Page 1
Page 2
Page 3
The Project Gutenberg eBook of A century of science in
America
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: A century of science in America
with special reference to the American Journal of Science,
1818-1918
Contributor: Edward Salisbury Dana
Joseph Barrell
Wesley R. Coe
H. W. Foote
William E. Ford
George L. Goodale
Herbert E. Gregory
Richard Swann Lull
Leigh Page
Louis V. Pirsson
Charles Schuchert
George Otis Smith
Robert B. Sosman
Horace L. Wells
Release date: May 11, 2024 [eBook #73605]
Language: English
Original publication: London: Yale University Press, 1918
America
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: A century of science in America
with special reference to the American Journal of Science,
1818-1918
Contributor: Edward Salisbury Dana
Joseph Barrell
Wesley R. Coe
H. W. Foote
William E. Ford
George L. Goodale
Herbert E. Gregory
Richard Swann Lull
Leigh Page
Louis V. Pirsson
Charles Schuchert
George Otis Smith
Robert B. Sosman
Horace L. Wells
Release date: May 11, 2024 [eBook #73605]
Language: English
Original publication: London: Yale University Press, 1918
Page 4
Other information and formats: www.gutenberg.org/ebooks/73605
Credits: Richard Tonsing, Charlene Taylor, and the Online Distributed
Proofreading Team at https://www.pgdp.net (This file was
produced from images generously made available by The
Internet Archive/American Libraries.)
*** START OF THE PROJECT GUTENBERG EBOOK A CENTURY OF
SCIENCE IN AMERICA ***
Transcriber’s Note:
New original cover art included with this eBook is
granted to the public domain.
Credits: Richard Tonsing, Charlene Taylor, and the Online Distributed
Proofreading Team at https://www.pgdp.net (This file was
produced from images generously made available by The
Internet Archive/American Libraries.)
*** START OF THE PROJECT GUTENBERG EBOOK A CENTURY OF
SCIENCE IN AMERICA ***
Transcriber’s Note:
New original cover art included with this eBook is
granted to the public domain.
Page 5
YALE UNIVERSITY
MRS. HEPSA ELY SILLIMAN
MEMORIAL LECTURES
In the year 1883 a legacy of eighty thousand dollars was left to the
President and Fellows of Yale College in the city of New Haven, to be held
in trust, as a gift from her children, in memory of their beloved and honored
mother, Mrs. Hepsa Ely Silliman.
On this foundation Yale College was requested and directed to establish
an annual course of lectures designed to illustrate the presence and
providence, the wisdom and goodness of God, as manifested in the natural
and moral world. These were to be designated as the Mrs. Hepsa Ely
Silliman Memorial Lectures. It was the belief of the testator that any orderly
presentation of the facts of nature or history contributed to the end of this
foundation more effectively than any attempt to emphasize the elements of
doctrine or of creed; and he therefore provided that lectures on dogmatic or
polemical theology should be excluded from the scope of this foundation,
and that the subjects should be selected rather from the domains of natural
science and history, giving special prominence to astronomy, chemistry,
geology, and anatomy.
It was further directed that each annual course should be made the basis
of a volume to form part of a series constituting a memorial to Mrs.
Silliman. The memorial fund came into the possession of the Corporation of
Yale University in the year 1901; and the present volume constitutes the
fourteenth of the series of memorial lectures.
MRS. HEPSA ELY SILLIMAN
MEMORIAL LECTURES
In the year 1883 a legacy of eighty thousand dollars was left to the
President and Fellows of Yale College in the city of New Haven, to be held
in trust, as a gift from her children, in memory of their beloved and honored
mother, Mrs. Hepsa Ely Silliman.
On this foundation Yale College was requested and directed to establish
an annual course of lectures designed to illustrate the presence and
providence, the wisdom and goodness of God, as manifested in the natural
and moral world. These were to be designated as the Mrs. Hepsa Ely
Silliman Memorial Lectures. It was the belief of the testator that any orderly
presentation of the facts of nature or history contributed to the end of this
foundation more effectively than any attempt to emphasize the elements of
doctrine or of creed; and he therefore provided that lectures on dogmatic or
polemical theology should be excluded from the scope of this foundation,
and that the subjects should be selected rather from the domains of natural
science and history, giving special prominence to astronomy, chemistry,
geology, and anatomy.
It was further directed that each annual course should be made the basis
of a volume to form part of a series constituting a memorial to Mrs.
Silliman. The memorial fund came into the possession of the Corporation of
Yale University in the year 1901; and the present volume constitutes the
fourteenth of the series of memorial lectures.
Page 6
SILLIMAN MEMORIAL LECTURES
PUBLISHED BY YALE UNIVERSITY PRESS
ELECTRICITY AND MATTER. By Joseph John Thomson, d.s.c., l.l.d,
ph.d., f.r.s., Fellow of Trinity College and Cavendish Professor of
Experimental Physics, Cambridge University.
(Fourth printing.) Price $1.50 net.
THE INTEGRATIVE ACTION OF THE NERVOUS SYSTEM. By
Charles S. Sherrington, d.sc., m.d., hon. ll.d. tor., f.r.s., Holt
Professor of Physiology, University of Liverpool.
(Fifth Printing.) Price $5.00 net.
RADIOACTIVE TRANSFORMATIONS. By Ernest Rutherford, d.sc,
ll.d., f.r.s., Macdonald Professor of Physics, McGill University.
Price $5.00 net.
EXPERIMENTAL AND THEORETICAL APPLICATIONS OF
THERMODYNAMICS TO CHEMISTRY. By Dr. Walter Nernst,
Professor and Director of the Institute of Physical Chemistry in the
University of Berlin.
Price $1.50 net.
PROBLEMS OF GENETICS. By William Bateson, m.a., f.r.s., Director
of the John Innes Horticultural Institution, Merton Park, Surrey,
England.
PUBLISHED BY YALE UNIVERSITY PRESS
ELECTRICITY AND MATTER. By Joseph John Thomson, d.s.c., l.l.d,
ph.d., f.r.s., Fellow of Trinity College and Cavendish Professor of
Experimental Physics, Cambridge University.
(Fourth printing.) Price $1.50 net.
THE INTEGRATIVE ACTION OF THE NERVOUS SYSTEM. By
Charles S. Sherrington, d.sc., m.d., hon. ll.d. tor., f.r.s., Holt
Professor of Physiology, University of Liverpool.
(Fifth Printing.) Price $5.00 net.
RADIOACTIVE TRANSFORMATIONS. By Ernest Rutherford, d.sc,
ll.d., f.r.s., Macdonald Professor of Physics, McGill University.
Price $5.00 net.
EXPERIMENTAL AND THEORETICAL APPLICATIONS OF
THERMODYNAMICS TO CHEMISTRY. By Dr. Walter Nernst,
Professor and Director of the Institute of Physical Chemistry in the
University of Berlin.
Price $1.50 net.
PROBLEMS OF GENETICS. By William Bateson, m.a., f.r.s., Director
of the John Innes Horticultural Institution, Merton Park, Surrey,
England.
Page 7
(Second printing.) Price $5.00 net.
STELLAR MOTIONS. With Special Reference to Motions Determined
by Means of the Spectrograph. By William Wallace Campbell, so.d,
ll.d., Director of the Lick Observatory, University of California.
(Second printing.) Price $5.00 net.
THEORIES OF SOLUTIONS. By Svante Arrhenius, ph.d., sc.d., m.d.,
Director of the Physico-Chemical Department of the Nobel Institute,
Stockholm, Sweden.
(Third printing.) Price $3.00 net.
IRRITABILITY. A Physiological Analysis of the General Effect of
Stimuli in Living Substances. By Max Verworn, m.d., ph.d., Professor
at Bonn Physiological Institute.
(Second printing.) Price $5.00 net.
PROBLEMS OF AMERICAN GEOLOGY. By William North Rice,
Frank D. Adams, Arthur P. Coleman, Charles D. Walcott,
Waldemar Lindgren, Frederick Leslie Ransome, and William D.
Matthew.
(Second printing.) Price $5.00 net.
THE PROBLEM OF VOLCANISM. By Joseph Paxson Iddings, ph.d.,
sc.d.
(Second printing.) Price $5.00 net.
ORGANISM AND ENVIRONMENT AS ILLUSTRATED BY THE
PHYSIOLOGY OF BREATHING. By John Scott Haldane, m.d., ll.d.,
f.r.s., Fellow of New College, Oxford University.
(Second printing.) Price $1.25 net.
STELLAR MOTIONS. With Special Reference to Motions Determined
by Means of the Spectrograph. By William Wallace Campbell, so.d,
ll.d., Director of the Lick Observatory, University of California.
(Second printing.) Price $5.00 net.
THEORIES OF SOLUTIONS. By Svante Arrhenius, ph.d., sc.d., m.d.,
Director of the Physico-Chemical Department of the Nobel Institute,
Stockholm, Sweden.
(Third printing.) Price $3.00 net.
IRRITABILITY. A Physiological Analysis of the General Effect of
Stimuli in Living Substances. By Max Verworn, m.d., ph.d., Professor
at Bonn Physiological Institute.
(Second printing.) Price $5.00 net.
PROBLEMS OF AMERICAN GEOLOGY. By William North Rice,
Frank D. Adams, Arthur P. Coleman, Charles D. Walcott,
Waldemar Lindgren, Frederick Leslie Ransome, and William D.
Matthew.
(Second printing.) Price $5.00 net.
THE PROBLEM OF VOLCANISM. By Joseph Paxson Iddings, ph.d.,
sc.d.
(Second printing.) Price $5.00 net.
ORGANISM AND ENVIRONMENT AS ILLUSTRATED BY THE
PHYSIOLOGY OF BREATHING. By John Scott Haldane, m.d., ll.d.,
f.r.s., Fellow of New College, Oxford University.
(Second printing.) Price $1.25 net.
Page 8
A CENTURY OF SCIENCE
IN AMERICA
IN AMERICA
Page 9
A
CENTURY OF SCIENCE
IN AMERICA
WITH SPECIAL REFERENCE TO THE AMERICAN
JOURNAL OF SCIENCE 1818–1918
BY
EDWARD SALISBURY DANA · CHARLES SCHUCHERT
HERBERT E. GREGORY · JOSEPH BARRELL · GEORGE OTIS SMITH
RICHARD SWANN LULL · LOUIS V. PIRSSON
WILLIAM E. FORD · R. B. SOSMAN · HORACE L. WELLS
HARRY W. FOOTE · LEIGH PAGE · WESLEY R. COE
AND GEORGE L. GOODALE
NEW HAVEN
CENTURY OF SCIENCE
IN AMERICA
WITH SPECIAL REFERENCE TO THE AMERICAN
JOURNAL OF SCIENCE 1818–1918
BY
EDWARD SALISBURY DANA · CHARLES SCHUCHERT
HERBERT E. GREGORY · JOSEPH BARRELL · GEORGE OTIS SMITH
RICHARD SWANN LULL · LOUIS V. PIRSSON
WILLIAM E. FORD · R. B. SOSMAN · HORACE L. WELLS
HARRY W. FOOTE · LEIGH PAGE · WESLEY R. COE
AND GEORGE L. GOODALE
NEW HAVEN
Page 10
YALE UNIVERSITY PRESS
LONDON · HUMPHREY MILFORD · OXFORD UNIVERSITY PRESS
MDCCCCXVIII
LONDON · HUMPHREY MILFORD · OXFORD UNIVERSITY PRESS
MDCCCCXVIII
Page 11
COPYRIGHT, 1918, BY
YALE UNIVERSITY PRESS
YALE UNIVERSITY PRESS
Page 12
PREFATORY NOTE
The present book commemorates the one-hundredth anniversary of the
founding of the American Journal of Science by Benjamin Silliman in July,
1818. The opening chapter gives a somewhat detailed account of the early
days of the Journal, with a sketch of its subsequent history. The remaining
chapters are devoted to the principal branches of science which have been
prominent in the pages of the Journal. They have been written with a view
to showing in each case the position of the science in 1818 and the general
progress made during the century; special prominence is given to American
science and particularly to the contributions to it to be found in the Journal’s
pages. References to specific papers in the Journal are in most cases
included in the text and give simply volume, page, and date, as (24, 105,
1833); when these and other references are in considerable number they
have been brought together as a Bibliography at the end of the chapter.
The entire cost of the present book is defrayed from the income of the
Mrs. Hepsa Ely Silliman Memorial Fund, established under the will of
Augustus Ely Silliman, a nephew of Benjamin Silliman, who died in 1884.
Certain of the chapters here printed have been made the basis of a series of
seven Silliman Lectures in accordance with the terms of that gift. The
selection of these lectures has been determined by the convenience of the
gentlemen concerned and in part also by the nature of the subject.
The present book commemorates the one-hundredth anniversary of the
founding of the American Journal of Science by Benjamin Silliman in July,
1818. The opening chapter gives a somewhat detailed account of the early
days of the Journal, with a sketch of its subsequent history. The remaining
chapters are devoted to the principal branches of science which have been
prominent in the pages of the Journal. They have been written with a view
to showing in each case the position of the science in 1818 and the general
progress made during the century; special prominence is given to American
science and particularly to the contributions to it to be found in the Journal’s
pages. References to specific papers in the Journal are in most cases
included in the text and give simply volume, page, and date, as (24, 105,
1833); when these and other references are in considerable number they
have been brought together as a Bibliography at the end of the chapter.
The entire cost of the present book is defrayed from the income of the
Mrs. Hepsa Ely Silliman Memorial Fund, established under the will of
Augustus Ely Silliman, a nephew of Benjamin Silliman, who died in 1884.
Certain of the chapters here printed have been made the basis of a series of
seven Silliman Lectures in accordance with the terms of that gift. The
selection of these lectures has been determined by the convenience of the
gentlemen concerned and in part also by the nature of the subject.
Page 13
TABLE OF CONTENTS
Page 14
Page
Prefatory Note vii
I. The American Journal of Science from
1818 to 1918. Edward Salisbury Dana 13
II. A Century of Geology: The Progress of
Historical Geology in North America.
Charles Schuchert 60
III. A Century of Geology: Steps of Progress
in the Interpretation of Land Forms.
Herbert E. Gregory 122
IV. A Century of Geology (continued): The
Growth of Knowledge of Earth
Structure. Joseph Barrell 153
V. A Century of Government Geological
Surveys. George Otis Smith 193
VI. On the Development of Vertebrate
Paleontology. Richard Swann Lull 217
VII. The Rise of Petrology as a Science.
Louis V. Pirsson 248
VIII. The Growth of Mineralogy from 1818 to
1918. William E. Ford 268
IX. The Work of the Geophysical Laboratory
of the Carnegie Institution of
Washington. R. B. Sosman 284
X. The Progress of Chemistry during the
Past One Hundred Years. Horace L.
Wells and Harry W. Foote 288
XI. A Century’s Progress in Physics. Leigh
Page 335
XII. A Century of Zoology in America.
Wesley R. Coe 391
XIII. The Development of Botany since 1818.
George L. Goodale 439
Prefatory Note vii
I. The American Journal of Science from
1818 to 1918. Edward Salisbury Dana 13
II. A Century of Geology: The Progress of
Historical Geology in North America.
Charles Schuchert 60
III. A Century of Geology: Steps of Progress
in the Interpretation of Land Forms.
Herbert E. Gregory 122
IV. A Century of Geology (continued): The
Growth of Knowledge of Earth
Structure. Joseph Barrell 153
V. A Century of Government Geological
Surveys. George Otis Smith 193
VI. On the Development of Vertebrate
Paleontology. Richard Swann Lull 217
VII. The Rise of Petrology as a Science.
Louis V. Pirsson 248
VIII. The Growth of Mineralogy from 1818 to
1918. William E. Ford 268
IX. The Work of the Geophysical Laboratory
of the Carnegie Institution of
Washington. R. B. Sosman 284
X. The Progress of Chemistry during the
Past One Hundred Years. Horace L.
Wells and Harry W. Foote 288
XI. A Century’s Progress in Physics. Leigh
Page 335
XII. A Century of Zoology in America.
Wesley R. Coe 391
XIII. The Development of Botany since 1818.
George L. Goodale 439
Page 15
PORTRAITS
Benjamin Silliman Frontispiece
From a painting by G. S. Hubbard, Esq., in possession of
Miss Henrietta W. Hubbard
Benjamin Silliman, Jr. opposite
page 28
James D. Dana „„ 36
Edward S. Dana „„ 48
Wolcott Gibbs „„ 52
James Hall „„ 84
G. K. Gilbert „„ 140
Edward Hitchcock „„ 156
O. C. Marsh „„ 232
F. V. Hayden „„ 196
J. W. Powell „„ 204
Clarence King „„ 208
George J. Brush „„ 276
J. Willard Gibbs „„ 324
H. A. Newton „„ 336
James Clerk Maxwell „„ 348
Louis Agassiz „„ 404
Thomas H. Huxley „„ 410
A. E. Verrill „„ 412
Asa Gray „„ 444
Charles Darwin „„ 452
Benjamin Silliman Frontispiece
From a painting by G. S. Hubbard, Esq., in possession of
Miss Henrietta W. Hubbard
Benjamin Silliman, Jr. opposite
page 28
James D. Dana „„ 36
Edward S. Dana „„ 48
Wolcott Gibbs „„ 52
James Hall „„ 84
G. K. Gilbert „„ 140
Edward Hitchcock „„ 156
O. C. Marsh „„ 232
F. V. Hayden „„ 196
J. W. Powell „„ 204
Clarence King „„ 208
George J. Brush „„ 276
J. Willard Gibbs „„ 324
H. A. Newton „„ 336
James Clerk Maxwell „„ 348
Louis Agassiz „„ 404
Thomas H. Huxley „„ 410
A. E. Verrill „„ 412
Asa Gray „„ 444
Charles Darwin „„ 452
Page 16
A CENTURY OF SCIENCE
IN AMERICA
I
THE AMERICAN JOURNAL OF SCIENCE FROM 1818 TO
1918
By EDWARD S. DANA
Introduction.
In July, 1818, one hundred years ago, the first number of the American
Journal of Science and Arts was given to the public. This is the only
scientific periodical in this country to maintain an uninterrupted existence
since that early date, and this honor is shared with hardly more than half a
dozen other independent scientific periodicals in the world at large. Similar
publications of learned societies for the same period are also very few in
number.
It is interesting, on the occasion of this centenary, to glance back at the
position of science and scientific literature in the world’s intellectual life in
the early part of the nineteenth century, and to consider briefly the
IN AMERICA
I
THE AMERICAN JOURNAL OF SCIENCE FROM 1818 TO
1918
By EDWARD S. DANA
Introduction.
In July, 1818, one hundred years ago, the first number of the American
Journal of Science and Arts was given to the public. This is the only
scientific periodical in this country to maintain an uninterrupted existence
since that early date, and this honor is shared with hardly more than half a
dozen other independent scientific periodicals in the world at large. Similar
publications of learned societies for the same period are also very few in
number.
It is interesting, on the occasion of this centenary, to glance back at the
position of science and scientific literature in the world’s intellectual life in
the early part of the nineteenth century, and to consider briefly the
Page 17
marvelous record of combined scientific and industrial progress of the
hundred years following—subjects to be handled in detail in the succeeding
chapters. It is fitting also that we should recall the man who founded the
Journal, the conditions under which he worked, and the difficulties he
encountered. Finally, we must review, but more briefly, the subsequent
history of what has so often been called after its founder, “Silliman’s
Journal.”
The nineteenth century, and particularly the hundred years in which we
are now interested, must always stand out in the history of the world as the
period which has combined the greatest development in all departments of
science with the most extraordinary industrial progress. It was not until this
century that scientific investigation used to their full extent the twin
methods of observation and experiment. In cases too numerous to mention
they have given us first, a tentative hypothesis; then, through the testing and
correcting of the hypothesis by newly acquired data, an accepted theory has
been arrived at; finally, by the same means carried further has been
established one of nature’s laws.
Early Science.—Looking far back into the past, it seems surprising that
science should have had so late a growth, but the wonderful record of man’s
genius in the monuments he erected and in architectural remains shows that
the working of the human mind found expression first in art and further
man also turned to literature. So far as man’s thought was constructive, the
early results were systems of philosophy, and explanations of the order of
things as seen from within, not as shown by nature herself. We date the real
beginning of science with the Greeks, but it was the century that preceded
Aristotle that saw the building of the Parthenon and the sculptures of
Phidias. Even the great Aristotle himself (384–322 B. C.) though he is
sometimes called the “founder of natural history,” was justly accused by
Lord Bacon many centuries later of having formed his theories first and
then to have forced the facts to agree with them.
The bringing together of facts through observation alone began, to be
sure, very early, for it was the motion of the sun, moon, and stars and the
relation of the earth to them that first excited interest, and, especially in the
countries of the East, led to the accumulation of data as to the motion of the
planets, of comets and the occurrence of eclipses. But there was no
coördination of these facts and they were so involved in man’s superstition
hundred years following—subjects to be handled in detail in the succeeding
chapters. It is fitting also that we should recall the man who founded the
Journal, the conditions under which he worked, and the difficulties he
encountered. Finally, we must review, but more briefly, the subsequent
history of what has so often been called after its founder, “Silliman’s
Journal.”
The nineteenth century, and particularly the hundred years in which we
are now interested, must always stand out in the history of the world as the
period which has combined the greatest development in all departments of
science with the most extraordinary industrial progress. It was not until this
century that scientific investigation used to their full extent the twin
methods of observation and experiment. In cases too numerous to mention
they have given us first, a tentative hypothesis; then, through the testing and
correcting of the hypothesis by newly acquired data, an accepted theory has
been arrived at; finally, by the same means carried further has been
established one of nature’s laws.
Early Science.—Looking far back into the past, it seems surprising that
science should have had so late a growth, but the wonderful record of man’s
genius in the monuments he erected and in architectural remains shows that
the working of the human mind found expression first in art and further
man also turned to literature. So far as man’s thought was constructive, the
early results were systems of philosophy, and explanations of the order of
things as seen from within, not as shown by nature herself. We date the real
beginning of science with the Greeks, but it was the century that preceded
Aristotle that saw the building of the Parthenon and the sculptures of
Phidias. Even the great Aristotle himself (384–322 B. C.) though he is
sometimes called the “founder of natural history,” was justly accused by
Lord Bacon many centuries later of having formed his theories first and
then to have forced the facts to agree with them.
The bringing together of facts through observation alone began, to be
sure, very early, for it was the motion of the sun, moon, and stars and the
relation of the earth to them that first excited interest, and, especially in the
countries of the East, led to the accumulation of data as to the motion of the
planets, of comets and the occurrence of eclipses. But there was no
coördination of these facts and they were so involved in man’s superstition
Page 18
as to be of little value. In passing, however, it is worthy of mention that the
Chinese astronomical data accumulated more than two thousand years
before the Christian era have in trained hands yielded results of no small
significance.
Doubtless were full knowledge available as to the science existing in the
early civilizations, we should rate it higher than we can at present, but it
would probably prove even then to have been developed from within, like
the philosophies of the Greeks, and with but minor influence from nature
herself. It is indeed remarkable that down to the time with which we are
immediately concerned, it was the branches of mathematics, as arithmetic
and geometry and later their applications, that were first and most fully
developed: in other words those lines of science least closely connected
with nature.
Of the importance to science of the Greek school at Alexandria in the
second and third centuries B. C., there can be no question. The geometry of
Euclid (about 300 B. C.) was marvelous in its completeness as in clearness
of logical method. Hipparchus (about 160–125 B. C.) gave the world the
elements of trigonometry and developed astronomy so that Ptolemy 260
years later was able to construct a system that was well developed, though
in error in the fundamental idea as to the relative position of the earth. It is
interesting to note that the Almagest of Ptolemy was thought worthy of
republication by the Carnegie Institution only a year or two since. This
great astronomical work, by the way, had no successor till that of the Arab
Ulugh Bey in the fifteenth century, which within a few months has also
been made available by the same Institution.
To the Alexandrian school also belongs Archimedes (287–212 B. C.),
who, as every school boy knows, was the founder of mechanics and in fact
almost a modern physical experimenter. He invented the water screw for
raising water; he discovered the principle of the lever, which appealed so
keenly to his imagination that he called for a ποῦ στῶ, or fulcrum, on which
to place it so as to move the earth itself. He was still nearer to modern
physics in his reputed plan of burning up a hostile fleet by converging the
sun’s rays by a system of great mirrors.
To the Romans, science owes little beyond what is implied in their vast
architectural monuments, buildings and aqueducts which were erected at
home and in the countries of their conquests. The elder Pliny (23–79 A. D.)
Chinese astronomical data accumulated more than two thousand years
before the Christian era have in trained hands yielded results of no small
significance.
Doubtless were full knowledge available as to the science existing in the
early civilizations, we should rate it higher than we can at present, but it
would probably prove even then to have been developed from within, like
the philosophies of the Greeks, and with but minor influence from nature
herself. It is indeed remarkable that down to the time with which we are
immediately concerned, it was the branches of mathematics, as arithmetic
and geometry and later their applications, that were first and most fully
developed: in other words those lines of science least closely connected
with nature.
Of the importance to science of the Greek school at Alexandria in the
second and third centuries B. C., there can be no question. The geometry of
Euclid (about 300 B. C.) was marvelous in its completeness as in clearness
of logical method. Hipparchus (about 160–125 B. C.) gave the world the
elements of trigonometry and developed astronomy so that Ptolemy 260
years later was able to construct a system that was well developed, though
in error in the fundamental idea as to the relative position of the earth. It is
interesting to note that the Almagest of Ptolemy was thought worthy of
republication by the Carnegie Institution only a year or two since. This
great astronomical work, by the way, had no successor till that of the Arab
Ulugh Bey in the fifteenth century, which within a few months has also
been made available by the same Institution.
To the Alexandrian school also belongs Archimedes (287–212 B. C.),
who, as every school boy knows, was the founder of mechanics and in fact
almost a modern physical experimenter. He invented the water screw for
raising water; he discovered the principle of the lever, which appealed so
keenly to his imagination that he called for a ποῦ στῶ, or fulcrum, on which
to place it so as to move the earth itself. He was still nearer to modern
physics in his reputed plan of burning up a hostile fleet by converging the
sun’s rays by a system of great mirrors.
To the Romans, science owes little beyond what is implied in their vast
architectural monuments, buildings and aqueducts which were erected at
home and in the countries of their conquests. The elder Pliny (23–79 A. D.)
Page 19
most nearly deserved to be called a man of science, but his work on natural
history, comprised in thirty-seven volumes, is hardly more than a
compilation of fable, fact, and fancy, and is sometimes termed a collection
of anecdotes. He lost his life in the “grandest geological event of antiquity,”
the eruption of Vesuvius, which is vividly described by his nephew, the
younger Pliny, in “one of the most remarkable literary productions in the
domain of geology” (Zittel).
With the fall of Rome and the decline of Roman civilization came a
period of intellectual darkness, from which the world did not emerge until
the revival of learning in the fifteenth and sixteenth centuries. Then the
extension of geographical knowledge went hand in hand with the
development of art, literature, and the birth of a new science. Copernicus
(1473–1543) gave the world at last a sun-controlled solar system; Kepler
(1571–1630) formulated the laws governing the motion of the planets;
Galileo (1564–1642) with his telescope opened up new vistas of
astronomical knowledge and laid the foundations of mechanics; while
Leonardo da Vinci (1452–1519), painter, sculptor, architect, engineer,
musician and true scientist, studied the laws of falling bodies and solved the
riddle of the fossils in the rocks. Still later Newton (1642–1727) established
the law of gravitation, developed the calculus, put mechanics upon a solid
basis and also worked out the properties of lenses and prisms so that his
Optics (1704) will always have a prominent place in the history of science.
From the time of the Renaissance on science grew steadily, but it was not
till the latter half of the eighteenth century that the foundations in most of
the lines recognized to-day were fully laid. Much of what was
accomplished then is, at least, outlined in the chapters following.
Our standpoint in the early years of the nineteenth century, just before the
American Journal had its beginning, may be briefly summarized as follows:
A desire for knowledge was almost universal and, therefore, also a general
interest in the development of science. Mathematics was firmly established
and the mathematical side of astronomy and natural philosophy—as physics
was then called—was well developed. Many of the phenomena of heat and
their applications, as in the steam engine of Watt, were known and even the
true nature of heat had been almost established by our countryman, Count
Rumford; but of electricity there were only a few sparks of knowledge.
Chemistry had had its foundation firmly laid by Priestley, Lavoisier, and
history, comprised in thirty-seven volumes, is hardly more than a
compilation of fable, fact, and fancy, and is sometimes termed a collection
of anecdotes. He lost his life in the “grandest geological event of antiquity,”
the eruption of Vesuvius, which is vividly described by his nephew, the
younger Pliny, in “one of the most remarkable literary productions in the
domain of geology” (Zittel).
With the fall of Rome and the decline of Roman civilization came a
period of intellectual darkness, from which the world did not emerge until
the revival of learning in the fifteenth and sixteenth centuries. Then the
extension of geographical knowledge went hand in hand with the
development of art, literature, and the birth of a new science. Copernicus
(1473–1543) gave the world at last a sun-controlled solar system; Kepler
(1571–1630) formulated the laws governing the motion of the planets;
Galileo (1564–1642) with his telescope opened up new vistas of
astronomical knowledge and laid the foundations of mechanics; while
Leonardo da Vinci (1452–1519), painter, sculptor, architect, engineer,
musician and true scientist, studied the laws of falling bodies and solved the
riddle of the fossils in the rocks. Still later Newton (1642–1727) established
the law of gravitation, developed the calculus, put mechanics upon a solid
basis and also worked out the properties of lenses and prisms so that his
Optics (1704) will always have a prominent place in the history of science.
From the time of the Renaissance on science grew steadily, but it was not
till the latter half of the eighteenth century that the foundations in most of
the lines recognized to-day were fully laid. Much of what was
accomplished then is, at least, outlined in the chapters following.
Our standpoint in the early years of the nineteenth century, just before the
American Journal had its beginning, may be briefly summarized as follows:
A desire for knowledge was almost universal and, therefore, also a general
interest in the development of science. Mathematics was firmly established
and the mathematical side of astronomy and natural philosophy—as physics
was then called—was well developed. Many of the phenomena of heat and
their applications, as in the steam engine of Watt, were known and even the
true nature of heat had been almost established by our countryman, Count
Rumford; but of electricity there were only a few sparks of knowledge.
Chemistry had had its foundation firmly laid by Priestley, Lavoisier, and
Page 20
Dalton, while Berzelius was pushing rapidly forward. Geology had also its
roots down, chiefly through the work of Hutton and William Smith, though
the earth was as yet essentially an unexplored field. Systematic zoology and
botany had been firmly grounded by Buffon, Lamarck and Cuvier, on the
one hand, and Linnæus on the other; but of all that is embraced under the
biology of the latter half of the nineteenth century the world knew nothing.
The statements of Silliman in his Introductory Remarks in the first number,
quoted in part on a following page, put the matter still more fully, but they
are influenced by the enthusiasm of the time and he could have had little
comprehension of what was to be the record of the next one hundred years.
Now, leaving this hasty and incomplete retrospect and coming down to
1918, we find the contrast between to-day and 1818 perhaps most strikingly
brought out, on the material side, if we consider the ability of man, in the
early part of the nineteenth century, to meet the demands upon him in the
matter of transportation of himself and his property. In 1800, he had hardly
advanced beyond his ancestor of the earliest civilization; on the contrary, he
was still dependent for transportation on land upon the muscular efforts of
himself and domesticated animals, while at sea he had only the use of sails
in addition. The first application of the steam engine with commercial
success was made by Fulton when, in 1807, the steamboat “Clermont”
made its famous trip on the Hudson River. Since then, step by step,
transportation has been made more and more rapid, economical and
convenient, both on land and water. This has come first through the
perfection of the steam engine; later through the agency of electricity, and
still further and more universally by the use of gasolene motors. Finally, in
these early years of the twentieth century, what seemed once a wild dream
of the imagination has been realized, and man has gained the conquest of
the air; while the perfection of the submarine is as wonderful as its work
can be deadly.
Hardly less marvelous is the practical annihilation of space and time in
the electric transmission of human thought and speech by wire and by ether
waves. While, still further, the same electrical current now gives man his
artificial illumination and serves him in a thousand ways besides.
But the limitations of space have also been conquered, during the same
period, by the spectroscope which brings a knowledge of the material
nature of the sun and the fixed stars and of their motion in the line of sight;
roots down, chiefly through the work of Hutton and William Smith, though
the earth was as yet essentially an unexplored field. Systematic zoology and
botany had been firmly grounded by Buffon, Lamarck and Cuvier, on the
one hand, and Linnæus on the other; but of all that is embraced under the
biology of the latter half of the nineteenth century the world knew nothing.
The statements of Silliman in his Introductory Remarks in the first number,
quoted in part on a following page, put the matter still more fully, but they
are influenced by the enthusiasm of the time and he could have had little
comprehension of what was to be the record of the next one hundred years.
Now, leaving this hasty and incomplete retrospect and coming down to
1918, we find the contrast between to-day and 1818 perhaps most strikingly
brought out, on the material side, if we consider the ability of man, in the
early part of the nineteenth century, to meet the demands upon him in the
matter of transportation of himself and his property. In 1800, he had hardly
advanced beyond his ancestor of the earliest civilization; on the contrary, he
was still dependent for transportation on land upon the muscular efforts of
himself and domesticated animals, while at sea he had only the use of sails
in addition. The first application of the steam engine with commercial
success was made by Fulton when, in 1807, the steamboat “Clermont”
made its famous trip on the Hudson River. Since then, step by step,
transportation has been made more and more rapid, economical and
convenient, both on land and water. This has come first through the
perfection of the steam engine; later through the agency of electricity, and
still further and more universally by the use of gasolene motors. Finally, in
these early years of the twentieth century, what seemed once a wild dream
of the imagination has been realized, and man has gained the conquest of
the air; while the perfection of the submarine is as wonderful as its work
can be deadly.
Hardly less marvelous is the practical annihilation of space and time in
the electric transmission of human thought and speech by wire and by ether
waves. While, still further, the same electrical current now gives man his
artificial illumination and serves him in a thousand ways besides.
But the limitations of space have also been conquered, during the same
period, by the spectroscope which brings a knowledge of the material
nature of the sun and the fixed stars and of their motion in the line of sight;
Page 21
while spectrum analysis has revealed the existence of many new elements
and opened up vistas as to the nature of matter.
The chemist and the physicist, often working together in the investigation
of the problems lying between their two departments, have accumulated a
staggering array of new facts from which the principles of their sciences
have been deduced. Many new elements have been discovered, in fact
nearly all called for by the periodic law; the so-called fixed gases have been
liquefied, and now air in liquid form is almost a plaything; the absolute zero
has been nearly reached in the boiling point of helium; physical
measurements in great precision have been carried out in both directions for
temperatures far beyond any scale that was early conceived possible; the
atom, once supposed to be indivisible, has been shown to be made up of the
much smaller electrons, while its disintegration in radium and its
derivatives has been traced out and with consequences only as yet partly
understood but certainly having far-reaching consequences; at one point we
seem to be brought near to the transmutation of the elements which was so
long the dream of the alchemist. Still again photography has been
discovered and perfected and with the use of X-rays it gives a picture of the
structure of bodies totally opaque to the eye; the same X-rays seem likely to
locate and determine the atoms in the crystal.
Here and at many other points we are reaching out to a knowledge of the
ultimate nature of matter.
In geology, vast progress has been made in the knowledge of the earth,
not only as to its features now exhibited at or near the surface, but also as to
its history in past ages, of the development of its structure, the minute
history of its life, the phenomena of its earthquakes, volcanoes, etc.
Geological surveys in all civilized countries have been carried to a high
degree of perfection.
In biology, itself a word which though used by Lamarck did not come
into use till taken up by Huxley, and then by Herbert Spencer in the middle
of the century, the progress is no less remarkable as is well developed in a
later chapter of this volume.
Although not falling within our sphere, it would be wrong, too, not to
recognize also the growth of medicine, especially through the knowledge of
bacteria and their functions, and of disease germs and the methods of
and opened up vistas as to the nature of matter.
The chemist and the physicist, often working together in the investigation
of the problems lying between their two departments, have accumulated a
staggering array of new facts from which the principles of their sciences
have been deduced. Many new elements have been discovered, in fact
nearly all called for by the periodic law; the so-called fixed gases have been
liquefied, and now air in liquid form is almost a plaything; the absolute zero
has been nearly reached in the boiling point of helium; physical
measurements in great precision have been carried out in both directions for
temperatures far beyond any scale that was early conceived possible; the
atom, once supposed to be indivisible, has been shown to be made up of the
much smaller electrons, while its disintegration in radium and its
derivatives has been traced out and with consequences only as yet partly
understood but certainly having far-reaching consequences; at one point we
seem to be brought near to the transmutation of the elements which was so
long the dream of the alchemist. Still again photography has been
discovered and perfected and with the use of X-rays it gives a picture of the
structure of bodies totally opaque to the eye; the same X-rays seem likely to
locate and determine the atoms in the crystal.
Here and at many other points we are reaching out to a knowledge of the
ultimate nature of matter.
In geology, vast progress has been made in the knowledge of the earth,
not only as to its features now exhibited at or near the surface, but also as to
its history in past ages, of the development of its structure, the minute
history of its life, the phenomena of its earthquakes, volcanoes, etc.
Geological surveys in all civilized countries have been carried to a high
degree of perfection.
In biology, itself a word which though used by Lamarck did not come
into use till taken up by Huxley, and then by Herbert Spencer in the middle
of the century, the progress is no less remarkable as is well developed in a
later chapter of this volume.
Although not falling within our sphere, it would be wrong, too, not to
recognize also the growth of medicine, especially through the knowledge of
bacteria and their functions, and of disease germs and the methods of
Page 22
combating them. The world can never forget the debt it owes to Pasteur and
Lister and many later investigators in this field.
To follow out this subject further would be to encroach upon the field of
the chapters following, but, more important and fundamental still than all
the facts discovered and the phenomena investigated has been the
establishment of certain broad scientific principles which have
revolutionized modern thought and shown the relation between sciences
seemingly independent. The law of conservation of energy in the physical
world and the principle of material and organic evolution may well be said
to be the greatest generalizations of the human mind. Although suggestions
in regard to them, particularly the latter, are to be found in the writings of
early authors, the establishment and general acceptance of these principles
belong properly to the middle of the nineteenth century. They stand as the
crowning achievement of the scientific thought of the period in which we
are interested.
Any mere enumeration of the vast fund of knowledge accumulated by the
efforts of man through observation and experiment in the period in which
we are interested would be a dry summary, and yet would give some
measure of what this marvelous period has accomplished. As in geography,
man’s energy has in recent years removed the reproach of a “Dark
Continent,” of “unexplored” central Asia and the once “inaccessible polar
regions,” so in the different departments of science, he has opened up many
unknown fields and accumulated vast stores of knowledge. It might even
seem as if the limit of the unknown were being approached. There remains,
however, this difference in the analogy, that in science the fundamental
relations—as, for example, the nature of gravitation, of matter, of energy, of
electricity; the actual nature and source of life—the solution of these and
other similar problems still lies in the future. What the result of continued
research may be no one can predict, but even with these possibilities before
us, it is hardly rash to say that so great a combined progress of pure and
applied science as that of the past hundred years is not likely to be again
realized.
Lister and many later investigators in this field.
To follow out this subject further would be to encroach upon the field of
the chapters following, but, more important and fundamental still than all
the facts discovered and the phenomena investigated has been the
establishment of certain broad scientific principles which have
revolutionized modern thought and shown the relation between sciences
seemingly independent. The law of conservation of energy in the physical
world and the principle of material and organic evolution may well be said
to be the greatest generalizations of the human mind. Although suggestions
in regard to them, particularly the latter, are to be found in the writings of
early authors, the establishment and general acceptance of these principles
belong properly to the middle of the nineteenth century. They stand as the
crowning achievement of the scientific thought of the period in which we
are interested.
Any mere enumeration of the vast fund of knowledge accumulated by the
efforts of man through observation and experiment in the period in which
we are interested would be a dry summary, and yet would give some
measure of what this marvelous period has accomplished. As in geography,
man’s energy has in recent years removed the reproach of a “Dark
Continent,” of “unexplored” central Asia and the once “inaccessible polar
regions,” so in the different departments of science, he has opened up many
unknown fields and accumulated vast stores of knowledge. It might even
seem as if the limit of the unknown were being approached. There remains,
however, this difference in the analogy, that in science the fundamental
relations—as, for example, the nature of gravitation, of matter, of energy, of
electricity; the actual nature and source of life—the solution of these and
other similar problems still lies in the future. What the result of continued
research may be no one can predict, but even with these possibilities before
us, it is hardly rash to say that so great a combined progress of pure and
applied science as that of the past hundred years is not likely to be again
realized.
Page 23
Scientific Periodical Literature in 1818.
The contrast in scientific activity between 1818 and 1918 is nowhere
more strikingly shown than in the amount of scientific periodical literature
of the two periods. Of the thousands of scientific journals and regular
publications by scientific societies and academies to-day, but a very small
number have carried on a continuous and practically unbroken existence
since 1818. This small amount of periodical scientific literature in the early
part of the last century is significant as giving a fair indication of the very
limited extent to which scientific investigation appealed to the intellectual
life of the time. Some definite facts in regard to the scientific publications
of those early days seem to be called for.
Learned societies and academies, devoted to literature and science, were
formed very early but at first for occasional meetings only and regular
publications were in most cases not begun till a very much later date. Some
of the earliest—not to go back of the Renaissance—are the following:
1560. Naples, Academia Secretorum Naturæ.
1603. Rome, Accademia dei Lincei.
1651. Leipzig, Academia Naturæ Curiosum.
1657. Florence, Accademia del Cimento.
1662. London, Royal Society.
1666. Paris, Académie des Sciences.
1690. Bologna, Accademia delle Scienze.
1700. Berlin, Societas Regia Scientiarum. This was the forerunner of the K. preuss. Akad. d.
Wissenschaften.
The Royal Society of London, whose existence dates from 1645, though
not definitely chartered until 1662, began the publication of its
“Philosophical Transactions” in 1665 and has continued it practically
unbroken to the present time; this is a unique record. Following this, other
early—but in most cases not continuous—publications were those of Paris
(1699); Berlin (1710); Upsala (1720); Petrograd, 1728; Stockholm (1739);
and Copenhagen (1743).
The contrast in scientific activity between 1818 and 1918 is nowhere
more strikingly shown than in the amount of scientific periodical literature
of the two periods. Of the thousands of scientific journals and regular
publications by scientific societies and academies to-day, but a very small
number have carried on a continuous and practically unbroken existence
since 1818. This small amount of periodical scientific literature in the early
part of the last century is significant as giving a fair indication of the very
limited extent to which scientific investigation appealed to the intellectual
life of the time. Some definite facts in regard to the scientific publications
of those early days seem to be called for.
Learned societies and academies, devoted to literature and science, were
formed very early but at first for occasional meetings only and regular
publications were in most cases not begun till a very much later date. Some
of the earliest—not to go back of the Renaissance—are the following:
1560. Naples, Academia Secretorum Naturæ.
1603. Rome, Accademia dei Lincei.
1651. Leipzig, Academia Naturæ Curiosum.
1657. Florence, Accademia del Cimento.
1662. London, Royal Society.
1666. Paris, Académie des Sciences.
1690. Bologna, Accademia delle Scienze.
1700. Berlin, Societas Regia Scientiarum. This was the forerunner of the K. preuss. Akad. d.
Wissenschaften.
The Royal Society of London, whose existence dates from 1645, though
not definitely chartered until 1662, began the publication of its
“Philosophical Transactions” in 1665 and has continued it practically
unbroken to the present time; this is a unique record. Following this, other
early—but in most cases not continuous—publications were those of Paris
(1699); Berlin (1710); Upsala (1720); Petrograd, 1728; Stockholm (1739);
and Copenhagen (1743).
Page 24
For the latter half of the eighteenth century, when the foundations of our
modern science were being rapidly laid, a considerable list might be given
of early publications of similar scientific bodies. Some of the prominent
ones are: Göttingen (1750), Munich (1759), Brussels (1769), Prague (1775),
Turin (1784), Dublin (1788), etc. The early years of the nineteenth century
saw the beginnings of many others, particularly in northern Italy. It is to be
noted that, as stated, only rarely were the publications of these learned
societies even approximately continuous. In the majority of cases the issue
of transactions or proceedings was highly irregular and often interrupted.
In this country the earliest scientific bodies are the following:
Philadelphia. American Philosophical Society, founded in 1743. Transactions were published
1771–1809; then interrupted until 1818 et seq.
Boston. American Academy of Arts and Sciences, founded in 1780. Memoirs, 1785–1821; and
then 1833 et seq.
New Haven. Connecticut Academy of Arts and Sciences, begun in 1799. Memoirs, vol. 1, 1810–
16; Transactions, 1866 et seq.
Philadelphia. Academy of Natural Sciences, begun in 1812. Journal, 1817–1842; and from 1847 et
seq.
New York. Lyceum of Natural History, 1817; later (1876) became the New York Academy of
Sciences. Annals from 1823; Proceedings from 1870.
The situation is somewhat similar as to independent scientific journals. A
list of the names of those started only to find an early death would be a very
long one, but interesting only historically and as showing a spasmodic but
unsustained striving after scientific growth.
It seems worth while, however, to give here the names of the periodicals
embracing one or more of the subjects of the American Journal, which
began at a very early date and most of which have maintained an
uninterrupted existence down to 1915. It should be added that certain
medical journals, not listed here, have also had a long and continued
existence.[1]
modern science were being rapidly laid, a considerable list might be given
of early publications of similar scientific bodies. Some of the prominent
ones are: Göttingen (1750), Munich (1759), Brussels (1769), Prague (1775),
Turin (1784), Dublin (1788), etc. The early years of the nineteenth century
saw the beginnings of many others, particularly in northern Italy. It is to be
noted that, as stated, only rarely were the publications of these learned
societies even approximately continuous. In the majority of cases the issue
of transactions or proceedings was highly irregular and often interrupted.
In this country the earliest scientific bodies are the following:
Philadelphia. American Philosophical Society, founded in 1743. Transactions were published
1771–1809; then interrupted until 1818 et seq.
Boston. American Academy of Arts and Sciences, founded in 1780. Memoirs, 1785–1821; and
then 1833 et seq.
New Haven. Connecticut Academy of Arts and Sciences, begun in 1799. Memoirs, vol. 1, 1810–
16; Transactions, 1866 et seq.
Philadelphia. Academy of Natural Sciences, begun in 1812. Journal, 1817–1842; and from 1847 et
seq.
New York. Lyceum of Natural History, 1817; later (1876) became the New York Academy of
Sciences. Annals from 1823; Proceedings from 1870.
The situation is somewhat similar as to independent scientific journals. A
list of the names of those started only to find an early death would be a very
long one, but interesting only historically and as showing a spasmodic but
unsustained striving after scientific growth.
It seems worth while, however, to give here the names of the periodicals
embracing one or more of the subjects of the American Journal, which
began at a very early date and most of which have maintained an
uninterrupted existence down to 1915. It should be added that certain
medical journals, not listed here, have also had a long and continued
existence.[1]
Page 25
Early Scientific Journals.
1771–1823. Journal de Physique, Paris; title changed several times.
1787–. Botanical Magazine. (For a time known as Curtis’s Journal).
1789–1816. Annales de Chimie, Paris. Continued from 1817 on as the Annales de Chimie et de
Physique.
1790. Journal der Physik, Halle (by Gren); from 1799 on became the Annalen der Physik (und
Chemie), Halle, Leipzig. The title has been somewhat changed from time to time though publication
has been continuous. Often referred to by the name of the editor-in-chief, as Gren, Gilbert,
Poggendorff, Wiedemann, etc.
1795–1815. Journal des Mines, Paris, continued from 1816 as the Annales des Mines.
1796–1815. Bibliothèque Britannique, Geneva. From 1816–1840, Bibliothèque Universelle, etc.
1846–1857, Archives des Sci. phys. nat. Since 1858 generally known as the Bibliothèque
Universelle.
1797. Journal of Natural Philosophy, Chemistry and the Arts (Nicholson’s Journal) London; united
in 1814 with the Philosophical Magazine (Tilloch’s Journal).
1798–. The Philosophical Magazine (originally by Tilloch). This absorbed Nicholson’s Journal
(above) in 1814; also the Annals of Philosophy (Thomson, Phillips) in 1827 and Brewsters’
Edinburgh Journal of Science in 1832.
1798–1803. Allgemeines Journal der Chemie (Scherer’s Journal). 1803–1806; continued as Neues
Allg. J. etc. (Gehlen’s Journal). Later title repeatedly changed and finally (1834 et seq.) Journal für
praktische Chemie.
1816–18. Journal of Science and the Arts, London. 181930, Quarterly J. etc. 1830–31, Journal of
the Royal Institution of Great Britain.
1818. American Journal of Science and Arts until 1880, when “the Arts” was dropped, New
Haven, Conn. First Series, 1–50, 1818–1845; Second Series, 1–50, 1846–1870; Third Series, 1–50,
1871–1895; Fourth Series, 1–45, 1896–June, 1918.
1818. Flora, or Allgemeine botanische Zeitung. Regensburg, Munich.
1820–1867. London Journal of Arts and Sciences (after 1855, Newton’s Journal).
1824–. Annales des sciences naturelles. Paris.
1826–. Linnæa, Berlin, Halle; from 1882 united with Jahrb. d. K. botan. Gartens.
1828–1840. Magazine of Natural History, London; united 1838 with the Annals of Natural History,
and known since 1841 as the Annals and Magazine of Natural History.
1828–. Journal of the Franklin Institute, Philadelphia, from 1826; earlier (1825) the American
Mechanics Magazine.
1832–. Annalen der Chemie (und Pharmacie) often known as Liebig’s Annalen. Leipzig, Lemgo.
1771–1823. Journal de Physique, Paris; title changed several times.
1787–. Botanical Magazine. (For a time known as Curtis’s Journal).
1789–1816. Annales de Chimie, Paris. Continued from 1817 on as the Annales de Chimie et de
Physique.
1790. Journal der Physik, Halle (by Gren); from 1799 on became the Annalen der Physik (und
Chemie), Halle, Leipzig. The title has been somewhat changed from time to time though publication
has been continuous. Often referred to by the name of the editor-in-chief, as Gren, Gilbert,
Poggendorff, Wiedemann, etc.
1795–1815. Journal des Mines, Paris, continued from 1816 as the Annales des Mines.
1796–1815. Bibliothèque Britannique, Geneva. From 1816–1840, Bibliothèque Universelle, etc.
1846–1857, Archives des Sci. phys. nat. Since 1858 generally known as the Bibliothèque
Universelle.
1797. Journal of Natural Philosophy, Chemistry and the Arts (Nicholson’s Journal) London; united
in 1814 with the Philosophical Magazine (Tilloch’s Journal).
1798–. The Philosophical Magazine (originally by Tilloch). This absorbed Nicholson’s Journal
(above) in 1814; also the Annals of Philosophy (Thomson, Phillips) in 1827 and Brewsters’
Edinburgh Journal of Science in 1832.
1798–1803. Allgemeines Journal der Chemie (Scherer’s Journal). 1803–1806; continued as Neues
Allg. J. etc. (Gehlen’s Journal). Later title repeatedly changed and finally (1834 et seq.) Journal für
praktische Chemie.
1816–18. Journal of Science and the Arts, London. 181930, Quarterly J. etc. 1830–31, Journal of
the Royal Institution of Great Britain.
1818. American Journal of Science and Arts until 1880, when “the Arts” was dropped, New
Haven, Conn. First Series, 1–50, 1818–1845; Second Series, 1–50, 1846–1870; Third Series, 1–50,
1871–1895; Fourth Series, 1–45, 1896–June, 1918.
1818. Flora, or Allgemeine botanische Zeitung. Regensburg, Munich.
1820–1867. London Journal of Arts and Sciences (after 1855, Newton’s Journal).
1824–. Annales des sciences naturelles. Paris.
1826–. Linnæa, Berlin, Halle; from 1882 united with Jahrb. d. K. botan. Gartens.
1828–1840. Magazine of Natural History, London; united 1838 with the Annals of Natural History,
and known since 1841 as the Annals and Magazine of Natural History.
1828–. Journal of the Franklin Institute, Philadelphia, from 1826; earlier (1825) the American
Mechanics Magazine.
1832–. Annalen der Chemie (und Pharmacie) often known as Liebig’s Annalen. Leipzig, Lemgo.
Page 26
The Founder of the American Journal of Science.
The establishment of a scientific journal in this country in 1818 was a
pioneer undertaking, requiring of its founder a rare degree of energy,
courage, and confidence in the future. It was necessary, not only to obtain
the material to fill its pages and the money to carry on the enterprise, but,
before the latter end could be accomplished, an audience must be found
among those who had hitherto felt little or no interest in the sciences. This
great work was accomplished by Benjamin Silliman, “the guardian of
American Science,” whose influence was second to none in the early
development of science in this country. Before speaking in some detail of
the early years of this Journal and of its subsequent history, it is proper that
some words should be given to its founder.
Benjamin Silliman, son of a general prominent in the Revolutionary War,
was born in Trumbull, Connecticut, on August 8, 1779. He was a graduate
of Yale College of the class of 1796. Though at first a student of law and
accepted for the bar in Connecticut, he was called in 1802 by President
Timothy Dwight—a man of rare breadth of mind—to occupy the newly
made chair of chemistry, mineralogy (and later geology) in Yale College at
New Haven. To fit himself for the work before him he carried on extensive
studies at home and in Philadelphia and spent the year 1805 in travels and
study at London and Edinburgh, and also on the Continent. His active duties
began in 1806 and from this time on he was in the service of Yale College
until his resignation in 1853. From the first, Silliman met with remarkable
success as a teacher and public lecturer in arousing an interest in science.
His breadth of knowledge, his enthusiasm for his chosen subjects and
power of clear presentation, combined with his fine presence and attractive
personality, made him a great leader in the science of the country and gave
him a unique position in the history of its development.
Much might be said of the man and his work, but, the best tribute is that
of James Dwight Dana, given in his inaugural address upon the occasion of
his beginning his duties as Silliman professor of geology in Yale College.
This was delivered on February 18, 1856, in what was then known as the
“Cabinet Building.” Dana says in part:
The establishment of a scientific journal in this country in 1818 was a
pioneer undertaking, requiring of its founder a rare degree of energy,
courage, and confidence in the future. It was necessary, not only to obtain
the material to fill its pages and the money to carry on the enterprise, but,
before the latter end could be accomplished, an audience must be found
among those who had hitherto felt little or no interest in the sciences. This
great work was accomplished by Benjamin Silliman, “the guardian of
American Science,” whose influence was second to none in the early
development of science in this country. Before speaking in some detail of
the early years of this Journal and of its subsequent history, it is proper that
some words should be given to its founder.
Benjamin Silliman, son of a general prominent in the Revolutionary War,
was born in Trumbull, Connecticut, on August 8, 1779. He was a graduate
of Yale College of the class of 1796. Though at first a student of law and
accepted for the bar in Connecticut, he was called in 1802 by President
Timothy Dwight—a man of rare breadth of mind—to occupy the newly
made chair of chemistry, mineralogy (and later geology) in Yale College at
New Haven. To fit himself for the work before him he carried on extensive
studies at home and in Philadelphia and spent the year 1805 in travels and
study at London and Edinburgh, and also on the Continent. His active duties
began in 1806 and from this time on he was in the service of Yale College
until his resignation in 1853. From the first, Silliman met with remarkable
success as a teacher and public lecturer in arousing an interest in science.
His breadth of knowledge, his enthusiasm for his chosen subjects and
power of clear presentation, combined with his fine presence and attractive
personality, made him a great leader in the science of the country and gave
him a unique position in the history of its development.
Much might be said of the man and his work, but, the best tribute is that
of James Dwight Dana, given in his inaugural address upon the occasion of
his beginning his duties as Silliman professor of geology in Yale College.
This was delivered on February 18, 1856, in what was then known as the
“Cabinet Building.” Dana says in part:
Page 27
“In entering upon the duties of this place, my thoughts turn rather to the past than to the subject of
the present hour. I feel that it is an honored place, honored by the labors of one who has been the
guardian of American Science from its childhood; who here first opened to the country the wonderful
records of geology; whose words of eloquence and earnest truth were but the overflow of a soul full
of noble sentiments and warm sympathies, the whole throwing a peculiar charm over his learning,
and rendering his name beloved as well as illustrious. Just fifty years since, Professor Silliman took
his station at the head of chemical and geological science in this college. Geology was then hardly
known by name in the land, out of these walls. Two years before, previous to his tour in Europe, the
whole cabinet of Yale was a half-bushel of unlabelled stones. On visiting England he found even in
London no school public or private, for geological instruction, and the science was not named in the
English universities. To the mines, quarries, and cliffs of England, the crags of Scotland, and the
meadows of Holland he looked for knowledge, and from these and the teachings of Murray, Jameson,
Hall, Hope, and Playfair, at Edinburgh, Professor Silliman returned, equipped for duty,—albeit a
great duty,—that of laying the foundation, and creating almost out of nothing a department not before
recognized in any institution in America.
He began his work in 1806. The science was without books—and, too, without system, except
such as its few cultivators had each for himself in his conceptions. It was the age of the first
beginnings of geology, when Wernerians and Huttonians were arrayed in a contest.... Professor
Silliman when at Edinburgh witnessed the strife, and while, as he says, his earliest predilections were
for the more peaceful mode of rock-making, these soon yielded to the accumulating evidence, and
both views became combined in his mind in one harmonious whole. The science, thus evolved, grew
with him and by him; for his own labors contributed to its extension. Every year was a year of
expansion and onward development, and the grandeur of the opening views found in him a ready and
appreciative response....
And while the sciences and truth have thus made progress here, through these labors of fifty years,
the means of study in the institution have no less increased. Instead of that half-bushel of stones,
which once went to Philadelphia for names, in a candle-box, you see above the largest mineral
cabinet in the country, which but for Professor Silliman, his attractions and his personal exertions
together, would never have been one of the glories of old Yale....
Moreover, the American Journal of Science,—now in its thirty-seventh year and seventieth volume
[1856],—projected and long-sustained solely by Professor Silliman, while ever distributing truth, has
also been ever gathering honors, and is one of the laurels of Yale.
We rejoice that in laying aside his studies, after so many years of labor, there is still no abated
vigor.... He retires as one whose right it is to throw the burden on others. Long may he be with us, to
enjoy the good he has done, and cheer us by his noble and benign presence.”
In addition to these words of Dana, much of vital interest in regard to
Silliman and his work will be gathered from what is given in the pages
immediately following, quoted from his personal statements in the early
volumes of the Journal.
the present hour. I feel that it is an honored place, honored by the labors of one who has been the
guardian of American Science from its childhood; who here first opened to the country the wonderful
records of geology; whose words of eloquence and earnest truth were but the overflow of a soul full
of noble sentiments and warm sympathies, the whole throwing a peculiar charm over his learning,
and rendering his name beloved as well as illustrious. Just fifty years since, Professor Silliman took
his station at the head of chemical and geological science in this college. Geology was then hardly
known by name in the land, out of these walls. Two years before, previous to his tour in Europe, the
whole cabinet of Yale was a half-bushel of unlabelled stones. On visiting England he found even in
London no school public or private, for geological instruction, and the science was not named in the
English universities. To the mines, quarries, and cliffs of England, the crags of Scotland, and the
meadows of Holland he looked for knowledge, and from these and the teachings of Murray, Jameson,
Hall, Hope, and Playfair, at Edinburgh, Professor Silliman returned, equipped for duty,—albeit a
great duty,—that of laying the foundation, and creating almost out of nothing a department not before
recognized in any institution in America.
He began his work in 1806. The science was without books—and, too, without system, except
such as its few cultivators had each for himself in his conceptions. It was the age of the first
beginnings of geology, when Wernerians and Huttonians were arrayed in a contest.... Professor
Silliman when at Edinburgh witnessed the strife, and while, as he says, his earliest predilections were
for the more peaceful mode of rock-making, these soon yielded to the accumulating evidence, and
both views became combined in his mind in one harmonious whole. The science, thus evolved, grew
with him and by him; for his own labors contributed to its extension. Every year was a year of
expansion and onward development, and the grandeur of the opening views found in him a ready and
appreciative response....
And while the sciences and truth have thus made progress here, through these labors of fifty years,
the means of study in the institution have no less increased. Instead of that half-bushel of stones,
which once went to Philadelphia for names, in a candle-box, you see above the largest mineral
cabinet in the country, which but for Professor Silliman, his attractions and his personal exertions
together, would never have been one of the glories of old Yale....
Moreover, the American Journal of Science,—now in its thirty-seventh year and seventieth volume
[1856],—projected and long-sustained solely by Professor Silliman, while ever distributing truth, has
also been ever gathering honors, and is one of the laurels of Yale.
We rejoice that in laying aside his studies, after so many years of labor, there is still no abated
vigor.... He retires as one whose right it is to throw the burden on others. Long may he be with us, to
enjoy the good he has done, and cheer us by his noble and benign presence.”
In addition to these words of Dana, much of vital interest in regard to
Silliman and his work will be gathered from what is given in the pages
immediately following, quoted from his personal statements in the early
volumes of the Journal.
Page 28
The Early Years of the Journal.
In no direction did Silliman’s enthusiastic activities in science produce a
more enduring result than in the founding and carrying on of the Journal.
The first suggestion in regard to the enterprise was made to Silliman by his
friend, Colonel George Gibbs, from whom the famous Gibbs collection of
minerals was bought by Yale College in 1825. Silliman says (25, 215,
1834):
In no direction did Silliman’s enthusiastic activities in science produce a
more enduring result than in the founding and carrying on of the Journal.
The first suggestion in regard to the enterprise was made to Silliman by his
friend, Colonel George Gibbs, from whom the famous Gibbs collection of
minerals was bought by Yale College in 1825. Silliman says (25, 215,
1834):
Page 29
“Col. Gibbs was the person who first suggested to the Editor the project of this Journal, and he
urged the topic with so much zeal and with such cogent arguments, as prevailed to induce the effort
in a case then viewed as of very dubious success. The subject was thus started in November, 1817;
proposals for the Journal were issued in January, 1818, and the first number appeared in July of that
year.”
He adds further (50, p. iii, 1847) that the conversation here recorded took
place “on an accidental meeting on board the steamboat Fulton in Long
urged the topic with so much zeal and with such cogent arguments, as prevailed to induce the effort
in a case then viewed as of very dubious success. The subject was thus started in November, 1817;
proposals for the Journal were issued in January, 1818, and the first number appeared in July of that
year.”
He adds further (50, p. iii, 1847) that the conversation here recorded took
place “on an accidental meeting on board the steamboat Fulton in Long
Page 30
Island Sound.” This was some ten years after Robert Fulton’s steamboat,
the Clermont, made its pioneer trip on the Hudson river, already alluded to.
The incident is not without significance in this connection. The deck of the
“Fulton” was not an inappropriate place for the inauguration of an
enterprise also great in its results for the country.
In the preface to the concluding volume of the First Series (loc. cit.)
Silliman adds the following remarks which show his natural modesty at the
thought of undertaking so serious a work. He says:
Although a different selection of an editor would have been much preferred, and many reasons,
public and personal, concurred to produce diffidence of success, the arguments of Col. Gibbs, whose
views on subjects of science were entitled to the most respectful consideration, and had justly great
weight, being pressed with zeal and ability, induced a reluctant assent; and accordingly, after due
consultation with many competent judges, the proposals were issued early in 1818, embracing the
whole range of physical science and its applications. The Editor in entering on the duty, regarded it as
an affair for life, and the thirty years of experience which he has now had, have proved that his views
of the exigencies of the service were not erroneous.
The plan with which the editor began his work and the lines laid down by
him at the outset can only be made clear by quoting entire the “Plan of the
Work” which opens the first number. It seems desirable also to give this in
its original form as to paragraphs and typography. The first page of the
cover of the opening number has also been reproduced here. It will be seen
that the plan of the young editor was as wide as the entire range of science
and its applications and extended out to music and the fine arts. This seems
strange to-day, but it must be remembered how few were the organs of
publication open to contributors at the time. If the plan was unreasonably
extended, that fact is to be taken not only as an expression of the
enthusiasm of the editor, as yet inexperienced in his work, but also of the
time when the sciences were still in their infancy.
He says (1, pp. v, vi):
the Clermont, made its pioneer trip on the Hudson river, already alluded to.
The incident is not without significance in this connection. The deck of the
“Fulton” was not an inappropriate place for the inauguration of an
enterprise also great in its results for the country.
In the preface to the concluding volume of the First Series (loc. cit.)
Silliman adds the following remarks which show his natural modesty at the
thought of undertaking so serious a work. He says:
Although a different selection of an editor would have been much preferred, and many reasons,
public and personal, concurred to produce diffidence of success, the arguments of Col. Gibbs, whose
views on subjects of science were entitled to the most respectful consideration, and had justly great
weight, being pressed with zeal and ability, induced a reluctant assent; and accordingly, after due
consultation with many competent judges, the proposals were issued early in 1818, embracing the
whole range of physical science and its applications. The Editor in entering on the duty, regarded it as
an affair for life, and the thirty years of experience which he has now had, have proved that his views
of the exigencies of the service were not erroneous.
The plan with which the editor began his work and the lines laid down by
him at the outset can only be made clear by quoting entire the “Plan of the
Work” which opens the first number. It seems desirable also to give this in
its original form as to paragraphs and typography. The first page of the
cover of the opening number has also been reproduced here. It will be seen
that the plan of the young editor was as wide as the entire range of science
and its applications and extended out to music and the fine arts. This seems
strange to-day, but it must be remembered how few were the organs of
publication open to contributors at the time. If the plan was unreasonably
extended, that fact is to be taken not only as an expression of the
enthusiasm of the editor, as yet inexperienced in his work, but also of the
time when the sciences were still in their infancy.
He says (1, pp. v, vi):
Page 31
“PLAN OF THE WORK.
This Journal is intended to embrace the circle of The Physical Sciences, with their application to
The Arts, and to every useful purpose.
It is designed as a deposit for original American communications; but will contain also occasional
selections from Foreign Journals, and notices of the progress of science in other countries. Within its
plan are embraced
Natural History, in its three great departments of Mineralogy, Botany, and Zoology;
Chemistry and Natural Philosophy, in their various branches: and Mathematics, pure and
mixed.
It will be a leading object to illustrate American Natural History, and especially our
Mineralogy and Geology.
The Applications of these sciences are obviously as numerous as physical arts, and physical
wants; for no one of these arts or wants can be named which is not connected with them.
While Science will be cherished for its own sake, and with a due respect for its own inherent
dignity; it will also be employed as the handmaid to the Arts. Its numerous applications to
Agriculture, the earliest and most important of them; to our Manufactures, both mechanical and
chemical; and to our Domestic Economy, will be carefully sought out, and faithfully made.
It is also within the design of this Journal to receive communications on Music, Sculpture,
Engraving, Painting, and generally on the fine and liberal, as well as useful arts;
On Military and Civil Engineering, and the art of Navigation.
This Journal is intended to embrace the circle of The Physical Sciences, with their application to
The Arts, and to every useful purpose.
It is designed as a deposit for original American communications; but will contain also occasional
selections from Foreign Journals, and notices of the progress of science in other countries. Within its
plan are embraced
Natural History, in its three great departments of Mineralogy, Botany, and Zoology;
Chemistry and Natural Philosophy, in their various branches: and Mathematics, pure and
mixed.
It will be a leading object to illustrate American Natural History, and especially our
Mineralogy and Geology.
The Applications of these sciences are obviously as numerous as physical arts, and physical
wants; for no one of these arts or wants can be named which is not connected with them.
While Science will be cherished for its own sake, and with a due respect for its own inherent
dignity; it will also be employed as the handmaid to the Arts. Its numerous applications to
Agriculture, the earliest and most important of them; to our Manufactures, both mechanical and
chemical; and to our Domestic Economy, will be carefully sought out, and faithfully made.
It is also within the design of this Journal to receive communications on Music, Sculpture,
Engraving, Painting, and generally on the fine and liberal, as well as useful arts;
On Military and Civil Engineering, and the art of Navigation.
Page 32
Notices, Reviews, and Analyses of new scientific works, and of new Inventions, and Specifications
of Patents;
Biographical and Obituary Notices of scientific men; essays on Comparative Anatomy and
Physiology, and generally on such other branches of medicine as depend on scientific principles;
Meteorological Registers, and Reports of Agricultural Experiments: and we would leave room also
for interesting miscellaneous things, not perhaps exactly included under either of the above heads.
Communications are respectfully solicited from men of science, and from men versed in the
practical arts.
Learned Societies are invited to make this Journal, occasionally, the vehicle of their
communications to the Public.
of Patents;
Biographical and Obituary Notices of scientific men; essays on Comparative Anatomy and
Physiology, and generally on such other branches of medicine as depend on scientific principles;
Meteorological Registers, and Reports of Agricultural Experiments: and we would leave room also
for interesting miscellaneous things, not perhaps exactly included under either of the above heads.
Communications are respectfully solicited from men of science, and from men versed in the
practical arts.
Learned Societies are invited to make this Journal, occasionally, the vehicle of their
communications to the Public.
Page 33
The editor will not hold himself responsible for the sentiments and opinions advanced by his
correspondents; but he will consider it as an allowed liberty to make slight verbal alterations, where
errors may be presumed to have arisen from inadvertency.”
In the “Advertisement” which precedes the above statement in the first
number, the editor remarks somewhat naïvely that he “does not pledge
himself that all the subjects shall be touched upon in every number. This is
plainly impossible unless every article should be very short and
imperfect....”
The whole subject is discussed in all its relations in the “Introductory
Remarks” which open the first volume. No apology is needed for quoting at
considerable length, for only in this way can the situation be made clear, as
seen by the editor in 1818. Further we gain here a picture of the intellectual
life of the times and, not less interesting, of the mind and personality of the
writer. With a frank kindliness, eminently characteristic of the man, as will
be seen, he takes the public fully into his confidence. In the remarks made
in subsequent volumes,—also extensively quoted—the vicissitudes in the
conduct of the enterprise are brought out and when success was no longer
doubtful, there is a tone of quiet satisfaction which was also characteristic
and which the circumstances fully justified.
The Introductory Remarks begin as follows:
The age in which we live is not less distinguished by a vigorous and successful cultivation of
physical science, than by its numerous and important applications to the practical arts, and to the
common purposes of life.
In every enlightened country, men illustrious for talent, worth and knowledge, are ardently
engaged in enlarging the boundaries of natural science; and the history of their labors and discoveries
is communicated to the world chiefly through the medium of scientific journals. The utility of such
journals has thus become generally evident; they are the heralds of science; they proclaim its toils
and its achievements; they demonstrate its intimate connection as well with the comfort, as with the
intellectual and moral improvement of our species; and they often procure for it enviable honors and
substantial rewards.
Mention is then made of the journals existing in England and France in
1818 “which have long enjoyed a high and deserved reputation.” He then
continues:
correspondents; but he will consider it as an allowed liberty to make slight verbal alterations, where
errors may be presumed to have arisen from inadvertency.”
In the “Advertisement” which precedes the above statement in the first
number, the editor remarks somewhat naïvely that he “does not pledge
himself that all the subjects shall be touched upon in every number. This is
plainly impossible unless every article should be very short and
imperfect....”
The whole subject is discussed in all its relations in the “Introductory
Remarks” which open the first volume. No apology is needed for quoting at
considerable length, for only in this way can the situation be made clear, as
seen by the editor in 1818. Further we gain here a picture of the intellectual
life of the times and, not less interesting, of the mind and personality of the
writer. With a frank kindliness, eminently characteristic of the man, as will
be seen, he takes the public fully into his confidence. In the remarks made
in subsequent volumes,—also extensively quoted—the vicissitudes in the
conduct of the enterprise are brought out and when success was no longer
doubtful, there is a tone of quiet satisfaction which was also characteristic
and which the circumstances fully justified.
The Introductory Remarks begin as follows:
The age in which we live is not less distinguished by a vigorous and successful cultivation of
physical science, than by its numerous and important applications to the practical arts, and to the
common purposes of life.
In every enlightened country, men illustrious for talent, worth and knowledge, are ardently
engaged in enlarging the boundaries of natural science; and the history of their labors and discoveries
is communicated to the world chiefly through the medium of scientific journals. The utility of such
journals has thus become generally evident; they are the heralds of science; they proclaim its toils
and its achievements; they demonstrate its intimate connection as well with the comfort, as with the
intellectual and moral improvement of our species; and they often procure for it enviable honors and
substantial rewards.
Mention is then made of the journals existing in England and France in
1818 “which have long enjoyed a high and deserved reputation.” He then
continues:
Page 34
From these sources our country reaps and will long continue to reap, an abundant harvest of
information: and if the light of science, as well as of day, springs from the East, we will welcome the
rays of both; nor should national pride induce us to reject so rich an offering.
But can we do nothing in return?
In a general diffusion of useful information through the various classes of society, in activity of
intellect and fertility of resource and invention, producing a highly intelligent population, we have no
reason to shrink from a comparison with any country. But the devoted cultivators of science in the
United States are comparatively few: they are, however, rapidly increasing in number. Among them
are persons distinguished for their capacity and attainments, and, notwithstanding the local feelings
nourished by our state sovereignties, and the rival claims of several of our larger cities, there is
evidently a predisposition towards a concentration of effort, from which we may hope for the
happiest results, with regard to the advancement of both the science and reputation of our country.
Is it not, therefore, desirable to furnish some rallying point, some object sufficiently interesting to
be nurtured by common efforts, and thus to become the basis of an enduring, common interest? To
produce these efforts, and to excite this interest, nothing, perhaps, bids fairer than a Scientific
Journal.
The valuable work already accomplished by various medical journals is
then spoken of and particularly that of the first scientific periodical in the
United States, Bruce’s Mineralogical Journal. This, as Silliman says (1, p. 3,
1818), although “both in this country and in Europe received in a very
flattering manner,” did not survive the death of its founder, and only a
single volume of 270 pages appeared (1810–1813).
Silliman continues:
No one, it is presumed, will doubt that a journal devoted to science, and embracing a sphere
sufficiently extensive to allure to its support the principal scientific men of our country, is greatly
needed; if cordially supported, it will be successful, and if successful, it will be a great public benefit.
Even a failure, in so good a cause, (unless it should arise from incapacity or unfaithfulness,) cannot
be regarded as dishonourable. It may prove only that the attempt was premature, and that our country
is not yet ripe for such an undertaking; for without the efficient support of talent, knowledge, and
money, it cannot long proceed. No editor can hope to carry forward such a work without the active
aid of scientific and practical men; but, at the same time, the public have a right to expect that he will
not be sparing of his own labour, and that his work shall be generally marked by the impress of his
own hand. To this extent the editor cheerfully acknowledges his obligations to the public; and it will
be his endeavour faithfully to redeem his pledge.
Most of the periodical works of our country have been short-lived. This, also, may perish in its
infancy; and if any degree of confidence is cherished that it will attain a maturer age, it is derived
from the obvious and intrinsic importance of the undertaking; from its being built upon permanent
and momentous national interests; from the evidence of a decided approbation of the design, on the
part of gentlemen of the first eminence, obtained in the progress of an extensive correspondence;
from assurance of support, in the way of contributions, from men of ability in many sections of the
union; and from the existence of such a crisis in the affairs of this country and of the world, as
appears peculiarly auspicious to the success of every wise and good undertaking.
information: and if the light of science, as well as of day, springs from the East, we will welcome the
rays of both; nor should national pride induce us to reject so rich an offering.
But can we do nothing in return?
In a general diffusion of useful information through the various classes of society, in activity of
intellect and fertility of resource and invention, producing a highly intelligent population, we have no
reason to shrink from a comparison with any country. But the devoted cultivators of science in the
United States are comparatively few: they are, however, rapidly increasing in number. Among them
are persons distinguished for their capacity and attainments, and, notwithstanding the local feelings
nourished by our state sovereignties, and the rival claims of several of our larger cities, there is
evidently a predisposition towards a concentration of effort, from which we may hope for the
happiest results, with regard to the advancement of both the science and reputation of our country.
Is it not, therefore, desirable to furnish some rallying point, some object sufficiently interesting to
be nurtured by common efforts, and thus to become the basis of an enduring, common interest? To
produce these efforts, and to excite this interest, nothing, perhaps, bids fairer than a Scientific
Journal.
The valuable work already accomplished by various medical journals is
then spoken of and particularly that of the first scientific periodical in the
United States, Bruce’s Mineralogical Journal. This, as Silliman says (1, p. 3,
1818), although “both in this country and in Europe received in a very
flattering manner,” did not survive the death of its founder, and only a
single volume of 270 pages appeared (1810–1813).
Silliman continues:
No one, it is presumed, will doubt that a journal devoted to science, and embracing a sphere
sufficiently extensive to allure to its support the principal scientific men of our country, is greatly
needed; if cordially supported, it will be successful, and if successful, it will be a great public benefit.
Even a failure, in so good a cause, (unless it should arise from incapacity or unfaithfulness,) cannot
be regarded as dishonourable. It may prove only that the attempt was premature, and that our country
is not yet ripe for such an undertaking; for without the efficient support of talent, knowledge, and
money, it cannot long proceed. No editor can hope to carry forward such a work without the active
aid of scientific and practical men; but, at the same time, the public have a right to expect that he will
not be sparing of his own labour, and that his work shall be generally marked by the impress of his
own hand. To this extent the editor cheerfully acknowledges his obligations to the public; and it will
be his endeavour faithfully to redeem his pledge.
Most of the periodical works of our country have been short-lived. This, also, may perish in its
infancy; and if any degree of confidence is cherished that it will attain a maturer age, it is derived
from the obvious and intrinsic importance of the undertaking; from its being built upon permanent
and momentous national interests; from the evidence of a decided approbation of the design, on the
part of gentlemen of the first eminence, obtained in the progress of an extensive correspondence;
from assurance of support, in the way of contributions, from men of ability in many sections of the
union; and from the existence of such a crisis in the affairs of this country and of the world, as
appears peculiarly auspicious to the success of every wise and good undertaking.
Page 35
An interesting discussion follows (pp. 5–8) as to the claims of the
different branches of science, and the extent to which they and their
applications had been already developed, also the spheres still open to
discovery.
The Introductory Remarks close, as follows:
In a word, the whole circle of physical science is directly applicable to human wants and
constantly holds out a light to the practical arts; it thus polishes and benefits society and everywhere
demonstrates both supreme intelligence and harmony and beneficence of design in the Creator.
The science of mathematics, both pure and mixed, can never cease to be interesting and important
to man, as long as the relations of quantity shall exist, as long as ships shall traverse the ocean, as
long as man shall measure the surface or heights of the earth on which he lives, or calculate the
distances and examine the relations of the planets and stars; and as long as the iron reign of war shall
demand the discharge of projectiles, or the construction of complicated defences.
The closing part of the paragraph shows the influence exerted upon the
mind of the editor by the serious wars of the years preceding 1818, a subject
alluded to again at the close of this chapter.
In February, 1822, with the completion of the fourth volume, the editor
reviews the situation which, though encouraging is by no means fully
assuring. He says (preface to vol. 4, dated Feb. 15, 1822):
Two years and a half have elapsed, since the publication of the first volume of this Journal, and
one year and ten months since the Editor assumed the pecuniary responsibility....
The work has not, even yet, reimbursed its expenses, (we speak not of editorial or of business
compensation,) we intend, that it has not paid for the paper, printing and engraving; the proprietors of
the first volume being in advance, on those accounts, and the Editor on the same score, with respect
to the aggregate expense of the three last volumes. This deficit is, however, no longer increasing, as
the receipts, at present, just about cover the expense of the physical materials, and of the manual
labour. A reiterated disclosure of this kind is not grateful, and would scarcely be manly, were it not
that the public, who alone have the power to remove the difficulty, have a right to a frank exposition
of the state of the case. As the patronage is, however, growing gradually more extensive, it is
believed that the work will be eventually sustained, although it may be long before it will command
any thing but gratuitous intellectual labour....
These facts, with the obvious one,—that its pages are supplied with contributions from all parts of
the Union, and occasionally from Europe, evince that the work is received as a national and not as a
local undertaking, and that the community consider it as having no sectional character. Encouraged
by this view of the subject, and by the favour of many distinguished men, both at home and abroad,
and supported by able contributors, to whom the Editor again tenders his grateful acknowledgments,
different branches of science, and the extent to which they and their
applications had been already developed, also the spheres still open to
discovery.
The Introductory Remarks close, as follows:
In a word, the whole circle of physical science is directly applicable to human wants and
constantly holds out a light to the practical arts; it thus polishes and benefits society and everywhere
demonstrates both supreme intelligence and harmony and beneficence of design in the Creator.
The science of mathematics, both pure and mixed, can never cease to be interesting and important
to man, as long as the relations of quantity shall exist, as long as ships shall traverse the ocean, as
long as man shall measure the surface or heights of the earth on which he lives, or calculate the
distances and examine the relations of the planets and stars; and as long as the iron reign of war shall
demand the discharge of projectiles, or the construction of complicated defences.
The closing part of the paragraph shows the influence exerted upon the
mind of the editor by the serious wars of the years preceding 1818, a subject
alluded to again at the close of this chapter.
In February, 1822, with the completion of the fourth volume, the editor
reviews the situation which, though encouraging is by no means fully
assuring. He says (preface to vol. 4, dated Feb. 15, 1822):
Two years and a half have elapsed, since the publication of the first volume of this Journal, and
one year and ten months since the Editor assumed the pecuniary responsibility....
The work has not, even yet, reimbursed its expenses, (we speak not of editorial or of business
compensation,) we intend, that it has not paid for the paper, printing and engraving; the proprietors of
the first volume being in advance, on those accounts, and the Editor on the same score, with respect
to the aggregate expense of the three last volumes. This deficit is, however, no longer increasing, as
the receipts, at present, just about cover the expense of the physical materials, and of the manual
labour. A reiterated disclosure of this kind is not grateful, and would scarcely be manly, were it not
that the public, who alone have the power to remove the difficulty, have a right to a frank exposition
of the state of the case. As the patronage is, however, growing gradually more extensive, it is
believed that the work will be eventually sustained, although it may be long before it will command
any thing but gratuitous intellectual labour....
These facts, with the obvious one,—that its pages are supplied with contributions from all parts of
the Union, and occasionally from Europe, evince that the work is received as a national and not as a
local undertaking, and that the community consider it as having no sectional character. Encouraged
by this view of the subject, and by the favour of many distinguished men, both at home and abroad,
and supported by able contributors, to whom the Editor again tenders his grateful acknowledgments,
Page 36
he will still persevere, in the hope of contributing something to the advancement of our science and
arts, and towards the elevation of our national character.
In the autumn of the same year, the editor closes the fifth volume with a
more confident tone (Sept. 25, 1822):
A trial of four years has decided the point, that the American Public will support this Journal. Its
pecuniary patronage is now such, that although not a lucrative, it is no longer a hazardous enterprise.
It is now also decided, that the intellectual resources of the country are sufficient to afford an
unfailing supply of valuable original communications and that nothing but perseverance and effort
are necessary to give perpetuity to the undertaking.
The decided and uniform expression of public favour which the Journal has received both at home
and abroad, affords the Editor such encouragement, that he cannot hesitate to persevere—and he now
renews the expression of his thanks to the friends and correspondents of the work, both in Europe and
the United States, requesting at the same time a continuance of their friendly influence and efforts.
Still again in the preface to the sixth volume (1823) he takes the reader
more fully into his confidence and shows that he regards the enterprise as
no longer of doubtful success. He says:
The conclusion of a new volume of a work, involving so much care, labour and responsibility, as
are necessarily attached, at the present day, to a Journal of Science and the Arts, naturally produces in
the mind, a state of not ungrateful calmness, and a disposition, partaking of social feeling, to say
something to those who honour such a production, by giving to it a small share of their money, and of
their time. The Editor’s first impression was, that the sixth volume should be sent into the world
without an introductory note, but he yields to the impulse already expressed, and to the established
usages of respectful courtesy to the public, which a short preface seems to imply. He has now
persevered almost five years, in an undertaking, regarded by many of the friends whom he originally
consulted, as hazardous, and to which not a few of them prophetically alloted only an ephemeral
existence. It has been his fortune to prosecute this work without, (till a very recent period,) returns,
adequate to its indispensable responsibilities;—under a heavy pressure of professional and private
duty; with trying fluctuations of health, and amidst severe and reiterated domestic afflictions. The
world are usually indulgent to allusions of this nature, when they have any relation to the discharge
of public duty; and in this view, it is with satisfaction, that the Editor adds, that he has now to look on
formidable difficulties, only in retrospect, and with something of the feeling of him, who sees a
powerful and vanquished foe, slowly retiring, and leaving a field no longer contested.
This Journal which, from the first, was fully supplied with original communications, is now
sustained by actual payment, to such an extent, that it may fairly be considered as an established
work; its patronage is regularly increasing, and we trust it will no longer justify such remarks as some
of the following, from the pen of one of the most eminent scientific men in Europe. “Nothing
surprises me more, than the little encouragement which your Journal,” (“which I always read with
very great interest, and of which I make great use,”) “experiences in America—this must surely arise
from the present depressed condition of trade, and cannot long continue.”
arts, and towards the elevation of our national character.
In the autumn of the same year, the editor closes the fifth volume with a
more confident tone (Sept. 25, 1822):
A trial of four years has decided the point, that the American Public will support this Journal. Its
pecuniary patronage is now such, that although not a lucrative, it is no longer a hazardous enterprise.
It is now also decided, that the intellectual resources of the country are sufficient to afford an
unfailing supply of valuable original communications and that nothing but perseverance and effort
are necessary to give perpetuity to the undertaking.
The decided and uniform expression of public favour which the Journal has received both at home
and abroad, affords the Editor such encouragement, that he cannot hesitate to persevere—and he now
renews the expression of his thanks to the friends and correspondents of the work, both in Europe and
the United States, requesting at the same time a continuance of their friendly influence and efforts.
Still again in the preface to the sixth volume (1823) he takes the reader
more fully into his confidence and shows that he regards the enterprise as
no longer of doubtful success. He says:
The conclusion of a new volume of a work, involving so much care, labour and responsibility, as
are necessarily attached, at the present day, to a Journal of Science and the Arts, naturally produces in
the mind, a state of not ungrateful calmness, and a disposition, partaking of social feeling, to say
something to those who honour such a production, by giving to it a small share of their money, and of
their time. The Editor’s first impression was, that the sixth volume should be sent into the world
without an introductory note, but he yields to the impulse already expressed, and to the established
usages of respectful courtesy to the public, which a short preface seems to imply. He has now
persevered almost five years, in an undertaking, regarded by many of the friends whom he originally
consulted, as hazardous, and to which not a few of them prophetically alloted only an ephemeral
existence. It has been his fortune to prosecute this work without, (till a very recent period,) returns,
adequate to its indispensable responsibilities;—under a heavy pressure of professional and private
duty; with trying fluctuations of health, and amidst severe and reiterated domestic afflictions. The
world are usually indulgent to allusions of this nature, when they have any relation to the discharge
of public duty; and in this view, it is with satisfaction, that the Editor adds, that he has now to look on
formidable difficulties, only in retrospect, and with something of the feeling of him, who sees a
powerful and vanquished foe, slowly retiring, and leaving a field no longer contested.
This Journal which, from the first, was fully supplied with original communications, is now
sustained by actual payment, to such an extent, that it may fairly be considered as an established
work; its patronage is regularly increasing, and we trust it will no longer justify such remarks as some
of the following, from the pen of one of the most eminent scientific men in Europe. “Nothing
surprises me more, than the little encouragement which your Journal,” (“which I always read with
very great interest, and of which I make great use,”) “experiences in America—this must surely arise
from the present depressed condition of trade, and cannot long continue.”
Page 37
Six years more of uninterrupted editorial work passed by, the sixteenth
volume was completed, and the editor was now in a position to review the
whole situation up to 1829. This preface (dated July 1, 1829), which is
quoted nearly in full, cannot fail to be found particularly interesting and
from several standpoints, not the least for the insight it gives into the
writer’s mind. It is also noteworthy that at this early date it was found
possible to pay for original contributions, a privilege far beyond the means
of the editor of to-day.
When this Journal was first projected, very few believed that it would succeed.
Among others, Dr. Dorsey wrote to the editor; “I predict a short life for you, although I wish, as
the Spaniards say, that you may live a thousand years.” The work has not lived a thousand years, but
as it has survived more than the hundredth part of that period, no reason is apparent why it may not
continue to exist. To the contributors, disinterested and arduous as have been their exertions, the
editor’s warmest thanks are due; and they are equally rendered to numerous personal friends for their
unwavering support: nor ought those subscribers to be forgotten who, occupied in the common
pursuits of life, have aided, by their money, in sustaining the hazardous novelty of an American
Journal of Science. A general approbation, sufficiently decided to encourage effort, where there was
no other reward, has supported the editor; but he has not been inattentive to the voice of criticism,
whether it has reached him in the tones of candor and kindness, or in those of severity. We must not
look to our friends for the full picture of our faults. He is unwise who neglects the maxim—
—fas est ab hoste doceri,
and we may be sure, that those are quite in earnest, whose pleasure it is, to place faults in a strong
light and bold relief; and to throw excellencies into the shadow of total eclipse. Minds at once
enlightened and amiable, viewing both in their proper proportions, will however render the equitable
verdict;
Non ego paucis offendar maculis,—
It is not pretended that this Journal has been faultless; there may be communications in it which had
been better omitted, and it is not doubted that the power to command intellectual effort, by suitable
pecuniary reward, would add to its purity, as a record of science, and to its richness, as a repository of
discoveries in the arts.
But the editor, even now, offers payment, at the rate adopted by the literary Journals, for able
original communications, containing especially important facts, investigations and discoveries in
science, and practical inventions in the useful and ornamental Arts.
As however his means are insufficient to pay for all the copy, it is earnestly requested, that those
gentlemen, who, from other motives, are still willing to write for this Journal, should continue to
favor it with their communications. That the period when satisfactory compensation can be made to
all writers whose pieces are inserted, and to whom payment will be acceptable, is not distant, may
perhaps be hoped, from the spontaneous expression of the following opinion, by the distinguished
editor of one of our principal literary journals, whose letter is now before me. “The character of the
American Journal is strictly national, and it is the only vehicle of communication in which an
inquirer may be sure to find what is most interesting in the wide range of topics, which its design
embraces. It has become in short, not more identified with the science than the literature of the
volume was completed, and the editor was now in a position to review the
whole situation up to 1829. This preface (dated July 1, 1829), which is
quoted nearly in full, cannot fail to be found particularly interesting and
from several standpoints, not the least for the insight it gives into the
writer’s mind. It is also noteworthy that at this early date it was found
possible to pay for original contributions, a privilege far beyond the means
of the editor of to-day.
When this Journal was first projected, very few believed that it would succeed.
Among others, Dr. Dorsey wrote to the editor; “I predict a short life for you, although I wish, as
the Spaniards say, that you may live a thousand years.” The work has not lived a thousand years, but
as it has survived more than the hundredth part of that period, no reason is apparent why it may not
continue to exist. To the contributors, disinterested and arduous as have been their exertions, the
editor’s warmest thanks are due; and they are equally rendered to numerous personal friends for their
unwavering support: nor ought those subscribers to be forgotten who, occupied in the common
pursuits of life, have aided, by their money, in sustaining the hazardous novelty of an American
Journal of Science. A general approbation, sufficiently decided to encourage effort, where there was
no other reward, has supported the editor; but he has not been inattentive to the voice of criticism,
whether it has reached him in the tones of candor and kindness, or in those of severity. We must not
look to our friends for the full picture of our faults. He is unwise who neglects the maxim—
—fas est ab hoste doceri,
and we may be sure, that those are quite in earnest, whose pleasure it is, to place faults in a strong
light and bold relief; and to throw excellencies into the shadow of total eclipse. Minds at once
enlightened and amiable, viewing both in their proper proportions, will however render the equitable
verdict;
Non ego paucis offendar maculis,—
It is not pretended that this Journal has been faultless; there may be communications in it which had
been better omitted, and it is not doubted that the power to command intellectual effort, by suitable
pecuniary reward, would add to its purity, as a record of science, and to its richness, as a repository of
discoveries in the arts.
But the editor, even now, offers payment, at the rate adopted by the literary Journals, for able
original communications, containing especially important facts, investigations and discoveries in
science, and practical inventions in the useful and ornamental Arts.
As however his means are insufficient to pay for all the copy, it is earnestly requested, that those
gentlemen, who, from other motives, are still willing to write for this Journal, should continue to
favor it with their communications. That the period when satisfactory compensation can be made to
all writers whose pieces are inserted, and to whom payment will be acceptable, is not distant, may
perhaps be hoped, from the spontaneous expression of the following opinion, by the distinguished
editor of one of our principal literary journals, whose letter is now before me. “The character of the
American Journal is strictly national, and it is the only vehicle of communication in which an
inquirer may be sure to find what is most interesting in the wide range of topics, which its design
embraces. It has become in short, not more identified with the science than the literature of the
Page 38
country.” It is believed that a strict examination of its contents will prove that its character has been
decidedly scientific; and the opinion is often expressed to the editor, that in common with the
journals of our Academies, it is a work of reference, indispensable to him who would examine the
progress of American science during the period which it covers. That it might not be too repulsive to
the general reader, some miscellaneous pieces have occasionally occupied its pages; but in smaller
proportion, than is common with several of the most distinguished British Journals of Science.
Still, the editor has been frequently solicited, both in public and private, to make it more
miscellaneous, that it might be more acceptable to the intelligent and well educated man, who does
not cultivate science; but he has never lost sight of his great object, which was to produce and
concentrate original American effort in science, and thus he has foregone pecuniary returns, which by
pursuing the other course, might have been rendered important. Others would not have him admit
any thing that is not strictly and technically scientific; and would make this journal for mere
professors and amateurs; especially in regard to those numerous details in natural history, which
although important to be registered, (and which, when presented, have always been recorded in the
American Journal,) can never exclusively occupy the pages of any such work without repelling the
majority of readers.
If this is true even in Great Britain it is still more so in this country; and our savants, unless they
would be, not only the exclusive admirers, but the sole purchasers of their own works, must permit a
little of the graceful drapery of general literature to flow around the cold statues of science. The
editor of this Journal, strongly inclined, both from opinion and habit, to gratify the cultivators of
science, will still do everything in his power to promote its high interests, and as he hopes in a better
manner than heretofore; but these respectable gentlemen will have the courtesy, to yield something to
the reading literary, as well as scientific public, and will not, we trust, be disgusted, if now and then
an Oasis relieves the eye, and a living stream refreshes the traveller. Not being inclined to renew the
abortive experiment, to please every body, which has been so long renowned in fable; the editor will
endeavor to pursue, the even tenor of his way; altogther inclined to be courteous and useful to his
fellow travellers, and hoping for their kindness and services in return.
decidedly scientific; and the opinion is often expressed to the editor, that in common with the
journals of our Academies, it is a work of reference, indispensable to him who would examine the
progress of American science during the period which it covers. That it might not be too repulsive to
the general reader, some miscellaneous pieces have occasionally occupied its pages; but in smaller
proportion, than is common with several of the most distinguished British Journals of Science.
Still, the editor has been frequently solicited, both in public and private, to make it more
miscellaneous, that it might be more acceptable to the intelligent and well educated man, who does
not cultivate science; but he has never lost sight of his great object, which was to produce and
concentrate original American effort in science, and thus he has foregone pecuniary returns, which by
pursuing the other course, might have been rendered important. Others would not have him admit
any thing that is not strictly and technically scientific; and would make this journal for mere
professors and amateurs; especially in regard to those numerous details in natural history, which
although important to be registered, (and which, when presented, have always been recorded in the
American Journal,) can never exclusively occupy the pages of any such work without repelling the
majority of readers.
If this is true even in Great Britain it is still more so in this country; and our savants, unless they
would be, not only the exclusive admirers, but the sole purchasers of their own works, must permit a
little of the graceful drapery of general literature to flow around the cold statues of science. The
editor of this Journal, strongly inclined, both from opinion and habit, to gratify the cultivators of
science, will still do everything in his power to promote its high interests, and as he hopes in a better
manner than heretofore; but these respectable gentlemen will have the courtesy, to yield something to
the reading literary, as well as scientific public, and will not, we trust, be disgusted, if now and then
an Oasis relieves the eye, and a living stream refreshes the traveller. Not being inclined to renew the
abortive experiment, to please every body, which has been so long renowned in fable; the editor will
endeavor to pursue, the even tenor of his way; altogther inclined to be courteous and useful to his
fellow travellers, and hoping for their kindness and services in return.
Page 39
The Close of the First Series.
The “First Series,” as it was henceforth to be known, closed with the
fiftieth volume (1847, pp. xx + 347). This final volume is devoted to an
exhaustive index to the forty-nine volumes preceding. In the preface (dated
April 19, 1847) the elder Silliman, now the senior editor, reviews the work
that had been accomplished with a frank expression of his feeling of
satisfaction in the victory won against great obstacles; with this every
reader must sympathize. He quotes here at length (but in slightly altered
form) the matter from the first volume (1818), which has been already
reproduced almost entire, and then goes on as follows (pp. xi et seq.):
The “First Series,” as it was henceforth to be known, closed with the
fiftieth volume (1847, pp. xx + 347). This final volume is devoted to an
exhaustive index to the forty-nine volumes preceding. In the preface (dated
April 19, 1847) the elder Silliman, now the senior editor, reviews the work
that had been accomplished with a frank expression of his feeling of
satisfaction in the victory won against great obstacles; with this every
reader must sympathize. He quotes here at length (but in slightly altered
form) the matter from the first volume (1818), which has been already
reproduced almost entire, and then goes on as follows (pp. xi et seq.):
Page 40
Such was the pledge which, on entering upon our editorial labors in 1818, we gave to the public,
and such were the views which we then entertained, regarding science and the arts as connected with
the interests and honor of our country and of mankind. In the retrospect, we realize a sober but
grateful feeling of satisfaction, in having, to the extent of our power, discharged these self-imposed
obligations; this feeling is chastened also by a deep sense of gratitude, first to God for life and power
continued for so high a purpose; and next, to our noble band of contributors, whose labors are
recorded in half a century of volumes, and in more than a quarter of a century of years. We need not
conceal our conviction, that the views expressed in these “Introductory Remarks,” have been fully
sustained by our fellow laborers.
and such were the views which we then entertained, regarding science and the arts as connected with
the interests and honor of our country and of mankind. In the retrospect, we realize a sober but
grateful feeling of satisfaction, in having, to the extent of our power, discharged these self-imposed
obligations; this feeling is chastened also by a deep sense of gratitude, first to God for life and power
continued for so high a purpose; and next, to our noble band of contributors, whose labors are
recorded in half a century of volumes, and in more than a quarter of a century of years. We need not
conceal our conviction, that the views expressed in these “Introductory Remarks,” have been fully
sustained by our fellow laborers.
Page 41
Should we appear to take higher ground than becomes us, we find our vindication in the fact, that
we have heralded chiefly the doings and the fame of others. The work has indeed borne throughout
“the impress” of editorial unity of design, and much that has flowed from one pen, and not a little
from the pens of others, has been without a name. The materials for the pile, have however been
selected and brought in, chiefly by other hands, and if the monument which has been reared should
prove to be “aere perennius,” the honor is not the sole property of the architect; those who have
quarried, hewn and polished the granite and the marble, are fully entitled to the enduring record of
their names already deeply cut into the massy blocks, which themselves have furnished.
If a retrospective survey of the labors of thirty years on this occasion has rekindled a degree of
enthusiasm, it is a natural result of an examination of all our volumes from the contents of which we
have endeavored to make out a summary both of the laborers and their works....
The series of volumes must ever form a work of permanent interest on account of its exhibiting the
progress of American science during the long period which it covers. Comparing 1817 with 1847, we
mark on this subject a very gratifying change. The cultivators of science in the United States were
then few—now they are numerous. Societies and associations of various names, for the cultivation of
natural history, have been instituted in very many of our cities and towns, and several of them have
been active and efficient in making original observations and forming collections.
A summary follows presenting some facts as to the growth of scientific
societies and scientific collections in this country during the period
involved: Then the striking contrast between 1818 and 1847 in the matter of
organized effort toward scientific exploration is discussed, as follows (pp.
xvi et seq.):
When we began our Journal, not one of the States had been surveyed in relation to its geology and
natural history; now those that have not been explored are few in number. State collections and a
United States Museum hold forth many allurements to the young naturalist, as well as to the
archaeologist and the student of his own race. The late Exploring Expedition [Wilkes] with the
National Institute, has enriched the capital with treasures rarely equalled in any country, and the
Smithsonian Institution recently organized at Washington, is about to begin its labors for the increase
and diffusion of knowledge among men.
It must not be forgotten that the American Association of Geologists and Naturalists—composed
of individuals assembled from widely separate portions of the Union—by the seven sessions which it
has held, and by its rich volume of reports, has produced a concentration and harmony of effort
which promise happy results, especially as, like the British Association, it visits different towns and
cities in its annual progress.
Astronomy now lifts its exploring tubes from the observatories of many of our institutions. Even
the Ohio, which within the memory of the oldest living men, rolled along its dark waters through
interminable forests, or received the stains of blood from deadly Indian warfare, now beholds on one
of its most beautiful hills, and near its splendid city, a permanent observatory with a noble telescope
sweeping the heavens, by the hand of a zealous and gifted observer. At Washington also, under the
powerful patronage of the general government, an excellent observatory has been established, and is
furnished with superior instruments, under the direction of a vigilant and well instructed astronomer
—seconded by able and zealous assistants.
we have heralded chiefly the doings and the fame of others. The work has indeed borne throughout
“the impress” of editorial unity of design, and much that has flowed from one pen, and not a little
from the pens of others, has been without a name. The materials for the pile, have however been
selected and brought in, chiefly by other hands, and if the monument which has been reared should
prove to be “aere perennius,” the honor is not the sole property of the architect; those who have
quarried, hewn and polished the granite and the marble, are fully entitled to the enduring record of
their names already deeply cut into the massy blocks, which themselves have furnished.
If a retrospective survey of the labors of thirty years on this occasion has rekindled a degree of
enthusiasm, it is a natural result of an examination of all our volumes from the contents of which we
have endeavored to make out a summary both of the laborers and their works....
The series of volumes must ever form a work of permanent interest on account of its exhibiting the
progress of American science during the long period which it covers. Comparing 1817 with 1847, we
mark on this subject a very gratifying change. The cultivators of science in the United States were
then few—now they are numerous. Societies and associations of various names, for the cultivation of
natural history, have been instituted in very many of our cities and towns, and several of them have
been active and efficient in making original observations and forming collections.
A summary follows presenting some facts as to the growth of scientific
societies and scientific collections in this country during the period
involved: Then the striking contrast between 1818 and 1847 in the matter of
organized effort toward scientific exploration is discussed, as follows (pp.
xvi et seq.):
When we began our Journal, not one of the States had been surveyed in relation to its geology and
natural history; now those that have not been explored are few in number. State collections and a
United States Museum hold forth many allurements to the young naturalist, as well as to the
archaeologist and the student of his own race. The late Exploring Expedition [Wilkes] with the
National Institute, has enriched the capital with treasures rarely equalled in any country, and the
Smithsonian Institution recently organized at Washington, is about to begin its labors for the increase
and diffusion of knowledge among men.
It must not be forgotten that the American Association of Geologists and Naturalists—composed
of individuals assembled from widely separate portions of the Union—by the seven sessions which it
has held, and by its rich volume of reports, has produced a concentration and harmony of effort
which promise happy results, especially as, like the British Association, it visits different towns and
cities in its annual progress.
Astronomy now lifts its exploring tubes from the observatories of many of our institutions. Even
the Ohio, which within the memory of the oldest living men, rolled along its dark waters through
interminable forests, or received the stains of blood from deadly Indian warfare, now beholds on one
of its most beautiful hills, and near its splendid city, a permanent observatory with a noble telescope
sweeping the heavens, by the hand of a zealous and gifted observer. At Washington also, under the
powerful patronage of the general government, an excellent observatory has been established, and is
furnished with superior instruments, under the direction of a vigilant and well instructed astronomer
—seconded by able and zealous assistants.
Page 42
Here also (in Yale College) successful observations have been made with good instruments,
although no permanent building has been erected for an Observatory.
We only give single examples by way of illustration, for the history of the progress of science in
the United States, and of institutions for its promotion, during the present generation, would demand
a volume. It is enough for our purpose that science is understood and valued, and the right methods
of prosecuting it are known, and the time is at hand when its moral and intellectual use will be as
obvious as its physical applications. Nor is it to be forgotten that we have awakened an European
interest in our researches: general science has been illustrated by treasures of facts drawn from this
country, and our discoveries are eagerly sought for and published abroad.
While with our co-workers in many parts of our broad land, we rejoice in this auspicious change,
we are far from arrogating it to ourselves. Multiplied labors of many hands have produced the great
results. In the place which we have occupied, we have persevered despite of all discouragements, and
may, with our numerous coadjutors, claim some share in the honors of the day. We do not say that our
work might not have been better done—but we may declare with truth that we have done all in our
power, and it is something to have excited many others to effort and to have chronicled their deeds in
our annals. Let those that follow us labor with like zeal and perseverance, and the good cause will
continue to advance and prosper. It is the cause of truth—science is only embodied and sympathized
truth and in the beautiful conception of our noble Agassiz—“it tells the thought of God.”
The preface closes with some personal remarks:
In tracing back the associations of many gone-by years, a host of thoughts rush in, and pensive
remembrance of the dead who have labored with us casts deep shadows into the vista through which
we view the past.
Anticipation of the hour of discharge, when our summons shall arrive, gives sobriety to thought
and checks the confidence which health and continued power to act might naturally inspire, were we
not reproved, almost every day, by the death of some co-eval, co-worker, companion, friend or
patron. This very hour is saddened by such an event,—but we will continue to labor on, and strive to
be found at our post of duty, until there is nothing more for us to do; trusting our hopes for a future
life in the hands of Him who placed us in the midst of the splendid garniture of this lower world, and
who has made not less ample provision for another and a better.
Editorial and financial.—The editorial labors on the Journal were carried
by the elder Silliman alone for twenty years from 1818 to 1838. As has been
clearly shown in his statements, already quoted, he was, after the first
beginning, personally responsible also for the financial side of the
enterprise. With volume 34 (1838) the name of Benjamin Silliman, Jr., is
added as co-editor on the title page. He was graduated from Yale College
the year preceding and at this date was only twenty-one years old. His aid
was unquestionably of much service from the beginning and increased
rapidly with years and experience. The elder Silliman introduces him in the
although no permanent building has been erected for an Observatory.
We only give single examples by way of illustration, for the history of the progress of science in
the United States, and of institutions for its promotion, during the present generation, would demand
a volume. It is enough for our purpose that science is understood and valued, and the right methods
of prosecuting it are known, and the time is at hand when its moral and intellectual use will be as
obvious as its physical applications. Nor is it to be forgotten that we have awakened an European
interest in our researches: general science has been illustrated by treasures of facts drawn from this
country, and our discoveries are eagerly sought for and published abroad.
While with our co-workers in many parts of our broad land, we rejoice in this auspicious change,
we are far from arrogating it to ourselves. Multiplied labors of many hands have produced the great
results. In the place which we have occupied, we have persevered despite of all discouragements, and
may, with our numerous coadjutors, claim some share in the honors of the day. We do not say that our
work might not have been better done—but we may declare with truth that we have done all in our
power, and it is something to have excited many others to effort and to have chronicled their deeds in
our annals. Let those that follow us labor with like zeal and perseverance, and the good cause will
continue to advance and prosper. It is the cause of truth—science is only embodied and sympathized
truth and in the beautiful conception of our noble Agassiz—“it tells the thought of God.”
The preface closes with some personal remarks:
In tracing back the associations of many gone-by years, a host of thoughts rush in, and pensive
remembrance of the dead who have labored with us casts deep shadows into the vista through which
we view the past.
Anticipation of the hour of discharge, when our summons shall arrive, gives sobriety to thought
and checks the confidence which health and continued power to act might naturally inspire, were we
not reproved, almost every day, by the death of some co-eval, co-worker, companion, friend or
patron. This very hour is saddened by such an event,—but we will continue to labor on, and strive to
be found at our post of duty, until there is nothing more for us to do; trusting our hopes for a future
life in the hands of Him who placed us in the midst of the splendid garniture of this lower world, and
who has made not less ample provision for another and a better.
Editorial and financial.—The editorial labors on the Journal were carried
by the elder Silliman alone for twenty years from 1818 to 1838. As has been
clearly shown in his statements, already quoted, he was, after the first
beginning, personally responsible also for the financial side of the
enterprise. With volume 34 (1838) the name of Benjamin Silliman, Jr., is
added as co-editor on the title page. He was graduated from Yale College
the year preceding and at this date was only twenty-one years old. His aid
was unquestionably of much service from the beginning and increased
rapidly with years and experience. The elder Silliman introduces him in the
Page 43
preface to vol. 34 (1838) and comes back to the subject again in the preface
to vol. 50 (1847). The whole editorial situation is here presented as follows:
“During twenty years from the inception of this Journal, the editor labored alone, although
overtures for editorial cooperation had been made to him by gentlemen commanding his confidence
and esteem, and who would personally have been very acceptable. It was, however, his opinion that
the unity of purpose and action so essential to the success of such a work were best secured by
individuality; but he made every effort, and not without success, to conciliate the good will and to
secure the assistance of gentlemen eminent in particular departments of knowledge. On the title page
of No. 1, vol. 34, published in July, 1838, a new name is introduced: the individual to whom it
belongs having been for several years more or less concerned in the management of the Journal, and
from his education, position, pursuits and taste, as well as from affinity, being almost identified with
the editor, he seemed to be quite a natural ally, and his adoption into the editorship was scarcely a
violation of individual unity. His assistance has proved to be very important:—his near relation to the
senior editor prevents him from saying more, while justice does not permit him to say less.”
As is distinctly intimated in the preceding paragraph the elder Silliman
was fortunate in obtaining the assistance in his editorial labors of numerous
gentlemen interested in the enterprise. Their cooperation provided many of
the scientific notices, book reviews and the like contained in the Miscellany
with which each number closed. It is impossible, at this date, to render the
credit due to Silliman’s helpers or even to mention them by name. Very
early Asa Gray was one of these as occasional notes are signed by his
initials. Dr. Levi Ives of New Haven was another. Prof. J. Griscom of Paris
also sent numerous contributions even as early as 1825 (see 9, 154, 1825;
22, 192, 1832; 24, 342, 1833, and others).
Some statements have already been quoted from the early volumes as to
the business part of Silliman’s enterprise. The subject is taken up more fully
in the preface to volume 50 (1847). No one can fail to marvel at the energy
and optimism required to push the Journal forward when conditions must
have been so difficult and encouragement so scanty. He says (pp. iii, iv):
This Journal first appeared in July, 1818, and in June, 1819, the first volume of four numbers and
448 pages was completed. This scale of publication, originally deemed sufficient, was found
inadequate to receive all the communications, and as the receipts proved insufficient to sustain the
expenses, the work, having but three hundred and fifty subscribers, was, at the end of the year,
abandoned by the publishers.
An unprofitable enterprise not being attractive to the trade, ten months elapsed before another
arrangement could be carried into effect, and, therefore, No. 1 of vol. 2 was not published until April,
1820. The new arrangement was one of mutual responsibility for the expenses, but the Editor was
constrained nevertheless to pledge his own personal credit to obtain from a bank the funds necessary
to vol. 50 (1847). The whole editorial situation is here presented as follows:
“During twenty years from the inception of this Journal, the editor labored alone, although
overtures for editorial cooperation had been made to him by gentlemen commanding his confidence
and esteem, and who would personally have been very acceptable. It was, however, his opinion that
the unity of purpose and action so essential to the success of such a work were best secured by
individuality; but he made every effort, and not without success, to conciliate the good will and to
secure the assistance of gentlemen eminent in particular departments of knowledge. On the title page
of No. 1, vol. 34, published in July, 1838, a new name is introduced: the individual to whom it
belongs having been for several years more or less concerned in the management of the Journal, and
from his education, position, pursuits and taste, as well as from affinity, being almost identified with
the editor, he seemed to be quite a natural ally, and his adoption into the editorship was scarcely a
violation of individual unity. His assistance has proved to be very important:—his near relation to the
senior editor prevents him from saying more, while justice does not permit him to say less.”
As is distinctly intimated in the preceding paragraph the elder Silliman
was fortunate in obtaining the assistance in his editorial labors of numerous
gentlemen interested in the enterprise. Their cooperation provided many of
the scientific notices, book reviews and the like contained in the Miscellany
with which each number closed. It is impossible, at this date, to render the
credit due to Silliman’s helpers or even to mention them by name. Very
early Asa Gray was one of these as occasional notes are signed by his
initials. Dr. Levi Ives of New Haven was another. Prof. J. Griscom of Paris
also sent numerous contributions even as early as 1825 (see 9, 154, 1825;
22, 192, 1832; 24, 342, 1833, and others).
Some statements have already been quoted from the early volumes as to
the business part of Silliman’s enterprise. The subject is taken up more fully
in the preface to volume 50 (1847). No one can fail to marvel at the energy
and optimism required to push the Journal forward when conditions must
have been so difficult and encouragement so scanty. He says (pp. iii, iv):
This Journal first appeared in July, 1818, and in June, 1819, the first volume of four numbers and
448 pages was completed. This scale of publication, originally deemed sufficient, was found
inadequate to receive all the communications, and as the receipts proved insufficient to sustain the
expenses, the work, having but three hundred and fifty subscribers, was, at the end of the year,
abandoned by the publishers.
An unprofitable enterprise not being attractive to the trade, ten months elapsed before another
arrangement could be carried into effect, and, therefore, No. 1 of vol. 2 was not published until April,
1820. The new arrangement was one of mutual responsibility for the expenses, but the Editor was
constrained nevertheless to pledge his own personal credit to obtain from a bank the funds necessary
Page 44
to begin again, and from this responsibility he was, for a series of years, seldom released. The single
volume per annum being found insufficient for the communications, two volumes a year were
afterward published, commencing with the second volume.
The publishers whose names appear on the title page of the four numbers
of the first volume are “J. Eastburn & Co., Literary Rooms, Broadway, New
York” and “Howe & Spalding, New Haven.” For the second volume and
those immediately following the corresponding statement “printed and
published by S. Converse [New Haven] for the Editor.”
Silliman adds (p. iv):
At the conclusion of vol. 10, in February, 1826, the work was again left upon the hands of its
Editor; all its receipts had been absorbed by the expenses, and it became necessary now to pay a
heavy sum to the retiring publisher, as an equivalent for his copies of previous volumes, as it was
deemed necessary either to control the work entirely or to abandon it. The Editor was not willing to
think of the latter, especially as he was encouraged by public approbation, and was cheered onward
in his labors by eminent men both at home and abroad, and he saw distinctly that the Journal was
rendering service not only to science and the arts, but to the reputation of his country. He reflected,
moreover, that in almost every valuable enterprise perseverance in effort is necessary to success. He
being now sole proprietor, a new arrangement was made for a single year, the publishers being at
liberty, at the end of that time, to retire, and the Editor to resume the Journal should he prefer that
course.
The latter alternative he adopted, taking upon himself the entire concern, including both the
business and the editorial duties, and of course, all the correspondence and accounts. From that time
the work has proceeded without interruption, two volumes per annum having been published for the
last twenty years; and its pecuniary claims ceased to be onerous, although its means have never been
large....
Later in the same preface he adds (p. xiv):
It may be interesting to our readers to know something of the patronage of the Journal. It has never
reached one thousand paying subscribers, and has rarely exceeded seven or eight hundred—for many
years it fluctuated between six and seven hundred.
It has been far from paying a reasonable editorial compensation; often it has paid nothing, and at
present it does little more than pay its bills. The number of engravings and the extra labor in printer’s
composition, cause it to be an expensive work, while its patronage is limited.
It is difficult at this date to give any adequate statement of the amount of
encouragement and active assistance given to Silliman by his scientific
colleagues in New Haven and elsewhere—a subject earlier alluded to. It is
volume per annum being found insufficient for the communications, two volumes a year were
afterward published, commencing with the second volume.
The publishers whose names appear on the title page of the four numbers
of the first volume are “J. Eastburn & Co., Literary Rooms, Broadway, New
York” and “Howe & Spalding, New Haven.” For the second volume and
those immediately following the corresponding statement “printed and
published by S. Converse [New Haven] for the Editor.”
Silliman adds (p. iv):
At the conclusion of vol. 10, in February, 1826, the work was again left upon the hands of its
Editor; all its receipts had been absorbed by the expenses, and it became necessary now to pay a
heavy sum to the retiring publisher, as an equivalent for his copies of previous volumes, as it was
deemed necessary either to control the work entirely or to abandon it. The Editor was not willing to
think of the latter, especially as he was encouraged by public approbation, and was cheered onward
in his labors by eminent men both at home and abroad, and he saw distinctly that the Journal was
rendering service not only to science and the arts, but to the reputation of his country. He reflected,
moreover, that in almost every valuable enterprise perseverance in effort is necessary to success. He
being now sole proprietor, a new arrangement was made for a single year, the publishers being at
liberty, at the end of that time, to retire, and the Editor to resume the Journal should he prefer that
course.
The latter alternative he adopted, taking upon himself the entire concern, including both the
business and the editorial duties, and of course, all the correspondence and accounts. From that time
the work has proceeded without interruption, two volumes per annum having been published for the
last twenty years; and its pecuniary claims ceased to be onerous, although its means have never been
large....
Later in the same preface he adds (p. xiv):
It may be interesting to our readers to know something of the patronage of the Journal. It has never
reached one thousand paying subscribers, and has rarely exceeded seven or eight hundred—for many
years it fluctuated between six and seven hundred.
It has been far from paying a reasonable editorial compensation; often it has paid nothing, and at
present it does little more than pay its bills. The number of engravings and the extra labor in printer’s
composition, cause it to be an expensive work, while its patronage is limited.
It is difficult at this date to give any adequate statement of the amount of
encouragement and active assistance given to Silliman by his scientific
colleagues in New Haven and elsewhere—a subject earlier alluded to. It is
Page 45
fortunately possible, however, to acknowledge the generous aid received by
the Journal in the early days from a source near at hand. It has already been
noted in another place that the dawning activity of science at New Haven
was recognized by the founding of the “Connecticut Academy of Arts and
Sciences,” formally established at New Haven in 1799 and the third
scientific body to be organized in this country. From the beginning of the
Journal in 1818, the Connecticut Academy freely gave its support both in
papers for publication and at least on one occasion later it gave important
financial aid. Upon the occasion of the celebration of the centennial
anniversary of the Academy on October 11, 1899, Professor, later Governor,
Baldwin, the president of the Academy, discusses this subject in some
detail. He says in part:
To support his [Silliman’s] undertaking, a vote had been passed in February [1818], “that the
Committee of Publication may allow such of the Academy’s papers as they think proper, to be
published in Mr. Silliman’s Scientific Journal.”
Free use was made of this authority, and a large part of the contents of the Journal was for many
years drawn from this source. In some cases this fact was noted in publication;[2] but in most it was
not....
In 1826, when the Journal was in great need of financial support, the Academy further voted to pay
for a year the cost of printing such of its papers as might be published in it. In Baldwin’s Annals of
Yale College, published in 1831, it is described as a publication “honorable to the science of our
common country,” and having “an additional value as being adopted as the acknowledged organ of
the Connecticut Academy of Arts and Sciences.”
Many active campaigns were carried on over the country through paid
agents to obtain new subscribers for the Journal and it was doubtless due to
these efforts that the nominal subscription list was, at times, as already
noted, relatively large as compared with that of a later date. The new
subscribers in many cases, however, did not remain permanently interested,
often failed to pay their bills, and the uncertain and varying demand upon
the supply of printed copies was doubtless one reason why many single
numbers became early out of print.
An interesting sidelight is thrown upon the efforts of Silliman to interest
the public in his work, at its beginning, by a letter to the editor from
Thomas Jefferson, then seventy-five years of age. The writer is indebted to
Mr. Robert B. Adam of Buffalo for a copy of this letter and its interest
justifies its being reproduced here entire. The letter is as follows:
the Journal in the early days from a source near at hand. It has already been
noted in another place that the dawning activity of science at New Haven
was recognized by the founding of the “Connecticut Academy of Arts and
Sciences,” formally established at New Haven in 1799 and the third
scientific body to be organized in this country. From the beginning of the
Journal in 1818, the Connecticut Academy freely gave its support both in
papers for publication and at least on one occasion later it gave important
financial aid. Upon the occasion of the celebration of the centennial
anniversary of the Academy on October 11, 1899, Professor, later Governor,
Baldwin, the president of the Academy, discusses this subject in some
detail. He says in part:
To support his [Silliman’s] undertaking, a vote had been passed in February [1818], “that the
Committee of Publication may allow such of the Academy’s papers as they think proper, to be
published in Mr. Silliman’s Scientific Journal.”
Free use was made of this authority, and a large part of the contents of the Journal was for many
years drawn from this source. In some cases this fact was noted in publication;[2] but in most it was
not....
In 1826, when the Journal was in great need of financial support, the Academy further voted to pay
for a year the cost of printing such of its papers as might be published in it. In Baldwin’s Annals of
Yale College, published in 1831, it is described as a publication “honorable to the science of our
common country,” and having “an additional value as being adopted as the acknowledged organ of
the Connecticut Academy of Arts and Sciences.”
Many active campaigns were carried on over the country through paid
agents to obtain new subscribers for the Journal and it was doubtless due to
these efforts that the nominal subscription list was, at times, as already
noted, relatively large as compared with that of a later date. The new
subscribers in many cases, however, did not remain permanently interested,
often failed to pay their bills, and the uncertain and varying demand upon
the supply of printed copies was doubtless one reason why many single
numbers became early out of print.
An interesting sidelight is thrown upon the efforts of Silliman to interest
the public in his work, at its beginning, by a letter to the editor from
Thomas Jefferson, then seventy-five years of age. The writer is indebted to
Mr. Robert B. Adam of Buffalo for a copy of this letter and its interest
justifies its being reproduced here entire. The letter is as follows:
Page 46
Monticello, Apr. 11. ’18.
Sir
The unlucky displacement of your letter of Mar 3 has been the cause of delay in my answer. altho’
I have very generally withdrawn from subscribing to or reading periodical publications from the love
of rest which age produces, yet I willingly subscribe to the journal you propose from a confidence
that the talent with which it will be edited will entitle it to attention among the things of select
reading for which alone I have time now left. be so good as to send it by mail, and the receipt of the
1st number will be considered as announcing that the work is commenced and the subscription
money for a year shall be forwarded. Accept the assurance of my great esteem and respect.
Th. Jefferson
Professor Silliman.
Contributors.—An interesting summary is also given by Silliman of the
contributors to the Journal and the extent of their work (vol. 50, pp. xii,
xiii); he says:
We find that there have been about 600 contributors of original matter to the Journal, and we have
the unexpected satisfaction of believing that probably five-sixths of them are still living; for we are
not certain that more than fifty are among the dead; of perhaps fifty more we are without information,
and if that additional number is to be enrolled among the “stelligeri,” we have still 500 remaining.
Among them are not a few of the veterans with whom we began our career, and several of these are
still active contributors. Shall we then conclude that the peaceful pursuits of knowledge are favorable
to long life? This we think is, cœteris paribus, certainly true: but in the present instance, another
reason can be assigned for the large amount of survivorship. As the Journal has advanced and death
has removed its scientific contributors, younger men and men still younger, have recruited the ranks,
and volunteers have enlisted in numbers constantly increasing, so that the flower of the host are now
in the morning and meridian of life.
We have been constantly advancing, like a traveller from the equinoctial towards the colder zones,
—as we have increased our latitude, stars have set and new stars have risen, while a few planetary
orbs visible in every zone, have continued to cheer us on our course.
The number of articles, almost exclusively original, contained in the Journal is about 1800, and the
Index will show how many have been contributed by each individual; we have doubtless included in
this number some few articles republished from foreign Journals—but we think they are even more
than counterbalanced by original communications without a name and by editorial articles, both of
which have been generally omitted in the enumeration.
Of smaller articles and notices in the Miscellany, we have not made any enumeration, but they
evidently are more numerous than the regular articles, and we presume that they may amount to at
least 2500.
Of party, either in politics or religion, there is no trace in our work; of personalities there are none,
except those that relate to priority of claims or other rights of individuals. Of these vindications the
number is not great, and we could heartily have wished that there had been no occasion for any.
Sir
The unlucky displacement of your letter of Mar 3 has been the cause of delay in my answer. altho’
I have very generally withdrawn from subscribing to or reading periodical publications from the love
of rest which age produces, yet I willingly subscribe to the journal you propose from a confidence
that the talent with which it will be edited will entitle it to attention among the things of select
reading for which alone I have time now left. be so good as to send it by mail, and the receipt of the
1st number will be considered as announcing that the work is commenced and the subscription
money for a year shall be forwarded. Accept the assurance of my great esteem and respect.
Th. Jefferson
Professor Silliman.
Contributors.—An interesting summary is also given by Silliman of the
contributors to the Journal and the extent of their work (vol. 50, pp. xii,
xiii); he says:
We find that there have been about 600 contributors of original matter to the Journal, and we have
the unexpected satisfaction of believing that probably five-sixths of them are still living; for we are
not certain that more than fifty are among the dead; of perhaps fifty more we are without information,
and if that additional number is to be enrolled among the “stelligeri,” we have still 500 remaining.
Among them are not a few of the veterans with whom we began our career, and several of these are
still active contributors. Shall we then conclude that the peaceful pursuits of knowledge are favorable
to long life? This we think is, cœteris paribus, certainly true: but in the present instance, another
reason can be assigned for the large amount of survivorship. As the Journal has advanced and death
has removed its scientific contributors, younger men and men still younger, have recruited the ranks,
and volunteers have enlisted in numbers constantly increasing, so that the flower of the host are now
in the morning and meridian of life.
We have been constantly advancing, like a traveller from the equinoctial towards the colder zones,
—as we have increased our latitude, stars have set and new stars have risen, while a few planetary
orbs visible in every zone, have continued to cheer us on our course.
The number of articles, almost exclusively original, contained in the Journal is about 1800, and the
Index will show how many have been contributed by each individual; we have doubtless included in
this number some few articles republished from foreign Journals—but we think they are even more
than counterbalanced by original communications without a name and by editorial articles, both of
which have been generally omitted in the enumeration.
Of smaller articles and notices in the Miscellany, we have not made any enumeration, but they
evidently are more numerous than the regular articles, and we presume that they may amount to at
least 2500.
Of party, either in politics or religion, there is no trace in our work; of personalities there are none,
except those that relate to priority of claims or other rights of individuals. Of these vindications the
number is not great, and we could heartily have wished that there had been no occasion for any.
Page 47
General Scope of Articles.—Many references will be found in the
chapters following which throw light upon the character and scope of the
papers published in the Journal, particularly in its early years; a few
additional statements here may, however, prove of interest.
One feature that is especially noticeable is the frequent publication of
articles planned to place before the readers of the Journal in full detail
subjects to which they might not otherwise have access. These are
sometimes translations; sometimes republications of articles that had
already appeared in English periodicals; again, they are exhaustive and
critical reviews of important memoirs or books. The value of this feature in
the early history of the Journal, when the distribution of scientific literature
had nothing of the thoroughness characteristic of recent years, is
sufficiently obvious.
It is also interesting to note the long articles of geological description and
others giving lists of mineral or botanical localities. Noteworthy, too, is the
attempt to keep abreast of occurring phenomena as in the many notes on
tornadoes and storms by Redfield, Loomis, etc.; on auroras at different
localities; on shooting stars by Herrick, Olmstead and others.
The wide range of topics treated of is quite in accordance with the plan of
the editor as given on an earlier page. Some notes, taken more or less at
random, may serve to illustrate this point. An extended and quite technical
discussion of “Musical Temperament” opens the first number (1, pp. 9–35)
and is concluded in the same volume (pp. 176–199). An article on
“Mystery” is given by Mark Hopkins, A.M., “late a tutor of Williams
College” (13, 217, 1828). There is an essay on “Gypsies” by J. Griscom
(from the Revue Encyclopédique) in volume 24 (pp. 342–345, 1833), while
some notes on American gypsies are added in vol. 26 (p. 189, 1834). The
“divining rod” is described at length in vol. 11 (pp. 201–212, 1826), but
without giving any comfort to the credulous; on the contrary the last
paragraph states that “the pretensions of diviners are worthless, etc.” A long
article by J. Finch on the forts of Boston harbour appeared in 1824 (8, 338–
348); the concluding paragraph seems worthy of quotation:
“Many centuries hence, if despotism without, or anarchy within, should cause the republican
institutions of America to fade, then these fortresses ought to be destroyed, because they would be a
constant reproach to the people; but until that period, they should be preserved as the noblest
monuments of liberty.”
chapters following which throw light upon the character and scope of the
papers published in the Journal, particularly in its early years; a few
additional statements here may, however, prove of interest.
One feature that is especially noticeable is the frequent publication of
articles planned to place before the readers of the Journal in full detail
subjects to which they might not otherwise have access. These are
sometimes translations; sometimes republications of articles that had
already appeared in English periodicals; again, they are exhaustive and
critical reviews of important memoirs or books. The value of this feature in
the early history of the Journal, when the distribution of scientific literature
had nothing of the thoroughness characteristic of recent years, is
sufficiently obvious.
It is also interesting to note the long articles of geological description and
others giving lists of mineral or botanical localities. Noteworthy, too, is the
attempt to keep abreast of occurring phenomena as in the many notes on
tornadoes and storms by Redfield, Loomis, etc.; on auroras at different
localities; on shooting stars by Herrick, Olmstead and others.
The wide range of topics treated of is quite in accordance with the plan of
the editor as given on an earlier page. Some notes, taken more or less at
random, may serve to illustrate this point. An extended and quite technical
discussion of “Musical Temperament” opens the first number (1, pp. 9–35)
and is concluded in the same volume (pp. 176–199). An article on
“Mystery” is given by Mark Hopkins, A.M., “late a tutor of Williams
College” (13, 217, 1828). There is an essay on “Gypsies” by J. Griscom
(from the Revue Encyclopédique) in volume 24 (pp. 342–345, 1833), while
some notes on American gypsies are added in vol. 26 (p. 189, 1834). The
“divining rod” is described at length in vol. 11 (pp. 201–212, 1826), but
without giving any comfort to the credulous; on the contrary the last
paragraph states that “the pretensions of diviners are worthless, etc.” A long
article by J. Finch on the forts of Boston harbour appeared in 1824 (8, 338–
348); the concluding paragraph seems worthy of quotation:
“Many centuries hence, if despotism without, or anarchy within, should cause the republican
institutions of America to fade, then these fortresses ought to be destroyed, because they would be a
constant reproach to the people; but until that period, they should be preserved as the noblest
monuments of liberty.”
Page 48
The promise to include the fine arts is kept by the publication of various
papers, as of the Trumbull paintings (16, 163, 1829); also by a series of
articles on “architecture in the United States” (17, 99, 1830; 18, 218, 220,
1830) and others. Quite in another line is the paper by J. W. Gibbs (33, 324,
1838) on “Arabic words in English.” A number of related linguistic papers
by the same author are to be found in other volumes. Papers in pure
mathematics are also not infrequent, though now not considered as falling
within the field of the Journal.
Applied science takes a prominent place through all the volume of the
First Series. An interesting paper is that on Eli Whitney, containing an
account of the cotton gin; this is accompanied by an excellent portrait (21,
201–264, 1832). The steam engine and its application are repeatedly
discussed and in the early volumes brief accounts are given of the early
steamboats in use; for example, between Stockholm and St. Petersburg (2,
347, 1820); Trieste and Venice (4, 377, 1822); on the Swiss Lakes (6, 385,
1823). The voyage of the first Atlantic steamboat, the “Savannah,” which
crossed from Savannah to Liverpool in 1819, is described (38, 155, 1840);
mention is also made of the “first iron boat” (3, 371, 1821; 5, 396, 1822). A
number of interesting letters on “Steam Navigation” are given in vol. 35,
160, 162, 332, 333, 336; some of the suggestions seem very quaint, viewed
in the light of the experience of to-day.
A very early form of explosive engine is described at length by Samuel
Morey (11, 104, 1826); this is an article that deserves mention in these days
of gasolene motors. Even more interesting is the description by Charles
Griswold (2, 94, 1820) of the first submarine invented by David Bushnell
and used in the Revolutionary War in August, 1776. An account is also
given of a dirigible balloon that may be fairly regarded as the original
ancestor of the Zeppelin (see 11, 346, 1826). The whole subject of aërial
navigation is treated at length by H. Strait (25, pp. 25, 26, 1834) and the
expression of his hopes for the future deserve quotation:
“Conveyance by air can be easily rendered as safe as by water or land, and more cheap and speedy,
while the universal and uniform diffusion of the air over every portion of the earth, will render aërial
navigation preferable to any other. To carry it into effect, there needs only an immediate appeal on a
sufficiently large scale, to experiment; reason has done her part, when experiment does hers, nature
will not refuse to sanction the whole. Aërial navigation will present the works of nature in all their
charms; to commerce and the diffusion of knowledge, it will bring the most efficient aid, and it can
thus be rendered serviceable to the whole human family.”
papers, as of the Trumbull paintings (16, 163, 1829); also by a series of
articles on “architecture in the United States” (17, 99, 1830; 18, 218, 220,
1830) and others. Quite in another line is the paper by J. W. Gibbs (33, 324,
1838) on “Arabic words in English.” A number of related linguistic papers
by the same author are to be found in other volumes. Papers in pure
mathematics are also not infrequent, though now not considered as falling
within the field of the Journal.
Applied science takes a prominent place through all the volume of the
First Series. An interesting paper is that on Eli Whitney, containing an
account of the cotton gin; this is accompanied by an excellent portrait (21,
201–264, 1832). The steam engine and its application are repeatedly
discussed and in the early volumes brief accounts are given of the early
steamboats in use; for example, between Stockholm and St. Petersburg (2,
347, 1820); Trieste and Venice (4, 377, 1822); on the Swiss Lakes (6, 385,
1823). The voyage of the first Atlantic steamboat, the “Savannah,” which
crossed from Savannah to Liverpool in 1819, is described (38, 155, 1840);
mention is also made of the “first iron boat” (3, 371, 1821; 5, 396, 1822). A
number of interesting letters on “Steam Navigation” are given in vol. 35,
160, 162, 332, 333, 336; some of the suggestions seem very quaint, viewed
in the light of the experience of to-day.
A very early form of explosive engine is described at length by Samuel
Morey (11, 104, 1826); this is an article that deserves mention in these days
of gasolene motors. Even more interesting is the description by Charles
Griswold (2, 94, 1820) of the first submarine invented by David Bushnell
and used in the Revolutionary War in August, 1776. An account is also
given of a dirigible balloon that may be fairly regarded as the original
ancestor of the Zeppelin (see 11, 346, 1826). The whole subject of aërial
navigation is treated at length by H. Strait (25, pp. 25, 26, 1834) and the
expression of his hopes for the future deserve quotation:
“Conveyance by air can be easily rendered as safe as by water or land, and more cheap and speedy,
while the universal and uniform diffusion of the air over every portion of the earth, will render aërial
navigation preferable to any other. To carry it into effect, there needs only an immediate appeal on a
sufficiently large scale, to experiment; reason has done her part, when experiment does hers, nature
will not refuse to sanction the whole. Aërial navigation will present the works of nature in all their
charms; to commerce and the diffusion of knowledge, it will bring the most efficient aid, and it can
thus be rendered serviceable to the whole human family.”
Page 49
A subject of quite another character is the first discussion of the
properties of chloroform (chloric ether) and its use as an anæsthetic
(Guthrie, 21, 64, 405, 1832; 22, 105, 1832; Levi Ives, 21, 406). Further
interesting communications are given of the first analyses of the gastric
juice and the part played by it in the process of digestion. Dr. William
Beaumont of St. Louis took advantage of a patient who through a gun-shot
wound was left with a permanent opening into his stomach through which
the gastric juice could be drawn off. The results of Dr. Beaumont and of
Professor Robley Dunglison, to whom samples were submitted, are given in
full in the life of Beaumont by Jesse S. Myer (St. Louis, 1912). The interest
of the matter, so far as the Journal is concerned, is chiefly because Dr.
Beaumont selected Professor Silliman as a chemist to whom samples for
examination were also submitted. An account of Silliman’s results is given
in the Beaumont volume referred to (see also 26, 193, 1834). Desiring the
support of a chemist of wider experience in organic analysis, he also sent a
sample through the Swedish consul to Berzelius in Stockholm. After some
months the sample was received and it is interesting to note in a perfectly
fresh condition; it is to be regretted, however, that the Swedish chemist
failed to add anything to the results already obtained in this country (27,
40b, 1835).
The above list, which might be greatly extended, seems to leave little
ground for the implied criticism replied to by Silliman as follows (16, p. v,
1829):
A celebrated scholar, while himself an editor, advised me, in a letter, to introduce into this Journal
as much “readable” matter as possible: and there was, pretty early, an earnest but respectful
recommendation in a Philadelphia paper, that Literature, in imitation of the London Quarterly Journal
of Science, &c. should be in form, inscribed among the titles of the work.
properties of chloroform (chloric ether) and its use as an anæsthetic
(Guthrie, 21, 64, 405, 1832; 22, 105, 1832; Levi Ives, 21, 406). Further
interesting communications are given of the first analyses of the gastric
juice and the part played by it in the process of digestion. Dr. William
Beaumont of St. Louis took advantage of a patient who through a gun-shot
wound was left with a permanent opening into his stomach through which
the gastric juice could be drawn off. The results of Dr. Beaumont and of
Professor Robley Dunglison, to whom samples were submitted, are given in
full in the life of Beaumont by Jesse S. Myer (St. Louis, 1912). The interest
of the matter, so far as the Journal is concerned, is chiefly because Dr.
Beaumont selected Professor Silliman as a chemist to whom samples for
examination were also submitted. An account of Silliman’s results is given
in the Beaumont volume referred to (see also 26, 193, 1834). Desiring the
support of a chemist of wider experience in organic analysis, he also sent a
sample through the Swedish consul to Berzelius in Stockholm. After some
months the sample was received and it is interesting to note in a perfectly
fresh condition; it is to be regretted, however, that the Swedish chemist
failed to add anything to the results already obtained in this country (27,
40b, 1835).
The above list, which might be greatly extended, seems to leave little
ground for the implied criticism replied to by Silliman as follows (16, p. v,
1829):
A celebrated scholar, while himself an editor, advised me, in a letter, to introduce into this Journal
as much “readable” matter as possible: and there was, pretty early, an earnest but respectful
recommendation in a Philadelphia paper, that Literature, in imitation of the London Quarterly Journal
of Science, &c. should be in form, inscribed among the titles of the work.
Page 50
The Second, Third and Fourth Series.
The Second Series of the Journal, as already stated, began with January,
1846. Up to this time the publication had been a quarterly or two volumes
annually of two numbers each. From 1846 until the completion of an
additional fifty volumes in 1871, the Journal was made a bimonthly, each of
the two yearly volumes having three numbers each. Furthermore, a general
index was given for each period of five years, that is for every ten volumes.
The Second Series of the Journal, as already stated, began with January,
1846. Up to this time the publication had been a quarterly or two volumes
annually of two numbers each. From 1846 until the completion of an
additional fifty volumes in 1871, the Journal was made a bimonthly, each of
the two yearly volumes having three numbers each. Furthermore, a general
index was given for each period of five years, that is for every ten volumes.
Page 51
Much more important than this change was the addition to the editorial
staff of James Dwight Dana, Silliman’s son-in-law. Dana returned from the
four-years cruise of the Wilkes Exploring Expedition in 1842; he settled in
New Haven, was married in 1844, and in 1850 was appointed Silliman
professor of Geology in Yale College. He was at this time actively engaged
in writing his three quarto reports for the Expedition and hence did not
begin his active professional duties in Yale College until 1856. Part of his
inaugural address was quoted on an earlier page.
staff of James Dwight Dana, Silliman’s son-in-law. Dana returned from the
four-years cruise of the Wilkes Exploring Expedition in 1842; he settled in
New Haven, was married in 1844, and in 1850 was appointed Silliman
professor of Geology in Yale College. He was at this time actively engaged
in writing his three quarto reports for the Expedition and hence did not
begin his active professional duties in Yale College until 1856. Part of his
inaugural address was quoted on an earlier page.
Page 52
Dana had already performed the severe labor of preparing the complete
index to the First Series, a volume of about 350 pages, finally issued in
1847. From the beginning of the Second Series he was closely associated
with his brother-in-law, the younger Silliman. Later the editorial labor
devolved more and more upon him and the larger part of this he carried
until about 1890. His work, was, however, somewhat interrupted during
periods of ill health. This was conspicuously true during a year’s absence in
Europe in 1859–60, made necessary in the search for health; during these
periods the editorial responsibility rested entirely upon the younger
Silliman. Of Dana’s contributions to science in general this is not the place
to speak, nor is the present writer the one to dwell in detail upon his work
for the Journal. This subject is to such an extent involved in the history of
geology and zoology, the subjects of several succeeding chapters, that it is
adequately presented in them.
It may, however, be worth stating that in the bibliography accompanying
the obituary notice of Dana (49, 329–356, 1895) some 250 titles of articles
in the Journal are enumerated; these aggregate approximately 2800 pages.
The number of critical notes, abstracts, book reviews, etc., could be also
given, were it worth while, but what is much more significant in this
connection, than their number or aggregate length, is the fact that these
notices are in a large number of cases—like those of Gray in botany—
minutely critical and original in matter. They thus give the writer’s own
opinion on a multitude of different subjects. It was a great benefit to Dana,
as it was to science also, that he had this prompt means at hand of putting
before the public the results of his active brain, which continued to work
unceasingly even in times of health prostration.
This may be the most convenient place to add that as Dana became
gradually less able to carry the burden of the details involved in editing the
Journal in addition to his more important scientific labors, particularly from
1890 on, this work devolved more and more upon his son, the present
editor, whose name was added to the editorial staff in 1875, with volume 9,
of the Third Series. The latter has served continuously until the present
time, with the exception of absences, due to ill health, in 1893–94 and in
1903; during the first of these Professor Henry S. Williams and during the
second Professor H. E. Gregory occupied the editorial chair.
index to the First Series, a volume of about 350 pages, finally issued in
1847. From the beginning of the Second Series he was closely associated
with his brother-in-law, the younger Silliman. Later the editorial labor
devolved more and more upon him and the larger part of this he carried
until about 1890. His work, was, however, somewhat interrupted during
periods of ill health. This was conspicuously true during a year’s absence in
Europe in 1859–60, made necessary in the search for health; during these
periods the editorial responsibility rested entirely upon the younger
Silliman. Of Dana’s contributions to science in general this is not the place
to speak, nor is the present writer the one to dwell in detail upon his work
for the Journal. This subject is to such an extent involved in the history of
geology and zoology, the subjects of several succeeding chapters, that it is
adequately presented in them.
It may, however, be worth stating that in the bibliography accompanying
the obituary notice of Dana (49, 329–356, 1895) some 250 titles of articles
in the Journal are enumerated; these aggregate approximately 2800 pages.
The number of critical notes, abstracts, book reviews, etc., could be also
given, were it worth while, but what is much more significant in this
connection, than their number or aggregate length, is the fact that these
notices are in a large number of cases—like those of Gray in botany—
minutely critical and original in matter. They thus give the writer’s own
opinion on a multitude of different subjects. It was a great benefit to Dana,
as it was to science also, that he had this prompt means at hand of putting
before the public the results of his active brain, which continued to work
unceasingly even in times of health prostration.
This may be the most convenient place to add that as Dana became
gradually less able to carry the burden of the details involved in editing the
Journal in addition to his more important scientific labors, particularly from
1890 on, this work devolved more and more upon his son, the present
editor, whose name was added to the editorial staff in 1875, with volume 9,
of the Third Series. The latter has served continuously until the present
time, with the exception of absences, due to ill health, in 1893–94 and in
1903; during the first of these Professor Henry S. Williams and during the
second Professor H. E. Gregory occupied the editorial chair.
Page 53
The Third Series began in 1871, after the completion of the one-
hundredth volume from the beginning in 1818. At this date the Journal was
made a monthly and as such it remains to-day. Fifty volumes again
completed this series, which closed in 1895.
The Fourth Series began with January, 1896, and the present number for
July, 1918, is the opening one of the forty-sixth volume or, in other words,
—the one hundred and ninety-sixth volume of the entire issue since 1818.
The Fourth Series, according to the precedent established, will end with
1920.
Associate Editors.—In 1851 the new policy was introduced of adding
“Associate Editors” to the staff. The first of these was Dr. Wolcott Gibbs of
Cambridge. He began his duties with the eleventh volume of the Second
Series in 1851 and continued them with unceasing care and thoroughness
for more than twenty years. In a note dated Jan. 1, 1851 (11, 105), he says:
It is my intention in future to prepare for the columns of this Journal abstracts of the more
important physical and chemical memoirs contained in foreign scientific journals, accompanied by
references, and by such critical observations as the occasion may demand. Contributions of a similar
character from others will of course not be excluded by this arrangement, but I shall hold myself
responsible only for those notices which appear over my initials.
The departments covered by Dr. Gibbs, in his excellent monthly
contributions, embraced chemistry and physics, and these subjects were
carried together until 1873 when they were separated and the physical notes
were furnished, first by Alfred M. Mayer and later successively by E. C.
Pickering (from 1874), J. P. Cooke (from 1877), and John Trowbridge (from
1880). The first instalment of the long series of notes in chemistry and
chemical physics by George F. Barker was printed in volume 50, 1870. He
came in at first to occasionally relieve Dr. Gibbs, but soon took the entire
responsibility. His name was placed among the associate editors on the
cover in 1877 and two years later Dr. Gibbs formally retired. It may be
added that from the beginning in 1851 to the present time, the notes in
“Chemistry and Physics” have been continued almost without interruption.
The other departments of science have been also fully represented in the
notes, abstracts of papers published, book notices, etc., of the successive
hundredth volume from the beginning in 1818. At this date the Journal was
made a monthly and as such it remains to-day. Fifty volumes again
completed this series, which closed in 1895.
The Fourth Series began with January, 1896, and the present number for
July, 1918, is the opening one of the forty-sixth volume or, in other words,
—the one hundred and ninety-sixth volume of the entire issue since 1818.
The Fourth Series, according to the precedent established, will end with
1920.
Associate Editors.—In 1851 the new policy was introduced of adding
“Associate Editors” to the staff. The first of these was Dr. Wolcott Gibbs of
Cambridge. He began his duties with the eleventh volume of the Second
Series in 1851 and continued them with unceasing care and thoroughness
for more than twenty years. In a note dated Jan. 1, 1851 (11, 105), he says:
It is my intention in future to prepare for the columns of this Journal abstracts of the more
important physical and chemical memoirs contained in foreign scientific journals, accompanied by
references, and by such critical observations as the occasion may demand. Contributions of a similar
character from others will of course not be excluded by this arrangement, but I shall hold myself
responsible only for those notices which appear over my initials.
The departments covered by Dr. Gibbs, in his excellent monthly
contributions, embraced chemistry and physics, and these subjects were
carried together until 1873 when they were separated and the physical notes
were furnished, first by Alfred M. Mayer and later successively by E. C.
Pickering (from 1874), J. P. Cooke (from 1877), and John Trowbridge (from
1880). The first instalment of the long series of notes in chemistry and
chemical physics by George F. Barker was printed in volume 50, 1870. He
came in at first to occasionally relieve Dr. Gibbs, but soon took the entire
responsibility. His name was placed among the associate editors on the
cover in 1877 and two years later Dr. Gibbs formally retired. It may be
added that from the beginning in 1851 to the present time, the notes in
“Chemistry and Physics” have been continued almost without interruption.
The other departments of science have been also fully represented in the
notes, abstracts of papers published, book notices, etc., of the successive
Page 54
numbers, but as with the chemistry and physics the subject of botany was
long treated in a similar formal manner. For the notes in this department, the
Journal was for many years indebted to Dr. Asa Gray, who became
associate editor in 1853, two years after Gibbs, although he had been a not
infrequent contributor for many years previously. Gray’s contributions were
furnished with great regularity and were always critical and original in
matter. They formed indeed one of the most valuable features of the Journal
for many years; as botanists well appreciate, and, as Professor Goodale has
emphasized in his chapter on botany, Gray’s notes are of vital importance in
the history of the development of his subject. With Gray’s retirement from
active duty, his colleague, George W. Goodale, took up the work in 1888
and in 1895 William G. Farlow, also of Cambridge, was added as an
associate editor in cryptogamic botany. At this time, however, and indeed
earlier, the sphere of the Journal had unavoidably contracted and botany
perforce ceased to occupy the prominent place it had long done in the
Journal pages.
This is not the place to present an appreciation of the truly magnificent
work of Asa Gray. It may not be out of place, however, to call attention to
the notice of Gray written for the Journal by his life-long friend, James D.
Dana (35, 181, 1888). The opening paragraph is as follows:
“Our friend and associate, Asa Gray, the eminent botanist of America, the broad-minded student of
nature, ended his life of unceasing and fruitful work on the 30th of January last. For thirty-five years
he has been one of the editors of this Journal, and for more than fifty years one of its contributors;
and through all his communications there is seen the profound and always delighted student, the
accomplished writer, the just and genial critic, and as Darwin has well said, ‘The lovable man.’”
The third associate editor, following Gray, was Louis Agassiz, whose
work for science, particularly in his adopted home in this country, calls for
no praise here. His term of service extended from 1853 to 1866 and,
particularly in the earlier years, his contributions were numerous and
important. The next gentleman in the list was Waldo I. Burnett, of Boston,
who served one year only, and then followed four of Dana’s colleagues in
New Haven, of whose generosity and able assistance it would be impossible
to say too much. These gentlemen were Brush in mineralogy; Johnson in
chemistry, particularly on the agricultural side; Newton in mathematics and
long treated in a similar formal manner. For the notes in this department, the
Journal was for many years indebted to Dr. Asa Gray, who became
associate editor in 1853, two years after Gibbs, although he had been a not
infrequent contributor for many years previously. Gray’s contributions were
furnished with great regularity and were always critical and original in
matter. They formed indeed one of the most valuable features of the Journal
for many years; as botanists well appreciate, and, as Professor Goodale has
emphasized in his chapter on botany, Gray’s notes are of vital importance in
the history of the development of his subject. With Gray’s retirement from
active duty, his colleague, George W. Goodale, took up the work in 1888
and in 1895 William G. Farlow, also of Cambridge, was added as an
associate editor in cryptogamic botany. At this time, however, and indeed
earlier, the sphere of the Journal had unavoidably contracted and botany
perforce ceased to occupy the prominent place it had long done in the
Journal pages.
This is not the place to present an appreciation of the truly magnificent
work of Asa Gray. It may not be out of place, however, to call attention to
the notice of Gray written for the Journal by his life-long friend, James D.
Dana (35, 181, 1888). The opening paragraph is as follows:
“Our friend and associate, Asa Gray, the eminent botanist of America, the broad-minded student of
nature, ended his life of unceasing and fruitful work on the 30th of January last. For thirty-five years
he has been one of the editors of this Journal, and for more than fifty years one of its contributors;
and through all his communications there is seen the profound and always delighted student, the
accomplished writer, the just and genial critic, and as Darwin has well said, ‘The lovable man.’”
The third associate editor, following Gray, was Louis Agassiz, whose
work for science, particularly in his adopted home in this country, calls for
no praise here. His term of service extended from 1853 to 1866 and,
particularly in the earlier years, his contributions were numerous and
important. The next gentleman in the list was Waldo I. Burnett, of Boston,
who served one year only, and then followed four of Dana’s colleagues in
New Haven, of whose generosity and able assistance it would be impossible
to say too much. These gentlemen were Brush in mineralogy; Johnson in
chemistry, particularly on the agricultural side; Newton in mathematics and
Page 55
astronomy, whose contributions will be spoken of elsewhere; and Verrill—a
student of Agassiz—in zoology.
All of these gentlemen, besides their frequent and important original
articles, were ever ready not only to give needed advice, but also, to furnish
brief communications, abstracts of papers and book reviews, and otherwise
to aid in the work. Verrill particularly furnished the Journal a long list of
original and important papers, chiefly in systematic zoology, extending
from 1865 almost down to the present year. His abstracts and book notices
also were numerous and trenchant and it is not too much to say that without
him the Journal never could have filled the place in zoology which it so
long held. Much later the list of New Haven men was increased by the
addition of Henry S. Williams (1894), and O. C. Marsh (1895).
student of Agassiz—in zoology.
All of these gentlemen, besides their frequent and important original
articles, were ever ready not only to give needed advice, but also, to furnish
brief communications, abstracts of papers and book reviews, and otherwise
to aid in the work. Verrill particularly furnished the Journal a long list of
original and important papers, chiefly in systematic zoology, extending
from 1865 almost down to the present year. His abstracts and book notices
also were numerous and trenchant and it is not too much to say that without
him the Journal never could have filled the place in zoology which it so
long held. Much later the list of New Haven men was increased by the
addition of Henry S. Williams (1894), and O. C. Marsh (1895).
Page 56
Of the valuable work of those more or less closely associated in the
conduct of the Journal at the present time, it would not be appropriate to
speak in detail. It must suffice to say that the services rendered freely by
them have been invaluable, and to their aid is due a large part of the success
of the Journal, especially since the Fourth Series began in 1896. But even
this statement is inadequate, for the editor-in-chief has had the generous
assistance of other gentlemen, whose names have not been placed on the
title page, and who have also played an important part in the conduct of the
Journal. This policy, indeed, is not a matter of recent date. Very early in the
First Series, Professor Griscom of Paris, as already noted, furnished notes
conduct of the Journal at the present time, it would not be appropriate to
speak in detail. It must suffice to say that the services rendered freely by
them have been invaluable, and to their aid is due a large part of the success
of the Journal, especially since the Fourth Series began in 1896. But even
this statement is inadequate, for the editor-in-chief has had the generous
assistance of other gentlemen, whose names have not been placed on the
title page, and who have also played an important part in the conduct of the
Journal. This policy, indeed, is not a matter of recent date. Very early in the
First Series, Professor Griscom of Paris, as already noted, furnished notes
Page 57
of interesting scientific discoveries abroad. Other gentlemen have from time
to time acted in the same capacity. The most prominent of them was
Professor Jerome Nicklès of Nancy, France, who regularly furnished a
series of valuable notes on varied subjects, chiefly from foreign sources,
extending from 1852 to 1869. On the latter date he met an untimely death in
his laboratory in connection with experiments upon hydrofluoric acid (47,
434, 1869).
It may be added, further, that one of the striking features about the
Journal, especially in the earlier half century of its existence, is the personal
nature of many of its contributions, which were very frequently in the form
of letters written to Benjamin Silliman or J. D. Dana. This is perhaps but
another reflection of the extent to which the growth of the magazine
centered around these two men, whose wide acquaintance and broad
scientific repute made of the Journal a natural place to record the new and
interesting things that were being discovered in science.
The following list gives the names and dates of service, as recorded on
the Journal title pages, of the gentlemen formally made Associate Editors:
to time acted in the same capacity. The most prominent of them was
Professor Jerome Nicklès of Nancy, France, who regularly furnished a
series of valuable notes on varied subjects, chiefly from foreign sources,
extending from 1852 to 1869. On the latter date he met an untimely death in
his laboratory in connection with experiments upon hydrofluoric acid (47,
434, 1869).
It may be added, further, that one of the striking features about the
Journal, especially in the earlier half century of its existence, is the personal
nature of many of its contributions, which were very frequently in the form
of letters written to Benjamin Silliman or J. D. Dana. This is perhaps but
another reflection of the extent to which the growth of the magazine
centered around these two men, whose wide acquaintance and broad
scientific repute made of the Journal a natural place to record the new and
interesting things that were being discovered in science.
The following list gives the names and dates of service, as recorded on
the Journal title pages, of the gentlemen formally made Associate Editors:
Page 58
Wolcott Gibbs (2) 11, 1851 to (3) 18, 1879
Asa Gray „ 15, 1853 „ „ 34, 1887
Louis Agassiz „ 16, 1853 „ (2) 41, 1866
Waldo I. Burnett „ 16, 1853 „ „ 17, 1853
George J. Brush „ 35, 1863 „ (3) 18, 1879
Samuel W. Johnson „ 35, 1863 „ „ 18, 1879
Hubert A. Newton (2) 38, 1864 to (4) 1, 1896
Addison E. Verrill „ 47, 1869
Alfred M. Mayer (3) 5, 1873 to (3) 6, 1873
Edward C. Pickering „ 7, 1874 „ „ 13, 1877
George F. Barker „ 14, 1877 „ (4) 29, 1910
Josiah P. Cooke „ 14, 1877 „ (3) 47, 1894
John Trowbridge (3) 19, 1880
George W. Goodale „ 35, 1888
Henry S. Williams „ 47, 1894
Henry P. Bowditch „ 49, 1895 to (4) 8, 1899
William G. Farlow „ 49, 1895
Othniel C. Marsh „ 49, 1895 to (4) 6, 1899
Henry A. Rowland (4) 1, 1896 „ „ 10, 1900
Joseph S. Diller „ 1, 1896
Louis V. Pirsson „ 7, 1899
William M. Davis „ 9, 1900
Joseph S. Ames „ 12, 1901
Horace L. Wells „ 18, 1904
Herbert E. Gregory „ 18, 1904
Horace S. Uhler „ 33, 1912
Asa Gray „ 15, 1853 „ „ 34, 1887
Louis Agassiz „ 16, 1853 „ (2) 41, 1866
Waldo I. Burnett „ 16, 1853 „ „ 17, 1853
George J. Brush „ 35, 1863 „ (3) 18, 1879
Samuel W. Johnson „ 35, 1863 „ „ 18, 1879
Hubert A. Newton (2) 38, 1864 to (4) 1, 1896
Addison E. Verrill „ 47, 1869
Alfred M. Mayer (3) 5, 1873 to (3) 6, 1873
Edward C. Pickering „ 7, 1874 „ „ 13, 1877
George F. Barker „ 14, 1877 „ (4) 29, 1910
Josiah P. Cooke „ 14, 1877 „ (3) 47, 1894
John Trowbridge (3) 19, 1880
George W. Goodale „ 35, 1888
Henry S. Williams „ 47, 1894
Henry P. Bowditch „ 49, 1895 to (4) 8, 1899
William G. Farlow „ 49, 1895
Othniel C. Marsh „ 49, 1895 to (4) 6, 1899
Henry A. Rowland (4) 1, 1896 „ „ 10, 1900
Joseph S. Diller „ 1, 1896
Louis V. Pirsson „ 7, 1899
William M. Davis „ 9, 1900
Joseph S. Ames „ 12, 1901
Horace L. Wells „ 18, 1904
Herbert E. Gregory „ 18, 1904
Horace S. Uhler „ 33, 1912
Page 59
Present and Future Conditions.
The field to be occupied by the “American Journal of Science and Arts,”
as seen by its founder in 1818 and presented by him in the first number, as
quoted entire on an earlier page, was as broad as the entire sphere of science
itself. It thus included all the departments of both pure and applied science
and extended even to music and fine arts also. As the years went by,
however, and the practical applications of science greatly increased,
technical journals started up, and the necessity of cultivating this constantly
expanding field diminished. It was not, however, until January, 1880, that
“the Arts” ceased to be a part of the name by which the Journal was known.
About the same date also—or better a little earlier—began an increasing
development of scientific research, particularly as fostered by the graduate
schools of our prominent universities. The full presentation of this subject
would require much space and is indeed unnecessary as the main facts must
be distinct in the mind of the reader. It is only right, however, that the large
part played in this movement by the Johns Hopkins University (founded in
1876) should be mentioned here.
As a result of this movement, which has been of great benefit in
stimulating the growth of science in the country, many new journals of
specialized character have come into existence from time to time. Further
localization and specialization of scientific publication have resulted from
the increased activity of scientific societies and academies at numerous
centers and the springing into existence thereby of new organs of
publication through them, as also through certain of the Government
Departments, the Carnegie Institution, and certain universities and
museums.
As bearing upon this subject, the following list of the more prominent
scientific periodicals started in this country since 1867 is not without
interest:
1867– . American Naturalist.
1875– . Botanical Bulletin; later Botanical Gazette.
1879–1913. American Chemical Journal.
The field to be occupied by the “American Journal of Science and Arts,”
as seen by its founder in 1818 and presented by him in the first number, as
quoted entire on an earlier page, was as broad as the entire sphere of science
itself. It thus included all the departments of both pure and applied science
and extended even to music and fine arts also. As the years went by,
however, and the practical applications of science greatly increased,
technical journals started up, and the necessity of cultivating this constantly
expanding field diminished. It was not, however, until January, 1880, that
“the Arts” ceased to be a part of the name by which the Journal was known.
About the same date also—or better a little earlier—began an increasing
development of scientific research, particularly as fostered by the graduate
schools of our prominent universities. The full presentation of this subject
would require much space and is indeed unnecessary as the main facts must
be distinct in the mind of the reader. It is only right, however, that the large
part played in this movement by the Johns Hopkins University (founded in
1876) should be mentioned here.
As a result of this movement, which has been of great benefit in
stimulating the growth of science in the country, many new journals of
specialized character have come into existence from time to time. Further
localization and specialization of scientific publication have resulted from
the increased activity of scientific societies and academies at numerous
centers and the springing into existence thereby of new organs of
publication through them, as also through certain of the Government
Departments, the Carnegie Institution, and certain universities and
museums.
As bearing upon this subject, the following list of the more prominent
scientific periodicals started in this country since 1867 is not without
interest:
1867– . American Naturalist.
1875– . Botanical Bulletin; later Botanical Gazette.
1879–1913. American Chemical Journal.
Page 60
1880–1915. School of Mines Quarterly.
1883– . Science.
1885– . Journal of Heredity.
1887– . Journal of Morphology.
1887–1908. Technology Quarterly.
1888–1905. American Geologist.
1891– . Journal of Comparative Neurology.
1893– . Journal of Geology.
1893– . Physical Review.
1895– . Astrophysical Journal.
1896– . Journal of Physical Chemistry.
1896– . Terrestrial Magnetism.
1897–1899. Zoological Bulletin; followed by
1900– . Biological Bulletin.
1901– . American Journal of Anatomy.
1904– . Journal of Experimental Zoology.
1905– . Economic Geology.
1906– . Anatomical Record.
1907– . Journal of Economic Entomology.
1911– . Journal of Animal Behavior.
1914– . American Journal of Botany.
1916– . Genetics.
1918– . American Journal of Physical Anthropology.
The result of the whole movement has been of necessity to narrow, little
by little, the sphere of a general scientific periodical such as the Journal has
been from the beginning. The exact change might be studied in detail by
tabulating as to subjects the contents of successive volumes, decade by
1883– . Science.
1885– . Journal of Heredity.
1887– . Journal of Morphology.
1887–1908. Technology Quarterly.
1888–1905. American Geologist.
1891– . Journal of Comparative Neurology.
1893– . Journal of Geology.
1893– . Physical Review.
1895– . Astrophysical Journal.
1896– . Journal of Physical Chemistry.
1896– . Terrestrial Magnetism.
1897–1899. Zoological Bulletin; followed by
1900– . Biological Bulletin.
1901– . American Journal of Anatomy.
1904– . Journal of Experimental Zoology.
1905– . Economic Geology.
1906– . Anatomical Record.
1907– . Journal of Economic Entomology.
1911– . Journal of Animal Behavior.
1914– . American Journal of Botany.
1916– . Genetics.
1918– . American Journal of Physical Anthropology.
The result of the whole movement has been of necessity to narrow, little
by little, the sphere of a general scientific periodical such as the Journal has
been from the beginning. The exact change might be studied in detail by
tabulating as to subjects the contents of successive volumes, decade by
Page 61
decade, from 1870 down. It is sufficient, here, however, to recognize the
general fact that while the number of original papers published in the
periodicals of this country, in 1910, for example, was very many times what
it was in 1825, a large part of these have naturally found their home in
periodicals devoted to the special subject dealt with in each case. That this
movement will continue, though in lessened degree now that the immediate
demand is measurably satisfied, is to be expected. At the same time it has
not seemed wise, at any time in the past, to formally restrict the pages of the
Journal to any single group of subjects. The future is before us and its
problems will be met as they arise. At the moment, however, there seems to
be still a place for a scientific monthly sufficiently broad to include original
papers of important general bearing even if special in immediate subject. In
this way it would seem that “Silliman’s Journal” can best continue to meet
the ideals of its honored founder, modified as they must be to meet the
change of conditions which a century of scientific investigation and growth
have wrought. Incidentally it is not out of place to add that a self-
supporting, non-subsidized scientific periodical may hope to find a larger
number of subscribers from among the workers in science and the libraries
if it is not too restricted in scope.
The last subject touched upon introduces the essential matter of financial
support without which no monthly publication can survive. With respect to
the periodicals of recent birth, listed above, it is safe to say that some form
of substantial support or subsidy—often very generous—is the rule, perhaps
the universal one. This has never been the case with the American Journal.
The liberality and broad-minded attitude of Yale College in the early days,
and of the Yale University that has developed from it, have never been
questioned. At the same time the special conditions have been such as to
make it desirable that the responsibility of meeting the financial
requirements should be carried by the editors-in-chief. At present the Yale
Library gives adequate payment for certain publications received by the
Journal in exchange, though for many years they were given to it as a
matter of course, free of charge. Beyond this there is nothing approaching a
subsidy.
The difficulties on the financial side met with by the elder Silliman have
been suggested, although not adequately presented, in the various
statements quoted from early volumes. The same problems in varying
degree have continued for the past sixty years. Since 1914 they have been
general fact that while the number of original papers published in the
periodicals of this country, in 1910, for example, was very many times what
it was in 1825, a large part of these have naturally found their home in
periodicals devoted to the special subject dealt with in each case. That this
movement will continue, though in lessened degree now that the immediate
demand is measurably satisfied, is to be expected. At the same time it has
not seemed wise, at any time in the past, to formally restrict the pages of the
Journal to any single group of subjects. The future is before us and its
problems will be met as they arise. At the moment, however, there seems to
be still a place for a scientific monthly sufficiently broad to include original
papers of important general bearing even if special in immediate subject. In
this way it would seem that “Silliman’s Journal” can best continue to meet
the ideals of its honored founder, modified as they must be to meet the
change of conditions which a century of scientific investigation and growth
have wrought. Incidentally it is not out of place to add that a self-
supporting, non-subsidized scientific periodical may hope to find a larger
number of subscribers from among the workers in science and the libraries
if it is not too restricted in scope.
The last subject touched upon introduces the essential matter of financial
support without which no monthly publication can survive. With respect to
the periodicals of recent birth, listed above, it is safe to say that some form
of substantial support or subsidy—often very generous—is the rule, perhaps
the universal one. This has never been the case with the American Journal.
The liberality and broad-minded attitude of Yale College in the early days,
and of the Yale University that has developed from it, have never been
questioned. At the same time the special conditions have been such as to
make it desirable that the responsibility of meeting the financial
requirements should be carried by the editors-in-chief. At present the Yale
Library gives adequate payment for certain publications received by the
Journal in exchange, though for many years they were given to it as a
matter of course, free of charge. Beyond this there is nothing approaching a
subsidy.
The difficulties on the financial side met with by the elder Silliman have
been suggested, although not adequately presented, in the various
statements quoted from early volumes. The same problems in varying
degree have continued for the past sixty years. Since 1914 they have been
Page 62
seriously aggravated for reasons that need not be enlarged upon. Prior to
that date the subscription list had, for reasons chiefly involved in the
development of special journals, been much smaller than the number
estimated by Silliman, for example, in volume 50 (p. xiv), although there
has been this partial compensation that the considerable number of well-
established libraries on the subscription list has meant a greater degree of
stability and a smaller proportion of bad accounts. The past four years,
however, the Journal, with all similar undertakings here and elsewhere, has
been compelled to bear its share of the burden of the world war in
diminished receipts and greatly increased expenses. It is gratifying to be
able to acknowledge here the generosity of the authors, or of the
laboratories with which they have been connected, in their willingness not
infrequently to give assistance, for example, in the payment of more or less
of the cost of engravings, or in a few special cases a large portion of the
total cost of publication. In this way the problem of ways and means,
constantly before the editor who bears the sole responsibility, has been
simplified.
It should also be stated that as those immediately interested have looked
forward to the present anniversary, it has been with the hope that this
occasion might be an appropriate one for the establishment of a “Silliman
Fund” to commemorate the life and work of Benjamin Silliman. The
income of such a fund would lift from the University the burden that must
unavoidably fall upon it when the responsibility for the conduct of the
Journal can no longer be carried by members of the family including the
editor and—as in years long past—a silent partner whose aid on the
business side has been essential to the efficiency and economy of the
enterprise. Present conditions are not favorable for such a movement,
although something has been already accomplished in the desired direction.
At the present time every patriotic citizen must feel it his first duty to give
his savings as well as his spare income to the support of the National
Government in the world struggle for freedom in which it is taking part.
But, whatever the exact condition of the future may be, it cannot be
questioned that the Journal founded by Benjamin Silliman in 1818 will
survive and will continue to play a vital part in the support and further
development of science.
The present year of 1918 finds the world at large, and with it the world of
science, painfully crushed beneath the overwhelming weight of a world war
that date the subscription list had, for reasons chiefly involved in the
development of special journals, been much smaller than the number
estimated by Silliman, for example, in volume 50 (p. xiv), although there
has been this partial compensation that the considerable number of well-
established libraries on the subscription list has meant a greater degree of
stability and a smaller proportion of bad accounts. The past four years,
however, the Journal, with all similar undertakings here and elsewhere, has
been compelled to bear its share of the burden of the world war in
diminished receipts and greatly increased expenses. It is gratifying to be
able to acknowledge here the generosity of the authors, or of the
laboratories with which they have been connected, in their willingness not
infrequently to give assistance, for example, in the payment of more or less
of the cost of engravings, or in a few special cases a large portion of the
total cost of publication. In this way the problem of ways and means,
constantly before the editor who bears the sole responsibility, has been
simplified.
It should also be stated that as those immediately interested have looked
forward to the present anniversary, it has been with the hope that this
occasion might be an appropriate one for the establishment of a “Silliman
Fund” to commemorate the life and work of Benjamin Silliman. The
income of such a fund would lift from the University the burden that must
unavoidably fall upon it when the responsibility for the conduct of the
Journal can no longer be carried by members of the family including the
editor and—as in years long past—a silent partner whose aid on the
business side has been essential to the efficiency and economy of the
enterprise. Present conditions are not favorable for such a movement,
although something has been already accomplished in the desired direction.
At the present time every patriotic citizen must feel it his first duty to give
his savings as well as his spare income to the support of the National
Government in the world struggle for freedom in which it is taking part.
But, whatever the exact condition of the future may be, it cannot be
questioned that the Journal founded by Benjamin Silliman in 1818 will
survive and will continue to play a vital part in the support and further
development of science.
The present year of 1918 finds the world at large, and with it the world of
science, painfully crushed beneath the overwhelming weight of a world war
Page 63
of unprecedented severity. The four terrible years now nearly finished have
seen a fearful destruction of life and property which must have a sad
influence on the progress of science for many years to come. Only in
certain restricted lines has there been a partial compensation in the
stimulating influence due to the immediate necessities connected with the
great conflict. One hundred years ago “the reign of war” was keenly in the
mind of the editor in beginning his work, but for him, happily, the long
period of the Napoleonic wars was already in the past, as also the brief
conflict of 1812, in which this country was engaged and in which Silliman
himself played a minor part. We, too, must believe, no matter how serious
the outlook of the present moment, that a fundamental change will come in
the not distant future; the nations of the world must sooner or later turn
once more to peaceful pursuits and the scientific men of different races
must become again not enemies but brothers engaged in the common cause
of uplifting human life. The peace that we look forward to to-day is not for
this country alone, but a peace which shall be a permanent blessing to the
entire world for ages to come.
Note.—The portrait which forms the frontispiece of this volume has
been reproduced from the plate in volume 50 (1847). The original painting
was made by H. Willard in 1835, when Silliman was in Boston engaged in
delivering the Lowell lectures; he was then nearly fifty-six years of age.
The engraving, as he states elsewhere, was made from this painting for the
Yale Literary Magazine, and was published in the number for December,
1839.
It is interesting to quote the remarks with which the editor introduces the
portrait (50, xviii, 1847). He says:
The portrait prefixed to this volume was engraved for a very different purpose and for others than
the patrons of this Journal. It has been suggested by friends, whose judgment we are accustomed to
respect, that it ought to find a place here, since it is regarded as an authentic, although, perhaps, a
rather austere resemblance. In yielding to this suggestion, it may be sufficient to quote the sentiment
of Cowper on a similar occasion, who remarked—“that after a man has, for many years, turned his
mind inside out before the world, it is only affectation to attempt to hide his face.”
seen a fearful destruction of life and property which must have a sad
influence on the progress of science for many years to come. Only in
certain restricted lines has there been a partial compensation in the
stimulating influence due to the immediate necessities connected with the
great conflict. One hundred years ago “the reign of war” was keenly in the
mind of the editor in beginning his work, but for him, happily, the long
period of the Napoleonic wars was already in the past, as also the brief
conflict of 1812, in which this country was engaged and in which Silliman
himself played a minor part. We, too, must believe, no matter how serious
the outlook of the present moment, that a fundamental change will come in
the not distant future; the nations of the world must sooner or later turn
once more to peaceful pursuits and the scientific men of different races
must become again not enemies but brothers engaged in the common cause
of uplifting human life. The peace that we look forward to to-day is not for
this country alone, but a peace which shall be a permanent blessing to the
entire world for ages to come.
Note.—The portrait which forms the frontispiece of this volume has
been reproduced from the plate in volume 50 (1847). The original painting
was made by H. Willard in 1835, when Silliman was in Boston engaged in
delivering the Lowell lectures; he was then nearly fifty-six years of age.
The engraving, as he states elsewhere, was made from this painting for the
Yale Literary Magazine, and was published in the number for December,
1839.
It is interesting to quote the remarks with which the editor introduces the
portrait (50, xviii, 1847). He says:
The portrait prefixed to this volume was engraved for a very different purpose and for others than
the patrons of this Journal. It has been suggested by friends, whose judgment we are accustomed to
respect, that it ought to find a place here, since it is regarded as an authentic, although, perhaps, a
rather austere resemblance. In yielding to this suggestion, it may be sufficient to quote the sentiment
of Cowper on a similar occasion, who remarked—“that after a man has, for many years, turned his
mind inside out before the world, it is only affectation to attempt to hide his face.”
Page 64
Notes.
1. The statements given are necessarily much condensed, without an attempt to follow all
changes of title; furthermore, the dates of actual publication for the academies given above are often
somewhat vaguely recorded. For fuller information see Scudder’s “Catalogue of Scientific Serials,
1633–1876,” Cambridge, 1876; also H. Carrington Bolton’s “Catalogue of Scientific and Technical
Periodicals, 1665–1882” (Smithsonian Institution, 1885). The writer is much indebted to Mr. C. J.
Barr, Assistant Librarian of Yale University Library, for his valuable assistance in this connection.
2. The following footnote accompanies the opening article of the first volume of the Journal.
“From the MS. papers of the Connecticut Academy, now published by permission.” Similar notes
appear elsewhere. Ed.
1. The statements given are necessarily much condensed, without an attempt to follow all
changes of title; furthermore, the dates of actual publication for the academies given above are often
somewhat vaguely recorded. For fuller information see Scudder’s “Catalogue of Scientific Serials,
1633–1876,” Cambridge, 1876; also H. Carrington Bolton’s “Catalogue of Scientific and Technical
Periodicals, 1665–1882” (Smithsonian Institution, 1885). The writer is much indebted to Mr. C. J.
Barr, Assistant Librarian of Yale University Library, for his valuable assistance in this connection.
2. The following footnote accompanies the opening article of the first volume of the Journal.
“From the MS. papers of the Connecticut Academy, now published by permission.” Similar notes
appear elsewhere. Ed.
Page 65
II
A CENTURY OF GEOLOGY.—THE PROGRESS OF
HISTORICAL GEOLOGY IN NORTH AMERICA
By CHARLES SCHUCHERT
Introduction.
The American Journal of Science, “one of the greatest influences in
American geology,” founded in 1818, has published a little more than
92,000 pages of scientific matter. Of geology, including mineralogy, there
appear to be upward of 20,000 pages. What a vast treasure house of
geologic knowledge is stored in these 194 volumes, and how well the
editors have lived up to their proposed “plan of work” as stated in the
opening volume, where Silliman says: “It is designed as a deposit for
original American communications” in “the physical sciences ... and
especially our mineralogy and geology” (1, v, 1818)! Not only is it the
oldest continuously published scientific journal of this country, but it has
proved itself to be “perhaps the most important geological periodical in
America” (Merrill). It is impossible to adequately present in this memorial
volume of the Journal the contents of the articles on the geological sciences.
Editor Silliman was not only the founder of the Journal, but the
generating center for the making of geologists and promoting geology
during the rise of this science in America. For nearly three decades, the
workers came to him for counsel and help, and he had a kind paternal word
for them all. This influence is also shown in the many letters which were
addressed to him, and which he published in the Journal. A similar
A CENTURY OF GEOLOGY.—THE PROGRESS OF
HISTORICAL GEOLOGY IN NORTH AMERICA
By CHARLES SCHUCHERT
Introduction.
The American Journal of Science, “one of the greatest influences in
American geology,” founded in 1818, has published a little more than
92,000 pages of scientific matter. Of geology, including mineralogy, there
appear to be upward of 20,000 pages. What a vast treasure house of
geologic knowledge is stored in these 194 volumes, and how well the
editors have lived up to their proposed “plan of work” as stated in the
opening volume, where Silliman says: “It is designed as a deposit for
original American communications” in “the physical sciences ... and
especially our mineralogy and geology” (1, v, 1818)! Not only is it the
oldest continuously published scientific journal of this country, but it has
proved itself to be “perhaps the most important geological periodical in
America” (Merrill). It is impossible to adequately present in this memorial
volume of the Journal the contents of the articles on the geological sciences.
Editor Silliman was not only the founder of the Journal, but the
generating center for the making of geologists and promoting geology
during the rise of this science in America. For nearly three decades, the
workers came to him for counsel and help, and he had a kind paternal word
for them all. This influence is also shown in the many letters which were
addressed to him, and which he published in the Journal. A similar
Page 66
influence, paternal care, and constructive criticism were continued by James
D. Dana, and especially in his earlier career as editor.
Not including mineralogy, there are in the Journal upward of 1500
distinct articles on geology. Of these, over 400 are on vertebrate
paleontology, about 325 on invertebrate paleontology, and 90 on
paleobotany. Of articles bearing on historical geology there are about 160,
and on stratigraphic geology more than 360. In addition to all this, there are
more than 2000 pages of geologic matter relating to books and of letters
communicated to the editors Silliman and Dana. We may summarize with
Doctor Merrill’s statement in his well-known Contributions to the History
of American Geology:
“From its earliest inception geological notes and papers occupied a prominent place in its pages,
and a perusal of the numbers from the date of issue down to the present time will, alone, afford a fair
idea of the gradual progress of American geology.”
Before presenting a synopsis of the more important steps in the progress
of historical geology in America, it will be well to introduce a rapid survey
of the rise of geology in Europe, for, after all, American geology grew out
of that of England, France and Germany. This dependence was
conspicuously true during the first four decades of the previous century.
With the rise of the first New York State Survey (1836–1843) and that of
Pennsylvania (1836–1844, 1858), American geology became more or less
independent of Europe. Finally, this article will conclude with a survey of
the rise of paleometeorology, paleogeography, evolution, and invertebrate
paleontology.
D. Dana, and especially in his earlier career as editor.
Not including mineralogy, there are in the Journal upward of 1500
distinct articles on geology. Of these, over 400 are on vertebrate
paleontology, about 325 on invertebrate paleontology, and 90 on
paleobotany. Of articles bearing on historical geology there are about 160,
and on stratigraphic geology more than 360. In addition to all this, there are
more than 2000 pages of geologic matter relating to books and of letters
communicated to the editors Silliman and Dana. We may summarize with
Doctor Merrill’s statement in his well-known Contributions to the History
of American Geology:
“From its earliest inception geological notes and papers occupied a prominent place in its pages,
and a perusal of the numbers from the date of issue down to the present time will, alone, afford a fair
idea of the gradual progress of American geology.”
Before presenting a synopsis of the more important steps in the progress
of historical geology in America, it will be well to introduce a rapid survey
of the rise of geology in Europe, for, after all, American geology grew out
of that of England, France and Germany. This dependence was
conspicuously true during the first four decades of the previous century.
With the rise of the first New York State Survey (1836–1843) and that of
Pennsylvania (1836–1844, 1858), American geology became more or less
independent of Europe. Finally, this article will conclude with a survey of
the rise of paleometeorology, paleogeography, evolution, and invertebrate
paleontology.
Page 67
The Rise of Geology in Europe.
Mineral Geology.—The geological sciences had their rise in the study of
minerals as carried on by the German chemist and physician George Bauer
(1494–1555), better known as Agricola. Bauer originated the critical study
of minerals, but did not distinguish his “fossilia,” the remains of organisms,
from the inorganic crystal forms. Mineral geology endured until the close of
the eighteenth century.
Cosmogonists.—Then came the expounders of the earth’s origin, the
cosmogonists of the sixteenth to the end of the eighteenth centuries. The
fashion of this time was to write histories of the earth derived out of the
imagination.
Earliest Historical Geology.—Even though Giovanni Arduino (1713–
1795) of Padua was not the first to classify the rocks into three series
according to their age, he did this more clearly than any one else before his
time. The rocks about Verona he grouped in 1759 into Primary, Secondary,
Tertiary, and Volcanic. This three-fold classification came into general use,
though modified with time.
Early in the nineteenth century it had become plain that formations of
very varying ages were included in each one of the three series. Through the
study of the fossils and the recognition of the fact that mountain ranges
have been raised at various times, causing younger fossiliferous strata to
take on the characters of the Primary, it was seen that these terms of
Arduino had lost their original significance.
The first one to describe in detail a local stratigraphic sequence was
Johann Gottlob Lehmann (died 1767). In 1756 he published “one of the
classics of geological literature,” distinguishing clearly thirty successive
sedimentary deposits, some of which he said had fossils, but he did not use
them to distinguish the strata.
What Lehmann did for the Permian system, George Christian Füchsel
(1722–1773) did even better for the Triassic of Thuringia, in 1762 and
1773. He pointed out not only the sequence, but also how the gently
inclined strata rest upon the older upturned masses of the mountains; also
that some formations have only marine fossils, while others have only
Mineral Geology.—The geological sciences had their rise in the study of
minerals as carried on by the German chemist and physician George Bauer
(1494–1555), better known as Agricola. Bauer originated the critical study
of minerals, but did not distinguish his “fossilia,” the remains of organisms,
from the inorganic crystal forms. Mineral geology endured until the close of
the eighteenth century.
Cosmogonists.—Then came the expounders of the earth’s origin, the
cosmogonists of the sixteenth to the end of the eighteenth centuries. The
fashion of this time was to write histories of the earth derived out of the
imagination.
Earliest Historical Geology.—Even though Giovanni Arduino (1713–
1795) of Padua was not the first to classify the rocks into three series
according to their age, he did this more clearly than any one else before his
time. The rocks about Verona he grouped in 1759 into Primary, Secondary,
Tertiary, and Volcanic. This three-fold classification came into general use,
though modified with time.
Early in the nineteenth century it had become plain that formations of
very varying ages were included in each one of the three series. Through the
study of the fossils and the recognition of the fact that mountain ranges
have been raised at various times, causing younger fossiliferous strata to
take on the characters of the Primary, it was seen that these terms of
Arduino had lost their original significance.
The first one to describe in detail a local stratigraphic sequence was
Johann Gottlob Lehmann (died 1767). In 1756 he published “one of the
classics of geological literature,” distinguishing clearly thirty successive
sedimentary deposits, some of which he said had fossils, but he did not use
them to distinguish the strata.
What Lehmann did for the Permian system, George Christian Füchsel
(1722–1773) did even better for the Triassic of Thuringia, in 1762 and
1773. He pointed out not only the sequence, but also how the gently
inclined strata rest upon the older upturned masses of the mountains; also
that some formations have only marine fossils, while others have only
Page 68
terrestrial forms and thus indicate the proximity of land. The deformed
strata he thought had fallen into the hollows within the earth, great caverns
that had also consumed much of the oceanic waters and had in so doing
greatly lowered the sea-level. It was Füchsel who first introduced the theory
of universal formations, and who defined the term formation, using it as we
now do, system or period. Even though Lehmann and Füchsel showed that
there was a definite order and process in the formation of the earth’s crust,
their example was barren of followers until the beginning of the eighteenth
century.
Wernerian Geology or Geognosy.—We come now to the time of
Abraham Gottlob Werner (1749–1817), who from 1775 to 1817 was
professor of mining and mineralogy in the Freiberg Academy of Mines.
Geikie, in his most interesting Founders of Geology, says that Werner
“bulks far more largely in the history of geology than any of those with
whom up to the present we have been concerned—a man who wielded an
enormous authority over the mineralogy and geology of his day.”
“Although he did great service by the precision of his lithological characters
and by his insistence on the doctrine of geological succession, yet as
regards geological theory, whether directly by his own teaching, or
indirectly by the labors of his pupils and followers, much of his influence
was disastrous to the higher interests of geology.”
Werner arranged the crust of the earth into a series of formations, as had
been done previously by Lehmann and Füchsel, and one of his fundamental
postulates was that all rocks were chemically precipitated in the ocean as
“universal formations.” For this reason Werner’s school were called the
Neptunists. Nowhere, however, did he explain how and where the deep and
primitive ocean had disappeared.
According to Werner, the first formed or oldest rocks were the chemically
deposited Primitive strata, including granite and other igneous and
metamorphic rocks. On these followed the Transition rocks, the earliest
sediments of mechanical origin, and above them the Floetz rocks, a term for
the horizontal stratified rocks. These last he said were partly of chemical
but chiefly of mechanical origin. Last of all came the Alluvial series.
The existence of volcanoes had been pointed out long before Werner’s
time by the Italian school of geologists, but as for “the universality and
potency of what is now termed igneous action,” all was “brushed aside by
strata he thought had fallen into the hollows within the earth, great caverns
that had also consumed much of the oceanic waters and had in so doing
greatly lowered the sea-level. It was Füchsel who first introduced the theory
of universal formations, and who defined the term formation, using it as we
now do, system or period. Even though Lehmann and Füchsel showed that
there was a definite order and process in the formation of the earth’s crust,
their example was barren of followers until the beginning of the eighteenth
century.
Wernerian Geology or Geognosy.—We come now to the time of
Abraham Gottlob Werner (1749–1817), who from 1775 to 1817 was
professor of mining and mineralogy in the Freiberg Academy of Mines.
Geikie, in his most interesting Founders of Geology, says that Werner
“bulks far more largely in the history of geology than any of those with
whom up to the present we have been concerned—a man who wielded an
enormous authority over the mineralogy and geology of his day.”
“Although he did great service by the precision of his lithological characters
and by his insistence on the doctrine of geological succession, yet as
regards geological theory, whether directly by his own teaching, or
indirectly by the labors of his pupils and followers, much of his influence
was disastrous to the higher interests of geology.”
Werner arranged the crust of the earth into a series of formations, as had
been done previously by Lehmann and Füchsel, and one of his fundamental
postulates was that all rocks were chemically precipitated in the ocean as
“universal formations.” For this reason Werner’s school were called the
Neptunists. Nowhere, however, did he explain how and where the deep and
primitive ocean had disappeared.
According to Werner, the first formed or oldest rocks were the chemically
deposited Primitive strata, including granite and other igneous and
metamorphic rocks. On these followed the Transition rocks, the earliest
sediments of mechanical origin, and above them the Floetz rocks, a term for
the horizontal stratified rocks. These last he said were partly of chemical
but chiefly of mechanical origin. Last of all came the Alluvial series.
The existence of volcanoes had been pointed out long before Werner’s
time by the Italian school of geologists, but as for “the universality and
potency of what is now termed igneous action,” all was “brushed aside by
Page 69
the oracle of Freiberg.” Reactions between the interior and exterior of our
earth “were utterly antagonistic to Werner’s conception of the structure and
history of the earth.” To him, volcanoes were “burning mountains” that
arose from the combustion of subterranean beds of coal, spontaneously
ignited.
The breaking down of the Wernerian doctrines began with two of
Werner’s most distinguished pupils, D’Aubuisson de Voisins (1769–1819)
and Von Buch. The former in 1803 had accepted Werner’s aqueous origin of
basalt, but after studying the celebrated and quite recent volcanic area of
Auvergne he recanted in 1804. Here he saw the basaltic rocks lying upon
and cutting through granite, and in places more than 1200 feet thick. “If
these basaltic rocks were lavas,” says Geikie, “they must, according to the
Wernerian doctrine, have resulted from the combustion of beds of coal. But
how could coal be supposed to exist under granite, which was the first
chemical precipitate of a primeval ocean?”
Leopold von Buch (1774–1853), “the most illustrious geologist that
Germany has produced,” after two years spent in Norway was satisfied
“that the rocks in the Christiania district could not be arranged according to
the Wernerian plan, which there completely broke down. Von Buch found a
mass of granite lying among fossiliferous limestones which were manifestly
metamorphosed, and were pierced by veins of granite, porphyry, and
syenite.” Even so, he was not ready to abandon the teachings of his master.
After a study of the mountain systems of Germany, however, “he declared
that the more elevated mountains had never been covered by the sea, as
Werner had taught, but were produced by successive ruptures and uplifts of
the terrestrial crust” (Geikie).
Rise of Geology and Conformism.—Modern geology has its rise in James
Hutton (1726–1797) of Edinburgh, Scotland. In 1785 and 1795, Hutton
published his Theory of the Earth, with Proofs and Illustrations. His
“immortal theory” is his only work on geology. “Fortunately for Hutton’s
fame and for the onward march of geology, the philosopher numbered
among his friends the illustrious mathematician and natural philosopher,
John Playfair (1748–1819), who had been closely associated with him in his
later years, and was intimately conversant with his geological opinions.” In
1802, Playfair published his Illustrations of the Huttonian Theory of the
earth “were utterly antagonistic to Werner’s conception of the structure and
history of the earth.” To him, volcanoes were “burning mountains” that
arose from the combustion of subterranean beds of coal, spontaneously
ignited.
The breaking down of the Wernerian doctrines began with two of
Werner’s most distinguished pupils, D’Aubuisson de Voisins (1769–1819)
and Von Buch. The former in 1803 had accepted Werner’s aqueous origin of
basalt, but after studying the celebrated and quite recent volcanic area of
Auvergne he recanted in 1804. Here he saw the basaltic rocks lying upon
and cutting through granite, and in places more than 1200 feet thick. “If
these basaltic rocks were lavas,” says Geikie, “they must, according to the
Wernerian doctrine, have resulted from the combustion of beds of coal. But
how could coal be supposed to exist under granite, which was the first
chemical precipitate of a primeval ocean?”
Leopold von Buch (1774–1853), “the most illustrious geologist that
Germany has produced,” after two years spent in Norway was satisfied
“that the rocks in the Christiania district could not be arranged according to
the Wernerian plan, which there completely broke down. Von Buch found a
mass of granite lying among fossiliferous limestones which were manifestly
metamorphosed, and were pierced by veins of granite, porphyry, and
syenite.” Even so, he was not ready to abandon the teachings of his master.
After a study of the mountain systems of Germany, however, “he declared
that the more elevated mountains had never been covered by the sea, as
Werner had taught, but were produced by successive ruptures and uplifts of
the terrestrial crust” (Geikie).
Rise of Geology and Conformism.—Modern geology has its rise in James
Hutton (1726–1797) of Edinburgh, Scotland. In 1785 and 1795, Hutton
published his Theory of the Earth, with Proofs and Illustrations. His
“immortal theory” is his only work on geology. “Fortunately for Hutton’s
fame and for the onward march of geology, the philosopher numbered
among his friends the illustrious mathematician and natural philosopher,
John Playfair (1748–1819), who had been closely associated with him in his
later years, and was intimately conversant with his geological opinions.” In
1802, Playfair published his Illustrations of the Huttonian Theory of the
Page 70
Earth, of which Geikie says, “Of this great classic it is impossible to speak
too highly,” as it is at the basis of all modern geology.
One of Hutton’s fundamental doctrines is that the earth is internally hot
and that in the past large masses of molten material, the granites, have been
intruded into the crust. It was these igneous views that led to his followers
being called the Plutonists. Another of his great doctrines was that “the
ruins of an earlier world lie beneath the secondary strata,” and that they are
separated by what is now known as unconformity. He clearly recognized a
lost interval in the broken relation of the structures, and that the ruins, the
detrital materials, of one world after another are superposed in the structure
of the earth.
Hutton also held that the deformation of once horizontally deposited
strata was probably brought about at different periods by great convulsions
that shook the very foundations of the earth. After a convulsion, there was a
long time of erosion, represented by the unconformity. Geikie says, “The
whole of the modern doctrine of earth sculpture is to be found in the
Huttonian theory.”
The Lyellian doctrine of metamorphism had its origin in Hutton, for he
showed that invading igneous granite had altered, through its heat and
expanding power, the originally waterlaid sediments, and that the schists of
the Alps had been born of the sea like other stratified rocks.
Hutton is the father of the Uniformitarian principle, for he “started with
the grand conception that the past history of our globe must be explained by
what can be seen to be happening now, or to have happened only recently.
The dominant idea in his philosophy is that the present is the key to the
past.” This principle has been impressed on all later geologists by Sir
Charles Lyell, and is the chief cornerstone of modern geology.
The principle of uniformitarianism has underlain geologic interpretation
since the days of Hutton, Playfair, and Lyell. However, it is often applied
too rigidly in interpretations based upon the present conditions, because in
the past there were long times when the topographic features of the earth
were very different from those of to-day. Throughout the Paleozoic, and,
less markedly, the Mesozoic, the oceans flooded the lands widely (at times
over 60 per cent of the total area), highlands were inconspicuous, sediments
far scarcer, and climates warm and equable throughout the world. Highland
conditions, and especially the broadly emergent continents of the present,
too highly,” as it is at the basis of all modern geology.
One of Hutton’s fundamental doctrines is that the earth is internally hot
and that in the past large masses of molten material, the granites, have been
intruded into the crust. It was these igneous views that led to his followers
being called the Plutonists. Another of his great doctrines was that “the
ruins of an earlier world lie beneath the secondary strata,” and that they are
separated by what is now known as unconformity. He clearly recognized a
lost interval in the broken relation of the structures, and that the ruins, the
detrital materials, of one world after another are superposed in the structure
of the earth.
Hutton also held that the deformation of once horizontally deposited
strata was probably brought about at different periods by great convulsions
that shook the very foundations of the earth. After a convulsion, there was a
long time of erosion, represented by the unconformity. Geikie says, “The
whole of the modern doctrine of earth sculpture is to be found in the
Huttonian theory.”
The Lyellian doctrine of metamorphism had its origin in Hutton, for he
showed that invading igneous granite had altered, through its heat and
expanding power, the originally waterlaid sediments, and that the schists of
the Alps had been born of the sea like other stratified rocks.
Hutton is the father of the Uniformitarian principle, for he “started with
the grand conception that the past history of our globe must be explained by
what can be seen to be happening now, or to have happened only recently.
The dominant idea in his philosophy is that the present is the key to the
past.” This principle has been impressed on all later geologists by Sir
Charles Lyell, and is the chief cornerstone of modern geology.
The principle of uniformitarianism has underlain geologic interpretation
since the days of Hutton, Playfair, and Lyell. However, it is often applied
too rigidly in interpretations based upon the present conditions, because in
the past there were long times when the topographic features of the earth
were very different from those of to-day. Throughout the Paleozoic, and,
less markedly, the Mesozoic, the oceans flooded the lands widely (at times
over 60 per cent of the total area), highlands were inconspicuous, sediments
far scarcer, and climates warm and equable throughout the world. Highland
conditions, and especially the broadly emergent continents of the present,
Page 71
were only periodically present in the Paleozoic and then for comparatively
short intervals between the periods. Therefore rates of denudation, solution,
sedimentation, and evolution have varied greatly throughout the geological
ages. These differences, however, relate to degrees of operation, and not to
kinds of processes; but the differences in degree of operation react mightily
on our views as to the age of the earth.
Geologic time had, for Hutton, no “vestige of a beginning, no prospect of
an end.” In other words, geologic time is infinite. He did not, however,
discover a method by which the chronology of the earth could be
determined.
First Important Text-books.—In 1822 appeared the ablest text-book so
far published, and the pattern for most of the later ones, Outlines of the
Geology of England and Wales, by W. D. Conybeare (1787–1857) and W.
Phillips (1775–1828). “In this excellent volume all that was then known
regarding the rocks of the country, from the youngest formations down to
the Old Red Sandstone, was summarized in so clear and methodical a
manner as to give a powerful impulse to the cultivation of geology in
England” (Geikie). This book is reviewed at great length by Edward
Hitchcock in the Journal (7, 203, 1824).
To indicate how far historical geology had progressed up to 1822 in
England, a digest of the geological column as presented in this text-book is
given in the following table, along with other information.
A text-book writer of yet greater influence was Charles Lyell (1797–
1875), whose Principles of Geology appeared in three volumes between
1830 and 1833. This and his other books were kept up to date through many
editions, and his Elements of Geology is, as Geikie says, “the hand book of
every English geologist” working with the fossiliferous formations.
short intervals between the periods. Therefore rates of denudation, solution,
sedimentation, and evolution have varied greatly throughout the geological
ages. These differences, however, relate to degrees of operation, and not to
kinds of processes; but the differences in degree of operation react mightily
on our views as to the age of the earth.
Geologic time had, for Hutton, no “vestige of a beginning, no prospect of
an end.” In other words, geologic time is infinite. He did not, however,
discover a method by which the chronology of the earth could be
determined.
First Important Text-books.—In 1822 appeared the ablest text-book so
far published, and the pattern for most of the later ones, Outlines of the
Geology of England and Wales, by W. D. Conybeare (1787–1857) and W.
Phillips (1775–1828). “In this excellent volume all that was then known
regarding the rocks of the country, from the youngest formations down to
the Old Red Sandstone, was summarized in so clear and methodical a
manner as to give a powerful impulse to the cultivation of geology in
England” (Geikie). This book is reviewed at great length by Edward
Hitchcock in the Journal (7, 203, 1824).
To indicate how far historical geology had progressed up to 1822 in
England, a digest of the geological column as presented in this text-book is
given in the following table, along with other information.
A text-book writer of yet greater influence was Charles Lyell (1797–
1875), whose Principles of Geology appeared in three volumes between
1830 and 1833. This and his other books were kept up to date through many
editions, and his Elements of Geology is, as Geikie says, “the hand book of
every English geologist” working with the fossiliferous formations.
Page 72
The Rise of Geology in North America.
The Generating Centers.—In America, geology had its rise
independently in three places: in the two scientific societies of Boston and
Philadelphia, and dominantly in Benjamin Silliman of Yale College. Stated
in another way, we may say that geology in America had its origin in the
following pioneers and founders: first, in William Maclure at Philadelphia,
and next in Benjamin Silliman at New Haven. Through the influence of the
latter, Amos Eaton, the botanist, became a geologist and taught geology at
Williams College and later at the Rensselaer School in Troy, New York.
Through the same influence Rev. Edward Hitchcock also became a
geologist and taught the subject after 1825 at Amherst College.
Silliman was the first to take up actively the teaching of mineralogy and
geology based on collections of specimens. He spread the knowledge in
popular lectures throughout the Eastern States, graduated many a student in
the sciences, making of some of them professional teachers and geologists,
provided all with a journal wherein they could publish their research,
organized the first geological society and through his students the first
official geological surveys, and by kind words and acts stimulated, fostered,
and held together American scientific men for fifty years. Of him it has
been truly said that he was “the guardian of American science from its
childhood.”
The American Academy in Boston.—The second oldest scientific society,
but the first one to publish on geological subjects, was the American
Academy of Arts and Sciences of Boston, instituted and publishing since
1780. Up to the time of the founding of this Journal, there had appeared in
the publications of the American Academy about a dozen papers of a
geologic character, none of which need to be mentioned here excepting one
by S. L. and J. F. Dana, entitled “Outlines of the Mineralogy and Geology
of Boston,” published in 1818. This is an early and important step in the
elucidation of one of the most intricate geologic areas, and is further
noteworthy for its geologic map, the third one to appear, the older ones
being by Maclure and Hitchcock (Merrill).
The Generating Centers.—In America, geology had its rise
independently in three places: in the two scientific societies of Boston and
Philadelphia, and dominantly in Benjamin Silliman of Yale College. Stated
in another way, we may say that geology in America had its origin in the
following pioneers and founders: first, in William Maclure at Philadelphia,
and next in Benjamin Silliman at New Haven. Through the influence of the
latter, Amos Eaton, the botanist, became a geologist and taught geology at
Williams College and later at the Rensselaer School in Troy, New York.
Through the same influence Rev. Edward Hitchcock also became a
geologist and taught the subject after 1825 at Amherst College.
Silliman was the first to take up actively the teaching of mineralogy and
geology based on collections of specimens. He spread the knowledge in
popular lectures throughout the Eastern States, graduated many a student in
the sciences, making of some of them professional teachers and geologists,
provided all with a journal wherein they could publish their research,
organized the first geological society and through his students the first
official geological surveys, and by kind words and acts stimulated, fostered,
and held together American scientific men for fifty years. Of him it has
been truly said that he was “the guardian of American science from its
childhood.”
The American Academy in Boston.—The second oldest scientific society,
but the first one to publish on geological subjects, was the American
Academy of Arts and Sciences of Boston, instituted and publishing since
1780. Up to the time of the founding of this Journal, there had appeared in
the publications of the American Academy about a dozen papers of a
geologic character, none of which need to be mentioned here excepting one
by S. L. and J. F. Dana, entitled “Outlines of the Mineralogy and Geology
of Boston,” published in 1818. This is an early and important step in the
elucidation of one of the most intricate geologic areas, and is further
noteworthy for its geologic map, the third one to appear, the older ones
being by Maclure and Hitchcock (Merrill).
Page 73
The Geological Column in 1822
Present American classification Conybeare and Phillips 1822 C. & P. orders Wernerian orders Other writers
Psychozoic or Recent Alluvial
Pleistocene Diluvial
Pliocene Upper Marine formation (Crag, Bagshot sand, and Isle of
Neogene
Miocene Wight) Superior Order Newest Floetz Class Tertiary Class
Cenozoic
Fresh-water formations
Oligocene London Clay
Paleogene
Eocene Plastic Clay
Cretaceous Chalk
Comanchian 1887 Beds between Chalk and Oolite Series (Chalk Marle,
Green Sand, Weald Clay, Iron Sand)
Upper Oolitic division (Purbeck beds, Portland Oolite,
Kimmeridge Clay)
Mesozoic Middle Oolitic division (Coral Rag, Oxford Clay)
Jurassic 1829 Supermedial Order
Lower Oolitic division (Cornbrash Stonesfield Slate,
Forest Marble, Great Oolite, Fullers’ Earth, Inferior
Oolite, Sand and Marlestone)
Lias
Triassic 1834 New Red Sandstone
Permian 1841 Magnesian Limestone
Coal Measures
Pennsylvanian 1891 Medial or Primitive Transition Primitive Intermediate
Mississippian 1869 Millstone Grit and Shale Carboniferous and Floetz Classes and Secondary classes
Old Red Sandstone Order
Paleozoic
Devonian 1839
Silurian 1835
Ordovician 1879
(=Lower Silurian 1835)
Cambrian 1833
Keweenawan
Unresolved Submedial and Inferior Orders
Animikian Huronian
Proterozoic
Huronian 1852
Sudburian
Keewatin Laurentian
Archeozoic
Coutchiching 1853
Early Geology in Philadelphia.—The oldest scientific society is the
American Philosophical Society of Philadelphia, started by the many-sided
Benjamin Franklin in 1769, and which has published since 1771. Up to the
time of the founding of the Journal in 1818, there had appeared in the
publications of this society thirteen papers of a geologic nature, nearly all
small building stones in the rising geologic story of North America. The
only fundamental ones were Maclure’s Observations of 1809 and 1817.
Later, in this same city, there was organized another scientific society that
came to be for a long time the most active one in America. This was the
Academy of Natural Sciences, started in 1812 with seven members, but it
was not until 1817 and the election of William Maclure as its first president
that the work of the Academy was of a far-reaching character. Here was
built up not only a society for the advancement of the natural sciences and
publications for the dissemination of such knowledge, but, what is equally
important, the first large library and general museum.
William Maclure (1763–1840), correctly named by Silliman the “father
of American geology,” was born and educated in Scotland, and died near
Mexico City. A merchant of London until 1796, when he had already
amassed “a considerable fortune,” he made a first short visit to New York
Present American classification Conybeare and Phillips 1822 C. & P. orders Wernerian orders Other writers
Psychozoic or Recent Alluvial
Pleistocene Diluvial
Pliocene Upper Marine formation (Crag, Bagshot sand, and Isle of
Neogene
Miocene Wight) Superior Order Newest Floetz Class Tertiary Class
Cenozoic
Fresh-water formations
Oligocene London Clay
Paleogene
Eocene Plastic Clay
Cretaceous Chalk
Comanchian 1887 Beds between Chalk and Oolite Series (Chalk Marle,
Green Sand, Weald Clay, Iron Sand)
Upper Oolitic division (Purbeck beds, Portland Oolite,
Kimmeridge Clay)
Mesozoic Middle Oolitic division (Coral Rag, Oxford Clay)
Jurassic 1829 Supermedial Order
Lower Oolitic division (Cornbrash Stonesfield Slate,
Forest Marble, Great Oolite, Fullers’ Earth, Inferior
Oolite, Sand and Marlestone)
Lias
Triassic 1834 New Red Sandstone
Permian 1841 Magnesian Limestone
Coal Measures
Pennsylvanian 1891 Medial or Primitive Transition Primitive Intermediate
Mississippian 1869 Millstone Grit and Shale Carboniferous and Floetz Classes and Secondary classes
Old Red Sandstone Order
Paleozoic
Devonian 1839
Silurian 1835
Ordovician 1879
(=Lower Silurian 1835)
Cambrian 1833
Keweenawan
Unresolved Submedial and Inferior Orders
Animikian Huronian
Proterozoic
Huronian 1852
Sudburian
Keewatin Laurentian
Archeozoic
Coutchiching 1853
Early Geology in Philadelphia.—The oldest scientific society is the
American Philosophical Society of Philadelphia, started by the many-sided
Benjamin Franklin in 1769, and which has published since 1771. Up to the
time of the founding of the Journal in 1818, there had appeared in the
publications of this society thirteen papers of a geologic nature, nearly all
small building stones in the rising geologic story of North America. The
only fundamental ones were Maclure’s Observations of 1809 and 1817.
Later, in this same city, there was organized another scientific society that
came to be for a long time the most active one in America. This was the
Academy of Natural Sciences, started in 1812 with seven members, but it
was not until 1817 and the election of William Maclure as its first president
that the work of the Academy was of a far-reaching character. Here was
built up not only a society for the advancement of the natural sciences and
publications for the dissemination of such knowledge, but, what is equally
important, the first large library and general museum.
William Maclure (1763–1840), correctly named by Silliman the “father
of American geology,” was born and educated in Scotland, and died near
Mexico City. A merchant of London until 1796, when he had already
amassed “a considerable fortune,” he made a first short visit to New York
Page 74
City in 1782. In 1796 he again came to America, this time to become a
citizen of this country and a liberal patron of science.
About 1803, single-handed and unsustained by government patronage,
Maclure interested himself most zealously and efficiently in American
geology. In 1809 he published his Observations on the Geology of the
United States, Explanatory of a Geological Map. This work he revised “on a
yet more extended scale,” issuing it in 1817 with 130 pages of text,
accompanied by a large colored geological map.
Silliman, the Pioneer Promoter of Geology.—In 1806 when Benjamin
Silliman (1779–1864) began actively to teach chemistry and mineralogy, all
the sciences in America were in a very backward state, and the earth
sciences were not recognized as such in the curricula of any of our colleges.
Silliman gave his first lecture in chemistry on April 4, 1804. In the summer
of that year, Yale College asked him to go to England to purchase material
for the College, and great possibilities for broadening his knowledge now
loomed before him. As Silliman himself (43, 225, 1842) has told the
interesting story of his sojourn in England and Scotland, it is worth while to
restate a part of it here.
“Passing over to England in the spring of 1805, and fixing my residence for six months in London,
I found there no school, public or private, for geological instruction, and no association for the
cultivation of the science, which was not even named in the English universities.” In geology
“Edinburgh was then far in advance of London.... Prof. Jameson having recently returned from the
school of Werner, fully instructed in the doctrines of his illustrious teacher, was ardently engaged to
maintain them, and his eloquent and acute friend, the late Dr. John Murray, was a powerful auxiliary
in the same cause; both of these philosophers strenuously maintaining the ascendancy of the aqueous
over the igneous agencies, in the geological phenomena of our planet.
On the other hand, the disciples and friends of Dr. Hutton were not less active. He died in 1797,
and his mantle fell upon Sir James Hall, who, with Prof. Playfair and Prof. Thomas Hope, maintained
with signal ability, the igneous theory of Hutton. It did not become one who was still a youth and a
novice, to enter the arena of the geological tournament where such powerful champions waged war;
but it was very interesting to view the combat, well sustained as it was on both sides, and protracted,
without a decisive issue, into a drawn battle....
The conflicts of the rival schools of Edinburgh—the Neptunists and the Vulcanists, the Wernerians
and the Huttonians, were sustained with great zeal, energy, talent, and science; they were indeed
marked too decidedly by a partisan spirit, but this very spirit excited untiring activity in discovering,
arranging, and criticising the facts of geology. It was a transition period between the epoch of
geological hypotheses and dreams, which had passed by, and the era of strict philosophical induction,
in which the geologists of the present day are trained....
I was a diligent and delighted listener to the discussions of both schools. Still the igneous
philosophers appeared to me to assume more than had been proved regarding internal heat. In
citizen of this country and a liberal patron of science.
About 1803, single-handed and unsustained by government patronage,
Maclure interested himself most zealously and efficiently in American
geology. In 1809 he published his Observations on the Geology of the
United States, Explanatory of a Geological Map. This work he revised “on a
yet more extended scale,” issuing it in 1817 with 130 pages of text,
accompanied by a large colored geological map.
Silliman, the Pioneer Promoter of Geology.—In 1806 when Benjamin
Silliman (1779–1864) began actively to teach chemistry and mineralogy, all
the sciences in America were in a very backward state, and the earth
sciences were not recognized as such in the curricula of any of our colleges.
Silliman gave his first lecture in chemistry on April 4, 1804. In the summer
of that year, Yale College asked him to go to England to purchase material
for the College, and great possibilities for broadening his knowledge now
loomed before him. As Silliman himself (43, 225, 1842) has told the
interesting story of his sojourn in England and Scotland, it is worth while to
restate a part of it here.
“Passing over to England in the spring of 1805, and fixing my residence for six months in London,
I found there no school, public or private, for geological instruction, and no association for the
cultivation of the science, which was not even named in the English universities.” In geology
“Edinburgh was then far in advance of London.... Prof. Jameson having recently returned from the
school of Werner, fully instructed in the doctrines of his illustrious teacher, was ardently engaged to
maintain them, and his eloquent and acute friend, the late Dr. John Murray, was a powerful auxiliary
in the same cause; both of these philosophers strenuously maintaining the ascendancy of the aqueous
over the igneous agencies, in the geological phenomena of our planet.
On the other hand, the disciples and friends of Dr. Hutton were not less active. He died in 1797,
and his mantle fell upon Sir James Hall, who, with Prof. Playfair and Prof. Thomas Hope, maintained
with signal ability, the igneous theory of Hutton. It did not become one who was still a youth and a
novice, to enter the arena of the geological tournament where such powerful champions waged war;
but it was very interesting to view the combat, well sustained as it was on both sides, and protracted,
without a decisive issue, into a drawn battle....
The conflicts of the rival schools of Edinburgh—the Neptunists and the Vulcanists, the Wernerians
and the Huttonians, were sustained with great zeal, energy, talent, and science; they were indeed
marked too decidedly by a partisan spirit, but this very spirit excited untiring activity in discovering,
arranging, and criticising the facts of geology. It was a transition period between the epoch of
geological hypotheses and dreams, which had passed by, and the era of strict philosophical induction,
in which the geologists of the present day are trained....
I was a diligent and delighted listener to the discussions of both schools. Still the igneous
philosophers appeared to me to assume more than had been proved regarding internal heat. In
Page 75
imagination we were plunged into a fiery Phlegethon, and I was glad to find relief in the cold bath of
the Wernerian ocean, where my predilections inclined me to linger.”
Silliman’s Students and Their Publications.—Silliman’s first student to
take up geology as a profession was Denison Olmstead (1791–1859),
educator, chemist, and geologist, who was graduated from Yale in 1813.
Four years later he was under special preparation with Silliman in
mineralogy and geology, and in that year was appointed professor of
chemistry in the University of North Carolina. In 1824–1825 Olmstead
issued a Report on the Geology of North Carolina, which is the first official
geological report issued by any state in America, “a conspicuous and
solitary instance,” according to Hitchcock’s review of it (14, 230, 1828), “in
which any of our state governments have undertaken thoroughly to develop
their mineral resources.”
Amos Eaton (1776–1842), lawyer, botanist, surveyor, and one of the
founders of American geology, was a graduate of Williams College in the
class of 1799. He studied with Silliman in 1815, attending his lectures on
chemistry, geology, and mineralogy. He also enjoyed access to the libraries
of Silliman and of the botanist, Levi Ives, in which works on botany and
materia medica were prominent, and was a diligent student of the College
cabinet of minerals. He settled as a lawyer and land agent in Catskill, New
York, and here in 1810 he gave a popular course of lectures on botany,
believed to have been the first attempted in the United States.
In 1818 appeared Eaton’s first noteworthy geological publication, the
Index to the Geology of the Northern States, a text-book for the classes in
geology at Williamstown. The controlling principle of this book was
Wernerism, a false doctrine from which Eaton was never able to free
himself. This book was “written over anew” and published in 1820.
While at Albany in 1818, Governor De Witt Clinton asked Eaton to
deliver a course of lectures on chemistry and geology before the members
of the legislature of New York. It is believed that Eaton is the only
American having this distinction, and because of it he became acquainted
with many leading men of the state, interesting them in geology and its
application to agriculture by means of surveys. In this way was sown the
idea which eventually was to fructify in that great official work: The
the Wernerian ocean, where my predilections inclined me to linger.”
Silliman’s Students and Their Publications.—Silliman’s first student to
take up geology as a profession was Denison Olmstead (1791–1859),
educator, chemist, and geologist, who was graduated from Yale in 1813.
Four years later he was under special preparation with Silliman in
mineralogy and geology, and in that year was appointed professor of
chemistry in the University of North Carolina. In 1824–1825 Olmstead
issued a Report on the Geology of North Carolina, which is the first official
geological report issued by any state in America, “a conspicuous and
solitary instance,” according to Hitchcock’s review of it (14, 230, 1828), “in
which any of our state governments have undertaken thoroughly to develop
their mineral resources.”
Amos Eaton (1776–1842), lawyer, botanist, surveyor, and one of the
founders of American geology, was a graduate of Williams College in the
class of 1799. He studied with Silliman in 1815, attending his lectures on
chemistry, geology, and mineralogy. He also enjoyed access to the libraries
of Silliman and of the botanist, Levi Ives, in which works on botany and
materia medica were prominent, and was a diligent student of the College
cabinet of minerals. He settled as a lawyer and land agent in Catskill, New
York, and here in 1810 he gave a popular course of lectures on botany,
believed to have been the first attempted in the United States.
In 1818 appeared Eaton’s first noteworthy geological publication, the
Index to the Geology of the Northern States, a text-book for the classes in
geology at Williamstown. The controlling principle of this book was
Wernerism, a false doctrine from which Eaton was never able to free
himself. This book was “written over anew” and published in 1820.
While at Albany in 1818, Governor De Witt Clinton asked Eaton to
deliver a course of lectures on chemistry and geology before the members
of the legislature of New York. It is believed that Eaton is the only
American having this distinction, and because of it he became acquainted
with many leading men of the state, interesting them in geology and its
application to agriculture by means of surveys. In this way was sown the
idea which eventually was to fructify in that great official work: The
Page 76
Natural History of New York. (See 43, 215, 1842; and Youmans’ sketch of
Eaton’s life, Pop. Sci. Monthly, Nov. 1890.)
Edward Hitchcock (1793–1864), reverend, state geologist, college
president, and another of the founders of American geology, was largely
self-taught. Previous to 1825, when he entered the theological department
of Yale College, he had met Amos Eaton, who interested him in botany and
mineralogy, and between 1815 and 1819 he had made lists of the plants and
minerals found about his native town, Deerfield, Massachusetts. Therefore,
while studying theology at Yale it was natural for him also to take up
mineralogy and geology with Silliman, whose acquaintance he had made at
least as early as 1818.
Hitchcock, who was destined to be one of the most prominent figures of
his time, was appointed in 1825 to the chair of chemistry and natural history
at Amherst College. His first geologic paper, one of five pages, appeared in
1815. Three years later appeared his more important paper on the Geology
and Mineralogy of a Section of Massachusetts, New Hampshire, and
Vermont (1, 105, 436, 1818). This is also noteworthy for its geological map,
the next one to be published after those of Maclure of 1809 and 1817. In
1823 came a still greater work, A Sketch of the Geology, Mineralogy, and
Scenery of the Regions contiguous to the River Connecticut (6, 1, 200,
1823; 7, 1, 1824). Here the map above referred to was greatly improved,
and the survey was one of the most important of the older publications.
Youmans in his account of Hitchcock (Pop. Sci. Monthly, Sept. 1895)
says:
“The State of Massachusetts commissioned him to make a geological survey of her territory in
1830. Three years were spent in the explorations, and the work was of such a high character that
other States were induced to follow the example of Massachusetts.... The State of New York sought
his advice in the organization of a survey, and followed his suggestions, particularly in the division of
the territory into four parts, and appointed him as the geologist of the first district. He entered upon
the work, but after a few days of labor he found that he must necessarily be separated from his
family, much to his disinclination. He also conceived the idea of urging a more thorough survey of
his own State; hence he resigned his commission and returned home. The effort for a resurvey of
Massachusetts was successful, and he was recommissioned to do the work. The results appeared in
1841 and 1844.”
Oliver P. Hubbard was assistant to Silliman in 1831–1836, and then up to
1866 taught chemistry, mineralogy, and geology at Dartmouth College.
Eaton’s life, Pop. Sci. Monthly, Nov. 1890.)
Edward Hitchcock (1793–1864), reverend, state geologist, college
president, and another of the founders of American geology, was largely
self-taught. Previous to 1825, when he entered the theological department
of Yale College, he had met Amos Eaton, who interested him in botany and
mineralogy, and between 1815 and 1819 he had made lists of the plants and
minerals found about his native town, Deerfield, Massachusetts. Therefore,
while studying theology at Yale it was natural for him also to take up
mineralogy and geology with Silliman, whose acquaintance he had made at
least as early as 1818.
Hitchcock, who was destined to be one of the most prominent figures of
his time, was appointed in 1825 to the chair of chemistry and natural history
at Amherst College. His first geologic paper, one of five pages, appeared in
1815. Three years later appeared his more important paper on the Geology
and Mineralogy of a Section of Massachusetts, New Hampshire, and
Vermont (1, 105, 436, 1818). This is also noteworthy for its geological map,
the next one to be published after those of Maclure of 1809 and 1817. In
1823 came a still greater work, A Sketch of the Geology, Mineralogy, and
Scenery of the Regions contiguous to the River Connecticut (6, 1, 200,
1823; 7, 1, 1824). Here the map above referred to was greatly improved,
and the survey was one of the most important of the older publications.
Youmans in his account of Hitchcock (Pop. Sci. Monthly, Sept. 1895)
says:
“The State of Massachusetts commissioned him to make a geological survey of her territory in
1830. Three years were spent in the explorations, and the work was of such a high character that
other States were induced to follow the example of Massachusetts.... The State of New York sought
his advice in the organization of a survey, and followed his suggestions, particularly in the division of
the territory into four parts, and appointed him as the geologist of the first district. He entered upon
the work, but after a few days of labor he found that he must necessarily be separated from his
family, much to his disinclination. He also conceived the idea of urging a more thorough survey of
his own State; hence he resigned his commission and returned home. The effort for a resurvey of
Massachusetts was successful, and he was recommissioned to do the work. The results appeared in
1841 and 1844.”
Oliver P. Hubbard was assistant to Silliman in 1831–1836, and then up to
1866 taught chemistry, mineralogy, and geology at Dartmouth College.
Page 77
James G. Percival was graduated at Yale in 1815, and in 1835 he and C. U.
Shepard of Amherst College were appointed state geologists of
Connecticut. Their report was issued in 1842.
James Dwight Dana (1813–1895) was undoubtedly the ablest of all of
Silliman’s students. Graduated at Yale in 1833, he spent fifteen months in
the United States Navy as instructor in mathematics, cruising off France,
Italy, Greece, and Turkey. In 1836 he was assistant to Silliman, and in 1837,
at the age of twenty-four years, he published his widely used System of
Mineralogy. Two years later Dana joined the Wilkes Exploring Expedition
as mineralogist, returning to America in 1842; his geological results of this
expedition were published in 1849. In 1863, during the Rebellion, he
published his Manual of Geology, and through four editions it remained for
forty years the standard text-book for American geologists.
First American Geological Society.—The founding in 1807 of the
Geological Society of London, the parent of geological societies,
undoubtedly had its stimulating effect on Silliman, and with his marked
organizing ability he began to think of forming an American society of the
same kind. This he brought about the year following the appearance of the
Journal, that is, in 1819. The American Geological Society, begun in 1819
(1, 442, 1819), was terminated in 1830 (17, 202, 1830). The first meeting
(September 6, 1819) and all the subsequent ones were held in the cabinet of
Yale College. The brief records of the doings of this society are printed in
volumes 1, 10, 15, and 18 of the Journal. Silliman was the attraction at the
meetings, surrounded by his mineral cabinet, and he gave “the true
scientific dress to all the naked mineralogical subjects” discussed.
Shepard of Amherst College were appointed state geologists of
Connecticut. Their report was issued in 1842.
James Dwight Dana (1813–1895) was undoubtedly the ablest of all of
Silliman’s students. Graduated at Yale in 1833, he spent fifteen months in
the United States Navy as instructor in mathematics, cruising off France,
Italy, Greece, and Turkey. In 1836 he was assistant to Silliman, and in 1837,
at the age of twenty-four years, he published his widely used System of
Mineralogy. Two years later Dana joined the Wilkes Exploring Expedition
as mineralogist, returning to America in 1842; his geological results of this
expedition were published in 1849. In 1863, during the Rebellion, he
published his Manual of Geology, and through four editions it remained for
forty years the standard text-book for American geologists.
First American Geological Society.—The founding in 1807 of the
Geological Society of London, the parent of geological societies,
undoubtedly had its stimulating effect on Silliman, and with his marked
organizing ability he began to think of forming an American society of the
same kind. This he brought about the year following the appearance of the
Journal, that is, in 1819. The American Geological Society, begun in 1819
(1, 442, 1819), was terminated in 1830 (17, 202, 1830). The first meeting
(September 6, 1819) and all the subsequent ones were held in the cabinet of
Yale College. The brief records of the doings of this society are printed in
volumes 1, 10, 15, and 18 of the Journal. Silliman was the attraction at the
meetings, surrounded by his mineral cabinet, and he gave “the true
scientific dress to all the naked mineralogical subjects” discussed.
Page 78
Wernerian Geology in North America.
The Father of American Geology.—Historical Geology begins in
America with William Maclure’s Observations on the Geology of the
United States, issued in 1809. This was the first important original work on
North American geology, and its colored geological map was the first one
of the area east of the Mississippi River. The classification was essentially
the Wernerian system. All of the strata of the Coastal Plain, now known to
range from the Lower Cretaceous to Recent, were referred to the Alluvial.
To the west, over the area of the Piedmont, were his Primitive rocks, while
the older Paleozoic formations of the Appalachian ranges were referred to
the Transition. West of the folded area, all was Floetz or Secondary, or what
we now know as Paleozoic sedimentaries. The Triassic of the Piedmont area
and that of Connecticut he called the Old Red Sandstone, and the coal
formations of the interior region he said rested upon the Secondary. The
second edition of the work in 1817 was much improved, along with the
map, which was also printed on a more correct geographic base. (For
greater detail, see Merrill, Contributions to the History of American
Geology, 1906.)
Even though Maclure’s geologic maps are much generalized, and the
scheme of classification adopted a very broad one, they are in the main
correct, even if they do emphasize unduly the rather simple geologic
structure of North America. This fact is patent all through Maclure’s
description. Cleaveland also refers to it in his treatise of 1816, and Silliman
in the opening volume of the Journal (1, 7, 1818) says: “The outlines of
American geology appear to be particularly grand, simple, and instructive.”
Then, all the kinds of rocks were comprehended under four classes,
Primitive, Transition, Alluvial, and Volcanic. It is also interesting to note
here that in 1822 Maclure had lost faith in the aqueous origin of the igneous
rocks and writes of the Wernerian system as “fast going out of fashion” (5,
197, 1822), while Hitchcock said about the same thing in 1825 (9, 146).
The Work of Eaton.—Amos Eaton, after traveling 10,000 miles and
completing his Erie Canal Report in 1824, “reviewed the whole line several
times,” and published in 1828 in the Journal (14, 145) a paper on
Geological Nomenclature, Classes of Rocks, etc. The broader classification
The Father of American Geology.—Historical Geology begins in
America with William Maclure’s Observations on the Geology of the
United States, issued in 1809. This was the first important original work on
North American geology, and its colored geological map was the first one
of the area east of the Mississippi River. The classification was essentially
the Wernerian system. All of the strata of the Coastal Plain, now known to
range from the Lower Cretaceous to Recent, were referred to the Alluvial.
To the west, over the area of the Piedmont, were his Primitive rocks, while
the older Paleozoic formations of the Appalachian ranges were referred to
the Transition. West of the folded area, all was Floetz or Secondary, or what
we now know as Paleozoic sedimentaries. The Triassic of the Piedmont area
and that of Connecticut he called the Old Red Sandstone, and the coal
formations of the interior region he said rested upon the Secondary. The
second edition of the work in 1817 was much improved, along with the
map, which was also printed on a more correct geographic base. (For
greater detail, see Merrill, Contributions to the History of American
Geology, 1906.)
Even though Maclure’s geologic maps are much generalized, and the
scheme of classification adopted a very broad one, they are in the main
correct, even if they do emphasize unduly the rather simple geologic
structure of North America. This fact is patent all through Maclure’s
description. Cleaveland also refers to it in his treatise of 1816, and Silliman
in the opening volume of the Journal (1, 7, 1818) says: “The outlines of
American geology appear to be particularly grand, simple, and instructive.”
Then, all the kinds of rocks were comprehended under four classes,
Primitive, Transition, Alluvial, and Volcanic. It is also interesting to note
here that in 1822 Maclure had lost faith in the aqueous origin of the igneous
rocks and writes of the Wernerian system as “fast going out of fashion” (5,
197, 1822), while Hitchcock said about the same thing in 1825 (9, 146).
The Work of Eaton.—Amos Eaton, after traveling 10,000 miles and
completing his Erie Canal Report in 1824, “reviewed the whole line several
times,” and published in 1828 in the Journal (14, 145) a paper on
Geological Nomenclature, Classes of Rocks, etc. The broader classification
Page 79
is the Wernerian one of Primitive, Transition, and Secondary classes. Under
the first two he has fossiliferous early Paleozoic formations, but does not
know it, because he pays no attention anywhere to the detail of the
entombed fossils, and all of his Secondary is what we now call Paleozoic.
The correlations of the latter are faulty throughout.
Then came his paper of 1830, Geological Prodromus (17, 63), in which
he says: “I intend to demonstrate ... that all geological strata are arranged in
five analogous series; and that each series consists of three formations; viz.,
the Carboniferous [meaning mud-stones], Quartzose, and Calcareous.” We
seem to see here expressed for the first time the idea of “cycles of
sedimentation,” but Eaton does not emphasize this idea, and the localities
given for each “formation” of “analogous series” demonstrate beyond a
doubt that he did not have a sedimentary sequence. The whole is simply a
jumble of unrelated formations that happen to agree more or less in their
physical characters.
“I intend to demonstrate,” he says further, “that the detritus of New
Jersey, embracing the marle, which contains those remarkable fossil relics,
is antediluvial, or the genuine Tertiary formation.” This correlation had
been clearly shown by Finch in 1824 (7, 31) and yet both are in error in that
they do not distinguish the included Cretaceous marls and greensands as
something apart from the Tertiary.
One gets impatient with the later writings of Eaton, because he does not
become liberalized with the progressive ideas in stratigraphic geology
developing first in Europe and then in America, especially among the
geologists of Philadelphia. Therefore it is not profitable to follow his work
further.
Early American Text-books of Geology.—The first American text-book of
geology bears the date of Boston 1816 and is entitled An Elementary
Treatise on Mineralogy and Geology, its author being Parker Cleaveland of
Bowdoin College. The second edition appeared in 1822. It also had a
geologic map of the United States, practically a copy of Maclure’s. To
mineralogy were devoted 585 pages, and to geology 55, of which 37
describe rocks and 5 the geology of the United States. The chronology is
Wernerian. Of “geological systems” there are two, “primitive and secondary
rocks.”
the first two he has fossiliferous early Paleozoic formations, but does not
know it, because he pays no attention anywhere to the detail of the
entombed fossils, and all of his Secondary is what we now call Paleozoic.
The correlations of the latter are faulty throughout.
Then came his paper of 1830, Geological Prodromus (17, 63), in which
he says: “I intend to demonstrate ... that all geological strata are arranged in
five analogous series; and that each series consists of three formations; viz.,
the Carboniferous [meaning mud-stones], Quartzose, and Calcareous.” We
seem to see here expressed for the first time the idea of “cycles of
sedimentation,” but Eaton does not emphasize this idea, and the localities
given for each “formation” of “analogous series” demonstrate beyond a
doubt that he did not have a sedimentary sequence. The whole is simply a
jumble of unrelated formations that happen to agree more or less in their
physical characters.
“I intend to demonstrate,” he says further, “that the detritus of New
Jersey, embracing the marle, which contains those remarkable fossil relics,
is antediluvial, or the genuine Tertiary formation.” This correlation had
been clearly shown by Finch in 1824 (7, 31) and yet both are in error in that
they do not distinguish the included Cretaceous marls and greensands as
something apart from the Tertiary.
One gets impatient with the later writings of Eaton, because he does not
become liberalized with the progressive ideas in stratigraphic geology
developing first in Europe and then in America, especially among the
geologists of Philadelphia. Therefore it is not profitable to follow his work
further.
Early American Text-books of Geology.—The first American text-book of
geology bears the date of Boston 1816 and is entitled An Elementary
Treatise on Mineralogy and Geology, its author being Parker Cleaveland of
Bowdoin College. The second edition appeared in 1822. It also had a
geologic map of the United States, practically a copy of Maclure’s. To
mineralogy were devoted 585 pages, and to geology 55, of which 37
describe rocks and 5 the geology of the United States. The chronology is
Wernerian. Of “geological systems” there are two, “primitive and secondary
rocks.”
Page 80
In 1818 appeared Amos Eaton’s Index to the Geology of the Northern
States, having 54 pages, and in 1820 came the second edition, “wholly
written over anew,” with 286 pages. The theory of the later edition is still
that of Werner, with “improvements of Cuvier and Bakewell,” and yet one
sees now-a-days but little in it of the far better English text-book. Eaton did
very little to advance philosophic geology in America. What is of most
value here are his personal observations in regard to the local geology of
western Massachusetts, Connecticut, southwestern Vermont, and eastern
New York (1, 69, 1819; also Merrill, p. 234).
We come now to the most comprehensive and advanced of the early text-
books used in America. This is the third English edition of Robert
Bakewell’s Introduction to Geology (400 pages, 1829), and the first
American edition “with an Appendix Containing an Outline of his Course
of Lectures on Geology at Yale College, by Benjamin Silliman” (128
pages). Bakewell’s good book is in keeping with the time, and while not so
advanced as Conybeare and Phillips’s Outlines of 1822, yet is far more so
than Silliman’s appendix. The latter is general and not specific as to details;
it is still decidedly Wernerian, though in a modified form. Silliman says he
is “neither Wernerian nor Huttonian,” and yet his summary on pages 120 to
126 shows clearly that he was not only a Wernerian but a pietist as well.
States, having 54 pages, and in 1820 came the second edition, “wholly
written over anew,” with 286 pages. The theory of the later edition is still
that of Werner, with “improvements of Cuvier and Bakewell,” and yet one
sees now-a-days but little in it of the far better English text-book. Eaton did
very little to advance philosophic geology in America. What is of most
value here are his personal observations in regard to the local geology of
western Massachusetts, Connecticut, southwestern Vermont, and eastern
New York (1, 69, 1819; also Merrill, p. 234).
We come now to the most comprehensive and advanced of the early text-
books used in America. This is the third English edition of Robert
Bakewell’s Introduction to Geology (400 pages, 1829), and the first
American edition “with an Appendix Containing an Outline of his Course
of Lectures on Geology at Yale College, by Benjamin Silliman” (128
pages). Bakewell’s good book is in keeping with the time, and while not so
advanced as Conybeare and Phillips’s Outlines of 1822, yet is far more so
than Silliman’s appendix. The latter is general and not specific as to details;
it is still decidedly Wernerian, though in a modified form. Silliman says he
is “neither Wernerian nor Huttonian,” and yet his summary on pages 120 to
126 shows clearly that he was not only a Wernerian but a pietist as well.
Page 81
Unearthing of the Cenozoic and Mesozoic in North America.
The Discerning of the Tertiary.—The New England States, with their
essentially igneous and metamorphic formations, could not furnish the
proper geologic environment for the development of stratigraphers and
paleontologists. So in America we see the rise of such geologists first in
Philadelphia, where they had easy access to the horizontal and highly
fossiliferous strata of the coastal plain. The first one to attract attention was
Thomas Say, after him came John Finch, followed by Lardner Vanuxem,
Isaac Lea, Samuel G. Morton, and T. A. Conrad. These men not only
worked out the succession of the Cenozoic and the upper part of the
Mesozoic, but blazed the way among the Paleozoic strata as well.
Thomas Say (1787–1834), in 1819, was the first American to point out
the chronogenetic value of fossils in his article, Observations on some
Species of Zoophytes, Shells, etc., principally Fossil (1, 381). He correctly
states that the progress of geology “must be in part founded on a knowledge
of the different genera and species of reliquiæ, which the various accessible
strata of the earth present.” Say fully realizes the difficulties in the study of
fossils, because of their fragmental character and changed nature, and that
their correct interpretation requires a knowledge of similar living
organisms.
The application of what Say pointed out came first in John Finch’s
Geological Essay on the Tertiary Formations in America (7, 31, 1824). Even
though the paper is still laboring under the mineral system and does not
discern the presence of Cretaceous strata among his Tertiary formations, yet
Finch also sees that “fossils constitute the medals of the ancient world, by
which to ascertain the various periods.”
Finch now objects to the wide misuse in America of the term alluvial and
holds that it is applied to what is elsewhere known as Tertiary. He says:
“Geology will achieve a triumph in America, when the term alluvial shall be banished from her
Geological Essays, or confined to its legitimate domain, and then her tertiary formations will be seen
to coincide with those of Europe, and the formations of London, Paris, and the Isle of Wight, will
find kindred associations in Virginia, the Carolinas, Georgias, the Floridas, and Louisiana.”
The Discerning of the Tertiary.—The New England States, with their
essentially igneous and metamorphic formations, could not furnish the
proper geologic environment for the development of stratigraphers and
paleontologists. So in America we see the rise of such geologists first in
Philadelphia, where they had easy access to the horizontal and highly
fossiliferous strata of the coastal plain. The first one to attract attention was
Thomas Say, after him came John Finch, followed by Lardner Vanuxem,
Isaac Lea, Samuel G. Morton, and T. A. Conrad. These men not only
worked out the succession of the Cenozoic and the upper part of the
Mesozoic, but blazed the way among the Paleozoic strata as well.
Thomas Say (1787–1834), in 1819, was the first American to point out
the chronogenetic value of fossils in his article, Observations on some
Species of Zoophytes, Shells, etc., principally Fossil (1, 381). He correctly
states that the progress of geology “must be in part founded on a knowledge
of the different genera and species of reliquiæ, which the various accessible
strata of the earth present.” Say fully realizes the difficulties in the study of
fossils, because of their fragmental character and changed nature, and that
their correct interpretation requires a knowledge of similar living
organisms.
The application of what Say pointed out came first in John Finch’s
Geological Essay on the Tertiary Formations in America (7, 31, 1824). Even
though the paper is still laboring under the mineral system and does not
discern the presence of Cretaceous strata among his Tertiary formations, yet
Finch also sees that “fossils constitute the medals of the ancient world, by
which to ascertain the various periods.”
Finch now objects to the wide misuse in America of the term alluvial and
holds that it is applied to what is elsewhere known as Tertiary. He says:
“Geology will achieve a triumph in America, when the term alluvial shall be banished from her
Geological Essays, or confined to its legitimate domain, and then her tertiary formations will be seen
to coincide with those of Europe, and the formations of London, Paris, and the Isle of Wight, will
find kindred associations in Virginia, the Carolinas, Georgias, the Floridas, and Louisiana.”
Page 82
The formations as he has them from the bottom upwards are: (1)
Ferruginous sand, (2) Plastic clay, (3) Calcaire Silicieuse of the Paris Basin,
(4) London Clay, (5) Calcaire Ostrée, (6) Upper marine formation, (7)
Diluvial.
The grandest of these early stratigraphic papers, however, is that by
Lardner Vanuxem (1792–1848), of only three pages, entitled “Remarks on
the Characters and Classification of Certain American Rock Formations”
(16, 254, 1829). Vanuxem, a cautious man and a profound thinker, had been
educated at the Paris School of Mines. James Hall told the writer in a
conversation that while the first New York State Survey was in operation,
all of its members looked to Vanuxem for advice.
In the paper above referred to, Vanuxem points out in a very concise
manner that:
“The alluvial of Mr. Maclure ... contains not only well characterized alluvion, but products of the
tertiary and secondary classes. Littoral shells, similar to those of the English and Paris basins, and
pelagic shells, similar to those of the chalk deposition or latest secondary, abound in it. These two
kinds of shells are not mixed with each other; they occur in different earthy matter, and, in the
southern states particularly, are at different levels. The incoherency or earthiness of the mass, and our
former ignorance of the true position of the shells, have been the sources of our erroneous views.”
The second error of the older geologists, according to Vanuxem, was the
extension of the secondary rocks over “the western country, and the back
and upper parts of New York.” They are now called Paleozoic. Some had
even tried to show the presence of Jurassic here because of the existence of
oölite strata. “It was taken for granted, that all horizontal rocks are
secondary, and as the rocks of these parts of the United States are horizontal
in their position, so they were supposed to be secondary.” He then shows on
the basis of similar Ordovician fossils that the rocks of Trenton Falls, New
York, recur at Frankfort in Kentucky, and at Nashville in Tennessee.
“It is also certain that an uplifting or downfalling force, or both, have
existed, but it is not certain that either or both these forces have acted in a
uniform manner.... Innumerable are the facts, which have fallen under my
observation, which show the fallacy of adopting inclination for the
character of a class,” such as the Transition class of strata. He then goes on
to say that in the interior of our country the so-called secondary rocks are
horizontal and in the mountains to the east the same strata are highly
Ferruginous sand, (2) Plastic clay, (3) Calcaire Silicieuse of the Paris Basin,
(4) London Clay, (5) Calcaire Ostrée, (6) Upper marine formation, (7)
Diluvial.
The grandest of these early stratigraphic papers, however, is that by
Lardner Vanuxem (1792–1848), of only three pages, entitled “Remarks on
the Characters and Classification of Certain American Rock Formations”
(16, 254, 1829). Vanuxem, a cautious man and a profound thinker, had been
educated at the Paris School of Mines. James Hall told the writer in a
conversation that while the first New York State Survey was in operation,
all of its members looked to Vanuxem for advice.
In the paper above referred to, Vanuxem points out in a very concise
manner that:
“The alluvial of Mr. Maclure ... contains not only well characterized alluvion, but products of the
tertiary and secondary classes. Littoral shells, similar to those of the English and Paris basins, and
pelagic shells, similar to those of the chalk deposition or latest secondary, abound in it. These two
kinds of shells are not mixed with each other; they occur in different earthy matter, and, in the
southern states particularly, are at different levels. The incoherency or earthiness of the mass, and our
former ignorance of the true position of the shells, have been the sources of our erroneous views.”
The second error of the older geologists, according to Vanuxem, was the
extension of the secondary rocks over “the western country, and the back
and upper parts of New York.” They are now called Paleozoic. Some had
even tried to show the presence of Jurassic here because of the existence of
oölite strata. “It was taken for granted, that all horizontal rocks are
secondary, and as the rocks of these parts of the United States are horizontal
in their position, so they were supposed to be secondary.” He then shows on
the basis of similar Ordovician fossils that the rocks of Trenton Falls, New
York, recur at Frankfort in Kentucky, and at Nashville in Tennessee.
“It is also certain that an uplifting or downfalling force, or both, have
existed, but it is not certain that either or both these forces have acted in a
uniform manner.... Innumerable are the facts, which have fallen under my
observation, which show the fallacy of adopting inclination for the
character of a class,” such as the Transition class of strata. He then goes on
to say that in the interior of our country the so-called secondary rocks are
horizontal and in the mountains to the east the same strata are highly
Page 83
inclined. “The analogy, or identity of rocks, I determine by their fossils in
the first instance, and their position and mineralogical characters in the
second or last instance.”
It appears that Isaac Lea (1792–1886) in his Contributions to Geology,
1833, was the first to transplant to America Lyell’s terms, Pliocene,
Miocene, and Eocene, proposed the previous year. The celebrated Claiborne
locality was made known to Lea in 1829, and in the work here cited he
describes from it 250 species, of which 200 are new. The horizon is
correlated with the London Clay and with the Calcaire Grossier of France,
both of Eocene time (25, 413, 1834).
Timothy A. Conrad began to write about the American Tertiary in 1830,
and his more important publications were issued at Philadelphia. His papers
in the Journal begin with 1833 and the last one on the Tertiary is in 1846.
The Tertiary faunas and stratigraphy have been modernized by William
H. Dall in his monumental work of 1650 pages and 60 plates entitled
“Contributions to the Tertiary Fauna of Florida” (1885–1903). Here more
than 3160 forms of the Atlantic and Gulf deposits are described, but in
order to understand their relations to the fossil faunas elsewhere and to the
living world, the author studied over 10,000 species. Since then, many other
workers have interested themselves in the Tertiary problems. Much good
work is also being done in the Pacific States where the sequence is being
rapidly developed.
The Discerning of the Eastern Cretaceous.—The Cretaceous sequence
was first determined by that “active and acute geologist,” Samuel G.
Morton (1799–1851), but that these rocks might be present along the
Atlantic border had been surmised as early as 1824 by Edward Hitchcock
(7, 216). Vanuxem, as above pointed out, indicated the presence of the
Cretaceous in 1829. In this same year Morton proved its presence before the
Philadelphia Academy of Natural Sciences.
Between 1830 and 1835 Morton published a series of papers in the
Journal under the title “Synopsis of the Organic Remains of the Ferruginous
Sand Formation of the United States, with Geological Remarks” (17, 274,
et seq.). In these he describes the Cretaceous fossils and demonstrates that
the “Diluvial” and Tertiary strata of the Atlantic border also have a long
sequence of Cretaceous formations. In the opening paper he writes: “I
consider the marl of New Jersey as referable to the great ferruginous sand
the first instance, and their position and mineralogical characters in the
second or last instance.”
It appears that Isaac Lea (1792–1886) in his Contributions to Geology,
1833, was the first to transplant to America Lyell’s terms, Pliocene,
Miocene, and Eocene, proposed the previous year. The celebrated Claiborne
locality was made known to Lea in 1829, and in the work here cited he
describes from it 250 species, of which 200 are new. The horizon is
correlated with the London Clay and with the Calcaire Grossier of France,
both of Eocene time (25, 413, 1834).
Timothy A. Conrad began to write about the American Tertiary in 1830,
and his more important publications were issued at Philadelphia. His papers
in the Journal begin with 1833 and the last one on the Tertiary is in 1846.
The Tertiary faunas and stratigraphy have been modernized by William
H. Dall in his monumental work of 1650 pages and 60 plates entitled
“Contributions to the Tertiary Fauna of Florida” (1885–1903). Here more
than 3160 forms of the Atlantic and Gulf deposits are described, but in
order to understand their relations to the fossil faunas elsewhere and to the
living world, the author studied over 10,000 species. Since then, many other
workers have interested themselves in the Tertiary problems. Much good
work is also being done in the Pacific States where the sequence is being
rapidly developed.
The Discerning of the Eastern Cretaceous.—The Cretaceous sequence
was first determined by that “active and acute geologist,” Samuel G.
Morton (1799–1851), but that these rocks might be present along the
Atlantic border had been surmised as early as 1824 by Edward Hitchcock
(7, 216). Vanuxem, as above pointed out, indicated the presence of the
Cretaceous in 1829. In this same year Morton proved its presence before the
Philadelphia Academy of Natural Sciences.
Between 1830 and 1835 Morton published a series of papers in the
Journal under the title “Synopsis of the Organic Remains of the Ferruginous
Sand Formation of the United States, with Geological Remarks” (17, 274,
et seq.). In these he describes the Cretaceous fossils and demonstrates that
the “Diluvial” and Tertiary strata of the Atlantic border also have a long
sequence of Cretaceous formations. In the opening paper he writes: “I
consider the marl of New Jersey as referable to the great ferruginous sand
Page 84
series, which in Prof. Buckland’s arrangement is designated by the name of
green sand.... On the continent this series is called the ancient chalk ...
lower chalk,” etc. Again, the marls of New Jersey are “geologically
equivalent to those beds which in Europe are interposed between the white
chalk and the Oölites.” This correlation is with the European Lower
Cretaceous, but we now know the marls to be of Upper Cretaceous age.
Although Eaton objected strenuously to Morton’s correlation, we find M.
Dufresnoy of France saying, “Your limestone above green sand reminds me
very much of the Mæstricht beds,” a correlation which stands to this day
(22, 94, 1832). In 1833 Morton announces that the Cretaceous is known all
along the Atlantic and Gulf border, and in the Mississippi valley. “The same
species of fossils are found throughout,” and none of them are known in the
Tertiary. He now arranges the strata of the former “Alluvial” as follows:
Alluvial.
Modern
Diluvial.
Upper Tertiary (Upper Marine).
Tertiary Middle Tertiary (London Clay).
Lower Tertiary (Plastic Clay).
Calcareous Strata
Secondary Cretaceous group, or Ferruginous Sand series (24, 128).
Ferruginous Sand
Western Cretaceous.—In 1841 and 1843 J. N. Nicollet announced the
discovery of Cretaceous in the Rocky Mountain area. Of 20 species of
fossils collected by him, 4 were said to occur on the Atlantic border, and of
the 200 forms of the Atlantic slope only 1 was found in Europe. Here we
see pointed out a specific dissimilarity between the continents, and a
similarity between the American areas of Cretaceous deposits (41, 181; 45,
153).
The Cretaceous of the Rocky Mountains was clearly developed by F. V.
Hayden in 1855–1888 and by F. B. Meek (1857–1876). Other workers in
this field were Charles A. White (1869–1891), and R. P. Whitfield (1877–
1889). Since 1891 T. W. Stanton has been actively interpreting its
stratigraphy and faunas.
Cretaceous and Comanche of Texas.—The broader outlines of the
Cretaceous of Texas had been described by Ferdinand Roemer in 1852 in
his good work, Kreidebildungen von Texas, but it was not until 1887 that
Robert T. Hill showed in the Journal (33, 291) that it included two great
series, the Gulf series, or what we now call Upper Cretaceous, and a new
green sand.... On the continent this series is called the ancient chalk ...
lower chalk,” etc. Again, the marls of New Jersey are “geologically
equivalent to those beds which in Europe are interposed between the white
chalk and the Oölites.” This correlation is with the European Lower
Cretaceous, but we now know the marls to be of Upper Cretaceous age.
Although Eaton objected strenuously to Morton’s correlation, we find M.
Dufresnoy of France saying, “Your limestone above green sand reminds me
very much of the Mæstricht beds,” a correlation which stands to this day
(22, 94, 1832). In 1833 Morton announces that the Cretaceous is known all
along the Atlantic and Gulf border, and in the Mississippi valley. “The same
species of fossils are found throughout,” and none of them are known in the
Tertiary. He now arranges the strata of the former “Alluvial” as follows:
Alluvial.
Modern
Diluvial.
Upper Tertiary (Upper Marine).
Tertiary Middle Tertiary (London Clay).
Lower Tertiary (Plastic Clay).
Calcareous Strata
Secondary Cretaceous group, or Ferruginous Sand series (24, 128).
Ferruginous Sand
Western Cretaceous.—In 1841 and 1843 J. N. Nicollet announced the
discovery of Cretaceous in the Rocky Mountain area. Of 20 species of
fossils collected by him, 4 were said to occur on the Atlantic border, and of
the 200 forms of the Atlantic slope only 1 was found in Europe. Here we
see pointed out a specific dissimilarity between the continents, and a
similarity between the American areas of Cretaceous deposits (41, 181; 45,
153).
The Cretaceous of the Rocky Mountains was clearly developed by F. V.
Hayden in 1855–1888 and by F. B. Meek (1857–1876). Other workers in
this field were Charles A. White (1869–1891), and R. P. Whitfield (1877–
1889). Since 1891 T. W. Stanton has been actively interpreting its
stratigraphy and faunas.
Cretaceous and Comanche of Texas.—The broader outlines of the
Cretaceous of Texas had been described by Ferdinand Roemer in 1852 in
his good work, Kreidebildungen von Texas, but it was not until 1887 that
Robert T. Hill showed in the Journal (33, 291) that it included two great
series, the Gulf series, or what we now call Upper Cretaceous, and a new
Page 85
one, the Comanche series. This was a very important step in the right
direction. Since then the Comanche series has been regarded by some
stratigraphers as of period value, while others call it Lower Cretaceous; the
rest of the Texas Cretaceous is divided by Hill into Middle and Upper
Cretaceous. On the other hand, Lower Cretaceous strata had been proved
even earlier in the state of California, for here in 1869 W. M. Gabb (1839–
1878) and J. D. Whitney (1819–1896) had defined their Shasta group,
which was wholly distinct faunally from the Comanche of Texas and the
southern part of the Great Plains country.
Jurassic and Triassic of the West.—In 1864, the Geological Survey of
California proved the presence of marine Upper Triassic in that State, and
since then it has been shown that not only is all of the Triassic present in
Idaho (where it has been known since 1877), Oregon, Nevada, and
California, but that the Upper Triassic is of very wide distribution
throughout western North America. Jurassic strata, on the other hand, were
not shown to be present in California until 1885, while in the Rocky
Mountain area of the United States there was long known an unresolved
series of “Red Beds” situated between the Carboniferous and Cretaceous.
This gave rise to the “Red Bed problem,” the history of which is given by
C. A. White in the Journal (17, 214, 1879). In 1869, F. V. Hayden
announced the discovery of marine Jurassic fossils in this series, and since
then they have come to be known as the Sundance fauna, extending from
southern Utah and Colorado into Alaska. Above lie the dinosaur-bearing
fresh-water deposits, since 1894 known as the Morrison beds. In 1896, O.
C. Marsh (1831–1899) announced the presence of Jurassic fresh-water
strata along the Atlantic coast (2, 433), but to-day only a small part of them
are regarded as of the age of the Morrison, while the far greater part are
referred to the Comanche or Lower Cretaceous. The red beds below the
Jurassic of the Rocky Mountain area have during the past twenty years been
shown to be in part of Upper Triassic age and of fresh-water origin, while
the greater lower part is connected with the Carboniferous series and is
made up of brackish— and fresh-water deposits of probable Permian time.
Triassic of Atlantic States.—The fresh-water Triassic of the Atlantic
border states was first mentioned by Maclure (1817), who regarded it as the
equivalent of the Old Red Sandstone of Europe. In this he was followed by
Hitchcock in 1823 (6, 39), the latter saying that above it lies “the coal
direction. Since then the Comanche series has been regarded by some
stratigraphers as of period value, while others call it Lower Cretaceous; the
rest of the Texas Cretaceous is divided by Hill into Middle and Upper
Cretaceous. On the other hand, Lower Cretaceous strata had been proved
even earlier in the state of California, for here in 1869 W. M. Gabb (1839–
1878) and J. D. Whitney (1819–1896) had defined their Shasta group,
which was wholly distinct faunally from the Comanche of Texas and the
southern part of the Great Plains country.
Jurassic and Triassic of the West.—In 1864, the Geological Survey of
California proved the presence of marine Upper Triassic in that State, and
since then it has been shown that not only is all of the Triassic present in
Idaho (where it has been known since 1877), Oregon, Nevada, and
California, but that the Upper Triassic is of very wide distribution
throughout western North America. Jurassic strata, on the other hand, were
not shown to be present in California until 1885, while in the Rocky
Mountain area of the United States there was long known an unresolved
series of “Red Beds” situated between the Carboniferous and Cretaceous.
This gave rise to the “Red Bed problem,” the history of which is given by
C. A. White in the Journal (17, 214, 1879). In 1869, F. V. Hayden
announced the discovery of marine Jurassic fossils in this series, and since
then they have come to be known as the Sundance fauna, extending from
southern Utah and Colorado into Alaska. Above lie the dinosaur-bearing
fresh-water deposits, since 1894 known as the Morrison beds. In 1896, O.
C. Marsh (1831–1899) announced the presence of Jurassic fresh-water
strata along the Atlantic coast (2, 433), but to-day only a small part of them
are regarded as of the age of the Morrison, while the far greater part are
referred to the Comanche or Lower Cretaceous. The red beds below the
Jurassic of the Rocky Mountain area have during the past twenty years been
shown to be in part of Upper Triassic age and of fresh-water origin, while
the greater lower part is connected with the Carboniferous series and is
made up of brackish— and fresh-water deposits of probable Permian time.
Triassic of Atlantic States.—The fresh-water Triassic of the Atlantic
border states was first mentioned by Maclure (1817), who regarded it as the
equivalent of the Old Red Sandstone of Europe. In this he was followed by
Hitchcock in 1823 (6, 39), the latter saying that above it lies “the coal
Page 86
formation,” which is true for Europe, but in America the coal strata are
older than these red beds, now known to be of Triassic age.
The first one to question this correlation was Alexandre Brongniart, who
had received from Hitchcock rock specimens and a fossil fish which he
erroneously identified with a Permian species, and accordingly referred the
strata to the Permian (3, 220, 1821; 6, 76, pl. 9, figs. 1, 2, 1823). The
discerning Professor Finch in 1826 remarked that the red beds of
Connecticut appear to belong “to the new or variegated sandstone,” because
of eight different criteria that he mentions. Of these, but two are of value in
correlation, their “geological position” and the presence of bones other than
fishes. In the Connecticut area, however, the geological position cannot be
determined even to-day, and in Finch’s time the bones of dinosaurs were
unknown. Finch then goes on to point out the occurrences of Old Red
Sandstone in Pennsylvania, but all of the places he refers to are either
younger or older in time. Here we again see the fatality of trying to make
positive correlations on the basis of lithology and color (10, 209, 1826). In
1835, however, Hitchcock showed that the bones that had been found in
1820 were those of a saurian, and accordingly referred the strata of the
Connecticut valley to the New Red Sandstone, a term that then covered
both the Permian and the Triassic. In 1842, W. B. Rogers referred the beds
to the Jurassic, on the basis of plants from Virginia. In 1856, W. C. Redfield
(1789–1857), because of the fishes, advocated a Lias, or Jurassic age, and
proposed the name Newark group for all the Triassic deposits of the
Atlantic border. More recently, on the basis of the plants studied by
Newberry, Fontaine, Sturr, and Ward, and the vertebrates described by
Marsh and Lull, the age has been definitely fixed as Upper Triassic (see
Dana’s Manual of Geology, 740, 1895).
older than these red beds, now known to be of Triassic age.
The first one to question this correlation was Alexandre Brongniart, who
had received from Hitchcock rock specimens and a fossil fish which he
erroneously identified with a Permian species, and accordingly referred the
strata to the Permian (3, 220, 1821; 6, 76, pl. 9, figs. 1, 2, 1823). The
discerning Professor Finch in 1826 remarked that the red beds of
Connecticut appear to belong “to the new or variegated sandstone,” because
of eight different criteria that he mentions. Of these, but two are of value in
correlation, their “geological position” and the presence of bones other than
fishes. In the Connecticut area, however, the geological position cannot be
determined even to-day, and in Finch’s time the bones of dinosaurs were
unknown. Finch then goes on to point out the occurrences of Old Red
Sandstone in Pennsylvania, but all of the places he refers to are either
younger or older in time. Here we again see the fatality of trying to make
positive correlations on the basis of lithology and color (10, 209, 1826). In
1835, however, Hitchcock showed that the bones that had been found in
1820 were those of a saurian, and accordingly referred the strata of the
Connecticut valley to the New Red Sandstone, a term that then covered
both the Permian and the Triassic. In 1842, W. B. Rogers referred the beds
to the Jurassic, on the basis of plants from Virginia. In 1856, W. C. Redfield
(1789–1857), because of the fishes, advocated a Lias, or Jurassic age, and
proposed the name Newark group for all the Triassic deposits of the
Atlantic border. More recently, on the basis of the plants studied by
Newberry, Fontaine, Sturr, and Ward, and the vertebrates described by
Marsh and Lull, the age has been definitely fixed as Upper Triassic (see
Dana’s Manual of Geology, 740, 1895).
Page 87
Unearthing of the Paleozoic in North America.
Permian of the United States.—In Europe, previous to 1841, the
formations now classed as Permian were included in the New Red
Sandstone, and with the Carboniferous were referred to the Secondary. In
that year Murchison proposed the period term Permian. In 1845 came the
classic Geology of Russia in Europe and the Ural Mountains, by
Murchison, Keyserling, and De Verneuil. In this great work the authors
separated out of the New Red the Magnesian Limestone of Great Britain
and the Rothliegende marls, Kupferschiefer, and Zechstein of Germany, and
with other formations of the Urals in Russia, referred them to the Permian
system. This step, one of the most discerning in historical geology, was all
the more important because they closed the Paleozoic era with the Permian,
beginning the Secondary, or Mesozoic, with the New Red Sandstone or the
Triassic period. There is a good review of this work by D. D. Owen (1807–
1860) in the Journal for 1847 (3, 153).
Owen, though accepting the Permian system, is not satisfied with its
reference to the Paleozoic, and he sets the matter forth in the Journal (3,
365, 1847). He doubts “the propriety of a classification which throws the
Permian and Carboniferous systems into the Paleozoic period.” This is
mainly because there is no “evidence of disturbance or unconformability”
between the Permian and Triassic systems. Rather “there is so complete a
blending of adjacent strata” that it is only in Russia that the Permian has
been distinguished from the Triassic. This view of Owen’s was not only
correct for Russia but even more so for the Alps and for India, and it has
taken a great deal of work and discussion to fix upon the disconformable
contact that distinguishes the Paleozoic from the Mesozoic in these areas. In
other words, there was here at this time no mountain making. Then Owen
goes on to state that because the Permian of Europe has reptiles, he sees in
them decisive Mesozoic evidence. “These are certainly strong arguments in
favor of placing, not only the Permian, but also the Carboniferous group in
the Mesozoic period, and terminating the Paleozoic division with the
commencement of the coal measures.” To this harking backward the
geologists of the world have not agreed, but have followed the better views
of Murchison and his associates.
Permian of the United States.—In Europe, previous to 1841, the
formations now classed as Permian were included in the New Red
Sandstone, and with the Carboniferous were referred to the Secondary. In
that year Murchison proposed the period term Permian. In 1845 came the
classic Geology of Russia in Europe and the Ural Mountains, by
Murchison, Keyserling, and De Verneuil. In this great work the authors
separated out of the New Red the Magnesian Limestone of Great Britain
and the Rothliegende marls, Kupferschiefer, and Zechstein of Germany, and
with other formations of the Urals in Russia, referred them to the Permian
system. This step, one of the most discerning in historical geology, was all
the more important because they closed the Paleozoic era with the Permian,
beginning the Secondary, or Mesozoic, with the New Red Sandstone or the
Triassic period. There is a good review of this work by D. D. Owen (1807–
1860) in the Journal for 1847 (3, 153).
Owen, though accepting the Permian system, is not satisfied with its
reference to the Paleozoic, and he sets the matter forth in the Journal (3,
365, 1847). He doubts “the propriety of a classification which throws the
Permian and Carboniferous systems into the Paleozoic period.” This is
mainly because there is no “evidence of disturbance or unconformability”
between the Permian and Triassic systems. Rather “there is so complete a
blending of adjacent strata” that it is only in Russia that the Permian has
been distinguished from the Triassic. This view of Owen’s was not only
correct for Russia but even more so for the Alps and for India, and it has
taken a great deal of work and discussion to fix upon the disconformable
contact that distinguishes the Paleozoic from the Mesozoic in these areas. In
other words, there was here at this time no mountain making. Then Owen
goes on to state that because the Permian of Europe has reptiles, he sees in
them decisive Mesozoic evidence. “These are certainly strong arguments in
favor of placing, not only the Permian, but also the Carboniferous group in
the Mesozoic period, and terminating the Paleozoic division with the
commencement of the coal measures.” To this harking backward the
geologists of the world have not agreed, but have followed the better views
of Murchison and his associates.
Page 88
In 1855 G. G. Shumard discovered, and in 1860 his brother B. F.
Shumard (1820–1869) announced, the presence of Permian strata in the
Guadalupe Mountains of Texas, and in 1902 George H. Girty (14, 363)
confirmed this. Girty regards the faunas as younger than any other late
Paleozoic ones of America, and says: “For this reason I propose to give
them a regional name, which shall be employed in a force similar to
Mississippian and Pennsylvanian.... The term Guadalupian is suggested.”
G. C. Swallow (1817–1899) in 1858 was the first to announce the
presence of Permian fossils in Kansas, and this led to a controversy between
himself and F. B. Meek, both claiming the discovery. It is only in more
recent years that it has been generally admitted that there is Permian in that
state, in Oklahoma, and in Texas. This admission came the more readily
through the discovery of many reptiles in the red beds of Texas, and through
the work of C. A. White, published in 1891, The Texan Permian and its
Mesozoic Types of Fossils (Bull. U. S. Geological Survey, No. 77).
Shumard (1820–1869) announced, the presence of Permian strata in the
Guadalupe Mountains of Texas, and in 1902 George H. Girty (14, 363)
confirmed this. Girty regards the faunas as younger than any other late
Paleozoic ones of America, and says: “For this reason I propose to give
them a regional name, which shall be employed in a force similar to
Mississippian and Pennsylvanian.... The term Guadalupian is suggested.”
G. C. Swallow (1817–1899) in 1858 was the first to announce the
presence of Permian fossils in Kansas, and this led to a controversy between
himself and F. B. Meek, both claiming the discovery. It is only in more
recent years that it has been generally admitted that there is Permian in that
state, in Oklahoma, and in Texas. This admission came the more readily
through the discovery of many reptiles in the red beds of Texas, and through
the work of C. A. White, published in 1891, The Texan Permian and its
Mesozoic Types of Fossils (Bull. U. S. Geological Survey, No. 77).
Page 89
Carboniferous Formations.—The coal formations are noted in a general
way throughout the earliest volumes of the Journal. The first accounts of the
presence of coal, in Ohio, are by Caleb Atwater (1, 227, 239, 1819), and S.
P. Hildreth (13, 38, 40, 1828). The first coal plants to be described and
illustrated were also from Ohio, in an article by Ebenezer Granger in 1821
(3, 5–7). The anthracite field was first described in 1822 by Zachariah Cist
(4, 1) and then by Benjamin Silliman (10, 331–351, 1826); that of western
Pennsylvania was described by William Meade in 1828 (13, 32).
The Lower Carboniferous was first recognized by W. W. Mather in 1838
(34, 356). Later, through the work of Alexander Winchell (1824–1891),
way throughout the earliest volumes of the Journal. The first accounts of the
presence of coal, in Ohio, are by Caleb Atwater (1, 227, 239, 1819), and S.
P. Hildreth (13, 38, 40, 1828). The first coal plants to be described and
illustrated were also from Ohio, in an article by Ebenezer Granger in 1821
(3, 5–7). The anthracite field was first described in 1822 by Zachariah Cist
(4, 1) and then by Benjamin Silliman (10, 331–351, 1826); that of western
Pennsylvania was described by William Meade in 1828 (13, 32).
The Lower Carboniferous was first recognized by W. W. Mather in 1838
(34, 356). Later, through the work of Alexander Winchell (1824–1891),
Page 90
beginning in 1862 (33, 352) and continuing until 1871, and through the
surveys of Iowa (1855–1858), Illinois (essentially the work of A. H.
Worthen, 1858–1888), Ohio (1838, Mather, etc.), and Indiana (Owen, etc.,
1838), there was eventually worked out the following succession:
Permian period.
Upper Barren series.
Dunkard group.
Washington group.
Pennsylvanian period.
Upper Productive Coal series. Monongahela series.
Lower Barren Coal Measures. Conemaugh series.
Lower Productive Coal Measures. Allegheny series.
Pottsville series.
The New York System.—We now come to the epochal survey of the State
of New York, one that established the principles of, and put order into,
American stratigraphy from the Upper Cambrian to the top of the
Devonian. No better area could have been selected for the establishing of
this sequence. This survey also developed a stratigraphic nomenclature
based on New York localities and rock exposures, and made full use of the
entombed fossils in correlation. Incidentally it developed and brought into
prominence James Hall, who continued the stratigraphic work so well
begun and who also laid the foundation for paleontology in America,
becoming its leading invertebrate worker.
This work is reviewed at great length in the Journal in the volumes for
1844–1847 by D. D. Owen. Evidently it followed too new a plan to receive
fulsome praise from conservative Owen, as it should have. He remarks that
the volumes “are not a little prolix, are voluminous and expensive, and do
not give as clear and connected a view of the geological features of the state
as could be wished.... We are of the opinion that before this work can
become generally useful and extensively circulated, it must be condensed
and arranged into one compendious volume” (46, 144, 1844). This was
never done and yet the work was everywhere accepted at once, and to this
end undoubtedly Owen’s detailed review helped much.
The Natural History Survey of New York was organized in 1836 and
completed in 1843. The state was divided into four districts, and to these
were finally assigned the following experienced geologists. The
southeastern part was named the First District, with W. W. Mather (1804–
1859) as geologist; the northeastern quarter was the Second District, with
surveys of Iowa (1855–1858), Illinois (essentially the work of A. H.
Worthen, 1858–1888), Ohio (1838, Mather, etc.), and Indiana (Owen, etc.,
1838), there was eventually worked out the following succession:
Permian period.
Upper Barren series.
Dunkard group.
Washington group.
Pennsylvanian period.
Upper Productive Coal series. Monongahela series.
Lower Barren Coal Measures. Conemaugh series.
Lower Productive Coal Measures. Allegheny series.
Pottsville series.
The New York System.—We now come to the epochal survey of the State
of New York, one that established the principles of, and put order into,
American stratigraphy from the Upper Cambrian to the top of the
Devonian. No better area could have been selected for the establishing of
this sequence. This survey also developed a stratigraphic nomenclature
based on New York localities and rock exposures, and made full use of the
entombed fossils in correlation. Incidentally it developed and brought into
prominence James Hall, who continued the stratigraphic work so well
begun and who also laid the foundation for paleontology in America,
becoming its leading invertebrate worker.
This work is reviewed at great length in the Journal in the volumes for
1844–1847 by D. D. Owen. Evidently it followed too new a plan to receive
fulsome praise from conservative Owen, as it should have. He remarks that
the volumes “are not a little prolix, are voluminous and expensive, and do
not give as clear and connected a view of the geological features of the state
as could be wished.... We are of the opinion that before this work can
become generally useful and extensively circulated, it must be condensed
and arranged into one compendious volume” (46, 144, 1844). This was
never done and yet the work was everywhere accepted at once, and to this
end undoubtedly Owen’s detailed review helped much.
The Natural History Survey of New York was organized in 1836 and
completed in 1843. The state was divided into four districts, and to these
were finally assigned the following experienced geologists. The
southeastern part was named the First District, with W. W. Mather (1804–
1859) as geologist; the northeastern quarter was the Second District, with
Page 91
Ebenezer Emmons (1799–1863) in charge; the central portion was the Third
District, under Lardner Vanuxem (1792–1848); while the western part was
James Hall’s (1811–1898) Fourth District. Paleontology for a time was in
charge of T. A. Conrad (1830–1877); the mineralogical and chemical work
was in the hands of Lewis C. Beck; the botanist was John Torrey; and the
zoologist James DeKay.
The New York State Survey published six annual reports of 1675 pages
octavo, and four final geological reports with 2079 pages quarto. Finally in
1846 Emmons added another volume on the soils and rocks of the state, in
which he also discussed the Taconic and New York systems; it has 371
pages. With the completion of the first survey, Hall took up his life work
under the auspices of the state—his monumental work, Paleontology of
New York, in fifteen quarto volumes of 4539 pages and 1081 plates of
fossils. In addition to all this, there are his annual and other reports to the
Regents of the State, so that it is safe to say that he published not less than
10,000 pages of printed matter on the geology and paleontology of North
America.
In regard to this great series of works, all that can be presented here is a
table of formations as developed by the New York State Survey. Practically
all of its results and formation names have come into general use, with the
exception of the Taconic system of Emmons and the division terms of the
New York system. (See p. 88.)
The New York State Survey, begun in 1836, was continued by James Hall
from 1843 to 1898. During this time he was also state geologist of Iowa
(1855–1858) and Michigan (1862). Since 1898, John M. Clarke has ably
continued the Geological Survey of New York, the state which continues to
be, in science and more especially in geology and paleontology, the
foremost in America.
Western Extension of the New York system.—Before Hall finished his
final report, we find him in 1841 on “a tour of exploration through the states
of Ohio, Indiana, Illinois, a part of Michigan, Kentucky, and Missouri, and
the territories of Iowa and Wisconsin.” This tour is described in the Journal
(42, 51, 1842) under the caption “Notes upon the Geology of the Western
States.” His object was to ascertain how far the New York system as the
standard of reference “was applicable in the western extension of the
series.” In a general way he was very successful in extending the system to
District, under Lardner Vanuxem (1792–1848); while the western part was
James Hall’s (1811–1898) Fourth District. Paleontology for a time was in
charge of T. A. Conrad (1830–1877); the mineralogical and chemical work
was in the hands of Lewis C. Beck; the botanist was John Torrey; and the
zoologist James DeKay.
The New York State Survey published six annual reports of 1675 pages
octavo, and four final geological reports with 2079 pages quarto. Finally in
1846 Emmons added another volume on the soils and rocks of the state, in
which he also discussed the Taconic and New York systems; it has 371
pages. With the completion of the first survey, Hall took up his life work
under the auspices of the state—his monumental work, Paleontology of
New York, in fifteen quarto volumes of 4539 pages and 1081 plates of
fossils. In addition to all this, there are his annual and other reports to the
Regents of the State, so that it is safe to say that he published not less than
10,000 pages of printed matter on the geology and paleontology of North
America.
In regard to this great series of works, all that can be presented here is a
table of formations as developed by the New York State Survey. Practically
all of its results and formation names have come into general use, with the
exception of the Taconic system of Emmons and the division terms of the
New York system. (See p. 88.)
The New York State Survey, begun in 1836, was continued by James Hall
from 1843 to 1898. During this time he was also state geologist of Iowa
(1855–1858) and Michigan (1862). Since 1898, John M. Clarke has ably
continued the Geological Survey of New York, the state which continues to
be, in science and more especially in geology and paleontology, the
foremost in America.
Western Extension of the New York system.—Before Hall finished his
final report, we find him in 1841 on “a tour of exploration through the states
of Ohio, Indiana, Illinois, a part of Michigan, Kentucky, and Missouri, and
the territories of Iowa and Wisconsin.” This tour is described in the Journal
(42, 51, 1842) under the caption “Notes upon the Geology of the Western
States.” His object was to ascertain how far the New York system as the
standard of reference “was applicable in the western extension of the
series.” In a general way he was very successful in extending the system to
Page 92
the Mississippi River, and he clearly saw “a great diminution, first of sandy
matter, and next of shale, as we go westward, and in the whole, a great
increase of calcareous matter in the same direction.” He also clearly noted
the warped nature of the strata, the “anticlinal axis,” since known as the
Cincinnati and Wabash uplifts and the Ozark dome.
Hall, however, fell into a number of flagrant errors because of a too great
reliance on lithologic correlation and supposedly similar sequence. For
instance, the Coal Measures of Pennsylvania were said to directly overlap
the Chemung group of southern New York, and now he finds the same
condition in Ohio, Indiana, and Illinois, failing to see that in most places
between the top of the New York system and the Coal Measures lay the
extensive Mississippian series, one that he generally confounded with the
Chemung, or included in the “Carboniferous group.” He states that the
Portage of New York is the same as the Waverly of Ohio, and at Louisville
the Middle Devonian waterlime is correlated with the similar rock of the
New York Silurian. Hall was especially desirous of fixing the horizon of the
Middle Ordovician lead-bearing rocks of Illinois, Wisconsin, and Iowa, but
unfortunately correlated them with the Niagaran, while the Middle
Devonian about Columbus, Ohio, and Louisville, Kentucky, he referred to
the same horizon. The Galena-Niagaran error was corrected in 1855, but the
Devonian and Mississippian ones remained unadjusted for a long time, and
in Iowa until toward the close of the nineteenth century.
The Geological Column of the New York Geologists of 1842–1843, according to W. W.
Mather 1842.
Alluvial division.
Quaternary system Quaternary division.
Drift division.
These strata are included in the
Tertiary system
next lower division.
Long Island division. Equals the
Tertiary and Cretaceous marls, New Red
sands, and clays of the coastal system of
Upper Secondary system plain of New Jersey. Emmons
Trappean division. The Palisades and Hall.
Red Sandstone division.
Coal system of Mather, and Carboniferous system of Hall.
Old Red system of Catskill Mountains of Emmons; Catskill division of Mather and Hall; and
Catskill group of Vanuxem.
matter, and next of shale, as we go westward, and in the whole, a great
increase of calcareous matter in the same direction.” He also clearly noted
the warped nature of the strata, the “anticlinal axis,” since known as the
Cincinnati and Wabash uplifts and the Ozark dome.
Hall, however, fell into a number of flagrant errors because of a too great
reliance on lithologic correlation and supposedly similar sequence. For
instance, the Coal Measures of Pennsylvania were said to directly overlap
the Chemung group of southern New York, and now he finds the same
condition in Ohio, Indiana, and Illinois, failing to see that in most places
between the top of the New York system and the Coal Measures lay the
extensive Mississippian series, one that he generally confounded with the
Chemung, or included in the “Carboniferous group.” He states that the
Portage of New York is the same as the Waverly of Ohio, and at Louisville
the Middle Devonian waterlime is correlated with the similar rock of the
New York Silurian. Hall was especially desirous of fixing the horizon of the
Middle Ordovician lead-bearing rocks of Illinois, Wisconsin, and Iowa, but
unfortunately correlated them with the Niagaran, while the Middle
Devonian about Columbus, Ohio, and Louisville, Kentucky, he referred to
the same horizon. The Galena-Niagaran error was corrected in 1855, but the
Devonian and Mississippian ones remained unadjusted for a long time, and
in Iowa until toward the close of the nineteenth century.
The Geological Column of the New York Geologists of 1842–1843, according to W. W.
Mather 1842.
Alluvial division.
Quaternary system Quaternary division.
Drift division.
These strata are included in the
Tertiary system
next lower division.
Long Island division. Equals the
Tertiary and Cretaceous marls, New Red
sands, and clays of the coastal system of
Upper Secondary system plain of New Jersey. Emmons
Trappean division. The Palisades and Hall.
Red Sandstone division.
Coal system of Mather, and Carboniferous system of Hall.
Old Red system of Catskill Mountains of Emmons; Catskill division of Mather and Hall; and
Catskill group of Vanuxem.
Page 93
According to Hall 1843, and essentially Vanuxem 1842.
Chemung, Portage or Nunda (divided into
Cashaqua, Gardeau, Portage), Genesee, Tully,
Erie division [Devonian]
Hamilton (divided into Ludlowville; Encrinal,
Moscow), and Marcellus.
Corniferous, Onondaga, Schoharie, Cauda-alli,
Helderberg series [Devonian- Oriskany, Upper Pentamerus, Encrinal,
Silurian] Delthyris, Pentamerus, Waterlime, Onondaga
salt group.
Ontario division [Silurian] Niagara, Clinton, and Medina.
Oneida or Shawangunk, Grey sandstone, Hudson
Champlain division [Silurian- River group, Utica, Trenton, Black River
Ordovician-Upper Cambrian] including Birdseye and Chazy, Calciferous
sandrock, and Potsdam.
According to Emmons 1842, Mather 1843, Vanuxem 1842, Hall 1843.
Taconic System [Ordovician and Granular quartz, Stockbridge limestone,
Lower Cambrian] Magnesian slate, and Taconic slate.
Primary or Hypogene system Metamorphic and Primary rocks.
Correlations with Europe.—The first effort toward correlating the New
York system with those of Europe was made by Conrad in his Notes on
American Geology in 1839 (35, 243). Here he compares it on faunal
grounds with the Silurian system. A more sustained effort was that of Hall
in 1843 (45, 157), when he said that the Silurian of Murchison was equal to
the New York system and embraced the Cambrian, Silurian, and Devonian,
which he considered as forming but one system. Hall in 1844 and Conrad
earlier were erroneously regarding the Middle Devonian of New York
(Hamilton) as “an equivalent of the Ludlow rocks of Mr. Murchison” (47,
118, 1844).
In 1846 E. P. De Verneuil spent the summer in America with a view to
correlating the formations of the New York system with those of Europe. At
this time he had had a wide field experience in France, Germany, and
Russia, was president of the Geological Society of France, and “virtually
the representative of European geology” (2, 153, 1846). Hall says, “No
other person could have presented so clear and perfect a coup d’oeil.” De
Verneuil’s results were translated by Hall and with his own comments were
published in the Journal in 1848 and 1849 under the title “On the
Parallelism of the Paleozoic Deposits of North America with those of
Europe.” De Verneuil was especially struck with the complete development
Chemung, Portage or Nunda (divided into
Cashaqua, Gardeau, Portage), Genesee, Tully,
Erie division [Devonian]
Hamilton (divided into Ludlowville; Encrinal,
Moscow), and Marcellus.
Corniferous, Onondaga, Schoharie, Cauda-alli,
Helderberg series [Devonian- Oriskany, Upper Pentamerus, Encrinal,
Silurian] Delthyris, Pentamerus, Waterlime, Onondaga
salt group.
Ontario division [Silurian] Niagara, Clinton, and Medina.
Oneida or Shawangunk, Grey sandstone, Hudson
Champlain division [Silurian- River group, Utica, Trenton, Black River
Ordovician-Upper Cambrian] including Birdseye and Chazy, Calciferous
sandrock, and Potsdam.
According to Emmons 1842, Mather 1843, Vanuxem 1842, Hall 1843.
Taconic System [Ordovician and Granular quartz, Stockbridge limestone,
Lower Cambrian] Magnesian slate, and Taconic slate.
Primary or Hypogene system Metamorphic and Primary rocks.
Correlations with Europe.—The first effort toward correlating the New
York system with those of Europe was made by Conrad in his Notes on
American Geology in 1839 (35, 243). Here he compares it on faunal
grounds with the Silurian system. A more sustained effort was that of Hall
in 1843 (45, 157), when he said that the Silurian of Murchison was equal to
the New York system and embraced the Cambrian, Silurian, and Devonian,
which he considered as forming but one system. Hall in 1844 and Conrad
earlier were erroneously regarding the Middle Devonian of New York
(Hamilton) as “an equivalent of the Ludlow rocks of Mr. Murchison” (47,
118, 1844).
In 1846 E. P. De Verneuil spent the summer in America with a view to
correlating the formations of the New York system with those of Europe. At
this time he had had a wide field experience in France, Germany, and
Russia, was president of the Geological Society of France, and “virtually
the representative of European geology” (2, 153, 1846). Hall says, “No
other person could have presented so clear and perfect a coup d’oeil.” De
Verneuil’s results were translated by Hall and with his own comments were
published in the Journal in 1848 and 1849 under the title “On the
Parallelism of the Paleozoic Deposits of North America with those of
Europe.” De Verneuil was especially struck with the complete development
Page 94
of American Paleozoic deposits and said it was the best anywhere. On the
other hand, he did not agree with the detailed arrangement of the formations
in the various divisions of the New York system, and Hall admitted
altogether too readily that the terms were proposed “as a matter of
concession, and it is to be regretted that such an artificial classification was
adopted.” De Verneuil’s correlations are as follows:
The Lower Silurian system begins with the Potsdam, the analogue of the
Obolus sandstone of Russia and Sweden. The Black River and Trenton hold
the position of the Orthoceras limestones of Sweden and Russia, while the
Utica and Lorraine are represented by the Graptolite beds of the same
countries. Both correlations are in partial error. He unites the Chazy,
Birdseye, and Black River in one series, and in another the Trenton, Utica,
and Lorraine. Of species common to Europe and America he makes out
seventeen.
In the Upper Silurian system, the Oneida and Shawangunk are taken out
of the Champlain division, and, with the Medina, are referred to the
Silurian, along with all of the Ontario division plus the Lower Helderberg.
The Clinton is regarded as highest Caradoc or as holding a stage between
that and the Wenlock. The Niagara group is held to be the exact equivalent
of the Wenlock, “while the five inferior groups of the Helderberg division
represent the rocks of Ludlow.” We now know that these Helderberg
formations are Lower Devonian in age. De Verneuil unites in one series the
Waterlime, Pentamerus, Delthyris, Encrinal, and Upper Pentamerus. Of
identical species there are forty common to Europe and America.
The Devonian system De Verneuil begins, “after much hesitation,” with
the Oriskany and certainly with the five upper members of Hall’s
Helderberg division, all of the Erie and the Old Red Sandstone. He also
adjusts Hall’s error by placing in the Devonian the Upper Cliff limestone of
Ohio and Indiana, regarded by the former as Silurian. The Oriskany is
correlated with the grauwackes of the Rhine, and the Onondaga or
Corniferous with the lower Eifelian. Cauda-galli, Schoharie, and Onondaga
are united in one series; Marcellus, Hamilton, Tully, and Genesee in
another; and Portage and Chemung in a third. Of species common to
Europe and America there are thirty-nine.
The Waverly of Ohio and that near Louisville, Kentucky, which Hall had
called Chemung, De Verneuil correctly refers to the Carboniferous, but to
other hand, he did not agree with the detailed arrangement of the formations
in the various divisions of the New York system, and Hall admitted
altogether too readily that the terms were proposed “as a matter of
concession, and it is to be regretted that such an artificial classification was
adopted.” De Verneuil’s correlations are as follows:
The Lower Silurian system begins with the Potsdam, the analogue of the
Obolus sandstone of Russia and Sweden. The Black River and Trenton hold
the position of the Orthoceras limestones of Sweden and Russia, while the
Utica and Lorraine are represented by the Graptolite beds of the same
countries. Both correlations are in partial error. He unites the Chazy,
Birdseye, and Black River in one series, and in another the Trenton, Utica,
and Lorraine. Of species common to Europe and America he makes out
seventeen.
In the Upper Silurian system, the Oneida and Shawangunk are taken out
of the Champlain division, and, with the Medina, are referred to the
Silurian, along with all of the Ontario division plus the Lower Helderberg.
The Clinton is regarded as highest Caradoc or as holding a stage between
that and the Wenlock. The Niagara group is held to be the exact equivalent
of the Wenlock, “while the five inferior groups of the Helderberg division
represent the rocks of Ludlow.” We now know that these Helderberg
formations are Lower Devonian in age. De Verneuil unites in one series the
Waterlime, Pentamerus, Delthyris, Encrinal, and Upper Pentamerus. Of
identical species there are forty common to Europe and America.
The Devonian system De Verneuil begins, “after much hesitation,” with
the Oriskany and certainly with the five upper members of Hall’s
Helderberg division, all of the Erie and the Old Red Sandstone. He also
adjusts Hall’s error by placing in the Devonian the Upper Cliff limestone of
Ohio and Indiana, regarded by the former as Silurian. The Oriskany is
correlated with the grauwackes of the Rhine, and the Onondaga or
Corniferous with the lower Eifelian. Cauda-galli, Schoharie, and Onondaga
are united in one series; Marcellus, Hamilton, Tully, and Genesee in
another; and Portage and Chemung in a third. Of species common to
Europe and America there are thirty-nine.
The Waverly of Ohio and that near Louisville, Kentucky, which Hall had
called Chemung, De Verneuil correctly refers to the Carboniferous, but to
Page 95
this Hall does not consent. De Verneuil points out that there are thirty-one
species in common between Europe and America. “And as to plants, the
immense quantity of terrestrial species identical on the two sides of the
Atlantic, proves that the coal was formed in the neighborhood of lands
already emerged, and placed in similar physical conditions.”
An analysis of the Paleozoic fossils of Europe and America leads De
Verneuil to “the conviction that identical species have lived at the same
epoch in America and in Europe, that they have had nearly the same
duration, and that they succeeded each other in the same order.” This he
states is independent of the depth of the seas, and of “the upheavings which
have affected the surface of the globe.” The species of a period begin and
drop out at different levels, and toward the top of a system the whole takes
on the character of the next one. “If it happens that in the two countries a
certain number of systems, characterized by the same fossils, are
superimposed in the same order, whatever may be, otherwise, their
thickness and the number of physical groups of which they are composed, it
is philosophical to consider these systems as parallel and synchronous.”
Because of the dominance of the sandstones and shales in eastern New
York, De Verneuil holds that a land lay to the east. The many fucoids and
ripple-marks from the Potsdam to the Portage indicated to him shallow
water and nearness to a shore.
The Oldest Geologic Eras.—We have seen in previous pages how the
Primitive rocks of Arduino and of Werner had been resolved, at least in part,
into the systems of the Paleozoic, but there still remained many areas of
ancient rocks that could not be adjusted into the accepted scheme. One of
the most extensive of these is in Canada, where the really Primitive
formations, of granites, gneisses, schists, and even undetermined sediments,
abound and are developed on a grander scale than elsewhere, covering more
than two million square miles and overlain unconformably by the Paleozoic
and later rocks. The first to call attention to them was J. I. Bigsby, a medical
staff officer of the British Army, in 1821 (3, 254). It was, however, William
E. Logan (1798–1875), the “father of Canadian geology,” who first
unravelled their historical sequence. At first he also called them Primary,
but after much work he perceived in them parallel structures and
metamorphosed sediments, underlain by and associated with pink granites.
For the oldest masses, essentially the granites, he proposed the term
species in common between Europe and America. “And as to plants, the
immense quantity of terrestrial species identical on the two sides of the
Atlantic, proves that the coal was formed in the neighborhood of lands
already emerged, and placed in similar physical conditions.”
An analysis of the Paleozoic fossils of Europe and America leads De
Verneuil to “the conviction that identical species have lived at the same
epoch in America and in Europe, that they have had nearly the same
duration, and that they succeeded each other in the same order.” This he
states is independent of the depth of the seas, and of “the upheavings which
have affected the surface of the globe.” The species of a period begin and
drop out at different levels, and toward the top of a system the whole takes
on the character of the next one. “If it happens that in the two countries a
certain number of systems, characterized by the same fossils, are
superimposed in the same order, whatever may be, otherwise, their
thickness and the number of physical groups of which they are composed, it
is philosophical to consider these systems as parallel and synchronous.”
Because of the dominance of the sandstones and shales in eastern New
York, De Verneuil holds that a land lay to the east. The many fucoids and
ripple-marks from the Potsdam to the Portage indicated to him shallow
water and nearness to a shore.
The Oldest Geologic Eras.—We have seen in previous pages how the
Primitive rocks of Arduino and of Werner had been resolved, at least in part,
into the systems of the Paleozoic, but there still remained many areas of
ancient rocks that could not be adjusted into the accepted scheme. One of
the most extensive of these is in Canada, where the really Primitive
formations, of granites, gneisses, schists, and even undetermined sediments,
abound and are developed on a grander scale than elsewhere, covering more
than two million square miles and overlain unconformably by the Paleozoic
and later rocks. The first to call attention to them was J. I. Bigsby, a medical
staff officer of the British Army, in 1821 (3, 254). It was, however, William
E. Logan (1798–1875), the “father of Canadian geology,” who first
unravelled their historical sequence. At first he also called them Primary,
but after much work he perceived in them parallel structures and
metamorphosed sediments, underlain by and associated with pink granites.
For the oldest masses, essentially the granites, he proposed the term
Page 96
Laurentian system (1853, 1863) and for the altered and deformed strata, the
name Huronian series (1857, 1863). Overlying these unconformably was a
third series, the copper-bearing rocks. Since his day a great host of
Canadian and American geologists have labored over this, the most intricate
of all geology, and now we have the following tentative chronology
(Schuchert and Barrell, 38, 1, 1914):
Late Proterozoic era.
Keweenawan, Animikian and Huronian periods.
Early Proterozoic era.
Sudburian period or older Huronian.
Archeozoic era.
Grenville series, etc.
Cosmic history.
name Huronian series (1857, 1863). Overlying these unconformably was a
third series, the copper-bearing rocks. Since his day a great host of
Canadian and American geologists have labored over this, the most intricate
of all geology, and now we have the following tentative chronology
(Schuchert and Barrell, 38, 1, 1914):
Late Proterozoic era.
Keweenawan, Animikian and Huronian periods.
Early Proterozoic era.
Sudburian period or older Huronian.
Archeozoic era.
Grenville series, etc.
Cosmic history.
Page 97
The Taconic System Resurrected.
The Taconic system was first announced by Ebenezer Emmons in 1841,
and clearly defined in 1842. It started the most bitter and most protracted
discussion in the annals of American geology. After Emmons’s subsequent
publications had put the Taconic system through three phases, Barrande of
Bohemia in 1860–1863 shed a great deal of new and correct light upon it,
affirming in a series of letters to Billings that the Taconic fossils are like
those of his Primordial system, or what we now call the Middle Cambrian
(31, 210, 1861, et seq.).
In a series of articles published by S. W. Ford in the Journal between
1871 and 1886, there was developed the further new fact that in Rensselaer
and Columbia counties, New York, the so-called Hudson River group
abounds in “Primordial” fossils wholly unlike those of the Potsdam, and
which Ford later on spoke of as belonging to “Lower Potsdam” time.
James D. Dana entered the field of the Taconic area in 1871 and
demonstrated that the system also abounds in Ordovician fossiliferous
formations. Then came the far-reaching work of Charles D. Walcott,
beginning in 1886, which showed that all through eastern New York and
into northern Vermont the Hudson River group and the Taconic system
abound not only in Ordovician but also in Cambrian fossils. Finally in 1888
Dana presented a Brief History of Taconic Ideas, and laid away the system
with these words (36, 27):
“It is almost fifty years since the Taconic system made its abrupt entrance into geological science.
Notwithstanding some good points, it has been through its greater errors, long a hindrance to
progress here and abroad ... But, whether the evil or the good has predominated, we may now hope,
while heartily honoring Professor Emmons for his earnest geological labors and his discoveries, that
Taconic ideas may be allowed to be and remain part of the past.”
As an epitaph Dana placed over the remains of the Taconic system the
black-faced numerals 1841–1888. That the remains of the system, however,
and the term Taconic are still alive and demanding a rehearing is apparent
to all interested stratigraphers. This is not the place to set the matter right,
The Taconic system was first announced by Ebenezer Emmons in 1841,
and clearly defined in 1842. It started the most bitter and most protracted
discussion in the annals of American geology. After Emmons’s subsequent
publications had put the Taconic system through three phases, Barrande of
Bohemia in 1860–1863 shed a great deal of new and correct light upon it,
affirming in a series of letters to Billings that the Taconic fossils are like
those of his Primordial system, or what we now call the Middle Cambrian
(31, 210, 1861, et seq.).
In a series of articles published by S. W. Ford in the Journal between
1871 and 1886, there was developed the further new fact that in Rensselaer
and Columbia counties, New York, the so-called Hudson River group
abounds in “Primordial” fossils wholly unlike those of the Potsdam, and
which Ford later on spoke of as belonging to “Lower Potsdam” time.
James D. Dana entered the field of the Taconic area in 1871 and
demonstrated that the system also abounds in Ordovician fossiliferous
formations. Then came the far-reaching work of Charles D. Walcott,
beginning in 1886, which showed that all through eastern New York and
into northern Vermont the Hudson River group and the Taconic system
abound not only in Ordovician but also in Cambrian fossils. Finally in 1888
Dana presented a Brief History of Taconic Ideas, and laid away the system
with these words (36, 27):
“It is almost fifty years since the Taconic system made its abrupt entrance into geological science.
Notwithstanding some good points, it has been through its greater errors, long a hindrance to
progress here and abroad ... But, whether the evil or the good has predominated, we may now hope,
while heartily honoring Professor Emmons for his earnest geological labors and his discoveries, that
Taconic ideas may be allowed to be and remain part of the past.”
As an epitaph Dana placed over the remains of the Taconic system the
black-faced numerals 1841–1888. That the remains of the system, however,
and the term Taconic are still alive and demanding a rehearing is apparent
to all interested stratigraphers. This is not the place to set the matter right,
Page 98
and all that can be done at the present time is to point out what are the
things that still keep alive Emmons’s system.
In the typical area of the Taconic system, i. e., in Rensselaer County,
Emmons in 1844–1846 produced the fossils Atops trilineatus and
Elliptocephala asaphoides. S. W. Ford, as stated above, later produced from
the same general area many other fossils that he demonstrated to be older
than the Potsdam sandstone. To this time he gave the name of Lower
Potsdam, thus proving on paleontological grounds that at least some part of
the Taconic system is older than the New York system, and therefore older
than the Hudson River group of Ordovician age.
In 1888 Walcott presented his conclusions in regard to the sequence of
the strata in the typical Taconic area and to the north and south of it. He
collected Lower Cambrian fossils at more than one hundred localities
“within the typical Taconic area,” and said that the thickness of his “terrane
No. 5” or “Cambrian (Georgia),” now referable to the Lower Cambrian, is
“14,000 feet or more.” He demonstrated that the Lower Cambrian is
infolded with the Lower and Middle Ordovician, and confirmed Emmons’s
statement that the former rests upon his Primary or Pre-Cambrian masses.
Elsewhere, he writes: “To the west of the Taconic range the section passes
down through the limestone (3) [of Lower and Middle Ordovician age] to
the hydromica schists (2) [whose age may also be of early Ordovician], and
thence to the great development of slates and shales with their interbedded
sparry limestones, calciferous and arenaceous strata, all of which contain
more or less of the Olenellus ... fauna.” He then knew thirty-five species in
Washington County, New York (35, 401, 1888).
Finally in 1915 Walcott said that in the Cordilleran area of America there
was a movement that brought about changes “in the sedimentation and
succession of the faunas which serve to draw a boundary line between the
Lower and Middle Cambrian series.... The length of this period of
interruption must have been considerable ... and when connection with the
Pacific was resumed a new fauna that had been developing in the Pacific
was then introduced into the Cordilleran sea and constituted the Middle
Cambrian fauna. The change in the species from the Lower to the Middle
Cambrian fauna is very great.” He then goes on to show that in the
Appalachian geosyncline there was another movement that shut out the
things that still keep alive Emmons’s system.
In the typical area of the Taconic system, i. e., in Rensselaer County,
Emmons in 1844–1846 produced the fossils Atops trilineatus and
Elliptocephala asaphoides. S. W. Ford, as stated above, later produced from
the same general area many other fossils that he demonstrated to be older
than the Potsdam sandstone. To this time he gave the name of Lower
Potsdam, thus proving on paleontological grounds that at least some part of
the Taconic system is older than the New York system, and therefore older
than the Hudson River group of Ordovician age.
In 1888 Walcott presented his conclusions in regard to the sequence of
the strata in the typical Taconic area and to the north and south of it. He
collected Lower Cambrian fossils at more than one hundred localities
“within the typical Taconic area,” and said that the thickness of his “terrane
No. 5” or “Cambrian (Georgia),” now referable to the Lower Cambrian, is
“14,000 feet or more.” He demonstrated that the Lower Cambrian is
infolded with the Lower and Middle Ordovician, and confirmed Emmons’s
statement that the former rests upon his Primary or Pre-Cambrian masses.
Elsewhere, he writes: “To the west of the Taconic range the section passes
down through the limestone (3) [of Lower and Middle Ordovician age] to
the hydromica schists (2) [whose age may also be of early Ordovician], and
thence to the great development of slates and shales with their interbedded
sparry limestones, calciferous and arenaceous strata, all of which contain
more or less of the Olenellus ... fauna.” He then knew thirty-five species in
Washington County, New York (35, 401, 1888).
Finally in 1915 Walcott said that in the Cordilleran area of America there
was a movement that brought about changes “in the sedimentation and
succession of the faunas which serve to draw a boundary line between the
Lower and Middle Cambrian series.... The length of this period of
interruption must have been considerable ... and when connection with the
Pacific was resumed a new fauna that had been developing in the Pacific
was then introduced into the Cordilleran sea and constituted the Middle
Cambrian fauna. The change in the species from the Lower to the Middle
Cambrian fauna is very great.” He then goes on to show that in the
Appalachian geosyncline there was another movement that shut out the
Page 99
Middle Cambrian Paradoxides fauna of the Atlantic realm from this trough,
and all deposition as well.
Conclusions.—Accordingly it appears that everywhere in America the
Lower Cambrian formations are separated by a land interval of long
duration from those of Middle Cambrian time. These formations therefore
unite into a natural system of rocks or a period of time. Between Middle
and Upper Cambrian time, however, there appears to be a complete
transition in the Cordilleran trough, binding these two series of deposits into
one natural or diastrophic system. Hence the writer proposes that the Lower
Cambrian of America be known as the Taconic system. The Middle and
Upper Cambrian series can be continued for the present under the term
Cambrian system, a term, however, that is by no means in good standing for
these formations, as will be demonstrated under the discussion of the
Silurian controversy.
and all deposition as well.
Conclusions.—Accordingly it appears that everywhere in America the
Lower Cambrian formations are separated by a land interval of long
duration from those of Middle Cambrian time. These formations therefore
unite into a natural system of rocks or a period of time. Between Middle
and Upper Cambrian time, however, there appears to be a complete
transition in the Cordilleran trough, binding these two series of deposits into
one natural or diastrophic system. Hence the writer proposes that the Lower
Cambrian of America be known as the Taconic system. The Middle and
Upper Cambrian series can be continued for the present under the term
Cambrian system, a term, however, that is by no means in good standing for
these formations, as will be demonstrated under the discussion of the
Silurian controversy.
Page 100
The Silurian Controversy.
Just as in America the base of the Paleozoic was involved in a protracted
controversy, so in England the Cambrian-Silurian succession was a subject
of long debate between Sedgwick and Murchison, and among the
succeeding geologists of Europe. The history of the solution is so well and
justly stated in the Journal by James D. Dana under the title “Sedgwick and
Murchison: Cambrian and Silurian” (39, 167, 1890), and by Sir Archibald
Geikie in his Text-book of Geology, 1903, that all that is here required is to
briefly restate it and to bring the solution up to date.
Adam Sedgwick (1785–1873) and R. I. Murchison (1792–1871) each
began to work in the areas of Cambria (Wales) and Siluria (England) in
1831, but the terms Cambrian and Silurian were not published until 1835.
Murchison was the first to satisfactorily work out the sequence of the
Silurian system because of the simpler structural and more fossiliferous
condition of his area. Sedgwick, on the other hand, had his academic duties
to perform at Cambridge University, and being an older and more
conservative man, delayed publishing his final results, because of the
further fact that his area was far more deformed and less fossiliferous. In
1834 they were working in concert in the Silurian area, and Sedgwick said:
“I was so struck by the clearness of the natural sections and the perfection
of his workmanship that I received, I might say, with implicit faith
everything which he then taught me.... The whole ‘Silurian system’ was by
its author placed above the great undulating slate-rocks of South Wales.” At
that time Murchison told Sedgwick that the Bala group of the latter, now
known to be in the middle of the Lower Silurian, could not be brought
within the limits of the Silurian system, and added, “I believe it to plunge
under the true Llandeilo-flags,” now placed next below the Bala and above
the Arenig, which at the present is regarded as at the base of the Ordovician.
The Silurian system was defined in print by Murchison in July, 1835, the
Upper Silurian embracing the Ludlow and Wenlock, while the Lower
Silurian was based on the Caradoc and Llandeilo. Murchison’s monumental
work, The Silurian System, of 100 pages and many plates of fossils,
appeared in 1838.
Just as in America the base of the Paleozoic was involved in a protracted
controversy, so in England the Cambrian-Silurian succession was a subject
of long debate between Sedgwick and Murchison, and among the
succeeding geologists of Europe. The history of the solution is so well and
justly stated in the Journal by James D. Dana under the title “Sedgwick and
Murchison: Cambrian and Silurian” (39, 167, 1890), and by Sir Archibald
Geikie in his Text-book of Geology, 1903, that all that is here required is to
briefly restate it and to bring the solution up to date.
Adam Sedgwick (1785–1873) and R. I. Murchison (1792–1871) each
began to work in the areas of Cambria (Wales) and Siluria (England) in
1831, but the terms Cambrian and Silurian were not published until 1835.
Murchison was the first to satisfactorily work out the sequence of the
Silurian system because of the simpler structural and more fossiliferous
condition of his area. Sedgwick, on the other hand, had his academic duties
to perform at Cambridge University, and being an older and more
conservative man, delayed publishing his final results, because of the
further fact that his area was far more deformed and less fossiliferous. In
1834 they were working in concert in the Silurian area, and Sedgwick said:
“I was so struck by the clearness of the natural sections and the perfection
of his workmanship that I received, I might say, with implicit faith
everything which he then taught me.... The whole ‘Silurian system’ was by
its author placed above the great undulating slate-rocks of South Wales.” At
that time Murchison told Sedgwick that the Bala group of the latter, now
known to be in the middle of the Lower Silurian, could not be brought
within the limits of the Silurian system, and added, “I believe it to plunge
under the true Llandeilo-flags,” now placed next below the Bala and above
the Arenig, which at the present is regarded as at the base of the Ordovician.
The Silurian system was defined in print by Murchison in July, 1835, the
Upper Silurian embracing the Ludlow and Wenlock, while the Lower
Silurian was based on the Caradoc and Llandeilo. Murchison’s monumental
work, The Silurian System, of 100 pages and many plates of fossils,
appeared in 1838.
Page 101
The Cambrian system was described for the first time by Sedgwick in
August, 1835, but the completed work—a classic in geology—Synopsis of
the Classification of the British Palæozoic Rocks, along with M’Coy’s
Descriptions of British Palæozoic Fossils, did not appear until 1852–1855.
Sedgwick’s original Upper Cambrian included the greater part of the chain
of the Berwyns, where he said it was connected with the Llandeilo flags of
the Silurian. The Middle Cambrian comprised the higher mountains of
Cærnarvonshire and Merionethshire, and the Lower Cambrian was said to
occupy the southwest coast of Cærnarvonshire, and to consist of chlorite
and mica schists, and some serpentine and granular limestone. In 1853 it
was seen that the fossiliferous Upper Cambrian included the Arenig,
Llandeilo, Bala, Caradoc, Coniston, Hirnant, and Lower Llandovery. On the
other hand, it was not until long after Murchison and Sedgwick passed
away that the Middle and Lower Cambrian were shown to have fossils, but
few of those that characterize what is now called Lower, Middle, and Upper
Cambrian time.
Not until long after the original announcement of the Cambrian system
did Sedgwick become aware “of the unfortunate mischief-involving fact”
that the most fossiliferous portion of the Cambrian—the Upper Cambrian—
and at that time the only part yielding determinable fossils, when compared
with the Lower Silurian was seen to be an equivalent formation but with
very different lithologic conditions. He began to see in 1842 that his
Cambrian was in conflict with the Silurian system, and four years later there
were serious divergencies of views between himself and Murchison. The
climax of the controversy was attained in 1852, when Sedgwick was
extending his Cambrian system upwards to include the Bala, Llandeilo, and
Caradoc, a proceeding not unlike that of Murchison, who earlier had been
extending his Silurian downward through all of the fossiliferous Cambrian
to the base of the Lingula flags.
Dana in his review of the Silurian-Cambrian controversy states: “The
claim of a worker to affix a name to a series of rocks first studied and
defined by him cannot be disputed.” We have seen that Murchison had
priority of publication in his term Silurian over Sedgwick’s Cambrian, but
that in a complete presentation, both stratigraphically and faunally, the
former had years of prior definition. What has even more weight is that
geologists nearly everywhere had accepted Murchison’s Silurian system as
founded upon the Lower and Upper Silurian formations. A nomenclature
August, 1835, but the completed work—a classic in geology—Synopsis of
the Classification of the British Palæozoic Rocks, along with M’Coy’s
Descriptions of British Palæozoic Fossils, did not appear until 1852–1855.
Sedgwick’s original Upper Cambrian included the greater part of the chain
of the Berwyns, where he said it was connected with the Llandeilo flags of
the Silurian. The Middle Cambrian comprised the higher mountains of
Cærnarvonshire and Merionethshire, and the Lower Cambrian was said to
occupy the southwest coast of Cærnarvonshire, and to consist of chlorite
and mica schists, and some serpentine and granular limestone. In 1853 it
was seen that the fossiliferous Upper Cambrian included the Arenig,
Llandeilo, Bala, Caradoc, Coniston, Hirnant, and Lower Llandovery. On the
other hand, it was not until long after Murchison and Sedgwick passed
away that the Middle and Lower Cambrian were shown to have fossils, but
few of those that characterize what is now called Lower, Middle, and Upper
Cambrian time.
Not until long after the original announcement of the Cambrian system
did Sedgwick become aware “of the unfortunate mischief-involving fact”
that the most fossiliferous portion of the Cambrian—the Upper Cambrian—
and at that time the only part yielding determinable fossils, when compared
with the Lower Silurian was seen to be an equivalent formation but with
very different lithologic conditions. He began to see in 1842 that his
Cambrian was in conflict with the Silurian system, and four years later there
were serious divergencies of views between himself and Murchison. The
climax of the controversy was attained in 1852, when Sedgwick was
extending his Cambrian system upwards to include the Bala, Llandeilo, and
Caradoc, a proceeding not unlike that of Murchison, who earlier had been
extending his Silurian downward through all of the fossiliferous Cambrian
to the base of the Lingula flags.
Dana in his review of the Silurian-Cambrian controversy states: “The
claim of a worker to affix a name to a series of rocks first studied and
defined by him cannot be disputed.” We have seen that Murchison had
priority of publication in his term Silurian over Sedgwick’s Cambrian, but
that in a complete presentation, both stratigraphically and faunally, the
former had years of prior definition. What has even more weight is that
geologists nearly everywhere had accepted Murchison’s Silurian system as
founded upon the Lower and Upper Silurian formations. A nomenclature
Page 102
once widely accepted is almost impossible to dislodge. However, in regard
to the controversy it should not be forgotten that it was only Murchison’s
Lower Silurian that was in conflict with Sedgwick’s Upper Cambrian. As
for the rest of the Cambrian, that was not involved in the controversy.
Dana goes on to state that science may accept a name, or not, according
as it is, or is not, needed. In the progress of geology, he thought that the
time had finally been reached when the name Cambrian was a necessity,
and he included both Cambrian and Silurian in the geological record. The
“Silurian,” however, included the Lower and Upper Silurian—not one
system of rocks, but two.
It is now twenty-seven years since Dana came to this conclusion, at a
time when it was believed that there was more or less continuous deposition
not only between the formations of a system but between the systems
themselves as well. To-day many geologists hold that in the course of time
the oceans pulsate back and forth over the continents, and accordingly that
the sequence of marine sedimentation in most places must be much broken,
and to-day we know that the breaks or land intervals in the marine record
are most marked between the eras, and shorter between all or at least most
of the periods. Furthermore, in North America, we have learned that the
breaks between the systems are most marked in the interior of the continent
and less so on or toward its margins.
Hardly any one now questions the fact of a long land interval between the
Lower Silurian and Upper Silurian in England, and it is to Sedgwick’s
credit that he was the first to point out this fact and also the presence of an
unconformity. It therefore follows that we cannot continue to use Silurian
system in the sense proposed by Murchison, since it includes two distinct
systems or periods. Dana, in the last edition of his Manual of Geology
(1895), also recognizes two systems, but curiously he saw nothing
incongruous in calling them “Lower Silurian era” and “Upper Silurian era.”
It certainly is not conducive to clear thinking, however, to refer to two
systems by the one name of Silurian and to speak of them individually as
Lower and Upper Silurian, thus giving the impression that the two systems
are but parts of one—the Silurian. Each one of the parts has its independent
faunal and physical characters.
We must digress a little here and note the work of Joachim Barrande
(1799–1883) in Bohemia. In 1846 he published a short account of the
to the controversy it should not be forgotten that it was only Murchison’s
Lower Silurian that was in conflict with Sedgwick’s Upper Cambrian. As
for the rest of the Cambrian, that was not involved in the controversy.
Dana goes on to state that science may accept a name, or not, according
as it is, or is not, needed. In the progress of geology, he thought that the
time had finally been reached when the name Cambrian was a necessity,
and he included both Cambrian and Silurian in the geological record. The
“Silurian,” however, included the Lower and Upper Silurian—not one
system of rocks, but two.
It is now twenty-seven years since Dana came to this conclusion, at a
time when it was believed that there was more or less continuous deposition
not only between the formations of a system but between the systems
themselves as well. To-day many geologists hold that in the course of time
the oceans pulsate back and forth over the continents, and accordingly that
the sequence of marine sedimentation in most places must be much broken,
and to-day we know that the breaks or land intervals in the marine record
are most marked between the eras, and shorter between all or at least most
of the periods. Furthermore, in North America, we have learned that the
breaks between the systems are most marked in the interior of the continent
and less so on or toward its margins.
Hardly any one now questions the fact of a long land interval between the
Lower Silurian and Upper Silurian in England, and it is to Sedgwick’s
credit that he was the first to point out this fact and also the presence of an
unconformity. It therefore follows that we cannot continue to use Silurian
system in the sense proposed by Murchison, since it includes two distinct
systems or periods. Dana, in the last edition of his Manual of Geology
(1895), also recognizes two systems, but curiously he saw nothing
incongruous in calling them “Lower Silurian era” and “Upper Silurian era.”
It certainly is not conducive to clear thinking, however, to refer to two
systems by the one name of Silurian and to speak of them individually as
Lower and Upper Silurian, thus giving the impression that the two systems
are but parts of one—the Silurian. Each one of the parts has its independent
faunal and physical characters.
We must digress a little here and note the work of Joachim Barrande
(1799–1883) in Bohemia. In 1846 he published a short account of the
Page 103
“Silurian system” of Bohemia, dividing it into étages lettered C to H.
Between 1852 and 1883 he issued his “Système Silurien du Centre de la
Bohème,” in eighteen quarto volumes with 5568 pages of text and 798
plates of fossils—a monumental work unrivalled in paleontology. In the
first volume the geology of Bohemia is set forth, and here we see that
étages A and B are Azoic or pre-Cambrian, and C to H make up his Silurian
system. Etage C has his “Primordial fauna,” now known to be of
Paradoxides or Middle Cambrian time, while D is Lower Silurian, E is
Upper Silurian, F is Lower Devonian, and G and H are Middle Devonian.
From this it appears that Barrande’s Silurian system is far more extensive
than that of Murchison, embracing twice as many periods as that of England
and Wales.
About 1879 there was in England a nearly general agreement that
Cambrian should embrace Barrande’s Primordial or Paradoxides faunas,
and in the North Wales area be continued up to the top of the Tremadoc
slates. To-day we would include Middle and Upper Cambrian. Lower
Cambrian in the sense of containing the Olenellus faunas was then
unknown in Great Britain.
Lapworth, recognizing the distinctness of the Lower Silurian as a system,
proposed in 1879 to recognize it as such, and named it Ordovician,
restricting Silurian to Murchison’s Upper Silurian. This term has not been
widely used either in Great Britain or on the Continent, but in the last
twenty years has been accepted more and more widely in America. Even
here, however, it is in direct conflict with the term Champlain, proposed by
the New York State Geologist in 1842.
In 1897 the International Geological Congress published E. Renevier’s
Chronographie Géologique, wherein we find the following:
Ludlowian (Murchison 1839).
Upper or Silurian (Murchison, restricted,
Wenlockian (Murchison 1839).
1835).
Landoverian (Murchison).
Caradocian (Murchison 1839).
Silurian Middle or Ordovician (Lapworth 1879). Landeilian (Murchison 1839).
Period. Arenigian (Sedgwick 1847).
Potsdamian (Emmons 1838).
Lower or Cambrian (Sedgwick, restricted, Menevian (Salter and Hicks
1835). 1865).
Georgian (Hitchcock 1861).
Between 1852 and 1883 he issued his “Système Silurien du Centre de la
Bohème,” in eighteen quarto volumes with 5568 pages of text and 798
plates of fossils—a monumental work unrivalled in paleontology. In the
first volume the geology of Bohemia is set forth, and here we see that
étages A and B are Azoic or pre-Cambrian, and C to H make up his Silurian
system. Etage C has his “Primordial fauna,” now known to be of
Paradoxides or Middle Cambrian time, while D is Lower Silurian, E is
Upper Silurian, F is Lower Devonian, and G and H are Middle Devonian.
From this it appears that Barrande’s Silurian system is far more extensive
than that of Murchison, embracing twice as many periods as that of England
and Wales.
About 1879 there was in England a nearly general agreement that
Cambrian should embrace Barrande’s Primordial or Paradoxides faunas,
and in the North Wales area be continued up to the top of the Tremadoc
slates. To-day we would include Middle and Upper Cambrian. Lower
Cambrian in the sense of containing the Olenellus faunas was then
unknown in Great Britain.
Lapworth, recognizing the distinctness of the Lower Silurian as a system,
proposed in 1879 to recognize it as such, and named it Ordovician,
restricting Silurian to Murchison’s Upper Silurian. This term has not been
widely used either in Great Britain or on the Continent, but in the last
twenty years has been accepted more and more widely in America. Even
here, however, it is in direct conflict with the term Champlain, proposed by
the New York State Geologist in 1842.
In 1897 the International Geological Congress published E. Renevier’s
Chronographie Géologique, wherein we find the following:
Ludlowian (Murchison 1839).
Upper or Silurian (Murchison, restricted,
Wenlockian (Murchison 1839).
1835).
Landoverian (Murchison).
Caradocian (Murchison 1839).
Silurian Middle or Ordovician (Lapworth 1879). Landeilian (Murchison 1839).
Period. Arenigian (Sedgwick 1847).
Potsdamian (Emmons 1838).
Lower or Cambrian (Sedgwick, restricted, Menevian (Salter and Hicks
1835). 1865).
Georgian (Hitchcock 1861).
Page 104
Regarding this period, which, by the way, is not very unlike that of
Barrande, Renevier remarks that it is “as important as the Cretaceous or the
Jurassic. Lapworth even gives it a value of the first order equal to the
Protozoic era.”
In the above there is an obvious objection in the double usage of the term
Silurian, and this difficulty was met later on in Lapparent’s Traité by the
proposal to substitute Gothlandian for Silurian. Of this change Geikie
remarks: “Such an arrangement ... might be adopted if it did not involve so
serious an alteration of the nomenclature in general use.” On the other hand,
if diastrophism and breaks in the stratigraphic and faunal sequence are to be
the basis for geologic time divisions, we cannot accept the above scheme,
for it recognizes but one period where there are at least four in nature.
Conclusions.—We have arrived at a time when our knowledge of the
stratigraphic and faunal sequence, plus the orogenic record as recognized in
the principle of diastrophism, should be reflected in the terminology of the
geologic time-table. It would be easy to offer a satisfactory nomenclature if
we were not bound by the law of priority in publication, and if no one had
the geologic chronology of his own time ingrained in his memory. In
addition, the endless literature, with its accepted nomenclature, bars our
way. Therefore with a view of creating the least change in geologic
nomenclature, and of doing the greatest justice to our predecessors that the
present conditions of our knowledge will allow, the following scheme is
offered:
Silurian period. Llandovery to top of Ludlow in Europe. Alexandrian-Cataract-Medina to top of
Manlius in America.
Champlain (1842) or Ordovician (1879) period. Arenig to top of Caradoc in Europe.
Beekmantown to top of Richmondian in America.
Cambrian period. In the Atlantic realm, begins with the Paradoxides, and in the Pacific, with the
Bathyuriscus and Ogygopsis faunas. The close is involved in Ulrich’s provisionally defined Ozarkian
system. When the latter is established, the Ozarkian period will hold the time between the Ordovician
and the Cambrian.
Taconic period. For the world-wide Olenellus or Mesonacidæ faunas.
Barrande, Renevier remarks that it is “as important as the Cretaceous or the
Jurassic. Lapworth even gives it a value of the first order equal to the
Protozoic era.”
In the above there is an obvious objection in the double usage of the term
Silurian, and this difficulty was met later on in Lapparent’s Traité by the
proposal to substitute Gothlandian for Silurian. Of this change Geikie
remarks: “Such an arrangement ... might be adopted if it did not involve so
serious an alteration of the nomenclature in general use.” On the other hand,
if diastrophism and breaks in the stratigraphic and faunal sequence are to be
the basis for geologic time divisions, we cannot accept the above scheme,
for it recognizes but one period where there are at least four in nature.
Conclusions.—We have arrived at a time when our knowledge of the
stratigraphic and faunal sequence, plus the orogenic record as recognized in
the principle of diastrophism, should be reflected in the terminology of the
geologic time-table. It would be easy to offer a satisfactory nomenclature if
we were not bound by the law of priority in publication, and if no one had
the geologic chronology of his own time ingrained in his memory. In
addition, the endless literature, with its accepted nomenclature, bars our
way. Therefore with a view of creating the least change in geologic
nomenclature, and of doing the greatest justice to our predecessors that the
present conditions of our knowledge will allow, the following scheme is
offered:
Silurian period. Llandovery to top of Ludlow in Europe. Alexandrian-Cataract-Medina to top of
Manlius in America.
Champlain (1842) or Ordovician (1879) period. Arenig to top of Caradoc in Europe.
Beekmantown to top of Richmondian in America.
Cambrian period. In the Atlantic realm, begins with the Paradoxides, and in the Pacific, with the
Bathyuriscus and Ogygopsis faunas. The close is involved in Ulrich’s provisionally defined Ozarkian
system. When the latter is established, the Ozarkian period will hold the time between the Ordovician
and the Cambrian.
Taconic period. For the world-wide Olenellus or Mesonacidæ faunas.
Page 105
Paleogeography.
When geologists began to perceive the vast significance of Hutton’s
doctrine that “the ruins of an earlier world lie beneath the secondary strata,”
and that great masses of bedded rocks are separated from one another by
periods of mountain making and by erosion intervals, it was natural for
them to look for the lands that had furnished the debris of the accumulated
sediments. In this way paleogeography had its origin, but it was at first of a
descriptive and not of a cartographic nature.
The word paleogeography was proposed by T. Sterry Hunt in 1872 in a
paper entitled “The Paleogeography of the North American Continent,” and
published in the Journal of the American Geographical Society for that year.
It has to do, he says, with the “geographical history of these ancient
geological periods.” It was again prominently used by Robert Etheridge in
his presidential address before the Geological Society of London in 1881.
Since Canu’s use of the term in 1896, it has been frequently seen in print,
and now is generally adopted to signify the geography of geologic time.
The French were the first to make paleogeographic maps, and Jules
Marcou relates in 1866 that Elie de Beaumont, as early as March, 1831, in
his course in the College of France and at the Paris School of Mines, used
to outline the relation of the lands and the seas in the center of Europe at the
different great geologic periods. His first printed paleogeographic map
appeared in 1833, and was of early Tertiary time. Other maps by Beaumont
were published by Beudant in 1841–1842. The Sicilian geologist
Gemmellaro published six maps of his country in 1834, and the Englishman
De La Beche had one in the same year. In America the first to show such
maps was Arnold Guyot in his Lowell lectures of 1848. James D. Dana
published three in the 1863 edition of his Manual of Geology. Of world
paleogeographic maps, Jules Marcou produced the first of Jurassic time,
publishing it in France in 1866, but the most celebrated of these early
attempts was the one by Neumayr published in 1883 in connection with his
Ueber klimatische Zonen während der Jura- und Kreidezeit.
The first geologist to produce a series of maps showing the progressive
geologic geography of a given area was Jukes-Brown, who in the volume
When geologists began to perceive the vast significance of Hutton’s
doctrine that “the ruins of an earlier world lie beneath the secondary strata,”
and that great masses of bedded rocks are separated from one another by
periods of mountain making and by erosion intervals, it was natural for
them to look for the lands that had furnished the debris of the accumulated
sediments. In this way paleogeography had its origin, but it was at first of a
descriptive and not of a cartographic nature.
The word paleogeography was proposed by T. Sterry Hunt in 1872 in a
paper entitled “The Paleogeography of the North American Continent,” and
published in the Journal of the American Geographical Society for that year.
It has to do, he says, with the “geographical history of these ancient
geological periods.” It was again prominently used by Robert Etheridge in
his presidential address before the Geological Society of London in 1881.
Since Canu’s use of the term in 1896, it has been frequently seen in print,
and now is generally adopted to signify the geography of geologic time.
The French were the first to make paleogeographic maps, and Jules
Marcou relates in 1866 that Elie de Beaumont, as early as March, 1831, in
his course in the College of France and at the Paris School of Mines, used
to outline the relation of the lands and the seas in the center of Europe at the
different great geologic periods. His first printed paleogeographic map
appeared in 1833, and was of early Tertiary time. Other maps by Beaumont
were published by Beudant in 1841–1842. The Sicilian geologist
Gemmellaro published six maps of his country in 1834, and the Englishman
De La Beche had one in the same year. In America the first to show such
maps was Arnold Guyot in his Lowell lectures of 1848. James D. Dana
published three in the 1863 edition of his Manual of Geology. Of world
paleogeographic maps, Jules Marcou produced the first of Jurassic time,
publishing it in France in 1866, but the most celebrated of these early
attempts was the one by Neumayr published in 1883 in connection with his
Ueber klimatische Zonen während der Jura- und Kreidezeit.
The first geologist to produce a series of maps showing the progressive
geologic geography of a given area was Jukes-Brown, who in the volume
Page 106
entitled “The Building of the British Isles,” 1888, included fifteen such
maps. Karpinsky published fourteen maps of Russia, and in 1896 Canu in
his Essai de paléogéographie has fifty-seven of France and Belgium.
Lapparent’s Traité of 1906 is famous for paleogeographic maps, for he has
twenty-three of the world, thirty-four of Europe, twenty-five of France, and
ten taken from other authors. Schuchert in 1910 published fifty-two to
illustrate the paleogeography of North America, and also gave an extended
list of such published maps. Another article on the subject is by Th. Arldt,
“Zur Geschichte der Paläogeographischen Rekonstructionen,” published in
1914. Edgar Dacqué in 1913 also produced a list in his
Paläogeographischen Karten, and two years later appeared his book of 500
pages, Grundlagen und Methoden der Paläogeographie, where the entire
subject is taken up in detail.
Conclusions.—Since 1833 there have been published not less than 500
different paleogeographic maps, and of this number about 210 relate to
North America. Nevertheless paleogeography is still in its infancy, and most
maps embrace too much geologic time, all of them tens of thousands, and
some of them millions of years. The geographic maps of the present show
the conditions of the strand-lines of to-day, and those made fifty years ago
have to be revised again and again if they are to be of value to the mariner
and merchant. Therefore in our future paleogeographic maps the tendency
must ever be toward smaller amounts of geologic time, if we are to show
the actual relation of water to land and the movements of the periodic
floodings. Moreover, the ancient shore lines are all more or less hypothetic
and are drawn in straight or sweeping curves, unlike modern strands with
their bays, deltas, and headlands, and the ancient lands are featureless
plains. We must also pay more attention to the distribution of brackish- and
fresh-water deposits. The periodically rising mountains will be the first
topographic features to be shown upon the ancient lands, and then more and
more of the drainage and the general climatic conditions must be portrayed.
In the seas, depth, temperature, and currents are yet to be deciphered.
Finally, other base maps than those of the geography of to-day will have to
be made, allowing for the compression of the mountainous areas, if we are
to show the true geographic configurations of the lands and seas of any
given geologic time.
maps. Karpinsky published fourteen maps of Russia, and in 1896 Canu in
his Essai de paléogéographie has fifty-seven of France and Belgium.
Lapparent’s Traité of 1906 is famous for paleogeographic maps, for he has
twenty-three of the world, thirty-four of Europe, twenty-five of France, and
ten taken from other authors. Schuchert in 1910 published fifty-two to
illustrate the paleogeography of North America, and also gave an extended
list of such published maps. Another article on the subject is by Th. Arldt,
“Zur Geschichte der Paläogeographischen Rekonstructionen,” published in
1914. Edgar Dacqué in 1913 also produced a list in his
Paläogeographischen Karten, and two years later appeared his book of 500
pages, Grundlagen und Methoden der Paläogeographie, where the entire
subject is taken up in detail.
Conclusions.—Since 1833 there have been published not less than 500
different paleogeographic maps, and of this number about 210 relate to
North America. Nevertheless paleogeography is still in its infancy, and most
maps embrace too much geologic time, all of them tens of thousands, and
some of them millions of years. The geographic maps of the present show
the conditions of the strand-lines of to-day, and those made fifty years ago
have to be revised again and again if they are to be of value to the mariner
and merchant. Therefore in our future paleogeographic maps the tendency
must ever be toward smaller amounts of geologic time, if we are to show
the actual relation of water to land and the movements of the periodic
floodings. Moreover, the ancient shore lines are all more or less hypothetic
and are drawn in straight or sweeping curves, unlike modern strands with
their bays, deltas, and headlands, and the ancient lands are featureless
plains. We must also pay more attention to the distribution of brackish- and
fresh-water deposits. The periodically rising mountains will be the first
topographic features to be shown upon the ancient lands, and then more and
more of the drainage and the general climatic conditions must be portrayed.
In the seas, depth, temperature, and currents are yet to be deciphered.
Finally, other base maps than those of the geography of to-day will have to
be made, allowing for the compression of the mountainous areas, if we are
to show the true geographic configurations of the lands and seas of any
given geologic time.
Page 107
Paleometeorology.
In accordance with the Laplacian theory, announced at the beginning of
the nineteenth century, all of the older geologists held that the earth began
as a hot star, and that in the course of time it slowly cooled and finally
attained its present zonal cold to tropical climatic conditions. That the earth
had very recently passed through a much colder climate, a glacial one, came
into general acceptance only during the latter half of the previous century.
Rise.—Our knowledge of glacial climates had its origin in the Alps, that
wonderland of mountains and glaciers. The rise of this knowledge in the
Alps is told in a charming and detailed manner by that erratic French-
American geologist, Jules Marcou (1824–1898), in his Life, Letters, and
Works of Louis Agassiz, 1896. He relates that the Alpine chamois hunter
Perraudin in 1815 directed the attention of the engineer De Charpentier to
the fact “that the large boulders perched on the sides of the Alpine valleys
were carried and left there by glaciers.” For a long time the latter thought
the conclusion extravagant, and in the meantime Perraudin told the same
thing to another engineer, Venetz. He, in 1829, convinced of the correctness
of the chamois hunter’s views, presented the matter before the Swiss
naturalists then meeting at St. Bernard’s. Venetz “told the Society that his
observations led him to believe that the whole Valais has been formerly
covered by an immense glacier and that it even extended outside of the
canton, covering all the Canton de Vaud, as far as the Jura Mountains,
carrying the boulders and erratic materials, which are now scattered all over
the large Swiss valley.” Eight years earlier, in 1821, similar views had been
presented by the same modest naturalist before the Helvetic Society, but it
was not until 1833 that De Charpentier found the manuscript and had it
published. Venetz’s conclusions were that all of the glaciers of the Bagnes
valley “have very recognizable moraines, which are about a league from the
present ice.” “The moraines ... date from an epoch which is lost in the night
of time.” Then in 1834 De Charpentier read a paper before the same society,
meeting at Lucerne. “Seldom, if ever, has such a small memoir so deeply
excited the scientific world. It was received at first with incredulity and
even scorn and mockery, Agassiz being among its opponents.” The paper
was published in 1835, first at Paris, then at Geneva, and finally in
In accordance with the Laplacian theory, announced at the beginning of
the nineteenth century, all of the older geologists held that the earth began
as a hot star, and that in the course of time it slowly cooled and finally
attained its present zonal cold to tropical climatic conditions. That the earth
had very recently passed through a much colder climate, a glacial one, came
into general acceptance only during the latter half of the previous century.
Rise.—Our knowledge of glacial climates had its origin in the Alps, that
wonderland of mountains and glaciers. The rise of this knowledge in the
Alps is told in a charming and detailed manner by that erratic French-
American geologist, Jules Marcou (1824–1898), in his Life, Letters, and
Works of Louis Agassiz, 1896. He relates that the Alpine chamois hunter
Perraudin in 1815 directed the attention of the engineer De Charpentier to
the fact “that the large boulders perched on the sides of the Alpine valleys
were carried and left there by glaciers.” For a long time the latter thought
the conclusion extravagant, and in the meantime Perraudin told the same
thing to another engineer, Venetz. He, in 1829, convinced of the correctness
of the chamois hunter’s views, presented the matter before the Swiss
naturalists then meeting at St. Bernard’s. Venetz “told the Society that his
observations led him to believe that the whole Valais has been formerly
covered by an immense glacier and that it even extended outside of the
canton, covering all the Canton de Vaud, as far as the Jura Mountains,
carrying the boulders and erratic materials, which are now scattered all over
the large Swiss valley.” Eight years earlier, in 1821, similar views had been
presented by the same modest naturalist before the Helvetic Society, but it
was not until 1833 that De Charpentier found the manuscript and had it
published. Venetz’s conclusions were that all of the glaciers of the Bagnes
valley “have very recognizable moraines, which are about a league from the
present ice.” “The moraines ... date from an epoch which is lost in the night
of time.” Then in 1834 De Charpentier read a paper before the same society,
meeting at Lucerne. “Seldom, if ever, has such a small memoir so deeply
excited the scientific world. It was received at first with incredulity and
even scorn and mockery, Agassiz being among its opponents.” The paper
was published in 1835, first at Paris, then at Geneva, and finally in
Page 108
Germany. It “attracted much attention, and the smile of incredulity with
which it was received when read at Lucerne soon changed into a desire to
know more about it.”
Louis Agassiz (1807–1873), who had long been acquainted with his
countryman, De Charpentier, spent several months with him in 1836, and
together they studied the glaciers of the Alps. Agassiz was at first “adverse
to the hypothesis, and did not believe in the great extension of glaciers and
their transportation of boulders, but on the contrary, was a partisan of
Lyell’s theory of transport by icebergs and ice-cakes ... but from being an
adversary of the glacial theory, he returned to Neuchâtel an enthusiastic
convert to the views of Venetz and De Charpentier.... With his power of
quick perception, his unmatched memory, his perspicacity and acuteness,
his way of classifying, judging and marshalling facts, Agassiz promptly
learned the whole mass of irresistible arguments collected patiently during
seven years by De Charpentier and Venetz, and with his insatiable appetite
and that faculty of assimilation which he possessed in such a wonderful
degree, he digested the whole doctrine of the glaciers in a few weeks.”
In July, 1837, Agassiz presented as his presidential address before the
Helvetic Society his memorable “Discours de Neuchâtel,” which was “the
starting point of all that has been written on the Ice-age,”—a term coined at
the time by his friend Schimper, a botanist. The first part of this address is
reprinted in French in Marcou’s book on Agassiz. The address was received
with astonishment, much incredulity, and indifference. Among the listeners
was the great German geologist Von Buch, who “was horrified, and with his
hands raised towards the sky, and his head bowed to the distant Bernese
Alps, exclaimed: ‘O Sancte de Saussure, ora pro nobis!’” Even De
Charpentier “was not gratified to see his glacial theory mixed with rather
uncalled for biological problems, the connection of which with the glacial
age was more than problematic.” Agassiz was then a Cuvierian catastrophist
and creationist, and advanced the idea of a series of glacial ages to explain
the destruction of the geologic succession of faunas! Curiously, this theory
was at once accepted by the American paleontologist T. A. Conrad (35, 239,
1839).
The classics in glacial geology are Agassiz’s Etudes sur les Glaciers,
1840, and De Charpentier’s Essai sur les Glaciers, 1841. Of the latter book,
Marcou states that it has been said: “It is impossible to be truly a geologist
which it was received when read at Lucerne soon changed into a desire to
know more about it.”
Louis Agassiz (1807–1873), who had long been acquainted with his
countryman, De Charpentier, spent several months with him in 1836, and
together they studied the glaciers of the Alps. Agassiz was at first “adverse
to the hypothesis, and did not believe in the great extension of glaciers and
their transportation of boulders, but on the contrary, was a partisan of
Lyell’s theory of transport by icebergs and ice-cakes ... but from being an
adversary of the glacial theory, he returned to Neuchâtel an enthusiastic
convert to the views of Venetz and De Charpentier.... With his power of
quick perception, his unmatched memory, his perspicacity and acuteness,
his way of classifying, judging and marshalling facts, Agassiz promptly
learned the whole mass of irresistible arguments collected patiently during
seven years by De Charpentier and Venetz, and with his insatiable appetite
and that faculty of assimilation which he possessed in such a wonderful
degree, he digested the whole doctrine of the glaciers in a few weeks.”
In July, 1837, Agassiz presented as his presidential address before the
Helvetic Society his memorable “Discours de Neuchâtel,” which was “the
starting point of all that has been written on the Ice-age,”—a term coined at
the time by his friend Schimper, a botanist. The first part of this address is
reprinted in French in Marcou’s book on Agassiz. The address was received
with astonishment, much incredulity, and indifference. Among the listeners
was the great German geologist Von Buch, who “was horrified, and with his
hands raised towards the sky, and his head bowed to the distant Bernese
Alps, exclaimed: ‘O Sancte de Saussure, ora pro nobis!’” Even De
Charpentier “was not gratified to see his glacial theory mixed with rather
uncalled for biological problems, the connection of which with the glacial
age was more than problematic.” Agassiz was then a Cuvierian catastrophist
and creationist, and advanced the idea of a series of glacial ages to explain
the destruction of the geologic succession of faunas! Curiously, this theory
was at once accepted by the American paleontologist T. A. Conrad (35, 239,
1839).
The classics in glacial geology are Agassiz’s Etudes sur les Glaciers,
1840, and De Charpentier’s Essai sur les Glaciers, 1841. Of the latter book,
Marcou states that it has been said: “It is impossible to be truly a geologist
Page 109
without having read and studied it.” In the English language there is
Tyndall’s Glaciers of the Alps, 1860.
The progress of the ideas in regard to Pleistocene glaciation is presented
in the following chapter by H. E. Gregory.
Older Glacial Climates.—Hardly had the Pleistocene glacial climate
been proved, when geologists began to point out the possibility of even
earlier ones. An enthusiastic Scotch writer, Sir Andrew Ramsay, in 1855
described certain late Paleozoic conglomerates of middle England, which
he said were of glacial origin, but his evidence, though never completely
gainsaid, has not been generally accepted. In the following year, an
Englishman, Doctor W. T. Blanford, said that the Talchir conglomerates of
central and southern India were of glacial origin, and since then the
evidence for a Permian glacial climate has been steadily accumulating.
Africa is the land of tillites, and here in 1870 Sutherland pointed out that the
conglomerates of the Karroo formation were of glacial origin. Australia also
has Permian glacial deposits, and they are known widely in eastern Brazil,
the Falkland Islands, the vicinity of Boston, and elsewhere. So convincing
is this testimony that all geologists are now ready to accept the conclusion
that a glacial climate was as wide-spread in early Permian time as was that
of the Pleistocene.[3]
In South Africa, beneath the marine Lower Devonian, occurs the Table
Mountain series, 5000 feet thick. The series is essentially one of quartzites,
with zones of shales or slates and with striated pebbles up to 15 inches long.
The latter occur in pockets and seem to be of glacial origin. There are here
no typical tillites, and no striated undergrounds have so far been found.
While the evidence of the deposits appears to favor the conclusion that the
Table Mountain strata were laid down in cold waters with floating ice
derived from glaciers, it is as yet impossible to assign these sediments a
definite geologic age. They are certainly not younger than the Lower
Devonian, but it has not yet been established to what period of the early
Paleozoic they belong.
In southeastern Australia occur tillites of wide distribution that lie
conformably beneath, but sharply separated from the fossiliferous marine
Lower Cambrian strata. David (1907), Howchin (1908), and other
Australian geologists think they are of Cambrian time, but to the writer they
seem more probably late Proterozoic in age. In arctic Norway Reusch
Tyndall’s Glaciers of the Alps, 1860.
The progress of the ideas in regard to Pleistocene glaciation is presented
in the following chapter by H. E. Gregory.
Older Glacial Climates.—Hardly had the Pleistocene glacial climate
been proved, when geologists began to point out the possibility of even
earlier ones. An enthusiastic Scotch writer, Sir Andrew Ramsay, in 1855
described certain late Paleozoic conglomerates of middle England, which
he said were of glacial origin, but his evidence, though never completely
gainsaid, has not been generally accepted. In the following year, an
Englishman, Doctor W. T. Blanford, said that the Talchir conglomerates of
central and southern India were of glacial origin, and since then the
evidence for a Permian glacial climate has been steadily accumulating.
Africa is the land of tillites, and here in 1870 Sutherland pointed out that the
conglomerates of the Karroo formation were of glacial origin. Australia also
has Permian glacial deposits, and they are known widely in eastern Brazil,
the Falkland Islands, the vicinity of Boston, and elsewhere. So convincing
is this testimony that all geologists are now ready to accept the conclusion
that a glacial climate was as wide-spread in early Permian time as was that
of the Pleistocene.[3]
In South Africa, beneath the marine Lower Devonian, occurs the Table
Mountain series, 5000 feet thick. The series is essentially one of quartzites,
with zones of shales or slates and with striated pebbles up to 15 inches long.
The latter occur in pockets and seem to be of glacial origin. There are here
no typical tillites, and no striated undergrounds have so far been found.
While the evidence of the deposits appears to favor the conclusion that the
Table Mountain strata were laid down in cold waters with floating ice
derived from glaciers, it is as yet impossible to assign these sediments a
definite geologic age. They are certainly not younger than the Lower
Devonian, but it has not yet been established to what period of the early
Paleozoic they belong.
In southeastern Australia occur tillites of wide distribution that lie
conformably beneath, but sharply separated from the fossiliferous marine
Lower Cambrian strata. David (1907), Howchin (1908), and other
Australian geologists think they are of Cambrian time, but to the writer they
seem more probably late Proterozoic in age. In arctic Norway Reusch
Page 110
discovered unmistakable tillites in 1891, and this occurrence was confirmed
by Strahan in 1897. It is not yet certainly known what their age is, but it
appears to be late Proterozoic rather than early Paleozoic. Other undated
Proterozoic tillites occur in China (Willis and Blackwelder 1907), Africa
(Schwarz 1906), India (Vredenburg 1907), Canada (Coleman 1908), and
possibly in Scotland.
The oldest known tillites are described by Coleman in 1907, and occur at
the base of the Lower Huronian or in early Proterozoic time. They extend
across northern Ontario for 1000 miles, and from the north shore of Lake
Huron northward for 750 miles.
Fossils as Climatic Indexes.—Paleontologists have long been aware that
variations in the climates of the past are indicated by the fossils, and
Neumayr in 1883 brought the evidence together in his study of climatic
zones mentioned elsewhere. Plants, and corals, cephalopods, and
foraminifers among marine animals, have long been recognized as
particularly good “life thermometers.” In fact, all fossils are climatic
indicators to some extent, and a good deal of evidence concerning
paleometeorology has been discerned in them. This evidence is briefly
stated in the paper by Schuchert already alluded to, and in W. D. Matthew’s
Climate and Evolution, 1915.
Sediments as Climatic Indexes.—Johannes Walther in the third part of his
Einleitung—Lithogenesis der Gegenwart, 1894—is the first one to
decidedly direct attention to the fact that the sediments also have within
themselves a climatic record. In America Joseph Barrell has since 1907
written much on the same subject. On the other hand, the periodic floodings
of the continents by the oceans, and the making of mountains, due to the
periodic shrinkage of the earth, as expressed in T. C. Chamberlin’s principle
of diastrophism and in his publications since 1897, are other criteria for
estimating the climates of the past.
Conclusions.—In summation of this subject Schuchert says:
“The marine ‘life thermometer’ indicates vast stretches of time of mild to warm and equable
temperatures, with but slight zonal differences between the equator and the poles. The great bulk of
marine fossils are those of the shallow seas, and the evolutionary changes recorded in these ‘medals
of creation’ are slight throughout vast lengths of time that are punctuated by short but decisive
periods of cooled waters and great mortality, followed by quick evolution, and the rise of new stocks.
The times of less warmth are the miotherm and those of greater heat the pliotherm periods of
Ramsay.
by Strahan in 1897. It is not yet certainly known what their age is, but it
appears to be late Proterozoic rather than early Paleozoic. Other undated
Proterozoic tillites occur in China (Willis and Blackwelder 1907), Africa
(Schwarz 1906), India (Vredenburg 1907), Canada (Coleman 1908), and
possibly in Scotland.
The oldest known tillites are described by Coleman in 1907, and occur at
the base of the Lower Huronian or in early Proterozoic time. They extend
across northern Ontario for 1000 miles, and from the north shore of Lake
Huron northward for 750 miles.
Fossils as Climatic Indexes.—Paleontologists have long been aware that
variations in the climates of the past are indicated by the fossils, and
Neumayr in 1883 brought the evidence together in his study of climatic
zones mentioned elsewhere. Plants, and corals, cephalopods, and
foraminifers among marine animals, have long been recognized as
particularly good “life thermometers.” In fact, all fossils are climatic
indicators to some extent, and a good deal of evidence concerning
paleometeorology has been discerned in them. This evidence is briefly
stated in the paper by Schuchert already alluded to, and in W. D. Matthew’s
Climate and Evolution, 1915.
Sediments as Climatic Indexes.—Johannes Walther in the third part of his
Einleitung—Lithogenesis der Gegenwart, 1894—is the first one to
decidedly direct attention to the fact that the sediments also have within
themselves a climatic record. In America Joseph Barrell has since 1907
written much on the same subject. On the other hand, the periodic floodings
of the continents by the oceans, and the making of mountains, due to the
periodic shrinkage of the earth, as expressed in T. C. Chamberlin’s principle
of diastrophism and in his publications since 1897, are other criteria for
estimating the climates of the past.
Conclusions.—In summation of this subject Schuchert says:
“The marine ‘life thermometer’ indicates vast stretches of time of mild to warm and equable
temperatures, with but slight zonal differences between the equator and the poles. The great bulk of
marine fossils are those of the shallow seas, and the evolutionary changes recorded in these ‘medals
of creation’ are slight throughout vast lengths of time that are punctuated by short but decisive
periods of cooled waters and great mortality, followed by quick evolution, and the rise of new stocks.
The times of less warmth are the miotherm and those of greater heat the pliotherm periods of
Ramsay.
Page 111
On the land the story of the climatic changes is different, but in general the equability of the
temperature simulates that of the oceanic areas. In other words, the lands also had long-enduring
times of mild to warm climates. Into the problem of land climates, however, enter other factors that
are absent in the oceanic regions, and these have great influence upon the climates of the continents.
Most important of these is the periodic warm-water inundation of the continents by the oceans,
causing insular climates that are milder and moister. With the vanishing of the floods somewhat
cooler and certainly drier climates are produced. The effects of these periodic floods must not be
underestimated, for the North American continent was variably submerged at least seventeen times,
and over an area of from 154,000 to 4,000,000 square miles.
When to these factors is added the effect upon the climate caused by the periodic rising of
mountain chains, it is at once apparent that the lands must have had constantly varying climates. In
general the temperature fluctuations seem to have been slight, but geographically the climates varied
between mild to warm pluvial, and mild to cool arid. The arid factor has been of the greatest import
to the organic world of the lands. Further, when to all of these causes is added the fact that during
emergent periods the formerly isolated lands were connected by land bridges, permitting
intermigration of the land floras and faunas, with the introduction of their parasites and parasitic
diseases, we learn that while the climatic environment is of fundamental importance it is not the only
cause for the more rapid evolution of terrestrial life....
Briefly, then, we may conclude that the markedly varying climates of the past seem to be due
primarily to periodic changes in the topographic form of the earth’s surface, plus variations in the
amount of heat stored by the oceans. The causation for the warmer interglacial climates is the most
difficult of all to explain, and it is here that factors other than those mentioned may enter.
Granting all this, there still seems to lie back of all these theories a greater question connected with
the major changes in paleometeorology. This is: What is it that forces the earth’s topography to
change with varying intensity at irregularly rhythmic intervals?... Are we not forced to conclude that
the earth’s shape changes periodically in response to gravitative forces that alter the body-form?”
temperature simulates that of the oceanic areas. In other words, the lands also had long-enduring
times of mild to warm climates. Into the problem of land climates, however, enter other factors that
are absent in the oceanic regions, and these have great influence upon the climates of the continents.
Most important of these is the periodic warm-water inundation of the continents by the oceans,
causing insular climates that are milder and moister. With the vanishing of the floods somewhat
cooler and certainly drier climates are produced. The effects of these periodic floods must not be
underestimated, for the North American continent was variably submerged at least seventeen times,
and over an area of from 154,000 to 4,000,000 square miles.
When to these factors is added the effect upon the climate caused by the periodic rising of
mountain chains, it is at once apparent that the lands must have had constantly varying climates. In
general the temperature fluctuations seem to have been slight, but geographically the climates varied
between mild to warm pluvial, and mild to cool arid. The arid factor has been of the greatest import
to the organic world of the lands. Further, when to all of these causes is added the fact that during
emergent periods the formerly isolated lands were connected by land bridges, permitting
intermigration of the land floras and faunas, with the introduction of their parasites and parasitic
diseases, we learn that while the climatic environment is of fundamental importance it is not the only
cause for the more rapid evolution of terrestrial life....
Briefly, then, we may conclude that the markedly varying climates of the past seem to be due
primarily to periodic changes in the topographic form of the earth’s surface, plus variations in the
amount of heat stored by the oceans. The causation for the warmer interglacial climates is the most
difficult of all to explain, and it is here that factors other than those mentioned may enter.
Granting all this, there still seems to lie back of all these theories a greater question connected with
the major changes in paleometeorology. This is: What is it that forces the earth’s topography to
change with varying intensity at irregularly rhythmic intervals?... Are we not forced to conclude that
the earth’s shape changes periodically in response to gravitative forces that alter the body-form?”
Page 112
Evolution.
Modern evolution, or the theory of life continuously descending from life
with change, may be said to have had its first marked development in
Comte de Buffon (1707–1788), a man of wealth and station, yet an
industrious compiler, a brilliant writer, and a popularizer of science. He was
not, however, a true scientific investigator, and his monument to fame is his
Histoire Naturelle, in forty-four volumes, 1749–1804. A. S. Packard in his
book on Lamarck, his Life and Work, 1901, concludes in regard to Buffon
as follows:
“The impression left on the mind, after reading Buffon, is that even if he threw out these
suggestions and then retracted them, from fear of annoyance or even persecution from the bigots of
his time, he did not himself always take them seriously, but rather jotted them down as passing
thoughts.... They appeared thirty-four years before Lamarck’s theory, and though not epoch-making,
they are such as will render the name of Buffon memorable for all time.”
Chevalier de Lamarck (1744–1829) may justly be regarded as the
founder of the doctrine of modern evolution. Previous to 1794 he was a
believer in the fixity of species, but by 1800 he stood definitely in favor of
evolution. Locy in his Biology and its Makers, 1908, states his theories in
the following simplified form:
“Variations of organs, according to Lamarck, arise in animals mainly through use and disuse, and
new organs have their origin in a physiological need. A new need felt by the animal [due to new
conditions in its life, or the environment] expresses itself on the organism, stimulating growth and
adaptations in a particular direction.”
To Lamarck, “inheritance was a simple, direct transmission of those
superficial changes that arise in organs within the lifetime of an individual
owing to use and disuse.” This part of his theory has come to be known as
“the inheritance of acquired characters.”
Georges Cuvier (1769–1832), a peer of France, was a decided believer in
the fixity of species and in their creation through divine acts. In 1796 he
began to see that among the fossils so plentiful about Paris many were of
Modern evolution, or the theory of life continuously descending from life
with change, may be said to have had its first marked development in
Comte de Buffon (1707–1788), a man of wealth and station, yet an
industrious compiler, a brilliant writer, and a popularizer of science. He was
not, however, a true scientific investigator, and his monument to fame is his
Histoire Naturelle, in forty-four volumes, 1749–1804. A. S. Packard in his
book on Lamarck, his Life and Work, 1901, concludes in regard to Buffon
as follows:
“The impression left on the mind, after reading Buffon, is that even if he threw out these
suggestions and then retracted them, from fear of annoyance or even persecution from the bigots of
his time, he did not himself always take them seriously, but rather jotted them down as passing
thoughts.... They appeared thirty-four years before Lamarck’s theory, and though not epoch-making,
they are such as will render the name of Buffon memorable for all time.”
Chevalier de Lamarck (1744–1829) may justly be regarded as the
founder of the doctrine of modern evolution. Previous to 1794 he was a
believer in the fixity of species, but by 1800 he stood definitely in favor of
evolution. Locy in his Biology and its Makers, 1908, states his theories in
the following simplified form:
“Variations of organs, according to Lamarck, arise in animals mainly through use and disuse, and
new organs have their origin in a physiological need. A new need felt by the animal [due to new
conditions in its life, or the environment] expresses itself on the organism, stimulating growth and
adaptations in a particular direction.”
To Lamarck, “inheritance was a simple, direct transmission of those
superficial changes that arise in organs within the lifetime of an individual
owing to use and disuse.” This part of his theory has come to be known as
“the inheritance of acquired characters.”
Georges Cuvier (1769–1832), a peer of France, was a decided believer in
the fixity of species and in their creation through divine acts. In 1796 he
began to see that among the fossils so plentiful about Paris many were of
Page 113
extinct forms, and later on that there was a succession of wholly extinct
faunas. This at first puzzling phenomenon he finally came to explain by
assuming that the earth had gone through a series of catastrophes, of which
the Deluge was the most recent but possibly not the last. With each
catastrophe all life was blotted out, and a new though improved set of
organisms was created by divine acts. The Cuvierian theory of
catastrophism was widely accepted during the first half of the nineteenth
century, and in America Louis Agassiz was long its greatest exponent. It
was this theory and the dominance of the brilliant Cuvier, not only in
science but socially as well, that blotted out the far more correct views of
the more philosophical Lamarck, who held that life throughout the ages had
been continuous and that through individual effort and the inheritance of
acquired characters had evolved the wonderful diversity of the present
living world.
In 1830 there was a public debate at Paris between Cuvier and Geoffroy
Saint-Hilaire, the one holding to the views of the fixity of species and
creation, the other that life is continuous and evolves into better adapted
forms. Cuvier, a gifted speaker and the greatest debater zoology ever had,
with an extraordinary memory that never failed him, defeated Saint-Hilaire
in each day’s debate, although the latter was in the right.
A book that did a great deal to prepare the English-speaking people for
the coming of evolution was “Vestiges of Creation,” published in 1844 by
an unknown author. In Darwin’s opinion, “the work, from its powerful and
brilliant style ... has done excellent service ... in thus preparing the ground
for the reception of analogous views.” This book was recommended to the
readers of the Journal (48, 395, 1845) with the editorial remark that “we
cannot subscribe to all of the author’s views.”
We can probably best illustrate the opinions of Americans on the question
of evolution just before the appearance of Darwin’s great work by directing
attention to James D. Dana’s Thoughts on Species (24, 305, 1857). After
reading this article and others of a similar nature by Agassiz, one comes to
the opinion that unconsciously both men are proving evolution, but
consciously they are firm creationists. It is astonishing that with their
extended and minute knowledge of living organisms and their philosophic
type of mind neither could see the true significance of the imperceptible
faunas. This at first puzzling phenomenon he finally came to explain by
assuming that the earth had gone through a series of catastrophes, of which
the Deluge was the most recent but possibly not the last. With each
catastrophe all life was blotted out, and a new though improved set of
organisms was created by divine acts. The Cuvierian theory of
catastrophism was widely accepted during the first half of the nineteenth
century, and in America Louis Agassiz was long its greatest exponent. It
was this theory and the dominance of the brilliant Cuvier, not only in
science but socially as well, that blotted out the far more correct views of
the more philosophical Lamarck, who held that life throughout the ages had
been continuous and that through individual effort and the inheritance of
acquired characters had evolved the wonderful diversity of the present
living world.
In 1830 there was a public debate at Paris between Cuvier and Geoffroy
Saint-Hilaire, the one holding to the views of the fixity of species and
creation, the other that life is continuous and evolves into better adapted
forms. Cuvier, a gifted speaker and the greatest debater zoology ever had,
with an extraordinary memory that never failed him, defeated Saint-Hilaire
in each day’s debate, although the latter was in the right.
A book that did a great deal to prepare the English-speaking people for
the coming of evolution was “Vestiges of Creation,” published in 1844 by
an unknown author. In Darwin’s opinion, “the work, from its powerful and
brilliant style ... has done excellent service ... in thus preparing the ground
for the reception of analogous views.” This book was recommended to the
readers of the Journal (48, 395, 1845) with the editorial remark that “we
cannot subscribe to all of the author’s views.”
We can probably best illustrate the opinions of Americans on the question
of evolution just before the appearance of Darwin’s great work by directing
attention to James D. Dana’s Thoughts on Species (24, 305, 1857). After
reading this article and others of a similar nature by Agassiz, one comes to
the opinion that unconsciously both men are proving evolution, but
consciously they are firm creationists. It is astonishing that with their
extended and minute knowledge of living organisms and their philosophic
type of mind neither could see the true significance of the imperceptible
Page 114
transitions between some species, which if they do not actually pass into, at
least shade towards, one another.
Dana speaks of “the endless diversities in individuals” that compose a
species, and then states that a living species, like an inorganic one, “is based
on a specific amount or condition of concentered force defined in the act or
law of creation.” Species, he says, are permanent, and hybrids “cannot
seriously trifle with the true units of nature, and at the best, can only make
temporary variations.” “We have therefore reason to believe from man’s
fertile intermixture, that he is one in species: and that all organic species are
divine appointments which cannot be obliterated, unless by annihilating the
individuals representing the species.”
Through the activities of the French the world was prepared for the
reception of evolution, and now it was already in the minds of many
advanced thinkers. In 1860 Asa Gray sent to the editor of the Journal (29, 1)
an article by the English botanist, Joseph D. Hooker, entitled “On the
Origination and Distribution of Species,” with these significant remarks:
“The essay cannot fail to attract the immediate and profound attention of scientific men.... It has
for some time been manifest that a re-statement of the Lamarckian hypothesis is at hand. We have
this, in an improved and truly scientific form, in the theories which, recently propounded by Mr.
Darwin, followed by Mr. Wallace, are here so ably and altogether independently maintained. When
these views are fully laid before them, the naturalists of this country will be able to take part in the
interesting discussion which they will not fail to call forth.”
Hooker took up a study of the flora of Tasmania, of which the above
cited article is but a chapter, with a view to trying out Darwin’s theory, and
he now accepts it. He says, “Species are derivative and mutable.” “The
limits of the majority of species are so undefinable that few naturalists are
agreed upon them.”
Asa Gray had received from Darwin an advance copy of the book that
was to revolutionize the thought of the world, and at once wrote for the
Journal a Review of Darwin’s Theory on the Origin of Species by means of
Natural Selection (29, 153, 1860). This is a splendid, critical but just,
scientific review of Darwin’s epoch-making book. Evidently views similar
to those, of the English scientist had long been in the mind of Gray, for he
easily and quickly mastered the work. He is easy on Dana’s Thoughts on
Species, which were idealistic and not in harmony with the naturalistic
least shade towards, one another.
Dana speaks of “the endless diversities in individuals” that compose a
species, and then states that a living species, like an inorganic one, “is based
on a specific amount or condition of concentered force defined in the act or
law of creation.” Species, he says, are permanent, and hybrids “cannot
seriously trifle with the true units of nature, and at the best, can only make
temporary variations.” “We have therefore reason to believe from man’s
fertile intermixture, that he is one in species: and that all organic species are
divine appointments which cannot be obliterated, unless by annihilating the
individuals representing the species.”
Through the activities of the French the world was prepared for the
reception of evolution, and now it was already in the minds of many
advanced thinkers. In 1860 Asa Gray sent to the editor of the Journal (29, 1)
an article by the English botanist, Joseph D. Hooker, entitled “On the
Origination and Distribution of Species,” with these significant remarks:
“The essay cannot fail to attract the immediate and profound attention of scientific men.... It has
for some time been manifest that a re-statement of the Lamarckian hypothesis is at hand. We have
this, in an improved and truly scientific form, in the theories which, recently propounded by Mr.
Darwin, followed by Mr. Wallace, are here so ably and altogether independently maintained. When
these views are fully laid before them, the naturalists of this country will be able to take part in the
interesting discussion which they will not fail to call forth.”
Hooker took up a study of the flora of Tasmania, of which the above
cited article is but a chapter, with a view to trying out Darwin’s theory, and
he now accepts it. He says, “Species are derivative and mutable.” “The
limits of the majority of species are so undefinable that few naturalists are
agreed upon them.”
Asa Gray had received from Darwin an advance copy of the book that
was to revolutionize the thought of the world, and at once wrote for the
Journal a Review of Darwin’s Theory on the Origin of Species by means of
Natural Selection (29, 153, 1860). This is a splendid, critical but just,
scientific review of Darwin’s epoch-making book. Evidently views similar
to those, of the English scientist had long been in the mind of Gray, for he
easily and quickly mastered the work. He is easy on Dana’s Thoughts on
Species, which were idealistic and not in harmony with the naturalistic
Page 115
views of Darwin. On the other hand, he contrasts Darwin’s views at length
with those of the creationists as exemplified by Louis Agassiz, and says
“The widest divergence appears.”
Gray says in part:
“The gist of Mr. Darwin’s work is to show that such varieties are gradually diverged into species
and genera through natural selection; that natural selection is the inevitable result of the struggle for
existence which all living things are engaged in; and that this struggle is an unavoidable consequence
of several natural causes, but mainly of the high rate at which all organic beings tend to increase.
Darwin is confident that intermediate forms must have existed; that in the olden times when the
genera, the families and the orders diverged from their parent stocks, gradations existed as fine as
those which now connect closely related species with varieties. But they have passed and left no sign.
The geological record, even if all displayed to view, is a book from which not only many pages, but
even whole alternate chapters have been lost out, or rather which were never printed from the
autographs of nature. The record was actually made in fossil lithography only at certain times and
under certain conditions (i.e., at periods of slow subsidence and places of abundant sediment); and of
these records all but the last volume is out of print; and of its pages only local glimpses have been
obtained. Geologists, except Lyell, will object to this,—some of them moderately, others with
vehemence. Mr. Darwin himself admits, with a candor rarely displayed on such occasions, that he
should have expected more geological evidence of transition than he finds, and that all the most
eminent paleontologists maintain the immutability of species.
The general fact, however, that the fossil fauna of each period as a whole is nearly intermediate in
character between the preceding and the succeeding faunas, is much relied on. We are brought one
step nearer to the desired inference by the similar ‘fact,’ insisted on by all paleontologists, that fossils
from two consecutive formations are far more closely related to each other, than are the fossils of two
remote formations.
It is well said that all organic beings have been formed on two great laws; Unity of type, and
Adaptation to the conditions of existence.... Mr. Darwin harmonizes and explains them naturally.
Adaptation to the conditions of existence is the result of Natural Selection; Unity of type, of unity of
descent.”
Gray’s article was soon followed by another one from Agassiz on
Individuality and Specific Differences among Acalephs, but the running
title is “Prof. Agassiz on the Origin of Species” (30, 142, 1860). Agassiz
stoutly maintains his well known views, and concludes as follows:
“Were the transmutation theory true, the geological record should exhibit an uninterrupted
succession of types blending gradually into one another. The fact is that throughout all geological
times each period is characterized by definite specific types, belonging to definite genera, and these
to definite families, referable to definite orders, constituting definite classes and definite branches,
built upon definite plans. Until the facts of Nature are shown to have been mistaken by those who
have collected them, and that they have a different meaning from that now generally assigned to
them, I shall therefore consider the transmutation theory as a scientific mistake, untrue in its facts,
unscientific in its method, and mischievous in its tendency.”
with those of the creationists as exemplified by Louis Agassiz, and says
“The widest divergence appears.”
Gray says in part:
“The gist of Mr. Darwin’s work is to show that such varieties are gradually diverged into species
and genera through natural selection; that natural selection is the inevitable result of the struggle for
existence which all living things are engaged in; and that this struggle is an unavoidable consequence
of several natural causes, but mainly of the high rate at which all organic beings tend to increase.
Darwin is confident that intermediate forms must have existed; that in the olden times when the
genera, the families and the orders diverged from their parent stocks, gradations existed as fine as
those which now connect closely related species with varieties. But they have passed and left no sign.
The geological record, even if all displayed to view, is a book from which not only many pages, but
even whole alternate chapters have been lost out, or rather which were never printed from the
autographs of nature. The record was actually made in fossil lithography only at certain times and
under certain conditions (i.e., at periods of slow subsidence and places of abundant sediment); and of
these records all but the last volume is out of print; and of its pages only local glimpses have been
obtained. Geologists, except Lyell, will object to this,—some of them moderately, others with
vehemence. Mr. Darwin himself admits, with a candor rarely displayed on such occasions, that he
should have expected more geological evidence of transition than he finds, and that all the most
eminent paleontologists maintain the immutability of species.
The general fact, however, that the fossil fauna of each period as a whole is nearly intermediate in
character between the preceding and the succeeding faunas, is much relied on. We are brought one
step nearer to the desired inference by the similar ‘fact,’ insisted on by all paleontologists, that fossils
from two consecutive formations are far more closely related to each other, than are the fossils of two
remote formations.
It is well said that all organic beings have been formed on two great laws; Unity of type, and
Adaptation to the conditions of existence.... Mr. Darwin harmonizes and explains them naturally.
Adaptation to the conditions of existence is the result of Natural Selection; Unity of type, of unity of
descent.”
Gray’s article was soon followed by another one from Agassiz on
Individuality and Specific Differences among Acalephs, but the running
title is “Prof. Agassiz on the Origin of Species” (30, 142, 1860). Agassiz
stoutly maintains his well known views, and concludes as follows:
“Were the transmutation theory true, the geological record should exhibit an uninterrupted
succession of types blending gradually into one another. The fact is that throughout all geological
times each period is characterized by definite specific types, belonging to definite genera, and these
to definite families, referable to definite orders, constituting definite classes and definite branches,
built upon definite plans. Until the facts of Nature are shown to have been mistaken by those who
have collected them, and that they have a different meaning from that now generally assigned to
them, I shall therefore consider the transmutation theory as a scientific mistake, untrue in its facts,
unscientific in its method, and mischievous in its tendency.”
Page 116
Dana, in reviewing Huxley’s well known book, Man’s Place in Nature
(35, 451, 1863), holds that man is apart from brute nature because man
exhibits “extreme cephalization” in that he has arms that no longer are used
in locomotion but go rather with the head, and because he has a far higher
mentality and speech. As for the Darwinian theory, the evidence, he says,
“comes from lower departments of life, and is acknowledged by its
advocates to be exceedingly scanty and imperfect.”
The growth of evolution is set forth in the Journal in Asa Gray’s article
on Charles Darwin (24, 453, 1882), which speaks of the latter as “the most
celebrated man of science of the nineteenth century,” and, in addition, as
“one of the most kindly and charming, unaffected, simple-hearted, and
lovable of men.” In regard to the rise of evolution in America, more can be
had from Dana’s paper on Asa Gray (35, 181, 1888). Here we read, as a
sequel to his Thoughts on Species, that the “paper may be taken, perhaps, as
a culmination of the past, just as the new future was to make its
appearance.” Finally, in this connection there should be mentioned O. C.
Marsh’s paper on Thomas Henry Huxley (50, 177, 1895), wherein is
recorded the latter’s share in the upbuilding of the evolutionary theory.
We have seen that originally Dana was a creationist, but in the course of
his long and fruitful life he gradually became an evolutionist, and rather a
Neo-Lamarckian than a Darwinian. This change may be traced in the
various editions of his Manual of Geology, and in the last edition of 1895 he
says his “speculative conclusions” of 1852 in regard to the origin of species
are not in “accord with the author’s present judgment.” “The evidence in
favor of evolution by variation is now regarded as essentially complete.”
On the other hand, while man is “unquestionably” closely related in
structure to the man-apes, yet he is not linked to them but stands apart,
through “the intervention of a Power above Nature.... Believing that Nature
exists through the will and ever-acting power of the Divine Being, and ...
that the whole Universe is not merely dependent on, but actually is, the Will
of one Supreme Intelligence, Nature, with Man as its culminant species, is
no longer a mystery.”
In America most of the paleontologists are Neo-Lamarckian, a school
that was developed independently by E. D. Cope (1840–1897) through the
vertebrate evidence, and by Alpheus Hyatt (1838–1902) mainly on the
evidence of the ammonites. They hold that variations and acquired
(35, 451, 1863), holds that man is apart from brute nature because man
exhibits “extreme cephalization” in that he has arms that no longer are used
in locomotion but go rather with the head, and because he has a far higher
mentality and speech. As for the Darwinian theory, the evidence, he says,
“comes from lower departments of life, and is acknowledged by its
advocates to be exceedingly scanty and imperfect.”
The growth of evolution is set forth in the Journal in Asa Gray’s article
on Charles Darwin (24, 453, 1882), which speaks of the latter as “the most
celebrated man of science of the nineteenth century,” and, in addition, as
“one of the most kindly and charming, unaffected, simple-hearted, and
lovable of men.” In regard to the rise of evolution in America, more can be
had from Dana’s paper on Asa Gray (35, 181, 1888). Here we read, as a
sequel to his Thoughts on Species, that the “paper may be taken, perhaps, as
a culmination of the past, just as the new future was to make its
appearance.” Finally, in this connection there should be mentioned O. C.
Marsh’s paper on Thomas Henry Huxley (50, 177, 1895), wherein is
recorded the latter’s share in the upbuilding of the evolutionary theory.
We have seen that originally Dana was a creationist, but in the course of
his long and fruitful life he gradually became an evolutionist, and rather a
Neo-Lamarckian than a Darwinian. This change may be traced in the
various editions of his Manual of Geology, and in the last edition of 1895 he
says his “speculative conclusions” of 1852 in regard to the origin of species
are not in “accord with the author’s present judgment.” “The evidence in
favor of evolution by variation is now regarded as essentially complete.”
On the other hand, while man is “unquestionably” closely related in
structure to the man-apes, yet he is not linked to them but stands apart,
through “the intervention of a Power above Nature.... Believing that Nature
exists through the will and ever-acting power of the Divine Being, and ...
that the whole Universe is not merely dependent on, but actually is, the Will
of one Supreme Intelligence, Nature, with Man as its culminant species, is
no longer a mystery.”
In America most of the paleontologists are Neo-Lamarckian, a school
that was developed independently by E. D. Cope (1840–1897) through the
vertebrate evidence, and by Alpheus Hyatt (1838–1902) mainly on the
evidence of the ammonites. They hold that variations and acquired
Page 117
characters arise through the effects of the environment, the mechanics of the
organism resulting from the use and disuse of organs, etc. One of the
leading exponents of this school is A. S. Packard, whose book on Lamarck,
His Life and Work, 1901, fully explains the doctrines of the Neo-
Lamarckians.
organism resulting from the use and disuse of organs, etc. One of the
leading exponents of this school is A. S. Packard, whose book on Lamarck,
His Life and Work, 1901, fully explains the doctrines of the Neo-
Lamarckians.
Page 118
The Growth of Invertebrate Paleontology.
How and by whom paleontology has been developed has been fully
stated in the Journal in a very clear manner by Professor Marsh in his
memorable presidential address of 1879, History and Methods of
Palæontological Discovery (18, 323, 1879), and by Karl von Zittel in his
most interesting book, History of Geology and Palæontology, 1901. In this
discussion we shall largely follow Marsh.
The science of paleontology has passed through four periods, the first of
them the long Mystic period extending up to the beginning of the
seventeenth century, when the idea that fossils were once living things was
only rarely perceived. The second period was the Diluvial period of the
eighteenth century, when nearly everyone regarded the fossils as remains of
the Noachian deluge. With the beginnings of the nineteenth century there
arose in western Europe the knowledge that fossils are the “medals of
creation” and that they have a chronogenetic significance; also that life had
been periodically destroyed through world-wide convulsions in nature.
From about 1800 to 1860 was the time of the creationists and catastrophists,
which may be known as the Catastrophic period. The fourth period began
in 1860 with Darwin’s Origin of Species. Since that time the theory of
evolution has pervaded all work in paleontology, and accordingly this time
may be known as the Evolutionary period.
Mystic Period.—The Mystic period in paleontology begins with the
Greeks, five centuries before the present era, and continues down to the
beginning of the seventeenth century of our time. Some correctly saw that
the fossils were once living marine animals, and that the sea had been
where they now occur. Others interpreted fossil mammal bones as those of
human giants, the Titans, but the Aristotelian view that they were of
spontaneous generation through the hidden forces of the earth dominated all
thought for about twenty centuries.
In the sixteenth century canals were being dug in Northern Italy, and the
many fossils so revealed led to a fierce discussion as to their actual nature.
Leonardo da Vinci (1452–1519) opposed the commonly accepted view of
their spontaneous generation and said that they were the remains of once
How and by whom paleontology has been developed has been fully
stated in the Journal in a very clear manner by Professor Marsh in his
memorable presidential address of 1879, History and Methods of
Palæontological Discovery (18, 323, 1879), and by Karl von Zittel in his
most interesting book, History of Geology and Palæontology, 1901. In this
discussion we shall largely follow Marsh.
The science of paleontology has passed through four periods, the first of
them the long Mystic period extending up to the beginning of the
seventeenth century, when the idea that fossils were once living things was
only rarely perceived. The second period was the Diluvial period of the
eighteenth century, when nearly everyone regarded the fossils as remains of
the Noachian deluge. With the beginnings of the nineteenth century there
arose in western Europe the knowledge that fossils are the “medals of
creation” and that they have a chronogenetic significance; also that life had
been periodically destroyed through world-wide convulsions in nature.
From about 1800 to 1860 was the time of the creationists and catastrophists,
which may be known as the Catastrophic period. The fourth period began
in 1860 with Darwin’s Origin of Species. Since that time the theory of
evolution has pervaded all work in paleontology, and accordingly this time
may be known as the Evolutionary period.
Mystic Period.—The Mystic period in paleontology begins with the
Greeks, five centuries before the present era, and continues down to the
beginning of the seventeenth century of our time. Some correctly saw that
the fossils were once living marine animals, and that the sea had been
where they now occur. Others interpreted fossil mammal bones as those of
human giants, the Titans, but the Aristotelian view that they were of
spontaneous generation through the hidden forces of the earth dominated all
thought for about twenty centuries.
In the sixteenth century canals were being dug in Northern Italy, and the
many fossils so revealed led to a fierce discussion as to their actual nature.
Leonardo da Vinci (1452–1519) opposed the commonly accepted view of
their spontaneous generation and said that they were the remains of once
Page 119
living animals and that the sea had been where they occur. “You tell me,” he
said, “that Nature and the influence of the stars have formed these shells in
the mountains; then show me a place in the mountains where the stars at the
present day make shelly forms of different ages, and of different species in
the same place.” However, nothing came of his teachings and those of his
countryman Fracastorio (1483–1553), who further ridiculed the idea that
they were the remains of the deluge. The first mineralogist, Agricola,
described them as minerals—fossilia—and said that they arose in the
ground from fatty matter set in fermentation by heat. Others said that they
were freaks of nature. Martin Lister (1638–1711) figured fossils side by
side with living shells to show that they were extinct forms of life. In the
seventeenth century, and especially in Italy and Germany, many books were
published on fossils, some with illustrations so accurate that the species can
be recognized to-day. Finally, toward the close of this century the influence
of Aristotle and the scholastic tendency to disputation came more or less to
an end. Fossils were already to many naturalists once living plants and
animals. Marsh states: “The many collections of fossils that had been
brought together, and the illustrated works that had been published about
them, were a foundation for greater progress, and, with the eighteenth
century, the second period in the history of paleontology began.”
Diluvial Period.—During the eighteenth century many more books on
fossils were published in western Europe, and now the prevalent
explanation was that they were the remains of the Noachian deluge. For
nearly a century theologians and laymen alike took this view, and some of
the books have become famous on this account, but the diluvial views
sensibly declined with the close of the eighteenth century.
The true nature of fossils had now been clearly determined. They were
the remains of plants and animals, deposited long before the deluge, part in
fresh water and part in the sea. “Some indicated a mild climate, and some
the tropics. That any of these were extinct species, was as yet only
suspected.” Yet before the close of the century there were men in England
and France who pointed out that different formations had different fossils
and that some of them were extinct. These views then led to many fantastic
theories as to how the earth was formed—dreams, most of them have been
called. Marsh says:
said, “that Nature and the influence of the stars have formed these shells in
the mountains; then show me a place in the mountains where the stars at the
present day make shelly forms of different ages, and of different species in
the same place.” However, nothing came of his teachings and those of his
countryman Fracastorio (1483–1553), who further ridiculed the idea that
they were the remains of the deluge. The first mineralogist, Agricola,
described them as minerals—fossilia—and said that they arose in the
ground from fatty matter set in fermentation by heat. Others said that they
were freaks of nature. Martin Lister (1638–1711) figured fossils side by
side with living shells to show that they were extinct forms of life. In the
seventeenth century, and especially in Italy and Germany, many books were
published on fossils, some with illustrations so accurate that the species can
be recognized to-day. Finally, toward the close of this century the influence
of Aristotle and the scholastic tendency to disputation came more or less to
an end. Fossils were already to many naturalists once living plants and
animals. Marsh states: “The many collections of fossils that had been
brought together, and the illustrated works that had been published about
them, were a foundation for greater progress, and, with the eighteenth
century, the second period in the history of paleontology began.”
Diluvial Period.—During the eighteenth century many more books on
fossils were published in western Europe, and now the prevalent
explanation was that they were the remains of the Noachian deluge. For
nearly a century theologians and laymen alike took this view, and some of
the books have become famous on this account, but the diluvial views
sensibly declined with the close of the eighteenth century.
The true nature of fossils had now been clearly determined. They were
the remains of plants and animals, deposited long before the deluge, part in
fresh water and part in the sea. “Some indicated a mild climate, and some
the tropics. That any of these were extinct species, was as yet only
suspected.” Yet before the close of the century there were men in England
and France who pointed out that different formations had different fossils
and that some of them were extinct. These views then led to many fantastic
theories as to how the earth was formed—dreams, most of them have been
called. Marsh says:
Page 120
“The dominant idea of the first sixteen centuries of the present era was, that the universe was made
for Man. This was the great obstacle to the correct determination of the position of the earth in the
universe, and, later, of the age of the earth.... In a superstitious age, when every natural event is
referred to a supernatural cause, science cannot live.... Scarcely less fatal to the growth of science is
the age of Authority, as the past proves too well. With freedom of thought, came definite knowledge,
and certain progress;—but two thousand years was long to wait.”
One of the most significant publications of this period was Linnæus’s
Systema Naturæ, which appeared in 1735. In this work was introduced
binomial nomenclature, or the system of giving each plant and animal
species a generic and specific name, as Felis leo for the lion. The system
was, however, not established until the tenth edition of the work in 1758,
which became the starting point of zoological nomenclature. Since then
there has been added another canon, the law of priority, which holds that the
first name applied to a given form shall stand against all later names given
to the same organism.
Catastrophic Period.—With the beginning of the nineteenth century
there started a new era in paleontology, and this was the time when the
foundations of the science were laid. The period continued for six decades,
or until the time of the Origin of Species. Marsh says that now “method
replaced disorder, and systematic study superseded casual observation.”
Fossils were accurately determined, comparisons were made with living
forms, and the species named according to the binomial system. However,
every species, recent and extinct, was regarded as a separate creation, and
because of the usually sharp separation of the superposed fossil faunas and
floras, these were held to have been destroyed through a series of periodic
catastrophes of which the Noachian deluge was the last.
Lamarck between 1802 and 1806 described the Tertiary shells of the
Paris basin. Comparing them with the living forms, he saw that most of the
fossils were of extinct species, and in this way he came to be the founder of
modern invertebrate paleontology. He also maintained after 1801 that life
has been continuous since its origin and that nature has been uniform in the
course of its development. Marsh adds:
“His researches on the invertebrate fossils of the Paris Basin, although less striking, were not less
important than those of Cuvier on the vertebrates; while the conclusions he derived from them form
the basis of modern biology.”
“Lamarck was the prophetic genius, half a century in advance of his time.”
for Man. This was the great obstacle to the correct determination of the position of the earth in the
universe, and, later, of the age of the earth.... In a superstitious age, when every natural event is
referred to a supernatural cause, science cannot live.... Scarcely less fatal to the growth of science is
the age of Authority, as the past proves too well. With freedom of thought, came definite knowledge,
and certain progress;—but two thousand years was long to wait.”
One of the most significant publications of this period was Linnæus’s
Systema Naturæ, which appeared in 1735. In this work was introduced
binomial nomenclature, or the system of giving each plant and animal
species a generic and specific name, as Felis leo for the lion. The system
was, however, not established until the tenth edition of the work in 1758,
which became the starting point of zoological nomenclature. Since then
there has been added another canon, the law of priority, which holds that the
first name applied to a given form shall stand against all later names given
to the same organism.
Catastrophic Period.—With the beginning of the nineteenth century
there started a new era in paleontology, and this was the time when the
foundations of the science were laid. The period continued for six decades,
or until the time of the Origin of Species. Marsh says that now “method
replaced disorder, and systematic study superseded casual observation.”
Fossils were accurately determined, comparisons were made with living
forms, and the species named according to the binomial system. However,
every species, recent and extinct, was regarded as a separate creation, and
because of the usually sharp separation of the superposed fossil faunas and
floras, these were held to have been destroyed through a series of periodic
catastrophes of which the Noachian deluge was the last.
Lamarck between 1802 and 1806 described the Tertiary shells of the
Paris basin. Comparing them with the living forms, he saw that most of the
fossils were of extinct species, and in this way he came to be the founder of
modern invertebrate paleontology. He also maintained after 1801 that life
has been continuous since its origin and that nature has been uniform in the
course of its development. Marsh adds:
“His researches on the invertebrate fossils of the Paris Basin, although less striking, were not less
important than those of Cuvier on the vertebrates; while the conclusions he derived from them form
the basis of modern biology.”
“Lamarck was the prophetic genius, half a century in advance of his time.”
Page 121
Cuvier established comparative anatomy and vertebrate paleontology,
and was one of the first to point out that fossil animals are nearly all extinct
forms. He came to the latter conclusion in 1796 through a study of fossil
elephants found in Europe. “Cuvier enriched the animal kingdom by the
introduction of fossil forms among the living, bringing all together into one
comprehensive system.” This opened to him entirely new views respecting
the theory of the earth, and he devoted more than twenty-five years to
developing the theories of special creation and catastrophism, described in
his Discourse on the Revolutions of the Surface of the Globe. “With all his
knowledge of the earth, he could not free himself from tradition, and
believed in the universality and power of the Mosaic deluge. Again, he
refused to admit the evidence brought forward by his distinguished
colleagues against the permanence of species, and used all his great
influence to crush out the doctrine of evolution, then first proposed”
(Marsh).
In England it was William Smith (1769–1839) who independently
discovered the chronogenetic significance of fossils, and in their
stratigraphic superposition indicated the way for the study of historical
geology. He first published on this matter in 1799, but his completed
statements came in works entitled “Strata identified by Organized Fossils,”
1816–1820, and “Stratigraphical System of Organized Fossils,” 1817.
Invertebrate paleontology in America during the Catastrophic period had
its beginning in Lesueur, who in 1818 described the Ordovician gastropod
Maclurites magna. All of the paleontologists of this time were satisfied to
describe species and genera and to ascertain in a broad way the stratigraphic
significance of the fossil faunas and floras. James Hall in 1854 (17, 312)
knew of 1588 species, described and undescribed, in the New York system,
while in England Morris listed in that year 8300 Paleozoic forms. In 1856
Dana recites the known fossil species as follows (22, 333): The whole
number of known American species of animals of the Permian to Recent is
about 2000; while in Britain and Europe, there were over 20,000 species. In
the Permian we have none, while Europe has over 200 species. In the
Triassic we have none, Europe 1000 species; Jurassic 60, Europe over
4000; Cretaceous 350 to 400, Europe about 6000; Tertiary hardly 1500,
Europe about 8000. Since that time nearly all of the larger American
Paleozoic faunas have been developed, but there are thousands of species
yet to be described. Who the more prominent American paleontologists of
and was one of the first to point out that fossil animals are nearly all extinct
forms. He came to the latter conclusion in 1796 through a study of fossil
elephants found in Europe. “Cuvier enriched the animal kingdom by the
introduction of fossil forms among the living, bringing all together into one
comprehensive system.” This opened to him entirely new views respecting
the theory of the earth, and he devoted more than twenty-five years to
developing the theories of special creation and catastrophism, described in
his Discourse on the Revolutions of the Surface of the Globe. “With all his
knowledge of the earth, he could not free himself from tradition, and
believed in the universality and power of the Mosaic deluge. Again, he
refused to admit the evidence brought forward by his distinguished
colleagues against the permanence of species, and used all his great
influence to crush out the doctrine of evolution, then first proposed”
(Marsh).
In England it was William Smith (1769–1839) who independently
discovered the chronogenetic significance of fossils, and in their
stratigraphic superposition indicated the way for the study of historical
geology. He first published on this matter in 1799, but his completed
statements came in works entitled “Strata identified by Organized Fossils,”
1816–1820, and “Stratigraphical System of Organized Fossils,” 1817.
Invertebrate paleontology in America during the Catastrophic period had
its beginning in Lesueur, who in 1818 described the Ordovician gastropod
Maclurites magna. All of the paleontologists of this time were satisfied to
describe species and genera and to ascertain in a broad way the stratigraphic
significance of the fossil faunas and floras. James Hall in 1854 (17, 312)
knew of 1588 species, described and undescribed, in the New York system,
while in England Morris listed in that year 8300 Paleozoic forms. In 1856
Dana recites the known fossil species as follows (22, 333): The whole
number of known American species of animals of the Permian to Recent is
about 2000; while in Britain and Europe, there were over 20,000 species. In
the Permian we have none, while Europe has over 200 species. In the
Triassic we have none, Europe 1000 species; Jurassic 60, Europe over
4000; Cretaceous 350 to 400, Europe about 6000; Tertiary hardly 1500,
Europe about 8000. Since that time nearly all of the larger American
Paleozoic faunas have been developed, but there are thousands of species
yet to be described. Who the more prominent American paleontologists of
Page 122
this period were has been told in the section on the development of the
geological column.
The grander paleontologic results of the Catastrophic period have been so
well stated by Marsh that it is worth our while to repeat them here:
“It had now been proved beyond question that portions at least of the earth’s surface had been
covered many times by the sea, with alternations of fresh water and of land; that the strata thus
deposited were formed in succession, the lowest of the series being the oldest; that a distinct
succession of animals and plants had inhabited the earth during the different geological periods; and
that the order of succession found in one part of the earth was essentially the same in all. More than
30,000 new species of extinct animals and plants had now been described. It had been found, too,
that from the oldest formations to the most recent, there had been an advance in the grade of life,
both animal and vegetable, the oldest forms being among the simplest, and the higher forms
successively making their appearance.
It had now become clearly evident, moreover, that the fossils from the older formations were all
extinct species, and that only in the most recent deposits were there remains of forms still living....
Another important conclusion reached, mainly through the labors of Lyell, was, that the earth had not
been subjected in the past to sudden and violent revolutions; but the great changes wrought had been
gradual, differing in no essential respect from those still in progress. Strangely enough, the corollary
to this proposition, that life, too, had been continuous on the earth, formed at that date no part of the
common stock of knowledge. In the physical world, the great law of ‘correlation of forces’ had been
announced, and widely accepted; but in the organic world, the dogma of the miraculous creation of
each separate species still held sway.”
Evolutionary Period.—This period begins with 1860 and the publication
of Darwin’s Origin of Species (late in 1859). It is the period of modern
paleontology, and is dominated by the belief that universal laws pervade not
only inorganic matter, but all life as well. Louis Agassiz had been in
America fourteen years when Darwin’s book appeared, and his wonderful
influence in bringing the zoology of our country to a high stand and the
further influence he exerted through his students was bound to react
beneficially on invertebrate paleontology. Shortly after the beginning of this
period, or in 1867, Alpheus Hyatt, one of Agassiz’s students, began to apply
the study of embryology to fossil cephalopods, showing clearly that these
shells retain a great deal of their growth stages or ontogeny. This method of
study was then followed by R. T. Jackson, C. E. Beecher, and J. P. Smith,
and has been productive of natural classifications of the Cephalopoda,
Brachiopoda, Trilobita, and Echinoidea.
The dominant invertebrate paleontologist of this period was of course
James Hall, who described about 5000 species of American Paleozoic
geological column.
The grander paleontologic results of the Catastrophic period have been so
well stated by Marsh that it is worth our while to repeat them here:
“It had now been proved beyond question that portions at least of the earth’s surface had been
covered many times by the sea, with alternations of fresh water and of land; that the strata thus
deposited were formed in succession, the lowest of the series being the oldest; that a distinct
succession of animals and plants had inhabited the earth during the different geological periods; and
that the order of succession found in one part of the earth was essentially the same in all. More than
30,000 new species of extinct animals and plants had now been described. It had been found, too,
that from the oldest formations to the most recent, there had been an advance in the grade of life,
both animal and vegetable, the oldest forms being among the simplest, and the higher forms
successively making their appearance.
It had now become clearly evident, moreover, that the fossils from the older formations were all
extinct species, and that only in the most recent deposits were there remains of forms still living....
Another important conclusion reached, mainly through the labors of Lyell, was, that the earth had not
been subjected in the past to sudden and violent revolutions; but the great changes wrought had been
gradual, differing in no essential respect from those still in progress. Strangely enough, the corollary
to this proposition, that life, too, had been continuous on the earth, formed at that date no part of the
common stock of knowledge. In the physical world, the great law of ‘correlation of forces’ had been
announced, and widely accepted; but in the organic world, the dogma of the miraculous creation of
each separate species still held sway.”
Evolutionary Period.—This period begins with 1860 and the publication
of Darwin’s Origin of Species (late in 1859). It is the period of modern
paleontology, and is dominated by the belief that universal laws pervade not
only inorganic matter, but all life as well. Louis Agassiz had been in
America fourteen years when Darwin’s book appeared, and his wonderful
influence in bringing the zoology of our country to a high stand and the
further influence he exerted through his students was bound to react
beneficially on invertebrate paleontology. Shortly after the beginning of this
period, or in 1867, Alpheus Hyatt, one of Agassiz’s students, began to apply
the study of embryology to fossil cephalopods, showing clearly that these
shells retain a great deal of their growth stages or ontogeny. This method of
study was then followed by R. T. Jackson, C. E. Beecher, and J. P. Smith,
and has been productive of natural classifications of the Cephalopoda,
Brachiopoda, Trilobita, and Echinoidea.
The dominant invertebrate paleontologist of this period was of course
James Hall, who described about 5000 species of American Paleozoic
Page 123
fossils. He also built up the New York State Museum, while around his
private collections of fossils have been developed the American Museum of
Natural History in New York City and the Walker Museum at the University
of Chicago. In his most important laboratory of paleontology at Albany,
there have been trained either wholly or in part the following
paleontologists: F. B. Meek, C. A. White, R. P. Whitfield, C. D. Walcott, C.
E. Beecher, John M. Clarke, and Charles Schuchert.
In Canada, through the work of the Geological Survey of the Dominion,
came the paleontologists Elkanah Billings and, later on, J. F. Whiteaves.
The “father of Canadian paleontology,” Sir William Dawson, who
developed independently, was active in all branches of the science and did
much to unravel the geology of eastern Canada. No organism has been
more discussed and more often rejected and accepted as a fossil than his
“dawn animal of Canada,” Eozoon canadense, first described in 1865. His
son, George M. Dawson, was one of the directors of the Geological Survey
of Canada. Finally the extensive paleontology of the Cambrian of Canada
was worked out by another self-made paleontologist, G. F. Matthew.
Paleobotany.—American paleobotany was developed during this, the
fourth period, through the state and national surveys, first in Leo
Lesquereux, a Swiss student induced by Agassiz to come to America, and in
J. S. Newberry. The second generation of paleobotanists is represented by
Lester F. Ward and W. N. Fontaine, and the third generation, the present
workers, includes F. H. Knowlton, David White, Arthur Hollick, and E. W.
Berry. A new line of paleobotanical work, the histology of woody but
pseudomorphous remains, has been developed by G. R. Wieland.
The grander results of the study of paleontology during the evolutionary
period may be summed up with the conclusions of Marsh:
“One of the main characteristics of this epoch is the belief that all life, living and extinct, has been
evolved from simple forms. Another prominent feature is the accepted fact of the great antiquity of
the human race. These are quite sufficient to distinguish this period sharply from those that preceded
it.”
Charles Darwin’s work at once aroused attention, and brought about in scientific thought a
revolution which “has influenced paleontology as extensively as any other department of science....
In the [previous period] species were represented independently by parallel lines; in the present
period, they are indicated by dependent, branching lines. The former was the analytic, the latter is the
synthetic period.”
private collections of fossils have been developed the American Museum of
Natural History in New York City and the Walker Museum at the University
of Chicago. In his most important laboratory of paleontology at Albany,
there have been trained either wholly or in part the following
paleontologists: F. B. Meek, C. A. White, R. P. Whitfield, C. D. Walcott, C.
E. Beecher, John M. Clarke, and Charles Schuchert.
In Canada, through the work of the Geological Survey of the Dominion,
came the paleontologists Elkanah Billings and, later on, J. F. Whiteaves.
The “father of Canadian paleontology,” Sir William Dawson, who
developed independently, was active in all branches of the science and did
much to unravel the geology of eastern Canada. No organism has been
more discussed and more often rejected and accepted as a fossil than his
“dawn animal of Canada,” Eozoon canadense, first described in 1865. His
son, George M. Dawson, was one of the directors of the Geological Survey
of Canada. Finally the extensive paleontology of the Cambrian of Canada
was worked out by another self-made paleontologist, G. F. Matthew.
Paleobotany.—American paleobotany was developed during this, the
fourth period, through the state and national surveys, first in Leo
Lesquereux, a Swiss student induced by Agassiz to come to America, and in
J. S. Newberry. The second generation of paleobotanists is represented by
Lester F. Ward and W. N. Fontaine, and the third generation, the present
workers, includes F. H. Knowlton, David White, Arthur Hollick, and E. W.
Berry. A new line of paleobotanical work, the histology of woody but
pseudomorphous remains, has been developed by G. R. Wieland.
The grander results of the study of paleontology during the evolutionary
period may be summed up with the conclusions of Marsh:
“One of the main characteristics of this epoch is the belief that all life, living and extinct, has been
evolved from simple forms. Another prominent feature is the accepted fact of the great antiquity of
the human race. These are quite sufficient to distinguish this period sharply from those that preceded
it.”
Charles Darwin’s work at once aroused attention, and brought about in scientific thought a
revolution which “has influenced paleontology as extensively as any other department of science....
In the [previous period] species were represented independently by parallel lines; in the present
period, they are indicated by dependent, branching lines. The former was the analytic, the latter is the
synthetic period.”
Page 124
Synthetic Period.—What is to be the next trend in paleontology? Clearly
it is to be the Synthetic period, one that Marsh in 1879 indicated in these
words: “But if we are permitted to continue in imagination the rapidly
converging lines of research pursued to-day, they seem to meet at the point
where organic and inorganic nature become one. That this point will yet be
reached, I cannot doubt.”
This Synthetic period, foreshadowed also in Herbert Spencer’s Synthetic
Philosophy, has not yet arrived, but before long another great leader will
appear. We have the prophecy of his coming in such books as The Fitness of
the Environment, by Lawrence J. Henderson, 1913; The Origin and Nature
of Life, by Benjamin Moore, 1913; The Organism as a Whole, by Jacques
Loeb, 1916; and The Origin and Evolution of Life, by Henry F. Osborn,
1917.
In all nature, inorganic and organic, there is continuity and consistency,
beauty and design. We are beginning to see that there are eternal laws, ever
interacting and resulting in progressive and regressive evolutions. The
realization of these scientific revelations kindles in us a desire for more
knowledge, and the grandest revelations are yet before us in the synthesis of
the sciences.
it is to be the Synthetic period, one that Marsh in 1879 indicated in these
words: “But if we are permitted to continue in imagination the rapidly
converging lines of research pursued to-day, they seem to meet at the point
where organic and inorganic nature become one. That this point will yet be
reached, I cannot doubt.”
This Synthetic period, foreshadowed also in Herbert Spencer’s Synthetic
Philosophy, has not yet arrived, but before long another great leader will
appear. We have the prophecy of his coming in such books as The Fitness of
the Environment, by Lawrence J. Henderson, 1913; The Origin and Nature
of Life, by Benjamin Moore, 1913; The Organism as a Whole, by Jacques
Loeb, 1916; and The Origin and Evolution of Life, by Henry F. Osborn,
1917.
In all nature, inorganic and organic, there is continuity and consistency,
beauty and design. We are beginning to see that there are eternal laws, ever
interacting and resulting in progressive and regressive evolutions. The
realization of these scientific revelations kindles in us a desire for more
knowledge, and the grandest revelations are yet before us in the synthesis of
the sciences.
Page 125
Notes.
Page 126
3. For more detail in regard to these tillites and the older ones see Climates of Geologic Time,
by Charles Schuchert, being Chapter XXI in Huntington’s Climatic Factor as Illustrated in Arid
America, Publication No. 192 of the Carnegie Institution of Washington, 1914. Also Arthur P.
Coleman’s presidential address before the Geological Society of America in 1915, Dry Land in
Geology, published in the Society’s Bulletin, 27, 175, 1916.
by Charles Schuchert, being Chapter XXI in Huntington’s Climatic Factor as Illustrated in Arid
America, Publication No. 192 of the Carnegie Institution of Washington, 1914. Also Arthur P.
Coleman’s presidential address before the Geological Society of America in 1915, Dry Land in
Geology, published in the Society’s Bulletin, 27, 175, 1916.
Page 127
III
A CENTURY OF GEOLOGY.—STEPS OF PROGRESS IN
THE INTERPRETATION OF LAND FORMS
By HERBERT E. GREGORY
The essence of physiography is the belief that land forms represent merely a
stage in the orderly development of the earth’s surface features; that the
various dynamic agents perform their characteristic work throughout all
geologic time. The formulation of principle and processes of earth sculpture
was, therefore, impossible on the hypothesis of a ready-made earth whose
features were substantially unchangeable, except when modified by
catastrophic processes. In 1821, J. W. Wilson wrote in the Journal: “Is it not
the best theory of the earth, that the Creator, in the beginning, at least at the
general deluge, formed it with all its present grand characteristic
features?”[4] If so, a search for causes is futile, and the study of the work
performed by streams and glaciers and wind is unprofitable. The belief in
the Deluge as the one great geological event in the history of the earth has
brought it about that the speculations of Aristotle, Herodotus, Strabo, and
Ovid, and the illustrious Arab, Avicenna (980–1037), unchecked by appeal
to facts but also unopposed by priesthood or popular prejudice, are nearer to
the truth than the intolerant controversial writings of the intellectual leaders
whose touchstone was orthodoxy. A few thinkers of the sixteenth century
revolted against the interminable repetition of error, and Peter Severinus
(1571) advised his students: “Burn up your books ... buy yourselves stout
shoes, get away to the mountains, search the valleys, the deserts, the shores
of the seas.... In this way and no other will you arrive at a knowledge of
things.” But the thoroughgoing “diluvialist” who believed that a million
A CENTURY OF GEOLOGY.—STEPS OF PROGRESS IN
THE INTERPRETATION OF LAND FORMS
By HERBERT E. GREGORY
The essence of physiography is the belief that land forms represent merely a
stage in the orderly development of the earth’s surface features; that the
various dynamic agents perform their characteristic work throughout all
geologic time. The formulation of principle and processes of earth sculpture
was, therefore, impossible on the hypothesis of a ready-made earth whose
features were substantially unchangeable, except when modified by
catastrophic processes. In 1821, J. W. Wilson wrote in the Journal: “Is it not
the best theory of the earth, that the Creator, in the beginning, at least at the
general deluge, formed it with all its present grand characteristic
features?”[4] If so, a search for causes is futile, and the study of the work
performed by streams and glaciers and wind is unprofitable. The belief in
the Deluge as the one great geological event in the history of the earth has
brought it about that the speculations of Aristotle, Herodotus, Strabo, and
Ovid, and the illustrious Arab, Avicenna (980–1037), unchecked by appeal
to facts but also unopposed by priesthood or popular prejudice, are nearer to
the truth than the intolerant controversial writings of the intellectual leaders
whose touchstone was orthodoxy. A few thinkers of the sixteenth century
revolted against the interminable repetition of error, and Peter Severinus
(1571) advised his students: “Burn up your books ... buy yourselves stout
shoes, get away to the mountains, search the valleys, the deserts, the shores
of the seas.... In this way and no other will you arrive at a knowledge of
things.” But the thoroughgoing “diluvialist” who believed that a million
Page 128
species of animals could occupy a 450–foot Ark, but not that pebbles
weathered from rock or that rivers erode, had no use for his powers of
observation.
Sporadic germs of a science of land forms scattered through the literature
of the seventeenth and eighteenth centuries found an unfavorable
environment and produced inconspicuous growths. Even their sponsors did
little to cultivate them. Steno (1631–1687) mildly suggested that surface
sculpturing, particularly on a small scale, is largely the work of running
water, and Guettard (1715–1786), a truly great mind, grasped the
fundamental principles of denudation and successfully entombed his views
as well as his reputation in scores of books and volumes of cumbrous
diffuse writing.
At the beginning of the nineteenth century a sufficient body of principles
had been established to justify the recognition of an earth science, geology,
and the 195 volumes of the Journal thus far published carry a large part of
the material which has won approval for the new science and given
prominence to American thought. From the pages in the Journal, the
progress of geology may be illustrated by tracing the fluctuation in the
development of fact and theory as relates to valleys and glacial features, the
subjects to which this chapter is devoted.
weathered from rock or that rivers erode, had no use for his powers of
observation.
Sporadic germs of a science of land forms scattered through the literature
of the seventeenth and eighteenth centuries found an unfavorable
environment and produced inconspicuous growths. Even their sponsors did
little to cultivate them. Steno (1631–1687) mildly suggested that surface
sculpturing, particularly on a small scale, is largely the work of running
water, and Guettard (1715–1786), a truly great mind, grasped the
fundamental principles of denudation and successfully entombed his views
as well as his reputation in scores of books and volumes of cumbrous
diffuse writing.
At the beginning of the nineteenth century a sufficient body of principles
had been established to justify the recognition of an earth science, geology,
and the 195 volumes of the Journal thus far published carry a large part of
the material which has won approval for the new science and given
prominence to American thought. From the pages in the Journal, the
progress of geology may be illustrated by tracing the fluctuation in the
development of fact and theory as relates to valleys and glacial features, the
subjects to which this chapter is devoted.
Page 129
The Interpretation of Valleys.
Page 130
The Pioneers.
Desmarest (1725–1815) might be styled the father of physiography. By
concrete examples and sound induction he established (1774) the doctrine
that the valleys of central France are formed by the streams which occupy
them. He also made the first attempt to trace the history of a landscape
through its successive stages on the basis of known causes. His methods
and reasoning are practically identical with those of Dutton working in the
ancient lavas of New Mexico; and Whitney’s description of the Table
Mountains of California might well have appeared in Desmarest’s memoirs.
[5]
The teachings of Desmarest were strengthened and expanded by
DeSaussure (1740–1799), the sponsor for the term, “Geology,” (1779) who
saw in the intimate relation of Alpine streams and valleys the evidence of
erosion by running water (1786).
The work of these acknowledged leaders of geological thought attracted
singularly little attention on the Continent, and Lamarck’s volume on
denudation (Hydrogéologie), which appeared in 1802, although an
important contribution, sank out of sight. But the seed of the French school
found fertile ground in Edinburgh, the center of the geological world during
the first quarter of the nineteenth century. Hutton’s “Theory of the Earth,
with Proofs and Illustrations,” in which the guidance of DeSaussure and
Desmarest is gratefully acknowledged, appeared in 1795. The original
publication aroused only local interest, but when placed in attractive form
by Playfair’s “Illustrations of the Huttonian Theory” (1802), the problem of
the origin and development of land forms assumed a commanding position
in geological thought. Hutton was peculiarly fortunate in his environment.
He had the support and assistance of a group of able scientific colleagues as
well as the bitter opposition of Jameson and of the defenders of orthodoxy.
His views were discussed in scientific publications and found their way to
literary and theological journals. Hutton’s conception of the processes of
land sculpture—slow upheaving and slow degradation of mountains,
differential weathering, and the carving of valleys by streams—has a very
modern aspect. Playfair’s book would scarcely be out of place in a
twentieth century class room. The following paragraphs are quoted from it:
[6]
Desmarest (1725–1815) might be styled the father of physiography. By
concrete examples and sound induction he established (1774) the doctrine
that the valleys of central France are formed by the streams which occupy
them. He also made the first attempt to trace the history of a landscape
through its successive stages on the basis of known causes. His methods
and reasoning are practically identical with those of Dutton working in the
ancient lavas of New Mexico; and Whitney’s description of the Table
Mountains of California might well have appeared in Desmarest’s memoirs.
[5]
The teachings of Desmarest were strengthened and expanded by
DeSaussure (1740–1799), the sponsor for the term, “Geology,” (1779) who
saw in the intimate relation of Alpine streams and valleys the evidence of
erosion by running water (1786).
The work of these acknowledged leaders of geological thought attracted
singularly little attention on the Continent, and Lamarck’s volume on
denudation (Hydrogéologie), which appeared in 1802, although an
important contribution, sank out of sight. But the seed of the French school
found fertile ground in Edinburgh, the center of the geological world during
the first quarter of the nineteenth century. Hutton’s “Theory of the Earth,
with Proofs and Illustrations,” in which the guidance of DeSaussure and
Desmarest is gratefully acknowledged, appeared in 1795. The original
publication aroused only local interest, but when placed in attractive form
by Playfair’s “Illustrations of the Huttonian Theory” (1802), the problem of
the origin and development of land forms assumed a commanding position
in geological thought. Hutton was peculiarly fortunate in his environment.
He had the support and assistance of a group of able scientific colleagues as
well as the bitter opposition of Jameson and of the defenders of orthodoxy.
His views were discussed in scientific publications and found their way to
literary and theological journals. Hutton’s conception of the processes of
land sculpture—slow upheaving and slow degradation of mountains,
differential weathering, and the carving of valleys by streams—has a very
modern aspect. Playfair’s book would scarcely be out of place in a
twentieth century class room. The following paragraphs are quoted from it:
[6]
Page 131
“... A river, of which the course is both serpentine and deeply excavated in the rock, is among the
phenomena, by which the slow waste of the land, and also the cause of that waste, are most directly
pointed out.
The structure of the vallies among mountains, shews clearly to what cause their existence is to be
ascribed. Here we have first a large valley, communicating directly with the plain, and winding
between high ridges of mountains, while the river in the bottom of it descends over a surface,
remarkable, in such a scene, for its uniform declivity. Into this, open a multitude of transverse or
secondary vallies, intersecting the ridges on either side of the former, each bringing a contribution to
the main stream, proportioned to its magnitude; and, except where a cataract now and then
intervenes, all having that nice adjustment in their levels, which is the more wonderful, the greater
the irregularity of the surface. These secondary vallies have others of a smaller size opening into
them; and, among mountains of the first order, where all is laid out on the greatest scale, these
ramifications are continued to a fourth, and even a fifth, each diminishing in size as it increases in
elevation, and as its supply of water is less. Through them all, this law is in general observed, that
where a higher valley joins a lower one, of the two angles which it makes with the latter, that which
is obtuse is always on the descending side; ... what else but the water itself, working its way through
obstacles of unequal resistance, could have opened or kept up a communication between the
inequalities of an irregular and alpine surface....
... The probability of such a constitution [arrangement of valleys] having arisen from another
cause, is, to the probability of its having arisen from the running of water, in such a proportion as
unity bears to a number infinitely great.
... With Dr. Hutton, we shall be disposed to consider those great chains of mountains, which
traverse the surface of the globe, as cut out of masses vastly greater, and more lofty than any thing
that now remains.
From this gradual change of lakes into rivers, it follows, that a lake is but a temporary and
accidental condition of a river, which is every day approaching to its termination; and the truth of this
is attested, not only by the lakes that have existed, but also by those that continue to exist.”
phenomena, by which the slow waste of the land, and also the cause of that waste, are most directly
pointed out.
The structure of the vallies among mountains, shews clearly to what cause their existence is to be
ascribed. Here we have first a large valley, communicating directly with the plain, and winding
between high ridges of mountains, while the river in the bottom of it descends over a surface,
remarkable, in such a scene, for its uniform declivity. Into this, open a multitude of transverse or
secondary vallies, intersecting the ridges on either side of the former, each bringing a contribution to
the main stream, proportioned to its magnitude; and, except where a cataract now and then
intervenes, all having that nice adjustment in their levels, which is the more wonderful, the greater
the irregularity of the surface. These secondary vallies have others of a smaller size opening into
them; and, among mountains of the first order, where all is laid out on the greatest scale, these
ramifications are continued to a fourth, and even a fifth, each diminishing in size as it increases in
elevation, and as its supply of water is less. Through them all, this law is in general observed, that
where a higher valley joins a lower one, of the two angles which it makes with the latter, that which
is obtuse is always on the descending side; ... what else but the water itself, working its way through
obstacles of unequal resistance, could have opened or kept up a communication between the
inequalities of an irregular and alpine surface....
... The probability of such a constitution [arrangement of valleys] having arisen from another
cause, is, to the probability of its having arisen from the running of water, in such a proportion as
unity bears to a number infinitely great.
... With Dr. Hutton, we shall be disposed to consider those great chains of mountains, which
traverse the surface of the globe, as cut out of masses vastly greater, and more lofty than any thing
that now remains.
From this gradual change of lakes into rivers, it follows, that a lake is but a temporary and
accidental condition of a river, which is every day approaching to its termination; and the truth of this
is attested, not only by the lakes that have existed, but also by those that continue to exist.”
Page 132
Steps Backward.
Even Hutton’s clear reasoning, firmly buttressed by concrete examples,
was insufficient to overcome the belief in ready-made or violently formed
valleys and original corrugations and irregularities of mountain surface. The
pages of the Journal show that the principles laid down by Playfair were too
far in advance of the times to secure general acceptance. In the first volume
of the Journal, the gorge of the French Broad River is assigned by Kain to
“some dreadful commotion in nature which probably shook these
mountains to their bases,”[7] and the gorge of the lower Connecticut is
considered by Hitchcock (1824)[8] as a breach which drained a series of
lakes “not many centuries before the settlement of this country.” The
prevailing American and English view for the first quarter of the nineteenth
century is expressed in the reviews in this Journal, where the well-known
conclusions of Conybeare and Phillips that streams are incompetent to
excavate valleys are quoted with approval and admiration is expressed for
Buckland’s famous “Reliquiæ Diluvianæ,” a 300–page quarto volume
devoted to proof of a deluge. The professor at Yale, Silliman, and the
professor at Oxford, Buckland, saw that an acceptance of Hutton’s views
involved a repudiation of the Biblical flood, and much space is devoted to
combating these “erroneous” and “unscientific” views. For example,
Buckland says:[9]
“... The general belief is, that existing streams, avalanches and lakes, bursting their barriers, are
sufficient to account for all their phenomena, and not a few geologists, especially those of the
Huttonian school, at whose head is Professor Playfair, have till recently been of this opinion.... But it
is now very clear to almost every man, who impartially examines the facts in regard to existing
vallies, that the causes now in action, mentioned above, are altogether inadequate to their production;
nay, that such a supposition would involve a physical impossibility. We do not believe that one-
thousandth part of our present vallies were excavated by the power of existing streams.... In very
many cases of large rivers, it is found, that so far from having formed their own beds, they are
actually in a gradual manner filling them up.
Again; how happens it that the source of a river is frequently below the head of a valley, if the
river excavated that valley?
The most powerful argument, however, in our opinion, against the supposition we are combating,
is the phenomena of transverse and longitudinal valleys; both of which could not possibly have been
formed by existing streams.”
Even Hutton’s clear reasoning, firmly buttressed by concrete examples,
was insufficient to overcome the belief in ready-made or violently formed
valleys and original corrugations and irregularities of mountain surface. The
pages of the Journal show that the principles laid down by Playfair were too
far in advance of the times to secure general acceptance. In the first volume
of the Journal, the gorge of the French Broad River is assigned by Kain to
“some dreadful commotion in nature which probably shook these
mountains to their bases,”[7] and the gorge of the lower Connecticut is
considered by Hitchcock (1824)[8] as a breach which drained a series of
lakes “not many centuries before the settlement of this country.” The
prevailing American and English view for the first quarter of the nineteenth
century is expressed in the reviews in this Journal, where the well-known
conclusions of Conybeare and Phillips that streams are incompetent to
excavate valleys are quoted with approval and admiration is expressed for
Buckland’s famous “Reliquiæ Diluvianæ,” a 300–page quarto volume
devoted to proof of a deluge. The professor at Yale, Silliman, and the
professor at Oxford, Buckland, saw that an acceptance of Hutton’s views
involved a repudiation of the Biblical flood, and much space is devoted to
combating these “erroneous” and “unscientific” views. For example,
Buckland says:[9]
“... The general belief is, that existing streams, avalanches and lakes, bursting their barriers, are
sufficient to account for all their phenomena, and not a few geologists, especially those of the
Huttonian school, at whose head is Professor Playfair, have till recently been of this opinion.... But it
is now very clear to almost every man, who impartially examines the facts in regard to existing
vallies, that the causes now in action, mentioned above, are altogether inadequate to their production;
nay, that such a supposition would involve a physical impossibility. We do not believe that one-
thousandth part of our present vallies were excavated by the power of existing streams.... In very
many cases of large rivers, it is found, that so far from having formed their own beds, they are
actually in a gradual manner filling them up.
Again; how happens it that the source of a river is frequently below the head of a valley, if the
river excavated that valley?
The most powerful argument, however, in our opinion, against the supposition we are combating,
is the phenomena of transverse and longitudinal valleys; both of which could not possibly have been
formed by existing streams.”
Page 133
Phillips writes in 1829:[10] “The excavation of valleys can be ascribed to
no other cause than a great flood of water which overtopped the hills,
whose summits those vallies descend.”
Faith in Noah’s flood as the dominant agent of erosion rapidly lost
ground through the teaching of Lyell after 1830, but the theory of
systematic development of landscapes by rivers gained little. In fact, Scrope
in 1830,[11] in showing that the entrenched meanders of the Moselle prove
gradual progressive stream work, was in advance of his English
contemporary. Judged by contributions to the Journal, Lyell’s teaching
served to standardize American opinion of earth sculpture somewhat as
follows: The ocean is the great valley maker, but rivers also make them; the
position of valleys is determined by original or renewed surface inequalities
or by faulting; exceptional occurrences—earthquakes, bursting of lakes,
upheavals and depressions—have played an important part. Hayes (1839)[12]
thought that the surface of New York was essentially an upraised sea-
bottom modified by erosion of waves and ocean currents. Sedgwick (1838)
[13]
considered high-lying lake basins proof of valleys which were shaped
under the sea. Many of the valleys in the Chilian Cordillera were thought by
Darwin (1844) to have been the work of waves and tides, and water gaps
are ascribed to currents “bursting through the range at those points where
the strata have been least inclined and the height consequently is less.”
Speaking of the magnificent stream-cut canyons of the Blue Mountains of
New South Wales, gorges which lead to narrow exits through monoclines,
Darwin says: “To attribute these hollows to alluvial action would be
preposterous.”[14]
The influence of structure in the formation of valleys is emphasized by
many contributors to the Journal. Hildreth in 1836, in a valuable paper,[15]
which is perhaps the first detailed topographic description of drainage in
folded strata, expresses the opinion that the West Virginia ridges and valleys
antedated the streams and that water gaps though cut by rivers involve pre-
existing lakes. Geddes (1826)[16] denied that Niagara River cut its channel
and speaks of valleys which “were valleys e’er moving spirit bade the
waters flow.” Conrad (1839)[17] discussed the structural control of the
Mohawk, the Ohio, and the Mississippi, and Lieutenant Warren (1859)[18]
concluded that the Niobrara must have originated in a fissure. According to
Lesley (1862)[19] the course of the New River across the Great Valley and
into the Appalachians “striking the escarpment in the face” is determined by
no other cause than a great flood of water which overtopped the hills,
whose summits those vallies descend.”
Faith in Noah’s flood as the dominant agent of erosion rapidly lost
ground through the teaching of Lyell after 1830, but the theory of
systematic development of landscapes by rivers gained little. In fact, Scrope
in 1830,[11] in showing that the entrenched meanders of the Moselle prove
gradual progressive stream work, was in advance of his English
contemporary. Judged by contributions to the Journal, Lyell’s teaching
served to standardize American opinion of earth sculpture somewhat as
follows: The ocean is the great valley maker, but rivers also make them; the
position of valleys is determined by original or renewed surface inequalities
or by faulting; exceptional occurrences—earthquakes, bursting of lakes,
upheavals and depressions—have played an important part. Hayes (1839)[12]
thought that the surface of New York was essentially an upraised sea-
bottom modified by erosion of waves and ocean currents. Sedgwick (1838)
[13]
considered high-lying lake basins proof of valleys which were shaped
under the sea. Many of the valleys in the Chilian Cordillera were thought by
Darwin (1844) to have been the work of waves and tides, and water gaps
are ascribed to currents “bursting through the range at those points where
the strata have been least inclined and the height consequently is less.”
Speaking of the magnificent stream-cut canyons of the Blue Mountains of
New South Wales, gorges which lead to narrow exits through monoclines,
Darwin says: “To attribute these hollows to alluvial action would be
preposterous.”[14]
The influence of structure in the formation of valleys is emphasized by
many contributors to the Journal. Hildreth in 1836, in a valuable paper,[15]
which is perhaps the first detailed topographic description of drainage in
folded strata, expresses the opinion that the West Virginia ridges and valleys
antedated the streams and that water gaps though cut by rivers involve pre-
existing lakes. Geddes (1826)[16] denied that Niagara River cut its channel
and speaks of valleys which “were valleys e’er moving spirit bade the
waters flow.” Conrad (1839)[17] discussed the structural control of the
Mohawk, the Ohio, and the Mississippi, and Lieutenant Warren (1859)[18]
concluded that the Niobrara must have originated in a fissure. According to
Lesley (1862)[19] the course of the New River across the Great Valley and
into the Appalachians “striking the escarpment in the face” is determined by
Page 134
the junction of anticlinal structures on the north with faulted monoclines
toward the south; a conclusion in harmony with the views of Edward
Hitchcock (1841)[17] that major valleys and mountain passes are structural in
origin and that even subordinate folds and faults may determine minor
features. “Is not this a beautiful example of prospective benevolence on the
part of the Deity, thus, by means of a violent fracture of primary mountains,
to provide for easy intercommunication through alpine regions, countless
ages afterwards!” The extent of the wandering from the guidance of
DeSaussure and Playfair after the lapse of 50 years is shown by students of
Switzerland. Alpine valleys to Murchison (1851) were bays of an ancient
sea; Schlaginweit (1852) found regional and local complicated crustal
movements a satisfactory cause, and Forbes (1863) saw only glaciers.
toward the south; a conclusion in harmony with the views of Edward
Hitchcock (1841)[17] that major valleys and mountain passes are structural in
origin and that even subordinate folds and faults may determine minor
features. “Is not this a beautiful example of prospective benevolence on the
part of the Deity, thus, by means of a violent fracture of primary mountains,
to provide for easy intercommunication through alpine regions, countless
ages afterwards!” The extent of the wandering from the guidance of
DeSaussure and Playfair after the lapse of 50 years is shown by students of
Switzerland. Alpine valleys to Murchison (1851) were bays of an ancient
sea; Schlaginweit (1852) found regional and local complicated crustal
movements a satisfactory cause, and Forbes (1863) saw only glaciers.
Page 135
Valleys Formed by Rivers.
One strong voice before 1860 appears to have called Americans back to
truths expounded by Desmarest and Hutton. Dana in 1850[20] amply
demonstrated that valleys on the Pacific Islands owe neither their origin,
position or form to the sea or to structural factors. They are the work of
existing streams which have eaten their way headwards. Even the valleys of
Australia cited by Darwin as type examples of ocean work are shown to be
products of normal stream work. Dana went further and gave a permanent
place to the Huttonian idea that many bays, inlets, and fiords are but the
drowned mouths of stream-made valleys. In the same volume in which
these conclusions appeared, Hubbard (1850)[21] announced that in New
Hampshire the “deepest valleys are but valleys of erosion.” The theory that
valleys are excavated by streams which occupy them was all but universally
accepted after F. V. Hayden’s description[22] of Rocky Mountain gorges
(1862) and Newberry’s interpretation of the canyons of Arizona (1862); but
the scientific world was poorly prepared for Newberry’s statement:[23]
“Like the great canons of the Colorado, the broad valleys bounded by high and perpendicular walls
belong to a vast system of erosion, and are wholly due to the action of water.... The first and most
plausible explanation of the striking surface features of this region will be to refer them to that
embodiment of resistless power—the sword that cuts so many geological knots—volcanic force. The
Great Canon of the Colorado would be considered a vast fissure or rent in the earth’s crust, and the
abrupt termination of the steps of the table lands as marking lines of displacement. This theory
though so plausible, and so entirely adequate to explain all the striking phenomena, lacks a single
requisite to acceptance, and that is truth.”
With such stupendous examples in mind, the dictum of Hutton seemed
reasonable: “there is no spot on which rivers may not formerly have run.”
One strong voice before 1860 appears to have called Americans back to
truths expounded by Desmarest and Hutton. Dana in 1850[20] amply
demonstrated that valleys on the Pacific Islands owe neither their origin,
position or form to the sea or to structural factors. They are the work of
existing streams which have eaten their way headwards. Even the valleys of
Australia cited by Darwin as type examples of ocean work are shown to be
products of normal stream work. Dana went further and gave a permanent
place to the Huttonian idea that many bays, inlets, and fiords are but the
drowned mouths of stream-made valleys. In the same volume in which
these conclusions appeared, Hubbard (1850)[21] announced that in New
Hampshire the “deepest valleys are but valleys of erosion.” The theory that
valleys are excavated by streams which occupy them was all but universally
accepted after F. V. Hayden’s description[22] of Rocky Mountain gorges
(1862) and Newberry’s interpretation of the canyons of Arizona (1862); but
the scientific world was poorly prepared for Newberry’s statement:[23]
“Like the great canons of the Colorado, the broad valleys bounded by high and perpendicular walls
belong to a vast system of erosion, and are wholly due to the action of water.... The first and most
plausible explanation of the striking surface features of this region will be to refer them to that
embodiment of resistless power—the sword that cuts so many geological knots—volcanic force. The
Great Canon of the Colorado would be considered a vast fissure or rent in the earth’s crust, and the
abrupt termination of the steps of the table lands as marking lines of displacement. This theory
though so plausible, and so entirely adequate to explain all the striking phenomena, lacks a single
requisite to acceptance, and that is truth.”
With such stupendous examples in mind, the dictum of Hutton seemed
reasonable: “there is no spot on which rivers may not formerly have run.”
Page 136
Denudation by Rivers.
The general recognition of the competency of streams to form valleys
was a necessary prelude to the broader view expressed by Jukes (1862)[24]
“The surfaces of our present lands are as much carved and sculptured surfaces as the medallion
carved from the slab, or the statue sculptured from the block. They have been gradually reached by
the removal of the rock that once covered them, and are themselves but of transient duration, always
slowly wasting from decay.”
Contributions to the Journal between 1850 and 1870 reveal a tendency to
accept greater degrees of erosion by rivers, but the necessary end-product of
subaërial erosion—a plain—is first clearly defined by Powell in 1875.[25] In
formulating his ideas Powell introduced the term “base-level,” which may
be called the germ word out of which has grown the “cycle of erosion,” the
master key of modern physiographers. The original definition of base-level
follows:
“We may consider the level of the sea to be a grand base-level, below which the dry lands cannot
be eroded; but we may also have, for local and temporary purposes, other base-levels of erosion,
which are the levels of the beds of the principal streams which carry away the products of erosion. (I
take some liberty in using the term ‘level’ in this connection, as the action of a running stream in
wearing its channel ceases, for all practical purposes, before its bed has quite reached the level of the
lower end of the stream. What I have called the base-level would, in fact, be an imaginary surface,
inclining slightly in all its parts toward the lower end of the principal stream draining the area
through which the level is supposed to extend, or having the inclination of its parts varied in direction
as determined by tributary streams.)”
Analysis of Powell’s view has given definiteness to the distinction
between “base-level,” an imaginary plane, and “a nearly featureless plain,”
the actual land surface produced in the last stage of subaërial erosion.
Following their discovery in the Colorado Plateau Province, denudation
surfaces were recognized on the Atlantic slope and discussed by McGee
(1888),[26] in a paper notable for the demonstration of the use of
physiographic methods and criteria in the solution of stratigraphic
problems. Davis (1889)[27] described the upland of southern New England
The general recognition of the competency of streams to form valleys
was a necessary prelude to the broader view expressed by Jukes (1862)[24]
“The surfaces of our present lands are as much carved and sculptured surfaces as the medallion
carved from the slab, or the statue sculptured from the block. They have been gradually reached by
the removal of the rock that once covered them, and are themselves but of transient duration, always
slowly wasting from decay.”
Contributions to the Journal between 1850 and 1870 reveal a tendency to
accept greater degrees of erosion by rivers, but the necessary end-product of
subaërial erosion—a plain—is first clearly defined by Powell in 1875.[25] In
formulating his ideas Powell introduced the term “base-level,” which may
be called the germ word out of which has grown the “cycle of erosion,” the
master key of modern physiographers. The original definition of base-level
follows:
“We may consider the level of the sea to be a grand base-level, below which the dry lands cannot
be eroded; but we may also have, for local and temporary purposes, other base-levels of erosion,
which are the levels of the beds of the principal streams which carry away the products of erosion. (I
take some liberty in using the term ‘level’ in this connection, as the action of a running stream in
wearing its channel ceases, for all practical purposes, before its bed has quite reached the level of the
lower end of the stream. What I have called the base-level would, in fact, be an imaginary surface,
inclining slightly in all its parts toward the lower end of the principal stream draining the area
through which the level is supposed to extend, or having the inclination of its parts varied in direction
as determined by tributary streams.)”
Analysis of Powell’s view has given definiteness to the distinction
between “base-level,” an imaginary plane, and “a nearly featureless plain,”
the actual land surface produced in the last stage of subaërial erosion.
Following their discovery in the Colorado Plateau Province, denudation
surfaces were recognized on the Atlantic slope and discussed by McGee
(1888),[26] in a paper notable for the demonstration of the use of
physiographic methods and criteria in the solution of stratigraphic
problems. Davis (1889)[27] described the upland of southern New England
Page 137
developed during Cretaceous time, introducing the term “peneplain,” “a
nearly featureless plain.” The short-lived opposition to the theory of
peneplanation indicates that in America at least the idea needed only
formulation to insure acceptance.
It is interesting to note that surfaces now classed as peneplains were fully
described by Percival (1842),[28] who assigned them to structure, and by
Kerr (1880),[29] who considered glaciers the agent. In Europe “plains of
denudation” have been clearly recognized by Ramsay (1846), Jukes (1862),
A. Geikie (1865), Foster and Topley (1865), Maw (1866), Wynne (1867),
Whitaker (1867), Macintosh (1869), Green (1882), Richthofen (1882), but
all of them were looked upon as products of marine work, and writers of
more recent date in England seem reluctant to give a subordinate place to
the erosive power of waves. Americans, on the other hand, have been
thinking in terms of rivers, and the great contribution of the American
school is not that peneplains exist, but that they are the result of normal
subaërial erosion. More precise field methods during the past decade have
revealed the fact that no one agent is responsible for the land forms classed
as peneplains; that not only rivers and ocean, but ice, wind, structure, and
topographic position must be taken into account.
The recognition of rivers as valley-makers and of the final result of
stream work necessarily preceded an analysis of the process of subaërial
erosion. The first and last terms were known, the intermediate terms and the
sequence remained to be established. A significant contribution to this
problem was made by Jukes (1862).[34]
“... I believe that the lateral valleys are those which were first formed by the drainage running
directly from the crests of the chains, the longitudinal ones being subsequently elaborated along the
strike of the softer or more erodable beds exposed on the flanks of those chains.”
Powell’s discussion of antecedent and consequent drainage (1875) and
Gilbert’s chapter on land sculpture in the Henry Mountain report (1880) are
classics, and McGee’s contribution[30] contains significant suggestions, but
the master papers are by Davis,[31] who introduces an analysis of land forms
based on structure and age by the statement:
“Being fully persuaded of the gradual and systematic evolution of topographical forms it is now
desired ... to seek the causes of the location of streams in their present courses; to go back if possible
nearly featureless plain.” The short-lived opposition to the theory of
peneplanation indicates that in America at least the idea needed only
formulation to insure acceptance.
It is interesting to note that surfaces now classed as peneplains were fully
described by Percival (1842),[28] who assigned them to structure, and by
Kerr (1880),[29] who considered glaciers the agent. In Europe “plains of
denudation” have been clearly recognized by Ramsay (1846), Jukes (1862),
A. Geikie (1865), Foster and Topley (1865), Maw (1866), Wynne (1867),
Whitaker (1867), Macintosh (1869), Green (1882), Richthofen (1882), but
all of them were looked upon as products of marine work, and writers of
more recent date in England seem reluctant to give a subordinate place to
the erosive power of waves. Americans, on the other hand, have been
thinking in terms of rivers, and the great contribution of the American
school is not that peneplains exist, but that they are the result of normal
subaërial erosion. More precise field methods during the past decade have
revealed the fact that no one agent is responsible for the land forms classed
as peneplains; that not only rivers and ocean, but ice, wind, structure, and
topographic position must be taken into account.
The recognition of rivers as valley-makers and of the final result of
stream work necessarily preceded an analysis of the process of subaërial
erosion. The first and last terms were known, the intermediate terms and the
sequence remained to be established. A significant contribution to this
problem was made by Jukes (1862).[34]
“... I believe that the lateral valleys are those which were first formed by the drainage running
directly from the crests of the chains, the longitudinal ones being subsequently elaborated along the
strike of the softer or more erodable beds exposed on the flanks of those chains.”
Powell’s discussion of antecedent and consequent drainage (1875) and
Gilbert’s chapter on land sculpture in the Henry Mountain report (1880) are
classics, and McGee’s contribution[30] contains significant suggestions, but
the master papers are by Davis,[31] who introduces an analysis of land forms
based on structure and age by the statement:
“Being fully persuaded of the gradual and systematic evolution of topographical forms it is now
desired ... to seek the causes of the location of streams in their present courses; to go back if possible
Page 138
to the early date when central Pennsylvania was first raised from the sea, and trace the development
of the several river systems then implanted upon it from their ancient beginning to the present time.”
That such a task could have been undertaken a quarter of a century ago
and to-day considered a part of everyday field work shows how completely
the lost ground of a half century has been regained and how rapid the
advance in the knowledge of land sculpture since the canyons of the
Colorado Plateau were interpreted.
of the several river systems then implanted upon it from their ancient beginning to the present time.”
That such a task could have been undertaken a quarter of a century ago
and to-day considered a part of everyday field work shows how completely
the lost ground of a half century has been regained and how rapid the
advance in the knowledge of land sculpture since the canyons of the
Colorado Plateau were interpreted.
Page 139
Features Resulting from Glaciation.
Page 140
The Problem Stated.
Early in the nineteenth century when speculation regarding the interior of
the earth gave place in part to observations of the surface of the earth,
geologists were confronted with perhaps the most difficult problem in the
history of the science. As stated by the editor of the Journal in 1821:[32]
“The almost universal existence of rolled pebbles, and boulders of rock, not only on the margin of
the oceans, seas, lakes, and rivers; but their existence, often in enormous quantities, in situations
quite removed from large waters; inland,—in high banks, embedded in strata, or scattered,
occasionally, in profusion, on the face of almost every region, and sometimes on the tops and
declivities of mountains, as well as in the vallies between them; their entire difference, in many
cases, from the rocks in the country where they lie—rounded masses and pebbles of primitive rocks
being deposited in secondary and alluvial regions, and vice versa; these and a multitude of similar
facts have ever struck us as being among the most interesting of geological occurrences, and as being
very inadequately accounted for by existing theories.”
The phenomena demanding explanation—jumbled masses of “diluvium,”
polished and striated rock, bowlders distributed with apparent disregard of
topography—were indeed startling. Even Lyell, the great exponent of
uniformitarianism, appears to have lost faith in his theories when
confronted with facts for which known causes seemed inadequate. The
interest aroused is attested by 31 titles in the Journal during its first two
decades, articles which include speculations unsupported by logic or fact,
field observation unaccompanied by explanation, field observation with
fantastic explanation, ex-cathedra pronouncements by prominent men,
sound reasoning from insufficient data, and unclouded recognition of cause
and effect by both obscure and prominent men. With little knowledge of
glaciers, areal geology, or of structure and composition of drift, all known
forces were called in: normal weathering, catastrophic floods, ocean
currents, waves, icebergs, glaciers, wind, and even depositions from a
primordial atmosphere (Chabier, 1823). Human agencies were not
discarded. Speaking of a granite bowlder at North Salem, New York,
described by Cornelius (1820)[33] as resting on limestone, Finch (1824)[34]
says: “it is a magnificent cromlech and the most ancient and venerable
Early in the nineteenth century when speculation regarding the interior of
the earth gave place in part to observations of the surface of the earth,
geologists were confronted with perhaps the most difficult problem in the
history of the science. As stated by the editor of the Journal in 1821:[32]
“The almost universal existence of rolled pebbles, and boulders of rock, not only on the margin of
the oceans, seas, lakes, and rivers; but their existence, often in enormous quantities, in situations
quite removed from large waters; inland,—in high banks, embedded in strata, or scattered,
occasionally, in profusion, on the face of almost every region, and sometimes on the tops and
declivities of mountains, as well as in the vallies between them; their entire difference, in many
cases, from the rocks in the country where they lie—rounded masses and pebbles of primitive rocks
being deposited in secondary and alluvial regions, and vice versa; these and a multitude of similar
facts have ever struck us as being among the most interesting of geological occurrences, and as being
very inadequately accounted for by existing theories.”
The phenomena demanding explanation—jumbled masses of “diluvium,”
polished and striated rock, bowlders distributed with apparent disregard of
topography—were indeed startling. Even Lyell, the great exponent of
uniformitarianism, appears to have lost faith in his theories when
confronted with facts for which known causes seemed inadequate. The
interest aroused is attested by 31 titles in the Journal during its first two
decades, articles which include speculations unsupported by logic or fact,
field observation unaccompanied by explanation, field observation with
fantastic explanation, ex-cathedra pronouncements by prominent men,
sound reasoning from insufficient data, and unclouded recognition of cause
and effect by both obscure and prominent men. With little knowledge of
glaciers, areal geology, or of structure and composition of drift, all known
forces were called in: normal weathering, catastrophic floods, ocean
currents, waves, icebergs, glaciers, wind, and even depositions from a
primordial atmosphere (Chabier, 1823). Human agencies were not
discarded. Speaking of a granite bowlder at North Salem, New York,
described by Cornelius (1820)[33] as resting on limestone, Finch (1824)[34]
says: “it is a magnificent cromlech and the most ancient and venerable
Page 141
monument which America possesses.” In the absence of a known cause,
catastrophic agencies seem reasonable.
catastrophic agencies seem reasonable.
Page 142
The Deluge.
In the seventh volume of the Journal (1824)[35] we read:
“After the production of these regular strata of sand, clay, limestone, &c. came a terrible irruption
of water from the north, or northwest, which in many places covered the preceding formations with
diluvial gravel, and carried along with it those immense masses of granite, and the older rocks, which
attest to the present day the destruction and ruin of a former world.”
Another author remarks:
“We find a mantle as it were of sand and gravel indifferently covering all the solid strata, and
evidently derived from some convulsion which has lacerated and partly broken up those strata....”
The catastrophe favored by most geologists was floods of water violently
released—“we believe,” says the editor, “that all geologists agree in
imputing ... the diluvium to the agency of a deluge at one period or
another.”[36] Such conclusions rested in no small way upon Hayden’s well-
known treatise on surficial deposits (1821),[37] a volume which deserves a
prominent place in American geological literature. Hayden clearly
distinguished the topographic and structural features of the drift but found
an adequate cause in general wide-spread currents which “flowed
impetuously across the whole continent ... from north east to south west.” In
reviewing Hayden’s book Silliman remarks:
“The general cause of these currents Mr. Hayden concludes to be the deluge of Noah. While no
one will object to the propriety of ascribing very many, probably most of our alluvial features, to that
catastrophe, we conceive that neither Mr. Hayden, nor any other man, is bound to prove the
immediate physical cause of that vindictive infliction.
We would beg leave to suggest the following as a cause which may have aided in deluging the
earth, and which, were there occasion, might do it again.
The existence of enormous caverns in the bowels of the earth, (so often imagined by authors,)
appears to be no very extravagant assumption. It is true it cannot be proved, but in a sphere of eight
thousand miles in diameter, it would appear in no way extraordinary, that many cavities might exist,
which collectively, or even singly, might well contain much more than all our oceans, seas, and other
superficial waters, none of which are probably more than a few miles in depth. If these cavities
communicate in any manner with the oceans, and are (as if they exist at all, they probably are,) filled
In the seventh volume of the Journal (1824)[35] we read:
“After the production of these regular strata of sand, clay, limestone, &c. came a terrible irruption
of water from the north, or northwest, which in many places covered the preceding formations with
diluvial gravel, and carried along with it those immense masses of granite, and the older rocks, which
attest to the present day the destruction and ruin of a former world.”
Another author remarks:
“We find a mantle as it were of sand and gravel indifferently covering all the solid strata, and
evidently derived from some convulsion which has lacerated and partly broken up those strata....”
The catastrophe favored by most geologists was floods of water violently
released—“we believe,” says the editor, “that all geologists agree in
imputing ... the diluvium to the agency of a deluge at one period or
another.”[36] Such conclusions rested in no small way upon Hayden’s well-
known treatise on surficial deposits (1821),[37] a volume which deserves a
prominent place in American geological literature. Hayden clearly
distinguished the topographic and structural features of the drift but found
an adequate cause in general wide-spread currents which “flowed
impetuously across the whole continent ... from north east to south west.” In
reviewing Hayden’s book Silliman remarks:
“The general cause of these currents Mr. Hayden concludes to be the deluge of Noah. While no
one will object to the propriety of ascribing very many, probably most of our alluvial features, to that
catastrophe, we conceive that neither Mr. Hayden, nor any other man, is bound to prove the
immediate physical cause of that vindictive infliction.
We would beg leave to suggest the following as a cause which may have aided in deluging the
earth, and which, were there occasion, might do it again.
The existence of enormous caverns in the bowels of the earth, (so often imagined by authors,)
appears to be no very extravagant assumption. It is true it cannot be proved, but in a sphere of eight
thousand miles in diameter, it would appear in no way extraordinary, that many cavities might exist,
which collectively, or even singly, might well contain much more than all our oceans, seas, and other
superficial waters, none of which are probably more than a few miles in depth. If these cavities
communicate in any manner with the oceans, and are (as if they exist at all, they probably are,) filled
Page 143
with water, there exist, we conceive, agents very competent to expel the water of these cavities, and
thus to deluge, at any time, the dry land.”
The teachings of Hayden were favorably received by Hitchcock, Struder,
and Hubbard, and many Europeans. They found a champion in Jackson,
who states (1839):[38]
“From the observations made upon Mount Ktaadn, it is proved, that the current did rush over the
summit of that lofty mountain, and consequently the diluvial waters rose to the height of more than
5,000 feet. Hence we are enabled to prove, that the ancient ocean, which rushed over the surface of
the State, was at least a mile in depth, and its transporting power must have been greatly increased by
its enormous pressure.”
Gibson, a student of western geology, reaches the same conclusion
(1836):[39]
“That a wide-spread current, although not, as imagined, fed from an inland sea, once swept over
the entire region between the Alleghany and the Rocky Mountains is established by plenary proof.”
Professor Sedgwick (1831) thought the sudden upheaval of mountains
sufficient to have caused floods again and again. The strength of the belief
in the Biblical flood, during the first quarter of the 19th century, may be
represented by the following remarks of Phillips (1832):[40]
“Of many important facts which come under the consideration of geologists, the ‘Deluge’ is,
perhaps, the most remarkable; and it is established by such clear and positive arguments, that if any
one point of natural history may be considered as proved, the deluge must be admitted to have
happened, because it has left full evidence in plain and characteristic effects upon the surface of the
earth.”
However, the theory of deluges, whether of ocean or land streams, did
not hold the field unopposed. In 1823, Granger,[41] an observer whose
contributions to science total only six pages, speaks of the striæ on the
shore of Lake Erie as
“having been formed by the powerful and continued attrition of some hard body.... To me, it does
not seem possible that water under any circumstances, could have effected it. The flutings in width,
thus to deluge, at any time, the dry land.”
The teachings of Hayden were favorably received by Hitchcock, Struder,
and Hubbard, and many Europeans. They found a champion in Jackson,
who states (1839):[38]
“From the observations made upon Mount Ktaadn, it is proved, that the current did rush over the
summit of that lofty mountain, and consequently the diluvial waters rose to the height of more than
5,000 feet. Hence we are enabled to prove, that the ancient ocean, which rushed over the surface of
the State, was at least a mile in depth, and its transporting power must have been greatly increased by
its enormous pressure.”
Gibson, a student of western geology, reaches the same conclusion
(1836):[39]
“That a wide-spread current, although not, as imagined, fed from an inland sea, once swept over
the entire region between the Alleghany and the Rocky Mountains is established by plenary proof.”
Professor Sedgwick (1831) thought the sudden upheaval of mountains
sufficient to have caused floods again and again. The strength of the belief
in the Biblical flood, during the first quarter of the 19th century, may be
represented by the following remarks of Phillips (1832):[40]
“Of many important facts which come under the consideration of geologists, the ‘Deluge’ is,
perhaps, the most remarkable; and it is established by such clear and positive arguments, that if any
one point of natural history may be considered as proved, the deluge must be admitted to have
happened, because it has left full evidence in plain and characteristic effects upon the surface of the
earth.”
However, the theory of deluges, whether of ocean or land streams, did
not hold the field unopposed. In 1823, Granger,[41] an observer whose
contributions to science total only six pages, speaks of the striæ on the
shore of Lake Erie as
“having been formed by the powerful and continued attrition of some hard body.... To me, it does
not seem possible that water under any circumstances, could have effected it. The flutings in width,
Page 144
depth, and direction, are as regular as if they had been cut out by a grooving plane. This, running
water could not effect, nor could its operation have produced that glassy smoothness, which, in many
parts, it still retains.”
Hayes and also Conrad expressed similar views in the Journal 16 years
later.
The idea that ice was in some way concerned with the transportation of
drift has had a curious history. The first unequivocal statement, based on
reading and keen observation, was made in the Journal by Dobson in 1826:
[42]
“I have had occasion to dig up a great number of bowlders, of red sandstone, and of the
conglomerate kind, in erecting a cotton manufactory; and it was not uncommon to find them worn
smooth on the under side, as if done by their having been dragged over rocks and gravelly earth, in
one steady position. On examination, they exhibit scratches and furrows on the abraded part; and if
among the minerals composing the rock, there happened to be pebbles of feldspar, or quartz, (which
was not uncommon,) they usually appeared not to be worn so much as the rest of the stone,
preserving their more tender parts in a ridge, extending some inches. When several of these pebbles
happen to be in one block, the preserved ridges were on the same side of the pebbles, so that it is easy
to determine which part of the stone moved forward, in the act of wearing.
These bowlders are found, not only on the surface, but I have discovered them a number of feet
deep, in the earth, in the hard compound of clay, sand, and gravel....
I think we cannot account for these appearances, unless we call in the aid of ice along with water,
and that they have been worn by being suspended and carried in ice, over rocks and earth, under
water.”
In Dobson’s day the hypothesis of “gigantic floods,” “debacles,”
“resistless world-wide currents,” was so firmly entrenched that the voice of
the observant layman found no hearers, and a letter from Dobson to
Hitchcock written in 1837 and containing additional evidence and argument
remained unpublished until Murchison, in 1842,[43] paid his respects to the
remarkable work of a remarkable man.[44]
“I take leave of the glacial theory in congratulating American science in having possessed the
original author of the best glacial theory, though his name had escaped notice; and in recommending
to you the terse argument of Peter Dobson, a previous acquaintance with which might have saved
volumes of disputation on both sides of the Atlantic.”
water could not effect, nor could its operation have produced that glassy smoothness, which, in many
parts, it still retains.”
Hayes and also Conrad expressed similar views in the Journal 16 years
later.
The idea that ice was in some way concerned with the transportation of
drift has had a curious history. The first unequivocal statement, based on
reading and keen observation, was made in the Journal by Dobson in 1826:
[42]
“I have had occasion to dig up a great number of bowlders, of red sandstone, and of the
conglomerate kind, in erecting a cotton manufactory; and it was not uncommon to find them worn
smooth on the under side, as if done by their having been dragged over rocks and gravelly earth, in
one steady position. On examination, they exhibit scratches and furrows on the abraded part; and if
among the minerals composing the rock, there happened to be pebbles of feldspar, or quartz, (which
was not uncommon,) they usually appeared not to be worn so much as the rest of the stone,
preserving their more tender parts in a ridge, extending some inches. When several of these pebbles
happen to be in one block, the preserved ridges were on the same side of the pebbles, so that it is easy
to determine which part of the stone moved forward, in the act of wearing.
These bowlders are found, not only on the surface, but I have discovered them a number of feet
deep, in the earth, in the hard compound of clay, sand, and gravel....
I think we cannot account for these appearances, unless we call in the aid of ice along with water,
and that they have been worn by being suspended and carried in ice, over rocks and earth, under
water.”
In Dobson’s day the hypothesis of “gigantic floods,” “debacles,”
“resistless world-wide currents,” was so firmly entrenched that the voice of
the observant layman found no hearers, and a letter from Dobson to
Hitchcock written in 1837 and containing additional evidence and argument
remained unpublished until Murchison, in 1842,[43] paid his respects to the
remarkable work of a remarkable man.[44]
“I take leave of the glacial theory in congratulating American science in having possessed the
original author of the best glacial theory, though his name had escaped notice; and in recommending
to you the terse argument of Peter Dobson, a previous acquaintance with which might have saved
volumes of disputation on both sides of the Atlantic.”
Page 145
Glaciers vs. Icebergs.
The glacial theory makes its way into geological literature with the
development of Agassiz (1837) of the views of Venetz (1833) and
Charpentier (1834), that the glaciers of the Alps once had greater extent.
The bold assumption was made that the surface of Europe as far south as
the shores of the Mediterranean and Caspian seas was covered by ice during
a period immediately preceding the present. The kernel of the present
glacial theory is readily recognizable in these early works, but it is wrapped
in a strange husk: it was assumed that the Alps were raised by a great
convulsion under the ice and that the erratics slid to their places over the
newly made declivities. The publication of the famous “Etudes sur les
Glaciers” (1840), remarkable alike for its clarity, its sound inductions, and
wealth of illustrations, brought the ideas of Agassiz more into prominence
and inaugurated a 30–years’ war with the proponents of currents and
icebergs. The outstanding objections to the theory were the requirement of a
frigid climate and the demand for glaciers of continental dimensions; very
strong objections, indeed, for the time when fossil evidence was not
available, the great polar ice sheets were unexplored, and the distinction
between till and waterlaid drift had not been established.
The glacial theory was cordially adopted by Buckland (1841)[45] and in
part by Lyell in England but viewed with suspicion by Sedgwick, Whewell,
and Mantell. In America the response to the new idea was immediate.
Hitchcock (1841)[46] concludes an able discussion with the statement: “So
remarkably does it solve most of the phenomena of diluvial action, that I
am constrained to believe its fundamental principles to be founded in truth.”
The theory formed the chief topic of discussion at the third and fourth
meetings of the Association of American Geologists and Naturalists (1842,
1843) under the lead of a committee on drift consisting of Emmons, W. B.
Rogers, Vanuxem, Nicollet, Jackson, and J. L. Hayes. The result of these
discussions was a curious reaction. Hitchcock complained that he “had been
supposed to be an advocate for the unmodified glacial theory, but he had
never been a believer in it,” and Jackson spoke for a number of men when
he stated:[47]
The glacial theory makes its way into geological literature with the
development of Agassiz (1837) of the views of Venetz (1833) and
Charpentier (1834), that the glaciers of the Alps once had greater extent.
The bold assumption was made that the surface of Europe as far south as
the shores of the Mediterranean and Caspian seas was covered by ice during
a period immediately preceding the present. The kernel of the present
glacial theory is readily recognizable in these early works, but it is wrapped
in a strange husk: it was assumed that the Alps were raised by a great
convulsion under the ice and that the erratics slid to their places over the
newly made declivities. The publication of the famous “Etudes sur les
Glaciers” (1840), remarkable alike for its clarity, its sound inductions, and
wealth of illustrations, brought the ideas of Agassiz more into prominence
and inaugurated a 30–years’ war with the proponents of currents and
icebergs. The outstanding objections to the theory were the requirement of a
frigid climate and the demand for glaciers of continental dimensions; very
strong objections, indeed, for the time when fossil evidence was not
available, the great polar ice sheets were unexplored, and the distinction
between till and waterlaid drift had not been established.
The glacial theory was cordially adopted by Buckland (1841)[45] and in
part by Lyell in England but viewed with suspicion by Sedgwick, Whewell,
and Mantell. In America the response to the new idea was immediate.
Hitchcock (1841)[46] concludes an able discussion with the statement: “So
remarkably does it solve most of the phenomena of diluvial action, that I
am constrained to believe its fundamental principles to be founded in truth.”
The theory formed the chief topic of discussion at the third and fourth
meetings of the Association of American Geologists and Naturalists (1842,
1843) under the lead of a committee on drift consisting of Emmons, W. B.
Rogers, Vanuxem, Nicollet, Jackson, and J. L. Hayes. The result of these
discussions was a curious reaction. Hitchcock complained that he “had been
supposed to be an advocate for the unmodified glacial theory, but he had
never been a believer in it,” and Jackson spoke for a number of men when
he stated:[47]
Page 146
“This country exhibits no proofs of the glacial theory as taught by Agassiz but on the contrary the
general bearing of the facts is against that theory.... Many eminent men incautiously embraced the
new theory, which within two or three years from its promulgation, had been found utterly
inadequate, and is now abandoned by many of its former supporters.”
Out of this symposium came also the strange contribution of H. D.
Rogers (1844),[48] who cast aside the teachings of deduction and observation
and returned to the views of the Medievalists.
“If we will conceive, then, a wide expanse of waters, less perhaps than one thousand feet in depth,
dislodged from some high northern or circumpolar basin, by a general lifting of that region of
perhaps a few hundred feet, and an equal subsidence of the country south, and imagine this whole
mass converted by earthquake pulsations of the breadth which such undulations have, into a series of
stupendous and rapid-moving waves of translation, helped on by the still more rapid flexures of the
floor over which they move, and then advert to the shattering and loosening power of the tremendous
jar of the earthquake, we shall have an agent adequate in every way to produce the results we see, to
float the northern ice from its moorings, to rip off, assisted with its aid, the outcrops of the hardest
strata, to grind up and strew wide their fragments, to scour down the whole rocky floor, and,
gathering energy with resistance, to sweep up the slopes and over the highest mountains.”
Because of the prominence of their author, Rogers’s views exerted some
influence and seemingly received support from England through the
elaborate mathematic discussions of Whewell (1848), who considered the
drift as “irresistible proof of paroxysmal action,” and Hopkins (1852), who
contended for “currents produced by repeated elevatory movements.”
After his arrival in America (1846), Agassiz’s influence was felt, and his
paper on the erratic phenomena about Lake Superior (1850),[49] in which he
called upon the advocates of water-borne ice to point out the barrier which
caused the current to subside, produced a salutary effect; yet Desor (1852)
[50]
states that in the region described by Agassiz “the assumption [of a
general ice cap] is no longer admissible,” and that the bowlders on Long
Island “were transported on ice rafts along the sea shore and stranded on the
ridges and eminences which were then shoals along the coast.” Twenty
years of discussion were insufficient to establish the glacial theory either in
Europe or America. The consensus of opinion among the more advanced
thinkers in 1860 is expressed by Dana:[51]
“In view of the whole subject, it appears reasonable to conclude that the Glacier theory affords the
best and fullest explanation of the phenomena over the general surface of the continents, and
general bearing of the facts is against that theory.... Many eminent men incautiously embraced the
new theory, which within two or three years from its promulgation, had been found utterly
inadequate, and is now abandoned by many of its former supporters.”
Out of this symposium came also the strange contribution of H. D.
Rogers (1844),[48] who cast aside the teachings of deduction and observation
and returned to the views of the Medievalists.
“If we will conceive, then, a wide expanse of waters, less perhaps than one thousand feet in depth,
dislodged from some high northern or circumpolar basin, by a general lifting of that region of
perhaps a few hundred feet, and an equal subsidence of the country south, and imagine this whole
mass converted by earthquake pulsations of the breadth which such undulations have, into a series of
stupendous and rapid-moving waves of translation, helped on by the still more rapid flexures of the
floor over which they move, and then advert to the shattering and loosening power of the tremendous
jar of the earthquake, we shall have an agent adequate in every way to produce the results we see, to
float the northern ice from its moorings, to rip off, assisted with its aid, the outcrops of the hardest
strata, to grind up and strew wide their fragments, to scour down the whole rocky floor, and,
gathering energy with resistance, to sweep up the slopes and over the highest mountains.”
Because of the prominence of their author, Rogers’s views exerted some
influence and seemingly received support from England through the
elaborate mathematic discussions of Whewell (1848), who considered the
drift as “irresistible proof of paroxysmal action,” and Hopkins (1852), who
contended for “currents produced by repeated elevatory movements.”
After his arrival in America (1846), Agassiz’s influence was felt, and his
paper on the erratic phenomena about Lake Superior (1850),[49] in which he
called upon the advocates of water-borne ice to point out the barrier which
caused the current to subside, produced a salutary effect; yet Desor (1852)
[50]
states that in the region described by Agassiz “the assumption [of a
general ice cap] is no longer admissible,” and that the bowlders on Long
Island “were transported on ice rafts along the sea shore and stranded on the
ridges and eminences which were then shoals along the coast.” Twenty
years of discussion were insufficient to establish the glacial theory either in
Europe or America. The consensus of opinion among the more advanced
thinkers in 1860 is expressed by Dana:[51]
“In view of the whole subject, it appears reasonable to conclude that the Glacier theory affords the
best and fullest explanation of the phenomena over the general surface of the continents, and
Page 147
encounters the fewest difficulties. But icebergs have aided beyond doubt in producing the results
along the borders of the continents, across ocean-channels like the German Ocean and the Baltic, and
possibly over great lakes like those of North America. Long Island Sound is so narrow that a glacier
may have stretched across it.”
Papers in the Journal of 1860–70 show a prevailing belief in icebergs, but
the evidence for land ice was accumulating as the deposits became better
known, and in 1871 field workers speak in unmistakable tones:[52]
“It is still a mooted question in American geology whether the events of the Glacial era were due
to glaciers or icebergs.... American geologists are still divided in opinion, and some of the most
eminent have pronounced in favor of icebergs.
Since, then, icebergs cannot pick up masses tons in weight from the bottom of a sea, or give a
general movement southward to the loose material of the surface; neither can produce the abrasion
observed over the rocks under its various conditions; and inasmuch as all direct evidence of the
submergence of the land required for an iceberg sea over New England fails, the conclusion appears
inevitable that icebergs had nothing to do with the drift of the New Haven region, in the Connecticut
valley; and, therefore, that the Glacial era in central New England was a Glacier era.”
Matthew (1871)[53] reached the same conclusion for the Lower Provinces
of Canada. In spite of the increasing clarity of the evidence, the battle for
the glacial theory was not yet won. The remaining opponents though few in
number were distinguished in attainments. Dawson clung to the outworn
doctrine until his death in 1899.
An interesting feature of the history of glacial theories is the calculation
by Maclaren (1842)[54] that the amount of water abstracted from the seas to
form the hypothetical ice sheet would lower the ocean level 350 feet—an
early form of the glacial control hypothesis (see Daly[55]).
along the borders of the continents, across ocean-channels like the German Ocean and the Baltic, and
possibly over great lakes like those of North America. Long Island Sound is so narrow that a glacier
may have stretched across it.”
Papers in the Journal of 1860–70 show a prevailing belief in icebergs, but
the evidence for land ice was accumulating as the deposits became better
known, and in 1871 field workers speak in unmistakable tones:[52]
“It is still a mooted question in American geology whether the events of the Glacial era were due
to glaciers or icebergs.... American geologists are still divided in opinion, and some of the most
eminent have pronounced in favor of icebergs.
Since, then, icebergs cannot pick up masses tons in weight from the bottom of a sea, or give a
general movement southward to the loose material of the surface; neither can produce the abrasion
observed over the rocks under its various conditions; and inasmuch as all direct evidence of the
submergence of the land required for an iceberg sea over New England fails, the conclusion appears
inevitable that icebergs had nothing to do with the drift of the New Haven region, in the Connecticut
valley; and, therefore, that the Glacial era in central New England was a Glacier era.”
Matthew (1871)[53] reached the same conclusion for the Lower Provinces
of Canada. In spite of the increasing clarity of the evidence, the battle for
the glacial theory was not yet won. The remaining opponents though few in
number were distinguished in attainments. Dawson clung to the outworn
doctrine until his death in 1899.
An interesting feature of the history of glacial theories is the calculation
by Maclaren (1842)[54] that the amount of water abstracted from the seas to
form the hypothetical ice sheet would lower the ocean level 350 feet—an
early form of the glacial control hypothesis (see Daly[55]).
Page 148
Extent of Glacial Drift.
By the middle of the nineteenth century, it was recognized that the
“drift,” whatever its origin, was not of world-wide extent. In America its
characteristic features were found best developed north of latitude 40
degrees; in Europe, the Alps, the Scottish Highlands, and Scandinavia were
recognized as type areas. The limits were unassigned, partly because the
field had not been surveyed, but largely because criteria for the recognition
of drift had not been established. The well-known hillocks and ridges of
“diluvium” and “alluvium” and “drift” of New Jersey and Ohio, and the
mounds of the Missouri Cotou elaborately described by Catlin (1840)[56]
bore little resemblance to the walls of unsorted rock which stand as
moraines bordering Alpine glaciers. The Orange sand of Mississippi was
included in the drift by Hilgard (1866),[57] and the gravels at Philadelphia by
Hall (1876).[58] Stevens (1873)[59] described trains of glacial erratics at
Richmond, Virginia, and William B. Rogers (1876)[60] accounts for certain
deposits in the Potomac, James, and Roanoke rivers by the presence of
Pleistocene ice tongues or swollen glacial rivers, and remarks: “It is highly
probable that glacial action had much to do with the original accumulation
of the rocky debris on the flanks of the Blue Ridge, and in the Appalachian
valleys beyond.” Kerr (1881)[61] referred the ancient erosion surface of the
Piedmont belt in North Carolina to glacial denudation, De la Beche
compared the drift of Jamaica with that of New England, and Agassiz
interpreted soils of Brazil as glacial.
The first detailed description and unequivocal interpretation of either
terminal or recessional moraines is from the pen of Gilbert (1871),[62]
geologist of the Ohio Survey. In discussing the former outlet of Lake Erie
through the Fort Wayne channel, Gilbert writes:
“The page of history recorded in these phenomena is by no means ambiguous. The ridges, or, more
properly, the ridge which determines the courses of the St. Joseph and St. Marys rivers is a buried
terminal moraine of the glacier that moved southwestward through the Maumee valley. The overlying
Erie Clay covers it from sight, but it is shadowed forth on the surface of that deposit, as the ground is
pictured through a deep and even canopy of snow. Its irregularly curved outline accords intimately
with the configuration of the valley, and with the direction of the ice markings; its concavity is turned
toward the source of motion; its greatest convexity is along the line of least resistance.
By the middle of the nineteenth century, it was recognized that the
“drift,” whatever its origin, was not of world-wide extent. In America its
characteristic features were found best developed north of latitude 40
degrees; in Europe, the Alps, the Scottish Highlands, and Scandinavia were
recognized as type areas. The limits were unassigned, partly because the
field had not been surveyed, but largely because criteria for the recognition
of drift had not been established. The well-known hillocks and ridges of
“diluvium” and “alluvium” and “drift” of New Jersey and Ohio, and the
mounds of the Missouri Cotou elaborately described by Catlin (1840)[56]
bore little resemblance to the walls of unsorted rock which stand as
moraines bordering Alpine glaciers. The Orange sand of Mississippi was
included in the drift by Hilgard (1866),[57] and the gravels at Philadelphia by
Hall (1876).[58] Stevens (1873)[59] described trains of glacial erratics at
Richmond, Virginia, and William B. Rogers (1876)[60] accounts for certain
deposits in the Potomac, James, and Roanoke rivers by the presence of
Pleistocene ice tongues or swollen glacial rivers, and remarks: “It is highly
probable that glacial action had much to do with the original accumulation
of the rocky debris on the flanks of the Blue Ridge, and in the Appalachian
valleys beyond.” Kerr (1881)[61] referred the ancient erosion surface of the
Piedmont belt in North Carolina to glacial denudation, De la Beche
compared the drift of Jamaica with that of New England, and Agassiz
interpreted soils of Brazil as glacial.
The first detailed description and unequivocal interpretation of either
terminal or recessional moraines is from the pen of Gilbert (1871),[62]
geologist of the Ohio Survey. In discussing the former outlet of Lake Erie
through the Fort Wayne channel, Gilbert writes:
“The page of history recorded in these phenomena is by no means ambiguous. The ridges, or, more
properly, the ridge which determines the courses of the St. Joseph and St. Marys rivers is a buried
terminal moraine of the glacier that moved southwestward through the Maumee valley. The overlying
Erie Clay covers it from sight, but it is shadowed forth on the surface of that deposit, as the ground is
pictured through a deep and even canopy of snow. Its irregularly curved outline accords intimately
with the configuration of the valley, and with the direction of the ice markings; its concavity is turned
toward the source of motion; its greatest convexity is along the line of least resistance.
Page 149
South of the St. Marys river are other and numerous moraines accompanied by glacial striæ. Their
character and courses have not yet been studied; but their presence carries the mind back to an epoch
of the cold period, when the margin of the icefield was farther south, and the glacier of the Maumee
valley was merged in the general mass. As the mantle of ice grew shorter—and, in fact, at every stage
of its existence—its margin must have been variously notched and lobed in conformity with the
contour of the country, the higher lands being first laid bare by the encroaching secular summer.
Early in the history of this encroachment the glacier of the Maumee valley constituted one of these
lobes, and has recorded its form in the two moraines that I have described.”
Three years after the recognition of moraines in the Maumee valley,
Chamberlin (1874)[63] showed that the seemingly disorganized mounds and
basins and ridges known as the Kettle range of Wisconsin is the terminal
moraine of the Green Bay glacier. At an earlier date (1864) Whittlesey
interpreted the kettles of the Wisconsin moraine as evidence of ice blocks
from a melting glacier and presented a map showing the “southern limit of
boulders and coarse drift.” In 1876 attention was called to the terminal
moraine of New England by G. Frederick Wright, who assigns the honor of
discovery to Clarence King.
character and courses have not yet been studied; but their presence carries the mind back to an epoch
of the cold period, when the margin of the icefield was farther south, and the glacier of the Maumee
valley was merged in the general mass. As the mantle of ice grew shorter—and, in fact, at every stage
of its existence—its margin must have been variously notched and lobed in conformity with the
contour of the country, the higher lands being first laid bare by the encroaching secular summer.
Early in the history of this encroachment the glacier of the Maumee valley constituted one of these
lobes, and has recorded its form in the two moraines that I have described.”
Three years after the recognition of moraines in the Maumee valley,
Chamberlin (1874)[63] showed that the seemingly disorganized mounds and
basins and ridges known as the Kettle range of Wisconsin is the terminal
moraine of the Green Bay glacier. At an earlier date (1864) Whittlesey
interpreted the kettles of the Wisconsin moraine as evidence of ice blocks
from a melting glacier and presented a map showing the “southern limit of
boulders and coarse drift.” In 1876 attention was called to the terminal
moraine of New England by G. Frederick Wright, who assigns the honor of
discovery to Clarence King.
Page 150
With the observations of Gilbert, Chamberlin, and King in mind, the
terminal moraine was traced by various workers across the United States
and into Canada and the extent of glacial cover revealed. Following 1875
the pages of the Journal contain many contributions dealing with the origin
and structure of moraines, eskers, kames, and drumlins. Before 1890
twenty-eight papers on the glacial phenomena of the Erie and Ohio basin
alone had appeared. By 1900 substantial agreement had been reached
regarding the significant features of the drift, the outline history of the Great
Lakes had been written, and the way had been paved for stratigraphic
terminal moraine was traced by various workers across the United States
and into Canada and the extent of glacial cover revealed. Following 1875
the pages of the Journal contain many contributions dealing with the origin
and structure of moraines, eskers, kames, and drumlins. Before 1890
twenty-eight papers on the glacial phenomena of the Erie and Ohio basin
alone had appeared. By 1900 substantial agreement had been reached
regarding the significant features of the drift, the outline history of the Great
Lakes had been written, and the way had been paved for stratigraphic
Page 151
studies of the Pleistocene, which bulk large in the pages of the Journal for
the last two decades.
the last two decades.
Page 152
Epochs of Glaciation.
For a decade following the general acceptance of the glacial origin of
“diluvium,” the deposits were embraced as “drift” and treated as the
products of one long period of glacial activity, and throughout the
controversy of iceberg and glacier the unity of the glacial period was
unquestioned. Beds of peat and fossiliferous lacustrine deposits in
Switzerland, England, and in America and the recognition of an “upper”
and a “lower” diluvium by Scandinavian geologists suggested two epochs,
and as the examples of such deposits increased in number and it became
evident that the plant fossils represented forms demanding a genial climate
and that the phenomena were seen in many countries, the belief grew that
minor fluctuations or gradual recession of an ice sheet were inadequate to
account for the phenomena observed.
It is natural that this problem should have found its solution in America,
where the Pleistocene is admirably displayed, and where the State and
Federal surveys were actively engaged in areal mapping. In 1883
Chamberlin[64] presented his views under the bold title, “Preliminary Paper
on the Terminal Moraine of the Second Glacial Epoch,” and the existence
of deposits of two or more ice sheets and the features of interglacial periods
were substantially established by the interesting debate in the Journal led by
Chamberlin, Wright, Upham and Dana.[65] Contributions since 1895 have
been concerned with the degree rather than the fact of complexity, and
continued study has resulted in the general recognition of five glacial stages
in North America and four in Europe.
For a decade following the general acceptance of the glacial origin of
“diluvium,” the deposits were embraced as “drift” and treated as the
products of one long period of glacial activity, and throughout the
controversy of iceberg and glacier the unity of the glacial period was
unquestioned. Beds of peat and fossiliferous lacustrine deposits in
Switzerland, England, and in America and the recognition of an “upper”
and a “lower” diluvium by Scandinavian geologists suggested two epochs,
and as the examples of such deposits increased in number and it became
evident that the plant fossils represented forms demanding a genial climate
and that the phenomena were seen in many countries, the belief grew that
minor fluctuations or gradual recession of an ice sheet were inadequate to
account for the phenomena observed.
It is natural that this problem should have found its solution in America,
where the Pleistocene is admirably displayed, and where the State and
Federal surveys were actively engaged in areal mapping. In 1883
Chamberlin[64] presented his views under the bold title, “Preliminary Paper
on the Terminal Moraine of the Second Glacial Epoch,” and the existence
of deposits of two or more ice sheets and the features of interglacial periods
were substantially established by the interesting debate in the Journal led by
Chamberlin, Wright, Upham and Dana.[65] Contributions since 1895 have
been concerned with the degree rather than the fact of complexity, and
continued study has resulted in the general recognition of five glacial stages
in North America and four in Europe.
Page 153
The Loess as a Glacial Deposit.
A curious side-product of the study of glaciation in North America is the
controversy over the origin of loess. The interest aroused is indicated by
scores of papers in American periodicals and State reports of the last quarter
of the 19th century—papers which bear the names of prominent geologists.
The “loess” in the valley of the Rhine had long been known, but the
subject assumed prominence by the publication in 1866 of Pumpelly’s
Travels in China.[66] Wide-spread deposits 200 to 1,000 feet thick were
described as very fine-grained yellowish earth of distinctive structure
without stratification but penetrated by innumerable tubes and containing
land or fresh-water shells. Pumpelly considered these deposits lacustrine, a
view which found general acceptance though combated by Kingsmill
(1871),[67] who argued for marine deposition. Baron Von Richthofen’s
classic on China, which appeared in 1877, amplifies the observations of
Pumpelly and marshals the evidence to support the hypothesis that the loess
is wind-laid both on dry land and within ancient salt lakes. The conclusions
of Von Richthofen were adopted by Pumpelly whose knowledge of the
Chinese deposits, supplemented by studies in Missouri, of which State he
was director of the Geological Survey in 1872–73, placed him in position to
form a correct judgment. He says:[68]
“Recognizing from personal observation the full identity of character of the loess of northern
China, Europe and the Missouri Valley, I am obliged to reject my own explanation of the origin of the
Chinese deposits, and to believe with Richthofen that the true loess, wherever it occurs, is a sub-
aerial deposit, formed in a dry central region, and that it owes its structure to the formative influence
of a steppe vegetation.
The one weak point of Richthofen’s theory is in the evident inadequacy of the current
disintegration as a source of material. When we consider the immense area covered by loess to
depths varying from 50 to 2,000 feet, and the fact that this is only the very finest portion of the
product of rock-destruction, and again that the accumulation represents only a very short period of
time, geologically speaking, surely we must seek a more fertile source of supply than is furnished by
the current decomposition of rock surface.
It seems to me that there are two important sources: I. The silt brought by rivers, many of them fed
by the products of glacial attrition flowing from the mountains into the central region. Where the
streams sink away, or where the lakes which receive them have dried up, the finer products of the
erosion of a large territory are left to be removed in dust storms.
II. The second ... source is the residuary products of a secular disintegration.”
A curious side-product of the study of glaciation in North America is the
controversy over the origin of loess. The interest aroused is indicated by
scores of papers in American periodicals and State reports of the last quarter
of the 19th century—papers which bear the names of prominent geologists.
The “loess” in the valley of the Rhine had long been known, but the
subject assumed prominence by the publication in 1866 of Pumpelly’s
Travels in China.[66] Wide-spread deposits 200 to 1,000 feet thick were
described as very fine-grained yellowish earth of distinctive structure
without stratification but penetrated by innumerable tubes and containing
land or fresh-water shells. Pumpelly considered these deposits lacustrine, a
view which found general acceptance though combated by Kingsmill
(1871),[67] who argued for marine deposition. Baron Von Richthofen’s
classic on China, which appeared in 1877, amplifies the observations of
Pumpelly and marshals the evidence to support the hypothesis that the loess
is wind-laid both on dry land and within ancient salt lakes. The conclusions
of Von Richthofen were adopted by Pumpelly whose knowledge of the
Chinese deposits, supplemented by studies in Missouri, of which State he
was director of the Geological Survey in 1872–73, placed him in position to
form a correct judgment. He says:[68]
“Recognizing from personal observation the full identity of character of the loess of northern
China, Europe and the Missouri Valley, I am obliged to reject my own explanation of the origin of the
Chinese deposits, and to believe with Richthofen that the true loess, wherever it occurs, is a sub-
aerial deposit, formed in a dry central region, and that it owes its structure to the formative influence
of a steppe vegetation.
The one weak point of Richthofen’s theory is in the evident inadequacy of the current
disintegration as a source of material. When we consider the immense area covered by loess to
depths varying from 50 to 2,000 feet, and the fact that this is only the very finest portion of the
product of rock-destruction, and again that the accumulation represents only a very short period of
time, geologically speaking, surely we must seek a more fertile source of supply than is furnished by
the current decomposition of rock surface.
It seems to me that there are two important sources: I. The silt brought by rivers, many of them fed
by the products of glacial attrition flowing from the mountains into the central region. Where the
streams sink away, or where the lakes which receive them have dried up, the finer products of the
erosion of a large territory are left to be removed in dust storms.
II. The second ... source is the residuary products of a secular disintegration.”
Page 154
The evidence presented by Pumpelly for the eolian origin of loess—
structure, texture, composition, fossil content and topographic position—is
complete, and to him belongs the credit for the correct interpretation of the
Mississippi valley deposits. Unfortunately his contribution came at a time
when the geologists of the central States were intent on tracing the paths
and explaining the work of Pleistocene glaciers, and the belief was strong
that loess was some phase of glacial work. Its position at the border of the
Iowan drift so obviously suggests a genetic relation that the fossil evidence
of steppe climate suggested by Binney in 1848[69] was minimized. Students
of Pleistocene geology in Minnesota, Iowa, Nebraska, Missouri, although
less vigorous in expression, were substantially in agreement with Hilgard
(1879).[70] “The sum total of anomalous conditions required to sustain the
eolian hypothesis partakes strongly of the marvellous.” The last edition of
Dana’s Manual, 1894, and of LeConte’s Geology, 1896, the two most
widely used text-books of their time, oppose the eolian theory, and
Chamberlin, in 1897,[71] states: “the aqueous hypothesis seems best
supported so far as concerns the deposits of the Mississippi Valley and
western Europe” (p. 795). Shimek, in papers published since 1896 has
shown that aquatic and glacial conditions can not account for the loess
fossils, and the return to the views of Pumpelly that the loess was deposited
on land by the agency of wind in a region of steppe vegetation is now all
but universal.
structure, texture, composition, fossil content and topographic position—is
complete, and to him belongs the credit for the correct interpretation of the
Mississippi valley deposits. Unfortunately his contribution came at a time
when the geologists of the central States were intent on tracing the paths
and explaining the work of Pleistocene glaciers, and the belief was strong
that loess was some phase of glacial work. Its position at the border of the
Iowan drift so obviously suggests a genetic relation that the fossil evidence
of steppe climate suggested by Binney in 1848[69] was minimized. Students
of Pleistocene geology in Minnesota, Iowa, Nebraska, Missouri, although
less vigorous in expression, were substantially in agreement with Hilgard
(1879).[70] “The sum total of anomalous conditions required to sustain the
eolian hypothesis partakes strongly of the marvellous.” The last edition of
Dana’s Manual, 1894, and of LeConte’s Geology, 1896, the two most
widely used text-books of their time, oppose the eolian theory, and
Chamberlin, in 1897,[71] states: “the aqueous hypothesis seems best
supported so far as concerns the deposits of the Mississippi Valley and
western Europe” (p. 795). Shimek, in papers published since 1896 has
shown that aquatic and glacial conditions can not account for the loess
fossils, and the return to the views of Pumpelly that the loess was deposited
on land by the agency of wind in a region of steppe vegetation is now all
but universal.
Page 155
Glacial Sculpture.
Within the present generation sculpture by glaciers has received much
attention and has involved a reconsideration of the ability of ice to erode
which in turn involves a crystallization of views of the mechanics of
moving ice. The evidence for glacier erosion has remained largely
physiographic and rests on a study of land forms. In fact, the inadequacy of
structural features or of river corrasion to account for flat-floored, steep-
walled gorges, hanging valleys, and many lake basins, rather than a
knowledge of the mechanics of ice has led to the present fairly general
belief that glaciers are powerful agents of rock sculpture. The details of the
process are not yet understood.
Erosion by glaciers enters the arena of active discussion in 1862–63. The
possibility had been suggested by Esmark (1827) and by Dana (1849) in the
description of fiords and by Hind (1855) with reference to the origin of the
Great Lakes. It appears full-fledged in Ramsay’s classic, which was
published simultaneously in England and in America.[72] The argument runs
as follows: There is a close association of ancient glaciers and lakes
especially in mountains; glaciers are amply able to erode; evidences of
faulting, special subsidence, river erosion, and marine erosion are absent
from the lake basins of Switzerland and Great Britain. To quote Ramsay:
“It required a solid body grinding steadily and powerfully in direct and heavy contact with and
across the rocks to scoop out deep hollows, the situations of which might either be determined by
unequal hardness of the rocks, by extra weight of ice in special places, or by accidental
circumstances, the clue to which is lost from our inability perfectly to reconstruct the original forms
of the glaciers.”
“I believe with the Italian geologists, that all that the glaciers as a whole effected was only slightly
to deepen these valleys and materially to modify their general outlines, and, further (a theory I am
alone responsible for), to deepen them in parts more considerably when, from various causes, the
grinding power of the ice was unusually powerful, especially where, as in the lowlands of
Switzerland, the Miocene strata are comparatively soft.”
Whittlesey (1864)[73] considered that the rock-bound lakes and narrow
bays near Lake Superior were partly excavated by ice. LeConte (1875)[74]
Within the present generation sculpture by glaciers has received much
attention and has involved a reconsideration of the ability of ice to erode
which in turn involves a crystallization of views of the mechanics of
moving ice. The evidence for glacier erosion has remained largely
physiographic and rests on a study of land forms. In fact, the inadequacy of
structural features or of river corrasion to account for flat-floored, steep-
walled gorges, hanging valleys, and many lake basins, rather than a
knowledge of the mechanics of ice has led to the present fairly general
belief that glaciers are powerful agents of rock sculpture. The details of the
process are not yet understood.
Erosion by glaciers enters the arena of active discussion in 1862–63. The
possibility had been suggested by Esmark (1827) and by Dana (1849) in the
description of fiords and by Hind (1855) with reference to the origin of the
Great Lakes. It appears full-fledged in Ramsay’s classic, which was
published simultaneously in England and in America.[72] The argument runs
as follows: There is a close association of ancient glaciers and lakes
especially in mountains; glaciers are amply able to erode; evidences of
faulting, special subsidence, river erosion, and marine erosion are absent
from the lake basins of Switzerland and Great Britain. To quote Ramsay:
“It required a solid body grinding steadily and powerfully in direct and heavy contact with and
across the rocks to scoop out deep hollows, the situations of which might either be determined by
unequal hardness of the rocks, by extra weight of ice in special places, or by accidental
circumstances, the clue to which is lost from our inability perfectly to reconstruct the original forms
of the glaciers.”
“I believe with the Italian geologists, that all that the glaciers as a whole effected was only slightly
to deepen these valleys and materially to modify their general outlines, and, further (a theory I am
alone responsible for), to deepen them in parts more considerably when, from various causes, the
grinding power of the ice was unusually powerful, especially where, as in the lowlands of
Switzerland, the Miocene strata are comparatively soft.”
Whittlesey (1864)[73] considered that the rock-bound lakes and narrow
bays near Lake Superior were partly excavated by ice. LeConte (1875)[74]
Page 156
records some significant observations in a pioneer paper on glacier erosion
which has not received adequate recognition. He says:
“... I am convinced that a glacier, by its enormous pressure and resistless onward movement, is
constantly breaking off large blocks from its bed and bounding walls. Its erosion is not only a
grinding and scoring, but also a crushing and breaking. It makes by its erosion not only rock-meal,
but also large rock-chips.... Its erosion is a constant process of alternate rough hewing and planing.
If Yosemite were unique, we might suppose that it was formed by violent cataclysms; but Yosemite
is not unique in form and therefore probably not in origin. There are many Yosemites. It is more
philosophical to account for them by the regular operation of known causes. I must believe that all
these deep perpendicular slots have been sawn out by the action of glaciers; the peculiar verticality of
the walls having been determined by the perpendicular cleavage structure.”... A lake in Bloody
Canyon “is a pure rock basin scooped out by the glacier at this place.... These ridges [separating
Hope, Faith, and Charity valleys] are in fact the lips of consecutive lake basins scooped out by ice.
... Water tends to form deep V-shaped canons, while ice produces broad valleys with lakes and
meadows.... I know not how general these distinctions may be, but certainly the Coast range of this
State is characterized by rounded summits and ridges, and deep V-shaped canons, while the high
Sierras are characterized on the contrary by sharp, spire-like, comb-like summits, and broad valleys;
and this difference I am convinced is due in part at least to the action of water on the one hand, and
of ice on the other.”
King (1878)[75] assigned to glacial erosion a commanding position in
mountain sculpture. In regard to the Uintas, he says:
“Glacial erosion has cut almost vertically down through the beds carving immense amphitheatres
with basin bottoms containing numerous Alpine lakes.... Post-glacial erosion has done an absolutely
trivial work. There is not a particle of direct evidence, so far as I can see, to warrant the belief that
these U-shaped canons were given their peculiar form by other means than the actual ploughing
erosion of glaciers....”
These contributions from the Cordilleras corroborating the conclusions of
Ramsay (1862), Tyndall (1862), Jukes (1862), Hector (1863), Logan
(1863), Close (1870), and James Geikie (1875), made little impression. The
views of Lyell (1833), Ball (1863), J. W. Dawson (1864), Falconer (1864),
Studer (1864), Murchison (1864, 1870), Ruskin (1865), Rutimeyer (1869),
Whymper (1871), Bonney (1873), Pfaff (1874), Gurlt (1874), Judd (1876),
prevailed, and the conclusions of Davis in 1882[76] fairly expressed the
prevailing belief in Europe and in America:
“The amount of glacial erosion in the central districts has been very considerable, but not greatly
in excess of pre-glacial soils and old talus and alluvial deposits. Most of the solid rock that was
which has not received adequate recognition. He says:
“... I am convinced that a glacier, by its enormous pressure and resistless onward movement, is
constantly breaking off large blocks from its bed and bounding walls. Its erosion is not only a
grinding and scoring, but also a crushing and breaking. It makes by its erosion not only rock-meal,
but also large rock-chips.... Its erosion is a constant process of alternate rough hewing and planing.
If Yosemite were unique, we might suppose that it was formed by violent cataclysms; but Yosemite
is not unique in form and therefore probably not in origin. There are many Yosemites. It is more
philosophical to account for them by the regular operation of known causes. I must believe that all
these deep perpendicular slots have been sawn out by the action of glaciers; the peculiar verticality of
the walls having been determined by the perpendicular cleavage structure.”... A lake in Bloody
Canyon “is a pure rock basin scooped out by the glacier at this place.... These ridges [separating
Hope, Faith, and Charity valleys] are in fact the lips of consecutive lake basins scooped out by ice.
... Water tends to form deep V-shaped canons, while ice produces broad valleys with lakes and
meadows.... I know not how general these distinctions may be, but certainly the Coast range of this
State is characterized by rounded summits and ridges, and deep V-shaped canons, while the high
Sierras are characterized on the contrary by sharp, spire-like, comb-like summits, and broad valleys;
and this difference I am convinced is due in part at least to the action of water on the one hand, and
of ice on the other.”
King (1878)[75] assigned to glacial erosion a commanding position in
mountain sculpture. In regard to the Uintas, he says:
“Glacial erosion has cut almost vertically down through the beds carving immense amphitheatres
with basin bottoms containing numerous Alpine lakes.... Post-glacial erosion has done an absolutely
trivial work. There is not a particle of direct evidence, so far as I can see, to warrant the belief that
these U-shaped canons were given their peculiar form by other means than the actual ploughing
erosion of glaciers....”
These contributions from the Cordilleras corroborating the conclusions of
Ramsay (1862), Tyndall (1862), Jukes (1862), Hector (1863), Logan
(1863), Close (1870), and James Geikie (1875), made little impression. The
views of Lyell (1833), Ball (1863), J. W. Dawson (1864), Falconer (1864),
Studer (1864), Murchison (1864, 1870), Ruskin (1865), Rutimeyer (1869),
Whymper (1871), Bonney (1873), Pfaff (1874), Gurlt (1874), Judd (1876),
prevailed, and the conclusions of Davis in 1882[76] fairly expressed the
prevailing belief in Europe and in America:
“The amount of glacial erosion in the central districts has been very considerable, but not greatly
in excess of pre-glacial soils and old talus and alluvial deposits. Most of the solid rock that was
Page 157
carried away came from ledges rather than from valleys; and glaciers had in general a smoothing
rather than a roughening effect. In the outer areas on which the ice advanced it only rubbed down the
projecting points; here it acted more frequently as a depositing than as an eroding agent.”
During the past quarter-century the cleavage in the ranks of geologists,
brought about by Ramsay’s classic paper, has remained. Fairchild and
others in America, Heim, Bonney, and Garwood in Europe argue for
insignificant erosion by glaciers; and Gannet, Davis, Gilbert, Tarr in
America followed by Austrian workers present evidence for erosion on a
gigantic scale. A perusal of the voluminous literature in the Journal and
elsewhere shows that the difference of opinion is in part one of terms, the
amount of erosion rather than the fact of erosion; it also arises from failure
to differentiate the work of mountain glaciers and continental ice sheets, of
Pleistocene glaciers and their present diminished representatives. The
irrelevant contribution of physicists has also made for confusion.
It is interesting to note that the criteria for erosion of valleys by glaciers
has long been established and by workers in different countries. Ramsay
(1862) in England outlined the problem and presented generalized
evidence. Hector (1863) in New Zealand pointed out the significance of
discordant drainage, the “hanging valleys” of Gilbert. The U-form, the
broad lake-dotted floor, and the presence of cirques and the process of
plucking were probably first described by LeConte (1873) in America. The
truncation of valley spurs by glaciers pointed out by Studer in the
Kerguelen Islands (1878) was used by Chamberlin (1883) as evidence of
glacial scouring.
rather than a roughening effect. In the outer areas on which the ice advanced it only rubbed down the
projecting points; here it acted more frequently as a depositing than as an eroding agent.”
During the past quarter-century the cleavage in the ranks of geologists,
brought about by Ramsay’s classic paper, has remained. Fairchild and
others in America, Heim, Bonney, and Garwood in Europe argue for
insignificant erosion by glaciers; and Gannet, Davis, Gilbert, Tarr in
America followed by Austrian workers present evidence for erosion on a
gigantic scale. A perusal of the voluminous literature in the Journal and
elsewhere shows that the difference of opinion is in part one of terms, the
amount of erosion rather than the fact of erosion; it also arises from failure
to differentiate the work of mountain glaciers and continental ice sheets, of
Pleistocene glaciers and their present diminished representatives. The
irrelevant contribution of physicists has also made for confusion.
It is interesting to note that the criteria for erosion of valleys by glaciers
has long been established and by workers in different countries. Ramsay
(1862) in England outlined the problem and presented generalized
evidence. Hector (1863) in New Zealand pointed out the significance of
discordant drainage, the “hanging valleys” of Gilbert. The U-form, the
broad lake-dotted floor, and the presence of cirques and the process of
plucking were probably first described by LeConte (1873) in America. The
truncation of valley spurs by glaciers pointed out by Studer in the
Kerguelen Islands (1878) was used by Chamberlin (1883) as evidence of
glacial scouring.
Page 158
Conclusion.
During the past century many principles of land sculpture have emerged
from the fog of intellectual speculation and unorganized observation and
taken their place among generally accepted truths. Many of them are no
longer subjects of controversy. Erosion has found its place as a major
geologic agent and has given a new conception of natural scenery. Lofty
mountains are no longer “ancient as the sun,” they are youthful features in
process of dissection; valleys and canyons are the work of streams and
glaciers; fiords are erosion forms; waterfalls and lakes are features in
process of elimination; many plains and plateaus owe their form and
position to long-continued denudation. Modern landscapes are no longer
viewed as original features or the product of a single agent acting at a
particular time, but as ephemeral forms which owe their present appearance
to their age and the particular forces at work upon them as well as to their
original structure.
It is interesting to note the halting steps leading to the present viewpoint,
to find that decades elapsed between the formulation of a theory or the
recording of significant facts and their final acceptance or rejection, and to
realize that the organization of principles and observations into a science of
physiography has been the work of the present generation. Progress has
been conditioned by a number of factors besides the intellectual ability of
individual workers.
The influence of locality is plainly seen. Convincing evidence of river
erosion was obtained in central France, the Pacific Islands, and the
Colorado Plateau—regions in which other causes were easily eliminated.
Sculpture by glaciers passed beyond the theoretical stage when the simple
forms of the Sierras and New Zealand Alps were described. The origin of
loess was first discerned in a region where glacial phenomena did not
obscure the vision. The complexity of the Glacial period asserted by
geologists of the Middle West was denied by eastern students. The work of
waves on the English coast impressed British geologists to such an extent
that plains of denudation and inland valleys were ascribed to ocean work.
During the past century many principles of land sculpture have emerged
from the fog of intellectual speculation and unorganized observation and
taken their place among generally accepted truths. Many of them are no
longer subjects of controversy. Erosion has found its place as a major
geologic agent and has given a new conception of natural scenery. Lofty
mountains are no longer “ancient as the sun,” they are youthful features in
process of dissection; valleys and canyons are the work of streams and
glaciers; fiords are erosion forms; waterfalls and lakes are features in
process of elimination; many plains and plateaus owe their form and
position to long-continued denudation. Modern landscapes are no longer
viewed as original features or the product of a single agent acting at a
particular time, but as ephemeral forms which owe their present appearance
to their age and the particular forces at work upon them as well as to their
original structure.
It is interesting to note the halting steps leading to the present viewpoint,
to find that decades elapsed between the formulation of a theory or the
recording of significant facts and their final acceptance or rejection, and to
realize that the organization of principles and observations into a science of
physiography has been the work of the present generation. Progress has
been conditioned by a number of factors besides the intellectual ability of
individual workers.
The influence of locality is plainly seen. Convincing evidence of river
erosion was obtained in central France, the Pacific Islands, and the
Colorado Plateau—regions in which other causes were easily eliminated.
Sculpture by glaciers passed beyond the theoretical stage when the simple
forms of the Sierras and New Zealand Alps were described. The origin of
loess was first discerned in a region where glacial phenomena did not
obscure the vision. The complexity of the Glacial period asserted by
geologists of the Middle West was denied by eastern students. The work of
waves on the English coast impressed British geologists to such an extent
that plains of denudation and inland valleys were ascribed to ocean work.
Page 159
In the establishment of principles, the friendly interchange of ideas has
yielded large returns. Many of the fundamental conceptions of earth
sculpture have come from groups of men so situated as to facilitate
criticism. It is impossible, even if desirable, to award individual credit to
Venetz, Charpentier, and Agassiz in the formulation of the glacial theory;
and the close association of Agassiz and Dana in New England and of
Chamberlin and Irving in Wisconsin was undoubtedly helpful in
establishing the theory of continental glaciation. From the intimate
companionship in field and laboratory of Hutton, Playfair and Hope, arose
the profound influence of the Edinburgh school, and the sympathetic
cooperation of Powell, Gilbert, and Dutton has given to the world its
classics in the genetic study of land forms.
The influence of ideas has been closely associated with clarity,
conciseness, and attractiveness of presentation. Hutton is known through
Playfair, Agassiz’s contributions to glacial geology are known to every
student, while Venetz, Charpentier, and Hugi are only names. Cuvier’s
discourses on dynamical geology were reprinted and translated into English
and German, but Lamarck’s “Hydrogéologie” is known only to book
collectors. The verbose works of Guettard, although carrying the same
message as Playfair’s “Illustrations” and Desmarest’s “Memoirs,” are
practically unknown, as is also Horace H. Hayden’s treatise (1821) on the
drift of eastern North America. It has been well said that the world-wide
influence of American physiographic teaching is due in no small part to the
masterly presentations of Gilbert and Davis.
It is surprising to note the delays, the backward steps, and the duplication
of effort resulting from lack of familiarity with the work of the pioneers.
Sabine says in 1864:[77]
“It often happens, not unnaturally, that those who are most occupied with the questions of the day
in an advancing science retain but an imperfect recollection of the obligations due to those who laid
the first foundations of our subsequent knowledge.”
The product of intellectual effort appears to be conditioned by time of
planting and character of soil as well as by quantity of seed. For example:
Erosion by rivers was as clearly shown by Desmarest as by Dana and
Newberry 50 years later. Criteria for the recognition of ancient fluviatile
yielded large returns. Many of the fundamental conceptions of earth
sculpture have come from groups of men so situated as to facilitate
criticism. It is impossible, even if desirable, to award individual credit to
Venetz, Charpentier, and Agassiz in the formulation of the glacial theory;
and the close association of Agassiz and Dana in New England and of
Chamberlin and Irving in Wisconsin was undoubtedly helpful in
establishing the theory of continental glaciation. From the intimate
companionship in field and laboratory of Hutton, Playfair and Hope, arose
the profound influence of the Edinburgh school, and the sympathetic
cooperation of Powell, Gilbert, and Dutton has given to the world its
classics in the genetic study of land forms.
The influence of ideas has been closely associated with clarity,
conciseness, and attractiveness of presentation. Hutton is known through
Playfair, Agassiz’s contributions to glacial geology are known to every
student, while Venetz, Charpentier, and Hugi are only names. Cuvier’s
discourses on dynamical geology were reprinted and translated into English
and German, but Lamarck’s “Hydrogéologie” is known only to book
collectors. The verbose works of Guettard, although carrying the same
message as Playfair’s “Illustrations” and Desmarest’s “Memoirs,” are
practically unknown, as is also Horace H. Hayden’s treatise (1821) on the
drift of eastern North America. It has been well said that the world-wide
influence of American physiographic teaching is due in no small part to the
masterly presentations of Gilbert and Davis.
It is surprising to note the delays, the backward steps, and the duplication
of effort resulting from lack of familiarity with the work of the pioneers.
Sabine says in 1864:[77]
“It often happens, not unnaturally, that those who are most occupied with the questions of the day
in an advancing science retain but an imperfect recollection of the obligations due to those who laid
the first foundations of our subsequent knowledge.”
The product of intellectual effort appears to be conditioned by time of
planting and character of soil as well as by quantity of seed. For example:
Erosion by rivers was as clearly shown by Desmarest as by Dana and
Newberry 50 years later. Criteria for the recognition of ancient fluviatile
Page 160
deposits were established by James Deane in 1847 in a study of the
Connecticut Valley Triassic. Agassiz’s proof that ice is an essential factor in
the formation of till is substantially a duplication of Dobson’s observations
(1826).
The volumes of the Journal with their very large number of articles and
reviews dealing with geology show that the interpretation of land forms as
products of subaërial erosion began in France and French Switzerland
during the later part of the eighteenth century as a phase of the intellectual
emancipation following the Revolution. Scotland and England assumed the
leadership for the first half of the nineteenth century, and the first 100
volumes of the Journal show the profound influence of English and French
teaching. In America, independent thinking, early exercised by the few,
became general with the establishment of the Federal survey, the increase in
university departments, geological societies and periodicals, and has given
to Americans the responsibilities of teachers.
Connecticut Valley Triassic. Agassiz’s proof that ice is an essential factor in
the formation of till is substantially a duplication of Dobson’s observations
(1826).
The volumes of the Journal with their very large number of articles and
reviews dealing with geology show that the interpretation of land forms as
products of subaërial erosion began in France and French Switzerland
during the later part of the eighteenth century as a phase of the intellectual
emancipation following the Revolution. Scotland and England assumed the
leadership for the first half of the nineteenth century, and the first 100
volumes of the Journal show the profound influence of English and French
teaching. In America, independent thinking, early exercised by the few,
became general with the establishment of the Federal survey, the increase in
university departments, geological societies and periodicals, and has given
to Americans the responsibilities of teachers.
Page 161
Bibliography.
(In the following list “this Journal” refers to the American Journal of
Science.)
4. Wilson, J. W., Bursting of lakes through mountains, this Journal, 3, 253, 1821.
5. Whitney, J. D., Progress of the Geological Survey of California, this Journal, 38, 263–264,
1864.
6. Playfair, John, Illustrations of the Huttonian theory of the earth, Edinburgh, 1802.
7. Kain, J. H., Remarks on the mineralogy and geology of northwestern Virginia and eastern
Tennessee, this Journal, 1, 60–67, 1819.
8. Hitchcock, Edward, Geology, etc., of regions contiguous to the Connecticut, this Journal, 7,
1–30, 1824.
9. Buckland, Wm., Reliquiæ diluvianæ, this Journal, 8, 150, 317, 1824.
10. Phillips, John, Geology of Yorkshire, this Journal, 21, 17–20, 1832.
11. Scrope, G. P., Excavation of valleys, Geol. Soc., London, No. 14, 1830.
12. Hayes, G. E., Remarks on geology and topography of western New York, this Journal, 35,
88–91, 1839.
13. Seventh Meeting of the British Association for the Advancement of Science, this Journal,
33, 288, 1838.
14. Darwin, Charles, Geological observations on the volcanic islands and parts of South
America, etc., second part of the Voyage of the “Beagle,” during 1832–1836. London, 1844.
15. Hildreth, S. P., Observations, etc., valley of the Ohio, this Journal, 29, 1–148, 1836.
16. Geddes, James, Observations on the geological features of the south side of Ontario valley,
this Journal, 11, 213–218, 1826.
18. Warren, G. K., Preliminary report of explorations in Nebraska and Dakota, this Journal, 27,
380, 1859.
19. Lesley, J. P., Observations on the Appalachian region of southern Virginia, this Journal, 34,
review, 413–415, 1862.
17. Conrad, T. A., Notes on American geology, this Journal, 35, 237–251, 1839.
20. Dana, J. D., On denudation in the Pacific, this Journal, 9, 48–62, 1850.
(In the following list “this Journal” refers to the American Journal of
Science.)
4. Wilson, J. W., Bursting of lakes through mountains, this Journal, 3, 253, 1821.
5. Whitney, J. D., Progress of the Geological Survey of California, this Journal, 38, 263–264,
1864.
6. Playfair, John, Illustrations of the Huttonian theory of the earth, Edinburgh, 1802.
7. Kain, J. H., Remarks on the mineralogy and geology of northwestern Virginia and eastern
Tennessee, this Journal, 1, 60–67, 1819.
8. Hitchcock, Edward, Geology, etc., of regions contiguous to the Connecticut, this Journal, 7,
1–30, 1824.
9. Buckland, Wm., Reliquiæ diluvianæ, this Journal, 8, 150, 317, 1824.
10. Phillips, John, Geology of Yorkshire, this Journal, 21, 17–20, 1832.
11. Scrope, G. P., Excavation of valleys, Geol. Soc., London, No. 14, 1830.
12. Hayes, G. E., Remarks on geology and topography of western New York, this Journal, 35,
88–91, 1839.
13. Seventh Meeting of the British Association for the Advancement of Science, this Journal,
33, 288, 1838.
14. Darwin, Charles, Geological observations on the volcanic islands and parts of South
America, etc., second part of the Voyage of the “Beagle,” during 1832–1836. London, 1844.
15. Hildreth, S. P., Observations, etc., valley of the Ohio, this Journal, 29, 1–148, 1836.
16. Geddes, James, Observations on the geological features of the south side of Ontario valley,
this Journal, 11, 213–218, 1826.
18. Warren, G. K., Preliminary report of explorations in Nebraska and Dakota, this Journal, 27,
380, 1859.
19. Lesley, J. P., Observations on the Appalachian region of southern Virginia, this Journal, 34,
review, 413–415, 1862.
17. Conrad, T. A., Notes on American geology, this Journal, 35, 237–251, 1839.
20. Dana, J. D., On denudation in the Pacific, this Journal, 9, 48–62, 1850.
Page 162
——, On the degradation of the rocks of New South Wales and formation of valleys, this
Journal, 9, 289–294, 1850.
21. Hubbard, O. P., On the condition of trap dikes in New Hampshire an evidence and measure
of erosion, this Journal, 9, 158–171, 1850.
22. Hayden, F. V., Some remarks in regard to the period of elevation of the Rocky Mountains,
this Journal, 33, 305–313, 1862.
23. Newberry, J. S., Colorado River of the West, this Journal, 33, review, 387–403, 1862.
24. Jukes, J. B., Address to the Geological Section of the British Association at Cambridge,
Quart. Jour. Geol. Soc., 18, 1862, this Journal, 34, 439, 1862.
25. Powell, J. W., Exploration of the Colorado River of the West, 1875. For Powell’s
preliminary article see this Journal, 5, 456–465, 1873.
26. McGee, W. J., Three formations of the Middle Atlantic slope, this Journal, 35, 120, 328, 367,
448, 1888.
27. Davis, W. M., Topographic development of the Triassic formation of the Connecticut Valley,
this Journal, 37, 423–434, 1889.
28. Percival, J. G., Geology of Connecticut, 1842.
29. Kerr, W. C., Origin of some new points in the topography of North Carolina, this Journal,
21, 216–219, 1881.
30. McGee, W. J., The classification of geographic forms by genesis, Nat. Geogr. Mag., 1, 27–
36, 1888.
31. Davis, W. M., The rivers and valleys of Pennsylvania, Nat. Geogr. Mag., 1, 183–253, 1889.
——, The rivers of northern New Jersey with notes on the classification of rivers in general,
ibid., 2, 81–110, 1890.
32. Silliman, Benjamin, Notice of Horace H. Hayden’s geological essays, this Journal, 3, 49,
1821.
33. Cornelius, Elias, Account of a singular position of a granite rock, this Journal, 2, 200–201,
1820.
34. Finch, John, On the Celtic antiquities of America, this Journal, 7, 149–161, 1824.
35. Finch, John, Geological essay on the Tertiary formations in America, this Journal, 7, 31–43,
1824.
36. Conybeare and Phillips, Outlines of the geology of England and Wales, this Journal, 7, 210,
211, 1824.
37. Hayden, Horace H., Geological essays, 1–412, 1821, this Journal, 3, 47–57, 1821.
Journal, 9, 289–294, 1850.
21. Hubbard, O. P., On the condition of trap dikes in New Hampshire an evidence and measure
of erosion, this Journal, 9, 158–171, 1850.
22. Hayden, F. V., Some remarks in regard to the period of elevation of the Rocky Mountains,
this Journal, 33, 305–313, 1862.
23. Newberry, J. S., Colorado River of the West, this Journal, 33, review, 387–403, 1862.
24. Jukes, J. B., Address to the Geological Section of the British Association at Cambridge,
Quart. Jour. Geol. Soc., 18, 1862, this Journal, 34, 439, 1862.
25. Powell, J. W., Exploration of the Colorado River of the West, 1875. For Powell’s
preliminary article see this Journal, 5, 456–465, 1873.
26. McGee, W. J., Three formations of the Middle Atlantic slope, this Journal, 35, 120, 328, 367,
448, 1888.
27. Davis, W. M., Topographic development of the Triassic formation of the Connecticut Valley,
this Journal, 37, 423–434, 1889.
28. Percival, J. G., Geology of Connecticut, 1842.
29. Kerr, W. C., Origin of some new points in the topography of North Carolina, this Journal,
21, 216–219, 1881.
30. McGee, W. J., The classification of geographic forms by genesis, Nat. Geogr. Mag., 1, 27–
36, 1888.
31. Davis, W. M., The rivers and valleys of Pennsylvania, Nat. Geogr. Mag., 1, 183–253, 1889.
——, The rivers of northern New Jersey with notes on the classification of rivers in general,
ibid., 2, 81–110, 1890.
32. Silliman, Benjamin, Notice of Horace H. Hayden’s geological essays, this Journal, 3, 49,
1821.
33. Cornelius, Elias, Account of a singular position of a granite rock, this Journal, 2, 200–201,
1820.
34. Finch, John, On the Celtic antiquities of America, this Journal, 7, 149–161, 1824.
35. Finch, John, Geological essay on the Tertiary formations in America, this Journal, 7, 31–43,
1824.
36. Conybeare and Phillips, Outlines of the geology of England and Wales, this Journal, 7, 210,
211, 1824.
37. Hayden, Horace H., Geological essays, 1–412, 1821, this Journal, 3, 47–57, 1821.
Page 163
38. Jackson, C. T., Reports on the geology of the State of Maine, and on the public lands
belonging to Maine and Massachusetts, this Journal, 36, 153, 1839.
39. Gibson, J. B., Remarks on the geology of the lakes and the valley of the Mississippi, this
Journal, 29, 201–213, 1836.
40. Phillips, John, Geology of Yorkshire, this Journal, 21, 14–15, 1832.
41. Granger, Ebenezer, Notice of a curious fluted rock at Sandusky Bay, Ohio, this Journal, 6,
180, 1823.
42. Dobson, Peter, Remarks on bowlders, this Journal, 10, 217–218, 1826.
43. Murchison, R. I., Address at anniversary meeting of the Geological Society of London, this
Journal, 43, 200–201, 1842.
44. Peter Dobson (1784–1878) came to this country from Preston, England, in 1809 and
established a cotton factory at Vernon, Conn.
45. Buckland, W., On the evidence of glaciers in Scotland and the north of England, Proc.
London Geol. Soc., 3, 1841.
46. Hitchcock, Edward, First anniversary address before the Association of American
Geologists, this Journal, 41, 232–275, 1841.
47. Third annual meeting of the Association of American Geologists and Naturalists, this
Journal, 43, 154, 1842; Abstract of proceedings of the fourth session of the Association of American
Geologists and Naturalists, ibid., 45, 321, 1843.
48. Rogers, H. D., Address delivered before Association of American Geologists and
Naturalists, this Journal, 47, 275, 1844.
49. Agassiz, Louis, The erratic phenomena about Lake Superior, this Journal, 10, 83–101, 1850.
50. Desor, E., On the drift of Lake Superior, this Journal, 13, 93–109, 1852; Post-Pliocene of the
southern States, etc., 14, 49–59, 1852.
51. Dana, J. D., Manual of geology, 546, Philadelphia, 1863.
52. Dana, J. D., on the Quaternary, or post-Tertiary of the New Haven region, this Journal, 1, 1–
5, 1871.
53. Matthew, G. F., Surface geology of New Brunswick, this Journal, 2, 371–372, 1871.
54. Maclaren, Charles, The glacial theory of Prof. Agassiz, this Journal, 42, 365, 1842.
55. Daly, R. A., Problems of the Pacific Islands, this Journal, 41, 153–186, 1916.
56. Catlin, George, Account of a journey to the Côteau des Prairies, this Journal, 38, 138–146,
1840.
57. Hilgard, E. W., Remarks on the drift of the western and southern States and its relation to the
glacier and iceberg theories, this Journal, 42, 343–347, 1866.
belonging to Maine and Massachusetts, this Journal, 36, 153, 1839.
39. Gibson, J. B., Remarks on the geology of the lakes and the valley of the Mississippi, this
Journal, 29, 201–213, 1836.
40. Phillips, John, Geology of Yorkshire, this Journal, 21, 14–15, 1832.
41. Granger, Ebenezer, Notice of a curious fluted rock at Sandusky Bay, Ohio, this Journal, 6,
180, 1823.
42. Dobson, Peter, Remarks on bowlders, this Journal, 10, 217–218, 1826.
43. Murchison, R. I., Address at anniversary meeting of the Geological Society of London, this
Journal, 43, 200–201, 1842.
44. Peter Dobson (1784–1878) came to this country from Preston, England, in 1809 and
established a cotton factory at Vernon, Conn.
45. Buckland, W., On the evidence of glaciers in Scotland and the north of England, Proc.
London Geol. Soc., 3, 1841.
46. Hitchcock, Edward, First anniversary address before the Association of American
Geologists, this Journal, 41, 232–275, 1841.
47. Third annual meeting of the Association of American Geologists and Naturalists, this
Journal, 43, 154, 1842; Abstract of proceedings of the fourth session of the Association of American
Geologists and Naturalists, ibid., 45, 321, 1843.
48. Rogers, H. D., Address delivered before Association of American Geologists and
Naturalists, this Journal, 47, 275, 1844.
49. Agassiz, Louis, The erratic phenomena about Lake Superior, this Journal, 10, 83–101, 1850.
50. Desor, E., On the drift of Lake Superior, this Journal, 13, 93–109, 1852; Post-Pliocene of the
southern States, etc., 14, 49–59, 1852.
51. Dana, J. D., Manual of geology, 546, Philadelphia, 1863.
52. Dana, J. D., on the Quaternary, or post-Tertiary of the New Haven region, this Journal, 1, 1–
5, 1871.
53. Matthew, G. F., Surface geology of New Brunswick, this Journal, 2, 371–372, 1871.
54. Maclaren, Charles, The glacial theory of Prof. Agassiz, this Journal, 42, 365, 1842.
55. Daly, R. A., Problems of the Pacific Islands, this Journal, 41, 153–186, 1916.
56. Catlin, George, Account of a journey to the Côteau des Prairies, this Journal, 38, 138–146,
1840.
57. Hilgard, E. W., Remarks on the drift of the western and southern States and its relation to the
glacier and iceberg theories, this Journal, 42, 343–347, 1866.
Page 164
58. Hall, C. E., Glacial phenomena along the Kittatinny or Blue Mountain, Pennsylvania, this
Journal, 11, review, 233, 1876.
59. Stevens, R. P., On glaciers of the glacial era in Virginia, this Journal, 6, 371–373, 1873.
60. Rogers, W. B., On the gravel and cobble-stone deposits of Virginia and the Middle States,
Proc. Boston Soc. Nat. Hist., 18, 1875; this Journal, 11, 60–61, 1876.
61. Kerr, W. C, Origin of some new points in the topography of North Carolina, this Journal, 21,
216–219, 1881.
62. Gilbert, G. K., On certain glacial and post-glacial phenomena of the Maumee valley, this
Journal, 1, 339–345, 1871.
63. Chamberlin, T. C., On the geology of eastern Wisconsin, Geol. of Wisconsin, 2, 1877; this
Journal, 15, 61, 406, 1878.
64. Chamberlin, T. C, Preliminary paper on the terminal moraine of the second glacial epoch, U.
S. Geol. Survey, Third Ann. Rept., 291–402, 1883.
65. Wright, G. F., Unity of the glacial epoch, this Journal, 44, 351–373, 1892.
Upham, Warren, The diversity of the glacial drift along its boundary, ibid., 47, 358–365, 1894.
Wright, G. F., Theory of an interglacial submergence in England, ibid., 43, 1–8, 1892.
Chamberlin, T. C., Diversity of the glacial period, ibid., 45, 171–200, 1983
Dana, J. D., On New England and the upper Mississippi basin in the glacial period, ibid., 46,
327–330, 1893.
Wright, G. F., Continuity of the glacial period, ibid., 47, 161–187, 1894.
Chamberlin, T. C. and Leverett, F., Further studies of the drainage features of the upper Ohio
basin, ibid., 47, 247–282, 1894.
66. Pumpelly, Raphael, Geological researches in China, Japan, and Mongolia, Smithsonian
Contributions, No. 202, 1866.
67. Kingsmill, T. W., The probable origin of “loess” in North China and eastern Asia, Quart.
Jour. Geol. Soc., 27, No. 108, 1871.
68. Pumpelly, Raphael, The relation of secular rock-disintegration to loess, glacial drift and rock
basins, this Journal, 17, 135, 1879.
69. Binney, A., Some geologic features at Natchez on the Mississippi River, Proc. Boston Soc.
Nat. Hist., 2, 126–130, 1848.
70. Hilgard, E. W., The loess of Mississippi Valley, and the eolian hypothesis, this Journal, 18,
106–112, 1879.
71. Chamberlin, T. C, Supplementary hypothesis respecting the origin of the loess of the
Mississippi Valley, Jour. Geol., 5, 795–802, 1897.
Journal, 11, review, 233, 1876.
59. Stevens, R. P., On glaciers of the glacial era in Virginia, this Journal, 6, 371–373, 1873.
60. Rogers, W. B., On the gravel and cobble-stone deposits of Virginia and the Middle States,
Proc. Boston Soc. Nat. Hist., 18, 1875; this Journal, 11, 60–61, 1876.
61. Kerr, W. C, Origin of some new points in the topography of North Carolina, this Journal, 21,
216–219, 1881.
62. Gilbert, G. K., On certain glacial and post-glacial phenomena of the Maumee valley, this
Journal, 1, 339–345, 1871.
63. Chamberlin, T. C., On the geology of eastern Wisconsin, Geol. of Wisconsin, 2, 1877; this
Journal, 15, 61, 406, 1878.
64. Chamberlin, T. C, Preliminary paper on the terminal moraine of the second glacial epoch, U.
S. Geol. Survey, Third Ann. Rept., 291–402, 1883.
65. Wright, G. F., Unity of the glacial epoch, this Journal, 44, 351–373, 1892.
Upham, Warren, The diversity of the glacial drift along its boundary, ibid., 47, 358–365, 1894.
Wright, G. F., Theory of an interglacial submergence in England, ibid., 43, 1–8, 1892.
Chamberlin, T. C., Diversity of the glacial period, ibid., 45, 171–200, 1983
Dana, J. D., On New England and the upper Mississippi basin in the glacial period, ibid., 46,
327–330, 1893.
Wright, G. F., Continuity of the glacial period, ibid., 47, 161–187, 1894.
Chamberlin, T. C. and Leverett, F., Further studies of the drainage features of the upper Ohio
basin, ibid., 47, 247–282, 1894.
66. Pumpelly, Raphael, Geological researches in China, Japan, and Mongolia, Smithsonian
Contributions, No. 202, 1866.
67. Kingsmill, T. W., The probable origin of “loess” in North China and eastern Asia, Quart.
Jour. Geol. Soc., 27, No. 108, 1871.
68. Pumpelly, Raphael, The relation of secular rock-disintegration to loess, glacial drift and rock
basins, this Journal, 17, 135, 1879.
69. Binney, A., Some geologic features at Natchez on the Mississippi River, Proc. Boston Soc.
Nat. Hist., 2, 126–130, 1848.
70. Hilgard, E. W., The loess of Mississippi Valley, and the eolian hypothesis, this Journal, 18,
106–112, 1879.
71. Chamberlin, T. C, Supplementary hypothesis respecting the origin of the loess of the
Mississippi Valley, Jour. Geol., 5, 795–802, 1897.
Page 165
72. Ramsay, A. C., On the glacial origin of certain lakes in Switzerland, the Black Forest, Great
Britain, Sweden, North America, and elsewhere, Quart. Jour. Geol. Soc., 1862; this Journal, 35, 324–
345, 1863. Preliminary statements of this theory appeared in 1859 and 1860.
73. Whittlesey, Charles, Smithsonian Contributions, No. 197, 1864.
74. LeConte, Joseph, On some of the ancient glaciers of the Sierras, this Journal, 5, 325–342,
1873, 10, 126–139, 1875.
75. King, Clarence, U. S. Geol. Expl. 40th Par., 1, 459–529, 1878.
76. Davis, W. M., Glacial erosion, Proc. Boston Soc. Nat. Hist., 22, 58, 1882.
77. Sabine, Sir Edward, Address of the president of the Royal Society, this Journal, 37, 108,
1864.
Britain, Sweden, North America, and elsewhere, Quart. Jour. Geol. Soc., 1862; this Journal, 35, 324–
345, 1863. Preliminary statements of this theory appeared in 1859 and 1860.
73. Whittlesey, Charles, Smithsonian Contributions, No. 197, 1864.
74. LeConte, Joseph, On some of the ancient glaciers of the Sierras, this Journal, 5, 325–342,
1873, 10, 126–139, 1875.
75. King, Clarence, U. S. Geol. Expl. 40th Par., 1, 459–529, 1878.
76. Davis, W. M., Glacial erosion, Proc. Boston Soc. Nat. Hist., 22, 58, 1882.
77. Sabine, Sir Edward, Address of the president of the Royal Society, this Journal, 37, 108,
1864.
Page 166
IV
A CENTURY OF GEOLOGY.—THE GROWTH OF
KNOWLEDGE OF EARTH STRUCTURE
By JOSEPH BARRELL
Introduction
The Intellectual Viewpoint in 1818.
In 1818, the year of the founding of the Journal, the natural sciences were
still in their infancy in Europe. Geology was still subordinate to mineralogy,
was hardly recognized as a distinct science, and consisted in little more than
a description of the character and distribution of minerals and rocks.
America was remote from the Old World centers of learning. The energy of
the young nation was absorbed in its own expansion, and but a few of those
who by aptitude were fitted to increase scientific knowledge were even
conscious of the existence of such a field of endeavor. Under these
circumstances the educative field open to a journal of science in the United
States was an almost virgin soil. Original contributions could most readily
be based upon the natural history of the New World, and the founder of the
Journal showed insight appreciative of the situation in stating in the “Plan
of the Work” in the introduction to the first volume that “It will be a leading
object to illustrate American Natural History, and especially our
Mineralogy and Geology.”
At this time educated people were still satisfied that the whole knowledge
of the origin and development of the earth so far as man could or should
know it was embraced in the Book of Genesis. They were inclined to look
A CENTURY OF GEOLOGY.—THE GROWTH OF
KNOWLEDGE OF EARTH STRUCTURE
By JOSEPH BARRELL
Introduction
The Intellectual Viewpoint in 1818.
In 1818, the year of the founding of the Journal, the natural sciences were
still in their infancy in Europe. Geology was still subordinate to mineralogy,
was hardly recognized as a distinct science, and consisted in little more than
a description of the character and distribution of minerals and rocks.
America was remote from the Old World centers of learning. The energy of
the young nation was absorbed in its own expansion, and but a few of those
who by aptitude were fitted to increase scientific knowledge were even
conscious of the existence of such a field of endeavor. Under these
circumstances the educative field open to a journal of science in the United
States was an almost virgin soil. Original contributions could most readily
be based upon the natural history of the New World, and the founder of the
Journal showed insight appreciative of the situation in stating in the “Plan
of the Work” in the introduction to the first volume that “It will be a leading
object to illustrate American Natural History, and especially our
Mineralogy and Geology.”
At this time educated people were still satisfied that the whole knowledge
of the origin and development of the earth so far as man could or should
know it was embraced in the Book of Genesis. They were inclined to look
Page 167
with misgiving at attempts to directly interrogate the earth as to its history.
Philosophers such as Descartes and Liebnitz, the cosmogonists de Maillet
and Buffon had been less instrumental in developing science than in fitting
a few facts and many speculations to their systems of philosophy. By the
opening of the nineteenth century, however, men of learning were coming
to appreciate that the way to advance science was to experiment and
observe, to collect facts and discourage unfounded speculation. Silliman’s
insight into the needs of geologic science is shown in the following
quotation (1, pp. 6, 7, 1818):
“Our geology, also, presents a most interesting field of inquiry. A grand outline has recently been
drawn by Mr. Maclure, with a masterly hand, and with a vast extent of personal observation and
labour: but to fill up the detail, both observation and labour still more extensive are demanded; nor
can the object be effected, till more good geologists are formed, and distributed over our extensive
territory.
To account for the formation and changes of our globe, by excursions of the imagination, often
splendid and imposing, but usually visionary, and almost always baseless, was, till within half a
century, the business of geological speculations; but this research has now assumed a more sober
character; the science of geology has been reared upon numerous and accurate observations of facts;
and standing thus upon the basis of induction, it is entitled to a rank among those sciences which
Lord Bacon’s Philosophy has contributed to create. Geological researches are now prosecuted by
actually exploring the structure and arrangement of districts, countries, and continents. The obliquity
of the strata of most rocks, causing their edges to project in many places above the surface; their
exposure, in other instances on the sides or tops of hills and mountains; or, in consequence of the
intersection of their strata, by roads, canals, and river-courses, or by the wearing of the ocean; or their
direct perforation, by the shafts of mines; all these causes, and others, afford extensive means of
reading the interior structure of the globe.
The outlines of American geology appear to be particularly grand, simple, and instructive; and a
knowledge of the important facts, and general principles of this science, is of vast practical use, as
regards the interests of agriculture, and the research for useful minerals. Geological and
mineralogical descriptions, and maps of particular states and districts, are very much needed in the
United States; and to excite a spirit to furnish them will form one leading object of this Journal.”
Philosophers such as Descartes and Liebnitz, the cosmogonists de Maillet
and Buffon had been less instrumental in developing science than in fitting
a few facts and many speculations to their systems of philosophy. By the
opening of the nineteenth century, however, men of learning were coming
to appreciate that the way to advance science was to experiment and
observe, to collect facts and discourage unfounded speculation. Silliman’s
insight into the needs of geologic science is shown in the following
quotation (1, pp. 6, 7, 1818):
“Our geology, also, presents a most interesting field of inquiry. A grand outline has recently been
drawn by Mr. Maclure, with a masterly hand, and with a vast extent of personal observation and
labour: but to fill up the detail, both observation and labour still more extensive are demanded; nor
can the object be effected, till more good geologists are formed, and distributed over our extensive
territory.
To account for the formation and changes of our globe, by excursions of the imagination, often
splendid and imposing, but usually visionary, and almost always baseless, was, till within half a
century, the business of geological speculations; but this research has now assumed a more sober
character; the science of geology has been reared upon numerous and accurate observations of facts;
and standing thus upon the basis of induction, it is entitled to a rank among those sciences which
Lord Bacon’s Philosophy has contributed to create. Geological researches are now prosecuted by
actually exploring the structure and arrangement of districts, countries, and continents. The obliquity
of the strata of most rocks, causing their edges to project in many places above the surface; their
exposure, in other instances on the sides or tops of hills and mountains; or, in consequence of the
intersection of their strata, by roads, canals, and river-courses, or by the wearing of the ocean; or their
direct perforation, by the shafts of mines; all these causes, and others, afford extensive means of
reading the interior structure of the globe.
The outlines of American geology appear to be particularly grand, simple, and instructive; and a
knowledge of the important facts, and general principles of this science, is of vast practical use, as
regards the interests of agriculture, and the research for useful minerals. Geological and
mineralogical descriptions, and maps of particular states and districts, are very much needed in the
United States; and to excite a spirit to furnish them will form one leading object of this Journal.”
Page 168
The Prolonged Influence of Outgrown Ideas.
Those interested in any branch of science should, as a matter of
education, read the history of that special subject. A knowledge of the
stages by which the present development has been attained is essential to
give a proper perspective to the literature of each period. Much of the
existing terminology is an inheritance from the first attempts at
nomenclature, or may rest upon theories long discarded. Popular notions at
variance with advanced teaching are often the forgotten inheritance of a
past generation.
Gneiss, trap, and Old Red Sandstone are names which we owe to Werner.
The “Tertiary period” and “drift” are relics of an early terminology. The
geology of tourist circulars still speaks of canyons as made by “convulsions
of nature.” Popular writers still attribute to geologists a belief in a molten
earth covered by a thin crust. Within the present century the eighteenth
century speculations of Werner and his predecessors, postulating a supposed
capacity of water to seep through the crust into the interior of the earth,
resulting in a hypothetical progressive desiccation of the surface, views
long abandoned by most modern geologists, have been revived by an
astronomer into a theory of “planetology.”
A review of the literature of a century brings to light certain tendencies in
the growth of science. Each decade has witnessed a larger accumulation of
observed facts and a fuller classification of these fundamental data, but the
pendulum of interpretative theory swings away from the path of progress,
now to one side, now to the other, testing out the proper direction. For
decades the understanding of certain classes of facts may be actually
retrogressive. A retrospect shows that certain minds, keen and unfettered by
a prevailing theory, have in some directions been in advance of their
generation. But the judgment of the times had not sufficient basis in
knowledge for the separation and acceptance of their truer views from the
contemporaneous tangle of false interpretations.
An interesting illustration of these statements regarding the slow settling
of opinion may be cited in regard to the significance of the dip of the
Triassic formations of the eastern United States. The strata of the
Those interested in any branch of science should, as a matter of
education, read the history of that special subject. A knowledge of the
stages by which the present development has been attained is essential to
give a proper perspective to the literature of each period. Much of the
existing terminology is an inheritance from the first attempts at
nomenclature, or may rest upon theories long discarded. Popular notions at
variance with advanced teaching are often the forgotten inheritance of a
past generation.
Gneiss, trap, and Old Red Sandstone are names which we owe to Werner.
The “Tertiary period” and “drift” are relics of an early terminology. The
geology of tourist circulars still speaks of canyons as made by “convulsions
of nature.” Popular writers still attribute to geologists a belief in a molten
earth covered by a thin crust. Within the present century the eighteenth
century speculations of Werner and his predecessors, postulating a supposed
capacity of water to seep through the crust into the interior of the earth,
resulting in a hypothetical progressive desiccation of the surface, views
long abandoned by most modern geologists, have been revived by an
astronomer into a theory of “planetology.”
A review of the literature of a century brings to light certain tendencies in
the growth of science. Each decade has witnessed a larger accumulation of
observed facts and a fuller classification of these fundamental data, but the
pendulum of interpretative theory swings away from the path of progress,
now to one side, now to the other, testing out the proper direction. For
decades the understanding of certain classes of facts may be actually
retrogressive. A retrospect shows that certain minds, keen and unfettered by
a prevailing theory, have in some directions been in advance of their
generation. But the judgment of the times had not sufficient basis in
knowledge for the separation and acceptance of their truer views from the
contemporaneous tangle of false interpretations.
An interesting illustration of these statements regarding the slow settling
of opinion may be cited in regard to the significance of the dip of the
Triassic formations of the eastern United States. The strata of the
Page 169
Massachusetts-Connecticut basin possess a monoclinal easterly dip which
averages about 20 degrees to the east. Those of the New Jersey-
Pennsylvania-Virginia basin possess a similar dip to the northwest. Both
basins are cut by great faults and the dip is now accepted by practically all
geologists as due to rotation of the crust blocks away from a geanticlinal
axis between the two basins. Edward Hitchcock, whose work from the first
shows an interpretative quality in advance of his time, states in 1823 (6,74)
regarding the dip of the Connecticut valley rocks:
“There is reason to believe that Mount Toby, the strata of which are almost horizontal, exhibits the
original dip of these rocks, and that those cases in which they are more highly inclined are the result
of some Plutonian convulsion. Such irregularity in the dip of coal fields is no uncommon
occurrence.”
In Hitchcock’s Geology of Massachusetts, published in 1833, ten years
later, geological structure sections of the Connecticut Valley rocks are
given, the facts are discussed in detail and the dip ascribed to the elevatory
forces. He says (l. c., pp. 213, 223):
“If it were possible to doubt that the new red sandstone formation was deposited from water, the
surface of some of the layers of this shale would settle the question demonstrably. For it exhibits
precisely those gentle undulations, which the loamy bottom of every river with a moderate current,
presents. (No. 198.) But such a surface could never have been formed while the layers had that high
inclination to the horizon, which many of them now present: so that we have here, also, decisive
evidence that they have been elevated subsequently to their deposition....
The objection of a writer in the American Journal of Science, that such a height of waters as would
deposit Mount Toby, must have produced a lake nearly to the upper part of New Hampshire, in the
Connecticut Valley, and thus have caused the same sandstone to be produced higher up that valley
than Northfield, loses its force, when it is recollected that this formation was deposited before its
strata were elevated. For the elevating force undoubtedly changed the relative level of different parts
of the country. In this case, the disturbing force must have acted beneath the primary rocks. And
besides, we have good evidence which will be shown by and by, that our new red sandstone was
formed beneath the ocean. We cannot then reason on this subject from present levels.”
averages about 20 degrees to the east. Those of the New Jersey-
Pennsylvania-Virginia basin possess a similar dip to the northwest. Both
basins are cut by great faults and the dip is now accepted by practically all
geologists as due to rotation of the crust blocks away from a geanticlinal
axis between the two basins. Edward Hitchcock, whose work from the first
shows an interpretative quality in advance of his time, states in 1823 (6,74)
regarding the dip of the Connecticut valley rocks:
“There is reason to believe that Mount Toby, the strata of which are almost horizontal, exhibits the
original dip of these rocks, and that those cases in which they are more highly inclined are the result
of some Plutonian convulsion. Such irregularity in the dip of coal fields is no uncommon
occurrence.”
In Hitchcock’s Geology of Massachusetts, published in 1833, ten years
later, geological structure sections of the Connecticut Valley rocks are
given, the facts are discussed in detail and the dip ascribed to the elevatory
forces. He says (l. c., pp. 213, 223):
“If it were possible to doubt that the new red sandstone formation was deposited from water, the
surface of some of the layers of this shale would settle the question demonstrably. For it exhibits
precisely those gentle undulations, which the loamy bottom of every river with a moderate current,
presents. (No. 198.) But such a surface could never have been formed while the layers had that high
inclination to the horizon, which many of them now present: so that we have here, also, decisive
evidence that they have been elevated subsequently to their deposition....
The objection of a writer in the American Journal of Science, that such a height of waters as would
deposit Mount Toby, must have produced a lake nearly to the upper part of New Hampshire, in the
Connecticut Valley, and thus have caused the same sandstone to be produced higher up that valley
than Northfield, loses its force, when it is recollected that this formation was deposited before its
strata were elevated. For the elevating force undoubtedly changed the relative level of different parts
of the country. In this case, the disturbing force must have acted beneath the primary rocks. And
besides, we have good evidence which will be shown by and by, that our new red sandstone was
formed beneath the ocean. We cannot then reason on this subject from present levels.”
Page 170
Courtesy of Popular Science Monthly.
In 1840, H. D. Rogers, a geologist who has acquired a more widely
known name than Hitchcock, but who in reality showed an inferior ability
in interpretation, made the following statements in explanation of the
regional monoclinal dip of the New Jersey Triassic rocks averaging 15 to 20
degrees to the northwest:[78]
“Their materials give evidence of having been swept into this estuary, or great ancient river, from
the south and southeast, by a current producing an almost universal dip of the beds towards the
northwest, a feature clearly not caused by any uplifting agency, but assumed originally at the time of
In 1840, H. D. Rogers, a geologist who has acquired a more widely
known name than Hitchcock, but who in reality showed an inferior ability
in interpretation, made the following statements in explanation of the
regional monoclinal dip of the New Jersey Triassic rocks averaging 15 to 20
degrees to the northwest:[78]
“Their materials give evidence of having been swept into this estuary, or great ancient river, from
the south and southeast, by a current producing an almost universal dip of the beds towards the
northwest, a feature clearly not caused by any uplifting agency, but assumed originally at the time of
Page 171
their deposition, in consequence of the setting of the current from the opposite or southeastern
shore.”
In 1842, at the third annual meeting of the Association of American
Geologists both H. D. and W. B. Rogers argued (43, 170, 1842) against Sir
Charles Lyell and E. Hitchcock that the present dip of the Triassic was the
original slope of deposition, stating among other reasons that the footprints
impressed upon the sediments often showed a slipping and a pushing of the
soft clay in the direction of the downhill slope. In 1858 H. D. Rogers still
held to the same views of original dip,[79] notwithstanding that a moderate
amount of observation on the mud-cracked and rain-pitted layers would
have supplied the proof that such must have dried as horizontal surfaces.
The idea of inclined deposition is not yet wholly dead as it has been
suggested more than once within the present generation as a means of
escaping from the necessity of accepting the very great thicknesses of this
and similar formations. Thus, as Brögger has remarked in another
connection,—the ghosts of the old time stand ever ready to reappear.
In the present essay on the rise of structural geology as reflected through
a century of publication in the Journal, attention will be given especially to
two fields, that of structures connected with igneous rocks and that of
structures connected with mountain making, and emphasis will be placed
upon the growth of understanding rather than upon the accumulating
knowledge of details. The growth in both of these divisions of structural
geology is well illustrated in the volumes of the Journal.
shore.”
In 1842, at the third annual meeting of the Association of American
Geologists both H. D. and W. B. Rogers argued (43, 170, 1842) against Sir
Charles Lyell and E. Hitchcock that the present dip of the Triassic was the
original slope of deposition, stating among other reasons that the footprints
impressed upon the sediments often showed a slipping and a pushing of the
soft clay in the direction of the downhill slope. In 1858 H. D. Rogers still
held to the same views of original dip,[79] notwithstanding that a moderate
amount of observation on the mud-cracked and rain-pitted layers would
have supplied the proof that such must have dried as horizontal surfaces.
The idea of inclined deposition is not yet wholly dead as it has been
suggested more than once within the present generation as a means of
escaping from the necessity of accepting the very great thicknesses of this
and similar formations. Thus, as Brögger has remarked in another
connection,—the ghosts of the old time stand ever ready to reappear.
In the present essay on the rise of structural geology as reflected through
a century of publication in the Journal, attention will be given especially to
two fields, that of structures connected with igneous rocks and that of
structures connected with mountain making, and emphasis will be placed
upon the growth of understanding rather than upon the accumulating
knowledge of details. The growth in both of these divisions of structural
geology is well illustrated in the volumes of the Journal.
Page 172
Structures and Relationships of Igneous Rocks.
Page 173
Opposed Interpretations of Plutonists and Neptunists.
During the first quarter of the nineteenth century the geologic
controversy between the Plutonists and Neptunists was at its height; the
Plutonists, following the Scotchman, Hutton, holding to the igneous origin
of basalt and granite, the Neptunists, after their German master, Werner of
Freiberg, maintaining that these rocks had been precipitated from a
primitive universal ocean. The Plutonists, although time has shown them to
have been correct in all essential particulars, were for a generation
submerged under the propaganda carried forward by the disciples of
Werner. The “Illustrations of the Huttonian Theory of the Earth,” a
remarkable classic, worthy of being studied to-day as well as a century ago,
was published in 1802 by John Playfair, professor of mathematics in the
University of Edinburgh and a friend of Hutton, who had died five years
previously. This volume was opposed by Robert Jameson, professor of
natural philosophy in the same university, who had absorbed the ideas of
the German school while at Freiberg and published in 1808 a volume on the
“Elements of Geognosy,” in which the philosophy of Werner is followed
throughout and even obsidian and pumice are argued to be aqueous
precipitates. The authority of the Wernerian autocracy caused its
nomenclature to be adopted in the new world, but strong evidence against
its interpretations was to be found in the actual structural relations displayed
by the igneous rocks.
During the first quarter of the nineteenth century the geologic
controversy between the Plutonists and Neptunists was at its height; the
Plutonists, following the Scotchman, Hutton, holding to the igneous origin
of basalt and granite, the Neptunists, after their German master, Werner of
Freiberg, maintaining that these rocks had been precipitated from a
primitive universal ocean. The Plutonists, although time has shown them to
have been correct in all essential particulars, were for a generation
submerged under the propaganda carried forward by the disciples of
Werner. The “Illustrations of the Huttonian Theory of the Earth,” a
remarkable classic, worthy of being studied to-day as well as a century ago,
was published in 1802 by John Playfair, professor of mathematics in the
University of Edinburgh and a friend of Hutton, who had died five years
previously. This volume was opposed by Robert Jameson, professor of
natural philosophy in the same university, who had absorbed the ideas of
the German school while at Freiberg and published in 1808 a volume on the
“Elements of Geognosy,” in which the philosophy of Werner is followed
throughout and even obsidian and pumice are argued to be aqueous
precipitates. The authority of the Wernerian autocracy caused its
nomenclature to be adopted in the new world, but strong evidence against
its interpretations was to be found in the actual structural relations displayed
by the igneous rocks.
Page 174
Contributions on Volcanic and Intrusive Rocks.
The accumulation and study of facts constituted the best cure for an
erroneous theory. The publications of the Journal contributed toward this
end by articles along several lines. The most original contributions were
those which dealt with the areal and structural geology of eastern North
America, but equally valuable at that time for the broadening of scientific
interest were the studies on the volcanic activities of the Hawaiian Islands,
published through many years. Perhaps most valuable from the educative
standpoint were the extensive republications in the Journal of the more
important European researches, making them accessible to American
readers. In volume 13 (1828), for example, a digest of Scrope’s work on
volcanoes is given, covering forty pages; and of Daubeny on active and
extinct volcanoes, running over seventy-five pages and extending into vol.
14. Through these comprehensive studies the nature of volcanic action
became generally understood during the first half of the nineteenth century
and the original publications in the Journal were valuable in giving a
knowledge of the activities of the Hawaiian volcanoes.
Early in the nineteenth century the whole of America still remained to be
explored by the geologist. The regions adjacent to the centers of learning
were among the first to receive attention and the Triassic basin of
Connecticut and Massachusetts yielded information in regard to the nature
of igneous intrusion. This basin, of unmetamorphic shales and sandstones,
is occupied by the Connecticut River except at its southern end. The
Formation contains within it sills, dikes, and outflows of basaltic rocks
which because of their superior resistance to erosion constitute prominent
hills, in places bounded by cliffs.
Silliman in 1806[80] described East Rock, New Haven, Connecticut, as a
whinstone, trap, or basalt, and accounted for its presence on the supposition
that it had
“actually been melted in the bowels of the earth and ejected among the superior strata by the force
of subterraneous fire, but never erupted like lava, cooling under the pressure of the superincumbent
strata and therefore compact or nonvesicular, its present form being due to erosion.”
The accumulation and study of facts constituted the best cure for an
erroneous theory. The publications of the Journal contributed toward this
end by articles along several lines. The most original contributions were
those which dealt with the areal and structural geology of eastern North
America, but equally valuable at that time for the broadening of scientific
interest were the studies on the volcanic activities of the Hawaiian Islands,
published through many years. Perhaps most valuable from the educative
standpoint were the extensive republications in the Journal of the more
important European researches, making them accessible to American
readers. In volume 13 (1828), for example, a digest of Scrope’s work on
volcanoes is given, covering forty pages; and of Daubeny on active and
extinct volcanoes, running over seventy-five pages and extending into vol.
14. Through these comprehensive studies the nature of volcanic action
became generally understood during the first half of the nineteenth century
and the original publications in the Journal were valuable in giving a
knowledge of the activities of the Hawaiian volcanoes.
Early in the nineteenth century the whole of America still remained to be
explored by the geologist. The regions adjacent to the centers of learning
were among the first to receive attention and the Triassic basin of
Connecticut and Massachusetts yielded information in regard to the nature
of igneous intrusion. This basin, of unmetamorphic shales and sandstones,
is occupied by the Connecticut River except at its southern end. The
Formation contains within it sills, dikes, and outflows of basaltic rocks
which because of their superior resistance to erosion constitute prominent
hills, in places bounded by cliffs.
Silliman in 1806[80] described East Rock, New Haven, Connecticut, as a
whinstone, trap, or basalt, and accounted for its presence on the supposition
that it had
“actually been melted in the bowels of the earth and ejected among the superior strata by the force
of subterraneous fire, but never erupted like lava, cooling under the pressure of the superincumbent
strata and therefore compact or nonvesicular, its present form being due to erosion.”
Page 175
In these conclusions Silliman was correct. With but a limited amount of
experience he was able to discriminate between the intrusive and effusive
rocks and saw that the prominence of this hill was due to the erosion of the
sediments which once surrounded it.
An extensive paper on the geology of this region was published by
Edward Hitchcock in 1823,[81] then just thirty years of age. This paper
shows the evidence of extensive field observations, and his comments in
regard to the trap and granite are of interest. Hitchcock gives five pages to
the subject of “Greenstone Dykes in Old Red Sandstone” (6, 56–60, 1823)
and makes the following statements:
“Professor Silliman conducted me to an interesting locality of these in East-Haven. They occur on
the main road from New-Haven to East-Haven, less than half a mile from Tomlinson’s bridge ... (p.
56).
They are an interesting feature in our geology, and deserve more attention; and it is peculiarly
fortunate that they should be situated so near a geological school and the first mineral cabinet in our
country ... (p. 58).
experience he was able to discriminate between the intrusive and effusive
rocks and saw that the prominence of this hill was due to the erosion of the
sediments which once surrounded it.
An extensive paper on the geology of this region was published by
Edward Hitchcock in 1823,[81] then just thirty years of age. This paper
shows the evidence of extensive field observations, and his comments in
regard to the trap and granite are of interest. Hitchcock gives five pages to
the subject of “Greenstone Dykes in Old Red Sandstone” (6, 56–60, 1823)
and makes the following statements:
“Professor Silliman conducted me to an interesting locality of these in East-Haven. They occur on
the main road from New-Haven to East-Haven, less than half a mile from Tomlinson’s bridge ... (p.
56).
They are an interesting feature in our geology, and deserve more attention; and it is peculiarly
fortunate that they should be situated so near a geological school and the first mineral cabinet in our
country ... (p. 58).
Page 176
Origin of Greenstone.
Does the greenstone of the Connecticut afford evidence in favour of the Wernerian or of the
Huttonian theory of its origin? Averse as I feel to taking a side in this controversy, I cannot but say,
that the man who maintains, in its length and breadth, the original hypothesis of Werner in regard to
the aqueous deposition of trap, will find it for his interest, if he wishes to keep clear of doubts, not to
follow the example of D’Aubuisson, by going forth to examine the greenstone of this region, lest,
like that geologist, he should be compelled, not only to abandon his theory, but to write a book
against it. Indeed, when surveying particular portions of this rock, I have sometimes thought
Bakewell did not much exaggerate when he said in regard to Werner’s hypothesis, that, ‘it is hardly
possible for the human mind to invent a system more repugnant to existing facts.’
On the other hand, the Huttonian would doubtless have his heart gladdened, and his faith
strengthened by a survey of the greater part of this rock. As he looked at the dikes of the old red
sandstone, he would almost see the melted rock forcing its way through the fissures; and when he
came to the amygdaloidal, especially to that variety which resembles lava, he might even be tempted
to apply his thermometer to it, in the suspicion that it was not yet quite cool ... (p. 59).
By treating the subject in this manner I mean no disrespect to any of the distinguished men who
have adopted either side of this question. To President Cooper especially, who regards the greenstone
of the Connecticut as volcanic, I feel much indebted for the great mass of facts he has collected on
the subject. And were I to adopt any hypothesis in regard to the origin of our greenstone, it would be
one not much different from his” (p. 60).
By 1833 and more clearly in 1841 Hitchcock had come to recognize the
distinction between intrusive and extrusive basaltic sheets in the
Connecticut valley. Dawson also came to regard the Acadian sheets as
extrusive, and Emerson in 1882 recalled again the evidence for
Massachusetts (24, 195, 1882). Davis, however, went a step further and by
applying distinctive criteria not only separated intrusive and extrusive
sheets throughout the whole Triassic area, but by using basalt flows as
stratigraphic horizons unraveled for the first time the system of faults which
cut the Triassic system. His preliminary paper (24, 345, 1882) was followed
by many others.
From 1880 onward begins the period of precise structural field work. The
older geologists mostly conceived their work after reconnaissance methods.
From 1870 to 1880 a group of younger men entered geology who paid close
attention to the solid geometry and mechanics of earth structures. In their
hands physical and dynamical geology began to assume the standing of a
precise and quantitative science. In the field of intrusive rocks the opening
classic was by Gilbert, who in his volume on the geology of the Henry
Does the greenstone of the Connecticut afford evidence in favour of the Wernerian or of the
Huttonian theory of its origin? Averse as I feel to taking a side in this controversy, I cannot but say,
that the man who maintains, in its length and breadth, the original hypothesis of Werner in regard to
the aqueous deposition of trap, will find it for his interest, if he wishes to keep clear of doubts, not to
follow the example of D’Aubuisson, by going forth to examine the greenstone of this region, lest,
like that geologist, he should be compelled, not only to abandon his theory, but to write a book
against it. Indeed, when surveying particular portions of this rock, I have sometimes thought
Bakewell did not much exaggerate when he said in regard to Werner’s hypothesis, that, ‘it is hardly
possible for the human mind to invent a system more repugnant to existing facts.’
On the other hand, the Huttonian would doubtless have his heart gladdened, and his faith
strengthened by a survey of the greater part of this rock. As he looked at the dikes of the old red
sandstone, he would almost see the melted rock forcing its way through the fissures; and when he
came to the amygdaloidal, especially to that variety which resembles lava, he might even be tempted
to apply his thermometer to it, in the suspicion that it was not yet quite cool ... (p. 59).
By treating the subject in this manner I mean no disrespect to any of the distinguished men who
have adopted either side of this question. To President Cooper especially, who regards the greenstone
of the Connecticut as volcanic, I feel much indebted for the great mass of facts he has collected on
the subject. And were I to adopt any hypothesis in regard to the origin of our greenstone, it would be
one not much different from his” (p. 60).
By 1833 and more clearly in 1841 Hitchcock had come to recognize the
distinction between intrusive and extrusive basaltic sheets in the
Connecticut valley. Dawson also came to regard the Acadian sheets as
extrusive, and Emerson in 1882 recalled again the evidence for
Massachusetts (24, 195, 1882). Davis, however, went a step further and by
applying distinctive criteria not only separated intrusive and extrusive
sheets throughout the whole Triassic area, but by using basalt flows as
stratigraphic horizons unraveled for the first time the system of faults which
cut the Triassic system. His preliminary paper (24, 345, 1882) was followed
by many others.
From 1880 onward begins the period of precise structural field work. The
older geologists mostly conceived their work after reconnaissance methods.
From 1870 to 1880 a group of younger men entered geology who paid close
attention to the solid geometry and mechanics of earth structures. In their
hands physical and dynamical geology began to assume the standing of a
precise and quantitative science. In the field of intrusive rocks the opening
classic was by Gilbert, who in his volume on the geology of the Henry
Page 177
Mountains, published in 1880, made laccoliths known to the world. With
the beginning of this new period we may well leave the subject of intrusive
rocks and turn to the progress of knowledge in regard to those deeper and
vaster bodies now known as batholiths. These, since erosion does not
expose their bottoms, Daly separates from intrusives and classifies as
subjacent. The batholiths consist typically of granite and granodiorite, and
introduce us to the problem of granite.
the beginning of this new period we may well leave the subject of intrusive
rocks and turn to the progress of knowledge in regard to those deeper and
vaster bodies now known as batholiths. These, since erosion does not
expose their bottoms, Daly separates from intrusives and classifies as
subjacent. The batholiths consist typically of granite and granodiorite, and
introduce us to the problem of granite.
Page 178
Views on the Structural Relations of Granite.
Conscientious field observations were sufficient to establish the true
nature of the intrusive and extrusive rocks. The case was very different,
however, with the nature and relations of the great bodies of granite, which
may be taken in the structural sense as including all the visibly crystalline
acidic and intermediate rocks, known more specifically as granite, syenite,
and diorite.
The large bodies of granite, structurally classified as stocks, or batholiths,
commonly show wedges, tongues, or dike networks cutting into the
surrounding rocks. The relations, however, are not all so simple as this.
Granites may cover vast areas, they are usually the older rocks, they are
generally associated with regional metamorphism of the intruded
formations, which metamorphism is now understood to be due chiefly to
the heat and mineralizers given off from the granite magma, associated with
mashing and shearing of the surrounding rocks. The granite was often
injected in successive stages which alternated with the stages of regional
mashing. A parallel or gneissic structure is thus developed which is in part
due to mashing, in part to igneous injection. Where the ascent of heat into
the cover is excessive, or where blocks are detached and involved in the
magma, the latter may dissolve some of the older cover rocks, even where
these were of sedimentary origin.
Thus between mashing, injection, and assimilation the genetic
relationships of a batholith to its surroundings are in many instances
obscure. Nevertheless, attention to the larger relations shows that the molten
magma originated at great depths in the earth’s crust, far below the bottoms
of geosynclines, and consists of primary igneous material, not of fused
sediments. From those depths it has ascended by various processes into the
outer crust, where it crystallized into granite masses, to be later exposed by
erosion. The amount of material which can be dissolved and assimilated
must be small in comparison with the whole body of the magma. The
original composition of the magma was probably basic, nearer that of a
basalt than that of a granite. Differentiation of the molten mass is thought to
cause the upper and lower parts of the chamber to become unlike, the
lighter and more acidic portion giving rise to the great bodies of granite.
Conscientious field observations were sufficient to establish the true
nature of the intrusive and extrusive rocks. The case was very different,
however, with the nature and relations of the great bodies of granite, which
may be taken in the structural sense as including all the visibly crystalline
acidic and intermediate rocks, known more specifically as granite, syenite,
and diorite.
The large bodies of granite, structurally classified as stocks, or batholiths,
commonly show wedges, tongues, or dike networks cutting into the
surrounding rocks. The relations, however, are not all so simple as this.
Granites may cover vast areas, they are usually the older rocks, they are
generally associated with regional metamorphism of the intruded
formations, which metamorphism is now understood to be due chiefly to
the heat and mineralizers given off from the granite magma, associated with
mashing and shearing of the surrounding rocks. The granite was often
injected in successive stages which alternated with the stages of regional
mashing. A parallel or gneissic structure is thus developed which is in part
due to mashing, in part to igneous injection. Where the ascent of heat into
the cover is excessive, or where blocks are detached and involved in the
magma, the latter may dissolve some of the older cover rocks, even where
these were of sedimentary origin.
Thus between mashing, injection, and assimilation the genetic
relationships of a batholith to its surroundings are in many instances
obscure. Nevertheless, attention to the larger relations shows that the molten
magma originated at great depths in the earth’s crust, far below the bottoms
of geosynclines, and consists of primary igneous material, not of fused
sediments. From those depths it has ascended by various processes into the
outer crust, where it crystallized into granite masses, to be later exposed by
erosion. The amount of material which can be dissolved and assimilated
must be small in comparison with the whole body of the magma. The
original composition of the magma was probably basic, nearer that of a
basalt than that of a granite. Differentiation of the molten mass is thought to
cause the upper and lower parts of the chamber to become unlike, the
lighter and more acidic portion giving rise to the great bodies of granite.
Page 179
With the exception of certain border zones the whole, however, is regarded
as igneous rock risen from the depths.
The complex border relations, but more particularly certain academic
hypotheses, led to a period of misunderstanding and retrogression in regard
to the nature of granites. It constitutes an interesting illustration of the
possibility of a wrong theory leading interpretation astray, chiefly through
the magnification of minor into major factors. This history illustrates the
dangers of qualitative science as compared to quantitative, of a single
hypothesis as matched against the method of multiple working hypothesis.
This flux of opinion in regard to the nature of granites may be traced
through the volumes of the Journal.
E. Hitchcock in 1824 (6, 12) noted that in places granite appeared
bedded, but in other places existed in veins which cut obliquely across the
strata. Silliman, although careful not to deny the aqueous origin of some
basalts, yet held that the field evidence of New England indicates for that
region the igneous or Huttonian origin of trap and granite (7, 238, 1824).
In 1832 the following article by Hitchcock appeared in the Journal (22, 1,
70):
Report on the Geology of Massachusetts; examined under the direction of the Government of that
State, during the years 1830 and 1831; by Edward Hitchcock, Prof. of Chemistry and Natural History
in Amherst College.
A footnote adds that this is “published in this Journal by consent of the Government of
Massachusetts, and intended to appear also in a separate form, and to be distributed among the
members of the Legislature of the same State, about the time of its appearance in this work. It is, we
believe, the first example in this country, of the geological survey of an entire State.”
This article includes a geological map of the state and covers the subject
of economic geology. The report brought forth the following remarks from
a French reviewer in the Revue Encyclopédique, Aug. 1832, quoted in the
Journal (23, 389, 1833):
“A single glance at this report, is sufficient to convince any one of the utility of such a work, to the
state which has undertaken it; and to regret that there is so very small a part of the French territory,
whose geological constitution is as well known to the public, as is now the state of Massachusetts.
France has the greater cause to regret her being distanced in this race by America, from her having a
corps of mining engineers, who if they had the means, would, in a very short time furnish a work of
the same kind, still more complete, of each of the departments.”
as igneous rock risen from the depths.
The complex border relations, but more particularly certain academic
hypotheses, led to a period of misunderstanding and retrogression in regard
to the nature of granites. It constitutes an interesting illustration of the
possibility of a wrong theory leading interpretation astray, chiefly through
the magnification of minor into major factors. This history illustrates the
dangers of qualitative science as compared to quantitative, of a single
hypothesis as matched against the method of multiple working hypothesis.
This flux of opinion in regard to the nature of granites may be traced
through the volumes of the Journal.
E. Hitchcock in 1824 (6, 12) noted that in places granite appeared
bedded, but in other places existed in veins which cut obliquely across the
strata. Silliman, although careful not to deny the aqueous origin of some
basalts, yet held that the field evidence of New England indicates for that
region the igneous or Huttonian origin of trap and granite (7, 238, 1824).
In 1832 the following article by Hitchcock appeared in the Journal (22, 1,
70):
Report on the Geology of Massachusetts; examined under the direction of the Government of that
State, during the years 1830 and 1831; by Edward Hitchcock, Prof. of Chemistry and Natural History
in Amherst College.
A footnote adds that this is “published in this Journal by consent of the Government of
Massachusetts, and intended to appear also in a separate form, and to be distributed among the
members of the Legislature of the same State, about the time of its appearance in this work. It is, we
believe, the first example in this country, of the geological survey of an entire State.”
This article includes a geological map of the state and covers the subject
of economic geology. The report brought forth the following remarks from
a French reviewer in the Revue Encyclopédique, Aug. 1832, quoted in the
Journal (23, 389, 1833):
“A single glance at this report, is sufficient to convince any one of the utility of such a work, to the
state which has undertaken it; and to regret that there is so very small a part of the French territory,
whose geological constitution is as well known to the public, as is now the state of Massachusetts.
France has the greater cause to regret her being distanced in this race by America, from her having a
corps of mining engineers, who if they had the means, would, in a very short time furnish a work of
the same kind, still more complete, of each of the departments.”
Page 180
The complete report published in 1833 is a work of 700 pages. Pages 465
to 517 are devoted to the subject of granite. Numerous detailed sketches are
given showing contact relations. Nine pages are given to theoretical
considerations and many lines of proof are given that granite is an igneous
rock, molten from the internal heat of the earth, and intruded into the
sedimentary strata. His statement is the clearest published in the world, so
far as the writer is aware, up to that date, and marks Edward Hitchcock as
one of the leading geologists of his generation in Europe as well as
America. Unfortunately his views were largely lost to sight during the
following generation.
In 1840 the first American edition of Mantell’s Wonders of Geology gave
currency to the idea that granite is proved to be of all geological ages up to
the Tertiary (39, 6, 1840). In 1843 J. D. Dana pointed out (45, 104) that
schistosity was no evidence of sedimentary origin. He regarded most
granites as igneous as shown by their structural relations, but considers that
some may have had a sedimentary origin.
to 517 are devoted to the subject of granite. Numerous detailed sketches are
given showing contact relations. Nine pages are given to theoretical
considerations and many lines of proof are given that granite is an igneous
rock, molten from the internal heat of the earth, and intruded into the
sedimentary strata. His statement is the clearest published in the world, so
far as the writer is aware, up to that date, and marks Edward Hitchcock as
one of the leading geologists of his generation in Europe as well as
America. Unfortunately his views were largely lost to sight during the
following generation.
In 1840 the first American edition of Mantell’s Wonders of Geology gave
currency to the idea that granite is proved to be of all geological ages up to
the Tertiary (39, 6, 1840). In 1843 J. D. Dana pointed out (45, 104) that
schistosity was no evidence of sedimentary origin. He regarded most
granites as igneous as shown by their structural relations, but considers that
some may have had a sedimentary origin.
Page 181
Rise and Decline of the Metamorphic Theory of Granite.
Up to 1860 granite was regarded on the basis of the facts of the field as
essentially an intrusive rock, but gneiss as a metamorphic product mostly of
sedimentary origin. It seemed as though sound methods of research and
interpretation were securely established. Nevertheless, a new era of
speculation and a modified Wernerism arose at that time with a paper by T.
Sterry Hunt, marking a retrogression in the theory of granite which lasted
until his death in 1892.
In November, 1859, Hunt read before the Geological Society of London a
paper on “Some Points in Chemical Geology” in which he announced that
igneous rocks are in all cases simply fused and displaced sediments, the
fusion taking place by the rise of the earth’s internal heat into deeply buried
and water-soaked masses of sediments (see 30, 133, 1860). The germ of this
idea of aqueo-igneous fusion was far older, due to Babbage and John
Herschel, neither of them geologists, but such sweeping extensions of it had
never before been published. Hunt had the advantage of a wide
acquaintanceship with geological literature and chemistry. He wrote
plausibly on chemical and theoretical geology, but his views were not
controlled by careful field observations. In fact he wrote confidently on
regions which apparently he had never seen and where a limited amount of
field work would have shown him to have been fundamentally in error. A
man of egotistical temperament, he sought to establish priority for himself
in many subjects and in order to cover the field made many poorly founded
assertions. Building on to another Wernerian idea, he held that many
metamorphic minerals had a chronologic value comparable to fossils—
staurolite for example indicating a pre-Silurian age—and on this basis
divided the crystalline rocks into five series. Although there is much of
value buried in Hunt’s work it is difficult to disentangle it, with the result
that his writings were a disservice to the science of geology. Although
carrying much weight in his lifetime, they have passed with his death nearly
into oblivion.
Marcou, with a limited knowledge of American geology, and but little
respect for the opinions of others, had published a geologic map of the
United States containing gross errors. In support of his views he read in
Up to 1860 granite was regarded on the basis of the facts of the field as
essentially an intrusive rock, but gneiss as a metamorphic product mostly of
sedimentary origin. It seemed as though sound methods of research and
interpretation were securely established. Nevertheless, a new era of
speculation and a modified Wernerism arose at that time with a paper by T.
Sterry Hunt, marking a retrogression in the theory of granite which lasted
until his death in 1892.
In November, 1859, Hunt read before the Geological Society of London a
paper on “Some Points in Chemical Geology” in which he announced that
igneous rocks are in all cases simply fused and displaced sediments, the
fusion taking place by the rise of the earth’s internal heat into deeply buried
and water-soaked masses of sediments (see 30, 133, 1860). The germ of this
idea of aqueo-igneous fusion was far older, due to Babbage and John
Herschel, neither of them geologists, but such sweeping extensions of it had
never before been published. Hunt had the advantage of a wide
acquaintanceship with geological literature and chemistry. He wrote
plausibly on chemical and theoretical geology, but his views were not
controlled by careful field observations. In fact he wrote confidently on
regions which apparently he had never seen and where a limited amount of
field work would have shown him to have been fundamentally in error. A
man of egotistical temperament, he sought to establish priority for himself
in many subjects and in order to cover the field made many poorly founded
assertions. Building on to another Wernerian idea, he held that many
metamorphic minerals had a chronologic value comparable to fossils—
staurolite for example indicating a pre-Silurian age—and on this basis
divided the crystalline rocks into five series. Although there is much of
value buried in Hunt’s work it is difficult to disentangle it, with the result
that his writings were a disservice to the science of geology. Although
carrying much weight in his lifetime, they have passed with his death nearly
into oblivion.
Marcou, with a limited knowledge of American geology, and but little
respect for the opinions of others, had published a geologic map of the
United States containing gross errors. In support of his views he read in
Page 182
November, 1861, a paper on the Taconic and Lower Silurian Rocks of
Vermont and Canada. In the following year he was severely reviewed by
“T,” who states positively in controverting Marcou (33, 282, 283, 1862) that
“the granites (of the Green Mountains) are evidently strata altered in place.”
“Mr. Marcou should further be informed that the granites of the Alpine summits, instead of being,
as was once supposed, eruptive rocks, are now known to be altered strata of newer Secondary and
Tertiary age. A simple structure holds good in the British Islands, where as Sir Roderick Murchison
has shown in his recent Geological map of Scotland, Ben Nevis and Ben Lawers are found to be
composed of higher strata, lying in synclinals. This great law of mountain structure would alone lead
us to suppose that the gneiss of the Green mountains, instead of being at the base, is really at the
summit of the series....
We cannot here stop to discuss Mr. Marcou’s remark about ‘the unstratified and oldest crystalline
rocks of the White mountains’ which he places beneath the lower Taconic series. Mr. Lesley has
shown that these granites are stratified, and with Mr. Hunt, regards them as of Devonian Age. (This
Journal, vol. 31, p. 403.) Mr. Marcou has come among us with notions of mountains upheaved by
intrusive granites, and similar antiquated traditions, now, happily for science, well nigh forgotten.”
It is seen that Marcou, notwithstanding the general character of his work,
happened to be nearer right in some matters than were his critics, and that
“T” had adopted to the limit the views of Hunt.
The recovery of geology from this period of confusion was partly owing
to the slow accumulation of opposed facts; especially to a recognition of the
fact that the overplaced relation of the granite gneisses in western Scotland
was due to great overthrusts; also to the evidence of the clearly intrusive
nature of many of the Cordilleran granites. The recovery of a sounder
theory was hastened, however, by the application of criticisms by J. D.
Dana in the Journal. In 1866 (42, 252) Dana pointed out that sedimentary
rocks in Pennsylvania, in Nova Scotia, and other regions which had been
buried to a depth of at least 16,000 feet are not metamorphic. Mere depth of
burial of sediments was not sufficient therefore to produce metamorphism
and aqueo-igneous fusion. The baseless and speculative character of the use
of minerals as an index of age and of Hunt’s interpretation of New England
geology in general was shown by Dana in 1872 (3, 91). The following year
Dana pointed out clearly that igneous eruptions in general have been
derived from a deep-seated source and did not come from the aqueo-
igneous fusion of sediments. As to gradations between true igneous rocks
and fused and displaced sediments he makes the following statements (6,
114, 1873):
Vermont and Canada. In the following year he was severely reviewed by
“T,” who states positively in controverting Marcou (33, 282, 283, 1862) that
“the granites (of the Green Mountains) are evidently strata altered in place.”
“Mr. Marcou should further be informed that the granites of the Alpine summits, instead of being,
as was once supposed, eruptive rocks, are now known to be altered strata of newer Secondary and
Tertiary age. A simple structure holds good in the British Islands, where as Sir Roderick Murchison
has shown in his recent Geological map of Scotland, Ben Nevis and Ben Lawers are found to be
composed of higher strata, lying in synclinals. This great law of mountain structure would alone lead
us to suppose that the gneiss of the Green mountains, instead of being at the base, is really at the
summit of the series....
We cannot here stop to discuss Mr. Marcou’s remark about ‘the unstratified and oldest crystalline
rocks of the White mountains’ which he places beneath the lower Taconic series. Mr. Lesley has
shown that these granites are stratified, and with Mr. Hunt, regards them as of Devonian Age. (This
Journal, vol. 31, p. 403.) Mr. Marcou has come among us with notions of mountains upheaved by
intrusive granites, and similar antiquated traditions, now, happily for science, well nigh forgotten.”
It is seen that Marcou, notwithstanding the general character of his work,
happened to be nearer right in some matters than were his critics, and that
“T” had adopted to the limit the views of Hunt.
The recovery of geology from this period of confusion was partly owing
to the slow accumulation of opposed facts; especially to a recognition of the
fact that the overplaced relation of the granite gneisses in western Scotland
was due to great overthrusts; also to the evidence of the clearly intrusive
nature of many of the Cordilleran granites. The recovery of a sounder
theory was hastened, however, by the application of criticisms by J. D.
Dana in the Journal. In 1866 (42, 252) Dana pointed out that sedimentary
rocks in Pennsylvania, in Nova Scotia, and other regions which had been
buried to a depth of at least 16,000 feet are not metamorphic. Mere depth of
burial of sediments was not sufficient therefore to produce metamorphism
and aqueo-igneous fusion. The baseless and speculative character of the use
of minerals as an index of age and of Hunt’s interpretation of New England
geology in general was shown by Dana in 1872 (3, 91). The following year
Dana pointed out clearly that igneous eruptions in general have been
derived from a deep-seated source and did not come from the aqueo-
igneous fusion of sediments. As to gradations between true igneous rocks
and fused and displaced sediments he makes the following statements (6,
114, 1873):
Page 183
“Again, the plastic rock-material that may be derived from the fusion or semifusion of the
supercrust, (that is, of rocks originally of sedimentary origin,) gives rise to “igneous” rocks often not
distinguishable from other igneous rocks, when it is ejected through fissures far from its place of
origin; while crystalline rocks are simply metamorphic if they remain in their original relations to the
associated rocks, or nearly so.
Between these latter igneous rocks and the metamorphic there may be indefinite gradations, as
claimed by Hunt. But if our reasonings are right, the great part of igneous rocks can be proved to
have had no such supercrust origin. The argument from the presence of moisture or of hydrous
minerals in such rocks in favor of their origin from the fusion of sediments has been shown to be
invalid.”
The injected marginal rocks and the post-intrusive metamorphism of
most of the New England granites has, however, obscured more or less their
real igneous nature so that the gradation from metamorphic sediments
through igneous gneisses to granites could be read in either direction. These
features misled Dana who accepted the prevailing idea of the general
metamorphic origin of granite. Dana makes the following statement (6, 164,
1873):
“But Hunt is right in holding that in general granite and syenite (the quartz-bearing syenite) are
undoubtedly metamorphic rocks where not vein-formations, as I know from the study of many
examples of them in New England; and the veins are results of infiltration through heated moisture
from the rocks adjoining some part of the opened fissures they fill.”
Granite, although regarded at this time as the extreme of the
metamorphic series and originating from sediments, was looked upon as
typically Archean in age, though in some cases younger. Such a doctrine
permitted such extreme misinterpretations as that of Clarence King and S.
F. Emmons on the nature of the intrusive granite of the Little Cottonwood
canyon in the Wahsatch Range. This body cuts across 30,000 feet of
Paleozoic rocks and to the careful observer, as later admitted by Emmons,
shows clear evidence of its transgressive nature. But at that time it was
generally considered that granite mountains were capable of resisting the
erosion of all geological time. Consequently it did not seem incredible to
King and his associates that here a great granite range of Archean origin had
stood up through Paleozoic time until gradual subsidence had permitted it to
be buried beneath 30,000 feet of sediments.[82]
It may seem to the present day reader that such a misinterpretation, doing
violence to fundamental geologic knowledge as now recognized, was
supercrust, (that is, of rocks originally of sedimentary origin,) gives rise to “igneous” rocks often not
distinguishable from other igneous rocks, when it is ejected through fissures far from its place of
origin; while crystalline rocks are simply metamorphic if they remain in their original relations to the
associated rocks, or nearly so.
Between these latter igneous rocks and the metamorphic there may be indefinite gradations, as
claimed by Hunt. But if our reasonings are right, the great part of igneous rocks can be proved to
have had no such supercrust origin. The argument from the presence of moisture or of hydrous
minerals in such rocks in favor of their origin from the fusion of sediments has been shown to be
invalid.”
The injected marginal rocks and the post-intrusive metamorphism of
most of the New England granites has, however, obscured more or less their
real igneous nature so that the gradation from metamorphic sediments
through igneous gneisses to granites could be read in either direction. These
features misled Dana who accepted the prevailing idea of the general
metamorphic origin of granite. Dana makes the following statement (6, 164,
1873):
“But Hunt is right in holding that in general granite and syenite (the quartz-bearing syenite) are
undoubtedly metamorphic rocks where not vein-formations, as I know from the study of many
examples of them in New England; and the veins are results of infiltration through heated moisture
from the rocks adjoining some part of the opened fissures they fill.”
Granite, although regarded at this time as the extreme of the
metamorphic series and originating from sediments, was looked upon as
typically Archean in age, though in some cases younger. Such a doctrine
permitted such extreme misinterpretations as that of Clarence King and S.
F. Emmons on the nature of the intrusive granite of the Little Cottonwood
canyon in the Wahsatch Range. This body cuts across 30,000 feet of
Paleozoic rocks and to the careful observer, as later admitted by Emmons,
shows clear evidence of its transgressive nature. But at that time it was
generally considered that granite mountains were capable of resisting the
erosion of all geological time. Consequently it did not seem incredible to
King and his associates that here a great granite range of Archean origin had
stood up through Paleozoic time until gradual subsidence had permitted it to
be buried beneath 30,000 feet of sediments.[82]
It may seem to the present day reader that such a misinterpretation, doing
violence to fundamental geologic knowledge as now recognized, was
Page 184
inexcusable; but in the light of the history of geology as here detailed it is
seen to have been the interpretation natural to that time. It is true that a
careful examination of the facts of that very field would have proved the
post-Paleozoic and intrusive nature of that great granite body now known as
the Little Cottonwood batholith, but Emmons has explained the rapid and
partial nature of the observations which they were compelled to make in
order to keep up to their schedule of progress (16, 139, 1903).
Whitney had found some years earlier that the granites of the Sierra
Nevada were igneous rocks intrusive into the Triassic and Jurassic strata.
The Lake Superior geologists began to show in the eighties that granite was
there an intrusive igneous rock. R. D. Irving and Wadsworth noted these
relations. Lawson in 1887 pointed out emphatically (33, 473) that the
granites of the Rainy Lake region, although basal, were younger than the
schists which lay above them. The granite gneisses he held were of clearly
the same igneous origin as the granites and neither gave any field evidence
of being fused and displaced sediments. From this time forward the truly
igneous nature of granite became increasingly accepted until now the notion
of its being made of sedimentary rocks softened and recrystallized by the
rise of the isogeotherms through deep burial is as obsolete as the still older
doctrine of the Neptunists that granite was laid down as a crystalline
precipitate on the floor of the primitive ocean.
The recognition of the truly igneous nature of granites has been followed
in the present generation by a series of studies on their structural relations
and mode of genesis. A number of important initial articles on various
aspects of structure and contact relations have appeared in the Journal, but
this sketch of the history of the subject may well stop with the introduction
to this modern period.
seen to have been the interpretation natural to that time. It is true that a
careful examination of the facts of that very field would have proved the
post-Paleozoic and intrusive nature of that great granite body now known as
the Little Cottonwood batholith, but Emmons has explained the rapid and
partial nature of the observations which they were compelled to make in
order to keep up to their schedule of progress (16, 139, 1903).
Whitney had found some years earlier that the granites of the Sierra
Nevada were igneous rocks intrusive into the Triassic and Jurassic strata.
The Lake Superior geologists began to show in the eighties that granite was
there an intrusive igneous rock. R. D. Irving and Wadsworth noted these
relations. Lawson in 1887 pointed out emphatically (33, 473) that the
granites of the Rainy Lake region, although basal, were younger than the
schists which lay above them. The granite gneisses he held were of clearly
the same igneous origin as the granites and neither gave any field evidence
of being fused and displaced sediments. From this time forward the truly
igneous nature of granite became increasingly accepted until now the notion
of its being made of sedimentary rocks softened and recrystallized by the
rise of the isogeotherms through deep burial is as obsolete as the still older
doctrine of the Neptunists that granite was laid down as a crystalline
precipitate on the floor of the primitive ocean.
The recognition of the truly igneous nature of granites has been followed
in the present generation by a series of studies on their structural relations
and mode of genesis. A number of important initial articles on various
aspects of structure and contact relations have appeared in the Journal, but
this sketch of the history of the subject may well stop with the introduction
to this modern period.
Page 185
Orogenic Structures.
Page 186
Views of Plutonists and Neptunists.
Orogenic structures are, as the name implies, those connected with the
birth of mountains. Nearly synonymous terms are deformative or secondary
structures. On a small scale this division embraces the phenomena exposed
in the rock ledge or quarry face, or in the dips and dislocations varying from
one exposure to another. These structures include faults, folds, and foliation.
On a larger scale are included the relations of the different ranges of a
mountain system to each other, relations to previous geologic history,
relations to the earth as a whole, and to the forces which have generated the
structures.
In order to see the stage of development of this subject in 1818 and its
progress as reflected through the publications of a century, more
particularly in the Journal, it is desirable to turn again to those two treatises
emanating from Edinburgh at the beginning of the nineteenth century and
representing two opposite schools of thought, the Plutonists and Neptunists.
Playfair, in 1802, devotes nineteen pages to the subject of the inflection
and elevation of strata.[83] He places emphasis on the characteristic
parallelism of the strike of the folds throughout a region, as shown through
the intersection of the folds by a horizontal plane of erosion. He contrasts
this with the arches shown in a transverse section and enlarges on our
ability to study the deeply buried strata through the denudation of the folded
structure. He argues from these relations that the structures can not be
explained by the vague appeal of the Neptunists to forces of crystallization,
to slopes of original deposition, or to sinking in of the roofs of caverns. The
causes he argues were heat combined with pressure. As to the directions in
which the pressure acted he is not altogether clear, but apparently regards
the pressure as acting in upward thrusts against the sedimentary planes, the
latter yielding as warped surfaces. His method of presentation is that of
inductive reasoning from facts, but he stopped short of the conception of
horizontal compression through terrestrial contraction.
Jameson, professor of natural history in the same university, in 1808
contemptuously ignores the work of Hutton and Playfair in what he calls
the “monstrosities known under the name of Theories of the Earth.” In a
Orogenic structures are, as the name implies, those connected with the
birth of mountains. Nearly synonymous terms are deformative or secondary
structures. On a small scale this division embraces the phenomena exposed
in the rock ledge or quarry face, or in the dips and dislocations varying from
one exposure to another. These structures include faults, folds, and foliation.
On a larger scale are included the relations of the different ranges of a
mountain system to each other, relations to previous geologic history,
relations to the earth as a whole, and to the forces which have generated the
structures.
In order to see the stage of development of this subject in 1818 and its
progress as reflected through the publications of a century, more
particularly in the Journal, it is desirable to turn again to those two treatises
emanating from Edinburgh at the beginning of the nineteenth century and
representing two opposite schools of thought, the Plutonists and Neptunists.
Playfair, in 1802, devotes nineteen pages to the subject of the inflection
and elevation of strata.[83] He places emphasis on the characteristic
parallelism of the strike of the folds throughout a region, as shown through
the intersection of the folds by a horizontal plane of erosion. He contrasts
this with the arches shown in a transverse section and enlarges on our
ability to study the deeply buried strata through the denudation of the folded
structure. He argues from these relations that the structures can not be
explained by the vague appeal of the Neptunists to forces of crystallization,
to slopes of original deposition, or to sinking in of the roofs of caverns. The
causes he argues were heat combined with pressure. As to the directions in
which the pressure acted he is not altogether clear, but apparently regards
the pressure as acting in upward thrusts against the sedimentary planes, the
latter yielding as warped surfaces. His method of presentation is that of
inductive reasoning from facts, but he stopped short of the conception of
horizontal compression through terrestrial contraction.
Jameson, professor of natural history in the same university, in 1808
contemptuously ignores the work of Hutton and Playfair in what he calls
the “monstrosities known under the name of Theories of the Earth.” In a
Page 187
couple of pages he confuses and dismisses the whole subject of
deformation. He states:[84]
“It is therefore a fact, that all inclined strata, with a very few exceptions, have been formed so
originally, and do not owe their inclination to a subsequent change.
When we examine the structure of a mountain, we must be careful that our observations be not too
micrological, otherwise we shall undoubtedly fail in acquiring a distinct conception of it. This will
appear evident when we reflect that the geognostic features of Nature are almost all on the great
scale. In no case is this rule to be more strictly followed than in the examination of the stratified
structure.
By not attending to this mode of examination, geognosts have fallen into numberless errors, and
have frequently given to extensive tracts of country a most irregular and confused structure.
Speculators building on these errors have represented the whole crust of the globe as an irregular and
unseemly mass. It is indeed surprising, that men possessed of any knowledge of the beautiful
harmony that prevails in the structure of organic beings could for a moment believe it possible, that
the great fabric of the globe itself,—that magnificent display of Omnipotence,—should be destitute
of all regularity in its structure, and be nothing more than a heap of ruins.”
This was the attitude of a leader of British opinion toward the subject of
deformational geology from which the infant science had to recover before
progress could be made. The early maps were essentially mineralogical and
lithological. The order of superposition and the consequent sequence of age
was regarded as settled by Werner in Germany and not requiring
investigation in America. The early examples of structure were sections
drawn with exaggerated vertical scales and those of Maclure do not show
detail.
deformation. He states:[84]
“It is therefore a fact, that all inclined strata, with a very few exceptions, have been formed so
originally, and do not owe their inclination to a subsequent change.
When we examine the structure of a mountain, we must be careful that our observations be not too
micrological, otherwise we shall undoubtedly fail in acquiring a distinct conception of it. This will
appear evident when we reflect that the geognostic features of Nature are almost all on the great
scale. In no case is this rule to be more strictly followed than in the examination of the stratified
structure.
By not attending to this mode of examination, geognosts have fallen into numberless errors, and
have frequently given to extensive tracts of country a most irregular and confused structure.
Speculators building on these errors have represented the whole crust of the globe as an irregular and
unseemly mass. It is indeed surprising, that men possessed of any knowledge of the beautiful
harmony that prevails in the structure of organic beings could for a moment believe it possible, that
the great fabric of the globe itself,—that magnificent display of Omnipotence,—should be destitute
of all regularity in its structure, and be nothing more than a heap of ruins.”
This was the attitude of a leader of British opinion toward the subject of
deformational geology from which the infant science had to recover before
progress could be made. The early maps were essentially mineralogical and
lithological. The order of superposition and the consequent sequence of age
was regarded as settled by Werner in Germany and not requiring
investigation in America. The early examples of structure were sections
drawn with exaggerated vertical scales and those of Maclure do not show
detail.
Page 188
Recognition of Appalachian Structures.
Following the founding of the Journal in 1818 there is observable a
growth in the quality and detail of geological mapping. Dr. Aiken, professor
of natural philosophy and chemistry in Mt. St. Mary’s College, published in
the Journal in 1834 (26, 219) a vertical section extending between
Baltimore and Wheeling, a distance of nearly 250 miles, on a scale of about
7 miles per inch. The succession of rocks is carefully shown and the
direction of dip, but no attempt is made to show the underground relations,
the stratigraphic sequence, and the folded structures which are so clear in
that Appalachian section. The text also shows that the author had not
recognized the folded structure. Furthermore, where the folds cease at the
Alleghany mountain front, the flat strata are shown as resting
unconformably on the folded rocks to the east.
R. C. Taylor, geologist, civil and mining engineer, was from 1830 to 1835
the leading student of Pennsylvanian geology as shown by the publication
in 1835 of four papers aggregating over 80 pages in the Transactions of the
Geological Society of Pennsylvania. His work is noticeable for accuracy in
detail and no doubt was influential in setting a high standard for the state
geological survey which immediately followed.
H. D. and W. B. Rogers have been given credit in this country, and in
Europe also, as being the leading expounders of Appalachian structure.
Merrill speaks of H. D. Rogers as unquestionably the leading structural
geologist of his time.[85] To the writer, this attributed position appears to be
due to his opportunities rather than to scientific acumen. The magnificent
but readily decipherable folded structure of Pennsylvania, the relationships
of coal and iron to this structure, the considerable sums of money
appropriated, and the work of a corps of able assistants were factors which
made it comparatively easy to reach important results. In ability to weigh
facts and interpret them Edward Hitchcock showed much more insight than
H. D. Rogers, while in the philosophic and comprehensive aspects of the
subject J. D. Dana far outranks him.
H. D. Rogers in his first report on the geological survey of New Jersey,
1836, recognizes that the Cambro-Silurian limestones (lower Secondary
Following the founding of the Journal in 1818 there is observable a
growth in the quality and detail of geological mapping. Dr. Aiken, professor
of natural philosophy and chemistry in Mt. St. Mary’s College, published in
the Journal in 1834 (26, 219) a vertical section extending between
Baltimore and Wheeling, a distance of nearly 250 miles, on a scale of about
7 miles per inch. The succession of rocks is carefully shown and the
direction of dip, but no attempt is made to show the underground relations,
the stratigraphic sequence, and the folded structures which are so clear in
that Appalachian section. The text also shows that the author had not
recognized the folded structure. Furthermore, where the folds cease at the
Alleghany mountain front, the flat strata are shown as resting
unconformably on the folded rocks to the east.
R. C. Taylor, geologist, civil and mining engineer, was from 1830 to 1835
the leading student of Pennsylvanian geology as shown by the publication
in 1835 of four papers aggregating over 80 pages in the Transactions of the
Geological Society of Pennsylvania. His work is noticeable for accuracy in
detail and no doubt was influential in setting a high standard for the state
geological survey which immediately followed.
H. D. and W. B. Rogers have been given credit in this country, and in
Europe also, as being the leading expounders of Appalachian structure.
Merrill speaks of H. D. Rogers as unquestionably the leading structural
geologist of his time.[85] To the writer, this attributed position appears to be
due to his opportunities rather than to scientific acumen. The magnificent
but readily decipherable folded structure of Pennsylvania, the relationships
of coal and iron to this structure, the considerable sums of money
appropriated, and the work of a corps of able assistants were factors which
made it comparatively easy to reach important results. In ability to weigh
facts and interpret them Edward Hitchcock showed much more insight than
H. D. Rogers, while in the philosophic and comprehensive aspects of the
subject J. D. Dana far outranks him.
H. D. Rogers in his first report on the geological survey of New Jersey,
1836, recognizes that the Cambro-Silurian limestones (lower Secondary
Page 189
limestones) were deposited as nearly horizontal beds and the ridges of pre-
Cambrian gneiss (Primary) had been pushed up as anticlinal axes (p. 128).
He also clearly recognized the distinction between slaty cleavage and true
dip as shown in the Ordovician slates (p. 97). Between 1836 and 1840 he
had learned a great deal on the nature of folds as is shown in his
Pennsylvania report for 1839 and the structure sections in his New Jersey
report for 1840.
R. C. Taylor, who had now become president of the board of directors of
the Dauphin and Susquehanna Coal Company, published in the Journal in
1841 (41, 80) an important paper entitled “Notice of a Model of the Western
portion of the Schuylkill or Southern Coal Field of Pennsylvania, in
illustration of an Address to the Association of American Geologists, on the
most appropriate modes for representing Geological Phenomena.” In this
paper he calls attention to the value of modeling as a means of showing true
relations in three dimensions. He condemns the custom prevalent among
geologists of showing structure sections with an exaggerated vertical scale
with its resultant topographic and structural distortions. Taylor was widely
acquainted with the structure of Pennsylvania, Maryland, and Virginia.
Cambrian gneiss (Primary) had been pushed up as anticlinal axes (p. 128).
He also clearly recognized the distinction between slaty cleavage and true
dip as shown in the Ordovician slates (p. 97). Between 1836 and 1840 he
had learned a great deal on the nature of folds as is shown in his
Pennsylvania report for 1839 and the structure sections in his New Jersey
report for 1840.
R. C. Taylor, who had now become president of the board of directors of
the Dauphin and Susquehanna Coal Company, published in the Journal in
1841 (41, 80) an important paper entitled “Notice of a Model of the Western
portion of the Schuylkill or Southern Coal Field of Pennsylvania, in
illustration of an Address to the Association of American Geologists, on the
most appropriate modes for representing Geological Phenomena.” In this
paper he calls attention to the value of modeling as a means of showing true
relations in three dimensions. He condemns the custom prevalent among
geologists of showing structure sections with an exaggerated vertical scale
with its resultant topographic and structural distortions. Taylor was widely
acquainted with the structure of Pennsylvania, Maryland, and Virginia.
Page 190
Nature of Forces Producing Folding.
In 1825 Dr. J. H. Steele sent to Professor Silliman two detailed drawings
and description of an overturned fold at Saratoga Lake, New York. As to the
significance of this feature Steele makes the following statement (9, 3,
1825):
“It is impossible to examine this locality without being strongly impressed with the belief that the
position which the strata here assume could not have been effected in any other way than by a power
operating from beneath upwards and at the same time possessing a progressive force; something
analogous to what takes place in the breaking up of the ice of large rivers. The continued swelling of
the stream first overcomes the resistance of its frozen surface and having elevated it to a certain
extent, it is forced into a vertical position, or thrown over upon the unbroken stratum behind, by the
progressive power of the current.”
So far as the present writer is aware this is the first recognition in
geological literature of the evidence of a horizontally compressive and
overturning force as a cause of folding.
To E. Hitchcock belongs the credit of being the first to describe
overturning and inversion of strata on a large scale, but without clearly
recognizing it as such. In western Massachusetts metamorphism is extreme
in the lower Paleozoic rocks in the vicinity of the overthrust mass of
Archean granite-gneiss which constitutes the Hoosic range. The Paleozoic
rocks of the valley to the west are overturned and appear to dip beneath the
older rocks. Farther west the metamorphism fades out and the series
assumes a normal position. Such an inverted relation, up to that time
unknown, is described in 1833 as follows by Hitchcock in his Geology of
Massachusetts (pp. 297, 298):
“But a singular anomaly in the superposition of the series of rocks above described, presents a
great difficulty in this case. The strata of these rocks almost uniformly dip to the east: that is, the
newer rocks seem to crop out beneath the older ones; so that the saccharine limestone, associated
with gneiss in the eastern part of the range, seems to occupy the uppermost place in the series. Now
as superposition is of more value in determining the relative ages of rocks than their mineral
characters, must we not conclude that the rocks, as we go westerly from Hoosac mountain, do in fact
belong to older groups? The petrifactions which some of them contain, and their decidedly
fragmentary character, will not allow such a supposition to be indulged for a moment. It is impossible
for a geologist to mistake the evidence, which he sees at almost every step, that he is passing from
In 1825 Dr. J. H. Steele sent to Professor Silliman two detailed drawings
and description of an overturned fold at Saratoga Lake, New York. As to the
significance of this feature Steele makes the following statement (9, 3,
1825):
“It is impossible to examine this locality without being strongly impressed with the belief that the
position which the strata here assume could not have been effected in any other way than by a power
operating from beneath upwards and at the same time possessing a progressive force; something
analogous to what takes place in the breaking up of the ice of large rivers. The continued swelling of
the stream first overcomes the resistance of its frozen surface and having elevated it to a certain
extent, it is forced into a vertical position, or thrown over upon the unbroken stratum behind, by the
progressive power of the current.”
So far as the present writer is aware this is the first recognition in
geological literature of the evidence of a horizontally compressive and
overturning force as a cause of folding.
To E. Hitchcock belongs the credit of being the first to describe
overturning and inversion of strata on a large scale, but without clearly
recognizing it as such. In western Massachusetts metamorphism is extreme
in the lower Paleozoic rocks in the vicinity of the overthrust mass of
Archean granite-gneiss which constitutes the Hoosic range. The Paleozoic
rocks of the valley to the west are overturned and appear to dip beneath the
older rocks. Farther west the metamorphism fades out and the series
assumes a normal position. Such an inverted relation, up to that time
unknown, is described in 1833 as follows by Hitchcock in his Geology of
Massachusetts (pp. 297, 298):
“But a singular anomaly in the superposition of the series of rocks above described, presents a
great difficulty in this case. The strata of these rocks almost uniformly dip to the east: that is, the
newer rocks seem to crop out beneath the older ones; so that the saccharine limestone, associated
with gneiss in the eastern part of the range, seems to occupy the uppermost place in the series. Now
as superposition is of more value in determining the relative ages of rocks than their mineral
characters, must we not conclude that the rocks, as we go westerly from Hoosac mountain, do in fact
belong to older groups? The petrifactions which some of them contain, and their decidedly
fragmentary character, will not allow such a supposition to be indulged for a moment. It is impossible
for a geologist to mistake the evidence, which he sees at almost every step, that he is passing from
Page 191
older to newer formations, just as soon as he begins to cross the valley of Berkshire towards the west.
We are driven then to the alternative of supposing, either that there must be a deception in the
apparent outcrop of the newer rocks from beneath the older, or that the whole series of strata has been
actually thrown over, so as to bring the newest rocks at the bottom. The latter supposition is so
improbable that I cannot at present admit it.”
Hitchcock tried to reconcile the evidence by a series of unconformities
and inclined deposition, but finds the solution unsatisfactory.
In this same year, 1833, Elie de Beaumont, a distinguished French
geologist, published his theory of the origin of mountains. He advanced the
idea that since the globe was cooling it was condensing, and the crust,
already cool, must suffer compression in adjusting itself to the shrinking
molten interior. He concluded from the evidence shown in Europe that the
collapse of the crust occurred violently and rapidly at widely spaced
intervals of time. This hypothesis introduced the idea of mountain folding
by horizontal compressive forces. The theoretical paper of de Beaumont,
together with further observations by Hitchcock and others, led the latter in
1841 to a final belief in the inversion of strata on a large scale by horizontal
compression. His conclusions are expressed in an important paper
published in the Journal (41, 268, 1841) and given on April 8, 1841, as the
First Anniversary Presidential Address before the Association of American
Geologists. This comprehensive summary of American geology occupies 43
pages. Three pages are given to the inverted structure of the Appalachians
from which the following paragraphs may be quoted:
“We have all read of the enormous dislocations and inversions of the strata of the Alps; and similar
phenomena are said to exist in the Andes. Will it be believed, that we have an example in the United
States on a still more magnificent scale than any yet described?...
Let us suppose the strata between Hudson and Connecticut rivers, while yet in the plastic state,
(and the supposition may be extended to any other section across this belt of country from Canada to
Alabama,) and while only slightly elevated, were acted upon by a force at the two rivers, exerted in
opposite directions. If powerful enough, it might cause them to fold up into several ridges; and if
more powerful along the western than the eastern side, they might fall over so as to take an inverted
dip, without producing any remarkable dislocations, while subsequent denudation would give to the
surface its present outline....
Fourthly, we should readily admit that such a plication and inversion of the strata might take place
on a small scale. If for instance, we were to press against the extremities of a series of plastic layers
two feet long, they could easily be made to assume the position into which the rocks under
consideration are thrown. Why then should we not be equally ready to admit that this might as easily
be done, over a breadth of fifty miles, and a length of twelve hundred, provided we can find in
We are driven then to the alternative of supposing, either that there must be a deception in the
apparent outcrop of the newer rocks from beneath the older, or that the whole series of strata has been
actually thrown over, so as to bring the newest rocks at the bottom. The latter supposition is so
improbable that I cannot at present admit it.”
Hitchcock tried to reconcile the evidence by a series of unconformities
and inclined deposition, but finds the solution unsatisfactory.
In this same year, 1833, Elie de Beaumont, a distinguished French
geologist, published his theory of the origin of mountains. He advanced the
idea that since the globe was cooling it was condensing, and the crust,
already cool, must suffer compression in adjusting itself to the shrinking
molten interior. He concluded from the evidence shown in Europe that the
collapse of the crust occurred violently and rapidly at widely spaced
intervals of time. This hypothesis introduced the idea of mountain folding
by horizontal compressive forces. The theoretical paper of de Beaumont,
together with further observations by Hitchcock and others, led the latter in
1841 to a final belief in the inversion of strata on a large scale by horizontal
compression. His conclusions are expressed in an important paper
published in the Journal (41, 268, 1841) and given on April 8, 1841, as the
First Anniversary Presidential Address before the Association of American
Geologists. This comprehensive summary of American geology occupies 43
pages. Three pages are given to the inverted structure of the Appalachians
from which the following paragraphs may be quoted:
“We have all read of the enormous dislocations and inversions of the strata of the Alps; and similar
phenomena are said to exist in the Andes. Will it be believed, that we have an example in the United
States on a still more magnificent scale than any yet described?...
Let us suppose the strata between Hudson and Connecticut rivers, while yet in the plastic state,
(and the supposition may be extended to any other section across this belt of country from Canada to
Alabama,) and while only slightly elevated, were acted upon by a force at the two rivers, exerted in
opposite directions. If powerful enough, it might cause them to fold up into several ridges; and if
more powerful along the western than the eastern side, they might fall over so as to take an inverted
dip, without producing any remarkable dislocations, while subsequent denudation would give to the
surface its present outline....
Fourthly, we should readily admit that such a plication and inversion of the strata might take place
on a small scale. If for instance, we were to press against the extremities of a series of plastic layers
two feet long, they could easily be made to assume the position into which the rocks under
consideration are thrown. Why then should we not be equally ready to admit that this might as easily
be done, over a breadth of fifty miles, and a length of twelve hundred, provided we can find in
Page 192
nature, forces sufficiently powerful? Finally, such forces do exist in nature, and have often been in
operation.”
The advanced nature of these conceptions may be appreciated by
contrasting them with those put forth by H. D. and W. B. Rogers on April
29, 1842, before the third annual meeting of the same body (43, 177, 1842)
and repeated by them before the British Association at Manchester two
months later. In their own words, the Rogers brothers from their studies on
the folds shown in Pennsylvania and Virginia, conceived mountain folds in
general to be produced by much elastic vapor escaping through many
parallel fissures formed in succession, producing violent propulsive wave
oscillations on the surface of the fluid earth beneath a thin crust. Thus actual
billows are assumed to have rolled along through the crust. They did not
think tangential pressure alone could produce folds. Such pressures were
regarded as secondary, produced by the propagation of the waves and the
only expression of tangential forces which they admitted was to fix the
folds and hold them in position after the violent oscillation had subsided
(44, 360, 1843). The leading British geologists De la Beche and Sedgwick
criticized adversely this remarkable theory, stating that they could see no
such analogy in mountain folds to violent earthquake waves and that in
their opinion the slow application of tangential force was sufficient to
account for the phenomena (44, 362–365, 1843).
H. D. Rogers in the prosecution of the geological survey of Pennsylvania
displayed notable organizing ability and persistence in accomplishment,
even to advancing personally considerable sums of money, trusting to the
state legislature to later reimburse him. Finally, after many delays by the
state, the publication was placed directly in his charge and he produced in
1858 a magnificent quarto work of over 1,600 pages, handsomely
illustrated, and accompanied by an atlas. It is excellent from the descriptive
standpoint, standing in the first class. Measured as a contribution to the
theory of dynamical geology, the explanatory portions were, however, thirty
years behind the times. The same hypotheses are put forth in 1858 as in
1842. There is no acceptance of the views of Lyell concerning the
uniformitarian principles expounded by this British leader in 1830, or of the
nature of orogenic forces as published by Elie de Beaumont in 1833. Rogers
rejects the view that cleavage is due to compression and suggests “that both
cleavage and foliation are due to the parallel transmission of planes or
operation.”
The advanced nature of these conceptions may be appreciated by
contrasting them with those put forth by H. D. and W. B. Rogers on April
29, 1842, before the third annual meeting of the same body (43, 177, 1842)
and repeated by them before the British Association at Manchester two
months later. In their own words, the Rogers brothers from their studies on
the folds shown in Pennsylvania and Virginia, conceived mountain folds in
general to be produced by much elastic vapor escaping through many
parallel fissures formed in succession, producing violent propulsive wave
oscillations on the surface of the fluid earth beneath a thin crust. Thus actual
billows are assumed to have rolled along through the crust. They did not
think tangential pressure alone could produce folds. Such pressures were
regarded as secondary, produced by the propagation of the waves and the
only expression of tangential forces which they admitted was to fix the
folds and hold them in position after the violent oscillation had subsided
(44, 360, 1843). The leading British geologists De la Beche and Sedgwick
criticized adversely this remarkable theory, stating that they could see no
such analogy in mountain folds to violent earthquake waves and that in
their opinion the slow application of tangential force was sufficient to
account for the phenomena (44, 362–365, 1843).
H. D. Rogers in the prosecution of the geological survey of Pennsylvania
displayed notable organizing ability and persistence in accomplishment,
even to advancing personally considerable sums of money, trusting to the
state legislature to later reimburse him. Finally, after many delays by the
state, the publication was placed directly in his charge and he produced in
1858 a magnificent quarto work of over 1,600 pages, handsomely
illustrated, and accompanied by an atlas. It is excellent from the descriptive
standpoint, standing in the first class. Measured as a contribution to the
theory of dynamical geology, the explanatory portions were, however, thirty
years behind the times. The same hypotheses are put forth in 1858 as in
1842. There is no acceptance of the views of Lyell concerning the
uniformitarian principles expounded by this British leader in 1830, or of the
nature of orogenic forces as published by Elie de Beaumont in 1833. Rogers
rejects the view that cleavage is due to compression and suggests “that both
cleavage and foliation are due to the parallel transmission of planes or
Page 193
waves of heat, awakening the molecular forces, and determining their
direction.”[86] Thus a mere maze of words takes the place of inductive
demonstrations already published.
In following the play of these opposing currents of geologic thought we
reach now the point where a period of brilliant progress in the knowledge of
mountains and of continental structures begins in the work of J. D. Dana. In
1842 Dana returned from the Wilkes Exploring Expedition and the
following year began the publication of the series of papers which for the
next half century marked him as the leader in geologic theory in America.
His work is of course to be judged against the background of his times. His
papers mark distinct advances in many lines and are characterized
throughout by breadth of conception and especially by clear and logical
thinking. His work was published very largely in the Journal, of which after
a few years he became chief editor. His first contribution on the subject of
mountain structures, entitled “Geological results of the earth’s contraction
in consequence of cooling,” was published in 1847 (3, 176). The evidence
of horizontal pressure was first perceived in France as shown by the
features of the Alps. Elie de Beaumont connected it, by means of the theory
of a cooling and contracting globe, with the other large fact of the increase
of temperature with descent in the crust. Dana credits the Rogers brothers
with first making known the folded structures of the Appalachians, but
objects to their interpretation of origin. He showed by means of diagrams
that the folds are to be explained by lateral pressure, the direction of
overturning indicating the direction from which the driving force
proceeded.
The Rogers brothers and especially James Hall, in working out the
Appalachian stratigraphy, had noted that the formations, although
accumulating to a maximum thickness of between 30,000 and 40,000 feet,
showed evidences that the successive formations were deposited in shallow
water. It suggested to them that the weight of the accumulating sediments
was the cause of subsidence, each foot of sediment causing a foot of down
sinking. This idea has continued to run through various text books in
geology for half a century, yet Dana early saw the fallacy and in 1863 in the
first edition of his Manual of Geology (p. 717) states “whether this is an
actual cause or not in geological dynamics is questionable.” In 1866 in an
important article on “Observations on the origins of some of the earth’s
features,” Dana deals more fully and finally with this subject (42, 205, 252,
direction.”[86] Thus a mere maze of words takes the place of inductive
demonstrations already published.
In following the play of these opposing currents of geologic thought we
reach now the point where a period of brilliant progress in the knowledge of
mountains and of continental structures begins in the work of J. D. Dana. In
1842 Dana returned from the Wilkes Exploring Expedition and the
following year began the publication of the series of papers which for the
next half century marked him as the leader in geologic theory in America.
His work is of course to be judged against the background of his times. His
papers mark distinct advances in many lines and are characterized
throughout by breadth of conception and especially by clear and logical
thinking. His work was published very largely in the Journal, of which after
a few years he became chief editor. His first contribution on the subject of
mountain structures, entitled “Geological results of the earth’s contraction
in consequence of cooling,” was published in 1847 (3, 176). The evidence
of horizontal pressure was first perceived in France as shown by the
features of the Alps. Elie de Beaumont connected it, by means of the theory
of a cooling and contracting globe, with the other large fact of the increase
of temperature with descent in the crust. Dana credits the Rogers brothers
with first making known the folded structures of the Appalachians, but
objects to their interpretation of origin. He showed by means of diagrams
that the folds are to be explained by lateral pressure, the direction of
overturning indicating the direction from which the driving force
proceeded.
The Rogers brothers and especially James Hall, in working out the
Appalachian stratigraphy, had noted that the formations, although
accumulating to a maximum thickness of between 30,000 and 40,000 feet,
showed evidences that the successive formations were deposited in shallow
water. It suggested to them that the weight of the accumulating sediments
was the cause of subsidence, each foot of sediment causing a foot of down
sinking. This idea has continued to run through various text books in
geology for half a century, yet Dana early saw the fallacy and in 1863 in the
first edition of his Manual of Geology (p. 717) states “whether this is an
actual cause or not in geological dynamics is questionable.” In 1866 in an
important article on “Observations on the origins of some of the earth’s
features,” Dana deals more fully and finally with this subject (42, 205, 252,
Page 194
1866). He shows that such an effect of accumulating sediment postulates a
delicate balance, a very thin crust and no resistance below. If such a
weakness were granted it would be impossible for the earth to hold up
mountains. Furthermore such subsidence was not regular during its progress
and finally in the long course of geologic time gave place to a reverse
movement of elevation.
Hall had pointed out the fact that the sediments were thickest on the east
in the region of mountain folding and thinned out to a fraction of this
thickness in the broad Mississippi basin. Hall argued that the mere
subsidence of the trough would produce the observed folding and that the
folding was unrelated to mountain making or crustal shortening. In
supposed proof he cited the fact that the Catskills consist of unfolded rock,
are higher than the folded region to the south, and nearly as high as the
highest metamorphic mountains to the east.[87] Hall and all his
contemporaries were handicapped in their geological theories by a complete
inappreciation of the importance of subaërial denudation. For subscribing to
these errors of their time even the ablest men should not be held
responsible. Hall was the most forcible personality in geology in his
generation. His contributions to paleontology were superb. His perception
of the relation existing between troughs of thick sediments and folded
structures was a contribution of the first importance; yet in the structural
field his argument as to the production of the Appalachian folds by mere
subsidence during deposition indicates a remarkable inability to apply the
logical consequences of his hypothesis to the nature of the folds as already
made known by the Rogers. Dana pointed out in reply to Hall that the
folding did not correspond to the requirements of Hall’s hypothesis,
especially as the folding took place not during, but after the close of the vast
Paleozoic deposition. Dana states in conclusion on Hall’s hypothesis (42,
209, 1866) that “It is a theory of the origin of mountains with the origin of
mountains left out.”
delicate balance, a very thin crust and no resistance below. If such a
weakness were granted it would be impossible for the earth to hold up
mountains. Furthermore such subsidence was not regular during its progress
and finally in the long course of geologic time gave place to a reverse
movement of elevation.
Hall had pointed out the fact that the sediments were thickest on the east
in the region of mountain folding and thinned out to a fraction of this
thickness in the broad Mississippi basin. Hall argued that the mere
subsidence of the trough would produce the observed folding and that the
folding was unrelated to mountain making or crustal shortening. In
supposed proof he cited the fact that the Catskills consist of unfolded rock,
are higher than the folded region to the south, and nearly as high as the
highest metamorphic mountains to the east.[87] Hall and all his
contemporaries were handicapped in their geological theories by a complete
inappreciation of the importance of subaërial denudation. For subscribing to
these errors of their time even the ablest men should not be held
responsible. Hall was the most forcible personality in geology in his
generation. His contributions to paleontology were superb. His perception
of the relation existing between troughs of thick sediments and folded
structures was a contribution of the first importance; yet in the structural
field his argument as to the production of the Appalachian folds by mere
subsidence during deposition indicates a remarkable inability to apply the
logical consequences of his hypothesis to the nature of the folds as already
made known by the Rogers. Dana pointed out in reply to Hall that the
folding did not correspond to the requirements of Hall’s hypothesis,
especially as the folding took place not during, but after the close of the vast
Paleozoic deposition. Dana states in conclusion on Hall’s hypothesis (42,
209, 1866) that “It is a theory of the origin of mountains with the origin of
mountains left out.”
Page 195
The Theory of Geosynclines and Geanticlines.
The fact that systems of folded strata lie along axes of especially thick
sediments and that this implied subsidence during deposition was Hall’s
contribution to geologic theory, but curiously enough he failed, as shown, to
connect it with the subsequent nature of mountain folding. He did not see
why such troughs should be weak to resist horizontal compression. The
clear recognition of this relationship was the contribution of Le Conte, who
in a paper on “A theory of the formation of the great features of the earth’s
surface” (4, 345, 460, 1872), reached the conclusion that “mountain chains
are formed by the mashing together and the up-swelling of sea bottoms
where immense thicknesses of sediment have accumulated.”
As to the cause why mashing should take place along troughs of thick
sediments Le Conte adopts the hypothesis of aqueo-igneous fusion
proposed independently long before by Babbage and Herschel and
elaborated into a theory of igneous rocks by Hunt. Under this view, as the
older sediments became deeply buried, the heat of the earth’s interior
ascended into them, and since they included the water of sedimentation a
softening and metamorphism resulted. Dana had shown, however, six years
previously (42, 252, 1866), as the following quotation will indicate, that
metamorphism of sediments required more than deep burial and that no
such weakening as was postulated by Herschel had occurred:
“The correctness of Herschel’s principle cannot be doubted. But the question of its actual agency
in ordinary metamorphism must be decided by an appeal to facts; and on this point I would here
present a few facts for consideration.
The numbers and boldness of the flexures in the rocks of most metamorphic regions have always
seemed to me to bear against the view that the heat causing the change had ascended by the very
quiet method recognized in this theory....
But there are other facts indicating a limited sufficiency to this means of metamorphism. These are
afforded by the great faults and sections of strata open to examination. In the Appalachian region,
both of Virginia and Pennsylvania, faults occur, as described by the Professors Rogers, and by Mr. J.
P. Lesley, which afford us important data for conclusions. Mr. Lesley, an excellent geologist and
geological observer, who has explored personally the regions referred to, states that at the great fault
of Juniata and Blair Cos., Pennsylvania, the rocks of the Trenton period are brought up to a level with
those of the Chemung, making a dislocation of at least 16,000, and probably of 20,000, feet. And yet
the Trenton limestone and Hudson River shales are not metamorphic. Some local cases of alteration
The fact that systems of folded strata lie along axes of especially thick
sediments and that this implied subsidence during deposition was Hall’s
contribution to geologic theory, but curiously enough he failed, as shown, to
connect it with the subsequent nature of mountain folding. He did not see
why such troughs should be weak to resist horizontal compression. The
clear recognition of this relationship was the contribution of Le Conte, who
in a paper on “A theory of the formation of the great features of the earth’s
surface” (4, 345, 460, 1872), reached the conclusion that “mountain chains
are formed by the mashing together and the up-swelling of sea bottoms
where immense thicknesses of sediment have accumulated.”
As to the cause why mashing should take place along troughs of thick
sediments Le Conte adopts the hypothesis of aqueo-igneous fusion
proposed independently long before by Babbage and Herschel and
elaborated into a theory of igneous rocks by Hunt. Under this view, as the
older sediments became deeply buried, the heat of the earth’s interior
ascended into them, and since they included the water of sedimentation a
softening and metamorphism resulted. Dana had shown, however, six years
previously (42, 252, 1866), as the following quotation will indicate, that
metamorphism of sediments required more than deep burial and that no
such weakening as was postulated by Herschel had occurred:
“The correctness of Herschel’s principle cannot be doubted. But the question of its actual agency
in ordinary metamorphism must be decided by an appeal to facts; and on this point I would here
present a few facts for consideration.
The numbers and boldness of the flexures in the rocks of most metamorphic regions have always
seemed to me to bear against the view that the heat causing the change had ascended by the very
quiet method recognized in this theory....
But there are other facts indicating a limited sufficiency to this means of metamorphism. These are
afforded by the great faults and sections of strata open to examination. In the Appalachian region,
both of Virginia and Pennsylvania, faults occur, as described by the Professors Rogers, and by Mr. J.
P. Lesley, which afford us important data for conclusions. Mr. Lesley, an excellent geologist and
geological observer, who has explored personally the regions referred to, states that at the great fault
of Juniata and Blair Cos., Pennsylvania, the rocks of the Trenton period are brought up to a level with
those of the Chemung, making a dislocation of at least 16,000, and probably of 20,000, feet. And yet
the Trenton limestone and Hudson River shales are not metamorphic. Some local cases of alteration
Page 196
occur there, including patches of roofing slate; but the greater part of the shales are no harder than the
ordinary shales of the Pennsylvania Coal formation.
At a depth of 16,000 feet the temperature of the earth’s crust, allowing an increase of 1° F. for 60
feet of descent, would be about 330° F.; or with 1° F. for 50 feet, about 380° F.—either of which
temperatures is far above the boiling point of water; and with the thinner crust of Paleozoic time the
temperature at this depth should have been still higher. But, notwithstanding this heat, and also the
compression from so great an overlying mass, the limestones and shales are not crystalline. The
change of parts of the shale to roofing slate is no evidence in favor of the efficiency of the alleged
cause; for such a cause should act uniformly over great areas.”
The next contribution to the theory of orogeny was a series of papers
published in 1873 by Dana, entitled “On some results of the earth’s
contraction from cooling, including a discussion on the origin of mountains
and the nature of the earth’s interior.”[88] This contribution, viewed as a
whole, ranks among the first half dozen papers on the science of mountains.
The following quoted paragraphs give a view of the scope of this article:
ordinary shales of the Pennsylvania Coal formation.
At a depth of 16,000 feet the temperature of the earth’s crust, allowing an increase of 1° F. for 60
feet of descent, would be about 330° F.; or with 1° F. for 50 feet, about 380° F.—either of which
temperatures is far above the boiling point of water; and with the thinner crust of Paleozoic time the
temperature at this depth should have been still higher. But, notwithstanding this heat, and also the
compression from so great an overlying mass, the limestones and shales are not crystalline. The
change of parts of the shale to roofing slate is no evidence in favor of the efficiency of the alleged
cause; for such a cause should act uniformly over great areas.”
The next contribution to the theory of orogeny was a series of papers
published in 1873 by Dana, entitled “On some results of the earth’s
contraction from cooling, including a discussion on the origin of mountains
and the nature of the earth’s interior.”[88] This contribution, viewed as a
whole, ranks among the first half dozen papers on the science of mountains.
The following quoted paragraphs give a view of the scope of this article:
Page 197
“Kinds and Structure of Mountains.”
“While mountains and mountain chains all over the world, and low lands, also, have undergone
uplifts, in the course of their long history, that are not explained on the idea that all mountain
elevating is simply what may come from plication or crushing, the component parts of mountain
chains, or those simple mountains or mountain ranges that are the product of one process of making
—may have received, at the time of their original making, no elevation beyond that resulting from
plication.
This leads us to a grand distinction in orography, hitherto neglected, which is fundamental and of
the highest interest in dynamical geology; a distinction between—
1. A simple or individual mountain mass or range, which is the result of one process of making,
like an individual in any process of evolution, and which may be distinguished as a monogenetic
range, being one in genesis; and
2. A composite or polygenetic range or chain, made up of two or more monogenetic ranges
combined.
The Appalachian chain—the mountain region along the Atlantic border of North America—is a
polygenetic chain; it consists, like the Rocky and other mountain chains, of several monogenetic
ranges, the more important of which are: 1. The Highland range (including the Blue Ridge or parts of
it, and the Adirondacks also, if these belong to the same process of making) pre-Silurian in
formation; 2. The Green Mountain range, in western New England and eastern New York, completed
essentially after the Lower Silurian era or during its closing period; 3. The Alleghany range,
extending from southern New York southwestward to Alabama, and completed immediately after the
Carboniferous age.
The making of the Alleghany range was carried forward at first through a long-continued
subsidence—a geosynclinal (not a true synclinal, since the rocks of the bending crust may have had
in them many true or simple synclinals as well as anticlinals), and a consequent accumulation of
sediments, which occupied the whole of Paleozoic time; and it was completed, finally, in great
breakings, faultings and foldings or plications of the strata, along with other results of disturbance.
These examples exhibit the characteristics of a large class of mountain masses or ranges. A
geosynclinal accompanied by sedimentary depositions, and ending in a catastrophe of plications and
solidification, are the essential steps, while metamorphism and igneous ejections are incidental
results. The process is one that produces final stability in the mass and its annexation generally to the
more stable part of the continent, though not stable against future oscillations of level of wider range,
nor against denudation.
It is apparent that in such a process of formation elevation by direct uplift of the underlying crust
has no necessary place. The attending plications may make elevations on a vast scale and so also may
the shoves upward along the lines of fracture, and crushing may sometimes add to the effect; but
elevation from an upward movement of the downward bent crust is only an incidental concomitant, if
it occur at all.
We perceive thus where the truth lies in Professor Le Conte’s important principle. It should have in
view alone monogenetic mountains and these only at the time of their making. It will then read,
plication and shovings along fractures being made more prominent than crushing:
Plication, shoving along fractures and crushing are the true sources of the elevation that takes place
during the making of geosynclinal monogenetic mountains.
“While mountains and mountain chains all over the world, and low lands, also, have undergone
uplifts, in the course of their long history, that are not explained on the idea that all mountain
elevating is simply what may come from plication or crushing, the component parts of mountain
chains, or those simple mountains or mountain ranges that are the product of one process of making
—may have received, at the time of their original making, no elevation beyond that resulting from
plication.
This leads us to a grand distinction in orography, hitherto neglected, which is fundamental and of
the highest interest in dynamical geology; a distinction between—
1. A simple or individual mountain mass or range, which is the result of one process of making,
like an individual in any process of evolution, and which may be distinguished as a monogenetic
range, being one in genesis; and
2. A composite or polygenetic range or chain, made up of two or more monogenetic ranges
combined.
The Appalachian chain—the mountain region along the Atlantic border of North America—is a
polygenetic chain; it consists, like the Rocky and other mountain chains, of several monogenetic
ranges, the more important of which are: 1. The Highland range (including the Blue Ridge or parts of
it, and the Adirondacks also, if these belong to the same process of making) pre-Silurian in
formation; 2. The Green Mountain range, in western New England and eastern New York, completed
essentially after the Lower Silurian era or during its closing period; 3. The Alleghany range,
extending from southern New York southwestward to Alabama, and completed immediately after the
Carboniferous age.
The making of the Alleghany range was carried forward at first through a long-continued
subsidence—a geosynclinal (not a true synclinal, since the rocks of the bending crust may have had
in them many true or simple synclinals as well as anticlinals), and a consequent accumulation of
sediments, which occupied the whole of Paleozoic time; and it was completed, finally, in great
breakings, faultings and foldings or plications of the strata, along with other results of disturbance.
These examples exhibit the characteristics of a large class of mountain masses or ranges. A
geosynclinal accompanied by sedimentary depositions, and ending in a catastrophe of plications and
solidification, are the essential steps, while metamorphism and igneous ejections are incidental
results. The process is one that produces final stability in the mass and its annexation generally to the
more stable part of the continent, though not stable against future oscillations of level of wider range,
nor against denudation.
It is apparent that in such a process of formation elevation by direct uplift of the underlying crust
has no necessary place. The attending plications may make elevations on a vast scale and so also may
the shoves upward along the lines of fracture, and crushing may sometimes add to the effect; but
elevation from an upward movement of the downward bent crust is only an incidental concomitant, if
it occur at all.
We perceive thus where the truth lies in Professor Le Conte’s important principle. It should have in
view alone monogenetic mountains and these only at the time of their making. It will then read,
plication and shovings along fractures being made more prominent than crushing:
Plication, shoving along fractures and crushing are the true sources of the elevation that takes place
during the making of geosynclinal monogenetic mountains.
Page 198
And the statement of Professor Hall may be made right if we recognize the same distinction, and,
also, reverse the order and causal relation of the two events, accumulation and subsidence; and so
make it read:
Regions of monogenetic mountains were, previous, and preparatory, to the making of the
mountains, areas each of a slowly progressing geosynclinal, and, consequently, of thick
accumulations of sediments.
The prominence and importance in orography of the mountain individualities described above as
originating through a geosynclinal make it desirable that they should have a distinctive name; and I
therefore propose to call a mountain range of this kind a synclinorium, from synclinal and the Greek
ὄρος, mountain.
This brings us to another important distinction in orographic geology—that of a second kind of
monogenetic mountain. The synclinoria were made through a progressing geosynclinal. Those of the
second kind, here referred to, were produced by a progressing geanticlinal. They are simply the
upward bendings in the oscillations of the earth’s crust—the geanticlinal waves, and hardly require a
special name. Yet, if one is desired, the term anticlinorium, the correlate of synclinorium, would be
appropriate. Many of them have disappeared in the course of the oscillations; and yet, some may
have been for a time—perhaps millions of years—respectable mountains.
The geosynclinal ranges or synclinoria have experienced in almost all cases, since their
completion, true elevation through great geanticlinal movements, but movements that embraced a
wider range of crust than that concerned in the preceding geosynclinal movements, indeed a range of
crust that comes strictly under the designation of a polygenetic mass.”
also, reverse the order and causal relation of the two events, accumulation and subsidence; and so
make it read:
Regions of monogenetic mountains were, previous, and preparatory, to the making of the
mountains, areas each of a slowly progressing geosynclinal, and, consequently, of thick
accumulations of sediments.
The prominence and importance in orography of the mountain individualities described above as
originating through a geosynclinal make it desirable that they should have a distinctive name; and I
therefore propose to call a mountain range of this kind a synclinorium, from synclinal and the Greek
ὄρος, mountain.
This brings us to another important distinction in orographic geology—that of a second kind of
monogenetic mountain. The synclinoria were made through a progressing geosynclinal. Those of the
second kind, here referred to, were produced by a progressing geanticlinal. They are simply the
upward bendings in the oscillations of the earth’s crust—the geanticlinal waves, and hardly require a
special name. Yet, if one is desired, the term anticlinorium, the correlate of synclinorium, would be
appropriate. Many of them have disappeared in the course of the oscillations; and yet, some may
have been for a time—perhaps millions of years—respectable mountains.
The geosynclinal ranges or synclinoria have experienced in almost all cases, since their
completion, true elevation through great geanticlinal movements, but movements that embraced a
wider range of crust than that concerned in the preceding geosynclinal movements, indeed a range of
crust that comes strictly under the designation of a polygenetic mass.”
Page 199
“The Condition of the Earth’s Interior.”
“The condition of the earth’s interior is not among the geological results of contraction from
cooling. But these results offer an argument of great weight respecting the earth’s interior condition,
and make it desirable that the subject should be discussed in this connection. Moreover, the facts
throw additional light on the preceding topic—the origin of mountains.
It seems now to be demonstrated by astronomical and physical arguments—arguments that are
independent, it should be noted, of direct geological observation—that the interior of our globe is
essentially solid. But the great oscillations of the earth’s surface, which have seemed to demand for
explanation a liquid interior, still remain facts, and present apparently a greater difficulty than ever to
the geologist. Professor Le Conte’s views, in volume iv, were offered by him as a method of meeting
this difficulty; yet, as he admits in his concluding remarks, the oscillations over the interior of a
continent, and the fact of the greater movements on the borders of the larger ocean, were left by him
unexplained. Yet these oscillations are not more real than the changes of level or greater oscillations
which occurred along the sea border, where mountains were the final result; and this being a
demonstrated truth, no less than the general solidity of the earth’s interior, the question comes up,
how are the two truths compatible?
The geological argument on the subject (the only one within our present purpose) has often been
presented. But it derives new force and gives clearer revelations when the facts are viewed in the
light of the principles that have been explained in the preceding part of this memoir.
The Appalachian subsidence in the Alleghany region of 35,000 to 40,000 feet, going on through all
the Paleozoic era, was due, as has been shown, to an actual sinking of the earth’s crust through lateral
pressure, and not to local contraction in the strata themselves or the terranes underneath. But such a
subsidence is not possible, unless seven miles—that is, seven miles in maximum depth and over a
hundred in total breadth—unless seven miles of something were removed, in its progress, from the
region beneath.
If the matter beneath was not aërial, then liquid or viscous rock was pushed aside. This being a
fact, it would follow that there existed, underneath a crust of unascertained thickness, a sea or lake of
mobile (viscous or plastic) rock, as large as the sinking region; and also that this great viscous sea
continued in existence through the whole period of subsidence, or, in the case of the Alleghany
region, through all Paleozoic time—an era estimated on a previous page to cover at least thirty-five
millions of years, if time since the Silurian age began embraced fifty millions of years.
The facts thus sustain the statement that lateral pressure produced not only the subsidence of the
Appalachian region through the Paleozoic, but also, cotemporaneously, and as its essential
prerequisite, the rising of a sea-border elevation, or geanticlinal, parallel with it; and that both
movements demanded the existence beneath of a great sea of mobile rock.”
The recognition of regional warping as a major factor in the larger
structure of mountain systems, and the expression of that factor in the terms
geosyncline and geanticline forms a notable advance in geologic thought.
Subsequent folding on a regional scale results in the development of
synclinoria and anticlinoria. Van Hise has given these latter terms wide
“The condition of the earth’s interior is not among the geological results of contraction from
cooling. But these results offer an argument of great weight respecting the earth’s interior condition,
and make it desirable that the subject should be discussed in this connection. Moreover, the facts
throw additional light on the preceding topic—the origin of mountains.
It seems now to be demonstrated by astronomical and physical arguments—arguments that are
independent, it should be noted, of direct geological observation—that the interior of our globe is
essentially solid. But the great oscillations of the earth’s surface, which have seemed to demand for
explanation a liquid interior, still remain facts, and present apparently a greater difficulty than ever to
the geologist. Professor Le Conte’s views, in volume iv, were offered by him as a method of meeting
this difficulty; yet, as he admits in his concluding remarks, the oscillations over the interior of a
continent, and the fact of the greater movements on the borders of the larger ocean, were left by him
unexplained. Yet these oscillations are not more real than the changes of level or greater oscillations
which occurred along the sea border, where mountains were the final result; and this being a
demonstrated truth, no less than the general solidity of the earth’s interior, the question comes up,
how are the two truths compatible?
The geological argument on the subject (the only one within our present purpose) has often been
presented. But it derives new force and gives clearer revelations when the facts are viewed in the
light of the principles that have been explained in the preceding part of this memoir.
The Appalachian subsidence in the Alleghany region of 35,000 to 40,000 feet, going on through all
the Paleozoic era, was due, as has been shown, to an actual sinking of the earth’s crust through lateral
pressure, and not to local contraction in the strata themselves or the terranes underneath. But such a
subsidence is not possible, unless seven miles—that is, seven miles in maximum depth and over a
hundred in total breadth—unless seven miles of something were removed, in its progress, from the
region beneath.
If the matter beneath was not aërial, then liquid or viscous rock was pushed aside. This being a
fact, it would follow that there existed, underneath a crust of unascertained thickness, a sea or lake of
mobile (viscous or plastic) rock, as large as the sinking region; and also that this great viscous sea
continued in existence through the whole period of subsidence, or, in the case of the Alleghany
region, through all Paleozoic time—an era estimated on a previous page to cover at least thirty-five
millions of years, if time since the Silurian age began embraced fifty millions of years.
The facts thus sustain the statement that lateral pressure produced not only the subsidence of the
Appalachian region through the Paleozoic, but also, cotemporaneously, and as its essential
prerequisite, the rising of a sea-border elevation, or geanticlinal, parallel with it; and that both
movements demanded the existence beneath of a great sea of mobile rock.”
The recognition of regional warping as a major factor in the larger
structure of mountain systems, and the expression of that factor in the terms
geosyncline and geanticline forms a notable advance in geologic thought.
Subsequent folding on a regional scale results in the development of
synclinoria and anticlinoria. Van Hise has given these latter terms wide
Page 200
currency, but apparently inadvertently has used synclinorium in a different
sense than that in which Dana defined it. Dana gave the word to a mountain
range made by the mashing and uplift of a geosyncline, Van Hise defines it
as a downfold of a large order of magnitude, embracing anticlines and
synclines within it; anticlinorium he uses for a corresponding up fold.[89]
Rice has called attention to this change of definition,[90] but Van Hise’s
usage is likely to prevail, since they are needed terms for the larger
mountain structure and do not require a determination of the previous limits
of upwarp and downwarp,—of original denudation and deposition.
Furthermore, a geosyncline in mountain folding may have one side uplifted,
the other side depressed and there are reasons for regarding the folds of
Pennsylvania, Dana’s type synclinorium, as representing but the western
and downfolded side of the Paleozoic geosyncline. Under that view the
folded Appalachians of Pennsylvania constitute a synclinorium in both the
sense of Dana and Van Hise.
sense than that in which Dana defined it. Dana gave the word to a mountain
range made by the mashing and uplift of a geosyncline, Van Hise defines it
as a downfold of a large order of magnitude, embracing anticlines and
synclines within it; anticlinorium he uses for a corresponding up fold.[89]
Rice has called attention to this change of definition,[90] but Van Hise’s
usage is likely to prevail, since they are needed terms for the larger
mountain structure and do not require a determination of the previous limits
of upwarp and downwarp,—of original denudation and deposition.
Furthermore, a geosyncline in mountain folding may have one side uplifted,
the other side depressed and there are reasons for regarding the folds of
Pennsylvania, Dana’s type synclinorium, as representing but the western
and downfolded side of the Paleozoic geosyncline. Under that view the
folded Appalachians of Pennsylvania constitute a synclinorium in both the
sense of Dana and Van Hise.
Page 201
The Ultimate Cause of Crustal Compression.
The next important advance in the theory of mountains was made by C.
E. Dutton who in 1874 published in the Journal (8, 113–123) an article
entitled “A criticism upon the contractional hypothesis.” Dutton gives
reasons for holding that the amount of folding and shortening exhibited in
mountain ranges, especially those of Tertiary date, is very much greater in
magnitude and is different in nature and distribution from that which would
be given by the surficial cooling of the globe. The following quotations
cover the principal points in the argument:
“The argument for the contractional hypothesis presupposes that the earth-mass may be considered
as consisting of two portions, a cooled exterior of undetermined (though probably comparatively
small) depth, inclosing a hot nucleus.... The secular loss of heat, it is assumed, would be greater from
the hot nucleus than from the exterior, and the greater consequent contraction of the nucleus would
therefore gradually withdraw the support of the exterior, which would collapse. The resulting strains
upon the exterior would be mainly tangential. Owing to considerable inequalities in the ability of
different portions to resist the strains thus developed, the yielding would take place at the lines, or
regions of least resistance, and the effects of the yielding would be manifested chiefly, or wholly, at
those places, in the form of mountain chains, or belts of table lands, and in the disturbances of
stratification. The primary division of the surface into areas of land and water are attributed to the
assumed smaller conductivity of materials underlying the land, which have been left behind in the
general convergence of the surface toward the center. Regarding these as the main and underlying
premises of the contractional argument, it is considered unnecessary to state the various subsidiary
propositions which have been advanced to explain the determination of this action to particular
phenomena, since the main proposition upon which they are based is considered untenable.
There can be no reasonable doubt that the earth-mass consists of a cooled exterior inclosing a hot
nucleus, and a necessary corollary to this must be secular cooling, probably accompanied by
contraction of the cooling portions. But when we apply the known laws of thermal physics to
ascertain the rate of this cooling, and its distribution through the mass, the objectionable character of
the contractional hypothesis becomes obvious.
That Fourier’s theorem, under the general conditions given, expresses the normal law of cooling, is
admitted by all mathematicians who have examined it. The only ground of controversy must be upon
the values to be assigned to the constants. But there seem to be no values consistent with probability
which can be of help to the contractional hypothesis. The application of the theorem shows that
below 200 or 300 miles the cooling has, up to the present time, been extremely little.... At present,
however, the unavoidable deduction from this theorem is that the greatest possible contraction due to
secular cooling is insufficient in amount to account for the phenomena attributed to it by the
contractional hypothesis.
The determination of plications to particular localities presents difficulties in the way of the
contractional hypothesis which have been underrated. It has been assumed that if a contraction of the
interior were to occur, the yielding of the outer crust would take place at localities of least resistance.
But this could be true only on the assumption that the crust could have a horizontal movement in
The next important advance in the theory of mountains was made by C.
E. Dutton who in 1874 published in the Journal (8, 113–123) an article
entitled “A criticism upon the contractional hypothesis.” Dutton gives
reasons for holding that the amount of folding and shortening exhibited in
mountain ranges, especially those of Tertiary date, is very much greater in
magnitude and is different in nature and distribution from that which would
be given by the surficial cooling of the globe. The following quotations
cover the principal points in the argument:
“The argument for the contractional hypothesis presupposes that the earth-mass may be considered
as consisting of two portions, a cooled exterior of undetermined (though probably comparatively
small) depth, inclosing a hot nucleus.... The secular loss of heat, it is assumed, would be greater from
the hot nucleus than from the exterior, and the greater consequent contraction of the nucleus would
therefore gradually withdraw the support of the exterior, which would collapse. The resulting strains
upon the exterior would be mainly tangential. Owing to considerable inequalities in the ability of
different portions to resist the strains thus developed, the yielding would take place at the lines, or
regions of least resistance, and the effects of the yielding would be manifested chiefly, or wholly, at
those places, in the form of mountain chains, or belts of table lands, and in the disturbances of
stratification. The primary division of the surface into areas of land and water are attributed to the
assumed smaller conductivity of materials underlying the land, which have been left behind in the
general convergence of the surface toward the center. Regarding these as the main and underlying
premises of the contractional argument, it is considered unnecessary to state the various subsidiary
propositions which have been advanced to explain the determination of this action to particular
phenomena, since the main proposition upon which they are based is considered untenable.
There can be no reasonable doubt that the earth-mass consists of a cooled exterior inclosing a hot
nucleus, and a necessary corollary to this must be secular cooling, probably accompanied by
contraction of the cooling portions. But when we apply the known laws of thermal physics to
ascertain the rate of this cooling, and its distribution through the mass, the objectionable character of
the contractional hypothesis becomes obvious.
That Fourier’s theorem, under the general conditions given, expresses the normal law of cooling, is
admitted by all mathematicians who have examined it. The only ground of controversy must be upon
the values to be assigned to the constants. But there seem to be no values consistent with probability
which can be of help to the contractional hypothesis. The application of the theorem shows that
below 200 or 300 miles the cooling has, up to the present time, been extremely little.... At present,
however, the unavoidable deduction from this theorem is that the greatest possible contraction due to
secular cooling is insufficient in amount to account for the phenomena attributed to it by the
contractional hypothesis.
The determination of plications to particular localities presents difficulties in the way of the
contractional hypothesis which have been underrated. It has been assumed that if a contraction of the
interior were to occur, the yielding of the outer crust would take place at localities of least resistance.
But this could be true only on the assumption that the crust could have a horizontal movement in
Page 202
which the nucleus does not necessarily share. A vertical section through the Appalachian region and
westward to the 100th meridian shows a surface highly disturbed for about two hundred and fifty
miles, and comparatively undisturbed for more than a thousand. No one would seriously argue that
the contraction of the nucleus had been confined to portions underlying the disturbed regions: yet if
the contraction was general, there must have been a large amount of slip of some portion of the
undisturbed segment over the nucleus. Such a proposition would be very difficult to defend, even if
the premises were granted. It seems as if the friction and adhesion of the crust upon the nucleus had
been overlooked. Nor could this be small, even though the crust rested upon liquid lava. The attempts
which some eminent geologists have recently made to explain surface corrugation by this method
clearly show a neglect on their part to analyze carefully the system of forces which a contraction of
the nucleus would generate in the crust. Their discussions have been argumentative and not
analytical. The latter method of examination would have shown them certain difficulties
irreconcilable with their knowledge of facts. Adopting the argumentative mode, and in conformity
with their view regarding the exterior as a shell of insufficient coherence to sustain itself when its
support is sensibly diminished, the tendency of corrugation to occur mainly along certain belts, with
series of parallel folds, is not explained by assuming that these localities are regions of weakness. For
a shrinkage of the nucleus would throw each elementary portion of the crust into a state of strain by
the action of forces in all directions within its own tangent plane. A relief by a horizontal yielding in
one direction would by no means be a general relief.”
Dutton’s criticisms robbed the current hypothesis of mountain-making of
its conventional basis without providing a new foundation. It was a quarter
of a century in advance of its time, has been seldom cited, and seems to
have had but little direct influence in shaping subsequent thought. It,
however, gave direction to Dutton’s views, and his later papers were far-
reaching in their influence.
If contraction from external cooling is not the cause of the compressive
forces it is necessary to seek another cause. Two years later, in 1876, Dutton
attempted to provide an answer to this open question.[91] A review of this
paper, evidently by J. D. Dana, is given in the Journal. The following
explanations of Dutton’s theory and of Dana’s comments upon it are
contained in a few paragraphs from this review (12, 142, 1876).
“Captain Dutton presents in this paper the views brought out in his article in volume viii of this
Journal, with fuller illustrations, and adds explanations of his theory of the origin of mountains. The
discussion should be read by all desiring to reach right conclusions, it presenting many arguments
from physical considerations against the contraction-theory, or that of the uplifting and folding of
strata through lateral pressure. There is much to be learned before any theory of mountain-making
shall have a sufficient foundation in observed facts to demand full confidence, and Captain Dutton
merits the thanks of geologists for the aid he has given them toward reaching right conclusions. His
discussions are not free from misunderstandings of geological facts, and if they fail to be finally
received it will be for this reason.
westward to the 100th meridian shows a surface highly disturbed for about two hundred and fifty
miles, and comparatively undisturbed for more than a thousand. No one would seriously argue that
the contraction of the nucleus had been confined to portions underlying the disturbed regions: yet if
the contraction was general, there must have been a large amount of slip of some portion of the
undisturbed segment over the nucleus. Such a proposition would be very difficult to defend, even if
the premises were granted. It seems as if the friction and adhesion of the crust upon the nucleus had
been overlooked. Nor could this be small, even though the crust rested upon liquid lava. The attempts
which some eminent geologists have recently made to explain surface corrugation by this method
clearly show a neglect on their part to analyze carefully the system of forces which a contraction of
the nucleus would generate in the crust. Their discussions have been argumentative and not
analytical. The latter method of examination would have shown them certain difficulties
irreconcilable with their knowledge of facts. Adopting the argumentative mode, and in conformity
with their view regarding the exterior as a shell of insufficient coherence to sustain itself when its
support is sensibly diminished, the tendency of corrugation to occur mainly along certain belts, with
series of parallel folds, is not explained by assuming that these localities are regions of weakness. For
a shrinkage of the nucleus would throw each elementary portion of the crust into a state of strain by
the action of forces in all directions within its own tangent plane. A relief by a horizontal yielding in
one direction would by no means be a general relief.”
Dutton’s criticisms robbed the current hypothesis of mountain-making of
its conventional basis without providing a new foundation. It was a quarter
of a century in advance of its time, has been seldom cited, and seems to
have had but little direct influence in shaping subsequent thought. It,
however, gave direction to Dutton’s views, and his later papers were far-
reaching in their influence.
If contraction from external cooling is not the cause of the compressive
forces it is necessary to seek another cause. Two years later, in 1876, Dutton
attempted to provide an answer to this open question.[91] A review of this
paper, evidently by J. D. Dana, is given in the Journal. The following
explanations of Dutton’s theory and of Dana’s comments upon it are
contained in a few paragraphs from this review (12, 142, 1876).
“Captain Dutton presents in this paper the views brought out in his article in volume viii of this
Journal, with fuller illustrations, and adds explanations of his theory of the origin of mountains. The
discussion should be read by all desiring to reach right conclusions, it presenting many arguments
from physical considerations against the contraction-theory, or that of the uplifting and folding of
strata through lateral pressure. There is much to be learned before any theory of mountain-making
shall have a sufficient foundation in observed facts to demand full confidence, and Captain Dutton
merits the thanks of geologists for the aid he has given them toward reaching right conclusions. His
discussions are not free from misunderstandings of geological facts, and if they fail to be finally
received it will be for this reason.
Page 203
We here give in a brief form, and nearly in his own words, the principal points in his theory of
mountain-making as explained in the later part of his memoir.
Accepting the proposition that there is a plastic condition of rock beneath the earth’s crust and that
metamorphism is a ‘hydrothermal process,’ and believing that ‘the penetration of water to profound
depths [in the earth’s crust] is a well sustained theory,’ he says that great pressure and a temperature
approaching redness are essential conditions of metamorphism.... ‘The heaviest portion would sink
into the lighter colloid mass underneath, protruding it laterally beneath the lighter portions where, by
its lighter density, it tends to accumulate.’ He adds: ‘The resulting movements would be determined,
first, by the amount of difference in the densities of the upper and lower masses, and, second, by
inequalities in the thickness of the strata: the forces now become adequate to the building of
mountains and the plication of strata, and their modes of operation agree with the classes of facts
already set forth as the concomitants of those features.’
The views are next applied to a system of plications. ‘It has been indicated that plications occur
where strata have rapidly accumulated in great volume and in elongated narrow belts; that the axes of
plications are parallel to the axes of maximum deposit; and that the movements immediately
followed the deposition’—the case of the Appalachians being an example in which the accumulations
averaged 40,000 feet. He observes: ‘Wherever the load of sediments becomes heaviest, there they
sink deepest, protruding the colloid magma beneath them to the adjoining areas, which are less
heavily weighted, forming at once both synclinals and anticlinals.’
With regard to this new theory, we might reasonably question the existence of the colloid magma
—a condition fundamental to the theory—and his evidence that water penetrates to profound depths
in the earth’s crust sufficient to make hydrous rocks. We might ask for evidence that the rocks
beneath the Cretaceous and Tertiary, and other underlying strata of the Uintahs, were in such a
colloid state, and this so near the surface, that the ‘beds subsided by their gross weight as rapidly as
they grew.’
Again, he says that the movements of mountain-making ‘immediately followed the deposition.’
‘Immediately’ sounds quick to one who appreciates the slowness of geological changes. The
Carboniferous age was very long; and somewhere in that part of geological time, either before the
age had fully ended, or some time after its close, the epoch of catastrophe began.”
We see foreshadowed in this paper the theory of isostasy, or condition of
vertical equilibrium in the crust which Dutton published in 1889. This
theory has borne remarkable fruit, but Dutton attempted to link to it the
horizontally compressive forces which have produced folding and
overthrusting. Willis in 1907[92] and Hayford in 1911, overlooking Dana’s
objections, have attempted to make a lateral isostatic undertow the cause of
all horizontal movements in the crust, adopting the mechanism of Dutton.
The present writer, although accepting the principle of isostasy as an
explanation of broad vertical movements, has published papers which go to
show the inadequacy of this hypothesis of lateral pressure; inadequate in
time relation, in amount, and in expression.[93]
In 1903 it was determined by several physicists that the materials of the
earth’s crust were radioactive and must generate throughout geologic time a
mountain-making as explained in the later part of his memoir.
Accepting the proposition that there is a plastic condition of rock beneath the earth’s crust and that
metamorphism is a ‘hydrothermal process,’ and believing that ‘the penetration of water to profound
depths [in the earth’s crust] is a well sustained theory,’ he says that great pressure and a temperature
approaching redness are essential conditions of metamorphism.... ‘The heaviest portion would sink
into the lighter colloid mass underneath, protruding it laterally beneath the lighter portions where, by
its lighter density, it tends to accumulate.’ He adds: ‘The resulting movements would be determined,
first, by the amount of difference in the densities of the upper and lower masses, and, second, by
inequalities in the thickness of the strata: the forces now become adequate to the building of
mountains and the plication of strata, and their modes of operation agree with the classes of facts
already set forth as the concomitants of those features.’
The views are next applied to a system of plications. ‘It has been indicated that plications occur
where strata have rapidly accumulated in great volume and in elongated narrow belts; that the axes of
plications are parallel to the axes of maximum deposit; and that the movements immediately
followed the deposition’—the case of the Appalachians being an example in which the accumulations
averaged 40,000 feet. He observes: ‘Wherever the load of sediments becomes heaviest, there they
sink deepest, protruding the colloid magma beneath them to the adjoining areas, which are less
heavily weighted, forming at once both synclinals and anticlinals.’
With regard to this new theory, we might reasonably question the existence of the colloid magma
—a condition fundamental to the theory—and his evidence that water penetrates to profound depths
in the earth’s crust sufficient to make hydrous rocks. We might ask for evidence that the rocks
beneath the Cretaceous and Tertiary, and other underlying strata of the Uintahs, were in such a
colloid state, and this so near the surface, that the ‘beds subsided by their gross weight as rapidly as
they grew.’
Again, he says that the movements of mountain-making ‘immediately followed the deposition.’
‘Immediately’ sounds quick to one who appreciates the slowness of geological changes. The
Carboniferous age was very long; and somewhere in that part of geological time, either before the
age had fully ended, or some time after its close, the epoch of catastrophe began.”
We see foreshadowed in this paper the theory of isostasy, or condition of
vertical equilibrium in the crust which Dutton published in 1889. This
theory has borne remarkable fruit, but Dutton attempted to link to it the
horizontally compressive forces which have produced folding and
overthrusting. Willis in 1907[92] and Hayford in 1911, overlooking Dana’s
objections, have attempted to make a lateral isostatic undertow the cause of
all horizontal movements in the crust, adopting the mechanism of Dutton.
The present writer, although accepting the principle of isostasy as an
explanation of broad vertical movements, has published papers which go to
show the inadequacy of this hypothesis of lateral pressure; inadequate in
time relation, in amount, and in expression.[93]
In 1903 it was determined by several physicists that the materials of the
earth’s crust were radioactive and must generate throughout geologic time a
Page 204
quantity of heat which perhaps equalled that lost by radiation into space. By
1907 this had become demonstrated. The remarkable conclusion had been
reached that the earth, although losing heat, is not a cooling globe. Dutton’s
contentions against mountain growth through external cooling and
contraction were thus unexpectedly, through a wholly new branch of
knowledge, demonstrated to be true.
Nevertheless, all students of orogeny are agreed that profound
compressive forces have been the chief agents in developing mountain
structures. Chamberlin was the first to arrive at the idea that the shrinkage
may originate in the deeper portions of the earth under the urgency of the
enormous pressures, apparently by giving rise to slow recombinations of
matter into denser forms.[94]
1907 this had become demonstrated. The remarkable conclusion had been
reached that the earth, although losing heat, is not a cooling globe. Dutton’s
contentions against mountain growth through external cooling and
contraction were thus unexpectedly, through a wholly new branch of
knowledge, demonstrated to be true.
Nevertheless, all students of orogeny are agreed that profound
compressive forces have been the chief agents in developing mountain
structures. Chamberlin was the first to arrive at the idea that the shrinkage
may originate in the deeper portions of the earth under the urgency of the
enormous pressures, apparently by giving rise to slow recombinations of
matter into denser forms.[94]
Page 205
The New Era in the Interpretation of Mountain Structures.
In the meantime, between 1874 and 1904, another advance in the
knowledge of mountain structures was taking place in Europe. Suess
studied the distribution of mountain arcs over the earth and dwelt upon the
prevalence of overthrust structures; the backland being thrust toward and
over the foreland, the rise of the mountain arc or geanticline depressing the
foredeep or geosyncline. Bertrand and Lugeon from 1884 to 1900 were
reinterpreting the Alpine structures on this basis. They showed that the
whole mountain system had been overturned and overthrust from the south
to an almost incredible degree. Enormous denudation had later dissevered
the northern outlying portions and given rise to “mountains without
roots,”—isolated outliers, consisting of overturned masses of strata which
had accumulated as sediments far to the southward in another portion of the
ancient geosyncline.
On a smaller scale similar phenomena are exhibited in the Appalachians.
Willis showed that the deep subsidence of the center of the geosyncline
gave an initial dip which determined the position of yielding under
compression. Laboratory experiments brought out the weakness of the
stratigraphic structure to resist horizontal compression. The nature of the
stratigraphic series was shown to determine whether the yielding would be
by mashing, competent folding, or breakage and overthrust. The problem of
mountain structures was thus brought into the realm of mechanics. These
results were published in three sources in 1893,—the Transactions of the
American Institute of Mining Engineers, the thirteenth annual report of the
United States Geological Survey, and the Journal (46, 257, 1893).
Finally should be noted the contributions of the Lake Superior school of
geology, in which the work of Van Hise stands preeminent. Under the
economic stimulus given by the discovery and development of enormously
rich bodies of iron ore, hidden under Pleistocene drift and involved in the
complex structures of vanished mountain systems of ancient date, structural
geology and metamorphism have become exact sciences to be drawn upon
in the search for mineral wealth and yielding also rich returns in a fuller
knowledge of early periods of earth history.
In the meantime, between 1874 and 1904, another advance in the
knowledge of mountain structures was taking place in Europe. Suess
studied the distribution of mountain arcs over the earth and dwelt upon the
prevalence of overthrust structures; the backland being thrust toward and
over the foreland, the rise of the mountain arc or geanticline depressing the
foredeep or geosyncline. Bertrand and Lugeon from 1884 to 1900 were
reinterpreting the Alpine structures on this basis. They showed that the
whole mountain system had been overturned and overthrust from the south
to an almost incredible degree. Enormous denudation had later dissevered
the northern outlying portions and given rise to “mountains without
roots,”—isolated outliers, consisting of overturned masses of strata which
had accumulated as sediments far to the southward in another portion of the
ancient geosyncline.
On a smaller scale similar phenomena are exhibited in the Appalachians.
Willis showed that the deep subsidence of the center of the geosyncline
gave an initial dip which determined the position of yielding under
compression. Laboratory experiments brought out the weakness of the
stratigraphic structure to resist horizontal compression. The nature of the
stratigraphic series was shown to determine whether the yielding would be
by mashing, competent folding, or breakage and overthrust. The problem of
mountain structures was thus brought into the realm of mechanics. These
results were published in three sources in 1893,—the Transactions of the
American Institute of Mining Engineers, the thirteenth annual report of the
United States Geological Survey, and the Journal (46, 257, 1893).
Finally should be noted the contributions of the Lake Superior school of
geology, in which the work of Van Hise stands preeminent. Under the
economic stimulus given by the discovery and development of enormously
rich bodies of iron ore, hidden under Pleistocene drift and involved in the
complex structures of vanished mountain systems of ancient date, structural
geology and metamorphism have become exact sciences to be drawn upon
in the search for mineral wealth and yielding also rich returns in a fuller
knowledge of early periods of earth history.
Page 206
Crust Movements as Revealed by Physiography.
During the last quarter of the nineteenth century another division of
geology, dominantly American, was taking form and growth,—the science
of land forms,—physiography. The history of that development is treated by
Gregory in the preceding chapter but some of its bearings upon theory, in so
far as they affect the subject of mountain origin, are necessarily given here.
Powell, Dutton, and Gilbert in their explorations of the West saw the
stupendous work of denudation which had been carried to completion again
and again during the progress of geologic time. The mountain relief
consequently may be much younger than the folding of the rocks, and may
be largely or even wholly due to recurrent plateau movement, a doctrine to
which Dana had previously arrived. But the introduction of the idea of the
peneplain opened up a new field for exploration in the nature and date of
crust movements. Davis by this means began to study the later chapters of
Appalachian history, the most important early paper being published in
1891.[95] Since then Davis, Willis, and many others have found that, girdling
the world, a large part of the mountainous relief is due to vertical elevatory
forces acting over regions of previous folding and overthrust. In addition,
great plateau areas of unfolded rocks have been bodily lifted one to two
miles, or more, above their earlier levels. They may be broad geanticlinal
arches or bounded by the walls of profound fractures.
The linear mountain systems made from deep troughs of sediments have
come then to be recognized as but one of several classes of mountains. This
class, from its clear development in the Appalachians, and the fact that
many of the laws of mountain structure pertaining to it were first worked
out there, has been called by Powell the Appalachian type (12, 414, 1876).
A classification of mountain systems was proposed by him in which
mountains are classified into two major divisions, those composed of
sedimentary strata altered or unaltered, and those composed in whole or in
part of extravasated material. The first class he subdivides into six sub-
classes of which the folded Appalachians illustrate one. It appears to the
writer that Powell’s classification gives disproportionate importance to
certain types which he described; but nevertheless, the fact that such a
During the last quarter of the nineteenth century another division of
geology, dominantly American, was taking form and growth,—the science
of land forms,—physiography. The history of that development is treated by
Gregory in the preceding chapter but some of its bearings upon theory, in so
far as they affect the subject of mountain origin, are necessarily given here.
Powell, Dutton, and Gilbert in their explorations of the West saw the
stupendous work of denudation which had been carried to completion again
and again during the progress of geologic time. The mountain relief
consequently may be much younger than the folding of the rocks, and may
be largely or even wholly due to recurrent plateau movement, a doctrine to
which Dana had previously arrived. But the introduction of the idea of the
peneplain opened up a new field for exploration in the nature and date of
crust movements. Davis by this means began to study the later chapters of
Appalachian history, the most important early paper being published in
1891.[95] Since then Davis, Willis, and many others have found that, girdling
the world, a large part of the mountainous relief is due to vertical elevatory
forces acting over regions of previous folding and overthrust. In addition,
great plateau areas of unfolded rocks have been bodily lifted one to two
miles, or more, above their earlier levels. They may be broad geanticlinal
arches or bounded by the walls of profound fractures.
The linear mountain systems made from deep troughs of sediments have
come then to be recognized as but one of several classes of mountains. This
class, from its clear development in the Appalachians, and the fact that
many of the laws of mountain structure pertaining to it were first worked
out there, has been called by Powell the Appalachian type (12, 414, 1876).
A classification of mountain systems was proposed by him in which
mountains are classified into two major divisions, those composed of
sedimentary strata altered or unaltered, and those composed in whole or in
part of extravasated material. The first class he subdivides into six sub-
classes of which the folded Appalachians illustrate one. It appears to the
writer that Powell’s classification gives disproportionate importance to
certain types which he described; but nevertheless, the fact that such a
Page 207
classification was made, indicates the growth of a more comprehensive
knowledge of mountains,—their origin, structure, and history.
knowledge of mountains,—their origin, structure, and history.
Page 208
Relations of Crust Movements to Density and Equilibrium.
A recent important development in the fields of geophysics and major
crust movements consists in the incorporation into geology of the doctrine
of isostasy. The evidence was developed in the middle of the nineteenth
century by the geodetic survey of India which indicated that the Himalayas
did not exert the gravitative influence that their volume called for. It was
clear that the crust beneath that mountain system was less dense than
beneath the plains of India and still less dense than the crust beneath the
Indian Ocean. This relation between density and elevation indicated some
approach to flotational equilibrium in the crust, comparable in its nature
though not in delicacy of adjustment to the elevation of the surface of an
iceberg above the ocean level owing to its depth and its density, less than
that of the surrounding medium. This important geological conception was
kept within the confines of astronomy and geodesy, however, until Dutton
in 1876, but especially in 1889, brought it into the geologic field. A test of
isostasy was made for the United States by Putnam and Gilbert in 1895 and
much more elaborate investigations have since been made by Hayford and
Bowie. These investigations demonstrate the importance and reality of
broad warping forces acting vertically and related to the regional variations
of density in the crust.
There are consequently two major and unrelated classes of forces
involved in the making of mountain structures,—the irresistible horizontal
compressive forces, arising apparently from condensation deep within the
earth, and vertical forces originating in the outer envelopes and tending
toward a hydrostatic equilibrium. In this latter field of investigation,
America, since the initial paper by Dutton, has taken the lead.
A recent important development in the fields of geophysics and major
crust movements consists in the incorporation into geology of the doctrine
of isostasy. The evidence was developed in the middle of the nineteenth
century by the geodetic survey of India which indicated that the Himalayas
did not exert the gravitative influence that their volume called for. It was
clear that the crust beneath that mountain system was less dense than
beneath the plains of India and still less dense than the crust beneath the
Indian Ocean. This relation between density and elevation indicated some
approach to flotational equilibrium in the crust, comparable in its nature
though not in delicacy of adjustment to the elevation of the surface of an
iceberg above the ocean level owing to its depth and its density, less than
that of the surrounding medium. This important geological conception was
kept within the confines of astronomy and geodesy, however, until Dutton
in 1876, but especially in 1889, brought it into the geologic field. A test of
isostasy was made for the United States by Putnam and Gilbert in 1895 and
much more elaborate investigations have since been made by Hayford and
Bowie. These investigations demonstrate the importance and reality of
broad warping forces acting vertically and related to the regional variations
of density in the crust.
There are consequently two major and unrelated classes of forces
involved in the making of mountain structures,—the irresistible horizontal
compressive forces, arising apparently from condensation deep within the
earth, and vertical forces originating in the outer envelopes and tending
toward a hydrostatic equilibrium. In this latter field of investigation,
America, since the initial paper by Dutton, has taken the lead.
Page 209
Conclusion on Contributions of America to Theories of Orogeny.
The sciences arose in Europe, but those which treated of the earth were
still in their infancy when transplanted to America. The first comprehensive
ideas on the nature of mountain structures arose in Great Britain and
France. These ideas served as a guide and stimulus to observation in the
recognition of deformations in the strata of the Appalachian system. Since
1840, however, America has ceased to be a pupil in this field of research but
has joined as an equal with the two older countries. New ideas have been
contributed, new and striking illustrations cited, first by the scientists of one
nation, next by those of another. The composite mass of knowledge has
grown as a common possession. Nevertheless, a review of the progress
since 1840 as measured by the contribution of new ideas shows on the
whole America at least equal to its intellectual rivals, and at certain times
actually the leader. This is true of the science of geology as a whole and
also of the subdivision of orogeny.
Thus far no mention has been made of German geologists, with the
exception of Suess, an Austrian. German geology is voluminous and the
names of many well-known geologists could be cited. But this article has
sought to trace the origin and growth of fundamental ideas. The Germans
have been assiduous observers of detail; preeminent as systematizers and
classifiers, seldom originators. Even petrology, which might be regarded as
their especial field, was transplanted from Great Britain. In the science of
mountains they have followed in their fundamental ideas especially the
French.
Turning to the mediums of publication through which this progress of
knowledge in earth structures has been recorded, the American Journal of
Science stands foremost as the only continuous record for the whole century
in American literature, fulfilling for this country what the Quarterly Journal
of the Geological Society has done for Great Britain since 1845, and the
Bulletin de la Société Géologique for France since 1830.
The sciences arose in Europe, but those which treated of the earth were
still in their infancy when transplanted to America. The first comprehensive
ideas on the nature of mountain structures arose in Great Britain and
France. These ideas served as a guide and stimulus to observation in the
recognition of deformations in the strata of the Appalachian system. Since
1840, however, America has ceased to be a pupil in this field of research but
has joined as an equal with the two older countries. New ideas have been
contributed, new and striking illustrations cited, first by the scientists of one
nation, next by those of another. The composite mass of knowledge has
grown as a common possession. Nevertheless, a review of the progress
since 1840 as measured by the contribution of new ideas shows on the
whole America at least equal to its intellectual rivals, and at certain times
actually the leader. This is true of the science of geology as a whole and
also of the subdivision of orogeny.
Thus far no mention has been made of German geologists, with the
exception of Suess, an Austrian. German geology is voluminous and the
names of many well-known geologists could be cited. But this article has
sought to trace the origin and growth of fundamental ideas. The Germans
have been assiduous observers of detail; preeminent as systematizers and
classifiers, seldom originators. Even petrology, which might be regarded as
their especial field, was transplanted from Great Britain. In the science of
mountains they have followed in their fundamental ideas especially the
French.
Turning to the mediums of publication through which this progress of
knowledge in earth structures has been recorded, the American Journal of
Science stands foremost as the only continuous record for the whole century
in American literature, fulfilling for this country what the Quarterly Journal
of the Geological Society has done for Great Britain since 1845, and the
Bulletin de la Société Géologique for France since 1830.
Page 210
Notes.
78. H. D. Rogers, Geology of New Jersey, Final Report, p. 115, 1840.
79. H. D. Rogers, Geology of Pennsylvania, vol. 2, pt. II, pp. 761, 762, 1858.
80. Connecticut Academy of Arts and Sciences, 1810; quoted by G. P. Merrill in Contributions
to the History of North American geology, Ann. Rpt. Smithsonian Institution for 1904, p. 216.
81. A Sketch of the geology, mineralogy, and scenery of the regions contiguous to the river
Connecticut; with a geological map and drawings of organic remains; and occasional botanical
notices, the Journal, 6, 1–86, 201–236, 1823; 7, 1–30, 1824.
82. Clarence King, U. S. Geol. Exploration of the Fortieth Parallel, vol. 1, pp. 16, 44–48, 1878.
83. Illustrations of the Huttonian Theory of the Earth, pp. 219–238, 1802.
84. Robert Jameson, Elements of Geognosy, pp. 55–57, 1808.
85. G. P. Merrill, Contributions to the History of American Geology. Report of the U. S.
National Museum for 1904, p. 328.
86. H. D. Rogers, Geology of Pennsylvania, vol. 2, p. 916, 1858.
87. James Hall, Natural History of New York, Paleontology, vol. 3, pp. 51–73, 1859.
88. The Journal, 5, 423–443, 474, 475; 6, 6–14, 104–115, 161–172, 304, 381, 382, 1873.
89. C. R. Van Hise, Principles of North American Pre-Cambrian Geology, U. S. Geol. Surv.,
16th Ann. Report, pt. I, pp. 607–612, 1896.
90. W. N. Rice, On the use of the words synclinorium and anticlinorium, Science, 23, 286, 287,
1906.
91. C. E. Dutton, Critical observations on theories of the earth’s physical evolution, The Penn
Monthly, May and June, 1876.
92. B. Willis, Research in China, vol. 2, 1907.
93. Joseph Barrell, Science, 39, 259, 260, 1909; Jour. Geol., 22, 672–683, 1914.
94. T. C. Chamberlin, Geology, vol. 1, pp. 541, 542, 1904.
95. W. M. Davis, The geological dates of origin of certain topographic forms on the Atlantic
slope of the United States, Geol. Soc. Am. Bull., 2, 541–542, 545–586, 1891.
78. H. D. Rogers, Geology of New Jersey, Final Report, p. 115, 1840.
79. H. D. Rogers, Geology of Pennsylvania, vol. 2, pt. II, pp. 761, 762, 1858.
80. Connecticut Academy of Arts and Sciences, 1810; quoted by G. P. Merrill in Contributions
to the History of North American geology, Ann. Rpt. Smithsonian Institution for 1904, p. 216.
81. A Sketch of the geology, mineralogy, and scenery of the regions contiguous to the river
Connecticut; with a geological map and drawings of organic remains; and occasional botanical
notices, the Journal, 6, 1–86, 201–236, 1823; 7, 1–30, 1824.
82. Clarence King, U. S. Geol. Exploration of the Fortieth Parallel, vol. 1, pp. 16, 44–48, 1878.
83. Illustrations of the Huttonian Theory of the Earth, pp. 219–238, 1802.
84. Robert Jameson, Elements of Geognosy, pp. 55–57, 1808.
85. G. P. Merrill, Contributions to the History of American Geology. Report of the U. S.
National Museum for 1904, p. 328.
86. H. D. Rogers, Geology of Pennsylvania, vol. 2, p. 916, 1858.
87. James Hall, Natural History of New York, Paleontology, vol. 3, pp. 51–73, 1859.
88. The Journal, 5, 423–443, 474, 475; 6, 6–14, 104–115, 161–172, 304, 381, 382, 1873.
89. C. R. Van Hise, Principles of North American Pre-Cambrian Geology, U. S. Geol. Surv.,
16th Ann. Report, pt. I, pp. 607–612, 1896.
90. W. N. Rice, On the use of the words synclinorium and anticlinorium, Science, 23, 286, 287,
1906.
91. C. E. Dutton, Critical observations on theories of the earth’s physical evolution, The Penn
Monthly, May and June, 1876.
92. B. Willis, Research in China, vol. 2, 1907.
93. Joseph Barrell, Science, 39, 259, 260, 1909; Jour. Geol., 22, 672–683, 1914.
94. T. C. Chamberlin, Geology, vol. 1, pp. 541, 542, 1904.
95. W. M. Davis, The geological dates of origin of certain topographic forms on the Atlantic
slope of the United States, Geol. Soc. Am. Bull., 2, 541–542, 545–586, 1891.
Page 211
V
A CENTURY OF GOVERNMENT GEOLOGICAL SURVEYS
By GEORGE OTIS SMITH
Director of the United States Geological Survey
Even a Federal Bureau must be considered a product of evolution: the past
of the United States Geological Survey far antedates March 3, 1879. The
scope of endeavor, the refinement of method, and especially the personnel
of the newly created service of that day were largely inherited from pioneer
organizations. Therefore a review of the country’s record of surveys under
Government auspices becomes more than a grateful acknowledgment by the
present generation of geologists of the credit due to those who blazed the
way; it shows the sequence and progress in the contributions made by
geologic science to industry.
The earlier stages in industrial evolution mentioned by Hess[96]—
exploitation, development, and maturity—determine a somewhat similar
progressive development in geologic investigation, so that geographic
exploration and geologic reconnaissance of the broadest type are the normal
contribution of exact science whenever and wherever a nation is in the state
of exploitation and initial development of its mineral and agricultural
resources. The refinements of detailed surveys and quantitative
examinations belong rather to the next stage of intensive utilization, or,
indeed, they are the essentials preliminary to full use. Thus regrets that the
results of present-day work were not available fifty years ago are largely
vain: the fathers may not have been without the vision; they simply did the
work as their day and generation needed it done.
A CENTURY OF GOVERNMENT GEOLOGICAL SURVEYS
By GEORGE OTIS SMITH
Director of the United States Geological Survey
Even a Federal Bureau must be considered a product of evolution: the past
of the United States Geological Survey far antedates March 3, 1879. The
scope of endeavor, the refinement of method, and especially the personnel
of the newly created service of that day were largely inherited from pioneer
organizations. Therefore a review of the country’s record of surveys under
Government auspices becomes more than a grateful acknowledgment by the
present generation of geologists of the credit due to those who blazed the
way; it shows the sequence and progress in the contributions made by
geologic science to industry.
The earlier stages in industrial evolution mentioned by Hess[96]—
exploitation, development, and maturity—determine a somewhat similar
progressive development in geologic investigation, so that geographic
exploration and geologic reconnaissance of the broadest type are the normal
contribution of exact science whenever and wherever a nation is in the state
of exploitation and initial development of its mineral and agricultural
resources. The refinements of detailed surveys and quantitative
examinations belong rather to the next stage of intensive utilization, or,
indeed, they are the essentials preliminary to full use. Thus regrets that the
results of present-day work were not available fifty years ago are largely
vain: the fathers may not have been without the vision; they simply did the
work as their day and generation needed it done.
Page 212
Twenty years ago S. F. Emmons, in a presidential address before the
Geological Society of Washington, divided the history of Governmental
surveys in this country into two periods, separated in a general way by the
Civil War. The first of these was the period of geographic exploration, the
second that of geologic exploration. Mr. Emmons of course regarded this
subdivision as not hard and fast, yet his dividing line seems logical, for not
only did the military activities in the East necessarily suspend exploration in
the West, but after the war national, political, and economic considerations
led naturally to the demand for a more exact knowledge of the vast national
domain in the West. Geography and geology are so closely related that Mr.
Emmons’s distinction of the two periods is useful only with the limitations
inferentially set by himself—namely, that while geologic investigation
entered into most of the explorations of the earlier period, the geologist was
regarded as only an accessory in these exploring expeditions; on the other
hand, in the later surveys the topographic work was developed because it
was essential to the geologic investigations.
The year 1818 was a notable one in American geology, first of all in the
appearance of the American Journal of Science, itself so perfect a vehicle
for geological thought that, as is so well stated by Dr. G. P. Merrill, “a
perusal of the numbers from the date of issue down to the present time will
alone afford a fair idea of the gradual progress of American geology.” The
beginning of publications on New England geology appeared that year in
Edward Hitchcock’s first paper on the Connecticut Valley (1, 105, 1818)
and the Danas’ (S. L. and J. F.) detailed geologic and mineralogic
description of Boston and vicinity; and the “Index” of Amos Eaton (noticed
in this Journal, 1, 69) was the first of that long list of notable contributions
to American stratigraphy that are to be credited to the New York geologists.
In the present discussion, too, the year 1918 can be regarded as in a way
the centennial of Government geologic surveys, for it was in 1818 that
Henry R. Schoolcraft began his trip to the Mississippi Valley—perhaps the
first geologic reconnaissance into the West—and it was his work in the lead
region which served to make him a member of the Cass expedition sent out
by the Secretary of War in 1820 to examine the metallic wealth of the Lake
Superior region. The earlier Government explorations of Lewis and Clark,
in 1803–7, and of Pike, in 1805–7, were so exclusively geographic that
geologic work under Federal auspices must be regarded as beginning with
Schoolcraft and with Edwin James, the geologist of the expedition of Major
Geological Society of Washington, divided the history of Governmental
surveys in this country into two periods, separated in a general way by the
Civil War. The first of these was the period of geographic exploration, the
second that of geologic exploration. Mr. Emmons of course regarded this
subdivision as not hard and fast, yet his dividing line seems logical, for not
only did the military activities in the East necessarily suspend exploration in
the West, but after the war national, political, and economic considerations
led naturally to the demand for a more exact knowledge of the vast national
domain in the West. Geography and geology are so closely related that Mr.
Emmons’s distinction of the two periods is useful only with the limitations
inferentially set by himself—namely, that while geologic investigation
entered into most of the explorations of the earlier period, the geologist was
regarded as only an accessory in these exploring expeditions; on the other
hand, in the later surveys the topographic work was developed because it
was essential to the geologic investigations.
The year 1818 was a notable one in American geology, first of all in the
appearance of the American Journal of Science, itself so perfect a vehicle
for geological thought that, as is so well stated by Dr. G. P. Merrill, “a
perusal of the numbers from the date of issue down to the present time will
alone afford a fair idea of the gradual progress of American geology.” The
beginning of publications on New England geology appeared that year in
Edward Hitchcock’s first paper on the Connecticut Valley (1, 105, 1818)
and the Danas’ (S. L. and J. F.) detailed geologic and mineralogic
description of Boston and vicinity; and the “Index” of Amos Eaton (noticed
in this Journal, 1, 69) was the first of that long list of notable contributions
to American stratigraphy that are to be credited to the New York geologists.
In the present discussion, too, the year 1918 can be regarded as in a way
the centennial of Government geologic surveys, for it was in 1818 that
Henry R. Schoolcraft began his trip to the Mississippi Valley—perhaps the
first geologic reconnaissance into the West—and it was his work in the lead
region which served to make him a member of the Cass expedition sent out
by the Secretary of War in 1820 to examine the metallic wealth of the Lake
Superior region. The earlier Government explorations of Lewis and Clark,
in 1803–7, and of Pike, in 1805–7, were so exclusively geographic that
geologic work under Federal auspices must be regarded as beginning with
Schoolcraft and with Edwin James, the geologist of the expedition of Major
Page 213
Long in 1819–20 to the Rocky Mountains. Both these observers published
reports that are valuable as contributions to the knowledge of littleknown
regions.
Any description of geologic work under the Federal Government that
included no reference to the State surveys would be inadequate, for in both
date of execution and stage of development the work of the State geologists
must be given precedence. In Merrill’s Contributions to the History of
American Geology,[97] whose modest title fails even to suggest that this
work not only furnishes the most useful chronologic record of the progress
of the science on the American continent but is in fact a very thesaurus of
incidents touching the personal side of geology, the author by his division
of his subject shows that four decades of the era of State surveys elapsed
before the era of national surveys began.
Thus the geologic surveys of some of the Eastern States antedate by
several decades any Federal organization of comparable geologic scope,
and in investigations directed to local utilitarian problems these pioneer
geologists working in the older settled States of the East were in fact
already conducting work as detailed in type as much of that attempted by
the Federal geologists of the later period. Even to-day it is true in a general
way that the State geologist can and should attack many of his local
problems with intensive methods and with detail of results that are neither
practicable nor desirable for the larger interstate investigations or for
examinations in newer territory. All this relation of State and Federal work
must be looked upon as normal evolutionary development of geologic
science in America.
One who reads the names of the Federal geologists of the early days,
beginning with Jackson and Owen and following with such leaders in
Federal work as Gilbert, Chamberlin, King, R. D. Irving, Pumpelly, Van
Hise, and Walcott, may note that these were all connected in their earlier
work with State surveys. Nor has the relation been one-sided, for among the
State geologists Whitney, Blake, Mather, Newberry, J. G. Norwood, Purdue,
Bain, Gregory, Ashley, Kirk, W. H. Emmons, DeWolf, Mathews, Brown,
Landes, Moore, and Crider received their field training in part or wholly as
members of a Federal Survey. Moreover, under the present plan of effective
cooperation of several of the State surveys with the United States
Geological Survey, it is often difficult to differentiate between the two in
reports that are valuable as contributions to the knowledge of littleknown
regions.
Any description of geologic work under the Federal Government that
included no reference to the State surveys would be inadequate, for in both
date of execution and stage of development the work of the State geologists
must be given precedence. In Merrill’s Contributions to the History of
American Geology,[97] whose modest title fails even to suggest that this
work not only furnishes the most useful chronologic record of the progress
of the science on the American continent but is in fact a very thesaurus of
incidents touching the personal side of geology, the author by his division
of his subject shows that four decades of the era of State surveys elapsed
before the era of national surveys began.
Thus the geologic surveys of some of the Eastern States antedate by
several decades any Federal organization of comparable geologic scope,
and in investigations directed to local utilitarian problems these pioneer
geologists working in the older settled States of the East were in fact
already conducting work as detailed in type as much of that attempted by
the Federal geologists of the later period. Even to-day it is true in a general
way that the State geologist can and should attack many of his local
problems with intensive methods and with detail of results that are neither
practicable nor desirable for the larger interstate investigations or for
examinations in newer territory. All this relation of State and Federal work
must be looked upon as normal evolutionary development of geologic
science in America.
One who reads the names of the Federal geologists of the early days,
beginning with Jackson and Owen and following with such leaders in
Federal work as Gilbert, Chamberlin, King, R. D. Irving, Pumpelly, Van
Hise, and Walcott, may note that these were all connected in their earlier
work with State surveys. Nor has the relation been one-sided, for among the
State geologists Whitney, Blake, Mather, Newberry, J. G. Norwood, Purdue,
Bain, Gregory, Ashley, Kirk, W. H. Emmons, DeWolf, Mathews, Brown,
Landes, Moore, and Crider received their field training in part or wholly as
members of a Federal Survey. Moreover, under the present plan of effective
cooperation of several of the State surveys with the United States
Geological Survey, it is often difficult to differentiate between the two in
Page 214
either personnel or results, for it even happens that the publishing
organization may not have been the major contributor. The full record of
American geology, past and present, can not be set forth in terms of Federal
auspices alone.
The three decades preceding the Civil War, then, constitute the era of
State surveys, well described by Merrill as at first characterized by a
contagious enthusiasm for beginning geologic work, later by a more normal
condition in which every available geologist seems to have been quietly at
work, and finally by renewed activity in creating new organizations. The
net result was that Louisiana and Oregon seem to have been the only States
not having at least one geological survey.
organization may not have been the major contributor. The full record of
American geology, past and present, can not be set forth in terms of Federal
auspices alone.
The three decades preceding the Civil War, then, constitute the era of
State surveys, well described by Merrill as at first characterized by a
contagious enthusiasm for beginning geologic work, later by a more normal
condition in which every available geologist seems to have been quietly at
work, and finally by renewed activity in creating new organizations. The
net result was that Louisiana and Oregon seem to have been the only States
not having at least one geological survey.
Page 215
From “Contributions to the History of American Geology”
by George P. Merrills.
The first specific appropriation by the Federal Government for geologic
investigation appears to have been made in 1834, when a supplemental
appropriation for surveys of roads and canals under the War Department,
authorized in 1824, contained the item “of which sum five thousand dollars
shall be appropriated and applied to geological and mineralogical survey
and researches.” In July, 1834, Mr. G. W. Featherstonhaugh was appointed
United States geologist and employed under Colonel Abert, U. S.
Topographical Engineers, to “personally inspect the mineral and geological
by George P. Merrills.
The first specific appropriation by the Federal Government for geologic
investigation appears to have been made in 1834, when a supplemental
appropriation for surveys of roads and canals under the War Department,
authorized in 1824, contained the item “of which sum five thousand dollars
shall be appropriated and applied to geological and mineralogical survey
and researches.” In July, 1834, Mr. G. W. Featherstonhaugh was appointed
United States geologist and employed under Colonel Abert, U. S.
Topographical Engineers, to “personally inspect the mineral and geological
Page 216
character” of the public lands of the Ozark Mountain region. Overlooking
the incidental fact that this Englishman—a man of scientific attainment and
large interest in public affairs—was never naturalized,[98] it must be placed
to the credit of this first of United States geologists that within seven
months he completed his field work and returned to Washington, and on
February 17, 1835, his report was transmitted to Congress. Two years
earlier Featherstonhaugh had memorialized Congress for aid in the
preparation of a geologic map of the whole territory of the United States,
and in connection with this project he suggested that geology as an aid to
military engineering should have a place in the curriculum at West Point.
This first United States geologist also appears to have combined an
appreciation of the practical worth of “the mineral riches of our country,
their quality, quantity, and the facility of procuring them,” with an interest
in the more scientific side of geology, though his hypotheses regarding both
economic geology and stratigraphic and structural geology have not won
the endorsement of all later workers in the same regions. In all these
respects, however, Featherstonhaugh may stand as a fairly good prototype.
His contributions to international affairs subsequent to his scientific service
to the United States are of interest; he served as one of Her Majesty’s
commissioners in the settlement of the Canadian-United States boundary
question in 1839–40 and made an examination of the disputed area, and
after the settlement of this controversy he was appointed British Consul for
the Department of the Seine, France, where in 1848 he personally
engineered the escape of Louis Philippe from Havre.
The Federal geologic work thus started was soon continued in surveys of
wider scope and more thorough accomplishment. The position of the
Government as the proprietor of mineral lands in the Upper Mississippi
Valley led to their examination. These Government lands containing lead
had been reserved from sale for lease since 1807, although no leases were
issued until 1822. The amount of illegal entry and consequent refusal of
smelters and miners to pay royalty after 1834 forced the issue upon the
attention of Congress, and in 1839 President Van Buren was requested to
present to Congress a plan for the sale of the public mineral lands. In
carrying out this policy Dr. David Dale Owen was selected to make the
necessary survey.
Owen had served as an assistant on the State Survey of Tennessee and as
the first State geologist of Indiana, and he organized the new work promptly
the incidental fact that this Englishman—a man of scientific attainment and
large interest in public affairs—was never naturalized,[98] it must be placed
to the credit of this first of United States geologists that within seven
months he completed his field work and returned to Washington, and on
February 17, 1835, his report was transmitted to Congress. Two years
earlier Featherstonhaugh had memorialized Congress for aid in the
preparation of a geologic map of the whole territory of the United States,
and in connection with this project he suggested that geology as an aid to
military engineering should have a place in the curriculum at West Point.
This first United States geologist also appears to have combined an
appreciation of the practical worth of “the mineral riches of our country,
their quality, quantity, and the facility of procuring them,” with an interest
in the more scientific side of geology, though his hypotheses regarding both
economic geology and stratigraphic and structural geology have not won
the endorsement of all later workers in the same regions. In all these
respects, however, Featherstonhaugh may stand as a fairly good prototype.
His contributions to international affairs subsequent to his scientific service
to the United States are of interest; he served as one of Her Majesty’s
commissioners in the settlement of the Canadian-United States boundary
question in 1839–40 and made an examination of the disputed area, and
after the settlement of this controversy he was appointed British Consul for
the Department of the Seine, France, where in 1848 he personally
engineered the escape of Louis Philippe from Havre.
The Federal geologic work thus started was soon continued in surveys of
wider scope and more thorough accomplishment. The position of the
Government as the proprietor of mineral lands in the Upper Mississippi
Valley led to their examination. These Government lands containing lead
had been reserved from sale for lease since 1807, although no leases were
issued until 1822. The amount of illegal entry and consequent refusal of
smelters and miners to pay royalty after 1834 forced the issue upon the
attention of Congress, and in 1839 President Van Buren was requested to
present to Congress a plan for the sale of the public mineral lands. In
carrying out this policy Dr. David Dale Owen was selected to make the
necessary survey.
Owen had served as an assistant on the State Survey of Tennessee and as
the first State geologist of Indiana, and he organized the new work promptly
Page 217
and effectively. Although suffering from the handicap unfortunately known
by geologists of the present day—the receipt late in the season (August 17,
1839) of authority to begin work—within exactly a month he had his force
of 139 assistants organized into 24 field parties, instructed in “such
elementary principles of geology as were necessary to their performance of
the duties required of them.” His plan of campaign provided for a
northward drive at a predetermined rate of traverse for each party, with
periodic reports to himself at appointed stations, “to receive which reports
and to examine the country in person” he crossed the area under survey
eleven times. The result of such masterful leadership was the completion of
the exploration of all the lands comprehended in his orders in two months
and six days, and his report on this great area—about 11,000 square miles—
bears date of April 2, 1840.
Eight years later Doctor Owen made a survey of an even larger area,
continuing his examination northward to Lake Superior. Again his report
was published promptly, and he continued for several years his examination
of the Northwest Territory, submitting his final report in 1851. It is
interesting to note that in his earlier report Doctor Owen subscribed himself
as “Principal Agent to explore the Mineral Lands of the United States,” but
that in the later report he was “U. S. Geologist for Wisconsin.” The two
surveys together covered 57,000 square miles.
During the same period similar surveys were being made in northern
Michigan by Dr. Charles T. Jackson, 1847–48, and Foster and Whitney,
1849–51. These surveys also had been hastened by the “copper fever” of
1844–46, with wholesale issue of permits and leases, Congress in 1847
authorizing the sale of the mineral lands and a geological survey of the
Lake Superior district. The execution of these surveys under Jackson and
under Foster and Whitney and the prompt publication in 1851 of the maps
of the whole region materially helped to establish copper mining on a more
conservative basis. and the development of the Lake Superior region was
rapid.[99]
These land-classification surveys, with their definite purpose, represent
the best geologic work of the time. The plan necessitated thoroughgoing
field work with considerable detail and prompt publication of systematic
reports, and in the working up of the results specialists like James Hall and
Joseph Leidy contributed, while F. B. Meek was an assistant of Owen. It is
by geologists of the present day—the receipt late in the season (August 17,
1839) of authority to begin work—within exactly a month he had his force
of 139 assistants organized into 24 field parties, instructed in “such
elementary principles of geology as were necessary to their performance of
the duties required of them.” His plan of campaign provided for a
northward drive at a predetermined rate of traverse for each party, with
periodic reports to himself at appointed stations, “to receive which reports
and to examine the country in person” he crossed the area under survey
eleven times. The result of such masterful leadership was the completion of
the exploration of all the lands comprehended in his orders in two months
and six days, and his report on this great area—about 11,000 square miles—
bears date of April 2, 1840.
Eight years later Doctor Owen made a survey of an even larger area,
continuing his examination northward to Lake Superior. Again his report
was published promptly, and he continued for several years his examination
of the Northwest Territory, submitting his final report in 1851. It is
interesting to note that in his earlier report Doctor Owen subscribed himself
as “Principal Agent to explore the Mineral Lands of the United States,” but
that in the later report he was “U. S. Geologist for Wisconsin.” The two
surveys together covered 57,000 square miles.
During the same period similar surveys were being made in northern
Michigan by Dr. Charles T. Jackson, 1847–48, and Foster and Whitney,
1849–51. These surveys also had been hastened by the “copper fever” of
1844–46, with wholesale issue of permits and leases, Congress in 1847
authorizing the sale of the mineral lands and a geological survey of the
Lake Superior district. The execution of these surveys under Jackson and
under Foster and Whitney and the prompt publication in 1851 of the maps
of the whole region materially helped to establish copper mining on a more
conservative basis. and the development of the Lake Superior region was
rapid.[99]
These land-classification surveys, with their definite purpose, represent
the best geologic work of the time. The plan necessitated thoroughgoing
field work with considerable detail and prompt publication of systematic
reports, and in the working up of the results specialists like James Hall and
Joseph Leidy contributed, while F. B. Meek was an assistant of Owen. It is
Page 218
worthy of note that had not Doctor Houghton, the State geologist of
Michigan, met an untimely death in 1847, effective cooperation of the State
Survey with the Federal officials would have combined geologic
investigation with the execution of the linear surveys.[100]
Belonging to the same period of geologic exploration was the service of
J. D. Dana, as United States Geologist on the Wilkes Exploring Expedition,
the disaster to which compelled his return from the Pacific Coast overland
and resulted in his geologic observations on Oregon and northern
California.
The military expeditions during the decade 1850–60 and the earlier
expeditions of Fremont added to the geographic knowledge of the Western
country and also contributed to geologic science, largely through collections
of rocks and fossils, usually reported on by the specialists of the day. Thus
the names of Hall, Conrad, Hitchcock, and Meek appear in the published
reports on these explorations, while Marcou, Blake, Newberry, Gibbs,
Evans, Hayden, Parry, Shumard, Schiel, Antisell, and Engelmann were
geologists attached to the field expeditions. In 1852 geologic investigation
was seemingly so popular as to necessitate the statutory prohibition “there
shall be no further geological survey by the Government unless hereafter
authorized by law.”
Certain of these explorations had a specific purpose: several of them
sought a practical route for a transcontinental railroad; another a new wagon
road across Utah and Nevada; and one under Colonel Pope, with G. G.
Shumard as geologist, was sent out “for boring Artesian Wells along the line
of the 32d Parallel” in New Mexico. The published reports varied greatly in
scientific value and in carefulness of preparation, while the publication of at
least two reports was delayed until long after the war, and the manuscript of
another was lost. The report of the expedition of Major Emory contained a
colored geologic map of the western half of the country, a pioneer
publication, for the map prepared by Marcou extended only to the 106th
meridian.
Thus in the first period of Government surveys, covering about forty
years, the great West, with its wealth of public lands, was well traversed by
exploratory surveys, which furnished, however, only general outlines for a
comprehension of the stratigraphy and structure of mountain and valley,
plain and plateau. To an even less degree was there any realization of the
Michigan, met an untimely death in 1847, effective cooperation of the State
Survey with the Federal officials would have combined geologic
investigation with the execution of the linear surveys.[100]
Belonging to the same period of geologic exploration was the service of
J. D. Dana, as United States Geologist on the Wilkes Exploring Expedition,
the disaster to which compelled his return from the Pacific Coast overland
and resulted in his geologic observations on Oregon and northern
California.
The military expeditions during the decade 1850–60 and the earlier
expeditions of Fremont added to the geographic knowledge of the Western
country and also contributed to geologic science, largely through collections
of rocks and fossils, usually reported on by the specialists of the day. Thus
the names of Hall, Conrad, Hitchcock, and Meek appear in the published
reports on these explorations, while Marcou, Blake, Newberry, Gibbs,
Evans, Hayden, Parry, Shumard, Schiel, Antisell, and Engelmann were
geologists attached to the field expeditions. In 1852 geologic investigation
was seemingly so popular as to necessitate the statutory prohibition “there
shall be no further geological survey by the Government unless hereafter
authorized by law.”
Certain of these explorations had a specific purpose: several of them
sought a practical route for a transcontinental railroad; another a new wagon
road across Utah and Nevada; and one under Colonel Pope, with G. G.
Shumard as geologist, was sent out “for boring Artesian Wells along the line
of the 32d Parallel” in New Mexico. The published reports varied greatly in
scientific value and in carefulness of preparation, while the publication of at
least two reports was delayed until long after the war, and the manuscript of
another was lost. The report of the expedition of Major Emory contained a
colored geologic map of the western half of the country, a pioneer
publication, for the map prepared by Marcou extended only to the 106th
meridian.
Thus in the first period of Government surveys, covering about forty
years, the great West, with its wealth of public lands, was well traversed by
exploratory surveys, which furnished, however, only general outlines for a
comprehension of the stratigraphy and structure of mountain and valley,
plain and plateau. To an even less degree was there any realization of the
Page 219
economic possibilities of the vast territory west of the Mississippi. President
Jefferson, in planning the Lewis and Clark expedition, had stated his special
interest in the mineral resources of the region to be traversed. Nearly forty
years later Doctor Owen was strongly impressed with the commercial
promise of the region he surveyed. His reports contain analyses of ores and
statistics of production; he compared the lead output of Wisconsin, Iowa,
and Illinois with that of Europe and foretold the value of the iron, copper,
and zinc deposits of the area; he outlined the extent of the Illinois coal field;
and he laid equal emphasis upon the agricultural possibilities of the region.
Indeed, so optimistic were Owen’s general conclusions that he referred to
his separate township plats, with their detailed descriptions, as the basis for
his sanguine opinions, realizing that “the explorer is apt to become the
special pleader.” With equal breadth of view and thoroughness of execution
the surveys of Foster and Whitney laid the foundation for the development
of the copper and iron resources of the Lake Superior region, and although
these areas were largely wilderness and not adapted to rapid traverse or easy
observation the reports on their explorations nevertheless compare most
favorably with the contributions of geologists working in the more
hospitable regions in the older States.
The period following the Civil War naturally became one of national
expansion, the faces of many were turned westward, and exploration of the
national domain for its industrial possibilities took on fresh interest. Home-
seekers and miners largely made up this army of peaceful invasion, and the
winning of the West began on a scale quite different from that of the days of
the military path-finding expeditions of Fremont and other Army officers.
Thus the nation was aroused to the task of investigating its public lands and
Congress gave the support needed to make geologic exploration possible on
a large scale.
Geologic surveys of a high order were continued in the older States, as
shown by the contributions during this period of J. P. Lesley and G. H.
Cook in the East, W. C. Kerr, E. W. Hilgard, and E. A. Smith in the South,
and J. S. Newberry, C. A. White, Raphael Pumpelly, T. C. Chamberlin,
Alexander Winchell, and T. B. Brooks in the Central States. To the north the
Canadian Survey, organized in 1841 under Logan, had continued under the
same sturdy leadership until 1869, when the experienced and talented
Doctor Selwyn became Director. As contrasted with the short careers of
most of the State Surveys and with the temporary character of all of the
Jefferson, in planning the Lewis and Clark expedition, had stated his special
interest in the mineral resources of the region to be traversed. Nearly forty
years later Doctor Owen was strongly impressed with the commercial
promise of the region he surveyed. His reports contain analyses of ores and
statistics of production; he compared the lead output of Wisconsin, Iowa,
and Illinois with that of Europe and foretold the value of the iron, copper,
and zinc deposits of the area; he outlined the extent of the Illinois coal field;
and he laid equal emphasis upon the agricultural possibilities of the region.
Indeed, so optimistic were Owen’s general conclusions that he referred to
his separate township plats, with their detailed descriptions, as the basis for
his sanguine opinions, realizing that “the explorer is apt to become the
special pleader.” With equal breadth of view and thoroughness of execution
the surveys of Foster and Whitney laid the foundation for the development
of the copper and iron resources of the Lake Superior region, and although
these areas were largely wilderness and not adapted to rapid traverse or easy
observation the reports on their explorations nevertheless compare most
favorably with the contributions of geologists working in the more
hospitable regions in the older States.
The period following the Civil War naturally became one of national
expansion, the faces of many were turned westward, and exploration of the
national domain for its industrial possibilities took on fresh interest. Home-
seekers and miners largely made up this army of peaceful invasion, and the
winning of the West began on a scale quite different from that of the days of
the military path-finding expeditions of Fremont and other Army officers.
Thus the nation was aroused to the task of investigating its public lands and
Congress gave the support needed to make geologic exploration possible on
a large scale.
Geologic surveys of a high order were continued in the older States, as
shown by the contributions during this period of J. P. Lesley and G. H.
Cook in the East, W. C. Kerr, E. W. Hilgard, and E. A. Smith in the South,
and J. S. Newberry, C. A. White, Raphael Pumpelly, T. C. Chamberlin,
Alexander Winchell, and T. B. Brooks in the Central States. To the north the
Canadian Survey, organized in 1841 under Logan, had continued under the
same sturdy leadership until 1869, when the experienced and talented
Doctor Selwyn became Director. As contrasted with the short careers of
most of the State Surveys and with the temporary character of all of the
Page 220
Federal undertakings in geologic investigation, the continuance of the
Canadian Geological Survey for more than half a century under two
directors gave opportunity for continuity of effort in making known to the
people of the Dominion its resources and at the same time contributing to
the world much pure science.
Passing with simple mention the two Government expeditions into the
Black Hills, which afforded opportunity for geologic exploration by N. H.
Winchell in 1874 and by Jenney and Newton in 1875, the record of
geologic work under Government auspices in the period immediately
following the Civil War groups itself around the names of four leaders—
Hayden, King, Powell, and Wheeler. The four organizations, distinguished
commonly by the names of these four masterful organizers, occupied the
Western field more or less continuously from 1867 to 1878, and the sum
total of their contributions to geography and geology was large indeed. In
the words of Clarence King,[101] “Eighteen hundred and sixty-seven,
therefore, marks, in the history of national geological work, a turning point,
when the science ceased to be dragged in the dust of rapid exploration and
took a commanding position in the professional work of the country.”
Together these four expeditions covered half a million square miles, or
more than a third of the area of the United States west of the one-hundredth
meridian, and the cost of all this work was approximately two million
dollars, which was a small fraction of its value to the nation counting only
the impetus given to settlement and utilization.
As viewed from a distance of nearly half a century, these four surveys
differed much in plan of organization, scope of purpose, and success of
execution, so that comparison would have little value except as possibly
bearing upon the work of the larger organization which followed them and
became the heir not only to much that had been attained by these pioneer
surveys but also to the great task uncompleted by them. So, if in the earliest
days of the present United States Geological Survey there may have been a
certain partisanship in tracing derived characters in the new organization, it
is even now worth while to recognize the real origin of much that is
credited to present-day development.
Dr. F. V. Hayden was the first of these Survey leaders to engage in
geological exploration. He visited the Badlands as early as 1853, and his
connection with subsequent expeditions was interrupted only by his service
Canadian Geological Survey for more than half a century under two
directors gave opportunity for continuity of effort in making known to the
people of the Dominion its resources and at the same time contributing to
the world much pure science.
Passing with simple mention the two Government expeditions into the
Black Hills, which afforded opportunity for geologic exploration by N. H.
Winchell in 1874 and by Jenney and Newton in 1875, the record of
geologic work under Government auspices in the period immediately
following the Civil War groups itself around the names of four leaders—
Hayden, King, Powell, and Wheeler. The four organizations, distinguished
commonly by the names of these four masterful organizers, occupied the
Western field more or less continuously from 1867 to 1878, and the sum
total of their contributions to geography and geology was large indeed. In
the words of Clarence King,[101] “Eighteen hundred and sixty-seven,
therefore, marks, in the history of national geological work, a turning point,
when the science ceased to be dragged in the dust of rapid exploration and
took a commanding position in the professional work of the country.”
Together these four expeditions covered half a million square miles, or
more than a third of the area of the United States west of the one-hundredth
meridian, and the cost of all this work was approximately two million
dollars, which was a small fraction of its value to the nation counting only
the impetus given to settlement and utilization.
As viewed from a distance of nearly half a century, these four surveys
differed much in plan of organization, scope of purpose, and success of
execution, so that comparison would have little value except as possibly
bearing upon the work of the larger organization which followed them and
became the heir not only to much that had been attained by these pioneer
surveys but also to the great task uncompleted by them. So, if in the earliest
days of the present United States Geological Survey there may have been a
certain partisanship in tracing derived characters in the new organization, it
is even now worth while to recognize the real origin of much that is
credited to present-day development.
Dr. F. V. Hayden was the first of these Survey leaders to engage in
geological exploration. He visited the Badlands as early as 1853, and his
connection with subsequent expeditions was interrupted only by his service
Page 221
as a surgeon in the Federal Army during the war. In 1867, however, Hayden
resumed his geologic work as United States Geologist in Nebraska,
operating under direction of the Commissioner of the General Land Office.
In the following eleven years the activities of the Hayden Survey—the
“Geological and Geographical Survey of the Territories”—extended into
Wyoming, Colorado, New Mexico, Montana, and Idaho, covering with
areal surveys 107,000 square miles. This Survey, as might be expected from
the long experience of its leader, made large contributions to stratigraphy,
which involved notable paleontologic work by Cope, Meek, and
Lesquereux. Next in importance was the structural work of A. C. Peale, W.
H. Holmes, Capt. C. E. Dutton, and Dr. Hayden himself, and the influence
of these expeditions in popularizing geology should not be overlooked. The
expedition of 1871 into the geyser region on the upper Yellowstone resulted
in the creation of the first of the national parks. W. H. Holmes began his
artistic contributions to geology in 1872 with this Survey. Topographic
mapping was added to the geologic exploration, James T. Gardner and A. D.
Wilson joining the Hayden Survey after earlier service on the King Survey
and Henry Gannett being a member of parties, first as astronomer and later
as topographer in charge. The accomplishment of the Hayden Survey itself
and the later work of many of its members show that this organization
possessed a corps of strong men.
The King Survey was a smaller organization, with Congressional
authorization of definite scope and a systematic plan of operation. The
beginning of construction of the Union Pacific terminated the period of the
railroad surveys under the War Department and afforded opportunity for
geologic work that would be more than exploratory: the opening up of the
new country made investigation of its resources logical. This fact was
recognized by Clarence King, who had traversed the same route as a
member of an emigrant train with his friend James T. Gardner. His plan to
make a geological cross section of the Cordilleras, with a study of the
resources along the route of the Pacific railroads, won the support of
Congress, and the “Geological Exploration of the Fortieth Parallel” was
authorized in 1867, with Clarence King as geologist in charge, under the
Chief of Engineers of the Army. Field work was begun in the summer of
that year, and it is interesting to note that Mr. King and his small force of
geological assistants—the two Hagues and S. F. Emmons—began at the
western end of this cross section, and in this and subsequent years extended
resumed his geologic work as United States Geologist in Nebraska,
operating under direction of the Commissioner of the General Land Office.
In the following eleven years the activities of the Hayden Survey—the
“Geological and Geographical Survey of the Territories”—extended into
Wyoming, Colorado, New Mexico, Montana, and Idaho, covering with
areal surveys 107,000 square miles. This Survey, as might be expected from
the long experience of its leader, made large contributions to stratigraphy,
which involved notable paleontologic work by Cope, Meek, and
Lesquereux. Next in importance was the structural work of A. C. Peale, W.
H. Holmes, Capt. C. E. Dutton, and Dr. Hayden himself, and the influence
of these expeditions in popularizing geology should not be overlooked. The
expedition of 1871 into the geyser region on the upper Yellowstone resulted
in the creation of the first of the national parks. W. H. Holmes began his
artistic contributions to geology in 1872 with this Survey. Topographic
mapping was added to the geologic exploration, James T. Gardner and A. D.
Wilson joining the Hayden Survey after earlier service on the King Survey
and Henry Gannett being a member of parties, first as astronomer and later
as topographer in charge. The accomplishment of the Hayden Survey itself
and the later work of many of its members show that this organization
possessed a corps of strong men.
The King Survey was a smaller organization, with Congressional
authorization of definite scope and a systematic plan of operation. The
beginning of construction of the Union Pacific terminated the period of the
railroad surveys under the War Department and afforded opportunity for
geologic work that would be more than exploratory: the opening up of the
new country made investigation of its resources logical. This fact was
recognized by Clarence King, who had traversed the same route as a
member of an emigrant train with his friend James T. Gardner. His plan to
make a geological cross section of the Cordilleras, with a study of the
resources along the route of the Pacific railroads, won the support of
Congress, and the “Geological Exploration of the Fortieth Parallel” was
authorized in 1867, with Clarence King as geologist in charge, under the
Chief of Engineers of the Army. Field work was begun in the summer of
that year, and it is interesting to note that Mr. King and his small force of
geological assistants—the two Hagues and S. F. Emmons—began at the
western end of this cross section, and in this and subsequent years extended
Page 222
the survey from the east front of the Sierra Nevada to Cheyenne, covering a
belt of territory about 100 miles in width. This comprehensive plan was
carried out in the field operations, and the scientific and economic results
were systematically worked up in the reports, which appeared in 1870–80.
The only departure from this plan was a study of the volcanic mountains
Shasta, Rainier, and Hood, in 1870, occasioned by an unexpected and
unsolicited appropriation for field work, and that summer’s work resulted in
the discovery of active glaciers, the first known within the United States.
The Fortieth Parallel Survey is to be credited with contributions to the
knowledge of the stratigraphy of the West, the region traversed being
remarkably representative of the stratigraphic column, to which was added
the paleontologic work of Marsh, Meek, Hall, and Whitfield, while the
attempt was made to interpret the sedimentary record in terms of Paleozoic,
Mesozoic, and Tertiary geography. King’s plan of survey included large use
of topographic mapping with astronomic base and triangulation control and
contours based upon barometric elevations. The results were pronounced by
an unfriendly critic[102] as “very valuable, especially from a geological point
of view,” but unfortunate in being the forerunner of work in which
Government geologists “have presumed to arrogate the control of the
fundamental operations of a topographic survey.” To the King Survey must
be credited the introduction of systematic contour mapping and the use of
contour maps for purposes of geology. In two other respects the King
Survey contributed largely to future Government work: microscopical
petrography in the United States may be said to have begun with the visit of
Professor Zirkel to this country as a member of this Survey in 1875, and the
report of J. D. Hague on “Mining Industry” was the fitting expression of the
emphasis then put on the study of the mineral resources of this newly
opened territory, a subject of investigation that was in large part the true
basis of King’s project rather than simply “the immediate excuse for the
Survey.” An earlier influence in the scientific study of ore deposits had
come from Von Richthofen’s investigation of the Comstock Lode in 1865
and his subsequent work with Whitney in California. The incident of King’s
relation to the diamond fraud in Arizona in 1872 furnished a precedent for
public servants of a later day; he investigated the reported find from
scientific interest but exposed it with all the zeal of a publicist and truth
lover. In a word, the Fortieth Parallel Survey commands our admiration for
belt of territory about 100 miles in width. This comprehensive plan was
carried out in the field operations, and the scientific and economic results
were systematically worked up in the reports, which appeared in 1870–80.
The only departure from this plan was a study of the volcanic mountains
Shasta, Rainier, and Hood, in 1870, occasioned by an unexpected and
unsolicited appropriation for field work, and that summer’s work resulted in
the discovery of active glaciers, the first known within the United States.
The Fortieth Parallel Survey is to be credited with contributions to the
knowledge of the stratigraphy of the West, the region traversed being
remarkably representative of the stratigraphic column, to which was added
the paleontologic work of Marsh, Meek, Hall, and Whitfield, while the
attempt was made to interpret the sedimentary record in terms of Paleozoic,
Mesozoic, and Tertiary geography. King’s plan of survey included large use
of topographic mapping with astronomic base and triangulation control and
contours based upon barometric elevations. The results were pronounced by
an unfriendly critic[102] as “very valuable, especially from a geological point
of view,” but unfortunate in being the forerunner of work in which
Government geologists “have presumed to arrogate the control of the
fundamental operations of a topographic survey.” To the King Survey must
be credited the introduction of systematic contour mapping and the use of
contour maps for purposes of geology. In two other respects the King
Survey contributed largely to future Government work: microscopical
petrography in the United States may be said to have begun with the visit of
Professor Zirkel to this country as a member of this Survey in 1875, and the
report of J. D. Hague on “Mining Industry” was the fitting expression of the
emphasis then put on the study of the mineral resources of this newly
opened territory, a subject of investigation that was in large part the true
basis of King’s project rather than simply “the immediate excuse for the
Survey.” An earlier influence in the scientific study of ore deposits had
come from Von Richthofen’s investigation of the Comstock Lode in 1865
and his subsequent work with Whitney in California. The incident of King’s
relation to the diamond fraud in Arizona in 1872 furnished a precedent for
public servants of a later day; he investigated the reported find from
scientific interest but exposed it with all the zeal of a publicist and truth
lover. In a word, the Fortieth Parallel Survey commands our admiration for
Page 223
its brilliant plan, thoroughgoing work in field and office, and high quality of
personnel.
Major J. W. Powell began his large contribution to Government surveys
with his exploration of the Grand Canyon in 1869, the Congressional
recognition of his expedition being limited to an authorization for the issue
of rations by the War Department. Small appropriations were made in the
following years, and in 1874 full authorization was given for the
continuance of his survey in Utah under the Secretary of the Interior and
personnel.
Major J. W. Powell began his large contribution to Government surveys
with his exploration of the Grand Canyon in 1869, the Congressional
recognition of his expedition being limited to an authorization for the issue
of rations by the War Department. Small appropriations were made in the
following years, and in 1874 full authorization was given for the
continuance of his survey in Utah under the Secretary of the Interior and
Page 224
was followed by the adoption of the name “United States Geographical and
Geological Survey of the Rocky Mountain Region.” This organization was
the least pretentious of the four operating during this period—it covered
less area, expended less public money, and published much less—but its
contribution to American geology is not to be measured by miles or pages
but by ideas. Its physical environment favored this survey, and in the work
of Powell, Dutton, and Gilbert can be seen the beginnings of physiography
on the heroic scale exemplified in the Grand Canyon and the High Plateaus.
The first use of terms like “base-level of erosion,” “consequent and
antecedent drainage,” and “laccolith” marked the introduction of new ideas
in the interpretation of land sculpture and geologic structure. The daring
boat trip of Powell was no less brilliant than his simple explanation of the
Grand Canyon itself.
“The United States Geographical Surveys West of the 100th Meridian”
was the title given to the explorations made under Lieut. G. M. Wheeler, of
the Engineer Corps, which began with topographic reconnaissances in
Nevada, Utah, and Arizona, specifically authorized by Congress in 1872.
From the standpoint of American geology this could be better known as the
Gilbert Survey, Mr. G. K. Gilbert serving for the three years 1871–73, the
later part of the time with the title of chief geological assistant. Gilbert’s
contributions included his description of Basin Range structure, his first
account of old Lake Bonneville, and his discussion of the erosion
phenomena of the desert country. J. J. Stevenson also served later as a
geologist of this Survey, and A. R. Marvine, E. E. Howell, E. D. Cope, Jules
Marcou, and I. C. Russell were connected with the field parties. Captain
Wheeler’s own claim for the work of his Survey emphasized its geographic
side, for he regarded the results as the partial completion of a systematic
topographic survey of the country.
By 1878, when the Fortieth Parallel Survey had completed the work
planned by its chief, three of these independent surveys still contended for
Federal support and for scientific occupation of the most attractive portions
of the Western country. Unrestrained competition of this kind, even in the
public service, proves as wasteful as unregulated competition in private
business,[103] and Congress appealed to the National Academy of Sciences
for a plan for Government surveys to “secure the best results at the least
possible cost.” Under instructions by Congress the National Academy
considered all the work relating to scientific surveys and reported to
Geological Survey of the Rocky Mountain Region.” This organization was
the least pretentious of the four operating during this period—it covered
less area, expended less public money, and published much less—but its
contribution to American geology is not to be measured by miles or pages
but by ideas. Its physical environment favored this survey, and in the work
of Powell, Dutton, and Gilbert can be seen the beginnings of physiography
on the heroic scale exemplified in the Grand Canyon and the High Plateaus.
The first use of terms like “base-level of erosion,” “consequent and
antecedent drainage,” and “laccolith” marked the introduction of new ideas
in the interpretation of land sculpture and geologic structure. The daring
boat trip of Powell was no less brilliant than his simple explanation of the
Grand Canyon itself.
“The United States Geographical Surveys West of the 100th Meridian”
was the title given to the explorations made under Lieut. G. M. Wheeler, of
the Engineer Corps, which began with topographic reconnaissances in
Nevada, Utah, and Arizona, specifically authorized by Congress in 1872.
From the standpoint of American geology this could be better known as the
Gilbert Survey, Mr. G. K. Gilbert serving for the three years 1871–73, the
later part of the time with the title of chief geological assistant. Gilbert’s
contributions included his description of Basin Range structure, his first
account of old Lake Bonneville, and his discussion of the erosion
phenomena of the desert country. J. J. Stevenson also served later as a
geologist of this Survey, and A. R. Marvine, E. E. Howell, E. D. Cope, Jules
Marcou, and I. C. Russell were connected with the field parties. Captain
Wheeler’s own claim for the work of his Survey emphasized its geographic
side, for he regarded the results as the partial completion of a systematic
topographic survey of the country.
By 1878, when the Fortieth Parallel Survey had completed the work
planned by its chief, three of these independent surveys still contended for
Federal support and for scientific occupation of the most attractive portions
of the Western country. Unrestrained competition of this kind, even in the
public service, proves as wasteful as unregulated competition in private
business,[103] and Congress appealed to the National Academy of Sciences
for a plan for Government surveys to “secure the best results at the least
possible cost.” Under instructions by Congress the National Academy
considered all the work relating to scientific surveys and reported to
Page 225
Congress a plan prepared by a special committee, whose membership
included the illustrious names of Marsh, Dana, Rogers, Newberry,
Trowbridge, Newcomb, and Agassiz. This report, which was adopted by the
Academy with only one dissenting vote, grouped all surveys—geodetic,
topographic, land parceling, and economic—under two distinct heads,
surveys of mensuration and surveys of geology. At that time five
independent organizations in three different departments were carrying on
surveys of mensuration, and the Academy recommended that all such work
be combined under the Coast and Geodetic Survey with the new name
Coast and Interior Survey. For the investigation of the natural resources of
the public domain and the classification of the public lands a new
organization was proposed, the United States Geological Survey. The
functions of these two surveys and of a third coordinate bureau in the
Interior Department, the Land Office, were carefully defined and their
interrelations fully recognized and provided for in the plan presented to
Congress. Viewed in the light of 39 years of experience the National
Academy plan would be indorsed by most of us as eminently practical, and
the report stands as a splendid example of public service rendered by
America’s leading scientists. The legislation which embodied the entire
plan, however, failed of passage in Congress.
The natural activity behind the scenes of the conflicting interests
represented by those connected with the several surveys may be seen in the
legislative history of the moves leading up to the creation of the United
States Geological Survey. In the last session of the 45th Congress the
special legislation embodying the recommendations of the National
Academy was included in the Legislative, Executive, and Judicial
Appropriation bill as it passed the House of Representatives, while the
Sundry Civil Appropriation bill carried an item simply making effective the
longer section in the other appropriation bill. The item in the Legislative
appropriation bill created the office of the Director of the Geological
Survey, provided his salary, and defined his duties, as well as specifically
terminating the operations of the three older organizations. The item in the
Sundry Civil bill as it passed the House appropriated $100,000 for the new
Geological Survey, but when this appropriation bill was reported to the
Senate a committee amendment added the words “of the Territories,” and
further amendments offered on the floor changed the item so as to provide
specifically and exclusively for the continuation of the Hayden Survey.
included the illustrious names of Marsh, Dana, Rogers, Newberry,
Trowbridge, Newcomb, and Agassiz. This report, which was adopted by the
Academy with only one dissenting vote, grouped all surveys—geodetic,
topographic, land parceling, and economic—under two distinct heads,
surveys of mensuration and surveys of geology. At that time five
independent organizations in three different departments were carrying on
surveys of mensuration, and the Academy recommended that all such work
be combined under the Coast and Geodetic Survey with the new name
Coast and Interior Survey. For the investigation of the natural resources of
the public domain and the classification of the public lands a new
organization was proposed, the United States Geological Survey. The
functions of these two surveys and of a third coordinate bureau in the
Interior Department, the Land Office, were carefully defined and their
interrelations fully recognized and provided for in the plan presented to
Congress. Viewed in the light of 39 years of experience the National
Academy plan would be indorsed by most of us as eminently practical, and
the report stands as a splendid example of public service rendered by
America’s leading scientists. The legislation which embodied the entire
plan, however, failed of passage in Congress.
The natural activity behind the scenes of the conflicting interests
represented by those connected with the several surveys may be seen in the
legislative history of the moves leading up to the creation of the United
States Geological Survey. In the last session of the 45th Congress the
special legislation embodying the recommendations of the National
Academy was included in the Legislative, Executive, and Judicial
Appropriation bill as it passed the House of Representatives, while the
Sundry Civil Appropriation bill carried an item simply making effective the
longer section in the other appropriation bill. The item in the Legislative
appropriation bill created the office of the Director of the Geological
Survey, provided his salary, and defined his duties, as well as specifically
terminating the operations of the three older organizations. The item in the
Sundry Civil bill as it passed the House appropriated $100,000 for the new
Geological Survey, but when this appropriation bill was reported to the
Senate a committee amendment added the words “of the Territories,” and
further amendments offered on the floor changed the item so as to provide
specifically and exclusively for the continuation of the Hayden Survey.
Page 226
Other amendments provided small appropriations for the completion of the
reports of the Powell and Wheeler surveys, and the bill passed the Senate in
this form. The Legislative Appropriation bill was similarly pruned, while in
the Senate, of all reference to the proposed new organization. This bill,
however, died in conference, but in the last hours of the session the
conferees on the Sundry Civil bill took unto themselves legislative powers
and transferred from the dead bill to the pending measure all the language
which constitutes the “organic act” of the United States Geological Survey.
This action was denounced in the Senate as “a wide departure from the
authority that is possessed by a conference committee,” and it was further
stated in debate that the inserted provision which created a new office and
discontinued the existing surveys was one “which neither the Committee of
the Senate nor the Senate itself ever saw.” This assertion was perhaps
parliamentarily sound in that the language was new to the Sundry Civil bill,
yet actually the Senate had only two days before stricken the same proposed
legislation from the pending Legislative Appropriation bill. However, the
House conferees—Representatives Atkins of Tennessee, Hewett of New
York, and Hale of Maine—had realized their tactical advantage, and the
Senate, after a brief debate, voted on March 3 to concur in the report of the
committee of conference, thus reversing all their earlier action, in which the
friends of the Hayden and Wheeler organizations apparently had
commanded more votes than the advocates of the National Academy plan.
Clarence King was appointed first Director of the United States
Geological Survey on April 3, 1879, and began the work of organization.
With his proven genius for administration, King promptly resolved the
doubt as to the meaning of the term “national domain” in the language
defining the duties of the Director by taking the conservative side and
limiting the work of the new organization to the region west of the 102d
meridian. This region was divided into four geological divisions, and for
economy of time and money field headquarters were established for these
divisions. The Division of the Rocky Mountains was placed under Mr.
Emmons as geologist in charge, the Division of the Colorado under Captain
Dutton, the Division of the Great Basin under Mr. Gilbert, and the Division
of the Pacific under Arnold Hague. The Division of the Colorado was
intended as merely temporary for the purpose of bringing to completion the
scientific work of the Powell Survey. Similarly Dr. Hayden was given the
opportunity to prepare a systematic digest of his scientific results. This
reports of the Powell and Wheeler surveys, and the bill passed the Senate in
this form. The Legislative Appropriation bill was similarly pruned, while in
the Senate, of all reference to the proposed new organization. This bill,
however, died in conference, but in the last hours of the session the
conferees on the Sundry Civil bill took unto themselves legislative powers
and transferred from the dead bill to the pending measure all the language
which constitutes the “organic act” of the United States Geological Survey.
This action was denounced in the Senate as “a wide departure from the
authority that is possessed by a conference committee,” and it was further
stated in debate that the inserted provision which created a new office and
discontinued the existing surveys was one “which neither the Committee of
the Senate nor the Senate itself ever saw.” This assertion was perhaps
parliamentarily sound in that the language was new to the Sundry Civil bill,
yet actually the Senate had only two days before stricken the same proposed
legislation from the pending Legislative Appropriation bill. However, the
House conferees—Representatives Atkins of Tennessee, Hewett of New
York, and Hale of Maine—had realized their tactical advantage, and the
Senate, after a brief debate, voted on March 3 to concur in the report of the
committee of conference, thus reversing all their earlier action, in which the
friends of the Hayden and Wheeler organizations apparently had
commanded more votes than the advocates of the National Academy plan.
Clarence King was appointed first Director of the United States
Geological Survey on April 3, 1879, and began the work of organization.
With his proven genius for administration, King promptly resolved the
doubt as to the meaning of the term “national domain” in the language
defining the duties of the Director by taking the conservative side and
limiting the work of the new organization to the region west of the 102d
meridian. This region was divided into four geological divisions, and for
economy of time and money field headquarters were established for these
divisions. The Division of the Rocky Mountains was placed under Mr.
Emmons as geologist in charge, the Division of the Colorado under Captain
Dutton, the Division of the Great Basin under Mr. Gilbert, and the Division
of the Pacific under Arnold Hague. The Division of the Colorado was
intended as merely temporary for the purpose of bringing to completion the
scientific work of the Powell Survey. Similarly Dr. Hayden was given the
opportunity to prepare a systematic digest of his scientific results. This
Page 227
organization of the work and the selection of geologists in charge showed
the relation of the new and the old, and a glance at the personnel of the new
Survey indicates the extent to which the geologic investigation of the
Western country was to continue without interruption. Of the twenty-four
geologists and topographers listed in the first administrative report, four had
been connected with the Powell Survey, two with the Hayden, three with
the Wheeler, and five with the King Survey.
the relation of the new and the old, and a glance at the personnel of the new
Survey indicates the extent to which the geologic investigation of the
Western country was to continue without interruption. Of the twenty-four
geologists and topographers listed in the first administrative report, four had
been connected with the Powell Survey, two with the Hayden, three with
the Wheeler, and five with the King Survey.
Page 228
In planning the initial work of the United States Geological Survey, the
Director speaks of the “most important geological subjects” and “mining
industries,” of “instructive geological structure” and “great bullion yield” in
the same sentences, so that the intent was plain to make the geologic
investigations both theoretical and practical.
It was expected that the field of operations of this Federal Survey would
be at once extended by Congress over the whole United States, but the
measure making this extension, which would simply carry out the intent of
the framers of the legislation creating the new bureau, passed the House
alone, and it was only by subsequent modification of the wording of
appropriation items that the United States Geological Survey became
national in scope as well as in name. The critical question of the effective
coördination of State and Federal geologic surveys was met by Director
King, who corrected an erroneous impression “industriously circulated” by
stating his policy to be to urge the inauguration and continuance of State
surveys.[104] This was the initial step in the cooperation between State and
Federal surveys which became effective on a large scale in subsequent
years.
Though the Geological Survey has extended its operations over the
whole United States, its largest activities have always been directed toward
the exploration and development of the newer territory in the public-land
States. All four of its directors had their field training in the West: the name
of Major Powell, who succeeded King in 1880, is inseparably connected
with scientific exploration; Charles D. Walcott, who was Director from
1894 to 1907, the period of the Survey’s greatest expansion, made the
largest contribution to the Paleozoic stratigraphy and paleontology of the
West; and the present Director spent seven field seasons in the Northern
Cascades and one in a mining district in Utah. The scope of the activities
both East and West as developed during the 39 years since the
establishment of the new bureau can be best described, perhaps, in terms of
its present functions as expressed in the organization of to-day.
The growth of the Survey is measured in the increase of annual
appropriation from $106,000 in 1879–80 to the amount available for the
current year—$1,925,520, not including half a million dollars from War
Department appropriations being spent in the topographic work of the
Survey. The corresponding increase in personnel has been from 39, listed in
Director speaks of the “most important geological subjects” and “mining
industries,” of “instructive geological structure” and “great bullion yield” in
the same sentences, so that the intent was plain to make the geologic
investigations both theoretical and practical.
It was expected that the field of operations of this Federal Survey would
be at once extended by Congress over the whole United States, but the
measure making this extension, which would simply carry out the intent of
the framers of the legislation creating the new bureau, passed the House
alone, and it was only by subsequent modification of the wording of
appropriation items that the United States Geological Survey became
national in scope as well as in name. The critical question of the effective
coördination of State and Federal geologic surveys was met by Director
King, who corrected an erroneous impression “industriously circulated” by
stating his policy to be to urge the inauguration and continuance of State
surveys.[104] This was the initial step in the cooperation between State and
Federal surveys which became effective on a large scale in subsequent
years.
Though the Geological Survey has extended its operations over the
whole United States, its largest activities have always been directed toward
the exploration and development of the newer territory in the public-land
States. All four of its directors had their field training in the West: the name
of Major Powell, who succeeded King in 1880, is inseparably connected
with scientific exploration; Charles D. Walcott, who was Director from
1894 to 1907, the period of the Survey’s greatest expansion, made the
largest contribution to the Paleozoic stratigraphy and paleontology of the
West; and the present Director spent seven field seasons in the Northern
Cascades and one in a mining district in Utah. The scope of the activities
both East and West as developed during the 39 years since the
establishment of the new bureau can be best described, perhaps, in terms of
its present functions as expressed in the organization of to-day.
The growth of the Survey is measured in the increase of annual
appropriation from $106,000 in 1879–80 to the amount available for the
current year—$1,925,520, not including half a million dollars from War
Department appropriations being spent in the topographic work of the
Survey. The corresponding increase in personnel has been from 39, listed in
Page 229
the first report, to 911 holding regular appointments at the present time,
divided among the different branches as follows: A scientific force of 173 in
the Geologic Branch, 169 in the Water Resources Branch, 71 in the
Topographic Branch, and 15 in the Land Classification Board, with a
clerical force of 168 divided among the same branches, and the remainder
the technical and clerical employees of the publication and administrative
branches. These personnel statistics are not expressive of normal
conditions, since a large number of the topographic engineers are
commissioned officers and thus are not included on the civilian roll, while,
on the other hand, the classification of the stock-raising homestead lands
makes the technical force of the Water Resources Branch unusually large
this year.
The primary aim of the Geological Survey is geologic, whether directed
by authority of law toward the “examination of the geological structure,
mineral resources, and products of the national domain,” toward the
preparation of the authorized “reports upon general and economic geology
and paleontology,” of the “geologic map of the United States,” or of the
“report on the mineral resources of the United States,” or toward the
“continuation of the investigation of the mineral resources of Alaska” or
“chemical and physical researches relating to the geology of the United
States.” The spirit and the purpose of the Survey’s work in all these fields
are not believed to have materially changed from those of the founders of
the science in America. From time to time too much emphasis may have
appeared to be laid upon applied geology as contrasted with pure science,
yet the report of the National Academy to Congress in terms placed the
stress upon economic resources and referred to paleontology as “necessarily
connected” with general and economic geology. The practical purpose of
geologic research under Government auspices must be recognized by the
administrator, whether he be the paleontologist like Walcott, the
philosopher like Powell, or the mining geologist like King. That the task of
steering the true course is no new problem can be seen from the statement
of Owen[105] written 70 years ago, and these words describe conditions of
Government geological work even to-day:
Scientific researches, which to some may seem purely speculative and curious, are essential as
preliminaries to these practical results. Further than such necessity dictates, they have not been
pushed, except as subordinate and incidental, and chiefly at such periods as, under the ordinary
requirements of public service, might be regarded as leisure moments; so that the contributions to
divided among the different branches as follows: A scientific force of 173 in
the Geologic Branch, 169 in the Water Resources Branch, 71 in the
Topographic Branch, and 15 in the Land Classification Board, with a
clerical force of 168 divided among the same branches, and the remainder
the technical and clerical employees of the publication and administrative
branches. These personnel statistics are not expressive of normal
conditions, since a large number of the topographic engineers are
commissioned officers and thus are not included on the civilian roll, while,
on the other hand, the classification of the stock-raising homestead lands
makes the technical force of the Water Resources Branch unusually large
this year.
The primary aim of the Geological Survey is geologic, whether directed
by authority of law toward the “examination of the geological structure,
mineral resources, and products of the national domain,” toward the
preparation of the authorized “reports upon general and economic geology
and paleontology,” of the “geologic map of the United States,” or of the
“report on the mineral resources of the United States,” or toward the
“continuation of the investigation of the mineral resources of Alaska” or
“chemical and physical researches relating to the geology of the United
States.” The spirit and the purpose of the Survey’s work in all these fields
are not believed to have materially changed from those of the founders of
the science in America. From time to time too much emphasis may have
appeared to be laid upon applied geology as contrasted with pure science,
yet the report of the National Academy to Congress in terms placed the
stress upon economic resources and referred to paleontology as “necessarily
connected” with general and economic geology. The practical purpose of
geologic research under Government auspices must be recognized by the
administrator, whether he be the paleontologist like Walcott, the
philosopher like Powell, or the mining geologist like King. That the task of
steering the true course is no new problem can be seen from the statement
of Owen[105] written 70 years ago, and these words describe conditions of
Government geological work even to-day:
Scientific researches, which to some may seem purely speculative and curious, are essential as
preliminaries to these practical results. Further than such necessity dictates, they have not been
pushed, except as subordinate and incidental, and chiefly at such periods as, under the ordinary
requirements of public service, might be regarded as leisure moments; so that the contributions to
Page 230
science thus incidentally afforded, and which a liberal policy forbade to neglect, may be considered,
in a measure, a voluntary offering, tendered at little or no additional expense to the department.
The increased attention given to mineral resources has been a matter of
gradual growth. Mr. King early organized a Division of Mining Geology
with Messrs. Pumpelly, Emmons, and Becker as geologists in charge, to
whom were assigned the collection of mineral statistics for the Tenth
Census. These Survey geologists and Director King himself held
appointments as special agents of the Census Bureau, and on the staff
selected for this work appear the names of T. B. Brooks, Edward Orton, T.
C. Chamberlin, Eugene A. Smith, George Little, J. R. Proctor, R. D. Irving,
N. S. Shaler, John Hays Hammond, Bailey Willis, and G. H. Eldridge,
indicating the extent to which the supervision of these inquiries was placed
in the hands of economic geologists. This procedure was reverted to by
Director Walcott and in the last ten years has become a well-established
policy, the statistics of annual production of all the important mineral
products being under the charge of geologists, as best qualified to
comprehend the resources of the country. Another of these special assistants
in 1880 was Albert Williams, Jr., who became the first chief of the Division
of Mineral Resources, in 1882. The study of ore deposits, which may be
said to have begun with the King Survey, was inspired by King’s own
appreciation of the broad geologic relations of the distribution of mineral
wealth and by the detailed studies of individual mining districts by his
associates, “based upon facts accurately determined in the light of modern
geology.”
Geological surveys have been prosecuted in Alaska since 1895, and in
the last few years the annual appropriation for the work has been the same
as that made for the expenses of the whole Survey in the first year of its
history. The Division of Alaskan Mineral Resources is in fact a geological
survey in itself, except that it shares in the administrative machinery of the
larger organization and has the advantage of the cooperation of the
scientific specialists of the Survey as they may be needed to supplement its
own force. All the investigations in this distant part of the country represent
the Geological Survey at its best, for here the organization’s long
experience in the Western States can be applied to most effective and
helpful work on the frontier, where the geologist and topographer in their
exploration do not always follow the prospector but often precede him.
in a measure, a voluntary offering, tendered at little or no additional expense to the department.
The increased attention given to mineral resources has been a matter of
gradual growth. Mr. King early organized a Division of Mining Geology
with Messrs. Pumpelly, Emmons, and Becker as geologists in charge, to
whom were assigned the collection of mineral statistics for the Tenth
Census. These Survey geologists and Director King himself held
appointments as special agents of the Census Bureau, and on the staff
selected for this work appear the names of T. B. Brooks, Edward Orton, T.
C. Chamberlin, Eugene A. Smith, George Little, J. R. Proctor, R. D. Irving,
N. S. Shaler, John Hays Hammond, Bailey Willis, and G. H. Eldridge,
indicating the extent to which the supervision of these inquiries was placed
in the hands of economic geologists. This procedure was reverted to by
Director Walcott and in the last ten years has become a well-established
policy, the statistics of annual production of all the important mineral
products being under the charge of geologists, as best qualified to
comprehend the resources of the country. Another of these special assistants
in 1880 was Albert Williams, Jr., who became the first chief of the Division
of Mineral Resources, in 1882. The study of ore deposits, which may be
said to have begun with the King Survey, was inspired by King’s own
appreciation of the broad geologic relations of the distribution of mineral
wealth and by the detailed studies of individual mining districts by his
associates, “based upon facts accurately determined in the light of modern
geology.”
Geological surveys have been prosecuted in Alaska since 1895, and in
the last few years the annual appropriation for the work has been the same
as that made for the expenses of the whole Survey in the first year of its
history. The Division of Alaskan Mineral Resources is in fact a geological
survey in itself, except that it shares in the administrative machinery of the
larger organization and has the advantage of the cooperation of the
scientific specialists of the Survey as they may be needed to supplement its
own force. All the investigations in this distant part of the country represent
the Geological Survey at its best, for here the organization’s long
experience in the Western States can be applied to most effective and
helpful work on the frontier, where the geologist and topographer in their
exploration do not always follow the prospector but often precede him.
Page 231
Undoubtedly no greater factor has contributed to the development of
Alaskan resources than this pioneer work of the Federal Survey, yet the
work has also contributed notable additions to the sciences of geology and
geography.
The first duty laid upon the Director of the Geological Survey in the law
of 1879 was “the classification of the public lands,” and this phrase
undoubtedly expressed the idea of the committee of the National Academy.
The same legislation, however, contained provision for the further
consideration by a commission of the classification and valuation of the
public lands, as also recommended by the National Academy. Thus the
decision of Director King that the classification intended by Congress was
scientific and was intended for general information and not to aid the Land
Office in the disposition of land by sale or otherwise was really based upon
the deliberate opinion of the Public Lands Commission, of which he was a
member, that classification would seriously impede rapid settlement of the
unoccupied lands. Nearly forty years later those who are intrusted with the
land-classification work of the Geological Survey recognize this familiar
argument, which undoubtedly had much more force in that earlier stage of
the utilization of the Nation’s resources of land.[106] The conception of land
classification as a business policy on the part of the Government as a landed
proprietor belongs rather to this day of more intensive development. At
present current public-land legislation calls for highest use, and hence
official investigation of natural values and possibilities must precede
disposition. This type of mineral and hydrographic classification of public
lands has been in progress in increasing amount since 1906, so that now the
Geological Survey is the kind of scientific adviser to the Secretary of the
Interior and Commissioner of the General Land Office that may have been
contemplated by the National Academy of Sciences in 1878. It is plain,
however, to everyone at all conversant with Western conditions that the
recent land-classification surveys in Wyoming, for instance—detailed
geologic surveys which form the basis for the valuation of public coal lands
in 40–acre units—would have possessed no utility in 1871, when the coal-
land law was passed but when the demand for railroad fuel had just begun.
The land-classification idea is of course the basis of the National forest
and irrigation movements. The laws of 1888 and 1896, which mark the
beginning of active endorsement by Congress of these conservation
movements, placed upon the Survey the duties of examining reservoir sites
Alaskan resources than this pioneer work of the Federal Survey, yet the
work has also contributed notable additions to the sciences of geology and
geography.
The first duty laid upon the Director of the Geological Survey in the law
of 1879 was “the classification of the public lands,” and this phrase
undoubtedly expressed the idea of the committee of the National Academy.
The same legislation, however, contained provision for the further
consideration by a commission of the classification and valuation of the
public lands, as also recommended by the National Academy. Thus the
decision of Director King that the classification intended by Congress was
scientific and was intended for general information and not to aid the Land
Office in the disposition of land by sale or otherwise was really based upon
the deliberate opinion of the Public Lands Commission, of which he was a
member, that classification would seriously impede rapid settlement of the
unoccupied lands. Nearly forty years later those who are intrusted with the
land-classification work of the Geological Survey recognize this familiar
argument, which undoubtedly had much more force in that earlier stage of
the utilization of the Nation’s resources of land.[106] The conception of land
classification as a business policy on the part of the Government as a landed
proprietor belongs rather to this day of more intensive development. At
present current public-land legislation calls for highest use, and hence
official investigation of natural values and possibilities must precede
disposition. This type of mineral and hydrographic classification of public
lands has been in progress in increasing amount since 1906, so that now the
Geological Survey is the kind of scientific adviser to the Secretary of the
Interior and Commissioner of the General Land Office that may have been
contemplated by the National Academy of Sciences in 1878. It is plain,
however, to everyone at all conversant with Western conditions that the
recent land-classification surveys in Wyoming, for instance—detailed
geologic surveys which form the basis for the valuation of public coal lands
in 40–acre units—would have possessed no utility in 1871, when the coal-
land law was passed but when the demand for railroad fuel had just begun.
The land-classification idea is of course the basis of the National forest
and irrigation movements. The laws of 1888 and 1896, which mark the
beginning of active endorsement by Congress of these conservation
movements, placed upon the Survey the duties of examining reservoir sites
Page 232
and forest reserves respectively. The earlier of these laws began the
investigation of the water resources of the country, which is still an
important phase of the Survey’s activity, and led to the creation of an
independent organization—the Reclamation Service. It is easy to trace the
beginnings of Federal reclamation of arid lands in the pioneer work of
Powell, whose report in 1878 on the arid region of the United States was the
first adequate statement of the problem of largest use of these lands in terms
broader than those of individualistic endeavor. For years, however, Powell’s
appeal for Congressional consideration of this National task was like the
“voice of one crying in the wilderness.”
In a somewhat similar way the forestry surveys under the Geological
Survey helped in the organization of a separate bureau—now the Forest
Service. The other important Federal bureau tracing direct relationship to
the Survey is the Bureau of Mines, established in 1910, which continued the
investigations in mining technology specifically provided for by Congress
for six years under the Geological Survey but in some degree begun in the
early days of the Survey under Directors King and Powell.
Another equally important organization of a public nature, though not a
Federal bureau, traces its beginnings to the Geological Survey: the
Geophysical Laboratory of the Carnegie Institution, which now exercises so
potent an influence over geologic investigation, had its origin in the official
work of the Geological Survey’s Division of Chemical and Physical
Research, and its personnel was at first largely recruited from the Survey.
The highly original experimental work of this laboratory has extended far
beyond the scope of the Survey’s work—at least far beyond the scope
possible with the Federal funds available—yet most of the results of these
investigations may eventually come under even a strict construction of the
language used in the Survey’s appropriation “for chemical and physical
researches relating to the geology of the United States.”
The topographic work of the present Survey continues with constant
refinement of standards and economy of methods the work of the earlier
organizations. The primary purpose of these topographic surveys is to
provide the bases for geologic maps, yet these topographic maps, which
cover 40 per cent of the area of the United States, are used in every type of
civil engineering as well as by the public generally. The annual distribution
investigation of the water resources of the country, which is still an
important phase of the Survey’s activity, and led to the creation of an
independent organization—the Reclamation Service. It is easy to trace the
beginnings of Federal reclamation of arid lands in the pioneer work of
Powell, whose report in 1878 on the arid region of the United States was the
first adequate statement of the problem of largest use of these lands in terms
broader than those of individualistic endeavor. For years, however, Powell’s
appeal for Congressional consideration of this National task was like the
“voice of one crying in the wilderness.”
In a somewhat similar way the forestry surveys under the Geological
Survey helped in the organization of a separate bureau—now the Forest
Service. The other important Federal bureau tracing direct relationship to
the Survey is the Bureau of Mines, established in 1910, which continued the
investigations in mining technology specifically provided for by Congress
for six years under the Geological Survey but in some degree begun in the
early days of the Survey under Directors King and Powell.
Another equally important organization of a public nature, though not a
Federal bureau, traces its beginnings to the Geological Survey: the
Geophysical Laboratory of the Carnegie Institution, which now exercises so
potent an influence over geologic investigation, had its origin in the official
work of the Geological Survey’s Division of Chemical and Physical
Research, and its personnel was at first largely recruited from the Survey.
The highly original experimental work of this laboratory has extended far
beyond the scope of the Survey’s work—at least far beyond the scope
possible with the Federal funds available—yet most of the results of these
investigations may eventually come under even a strict construction of the
language used in the Survey’s appropriation “for chemical and physical
researches relating to the geology of the United States.”
The topographic work of the present Survey continues with constant
refinement of standards and economy of methods the work of the earlier
organizations. The primary purpose of these topographic surveys is to
provide the bases for geologic maps, yet these topographic maps, which
cover 40 per cent of the area of the United States, are used in every type of
civil engineering as well as by the public generally. The annual distribution
Page 233
by sale of half a million of these maps is an index of their value to the
people.
The hot discussion that was waged for years on the question of military
versus scientific administration of topographic surveys is in striking
contrast with the present concentration of all the topographic mapping
under the Geological Survey in those areas where it may best serve the
needs of the Army. In 1916 Congress specifically recognized the possibility
of greater cooperation of this kind, both in the appropriation made to the
Geological Survey and in a special appropriation made to the War
Department. For a number of years indeed special military information had
been contributed to the Army by the Survey topographers, but since March
26, 1917, every Geological Survey topographer has worked exclusively on
the program of military surveys laid down by the General Staff of the Army,
and the places of some of the 44 Survey topographers now in France as
engineer officers are filled by 34 other reserve engineer officers detailed by
order of the Secretary of War to the Director of the Geological Survey to
assist in this military mapping and to receive instruction fitting them in turn
for topographic service in France.
The contribution of this civilian service to the military operations in the
present emergency forms a fitting conclusion to this review of a century of
Government surveys. At present 215 members of the Geological Survey are
in uniform, 107 as engineer officers, two of whom are on the staff of the
American Commanding General in France. In the war work carried on in
the United States the Survey’s contribution is by no means limited to
military mapping: the geologists are also mobilized for meeting war needs,
assisting in developing new sources of the essential war minerals, in
speeding up production of mineral products, in collecting information for
the purchasing officers both of our own and of the Allied governments, in
coöperating with the constructing quarter-masters in the location of gravel
and sand for structural use and in both general and special examinations of
underground water supply and of drainage possibilities at cantonment sites,
and in supplying the Navy Department with similar technical data. A special
contribution has been the application to aërial surveys of photogrammetric
methods developed in the Alaskan topographic work and the perfection of a
camera specially adapted to airplane use. The utilization of the Survey’s
map engraving and printing plant for confidential and urgent work for both
the Army and Navy has necessitated postponement of current work for the
people.
The hot discussion that was waged for years on the question of military
versus scientific administration of topographic surveys is in striking
contrast with the present concentration of all the topographic mapping
under the Geological Survey in those areas where it may best serve the
needs of the Army. In 1916 Congress specifically recognized the possibility
of greater cooperation of this kind, both in the appropriation made to the
Geological Survey and in a special appropriation made to the War
Department. For a number of years indeed special military information had
been contributed to the Army by the Survey topographers, but since March
26, 1917, every Geological Survey topographer has worked exclusively on
the program of military surveys laid down by the General Staff of the Army,
and the places of some of the 44 Survey topographers now in France as
engineer officers are filled by 34 other reserve engineer officers detailed by
order of the Secretary of War to the Director of the Geological Survey to
assist in this military mapping and to receive instruction fitting them in turn
for topographic service in France.
The contribution of this civilian service to the military operations in the
present emergency forms a fitting conclusion to this review of a century of
Government surveys. At present 215 members of the Geological Survey are
in uniform, 107 as engineer officers, two of whom are on the staff of the
American Commanding General in France. In the war work carried on in
the United States the Survey’s contribution is by no means limited to
military mapping: the geologists are also mobilized for meeting war needs,
assisting in developing new sources of the essential war minerals, in
speeding up production of mineral products, in collecting information for
the purchasing officers both of our own and of the Allied governments, in
coöperating with the constructing quarter-masters in the location of gravel
and sand for structural use and in both general and special examinations of
underground water supply and of drainage possibilities at cantonment sites,
and in supplying the Navy Department with similar technical data. A special
contribution has been the application to aërial surveys of photogrammetric
methods developed in the Alaskan topographic work and the perfection of a
camera specially adapted to airplane use. The utilization of the Survey’s
map engraving and printing plant for confidential and urgent work for both
the Army and Navy has necessitated postponement of current work for the
Page 234
Geological Survey itself. Throughout the organization the records, the
methods, and the personnel which represent the product of many years of
scientific activity are all being utilized; thus is the experience of the past
translated into special service in the present crisis.
methods, and the personnel which represent the product of many years of
scientific activity are all being utilized; thus is the experience of the past
translated into special service in the present crisis.
Page 235
Notes.
96. Hess, R. H., Foundations of National Prosperity, p. 100.
97. Report Nat’l Museum, 1904, pp. 189–733.
98. Featherstonhaugh, J. D., Am. Geol., 3, 220, 1889.
99. Whitney, Mineral Wealth of the United States, pp. 248–250.
100. Foster and Whitney, 31st Cong., 1st session, House Doc. 69, pp. 13–14, 1850.
101. First Annual Rept. U. S. Geol. Survey, p. 4.
102. Wheeler, Report 3d Internat’l Geog. Cong., p. 492, 1885.
103. The views of the writer on “natural monopolies” in the Government service are set forth in
an address delivered at the centennial celebration of the U. S. Coast and Geodetic Survey, April 5,
1916. (See Science, vol. 43, pp. 659–665, May 12, 1916.)
104. For correspondence on this subject, see Minnesota Geol. Survey, Eighth Ann. Rept., 1880,
p. 173.
105. Owen, D. D., 30th Cong., 1st sess., Senate Doc. No. 57, p. 7, 1848.
106. This essential difference between present-day requirements and the needs of earlier
generations has been discussed by W. C. Mendenhall, the geologist in charge of the Land
Classification Board of the Geological Survey: Proceedings 2d Pan-American Sci. Cong., 1915–16,
3, 761.
96. Hess, R. H., Foundations of National Prosperity, p. 100.
97. Report Nat’l Museum, 1904, pp. 189–733.
98. Featherstonhaugh, J. D., Am. Geol., 3, 220, 1889.
99. Whitney, Mineral Wealth of the United States, pp. 248–250.
100. Foster and Whitney, 31st Cong., 1st session, House Doc. 69, pp. 13–14, 1850.
101. First Annual Rept. U. S. Geol. Survey, p. 4.
102. Wheeler, Report 3d Internat’l Geog. Cong., p. 492, 1885.
103. The views of the writer on “natural monopolies” in the Government service are set forth in
an address delivered at the centennial celebration of the U. S. Coast and Geodetic Survey, April 5,
1916. (See Science, vol. 43, pp. 659–665, May 12, 1916.)
104. For correspondence on this subject, see Minnesota Geol. Survey, Eighth Ann. Rept., 1880,
p. 173.
105. Owen, D. D., 30th Cong., 1st sess., Senate Doc. No. 57, p. 7, 1848.
106. This essential difference between present-day requirements and the needs of earlier
generations has been discussed by W. C. Mendenhall, the geologist in charge of the Land
Classification Board of the Geological Survey: Proceedings 2d Pan-American Sci. Cong., 1915–16,
3, 761.
Page 236
VI
ON THE DEVELOPMENT OF VERTEBRATE
PALEONTOLOGY
By RICHARD SWANN LULL
Introduction.
Unlike its sister science of Invertebrate Paleontology, which has been
approached so largely from the viewpoint of stratigraphic geology, that of
the vertebrates is essentially a biologic science, having its inception in the
masterly work of Cuvier, who is also to be regarded as the founder of
comparative anatomy. For long decades, vertebrate paleontology was
simply a branch of comparative anatomy or morphology in that it dealt
almost exclusively with the form and other peculiarities of fossil bones and
teeth, often in a more or less fragmentary condition, very little or no
attention being paid to any other system of the creature’s anatomy.
Distribution both in space and in time was recorded, but the value of
vertebrates in stratigraphy was still to be appreciated and has hardly yet
come into its own. It is readily seen, therefore, that the two departments of
paleontology did not enlist the same workers or even the same type of
investigators, for while the two sciences have much in common and should
have more, the vertebratist must, above all else, be a morphologist, with a
keen appreciation of form, and a mind capable of retaining endless
structural details and of visualizing as a whole what may be known only in
part. The initial work of the brilliant Cuvier set so high a standard of
preparedness and mental equipment that as a consequence, the number of
those engaged in vertebrate research has never been large as compared with
ON THE DEVELOPMENT OF VERTEBRATE
PALEONTOLOGY
By RICHARD SWANN LULL
Introduction.
Unlike its sister science of Invertebrate Paleontology, which has been
approached so largely from the viewpoint of stratigraphic geology, that of
the vertebrates is essentially a biologic science, having its inception in the
masterly work of Cuvier, who is also to be regarded as the founder of
comparative anatomy. For long decades, vertebrate paleontology was
simply a branch of comparative anatomy or morphology in that it dealt
almost exclusively with the form and other peculiarities of fossil bones and
teeth, often in a more or less fragmentary condition, very little or no
attention being paid to any other system of the creature’s anatomy.
Distribution both in space and in time was recorded, but the value of
vertebrates in stratigraphy was still to be appreciated and has hardly yet
come into its own. It is readily seen, therefore, that the two departments of
paleontology did not enlist the same workers or even the same type of
investigators, for while the two sciences have much in common and should
have more, the vertebratist must, above all else, be a morphologist, with a
keen appreciation of form, and a mind capable of retaining endless
structural details and of visualizing as a whole what may be known only in
part. The initial work of the brilliant Cuvier set so high a standard of
preparedness and mental equipment that as a consequence, the number of
those engaged in vertebrate research has never been large as compared with
Page 237
the workers in some other branches of science, but the results achieved by
the few who have consecrated their research to the fossil vertebrates has
been in the main of a high order.
At first, as has been emphasized, this work was largely morphological,
dealing both with the individual skeletal elements and later with the bony
framework as a whole. Then came the endeavor to clothe the bones with
sinews and with flesh—to imagine, in other words, the life-appearance of
the ages-departed form—with such of its habits as could be deduced from
structure of body, tooth, and limb. Next came the working out of systematic
series of vertebrates and their marshalling into species, genera, and larger
groups, and much time was thus spent, especially when rapid discovery
brought a continual stream of new forms before the systematist, and hence
some appreciation of the countless hosts of bygone creatures which peopled
the world in the geologic past. This systematic work, however, was based
upon the most painstaking morphologic comparisons and so the science was
still within the scope of comparative anatomy.
In connection with taxonomic research came increasingly tangible
evidence in favor of the law of evolution; investigators turned to the
working out of phyletic series showing the actual record of the successive
evolutionary changes that the various races had undergone. Coupled with
this evolutionary evidence came an increased attention to the sequential
occurrence in successive geologic strata, and the stratigraphic distribution
of vertebrates became known with greater and greater detail. Then followed
the assemblage of faunas, which brought the study of the fossil forms
within the realm of historical geology, rather than being the mere phylogeny
of a single race, and the value of vertebrate fossils as horizon markers
became more and more appreciated by the stratigrapher. They serve to
supplement the knowledge gained from the invertebrates, and in this
connection are especially valuable in that they often give data concerning
continental formations about which invertebrate paleontology is largely
silent.
the few who have consecrated their research to the fossil vertebrates has
been in the main of a high order.
At first, as has been emphasized, this work was largely morphological,
dealing both with the individual skeletal elements and later with the bony
framework as a whole. Then came the endeavor to clothe the bones with
sinews and with flesh—to imagine, in other words, the life-appearance of
the ages-departed form—with such of its habits as could be deduced from
structure of body, tooth, and limb. Next came the working out of systematic
series of vertebrates and their marshalling into species, genera, and larger
groups, and much time was thus spent, especially when rapid discovery
brought a continual stream of new forms before the systematist, and hence
some appreciation of the countless hosts of bygone creatures which peopled
the world in the geologic past. This systematic work, however, was based
upon the most painstaking morphologic comparisons and so the science was
still within the scope of comparative anatomy.
In connection with taxonomic research came increasingly tangible
evidence in favor of the law of evolution; investigators turned to the
working out of phyletic series showing the actual record of the successive
evolutionary changes that the various races had undergone. Coupled with
this evolutionary evidence came an increased attention to the sequential
occurrence in successive geologic strata, and the stratigraphic distribution
of vertebrates became known with greater and greater detail. Then followed
the assemblage of faunas, which brought the study of the fossil forms
within the realm of historical geology, rather than being the mere phylogeny
of a single race, and the value of vertebrate fossils as horizon markers
became more and more appreciated by the stratigrapher. They serve to
supplement the knowledge gained from the invertebrates, and in this
connection are especially valuable in that they often give data concerning
continental formations about which invertebrate paleontology is largely
silent.
Page 238
Rise of Vertebrate Paleontology in Europe.
To those who had been nurtured in the belief in a relatively recent
creation covering in its entirety a period of but six days, and occurring but
four millenniums before the time of Christ, the appearance of the remains of
creatures in the rocks, the like of which no man ever saw alive, must have
given scope to the wildest imaginings concerning their origin and
significance; for many believed that not only had no new forms been added
to the world’s fauna since the creation, except possibly by hybridizing, but
that none had become extinct save a very few through the agency of human
interference. The supposition was, therefore, that such creatures as were
thus discovered were still extant in some more remote fastnesses of the
world. Thus, our second president, Thomas Jefferson, who wrote one of the
first papers on American fossil vertebrates, published in 1798, discussed
therein the remains of a huge ground-sloth which has since borne the name
Megalonyx jeffersoni. Jefferson, however, described the great claws as
pertaining to a huge leonine animal which he firmly believed was yet living
among the mountains of Virginia.
Cuvier (1769–1832) has been spoken of as the founder of our science.
His opportunity lay in the profusion of bones buried in the gypsum deposits
of Montmartre within the environs of the city of Paris. Cuvier’s studies of
these remains, done in the light of his very broad anatomical knowledge,
enabled him to prepare the first reconstructions of fossil vertebrates ever
attempted and to bring before the eyes of his contemporaries a world
peopled with forms which were utterly extinct. That these creatures were no
longer living, none was a better judge than Cuvier, for his prominence was
such that material was sent him from all parts of the world, to which must
be added that which he saw in his visits to the various museums of Europe.
He felt it safe, therefore, to affirm the unlikelihood of any further discovery
of unknown forms among the great mammals of the present fauna of our
globe, and few indeed have been the additions since his day. To Cuvier is
due not alone the masterly contribution to the sister sciences of comparative
anatomy and vertebrate paleontology—the Ossements Fossiles (1812)—but
he also announced the presence in continental strata of a series of faunas
which showed a gradual organic improvement from the earliest such
To those who had been nurtured in the belief in a relatively recent
creation covering in its entirety a period of but six days, and occurring but
four millenniums before the time of Christ, the appearance of the remains of
creatures in the rocks, the like of which no man ever saw alive, must have
given scope to the wildest imaginings concerning their origin and
significance; for many believed that not only had no new forms been added
to the world’s fauna since the creation, except possibly by hybridizing, but
that none had become extinct save a very few through the agency of human
interference. The supposition was, therefore, that such creatures as were
thus discovered were still extant in some more remote fastnesses of the
world. Thus, our second president, Thomas Jefferson, who wrote one of the
first papers on American fossil vertebrates, published in 1798, discussed
therein the remains of a huge ground-sloth which has since borne the name
Megalonyx jeffersoni. Jefferson, however, described the great claws as
pertaining to a huge leonine animal which he firmly believed was yet living
among the mountains of Virginia.
Cuvier (1769–1832) has been spoken of as the founder of our science.
His opportunity lay in the profusion of bones buried in the gypsum deposits
of Montmartre within the environs of the city of Paris. Cuvier’s studies of
these remains, done in the light of his very broad anatomical knowledge,
enabled him to prepare the first reconstructions of fossil vertebrates ever
attempted and to bring before the eyes of his contemporaries a world
peopled with forms which were utterly extinct. That these creatures were no
longer living, none was a better judge than Cuvier, for his prominence was
such that material was sent him from all parts of the world, to which must
be added that which he saw in his visits to the various museums of Europe.
He felt it safe, therefore, to affirm the unlikelihood of any further discovery
of unknown forms among the great mammals of the present fauna of our
globe, and few indeed have been the additions since his day. To Cuvier is
due not alone the masterly contribution to the sister sciences of comparative
anatomy and vertebrate paleontology—the Ossements Fossiles (1812)—but
he also announced the presence in continental strata of a series of faunas
which showed a gradual organic improvement from the earliest such
Page 239
assemblage to the most modern, an idea of the most fundamental
importance and one with which he is rarely credited. He believed in the
sudden and complete extinction of faunas, and the facts then known were in
accord with this idea, as no common genera nor transitional forms
connected the creatures of the Paris gypsum with the mastodons, elephants,
and hippopotami which the later strata disclosed. It is not remarkable,
therefore, that Cuvier advanced his theory of catastrophism to account for
these extinctions. He should not, however, according to Depéret, be credited
with the idea of successive re-creations, such as that held by D’Orbigny and
others, but of repopulation by immigration from some area which the
catastrophe, be it flood or other destructive agency, failed to reach.
Cuvier was followed in Europe by a number of illustrious men, none of
whom, however, with the exception of Sir Richard Owen, possessed his
breadth of knowledge of comparative anatomy upon which to base their
researches among the prehistoric. The more notable of them may be
enumerated before going on to a discussion of the American contributions
to the science.
They were, first, Louis Agassiz, a pupil of Cuvier and later a resident of
America, whose researches on the fossil fishes of Europe are a monumental
work, the result of ten years of investigation in all of the larger museums of
that continent, and which appeared in 1833–43, while he was yet a young
man. The fishes were practically the only fossil vertebrates to come within
the scope of his investigations, for his later time was consumed in the study
of glaciers and of recent marine zoology. Another student of these most
primitive vertebrates who left an enduring monument was Johannes Mϋller.
Huxley, Traquair, and Jaekel also did masterly work upon this group, while
Smith Woodward of the British Museum is considered the highest living
authority upon fossil fishes.
Of the Amphibia, the most famous foreign students were Brongniart,
Jaeger, Burmeister, Von Meyer, and Owen, although Owen’s claim to
eminence lies rather in the investigations of fossil reptiles which he began
in 1839 and continued over a period of fifty years of remarkable
achievement. Not only did he describe the dinosaurs of Great Britain in a
series of splendidly illustrated monographs, but extended his researches to
the curious reptilian forms from the Karroo formation of South Africa. It
was to him, moreover, that the establishment of the true position of the
importance and one with which he is rarely credited. He believed in the
sudden and complete extinction of faunas, and the facts then known were in
accord with this idea, as no common genera nor transitional forms
connected the creatures of the Paris gypsum with the mastodons, elephants,
and hippopotami which the later strata disclosed. It is not remarkable,
therefore, that Cuvier advanced his theory of catastrophism to account for
these extinctions. He should not, however, according to Depéret, be credited
with the idea of successive re-creations, such as that held by D’Orbigny and
others, but of repopulation by immigration from some area which the
catastrophe, be it flood or other destructive agency, failed to reach.
Cuvier was followed in Europe by a number of illustrious men, none of
whom, however, with the exception of Sir Richard Owen, possessed his
breadth of knowledge of comparative anatomy upon which to base their
researches among the prehistoric. The more notable of them may be
enumerated before going on to a discussion of the American contributions
to the science.
They were, first, Louis Agassiz, a pupil of Cuvier and later a resident of
America, whose researches on the fossil fishes of Europe are a monumental
work, the result of ten years of investigation in all of the larger museums of
that continent, and which appeared in 1833–43, while he was yet a young
man. The fishes were practically the only fossil vertebrates to come within
the scope of his investigations, for his later time was consumed in the study
of glaciers and of recent marine zoology. Another student of these most
primitive vertebrates who left an enduring monument was Johannes Mϋller.
Huxley, Traquair, and Jaekel also did masterly work upon this group, while
Smith Woodward of the British Museum is considered the highest living
authority upon fossil fishes.
Of the Amphibia, the most famous foreign students were Brongniart,
Jaeger, Burmeister, Von Meyer, and Owen, although Owen’s claim to
eminence lies rather in the investigations of fossil reptiles which he began
in 1839 and continued over a period of fifty years of remarkable
achievement. Not only did he describe the dinosaurs of Great Britain in a
series of splendidly illustrated monographs, but extended his researches to
the curious reptilian forms from the Karroo formation of South Africa. It
was to him, moreover, that the establishment of the true position of the
Page 240
famous Archœopteryx as the earliest known bird and not a reptile is due.
Von Meyer also enriched the literature of fossil reptiles, discussing
exhaustively those occurring in Germany, while Huxley’s classic work on
the crocodiles as well as on dinosaurs, and the labors of Buckland, Fraas,
Koken, Von Huene, Gaudry, Hulke, Seeley, and Lydekker have added
immensely to our knowledge of the group.
Of the birds, which at best are rare as fossils, our knowledge, especially
of the huge flightless moas, is due largely again to Owen, and his
realization of the systematic position of Archœopteryx has already been
mentioned.
The mammals were, perhaps, the most prolific source of paleontological
research during the nineteenth century, for, as Zittel has said, Cuvier’s
famous investigations on the fossil bones, mentioned above, not only
contain the principles of comparative osteology, but also show in a manner
which has never been surpassed how fossil vertebrates ought to be studied,
and what are the broad inductions which may be drawn from a series of
methodical observations. Such was Cuvier’s influence that until Darwin
began to interest himself in mammalian paleontology the study of these
forms was conducted entirely along the lines indicated by the French
savant. This was seen in a large work, Osteology of Recent and Fossil
Mammalia, by De Blainville, which, although not up to the standard set by
the master, is nevertheless a notable contribution, as was also the Osteology
prepared by Pander and D’Alton. A summary of the knowledge of the fossil
Mammalia up to the year 1847 is contained in Giebel’s Fauna der Vorwelt,
and Lydekker has done for the mammals in the British Museum what Smith
Woodward did for the fishes, producing vastly more than the mere
catalogue which the title implies.
The first work wherein the fossil mammals were treated genealogically
was Gaudry’s Enchaînements du Monde Animal, written in 1878. Other
work on the fossil Mammalia was done by Kaup, who described those from
the Mainz basin and from Epplesheim near Worms whence came one of the
most famous of prehistoric horses, the Hipparion; this horse, together with
the remarkable proboscidean Dinotherium, was described by Von Meyer.
One of the most remarkable discoveries, ranking in importance, perhaps,
next to Montmartre, was that of the Pliocene fauna of Pikermi near Athens,
Greece, first made known through the publications of A. Wagner of Munich
Von Meyer also enriched the literature of fossil reptiles, discussing
exhaustively those occurring in Germany, while Huxley’s classic work on
the crocodiles as well as on dinosaurs, and the labors of Buckland, Fraas,
Koken, Von Huene, Gaudry, Hulke, Seeley, and Lydekker have added
immensely to our knowledge of the group.
Of the birds, which at best are rare as fossils, our knowledge, especially
of the huge flightless moas, is due largely again to Owen, and his
realization of the systematic position of Archœopteryx has already been
mentioned.
The mammals were, perhaps, the most prolific source of paleontological
research during the nineteenth century, for, as Zittel has said, Cuvier’s
famous investigations on the fossil bones, mentioned above, not only
contain the principles of comparative osteology, but also show in a manner
which has never been surpassed how fossil vertebrates ought to be studied,
and what are the broad inductions which may be drawn from a series of
methodical observations. Such was Cuvier’s influence that until Darwin
began to interest himself in mammalian paleontology the study of these
forms was conducted entirely along the lines indicated by the French
savant. This was seen in a large work, Osteology of Recent and Fossil
Mammalia, by De Blainville, which, although not up to the standard set by
the master, is nevertheless a notable contribution, as was also the Osteology
prepared by Pander and D’Alton. A summary of the knowledge of the fossil
Mammalia up to the year 1847 is contained in Giebel’s Fauna der Vorwelt,
and Lydekker has done for the mammals in the British Museum what Smith
Woodward did for the fishes, producing vastly more than the mere
catalogue which the title implies.
The first work wherein the fossil mammals were treated genealogically
was Gaudry’s Enchaînements du Monde Animal, written in 1878. Other
work on the fossil Mammalia was done by Kaup, who described those from
the Mainz basin and from Epplesheim near Worms whence came one of the
most famous of prehistoric horses, the Hipparion; this horse, together with
the remarkable proboscidean Dinotherium, was described by Von Meyer.
One of the most remarkable discoveries, ranking in importance, perhaps,
next to Montmartre, was that of the Pliocene fauna of Pikermi near Athens,
Greece, first made known through the publications of A. Wagner of Munich
Page 241
and later, and much more extensively, through that of Gaudry (1862–1867).
H. von Meyer was Germany’s best authority on fossil Mammalia. After his
death the work was carried on by Quenstedt, Oscar Fraas, Schlosser, Koken,
and Pohlig, among others.
In France, rich deposits of fossil mammals were discovered in the
Department of Puy-de-Dôme, the Rhone basin, Sansan, Quercy, and near
Rheims. These were described by a number of writers, notably Croizet and
Jobert, Pomel, Lartet, Filhol, and Lemoine.
Rütimeyer of Bâle was one of the most famous European writers on
mammalian paleontology, and his researches were both comprehensive and
clothed in such form as to give them a high place in paleontological
literature. He studied comparatively the teeth of ungulates, discussed the
genealogy of mammals, and the relationships of those of the Old and New
Worlds. He was an exponent of the law of evolution as set forth by Darwin,
and his “genealogical trees of the Mammalia show a complete knowledge
of all the data concerning the different members in the succession, and are
amongst the finest results hitherto obtained by means of strict scientific
methods of investigation” (Zittel, History of Geology and Palæontology,
1901). The mammals of the Swiss Eocene have been studied in much detail
by Stehlin.
For Great Britain, the most notable contributors were Buckland in his
Reliquiæ Diluvianæ; Falconer, co-author with Cautley on the Tertiary
mammals of India; Charles Murchison, who wrote on rhinoceroses and
proboscideans; and more recently Bush, Flower, Lydekker, Boyd Dawkins,
L. Adams, and C. W. Andrews. But by far the most commanding figure of
all was Sir Richard Owen, who for half a century stood without a peer as
the greatest of authorities on fossil mammals. It was the Natural History of
the British Fossil Mammals and Birds, published in 1846, that established
Sir Richard’s reputation.
Russia has produced much mammalian material, especially from the
Tertiary of Odessa and Bessarabia, and from the Quaternary of northern
Russia and Siberia. These have been described mainly by J. F. Brandt, A.
von Nordmann, but especially by Mme. M. Pavlow of Moscow.
Forsyth-Major discovered in 1887 a fauna contemporaneous with that of
Pikermi in the Island of Samos in the Mediterranean.
H. von Meyer was Germany’s best authority on fossil Mammalia. After his
death the work was carried on by Quenstedt, Oscar Fraas, Schlosser, Koken,
and Pohlig, among others.
In France, rich deposits of fossil mammals were discovered in the
Department of Puy-de-Dôme, the Rhone basin, Sansan, Quercy, and near
Rheims. These were described by a number of writers, notably Croizet and
Jobert, Pomel, Lartet, Filhol, and Lemoine.
Rütimeyer of Bâle was one of the most famous European writers on
mammalian paleontology, and his researches were both comprehensive and
clothed in such form as to give them a high place in paleontological
literature. He studied comparatively the teeth of ungulates, discussed the
genealogy of mammals, and the relationships of those of the Old and New
Worlds. He was an exponent of the law of evolution as set forth by Darwin,
and his “genealogical trees of the Mammalia show a complete knowledge
of all the data concerning the different members in the succession, and are
amongst the finest results hitherto obtained by means of strict scientific
methods of investigation” (Zittel, History of Geology and Palæontology,
1901). The mammals of the Swiss Eocene have been studied in much detail
by Stehlin.
For Great Britain, the most notable contributors were Buckland in his
Reliquiæ Diluvianæ; Falconer, co-author with Cautley on the Tertiary
mammals of India; Charles Murchison, who wrote on rhinoceroses and
proboscideans; and more recently Bush, Flower, Lydekker, Boyd Dawkins,
L. Adams, and C. W. Andrews. But by far the most commanding figure of
all was Sir Richard Owen, who for half a century stood without a peer as
the greatest of authorities on fossil mammals. It was the Natural History of
the British Fossil Mammals and Birds, published in 1846, that established
Sir Richard’s reputation.
Russia has produced much mammalian material, especially from the
Tertiary of Odessa and Bessarabia, and from the Quaternary of northern
Russia and Siberia. These have been described mainly by J. F. Brandt, A.
von Nordmann, but especially by Mme. M. Pavlow of Moscow.
Forsyth-Major discovered in 1887 a fauna contemporaneous with that of
Pikermi in the Island of Samos in the Mediterranean.
Page 242
One of the most remarkable recent discoveries of fossil localities was that
announced in 1901 by Mr. Hugh J. L. Beadnell of the Geological Survey of
Egypt and Doctor C. W. Andrews of the British Museum of London, of
numerous land and sea mammals of Upper Eocene and Lower Oligocene
age in northern Egypt. The exposures lay about 80 miles southwest of Cairo
in the Fayûm district and are the sediments of an ancient Tertiary lake, a
relic of which, Birket-el-Qurun, yet remains. These beds contained ancient
Hyracoidea, Sirenia, and Zeuglodontia, but above all, ancestral Proboscidea
which, together with those known elsewhere, enabled Andrews to
demonstrate the origin and evolutionary features of this most remarkable
group of beasts. This discovery in the Fayûm lends color to the belief that
Africa may have been the ancestral home of at least five of the mammalian
orders, those mentioned above, together with the Embrithopoda, a group
unknown elsewhere. This theory had been advanced independently by
Tullberg, Stehlin, and Osborn, before the discovery in Egypt.
Another European worker of pre-eminence who wrote more broadly than
the faunal studies mentioned above was W. Kowalewsky. He discussed
especially the evolutionary changes of feet and teeth in ungulates, a line of
research afterward developed in greater detail by the Americans, Cope and
Osborn.
South America has yielded series of rich faunas which have been
exploited by the great Argentinian, Florentino Ameghino, and by the
Europeans, Owen, Gervais, Huxley, Von Meyer, and more recently by
Burmeister and Lydekker. Later exploration and research by Hatcher and
Scott of North America will be discussed further on in this paper.
announced in 1901 by Mr. Hugh J. L. Beadnell of the Geological Survey of
Egypt and Doctor C. W. Andrews of the British Museum of London, of
numerous land and sea mammals of Upper Eocene and Lower Oligocene
age in northern Egypt. The exposures lay about 80 miles southwest of Cairo
in the Fayûm district and are the sediments of an ancient Tertiary lake, a
relic of which, Birket-el-Qurun, yet remains. These beds contained ancient
Hyracoidea, Sirenia, and Zeuglodontia, but above all, ancestral Proboscidea
which, together with those known elsewhere, enabled Andrews to
demonstrate the origin and evolutionary features of this most remarkable
group of beasts. This discovery in the Fayûm lends color to the belief that
Africa may have been the ancestral home of at least five of the mammalian
orders, those mentioned above, together with the Embrithopoda, a group
unknown elsewhere. This theory had been advanced independently by
Tullberg, Stehlin, and Osborn, before the discovery in Egypt.
Another European worker of pre-eminence who wrote more broadly than
the faunal studies mentioned above was W. Kowalewsky. He discussed
especially the evolutionary changes of feet and teeth in ungulates, a line of
research afterward developed in greater detail by the Americans, Cope and
Osborn.
South America has yielded series of rich faunas which have been
exploited by the great Argentinian, Florentino Ameghino, and by the
Europeans, Owen, Gervais, Huxley, Von Meyer, and more recently by
Burmeister and Lydekker. Later exploration and research by Hatcher and
Scott of North America will be discussed further on in this paper.
Page 243
Vertebrate Paleontology in America.
Early Writers.—Having thus summarized paleontological progress in the
Old World, we can turn to a consideration of the work done in the New,
especially in the United States, because while the Old World investigation
has been invaluable, a science of vertebrate paleontology, very complete
both as to its zoological and geological scope and in the extent and value of
published results, could be built exclusively upon the discoveries and
researches made by Americans. The science of vertebrate paleontology may
be said to have had its beginnings in North America with the activities of
Thomas Jefferson, who, like Franklin, felt so strong an interest in scientific
pursuits that even the graver duties of the highest office in the gift of the
American people could not deter him from them. When in 1797 Jefferson
came to be inaugurated as vice-president of the United States, he brought
with him to Philadelphia not only his manuscript but the actual fossil bones
upon which it was based. Again in 1801 he was greatly interested in the
Shawangunk mastodon, despite heavy cares of state, and in 1808 made part
of the executive mansion in Washington serve as a paleontological
laboratory, displaying therein for study the bones of proboscideans and their
contemporaries which the Big Bone Lick of Kentucky had produced.
Jefferson’s work would not, perhaps, have been epoch-making were it not
for its unique chronological position in the annals of the science.
Jefferson was followed by another man—this time one whose diverging
lines of interest led him not into the realm of political service, but of art, for
Rembrandt Peale possessed an enviable reputation among the early painters
of America. Peale published in 1802 an account of the skeleton of the
“mammoth,” really the mastodon, M. americanus, speaking of it as a
nondescript carnivorous animal of immense size found in America. It was
because of the form of the molar teeth that Peale said of it: “If this animal
was indeed carnivorous, which I believe cannot be doubted, though we may
as philosophers regret it, as men we cannot but thank Heaven that its whole
generation is probably extinct.”
With the work of these men as a beginning, it is not strange that the more
conspicuous Pleistocene fossils of the East should have attracted the
attention of many subsequent writers in the first part of the nineteenth
Early Writers.—Having thus summarized paleontological progress in the
Old World, we can turn to a consideration of the work done in the New,
especially in the United States, because while the Old World investigation
has been invaluable, a science of vertebrate paleontology, very complete
both as to its zoological and geological scope and in the extent and value of
published results, could be built exclusively upon the discoveries and
researches made by Americans. The science of vertebrate paleontology may
be said to have had its beginnings in North America with the activities of
Thomas Jefferson, who, like Franklin, felt so strong an interest in scientific
pursuits that even the graver duties of the highest office in the gift of the
American people could not deter him from them. When in 1797 Jefferson
came to be inaugurated as vice-president of the United States, he brought
with him to Philadelphia not only his manuscript but the actual fossil bones
upon which it was based. Again in 1801 he was greatly interested in the
Shawangunk mastodon, despite heavy cares of state, and in 1808 made part
of the executive mansion in Washington serve as a paleontological
laboratory, displaying therein for study the bones of proboscideans and their
contemporaries which the Big Bone Lick of Kentucky had produced.
Jefferson’s work would not, perhaps, have been epoch-making were it not
for its unique chronological position in the annals of the science.
Jefferson was followed by another man—this time one whose diverging
lines of interest led him not into the realm of political service, but of art, for
Rembrandt Peale possessed an enviable reputation among the early painters
of America. Peale published in 1802 an account of the skeleton of the
“mammoth,” really the mastodon, M. americanus, speaking of it as a
nondescript carnivorous animal of immense size found in America. It was
because of the form of the molar teeth that Peale said of it: “If this animal
was indeed carnivorous, which I believe cannot be doubted, though we may
as philosophers regret it, as men we cannot but thank Heaven that its whole
generation is probably extinct.”
With the work of these men as a beginning, it is not strange that the more
conspicuous Pleistocene fossils of the East should have attracted the
attention of many subsequent writers in the first part of the nineteenth
Page 244
century, nor that the early papers to appear in the Journal should pertain to
proboscideans or to the huge edentate ground-sloths and the aberrant
zeuglodons whose bones frequently came to light. Therefore a number of
men such as Koch, both Sillimans, J. C. Warren, and others made these
forms their chief concern.
Fossil Footprints.—Among the early writers who concerned themselves
with these greater fossils was Edward Hitchcock, sometime president of
Amherst College, and a geologist of high repute among his contemporaries.
Hitchcock is, however, better and more widely known as the pioneer worker
on a series of phenomena displayed as in no other place in the region in
which he made his home. These are fossil footprints impressed upon the
Triassic rocks of the Connecticut valley. It was in the Journal for the year
1836 (29, 307–340) that Hitchcock first called attention to the footmarks,
although they had been known and discussed popularly for a number of
years previous. James Deane, of Greenfield, was perhaps the first to
appreciate the scientific interest of these phenomena, but deeming his own
qualifications insufficient properly to describe them, he brought them to the
attention of Hitchcock, and the interest of the latter never waned until his
death in 1864. Hitchcock wrote paper after paper, publishing many of them
in the Journal, again in his Final Report on the Geology of Massachusetts
(1841), and later in quarto works, one in the Memoirs of the American
Academy of Arts and Sciences and the two others under the authority of the
Commonwealth, the Ichnology in 1858, and the Supplement in 1865, the
last being a posthumous work edited by his son, Charles H. Hitchcock.
Hitchcock’s conception of the track-makers was more or less imperfect
because of the fact that for a long time but a few fragmentary osseous
remains were known, either directly or indirectly associated with the tracks,
while on the other hand the bird-like character of many of the latter and the
discovery of huge flightless birds elsewhere on the globe suggested a very
close analogy if not a direct relationship. Hence “bird tracks” they were
straightway called, a designation which it has been difficult to remove, even
though in 1843 Owen called attention to the need of caution in assuming the
existence of so highly organized birds at so early a period, especially when
large reptiles were known which might readily form very similar tracks.
The footprints are now believed to be very largely of dinosaurian origin,
and dinosaurs whose feet corresponded in every detail with the footprints
have actually come to light within the same geologic and geographic
proboscideans or to the huge edentate ground-sloths and the aberrant
zeuglodons whose bones frequently came to light. Therefore a number of
men such as Koch, both Sillimans, J. C. Warren, and others made these
forms their chief concern.
Fossil Footprints.—Among the early writers who concerned themselves
with these greater fossils was Edward Hitchcock, sometime president of
Amherst College, and a geologist of high repute among his contemporaries.
Hitchcock is, however, better and more widely known as the pioneer worker
on a series of phenomena displayed as in no other place in the region in
which he made his home. These are fossil footprints impressed upon the
Triassic rocks of the Connecticut valley. It was in the Journal for the year
1836 (29, 307–340) that Hitchcock first called attention to the footmarks,
although they had been known and discussed popularly for a number of
years previous. James Deane, of Greenfield, was perhaps the first to
appreciate the scientific interest of these phenomena, but deeming his own
qualifications insufficient properly to describe them, he brought them to the
attention of Hitchcock, and the interest of the latter never waned until his
death in 1864. Hitchcock wrote paper after paper, publishing many of them
in the Journal, again in his Final Report on the Geology of Massachusetts
(1841), and later in quarto works, one in the Memoirs of the American
Academy of Arts and Sciences and the two others under the authority of the
Commonwealth, the Ichnology in 1858, and the Supplement in 1865, the
last being a posthumous work edited by his son, Charles H. Hitchcock.
Hitchcock’s conception of the track-makers was more or less imperfect
because of the fact that for a long time but a few fragmentary osseous
remains were known, either directly or indirectly associated with the tracks,
while on the other hand the bird-like character of many of the latter and the
discovery of huge flightless birds elsewhere on the globe suggested a very
close analogy if not a direct relationship. Hence “bird tracks” they were
straightway called, a designation which it has been difficult to remove, even
though in 1843 Owen called attention to the need of caution in assuming the
existence of so highly organized birds at so early a period, especially when
large reptiles were known which might readily form very similar tracks.
The footprints are now believed to be very largely of dinosaurian origin,
and dinosaurs whose feet corresponded in every detail with the footprints
have actually come to light within the same geologic and geographic
Page 245
limitations. This of course refers to the bipedal, functionally three-toed
tracks. Of the makers of certain of the obscurer of the quadrupedal trails we
are as much in the dark to-day as were the first discoverers of a century ago,
so far as demonstrable proof is concerned. We assume, however, that they
were the tracks of amphibia and reptiles, beyond which we may not go with
certainty.
Agassiz, writing in 1865 (Geological Sketches), says:
“To sum up my opinion respecting these footmarks, I believe that they were made by animals of a
prophetic type, belonging to the class of reptiles, and exhibiting many synthetic characters. The more
closely we study past creations, the more impressive and significant do the synthetic types,
presenting features of the higher classes under the guise of the lower ones, become. They hold the
promise of the future. As the opening overture of an opera contains all the musical elements to be
therein developed, so this living prelude of the creative work comprises all the organic elements to be
successively developed in the course of time.”
Of those whose work was contemporaneous with that of Hitchcock, but
one, W. C. Redfield, wrote on Triassic phenomena, and he concerned
himself mainly with the fossil fishes of that time, his first paper on this
subject appearing in 1837 in the Journal (34, 201), and the last twenty years
later.
Paleozoic Vertebrates.—Later the vertebrates of the Paleozoic began to
attract attention, footprints from Pennsylvania being described by Isaac Lea,
beginning in 1849, a notice of his first paper appearing in the Journal for
that year (9, 124). Several papers followed on the reptile Clepsysaurus.
Alfred King also wrote on the Carboniferous ichnites, his work slightly
antedating that of Lea, but being less authoritative.
But by far the most illuminating of the mid-century writers on Paleozoic
vertebrates was Sir William Dawson, a very large proportion of whose
numerous papers relate to the Coal Measures of Nova Scotia and their
contained plant and animal remains. In 1853 appeared Dawson’s first
announcement, written in collaboration with Sir Charles Lyell, of the
finding of the bones of vertebrates within the base of an upright fossil tree
trunk at South Joggins. These bones were identified by Owen and Wyman
as pertaining to a reptilian or amphibian to which the name Dendrerpeton
acadianum was given. Following this were several papers published in the
Quarterly Journal of the Geological Society, London, describing more
tracks. Of the makers of certain of the obscurer of the quadrupedal trails we
are as much in the dark to-day as were the first discoverers of a century ago,
so far as demonstrable proof is concerned. We assume, however, that they
were the tracks of amphibia and reptiles, beyond which we may not go with
certainty.
Agassiz, writing in 1865 (Geological Sketches), says:
“To sum up my opinion respecting these footmarks, I believe that they were made by animals of a
prophetic type, belonging to the class of reptiles, and exhibiting many synthetic characters. The more
closely we study past creations, the more impressive and significant do the synthetic types,
presenting features of the higher classes under the guise of the lower ones, become. They hold the
promise of the future. As the opening overture of an opera contains all the musical elements to be
therein developed, so this living prelude of the creative work comprises all the organic elements to be
successively developed in the course of time.”
Of those whose work was contemporaneous with that of Hitchcock, but
one, W. C. Redfield, wrote on Triassic phenomena, and he concerned
himself mainly with the fossil fishes of that time, his first paper on this
subject appearing in 1837 in the Journal (34, 201), and the last twenty years
later.
Paleozoic Vertebrates.—Later the vertebrates of the Paleozoic began to
attract attention, footprints from Pennsylvania being described by Isaac Lea,
beginning in 1849, a notice of his first paper appearing in the Journal for
that year (9, 124). Several papers followed on the reptile Clepsysaurus.
Alfred King also wrote on the Carboniferous ichnites, his work slightly
antedating that of Lea, but being less authoritative.
But by far the most illuminating of the mid-century writers on Paleozoic
vertebrates was Sir William Dawson, a very large proportion of whose
numerous papers relate to the Coal Measures of Nova Scotia and their
contained plant and animal remains. In 1853 appeared Dawson’s first
announcement, written in collaboration with Sir Charles Lyell, of the
finding of the bones of vertebrates within the base of an upright fossil tree
trunk at South Joggins. These bones were identified by Owen and Wyman
as pertaining to a reptilian or amphibian to which the name Dendrerpeton
acadianum was given. Following this were several papers published in the
Quarterly Journal of the Geological Society, London, describing more
Page 246
vertebrates and associated terrestrial molluscs. In 1863 Dawson
summarized his discoveries in the Journal (36, 430–432) under the title of
“Air-breathers of the Coal Period,” a paper which was expanded and
published under the same title in the Canadian Naturalist and Geologist for
the same year. Dawson also printed in the same volume the first account of
reptilian(?) footprints from the coal. Thus from time to time there emanated
from his prolific pen the account of further discoveries, both in bones and
footprints, his final synopsis of the air-breathing animals of the Paleozoic of
Canada appearing in 1895. The only other group of vertebrates which
claimed his attention were certain whales, on which he occasionally wrote.
Fishes.—The fossil fishes from the Devonian of Ohio found their first
exponent in J. S. Newberry, appointed chief geologist of the second
geological survey of Ohio, which was established in 1869. These fishes
from the Devonian shales belonged for the greater part to the curious group
of armored placoderms, the remains of which consist very largely of armor
plates with little or no traces of internal skeleton. There was also found in
association a shark, Cladoselache, of such marvelous preservation that from
some of the Newberry specimens now in the American Museum of Natural
History, New York, Bashford Dean has demonstrated the histology of
muscle and visceral organs, in addition to the very complete skeletal
remains.
Newberry’s work on these forms, begun in 1868, has been carried to
further completion by Bashford Dean and his pupil L. Hussakof, as well as
by C. R. Eastman. Newberry’s other paleontological work was with the
Carboniferous fishes of Ohio, the Carboniferous and Triassic fishes of the
region from Sante Fé to the Grand and Green rivers, Colorado, and on the
fishes and plants of the Newark system of the Connecticut valley and New
Jersey. He also discussed certain mastodon and mammoth remains, and
those of the peccary of Ohio, Dicotyles.
summarized his discoveries in the Journal (36, 430–432) under the title of
“Air-breathers of the Coal Period,” a paper which was expanded and
published under the same title in the Canadian Naturalist and Geologist for
the same year. Dawson also printed in the same volume the first account of
reptilian(?) footprints from the coal. Thus from time to time there emanated
from his prolific pen the account of further discoveries, both in bones and
footprints, his final synopsis of the air-breathing animals of the Paleozoic of
Canada appearing in 1895. The only other group of vertebrates which
claimed his attention were certain whales, on which he occasionally wrote.
Fishes.—The fossil fishes from the Devonian of Ohio found their first
exponent in J. S. Newberry, appointed chief geologist of the second
geological survey of Ohio, which was established in 1869. These fishes
from the Devonian shales belonged for the greater part to the curious group
of armored placoderms, the remains of which consist very largely of armor
plates with little or no traces of internal skeleton. There was also found in
association a shark, Cladoselache, of such marvelous preservation that from
some of the Newberry specimens now in the American Museum of Natural
History, New York, Bashford Dean has demonstrated the histology of
muscle and visceral organs, in addition to the very complete skeletal
remains.
Newberry’s work on these forms, begun in 1868, has been carried to
further completion by Bashford Dean and his pupil L. Hussakof, as well as
by C. R. Eastman. Newberry’s other paleontological work was with the
Carboniferous fishes of Ohio, the Carboniferous and Triassic fishes of the
region from Sante Fé to the Grand and Green rivers, Colorado, and on the
fishes and plants of the Newark system of the Connecticut valley and New
Jersey. He also discussed certain mastodon and mammoth remains, and
those of the peccary of Ohio, Dicotyles.
Page 247
Joseph Leidy (1823–1891).
We now come to a consideration of the work of Joseph Leidy, one of the
three great pioneers in American vertebrate paleontology, for if we
disregard the work of Hitchcock and others on the fossil footprints, few of
the results thus far obtained were based upon the fruits of organized
research. Leidy began his publication in 1847 and continued to issue papers
and books from time to time until the year 1892, having published no fewer
than 219 paleontological titles, and 553 all told. His earlier paleontological
researches were exclusively on the Mammalia, which were then coming in
from the newly discovered fossil localities of the West. The discovery of
these forms, one of the most notable events in the history of our science,
will bear re-telling.
The first announcement was made in 1847, when Hiram A. Prout of St.
Louis published in the Journal (3, 248–250) the description of the maxillary
bone of “Palæotherium” (= Titanotherium proutii)from near White River,
Nebraska. This at once drew the attention of geologists and paleontologists
to the Bad Lands, or Mauvaises Terres, which were to prove so highly
productive of fossil forms. About the same time S. D. Culbertson of
Chambersburg, Pennsylvania, submitted to the Academy of Natural
Sciences at Philadelphia some fossils sent to him from Nebraska by
Alexander Culbertson. These were afterward described by Leidy in the
Proceedings of the Academy, together with the paleotheroid jaw, in addition
to which three other collections which had been made were also placed at
his disposal for study.
This aroused the interest of Doctor Spencer F. Baird of the Smithsonian
Institution, who sent T. A. Culbertson to the Bad Lands to make further
collections. The latter was successful in securing a valuable series of
mammalian and chelonian remains. These, together with other specimens
from the same locality, were sent to Leidy, for, as Baird remarked, Leidy,
although only thirty years of age, was the only anatomist in the United
States qualified to determine their nature. The outcome of Leidy’s study of
this material was “The Ancient Fauna of Nebraska,” published in 1853, and
constituting the most brilliant work which up to that time American
paleontology had produced. Leidy’s determinations, which are in the main
We now come to a consideration of the work of Joseph Leidy, one of the
three great pioneers in American vertebrate paleontology, for if we
disregard the work of Hitchcock and others on the fossil footprints, few of
the results thus far obtained were based upon the fruits of organized
research. Leidy began his publication in 1847 and continued to issue papers
and books from time to time until the year 1892, having published no fewer
than 219 paleontological titles, and 553 all told. His earlier paleontological
researches were exclusively on the Mammalia, which were then coming in
from the newly discovered fossil localities of the West. The discovery of
these forms, one of the most notable events in the history of our science,
will bear re-telling.
The first announcement was made in 1847, when Hiram A. Prout of St.
Louis published in the Journal (3, 248–250) the description of the maxillary
bone of “Palæotherium” (= Titanotherium proutii)from near White River,
Nebraska. This at once drew the attention of geologists and paleontologists
to the Bad Lands, or Mauvaises Terres, which were to prove so highly
productive of fossil forms. About the same time S. D. Culbertson of
Chambersburg, Pennsylvania, submitted to the Academy of Natural
Sciences at Philadelphia some fossils sent to him from Nebraska by
Alexander Culbertson. These were afterward described by Leidy in the
Proceedings of the Academy, together with the paleotheroid jaw, in addition
to which three other collections which had been made were also placed at
his disposal for study.
This aroused the interest of Doctor Spencer F. Baird of the Smithsonian
Institution, who sent T. A. Culbertson to the Bad Lands to make further
collections. The latter was successful in securing a valuable series of
mammalian and chelonian remains. These, together with other specimens
from the same locality, were sent to Leidy, for, as Baird remarked, Leidy,
although only thirty years of age, was the only anatomist in the United
States qualified to determine their nature. The outcome of Leidy’s study of
this material was “The Ancient Fauna of Nebraska,” published in 1853, and
constituting the most brilliant work which up to that time American
paleontology had produced. Leidy’s determinations, which are in the main
Page 248
correct, are the more remarkable when it is realized that he had little recent
osteological material for comparative study. The forms thus described by
him were new to science, of a more generalized character than those now
living, and yet their distinguished describer recognized, either at that time
or a little later, their true relationship to the modern types. The extent of
Leidy’s anatomical knowledge was almost Cuvierian, and Cuvier-like he
established the fact of the presence of the rhinoceroses, then unheard of in
the American fauna, from a few small fragments of molar teeth, an opinion
shortly to be fully sustained through the finding of complete molars and the
entire skull of the same individual animal.
Leidy next turned his attention to the huge edentates, which he studied
exhaustively, publishing his results in the form of a memoir in 1855, two
years after the appearance of the “Ancient Fauna.”
Extinct fishes of the Devonian of Illinois and Missouri and the Devonian
and Carboniferous of Pennsylvania were made the subjects of his next
researches, after which he described the peccaries of Ohio, and later, in a
much larger and most important work, the Cretaceous reptiles of the United
States (1865). Most of the fossils discussed in this last work are from the
New Jersey Cretaceous marls and of them the most notable was the
herbivorous dinosaur Hadrosaurus, the structure and habits of which,
together with its affinities with the Old World iguanodons, Leidy described
in detail. From Leidy’s descriptions and with his aid, Waterhouse Hawkins
was enabled to restore a replica of the skeleton in a remarkably efficient
way. This restoration for a long time graced the museum of the Philadelphia
Academy of Natural Sciences and there was a plaster replica of it in the
United States National Museum. These, together with plaster replicas of
Iguanodon from the Royal College of Surgeons in London, gave to
Americans their first real conceptions of members of this most remarkable
group. The associated fossils from the New Jersey marls were chiefly
crocodiles and turtles.
From 1853 to 1866 F. V. Hayden was carrying on a series of most
energetic explorations in the West, especially in Nebraska and Dakota as
then delimited, returning from each trip laden with fossils which were given
to Leidy for determination. The results appeared in 1869 in Leidy’s Extinct
Mammalian Fauna of Dakota and Nebraska, published as volume 7 of the
Journal of the Philadelphia Academy. In this large volume no fewer than
osteological material for comparative study. The forms thus described by
him were new to science, of a more generalized character than those now
living, and yet their distinguished describer recognized, either at that time
or a little later, their true relationship to the modern types. The extent of
Leidy’s anatomical knowledge was almost Cuvierian, and Cuvier-like he
established the fact of the presence of the rhinoceroses, then unheard of in
the American fauna, from a few small fragments of molar teeth, an opinion
shortly to be fully sustained through the finding of complete molars and the
entire skull of the same individual animal.
Leidy next turned his attention to the huge edentates, which he studied
exhaustively, publishing his results in the form of a memoir in 1855, two
years after the appearance of the “Ancient Fauna.”
Extinct fishes of the Devonian of Illinois and Missouri and the Devonian
and Carboniferous of Pennsylvania were made the subjects of his next
researches, after which he described the peccaries of Ohio, and later, in a
much larger and most important work, the Cretaceous reptiles of the United
States (1865). Most of the fossils discussed in this last work are from the
New Jersey Cretaceous marls and of them the most notable was the
herbivorous dinosaur Hadrosaurus, the structure and habits of which,
together with its affinities with the Old World iguanodons, Leidy described
in detail. From Leidy’s descriptions and with his aid, Waterhouse Hawkins
was enabled to restore a replica of the skeleton in a remarkably efficient
way. This restoration for a long time graced the museum of the Philadelphia
Academy of Natural Sciences and there was a plaster replica of it in the
United States National Museum. These, together with plaster replicas of
Iguanodon from the Royal College of Surgeons in London, gave to
Americans their first real conceptions of members of this most remarkable
group. The associated fossils from the New Jersey marls were chiefly
crocodiles and turtles.
From 1853 to 1866 F. V. Hayden was carrying on a series of most
energetic explorations in the West, especially in Nebraska and Dakota as
then delimited, returning from each trip laden with fossils which were given
to Leidy for determination. The results appeared in 1869 in Leidy’s Extinct
Mammalian Fauna of Dakota and Nebraska, published as volume 7 of the
Journal of the Philadelphia Academy. In this large volume no fewer than
Page 249
seventy genera and numerous species of forms, many of them new to
science, were described, representing many of the principal mammalian
orders; horses were, however, especially conspicuous. This last group led
Leidy to the conclusion, afterward emphasized by Huxley, that North
America was the home of the horse in geologic time, there being here a
greater representation of different species than in any recent fauna of the
world. Leidy’s interest in the horses, for the forwarding of which he made a
large collection of recent material, extended over many years, as his first
paper on the subject bears the date of 1847, the last that of 1890.
Next came the discovery of Eocene material from the vicinity of Fort
Bridger, Wyoming, geologically older than the Nebraska and Dakota
formations. This, together with specimens from the Green River and
Sweetwater River deposits of Wyoming and the John Day River
(Oligocene) of Oregon, was also referred to Leidy, and added yet more to
the list of newly discovered species with which he had already become
familiar in his earlier researches. The results of this study were published by
the Hayden Survey in 1873, under the title “Contributions to the Extinct
Vertebrate Fauna of the Western Territories.” This was the last of Leidy’s
major works, but he continued up to the time of his death to report to the
Academy concerning the various fossil forms that were submitted to him
for identification. Of such reports the most important was one on the fossils
of the phosphate beds of South Carolina, published in the Journal of the
Academy in 1887.
As a paleontologist, Leidy ranks with Cope and Marsh high among those
who enriched the American literature of the subject, but it must be
remembered that this was but a single aspect of his many-sided scientific
career, for he made many contributions of high order to botany, zoology,
and general and comparative anatomy as well, nor did his knowledge and
usefulness as an instructor of his fellow men keep within the limitations of
these subjects.
science, were described, representing many of the principal mammalian
orders; horses were, however, especially conspicuous. This last group led
Leidy to the conclusion, afterward emphasized by Huxley, that North
America was the home of the horse in geologic time, there being here a
greater representation of different species than in any recent fauna of the
world. Leidy’s interest in the horses, for the forwarding of which he made a
large collection of recent material, extended over many years, as his first
paper on the subject bears the date of 1847, the last that of 1890.
Next came the discovery of Eocene material from the vicinity of Fort
Bridger, Wyoming, geologically older than the Nebraska and Dakota
formations. This, together with specimens from the Green River and
Sweetwater River deposits of Wyoming and the John Day River
(Oligocene) of Oregon, was also referred to Leidy, and added yet more to
the list of newly discovered species with which he had already become
familiar in his earlier researches. The results of this study were published by
the Hayden Survey in 1873, under the title “Contributions to the Extinct
Vertebrate Fauna of the Western Territories.” This was the last of Leidy’s
major works, but he continued up to the time of his death to report to the
Academy concerning the various fossil forms that were submitted to him
for identification. Of such reports the most important was one on the fossils
of the phosphate beds of South Carolina, published in the Journal of the
Academy in 1887.
As a paleontologist, Leidy ranks with Cope and Marsh high among those
who enriched the American literature of the subject, but it must be
remembered that this was but a single aspect of his many-sided scientific
career, for he made many contributions of high order to botany, zoology,
and general and comparative anatomy as well, nor did his knowledge and
usefulness as an instructor of his fellow men keep within the limitations of
these subjects.
Page 250
Othniel Charles Marsh (1831–1899).
The sixth decade of the nineteenth century saw the beginning of the
labors of several paleontologists who, like Leidy, were destined to raise the
science of fossil vertebrates in America to the level of attainment of the Old
World. They were, among others, Othniel Charles Marsh and Edward
Drinker Cope. Of these the names of Marsh and Cope are linked together
by the brilliance of their attainments, their contemporaneity, and the rivalry
which the similarity of their pursuits unfortunately engendered. Marsh
produced his first paleontological paper in 1862 (33, 278), Cope in 1864,
but the latter died first, so that his life of research was shorter.
The sixth decade of the nineteenth century saw the beginning of the
labors of several paleontologists who, like Leidy, were destined to raise the
science of fossil vertebrates in America to the level of attainment of the Old
World. They were, among others, Othniel Charles Marsh and Edward
Drinker Cope. Of these the names of Marsh and Cope are linked together
by the brilliance of their attainments, their contemporaneity, and the rivalry
which the similarity of their pursuits unfortunately engendered. Marsh
produced his first paleontological paper in 1862 (33, 278), Cope in 1864,
but the latter died first, so that his life of research was shorter.
Page 251
To Professor Marsh should be given credit for the first organized
expedition designed exclusively for the collection of vertebrate remains, the
results of which contain so much material that it has not yet entirely seen
the light of scientific exposition. Marsh’s first trip to the West was in 1868,
the first formal expedition being organized two years later. These
expeditions, of which there were four, were privately financed except for
the material and military escort furnished by the United States Government,
and consisted of a personnel drawn entirely from the graduate or
undergraduate body of Yale University. These parties explored Kansas,
Nebraska, Wyoming, Utah, and Oregon, and returned laden with material
expedition designed exclusively for the collection of vertebrate remains, the
results of which contain so much material that it has not yet entirely seen
the light of scientific exposition. Marsh’s first trip to the West was in 1868,
the first formal expedition being organized two years later. These
expeditions, of which there were four, were privately financed except for
the material and military escort furnished by the United States Government,
and consisted of a personnel drawn entirely from the graduate or
undergraduate body of Yale University. These parties explored Kansas,
Nebraska, Wyoming, Utah, and Oregon, and returned laden with material
Page 252
from the Cretaceous and Tertiary formations of the West. Some of this is of
necessity somewhat fragmentary, but type after type was secured which,
with his exhaustive knowledge of comparative anatomy, enabled Marsh to
announce discovery after discovery of species, genera, families, and even
orders of mammals, birds, and reptiles which were unknown to science. The
year 1873 saw the last of the student expeditions, and thereafter until the
close of his life the work of collecting was done under Marsh’s supervision,
but by paid explorers, many of whom had been his scouts and guides in the
formal expeditions or had been especially trained by him in the East. In
1882, after fourteen years of the experience thus gained, Marsh was
appointed vertebrate paleontologist to the United States Geological Survey,
which relieved him in part of the personal expense connected with the
collecting, although up to within a short time of his death his own fortune
was very largely spent in enlarging his collections. After his connection
with the Survey was established, Marsh had two main purposes in view in
making the collections: (1) to determine the geological horizon of each
locality where a large series of vertebrate fossils was found, and (2) to
secure from these localities large collections of the more important forms
sufficiently extensive to reveal, if possible, the life histories of each. Marsh
believed that the material thus secured would serve as key or diagnostic
fossils to all horizons of our western geology above the Paleozoic, a belief
in which he was in advance of his time, for few of his contemporaries
appreciated the value of vertebrates as horizon markers. The result of the
fulfilment of his second purpose saw the accumulation of huge collections
from all horizons above the Triassic and some Paleozoic and Triassic as
well. These contained some very remarkable series, each of which Marsh
hoped to make the basis of an elaborate monograph to be published under
the auspices of the Survey. One can visualize the scope of his ambitions by
the fact that no fewer than twenty-seven projected quarto volumes, to
contain at least 850 lithographic plates, were listed by him in 1877. These
covered, among other groups, the toothed birds (Odontornithes),
Dinocerata, horses, brontotheres, pterodactyls, mosasaurs and plesiosaurs,
monkeys, carnivores, perissodactyls and artiodactyls, crocodiles, lizards,
dinosaurs, various birds, proboscideans, edentates and marsupials, brain
evolution, and the Connecticut Valley footprints. Much was done towards
the preparation of these memoirs, as evidenced by the long list of
preliminary papers, admirably illustrated by woodcuts which were to form
necessity somewhat fragmentary, but type after type was secured which,
with his exhaustive knowledge of comparative anatomy, enabled Marsh to
announce discovery after discovery of species, genera, families, and even
orders of mammals, birds, and reptiles which were unknown to science. The
year 1873 saw the last of the student expeditions, and thereafter until the
close of his life the work of collecting was done under Marsh’s supervision,
but by paid explorers, many of whom had been his scouts and guides in the
formal expeditions or had been especially trained by him in the East. In
1882, after fourteen years of the experience thus gained, Marsh was
appointed vertebrate paleontologist to the United States Geological Survey,
which relieved him in part of the personal expense connected with the
collecting, although up to within a short time of his death his own fortune
was very largely spent in enlarging his collections. After his connection
with the Survey was established, Marsh had two main purposes in view in
making the collections: (1) to determine the geological horizon of each
locality where a large series of vertebrate fossils was found, and (2) to
secure from these localities large collections of the more important forms
sufficiently extensive to reveal, if possible, the life histories of each. Marsh
believed that the material thus secured would serve as key or diagnostic
fossils to all horizons of our western geology above the Paleozoic, a belief
in which he was in advance of his time, for few of his contemporaries
appreciated the value of vertebrates as horizon markers. The result of the
fulfilment of his second purpose saw the accumulation of huge collections
from all horizons above the Triassic and some Paleozoic and Triassic as
well. These contained some very remarkable series, each of which Marsh
hoped to make the basis of an elaborate monograph to be published under
the auspices of the Survey. One can visualize the scope of his ambitions by
the fact that no fewer than twenty-seven projected quarto volumes, to
contain at least 850 lithographic plates, were listed by him in 1877. These
covered, among other groups, the toothed birds (Odontornithes),
Dinocerata, horses, brontotheres, pterodactyls, mosasaurs and plesiosaurs,
monkeys, carnivores, perissodactyls and artiodactyls, crocodiles, lizards,
dinosaurs, various birds, proboscideans, edentates and marsupials, brain
evolution, and the Connecticut Valley footprints. Much was done towards
the preparation of these memoirs, as evidenced by the long list of
preliminary papers, admirably illustrated by woodcuts which were to form
Page 253
the text figures of the memoirs, which appeared with great regularity in the
pages of the Journal for a period of thirty years. Of the actual memoirs,
however, but two had been published at the time of Marsh’s death in 1899
—the Odontornithes in 1880 and the Dinocerata in 1884. One must not
overlook, however, the epoch-making Dinosaurs of North America, which
was published by the Survey in 1896, although it was not in the form nor
had it the scope of the proposed monographs. This was not due to lack of
application, for Professor Marsh was an indefatigable worker, but rather to
the fact that the program was of such magnitude as to necessitate a
patriarchal life span for its consummation. As it is, Professor Marsh’s fame
rests first upon his ability and intrepidity as a collector, ready himself to
brave the very certain hardships and dangers which beset the field
paleontologist in the pioneer days, and also by his judgment and command
of men to secure the very adequate services of others and so to direct their
endeavors that the results were of the highest value. The material witness to
Marsh’s skill as a collector lies in the collections of the Peabody Museum at
Yale and in the Marsh collection at the United States National Museum, the
latter secured through the funds of the United States Geological Survey.
Together they constitute what is possibly the greatest collection of fossil
vertebrates in America, if not in the world; individually, they are second
only to that of the American Museum in New York City, the result of the
combined labors of Osborn and Cope and their very able corps of assistants.
As a scientist Marsh possessed in large measure that wide knowledge of
comparative anatomy so necessary to the vertebrate paleontologist, and as a
consequence was not only able to recognize affinities and classify
unerringly, but also to recognize the salient diagnostic features of the form
before him and in few words so to describe them as to render the
recognition of the species by another worker relatively easy. The
publication of hundreds of these specific diagnoses in the Journal
constitutes a very large and valuable part of that periodical’s contribution to
the advancement of our science. Marsh’s method of indicating forms by so
brief a statement leaves much to be done, however, in the way of further
description of his types, which in many instances were but partially
prepared.
Yet another important service which Marsh rendered to science was the
restoration of the creatures as a whole, made with the most painstaking care
and precision through assembling the drawings of the individual bones.
pages of the Journal for a period of thirty years. Of the actual memoirs,
however, but two had been published at the time of Marsh’s death in 1899
—the Odontornithes in 1880 and the Dinocerata in 1884. One must not
overlook, however, the epoch-making Dinosaurs of North America, which
was published by the Survey in 1896, although it was not in the form nor
had it the scope of the proposed monographs. This was not due to lack of
application, for Professor Marsh was an indefatigable worker, but rather to
the fact that the program was of such magnitude as to necessitate a
patriarchal life span for its consummation. As it is, Professor Marsh’s fame
rests first upon his ability and intrepidity as a collector, ready himself to
brave the very certain hardships and dangers which beset the field
paleontologist in the pioneer days, and also by his judgment and command
of men to secure the very adequate services of others and so to direct their
endeavors that the results were of the highest value. The material witness to
Marsh’s skill as a collector lies in the collections of the Peabody Museum at
Yale and in the Marsh collection at the United States National Museum, the
latter secured through the funds of the United States Geological Survey.
Together they constitute what is possibly the greatest collection of fossil
vertebrates in America, if not in the world; individually, they are second
only to that of the American Museum in New York City, the result of the
combined labors of Osborn and Cope and their very able corps of assistants.
As a scientist Marsh possessed in large measure that wide knowledge of
comparative anatomy so necessary to the vertebrate paleontologist, and as a
consequence was not only able to recognize affinities and classify
unerringly, but also to recognize the salient diagnostic features of the form
before him and in few words so to describe them as to render the
recognition of the species by another worker relatively easy. The
publication of hundreds of these specific diagnoses in the Journal
constitutes a very large and valuable part of that periodical’s contribution to
the advancement of our science. Marsh’s method of indicating forms by so
brief a statement leaves much to be done, however, in the way of further
description of his types, which in many instances were but partially
prepared.
Yet another important service which Marsh rendered to science was the
restoration of the creatures as a whole, made with the most painstaking care
and precision through assembling the drawings of the individual bones.
Page 254
These restorations have become classic, embracing as they did a score or
more of forms, of beast, bird, and reptile. They also were published first in
the Journal, although they have subsequently been reproduced in text-books
and other works the world over. Part of Marsh’s popular reputation, at least,
which was second to that of no other American in his line, was due to his
skill in attaining publicity, for his papers, of whatever extent, were carefully
and methodically sent to correspondents in the uttermost parts of the earth,
and thus the Marsh collection has reflected the fame of its maker.
more of forms, of beast, bird, and reptile. They also were published first in
the Journal, although they have subsequently been reproduced in text-books
and other works the world over. Part of Marsh’s popular reputation, at least,
which was second to that of no other American in his line, was due to his
skill in attaining publicity, for his papers, of whatever extent, were carefully
and methodically sent to correspondents in the uttermost parts of the earth,
and thus the Marsh collection has reflected the fame of its maker.
Page 255
Edward Drinker Cope (1840–1897).
The third great name in American vertebrate paleontology, that of
Edward Drinker Cope, stands out in sharp contrast with the other two,
although in the range of his interests he was probably more nearly
comparable with Leidy than with Marsh. The beginning of Cope’s scientific
labors dates from 1859, the year made famous in the annals of science by
the appearance of Darwin’s Origin of Species. It is not surprising, therefore,
that matters evolutional should have interested him to the very end of his
career. Cope was not merely a paleontologist, but was interested in recent
forms, especially the three lower classes of vertebrates, to such an extent
that his work therewith is highly authoritative and in some respects epoch-
making. Thirty-eight years of almost continual toil were his, and the mere
mass of his literary productions is prodigious, especially when one realizes
that, unlike those of a writer of fiction, they were based on painstaking
research and philosophical thought. The greater part of Cope’s life was
spent in or near Philadelphia except for his western explorations, and he is
best known as professor of geology and paleontology in the University of
Pennsylvania, although he served other institutions as well.
Cope’s early work was among the amphibia and reptiles, his first
paleontological paper, the description of Amphibamus grandiceps,
appearing in 1865. This year he also began his studies of the mammals,
especially the Cetacea, both living and extinct, from the Atlantic seaboard.
The next year saw the beginning of his work on the material from the
Cretaceous marls of New Jersey, describing therefrom one of the first
carnivorous dinosaurs, Lælaps, to be discovered in America. In 1868 Cope
began to describe the vertebrates from the Kansas chalk and three years
later made his first exploration of these beds. This led to his connection
with the United States Geological Survey of the Territories under Hayden,
and to continued exploration of Wyoming and Colorado in 1872 and 1873.
The material thus gained, consisting of fishes, mosasaurs, dinosaurs, and
other reptiles, was described in the Transactions of the American
Philosophical Society as well as in the Survey Bulletins. In 1875 these
results were summarized in a large quarto volume entitled “Vertebrata of
the Cretaceous formations of the West.” Subsequent summers were spent in
The third great name in American vertebrate paleontology, that of
Edward Drinker Cope, stands out in sharp contrast with the other two,
although in the range of his interests he was probably more nearly
comparable with Leidy than with Marsh. The beginning of Cope’s scientific
labors dates from 1859, the year made famous in the annals of science by
the appearance of Darwin’s Origin of Species. It is not surprising, therefore,
that matters evolutional should have interested him to the very end of his
career. Cope was not merely a paleontologist, but was interested in recent
forms, especially the three lower classes of vertebrates, to such an extent
that his work therewith is highly authoritative and in some respects epoch-
making. Thirty-eight years of almost continual toil were his, and the mere
mass of his literary productions is prodigious, especially when one realizes
that, unlike those of a writer of fiction, they were based on painstaking
research and philosophical thought. The greater part of Cope’s life was
spent in or near Philadelphia except for his western explorations, and he is
best known as professor of geology and paleontology in the University of
Pennsylvania, although he served other institutions as well.
Cope’s early work was among the amphibia and reptiles, his first
paleontological paper, the description of Amphibamus grandiceps,
appearing in 1865. This year he also began his studies of the mammals,
especially the Cetacea, both living and extinct, from the Atlantic seaboard.
The next year saw the beginning of his work on the material from the
Cretaceous marls of New Jersey, describing therefrom one of the first
carnivorous dinosaurs, Lælaps, to be discovered in America. In 1868 Cope
began to describe the vertebrates from the Kansas chalk and three years
later made his first exploration of these beds. This led to his connection
with the United States Geological Survey of the Territories under Hayden,
and to continued exploration of Wyoming and Colorado in 1872 and 1873.
The material thus gained, consisting of fishes, mosasaurs, dinosaurs, and
other reptiles, was described in the Transactions of the American
Philosophical Society as well as in the Survey Bulletins. In 1875 these
results were summarized in a large quarto volume entitled “Vertebrata of
the Cretaceous formations of the West.” Subsequent summers were spent in
Page 256
further exploration of the Bridger, Washakie, and Wasatch formations of
Wyoming, the Puerco and Torrejon of New Mexico, and the Judith River of
Montana. The material gathered in New Mexico proved particularly
valuable, and led to the publication in 1877 of another notable volume
entitled “Report upon the Extinct Vertebrata obtained in New Mexico by
Parties of the Expedition of 1874.”
Material was now accumulating so fast as to necessitate the concentration
of Cope’s own time on research, so that, while he continued to make brief
journeys to the West, the real work of exploration was delegated to Charles
H. Sternberg and J. L. Wortman, both of whom became subsequently very
well known, the former as a collector whose active service has not yet
ceased, the latter as an explorer and later an investigator of extremely high
promise.
As early as 1865, Cope began no fewer than five separate lines of
research which he pursued concurrently for the remainder of his career. On
the fishes, he became a high authority in the larger classification, owing to
his researches into their phylogeny, for which a knowledge of extinct forms
is imperative. On amphibia, he wrote more voluminously than any other
naturalist, discussing not only the morphology but the paleontology and
taxonomy as well. In this connection must be mentioned not only Cope’s
exploration and collections in the Permian of Ohio and Illinois, but
especially the remains from the Texas Permian, first received in 1877, upon
which some of his most brilliant results were based; these of course
included reptilian as well as amphibian material. His third line of research,
the Reptilia, is in part included in the foregoing, but also embraced the
reptiles of the Bridger and other Tertiary deposits, those of the Kansas
Cretaceous, and the Cretaceous dinosaurs.
Up to 1868 Leidy alone was engaged in research in the West, but that
year saw the simultaneous entrance of Marsh and Cope into this new field
of research, and their exploration and descriptions of similar regions and
forms soon led to a rivalry which in turn developed into a most unfortunate
series of controversies, mainly over the subject of priority. This resulted in a
permanent rupture of friendship and the division of American workers into
two opposing camps to the detriment of the progress of our science. This
breach has now been happily healed, and for a number of years the degree
Wyoming, the Puerco and Torrejon of New Mexico, and the Judith River of
Montana. The material gathered in New Mexico proved particularly
valuable, and led to the publication in 1877 of another notable volume
entitled “Report upon the Extinct Vertebrata obtained in New Mexico by
Parties of the Expedition of 1874.”
Material was now accumulating so fast as to necessitate the concentration
of Cope’s own time on research, so that, while he continued to make brief
journeys to the West, the real work of exploration was delegated to Charles
H. Sternberg and J. L. Wortman, both of whom became subsequently very
well known, the former as a collector whose active service has not yet
ceased, the latter as an explorer and later an investigator of extremely high
promise.
As early as 1865, Cope began no fewer than five separate lines of
research which he pursued concurrently for the remainder of his career. On
the fishes, he became a high authority in the larger classification, owing to
his researches into their phylogeny, for which a knowledge of extinct forms
is imperative. On amphibia, he wrote more voluminously than any other
naturalist, discussing not only the morphology but the paleontology and
taxonomy as well. In this connection must be mentioned not only Cope’s
exploration and collections in the Permian of Ohio and Illinois, but
especially the remains from the Texas Permian, first received in 1877, upon
which some of his most brilliant results were based; these of course
included reptilian as well as amphibian material. His third line of research,
the Reptilia, is in part included in the foregoing, but also embraced the
reptiles of the Bridger and other Tertiary deposits, those of the Kansas
Cretaceous, and the Cretaceous dinosaurs.
Up to 1868 Leidy alone was engaged in research in the West, but that
year saw the simultaneous entrance of Marsh and Cope into this new field
of research, and their exploration and descriptions of similar regions and
forms soon led to a rivalry which in turn developed into a most unfortunate
series of controversies, mainly over the subject of priority. This resulted in a
permanent rupture of friendship and the division of American workers into
two opposing camps to the detriment of the progress of our science. This
breach has now been happily healed, and for a number of years the degree
Page 257
of mutual good will and aid on the part of our workers has been of the
highest sort.
The extent of the western fossil area, and particularly the explorations of
three of Cope’s aids, Wortman in the Big Horn and Wasatch basins,
Baldwin in the Puerco of New Mexico, and Cummins in the Permian of
Texas, gave him so fruitful a field of endeavor that the occasion for jealous
rivalry was largely removed. The most manifest result of Cope’s western
work was the publication in 1883 of his Vertebrata of the Tertiary
Formations of the West, which formed volume 3 of the quarto publications
of the Hayden Survey. This huge book contains more than 1000 pages and
80 plates and has been facetiously called “Cope’s Bible.”
Cope’s philosophical contributions, which covered the domains of
evolution, psychology, ethics, and metaphysics, began in 1868 with his
paper on The Origin of Genera. In evolution he was a follower of Lamarck,
and as such, with Hyatt, Ryder, and Packard, was one of the founders of the
so-called Neo-Lamarckian School in America. Cope’s principal
contribution, set forth in his Factors of Organic Evolution, is the idea of
kinetogenesis or mechanical genesis, the principle that all structures are the
direct outcome of the stresses and strains to which the organism is
subjected. Weismann’s forcible attack on the transmission theory did not
shake Cope’s faith in these doctrines, for he claimed that the
paleontological evidence for the inheritance of such characters as are
apparently the result of individual modification was too strong to be
refuted. Cope was more like Lamarck than any other naturalist in his mental
make-up as well as his ideas. He was also, like Haeckel, given to working
out the phylogeny of whatever type lay before him, and in many instances
arrived marvellously near the truth as we now see it.
Associated for a while with A. S. Packard, Cope soon became chief
editor and proprietor of the American Naturalist, which was for many years
his main means of publication and thus served our science in a way
comparable to the Journal. As Osborn says by way of summation:
“Cope is not to be thought of merely as a specialist in Paleontology. After Huxley he was the last
representative of the old broad-gauge school of anatomists and is only to be compared with members
of that school. His life work bears marks of great genius, of solid and accurate observation, and at
times of inaccuracy due to bad logic or haste and overpressure of work.... As a comparative anatomist
he ranks both in the range and effectiveness of his knowledge and his ideas with Cuvier and Owen....
highest sort.
The extent of the western fossil area, and particularly the explorations of
three of Cope’s aids, Wortman in the Big Horn and Wasatch basins,
Baldwin in the Puerco of New Mexico, and Cummins in the Permian of
Texas, gave him so fruitful a field of endeavor that the occasion for jealous
rivalry was largely removed. The most manifest result of Cope’s western
work was the publication in 1883 of his Vertebrata of the Tertiary
Formations of the West, which formed volume 3 of the quarto publications
of the Hayden Survey. This huge book contains more than 1000 pages and
80 plates and has been facetiously called “Cope’s Bible.”
Cope’s philosophical contributions, which covered the domains of
evolution, psychology, ethics, and metaphysics, began in 1868 with his
paper on The Origin of Genera. In evolution he was a follower of Lamarck,
and as such, with Hyatt, Ryder, and Packard, was one of the founders of the
so-called Neo-Lamarckian School in America. Cope’s principal
contribution, set forth in his Factors of Organic Evolution, is the idea of
kinetogenesis or mechanical genesis, the principle that all structures are the
direct outcome of the stresses and strains to which the organism is
subjected. Weismann’s forcible attack on the transmission theory did not
shake Cope’s faith in these doctrines, for he claimed that the
paleontological evidence for the inheritance of such characters as are
apparently the result of individual modification was too strong to be
refuted. Cope was more like Lamarck than any other naturalist in his mental
make-up as well as his ideas. He was also, like Haeckel, given to working
out the phylogeny of whatever type lay before him, and in many instances
arrived marvellously near the truth as we now see it.
Associated for a while with A. S. Packard, Cope soon became chief
editor and proprietor of the American Naturalist, which was for many years
his main means of publication and thus served our science in a way
comparable to the Journal. As Osborn says by way of summation:
“Cope is not to be thought of merely as a specialist in Paleontology. After Huxley he was the last
representative of the old broad-gauge school of anatomists and is only to be compared with members
of that school. His life work bears marks of great genius, of solid and accurate observation, and at
times of inaccuracy due to bad logic or haste and overpressure of work.... As a comparative anatomist
he ranks both in the range and effectiveness of his knowledge and his ideas with Cuvier and Owen....
Page 258
As a natural philosopher, while far less logical than Huxley, he was more creative and constructive,
his metaphysics ending in theism rather than agnosticism.”
his metaphysics ending in theism rather than agnosticism.”
Page 259
1870–1880.
The seventh decade was productive of comparatively few great names in
the history of our science, but two, J. A. Ryder and Samuel W. Williston,
being notable contributors. The former produced but few papers and those
between 1877 and 1892, yet they were of note and such was their influence
that he is named with Hyatt, Packard, and Cope as one of the founders of
the Neo-Lamarckian School of evolutionists in America. Ryder was a
particular friend and a colleague of Cope, as they were both concerned with
the back-boned animals, while the other two were invertebratists. Ryder
wrote on mechanical genesis of tooth forms and on scales of fishes, also on
the morphology and evolution of the tails of fishes, cetaceans, and
sirenians, and of the other fins of aquatic types. He did, on the other hand,
practically no systematic or descriptive work.
Williston, on the contrary, has had a long and varied career as an
investigator and as an educator. Trained at Yale, he prepared for medicine,
and much of his teaching has been of human anatomy, both at Yale and at
the University of Kansas where he served for a number of years as dean of
the Medical School. He is also a student of flies, and as such not only the
foremost but indeed almost the only dipterologist in the United States. But
it is with his work as a vertebrate paleontologist that we are chiefly
concerned, and here again he stands among the foremost. His initial work
and training in this department of science were with Marsh, for whom he
spent many months in field work, collecting largely in the Niobrara
Cretaceous of Kansas. He did, however, no research while with Marsh,
owing to the latter’s disinclination to foster such work on the part of his
associates. Williston began his publications in 1878 and has continued them
until the present, working mainly with Cretaceous mosasaurs, plesiosaurs,
and pterodactyls. Of late, since his transference to the University of
Chicago, where as professor of paleontology and director of the Walker
Museum he has served since 1902, his interest has lain mainly among the
Paleozoic reptiles and amphibia. Williston’s more notable works are
American Permian Vertebrates and Water Reptiles of the Past and Present,
wherein he sets forth his views of the phylogenesis and taxonomy of the
reptilian class. He is at present at work on the evolution of the reptiles, a
The seventh decade was productive of comparatively few great names in
the history of our science, but two, J. A. Ryder and Samuel W. Williston,
being notable contributors. The former produced but few papers and those
between 1877 and 1892, yet they were of note and such was their influence
that he is named with Hyatt, Packard, and Cope as one of the founders of
the Neo-Lamarckian School of evolutionists in America. Ryder was a
particular friend and a colleague of Cope, as they were both concerned with
the back-boned animals, while the other two were invertebratists. Ryder
wrote on mechanical genesis of tooth forms and on scales of fishes, also on
the morphology and evolution of the tails of fishes, cetaceans, and
sirenians, and of the other fins of aquatic types. He did, on the other hand,
practically no systematic or descriptive work.
Williston, on the contrary, has had a long and varied career as an
investigator and as an educator. Trained at Yale, he prepared for medicine,
and much of his teaching has been of human anatomy, both at Yale and at
the University of Kansas where he served for a number of years as dean of
the Medical School. He is also a student of flies, and as such not only the
foremost but indeed almost the only dipterologist in the United States. But
it is with his work as a vertebrate paleontologist that we are chiefly
concerned, and here again he stands among the foremost. His initial work
and training in this department of science were with Marsh, for whom he
spent many months in field work, collecting largely in the Niobrara
Cretaceous of Kansas. He did, however, no research while with Marsh,
owing to the latter’s disinclination to foster such work on the part of his
associates. Williston began his publications in 1878 and has continued them
until the present, working mainly with Cretaceous mosasaurs, plesiosaurs,
and pterodactyls. Of late, since his transference to the University of
Chicago, where as professor of paleontology and director of the Walker
Museum he has served since 1902, his interest has lain mainly among the
Paleozoic reptiles and amphibia. Williston’s more notable works are
American Permian Vertebrates and Water Reptiles of the Past and Present,
wherein he sets forth his views of the phylogenesis and taxonomy of the
reptilian class. He is at present at work on the evolution of the reptiles, a
Page 260
volume which is eagerly awaited by his colleagues. It is in morphology that
Williston’s greatest strength lies and some of his most effective work on the
mosasaurs has appeared in the Journal.
Williston’s greatest strength lies and some of his most effective work on the
mosasaurs has appeared in the Journal.
Page 261
1880–1900.
The next decade, that of 1880–1890, saw a number of notable additions
to the workers in vertebrate paleontology: Henry F. Osborn, W. B. Scott, R.
W. Shufeldt, J. L. Wortman, George Baur, F. A. Lucas, and F. W. True.
Shufeldt is our highest authority on the osteology of birds, both recent and
extinct, having recently described all of the extinct forms contained in the
Marsh collection; True wrote of Cetacea; Lucas of marine and Pleistocene
mammals and birds, and has also written popular books on prehistoric life.
Lucas’s greatest service, however, lies in the museums, where he has
manifested a genius second to none in the installation of mute evidences of
living and past organisms. Wortman was for a time associated with Cope,
later with Osborn in the American Museum, again at the Carnegie Museum
at Pittsburgh, and finally at Yale in research on the Bridger Eocene portion
of the Marsh collection. His work has been chiefly the perfection of field
methods in vertebrate paleontology, and as a special investigator of Tertiary
Mammalia, treating the latter largely from the morphologic and taxonomic
standpoints. Wortman’s Yale results on the carnivores and primates of the
Eocene, as yet unfinished, were published in the Journal in 1901–1904.
William B. Scott is a graduate of Princeton, and has spent thirty-four
years in her service as Blair Professor of Geology and Paleontology. His
first publication, in 1878, issued in conjunction with Osborn and Speir,
described material collected by them in the Eocene formations of the West,
and since that time Scott’s research has been entirely with the mammals, on
which he is one of our highest authorities. His most notable works have
been a History of Land Mammals of the Western Hemisphere, 1913, and the
results of the Patagonian expeditions by Hatcher, which are published in a
quarto series in conjunction with W. J. Sinclair, although they are the
authors of separate volumes, Scott’s work being mainly on the carnivores
and edentates of the Santa Cruz formation. It is as a systematist in research
and as an educator that Scott has attained his highest usefulness.
The man who, next to the three pioneers, has attained the highest
reputation in vertebrate paleontologic research, is Henry Fairfield Osborn.
Graduate of Princeton in the same class that produced Scott, Osborn served
for a time as professor of comparative anatomy in that institution, and in
The next decade, that of 1880–1890, saw a number of notable additions
to the workers in vertebrate paleontology: Henry F. Osborn, W. B. Scott, R.
W. Shufeldt, J. L. Wortman, George Baur, F. A. Lucas, and F. W. True.
Shufeldt is our highest authority on the osteology of birds, both recent and
extinct, having recently described all of the extinct forms contained in the
Marsh collection; True wrote of Cetacea; Lucas of marine and Pleistocene
mammals and birds, and has also written popular books on prehistoric life.
Lucas’s greatest service, however, lies in the museums, where he has
manifested a genius second to none in the installation of mute evidences of
living and past organisms. Wortman was for a time associated with Cope,
later with Osborn in the American Museum, again at the Carnegie Museum
at Pittsburgh, and finally at Yale in research on the Bridger Eocene portion
of the Marsh collection. His work has been chiefly the perfection of field
methods in vertebrate paleontology, and as a special investigator of Tertiary
Mammalia, treating the latter largely from the morphologic and taxonomic
standpoints. Wortman’s Yale results on the carnivores and primates of the
Eocene, as yet unfinished, were published in the Journal in 1901–1904.
William B. Scott is a graduate of Princeton, and has spent thirty-four
years in her service as Blair Professor of Geology and Paleontology. His
first publication, in 1878, issued in conjunction with Osborn and Speir,
described material collected by them in the Eocene formations of the West,
and since that time Scott’s research has been entirely with the mammals, on
which he is one of our highest authorities. His most notable works have
been a History of Land Mammals of the Western Hemisphere, 1913, and the
results of the Patagonian expeditions by Hatcher, which are published in a
quarto series in conjunction with W. J. Sinclair, although they are the
authors of separate volumes, Scott’s work being mainly on the carnivores
and edentates of the Santa Cruz formation. It is as a systematist in research
and as an educator that Scott has attained his highest usefulness.
The man who, next to the three pioneers, has attained the highest
reputation in vertebrate paleontologic research, is Henry Fairfield Osborn.
Graduate of Princeton in the same class that produced Scott, Osborn served
for a time as professor of comparative anatomy in that institution, and in
Page 262
1891 was called to New York to organize the department of zoology in
Columbia University and that of vertebrate paleontology in the American
Museum of Natural History. He had, early in his career, gone west in
company with Professor Scott, and had collected material from the Eocene
formation of Wyoming, upon which they based their first joint paper in
1878, Osborn’s first independent production, a memoir on two genera of
Dinocerata, appearing in 1881. A number of papers followed, on the
Mesozoic Mammalia, on Cope’s tritubercular theory, and on certain
apparent evidences for the transmission of acquired characters. It was,
however, with his acceptance of the New York responsibilities, especially at
the American Museum, that Osborn’s most significant work began. Aided
first by Wortman and Earle, later by W. D. Matthew and others, he has built
up the greatest and most complete collection of fossil vertebrates extant; its
value, however, was largely enhanced through the purchase of the private
collection of Professor Cope, which of course included a large number of
types. The American Museum collection thus contains not only a vast series
of representative specimens from every class and order of vertebrates,
secured by purchase or expedition from nearly all the great localities of the
world, but an exhibition series of skulls and partial and entire skeletons and
restorations which no other institution can hope to equal. Based upon this
wonderful material is a large amount of research, filling many volumes,
published for the greater part in the bulletin and memoirs of the Museum.
This research is not only the product of the staff, including Walter Granger,
Barnum Brown, W. D. Matthew, and W. K. Gregory, but also of a number
of other American and some foreign paleontologists as well.
Professor Osborn’s own work has been voluminous, his bibliography
from 1877 to 1916 containing no fewer than 441 titles, ranging over the
fields of paleontology,—which of course includes the greater number—
geology, correlation and paleogeography, evolutionary principles
exemplified in the Mammalia, man, neurology and embryology,
biographies, and the theory of education.
In paleontology, Osborn’s researches have been largely with the Reptilia
and Mammalia, partly morphological, but also taxonomic and evolutional.
Faunistic studies have also been made of the mammals. Of his published
volumes the most important are, first, the Age of Mammals (1910), in
which he treats not of evolutionary series of phylogenies, but of faunas and
their origin, migrations, and extinctions, and of the correlation of Old and
Columbia University and that of vertebrate paleontology in the American
Museum of Natural History. He had, early in his career, gone west in
company with Professor Scott, and had collected material from the Eocene
formation of Wyoming, upon which they based their first joint paper in
1878, Osborn’s first independent production, a memoir on two genera of
Dinocerata, appearing in 1881. A number of papers followed, on the
Mesozoic Mammalia, on Cope’s tritubercular theory, and on certain
apparent evidences for the transmission of acquired characters. It was,
however, with his acceptance of the New York responsibilities, especially at
the American Museum, that Osborn’s most significant work began. Aided
first by Wortman and Earle, later by W. D. Matthew and others, he has built
up the greatest and most complete collection of fossil vertebrates extant; its
value, however, was largely enhanced through the purchase of the private
collection of Professor Cope, which of course included a large number of
types. The American Museum collection thus contains not only a vast series
of representative specimens from every class and order of vertebrates,
secured by purchase or expedition from nearly all the great localities of the
world, but an exhibition series of skulls and partial and entire skeletons and
restorations which no other institution can hope to equal. Based upon this
wonderful material is a large amount of research, filling many volumes,
published for the greater part in the bulletin and memoirs of the Museum.
This research is not only the product of the staff, including Walter Granger,
Barnum Brown, W. D. Matthew, and W. K. Gregory, but also of a number
of other American and some foreign paleontologists as well.
Professor Osborn’s own work has been voluminous, his bibliography
from 1877 to 1916 containing no fewer than 441 titles, ranging over the
fields of paleontology,—which of course includes the greater number—
geology, correlation and paleogeography, evolutionary principles
exemplified in the Mammalia, man, neurology and embryology,
biographies, and the theory of education.
In paleontology, Osborn’s researches have been largely with the Reptilia
and Mammalia, partly morphological, but also taxonomic and evolutional.
Faunistic studies have also been made of the mammals. Of his published
volumes the most important are, first, the Age of Mammals (1910), in
which he treats not of evolutionary series of phylogenies, but of faunas and
their origin, migrations, and extinctions, and of the correlation of Old and
Page 263
New World Tertiary deposits and their contents. Men of the Old Stone Age
(1916) is an exhaustive treatise and is the first full and authoritative
American presentation of what has been discovered up to the present time
throughout the world in regard to human prehistory. In his latest volume,
The Origin and Evolution of Life (1917), Osborn presents a new energy
conception of evolution and heredity as against the prevailing matter and
form conceptions. In this volume there is summed up the whole story of the
origin and evolution of life on earth up to the appearance of man. This last
book is novel in its conceptions, but it is too early as yet to judge of the
acceptance of Osborn’s theses by his fellow workers in science.
Since the death of Professor Marsh, Osborn has served as vertebrate
paleontologist to the United States Geological Survey, and has in charge the
carrying through to completion of the many monographs proposed by his
distinguished predecessor. One of these, that on the horned dinosaurs, has
been completed by Hatcher and Lull (1907), another on the stegosaurian
dinosaurs has been carried forward by C. W. Gilmore of the United States
National Museum, while under Osborn’s own hand are the memoirs on the
titanotheres (aided by W. K. Gregory), the horses, and the sauropod
dinosaurs. Of these, the first, when it shall have been completed, promises
to be the most monumental and exhaustive study of a group of fossil
organisms ever undertaken.
As a leader in science, a teacher and administrator, Professor Osborn’s
rank is high among the leading vertebratists. He is remarkably successful in
his choice of assistants and in stimulating them in their productiveness so
that their combined results form a very considerable share of the later
literature in America.
The ninth decade ushered in the work of a valuable group of students, of
whom John Bell Hatcher should be mentioned in particular, as his work is
done. Graduate of Yale in 1884, he spent a number of years assisting his
teacher, Professor Marsh, mainly in the field, collecting during that time,
either for Yale or for the United States Geological Survey, an enormous
amount of very fine material, especially from the West, although he also
collected in the older Tertiary and Potomac beds near Washington. In the
West he secured no fewer than 105 titanothere skulls, explored the Tertiary,
Judith River, and Lance formations, collected and in fact virtually
discovered the remains of the Cretaceous mammals and of the horned
(1916) is an exhaustive treatise and is the first full and authoritative
American presentation of what has been discovered up to the present time
throughout the world in regard to human prehistory. In his latest volume,
The Origin and Evolution of Life (1917), Osborn presents a new energy
conception of evolution and heredity as against the prevailing matter and
form conceptions. In this volume there is summed up the whole story of the
origin and evolution of life on earth up to the appearance of man. This last
book is novel in its conceptions, but it is too early as yet to judge of the
acceptance of Osborn’s theses by his fellow workers in science.
Since the death of Professor Marsh, Osborn has served as vertebrate
paleontologist to the United States Geological Survey, and has in charge the
carrying through to completion of the many monographs proposed by his
distinguished predecessor. One of these, that on the horned dinosaurs, has
been completed by Hatcher and Lull (1907), another on the stegosaurian
dinosaurs has been carried forward by C. W. Gilmore of the United States
National Museum, while under Osborn’s own hand are the memoirs on the
titanotheres (aided by W. K. Gregory), the horses, and the sauropod
dinosaurs. Of these, the first, when it shall have been completed, promises
to be the most monumental and exhaustive study of a group of fossil
organisms ever undertaken.
As a leader in science, a teacher and administrator, Professor Osborn’s
rank is high among the leading vertebratists. He is remarkably successful in
his choice of assistants and in stimulating them in their productiveness so
that their combined results form a very considerable share of the later
literature in America.
The ninth decade ushered in the work of a valuable group of students, of
whom John Bell Hatcher should be mentioned in particular, as his work is
done. Graduate of Yale in 1884, he spent a number of years assisting his
teacher, Professor Marsh, mainly in the field, collecting during that time,
either for Yale or for the United States Geological Survey, an enormous
amount of very fine material, especially from the West, although he also
collected in the older Tertiary and Potomac beds near Washington. In the
West he secured no fewer than 105 titanothere skulls, explored the Tertiary,
Judith River, and Lance formations, collected and in fact virtually
discovered the remains of the Cretaceous mammals and of the horned
Page 264
dinosaurs which he was later privileged to describe. He then (1893) went to
Princeton, which he served for seven years, his principal work being
explorations in Patagonia for the E. and M. Museum, one direct result of
which was the publication of a large quarto on the narrative of the
expedition and the geography and ethnography of the region. Going to the
Carnegie Museum in Pittsburgh in 1900, Hatcher carried forward the work
of exploration and collecting begun for that institution by Wortman, and as
a partial result prepared many papers, the principal ones being memoirs on
the dinosaurs Haplocanthosaurus and Diplodocus. In 1903, with T. W.
Stanton of the United States Geological Survey, Hatcher explored the Judith
River beds and together they settled the vexatious problem of their age, the
published results appearing in 1905, after Hatcher’s death. His last piece of
research, begun in 1902 and continued until his death in 1904, was an
elaborate monograph on the Ceratopsia, one of the many projected by
Marsh. Of this memoir Hatcher had completed some 150 printed quarto
pages, giving a rare insight into the anatomy of these strange forms. The
final chapters, however, which were based very largely upon Hatcher’s own
opinions, had to be prepared by another hand.
Despite his early death, therefore, Hatcher rendered a very signal service
to American paleontology—in exploration, stratigraphy, morphology, and
systematic revision—and his activity in planning new fields of research,
such, for instance, as the exploration of the Antarctic continent, gave
promise of further high attainment, when his hand was arrested by death.
Princeton, which he served for seven years, his principal work being
explorations in Patagonia for the E. and M. Museum, one direct result of
which was the publication of a large quarto on the narrative of the
expedition and the geography and ethnography of the region. Going to the
Carnegie Museum in Pittsburgh in 1900, Hatcher carried forward the work
of exploration and collecting begun for that institution by Wortman, and as
a partial result prepared many papers, the principal ones being memoirs on
the dinosaurs Haplocanthosaurus and Diplodocus. In 1903, with T. W.
Stanton of the United States Geological Survey, Hatcher explored the Judith
River beds and together they settled the vexatious problem of their age, the
published results appearing in 1905, after Hatcher’s death. His last piece of
research, begun in 1902 and continued until his death in 1904, was an
elaborate monograph on the Ceratopsia, one of the many projected by
Marsh. Of this memoir Hatcher had completed some 150 printed quarto
pages, giving a rare insight into the anatomy of these strange forms. The
final chapters, however, which were based very largely upon Hatcher’s own
opinions, had to be prepared by another hand.
Despite his early death, therefore, Hatcher rendered a very signal service
to American paleontology—in exploration, stratigraphy, morphology, and
systematic revision—and his activity in planning new fields of research,
such, for instance, as the exploration of the Antarctic continent, gave
promise of further high attainment, when his hand was arrested by death.
Page 265
Summary.
It is not surprising that American vertebrate paleontology has arisen to so
high a plane, when one considers the material at its disposal. Having a vast
and virgin field for exploration, a sufficient number of collectors, some of
whom have devoted much of their lives to the work, and a refinement of
technique that permitted the preservation of the fragmental and ill
conserved as well as the finer specimens, the results could hardly have been
otherwise. Thus it has been possible to secure material almost unique
throughout the world for extent, for completeness, and for variety. To this
must be added a certain American daring in the matter of the restoration of
missing portions, both of the individual bones and of the skeleton as a
whole, such as European conservatism will not as a rule permit. This work
has for the most part been done after the most painstaking comparison and
research and is highly justified in the accuracy of the results, which render
the fabric of the skeleton much more intelligible, both to the scientist and to
the layman. Material once secured and prepared is then mounted, and here
again American ingenuity has accomplished some remarkable results. Some
of the specimens thus mounted are so small and delicate as to require
holding devices comparable to those for the display of jewels; yet others—
huge dinosaurs the bones of which are enormously heavy, but so brittle that
they will not bear even the weight of a process unsupported—require a
carefully designed and skilfully worked out series of supports of steel or
iron which must be perfectly secure and at the same time as inconspicuous
as possible. And of late the lifelike pose of the individual skeleton has been
augmented by the preparation of groups of several animals which
collectively exhibit sex, size, or other individual variations and the full
mechanics of the skeleton under the varying poses assumed by the creature
during life.
The work of further restoration has been rendered possible through
comparative anatomical study, enabling us to essay restorations in entirety
by means of models and drawings, clothing the bones with sinews and with
flesh and the flesh with skin and hair, if such the creature bore; while the
laws of faunal coloration have permitted the coloring of the restoration in a
way which if not the actual hue of life is a very reasonable possibility.
It is not surprising that American vertebrate paleontology has arisen to so
high a plane, when one considers the material at its disposal. Having a vast
and virgin field for exploration, a sufficient number of collectors, some of
whom have devoted much of their lives to the work, and a refinement of
technique that permitted the preservation of the fragmental and ill
conserved as well as the finer specimens, the results could hardly have been
otherwise. Thus it has been possible to secure material almost unique
throughout the world for extent, for completeness, and for variety. To this
must be added a certain American daring in the matter of the restoration of
missing portions, both of the individual bones and of the skeleton as a
whole, such as European conservatism will not as a rule permit. This work
has for the most part been done after the most painstaking comparison and
research and is highly justified in the accuracy of the results, which render
the fabric of the skeleton much more intelligible, both to the scientist and to
the layman. Material once secured and prepared is then mounted, and here
again American ingenuity has accomplished some remarkable results. Some
of the specimens thus mounted are so small and delicate as to require
holding devices comparable to those for the display of jewels; yet others—
huge dinosaurs the bones of which are enormously heavy, but so brittle that
they will not bear even the weight of a process unsupported—require a
carefully designed and skilfully worked out series of supports of steel or
iron which must be perfectly secure and at the same time as inconspicuous
as possible. And of late the lifelike pose of the individual skeleton has been
augmented by the preparation of groups of several animals which
collectively exhibit sex, size, or other individual variations and the full
mechanics of the skeleton under the varying poses assumed by the creature
during life.
The work of further restoration has been rendered possible through
comparative anatomical study, enabling us to essay restorations in entirety
by means of models and drawings, clothing the bones with sinews and with
flesh and the flesh with skin and hair, if such the creature bore; while the
laws of faunal coloration have permitted the coloring of the restoration in a
way which if not the actual hue of life is a very reasonable possibility.
Page 266
Thus the American paleontologists have blazed a trail which has been
followed to good effect by certain of their Old World colleagues.
With such means and methods and such material available, it is again not
surprising that American paleontology has furnished more and more of the
evidences of evolution, and disclosed to the eyes of scientists animal
relationships which were undreamed of by the systematist whose research
dealt only with the existing. It has also explained some vexatious problems
of animal distribution and of extinction, and has connected up cause and
effect in the great evolutionary movements which are recorded.
The results of systematic research have added hosts of new genera and
species and of families, but of orders there are relatively few. Nevertheless a
number, especially among reptiles and mammals, have come to light as the
fruits of American discovery. But aside from the dry cataloguing of such
groups, the American systematists have worked out some very remarkable
phylogenies and have thus clarified our vision of animal relationships in a
way which the recent zoologist could never have done. In this connection,
the Permian vertebrates, which have been collected and studied with
amazing success, principally by Williston and Case, should be mentioned,
although the work is yet incomplete. Some of these forms are amphibian,
others reptilian, yet others of such character as to link the two classes as
transitional forms. Of the Mesozoic reptiles, a very remarkable assemblage
has come to light, in a degree of perfection unknown elsewhere. These are
dinosaurs, of which several phyla are now known; carnivores both great and
small, some of the latter being actually toothless; Sauropoda, whose
perfection and dimensions are incomparable except for those found in East
Africa; and predentates, armored, unarmored, and horned, the last
exclusively American. The unarmored trachodonts are now known in their
entirety, for not only has our West produced articulated skeletons but
mummified carcasses whose skin and other portions of their soft anatomy
are represented, and which are thus far without a parallel elsewhere in the
world. Other reptilian groups are well known, notably the Triassic
ichthyosaurs, and the mosasaurs and plesiosaurs of the Kansas chalk. The
last formation has also produced toothed birds, Hesperornis and
Ichthyornis, which again are absolutely unique.
But it is in the mammalian class that the phylogenies become so highly
complete and of such great importance as evolutionary evidences, for
followed to good effect by certain of their Old World colleagues.
With such means and methods and such material available, it is again not
surprising that American paleontology has furnished more and more of the
evidences of evolution, and disclosed to the eyes of scientists animal
relationships which were undreamed of by the systematist whose research
dealt only with the existing. It has also explained some vexatious problems
of animal distribution and of extinction, and has connected up cause and
effect in the great evolutionary movements which are recorded.
The results of systematic research have added hosts of new genera and
species and of families, but of orders there are relatively few. Nevertheless a
number, especially among reptiles and mammals, have come to light as the
fruits of American discovery. But aside from the dry cataloguing of such
groups, the American systematists have worked out some very remarkable
phylogenies and have thus clarified our vision of animal relationships in a
way which the recent zoologist could never have done. In this connection,
the Permian vertebrates, which have been collected and studied with
amazing success, principally by Williston and Case, should be mentioned,
although the work is yet incomplete. Some of these forms are amphibian,
others reptilian, yet others of such character as to link the two classes as
transitional forms. Of the Mesozoic reptiles, a very remarkable assemblage
has come to light, in a degree of perfection unknown elsewhere. These are
dinosaurs, of which several phyla are now known; carnivores both great and
small, some of the latter being actually toothless; Sauropoda, whose
perfection and dimensions are incomparable except for those found in East
Africa; and predentates, armored, unarmored, and horned, the last
exclusively American. The unarmored trachodonts are now known in their
entirety, for not only has our West produced articulated skeletons but
mummified carcasses whose skin and other portions of their soft anatomy
are represented, and which are thus far without a parallel elsewhere in the
world. Other reptilian groups are well known, notably the Triassic
ichthyosaurs, and the mosasaurs and plesiosaurs of the Kansas chalk. The
last formation has also produced toothed birds, Hesperornis and
Ichthyornis, which again are absolutely unique.
But it is in the mammalian class that the phylogenies become so highly
complete and of such great importance as evolutionary evidences, for
Page 267
nowhere else than in our own West have such series been found as the
Dinocerata and creodonts among archaic forms, the primitive primates from
the Eocene, the carnivores such as the dogs and cats and mustellids, but
especially the hoofed orders such as the horses. Of these hoofed orders, the
classic American series of horses is complete, that of the camels probably
no less so, while much is known of the deer and oreodonts, the last showing
several parallel phyla, and of the proboscideans, which while having their
pristine home in the Old World nevertheless soon sought the new where
their remains are found from the Miocene until their final and apparently
very recent extinction. These creatures show increase of bulk, perfection of
feet and teeth, development of various weapons, horns and antlers, which
may be studied in their relationship with the other organs to make the
evolving whole, or their evolution may be traced as individual structures
which have their rise, culmination, and sometimes their senile atrophy in a
way comparable to that of the representatives of the order as a whole. Thus,
for example, Osborn has traced the evolution of the molar teeth, and Cope
of the feet, while Marsh has shown that brain development runs a similar
course and that its degree of perfection within a group is a potent factor for
survival.
As a student of evolution, the paleontologist sees things in a very
different light from the zoologist. The latter is concerned largely with
matters of detail—with the inheritance of color or of the minor and more
superficial characteristics of animals—and the period of observation of such
phenomena is of necessity brief because of the mortality of the observer.
Whereas the paleontologist has a perspective which the other lacks, since
for him time means little in the terms of his own life, and he can look into
the past and see the great and fundamental changes which evolution has
wrought, the rise of phyla, of classes, of orders, and he alone can see the
orderliness of the process and sense the majesty of the laws which govern
it.
Dinocerata and creodonts among archaic forms, the primitive primates from
the Eocene, the carnivores such as the dogs and cats and mustellids, but
especially the hoofed orders such as the horses. Of these hoofed orders, the
classic American series of horses is complete, that of the camels probably
no less so, while much is known of the deer and oreodonts, the last showing
several parallel phyla, and of the proboscideans, which while having their
pristine home in the Old World nevertheless soon sought the new where
their remains are found from the Miocene until their final and apparently
very recent extinction. These creatures show increase of bulk, perfection of
feet and teeth, development of various weapons, horns and antlers, which
may be studied in their relationship with the other organs to make the
evolving whole, or their evolution may be traced as individual structures
which have their rise, culmination, and sometimes their senile atrophy in a
way comparable to that of the representatives of the order as a whole. Thus,
for example, Osborn has traced the evolution of the molar teeth, and Cope
of the feet, while Marsh has shown that brain development runs a similar
course and that its degree of perfection within a group is a potent factor for
survival.
As a student of evolution, the paleontologist sees things in a very
different light from the zoologist. The latter is concerned largely with
matters of detail—with the inheritance of color or of the minor and more
superficial characteristics of animals—and the period of observation of such
phenomena is of necessity brief because of the mortality of the observer.
Whereas the paleontologist has a perspective which the other lacks, since
for him time means little in the terms of his own life, and he can look into
the past and see the great and fundamental changes which evolution has
wrought, the rise of phyla, of classes, of orders, and he alone can see the
orderliness of the process and sense the majesty of the laws which govern
it.
Page 268
Influence of the American Journal of Science.
The influence of the American Journal of Science as a medium for the
dissemination of the results of vertebrate research has been in evidence
throughout this discussion, but it were well, perhaps, to emphasize that
service more fully. The Journal was, as we have seen, the chief outlet for
Professor Marsh’s research, for there were published in it during his
lifetime no fewer than 175 papers descriptive of the forms which he studied,
as well as a great part of the material in the published monographs. As
Marsh left very few manuscript notes, the importance of these frequent
publications in thus setting forth much that he thought and learned
concerning the material is very great indeed. The combined titles of all
other authors in the Journal in this line of research for the century of its life
fall far short of the number produced by Marsh alone, as they include 136
all told, but the range of subjects is highly representative of the entire field
of vertebrate research. It should be borne in mind, moreover, that Leidy,
Cope, and Osborn each had another medium of publication, which of course
is true of other workers in the great museums such as the American,
National, and Carnegie, all of which issue bulletins and quarto publications
for the purpose of disseminating the work of their staff. Many of the earlier
announcements of the discovery of vertebrate relics appeared in the Journal,
as did practically all the literature of the science of fossil footprints
(ichnology), except of course the larger quartos of Hitchcock and Deane. Of
the footprint papers by Hitchcock, Deane, and others, there were no fewer
than thirty-two, with a number of additional communications on attendant
phenomena bones and plants.
Up to 1847, except for a few foreign announcements, the Journal
published almost exclusively on eastern American paleontology, the only
exception being a notice of bones from Oregon by Perkins in 1842. In 1847
came the announcement of a western “Palæothere” by Prout, which marked
the beginning of the researches of Leidy and others in the Bad Lands of the
great Nebraska plains. The Journal thenceforth published paper after paper
on forms from all over North America, and on all aspects of our science:
discovery, systematic description, faunal relationships, evolutionary
The influence of the American Journal of Science as a medium for the
dissemination of the results of vertebrate research has been in evidence
throughout this discussion, but it were well, perhaps, to emphasize that
service more fully. The Journal was, as we have seen, the chief outlet for
Professor Marsh’s research, for there were published in it during his
lifetime no fewer than 175 papers descriptive of the forms which he studied,
as well as a great part of the material in the published monographs. As
Marsh left very few manuscript notes, the importance of these frequent
publications in thus setting forth much that he thought and learned
concerning the material is very great indeed. The combined titles of all
other authors in the Journal in this line of research for the century of its life
fall far short of the number produced by Marsh alone, as they include 136
all told, but the range of subjects is highly representative of the entire field
of vertebrate research. It should be borne in mind, moreover, that Leidy,
Cope, and Osborn each had another medium of publication, which of course
is true of other workers in the great museums such as the American,
National, and Carnegie, all of which issue bulletins and quarto publications
for the purpose of disseminating the work of their staff. Many of the earlier
announcements of the discovery of vertebrate relics appeared in the Journal,
as did practically all the literature of the science of fossil footprints
(ichnology), except of course the larger quartos of Hitchcock and Deane. Of
the footprint papers by Hitchcock, Deane, and others, there were no fewer
than thirty-two, with a number of additional communications on attendant
phenomena bones and plants.
Up to 1847, except for a few foreign announcements, the Journal
published almost exclusively on eastern American paleontology, the only
exception being a notice of bones from Oregon by Perkins in 1842. In 1847
came the announcement of a western “Palæothere” by Prout, which marked
the beginning of the researches of Leidy and others in the Bad Lands of the
great Nebraska plains. The Journal thenceforth published paper after paper
on forms from all over North America, and on all aspects of our science:
discovery, systematic description, faunal relationships, evolutionary
Page 269
evidences—thus showing that breadth and catholicity which has made it so
great a power in the advancement of science.
great a power in the advancement of science.
Page 270
VII
THE RISE OF PETROLOGY AS A SCIENCE
By LOUIS V. PIRSSON
This chapter is intended to present a brief sketch of the progress of the
science of petrology from its early beginnings down to the present time.
The field to be covered is so large that this can be done only in broadest
outline, and it has therefore been restricted chiefly to what has been
accomplished in America. Although the period covered by the life of the
Journal extends backward for a century it is, however, practically only
within the last fifty years that the rocks of the earth’s crust have been made
the subject of such systematic investigation by minute and delicately
accurate methods of research as to give rise to a distinct branch of geologic
science. It is not intended of course to affirm by this statement that the
broader features of the rocks, especially those which may be observed in the
field and which concern their relations as geologic masses, had not been
made the object of inquiry before this time, since this is the very foundation
of geology itself. Moreover, a certain amount of investigation of rocks, as to
the minerals of which they were composed, the significance of their
textures, and their chemical composition, had been carried out, concomitant
with the growth from early times of geology and mineralogy. Thus, in 1815,
Cordier by a process of washing separated the components of a basalt and
by chemical tests determined the constituent minerals. At the time the
Journal was founded, and for many years following, the genesis of rocks,
especially of igneous rocks, was a subject of inquiry and of prolonged
discussion. The aid of the rapidly growing science of chemistry was
invoked by the geologists and analyses of rocks were made in the attempt to
THE RISE OF PETROLOGY AS A SCIENCE
By LOUIS V. PIRSSON
This chapter is intended to present a brief sketch of the progress of the
science of petrology from its early beginnings down to the present time.
The field to be covered is so large that this can be done only in broadest
outline, and it has therefore been restricted chiefly to what has been
accomplished in America. Although the period covered by the life of the
Journal extends backward for a century it is, however, practically only
within the last fifty years that the rocks of the earth’s crust have been made
the subject of such systematic investigation by minute and delicately
accurate methods of research as to give rise to a distinct branch of geologic
science. It is not intended of course to affirm by this statement that the
broader features of the rocks, especially those which may be observed in the
field and which concern their relations as geologic masses, had not been
made the object of inquiry before this time, since this is the very foundation
of geology itself. Moreover, a certain amount of investigation of rocks, as to
the minerals of which they were composed, the significance of their
textures, and their chemical composition, had been carried out, concomitant
with the growth from early times of geology and mineralogy. Thus, in 1815,
Cordier by a process of washing separated the components of a basalt and
by chemical tests determined the constituent minerals. At the time the
Journal was founded, and for many years following, the genesis of rocks,
especially of igneous rocks, was a subject of inquiry and of prolonged
discussion. The aid of the rapidly growing science of chemistry was
invoked by the geologists and analyses of rocks were made in the attempt to
Page 271
throw light on important questions. It is remarkable, also, how keen were
the observations that the geologists of those days made upon the rocks, as to
their component minerals and structures, aided only by the pocket lens.
Many ideas were put forward, the essentials of which have persisted to the
present day and have become interwoven into the science, whereas others
gave rise to contentions which have not yet been settled to the satisfaction
of all. At times in these earlier days the microscope was called into use to
help in solving questions regarding the finer grained rocks, but this
employment, as Zirkel has shown, was merely incidental, and no definite
technique or purpose for the instrument was established.
On the other hand, the fact that up to the middle of the last century a
large store of information relating to the occurrence of rocks, and to the
mineral composition of those of coarser grain, and somewhat in respect to
their structure, had been accumulated, caused attempts in one way or
another to find means of coördinating these data and to produce
classifications, such as those of Von Cotta and Cordier. The history of these
attempts at classification, before the revelations made by the use of the
microscope had become general, has been admirably reviewed by Whitman
Cross[107] and need not be further enlarged upon here.
That a considerable amount of work was done along chemical lines also
is testified to by the publication of Roth’s Tabellen in 1861, in which all
published analyses of rocks up to that date were collected. What was
accomplished during this period was done chiefly on the continent of
Europe, and little attention had been paid to the subject of rocks either in
America or in Great Britain—even so late as 1870 Geikie remarks, as
referred to by Cross,[108] that there was no good English treatise on
petrography, or the classification and description of rocks. In this country
still less had been accomplished, interest being almost wholly confined to
the vigorous and growing sciences of geology and mineralogy. This was
natural, for mineralogy is the chief buttress on which the structure of
petrology rests and must naturally develop first, especially in a relatively
new and unexplored region, whose mineral resources first attract attention.
The geologists in carrying out their studies also observed the rocks as they
saw them in the field and made incidental reference to them, but
investigations of the rocks themselves was very little attempted. An
inspection of the first two series of the Journal shows relatively little of
importance in petrology published in this country; a few analyses of rocks,
the observations that the geologists of those days made upon the rocks, as to
their component minerals and structures, aided only by the pocket lens.
Many ideas were put forward, the essentials of which have persisted to the
present day and have become interwoven into the science, whereas others
gave rise to contentions which have not yet been settled to the satisfaction
of all. At times in these earlier days the microscope was called into use to
help in solving questions regarding the finer grained rocks, but this
employment, as Zirkel has shown, was merely incidental, and no definite
technique or purpose for the instrument was established.
On the other hand, the fact that up to the middle of the last century a
large store of information relating to the occurrence of rocks, and to the
mineral composition of those of coarser grain, and somewhat in respect to
their structure, had been accumulated, caused attempts in one way or
another to find means of coördinating these data and to produce
classifications, such as those of Von Cotta and Cordier. The history of these
attempts at classification, before the revelations made by the use of the
microscope had become general, has been admirably reviewed by Whitman
Cross[107] and need not be further enlarged upon here.
That a considerable amount of work was done along chemical lines also
is testified to by the publication of Roth’s Tabellen in 1861, in which all
published analyses of rocks up to that date were collected. What was
accomplished during this period was done chiefly on the continent of
Europe, and little attention had been paid to the subject of rocks either in
America or in Great Britain—even so late as 1870 Geikie remarks, as
referred to by Cross,[108] that there was no good English treatise on
petrography, or the classification and description of rocks. In this country
still less had been accomplished, interest being almost wholly confined to
the vigorous and growing sciences of geology and mineralogy. This was
natural, for mineralogy is the chief buttress on which the structure of
petrology rests and must naturally develop first, especially in a relatively
new and unexplored region, whose mineral resources first attract attention.
The geologists in carrying out their studies also observed the rocks as they
saw them in the field and made incidental reference to them, but
investigations of the rocks themselves was very little attempted. An
inspection of the first two series of the Journal shows relatively little of
importance in petrology published in this country; a few analyses of rocks,
Page 272
occasional mention of mineral composition, of weathering properties, and
notices of methods of classification proposed by French and German
geologists nearly exhaust the list.
notices of methods of classification proposed by French and German
geologists nearly exhaust the list.
Page 273
Introduction of the Microscope.
The beginnings of a particular branch of science are generally obscure
and rooted so imperceptibly in the foundations on which it rests that it is
difficult to point to any particular place in its development and say that this
is the start. There are exceptions of course, like the remarkable work of
Willard Gibbs in physical chemistry, and it may chance that the happy
inspiration of a single worker may give such direction to methods of
investigation as to open the gates into a whole new realm of research, and to
thus create a separate scientific field, as happened in Radiochemistry.
This is what occurred in petrology when Sorby in England, in 1858,[109]
pointed out the value of the microscope as an instrument of research in
geologic investigations, and demonstrated that its employment in the study
of thin sections of rocks would yield information of the highest value.
Others beside Sorby had made use of the microscope, as pointed out by
Zirkel,[110] but, as he indicates, no one before him had recognized its value.
During the next ten years or so, however, its recognition was very slow and
the papers published by Sorby himself were mainly concerned in settling
very special matters.
As Williams[111] has suggested, the greatest service of Sorby was, perhaps,
his instructing Zirkel in his ideas and methods, for the latter threw himself
whole-heartedly into the study of rocks by the aid of the microscope and his
discoveries stimulated other workers in this field in Germany, his native
country, until the dawning science of petrology began to assume form. A
further step forward was taken in 1873 in the appearance of the text-books
of Zirkel[112] and Rosenbusch[113] which collated the knowledge which had
been gained and furnished the investigator more precise methods of work. It
is difficult for the student of to-day to realize how much had been learned in
the interval and, for that matter, how much has been gained since 1873,
without an inspection of these now obsolete texts. In 1863, Zirkel, who was
then at the beginning of his work, said in his first paper presented to the
Vienna Academy of Sciences[114] that if he confined himself chiefly to the
structure of the rocks investigated and of their component minerals, and
stated little as to what these minerals were, the reason for that was because
“although the microscope serves splendidly for the investigation of the
The beginnings of a particular branch of science are generally obscure
and rooted so imperceptibly in the foundations on which it rests that it is
difficult to point to any particular place in its development and say that this
is the start. There are exceptions of course, like the remarkable work of
Willard Gibbs in physical chemistry, and it may chance that the happy
inspiration of a single worker may give such direction to methods of
investigation as to open the gates into a whole new realm of research, and to
thus create a separate scientific field, as happened in Radiochemistry.
This is what occurred in petrology when Sorby in England, in 1858,[109]
pointed out the value of the microscope as an instrument of research in
geologic investigations, and demonstrated that its employment in the study
of thin sections of rocks would yield information of the highest value.
Others beside Sorby had made use of the microscope, as pointed out by
Zirkel,[110] but, as he indicates, no one before him had recognized its value.
During the next ten years or so, however, its recognition was very slow and
the papers published by Sorby himself were mainly concerned in settling
very special matters.
As Williams[111] has suggested, the greatest service of Sorby was, perhaps,
his instructing Zirkel in his ideas and methods, for the latter threw himself
whole-heartedly into the study of rocks by the aid of the microscope and his
discoveries stimulated other workers in this field in Germany, his native
country, until the dawning science of petrology began to assume form. A
further step forward was taken in 1873 in the appearance of the text-books
of Zirkel[112] and Rosenbusch[113] which collated the knowledge which had
been gained and furnished the investigator more precise methods of work. It
is difficult for the student of to-day to realize how much had been learned in
the interval and, for that matter, how much has been gained since 1873,
without an inspection of these now obsolete texts. In 1863, Zirkel, who was
then at the beginning of his work, said in his first paper presented to the
Vienna Academy of Sciences[114] that if he confined himself chiefly to the
structure of the rocks investigated and of their component minerals, and
stated little as to what these minerals were, the reason for that was because
“although the microscope serves splendidly for the investigation of the
Page 274
former relations, it promises very little help for the latter. Labradorite,
oligoclase and orthoclase, augite and hornblende, minerals whose
recognition offers the most important problems in petrography, in most
cases cannot be distinguished from one another under the microscope.”
How little could Zirkel have foreseen, at this time, less than forty years
later, that not only could labradorite be accurately determined in a rock-
section, but that in a few minutes by the making of two or three
measurements on a properly selected section, its chemical composition and
the crystallographic orientation of the section itself could be determined!
oligoclase and orthoclase, augite and hornblende, minerals whose
recognition offers the most important problems in petrography, in most
cases cannot be distinguished from one another under the microscope.”
How little could Zirkel have foreseen, at this time, less than forty years
later, that not only could labradorite be accurately determined in a rock-
section, but that in a few minutes by the making of two or three
measurements on a properly selected section, its chemical composition and
the crystallographic orientation of the section itself could be determined!
Page 275
The Thin Section.
Before going further we may pause here a moment to consider the origin
and development of the thin section, without which no progress could have
been made in this field of research. When we reflect upon the matter, it
seems a marvelous thing indeed that the densest, blackest rock can be made
to yield a section of the ¹⁄₁₀₀₀ of an inch in thickness, so thin and transparent
that fine printing can be easily read through it, and transmitting light so
clearly that the most high-powered objectives of the microscope can be
used to discern and study the minutest structures it presents with the same
capacity that they can be employed upon sections of organic material
prepared by the microtome. This is no small achievement.
The first thin sections appear to have been prepared in 1828 by William
Nicol of Edinburgh, to whom we owe the prism which carries his name. He
undertook the making of sections from fossil wood for the purpose of
studying its structure. The method he developed was in principle the same
as that employed to-day, where machinery is not used; that is, he ground a
flat smooth surface upon one side of a chip of his petrified wood, then
cemented this to a bit of glass plate with Canada balsam, and ground down
the other side until the section was sufficiently thin. This method was used
by others for the study of fossil woods, coal, etc., but it was not applied to
rocks until 1850, when Sorby used it for investigating a calcareous grit.
Oschatz, in Germany, also about this time independently discovered the
same method. A further advance was made in melting the cement, floating
off the slice, and transferring it to a suitable object-glass with cover, a
process still employed by many; though most operators now cement the
first prepared surface of the rock chip directly to the object-glass, and
mount the section without transferring it.
Next came the use of machinery to save labor in grinding, and another
step was made in the introduction of the saw, a circular disk of sheet iron
whose edge was furnished with embedded diamond dust. This makes it
possible to cut relatively thin slices with comparative rapidity, but the final
grinding which requires experience and skill must still be done by hand.
Carborundum has also largely replaced emery. The skill and technique of
Before going further we may pause here a moment to consider the origin
and development of the thin section, without which no progress could have
been made in this field of research. When we reflect upon the matter, it
seems a marvelous thing indeed that the densest, blackest rock can be made
to yield a section of the ¹⁄₁₀₀₀ of an inch in thickness, so thin and transparent
that fine printing can be easily read through it, and transmitting light so
clearly that the most high-powered objectives of the microscope can be
used to discern and study the minutest structures it presents with the same
capacity that they can be employed upon sections of organic material
prepared by the microtome. This is no small achievement.
The first thin sections appear to have been prepared in 1828 by William
Nicol of Edinburgh, to whom we owe the prism which carries his name. He
undertook the making of sections from fossil wood for the purpose of
studying its structure. The method he developed was in principle the same
as that employed to-day, where machinery is not used; that is, he ground a
flat smooth surface upon one side of a chip of his petrified wood, then
cemented this to a bit of glass plate with Canada balsam, and ground down
the other side until the section was sufficiently thin. This method was used
by others for the study of fossil woods, coal, etc., but it was not applied to
rocks until 1850, when Sorby used it for investigating a calcareous grit.
Oschatz, in Germany, also about this time independently discovered the
same method. A further advance was made in melting the cement, floating
off the slice, and transferring it to a suitable object-glass with cover, a
process still employed by many; though most operators now cement the
first prepared surface of the rock chip directly to the object-glass, and
mount the section without transferring it.
Next came the use of machinery to save labor in grinding, and another
step was made in the introduction of the saw, a circular disk of sheet iron
whose edge was furnished with embedded diamond dust. This makes it
possible to cut relatively thin slices with comparative rapidity, but the final
grinding which requires experience and skill must still be done by hand.
Carborundum has also largely replaced emery. The skill and technique of
Page 276
preparers has reached a point where sections of rocks of the desired
thinness (0·001 inch), and four or five inches square have been exhibited.
thinness (0·001 inch), and four or five inches square have been exhibited.
Page 277
The Era of Petrography.
In these earlier days of the science, as noted above, great difficulty was at
first experienced in the recognition of the minerals as they were
encountered in the study of rocks under the microscope. At that time the
chemical composition and outward crystal form of minerals were relatively
much better known than their physical and, especially, their optical
properties and constants. Some beginnings in this had been made by
Brewster, Nicol, and other physicists, and the mineralogists had
commenced to study minerals from this viewpoint. Especially Des
Cloiseaux had devoted himself to determining the optical properties of
many minerals, and the writer, when a student in the laboratory of
Rosenbusch in 1890, well recalls the tribute that he paid to the work of Des
Cloiseaux for the aid which it had afforded him in his earlier researches in
petrography.
The twenty years following the publication of the texts of Rosenbusch
and Zirkel may be characterized as the era of microscopical petrography. A
distinction is drawn here between the latter word and petrology, a
distinction often overlooked, for petrography means literally the description
of rocks, whereas petrology denotes the science of rocks. As time passed the
broader and more fundamental features of rocks, especially of igneous and
metamorphic rocks, in addition to their mineral constitution, were more
studied and gained greater recognition, petrography gradually became a
department of the larger field of petrology—the science of to-day.
The use of the microscope, as soon as the method became more generally
understood, opened up so vast a field for investigation that at first the study
and description of the rocks seemed of prime importance. This was natural,
for hitherto the finer grained rocks had for the most part defied any
adequate elucidation and here was a key which enabled one to read the
cipher. A flood of literature upon the composition, structure, and other
characters of rocks from all parts of the world began to appear in ever
increasing volume. The demands of the petrographers for a greater and
more accurate knowledge of the physical and optical constants of minerals
stimulated this side of mineralogy, and increasing attention was given to
investigations in this direction. No definite line between the two closely
In these earlier days of the science, as noted above, great difficulty was at
first experienced in the recognition of the minerals as they were
encountered in the study of rocks under the microscope. At that time the
chemical composition and outward crystal form of minerals were relatively
much better known than their physical and, especially, their optical
properties and constants. Some beginnings in this had been made by
Brewster, Nicol, and other physicists, and the mineralogists had
commenced to study minerals from this viewpoint. Especially Des
Cloiseaux had devoted himself to determining the optical properties of
many minerals, and the writer, when a student in the laboratory of
Rosenbusch in 1890, well recalls the tribute that he paid to the work of Des
Cloiseaux for the aid which it had afforded him in his earlier researches in
petrography.
The twenty years following the publication of the texts of Rosenbusch
and Zirkel may be characterized as the era of microscopical petrography. A
distinction is drawn here between the latter word and petrology, a
distinction often overlooked, for petrography means literally the description
of rocks, whereas petrology denotes the science of rocks. As time passed the
broader and more fundamental features of rocks, especially of igneous and
metamorphic rocks, in addition to their mineral constitution, were more
studied and gained greater recognition, petrography gradually became a
department of the larger field of petrology—the science of to-day.
The use of the microscope, as soon as the method became more generally
understood, opened up so vast a field for investigation that at first the study
and description of the rocks seemed of prime importance. This was natural,
for hitherto the finer grained rocks had for the most part defied any
adequate elucidation and here was a key which enabled one to read the
cipher. A flood of literature upon the composition, structure, and other
characters of rocks from all parts of the world began to appear in ever
increasing volume. The demands of the petrographers for a greater and
more accurate knowledge of the physical and optical constants of minerals
stimulated this side of mineralogy, and increasing attention was given to
investigations in this direction. No definite line between the two closely
Page 278
related sciences could be drawn, and a large part of the work published
under the heading of petrography could perhaps be as well, or better,
described under the title of micro-mineralogy. To some, in truth, the rocks
presented themselves simply as aggregates of minerals, occurring in fine
grains.
The work of the German petrographers attracted attention and drew
students from all parts of the world to their laboratories, especially to those
of Zirkel and Rosenbusch. The great opportunities, facilities, and freedom
for work which the German universities had long offered to foreign students
of science naturally encouraged this. In France a brilliant school of
petrologists, under the able leadership of Michel-Lévy and Fouqué, had
arisen whose work has been continued by Barrois, Lacroix and others, but
the rigid structure of the French universities at that period did not permit of
the offering of great inducements for the attendance of foreign students. The
work of the French petrographers will be noticed in another connection.
In Great Britain, the home of Sorby, the new science progressed at first
slowly, until it was taken up by Allport, Bonney, Judd, Rutley, and others.
In 1885 the evidence of the advance that had been made and of the firm
basis on which the new science was now placed appeared in Teall’s great
work, “British Petrography,” which marked an epoch in that country in
petrographic publication. This work was of importance also in another
direction than that of descriptive petrography, in that it contains valuable
suggestions for the application of the principles of modern physical
chemistry in solving the problems of the origin of igneous rocks. In it, as in
the publications of Lagorio, we see the passage of the petrographic into the
petrologic phase of the science.
The earliest publication in America of the results of microscopic
investigation of rocks that the writer has been able to find is by A. A. Julien
and C. E. Wright, chiefly on greenstones and chloritic schists from the iron-
bearing regions of upper Michigan.[115] Naturally, it was of a brief and
elementary character. In 1874 E. S. Dana read a paper before the American
Association for the Advancement of Science on the result of his studies on
the “Trap-rocks of the Connecticut valley,” an abstract of which was
published in this Journal.[116] Meanwhile Clarence King, in charge of the
40th Parallel survey, feeling the need of a systematic study of the crystalline
rocks which had been encountered, and finding no one in this country
under the heading of petrography could perhaps be as well, or better,
described under the title of micro-mineralogy. To some, in truth, the rocks
presented themselves simply as aggregates of minerals, occurring in fine
grains.
The work of the German petrographers attracted attention and drew
students from all parts of the world to their laboratories, especially to those
of Zirkel and Rosenbusch. The great opportunities, facilities, and freedom
for work which the German universities had long offered to foreign students
of science naturally encouraged this. In France a brilliant school of
petrologists, under the able leadership of Michel-Lévy and Fouqué, had
arisen whose work has been continued by Barrois, Lacroix and others, but
the rigid structure of the French universities at that period did not permit of
the offering of great inducements for the attendance of foreign students. The
work of the French petrographers will be noticed in another connection.
In Great Britain, the home of Sorby, the new science progressed at first
slowly, until it was taken up by Allport, Bonney, Judd, Rutley, and others.
In 1885 the evidence of the advance that had been made and of the firm
basis on which the new science was now placed appeared in Teall’s great
work, “British Petrography,” which marked an epoch in that country in
petrographic publication. This work was of importance also in another
direction than that of descriptive petrography, in that it contains valuable
suggestions for the application of the principles of modern physical
chemistry in solving the problems of the origin of igneous rocks. In it, as in
the publications of Lagorio, we see the passage of the petrographic into the
petrologic phase of the science.
The earliest publication in America of the results of microscopic
investigation of rocks that the writer has been able to find is by A. A. Julien
and C. E. Wright, chiefly on greenstones and chloritic schists from the iron-
bearing regions of upper Michigan.[115] Naturally, it was of a brief and
elementary character. In 1874 E. S. Dana read a paper before the American
Association for the Advancement of Science on the result of his studies on
the “Trap-rocks of the Connecticut valley,” an abstract of which was
published in this Journal.[116] Meanwhile Clarence King, in charge of the
40th Parallel survey, feeling the need of a systematic study of the crystalline
rocks which had been encountered, and finding no one in this country
Page 279
prepared to undertake it, had induced Zirkel to give his attention to this
task. The result of this labor appeared in 1876 in a fine volume[117] which
attracted great attention. In the same year appeared also petrographical
papers by J. H. Caswell,[118] E. S. Dana[119] and G. W. Hawes.[120] The latter
devoted himself almost entirely to this field of research and may thus,
perhaps, be termed the earliest of the petrographers in this country. His
work, “The Mineralogy and Lithology of New Hampshire,” issued in 1878
as one of the reports of the State Survey under Prof. C. H. Hitchcock, was
the first considerable memoir by an American. This was followed by
various papers, one on the “Albany Granite and its contact phenomena,”[121]
being of especial interest as one of the earliest studies of a contact zone, and
in the fullness of methods employed in attacking the problem forecasting
the change to the petrology era.
During the ten years following, or from 1880 to 1890, the new science of
petrography flourished and grew exceedingly. Many young geologists
abroad devoted themselves to this field of research and the store of
accumulated knowledge concerning rocks from all parts of the world, and
their relations grew apace. The work of Teall has been noticed and among
others might be mentioned the name of Brögger, whose first contribution[122]
in this field gave evidence that his publications would become classics in
the science.
In America there appeared in this period a number of eager workers,
trained in part in the laboratories of Rosenbusch and Zirkel, whose
researches were destined to place the science on the secure footing in this
country which it occupies to-day. Among the earlier of these may be
mentioned Whitman Cross, R. D. Irving, J. P. Iddings, G. H. Williams, J. F.
Kemp, J. S. Diller, B. K. Emerson, M. E. Wadsworth, G. P. Merrill, N. H.
Winchell, and F. D. Adams in Canada. Others were added yearly to this
group. As a result of their work a constantly growing volume of information
about the rocks of America became available, and one has only to examine
the files of the Journal and other periodicals and the listed publications of
the National and State Surveys to appreciate this.
In the Journal, for example, we may refer to papers[123] by Emerson on the
Deerfield dike and its minerals, and on the occurrence of nephelite syenite
at Beemersville, N. J.; to various interesting articles by Cross on lavas from
Colorado and the pneumatolytic and other minerals associated with them; to
task. The result of this labor appeared in 1876 in a fine volume[117] which
attracted great attention. In the same year appeared also petrographical
papers by J. H. Caswell,[118] E. S. Dana[119] and G. W. Hawes.[120] The latter
devoted himself almost entirely to this field of research and may thus,
perhaps, be termed the earliest of the petrographers in this country. His
work, “The Mineralogy and Lithology of New Hampshire,” issued in 1878
as one of the reports of the State Survey under Prof. C. H. Hitchcock, was
the first considerable memoir by an American. This was followed by
various papers, one on the “Albany Granite and its contact phenomena,”[121]
being of especial interest as one of the earliest studies of a contact zone, and
in the fullness of methods employed in attacking the problem forecasting
the change to the petrology era.
During the ten years following, or from 1880 to 1890, the new science of
petrography flourished and grew exceedingly. Many young geologists
abroad devoted themselves to this field of research and the store of
accumulated knowledge concerning rocks from all parts of the world, and
their relations grew apace. The work of Teall has been noticed and among
others might be mentioned the name of Brögger, whose first contribution[122]
in this field gave evidence that his publications would become classics in
the science.
In America there appeared in this period a number of eager workers,
trained in part in the laboratories of Rosenbusch and Zirkel, whose
researches were destined to place the science on the secure footing in this
country which it occupies to-day. Among the earlier of these may be
mentioned Whitman Cross, R. D. Irving, J. P. Iddings, G. H. Williams, J. F.
Kemp, J. S. Diller, B. K. Emerson, M. E. Wadsworth, G. P. Merrill, N. H.
Winchell, and F. D. Adams in Canada. Others were added yearly to this
group. As a result of their work a constantly growing volume of information
about the rocks of America became available, and one has only to examine
the files of the Journal and other periodicals and the listed publications of
the National and State Surveys to appreciate this.
In the Journal, for example, we may refer to papers[123] by Emerson on the
Deerfield dike and its minerals, and on the occurrence of nephelite syenite
at Beemersville, N. J.; to various interesting articles by Cross on lavas from
Colorado and the pneumatolytic and other minerals associated with them; to
Page 280
important papers by Iddings on the rocks of the volcanoes of the Northwest,
and those of the Great Basin, to primary quartz in basalt, and the origin of
lithophysæ; to the results of researches by G. H. Williams on the rocks of
the Cortlandt series, and on peridotite near Syracuse, N. Y.; to papers by
Diller on the peridotites of Kentucky, and recent volcanic eruptions in
California; to articles by R. D. Irving on the copper-bearing and other rocks
of the Lake Superior region, and to Kemp on dikes and other eruptives in
southern New York and northern New Jersey. Other publications would
greatly extend this list.
and those of the Great Basin, to primary quartz in basalt, and the origin of
lithophysæ; to the results of researches by G. H. Williams on the rocks of
the Cortlandt series, and on peridotite near Syracuse, N. Y.; to papers by
Diller on the peridotites of Kentucky, and recent volcanic eruptions in
California; to articles by R. D. Irving on the copper-bearing and other rocks
of the Lake Superior region, and to Kemp on dikes and other eruptives in
southern New York and northern New Jersey. Other publications would
greatly extend this list.
Page 281
The Petrologic Era.
As the chief facts regarding rocks, especially igneous rocks, as to their
mineral and chemical composition, their structure and texture and the limits
within which these are enclosed, became better known; and the relations,
which these bear to the associations of rocks and their modes of occurrence,
began to be perceived, the science assumed a broader aspect. The
perception that rocks were no longer to be regarded merely as interesting
assemblages of minerals, but as entities whose characters and associations
had a meaning, increased. More and better rock analyses stimulated interest
on the chemical side and this and the genesis of their minerals led to a
consideration of the magmas and their functions in rock-making. The fact
that the different kinds of rocks were not scattered indiscriminately, but that
different regions exhibited certain groupings with common characters, was
noticed. These features led to attempts to classify igneous rocks on different
lines from those hitherto employed, and to account for their origin on broad
principles. In other words, the descriptive science of petrography merged
into the broader one of petrology. No exact time can be set which marks this
passage, since the evolution was gradual. Yet for this country, in reviewing
the literature, for which the successive issues of the “Bibliography of North
American Geology” published by the U. S. Geological Survey has been of
the greatest value; the writer has been struck by the fact that in the first
volume containing the index of papers down to and including 1891, the
articles on subjects of this nature are listed under the heading of
petrography, whereas in the second volume (1892–1900) they are grouped
under petrology and the former heading is omitted. A justification for this is
found in examining the list of publications and noting their character. With
some reason, therefore, the beginning of this period may be placed as in the
early years of this decade. Furthermore, it was at this time that the great
work of Zirkel[124] began to appear, which sums up so completely the results
of the petrographic era. Rosenbusch[125] was formulating more definitely his
views on the division of rocks into magmatic groups, as displayed by their
associations in the field, and using this in classification; an idea which,
appearing first in the second edition of his “Physiographie der massigen
Gesteine,” finds fuller development in the third and last editions of this
As the chief facts regarding rocks, especially igneous rocks, as to their
mineral and chemical composition, their structure and texture and the limits
within which these are enclosed, became better known; and the relations,
which these bear to the associations of rocks and their modes of occurrence,
began to be perceived, the science assumed a broader aspect. The
perception that rocks were no longer to be regarded merely as interesting
assemblages of minerals, but as entities whose characters and associations
had a meaning, increased. More and better rock analyses stimulated interest
on the chemical side and this and the genesis of their minerals led to a
consideration of the magmas and their functions in rock-making. The fact
that the different kinds of rocks were not scattered indiscriminately, but that
different regions exhibited certain groupings with common characters, was
noticed. These features led to attempts to classify igneous rocks on different
lines from those hitherto employed, and to account for their origin on broad
principles. In other words, the descriptive science of petrography merged
into the broader one of petrology. No exact time can be set which marks this
passage, since the evolution was gradual. Yet for this country, in reviewing
the literature, for which the successive issues of the “Bibliography of North
American Geology” published by the U. S. Geological Survey has been of
the greatest value; the writer has been struck by the fact that in the first
volume containing the index of papers down to and including 1891, the
articles on subjects of this nature are listed under the heading of
petrography, whereas in the second volume (1892–1900) they are grouped
under petrology and the former heading is omitted. A justification for this is
found in examining the list of publications and noting their character. With
some reason, therefore, the beginning of this period may be placed as in the
early years of this decade. Furthermore, it was at this time that the great
work of Zirkel[124] began to appear, which sums up so completely the results
of the petrographic era. Rosenbusch[125] was formulating more definitely his
views on the division of rocks into magmatic groups, as displayed by their
associations in the field, and using this in classification; an idea which,
appearing first in the second edition of his “Physiographie der massigen
Gesteine,” finds fuller development in the third and last editions of this
Page 282
work. In this country Iddings[126] published an important paper, in which the
family relationships of igneous rocks and the derivation of diverse groups
from a common magma by differentiation are clearly brought out. The
fundamental problems underlying the genesis of igneous rocks had now
been clearly recognized, and with this recognition the science passed into
the petrologic phase. Brögger[127] also had ascribed to the alkalic rocks of
South Norway a common parentage and had pointed out their regional
peculiarities.
From this time forward an attempt may be noted to find an analogy
between rocks and the forms of organic life and to apply those principles of
evolution and descent, which have proved so fruitful in the advancement of
the biological sciences, to the genesis and classification of igneous rocks.
This, perhaps, has on the whole been more apparent than real, in the
constant borrowing of terms from those sciences to express certain features
and relationships observed, or imagined, to obtain among rocks.
Nevertheless, the perception of certain relations which we owe so largely to
Rosenbusch and to Brögger[128] has proved of undoubted value in furnishing
a stimulus for the investigation of new regions, and in affording indications
of what the petrologist should anticipate in his work.
Thus, the labors of the men previously mentioned, with those of Bayley,
Bascom, Cushing, Daly, Lane, Lawson, Lindgren, Pirsson, J. F. Williams,
Washington, and others, have thrown a flood of light upon the igneous
rocks of this continent, and has made it possible to draw many broad
generalizations concerning their origin and distribution. Thus, the
differentiated laccoliths of Montana[129] have been of service in affording
clear examples of the process of local differentiation. Many papers
published in the Journal during the last twenty years show this evolution
and growth of petrological ideas. The contributions from American sources
during this later period, and of which those in the Journal form a
considerable fraction, have indeed been of great weight in shaping the
development and future of the science.
By referring to the files of the Journal, it will be seen that they cover a
continually widening range of subjects concerning rocks, and articles of
theoretical interest are more and more in evidence, along with those of a
purely descriptive character.[130] Thus we find discussions by Becker on the
physical constants of rocks, on fractional crystallization, and on
family relationships of igneous rocks and the derivation of diverse groups
from a common magma by differentiation are clearly brought out. The
fundamental problems underlying the genesis of igneous rocks had now
been clearly recognized, and with this recognition the science passed into
the petrologic phase. Brögger[127] also had ascribed to the alkalic rocks of
South Norway a common parentage and had pointed out their regional
peculiarities.
From this time forward an attempt may be noted to find an analogy
between rocks and the forms of organic life and to apply those principles of
evolution and descent, which have proved so fruitful in the advancement of
the biological sciences, to the genesis and classification of igneous rocks.
This, perhaps, has on the whole been more apparent than real, in the
constant borrowing of terms from those sciences to express certain features
and relationships observed, or imagined, to obtain among rocks.
Nevertheless, the perception of certain relations which we owe so largely to
Rosenbusch and to Brögger[128] has proved of undoubted value in furnishing
a stimulus for the investigation of new regions, and in affording indications
of what the petrologist should anticipate in his work.
Thus, the labors of the men previously mentioned, with those of Bayley,
Bascom, Cushing, Daly, Lane, Lawson, Lindgren, Pirsson, J. F. Williams,
Washington, and others, have thrown a flood of light upon the igneous
rocks of this continent, and has made it possible to draw many broad
generalizations concerning their origin and distribution. Thus, the
differentiated laccoliths of Montana[129] have been of service in affording
clear examples of the process of local differentiation. Many papers
published in the Journal during the last twenty years show this evolution
and growth of petrological ideas. The contributions from American sources
during this later period, and of which those in the Journal form a
considerable fraction, have indeed been of great weight in shaping the
development and future of the science.
By referring to the files of the Journal, it will be seen that they cover a
continually widening range of subjects concerning rocks, and articles of
theoretical interest are more and more in evidence, along with those of a
purely descriptive character.[130] Thus we find discussions by Becker on the
physical constants of rocks, on fractional crystallization, and on
Page 283
differentiation; by Cross on classification; by Adams on the physical
properties of rocks; by Daly on the methods of igneous intrusion; by Wright
on schistosity; by Fenner on the crystallization of basaltic magma; by
Bowen on differentiation by crystallization; by the writer on
complementary rocks and on the origin of phenocrysts; by Smyth on the
origin of alkalic rocks; by Murgoci on the genesis of riebeckite rocks; and
by Barrell on contact-metamorphism. These may serve as examples,
selected almost at random, from the files of the Journal, and we find with
them articles descriptive of the petrology of many particular regions, which
often contain also matter of general interest and importance, such as papers
by Lindgren on the granodiorite and related rocks of the Sierra Nevada; by
Ransome on latite; by Cross on the Leucite Hills; by Hague on the lavas of
the Yellowstone Park; by Pogue on ancient volcanic rocks from North
Carolina; by Warren on peridotites from Cumberland, R. I.; on sandstone
from Texas by Goldman; and on the petrology of various localities in
central New Hampshire by Washington and the writer. Such a list could of
course be much extended and other papers of importance be cited, but
enough has been said to indicate how important a repository of the results
of petrologic research the Journal has been and continues to be.
In thus looking backward over the list of active workers we are
involuntarily led to pause and reflect how great a loss American petrology
has sustained in the premature death of some of its most brilliant and
promising exponents; it is only necessary to recall the names of R. D.
Irving, G. H. Williams, G. W. Hawes, J. F. Williams and Carville Lewis, to
appreciate this.
The store of material gathered during these years has led to the
publication of extensive memoirs, in which the science is treated not from
the older descriptive side, but from the theoretical standpoint and of
classification.[131] In these works strong divergencies of views and opinions
are observed, which is a healthy sign in a developing science.
It should be also noted that along with this evolution on the theoretical
side there has been a constant improvement in the technique of
investigating rocks. It is only necessary to compare the older handbooks of
Zirkel and Rosenbusch with the many modern treatises on petrographic
methods to be assured of this.[132] It is due on the one hand to the vast
amount of careful work which has been done in accurately determining the
properties of rocks; by Daly on the methods of igneous intrusion; by Wright
on schistosity; by Fenner on the crystallization of basaltic magma; by
Bowen on differentiation by crystallization; by the writer on
complementary rocks and on the origin of phenocrysts; by Smyth on the
origin of alkalic rocks; by Murgoci on the genesis of riebeckite rocks; and
by Barrell on contact-metamorphism. These may serve as examples,
selected almost at random, from the files of the Journal, and we find with
them articles descriptive of the petrology of many particular regions, which
often contain also matter of general interest and importance, such as papers
by Lindgren on the granodiorite and related rocks of the Sierra Nevada; by
Ransome on latite; by Cross on the Leucite Hills; by Hague on the lavas of
the Yellowstone Park; by Pogue on ancient volcanic rocks from North
Carolina; by Warren on peridotites from Cumberland, R. I.; on sandstone
from Texas by Goldman; and on the petrology of various localities in
central New Hampshire by Washington and the writer. Such a list could of
course be much extended and other papers of importance be cited, but
enough has been said to indicate how important a repository of the results
of petrologic research the Journal has been and continues to be.
In thus looking backward over the list of active workers we are
involuntarily led to pause and reflect how great a loss American petrology
has sustained in the premature death of some of its most brilliant and
promising exponents; it is only necessary to recall the names of R. D.
Irving, G. H. Williams, G. W. Hawes, J. F. Williams and Carville Lewis, to
appreciate this.
The store of material gathered during these years has led to the
publication of extensive memoirs, in which the science is treated not from
the older descriptive side, but from the theoretical standpoint and of
classification.[131] In these works strong divergencies of views and opinions
are observed, which is a healthy sign in a developing science.
It should be also noted that along with this evolution on the theoretical
side there has been a constant improvement in the technique of
investigating rocks. It is only necessary to compare the older handbooks of
Zirkel and Rosenbusch with the many modern treatises on petrographic
methods to be assured of this.[132] It is due on the one hand to the vast
amount of careful work which has been done in accurately determining the
Page 284
physical constants of rock-minerals[133] and in arranging these for their
determination microscopically, as in the remarkable studies on the feldspars
by Michel-Lévy, and on the other in researches on the apparatus employed,
and in consequent improvements in them and in ways of using them, as
exemplified in the delicately accurate methods introduced by Wright.[134]
The development of the microscope itself as an instrument of research in
this field and in mineralogy deserves a further word in this connection. The
first step toward making the ordinary microscope of special use in this way
was taken by Henry Fox Talbot of England, when he introduced in 1834 the
employment of the recently invented nicol prisms for testing objects in
polarized light. The modern instrument may be said to date from the design
offered by Rosenbusch in 1876. Since that time there have been constant
improvements, almost year by year, until the instrument has become one of
great precision and convenience, remarkably well adapted for the work it is
called upon to perform, with special designs for various kinds of use, and an
almost endless number of accessory appliances for research in different
branches of mineralogy and crystallography, as well as in petrography
proper.[135] This also calls to mind the fact that for the convenience of those
who are not able to use the microscope special manuals of petrology have
been prepared in which rocks are treated from the megascopic standpoint.
[136]
determination microscopically, as in the remarkable studies on the feldspars
by Michel-Lévy, and on the other in researches on the apparatus employed,
and in consequent improvements in them and in ways of using them, as
exemplified in the delicately accurate methods introduced by Wright.[134]
The development of the microscope itself as an instrument of research in
this field and in mineralogy deserves a further word in this connection. The
first step toward making the ordinary microscope of special use in this way
was taken by Henry Fox Talbot of England, when he introduced in 1834 the
employment of the recently invented nicol prisms for testing objects in
polarized light. The modern instrument may be said to date from the design
offered by Rosenbusch in 1876. Since that time there have been constant
improvements, almost year by year, until the instrument has become one of
great precision and convenience, remarkably well adapted for the work it is
called upon to perform, with special designs for various kinds of use, and an
almost endless number of accessory appliances for research in different
branches of mineralogy and crystallography, as well as in petrography
proper.[135] This also calls to mind the fact that for the convenience of those
who are not able to use the microscope special manuals of petrology have
been prepared in which rocks are treated from the megascopic standpoint.
[136]
Page 285
Metamorphic Rocks.
In this connection the metamorphic rocks should not be forgotten. They
afford indeed the most difficult problems with which the geologist has to
deal; every branch of geological science may in turn be called upon to
furnish its quota for help in solving them. Under the attack of careful,
accurate and persistent work in the field, under the microscope and in the
chemical laboratory, with the aid of the garnered knowledge in petrology,
stratigraphy, physiography, and other fields of geologic science, their
mystery has in large part given way. The inaugural work of Lehmann,
Lossen, Barrois, Bonney, Teall, and other European geologists, was
paralleled in America by that of R. D. Irving, owing to whose efforts the
Lake Superior region became the chief place of study of the metamorphic
rocks in this country. Irving soon obtained the assistance of G. H. Williams,
who had been engaged in the study of such rocks, and the latter published a
memoir on the greenstone schist areas of Menominee and Marquette in
Michigan[137] which will always remain one of the classics in the literature
of metamorphic rocks. Irving’s own contributions to petrology, though
valuable, were cut short by his untimely death, but the study of this region
under the direction of his associate and successor, C. R. Van Hise, with his
co-laborers, has yielded a mass of information of fundamental importance
in our understanding of metamorphism and the crystalline schists. Its
fruitage appears in the memoir by Van Hise[138] which is the authoritative
work of reference on metamorphism, and in various publications by him
and his assistants, Bayley, Clements, Leith, and others. The work of the
Canadian geologists, and of Kemp, Cushing, Smyth and Miller in the
Adirondack region, should also be mentioned in connection with this field
of petrology.
In this connection the metamorphic rocks should not be forgotten. They
afford indeed the most difficult problems with which the geologist has to
deal; every branch of geological science may in turn be called upon to
furnish its quota for help in solving them. Under the attack of careful,
accurate and persistent work in the field, under the microscope and in the
chemical laboratory, with the aid of the garnered knowledge in petrology,
stratigraphy, physiography, and other fields of geologic science, their
mystery has in large part given way. The inaugural work of Lehmann,
Lossen, Barrois, Bonney, Teall, and other European geologists, was
paralleled in America by that of R. D. Irving, owing to whose efforts the
Lake Superior region became the chief place of study of the metamorphic
rocks in this country. Irving soon obtained the assistance of G. H. Williams,
who had been engaged in the study of such rocks, and the latter published a
memoir on the greenstone schist areas of Menominee and Marquette in
Michigan[137] which will always remain one of the classics in the literature
of metamorphic rocks. Irving’s own contributions to petrology, though
valuable, were cut short by his untimely death, but the study of this region
under the direction of his associate and successor, C. R. Van Hise, with his
co-laborers, has yielded a mass of information of fundamental importance
in our understanding of metamorphism and the crystalline schists. Its
fruitage appears in the memoir by Van Hise[138] which is the authoritative
work of reference on metamorphism, and in various publications by him
and his assistants, Bayley, Clements, Leith, and others. The work of the
Canadian geologists, and of Kemp, Cushing, Smyth and Miller in the
Adirondack region, should also be mentioned in connection with this field
of petrology.
Page 286
Chemical Analyses of Rocks.
It has been previously pointed out that, as the science of petrology grew,
chemical investigations of rocks in bulk were undertaken. The object of
such analyses was to obtain on the one hand a better control over the
mineral composition and on the other to gain an idea of the nature of the
magmas from which igneous rocks had formed. The earliest analysis of an
American rock of which I can find record is of a “wacke” by J. W. Webster
given in the first volume of the Journal, page 296, 1818.
During the next 40 years a few occasional analyses were undertaken by
American chemists, by C. T. Jackson, T. Sterry Hunt, and others. In 1861,
Justus Roth published the first edition of his Tabellen, in which he included
all analyses which had been made to that date and which he considered
were worthy of preservation. Although, naturally, from the status of
analytical chemistry up to that time, most of these would now be considered
rather crude, the publication of the work was of great service and marked an
epoch in geochemistry. In these tables Roth lists four analyses of American
igneous rocks, two from the Lake Superior region by Jackson and J. D.
Whitney and two by European chemists, one of whom was Bunsen. The
material of the last two was a “dolerite” and the same locality is given for
each—“Sierra Nevada between 38° and 41°” which was probably
considered quite precise for western America in those days.
From these feeble beginnings the forward progress of petrology on the
chemical side in this country has been a steady one until its development
has reached the point which will be indicated in what follows.
The collection of material by the various State surveys and by those
initiated by the National Government led to an increasing number of rocks
being analyzed during the petrographic period. These became also
increasingly good in quality, like those published by G. W. Hawes in his
papers. When, however, chemists were appointed to definite positions on
the staffs of the Government surveys and especially when, after the
organization of the U. S. Geological Survey in 1879, a general central
laboratory was founded in 1883 with F. W. Clarke in charge, then a new era
in the chemical investigation of rocks may be said to have started. In this
It has been previously pointed out that, as the science of petrology grew,
chemical investigations of rocks in bulk were undertaken. The object of
such analyses was to obtain on the one hand a better control over the
mineral composition and on the other to gain an idea of the nature of the
magmas from which igneous rocks had formed. The earliest analysis of an
American rock of which I can find record is of a “wacke” by J. W. Webster
given in the first volume of the Journal, page 296, 1818.
During the next 40 years a few occasional analyses were undertaken by
American chemists, by C. T. Jackson, T. Sterry Hunt, and others. In 1861,
Justus Roth published the first edition of his Tabellen, in which he included
all analyses which had been made to that date and which he considered
were worthy of preservation. Although, naturally, from the status of
analytical chemistry up to that time, most of these would now be considered
rather crude, the publication of the work was of great service and marked an
epoch in geochemistry. In these tables Roth lists four analyses of American
igneous rocks, two from the Lake Superior region by Jackson and J. D.
Whitney and two by European chemists, one of whom was Bunsen. The
material of the last two was a “dolerite” and the same locality is given for
each—“Sierra Nevada between 38° and 41°” which was probably
considered quite precise for western America in those days.
From these feeble beginnings the forward progress of petrology on the
chemical side in this country has been a steady one until its development
has reached the point which will be indicated in what follows.
The collection of material by the various State surveys and by those
initiated by the National Government led to an increasing number of rocks
being analyzed during the petrographic period. These became also
increasingly good in quality, like those published by G. W. Hawes in his
papers. When, however, chemists were appointed to definite positions on
the staffs of the Government surveys and especially when, after the
organization of the U. S. Geological Survey in 1879, a general central
laboratory was founded in 1883 with F. W. Clarke in charge, then a new era
in the chemical investigation of rocks may be said to have started. In this
Page 287
connection should be mentioned the work of W. F. Hillebrand, who set a
standard of accuracy and detail in rock analysis which had not hitherto been
attempted. As a consequence of his accurate and thorough methods and
results the mass of analyses performed by him and his fellow chemists in
this laboratory affords us the greatest single contribution to chemical
petrology which has been made. Up to January, 1914, the report of
Clarke[139] lists some 8000 analyses of various kinds made in this laboratory
for geologic purposes. Nearly everywhere also a great improvement in the
quality of rock-analyses is to be noted, and in the manuals of Hillebrand[140]
and Washington[141] the rock analyst has now at his command the methods
of a greatly perfected technique which should insure him the best results.
Roth’s Tabellen have been previously mentioned; several supplements
were published, but after his death a long interval elapsed before this
convenient and useful work was again taken up by Washington[142] and
Osann.[143] A new edition of Washington’s Tables has recently been
published, listing some 8600 analyses of igneous rocks made up to the close
of 1913.[144]
On the theoretical side also, where petrology passes into geology, the
investigator of to-day will find a mass of most useful and accurate data well
discussed in the modern representative of Bischof’s Chemical Geology—
Clarke’s Data of Geochemistry.[145] The advance on the chemical side,
therefore, has been quite commensurate with that in the microscope as an
instrument, and in the results obtained by it.
standard of accuracy and detail in rock analysis which had not hitherto been
attempted. As a consequence of his accurate and thorough methods and
results the mass of analyses performed by him and his fellow chemists in
this laboratory affords us the greatest single contribution to chemical
petrology which has been made. Up to January, 1914, the report of
Clarke[139] lists some 8000 analyses of various kinds made in this laboratory
for geologic purposes. Nearly everywhere also a great improvement in the
quality of rock-analyses is to be noted, and in the manuals of Hillebrand[140]
and Washington[141] the rock analyst has now at his command the methods
of a greatly perfected technique which should insure him the best results.
Roth’s Tabellen have been previously mentioned; several supplements
were published, but after his death a long interval elapsed before this
convenient and useful work was again taken up by Washington[142] and
Osann.[143] A new edition of Washington’s Tables has recently been
published, listing some 8600 analyses of igneous rocks made up to the close
of 1913.[144]
On the theoretical side also, where petrology passes into geology, the
investigator of to-day will find a mass of most useful and accurate data well
discussed in the modern representative of Bischof’s Chemical Geology—
Clarke’s Data of Geochemistry.[145] The advance on the chemical side,
therefore, has been quite commensurate with that in the microscope as an
instrument, and in the results obtained by it.
Page 288
Physico-Chemical Work.
The study of geological results by experimental methods, which should
gain information concerning the processes by which those results are
caused, and the conditions under which they operate, has been from the
earliest days of the developing science recognized as most important, and
the record of the literature shows considerable was done in this direction.
Experimental work in modern petrology may, however, be considered to
date from 1882 when Fouqué and Michel-Lévy[146] published the results of
their extensive researches on the synthesis of minerals and rocks by
pyrogenous methods. The brilliant experiments of the French petrologists at
once attracted attention, and since that time a considerable volume of
valuable work has been done in this field by a number of men, among
whom may be mentioned Morozewicz,[147] Doelter,[148] Tamman,[149] and
Meunier.[150] As this work continued the results of the rapid advances made
in physical chemistry began to be applied in this field with increasing value.
To J. H. L. Vogt we owe a valuable series of papers,[151] in which the
formation of minerals and rocks from magmas is treated from this
standpoint. Most important of all for the future of petrology has been the
founding in Washington of the splendid research institution, the Carnegie
Geophysical Laboratory, under the leadership of Dr. A. L. Day with its
corps of trained physicists, chemists and petrologists, devoted to the solving
of the problems which the progress of geological science raises. The
publications of this institution (many of them published in the Journal) are
too numerous to be mentioned here; many of them treat successfully of
matters of the greatest importance in petrology. This is an earnest of what
we may hope in the future. The accumulation of the exact physical and
chemical data, which is its aim, will serve as a necessary check to
hypothetical speculation and bring petrology, and especially petrogenesis,
in line with the other more exact sciences by furnishing quantitative
foundations for its structure of theory to rest upon.
While the achievements of this great organization seem to minimize the
work of the individual investigator in this field, he may take heart by
observing the important results on the strength of rocks under various
conditions which have been obtained by Adams in recent years, data of
The study of geological results by experimental methods, which should
gain information concerning the processes by which those results are
caused, and the conditions under which they operate, has been from the
earliest days of the developing science recognized as most important, and
the record of the literature shows considerable was done in this direction.
Experimental work in modern petrology may, however, be considered to
date from 1882 when Fouqué and Michel-Lévy[146] published the results of
their extensive researches on the synthesis of minerals and rocks by
pyrogenous methods. The brilliant experiments of the French petrologists at
once attracted attention, and since that time a considerable volume of
valuable work has been done in this field by a number of men, among
whom may be mentioned Morozewicz,[147] Doelter,[148] Tamman,[149] and
Meunier.[150] As this work continued the results of the rapid advances made
in physical chemistry began to be applied in this field with increasing value.
To J. H. L. Vogt we owe a valuable series of papers,[151] in which the
formation of minerals and rocks from magmas is treated from this
standpoint. Most important of all for the future of petrology has been the
founding in Washington of the splendid research institution, the Carnegie
Geophysical Laboratory, under the leadership of Dr. A. L. Day with its
corps of trained physicists, chemists and petrologists, devoted to the solving
of the problems which the progress of geological science raises. The
publications of this institution (many of them published in the Journal) are
too numerous to be mentioned here; many of them treat successfully of
matters of the greatest importance in petrology. This is an earnest of what
we may hope in the future. The accumulation of the exact physical and
chemical data, which is its aim, will serve as a necessary check to
hypothetical speculation and bring petrology, and especially petrogenesis,
in line with the other more exact sciences by furnishing quantitative
foundations for its structure of theory to rest upon.
While the achievements of this great organization seem to minimize the
work of the individual investigator in this field, he may take heart by
observing the important results on the strength of rocks under various
conditions which have been obtained by Adams in recent years, data of
Page 289
wide application in theoretical geology. In this field also a special text has
appeared in which the principles and acquired data are given.[152]
appeared in which the principles and acquired data are given.[152]
Page 290
Summary.
In this brief retrospect, giving only the barest outlines and omitting from
necessity much of importance, we have seen petrology grow from
occasional crude experiments into a fully organized science in the last half
century. It has to-day a well-perfected technique, a large volume of
literature, texts treating of general principles, of methods of work,
descriptive handbooks on the morphological side, and has attained general
recognition as a field, which, though not large, is worthy of the
concentration of intellectual endeavor. Like other healthy growing
organisms it has given rise to offshoots, and the sciences of metallography
and of the micro-study of ore deposits, which are rapidly assuming form,
have branched from it.
What of the future? The old days of mostly descriptive work, and of
theorizing purely from observed results, have passed. The science has
entered upon the stage where work and theory must be continually brought
into agreement with chemical, physical and mathematical laws and data,
and in the application of these new problems present themselves. As we
climb, in fact, new horizons open to our view indicating fresh regions for
exploration, for acquiring human knowledge and for our satisfaction.
In this brief retrospect, giving only the barest outlines and omitting from
necessity much of importance, we have seen petrology grow from
occasional crude experiments into a fully organized science in the last half
century. It has to-day a well-perfected technique, a large volume of
literature, texts treating of general principles, of methods of work,
descriptive handbooks on the morphological side, and has attained general
recognition as a field, which, though not large, is worthy of the
concentration of intellectual endeavor. Like other healthy growing
organisms it has given rise to offshoots, and the sciences of metallography
and of the micro-study of ore deposits, which are rapidly assuming form,
have branched from it.
What of the future? The old days of mostly descriptive work, and of
theorizing purely from observed results, have passed. The science has
entered upon the stage where work and theory must be continually brought
into agreement with chemical, physical and mathematical laws and data,
and in the application of these new problems present themselves. As we
climb, in fact, new horizons open to our view indicating fresh regions for
exploration, for acquiring human knowledge and for our satisfaction.
Page 291
Bibliography.
107. W. Cross, Jour. Geology, 10, 451, 1902.
108. Ibid., p. 45.
109. Sorby, Quart. Jour. Geol. Soc., 14, 453, 1858.
110. Zirkel, Einführung des Mikroskops in das mineralogisch-geologische Studium, 1881.
111. Williams, G. H., Modern Petrography, 1886.
112. Zirkel, Mikroskopische Beschaffenheit der Mineralien und Gesteine.
113. Rosenbusch, Mikroskopische Physiographie der petrographisch wichtigen Mineralien.
114. Zirkel, Mikroskopische Gesteinstudien, Sitzung vom 12 März, 1863.
115. Julien and Wright, Geol. Surv. of Michigan, 2, 1873. Appendices A and C.
116. Dana, E. S., the Journal, 8, 390–392, 1874.
117. Zirkel, Geological Exploration of the 40th Parallel; vol. VI, Microscopical Petrography.
118. Caswell, Microscopical Petrography of the Black Hills. U. S. Geog. and Geol. Surv. Rocky
Mts. Rep. on Black Hills of Dakota, 469–527. The separate copies issued bear the imprint 1876; the
complete report 1880.
119. Dana, E. S., Igneous Rocks in the Judith Mts. Rep. of Reconnaissance Carroll, Mont., to
Yellowstone Park in 1875. Col. Wm. Ludlow, War Dept., Washington, 105–106.
120. Hawes, G. W., Rocks of the Chlorite Formation, etc., the Journal, 11, 122–126, 1876.
Greenstones of New Hampshire, etc, ibid., 12, 129–137, 1876.
121. Hawes, G. W., the Journal, 21, 21–32, 1881.
122. Brögger, Die silurischen Etagen 2 und 3, Kristiania, 1882.
123. The references for the papers alluded to, all of them in the Journal, are as follows:
Emerson, 24, 195–202, 270–278, 349–359, 1882;
——, 23, 302–308, 1882.
Cross, 27, 94–96, 1884; 31, 432–438, 1886; 39, 359–370, 1890; 41, 466–475, 1891; 23,
452–458, 1882.
Iddings, 26, 222–235, 1883;
——, 27, 453–463, 1884;
——, 36, 208–221, 1888;
——, 33, 36–45, 1887.
Williams, 31, 26–41, 1886; 33, 135–144, 191–199, 1887; 35, 433–448, 1888; 36, 254–259,
1888.
107. W. Cross, Jour. Geology, 10, 451, 1902.
108. Ibid., p. 45.
109. Sorby, Quart. Jour. Geol. Soc., 14, 453, 1858.
110. Zirkel, Einführung des Mikroskops in das mineralogisch-geologische Studium, 1881.
111. Williams, G. H., Modern Petrography, 1886.
112. Zirkel, Mikroskopische Beschaffenheit der Mineralien und Gesteine.
113. Rosenbusch, Mikroskopische Physiographie der petrographisch wichtigen Mineralien.
114. Zirkel, Mikroskopische Gesteinstudien, Sitzung vom 12 März, 1863.
115. Julien and Wright, Geol. Surv. of Michigan, 2, 1873. Appendices A and C.
116. Dana, E. S., the Journal, 8, 390–392, 1874.
117. Zirkel, Geological Exploration of the 40th Parallel; vol. VI, Microscopical Petrography.
118. Caswell, Microscopical Petrography of the Black Hills. U. S. Geog. and Geol. Surv. Rocky
Mts. Rep. on Black Hills of Dakota, 469–527. The separate copies issued bear the imprint 1876; the
complete report 1880.
119. Dana, E. S., Igneous Rocks in the Judith Mts. Rep. of Reconnaissance Carroll, Mont., to
Yellowstone Park in 1875. Col. Wm. Ludlow, War Dept., Washington, 105–106.
120. Hawes, G. W., Rocks of the Chlorite Formation, etc., the Journal, 11, 122–126, 1876.
Greenstones of New Hampshire, etc, ibid., 12, 129–137, 1876.
121. Hawes, G. W., the Journal, 21, 21–32, 1881.
122. Brögger, Die silurischen Etagen 2 und 3, Kristiania, 1882.
123. The references for the papers alluded to, all of them in the Journal, are as follows:
Emerson, 24, 195–202, 270–278, 349–359, 1882;
——, 23, 302–308, 1882.
Cross, 27, 94–96, 1884; 31, 432–438, 1886; 39, 359–370, 1890; 41, 466–475, 1891; 23,
452–458, 1882.
Iddings, 26, 222–235, 1883;
——, 27, 453–463, 1884;
——, 36, 208–221, 1888;
——, 33, 36–45, 1887.
Williams, 31, 26–41, 1886; 33, 135–144, 191–199, 1887; 35, 433–448, 1888; 36, 254–259,
1888.
Page 292
——, 34, 137–145, 1887.
Diller, 32, 121–125, 1886; 37, 219–220, 1889;
——, 33, 45–50, 1887.
Irving (26, 27–32, 321–322, 27, 130–134, 1883; 29, 358–359, 1885).
Kemp (35, 331–332, 1888; 36, 247–253, 1888; 38, 130–134, 1889).
124. Zirkel, Lehrbuch der Petrographie, 2d ed., 1893.
125. Hunter and Rosenbusch, Ueber Monchiquit, etc., Min. petr. Mitth., 11, 445, 1890.
Rosenbusch, Ueber Structur und Class. der Eruptivgesteine, ibid., 12, 351, 1891.
126. Iddings, Origin of Igneous Rocks, Bull. Phil, Soc. Washington, 12, 89–213, 1892.
127. Brögger, Mineralien der Syenit-pegmatit-gànge, etc., Zs. Kryst., 16, 1890.
128. ——, Basic Eruptive Rocks of Gran, Quart. Jour. Geol. Soc., 50, 15, 1894; Grorudit-
Tinguait-Serie, Vidensk. Skrift. 1 Math. nat. Kl., No. 4, 1894.
129. Weed and Pirsson, e. g. Shonkin Sag, the Journal, 12, 1–17, 1901.
130. The references for the articles mentioned (all in the Journal) are as follows:
Becker, 46, 1893; 4, 257, 1897; 3, 21–40, 1897.
Cross, 39, 657–661, 1915.
Adams, 22, 95–123, 1906; 29, 465–487, 1910.
Daly, 22, 195–216, 1906; 26, 17–50, 1908.
Wright, 22, 224–230, 1906.
Fenner, 29, 217–234, 1910.
Bowen, 39, 175–191; 40, 161–185, 1915.
Pirsson, 50, 116–121, 1895; 7, 271–280, 1899.
Smyth, 36, 33–46, 1913.
Murgoci, 20, 133–145, 1905.
Barrell, 13, 279–296, 1902.
Lindgren, 3, 301–314, 1897; 9, 269–282, 1900.
Ransome, 5, 355–375, 1898.
Cross, 4, 115–141, 1897.
Hague, 1, 445–457, 1896.
Pogue, 28, 218–238, 1909.
Warren, 25, 12–36, 1908.
Goldman, 39, 261–288, 1915.
Washington and Pirsson, Belknap Mts., 20, 344–353, 1905; 22, 439–457, 493–515, 1906.
——, Red Hill, 23, 257–276, 433–447, 1907.
——, Tripyramid Mt., 31, 405–431, 1911.
131. Quantitative Classification of Igneous Rocks, Cross, Iddings, Pirsson and Washington,
Chicago, 1903.
Petrogenesis, C. Doelter, Braunschweig, 1906.
Igneous Rocks, vols. 1 and 2, J. P. Iddings, New York, 1909 and 1913.
Problem of Volcanism, Iddings, New Haven, 1914.
Natural History of Igneous Rocks, Alfred Harker, London, 1909.
Diller, 32, 121–125, 1886; 37, 219–220, 1889;
——, 33, 45–50, 1887.
Irving (26, 27–32, 321–322, 27, 130–134, 1883; 29, 358–359, 1885).
Kemp (35, 331–332, 1888; 36, 247–253, 1888; 38, 130–134, 1889).
124. Zirkel, Lehrbuch der Petrographie, 2d ed., 1893.
125. Hunter and Rosenbusch, Ueber Monchiquit, etc., Min. petr. Mitth., 11, 445, 1890.
Rosenbusch, Ueber Structur und Class. der Eruptivgesteine, ibid., 12, 351, 1891.
126. Iddings, Origin of Igneous Rocks, Bull. Phil, Soc. Washington, 12, 89–213, 1892.
127. Brögger, Mineralien der Syenit-pegmatit-gànge, etc., Zs. Kryst., 16, 1890.
128. ——, Basic Eruptive Rocks of Gran, Quart. Jour. Geol. Soc., 50, 15, 1894; Grorudit-
Tinguait-Serie, Vidensk. Skrift. 1 Math. nat. Kl., No. 4, 1894.
129. Weed and Pirsson, e. g. Shonkin Sag, the Journal, 12, 1–17, 1901.
130. The references for the articles mentioned (all in the Journal) are as follows:
Becker, 46, 1893; 4, 257, 1897; 3, 21–40, 1897.
Cross, 39, 657–661, 1915.
Adams, 22, 95–123, 1906; 29, 465–487, 1910.
Daly, 22, 195–216, 1906; 26, 17–50, 1908.
Wright, 22, 224–230, 1906.
Fenner, 29, 217–234, 1910.
Bowen, 39, 175–191; 40, 161–185, 1915.
Pirsson, 50, 116–121, 1895; 7, 271–280, 1899.
Smyth, 36, 33–46, 1913.
Murgoci, 20, 133–145, 1905.
Barrell, 13, 279–296, 1902.
Lindgren, 3, 301–314, 1897; 9, 269–282, 1900.
Ransome, 5, 355–375, 1898.
Cross, 4, 115–141, 1897.
Hague, 1, 445–457, 1896.
Pogue, 28, 218–238, 1909.
Warren, 25, 12–36, 1908.
Goldman, 39, 261–288, 1915.
Washington and Pirsson, Belknap Mts., 20, 344–353, 1905; 22, 439–457, 493–515, 1906.
——, Red Hill, 23, 257–276, 433–447, 1907.
——, Tripyramid Mt., 31, 405–431, 1911.
131. Quantitative Classification of Igneous Rocks, Cross, Iddings, Pirsson and Washington,
Chicago, 1903.
Petrogenesis, C. Doelter, Braunschweig, 1906.
Igneous Rocks, vols. 1 and 2, J. P. Iddings, New York, 1909 and 1913.
Problem of Volcanism, Iddings, New Haven, 1914.
Natural History of Igneous Rocks, Alfred Harker, London, 1909.
Page 293
Igneous Rocks and their Origin, R. A. Daly, New York, 1914.
132. Among these may be mentioned:
Rosenbusch u. Wülfing, Physiog. der petrog. wicht. Min., Stuttgart, 1905.
Iddings, J. P., Rock-Minerals, 1st ed., New York, 1906.
Johannsen, A., Manual of Petrographic Methods, New York, 1914.
Winchell, N. H. and A. N., Elements of Optical Mineralogy, New York, 1909.
133. We may mention here, for example, the work in mineralogy of Penfield, noticed in the
accompanying chapter on mineralogy. In addition to the accurate determination of the composition
and constants of many minerals, some of which have importance from the petrographic standpoint,
we owe to him more than anyone the recognition of fluorine and hydroxyl in a variety of species, and
thereby the perception of their pneumatolytic origin. His papers have been published almost entirely
in the Journal.
134. Wright, Methods of Petrographic-Microscopic Research, Carnegie Inst., Washington, 1911,
and various papers; many in the Journal.
135. Conf. Wright’s work quoted above and the various manuals previously mentioned.
136. Kemp, Hand-book of Rocks, 3d ed., New York, 1904. Pirsson, Rocks and Rock-Minerals,
New York, 1910.
137. Williams, G. H., U. S. Geol. Surv., Bull. 62, Washington, 1890.
138. Van Hise, Treatise on Metamorphism, U. S. Geol. Surv., Monograph 17.
139. F. W. Clarke, U. S. Geol. Surv., Bull. 591, 1915.
140. Hillebrand, Analysis of Silicate and Carbonate Rocks, U. S. Geol. Surv., Bull. 422, 1910.
141. Washington, Chemical Analysis of Rocks, pp. 200, New York, 1910.
142. Id., Chemical Analyses of Igneous Rocks (1884–1900), U. S. Geol. Surv., Prof. Paper, No.
14, 1903.
143. Osann, Beitr. zu chem. Petrogr., II Teil. Anal. d. Eruptivgest., 1884–1900, Stuttgart, 1905.
144. Washington, ibid., 2d ed., U. S. Geol. Surv., Prof. Paper 99, pp. 1216, 1917.
145. Clarke, U. S. Geol. Surv., Bull. 616, 1916.
146. Fouqué and Michel-Lévy, Synthese des Mineraux et des Roches, Paris, 1882.
147. Morozewicz, Exper. Untersuch. u. Bildung der Min. im Magma, Min. petr. Mitt., 18, 1898.
148. Doelter, Synthetische Studien, N. Jahrb. Min. 1897, 1, 1–26. Allg. chem. Mineralogie, etc.
149. Tamman, Krystallisieren und Schmelzen, 1903.
150. St. Meunier, Les Méthodes de Synthèse en Minéralogie, Paris, 1891.
132. Among these may be mentioned:
Rosenbusch u. Wülfing, Physiog. der petrog. wicht. Min., Stuttgart, 1905.
Iddings, J. P., Rock-Minerals, 1st ed., New York, 1906.
Johannsen, A., Manual of Petrographic Methods, New York, 1914.
Winchell, N. H. and A. N., Elements of Optical Mineralogy, New York, 1909.
133. We may mention here, for example, the work in mineralogy of Penfield, noticed in the
accompanying chapter on mineralogy. In addition to the accurate determination of the composition
and constants of many minerals, some of which have importance from the petrographic standpoint,
we owe to him more than anyone the recognition of fluorine and hydroxyl in a variety of species, and
thereby the perception of their pneumatolytic origin. His papers have been published almost entirely
in the Journal.
134. Wright, Methods of Petrographic-Microscopic Research, Carnegie Inst., Washington, 1911,
and various papers; many in the Journal.
135. Conf. Wright’s work quoted above and the various manuals previously mentioned.
136. Kemp, Hand-book of Rocks, 3d ed., New York, 1904. Pirsson, Rocks and Rock-Minerals,
New York, 1910.
137. Williams, G. H., U. S. Geol. Surv., Bull. 62, Washington, 1890.
138. Van Hise, Treatise on Metamorphism, U. S. Geol. Surv., Monograph 17.
139. F. W. Clarke, U. S. Geol. Surv., Bull. 591, 1915.
140. Hillebrand, Analysis of Silicate and Carbonate Rocks, U. S. Geol. Surv., Bull. 422, 1910.
141. Washington, Chemical Analysis of Rocks, pp. 200, New York, 1910.
142. Id., Chemical Analyses of Igneous Rocks (1884–1900), U. S. Geol. Surv., Prof. Paper, No.
14, 1903.
143. Osann, Beitr. zu chem. Petrogr., II Teil. Anal. d. Eruptivgest., 1884–1900, Stuttgart, 1905.
144. Washington, ibid., 2d ed., U. S. Geol. Surv., Prof. Paper 99, pp. 1216, 1917.
145. Clarke, U. S. Geol. Surv., Bull. 616, 1916.
146. Fouqué and Michel-Lévy, Synthese des Mineraux et des Roches, Paris, 1882.
147. Morozewicz, Exper. Untersuch. u. Bildung der Min. im Magma, Min. petr. Mitt., 18, 1898.
148. Doelter, Synthetische Studien, N. Jahrb. Min. 1897, 1, 1–26. Allg. chem. Mineralogie, etc.
149. Tamman, Krystallisieren und Schmelzen, 1903.
150. St. Meunier, Les Méthodes de Synthèse en Minéralogie, Paris, 1891.
Page 294
151. Vogt, Mineralbildung in Smelzmassen, Christiania, 1892; Silikatschmelzlösungen, 1 and 2,
1903, 1904, and various other papers, esp. in Min. petr. Mitt., vols. 24 and 25, 1906.
152. H. E. Boeke, Grundlagen der physikalisch-chemischen Petrographie, Berlin, 1915.
1903, 1904, and various other papers, esp. in Min. petr. Mitt., vols. 24 and 25, 1906.
152. H. E. Boeke, Grundlagen der physikalisch-chemischen Petrographie, Berlin, 1915.
Page 295
VIII
THE GROWTH OF MINERALOGY FROM 1818 TO 1918
By WILLIAM E. FORD
Mineralogy to-day would certainly be generally considered one of the
minor members of the group of the Geological Sciences. We commonly
look upon it in the light of an useful handmaiden, whose chief function is to
serve the other branches, and we are inclined to forget that, in reality,
mineralogy was the first to be recognized and, with considerable truth,
might be claimed as the mother of all the others. Minerals, because of their
frequent beauty of color and form, and their uses as gems and as ornamental
stones, were the first inorganic objects to excite wonder and comment and
we find many of them named and described in very early writings.
Theophrastus (368–284 B. C.), a famous pupil of Aristotle, wrote a treatise
“On Stones” in which he collected a large amount of information about
minerals and fossils. The elder Pliny (23–79 A. D.), more than three
centuries later, in his Natural History, described and named many of the
commoner minerals. At this time it was natural that no clear distinction
should be drawn between minerals and rocks, or even between minerals and
fossils. As long as all study of the materials of the earth’s crust was
concerned with their superficial characters, it was logical to include
everything under the single head. There were some writers in the early
centuries of the Christian era, however, who believed that fossils had been
derived from living animals but the majority considered them to be only
strange and unusual forms of minerals. During many succeeding centuries
little was added to the general store of geological knowledge and it was not
until the beginning of the sixteenth century, that any further notable
THE GROWTH OF MINERALOGY FROM 1818 TO 1918
By WILLIAM E. FORD
Mineralogy to-day would certainly be generally considered one of the
minor members of the group of the Geological Sciences. We commonly
look upon it in the light of an useful handmaiden, whose chief function is to
serve the other branches, and we are inclined to forget that, in reality,
mineralogy was the first to be recognized and, with considerable truth,
might be claimed as the mother of all the others. Minerals, because of their
frequent beauty of color and form, and their uses as gems and as ornamental
stones, were the first inorganic objects to excite wonder and comment and
we find many of them named and described in very early writings.
Theophrastus (368–284 B. C.), a famous pupil of Aristotle, wrote a treatise
“On Stones” in which he collected a large amount of information about
minerals and fossils. The elder Pliny (23–79 A. D.), more than three
centuries later, in his Natural History, described and named many of the
commoner minerals. At this time it was natural that no clear distinction
should be drawn between minerals and rocks, or even between minerals and
fossils. As long as all study of the materials of the earth’s crust was
concerned with their superficial characters, it was logical to include
everything under the single head. There were some writers in the early
centuries of the Christian era, however, who believed that fossils had been
derived from living animals but the majority considered them to be only
strange and unusual forms of minerals. During many succeeding centuries
little was added to the general store of geological knowledge and it was not
until the beginning of the sixteenth century, that any further notable
Page 296
progress was made. Agricola (1494–1555) was a physician, who, for a time,
lived in the mining district of Joachimstal. He studied and described the
minerals that he collected there. He was the first to give careful and critical
descriptions of minerals, of their crystals and general physical properties.
Unfortunately, he also did not realize the fundamental distinction between
fossils and minerals, and probably because of his influence this error
persisted, even until the middle of the eighteenth century. But, naturally, as
the number of scientific students increased, the number of those who
rejected this conclusion grew, until at last, the true character of fossils was
established. The keen interest in minerals and fossils which was aroused by
this controversy, together with the rapid extension of mining operations,
drew the attention of scientific men to other features of the earth’s surface
and led to a more extended investigation of its characters and thus to the
development of geology proper. It is interesting to note also that mineralogy
was the first of the Geological Sciences to be officially recognized and
taught by the universities.
Although, as has been shown, the beginnings of mineralogy lie in the
remote past, the science, as we know it to-day, can be said to have had
practically its whole growth during the last one hundred years. Of the more
than one thousand mineral species that may now be considered as definitely
established hardly more than two hundred were known in the year 1800 and
these were only partially described or understood. It is true that Haüy, the
“father of crystallography,” had before this date discovered and formulated
the laws of crystal symmetry, and had shown that rational relations existed
between the intercepts upon the axes of the different faces of a crystal. It
was not until 1809, however, that Wollaston described the first form of a
reflecting goniometer, and thus made possible the beginning of exact
investigation of crystals. The distinctions between the different crystal
groups were developed by Bernhardi, Weiss and Mohs between the years
1807 and 1820, while the Naumann system of crystal symbols was not
proposed until 1826. The fact that doubly refracting minerals also polarize
light was discovered by Malus in 1808, and in 1813 Brewster first
recognized the optical differences between uniaxial and biaxial minerals.
The modern science of chemistry was also just beginning to develop at this
period, enabling mineralogists to make analyses more and more accurately
and thus by chemical means to establish the true character of minerals, and
to properly classify them.
lived in the mining district of Joachimstal. He studied and described the
minerals that he collected there. He was the first to give careful and critical
descriptions of minerals, of their crystals and general physical properties.
Unfortunately, he also did not realize the fundamental distinction between
fossils and minerals, and probably because of his influence this error
persisted, even until the middle of the eighteenth century. But, naturally, as
the number of scientific students increased, the number of those who
rejected this conclusion grew, until at last, the true character of fossils was
established. The keen interest in minerals and fossils which was aroused by
this controversy, together with the rapid extension of mining operations,
drew the attention of scientific men to other features of the earth’s surface
and led to a more extended investigation of its characters and thus to the
development of geology proper. It is interesting to note also that mineralogy
was the first of the Geological Sciences to be officially recognized and
taught by the universities.
Although, as has been shown, the beginnings of mineralogy lie in the
remote past, the science, as we know it to-day, can be said to have had
practically its whole growth during the last one hundred years. Of the more
than one thousand mineral species that may now be considered as definitely
established hardly more than two hundred were known in the year 1800 and
these were only partially described or understood. It is true that Haüy, the
“father of crystallography,” had before this date discovered and formulated
the laws of crystal symmetry, and had shown that rational relations existed
between the intercepts upon the axes of the different faces of a crystal. It
was not until 1809, however, that Wollaston described the first form of a
reflecting goniometer, and thus made possible the beginning of exact
investigation of crystals. The distinctions between the different crystal
groups were developed by Bernhardi, Weiss and Mohs between the years
1807 and 1820, while the Naumann system of crystal symbols was not
proposed until 1826. The fact that doubly refracting minerals also polarize
light was discovered by Malus in 1808, and in 1813 Brewster first
recognized the optical differences between uniaxial and biaxial minerals.
The modern science of chemistry was also just beginning to develop at this
period, enabling mineralogists to make analyses more and more accurately
and thus by chemical means to establish the true character of minerals, and
to properly classify them.
Page 297
Franz von Kobell, on page 372 of his “Geschichte der Mineralogie,”
somewhat poetically describes the condition of the science at this period as
follows: “With the end of the eighteenth and the commencement of the
nineteenth centuries exact investigations in mineralogy first began. The
mineralogist was no longer content with approximate descriptions of
minerals, but strove rather to separate the essential facts from those that
were accidental, to discover definite laws, and to learn the relations between
the physical and chemical characters of a mineral. The use of mathematics
gave a new aspect to crystallography, and the development of the optical
relationships opened a magnificent field of wonderful phenomena which
can be described as a garden gay with flowers of light, charming in
themselves and interesting in their relations to the forces which guide and
govern the regular structure of matter.”
In the Medical Repository (vol. 2, p. 114, New York, 1799), there occurs
the following notice: “Since the publication of the last number of the
Repository an Association has been formed in the city of New York ‘for the
investigation of the Mineral and Fossil bodies which compose the fabric of
the Globe; and, more especially, for the Natural and Chemical History of
the Minerals and Fossils of the United States,’ by the name and style of The
American Mineralogical Society.” With this announcement is given an
advertisement in which the society “earnestly solicits the citizens of the
United States to communicate to them, on all mineralogical subjects, but
especially on the following: 1, concerning stones suitable for gun flints; 2,
concerning native brimstone or sulphur; 3, concerning salt-petre; 4,
concerning mines and ores of lead.” Further the society asks “that
specimens of all kinds be sent to it for examination and determination.”
This marks apparently the beginning of the serious study of the science
of mineralogy in the United States. From this time on, articles on
mineralogical topics appeared with increasing frequency in the Medical
Repository. Most of these were brief and were largely concerned with the
description of the general characters and modes of occurrence of various
minerals. Nothing of much moment from the scientific point of view
appeared until many years later, but the growing interest in things
mineralogical was clearly manifest. An important stimulus to this increasing
knowledge and discussion was furnished by Col. George Gibbs who, about
the year 1808, brought to this country a large and notable mineral
somewhat poetically describes the condition of the science at this period as
follows: “With the end of the eighteenth and the commencement of the
nineteenth centuries exact investigations in mineralogy first began. The
mineralogist was no longer content with approximate descriptions of
minerals, but strove rather to separate the essential facts from those that
were accidental, to discover definite laws, and to learn the relations between
the physical and chemical characters of a mineral. The use of mathematics
gave a new aspect to crystallography, and the development of the optical
relationships opened a magnificent field of wonderful phenomena which
can be described as a garden gay with flowers of light, charming in
themselves and interesting in their relations to the forces which guide and
govern the regular structure of matter.”
In the Medical Repository (vol. 2, p. 114, New York, 1799), there occurs
the following notice: “Since the publication of the last number of the
Repository an Association has been formed in the city of New York ‘for the
investigation of the Mineral and Fossil bodies which compose the fabric of
the Globe; and, more especially, for the Natural and Chemical History of
the Minerals and Fossils of the United States,’ by the name and style of The
American Mineralogical Society.” With this announcement is given an
advertisement in which the society “earnestly solicits the citizens of the
United States to communicate to them, on all mineralogical subjects, but
especially on the following: 1, concerning stones suitable for gun flints; 2,
concerning native brimstone or sulphur; 3, concerning salt-petre; 4,
concerning mines and ores of lead.” Further the society asks “that
specimens of all kinds be sent to it for examination and determination.”
This marks apparently the beginning of the serious study of the science
of mineralogy in the United States. From this time on, articles on
mineralogical topics appeared with increasing frequency in the Medical
Repository. Most of these were brief and were largely concerned with the
description of the general characters and modes of occurrence of various
minerals. Nothing of much moment from the scientific point of view
appeared until many years later, but the growing interest in things
mineralogical was clearly manifest. An important stimulus to this increasing
knowledge and discussion was furnished by Col. George Gibbs who, about
the year 1808, brought to this country a large and notable mineral
Page 298
collection. In the Medical Repository (vol. 11, p. 213, 1808), is found a
notice of this collection, a portion of which is reproduced below:
notice of this collection, a portion of which is reproduced below:
Page 299
“Gibbs’ grand Collection of Minerals.
One of the most zealous cultivators of mineralogy in the United States is Col. G. Gibbs of Rhode
Island and his taste and his fortune have concurred in making him the proprietor of the most
extensive and valuable assortment of minerals that probably exists in America.
This rich collection consists of the cabinets possessed by the late Mons. Gigot D’Orcy of Paris and
the Count Gregoire de Rozamonsky, a Russian nobleman, long resident in Switzerland. To which the
present proprietor has added a number, either gathered by himself on the spot, or purchased in
different parts of Europe.... The whole consists of about twenty thousand specimens. A small part of
this collection was opened to amateurs at Rhode Island, the last summer, and the next, if
circumstances permit, the remainder will be exposed.”
In 1802 Benjamin Silliman was appointed professor of chemistry and
mineralogy in Yale College. After the Gibbs Collection was brought to
America he spent much time with the owner in studying it and, as a result,
Col. Gibbs offered to place the collection on exhibition in New Haven if
suitable quarters would be furnished by the college. This was quickly
accomplished and in 1810, 1811 and 1812 the collection was transferred to
New Haven and arranged for exhibition by Col. Gibbs. Later, in 1825, it
was purchased by Yale and served as the nucleus about which the present
Museum collection of the University has been formed. There is no doubt
but that the presence at this early date of this large and unusual mineral
collection had a great influence upon the development of mineralogical
science at Yale, and in the country at large.
In the year 1810 Dr. Archibald Bruce started the “American
Mineralogical Journal,” the title page of which reads in part as follows:
“The American Mineralogical Journal, being a Collection of Facts and
Observations tending to elucidate the Mineralogy and Geology of the
United States of America, together with other Information relating to
Mineralogy, Geology and Chemistry, derived from Scientific Sources.”
Unfortunately the health of Dr. Bruce failed, and the journal lasted only
through its first volume. It had, however, “been most favorably received,”
as Silliman remarks, and it was felt that another journal of a similar type
should be instituted. Such a suggestion was made by Col. Gibbs to
Professor Silliman in 1817 and this led directly to the founding of the
American Journal of Science in 1818 under the latter’s editorship. Although
One of the most zealous cultivators of mineralogy in the United States is Col. G. Gibbs of Rhode
Island and his taste and his fortune have concurred in making him the proprietor of the most
extensive and valuable assortment of minerals that probably exists in America.
This rich collection consists of the cabinets possessed by the late Mons. Gigot D’Orcy of Paris and
the Count Gregoire de Rozamonsky, a Russian nobleman, long resident in Switzerland. To which the
present proprietor has added a number, either gathered by himself on the spot, or purchased in
different parts of Europe.... The whole consists of about twenty thousand specimens. A small part of
this collection was opened to amateurs at Rhode Island, the last summer, and the next, if
circumstances permit, the remainder will be exposed.”
In 1802 Benjamin Silliman was appointed professor of chemistry and
mineralogy in Yale College. After the Gibbs Collection was brought to
America he spent much time with the owner in studying it and, as a result,
Col. Gibbs offered to place the collection on exhibition in New Haven if
suitable quarters would be furnished by the college. This was quickly
accomplished and in 1810, 1811 and 1812 the collection was transferred to
New Haven and arranged for exhibition by Col. Gibbs. Later, in 1825, it
was purchased by Yale and served as the nucleus about which the present
Museum collection of the University has been formed. There is no doubt
but that the presence at this early date of this large and unusual mineral
collection had a great influence upon the development of mineralogical
science at Yale, and in the country at large.
In the year 1810 Dr. Archibald Bruce started the “American
Mineralogical Journal,” the title page of which reads in part as follows:
“The American Mineralogical Journal, being a Collection of Facts and
Observations tending to elucidate the Mineralogy and Geology of the
United States of America, together with other Information relating to
Mineralogy, Geology and Chemistry, derived from Scientific Sources.”
Unfortunately the health of Dr. Bruce failed, and the journal lasted only
through its first volume. It had, however, “been most favorably received,”
as Silliman remarks, and it was felt that another journal of a similar type
should be instituted. Such a suggestion was made by Col. Gibbs to
Professor Silliman in 1817 and this led directly to the founding of the
American Journal of Science in 1818 under the latter’s editorship. Although
Page 300
the field of the Journal at the very beginning was made broad and inclusive
it has always published many articles on mineralogical subjects. Three of its
editors-in-chief have been eminent mineralogists, and without question it
has been the most important single force in the development of this science
in the country. More than 800 well-established mineral species have been
described since the year 1800, of which approximately 150 have been from
American sources. More than two-thirds of the articles describing these new
American minerals have first appeared in the pages of the Journal. While
the description of new species is not always the most important part of
mineralogical investigation, still these figures serve to show the large part
that the Journal has played in the growth of American mineralogy.
It is convenient to review the progress in Mineralogy according to the
divisions formed by the different series, consisting of fifty volumes each, in
which the Journal has been published. These divisions curiously enough
will be found to correspond closely to four quite definite phases through
which mineralogical investigation in America has passed. The first series
covered the years from 1817 to 1845. In looking through these volumes one
finds a large number of mineralogical articles, the work of many
contributors. The great majority of these papers are purely descriptive in
character, frequently giving only general accounts of the mineral
occurrences of particular regions. However, a number of articles dealing
with more detailed physical and chemical descriptions of rare or new
species also belong in this period. Among the mineralogists engaged at this
time in the description of individual species, none was more indefatigable
than Charles U. Shepard. He was graduated from Amherst College in 1824,
at the age of twenty. In 1827 he became assistant to Professor Silliman in
New Haven, continuing in this position for four years. Later he was a
lecturer in natural history at Yale, and was at various times connected with
Amherst College and the South Carolina Medical College at Charleston.
His articles on mineralogy were very numerous. He assigned a large
number of new names to minerals, although with the exception of some half
dozen cases, these have later been shown to be varieties of minerals already
known and described, rather than new species. In spite, however, of his
frequent hasty and inaccurate decision as to the character of a mineral, his
influence on the progress of mineralogy was marked. His great enthusiasm
and ceaseless industry throughout a long life could not help but make a
definite contribution to the science. His “Treatise on Mineralogy” will be
it has always published many articles on mineralogical subjects. Three of its
editors-in-chief have been eminent mineralogists, and without question it
has been the most important single force in the development of this science
in the country. More than 800 well-established mineral species have been
described since the year 1800, of which approximately 150 have been from
American sources. More than two-thirds of the articles describing these new
American minerals have first appeared in the pages of the Journal. While
the description of new species is not always the most important part of
mineralogical investigation, still these figures serve to show the large part
that the Journal has played in the growth of American mineralogy.
It is convenient to review the progress in Mineralogy according to the
divisions formed by the different series, consisting of fifty volumes each, in
which the Journal has been published. These divisions curiously enough
will be found to correspond closely to four quite definite phases through
which mineralogical investigation in America has passed. The first series
covered the years from 1817 to 1845. In looking through these volumes one
finds a large number of mineralogical articles, the work of many
contributors. The great majority of these papers are purely descriptive in
character, frequently giving only general accounts of the mineral
occurrences of particular regions. However, a number of articles dealing
with more detailed physical and chemical descriptions of rare or new
species also belong in this period. Among the mineralogists engaged at this
time in the description of individual species, none was more indefatigable
than Charles U. Shepard. He was graduated from Amherst College in 1824,
at the age of twenty. In 1827 he became assistant to Professor Silliman in
New Haven, continuing in this position for four years. Later he was a
lecturer in natural history at Yale, and was at various times connected with
Amherst College and the South Carolina Medical College at Charleston.
His articles on mineralogy were very numerous. He assigned a large
number of new names to minerals, although with the exception of some half
dozen cases, these have later been shown to be varieties of minerals already
known and described, rather than new species. In spite, however, of his
frequent hasty and inaccurate decision as to the character of a mineral, his
influence on the progress of mineralogy was marked. His great enthusiasm
and ceaseless industry throughout a long life could not help but make a
definite contribution to the science. His “Treatise on Mineralogy” will be
Page 301
spoken of in a later paragraph. He died in May, 1886, having published his
last paper in the Journal in the previous September.
The first book on mineralogy published in America was that by Parker
Cleaveland, professor of mathematics, natural philosophy, chemistry and
mineralogy in Bowdoin College. The first edition was printed in 1816 and
an exhaustive notice is given in the first volume of the Journal (1, 35, 308,
1818); a second edition followed in 1822. In his preface Cleaveland gives
an interesting discussion concerning the two opposing European methods of
classifying minerals. The German school, led by Werner, classified minerals
according to their external characters while the French school, following
Haüy, put the emphasis on the “true composition.” Cleaveland remarks that
“the German school seems to be most distinguished by a technical and
minutely descriptive language; and the French, by the use of accurate and
scientific principles in the classification or arrangement of minerals.” He,
himself, tried to combine in a measure the two methods, basing the
fundamental divisions upon the chemical composition and using the
accurate description of the physical properties to distinguish similar species
and varieties from each other.
Cleaveland’s mineralogy was followed nearly twenty years later by the
Treatise on Mineralogy by Charles U. Shepard already mentioned. The first
part of this book was published in 1832. This contained chiefly an account
of the natural history classification of minerals according to the general plan
adopted by Mohs, the Austrian mineralogist. The second part of the book,
which appeared in 1835, gave the description of individual species, the
arrangement here being an alphabetical one throughout. Subsequent
editions appeared in 1844, 1852 and 1857.
James Dwight Dana was graduated from Yale College in 1833 at the age
of twenty. Four years later (1837) he published “The System of
Mineralogy,” a volume of 580 pages. The appearance of this book was an
event of surpassing importance in the development of the science. The
book, of course, depended largely upon the previous works of Haüy, Mohs,
Naumann and other European mineralogists, but was in no sense merely a
compilation from them. Dana, particularly in his discussion of mathematical
crystallography, showed much original thought. He also proved his
originality by proposing and using an elaborate system of classification
patterned after those already in use in the sciences of botany and zoology.
last paper in the Journal in the previous September.
The first book on mineralogy published in America was that by Parker
Cleaveland, professor of mathematics, natural philosophy, chemistry and
mineralogy in Bowdoin College. The first edition was printed in 1816 and
an exhaustive notice is given in the first volume of the Journal (1, 35, 308,
1818); a second edition followed in 1822. In his preface Cleaveland gives
an interesting discussion concerning the two opposing European methods of
classifying minerals. The German school, led by Werner, classified minerals
according to their external characters while the French school, following
Haüy, put the emphasis on the “true composition.” Cleaveland remarks that
“the German school seems to be most distinguished by a technical and
minutely descriptive language; and the French, by the use of accurate and
scientific principles in the classification or arrangement of minerals.” He,
himself, tried to combine in a measure the two methods, basing the
fundamental divisions upon the chemical composition and using the
accurate description of the physical properties to distinguish similar species
and varieties from each other.
Cleaveland’s mineralogy was followed nearly twenty years later by the
Treatise on Mineralogy by Charles U. Shepard already mentioned. The first
part of this book was published in 1832. This contained chiefly an account
of the natural history classification of minerals according to the general plan
adopted by Mohs, the Austrian mineralogist. The second part of the book,
which appeared in 1835, gave the description of individual species, the
arrangement here being an alphabetical one throughout. Subsequent
editions appeared in 1844, 1852 and 1857.
James Dwight Dana was graduated from Yale College in 1833 at the age
of twenty. Four years later (1837) he published “The System of
Mineralogy,” a volume of 580 pages. The appearance of this book was an
event of surpassing importance in the development of the science. The
book, of course, depended largely upon the previous works of Haüy, Mohs,
Naumann and other European mineralogists, but was in no sense merely a
compilation from them. Dana, particularly in his discussion of mathematical
crystallography, showed much original thought. He also proved his
originality by proposing and using an elaborate system of classification
patterned after those already in use in the sciences of botany and zoology.
Page 302
He later became convinced of the undesirability of this method of
classification and abandoned it entirely in the fourth edition of the System,
published in 1854, substituting for it the chemical classification which, in
its essential features, is in general use to-day. The System of Mineralogy
started in this way in 1837, has continued by means of successive editions
to be the standard reference book in the subject. The various editions
appeared as follows: I, 1837; II, 1844; III, 1850; IV, 1854; V, 1868; VI,
1892 (by Edward S. Dana).
J. D. Dana also contributed numerous mineralogical articles to the first
series of volumes of the Journal. It is interesting to note that they are chiefly
concerned with the more theoretical aspects of the subject, in fact they
constitute practically the only articles of such a character that appeared
during this period. Among the subjects treated were crystallographic
symbols, formation of twin crystals; pseudomorphism, origin of minerals in
metamorphosed limestones, origin of serpentine, classification of minerals,
etc.
The volumes of the Second Series of the Journal covered the years from
1846 through 1870. This period was characterized by great activity in the
study of the chemical composition of minerals. A number of skilled
chemists, notably J. Lawrence Smith, George J. Brush and Frederick A.
Genth, began about 1850 a long series of chemical investigations of
American minerals. Very few articles during this time paid much attention
to the physical properties of the minerals under discussion, practically no
description of optical characters was attempted, and only occasionally were
the crystals of a mineral mentioned. J. D. Dana was almost the only writer
who constantly endeavored to discover the fundamental characters and
relationships in minerals. He published many articles in these years which
were concerned chiefly with the classification and grouping of minerals,
with similarities in the crystal forms of different species, with relations
between chemical composition and crystal form, chemical formulas,
mineral nomenclature, etc. The following titles give an idea of the character
of the more important series of articles by him which belong to this
category: On the isomorphism and atomic volume of some minerals (9, 220,
1850); various notes and articles on homœomorphism of minerals (17, 85,
86, 210, 430; 18, 35, 131, 1854); on a connection between crystalline form
and chemical constitution, with some inferences therefrom (44, 89, 252,
398, 1867).
classification and abandoned it entirely in the fourth edition of the System,
published in 1854, substituting for it the chemical classification which, in
its essential features, is in general use to-day. The System of Mineralogy
started in this way in 1837, has continued by means of successive editions
to be the standard reference book in the subject. The various editions
appeared as follows: I, 1837; II, 1844; III, 1850; IV, 1854; V, 1868; VI,
1892 (by Edward S. Dana).
J. D. Dana also contributed numerous mineralogical articles to the first
series of volumes of the Journal. It is interesting to note that they are chiefly
concerned with the more theoretical aspects of the subject, in fact they
constitute practically the only articles of such a character that appeared
during this period. Among the subjects treated were crystallographic
symbols, formation of twin crystals; pseudomorphism, origin of minerals in
metamorphosed limestones, origin of serpentine, classification of minerals,
etc.
The volumes of the Second Series of the Journal covered the years from
1846 through 1870. This period was characterized by great activity in the
study of the chemical composition of minerals. A number of skilled
chemists, notably J. Lawrence Smith, George J. Brush and Frederick A.
Genth, began about 1850 a long series of chemical investigations of
American minerals. Very few articles during this time paid much attention
to the physical properties of the minerals under discussion, practically no
description of optical characters was attempted, and only occasionally were
the crystals of a mineral mentioned. J. D. Dana was almost the only writer
who constantly endeavored to discover the fundamental characters and
relationships in minerals. He published many articles in these years which
were concerned chiefly with the classification and grouping of minerals,
with similarities in the crystal forms of different species, with relations
between chemical composition and crystal form, chemical formulas,
mineral nomenclature, etc. The following titles give an idea of the character
of the more important series of articles by him which belong to this
category: On the isomorphism and atomic volume of some minerals (9, 220,
1850); various notes and articles on homœomorphism of minerals (17, 85,
86, 210, 430; 18, 35, 131, 1854); on a connection between crystalline form
and chemical constitution, with some inferences therefrom (44, 89, 252,
398, 1867).
Page 303
A great many new mineral names were proposed between 1850 and
1870, a large number of which have continued to be well-recognized
species. But there was also a tendency, which has not wholly disappeared
even now, to base a mineral determination upon insufficient evidence, and
to propose a new species with but little justification for it. In this connection
a quotation from the introduction by J. D. Dana to the 3rd Supplement to
the System of Mineralogy (4th edition) published in the Journal (22, page
246, 1856), will be of interest. He says:
“It is a matter of regret, that mineral species are so often brought out, especially in this country,
without sufficient investigation and full description. It is not meeting the just demands of the science
of mineralogy to say that a mineral has probably certain constituents, or to state the composition in a
general way without a complete and detailed analysis, especially when there are no crystallographic
characters to afford the species a good foundation. We have a right to demand that those who name
species, should use all the means the science of the age admits of, to prove that the species is one that
nature will own, for only such belong to science, and if enough of the material has not been found for
a good description there is not enough to authorize the introduction of a new name in the science.
The publication of factitious species, in whatever department of science, is progress not towards
truth, but into regions of error; and often much and long labor is required before the science recovers
from these backward steps.”
J. Lawrence Smith was born in 1818 and died in 1883. He was a graduate
of the University of Virginia and of the Medical College of Charleston and
later spent three years studying in Paris. Shortly after the completion of his
studies he went to Turkey as an advisor to the government of that country in
connection with the growing of cotton there. During this time he
investigated the emery mines of Asia Minor, and wrote a memoir upon
them which was later published by the French Academy. He served as
professor of chemistry in the University of Virginia and later held the same
chair in the University of Illinois. He published a long series of papers on
the chemical composition of minerals and meteorites, as well as on pure
chemical subjects. Among the more notable of his contributions are the
“Memoir on Emery” (1850), a series of papers on the “Reëxamination of
American Minerals” (1853) written with the collaboration of George J.
Brush, and his “Memoir on Meteorites” (1855).
1870, a large number of which have continued to be well-recognized
species. But there was also a tendency, which has not wholly disappeared
even now, to base a mineral determination upon insufficient evidence, and
to propose a new species with but little justification for it. In this connection
a quotation from the introduction by J. D. Dana to the 3rd Supplement to
the System of Mineralogy (4th edition) published in the Journal (22, page
246, 1856), will be of interest. He says:
“It is a matter of regret, that mineral species are so often brought out, especially in this country,
without sufficient investigation and full description. It is not meeting the just demands of the science
of mineralogy to say that a mineral has probably certain constituents, or to state the composition in a
general way without a complete and detailed analysis, especially when there are no crystallographic
characters to afford the species a good foundation. We have a right to demand that those who name
species, should use all the means the science of the age admits of, to prove that the species is one that
nature will own, for only such belong to science, and if enough of the material has not been found for
a good description there is not enough to authorize the introduction of a new name in the science.
The publication of factitious species, in whatever department of science, is progress not towards
truth, but into regions of error; and often much and long labor is required before the science recovers
from these backward steps.”
J. Lawrence Smith was born in 1818 and died in 1883. He was a graduate
of the University of Virginia and of the Medical College of Charleston and
later spent three years studying in Paris. Shortly after the completion of his
studies he went to Turkey as an advisor to the government of that country in
connection with the growing of cotton there. During this time he
investigated the emery mines of Asia Minor, and wrote a memoir upon
them which was later published by the French Academy. He served as
professor of chemistry in the University of Virginia and later held the same
chair in the University of Illinois. He published a long series of papers on
the chemical composition of minerals and meteorites, as well as on pure
chemical subjects. Among the more notable of his contributions are the
“Memoir on Emery” (1850), a series of papers on the “Reëxamination of
American Minerals” (1853) written with the collaboration of George J.
Brush, and his “Memoir on Meteorites” (1855).
Page 304
George J. Brush entered on his scientific career at the moment when
science and scientific methods of research were just beginning to be
appreciated in this country, and he soon became one of the leading pioneers
in the movement. While his half century of active service was largely
occupied by administrative duties in connection with the Sheffield
Scientific School, his interest in mineralogy never flagged. His papers on
mineralogical subjects number about thirty, all of which were published in
the Journal. These began in 1849, even before his graduation from college,
and continued until his last paper (in collaboration with S. L. Penfield)
appeared in 1883. Three of the early papers were written with J. Lawrence
Smith as noted above. These papers first set in this country the standard for
thorough and accurate scientific mineral investigation. Later in life he was
science and scientific methods of research were just beginning to be
appreciated in this country, and he soon became one of the leading pioneers
in the movement. While his half century of active service was largely
occupied by administrative duties in connection with the Sheffield
Scientific School, his interest in mineralogy never flagged. His papers on
mineralogical subjects number about thirty, all of which were published in
the Journal. These began in 1849, even before his graduation from college,
and continued until his last paper (in collaboration with S. L. Penfield)
appeared in 1883. Three of the early papers were written with J. Lawrence
Smith as noted above. These papers first set in this country the standard for
thorough and accurate scientific mineral investigation. Later in life he was
Page 305
active in the development of the remarkable mineral locality at Branchville,
Conn., and, with the collaboration of E. S. Dana, published in the Journal
(1878–90) five important articles on its minerals. This locality, with the
exception of the zinc deposits at Franklin Furnace, N. J., was the most
remarkable yet discovered in this country. Nearly forty different mineral
species were found there, of which nine (mostly phosphates) were new to
science. There has certainly been no other series of descriptive papers on a
mineralogical locality of equal importance published in this country.
In addition to publishing original papers, Brush did considerable editorial
work in connection with the fourth (1854) and fifth (1868) editions of the
System of Mineralogy and the Appendices to them. His Manual of
Determinative Mineralogy, with a series of determinative tables adapted
from similar ones by von Kobell, was first published in 1874. It was revised
in 1878 and later rewritten by S. L. Penfield. This book did much to make
possible the rapid and accurate determination of mineral species.
Throughout his life, Brush was an enthusiastic collector of minerals,
building up the notable collection that now bears his name. Perhaps,
however, his most important contribution to the development of mineralogy
in America lay rather in his influence upon his many students. With his
enthusiasm for accurate and painstaking investigation he was an inspiration
to all who came in contact with him and his own field and science in
general owes much to that influence.
Among the early mineralogists in this country, who were concerned in
the chemical analyses of minerals, none accomplished more or better work
than Frederick A. Genth. He was born in Germany in 1820 and lived in that
country until 1848, when he came to the United States and settled in
Philadelphia. He had studied in various German universities and worked
under some of the most famous chemists of that time. His papers in
mineralogy number more than seventy-five, in the great majority of which
chemical analyses are given. He published fifty-four successive articles, the
greater part of which appeared in the Journal, which were entitled
Contributions to Mineralogy. In these he gave descriptions of more than
two hundred different minerals, most of which were accompanied by
analyses. He described more than a dozen new and well-established mineral
species. He was especially interested in the rarer elements and many of his
analyses were of minerals containing them. Especially interesting was his
work with the tellurides, the species coloradoite, melonite and calaverite
Conn., and, with the collaboration of E. S. Dana, published in the Journal
(1878–90) five important articles on its minerals. This locality, with the
exception of the zinc deposits at Franklin Furnace, N. J., was the most
remarkable yet discovered in this country. Nearly forty different mineral
species were found there, of which nine (mostly phosphates) were new to
science. There has certainly been no other series of descriptive papers on a
mineralogical locality of equal importance published in this country.
In addition to publishing original papers, Brush did considerable editorial
work in connection with the fourth (1854) and fifth (1868) editions of the
System of Mineralogy and the Appendices to them. His Manual of
Determinative Mineralogy, with a series of determinative tables adapted
from similar ones by von Kobell, was first published in 1874. It was revised
in 1878 and later rewritten by S. L. Penfield. This book did much to make
possible the rapid and accurate determination of mineral species.
Throughout his life, Brush was an enthusiastic collector of minerals,
building up the notable collection that now bears his name. Perhaps,
however, his most important contribution to the development of mineralogy
in America lay rather in his influence upon his many students. With his
enthusiasm for accurate and painstaking investigation he was an inspiration
to all who came in contact with him and his own field and science in
general owes much to that influence.
Among the early mineralogists in this country, who were concerned in
the chemical analyses of minerals, none accomplished more or better work
than Frederick A. Genth. He was born in Germany in 1820 and lived in that
country until 1848, when he came to the United States and settled in
Philadelphia. He had studied in various German universities and worked
under some of the most famous chemists of that time. His papers in
mineralogy number more than seventy-five, in the great majority of which
chemical analyses are given. He published fifty-four successive articles, the
greater part of which appeared in the Journal, which were entitled
Contributions to Mineralogy. In these he gave descriptions of more than
two hundred different minerals, most of which were accompanied by
analyses. He described more than a dozen new and well-established mineral
species. He was especially interested in the rarer elements and many of his
analyses were of minerals containing them. Especially interesting was his
work with the tellurides, the species coloradoite, melonite and calaverite
Page 306
being first described by him. A long and important investigation was
recorded on Corundum, “Its Alterations and Associate Minerals,” published
in the Proceedings of the American Philosophical Society in 1873 (13, 361).
Dr. Genth died in 1893.
The period from 1860 until 1875 was not very productive in
mineralogical investigations. The first ten volumes of the Third Series of
the Journal, covering the years 1871–1876, contained mineralogical articles
by only some fifteen different authors. But from that time on, the amount of
work done and the number of investigators grew rapidly. With this increase
in activity came also a decided change in the character of the work. The
period between 1871 and 1895 can be characterized as one in which all the
various aspects of mineral investigation received more nearly equal
prominence. While the chemical composition of minerals still held rightly
its prominent place, the investigation of the crystallographic and optical
characters and the relationships existing between all three were of much
more frequent occurrence. Edward S. Dana commenced his scientific work
by publishing in 1872 an article on the crystals of datolite which was
probably the first American article concerned wholly with the description of
the crystallography of a mineral. Samuel L. Penfield began his important
investigations in 1877 and the first articles by Frank W. Clarke appeared
during this period. The first edition of the Text Book of Mineralogy by
Edward S. Dana with its important chapters on Crystallography and Optical
Mineralogy was published in 1877 and his revision of the System of
Mineralogy (sixth edition) appeared in 1892.
Unquestionably the foremost figure in American mineralogy during this
period was that of Samuel L. Penfield. He embodied in an unusual degree
the characters making for success in this science, for few investigators in
mineralogy have shown, as he did, equal facility in all branches of
descriptive mineralogy. He was a skilled chemist and possessed in a high
degree that ingenuity in manipulation so necessary to a great analyst. He
was also an accurate and resourceful crystallographer and optical
mineralogist. His contributions to the science of mineralogy can be partially
judged by the following brief summary of his work. He published over
eighty mineralogical papers, practically all of which were printed in the
Journal. These included the descriptions of fourteen new mineral species,
the establishment of the chemical composition of more than twenty others,
and the crystallization of about a dozen more. By a series of brilliant
recorded on Corundum, “Its Alterations and Associate Minerals,” published
in the Proceedings of the American Philosophical Society in 1873 (13, 361).
Dr. Genth died in 1893.
The period from 1860 until 1875 was not very productive in
mineralogical investigations. The first ten volumes of the Third Series of
the Journal, covering the years 1871–1876, contained mineralogical articles
by only some fifteen different authors. But from that time on, the amount of
work done and the number of investigators grew rapidly. With this increase
in activity came also a decided change in the character of the work. The
period between 1871 and 1895 can be characterized as one in which all the
various aspects of mineral investigation received more nearly equal
prominence. While the chemical composition of minerals still held rightly
its prominent place, the investigation of the crystallographic and optical
characters and the relationships existing between all three were of much
more frequent occurrence. Edward S. Dana commenced his scientific work
by publishing in 1872 an article on the crystals of datolite which was
probably the first American article concerned wholly with the description of
the crystallography of a mineral. Samuel L. Penfield began his important
investigations in 1877 and the first articles by Frank W. Clarke appeared
during this period. The first edition of the Text Book of Mineralogy by
Edward S. Dana with its important chapters on Crystallography and Optical
Mineralogy was published in 1877 and his revision of the System of
Mineralogy (sixth edition) appeared in 1892.
Unquestionably the foremost figure in American mineralogy during this
period was that of Samuel L. Penfield. He embodied in an unusual degree
the characters making for success in this science, for few investigators in
mineralogy have shown, as he did, equal facility in all branches of
descriptive mineralogy. He was a skilled chemist and possessed in a high
degree that ingenuity in manipulation so necessary to a great analyst. He
was also an accurate and resourceful crystallographer and optical
mineralogist. His contributions to the science of mineralogy can be partially
judged by the following brief summary of his work. He published over
eighty mineralogical papers, practically all of which were printed in the
Journal. These included the descriptions of fourteen new mineral species,
the establishment of the chemical composition of more than twenty others,
and the crystallization of about a dozen more. By a series of brilliant
Page 307
investigations he established the isomorphism between fluorine and the
hydroxyl radical. He first enunciated the theory that the crystalline form of
a mineral was due to the mass effect of the acid present rather than that of
the bases. He contributed also a number of articles on the stereographic
projection and its use in crystallographic investigations, devising a series of
protractors and scales to make possible the rapid and accurate use of this
projection in solving problems in crystallography.
Penfield was born in 1856, was graduated from the Sheffield Scientific
School in 1877 and immediately became an assistant in the chemical
laboratory of that institution. At this time he, together with his colleague
Horace L. Wells, made the analyses of the minerals from the newly
discovered Branchville locality. He spent the years 1880 and 1881 in
studying chemistry in Germany, returning to Yale as an instructor in
mineralogy in the fall of 1881. Except for another semester in Europe at
Heidelberg he continued as instructor and professor of mineralogy in the
Sheffield Scientific School until his early death in 1906.
It is difficult to choose for mention the names of other investigators in
Mineralogy during this period. Toward its end a great many writers
contributed to the pages of the Journal, more than fifty different names
being counted for the volumes 41 to 50 of the Third Series. Many of these
are still living and still active in scientific research. Mention should be
made of Frank W. Clarke, who contributed many important articles
concerning the chemical constitution of the silicates. His work on the mica
and zeolite groups is especially noteworthy. The work of W. H. Hillebrand,
particularly in regard to his analytical investigations of the minerals
containing the rarer elements, was of great importance. The name of W. E.
Hidden should be remembered, because, with his keen and discriminating
eye and active search for new mineral localities, he was able to make many
additions to the science.
In glancing over the indices to the Journal the close interrelation of
mineralogy to the other sciences is strikingly shown by the fact that so
many scientists whose particular fields are along other lines have published
occasional mineralogical papers. Frequently a young man has commenced
with mineralogical investigations and then later been drawn definitely into
one of these allied subjects. Men, who have won their reputation in
chemistry, physics, and all the various divisions of geology, even that of
hydroxyl radical. He first enunciated the theory that the crystalline form of
a mineral was due to the mass effect of the acid present rather than that of
the bases. He contributed also a number of articles on the stereographic
projection and its use in crystallographic investigations, devising a series of
protractors and scales to make possible the rapid and accurate use of this
projection in solving problems in crystallography.
Penfield was born in 1856, was graduated from the Sheffield Scientific
School in 1877 and immediately became an assistant in the chemical
laboratory of that institution. At this time he, together with his colleague
Horace L. Wells, made the analyses of the minerals from the newly
discovered Branchville locality. He spent the years 1880 and 1881 in
studying chemistry in Germany, returning to Yale as an instructor in
mineralogy in the fall of 1881. Except for another semester in Europe at
Heidelberg he continued as instructor and professor of mineralogy in the
Sheffield Scientific School until his early death in 1906.
It is difficult to choose for mention the names of other investigators in
Mineralogy during this period. Toward its end a great many writers
contributed to the pages of the Journal, more than fifty different names
being counted for the volumes 41 to 50 of the Third Series. Many of these
are still living and still active in scientific research. Mention should be
made of Frank W. Clarke, who contributed many important articles
concerning the chemical constitution of the silicates. His work on the mica
and zeolite groups is especially noteworthy. The work of W. H. Hillebrand,
particularly in regard to his analytical investigations of the minerals
containing the rarer elements, was of great importance. The name of W. E.
Hidden should be remembered, because, with his keen and discriminating
eye and active search for new mineral localities, he was able to make many
additions to the science.
In glancing over the indices to the Journal the close interrelation of
mineralogy to the other sciences is strikingly shown by the fact that so
many scientists whose particular fields are along other lines have published
occasional mineralogical papers. Frequently a young man has commenced
with mineralogical investigations and then later been drawn definitely into
one of these allied subjects. Men, who have won their reputation in
chemistry, physics, and all the various divisions of geology, even that of
Page 308
palaeontology, have all contributed articles distinctly mineralogical in
character. For this reason the number of American writers who have
published what may be called casual papers on mineralogy is very great in
comparison to the number of those who continue such publications over a
series of years.
That the subject of meteorites is one which has been constantly studied
by American mineralogists and petrographers is shown by the long list of
papers concerning it that have been published in the Journal; it should,
therefore, be considered briefly here. Many of these papers are short and of
a general descriptive nature but others which give more fully the chemical,
mineralogical and physical details are numerous. Among the earlier writers
on this subject Benjamin Silliman, Jr., and C. U. Shepard should be
mentioned. The latter was the first to recognize a new mineral in the
Bishopville meteorite which he called chladnite. The same substance was
afterwards found in a terrestial occurrence and was more accurately
described by Kenngott under the name of enstatite. J. Lawrence Smith later
showed that these two substances were identical. Smith did a large amount
of important chemical work on meteorites. He was the first to note the
presence of ferrous chloride in meteoric iron, the mineral being afterwards
named lawrencite in his honor. The iron-chronium sulphide, daubreelite,
was also first described by him. Other names that should be mentioned in
this connection are those of A. W. Wright who studied the gaseous
constituents of meteorites, G. F. Kunz, W. E. Hidden, A. E. Foote and H. A.
Ward, all of whom published numerous descriptions of these bodies.
Among the more recent workers in this field the names of G. P. Merrill and
O. C. Farrington deserve especial mention.
The publication of the Fourth Series of the Journal began in 1896.
Although the years since then have seen a great amount of very important
work accomplished, the history of the period is fresh in the minds of all and
as the majority of the active workers are still living and productive it seems
hardly necessary to go into great detail concerning it. Twenty years ago it
seemed to some mineralogists that the science could almost be considered
complete. All the commoner minerals had certainly been discovered and
exhaustively studied. Little apparently was left that could be added to our
knowledge of them. New occurrences would still be recorded, new crystal
habits would be observed, and an occasional new and small crystal face
might be listed, but few facts of great importance seemed undiscovered.
character. For this reason the number of American writers who have
published what may be called casual papers on mineralogy is very great in
comparison to the number of those who continue such publications over a
series of years.
That the subject of meteorites is one which has been constantly studied
by American mineralogists and petrographers is shown by the long list of
papers concerning it that have been published in the Journal; it should,
therefore, be considered briefly here. Many of these papers are short and of
a general descriptive nature but others which give more fully the chemical,
mineralogical and physical details are numerous. Among the earlier writers
on this subject Benjamin Silliman, Jr., and C. U. Shepard should be
mentioned. The latter was the first to recognize a new mineral in the
Bishopville meteorite which he called chladnite. The same substance was
afterwards found in a terrestial occurrence and was more accurately
described by Kenngott under the name of enstatite. J. Lawrence Smith later
showed that these two substances were identical. Smith did a large amount
of important chemical work on meteorites. He was the first to note the
presence of ferrous chloride in meteoric iron, the mineral being afterwards
named lawrencite in his honor. The iron-chronium sulphide, daubreelite,
was also first described by him. Other names that should be mentioned in
this connection are those of A. W. Wright who studied the gaseous
constituents of meteorites, G. F. Kunz, W. E. Hidden, A. E. Foote and H. A.
Ward, all of whom published numerous descriptions of these bodies.
Among the more recent workers in this field the names of G. P. Merrill and
O. C. Farrington deserve especial mention.
The publication of the Fourth Series of the Journal began in 1896.
Although the years since then have seen a great amount of very important
work accomplished, the history of the period is fresh in the minds of all and
as the majority of the active workers are still living and productive it seems
hardly necessary to go into great detail concerning it. Twenty years ago it
seemed to some mineralogists that the science could almost be considered
complete. All the commoner minerals had certainly been discovered and
exhaustively studied. Little apparently was left that could be added to our
knowledge of them. New occurrences would still be recorded, new crystal
habits would be observed, and an occasional new and small crystal face
might be listed, but few facts of great importance seemed undiscovered.
Page 309
This view was not wholly justified because new facts of interest and
importance have continuously been brought forward, and the finding of new
minerals does not appear to diminish in amount with the years. The work of
the investigators on the United States Geological Survey along these lines is
especially noteworthy.
This last of our periods, however, is chiefly signalized by a practically
new development along the lines that might be characterized as
experimental mineralogy. New ways have been discovered in which to
study minerals. The important but hitherto baffling problems of their
genesis, together with their relations to their surroundings, and to associated
minerals, have been attacked by novel methods.
In this pioneer work that of the Geophysical Laboratory of the Carnegie
Institution of Washington has been of the greatest importance. This
laboratory was established in 1905 and, under the directorship of Arthur L.
Day, a notable corps of investigators has been assembled and remarkable
work already accomplished. While the field of investigation of the
laboratory is broader than that of mineralogy, including much that belongs
to petrography, vulcanology, etc., still the greater part of the work done can
be properly classed as mineralogical in character and should be considered
here. Because of its great value, however, it was felt that an authoritative,
although necessarily, under existing conditions, a brief, account of it should
be given. A concise summary of the objects, methods and results of the
investigations of the laboratory has been kindly prepared by a member of its
staff, Dr. R. B. Sosman, and is given later.
During the last few years another line of investigation has been opened
by the discovery of the effect of crystalline structure upon X-rays. Through
the refraction or reflection of the X-ray by means of the ordered
arrangement of the particles forming the crystalline network, we are
apparently going to be able to discover much concerning the internal
structure of crystals. And, partly through these discoveries, is likely to come
in turn the solution of the hitherto insolvable mystery of the constitution of
matter. Without doubt the multitudinous facts of mineralogy assembled
during the past century by the painstaking investigation of a large number
of scientists are destined to play a large part in the solution of this problem.
Further, it does not seem too bold a prophecy to suggest, that the time will
come when it will be possible to assemble all these unorganized facts that
importance have continuously been brought forward, and the finding of new
minerals does not appear to diminish in amount with the years. The work of
the investigators on the United States Geological Survey along these lines is
especially noteworthy.
This last of our periods, however, is chiefly signalized by a practically
new development along the lines that might be characterized as
experimental mineralogy. New ways have been discovered in which to
study minerals. The important but hitherto baffling problems of their
genesis, together with their relations to their surroundings, and to associated
minerals, have been attacked by novel methods.
In this pioneer work that of the Geophysical Laboratory of the Carnegie
Institution of Washington has been of the greatest importance. This
laboratory was established in 1905 and, under the directorship of Arthur L.
Day, a notable corps of investigators has been assembled and remarkable
work already accomplished. While the field of investigation of the
laboratory is broader than that of mineralogy, including much that belongs
to petrography, vulcanology, etc., still the greater part of the work done can
be properly classed as mineralogical in character and should be considered
here. Because of its great value, however, it was felt that an authoritative,
although necessarily, under existing conditions, a brief, account of it should
be given. A concise summary of the objects, methods and results of the
investigations of the laboratory has been kindly prepared by a member of its
staff, Dr. R. B. Sosman, and is given later.
During the last few years another line of investigation has been opened
by the discovery of the effect of crystalline structure upon X-rays. Through
the refraction or reflection of the X-ray by means of the ordered
arrangement of the particles forming the crystalline network, we are
apparently going to be able to discover much concerning the internal
structure of crystals. And, partly through these discoveries, is likely to come
in turn the solution of the hitherto insolvable mystery of the constitution of
matter. Without doubt the multitudinous facts of mineralogy assembled
during the past century by the painstaking investigation of a large number
of scientists are destined to play a large part in the solution of this problem.
Further, it does not seem too bold a prophecy to suggest, that the time will
come when it will be possible to assemble all these unorganized facts that
Page 310
we know about minerals into a harmonious whole and that we shall be then
able to formulate the underlying and fundamental principles upon which
they all depend. These are the great problems for the future of mineralogical
investigation.
able to formulate the underlying and fundamental principles upon which
they all depend. These are the great problems for the future of mineralogical
investigation.
Page 311
IX
THE WORK OF THE GEOPHYSICAL LABORATORY OF
THE CARNEGIE INSTITUTION OF WASHINGTON
By R. B. SOSMAN
There are three methods of approach to the great problem of rock
formation. The first undertakes to reproduce by suitable laboratory
experiments some of the observed changes in natural rocks. The second
seeks to apply the principles of physical chemistry to a great body of
carefully gathered statistics. The third method of attack is like the first in
being a laboratory method, and like the second in seeking to apply existing
knowledge to the association of minerals as found in rocks, but in its
procedure differs widely from both. It consists of bringing together pure
materials under measurable conditions, and thus in establishing by strictly
quantitative methods the relations in which minerals can exist together
under the conditions of temperature and pressure that have the power to
affect such relations.
It is to this third method of investigation of the problems of the rocks that
the Geophysical Laboratory has been devoted since its establishment in
1905. It has proved entirely practicable to make quantitative studies of the
relations among the principal earth-forming oxides (silica, alumina,
magnesia, lime, soda, potash, and the oxides of iron) over a very wide range
of temperatures. The resources of physics have proved adequate to establish
temperature with a high degree of precision and to measure the quantity of
energy involved in the various reactions. The chemist has been able to
obtain materials in a high degree of purity, and to follow out in detail the
chemical relationships that exist among the earth-forming oxides. The
THE WORK OF THE GEOPHYSICAL LABORATORY OF
THE CARNEGIE INSTITUTION OF WASHINGTON
By R. B. SOSMAN
There are three methods of approach to the great problem of rock
formation. The first undertakes to reproduce by suitable laboratory
experiments some of the observed changes in natural rocks. The second
seeks to apply the principles of physical chemistry to a great body of
carefully gathered statistics. The third method of attack is like the first in
being a laboratory method, and like the second in seeking to apply existing
knowledge to the association of minerals as found in rocks, but in its
procedure differs widely from both. It consists of bringing together pure
materials under measurable conditions, and thus in establishing by strictly
quantitative methods the relations in which minerals can exist together
under the conditions of temperature and pressure that have the power to
affect such relations.
It is to this third method of investigation of the problems of the rocks that
the Geophysical Laboratory has been devoted since its establishment in
1905. It has proved entirely practicable to make quantitative studies of the
relations among the principal earth-forming oxides (silica, alumina,
magnesia, lime, soda, potash, and the oxides of iron) over a very wide range
of temperatures. The resources of physics have proved adequate to establish
temperature with a high degree of precision and to measure the quantity of
energy involved in the various reactions. The chemist has been able to
obtain materials in a high degree of purity, and to follow out in detail the
chemical relationships that exist among the earth-forming oxides. The
Page 312
petrographic laboratory has been available for the comparison of synthetic
laboratory products with the corresponding natural minerals.
It has also proved entirely practicable to extend the same methods of
research to some of the principal ore minerals such as the sulphides of
copper. Other information which is certain to be of ultimate economic value
has also come out of the thorough study of the silicates, which are basic
materials for the vast variety of industries which are classed under the name
of ceramic industries. The best example of this is the facility with which the
experience and the personnel of the laboratory has been adapted to the very
important problem of manufacturing an adequate supply of optical glass for
the needs of the United States in the present war.
It has further been possible to show within the last two years that rock
formation in which volatile ingredients play a necessary and determining
part can be completely studied in the laboratory with as much precision as
though all the components were solids or liquids.
Along with the laboratory work on the formation of minerals and rocks
has gone an increasing amount of field work on the activities of accessible
volcanoes, such as Kilauea and Vesuvius, where the fusion and
recrystallization of rocks on a large scale can be observed and studied.
There was once a time when the confidence of the laboratory in the
capacity of physics and chemistry to solve geological problems was not
shared by all geologists. There were some who were inclined to view with
considerable apprehension the vast ramifications and complications of
natural rock formation as a problem impossible of adequate solution in the
laboratory. It is, therefore, a matter of satisfaction to all those who have
participated in these efforts to see the evidences of this apprehension
disappearing gradually as the work has progressed. A careful appraisement
of the situation to-day, after ten years of activity, reveals the fact that the
tangible grounds for anxiety about the accessibility of the problems which
were confronted at first are now for the most part dissipated.
It will not be possible to review in detail the lines of work sketched
above. An outline of the synthetic work on systems of the mineral oxides
and a paragraph on the volcano researches will perhaps suffice to indicate
the general plan and purpose of the laboratory’s work. It should be added
that the results of many of the researches of the laboratory, detailed below,
laboratory products with the corresponding natural minerals.
It has also proved entirely practicable to extend the same methods of
research to some of the principal ore minerals such as the sulphides of
copper. Other information which is certain to be of ultimate economic value
has also come out of the thorough study of the silicates, which are basic
materials for the vast variety of industries which are classed under the name
of ceramic industries. The best example of this is the facility with which the
experience and the personnel of the laboratory has been adapted to the very
important problem of manufacturing an adequate supply of optical glass for
the needs of the United States in the present war.
It has further been possible to show within the last two years that rock
formation in which volatile ingredients play a necessary and determining
part can be completely studied in the laboratory with as much precision as
though all the components were solids or liquids.
Along with the laboratory work on the formation of minerals and rocks
has gone an increasing amount of field work on the activities of accessible
volcanoes, such as Kilauea and Vesuvius, where the fusion and
recrystallization of rocks on a large scale can be observed and studied.
There was once a time when the confidence of the laboratory in the
capacity of physics and chemistry to solve geological problems was not
shared by all geologists. There were some who were inclined to view with
considerable apprehension the vast ramifications and complications of
natural rock formation as a problem impossible of adequate solution in the
laboratory. It is, therefore, a matter of satisfaction to all those who have
participated in these efforts to see the evidences of this apprehension
disappearing gradually as the work has progressed. A careful appraisement
of the situation to-day, after ten years of activity, reveals the fact that the
tangible grounds for anxiety about the accessibility of the problems which
were confronted at first are now for the most part dissipated.
It will not be possible to review in detail the lines of work sketched
above. An outline of the synthetic work on systems of the mineral oxides
and a paragraph on the volcano researches will perhaps suffice to indicate
the general plan and purpose of the laboratory’s work. It should be added
that the results of many of the researches of the laboratory, detailed below,
Page 313
have been published in the pages of the Journal (see 21, 89, 1906, and later
volumes).
Mineral Researches.—The mineral studies include:
I. One-component systems: silica, with its numerous polymorphic forms
and their relations to temperature and the conditions of rock formation;
alumina; magnesia; and lime.
II. Two-component systems: silica-alumina, including sillimanite and
related minerals; silica-magnesia, including the tetramorphic metasilicate
MgSiO3; silica-lime, including wollastonite; the alkali silicates, particularly
with reference to their equilibria with carbon dioxide and with water; ferric
oxide-lime; alumina-lime; alumina-magnesia, including spinel; and
hematite-magnetite, a solid-solution series of an unusual type.
III. Three-component systems: silica-alumina-magnesia, completed but
not yet published; silica-alumina-lime, complete, including the compounds
that enter into the composition of portland cement; silica-magnesia-lime,
completed but not yet published, including, however, published work on the
diopside-forsterite-silica system, and on the CaSiO3-MgSiO3 series; and
alumina-magnesia-lime.
IV. Four components: SiO2-Al2O3-MgO-CaO: the incomplete system
anorthite-forsterite-silica; SiO2-Al2O3-CaO-Na2O: the series of lime-soda
feldspars (albite-anorthite), and the series nephelite (carnegieite)-anorthite;
SiO2-Al2O3-Na2O-K2O: the sodium-potassium nephelites.
V. Five components: SiO2-Al2O3-MgO-CaO-Na2O: the ternary system
diopside-anorthite-albite (haplo-basaltic and haplo-dioritic magmas).
Fairly complete studies have also been made of the mineral sulphides of
iron, copper, zinc, cadmium, and mercury, and the conditions controlling
the secondary enrichment of copper sulphide ores are now being
investigated. In connection with the sulphide investigations, the hydrated
oxides of iron have been studied chemically and microscopically and the
results will soon be ready for publication.
Throughout the work the mere accumulation of bodies of facts has been
held to be secondary in importance to the development of new methods of
attack and the evaluation of new general principles, and the specific
problems studied have been selected from this point of view.
volumes).
Mineral Researches.—The mineral studies include:
I. One-component systems: silica, with its numerous polymorphic forms
and their relations to temperature and the conditions of rock formation;
alumina; magnesia; and lime.
II. Two-component systems: silica-alumina, including sillimanite and
related minerals; silica-magnesia, including the tetramorphic metasilicate
MgSiO3; silica-lime, including wollastonite; the alkali silicates, particularly
with reference to their equilibria with carbon dioxide and with water; ferric
oxide-lime; alumina-lime; alumina-magnesia, including spinel; and
hematite-magnetite, a solid-solution series of an unusual type.
III. Three-component systems: silica-alumina-magnesia, completed but
not yet published; silica-alumina-lime, complete, including the compounds
that enter into the composition of portland cement; silica-magnesia-lime,
completed but not yet published, including, however, published work on the
diopside-forsterite-silica system, and on the CaSiO3-MgSiO3 series; and
alumina-magnesia-lime.
IV. Four components: SiO2-Al2O3-MgO-CaO: the incomplete system
anorthite-forsterite-silica; SiO2-Al2O3-CaO-Na2O: the series of lime-soda
feldspars (albite-anorthite), and the series nephelite (carnegieite)-anorthite;
SiO2-Al2O3-Na2O-K2O: the sodium-potassium nephelites.
V. Five components: SiO2-Al2O3-MgO-CaO-Na2O: the ternary system
diopside-anorthite-albite (haplo-basaltic and haplo-dioritic magmas).
Fairly complete studies have also been made of the mineral sulphides of
iron, copper, zinc, cadmium, and mercury, and the conditions controlling
the secondary enrichment of copper sulphide ores are now being
investigated. In connection with the sulphide investigations, the hydrated
oxides of iron have been studied chemically and microscopically and the
results will soon be ready for publication.
Throughout the work the mere accumulation of bodies of facts has been
held to be secondary in importance to the development of new methods of
attack and the evaluation of new general principles, and the specific
problems studied have been selected from this point of view.
Page 314
Volcano Researches.—A branch of the laboratory’s work that is of
general as well as petrological interest is the study of active volcanoes.
Observations and collections have been made at Kilauea, Vesuvius, Etna,
Stromboli, Vulcano, and (through the courtesy of the directors of the
National Geographic Society) Katmai in Alaska. The great importance of
gases in volcanicity is emphasized by all the studies. The active gases
include hydrogen and water vapor, carbon monoxide and carbon dioxide,
and sulphur and its oxides, as well as a variety of other compounds of lesser
importance. The crater of Kilauea proves to be an active natural gas-
furnace, in which reactions are continuously occurring among the gases,
often resulting in making the lava basin hotter at the surface than it is at
some depth. These reactions are being studied in the laboratory on mixtures
of the pure constituent gases in known proportions, in order to lay the
foundation for accurate interpretation and prediction concerning the gases
as actually collected from the volcanoes themselves.
general as well as petrological interest is the study of active volcanoes.
Observations and collections have been made at Kilauea, Vesuvius, Etna,
Stromboli, Vulcano, and (through the courtesy of the directors of the
National Geographic Society) Katmai in Alaska. The great importance of
gases in volcanicity is emphasized by all the studies. The active gases
include hydrogen and water vapor, carbon monoxide and carbon dioxide,
and sulphur and its oxides, as well as a variety of other compounds of lesser
importance. The crater of Kilauea proves to be an active natural gas-
furnace, in which reactions are continuously occurring among the gases,
often resulting in making the lava basin hotter at the surface than it is at
some depth. These reactions are being studied in the laboratory on mixtures
of the pure constituent gases in known proportions, in order to lay the
foundation for accurate interpretation and prediction concerning the gases
as actually collected from the volcanoes themselves.
Page 315
X
THE PROGRESS OF CHEMISTRY DURING THE PAST
ONE HUNDRED YEARS
By HORACE L. WELLS and HARRY W. FOOTE
Introduction.
As we look back to the time of the founding of the Journal in 1818, we see
that the science of chemistry had recently made and was then making great
advances. That the scientific men of those days were much impressed with
what was being accomplished is well shown by the following statement
made in an early number of the Journal (3, 330, 1821) by its founder in
reviewing Gorham’s Elements of Chemical Science. He says: “The present
period is distinguished by wonderful mental activity; it might indeed be
denominated as the intellectual age of the world. At no former period has
the mind of man been directed at one time to so many and so useful
researches.”
A very remarkable revolution in chemical ideas had recently taken place.
Soon after the discovery of oxygen by Priestley in 1774, and the subsequent
discovery by Cavendish that water was formed by the combustion of
hydrogen and oxygen, Lavoisier had explained combustion in general as
oxidation, thus overthrowing the curious old phlogiston theory which had
prevailed as the basis of chemical philosophy for nearly a century.
The era of modern chemistry had thus begun, and the additional views
that matter was indestructible and that chemical compounds were of
THE PROGRESS OF CHEMISTRY DURING THE PAST
ONE HUNDRED YEARS
By HORACE L. WELLS and HARRY W. FOOTE
Introduction.
As we look back to the time of the founding of the Journal in 1818, we see
that the science of chemistry had recently made and was then making great
advances. That the scientific men of those days were much impressed with
what was being accomplished is well shown by the following statement
made in an early number of the Journal (3, 330, 1821) by its founder in
reviewing Gorham’s Elements of Chemical Science. He says: “The present
period is distinguished by wonderful mental activity; it might indeed be
denominated as the intellectual age of the world. At no former period has
the mind of man been directed at one time to so many and so useful
researches.”
A very remarkable revolution in chemical ideas had recently taken place.
Soon after the discovery of oxygen by Priestley in 1774, and the subsequent
discovery by Cavendish that water was formed by the combustion of
hydrogen and oxygen, Lavoisier had explained combustion in general as
oxidation, thus overthrowing the curious old phlogiston theory which had
prevailed as the basis of chemical philosophy for nearly a century.
The era of modern chemistry had thus begun, and the additional views
that matter was indestructible and that chemical compounds were of
Page 316
constant composition had been generally accepted at the beginning of the
nineteenth century.
Dalton had announced his atomic theory in 1802, having based it largely
upon the law of multiple proportions which he had previously discovered,
and he had begun to express the formulas for compounds in terms of atomic
symbols.
In 1808 Gay-Lussac had discovered his law of gas combination in simple
proportions,[153] a law of supreme importance in connection with the atomic
theory, but neither he nor Dalton had seen this theoretical connection.
Avogadro had understood it, however, and in 1811 had reached the
momentous conclusion that all gases and vapors have equal numbers of
molecules in equal volumes at the same temperature and pressure.
Davy in 1807 had isolated the alkali-metals, sodium and potassium, by
means of electrolysis, thus practically dispelling the view that certain earthy
substances might be elementary; and about four years later he had
demonstrated that chlorine was an element, not an oxide as had been
supposed previously, thus overthrowing Lavoisier’s view that oxygen was
the characteristic constituent of all acids.
At the time that our period of history begins, the atomic theory had been
accepted generally, but in a somewhat indefinite form, since little attention
had been paid to Avogadro’s principle, and since Dalton had used only the
principle of greatest simplicity in writing the formulas of compounds,
considering water as HO and ammonia NH, for example. At this time,
however, Berzelius for ten or fifteen years had been devoting tremendous
energy to the task of determining the atomic weights of nearly all of the
elements then known by analyzing their compounds. He had confirmed the
law of multiple proportions, accepted the atomic theory, and utilized
Avogadro’s principle, and it is an interesting coincidence that his first table
of atomic weights was published in the year 1818.
An interesting account of the views on chemistry held at about that time
was published in the Journal by Denison Olmsted (11, 349, 1826; 12, 1,
1827), who had recently become professor of natural philosophy in Yale
College.
The most illustrious European chemists of that time were Berzelius of
Sweden, Davy of England, and Gay-Lussac of France, and the curious
circumstance may be mentioned that all three of them and also Benjamin
nineteenth century.
Dalton had announced his atomic theory in 1802, having based it largely
upon the law of multiple proportions which he had previously discovered,
and he had begun to express the formulas for compounds in terms of atomic
symbols.
In 1808 Gay-Lussac had discovered his law of gas combination in simple
proportions,[153] a law of supreme importance in connection with the atomic
theory, but neither he nor Dalton had seen this theoretical connection.
Avogadro had understood it, however, and in 1811 had reached the
momentous conclusion that all gases and vapors have equal numbers of
molecules in equal volumes at the same temperature and pressure.
Davy in 1807 had isolated the alkali-metals, sodium and potassium, by
means of electrolysis, thus practically dispelling the view that certain earthy
substances might be elementary; and about four years later he had
demonstrated that chlorine was an element, not an oxide as had been
supposed previously, thus overthrowing Lavoisier’s view that oxygen was
the characteristic constituent of all acids.
At the time that our period of history begins, the atomic theory had been
accepted generally, but in a somewhat indefinite form, since little attention
had been paid to Avogadro’s principle, and since Dalton had used only the
principle of greatest simplicity in writing the formulas of compounds,
considering water as HO and ammonia NH, for example. At this time,
however, Berzelius for ten or fifteen years had been devoting tremendous
energy to the task of determining the atomic weights of nearly all of the
elements then known by analyzing their compounds. He had confirmed the
law of multiple proportions, accepted the atomic theory, and utilized
Avogadro’s principle, and it is an interesting coincidence that his first table
of atomic weights was published in the year 1818.
An interesting account of the views on chemistry held at about that time
was published in the Journal by Denison Olmsted (11, 349, 1826; 12, 1,
1827), who had recently become professor of natural philosophy in Yale
College.
The most illustrious European chemists of that time were Berzelius of
Sweden, Davy of England, and Gay-Lussac of France, and the curious
circumstance may be mentioned that all three of them and also Benjamin
Page 317
Silliman, the founder of the Journal, were born within a period of eight
months in 1778–1779.
In this country Robert Hare of Philadelphia and Benjamin Silliman were
undoubtedly the most prominent chemists of those days. Hare is best known
for his invention of the compound blowpipe, but his contributions to the
Journal were very numerous, beginning almost with the first volume and
continuing for over thirty years. Among the first of these contributions was
a most vigorous but well-merited attack upon a Doctor Clark of Cambridge,
England, who had copied his invention without giving him proper credit.
He begins (2, 281, 1820) by saying: “Dr. Clark has published a book on the
gas blowpipe in which he professes a sincere desire to render everyone his
due. That it would be difficult for the conduct of any author to be more
discordant with these professions, I pledge myself to prove in the following
pages.”
Hare also invented a galvanic battery which he called a “deflagrator,”
consisting of a large number of single cells in series. With this, using carbon
electrodes, he was able to obtain a higher temperature than with his oxy-
hydrogen blowpipe. He was the first to apply galvanic ignition to blasting
(21, 139, 1832), and he first carried out electrolyses with the use of mercury
as the cathode (37, 267, 1839). In this way he prepared metallic calcium
and other metals from solutions of their chlorides, while the principle
employed by him has in recent times been used as the basis of a very
important process for manufacturing caustic potash and soda.
Silliman, who had become an intimate friend of Hare during two periods
of chemical study under Woodhouse in Philadelphia in 1802–1804, and who
soon afterwards spent fourteen months as a student abroad, chiefly in
England and Scotland, took a broad interest in science and gave much
attention to geology as well as to chemistry. In spite of this divided interest
and his work as a teacher, popular scientific lecturer, and editor, he found
time for a surprising amount of original chemical work. For instance, using
Hare’s deflagrator, he showed that carbon was volatilized in the electric arc
(5, 108, 1822); he was the first in this country to prepare hydrofluoric acid
(6, 354, 1823), and he first detected bromine in one of our natural brines
(18, 142, 1830).
months in 1778–1779.
In this country Robert Hare of Philadelphia and Benjamin Silliman were
undoubtedly the most prominent chemists of those days. Hare is best known
for his invention of the compound blowpipe, but his contributions to the
Journal were very numerous, beginning almost with the first volume and
continuing for over thirty years. Among the first of these contributions was
a most vigorous but well-merited attack upon a Doctor Clark of Cambridge,
England, who had copied his invention without giving him proper credit.
He begins (2, 281, 1820) by saying: “Dr. Clark has published a book on the
gas blowpipe in which he professes a sincere desire to render everyone his
due. That it would be difficult for the conduct of any author to be more
discordant with these professions, I pledge myself to prove in the following
pages.”
Hare also invented a galvanic battery which he called a “deflagrator,”
consisting of a large number of single cells in series. With this, using carbon
electrodes, he was able to obtain a higher temperature than with his oxy-
hydrogen blowpipe. He was the first to apply galvanic ignition to blasting
(21, 139, 1832), and he first carried out electrolyses with the use of mercury
as the cathode (37, 267, 1839). In this way he prepared metallic calcium
and other metals from solutions of their chlorides, while the principle
employed by him has in recent times been used as the basis of a very
important process for manufacturing caustic potash and soda.
Silliman, who had become an intimate friend of Hare during two periods
of chemical study under Woodhouse in Philadelphia in 1802–1804, and who
soon afterwards spent fourteen months as a student abroad, chiefly in
England and Scotland, took a broad interest in science and gave much
attention to geology as well as to chemistry. In spite of this divided interest
and his work as a teacher, popular scientific lecturer, and editor, he found
time for a surprising amount of original chemical work. For instance, using
Hare’s deflagrator, he showed that carbon was volatilized in the electric arc
(5, 108, 1822); he was the first in this country to prepare hydrofluoric acid
(6, 354, 1823), and he first detected bromine in one of our natural brines
(18, 142, 1830).
Page 318
Atomic Weights.
As soon as the atomic theory was accepted, the relative weights of the
atoms became a matter of vital importance in connection with formulas and
chemical calculations. In advancing his theory, Dalton had made some very
rough atomic weight determinations, and it has been mentioned already that
Berzelius, at the time that our historical period begins, was engaged in the
prodigious task of accurately determining these constants for nearly all the
known elements. It is recorded that he analyzed quantitatively no less than
two thousand compounds in connection with this work during his career.
His table of 1818 has proved to be remarkably accurate for that pioneer
period, and it indicates his remarkable skill as an analyst.
It is to be observed that Berzelius in this early table made use of
Avogadro’s principle in connection with elements forming gaseous
compounds, and thus obtained correct formulas and atomic weights in such
cases, but that in many instances his atomic weights and those now
accepted bear the relation of simple multiples to one another, because he
had then no means of deciding upon the formulas of many compounds
except the rule of assumed simplicity. For example, the two oxides of iron
now considered to be FeO and Fe2O3 he regarded as FeO2 and FeO3,
knowing as he did that the ratio of oxygen in them was 2 to 3, and believing
that a single atom of iron in each was the simplest view of the case, so that
as the consequence of these formulas the atomic weight of iron was then
considered to be practically twice as great in its relation to oxygen as at
present.
These old atomic weights of Berzelius, used with the corresponding
formulas, were just as serviceable for calculating compositions and
analytical factors as though the correct multiples had been selected. As time
went on, the true multiples were gradually found from considerations of
atomic heats, isomorphism, vapor densities, the periodic law, and so on, and
suitable changes were made in the chemical formulas.
Berzelius used 100 parts of oxygen as the basis of his atomic weights, a
practice which was generally followed for several decades. Dalton,
however, had originally used hydrogen as unity as the basis, and this plan
As soon as the atomic theory was accepted, the relative weights of the
atoms became a matter of vital importance in connection with formulas and
chemical calculations. In advancing his theory, Dalton had made some very
rough atomic weight determinations, and it has been mentioned already that
Berzelius, at the time that our historical period begins, was engaged in the
prodigious task of accurately determining these constants for nearly all the
known elements. It is recorded that he analyzed quantitatively no less than
two thousand compounds in connection with this work during his career.
His table of 1818 has proved to be remarkably accurate for that pioneer
period, and it indicates his remarkable skill as an analyst.
It is to be observed that Berzelius in this early table made use of
Avogadro’s principle in connection with elements forming gaseous
compounds, and thus obtained correct formulas and atomic weights in such
cases, but that in many instances his atomic weights and those now
accepted bear the relation of simple multiples to one another, because he
had then no means of deciding upon the formulas of many compounds
except the rule of assumed simplicity. For example, the two oxides of iron
now considered to be FeO and Fe2O3 he regarded as FeO2 and FeO3,
knowing as he did that the ratio of oxygen in them was 2 to 3, and believing
that a single atom of iron in each was the simplest view of the case, so that
as the consequence of these formulas the atomic weight of iron was then
considered to be practically twice as great in its relation to oxygen as at
present.
These old atomic weights of Berzelius, used with the corresponding
formulas, were just as serviceable for calculating compositions and
analytical factors as though the correct multiples had been selected. As time
went on, the true multiples were gradually found from considerations of
atomic heats, isomorphism, vapor densities, the periodic law, and so on, and
suitable changes were made in the chemical formulas.
Berzelius used 100 parts of oxygen as the basis of his atomic weights, a
practice which was generally followed for several decades. Dalton,
however, had originally used hydrogen as unity as the basis, and this plan
Page 319
finally came into use everywhere, as it seemed to be more logical and
convenient, because hydrogen has the smallest atomic weight, and also
because the atomic weights of a number of common elements appeared to
be exact multiples of that of hydrogen, thus giving simpler numbers for use
in calculations.
Within a few years a slight change has been made by the adoption of
oxygen as exactly 16 as the basis, which gives hydrogen the value of 1·008.
As early as 1815, Prout, an English physician, had advanced the view
that hydrogen is the primordial substance of all the elements, and
consequently that the atomic weights are all exact multiples of that of
hydrogen. This hypothesis has been one of the incentives to investigations
upon atomic weights, for it has been found that these constants in the cases
of a considerable number of the elements are very close to whole numbers
when based upon hydrogen as unity, or even still closer when based upon
oxygen as 16.
With our present knowledge Prout’s hypothesis may be regarded as
disproved for nearly all the elements whose atomic weights have been
accurately determined, but the close or even exact agreement with it in a
few cases is still worthy of consideration. There is an interesting letter from
Berzelius to B. Silliman, Jr., in the Journal (48, 369, 1845) in which
Berzelius considers the theory entirely disproved.
For a long time entire reliance was placed upon the atomic weights
obtained by Berzelius, but it came to be observed that the calculation of
carbon from carbon dioxide appeared to give high results in certain cases,
so that doubt arose as to the accuracy of Berzelius’s work. Consequently in
1840 Dumas, assisted by his pupil Stas, made a new determination of the
atomic weight of carbon, and found that the number obtained by Berzelius,
12·12, was slightly too large. Subsequently Dumas determined more than
twenty other atomic weights, but this great amount of work did not bring
about any considerable improvement, for it appears that Dumas did not
greatly excel Berzelius in accuracy, and that the latter had made one of his
most noticeable errors in connection with carbon.
Soon after assisting Dumas in the work upon carbon, Stas began his very
extensive and accurate, independent determinations, leading to the
publication of a book in 1867 describing his work. Stas made many
improvements in methods by the use of great care in purifying the
convenient, because hydrogen has the smallest atomic weight, and also
because the atomic weights of a number of common elements appeared to
be exact multiples of that of hydrogen, thus giving simpler numbers for use
in calculations.
Within a few years a slight change has been made by the adoption of
oxygen as exactly 16 as the basis, which gives hydrogen the value of 1·008.
As early as 1815, Prout, an English physician, had advanced the view
that hydrogen is the primordial substance of all the elements, and
consequently that the atomic weights are all exact multiples of that of
hydrogen. This hypothesis has been one of the incentives to investigations
upon atomic weights, for it has been found that these constants in the cases
of a considerable number of the elements are very close to whole numbers
when based upon hydrogen as unity, or even still closer when based upon
oxygen as 16.
With our present knowledge Prout’s hypothesis may be regarded as
disproved for nearly all the elements whose atomic weights have been
accurately determined, but the close or even exact agreement with it in a
few cases is still worthy of consideration. There is an interesting letter from
Berzelius to B. Silliman, Jr., in the Journal (48, 369, 1845) in which
Berzelius considers the theory entirely disproved.
For a long time entire reliance was placed upon the atomic weights
obtained by Berzelius, but it came to be observed that the calculation of
carbon from carbon dioxide appeared to give high results in certain cases,
so that doubt arose as to the accuracy of Berzelius’s work. Consequently in
1840 Dumas, assisted by his pupil Stas, made a new determination of the
atomic weight of carbon, and found that the number obtained by Berzelius,
12·12, was slightly too large. Subsequently Dumas determined more than
twenty other atomic weights, but this great amount of work did not bring
about any considerable improvement, for it appears that Dumas did not
greatly excel Berzelius in accuracy, and that the latter had made one of his
most noticeable errors in connection with carbon.
Soon after assisting Dumas in the work upon carbon, Stas began his very
extensive and accurate, independent determinations, leading to the
publication of a book in 1867 describing his work. Stas made many
improvements in methods by the use of great care in purifying the
Page 320
substances employed, and especially by using large quantities of material in
his determinations, thus diminishing the proportional errors in weighing.
His results, which dealt with most of the common elements, were accepted
with much confidence by chemists everywhere.
Stas reached the conclusion that there could be no real foundation for
Prout’s hypothesis, since so many of his atomic weights varied from whole
numbers, and this opinion has been generally accepted.
The first accurate atomic weight determination published in the Journal
was that by Mallett on lithium (22, 349, 1856; 28, 349, 1859), showing a
result almost identical with that accepted at the present time. Johnson and
Allen’s determination (35, 94, 1863) on the rare element cæsium was
carried out with extraordinary accuracy. Lee, working with Wolcott Gibbs,
made good determinations on nickel and cobalt (2, 44, 1871). The work of
Cooke on antimony (15, 41, 107, 1878) was excellent.
Concerning the more recent work published elsewhere than in the
Journal, attention should be called particularly to the investigations that
have been carried on for the past twenty-five years by Richards and his
associates at Harvard University. Richards has shown masterly ability in the
selection of methods and in avoiding errors. His results have displayed such
marvelous agreements among repeated determinations by the same and by
different processes as to inspire the greatest confidence. His work has been
very extensive, and it is a great credit to our country that this atomic weight
work, so superior to all that has been previously done, is being carried out
here.
It may be mentioned that for a number of years the decision in regard to
the atomic weights to be accepted has been in the hands of an International
Committee of which our fellow countryman F. W. Clarke has been
chairman. In connection with this position and previously, Clarke has done
valuable service in re-calculating and summarizing atomic weight
determinations.
his determinations, thus diminishing the proportional errors in weighing.
His results, which dealt with most of the common elements, were accepted
with much confidence by chemists everywhere.
Stas reached the conclusion that there could be no real foundation for
Prout’s hypothesis, since so many of his atomic weights varied from whole
numbers, and this opinion has been generally accepted.
The first accurate atomic weight determination published in the Journal
was that by Mallett on lithium (22, 349, 1856; 28, 349, 1859), showing a
result almost identical with that accepted at the present time. Johnson and
Allen’s determination (35, 94, 1863) on the rare element cæsium was
carried out with extraordinary accuracy. Lee, working with Wolcott Gibbs,
made good determinations on nickel and cobalt (2, 44, 1871). The work of
Cooke on antimony (15, 41, 107, 1878) was excellent.
Concerning the more recent work published elsewhere than in the
Journal, attention should be called particularly to the investigations that
have been carried on for the past twenty-five years by Richards and his
associates at Harvard University. Richards has shown masterly ability in the
selection of methods and in avoiding errors. His results have displayed such
marvelous agreements among repeated determinations by the same and by
different processes as to inspire the greatest confidence. His work has been
very extensive, and it is a great credit to our country that this atomic weight
work, so superior to all that has been previously done, is being carried out
here.
It may be mentioned that for a number of years the decision in regard to
the atomic weights to be accepted has been in the hands of an International
Committee of which our fellow countryman F. W. Clarke has been
chairman. In connection with this position and previously, Clarke has done
valuable service in re-calculating and summarizing atomic weight
determinations.
Page 321
Analytical Chemistry.
Analysis is of such fundamental importance in nearly every other branch
of chemical investigation that its development has been of the utmost
importance in connection with the advancement of the science. It attained,
therefore, a comparatively early development, and one hundred years ago it
was in a flourishing condition, particularly as far as inorganic qualitative
and gravimetric analysis were concerned. There is no doubt that Berzelius,
whose atomic weight determinations have already been mentioned,
surpassed all other analysts of that time in the amount, variety, and accuracy
of his gravimetric work. He lived through three decades of our period, until
1848.
During the past century there has been constant progress in inorganic
analysis, due to improved methods, better apparatus and accumulated
experience. An excellent work on this subject was published by H. Rose, a
pupil of Berzelius, and the methods of the latter, with many improvements
and additions by the author and others, were thus made accessible.
Fresenius, who was born in 1818, did much service in establishing a
laboratory in which the teaching of analytical chemistry was made a
specialty, in writing text-books on the subject and in establishing in 1862
the “Zeitschrift für analytische Chemie,” which has continued up to the
present time.
Besides Berzelius, who was the first to show that minerals were definite
chemical compounds, there have been many prominent mineral analysts in
Europe, among whom Rammelsberg and Bunsen may be mentioned, but
there came a time towards the end of the nineteenth century when the
attention of chemists, particularly in Germany, was so much absorbed by
organic chemistry that mineral analysis came near becoming a lost art there.
It was during that period that an English mineralogist, visiting New Haven
and praising the mineral analyses that were being carried out at Yale,
expressed regret that there appeared to be no one in England, or in Germany
either, who could analyze minerals.
The best analytical work done in this country in the early part of our
period was chiefly in connection with mineral analysis, and a large share of
Analysis is of such fundamental importance in nearly every other branch
of chemical investigation that its development has been of the utmost
importance in connection with the advancement of the science. It attained,
therefore, a comparatively early development, and one hundred years ago it
was in a flourishing condition, particularly as far as inorganic qualitative
and gravimetric analysis were concerned. There is no doubt that Berzelius,
whose atomic weight determinations have already been mentioned,
surpassed all other analysts of that time in the amount, variety, and accuracy
of his gravimetric work. He lived through three decades of our period, until
1848.
During the past century there has been constant progress in inorganic
analysis, due to improved methods, better apparatus and accumulated
experience. An excellent work on this subject was published by H. Rose, a
pupil of Berzelius, and the methods of the latter, with many improvements
and additions by the author and others, were thus made accessible.
Fresenius, who was born in 1818, did much service in establishing a
laboratory in which the teaching of analytical chemistry was made a
specialty, in writing text-books on the subject and in establishing in 1862
the “Zeitschrift für analytische Chemie,” which has continued up to the
present time.
Besides Berzelius, who was the first to show that minerals were definite
chemical compounds, there have been many prominent mineral analysts in
Europe, among whom Rammelsberg and Bunsen may be mentioned, but
there came a time towards the end of the nineteenth century when the
attention of chemists, particularly in Germany, was so much absorbed by
organic chemistry that mineral analysis came near becoming a lost art there.
It was during that period that an English mineralogist, visiting New Haven
and praising the mineral analyses that were being carried out at Yale,
expressed regret that there appeared to be no one in England, or in Germany
either, who could analyze minerals.
The best analytical work done in this country in the early part of our
period was chiefly in connection with mineral analysis, and a large share of
Page 322
it was published in the Journal. Henry Seybert, of Philadelphia, in
particular, showed remarkable skill in this direction, and published
numerous analyses of silicates and other minerals, beginning in 1822. It was
he who first detected boric acid in tourmaline (6, 155, 1822), and beryllium
in chrysoberyl (8, 105, 1824). His methods for silicate analyses were very
similar to those used at the present time.
J. Lawrence Smith in 1853 described his method for determining alkalies
in minerals (16, 53), a method which in its final form (1, 269, 1871) is the
best ever devised for the purpose. He also described (15, 94, 1853) a very
useful method, still largely used in analytical work, for destroying
ammonium salts by means of aqua regia. Carey Lea (42, 109, 1866)
described the well-known test for iodides by means of potassium
dichromate. F. W. Clarke (49, 48, 1870) showed that antimony and arsenic
could be quantitatively separated from tin by the precipitation of the
sulphides in the presence of oxalic acid. In 1864 Wolcott Gibbs (37, 346)
began an important series of analytical notes from the Lawrence Scientific
School, and he worked out later many difficult analytical problems,
particularly in connection with his extensive researches upon the complex
inorganic acids.
From 1850 on, Brush and his students made many important
investigations upon minerals, and from 1877 Penfield (13, 425), beginning
with an analysis of a new mineral from Branchville, Connecticut, described
by Brush and E. S. Dana, displayed remarkable skill and industry in this
kind of work. Both of the writers of this article were fortunate in being
associated with Penfield in some of his researches upon minerals and one of
us began as he did with the Branchville work. It is probably fair to say that
Penfield did the most accurate work in mineral analysis that has ever been
accomplished, and that he was similarly successful in crystallography and
other physical branches of mineralogy.
The American analytical investigations that have been mentioned were
all published in the Journal, with the exception of a part of Gibbs’s work.
Many other American workers at mineral analysis might be alluded to here,
but only the excellent work of a number of chemists in the United States
Geological Survey will be mentioned. Among these Hillebrand deserves
particular praise for the extent of his investigations and for his careful
researches in improving the methods of rock analysis.
particular, showed remarkable skill in this direction, and published
numerous analyses of silicates and other minerals, beginning in 1822. It was
he who first detected boric acid in tourmaline (6, 155, 1822), and beryllium
in chrysoberyl (8, 105, 1824). His methods for silicate analyses were very
similar to those used at the present time.
J. Lawrence Smith in 1853 described his method for determining alkalies
in minerals (16, 53), a method which in its final form (1, 269, 1871) is the
best ever devised for the purpose. He also described (15, 94, 1853) a very
useful method, still largely used in analytical work, for destroying
ammonium salts by means of aqua regia. Carey Lea (42, 109, 1866)
described the well-known test for iodides by means of potassium
dichromate. F. W. Clarke (49, 48, 1870) showed that antimony and arsenic
could be quantitatively separated from tin by the precipitation of the
sulphides in the presence of oxalic acid. In 1864 Wolcott Gibbs (37, 346)
began an important series of analytical notes from the Lawrence Scientific
School, and he worked out later many difficult analytical problems,
particularly in connection with his extensive researches upon the complex
inorganic acids.
From 1850 on, Brush and his students made many important
investigations upon minerals, and from 1877 Penfield (13, 425), beginning
with an analysis of a new mineral from Branchville, Connecticut, described
by Brush and E. S. Dana, displayed remarkable skill and industry in this
kind of work. Both of the writers of this article were fortunate in being
associated with Penfield in some of his researches upon minerals and one of
us began as he did with the Branchville work. It is probably fair to say that
Penfield did the most accurate work in mineral analysis that has ever been
accomplished, and that he was similarly successful in crystallography and
other physical branches of mineralogy.
The American analytical investigations that have been mentioned were
all published in the Journal, with the exception of a part of Gibbs’s work.
Many other American workers at mineral analysis might be alluded to here,
but only the excellent work of a number of chemists in the United States
Geological Survey will be mentioned. Among these Hillebrand deserves
particular praise for the extent of his investigations and for his careful
researches in improving the methods of rock analysis.
Page 323
To our own Professor Gooch especial praise must be accorded for the
very large number of analytical methods that have been devised, or
critically studied, by him and his students, and for the excellent quality of
this work. The publications in the Journal from his laboratory began in 1890
(39, 188), and the extraordinary extent of this work is shown by the fact that
the three hundredth paper from the Kent Laboratory appeared in May, 1918.
These very numerous and important investigations have been of great
scientific and practical value, and they have formed a striking feature of the
Journal for nearly 30 years. In 1912 Gooch published his “Methods in
Chemical Analysis,” a book of over 500 pages, in which the work in the
Kent Chemical Laboratory up to that time was concisely presented. Among
the many workers who have assisted in these investigations, P. E.
Browning, W. A. Drushel, F. S. Havens, D. A. Kreider, C. A. Peters, I. K.
Phelps and R. G. Van Name are particularly prominent. Besides many other
useful pieces of apparatus, the perforated filtering crucible was devised by
Gooch, and this has brought his name into everyday use in all chemical
laboratories.
Volumetric analysis was originated by Gay-Lussac, who described a
method for chlorimetry in 1824, for alkalimetry in 1828, and for the
determination of silver and chlorides in 1832. Margueritte devised titrations
with potassium permanganate in 1846, while Bunsen, not far from the same
time, introduced the use of iodine and sulphur dioxide solutions for the
purpose of determining many oxidations and reductions. We owe to Mohr
some improvements in apparatus and a German text-book on the subject,
while Sutton wrote an excellent English work on volumetric analysis, of
which many editions have appeared.
While volumetric analysis began to be used less than one hundred years
ago, its applications have been gradually extended to a very great degree,
and it is not only exceedingly important in investigations in pure chemistry,
but its use is especially extensive in technical laboratories where large
numbers of rapid analyses are required.
Not a few volumetric methods have been devised or improved in the
United States, but mention will be made here only of Cooke’s important
method for the determination of ferrous iron in insoluble silicates, published
in the Journal (44, 347, 1867); to Penfield’s method for the determination of
fluorine in 1878; and to the more recent general method of titration with an
very large number of analytical methods that have been devised, or
critically studied, by him and his students, and for the excellent quality of
this work. The publications in the Journal from his laboratory began in 1890
(39, 188), and the extraordinary extent of this work is shown by the fact that
the three hundredth paper from the Kent Laboratory appeared in May, 1918.
These very numerous and important investigations have been of great
scientific and practical value, and they have formed a striking feature of the
Journal for nearly 30 years. In 1912 Gooch published his “Methods in
Chemical Analysis,” a book of over 500 pages, in which the work in the
Kent Chemical Laboratory up to that time was concisely presented. Among
the many workers who have assisted in these investigations, P. E.
Browning, W. A. Drushel, F. S. Havens, D. A. Kreider, C. A. Peters, I. K.
Phelps and R. G. Van Name are particularly prominent. Besides many other
useful pieces of apparatus, the perforated filtering crucible was devised by
Gooch, and this has brought his name into everyday use in all chemical
laboratories.
Volumetric analysis was originated by Gay-Lussac, who described a
method for chlorimetry in 1824, for alkalimetry in 1828, and for the
determination of silver and chlorides in 1832. Margueritte devised titrations
with potassium permanganate in 1846, while Bunsen, not far from the same
time, introduced the use of iodine and sulphur dioxide solutions for the
purpose of determining many oxidations and reductions. We owe to Mohr
some improvements in apparatus and a German text-book on the subject,
while Sutton wrote an excellent English work on volumetric analysis, of
which many editions have appeared.
While volumetric analysis began to be used less than one hundred years
ago, its applications have been gradually extended to a very great degree,
and it is not only exceedingly important in investigations in pure chemistry,
but its use is especially extensive in technical laboratories where large
numbers of rapid analyses are required.
Not a few volumetric methods have been devised or improved in the
United States, but mention will be made here only of Cooke’s important
method for the determination of ferrous iron in insoluble silicates, published
in the Journal (44, 347, 1867); to Penfield’s method for the determination of
fluorine in 1878; and to the more recent general method of titration with an
Page 324
iodate in strong hydrochloric acid solutions, due to L. W. Andrews, a
number of applications of which have been worked out in the Sheffield
Laboratory.
A considerable amount of work with gases had been done by Priestley,
Scheele, Cavendish, Lavoisier, Dalton, Gay-Lussac, and others before our
hundred-year period began. Cavendish, about 1780, had analyzed
atmospheric air with remarkable accuracy, and had even separated the argon
from it and wondered what it was, and later Gay-Lussac had shown great
skill in the study of gas reactions. During our period gas analysis has been
further developed by many chemists. Bunsen, in particular, brought the art
to a high degree of perfection in the course of a long period beginning about
1838, the last edition of his “Methods of Gas Analysis” having been
published in 1877.
Important devices for the simplification of gas analysis in order that it
might be used more conveniently for technical purposes have been
introduced by Orsat in France and by Winkler, Hempel and Bunte in
Germany.
It appears that our countryman Morley has surpassed all others in
accurate work with gases in connection with his determinations of the
combining weights and volumes of hydrogen and oxygen about the year
1891. Some of his publications have appeared in the Journal (30, 140, 1885;
41, 220, 1891; and others).
Electrolytic analysis, involving the deposition of metals, or sometimes of
oxides, usually upon a platinum electrode, was brought into use in 1865 by
Wolcott Gibbs through an article published in the Journal (39, 58, 1865). He
there described the electrolytic precipitation of copper and of nickel by the
methods still in use. The application of the process has been extended to a
number of other metals, and it has been largely employed, particularly in
technical analyses. Important investigations and excellent books on this
subject have been the contributions of Edgar F. Smith of the University of
Pennsylvania, and the useful improvement, the rotating cathode, was
devised by Gooch and described in the Journal (15, 320, 1903).
number of applications of which have been worked out in the Sheffield
Laboratory.
A considerable amount of work with gases had been done by Priestley,
Scheele, Cavendish, Lavoisier, Dalton, Gay-Lussac, and others before our
hundred-year period began. Cavendish, about 1780, had analyzed
atmospheric air with remarkable accuracy, and had even separated the argon
from it and wondered what it was, and later Gay-Lussac had shown great
skill in the study of gas reactions. During our period gas analysis has been
further developed by many chemists. Bunsen, in particular, brought the art
to a high degree of perfection in the course of a long period beginning about
1838, the last edition of his “Methods of Gas Analysis” having been
published in 1877.
Important devices for the simplification of gas analysis in order that it
might be used more conveniently for technical purposes have been
introduced by Orsat in France and by Winkler, Hempel and Bunte in
Germany.
It appears that our countryman Morley has surpassed all others in
accurate work with gases in connection with his determinations of the
combining weights and volumes of hydrogen and oxygen about the year
1891. Some of his publications have appeared in the Journal (30, 140, 1885;
41, 220, 1891; and others).
Electrolytic analysis, involving the deposition of metals, or sometimes of
oxides, usually upon a platinum electrode, was brought into use in 1865 by
Wolcott Gibbs through an article published in the Journal (39, 58, 1865). He
there described the electrolytic precipitation of copper and of nickel by the
methods still in use. The application of the process has been extended to a
number of other metals, and it has been largely employed, particularly in
technical analyses. Important investigations and excellent books on this
subject have been the contributions of Edgar F. Smith of the University of
Pennsylvania, and the useful improvement, the rotating cathode, was
devised by Gooch and described in the Journal (15, 320, 1903).
Page 325
General Inorganic Chemistry.
The Chemical Symbols.—It is to Berzelius that we owe our symbols for
the atoms, derived usually from their Latin names, such as C for carbon, Na
for sodium, Cl for chlorine, Fe for iron, Ag for silver, and Au for gold. We
owe to him also the use of small figures to show the number of atoms in a
formula, as in N2O5. This was a marked improvement over the hieroglyphic
symbols proposed by Dalton, which were set down as many times as the
atoms were supposed to occur in formulas, forming groups of curious
appearance, but in some respects not unlike some of our modern developed
formulas. The advantages of Berzelius’s symbols were their simplicity,
legibility, and the fact that they could be printed without the need of special
type. It is true that at a later period Berzelius used certain symbols with
horizontal lines crossing them to represent double atoms, and that these
made some difficulty in printing. It should be mentioned also that Berzelius
at one time made an effort to simplify formulas by placing dots over other
symbols to represent oxygen, and commas to represent sulphur atoms.
Examples of these are:
ĊaS⃛, calcium sulphate; F̋ e, iron disulphide
This form of notation was quite extensively employed for a time,
especially by mineralogists, but it was entirely abandoned later.
It is interesting to notice that Dalton, who lived until 1844, to reach the
age of 78, differed from other chemists in refusing to accept the letter-
symbols of Berzelius. In a letter written to Graham in 1837 he said:
“Berzelius’s symbols are horrifying. A young student in chemistry might as
soon learn Hebrew as to make himself acquainted with them. They appear
like a chaos of atoms ... and to equally perplex the adepts of science, to
discourage the learner, as well as to cloud the beauty and simplicity of the
atomic theory.”
This forcibly expressed opinion was apparently tinged with self-esteem,
but there is no doubt that Dalton was sincere in believing that the atoms
were best represented by his circular symbols, because, as is well known, he
thought that all the atoms were spherical in form, and it is evident that
The Chemical Symbols.—It is to Berzelius that we owe our symbols for
the atoms, derived usually from their Latin names, such as C for carbon, Na
for sodium, Cl for chlorine, Fe for iron, Ag for silver, and Au for gold. We
owe to him also the use of small figures to show the number of atoms in a
formula, as in N2O5. This was a marked improvement over the hieroglyphic
symbols proposed by Dalton, which were set down as many times as the
atoms were supposed to occur in formulas, forming groups of curious
appearance, but in some respects not unlike some of our modern developed
formulas. The advantages of Berzelius’s symbols were their simplicity,
legibility, and the fact that they could be printed without the need of special
type. It is true that at a later period Berzelius used certain symbols with
horizontal lines crossing them to represent double atoms, and that these
made some difficulty in printing. It should be mentioned also that Berzelius
at one time made an effort to simplify formulas by placing dots over other
symbols to represent oxygen, and commas to represent sulphur atoms.
Examples of these are:
ĊaS⃛, calcium sulphate; F̋ e, iron disulphide
This form of notation was quite extensively employed for a time,
especially by mineralogists, but it was entirely abandoned later.
It is interesting to notice that Dalton, who lived until 1844, to reach the
age of 78, differed from other chemists in refusing to accept the letter-
symbols of Berzelius. In a letter written to Graham in 1837 he said:
“Berzelius’s symbols are horrifying. A young student in chemistry might as
soon learn Hebrew as to make himself acquainted with them. They appear
like a chaos of atoms ... and to equally perplex the adepts of science, to
discourage the learner, as well as to cloud the beauty and simplicity of the
atomic theory.”
This forcibly expressed opinion was apparently tinged with self-esteem,
but there is no doubt that Dalton was sincere in believing that the atoms
were best represented by his circular symbols, because, as is well known, he
thought that all the atoms were spherical in form, and it is evident that
Page 326
circles give the proper picture of spherical objects. At the present time some
insight as to the structure of atoms is being gained, and it appears possible
that the time may come when pictures of their external appearance that are
not wholly imaginary may be made.
Changes in Formulas.—Even before the year 1826, Berzelius displayed
great skill in arriving at many formulas that agree with our present ones, for
example, H2O for water, ZnCl2 for zinc chloride, N2O5 for nitric acid
(anhydride), CaO for calcium oxide, CO and CO2 for the oxides of carbon,
and many others. But at the same period other authorities, especially Gay-
Lussac in France and Gmelin in Germany, on account of a lack of
appreciation for Avogadro’s principle and for other reasons, such as the use
of symbols to represent combining weights rather than atoms, were using
different formulas for some of these compounds, such as HO, ZnCl and
NO5, so that their formulas for many of the compounds of hydrogen,
chlorine, nitrogen and several other elements differed from those of
Berzelius. The employment of different formulas involved the use of
different atomic or combining weights. For example, with the formula H2O
for water the composition by weight requires the ratio 1 to 16 for the
weights of the hydrogen and oxygen atoms, while with HO the ratio is 1 to
8.
Berzelius attempted to bring about greater uniformity in formulas and
atomic weights by making changes in his table of atomic weights published
in 1826. He practically doubled the relative atomic weights of hydrogen,
chlorine, nitrogen, and of the other elements that gave twice as many atoms
in his formulas as in those of others, and at the same time he wrote the
symbols of these elements with a bar across them to indicate that they
represented double atoms. For example, he wrote:
H̶O ZnC̶l N̶O5,
instead of
H2O, ZnCl2 N2O5
This appears to have been an unfortunate concession to the views of
others on the part of Berzelius, for the barred symbols were not generally
adopted, partly on account of difficulties in printing, and the great
insight as to the structure of atoms is being gained, and it appears possible
that the time may come when pictures of their external appearance that are
not wholly imaginary may be made.
Changes in Formulas.—Even before the year 1826, Berzelius displayed
great skill in arriving at many formulas that agree with our present ones, for
example, H2O for water, ZnCl2 for zinc chloride, N2O5 for nitric acid
(anhydride), CaO for calcium oxide, CO and CO2 for the oxides of carbon,
and many others. But at the same period other authorities, especially Gay-
Lussac in France and Gmelin in Germany, on account of a lack of
appreciation for Avogadro’s principle and for other reasons, such as the use
of symbols to represent combining weights rather than atoms, were using
different formulas for some of these compounds, such as HO, ZnCl and
NO5, so that their formulas for many of the compounds of hydrogen,
chlorine, nitrogen and several other elements differed from those of
Berzelius. The employment of different formulas involved the use of
different atomic or combining weights. For example, with the formula H2O
for water the composition by weight requires the ratio 1 to 16 for the
weights of the hydrogen and oxygen atoms, while with HO the ratio is 1 to
8.
Berzelius attempted to bring about greater uniformity in formulas and
atomic weights by making changes in his table of atomic weights published
in 1826. He practically doubled the relative atomic weights of hydrogen,
chlorine, nitrogen, and of the other elements that gave twice as many atoms
in his formulas as in those of others, and at the same time he wrote the
symbols of these elements with a bar across them to indicate that they
represented double atoms. For example, he wrote:
H̶O ZnC̶l N̶O5,
instead of
H2O, ZnCl2 N2O5
This appears to have been an unfortunate concession to the views of
others on the part of Berzelius, for the barred symbols were not generally
adopted, partly on account of difficulties in printing, and the great
Page 327
achievement in theory made by him was lost sight of for a long period of
time.
The Law of Atomic Heats.—In 1819, Dulong and Petit of France, from
experiments upon the specific heats of a number of solid elementary
substances, came to the conclusion that the atoms of simple substances have
equal capacities for heat, or in other words, that the specific heats of
elements multiplied by their atomic weights give a constant called the
atomic heat. For instance, the specific heats of sulphur, iron, and gold have
been given as 0·2026, 0·110, and 0·0324, while their atomic weights are
about 32, 56, and 197, respectively; hence the atomic heats obtained by
multiplication are 6·483, 6·116, and 6·383.
Further investigations showed that the atomic heats display a
considerable variation. Those of carbon, boron, beryllium, and silicon are
very low at ordinary temperatures, although they increase and approach the
usual values at higher temperatures. More recent work has shown, however,
that the specific heats of other elements vary greatly with the temperature,
almost disappearing at the temperature of liquid hydrogen, and hence
possibly disappearing entirely at the absolute zero, where the electrical
resistance of the metals appears to vanish likewise.
It has been found that most of the solid elements near ordinary
temperatures give atomic heats that are approximately 6·4. Berzelius
applied the law in fixing a number of atomic weights, and its importance for
this purpose is still recognized.
It may be mentioned here that two well-known Yale men, W. O. Mixter
and E. S. Dana, while students in Bunsen’s laboratory at Heidelberg in
1873, made determinations of the specific heats of boron, silicon, and
zirconium. This was the first determination of this constant for zirconium,
and it was consequently important in establishing the atomic weight of that
element.
Isomorphism and Polymorphism.—Mitscherlich observed in 1818 that
certain phosphates and arsenates have the same crystalline form, and
afterwards he reached the conclusion that identity in form indicates
similarity in composition in connection with the number of atoms and their
arrangement. This law of isomorphism was of much assistance in the
establishment of correct formulas and consequently of atomic weights. For
instance, since the carbonates of barium, strontium, and lead crystallize in
time.
The Law of Atomic Heats.—In 1819, Dulong and Petit of France, from
experiments upon the specific heats of a number of solid elementary
substances, came to the conclusion that the atoms of simple substances have
equal capacities for heat, or in other words, that the specific heats of
elements multiplied by their atomic weights give a constant called the
atomic heat. For instance, the specific heats of sulphur, iron, and gold have
been given as 0·2026, 0·110, and 0·0324, while their atomic weights are
about 32, 56, and 197, respectively; hence the atomic heats obtained by
multiplication are 6·483, 6·116, and 6·383.
Further investigations showed that the atomic heats display a
considerable variation. Those of carbon, boron, beryllium, and silicon are
very low at ordinary temperatures, although they increase and approach the
usual values at higher temperatures. More recent work has shown, however,
that the specific heats of other elements vary greatly with the temperature,
almost disappearing at the temperature of liquid hydrogen, and hence
possibly disappearing entirely at the absolute zero, where the electrical
resistance of the metals appears to vanish likewise.
It has been found that most of the solid elements near ordinary
temperatures give atomic heats that are approximately 6·4. Berzelius
applied the law in fixing a number of atomic weights, and its importance for
this purpose is still recognized.
It may be mentioned here that two well-known Yale men, W. O. Mixter
and E. S. Dana, while students in Bunsen’s laboratory at Heidelberg in
1873, made determinations of the specific heats of boron, silicon, and
zirconium. This was the first determination of this constant for zirconium,
and it was consequently important in establishing the atomic weight of that
element.
Isomorphism and Polymorphism.—Mitscherlich observed in 1818 that
certain phosphates and arsenates have the same crystalline form, and
afterwards he reached the conclusion that identity in form indicates
similarity in composition in connection with the number of atoms and their
arrangement. This law of isomorphism was of much assistance in the
establishment of correct formulas and consequently of atomic weights. For
instance, since the carbonates of barium, strontium, and lead crystallize in
Page 328
the same form, the oxides of these metals must have analogous formulas.
From such considerations Berzelius was able to make several improvements
in his atomic weight table of 1826.
Mitscherlich was the first to observe two forms of sulphur crystals, and
from this and other cases of dimorphism or of polymorphism it became
evident that analogous compounds were not necessarily always
isomorphous, a circumstance which has restricted the application of the law
to some extent.
Besides its application in fixing analogous formulas, the law of
isomorphism has come to be of much practical use in the understanding and
simplification of the formulas for minerals, for these natural crystals very
often contain several isomorphous compounds in varying proportions, and
an understanding of this “isomorphous replacement,” as it is called, makes
it possible to deduce simple general formulas for them.
In some cases isomorphism takes place to a greater or less extent
between substances which are not chemically similar, and this brings about
a variation in composition which at times has caused confusion. For
instance, the mineral pyrrhotite has a composition which usually varies
between Fe7S8 and Fe11S12, and both these formulas have been assigned to
it. It was recently shown by Allen, Crenshaw and Johnston in the Journal
(33, 169, 1912) that this is a case where the compound FeS is capable of
taking up various amounts of sulphur isomorphously.
The idea of solid solution was advanced by van’t Hoff to explain the
crystallization of mixtures, including cases of evident isomorphism. This
view has been widely accepted, and it has been particularly useful in cases
where isomorphism is not evident. Solid solution between metals has been
found to be exceedingly common, many alloys being of this character. A
case of this kind was observed by Cooke and described in the Journal (20,
222, 1855). He prepared two well-crystallized compounds of zinc and
antimony to which he gave the formulas Zn3Sb and Zn2Sb, but he observed
that excellent crystals of each could be obtained which varied largely in
composition from these formulas. As the two compounds were dissimilar in
their formulas and crystalline forms, Cooke assumed that isomorphism was
impossible and concluded “that it is due to an actual perturbation of the law
of definite proportions, produced by the influence of mass.” We should now
regard this as a case of solid solution.
From such considerations Berzelius was able to make several improvements
in his atomic weight table of 1826.
Mitscherlich was the first to observe two forms of sulphur crystals, and
from this and other cases of dimorphism or of polymorphism it became
evident that analogous compounds were not necessarily always
isomorphous, a circumstance which has restricted the application of the law
to some extent.
Besides its application in fixing analogous formulas, the law of
isomorphism has come to be of much practical use in the understanding and
simplification of the formulas for minerals, for these natural crystals very
often contain several isomorphous compounds in varying proportions, and
an understanding of this “isomorphous replacement,” as it is called, makes
it possible to deduce simple general formulas for them.
In some cases isomorphism takes place to a greater or less extent
between substances which are not chemically similar, and this brings about
a variation in composition which at times has caused confusion. For
instance, the mineral pyrrhotite has a composition which usually varies
between Fe7S8 and Fe11S12, and both these formulas have been assigned to
it. It was recently shown by Allen, Crenshaw and Johnston in the Journal
(33, 169, 1912) that this is a case where the compound FeS is capable of
taking up various amounts of sulphur isomorphously.
The idea of solid solution was advanced by van’t Hoff to explain the
crystallization of mixtures, including cases of evident isomorphism. This
view has been widely accepted, and it has been particularly useful in cases
where isomorphism is not evident. Solid solution between metals has been
found to be exceedingly common, many alloys being of this character. A
case of this kind was observed by Cooke and described in the Journal (20,
222, 1855). He prepared two well-crystallized compounds of zinc and
antimony to which he gave the formulas Zn3Sb and Zn2Sb, but he observed
that excellent crystals of each could be obtained which varied largely in
composition from these formulas. As the two compounds were dissimilar in
their formulas and crystalline forms, Cooke assumed that isomorphism was
impossible and concluded “that it is due to an actual perturbation of the law
of definite proportions, produced by the influence of mass.” We should now
regard this as a case of solid solution.
Page 329
A Lack of Confidence in Avogadro’s Principle.—One reason why
chemists were so slow in arriving at the correct atomic weights and
formulas was a partial loss of confidence in Avogadro’s principle. About
1826 the young French chemist Dumas devised an excellent method for the
determination of vapor densities at high temperatures, and his results and
those of others showed some discrepancies in the expected densities. For
example, the vapor density of sulphur was found to be about three times too
great, that of phosphorus twice too great, that of mercury vapor and that of
ammonium chloride only about half large enough to correspond to the
values expected from analogy and other considerations. Thus, one volume
of oxygen with two volumes of hydrogen make two volumes of steam, but
only one third of a volume of sulphur vapor was found to unite with two
volumes of hydrogen to make two volumes of hydrogen sulphide. Berzelius
saw clearly that the results pointed to the existence of such molecules as S6,
P4, and Hg1, but it was not generally realized in those days that Avogadro’s
rule is fundamentally reliable, and Berzelius himself appears to have lost
confidence in it on account of these complications, for he did not apply
Avogadro’s principle to decisions about atomic weights, except in the cases
of substances gaseous at ordinary temperatures.
Electro-chemical Theories.—The observation was made by Nicholson
and Carlisle in 1800 that water was decomposed into its constituent gases
by the electric current. Then in 1803 Berzelius and Hisinger found that salts
were decomposed into their bases and acids by the same agency, and in
1807 Davy isolated potassium, sodium, and other metals afterwards, by a
similar decomposition. Since those early times a vast amount of attention
has been paid to the relation of electricity to chemical changes, a relation
that is evidently of great importance from the fact that while electric
currents decompose chemical compounds, these currents, on the other hand,
are produced by chemical reactions.
Berzelius was particularly prominent in this direction, and in 1819 he
published an elaborate electro-chemical theory. He believed that atoms were
electrically polarized, and that this was the cause of their combination with
one another. He extended this idea to groups of atoms, particularly to
oxides, and regarded these groups as positive or negative, according to the
excess of positive or negative electricity derived from their constituent
atoms and remaining free. He thus arrived at his dualistic theory of
chemists were so slow in arriving at the correct atomic weights and
formulas was a partial loss of confidence in Avogadro’s principle. About
1826 the young French chemist Dumas devised an excellent method for the
determination of vapor densities at high temperatures, and his results and
those of others showed some discrepancies in the expected densities. For
example, the vapor density of sulphur was found to be about three times too
great, that of phosphorus twice too great, that of mercury vapor and that of
ammonium chloride only about half large enough to correspond to the
values expected from analogy and other considerations. Thus, one volume
of oxygen with two volumes of hydrogen make two volumes of steam, but
only one third of a volume of sulphur vapor was found to unite with two
volumes of hydrogen to make two volumes of hydrogen sulphide. Berzelius
saw clearly that the results pointed to the existence of such molecules as S6,
P4, and Hg1, but it was not generally realized in those days that Avogadro’s
rule is fundamentally reliable, and Berzelius himself appears to have lost
confidence in it on account of these complications, for he did not apply
Avogadro’s principle to decisions about atomic weights, except in the cases
of substances gaseous at ordinary temperatures.
Electro-chemical Theories.—The observation was made by Nicholson
and Carlisle in 1800 that water was decomposed into its constituent gases
by the electric current. Then in 1803 Berzelius and Hisinger found that salts
were decomposed into their bases and acids by the same agency, and in
1807 Davy isolated potassium, sodium, and other metals afterwards, by a
similar decomposition. Since those early times a vast amount of attention
has been paid to the relation of electricity to chemical changes, a relation
that is evidently of great importance from the fact that while electric
currents decompose chemical compounds, these currents, on the other hand,
are produced by chemical reactions.
Berzelius was particularly prominent in this direction, and in 1819 he
published an elaborate electro-chemical theory. He believed that atoms were
electrically polarized, and that this was the cause of their combination with
one another. He extended this idea to groups of atoms, particularly to
oxides, and regarded these groups as positive or negative, according to the
excess of positive or negative electricity derived from their constituent
atoms and remaining free. He thus arrived at his dualistic theory of
Page 330
chemical compounds, which attained great prominence and prevailed for a
long time in chemical theory. According to this idea, each compound was
supposed to be made up of a positive and a negative atom or group of
atoms. For example, the formulas for potassium nitrate, calcium carbonate,
and sulphuric acid corresponded to K2O.N2O5, CaO.CO2 and H2O.SO3
where we now write KNO3, CaCO3 and H2SO4, and the theory was
extended to embrace organic compounds also.
The eminent English chemist and physicist Faraday announced the
important law of electro-chemical equivalents in 1834. This law shows that
the quantities of elements set free by the passage of a given quantity of
electricity through their solutions correspond to the chemical equivalents of
those elements. Faraday made a table of the equivalents of a number of
elements, regarding them important in connection with atomic weights, but
at that time no sharp distinction was usually made between equivalents and
atomic weights, and it was not fully realized that one atom of a given
element may be the electrical equivalent of several atoms of another.
Faraday’s law, which is still regarded as fundamentally exact, has been of
much practical use in the measurement of electric currents and in
calculations connected with electro-chemical processes. In discussing his
experiments, Faraday made use of several new terms, such as “electrolyte”
for a substance which conducts electricity when in solution, and is thus
“electrolyzed,” “electrode,” “anode,” and “cathode,” terms that have come
into general use, and finally “ions” for the particles that were supposed to
“wander” towards the electrodes to be set free there.
This term “ion” remained in comparative obscurity for more than half a
century, when it was brought into great prominence among chemists by
Arrhenius in connection with the ionic theory.
Cannizzaro’s Ideas.—Up to about 1869 chaos reigned among the
formulas used by different chemists. Various compound radicals and
numerous type-formulas were employed, dualistic and unitary formulas of
several kinds were in use, but the worst feature of the situation was the fact
that more than one system of atomic weights was in vogue, so that water
might be written
HO, H̶O, or H20
long time in chemical theory. According to this idea, each compound was
supposed to be made up of a positive and a negative atom or group of
atoms. For example, the formulas for potassium nitrate, calcium carbonate,
and sulphuric acid corresponded to K2O.N2O5, CaO.CO2 and H2O.SO3
where we now write KNO3, CaCO3 and H2SO4, and the theory was
extended to embrace organic compounds also.
The eminent English chemist and physicist Faraday announced the
important law of electro-chemical equivalents in 1834. This law shows that
the quantities of elements set free by the passage of a given quantity of
electricity through their solutions correspond to the chemical equivalents of
those elements. Faraday made a table of the equivalents of a number of
elements, regarding them important in connection with atomic weights, but
at that time no sharp distinction was usually made between equivalents and
atomic weights, and it was not fully realized that one atom of a given
element may be the electrical equivalent of several atoms of another.
Faraday’s law, which is still regarded as fundamentally exact, has been of
much practical use in the measurement of electric currents and in
calculations connected with electro-chemical processes. In discussing his
experiments, Faraday made use of several new terms, such as “electrolyte”
for a substance which conducts electricity when in solution, and is thus
“electrolyzed,” “electrode,” “anode,” and “cathode,” terms that have come
into general use, and finally “ions” for the particles that were supposed to
“wander” towards the electrodes to be set free there.
This term “ion” remained in comparative obscurity for more than half a
century, when it was brought into great prominence among chemists by
Arrhenius in connection with the ionic theory.
Cannizzaro’s Ideas.—Up to about 1869 chaos reigned among the
formulas used by different chemists. Various compound radicals and
numerous type-formulas were employed, dualistic and unitary formulas of
several kinds were in use, but the worst feature of the situation was the fact
that more than one system of atomic weights was in vogue, so that water
might be written
HO, H̶O, or H20
Page 331
and similar discrepancies might appear in nearly all formulas containing
elements of different valencies. In 1858, however, an article by the Italian
chemist Cannizzaro appeared in which the outlines of a course in chemical
philosophy were presented. This acquired wide circulation in the form of a
pamphlet at a chemical convention somewhat later, and it dealt so clearly
and ably with Avogadro’s principle, Dulong and Petit’s law, and other
points in connection with formulas that it led to a rapid and almost universal
reform among those who were using unsatisfactory formulas.
At about this time also the dualistic formulas of Berzelius were generally
abandoned, and hydrogen came to be regarded as the characteristic element
of all acids. For instance, CaO.SO3, called “sulphate of lime,” came to be
written CaSO4 and was called “calcium sulphate,” and while it had been
shown as early as 1815 by Davy that “iodic acid,” I2O5, showed no acid
reaction until it was combined with water, the accumulation of similar facts
led to the formulation of sulphuric acid as H2SO4 instead of SO3 or
H2O.SO3, and that of other “oxygen acids” in a similar way. As a necessary
consequence of this view of acids, the bases came to be regarded as
compounds of the “hydroxyl” group, OH. Therefore the formula for caustic
soda came to be written NaOH instead of Na2O.H2O, and so on.
The Periodic System of the Elements.—The periodicity of the elements in
connection with their atomic weights was roughly grasped by Newlands in
England, who announced his “law of octaves” in 1863. This was at the time
when the atomic weights were being modified and their numerical relations
properly shown. The subject was worked out more fully by L. Meyer in
Germany a little later, but it was most clearly and elaborately presented by
the Russian chemist Mendeléeff in 1869.
In order that this subject may be explained to some extent Mendeléeff’s
table is given here, with the addition of the recently discovered elements
and some other modifications.
elements of different valencies. In 1858, however, an article by the Italian
chemist Cannizzaro appeared in which the outlines of a course in chemical
philosophy were presented. This acquired wide circulation in the form of a
pamphlet at a chemical convention somewhat later, and it dealt so clearly
and ably with Avogadro’s principle, Dulong and Petit’s law, and other
points in connection with formulas that it led to a rapid and almost universal
reform among those who were using unsatisfactory formulas.
At about this time also the dualistic formulas of Berzelius were generally
abandoned, and hydrogen came to be regarded as the characteristic element
of all acids. For instance, CaO.SO3, called “sulphate of lime,” came to be
written CaSO4 and was called “calcium sulphate,” and while it had been
shown as early as 1815 by Davy that “iodic acid,” I2O5, showed no acid
reaction until it was combined with water, the accumulation of similar facts
led to the formulation of sulphuric acid as H2SO4 instead of SO3 or
H2O.SO3, and that of other “oxygen acids” in a similar way. As a necessary
consequence of this view of acids, the bases came to be regarded as
compounds of the “hydroxyl” group, OH. Therefore the formula for caustic
soda came to be written NaOH instead of Na2O.H2O, and so on.
The Periodic System of the Elements.—The periodicity of the elements in
connection with their atomic weights was roughly grasped by Newlands in
England, who announced his “law of octaves” in 1863. This was at the time
when the atomic weights were being modified and their numerical relations
properly shown. The subject was worked out more fully by L. Meyer in
Germany a little later, but it was most clearly and elaborately presented by
the Russian chemist Mendeléeff in 1869.
In order that this subject may be explained to some extent Mendeléeff’s
table is given here, with the addition of the recently discovered elements
and some other modifications.
Page 332
Note.—Distinctions in printing: Gaseous elements. Other non-metallic elements, metallic
elements. The heavy line encloses approximately the acid-forming elements.
In this table the elements arranged in the order of their atomic weights
fall into eight groups where the known oxides progress regularly, with the
exception of two or three elements, from R2O in Group I to R2O7 in Group
VII, while in Group VIII two oxides (of ruthenium and osmium) are known
which carry the progression to RO4.
It was pointed out by Mendeléeff that, with the exception of series 1 and
2 at the top of the table, the alternate members of the groups show
particularly close relationships. These subordinate groups, marked A and B,
in most cases show remarkable analogies and gradations in their properties,
for example, in the alkali-metals from lithium to cæsium, and in the
halogens from fluorine to iodine. The two divisions of a group do not
usually show very close relations to each other, except in their valency, and
they even display, in several instances, opposite gradations in chemical
activity in the order of their atomic weights. For instance, cæsium stands at
the electro-positive end, while gold stands at the electro-negative end of its
subordinate group. The difference between the two divisions is very great in
Groups VI and VII, but it is extreme in Group VIII, where heavy metals are
elements. The heavy line encloses approximately the acid-forming elements.
In this table the elements arranged in the order of their atomic weights
fall into eight groups where the known oxides progress regularly, with the
exception of two or three elements, from R2O in Group I to R2O7 in Group
VII, while in Group VIII two oxides (of ruthenium and osmium) are known
which carry the progression to RO4.
It was pointed out by Mendeléeff that, with the exception of series 1 and
2 at the top of the table, the alternate members of the groups show
particularly close relationships. These subordinate groups, marked A and B,
in most cases show remarkable analogies and gradations in their properties,
for example, in the alkali-metals from lithium to cæsium, and in the
halogens from fluorine to iodine. The two divisions of a group do not
usually show very close relations to each other, except in their valency, and
they even display, in several instances, opposite gradations in chemical
activity in the order of their atomic weights. For instance, cæsium stands at
the electro-positive end, while gold stands at the electro-negative end of its
subordinate group. The difference between the two divisions is very great in
Groups VI and VII, but it is extreme in Group VIII, where heavy metals are
Page 333
on one side and inactive gases on the other. Many authorities separate these
gases into a “Group O” by themselves at the left-hand side of the table, but
this does not change their relative positions, and the plan may be objected
to on the ground that many vacant places are thus left in the groups VIII and
O.
The periodic law has been useful in rectifying certain atomic weights. At
the outset Mendeléeff was obliged to change beryllium from 14·5
(assuming Be2O3) to 9 (assuming BeO), and later the atomic weights of
indium and uranium were changed to make them fit the system. All of these
changes have been confirmed by physical means.
Mendeléeff found a number of vacant places in his table, and was thus
able to render further service to chemical science by predicting the
properties of undiscovered elements, and his predictions were very closely
confirmed by the later discovery of scandium, gallium, and germanium. The
table indicates that there are still two undiscovered elements below
manganese and probably two more among the rare-earth metals. The
interesting observation has just recently been made by Soddy that the
products of radioactive disintegration appear to pass in a symmetrical way
through positions in the periodic system, giving off a helium molecule at
alternate transformations until the place of lead is reached. It appears,
therefore, that the five vacant places in the table above bismuth are
probably occupied by these evanescent elements, and it is to be noticed that
all of the elements that have been placed in this region of high atomic
weights are radioactive.
There are some inconsistencies in the periodic system. The increments in
the atomic weights are irregular, and there are three cases, argon and
potassium, cobalt and nickel, and tellurium and iodine, where a higher
atomic weight is placed before a lower one in order to bring these elements
into their undoubtedly proper places. There is a peculiarity also in the
heavy-metal division of Group VIII, where three similar elements occur in
each of three places, and where the usual periodicity appears to be
suspended, or nearly so, in comparison with most of the other elements.
However, there seems to be a still more remarkable case of this kind in
Group III, where fourteen metals of the rare earths have been placed. They
are astonishingly similar in their chemical properties, hence it seems
necessary to assume that periodicity is suspended here throughout the wide
gases into a “Group O” by themselves at the left-hand side of the table, but
this does not change their relative positions, and the plan may be objected
to on the ground that many vacant places are thus left in the groups VIII and
O.
The periodic law has been useful in rectifying certain atomic weights. At
the outset Mendeléeff was obliged to change beryllium from 14·5
(assuming Be2O3) to 9 (assuming BeO), and later the atomic weights of
indium and uranium were changed to make them fit the system. All of these
changes have been confirmed by physical means.
Mendeléeff found a number of vacant places in his table, and was thus
able to render further service to chemical science by predicting the
properties of undiscovered elements, and his predictions were very closely
confirmed by the later discovery of scandium, gallium, and germanium. The
table indicates that there are still two undiscovered elements below
manganese and probably two more among the rare-earth metals. The
interesting observation has just recently been made by Soddy that the
products of radioactive disintegration appear to pass in a symmetrical way
through positions in the periodic system, giving off a helium molecule at
alternate transformations until the place of lead is reached. It appears,
therefore, that the five vacant places in the table above bismuth are
probably occupied by these evanescent elements, and it is to be noticed that
all of the elements that have been placed in this region of high atomic
weights are radioactive.
There are some inconsistencies in the periodic system. The increments in
the atomic weights are irregular, and there are three cases, argon and
potassium, cobalt and nickel, and tellurium and iodine, where a higher
atomic weight is placed before a lower one in order to bring these elements
into their undoubtedly proper places. There is a peculiarity also in the
heavy-metal division of Group VIII, where three similar elements occur in
each of three places, and where the usual periodicity appears to be
suspended, or nearly so, in comparison with most of the other elements.
However, there seems to be a still more remarkable case of this kind in
Group III, where fourteen metals of the rare earths have been placed. They
are astonishingly similar in their chemical properties, hence it seems
necessary to assume that periodicity is suspended here throughout the wide
Page 334
range of atomic weights from 139 to 174, where no elements save these
have been found.
Several other interesting features of the table may be pointed out. The
chlorides and hydrides, as indicated by the “typical compounds,” show a
regular progression in both directions towards Group IV. (Where the type-
formulas do not apply, as far as is known, to more than one or two
elements, they have been placed in parentheses in the table given here.) It is
a striking fact that the acid-forming elements occur together in a definite
part of the table, and that the gases and other non-metallic elements, except
the inactive gases of Group VIII, occur in the same region.
Atomic Numbers.—As the result of a spectroscopic study of the wave
lengths or frequencies of the X-rays produced when cathode rays strike
upon anticathodes composed of different elements, Moseley in 1914
discovered that whole numbers in a simple series can be attributed to the
atoms. These atomic numbers are: 1 for hydrogen, 2 for helium, 3 for
lithium, 4 for beryllium, and so on, in the order in which the elements occur
in Mendeléeff’s periodic table, and in the cases of argon and potassium,
cobalt and nickel, and tellurium and iodine, they follow the correct
chemical order, while the atomic weights do not. They appear to indicate,
therefore, an even more fundamental relation between the atoms than that
shown by the atomic weights.
These numbers are now available for every element up to lead, and they
are particularly interesting in indicating, on account of missing numbers,
the existence of two undiscovered elements in the manganese group, and
two more among the rare-earth metals, in confirmation of the vacant places
below lead in Mendeléeff’s table.
The Isolation of Elements.—In the year 1818 about 53 elements were
recognized, and since that time about 30 more have been discovered, but
the elements already known comprised the more common ones, and nearly
all of those which have been commercially important. A few of them,
including beryllium, aluminium, silicon, magnesium, and fluorine, were
then known only in their compounds, as they had not yet been isolated in
the free condition.
Berzelius in 1823 prepared silicon, a non-metallic element resembling
carbon in many respects. This element has recently been prepared on a
have been found.
Several other interesting features of the table may be pointed out. The
chlorides and hydrides, as indicated by the “typical compounds,” show a
regular progression in both directions towards Group IV. (Where the type-
formulas do not apply, as far as is known, to more than one or two
elements, they have been placed in parentheses in the table given here.) It is
a striking fact that the acid-forming elements occur together in a definite
part of the table, and that the gases and other non-metallic elements, except
the inactive gases of Group VIII, occur in the same region.
Atomic Numbers.—As the result of a spectroscopic study of the wave
lengths or frequencies of the X-rays produced when cathode rays strike
upon anticathodes composed of different elements, Moseley in 1914
discovered that whole numbers in a simple series can be attributed to the
atoms. These atomic numbers are: 1 for hydrogen, 2 for helium, 3 for
lithium, 4 for beryllium, and so on, in the order in which the elements occur
in Mendeléeff’s periodic table, and in the cases of argon and potassium,
cobalt and nickel, and tellurium and iodine, they follow the correct
chemical order, while the atomic weights do not. They appear to indicate,
therefore, an even more fundamental relation between the atoms than that
shown by the atomic weights.
These numbers are now available for every element up to lead, and they
are particularly interesting in indicating, on account of missing numbers,
the existence of two undiscovered elements in the manganese group, and
two more among the rare-earth metals, in confirmation of the vacant places
below lead in Mendeléeff’s table.
The Isolation of Elements.—In the year 1818 about 53 elements were
recognized, and since that time about 30 more have been discovered, but
the elements already known comprised the more common ones, and nearly
all of those which have been commercially important. A few of them,
including beryllium, aluminium, silicon, magnesium, and fluorine, were
then known only in their compounds, as they had not yet been isolated in
the free condition.
Berzelius in 1823 prepared silicon, a non-metallic element resembling
carbon in many respects. This element has recently been prepared on a
Page 335
rather large scale in electric furnaces at Niagara Falls, and has been used for
certain purposes in the form of castings.
Wöhler created much sensation in 1827 by isolating aluminium and
finding it to be a very light, strong and malleable metal, stable in the air,
and of a silver-white color. For a long time this metal was a comparative
rarity, being prepared by the reduction of aluminium chloride with metallic
sodium; but about 25 years ago Hall, an American, devised a method of
preparing it by electrolyzing aluminium oxide dissolved in fused cryolite.
This process reduced the cost of aluminium to such an extent that it has
now come into common use.
Wöhler and Bussy prepared beryllium in 1828, and Liebig and Bussy did
the same service for magnesium in 1830. The latter metal has come to be of
much practical importance, both as a very powerful reducing agent in
chemical operations, and as an ingredient of flash-light powders and of
mixtures used for fireworks. It is also used in making certain light alloys.
After almost innumerable attempts to isolate fluorine, during a period of
nearly a century, this was finally accomplished in 1886 by Moissan in
France by the electrolysis of anhydrous hydrogen fluoride. The free fluorine
proved to be a gas of extraordinary chemical activity, decomposing water at
once with the formation of hydrogen fluoride and ozonized oxygen. This
fact explains the failure of many previous attempts to prepare it in the
presence of water.
Early Discoveries of New Elements.—The remarkable activity of
chemical research at the beginning of our period is illustrated by the fact
that three new elements were discovered in 1817. In that year Berzelius had
discovered selenium, Arfvedson, working in Berzelius’s laboratory had
discovered the important alkali-metal lithium, and Stromeyer had
discovered cadmium.
In 1826 Ballard in France discovered bromine in the mother-liquor from
the crystallization of common salt from sea water. Bromine proved to be an
unusually interesting element, being the only non-metallic one that is liquid
at ordinary temperatures, and being strikingly intermediate in its properties
between chlorine and iodine. It has been obtained in large quantities from
brines, and is produced extensively in the United States. The elementary
substance and its compounds have found important applications in chemical
certain purposes in the form of castings.
Wöhler created much sensation in 1827 by isolating aluminium and
finding it to be a very light, strong and malleable metal, stable in the air,
and of a silver-white color. For a long time this metal was a comparative
rarity, being prepared by the reduction of aluminium chloride with metallic
sodium; but about 25 years ago Hall, an American, devised a method of
preparing it by electrolyzing aluminium oxide dissolved in fused cryolite.
This process reduced the cost of aluminium to such an extent that it has
now come into common use.
Wöhler and Bussy prepared beryllium in 1828, and Liebig and Bussy did
the same service for magnesium in 1830. The latter metal has come to be of
much practical importance, both as a very powerful reducing agent in
chemical operations, and as an ingredient of flash-light powders and of
mixtures used for fireworks. It is also used in making certain light alloys.
After almost innumerable attempts to isolate fluorine, during a period of
nearly a century, this was finally accomplished in 1886 by Moissan in
France by the electrolysis of anhydrous hydrogen fluoride. The free fluorine
proved to be a gas of extraordinary chemical activity, decomposing water at
once with the formation of hydrogen fluoride and ozonized oxygen. This
fact explains the failure of many previous attempts to prepare it in the
presence of water.
Early Discoveries of New Elements.—The remarkable activity of
chemical research at the beginning of our period is illustrated by the fact
that three new elements were discovered in 1817. In that year Berzelius had
discovered selenium, Arfvedson, working in Berzelius’s laboratory had
discovered the important alkali-metal lithium, and Stromeyer had
discovered cadmium.
In 1826 Ballard in France discovered bromine in the mother-liquor from
the crystallization of common salt from sea water. Bromine proved to be an
unusually interesting element, being the only non-metallic one that is liquid
at ordinary temperatures, and being strikingly intermediate in its properties
between chlorine and iodine. It has been obtained in large quantities from
brines, and is produced extensively in the United States. The elementary
substance and its compounds have found important applications in chemical
Page 336
operations, while the bromides have been found valuable in medicine and
silver bromide is very extensively used in photography.
In 1828 Berzelius discovered thorium. The oxide of this metal has
recently been employed extensively as the principal constituent of
incandescent gas-mantles, and the element has acquired particular
importance from the fact that, like uranium, it is radioactive, decomposing
spontaneously into other elements.
Vanadium had been encountered as early as 1801 by Del Rio, who named
it “erythronium,” but a little later it was thought to be identical with
chromium and was lost sight of for a while. In 1830, however, it was re-
discovered by, and received its present name from Sefström in Sweden.
Berzelius immediately made an extensive study of vanadium compounds,
but he gave them incorrect formulas and derived an incorrect atomic weight
for the element, because he mistook a lower oxide for the element itself.
Roscoe in England in 1867 isolated vanadium for the first time, found the
right atomic weight, and gave correct formulas to its compounds. Vanadium
is particularly interesting from the fact that it displays several valencies in
its compounds, many of which are highly colored. It has found important
use as an ingredient in very small proportions in certain “special steels” to
which it imparts a high degree of resistance to rupture by repeated shocks.
Columbium was discovered early in the nineteenth century in the mineral
columbite from Connecticut by Hatchett, an Englishman, who did not,
however, obtain the pure oxide. It was afterwards obtained by Rose who
named it niobium. Both names for the element are in use, but the former has
priority. Attention was called to this fact by an article in the Journal by
Connell, an Englishman (18, 392, 1854).
The Platinum Group of Metals.—In 1854 a new member of the platinum
group of metals, ruthenium, was discovered by Claus. Platinum had been
discovered about the middle of the eighteenth century, while its other rarer
associates, iridium, osmium, palladium, and rhodium, had been recognized
in the very early years of the nineteenth century. It was during the latter
period that platinum ware began to be employed to a considerable extent in
chemical operations, and this use was greatly extended as time went on. The
discovery was made by Phillips in 1831 that finely divided platinum by
contact would bring about the combination of sulphur dioxide with
atmospheric oxygen, and this application during the past 20 years has
silver bromide is very extensively used in photography.
In 1828 Berzelius discovered thorium. The oxide of this metal has
recently been employed extensively as the principal constituent of
incandescent gas-mantles, and the element has acquired particular
importance from the fact that, like uranium, it is radioactive, decomposing
spontaneously into other elements.
Vanadium had been encountered as early as 1801 by Del Rio, who named
it “erythronium,” but a little later it was thought to be identical with
chromium and was lost sight of for a while. In 1830, however, it was re-
discovered by, and received its present name from Sefström in Sweden.
Berzelius immediately made an extensive study of vanadium compounds,
but he gave them incorrect formulas and derived an incorrect atomic weight
for the element, because he mistook a lower oxide for the element itself.
Roscoe in England in 1867 isolated vanadium for the first time, found the
right atomic weight, and gave correct formulas to its compounds. Vanadium
is particularly interesting from the fact that it displays several valencies in
its compounds, many of which are highly colored. It has found important
use as an ingredient in very small proportions in certain “special steels” to
which it imparts a high degree of resistance to rupture by repeated shocks.
Columbium was discovered early in the nineteenth century in the mineral
columbite from Connecticut by Hatchett, an Englishman, who did not,
however, obtain the pure oxide. It was afterwards obtained by Rose who
named it niobium. Both names for the element are in use, but the former has
priority. Attention was called to this fact by an article in the Journal by
Connell, an Englishman (18, 392, 1854).
The Platinum Group of Metals.—In 1854 a new member of the platinum
group of metals, ruthenium, was discovered by Claus. Platinum had been
discovered about the middle of the eighteenth century, while its other rarer
associates, iridium, osmium, palladium, and rhodium, had been recognized
in the very early years of the nineteenth century. It was during the latter
period that platinum ware began to be employed to a considerable extent in
chemical operations, and this use was greatly extended as time went on. The
discovery was made by Phillips in 1831 that finely divided platinum by
contact would bring about the combination of sulphur dioxide with
atmospheric oxygen, and this application during the past 20 years has
Page 337
become enormously important in the sulphuric acid industry, while other
important applications of platinum as a “catalytic agent” have also been
made. Wolcott Gibbs and Carey Lea have contributed perhaps more than
any other recent chemists to a knowledge of the platinum metals. Carey Lea
(38, 81, 248, 1864) dealt chiefly with the separation of the metals from each
other, while Gibbs’s work (31, 63, 1861; 34, 341, 1862) included
investigations of many of the compounds.
It may be mentioned that while platinum and its associates were formerly
known only in the uncombined condition in nature, the arsenide sperrylite,
PtAs2, was described by the late S. L. Penfield, and the senior writer of this
chapter, in articles published in the Journal (37, 67, 71, 1889).
Applications of the Spectroscope.—The discovery in certain mineral
waters of the rare alkali-metals rubidium and cæsium by Bunsen and
Kirchoff in 1861 was in consequence of the application of spectroscopy by
these same scientists a short time previously to the identification of
elements imparting colors to the flame. Since that time the employment of
the spectroscope for chemical purposes has been much extended, as it has
been used in the examination of light from electric sparks and arcs, as well
as from Geissler tube discharges and from colored solutions.
The metals rubidium and cæsium are interesting in being closely
analogous to potassium and in standing at the extreme electro-positive end
of the series of known metals. It should be noticed here that Johnson and
Allen of our Sheffield Laboratory, having obtained a good supply of
rubidium and cæsium material from the lepidolite of Hebron, Maine, made
some important researches upon these elements, accounts of which were
published in the Journal (34, 367, 1862; 35, 94, 1863). They established the
atomic weight of cæsium, thus correcting Bunsen’s determination which
was unsatisfactory on account of the small quantity and impurity of his
material. Pollucite, a mineral rich in cæsium, which had been found in very
small amount on the Island of Elba, has more recently been obtained in
large quantities—hundreds of pounds—at Paris, Maine, and its vicinity.
This American pollucite was first analyzed and identified by the senior
writer of this article (41, 213, 1891), and later (43, 17, 1892 et seq.) the
results of many investigations on cæsium and rubidium compounds, in
which the junior writer played an important part, carried out in Sheffield
Laboratory, were published in the Journal.
important applications of platinum as a “catalytic agent” have also been
made. Wolcott Gibbs and Carey Lea have contributed perhaps more than
any other recent chemists to a knowledge of the platinum metals. Carey Lea
(38, 81, 248, 1864) dealt chiefly with the separation of the metals from each
other, while Gibbs’s work (31, 63, 1861; 34, 341, 1862) included
investigations of many of the compounds.
It may be mentioned that while platinum and its associates were formerly
known only in the uncombined condition in nature, the arsenide sperrylite,
PtAs2, was described by the late S. L. Penfield, and the senior writer of this
chapter, in articles published in the Journal (37, 67, 71, 1889).
Applications of the Spectroscope.—The discovery in certain mineral
waters of the rare alkali-metals rubidium and cæsium by Bunsen and
Kirchoff in 1861 was in consequence of the application of spectroscopy by
these same scientists a short time previously to the identification of
elements imparting colors to the flame. Since that time the employment of
the spectroscope for chemical purposes has been much extended, as it has
been used in the examination of light from electric sparks and arcs, as well
as from Geissler tube discharges and from colored solutions.
The metals rubidium and cæsium are interesting in being closely
analogous to potassium and in standing at the extreme electro-positive end
of the series of known metals. It should be noticed here that Johnson and
Allen of our Sheffield Laboratory, having obtained a good supply of
rubidium and cæsium material from the lepidolite of Hebron, Maine, made
some important researches upon these elements, accounts of which were
published in the Journal (34, 367, 1862; 35, 94, 1863). They established the
atomic weight of cæsium, thus correcting Bunsen’s determination which
was unsatisfactory on account of the small quantity and impurity of his
material. Pollucite, a mineral rich in cæsium, which had been found in very
small amount on the Island of Elba, has more recently been obtained in
large quantities—hundreds of pounds—at Paris, Maine, and its vicinity.
This American pollucite was first analyzed and identified by the senior
writer of this article (41, 213, 1891), and later (43, 17, 1892 et seq.) the
results of many investigations on cæsium and rubidium compounds, in
which the junior writer played an important part, carried out in Sheffield
Laboratory, were published in the Journal.
Page 338
The application of the spectroscope led to the discovery of thallium in
1861 by Crookes of England, and to that of indium in 1863 by Reich and
Richter in Germany. Both of these metals are extremely rare, but they are of
considerable theoretical interest. Thallium is particularly remarkable in
showing resemblances in its different compounds to several groups of
metals.
The spectroscope was employed again in connection with the discovery
of gallium in 1875 by Boisbaudran. It is in the same periodic group as
thallium and indium, and it has a remarkably low melting point, just above
ordinary room-temperature. It has been among the rarest of the rare
elements, but within two or three years a source of it has been found in the
United States in certain residues from the refining of commercial zinc. The
recent issues of the Journal (41, 351, 1916; 42, 389, 1916) show that
Browning and Uhler of Yale have availed themselves of this new material in
order to make important chemical and physical researches upon this metal.
Germanium.—The discovery of germanium in the mineral argyrodite in
1886 by Winkler revealed a curious metal which gives a white sulphide that
may be easily mistaken for sulphur and which is volatilized completely
when its hydrochloric acid solution is evaporated, so that it is evasive in
analytical operations. This element had been predicted with much accuracy
by Mendeléeff, and it is rather closely related to tin.
A few years after the discovery of germanium, Penfield published in the
Journal (46, 107, 1893; 47, 451, 1894) some analyses of argyrodite,
correcting the formula given by Winkler to the mineral; also he described
canfieldite, an analogous mineral from Bolivia, in which a large part of the
germanium was replaced by tin.
The Rare Earths.—Before the year 1818 two rare earths, the oxides of
yttrium and cerium, were known in an impure condition. Since that time
about fourteen others have been discovered as associates of the first two.
The rare earths are peculiar from the fact that many of them are always
found mixed together in the minerals containing them, and also from the
circumstance that most of them are remarkably similar in their chemical
reactions and consequently exceedingly difficult to separate from each
other. In many cases multitudes of fractional precipitations or
crystallizations are needed to obtain pure salts of a number of these metals.
The solutions of the salts of several of these elements give characteristic
1861 by Crookes of England, and to that of indium in 1863 by Reich and
Richter in Germany. Both of these metals are extremely rare, but they are of
considerable theoretical interest. Thallium is particularly remarkable in
showing resemblances in its different compounds to several groups of
metals.
The spectroscope was employed again in connection with the discovery
of gallium in 1875 by Boisbaudran. It is in the same periodic group as
thallium and indium, and it has a remarkably low melting point, just above
ordinary room-temperature. It has been among the rarest of the rare
elements, but within two or three years a source of it has been found in the
United States in certain residues from the refining of commercial zinc. The
recent issues of the Journal (41, 351, 1916; 42, 389, 1916) show that
Browning and Uhler of Yale have availed themselves of this new material in
order to make important chemical and physical researches upon this metal.
Germanium.—The discovery of germanium in the mineral argyrodite in
1886 by Winkler revealed a curious metal which gives a white sulphide that
may be easily mistaken for sulphur and which is volatilized completely
when its hydrochloric acid solution is evaporated, so that it is evasive in
analytical operations. This element had been predicted with much accuracy
by Mendeléeff, and it is rather closely related to tin.
A few years after the discovery of germanium, Penfield published in the
Journal (46, 107, 1893; 47, 451, 1894) some analyses of argyrodite,
correcting the formula given by Winkler to the mineral; also he described
canfieldite, an analogous mineral from Bolivia, in which a large part of the
germanium was replaced by tin.
The Rare Earths.—Before the year 1818 two rare earths, the oxides of
yttrium and cerium, were known in an impure condition. Since that time
about fourteen others have been discovered as associates of the first two.
The rare earths are peculiar from the fact that many of them are always
found mixed together in the minerals containing them, and also from the
circumstance that most of them are remarkably similar in their chemical
reactions and consequently exceedingly difficult to separate from each
other. In many cases multitudes of fractional precipitations or
crystallizations are needed to obtain pure salts of a number of these metals.
The solutions of the salts of several of these elements give characteristic
Page 339
absorption bands when examined spectroscopically by the use of
transmitted light.
No important practical application has been found for any of these earthy
oxides, except that about one per cent of cerium oxide is mixed with
thorium oxide in incandescent gas-mantles in order to obtain greatly
increased luminosity.
The Inactive Gases.—As long ago as 1785, Cavendish, that remarkable
Englishman who first weighed the world and first discovered the
composition of water, actually obtained a little argon in a pure condition by
sparking atmospheric nitrogen with oxygen converting it into nitric acid
(another discovery of his) and absorbing the excess of oxygen. The volume
of this residual gas as estimated by him corresponds very closely to the
volume of argon in the atmosphere, as now known.
It was more than a century later, in 1894, that Rayleigh and Ramsay
discovered argon in the air. Lord Rayleigh had found that atmospheric
nitrogen was about one-half per cent heavier than chemical nitrogen, a fact
which led to the investigation. It was only necessary to repeat Cavendish’s
experiment on a large scale, or to absorb oxygen with hot copper and
nitrogen with hot magnesium, in order to obtain argon. The gas attracted
much attention, both on account of having but a single atom in its molecule,
and particularly because it failed to enter into chemical combination of any
kind. This gas has been used of late for filling the bulbs of incandescent
electric lamps in cases where a gas pressure without chemical action is
desired.
In 1890 and 1891, Hillebrand published in the Journal (40, 384, 1890: 42,
390, 1891) a series of analyses of the mineral uraninite and reported in
some samples of the mineral as much as 2·5 per cent of an inactive gas.
Hillebrand examined the gas spectroscopically but, just missing an
important discovery, he detected only the spectrum lines of nitrogen.
Ramsay, in searching for argon in some sort of natural combination, and
doubtless remembering Hillebrand’s work, heated some cleveite, a variety
of uraninite, and obtained, not argon, but a new gas. This gave a yellow
spectrum-line corresponding to a line previously observed in the light of the
sun’s corona and attributed to an element in the sun called helium. Helium,
therefore, in 1895 had been found on the earth. This gas is a constant
constituent of uranium minerals, as it is produced by the breaking down of
transmitted light.
No important practical application has been found for any of these earthy
oxides, except that about one per cent of cerium oxide is mixed with
thorium oxide in incandescent gas-mantles in order to obtain greatly
increased luminosity.
The Inactive Gases.—As long ago as 1785, Cavendish, that remarkable
Englishman who first weighed the world and first discovered the
composition of water, actually obtained a little argon in a pure condition by
sparking atmospheric nitrogen with oxygen converting it into nitric acid
(another discovery of his) and absorbing the excess of oxygen. The volume
of this residual gas as estimated by him corresponds very closely to the
volume of argon in the atmosphere, as now known.
It was more than a century later, in 1894, that Rayleigh and Ramsay
discovered argon in the air. Lord Rayleigh had found that atmospheric
nitrogen was about one-half per cent heavier than chemical nitrogen, a fact
which led to the investigation. It was only necessary to repeat Cavendish’s
experiment on a large scale, or to absorb oxygen with hot copper and
nitrogen with hot magnesium, in order to obtain argon. The gas attracted
much attention, both on account of having but a single atom in its molecule,
and particularly because it failed to enter into chemical combination of any
kind. This gas has been used of late for filling the bulbs of incandescent
electric lamps in cases where a gas pressure without chemical action is
desired.
In 1890 and 1891, Hillebrand published in the Journal (40, 384, 1890: 42,
390, 1891) a series of analyses of the mineral uraninite and reported in
some samples of the mineral as much as 2·5 per cent of an inactive gas.
Hillebrand examined the gas spectroscopically but, just missing an
important discovery, he detected only the spectrum lines of nitrogen.
Ramsay, in searching for argon in some sort of natural combination, and
doubtless remembering Hillebrand’s work, heated some cleveite, a variety
of uraninite, and obtained, not argon, but a new gas. This gave a yellow
spectrum-line corresponding to a line previously observed in the light of the
sun’s corona and attributed to an element in the sun called helium. Helium,
therefore, in 1895 had been found on the earth. This gas is a constant
constituent of uranium minerals, as it is produced by the breaking down of
Page 340
radioactive elements. It has been found in very small quantity in the
atmosphere, and is the most difficult of all known gases to liquefy, as its
boiling point, as shown by Onnes in 1908, is only 4° above the absolute
zero. It has not yet been solidified.
In 1898 Ramsay and Travers, by the use of ingenious methods of
fractional distillation and absorption by charcoal, obtained three other much
rarer inactive gases from the atmosphere which they called neon, krypton
and xenon.
The inactive gases are all colorless, and as they form no chemical
compounds they are characterized by their densities, which give their
atomic weights, by their boiling points, and by their characteristic Geissler-
tube spectra.
The gaseous radium emanation, or niton, belongs also to the inactive
group, and it was also collected and studied by Ramsay who was compelled
to work with only 0·0001 cc. of it, as the volume obtained by heating
radium salts is very small. It is an evanescent element, disappearing within
a few days on account of radioactive disintegration. Meanwhile it glows
brilliantly when liquefied and cooled to the temperature of liquid air. It has
an atomic weight of 222, four units below that of radium, and the difference
is considered as due to the loss by radium of an atom of helium in passing
into the emanation.
The Radioactive Elements.—The discovery of radium in 1898 by
Madame Curie, and the study of that and other radioactive elements has
produced a profound effect upon chemical theory. It was found that the two
elements of the highest atomic weights, uranium and thorium, are always
spontaneously decomposing into other elements at a fixed rate of speed
which can be controlled by no artificial means, and that the elements
resulting from these decompositions likewise undergo spontaneous changes
into still other elements at greatly varying rates of speed, forming in each
case a remarkable series of temporary elements. These transformations are
accompanied by the emission at enormous velocities of three kinds of rays,
one variety of which has been shown to consist of helium atoms. The
greater number of the elements formed in these transformations have not as
yet been obtained in a pure condition, and they are known only in
connection with their radioactivity, volatility, etc.; but radium and niton,
atmosphere, and is the most difficult of all known gases to liquefy, as its
boiling point, as shown by Onnes in 1908, is only 4° above the absolute
zero. It has not yet been solidified.
In 1898 Ramsay and Travers, by the use of ingenious methods of
fractional distillation and absorption by charcoal, obtained three other much
rarer inactive gases from the atmosphere which they called neon, krypton
and xenon.
The inactive gases are all colorless, and as they form no chemical
compounds they are characterized by their densities, which give their
atomic weights, by their boiling points, and by their characteristic Geissler-
tube spectra.
The gaseous radium emanation, or niton, belongs also to the inactive
group, and it was also collected and studied by Ramsay who was compelled
to work with only 0·0001 cc. of it, as the volume obtained by heating
radium salts is very small. It is an evanescent element, disappearing within
a few days on account of radioactive disintegration. Meanwhile it glows
brilliantly when liquefied and cooled to the temperature of liquid air. It has
an atomic weight of 222, four units below that of radium, and the difference
is considered as due to the loss by radium of an atom of helium in passing
into the emanation.
The Radioactive Elements.—The discovery of radium in 1898 by
Madame Curie, and the study of that and other radioactive elements has
produced a profound effect upon chemical theory. It was found that the two
elements of the highest atomic weights, uranium and thorium, are always
spontaneously decomposing into other elements at a fixed rate of speed
which can be controlled by no artificial means, and that the elements
resulting from these decompositions likewise undergo spontaneous changes
into still other elements at greatly varying rates of speed, forming in each
case a remarkable series of temporary elements. These transformations are
accompanied by the emission at enormous velocities of three kinds of rays,
one variety of which has been shown to consist of helium atoms. The
greater number of the elements formed in these transformations have not as
yet been obtained in a pure condition, and they are known only in
connection with their radioactivity, volatility, etc.; but radium and niton,
Page 341
two of these products, have been obtained in a pure condition, so that their
atomic weights and their places in the periodic system have been fixed.
We owe much of our knowledge of the radioactive transformations to the
researches of Rutherford and of Soddy, and of their co-workers, but one of
the important products of the transformation of uranium, an element which
he called ionium, was characterized by Boltwood of Yale (25, 365, 1908).
Radium and niton, apart from their radioactive properties, resemble
barium and the inert gases of the atmosphere, respectively. The rates at
which their progenitors produce them, and the rates at which they
themselves decompose, bring about a state of equilibrium after a time.
Therefore a given amount of uranium, which decomposes exceedingly
slowly, can yield even after thousands of years only a very small
proportional quantity of undecomposed radium, one-half of which
disappears in about 2500 years, because the amount decomposed must
eventually be equal to the amount produced. The first conclusive evidence
that radium is a product of the decomposition of uranium was given by
Boltwood in the Journal (18, 97, 1904). He found that all uranium minerals
contain radium; and the amount of radium present is always proportional to
the amount of uranium, which shows the genetic relation between the two.
In the case of niton, which is produced by radium, and is called also the
radium emanation, the rate of decay is rapid, so that if the gas is expelled
from radium by heating, equilibrium is reached after a few days, with the
accumulation of the largest possible amount of niton.
The conclusion has been reached by Rutherford and others that the final
product besides helium, in the radioactive transformations, is lead, or at
least an element or elements resembling lead to such a degree that no
separation of them by chemical means is possible. Atomic weight
determinations by Richards and others have shown that specimens of lead
found in radioactive minerals give distinctly different atomic weights from
that of ordinary lead. This fact has led to the view that possibly the atoms of
the elements are not all of the same weight, but vary within certain limits—
a view that is contrary to previous conclusions derived from the uniformity
in atomic weights obtained with material from many different sources.
The results of the investigations upon radioactivity have led to modified
views in regard to the stability of the elements in general. There has been
little or no proof obtained that any artificial transmutation of the elements is
atomic weights and their places in the periodic system have been fixed.
We owe much of our knowledge of the radioactive transformations to the
researches of Rutherford and of Soddy, and of their co-workers, but one of
the important products of the transformation of uranium, an element which
he called ionium, was characterized by Boltwood of Yale (25, 365, 1908).
Radium and niton, apart from their radioactive properties, resemble
barium and the inert gases of the atmosphere, respectively. The rates at
which their progenitors produce them, and the rates at which they
themselves decompose, bring about a state of equilibrium after a time.
Therefore a given amount of uranium, which decomposes exceedingly
slowly, can yield even after thousands of years only a very small
proportional quantity of undecomposed radium, one-half of which
disappears in about 2500 years, because the amount decomposed must
eventually be equal to the amount produced. The first conclusive evidence
that radium is a product of the decomposition of uranium was given by
Boltwood in the Journal (18, 97, 1904). He found that all uranium minerals
contain radium; and the amount of radium present is always proportional to
the amount of uranium, which shows the genetic relation between the two.
In the case of niton, which is produced by radium, and is called also the
radium emanation, the rate of decay is rapid, so that if the gas is expelled
from radium by heating, equilibrium is reached after a few days, with the
accumulation of the largest possible amount of niton.
The conclusion has been reached by Rutherford and others that the final
product besides helium, in the radioactive transformations, is lead, or at
least an element or elements resembling lead to such a degree that no
separation of them by chemical means is possible. Atomic weight
determinations by Richards and others have shown that specimens of lead
found in radioactive minerals give distinctly different atomic weights from
that of ordinary lead. This fact has led to the view that possibly the atoms of
the elements are not all of the same weight, but vary within certain limits—
a view that is contrary to previous conclusions derived from the uniformity
in atomic weights obtained with material from many different sources.
The results of the investigations upon radioactivity have led to modified
views in regard to the stability of the elements in general. There has been
little or no proof obtained that any artificial transmutation of the elements is
Page 342
possible, but the spontaneous transformation of the radioactive elements
brings forward the possibility that other elements are changing
imperceptibly, and that a state of evolution exists among them. All of the
radioactive changes that we know proceed from higher to lower atomic
weights, and we are entirely ignorant of the process by which uranium and
thorium must have been produced originally.
Since radioactive changes have been found to be accompanied by the
release of vast amounts of energy, compared with which the energy of
chemical reactions is trivial, a new aspect in regard to the structure of atoms
has arisen,—they must be complex in structure, the seats of enormous
energy.
The determination of the amount of radium in the earth’s crust has
indicated that the heat produced by it is amply sufficient to supply the loss
of heat due to radiation, and this source of heat is regarded by many as the
cause of volcanic action. The sun’s radiant heat also has been supposed to
be supplied by radioactive action, so that the older views regarding the
limitation of the age of the earth and the solar system on account of loss of
heat have been considerably modified by our knowledge of radioactivity.
brings forward the possibility that other elements are changing
imperceptibly, and that a state of evolution exists among them. All of the
radioactive changes that we know proceed from higher to lower atomic
weights, and we are entirely ignorant of the process by which uranium and
thorium must have been produced originally.
Since radioactive changes have been found to be accompanied by the
release of vast amounts of energy, compared with which the energy of
chemical reactions is trivial, a new aspect in regard to the structure of atoms
has arisen,—they must be complex in structure, the seats of enormous
energy.
The determination of the amount of radium in the earth’s crust has
indicated that the heat produced by it is amply sufficient to supply the loss
of heat due to radiation, and this source of heat is regarded by many as the
cause of volcanic action. The sun’s radiant heat also has been supposed to
be supplied by radioactive action, so that the older views regarding the
limitation of the age of the earth and the solar system on account of loss of
heat have been considerably modified by our knowledge of radioactivity.
Page 343
Physical Chemistry.
The application of physical methods as aids to chemical science began in
early times, and some of these, such as the determinations of gas and vapor
densities, specific heats, and crystalline forms have been mentioned already
in this article. Within recent times physical chemistry has greatly developed
and a few of its important achievements will now be described.
Molecular Weight Determinations.—Gas and vapor densities in
connection with Avogadro’s principle, formed the only basis for molecular
weight determinations until comparatively recent times. The early methods
of Gay-Lussac and Dumas for vapor density were supplemented in 1868 by
the method of Hofmann, whereby vapors were measured under diminished
pressure over mercury. In 1878 Victor Meyer introduced a simpler method
depending upon the displacement of air or other gas by the vapor in a
heated tube. As refractory tubes, such as those of porcelain or even iridium,
could be used in this method, molecular weights at extremely high
temperatures were determined with interesting results. For instance, it was
found that iodine vapor, which shows the molecule I2 at lower temperatures,
gradually becomes monatomic with rise in temperature, that sulphur vapor
dissociates from S8 to S2 under similar conditions, and that most of the
metals, including silver, have monatomic vapors.
In 1883 and later it was pointed out by Raoult that the molecular weights
of substances could be found from the freezing points of their solutions, but
this method was complicated from the fact that salts, strong acids and
strong bases behaved quite differently from other substances in this respect,
and allowances had to be made for the types of substances used. The
complication was afterwards explained by the ionization theory of
Arrhenius. Better apparatus for this method was soon devised by
Beckmann, who introduced also a method depending upon the boiling
points of solutions, and these two methods are still the standard ones for
determining molecular weights in solution. They are very extensively
employed by organic chemists.
It has been found that the majority of substances when dissolved have the
same molecular weight as in the gaseous condition, provided that they can
The application of physical methods as aids to chemical science began in
early times, and some of these, such as the determinations of gas and vapor
densities, specific heats, and crystalline forms have been mentioned already
in this article. Within recent times physical chemistry has greatly developed
and a few of its important achievements will now be described.
Molecular Weight Determinations.—Gas and vapor densities in
connection with Avogadro’s principle, formed the only basis for molecular
weight determinations until comparatively recent times. The early methods
of Gay-Lussac and Dumas for vapor density were supplemented in 1868 by
the method of Hofmann, whereby vapors were measured under diminished
pressure over mercury. In 1878 Victor Meyer introduced a simpler method
depending upon the displacement of air or other gas by the vapor in a
heated tube. As refractory tubes, such as those of porcelain or even iridium,
could be used in this method, molecular weights at extremely high
temperatures were determined with interesting results. For instance, it was
found that iodine vapor, which shows the molecule I2 at lower temperatures,
gradually becomes monatomic with rise in temperature, that sulphur vapor
dissociates from S8 to S2 under similar conditions, and that most of the
metals, including silver, have monatomic vapors.
In 1883 and later it was pointed out by Raoult that the molecular weights
of substances could be found from the freezing points of their solutions, but
this method was complicated from the fact that salts, strong acids and
strong bases behaved quite differently from other substances in this respect,
and allowances had to be made for the types of substances used. The
complication was afterwards explained by the ionization theory of
Arrhenius. Better apparatus for this method was soon devised by
Beckmann, who introduced also a method depending upon the boiling
points of solutions, and these two methods are still the standard ones for
determining molecular weights in solution. They are very extensively
employed by organic chemists.
It has been found that the majority of substances when dissolved have the
same molecular weight as in the gaseous condition, provided that they can
Page 344
be volatilized at comparable temperatures. For instance, sulphur in solution
has the formula S8, iodine is I2 and the metals are monatomic.
Van’t Hoff’s Law and Arrhenius’s Theory of Ions.—Modern views on
solutions date largely from 1886, when van’t Hoff called attention to the
relations existing between the osmotic pressure exerted by dissolved
substances and gas pressure.
Pfeffer, a botanist, was the first to measure osmotic pressure (1877).
Basing his conclusions chiefly upon Pfeffer’s determinations, van’t Hoff
formulated a new and highly important law, which may be stated as
follows: The osmotic pressure exerted by a substance in solution is equal to
the gas pressure that the substance would exert if it were a gas at the same
temperature and the same volume. Further investigations have fully
established the fact that molecules in dilute solution obey the simple laws of
gases.
It was pointed out by van’t Hoff that salts, strong acids and strong bases
showed marked exceptions to his law in exerting much greater osmotic
pressures than those calculated for them.
The next year in 1887, Arrhenius explained this abnormal behavior of
salts, strong acids and strong bases by assuming that they dissociate
spontaneously into ions when they dissolve, and that these more numerous
particles act like molecules in producing osmotic pressure. He showed that
these exceptional substances all conduct electricity in solution, while those
conforming with van’t Hoff’s law do not, and according to his theory the
ions become positively or negatively charged when they are formed, and
these charged ions conduct the current. For example a molecule of sodium
chloride was supposed to give the two ions Na+ and Cl-, thus exerting twice
as much osmotic pressure as a single molecule.
Determinations of osmotic pressure or related values, such as depression
of the freezing point and of electric conductivity, indicated that ionization
could not be regarded as complete in any case except in exceedingly dilute
solutions, and that the extent of ionization varied with different substances.
The fact that osmotic pressures and electric conductivities gave closely
agreeing results in regard to the extent of ionization in various cases, is the
strongest evidence in support of the theory.
has the formula S8, iodine is I2 and the metals are monatomic.
Van’t Hoff’s Law and Arrhenius’s Theory of Ions.—Modern views on
solutions date largely from 1886, when van’t Hoff called attention to the
relations existing between the osmotic pressure exerted by dissolved
substances and gas pressure.
Pfeffer, a botanist, was the first to measure osmotic pressure (1877).
Basing his conclusions chiefly upon Pfeffer’s determinations, van’t Hoff
formulated a new and highly important law, which may be stated as
follows: The osmotic pressure exerted by a substance in solution is equal to
the gas pressure that the substance would exert if it were a gas at the same
temperature and the same volume. Further investigations have fully
established the fact that molecules in dilute solution obey the simple laws of
gases.
It was pointed out by van’t Hoff that salts, strong acids and strong bases
showed marked exceptions to his law in exerting much greater osmotic
pressures than those calculated for them.
The next year in 1887, Arrhenius explained this abnormal behavior of
salts, strong acids and strong bases by assuming that they dissociate
spontaneously into ions when they dissolve, and that these more numerous
particles act like molecules in producing osmotic pressure. He showed that
these exceptional substances all conduct electricity in solution, while those
conforming with van’t Hoff’s law do not, and according to his theory the
ions become positively or negatively charged when they are formed, and
these charged ions conduct the current. For example a molecule of sodium
chloride was supposed to give the two ions Na+ and Cl-, thus exerting twice
as much osmotic pressure as a single molecule.
Determinations of osmotic pressure or related values, such as depression
of the freezing point and of electric conductivity, indicated that ionization
could not be regarded as complete in any case except in exceedingly dilute
solutions, and that the extent of ionization varied with different substances.
The fact that osmotic pressures and electric conductivities gave closely
agreeing results in regard to the extent of ionization in various cases, is the
strongest evidence in support of the theory.
Page 345
It was difficult at first for many chemists to believe that atoms, such as
those of sodium and chlorine, and groups such as NH4 and SO4 could exist
independently in solution, even though electrically charged. However, the
theory rapidly gained ground and is now accepted by nearly every chemist
as a satisfactory explanation of many facts.
During recent years, many investigations relating to osmotic pressure and
ionization have been carried out in the United States, but only the work of
Morse, A. A. Noyes, and the late H. C. Jones can be merely alluded to here.
It should be mentioned that the eminent author of the ionic hypothesis gave
the Silliman Memorial course of lectures at Yale in 1911 on Theories of
Solution.
Colloidal Solutions.—Graham, an English chemist, in 1861 was the first
to make a distinction between substances forming true solutions, which he
called crystalloids, and those of a gummy nature resembling glue, which in
solution do not diffuse readily through parchment membranes, as
crystalloids do, and which he called colloids. The separation of colloids by
means of parchment was called dialysis, and this process has come into
extensive use in preparing pure colloidal solutions. Slow diffusion is now
regarded as characteristic of colloids rather than their gummy condition.
Colloidal solutions occupy an intermediate position between true
solutions and suspensions, resembling one or the other according to the
kind of colloid and the fineness of division. By preparing filters with pores
of varying degrees of fineness, Bechold has been able to separate colloids
from each other in accordance with the size of their particles. It has also
been possible to prepare different solutions of a colloid varying gradually
from one in which the particles were undoubtedly in suspension to one
which had many of the properties of a true solution.
Beginning in 1889, Carey Lea described in the Journal (37, 476, 1889 et
seq.) a variety of methods for preparing colloidal solutions of the metals,
consisting in general of treating solutions of metallic salts with mild
reducing agents. His work on colloidal silver was particularly extensive and
interesting. Solutions of this kind have recently yielded some extremely
interesting results by means of the ultra-microscope, an apparatus devised
by Zsigmondy and Siedentopf. A very intense beam of light is passed
through the solution and observed at right angles with a powerful
microscope. Under these conditions, particles much too small to be seen by
those of sodium and chlorine, and groups such as NH4 and SO4 could exist
independently in solution, even though electrically charged. However, the
theory rapidly gained ground and is now accepted by nearly every chemist
as a satisfactory explanation of many facts.
During recent years, many investigations relating to osmotic pressure and
ionization have been carried out in the United States, but only the work of
Morse, A. A. Noyes, and the late H. C. Jones can be merely alluded to here.
It should be mentioned that the eminent author of the ionic hypothesis gave
the Silliman Memorial course of lectures at Yale in 1911 on Theories of
Solution.
Colloidal Solutions.—Graham, an English chemist, in 1861 was the first
to make a distinction between substances forming true solutions, which he
called crystalloids, and those of a gummy nature resembling glue, which in
solution do not diffuse readily through parchment membranes, as
crystalloids do, and which he called colloids. The separation of colloids by
means of parchment was called dialysis, and this process has come into
extensive use in preparing pure colloidal solutions. Slow diffusion is now
regarded as characteristic of colloids rather than their gummy condition.
Colloidal solutions occupy an intermediate position between true
solutions and suspensions, resembling one or the other according to the
kind of colloid and the fineness of division. By preparing filters with pores
of varying degrees of fineness, Bechold has been able to separate colloids
from each other in accordance with the size of their particles. It has also
been possible to prepare different solutions of a colloid varying gradually
from one in which the particles were undoubtedly in suspension to one
which had many of the properties of a true solution.
Beginning in 1889, Carey Lea described in the Journal (37, 476, 1889 et
seq.) a variety of methods for preparing colloidal solutions of the metals,
consisting in general of treating solutions of metallic salts with mild
reducing agents. His work on colloidal silver was particularly extensive and
interesting. Solutions of this kind have recently yielded some extremely
interesting results by means of the ultra-microscope, an apparatus devised
by Zsigmondy and Siedentopf. A very intense beam of light is passed
through the solution and observed at right angles with a powerful
microscope. Under these conditions, particles much too small to be seen by
Page 346
other means, reveal their presence by reflected light. It has been possible in
a very dilute solution of known strength to count the particles and thus to
calculate their size. The smallest colloidal particles measured in this way
were of gold and were shown to have approximately ten times the diameter,
or 1000 times the volume, attributed to ordinary molecules. It is of interest
that the particles appear in rapid motion corresponding to the well-known
Brownian movement.
The chemistry of colloids has now assumed such importance that it may
be considered as a separate branch of the science. It has its own technical
journal and deals largely with the chemistry of organic products. All living
matter is built up of colloids, and hæmoglobin, starch, proteins, rubber and
milk are examples of colloidal substances or solutions. Among inorganic
substances, many sulphides, silicic acid, and the amorphous hydroxides,
like ferric hydroxide, frequently act as colloids.
Law of Mass Action.—Berthollet about the beginning of the last century
was the first chemist to study the effect of mass, or more correctly, the
concentration of substances on chemical action. His views summarized by
himself are as follows: “The chemical activity of a substance depends upon
the force of its affinity and upon the mass which is present in a given
volume.” The development of this idea, which is fundamentally correct,
was greatly hindered by the fact that Berthollet drew the incorrect
conclusion that the composition of chemical compounds depended upon the
masses of the substances combining to produce them, a conclusion in direct
contradiction to the law of definite proportions, and since this view was
soon disproved by Proust and others, Berthollet’s law in its other
applications received no immediate attention. Mitchell, however, pointed
out in the Journal (16, 234, 1829) the importance of Berthollet’s work, and
Heinrich Rose in 1842 again called attention to the effect of mass,
mentioning as one illustration the effect of water and carbonic acid in
decomposing the very stable natural silicates. Somewhat later several other
chemists made important contributions to the question of the influence of
concentration upon chemical action, but it was the Norwegians, Guldberg
and Waage, who first formulated the law of mass action in 1867.
This law has been of enormous importance in chemical theory, since it
explains a great many facts upon a mathematical basis. It applies
particularly to equilibrium in reversible reactions, where it states that the
a very dilute solution of known strength to count the particles and thus to
calculate their size. The smallest colloidal particles measured in this way
were of gold and were shown to have approximately ten times the diameter,
or 1000 times the volume, attributed to ordinary molecules. It is of interest
that the particles appear in rapid motion corresponding to the well-known
Brownian movement.
The chemistry of colloids has now assumed such importance that it may
be considered as a separate branch of the science. It has its own technical
journal and deals largely with the chemistry of organic products. All living
matter is built up of colloids, and hæmoglobin, starch, proteins, rubber and
milk are examples of colloidal substances or solutions. Among inorganic
substances, many sulphides, silicic acid, and the amorphous hydroxides,
like ferric hydroxide, frequently act as colloids.
Law of Mass Action.—Berthollet about the beginning of the last century
was the first chemist to study the effect of mass, or more correctly, the
concentration of substances on chemical action. His views summarized by
himself are as follows: “The chemical activity of a substance depends upon
the force of its affinity and upon the mass which is present in a given
volume.” The development of this idea, which is fundamentally correct,
was greatly hindered by the fact that Berthollet drew the incorrect
conclusion that the composition of chemical compounds depended upon the
masses of the substances combining to produce them, a conclusion in direct
contradiction to the law of definite proportions, and since this view was
soon disproved by Proust and others, Berthollet’s law in its other
applications received no immediate attention. Mitchell, however, pointed
out in the Journal (16, 234, 1829) the importance of Berthollet’s work, and
Heinrich Rose in 1842 again called attention to the effect of mass,
mentioning as one illustration the effect of water and carbonic acid in
decomposing the very stable natural silicates. Somewhat later several other
chemists made important contributions to the question of the influence of
concentration upon chemical action, but it was the Norwegians, Guldberg
and Waage, who first formulated the law of mass action in 1867.
This law has been of enormous importance in chemical theory, since it
explains a great many facts upon a mathematical basis. It applies
particularly to equilibrium in reversible reactions, where it states that the
Page 347
product of the concentrations on the one side of a simple reversible
equation bears a constant relation to the products of the concentrations on
the other side, provided that the temperature remains constant. In cases of
this kind where two gases or vapors react with two solids, the latter if
always in excess may be regarded as constant in concentration, and the law
takes on a simpler aspect in applying only to the concentrations of the
gaseous substances. For example, in the reversible reaction
3Fe + 4H2O ⇄ Fe3O4 + 4H2,
which takes place at rather high temperatures, a definite mixture of steam
and hydrogen at a definite temperature will cause the reaction to proceed
with equal rapidity in both directions, thus maintaining a state of
equilibrium, provided that both iron and the oxide are present in excess. If,
however, the relative concentrations of the hydrogen and steam are
changed, or even if the temperature is changed, the reaction will proceed
faster in one direction than in the other until equilibrium is again attained.
The principle of mass action also explains why it is sometimes possible
for a reversible reaction to become complete in either direction. For
instance, in connection with the reaction that has just been considered, if
steam is passed over heated iron and if hydrogen is passed over the heated
oxide, the gaseous product in each case is gradually carried away, and the
reaction continually proceeds faster in one direction than in the other until it
is complete, according to the equations
3Fe + 4H2O → 3Fe3O4 + 4H2, and
Fe3O4 + 4H2 → 3Fe + 4H2O.
Many other well-known and important facts, both chemical and physical,
depend upon this law. It explains the circumstance that a vapor-pressure is
not dependent upon the amount of the liquid that is present; it also explains
the constant dissociation pressure of calcium carbonate at a given
temperature, irrespective of the amounts of carbonate and oxide present; in
connection with the ionic theory, it furnishes the reason for the variable
solubility of salts due to the presence of electrolytes containing ions in
common; and it elucidates Henry’s law which states that the solubilities of
gases are proportional to their pressures.
equation bears a constant relation to the products of the concentrations on
the other side, provided that the temperature remains constant. In cases of
this kind where two gases or vapors react with two solids, the latter if
always in excess may be regarded as constant in concentration, and the law
takes on a simpler aspect in applying only to the concentrations of the
gaseous substances. For example, in the reversible reaction
3Fe + 4H2O ⇄ Fe3O4 + 4H2,
which takes place at rather high temperatures, a definite mixture of steam
and hydrogen at a definite temperature will cause the reaction to proceed
with equal rapidity in both directions, thus maintaining a state of
equilibrium, provided that both iron and the oxide are present in excess. If,
however, the relative concentrations of the hydrogen and steam are
changed, or even if the temperature is changed, the reaction will proceed
faster in one direction than in the other until equilibrium is again attained.
The principle of mass action also explains why it is sometimes possible
for a reversible reaction to become complete in either direction. For
instance, in connection with the reaction that has just been considered, if
steam is passed over heated iron and if hydrogen is passed over the heated
oxide, the gaseous product in each case is gradually carried away, and the
reaction continually proceeds faster in one direction than in the other until it
is complete, according to the equations
3Fe + 4H2O → 3Fe3O4 + 4H2, and
Fe3O4 + 4H2 → 3Fe + 4H2O.
Many other well-known and important facts, both chemical and physical,
depend upon this law. It explains the circumstance that a vapor-pressure is
not dependent upon the amount of the liquid that is present; it also explains
the constant dissociation pressure of calcium carbonate at a given
temperature, irrespective of the amounts of carbonate and oxide present; in
connection with the ionic theory, it furnishes the reason for the variable
solubility of salts due to the presence of electrolytes containing ions in
common; and it elucidates Henry’s law which states that the solubilities of
gases are proportional to their pressures.
Page 348
Ostwald, more than any other chemist, has been instrumental in making
general applications of this law, and he made particularly extensive use of it
in connection with analytical chemistry in a book upon this subject which
he published.
The Phase Rule.—In 1876 Willard Gibbs of Yale published a paper in the
Proceedings of the Connecticut Academy of Science on the “Equilibrium of
Heterogeneous Substances,” and two years later he published an abstract of
the article in the Journal (16, 441, 1878). He had discovered a new law of
nature of momentous importance and wide application which is called the
“Phase-Rule” and is expressed by a very simple formula.
The application of this great discovery to chemical theory was delayed
for ten years, partly, perhaps, because it was not sufficiently brought to the
attention of chemists, but largely it appears because it was not at first
understood, since its presentation was entirely mathematical.
It was Rooseboom, a Dutch chemist, who first applied the phase-rule. It
soon attracted profound attention, and the name of Willard Gibbs attained
world-wide fame among chemists. When Nernst, who is perhaps the most
eminent physical chemist of the present time, was delivering the Silliman
Memorial Lectures at Yale a few years ago, he took occasion to place a
wreath on the grave of Willard Gibbs in recognition of his achievements.
To understand the rule, it is necessary to define the three terms,
introduced by Gibbs, phase, degrees of freedom and component.
By the first term, is meant the parts of any system of substances which
are mechanically separable. For instance, water in contact with its vapor has
two phases, while a solution of salt and water is composed of but one. The
degrees of freedom are the number of physical conditions, including
pressure, temperature and concentration, which can be varied independently
in a system without destroying a phase. The exact definition of a component
is not so simple, but in general, the components of a system are the integral
parts of which it is composed. Any system made up of the compound H2O,
for instance, whether as ice, water or vapor, contains but one component,
while a solution of salt and water contains two. Letting P, F, and C stand for
the three terms, the phase-rule is simply
F=C+2−P
general applications of this law, and he made particularly extensive use of it
in connection with analytical chemistry in a book upon this subject which
he published.
The Phase Rule.—In 1876 Willard Gibbs of Yale published a paper in the
Proceedings of the Connecticut Academy of Science on the “Equilibrium of
Heterogeneous Substances,” and two years later he published an abstract of
the article in the Journal (16, 441, 1878). He had discovered a new law of
nature of momentous importance and wide application which is called the
“Phase-Rule” and is expressed by a very simple formula.
The application of this great discovery to chemical theory was delayed
for ten years, partly, perhaps, because it was not sufficiently brought to the
attention of chemists, but largely it appears because it was not at first
understood, since its presentation was entirely mathematical.
It was Rooseboom, a Dutch chemist, who first applied the phase-rule. It
soon attracted profound attention, and the name of Willard Gibbs attained
world-wide fame among chemists. When Nernst, who is perhaps the most
eminent physical chemist of the present time, was delivering the Silliman
Memorial Lectures at Yale a few years ago, he took occasion to place a
wreath on the grave of Willard Gibbs in recognition of his achievements.
To understand the rule, it is necessary to define the three terms,
introduced by Gibbs, phase, degrees of freedom and component.
By the first term, is meant the parts of any system of substances which
are mechanically separable. For instance, water in contact with its vapor has
two phases, while a solution of salt and water is composed of but one. The
degrees of freedom are the number of physical conditions, including
pressure, temperature and concentration, which can be varied independently
in a system without destroying a phase. The exact definition of a component
is not so simple, but in general, the components of a system are the integral
parts of which it is composed. Any system made up of the compound H2O,
for instance, whether as ice, water or vapor, contains but one component,
while a solution of salt and water contains two. Letting P, F, and C stand for
the three terms, the phase-rule is simply
F=C+2−P
Page 349
that is, the number of degrees of freedom in a system in equilibrium equals
the number of components, plus two, minus the number of phases. The rule
can be easily understood by means of a simple illustration. In a system
composed of ice, water and water vapor, there are three phases and one
component and therefore
F=1+2−3=0
Such a system has no degrees of freedom. This means that no physical
condition, pressure or temperature can be varied without destroying a
phase, so that such a system can only exist in equilibrium at one fixed
temperature, with a fixed value for its vapor-pressure.
the number of components, plus two, minus the number of phases. The rule
can be easily understood by means of a simple illustration. In a system
composed of ice, water and water vapor, there are three phases and one
component and therefore
F=1+2−3=0
Such a system has no degrees of freedom. This means that no physical
condition, pressure or temperature can be varied without destroying a
phase, so that such a system can only exist in equilibrium at one fixed
temperature, with a fixed value for its vapor-pressure.
Page 350
For instance, if the system is heated above the fixed temperature, ice
disappears and if the pressure is raised, vapor is condensed. If this same
system of water alone contains but two phases, for instance, liquid and
vapor, F = 1 + 2 − 2 = 1, or there is one degree of freedom. In such a
system, one physical condition such as temperature can be varied
independently, but only one, without destroying a phase. For instance, the
temperature may be raised or lowered, but for every value of temperature
there is a corresponding value for the vapor-pressure. One is a function of
the other. If both values are varied independently, one phase will disappear,
either vapor condensing entirely to water or the reverse. Finally if the
disappears and if the pressure is raised, vapor is condensed. If this same
system of water alone contains but two phases, for instance, liquid and
vapor, F = 1 + 2 − 2 = 1, or there is one degree of freedom. In such a
system, one physical condition such as temperature can be varied
independently, but only one, without destroying a phase. For instance, the
temperature may be raised or lowered, but for every value of temperature
there is a corresponding value for the vapor-pressure. One is a function of
the other. If both values are varied independently, one phase will disappear,
either vapor condensing entirely to water or the reverse. Finally if the
Page 351
system consists of one phase only, as water vapor, F = 2, or the system is
divariant, which means that at any given temperature it is possible for vapor
to exist at varying pressures.
The illustration which has been given relates to physical equilibrium, but
the rule is applicable to cases involving chemical changes as well. In
comparing the phase-rule with the law of mass action, it will be noticed that
both have to do with equilibrium. The great advantage of the former is that
it is entirely independent of the molecular condition of the substances in the
different phases. For instance, it makes no difference so far as the
application of the rule is concerned, whether a substance in solution is
dissociated, undissociated or combined with the solvent. In any case, the
solution constitutes one phase. On the other hand, the rule is purely
qualitative, giving information only as to whether a given change in
conditions is possible. The law of mass action is a quantitative expression
so that when the value of the constant is once known, the change can be
calculated which takes place in the entire system if the concentration of one
substance is varied. The law, however, requires a knowledge of the
molecular condition of the reacting substances, which may be uncertain or
unknown, and chiefly on this account it has, like the phase-rule, often only
a qualitative significance.
The phase rule has served as a most valuable means of classifying
systems in equilibrium and as a guide in determining the possible
conditions under which such systems can exist. As illustrations of its
practical application, van’t Hoff used it as an underlying principle in his
investigations on the conditions under which salt deposits have been formed
in nature, and Rooseboom was able by its means to explain the very
complicated relations existing in the alloys of iron and carbon which form
the various grades of wrought iron, steel and cast iron.
Thermochemistry.—This branch of chemistry has to do with heat evolved
or absorbed in chemical reactions. It is important chiefly because in many
cases it furnishes the only measure we have of the energy changes involved
in reactions. To a great extent, it dates from the discovery by Hess in 1840
of a fundamental law which states that the heat evolved in a reaction is the
same whether it takes place in one or in several stages. This law has made it
possible to calculate the heat values of a large number of reactions which
cannot be determined by direct experiment.
divariant, which means that at any given temperature it is possible for vapor
to exist at varying pressures.
The illustration which has been given relates to physical equilibrium, but
the rule is applicable to cases involving chemical changes as well. In
comparing the phase-rule with the law of mass action, it will be noticed that
both have to do with equilibrium. The great advantage of the former is that
it is entirely independent of the molecular condition of the substances in the
different phases. For instance, it makes no difference so far as the
application of the rule is concerned, whether a substance in solution is
dissociated, undissociated or combined with the solvent. In any case, the
solution constitutes one phase. On the other hand, the rule is purely
qualitative, giving information only as to whether a given change in
conditions is possible. The law of mass action is a quantitative expression
so that when the value of the constant is once known, the change can be
calculated which takes place in the entire system if the concentration of one
substance is varied. The law, however, requires a knowledge of the
molecular condition of the reacting substances, which may be uncertain or
unknown, and chiefly on this account it has, like the phase-rule, often only
a qualitative significance.
The phase rule has served as a most valuable means of classifying
systems in equilibrium and as a guide in determining the possible
conditions under which such systems can exist. As illustrations of its
practical application, van’t Hoff used it as an underlying principle in his
investigations on the conditions under which salt deposits have been formed
in nature, and Rooseboom was able by its means to explain the very
complicated relations existing in the alloys of iron and carbon which form
the various grades of wrought iron, steel and cast iron.
Thermochemistry.—This branch of chemistry has to do with heat evolved
or absorbed in chemical reactions. It is important chiefly because in many
cases it furnishes the only measure we have of the energy changes involved
in reactions. To a great extent, it dates from the discovery by Hess in 1840
of a fundamental law which states that the heat evolved in a reaction is the
same whether it takes place in one or in several stages. This law has made it
possible to calculate the heat values of a large number of reactions which
cannot be determined by direct experiment.
Page 352
Thermochemistry has been developed by a comparatively few men who
have contributed a surprisingly large number of results. Favre and
Silbermann, beginning shortly after 1850, improved the apparatus for
calorimetric determinations, which is called the calorimeter, and published
many results. At about the same time Julius Thomsen, and in 1873
Berthelot, began their remarkable series of publications which continued
until recently. Thomsen’s investigations were published in 1882 in 4
volumes. It is probably safe to say that the greater part of the data of
thermochemistry was obtained by these two investigators. The bomb
calorimeter, an apparatus for determining heat values by direct combustion,
was developed by Berthelot. The recent work of Mixter at Yale, published
in the Journal, and of Richards at Harvard should be mentioned particularly.
Mixter’s work in this field began in 1901 (12, 347). Using an improved
bomb calorimeter, he has developed a method of determining the heats of
formation of oxides by combustion with sodium peroxide. By this same
method as well as by direct combustion in oxygen, he has obtained results
which appear to equal or excel in accuracy any which have ever been
obtained in his field of work. Richards’s work has consisted largely of
improvements in apparatus. He developed the so-called adiabatic
calorimeter which practically eliminates one of the chief errors in thermal
work caused by the heating or cooling effect of the surroundings. This
modification is being generally adopted where extremely accurate work is
required.
have contributed a surprisingly large number of results. Favre and
Silbermann, beginning shortly after 1850, improved the apparatus for
calorimetric determinations, which is called the calorimeter, and published
many results. At about the same time Julius Thomsen, and in 1873
Berthelot, began their remarkable series of publications which continued
until recently. Thomsen’s investigations were published in 1882 in 4
volumes. It is probably safe to say that the greater part of the data of
thermochemistry was obtained by these two investigators. The bomb
calorimeter, an apparatus for determining heat values by direct combustion,
was developed by Berthelot. The recent work of Mixter at Yale, published
in the Journal, and of Richards at Harvard should be mentioned particularly.
Mixter’s work in this field began in 1901 (12, 347). Using an improved
bomb calorimeter, he has developed a method of determining the heats of
formation of oxides by combustion with sodium peroxide. By this same
method as well as by direct combustion in oxygen, he has obtained results
which appear to equal or excel in accuracy any which have ever been
obtained in his field of work. Richards’s work has consisted largely of
improvements in apparatus. He developed the so-called adiabatic
calorimeter which practically eliminates one of the chief errors in thermal
work caused by the heating or cooling effect of the surroundings. This
modification is being generally adopted where extremely accurate work is
required.
Page 353
Organic Chemistry.
One hundred years ago qualitative tests for a few organic compounds
were known, the elements usually occurring in them were recognized, and
some of them had been analyzed quantitatively, but organic chemistry was
far less advanced than inorganic, and almost the whole of its enormous
development has taken place during our period.
Berzelius made a great advance in the subject by establishing the fact,
which had been doubted previously, that the elements in organic
compounds are combined in constant, definite proportions. In 1823 Liebig
brought to light the exceedingly important fact of isomerism by showing
that silver fulminate had the same percentage composition as silver cyanate,
a compound of very different properties. Isomeric compounds with identical
molecular weight as well as the same composition have since been found in
very many cases, and they have played a most important part in determining
the arrangements of atoms in molecules. They have been found to be very
numerous in many cases. For instance, three pentanes with the formula
C5H12are known, all that are possible according to theory, and in each case
the structure of the molecule has been established. On theoretical grounds it
has been calculated that 802 isomeric compounds with the formula C13H28
are possible, while with more complex formulas the numbers of isomers
may be very much greater.
A particularly interesting case of isomerism was observed by Wöhler in
1828, when he found that ammonium cyanate changes spontaneously into
urea
(NH4CNO → N2H4CO).
This was the first synthesis of an organic compound from inorganic
material, and it overthrew the prevailing view that vital forces were
essential in the formation of organic substances. A great many natural
organic compounds have been made artificially since that time, and some of
them, such as artificial alizarin, indigo, oil of wintergreen, and vanillin,
have more or less fully replaced the natural products. The preparation of a
vast number of compounds not known in nature, many of which are of
One hundred years ago qualitative tests for a few organic compounds
were known, the elements usually occurring in them were recognized, and
some of them had been analyzed quantitatively, but organic chemistry was
far less advanced than inorganic, and almost the whole of its enormous
development has taken place during our period.
Berzelius made a great advance in the subject by establishing the fact,
which had been doubted previously, that the elements in organic
compounds are combined in constant, definite proportions. In 1823 Liebig
brought to light the exceedingly important fact of isomerism by showing
that silver fulminate had the same percentage composition as silver cyanate,
a compound of very different properties. Isomeric compounds with identical
molecular weight as well as the same composition have since been found in
very many cases, and they have played a most important part in determining
the arrangements of atoms in molecules. They have been found to be very
numerous in many cases. For instance, three pentanes with the formula
C5H12are known, all that are possible according to theory, and in each case
the structure of the molecule has been established. On theoretical grounds it
has been calculated that 802 isomeric compounds with the formula C13H28
are possible, while with more complex formulas the numbers of isomers
may be very much greater.
A particularly interesting case of isomerism was observed by Wöhler in
1828, when he found that ammonium cyanate changes spontaneously into
urea
(NH4CNO → N2H4CO).
This was the first synthesis of an organic compound from inorganic
material, and it overthrew the prevailing view that vital forces were
essential in the formation of organic substances. A great many natural
organic compounds have been made artificially since that time, and some of
them, such as artificial alizarin, indigo, oil of wintergreen, and vanillin,
have more or less fully replaced the natural products. The preparation of a
vast number of compounds not known in nature, many of which are of
Page 354
practical importance as medicines, dyes, explosives, etc., has been another
great achievement of organic chemistry.
The development of our present formulas for organic compounds, by
means of which in many cases the relative positions of the atoms can be
shown with the greatest confidence, has been gradual. Formulas based on
the dualistic idea of Berzelius were used for some time, type-formulas, with
the employment of compound radicals, came later, the substitution of atoms
or groups of atoms for others in chemical reactions came to be recognized,
but one of the most important steps was the recognition of the
quadrivalence of carbon and the general application of valency to atoms by
Kekulé about 1858. This led directly to the use of modern structural
formulas which have been of the greatest value in the theoretical
interpretation of organic reactions. It was Kekulé also who proposed the
hexagonal ring-formula for benzene, C6H6, which led to exceedingly
important theoretical and practical developments. The details of the
formulas for many other rings and complex structures have been established
since that time, and there is no doubt that the remarkable achievements in
organic chemistry during the past sixty years have been much facilitated by
the use of these formulas.
Many important researches in organic chemistry have been carried out in
the United States, and the activity in this direction has greatly increased in
recent years. In this connection the large amount of work of this kind
accomplished in the Sheffield Laboratory, at present under the guidance of
Professor T. B. Johnson, should be mentioned.
It has happened that comparatively few publications on organic
chemistry have appeared in the Journal, but it may be stated that the
preparation of chloroform and its physiological effects were described by
Guthrie (21, 64, 1832). Unknown to him, it had been prepared by
Souberain, a French chemist, the previous year, but the former was the first
to describe its physiological action. Silliman gave a sample to Doctor Eli
Ives of the Yale Medical School, who used it to relieve a case of asthma.
This was the first use of chloroform in medical practice (21, 405, 1832).
Guthrie also described in the Journal (21, 284, 1832) his new process for
converting potato starch into glucose, a method which is essentially the
same as that used to-day in converting cornstarch into glucose. Lawrence
Smith (43, 301, 1842 et seq.), Horsford (3, 369, 1847 et seq.), Sterry Hunt
great achievement of organic chemistry.
The development of our present formulas for organic compounds, by
means of which in many cases the relative positions of the atoms can be
shown with the greatest confidence, has been gradual. Formulas based on
the dualistic idea of Berzelius were used for some time, type-formulas, with
the employment of compound radicals, came later, the substitution of atoms
or groups of atoms for others in chemical reactions came to be recognized,
but one of the most important steps was the recognition of the
quadrivalence of carbon and the general application of valency to atoms by
Kekulé about 1858. This led directly to the use of modern structural
formulas which have been of the greatest value in the theoretical
interpretation of organic reactions. It was Kekulé also who proposed the
hexagonal ring-formula for benzene, C6H6, which led to exceedingly
important theoretical and practical developments. The details of the
formulas for many other rings and complex structures have been established
since that time, and there is no doubt that the remarkable achievements in
organic chemistry during the past sixty years have been much facilitated by
the use of these formulas.
Many important researches in organic chemistry have been carried out in
the United States, and the activity in this direction has greatly increased in
recent years. In this connection the large amount of work of this kind
accomplished in the Sheffield Laboratory, at present under the guidance of
Professor T. B. Johnson, should be mentioned.
It has happened that comparatively few publications on organic
chemistry have appeared in the Journal, but it may be stated that the
preparation of chloroform and its physiological effects were described by
Guthrie (21, 64, 1832). Unknown to him, it had been prepared by
Souberain, a French chemist, the previous year, but the former was the first
to describe its physiological action. Silliman gave a sample to Doctor Eli
Ives of the Yale Medical School, who used it to relieve a case of asthma.
This was the first use of chloroform in medical practice (21, 405, 1832).
Guthrie also described in the Journal (21, 284, 1832) his new process for
converting potato starch into glucose, a method which is essentially the
same as that used to-day in converting cornstarch into glucose. Lawrence
Smith (43, 301, 1842 et seq.), Horsford (3, 369, 1847 et seq.), Sterry Hunt
Page 355
(7, 399, 1849), Carey Lea (26, 379, 1858 et seq.), Remsen (5, 179, 1873 et
seq.), and others have contributed articles on organic chemistry.
seq.), and others have contributed articles on organic chemistry.
Page 356
Agricultural Chemistry.
Until near the middle of the nineteenth century, it was believed that
plants, like animals, used organic matter for food, and depended chiefly
upon the humus of the soil for their growth. This view was held even long
after it was known that plant leaves absorb carbon dioxide and give off
oxygen, and after the ashes of plants had been accurately analyzed.
This incorrect view was overthrown by the celebrated German chemist,
Liebig, who made many investigations upon the subject, and, properly
interpreting previous knowledge, published a book in 1840 upon the
application of chemistry to agriculture and physiology in which he
maintained that the nutritive materials of all green plants are inorganic
substances, namely, carbon dioxide, water, ammonia (nitrates), sulphates,
phosphates, silica, lime, magnesia, potash, iron, and sometimes common
salt. He drew the vastly important conclusion that the effective fertilization
of soils depends upon replenishing the inorganic substances that have been
exhausted by the crops.
The fundamental principles set forth by Liebig have been confirmed, and
it has been found that the fertilizing constituents most commonly lacking in
soils are nitrogen compounds, phosphates, and potassium salts, so that these
have formed the important constituents of artificial fertilizers. Liebig
himself found that humus is valuable in soils, because it absorbs and retains
the soluble salts.
The foundation established by Liebig in regard to artificial fertilizers has
led to an enormous application of these materials, much to the advantage of
the world’s food supply.
It was Liebig’s belief, in accordance with the prevailing views, that decay
and putrefaction as well as alcoholic and other fermentations were
spontaneous processes, and when the eminent French chemist, Pasteur, in
1857, explained fermentation as directly caused by yeast, an epoch-making
discovery which led to the explanation of decay and putrefaction by
bacterial action and to the germ-theory of disease, the explanation was
violently opposed by Liebig and other German chemists. Pasteur’s view
prevailed, however, and since that time it has been found that various kinds
Until near the middle of the nineteenth century, it was believed that
plants, like animals, used organic matter for food, and depended chiefly
upon the humus of the soil for their growth. This view was held even long
after it was known that plant leaves absorb carbon dioxide and give off
oxygen, and after the ashes of plants had been accurately analyzed.
This incorrect view was overthrown by the celebrated German chemist,
Liebig, who made many investigations upon the subject, and, properly
interpreting previous knowledge, published a book in 1840 upon the
application of chemistry to agriculture and physiology in which he
maintained that the nutritive materials of all green plants are inorganic
substances, namely, carbon dioxide, water, ammonia (nitrates), sulphates,
phosphates, silica, lime, magnesia, potash, iron, and sometimes common
salt. He drew the vastly important conclusion that the effective fertilization
of soils depends upon replenishing the inorganic substances that have been
exhausted by the crops.
The fundamental principles set forth by Liebig have been confirmed, and
it has been found that the fertilizing constituents most commonly lacking in
soils are nitrogen compounds, phosphates, and potassium salts, so that these
have formed the important constituents of artificial fertilizers. Liebig
himself found that humus is valuable in soils, because it absorbs and retains
the soluble salts.
The foundation established by Liebig in regard to artificial fertilizers has
led to an enormous application of these materials, much to the advantage of
the world’s food supply.
It was Liebig’s belief, in accordance with the prevailing views, that decay
and putrefaction as well as alcoholic and other fermentations were
spontaneous processes, and when the eminent French chemist, Pasteur, in
1857, explained fermentation as directly caused by yeast, an epoch-making
discovery which led to the explanation of decay and putrefaction by
bacterial action and to the germ-theory of disease, the explanation was
violently opposed by Liebig and other German chemists. Pasteur’s view
prevailed, however, and since that time it has been found that various kinds
Page 357
of bacteria are responsible for the formation of ammonia from nitrogenous
organic matter and also for the change of ammonia into the nitrates that are
available as plant-food.
The long-debated question as to the availability of atmospheric nitrogen
for plant-food was settled in 1886 by the discovery of Hellriegel that
bacteria contained in nodules on the roots, especially of leguminous plants,
are capable of bringing nitrogen into combination and furnishing it to the
plants.
No more than an allusion can be made to agricultural experiment stations
where soils, fertilizers, foods and other products are examined, and where
other problems connected with agriculture are studied.
The late S. W. Johnson of Yale studied with Liebig and subsequently did
much service for agricultural chemistry in this country, by his
investigations, his teaching, and his writings. His book, “How Crops
Grow,” published in 1868, gave an excellent account of the principles of
agricultural chemistry. He did much to bring about the establishment of
agricultural experiment stations in this country, and for a long time he was
the director of the Connecticut Station.
In the Journal, as early as 1827, Amos Eaton (12, 370) published a simple
method for the mechanical analysis of soils to determine their suitability for
wheat-culture, and Hilgard, between 1872 and 1874, described an elaborate
study of soil-analysis. J. P. Norton, a Yale professor, in 1847 (3, 322)
published an investigation on the analysis of the oat, which was awarded a
prize of fifty sovereigns by a Scotch agricultural society, while Johnson,
Atwater, and others have contributed articles on the analysis of various farm
products.
organic matter and also for the change of ammonia into the nitrates that are
available as plant-food.
The long-debated question as to the availability of atmospheric nitrogen
for plant-food was settled in 1886 by the discovery of Hellriegel that
bacteria contained in nodules on the roots, especially of leguminous plants,
are capable of bringing nitrogen into combination and furnishing it to the
plants.
No more than an allusion can be made to agricultural experiment stations
where soils, fertilizers, foods and other products are examined, and where
other problems connected with agriculture are studied.
The late S. W. Johnson of Yale studied with Liebig and subsequently did
much service for agricultural chemistry in this country, by his
investigations, his teaching, and his writings. His book, “How Crops
Grow,” published in 1868, gave an excellent account of the principles of
agricultural chemistry. He did much to bring about the establishment of
agricultural experiment stations in this country, and for a long time he was
the director of the Connecticut Station.
In the Journal, as early as 1827, Amos Eaton (12, 370) published a simple
method for the mechanical analysis of soils to determine their suitability for
wheat-culture, and Hilgard, between 1872 and 1874, described an elaborate
study of soil-analysis. J. P. Norton, a Yale professor, in 1847 (3, 322)
published an investigation on the analysis of the oat, which was awarded a
prize of fifty sovereigns by a Scotch agricultural society, while Johnson,
Atwater, and others have contributed articles on the analysis of various farm
products.
Page 358
Industrial Acids and Alkalies.
One hundred years ago sulphuric acid was manufactured on a
comparatively very small scale in lead chambers. In 1818, an English
manufacturer of the acid introduced the modern feature of using pyrites in
the place of brimstone, while the Gay-Lussac tower in 1827 and the Glover
tower in 1859 began to be applied as great improvements in the chamber
process. Within about twenty years the contact process, employing
platinized asbestos, has replaced the old chamber process to a large extent.
It has the advantage of producing the concentrated acid, or the fuming acid,
directly.
During our period the manufacture of sulphuric acid has increased
enormously. Very large quantities of it have been used in connection with
the Leblanc soda process in its rapid development. It came to be employed
extensively for absorbing ammonia in the illuminating-gas industry, which
was in its infancy one hundred years ago. New industries such as the
manufacture of “superphosphates” as artificial fertilizers, the refining of
petroleum, the manufacture of artificial dyestuffs and many other modern
chemical products have greatly increased the demand for it, while its
employment in the production of nitric and other acids, and for many other
purposes not already mentioned, has been very great.
The manufacture of nitric acid has been greatly extended during our
period on account of its employment for producing explosives, artificial
dyestuffs, and for many other purposes. Chile saltpeter became available for
making it about 1852. This acid has been manufactured recently from
atmospheric nitrogen and oxygen by combining them by the aid of powerful
electric discharges. This process has been used chiefly in Norway where
water-power is abundant, as it requires a large expenditure of energy. A still
more recent method for the production of nitric acid depends upon the
oxidation of ammonia by air with the aid of a contact substance, such as
platinized asbestos.
The production of ammonia, which was very small a hundred years ago,
has been vastly increased in connection with the development of the
illuminating-gas industry and the employment of by-product coke ovens.
One hundred years ago sulphuric acid was manufactured on a
comparatively very small scale in lead chambers. In 1818, an English
manufacturer of the acid introduced the modern feature of using pyrites in
the place of brimstone, while the Gay-Lussac tower in 1827 and the Glover
tower in 1859 began to be applied as great improvements in the chamber
process. Within about twenty years the contact process, employing
platinized asbestos, has replaced the old chamber process to a large extent.
It has the advantage of producing the concentrated acid, or the fuming acid,
directly.
During our period the manufacture of sulphuric acid has increased
enormously. Very large quantities of it have been used in connection with
the Leblanc soda process in its rapid development. It came to be employed
extensively for absorbing ammonia in the illuminating-gas industry, which
was in its infancy one hundred years ago. New industries such as the
manufacture of “superphosphates” as artificial fertilizers, the refining of
petroleum, the manufacture of artificial dyestuffs and many other modern
chemical products have greatly increased the demand for it, while its
employment in the production of nitric and other acids, and for many other
purposes not already mentioned, has been very great.
The manufacture of nitric acid has been greatly extended during our
period on account of its employment for producing explosives, artificial
dyestuffs, and for many other purposes. Chile saltpeter became available for
making it about 1852. This acid has been manufactured recently from
atmospheric nitrogen and oxygen by combining them by the aid of powerful
electric discharges. This process has been used chiefly in Norway where
water-power is abundant, as it requires a large expenditure of energy. A still
more recent method for the production of nitric acid depends upon the
oxidation of ammonia by air with the aid of a contact substance, such as
platinized asbestos.
The production of ammonia, which was very small a hundred years ago,
has been vastly increased in connection with the development of the
illuminating-gas industry and the employment of by-product coke ovens.
Page 359
This substance is very extensively used in refrigerating machines and also
in a great many chemical operations, including the Solvay soda process.
Ammonium salts are of great importance also as fertilizers in agriculture.
The conversion of atmospheric nitrogen into ammonia on a commercial
scale is a recent achievement. It has been accomplished by heating calcium
carbide, an electric-furnace product made from lime and coke, with
nitrogen gas, thus producing calcium cyanamide, and then treating this
cyanamide with water under proper conditions. Another method devised by
Haber consists in directly combining nitrogen and hydrogen gases under
high pressure with the aid of a contact substance.
Leblanc’s method for obtaining sodium carbonate from sodium chloride
by first converting the latter into the sulphate by means of sulphuric acid
and then heating the sulphate with lime and coal in a furnace was invented
as early as 1791, but it was not rapidly developed and did not gain a
foothold in England until 1826 on account of a high duty on salt up to that
time. Afterwards the process flourished greatly in connection with the
sulphuric acid industry upon which it depended, and with the bleaching-
powder industry which utilized the hydrochloric acid incidentally produced
by it, and, of course, in connection with soap manufacture and many other
industries in which the soda itself was employed.
About 1866 the Solvay process appeared as a rival to the Leblanc
process. This depends upon the precipitation of sodium bicarbonate from
salt solutions by means of carbon dioxide and ammonia, with the
subsequent recovery of the ammonia. It has displaced the older process to a
large extent, and it is carried on extensively in this country, for instance, at
Syracuse, New York.
Other processes for soda depend upon the electrolysis of sodium chloride
solutions. In this case caustic soda and chlorine are the direct products, and
the chlorine thus produced and liquefied by pressure in steel cylinders, has
become an important commercial article.
In earlier times wood-ashes were the source of potash and potassium
salts. Wurtz in the Journal (10, 326, 1850) suggested the availability of New
Jersey greensand as a source of potash and showed how this mineral could
be decomposed, but it does not appear that this mineral has ever been
utilized for the purpose. About 1861 the German potash-salt deposits began
to be developed, and these have since become the chief source of this
in a great many chemical operations, including the Solvay soda process.
Ammonium salts are of great importance also as fertilizers in agriculture.
The conversion of atmospheric nitrogen into ammonia on a commercial
scale is a recent achievement. It has been accomplished by heating calcium
carbide, an electric-furnace product made from lime and coke, with
nitrogen gas, thus producing calcium cyanamide, and then treating this
cyanamide with water under proper conditions. Another method devised by
Haber consists in directly combining nitrogen and hydrogen gases under
high pressure with the aid of a contact substance.
Leblanc’s method for obtaining sodium carbonate from sodium chloride
by first converting the latter into the sulphate by means of sulphuric acid
and then heating the sulphate with lime and coal in a furnace was invented
as early as 1791, but it was not rapidly developed and did not gain a
foothold in England until 1826 on account of a high duty on salt up to that
time. Afterwards the process flourished greatly in connection with the
sulphuric acid industry upon which it depended, and with the bleaching-
powder industry which utilized the hydrochloric acid incidentally produced
by it, and, of course, in connection with soap manufacture and many other
industries in which the soda itself was employed.
About 1866 the Solvay process appeared as a rival to the Leblanc
process. This depends upon the precipitation of sodium bicarbonate from
salt solutions by means of carbon dioxide and ammonia, with the
subsequent recovery of the ammonia. It has displaced the older process to a
large extent, and it is carried on extensively in this country, for instance, at
Syracuse, New York.
Other processes for soda depend upon the electrolysis of sodium chloride
solutions. In this case caustic soda and chlorine are the direct products, and
the chlorine thus produced and liquefied by pressure in steel cylinders, has
become an important commercial article.
In earlier times wood-ashes were the source of potash and potassium
salts. Wurtz in the Journal (10, 326, 1850) suggested the availability of New
Jersey greensand as a source of potash and showed how this mineral could
be decomposed, but it does not appear that this mineral has ever been
utilized for the purpose. About 1861 the German potash-salt deposits began
to be developed, and these have since become the chief source of this
Page 360
material. At present many efforts are being made to obtain potassium
compounds from other sources, such as brines, cement-kiln dust, and
feldspar and other minerals but thus far the results have not satisfied the
demand.
compounds from other sources, such as brines, cement-kiln dust, and
feldspar and other minerals but thus far the results have not satisfied the
demand.
Page 361
Conclusion.
This account of chemical progress has given only a limited view of small
portions of the subject, because the amount of available material is so vast
in comparison with the space allowed for its presentation. Since the Journal
has published comparatively little organic chemistry, it was decided to
make room for a better presentation of other things by giving only a brief
discussion of this exceedingly active and important branch of the science.
For similar reasons industrial and metallurgical chemistry, and other
branches besides, in spite of their great growth and importance, have been
neglected, except for some incidental references to them, and some account
of a few of the more important industrial chemicals.
It appears that we have much reason to be proud of the advances in
chemistry that have been made during the Journal’s period, and of the part
that the Journal has taken in connection with them, and there seems to be no
doubt that this progress has not diminished during more recent times.
The present tendency of chemical research is evidently towards a still
greater development of organic chemistry, and an increased application of
physics and mathematics to chemical theory and practice.
The very great improvements that have been made in chemical education,
both in the number of students and the quality of instruction, during the
period under discussion, and particularly in rather recent times, gives
promise for excellent future progress.
This account of chemical progress has given only a limited view of small
portions of the subject, because the amount of available material is so vast
in comparison with the space allowed for its presentation. Since the Journal
has published comparatively little organic chemistry, it was decided to
make room for a better presentation of other things by giving only a brief
discussion of this exceedingly active and important branch of the science.
For similar reasons industrial and metallurgical chemistry, and other
branches besides, in spite of their great growth and importance, have been
neglected, except for some incidental references to them, and some account
of a few of the more important industrial chemicals.
It appears that we have much reason to be proud of the advances in
chemistry that have been made during the Journal’s period, and of the part
that the Journal has taken in connection with them, and there seems to be no
doubt that this progress has not diminished during more recent times.
The present tendency of chemical research is evidently towards a still
greater development of organic chemistry, and an increased application of
physics and mathematics to chemical theory and practice.
The very great improvements that have been made in chemical education,
both in the number of students and the quality of instruction, during the
period under discussion, and particularly in rather recent times, gives
promise for excellent future progress.
Page 362
Note.
153. It appears that the most accurate experimental demonstration ever made of this law was
that of E. W. Morley, published in the Journal (41, 220, 276, 1891). He showed that 2·0002 volumes
of hydrogen combine with one volume of oxygen.
153. It appears that the most accurate experimental demonstration ever made of this law was
that of E. W. Morley, published in the Journal (41, 220, 276, 1891). He showed that 2·0002 volumes
of hydrogen combine with one volume of oxygen.
Page 363
XI
A CENTURY’S PROGRESS IN PHYSICS
By LEIGH PAGE
Dynamics.—At the beginning of the nineteenth century mechanics was the
only major branch of physical science which had attained any considerable
degree of development. Two centuries earlier, Galileo’s experiments on the
rate of fall of iron balls dropped from the top of the Leaning Tower of Pisa,
had marked the origin of dynamics. He had easily disproved the prevalent
idea that even under conditions where air resistance is negligible heavy
bodies would fall more rapidly than light ones, and further experiments had
led him to conclude that the increase in velocity is proportional to the time
elapsed, and not to the distance traversed, as he had at first supposed. Less
than a century later Newton had formulated the laws of motion in the same
words in which they are given to-day. These laws of motion, coupled with
his discovery of the law of universal gravitation, had enabled him to
correlate at once the planetary notions which had proved so puzzling to his
predecessors. His success gave a tremendous stimulus to the development
and extension of the fundamental dynamical principles that he had brought
to light, which culminated in the work of the great French mathematicians,
Lagrange and Laplace, a little over a hundred years ago.
Newton’s laws of motion, it must be remembered, apply only to a
particle, or to those bodies which can be treated as particles in the problem
under consideration. In his “Mécanique Analytique” Lagrange extended
these principles so as to make it possible to treat the motion of a connected
system by a method almost as simple as that contained in the second law of
motion. Instead of three scalar equations for each of the innumerably large
A CENTURY’S PROGRESS IN PHYSICS
By LEIGH PAGE
Dynamics.—At the beginning of the nineteenth century mechanics was the
only major branch of physical science which had attained any considerable
degree of development. Two centuries earlier, Galileo’s experiments on the
rate of fall of iron balls dropped from the top of the Leaning Tower of Pisa,
had marked the origin of dynamics. He had easily disproved the prevalent
idea that even under conditions where air resistance is negligible heavy
bodies would fall more rapidly than light ones, and further experiments had
led him to conclude that the increase in velocity is proportional to the time
elapsed, and not to the distance traversed, as he had at first supposed. Less
than a century later Newton had formulated the laws of motion in the same
words in which they are given to-day. These laws of motion, coupled with
his discovery of the law of universal gravitation, had enabled him to
correlate at once the planetary notions which had proved so puzzling to his
predecessors. His success gave a tremendous stimulus to the development
and extension of the fundamental dynamical principles that he had brought
to light, which culminated in the work of the great French mathematicians,
Lagrange and Laplace, a little over a hundred years ago.
Newton’s laws of motion, it must be remembered, apply only to a
particle, or to those bodies which can be treated as particles in the problem
under consideration. In his “Mécanique Analytique” Lagrange extended
these principles so as to make it possible to treat the motion of a connected
system by a method almost as simple as that contained in the second law of
motion. Instead of three scalar equations for each of the innumerably large
Page 364
number of particles involved, he showed how to reduce the ordinary
dynamical equations to a number equal to that of the degrees of freedom of
the system. This is made possible by a combination of d’Alembert’s
principle, which eliminates the forces due to the connections between the
particles, and the principle of virtual work, which confines the number of
equations to the number of possible independent displacements. The aim of
Lagrange was to make dynamics into a branch of analysis, and his success
may be inferred from the fact that not a single diagram or geometrical
figure is to be found in his great work.
Celestial Mechanics.—Almost simultaneously with the publication of the
“Mécanique Analytique” appeared Laplace’s “Mécanique Celeste.”
Laplace’s avowed aim was to offer a complete solution of the great
dynamical problem involved in the solar system, taking into account, in
addition to the effect of the sun’s gravitational field, those perturbations in
the motion of each planet caused by the approach and recession of its
neighbors. So successful was his analysis of planetary motions that his
contemporaries believed that they were not far from a complete explanation
of the world on mechanical principles. Laplace himself was undoubtedly
convinced that nothing was needed beyond a knowledge of the masses,
positions, and initial velocities of every material particle in the universe in
order to completely predetermine all subsequent motion.
The greatest triumph of these dynamical methods was to come half a
century later. The planet Uranus, discovered in 1781 by the elder Herschel,
was at that time the farthest known planet from the sun. But the orbit of
Uranus was subject to some puzzling variations. After sifting all the known
causes of these disturbances, Leverrier in France and Adams in England
independently reached the conclusion that another planet still more remote
from the sun must be responsible, and computed its orbit. Leverrier
communicated to Galle of Berlin the results of his calculations, and during
the next few days the German astronomer discovered Neptune within one
degree of its predicted position!
dynamical equations to a number equal to that of the degrees of freedom of
the system. This is made possible by a combination of d’Alembert’s
principle, which eliminates the forces due to the connections between the
particles, and the principle of virtual work, which confines the number of
equations to the number of possible independent displacements. The aim of
Lagrange was to make dynamics into a branch of analysis, and his success
may be inferred from the fact that not a single diagram or geometrical
figure is to be found in his great work.
Celestial Mechanics.—Almost simultaneously with the publication of the
“Mécanique Analytique” appeared Laplace’s “Mécanique Celeste.”
Laplace’s avowed aim was to offer a complete solution of the great
dynamical problem involved in the solar system, taking into account, in
addition to the effect of the sun’s gravitational field, those perturbations in
the motion of each planet caused by the approach and recession of its
neighbors. So successful was his analysis of planetary motions that his
contemporaries believed that they were not far from a complete explanation
of the world on mechanical principles. Laplace himself was undoubtedly
convinced that nothing was needed beyond a knowledge of the masses,
positions, and initial velocities of every material particle in the universe in
order to completely predetermine all subsequent motion.
The greatest triumph of these dynamical methods was to come half a
century later. The planet Uranus, discovered in 1781 by the elder Herschel,
was at that time the farthest known planet from the sun. But the orbit of
Uranus was subject to some puzzling variations. After sifting all the known
causes of these disturbances, Leverrier in France and Adams in England
independently reached the conclusion that another planet still more remote
from the sun must be responsible, and computed its orbit. Leverrier
communicated to Galle of Berlin the results of his calculations, and during
the next few days the German astronomer discovered Neptune within one
degree of its predicted position!
Page 365
We shall mention but one other achievement of the methods of celestial
mechanics. Those visitors of the skies, the comets, which become so
prominent only to fade away and vanish perhaps forever, had interested
astronomers from the earliest times. Soon after the discovery of the law of
gravitation, Newton had worked out a method by which the elements of a
comet’s orbit can be computed from observations of its position. It was
found that the great majority of these bodies move in nearly parabolic paths
and only a few in ellipses. Of the latter the most prominent is the brilliant
comet first observed by Halley in 1681. It has reappeared regularly at
intervals of seventy-six years; the last appearance in the spring of 1910 is
no doubt well remembered by the reader. Kant had considered comets to be
formed by condensing solar nebulæ, whereas Laplace had maintained that
they originate in matter which is scattered throughout stellar space and has
mechanics. Those visitors of the skies, the comets, which become so
prominent only to fade away and vanish perhaps forever, had interested
astronomers from the earliest times. Soon after the discovery of the law of
gravitation, Newton had worked out a method by which the elements of a
comet’s orbit can be computed from observations of its position. It was
found that the great majority of these bodies move in nearly parabolic paths
and only a few in ellipses. Of the latter the most prominent is the brilliant
comet first observed by Halley in 1681. It has reappeared regularly at
intervals of seventy-six years; the last appearance in the spring of 1910 is
no doubt well remembered by the reader. Kant had considered comets to be
formed by condensing solar nebulæ, whereas Laplace had maintained that
they originate in matter which is scattered throughout stellar space and has
Page 366
no connection with the solar system. A study of the distribution of
inclinations of comet orbits by H. A. Newton (16, 165, 1878) of New Haven
substantiated Laplace’s hypothesis, and led to the conclusion that the
periodic comets have been captured by the attraction of those planets near
to which they have passed. Of these comets a number have comparatively
short periods, and are found to have orbits which are in general only
slightly inclined to those of the planets, and are traversed in the same
direction. Moreover, the fact that the orbit of each of these comets comes
very close to that of Jupiter made it seem probable that they have been
attached to the solar system by the attraction of this planet. Further
confirmation of this hypothesis was furnished by H. A. Newton’s (42, 183
and 482, 1891) explanation of the small inclination of their orbits and the
scarcity of retrograde motions among them.
In 1833 occurred one of the greatest meteoric showers of history.
Olmstead (26, 132, 1834) and Twining (26, 320, 1834) of New Haven
noticed that these shooting stars traverse parallel paths, and were the first to
suggest that they must be moving in swarms in a permanent orbit. From an
examination of all accessible records, H. A. Newton (37, 377, 1864; 38, 53,
1864) was able to show that meteoric showers are common in November,
and of particular intensity at intervals of 33 or 34 years. He confidently
predicted a great shower for Nov. 13th, 1866, which not only actually
occurred but was followed by another a year later, showing that the
meteoric swarm extended so far as to require two years to cross the earth’s
orbit. H. A. Newton (36, 1, 1888) in America and Adams in England took
up the study of meteoric orbits with great interest, and the former concluded
that these orbits are in every sense similar to those of the periodic comets,
implying that a swarm of meteors originates in the disintegration of a
comet. In fact Schiaparelli actually identified the orbit of the Perseids, or
August meteors, with Tuttle’s comet of 1862, and shortly after the orbit of
the Leonids, or November meteors, was found to be the same as that of
Tempel’s comet.
Electromagnetism.—During the eighteenth century much interest had
been manifested in the study of electrostatics and magnetism. Du Fay,
Cavendish, Michell and Coulomb abroad and Franklin in America had
subjected to experimental investigation many of the phenomena of one or
both of these sciences, and in the early years of the nineteenth century
Poisson developed to a remarkable extent the analytical consequences of
inclinations of comet orbits by H. A. Newton (16, 165, 1878) of New Haven
substantiated Laplace’s hypothesis, and led to the conclusion that the
periodic comets have been captured by the attraction of those planets near
to which they have passed. Of these comets a number have comparatively
short periods, and are found to have orbits which are in general only
slightly inclined to those of the planets, and are traversed in the same
direction. Moreover, the fact that the orbit of each of these comets comes
very close to that of Jupiter made it seem probable that they have been
attached to the solar system by the attraction of this planet. Further
confirmation of this hypothesis was furnished by H. A. Newton’s (42, 183
and 482, 1891) explanation of the small inclination of their orbits and the
scarcity of retrograde motions among them.
In 1833 occurred one of the greatest meteoric showers of history.
Olmstead (26, 132, 1834) and Twining (26, 320, 1834) of New Haven
noticed that these shooting stars traverse parallel paths, and were the first to
suggest that they must be moving in swarms in a permanent orbit. From an
examination of all accessible records, H. A. Newton (37, 377, 1864; 38, 53,
1864) was able to show that meteoric showers are common in November,
and of particular intensity at intervals of 33 or 34 years. He confidently
predicted a great shower for Nov. 13th, 1866, which not only actually
occurred but was followed by another a year later, showing that the
meteoric swarm extended so far as to require two years to cross the earth’s
orbit. H. A. Newton (36, 1, 1888) in America and Adams in England took
up the study of meteoric orbits with great interest, and the former concluded
that these orbits are in every sense similar to those of the periodic comets,
implying that a swarm of meteors originates in the disintegration of a
comet. In fact Schiaparelli actually identified the orbit of the Perseids, or
August meteors, with Tuttle’s comet of 1862, and shortly after the orbit of
the Leonids, or November meteors, was found to be the same as that of
Tempel’s comet.
Electromagnetism.—During the eighteenth century much interest had
been manifested in the study of electrostatics and magnetism. Du Fay,
Cavendish, Michell and Coulomb abroad and Franklin in America had
subjected to experimental investigation many of the phenomena of one or
both of these sciences, and in the early years of the nineteenth century
Poisson developed to a remarkable extent the analytical consequences of
Page 367
the law of force which experiment had revealed. Both Laplace and he made
much use of the function to which Green gave the name “potential” in
1828, and which is such a powerful aid in solving problems involving
magnetism or electricity at rest.
Meantime electric currents had been brought under the hand of the
experimenter by the discoveries of Galvani and Volta. Large numbers of
cells were connected in series, and interest seemed to lie largely in
producing brilliant sparks or fusing metals by means of a heavy current.
Hare (3, 105, 1821) of the University of Pennsylvania constructed a battery
consisting of two troughs of forty cells each, so arranged that the coppers
and zincs can be lowered simultaneously into the acid and large currents
obtained before polarization has a chance to interfere. This “deflagrator”
was used to ignite charcoal in the circuit, or melt fine wires, and was for
some time the most powerful arrangement of its kind. That “galvanism” is
something quite different from static electricity was the opinion of many
investigators; Hare considered the heat developed to be the distinguishing
mark of the electric current. He says: “It is admitted that the action of the
galvanic fluid is upon or between atoms; while mechanical electricity when
uncoerced, acts only upon masses. This difference has not been explained
unless by my hypothesis, in which caloric, of which the influence is only
exerted between atoms, is supposed to be a principal agent in galvanism.”
Questioning minds were beginning to suspect that there must be some
connection between electricity and magnetism. For lightning had been
known to make magnets of steel knives and forks, and Franklin had
magnetized a sewing needle by the discharge from a Leyden jar. Finally
Oersted of Copenhagen undertook systematic investigation of the effect of
electricity on the magnetic needle. His researches were without result until
during the course of a series of lectures on “Electricity, Galvanism, and
Magnetism” delivered during the winter of 1819–20 it occurred to him to
investigate the action of an electric current on a magnetic needle. At first he
placed the wire bearing the current at right angles to the needle, with, of
course, no result; then it occurred to him to place it parallel. A deflection
was observed, for to his surprise the needle insisted on turning until
perpendicular to the wire.
Oersted’s discovery that an electric current exerts a couple on a magnetic
needle was followed a few months later by Ampère’s demonstration before
much use of the function to which Green gave the name “potential” in
1828, and which is such a powerful aid in solving problems involving
magnetism or electricity at rest.
Meantime electric currents had been brought under the hand of the
experimenter by the discoveries of Galvani and Volta. Large numbers of
cells were connected in series, and interest seemed to lie largely in
producing brilliant sparks or fusing metals by means of a heavy current.
Hare (3, 105, 1821) of the University of Pennsylvania constructed a battery
consisting of two troughs of forty cells each, so arranged that the coppers
and zincs can be lowered simultaneously into the acid and large currents
obtained before polarization has a chance to interfere. This “deflagrator”
was used to ignite charcoal in the circuit, or melt fine wires, and was for
some time the most powerful arrangement of its kind. That “galvanism” is
something quite different from static electricity was the opinion of many
investigators; Hare considered the heat developed to be the distinguishing
mark of the electric current. He says: “It is admitted that the action of the
galvanic fluid is upon or between atoms; while mechanical electricity when
uncoerced, acts only upon masses. This difference has not been explained
unless by my hypothesis, in which caloric, of which the influence is only
exerted between atoms, is supposed to be a principal agent in galvanism.”
Questioning minds were beginning to suspect that there must be some
connection between electricity and magnetism. For lightning had been
known to make magnets of steel knives and forks, and Franklin had
magnetized a sewing needle by the discharge from a Leyden jar. Finally
Oersted of Copenhagen undertook systematic investigation of the effect of
electricity on the magnetic needle. His researches were without result until
during the course of a series of lectures on “Electricity, Galvanism, and
Magnetism” delivered during the winter of 1819–20 it occurred to him to
investigate the action of an electric current on a magnetic needle. At first he
placed the wire bearing the current at right angles to the needle, with, of
course, no result; then it occurred to him to place it parallel. A deflection
was observed, for to his surprise the needle insisted on turning until
perpendicular to the wire.
Oersted’s discovery that an electric current exerts a couple on a magnetic
needle was followed a few months later by Ampère’s demonstration before
Page 368
the French Academy that two currents flowing in the same direction attract
each other, while two in opposite directions repel. The story goes that a
critic attempted to belittle this discovery by remarking that as it was known
that two currents act on one and the same magnet, it was obvious that they
would act upon each other. Whereupon Arago arose to defend his friend.
Drawing two keys out of his pocket he said, “Each of these keys attracts a
magnet; do you believe that they therefore attract each other?”
A few years later Ampère showed how to express quantitatively the force
between current elements, and indeed developed to a considerable degree
the equivalence between a closed circuit carrying a current and a magnetic
shell. So convincing was his analysis and so thorough his discussion of the
subject, that Maxwell said of this memoir half a century later, “The whole,
theory and experiment, seems as if it had leaped, full grown and full armed,
from the brain of the ‘Newton of electricity.’ It is perfect in form and
unassailable in accuracy; and it is summed up in a formula from which all
the phenomena may be deduced, and which must always remain the
cardinal formula of electrodynamics.”
Shortly afterwards the dependence of a current on the conductivity of the
wire used and the grouping of cells employed, was made clear by the work
of Ohm. Many of his results were obtained independently by Joseph Henry
(19, 400, 1831) of the Albany Academy, who described in 1831 a powerful
electromagnet in which a great many coils of wire insulated with silk were
wound around an iron core and connected in parallel with a single cell. He
remarks in this paper that with long wires, as in the telegraph, many cells
arranged in series should be used, whereas for several short wires connected
in parallel a single cell with large plates is more efficient.
Current Induction.—Impressed by the fact that electric charges have the
power of inducing other charges on neighboring conductors without coming
into contact with them, Faraday was engaged in investigating the possibility
of an analogous phenomenon in the case of electric currents. His idea at
first seems to have been that a current should induce another current in any
closed conducting circuit which happens to be in its vicinity. Experiment
readily showed the falsity of this conception, but a brief deflection of the
galvanometer in the secondary circuit was noticed at the instant of making
and breaking the current in the primary. Further experiments showed that
thrusting a permanent steel magnet into a coil connected to a galvanometer
each other, while two in opposite directions repel. The story goes that a
critic attempted to belittle this discovery by remarking that as it was known
that two currents act on one and the same magnet, it was obvious that they
would act upon each other. Whereupon Arago arose to defend his friend.
Drawing two keys out of his pocket he said, “Each of these keys attracts a
magnet; do you believe that they therefore attract each other?”
A few years later Ampère showed how to express quantitatively the force
between current elements, and indeed developed to a considerable degree
the equivalence between a closed circuit carrying a current and a magnetic
shell. So convincing was his analysis and so thorough his discussion of the
subject, that Maxwell said of this memoir half a century later, “The whole,
theory and experiment, seems as if it had leaped, full grown and full armed,
from the brain of the ‘Newton of electricity.’ It is perfect in form and
unassailable in accuracy; and it is summed up in a formula from which all
the phenomena may be deduced, and which must always remain the
cardinal formula of electrodynamics.”
Shortly afterwards the dependence of a current on the conductivity of the
wire used and the grouping of cells employed, was made clear by the work
of Ohm. Many of his results were obtained independently by Joseph Henry
(19, 400, 1831) of the Albany Academy, who described in 1831 a powerful
electromagnet in which a great many coils of wire insulated with silk were
wound around an iron core and connected in parallel with a single cell. He
remarks in this paper that with long wires, as in the telegraph, many cells
arranged in series should be used, whereas for several short wires connected
in parallel a single cell with large plates is more efficient.
Current Induction.—Impressed by the fact that electric charges have the
power of inducing other charges on neighboring conductors without coming
into contact with them, Faraday was engaged in investigating the possibility
of an analogous phenomenon in the case of electric currents. His idea at
first seems to have been that a current should induce another current in any
closed conducting circuit which happens to be in its vicinity. Experiment
readily showed the falsity of this conception, but a brief deflection of the
galvanometer in the secondary circuit was noticed at the instant of making
and breaking the current in the primary. Further experiments showed that
thrusting a permanent steel magnet into a coil connected to a galvanometer
Page 369
caused the needle to deflect. In fact Faraday’s report to the Royal Society
on November 24th, 1831, contains a complete account of all experimental
methods available for inducing a current in a closed circuit.
While Faraday is entitled to credit for the discovery of current induction
by virtue of the priority of his publication, it must not pass unnoticed that
Henry obtained many of the same experimental results independently and
some even earlier. Henry was at this time instructor in mathematics at the
Albany Academy, and seven hours of teaching a day made it well nigh
impossible to carry on original research except during the vacation month
of August. As early as the summer of 1830 he had wound 30 feet of copper
wire around the armature of a horseshoe electromagnet and connected it to
a galvanometer. When the magnet was excited, a momentary deflection was
observed. “I was, however, much surprised,” he says, “to see the needle
suddenly deflected from a state of rest to about 20° to the east, or in a
contrary direction, when the battery was withdrawn from the acid, and
again deflected to the west when it was re-immersed.” In addition a
deflection was obtained by detaching the armature from the magnet, or by
bringing it again into contact. Had the results of these experiments been
published promptly, America would have been entitled to credit for the
most important discovery of the greatest of England’s many great
experimenters. But Henry desired first to repeat his experiments on a larger
scale, and while new magnets were being constructed, the news of
Faraday’s discovery arrived. This occasioned hasty publication of the work
already done in an appendix to volume 22, 1832, of the Journal.
At almost the same time Henry made another important discovery and
this time he was anticipated by no other investigator in making public his
results. In the paper already referred to be describes the phenomenon
known to-day as self-induction. “When a small battery is moderately
excited by diluted acid and its poles, which must be terminated by cups of
mercury, are connected by a copper wire not more than a foot in length, no
spark is perceived when the connection is either formed or broken; but if a
wire thirty or forty feet long be used, instead of the short wire, though no
spark will be perceptible when the connection is made, yet when it is
broken by drawing one end of the wire from its cup of mercury a vivid
spark is produced.... The effect appears somewhat increased by coiling the
wire into a helix; it seems to depend in some measure on the length and
thickness of the wire; I can account for these phenomena only by supposing
on November 24th, 1831, contains a complete account of all experimental
methods available for inducing a current in a closed circuit.
While Faraday is entitled to credit for the discovery of current induction
by virtue of the priority of his publication, it must not pass unnoticed that
Henry obtained many of the same experimental results independently and
some even earlier. Henry was at this time instructor in mathematics at the
Albany Academy, and seven hours of teaching a day made it well nigh
impossible to carry on original research except during the vacation month
of August. As early as the summer of 1830 he had wound 30 feet of copper
wire around the armature of a horseshoe electromagnet and connected it to
a galvanometer. When the magnet was excited, a momentary deflection was
observed. “I was, however, much surprised,” he says, “to see the needle
suddenly deflected from a state of rest to about 20° to the east, or in a
contrary direction, when the battery was withdrawn from the acid, and
again deflected to the west when it was re-immersed.” In addition a
deflection was obtained by detaching the armature from the magnet, or by
bringing it again into contact. Had the results of these experiments been
published promptly, America would have been entitled to credit for the
most important discovery of the greatest of England’s many great
experimenters. But Henry desired first to repeat his experiments on a larger
scale, and while new magnets were being constructed, the news of
Faraday’s discovery arrived. This occasioned hasty publication of the work
already done in an appendix to volume 22, 1832, of the Journal.
At almost the same time Henry made another important discovery and
this time he was anticipated by no other investigator in making public his
results. In the paper already referred to be describes the phenomenon
known to-day as self-induction. “When a small battery is moderately
excited by diluted acid and its poles, which must be terminated by cups of
mercury, are connected by a copper wire not more than a foot in length, no
spark is perceived when the connection is either formed or broken; but if a
wire thirty or forty feet long be used, instead of the short wire, though no
spark will be perceptible when the connection is made, yet when it is
broken by drawing one end of the wire from its cup of mercury a vivid
spark is produced.... The effect appears somewhat increased by coiling the
wire into a helix; it seems to depend in some measure on the length and
thickness of the wire; I can account for these phenomena only by supposing
Page 370
the long wire to become charged with electricity which by its reaction on
itself projects a spark when the connection is broken.”
Soon after, Henry went to Princeton and there continued his experiments
in electromagnetism. No difficulty was experienced in inducing currents of
the third, fourth and fifth orders by using the first secondary as primary for
yet another secondary circuit, and so on (38, 209, 1840). The directions of
these currents of higher orders when the primary is made or broken proved
puzzling at first, but were satisfactorily explained a year later (41, 117,
1841). In addition induced currents were obtained from a Leyden jar
discharge. Faraday failed to find any screening effect of a conducting
cylinder placed around the primary and inside the secondary. Henry
examined the matter, and found that the screening effect exists only when
the induced current is due to a make or break of the primary circuit, and not
when it is caused by motion of the primary.
Henry’s work was mainly descriptive; it remained for Faraday to develop
a theory to account for the phenomena discovered and to prepare the way
for quantitative formulation of the laws of current induction. This he did in
his representation of a magnetic field by means of lines of force; a
conception which he found afterwards to be equally valuable when applied
to electrostatic problems. Every magnet and every current gives rise to
these closed curves; in the case of a magnet they thread it from south pole
to north, while a straight wire bearing a current is surrounded by concentric
rings. The connection between lines of force and the induction of currents is
contained in the rule that a current is induced in a closed circuit only when a
change takes place in the number of lines of force passing through it.
Furthermore the dependence of the current strength on the conductivity of
the wire employed has led to recognition of the fact that it is the
electromotive force and not the current itself which is conditioned by the
change in magnetic flux.
Great interest was attached to the utilization of the newly discovered
forces of electromagnetism. In 1831 Henry (20, 340, 1831) described a
reciprocating engine depending on magnetic attraction and repulsion, and
C. G. Page (33, 118, 1838; 49, 131, 1845) devised many others. The latter’s
most important work, however, was the invention of the Ruhmkorff coil. In
1836 (31, 137, 1837) he found the strongest shocks to be obtained, from a
secondary coil of many windings forming a continuation of a primary of
itself projects a spark when the connection is broken.”
Soon after, Henry went to Princeton and there continued his experiments
in electromagnetism. No difficulty was experienced in inducing currents of
the third, fourth and fifth orders by using the first secondary as primary for
yet another secondary circuit, and so on (38, 209, 1840). The directions of
these currents of higher orders when the primary is made or broken proved
puzzling at first, but were satisfactorily explained a year later (41, 117,
1841). In addition induced currents were obtained from a Leyden jar
discharge. Faraday failed to find any screening effect of a conducting
cylinder placed around the primary and inside the secondary. Henry
examined the matter, and found that the screening effect exists only when
the induced current is due to a make or break of the primary circuit, and not
when it is caused by motion of the primary.
Henry’s work was mainly descriptive; it remained for Faraday to develop
a theory to account for the phenomena discovered and to prepare the way
for quantitative formulation of the laws of current induction. This he did in
his representation of a magnetic field by means of lines of force; a
conception which he found afterwards to be equally valuable when applied
to electrostatic problems. Every magnet and every current gives rise to
these closed curves; in the case of a magnet they thread it from south pole
to north, while a straight wire bearing a current is surrounded by concentric
rings. The connection between lines of force and the induction of currents is
contained in the rule that a current is induced in a closed circuit only when a
change takes place in the number of lines of force passing through it.
Furthermore the dependence of the current strength on the conductivity of
the wire employed has led to recognition of the fact that it is the
electromotive force and not the current itself which is conditioned by the
change in magnetic flux.
Great interest was attached to the utilization of the newly discovered
forces of electromagnetism. In 1831 Henry (20, 340, 1831) described a
reciprocating engine depending on magnetic attraction and repulsion, and
C. G. Page (33, 118, 1838; 49, 131, 1845) devised many others. The latter’s
most important work, however, was the invention of the Ruhmkorff coil. In
1836 (31, 137, 1837) he found the strongest shocks to be obtained, from a
secondary coil of many windings forming a continuation of a primary of
Page 371
half the number of turns. His perfection of the self-acting circuit breaker
(35, 252, 1839) widened the usefulness of the induction coil, and his
substitution of a bundle of iron wires for a solid iron core (34, 163, 1838)
greatly increased its efficiency.
Conservation of Energy.—Perhaps the most important advance of the
nineteenth century has been the establishment of the principle of
conservation of energy. Despite the fact that the “principe de la
conservation des force vives” had been recognized by the French
mathematicians of the early part of the century, the application of this
principle even to purely mechanical problems was contested by some
scientists. Through the early numbers of the Journal runs a lively
controversy as to whether there is not a loss of power involved in imparting
momentum to the reciprocating parts of a steam engine only to check the
motion later on in the stroke. Finally Isaac Doolittle (14, 60, 1828), of the
Bennington Iron Works, ends the discussion by the pertinent remark: “If
there be, as is contended by one of your correspondents, a loss of more than
one third of the power, in transforming an alternating rectilinear movement
into a continuous circular one by means of a crank, I should like to be
informed what would be the effect if the proposition were reversed, as in
the case of the common saw mill, and in many other instances in practical
mechanics.”
A realization of the equivalence of heat and mechanical work did not
come until the middle of the century, in spite of the conclusive experiments
of the American Count Rumford and the English Davy before the year
1800. So firmly enthroned was the caloric theory, according to which heat
is an indestructible fluid, that evidence against it was given scant
consideration. In fact the success of the analytical method introduced by
Fourier in 1822 for the solution of problems in conduction of heat only
added to the difficulties of the adherents of the kinetic theory. But
recognition of heat as a form of energy was on the way, and when it came it
made its appearance almost simultaneously in half a dozen different places.
Perhaps Robert Mayer of Heilbronn was the first to state explicitly the new
principle. His paper “On the Forces of Inorganic Nature” was refused
publication in Poggendorff’s Annalen, but fared better at the hands of
another editor. During the next few years Joule determined the mechanical
equivalent of heat experimentally by a number of different methods, some
of which had already been devised by Carnot. Of those he used, the most
(35, 252, 1839) widened the usefulness of the induction coil, and his
substitution of a bundle of iron wires for a solid iron core (34, 163, 1838)
greatly increased its efficiency.
Conservation of Energy.—Perhaps the most important advance of the
nineteenth century has been the establishment of the principle of
conservation of energy. Despite the fact that the “principe de la
conservation des force vives” had been recognized by the French
mathematicians of the early part of the century, the application of this
principle even to purely mechanical problems was contested by some
scientists. Through the early numbers of the Journal runs a lively
controversy as to whether there is not a loss of power involved in imparting
momentum to the reciprocating parts of a steam engine only to check the
motion later on in the stroke. Finally Isaac Doolittle (14, 60, 1828), of the
Bennington Iron Works, ends the discussion by the pertinent remark: “If
there be, as is contended by one of your correspondents, a loss of more than
one third of the power, in transforming an alternating rectilinear movement
into a continuous circular one by means of a crank, I should like to be
informed what would be the effect if the proposition were reversed, as in
the case of the common saw mill, and in many other instances in practical
mechanics.”
A realization of the equivalence of heat and mechanical work did not
come until the middle of the century, in spite of the conclusive experiments
of the American Count Rumford and the English Davy before the year
1800. So firmly enthroned was the caloric theory, according to which heat
is an indestructible fluid, that evidence against it was given scant
consideration. In fact the success of the analytical method introduced by
Fourier in 1822 for the solution of problems in conduction of heat only
added to the difficulties of the adherents of the kinetic theory. But
recognition of heat as a form of energy was on the way, and when it came it
made its appearance almost simultaneously in half a dozen different places.
Perhaps Robert Mayer of Heilbronn was the first to state explicitly the new
principle. His paper “On the Forces of Inorganic Nature” was refused
publication in Poggendorff’s Annalen, but fared better at the hands of
another editor. During the next few years Joule determined the mechanical
equivalent of heat experimentally by a number of different methods, some
of which had already been devised by Carnot. Of those he used, the most
Page 372
familiar consists in churning up a measured mass of water by means of
paddles actuated by falling weights and calculating the heat developed from
the rise in temperature. However, the work of the young Manchester brewer
received little attention from the members of the British Association before
whom it was reported until Kelvin showed them its significance and
attracted their interest to it. Meanwhile Helmholtz had completed a very
thorough disquisition on the conservation of energy not only in dynamics
and heat but in other departments of physics as well. His paper on “Die
Erhaltung der Kraft” was frowned upon by the members of the Physical
Society of Berlin before whom he read it, and received the same treatment
as Mayer’s from the editor of Poggendorff’s Annalen. Helmholtz’s “Kraft,”
like the “vis viva” of other writers, is the quantity which Young had already
christened energy. Not many years elapsed, however, until the convictions
of Mayer, Joule, Kelvin and Helmholtz became the most clearly recognized
of all physical principles. As early as 1850 Jeremiah Day (10, 174, 1850),
late president of Yale College, admitted the improbability of constructing a
machine capable of perpetual motion, even though the “imponderable
agents” of electricity, galvanism and magnetism be utilized.
Thermodynamics.—The importance of the principle of conservation of
energy lies in the fact that it unites under one rule such diverse phenomena
as gravitation, electromagnetism, heat and chemical action. Another
principle as universal in its scope, although depending upon the coarseness
of human observations for its validity rather than upon the immutable laws
of nature, was foreshadowed even before the first law of thermodynamics,
or principle of conservation of energy, was clearly recognized. This second
law was the consequence of efforts to improve the efficiency of heat
engines. In 1824 Carnot introduced the conception of cyclic operations into
the theory of such engines. Assuming the impossibility of perpetual motion,
he showed that no engine can have an efficiency greater than that of a
reversible engine. Finally Clausius expressed concisely the principle toward
which Carnot’s work had been leading, when he asserted that “it is
impossible for a self-acting machine, unaided by any external agency, to
convey heat from one body to another at a higher temperature.” Kelvin’s
formulation of the same law states that “it is impossible, by means of
inanimate material agency, to derive mechanical effect from any portion of
matter by cooling it below the temperature of the coldest of the surrounding
objects.”
paddles actuated by falling weights and calculating the heat developed from
the rise in temperature. However, the work of the young Manchester brewer
received little attention from the members of the British Association before
whom it was reported until Kelvin showed them its significance and
attracted their interest to it. Meanwhile Helmholtz had completed a very
thorough disquisition on the conservation of energy not only in dynamics
and heat but in other departments of physics as well. His paper on “Die
Erhaltung der Kraft” was frowned upon by the members of the Physical
Society of Berlin before whom he read it, and received the same treatment
as Mayer’s from the editor of Poggendorff’s Annalen. Helmholtz’s “Kraft,”
like the “vis viva” of other writers, is the quantity which Young had already
christened energy. Not many years elapsed, however, until the convictions
of Mayer, Joule, Kelvin and Helmholtz became the most clearly recognized
of all physical principles. As early as 1850 Jeremiah Day (10, 174, 1850),
late president of Yale College, admitted the improbability of constructing a
machine capable of perpetual motion, even though the “imponderable
agents” of electricity, galvanism and magnetism be utilized.
Thermodynamics.—The importance of the principle of conservation of
energy lies in the fact that it unites under one rule such diverse phenomena
as gravitation, electromagnetism, heat and chemical action. Another
principle as universal in its scope, although depending upon the coarseness
of human observations for its validity rather than upon the immutable laws
of nature, was foreshadowed even before the first law of thermodynamics,
or principle of conservation of energy, was clearly recognized. This second
law was the consequence of efforts to improve the efficiency of heat
engines. In 1824 Carnot introduced the conception of cyclic operations into
the theory of such engines. Assuming the impossibility of perpetual motion,
he showed that no engine can have an efficiency greater than that of a
reversible engine. Finally Clausius expressed concisely the principle toward
which Carnot’s work had been leading, when he asserted that “it is
impossible for a self-acting machine, unaided by any external agency, to
convey heat from one body to another at a higher temperature.” Kelvin’s
formulation of the same law states that “it is impossible, by means of
inanimate material agency, to derive mechanical effect from any portion of
matter by cooling it below the temperature of the coldest of the surrounding
objects.”
Page 373
The consequences of the second law were rapidly developed by Kelvin,
Clausius, Rankine, Barnard (16, 218, 1853, et seq.) and others. Kelvin
introduced the thermodynamic scale of temperature, which he showed to be
independent of such properties of matter as condition the size of the degree
indicated by the mercury thermometer. This scale, which is equivalent to
that of the ideal gas thermometer, was used subsequently by Rowland in his
exhaustive determination of the mechanical equivalent of heat by an
improved form of Joule’s method. He found different values for different
ranges in temperature, showing that the specific heat of water is by no
means constant. Since then electrical methods of measuring this important
quantity have been used to confirm the results of purely mechanical
determinations.
The definition of a new quantity, entropy, was found necessary for a
mathematical formulation of the second law of thermodynamics. This
quantity, which acts as a measure of the unavailability of heat energy, was
given a new significance when Boltzmann showed its connection with the
probability of the thermodynamic state of the substance under
consideration. If two bodies have widely different temperatures, a large
amount of the heat energy of the system is available for conversion into
mechanical work. From the macroscopic point of view this is expressed by
saying that the entropy is small, or if the motions of the individual
molecules are taken into account, the probability of the state is low. The
interpretation of entropy as the logarithm of the thermodynamic probability
has thrown much light on the meaning of this rather abstruse quantity.
Gibbs’s “Elementary Principles in Statistical Mechanics” treats in detail the
fundamental assumptions involved in this point of view, its limitations and
its consequences. In his “Equilibrium of Heterogeneous Substances”[154] he
had already extended the principle of thermal equilibrium to include
substances which are no longer homogeneous. The value of the chemical
potential he introduced determines whether one phase is to gain at the
expense of another or lose to it. It is unfortunate that the analytical rigor and
austerity of his reasoning combined with lack of mathematical training on
the part of the average chemist, delayed true appreciation of his work and
full utilization of the new field which he opened up.
Liquefaction of Gases.—Meanwhile the problem of liquefying gases was
attracting much attention on the part of experimental physicists. Faraday
had succeeded in making liquid a number of substances which had hitherto
Clausius, Rankine, Barnard (16, 218, 1853, et seq.) and others. Kelvin
introduced the thermodynamic scale of temperature, which he showed to be
independent of such properties of matter as condition the size of the degree
indicated by the mercury thermometer. This scale, which is equivalent to
that of the ideal gas thermometer, was used subsequently by Rowland in his
exhaustive determination of the mechanical equivalent of heat by an
improved form of Joule’s method. He found different values for different
ranges in temperature, showing that the specific heat of water is by no
means constant. Since then electrical methods of measuring this important
quantity have been used to confirm the results of purely mechanical
determinations.
The definition of a new quantity, entropy, was found necessary for a
mathematical formulation of the second law of thermodynamics. This
quantity, which acts as a measure of the unavailability of heat energy, was
given a new significance when Boltzmann showed its connection with the
probability of the thermodynamic state of the substance under
consideration. If two bodies have widely different temperatures, a large
amount of the heat energy of the system is available for conversion into
mechanical work. From the macroscopic point of view this is expressed by
saying that the entropy is small, or if the motions of the individual
molecules are taken into account, the probability of the state is low. The
interpretation of entropy as the logarithm of the thermodynamic probability
has thrown much light on the meaning of this rather abstruse quantity.
Gibbs’s “Elementary Principles in Statistical Mechanics” treats in detail the
fundamental assumptions involved in this point of view, its limitations and
its consequences. In his “Equilibrium of Heterogeneous Substances”[154] he
had already extended the principle of thermal equilibrium to include
substances which are no longer homogeneous. The value of the chemical
potential he introduced determines whether one phase is to gain at the
expense of another or lose to it. It is unfortunate that the analytical rigor and
austerity of his reasoning combined with lack of mathematical training on
the part of the average chemist, delayed true appreciation of his work and
full utilization of the new field which he opened up.
Liquefaction of Gases.—Meanwhile the problem of liquefying gases was
attracting much attention on the part of experimental physicists. Faraday
had succeeded in making liquid a number of substances which had hitherto
Page 374
been known only in the gaseous state. His method consists in evolving the
gas from chemicals placed in one end of a bent tube, the other end of which
is immersed in a freezing mixture. The high pressure caused by the
production of the gas combined with the low temperature is sufficient to
bring about liquefaction in many cases. Failure with other more permanent
gases was unexplained until the researches of Andrews in 1863 showed that
no amount of pressure will produce liquefaction unless the temperature is
below a certain critical value. The method of reducing the temperature in
use to-day depends on a fact discovered by Kelvin and Joule in connection
with the free expansion of a gas. These investigators allowed the gas to
escape through a porous plug from a chamber in which the pressure was
relatively high. With the single exception of hydrogen, the effect of the
sudden expansion is to cool the gas, and even with it cooling is found to
take place after the temperature has been made sufficiently low. By this
method all known gases have been liquefied. Helium, with a boiling point
of –269°C, or only 4°C. above the absolute zero, was the last to be made a
liquid, finally yielding to the efforts of Kammerlingh Onnes in 1907. This
investigator[155] finds that at temperatures near the absolute zero the
electrical conductivity of certain substances undergoes a profound
modification. For example, a coil of lead shows a superconductivity so
great that a current once started in it persists for days after the electromotive
force has ceased to act.
Electrodynamics.—Faraday’s representation of electric and magnetic
fields by lines of force had been of great value in predicting the results of
experiments in electromagnetism. But a more mathematical formulation of
the laws governing these phenomena was needed in order to make possible
quantitative development of the theory. This was supplied by Maxwell in
his epoch-making treatise on “Electricity and Magnetism.” Starting with
electrostatics and magnetism, he gives a complete account of the
mathematical methods which had been devised for the solution of problems
in these branches of the subject, and then turning to Ampère’s work he
shows how the Lagrangian equations of motion lead to Faraday’s law if the
single assumption is made that the magnetic energy of the field is kinetic. In
the treatment of open circuits Maxwell’s intuition led to a great advance, the
introduction of the displacement current. Consider a charged condenser, the
plates of which are suddenly connected by a wire. A current will flow
through the wire from the positively charged plate to the negative, but in the
gas from chemicals placed in one end of a bent tube, the other end of which
is immersed in a freezing mixture. The high pressure caused by the
production of the gas combined with the low temperature is sufficient to
bring about liquefaction in many cases. Failure with other more permanent
gases was unexplained until the researches of Andrews in 1863 showed that
no amount of pressure will produce liquefaction unless the temperature is
below a certain critical value. The method of reducing the temperature in
use to-day depends on a fact discovered by Kelvin and Joule in connection
with the free expansion of a gas. These investigators allowed the gas to
escape through a porous plug from a chamber in which the pressure was
relatively high. With the single exception of hydrogen, the effect of the
sudden expansion is to cool the gas, and even with it cooling is found to
take place after the temperature has been made sufficiently low. By this
method all known gases have been liquefied. Helium, with a boiling point
of –269°C, or only 4°C. above the absolute zero, was the last to be made a
liquid, finally yielding to the efforts of Kammerlingh Onnes in 1907. This
investigator[155] finds that at temperatures near the absolute zero the
electrical conductivity of certain substances undergoes a profound
modification. For example, a coil of lead shows a superconductivity so
great that a current once started in it persists for days after the electromotive
force has ceased to act.
Electrodynamics.—Faraday’s representation of electric and magnetic
fields by lines of force had been of great value in predicting the results of
experiments in electromagnetism. But a more mathematical formulation of
the laws governing these phenomena was needed in order to make possible
quantitative development of the theory. This was supplied by Maxwell in
his epoch-making treatise on “Electricity and Magnetism.” Starting with
electrostatics and magnetism, he gives a complete account of the
mathematical methods which had been devised for the solution of problems
in these branches of the subject, and then turning to Ampère’s work he
shows how the Lagrangian equations of motion lead to Faraday’s law if the
single assumption is made that the magnetic energy of the field is kinetic. In
the treatment of open circuits Maxwell’s intuition led to a great advance, the
introduction of the displacement current. Consider a charged condenser, the
plates of which are suddenly connected by a wire. A current will flow
through the wire from the positively charged plate to the negative, but in the
Page 375
gap between the two plates the conduction current is missing. So convinced
was Maxwell that currents must always flow in closed circuits, that he
postulated an electrical displacement in the medium between the plates of a
charged condenser, which disappears when the condenser is short-circuited.
Thus even in the so-called open circuit the current flows along a closed
path.
Maxwell’s theory of the electromagnetic field is based essentially on
Faraday’s representation by lines of force of the strains and stresses of a
universal medium. So it is not surprising that he was led to a consideration
of the propagation of waves through this medium. The introduction of the
displacement current made the form of the electrodynamic equations such
as to yield a typical wave equation for space free from electrical charges
and currents. Moreover, the disturbance was found to be transverse, and its
velocity turned out to be identical with that of light. The conclusion was
irresistible. That light could consist of anything but electromagnetic waves
of extremely short length was inconceivable. In fact so certain was Maxwell
of this deduction from theory that he felt it altogether unnecessary to resort
to the test of experiment. For the electromagnetic theory explained so many
of the details which had been revealed by experiments in light, that no
doubt of its validity could be entertained. Even dispersion received ready
elucidation on the assumption that the dispersing medium is made up of
vibrators having a natural period comparable with that of the light passing
through it.
was Maxwell that currents must always flow in closed circuits, that he
postulated an electrical displacement in the medium between the plates of a
charged condenser, which disappears when the condenser is short-circuited.
Thus even in the so-called open circuit the current flows along a closed
path.
Maxwell’s theory of the electromagnetic field is based essentially on
Faraday’s representation by lines of force of the strains and stresses of a
universal medium. So it is not surprising that he was led to a consideration
of the propagation of waves through this medium. The introduction of the
displacement current made the form of the electrodynamic equations such
as to yield a typical wave equation for space free from electrical charges
and currents. Moreover, the disturbance was found to be transverse, and its
velocity turned out to be identical with that of light. The conclusion was
irresistible. That light could consist of anything but electromagnetic waves
of extremely short length was inconceivable. In fact so certain was Maxwell
of this deduction from theory that he felt it altogether unnecessary to resort
to the test of experiment. For the electromagnetic theory explained so many
of the details which had been revealed by experiments in light, that no
doubt of its validity could be entertained. Even dispersion received ready
elucidation on the assumption that the dispersing medium is made up of
vibrators having a natural period comparable with that of the light passing
through it.
Page 376
Maxwell’s book was published in 1873. Fifteen years later, Hertz,[156] at
the instigation of Helmholtz, succeeded in detecting experimentally the
electromagnetic waves predicted by Maxwell’s theory. His oscillator
consisted of two sheets of metal in the same plane, to each of which was
attached a short wire terminating in a knob. The knobs were placed within a
short distance of each other, and connected to the terminals of an induction
coil. By reflection standing waves were formed, and the positions of nodes
and loops determined by a detector composed of a movable loop of wire
containing an air gap. Thus the wave length was measured. Hertz calculated
the frequency of his radiator from its dimensions, and then computed the
velocity of the disturbance. In spite of an error in his calculations, later
the instigation of Helmholtz, succeeded in detecting experimentally the
electromagnetic waves predicted by Maxwell’s theory. His oscillator
consisted of two sheets of metal in the same plane, to each of which was
attached a short wire terminating in a knob. The knobs were placed within a
short distance of each other, and connected to the terminals of an induction
coil. By reflection standing waves were formed, and the positions of nodes
and loops determined by a detector composed of a movable loop of wire
containing an air gap. Thus the wave length was measured. Hertz calculated
the frequency of his radiator from its dimensions, and then computed the
velocity of the disturbance. In spite of an error in his calculations, later
Page 377
pointed out by Poincaré, he obtained very nearly the velocity of light for
waves traveling through air, but a velocity considerably smaller for those
propagated along wires. Subsequent work by Lecher, Sarasin and de la
Rive, and Trowbridge and Duane (49, 297, 1895; 50, 104, 1895) cleared up
this discrepancy, and showed the velocity to be in both cases identical with
that of light. The last-named investigators increased the size of the oscillator
until it was possible to measure the frequency by photographing the spark
in the secondary with a rotating mirror. The positions of nodes and loops
were obtained by means of a bolometer after the secondary had been tuned
to resonance with the vibrator. The velocity thus found for electromagnetic
waves along wires is within one-tenth of one percent of the accepted value
of the velocity of light. Hertz’s later experiments showed that waves in air
suffer refraction and diffraction, and he succeeded in polarizing the
radiation by passing it through a grating constructed of parallel metallic
wires.
In order to satisfy the law of action and reaction, it is found necessary to
attribute a quasi-momentum to electromagnetic waves. When a train of such
waves is absorbed, their momentum is transferred to the absorbing body,
while if they are reflected an impulse twice as great is imparted. This
consequence of theory, foreseen by Maxwell and developed in detail by
Poynting, Abraham and Larmor, has been verified by the experiments of
Lebedew, and Nichols and Hull.[157] The latter used a delicate torsion
balance from which was suspended a couple of silvered glass vanes. In
order to eliminate the effect of impulses imparted by the molecules of the
residual gas, such as Crookes had observed in his radiometer, readings were
made at many different pressures and the ballistic rather than the static
deflection recorded. After the pressure produced by light from a carbon arc
had been measured, the intensity of the radiation was determined with a
bolometer. Preliminary experiments indicated the existence of a pressure of
the order expected, and later more careful measurements showed good
quantitative agreement with theory. This pressure had already found an
important application in Lebedew’s explanation of the solar repulsion of
comet’s tails. These tails are made up of enormous swarms of very minute
particles, and as the comet swings around the sun they suffer a repulsion
due to the pressure of the intense solar radiation which counteracts the sun’s
gravitational attraction. Hence the tail, instead of following after the comet
in its orbit, points in a direction away from the sun.
waves traveling through air, but a velocity considerably smaller for those
propagated along wires. Subsequent work by Lecher, Sarasin and de la
Rive, and Trowbridge and Duane (49, 297, 1895; 50, 104, 1895) cleared up
this discrepancy, and showed the velocity to be in both cases identical with
that of light. The last-named investigators increased the size of the oscillator
until it was possible to measure the frequency by photographing the spark
in the secondary with a rotating mirror. The positions of nodes and loops
were obtained by means of a bolometer after the secondary had been tuned
to resonance with the vibrator. The velocity thus found for electromagnetic
waves along wires is within one-tenth of one percent of the accepted value
of the velocity of light. Hertz’s later experiments showed that waves in air
suffer refraction and diffraction, and he succeeded in polarizing the
radiation by passing it through a grating constructed of parallel metallic
wires.
In order to satisfy the law of action and reaction, it is found necessary to
attribute a quasi-momentum to electromagnetic waves. When a train of such
waves is absorbed, their momentum is transferred to the absorbing body,
while if they are reflected an impulse twice as great is imparted. This
consequence of theory, foreseen by Maxwell and developed in detail by
Poynting, Abraham and Larmor, has been verified by the experiments of
Lebedew, and Nichols and Hull.[157] The latter used a delicate torsion
balance from which was suspended a couple of silvered glass vanes. In
order to eliminate the effect of impulses imparted by the molecules of the
residual gas, such as Crookes had observed in his radiometer, readings were
made at many different pressures and the ballistic rather than the static
deflection recorded. After the pressure produced by light from a carbon arc
had been measured, the intensity of the radiation was determined with a
bolometer. Preliminary experiments indicated the existence of a pressure of
the order expected, and later more careful measurements showed good
quantitative agreement with theory. This pressure had already found an
important application in Lebedew’s explanation of the solar repulsion of
comet’s tails. These tails are made up of enormous swarms of very minute
particles, and as the comet swings around the sun they suffer a repulsion
due to the pressure of the intense solar radiation which counteracts the sun’s
gravitational attraction. Hence the tail, instead of following after the comet
in its orbit, points in a direction away from the sun.
Page 378
Some uncertainty existed as to whether a convection current produces a
magnetic field. A compass needle is deflected by a current from a Daniell
cell; is the same effect obtained when a conductor is charged
electrostatically and then whirled around the needle by means of an
insulating handle? The experimental difficulties involved in settling this
question are realized when the enormous difference between the
electrostatic and electromagnetic units of current is taken into
consideration. For a sphere one centimeter in radius, charged to a potential
of 20,000 volts, and revolving in a circle sixty times a second, constitutes a
current of little over a millionth of an ampere.
This problem was undertaken by Rowland (15, 30, 1878) in Helmholtz’s
laboratory at Berlin in 1876. A hard rubber disk coated on both sides with
gold was charged and rotated about a vertical axis at a rate of sixty
revolutions a second. On reversing the sign of the electrification on the
disk, the astatic needle hung above its center showed a deflection of over
five millimeters. The current was calculated in electrostatic units from the
charge on the disk and its rate of motion, and in electromagnetic units from
the magnetic deflection. The ratio of these two quantities gave fair
agreement with its theoretical value, the velocity of light.
Although the result of this experiment was confirmed by Rowland and
Hutchinson in 1889, Crémieu was convinced by an investigation carried out
at Paris in 1900 that the Rowland effect did not exist. Consequently further
repetition of the experiment was desirable. So the following year Adams
(12, 155, 1901) arranged two rings of eight spheres each so that they could
be rotated about their common axis from fifty to sixty times a second. One
set of spheres was connected by brushes to the positive pole of a battery of
20,000 volts, the other to the negative pole. The deflection of a nearby
magnetometer needle was observed when the electrification of the two rings
was reversed, and from the reading so obtained the ratio of the
electromagnetic to the electrostatic unit of current computed. This quantity
was found to differ from the velocity of light by only a few percent. This
experiment and the even more exhaustive investigations carried out by
Pender, both independently and in collaboration with Crémieu, finally
convinced the scientific world that a convection current produces the same
magnetic field as a conduction current of the same magnitude.
magnetic field. A compass needle is deflected by a current from a Daniell
cell; is the same effect obtained when a conductor is charged
electrostatically and then whirled around the needle by means of an
insulating handle? The experimental difficulties involved in settling this
question are realized when the enormous difference between the
electrostatic and electromagnetic units of current is taken into
consideration. For a sphere one centimeter in radius, charged to a potential
of 20,000 volts, and revolving in a circle sixty times a second, constitutes a
current of little over a millionth of an ampere.
This problem was undertaken by Rowland (15, 30, 1878) in Helmholtz’s
laboratory at Berlin in 1876. A hard rubber disk coated on both sides with
gold was charged and rotated about a vertical axis at a rate of sixty
revolutions a second. On reversing the sign of the electrification on the
disk, the astatic needle hung above its center showed a deflection of over
five millimeters. The current was calculated in electrostatic units from the
charge on the disk and its rate of motion, and in electromagnetic units from
the magnetic deflection. The ratio of these two quantities gave fair
agreement with its theoretical value, the velocity of light.
Although the result of this experiment was confirmed by Rowland and
Hutchinson in 1889, Crémieu was convinced by an investigation carried out
at Paris in 1900 that the Rowland effect did not exist. Consequently further
repetition of the experiment was desirable. So the following year Adams
(12, 155, 1901) arranged two rings of eight spheres each so that they could
be rotated about their common axis from fifty to sixty times a second. One
set of spheres was connected by brushes to the positive pole of a battery of
20,000 volts, the other to the negative pole. The deflection of a nearby
magnetometer needle was observed when the electrification of the two rings
was reversed, and from the reading so obtained the ratio of the
electromagnetic to the electrostatic unit of current computed. This quantity
was found to differ from the velocity of light by only a few percent. This
experiment and the even more exhaustive investigations carried out by
Pender, both independently and in collaboration with Crémieu, finally
convinced the scientific world that a convection current produces the same
magnetic field as a conduction current of the same magnitude.
Page 379
In discussing the ponderomotive force experienced in a magnetic field by
a conductor through which a current is passing, Maxwell had said, “It must
be carefully remembered, that the mechanical force which urges a
conductor carrying a current across the lines of magnetic force, acts, not on
the electric current, but on the conductor which carries it.” Hall (19, 200,
1880), one of Rowland’s students, questioned this statement, and
determined to put it to the test of experiment. Efforts to find an increase in
the resistance of a wire placed at right angles to the lines of magnetic force
were unsuccessful. So the current was passed through a moderately broad
strip of gold leaf and the effect of the magnetic field on the equipotential
lines investigated. The results obtained confirmed Hall’s belief that the
force exerted by the field acts on the current itself, and is transmitted
through it to the conductor. Further investigation (20, 161, 1880) revealed
the same deflection of equipotential lines in thin strips of other metals,
although the effect was found to be reversed in iron.
During the closing years of the nineteenth century occurred three events
of far reaching importance. The electron was isolated, and its charge and
mass measured by J. J. Thomson in England; X-rays were discovered by
Röntgen in Germany; and the first indications of radioactivity were found
by Becquerel in France. The first two are certainly to be attributed largely to
the great advances which had been made in obtaining high vacua, and the
last two might not have occurred so soon had it not been for the
photographic plate.
The Electron.—The atomic theory of electricity dates from the time of
Faraday. His experiments on electrolysis showed that each monovalent
atom or radical, whatever its nature, carries the same charge, each bivalent
ion a charge twice as great. Only a lack of knowledge of the number of
atoms in a gram of the dissociated salt prevented him from calculating the
value of the elementary charge. As the discharge of electricity through gases
at low pressures became a subject for experimental investigation, another
line of approach to the study of the atom of electricity was opened up. As
early as the seventies Hittorf and Goldstein had observed that a shadow is
cast by a screen placed in front of the cathode of a Crookes tube. Varley
suggested that the cathode rays producing the shadow consist of “attenuated
particles of matter, projected from the negative pole by electricity.” The
discovery that these rays are deflected by a magnetic field led English
physicists to the conclusion that they must be composed of charged
a conductor through which a current is passing, Maxwell had said, “It must
be carefully remembered, that the mechanical force which urges a
conductor carrying a current across the lines of magnetic force, acts, not on
the electric current, but on the conductor which carries it.” Hall (19, 200,
1880), one of Rowland’s students, questioned this statement, and
determined to put it to the test of experiment. Efforts to find an increase in
the resistance of a wire placed at right angles to the lines of magnetic force
were unsuccessful. So the current was passed through a moderately broad
strip of gold leaf and the effect of the magnetic field on the equipotential
lines investigated. The results obtained confirmed Hall’s belief that the
force exerted by the field acts on the current itself, and is transmitted
through it to the conductor. Further investigation (20, 161, 1880) revealed
the same deflection of equipotential lines in thin strips of other metals,
although the effect was found to be reversed in iron.
During the closing years of the nineteenth century occurred three events
of far reaching importance. The electron was isolated, and its charge and
mass measured by J. J. Thomson in England; X-rays were discovered by
Röntgen in Germany; and the first indications of radioactivity were found
by Becquerel in France. The first two are certainly to be attributed largely to
the great advances which had been made in obtaining high vacua, and the
last two might not have occurred so soon had it not been for the
photographic plate.
The Electron.—The atomic theory of electricity dates from the time of
Faraday. His experiments on electrolysis showed that each monovalent
atom or radical, whatever its nature, carries the same charge, each bivalent
ion a charge twice as great. Only a lack of knowledge of the number of
atoms in a gram of the dissociated salt prevented him from calculating the
value of the elementary charge. As the discharge of electricity through gases
at low pressures became a subject for experimental investigation, another
line of approach to the study of the atom of electricity was opened up. As
early as the seventies Hittorf and Goldstein had observed that a shadow is
cast by a screen placed in front of the cathode of a Crookes tube. Varley
suggested that the cathode rays producing the shadow consist of “attenuated
particles of matter, projected from the negative pole by electricity.” The
discovery that these rays are deflected by a magnetic field led English
physicists to the conclusion that they must be composed of charged
Page 380
particles, and the direction of the deflection was such as to require the
charge to be negative. Hertz contested this view on the ground that his
experiments showed the rays to be unaffected by an electrostatic field, and
suggested that they consist of etherial disturbances. Finally Perrin
succeeded in passing the rays into a metal cylinder which received from
them a negative charge, and Lenard showed how excessively minute these
negatively charged particles must be by actually passing them through a
thin sheet of aluminium in the wall of a vacuum tube, and detecting their
presence in the air outside. Conclusive information as to the nature of the
electron, as it was named by Johnstone Stoney, was supplied by the classic
experiments of J. J. Thomson.[158] First he showed that Hertz’s failure to find
a deflection when a stream of electrons passes between the plates of a
charged condenser was due to the screening effect of the gaseous ions
produced by the discharge. With a much more highly evacuated tube he
found no difficulty in obtaining a deflection in an electrostatic field. By
using crossed electric and magnetic fields the deflection produced by one
was just balanced by that caused by the other, and from the field strengths
employed both the velocity of the particles and the ratio me of charge to mass
was calculated. The former was found to be about one-tenth the velocity of
light, but the most startling result of the experiment was that the same value
of me was obtained no matter what residual gas was contained in the tube or
of what metal the cathode was made.
To calculate e and then m other methods are necessary. C. T. R. Wilson
has shown that in supersaturated air, water drops form easily on charged
molecules, and that negative ions are more effective in causing
condensation than positive ones. By making use of the results of this
research Thomson has been able to measure the elementary charge. For
suppose a stream of negative ions to pass through supersaturated air. A little
drop forms on each charged particle, and the cloud of condensed vapor
settles to the bottom of the vessel. The charge carried and the mass of water
deposited can be measured directly. Stokes’ law for the rate of fall of a
minute particle through a gaseous medium enables the average size of the
drops to be computed from the observed rate of descent of the cloud. Hence
the number of drops formed and the charge carried by each follows at once.
H. A. Wilson improved the method by noting the effect of an electric field
upon the rate of fall of the charged drops, and subsequent experiments
undertaken by Millikan[159] have been of such a character as to enable him to
charge to be negative. Hertz contested this view on the ground that his
experiments showed the rays to be unaffected by an electrostatic field, and
suggested that they consist of etherial disturbances. Finally Perrin
succeeded in passing the rays into a metal cylinder which received from
them a negative charge, and Lenard showed how excessively minute these
negatively charged particles must be by actually passing them through a
thin sheet of aluminium in the wall of a vacuum tube, and detecting their
presence in the air outside. Conclusive information as to the nature of the
electron, as it was named by Johnstone Stoney, was supplied by the classic
experiments of J. J. Thomson.[158] First he showed that Hertz’s failure to find
a deflection when a stream of electrons passes between the plates of a
charged condenser was due to the screening effect of the gaseous ions
produced by the discharge. With a much more highly evacuated tube he
found no difficulty in obtaining a deflection in an electrostatic field. By
using crossed electric and magnetic fields the deflection produced by one
was just balanced by that caused by the other, and from the field strengths
employed both the velocity of the particles and the ratio me of charge to mass
was calculated. The former was found to be about one-tenth the velocity of
light, but the most startling result of the experiment was that the same value
of me was obtained no matter what residual gas was contained in the tube or
of what metal the cathode was made.
To calculate e and then m other methods are necessary. C. T. R. Wilson
has shown that in supersaturated air, water drops form easily on charged
molecules, and that negative ions are more effective in causing
condensation than positive ones. By making use of the results of this
research Thomson has been able to measure the elementary charge. For
suppose a stream of negative ions to pass through supersaturated air. A little
drop forms on each charged particle, and the cloud of condensed vapor
settles to the bottom of the vessel. The charge carried and the mass of water
deposited can be measured directly. Stokes’ law for the rate of fall of a
minute particle through a gaseous medium enables the average size of the
drops to be computed from the observed rate of descent of the cloud. Hence
the number of drops formed and the charge carried by each follows at once.
H. A. Wilson improved the method by noting the effect of an electric field
upon the rate of fall of the charged drops, and subsequent experiments
undertaken by Millikan[159] have been of such a character as to enable him to
Page 381
follow the motion of a single drop. Instead of water, the latter uses oil drops
less than one ten-thousandth of a centimeter in diameter. A drop, after one
or more electrons have attached themselves to it, is actually weighed in
terms of the charge on its surface by applying an upward electric force just
sufficient to balance the force of gravity. Then its weight is independently
obtained from the density of the oil and the radius of the drop as determined
by the rate of fall when the electric field is absent. Comparison of these two
expressions gives 4·774(10)–10 electrostatic units for the elementary charge.
Combining this result with the value of me found by Thomson, the mass of
the electron comes out to be about one eighteen-hundredth that of an atom
of the lightest known element, hydrogen.
That the electron is a fundamental constituent of all matter is attested by
the fact that charge and mass are the same regardless of the source or
manner of production. Whether emitted by a heated metal, under the action
of ultra-violet light, from a radioactive substance, by a body exposed to X-
rays, as a result of friction, it is the same negatively charged particle that
constitutes the cathode ray of the discharge tube. Moreover, it makes its
effect felt indirectly in many other phenomena, and from an investigation of
some of these the ratio of charge to mass can be determined independently.
Of such perhaps the most interesting is the Zeeman effect.
Spectroscopy.—Early in the nineteenth century Fraunhofer had observed
that the solar spectrum is crossed by a large number of dark lines. Their
presence was unexplained until in 1859 Kirchhoff and Bunsen showed “that
a colored flame, the spectrum of which contains bright sharp lines, so
weakens rays of the color of these lines when they pass through it, that dark
lines appear in place of bright lines as soon as there is placed behind the
flame a light of sufficient intensity, in which the lines are otherwise absent.”
For intra-atomic oscillators must have the natural frequency of the radiation
which they emit, and consequently resonance will take place when they are
exposed to rays of this frequency coming from an outside source, and
selective absorption ensue. By comparing the bright lines in the spectra of
metallic vapors made luminous by a gas flame with the dark lines in the
sun’s spectrum these investigators showed that many of the common
terrestrial elements exist in the sun. The interest in spectroscopy grew
rapidly. The excellent diffraction gratings made by Rutherfurd were
succeeded by the superior concave gratings of Rowland. In 1877 Draper
(14, 89, 1877) announced the discovery of the bright lines of oxygen in the
less than one ten-thousandth of a centimeter in diameter. A drop, after one
or more electrons have attached themselves to it, is actually weighed in
terms of the charge on its surface by applying an upward electric force just
sufficient to balance the force of gravity. Then its weight is independently
obtained from the density of the oil and the radius of the drop as determined
by the rate of fall when the electric field is absent. Comparison of these two
expressions gives 4·774(10)–10 electrostatic units for the elementary charge.
Combining this result with the value of me found by Thomson, the mass of
the electron comes out to be about one eighteen-hundredth that of an atom
of the lightest known element, hydrogen.
That the electron is a fundamental constituent of all matter is attested by
the fact that charge and mass are the same regardless of the source or
manner of production. Whether emitted by a heated metal, under the action
of ultra-violet light, from a radioactive substance, by a body exposed to X-
rays, as a result of friction, it is the same negatively charged particle that
constitutes the cathode ray of the discharge tube. Moreover, it makes its
effect felt indirectly in many other phenomena, and from an investigation of
some of these the ratio of charge to mass can be determined independently.
Of such perhaps the most interesting is the Zeeman effect.
Spectroscopy.—Early in the nineteenth century Fraunhofer had observed
that the solar spectrum is crossed by a large number of dark lines. Their
presence was unexplained until in 1859 Kirchhoff and Bunsen showed “that
a colored flame, the spectrum of which contains bright sharp lines, so
weakens rays of the color of these lines when they pass through it, that dark
lines appear in place of bright lines as soon as there is placed behind the
flame a light of sufficient intensity, in which the lines are otherwise absent.”
For intra-atomic oscillators must have the natural frequency of the radiation
which they emit, and consequently resonance will take place when they are
exposed to rays of this frequency coming from an outside source, and
selective absorption ensue. By comparing the bright lines in the spectra of
metallic vapors made luminous by a gas flame with the dark lines in the
sun’s spectrum these investigators showed that many of the common
terrestrial elements exist in the sun. The interest in spectroscopy grew
rapidly. The excellent diffraction gratings made by Rutherfurd were
succeeded by the superior concave gratings of Rowland. In 1877 Draper
(14, 89, 1877) announced the discovery of the bright lines of oxygen in the
Page 382
solar spectrum, but his interpretation of his photographs has not been
corroborated by the work of later investigators. Langley (11, 401, 1901), by
the aid of his newly invented bolometer, succeeded in detecting the
emission of energy from the sun in the infra-red in amounts far exceeding
that contained in the visible spectrum. In 1842 Doppler drew attention to
the fact that motion of the source should cause a displacement of the
spectral lines, the shift being to the blue if the light is approaching and to
the red if it is receding, and a few years later Fizeau suggested the
application of Doppler’s principle to the measurement of the velocity of a
star moving in the line of sight. Thus the spectroscope has been able to
supply one of the deficiencies of the telescope, and the two together are
sufficient to reveal all components of stellar motion. When spectra formed
by light from the sun’s limb and from its center are compared, the same
effect reveals the rotation of the sun about its axis. (C. S. Hastings, 5, 369,
1873; C. A. Young, 12, 321, 1876.)
Further Evidence of the Electron.—In 1845 Faraday discovered a
rotation of the plane of polarization when light passes in the direction of the
lines of force through a piece of glass placed between the poles of an
electromagnet. Examination of the spectrum from a glowing vapor situated
between the poles of a magnet, however, failed to reveal any effect of the
field. The latter problem was attacked anew by Zeeman[160] in 1896, and
with the aid of the improved appliances of modern science he succeeded in
detecting a broadening of the lines. Later experiments with more powerful
apparatus resolved these broadening lines into several components.
Lorentz[161] showed at once how the electron theory furnishes an
explanation of the Zeeman effect. He found that when the source is viewed
at right angles to the lines of magnetic force, a spectral line should be split
into three components. Of these he predicted that the middle, or undisplaced
component, would be found to be polarized at right angles to the direction
of the field, and the other components parallel to the field. When the light
proceeds from the source in a direction parallel to the magnetic lines of
force, two components only should be formed, and these should be
circularly polarized in opposite senses. Moreover, from the separation of the
components can be calculated the ratio of charge to mass of the electronic
vibrator which is responsible for the emission of radiant energy. Zeeman’s
experiments confirmed Lorentz’s theory in every detail, and yielded a value
of me in substantial agreement with that obtained for cathode rays.
corroborated by the work of later investigators. Langley (11, 401, 1901), by
the aid of his newly invented bolometer, succeeded in detecting the
emission of energy from the sun in the infra-red in amounts far exceeding
that contained in the visible spectrum. In 1842 Doppler drew attention to
the fact that motion of the source should cause a displacement of the
spectral lines, the shift being to the blue if the light is approaching and to
the red if it is receding, and a few years later Fizeau suggested the
application of Doppler’s principle to the measurement of the velocity of a
star moving in the line of sight. Thus the spectroscope has been able to
supply one of the deficiencies of the telescope, and the two together are
sufficient to reveal all components of stellar motion. When spectra formed
by light from the sun’s limb and from its center are compared, the same
effect reveals the rotation of the sun about its axis. (C. S. Hastings, 5, 369,
1873; C. A. Young, 12, 321, 1876.)
Further Evidence of the Electron.—In 1845 Faraday discovered a
rotation of the plane of polarization when light passes in the direction of the
lines of force through a piece of glass placed between the poles of an
electromagnet. Examination of the spectrum from a glowing vapor situated
between the poles of a magnet, however, failed to reveal any effect of the
field. The latter problem was attacked anew by Zeeman[160] in 1896, and
with the aid of the improved appliances of modern science he succeeded in
detecting a broadening of the lines. Later experiments with more powerful
apparatus resolved these broadening lines into several components.
Lorentz[161] showed at once how the electron theory furnishes an
explanation of the Zeeman effect. He found that when the source is viewed
at right angles to the lines of magnetic force, a spectral line should be split
into three components. Of these he predicted that the middle, or undisplaced
component, would be found to be polarized at right angles to the direction
of the field, and the other components parallel to the field. When the light
proceeds from the source in a direction parallel to the magnetic lines of
force, two components only should be formed, and these should be
circularly polarized in opposite senses. Moreover, from the separation of the
components can be calculated the ratio of charge to mass of the electronic
vibrator which is responsible for the emission of radiant energy. Zeeman’s
experiments confirmed Lorentz’s theory in every detail, and yielded a value
of me in substantial agreement with that obtained for cathode rays.
Page 383
Subsequent research, however, has shown that in many cases more
components are found than the elementary theory calls for. Hale has
detected the Zeeman effect in light from sun spots, proving that these
blemishes on the sun’s face are vortices caused by whirling swarms of
electrified particles. Recently Stark and Lo Surdo have found a similar
splitting up of lines in the spectrum formed by light from canal rays (rays of
positively charged particles) passing through an intense electric field. This
phenomenon has as yet received no adequate explanation.
On discovering that an electric current is capable of producing a
magnetic field, Ampère had suggested that the magnetic properties of such
substances as iron might be explained on the assumption of molecular
currents. The electron theory considers these currents to be due to the
revolution, inside the atom, of negatively charged particles about an
attracting nucleus. It occurred to Richardson that this motion should give
the atom the properties of a gyrostat. Hence if an iron bar be rotated about
its axis, the atoms should orient themselves so as to make their axes more
nearly parallel to the axis of rotation. Thus its rotation should cause the bar
to become a magnet. Barnett[162] has tested this hypothesis, and has found
the effect Richardson had predicted. From the strength of the magnetization
produced, the value of me can be computed. Barnett finds a value somewhat
smaller than that for cathode rays, but of the right order of magnitude and
sign. Einstein and De Haas have detected the inverse of this effect, i. e., the
rotation of an iron rod when it is suddenly magnetized.
X-Rays.—In 1895, on developing a plate which had been lying near a
vacuum tube, Röntgen[163] was surprised to find distinct markings on it. As
the plate had never been exposed to light, it was necessary to suppose the
effect to be due to some new and unknown type of radiation. Further
investigation showed that this radiation originates at the points where
cathode rays impinge on the glass walls of the tube. Besides being able to
pass with ease through all but the most dense material objects X-rays were
found to have the power of ionizing gases through which they pass and
ejecting electrons from metal surfaces against which they strike. The points
at which these electrons are produced are in turn the sources of secondary
X-rays whose properties are characteristic of the metal from which they
come.
components are found than the elementary theory calls for. Hale has
detected the Zeeman effect in light from sun spots, proving that these
blemishes on the sun’s face are vortices caused by whirling swarms of
electrified particles. Recently Stark and Lo Surdo have found a similar
splitting up of lines in the spectrum formed by light from canal rays (rays of
positively charged particles) passing through an intense electric field. This
phenomenon has as yet received no adequate explanation.
On discovering that an electric current is capable of producing a
magnetic field, Ampère had suggested that the magnetic properties of such
substances as iron might be explained on the assumption of molecular
currents. The electron theory considers these currents to be due to the
revolution, inside the atom, of negatively charged particles about an
attracting nucleus. It occurred to Richardson that this motion should give
the atom the properties of a gyrostat. Hence if an iron bar be rotated about
its axis, the atoms should orient themselves so as to make their axes more
nearly parallel to the axis of rotation. Thus its rotation should cause the bar
to become a magnet. Barnett[162] has tested this hypothesis, and has found
the effect Richardson had predicted. From the strength of the magnetization
produced, the value of me can be computed. Barnett finds a value somewhat
smaller than that for cathode rays, but of the right order of magnitude and
sign. Einstein and De Haas have detected the inverse of this effect, i. e., the
rotation of an iron rod when it is suddenly magnetized.
X-Rays.—In 1895, on developing a plate which had been lying near a
vacuum tube, Röntgen[163] was surprised to find distinct markings on it. As
the plate had never been exposed to light, it was necessary to suppose the
effect to be due to some new and unknown type of radiation. Further
investigation showed that this radiation originates at the points where
cathode rays impinge on the glass walls of the tube. Besides being able to
pass with ease through all but the most dense material objects X-rays were
found to have the power of ionizing gases through which they pass and
ejecting electrons from metal surfaces against which they strike. The points
at which these electrons are produced are in turn the sources of secondary
X-rays whose properties are characteristic of the metal from which they
come.
Page 384
Röntgen’s discovery excited intense interest among laymen as well as in
scientific circles. Of the many X-ray photographs taken, those of Wright (1,
235, 1896) of Yale were the first to be produced in this country. His
experiments were made immediately on receipt of the news of Röntgen’s
research, and resulted in the publication of a number of photographs
showing the translucency for these rays of paper, wood, and even
aluminium.
As X-rays are undeviated by electric or magnetic fields, Schuster, and
later Wiechert and Stokes, suggested that they might be electromagnetic
waves of the same nature as light, but much shorter and less regular. The
great objection to this hypothesis was the failure either to refract or diffract
these rays. In fact Bragg contended that they were not etherial disturbances
at all, but consisted of neutral particles moving with very high velocities.
Finally Laue[164] demonstrated their undulatory nature by showing that
diffraction took place under proper conditions. Just as the distance between
adjacent lines of a grating must be comparable to the wave length of light
for a spectrum to be formed, a periodic structure with a grating space of
their very much shorter wave length is necessary to diffract X-rays. Such a
structure is altogether too fine to be made by human tools. Nature, however,
has already prepared it for man’s use. The distance between the atoms of a
crystal is just right to make it an excellent X-ray grating, and Laue had no
difficulty in obtaining diffraction patterns when Röntgen rays were passed
through a block of zincblende. The distance between adjacent atoms of this
cubic crystal can be computed at once from its density and molecular
weight, and then the wave length of the radiation calculated from the
deviation suffered. In this way X-rays are found to have a length less than
one thousandth as great as visible light. Further study of this phenomenon,
particularly by the two Braggs, father and son, has revealed many of the
structural details of more complicated crystals.
The most significant investigation in the field opened up by Laue’s
discovery is that undertaken by Moseley[165] only a couple of years before he
lost his life in the trenches at Gallipoli. Using many different metals as
anticathodes in a vacuum tube, he measured the frequencies of the
characteristic rays emitted. He found that if the elements are arranged in
order of increasing atomic weight, the square roots of the characteristic
frequencies form an arithmetical progression. If to each element is assigned
an integer, beginning with one for hydrogen, two for helium, and so on, the
scientific circles. Of the many X-ray photographs taken, those of Wright (1,
235, 1896) of Yale were the first to be produced in this country. His
experiments were made immediately on receipt of the news of Röntgen’s
research, and resulted in the publication of a number of photographs
showing the translucency for these rays of paper, wood, and even
aluminium.
As X-rays are undeviated by electric or magnetic fields, Schuster, and
later Wiechert and Stokes, suggested that they might be electromagnetic
waves of the same nature as light, but much shorter and less regular. The
great objection to this hypothesis was the failure either to refract or diffract
these rays. In fact Bragg contended that they were not etherial disturbances
at all, but consisted of neutral particles moving with very high velocities.
Finally Laue[164] demonstrated their undulatory nature by showing that
diffraction took place under proper conditions. Just as the distance between
adjacent lines of a grating must be comparable to the wave length of light
for a spectrum to be formed, a periodic structure with a grating space of
their very much shorter wave length is necessary to diffract X-rays. Such a
structure is altogether too fine to be made by human tools. Nature, however,
has already prepared it for man’s use. The distance between the atoms of a
crystal is just right to make it an excellent X-ray grating, and Laue had no
difficulty in obtaining diffraction patterns when Röntgen rays were passed
through a block of zincblende. The distance between adjacent atoms of this
cubic crystal can be computed at once from its density and molecular
weight, and then the wave length of the radiation calculated from the
deviation suffered. In this way X-rays are found to have a length less than
one thousandth as great as visible light. Further study of this phenomenon,
particularly by the two Braggs, father and son, has revealed many of the
structural details of more complicated crystals.
The most significant investigation in the field opened up by Laue’s
discovery is that undertaken by Moseley[165] only a couple of years before he
lost his life in the trenches at Gallipoli. Using many different metals as
anticathodes in a vacuum tube, he measured the frequencies of the
characteristic rays emitted. He found that if the elements are arranged in
order of increasing atomic weight, the square roots of the characteristic
frequencies form an arithmetical progression. If to each element is assigned
an integer, beginning with one for hydrogen, two for helium, and so on, the
Page 385
square root of the frequency of the characteristic radiation is found to be
proportional to this atomic number. Even though Uhler has shown recently
that over wide ranges Moseley’s law does not hold within the limits of
experimental error, there is undoubtedly much significance to be attached to
this simple relation.
Radioactivity.—The year following the discovery of X-rays, Becquerel
found that a photographic plate is similarly affected by radiations from
uranium salts. Two years later the Curies separated from pitchblende the
very active elements polonium and radium. Passage of the rays from these
substances through electric and magnetic fields revealed the existence of
three types. The alpha rays have been shown by Rutherford and his co-
workers to be positively charged helium atoms; the beta rays are very
rapidly moving electrons; and the gamma rays are electromagnetic pulses of
the same nature as X-rays but somewhat shorter. In 1902 Rutherford and
Soddy advanced the theory of atomic disintegration, according to which the
emission of a ray is an indication of the breaking down of the atom to a
simpler form. Thus in the radioactive substances there is going on before
our eyes a continual transformation of one element into another, a change,
by the way, which appears to be in no slightest degree either hastened or
delayed by changes in temperature (H. L. Bronson, 20, 60, 1905) or
external electrical condition of the radioactive element. Uranium is the
progenitor of a long line of descendants, of which radium was supposed for
some time to be the first member. Boltwood (25, 365, 1908) of Yale,
however, showed that the slow growth of radium in uranium solutions is
incompatible with this assumption, and soon isolated an intermediate
product which he named ionium. Radium itself disintegrates into a gas
known as radium emanation, which in turn gives rise to a succession of
other products. Analyses by Boltwood (23, 77, 1907) of radioactive
minerals from the same locality show such a constant ratio between the
amounts of uranium and lead present that it is natural to conclude that lead
is the end product of the series. This hypothesis is confirmed by the fact that
the oldest rocks show relatively the greatest amounts of this element.
In addition to the Ionium-Radium series two others have been
discovered. Of these Boltwood’s (25, 269, 1908) investigations seem to
indicate that the one which starts with actinium is a collateral branch of the
radium series and comes from the same parent uranium. The other begins
with thorium and comprises ten members. As yet the end products of the
proportional to this atomic number. Even though Uhler has shown recently
that over wide ranges Moseley’s law does not hold within the limits of
experimental error, there is undoubtedly much significance to be attached to
this simple relation.
Radioactivity.—The year following the discovery of X-rays, Becquerel
found that a photographic plate is similarly affected by radiations from
uranium salts. Two years later the Curies separated from pitchblende the
very active elements polonium and radium. Passage of the rays from these
substances through electric and magnetic fields revealed the existence of
three types. The alpha rays have been shown by Rutherford and his co-
workers to be positively charged helium atoms; the beta rays are very
rapidly moving electrons; and the gamma rays are electromagnetic pulses of
the same nature as X-rays but somewhat shorter. In 1902 Rutherford and
Soddy advanced the theory of atomic disintegration, according to which the
emission of a ray is an indication of the breaking down of the atom to a
simpler form. Thus in the radioactive substances there is going on before
our eyes a continual transformation of one element into another, a change,
by the way, which appears to be in no slightest degree either hastened or
delayed by changes in temperature (H. L. Bronson, 20, 60, 1905) or
external electrical condition of the radioactive element. Uranium is the
progenitor of a long line of descendants, of which radium was supposed for
some time to be the first member. Boltwood (25, 365, 1908) of Yale,
however, showed that the slow growth of radium in uranium solutions is
incompatible with this assumption, and soon isolated an intermediate
product which he named ionium. Radium itself disintegrates into a gas
known as radium emanation, which in turn gives rise to a succession of
other products. Analyses by Boltwood (23, 77, 1907) of radioactive
minerals from the same locality show such a constant ratio between the
amounts of uranium and lead present that it is natural to conclude that lead
is the end product of the series. This hypothesis is confirmed by the fact that
the oldest rocks show relatively the greatest amounts of this element.
In addition to the Ionium-Radium series two others have been
discovered. Of these Boltwood’s (25, 269, 1908) investigations seem to
indicate that the one which starts with actinium is a collateral branch of the
radium series and comes from the same parent uranium. The other begins
with thorium and comprises ten members. As yet the end products of the
Page 386
actinium and thorium series have not been identified, although there is
some reason for believing that an isotope of lead may be the final member
of the latter.
As the amount of a radioactive element which disintegrates in a given
time is proportional to the total mass present, an infinite time would be
required for the substance to be completely transformed. Hence the life of
such an element is measured by the half value period, or time taken for half
the initial mass to disintegrate. This time varies widely for different
radioactive substances, ranging from a small fraction of a second for
actinium A to five billion years for uranium. Boltwood’s (25, 493, 1908)
original determination of the life of radium from the rate of its growth in a
solution containing ionium gave 2000 years as its result, although recent
measurements by Miss Gleditsch (41, 112, 1916) agree more closely with
the value 1760 years obtained by Rutherford and Geiger from the number
of alpha particles emitted.
Under the action of X-rays or the radiations from radioactive substances,
gases acquire a conductivity which has been attributed by Thomson and
Rutherford to the formation of ions. Zeleny has found that ions of opposite
sign have somewhat different mobilities in an electric field, and
experiments of Wellisch (39, 583, 1915) show that at low pressures some of
the negative ions are electrons. T. S. Taylor (26, 169, 1908 et seq.) and
Duane (26, 464, 1908) have investigated the ionization produced by alpha
particles, and Bumstead (32, 403, 1911 et seq.) has studied the emission of
electrons from metals which are bombarded by these rays. The
investigations of Franck and Hertz, and McLennan and Henderson, show a
significant relation between the ionizing potential (energy which must be
possessed by an electron in order to produce an ion on colliding with an
atom) and a quantity, to be considered later in more detail, which has been
introduced by Planck into the theory of radiation.
Methods of Science.—Scientific progress seems to follow a more or less
clearly defined path. Experimentation brings to light the hidden processes
of nature, and hypotheses are advanced to correlate the facts discovered. As
more and more phenomena are found to fit into the same scheme, the
hypotheses at first proposed tentatively, although often only after extensive
alterations, become firmly established as theories. Finally there may appear
a fundamental clash between two theories, each of which in its respective
some reason for believing that an isotope of lead may be the final member
of the latter.
As the amount of a radioactive element which disintegrates in a given
time is proportional to the total mass present, an infinite time would be
required for the substance to be completely transformed. Hence the life of
such an element is measured by the half value period, or time taken for half
the initial mass to disintegrate. This time varies widely for different
radioactive substances, ranging from a small fraction of a second for
actinium A to five billion years for uranium. Boltwood’s (25, 493, 1908)
original determination of the life of radium from the rate of its growth in a
solution containing ionium gave 2000 years as its result, although recent
measurements by Miss Gleditsch (41, 112, 1916) agree more closely with
the value 1760 years obtained by Rutherford and Geiger from the number
of alpha particles emitted.
Under the action of X-rays or the radiations from radioactive substances,
gases acquire a conductivity which has been attributed by Thomson and
Rutherford to the formation of ions. Zeleny has found that ions of opposite
sign have somewhat different mobilities in an electric field, and
experiments of Wellisch (39, 583, 1915) show that at low pressures some of
the negative ions are electrons. T. S. Taylor (26, 169, 1908 et seq.) and
Duane (26, 464, 1908) have investigated the ionization produced by alpha
particles, and Bumstead (32, 403, 1911 et seq.) has studied the emission of
electrons from metals which are bombarded by these rays. The
investigations of Franck and Hertz, and McLennan and Henderson, show a
significant relation between the ionizing potential (energy which must be
possessed by an electron in order to produce an ion on colliding with an
atom) and a quantity, to be considered later in more detail, which has been
introduced by Planck into the theory of radiation.
Methods of Science.—Scientific progress seems to follow a more or less
clearly defined path. Experimentation brings to light the hidden processes
of nature, and hypotheses are advanced to correlate the facts discovered. As
more and more phenomena are found to fit into the same scheme, the
hypotheses at first proposed tentatively, although often only after extensive
alterations, become firmly established as theories. Finally there may appear
a fundamental clash between two theories, each of which in its respective
Page 387
domain seems to represent the only possible manner in which a large group
of phenomena can be correlated. The maze becomes more perplexing at
every step. At last a genius appears on the scene, approaches the problem
from a new and unsuspected point of view, and the paradox vanishes. Such
changes in point of view are the milestones which mark the progress of
science. That science is stagnant whose only function is to collect, classify
and correlate vast stores of experimental data. The sign of vitality is the
existence of clearly defined and fundamental problems any possible
solution of which seems irreconcilable with the most basic truths of the
science in question. The greater the paradox grows, the more certain the
advent of a new point of view which will bring one step nearer the
comprehensive picture of nature which is the goal of natural philosophy.
The Ether.—From the earliest times philosophers have been attracted by
the possibility of explaining physical phenomena in terms of an all-
pervading medium. So strong had this tendency become by the middle of
the nineteenth century that the English school of physicists were attributing
rigidity, density and nearly all the properties of material media to the ether.
In fact most physicists seemed to have forgotten that no experiment had
ever given direct evidence of the existence of such a medium. Not until the
first decade of the twentieth century was it realized that the experimental
evidence actually pointed in quite the opposite direction, and that a new
point of view was needed in dealing with those phenomena of light and
electromagnetism which had been previously described in terms of a
universal medium. Some account of the development of the ether theory
and of the origin and growth of the point of view which has its principal
exemplification in the principle of relativity is essential for an
understanding of present tendencies in formulating a philosophic basis for
scientific thought.
In the time of Newton and for a century after there was much controversy
between the adherents of two irreconcilable theories of light. Hooke had
suggested that light is a wave motion traveling through a homogeneous
medium which fills all space, and Huygens had shown that the law of
refraction can be deduced at once from this hypothesis if it is assumed that
the velocity of light in a transparent body is less than that in free ether.
However, Newton, impressed by the fact that a ray obtained by double
refraction in Iceland spar differs from a ray of ordinary light just as a rod of
rectangular cross section differs from one of circular cross section, and
of phenomena can be correlated. The maze becomes more perplexing at
every step. At last a genius appears on the scene, approaches the problem
from a new and unsuspected point of view, and the paradox vanishes. Such
changes in point of view are the milestones which mark the progress of
science. That science is stagnant whose only function is to collect, classify
and correlate vast stores of experimental data. The sign of vitality is the
existence of clearly defined and fundamental problems any possible
solution of which seems irreconcilable with the most basic truths of the
science in question. The greater the paradox grows, the more certain the
advent of a new point of view which will bring one step nearer the
comprehensive picture of nature which is the goal of natural philosophy.
The Ether.—From the earliest times philosophers have been attracted by
the possibility of explaining physical phenomena in terms of an all-
pervading medium. So strong had this tendency become by the middle of
the nineteenth century that the English school of physicists were attributing
rigidity, density and nearly all the properties of material media to the ether.
In fact most physicists seemed to have forgotten that no experiment had
ever given direct evidence of the existence of such a medium. Not until the
first decade of the twentieth century was it realized that the experimental
evidence actually pointed in quite the opposite direction, and that a new
point of view was needed in dealing with those phenomena of light and
electromagnetism which had been previously described in terms of a
universal medium. Some account of the development of the ether theory
and of the origin and growth of the point of view which has its principal
exemplification in the principle of relativity is essential for an
understanding of present tendencies in formulating a philosophic basis for
scientific thought.
In the time of Newton and for a century after there was much controversy
between the adherents of two irreconcilable theories of light. Hooke had
suggested that light is a wave motion traveling through a homogeneous
medium which fills all space, and Huygens had shown that the law of
refraction can be deduced at once from this hypothesis if it is assumed that
the velocity of light in a transparent body is less than that in free ether.
However, Newton, impressed by the fact that a ray obtained by double
refraction in Iceland spar differs from a ray of ordinary light just as a rod of
rectangular cross section differs from one of circular cross section, and
Page 388
seeing no way of explaining this dissymmetry in terms of a wave motion
analogous to longitudinal sound waves, adhered to the view that light
consists of infinitesimal particles shot out from the luminous body with
enormous velocities. So great was his reputation on account of his
discoveries in other fields that this theory of light held sway among his
contemporaries and successors until the labors of Young and Fresnel at the
beginning of the nineteenth century definitely established the undulatory
theory. However, in spite of the fact that a corpuscular theory of light made
the assumption of an ether unnecessary in so far as the simpler of the
observed phenomena are concerned, even Newton postulated the existence
of such a medium, partly in order to explain the more complicated results of
experiments in light, and partly in order to provide a vehicle for the
propagation of gravitational forces.
Now an ether, if it is to explain anything at all, must have at least some of
the simpler properties of material media. The most fundamental of these,
perhaps, is position in space. As a first approximation in explaining optical
phenomena on the earth’s surface, the earth might be supposed to be at rest
relative to the ether. But the establishment of the Copernican system made
the sun the center of the solar system and gave the earth an orbital speed of
eighteen miles a second. It may be remarked parenthetically that the speed
of a point on the equator due to the earth’s diurnal rotation is quite
insignificant compared to its orbital velocity. Hence as a second
approximation the sun might be considered at rest relative to the ether and
the earth as moving through this unresisting medium.
The first indication of this motion lay in the discovery of aberration by
the British astronomer Bradley in 1728. Bradley noticed that stars near the
pole of the ecliptic describe small circles during the course of a year, while
those in the plane of the ecliptic vibrate back and forth in straight lines,
stars in intermediate positions describing ellipses. The surprising thing,
however, was that the time taken to complete one of these small orbits is in
all cases exactly a year. Bradley concluded that the phenomenon is in some
way dependent on the earth’s motion around the sun, and he was not long in
reaching the correct explanation. For suppose the earth to be at rest. Then in
observing a star at the pole of the ecliptic it would be necessary to keep the
axis of the telescope exactly at right angles to the plane of the earth’s orbit.
However, as the earth is in motion, the telescope must be pointed a little
forward, just as in walking rapidly through the rain an umbrella must be
analogous to longitudinal sound waves, adhered to the view that light
consists of infinitesimal particles shot out from the luminous body with
enormous velocities. So great was his reputation on account of his
discoveries in other fields that this theory of light held sway among his
contemporaries and successors until the labors of Young and Fresnel at the
beginning of the nineteenth century definitely established the undulatory
theory. However, in spite of the fact that a corpuscular theory of light made
the assumption of an ether unnecessary in so far as the simpler of the
observed phenomena are concerned, even Newton postulated the existence
of such a medium, partly in order to explain the more complicated results of
experiments in light, and partly in order to provide a vehicle for the
propagation of gravitational forces.
Now an ether, if it is to explain anything at all, must have at least some of
the simpler properties of material media. The most fundamental of these,
perhaps, is position in space. As a first approximation in explaining optical
phenomena on the earth’s surface, the earth might be supposed to be at rest
relative to the ether. But the establishment of the Copernican system made
the sun the center of the solar system and gave the earth an orbital speed of
eighteen miles a second. It may be remarked parenthetically that the speed
of a point on the equator due to the earth’s diurnal rotation is quite
insignificant compared to its orbital velocity. Hence as a second
approximation the sun might be considered at rest relative to the ether and
the earth as moving through this unresisting medium.
The first indication of this motion lay in the discovery of aberration by
the British astronomer Bradley in 1728. Bradley noticed that stars near the
pole of the ecliptic describe small circles during the course of a year, while
those in the plane of the ecliptic vibrate back and forth in straight lines,
stars in intermediate positions describing ellipses. The surprising thing,
however, was that the time taken to complete one of these small orbits is in
all cases exactly a year. Bradley concluded that the phenomenon is in some
way dependent on the earth’s motion around the sun, and he was not long in
reaching the correct explanation. For suppose the earth to be at rest. Then in
observing a star at the pole of the ecliptic it would be necessary to keep the
axis of the telescope exactly at right angles to the plane of the earth’s orbit.
However, as the earth is in motion, the telescope must be pointed a little
forward, just as in walking rapidly through the rain an umbrella must be
Page 389
inclined forward so as to intercept the raindrops which would otherwise fall
on the spot to be occupied at the end of the next step. The angle through
which the telescope has to be tilted is known as the angle of aberration, and
the tangent of this angle may easily be shown to be equal to the ratio of the
velocity of the earth to the velocity of light. Knowing the velocity of the
earth, the velocity of light can then be calculated. This method was one of
the first of obtaining the value of this important quantity.
More recently, terrestrial methods of great precision have been devised
for measuring the velocity of light. The most accurate of these is that
employed by the French physicist Foucault in 1862. A ray of light is
reflected by a rotating mirror to a fixed mirror placed at some distance,
which in turn reflects the ray back to the moving mirror. The latter,
however, has turned through a small angle during the time elapsed since the
first reflection, and consequently the direction of the ray on returning to the
source is not quite opposite to that in which it had started out. This
deviation in direction is determined from the displacement of the image
formed by the returning light, and from it the velocity of light is calculated.
In order to make the deflection appreciable the distance between the two
mirrors should be very great. As originally arranged by Foucault, it was
found impractical to make this distance greater than twenty meters, and
consequently the displacement of the image was less than a millimeter.
Such a small deflection limited the accuracy of the experiment to one
percent. In 1879, however, Michelson (18, 390, 1879), then a master in the
United States Navy, improved Foucault’s optical arrangements to such an
extent that he was able to use a distance of nearly seven hundred meters
between the two mirrors. With a rate of two hundred and fifty-seven
revolutions a second for the rotating mirror, the displacement obtained was
over thirteen centimeters. This experiment gave 299,910 kilometers a
second for the velocity of light, with a probable error of one part in ten
thousand. Later investigations by Newcomb and Michelson (31, 62, 1886)
gave substantially the same result. So great has been the accuracy of these
terrestrial determinations that recent practice has been to calculate from
them and the angle of aberration the earth’s orbital velocity, and hence the
distance of the earth from the sun. This indirect method of measuring the
astronomical unit has a probable error no greater than the best parallax
methods of the astronomer. (J. Lovering, 36, 161, 1863.)
on the spot to be occupied at the end of the next step. The angle through
which the telescope has to be tilted is known as the angle of aberration, and
the tangent of this angle may easily be shown to be equal to the ratio of the
velocity of the earth to the velocity of light. Knowing the velocity of the
earth, the velocity of light can then be calculated. This method was one of
the first of obtaining the value of this important quantity.
More recently, terrestrial methods of great precision have been devised
for measuring the velocity of light. The most accurate of these is that
employed by the French physicist Foucault in 1862. A ray of light is
reflected by a rotating mirror to a fixed mirror placed at some distance,
which in turn reflects the ray back to the moving mirror. The latter,
however, has turned through a small angle during the time elapsed since the
first reflection, and consequently the direction of the ray on returning to the
source is not quite opposite to that in which it had started out. This
deviation in direction is determined from the displacement of the image
formed by the returning light, and from it the velocity of light is calculated.
In order to make the deflection appreciable the distance between the two
mirrors should be very great. As originally arranged by Foucault, it was
found impractical to make this distance greater than twenty meters, and
consequently the displacement of the image was less than a millimeter.
Such a small deflection limited the accuracy of the experiment to one
percent. In 1879, however, Michelson (18, 390, 1879), then a master in the
United States Navy, improved Foucault’s optical arrangements to such an
extent that he was able to use a distance of nearly seven hundred meters
between the two mirrors. With a rate of two hundred and fifty-seven
revolutions a second for the rotating mirror, the displacement obtained was
over thirteen centimeters. This experiment gave 299,910 kilometers a
second for the velocity of light, with a probable error of one part in ten
thousand. Later investigations by Newcomb and Michelson (31, 62, 1886)
gave substantially the same result. So great has been the accuracy of these
terrestrial determinations that recent practice has been to calculate from
them and the angle of aberration the earth’s orbital velocity, and hence the
distance of the earth from the sun. This indirect method of measuring the
astronomical unit has a probable error no greater than the best parallax
methods of the astronomer. (J. Lovering, 36, 161, 1863.)
Page 390
Aberration is a first order effect, i. e., it depends upon the first power of
the ratio of the velocity of the earth to the velocity of light, and at first sight
it seemed to prove conclusively that the earth must be in motion relative to
the luminiferous medium. Other questions had to be settled, however, and
one of these was whether or not light coming from a star would be refracted
differently when passing through optical instruments from light which had a
terrestial origin. Arago subjected the matter to experiment, and concluded
that in every respect the light from a star behaved as if the earth were at rest
and the star actually occupied the position which it appears to occupy on
account of aberration. Finally optical experiments with terrestrial sources
seemed to be in no way affected by the motion of the earth through the
ether.
In order to account for these facts Fresnel advanced the following theory.
To explain the refraction that takes place when light enters a transparent
body, it is necessary to assume that light waves travel more slowly through
matter than in free ether. Now the velocity of sound is known to vary
inversely with the square root of the density of the material medium
through which it passes. Hence it is natural to assume that ether is
condensed inside material objects to such an extent that this same relation
connects its density with the velocity of light traveling through it. But when
a lens or prism is set in motion, Fresnel supposed it to carry along only the
excess ether which it contains, ether of the normal density remaining
behind. This assumption suffices to explain Arago’s results, and yet fits in
with the phenomenon of aberration. It gives for light traveling in the
direction of motion through a moving material medium of index of
refraction n an absolute velocity greater than that when the medium is at
rest by an amount
(1 − 1/n2)v,
which is only a fraction of the velocity v which would have to be added if
convected matter carried along all the ether which resides within it. This
expression was tested directly, first by Fizeau in 1851, and later by
Michelson and Morley (31, 377, 1886) in this country. The experiment
consists in bifurcating a beam of light, passing one-half in one direction and
the other in the opposite direction through a stream of running water. On
reuniting the two rays the usual interference fringes are produced.
Reversing the direction of motion of the water causes the fringes to shift,
the ratio of the velocity of the earth to the velocity of light, and at first sight
it seemed to prove conclusively that the earth must be in motion relative to
the luminiferous medium. Other questions had to be settled, however, and
one of these was whether or not light coming from a star would be refracted
differently when passing through optical instruments from light which had a
terrestial origin. Arago subjected the matter to experiment, and concluded
that in every respect the light from a star behaved as if the earth were at rest
and the star actually occupied the position which it appears to occupy on
account of aberration. Finally optical experiments with terrestrial sources
seemed to be in no way affected by the motion of the earth through the
ether.
In order to account for these facts Fresnel advanced the following theory.
To explain the refraction that takes place when light enters a transparent
body, it is necessary to assume that light waves travel more slowly through
matter than in free ether. Now the velocity of sound is known to vary
inversely with the square root of the density of the material medium
through which it passes. Hence it is natural to assume that ether is
condensed inside material objects to such an extent that this same relation
connects its density with the velocity of light traveling through it. But when
a lens or prism is set in motion, Fresnel supposed it to carry along only the
excess ether which it contains, ether of the normal density remaining
behind. This assumption suffices to explain Arago’s results, and yet fits in
with the phenomenon of aberration. It gives for light traveling in the
direction of motion through a moving material medium of index of
refraction n an absolute velocity greater than that when the medium is at
rest by an amount
(1 − 1/n2)v,
which is only a fraction of the velocity v which would have to be added if
convected matter carried along all the ether which resides within it. This
expression was tested directly, first by Fizeau in 1851, and later by
Michelson and Morley (31, 377, 1886) in this country. The experiment
consists in bifurcating a beam of light, passing one-half in one direction and
the other in the opposite direction through a stream of running water. On
reuniting the two rays the usual interference fringes are produced.
Reversing the direction of motion of the water causes the fringes to shift,
Page 391
and from the amount of this shift the velocity imparted to the light by the
motion of the stream is computed. The divergence between the
experimental value of this quantity and that calculated from Fresnel’s
coefficient of entrainment was found by Michelson and Morley to be less
than one percent, which was about their experimental error. Thus Fresnel’s
expression for the velocity of light in a moving medium is entirely
confirmed by experiment. The derivation of it accepted to-day, however, is
very different from his original deduction.
It has been noted that the phenomena of polarization led Newton to reject
the wave theory of light. The only type of wave known to him was the
longitudinal wave, in which the vibrations of the particles of the medium
are in the same direction as that of propagation of the wave, and it was
impossible to suppose that such a wave could have different properties in
different directions at right angles to the line in which it is advancing. But
in 1817 Young suggested that this inconsistency between the wave theory
and the facts of polarization could be removed by supposing the vibrations
constituting light to be executed at right angles to the direction of
propagation. Thus in ordinary light the vibrations are to be conceived as
taking place haphazard in all directions in the plane perpendicular to the
ray, while in plane polarized light these vibrations are confined to a single
direction. This supposition explained so many of the puzzling results of
experiment, that it was accepted at once and led to the complete vindication
of the undulatory theory.
Elastic Solid Theory.—Shortly afterwards Poisson succeeded in solving
the differential equation which determines the motion of a wave through an
elastic medium. His solution shows that such a medium is capable of
transmitting two types of wave—one longitudinal, the other transverse. If κ
denotes the volume elasticity, η the rigidity and ρ the density of the
medium, the velocities of the two waves are respectively
√((κ + (⁴⁄₃)η)/ρ) and √(η/ρ)
Now a solid has both compressibility and rigidity, and transmits in general
both types of wave. A fluid, on the other hand, on account of its lack of
rigidity, cannot support a transverse vibration. Hence it was natural that
Green, in searching for a dynamical explanation of the ether, should have
proposed in a paper read before the Cambridge Philosophical Society in
1837 that the ether has the elastic properties of a solid. One great difficulty
motion of the stream is computed. The divergence between the
experimental value of this quantity and that calculated from Fresnel’s
coefficient of entrainment was found by Michelson and Morley to be less
than one percent, which was about their experimental error. Thus Fresnel’s
expression for the velocity of light in a moving medium is entirely
confirmed by experiment. The derivation of it accepted to-day, however, is
very different from his original deduction.
It has been noted that the phenomena of polarization led Newton to reject
the wave theory of light. The only type of wave known to him was the
longitudinal wave, in which the vibrations of the particles of the medium
are in the same direction as that of propagation of the wave, and it was
impossible to suppose that such a wave could have different properties in
different directions at right angles to the line in which it is advancing. But
in 1817 Young suggested that this inconsistency between the wave theory
and the facts of polarization could be removed by supposing the vibrations
constituting light to be executed at right angles to the direction of
propagation. Thus in ordinary light the vibrations are to be conceived as
taking place haphazard in all directions in the plane perpendicular to the
ray, while in plane polarized light these vibrations are confined to a single
direction. This supposition explained so many of the puzzling results of
experiment, that it was accepted at once and led to the complete vindication
of the undulatory theory.
Elastic Solid Theory.—Shortly afterwards Poisson succeeded in solving
the differential equation which determines the motion of a wave through an
elastic medium. His solution shows that such a medium is capable of
transmitting two types of wave—one longitudinal, the other transverse. If κ
denotes the volume elasticity, η the rigidity and ρ the density of the
medium, the velocities of the two waves are respectively
√((κ + (⁴⁄₃)η)/ρ) and √(η/ρ)
Now a solid has both compressibility and rigidity, and transmits in general
both types of wave. A fluid, on the other hand, on account of its lack of
rigidity, cannot support a transverse vibration. Hence it was natural that
Green, in searching for a dynamical explanation of the ether, should have
proposed in a paper read before the Cambridge Philosophical Society in
1837 that the ether has the elastic properties of a solid. One great difficulty
Page 392
presented itself; disturbances inside an elastic solid must give rise to
compressional as well as to transverse waves. But no such thing as a
compressional wave had been found in the experimental study of light.
Green attempted to overcome this difficulty by attributing an infinite
volume elasticity to the ether. The expression above shows that longitudinal
waves originating in such an incompressible medium would be carried
away with an infinite velocity, and it may be shown that the energy
associated with them would be infinitesimal in amount. The next step was
to calculate the coefficients of transmission and reflection for light passing
from one material medium to another. Here the elastic solid theory is not
altogether successful. If the ether is supposed to have different densities in
the two media, as in Fresnel’s theory, but the same rigidity, certain of these
coefficients fail to give the values demanded by experiment, while if the
densities are assumed the same but the rigidities different, other of the
coefficients have discordant values. In connection with the phenomena of
double refraction even more serious difficulties are encountered.
Electromagnetic Theory.—It was beginning to be felt that an ether must
explain more than the phenomena of light, for Faraday’s conception of
electromagnetic action as carried on through the agency of a medium had
added greatly to its functions. Finally Maxwell’s demonstration that
electromagnetic waves are propagated with the velocity of light made the
theory of light into a subdivision of electrodynamics. Maxwell himself did
not apply electromagnetic theory to the explanation of reflection and
refraction. This deficiency, however, was remedied by Lorentz in 1875. The
results obtained, as well as those for double refraction (J. W. Gibbs, 23, 262,
1882 et seq.), and metallic reflection (L. P. Wheeler, 32, 85, 1911), provided
a complete vindication of the electromagnetic theory of light. This is all the
more significant when the extreme precision obtainable in optical
experiments is taken into account. For instance, Hastings (35, 60, 1888) has
tested Huygens’ construction for double refraction in Iceland spar and found
that “the difference between a measured index of refraction ... at an angle of
30° with the crystalline axis, and the index calculated from Huygens’ law
and the measured principal indices of refraction” is a matter of only 4–5
units in the sixth decimal place. Since Maxwell’s time the gamut of
electromagnetic waves has been steadily extended. The shortest Hertzian
waves merge almost imperceptibly into the longest heat waves of the infra-
red, and from there the known spectrum runs continuously through the
compressional as well as to transverse waves. But no such thing as a
compressional wave had been found in the experimental study of light.
Green attempted to overcome this difficulty by attributing an infinite
volume elasticity to the ether. The expression above shows that longitudinal
waves originating in such an incompressible medium would be carried
away with an infinite velocity, and it may be shown that the energy
associated with them would be infinitesimal in amount. The next step was
to calculate the coefficients of transmission and reflection for light passing
from one material medium to another. Here the elastic solid theory is not
altogether successful. If the ether is supposed to have different densities in
the two media, as in Fresnel’s theory, but the same rigidity, certain of these
coefficients fail to give the values demanded by experiment, while if the
densities are assumed the same but the rigidities different, other of the
coefficients have discordant values. In connection with the phenomena of
double refraction even more serious difficulties are encountered.
Electromagnetic Theory.—It was beginning to be felt that an ether must
explain more than the phenomena of light, for Faraday’s conception of
electromagnetic action as carried on through the agency of a medium had
added greatly to its functions. Finally Maxwell’s demonstration that
electromagnetic waves are propagated with the velocity of light made the
theory of light into a subdivision of electrodynamics. Maxwell himself did
not apply electromagnetic theory to the explanation of reflection and
refraction. This deficiency, however, was remedied by Lorentz in 1875. The
results obtained, as well as those for double refraction (J. W. Gibbs, 23, 262,
1882 et seq.), and metallic reflection (L. P. Wheeler, 32, 85, 1911), provided
a complete vindication of the electromagnetic theory of light. This is all the
more significant when the extreme precision obtainable in optical
experiments is taken into account. For instance, Hastings (35, 60, 1888) has
tested Huygens’ construction for double refraction in Iceland spar and found
that “the difference between a measured index of refraction ... at an angle of
30° with the crystalline axis, and the index calculated from Huygens’ law
and the measured principal indices of refraction” is a matter of only 4–5
units in the sixth decimal place. Since Maxwell’s time the gamut of
electromagnetic waves has been steadily extended. The shortest Hertzian
waves merge almost imperceptibly into the longest heat waves of the infra-
red, and from there the known spectrum runs continuously through the
Page 393
visible region to the short waves of the extreme ultra-violet recently
disclosed by Lyman. Here there is a short gap until soft X-rays are reached,
and finally the domain of radiation comes to an end with gamma rays a
billionth of a centimeter in length.
Maxwell’s ether was not a dynamical ether in the sense of Green’s elastic
solid medium. In spite of the fact that Maxwell was always active in
devising mechanical analogues to illustrate the phenomena of
electromagnetism, he was never enthusiastic over the speculations of the
advocates of a dynamical ether. The electrodynamic equations provided an
accurate representation of the electric and magnetic fields, and beyond that
he felt it was needless to go. That Gibbs (23, 475, 1882) held the same view
is made evident by the closing paragraphs of a paper in which he shows that
the electromagnetic theory of light accounts in minutest detail for the
intricate phenomena accompanying the passage of light through circularly
polarizing media. He says:
“The laws of the propagation of light in plane waves, which have thus been derived from the single
hypothesis that the disturbance by which light is transmitted consists of solenoidal electrical
fluxes, ... are essentially those which are received as embodying the results of experiment. In no
particular, so far as the writer is aware, do they conflict with the results of experiment, or require the
aid of auxiliary and forced hypotheses to bring them into harmony therewith.
In this respect the electromagnetic theory of light stands in marked contrast with that theory in
which the properties of an elastic solid are attributed to the ether,—a contrast which was very distinct
in Maxwell’s derivation of Fresnel’s laws from electrical principles, but becomes more striking as we
follow the subject farther into its details, and take account of the want of absolute homogeneity in the
medium, so as to embrace the phenomena of the dispersion of colors and circular and elliptical
polarization.”
Further Dynamical Theories.—Kelvin, however, was not satisfied with
this type of ether. To him dynamics was the foundation of all physical
phenomena, and nothing could be said to be explained until a mechanical
model was provided. So he returned to the elastic solid theory, and
developed the consequences of the assumption, already made use of by
Cauchy, that the ether has a negative volume elasticity of such a value as to
make the velocity of the compressional wave zero. In order to prevent such
an ether from collapsing it is necessary to assume that it is rigidly attached
at its boundaries and that cavities cannot be formed at any point in its
interior. Now Gibbs (37, 129, 1889) has pointed out the remarkable fact that
the equations describing the motion of Kelvin’s quasi-labile ether are of
disclosed by Lyman. Here there is a short gap until soft X-rays are reached,
and finally the domain of radiation comes to an end with gamma rays a
billionth of a centimeter in length.
Maxwell’s ether was not a dynamical ether in the sense of Green’s elastic
solid medium. In spite of the fact that Maxwell was always active in
devising mechanical analogues to illustrate the phenomena of
electromagnetism, he was never enthusiastic over the speculations of the
advocates of a dynamical ether. The electrodynamic equations provided an
accurate representation of the electric and magnetic fields, and beyond that
he felt it was needless to go. That Gibbs (23, 475, 1882) held the same view
is made evident by the closing paragraphs of a paper in which he shows that
the electromagnetic theory of light accounts in minutest detail for the
intricate phenomena accompanying the passage of light through circularly
polarizing media. He says:
“The laws of the propagation of light in plane waves, which have thus been derived from the single
hypothesis that the disturbance by which light is transmitted consists of solenoidal electrical
fluxes, ... are essentially those which are received as embodying the results of experiment. In no
particular, so far as the writer is aware, do they conflict with the results of experiment, or require the
aid of auxiliary and forced hypotheses to bring them into harmony therewith.
In this respect the electromagnetic theory of light stands in marked contrast with that theory in
which the properties of an elastic solid are attributed to the ether,—a contrast which was very distinct
in Maxwell’s derivation of Fresnel’s laws from electrical principles, but becomes more striking as we
follow the subject farther into its details, and take account of the want of absolute homogeneity in the
medium, so as to embrace the phenomena of the dispersion of colors and circular and elliptical
polarization.”
Further Dynamical Theories.—Kelvin, however, was not satisfied with
this type of ether. To him dynamics was the foundation of all physical
phenomena, and nothing could be said to be explained until a mechanical
model was provided. So he returned to the elastic solid theory, and
developed the consequences of the assumption, already made use of by
Cauchy, that the ether has a negative volume elasticity of such a value as to
make the velocity of the compressional wave zero. In order to prevent such
an ether from collapsing it is necessary to assume that it is rigidly attached
at its boundaries and that cavities cannot be formed at any point in its
interior. Now Gibbs (37, 129, 1889) has pointed out the remarkable fact that
the equations describing the motion of Kelvin’s quasi-labile ether are of
Page 394
exactly the same form as the electromagnetic equations. Electric
displacement is represented by an actual displacement of the ether,
magnetic intensity by a rotation. Hence everything which can be explained
by the electrodynamic equations finds an analogue in terms of Kelvin’s
ether. Still another type of dynamic ether which fits the known facts was
proposed by McCullagh and perfected by Larmor. In this ether a rotational
elasticity is premised, such as would exist if each particle of the medium
consisted of three rigidly connected gyrostats with mutually perpendicular
axes. In this ether electrical displacements correspond to rotations, and
magnetic strains to etherial displacement.
A New Point of View.—While the dynamical school was still dominant in
England, another point of view was developing on the continent. Kirchhoff
denied that it was the province of science to provide mechanical
explanations of the ether and electrodynamic phenomena such as Kelvin
conceived to be necessary in order to make these phenomena intelligible.
Kirchhoff’s contention was that the object of science is purely descriptive,
—phenomena must be observed, classified, and mutual connections
described by the fewest number of differential equations possible. Mach
expressed the same idea somewhat more concisely when he asserted that
the aim of science is “economy of thought.” For instance, in the time of
Newton, planetary motions could be described quite satisfactorily by means
of the three laws of Kepler. The motion of falling bodies on the earth’s
surface had been described with a fair degree of accuracy by Galileo. The
value of Newton’s law of gravitation, however, lay in the fact that this great
generalization made it possible to describe these and many other types of
motion by a single simple formula, instead of leaving each to be governed
by a number of separate and apparently unrelated laws. The importance of
such a generalization is measured by the economy of thought which it
introduces.
displacement is represented by an actual displacement of the ether,
magnetic intensity by a rotation. Hence everything which can be explained
by the electrodynamic equations finds an analogue in terms of Kelvin’s
ether. Still another type of dynamic ether which fits the known facts was
proposed by McCullagh and perfected by Larmor. In this ether a rotational
elasticity is premised, such as would exist if each particle of the medium
consisted of three rigidly connected gyrostats with mutually perpendicular
axes. In this ether electrical displacements correspond to rotations, and
magnetic strains to etherial displacement.
A New Point of View.—While the dynamical school was still dominant in
England, another point of view was developing on the continent. Kirchhoff
denied that it was the province of science to provide mechanical
explanations of the ether and electrodynamic phenomena such as Kelvin
conceived to be necessary in order to make these phenomena intelligible.
Kirchhoff’s contention was that the object of science is purely descriptive,
—phenomena must be observed, classified, and mutual connections
described by the fewest number of differential equations possible. Mach
expressed the same idea somewhat more concisely when he asserted that
the aim of science is “economy of thought.” For instance, in the time of
Newton, planetary motions could be described quite satisfactorily by means
of the three laws of Kepler. The motion of falling bodies on the earth’s
surface had been described with a fair degree of accuracy by Galileo. The
value of Newton’s law of gravitation, however, lay in the fact that this great
generalization made it possible to describe these and many other types of
motion by a single simple formula, instead of leaving each to be governed
by a number of separate and apparently unrelated laws. The importance of
such a generalization is measured by the economy of thought which it
introduces.
Page 395
Fig. 1. Fig. 2. Fig. 3.
Electron Theory.—The electron theory was leading to a reversal of
Kelvin’s idea that dynamical principles must underlie electrodynamics.
Lorentz had shown that a rigorous solution of the electrodynamic equations
did away entirely with Maxwell’s displacement current, but made the
electromagnetic field at a point in space depend not upon the distribution of
charges and currents at the same instant, but at a time earlier sufficient to
allow the effect to travel with the velocity of light from the charges and
currents producing the field to the point at which the electric and magnetic
intensities are to be found. The position of a charge or current element at
this earlier time he denoted its “effective position.” The effective
distribution, then, is that actually seen by an observer stationed at the point
under consideration at the instant for which the intensity of the
electromagnetic field is to be determined. This solution of the
electrodynamic equations led in turn to rigorous expressions for the electric
and magnetic intensities produced by a very small charged particle, such as
an electron. Fig. 1 shows the electrostatic field produced by a charged
particle at rest. The lines of force spread out radially and uniformly in all
directions. In fig. 2 the electron is supposed to have a velocity v
horizontally to the right of an amount smaller than, though comparable
with, the velocity of light c. It is seen that the lines of electric force still
diverge radially from the charge, but are crowded in the equatorial plane
and spread apart in the polar regions. The dissymmetry grows as the
velocity increases until if the velocity of light should be reached the field
would be entirely concentrated in a plane at right angles to the direction of
Electron Theory.—The electron theory was leading to a reversal of
Kelvin’s idea that dynamical principles must underlie electrodynamics.
Lorentz had shown that a rigorous solution of the electrodynamic equations
did away entirely with Maxwell’s displacement current, but made the
electromagnetic field at a point in space depend not upon the distribution of
charges and currents at the same instant, but at a time earlier sufficient to
allow the effect to travel with the velocity of light from the charges and
currents producing the field to the point at which the electric and magnetic
intensities are to be found. The position of a charge or current element at
this earlier time he denoted its “effective position.” The effective
distribution, then, is that actually seen by an observer stationed at the point
under consideration at the instant for which the intensity of the
electromagnetic field is to be determined. This solution of the
electrodynamic equations led in turn to rigorous expressions for the electric
and magnetic intensities produced by a very small charged particle, such as
an electron. Fig. 1 shows the electrostatic field produced by a charged
particle at rest. The lines of force spread out radially and uniformly in all
directions. In fig. 2 the electron is supposed to have a velocity v
horizontally to the right of an amount smaller than, though comparable
with, the velocity of light c. It is seen that the lines of electric force still
diverge radially from the charge, but are crowded in the equatorial plane
and spread apart in the polar regions. The dissymmetry grows as the
velocity increases until if the velocity of light should be reached the field
would be entirely concentrated in a plane at right angles to the direction of
Page 396
motion. Now it may be shown that fig. 2 is obtainable from fig. 1 by
reducing dimensions in the direction of motion in the ratio of
√(1 − β2) : 1, where β ≡ v/c.
For a uniformly convected electric field differs from an electrostatic field
only in that the dimensions in the direction of motion are contracted in this
particular ratio. Fig. 3 represents the electric field of a charged particle
which has a uniform acceleration to the right. Consider Faraday’s analogy
between lines of force and stretched elastic bands. The symmetry of the first
two figures shows that in neither of these cases would there be a resultant
force on the charged particle. But in the third figure it is obvious that a force
to the left is exerted on the charge by its own field. Calculation shows this
force to be proportional in magnitude to the acceleration. Let it be
postulated that the resultant force on a charged particle is always zero. Then
if F is the applied force, the force on the particle due to the reaction of its
field will be — m f, where f stands for the acceleration and m is a positive
constant, and we have the fundamental equation of dynamics
F−mf=0
Hence, instead of admitting Kelvin’s contention that all physical
phenomena must be given a mechanical explanation, it would seem more
logical to assert that electrodynamics actually underlies mechanics.
Calculation shows the electromagnetic mass m to vary inversely with the
radius of the charged particle. Now Thomson’s experiments made it
possible to calculate the mass of an electron. Hence its radius can be
computed, and is found to be about 2(10)–13 part of a centimeter, or one
fifty-thousandth part of the radius of the atom. Since numbers so small
convey little meaning, consider the following illustration, due, in part, to
Kelvin. Imagine a single drop of water to be magnified until it is as large as
the earth. The individual atoms would then have the size of baseballs. Now
magnify one of these atoms until it is comparable in size with St. Peter’s
cathedral at Rome. The electrons within the atom would appear as a few
grains of sand scattered about the nave. This separation between the
constituent electrons of the atom,—so great in comparison with their
dimensions,—explains how alpha particles can be shot by the billion
through thin-walled glass tubing without leaving any holes behind or
impairing in the slightest degree the high vacuum within the tube. The
reducing dimensions in the direction of motion in the ratio of
√(1 − β2) : 1, where β ≡ v/c.
For a uniformly convected electric field differs from an electrostatic field
only in that the dimensions in the direction of motion are contracted in this
particular ratio. Fig. 3 represents the electric field of a charged particle
which has a uniform acceleration to the right. Consider Faraday’s analogy
between lines of force and stretched elastic bands. The symmetry of the first
two figures shows that in neither of these cases would there be a resultant
force on the charged particle. But in the third figure it is obvious that a force
to the left is exerted on the charge by its own field. Calculation shows this
force to be proportional in magnitude to the acceleration. Let it be
postulated that the resultant force on a charged particle is always zero. Then
if F is the applied force, the force on the particle due to the reaction of its
field will be — m f, where f stands for the acceleration and m is a positive
constant, and we have the fundamental equation of dynamics
F−mf=0
Hence, instead of admitting Kelvin’s contention that all physical
phenomena must be given a mechanical explanation, it would seem more
logical to assert that electrodynamics actually underlies mechanics.
Calculation shows the electromagnetic mass m to vary inversely with the
radius of the charged particle. Now Thomson’s experiments made it
possible to calculate the mass of an electron. Hence its radius can be
computed, and is found to be about 2(10)–13 part of a centimeter, or one
fifty-thousandth part of the radius of the atom. Since numbers so small
convey little meaning, consider the following illustration, due, in part, to
Kelvin. Imagine a single drop of water to be magnified until it is as large as
the earth. The individual atoms would then have the size of baseballs. Now
magnify one of these atoms until it is comparable in size with St. Peter’s
cathedral at Rome. The electrons within the atom would appear as a few
grains of sand scattered about the nave. This separation between the
constituent electrons of the atom,—so great in comparison with their
dimensions,—explains how alpha particles can be shot by the billion
through thin-walled glass tubing without leaving any holes behind or
impairing in the slightest degree the high vacuum within the tube. The
Page 397
much smaller high speed beta particles pass through an average of ten
thousand atoms without even coming near enough to one of the component
electrons to detach it and form an ion.
Michelson-Morley Experiment.—In 1881 Michelson (22, 120, 1881)
conceived an ingenious and bold method of measuring the orbital motion of
the earth through the luminiferous ether. As the experiment was one
involving considerable expense, Bell, the inventor of the telephone receiver,
was appealed to successfully for the funds necessary to carry it through.
Michelson’s experimental plan was as follows: A beam of light traveling in
the direction of the earth’s motion strikes an unsilvered mirror m at an angle
of 45°. Part of the light passes through, the rest being reflected at right
angles to its original direction. Each ray is returned by a mirror at a distance
l from m. On meeting again, the ray whose path has been at right angles to
the direction of the earth’s motion passes on through the mirror, while the
other ray is reflected so as to bring the two in line and form interference
fringes. Now consider the effect of the earth’s motion on the paths of the
two rays. In fig. 4 the earth is supposed to be moving to the right. The
unsilvered mirror m bifurcates a beam of light coming from a source a. By
the time the ray reflected from m has traveled to the mirror b and back, m
will have moved forward to m’; a distance 2βl, where the small quantity β is
the ratio of the earth’s velocity to the velocity of light. Hence the length of
the path traversed by this ray is approximately
2l(1 + ½β2).
The other ray will reach the mirror c after the latter has moved forward a
distance
βl
/(1 − β2)
and on returning find m at m’. Hence its path has a length of roughly 2l(1 +
β2). The difference in path of the two rays is β2l and consequently they
should be a little out of phase on meeting at d. By rotating the apparatus
clockwise through 90° the directions of the two rays relative to the earth’s
motion are interchanged, and the interference fringes would be expected to
shift an amount corresponding to a difference in path of 2β2l. This quantity
is of course small,—β2 is about one one hundred millionth,—but so
sensitive are the methods of interferometry that Michelson felt confident
that he would be able to detect the earth’s motion through the ether. The
thousand atoms without even coming near enough to one of the component
electrons to detach it and form an ion.
Michelson-Morley Experiment.—In 1881 Michelson (22, 120, 1881)
conceived an ingenious and bold method of measuring the orbital motion of
the earth through the luminiferous ether. As the experiment was one
involving considerable expense, Bell, the inventor of the telephone receiver,
was appealed to successfully for the funds necessary to carry it through.
Michelson’s experimental plan was as follows: A beam of light traveling in
the direction of the earth’s motion strikes an unsilvered mirror m at an angle
of 45°. Part of the light passes through, the rest being reflected at right
angles to its original direction. Each ray is returned by a mirror at a distance
l from m. On meeting again, the ray whose path has been at right angles to
the direction of the earth’s motion passes on through the mirror, while the
other ray is reflected so as to bring the two in line and form interference
fringes. Now consider the effect of the earth’s motion on the paths of the
two rays. In fig. 4 the earth is supposed to be moving to the right. The
unsilvered mirror m bifurcates a beam of light coming from a source a. By
the time the ray reflected from m has traveled to the mirror b and back, m
will have moved forward to m’; a distance 2βl, where the small quantity β is
the ratio of the earth’s velocity to the velocity of light. Hence the length of
the path traversed by this ray is approximately
2l(1 + ½β2).
The other ray will reach the mirror c after the latter has moved forward a
distance
βl
/(1 − β2)
and on returning find m at m’. Hence its path has a length of roughly 2l(1 +
β2). The difference in path of the two rays is β2l and consequently they
should be a little out of phase on meeting at d. By rotating the apparatus
clockwise through 90° the directions of the two rays relative to the earth’s
motion are interchanged, and the interference fringes would be expected to
shift an amount corresponding to a difference in path of 2β2l. This quantity
is of course small,—β2 is about one one hundred millionth,—but so
sensitive are the methods of interferometry that Michelson felt confident
that he would be able to detect the earth’s motion through the ether. The
Page 398
apparatus consisted of a table which could be rotated about a vertical axis in
much the same way as a spectrometer table, and provided with arms a meter
long to carry the mirrors b and c. With this length of arm the interference
fringes from sodium light should shift by an amount corresponding to four
hundredths of a wave length when the table is rotated through a right angle.
When the experiment was first performed the apparatus was placed on a
stone pier in the Physical Institute at Berlin. So sensitive was the instrument
to outside vibrations that even after midnight it was found impossible to get
consistent readings. Finally a satisfactory foundation was constructed in the
cellar of the Astrophysical observatory at Potsdam. But what was the
astonishment of the experimenters to find that the expected shift of the
interference fringes did not exist!
Fig. 4.
The extreme delicacy of the experiment made it desirable to confirm the
result by repeating it. This was done by Michelson and Morley (34, 333,
1887) in 1887. In place of a revolving table a massive slab of stone floating
on mercury was used to carry the apparatus. This slab was kept in constant
rotation, the observer following it around. Moreover, the precision of the
experiment was greatly increased by reflecting each ray back and forth
across the slab a number of times between leaving and returning to the
much the same way as a spectrometer table, and provided with arms a meter
long to carry the mirrors b and c. With this length of arm the interference
fringes from sodium light should shift by an amount corresponding to four
hundredths of a wave length when the table is rotated through a right angle.
When the experiment was first performed the apparatus was placed on a
stone pier in the Physical Institute at Berlin. So sensitive was the instrument
to outside vibrations that even after midnight it was found impossible to get
consistent readings. Finally a satisfactory foundation was constructed in the
cellar of the Astrophysical observatory at Potsdam. But what was the
astonishment of the experimenters to find that the expected shift of the
interference fringes did not exist!
Fig. 4.
The extreme delicacy of the experiment made it desirable to confirm the
result by repeating it. This was done by Michelson and Morley (34, 333,
1887) in 1887. In place of a revolving table a massive slab of stone floating
on mercury was used to carry the apparatus. This slab was kept in constant
rotation, the observer following it around. Moreover, the precision of the
experiment was greatly increased by reflecting each ray back and forth
across the slab a number of times between leaving and returning to the
Page 399
mirror m. The accuracy attained was such as to justify Michelson in
declaring that if the effect sought actually existed it could not be so great as
one-twentieth of its calculated value. In 1905 Morley and Miller[166]
repeated the experiment for the second time and succeeded in increasing the
sensitiveness of the apparatus to a point such that a motion through the
ether of one-tenth of the earth’s orbital velocity could have been detected.
The displacement looked for in the Michelson-Morley experiment is
known as a second-order effect in that it depends upon the square of the
ratio of the velocity of the earth to that of light. Michelson at first
considered that the negative result obtained confirmed a theory proposed by
Stokes in which it was assumed that the ether inside and near its surface
partakes of the motion of the earth, while that at a distance is practically
quiescent. But there are many objections to Stokes’ theory, one of which
was brought out by an experiment of Michelson’s (3, 475, 1897) in which
he attempted by an interference method to detect a difference in the velocity
of light at different levels above the earth’s surface. The negative result
obtained led him to conclude that if Stokes’ theory were true the earth’s
influence on the ether would have to extend to a distance above its surface
comparable with its diameter. Meanwhile a more satisfactory explanation
was forthcoming. It has been pointed out that a uniformly convected
electric field is derivable from an electrostatic field by contracting
dimensions in the direction of motion in the ratio
√(1 − β2) : 1.
Fitzgerald and Lorentz showed independently that if moving matter is
distorted in this same way the result obtained by Michelson would be just
that to be expected. For then the distance of the mirror c from m would be
l√(1 − β2)
instead of l, and the path of the ray moving parallel to the earth’s orbit
2l(1 + ½β2),
which is just that of the other ray. Of course when the apparatus is rotated
through 90°, the distance of this mirror from m assumes its normal value
again, and the distance of the other mirror becomes shortened. As all
measurement consists in comparing the object to be measured with a
standard this contraction could never be detected by experimental methods,
declaring that if the effect sought actually existed it could not be so great as
one-twentieth of its calculated value. In 1905 Morley and Miller[166]
repeated the experiment for the second time and succeeded in increasing the
sensitiveness of the apparatus to a point such that a motion through the
ether of one-tenth of the earth’s orbital velocity could have been detected.
The displacement looked for in the Michelson-Morley experiment is
known as a second-order effect in that it depends upon the square of the
ratio of the velocity of the earth to that of light. Michelson at first
considered that the negative result obtained confirmed a theory proposed by
Stokes in which it was assumed that the ether inside and near its surface
partakes of the motion of the earth, while that at a distance is practically
quiescent. But there are many objections to Stokes’ theory, one of which
was brought out by an experiment of Michelson’s (3, 475, 1897) in which
he attempted by an interference method to detect a difference in the velocity
of light at different levels above the earth’s surface. The negative result
obtained led him to conclude that if Stokes’ theory were true the earth’s
influence on the ether would have to extend to a distance above its surface
comparable with its diameter. Meanwhile a more satisfactory explanation
was forthcoming. It has been pointed out that a uniformly convected
electric field is derivable from an electrostatic field by contracting
dimensions in the direction of motion in the ratio
√(1 − β2) : 1.
Fitzgerald and Lorentz showed independently that if moving matter is
distorted in this same way the result obtained by Michelson would be just
that to be expected. For then the distance of the mirror c from m would be
l√(1 − β2)
instead of l, and the path of the ray moving parallel to the earth’s orbit
2l(1 + ½β2),
which is just that of the other ray. Of course when the apparatus is rotated
through 90°, the distance of this mirror from m assumes its normal value
again, and the distance of the other mirror becomes shortened. As all
measurement consists in comparing the object to be measured with a
standard this contraction could never be detected by experimental methods,
Page 400
for the measuring rod would contract in exactly the same ratio as the body
to be measured.
In computing its electromagnetic mass Abraham had assumed the
electron to be a uniformly charged rigid sphere which keeps its spherical
form no matter how great a velocity it may be given. He found that the
mass increases with the speed at very high velocities, becoming infinite as
the velocity of light is approached, and that its value depends upon the
direction of the applied force. After the Fitzgerald-Lorentz contraction was
seen to be necessary in order to explain Michelson’s result, Lorentz
calculated the electromagnetic mass of a charged sphere which is deformed
into an oblate spheroid when set in motion. For this type of electron too, the
mass approaches infinity for velocities as great as that of light, and is
different for different directions. If a force is applied in the direction of
motion the inertia to be overcome is a little greater than when the force is
applied at right angles to this direction. Thus we have to distinguish
between longitudinal and transverse masses. But the masses of Lorentz’s
electron are not the same functions of its velocity as those of Abraham’s.
Kaufmann and after him Bucherer tested experimentally the relation
between transverse mass and velocity by observing the deflections
produced by electric and magnetic fields in the paths of high speed beta
particles. The latter’s work was such an ample confirmation of Lorentz’s
formula that it may be considered as proven that a moving electron at least
suffers contraction in the direction of motion in the ratio
√(1 − β2) : 1.
The electromagnetic theory of light had proved so successful when
applied to bodies at rest that Lorentz was anxious to extend this theory to
the optics of moving media. His problem was to find a group of
homogeneous linear transformations that would leave the form of the
electrodynamic equations unchanged. The Michelson-Morley experiment
had shown that dimensions in the direction of motion must be contracted in
the moving system, those at right angles remaining unaltered. But Lorentz
soon found that it was also necessary to use a new unit of time in the
moving system, and as this time was found to depend upon the position of
the point at which it is to be determined, he called it the local time.
Lorentz’s transformation is just that of the principle of relativity, but he did
not succeed in expressing the electrodynamic equations in terms of the new
to be measured.
In computing its electromagnetic mass Abraham had assumed the
electron to be a uniformly charged rigid sphere which keeps its spherical
form no matter how great a velocity it may be given. He found that the
mass increases with the speed at very high velocities, becoming infinite as
the velocity of light is approached, and that its value depends upon the
direction of the applied force. After the Fitzgerald-Lorentz contraction was
seen to be necessary in order to explain Michelson’s result, Lorentz
calculated the electromagnetic mass of a charged sphere which is deformed
into an oblate spheroid when set in motion. For this type of electron too, the
mass approaches infinity for velocities as great as that of light, and is
different for different directions. If a force is applied in the direction of
motion the inertia to be overcome is a little greater than when the force is
applied at right angles to this direction. Thus we have to distinguish
between longitudinal and transverse masses. But the masses of Lorentz’s
electron are not the same functions of its velocity as those of Abraham’s.
Kaufmann and after him Bucherer tested experimentally the relation
between transverse mass and velocity by observing the deflections
produced by electric and magnetic fields in the paths of high speed beta
particles. The latter’s work was such an ample confirmation of Lorentz’s
formula that it may be considered as proven that a moving electron at least
suffers contraction in the direction of motion in the ratio
√(1 − β2) : 1.
The electromagnetic theory of light had proved so successful when
applied to bodies at rest that Lorentz was anxious to extend this theory to
the optics of moving media. His problem was to find a group of
homogeneous linear transformations that would leave the form of the
electrodynamic equations unchanged. The Michelson-Morley experiment
had shown that dimensions in the direction of motion must be contracted in
the moving system, those at right angles remaining unaltered. But Lorentz
soon found that it was also necessary to use a new unit of time in the
moving system, and as this time was found to depend upon the position of
the point at which it is to be determined, he called it the local time.
Lorentz’s transformation is just that of the principle of relativity, but he did
not succeed in expressing the electrodynamic equations in terms of the new
Page 401
coördinates and time in exactly the same form as for a system at rest, for the
reason that he failed to endow these new units with sufficient reality to
justify him in using them when it came to transforming the velocity term
involved in an electric current.
Principle of Relativity.—In 1905 appeared in the Annalen der Physik[167] a
paper destined to alter entirely the point of view from which problems in
light and electromagnetic theory are to be approached. The author was
Albert Einstein, of Berne, Switzerland, a young man of twenty-six who had
already made a number of notable contributions to theoretical physics.
The principle of relativity proposed by Einstein was by no means new to
students of dynamics. Newton’s first two laws of motion express very
clearly the fact that in mechanics all motion is relative. Force is
proportional to acceleration, and the relation between the two is the same
whether the motion under consideration is referred to fixed axes or to axes
moving with a constant velocity. But in connection with the phenomena of
light and electromagnetism the case seemed to be quite different. There
everything was referred to a fixed ether, and even though Lorentz had found
a set of transformations which left the electrodymanic equations practically
unchanged, he continued to think in terms of an ether. So physicists were
not a little startled when Einstein postulated that no experiment, practical or
ideal, could ever distinguish between two systems in such a manner as to
warrant the assertion that one of them is at rest and the other in motion. All
motion is relative, and the laws governing physical, chemical and biological
phenomena are the same in terms of the units of one system as in terms of
those of any other.
Einstein next considers some very fundamental questions. What do we
mean when we say that two events, one at A and the other at a point B far
from A, occur at the same time? Obviously the expression has no
significance unless synchronous clocks are stationed at the two points. But
how is it to be determined whether or not these two clocks are
synchronous? If instantaneous communication could be established between
A and B the matter would be simple enough. Since no infinite velocity of
transmission is available, however, let a light wave be sent from A to B and
returned to A immediately upon its arrival. If the time indicated by the clock
at B when the signal is received is half way between that at which it left A
and the time at which it arrives on its return, then the two clocks may be
reason that he failed to endow these new units with sufficient reality to
justify him in using them when it came to transforming the velocity term
involved in an electric current.
Principle of Relativity.—In 1905 appeared in the Annalen der Physik[167] a
paper destined to alter entirely the point of view from which problems in
light and electromagnetic theory are to be approached. The author was
Albert Einstein, of Berne, Switzerland, a young man of twenty-six who had
already made a number of notable contributions to theoretical physics.
The principle of relativity proposed by Einstein was by no means new to
students of dynamics. Newton’s first two laws of motion express very
clearly the fact that in mechanics all motion is relative. Force is
proportional to acceleration, and the relation between the two is the same
whether the motion under consideration is referred to fixed axes or to axes
moving with a constant velocity. But in connection with the phenomena of
light and electromagnetism the case seemed to be quite different. There
everything was referred to a fixed ether, and even though Lorentz had found
a set of transformations which left the electrodymanic equations practically
unchanged, he continued to think in terms of an ether. So physicists were
not a little startled when Einstein postulated that no experiment, practical or
ideal, could ever distinguish between two systems in such a manner as to
warrant the assertion that one of them is at rest and the other in motion. All
motion is relative, and the laws governing physical, chemical and biological
phenomena are the same in terms of the units of one system as in terms of
those of any other.
Einstein next considers some very fundamental questions. What do we
mean when we say that two events, one at A and the other at a point B far
from A, occur at the same time? Obviously the expression has no
significance unless synchronous clocks are stationed at the two points. But
how is it to be determined whether or not these two clocks are
synchronous? If instantaneous communication could be established between
A and B the matter would be simple enough. Since no infinite velocity of
transmission is available, however, let a light wave be sent from A to B and
returned to A immediately upon its arrival. If the time indicated by the clock
at B when the signal is received is half way between that at which it left A
and the time at which it arrives on its return, then the two clocks may be
Page 402
considered synchronous. Now if it desired to measure the length of a bar
which is moving parallel to the scale with which the measurement is to be
made, it is necessary to note the positions of the two ends of the bar at the
same instant. So even the measurement of the length of a moving body
depends upon the condition of synchronism at different points in space.
The principle of relativity requires that the velocity of light shall be the
same in one system as in another relative to which the first is in motion.
Hence the definition of synchronism makes it possible to obtain a set of
transformations connecting space and time measurement on one system
with those on another. This group of transformations is exactly that which
Lorentz had found would transform the electrodynamic equations into
themselves. But Einstein’s point of view brought out a remarkable
reciprocity which Lorentz had missed. If two parallel rods MN and OP are
in motion relative to each other in the direction of their lengths, not only
does OP appear shortened to an observer at rest with respect to MN, but
MN appears shorter than normal in the same ratio to an observer who is
moving along with the rod OP.
Einstein’s theory makes the velocity of light the maximum speed with
which a signal can be transmitted. This leads to his celebrated addition
theorem. Consider three observers A, B and C. Let B be moving relative to
A with a velocity of nine-tenths the velocity of light, and C in the same
direction with an equal velocity relative to B. In terms of old-fashioned
notions of time and space, the velocity of C relative to A would be
computed as one and eight-tenths the velocity of light. But the relativity
theory gives it as ninety-nine hundredths the velocity of light. For the
velocity of light can never be surpassed by that of any material object. This
deduction from theory is most strikingly confirmed by the fact that although
beta particles have been observed with velocities as high as ninety-nine
hundredths that of light, the velocity of light is never quite equalled. It may
be remarked in passing that the principle of relativity requires that the
masses of all material bodies shall vary with the velocity in the same
manner as Lorentz found to be the case for the electromagnetic mass of the
deformable electron. In this connection Bumstead (26, 498, 1908) has
devised an elegant method of deducing the ratio of longitudinal to
transverse mass.
which is moving parallel to the scale with which the measurement is to be
made, it is necessary to note the positions of the two ends of the bar at the
same instant. So even the measurement of the length of a moving body
depends upon the condition of synchronism at different points in space.
The principle of relativity requires that the velocity of light shall be the
same in one system as in another relative to which the first is in motion.
Hence the definition of synchronism makes it possible to obtain a set of
transformations connecting space and time measurement on one system
with those on another. This group of transformations is exactly that which
Lorentz had found would transform the electrodynamic equations into
themselves. But Einstein’s point of view brought out a remarkable
reciprocity which Lorentz had missed. If two parallel rods MN and OP are
in motion relative to each other in the direction of their lengths, not only
does OP appear shortened to an observer at rest with respect to MN, but
MN appears shorter than normal in the same ratio to an observer who is
moving along with the rod OP.
Einstein’s theory makes the velocity of light the maximum speed with
which a signal can be transmitted. This leads to his celebrated addition
theorem. Consider three observers A, B and C. Let B be moving relative to
A with a velocity of nine-tenths the velocity of light, and C in the same
direction with an equal velocity relative to B. In terms of old-fashioned
notions of time and space, the velocity of C relative to A would be
computed as one and eight-tenths the velocity of light. But the relativity
theory gives it as ninety-nine hundredths the velocity of light. For the
velocity of light can never be surpassed by that of any material object. This
deduction from theory is most strikingly confirmed by the fact that although
beta particles have been observed with velocities as high as ninety-nine
hundredths that of light, the velocity of light is never quite equalled. It may
be remarked in passing that the principle of relativity requires that the
masses of all material bodies shall vary with the velocity in the same
manner as Lorentz found to be the case for the electromagnetic mass of the
deformable electron. In this connection Bumstead (26, 498, 1908) has
devised an elegant method of deducing the ratio of longitudinal to
transverse mass.
Page 403
The close connection between electrodynamics and the principle of
relativity is obvious from the fact that both lead to the same time and space
transformations. Furthermore L. Page (37, 169, 1914) has shown that the
electrodynamic equations can be derived exactly and in their entirety from
nothing more than the kinematics of relativity and the assumption that every
element of charge is a center of uniformly diverging lines of force. Hence it
may safely be asserted that no purely electromagnetic phenomenon can ever
come into contradiction with this principle. The simplicity thus introduced
into the solution of a certain class of problems is enormous. As an example
consider the question as to whether a moving star is retarded by the reaction
of its own radiation. This purely electrodynamical problem is of such
complexity that attempts to solve it have led to some controversy among
mathematical physicists. The principle of relativity tells us without recourse
to analysis that no retardation can exist.
Throughout the nineteenth century the ether has played a fundamental
part in all important physical theories of light and electromagnetism. But if
it is not possible for experiment to detect even the state of motion of the
ether, why postulate the existence of such a medium? If it does not possess
the most fundamental characteristic of matter, how can it possess such
derived properties as density and elasticity,—properties which any
conceivable mechanical medium must have in order to transmit transverse
vibrations? The relativist does not deny the existence of an ether. To him the
question has no more meaning than if he were asked to express an opinion
as to the reality of parallels of latitude on the earth’s surface. As a
convenient medium of expression in describing certain phenomena the ether
has justified much of the use which has been made of it. But to attribute to
it a degree of substantiality for which there is no warrant in experiment, is
to change it from an aid into an obstacle to the progress of science. From
the relativist point of view the distinction is very sharp between those
motions of charged particles which are experimentally observable, and such
geometrical conventions as electromagnetic fields, or analytical symbols as
electric and magnetic intensities. These modes of representation have been
and still are of the greatest use and importance, but their value in scientific
description must not lead to lack of appreciation of their purely speculative
character.
Finally attention must be drawn to the fact that the discoveries of
inductive science, embodied in the great generalization we have just been
relativity is obvious from the fact that both lead to the same time and space
transformations. Furthermore L. Page (37, 169, 1914) has shown that the
electrodynamic equations can be derived exactly and in their entirety from
nothing more than the kinematics of relativity and the assumption that every
element of charge is a center of uniformly diverging lines of force. Hence it
may safely be asserted that no purely electromagnetic phenomenon can ever
come into contradiction with this principle. The simplicity thus introduced
into the solution of a certain class of problems is enormous. As an example
consider the question as to whether a moving star is retarded by the reaction
of its own radiation. This purely electrodynamical problem is of such
complexity that attempts to solve it have led to some controversy among
mathematical physicists. The principle of relativity tells us without recourse
to analysis that no retardation can exist.
Throughout the nineteenth century the ether has played a fundamental
part in all important physical theories of light and electromagnetism. But if
it is not possible for experiment to detect even the state of motion of the
ether, why postulate the existence of such a medium? If it does not possess
the most fundamental characteristic of matter, how can it possess such
derived properties as density and elasticity,—properties which any
conceivable mechanical medium must have in order to transmit transverse
vibrations? The relativist does not deny the existence of an ether. To him the
question has no more meaning than if he were asked to express an opinion
as to the reality of parallels of latitude on the earth’s surface. As a
convenient medium of expression in describing certain phenomena the ether
has justified much of the use which has been made of it. But to attribute to
it a degree of substantiality for which there is no warrant in experiment, is
to change it from an aid into an obstacle to the progress of science. From
the relativist point of view the distinction is very sharp between those
motions of charged particles which are experimentally observable, and such
geometrical conventions as electromagnetic fields, or analytical symbols as
electric and magnetic intensities. These modes of representation have been
and still are of the greatest use and importance, but their value in scientific
description must not lead to lack of appreciation of their purely speculative
character.
Finally attention must be drawn to the fact that the discoveries of
inductive science, embodied in the great generalization we have just been
Page 404
discussing, have led to a more intimate knowledge of the nature of time and
space than twenty centuries of introspection on the part of professional
philosophers. Minskowski, whose promise of greater achievement was cut
off by an untimely death, has shown that four dimensional geometry makes
possible the representation with beautiful simplicity of the time and space
relationships of this theory. The one time and three space dimensions merge
in such a manner as to form a single whole with not a vestige of
differentiation between these fundamental quantities. Wilson and Lewis[168]
have made this representation familiar to American readers through their
admirable translation of Minskowski’s work into the notation of Gibbs’s
vector analysis.
Aberration, the Doppler effect, anomalous dispersion, —indeed all
known phenomena,—are found to be in accord with the principle of
relativity. It must be borne in mind, however, that this principle applies only
to systems moving relative to one another in straight lines with constant
velocities. That there is something absolute about rotation has been
recognized since Foucault performed his famous pendulum experiment in
1851. This experiment (C. S. Lyman, 12, 251 and 398, 1851) consisted in
setting a pendulum composed of a heavy-brass ball suspended by a long
wire into oscillation in such a way as to avoid appreciable ellipticity in its
motion. Observation of the rate at which the ground rotates relative to the
plane of vibration of the pendulum furnished a method of measuring the
rotation of the earth about its axis without reference to celestial bodies. The
gyroscopic compass in use to-day provides yet another terrestrial method of
detecting this rotation.
The Future of Physics.—At times during the history of physics it has
seemed as if the fundamental laws of this science had been so completely
formulated that nothing remained to future generations beyond the routine
of deducing to the full the consequences of these laws, and increasing the
precision of the methods used to measure the constants appearing in them.
That Laplace held this view has already been pointed out, and Maxwell, in
his introductory lecture at the opening of the Cavendish laboratory in 1871,
said, “This characteristic of modern experiments—that they consist
principally of measurements—is so prominent, that the opinion seems to
have gotten abroad that in a few years all the great physical constants will
have been approximately estimated, and that the only occupation which will
then be left to men of science will be to carry on these measurements to
space than twenty centuries of introspection on the part of professional
philosophers. Minskowski, whose promise of greater achievement was cut
off by an untimely death, has shown that four dimensional geometry makes
possible the representation with beautiful simplicity of the time and space
relationships of this theory. The one time and three space dimensions merge
in such a manner as to form a single whole with not a vestige of
differentiation between these fundamental quantities. Wilson and Lewis[168]
have made this representation familiar to American readers through their
admirable translation of Minskowski’s work into the notation of Gibbs’s
vector analysis.
Aberration, the Doppler effect, anomalous dispersion, —indeed all
known phenomena,—are found to be in accord with the principle of
relativity. It must be borne in mind, however, that this principle applies only
to systems moving relative to one another in straight lines with constant
velocities. That there is something absolute about rotation has been
recognized since Foucault performed his famous pendulum experiment in
1851. This experiment (C. S. Lyman, 12, 251 and 398, 1851) consisted in
setting a pendulum composed of a heavy-brass ball suspended by a long
wire into oscillation in such a way as to avoid appreciable ellipticity in its
motion. Observation of the rate at which the ground rotates relative to the
plane of vibration of the pendulum furnished a method of measuring the
rotation of the earth about its axis without reference to celestial bodies. The
gyroscopic compass in use to-day provides yet another terrestrial method of
detecting this rotation.
The Future of Physics.—At times during the history of physics it has
seemed as if the fundamental laws of this science had been so completely
formulated that nothing remained to future generations beyond the routine
of deducing to the full the consequences of these laws, and increasing the
precision of the methods used to measure the constants appearing in them.
That Laplace held this view has already been pointed out, and Maxwell, in
his introductory lecture at the opening of the Cavendish laboratory in 1871,
said, “This characteristic of modern experiments—that they consist
principally of measurements—is so prominent, that the opinion seems to
have gotten abroad that in a few years all the great physical constants will
have been approximately estimated, and that the only occupation which will
then be left to men of science will be to carry on these measurements to
Page 405
another place of decimals.” That he himself did not entertain this view is
made evident by a succeeding paragraph. “But we have no right to think
thus of the unsearchable riches of creation, or of the untried fertility of
those fresh minds into which these riches will continue to be poured. It may
possibly be true that, in some of those fields of discovery which lie open to
such rough observations as can be made without artificial methods, the
great explorers of former times have appropriated most of what is valuable,
and that the gleanings which remain are sought after rather for their
abstruseness than for their intrinsic worth. But the history of science shows
that even during that phase of her progress in which she devotes herself to
improving the accuracy of the numerical measurement of quantities with
which she has long been familiar, she is preparing the materials for the
subjugation of new regions, which would have remained unknown if she
had been contented with the rough methods of her early pioneers....”
That Maxwell’s forecast of the prospects of his science was no
overestimate will be granted by those who have followed the progress of
physics during the last twenty years. Yet the work accomplished in the past
appears small compared to that which is left to the future. Many of the
unsolved problems are matters of fitting together puzzling details, but there
is at least one whose solution appears to demand a radical modification in
our fundamental physical conceptions. This is the formulation of the laws
which govern the motions of electrons and positively charged particles
inside the atom.
Black Radiation.—The significance of the problem was first brought to
light through the study of black radiation. By a black body is meant one
whose distinguishing characteristic is that it emits and absorbs radiation of
all frequencies, and black radiation is that which will exist in thermal
equilibrium with such a body. The interest of this type of radiation lies in
the fact, demonstrated by Kirchhoff, that its nature depends only upon the
temperature of the black body with which it is in equilibrium, and on none
of this body’s physical or chemical characteristics. Thus we may speak of
the “temperature” of the radiation itself, meaning by this the temperature of
the material body with which it would be in equilibrium.
The problem of black radiation is to find the distribution of energy
among the waves of different frequencies at any given temperature. The
first step toward a solution was made when Stefan showed experimentally,
made evident by a succeeding paragraph. “But we have no right to think
thus of the unsearchable riches of creation, or of the untried fertility of
those fresh minds into which these riches will continue to be poured. It may
possibly be true that, in some of those fields of discovery which lie open to
such rough observations as can be made without artificial methods, the
great explorers of former times have appropriated most of what is valuable,
and that the gleanings which remain are sought after rather for their
abstruseness than for their intrinsic worth. But the history of science shows
that even during that phase of her progress in which she devotes herself to
improving the accuracy of the numerical measurement of quantities with
which she has long been familiar, she is preparing the materials for the
subjugation of new regions, which would have remained unknown if she
had been contented with the rough methods of her early pioneers....”
That Maxwell’s forecast of the prospects of his science was no
overestimate will be granted by those who have followed the progress of
physics during the last twenty years. Yet the work accomplished in the past
appears small compared to that which is left to the future. Many of the
unsolved problems are matters of fitting together puzzling details, but there
is at least one whose solution appears to demand a radical modification in
our fundamental physical conceptions. This is the formulation of the laws
which govern the motions of electrons and positively charged particles
inside the atom.
Black Radiation.—The significance of the problem was first brought to
light through the study of black radiation. By a black body is meant one
whose distinguishing characteristic is that it emits and absorbs radiation of
all frequencies, and black radiation is that which will exist in thermal
equilibrium with such a body. The interest of this type of radiation lies in
the fact, demonstrated by Kirchhoff, that its nature depends only upon the
temperature of the black body with which it is in equilibrium, and on none
of this body’s physical or chemical characteristics. Thus we may speak of
the “temperature” of the radiation itself, meaning by this the temperature of
the material body with which it would be in equilibrium.
The problem of black radiation is to find the distribution of energy
among the waves of different frequencies at any given temperature. The
first step toward a solution was made when Stefan showed experimentally,
Page 406
and Boltzmann as a deduction from thermodynamics and electrodynamics,
that the total energy density summed up over all wave lengths varies with
the fourth power of the absolute temperature. If the energy density is plotted
as ordinate against the wave length as abscissa, the experimental curve for
any one temperature rises from the axis of abscissas at the origin, reaches a
maximum, and falls to zero again as the wave length becomes infinitely
great. Now Wien’s displacement law, the second important step toward the
determination of the form of this curve, shows that as the temperature is
raised the wave length to which its highest point corresponds becomes
shorter,—in fact this particular wave length varies inversely with the
absolute temperature. This theoretical conclusion is entirely confirmed by
experiment. (J. W. Draper, 4, 388, 1847.)
Farther than this general thermodynamical principles are unable to go.
Statistical mechanics, however, asserts that when a large number of like
elements are in thermal equilibrium, the average kinetic energy associated
with each degree of freedom is equal to a universal constant multiplied by
the absolute temperature. This “principle of equi-partition of energy” has
been applied in various ways to obtain a radiation law. The most
straightforward method is based on the equilibrium which must ensue
between radiation field and material oscillators when the latter emit, on the
average, as much energy as they absorb. From whatever aspect the problem
is treated, however, the radiation law obtained from the application of the
equi-partition principle is the same. And while this law agrees well with the
experimental curve for long wave lengths, it shows an energy density that
becomes indefinitely great for extremely short waves, which is not only at
variance with the facts, but actually leads to an infinite value of this
quantity when integrated over the entire spectrum.
The Energy Quantum.—Now the principle of equi-partition of energy
rests securely on most general dynamical principles. That these dynamical
laws are inexact to any such extent as the divergence between theory and
experiment would indicate, is inconceivable; that they are insufficient when
applied to motions of electrons in such intense fields as occur within the
atom seems no longer open to doubt. In order to obtain a radiation formula
in accord with experiment Planck has found it necessary to extend the
atomic idea to energy, which he conceives to exist in multiples of a
fundamental quantum hν, ν being the frequency and h Planck’s constant.
That some such hypothesis of discontinuity is essential in order to obtain
that the total energy density summed up over all wave lengths varies with
the fourth power of the absolute temperature. If the energy density is plotted
as ordinate against the wave length as abscissa, the experimental curve for
any one temperature rises from the axis of abscissas at the origin, reaches a
maximum, and falls to zero again as the wave length becomes infinitely
great. Now Wien’s displacement law, the second important step toward the
determination of the form of this curve, shows that as the temperature is
raised the wave length to which its highest point corresponds becomes
shorter,—in fact this particular wave length varies inversely with the
absolute temperature. This theoretical conclusion is entirely confirmed by
experiment. (J. W. Draper, 4, 388, 1847.)
Farther than this general thermodynamical principles are unable to go.
Statistical mechanics, however, asserts that when a large number of like
elements are in thermal equilibrium, the average kinetic energy associated
with each degree of freedom is equal to a universal constant multiplied by
the absolute temperature. This “principle of equi-partition of energy” has
been applied in various ways to obtain a radiation law. The most
straightforward method is based on the equilibrium which must ensue
between radiation field and material oscillators when the latter emit, on the
average, as much energy as they absorb. From whatever aspect the problem
is treated, however, the radiation law obtained from the application of the
equi-partition principle is the same. And while this law agrees well with the
experimental curve for long wave lengths, it shows an energy density that
becomes indefinitely great for extremely short waves, which is not only at
variance with the facts, but actually leads to an infinite value of this
quantity when integrated over the entire spectrum.
The Energy Quantum.—Now the principle of equi-partition of energy
rests securely on most general dynamical principles. That these dynamical
laws are inexact to any such extent as the divergence between theory and
experiment would indicate, is inconceivable; that they are insufficient when
applied to motions of electrons in such intense fields as occur within the
atom seems no longer open to doubt. In order to obtain a radiation formula
in accord with experiment Planck has found it necessary to extend the
atomic idea to energy, which he conceives to exist in multiples of a
fundamental quantum hν, ν being the frequency and h Planck’s constant.
That some such hypothesis of discontinuity is essential in order to obtain
Page 407
any law that will even approximately fit the experimental facts has been
proved by Poincaré. But the precise spot at which the quantum is introduced
differs for every new derivation of Planck’s law. As deduced most recently
by Planck himself, the quantum shows itself in connection with the
emission of energy by the material oscillators with which the radiation field
is in equilibrium. These oscillators are supposed to act quite normally in
every respect except emission; here the radiation demanded by the
electrodynamic equations is cast aside, and an oscillator is supposed to emit
at once all its energy after it has accumulated an amount equal to some
integral multiple of hν. A form of the theory which does not contain this
improbable contradiction of the firmly established facts of electrodynamics
introduces the quantum into the specification of the energy of vibration
which is permitted to each oscillator. Here both emission and absorption
follow the classical theory, but the motion of an emitting and absorbing
linear oscillator of frequency ν is supposed to be stable only for those
amplitudes for which the energy of its oscillations is an integral multiple of
hν. In order to maintain the energy at these particular values, the oscillator
may draw energy from, or deposit surplus energy with, other degrees of
freedom which partake neither in emission nor absorption, but act merely as
storehouses.
Photoelectric Effect.—When investigating the production of
electromagnetic waves, Hertz had noticed that a spark passed more readily
between the terminals of his oscillator when the negative electrode was
illuminated by light from another spark. Further investigation by
Hallwachs, Elster and Geitel, and others showed that this effect was due to
the emission of electrons by a metal exposed to the influence of ultra-violet
light. Lenard discovered that the energy with which a negatively charged
particle is ejected is entirely independent of the intensity of the light, and
further investigation showed it to depend only on the frequency. Einstein
suggested that the electrons appearing in this so-called photo-electric effect
start from within the metal with an initial energy hν. In passing through the
surface a resistance is encountered, however, so he concluded that the
energy with which the fastest moving electrons appear outside the metal
should be equal to hν less the work done in overcoming this resistance.
Recent experiments not only confirm this relation, but provide a most
satisfactory method of determining the value of h. Millikan[169] finds it to be
6·57(10)–27 ergs sec., which gives the quantum for yellow light a value sixty
proved by Poincaré. But the precise spot at which the quantum is introduced
differs for every new derivation of Planck’s law. As deduced most recently
by Planck himself, the quantum shows itself in connection with the
emission of energy by the material oscillators with which the radiation field
is in equilibrium. These oscillators are supposed to act quite normally in
every respect except emission; here the radiation demanded by the
electrodynamic equations is cast aside, and an oscillator is supposed to emit
at once all its energy after it has accumulated an amount equal to some
integral multiple of hν. A form of the theory which does not contain this
improbable contradiction of the firmly established facts of electrodynamics
introduces the quantum into the specification of the energy of vibration
which is permitted to each oscillator. Here both emission and absorption
follow the classical theory, but the motion of an emitting and absorbing
linear oscillator of frequency ν is supposed to be stable only for those
amplitudes for which the energy of its oscillations is an integral multiple of
hν. In order to maintain the energy at these particular values, the oscillator
may draw energy from, or deposit surplus energy with, other degrees of
freedom which partake neither in emission nor absorption, but act merely as
storehouses.
Photoelectric Effect.—When investigating the production of
electromagnetic waves, Hertz had noticed that a spark passed more readily
between the terminals of his oscillator when the negative electrode was
illuminated by light from another spark. Further investigation by
Hallwachs, Elster and Geitel, and others showed that this effect was due to
the emission of electrons by a metal exposed to the influence of ultra-violet
light. Lenard discovered that the energy with which a negatively charged
particle is ejected is entirely independent of the intensity of the light, and
further investigation showed it to depend only on the frequency. Einstein
suggested that the electrons appearing in this so-called photo-electric effect
start from within the metal with an initial energy hν. In passing through the
surface a resistance is encountered, however, so he concluded that the
energy with which the fastest moving electrons appear outside the metal
should be equal to hν less the work done in overcoming this resistance.
Recent experiments not only confirm this relation, but provide a most
satisfactory method of determining the value of h. Millikan[169] finds it to be
6·57(10)–27 ergs sec., which gives the quantum for yellow light a value sixty
Page 408
times as great as the heat energy of a monatomic gas molecule at O°C. That
this large amount of energy can be transferred from the incident light to the
ejected electron is quite out of the question; it must come from within the
atom. In this way some indication is obtained of how vast intra-atomic
energies must be.
Structure of the Atom.—The generally accepted model of the atom is that
due chiefly to Rutherford.[170] He considers it to be constituted of electrons
revolving about a positive nucleus either singly or grouped in concentric
rings, in much the same manner as the planets revolve around the sun.
Experiments on the scattering of alpha rays, however, show that the
nucleus, while it must have a positive charge sufficient to neutralize the
charges of all the electrons moving around it, cannot have a volume of an
order of magnitude greater than that of the electron. The number of unit
charges residing on it, except in the case of hydrogen, which is supposed to
consist of a singly charged nucleus and only one electron, is found to be
approximately half the atomic weight. Thus helium, with an atomic weight
of about four, has a doubly charged nucleus with two electrons revolving
about it, and lithium a triply charged nucleus and three electrons. The
number of unit charges on the nucleus is supposed to correspond with the
atomic number used by Moseley in interpreting the results of his
experiment on the X-ray spectra of the elements.
Now the electron which is revolving around the positive nucleus of a
hydrogen atom, must, according to electrodynamic laws, radiate energy.
This radiation will act as a resistance to its motion, causing its orbit to
become smaller and its frequency to increase. Hence luminous hydrogen
would be expected to give off a continuous spectrum. The very fine lines
actually found seem inexplicable on the classical dynamical and
electrodynamical theories. These lines, and those of many other spectra,
may even be grouped into series, and the relations between them expressed
in mathematical form. Formulæ have been proposed by Balmer, Rydberg,
Ritz and others, all of which contain a universal constant N as well as
certain parameters which must be varied by unity in passing from one line
of a series to the next.
In 1913 Bohr[171] proposed anatomic theory which brings to light a
remarkable numerical relationship between this quantity N and Planck’s
constant h. He postulated that the electron in the hydrogen atom, for
this large amount of energy can be transferred from the incident light to the
ejected electron is quite out of the question; it must come from within the
atom. In this way some indication is obtained of how vast intra-atomic
energies must be.
Structure of the Atom.—The generally accepted model of the atom is that
due chiefly to Rutherford.[170] He considers it to be constituted of electrons
revolving about a positive nucleus either singly or grouped in concentric
rings, in much the same manner as the planets revolve around the sun.
Experiments on the scattering of alpha rays, however, show that the
nucleus, while it must have a positive charge sufficient to neutralize the
charges of all the electrons moving around it, cannot have a volume of an
order of magnitude greater than that of the electron. The number of unit
charges residing on it, except in the case of hydrogen, which is supposed to
consist of a singly charged nucleus and only one electron, is found to be
approximately half the atomic weight. Thus helium, with an atomic weight
of about four, has a doubly charged nucleus with two electrons revolving
about it, and lithium a triply charged nucleus and three electrons. The
number of unit charges on the nucleus is supposed to correspond with the
atomic number used by Moseley in interpreting the results of his
experiment on the X-ray spectra of the elements.
Now the electron which is revolving around the positive nucleus of a
hydrogen atom, must, according to electrodynamic laws, radiate energy.
This radiation will act as a resistance to its motion, causing its orbit to
become smaller and its frequency to increase. Hence luminous hydrogen
would be expected to give off a continuous spectrum. The very fine lines
actually found seem inexplicable on the classical dynamical and
electrodynamical theories. These lines, and those of many other spectra,
may even be grouped into series, and the relations between them expressed
in mathematical form. Formulæ have been proposed by Balmer, Rydberg,
Ritz and others, all of which contain a universal constant N as well as
certain parameters which must be varied by unity in passing from one line
of a series to the next.
In 1913 Bohr[171] proposed anatomic theory which brings to light a
remarkable numerical relationship between this quantity N and Planck’s
constant h. He postulated that the electron in the hydrogen atom, for
Page 409
instance, cannot revolve in a circle of any arbitrary radius, but is confined to
those orbits for which its kinetic energy is an integral multiple of ½hn, n
being its orbital frequency. Now at times this electron is supposed to jump
from an outer to an inner orbit, when the excess energy of the first orbit
over the second is radiated away. But the energy emitted is also taken to be
equal to hν, where ν is the frequency of the radiation. Hence ν can be
determined, and the expression obtained for it is exactly that given long
before by Balmer as an empirical law. The most remarkable thing about it,
however, is that Bohr’s result contains a constant involving h and the
electronic charge and mass which has precisely the value of the universal
constant N of Balmer’s and Rydberg’s formulæ. In all, the theory accounts
for three series of hydrogen, and yields satisfactory results for helium atoms
which have lost an electron, or lithium atoms which have a double positive
charge. But for atoms which retain more than a single electron it seems no
longer to hold.
The three mentioned are only the most clearly defined of a growing
group of phenomena in which the quantum manifests itself. Its significance
and the alteration in our fundamental conceptions to which it seems to be
leading is for the future to make clear. That it presents the most important
and interesting problem as yet unsolved few physicists would deny.
American Physicists.—In attempting to cover the progress of physics
during the last hundred years in the space of a few pages, many important
developments of the subject have of necessity remained untouched, and the
treatment of many others has been entirely inadequate. Among those
appearing in the Journal of which no mention has been made are LeConte’s
(25, 62, 1858) discovery of the sensitive flame and Rood’s (46, 173, 1893)
invention of the flicker photometer. However, enough has been recounted to
indicate the preeminent position in the history of physics in America
occupied by four men: Joseph Henry, of the Albany Academy, Princeton,
and the Smithsonian Institution; Henry Augustus Rowland, of Johns
Hopkins University; Josiah Willard Gibbs, of Yale; and Albert Abraham
Michelson, of the United States Naval Academy, Case School of Applied
Science, Clark University, and the University of Chicago. Of these, the last
named has the distinction of being the only American physicist to have
received the Nobel prize, though there is little doubt that the other three
would have been similarly honored had not their important work been
published prior to the institution of this award. All four occupy high places
those orbits for which its kinetic energy is an integral multiple of ½hn, n
being its orbital frequency. Now at times this electron is supposed to jump
from an outer to an inner orbit, when the excess energy of the first orbit
over the second is radiated away. But the energy emitted is also taken to be
equal to hν, where ν is the frequency of the radiation. Hence ν can be
determined, and the expression obtained for it is exactly that given long
before by Balmer as an empirical law. The most remarkable thing about it,
however, is that Bohr’s result contains a constant involving h and the
electronic charge and mass which has precisely the value of the universal
constant N of Balmer’s and Rydberg’s formulæ. In all, the theory accounts
for three series of hydrogen, and yields satisfactory results for helium atoms
which have lost an electron, or lithium atoms which have a double positive
charge. But for atoms which retain more than a single electron it seems no
longer to hold.
The three mentioned are only the most clearly defined of a growing
group of phenomena in which the quantum manifests itself. Its significance
and the alteration in our fundamental conceptions to which it seems to be
leading is for the future to make clear. That it presents the most important
and interesting problem as yet unsolved few physicists would deny.
American Physicists.—In attempting to cover the progress of physics
during the last hundred years in the space of a few pages, many important
developments of the subject have of necessity remained untouched, and the
treatment of many others has been entirely inadequate. Among those
appearing in the Journal of which no mention has been made are LeConte’s
(25, 62, 1858) discovery of the sensitive flame and Rood’s (46, 173, 1893)
invention of the flicker photometer. However, enough has been recounted to
indicate the preeminent position in the history of physics in America
occupied by four men: Joseph Henry, of the Albany Academy, Princeton,
and the Smithsonian Institution; Henry Augustus Rowland, of Johns
Hopkins University; Josiah Willard Gibbs, of Yale; and Albert Abraham
Michelson, of the United States Naval Academy, Case School of Applied
Science, Clark University, and the University of Chicago. Of these, the last
named has the distinction of being the only American physicist to have
received the Nobel prize, though there is little doubt that the other three
would have been similarly honored had not their important work been
published prior to the institution of this award. All four occupy high places
Page 410
in the ranks of the world’s great men of science, and the investigations
carried out by them and their fellow workers in America have given to their
country a position in the annals of physics which is by no means
insignificant.
carried out by them and their fellow workers in America have given to their
country a position in the annals of physics which is by no means
insignificant.
Page 411
The Journal’s Part in Meteorology.
The meteorological investigations published in the early numbers of the
Journal have played an important role in establishing a correct theory of
storms. Before the origin of the United States Signal Service in 1871 no
systematic weather reports were issued by any governmental agency in this
country, and consequently the work of collecting as well as interpreting
meteorological data rested entirely in the hands of interested individuals
and institutions. The earliest important studies of storms to appear in the
Journal were contributed by Redfield of New York, whose first paper (20,
17, 1831) treated in considerable detail a violent storm which passed over
Long Island, Connecticut and Massachusetts in 1821. He concluded that
“the direction of the wind at a particular place, forms no part of the essential
character of a storm, but is only incidental to that particular portion ... of the
track of the storm which may chance to become the point of observation, ...
the direction of the wind being, in all cases, compounded of both the
rotative and progressive velocities of the storm.” A few years later, analyses
of twelve “gales and hurricanes of the Western Atlantic” (31, 115, 1837) led
to the statement that the phenomena involved “are to be ascribed mainly to
the mechanical gravitation of the atmosphere, as connected with the rotative
and orbital movements of the earth’s surface.” In this paper is emphasized
the fact that the wind may blow in diametrically opposite directions at
points near the storm center. “While one vessel has been lying-to in a heavy
gale of wind, another, not more than thirty leagues distant, has at the very
same time been in another gale equally heavy, and lying-to with the wind in
quite an opposite direction.” From an accompanying sketch showing wind
directions, the reader would infer that, at this time, Redfield believed the
motion of the air to be very nearly in circles about the storm center. The
same idea is conveyed by a later paper (42, 112, 1842). Espy (39, 120,
1840) of Philadelphia, however, claimed that observation showed rather that
the wind blew inwards toward a central point, if the storm were round in
shape, or toward a central line, if it were oblong. This view Redfield (42,
112, 1842) contested, and brought forth much evidence to prove its falsity.
A later statement (1, 1, 1846) of his own theory is as follows: “I have never
been able to conceive, that the wind in violent storms moves only in circles.
The meteorological investigations published in the early numbers of the
Journal have played an important role in establishing a correct theory of
storms. Before the origin of the United States Signal Service in 1871 no
systematic weather reports were issued by any governmental agency in this
country, and consequently the work of collecting as well as interpreting
meteorological data rested entirely in the hands of interested individuals
and institutions. The earliest important studies of storms to appear in the
Journal were contributed by Redfield of New York, whose first paper (20,
17, 1831) treated in considerable detail a violent storm which passed over
Long Island, Connecticut and Massachusetts in 1821. He concluded that
“the direction of the wind at a particular place, forms no part of the essential
character of a storm, but is only incidental to that particular portion ... of the
track of the storm which may chance to become the point of observation, ...
the direction of the wind being, in all cases, compounded of both the
rotative and progressive velocities of the storm.” A few years later, analyses
of twelve “gales and hurricanes of the Western Atlantic” (31, 115, 1837) led
to the statement that the phenomena involved “are to be ascribed mainly to
the mechanical gravitation of the atmosphere, as connected with the rotative
and orbital movements of the earth’s surface.” In this paper is emphasized
the fact that the wind may blow in diametrically opposite directions at
points near the storm center. “While one vessel has been lying-to in a heavy
gale of wind, another, not more than thirty leagues distant, has at the very
same time been in another gale equally heavy, and lying-to with the wind in
quite an opposite direction.” From an accompanying sketch showing wind
directions, the reader would infer that, at this time, Redfield believed the
motion of the air to be very nearly in circles about the storm center. The
same idea is conveyed by a later paper (42, 112, 1842). Espy (39, 120,
1840) of Philadelphia, however, claimed that observation showed rather that
the wind blew inwards toward a central point, if the storm were round in
shape, or toward a central line, if it were oblong. This view Redfield (42,
112, 1842) contested, and brought forth much evidence to prove its falsity.
A later statement (1, 1, 1846) of his own theory is as follows: “I have never
been able to conceive, that the wind in violent storms moves only in circles.
Page 412
On the contrary, a vortical movement ... appears to be an essential element
of their violent and long-continued action, of their increased energy towards
the center or axis, and of the accompanying rain.... The degree of vorticular
inclination in violent storms must be subject, locally, to great variations; but
it is not probable that, on an average of the different sides, it ever comes
near to forty-five degrees from the tangent of a circle,—and that such
average inclination ever exceeds two points of the compass, may well be
doubted.” A qualitative explanation of the effect of the earth’s rotation on
the direction of the wind near the storm center had already been given by
Tracy (45, 65, 1843), and this was followed some years later by Ferrel’s
(31, 27, 1861) very thorough quantitative investigation of the dynamics of
the atmosphere.
A number of individuals kept systematic records of meteorological
observations, among whom was Loomis, whose storm analyses did much to
settle the merits of the rival theories of Redfield and Espy. In studying the
storm of 1836 (40, 34, 1841) he had drawn on the map lines through those
points in the track of the storm where the barometer, at any given hour, is
lowest. While this method revealed the general direction in which the storm
was progressing, it failed to give much indication of its size or shape. In
discussing the two tornadoes of February, 1842, one of which had already
been described in the Journal (43, 278, 1842), he adopted a new and more
illuminating graphical method. Instead of connecting points of lowest
pressure, he drew a curve through all points where the barometer stood at
its normal level, then one through those points at which the pressure was ²⁄₁₀
of an inch below normal, and so on. Temperature he treated in much the
same way, and the strength and direction of the wind were indicated by
arrows. This innovation gave to his storm analyses a significance which had
been entirely lacking in those of his predecessors, and led to the familiar
systems of isobars and isotherms in use on the daily charts issued by the
Weather Bureau at the present time. Loomis advocated careful observations
for one year at stations 50 miles apart all over the United States, so that
sufficient data might be obtained to settle once for all the law of storms. His
efforts, seconded by those of Henry, Bache, Pierce, Abbe, and Lapham, led
eventually to the establishment of the Signal Service, and the publication of
daily weather maps according to the plan advocated thirty years before.
These maps afforded a basis for further analyses of storms, which he
of their violent and long-continued action, of their increased energy towards
the center or axis, and of the accompanying rain.... The degree of vorticular
inclination in violent storms must be subject, locally, to great variations; but
it is not probable that, on an average of the different sides, it ever comes
near to forty-five degrees from the tangent of a circle,—and that such
average inclination ever exceeds two points of the compass, may well be
doubted.” A qualitative explanation of the effect of the earth’s rotation on
the direction of the wind near the storm center had already been given by
Tracy (45, 65, 1843), and this was followed some years later by Ferrel’s
(31, 27, 1861) very thorough quantitative investigation of the dynamics of
the atmosphere.
A number of individuals kept systematic records of meteorological
observations, among whom was Loomis, whose storm analyses did much to
settle the merits of the rival theories of Redfield and Espy. In studying the
storm of 1836 (40, 34, 1841) he had drawn on the map lines through those
points in the track of the storm where the barometer, at any given hour, is
lowest. While this method revealed the general direction in which the storm
was progressing, it failed to give much indication of its size or shape. In
discussing the two tornadoes of February, 1842, one of which had already
been described in the Journal (43, 278, 1842), he adopted a new and more
illuminating graphical method. Instead of connecting points of lowest
pressure, he drew a curve through all points where the barometer stood at
its normal level, then one through those points at which the pressure was ²⁄₁₀
of an inch below normal, and so on. Temperature he treated in much the
same way, and the strength and direction of the wind were indicated by
arrows. This innovation gave to his storm analyses a significance which had
been entirely lacking in those of his predecessors, and led to the familiar
systems of isobars and isotherms in use on the daily charts issued by the
Weather Bureau at the present time. Loomis advocated careful observations
for one year at stations 50 miles apart all over the United States, so that
sufficient data might be obtained to settle once for all the law of storms. His
efforts, seconded by those of Henry, Bache, Pierce, Abbe, and Lapham, led
eventually to the establishment of the Signal Service, and the publication of
daily weather maps according to the plan advocated thirty years before.
These maps afforded a basis for further analyses of storms, which he
Page 413
published in numerous “Contributions to Meteorology” (8, 1, 1874, et seq.)
between 1874 and his death in 1890.
In addition to his work on storms, Loomis made a careful study of the
earth’s magnetism (34, 290, 1838 et seq.), and of the aurora borealis (28,
385, 1859 et seq.). That a connection existed between sunspots, aurora, and
terrestrial magnetism was already recognized. Loomis (50, 153, 1870 et
seq.), however, showed that the periodicity of the aurora borealis, as well as
of excessive disturbances in the earth’s magnetic field, corresponds very
closely with that of sunspots.
between 1874 and his death in 1890.
In addition to his work on storms, Loomis made a careful study of the
earth’s magnetism (34, 290, 1838 et seq.), and of the aurora borealis (28,
385, 1859 et seq.). That a connection existed between sunspots, aurora, and
terrestrial magnetism was already recognized. Loomis (50, 153, 1870 et
seq.), however, showed that the periodicity of the aurora borealis, as well as
of excessive disturbances in the earth’s magnetic field, corresponds very
closely with that of sunspots.
Page 414
Notes.
154. J. W. Gibbs, Trans. Conn. Acad. Arts and Sci., 3, 108 and 343. Abstract by the author, the
Journal, 16, 441, 1878.
155. H. K. Onnes, Nature, 93, 481, 1914.
156. H. Hertz, Wied. Ann., 34, 551, 1888 et seq.
157. E. F. Nichols and G. F. Hull, Phys. Rev., 13, 307, 1901 et seq.
158. J. J. Thomson, Phil. Mag., 44, 293, 1897.
159. R. A. Millikan, Phys. Rev., 2, 109, 1913.
160. P. Zeeman, Phil. Mag., 43, 226, 1897.
161. H. A. Lorentz, Phil. Mag., 43, 232, 1897.
162. S. J. Barnett, Phys. Rev., 6, 239, 1915, and 10, 7, 1917.
163. W. C. Röntgen, Wied. Ann., 64, 1, 1898 et seq.
164. W. Friedrich, P. Knipping, and M. Laue, Ann. d. Phys., 41, 971, 1913.
165. H. G. J. Moseley, Phil. Mag., 26, 1024, 1913, and 27, 703, 1914.
166. E. W. Morley and D. C. Miller, Phil. Mag., 9, 680, 1905.
167. 17, 891, 1905.
168. E. B. Wilson and G. N. Lewis, Proc. Am. Acad., of Arts and Sci., 48, 389, 1912.
169. R. A. Millikan, Phys. Rev., 7, 355, 1916.
170. E. Rutherford, Phil. Mag., 21, 669, 1911.
171. N. Bohr, Phil. Mag., 26, 1, 1913 et seq.
154. J. W. Gibbs, Trans. Conn. Acad. Arts and Sci., 3, 108 and 343. Abstract by the author, the
Journal, 16, 441, 1878.
155. H. K. Onnes, Nature, 93, 481, 1914.
156. H. Hertz, Wied. Ann., 34, 551, 1888 et seq.
157. E. F. Nichols and G. F. Hull, Phys. Rev., 13, 307, 1901 et seq.
158. J. J. Thomson, Phil. Mag., 44, 293, 1897.
159. R. A. Millikan, Phys. Rev., 2, 109, 1913.
160. P. Zeeman, Phil. Mag., 43, 226, 1897.
161. H. A. Lorentz, Phil. Mag., 43, 232, 1897.
162. S. J. Barnett, Phys. Rev., 6, 239, 1915, and 10, 7, 1917.
163. W. C. Röntgen, Wied. Ann., 64, 1, 1898 et seq.
164. W. Friedrich, P. Knipping, and M. Laue, Ann. d. Phys., 41, 971, 1913.
165. H. G. J. Moseley, Phil. Mag., 26, 1024, 1913, and 27, 703, 1914.
166. E. W. Morley and D. C. Miller, Phil. Mag., 9, 680, 1905.
167. 17, 891, 1905.
168. E. B. Wilson and G. N. Lewis, Proc. Am. Acad., of Arts and Sci., 48, 389, 1912.
169. R. A. Millikan, Phys. Rev., 7, 355, 1916.
170. E. Rutherford, Phil. Mag., 21, 669, 1911.
171. N. Bohr, Phil. Mag., 26, 1, 1913 et seq.
Page 415
XII
A CENTURY OF ZOOLOGY IN AMERICA
By WESLEY K. COE
This article is intended as a brief survey of the development of zoology in
America, and no attempt is made to give a general history of the science.
There are numerous accounts in several languages of zoological history in
general, among them being W. A. Locy’s “Biology and its Makers.” Brief
outlines of the history of zoology may be found in many zoological and
biological text-books.
For the history of American zoology the reader is referred to Packard’s
report on “A Century’s Progress in American Zoology,” published in the
American Naturalist, (10, 591, 1876), to Packard’s “History of Zoology,”
published in volume 1 of the Standard Natural History (pp. lxii to lxxii,
1885); to G. B. Goode’s “Beginnings of Natural History in America,”[172]
and “Beginnings of American Science,”[173] and to H. S. Pratt’s Manual of
the Common Invertebrate Animals (pp. 1–9), 1916. In Binney’s “Terrestrial
Air-breathing Mollusks of the United States” (1851) is a chapter on the rise
of scientific zoology in the United States which well describes the
zoological conditions in the early part of the century, while numerous
monographs and papers give the history of the investigations on the various
groups of animals or on special fields of study.
Brief biographical sketches of the most distinguished of our older
Naturalists—Wilson, Audubon, Agassiz, Wyman, Gray, Dana, Baird,
Marsh, Cope, Goode and Brooks are given in “Leading American Men of
Science,” edited by David Starr Jordan, 1910. More extensive biographies
have been published separately, and the activities of a number of the more
A CENTURY OF ZOOLOGY IN AMERICA
By WESLEY K. COE
This article is intended as a brief survey of the development of zoology in
America, and no attempt is made to give a general history of the science.
There are numerous accounts in several languages of zoological history in
general, among them being W. A. Locy’s “Biology and its Makers.” Brief
outlines of the history of zoology may be found in many zoological and
biological text-books.
For the history of American zoology the reader is referred to Packard’s
report on “A Century’s Progress in American Zoology,” published in the
American Naturalist, (10, 591, 1876), to Packard’s “History of Zoology,”
published in volume 1 of the Standard Natural History (pp. lxii to lxxii,
1885); to G. B. Goode’s “Beginnings of Natural History in America,”[172]
and “Beginnings of American Science,”[173] and to H. S. Pratt’s Manual of
the Common Invertebrate Animals (pp. 1–9), 1916. In Binney’s “Terrestrial
Air-breathing Mollusks of the United States” (1851) is a chapter on the rise
of scientific zoology in the United States which well describes the
zoological conditions in the early part of the century, while numerous
monographs and papers give the history of the investigations on the various
groups of animals or on special fields of study.
Brief biographical sketches of the most distinguished of our older
Naturalists—Wilson, Audubon, Agassiz, Wyman, Gray, Dana, Baird,
Marsh, Cope, Goode and Brooks are given in “Leading American Men of
Science,” edited by David Starr Jordan, 1910. More extensive biographies
have been published separately, and the activities of a number of the more
Page 416
prominent American zoologists have been recorded in the Biographical
Memoirs of the National Academy of Sciences.
The developmental history of zoology in America falls naturally into four
fairly well marked periods, namely:—1, Period of descriptive natural
history, previous to 1847, embracing the early studies on the classification
and habits of animals, characteristic of the zoological work previous to the
arrival of Louis Agassiz in America. 2, Period of morphology and
embryology, 1847–1870, during which the influence of Agassiz directed the
zoological studies toward problems concerning the relationships of animals
as indicated by their structure and developmental history. 3, Period of
evolution, 1870–1890, when the principle of natural selection received
general recognition and the zoological studies were largely devoted to the
applications of the theory to all groups of animals. 4, Period of
experimental biology, since 1890, during which time have occurred the
remarkable advances in our knowledge of the nature of organisms through
the application of experimental methods in the various branches of the
modern science of biology.
Memoirs of the National Academy of Sciences.
The developmental history of zoology in America falls naturally into four
fairly well marked periods, namely:—1, Period of descriptive natural
history, previous to 1847, embracing the early studies on the classification
and habits of animals, characteristic of the zoological work previous to the
arrival of Louis Agassiz in America. 2, Period of morphology and
embryology, 1847–1870, during which the influence of Agassiz directed the
zoological studies toward problems concerning the relationships of animals
as indicated by their structure and developmental history. 3, Period of
evolution, 1870–1890, when the principle of natural selection received
general recognition and the zoological studies were largely devoted to the
applications of the theory to all groups of animals. 4, Period of
experimental biology, since 1890, during which time have occurred the
remarkable advances in our knowledge of the nature of organisms through
the application of experimental methods in the various branches of the
modern science of biology.
Page 417
American Zoology in 1818.
At the beginning of the century which this volume commemorates, the
accumulated biological knowledge of the world consisted mainly of what is
to-day called descriptive natural history. The zoological treatises of the time
were devoted to the names, distinguishing characters and habits of the
species of animals and plants known to the naturalists of Europe either as
native species or as the results of explorations in other parts of the world.
This required little more than a superficial knowledge of their general
anatomical structures.
The naturalists of those days had no conception of the life within the cell
which we now know to form the basis of all the activities of animals and
plants, nor had they even the necessary means of studying such life. The
compound microscope, so necessary for the study of even the largest of the
cells of the body, was not adapted to such use until 1835, although the
instrument was invented in the seventeenth century. With the perfection of
the microscope came a period of enthusiastic study of microscopic
organisms and microscopic structures of higher animals and plants. It was
not until twenty years after the founding of the Journal that the cell theory
of structure and function in all organisms was established by the discoveries
of Schleiden and Schwann.
The beginning of the nineteenth century saw great zoological activity in
Europe, and particularly in France. Buffon’s great work on the Natural
History of Animals had recently been completed, Cuvier had only one year
before published his classic work in comparative anatomy, “Le Regne
Animal,” and Lamarck’s “Philosophie Zoologique” had then aroused a new
interest in classification and comparative anatomy from an evolutionary
standpoint. E. Geoffroy St.-Hilaire was at the same time supporting an
evolutionary theory based on embryonic influences resulting in sudden
modifications of adult structure. These epoch-making discoveries and
theories gained a considerable following in France, Germany and England,
but seem to have had little influence on the zoological work of the
following half century in America.
At the beginning of the century which this volume commemorates, the
accumulated biological knowledge of the world consisted mainly of what is
to-day called descriptive natural history. The zoological treatises of the time
were devoted to the names, distinguishing characters and habits of the
species of animals and plants known to the naturalists of Europe either as
native species or as the results of explorations in other parts of the world.
This required little more than a superficial knowledge of their general
anatomical structures.
The naturalists of those days had no conception of the life within the cell
which we now know to form the basis of all the activities of animals and
plants, nor had they even the necessary means of studying such life. The
compound microscope, so necessary for the study of even the largest of the
cells of the body, was not adapted to such use until 1835, although the
instrument was invented in the seventeenth century. With the perfection of
the microscope came a period of enthusiastic study of microscopic
organisms and microscopic structures of higher animals and plants. It was
not until twenty years after the founding of the Journal that the cell theory
of structure and function in all organisms was established by the discoveries
of Schleiden and Schwann.
The beginning of the nineteenth century saw great zoological activity in
Europe, and particularly in France. Buffon’s great work on the Natural
History of Animals had recently been completed, Cuvier had only one year
before published his classic work in comparative anatomy, “Le Regne
Animal,” and Lamarck’s “Philosophie Zoologique” had then aroused a new
interest in classification and comparative anatomy from an evolutionary
standpoint. E. Geoffroy St.-Hilaire was at the same time supporting an
evolutionary theory based on embryonic influences resulting in sudden
modifications of adult structure. These epoch-making discoveries and
theories gained a considerable following in France, Germany and England,
but seem to have had little influence on the zoological work of the
following half century in America.
Page 418
The science of zoology as understood to-day is commonly said to have
been founded by Linnæus by the publication of the modern system of
classification in the tenth edition of his “Systema Naturæ” in 1758. The
influence of Linnæus aroused an interest in biological studies throughout
Europe and stimulated new investigations in all groups of organisms. Such
studies as related to animals naturally followed first the classification and
relationship of species, that is, systematic zoology, and then led gradually
into the development of the different branches of the subject, as
morphology, comparative anatomy, physiology, and embryology, which
eventually were recognized as almost independent sciences.
Of these sciences systematic zoology, which has come to mean the
classification, structure, relationship, distribution and habits, or natural
history, is the pioneer in any region. Thus we find in our new country at the
time of the founding of the Journal in 1818, only sixty years after the
publication of Linnæus’ great work, the beginning of American zoology
taking the form of the collection and description of our native animals.
It is true that many of our more conspicuous and easily collected animals
were described long before the opening of the nineteenth century, but this is
to be credited mainly to the work of European naturalists who had made
expeditions to this country for the purpose of studying and collecting. These
collections were then taken to Europe and the results published there. We
thus find in the 12th edition of Linnæus descriptions of over 500 American
species, about half of which were birds. As an illustration of the extent to
which some of these works covered the field even in those early days may
be mentioned a monograph in two quarto volumes with many beautifully
colored plates on the “Natural History of the rarer Lepidopterous Insects of
Georgia.” This was published in London in 1797 by J. E. Smith from the
notes and drawings of John Abbot, one of the keenest naturalists of any
period.
During the early years of the nineteenth century, however, economic
conditions in our country became such as to give opportunity for scientific
thought. Educated men then formed themselves into societies for the
discussion of scientific matters. This naturally led to the establishment of
publications whereby the papers presented to the societies could be
published and made available to the advancement of science generally. The
most influential of these was the Journal of the Philadelphia Academy of
been founded by Linnæus by the publication of the modern system of
classification in the tenth edition of his “Systema Naturæ” in 1758. The
influence of Linnæus aroused an interest in biological studies throughout
Europe and stimulated new investigations in all groups of organisms. Such
studies as related to animals naturally followed first the classification and
relationship of species, that is, systematic zoology, and then led gradually
into the development of the different branches of the subject, as
morphology, comparative anatomy, physiology, and embryology, which
eventually were recognized as almost independent sciences.
Of these sciences systematic zoology, which has come to mean the
classification, structure, relationship, distribution and habits, or natural
history, is the pioneer in any region. Thus we find in our new country at the
time of the founding of the Journal in 1818, only sixty years after the
publication of Linnæus’ great work, the beginning of American zoology
taking the form of the collection and description of our native animals.
It is true that many of our more conspicuous and easily collected animals
were described long before the opening of the nineteenth century, but this is
to be credited mainly to the work of European naturalists who had made
expeditions to this country for the purpose of studying and collecting. These
collections were then taken to Europe and the results published there. We
thus find in the 12th edition of Linnæus descriptions of over 500 American
species, about half of which were birds. As an illustration of the extent to
which some of these works covered the field even in those early days may
be mentioned a monograph in two quarto volumes with many beautifully
colored plates on the “Natural History of the rarer Lepidopterous Insects of
Georgia.” This was published in London in 1797 by J. E. Smith from the
notes and drawings of John Abbot, one of the keenest naturalists of any
period.
During the early years of the nineteenth century, however, economic
conditions in our country became such as to give opportunity for scientific
thought. Educated men then formed themselves into societies for the
discussion of scientific matters. This naturally led to the establishment of
publications whereby the papers presented to the societies could be
published and made available to the advancement of science generally. The
most influential of these was the Journal of the Philadelphia Academy of
Page 419
Natural Science, which was established in 1817, and was devoted largely to
zoological papers. The Annals of the New York Lyceum of Natural History
date from 1823, and the Journal of the Boston Society of Natural History
from 1834. The Transactions of the American Philosophical Society in
Philadelphia and the Memoirs of the American Academy of Arts and
Sciences in Boston also published many zoological articles.
In these publications and in the Journal, which was founded in 1818,
appear the descriptions of newly discovered animal species, with
observations on their habits.
The number of investigators in this field in the first quarter of the
nineteenth century was but few, and most of these were compelled to take
for the work such time as they could spare from their various occupations.
Gradually the workers became more numerous until about the middle of
the century zoology was taught in all the larger colleges. The science
thereby developed into a profession.
For some years the studies remained largely of a systematic nature, and
embraced all groups of animals, but long before the close of the century the
attention of the majority of the ever increasing group of zoologists was
directed into more promising channels for research and there came the
development of the sciences of comparative anatomy, physiology,
embryology, experimental zoology, cytology, genetics, and the like, while
the systematists became specialists in the various animal groups.
But the work in systematic zoology remains incomplete and many native
species are still undescribed or imperfectly classified. It is perhaps fortunate
that a few faithful systematists remain at their tasks and tend to keep the
experimentalists from the disaster which might otherwise result from the
confusion of the species under investigation.
zoological papers. The Annals of the New York Lyceum of Natural History
date from 1823, and the Journal of the Boston Society of Natural History
from 1834. The Transactions of the American Philosophical Society in
Philadelphia and the Memoirs of the American Academy of Arts and
Sciences in Boston also published many zoological articles.
In these publications and in the Journal, which was founded in 1818,
appear the descriptions of newly discovered animal species, with
observations on their habits.
The number of investigators in this field in the first quarter of the
nineteenth century was but few, and most of these were compelled to take
for the work such time as they could spare from their various occupations.
Gradually the workers became more numerous until about the middle of
the century zoology was taught in all the larger colleges. The science
thereby developed into a profession.
For some years the studies remained largely of a systematic nature, and
embraced all groups of animals, but long before the close of the century the
attention of the majority of the ever increasing group of zoologists was
directed into more promising channels for research and there came the
development of the sciences of comparative anatomy, physiology,
embryology, experimental zoology, cytology, genetics, and the like, while
the systematists became specialists in the various animal groups.
But the work in systematic zoology remains incomplete and many native
species are still undescribed or imperfectly classified. It is perhaps fortunate
that a few faithful systematists remain at their tasks and tend to keep the
experimentalists from the disaster which might otherwise result from the
confusion of the species under investigation.
Page 420
Period of Descriptive Natural History.—Previous to 1847.
Of the few American naturalists whose writings were published toward
the end of the eighteenth century and at the beginning of the nineteenth the
names of William Bartram (1739–1823), Benjamin Barton (1766–1815),
Samuel Mitchill (1764–1831), William Peck (1763–1822), and Thomas
Jefferson (1743–1826), require special mention. Bartram’s entertaining
volume describing his travels through the Carolinas, Georgia and Florida,
published in 1793, contains a most interesting account of the birds and other
animals which he found.
Barton wrote many charming essays on the natural history of animals,
but was more particularly interested in botany. Mitchill’s most important
works include a history of the fishes of New York (1814), and additions to
an edition of Bewick’s General History of Quadrupeds. The latter,
published in 1804, contains descriptions and figures of some American
species and is the first American work on mammals.
Peck has the distinction of writing the first paper on systematic zoology
published in America. This was a description of new species of fishes and
was printed in 1794. He is also well known for his work on insects and
fungi.
Jefferson in 1781 published an interesting book describing the natural
history of Virginia, and during his presidency was of inestimable service to
zoology through his support of scientific expeditions to the western portions
of the country.
Previous to Agassiz’s introduction of laboratory methods of study in
comparative anatomy and embryology in 1847, American naturalists
generally confined their attention to the study of the classification and
habits of the multitude of undescribed animals and plants of the region.
Such studies were naturally begun on the larger and more generally
interesting animals such as the birds and mammals, and although many of
these were fairly well described as to species before the opening of the
nineteenth century, little was known of their habits. The natural history of
our eastern birds first became well known through the accurate illustrations
and exquisitely written descriptions of Alexander Wilson (in 1808–1813).
Of the few American naturalists whose writings were published toward
the end of the eighteenth century and at the beginning of the nineteenth the
names of William Bartram (1739–1823), Benjamin Barton (1766–1815),
Samuel Mitchill (1764–1831), William Peck (1763–1822), and Thomas
Jefferson (1743–1826), require special mention. Bartram’s entertaining
volume describing his travels through the Carolinas, Georgia and Florida,
published in 1793, contains a most interesting account of the birds and other
animals which he found.
Barton wrote many charming essays on the natural history of animals,
but was more particularly interested in botany. Mitchill’s most important
works include a history of the fishes of New York (1814), and additions to
an edition of Bewick’s General History of Quadrupeds. The latter,
published in 1804, contains descriptions and figures of some American
species and is the first American work on mammals.
Peck has the distinction of writing the first paper on systematic zoology
published in America. This was a description of new species of fishes and
was printed in 1794. He is also well known for his work on insects and
fungi.
Jefferson in 1781 published an interesting book describing the natural
history of Virginia, and during his presidency was of inestimable service to
zoology through his support of scientific expeditions to the western portions
of the country.
Previous to Agassiz’s introduction of laboratory methods of study in
comparative anatomy and embryology in 1847, American naturalists
generally confined their attention to the study of the classification and
habits of the multitude of undescribed animals and plants of the region.
Such studies were naturally begun on the larger and more generally
interesting animals such as the birds and mammals, and although many of
these were fairly well described as to species before the opening of the
nineteenth century, little was known of their habits. The natural history of
our eastern birds first became well known through the accurate illustrations
and exquisitely written descriptions of Alexander Wilson (in 1808–1813).
Page 421
Bonaparte’s continuation of Wilson’s work was published in four folio
volumes beginning in 1826.
In 1828 appeared the first of Audubon’s magnificent folio illustrations of
our birds. These were published in England, with later editions of smaller
plates in America. Nuttall’s Manual of the Ornithology of the United States
appeared in 1832–1834.
The second work on American mammals appeared in the second
American edition of Guthrie’s Geography, published in 1815. The author is
supposed to have been George Ord, although his name does not appear. In
1825 Harlan published his “Fauna Americana: Descriptions of the
Mammiferous Animals inhabiting North America.” This was largely a
compilation from European writers, particularly from Demarest’s
Mammalogie, and had little value.
In 1826 Amos Eaton published a small “Zoological Text-book
comprising Cuvier’s four grand divisions of Animals: also Shaw’s improved
Linnean genera, arranged according to the classes and orders of Cuvier and
Latreille. Short descriptions of some of the most common species are given
for students’ exercises. Prepared for Rensselaer school and the popular class
room.” “Four hundred and sixty-one genera are described in this text-book.
They embrace every known species of the Animal Kingdom.” This is a
compilation from European sources with a few American species of various
groups included. On the other hand, Godman’s Natural History, in three
volumes (1826–1828), was an illustrated and creditable work. Such was
also the case with Sir John Richardson’s Fauna Boreali Americana of which
the volume on quadrupeds was published in England in 1829. The other
volumes on birds, fishes and insects appeared between 1827 and 1836.
Audubon and Bachman’s beautifully illustrated “Quadrupeds of North
America” was issued between 1841 and 1850.
About 1840 several of the states inaugurated natural history surveys and
published catalogues of the local faunas. The reports on the animals of
Massachusetts and New York are the most complete zoological monographs
published in America up to that time. This is particularly true of DeKay’s
Natural History of New York published between 1842 and 1844 in
beautifully illustrated quarto volumes.
The leader in the systematic studies in the early part of the century was
Thomas Say, who published descriptions of a large number of new species
volumes beginning in 1826.
In 1828 appeared the first of Audubon’s magnificent folio illustrations of
our birds. These were published in England, with later editions of smaller
plates in America. Nuttall’s Manual of the Ornithology of the United States
appeared in 1832–1834.
The second work on American mammals appeared in the second
American edition of Guthrie’s Geography, published in 1815. The author is
supposed to have been George Ord, although his name does not appear. In
1825 Harlan published his “Fauna Americana: Descriptions of the
Mammiferous Animals inhabiting North America.” This was largely a
compilation from European writers, particularly from Demarest’s
Mammalogie, and had little value.
In 1826 Amos Eaton published a small “Zoological Text-book
comprising Cuvier’s four grand divisions of Animals: also Shaw’s improved
Linnean genera, arranged according to the classes and orders of Cuvier and
Latreille. Short descriptions of some of the most common species are given
for students’ exercises. Prepared for Rensselaer school and the popular class
room.” “Four hundred and sixty-one genera are described in this text-book.
They embrace every known species of the Animal Kingdom.” This is a
compilation from European sources with a few American species of various
groups included. On the other hand, Godman’s Natural History, in three
volumes (1826–1828), was an illustrated and creditable work. Such was
also the case with Sir John Richardson’s Fauna Boreali Americana of which
the volume on quadrupeds was published in England in 1829. The other
volumes on birds, fishes and insects appeared between 1827 and 1836.
Audubon and Bachman’s beautifully illustrated “Quadrupeds of North
America” was issued between 1841 and 1850.
About 1840 several of the states inaugurated natural history surveys and
published catalogues of the local faunas. The reports on the animals of
Massachusetts and New York are the most complete zoological monographs
published in America up to that time. This is particularly true of DeKay’s
Natural History of New York published between 1842 and 1844 in
beautifully illustrated quarto volumes.
The leader in the systematic studies in the early part of the century was
Thomas Say, who published descriptions of a large number of new species
Page 422
of animals, particularly reptiles, mollusks, crustacea and insects. Say’s
conchology, printed in 1816 in Nicholson’s Cyclopedia, is the first
American work of its kind. This was reprinted in 1819 under the title “Land
and Fresh-water Shells of the United States.” In 1824–1828 appeared the
three volumes of Say’s American Entomology.
The prominent position held by Say in the zoological work of this period
is illustrated by the following paragraph from Eaton’s Zoological Text-book
(1826, p. 133): “At present but a small proportion of American Animals,
excepting those of large size, have been sought out ... And though Mr. Say
is doing much; without assistance, his life must be protracted to a very
advanced period to afford him time to complete the work. But if every
student will contribute his mite, by sending Mr. Say duplicates of all
undescribed species, we shall probably be in possession of a system, very
nearly complete, in a few years.” How different is the attitude of the
zoologist of to-day who sees the goal much further away after a century’s
progress through the industry of hundreds of investigators.
During the period of Say’s most active work he is reported to have “slept
in the hall of the Philadelphia Academy of Natural Sciences, where he made
his bed beneath the skeleton of a horse and fed himself on bread and milk.”
Next to Say, the most active zoologist of the early part of the century was
Charles Alexander Lesueur, who described and beautifully illustrated many
new species of fishes, reptiles, and marine invertebrates. A memoir by
George Ord, published in this Journal (8, 189, 1849), gives a full list of
Lesueur’s papers.
One of the most prolific writers of the period was Constantine
Rafinesque, a man of great brilliancy but one whose imagination so often
dominated his observations that many of his descriptions of plants and
animals are wholly unreliable.
United States Exploring Expedition.—In 1838 a fortunate circumstance
occurred which eventually brought American systematic zoology into the
front ranks of the science. This opportunity was offered by the United
States Exploring Expedition under the command of Admiral Wilkes. With
James D. Dana as naturalist, the expedition visited Madeira, Cape Verde
Islands, eastern and western coasts of South America, Polynesia, Samoa,
Australia, New Zealand, Fiji, Hawaiian Islands, west coast of United States,
Philippines, Singapore, Cape of Good Hope, etc.
conchology, printed in 1816 in Nicholson’s Cyclopedia, is the first
American work of its kind. This was reprinted in 1819 under the title “Land
and Fresh-water Shells of the United States.” In 1824–1828 appeared the
three volumes of Say’s American Entomology.
The prominent position held by Say in the zoological work of this period
is illustrated by the following paragraph from Eaton’s Zoological Text-book
(1826, p. 133): “At present but a small proportion of American Animals,
excepting those of large size, have been sought out ... And though Mr. Say
is doing much; without assistance, his life must be protracted to a very
advanced period to afford him time to complete the work. But if every
student will contribute his mite, by sending Mr. Say duplicates of all
undescribed species, we shall probably be in possession of a system, very
nearly complete, in a few years.” How different is the attitude of the
zoologist of to-day who sees the goal much further away after a century’s
progress through the industry of hundreds of investigators.
During the period of Say’s most active work he is reported to have “slept
in the hall of the Philadelphia Academy of Natural Sciences, where he made
his bed beneath the skeleton of a horse and fed himself on bread and milk.”
Next to Say, the most active zoologist of the early part of the century was
Charles Alexander Lesueur, who described and beautifully illustrated many
new species of fishes, reptiles, and marine invertebrates. A memoir by
George Ord, published in this Journal (8, 189, 1849), gives a full list of
Lesueur’s papers.
One of the most prolific writers of the period was Constantine
Rafinesque, a man of great brilliancy but one whose imagination so often
dominated his observations that many of his descriptions of plants and
animals are wholly unreliable.
United States Exploring Expedition.—In 1838 a fortunate circumstance
occurred which eventually brought American systematic zoology into the
front ranks of the science. This opportunity was offered by the United
States Exploring Expedition under the command of Admiral Wilkes. With
James D. Dana as naturalist, the expedition visited Madeira, Cape Verde
Islands, eastern and western coasts of South America, Polynesia, Samoa,
Australia, New Zealand, Fiji, Hawaiian Islands, west coast of United States,
Philippines, Singapore, Cape of Good Hope, etc.
Page 423
Of the extensive collections made on this four-years’ cruise, Dana had
devoted particular attention to the study of the corals and allied animals
(Zoophytes) and to the crustacea. In 1846 the report on the Zoophytes was
published in elegant folio form with colored plates. Six years later the first
volume of the report on Crustacea appeared, with a second volume after
two additional years (1854). These reports describe and beautifully illustrate
hundreds of new species, and include the first comprehensive studies of the
animals forming well-known corals. They remain as the most conspicuous
monuments in American invertebrate zoology. Unfortunately the very
limited edition makes them accessible in only a few large libraries. The
other, equally magnificent, volumes include: Mollusca and Shells, by A. A.
Gould, 1856; Herpetology, by Charles Girard, 1858; Mammalogy and
Ornithology, by John Cassin, 1858.
Principal investigators.—Of the many writers on animals at this period
of descriptive natural history, the following were prominent in their special
fields of study:
Ayres, Lesueur, Mitchill, Storer, Linsley, Wyman, DeKay, Smith,
Kirtland, Rafinesque and Haldeman described the fishes.
Green, Barton, Harlan, Le Conte, Say, and especially Holbrook, studied
the reptiles and amphibia. Holbrook’s great monograph of the reptiles
(North American Herpetology) was published between 1834 and 1845.
Wilson, Audubon, Nuttall, Cooper, DeKay, Brewer, Ord, Baird, Gould,
Bachman, Linsley and Fox were among the numerous writers on birds.
Godman, Ord, Richardson, Audubon, Bachman, DeKay, Linsley and
Harlan published accounts of mammals.
On the invertebrates an important general work entitled “Invertebrata of
Massachusetts; Mollusca, Crustacea, Annelida and Radiata” was published
by A. A. Gould in 1841, which contains all the New England species of
these groups known to that date.
Lea, Totten, Adams, Barnes, Gould, Binney, Conrad, Hildreth, Haldeman,
were the principal writers on mollusks. The crustacea were studied by Say,
Gould, Haldeman, Dana; the insects by Say, Melsheimer, Peck, Harris,
Kirby, Herrick; the spiders by Hentz; the worms by Lee; the coelenterates
and echinoderms by Say, Mantell and others.
devoted particular attention to the study of the corals and allied animals
(Zoophytes) and to the crustacea. In 1846 the report on the Zoophytes was
published in elegant folio form with colored plates. Six years later the first
volume of the report on Crustacea appeared, with a second volume after
two additional years (1854). These reports describe and beautifully illustrate
hundreds of new species, and include the first comprehensive studies of the
animals forming well-known corals. They remain as the most conspicuous
monuments in American invertebrate zoology. Unfortunately the very
limited edition makes them accessible in only a few large libraries. The
other, equally magnificent, volumes include: Mollusca and Shells, by A. A.
Gould, 1856; Herpetology, by Charles Girard, 1858; Mammalogy and
Ornithology, by John Cassin, 1858.
Principal investigators.—Of the many writers on animals at this period
of descriptive natural history, the following were prominent in their special
fields of study:
Ayres, Lesueur, Mitchill, Storer, Linsley, Wyman, DeKay, Smith,
Kirtland, Rafinesque and Haldeman described the fishes.
Green, Barton, Harlan, Le Conte, Say, and especially Holbrook, studied
the reptiles and amphibia. Holbrook’s great monograph of the reptiles
(North American Herpetology) was published between 1834 and 1845.
Wilson, Audubon, Nuttall, Cooper, DeKay, Brewer, Ord, Baird, Gould,
Bachman, Linsley and Fox were among the numerous writers on birds.
Godman, Ord, Richardson, Audubon, Bachman, DeKay, Linsley and
Harlan published accounts of mammals.
On the invertebrates an important general work entitled “Invertebrata of
Massachusetts; Mollusca, Crustacea, Annelida and Radiata” was published
by A. A. Gould in 1841, which contains all the New England species of
these groups known to that date.
Lea, Totten, Adams, Barnes, Gould, Binney, Conrad, Hildreth, Haldeman,
were the principal writers on mollusks. The crustacea were studied by Say,
Gould, Haldeman, Dana; the insects by Say, Melsheimer, Peck, Harris,
Kirby, Herrick; the spiders by Hentz; the worms by Lee; the coelenterates
and echinoderms by Say, Mantell and others.
Page 424
The history of entomology in the United States previous to 1846 is given
by John G. Morris in the Journal (1, 17, 1846). In this article F. V.
Melsheimer is stated to be the father of American Entomology, while Say
was the most prolific writer. Say’s entomological papers, edited by J. L. Le
Conte, were completely reprinted with their colored illustrations in 1859.
The first economic treatise is that by Harris on Insects Injurious to
Vegetation; printed in 1841. This has had many editions.
by John G. Morris in the Journal (1, 17, 1846). In this article F. V.
Melsheimer is stated to be the father of American Entomology, while Say
was the most prolific writer. Say’s entomological papers, edited by J. L. Le
Conte, were completely reprinted with their colored illustrations in 1859.
The first economic treatise is that by Harris on Insects Injurious to
Vegetation; printed in 1841. This has had many editions.
Page 425
Zoology in the American Journal of Science, 1818–1846.
The establishment of the Journal gave a further impetus to the scientific
activities of Americans in furnishing a convenient means for publishing the
results of their work. In the first volume of the Journal, for example, are two
zoological articles by Say and a dozen short articles on various topics by
Rafinesque, the latter being curious combinations of facts and fancy. Most
of the zoological papers appearing in its first series of 50 volumes are
characteristic of an undeveloped science in an undeveloped country. They
deal, naturally, with observational studies on the structure and classification
of species discovered in a virgin field, with notes on habits and life
histories.
Many of the papers are purely systematic and include the first
descriptions of numerous species of our mollusks, crustacea, insects,
vertebrates and other groups. Of these, the writings of C. B. Adams, Barnes,
A. A. Gould and Totten on mollusks, of J. D. Dana on corals and crustacea,
of Harris on insects, of Harlan on reptiles, and of Jeffries Wyman and D.
Humphreys Storer on fishes are representative and important.
The progress of zoology in America during the first twenty-eight years of
the Journal’s existence, that is, up to the year 1846, is thus summarized by
Professor Silliman in the preface to vol. 50 (page ix), 1847:
“Our zoology has been more fully investigated than our mineralogy and botany; but neither
department is in danger of being exhausted. The interesting travels of Lewis and Clark have recently
brought to our knowledge several plants and animals before unknown. Foreign naturalists are
frequently visiting our territory; and, for the most part, convey to Europe the fruits of their
researches, while but a small part of our own is examined and described by Americans: certainly this
is little to our credit and still less to our advantage. Honorable exceptions to the truth of this remark
are furnished by the exertions of some gentlemen in our principal cities, and in various other parts of
the Union.”
During these 28 years the Journal had been of great service to zoology
not only in the publication of the results of investigations but also in the
review of important zoological publications in Europe as well as in
America. There were also the reports of meetings of scientific societies. In
The establishment of the Journal gave a further impetus to the scientific
activities of Americans in furnishing a convenient means for publishing the
results of their work. In the first volume of the Journal, for example, are two
zoological articles by Say and a dozen short articles on various topics by
Rafinesque, the latter being curious combinations of facts and fancy. Most
of the zoological papers appearing in its first series of 50 volumes are
characteristic of an undeveloped science in an undeveloped country. They
deal, naturally, with observational studies on the structure and classification
of species discovered in a virgin field, with notes on habits and life
histories.
Many of the papers are purely systematic and include the first
descriptions of numerous species of our mollusks, crustacea, insects,
vertebrates and other groups. Of these, the writings of C. B. Adams, Barnes,
A. A. Gould and Totten on mollusks, of J. D. Dana on corals and crustacea,
of Harris on insects, of Harlan on reptiles, and of Jeffries Wyman and D.
Humphreys Storer on fishes are representative and important.
The progress of zoology in America during the first twenty-eight years of
the Journal’s existence, that is, up to the year 1846, is thus summarized by
Professor Silliman in the preface to vol. 50 (page ix), 1847:
“Our zoology has been more fully investigated than our mineralogy and botany; but neither
department is in danger of being exhausted. The interesting travels of Lewis and Clark have recently
brought to our knowledge several plants and animals before unknown. Foreign naturalists are
frequently visiting our territory; and, for the most part, convey to Europe the fruits of their
researches, while but a small part of our own is examined and described by Americans: certainly this
is little to our credit and still less to our advantage. Honorable exceptions to the truth of this remark
are furnished by the exertions of some gentlemen in our principal cities, and in various other parts of
the Union.”
During these 28 years the Journal had been of great service to zoology
not only in the publication of the results of investigations but also in the
review of important zoological publications in Europe as well as in
America. There were also the reports of meetings of scientific societies. In
Page 426
fact all matters of zoological interest were brought to the attention of the
Journal’s readers.
Journal’s readers.
Page 427
The Influence of Louis Agassiz.
At the time of the founding of the Journal and for nearly thirty years
thereafter descriptive natural history constituted practically the entire work
of American zoologists. In this respect American science was far behind
that in Europe and particularly in France. It was not until the fortunate
circumstances which brought the Swiss naturalist, Louis Agassiz, to our
country in 1846 that the modern conceptions of biological science were
established in America.
Agassiz was then 39 years of age and had already absorbed the spirit of
generalization in comparative anatomy which dominated the work of the
great leaders in Europe, and particularly in Paris. The influence of Leuckart,
Tiedemann, Braun, Cuvier and Von Humboldt directed Agassiz’s great
ability to similar investigations, and he was rapidly coming into prominence
in the study of modern and fossil fishes when the opportunity to continue
his research in America was presented. On arriving on our shores the young
zoologist was so inspired with the opportunities for his studies in the new
country that he decided to remain.
Bringing with him the broad conceptions of his distinguished European
masters, he naturally founded a similar school of zoology in America. It is
from this beginning that the present science of zoology with its many
branches has developed.
It must be remembered in this connection that the great service which
Agassiz rendered to American zoology consisted mainly in making
available to students in America the ideals and methods of European
zoologists. This he was eminently fitted to do both because of his European
training and because of his natural ability as an inspiring leader.
The times in America, moreover, were fully ripe for the advent of
European culture. There were already in existence natural history societies
in many of our cities and college communities. These societies not only
held meetings for the discussion of biological topics, but established
museums open to the public, and to which the public was invited to
contribute both funds and specimens. This led to a wide popular interest in
At the time of the founding of the Journal and for nearly thirty years
thereafter descriptive natural history constituted practically the entire work
of American zoologists. In this respect American science was far behind
that in Europe and particularly in France. It was not until the fortunate
circumstances which brought the Swiss naturalist, Louis Agassiz, to our
country in 1846 that the modern conceptions of biological science were
established in America.
Agassiz was then 39 years of age and had already absorbed the spirit of
generalization in comparative anatomy which dominated the work of the
great leaders in Europe, and particularly in Paris. The influence of Leuckart,
Tiedemann, Braun, Cuvier and Von Humboldt directed Agassiz’s great
ability to similar investigations, and he was rapidly coming into prominence
in the study of modern and fossil fishes when the opportunity to continue
his research in America was presented. On arriving on our shores the young
zoologist was so inspired with the opportunities for his studies in the new
country that he decided to remain.
Bringing with him the broad conceptions of his distinguished European
masters, he naturally founded a similar school of zoology in America. It is
from this beginning that the present science of zoology with its many
branches has developed.
It must be remembered in this connection that the great service which
Agassiz rendered to American zoology consisted mainly in making
available to students in America the ideals and methods of European
zoologists. This he was eminently fitted to do both because of his European
training and because of his natural ability as an inspiring leader.
The times in America, moreover, were fully ripe for the advent of
European culture. There were already in existence natural history societies
in many of our cities and college communities. These societies not only
held meetings for the discussion of biological topics, but established
museums open to the public, and to which the public was invited to
contribute both funds and specimens. This led to a wide popular interest in
Page 428
natural history. It was therefore comparatively easy for such a man as
Agassiz to develop this favorable public attitude into genuine enthusiasm.
The American Journal of Science announces the expected visit of Agassiz
as a most promising event for American Zoology (1, 451, 1846): “His
devotion, ability, and zeal—his high and deserved reputation and ... his
amiable and conciliating character, will, without doubt, secure for him the
cordial cooperation of our naturalists ... nor do we entertain a doubt that we
shall be liberally repaid by his able review and exploration of our country.”
We of to-day can realize how abundantly this prophecy was fulfilled.
In the succeeding volume (2, 440, 1846) occurs the record of Agassiz’s
arrival. “We learn with pleasure that he will spend several years among us,
in order thoroughly to understand our natural history.”
Immediately on reaching Boston, Agassiz began the publication of
articles on our fauna, and the following year he was appointed to a
professorship at Harvard. The Journal says (4, 449, 1847): “Every scientific
man in America will be rejoiced to hear so unexpected a piece of good
news.” The next year the Journal (5, 139, 1848) records Agassiz’s lecture
courses at New York and Charleston, his popularity with all classes of the
people and the gift of a silver case containing $250 in half eagles from the
students of the College of Physicians and Surgeons.
The service of Agassiz to American zoology, therefore, consisted not
only in the publication of the results of his researches and his philosophical
considerations therefrom, but also, and perhaps in even greater degree, in
the popularization of science. In the latter direction were his inspiring
lectures before popular audiences and the early publication of a zoological
text-book. This book, published in 1848, was entitled “Principles of
Zoology, touching the Structure, Development, Distribution and Natural
arrangement of the races of Animals, living and extinct, with numerous
illustrations.” It was written with the cooperation of Augustus A. Gould.
The review of this book in the Journal (6, 151, 1848) indicates clearly the
broad modern principles underlying the new era which was beginning for
American zoology.
“A work emanating from so high a source as the Principles of Zoology, hardly requires
commendation to give it currency. The public have become acquainted with the eminent abilities of
Prof. Agassiz through his lectures, and are aware of his vast learning, wide reach of mind, and
popular mode of illustrating scientific subjects ... The volume is prepared for the student in
Agassiz to develop this favorable public attitude into genuine enthusiasm.
The American Journal of Science announces the expected visit of Agassiz
as a most promising event for American Zoology (1, 451, 1846): “His
devotion, ability, and zeal—his high and deserved reputation and ... his
amiable and conciliating character, will, without doubt, secure for him the
cordial cooperation of our naturalists ... nor do we entertain a doubt that we
shall be liberally repaid by his able review and exploration of our country.”
We of to-day can realize how abundantly this prophecy was fulfilled.
In the succeeding volume (2, 440, 1846) occurs the record of Agassiz’s
arrival. “We learn with pleasure that he will spend several years among us,
in order thoroughly to understand our natural history.”
Immediately on reaching Boston, Agassiz began the publication of
articles on our fauna, and the following year he was appointed to a
professorship at Harvard. The Journal says (4, 449, 1847): “Every scientific
man in America will be rejoiced to hear so unexpected a piece of good
news.” The next year the Journal (5, 139, 1848) records Agassiz’s lecture
courses at New York and Charleston, his popularity with all classes of the
people and the gift of a silver case containing $250 in half eagles from the
students of the College of Physicians and Surgeons.
The service of Agassiz to American zoology, therefore, consisted not
only in the publication of the results of his researches and his philosophical
considerations therefrom, but also, and perhaps in even greater degree, in
the popularization of science. In the latter direction were his inspiring
lectures before popular audiences and the early publication of a zoological
text-book. This book, published in 1848, was entitled “Principles of
Zoology, touching the Structure, Development, Distribution and Natural
arrangement of the races of Animals, living and extinct, with numerous
illustrations.” It was written with the cooperation of Augustus A. Gould.
The review of this book in the Journal (6, 151, 1848) indicates clearly the
broad modern principles underlying the new era which was beginning for
American zoology.
“A work emanating from so high a source as the Principles of Zoology, hardly requires
commendation to give it currency. The public have become acquainted with the eminent abilities of
Prof. Agassiz through his lectures, and are aware of his vast learning, wide reach of mind, and
popular mode of illustrating scientific subjects ... The volume is prepared for the student in
Page 429
zoological science; it is simple and elementary in style, full in its illustrations, comprehensive in its
range, yet well considered and brought into the narrow compass requisite for the purpose intended.”
The titles of its chapters will show how little it differs in general subject
matter from the most recent text-book in biology. Chapter I, The Sphere and
fundamental principles of Zoology; II, General Properties of Organized
Bodies; III, Organs and Functions of Animal Life; IV, Of Intelligence and
Instinct; V, Of Motion (apparatus and modes); VI, Of Nutrition; VII, Of the
Blood and Circulation; VIII, Of Respiration; IX, Of the Secretions; X,
Embryology (Egg and its Development); XI, Peculiar Modes of
Reproduction; XII, Metamorphoses of Animals; XIII, Geographical
Distribution of Animals; XIV, Geological Succession of Animals, or their
Distribution in Time.
A moment’s consideration of the fact that all these topics are excellently
treated will show how great had been the progress of zoology in the first
half of the nineteenth century. The sixty years that have elapsed since the
publication of this book have served principally to develop these separate
lines of biology into special fields of science without reorganization of the
essential principles here recognized. This remained for many years the
standard zoological and physiological text-book, and was republished in
several editions here and in England. Another popular book is entitled
“Methods of Study in Natural History” (1864).
More than 400 books and papers were written by Agassiz, over a third of
which were published before he came to America. They cover both
zoological and geological topics, including systematic papers on living and
fossil groups of animals, but most important of all are his philosophical
essays on the general principles of biology.
One of Agassiz’s greatest services to zoology was the publication of his
“Bibliographia Zoologiæ et Geologiæ” by the Ray Society, beginning with
1848. The publication of the Lowell lectures in Comparative Embryology in
1849 gave wide audience to the general principles now recognized in the
biogenetic law of ancestral reminiscence. As stated in the Journal (8, 157,
1849), the “object of the Lectures is to demonstrate that a natural method of
classifying the animal kingdom may be attained by a comparison of the
changes which are passed through by different animals in the course of their
development from the egg to the perfect state; the change they undergo
range, yet well considered and brought into the narrow compass requisite for the purpose intended.”
The titles of its chapters will show how little it differs in general subject
matter from the most recent text-book in biology. Chapter I, The Sphere and
fundamental principles of Zoology; II, General Properties of Organized
Bodies; III, Organs and Functions of Animal Life; IV, Of Intelligence and
Instinct; V, Of Motion (apparatus and modes); VI, Of Nutrition; VII, Of the
Blood and Circulation; VIII, Of Respiration; IX, Of the Secretions; X,
Embryology (Egg and its Development); XI, Peculiar Modes of
Reproduction; XII, Metamorphoses of Animals; XIII, Geographical
Distribution of Animals; XIV, Geological Succession of Animals, or their
Distribution in Time.
A moment’s consideration of the fact that all these topics are excellently
treated will show how great had been the progress of zoology in the first
half of the nineteenth century. The sixty years that have elapsed since the
publication of this book have served principally to develop these separate
lines of biology into special fields of science without reorganization of the
essential principles here recognized. This remained for many years the
standard zoological and physiological text-book, and was republished in
several editions here and in England. Another popular book is entitled
“Methods of Study in Natural History” (1864).
More than 400 books and papers were written by Agassiz, over a third of
which were published before he came to America. They cover both
zoological and geological topics, including systematic papers on living and
fossil groups of animals, but most important of all are his philosophical
essays on the general principles of biology.
One of Agassiz’s greatest services to zoology was the publication of his
“Bibliographia Zoologiæ et Geologiæ” by the Ray Society, beginning with
1848. The publication of the Lowell lectures in Comparative Embryology in
1849 gave wide audience to the general principles now recognized in the
biogenetic law of ancestral reminiscence. As stated in the Journal (8, 157,
1849), the “object of the Lectures is to demonstrate that a natural method of
classifying the animal kingdom may be attained by a comparison of the
changes which are passed through by different animals in the course of their
development from the egg to the perfect state; the change they undergo
Page 430
being considered as a scale to appreciate the relative position of the
species.” These “principles of classification” are fully elucidated in a
separate pamphlet, and are discussed at length in the Journal (11, 122,
1851).
One of the most interesting of Agassiz’s numerous philosophical essays,
originally contributed to the Journal (9, 369, 1850), discusses the “Natural
Relations between Animals and the elements in which they live.” Another
philosophical paper contributed to the Journal discusses the “Primitive
diversity and number of Animals in Geological times” (17, 309, 1854). Of
his systematic papers, those on the fishes of the Tennessee river, describing
many new species, were published in the Journal (17, 297, 353, 1854).
species.” These “principles of classification” are fully elucidated in a
separate pamphlet, and are discussed at length in the Journal (11, 122,
1851).
One of the most interesting of Agassiz’s numerous philosophical essays,
originally contributed to the Journal (9, 369, 1850), discusses the “Natural
Relations between Animals and the elements in which they live.” Another
philosophical paper contributed to the Journal discusses the “Primitive
diversity and number of Animals in Geological times” (17, 309, 1854). Of
his systematic papers, those on the fishes of the Tennessee river, describing
many new species, were published in the Journal (17, 297, 353, 1854).
Page 431
Agassiz’s beautifully illustrated “Contributions to the Natural History of
the United States” cover many subjects in morphology and embryology,
which are treated with such thoroughness and breadth of view as to give
them a place among the zoological classics. The Essay on Classification,
the North American Testudinata, the Embryology of the turtle, and the
Acalephs are the special topics. These are summarized and discussed at
length in the Journal (25, 126, 202, 321, 342, 1858; 30, 142, 1860; 31, 295,
1861).
the United States” cover many subjects in morphology and embryology,
which are treated with such thoroughness and breadth of view as to give
them a place among the zoological classics. The Essay on Classification,
the North American Testudinata, the Embryology of the turtle, and the
Acalephs are the special topics. These are summarized and discussed at
length in the Journal (25, 126, 202, 321, 342, 1858; 30, 142, 1860; 31, 295,
1861).
Page 432
The volume on the “Journey in Brazil” (1868) in joint authorship with
Mrs. Agassiz is a fascinating narrative of exploration.
The conceptions which Agassiz held as to the most essential aim of
zoological study are well illustrated in his autobiographical sketch, where
he writes:[174]
“I did not then know how much more important it is to the naturalist to understand the structure of
a few animals, than to command the whole field of scientific nomenclature. Since I have become a
teacher, and have watched the progress of students, I have seen that they all begin in the same way;
but how many have grown old in the pursuit, without ever rising to any higher conception of the
study of nature, spending their life in the determination of species, and in extending scientific
terminology!”
It is not surprising, then, that under such influence the older systematic
studies should be replaced in large measure by those of a morphological and
embryological nature.
The personal influence of Agassiz is still felt in the lives of even the
younger zoologists of the present day. For the investigators of the present
generation are for the most part indebted to one or another of Agassiz’s
pupils for their guidance in zoological studies. These pupils include his son
Alexander Agassiz, Allen, Brooks, Clarke, Fewkes, Goode, Hyatt, Jordan,
Lyman, Morse, Packard, Scudder, Verrill, Wilder, and others—leaders in
zoological work during the last third of the nineteenth century. Through
such men as these the inspiration of Agassiz has been handed on in turn to
their pupils and from them to the younger generation of zoologists.
The essential difference between the work of Agassiz and that of the
American zoologists who preceded him was in his power of broad
generalizations. To him the organism meant a living witness of some great
natural law, in the interpretation of which zoology was engaged. The
organism in its structure, in its development, in its habits furnished links in
the chain of evidence which, when completed, would reveal the meaning of
nature. Of all Agassiz’s pupils, probably William K. Brooks most fittingly
perpetuated his master’s ideals.
Mrs. Agassiz is a fascinating narrative of exploration.
The conceptions which Agassiz held as to the most essential aim of
zoological study are well illustrated in his autobiographical sketch, where
he writes:[174]
“I did not then know how much more important it is to the naturalist to understand the structure of
a few animals, than to command the whole field of scientific nomenclature. Since I have become a
teacher, and have watched the progress of students, I have seen that they all begin in the same way;
but how many have grown old in the pursuit, without ever rising to any higher conception of the
study of nature, spending their life in the determination of species, and in extending scientific
terminology!”
It is not surprising, then, that under such influence the older systematic
studies should be replaced in large measure by those of a morphological and
embryological nature.
The personal influence of Agassiz is still felt in the lives of even the
younger zoologists of the present day. For the investigators of the present
generation are for the most part indebted to one or another of Agassiz’s
pupils for their guidance in zoological studies. These pupils include his son
Alexander Agassiz, Allen, Brooks, Clarke, Fewkes, Goode, Hyatt, Jordan,
Lyman, Morse, Packard, Scudder, Verrill, Wilder, and others—leaders in
zoological work during the last third of the nineteenth century. Through
such men as these the inspiration of Agassiz has been handed on in turn to
their pupils and from them to the younger generation of zoologists.
The essential difference between the work of Agassiz and that of the
American zoologists who preceded him was in his power of broad
generalizations. To him the organism meant a living witness of some great
natural law, in the interpretation of which zoology was engaged. The
organism in its structure, in its development, in its habits furnished links in
the chain of evidence which, when completed, would reveal the meaning of
nature. Of all Agassiz’s pupils, probably William K. Brooks most fittingly
perpetuated his master’s ideals.
Page 433
Period of Morphology and Embryology, 1847–1870.
The new aspect of zoology which came as a result of the influence of
Agassiz characterized the zoological work of the fifties and sixties, that is,
until the significance of the natural selection theory of Darwin and Wallace
became generally appreciated.
The work in these years and well into the seventies was largely
influenced by the morphological, embryological and systematic studies of
Louis Agassiz and his school. The structure, development, and homologies
of animals as indicating their relationship and position in the scheme of
classification was prominent in the work of this period. The adaptations of
animals to their environment and the application of the biogenetic law to
the various groups of animals were also favorite subjects of study.
The most successful investigators in this period on the different groups of
animals include:—Louis Agassiz on the natural history and embryology of
coelenterates and turtles; A. Agassiz, embryology of echinoderms and
worms; H. J. Clark, embryology of turtles and systematic papers on sponges
and coelenterates; E. Desor, echinoderms and embryology of worms; C.
Girard, embryology, worms, and reptiles; J. Leidy, protozoa, coelenterates,
worms, anatomy of mollusks; W. O. Ayres and T. Lyman, natural history of
echinoderms; McCrady, development of acalephs; W. Stimpson, marine
invertebrates; A. E. Verrill, coelenterates, echinoderms, worms; A. Hyatt,
evolutionary theories, bryozoa and mollusks; Pourtales, deep sea fauna; C.
B. Adams, A. and W. G. Binney, Brooks, Carpenter, Conrad, Dall, Jay, Lea,
S. Smith, Tryon, mollusks; E. S. Morse, brachiopods, mollusks; J. D. Dana,
coelenterates and Crustacea; Kirtland, Loew, Edwards, Hagen, Melsheimer,
Packard, Riley, Scudder, Walsh, insects; Gill, Holbrook, Storer, fishes;
Cope, evolutionary theories, fishes and amphibia; Baird, reptiles and birds;
J. A. Allen, amphibia, reptiles and birds; Brewer, Cassin, Coues, Lawrence,
birds; Audubon, Bachman, Baird, Cope, Wilder, mammals.
The progress of ornithology in the United States previous to 1876 is well
described in a paper by J. A. Allen in the American Naturalist (10, 536,
1876). A sketch of the early history of conchology is given by A. W. Tryon
in the Journal (33, 13, 1862).
The new aspect of zoology which came as a result of the influence of
Agassiz characterized the zoological work of the fifties and sixties, that is,
until the significance of the natural selection theory of Darwin and Wallace
became generally appreciated.
The work in these years and well into the seventies was largely
influenced by the morphological, embryological and systematic studies of
Louis Agassiz and his school. The structure, development, and homologies
of animals as indicating their relationship and position in the scheme of
classification was prominent in the work of this period. The adaptations of
animals to their environment and the application of the biogenetic law to
the various groups of animals were also favorite subjects of study.
The most successful investigators in this period on the different groups of
animals include:—Louis Agassiz on the natural history and embryology of
coelenterates and turtles; A. Agassiz, embryology of echinoderms and
worms; H. J. Clark, embryology of turtles and systematic papers on sponges
and coelenterates; E. Desor, echinoderms and embryology of worms; C.
Girard, embryology, worms, and reptiles; J. Leidy, protozoa, coelenterates,
worms, anatomy of mollusks; W. O. Ayres and T. Lyman, natural history of
echinoderms; McCrady, development of acalephs; W. Stimpson, marine
invertebrates; A. E. Verrill, coelenterates, echinoderms, worms; A. Hyatt,
evolutionary theories, bryozoa and mollusks; Pourtales, deep sea fauna; C.
B. Adams, A. and W. G. Binney, Brooks, Carpenter, Conrad, Dall, Jay, Lea,
S. Smith, Tryon, mollusks; E. S. Morse, brachiopods, mollusks; J. D. Dana,
coelenterates and Crustacea; Kirtland, Loew, Edwards, Hagen, Melsheimer,
Packard, Riley, Scudder, Walsh, insects; Gill, Holbrook, Storer, fishes;
Cope, evolutionary theories, fishes and amphibia; Baird, reptiles and birds;
J. A. Allen, amphibia, reptiles and birds; Brewer, Cassin, Coues, Lawrence,
birds; Audubon, Bachman, Baird, Cope, Wilder, mammals.
The progress of ornithology in the United States previous to 1876 is well
described in a paper by J. A. Allen in the American Naturalist (10, 536,
1876). A sketch of the early history of conchology is given by A. W. Tryon
in the Journal (33, 13, 1862).
Page 434
Jeffries Wyman was the most prominent comparative anatomist of this
period. His work includes classic papers on the anatomy and embryology of
fishes, amphibia, and reptiles.
period. His work includes classic papers on the anatomy and embryology of
fishes, amphibia, and reptiles.
Page 435
Zoology in the American Journal of Science, 1846–1870.
The fifty volumes of the second series of the Journal, including the years
1846 to 1870, cover approximately this period of morphology and
embryology. During this period the Journal occupied a very important place
in zoological circles, for J. D. Dana was for most of this period the editor-
in-chief, while Louis Agassiz and Asa Gray were connected with it as
associate editors. Moreover, in 1864 one of the most promising of Agassiz’s
pupils, Addison E. Verrill, was called to Yale as professor of zoology and
was made an associate editor in 1869.
In the Journal, therefore, may be found, in its original articles, together
with its reports of meetings and addresses and its reviews of literature, a
fairly complete account of the zoological activity of the period. The most
important zoological researches, both in Europe and America, were
reviewed in the bibliographic notices.
The most important series of zoological articles are by Dana himself. As
his work on the zoophytes and crustacea of the U. S. Exploring Expedition
continued, he published from time to time general summaries of his
conclusions regarding the relationships of the various groups. Included
among these papers are philosophical essays on general biological
principles which must have had much influence on the biological studies of
the time, and which form a basis for many of our present concepts.
The importance of these papers warrants the list being given in full. The
titles are here in many cases abbreviated and the subjects consolidated.
General views on Classification, 1, 286, 1846.
Zoophytes, 2, 64, 187, 1846; 3, 1, 160, 337, 1847.
Genus Astraea, 9, 295, 1850.
Conspectus crustaceorum, 8, 276, 424, 1849; 9, 129, 1850; 11, 268, 1851.
Genera of Gammaracea, 8, 135, 1849; of Cyclopacea, 1, 225, 1846.
Markings of Carapax of Crabs, 11, 95, 1851.
Classification of Crustacea, 11, 223, 425; 12, 121, 238, 1851; 13, 119; 14, 297, 1852; 22, 14, 1856.
Geographical distribution of Crustacea, 18, 314, 1854; 19, 6; 20, 168, 349, 1855.
Alternation of Generations in Plants and Radiata, 10, 341, 1850.
Parthenogenesis, 24, 399, 1857.
The fifty volumes of the second series of the Journal, including the years
1846 to 1870, cover approximately this period of morphology and
embryology. During this period the Journal occupied a very important place
in zoological circles, for J. D. Dana was for most of this period the editor-
in-chief, while Louis Agassiz and Asa Gray were connected with it as
associate editors. Moreover, in 1864 one of the most promising of Agassiz’s
pupils, Addison E. Verrill, was called to Yale as professor of zoology and
was made an associate editor in 1869.
In the Journal, therefore, may be found, in its original articles, together
with its reports of meetings and addresses and its reviews of literature, a
fairly complete account of the zoological activity of the period. The most
important zoological researches, both in Europe and America, were
reviewed in the bibliographic notices.
The most important series of zoological articles are by Dana himself. As
his work on the zoophytes and crustacea of the U. S. Exploring Expedition
continued, he published from time to time general summaries of his
conclusions regarding the relationships of the various groups. Included
among these papers are philosophical essays on general biological
principles which must have had much influence on the biological studies of
the time, and which form a basis for many of our present concepts.
The importance of these papers warrants the list being given in full. The
titles are here in many cases abbreviated and the subjects consolidated.
General views on Classification, 1, 286, 1846.
Zoophytes, 2, 64, 187, 1846; 3, 1, 160, 337, 1847.
Genus Astraea, 9, 295, 1850.
Conspectus crustaceorum, 8, 276, 424, 1849; 9, 129, 1850; 11, 268, 1851.
Genera of Gammaracea, 8, 135, 1849; of Cyclopacea, 1, 225, 1846.
Markings of Carapax of Crabs, 11, 95, 1851.
Classification of Crustacea, 11, 223, 425; 12, 121, 238, 1851; 13, 119; 14, 297, 1852; 22, 14, 1856.
Geographical distribution of Crustacea, 18, 314, 1854; 19, 6; 20, 168, 349, 1855.
Alternation of Generations in Plants and Radiata, 10, 341, 1850.
Parthenogenesis, 24, 399, 1857.
Page 436
On Species, 24, 305, 1857.
Classification of Mammals, 35, 65, 1863; 37, 157, 1864.
Cephalization, 22, 14, 1856; 36, 1, 321, 440, 1863; 37, 10, 157, 184, 1864; 41, 163, 1866; 12, 245,
1876.
Homologies of insectean and crustacean types, 36, 233, 1863; 47, 325, 1894.
Origin of life, 41, 389, 1866.
Relations of death to life in nature, 34, 316, 1862.
Of the above, the articles on cephalization as a fundamental principle in
the development of the system of animal life have attracted much attention.
The evidence from comparative anatomy, paleontology, and embryology
alike supports the view that advance in the ontogenetic as well as in the
phylogenetic stages is correlated with the unequal growth of the cephalic
region as compared with the rest of the body. Dana shows that this principle
holds good for all groups of animals. His homologies of the limbs of
arthropods and vertebrates, however, do not accord with more modern
views.
Other papers on the same and allied topics were published by Dana in
other periodicals. His most conspicuous zoological works, however, are his
reports on the Zoophytes and Crustacea of the United States Exploring
Expedition, 1837–1842. The former consists of 741 quarto pages and 61
folio plates, describing over 200 new species, while the Crustacea report, in
two volumes, has 1620 pages and 96 folio plates, with descriptions of about
500 new species. Each of these remains to-day as the most important
contribution to the classification of the respective groups. The relationships
of the species, genera and families were recognized with such remarkable
judgment that Dana’s admirable system of classification has remained the
basis for all subsequent work.
Dana’s critical reviews (25, 202, 321, 1858) of Agassiz’s “Contribution to
the Natural History of the United States” are among the most interesting of
his philosophical discussions concerning the relationships of animals as
revealed by their structure, their embryology, and their geological history.
The remaining zoological articles in this series cover nearly the whole
range of systematic zoology. Especially important are the articles by Verrill
on coelenterates, echinoderms, worms and other invertebrates.
Classification of Mammals, 35, 65, 1863; 37, 157, 1864.
Cephalization, 22, 14, 1856; 36, 1, 321, 440, 1863; 37, 10, 157, 184, 1864; 41, 163, 1866; 12, 245,
1876.
Homologies of insectean and crustacean types, 36, 233, 1863; 47, 325, 1894.
Origin of life, 41, 389, 1866.
Relations of death to life in nature, 34, 316, 1862.
Of the above, the articles on cephalization as a fundamental principle in
the development of the system of animal life have attracted much attention.
The evidence from comparative anatomy, paleontology, and embryology
alike supports the view that advance in the ontogenetic as well as in the
phylogenetic stages is correlated with the unequal growth of the cephalic
region as compared with the rest of the body. Dana shows that this principle
holds good for all groups of animals. His homologies of the limbs of
arthropods and vertebrates, however, do not accord with more modern
views.
Other papers on the same and allied topics were published by Dana in
other periodicals. His most conspicuous zoological works, however, are his
reports on the Zoophytes and Crustacea of the United States Exploring
Expedition, 1837–1842. The former consists of 741 quarto pages and 61
folio plates, describing over 200 new species, while the Crustacea report, in
two volumes, has 1620 pages and 96 folio plates, with descriptions of about
500 new species. Each of these remains to-day as the most important
contribution to the classification of the respective groups. The relationships
of the species, genera and families were recognized with such remarkable
judgment that Dana’s admirable system of classification has remained the
basis for all subsequent work.
Dana’s critical reviews (25, 202, 321, 1858) of Agassiz’s “Contribution to
the Natural History of the United States” are among the most interesting of
his philosophical discussions concerning the relationships of animals as
revealed by their structure, their embryology, and their geological history.
The remaining zoological articles in this series cover nearly the whole
range of systematic zoology. Especially important are the articles by Verrill
on coelenterates, echinoderms, worms and other invertebrates.
Page 437
In the years following the publication of Darwin’s Origin of Species in
1859 occur many articles on the theory of natural selection. Some of the
writers attack the theory, while others give it more or less enthusiastic
support.
Experimental methods in solving biological problems were little used at
this time, although a few articles of this nature appear in the Journal. Of
these, a paper by W. C. Minor (35, 35, 1863) on natural and artificial fission
in some annelids has considerable interest to-day.
1859 occur many articles on the theory of natural selection. Some of the
writers attack the theory, while others give it more or less enthusiastic
support.
Experimental methods in solving biological problems were little used at
this time, although a few articles of this nature appear in the Journal. Of
these, a paper by W. C. Minor (35, 35, 1863) on natural and artificial fission
in some annelids has considerable interest to-day.
Page 438
Exploring Expeditions.
Of the important zoological expeditions the following may be selected as
showing their influence on American Zoology:
The North Pacific Expedition, with William Stimpson as zoologist,
returned in 1856 with much new information concerning the marine life of
the coasts of Alaska and Japan and many new species of invertebrates.
In 1867–1869 the United States Coast Survey extended its explorations
to include the deep sea marine life off the southeastern coasts and Gulf of
Mexico under the leadership of Pourtales and Agassiz.
The Challenger explorations (1872–1876) added greatly to the
knowledge of marine life off the American coast as well as in other parts of
the world.
The explorations of the United States Fish Commission succeeded those
of the Coast Survey in the collection of marine life off our coasts and in our
fresh waters. These have continued since 1872 and have yielded most
important results from both the scientific and economic standpoints.
Under the charge of Alexander Agassiz the Coast Survey Steamer
“Blake,” in 1877 to 1880, was engaged in dredging operations in three
cruises to various parts of the Atlantic. The U. S. Fish Commission Steamer
“Albatross,” also in charge of Agassiz, made three expeditions in the
tropical and other parts of the Pacific in the years from 1891 to 1905. The
study of these collections has added greatly to our knowledge of systematic
zoology and geographical distribution. The reports on some of the groups
are still in course of preparation.
Of the important zoological expeditions the following may be selected as
showing their influence on American Zoology:
The North Pacific Expedition, with William Stimpson as zoologist,
returned in 1856 with much new information concerning the marine life of
the coasts of Alaska and Japan and many new species of invertebrates.
In 1867–1869 the United States Coast Survey extended its explorations
to include the deep sea marine life off the southeastern coasts and Gulf of
Mexico under the leadership of Pourtales and Agassiz.
The Challenger explorations (1872–1876) added greatly to the
knowledge of marine life off the American coast as well as in other parts of
the world.
The explorations of the United States Fish Commission succeeded those
of the Coast Survey in the collection of marine life off our coasts and in our
fresh waters. These have continued since 1872 and have yielded most
important results from both the scientific and economic standpoints.
Under the charge of Alexander Agassiz the Coast Survey Steamer
“Blake,” in 1877 to 1880, was engaged in dredging operations in three
cruises to various parts of the Atlantic. The U. S. Fish Commission Steamer
“Albatross,” also in charge of Agassiz, made three expeditions in the
tropical and other parts of the Pacific in the years from 1891 to 1905. The
study of these collections has added greatly to our knowledge of systematic
zoology and geographical distribution. The reports on some of the groups
are still in course of preparation.
Page 439
Period of Evolution, 1870–1890.
The time from 1870 to 1890 may be appropriately called the period of
evolution, for although it commences eleven years after the publication of
the Origin of Species, the importance of the natural selection theory was but
slowly receiving general recognition. The hesitation in accepting this theory
was due in no small degree to the opposition of Louis Agassiz. After the
acceptance of evolution, although morphological and embryological studies
continued as before, they were prosecuted with reference to their bearing on
evolutionary problems.
Following closely the methods which had produced so much progress
during the life of Agassiz, the field of zoology was now occupied by a new
generation, among whom the pupils of Agassiz were the most prominent.
The time from 1870 to 1890 may be appropriately called the period of
evolution, for although it commences eleven years after the publication of
the Origin of Species, the importance of the natural selection theory was but
slowly receiving general recognition. The hesitation in accepting this theory
was due in no small degree to the opposition of Louis Agassiz. After the
acceptance of evolution, although morphological and embryological studies
continued as before, they were prosecuted with reference to their bearing on
evolutionary problems.
Following closely the methods which had produced so much progress
during the life of Agassiz, the field of zoology was now occupied by a new
generation, among whom the pupils of Agassiz were the most prominent.
Page 440
The teaching of biology at this time was also strongly influenced by
Huxley, whose methods of conducting laboratory classes for elementary
students were adopted in most of our large schools and colleges. This
placed biology on the same plane with chemistry as a means for training in
laboratory methods and discipline, with the added advantage that the
subject of biology is much more intimately connected with the student’s
everyday life and affairs.
Huxley, whose methods of conducting laboratory classes for elementary
students were adopted in most of our large schools and colleges. This
placed biology on the same plane with chemistry as a means for training in
laboratory methods and discipline, with the added advantage that the
subject of biology is much more intimately connected with the student’s
everyday life and affairs.
Page 441
This increasing demand for instruction in biology and the consequent
necessity for more teachers brought an increasing number of investigators
into this field.
Conspicuous in this period was the work of E. D. Cope, best known as a
paleontologist, but whose work on the classification of the various groups
of vertebrates stands preeminent, and whose philosophical essays on
evolution had much influence on the evolutionary thought of the time. He
was a staunch supporter of the Lamarckian doctrine. Alpheus Hyatt also
maintained this theory, and brought together a great accumulation of facts
in its support. He thereby contributed largely to our knowledge of
comparative anatomy and embryology. A. S. Packard, whose publications
cover a wide range of topics, was best known for his text-books of zoology
and his manuals on insects.
W. K. Brooks was a leading morphologist and embryologist. S. F. Baird,
for many years the head of the United States Fish Commission, was the
foremost authority on fish and fisheries and is also noted for his work on
reptiles, birds and mammals. The man of greatest influence, although by no
means the greatest investigator, was C. O. Whitman. It is to him that we
owe the inception of the Marine Biological Laboratory, the most potent
influence in American zoology to-day; the organization of the American
Morphological Society, the forerunner of the present American Society of
Zoologists; and the establishment of the Journal of Morphology. G. B.
Goode was distinguished for his work on fishes and for his writings on the
history of science.
E. L. Mark, C. S. Minot, and Alexander Agassiz were acknowledged
leaders in their special fields of research—Mark in invertebrate morphology
and embryology, and Minot in vertebrate embryology, while Alexander
Agassiz made many important discoveries in the systematic zoology and
embryology of marine animals, and to him we owe in large measure our
knowledge of the life in the oceans of nearly all parts of the world.
The knowledge of the representatives of the different divisions of the
American fauna had now become sufficient to allow the publication of
monographs on the various classes, orders and families. At this time also
particular attention was given to the marine invertebrates of all groups.
Of the many investigators working on the various groups of animals at
this time only a few may be mentioned. The protozoa were studied by
necessity for more teachers brought an increasing number of investigators
into this field.
Conspicuous in this period was the work of E. D. Cope, best known as a
paleontologist, but whose work on the classification of the various groups
of vertebrates stands preeminent, and whose philosophical essays on
evolution had much influence on the evolutionary thought of the time. He
was a staunch supporter of the Lamarckian doctrine. Alpheus Hyatt also
maintained this theory, and brought together a great accumulation of facts
in its support. He thereby contributed largely to our knowledge of
comparative anatomy and embryology. A. S. Packard, whose publications
cover a wide range of topics, was best known for his text-books of zoology
and his manuals on insects.
W. K. Brooks was a leading morphologist and embryologist. S. F. Baird,
for many years the head of the United States Fish Commission, was the
foremost authority on fish and fisheries and is also noted for his work on
reptiles, birds and mammals. The man of greatest influence, although by no
means the greatest investigator, was C. O. Whitman. It is to him that we
owe the inception of the Marine Biological Laboratory, the most potent
influence in American zoology to-day; the organization of the American
Morphological Society, the forerunner of the present American Society of
Zoologists; and the establishment of the Journal of Morphology. G. B.
Goode was distinguished for his work on fishes and for his writings on the
history of science.
E. L. Mark, C. S. Minot, and Alexander Agassiz were acknowledged
leaders in their special fields of research—Mark in invertebrate morphology
and embryology, and Minot in vertebrate embryology, while Alexander
Agassiz made many important discoveries in the systematic zoology and
embryology of marine animals, and to him we owe in large measure our
knowledge of the life in the oceans of nearly all parts of the world.
The knowledge of the representatives of the different divisions of the
American fauna had now become sufficient to allow the publication of
monographs on the various classes, orders and families. At this time also
particular attention was given to the marine invertebrates of all groups.
Of the many investigators working on the various groups of animals at
this time only a few may be mentioned. The protozoa were studied by
Page 442
Leidy, Clark, Ryder, Stokes; the sponges by Clark, Hyatt; the coelenterates
by A. Agassiz, S. F. Clarke, Verrill; the echinoderms by A. Agassiz, Brooks,
Kingsley, Fewkes, Lyman, Verrill; the various groups of worms by
Benedict, Eisen, Silliman, Verrill, Webster, Whitman; the mollusks by A.
and W. G. Binney, Tryon, Conrad, Dall, Sanderson Smith, Stearns, Verrill;
the Brachiopods by Dall and Morse; the Bryozoa by Hyatt; the crustacea by
S. I. Smith, Harger, Hagen, Packard, Kingsley, Faxon, Herrick; the insects
by Packard, Horn, Scudder, C. H. Fernald, Williston, Norton, Walsh, Fitch,
J. B. Smith, Comstock, Howard, Riley and many others; spiders by
Emerton, Marx, McCook; tunicates by Packard and Verrill; fishes by Baird,
Bean, Cope, Gilbert, Gill, Goode, Jordan, Putnam; amphibians and reptiles
by Cope; birds by Baird, Brewer, Coues, Elliott, Henshaw, Allen, Merriam,
Brewster, Ridgway; and the mammals by Allen, Baird, Cope, Coues, Elliott,
Merriam, Wilder.
Interest in the evolutionary theory continued to increase and eventually
developed into the morphological and embryological studies which reached
their culmination between 1885 and 1890 under the guidance of Whitman,
Mark, Minot, Brooks, Kingsley, E. B. Wilson and other famous zoologists
of the time. In these years the Journal of Morphology was established and
the American Morphological Society was formed.
The morphological, embryological and paleontological evidences of
evolution as indicated by homologies, developmental stages and adaptations
were the most absorbing subjects of zoological research and discussion.
by A. Agassiz, S. F. Clarke, Verrill; the echinoderms by A. Agassiz, Brooks,
Kingsley, Fewkes, Lyman, Verrill; the various groups of worms by
Benedict, Eisen, Silliman, Verrill, Webster, Whitman; the mollusks by A.
and W. G. Binney, Tryon, Conrad, Dall, Sanderson Smith, Stearns, Verrill;
the Brachiopods by Dall and Morse; the Bryozoa by Hyatt; the crustacea by
S. I. Smith, Harger, Hagen, Packard, Kingsley, Faxon, Herrick; the insects
by Packard, Horn, Scudder, C. H. Fernald, Williston, Norton, Walsh, Fitch,
J. B. Smith, Comstock, Howard, Riley and many others; spiders by
Emerton, Marx, McCook; tunicates by Packard and Verrill; fishes by Baird,
Bean, Cope, Gilbert, Gill, Goode, Jordan, Putnam; amphibians and reptiles
by Cope; birds by Baird, Brewer, Coues, Elliott, Henshaw, Allen, Merriam,
Brewster, Ridgway; and the mammals by Allen, Baird, Cope, Coues, Elliott,
Merriam, Wilder.
Interest in the evolutionary theory continued to increase and eventually
developed into the morphological and embryological studies which reached
their culmination between 1885 and 1890 under the guidance of Whitman,
Mark, Minot, Brooks, Kingsley, E. B. Wilson and other famous zoologists
of the time. In these years the Journal of Morphology was established and
the American Morphological Society was formed.
The morphological, embryological and paleontological evidences of
evolution as indicated by homologies, developmental stages and adaptations
were the most absorbing subjects of zoological research and discussion.
Page 443
Page 444
Zoology in the American Journal of Science, 1870–1918.
The third series of the Journal (1870–1895), likewise including fifty
volumes, embraces this period of zoological activity in morphological and
embryological studies, culminating with the inception of the modern
experimental methods.
In this period also occurred the greatest progress in marine systematic
zoology, due to the explorations of the United States Fish Commission off
the Atlantic Coast. The Journal had an important share in the zoological
development of this period also, for A. E. Verrill, who was now an associate
editor, was in charge of the collections of marine invertebrates.
Consequently most of the discoveries in this field were published in the
Journal in numerous original contributions by Verrill and his associates. The
explorations of the U. S. Fish Commission Steamer “Albatross” are
described from year to year by Verrill, with descriptions of the new species
of invertebrates discovered.
The numerous original contributions by Verrill on subjects of general
zoological interest as well as on those of a systematic nature give this third
series of the Journal much zoological importance. Verrill’s papers cover
almost the whole field of descriptive zoology, but are mainly devoted to
marine invertebrates. Those which were originally contributed to the
Journal or summarized by him in his literature reviews include the
following topics:
Sponges, 16, 406, 1878.
Coelenterates, 37, 450, 1864; 44, 125, 1867; 45, 411, 186; 46, 143, 1868; 47, 282, 1869; 48, 116,
419, 1869; 49, 370, 1870; 3, 187, 432, 1872; 6, 68, 1873; 21, 508, 1881; 6, 493, 1898; 7, 41, 143,
205, 375, 1899; 13, 75, 1902.
Echinoderms, 44, 125, 1867; 45, 417, 1868; 49, 93, 101, 1870; 2, 430, 1871; 11, 416, 1876; 49,
127, 199, 1895; 28, 59, 1909; 35, 477, 1913; 37, 483, 1914; 38, 107, 1914; 39, 684, 1915.
Worms, 50, 223, 1870; 3, 126, 1872.
Mollusks, 49, 217, 1870; 50, 405, 1870; 3, 209, 281, 1872; 5, 465, 1873; 7, 136, 158, 1874; 9, 123,
177, 1875; 10, 213, 1875; 12, 236, 1876; 14, 425, 1877; 19, 284, 1880; 20, 250, 251, 1880; 2, 74, 91,
1896; 3, 51, 79, 162, 355, 1897.
Crustacea, 44, 126, 1867; 48, 244, 430, 1869; 25, 119, 534, 1908.
Ascidians, 1, 54, 93, 211, 288, 443, 1871; 20, 251, 1880.
The third series of the Journal (1870–1895), likewise including fifty
volumes, embraces this period of zoological activity in morphological and
embryological studies, culminating with the inception of the modern
experimental methods.
In this period also occurred the greatest progress in marine systematic
zoology, due to the explorations of the United States Fish Commission off
the Atlantic Coast. The Journal had an important share in the zoological
development of this period also, for A. E. Verrill, who was now an associate
editor, was in charge of the collections of marine invertebrates.
Consequently most of the discoveries in this field were published in the
Journal in numerous original contributions by Verrill and his associates. The
explorations of the U. S. Fish Commission Steamer “Albatross” are
described from year to year by Verrill, with descriptions of the new species
of invertebrates discovered.
The numerous original contributions by Verrill on subjects of general
zoological interest as well as on those of a systematic nature give this third
series of the Journal much zoological importance. Verrill’s papers cover
almost the whole field of descriptive zoology, but are mainly devoted to
marine invertebrates. Those which were originally contributed to the
Journal or summarized by him in his literature reviews include the
following topics:
Sponges, 16, 406, 1878.
Coelenterates, 37, 450, 1864; 44, 125, 1867; 45, 411, 186; 46, 143, 1868; 47, 282, 1869; 48, 116,
419, 1869; 49, 370, 1870; 3, 187, 432, 1872; 6, 68, 1873; 21, 508, 1881; 6, 493, 1898; 7, 41, 143,
205, 375, 1899; 13, 75, 1902.
Echinoderms, 44, 125, 1867; 45, 417, 1868; 49, 93, 101, 1870; 2, 430, 1871; 11, 416, 1876; 49,
127, 199, 1895; 28, 59, 1909; 35, 477, 1913; 37, 483, 1914; 38, 107, 1914; 39, 684, 1915.
Worms, 50, 223, 1870; 3, 126, 1872.
Mollusks, 49, 217, 1870; 50, 405, 1870; 3, 209, 281, 1872; 5, 465, 1873; 7, 136, 158, 1874; 9, 123,
177, 1875; 10, 213, 1875; 12, 236, 1876; 14, 425, 1877; 19, 284, 1880; 20, 250, 251, 1880; 2, 74, 91,
1896; 3, 51, 79, 162, 355, 1897.
Crustacea, 44, 126, 1867; 48, 244, 430, 1869; 25, 119, 534, 1908.
Ascidians, 1, 54, 93, 211, 288, 443, 1871; 20, 251, 1880.
Page 445
Dredging operations and marine fauna, 49, 129, 1870; 2, 357, 1871; 5, 1, 98, 1873; 6, 435, 1873;
7, 38, 131, 405, 409, 498, 608, 1874; 9, 411, 1875; 10, 36, 196, 1875; 16, 207, 371, 1878; 17, 239,
258, 309, 472, 1879; 18, 52, 468, 1879; 19, 137, 187; 20, 390, 1880; 22, 292, 1881; 23, 135, 216,
309, 406, 1882; 24, 360, 477, 1882; 28, 213, 378, 1884; 29, 149, 1885.
Miscellaneous, 39, 221, 1865; 41, 249, 268, 1866; 44, 126, 1867; 48, 92, 1869; 3, 386, 1872; 7,
134, 1847; 10, 364, 1875; 16, 323, 1878; 20, 251, 1880; 3, 132, 135, 1897; 9, 313, 1900; 12, 88,
1901; 13, 327, 1902; 14, 72, 1902; 15, 332, 1903; 24, 179, 1907; 29, 561, 1910.
S. I. Smith describes the metamorphosis of the Crustacea (3, 401, 1872;
6, 67, 1873), species of crustacea (3, 373, 1872; 7, 601, 1874; 9, 476, 1875),
and dredging operations in Lake Superior (2, 373, 448, 1871). In this series
occurs also a series of papers on comparative anatomy and embryology
from the Chesapeake Zoological Laboratory in charge of W. K. Brooks. In
the 39th and 40th volumes of the third series (1890) occur several papers on
evolutionary topics by John T. Gulick (39, 21; 40, 1, 437) which have
attracted much attention.
Before the end of this period, however, the Journal was relieved from the
necessity of publishing zoological articles by the establishment of several
periodicals devoted especially to the various fields of zoology. We find,
therefore, but few exclusively zoological papers after 1885, although
articles of a general biological interest and the reviews of zoological books
continue.
In the fourth series of the Journal, beginning in 1896, occur also a
number of articles on systematic zoology by Verrill and others and several
papers having a general biological interest. Brief reviews of a small number
of zoological books are still continued, but at the present day the Journal,
which played so important a part in the early development of American
zoology, has been given over to the geological and physical sciences in
harmony with the modern demand for specialization.
7, 38, 131, 405, 409, 498, 608, 1874; 9, 411, 1875; 10, 36, 196, 1875; 16, 207, 371, 1878; 17, 239,
258, 309, 472, 1879; 18, 52, 468, 1879; 19, 137, 187; 20, 390, 1880; 22, 292, 1881; 23, 135, 216,
309, 406, 1882; 24, 360, 477, 1882; 28, 213, 378, 1884; 29, 149, 1885.
Miscellaneous, 39, 221, 1865; 41, 249, 268, 1866; 44, 126, 1867; 48, 92, 1869; 3, 386, 1872; 7,
134, 1847; 10, 364, 1875; 16, 323, 1878; 20, 251, 1880; 3, 132, 135, 1897; 9, 313, 1900; 12, 88,
1901; 13, 327, 1902; 14, 72, 1902; 15, 332, 1903; 24, 179, 1907; 29, 561, 1910.
S. I. Smith describes the metamorphosis of the Crustacea (3, 401, 1872;
6, 67, 1873), species of crustacea (3, 373, 1872; 7, 601, 1874; 9, 476, 1875),
and dredging operations in Lake Superior (2, 373, 448, 1871). In this series
occurs also a series of papers on comparative anatomy and embryology
from the Chesapeake Zoological Laboratory in charge of W. K. Brooks. In
the 39th and 40th volumes of the third series (1890) occur several papers on
evolutionary topics by John T. Gulick (39, 21; 40, 1, 437) which have
attracted much attention.
Before the end of this period, however, the Journal was relieved from the
necessity of publishing zoological articles by the establishment of several
periodicals devoted especially to the various fields of zoology. We find,
therefore, but few exclusively zoological papers after 1885, although
articles of a general biological interest and the reviews of zoological books
continue.
In the fourth series of the Journal, beginning in 1896, occur also a
number of articles on systematic zoology by Verrill and others and several
papers having a general biological interest. Brief reviews of a small number
of zoological books are still continued, but at the present day the Journal,
which played so important a part in the early development of American
zoology, has been given over to the geological and physical sciences in
harmony with the modern demand for specialization.
Page 446
Period of Experimental Biology, since 1890.
Zoological studies remained in large measure observational and
comparative until about 1890 when the experimental methods of Roux,
Driesch and others came into prominence. Interest then turned from the
accumulation of facts to an analysis of the underlying principles of
biological phenomena. The question now was not so much what the
organism does as how it does what is observed, and this question could be
answered only by the experimental control of the conditions. These
experimental studies met with such remarkable success that in a few years
the older morphological studies were largely abandoned, the Morphological
Society changed its name to the Society of Zoologists, and in 1904 the
Journal of Experimental Zoology was established. The experimental
methods were applied to all branches of biological science, and while it
must be freely admitted that little progress has been made toward an
understanding of the ultimate causes which underlie biological phenomena,
a great advance has been made in the elucidation of the general principles
involved.
Experimental embryology, histology, regeneration, comparative
physiology, neurology, cytology, and heredity have in recent years
successfully adopted an experimental aspect and have made significant
progress thereby. Biology has now taken its place beside chemistry and
physics as an experimental science.
The latest great advance in biology has been in the field of heredity. The
rediscovery of the Mendelian principles of heredity in 1900 brought to light
the most important generalization in biology in recent times. The new
science of genetics is essentially the experimental study of heredity.
We are at the moment in the midst of an effort to establish in biology a
few relatively simple laws by using for the purpose the vast accumulations
of observational data gathered in past years, supplemented by such
experimental data as have been provided by these more recent
investigations. Such hypotheses as have been formulated are for the most
part only tentatively held, for their validity is generally incapable of a
critical test. But wherever such tests have been possible, the laws of
Zoological studies remained in large measure observational and
comparative until about 1890 when the experimental methods of Roux,
Driesch and others came into prominence. Interest then turned from the
accumulation of facts to an analysis of the underlying principles of
biological phenomena. The question now was not so much what the
organism does as how it does what is observed, and this question could be
answered only by the experimental control of the conditions. These
experimental studies met with such remarkable success that in a few years
the older morphological studies were largely abandoned, the Morphological
Society changed its name to the Society of Zoologists, and in 1904 the
Journal of Experimental Zoology was established. The experimental
methods were applied to all branches of biological science, and while it
must be freely admitted that little progress has been made toward an
understanding of the ultimate causes which underlie biological phenomena,
a great advance has been made in the elucidation of the general principles
involved.
Experimental embryology, histology, regeneration, comparative
physiology, neurology, cytology, and heredity have in recent years
successfully adopted an experimental aspect and have made significant
progress thereby. Biology has now taken its place beside chemistry and
physics as an experimental science.
The latest great advance in biology has been in the field of heredity. The
rediscovery of the Mendelian principles of heredity in 1900 brought to light
the most important generalization in biology in recent times. The new
science of genetics is essentially the experimental study of heredity.
We are at the moment in the midst of an effort to establish in biology a
few relatively simple laws by using for the purpose the vast accumulations
of observational data gathered in past years, supplemented by such
experimental data as have been provided by these more recent
investigations. Such hypotheses as have been formulated are for the most
part only tentatively held, for their validity is generally incapable of a
critical test. But wherever such tests have been possible, the laws of
Page 447
mathematics, physics and chemistry are found applicable to biological
phenomena.
The number of investigators has now become so great and their activities
so prolific that the list and synopses of the zoological publications each year
cover upwards of 1000 to 1500 pages in the International Catalogue of
Scientific Literature.
American Leadership.—During the first half of the century the progress
of zoology in America remained distinctly behind that of Europe. At the
beginning of the century the science was farthest developed by the French
and English, although Linnæus was a Swede and took his degree in
Holland. Under the influence of Von Baer and his monumental treatise on
embryology (Ueber Entwicklungsgeschichte der Thiere, 1828), and
supported later by the great physiologist, Johannes Müller, whose
“Physiologie des Menschen” (1846) forms the basis of modern physiology,
the German school forged rapidly ahead and eventually assumed the
leadership in zoology, as in several other branches of science.
In the latter half of the century the influence of the German universities
dominated in a large measure the zoological investigations in America. The
reason for this is partly due to the fact that many of our young zoologists,
after finishing their college course, completed their preparation for research
by a year or more at a German university. The more mature zoologists, too,
looked forward with keen anticipation to spending their summer vacations
and sabbatical years in research in a German laboratory or at the famous
Naples station in which the German influence was dominant.
With the rise of experimental biology since 1890, however, the American
zoologists have shown so high a degree of originality in devising
experiments, so much skill in performing them, and such keenness in
analyzing the results, that they have assumed the world leadership in
several of the special fields into which the science of zoology is now
divided.
phenomena.
The number of investigators has now become so great and their activities
so prolific that the list and synopses of the zoological publications each year
cover upwards of 1000 to 1500 pages in the International Catalogue of
Scientific Literature.
American Leadership.—During the first half of the century the progress
of zoology in America remained distinctly behind that of Europe. At the
beginning of the century the science was farthest developed by the French
and English, although Linnæus was a Swede and took his degree in
Holland. Under the influence of Von Baer and his monumental treatise on
embryology (Ueber Entwicklungsgeschichte der Thiere, 1828), and
supported later by the great physiologist, Johannes Müller, whose
“Physiologie des Menschen” (1846) forms the basis of modern physiology,
the German school forged rapidly ahead and eventually assumed the
leadership in zoology, as in several other branches of science.
In the latter half of the century the influence of the German universities
dominated in a large measure the zoological investigations in America. The
reason for this is partly due to the fact that many of our young zoologists,
after finishing their college course, completed their preparation for research
by a year or more at a German university. The more mature zoologists, too,
looked forward with keen anticipation to spending their summer vacations
and sabbatical years in research in a German laboratory or at the famous
Naples station in which the German influence was dominant.
With the rise of experimental biology since 1890, however, the American
zoologists have shown so high a degree of originality in devising
experiments, so much skill in performing them, and such keenness in
analyzing the results, that they have assumed the world leadership in
several of the special fields into which the science of zoology is now
divided.
Page 448
Biological Periodicals.
Perhaps in no better way can the progress of biology in America be
illustrated than by a brief survey of the origin and development of the more
important biological journals. For it will be seen that these publications
have become more numerous and more specialized as the science has
advanced in specialization.
The early publications—which as is well known, treated mainly of the
birds, mammals and other vertebrates, and of insects, crustacea and shells—
consisted mainly of separate books or pamphlets, published by private
subscription. After the establishment of the so-called Academies of Science,
or of Arts and Sciences, toward the end of the eighteenth and in the first
quarter of the nineteenth century, the reports of the meetings began to be
published as periodical Journals, supported by the academies. In these
publications, and in the Journal which was founded at the same time, appear
papers on all branches of science, including zoology. As soon as zoology in
America assumed its modern aspects through the influence of Louis
Agassiz and his followers the earliest strictly zoological journals were
established.
It should be noted, however, that the journals of the scientific and natural
history societies were more or less fully devoted to zoological topics
according to the nature of the activities of the members and correspondents.
After the establishment of the Museum of Comparative Zoology by Louis
Agassiz came the founding in 1863 of its Bulletin and later its Memoirs.
These publications have continued to the present day as a standard of
excellence for the reports of zoological investigations. In connection with
the systematic work on mollusks, the American Journal of Conchology was
established in 1865. The American Naturalist was founded in 1867 by four
of Louis Agassiz’s pupils, Hyatt, Morse, Packard and Putnam. It was later
edited by Cope as a leading periodical for the publication of biological
papers, particularly those relating to evolution, and is at present devoted to
evolutionary topics. It is now in the 52d volume of its new series.
With the awakened interest in comparative anatomy and embryology
came the need for an American journal which should supply a means of
Perhaps in no better way can the progress of biology in America be
illustrated than by a brief survey of the origin and development of the more
important biological journals. For it will be seen that these publications
have become more numerous and more specialized as the science has
advanced in specialization.
The early publications—which as is well known, treated mainly of the
birds, mammals and other vertebrates, and of insects, crustacea and shells—
consisted mainly of separate books or pamphlets, published by private
subscription. After the establishment of the so-called Academies of Science,
or of Arts and Sciences, toward the end of the eighteenth and in the first
quarter of the nineteenth century, the reports of the meetings began to be
published as periodical Journals, supported by the academies. In these
publications, and in the Journal which was founded at the same time, appear
papers on all branches of science, including zoology. As soon as zoology in
America assumed its modern aspects through the influence of Louis
Agassiz and his followers the earliest strictly zoological journals were
established.
It should be noted, however, that the journals of the scientific and natural
history societies were more or less fully devoted to zoological topics
according to the nature of the activities of the members and correspondents.
After the establishment of the Museum of Comparative Zoology by Louis
Agassiz came the founding in 1863 of its Bulletin and later its Memoirs.
These publications have continued to the present day as a standard of
excellence for the reports of zoological investigations. In connection with
the systematic work on mollusks, the American Journal of Conchology was
established in 1865. The American Naturalist was founded in 1867 by four
of Louis Agassiz’s pupils, Hyatt, Morse, Packard and Putnam. It was later
edited by Cope as a leading periodical for the publication of biological
papers, particularly those relating to evolution, and is at present devoted to
evolutionary topics. It is now in the 52d volume of its new series.
With the awakened interest in comparative anatomy and embryology
came the need for an American journal which should supply a means of
Page 449
publication for the reports of researches accomplished by the increasing
number of workers in these fields. This need was fully met by the
establishment of the Journal of Morphology in 1887. This publication, now
in its 30th volume, has equalled the best European journals in the character
of its papers. A few years later (1891) came the Journal of Comparative
Neurology for the publication of investigations relating to the morphology
and physiology of the nervous system and to nervous and allied phenomena
in all groups of organisms. Twenty-eight volumes of this journal have been
completed. The Zoological Bulletin was started under the auspices of the
Marine Biological Laboratory in 1897 for the publication of papers of a less
extensive nature and which could be more promptly issued than those in the
Journal of Morphology where elaborate plates were required. After two
years the scope of the Bulletin was enlarged to include botanical and
physiological subjects. The name was correspondingly changed to the
Biological Bulletin. Of this important periodical 33 volumes have been
issued.
For the publication of papers on human and comparative anatomy and
embryology, the American Journal of Anatomy was established in 1901,
and is now in its twenty-third volume.
Meanwhile the trend of zoological interest was toward topics connected
with the ultimate nature of biological phenomena. The meaning of these
phenomena could be determined only by the experimental method.
Researches in this field became more prominent and the adequate
publication of the numerous papers required the establishment of a new
journal in 1904. This was named the Journal of Experimental Zoology. It
immediately took its place in the front rank of American zoological
periodicals. Twenty-four volumes have been published.
In spite of the constantly increasing number of journals, the science grew
faster than the means of publication. So crowded did the American journals
become that long delays often resulted before the results of an investigation
could be issued. This condition was met in part by the sending of many
papers to be published in European journals (a necessity most discreditable
to American zoology) and in part by the establishment of additional means
of publication. Of the latter the Anatomical Record, now in its fourteenth
volume, was begun in 1906 for the prompt publication of briefer papers on
number of workers in these fields. This need was fully met by the
establishment of the Journal of Morphology in 1887. This publication, now
in its 30th volume, has equalled the best European journals in the character
of its papers. A few years later (1891) came the Journal of Comparative
Neurology for the publication of investigations relating to the morphology
and physiology of the nervous system and to nervous and allied phenomena
in all groups of organisms. Twenty-eight volumes of this journal have been
completed. The Zoological Bulletin was started under the auspices of the
Marine Biological Laboratory in 1897 for the publication of papers of a less
extensive nature and which could be more promptly issued than those in the
Journal of Morphology where elaborate plates were required. After two
years the scope of the Bulletin was enlarged to include botanical and
physiological subjects. The name was correspondingly changed to the
Biological Bulletin. Of this important periodical 33 volumes have been
issued.
For the publication of papers on human and comparative anatomy and
embryology, the American Journal of Anatomy was established in 1901,
and is now in its twenty-third volume.
Meanwhile the trend of zoological interest was toward topics connected
with the ultimate nature of biological phenomena. The meaning of these
phenomena could be determined only by the experimental method.
Researches in this field became more prominent and the adequate
publication of the numerous papers required the establishment of a new
journal in 1904. This was named the Journal of Experimental Zoology. It
immediately took its place in the front rank of American zoological
periodicals. Twenty-four volumes have been published.
In spite of the constantly increasing number of journals, the science grew
faster than the means of publication. So crowded did the American journals
become that long delays often resulted before the results of an investigation
could be issued. This condition was met in part by the sending of many
papers to be published in European journals (a necessity most discreditable
to American zoology) and in part by the establishment of additional means
of publication. Of the latter the Anatomical Record, now in its fourteenth
volume, was begun in 1906 for the prompt publication of briefer papers on
Page 450
vertebrate anatomy, embryology and histology and for preliminary reports
and notes on technique.
During the past few years has come a great advance in the experimental
breeding of plants and animals. Problems in heredity and evolution have
taken on a new interest since the importance and validity of Mendel’s
discovery have been recognized. To meet this development of biology the
journal Genetics was begun in 1916 for the publication of technical papers,
while the Journal of Heredity, modified from the American Breeders
Magazine, is devoted to popular articles on animal and plant breeding, and
Eugenics.
On the whole, the science of zoology is now assuming a closer relation to
practical affairs. Entomology, for example, is now represented by the
Journal of Economic Entomology, of which 10 volumes have been issued
since 1907. The Journal of Animal Behavior covers another practical field
of research. The Proceedings of the Society for Experimental Biology and
Medicine, starting in 1903, the American Journal of Physiology, and several
other publications cover the physiological field. The Journal of
Parasitology, established 1914, now in its fourth volume, is devoted to the
interests of medical zoology. The Auk, now in the 34th volume of its new
series (42d of old series), is the official organ of the American
Ornithologists Union and is devoted to the dissemination of knowledge
concerning bird life. The Annals of the Entomological Society of America,
established in 1908, and now in its 10th volume, is one of several important
entomological journals. The Nautilus, of which 28 volumes have been
issued, is one of the more successful journals devoted to conchology. This
list might be extended to include numerous other periodicals of importance,
both technical and popular, which have been of great service in the various
fields of biology.
In addition to these are the many volumes of systematic papers in the
Proceedings of the United States National Museum, the practical reports in
the Bulletin of the United States Fish Commission, the vast literature issued
yearly by the various divisions of the United States Department of
Agriculture, Public Health Service and other Governmental departments,
while the list of publications by scientific societies, museums, and other
institutes is constantly increasing and covers all fields of biological
research.
and notes on technique.
During the past few years has come a great advance in the experimental
breeding of plants and animals. Problems in heredity and evolution have
taken on a new interest since the importance and validity of Mendel’s
discovery have been recognized. To meet this development of biology the
journal Genetics was begun in 1916 for the publication of technical papers,
while the Journal of Heredity, modified from the American Breeders
Magazine, is devoted to popular articles on animal and plant breeding, and
Eugenics.
On the whole, the science of zoology is now assuming a closer relation to
practical affairs. Entomology, for example, is now represented by the
Journal of Economic Entomology, of which 10 volumes have been issued
since 1907. The Journal of Animal Behavior covers another practical field
of research. The Proceedings of the Society for Experimental Biology and
Medicine, starting in 1903, the American Journal of Physiology, and several
other publications cover the physiological field. The Journal of
Parasitology, established 1914, now in its fourth volume, is devoted to the
interests of medical zoology. The Auk, now in the 34th volume of its new
series (42d of old series), is the official organ of the American
Ornithologists Union and is devoted to the dissemination of knowledge
concerning bird life. The Annals of the Entomological Society of America,
established in 1908, and now in its 10th volume, is one of several important
entomological journals. The Nautilus, of which 28 volumes have been
issued, is one of the more successful journals devoted to conchology. This
list might be extended to include numerous other periodicals of importance,
both technical and popular, which have been of great service in the various
fields of biology.
In addition to these are the many volumes of systematic papers in the
Proceedings of the United States National Museum, the practical reports in
the Bulletin of the United States Fish Commission, the vast literature issued
yearly by the various divisions of the United States Department of
Agriculture, Public Health Service and other Governmental departments,
while the list of publications by scientific societies, museums, and other
institutes is constantly increasing and covers all fields of biological
research.
Page 451
At the present time facilities for the publication of research on any
branch of zoology are as a rule entirely adequate. For this highly
satisfactory condition the science is indebted to the support given five of its
most important journals by the Wistar Institute of Anatomy and Biology.
branch of zoology are as a rule entirely adequate. For this highly
satisfactory condition the science is indebted to the support given five of its
most important journals by the Wistar Institute of Anatomy and Biology.
Page 452
Biological Associations.
An important light on the history of biology in America can be thrown by
a glance at the rise and development of societies or associations for the
report and discussion of papers relating to that branch of science. In the first
half of the nineteenth century natural history societies were formed in most
cities and centers of learning. These were very important factors in the
promotion of scientific research as well as in the diffusion of popular
knowledge of living things. The aims and activities of twenty-nine such
scientific societies, many of which were devoted especially to natural
history, are described in one of the early volumes of the Journal (10, 369,
1826). The Connecticut Academy of Arts and Sciences, dating from 1799,
the Philadelphia Academy of Natural Sciences from 1812, and the New
York Lyceum of Natural History (in 1876 name changed to New York
Academy of Sciences) from 1817 are among the oldest of those which still
exist.
Of national institutions the American Philosophical Society was founded
in 1743, the American Academy of Arts and Sciences in 1780, and the
National Academy of Sciences in 1863.
The American Association for the Advancement of Science, with its
thousands of members, now has separate sections for each of the special
branches of science. This great association was organized in 1848, as the
successor of the Association of American Geologists and Naturalists. This
was itself a revival of the American Geological Society which first met at
Yale in 1819. Its meetings have given a great support to the scientific work
of the country.
The American Society of Naturalists was founded in 1883. The original
plan of the society was for the discussion of methods of investigation,
administration and instruction in the natural sciences, but its program is
now entirely devoted to discussions and papers of a broad biological
interest. It also arranges for an annual dinner of the several biological
societies and an address on some general biological topic.
In 1890, toward the end of the period in which morphological studies
were being emphasized, the professional zoologists of the eastern states
An important light on the history of biology in America can be thrown by
a glance at the rise and development of societies or associations for the
report and discussion of papers relating to that branch of science. In the first
half of the nineteenth century natural history societies were formed in most
cities and centers of learning. These were very important factors in the
promotion of scientific research as well as in the diffusion of popular
knowledge of living things. The aims and activities of twenty-nine such
scientific societies, many of which were devoted especially to natural
history, are described in one of the early volumes of the Journal (10, 369,
1826). The Connecticut Academy of Arts and Sciences, dating from 1799,
the Philadelphia Academy of Natural Sciences from 1812, and the New
York Lyceum of Natural History (in 1876 name changed to New York
Academy of Sciences) from 1817 are among the oldest of those which still
exist.
Of national institutions the American Philosophical Society was founded
in 1743, the American Academy of Arts and Sciences in 1780, and the
National Academy of Sciences in 1863.
The American Association for the Advancement of Science, with its
thousands of members, now has separate sections for each of the special
branches of science. This great association was organized in 1848, as the
successor of the Association of American Geologists and Naturalists. This
was itself a revival of the American Geological Society which first met at
Yale in 1819. Its meetings have given a great support to the scientific work
of the country.
The American Society of Naturalists was founded in 1883. The original
plan of the society was for the discussion of methods of investigation,
administration and instruction in the natural sciences, but its program is
now entirely devoted to discussions and papers of a broad biological
interest. It also arranges for an annual dinner of the several biological
societies and an address on some general biological topic.
In 1890, toward the end of the period in which morphological studies
were being emphasized, the professional zoologists of the eastern states
Page 453
founded the American Morphological Society. This association held annual
meetings during the Christmas holidays for the presentation of zoological
papers. This name became less appropriate after a few years because of the
gradual decrease in the proportion of morphological investigations owing to
the greater attention being directed to problems in experimental zoology
and physiology. Consequently the name was changed to the American
Society of Zoologists. To be eligible for membership in this society a
person must be an active investigator in some branch of zoology, as
indicated by the published results.
The American Association of Anatomists includes in its membership
investigators and teachers in comparative anatomy, embryology, and
histology as well as in human anatomy. Many professional zoologists and
experimental biologists present their papers before this society, or at the
meetings of the American Physiological Society. The Entomological
Society of America and the American Association of Economic
Entomologists are large and active societies.
These national societies have been of great service in fostering a high
standard of zoological research. A still more important service, though
generally less conspicuous, is rendered by the journal clubs in connection
with all the larger zoological laboratories, and by local scientific societies
which are now maintained in all the larger centers of learning throughout
the country. There are also specific societies for some of the different fields
of biological work.
meetings during the Christmas holidays for the presentation of zoological
papers. This name became less appropriate after a few years because of the
gradual decrease in the proportion of morphological investigations owing to
the greater attention being directed to problems in experimental zoology
and physiology. Consequently the name was changed to the American
Society of Zoologists. To be eligible for membership in this society a
person must be an active investigator in some branch of zoology, as
indicated by the published results.
The American Association of Anatomists includes in its membership
investigators and teachers in comparative anatomy, embryology, and
histology as well as in human anatomy. Many professional zoologists and
experimental biologists present their papers before this society, or at the
meetings of the American Physiological Society. The Entomological
Society of America and the American Association of Economic
Entomologists are large and active societies.
These national societies have been of great service in fostering a high
standard of zoological research. A still more important service, though
generally less conspicuous, is rendered by the journal clubs in connection
with all the larger zoological laboratories, and by local scientific societies
which are now maintained in all the larger centers of learning throughout
the country. There are also specific societies for some of the different fields
of biological work.
Page 454
Biological Stations.
No insignificant factor in the development of biological science has been
the establishment of biological stations where investigators, teachers and
students meet in the Summer vacation for special studies, discussions and
research. The most successful of these laboratories have been located on the
seashore and here the study of marine life in Summer supplements the work
of the school or university biological courses. The famous Naples Station
was founded in 1870, and was shortly after followed by several others.
Similar biological stations are now supported on almost every coast in
Europe and in several inland localities.
The first such American school was established by Louis Agassiz at the
island of Penikese on the coast of Massachusetts in 1873, succeeding his
private laboratory at Nahant. During that Summer more than forty students
gained enthusiasm for the work of future years. Unfortunately the
laboratory so auspiciously started was of brief duration, for the death of
Agassiz occurred in December of the same year, and the laboratory was
discontinued at the end of the following Summer. Shortly afterward
Alexander Agassiz equipped a small private laboratory at Newport, Rhode
Island, and W. K. Brooks established the Chesapeake Bay Zoological
Laboratory.
At this time the United States Fish Commission was engaged under the
direction of Spencer F. Baird in a survey of the marine life of the waters off
the Eastern Coast. Between 1881 and 1886 the Commission established the
splendidly equipped biological station at Woods Hole, Massachusetts. Both
here and at the Fish Commission Laboratory at Beaufort, North Carolina,
much work in general zoology as well as in economic problems is
accomplished. These laboratories are designed particularly for specialists
engaged in researches connected with the work of the Fish Commission.
A need was soon felt for a marine laboratory along broader lines, and one
available to the students and teachers of the schools and colleges. To meet
these requirements the Woods Hole Marine Biological Laboratory was
started in 1887, as the successor to an earlier laboratory at Annisquam, and
has since become a great Summer congress for biologists from all parts of
No insignificant factor in the development of biological science has been
the establishment of biological stations where investigators, teachers and
students meet in the Summer vacation for special studies, discussions and
research. The most successful of these laboratories have been located on the
seashore and here the study of marine life in Summer supplements the work
of the school or university biological courses. The famous Naples Station
was founded in 1870, and was shortly after followed by several others.
Similar biological stations are now supported on almost every coast in
Europe and in several inland localities.
The first such American school was established by Louis Agassiz at the
island of Penikese on the coast of Massachusetts in 1873, succeeding his
private laboratory at Nahant. During that Summer more than forty students
gained enthusiasm for the work of future years. Unfortunately the
laboratory so auspiciously started was of brief duration, for the death of
Agassiz occurred in December of the same year, and the laboratory was
discontinued at the end of the following Summer. Shortly afterward
Alexander Agassiz equipped a small private laboratory at Newport, Rhode
Island, and W. K. Brooks established the Chesapeake Bay Zoological
Laboratory.
At this time the United States Fish Commission was engaged under the
direction of Spencer F. Baird in a survey of the marine life of the waters off
the Eastern Coast. Between 1881 and 1886 the Commission established the
splendidly equipped biological station at Woods Hole, Massachusetts. Both
here and at the Fish Commission Laboratory at Beaufort, North Carolina,
much work in general zoology as well as in economic problems is
accomplished. These laboratories are designed particularly for specialists
engaged in researches connected with the work of the Fish Commission.
A need was soon felt for a marine laboratory along broader lines, and one
available to the students and teachers of the schools and colleges. To meet
these requirements the Woods Hole Marine Biological Laboratory was
started in 1887, as the successor to an earlier laboratory at Annisquam, and
has since become a great Summer congress for biologists from all parts of
Page 455
the country. It is safe to say that no other institution has been of equal
service in securing for biology the high plane it now occupies in American
science. The leading spirit in the establishment of this laboratory and its
director for many years was Charles O. Whitman.
Successful marine laboratories are located also at Cold Spring Harbor,
Long Island; at Harpswell, Maine; and at Bermuda. The Carnegie
Institution maintains a laboratory at Tortugas Island, Florida, for the
investigation of tropical marine life.
On the Pacific Coast marine laboratories are located at Pacific Grove and
at La Jolla, California, and at Friday Harbor, Washington. Several other
biological laboratories are open each Summer on our coasts, as well as a
number of fresh-water laboratories on the interior lakes. There are also
several mountain laboratories. The influence of these laboratories on
American biology is immeasurable.
service in securing for biology the high plane it now occupies in American
science. The leading spirit in the establishment of this laboratory and its
director for many years was Charles O. Whitman.
Successful marine laboratories are located also at Cold Spring Harbor,
Long Island; at Harpswell, Maine; and at Bermuda. The Carnegie
Institution maintains a laboratory at Tortugas Island, Florida, for the
investigation of tropical marine life.
On the Pacific Coast marine laboratories are located at Pacific Grove and
at La Jolla, California, and at Friday Harbor, Washington. Several other
biological laboratories are open each Summer on our coasts, as well as a
number of fresh-water laboratories on the interior lakes. There are also
several mountain laboratories. The influence of these laboratories on
American biology is immeasurable.
Page 456
Natural History Museums.
Museums of Natural History or “Cabinets of Natural Curios” as they
were sometimes called, were established in the first half of the nineteenth
century in connection with the various natural history societies. These were
of much service in stimulating the collection of zoological “specimens” and
in arousing a popular interest in natural history.
The zoological museum of earlier days consisted of rows on rows of
systematically arranged specimens, each carefully labelled with scientific
name, locality, date of collection and donor—much like the pages of a
catalogue. All this has now been changed; the bottles of specimens have
been relegated to the storeroom, and the great plate glass cases of the
modern museum represent individual studies in the various fields of modern
zoological research, or individual chapters in the latest biological text-
books. Often the talent of the artist and the skill of the taxidermist are
cunningly combined to produce most realistic bits of nature.
The United States National Museum, the American Museum of Natural
History, the Field Columbian Museum and the Museum of Comparative
Zoology are among the finest museums of the world, while many of the
states, cities, and universities maintain public museums as a part of their
educational systems.
Museums of Natural History or “Cabinets of Natural Curios” as they
were sometimes called, were established in the first half of the nineteenth
century in connection with the various natural history societies. These were
of much service in stimulating the collection of zoological “specimens” and
in arousing a popular interest in natural history.
The zoological museum of earlier days consisted of rows on rows of
systematically arranged specimens, each carefully labelled with scientific
name, locality, date of collection and donor—much like the pages of a
catalogue. All this has now been changed; the bottles of specimens have
been relegated to the storeroom, and the great plate glass cases of the
modern museum represent individual studies in the various fields of modern
zoological research, or individual chapters in the latest biological text-
books. Often the talent of the artist and the skill of the taxidermist are
cunningly combined to produce most realistic bits of nature.
The United States National Museum, the American Museum of Natural
History, the Field Columbian Museum and the Museum of Comparative
Zoology are among the finest museums of the world, while many of the
states, cities, and universities maintain public museums as a part of their
educational systems.
Page 457
Systematic Zoology and Taxonomy.
The work in systematic zoology is now mainly carried on by specialists
in relatively small groups of animals. This is necessitated both by the
increasingly large number of species known to science and by the
completeness and exactness with which species must now be defined. The
majority of systematic workers are now connected with museums where the
large collections furnish material for comparative studies.
Prominent in this field is the United States National Museum, the
publications of which are mainly taxonomic and zoogeographic, and cover
every group of organism. The adequacy of this great museum for such
studies may be illustrated by the collection of mammals. This museum has
the types of 1135 of the 2138 forms (including species and subspecies) of
North American mammals recognized in Miller’s list,[175] and less than 200
forms lack representatives among the 120,000 specimens of mammals.
Systematic monographs of several of the orders of mammals have been
published.
Systematic study of the birds has brought the number of species and
subspecies known to inhabit North and Middle America to above 3000. The
most comprehensive systematic treatise is the still incomplete report of
Ridgeway[176] of which seven large volumes have already been issued.
On the reptiles, the most complete monograph is that by Cope[177] entitled
“The Crocodilians, Lizards and Snakes of North America.”
The Amphibia have also been studied by Cope, whose report on the
Batrachia of North America[178] is the standard taxonomic work.
The most comprehensive systematic work on fishes is the “Descriptive
Catalogue of the Fishes of North and Middle America” by Jordan and
Evermann.[179]
The invertebrate groups have been in part similarly monographed by the
members of the U. S. National Museum staff and others, and further studies
are in progress. Other taxonomic monographs published by this museum
include the various groups of animals from many different parts of the
world.
The work in systematic zoology is now mainly carried on by specialists
in relatively small groups of animals. This is necessitated both by the
increasingly large number of species known to science and by the
completeness and exactness with which species must now be defined. The
majority of systematic workers are now connected with museums where the
large collections furnish material for comparative studies.
Prominent in this field is the United States National Museum, the
publications of which are mainly taxonomic and zoogeographic, and cover
every group of organism. The adequacy of this great museum for such
studies may be illustrated by the collection of mammals. This museum has
the types of 1135 of the 2138 forms (including species and subspecies) of
North American mammals recognized in Miller’s list,[175] and less than 200
forms lack representatives among the 120,000 specimens of mammals.
Systematic monographs of several of the orders of mammals have been
published.
Systematic study of the birds has brought the number of species and
subspecies known to inhabit North and Middle America to above 3000. The
most comprehensive systematic treatise is the still incomplete report of
Ridgeway[176] of which seven large volumes have already been issued.
On the reptiles, the most complete monograph is that by Cope[177] entitled
“The Crocodilians, Lizards and Snakes of North America.”
The Amphibia have also been studied by Cope, whose report on the
Batrachia of North America[178] is the standard taxonomic work.
The most comprehensive systematic work on fishes is the “Descriptive
Catalogue of the Fishes of North and Middle America” by Jordan and
Evermann.[179]
The invertebrate groups have been in part similarly monographed by the
members of the U. S. National Museum staff and others, and further studies
are in progress. Other taxonomic monographs published by this museum
include the various groups of animals from many different parts of the
world.
Page 458
A number of the larger State, municipal, and university museums publish
bulletins on special groups represented in their collections as well as articles
of general zoological interest.
Expeditions, subsidized by museum and private funds, are from time to
time sent to various parts of the world and their results are often published
in sumptuous manner.
The total number of living species of animals is unknown, but
considering that about a quarter of a million new species have been
described during the past thirty years, it is probable that several million
species are in existence to-day. More than half a million have been
described. These are probably but a small fraction of the number that have
existed in past geological ages.
Thus, in spite of all the work that has been done in systematic zoology
and as the number of known species continues to increase, there still remain
many groups of animals, some of which are by no means rare or minute, in
which probably only a small proportion of the species are as yet capable of
identification.
It is only since the publication of Ward and Whipple’s “Fresh-water
Biology” within the past year that the amateur zoologist could hope to find
even the names of all the organisms which may be collected from a single
pool of water. And in many cases he will still meet with disappointment, for
many of our protozoa and other fresh-water organisms have not yet been
described as species.
During the past few years there has been a tendency on the part of some
of our biologists engaged in experimental work to disparage the studies of
the systematists. It must be granted, however, that both lines of work are
essential to the sound development of zoological science, for experimental
investigations in which the accurate diagnosis of species is ignored always
result in confusion.
Ecology.—The marvelous modifications in structure and instincts by
which the various animals are adapted to their surroundings now forms a
special topic in biological research and one of the most fascinating. The
adaptations in habitat, time, behavior, appearance and even in structure are
found capable of a certain individual modification when studied
experimentally.
bulletins on special groups represented in their collections as well as articles
of general zoological interest.
Expeditions, subsidized by museum and private funds, are from time to
time sent to various parts of the world and their results are often published
in sumptuous manner.
The total number of living species of animals is unknown, but
considering that about a quarter of a million new species have been
described during the past thirty years, it is probable that several million
species are in existence to-day. More than half a million have been
described. These are probably but a small fraction of the number that have
existed in past geological ages.
Thus, in spite of all the work that has been done in systematic zoology
and as the number of known species continues to increase, there still remain
many groups of animals, some of which are by no means rare or minute, in
which probably only a small proportion of the species are as yet capable of
identification.
It is only since the publication of Ward and Whipple’s “Fresh-water
Biology” within the past year that the amateur zoologist could hope to find
even the names of all the organisms which may be collected from a single
pool of water. And in many cases he will still meet with disappointment, for
many of our protozoa and other fresh-water organisms have not yet been
described as species.
During the past few years there has been a tendency on the part of some
of our biologists engaged in experimental work to disparage the studies of
the systematists. It must be granted, however, that both lines of work are
essential to the sound development of zoological science, for experimental
investigations in which the accurate diagnosis of species is ignored always
result in confusion.
Ecology.—The marvelous modifications in structure and instincts by
which the various animals are adapted to their surroundings now forms a
special topic in biological research and one of the most fascinating. The
adaptations in habitat, time, behavior, appearance and even in structure are
found capable of a certain individual modification when studied
experimentally.
Page 459
Zoogeography.—Closely associated with systematic zoology, and indeed
a part of the subject in its broader sense, is the study of the geographical
distribution of animal species and larger groups.
Paleontology.—The geological succession of organisms embraces a field
where zoologist and geologist meet. The wonderful progress made by
American investigators is well described in the preceding chapters on
Historical Geology and Vertebrate Paleontology.
a part of the subject in its broader sense, is the study of the geographical
distribution of animal species and larger groups.
Paleontology.—The geological succession of organisms embraces a field
where zoologist and geologist meet. The wonderful progress made by
American investigators is well described in the preceding chapters on
Historical Geology and Vertebrate Paleontology.
Page 460
Biometry.
Since Darwin’s theory of evolution postulated the origin of new species
by means of natural selection, it was obviously necessary in order to apply a
critical test to determine the precise limits of a species. It was, therefore,
proposed to subject a given species to a strict examination by the
application of statistical methods to determine the range of variation of its
members and the extent to which the species intergrades with others. Other
problems, particularly those concerning heredity, were treated in similar
manner. This branch of biological science was particularly developed by the
English School, led by Sir Francis Galton, followed by Karl Pearson and
William Bateson.
In America the methods of biometry have been utilized extensively by
Charles B. Davenport, Raymond Pearl, H. S. Jennings and others in the
solution of problems in genetics and evolution. Their work shows the great
value of critical statistical analysis in the interpretation of biological data. A
thorough training in mathematics is now found to be hardly less important
for the biologist than is a knowledge of physics and chemistry, for the
science of biometry has become one of the most important adjuncts to the
study of genetics.
Since Darwin’s theory of evolution postulated the origin of new species
by means of natural selection, it was obviously necessary in order to apply a
critical test to determine the precise limits of a species. It was, therefore,
proposed to subject a given species to a strict examination by the
application of statistical methods to determine the range of variation of its
members and the extent to which the species intergrades with others. Other
problems, particularly those concerning heredity, were treated in similar
manner. This branch of biological science was particularly developed by the
English School, led by Sir Francis Galton, followed by Karl Pearson and
William Bateson.
In America the methods of biometry have been utilized extensively by
Charles B. Davenport, Raymond Pearl, H. S. Jennings and others in the
solution of problems in genetics and evolution. Their work shows the great
value of critical statistical analysis in the interpretation of biological data. A
thorough training in mathematics is now found to be hardly less important
for the biologist than is a knowledge of physics and chemistry, for the
science of biometry has become one of the most important adjuncts to the
study of genetics.
Page 461
Comparative Anatomy and Embryology.
Comparative Anatomy.—Upon the foundations laid down by Cuvier a
century ago the present elaborate structure of comparative anatomy of
animals, both vertebrate and invertebrate, has been developed. Vast as is the
present accumulation of facts and theories many important problems still
await their solution. Jeffries Wyman was long a leader in this field, where
many workers are now engaged.
Embryology.—The embryological studies, so brilliantly begun by Von
Baer early in the nineteenth century, are still in progress. They have now
been extended to the groups more difficult of investigation and into the
earliest stages of fertilization and implantation in the mammals. Artificial
cultural methods have yielded important results. Louis and Alexander
Agassiz, Mark, Minot, Brooks, Whitman, Conklin and E. B. Wilson have
taken prominent parts in this work.
In the early nineties embryological studies were directed to the
arrangement of cells in the dividing egg, and there was much discussion of
“cell lineage” in development. Valuable as were these studies they threw
comparatively little light on the general problems of evolution.
Experimental Embryology.—A more fertile field, developed at the same
period and a little later, was found in experimental embryology. The
discoveries made by Driesch and others in shaking apart the cells of the
dividing egg or by destroying one or more of these cells gave a new insight
into the potency of cells for compensatory and regenerative processes.
These studies attracted many able investigators, who made still further
advance by subjecting the germ cells, developing eggs, embryos, and
developing organs to a great variety of artificial conditions.
Artificial Parthenogenesis.—Another question concerns the nature of the
process of fertilization and the agencies which cause the fertilized egg to
develop into an embryo. In 1899 Jacques Loeb succeeded in causing
development in unfertilized sea-urchin eggs by subjecting them to
concentrated sea water for a period and then returning them to their normal
environment. To this promising field of experimental work came many of
the foremost biologists both in America and Europe. It was soon found that
Comparative Anatomy.—Upon the foundations laid down by Cuvier a
century ago the present elaborate structure of comparative anatomy of
animals, both vertebrate and invertebrate, has been developed. Vast as is the
present accumulation of facts and theories many important problems still
await their solution. Jeffries Wyman was long a leader in this field, where
many workers are now engaged.
Embryology.—The embryological studies, so brilliantly begun by Von
Baer early in the nineteenth century, are still in progress. They have now
been extended to the groups more difficult of investigation and into the
earliest stages of fertilization and implantation in the mammals. Artificial
cultural methods have yielded important results. Louis and Alexander
Agassiz, Mark, Minot, Brooks, Whitman, Conklin and E. B. Wilson have
taken prominent parts in this work.
In the early nineties embryological studies were directed to the
arrangement of cells in the dividing egg, and there was much discussion of
“cell lineage” in development. Valuable as were these studies they threw
comparatively little light on the general problems of evolution.
Experimental Embryology.—A more fertile field, developed at the same
period and a little later, was found in experimental embryology. The
discoveries made by Driesch and others in shaking apart the cells of the
dividing egg or by destroying one or more of these cells gave a new insight
into the potency of cells for compensatory and regenerative processes.
These studies attracted many able investigators, who made still further
advance by subjecting the germ cells, developing eggs, embryos, and
developing organs to a great variety of artificial conditions.
Artificial Parthenogenesis.—Another question concerns the nature of the
process of fertilization and the agencies which cause the fertilized egg to
develop into an embryo. In 1899 Jacques Loeb succeeded in causing
development in unfertilized sea-urchin eggs by subjecting them to
concentrated sea water for a period and then returning them to their normal
environment. To this promising field of experimental work came many of
the foremost biologists both in America and Europe. It was soon found that
Page 462
the eggs of most groups of animals except the higher vertebrates could be
made to develop into more or less perfect embryos and larval forms by
treatment with a great variety of chemical substances, by increased
temperature, by mechanical stimuli and by other means. This artificial
parthenogenesis, as it is called, has also been successful in plants (Fucus),
and recently Loeb has reared several frogs to sexual maturity by merely
puncturing with a sharp needle the eggs from which they were derived.
Loeb, then, maintains that “the egg is the future embryo and animal; and
that the spermatozoon, aside from its activating effect, only transmits
Mendelian characters to the egg.”[180]
Further experimental analyses of the nature of the fertilization
mechanism have recently been made by Morgan, Conklin, F. R. Lillie, and
others.
Germinal Localization.—The question as to whether the egg contains
localized organ-forming substances has been studied experimentally
particularly by means of the centrifuge. The results indicate that neither of
the older opposing theories of “performation” or “epigenesis” is applicable
to all eggs, but that in certain organisms the eggs possess a well marked
differentiation while in others each part of the egg is essentially, although
probably not absolutely, equipotential.
The Germplasm Cycle.—Since Weismann’s postulation of the
independence of soma and germplasm in 1885 many attempts have been
made to trace the path of the hereditary substance from one generation to
the next. A recent book by Hegner[181] summarizes the success attained in
various groups of animals.
made to develop into more or less perfect embryos and larval forms by
treatment with a great variety of chemical substances, by increased
temperature, by mechanical stimuli and by other means. This artificial
parthenogenesis, as it is called, has also been successful in plants (Fucus),
and recently Loeb has reared several frogs to sexual maturity by merely
puncturing with a sharp needle the eggs from which they were derived.
Loeb, then, maintains that “the egg is the future embryo and animal; and
that the spermatozoon, aside from its activating effect, only transmits
Mendelian characters to the egg.”[180]
Further experimental analyses of the nature of the fertilization
mechanism have recently been made by Morgan, Conklin, F. R. Lillie, and
others.
Germinal Localization.—The question as to whether the egg contains
localized organ-forming substances has been studied experimentally
particularly by means of the centrifuge. The results indicate that neither of
the older opposing theories of “performation” or “epigenesis” is applicable
to all eggs, but that in certain organisms the eggs possess a well marked
differentiation while in others each part of the egg is essentially, although
probably not absolutely, equipotential.
The Germplasm Cycle.—Since Weismann’s postulation of the
independence of soma and germplasm in 1885 many attempts have been
made to trace the path of the hereditary substance from one generation to
the next. A recent book by Hegner[181] summarizes the success attained in
various groups of animals.
Page 463
Cytology.
Another important field of investigation which has attracted many
workers is that which pertains to the life of the cell—the science of
cytology. Although the celltheory was established as early as 1839, little
advance was made in this subject in America before 1880. Since that time,
however, Americans have been so successful in cytological discoveries that
they are now among the world’s leaders in this field.
These studies have been followed along both descriptive and
experimental lines. The most prominent of the early workers in this field are
E. L. Mark and E. B. Wilson. Mark’s description of the maturation,
fecundation, and segmentation of the egg is the most accurate and complete
of the early cytological studies. Wilson’s discoveries concerning the details
of fertilization and his “Atlas of Fertilization and Karyokinesis,” published
in 1895, have now become classic. Wilson, too, has published the only
American text-book on cytology,[182] and has more recently taken the lead in
studies concerning the relation between the chromosomes and sex. Besides
Wilson, Montgomery, Mark, McClung, Morgan, Miss Stevens, Conklin and
their associates and students have now furnished conclusive evidence that
the sex of an organism is determined by, or associated with, the nuclear
constitution of the fertilized egg. This constitution is moreover shown to be
dependent upon the chromosomes received from the germ cells.
This explanation is in strict accordance with the results of experimental
breeding. It is also quite in harmony with the Mendelian law of inheritance,
and in fact forms one of the strongest supports for the view that all
Mendelian factors are resident in the chromosomes. Recent work has also
discovered the mechanism which governs the complicated conditions of sex
which occur in those animals which exhibit alternating sexual and
parthenogenetic generations. These remarkable processes are in all cases
found to depend upon a definite distribution of the chromosomes.
Other recent experimental work has shown that while the sex is thus
normally determined in the fertilized egg, it is in some animals not
irrevocably fixed, and the normal effect of the sex chromosomes may be
Another important field of investigation which has attracted many
workers is that which pertains to the life of the cell—the science of
cytology. Although the celltheory was established as early as 1839, little
advance was made in this subject in America before 1880. Since that time,
however, Americans have been so successful in cytological discoveries that
they are now among the world’s leaders in this field.
These studies have been followed along both descriptive and
experimental lines. The most prominent of the early workers in this field are
E. L. Mark and E. B. Wilson. Mark’s description of the maturation,
fecundation, and segmentation of the egg is the most accurate and complete
of the early cytological studies. Wilson’s discoveries concerning the details
of fertilization and his “Atlas of Fertilization and Karyokinesis,” published
in 1895, have now become classic. Wilson, too, has published the only
American text-book on cytology,[182] and has more recently taken the lead in
studies concerning the relation between the chromosomes and sex. Besides
Wilson, Montgomery, Mark, McClung, Morgan, Miss Stevens, Conklin and
their associates and students have now furnished conclusive evidence that
the sex of an organism is determined by, or associated with, the nuclear
constitution of the fertilized egg. This constitution is moreover shown to be
dependent upon the chromosomes received from the germ cells.
This explanation is in strict accordance with the results of experimental
breeding. It is also quite in harmony with the Mendelian law of inheritance,
and in fact forms one of the strongest supports for the view that all
Mendelian factors are resident in the chromosomes. Recent work has also
discovered the mechanism which governs the complicated conditions of sex
which occur in those animals which exhibit alternating sexual and
parthenogenetic generations. These remarkable processes are in all cases
found to depend upon a definite distribution of the chromosomes.
Other recent experimental work has shown that while the sex is thus
normally determined in the fertilized egg, it is in some animals not
irrevocably fixed, and the normal effect of the sex chromosomes may be
Page 464
inhibited by abnormal conditions in the developing embryo, as is
demonstrated by the recent work of Lillie and others.
The cytological basis for Mendelian inheritance has been very
extensively studied by Morgan and his pupils in connection with their work
on inheritance in the common fruit fly Drosophila. The evidence supports
Weismann’s earlier hypothesis that the chromosomes are the bearers of the
heritable factors, and that these are arranged in a series in the different
chromosomes. This theory is shown to be in such strict accord with both the
cytological studies and the results of experimental breeding that Morgan has
ventured to indicate definite points in particular chromosomes as the loci of
definite heritable factors, or genes.
Confirmation of this view is furnished by the behavior of the so-called
sex-linked characters, the genes for which are situated in the same
chromosome as that which carries the sex factor. Many ingenious breeding
experiments indicate further that all the hereditary characters in Drosophila
are borne in four great linkage groups corresponding with the four pairs of
chromosomes which the cells of this fly possess.
demonstrated by the recent work of Lillie and others.
The cytological basis for Mendelian inheritance has been very
extensively studied by Morgan and his pupils in connection with their work
on inheritance in the common fruit fly Drosophila. The evidence supports
Weismann’s earlier hypothesis that the chromosomes are the bearers of the
heritable factors, and that these are arranged in a series in the different
chromosomes. This theory is shown to be in such strict accord with both the
cytological studies and the results of experimental breeding that Morgan has
ventured to indicate definite points in particular chromosomes as the loci of
definite heritable factors, or genes.
Confirmation of this view is furnished by the behavior of the so-called
sex-linked characters, the genes for which are situated in the same
chromosome as that which carries the sex factor. Many ingenious breeding
experiments indicate further that all the hereditary characters in Drosophila
are borne in four great linkage groups corresponding with the four pairs of
chromosomes which the cells of this fly possess.
Page 465
Comparative Physiology.
None of the experimental fields has been of greater importance in
zoological progress than that which concerns the functions of the various
organs. Without this companion science morphology and comparative
anatomy would have become unintelligible. American investigators, among
whom G. H. Parker stands prominent, have taken a leading part in this field
also.
Neurology.—The physiological analysis of the components of the
nervous system, both in vertebrates and invertebrates, is another important
branch of experimental biology. The 28 volumes of the Journal of
Comparative Neurology attest the large influence that American
investigators have had in the development of this science.
Regeneration.—Experimental studies on the powers of regeneration in
plants and animals have been made from the earliest times. During the past
few years, however, there has been made a concerted attempt to analyze the
factors which determine the amount and rate of regeneration. Much
progress has been made toward the postulation of definite laws applicable
to the regenerative processes of the parts of each organism. The critical
analyses of Morgan, Loeb and Child have been particularly stimulating.
Tissue Culture.—Another line of experimental work which has been
developed within the past few years by Harrison, Carrell, and others is the
culture of body tissues in artificial media. These experiments have included
the cultivation in tubes or on glass slides of the various tissues of numerous
species of animals. They have yielded much information regarding the
structure, growth and multiplication of cells, the formation of tissues, and
the healing of wounds.
Transplantation and Grafting.—Closely associated experiments consist
in the transplantation of organs or other portions of the body to abnormal
positions, to the bodies of other animals of the same species or of other
species. In this way much has been learned about the potentiality of organs
for self-differentiation, for regulation, for regeneration and for
compensatory adaptations. The experiments have shown, further, the
None of the experimental fields has been of greater importance in
zoological progress than that which concerns the functions of the various
organs. Without this companion science morphology and comparative
anatomy would have become unintelligible. American investigators, among
whom G. H. Parker stands prominent, have taken a leading part in this field
also.
Neurology.—The physiological analysis of the components of the
nervous system, both in vertebrates and invertebrates, is another important
branch of experimental biology. The 28 volumes of the Journal of
Comparative Neurology attest the large influence that American
investigators have had in the development of this science.
Regeneration.—Experimental studies on the powers of regeneration in
plants and animals have been made from the earliest times. During the past
few years, however, there has been made a concerted attempt to analyze the
factors which determine the amount and rate of regeneration. Much
progress has been made toward the postulation of definite laws applicable
to the regenerative processes of the parts of each organism. The critical
analyses of Morgan, Loeb and Child have been particularly stimulating.
Tissue Culture.—Another line of experimental work which has been
developed within the past few years by Harrison, Carrell, and others is the
culture of body tissues in artificial media. These experiments have included
the cultivation in tubes or on glass slides of the various tissues of numerous
species of animals. They have yielded much information regarding the
structure, growth and multiplication of cells, the formation of tissues, and
the healing of wounds.
Transplantation and Grafting.—Closely associated experiments consist
in the transplantation of organs or other portions of the body to abnormal
positions, to the bodies of other animals of the same species or of other
species. In this way much has been learned about the potentiality of organs
for self-differentiation, for regulation, for regeneration and for
compensatory adaptations. The experiments have shown, further, the
Page 466
independence of soma and germplasm and have revealed the nature of
certain organs whose functions were previously obscure.
Tropisms and Instincts.—Another field of experimental biology concerns
the analysis of behavior of organisms in response to various forms of
stimuli. These studies are being prosecuted on all groups of organisms,
including the larval stages of many animals, and are yielding most
remarkable results. The success in this field of research is largely due to
stimulating influence of Jacques Loeb, Parker, Jennings, and their co-
workers.
Biological Chemistry.—Still another experimental field which has
developed into one of the most important of the biological sciences relates
to the fundamental chemical and physical changes which underlie all
organic phenomena. A knowledge of both physiological and physical
chemistry is to-day essential for all advanced biological work. The peculiar
nature of life itself, of growth, disease, old-age, degeneration, death and
dissolution are presumably only manifestations of chemical and physical
laws. The ultimate goal of all experimental biology, therefore, will be
reached only when the basic physico-chemical properties of life are
understood. At that time only will the perennial controversy between
vitalism and mechanism be ended.
certain organs whose functions were previously obscure.
Tropisms and Instincts.—Another field of experimental biology concerns
the analysis of behavior of organisms in response to various forms of
stimuli. These studies are being prosecuted on all groups of organisms,
including the larval stages of many animals, and are yielding most
remarkable results. The success in this field of research is largely due to
stimulating influence of Jacques Loeb, Parker, Jennings, and their co-
workers.
Biological Chemistry.—Still another experimental field which has
developed into one of the most important of the biological sciences relates
to the fundamental chemical and physical changes which underlie all
organic phenomena. A knowledge of both physiological and physical
chemistry is to-day essential for all advanced biological work. The peculiar
nature of life itself, of growth, disease, old-age, degeneration, death and
dissolution are presumably only manifestations of chemical and physical
laws. The ultimate goal of all experimental biology, therefore, will be
reached only when the basic physico-chemical properties of life are
understood. At that time only will the perennial controversy between
vitalism and mechanism be ended.
Page 467
Economic Zoology.
A moment’s reflection will show that economic biology is the most
essential of all sciences to the human welfare and progress. For man’s
relation to his environment is such that the penalty for ignorance or neglect
of the biological principles involved in the struggle for existence quickly
overwhelms him with a horde of parasites or other enemies.
It is only by the intelligent application of biological knowledge that our
food supplies, our forests, our domesticated animals and our bodies can be
protected from the ever ravenous organisms which surround us.
The losses to food supplies and other products by insects alone amounts
to 100 millions of dollars a month in the United States. And the parasites
cause losses in sickness and premature deaths each year of many millions
more. Then there are the destructive rodents and other animals which add
largely to our burdens of support. These enemies next to wars and fungi are
the most destructive agencies on earth. Could they but be eliminated man’s
struggle against opposing forces would be in large measure overcome. The
results of recent work in economic zoology, both in regard to the
destruction of enemies and protection of useful mammals, birds and fishes,
furnish a bright outlook for the future.
Protozoology.—Partly as an experimental field for the solution of general
biological problems and partly because of its practical applications the
study of protozoa has now developed into a special science.
The results of the investigations of Calkins, Woodruff, Jennings and
others have greatly supplemented our understanding of the signification of
such important biological phenomena as reproduction, sexual
differentiation, conjugation, tropisms, and metabolism.
From an economic standpoint the protozoa have recently been shown to
be of the greatest importance because of the human and animal diseases for
which they are responsible.
Parasitology.—The animal parasites of man, domesticated animals and
plants include numerous species of protozoa, worms, and insects. Together
with the bacteria and a few higher fungi they cause all communicable
diseases. When we consider that not only our health but also our entire food
A moment’s reflection will show that economic biology is the most
essential of all sciences to the human welfare and progress. For man’s
relation to his environment is such that the penalty for ignorance or neglect
of the biological principles involved in the struggle for existence quickly
overwhelms him with a horde of parasites or other enemies.
It is only by the intelligent application of biological knowledge that our
food supplies, our forests, our domesticated animals and our bodies can be
protected from the ever ravenous organisms which surround us.
The losses to food supplies and other products by insects alone amounts
to 100 millions of dollars a month in the United States. And the parasites
cause losses in sickness and premature deaths each year of many millions
more. Then there are the destructive rodents and other animals which add
largely to our burdens of support. These enemies next to wars and fungi are
the most destructive agencies on earth. Could they but be eliminated man’s
struggle against opposing forces would be in large measure overcome. The
results of recent work in economic zoology, both in regard to the
destruction of enemies and protection of useful mammals, birds and fishes,
furnish a bright outlook for the future.
Protozoology.—Partly as an experimental field for the solution of general
biological problems and partly because of its practical applications the
study of protozoa has now developed into a special science.
The results of the investigations of Calkins, Woodruff, Jennings and
others have greatly supplemented our understanding of the signification of
such important biological phenomena as reproduction, sexual
differentiation, conjugation, tropisms, and metabolism.
From an economic standpoint the protozoa have recently been shown to
be of the greatest importance because of the human and animal diseases for
which they are responsible.
Parasitology.—The animal parasites of man, domesticated animals and
plants include numerous species of protozoa, worms, and insects. Together
with the bacteria and a few higher fungi they cause all communicable
diseases. When we consider that not only our health but also our entire food
Page 468
supply is dependent upon the elimination of these organisms we must admit
that parasitology is the most important economically of all the sciences.
The reports of the investigations of Stiles and his associates in the
Hygienic Laboratory and of Ransom and his staff in the Bureau of Animal
Industry are widely distributed by the federal government. The systematic
studies so ably begun by Joseph Leidy in the middle of the last century have
been continued by Ward, Linton, Pratt, Curtis and others on the parasites of
many groups of animals.
Economic Entomology.—Another extremely important biological
science, the practical applications of which are second only to those of
parasitology in importance, is entomology. In the last few years economic
entomology has exceeded any of the other branches of biology in the
number of its investigators. The American Association of Economic
Entomologists has a membership of about five hundred. The work of most
of these is supported by appropriations from the State and federal
governments, and the results of their investigations are widely published.
It is now well known that some of the protozoon parasites are conveyed
from man to man only through the bites of insects. The local eradication of
several of our most fatal diseases has recently been brought about by the
application of measures to destroy such insects. This is the greatest triumph
of economic zoology.
Economic Ichthyology.—The U. S. Fish Commission has for many years
been actively engaged in investigations on the food fishes, including
methods for increasing the food supply by suitable protection and artificial
propagation. The work includes also edible and otherwise useful mollusks
and crustacea. Their marine and fresh-water laboratories have also been of
great service to general biological science.
Economic Ornithology and Mammalogy.—In addition to the local bird
clubs and the American Ornithologists Union for the study and preservation
of bird and mammal life, the Bureau of Biological Survey has for some
years conducted investigations on the economic importance of the various
species. The publications of this Bureau are of great value both in
determining the economic status of our birds and mammals, and also in
recommending means for the protection of the beneficial species and the
destruction of the injurious. Several of the States issue similar publications.
that parasitology is the most important economically of all the sciences.
The reports of the investigations of Stiles and his associates in the
Hygienic Laboratory and of Ransom and his staff in the Bureau of Animal
Industry are widely distributed by the federal government. The systematic
studies so ably begun by Joseph Leidy in the middle of the last century have
been continued by Ward, Linton, Pratt, Curtis and others on the parasites of
many groups of animals.
Economic Entomology.—Another extremely important biological
science, the practical applications of which are second only to those of
parasitology in importance, is entomology. In the last few years economic
entomology has exceeded any of the other branches of biology in the
number of its investigators. The American Association of Economic
Entomologists has a membership of about five hundred. The work of most
of these is supported by appropriations from the State and federal
governments, and the results of their investigations are widely published.
It is now well known that some of the protozoon parasites are conveyed
from man to man only through the bites of insects. The local eradication of
several of our most fatal diseases has recently been brought about by the
application of measures to destroy such insects. This is the greatest triumph
of economic zoology.
Economic Ichthyology.—The U. S. Fish Commission has for many years
been actively engaged in investigations on the food fishes, including
methods for increasing the food supply by suitable protection and artificial
propagation. The work includes also edible and otherwise useful mollusks
and crustacea. Their marine and fresh-water laboratories have also been of
great service to general biological science.
Economic Ornithology and Mammalogy.—In addition to the local bird
clubs and the American Ornithologists Union for the study and preservation
of bird and mammal life, the Bureau of Biological Survey has for some
years conducted investigations on the economic importance of the various
species. The publications of this Bureau are of great value both in
determining the economic status of our birds and mammals, and also in
recommending means for the protection of the beneficial species and the
destruction of the injurious. Several of the States issue similar publications.
Page 469
Genetics.
One of the most interesting chapters in biology relates to the
development of the modern science of heredity, or genetics.
Previous to the year 1900, when the Mendelian principle of inheritance
was re-discovered, the relative importance of heredity and of environment
in the development of an organism was little understood. It is true that
Weismann had insisted on the independence of soma and germplasm some
years earlier (1883), but the body of the individual was still generally
considered the key to its inheritance.
The recognition of the general application of Mendel’s discovery gave a
great impetus to experimental breeding both in plants and animals. While
heretofore it had been necessary to depend upon the somatic characters as
evidence of the hereditary constitution of an individual, it now became
possible, knowing the hereditary constitution of the parents of any pair of
individuals, to predict with almost mathematical certainty the characters of
their possible offspring.
In general, the laws of possible chance combinations of any group of
characters determine the probability of any particular offspring possessing
one or many of those characters. The physical basis for such Mendelian
inheritance is evidently the chance combinations of chromosomes which
result from the processes of maturation and union of the germ cells.
Certain limitations to the law are met with because the relatively small
number of chromosomes involves linkage of genes, because of the
occasional interchange of groups of genes between homologous
chromosomes, and because the relative activity or potency of any particular
gene may differ in different races, and, finally, because the normal activity
of any given gene may be modified or inhibited by the action of other
genes. It is by no means certain, however, that all inheritance is Mendelian,
for there still remains much evidence that the hereditary basis of certain
characters may be resident in the cytoplasm, rather than in the
chromosomes. A recent book by Morgan, Sturtevant, Müller and Bridges
(1915), entitled “the mechanism of Mendelian heredity” gives the
cytological explanation of Mendelian inheritance.
One of the most interesting chapters in biology relates to the
development of the modern science of heredity, or genetics.
Previous to the year 1900, when the Mendelian principle of inheritance
was re-discovered, the relative importance of heredity and of environment
in the development of an organism was little understood. It is true that
Weismann had insisted on the independence of soma and germplasm some
years earlier (1883), but the body of the individual was still generally
considered the key to its inheritance.
The recognition of the general application of Mendel’s discovery gave a
great impetus to experimental breeding both in plants and animals. While
heretofore it had been necessary to depend upon the somatic characters as
evidence of the hereditary constitution of an individual, it now became
possible, knowing the hereditary constitution of the parents of any pair of
individuals, to predict with almost mathematical certainty the characters of
their possible offspring.
In general, the laws of possible chance combinations of any group of
characters determine the probability of any particular offspring possessing
one or many of those characters. The physical basis for such Mendelian
inheritance is evidently the chance combinations of chromosomes which
result from the processes of maturation and union of the germ cells.
Certain limitations to the law are met with because the relatively small
number of chromosomes involves linkage of genes, because of the
occasional interchange of groups of genes between homologous
chromosomes, and because the relative activity or potency of any particular
gene may differ in different races, and, finally, because the normal activity
of any given gene may be modified or inhibited by the action of other
genes. It is by no means certain, however, that all inheritance is Mendelian,
for there still remains much evidence that the hereditary basis of certain
characters may be resident in the cytoplasm, rather than in the
chromosomes. A recent book by Morgan, Sturtevant, Müller and Bridges
(1915), entitled “the mechanism of Mendelian heredity” gives the
cytological explanation of Mendelian inheritance.
Page 470
Americans have from the first taken a leading part in this field of
research and have been quick to recognize its practical applications to the
improvement of breeds in both animals and plants. This prominent position
is largely due to the experimental work of Castle, Davenport, Morgan,
Jennings, Pearl, and their co-workers on animals and that of East, Emerson,
Davis, Hayes and Shull on plants.
The geneticist now realizes that the appearance of the body (phenotype)
gives but little clue to the inheritance (genotype). That two white flowers
produce only purple offspring, or two white fowls only deeply colored
chickens, or that a pair of guinea pigs, one of which is black and the other
white, have only gray agouti offspring, while other apparently similar white
flowers or white animals produce offspring like themselves, is now readily
comprehensible and mathematically predictable.
The most important application of our newly acquired knowledge of
inheritance is in the improvement of the human race. The wonderful
opportunity in this direction must be apparent to all. The welfare of
humanity depends upon the immediate adoption of eugenic principles. The
Eugenics Record Office has secured many of the essential data.
With the destruction of the world’s best germ plasm at a rate never
equalled before, the outlook for the future race would be appalling were it
not for the hope that with the advent of a righteous peace will come a
realization of the necessity of applying these new biological discoveries to
improving the races of men. That the discoveries have been made too late in
the world’s history to be of such use to humanity must not be thought
possible.
research and have been quick to recognize its practical applications to the
improvement of breeds in both animals and plants. This prominent position
is largely due to the experimental work of Castle, Davenport, Morgan,
Jennings, Pearl, and their co-workers on animals and that of East, Emerson,
Davis, Hayes and Shull on plants.
The geneticist now realizes that the appearance of the body (phenotype)
gives but little clue to the inheritance (genotype). That two white flowers
produce only purple offspring, or two white fowls only deeply colored
chickens, or that a pair of guinea pigs, one of which is black and the other
white, have only gray agouti offspring, while other apparently similar white
flowers or white animals produce offspring like themselves, is now readily
comprehensible and mathematically predictable.
The most important application of our newly acquired knowledge of
inheritance is in the improvement of the human race. The wonderful
opportunity in this direction must be apparent to all. The welfare of
humanity depends upon the immediate adoption of eugenic principles. The
Eugenics Record Office has secured many of the essential data.
With the destruction of the world’s best germ plasm at a rate never
equalled before, the outlook for the future race would be appalling were it
not for the hope that with the advent of a righteous peace will come a
realization of the necessity of applying these new biological discoveries to
improving the races of men. That the discoveries have been made too late in
the world’s history to be of such use to humanity must not be thought
possible.
Page 471
Evolution.
Previous to the publication of Darwin’s “Origin of Species” in 1859,
American zoologists were generally inclined toward special creation, in
spite of the evidences for evolution which had been presented by Erasmus
Darwin, Buffon, Lamarck, and Geoffroy St.-Hilaire. This attitude of mind
continued for some years after the publication of the natural selection
theory of Darwin and Wallace. This was in part due to the powerful
influence of Louis Agassiz and others who bitterly opposed the Darwinian
theory. The influence of Asa Gray in gaining a general acceptance for this
theory is explained in the following chapter.
A modified Lamarckian doctrine was widely accepted in the last quarter
of the century, due largely to the influence of Cope, Hyatt and Packard. The
inheritance of “acquired characters” demanded by this theory seems
incompatible with the discoveries of recent times, so that “to-day the theory
has few followers amongst trained investigators, but it still has a popular
vogue that is wide-spread and vociferous.”[183]
The origin of new varieties and species by accidental and fortuitous
modifications (mutations) of the germplasm is now the most widely
accepted theory of evolution.
Some of the most important discoveries regarding the origin of new
forms have been recently made by Morgan and his pupils. From a stock of
the common fruit fly (Drosophila ampelophila) more than 125 new types
have arisen within six years. Each of these types breeds true. “Each has
arisen independently and suddenly. Every part of the body has been affected
by one or another of these mutations.” To arrange these mutations
arbitrarily into graded series would give the impression of an evolutionary
series, but this is directly contrary to the known facts concerning their
origin, for each mutation “originated independently from the wild type.”
“Evolution has taken place by the incorporation into the race of those
mutations that are beneficial to the life and reproduction of the individual.”
This evolutionary process is usually accompanied by the elimination of
those forms which have remained stable or which have developed adverse
mutations.
Previous to the publication of Darwin’s “Origin of Species” in 1859,
American zoologists were generally inclined toward special creation, in
spite of the evidences for evolution which had been presented by Erasmus
Darwin, Buffon, Lamarck, and Geoffroy St.-Hilaire. This attitude of mind
continued for some years after the publication of the natural selection
theory of Darwin and Wallace. This was in part due to the powerful
influence of Louis Agassiz and others who bitterly opposed the Darwinian
theory. The influence of Asa Gray in gaining a general acceptance for this
theory is explained in the following chapter.
A modified Lamarckian doctrine was widely accepted in the last quarter
of the century, due largely to the influence of Cope, Hyatt and Packard. The
inheritance of “acquired characters” demanded by this theory seems
incompatible with the discoveries of recent times, so that “to-day the theory
has few followers amongst trained investigators, but it still has a popular
vogue that is wide-spread and vociferous.”[183]
The origin of new varieties and species by accidental and fortuitous
modifications (mutations) of the germplasm is now the most widely
accepted theory of evolution.
Some of the most important discoveries regarding the origin of new
forms have been recently made by Morgan and his pupils. From a stock of
the common fruit fly (Drosophila ampelophila) more than 125 new types
have arisen within six years. Each of these types breeds true. “Each has
arisen independently and suddenly. Every part of the body has been affected
by one or another of these mutations.” To arrange these mutations
arbitrarily into graded series would give the impression of an evolutionary
series, but this is directly contrary to the known facts concerning their
origin, for each mutation “originated independently from the wild type.”
“Evolution has taken place by the incorporation into the race of those
mutations that are beneficial to the life and reproduction of the individual.”
This evolutionary process is usually accompanied by the elimination of
those forms which have remained stable or which have developed adverse
mutations.
Page 472
A question that is being vigorously debated at this time concerns the
possible effects of selection on the hereditary factors. Are the genes fixed
both qualitatively and quantitatively or does a given gene vary in potency
under different conditions and in different individuals? In the former case
selection can only separate the existing genes into separate pure strains. But
if the gene be quantitatively variable, then selection will result in the
establishment of new types.
Castle has long stoutly maintained the effect of such selection, and his
forces have recently been augmented by Jennings. The experimental work
now in process will doubtless yield a decisive answer.
possible effects of selection on the hereditary factors. Are the genes fixed
both qualitatively and quantitatively or does a given gene vary in potency
under different conditions and in different individuals? In the former case
selection can only separate the existing genes into separate pure strains. But
if the gene be quantitatively variable, then selection will result in the
establishment of new types.
Castle has long stoutly maintained the effect of such selection, and his
forces have recently been augmented by Jennings. The experimental work
now in process will doubtless yield a decisive answer.
Page 473
Conclusion.
A comparison of the simple descriptive natural history of a century ago
with the foregoing manifold developments of modern biology will indicate
the wonderful progress which has occurred during this period. The path has
led from the crude methods of the almost unaided eye and hand to the
applications of the most delicate experimental apparatus. For the marvelous
success which zoology has attained has been possible only by the skillful
use of scalpel, microscope, microtome and other mechanical devices and by
the refined methods of the chemist and physicist.
The central truth to which all these discoveries consistently point is the
unity and harmony of all biological phenomena, and indeed of all nature.
No longer does the zoologist find any demarcated line separating his field
of research from that of the botanist or the chemist or even of the physicist,
for all the natural sciences obviously deal with closely associated
phenomena. The aim of the future will be both to complete fields of study
already marked out and to derive a comprehensive explanation of the
general principles involved.
A comparison of the simple descriptive natural history of a century ago
with the foregoing manifold developments of modern biology will indicate
the wonderful progress which has occurred during this period. The path has
led from the crude methods of the almost unaided eye and hand to the
applications of the most delicate experimental apparatus. For the marvelous
success which zoology has attained has been possible only by the skillful
use of scalpel, microscope, microtome and other mechanical devices and by
the refined methods of the chemist and physicist.
The central truth to which all these discoveries consistently point is the
unity and harmony of all biological phenomena, and indeed of all nature.
No longer does the zoologist find any demarcated line separating his field
of research from that of the botanist or the chemist or even of the physicist,
for all the natural sciences obviously deal with closely associated
phenomena. The aim of the future will be both to complete fields of study
already marked out and to derive a comprehensive explanation of the
general principles involved.
Page 474
Notes.
172. Proc. Biol. Soc. Washington, 3, 35, 1886.
173. Ibid., 4, 9, 1888. Both of these papers are reprinted in Ann. Rept. Smithsonian Inst., 1897,
U. S. Nat. Mus., Pt. 2, pp. 357–466, 1901.
174. Louis Agassiz: his Life and Correspondence, by Elizabeth Carey Agassiz, p. 145, 1885.
175. List of North American Land Mammals in the United States National Museum, 1911. Bull.
79, U. S. Nat. Mus., 1912.
176. Birds of North and Middle America, Bull. 50, parts I-VII, U. S. Nat. Mus., 1901–1916.
177. Report U. S. Nat. Mus. for 1898, pp. 153–1270, 1900.
178. Bull. 34, U. S. Nat. Mus., 1889.
179. Bull. 47, parts I-IV, U. S. Nat. Mus., 1896–1900.
180. J. Loeb, The Organism as a Whole, p. 126, 1916.
181. The Germ-cell Cycle in Animals, 1914.
182. The Cell in Development and Inheritance, 1896; second edition, 1900.
183. Morgan, T. H. A critique of the theory of evolution, p. 32, 1916.
172. Proc. Biol. Soc. Washington, 3, 35, 1886.
173. Ibid., 4, 9, 1888. Both of these papers are reprinted in Ann. Rept. Smithsonian Inst., 1897,
U. S. Nat. Mus., Pt. 2, pp. 357–466, 1901.
174. Louis Agassiz: his Life and Correspondence, by Elizabeth Carey Agassiz, p. 145, 1885.
175. List of North American Land Mammals in the United States National Museum, 1911. Bull.
79, U. S. Nat. Mus., 1912.
176. Birds of North and Middle America, Bull. 50, parts I-VII, U. S. Nat. Mus., 1901–1916.
177. Report U. S. Nat. Mus. for 1898, pp. 153–1270, 1900.
178. Bull. 34, U. S. Nat. Mus., 1889.
179. Bull. 47, parts I-IV, U. S. Nat. Mus., 1896–1900.
180. J. Loeb, The Organism as a Whole, p. 126, 1916.
181. The Germ-cell Cycle in Animals, 1914.
182. The Cell in Development and Inheritance, 1896; second edition, 1900.
183. Morgan, T. H. A critique of the theory of evolution, p. 32, 1916.
Page 475
XIII
THE DEVELOPMENT OF BOTANY SINCE 1818
By GEORGE L. GOODALE
“Our Botany, it is true, has been extensively and successfully investigated, but this field is still
rich, and rewards every new research with some interesting discovery.”
Such are the words with which the sagacious and far-sighted founder of the
American Journal of Science and Arts, in his general introduction to the
first volume, alludes to the study of plants. It is plain that the editor,
embarking on this new enterprise, appreciated the attractions of this inviting
field and sympathetically recognized the good work which was being done
in it. It is not surprising, therefore, to find that he welcomed to the pages of
his initial number contributions to botany.
Early Botanical Works.—The collections of dried and living North
American plants, which had been carried from time to time to botanists in
Europe, had been eagerly studied, and the results had been published in
accessible treatises. Besides these general treatises, there had been issued
certain works, wholly devoted to the American Flora. Among these latter
may be mentioned Pursh’s “Flora” (1814) and Nuttall’s “Genera” (1818).
There were also a few works which were rather popular in their character,
such as Amos Eaton’s “Manual of Botany for North America” (1817), and
Bigelow’s “Collection of the Plants of Boston and environs” (1814). These
handbooks were convenient, and possessed the charm of not being
exhaustive; consequently a botanist, whether professional or amateur, was
stimulated to feel that he had a good chance of enriching the list of species
and adding to the next edition.
THE DEVELOPMENT OF BOTANY SINCE 1818
By GEORGE L. GOODALE
“Our Botany, it is true, has been extensively and successfully investigated, but this field is still
rich, and rewards every new research with some interesting discovery.”
Such are the words with which the sagacious and far-sighted founder of the
American Journal of Science and Arts, in his general introduction to the
first volume, alludes to the study of plants. It is plain that the editor,
embarking on this new enterprise, appreciated the attractions of this inviting
field and sympathetically recognized the good work which was being done
in it. It is not surprising, therefore, to find that he welcomed to the pages of
his initial number contributions to botany.
Early Botanical Works.—The collections of dried and living North
American plants, which had been carried from time to time to botanists in
Europe, had been eagerly studied, and the results had been published in
accessible treatises. Besides these general treatises, there had been issued
certain works, wholly devoted to the American Flora. Among these latter
may be mentioned Pursh’s “Flora” (1814) and Nuttall’s “Genera” (1818).
There were also a few works which were rather popular in their character,
such as Amos Eaton’s “Manual of Botany for North America” (1817), and
Bigelow’s “Collection of the Plants of Boston and environs” (1814). These
handbooks were convenient, and possessed the charm of not being
exhaustive; consequently a botanist, whether professional or amateur, was
stimulated to feel that he had a good chance of enriching the list of species
and adding to the next edition.
Page 476
Page 477
The Early Years of Botany in the Journal.
At that time, the botanists had no journal in this country devoted to their
science. Here and there they found opportunity for publishing their
discoveries in some medical periodical or in a local newspaper. Hence
American botanists availed themselves of the welcome extended by
Silliman to botanical contributors to place their results on record in a
magazine devoted to science in its wide sense. Specialization and
subdivision of science had not then begun to dissociate allied subjects, and,
consequently, botanists felt that they would be at home in this journal
conducted by a chemist. Botanists responded promptly to this invitation
with interesting contributions.
It is well to remember that the appliances at the command of naturalists
at the date when the Journal began its service, were imperfect and
inadequate. The botanist did not possess a convenient achromatic
microscope, and he was not in possession of the chemical aids now deemed
necessary in even the simplest research. Hence, attention was given almost
wholly to such matters as the forms of plants and the more obvious
phenomena of plant-life. In view of the poverty of instrumental aids in
research, the results attained must be regarded as surprising.
In the very first volume of the Journal, bearing the date of 1818, there are
descriptions of four new genera and of four new species of plants; certainly
a large share to give to systematic botany. Besides these articles, there are
some instructive notes concerning a few plants, which up to that time had
been imperfectly understood. There are four Floral Calendars which give
details in regard to the blossoming and the fruiting of plants in limited
districts, a botanical subject of some importance but likely to become
tedious in the long run. Just here, the skill of the editor in limiting
undesirable contributions is shown by his tactful remark designed to soothe
the feelings of a prolix writer whose too long list of plants in a floral
calendar he had editorially cut down to reasonable limits. The editor
remarks, “such extended observations are desirable, but it may not always
be convenient to insert very voluminous details of daily floral occurrence.”
It is convenient to consider by themselves some of the botanical
contributions published in the first series of volumes of the Journal during a
At that time, the botanists had no journal in this country devoted to their
science. Here and there they found opportunity for publishing their
discoveries in some medical periodical or in a local newspaper. Hence
American botanists availed themselves of the welcome extended by
Silliman to botanical contributors to place their results on record in a
magazine devoted to science in its wide sense. Specialization and
subdivision of science had not then begun to dissociate allied subjects, and,
consequently, botanists felt that they would be at home in this journal
conducted by a chemist. Botanists responded promptly to this invitation
with interesting contributions.
It is well to remember that the appliances at the command of naturalists
at the date when the Journal began its service, were imperfect and
inadequate. The botanist did not possess a convenient achromatic
microscope, and he was not in possession of the chemical aids now deemed
necessary in even the simplest research. Hence, attention was given almost
wholly to such matters as the forms of plants and the more obvious
phenomena of plant-life. In view of the poverty of instrumental aids in
research, the results attained must be regarded as surprising.
In the very first volume of the Journal, bearing the date of 1818, there are
descriptions of four new genera and of four new species of plants; certainly
a large share to give to systematic botany. Besides these articles, there are
some instructive notes concerning a few plants, which up to that time had
been imperfectly understood. There are four Floral Calendars which give
details in regard to the blossoming and the fruiting of plants in limited
districts, a botanical subject of some importance but likely to become
tedious in the long run. Just here, the skill of the editor in limiting
undesirable contributions is shown by his tactful remark designed to soothe
the feelings of a prolix writer whose too long list of plants in a floral
calendar he had editorially cut down to reasonable limits. The editor
remarks, “such extended observations are desirable, but it may not always
be convenient to insert very voluminous details of daily floral occurrence.”
It is convenient to consider by themselves some of the botanical
contributions published in the first series of volumes of the Journal during a
Page 478
period of twenty years, the period before Asa Gray became actively and
constantly associated with the Journal.
In systematic and geographical botany one finds communications from
Douglass and Torrey (4, 56, 1822) on the plants of what was then the
Northwest; Lewis C. Beck (10, 257, 1826; 11, 167, 1826; 14, 112, 1828)
contributed valuable papers on the botany of Illinois and Missouri; there is
a literal translation by Dr. Ruschenberger (19, 63, 299, 1831; 20, 248, 1831;
23, 78, 250, 1833) of a very long list of the plants of Chili; Wolle and
Huebener (37, 310, 1839) gave an annotated catalogue of botanical
specimens collected in Pennsylvania; Tuckerman (45, 27, 1843) presented
communications in regard to numerous species which he had examined
critically; Darlington (41, 365, 1841) published his lecture on grasses; Asa
Gray (40, 1, 1841) gave an instructive account of European herbaria visited
by him, and he contributed also a charming account (42, 1, 1842) of a
botanical journey to the mountains of North Carolina. The most extensive
series of botanical communication at this time was the Caricography by
Professor Dewey of Williams College, presented in many numbers of the
Journal; the first of these in 7, pp. 264–278, 1824. There were also
descriptions of certain new genera, and species, and critical studies in
synonyms.
Cryptogamic botany is represented in the first series of volumes of the
Journal by L. C. Beck’s (15, 287, 1829) study of ferns and mosses, by
Bailey’s (35, 113, 1839) histology of the vascular system of ferns, by Fries’
Systema mycologicum (12, 235, 1829), and by De Schweinitz (9, 397,
1825) and Halsey, who had in hand a cryptogamic manual. There are two
important papers by Alexander Braun, translated by Dr. George Engelmann,
one on the Equisetaceæ of North America (46, 81, 1844) and the other on
the Characeæ (46, 92, 1844).
Vegetable paleontology had begun to attract attention in many places in
this country, and therefore the translated contributions by Brongniart on
fossil plants were given space in the Journal. Plant-physiology received a
good share of attention either in short notices or in longer articles. Such
titles appear as, the respiration of plants, the circulation of sap, the
excrementitious matter thrown off by plants, the effects of certain gases and
poisons on plants, and the relations of plants to different colored light. One
of the most important of the notes is that in which is described the
constantly associated with the Journal.
In systematic and geographical botany one finds communications from
Douglass and Torrey (4, 56, 1822) on the plants of what was then the
Northwest; Lewis C. Beck (10, 257, 1826; 11, 167, 1826; 14, 112, 1828)
contributed valuable papers on the botany of Illinois and Missouri; there is
a literal translation by Dr. Ruschenberger (19, 63, 299, 1831; 20, 248, 1831;
23, 78, 250, 1833) of a very long list of the plants of Chili; Wolle and
Huebener (37, 310, 1839) gave an annotated catalogue of botanical
specimens collected in Pennsylvania; Tuckerman (45, 27, 1843) presented
communications in regard to numerous species which he had examined
critically; Darlington (41, 365, 1841) published his lecture on grasses; Asa
Gray (40, 1, 1841) gave an instructive account of European herbaria visited
by him, and he contributed also a charming account (42, 1, 1842) of a
botanical journey to the mountains of North Carolina. The most extensive
series of botanical communication at this time was the Caricography by
Professor Dewey of Williams College, presented in many numbers of the
Journal; the first of these in 7, pp. 264–278, 1824. There were also
descriptions of certain new genera, and species, and critical studies in
synonyms.
Cryptogamic botany is represented in the first series of volumes of the
Journal by L. C. Beck’s (15, 287, 1829) study of ferns and mosses, by
Bailey’s (35, 113, 1839) histology of the vascular system of ferns, by Fries’
Systema mycologicum (12, 235, 1829), and by De Schweinitz (9, 397,
1825) and Halsey, who had in hand a cryptogamic manual. There are two
important papers by Alexander Braun, translated by Dr. George Engelmann,
one on the Equisetaceæ of North America (46, 81, 1844) and the other on
the Characeæ (46, 92, 1844).
Vegetable paleontology had begun to attract attention in many places in
this country, and therefore the translated contributions by Brongniart on
fossil plants were given space in the Journal. Plant-physiology received a
good share of attention either in short notices or in longer articles. Such
titles appear as, the respiration of plants, the circulation of sap, the
excrementitious matter thrown off by plants, the effects of certain gases and
poisons on plants, and the relations of plants to different colored light. One
of the most important of the notes is that in which is described the
Page 479
discovery by Robert Brown (19, 393, 1831) of the constant movement of
minute particles suspended in a liquid, first detected by him in the fovilla of
pollen grains, and now known as the Brownian (or Brunonian) movement.
The heading under which this note appears is of interest, “The motion of
living particles in all kinds of matter.”
One side of botany touches agriculture and economics. That side was
represented even in the first volume of the Journal by a study of “the
comparative quantity of nutritious matter which may be obtained from an
acre of land when cultivated with potatoes or wheat.” Succeeding volumes
in this series likewise present phases which are of special interest regarded
from the point of view of economics; for example, those which treat of
rotation of crops and of enriching the soil. Probably the economic paper
which may be regarded as the most important, in fact epoch-making, is the
full account of the invention by Appert of a method for preserving food
indefinitely (13, 163, 1828). We all know that Appert’s process has
revolutionized the preservation of foods, and in its modern modification
underlies the vast industry of canned fruits, vegetables and so on. There are
suggestions, also, as to the utilization of new foods, or of old foods in a new
way, which resemble the suggestions made in these days of food
conservation. For example, it is shown that flour can be made from
leguminous seeds by steaming and subsequent drying, and pulverizing.
There are excellent hints as to the best ways of preparing and using
potatoes, and also for preserving them underground, where they will remain
good for a year or two. It is shown that potato flour can be made into
excellent bread. Another method of making bread, namely from wood, is
described, but it does not seem quite so practicable. There are interesting
notes on the sugar-beet as a source of sugar, and here appears one of the
earliest accounts of the Assam tea-plant, which was destined to
revolutionize the tea industry throughout the world. Cordage and textile
fibers of bark and of wood should be utilized in the manufacture of paper.
In fact one comes upon many such surprises in economic botany as the
earlier volumes of the Journal are carefully examined.
Early numbers of the Journal present with sufficient fullness accounts of
the remarkable discovery by Daguerre and others of a process for taking
pictures by light, on a silver plate or upon paper (37, 374, 1839; 38, 97,
1840, etc.). Before many years passed, the Journal had occasion to show
that these novel photographic delineations could be made useful in the
minute particles suspended in a liquid, first detected by him in the fovilla of
pollen grains, and now known as the Brownian (or Brunonian) movement.
The heading under which this note appears is of interest, “The motion of
living particles in all kinds of matter.”
One side of botany touches agriculture and economics. That side was
represented even in the first volume of the Journal by a study of “the
comparative quantity of nutritious matter which may be obtained from an
acre of land when cultivated with potatoes or wheat.” Succeeding volumes
in this series likewise present phases which are of special interest regarded
from the point of view of economics; for example, those which treat of
rotation of crops and of enriching the soil. Probably the economic paper
which may be regarded as the most important, in fact epoch-making, is the
full account of the invention by Appert of a method for preserving food
indefinitely (13, 163, 1828). We all know that Appert’s process has
revolutionized the preservation of foods, and in its modern modification
underlies the vast industry of canned fruits, vegetables and so on. There are
suggestions, also, as to the utilization of new foods, or of old foods in a new
way, which resemble the suggestions made in these days of food
conservation. For example, it is shown that flour can be made from
leguminous seeds by steaming and subsequent drying, and pulverizing.
There are excellent hints as to the best ways of preparing and using
potatoes, and also for preserving them underground, where they will remain
good for a year or two. It is shown that potato flour can be made into
excellent bread. Another method of making bread, namely from wood, is
described, but it does not seem quite so practicable. There are interesting
notes on the sugar-beet as a source of sugar, and here appears one of the
earliest accounts of the Assam tea-plant, which was destined to
revolutionize the tea industry throughout the world. Cordage and textile
fibers of bark and of wood should be utilized in the manufacture of paper.
In fact one comes upon many such surprises in economic botany as the
earlier volumes of the Journal are carefully examined.
Early numbers of the Journal present with sufficient fullness accounts of
the remarkable discovery by Daguerre and others of a process for taking
pictures by light, on a silver plate or upon paper (37, 374, 1839; 38, 97,
1840, etc.). Before many years passed, the Journal had occasion to show
that these novel photographic delineations could be made useful in the
Page 480
investigation of problems in botany. In the pages of the Journal it would be
easily possible to trace the development of this art in its relations to natural
history. Silliman possessed great sagacity in selecting for his enterprise all
the novelties which promised to be of service in the advancement of
science. In 1825 (9, 263) the Journal republished from the Edinburgh
Journal of Science an essay by Dr. (afterwards Sir) William Jackson
Hooker, on American Botany. In this essay the author states that “the
various scientific Journals” which “are published in America, contain many
memoirs upon the indigenous plants. Among the first of these in point of
value, and we think also the first with regard to time, we must name
Silliman’s Journal of Science.” The author enumerates some of the
contributors to the Journal and the titles of their papers.
It has been a useful practice of the Journal, almost from the first, to
transfer to its pages memoirs which would otherwise be likely to escape the
notice of the majority of American botanists. The book notices and the
longer book reviews covered so wide a field that they placed the readers of
the Journal in touch with nearly all of the current botanical literature both
here and abroad. These critical notices did much towards the symmetrical
development of botany in the United States. And as we shall now see, the
Journal notices and reviews in the hands of Asa Gray continued to be one of
the most important factors in the advancement of American botany.
easily possible to trace the development of this art in its relations to natural
history. Silliman possessed great sagacity in selecting for his enterprise all
the novelties which promised to be of service in the advancement of
science. In 1825 (9, 263) the Journal republished from the Edinburgh
Journal of Science an essay by Dr. (afterwards Sir) William Jackson
Hooker, on American Botany. In this essay the author states that “the
various scientific Journals” which “are published in America, contain many
memoirs upon the indigenous plants. Among the first of these in point of
value, and we think also the first with regard to time, we must name
Silliman’s Journal of Science.” The author enumerates some of the
contributors to the Journal and the titles of their papers.
It has been a useful practice of the Journal, almost from the first, to
transfer to its pages memoirs which would otherwise be likely to escape the
notice of the majority of American botanists. The book notices and the
longer book reviews covered so wide a field that they placed the readers of
the Journal in touch with nearly all of the current botanical literature both
here and abroad. These critical notices did much towards the symmetrical
development of botany in the United States. And as we shall now see, the
Journal notices and reviews in the hands of Asa Gray continued to be one of
the most important factors in the advancement of American botany.
Page 481
Asa Gray and the Journal.
In 1834 there appears in the Journal (25, 346) a “Sketch of the
Mineralogy of a portion of Jefferson and St. Lawrence Counties, New York,
by J. B. Crawe of Watertown and A. Gray of Utica, New York.” This
appears to be the first mention in the Journal of the name of Dr. Asa Gray,
who, shortly after that date, became thoroughly identified with its botanical
interests. In the early part of his career both before and immediately after
graduating in medicine, Gray gave much attention to the different branches
of natural history in its wide sense. He not only studied but taught
“chemistry, geology, mineralogy, and botany,” the latter branch being the
one to which he devoted most of his attention. Among his early guides in
the pursuit of botany may be mentioned Dr. Hadley, “who had learned some
botany from Dr. Ives of New Haven,” and Dr. Lewis C. Beck of Albany,
author of Botany of the United States North of Virginia. At that period he
made the acquaintance of Dr. John Torrey of New York, with whom he later
became associated in most important descriptive work. During the years
between his graduation in medicine and 1842, the year when he came to
Harvard College, his activities were diverse and intense; so that his
preparation for his distinguished career was very broad and thorough. His
first visit to Europe, in 1838, brought him into personal relations with a
large number of the botanists of Great Britain and the Continent. This
extensive acquaintance, added to his broad training, enabled him even from
the outset to exert a profound influence upon the progress of his favorite
science. He made the Journal tributary to this development. His name first
appears as associate editor in 1853, but there are articles in the Journal from
his pen which bear an earlier date. The first of these early botanical papers
is the following: “A Translation of a memoir entitled ‘Beiträge zur Lehre
von der Befruchtung der Pflanzen,’ (contributions to the doctrine of the
impregnation of plants, by A. J. C. Corda:) with prefatory remarks on the
progress of discovery relative to vegetable fecundation; by Asa Gray, M.
D.” (31, 308, 1837). Dr. Gray says that he made the translation from the
German for his own private use, but thinking that it might be interesting to
the Lyceum, he brought it before the Society, with “a cursory account of the
progress of discovery respecting the fecundation of flowering plants, for the
In 1834 there appears in the Journal (25, 346) a “Sketch of the
Mineralogy of a portion of Jefferson and St. Lawrence Counties, New York,
by J. B. Crawe of Watertown and A. Gray of Utica, New York.” This
appears to be the first mention in the Journal of the name of Dr. Asa Gray,
who, shortly after that date, became thoroughly identified with its botanical
interests. In the early part of his career both before and immediately after
graduating in medicine, Gray gave much attention to the different branches
of natural history in its wide sense. He not only studied but taught
“chemistry, geology, mineralogy, and botany,” the latter branch being the
one to which he devoted most of his attention. Among his early guides in
the pursuit of botany may be mentioned Dr. Hadley, “who had learned some
botany from Dr. Ives of New Haven,” and Dr. Lewis C. Beck of Albany,
author of Botany of the United States North of Virginia. At that period he
made the acquaintance of Dr. John Torrey of New York, with whom he later
became associated in most important descriptive work. During the years
between his graduation in medicine and 1842, the year when he came to
Harvard College, his activities were diverse and intense; so that his
preparation for his distinguished career was very broad and thorough. His
first visit to Europe, in 1838, brought him into personal relations with a
large number of the botanists of Great Britain and the Continent. This
extensive acquaintance, added to his broad training, enabled him even from
the outset to exert a profound influence upon the progress of his favorite
science. He made the Journal tributary to this development. His name first
appears as associate editor in 1853, but there are articles in the Journal from
his pen which bear an earlier date. The first of these early botanical papers
is the following: “A Translation of a memoir entitled ‘Beiträge zur Lehre
von der Befruchtung der Pflanzen,’ (contributions to the doctrine of the
impregnation of plants, by A. J. C. Corda:) with prefatory remarks on the
progress of discovery relative to vegetable fecundation; by Asa Gray, M.
D.” (31, 308, 1837). Dr. Gray says that he made the translation from the
German for his own private use, but thinking that it might be interesting to
the Lyceum, he brought it before the Society, with “a cursory account of the
progress of discovery respecting the fecundation of flowering plants, for the
Page 482
purpose of rendering the memoir more generally intelligible to those who
are not particularly conversant with the present state of botanical science.”
The translation occupies six pages of the Journal, while the prefatory
remarks fill nine pages. The prefatory remarks constitute an exhaustive
essay on the subject, embodied in attractive and perfectly clear language.
The translator shows complete familiarity with the matter in hand and gives
an adequate account of all the work done on the subject up to the date of M.
Corda’s paper. A second important paper by him near this period is his
review of “A Natural System of Botany: or a systematic view of the
Organization, Natural Affinities, and Geographical Distribution of the
whole Vegetable Kingdom; together with the use of the more important
species in Medicine, the Arts, and rural and domestic economy, by John
Lindley. Second edition, with numerous additions and corrections, and a
complete list of genera and their synonyms. London: 1836” (32, 292, 1837).
A very brief notice of this work in the first part of the volume for 1837
closes with the words, “A more extended notice of the work may be
expected in the ensuing number of the Journal.” The extended notice proved
to be a critical study of the work, signed by the initials A. G. which later
became so familiar to readers of the Journal. Citation of a few of its
sentences will indicate the strong and quiet manner in which Dr. Gray, even
at the outset, wrote his notices of books. In speaking of the second edition
of Professor Lindley’s work, he says:
are not particularly conversant with the present state of botanical science.”
The translation occupies six pages of the Journal, while the prefatory
remarks fill nine pages. The prefatory remarks constitute an exhaustive
essay on the subject, embodied in attractive and perfectly clear language.
The translator shows complete familiarity with the matter in hand and gives
an adequate account of all the work done on the subject up to the date of M.
Corda’s paper. A second important paper by him near this period is his
review of “A Natural System of Botany: or a systematic view of the
Organization, Natural Affinities, and Geographical Distribution of the
whole Vegetable Kingdom; together with the use of the more important
species in Medicine, the Arts, and rural and domestic economy, by John
Lindley. Second edition, with numerous additions and corrections, and a
complete list of genera and their synonyms. London: 1836” (32, 292, 1837).
A very brief notice of this work in the first part of the volume for 1837
closes with the words, “A more extended notice of the work may be
expected in the ensuing number of the Journal.” The extended notice proved
to be a critical study of the work, signed by the initials A. G. which later
became so familiar to readers of the Journal. Citation of a few of its
sentences will indicate the strong and quiet manner in which Dr. Gray, even
at the outset, wrote his notices of books. In speaking of the second edition
of Professor Lindley’s work, he says:
Page 483
“It is not necessary to state that a treatise of this kind was greatly needed, or to allude to the
peculiar qualifications of the learned and industrious author for the accomplishment of the task, or
the high estimation in which the work is held in Europe. But we may properly offer our testimony
respecting the great and favorable influence which it has exerted upon the progress of botanical
science in the United States. Great as the merits of the work undoubtedly are, we must nevertheless
be excused from adopting the terms of extravagant and sometimes equivocal eulogy employed by a
peculiar qualifications of the learned and industrious author for the accomplishment of the task, or
the high estimation in which the work is held in Europe. But we may properly offer our testimony
respecting the great and favorable influence which it has exerted upon the progress of botanical
science in the United States. Great as the merits of the work undoubtedly are, we must nevertheless
be excused from adopting the terms of extravagant and sometimes equivocal eulogy employed by a
Page 484
popular author, who gravely informs his readers that no book, since printed Bibles were first sold in
Paris by Dr. Faustus, ever excited so much surprise and wonder as did Dr. Torrey’s edition of
Lindley’s Introduction to the Natural System of Botany. Now we can hardly believe that either the
author or the American editor of the work referred to was ever in danger, as was honest Dr. Faustus,
of being burned for witchcraft, neither do we find anything in its pages calculated to produce such
astonishing effects, except, perhaps, upon the minds of those botanists, if such they may be called,
who had never dreamed of any important changes in the science since the appearance of good Dr.
Turton’s translation of the Species Plantarum, and who speak of Jussieu as a writer who has greatly
improved the natural orders of Linnæus.”
In the Journal for 1840 there is a large group of unsigned book reviews
under the heading, “Brief notices of recent Botanical works, especially
those most interesting to the student of North American Botany.” The first
of these short reviews deals with the second section of Part VII of De
Candolle’s “Prodromus.” In 1847 the consideration of the “Prodromus” is
resumed by the same author and the initials of A. G. are appended. This
indicates that Dr. Gray was probably the writer of some of the unsigned
book reviews which had appeared in the Journal between 1837 and 1840.
Doubtless Silliman availed himself of the assistance of his associates, Eli
Ives and others, in New Haven, in the examination of current botanical
literature, and it is extremely probable that he early secured help from
young Dr. Gray, who had shown himself to be a keen critic as well as a
pleasing writer. The notices of botanical works from 1840 bear marks of
having been from the same hand. They cover an extremely wide range of
subjects. While they are good-tempered they are critical, and they had much
to do with the development of botany, in this country, along safe lines.
Gray as Editor.—Gray’s name as associate editor of the Journal appears
in 1853. He had been a welcome contributor, as we have seen, for many
years. His influence upon the progress of botany in the United States was
largely due to his connection with the Journal. His reviews extended over a
very wide range, and supplemented to a remarkable degree his other
educational work. It must be permitted to allude here to his sagacity as a
writer of educational treatises. In his first elementary text-book, published
in 1836, he expressed wholly original views in regard to certain phases of
structure and function in plants, which became generally adopted at a later
date. His Manual of Botany was constructed, and subsequent editions were
kept, on a plan which made no appeal to those who wanted to work on lines
of least resistance; in fact he had no patience with those who desired merely
Paris by Dr. Faustus, ever excited so much surprise and wonder as did Dr. Torrey’s edition of
Lindley’s Introduction to the Natural System of Botany. Now we can hardly believe that either the
author or the American editor of the work referred to was ever in danger, as was honest Dr. Faustus,
of being burned for witchcraft, neither do we find anything in its pages calculated to produce such
astonishing effects, except, perhaps, upon the minds of those botanists, if such they may be called,
who had never dreamed of any important changes in the science since the appearance of good Dr.
Turton’s translation of the Species Plantarum, and who speak of Jussieu as a writer who has greatly
improved the natural orders of Linnæus.”
In the Journal for 1840 there is a large group of unsigned book reviews
under the heading, “Brief notices of recent Botanical works, especially
those most interesting to the student of North American Botany.” The first
of these short reviews deals with the second section of Part VII of De
Candolle’s “Prodromus.” In 1847 the consideration of the “Prodromus” is
resumed by the same author and the initials of A. G. are appended. This
indicates that Dr. Gray was probably the writer of some of the unsigned
book reviews which had appeared in the Journal between 1837 and 1840.
Doubtless Silliman availed himself of the assistance of his associates, Eli
Ives and others, in New Haven, in the examination of current botanical
literature, and it is extremely probable that he early secured help from
young Dr. Gray, who had shown himself to be a keen critic as well as a
pleasing writer. The notices of botanical works from 1840 bear marks of
having been from the same hand. They cover an extremely wide range of
subjects. While they are good-tempered they are critical, and they had much
to do with the development of botany, in this country, along safe lines.
Gray as Editor.—Gray’s name as associate editor of the Journal appears
in 1853. He had been a welcome contributor, as we have seen, for many
years. His influence upon the progress of botany in the United States was
largely due to his connection with the Journal. His reviews extended over a
very wide range, and supplemented to a remarkable degree his other
educational work. It must be permitted to allude here to his sagacity as a
writer of educational treatises. In his first elementary text-book, published
in 1836, he expressed wholly original views in regard to certain phases of
structure and function in plants, which became generally adopted at a later
date. His Manual of Botany was constructed, and subsequent editions were
kept, on a plan which made no appeal to those who wanted to work on lines
of least resistance; in fact he had no patience with those who desired merely
Page 485
to ascertain the name of a plant. In the Journal he emphasizes the
desirability of learning all the affinities of the plant under consideration. At
a later period, when entirely new chapters had been opened in the life of
plants, he sought by his contributions in the Journal to interest students in
this wider outlook.
Professor C. S. Sargent has selected with good judgment some of the
more important scientific papers by Professor Gray and has republished
them in a convenient form.[184] Many of these papers were contributed to the
Journal in the form of reviews. These reviews touch nearly every branch of
the science of botany. As Sargent justly says, “Many of the reviews are
filled with original and suggestive observations, and taken together, furnish
the best account of the development of botanical literature during the last
fifty years that has yet been written.” In these longer reviews in the Journal,
Gray was wont to take a book under review as affording an opportunity to
illustrate some important subject, and many of the reviews are crowded
with his expositions. For example, in his examination of vonMohl’s
“Vegetable Cell” (15, 451, 1853) he takes up the whole subject of
microscopic structure, so far as it was then understood, and he points out
the probable errors of some of Mohl’s contemporaries, showing what and
how great were Mohl’s own contributions to histology. Such a review is a
landmark in the science. The physiology of the cell and the nutrition of the
plant were favorite topics with Professor Gray, and he brought much of his
knowledge in regard to them into such a review as that of Boussingault (25,
120, 1858) on the “Influence of nitrates on the production of vegetable
matter.”
As a systematic botanist, Gray was naturally much interested in the
vexed question of nomenclature of plants. One of his most important
communications to the Journal is his review, in the volume for 1883 (26,
417), of DeCandolle’s work on the subject. He deals with this strictly
technical matter much as he did in a contribution to the Journal which he
made in 1868 (46, 63). In both of these papers he states with clearness the
general features of the code of nomenclature. He says explicitly that the
code does not make, but rather declares, the common law of botanists. The
treatment of the subject at his hands would rightly impress a general reader
as showing a strong desire to have common sense applied to doubtful cases,
instead of insisting on inflexible rules. For this reason, his rule of practice
was not always acceptable to those who were anxious to secure conformity
desirability of learning all the affinities of the plant under consideration. At
a later period, when entirely new chapters had been opened in the life of
plants, he sought by his contributions in the Journal to interest students in
this wider outlook.
Professor C. S. Sargent has selected with good judgment some of the
more important scientific papers by Professor Gray and has republished
them in a convenient form.[184] Many of these papers were contributed to the
Journal in the form of reviews. These reviews touch nearly every branch of
the science of botany. As Sargent justly says, “Many of the reviews are
filled with original and suggestive observations, and taken together, furnish
the best account of the development of botanical literature during the last
fifty years that has yet been written.” In these longer reviews in the Journal,
Gray was wont to take a book under review as affording an opportunity to
illustrate some important subject, and many of the reviews are crowded
with his expositions. For example, in his examination of vonMohl’s
“Vegetable Cell” (15, 451, 1853) he takes up the whole subject of
microscopic structure, so far as it was then understood, and he points out
the probable errors of some of Mohl’s contemporaries, showing what and
how great were Mohl’s own contributions to histology. Such a review is a
landmark in the science. The physiology of the cell and the nutrition of the
plant were favorite topics with Professor Gray, and he brought much of his
knowledge in regard to them into such a review as that of Boussingault (25,
120, 1858) on the “Influence of nitrates on the production of vegetable
matter.”
As a systematic botanist, Gray was naturally much interested in the
vexed question of nomenclature of plants. One of his most important
communications to the Journal is his review, in the volume for 1883 (26,
417), of DeCandolle’s work on the subject. He deals with this strictly
technical matter much as he did in a contribution to the Journal which he
made in 1868 (46, 63). In both of these papers he states with clearness the
general features of the code of nomenclature. He says explicitly that the
code does not make, but rather declares, the common law of botanists. The
treatment of the subject at his hands would rightly impress a general reader
as showing a strong desire to have common sense applied to doubtful cases,
instead of insisting on inflexible rules. For this reason, his rule of practice
was not always acceptable to those who were anxious to secure conformity
Page 486
to arbitrary rules at whatever cost. As he said in a paper published in the
Journal in 1847 (3, 302), “The difficulty of a reform increases with its
necessity. It is much easier to state the evils than to relieve them; and the
well-meant endeavors that have recently been made to this end, are, some
of them, likely, if adopted, to make confusion worse confounded.” This
feeling led him to be very conservative in the matter of reform in
nomenclature.
This subject of botanical nomenclature illustrates a method frequently
employed by Professor Gray to elucidate a difficult matter. He would find
in the treatise under review a text, or texts, on which he would build a
treatise of his own, and in this way he made clear his own views relative to
most of the important phases of botany. When he faced controverted
matters, his attitude still remained judicial. While he was tolerant of
opinions which clashed with his own, he was always severe upon
charlatanism and impatient of inaccuracy. The pages of the Journal contain
many severe criticisms at his hands, but an unprejudiced person would say
that the severity is merited.
Sometimes, however, instead of reviewing a book or an address, he
would follow the custom inaugurated early in the history of the Journal, of
making copious extracts, and thus give to its readers an opportunity of
examining materials which otherwise might not fall in their way.
Gray’s contributions to the Journal comprise more than one thousand
titles, without counting the memorial notices and the shorter obituary notes.
In these notices he sums up in a few well-chosen words the contributions
made to botany by his contemporaries. Even in the few instances in which
he felt obliged to note with disapproval some of the work, he expressed
himself with personal friendliness. The necrology, as it appeared from
month to month, was a labor of love. All of the longer memorial notices are
what it is the fashion now-a-days to call appreciations, and these are so
happily phrased that it would seem as if the writer in many a case asked
himself, “Would my friend, about whom I am now writing, make any
change in this sketch?”
Gray on Darwinism.—In October, 1859, Darwin’s epoch-making work,
“The Origin of Species,” was published. An early copy was sent to the
editor of the Journal, Professor James D. Dana. This arrived in New Haven
on December 21, but it was preceded by a personal letter which is of so
Journal in 1847 (3, 302), “The difficulty of a reform increases with its
necessity. It is much easier to state the evils than to relieve them; and the
well-meant endeavors that have recently been made to this end, are, some
of them, likely, if adopted, to make confusion worse confounded.” This
feeling led him to be very conservative in the matter of reform in
nomenclature.
This subject of botanical nomenclature illustrates a method frequently
employed by Professor Gray to elucidate a difficult matter. He would find
in the treatise under review a text, or texts, on which he would build a
treatise of his own, and in this way he made clear his own views relative to
most of the important phases of botany. When he faced controverted
matters, his attitude still remained judicial. While he was tolerant of
opinions which clashed with his own, he was always severe upon
charlatanism and impatient of inaccuracy. The pages of the Journal contain
many severe criticisms at his hands, but an unprejudiced person would say
that the severity is merited.
Sometimes, however, instead of reviewing a book or an address, he
would follow the custom inaugurated early in the history of the Journal, of
making copious extracts, and thus give to its readers an opportunity of
examining materials which otherwise might not fall in their way.
Gray’s contributions to the Journal comprise more than one thousand
titles, without counting the memorial notices and the shorter obituary notes.
In these notices he sums up in a few well-chosen words the contributions
made to botany by his contemporaries. Even in the few instances in which
he felt obliged to note with disapproval some of the work, he expressed
himself with personal friendliness. The necrology, as it appeared from
month to month, was a labor of love. All of the longer memorial notices are
what it is the fashion now-a-days to call appreciations, and these are so
happily phrased that it would seem as if the writer in many a case asked
himself, “Would my friend, about whom I am now writing, make any
change in this sketch?”
Gray on Darwinism.—In October, 1859, Darwin’s epoch-making work,
“The Origin of Species,” was published. An early copy was sent to the
editor of the Journal, Professor James D. Dana. This arrived in New Haven
on December 21, but it was preceded by a personal letter which is of so
Page 487
much interest that it is here transcribed in full. It should be added that Dana
was at this time in Europe where he was spending a year in the search for
health after a serious nervous breakdown. In his absence the book was
noticed by Gray as stated below. The letter is, as follows:
Down, Bromley, Kent.
Nov. 11th, 1859.
My dear Sir,
I have sent you a copy of my Book (as yet only an abstract) on the Origin of Species. I know too
well that the conclusion, at which I have arrived, will horrify you, but you will, I believe and hope,
give me credit for at least an honest search after the truth. I hope that you will read my Book, straight
through; otherwise from the great condensation it will be unintelligible. Do not, I pray, think me so
presumptuous as to hope to convert you; but if you can spare time to read it with care, and will then
do what is far more important, keep the subject under my point of view for some little time
occasionally before your mind, I have hopes that you will agree that more can be said in favour of the
mutability of species, than is at first apparent. It took me many long years before I wholly gave up
the common view of the separate creation of each species. Believe me, with sincere respect and with
cordial thanks for the many acts of scientific kindness which I have received from you,
My dear Sir,
Yours very sincerely,
Charles Darwin.
In March, 1860 (29, 153), Gray published in the Journal an elaborate and
cautious review of Darwin’s work. He alluded to the absence of the chief
editor of the Journal in the following words:
“The duty of reviewing this volume in the American Journal of Science would naturally devolve
upon the principal editor whose wide observation and profound knowledge of various departments of
natural history, as well as of geology, particularly qualify him for the task. But he has been obliged to
lay aside his pen to seek in distant lands the entire repose from scientific labor so essential to the
restoration of his health, a consummation devoutly to be wished and confidently to be expected.
Interested as Mr. Dana would be in this volume, he could not be expected to accept its doctrine.
Views so idealistic as those upon which his ‘Thoughts upon Species’ are grounded, will not
harmonize readily with a doctrine so thoroughly naturalistic as that of Mr. Darwin.... Between the
doctrines of this volume and those of the great naturalist whose name adorns the title page of this
Journal [Mr. Agassiz] the widest divergence appears.”
Gray then proceeds to contrast the two views of Darwin and Agassiz, “for
this contrast brings out most prominently and sets in strongest light and
shade the main features of the theory of the origination of species by means
was at this time in Europe where he was spending a year in the search for
health after a serious nervous breakdown. In his absence the book was
noticed by Gray as stated below. The letter is, as follows:
Down, Bromley, Kent.
Nov. 11th, 1859.
My dear Sir,
I have sent you a copy of my Book (as yet only an abstract) on the Origin of Species. I know too
well that the conclusion, at which I have arrived, will horrify you, but you will, I believe and hope,
give me credit for at least an honest search after the truth. I hope that you will read my Book, straight
through; otherwise from the great condensation it will be unintelligible. Do not, I pray, think me so
presumptuous as to hope to convert you; but if you can spare time to read it with care, and will then
do what is far more important, keep the subject under my point of view for some little time
occasionally before your mind, I have hopes that you will agree that more can be said in favour of the
mutability of species, than is at first apparent. It took me many long years before I wholly gave up
the common view of the separate creation of each species. Believe me, with sincere respect and with
cordial thanks for the many acts of scientific kindness which I have received from you,
My dear Sir,
Yours very sincerely,
Charles Darwin.
In March, 1860 (29, 153), Gray published in the Journal an elaborate and
cautious review of Darwin’s work. He alluded to the absence of the chief
editor of the Journal in the following words:
“The duty of reviewing this volume in the American Journal of Science would naturally devolve
upon the principal editor whose wide observation and profound knowledge of various departments of
natural history, as well as of geology, particularly qualify him for the task. But he has been obliged to
lay aside his pen to seek in distant lands the entire repose from scientific labor so essential to the
restoration of his health, a consummation devoutly to be wished and confidently to be expected.
Interested as Mr. Dana would be in this volume, he could not be expected to accept its doctrine.
Views so idealistic as those upon which his ‘Thoughts upon Species’ are grounded, will not
harmonize readily with a doctrine so thoroughly naturalistic as that of Mr. Darwin.... Between the
doctrines of this volume and those of the great naturalist whose name adorns the title page of this
Journal [Mr. Agassiz] the widest divergence appears.”
Gray then proceeds to contrast the two views of Darwin and Agassiz, “for
this contrast brings out most prominently and sets in strongest light and
shade the main features of the theory of the origination of species by means
Page 488
of Natural Selection.” He then states both sides with great fairness, and
proceeds:
“Who shall decide between such extreme views so ably maintained on either hand, and say how
much truth there may be in each. The present reviewer has not the presumption to undertake such a
task. Having no prepossession in favor of naturalistic theories, but struck with the eminent ability of
Mr. Darwin’s work, and charmed with its fairness, our humbler duty will be performed if, laying
aside prejudice as much as we can, we shall succeed in giving a fair account of its method and
argument, offering by the way a few suggestions such as might occur to any naturalist of an inquiring
mind. An editorial character for this article must in justice be disclaimed. The plural pronoun is
employed not to give editorial weight, but to avoid even the appearance of egotism and also the
circumlocution which attends a rigorous adherence to the impersonal style.”
In this review he moves slowly and thoughtfully, but not timidly, over the
new paths. There is no clear indication in the review that he has yet made
up his mind as to the validity of Darwin’s hypothesis. But, in a second
article appearing in the Journal for September of the same year (30, 226),
under the title “Discussion between two readers of Darwin’s treatise on the
origin of species upon its natural theology” Gray plainly begins to incline to
take a very favorable view of the Darwinian theory, and makes use of the
following ingenious illustration to show that it is not inconsistent with
theistic design. A few paragraphs here quoted show the felicity of his style
in a controverted matter:
“Recall a woman of a past generation and show her a web of cloth; ask her how it was made, and
she will say that the wool or cotton was carded, spun, and woven by hand. When you tell her it was
not made by manual labor, that probably no hands have touched the materials throughout the process,
it is possible that she might at first regard your statement as tantamount to the assertion that the cloth
was made without design. If she did, she would not credit your statement. If you patiently explained
to her the theory of carding-machines, spinning-jennies, and power-looms, would her reception of
your explanation weaken her conviction that the cloth was the result of design? It is certain that she
would believe in design as firmly as before, and that this belief would be attended by a higher
conception and reverent admiration of a wisdom, skill, and power greatly beyond anything she had
previously conceived possible.”
By this review Gray disarmed hostility to such an extent that some
persons who had been antagonistic to Darwinism accepted it with only
slight reservation. It may be fairly claimed that the Journal bore a leading
part in influencing the views of naturalists in America in regard to the
Darwinian theory.
proceeds:
“Who shall decide between such extreme views so ably maintained on either hand, and say how
much truth there may be in each. The present reviewer has not the presumption to undertake such a
task. Having no prepossession in favor of naturalistic theories, but struck with the eminent ability of
Mr. Darwin’s work, and charmed with its fairness, our humbler duty will be performed if, laying
aside prejudice as much as we can, we shall succeed in giving a fair account of its method and
argument, offering by the way a few suggestions such as might occur to any naturalist of an inquiring
mind. An editorial character for this article must in justice be disclaimed. The plural pronoun is
employed not to give editorial weight, but to avoid even the appearance of egotism and also the
circumlocution which attends a rigorous adherence to the impersonal style.”
In this review he moves slowly and thoughtfully, but not timidly, over the
new paths. There is no clear indication in the review that he has yet made
up his mind as to the validity of Darwin’s hypothesis. But, in a second
article appearing in the Journal for September of the same year (30, 226),
under the title “Discussion between two readers of Darwin’s treatise on the
origin of species upon its natural theology” Gray plainly begins to incline to
take a very favorable view of the Darwinian theory, and makes use of the
following ingenious illustration to show that it is not inconsistent with
theistic design. A few paragraphs here quoted show the felicity of his style
in a controverted matter:
“Recall a woman of a past generation and show her a web of cloth; ask her how it was made, and
she will say that the wool or cotton was carded, spun, and woven by hand. When you tell her it was
not made by manual labor, that probably no hands have touched the materials throughout the process,
it is possible that she might at first regard your statement as tantamount to the assertion that the cloth
was made without design. If she did, she would not credit your statement. If you patiently explained
to her the theory of carding-machines, spinning-jennies, and power-looms, would her reception of
your explanation weaken her conviction that the cloth was the result of design? It is certain that she
would believe in design as firmly as before, and that this belief would be attended by a higher
conception and reverent admiration of a wisdom, skill, and power greatly beyond anything she had
previously conceived possible.”
By this review Gray disarmed hostility to such an extent that some
persons who had been antagonistic to Darwinism accepted it with only
slight reservation. It may be fairly claimed that the Journal bore a leading
part in influencing the views of naturalists in America in regard to the
Darwinian theory.
Page 489
Dr. Gray soon put the Darwinian hypothesis to a severe test. In the
Journal for 1840 he had called attention to the remarkable similarity which
exists between the flora of Japan and a part of the temperate portion of
North America. The first notice of this subject by him occurs in a short
review of Dr. Zuccarini’s “Flora Japonica,” a work based on material
furnished by Dr. Siebold, who had long lived in Japan. In this review (39,
175, 1840), he enumerates certain plants common to the two regions, and
says, “It is interesting to remark how many of our characteristic genera are
reproduced in Japan, not to speak of striking analogous forms.” In a
subsequent paper (28, 187, 1859), he recurs to this subject, and, after
alluding to geological data furnished by J. D. Dana, he says:
“I cannot resist the conclusion that the extant vegetable kingdom has a long and eventful history,
and that the explanation of apparent anomalies in the geographical distribution of species may be
found in the various and prolonged climatic or other vicissitudes to which they have been subject in
earlier times; that the occurrence of certain species, formerly supposed to be peculiar to North
America, in a remote or antipodal region, affords in itself no presumption that they were originated
there, and that interchange of plants between eastern North America and eastern Asia is explicable
upon the most natural and generally received hypothesis (or at least offers no greater difficulty than
does the arctic flora, the general homogeneousness of which round the world has always been
thought compatible with local origin of the species) and is perhaps not more extensive than might be
expected under the circumstances. That the interchange has mainly taken place in high northern
latitudes, and that the isothermal lines have in earlier times turned northward on our eastern and
southward on our northwest coast, as they do now, are points which go far towards explaining why
eastern North America, rather than Oregon and California, has been mainly concerned in this
interchange, and why the temperate interchange, even with Europe, has principally taken place
through Asia.”
Journal for 1840 he had called attention to the remarkable similarity which
exists between the flora of Japan and a part of the temperate portion of
North America. The first notice of this subject by him occurs in a short
review of Dr. Zuccarini’s “Flora Japonica,” a work based on material
furnished by Dr. Siebold, who had long lived in Japan. In this review (39,
175, 1840), he enumerates certain plants common to the two regions, and
says, “It is interesting to remark how many of our characteristic genera are
reproduced in Japan, not to speak of striking analogous forms.” In a
subsequent paper (28, 187, 1859), he recurs to this subject, and, after
alluding to geological data furnished by J. D. Dana, he says:
“I cannot resist the conclusion that the extant vegetable kingdom has a long and eventful history,
and that the explanation of apparent anomalies in the geographical distribution of species may be
found in the various and prolonged climatic or other vicissitudes to which they have been subject in
earlier times; that the occurrence of certain species, formerly supposed to be peculiar to North
America, in a remote or antipodal region, affords in itself no presumption that they were originated
there, and that interchange of plants between eastern North America and eastern Asia is explicable
upon the most natural and generally received hypothesis (or at least offers no greater difficulty than
does the arctic flora, the general homogeneousness of which round the world has always been
thought compatible with local origin of the species) and is perhaps not more extensive than might be
expected under the circumstances. That the interchange has mainly taken place in high northern
latitudes, and that the isothermal lines have in earlier times turned northward on our eastern and
southward on our northwest coast, as they do now, are points which go far towards explaining why
eastern North America, rather than Oregon and California, has been mainly concerned in this
interchange, and why the temperate interchange, even with Europe, has principally taken place
through Asia.”
Page 490
From “Life and Letters of Charles Darwin” by Francis
Darwin.
This paper was communicated in 1859, on the eve of the publication of
Darwin’s “Origin of Species.” At a later date he applied the Darwinian
theory to the possible solution of the problem, and came to the conclusion
that the two floras had a common origin in the Arctic zone, during the
Tertiary period, or the Cretaceous which preceded it, and the descendants
had made their way down different lines toward the south, the species
varying under different climatic conditions, and thus exhibiting similarity
but not absolute identity of form. Before the American Association for the
Darwin.
This paper was communicated in 1859, on the eve of the publication of
Darwin’s “Origin of Species.” At a later date he applied the Darwinian
theory to the possible solution of the problem, and came to the conclusion
that the two floras had a common origin in the Arctic zone, during the
Tertiary period, or the Cretaceous which preceded it, and the descendants
had made their way down different lines toward the south, the species
varying under different climatic conditions, and thus exhibiting similarity
but not absolute identity of form. Before the American Association for the
Page 491
Advancement of Science, in his Presidential address, in 1872, he used the
following language:
“According to these views, as regards plants at least, the adaptation to successive times and
changed conditions has been maintained, not by absolute renewals, but by gradual modifications. I,
for one, cannot doubt that the present existing species are the lineal successors of those that garnished
the earth in the old time before them, and that they were as well adapted to their surroundings then,
as those which flourish and bloom around us are to their conditions now. Order and exquisite
adaptation did not wait for man’s coming, nor were they ever stereotyped. Organic Nature—by which
I mean the system and totality of living things, and their adaptation to each other and to the world—
with all its apparent and indeed real stability, should be likened, not to the ocean, which varies only
by tidal oscillations from a fixed level to which it is always returning, but rather to a river, so vast
that we can neither discern its shores nor reach its sources, whose onward flow is not less actual
because too slow to be observed by the ephemeræ which hover over its surface, or are borne upon its
bosom.”
Gray’s active interest in the Journal continued until the very end of his
life. There were many critical notices from his pen in 1887. His last
contribution to its pages was the botanical necrology, which appeared
posthumously in volume 35, of the third series (1888). His connection with
the Journal covered, therefore, a period of more than a half a century of its
life.[185]
The changes that were wrought in botany by the application of
Darwinism were far reaching. Attempts were promptly made to reconstruct
the system of botanical classification on the basis of descent. The more
successful of these endeavors met with welcome, and now form the
groundwork of arrangement of families, genera, and species, in the Herbaria
in this country, in the manuals of descriptive botany, and in the text-books
of higher grade. This overturn did not take place until after Gray’s death,
although he foresaw that the revolution was impending.
One of the most obvious changes was that which gave a high degree of
prominence in American school treatises to the study of the lower instead of
the higher or flowering plants, these latter being treated merely as members
in a long series, and with scant consideration. But of late years, there has
been a renewed popular interest in the phænogamia, leading to a more
thorough investigation of local floras, and also to the examination of the
relations of plants to their surroundings. The results of a large part of this
technical work are published in strictly botanical periodicals and now-a-
days seldom find a place in the pages of a general journal of science.
following language:
“According to these views, as regards plants at least, the adaptation to successive times and
changed conditions has been maintained, not by absolute renewals, but by gradual modifications. I,
for one, cannot doubt that the present existing species are the lineal successors of those that garnished
the earth in the old time before them, and that they were as well adapted to their surroundings then,
as those which flourish and bloom around us are to their conditions now. Order and exquisite
adaptation did not wait for man’s coming, nor were they ever stereotyped. Organic Nature—by which
I mean the system and totality of living things, and their adaptation to each other and to the world—
with all its apparent and indeed real stability, should be likened, not to the ocean, which varies only
by tidal oscillations from a fixed level to which it is always returning, but rather to a river, so vast
that we can neither discern its shores nor reach its sources, whose onward flow is not less actual
because too slow to be observed by the ephemeræ which hover over its surface, or are borne upon its
bosom.”
Gray’s active interest in the Journal continued until the very end of his
life. There were many critical notices from his pen in 1887. His last
contribution to its pages was the botanical necrology, which appeared
posthumously in volume 35, of the third series (1888). His connection with
the Journal covered, therefore, a period of more than a half a century of its
life.[185]
The changes that were wrought in botany by the application of
Darwinism were far reaching. Attempts were promptly made to reconstruct
the system of botanical classification on the basis of descent. The more
successful of these endeavors met with welcome, and now form the
groundwork of arrangement of families, genera, and species, in the Herbaria
in this country, in the manuals of descriptive botany, and in the text-books
of higher grade. This overturn did not take place until after Gray’s death,
although he foresaw that the revolution was impending.
One of the most obvious changes was that which gave a high degree of
prominence in American school treatises to the study of the lower instead of
the higher or flowering plants, these latter being treated merely as members
in a long series, and with scant consideration. But of late years, there has
been a renewed popular interest in the phænogamia, leading to a more
thorough investigation of local floras, and also to the examination of the
relations of plants to their surroundings. The results of a large part of this
technical work are published in strictly botanical periodicals and now-a-
days seldom find a place in the pages of a general journal of science.
Page 492
Cryptogamic Botany in the Journal since 1846.
In glancing rapidly at the First Series it has been seen that a fair share of
attention was early paid by the Journal to the flowerless plants. So far as the
means and methods of the time permitted, the ferns, mosses, lichens, and
the larger algæ and fungi of America were studied assiduously and
important results were published, chiefly on the side of systematic botany.
The Second Series comprises the years between 1846 and 1871. In this
series one finds that the range of cryptogamic botany is much widened.
Besides interesting book notices relative to these plants, there are a good
many papers on the larger fungi, on the algæ, and mosses. Here are
contributions by Curtis, by Ravenel, by Bailey, and by Sullivant. The
lichens are treated of in detail by Tuckerman, and there are some excellent
translations by Dr. Engelmann of papers by Alexander Braun. Some of the
destructive fungi are considered, as might well be the case in the period of
the potato famine. It is in these years that one first finds the name of Daniel
Cady Eaton, who later had so much to do with developing an interest in the
subject of ferns in this country. He was a frequent contributor of critical
notices.
Cryptogamic Botany, as it is now understood, is a comparatively modern
branch of science. The appliances and the methods for investigating the
more obscure groups, and especially for revealing the successive stages of
their development, were unsatisfactory until the latter half of the last
century. Gray recognized this condition of affairs, and appreciated the
importance of the new methods and the better appliances. Therefore he
viewed with satisfaction the pursuit of these studies abroad by one of his
students and assistants, William G. Farlow. Dr. Farlow carried to his studies
under DeBary and others unusual powers of observation and great industry.
He speedily became an accomplished investigator in cryptogamic botany
and enriched the science by notable discoveries, one of which to-day bears
his name in botanical literature. On his return to the United States, Farlow
entered at once upon a successful career as an inspiring teacher and a
fruitful investigator. He became a frequent contributor to the Journal,
keeping its readers in touch with the more important additions to
cryptogamic botany. He had wisely chosen to deal with the whole field, and
In glancing rapidly at the First Series it has been seen that a fair share of
attention was early paid by the Journal to the flowerless plants. So far as the
means and methods of the time permitted, the ferns, mosses, lichens, and
the larger algæ and fungi of America were studied assiduously and
important results were published, chiefly on the side of systematic botany.
The Second Series comprises the years between 1846 and 1871. In this
series one finds that the range of cryptogamic botany is much widened.
Besides interesting book notices relative to these plants, there are a good
many papers on the larger fungi, on the algæ, and mosses. Here are
contributions by Curtis, by Ravenel, by Bailey, and by Sullivant. The
lichens are treated of in detail by Tuckerman, and there are some excellent
translations by Dr. Engelmann of papers by Alexander Braun. Some of the
destructive fungi are considered, as might well be the case in the period of
the potato famine. It is in these years that one first finds the name of Daniel
Cady Eaton, who later had so much to do with developing an interest in the
subject of ferns in this country. He was a frequent contributor of critical
notices.
Cryptogamic Botany, as it is now understood, is a comparatively modern
branch of science. The appliances and the methods for investigating the
more obscure groups, and especially for revealing the successive stages of
their development, were unsatisfactory until the latter half of the last
century. Gray recognized this condition of affairs, and appreciated the
importance of the new methods and the better appliances. Therefore he
viewed with satisfaction the pursuit of these studies abroad by one of his
students and assistants, William G. Farlow. Dr. Farlow carried to his studies
under DeBary and others unusual powers of observation and great industry.
He speedily became an accomplished investigator in cryptogamic botany
and enriched the science by notable discoveries, one of which to-day bears
his name in botanical literature. On his return to the United States, Farlow
entered at once upon a successful career as an inspiring teacher and a
fruitful investigator. He became a frequent contributor to the Journal,
keeping its readers in touch with the more important additions to
cryptogamic botany. He had wisely chosen to deal with the whole field, and
Page 493
consequently he has been able to preserve a better perspective than is kept
by the extreme specialist. The greater number of cryptogamic botanists in
this country have been under Professor Farlow’s instruction.
by the extreme specialist. The greater number of cryptogamic botanists in
this country have been under Professor Farlow’s instruction.
Page 494
Systematic and Geographical Botany of Late Years.
The usefulness of the Journal in descriptive systematic botany of
phanerogams is shown not only by its acceptance of the leading features of
DeCandolle’s Phytography, where very exact methods are inculcated, but
by the very numerous contributions by Sereno Watson and others at the
Harvard University Herbarium, as well as from private systematists. It is in
the pages of the Journal that one finds the record of much of the critical
work of Tuckerman and of Engelmann, in interesting Phanerogamia. Of late
years the Journal has had the privilege, of publishing a good deal of the
careful work of Theo Holm, in the difficult groups of Cyperaceæ, and also
his admirable studies in the morphology and the anatomy of certain
interesting plants of higher orders.
Attention was called, in passing, to Gray’s deep interest in geographical
botany. In this important branch, besides his contributions, one finds,
among many others, such papers as LeConte’s “Flora of the Coast Islands
of California in Relation to Recent Changes of Physical Geography” (34,
457, 1887), and Sargent’s “Forests of Central Nevada” (17, 417, 1879).
Examination reveals a surprising number of communications which bear
indirectly upon this subject.
The usefulness of the Journal in descriptive systematic botany of
phanerogams is shown not only by its acceptance of the leading features of
DeCandolle’s Phytography, where very exact methods are inculcated, but
by the very numerous contributions by Sereno Watson and others at the
Harvard University Herbarium, as well as from private systematists. It is in
the pages of the Journal that one finds the record of much of the critical
work of Tuckerman and of Engelmann, in interesting Phanerogamia. Of late
years the Journal has had the privilege, of publishing a good deal of the
careful work of Theo Holm, in the difficult groups of Cyperaceæ, and also
his admirable studies in the morphology and the anatomy of certain
interesting plants of higher orders.
Attention was called, in passing, to Gray’s deep interest in geographical
botany. In this important branch, besides his contributions, one finds,
among many others, such papers as LeConte’s “Flora of the Coast Islands
of California in Relation to Recent Changes of Physical Geography” (34,
457, 1887), and Sargent’s “Forests of Central Nevada” (17, 417, 1879).
Examination reveals a surprising number of communications which bear
indirectly upon this subject.
Page 495
Paleontological Botany.
When the Journal began its career, the subject of fossil plants was very
obscure. Brongniart’s papers, especially the Journal translations, enabled
the students in America to undertake the investigation of such fossils and
the results were to a considerable extent published in the Journal. Since the
subject belongs as much to geology as to botany, it finds its appropriate
home in the pages of the Journal. The recent papers on this topic show how
great has been the advance in methods and results since the early days of
the Journal’s century. Under the care of George E. Wieland, the
communications and the bibliographical notices of paleontological treatises
show the progress which he and others are making in this attractive field.
When the Journal began its career, the subject of fossil plants was very
obscure. Brongniart’s papers, especially the Journal translations, enabled
the students in America to undertake the investigation of such fossils and
the results were to a considerable extent published in the Journal. Since the
subject belongs as much to geology as to botany, it finds its appropriate
home in the pages of the Journal. The recent papers on this topic show how
great has been the advance in methods and results since the early days of
the Journal’s century. Under the care of George E. Wieland, the
communications and the bibliographical notices of paleontological treatises
show the progress which he and others are making in this attractive field.
Page 496
Economic Botany, Plant Physiology, etc.
At the outset, the Journal, as we have seen, devoted much attention to
certain phases of economic botany, and, even down to the present, it has
maintained its hold upon the subject. The correspondence of Jerome
Nicklès from 1853 to 1867 brought before its readers a vast number of
valuable items which would not in any other way have been known to them.
And the Journal dealt wisely with the scientific side of agriculture, under
the hands of S. W. Johnson and J. H. Gilbert, and others, placing it on its
proper basis. This work was supplemented by Norton’s remarkable work in
the chemistry of certain plants, the oat, for example, and certain plant-
products. In fact it might be possible to construct from the pages of the
Journal a fair synopsis of the important principles of agronomy.
Physiology has been represented not only by the studies which had been
inaugurated and stimulated by the Darwinian theory, such as the cross-
fertilization and the close-fertilization of plants, plant-movements, and the
like, but there have been a good many special communications, such as
Dandeno on toxicity, Plowman on electrical relations, and ionization, and
W. P. Wilson on respiration.
There are many broad philosophical questions which have found an
appropriate home in the Journal, such as “The Plant-individual in its
relation to the species” (Alexander Braun, 19, 297, 1855; 20, 181, 1855),
and “The analogy between the mode of reproduction in plants and the
alternation of generations observed in some radiata” (J. D. Dana, 10, 341,
1850). Akin to these are many of the reflections which one finds scattered
throughout the pages of the Journal, frequently in minor book notices. As
might be expected, some attention has been paid to the very special branch
of botany which is strictly called medical. For example, early in its history,
the Journal published a long treatise by Dr. William Tully (2, 45, 1820), on
the ergot of rye. This is considered from a structural as well as from a
medical point of view and is decidedly ahead of the time in which it was
written. There are a few references to vegetable poisons, and there is a
fascinating account of the effect of the common white ash on the activities
of the rattlesnake. In short it may be said that the editor did much towards
making the Journal readable as well as strictly scientific.
At the outset, the Journal, as we have seen, devoted much attention to
certain phases of economic botany, and, even down to the present, it has
maintained its hold upon the subject. The correspondence of Jerome
Nicklès from 1853 to 1867 brought before its readers a vast number of
valuable items which would not in any other way have been known to them.
And the Journal dealt wisely with the scientific side of agriculture, under
the hands of S. W. Johnson and J. H. Gilbert, and others, placing it on its
proper basis. This work was supplemented by Norton’s remarkable work in
the chemistry of certain plants, the oat, for example, and certain plant-
products. In fact it might be possible to construct from the pages of the
Journal a fair synopsis of the important principles of agronomy.
Physiology has been represented not only by the studies which had been
inaugurated and stimulated by the Darwinian theory, such as the cross-
fertilization and the close-fertilization of plants, plant-movements, and the
like, but there have been a good many special communications, such as
Dandeno on toxicity, Plowman on electrical relations, and ionization, and
W. P. Wilson on respiration.
There are many broad philosophical questions which have found an
appropriate home in the Journal, such as “The Plant-individual in its
relation to the species” (Alexander Braun, 19, 297, 1855; 20, 181, 1855),
and “The analogy between the mode of reproduction in plants and the
alternation of generations observed in some radiata” (J. D. Dana, 10, 341,
1850). Akin to these are many of the reflections which one finds scattered
throughout the pages of the Journal, frequently in minor book notices. As
might be expected, some attention has been paid to the very special branch
of botany which is strictly called medical. For example, early in its history,
the Journal published a long treatise by Dr. William Tully (2, 45, 1820), on
the ergot of rye. This is considered from a structural as well as from a
medical point of view and is decidedly ahead of the time in which it was
written. There are a few references to vegetable poisons, and there is a
fascinating account of the effect of the common white ash on the activities
of the rattlesnake. In short it may be said that the editor did much towards
making the Journal readable as well as strictly scientific.
Page 497
The list of reviewers who have been permitted to use the pages of the
Journal for notices of botanical and allied books in recent years is pretty
long. One finds the initials of Wesley R. Coe, George P. Clinton, Arthur L.
Dean, Alexander W. Evans, William G. Farlow, George L. Goodale, Arthur
H. Graves, Herbert E. Gregory, Lafayette B. Mendel, Leo F. Rettger,
Benjamin L. Robinson, George R. Wieland, and others.
At the present time, in the biological sciences, as in every department of
thought, there is great specialization, and each specialty demands its own
private organ of publication. Naturally this has led to a falling off in the
botanical communications to the Journal, but it cannot be forgotten that the
history of North American Botany has been largely recorded in its pages.
Journal for notices of botanical and allied books in recent years is pretty
long. One finds the initials of Wesley R. Coe, George P. Clinton, Arthur L.
Dean, Alexander W. Evans, William G. Farlow, George L. Goodale, Arthur
H. Graves, Herbert E. Gregory, Lafayette B. Mendel, Leo F. Rettger,
Benjamin L. Robinson, George R. Wieland, and others.
At the present time, in the biological sciences, as in every department of
thought, there is great specialization, and each specialty demands its own
private organ of publication. Naturally this has led to a falling off in the
botanical communications to the Journal, but it cannot be forgotten that the
history of North American Botany has been largely recorded in its pages.
Page 498
Notes.
184. Scientific Papers of Asa Gray. Selected by Charles Sprague Sargent. Two volumes, Boston,
1889 (see notice in vol. 38, 419, 1889).
185. A notice of Gray’s life and works is given by his life-long friend, J. D. Dana, in the Journal
in 1888 (35, 181–203).
184. Scientific Papers of Asa Gray. Selected by Charles Sprague Sargent. Two volumes, Boston,
1889 (see notice in vol. 38, 419, 1889).
185. A notice of Gray’s life and works is given by his life-long friend, J. D. Dana, in the Journal
in 1888 (35, 181–203).
Page 499
Page 500
TRANSCRIBER’S NOTES
1. Typos fixed; non-standard spelling and dialect retained.
2. Used numbers for footnotes.
1. Typos fixed; non-standard spelling and dialect retained.
2. Used numbers for footnotes.
Page 501
*** END OF THE PROJECT GUTENBERG EBOOK A CENTURY OF
SCIENCE IN AMERICA ***
Updated editions will replace the previous one—the old editions will
be renamed.
Creating the works from print editions not protected by U.S. copyright
law means that no one owns a United States copyright in these works,
so the Foundation (and you!) can copy and distribute it in the United
States without permission and without paying copyright royalties.
Special rules, set forth in the General Terms of Use part of this license,
apply to copying and distributing Project Gutenberg™ electronic
works to protect the PROJECT GUTENBERG™ concept and
trademark. Project Gutenberg is a registered trademark, and may not
be used if you charge for an eBook, except by following the terms of
the trademark license, including paying royalties for use of the Project
Gutenberg trademark. If you do not charge anything for copies of this
eBook, complying with the trademark license is very easy. You may
use this eBook for nearly any purpose such as creation of derivative
works, reports, performances and research. Project Gutenberg eBooks
may be modified and printed and given away—you may do practically
ANYTHING in the United States with eBooks not protected by U.S.
copyright law. Redistribution is subject to the trademark license,
especially commercial redistribution.
START: FULL LICENSE
SCIENCE IN AMERICA ***
Updated editions will replace the previous one—the old editions will
be renamed.
Creating the works from print editions not protected by U.S. copyright
law means that no one owns a United States copyright in these works,
so the Foundation (and you!) can copy and distribute it in the United
States without permission and without paying copyright royalties.
Special rules, set forth in the General Terms of Use part of this license,
apply to copying and distributing Project Gutenberg™ electronic
works to protect the PROJECT GUTENBERG™ concept and
trademark. Project Gutenberg is a registered trademark, and may not
be used if you charge for an eBook, except by following the terms of
the trademark license, including paying royalties for use of the Project
Gutenberg trademark. If you do not charge anything for copies of this
eBook, complying with the trademark license is very easy. You may
use this eBook for nearly any purpose such as creation of derivative
works, reports, performances and research. Project Gutenberg eBooks
may be modified and printed and given away—you may do practically
ANYTHING in the United States with eBooks not protected by U.S.
copyright law. Redistribution is subject to the trademark license,
especially commercial redistribution.
START: FULL LICENSE
Page 502
THE FULL PROJECT GUTENBERG™ LICENSE
PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK
To protect the Project Gutenberg™ mission of promoting the free
distribution of electronic works, by using or distributing this work (or
any other work associated in any way with the phrase “Project
Gutenberg”), you agree to comply with all the terms of the Full Project
Gutenberg License available with this file or online at
www.gutenberg.org/license.
Section 1. General Terms of Use and Redistributing
Project Gutenberg electronic works
1.A. By reading or using any part of this Project Gutenberg electronic
work, you indicate that you have read, understand, agree to and accept
all the terms of this license and intellectual property
(trademark/copyright) agreement. If you do not agree to abide by all
the terms of this agreement, you must cease using and return or destroy
all copies of Project Gutenberg electronic works in your possession. If
you paid a fee for obtaining a copy of or access to a Project Gutenberg
electronic work and you do not agree to be bound by the terms of this
agreement, you may obtain a refund from the person or entity to whom
you paid the fee as set forth in paragraph 1.E.8.
1.B. “Project Gutenberg” is a registered trademark. It may only be
used on or associated in any way with an electronic work by people
who agree to be bound by the terms of this agreement. There are a few
things that you can do with most Project Gutenberg electronic works
even without complying with the full terms of this agreement. See
paragraph 1.C below. There are a lot of things you can do with Project
Gutenberg electronic works if you follow the terms of this agreement
and help preserve free future access to Project Gutenberg electronic
works. See paragraph 1.E below.
1.C. The Project Gutenberg Literary Archive Foundation (“the
Foundation” or PGLAF), owns a compilation copyright in the
PLEASE READ THIS BEFORE YOU DISTRIBUTE OR USE THIS WORK
To protect the Project Gutenberg™ mission of promoting the free
distribution of electronic works, by using or distributing this work (or
any other work associated in any way with the phrase “Project
Gutenberg”), you agree to comply with all the terms of the Full Project
Gutenberg License available with this file or online at
www.gutenberg.org/license.
Section 1. General Terms of Use and Redistributing
Project Gutenberg electronic works
1.A. By reading or using any part of this Project Gutenberg electronic
work, you indicate that you have read, understand, agree to and accept
all the terms of this license and intellectual property
(trademark/copyright) agreement. If you do not agree to abide by all
the terms of this agreement, you must cease using and return or destroy
all copies of Project Gutenberg electronic works in your possession. If
you paid a fee for obtaining a copy of or access to a Project Gutenberg
electronic work and you do not agree to be bound by the terms of this
agreement, you may obtain a refund from the person or entity to whom
you paid the fee as set forth in paragraph 1.E.8.
1.B. “Project Gutenberg” is a registered trademark. It may only be
used on or associated in any way with an electronic work by people
who agree to be bound by the terms of this agreement. There are a few
things that you can do with most Project Gutenberg electronic works
even without complying with the full terms of this agreement. See
paragraph 1.C below. There are a lot of things you can do with Project
Gutenberg electronic works if you follow the terms of this agreement
and help preserve free future access to Project Gutenberg electronic
works. See paragraph 1.E below.
1.C. The Project Gutenberg Literary Archive Foundation (“the
Foundation” or PGLAF), owns a compilation copyright in the
Page 503
collection of Project Gutenberg electronic works. Nearly all the
individual works in the collection are in the public domain in the
United States. If an individual work is unprotected by copyright law in
the United States and you are located in the United States, we do not
claim a right to prevent you from copying, distributing, performing,
displaying or creating derivative works based on the work as long as
all references to Project Gutenberg are removed. Of course, we hope
that you will support the Project Gutenberg mission of promoting free
access to electronic works by freely sharing Project Gutenberg works
in compliance with the terms of this agreement for keeping the Project
Gutenberg name associated with the work. You can easily comply with
the terms of this agreement by keeping this work in the same format
with its attached full Project Gutenberg License when you share it
without charge with others.
1.D. The copyright laws of the place where you are located also govern
what you can do with this work. Copyright laws in most countries are
in a constant state of change. If you are outside the United States,
check the laws of your country in addition to the terms of this
agreement before downloading, copying, displaying, performing,
distributing or creating derivative works based on this work or any
other Project Gutenberg work. The Foundation makes no
representations concerning the copyright status of any work in any
country other than the United States.
1.E. Unless you have removed all references to Project Gutenberg:
1.E.1. The following sentence, with active links to, or other immediate
access to, the full Project Gutenberg License must appear prominently
whenever any copy of a Project Gutenberg work (any work on which
the phrase “Project Gutenberg” appears, or with which the phrase
“Project Gutenberg” is associated) is accessed, displayed, performed,
viewed, copied or distributed:
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
individual works in the collection are in the public domain in the
United States. If an individual work is unprotected by copyright law in
the United States and you are located in the United States, we do not
claim a right to prevent you from copying, distributing, performing,
displaying or creating derivative works based on the work as long as
all references to Project Gutenberg are removed. Of course, we hope
that you will support the Project Gutenberg mission of promoting free
access to electronic works by freely sharing Project Gutenberg works
in compliance with the terms of this agreement for keeping the Project
Gutenberg name associated with the work. You can easily comply with
the terms of this agreement by keeping this work in the same format
with its attached full Project Gutenberg License when you share it
without charge with others.
1.D. The copyright laws of the place where you are located also govern
what you can do with this work. Copyright laws in most countries are
in a constant state of change. If you are outside the United States,
check the laws of your country in addition to the terms of this
agreement before downloading, copying, displaying, performing,
distributing or creating derivative works based on this work or any
other Project Gutenberg work. The Foundation makes no
representations concerning the copyright status of any work in any
country other than the United States.
1.E. Unless you have removed all references to Project Gutenberg:
1.E.1. The following sentence, with active links to, or other immediate
access to, the full Project Gutenberg License must appear prominently
whenever any copy of a Project Gutenberg work (any work on which
the phrase “Project Gutenberg” appears, or with which the phrase
“Project Gutenberg” is associated) is accessed, displayed, performed,
viewed, copied or distributed:
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
Page 504
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.
1.E.2. If an individual Project Gutenberg electronic work is derived
from texts not protected by U.S. copyright law (does not contain a
notice indicating that it is posted with permission of the copyright
holder), the work can be copied and distributed to anyone in the United
States without paying any fees or charges. If you are redistributing or
providing access to a work with the phrase “Project Gutenberg”
associated with or appearing on the work, you must comply either with
the requirements of paragraphs 1.E.1 through 1.E.7 or obtain
permission for the use of the work and the Project Gutenberg
trademark as set forth in paragraphs 1.E.8 or 1.E.9.
1.E.3. If an individual Project Gutenberg electronic work is posted
with the permission of the copyright holder, your use and distribution
must comply with both paragraphs 1.E.1 through 1.E.7 and any
additional terms imposed by the copyright holder. Additional terms
will be linked to the Project Gutenberg License for all works posted
with the permission of the copyright holder found at the beginning of
this work.
1.E.4. Do not unlink or detach or remove the full Project Gutenberg
License terms from this work, or any files containing a part of this
work or any other work associated with Project Gutenberg.
1.E.5. Do not copy, display, perform, distribute or redistribute this
electronic work, or any part of this electronic work, without
prominently displaying the sentence set forth in paragraph 1.E.1 with
active links or immediate access to the full terms of the Project
Gutenberg License.
1.E.6. You may convert to and distribute this work in any binary,
compressed, marked up, nonproprietary or proprietary form, including
any word processing or hypertext form. However, if you provide
access to or distribute copies of a Project Gutenberg work in a format
other than “Plain Vanilla ASCII” or other format used in the official
in the United States, you will have to check the laws of the
country where you are located before using this eBook.
1.E.2. If an individual Project Gutenberg electronic work is derived
from texts not protected by U.S. copyright law (does not contain a
notice indicating that it is posted with permission of the copyright
holder), the work can be copied and distributed to anyone in the United
States without paying any fees or charges. If you are redistributing or
providing access to a work with the phrase “Project Gutenberg”
associated with or appearing on the work, you must comply either with
the requirements of paragraphs 1.E.1 through 1.E.7 or obtain
permission for the use of the work and the Project Gutenberg
trademark as set forth in paragraphs 1.E.8 or 1.E.9.
1.E.3. If an individual Project Gutenberg electronic work is posted
with the permission of the copyright holder, your use and distribution
must comply with both paragraphs 1.E.1 through 1.E.7 and any
additional terms imposed by the copyright holder. Additional terms
will be linked to the Project Gutenberg License for all works posted
with the permission of the copyright holder found at the beginning of
this work.
1.E.4. Do not unlink or detach or remove the full Project Gutenberg
License terms from this work, or any files containing a part of this
work or any other work associated with Project Gutenberg.
1.E.5. Do not copy, display, perform, distribute or redistribute this
electronic work, or any part of this electronic work, without
prominently displaying the sentence set forth in paragraph 1.E.1 with
active links or immediate access to the full terms of the Project
Gutenberg License.
1.E.6. You may convert to and distribute this work in any binary,
compressed, marked up, nonproprietary or proprietary form, including
any word processing or hypertext form. However, if you provide
access to or distribute copies of a Project Gutenberg work in a format
other than “Plain Vanilla ASCII” or other format used in the official
Page 505
version posted on the official Project Gutenberg website
(www.gutenberg.org), you must, at no additional cost, fee or expense
to the user, provide a copy, a means of exporting a copy, or a means of
obtaining a copy upon request, of the work in its original “Plain
Vanilla ASCII” or other form. Any alternate format must include the
full Project Gutenberg License as specified in paragraph 1.E.1.
1.E.7. Do not charge a fee for access to, viewing, displaying,
performing, copying or distributing any Project Gutenberg works
unless you comply with paragraph 1.E.8 or 1.E.9.
1.E.8. You may charge a reasonable fee for copies of or providing
access to or distributing Project Gutenberg electronic works provided
that:
• You pay a royalty fee of 20% of the gross profits you derive from the
use of Project Gutenberg works calculated using the method you
already use to calculate your applicable taxes. The fee is owed to the
owner of the Project Gutenberg trademark, but he has agreed to donate
royalties under this paragraph to the Project Gutenberg Literary
Archive Foundation. Royalty payments must be paid within 60 days
following each date on which you prepare (or are legally required to
prepare) your periodic tax returns. Royalty payments should be clearly
marked as such and sent to the Project Gutenberg Literary Archive
Foundation at the address specified in Section 4, “Information about
donations to the Project Gutenberg Literary Archive Foundation.”
• You provide a full refund of any money paid by a user who notifies
you in writing (or by e-mail) within 30 days of receipt that s/he does
not agree to the terms of the full Project Gutenberg™ License. You
must require such a user to return or destroy all copies of the works
possessed in a physical medium and discontinue all use of and all
access to other copies of Project Gutenberg™ works.
• You provide, in accordance with paragraph 1.F.3, a full refund of any
money paid for a work or a replacement copy, if a defect in the
electronic work is discovered and reported to you within 90 days of
receipt of the work.
(www.gutenberg.org), you must, at no additional cost, fee or expense
to the user, provide a copy, a means of exporting a copy, or a means of
obtaining a copy upon request, of the work in its original “Plain
Vanilla ASCII” or other form. Any alternate format must include the
full Project Gutenberg License as specified in paragraph 1.E.1.
1.E.7. Do not charge a fee for access to, viewing, displaying,
performing, copying or distributing any Project Gutenberg works
unless you comply with paragraph 1.E.8 or 1.E.9.
1.E.8. You may charge a reasonable fee for copies of or providing
access to or distributing Project Gutenberg electronic works provided
that:
• You pay a royalty fee of 20% of the gross profits you derive from the
use of Project Gutenberg works calculated using the method you
already use to calculate your applicable taxes. The fee is owed to the
owner of the Project Gutenberg trademark, but he has agreed to donate
royalties under this paragraph to the Project Gutenberg Literary
Archive Foundation. Royalty payments must be paid within 60 days
following each date on which you prepare (or are legally required to
prepare) your periodic tax returns. Royalty payments should be clearly
marked as such and sent to the Project Gutenberg Literary Archive
Foundation at the address specified in Section 4, “Information about
donations to the Project Gutenberg Literary Archive Foundation.”
• You provide a full refund of any money paid by a user who notifies
you in writing (or by e-mail) within 30 days of receipt that s/he does
not agree to the terms of the full Project Gutenberg™ License. You
must require such a user to return or destroy all copies of the works
possessed in a physical medium and discontinue all use of and all
access to other copies of Project Gutenberg™ works.
• You provide, in accordance with paragraph 1.F.3, a full refund of any
money paid for a work or a replacement copy, if a defect in the
electronic work is discovered and reported to you within 90 days of
receipt of the work.
Page 506
• You comply with all other terms of this agreement for free distribution
of Project Gutenberg™ works.
1.E.9. If you wish to charge a fee or distribute a Project Gutenberg™
electronic work or group of works on different terms than are set forth
in this agreement, you must obtain permission in writing from the
Project Gutenberg Literary Archive Foundation, the manager of the
Project Gutenberg™ trademark. Contact the Foundation as set forth in
Section 3 below.
1.F.
1.F.1. Project Gutenberg volunteers and employees expend
considerable effort to identify, do copyright research on, transcribe and
proofread works not protected by U.S. copyright law in creating the
Project Gutenberg™ collection. Despite these efforts, Project
Gutenberg™ electronic works, and the medium on which they may be
stored, may contain “Defects,” such as, but not limited to, incomplete,
inaccurate or corrupt data, transcription errors, a copyright or other
intellectual property infringement, a defective or damaged disk or
other medium, a computer virus, or computer codes that damage or
cannot be read by your equipment.
1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES -
Except for the “Right of Replacement or Refund” described in
paragraph 1.F.3, the Project Gutenberg Literary Archive Foundation,
the owner of the Project Gutenberg™ trademark, and any other party
distributing a Project Gutenberg™ electronic work under this
agreement, disclaim all liability to you for damages, costs and
expenses, including legal fees. YOU AGREE THAT YOU HAVE NO
REMEDIES FOR NEGLIGENCE, STRICT LIABILITY, BREACH
OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE
PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE
FOUNDATION, THE TRADEMARK OWNER, AND ANY
DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE
LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT,
CONSEQUENTIAL, PUNITIVE OR INCIDENTAL DAMAGES
of Project Gutenberg™ works.
1.E.9. If you wish to charge a fee or distribute a Project Gutenberg™
electronic work or group of works on different terms than are set forth
in this agreement, you must obtain permission in writing from the
Project Gutenberg Literary Archive Foundation, the manager of the
Project Gutenberg™ trademark. Contact the Foundation as set forth in
Section 3 below.
1.F.
1.F.1. Project Gutenberg volunteers and employees expend
considerable effort to identify, do copyright research on, transcribe and
proofread works not protected by U.S. copyright law in creating the
Project Gutenberg™ collection. Despite these efforts, Project
Gutenberg™ electronic works, and the medium on which they may be
stored, may contain “Defects,” such as, but not limited to, incomplete,
inaccurate or corrupt data, transcription errors, a copyright or other
intellectual property infringement, a defective or damaged disk or
other medium, a computer virus, or computer codes that damage or
cannot be read by your equipment.
1.F.2. LIMITED WARRANTY, DISCLAIMER OF DAMAGES -
Except for the “Right of Replacement or Refund” described in
paragraph 1.F.3, the Project Gutenberg Literary Archive Foundation,
the owner of the Project Gutenberg™ trademark, and any other party
distributing a Project Gutenberg™ electronic work under this
agreement, disclaim all liability to you for damages, costs and
expenses, including legal fees. YOU AGREE THAT YOU HAVE NO
REMEDIES FOR NEGLIGENCE, STRICT LIABILITY, BREACH
OF WARRANTY OR BREACH OF CONTRACT EXCEPT THOSE
PROVIDED IN PARAGRAPH 1.F.3. YOU AGREE THAT THE
FOUNDATION, THE TRADEMARK OWNER, AND ANY
DISTRIBUTOR UNDER THIS AGREEMENT WILL NOT BE
LIABLE TO YOU FOR ACTUAL, DIRECT, INDIRECT,
CONSEQUENTIAL, PUNITIVE OR INCIDENTAL DAMAGES
Page 507
EVEN IF YOU GIVE NOTICE OF THE POSSIBILITY OF SUCH
DAMAGE.
1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you
discover a defect in this electronic work within 90 days of receiving it,
you can receive a refund of the money (if any) you paid for it by
sending a written explanation to the person you received the work
from. If you received the work on a physical medium, you must return
the medium with your written explanation. The person or entity that
provided you with the defective work may elect to provide a
replacement copy in lieu of a refund. If you received the work
electronically, the person or entity providing it to you may choose to
give you a second opportunity to receive the work electronically in lieu
of a refund. If the second copy is also defective, you may demand a
refund in writing without further opportunities to fix the problem.
1.F.4. Except for the limited right of replacement or refund set forth in
paragraph 1.F.3, this work is provided to you ‘AS-IS’, WITH NO
OTHER WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED,
INCLUDING BUT NOT LIMITED TO WARRANTIES OF
MERCHANTABILITY OR FITNESS FOR ANY PURPOSE.
1.F.5. Some states do not allow disclaimers of certain implied
warranties or the exclusion or limitation of certain types of damages. If
any disclaimer or limitation set forth in this agreement violates the law
of the state applicable to this agreement, the agreement shall be
interpreted to make the maximum disclaimer or limitation permitted by
the applicable state law. The invalidity or unenforceability of any
provision of this agreement shall not void the remaining provisions.
1.F.6. INDEMNITY - You agree to indemnify and hold the
Foundation, the trademark owner, any agent or employee of the
Foundation, anyone providing copies of Project Gutenberg™
electronic works in accordance with this agreement, and any
volunteers associated with the production, promotion and distribution
of Project Gutenberg™ electronic works, harmless from all liability,
costs and expenses, including legal fees, that arise directly or indirectly
from any of the following which you do or cause to occur: (a)
DAMAGE.
1.F.3. LIMITED RIGHT OF REPLACEMENT OR REFUND - If you
discover a defect in this electronic work within 90 days of receiving it,
you can receive a refund of the money (if any) you paid for it by
sending a written explanation to the person you received the work
from. If you received the work on a physical medium, you must return
the medium with your written explanation. The person or entity that
provided you with the defective work may elect to provide a
replacement copy in lieu of a refund. If you received the work
electronically, the person or entity providing it to you may choose to
give you a second opportunity to receive the work electronically in lieu
of a refund. If the second copy is also defective, you may demand a
refund in writing without further opportunities to fix the problem.
1.F.4. Except for the limited right of replacement or refund set forth in
paragraph 1.F.3, this work is provided to you ‘AS-IS’, WITH NO
OTHER WARRANTIES OF ANY KIND, EXPRESS OR IMPLIED,
INCLUDING BUT NOT LIMITED TO WARRANTIES OF
MERCHANTABILITY OR FITNESS FOR ANY PURPOSE.
1.F.5. Some states do not allow disclaimers of certain implied
warranties or the exclusion or limitation of certain types of damages. If
any disclaimer or limitation set forth in this agreement violates the law
of the state applicable to this agreement, the agreement shall be
interpreted to make the maximum disclaimer or limitation permitted by
the applicable state law. The invalidity or unenforceability of any
provision of this agreement shall not void the remaining provisions.
1.F.6. INDEMNITY - You agree to indemnify and hold the
Foundation, the trademark owner, any agent or employee of the
Foundation, anyone providing copies of Project Gutenberg™
electronic works in accordance with this agreement, and any
volunteers associated with the production, promotion and distribution
of Project Gutenberg™ electronic works, harmless from all liability,
costs and expenses, including legal fees, that arise directly or indirectly
from any of the following which you do or cause to occur: (a)
Page 508
distribution of this or any Project Gutenberg work, (b) alteration,
modification, or additions or deletions to any Project Gutenberg work,
and (c) any Defect you cause.
Section 2. Information about the Mission of Project
Gutenberg
Project Gutenberg is synonymous with the free distribution of
electronic works in formats readable by the widest variety of
computers including obsolete, old, middle-aged and new computers. It
exists because of the efforts of hundreds of volunteers and donations
from people in all walks of life.
Volunteers and financial support to provide volunteers with the
assistance they need are critical to reaching Project Gutenberg’s goals
and ensuring that the Project Gutenberg collection will remain freely
available for generations to come. In 2001, the Project Gutenberg
Literary Archive Foundation was created to provide a secure and
permanent future for Project Gutenberg and future generations. To
learn more about the Project Gutenberg Literary Archive Foundation
and how your efforts and donations can help, see Sections 3 and 4 and
the Foundation information page at www.gutenberg.org.
Section 3. Information about the Project Gutenberg
Literary Archive Foundation
The Project Gutenberg Literary Archive Foundation is a non-profit
501(c)(3) educational corporation organized under the laws of the state
of Mississippi and granted tax exempt status by the Internal Revenue
Service. The Foundation’s EIN or federal tax identification number is
64-6221541. Contributions to the Project Gutenberg Literary Archive
Foundation are tax deductible to the full extent permitted by U.S.
federal laws and your state’s laws.
The Foundation’s business office is located at 41 Watchung Plaza
#516, Montclair NJ 07042, USA, +1 (862) 621-9288. Email contact
modification, or additions or deletions to any Project Gutenberg work,
and (c) any Defect you cause.
Section 2. Information about the Mission of Project
Gutenberg
Project Gutenberg is synonymous with the free distribution of
electronic works in formats readable by the widest variety of
computers including obsolete, old, middle-aged and new computers. It
exists because of the efforts of hundreds of volunteers and donations
from people in all walks of life.
Volunteers and financial support to provide volunteers with the
assistance they need are critical to reaching Project Gutenberg’s goals
and ensuring that the Project Gutenberg collection will remain freely
available for generations to come. In 2001, the Project Gutenberg
Literary Archive Foundation was created to provide a secure and
permanent future for Project Gutenberg and future generations. To
learn more about the Project Gutenberg Literary Archive Foundation
and how your efforts and donations can help, see Sections 3 and 4 and
the Foundation information page at www.gutenberg.org.
Section 3. Information about the Project Gutenberg
Literary Archive Foundation
The Project Gutenberg Literary Archive Foundation is a non-profit
501(c)(3) educational corporation organized under the laws of the state
of Mississippi and granted tax exempt status by the Internal Revenue
Service. The Foundation’s EIN or federal tax identification number is
64-6221541. Contributions to the Project Gutenberg Literary Archive
Foundation are tax deductible to the full extent permitted by U.S.
federal laws and your state’s laws.
The Foundation’s business office is located at 41 Watchung Plaza
#516, Montclair NJ 07042, USA, +1 (862) 621-9288. Email contact
Page 509
links and up to date contact information can be found at the
Foundation’s website and official page at www.gutenberg.org/contact
Section 4. Information about Donations to the Project
Gutenberg Literary Archive Foundation
Project Gutenberg™ depends upon and cannot survive without
widespread public support and donations to carry out its mission of
increasing the number of public domain and licensed works that can be
freely distributed in machine-readable form accessible by the widest
array of equipment including outdated equipment. Many small
donations ($1 to $5,000) are particularly important to maintaining tax
exempt status with the IRS.
The Foundation is committed to complying with the laws regulating
charities and charitable donations in all 50 states of the United States.
Compliance requirements are not uniform and it takes a considerable
effort, much paperwork and many fees to meet and keep up with these
requirements. We do not solicit donations in locations where we have
not received written confirmation of compliance. To SEND
DONATIONS or determine the status of compliance for any particular
state visit www.gutenberg.org/donate.
While we cannot and do not solicit contributions from states where we
have not met the solicitation requirements, we know of no prohibition
against accepting unsolicited donations from donors in such states who
approach us with offers to donate.
International donations are gratefully accepted, but we cannot make
any statements concerning tax treatment of donations received from
outside the United States. U.S. laws alone swamp our small staff.
Please check the Project Gutenberg web pages for current donation
methods and addresses. Donations are accepted in a number of other
ways including checks, online payments and credit card donations. To
donate, please visit: www.gutenberg.org/donate.
Foundation’s website and official page at www.gutenberg.org/contact
Section 4. Information about Donations to the Project
Gutenberg Literary Archive Foundation
Project Gutenberg™ depends upon and cannot survive without
widespread public support and donations to carry out its mission of
increasing the number of public domain and licensed works that can be
freely distributed in machine-readable form accessible by the widest
array of equipment including outdated equipment. Many small
donations ($1 to $5,000) are particularly important to maintaining tax
exempt status with the IRS.
The Foundation is committed to complying with the laws regulating
charities and charitable donations in all 50 states of the United States.
Compliance requirements are not uniform and it takes a considerable
effort, much paperwork and many fees to meet and keep up with these
requirements. We do not solicit donations in locations where we have
not received written confirmation of compliance. To SEND
DONATIONS or determine the status of compliance for any particular
state visit www.gutenberg.org/donate.
While we cannot and do not solicit contributions from states where we
have not met the solicitation requirements, we know of no prohibition
against accepting unsolicited donations from donors in such states who
approach us with offers to donate.
International donations are gratefully accepted, but we cannot make
any statements concerning tax treatment of donations received from
outside the United States. U.S. laws alone swamp our small staff.
Please check the Project Gutenberg web pages for current donation
methods and addresses. Donations are accepted in a number of other
ways including checks, online payments and credit card donations. To
donate, please visit: www.gutenberg.org/donate.
Page 510
Section 5. General Information About Project Gutenberg
electronic works
Professor Michael S. Hart was the originator of the Project Gutenberg
concept of a library of electronic works that could be freely shared
with anyone. For forty years, he produced and distributed Project
Gutenberg eBooks with only a loose network of volunteer support.
Project Gutenberg eBooks are often created from several printed
editions, all of which are confirmed as not protected by copyright in
the U.S. unless a copyright notice is included. Thus, we do not
necessarily keep eBooks in compliance with any particular paper
edition.
Most people start at our website which has the main PG search facility:
www.gutenberg.org.
This website includes information about Project Gutenberg, including
how to make donations to the Project Gutenberg Literary Archive
Foundation, how to help produce our new eBooks, and how to
subscribe to our email newsletter to hear about new eBooks.
electronic works
Professor Michael S. Hart was the originator of the Project Gutenberg
concept of a library of electronic works that could be freely shared
with anyone. For forty years, he produced and distributed Project
Gutenberg eBooks with only a loose network of volunteer support.
Project Gutenberg eBooks are often created from several printed
editions, all of which are confirmed as not protected by copyright in
the U.S. unless a copyright notice is included. Thus, we do not
necessarily keep eBooks in compliance with any particular paper
edition.
Most people start at our website which has the main PG search facility:
www.gutenberg.org.
This website includes information about Project Gutenberg, including
how to make donations to the Project Gutenberg Literary Archive
Foundation, how to help produce our new eBooks, and how to
subscribe to our email newsletter to hear about new eBooks.