauna of the most
pronounced kind, the abysmal fauna. Another distinct fauna occupies the
open-ocean surface, the pelagic fauna. Still a third fauna occupies the
shallow-water tract, whose bottom lies within the light zone—the
photobathic zone—and embraces the animals that are dependent on the
plants of this zone, or on its light and warmth, and that are more or less
fixed to the bottom or confined to the zone because their food is there.
The physical plane of demarkation between the surface or pelagic fauna
and the abysmal fauna is much more distinct and more fundamental than
any that is found in ascending above the surface of the sea. The habitat of
the shallow-water fauna is limited below by the darkness, limited above by
the water-surface, limited at one side by the land, and limited on the other
side by the deep sea. It is hemmed in vertically between two planes only a
few hundred feet apart. Laterally, it is confined to a narrow belt about the
borders of the continents and to the more or less land-girt epicontinental
seas. Its vertical limits are fixed, but its lateral extent varies with the
relations of the sea to the surface of the continental platforms.
This variation profoundly affects the development of the fauna. When a
major deformation of the earth takes place which increases the capacity of
the oceanic basins, the water is drawn down into them more fully, and
correspondingly retreats from the continental shelf. The shore is thus
carried out toward or to the border of the shelf, or even perhaps down to
some line on the abysmal slope. In either case, the zone of shallow water
suited to the photobathic life is narrowed, and at points it may be practically
cut in two. There are, however, shelves and tracts that were below the light
zone before, which now are brought within it by the lowering of the sea-
level. Into these, as into harbors of refuge, the life migrates so far as it may.
But these tracts are less prevalent and continuous than the typical
continental shelf, and under the conditions supposed they would be but
imperfectly connected with each other by available shallow-water tracts.
(The steep shelving shore tracts, although furnishing a shallow-water
connection possibly available for some species, would be unsuited to others
and, under certain conditions of the sea-currents, would be an effective
barrier.) To these limited tracts, therefore, the life of the photobathic type is
forms are a very distinct type of life, and constitute a fauna of the most
pronounced kind, the abysmal fauna. Another distinct fauna occupies the
open-ocean surface, the pelagic fauna. Still a third fauna occupies the
shallow-water tract, whose bottom lies within the light zone—the
photobathic zone—and embraces the animals that are dependent on the
plants of this zone, or on its light and warmth, and that are more or less
fixed to the bottom or confined to the zone because their food is there.
The physical plane of demarkation between the surface or pelagic fauna
and the abysmal fauna is much more distinct and more fundamental than
any that is found in ascending above the surface of the sea. The habitat of
the shallow-water fauna is limited below by the darkness, limited above by
the water-surface, limited at one side by the land, and limited on the other
side by the deep sea. It is hemmed in vertically between two planes only a
few hundred feet apart. Laterally, it is confined to a narrow belt about the
borders of the continents and to the more or less land-girt epicontinental
seas. Its vertical limits are fixed, but its lateral extent varies with the
relations of the sea to the surface of the continental platforms.
This variation profoundly affects the development of the fauna. When a
major deformation of the earth takes place which increases the capacity of
the oceanic basins, the water is drawn down into them more fully, and
correspondingly retreats from the continental shelf. The shore is thus
carried out toward or to the border of the shelf, or even perhaps down to
some line on the abysmal slope. In either case, the zone of shallow water
suited to the photobathic life is narrowed, and at points it may be practically
cut in two. There are, however, shelves and tracts that were below the light
zone before, which now are brought within it by the lowering of the sea-
level. Into these, as into harbors of refuge, the life migrates so far as it may.
But these tracts are less prevalent and continuous than the typical
continental shelf, and under the conditions supposed they would be but
imperfectly connected with each other by available shallow-water tracts.
(The steep shelving shore tracts, although furnishing a shallow-water
connection possibly available for some species, would be unsuited to others
and, under certain conditions of the sea-currents, would be an effective
barrier.) To these limited tracts, therefore, the life of the photobathic type is
Page 760
restricted and measurably isolated, and develops into local and provincial
faunas.
After a deforming movement has ceased, the seashore habitually
advances, developing a new continental shelf, and in time new
epicontinental gulfs and seas. In this it is assisted by the erosion of the
continent and the filling of the sea, and probably by the slow settling of the
continents. As the sea-shelf broadens, the isolated tracts, the harbors of
refuge, become connected, and migration is facilitated. When the
connection becomes general and broad, and when epicontinental seas have
formed available tracts across the face of the continents, a general
commingling of faunas follows, and a cosmopolitan fauna results.
In the same way, but more obviously, when the land is extended and
connection between the continents becomes general, there is migration and
commingling of the land faunas and floras, and cosmopolitan communities
are the result.
It is obvious that the development on the land is the reciprocal of that in
the sea. When the seas are extended and their life is tending toward
cosmopolitanism, the lands are dissevered, and their life is tending toward
provincialism, and vice versa. When, however, the land is greatly extended,
it is usually accentuated by mountain ranges, and other products of the
deformation which extended it, and these form barriers. Desert wastes and
other inhospitable tracts, and even glaciation, are liable to develop as
secondary consequences, and to interpose barriers, and hence the
cosmopolitanism of the land-life is liable to be less complete than that of
the sea-life.
Restrictive and expansional evolution.—It is obvious from the last
discussion that if the picture of the earth’s movement above drawn be true,
the areas available for particular classes of life may vary greatly from age to
age. At times the shallow-water sea-life may be forced to retreat into a very
narrow tract on the border of the land, and into chance expansions here and
there. In being crowded into this limited tract, perhaps also less adapted for
a habitat on account of the change, the life is subjected to severe
competition and to hard conditions, and must experience in an intensified
degree the effects of the struggle for existence. Whatever of evolutionary
faunas.
After a deforming movement has ceased, the seashore habitually
advances, developing a new continental shelf, and in time new
epicontinental gulfs and seas. In this it is assisted by the erosion of the
continent and the filling of the sea, and probably by the slow settling of the
continents. As the sea-shelf broadens, the isolated tracts, the harbors of
refuge, become connected, and migration is facilitated. When the
connection becomes general and broad, and when epicontinental seas have
formed available tracts across the face of the continents, a general
commingling of faunas follows, and a cosmopolitan fauna results.
In the same way, but more obviously, when the land is extended and
connection between the continents becomes general, there is migration and
commingling of the land faunas and floras, and cosmopolitan communities
are the result.
It is obvious that the development on the land is the reciprocal of that in
the sea. When the seas are extended and their life is tending toward
cosmopolitanism, the lands are dissevered, and their life is tending toward
provincialism, and vice versa. When, however, the land is greatly extended,
it is usually accentuated by mountain ranges, and other products of the
deformation which extended it, and these form barriers. Desert wastes and
other inhospitable tracts, and even glaciation, are liable to develop as
secondary consequences, and to interpose barriers, and hence the
cosmopolitanism of the land-life is liable to be less complete than that of
the sea-life.
Restrictive and expansional evolution.—It is obvious from the last
discussion that if the picture of the earth’s movement above drawn be true,
the areas available for particular classes of life may vary greatly from age to
age. At times the shallow-water sea-life may be forced to retreat into a very
narrow tract on the border of the land, and into chance expansions here and
there. In being crowded into this limited tract, perhaps also less adapted for
a habitat on account of the change, the life is subjected to severe
competition and to hard conditions, and must experience in an intensified
degree the effects of the struggle for existence. Whatever of evolutionary
Page 761
potency there may be in such a struggle under such restrictive conditions
should be revealed in the modifications of the fauna that ensued.
On the other hand, when the shallow seas are generally extending
themselves upon the land and the land is being base-leveled, and thus
adapted to shallow submergence, the shallow-water life enjoys an enlarging
realm, and should reveal the effects of evolution under expansional
conditions. In affording a comparison between these opposite and
alternating phases of restrictional and expansional evolution, geology
makes one of its great contributions to the external causes and conditions of
organic evolution. These will come under repeated consideration in the
historical chapters.
should be revealed in the modifications of the fauna that ensued.
On the other hand, when the shallow seas are generally extending
themselves upon the land and the land is being base-leveled, and thus
adapted to shallow submergence, the shallow-water life enjoys an enlarging
realm, and should reveal the effects of evolution under expansional
conditions. In affording a comparison between these opposite and
alternating phases of restrictional and expansional evolution, geology
makes one of its great contributions to the external causes and conditions of
organic evolution. These will come under repeated consideration in the
historical chapters.
Page 762
INDEX.
VOLUME I.
Abbot, M. L. (and Humphreys, A. A.), 106, 202
Abrasion,
by ice, 281
by streams, 119
by waves, 342
by wind, 38
Abysmal fauna, 671
Abysmal sea, 326
Accretion hypothesis,
internal temperature on, 564, 567
recombination of material on, 568
Actinolite, 447, 460
Adams, F. D., 474
Adjustment of streams,
structural, 146, 150
topographic, 162, 163, 197
Adobe, 467
Agassiz, 366, 604
Agassiz, L., 321, 322, 323, 366
Agate, 460
Agate structure, 436
Agglomerate, 434, 467
Aggradation,
by ice, 298
by streams, 2, 177
VOLUME I.
Abbot, M. L. (and Humphreys, A. A.), 106, 202
Abrasion,
by ice, 281
by streams, 119
by waves, 342
by wind, 38
Abysmal fauna, 671
Abysmal sea, 326
Accretion hypothesis,
internal temperature on, 564, 567
recombination of material on, 568
Actinolite, 447, 460
Adams, F. D., 474
Adjustment of streams,
structural, 146, 150
topographic, 162, 163, 197
Adobe, 467
Agassiz, 366, 604
Agassiz, L., 321, 322, 323, 366
Agate, 460
Agate structure, 436
Agglomerate, 434, 467
Aggradation,
by ice, 298
by streams, 2, 177
Page 763
by wind, 25
in sea, 333, 355
Aggrading streams, characteristics, 179, 187
Airy, Sir G., 341
Alabaster, 460
Albite, 400, 460
Alferric rocks, 454
Algæ,
geologic contribution of, 653
influence on precipitation, 225
Alkalicalcic rocks, 458
Alluvial cone, 181–3
growth, 181
levees, 182
Alluvial deposits, 177–96
Alluvial fans, 181–3
Alluvial plains, 181, 184–96
material of, 196
origin of, 184, 185
piedmont, 183
topography of, 196
Alluviation, 181, 196, 467
ill-defined, 183
Alpine glaciers, 251
Alps,
crustal shortening involved in formation of, 549, 576
structure, 504, 507
Amber, 646
Amethyst, 460
Amphibole, 460
Amphiboles, 400
Amygdaloid, 411, 467
in sea, 333, 355
Aggrading streams, characteristics, 179, 187
Airy, Sir G., 341
Alabaster, 460
Albite, 400, 460
Alferric rocks, 454
Algæ,
geologic contribution of, 653
influence on precipitation, 225
Alkalicalcic rocks, 458
Alluvial cone, 181–3
growth, 181
levees, 182
Alluvial deposits, 177–96
Alluvial fans, 181–3
Alluvial plains, 181, 184–96
material of, 196
origin of, 184, 185
piedmont, 183
topography of, 196
Alluviation, 181, 196, 467
ill-defined, 183
Alpine glaciers, 251
Alps,
crustal shortening involved in formation of, 549, 576
structure, 504, 507
Amber, 646
Amethyst, 460
Amphibole, 460
Amphiboles, 400
Amygdaloid, 411, 467
Page 764
Analcite, 460
Analyses,
American river-waters, 107
American spring-waters, 235
rain-waters, 107
river-waters, 106, 107, 108
sea-water, 324
waters of enclosed lakes, 392
Anamorphism, 446
Andalusite, 460
Andes, snow-line in, 246
Andesine, 400, 460
Andesite, 467
Angiosperms, 657
Anhydrite, 460
Animal kingdom,
geologic contribution of, 658–63
synopsis of, 659
Anorthite, 460
Anorthosite, 467
Antarctica, snow-line in, 246
Antecedent streams, 169, 173
Anthracite, 426, 460
Anticlinal valleys, 159
Anticline, 504
plunging, 155, 157, 506
Anticlinoria, 504
Antimony, 460
Apatite, 460
Aphanite, 451, 452, 467
Aplite, 415
Analyses,
American river-waters, 107
American spring-waters, 235
rain-waters, 107
river-waters, 106, 107, 108
sea-water, 324
waters of enclosed lakes, 392
Anamorphism, 446
Andalusite, 460
Andes, snow-line in, 246
Andesine, 400, 460
Andesite, 467
Angiosperms, 657
Anhydrite, 460
Animal kingdom,
geologic contribution of, 658–63
synopsis of, 659
Anorthite, 460
Anorthosite, 467
Antarctica, snow-line in, 246
Antecedent streams, 169, 173
Anthracite, 426, 460
Anticlinal valleys, 159
Anticline, 504
plunging, 155, 157, 506
Anticlinoria, 504
Antimony, 460
Apatite, 460
Aphanite, 451, 452, 467
Aplite, 415
Page 765
Appalachian Riser, 173
Appalachians,
crustal shortening due to folding, 549
extent of piracy in, 169
peculiarities of drainage, 169
rejuvenation of streams in, 165
stream adjustment in, 147
Aqueous rocks, 467
Aragonite, 460
Archean complex, 18
Arch of earth’s crust, strength of, 582
Archeozoic era, 19
Arenaceous rocks, 468
Arid regions, erosion in, 131
Argillite, 448, 468
Arkose, 422, 468, 645
Artesian wells, 242
Arthropoda, geologic contribution of, 662
Asiderites, 5
Asphaltum, 460
Asteroids, 661
Astronomic geology, 1, 2
Atlantic coastal plain, 587
Atmosphere, 5
affected by life, 639, 640
carbonation by, 43
chemical work of, 41–43
evaporation and precipitation, 50
fluctuations in composition, 639–44
geologic activity of, 6, 21–43
mass and extent, 6
mechanical work of, 21–41
Appalachians,
crustal shortening due to folding, 549
extent of piracy in, 169
peculiarities of drainage, 169
rejuvenation of streams in, 165
stream adjustment in, 147
Aqueous rocks, 467
Aragonite, 460
Archean complex, 18
Arch of earth’s crust, strength of, 582
Archeozoic era, 19
Arenaceous rocks, 468
Arid regions, erosion in, 131
Argillite, 448, 468
Arkose, 422, 468, 645
Artesian wells, 242
Arthropoda, geologic contribution of, 662
Asiderites, 5
Asphaltum, 460
Asteroids, 661
Astronomic geology, 1, 2
Atlantic coastal plain, 587
Atmosphere, 5
affected by life, 639, 640
carbonation by, 43
chemical work of, 41–43
evaporation and precipitation, 50
fluctuations in composition, 639–44
geologic activity of, 6, 21–43
mass and extent, 6
mechanical work of, 21–41
Page 766
oxidation by, 42
thermal effects of, 7
Atmospheric electricity, 43, 52
Atmospheric precipitation, amount of, 51
Augite, 400, 429, 461
Augitite, 468
Autoclastic rock, 444
Australia, fauna of, 668
Babb, C. C., 107
Bad-lands, 93, 130
Badger Mountain, 231
Bain, H. F., 67, 474
Barbadoes earth, 661
Barite, 461
Barrier, the, 356
Bars, 181, 357
Barus, Carl, 562, 563
Basalt, 417, 452, 468
Basaltic columns, 417
Base-level, 60, 62, 82, 168
Cretaceous, 169
Kiltatinny, 168
temporary, 84
Basement complex, 18
Batholiths, 500, 592
Bayou, 192
Bayou lakes, 193
Bays, origin of, 331, 332
Beach, the, 355
thermal effects of, 7
Atmospheric electricity, 43, 52
Atmospheric precipitation, amount of, 51
Augite, 400, 429, 461
Augitite, 468
Autoclastic rock, 444
Australia, fauna of, 668
Babb, C. C., 107
Bad-lands, 93, 130
Badger Mountain, 231
Bain, H. F., 67, 474
Barbadoes earth, 661
Barite, 461
Barrier, the, 356
Bars, 181, 357
Barus, Carl, 562, 563
Basalt, 417, 452, 468
Basaltic columns, 417
Base-level, 60, 62, 82, 168
Cretaceous, 169
Kiltatinny, 168
temporary, 84
Basement complex, 18
Batholiths, 500, 592
Bayou, 192
Bayou lakes, 193
Bays, origin of, 331, 332
Beach, the, 355
Page 767
Beauxite, 461
Beck, R., 474
Becker, G. F., 474
Bergschrund, 258
Bertin, 323
Beryl, 461
Bighorn Mountains, lateral moraines in, 302
Biotite, 400, 461
Bischoff, Gustav, 108
Bismuth, 461
“Bittern,” 377
Bitumen, 461
Bituminous coal, 426, 468
Blake, W. P., 474
Blanford, W. T., 28, 203
Blood rain, 25
Blue mud, 380
Bone beds, 663
Bonneville lake, 360
Bonneville shore, 352
Bottom-set beds, 202
Bowlders, 468
Brachiopods, geologic contributions of, 662
Brahmaputra delta, 203
Branner, J. C., 489
Breakers, 341
force of, 344
Breccia, 423, 434, 468
Britannare, 459
Bronzite, 461
Beck, R., 474
Becker, G. F., 474
Bergschrund, 258
Bertin, 323
Beryl, 461
Bighorn Mountains, lateral moraines in, 302
Biotite, 400, 461
Bischoff, Gustav, 108
Bismuth, 461
“Bittern,” 377
Bitumen, 461
Bituminous coal, 426, 468
Blake, W. P., 474
Blanford, W. T., 28, 203
Blood rain, 25
Blue mud, 380
Bone beds, 663
Bonneville lake, 360
Bonneville shore, 352
Bottom-set beds, 202
Bowlders, 468
Brachiopods, geologic contributions of, 662
Brahmaputra delta, 203
Branner, J. C., 489
Breakers, 341
force of, 344
Breccia, 423, 434, 468
Britannare, 459
Bronzite, 461
Page 768
Bryozoans, geologic contributions of, 662
Buckley, E. R., 48, 50, 221
Buhrstone, 468
Burton (and Milne, J.), 636
Buttes, 142
Bysmaliths, 500, 592
Calcareous springs, 235
Calcareous tufa, 390
Calcimiric rocks, 458
Calcite, 461
Calc-sinter, 468
Calumet and Hecla mine, temperature in, 569
Calvin, S., 88, 204, 373, 389
Campbell, M. R., 167, 171, 173
Camphene, 646
Cannel coal, 468
Canoe-shaped valleys, 155
Canyons, 94–100
Colorado, 98, 233
Niagara, 99
Yellowstone, 100
Carbonation, 43, 429
Carbon dioxide,
amount in air, 5, 640
and plant-life, 665
climatic effects of, 643
loss of, 640
supply of, 618, 640
Cascade, 264
Cassiterite, 461
Buckley, E. R., 48, 50, 221
Buhrstone, 468
Burton (and Milne, J.), 636
Buttes, 142
Bysmaliths, 500, 592
Calcareous springs, 235
Calcareous tufa, 390
Calcimiric rocks, 458
Calcite, 461
Calc-sinter, 468
Calumet and Hecla mine, temperature in, 569
Calvin, S., 88, 204, 373, 389
Campbell, M. R., 167, 171, 173
Camphene, 646
Cannel coal, 468
Canoe-shaped valleys, 155
Canyons, 94–100
Colorado, 98, 233
Niagara, 99
Yellowstone, 100
Carbonation, 43, 429
Carbon dioxide,
amount in air, 5, 640
and plant-life, 665
climatic effects of, 643
loss of, 640
supply of, 618, 640
Cascade, 264
Cassiterite, 461
Page 769
Catlinite, 461
Causes of crustal movement, 551–557
Caverns (see Caves)
Caves, 143, 227–231
deposits in, 228
Mammoth, 227
sea, 350
Wyandotte, 227
Cazin, F. M. F., 474
Cementation,
effected through chemical precipitation, 222, 225, 226
effected through evaporation, 42
Cephalopods, geologic contributions of, 662
Chalcedony, 461
Chalk, 468, 660
Challenger deep, 587, 588
Chalybeate springs, 235
Chamberlin, T. C., 23, 242, 256, 322, 477, 565, 668
Changes of level, 537–551
caused by earthquakes, 536
causes of, 551–557
effect on drainage, 161
sea versus land, 538
Changes of temperature,
conditions affecting, 45
effect on rocks, 44, 49
internal (see Internal temperatures)
Charleston earthquake, 530
Chatter marks, 284
Chemical combination, cause of crustal movement, 556
Chemical deposits, 222–26
in deep sea, 383
in lakes, 391
Causes of crustal movement, 551–557
Caverns (see Caves)
Caves, 143, 227–231
deposits in, 228
Mammoth, 227
sea, 350
Wyandotte, 227
Cazin, F. M. F., 474
Cementation,
effected through chemical precipitation, 222, 225, 226
effected through evaporation, 42
Cephalopods, geologic contributions of, 662
Chalcedony, 461
Chalk, 468, 660
Challenger deep, 587, 588
Chalybeate springs, 235
Chamberlin, T. C., 23, 242, 256, 322, 477, 565, 668
Changes of level, 537–551
caused by earthquakes, 536
causes of, 551–557
effect on drainage, 161
sea versus land, 538
Changes of temperature,
conditions affecting, 45
effect on rocks, 44, 49
internal (see Internal temperatures)
Charleston earthquake, 530
Chatter marks, 284
Chemical combination, cause of crustal movement, 556
Chemical deposits, 222–26
in deep sea, 383
in lakes, 391
Page 770
in shallow sea, 374–378
Chemical work of atmosphere, 41–43
Chemical work of life, 638–46
Chert, 426, 468
Chiastolite, 461
Chimney rocks, 350
Chlorite, 461
Chlorite schist, 468
Chloritic rock, 431
Chromite, 461
Chrysolite, 462
Chrysotile, 462
Cinder-cones, 608
Cinders, 405
Cirques, 286
Clarke, F. W., 396, 573
Classification of rocks, 449
new system of, 451
Clastic rock, 468
Clay, 468
Clay ironstone, 468
Claypole, E. W., 549
Cleavage planes and erosion, 125
development of (see Slate and Schist)
Cliff glacier, 256
Climate, influence on erosion, 127–132
Climatic effects of carbon dioxide, 643
Climatic effects of life, 643
Climatic effects of water vapor, 643
Clinkstone, 468
Chemical work of atmosphere, 41–43
Chemical work of life, 638–46
Chert, 426, 468
Chiastolite, 461
Chimney rocks, 350
Chlorite, 461
Chlorite schist, 468
Chloritic rock, 431
Chromite, 461
Chrysolite, 462
Chrysotile, 462
Cinder-cones, 608
Cinders, 405
Cirques, 286
Clarke, F. W., 396, 573
Classification of rocks, 449
new system of, 451
Clastic rock, 468
Clay, 468
Clay ironstone, 468
Claypole, E. W., 549
Cleavage planes and erosion, 125
development of (see Slate and Schist)
Cliff glacier, 256
Climate, influence on erosion, 127–132
Climatic effects of carbon dioxide, 643
Climatic effects of life, 643
Climatic effects of water vapor, 643
Clinkstone, 468
Page 771
Clinometer, 501
Coal, 468
Coast-lines 353, 363–6
effect of gradation on, 333, 363
effect of subsidence on, 329, 332
effect of vulcanism on, 332–33
forms of, 329, 333, 363, 364
Coast ranges, crustal, shortening due to folding of, 549
Coasts, natural bridges on, 351
Cobb, C., 36
Cœlenterata, geologic contribution of, 661
Collins, A. L., 474
Colorado, Canyon of, 98, 233
Columbia River, 171
Columnar structure, 498–500
effect on weathering, 153, 154
Common springs, 235
Compression joints, 514
Concave tracts of crust, 585, 586
Concretions, 438, 468, 490
Cones,
cinder, 608
composite, 610
formation of, 608
geyser, 237
lava, 608
spatter, 610
tufa, 611
Configuration of coasts, 329, 330, 331, 332, 333, 353, 363–6
Conformability, 15
Conglomerate, 423, 434, 468, 487
Continental glaziers, 251
Coal, 468
Coast-lines 353, 363–6
effect of gradation on, 333, 363
effect of subsidence on, 329, 332
effect of vulcanism on, 332–33
forms of, 329, 333, 363, 364
Coast ranges, crustal, shortening due to folding of, 549
Coasts, natural bridges on, 351
Cobb, C., 36
Cœlenterata, geologic contribution of, 661
Collins, A. L., 474
Colorado, Canyon of, 98, 233
Columbia River, 171
Columnar structure, 498–500
effect on weathering, 153, 154
Common springs, 235
Compression joints, 514
Concave tracts of crust, 585, 586
Concretions, 438, 468, 490
Cones,
cinder, 608
composite, 610
formation of, 608
geyser, 237
lava, 608
spatter, 610
tufa, 611
Configuration of coasts, 329, 330, 331, 332, 333, 353, 363–6
Conformability, 15
Conglomerate, 423, 434, 468, 487
Continental glaziers, 251
Page 772
Continental platforms, 11
relief of, 11
Continental segments, size of, 547
Continental shelf, 11
Continent-forming movements, 544
Contour interval, 31
Contour lines, 31
Convection hypothesis,
internal heat on, 559
thermal distribution on, 559
Cooley, E. G., 195
Coon Butte, 596
Copalite, 646
Coprolites, 646
Coquina, 469
Coral mud, 380
Cornish, V., 26, 28, 29
Corrasion, 110, 113
by glaciers, 281–86
by streams, 119
by waves, 342–49
by wind, 38
effect of sediment on, 120
Corthell, E. L., 202
Cosmopolitan faunas, 668
Coulter, J. M., 667
Coves, 143
Cowles, H. C., 35, 667
Credner, H., 35, 538
Creep, 231
Cretaceous base-level, 169
relief of, 11
Continental segments, size of, 547
Continental shelf, 11
Continent-forming movements, 544
Contour interval, 31
Contour lines, 31
Convection hypothesis,
internal heat on, 559
thermal distribution on, 559
Cooley, E. G., 195
Coon Butte, 596
Copalite, 646
Coprolites, 646
Coquina, 469
Coral mud, 380
Cornish, V., 26, 28, 29
Corrasion, 110, 113
by glaciers, 281–86
by streams, 119
by waves, 342–49
by wind, 38
effect of sediment on, 120
Corthell, E. L., 202
Cosmopolitan faunas, 668
Coulter, J. M., 667
Coves, 143
Cowles, H. C., 35, 667
Credner, H., 35, 538
Creep, 231
Cretaceous base-level, 169
Page 773
Crevasses, 264
Crinoids, 661
Croll, James, 322, 323, 339
Crosby, W. O., 513
Cross-bedding, 373, 487
Cross-currents, in streams, 117
Cross, Whitman, 412, 451, 535, 573
Croton River, material in solution in, 108
Crustal movements, 526–589
causes of, 551–57
differential extent of, 548
due to chemical changes, 556
due to cohesion and crystallization, 554
due to diffusion, 555
earthquake, 527–33
minute and rapid, 526
periodicity of, 517, 539
resistance to, 557
slow and massive, 537–59
Crustal shortening, 548–51
Crust of earth, 13
depth of, 14
varieties of rock in, 14
Crystalline rocks, types of, 16
Crystallites, 407
Crystallization of lava, 401–2
stages of, 403
Crystals, enlargement of, 435
Cut-and-fill, 190, 193
Cut-off, 191
Cycle of erosion,
its stages, 80
definition of, 82
Crinoids, 661
Croll, James, 322, 323, 339
Crosby, W. O., 513
Cross-bedding, 373, 487
Cross-currents, in streams, 117
Cross, Whitman, 412, 451, 535, 573
Croton River, material in solution in, 108
Crustal movements, 526–589
causes of, 551–57
differential extent of, 548
due to chemical changes, 556
due to cohesion and crystallization, 554
due to diffusion, 555
earthquake, 527–33
minute and rapid, 526
periodicity of, 517, 539
resistance to, 557
slow and massive, 537–59
Crustal shortening, 548–51
Crust of earth, 13
depth of, 14
varieties of rock in, 14
Crystalline rocks, types of, 16
Crystallites, 407
Crystallization of lava, 401–2
stages of, 403
Crystals, enlargement of, 435
Cut-and-fill, 190, 193
Cut-off, 191
Cycle of erosion,
its stages, 80
definition of, 82
Page 774
recognition of, 164
Cystoids, 661
Dacite, 469
Dale, T. N., 505
Daly, R. A., 631
Dana, J. D., 203, 340, 349, 511, 543, 604, 636
Daniell, A., 572, 573
Danube River,
delta of, 202
material in solution in, 108
sediment carried by, 107
Darton, N. H., 41, 50, 53, 94, 135, 154, 494, 570
Darwin, C., 604, 636, 665
Darwin, G. H., 534, 561, 576, 579, 583, 604
Daubree, G. A., 626
Davis, B. M., 225
Davis, W. M., 83, 159, 164, 170, 188, 202, 204 210 349,
and Shaler, N. S., 256
Davis, C. A., 655
Davison, C., 527, 538, 561
DeBeaumont, Eli, 323
Decarbonation, 429, 430
DeCharpentier, J., 321, 322, 323
Deeley, R. M., 322
Deep-sea deposits, 368, 378–86
chemical, 383–86
extra-terrestrial, 381
inorganic, 380
manganiferous, 384
organic, 382
Cystoids, 661
Dacite, 469
Dale, T. N., 505
Daly, R. A., 631
Dana, J. D., 203, 340, 349, 511, 543, 604, 636
Daniell, A., 572, 573
Danube River,
delta of, 202
material in solution in, 108
sediment carried by, 107
Darton, N. H., 41, 50, 53, 94, 135, 154, 494, 570
Darwin, C., 604, 636, 665
Darwin, G. H., 534, 561, 576, 579, 583, 604
Daubree, G. A., 626
Davis, B. M., 225
Davis, W. M., 83, 159, 164, 170, 188, 202, 204 210 349,
and Shaler, N. S., 256
Davis, C. A., 655
Davison, C., 527, 538, 561
DeBeaumont, Eli, 323
Decarbonation, 429, 430
DeCharpentier, J., 321, 322, 323
Deeley, R. M., 322
Deep-sea deposits, 368, 378–86
chemical, 383–86
extra-terrestrial, 381
inorganic, 380
manganiferous, 384
organic, 382
Page 775
Deep-sea fauna, 670
Deposition,
by glaciers, 298–305
by streams, 177–204
by shore currents, 355
by undertow, 355
by waves, 355–63
by wind, 25–37
Deformation of earth’s crust, 526–89
causes of, 551–57, 574–89
relation to distribution of volcanoes, 601, 604, 627, 629
Deformation of ice, 312
Degradation, 2
by water, 58–177
rate of, 105
De Launay, L. C., 474
Delesse, A., 221, 341
Delessite, 462
Dells of the Wisconsin, 152
Delta lakes, 204
Deltas, 181, 198–204
bottom set beds, 202
development, 199
fore-set beds, 202
fossil, 203
in tidal seas, 202
of the Ganges and Brahmaputra, 202
of the Hoang-Ho, 202, 203
of the Mackenzie, 202
of the Mississippi, 197, 202
of the Nile, 202
of the Po, 202
of the Rhone, 203
of the Yukon, 202
Deposition,
by glaciers, 298–305
by streams, 177–204
by shore currents, 355
by undertow, 355
by waves, 355–63
by wind, 25–37
Deformation of earth’s crust, 526–89
causes of, 551–57, 574–89
relation to distribution of volcanoes, 601, 604, 627, 629
Deformation of ice, 312
Degradation, 2
by water, 58–177
rate of, 105
De Launay, L. C., 474
Delesse, A., 221, 341
Delessite, 462
Dells of the Wisconsin, 152
Delta lakes, 204
Deltas, 181, 198–204
bottom set beds, 202
development, 199
fore-set beds, 202
fossil, 203
in tidal seas, 202
of the Ganges and Brahmaputra, 202
of the Hoang-Ho, 202, 203
of the Mackenzie, 202
of the Mississippi, 197, 202
of the Nile, 202
of the Po, 202
of the Rhone, 203
of the Yukon, 202
Page 776
rate of growth, 202
shape, 201
structure, 198, 199
top-set beds, 202
Densities within the earth, on Laplace’s law, 564
Denudation and volcanic action, 627
Deoxidation, 427
Deposition of mineral matter from solution, 50, 225, 428
at surface, 50, 224
by ground-water, 224, 428
in lakes, 387
in sea, 375, 383
Deposition of sediment, 66
by rivers, 177–204
by wind, 25–38
in ocean, 355–63, 368–86
Deposition of drift, at edge of glaciers, 299
at end glaciers 299
beneath ice, 298
Deposits,
deep-sea, 368, 378–86
hot springs, 237, 241
lacustrine, 387
littoral, 369
made by animals, 658–63
made by Arthropoda, 662
made by Bryophytes, 656
made by Echinodermata, 661
made by ice, 298–305
made by Mollusca, 662
made by Molluscoidea, 662
made by Protozoa, 660
made by Pteridophytes, 657
made by plant kingdom, 652–58
made by rivers, 177–204
shape, 201
structure, 198, 199
top-set beds, 202
Densities within the earth, on Laplace’s law, 564
Denudation and volcanic action, 627
Deoxidation, 427
Deposition of mineral matter from solution, 50, 225, 428
at surface, 50, 224
by ground-water, 224, 428
in lakes, 387
in sea, 375, 383
Deposition of sediment, 66
by rivers, 177–204
by wind, 25–38
in ocean, 355–63, 368–86
Deposition of drift, at edge of glaciers, 299
at end glaciers 299
beneath ice, 298
Deposits,
deep-sea, 368, 378–86
hot springs, 237, 241
lacustrine, 387
littoral, 369
made by animals, 658–63
made by Arthropoda, 662
made by Bryophytes, 656
made by Echinodermata, 661
made by ice, 298–305
made by Mollusca, 662
made by Molluscoidea, 662
made by Protozoa, 660
made by Pteridophytes, 657
made by plant kingdom, 652–58
made by rivers, 177–204
Page 777
made by Spermatophytes, 657
made by Thallophytes, 653
made by Vermes, 662
made by Vertebrata, 663
made by wind, 25–38
shallow-water, 369–78
silicious, 237, 241, 425
tufa, 237, 241, 473, 611, 653
Depression and volcanic action, 629
Depth of the ocean, 7
greatest, 8, 548
Diabases, 418, 431, 469
Diallage, 400, 462
Diastrophism, 2, 329, 526
effect on coast lines, 329
Diatom ooze, 380, 382, 425, 469
Diffusion,
in earth’s interior, 555
cause of crustal movement, 555
Dikes, 591
effect on topography, 143
sandstone, 514
Diller, J. S., 29, 514
Diorites, 416, 452, 469
Dip, 501
quaquaversal, 504
Dip-fault, 522
DiRossi, M. S., 537
Displacement of fault, 514
Disruption of rock, due to changes of temperature, 44, 49
by carbonation, 43
by hydration, 111
Distributive fault, 519
made by Thallophytes, 653
made by Vermes, 662
made by Vertebrata, 663
made by wind, 25–38
shallow-water, 369–78
silicious, 237, 241, 425
tufa, 237, 241, 473, 611, 653
Depression and volcanic action, 629
Depth of the ocean, 7
greatest, 8, 548
Diabases, 418, 431, 469
Diallage, 400, 462
Diastrophism, 2, 329, 526
effect on coast lines, 329
Diatom ooze, 380, 382, 425, 469
Diffusion,
in earth’s interior, 555
cause of crustal movement, 555
Dikes, 591
effect on topography, 143
sandstone, 514
Diller, J. S., 29, 514
Diorites, 416, 452, 469
Dip, 501
quaquaversal, 504
Dip-fault, 522
DiRossi, M. S., 537
Displacement of fault, 514
Disruption of rock, due to changes of temperature, 44, 49
by carbonation, 43
by hydration, 111
Distributive fault, 519
Page 778
Divides, permanence of, 69
Docalcic rocks, 458
Dodge, R. E., 204
Dofemane, 455
Dofemic rocks, 454
Doferrous rocks, 459
Dohemic rocks, 457
Dolenic rocks, 456
Dolerites, 417, 452, 469
Dolomites, 424, 469
Domagnesic rocks, 459
Domalkalic rocks, 458
Domes of crust, strength of, 581, 582
Domilic rocks, 582
Domiric rocks, 458
Domirlic rocks, 458
Domitic rocks, 457
Dopolic rocks, 456
Dopotassic rocks, 458
Dopyric rocks, 457
Doquaric rocks, 456
Dosalic rocks, 454
Dosodic rocks, 458
Dotilic rocks, 457
Drainage,
effect of change of level on, 161
mature, 86
of glaciers, 273
old age, 89
youthful, 86
Dreikanter, 40
Docalcic rocks, 458
Dodge, R. E., 204
Dofemane, 455
Dofemic rocks, 454
Doferrous rocks, 459
Dohemic rocks, 457
Dolenic rocks, 456
Dolerites, 417, 452, 469
Dolomites, 424, 469
Domagnesic rocks, 459
Domalkalic rocks, 458
Domes of crust, strength of, 581, 582
Domilic rocks, 582
Domiric rocks, 458
Domirlic rocks, 458
Domitic rocks, 457
Dopolic rocks, 456
Dopotassic rocks, 458
Dopyric rocks, 457
Doquaric rocks, 456
Dosalic rocks, 454
Dosodic rocks, 458
Dotilic rocks, 457
Drainage,
effect of change of level on, 161
mature, 86
of glaciers, 273
old age, 89
youthful, 86
Dreikanter, 40
Page 779
Drift, 287, 469
composition of, 304
deposition of, 298–305
wear of, in transit, 298
Drygalski, E. von, 322
Dump moraine, 301
Dune areas, topography of, 32
Dunes, 24–37
distribution of, 35
effect of vegetation on, 29
formation of, 26
migration of, 33
shapes of, 26
slopes of, 29
Dust,
volcanic, 22, 23
wind-blown, 22
Dust-wells, 269, 280
Dutton, C. E., 132, 534, 574, 636
Dynamic geology, 1
Earth, the,
as a planet, 2
constitution, 5
crust, 13
deformation of, 526
dependence on sun, 4
distance from sun, 3
inclination of axis, 3
interior of, 14, 559
internal heat, 559–74
motions, 3
orbit, 3
tremors of surface, 526
composition of, 304
deposition of, 298–305
wear of, in transit, 298
Drygalski, E. von, 322
Dump moraine, 301
Dune areas, topography of, 32
Dunes, 24–37
distribution of, 35
effect of vegetation on, 29
formation of, 26
migration of, 33
shapes of, 26
slopes of, 29
Dust,
volcanic, 22, 23
wind-blown, 22
Dust-wells, 269, 280
Dutton, C. E., 132, 534, 574, 636
Dynamic geology, 1
Earth, the,
as a planet, 2
constitution, 5
crust, 13
deformation of, 526
dependence on sun, 4
distance from sun, 3
inclination of axis, 3
interior of, 14, 559
internal heat, 559–74
motions, 3
orbit, 3
tremors of surface, 526
Page 780
warpings of crust, 526–89
Earthquakes, 527–537
causes of, 527
destruction of life by, 536
distribution of, 533
destructive effects of, 530
epicentra of, 531
foci of, 527
gaseous emanations during, 533
geologic effects of, 534–537
Earthquake vibrations, 526
amplitude of, 529
Charleston, 534
Lisbon, 535
sequences of, 533
Earth’s crust,
composition of, 14, 396
warpings of, 538–551
Eastman, C. R., 658
Echinodermata, geologic contributions of, 661
Echinoids, geologic contributions of, 661
Economic geology, 1
Efflorescence, 42
Elæolite, 462
Electricity,
atmospheric, 43
chemical effects of, 43
geological effects of, 43, 52
Ells, R., 443
Emmons, S. F., 474
Emmons, W. H., 474, 573, 585
Englacial drift, 282
Enlargement of crystals, by secondary growth, 435
Earthquakes, 527–537
causes of, 527
destruction of life by, 536
distribution of, 533
destructive effects of, 530
epicentra of, 531
foci of, 527
gaseous emanations during, 533
geologic effects of, 534–537
Earthquake vibrations, 526
amplitude of, 529
Charleston, 534
Lisbon, 535
sequences of, 533
Earth’s crust,
composition of, 14, 396
warpings of, 538–551
Eastman, C. R., 658
Echinodermata, geologic contributions of, 661
Echinoids, geologic contributions of, 661
Economic geology, 1
Efflorescence, 42
Elæolite, 462
Electricity,
atmospheric, 43
chemical effects of, 43
geological effects of, 43, 52
Ells, R., 443
Emmons, S. F., 474
Emmons, W. H., 474, 573, 585
Englacial drift, 282
Enlargement of crystals, by secondary growth, 435
Page 781
Enstatite, 400, 462
Eolian rocks, 469
Epeirogenic movements, 537
Epicontinental seas, 11, 326
Epidote, 431, 462
Equisetæ, geologic contribution of, 657
Eras, 17–19
Erosion,
affected by rotation, 194
analysis of, 110
base-level of, 60
by glaciers, 281–286
by rain, 57
by rivers, 56–177
by undertow, 342, 346
by waves, 342–349
by wind, 38
conditions affecting rate of, by glaciers, 283
conditions affecting rate of, by running water, 123
cycle of, 80, 82, 164
in arid regions, 131
influenced by climate, 127, 128, 129
influenced by composition of rock, 124
influenced by declivity, 123
influenced by structure, 124, 126
influenced by vegetation, 129, 644
sheet, 59
subaërial, 58
Erosion and cleavage planes, 125
Erosion and joints, 125
Erosion by streams (see Erosion by running water)
Eruptions, 591
fissure, 593
volcanic, 594
Eolian rocks, 469
Epeirogenic movements, 537
Epicontinental seas, 11, 326
Epidote, 431, 462
Equisetæ, geologic contribution of, 657
Eras, 17–19
Erosion,
affected by rotation, 194
analysis of, 110
base-level of, 60
by glaciers, 281–286
by rain, 57
by rivers, 56–177
by undertow, 342, 346
by waves, 342–349
by wind, 38
conditions affecting rate of, by glaciers, 283
conditions affecting rate of, by running water, 123
cycle of, 80, 82, 164
in arid regions, 131
influenced by climate, 127, 128, 129
influenced by composition of rock, 124
influenced by declivity, 123
influenced by structure, 124, 126
influenced by vegetation, 129, 644
sheet, 59
subaërial, 58
Erosion and cleavage planes, 125
Erosion and joints, 125
Erosion by streams (see Erosion by running water)
Eruptions, 591
fissure, 593
volcanic, 594
Page 782
Eskers, 306
Etna, 605, 610
discharge of stream from, 636
Evaporation, 50
Everett, 578
Evolution restrictive and expansional, 672
Exfoliation, 44
Expansional evolution, 672
Expansion and contraction,
due to temperature, 44
due to wetting and drying, 52
Extinct lakes, 388
Extrusive processes, 590–637
Falb, R., 537
False bedding, 487
Faulting and vulcanism, 627
Faults,
conditions of, 521
dip, 522
displacement, 514
distributive, 519
effect on outcrops, 522
hade, 514
heave of, 514
normal, 517
oblique, 525
relation to folds, 515
reversed, 517, 521
stratigraphic throw, 518
significance of, 521
strike, 522
thrust, 517, 518
Etna, 605, 610
discharge of stream from, 636
Evaporation, 50
Everett, 578
Evolution restrictive and expansional, 672
Exfoliation, 44
Expansional evolution, 672
Expansion and contraction,
due to temperature, 44
due to wetting and drying, 52
Extinct lakes, 388
Extrusive processes, 590–637
Falb, R., 537
False bedding, 487
Faulting and vulcanism, 627
Faults,
conditions of, 521
dip, 522
displacement, 514
distributive, 519
effect on outcrops, 522
hade, 514
heave of, 514
normal, 517
oblique, 525
relation to folds, 515
reversed, 517, 521
stratigraphic throw, 518
significance of, 521
strike, 522
thrust, 517, 518
Page 783
Fault scarp, 514
Faunas,
abysmal, 670
Australian, 668
cosmopolitan, 668
deep-sea, 670
pelagic, 670
photobathic, 670
Faunas and floras,
basis of, 663
effect of geographic conditions on evolution of, 668
Feldspar, 462
Feldspar-leucophyres, 453
Feldspar-melaphyres, 453
Feldspathic minerals, 400
Feldspathoids, 400
Felsites, 452, 469
Fenneman, N. M., 339
Ferguson, A. M., 203
Ferns, geologic contribution of, 657
Fiords, 290
Fisher, O., 561, 565, 574, 581
Fissure eruptions, 593
Fletcher, G. (and Deeley, R. M.), 322
Flints, 426, 469
Floods, 109
of the Mississippi, 188
Flood-plain meanders, 190
Flood-plains, 184–98
development of, 165
materials of, 196
Mississippi, 194
Faunas,
abysmal, 670
Australian, 668
cosmopolitan, 668
deep-sea, 670
pelagic, 670
photobathic, 670
Faunas and floras,
basis of, 663
effect of geographic conditions on evolution of, 668
Feldspar, 462
Feldspar-leucophyres, 453
Feldspar-melaphyres, 453
Feldspathic minerals, 400
Feldspathoids, 400
Felsites, 452, 469
Fenneman, N. M., 339
Ferguson, A. M., 203
Ferns, geologic contribution of, 657
Fiords, 290
Fisher, O., 561, 565, 574, 581
Fissure eruptions, 593
Fletcher, G. (and Deeley, R. M.), 322
Flints, 426, 469
Floods, 109
of the Mississippi, 188
Flood-plain meanders, 190
Flood-plains, 184–98
development of, 165
materials of, 196
Mississippi, 194
Page 784
relation to terraces, 205
topography, 196
Floras and faunas,
basis of, 663
effect of geographic conditions on, 668
Flowering plants, geologic contributions of, 657
Flowing wells, 234, 242
Flow structure of lavas, 410
Fluorite, 462
Fluvio-glacial work, 305–7
Folded ranges, distribution of, 543
Folding and vulcanism, 628
Folds,
anticlinal, 504, 505
effect on valleys, 154
isoclinal, 504
synclinal, 504
Folds and faults, 515
Foliation of ice, 272
Foliation of rocks, 443
Foraminifera, geologic contribution of, 660
Forbes, J. D., 256, 322
Forel, F. A., 323, 386
Fore-set beds, 202
Formation, 487
Forster, W. G., 536
“Fossil” deltas, 203
Fossils, 16, 646
a means of correlation, 647
Fossils and stratigraphy, 647
Fouqué, F., 635, 636
topography, 196
Floras and faunas,
basis of, 663
effect of geographic conditions on, 668
Flowering plants, geologic contributions of, 657
Flowing wells, 234, 242
Flow structure of lavas, 410
Fluorite, 462
Fluvio-glacial work, 305–7
Folded ranges, distribution of, 543
Folding and vulcanism, 628
Folds,
anticlinal, 504, 505
effect on valleys, 154
isoclinal, 504
synclinal, 504
Folds and faults, 515
Foliation of ice, 272
Foliation of rocks, 443
Foraminifera, geologic contribution of, 660
Forbes, J. D., 256, 322
Forel, F. A., 323, 386
Fore-set beds, 202
Formation, 487
Forster, W. G., 536
“Fossil” deltas, 203
Fossils, 16, 646
a means of correlation, 647
Fossils and stratigraphy, 647
Fouqué, F., 635, 636
Page 785
Fracture, zone of, 219
Frank, A. B., 642
Freestone, 469
French Broad River, the, 168
Fulgurites, 52, 469
Fungi, geologic contribution of, 653
Gabbroids, 453
Gabbros, 416, 452, 469
Galenite, 441
Ganges River, delta of, 203
Gangue, 469
Gannister, 469
Garnet, 462
Garnetite, 469
Gaseous emanations,
during earthquakes, 533
from volcanoes, 617
Gases in volcanic rocks, 619
Gases, volcanic, 617–623
amount of, 620
kinds of, 618, 619
proportions of, 620, 622
sources of, 621
Gastropods, geologic contributions of, 662
Geantcline, 505
Geest, 469
Geikie, A., 203, 224, 344, 534–536, 636
Geodes, 436, 497
Geognosy, 1, 5, 393–485
Geologic effects of earthquakes, 534
Frank, A. B., 642
Freestone, 469
French Broad River, the, 168
Fulgurites, 52, 469
Fungi, geologic contribution of, 653
Gabbroids, 453
Gabbros, 416, 452, 469
Galenite, 441
Ganges River, delta of, 203
Gangue, 469
Gannister, 469
Garnet, 462
Garnetite, 469
Gaseous emanations,
during earthquakes, 533
from volcanoes, 617
Gases in volcanic rocks, 619
Gases, volcanic, 617–623
amount of, 620
kinds of, 618, 619
proportions of, 620, 622
sources of, 621
Gastropods, geologic contributions of, 662
Geantcline, 505
Geest, 469
Geikie, A., 203, 224, 344, 534–536, 636
Geodes, 436, 497
Geognosy, 1, 5, 393–485
Geologic effects of earthquakes, 534
Page 786
Geologic functions of life, 638
Geologic processes, man’s influence on, 649
Geologic time divisions, 19
Geology,
astronomic, 1, 2
atmospheric, 2
cosmic, 1
dominant processes of, 2
dynamic, 1
economic, 1
geotectonic, 1, 486
glacial, 2
historical, 1
mining, 1
paleontologic, 1
philosophic, 1
physiographic, 1
scope of, 1
structural, 1, 486
subdivisions of, 1
George, R. D., 545
Geosyncline, 505
Geotectonic geology, 1, 486–525
Gerber, E., 195
Gerland, 538
Geschiebe wall, 300
Geyserite, 463, 469
Geysers, 236
deposits of, 237
of Yellowstone Park, 239
period of eruption, 240
positions of, 241
Gilbert, G. K., 11, 110, 140, 194, 198, 203, 339, 355, 388, 489, 596
Glacial débris,
Geologic processes, man’s influence on, 649
Geologic time divisions, 19
Geology,
astronomic, 1, 2
atmospheric, 2
cosmic, 1
dominant processes of, 2
dynamic, 1
economic, 1
geotectonic, 1, 486
glacial, 2
historical, 1
mining, 1
paleontologic, 1
philosophic, 1
physiographic, 1
scope of, 1
structural, 1, 486
subdivisions of, 1
George, R. D., 545
Geosyncline, 505
Geotectonic geology, 1, 486–525
Gerber, E., 195
Gerland, 538
Geschiebe wall, 300
Geyserite, 463, 469
Geysers, 236
deposits of, 237
of Yellowstone Park, 239
period of eruption, 240
positions of, 241
Gilbert, G. K., 11, 110, 140, 194, 198, 203, 339, 355, 388, 489, 596
Glacial débris,
Page 787
how carried, 290
nature of, 286
shifting position in transit, 292, 293, 294, 296, 297
Glacial deposits, nature of, 304
Glacial erosion,
conditions influencing, 283
topographic effects of, 287
Glacial motion, 313–321
auxiliary elements of, 317
fundamental element of, 313
Glacial plucking, 282
Glaciated rock surfaces, 304
Glacier ice,
beginning of movement, 248
definition of, 250
granular texture of, 247
shearing of, 317
Glacier movement, 259, 313–323
at low temperature, 279
effect of water on, 318
rates, 260, 261
views of, 321
Glaciers,
alpine, 254
cliff, 256
compared with rivers, 262
conditions influencing movement, 261
constitution, 308
continental, 251
crevasses, 264
deformation, 312
drainage of, 273, 280
foliation, 247, 272
evaporation, 279
general phenomena, 256
nature of, 286
shifting position in transit, 292, 293, 294, 296, 297
Glacial deposits, nature of, 304
Glacial erosion,
conditions influencing, 283
topographic effects of, 287
Glacial motion, 313–321
auxiliary elements of, 317
fundamental element of, 313
Glacial plucking, 282
Glaciated rock surfaces, 304
Glacier ice,
beginning of movement, 248
definition of, 250
granular texture of, 247
shearing of, 317
Glacier movement, 259, 313–323
at low temperature, 279
effect of water on, 318
rates, 260, 261
views of, 321
Glaciers,
alpine, 254
cliff, 256
compared with rivers, 262
conditions influencing movement, 261
constitution, 308
continental, 251
crevasses, 264
deformation, 312
drainage of, 273, 280
foliation, 247, 272
evaporation, 279
general phenomena, 256
Page 788
getting load, 282
growth of, 308
growth of granules, 310, 311
high-latitude, 254
limits of, 258
motion in terminal part, 316
movements of, 259, 279, 313–323
piedmont, 254
polar, 254
rate of movement of, 260, 261
reconstructed, 256
stratification of, 247
structure of, 308
surface features of, 266
temperature of, 273–279
thickening of layers at end, 297
topography of, 266
types of, 251
upturning of ice at ends and edges, 296, 297, 298
valley, 254
waste of, 273
work of, 244, 281
Glacio-fluvial work, 305–308
Glass, volcanic, 451
Glassy rocks, 406
Glauconite, 384, 386, 463
Globigerina ooze, 380, 382, 660
Globulites, 407, 469
Gneiss, 415, 446, 448, 469
Gooch, F. A. (and Whitfield, J. E.), 236
Gorge, 100
Grad, Ch., 322
Gradation, 2
by running water, 56–212
growth of, 308
growth of granules, 310, 311
high-latitude, 254
limits of, 258
motion in terminal part, 316
movements of, 259, 279, 313–323
piedmont, 254
polar, 254
rate of movement of, 260, 261
reconstructed, 256
stratification of, 247
structure of, 308
surface features of, 266
temperature of, 273–279
thickening of layers at end, 297
topography of, 266
types of, 251
upturning of ice at ends and edges, 296, 297, 298
valley, 254
waste of, 273
work of, 244, 281
Glacio-fluvial work, 305–308
Glass, volcanic, 451
Glassy rocks, 406
Glauconite, 384, 386, 463
Globigerina ooze, 380, 382, 660
Globulites, 407, 469
Gneiss, 415, 446, 448, 469
Gooch, F. A. (and Whitfield, J. E.), 236
Gorge, 100
Grad, Ch., 322
Gradation, 2
by running water, 56–212
Page 789
effect on coast-lines, 334
in ocean, 334
Grade, 61
Graded plain, 82, 169
Graded valley, 83
Granitell, 470
Granites, 413, 452, 469
Granitite, 470
Granitoids, 420, 453
Granulite, 470
Graphite, 426, 463
Gravitational energy, 552
Gravitational force, 552, 553
Gravity,
a cause of crustal movements, 552
effect on erosion, 113
Gray, T. (and Milne, J.), 578
Greenland,
glaciers of, 246
snow-fields of, 245
snow-line in, 246
Green mud, 380
Greensand, 470
Greensand marl, 386
Greenstone, 419, 470
Greisen, 415, 470
Greywacke, 470
Ground ice, 119
Ground moraine, 301
Ground-water, 213–243
affects internal heat, 570
in ocean, 334
Grade, 61
Graded plain, 82, 169
Graded valley, 83
Granitell, 470
Granites, 413, 452, 469
Granitite, 470
Granitoids, 420, 453
Granulite, 470
Graphite, 426, 463
Gravitational energy, 552
Gravitational force, 552, 553
Gravity,
a cause of crustal movements, 552
effect on erosion, 113
Gray, T. (and Milne, J.), 578
Greenland,
glaciers of, 246
snow-fields of, 245
snow-line in, 246
Green mud, 380
Greensand, 470
Greensand marl, 386
Greenstone, 419, 470
Greisen, 415, 470
Greywacke, 470
Ground ice, 119
Ground moraine, 301
Ground-water, 213–243
affects internal heat, 570
Page 790
amount of, 221
descent of, 213
fate of, 221
lower limit of, 216
movement of, 220
results of, 226
solution by, 222, 223
work of, 222
Ground-water and vulcanism, 635
Ground-water level, 71, 215
Ground-water surface, 71, 215
Guano, 646
Gulf stream, 366
Gullies, growth of, 63
Gymnosperms, geologic contributions of, 657
Gypsum, deposition of, 376, 377
Hade of faults, 514
Hall, Jas., 511
Halleflinta, 470
Halophytes, geologic contributions of, 667
Hanging valley, 164, 290
Haüynite, 463
Hayes, W., 173
Hayes, W. (and Campbell, M. R.), 171
Head erosion, 64
Heat, by compression of ice, 311
causes crustal movement, 557
causes of, in ice, 278, 279
distribution of, within earth, 559
distribution, original, 559
internal, of earth, 559–570
descent of, 213
fate of, 221
lower limit of, 216
movement of, 220
results of, 226
solution by, 222, 223
work of, 222
Ground-water and vulcanism, 635
Ground-water level, 71, 215
Ground-water surface, 71, 215
Guano, 646
Gulf stream, 366
Gullies, growth of, 63
Gymnosperms, geologic contributions of, 657
Gypsum, deposition of, 376, 377
Hade of faults, 514
Hall, Jas., 511
Halleflinta, 470
Halophytes, geologic contributions of, 667
Hanging valley, 164, 290
Haüynite, 463
Hayes, W., 173
Hayes, W. (and Campbell, M. R.), 171
Head erosion, 64
Heat, by compression of ice, 311
causes crustal movement, 557
causes of, in ice, 278, 279
distribution of, within earth, 559
distribution, original, 559
internal, of earth, 559–570
Page 791
metamorphism by, 446, 448
original distribution of, 559
Heave of faults, 514
Heilprin, A., 636
Heim, A., 256, 322, 549, 576
Hematite, 425, 447, 463
High-latitude glaciers, 254
Himalayas, snow-line in, 246
Historical geology, 1
Hoang-Ho delta, 202, 203
Hog-backs, 142
Holden, E. S., 538
Holmes, W. H., 99
Holocrystalline rock, 412
Holosiderites, 5
Hook (along shore), 363
Hopkins, W., 322
Horizontal configuration of coasts, due to deposition, 363, 364
due to wave erosion, 353
Hornblende, 400, 463
Hornblende-granite, 415
Hornblendite, 417, 452, 470
Hornstone, 470
Horsetails (see Equisetæ)
Hoskins, L. M., 219, 552, 581
Hot springs, deposits of, 225
Howell, Capt., 171
Hudson River, material in solution in, 108
Hugi, F. J., 321
Hull, E., 636
original distribution of, 559
Heave of faults, 514
Heilprin, A., 636
Heim, A., 256, 322, 549, 576
Hematite, 425, 447, 463
High-latitude glaciers, 254
Himalayas, snow-line in, 246
Historical geology, 1
Hoang-Ho delta, 202, 203
Hog-backs, 142
Holden, E. S., 538
Holmes, W. H., 99
Holocrystalline rock, 412
Holosiderites, 5
Hook (along shore), 363
Hopkins, W., 322
Horizontal configuration of coasts, due to deposition, 363, 364
due to wave erosion, 353
Hornblende, 400, 463
Hornblende-granite, 415
Hornblendite, 417, 452, 470
Hornstone, 470
Horsetails (see Equisetæ)
Hoskins, L. M., 219, 552, 581
Hot springs, deposits of, 225
Howell, Capt., 171
Hudson River, material in solution in, 108
Hugi, F. J., 321
Hull, E., 636
Page 792
Humphreys, A. A. (and Abbot, M. L.), 106, 202
Huxley, T. H., 322
Hyalite, 463
Hydration, 43, 222
disruption of rock by, 111
Hydrophytes, geologic contributions of, 667
Hydrosphere, the, 7 (see also Ground-water and Ocean)
geologic activity of, 8
horizons of activity, 9
Hypersthene, 400, 463
Hypogene rocks, 470
Ice, glacial (see Glaciers)
ground, 119
of lakes, 389
of rivers, 118
Icebergs, 307
Ice-caps, 249, 250
Ice crystals, arrangement in glacier ice, 311
Ice-fall, 264
Iceland spar, 463
Iddings, J. P., 412, 451, 573, 614, 636
Igneous rocks, 16
composition of, 395
leading minerals of, 399
origin of, 393
relations to stratified rocks, 16
structural features of, 498
Ilmenite, 463
Incrustation, 223
Infusorial earth, 470
Inorganic deposits, in deep sea, 380
Huxley, T. H., 322
Hyalite, 463
Hydration, 43, 222
disruption of rock by, 111
Hydrophytes, geologic contributions of, 667
Hydrosphere, the, 7 (see also Ground-water and Ocean)
geologic activity of, 8
horizons of activity, 9
Hypersthene, 400, 463
Hypogene rocks, 470
Ice, glacial (see Glaciers)
ground, 119
of lakes, 389
of rivers, 118
Icebergs, 307
Ice-caps, 249, 250
Ice crystals, arrangement in glacier ice, 311
Ice-fall, 264
Iceland spar, 463
Iddings, J. P., 412, 451, 573, 614, 636
Igneous rocks, 16
composition of, 395
leading minerals of, 399
origin of, 393
relations to stratified rocks, 16
structural features of, 498
Ilmenite, 463
Incrustation, 223
Infusorial earth, 470
Inorganic deposits, in deep sea, 380
Page 793
Interior of earth, 14 (see Vulcanism)
densities, based on Laplace’s law, 564
heat of, 562, 564
pressures, 564
Intermittent springs, 235
Internal heat (see Internal temperature)
Internal temperature, 562
affected by ground-water, 570
at centre of earth, 571
on accretion hypothesis, 564, 567
on convection hypothesis, 559
on Laplacian hypothesis, 559
Intrusions, 591
Iron-ore beds, origin, 425
Iron oxide, 400
Iron pyrites, 463
Ironstone, 425, 470
Irruptions, 591
Isoclinal folds, 504
Isoseismals, 532
Itacolumite, 470
Italy, lateral moraines in, 303
Jasper, 470
Jefferson, M. W., 193
Johnson, S. W., 109, 190, 665
Johnston-Lavis, H. J., 636
Joints, 510
causes of, 511, 531
compression, 514
effect on valleys, 150
Joints, tension, 514
densities, based on Laplace’s law, 564
heat of, 562, 564
pressures, 564
Intermittent springs, 235
Internal heat (see Internal temperature)
Internal temperature, 562
affected by ground-water, 570
at centre of earth, 571
on accretion hypothesis, 564, 567
on convection hypothesis, 559
on Laplacian hypothesis, 559
Intrusions, 591
Iron-ore beds, origin, 425
Iron oxide, 400
Iron pyrites, 463
Ironstone, 425, 470
Irruptions, 591
Isoclinal folds, 504
Isoseismals, 532
Itacolumite, 470
Italy, lateral moraines in, 303
Jasper, 470
Jefferson, M. W., 193
Johnson, S. W., 109, 190, 665
Johnston-Lavis, H. J., 636
Joints, 510
causes of, 511, 531
compression, 514
effect on valleys, 150
Joints, tension, 514
Page 794
Joints and erosion, 125
Judd, J. W., 636
Kaaterskill Creek, piracy of, 105
Kames, 307
serpentine, 306
Kansas, volcanic dust in, 23
Kanawha River, 168
Kaolin, 463
Katamorphism, 446
Keith, A., 442, 444
Kelvin, Lord, 560, 583
Keratophyre, 470
Kersantite, 470
Keyes, C. R., 474
Kidd, D. A., 313
Kilauea, 605
King, C., 560
King, F. H., 220
Kittatinny base-level, 168
Kotö, Dr., 534
Krakatoa, 22, 610, 611, 618
Kümmel, H. B., 203
Labradorite, 400, 429, 464
Laccolith, 500, 592
Lacustrine deposits, 388
Lake ice, 389
Lake Pepin, 179
Judd, J. W., 636
Kaaterskill Creek, piracy of, 105
Kames, 307
serpentine, 306
Kansas, volcanic dust in, 23
Kanawha River, 168
Kaolin, 463
Katamorphism, 446
Keith, A., 442, 444
Kelvin, Lord, 560, 583
Keratophyre, 470
Kersantite, 470
Keyes, C. R., 474
Kidd, D. A., 313
Kilauea, 605
King, C., 560
King, F. H., 220
Kittatinny base-level, 168
Kotö, Dr., 534
Krakatoa, 22, 610, 611, 618
Kümmel, H. B., 203
Labradorite, 400, 429, 464
Laccolith, 500, 592
Lacustrine deposits, 388
Lake ice, 389
Lake Pepin, 179
Page 795
Lakes, 386–392
bayou, 192, 193
changes taking place in, 387
delta, 204
deposits in, 387
extinct, 388
formed by rivers, 191, 192, 198
ice of, 389
ox-bow, 192, 198
Landslide, 231
topography of, 230
Landslip mountain, 230
Lane, A. C., 557, 636
Lapilli, 470
in sea, 381, 405
Laplace, Marquis de, 564
Laramide range, crustal shortening due to folding, 549
Lateral moraines, 266, 302
in Bighorn Mountains, 303
in Italy, 303
in Uinta Mountains, 303
in Wasatch Mountains, 303
Lateral pressure, metamorphism by, 448
Laterite, 470
Lava cones, 608
Lavas, 612–616
and ground-water, 616
consanguinity and succession of, 614
crystallization of, 402, 403
depth of source of, 616
modes of reaching surface, 631
origin of, 623–631
rhyolitic (flow) structure of, 410
solidification of, 393
bayou, 192, 193
changes taking place in, 387
delta, 204
deposits in, 387
extinct, 388
formed by rivers, 191, 192, 198
ice of, 389
ox-bow, 192, 198
Landslide, 231
topography of, 230
Landslip mountain, 230
Lane, A. C., 557, 636
Lapilli, 470
in sea, 381, 405
Laplace, Marquis de, 564
Laramide range, crustal shortening due to folding, 549
Lateral moraines, 266, 302
in Bighorn Mountains, 303
in Italy, 303
in Uinta Mountains, 303
in Wasatch Mountains, 303
Lateral pressure, metamorphism by, 448
Laterite, 470
Lava cones, 608
Lavas, 612–616
and ground-water, 616
consanguinity and succession of, 614
crystallization of, 402, 403
depth of source of, 616
modes of reaching surface, 631
origin of, 623–631
rhyolitic (flow) structure of, 410
solidification of, 393
Page 796
temperatures of, 615, 626
Lavas and underground water, 627
LeConte, J., 474, 549
Lendofelic, 456
Lenfelic, 456
Lepidolite, 464
Leucite, 464
Leucophyre, 412, 453
Levees, breaking of, 188
miniature, 182
natural, 188
on alluvial cones, 182
Level of no stress, 561
Life, 638–672
atmospheric effects of, 638–644
chemical work of, 638–646
climatic effects of, 643
effect on rock decomposition, 130, 644
geologic effects of, 639
inorganic rocks due to, 646
influenced by environment, 666
man’s influence on, 650
protection against erosion, 130, 644
Life and carbon dioxide, 640, 642, 643
Lightning, effects of, 52
Lignite, 426, 470
Limburgite, 470
Lime carbonate, deposition of, 375, 376
Limonite, 425
Limestone, 378, 424, 434
origin of, 378, 654, 655
stratification of, 487
Lavas and underground water, 627
LeConte, J., 474, 549
Lendofelic, 456
Lenfelic, 456
Lepidolite, 464
Leucite, 464
Leucophyre, 412, 453
Levees, breaking of, 188
miniature, 182
natural, 188
on alluvial cones, 182
Level of no stress, 561
Life, 638–672
atmospheric effects of, 638–644
chemical work of, 638–646
climatic effects of, 643
effect on rock decomposition, 130, 644
geologic effects of, 639
inorganic rocks due to, 646
influenced by environment, 666
man’s influence on, 650
protection against erosion, 130, 644
Life and carbon dioxide, 640, 642, 643
Lightning, effects of, 52
Lignite, 426, 470
Limburgite, 470
Lime carbonate, deposition of, 375, 376
Limonite, 425
Limestone, 378, 424, 434
origin of, 378, 654, 655
stratification of, 487
Page 797
Limestone-forming animals, 660–662
plants, 654, 655
Limestone sinks, 227, 231
Lindgren, W., 474
Liparase, 459
Liparite, 470
Lisbon earthquake, 535
Lithosphere, 9–19
crust of, 13
irregularities of, 10
relief of, 11
size and shape of, 9
surface mantle of, 12
Littoral currents, 342
Littoral deposits, 368, 369, 379
Littoral zone, 369
Liverworts, geologic contribution of, 656
Livingstone, D., 49
Load (of streams), 177–179
Loess, 23, 470
Lodge moraine, 301
Loop (along shore), 357, 363
Lunar craters, 598
Lunn, A. C., 552, 565, 566, 567, 572
Lycopods, geologic work of, 657
Lydekker, R. (and Nicholson, A.), 658
Lyell, Sir Charles, 649
Mackenzie River, delta, 202
Magma, nature of, 401
Magnesite, 464
plants, 654, 655
Limestone sinks, 227, 231
Lindgren, W., 474
Liparase, 459
Liparite, 470
Lisbon earthquake, 535
Lithosphere, 9–19
crust of, 13
irregularities of, 10
relief of, 11
size and shape of, 9
surface mantle of, 12
Littoral currents, 342
Littoral deposits, 368, 369, 379
Littoral zone, 369
Liverworts, geologic contribution of, 656
Livingstone, D., 49
Load (of streams), 177–179
Loess, 23, 470
Lodge moraine, 301
Loop (along shore), 357, 363
Lunar craters, 598
Lunn, A. C., 552, 565, 566, 567, 572
Lycopods, geologic work of, 657
Lydekker, R. (and Nicholson, A.), 658
Lyell, Sir Charles, 649
Mackenzie River, delta, 202
Magma, nature of, 401
Magnesite, 464
Page 798
Magnesium salts in sea, 377
Magnetic nodules in sea, 381
Magnetite, 464
Malay peninsula, tin ores of, 478
Malaspina glacier, 254
Mallet, R., 322, 537, 538, 628, 636
Mammoth Cave, 227
Mammoth hot springs, 654
Manganiferous deposits, 384
Mantle rock, 12, 422
Marble, 447, 471
Marcasite, 464
Marine deposits, 355–363, 370–386
chemical, 367, 375, 383
deep-sea, 368, 378–386
extra-terrestrial, 381
littoral, 368, 369
mechanical, 369, 380
organic, 375
shallow-water, 369–378
table of, 380
Marine life, distribution of, 328
Marl, 471 (see also Greensand marl and Shell marl)
formed by plants, 655
green-sand (see Greensand marl)
Martinique, 605
Martite, 464
Mason, W. P., 107
Mass action, 478, 484, 554
Mature drainage, 86
Mature streams, characteristics of, 86
Mauna Loa, 605, 606, 624
Magnetic nodules in sea, 381
Magnetite, 464
Malay peninsula, tin ores of, 478
Malaspina glacier, 254
Mallet, R., 322, 537, 538, 628, 636
Mammoth Cave, 227
Mammoth hot springs, 654
Manganiferous deposits, 384
Mantle rock, 12, 422
Marble, 447, 471
Marcasite, 464
Marine deposits, 355–363, 370–386
chemical, 367, 375, 383
deep-sea, 368, 378–386
extra-terrestrial, 381
littoral, 368, 369
mechanical, 369, 380
organic, 375
shallow-water, 369–378
table of, 380
Marine life, distribution of, 328
Marl, 471 (see also Greensand marl and Shell marl)
formed by plants, 655
green-sand (see Greensand marl)
Martinique, 605
Martite, 464
Mason, W. P., 107
Mass action, 478, 484, 554
Mature drainage, 86
Mature streams, characteristics of, 86
Mauna Loa, 605, 606, 624
Page 799
McConnell, J. C., 313, 322, 323, 549
McGee, W. J., 59, 524
Meander belt, relation to width of stream, 193
Meanders, flood-plain, 190
intrenched, 164
of the Meuse, 164
of the Moselle, 164
of the Seine, 164
Mean sphere level, 548
Medial moraine, 266, 297
Medlicott, H. B., 203
Medicinal springs, 235
Melaphyres, 412, 431, 453, 471
Menaccanite, 464
Mendelejeff, D. (and Moissan, H.), 646
Mental element, material effects of, 649
Merrill, G. P., 35, 111, 221
Mesas, 142
Mesophytes, 667
Meta-diabase, 471
Meta-igneous rock, 471
Metamorphic rocks, 17
Metamorphism, 427, 433, 440, 449
by heat, 446
by lateral pressure, 448
deep-seated, 449
Meteorites, 4
number of, 381
Meuse, meanders of, 164
Mica, 400, 464
Mica schists, 448
McGee, W. J., 59, 524
Meander belt, relation to width of stream, 193
Meanders, flood-plain, 190
intrenched, 164
of the Meuse, 164
of the Moselle, 164
of the Seine, 164
Mean sphere level, 548
Medial moraine, 266, 297
Medlicott, H. B., 203
Medicinal springs, 235
Melaphyres, 412, 431, 453, 471
Menaccanite, 464
Mendelejeff, D. (and Moissan, H.), 646
Mental element, material effects of, 649
Merrill, G. P., 35, 111, 221
Mesas, 142
Mesophytes, 667
Meta-diabase, 471
Meta-igneous rock, 471
Metamorphic rocks, 17
Metamorphism, 427, 433, 440, 449
by heat, 446
by lateral pressure, 448
deep-seated, 449
Meteorites, 4
number of, 381
Meuse, meanders of, 164
Mica, 400, 464
Mica schists, 448
Page 800
Microcline, 400, 464
Microlites, 407, 471
Microgranite, 471
Migration of dunes, 33
Millstone, 471
Milne, J., 533, 537, 538, 583
(and Gray, T.), 578
(and Burton), 636
Mineral matter in sea, 324–326
amount of, 325
Minerals, felspathic, 400, 462
ferromagnesian, 400, 460
formation of, 397, 612
of igneous rocks, 399
list of, 460–467
Mineral springs, 235
Minette, 415, 471
Mining geology, 1
Minnehaha Falls, 137
Mirlic rocks, 458
Mississippi River, delta, 197, 202
depth of channel, 171
flood-plain, 194
floods of, 188
levees of, 188
material in solution in, 108
sediment carried by, 106
Mississippi flood-plain, 194
lakes of, 192
Missouri River, scour-and-fill of, 195
Mitic rocks, 456
Moissan, H., 646
Microlites, 407, 471
Microgranite, 471
Migration of dunes, 33
Millstone, 471
Milne, J., 533, 537, 538, 583
(and Gray, T.), 578
(and Burton), 636
Mineral matter in sea, 324–326
amount of, 325
Minerals, felspathic, 400, 462
ferromagnesian, 400, 460
formation of, 397, 612
of igneous rocks, 399
list of, 460–467
Mineral springs, 235
Minette, 415, 471
Mining geology, 1
Minnehaha Falls, 137
Mirlic rocks, 458
Mississippi River, delta, 197, 202
depth of channel, 171
flood-plain, 194
floods of, 188
levees of, 188
material in solution in, 108
sediment carried by, 106
Mississippi flood-plain, 194
lakes of, 192
Missouri River, scour-and-fill of, 195
Mitic rocks, 456
Moissan, H., 646
Page 801
Mollusca, geologic contribution of, 662
Molluscoidea, geologic contribution of, 662
Molten interior, lava from, 624
Molten magmas, nature of, 401
Molten reservoirs, lavas from, 624
Monadnocks, 145
Monoclinal shifting, 127
Monocline, 504
Monzonite, 471
Moon, 3, 598
Moraines, dump, 301
ground, 302
lateral, 266, 302
lodge, 301
medial, 266, 297
molluscan shells in, 297
push, 301
surface, 266
terminal, 266, 301
types, 301
Moselle River, intrenchment meanders, 164
Moseley, H., 322
Mosses, geologic contributions of, 656
Moulton, F. R., 565
Mountain-forming movements, 542
Mountains, serration of, 48, 50
Mount Erebus, 603
Mount Hecla, 603
Mount Shasta, 611
Mount Terror, 603
Movements of glaciers, 259, 261, 279, 313–323
Molluscoidea, geologic contribution of, 662
Molten interior, lava from, 624
Molten magmas, nature of, 401
Molten reservoirs, lavas from, 624
Monadnocks, 145
Monoclinal shifting, 127
Monocline, 504
Monzonite, 471
Moon, 3, 598
Moraines, dump, 301
ground, 302
lateral, 266, 302
lodge, 301
medial, 266, 297
molluscan shells in, 297
push, 301
surface, 266
terminal, 266, 301
types, 301
Moselle River, intrenchment meanders, 164
Moseley, H., 322
Mosses, geologic contributions of, 656
Moulton, F. R., 565
Mountain-forming movements, 542
Mountains, serration of, 48, 50
Mount Erebus, 603
Mount Hecla, 603
Mount Shasta, 611
Mount Terror, 603
Movements of glaciers, 259, 261, 279, 313–323
Page 802
Movements of sea-water, 334–342
causes of, 334–339
Movements of the earth’s body, 526–589
causes of, 551–557
continent-forming, 544
distribution in time, 545
epeirogenic, 537
folding movements, 545
minute and rapid, 526
mountain-forming, 542
orogenic, 537
periodic, 542
plateau-forming, 543
relation of vertical and horizontal, 545
slow and massive, 537
Mud-cracks, 489
Mud-flows, volcanic, 610
Mud-rain, 25
Mudstone, 471
Mügge, O., 313, 322, 323
Muir glacier, 259
Murray, Sir John, 11, 215, 325, 326, 369, 604, 655
Muscovite, 400, 464
Narrows, 141
Natural bridges, 153, 231
of Virginia, 156
on coasts, 351
Natural gases, 646
Natural levees (see Levees)
Natural oils, 646
Nebraska, volcanic dust in, 23
causes of, 334–339
Movements of the earth’s body, 526–589
causes of, 551–557
continent-forming, 544
distribution in time, 545
epeirogenic, 537
folding movements, 545
minute and rapid, 526
mountain-forming, 542
orogenic, 537
periodic, 542
plateau-forming, 543
relation of vertical and horizontal, 545
slow and massive, 537
Mud-cracks, 489
Mud-flows, volcanic, 610
Mud-rain, 25
Mudstone, 471
Mügge, O., 313, 322, 323
Muir glacier, 259
Murray, Sir John, 11, 215, 325, 326, 369, 604, 655
Muscovite, 400, 464
Narrows, 141
Natural bridges, 153, 231
of Virginia, 156
on coasts, 351
Natural gases, 646
Natural levees (see Levees)
Natural oils, 646
Nebraska, volcanic dust in, 23
Page 803
Nephelinite, 471
Nephelite, 400, 464
Nevadite, 471
Névé, 246
New River, 168
Newsom, J. F., 514
Niagara Falls, 139
recession of, 139
Niagara River, 120
Nicholson, A. (and Lydekker, R.), 658
Nile River, delta of, 202
material in solution in, 108
sediment carried by, 107
Nitrogen and life, 642
Nodules, 471
Nomenclature of rocks, 449
new system of, 451
Norite, 471
Normal faults, 517
North America, average elevation of, 106
Nosite, 465
Novaculite, 471
Nummulites, 661
Oblique fault, 525
Obsidian, 407, 453, 471
Ocean basins, 11
areas of, 7
connection of, 8
deposits on, 368–386
relief of bottom, 11
Nephelite, 400, 464
Nevadite, 471
Névé, 246
New River, 168
Newsom, J. F., 514
Niagara Falls, 139
recession of, 139
Niagara River, 120
Nicholson, A. (and Lydekker, R.), 658
Nile River, delta of, 202
material in solution in, 108
sediment carried by, 107
Nitrogen and life, 642
Nodules, 471
Nomenclature of rocks, 449
new system of, 451
Norite, 471
Normal faults, 517
North America, average elevation of, 106
Nosite, 465
Novaculite, 471
Nummulites, 661
Oblique fault, 525
Obsidian, 407, 453, 471
Ocean basins, 11
areas of, 7
connection of, 8
deposits on, 368–386
relief of bottom, 11
Page 804
topography of, 326
Ocean basin segments, size of, 547
Oceanic deposits, chemical, 375
deep-sea, 368, 378–386
organic, 375, 382
shallow water, 369–378
Ocean, the, 7, 324–392
changes in, 329
composition of, 324
diastrophism in, 329
gradation in, 333
salts of, 324
volume of, 8
vulcanism in, 332
work of, 324–392
Offset with gap, 525
Offset with overlap, 525
Oldham, R. D., 534, 535
Oligoclase, 400, 465
Olivine, 400, 465
Omeose, 459
Omphacite, 465
Onyx, 471
Oolite, 435, 471, 496
Ooze, 471
Opal, 465
Ore deposits (see Ores)
O’Reilly, J. P., 538
Ore regions, origin of, 477
Ores, 428, 474–485
concentration by reprecipitation, 479
concentration by solution, 479
Ocean basin segments, size of, 547
Oceanic deposits, chemical, 375
deep-sea, 368, 378–386
organic, 375, 382
shallow water, 369–378
Ocean, the, 7, 324–392
changes in, 329
composition of, 324
diastrophism in, 329
gradation in, 333
salts of, 324
volume of, 8
vulcanism in, 332
work of, 324–392
Offset with gap, 525
Offset with overlap, 525
Oldham, R. D., 534, 535
Oligoclase, 400, 465
Olivine, 400, 465
Omeose, 459
Omphacite, 465
Onyx, 471
Oolite, 435, 471, 496
Ooze, 471
Opal, 465
Ore deposits (see Ores)
O’Reilly, J. P., 538
Ore regions, origin of, 477
Ores, 428, 474–485
concentration by reprecipitation, 479
concentration by solution, 479
Page 805
concentration by surface leaching, 478
“flaxseed,” 497
influence of rock walls on deposition, 484
magmatic segregation, 475
marine segregation, 476
original distribution, 475
purification by leaching, 478
residual concentration, 478
Organic processes, 638
Organic residue, 640, 641
Organic rocks, 449, 646
Original heat distribution, 559–568
Origin and descent of rocks, 393–484
Orogenic movements, 537
Orthoclase, 400, 465
Orthophyre, 471
Osars, 306
Outcrops, effects of faults on, 522
Outwash plain, 306
Overloading of streams, 177, 178, 186
Overthrust, 518
Oxbow lakes, 192, 198
Oxidation, 42, 427
Ozocerite, 465, 646
Paleontologic geology, 1
Paleontology, 1
Paraffine, 646
Peastone, 472
Peat, 406, 472
Pegmatite, 472
“flaxseed,” 497
influence of rock walls on deposition, 484
magmatic segregation, 475
marine segregation, 476
original distribution, 475
purification by leaching, 478
residual concentration, 478
Organic processes, 638
Organic residue, 640, 641
Organic rocks, 449, 646
Original heat distribution, 559–568
Origin and descent of rocks, 393–484
Orogenic movements, 537
Orthoclase, 400, 465
Orthophyre, 471
Osars, 306
Outcrops, effects of faults on, 522
Outwash plain, 306
Overloading of streams, 177, 178, 186
Overthrust, 518
Oxbow lakes, 192, 198
Oxidation, 42, 427
Ozocerite, 465, 646
Paleontologic geology, 1
Paleontology, 1
Paraffine, 646
Peastone, 472
Peat, 406, 472
Pegmatite, 472
Page 806
Pelagic deposits, 379–386
organic constituents of, 382
Pelagic fauna, 670
Pelecypods, shells of, 662
Pele’s, 618
“Pele’s hair,” 404
Pelites, 472
Peneplain, 81, 169
Penrose, R. A. F., Jr., 478
Peralkalic rocks, 458
Percaleic rocks, 458, 459
Perfemane, 455
Perfemic rocks, 454
Perfelic rocks, 456
Perferrous rocks, 459
Peridotites, 416, 453
Perlenic rocks, 456
Perlite, 408, 453, 472
Permiric rocks, 458
Permirlic rocks, 458
Permitic rocks, 457
Perolic rocks, 457
Perpolic rocks, 456
Perpotassic rocks, 458
Perpyric rocks, 457
Perquaric rocks, 456
Perrey, A., 537
Perrine, 538
Persalane, 455, 459
Persalic rocks, 454
organic constituents of, 382
Pelagic fauna, 670
Pelecypods, shells of, 662
Pele’s, 618
“Pele’s hair,” 404
Pelites, 472
Peneplain, 81, 169
Penrose, R. A. F., Jr., 478
Peralkalic rocks, 458
Percaleic rocks, 458, 459
Perfemane, 455
Perfemic rocks, 454
Perfelic rocks, 456
Perferrous rocks, 459
Peridotites, 416, 453
Perlenic rocks, 456
Perlite, 408, 453, 472
Permiric rocks, 458
Permirlic rocks, 458
Permitic rocks, 457
Perolic rocks, 457
Perpolic rocks, 456
Perpotassic rocks, 458
Perpyric rocks, 457
Perquaric rocks, 456
Perrey, A., 537
Perrine, 538
Persalane, 455, 459
Persalic rocks, 454
Page 807
Persodic rocks, 458
Pertilic rocks, 457
Petrifaction, 223
“Petrified turtles,” 496
Petroleum, 465
Petrology, 1, 393–485
Petrosilex, 472
Pfaff, F., 537
Phanerites, 451
Phanerocrystalline rocks, 412
Phenocrysts, 412
Philosophic geology, 1
Phonolite, 472
Photobathic fauna, 670
Photobathic zone, 670
Phyllite, 472
Physiographic geology, 1
Picrolite, 465
Pictotite, 465
Piedmontite, 465
Piedmont glacier, 254
Piedmont plain, alluvial, 183
Piracy, 160
domestic, 104
extent of, in Appalachians, 170
foreign, 104
of Kaaterskill Creek, 105
of Plaaterskill Creek, 105
Pirsson, Louis V., 412 451, 573
Pisolite, 465, 496
Pitchstones, 408, 453, 472
Pertilic rocks, 457
Petrifaction, 223
“Petrified turtles,” 496
Petroleum, 465
Petrology, 1, 393–485
Petrosilex, 472
Pfaff, F., 537
Phanerites, 451
Phanerocrystalline rocks, 412
Phenocrysts, 412
Philosophic geology, 1
Phonolite, 472
Photobathic fauna, 670
Photobathic zone, 670
Phyllite, 472
Physiographic geology, 1
Picrolite, 465
Pictotite, 465
Piedmontite, 465
Piedmont glacier, 254
Piedmont plain, alluvial, 183
Piracy, 160
domestic, 104
extent of, in Appalachians, 170
foreign, 104
of Kaaterskill Creek, 105
of Plaaterskill Creek, 105
Pirsson, Louis V., 412 451, 573
Pisolite, 465, 496
Pitchstones, 408, 453, 472
Page 808
Plagioclase, 465
Plain, alluvial, 181, 184
graded, 169
outwash, 306
Planation, 82
Plant kingdom, geologic contributions of, 652–658
Plant life and carbon dioxide, 665
Plant societies, 667
Plants, contributions to deposits, 652–658
contribution to limestone, 654
effect on erosion, 131, 644
reference table of, 653
weathering influenced by, 112
Platte River, 187
Plaaterskill Creek, piracy of, 105
Plugs, volcanic, 591
Plumbago, 465
Plunging anticline, 155
Plutonic rocks, 472
Polar glaciers, 254
Poincaré, H., 576
Polic rocks, 456
Polmitic rocks, 457
Ponding of streams, 171
Po River, delta of, 202
sediment carried by, 107
Porphyries, 453
Porphyrite, 472
Porphyritic rocks, 411
Porphyry, 472
Posepny, F., 474
Plain, alluvial, 181, 184
graded, 169
outwash, 306
Planation, 82
Plant kingdom, geologic contributions of, 652–658
Plant life and carbon dioxide, 665
Plant societies, 667
Plants, contributions to deposits, 652–658
contribution to limestone, 654
effect on erosion, 131, 644
reference table of, 653
weathering influenced by, 112
Platte River, 187
Plaaterskill Creek, piracy of, 105
Plugs, volcanic, 591
Plumbago, 465
Plunging anticline, 155
Plutonic rocks, 472
Polar glaciers, 254
Poincaré, H., 576
Polic rocks, 456
Polmitic rocks, 457
Ponding of streams, 171
Po River, delta of, 202
sediment carried by, 107
Porphyries, 453
Porphyrite, 472
Porphyritic rocks, 411
Porphyry, 472
Posepny, F., 474
Page 809
Potash, in sea-water, 377
Pot holes, 140
Potomac River, 168
sediment carried by, 107
Potonié, H., 652
Powell, J. W., 519, 521
Precipitation, 50
from atmosphere, 51
from solution, 41, 225, 239, 375–379
Precipitation from solution, conditions influencing, 225
influenced by algæ, 225
Pressures within earth, based on Laplace’s law, 564
Prestwich, J., 203, 225
Propylite, 472
Protogine, 472
Protozoa, geologic contribution of, 660
Provincial faunas, 668
Pseudomorphs, 465
Psilomelane, 465
Psychological factors 651
Pteridophytes, geologic contribution of, 657
Pteropod ooze, 380, 382
“Pulpit rocks,” 350
Pumice, 406, 453, 472
Push moraine, 301
Puzzalana, 405
Pyrite, 465
Pyroclastic rocks, 404, 406, 472
Pyrolic rocks, 457
Pyroxene, 400, 465
Pot holes, 140
Potomac River, 168
sediment carried by, 107
Potonié, H., 652
Powell, J. W., 519, 521
Precipitation, 50
from atmosphere, 51
from solution, 41, 225, 239, 375–379
Precipitation from solution, conditions influencing, 225
influenced by algæ, 225
Pressures within earth, based on Laplace’s law, 564
Prestwich, J., 203, 225
Propylite, 472
Protogine, 472
Protozoa, geologic contribution of, 660
Provincial faunas, 668
Pseudomorphs, 465
Psilomelane, 465
Psychological factors 651
Pteridophytes, geologic contribution of, 657
Pteropod ooze, 380, 382
“Pulpit rocks,” 350
Pumice, 406, 453, 472
Push moraine, 301
Puzzalana, 405
Pyrite, 465
Pyroclastic rocks, 404, 406, 472
Pyrolic rocks, 457
Pyroxene, 400, 465
Page 810
Pyroxenite, 417, 452, 472
Quaquaversal dip, 504
Quardofelic rocks, 456
Quarfelic rocks, 456
Quartz, 466
Quartzite, 447, 472
Quartz-leucophyres, 453
Quartzophyres, 453
Quartz-porphyries, 453
Radiolarian ooze, 380, 382, 425, 661
Rain, amount of, 51
erosion by, 57
mechanical work of, 51
Rain-drop impressions, 490
Rainfall, effect on erosion, 128
Ransome, F. L., 130, 513
Rapids, development of, 133, 146
Rate of erosion, conditions affecting, 123
Ravine, 64
Raymond, R. W., 474
Reade, T. M., 225, 366, 561, 572
Reconstructed glacier, 256
Red clay, 380, 383, 384
Red mud, 380
Red River of Louisiana, 188
Reid, H. F., 256, 259, 261
Regolith, 400, 472
Rejuvenation of streams, 162–163
Quaquaversal dip, 504
Quardofelic rocks, 456
Quarfelic rocks, 456
Quartz, 466
Quartzite, 447, 472
Quartz-leucophyres, 453
Quartzophyres, 453
Quartz-porphyries, 453
Radiolarian ooze, 380, 382, 425, 661
Rain, amount of, 51
erosion by, 57
mechanical work of, 51
Rain-drop impressions, 490
Rainfall, effect on erosion, 128
Ransome, F. L., 130, 513
Rapids, development of, 133, 146
Rate of erosion, conditions affecting, 123
Ravine, 64
Raymond, R. W., 474
Reade, T. M., 225, 366, 561, 572
Reconstructed glacier, 256
Red clay, 380, 383, 384
Red mud, 380
Red River of Louisiana, 188
Reid, H. F., 256, 259, 261
Regolith, 400, 472
Rejuvenation of streams, 162–163
Page 811
criteria of, 164, 165, 166
Relief, of lithosphere, 11
of ocean basins, 11
representation on maps, 30
Relief of pressure, a cause of volcanic action, 627
Rendu, L. C., 321, 322
Restrictive evolution, 672
Reversed fault, 517, 521
Reyer, E., 636
Rhine River, material in solution in, 108
Rhizopoda, geologic contributions of, 660
Rhone River, delta of, 203
material in solution in, 108
sediment carried by, 107
Rhyolite, 472
Rhyolitic structure, of lavas, 41
Ricard, T. A., 474
Richthofen, Baron von, 23, 604, 614, 615
Rigidity, distribution of, 578
Rill-marks, 372, 489
Rink, H., 248
Ripple-marks, 371, 489
due to wind, 37
Rio Grande River, sediment of, 107
River lakes, 198
River erosion (see Stream erosion)
Roanoke River, 168
Roches Moutonnées, 304
Rock breaking, by changes of temperature, 44, 49
Rocks, alferric, 454
alkalicalcic, 458
Relief, of lithosphere, 11
of ocean basins, 11
representation on maps, 30
Relief of pressure, a cause of volcanic action, 627
Rendu, L. C., 321, 322
Restrictive evolution, 672
Reversed fault, 517, 521
Reyer, E., 636
Rhine River, material in solution in, 108
Rhizopoda, geologic contributions of, 660
Rhone River, delta of, 203
material in solution in, 108
sediment carried by, 107
Rhyolite, 472
Rhyolitic structure, of lavas, 41
Ricard, T. A., 474
Richthofen, Baron von, 23, 604, 614, 615
Rigidity, distribution of, 578
Rill-marks, 372, 489
Rink, H., 248
Ripple-marks, 371, 489
due to wind, 37
Rio Grande River, sediment of, 107
River lakes, 198
River erosion (see Stream erosion)
Roanoke River, 168
Roches Moutonnées, 304
Rock breaking, by changes of temperature, 44, 49
Rocks, alferric, 454
alkalicalcic, 458
Page 812
alkalimirlic, 458
alterations of, 426
aqueous, 467
arenaceous, 468
autoclastic, 444
calcimiric, 458
“chimney,” 350
chloritic, 431
classification and nomenclature, 449
clastic, 468
crystalline, 16
determination of age, 15
disruption by hydration, 111
docalcic, 458
dofemic, 454
doferrous, 459
dohemic, 457
dolenic, 456
domagnesic, 459
domalkalic, 458
domilic, 457
domiric, 458
domirlic, 458
domitic, 457
dopolic, 456
dopotassic, 458
dopyric, 457
doquaric, 456
dosalic, 454
dosodic, 458
dotilic, 457
eolian, 469
femic, 454
glassy, 406
holocrystalline, 412
hypogene, 470
igneous, 16, 393, 498
alterations of, 426
aqueous, 467
arenaceous, 468
autoclastic, 444
calcimiric, 458
“chimney,” 350
chloritic, 431
classification and nomenclature, 449
clastic, 468
crystalline, 16
determination of age, 15
disruption by hydration, 111
docalcic, 458
dofemic, 454
doferrous, 459
dohemic, 457
dolenic, 456
domagnesic, 459
domalkalic, 458
domilic, 457
domiric, 458
domirlic, 458
domitic, 457
dopolic, 456
dopotassic, 458
dopyric, 457
doquaric, 456
dosalic, 454
dosodic, 458
dotilic, 457
eolian, 469
femic, 454
glassy, 406
holocrystalline, 412
hypogene, 470
igneous, 16, 393, 498
Page 813
leading elements of, 396
lendofelic, 456
lenfelic, 456
magnesiferrous, 459
meta-igneous, 471
metamorphic, 16
mirlic, 458
mitic, 456
organic, 646
origin and descent of, 393–485
peralkalic, 458
percalcic, 458, 459
perfelic, 456
perfemic, 454
perferrous, 459
perhemic 457
perlenic, 456
permagnesic, 459
permiric, 458
permerlic, 458
permitic, 457
perolic, 457
perpolic, 456
perpotassic, 458
perquaric, 456
persalic, 454
persodic, 458
pertilic, 457
perpyric, 457
phanerocrystalline, 412
plutonic, 472
polic, 456
polmitic, 457
porphyritic, 411
precipitate, 427
“pulpit,” 350
pyroclastic, 404, 406, 472
lendofelic, 456
lenfelic, 456
magnesiferrous, 459
meta-igneous, 471
metamorphic, 16
mirlic, 458
mitic, 456
organic, 646
origin and descent of, 393–485
peralkalic, 458
percalcic, 458, 459
perfelic, 456
perfemic, 454
perferrous, 459
perhemic 457
perlenic, 456
permagnesic, 459
permiric, 458
permerlic, 458
permitic, 457
perolic, 457
perpolic, 456
perpotassic, 458
perquaric, 456
persalic, 454
persodic, 458
pertilic, 457
perpyric, 457
phanerocrystalline, 412
plutonic, 472
polic, 456
polmitic, 457
porphyritic, 411
precipitate, 427
“pulpit,” 350
pyroclastic, 404, 406, 472
Page 814
quardofelic, 456
quarfelic, 456
salfemic, 454
salic, 454
secondary, 420
sedimentary, 422, 486
sodipotassic, 458
solution of, 427
specific heat of, 552
stratified, 14
talcose, 431
tilhemic, 457
Rock terraces, 140, 204
Rock waste, 12
Roots, wedge-work of, 112, 131, 150
Rotation of earth, change in rate of, 575
effect on stream erosion, 194
Rotation and vulcanism, 604
Roth, J., 108
Running water (see Streams)
Run-off, 59
Russell, I. C., 108, 118, 151, 172, 194, 203, 232, 256, 283, 388, 392,
636
Rutile, 466
Saint Vincent, 605
Salfemane, 455
Salfemic rocks, 454
Saline lakes (see Salt lakes)
Saline springs, 235
Salisbury, R. D., 203, 256
Salt lakes, 391
quarfelic, 456
salfemic, 454
salic, 454
secondary, 420
sedimentary, 422, 486
sodipotassic, 458
solution of, 427
specific heat of, 552
stratified, 14
talcose, 431
tilhemic, 457
Rock terraces, 140, 204
Rock waste, 12
Roots, wedge-work of, 112, 131, 150
Rotation of earth, change in rate of, 575
effect on stream erosion, 194
Rotation and vulcanism, 604
Roth, J., 108
Running water (see Streams)
Run-off, 59
Russell, I. C., 108, 118, 151, 172, 194, 203, 232, 256, 283, 388, 392,
636
Rutile, 466
Saint Vincent, 605
Salfemane, 455
Salfemic rocks, 454
Saline lakes (see Salt lakes)
Saline springs, 235
Salisbury, R. D., 203, 256
Salt lakes, 391
Page 815
composition of, 372
deposits in, 388
Salts, deposition of, 375–378
in sea-water, 324–326
Sand, eolian, 26–37
Sandstone, 422, 434, 472
stratification of, 487
Sandstone dikes, 514
Sanidine, 466
Sapping, 127, 133
Satinspar, 466
Schist, 446, 472
Schistosity, 443
Schmidt, J. F. J., 537
Schoharie Creek, beheaded, 105
Scoriæ, 405, 473
Scour-and-fill, 194
of Missouri River, 195
Scrope, G. P., 636
Sea-caves, 350
Sea-cliffs, 349
Sea, the (see Ocean)
Sea-water, aperiodic movements of, 338
movements generated by attraction, 337
movements of, 334–342
salts in, 376, 377, 378
Sea-waves, caused by earthquake, 535
Secondary rocks, derivation of, 420
“Second bottoms,” 205
Secretions, 497
Sediment, carried by Danube, 107
deposits in, 388
Salts, deposition of, 375–378
in sea-water, 324–326
Sand, eolian, 26–37
Sandstone, 422, 434, 472
stratification of, 487
Sandstone dikes, 514
Sanidine, 466
Sapping, 127, 133
Satinspar, 466
Schist, 446, 472
Schistosity, 443
Schmidt, J. F. J., 537
Schoharie Creek, beheaded, 105
Scoriæ, 405, 473
Scour-and-fill, 194
of Missouri River, 195
Scrope, G. P., 636
Sea-caves, 350
Sea-cliffs, 349
Sea, the (see Ocean)
Sea-water, aperiodic movements of, 338
movements generated by attraction, 337
movements of, 334–342
salts in, 376, 377, 378
Sea-waves, caused by earthquake, 535
Secondary rocks, derivation of, 420
“Second bottoms,” 205
Secretions, 497
Sediment, carried by Danube, 107
Page 816
carried by Irrawaddy, 107
carried by Mississippi, 107
carried by Nile, 107
carried by Po, 107
carried by Potomac, 107
carried by Rhone, 107
carried by Rio Grande, 107
carried by Uruguay, 107
character of, influenced by land vegetation, 645
deposited by rivers, 65, 177–204
deposited in lakes, 387
deposited in sea, 368–386
effect on corrasion, 120
effect on falls, 137
how carried by streams, 116
Sedimentary rocks, classes of, 422
structural features of, 486
Sedimentation and vulcanism, 629
Seed-plants, 657
Segregation of ores, 475
Seiches, 386
Seine River, intrenched meanders of, 164
Selenite, 466
Septaria, 473, 495
Serpentine, 431, 466, 473
Serpentine kames, 306
Seward, A. C., 652
Shale, 422, 434, 473
stratification of, 487
Shaler, N. S., 227, 349, 357 (and Davis, W. M.), 256
Shallow-water deposits, 368, 369, 379
characteristics of, 373
topography of, 374
carried by Mississippi, 107
carried by Nile, 107
carried by Po, 107
carried by Potomac, 107
carried by Rhone, 107
carried by Rio Grande, 107
carried by Uruguay, 107
character of, influenced by land vegetation, 645
deposited by rivers, 65, 177–204
deposited in lakes, 387
deposited in sea, 368–386
effect on corrasion, 120
effect on falls, 137
how carried by streams, 116
Sedimentary rocks, classes of, 422
structural features of, 486
Sedimentation and vulcanism, 629
Seed-plants, 657
Segregation of ores, 475
Seiches, 386
Seine River, intrenched meanders of, 164
Selenite, 466
Septaria, 473, 495
Serpentine, 431, 466, 473
Serpentine kames, 306
Seward, A. C., 652
Shale, 422, 434, 473
stratification of, 487
Shaler, N. S., 227, 349, 357 (and Davis, W. M.), 256
Shallow-water deposits, 368, 369, 379
characteristics of, 373
topography of, 374
Page 817
Shearing of glacier ice, 317
Sheet erosion, 59
Shell marl, 655
Shore currents, 342
deposition by, 355
Shore deposition and coastal configuration, 363
Shore drift, 355
Shore ice, 389
Shoshone Falls, 135
Siderite, 425, 466
Silicified wood, 439
Silicious deposits, 425
Sills, 446, 592
Sketcherly, S. B., 23
Slate, 473
Slaty structure, 441
Slichter, C. S., 221, 563, 576
Slumps, 231
Smaragdite, 466
Smith, E. A., 543
Snow-fields, 244
distribution of, 244
Snowflakes, forms of, 310
Snow-line, 245
in Andes, 246
in Antarctica, 246
in Greenland, 246
in Himalayas, 246
Snow, work of, 244
Soapstone, 431, 473
Sodipotassic rocks, 458
Sheet erosion, 59
Shell marl, 655
Shore currents, 342
deposition by, 355
Shore deposition and coastal configuration, 363
Shore drift, 355
Shore ice, 389
Shoshone Falls, 135
Siderite, 425, 466
Silicified wood, 439
Silicious deposits, 425
Sills, 446, 592
Sketcherly, S. B., 23
Slate, 473
Slaty structure, 441
Slichter, C. S., 221, 563, 576
Slumps, 231
Smaragdite, 466
Smith, E. A., 543
Snow-fields, 244
distribution of, 244
Snowflakes, forms of, 310
Snow-line, 245
in Andes, 246
in Antarctica, 246
in Greenland, 246
in Himalayas, 246
Snow, work of, 244
Soapstone, 431, 473
Sodipotassic rocks, 458
Page 818
Solms-Laubach, 652
Solution, by ground-water, 222
by rivers, 108, 122
Solution of rocks, 427
Solvent action, location of, 480
Sorby, H. C., 367
Source of streams, 178
Spatter cones, 609, 610
Specific heat of rock, 552
Spermatophytes, geologic contribution of, 657
Sphenophyllum, 657
Sphericity, a factor in deformation, 580
Spherosiderite, 466
Spinel, 466
Spit, the, 357
Sponges, secretions of, 661
Sporadosiderites, 5
“Spouting horn,” 351
Springs, calcareous, 235
chalybeate, 235
cold, 234
common, 235
deep, 234
intermittent, 235
medicinal, 235
mineral, 235
saline, 235
shallow, 234
sulphur, 235
Stalactite, 437, 473
formation of, 227
Stalagmite 437, 473
Solution, by ground-water, 222
by rivers, 108, 122
Solution of rocks, 427
Solvent action, location of, 480
Sorby, H. C., 367
Source of streams, 178
Spatter cones, 609, 610
Specific heat of rock, 552
Spermatophytes, geologic contribution of, 657
Sphenophyllum, 657
Sphericity, a factor in deformation, 580
Spherosiderite, 466
Spinel, 466
Spit, the, 357
Sponges, secretions of, 661
Sporadosiderites, 5
“Spouting horn,” 351
Springs, calcareous, 235
chalybeate, 235
cold, 234
common, 235
deep, 234
intermittent, 235
medicinal, 235
mineral, 235
saline, 235
shallow, 234
sulphur, 235
Stalactite, 437, 473
formation of, 227
Stalagmite 437, 473
Page 819
St. Anthony Falls, 136
Stapff, F. M. 388
Staurolite, 466
Steam discharge from volcanoes, 635
Steatite, 431, 466, 473
Stevenson, D., 341, 344, 370
Stoping, 632
Stoss side, 299
Strachey, R., 51
Stratification, 486
Stratified rocks, 14
Stratigraphic geology, 1
Stratigraphy and fossils, 647
Stratigraphy and paleontology, 647
Stream erosion, 56–177
economic effects of, 108
influenced by rock, 124
influenced by declivity, 123
influenced by structure, 125, 127
topography developed by, 92
Streams, abrasion by, 119
adjustment in Appalachians, 148
adjustment of, 146, 147
affected by rotation of earth, 194
aggradational work of, 177–204
antecedent, 169, 171
characteristics of aggrading, 179, 187
compared with glaciers, 262
consequent, 78
corrasion by, 119
cross-currents in, 117
decrease in size of, 179, 180
deposition by, 177
Stapff, F. M. 388
Staurolite, 466
Steam discharge from volcanoes, 635
Steatite, 431, 466, 473
Stevenson, D., 341, 344, 370
Stoping, 632
Stoss side, 299
Strachey, R., 51
Stratification, 486
Stratified rocks, 14
Stratigraphic geology, 1
Stratigraphy and fossils, 647
Stratigraphy and paleontology, 647
Stream erosion, 56–177
economic effects of, 108
influenced by rock, 124
influenced by declivity, 123
influenced by structure, 125, 127
topography developed by, 92
Streams, abrasion by, 119
adjustment in Appalachians, 148
adjustment of, 146, 147
affected by rotation of earth, 194
aggradational work of, 177–204
antecedent, 169, 171
characteristics of aggrading, 179, 187
compared with glaciers, 262
consequent, 78
corrasion by, 119
cross-currents in, 117
decrease in size of, 179, 180
deposition by, 177
Page 820
drowning of, 170
effect of change of level on, 161, 171
erosion by, 57–177
floods of, 109
ice of, 118
intermittent, 71, 72
mature, 86
mechanical work of, 226
migration from synclines to anticlines, 159
mineral matter in solution in, 225
old age of, 89
overloading of, 178, 179, 186
permanent, 70
piracy of, 103
ponding of, 171
relation of width to meander belt, 193
solution by, 108, 122
sources of, 178
struggle for existence among, 100
superimposed, 150
topographic adjustment of, 162, 163, 197
transportation by, 115, 116
velocity of, 115
young, 85
Stream-terraces, 204–212
Stream velocity, effect on transportation, 115
Stream work, 57–212
Stress-accumulation, 583, 588
Striæ, 283
Strike, 501
Strike fault, 522
Stromboli, 636
Structural adjustment of valleys, 147
Structural features of rocks, 486–525
effect of change of level on, 161, 171
erosion by, 57–177
floods of, 109
ice of, 118
intermittent, 71, 72
mature, 86
mechanical work of, 226
migration from synclines to anticlines, 159
mineral matter in solution in, 225
old age of, 89
overloading of, 178, 179, 186
permanent, 70
piracy of, 103
ponding of, 171
relation of width to meander belt, 193
solution by, 108, 122
sources of, 178
struggle for existence among, 100
superimposed, 150
topographic adjustment of, 162, 163, 197
transportation by, 115, 116
velocity of, 115
young, 85
Stream-terraces, 204–212
Stream velocity, effect on transportation, 115
Stream work, 57–212
Stress-accumulation, 583, 588
Striæ, 283
Strike, 501
Strike fault, 522
Stromboli, 636
Structural adjustment of valleys, 147
Structural features of rocks, 486–525
Page 821
arising from disturbance, 500
of igneous rocks, 498
of sedimentary rock, 486
Structural geology, 1, 486
Structural valleys, 77
Structure of glacier ice, 308
Structure of rock, influence on erosion, 125
Struggle for existence among valleys, 100
Subaërial erosion, 58
Sub-atomic forces, causes of crustal movement, 556
Subdivisions of geology, 1
Subglacial load, 282
Subsidence, effect on coast-lines, 331
Suess, Edw., 538
Sulphur, 466
Sulphur springs, 235
Sun-cracks, 373, 490
Superglacial load, 282
Superimposed streams, 150
Surface moraines, 266
Susquehanna River, 168
Switzerland, snow-fields of, 245
Syenites, 415, 452, 473
Syncline, 157, 504
Synclinoria, 504
Syssiderites, 5
Tachylite, 473
Tait, P. G., 552, 572, 573 (and Thompson, J.), 560, 579
Talc, 466
of igneous rocks, 498
of sedimentary rock, 486
Structural geology, 1, 486
Structural valleys, 77
Structure of glacier ice, 308
Structure of rock, influence on erosion, 125
Struggle for existence among valleys, 100
Subaërial erosion, 58
Sub-atomic forces, causes of crustal movement, 556
Subdivisions of geology, 1
Subglacial load, 282
Subsidence, effect on coast-lines, 331
Suess, Edw., 538
Sulphur, 466
Sulphur springs, 235
Sun-cracks, 373, 490
Superglacial load, 282
Superimposed streams, 150
Surface moraines, 266
Susquehanna River, 168
Switzerland, snow-fields of, 245
Syenites, 415, 452, 473
Syncline, 157, 504
Synclinoria, 504
Syssiderites, 5
Tachylite, 473
Tait, P. G., 552, 572, 573 (and Thompson, J.), 560, 579
Talc, 466
Page 822
Talcose rock, 431
Talus, 112
Talus cone, 182
Talus glacier, 233, 232
Tarr, R. S., 165
Temperature, at centre of earth, 571
atmospheric, 43, 46, 49
based on Laplace’s law, 564
effect on erosion, 129
effects of changes on rocks, 44
expansion and contraction due to changes of, 44
in excavations, 569
of interior of earth, 559–570
of lavas, 615, 627
Tennessee River, history of, 168–169
Tension joints, 514
Terminal moraine, 266, 301
Terraces, stream, 204–212
flood-plain, 205
rock, 140, 204
termini of, 210
wave-built, 363
wave-cut, 351, 353
Terrigenous deposits, in sea, 379
Thallophytes, geologic contribution of, 653
Thames River, 224
material in solution in, 108
Thibetan plateau, 548
Thompson, James, 322, 560, 579
Thompson, W. G., 119
“Thorofares,” 358
Thrust-fault, 517, 518
Talus, 112
Talus cone, 182
Talus glacier, 233, 232
Tarr, R. S., 165
Temperature, at centre of earth, 571
atmospheric, 43, 46, 49
based on Laplace’s law, 564
effect on erosion, 129
effects of changes on rocks, 44
expansion and contraction due to changes of, 44
in excavations, 569
of interior of earth, 559–570
of lavas, 615, 627
Tennessee River, history of, 168–169
Tension joints, 514
Terminal moraine, 266, 301
Terraces, stream, 204–212
flood-plain, 205
rock, 140, 204
termini of, 210
wave-built, 363
wave-cut, 351, 353
Terrigenous deposits, in sea, 379
Thallophytes, geologic contribution of, 653
Thames River, 224
material in solution in, 108
Thibetan plateau, 548
Thompson, James, 322, 560, 579
Thompson, W. G., 119
“Thorofares,” 358
Thrust-fault, 517, 518
Page 823
Tides, 4, 338
effect on rotation, 4
Tilden, W. A., 620
Tilhemic rocks, 457
Till, 473
Titanite, 467
Todd, J. E., 195
Topaz, 467
Topographic adjustment of streams, 162, 163, 197
Topographic effects of glacial erosion, 287
Topographic effects of ground-water, 231
Topographic map, explanation of, 30
Topographic maturity, 86
Topographic old age, 89
Topographic youth, 86
Topography, developed by river erosion, 92
dune, 32
landslide, 231
mature, 86
of alluvial deposits, 196
of glaciers, 266
of ocean bottom, 326
of shallow-water deposits, 374
youthful 86
Top-set beds, 202
Trachyte, 473
Transportation, 110
by glaciers, 281
by ocean currents, 367
by streams, 115, 119
by waves, 354
by wind, 22, 25
effect on rotation, 4
Tilden, W. A., 620
Tilhemic rocks, 457
Till, 473
Titanite, 467
Todd, J. E., 195
Topaz, 467
Topographic adjustment of streams, 162, 163, 197
Topographic effects of glacial erosion, 287
Topographic effects of ground-water, 231
Topographic map, explanation of, 30
Topographic maturity, 86
Topographic old age, 89
Topographic youth, 86
Topography, developed by river erosion, 92
dune, 32
landslide, 231
mature, 86
of alluvial deposits, 196
of glaciers, 266
of ocean bottom, 326
of shallow-water deposits, 374
youthful 86
Top-set beds, 202
Trachyte, 473
Transportation, 110
by glaciers, 281
by ocean currents, 367
by streams, 115, 119
by waves, 354
by wind, 22, 25
Page 824
Trap, 419, 473
Travertine, 473
Trees, uprooting of, 40
Tremolite, 447, 467
Tributaries, development of, 78
position of, 79
topographic adjustment of, 197
Tripoli, 661
Tripolite, 426
Trout creek, 193
Tschermak, G., 538
Tufa (see Tuffs)
Tufa cones, 611
Tufa deposits, 611
Tuffs, 404, 434, 473
Tuscarora deep, 548
Two Medicine River, 154, 157
Tyndall, J., and Huxley, T. H., 322
Udden, J. A., 22
Uinta Mountains, lateral moraines of, 303
Underground water (see Ground-water)
Undertow, 341
deposition by, 355
erosion by, 342, 347
United States Geological Survey, VI., 32
Upham, W., 388
Uprooting of trees, 40
Uralite, 431
Uruguay River, sediment carried by, 107
Travertine, 473
Trees, uprooting of, 40
Tremolite, 447, 467
Tributaries, development of, 78
position of, 79
topographic adjustment of, 197
Tripoli, 661
Tripolite, 426
Trout creek, 193
Tschermak, G., 538
Tufa (see Tuffs)
Tufa cones, 611
Tufa deposits, 611
Tuffs, 404, 434, 473
Tuscarora deep, 548
Two Medicine River, 154, 157
Tyndall, J., and Huxley, T. H., 322
Udden, J. A., 22
Uinta Mountains, lateral moraines of, 303
Underground water (see Ground-water)
Undertow, 341
deposition by, 355
erosion by, 342, 347
United States Geological Survey, VI., 32
Upham, W., 388
Uprooting of trees, 40
Uralite, 431
Uruguay River, sediment carried by, 107
Page 825
Usiglio, 375
Valleys,
affected by folds, 154
antecedent (see Streams, antecedent)
canoe-shaped, 155
consequent, 78
courses of, 77
development of, 63, 70, 73, 80
hanging, 164, 290
limits of growth, 67
oldest parts, 76
profiles of, 66
relations to lakes, 74
slopes of, 94
special forms of, 94
structural, 77
struggle for existence among, 100
Van Hise, C. R., 219, 434, 448, 474, 479, 504, 543, 555, 570
Vegetation,
effect on dunes, 29
effect on erosion, 131, 644
effect on sediments, 645
effect on weathering, 131
Veins, 223, 428, 511
Vermes, geologic contribution of, 662
Vermeule, C. C., 109
Vertebrata, geologic contribution of, 663
Vesuvius, 605
Virginia, natural bridge of, 156
Viridite, 467
Volcanic action, causes of, 623–633
activity, periodicity of, 607
ash, 23, 404, 592, 617
Valleys,
affected by folds, 154
antecedent (see Streams, antecedent)
canoe-shaped, 155
consequent, 78
courses of, 77
development of, 63, 70, 73, 80
hanging, 164, 290
limits of growth, 67
oldest parts, 76
profiles of, 66
relations to lakes, 74
slopes of, 94
special forms of, 94
structural, 77
struggle for existence among, 100
Van Hise, C. R., 219, 434, 448, 474, 479, 504, 543, 555, 570
Vegetation,
effect on dunes, 29
effect on erosion, 131, 644
effect on sediments, 645
effect on weathering, 131
Veins, 223, 428, 511
Vermes, geologic contribution of, 662
Vermeule, C. C., 109
Vertebrata, geologic contribution of, 663
Vesuvius, 605
Virginia, natural bridge of, 156
Viridite, 467
Volcanic action, causes of, 623–633
activity, periodicity of, 607
ash, 23, 404, 592, 617
Page 826
bombs, 406, 592, 617
cinders, 592
cones, 500
débris in sea, 381
dust (see Volcanic ash)
eruptions, 594
and atmospheric pressure, 606
and tidal strain, 607
types of, 593
gases, 617–623
action of, 617
kinds of, 618
proportions of, 620, 622
sources of, 619, 620, 621, 633
glass (see Obsidian)
in sea, 381
mud, 380
flows of, 610
neck, 500
plug, 500
rocks, 395–418
residual gases in, 619
smoke, 592, 617
Volcanoes, 599–611
coincidence in eruption of, 606
cones of, 608
distribution of, in curved lines, 603
distribution of, in latitude, 603
distribution of, in relation to crustal movements, 601, 604, 628
distribution of, in relation to land and sea, 599
distribution of, in time, 599
independence of, 605, 623
periodicity of, 607
relations of, 604–607
relations to one another, 605
Volume of ocean, 325
cinders, 592
cones, 500
débris in sea, 381
dust (see Volcanic ash)
eruptions, 594
and atmospheric pressure, 606
and tidal strain, 607
types of, 593
gases, 617–623
action of, 617
kinds of, 618
proportions of, 620, 622
sources of, 619, 620, 621, 633
glass (see Obsidian)
in sea, 381
mud, 380
flows of, 610
neck, 500
plug, 500
rocks, 395–418
residual gases in, 619
smoke, 592, 617
Volcanoes, 599–611
coincidence in eruption of, 606
cones of, 608
distribution of, in curved lines, 603
distribution of, in latitude, 603
distribution of, in relation to crustal movements, 601, 604, 628
distribution of, in relation to land and sea, 599
distribution of, in time, 599
independence of, 605, 623
periodicity of, 607
relations of, 604–607
relations to one another, 605
Volume of ocean, 325
Page 827
Vuggs, 437
Vulcanism, 2, 590–637
causes of, 623–633
effects on coast-lines, 332
in ocean, 332
Vulcanism and deep sedimentation, 629
ground-water, 635
rotation, 603
Wacke, 422, 473, 645
Wad, 467
Walcott, C. D., 194, 246, 371, 438, 440, 441, 502, 503, 509
Wallace, A. R., 665, 668
Walther, J., 50, 670
Warming, E., 667
Warping, effect of, on streams, 171
of earth’s crust, 526, 541, 542
Wasatch Mountains, lateral moraines of, 303
Washington, H. S., 412, 451, 573
Waste of glaciers, 273
Water (see Streams, Ground-water, Ocean, etc.)
amount of, 7
geologic activity of, 8
Water-gaps, 141, 167
Waterfalls, 132
development of, 133
Minnehaha, 137
Niagara, 139
Shoshone, 135
St. Anthony, 135
Upper Yosemite, 138
Yellowstone, 135
Vulcanism, 2, 590–637
causes of, 623–633
effects on coast-lines, 332
in ocean, 332
Vulcanism and deep sedimentation, 629
ground-water, 635
rotation, 603
Wacke, 422, 473, 645
Wad, 467
Walcott, C. D., 194, 246, 371, 438, 440, 441, 502, 503, 509
Wallace, A. R., 665, 668
Walther, J., 50, 670
Warming, E., 667
Warping, effect of, on streams, 171
of earth’s crust, 526, 541, 542
Wasatch Mountains, lateral moraines of, 303
Washington, H. S., 412, 451, 573
Waste of glaciers, 273
Water (see Streams, Ground-water, Ocean, etc.)
amount of, 7
geologic activity of, 8
Water-gaps, 141, 167
Waterfalls, 132
development of, 133
Minnehaha, 137
Niagara, 139
Shoshone, 135
St. Anthony, 135
Upper Yosemite, 138
Yellowstone, 135
Page 828
Waterfalls and sediment, 137
Water-lime, 473
Water-table, 71, 215
Water-vapor, climatic effects of, 643
Wave-built terraces, 363
Wave-cut terraces, 351, 352
Wave erosion, 342–354
range of, 346
topographic features developed by, 349
Wave erosion and horizontal configuration, 353, 363, 364
Wave-marks, 490
Wave-motion, 339
Waves, 339
deposition by, 355
erosion by, 342–354
force of, 344
transportation by, 354
work of, 342–366
Weathering, 54, 110, 226
affected by life, 644
aided by plants, 112
aided by hot vapors, 113
effect of gravity, 112
effect of joints, 151, 153
importance of, in valley growth, 114
Wedgework of ice, 45, 48, 150
of roots, 112, 131, 150
Weed, W. H., 225, 237, 474, 656
Wells,
artesian, 242
flowing, 234, 242, 243
Wheeling well, temperature of, 569
White glacier, 263
Water-lime, 473
Water-table, 71, 215
Water-vapor, climatic effects of, 643
Wave-built terraces, 363
Wave-cut terraces, 351, 352
Wave erosion, 342–354
range of, 346
topographic features developed by, 349
Wave erosion and horizontal configuration, 353, 363, 364
Wave-marks, 490
Wave-motion, 339
Waves, 339
deposition by, 355
erosion by, 342–354
force of, 344
transportation by, 354
work of, 342–366
Weathering, 54, 110, 226
affected by life, 644
aided by plants, 112
aided by hot vapors, 113
effect of gravity, 112
effect of joints, 151, 153
importance of, in valley growth, 114
Wedgework of ice, 45, 48, 150
of roots, 112, 131, 150
Weed, W. H., 225, 237, 474, 656
Wells,
artesian, 242
flowing, 234, 242, 243
Wheeling well, temperature of, 569
White glacier, 263
Page 829
Whitfield, J. E. (and Gooch, F. A.), 236
Williams, H. S., 658
Willis, B., 157, 168, 169, 257, 344, 355, 365, 516, 543, 550
Winchell, H. V., 474
Wind, abrasion by, 38
effects on plants, 40
movements of sea, generated by, 336
transports organisms, 41
work of, 21–41
Wind-blown dust, 22
Wind-blown sands, 25
Wind-ripples, 37
Winslow, A., 474
Wisconsin River, dells of, 152
Woodward, R. S., 560, 581
Work of glaciers, 281
Wyandotte Cave, 227, 228
Yazoo River, 188
Yellowstone Park,
geysers of, 238
hot springs of, 225
Yellowstone River,
canyon of, 100
falls of, 135
Yukon River, delta of, 202
Zeiller, 652
Zeolites, 428, 467
Zircon, 467
Zittel, K. von, 658, 659
Williams, H. S., 658
Willis, B., 157, 168, 169, 257, 344, 355, 365, 516, 543, 550
Winchell, H. V., 474
Wind, abrasion by, 38
effects on plants, 40
movements of sea, generated by, 336
transports organisms, 41
work of, 21–41
Wind-blown dust, 22
Wind-blown sands, 25
Wind-ripples, 37
Winslow, A., 474
Wisconsin River, dells of, 152
Woodward, R. S., 560, 581
Work of glaciers, 281
Wyandotte Cave, 227, 228
Yazoo River, 188
Yellowstone Park,
geysers of, 238
hot springs of, 225
Yellowstone River,
canyon of, 100
falls of, 135
Yukon River, delta of, 202
Zeiller, 652
Zeolites, 428, 467
Zircon, 467
Zittel, K. von, 658, 659
Page 830
Zone of fracture, 219, 427
Page 831
FOOTNOTES:
[1] The Earth. Johnson’s Encyclopædia. See also statement of Murray in Smithsonian An. Rept.,
1899, p. 312. Reprint from Brit. A. A. S., Dover meeting, 1899, and Scot. Geog. Mag., Vol.
XV, 1899, p. 511.
[2] Its specific gravity as a whole is about 5.57, and the specific gravity of its outer portion is
about 2.7.
[3] For an excellent study of the erosion, transportation, and sedimentation performed by the
atmosphere, see Udden, Jour. of Geol., Vol. II, pp. 318–331. See also Pop. Sci. Mo.,
September, 1896.
[4] The Eruption of Krakatoa. Committee of the Royal Society, 1888.
[5] A brief account of the influence of the dust on sunsets is found in Davis’s Elementary
Meteorology, pp. 85 and 119.
[6] Science, New Ser., Vol. IV, p. 816, 1896.
[7] Von Richtofen. “China.”
[8] Sketcherley and Kingsmill. Quar. Jour. Geol. Soc., Vol. LI, 1895, pp. 238–254.
[9] Chamberlin. Jour. of Geol., Vol. V, p. 795.
[10] A thoroughgoing study of the Formation of Sand Dunes (by V. Cornish) is to be found in the
Geog. Jour., Vol. IX, 1897, pp. 278–309.
[11] Blanford. Geology of India, 2d ed., p. 455 et seq.
[12] Cornish, loc. cit.
[13] Cornish, loc. cit., p. 294.
[14] Diller states (17th Ann. Rept., U. S. Geol. Surv., Pt. I, p. 450) that on the coast of Oregon the
slope of dunes is sometimes 40°.
[15] From folio preface, U. S. Geol. Surv.
[16] Credner. Elemente der Geologie, 6th ed., p. 271.
[17] Merrill. Rocks, Rock Weathering, and Soils, p. 295.
[18] Cowles. The Ecological Relations of the Vegetation of the Sand Dunes of Lake Michigan.
Botanical Gazette, Vol. XXVII, 1899. An excellent study of the relations of sand dunes and
vegetation.
[19] For example, in the Big Horn Mountains of Wyoming.
[20] It should be noted that it is the change of temperature of the rock surface, not the change of
temperature of the air above it, which is to be considered. Many data concerning temperature
changes are to be found in Bartholomew’s Atlas of Meteorology.
[21] Buckley. Wisconsin Survey, Bull. IV, 1899, pp. 81–3.
[22] Livingstone has reported that the temperature of rock surfaces in Africa sometimes reaches
137° Fahr. during the day, and cools sufficiently at night to split off blocks of 200 lbs. weight.
[23] Buckley. Surv. of Wis., Bull. IV, pp. 19, 20.
[1] The Earth. Johnson’s Encyclopædia. See also statement of Murray in Smithsonian An. Rept.,
1899, p. 312. Reprint from Brit. A. A. S., Dover meeting, 1899, and Scot. Geog. Mag., Vol.
XV, 1899, p. 511.
[2] Its specific gravity as a whole is about 5.57, and the specific gravity of its outer portion is
about 2.7.
[3] For an excellent study of the erosion, transportation, and sedimentation performed by the
atmosphere, see Udden, Jour. of Geol., Vol. II, pp. 318–331. See also Pop. Sci. Mo.,
September, 1896.
[4] The Eruption of Krakatoa. Committee of the Royal Society, 1888.
[5] A brief account of the influence of the dust on sunsets is found in Davis’s Elementary
Meteorology, pp. 85 and 119.
[6] Science, New Ser., Vol. IV, p. 816, 1896.
[7] Von Richtofen. “China.”
[8] Sketcherley and Kingsmill. Quar. Jour. Geol. Soc., Vol. LI, 1895, pp. 238–254.
[9] Chamberlin. Jour. of Geol., Vol. V, p. 795.
[10] A thoroughgoing study of the Formation of Sand Dunes (by V. Cornish) is to be found in the
Geog. Jour., Vol. IX, 1897, pp. 278–309.
[11] Blanford. Geology of India, 2d ed., p. 455 et seq.
[12] Cornish, loc. cit.
[13] Cornish, loc. cit., p. 294.
[14] Diller states (17th Ann. Rept., U. S. Geol. Surv., Pt. I, p. 450) that on the coast of Oregon the
slope of dunes is sometimes 40°.
[15] From folio preface, U. S. Geol. Surv.
[16] Credner. Elemente der Geologie, 6th ed., p. 271.
[17] Merrill. Rocks, Rock Weathering, and Soils, p. 295.
[18] Cowles. The Ecological Relations of the Vegetation of the Sand Dunes of Lake Michigan.
Botanical Gazette, Vol. XXVII, 1899. An excellent study of the relations of sand dunes and
vegetation.
[19] For example, in the Big Horn Mountains of Wyoming.
[20] It should be noted that it is the change of temperature of the rock surface, not the change of
temperature of the air above it, which is to be considered. Many data concerning temperature
changes are to be found in Bartholomew’s Atlas of Meteorology.
[21] Buckley. Wisconsin Survey, Bull. IV, 1899, pp. 81–3.
[22] Livingstone has reported that the temperature of rock surfaces in Africa sometimes reaches
137° Fahr. during the day, and cools sufficiently at night to split off blocks of 200 lbs. weight.
[23] Buckley. Surv. of Wis., Bull. IV, pp. 19, 20.
Page 832
[24] For an excellent discussion of erosion in dry regions see Walther’s Die Denudation in der
Wüste.
[25] On the assumption that condensation takes place at an average elevation of 3000 feet, it has
been estimated that the force necessary to evaporate and diffuse the moisture which falls as
rain and snow would be equivalent to 300,000,000,000 horse-power constantly in operation.
(Strachey, Lectures on Geography, p. 145.)
[26] McGee. Bull. Geol. Soc. Am., Vol. VIII, pp. 87–112.
[27] For a discussion of convex and concave erosion slopes see Bain, Geol. Surv. of Ia., Vol. VI, p.
449.
[28] Great rivers, like the Mississippi, cut their channels somewhat below sea-level, but probably
not by an amount exceeding the depth of the stream itself (see p. 79).
[29] Davis. Jour. of Geol., Vol. X, p. 87.
[30] Ibid., p. 77 et seq.
[31] In regions where canyons are common, the term is often applied to all valleys.
[32] Humphreys and Abbot. Physics and Hydraulics of the Mississippi River.
[33] From Russell’s Rivers of North America, p. 78.
[34] Alkaline carbonates considered as sodium carbonates.
[35] Carbonic acid by difference.
[36] Babb. Science, Vol. XXI, p. 343. 1893.
[37] Quoted by Mason. Water-supply, p. 204.
[38] Sot. Geog. Mag., Vol. III, p. 76. 1887.
[39] Acids and bases combined according to the principles indicated by Bunsen.
[40] Chemical Geology, Vol. I, pp. 76, 77, English ed., 1854.
[41] Allgemeine und chemische Geologie, Vol. I, pp. 456, 457. 1879.
[42] Russell. Rivers of North America, p. 79.
[43] For disastrous floods of the lower Mississippi, see Johnson, Bull. Geol. Soc. Am., Vol. II, pp.
20–25. For effect of precipitation and forests on floods, see Russell’s Meteorology, pp. 198–
217, and Vermeule, Report on Water Supply, Geol. Surv. of N. J.
[44] An excellent discussion of this subject is given by Gilbert in The Henry Mountains, pp. 99 et
seq., and more briefly in the Am. Jour. Sci., Vol. XII, p. 85 et seq. 1876.
[45] Jour. of Geol., Vol. IV, p. 718. An excellent summary of the principles of Rock Weathering.
[46] Russell. Rivers of North America, p. 17.
[47] W. G. Thompson. Nature, Vol. I, p. 555, 1870. The Matapediac River, N. B. Cited by Russell
in Rivers of North America, p. 25.
[48] Dutton. Tertiary History of the Grand Canyon District, Mono. II, U. S. Geological Survey.
[49] The terms rapids, falls, and cataracts are rather loosely used. Many moderate rapids are
incorrectly called falls. The “Falls of the Ohio” is an example. The term cataract is often
applied to very steep rapids or falls.
[50] Gilbert, article on Niagara Falls, in Physiography of the United States.
[51] Gilbert. Am. Jour. Sci., Vol. XII. p. 99, 1876.
Wüste.
[25] On the assumption that condensation takes place at an average elevation of 3000 feet, it has
been estimated that the force necessary to evaporate and diffuse the moisture which falls as
rain and snow would be equivalent to 300,000,000,000 horse-power constantly in operation.
(Strachey, Lectures on Geography, p. 145.)
[26] McGee. Bull. Geol. Soc. Am., Vol. VIII, pp. 87–112.
[27] For a discussion of convex and concave erosion slopes see Bain, Geol. Surv. of Ia., Vol. VI, p.
449.
[28] Great rivers, like the Mississippi, cut their channels somewhat below sea-level, but probably
not by an amount exceeding the depth of the stream itself (see p. 79).
[29] Davis. Jour. of Geol., Vol. X, p. 87.
[30] Ibid., p. 77 et seq.
[31] In regions where canyons are common, the term is often applied to all valleys.
[32] Humphreys and Abbot. Physics and Hydraulics of the Mississippi River.
[33] From Russell’s Rivers of North America, p. 78.
[34] Alkaline carbonates considered as sodium carbonates.
[35] Carbonic acid by difference.
[36] Babb. Science, Vol. XXI, p. 343. 1893.
[37] Quoted by Mason. Water-supply, p. 204.
[38] Sot. Geog. Mag., Vol. III, p. 76. 1887.
[39] Acids and bases combined according to the principles indicated by Bunsen.
[40] Chemical Geology, Vol. I, pp. 76, 77, English ed., 1854.
[41] Allgemeine und chemische Geologie, Vol. I, pp. 456, 457. 1879.
[42] Russell. Rivers of North America, p. 79.
[43] For disastrous floods of the lower Mississippi, see Johnson, Bull. Geol. Soc. Am., Vol. II, pp.
20–25. For effect of precipitation and forests on floods, see Russell’s Meteorology, pp. 198–
217, and Vermeule, Report on Water Supply, Geol. Surv. of N. J.
[44] An excellent discussion of this subject is given by Gilbert in The Henry Mountains, pp. 99 et
seq., and more briefly in the Am. Jour. Sci., Vol. XII, p. 85 et seq. 1876.
[45] Jour. of Geol., Vol. IV, p. 718. An excellent summary of the principles of Rock Weathering.
[46] Russell. Rivers of North America, p. 17.
[47] W. G. Thompson. Nature, Vol. I, p. 555, 1870. The Matapediac River, N. B. Cited by Russell
in Rivers of North America, p. 25.
[48] Dutton. Tertiary History of the Grand Canyon District, Mono. II, U. S. Geological Survey.
[49] The terms rapids, falls, and cataracts are rather loosely used. Many moderate rapids are
incorrectly called falls. The “Falls of the Ohio” is an example. The term cataract is often
applied to very steep rapids or falls.
[50] Gilbert, article on Niagara Falls, in Physiography of the United States.
[51] Gilbert. Am. Jour. Sci., Vol. XII. p. 99, 1876.
Page 833
[52] For a brief account of this fall see Gilbert in Physiography of the United States.
[53] Gilbert. Science, Vol. VIII, p. 205, 1886.
[54] See Campbell, Jour. Geol., Vol. IV, pp. 567, 657.
[55] Russell. Rivers of North America, p. 280. The influence of joints on drainage is further
discussed by Hobbs, Jour. Geol., Vol. IX, p. 469.
[56] See Willis. The Northern Appalachians, in Physiography of the United States.
[57] This process of adjustment has been well described by Davis in The Rivers and Valleys of
Pennsylvania, Natl. Geog. Mag., Vol. I, p. 211 et seq.
[58] This sort of adjustment may be called topographic adjustment. A tributary is in topographic
adjustment when its gradient is harmonious with that of its main.
[59] Davis. The Seine, the Meuse and the Moselle. Nat’l Geog. Mag., Vol. VII, pp. 181–202, and
228–238. An article which throws much light on the behavior of rivers.
[60] Another view has been advocated by Tarr, Am. Geol. Vol. XXI, pp. 351–370.
[61] Campbell. Bull. Geol. Soc. of Am., Vol. XIV, p. 277.
[62] Willis. Physiography of the United States. The Northern Appalachians.
[62a] Willis. Physiography of the United States. The Northern Appalachians.
[63] For excellent accounts of the rivers of the Appalachian Mountains see Davis, Rivers of
Northern New Jersey, Nat’l Geog. Mag., Vol. II, pp. 81–110; and Rivers of Pennsylvania, op.
cit., pp. 183–253; Willis, The Northern Appalachians, Physiography of the United States, pp.
169–202; Hayes, the Southern Appalachians, op. cit., pp. 305–336; Hayes and Campbell, The
Geomorphology of the Southern Appalachians, Nat’l Geog. Mag., Vol. VI, pp. 63–126, and
Hayes, Physiography of the Chattanooga District, 19th Ann. Rep. U. S. Geol. Surv., Pt. II, pp.
1–58.
[64] This is the case at Davis and Lone Star. Capt Howell, Miss. Riv. Commission.
[65] Russell. Rivers of North America, p. 279.
[66] Russell. Rivers of North America, p. 279.
[67] Hayes. Physiography of the Chattanooga District, 19th Ann. Rep., U. S. Geol. Surv., Pt. II, pp.
9–58. See, also, Hayes and Campbell, Geomorphology of the Southern Appalachians, Nat’l
Geog. Mag., Vol. VI, pp. 63–126.
[68] Figs. 165–168 are based on reports of Hayes, and Hayes and Campbell, already referred to.
Drawn by E. S. Bastin.
[69] A question might be raised in this case as to what should be called the source. A spring issues
from beneath the surface and flows away in a stream. The stream is said to begin where the
water appears at the surface, though in some cases the water of the spring was a subsurface
stream before it reached the surface. Water escaping from beneath a glacier as a stream may
likewise be considered a spring at the point of its issue.
[70] Davis. Science, Vol. X, p. 142, 1887.
[71] L. C. Johnson. Bull. Geol. Soc. Am., Vol. II, pp. 20–25, 1891.
[72] Jefferson. Nat’l Geog. Mag., Vol. XIII, pp. 373–84.
[73] According to map published by the Mississippi River Commission in 1887.
[74] Russell. Rivers of North America, p. 114.
[75] Gilbert. Am. Jour. Sci., Vol. XXVII, 1884, pp. 427–34.
[53] Gilbert. Science, Vol. VIII, p. 205, 1886.
[54] See Campbell, Jour. Geol., Vol. IV, pp. 567, 657.
[55] Russell. Rivers of North America, p. 280. The influence of joints on drainage is further
discussed by Hobbs, Jour. Geol., Vol. IX, p. 469.
[56] See Willis. The Northern Appalachians, in Physiography of the United States.
[57] This process of adjustment has been well described by Davis in The Rivers and Valleys of
Pennsylvania, Natl. Geog. Mag., Vol. I, p. 211 et seq.
[58] This sort of adjustment may be called topographic adjustment. A tributary is in topographic
adjustment when its gradient is harmonious with that of its main.
[59] Davis. The Seine, the Meuse and the Moselle. Nat’l Geog. Mag., Vol. VII, pp. 181–202, and
228–238. An article which throws much light on the behavior of rivers.
[60] Another view has been advocated by Tarr, Am. Geol. Vol. XXI, pp. 351–370.
[61] Campbell. Bull. Geol. Soc. of Am., Vol. XIV, p. 277.
[62] Willis. Physiography of the United States. The Northern Appalachians.
[62a] Willis. Physiography of the United States. The Northern Appalachians.
[63] For excellent accounts of the rivers of the Appalachian Mountains see Davis, Rivers of
Northern New Jersey, Nat’l Geog. Mag., Vol. II, pp. 81–110; and Rivers of Pennsylvania, op.
cit., pp. 183–253; Willis, The Northern Appalachians, Physiography of the United States, pp.
169–202; Hayes, the Southern Appalachians, op. cit., pp. 305–336; Hayes and Campbell, The
Geomorphology of the Southern Appalachians, Nat’l Geog. Mag., Vol. VI, pp. 63–126, and
Hayes, Physiography of the Chattanooga District, 19th Ann. Rep. U. S. Geol. Surv., Pt. II, pp.
1–58.
[64] This is the case at Davis and Lone Star. Capt Howell, Miss. Riv. Commission.
[65] Russell. Rivers of North America, p. 279.
[66] Russell. Rivers of North America, p. 279.
[67] Hayes. Physiography of the Chattanooga District, 19th Ann. Rep., U. S. Geol. Surv., Pt. II, pp.
9–58. See, also, Hayes and Campbell, Geomorphology of the Southern Appalachians, Nat’l
Geog. Mag., Vol. VI, pp. 63–126.
[68] Figs. 165–168 are based on reports of Hayes, and Hayes and Campbell, already referred to.
Drawn by E. S. Bastin.
[69] A question might be raised in this case as to what should be called the source. A spring issues
from beneath the surface and flows away in a stream. The stream is said to begin where the
water appears at the surface, though in some cases the water of the spring was a subsurface
stream before it reached the surface. Water escaping from beneath a glacier as a stream may
likewise be considered a spring at the point of its issue.
[70] Davis. Science, Vol. X, p. 142, 1887.
[71] L. C. Johnson. Bull. Geol. Soc. Am., Vol. II, pp. 20–25, 1891.
[72] Jefferson. Nat’l Geog. Mag., Vol. XIII, pp. 373–84.
[73] According to map published by the Mississippi River Commission in 1887.
[74] Russell. Rivers of North America, p. 114.
[75] Gilbert. Am. Jour. Sci., Vol. XXVII, 1884, pp. 427–34.
Page 834
[76] Cooley. Rept. U. S. Engineers for 1879–80, Pt. II, pp. 1060 and 1071.
[77] Gerber. Cited by Todd. Bull. 158, U. S. Geol. Surv., pp. 150, 151.
[78] Chamberlin. Jour. of Geol., Vol. X, pp. 747–754.
[79] For an excellent discussion of deltas, see Gilbert, Fifth Ann. Rept. U. S. Geol. Surv., pp 104–
8. Also Lake Bonneville, Monograph I, U. S. Geol. Surv. (same article).
[80] Davis. Physical Geography, p. 294.
[81] Humphreys and Abbot. Physics and Hydraulics of the Mississippi River.
[82] Corthell. Nat’l Geog. Mag., Vol. VIII, p. 351, 1897.
[83] Russell. Rivers of North America, p. 132.
[84] Prestwich. Chemical and Physical Geology, Vol. I, p. 85.
[85] Geike. Text-book of Geology, 3d ed., p. 402.
[86] Medlicott and Blanford, Geology of India. Chap. XVII; Medlicott, Records of the Geological
Survey of India, 1881; Oldham, Geology of India, 2d ed., Chap. XVII; and Ferguson, Q. J. G.
S., Vol. XIX, pp. 321–54. The extent of this and other deltas is variously stated, probably
because it is difficult to determine the exact position of its head and borders.
[87] Dana. Manual of Geology, 4th ed., p. 198.
[88] Salisbury and Kümmel. Lake Passaic. Ann. Rept. of the State Geologist of New Jersey, 1893,
and Jour. of Geol., Vol. III. p. 533.
[89] Gilbert. Lake Bonneville, Mono. I, U. S. Geol. Surv.
[90] For discussions of terraces see Gilbert’s Henry Mountains, p. 126; Davis’ River Terraces in
New England, Bull. of the Mus. of Comp. Zool., Geol. Series, Vol. V, pp. 282–346; and
Dodge, Proc. Boston Soc. of Nat. Hist., Vol. XXVI, pp. 257–73.
[91] Davis, Bull. Mus. Comp. Zool., Geol. Ser., Vol. V.
[92] This point has recently been emphasized by Davis, loc. cit., pp. 282–346.
[93] Murray. Scot. Geog. Mag., Vol. III, p. 70, 1887.
[94] Hoskins. 16th Ann. Rept., U. S. Geol. Surv., p. 853.
[95] Van Hise. Principles of North American Pre-Cambrian Geology, 16th Ann. Rept., U. S. Geol.
Surv.
[96] For a full discussion of this subject see King, 19th Ann. Rept., U. S. Geol. Surv., Pt. II, and
Slichter, Water Supply and Irrigation, Paper No. 67, U. S. Geol. Surv.
[97] For tables see Buckley, Building and Ornamental Stones, Bull. IV, Wis. Surv., and Merrill,
Stones for Building and Decoration, and various Survey Reports.
[98] It is probable that the porosity decreases in more than an arithmetic ratio, both because the
deeper rocks are not of porous kinds, and because of the pressure which tends to close
openings.
[99] Slichter (op. cit., p. 15) estimates that the ground-water is sufficient in amount to cover the
earth’s surface to a depth of 3000 to 3500 feet. Earlier estimates gave still higher figures (see
Delesse, Bull. Soc. Geol., France, Second Series, Vol. XIX, 1861–62, p. 64).
[100] Geikie. Text-book of Geology, 3d ed., p. 367.
[101] Ibid., p. 378.
[102] Prestwich, Q. J. Geol. Soc., Vol. XXVIII, p. lxvii.
[77] Gerber. Cited by Todd. Bull. 158, U. S. Geol. Surv., pp. 150, 151.
[78] Chamberlin. Jour. of Geol., Vol. X, pp. 747–754.
[79] For an excellent discussion of deltas, see Gilbert, Fifth Ann. Rept. U. S. Geol. Surv., pp 104–
8. Also Lake Bonneville, Monograph I, U. S. Geol. Surv. (same article).
[80] Davis. Physical Geography, p. 294.
[81] Humphreys and Abbot. Physics and Hydraulics of the Mississippi River.
[82] Corthell. Nat’l Geog. Mag., Vol. VIII, p. 351, 1897.
[83] Russell. Rivers of North America, p. 132.
[84] Prestwich. Chemical and Physical Geology, Vol. I, p. 85.
[85] Geike. Text-book of Geology, 3d ed., p. 402.
[86] Medlicott and Blanford, Geology of India. Chap. XVII; Medlicott, Records of the Geological
Survey of India, 1881; Oldham, Geology of India, 2d ed., Chap. XVII; and Ferguson, Q. J. G.
S., Vol. XIX, pp. 321–54. The extent of this and other deltas is variously stated, probably
because it is difficult to determine the exact position of its head and borders.
[87] Dana. Manual of Geology, 4th ed., p. 198.
[88] Salisbury and Kümmel. Lake Passaic. Ann. Rept. of the State Geologist of New Jersey, 1893,
and Jour. of Geol., Vol. III. p. 533.
[89] Gilbert. Lake Bonneville, Mono. I, U. S. Geol. Surv.
[90] For discussions of terraces see Gilbert’s Henry Mountains, p. 126; Davis’ River Terraces in
New England, Bull. of the Mus. of Comp. Zool., Geol. Series, Vol. V, pp. 282–346; and
Dodge, Proc. Boston Soc. of Nat. Hist., Vol. XXVI, pp. 257–73.
[91] Davis, Bull. Mus. Comp. Zool., Geol. Ser., Vol. V.
[92] This point has recently been emphasized by Davis, loc. cit., pp. 282–346.
[93] Murray. Scot. Geog. Mag., Vol. III, p. 70, 1887.
[94] Hoskins. 16th Ann. Rept., U. S. Geol. Surv., p. 853.
[95] Van Hise. Principles of North American Pre-Cambrian Geology, 16th Ann. Rept., U. S. Geol.
Surv.
[96] For a full discussion of this subject see King, 19th Ann. Rept., U. S. Geol. Surv., Pt. II, and
Slichter, Water Supply and Irrigation, Paper No. 67, U. S. Geol. Surv.
[97] For tables see Buckley, Building and Ornamental Stones, Bull. IV, Wis. Surv., and Merrill,
Stones for Building and Decoration, and various Survey Reports.
[98] It is probable that the porosity decreases in more than an arithmetic ratio, both because the
deeper rocks are not of porous kinds, and because of the pressure which tends to close
openings.
[99] Slichter (op. cit., p. 15) estimates that the ground-water is sufficient in amount to cover the
earth’s surface to a depth of 3000 to 3500 feet. Earlier estimates gave still higher figures (see
Delesse, Bull. Soc. Geol., France, Second Series, Vol. XIX, 1861–62, p. 64).
[100] Geikie. Text-book of Geology, 3d ed., p. 367.
[101] Ibid., p. 378.
[102] Prestwich, Q. J. Geol. Soc., Vol. XXVIII, p. lxvii.
Page 835
[103] Reade. Liverpool Geol. Soc., 1876 and 1884.
[104] This is not true in the case of minerals, such as lime carbonate, dissolved under the influence
of gases in solution in the water.
[105] Weed. The Formation of Hot Springs Deposits. Excursion to the Rocky Mountains. Compte
Rendu. Fifth Session of the International Geological Congress, p. 360, and Ninth Ann. Rept.
U. S. Geol. Surv., pp. 613–76. Also B. M. Davis, Science, Vol. VI, pp. 145–57, 1897.
[106] For a racy and interesting account of caverns see Shaler’s Aspects of the Earth.
[107] Russell has emphasized this point in 20th Ann. U. S. Geol. Surv., Pt. II, pp. 193–202, and
Cross, 21st Ann. U. S. Geol. Surv., Part II, pp. 129–150.
[108] Gooch and Whitfield. Bull. 47, U. S. Geol. Surv.
[109] Copied from Russell, Mono., XI. U. S. Geol. Surv., p. 176.
[110] Correction for specific gravity only approximate, as specific gravity was not given in original
analyses.
[111] As carbonates.
[112] As carbonate.
[113] As oxide.
[114] As carbonate.
[115] As sodium chloride.
[116] As fluoride of calcium.
[117] Oxygen added to SiO2 to form SiO3 of Na2SiO3.
[118] Liters of gas thrown off per liter of water.
[119] Weed. Ninth Ann. Rept. U. S. Geol. Surv., pp. 613–76, and Am. Jour. Sci., Vol. XXXVII,
1889, pp. 351–59.
[120] Geikie. Geological Sketches, pp. 206–38. Hayden. Amer. Jour. Sci., Vol. III, 1872, pp. 105–15
and 161–76.
[121] Chamberlin. Geol. of Wis., Vol. I, pp. 689–97, and Fifth Ann. Rept., U. S. Geol. Surv., pp.
131–73. The former a brief, and the latter an elaborate, exposition of the principles involved.
[122] Russell. Nat’l Geog. Mag., Vol. III, pp. 127 and 181.
[123] For an account of experiments illustrating the mobility of ice see Aitkin, Am. Jour. Sci., Vols.
V, p. 303, and XXXIV, p. 149, and Nature, Vol. XXXIX, p. 203.
[124] Jour. of Geol., Vol. III, p. 888.
[125] The following list includes many of the more available articles and treatises on existing
glaciers; others are referred to in the following pages.
Alaskan glaciers: Reid, (1) Nat. Geog. Mag., Vol. IV, pp. 19–55; (2) Sixteenth Ann. Rept.,
U. S. Geol. Surv., Part I, pp. 421–461. Russell, (1) Nat. Geog. Mag., Vol. III, pp. 176–188; (2)
Jour. of Geol., Vol. I, pp. 219–245.
Glaciers in the United States: Russell, (1) Fifth Ann. Rept., U. S. Geol. Surv., pp. 309–355;
(2) Eighteenth Ann. Rept., U. S. Geol. Surv., Part II, pp. 379–409; (3) Glaciers of North
America.
Greenland glaciers: Chamberlin, Jour. of Geol., Vol. II, pp. 768–788; Vol. III, pp. 61–69,
198–218, 469–480, 565–582, 668–681, and 833–843; Vol. IV, pp. 582–592. Salisbury, Jour. of
[104] This is not true in the case of minerals, such as lime carbonate, dissolved under the influence
of gases in solution in the water.
[105] Weed. The Formation of Hot Springs Deposits. Excursion to the Rocky Mountains. Compte
Rendu. Fifth Session of the International Geological Congress, p. 360, and Ninth Ann. Rept.
U. S. Geol. Surv., pp. 613–76. Also B. M. Davis, Science, Vol. VI, pp. 145–57, 1897.
[106] For a racy and interesting account of caverns see Shaler’s Aspects of the Earth.
[107] Russell has emphasized this point in 20th Ann. U. S. Geol. Surv., Pt. II, pp. 193–202, and
Cross, 21st Ann. U. S. Geol. Surv., Part II, pp. 129–150.
[108] Gooch and Whitfield. Bull. 47, U. S. Geol. Surv.
[109] Copied from Russell, Mono., XI. U. S. Geol. Surv., p. 176.
[110] Correction for specific gravity only approximate, as specific gravity was not given in original
analyses.
[111] As carbonates.
[112] As carbonate.
[113] As oxide.
[114] As carbonate.
[115] As sodium chloride.
[116] As fluoride of calcium.
[117] Oxygen added to SiO2 to form SiO3 of Na2SiO3.
[118] Liters of gas thrown off per liter of water.
[119] Weed. Ninth Ann. Rept. U. S. Geol. Surv., pp. 613–76, and Am. Jour. Sci., Vol. XXXVII,
1889, pp. 351–59.
[120] Geikie. Geological Sketches, pp. 206–38. Hayden. Amer. Jour. Sci., Vol. III, 1872, pp. 105–15
and 161–76.
[121] Chamberlin. Geol. of Wis., Vol. I, pp. 689–97, and Fifth Ann. Rept., U. S. Geol. Surv., pp.
131–73. The former a brief, and the latter an elaborate, exposition of the principles involved.
[122] Russell. Nat’l Geog. Mag., Vol. III, pp. 127 and 181.
[123] For an account of experiments illustrating the mobility of ice see Aitkin, Am. Jour. Sci., Vols.
V, p. 303, and XXXIV, p. 149, and Nature, Vol. XXXIX, p. 203.
[124] Jour. of Geol., Vol. III, p. 888.
[125] The following list includes many of the more available articles and treatises on existing
glaciers; others are referred to in the following pages.
Alaskan glaciers: Reid, (1) Nat. Geog. Mag., Vol. IV, pp. 19–55; (2) Sixteenth Ann. Rept.,
U. S. Geol. Surv., Part I, pp. 421–461. Russell, (1) Nat. Geog. Mag., Vol. III, pp. 176–188; (2)
Jour. of Geol., Vol. I, pp. 219–245.
Glaciers in the United States: Russell, (1) Fifth Ann. Rept., U. S. Geol. Surv., pp. 309–355;
(2) Eighteenth Ann. Rept., U. S. Geol. Surv., Part II, pp. 379–409; (3) Glaciers of North
America.
Greenland glaciers: Chamberlin, Jour. of Geol., Vol. II, pp. 768–788; Vol. III, pp. 61–69,
198–218, 469–480, 565–582, 668–681, and 833–843; Vol. IV, pp. 582–592. Salisbury, Jour. of
Page 836
Geol., Vol. III, pp. 875–902, and Vol. IV, pp. 769–810.
Glaciers in general: Shaler and Davis, Illustrations of the Earth’s Surface; Forbes, Norway
and its Glaciers, and Theory of Glaciers; Heim, Handbuch der Gletscherkunde.
[126] Reid. Natl. Geog. Mag., Vol. IV, p. 44.
[127] Rink’s Greenland.
[128] Reid. Variations of Glaciers. Jour. of Geol., Vols. III, p. 278; V, p. 378; VI, p. 473; VII, p. 217;
VIII, p. 154; IX, p. 250, and X, p. 313.
[129] For example, in the Middle Blase Dale glacier, Island of Disco, Jour. of Geol., Vol. II, p. 784,
and in the Bowdoin glacier (Fig. 242).
[130] Centimeter-gramme-second system. The rate of conductivity has not been very accurately
determined.
[131] Russell. Jour. of Geol., Vol. III, p. 823.
[132] Geikie. The Great Ice Age, 3d ed., p. 529.
[133] Carried out by C. E. Peet and E. C. Perisho under the direction of one of the authors.
[134] Ueber die Plasticität der Eiskrystalle. Neues Jahrbuch für Mineralogie, etc., 1895, Bd. II, p.
211.
[135] On the Plasticity of Glaciers and other Ice. Proc. Roy. Soc., Vol. XLIV, 1888, pp. 331–67
(with D. A. Kidd); Vol. XLVIII, 1890, pp. 259, 260; Vol. XLIX, 1891, pp. 323–43.
[136] Grönland-Expedition der Gesellschaft für Erdkunde zu Berlin, 1891–93, Bd. I, p. 491 et seq.
[137] References on glacier structure and motion.—L. Agassiz, Études sur les Glaciers, Neuchâtel,
1840. Rendu, Théorie des Glaciers de la Savoie, Soc. Roy. Acad., Savoie, Mém. 1840 (in
English, ed. by Geo. Forbes, London, 1874). J. de Charpentier, Essai sur les Glaciers et le
terrain erratique du Basin du Rhone, Lausanne, 1841. F. J. Hugi, Ueber das Wesen der
Gletscher und Wintereise in dem Eismeer, Stuttgart, 1842. R. Mallet, The Mechanism of
Glaciers, Jour. Geol. Soc. Dublin, Vol. I, p. 317; On the Plasticity of Glacier Ice, Jour. Geol.
Soc. Dublin, 1845, Vol. III, p. 122; On the Brittleness and Non-plasticity of Glacier Ice, Phil.
Mag., XXVI, p. 586. James Thompson, On the Plasticity of Ice as Manifested in Glaciers,
Roy. Soc. Proc., Vol. 8, 1857, pp. 455–58. J. Tyndall and T. H. Huxley, On the Structure and
Motion of Glaciers, Phil. Trans., 1857, Vol. CXLVII, p. 327. J. D. Forbes, Occasional Papers
on the Theory of Glaciers, Edinburgh, 1859. W. Hopkins, On the Theory of the Motion of
Glaciers, Phil. Trans., 1862, p. 677; Phil. Mag., 1863, Vol. XXV, p. 224. J. Tyndall, Forms of
Water, New York, 1872; The Glaciers of the Alps, London, 1861. James Croll, On the
Physical Cause of the Motion of Glaciers, Phil. Mag., 1869, Vol. 38, pp. 201–6. A. Heim, On
Glaciers, Phil. Mag., 1871, Vol. 41, pp. 485–508; Handbuch der Gletscherkunde, 1885. H.
Moseley, On the Cause of the Descent of Glaciers, Br. Assoc. Rept., 1860, Pt. 2, p. 48; also
Phil. Mag., 1869, Vol. 37, pp. 229, 363; Vol. 39, p. 241; Vol. 42, p. 138; Vol. 43, p. 38. Ch.
Grad, La Constitution et le movement des Glaciers, Revue Sci., 1872. H. J. Rink, Danish
Greenland, 1877. R. M. Deeley, A Theory of Glacial Motion, Phil. Mag., 1888, Vol. 25, pp.
136–64. J. C. McConnel, On the Plasticity of an Ice Crystal, Proc. Roy. Soc. London, Vol. 48,
1890, pp. 256–60; ibid., Vol. 49, 1891, pp. 323–43. O. Mügge, Über die Plasticität der
Eiskrystalle, Nachr. k. Ges. d. Wiss., Göttingen, 1895, pp. 1–4. R. M. Deeley and George
Fletcher, The Structure of Glacier Ice and its Bearings on Glacier Motion, Geol. Mag.
(London), Decade 4, Vol. 2, 1895, pp. 152–62. T. C. Chamberlin, Presidential address before
the Geol. Soc. Am., Bull. Geol. Soc. Am., Vol. VI, February 1895, pp. 199–220. Reid,
Mechanics of Glaciers, Jour. Geol., Vol. IV, 1896, p. 912. Erich von Drygalski, Grönland-
Expedition der Gesellschaft für Erdkunde zu Berlin, 1891–93, Vol. I, 1897.
Glaciers in general: Shaler and Davis, Illustrations of the Earth’s Surface; Forbes, Norway
and its Glaciers, and Theory of Glaciers; Heim, Handbuch der Gletscherkunde.
[126] Reid. Natl. Geog. Mag., Vol. IV, p. 44.
[127] Rink’s Greenland.
[128] Reid. Variations of Glaciers. Jour. of Geol., Vols. III, p. 278; V, p. 378; VI, p. 473; VII, p. 217;
VIII, p. 154; IX, p. 250, and X, p. 313.
[129] For example, in the Middle Blase Dale glacier, Island of Disco, Jour. of Geol., Vol. II, p. 784,
and in the Bowdoin glacier (Fig. 242).
[130] Centimeter-gramme-second system. The rate of conductivity has not been very accurately
determined.
[131] Russell. Jour. of Geol., Vol. III, p. 823.
[132] Geikie. The Great Ice Age, 3d ed., p. 529.
[133] Carried out by C. E. Peet and E. C. Perisho under the direction of one of the authors.
[134] Ueber die Plasticität der Eiskrystalle. Neues Jahrbuch für Mineralogie, etc., 1895, Bd. II, p.
211.
[135] On the Plasticity of Glaciers and other Ice. Proc. Roy. Soc., Vol. XLIV, 1888, pp. 331–67
(with D. A. Kidd); Vol. XLVIII, 1890, pp. 259, 260; Vol. XLIX, 1891, pp. 323–43.
[136] Grönland-Expedition der Gesellschaft für Erdkunde zu Berlin, 1891–93, Bd. I, p. 491 et seq.
[137] References on glacier structure and motion.—L. Agassiz, Études sur les Glaciers, Neuchâtel,
1840. Rendu, Théorie des Glaciers de la Savoie, Soc. Roy. Acad., Savoie, Mém. 1840 (in
English, ed. by Geo. Forbes, London, 1874). J. de Charpentier, Essai sur les Glaciers et le
terrain erratique du Basin du Rhone, Lausanne, 1841. F. J. Hugi, Ueber das Wesen der
Gletscher und Wintereise in dem Eismeer, Stuttgart, 1842. R. Mallet, The Mechanism of
Glaciers, Jour. Geol. Soc. Dublin, Vol. I, p. 317; On the Plasticity of Glacier Ice, Jour. Geol.
Soc. Dublin, 1845, Vol. III, p. 122; On the Brittleness and Non-plasticity of Glacier Ice, Phil.
Mag., XXVI, p. 586. James Thompson, On the Plasticity of Ice as Manifested in Glaciers,
Roy. Soc. Proc., Vol. 8, 1857, pp. 455–58. J. Tyndall and T. H. Huxley, On the Structure and
Motion of Glaciers, Phil. Trans., 1857, Vol. CXLVII, p. 327. J. D. Forbes, Occasional Papers
on the Theory of Glaciers, Edinburgh, 1859. W. Hopkins, On the Theory of the Motion of
Glaciers, Phil. Trans., 1862, p. 677; Phil. Mag., 1863, Vol. XXV, p. 224. J. Tyndall, Forms of
Water, New York, 1872; The Glaciers of the Alps, London, 1861. James Croll, On the
Physical Cause of the Motion of Glaciers, Phil. Mag., 1869, Vol. 38, pp. 201–6. A. Heim, On
Glaciers, Phil. Mag., 1871, Vol. 41, pp. 485–508; Handbuch der Gletscherkunde, 1885. H.
Moseley, On the Cause of the Descent of Glaciers, Br. Assoc. Rept., 1860, Pt. 2, p. 48; also
Phil. Mag., 1869, Vol. 37, pp. 229, 363; Vol. 39, p. 241; Vol. 42, p. 138; Vol. 43, p. 38. Ch.
Grad, La Constitution et le movement des Glaciers, Revue Sci., 1872. H. J. Rink, Danish
Greenland, 1877. R. M. Deeley, A Theory of Glacial Motion, Phil. Mag., 1888, Vol. 25, pp.
136–64. J. C. McConnel, On the Plasticity of an Ice Crystal, Proc. Roy. Soc. London, Vol. 48,
1890, pp. 256–60; ibid., Vol. 49, 1891, pp. 323–43. O. Mügge, Über die Plasticität der
Eiskrystalle, Nachr. k. Ges. d. Wiss., Göttingen, 1895, pp. 1–4. R. M. Deeley and George
Fletcher, The Structure of Glacier Ice and its Bearings on Glacier Motion, Geol. Mag.
(London), Decade 4, Vol. 2, 1895, pp. 152–62. T. C. Chamberlin, Presidential address before
the Geol. Soc. Am., Bull. Geol. Soc. Am., Vol. VI, February 1895, pp. 199–220. Reid,
Mechanics of Glaciers, Jour. Geol., Vol. IV, 1896, p. 912. Erich von Drygalski, Grönland-
Expedition der Gesellschaft für Erdkunde zu Berlin, 1891–93, Vol. I, 1897.
Page 837
[138] Much information on these and other points is to be found in the following books: Wild’s
Thalassa; Thompson’s Depths of the Sea; Barker’s Deep Sea Soundings, and Maury’s
Physical Geography; Agassiz’ The Three Cruises of the Blake, and the Challenger Reports
give much more detailed information concerning these and other matters.
[139] Dittmar, Challenger Reports, Physics and Chemistry, Vol. I, p. 204.
[140] For a discussion of the way in which this gas is held in solution, see Tolman, Jour. of Geol.,
Vol. VII, pp. 598–618.
[141] Murray, Scot. Geogr. Mag., Vol. IV, p. 39.
[142] Murray, Scot. Geogr. Mag., Vol. III, p. 76.
[143] Ibid., p. 70.
[144] Limited areas of the ocean bottom are actually concave upward; that is, they are basins in the
more commonly accepted sense of the term (see Chapter IX).
[145] J. Geikie. Earth Sculpture, p. 329.
[146] Murray. Scottish Geographical Magazine, Vol. XV, p. 507.
[147] Lindenkohl. Science, Vol. X, 1899, p. 807.
[148] This does not hold for tropical latitudes.
[149] National Geographic Magazine, Vol. XI, pp. 377–392.
[150] For causes of ocean-currents, see Croll’s Climate and Time; Proc. Roy. Soc., 1869–73, and
Jour. Roy. Geog. Soc., 1871–77.
[151] In the following pages concerning the waves and their work Gilbert’s classic discussion of
shore features, in the Fifth Annual Report of the U. S. Geol. Survey, pp. 80–100, is freely
drawn on. Another incisive discussion of certain shore phenomena is that of Fenneman, Jour.
of Geol., Vol. X, pp. 1–32.
[152] Dana. Manual of Geology, 4th ed., p. 213.
[153] Delesse. Lithologie des Mers de France. Cited by Geikie, Text-book of Geology, 3d ed., p.
438.
[154] Sir G. Airy. Encyclopedia Metropolitana, Art. Waves. Cited by Geikie, loc. cit., p. 438.
[155] Stevenson. Treatise on Harbors.
[156] Willis. Jour. of Geol., Vol. I, p. 481.
[157] Stevenson. Trans. Roy. Soc. Edin., Vol. XVI, p. 25. Treatise on Harbors, p. 42. Quoted by
Geikie, Text-book of Geology, p. 437.
[158] Geikie. Text-book of Geology, 3d ed., p. 437.
[159] Brit. Assoc. Rept., 1850, p. 26.
[160] Davis. Physical Geography, p. 354.
[161] Dana. Manual of Geology, 4th ed., p. 219.
[162] Shaler. Sea and Land, p. 29.
[163] Gulliver, Shore Line Topography: Proc. Am. Acad. Arts and Sci., Vol. XXXIV, 1899, pp. 151–
258. A valuable study of shore-line topography.
[164] Willis. Jour. of Geol., Vol. I, p. 481.
[165] See Gilbert. Topographic Features of Lake Shores, 5th Ann. Rept. U. S. Geol. Surv.
Thalassa; Thompson’s Depths of the Sea; Barker’s Deep Sea Soundings, and Maury’s
Physical Geography; Agassiz’ The Three Cruises of the Blake, and the Challenger Reports
give much more detailed information concerning these and other matters.
[139] Dittmar, Challenger Reports, Physics and Chemistry, Vol. I, p. 204.
[140] For a discussion of the way in which this gas is held in solution, see Tolman, Jour. of Geol.,
Vol. VII, pp. 598–618.
[141] Murray, Scot. Geogr. Mag., Vol. IV, p. 39.
[142] Murray, Scot. Geogr. Mag., Vol. III, p. 76.
[143] Ibid., p. 70.
[144] Limited areas of the ocean bottom are actually concave upward; that is, they are basins in the
more commonly accepted sense of the term (see Chapter IX).
[145] J. Geikie. Earth Sculpture, p. 329.
[146] Murray. Scottish Geographical Magazine, Vol. XV, p. 507.
[147] Lindenkohl. Science, Vol. X, 1899, p. 807.
[148] This does not hold for tropical latitudes.
[149] National Geographic Magazine, Vol. XI, pp. 377–392.
[150] For causes of ocean-currents, see Croll’s Climate and Time; Proc. Roy. Soc., 1869–73, and
Jour. Roy. Geog. Soc., 1871–77.
[151] In the following pages concerning the waves and their work Gilbert’s classic discussion of
shore features, in the Fifth Annual Report of the U. S. Geol. Survey, pp. 80–100, is freely
drawn on. Another incisive discussion of certain shore phenomena is that of Fenneman, Jour.
of Geol., Vol. X, pp. 1–32.
[152] Dana. Manual of Geology, 4th ed., p. 213.
[153] Delesse. Lithologie des Mers de France. Cited by Geikie, Text-book of Geology, 3d ed., p.
438.
[154] Sir G. Airy. Encyclopedia Metropolitana, Art. Waves. Cited by Geikie, loc. cit., p. 438.
[155] Stevenson. Treatise on Harbors.
[156] Willis. Jour. of Geol., Vol. I, p. 481.
[157] Stevenson. Trans. Roy. Soc. Edin., Vol. XVI, p. 25. Treatise on Harbors, p. 42. Quoted by
Geikie, Text-book of Geology, p. 437.
[158] Geikie. Text-book of Geology, 3d ed., p. 437.
[159] Brit. Assoc. Rept., 1850, p. 26.
[160] Davis. Physical Geography, p. 354.
[161] Dana. Manual of Geology, 4th ed., p. 219.
[162] Shaler. Sea and Land, p. 29.
[163] Gulliver, Shore Line Topography: Proc. Am. Acad. Arts and Sci., Vol. XXXIV, 1899, pp. 151–
258. A valuable study of shore-line topography.
[164] Willis. Jour. of Geol., Vol. I, p. 481.
[165] See Gilbert. Topographic Features of Lake Shores, 5th Ann. Rept. U. S. Geol. Surv.
Page 838
[166] Shaler, Sea Coast Swamps of the U. S., 6th Ann. Rept. U. S. Geol. Surv.; and Merrill, Pop.
Sci. Mo., Oct., 1890.
[167] Willis. Bull. Geol. Soc. Amer., Vol. IX, p. 113, and Tacoma, Wash., Folio, U. S. Geol. Surv.
[168] Agassiz. Three Cruises of the Blake, Vol. I, p. 259. Agassiz would ascribe the Blake plateau
itself to the Gulf Stream, p. 138. See also Am. Jour. Sci., Vol XXXV, 1888, p. 498.
[169] Reade. Phil. Mag., Vol. XXV (1888), p. 342.
[170] Murray. Challenger Report, Deep Sea Deposits, pp. 184, 185.
[171] Murray, loc. cit., pp. 187, 188.
[172] Ibid.
[173] Stevenson. Harbors, 2d ed., p. 15.
[174] Usiglio. Encyclopædia Britannica. Article on Salt.
[175] Willis. Jour. of Geol., Vol. I, p. 500, where the evidences for deposition are fully set forth.
[176] Murray, loc. cit.
[177] Ibid., p. 186.
[178] Murray, loc. cit., p. 295.
[179] Challenger Report, Deep Sea Deposits, p. 327.
[180] Young’s Astronomy, p. 472.
[181] Murray. Scottish Geog. Mag., Vol. XV, p. 511. An excellent summary of deep-sea deposits.
[182] Murray, Challenger Report on Deep Sea Deposits, p. 337 et seq., and Buchanan, Proc. Roy.
Soc. Edin., Vol. XVIII, 1892, pp. 17–39.
[183] Challenger Report on Deep Sea Deposits, pp. 385–391. See also Jour. of Geol., Vol. II, pp.
167–172.
[184] Forel, Compte Rendu, 1875, 1876, 1878, 1879, and p. Du Bois, 1891. Also Forel’s Lac
Leman.
[185] C. A. Davis, Journ. of Geol., Vol. VIII, pp. 485–97, and 498–503, and Vol. IX, pp. 491–506.
[186] Russell, Lake Lahontan, Mono. XI, U. S. Geol. Surv., Chap. V; also Third Ann. Rept., pp.
211–221. Gilbert, Lake Bonneville, Mono. I, U. S. Geol. Surv., p. 167.
[187] Stapff, Zeit. deut. geol. Gesell., Vol. XVIII, pp. 86–173.
[188] Upham, Lake Agassiz, Mono. XXV, U. S. Geol. Surv.; Salisbury and Kümmel, Lake Passaic,
Rept. of the State Geologist of N. J., 1893, and Jour. of Geol., Vol. III, pp. 533–560; Gilbert,
Lake Bonneville, Mono. I, U. S. Geol. Surv.; Russell, Lake Lahontan, Mono. XI, U. S. Geol.
Surv.; and Mono Lake, Eighth Ann. Rept., U. S. Geol. Surv., Pt. I.
[189] Gilbert, Lake Bonneville, Mono. I, U. S. Geol. Surv., p. 71, and Topographic Features of Lake
Shores, Fifth Ann. Rept. U. S. Geol. Surv., p. 109.
[190] Buckley. Wis. Acad. of Sci., Vol. XIII, Pt. I, 1900. A study of ice ramparts formed about the
shores of Lake Mendota, Wis., in 1898–99.
[191] Copied from Russell’s Lake Lahontan, Mono. XI, U. S. Geol. Surv.
[192] Less .04254 carbonic acid added to amount found. Average of two analyses.
[193] Average from four analyses.
[194] Average of two analyses.
Sci. Mo., Oct., 1890.
[167] Willis. Bull. Geol. Soc. Amer., Vol. IX, p. 113, and Tacoma, Wash., Folio, U. S. Geol. Surv.
[168] Agassiz. Three Cruises of the Blake, Vol. I, p. 259. Agassiz would ascribe the Blake plateau
itself to the Gulf Stream, p. 138. See also Am. Jour. Sci., Vol XXXV, 1888, p. 498.
[169] Reade. Phil. Mag., Vol. XXV (1888), p. 342.
[170] Murray. Challenger Report, Deep Sea Deposits, pp. 184, 185.
[171] Murray, loc. cit., pp. 187, 188.
[172] Ibid.
[173] Stevenson. Harbors, 2d ed., p. 15.
[174] Usiglio. Encyclopædia Britannica. Article on Salt.
[175] Willis. Jour. of Geol., Vol. I, p. 500, where the evidences for deposition are fully set forth.
[176] Murray, loc. cit.
[177] Ibid., p. 186.
[178] Murray, loc. cit., p. 295.
[179] Challenger Report, Deep Sea Deposits, p. 327.
[180] Young’s Astronomy, p. 472.
[181] Murray. Scottish Geog. Mag., Vol. XV, p. 511. An excellent summary of deep-sea deposits.
[182] Murray, Challenger Report on Deep Sea Deposits, p. 337 et seq., and Buchanan, Proc. Roy.
Soc. Edin., Vol. XVIII, 1892, pp. 17–39.
[183] Challenger Report on Deep Sea Deposits, pp. 385–391. See also Jour. of Geol., Vol. II, pp.
167–172.
[184] Forel, Compte Rendu, 1875, 1876, 1878, 1879, and p. Du Bois, 1891. Also Forel’s Lac
Leman.
[185] C. A. Davis, Journ. of Geol., Vol. VIII, pp. 485–97, and 498–503, and Vol. IX, pp. 491–506.
[186] Russell, Lake Lahontan, Mono. XI, U. S. Geol. Surv., Chap. V; also Third Ann. Rept., pp.
211–221. Gilbert, Lake Bonneville, Mono. I, U. S. Geol. Surv., p. 167.
[187] Stapff, Zeit. deut. geol. Gesell., Vol. XVIII, pp. 86–173.
[188] Upham, Lake Agassiz, Mono. XXV, U. S. Geol. Surv.; Salisbury and Kümmel, Lake Passaic,
Rept. of the State Geologist of N. J., 1893, and Jour. of Geol., Vol. III, pp. 533–560; Gilbert,
Lake Bonneville, Mono. I, U. S. Geol. Surv.; Russell, Lake Lahontan, Mono. XI, U. S. Geol.
Surv.; and Mono Lake, Eighth Ann. Rept., U. S. Geol. Surv., Pt. I.
[189] Gilbert, Lake Bonneville, Mono. I, U. S. Geol. Surv., p. 71, and Topographic Features of Lake
Shores, Fifth Ann. Rept. U. S. Geol. Surv., p. 109.
[190] Buckley. Wis. Acad. of Sci., Vol. XIII, Pt. I, 1900. A study of ice ramparts formed about the
shores of Lake Mendota, Wis., in 1898–99.
[191] Copied from Russell’s Lake Lahontan, Mono. XI, U. S. Geol. Surv.
[192] Less .04254 carbonic acid added to amount found. Average of two analyses.
[193] Average from four analyses.
[194] Average of two analyses.
Page 839
[195] As sesquicarbonates.
[196] As chloride.
[197] As peroxide.
[198] Carbonic acid by difference.
[199] Analyses of Rocks, Bull. 168, U. S. Geol. Surv., 1900, p. 15.
[200] Quantitative Classification of Igneous Rocks, by Whitman Cross, Joseph p. Iddings, Louis V.
Pirsson, and Henry S. Washington. 1903.
[201] Van Hise. 16th Ann. U. S. Geol. Surv., Pt. I, pp. 589–94.
[202] The application of these principles we owe chiefly to Van Hise: Metamorphism of Rocks and
Rock Flowage, Bull. Geol. Soc. Am., Vol. 9, pp. 269–328.
[203] Cross, Iddings, Pirsson, and Washington. Quantitative Classification of Igneous Rocks.
[204] The initials f.n. (field names) are introduced to show that the term is used in the broad field
sense proposed.
[205] Added by the authors of this work.
[206] The following definitions are given, as nearly as practicable, in accordance with present
common usage, which is, however, more or less varying and inconsistent.
[207] A comprehensive discussion of the “Genesis of Ore Deposits” may be found in Vols. XXIII
and XXIV of the Trans. of the Am. Inst. of Min. Eng. (also printed with additions in book
form by the Institute, 1902), in which Posepny, Emmons, Van Hise, LeConte, Blake, Becker,
Ricard, Raymond, Lindgren, Weed, Vogt, Winslow, Winchell (H. V.), Church, Cazin, Adams,
Keyes, Bain, Collins, Beck, and DeLaunay participated. Various phases of the leading modern
views are set forth.
[208] Chamberlin. Geol. of Wis., Vol. IV, p. 599 et seq., 1882.
[209] Penrose. Jour. of Geol., Vol. XI, pp. 135–155, 1903.
[210] Van Hise, Mono. XIX, U. S. Geol. Surv., pp. 268–295, 1892.
[211] Gilbert. Bull. Geol. Soc. Am., Vol. X, pp. 135–140, 1898.
[212] Branner. Jour. of Geol., Vol. VIII, pp. 481–484, 1900.
[213] Iddings. Jour. of Geol., Vol. VI, pp. 704–710.
[214] Daubrée. Géologie d’Expérimentale, pp. 306–372.
[215] Crosby. American Geologist, Vol. XII, 1893, pp. 368–375.
[216] Becker. Bull. U. S. Geol. Surv., Vol. X, pp. 41–75.
[217] Van Hise. Principles of North American Pre-Cambrian Geology. 16th Ann. Rept. U. S. Geol.
Surv., Pt. I, pp. 668–672.
[218] Diller. Bull. Geol. Soc. Am., Vol. I, pp. 441–442. Ibid. Hay, Vol. III, pp. 50–55; and Newsom,
ibid. Vol. XIV, pp. 227–268.
[219] Willis. Bull. Geol. Soc. of Am., Vol. XIII, pp. 331–336.
[220] McConnell. Canada Geol. and Nat. Hist. Surv., 1886, Pt. II.
[221] Geikie. Text-book of Geology.
[222] Becker. Geology of the Comstock Lode, Mono. III, U. S. Geol. Surv., Chapter IV.
[223] Reference, Van Hise. Sixteenth Ann. Rept. U. S. Geol. Surv., Pt. I, pp. 672–678.
[196] As chloride.
[197] As peroxide.
[198] Carbonic acid by difference.
[199] Analyses of Rocks, Bull. 168, U. S. Geol. Surv., 1900, p. 15.
[200] Quantitative Classification of Igneous Rocks, by Whitman Cross, Joseph p. Iddings, Louis V.
Pirsson, and Henry S. Washington. 1903.
[201] Van Hise. 16th Ann. U. S. Geol. Surv., Pt. I, pp. 589–94.
[202] The application of these principles we owe chiefly to Van Hise: Metamorphism of Rocks and
Rock Flowage, Bull. Geol. Soc. Am., Vol. 9, pp. 269–328.
[203] Cross, Iddings, Pirsson, and Washington. Quantitative Classification of Igneous Rocks.
[204] The initials f.n. (field names) are introduced to show that the term is used in the broad field
sense proposed.
[205] Added by the authors of this work.
[206] The following definitions are given, as nearly as practicable, in accordance with present
common usage, which is, however, more or less varying and inconsistent.
[207] A comprehensive discussion of the “Genesis of Ore Deposits” may be found in Vols. XXIII
and XXIV of the Trans. of the Am. Inst. of Min. Eng. (also printed with additions in book
form by the Institute, 1902), in which Posepny, Emmons, Van Hise, LeConte, Blake, Becker,
Ricard, Raymond, Lindgren, Weed, Vogt, Winslow, Winchell (H. V.), Church, Cazin, Adams,
Keyes, Bain, Collins, Beck, and DeLaunay participated. Various phases of the leading modern
views are set forth.
[208] Chamberlin. Geol. of Wis., Vol. IV, p. 599 et seq., 1882.
[209] Penrose. Jour. of Geol., Vol. XI, pp. 135–155, 1903.
[210] Van Hise, Mono. XIX, U. S. Geol. Surv., pp. 268–295, 1892.
[211] Gilbert. Bull. Geol. Soc. Am., Vol. X, pp. 135–140, 1898.
[212] Branner. Jour. of Geol., Vol. VIII, pp. 481–484, 1900.
[213] Iddings. Jour. of Geol., Vol. VI, pp. 704–710.
[214] Daubrée. Géologie d’Expérimentale, pp. 306–372.
[215] Crosby. American Geologist, Vol. XII, 1893, pp. 368–375.
[216] Becker. Bull. U. S. Geol. Surv., Vol. X, pp. 41–75.
[217] Van Hise. Principles of North American Pre-Cambrian Geology. 16th Ann. Rept. U. S. Geol.
Surv., Pt. I, pp. 668–672.
[218] Diller. Bull. Geol. Soc. Am., Vol. I, pp. 441–442. Ibid. Hay, Vol. III, pp. 50–55; and Newsom,
ibid. Vol. XIV, pp. 227–268.
[219] Willis. Bull. Geol. Soc. of Am., Vol. XIII, pp. 331–336.
[220] McConnell. Canada Geol. and Nat. Hist. Surv., 1886, Pt. II.
[221] Geikie. Text-book of Geology.
[222] Becker. Geology of the Comstock Lode, Mono. III, U. S. Geol. Surv., Chapter IV.
[223] Reference, Van Hise. Sixteenth Ann. Rept. U. S. Geol. Surv., Pt. I, pp. 672–678.
Page 840
[224] Davison. Jour. of Geol., Vol. VIII, p. 301.
[225] Nature, October 24, 1895.
[226] Milne. The Geog. Jour., Vol. XXI, p. 1. See also Seismology, a more technical work than the
same author’s Earthquakes.
[227] Darwin. Journal of Researches, 1845, p. 303.
[228] Oldham. Quar. Jour. Geol. Soc., Vol. XXVIII, p. 257.
[229] Geikie. Text-book of Geology, 4th ed., p. 372.
[230] Kotô. Jour. Coll. Sci., Japan, Vol. V, Pt. IV (1893), pp. 329, 339. Cited by Geikie, loc. cit., p.
373.
[231] An elaborate account of this earthquake is given by Dutton, Ninth Ann. Rept., U. S. Geol.
Surv., pp. 209–528.
[232] Cross. Twenty-first Ann. Rept., U. S. Geol. Surv., Pt. II, Chap. V.
[233] Oldham. Report on the Indian Earthquake of June 12, 1897, p. 138. Mem. Geol. Surv. of
India. Cited by Geikie, loc. cit., p. 374.
[234] Oldham, loc. cit., p. 80.
[235] Geikie. Text-book of Geology, 4th ed., p. 375.
[236] Ibid., p. 376.
[237] Forster, Seismology, 1877. Summarized in the Am. Geol., Vol. III, 1889, p. 182.
[238] The literature of seismology is very extensive. Some of the more general treatises are the
following: Mallet, Brit. Assoc., 1847, Part II, p. 30; 1850, p. 1; 1851, p. 272; 1852, p. 1; 1858,
p. 1; 1861, p. 201; and The Great Neapolitan Earthquake of 1857, 2 Vols., 1862; A. Perrey,
Mém. Couronn. Bruxelles, XVIII (1844), Comptes Rendus, LII, p. 146; R. Falb, Grundzüge
einer Theorie der Erdbeben und Vulkanenausbrüche, Graz, 1871, and Gedanken und Studien
über den Vulkanismus, etc., 1874; Pfaff, Allgemeine Geologie als exacte Wissenschaft,
Leipzig, 1873, p. 224; Schmidt, Studien über Erdbeben, 2d ed., 1879, and Studien über
Vulkane und Erdbeben, 1881; Dieffenbach, Neues Jahrb., 1872, p. 155; M. S. di Rossi, La
Meteorologia Endogena, 2 Vols., 1879 and 1882; J. Milne, Earthquakes and other Earth-
movements (contains a bibliography), 4th ed., 1898; Seismology, ibid., 1898; Dutton,
Earthquakes, 1904.
Records of earthquakes have been preserved more or less fully in several countries,
especially in recent years. A few of the more accessible publications where these records are
found are cited below: California earthquakes, Perrine, Bull. 147, U. S. Geol. Surv.;
Earthquakes of the Pacific Coast, Holden, Smithson. Misc. Coll., No. 1087, 1898; Records of
recent earthquake movements in Great Britain since 1890 are published by Davison in Quar.
Jour. Geol. Soc., Geol. Mag., and Nature; Records of earlier earthquakes are found in the
reports of the Brit. Assoc. (Mallet), in the Edinburgh New Philos. Jour., Vols. XXXI-XXXVI
(Milne), and in Trans. of the Roy. Irish Acad., 1884 and 1886 (O’Reilly); The Earthquakes of
Scandinavia have been recorded in volumes of the Geol. Fören, Förhandl.; Records of other
continental European earthquakes are found in Gerland’s Beiträge zur Geophysik, 1895, 1900,
and 1901; Neues Jahrb., 1865–71; Zeitschr. Naturwissen. (1884), (Credner); Bericht. k. Sachs.
Geol. Wissen., 1889 and 1900 (Credner); Jahrb. Geol. Reichsanst., 1895 and 1897;
Tschermak’s Min. Mitth., 1873, and later; Transactions of the Seismological Soc. of Japan. An
index to these Transactions is given at the end of Milne’s Seismology.
[239] Antlitz der Erde. Vol. 1, p. 136.
[225] Nature, October 24, 1895.
[226] Milne. The Geog. Jour., Vol. XXI, p. 1. See also Seismology, a more technical work than the
same author’s Earthquakes.
[227] Darwin. Journal of Researches, 1845, p. 303.
[228] Oldham. Quar. Jour. Geol. Soc., Vol. XXVIII, p. 257.
[229] Geikie. Text-book of Geology, 4th ed., p. 372.
[230] Kotô. Jour. Coll. Sci., Japan, Vol. V, Pt. IV (1893), pp. 329, 339. Cited by Geikie, loc. cit., p.
373.
[231] An elaborate account of this earthquake is given by Dutton, Ninth Ann. Rept., U. S. Geol.
Surv., pp. 209–528.
[232] Cross. Twenty-first Ann. Rept., U. S. Geol. Surv., Pt. II, Chap. V.
[233] Oldham. Report on the Indian Earthquake of June 12, 1897, p. 138. Mem. Geol. Surv. of
India. Cited by Geikie, loc. cit., p. 374.
[234] Oldham, loc. cit., p. 80.
[235] Geikie. Text-book of Geology, 4th ed., p. 375.
[236] Ibid., p. 376.
[237] Forster, Seismology, 1877. Summarized in the Am. Geol., Vol. III, 1889, p. 182.
[238] The literature of seismology is very extensive. Some of the more general treatises are the
following: Mallet, Brit. Assoc., 1847, Part II, p. 30; 1850, p. 1; 1851, p. 272; 1852, p. 1; 1858,
p. 1; 1861, p. 201; and The Great Neapolitan Earthquake of 1857, 2 Vols., 1862; A. Perrey,
Mém. Couronn. Bruxelles, XVIII (1844), Comptes Rendus, LII, p. 146; R. Falb, Grundzüge
einer Theorie der Erdbeben und Vulkanenausbrüche, Graz, 1871, and Gedanken und Studien
über den Vulkanismus, etc., 1874; Pfaff, Allgemeine Geologie als exacte Wissenschaft,
Leipzig, 1873, p. 224; Schmidt, Studien über Erdbeben, 2d ed., 1879, and Studien über
Vulkane und Erdbeben, 1881; Dieffenbach, Neues Jahrb., 1872, p. 155; M. S. di Rossi, La
Meteorologia Endogena, 2 Vols., 1879 and 1882; J. Milne, Earthquakes and other Earth-
movements (contains a bibliography), 4th ed., 1898; Seismology, ibid., 1898; Dutton,
Earthquakes, 1904.
Records of earthquakes have been preserved more or less fully in several countries,
especially in recent years. A few of the more accessible publications where these records are
found are cited below: California earthquakes, Perrine, Bull. 147, U. S. Geol. Surv.;
Earthquakes of the Pacific Coast, Holden, Smithson. Misc. Coll., No. 1087, 1898; Records of
recent earthquake movements in Great Britain since 1890 are published by Davison in Quar.
Jour. Geol. Soc., Geol. Mag., and Nature; Records of earlier earthquakes are found in the
reports of the Brit. Assoc. (Mallet), in the Edinburgh New Philos. Jour., Vols. XXXI-XXXVI
(Milne), and in Trans. of the Roy. Irish Acad., 1884 and 1886 (O’Reilly); The Earthquakes of
Scandinavia have been recorded in volumes of the Geol. Fören, Förhandl.; Records of other
continental European earthquakes are found in Gerland’s Beiträge zur Geophysik, 1895, 1900,
and 1901; Neues Jahrb., 1865–71; Zeitschr. Naturwissen. (1884), (Credner); Bericht. k. Sachs.
Geol. Wissen., 1889 and 1900 (Credner); Jahrb. Geol. Reichsanst., 1895 and 1897;
Tschermak’s Min. Mitth., 1873, and later; Transactions of the Seismological Soc. of Japan. An
index to these Transactions is given at the end of Milne’s Seismology.
[239] Antlitz der Erde. Vol. 1, p. 136.
Page 841
[240] Eugene A. Smith. Underthrust Folds and Faults, Am. Jour. Sci., Vol. XLV, 1893, pp. 305–6.
[241] Manual of Geology, 3d ed., p. 23.
[242] For discussions of folds, see Van Hise, Sixteenth Ann. Rept. U. S. Geol. Surv., Pt. I, pp. 603–
632; and Willis, Thirteenth Ann. Rept., Pt. II, pp. 217–296.
[243] Mechanismus der Gebirgsbildung, p. 213.
[244] Am. Nat., Vol. XIX, p. 257, 1885.
[245] Geol. Surv. of Canada, p. 33 D, 1886.
[246] Elements of Geology, 5th ed., p. 266.
[247] Van Hise. Bull. Geol. Soc. of Am., 1897, Vol. IX, p. 291.
[248] See Woodward’s address, Mathematical Theories of the Earth, Proc. Am. Assc. for Adv. Sci.,
1889, pp. 59–63.
[249] Nat. Phil. Thompson and Tait, Pt. II, p. 477. See also Popular Lectures and Addresses, 1894,
II, p. 313.
[250] Physics of the Earth’s Crust, Fisher, p. 95.
[251] Origin of Mountain Ranges, T. Mellard Reade, p. 125.
[252] Phil. Trans. Roy. Soc., Vol. 178, pp. 231–49.
[253] Amer. Jour. Sci., 1893, 3d series, Vol. 45, p. 7.
[254] Essentially the same as atmospheres.
[255] The pressures and densities here given are essentially the same as those previously worked out
by others and already published. The temperatures are the results of recent preliminary
computations made under the auspices of the Carnegie Institution, and are subject to change
on further study. They are based on the assumption that the increase in density is due to
compression. They are in general accord with the results previously reached by Dr. F. R.
Moulton (see “A Group of Hypotheses Bearing on Climatic Changes,” by T. C. Chamberlin,
Jour. of Geol., 1897, p. 674). The Rev. O. Fisher, in the Am. Jour. of Sci., 1901, p. 420, gives
much higher results.
[256] Attention was called to this feature by Chamberlin in a paper before the Geol. Soc. of Am. at
Rochester, December, 1901.
[257] These are reckoned by assuming that the temperature of no variation at 50 feet below the
surface is 40° F.
[258] Am. Jour. of Sci., Vol. V, 1898, p. 161.
[259] Van Hise. Personal communication.
[260] Bull. 168 U. S. Geol. Surv., p. 14.
[261] Daniell’s Physics, p. 407.
[262] Heat. Tait, p. 225.
[263] All the feldspars are calculated as anorthite. Augite is used for hypersthene, ilmenite is
included with magnetite, and all minerals are calculated as if of the isometric system.
[264] Physics of the Earth’s Crust, Chap. VIII.
[265] Penn Monthly, Philadelphia, May, 1876.
[266] The following conclusion by an eminent authority has come to our notice since this was
written:
[241] Manual of Geology, 3d ed., p. 23.
[242] For discussions of folds, see Van Hise, Sixteenth Ann. Rept. U. S. Geol. Surv., Pt. I, pp. 603–
632; and Willis, Thirteenth Ann. Rept., Pt. II, pp. 217–296.
[243] Mechanismus der Gebirgsbildung, p. 213.
[244] Am. Nat., Vol. XIX, p. 257, 1885.
[245] Geol. Surv. of Canada, p. 33 D, 1886.
[246] Elements of Geology, 5th ed., p. 266.
[247] Van Hise. Bull. Geol. Soc. of Am., 1897, Vol. IX, p. 291.
[248] See Woodward’s address, Mathematical Theories of the Earth, Proc. Am. Assc. for Adv. Sci.,
1889, pp. 59–63.
[249] Nat. Phil. Thompson and Tait, Pt. II, p. 477. See also Popular Lectures and Addresses, 1894,
II, p. 313.
[250] Physics of the Earth’s Crust, Fisher, p. 95.
[251] Origin of Mountain Ranges, T. Mellard Reade, p. 125.
[252] Phil. Trans. Roy. Soc., Vol. 178, pp. 231–49.
[253] Amer. Jour. Sci., 1893, 3d series, Vol. 45, p. 7.
[254] Essentially the same as atmospheres.
[255] The pressures and densities here given are essentially the same as those previously worked out
by others and already published. The temperatures are the results of recent preliminary
computations made under the auspices of the Carnegie Institution, and are subject to change
on further study. They are based on the assumption that the increase in density is due to
compression. They are in general accord with the results previously reached by Dr. F. R.
Moulton (see “A Group of Hypotheses Bearing on Climatic Changes,” by T. C. Chamberlin,
Jour. of Geol., 1897, p. 674). The Rev. O. Fisher, in the Am. Jour. of Sci., 1901, p. 420, gives
much higher results.
[256] Attention was called to this feature by Chamberlin in a paper before the Geol. Soc. of Am. at
Rochester, December, 1901.
[257] These are reckoned by assuming that the temperature of no variation at 50 feet below the
surface is 40° F.
[258] Am. Jour. of Sci., Vol. V, 1898, p. 161.
[259] Van Hise. Personal communication.
[260] Bull. 168 U. S. Geol. Surv., p. 14.
[261] Daniell’s Physics, p. 407.
[262] Heat. Tait, p. 225.
[263] All the feldspars are calculated as anorthite. Augite is used for hypersthene, ilmenite is
included with magnetite, and all minerals are calculated as if of the isometric system.
[264] Physics of the Earth’s Crust, Chap. VIII.
[265] Penn Monthly, Philadelphia, May, 1876.
[266] The following conclusion by an eminent authority has come to our notice since this was
written:
Page 842
L’influence des marées océanienes sur la durée du jour est donc tout à fait minime et n’est
nullement comparable à l’effet des marées dues à la viscosité et à l’elasticité de la partie
solide du globe, effet sur lequel M. Darwin à insisté dans une series de Mémoires du plus haut
intérêt. Par H. Poincaré, Bulletin Astronomique, tome XX (June, 1903), p. 223.
[267] On the Secular Changes in the Elements of the Orbit of a Satellite revolving about a Tidally-
distorted Planet. Phil. Trans., Roy. Soc., Pt. II, 1880.
[268] Jour. Geol., Vol. VI, 1898, p. 65.
[269] Quar. Jour. Geol. Soc., Vol. 39, 1883, p. 140. Everett (Units and Physical Constants) gives 837
× 106 for steel, but as the modulus for granite seems low, we have taken the lower estimate for
steel to avoid exaggerating the ratio between them.
[270] Nat. Phil. Thompson & Tait, Vol. II, p. 424, 1890.
[271] Computations made at the request of the authors. See also Fisher, Physics of the Earth’s Crust,
p. 36.
[272] Of like import is the statement of Woodward—“If the crust of the earth were self-supporting,
its crushing strength would have to be about thirty times that of the best cast steel, or five
hundred to one thousand times that of granite.” Mathematical Theories of the Earth, Proc.
Am. Assoc. for Adv. Sci., 1889, p. 49.
[273] It is assumed that the direction of the supporting thrust at the periphery of the dome is at every
point parallel to the tangent to the domed surface. This is justified by symmetry in the case of
a shell conforming to the sphericity of the earth, and in the other cases it would seem to be as
favorable an assumption in the direction of high supporting capacity as can reasonably be
made.
[274] Prepared at the authors’ request by W. H. Emmons.
[275] The terms are here used in their narrow technical sense. Extrusion is also used in a broad
generic sense to indicate the whole process of outward movement.
[276] Gilbert. 14th Ann. Rept. U. S. Geol. Surv., Pt. I, p. 187.
[277] Gilbert, after a careful study of the moon’s topography, has suggested that the lunar pits may
be indentations produced by infalling meteorites or planetoids, and has shown by experiment
that pits of a similar type, with similar central cones, can be produced by impact. The Moon’s
Face: A Study of the Origin of its Features. Presidential address, Phil. Soc. of Washington,
1892, Bull. Vol. XII, pp. 241–292.
[278] Structure and Distribution of Coral Islands.
[279] Corals and Coral Islands.
[280] Proc. Roy. Soc. Edin., Vol. X, pp. 505–18, and Vol. XVII, pp. 79–109; Nature, Vol. XXXII, p.
613; Narrative Chal. Exp., Vol. I, pp. 781–2.
[281] Bull. Mus. Comp. Zool., Vol. XVII, 1889.
[282] Ante, p. 22.
[283] Origin of Igneous Rocks. Phil. Soc. of Wash., Vol. XII, pp. 89–214.
[284] The Natural System of Volcanic Rocks. Cal. Acad. of Sci., 1868.
[285] Chemical News, April 9, 1897.
[286] Phil. Trans., 1873.
[287] Mechanics of Igneous Intrusion, Am. Jour. Sci., Apr., p. 269, and Aug., p. 107, 1903.
nullement comparable à l’effet des marées dues à la viscosité et à l’elasticité de la partie
solide du globe, effet sur lequel M. Darwin à insisté dans une series de Mémoires du plus haut
intérêt. Par H. Poincaré, Bulletin Astronomique, tome XX (June, 1903), p. 223.
[267] On the Secular Changes in the Elements of the Orbit of a Satellite revolving about a Tidally-
distorted Planet. Phil. Trans., Roy. Soc., Pt. II, 1880.
[268] Jour. Geol., Vol. VI, 1898, p. 65.
[269] Quar. Jour. Geol. Soc., Vol. 39, 1883, p. 140. Everett (Units and Physical Constants) gives 837
× 106 for steel, but as the modulus for granite seems low, we have taken the lower estimate for
steel to avoid exaggerating the ratio between them.
[270] Nat. Phil. Thompson & Tait, Vol. II, p. 424, 1890.
[271] Computations made at the request of the authors. See also Fisher, Physics of the Earth’s Crust,
p. 36.
[272] Of like import is the statement of Woodward—“If the crust of the earth were self-supporting,
its crushing strength would have to be about thirty times that of the best cast steel, or five
hundred to one thousand times that of granite.” Mathematical Theories of the Earth, Proc.
Am. Assoc. for Adv. Sci., 1889, p. 49.
[273] It is assumed that the direction of the supporting thrust at the periphery of the dome is at every
point parallel to the tangent to the domed surface. This is justified by symmetry in the case of
a shell conforming to the sphericity of the earth, and in the other cases it would seem to be as
favorable an assumption in the direction of high supporting capacity as can reasonably be
made.
[274] Prepared at the authors’ request by W. H. Emmons.
[275] The terms are here used in their narrow technical sense. Extrusion is also used in a broad
generic sense to indicate the whole process of outward movement.
[276] Gilbert. 14th Ann. Rept. U. S. Geol. Surv., Pt. I, p. 187.
[277] Gilbert, after a careful study of the moon’s topography, has suggested that the lunar pits may
be indentations produced by infalling meteorites or planetoids, and has shown by experiment
that pits of a similar type, with similar central cones, can be produced by impact. The Moon’s
Face: A Study of the Origin of its Features. Presidential address, Phil. Soc. of Washington,
1892, Bull. Vol. XII, pp. 241–292.
[278] Structure and Distribution of Coral Islands.
[279] Corals and Coral Islands.
[280] Proc. Roy. Soc. Edin., Vol. X, pp. 505–18, and Vol. XVII, pp. 79–109; Nature, Vol. XXXII, p.
613; Narrative Chal. Exp., Vol. I, pp. 781–2.
[281] Bull. Mus. Comp. Zool., Vol. XVII, 1889.
[282] Ante, p. 22.
[283] Origin of Igneous Rocks. Phil. Soc. of Wash., Vol. XII, pp. 89–214.
[284] The Natural System of Volcanic Rocks. Cal. Acad. of Sci., 1868.
[285] Chemical News, April 9, 1897.
[286] Phil. Trans., 1873.
[287] Mechanics of Igneous Intrusion, Am. Jour. Sci., Apr., p. 269, and Aug., p. 107, 1903.
Page 843
[288] Frank. Lehrbuch der Botanik, I, p. 576, 1892.
[289] Science, Vol. VI, p. 838, 1897. Zeitschrift für Anorganische Chemie, 1897.
[290] Reference works: Scott, Studies in Fossil Plants, 1900; Zeiller, Éléments de Paléobotanique,
1900; Potonié, Lehrbuch der Pflanzenpaleontologie, 1899; Seward, Fossil Plants, 1898;
Solms-Laubach, Fossil Botany, 1887.
[291] Weed. Ninth Ann. Rept. U. S. Geol. Surv., 1887–88, pp. 613–76; also Bradley M. Davis.
Science, Vol. VI, 1897, pp. 145–57.
[292] Cohn. Abhandl. Schles. Gesell. Naturwiss., Heft II, 1862.
[293] Deep Sea Deposits, p. 257.
[294] C. A. Davis. Jour. of Geol., Vol. IX, 1901, p. 491.
[295] Weed. Ninth Ann. Rept. U. S. Geol. Surv., 1887–8.
[296] Reference books: Zittel’s Text-book on Paleontology, translated and edited by Eastman;
Williams’ Geological Biology; Nicholson’s Manual of Paleontology.
[297] After Zittel in the main.
[298] S. W. Johnson, How Crops Feed, p. 47.
[299] Reference works: Plant Relations, Coulter, 1900,—a convenient elementary work; Schimper,
Pflanzengeographie, 1898; Warming, Lehrbuch der oekologischen Pflanzengeographie, 1896;
Cowles, Botanical Gazette, Vol. XXVII, 1898.
[300] One of the earliest attempts to map these and develop their significance and value is found in
Vol. II, Geol. of Wis., 1873–77, Native Vegetation, pp. 176–87.
[301] Chamberlin. A Systematic Source of Evolution of Provincial Faunas, Jour. of Geol., Vol. VI,
1898, pp. 597–609.
[302] Wallace. Island Life.
[303] For data, see Walther’s Einleitung in die Geologie, pp. 35–45.
Transcriber’s Notes:
New original cover art included with this eBook is granted to the public domain.
Obvious typographical errors have been silently corrected.
Fig. 332 is skipped in the source.
[289] Science, Vol. VI, p. 838, 1897. Zeitschrift für Anorganische Chemie, 1897.
[290] Reference works: Scott, Studies in Fossil Plants, 1900; Zeiller, Éléments de Paléobotanique,
1900; Potonié, Lehrbuch der Pflanzenpaleontologie, 1899; Seward, Fossil Plants, 1898;
Solms-Laubach, Fossil Botany, 1887.
[291] Weed. Ninth Ann. Rept. U. S. Geol. Surv., 1887–88, pp. 613–76; also Bradley M. Davis.
Science, Vol. VI, 1897, pp. 145–57.
[292] Cohn. Abhandl. Schles. Gesell. Naturwiss., Heft II, 1862.
[293] Deep Sea Deposits, p. 257.
[294] C. A. Davis. Jour. of Geol., Vol. IX, 1901, p. 491.
[295] Weed. Ninth Ann. Rept. U. S. Geol. Surv., 1887–8.
[296] Reference books: Zittel’s Text-book on Paleontology, translated and edited by Eastman;
Williams’ Geological Biology; Nicholson’s Manual of Paleontology.
[297] After Zittel in the main.
[298] S. W. Johnson, How Crops Feed, p. 47.
[299] Reference works: Plant Relations, Coulter, 1900,—a convenient elementary work; Schimper,
Pflanzengeographie, 1898; Warming, Lehrbuch der oekologischen Pflanzengeographie, 1896;
Cowles, Botanical Gazette, Vol. XXVII, 1898.
[300] One of the earliest attempts to map these and develop their significance and value is found in
Vol. II, Geol. of Wis., 1873–77, Native Vegetation, pp. 176–87.
[301] Chamberlin. A Systematic Source of Evolution of Provincial Faunas, Jour. of Geol., Vol. VI,
1898, pp. 597–609.
[302] Wallace. Island Life.
[303] For data, see Walther’s Einleitung in die Geologie, pp. 35–45.
Transcriber’s Notes:
New original cover art included with this eBook is granted to the public domain.
Obvious typographical errors have been silently corrected.
Fig. 332 is skipped in the source.
Page 844
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