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The Project Gutenberg eBook of The Geologic Story of
Yellowstone National Park
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
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have to check the laws of the country where you are located before
using this eBook.
Title: The Geologic Story of Yellowstone National Park
Author: William R. Keefer
Illustrator: John R. Stacy
Release date: October 25, 2019 [eBook #60574]
Most recently updated: October 17, 2024
Language: English
Other information and formats: www.gutenberg.org/ebooks/60574
Credits: Produced by Stephen Hutcheson and the Online Distributed
Proofreading Team at http://www.pgdp.net
*** START OF THE PROJECT GUTENBERG EBOOK THE GEOLOGIC
STORY OF YELLOWSTONE NATIONAL PARK ***
Yellowstone National Park
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: The Geologic Story of Yellowstone National Park
Author: William R. Keefer
Illustrator: John R. Stacy
Release date: October 25, 2019 [eBook #60574]
Most recently updated: October 17, 2024
Language: English
Other information and formats: www.gutenberg.org/ebooks/60574
Credits: Produced by Stephen Hutcheson and the Online Distributed
Proofreading Team at http://www.pgdp.net
*** START OF THE PROJECT GUTENBERG EBOOK THE GEOLOGIC
STORY OF YELLOWSTONE NATIONAL PARK ***
Page 4
Geology of
YELLOWSTONE
A review of the geologic processes and events responsible for the
spectacular natural wonders of the Yellowstone country,
commemorating the 100th anniversary of the oldest and largest
of our national parks.
For sale by the Superintendent of Documents, U.S. Government Printing Office
Washington, DC. 20402—Price $1.25
Stock Number 2401-1209
II
YELLOWSTONE
A review of the geologic processes and events responsible for the
spectacular natural wonders of the Yellowstone country,
commemorating the 100th anniversary of the oldest and largest
of our national parks.
For sale by the Superintendent of Documents, U.S. Government Printing Office
Washington, DC. 20402—Price $1.25
Stock Number 2401-1209
II
Page 5
“* * * and behold! The whole country beyond was smoking with
vapor from boiling springs, and burning with gases issuing from
small craters, each of which was emitting a sharp, whistling sound.
* * * The general face of the country was smooth and rolling, being
a level plain, dotted with cone-shaped mounds. On the summit of
these mounds were small craters from four to six feet in diameter.
Interspersed among these on the level plain were larger craters,
some of them four to six miles across. Out of these craters, issued
blue flames and molten brimstone.”
vapor from boiling springs, and burning with gases issuing from
small craters, each of which was emitting a sharp, whistling sound.
* * * The general face of the country was smooth and rolling, being
a level plain, dotted with cone-shaped mounds. On the summit of
these mounds were small craters from four to six feet in diameter.
Interspersed among these on the level plain were larger craters,
some of them four to six miles across. Out of these craters, issued
blue flames and molten brimstone.”
Page 6
Description credited to Joseph Meek, 1829; quotation from page 40 of the
book “The Yellowstone National Park” by Hiram Martin Chittenden (as edited
and published by Richard A. Bartlett, University of Oklahoma Press, Norman,
Oklahoma, 1964). Photograph is of Midway Geyser Basin.
IV
“Be it enacted by the Senate and House of Representatives of the
United States of America in Congress assembled, that the tract of
land in the territories of Montana and Wyoming lying near the
headwaters of the Yellowstone River is hereby reserved and
withdrawn from settlement, occupancy, or sale under the laws of
the United States, and dedicated and set apart as a public park
or pleasuring ground for the benefit and enjoyment of the people
* * *”
Approved March 1, 1872—signed by:
James G. Blaine, Speaker of the House
Schuyler Colfax, Vice-President of the United States and President of the
Senate
book “The Yellowstone National Park” by Hiram Martin Chittenden (as edited
and published by Richard A. Bartlett, University of Oklahoma Press, Norman,
Oklahoma, 1964). Photograph is of Midway Geyser Basin.
IV
“Be it enacted by the Senate and House of Representatives of the
United States of America in Congress assembled, that the tract of
land in the territories of Montana and Wyoming lying near the
headwaters of the Yellowstone River is hereby reserved and
withdrawn from settlement, occupancy, or sale under the laws of
the United States, and dedicated and set apart as a public park
or pleasuring ground for the benefit and enjoyment of the people
* * *”
Approved March 1, 1872—signed by:
James G. Blaine, Speaker of the House
Schuyler Colfax, Vice-President of the United States and President of the
Senate
Page 7
Ulysses S. Grant, President of the United States
V
The Geologic Story of
YELLOWSTONE
NATIONAL PARK
By William R. Keefer
Illustrated by John R. Stacy
Based on a planned series of technical reports resulting from
comprehensive geologic studies in Yellowstone National Park by the
author and his colleagues, H. R. Blank, Jr., R. L. Christiansen, R. O.
Fournier, J. D. Love, L. J. P. Muffler, J. D. Obradovich, K. L. Pierce, H. J.
Prostka, G. M. Richmond, Meyer Rubin, E. T. Ruppel, H. W. Smedes, A.
H. Truesdell, H. A. Waldrop, and D. E. White.
GEOLOGICAL SURVEY BULLETIN 1347
VI
UNITED STATES DEPARTMENT OF THE INTERIOR
ROGERS C. B. MORTON, Secretary
GEOLOGICAL SURVEY
V. E. McKelvey, Director
Library of Congress catalog-card No. 79-169200
V
The Geologic Story of
YELLOWSTONE
NATIONAL PARK
By William R. Keefer
Illustrated by John R. Stacy
Based on a planned series of technical reports resulting from
comprehensive geologic studies in Yellowstone National Park by the
author and his colleagues, H. R. Blank, Jr., R. L. Christiansen, R. O.
Fournier, J. D. Love, L. J. P. Muffler, J. D. Obradovich, K. L. Pierce, H. J.
Prostka, G. M. Richmond, Meyer Rubin, E. T. Ruppel, H. W. Smedes, A.
H. Truesdell, H. A. Waldrop, and D. E. White.
GEOLOGICAL SURVEY BULLETIN 1347
VI
UNITED STATES DEPARTMENT OF THE INTERIOR
ROGERS C. B. MORTON, Secretary
GEOLOGICAL SURVEY
V. E. McKelvey, Director
Library of Congress catalog-card No. 79-169200
Page 8
First printing 1971 (1972)
Second printing 1972
VII
Second printing 1972
VII
Page 9
Foreword
In the aftermath of the Civil War, the United States expanded the exploration
of her western frontiers to gain a measure of the vast lands and natural
resources in the region now occupied by our Rocky Mountain States. As part
of this effort, the Geological and Geographical Survey of the Territories was
organized within the Department of the Interior, and staffed by a group of
hardy, pioneering scientists under the leadership of geologist F. V. Hayden.
During the summer of 1871, these men, accompanied by photographer
William H. Jackson and artist Thomas Moran, made a reconnaissance
geological study of the legendary and mysterious “Yellowstone Wonderland”
in remote northwestern Wyoming Territory. The scientific reports and
illustrations prepared by Hayden and his colleagues, supplementing the
startling accounts that had been published by members of the famous
Washburn-Doane Expedition a year earlier, erased all doubts that this unique
land was eminently worthy of being set aside “for the benefit and enjoyment
of the people.” By Act of Congress on March 1, 1872, our first National Park
was established.
During the past century, 50 million people have toured Yellowstone National
Park, marveling at its never-ending display of natural wonders. No doubt
many have paused to wonder about the origin of these unusual and complex
geological features—a question, needless to say, that has intrigued and
challenged scientists from the very first days of the Hayden Survey. During
the past decade a group of U. S. Geological Survey scientists, in cooperation
with the National Park Service and aided by the interest of the National
Aeronautics and Space Administration in remote sensing of the geologic
phenomena, has been probing the depths and farthest corners of the Park
seeking more of the answers. Some of the results of this work, and those of
earlier studies, are described in this book to provide a better understanding
and enjoyment of this great National Park.
In the aftermath of the Civil War, the United States expanded the exploration
of her western frontiers to gain a measure of the vast lands and natural
resources in the region now occupied by our Rocky Mountain States. As part
of this effort, the Geological and Geographical Survey of the Territories was
organized within the Department of the Interior, and staffed by a group of
hardy, pioneering scientists under the leadership of geologist F. V. Hayden.
During the summer of 1871, these men, accompanied by photographer
William H. Jackson and artist Thomas Moran, made a reconnaissance
geological study of the legendary and mysterious “Yellowstone Wonderland”
in remote northwestern Wyoming Territory. The scientific reports and
illustrations prepared by Hayden and his colleagues, supplementing the
startling accounts that had been published by members of the famous
Washburn-Doane Expedition a year earlier, erased all doubts that this unique
land was eminently worthy of being set aside “for the benefit and enjoyment
of the people.” By Act of Congress on March 1, 1872, our first National Park
was established.
During the past century, 50 million people have toured Yellowstone National
Park, marveling at its never-ending display of natural wonders. No doubt
many have paused to wonder about the origin of these unusual and complex
geological features—a question, needless to say, that has intrigued and
challenged scientists from the very first days of the Hayden Survey. During
the past decade a group of U. S. Geological Survey scientists, in cooperation
with the National Park Service and aided by the interest of the National
Aeronautics and Space Administration in remote sensing of the geologic
phenomena, has been probing the depths and farthest corners of the Park
seeking more of the answers. Some of the results of this work, and those of
earlier studies, are described in this book to provide a better understanding
and enjoyment of this great National Park.
Page 10
V. E. McKelvey, Director
U. S. Geological Survey
IX
U. S. Geological Survey
IX
Page 11
Contents
Page
Foreword VII
Yellowstone country 1
A geological preview 4
Geologic history of the Yellowstone region 7
The nature of the rocks reveals their origins 7
The oldest rocks 7
The deposits of the shifting seas 13
The first mountain-building episode 19
Volcanic activity 23
A quiet period 31
More mountain building and deep erosion 32
Formation of the Yellowstone caldera 34
The eruption 38
The collapse 39
The outpouring of lava 44
Final sculpturing of the landscape 53
Glaciation 53
Running water—canyons and waterfalls 63
Grand Canyon of the Yellowstone 64
Hot-water and steam phenomena 71
How a thermal system operates 71
Hot-spring deposits and algae 75
Hot springs and geysers 79
Mudpots 82
Fumaroles 85
Thermal explosions 85
Faulting and its control of thermal activity 86
Earthquakes 87
The Park and man 89
Acknowledgments 90
Selected additional reading 91
Page
Foreword VII
Yellowstone country 1
A geological preview 4
Geologic history of the Yellowstone region 7
The nature of the rocks reveals their origins 7
The oldest rocks 7
The deposits of the shifting seas 13
The first mountain-building episode 19
Volcanic activity 23
A quiet period 31
More mountain building and deep erosion 32
Formation of the Yellowstone caldera 34
The eruption 38
The collapse 39
The outpouring of lava 44
Final sculpturing of the landscape 53
Glaciation 53
Running water—canyons and waterfalls 63
Grand Canyon of the Yellowstone 64
Hot-water and steam phenomena 71
How a thermal system operates 71
Hot-spring deposits and algae 75
Hot springs and geysers 79
Mudpots 82
Fumaroles 85
Thermal explosions 85
Faulting and its control of thermal activity 86
Earthquakes 87
The Park and man 89
Acknowledgments 90
Selected additional reading 91
Page 12
X
Figures
Page
Frontispiece Midway Geyser Basin II
Plate 1. Geologic map of Yellowstone National Park 36
Figure 1. Geographic map of Yellowstone National Park 2
2. Index map showing photograph localities 3
3. Skyline of the Gallatin Range in northwestern Yellowstone National Park 6
4. View north along the Yellowstone River and Hayden Valley toward the
Washburn Range
6
5. The rocks of Yellowstone National Park 8
6. The geologic time scale 10
7. View downstream along the Lamar River and closeup view of
Precambrian gneiss
12
8. Positions of seaways and landmasses during the middle part of Permian
time
14
9. Crowfoot Ridge in the southern Gallatin Range 15
10. Mount Everts 16
11. The faunal succession in sedimentary rocks 17
12. Beds of limestone along Pebble Creek and closeup views of outcrop and
fossils
18
13. Common kinds of geologic structures produced by deformation of the
earth’s crust
20
14. Geologic structures in Yellowstone National Park 22
15. Intrusive and extrusive igneous rock bodies 24
16. The Absaroka volcanoes and their rocks 25
17. Massive beds of volcanic breccia of the Absaroka volcanic rocks and
closeup view of outcrop
26
Figures
Page
Frontispiece Midway Geyser Basin II
Plate 1. Geologic map of Yellowstone National Park 36
Figure 1. Geographic map of Yellowstone National Park 2
2. Index map showing photograph localities 3
3. Skyline of the Gallatin Range in northwestern Yellowstone National Park 6
4. View north along the Yellowstone River and Hayden Valley toward the
Washburn Range
6
5. The rocks of Yellowstone National Park 8
6. The geologic time scale 10
7. View downstream along the Lamar River and closeup view of
Precambrian gneiss
12
8. Positions of seaways and landmasses during the middle part of Permian
time
14
9. Crowfoot Ridge in the southern Gallatin Range 15
10. Mount Everts 16
11. The faunal succession in sedimentary rocks 17
12. Beds of limestone along Pebble Creek and closeup views of outcrop and
fossils
18
13. Common kinds of geologic structures produced by deformation of the
earth’s crust
20
14. Geologic structures in Yellowstone National Park 22
15. Intrusive and extrusive igneous rock bodies 24
16. The Absaroka volcanoes and their rocks 25
17. Massive beds of volcanic breccia of the Absaroka volcanic rocks and
closeup view of outcrop
26
Page 13
18. Massive layered breccias of the Absaroka volcanic rocks at Barronette
Peak
28
19. Giant petrified tree trunks in Yellowstone’s fossil forest 29
20. Closeup view of a specimen of intrusive igneous rock 30
21. Bunsen Peak, a body of intrusive igneous rock 31
22. Outline of the Yellowstone caldera 35
23. Various stages in the development of the Yellowstone caldera 40
24. Extent of the rhyolite welded tuffs that once covered Yellowstone
National Park
42
25. The Yellowstone Tuff at Golden Gate and closeup views of tuff
specimens
43
26. Cross section through the Mount Washburn-Canyon area, showing
relationships along north edge of the Yellowstone caldera
44
27. View southeast across Yellowstone Lake toward the Absaroka Range 45
28. Radar image of lava flows in southwestern Yellowstone National Park 46
29. Obsidian Cliff 47
30. Thick rhyolite lava flow along Firehole River and closeup view of
specimen
48
31. Brecciated lava flows 49
32. Outcrop and closeup view of glassy rhyolite lava 50
33. Basalt flows at Tower and closeup views of outcrop and specimen 52
34. Giant glacial boulder of Precambrian gneiss at Inspiration Point 54
35. Glacial terrain along the Northeast Entrance Road 56
36. Typical profiles of canyons cut by stream erosion and glaciation 57
37. Aerial oblique view of Electric Peak 58
38. Extent of ice in Yellowstone National Park during the maximum
spreading of the Pinedale glaciers
60
39. Beds of sand, silt, and clay deposited in a glacially dammed lake in
Hayden Valley
61
40. Waterfalls in Yellowstone National Park 62
41. Grand Canyon and Lower Falls of the Yellowstone River 65
Peak
28
19. Giant petrified tree trunks in Yellowstone’s fossil forest 29
20. Closeup view of a specimen of intrusive igneous rock 30
21. Bunsen Peak, a body of intrusive igneous rock 31
22. Outline of the Yellowstone caldera 35
23. Various stages in the development of the Yellowstone caldera 40
24. Extent of the rhyolite welded tuffs that once covered Yellowstone
National Park
42
25. The Yellowstone Tuff at Golden Gate and closeup views of tuff
specimens
43
26. Cross section through the Mount Washburn-Canyon area, showing
relationships along north edge of the Yellowstone caldera
44
27. View southeast across Yellowstone Lake toward the Absaroka Range 45
28. Radar image of lava flows in southwestern Yellowstone National Park 46
29. Obsidian Cliff 47
30. Thick rhyolite lava flow along Firehole River and closeup view of
specimen
48
31. Brecciated lava flows 49
32. Outcrop and closeup view of glassy rhyolite lava 50
33. Basalt flows at Tower and closeup views of outcrop and specimen 52
34. Giant glacial boulder of Precambrian gneiss at Inspiration Point 54
35. Glacial terrain along the Northeast Entrance Road 56
36. Typical profiles of canyons cut by stream erosion and glaciation 57
37. Aerial oblique view of Electric Peak 58
38. Extent of ice in Yellowstone National Park during the maximum
spreading of the Pinedale glaciers
60
39. Beds of sand, silt, and clay deposited in a glacially dammed lake in
Hayden Valley
61
40. Waterfalls in Yellowstone National Park 62
41. Grand Canyon and Lower Falls of the Yellowstone River 65
Page 14
42. Various stages in the development of the Grand Canyon of the
Yellowstone
66
43. Common kinds of thermal features in Yellowstone National Park 70
44. Norris Geyser Basin, showing solid floor of hot spring deposits 72
45. Diagram of a thermal system 72
46. Infrared image of a portion of Upper Geyser Basin 73
47. Mound of geyserite (sinter) at Castle Geyser 75
48. Terraces of travertine at Opal Springs and closeup of specimen 76
49. Algal-colored terraces lining the west bank of the Firehole River 78
50. A geyser in action 80
51. Rock rubble surrounding Seismic Geyser in Upper Geyser Basin 83
52. Old Faithful in full eruption 84
53. Mud volcano near Pocket Basin in Lower Geyser Basin 86
54. Reactivation of a fault during the Hebgen Lake earthquake of August 17,
1959
88
1
Yellowstone
66
43. Common kinds of thermal features in Yellowstone National Park 70
44. Norris Geyser Basin, showing solid floor of hot spring deposits 72
45. Diagram of a thermal system 72
46. Infrared image of a portion of Upper Geyser Basin 73
47. Mound of geyserite (sinter) at Castle Geyser 75
48. Terraces of travertine at Opal Springs and closeup of specimen 76
49. Algal-colored terraces lining the west bank of the Firehole River 78
50. A geyser in action 80
51. Rock rubble surrounding Seismic Geyser in Upper Geyser Basin 83
52. Old Faithful in full eruption 84
53. Mud volcano near Pocket Basin in Lower Geyser Basin 86
54. Reactivation of a fault during the Hebgen Lake earthquake of August 17,
1959
88
1
Page 15
Yellowstone Country
The vivid descriptions brought back from the Yellowstone country by the
early explorers and trappers (see frontispiece), whose reputations for telling
tall tales were widely accepted if not altogether deserved, fell upon the
disbelieving ears of the nation for more than half a century. Yet the
intriguing rumors persisted, and during the years 1869-71 several
expeditions staffed partly by scientists and engineers rediscovered this
unique region atop the backbone of our nation. We now know that the
earliest visitors, even if prone to exaggerate, could not do justice to the long-
hidden secrets of Yellowstone, for none of them saw all of the fascinating
features that occur within this great National Park.
By the time the modern-day visitor enters Yellowstone National Park
through any of its five entrances, he probably will have traveled through
many parts of the Rocky Mountains and grown somewhat accustomed to the
“lay of the land.” But this will in no way lessen the exciting impact of
viewing the natural wonders of Yellowstone for the first time. Immediate
attention, of course, is still drawn to the remarkable array of geysers, hot
springs, and other thermal phenomena which in sheer numbers and variety
The vivid descriptions brought back from the Yellowstone country by the
early explorers and trappers (see frontispiece), whose reputations for telling
tall tales were widely accepted if not altogether deserved, fell upon the
disbelieving ears of the nation for more than half a century. Yet the
intriguing rumors persisted, and during the years 1869-71 several
expeditions staffed partly by scientists and engineers rediscovered this
unique region atop the backbone of our nation. We now know that the
earliest visitors, even if prone to exaggerate, could not do justice to the long-
hidden secrets of Yellowstone, for none of them saw all of the fascinating
features that occur within this great National Park.
By the time the modern-day visitor enters Yellowstone National Park
through any of its five entrances, he probably will have traveled through
many parts of the Rocky Mountains and grown somewhat accustomed to the
“lay of the land.” But this will in no way lessen the exciting impact of
viewing the natural wonders of Yellowstone for the first time. Immediate
attention, of course, is still drawn to the remarkable array of geysers, hot
springs, and other thermal phenomena which in sheer numbers and variety
Page 16
are unsurpassed throughout the world. But, as if these were not enough of an
attraction, nature has also provided an incredible setting of sparkling rivers
and lakes, thundering waterfalls and cataracts, awesome canyons and gorges,
and lofty glaciated mountain peaks and extinct volcanoes. Truly this is a land
apart, a spectacular masterpiece of nature that fully deserves the accolade of
“wonderland” bestowed long ago by early explorers and trappers. (See figs.
1 and 2.)
2
attraction, nature has also provided an incredible setting of sparkling rivers
and lakes, thundering waterfalls and cataracts, awesome canyons and gorges,
and lofty glaciated mountain peaks and extinct volcanoes. Truly this is a land
apart, a spectacular masterpiece of nature that fully deserves the accolade of
“wonderland” bestowed long ago by early explorers and trappers. (See figs.
1 and 2.)
2
Page 17
YELLOWSTONE NATIONAL PARK AREA, showing rivers, lakes, landforms,
roads, towns, settlements, and major geyser basins (stippled). The Park
embraces 3,472 square miles (2,221,770 acres), and its boundaries traverse a
roads, towns, settlements, and major geyser basins (stippled). The Park
embraces 3,472 square miles (2,221,770 acres), and its boundaries traverse a
Page 18
distance of nearly 300 miles. Yellowstone Lake, with an irregular shoreline of
110 miles and a surface area of 137 square miles, is one of the largest natural
mountain lakes in the United States. (Fig. 1)
3
INDEX MAP showing localities where photographs (and one sketch, fig. 35)
were taken to illustrate this bulletin. For photographs of distant views, arrows
point in direction of view. Numbers refer to figure numbers in text. (Fig. 2)
110 miles and a surface area of 137 square miles, is one of the largest natural
mountain lakes in the United States. (Fig. 1)
3
INDEX MAP showing localities where photographs (and one sketch, fig. 35)
were taken to illustrate this bulletin. For photographs of distant views, arrows
point in direction of view. Numbers refer to figure numbers in text. (Fig. 2)
Page 19
Beyond the first stirring impressions derived from the grandeur of the vast
Yellowstone wilderness and its myriad wildlife, assuredly shared by people
of all ages and from all walks of life, the various aspects of the Park take on
a very different meaning for different individuals. The artist sees grand vistas
to be painted, the naturalist delights in the flower-laden meadows and the
native habitats of many kinds of birds and animals, the engineer visualizes
the amount of energy stored in the waterfalls and steaming geysers, and so
on. To the geologist, in particular, who studies rocks and fossils and all 4
of the natural processes involved in shaping the surface of the land, and
to all those who would share such interests, Yellowstone takes on a very
special meaning. For the Park is foremost a geological Park, created by an
extraordinary sequence of natural processes and events that have combined
to produce an immense outdoor laboratory for studies that have contributed
to a fuller knowledge and a better understanding of the earth itself. The
geological aspect of the Yellowstone country is reflected by its very name,
given long ago to the river that issues from the great canyon of the “yellow
[1]
rocks.” This report, borrowing from a century of scientific study within
and around the Park area, describes the geological “how, why, and when” of
this unique and fascinating region.
A geological preview
Some 600,000 years ago the rumblings of an impending volcanic eruption
sounded ominously across the Yellowstone country. Suddenly, in a mighty
crescendo of deafening explosions, tremendous quantities of hot volcanic
ash and pumice spewed from giant cracks at the earth’s surface. Towering
dust clouds blackened the sky, and vast sheets of volcanic debris spread out
rapidly across the countryside in all directions, covering thousands of square
miles in a matter of minutes with a blanket of utter devastation. Abruptly, a
great smoldering pit—a caldera 30 miles across, 45 miles long, and several
thousand feet deep—appeared in the central Yellowstone region, the ground
having fallen into the huge underground cavern that was left by the earth-
shaking eruptions. Lava then began oozing from the cracks to fill the still-
smoking caldera.
Yellowstone wilderness and its myriad wildlife, assuredly shared by people
of all ages and from all walks of life, the various aspects of the Park take on
a very different meaning for different individuals. The artist sees grand vistas
to be painted, the naturalist delights in the flower-laden meadows and the
native habitats of many kinds of birds and animals, the engineer visualizes
the amount of energy stored in the waterfalls and steaming geysers, and so
on. To the geologist, in particular, who studies rocks and fossils and all 4
of the natural processes involved in shaping the surface of the land, and
to all those who would share such interests, Yellowstone takes on a very
special meaning. For the Park is foremost a geological Park, created by an
extraordinary sequence of natural processes and events that have combined
to produce an immense outdoor laboratory for studies that have contributed
to a fuller knowledge and a better understanding of the earth itself. The
geological aspect of the Yellowstone country is reflected by its very name,
given long ago to the river that issues from the great canyon of the “yellow
[1]
rocks.” This report, borrowing from a century of scientific study within
and around the Park area, describes the geological “how, why, and when” of
this unique and fascinating region.
A geological preview
Some 600,000 years ago the rumblings of an impending volcanic eruption
sounded ominously across the Yellowstone country. Suddenly, in a mighty
crescendo of deafening explosions, tremendous quantities of hot volcanic
ash and pumice spewed from giant cracks at the earth’s surface. Towering
dust clouds blackened the sky, and vast sheets of volcanic debris spread out
rapidly across the countryside in all directions, covering thousands of square
miles in a matter of minutes with a blanket of utter devastation. Abruptly, a
great smoldering pit—a caldera 30 miles across, 45 miles long, and several
thousand feet deep—appeared in the central Yellowstone region, the ground
having fallen into the huge underground cavern that was left by the earth-
shaking eruptions. Lava then began oozing from the cracks to fill the still-
smoking caldera.
Page 20
Thus, in one brief “moment” of geologic time there was launched that 5
incredible chain of events which led to the creation of many of the
natural wonders of Yellowstone National Park. Heat from the enormous
reservoir of molten rock which produced the massive eruption still remains
deep within the earth beneath Yellowstone, sustaining the spectacular hot-
water and steam phenomena for which the Park is so justly famous. The
formation of the caldera and the eruption of lavas profoundly influenced the
shape of the present-day landscape. Once a land covered almost entirely by
mountains, the part that collapsed—nearly one-third of the total Park area—
is now characterized by low rolling plateaus formed from the thick lava
flows that filled the caldera (figs. 1 and 2; see fig. 22 for the outline of the
Yellowstone caldera). Moreover, the carving of the spectacular Grand
Canyon of the Yellowstone (fig. 41) and the fashioning of the large interior
basin now occupied by beautiful Yellowstone Lake (fig. 27) were closely
related to this mighty volcanic event.
North, east, and south of the central plateaus are extensive mountain ranges
and other highlands which provide much of the Park’s scenic beauty (figs. 3
and 4). Formed by many episodes of intense mountain building and ancient
volcanism, these uplands bear the lasting imprints of a wide variety of
geological activities that date back approximately 2.7 billion years. Indeed,
as we study all the features of the Yellowstone landscape, we find in them a
most impressive and fascinating story of that ageless conflict between the
internal forces of nature that raise the land through the upheaval of
mountains and the eruption of volcanoes, and the external forces of erosion
that wear the land down. It is this vast relentless interplay of giant forces that
determines the appearance of any given place upon the earth’s surface. And,
in few other places around the globe can the processes of both building up
and tearing down the landscape be illustrated more dramatically than in
Yellowstone National Park.
6
incredible chain of events which led to the creation of many of the
natural wonders of Yellowstone National Park. Heat from the enormous
reservoir of molten rock which produced the massive eruption still remains
deep within the earth beneath Yellowstone, sustaining the spectacular hot-
water and steam phenomena for which the Park is so justly famous. The
formation of the caldera and the eruption of lavas profoundly influenced the
shape of the present-day landscape. Once a land covered almost entirely by
mountains, the part that collapsed—nearly one-third of the total Park area—
is now characterized by low rolling plateaus formed from the thick lava
flows that filled the caldera (figs. 1 and 2; see fig. 22 for the outline of the
Yellowstone caldera). Moreover, the carving of the spectacular Grand
Canyon of the Yellowstone (fig. 41) and the fashioning of the large interior
basin now occupied by beautiful Yellowstone Lake (fig. 27) were closely
related to this mighty volcanic event.
North, east, and south of the central plateaus are extensive mountain ranges
and other highlands which provide much of the Park’s scenic beauty (figs. 3
and 4). Formed by many episodes of intense mountain building and ancient
volcanism, these uplands bear the lasting imprints of a wide variety of
geological activities that date back approximately 2.7 billion years. Indeed,
as we study all the features of the Yellowstone landscape, we find in them a
most impressive and fascinating story of that ageless conflict between the
internal forces of nature that raise the land through the upheaval of
mountains and the eruption of volcanoes, and the external forces of erosion
that wear the land down. It is this vast relentless interplay of giant forces that
determines the appearance of any given place upon the earth’s surface. And,
in few other places around the globe can the processes of both building up
and tearing down the landscape be illustrated more dramatically than in
Yellowstone National Park.
6
Page 21
SKYLINE OF THE GALLATIN RANGE in northwestern Yellowstone National
Park, as viewed from a point on the road between Canyon Village and Norris
Junction. The range consists chiefly of Paleozoic and Mesozoic sedimentary
rocks and Precambrian metamorphic rocks that were uplifted by folding and
faulting of the earth’s crust. The dark-gray rocks along the roadcut in the left
foreground are rhyolite lava flows of the Solfatara Plateau. (Fig. 3)
Park, as viewed from a point on the road between Canyon Village and Norris
Junction. The range consists chiefly of Paleozoic and Mesozoic sedimentary
rocks and Precambrian metamorphic rocks that were uplifted by folding and
faulting of the earth’s crust. The dark-gray rocks along the roadcut in the left
foreground are rhyolite lava flows of the Solfatara Plateau. (Fig. 3)
Page 22
HAYDEN VALLEY. View north along the Yellowstone River and Hayden Valley
toward the Washburn Range. Mount Washburn, part of an ancient Absaroka
volcano, is the highest prominence (elevation, 10,293 feet) on the skyline to
the right, and Dunraven Pass is in the notch in the center of the skyline. The
foot of the range marks the north edge of the Yellowstone caldera. Hayden
Valley is cut in glacial lake sediments that overlie thick lava flows covering
the caldera floor. (Fig. 4)
7
toward the Washburn Range. Mount Washburn, part of an ancient Absaroka
volcano, is the highest prominence (elevation, 10,293 feet) on the skyline to
the right, and Dunraven Pass is in the notch in the center of the skyline. The
foot of the range marks the north edge of the Yellowstone caldera. Hayden
Valley is cut in glacial lake sediments that overlie thick lava flows covering
the caldera floor. (Fig. 4)
7
Page 23
Geologic History of the Yellowstone
Region
The nature of the rocks reveals their origins
Geologists believe that “the present is the key to the past.” After observing
lava erupting from a present-day volcano or limestone forming in marine
waters, we infer that similar types of ancient lavas or ancient limestones
formed in virtually the same ways. This kind of reasoning is used to interpret
the origins of all types of ancient rocks, for all the known geological
processes that form rocks seem to have been operating since the earth’s
beginning.
Figure 5 shows the many different rock units that have been recognized in
Yellowstone National Park. Arranged in a vertical column according to the
geologic time intervals in which they formed, these rocks represent a large
part of total earth history (fig. 6). A generalized geologic map (plate 1)
shows the distribution of the various units (or groups of closely related units)
exposed at the surface throughout the Park area. This map and figure 5
summarize much of the information that is necessary to interpret the Park’s
geologic history—in essence, to provide answers to these two important
Region
The nature of the rocks reveals their origins
Geologists believe that “the present is the key to the past.” After observing
lava erupting from a present-day volcano or limestone forming in marine
waters, we infer that similar types of ancient lavas or ancient limestones
formed in virtually the same ways. This kind of reasoning is used to interpret
the origins of all types of ancient rocks, for all the known geological
processes that form rocks seem to have been operating since the earth’s
beginning.
Figure 5 shows the many different rock units that have been recognized in
Yellowstone National Park. Arranged in a vertical column according to the
geologic time intervals in which they formed, these rocks represent a large
part of total earth history (fig. 6). A generalized geologic map (plate 1)
shows the distribution of the various units (or groups of closely related units)
exposed at the surface throughout the Park area. This map and figure 5
summarize much of the information that is necessary to interpret the Park’s
geologic history—in essence, to provide answers to these two important
Page 24
questions: What were the geologic events that formed the rocks? When did
these events occur?
The oldest rocks
If we were to walk backward in time at the rate of one century per step, the
first step would return us to 1872, the year that Yellowstone National Park
was established. But to return to the oldest recorded event in its geologic
history, we would have to walk (at 3 feet per step) some 15,000 miles, or
three-fifths of the way around the world! Occurring far back in the antiquity
of the Precambrian Era—approximately 2.7 billion years ago according to
radiometric dating (fig. 6)—the oldest event resulted in rocks so crumpled
and changed by heat and pressure that their original character is obscure.
These rocks, having been transformed from still older ones, are called
metamorphic rocks. Considered to form part of the very foundation of the
continent itself, they are also commonly referred to as basement rocks.
8
these events occur?
The oldest rocks
If we were to walk backward in time at the rate of one century per step, the
first step would return us to 1872, the year that Yellowstone National Park
was established. But to return to the oldest recorded event in its geologic
history, we would have to walk (at 3 feet per step) some 15,000 miles, or
three-fifths of the way around the world! Occurring far back in the antiquity
of the Precambrian Era—approximately 2.7 billion years ago according to
radiometric dating (fig. 6)—the oldest event resulted in rocks so crumpled
and changed by heat and pressure that their original character is obscure.
These rocks, having been transformed from still older ones, are called
metamorphic rocks. Considered to form part of the very foundation of the
continent itself, they are also commonly referred to as basement rocks.
8
Page 25
THE ROCKS of Yellowstone National Park, separated into individual units or
formations and arranged according to their geologic ages (see fig. 6). A
formation is a body of rock that contains certain identifying features (such as
composition, color, and fossils) which set it apart from all other rock units.
The identifying features of each formation provide valuable clues bearing on
its origin. Most formations are given formal names, and usually each
formation is thick and widespread enough to be recognized over broad areas.
Some, however, change character from place to place, and different names
may be used in different areas even though the rocks represent the same
geologic time interval. (Fig. 5)
High-resolution Version
AGE, IN THOUSANDS OF YEARS ROCK FORMATION OR UNIT
40± to present Stream sand and gravel
Hot-spring deposits
9 to 250± Glacial deposits
60 to 600 Plateau Rhyolite
600 Upper Unit, Yellowstone Tuff
600 to 2,000 Rhyolite and basalt lava flows
formations and arranged according to their geologic ages (see fig. 6). A
formation is a body of rock that contains certain identifying features (such as
composition, color, and fossils) which set it apart from all other rock units.
The identifying features of each formation provide valuable clues bearing on
its origin. Most formations are given formal names, and usually each
formation is thick and widespread enough to be recognized over broad areas.
Some, however, change character from place to place, and different names
may be used in different areas even though the rocks represent the same
geologic time interval. (Fig. 5)
High-resolution Version
AGE, IN THOUSANDS OF YEARS ROCK FORMATION OR UNIT
40± to present Stream sand and gravel
Hot-spring deposits
9 to 250± Glacial deposits
60 to 600 Plateau Rhyolite
600 Upper Unit, Yellowstone Tuff
600 to 2,000 Rhyolite and basalt lava flows
Page 26
2,000 Lower Unit, Yellowstone Tuff
2,000+ Rhyolite and basalt lava flows
KINDS OF ROCKS SHOWN IN COLUMNS
Sandstone or stream sand
Conglomerate, glacial moraines, or stream gravels
Volcanic breccia
Shale
Limestone
Dolomite
Lava flows
Welded tuff
Travertine or geyserite
ROCK FORMATIONS AGE, IN
MILLIONS
Northern part of park Southern part of park OF YEARS PERIOD ERA
Thick lava flows, welded tuffs, glacial deposits, QUATERNARY CENOZOIC
and hot-spring deposits
2-3
Pliocene, Miocene, and Oligocene rocks not
known to be present
37-38
Absaroka volcanic Absaroka volcanic rocks TERTIARY
rocks (Eocene)
53-54
Volcanic and Pinyon Conglomerate
sedimentary rocks (Paleocene and
(largely eroded away Cretaceous)
before Absaroka
volcanic rocks were
deposited)
65
Landslide Creek Fm Harebell Formation CRETACEOUS MESOZOIC
Everts Formation (Eroded away before
Harebell was deposited)
Eagle Sandstone Bacon Ridge Sandstone
Telegraph Creek Fm ″
Cody Shale Cody Shale
Frontier Formation Frontier Formation
Mowry Shale Mowry Shale
Thermopolis Shale Thermopolis Shale
2,000+ Rhyolite and basalt lava flows
KINDS OF ROCKS SHOWN IN COLUMNS
Sandstone or stream sand
Conglomerate, glacial moraines, or stream gravels
Volcanic breccia
Shale
Limestone
Dolomite
Lava flows
Welded tuff
Travertine or geyserite
ROCK FORMATIONS AGE, IN
MILLIONS
Northern part of park Southern part of park OF YEARS PERIOD ERA
Thick lava flows, welded tuffs, glacial deposits, QUATERNARY CENOZOIC
and hot-spring deposits
2-3
Pliocene, Miocene, and Oligocene rocks not
known to be present
37-38
Absaroka volcanic Absaroka volcanic rocks TERTIARY
rocks (Eocene)
53-54
Volcanic and Pinyon Conglomerate
sedimentary rocks (Paleocene and
(largely eroded away Cretaceous)
before Absaroka
volcanic rocks were
deposited)
65
Landslide Creek Fm Harebell Formation CRETACEOUS MESOZOIC
Everts Formation (Eroded away before
Harebell was deposited)
Eagle Sandstone Bacon Ridge Sandstone
Telegraph Creek Fm ″
Cody Shale Cody Shale
Frontier Formation Frontier Formation
Mowry Shale Mowry Shale
Thermopolis Shale Thermopolis Shale
Page 27
Kootenai Formation Cloverly Formation
136
Morrison Formation Morrison(?) Fm JURASSIC
Swift Formation Sundance Formation
Rierdon Formation ″
Sawtooth Formation Gypsum Spring Fm
190-195
Woodside & Chugwater Formation TRIASSIC
Thaynes(?)
Formations
Dinwoody Formation Dinwoody Formation
225
Shedhorn Sandstone Phosphoria Fm and PERMIAN PALEOZOIC
related rocks
280
Quadrant Sandstone Tensleep Formation PENNSYLVANIAN
Amsden Formation Amsden Formation
Mission Canyon Madison Limestone MISSISSIPIAN
Limestone
Lodgepole Limestone ″
345
Three Forks Fm Darby Formation DEVONIAN
Jefferson Formation ″
Bighorn Dolomite (Not exposed, except for ORDOVICIAN
isolated outcrops of
some formations in Falls
River area, in
southwestern part of
park)
500
Snowy Range Fm ″ CAMBRIAN
Pilgrim Limestone
Park Shale
Meagher Limestone
Wolsey Shale
Flathead Sandstone
570
Gneiss and Schist (Not exposed) PRECAMBRIAN
2,700
10
A
CENOZOIC
50 M.Y.
136
Morrison Formation Morrison(?) Fm JURASSIC
Swift Formation Sundance Formation
Rierdon Formation ″
Sawtooth Formation Gypsum Spring Fm
190-195
Woodside & Chugwater Formation TRIASSIC
Thaynes(?)
Formations
Dinwoody Formation Dinwoody Formation
225
Shedhorn Sandstone Phosphoria Fm and PERMIAN PALEOZOIC
related rocks
280
Quadrant Sandstone Tensleep Formation PENNSYLVANIAN
Amsden Formation Amsden Formation
Mission Canyon Madison Limestone MISSISSIPIAN
Limestone
Lodgepole Limestone ″
345
Three Forks Fm Darby Formation DEVONIAN
Jefferson Formation ″
Bighorn Dolomite (Not exposed, except for ORDOVICIAN
isolated outcrops of
some formations in Falls
River area, in
southwestern part of
park)
500
Snowy Range Fm ″ CAMBRIAN
Pilgrim Limestone
Park Shale
Meagher Limestone
Wolsey Shale
Flathead Sandstone
570
Gneiss and Schist (Not exposed) PRECAMBRIAN
2,700
10
A
CENOZOIC
50 M.Y.
Page 28
MESOZOIC
200 M.Y.
PALEOZOIC
500 M.Y.
PRECAMBRIAN
4.5 B.Y.
B
Quaternary—Early man
2
Tertiary
65
Cretaceous
140
Jurassic
190
Triassic
220
Permian
280
Pennsylvanian
310
Mississippian
340
Devonian
390
Silurian
440
Ordovician
500
Cambrian
575 First abundant fossils
Precambrian
2700 Oldest rocks in Yellowstone
Beginning of the earth
4,500 M.Y.
C
PRINCIPAL EVENTS
Holocene
200 M.Y.
PALEOZOIC
500 M.Y.
PRECAMBRIAN
4.5 B.Y.
B
Quaternary—Early man
2
Tertiary
65
Cretaceous
140
Jurassic
190
Triassic
220
Permian
280
Pennsylvanian
310
Mississippian
340
Devonian
390
Silurian
440
Ordovician
500
Cambrian
575 First abundant fossils
Precambrian
2700 Oldest rocks in Yellowstone
Beginning of the earth
4,500 M.Y.
C
PRINCIPAL EVENTS
Holocene
Page 29
Glaciation, canyon cutting, thermal activity, eruption of Plateau
Rhyolite
Pleistocene
Eruption of Yellowstone Tuff and associated lava flow; collapse of
Yellowstone caldera; normal faulting
2
Pliocene
Regional uplift; large-scale normal faulting and uplift of mountain
ranges; deep erosion
12
Miocene
Moderate erosion; possibly some volcanic activity
26
Oligocene
″
37
Eocene
Eruption and deposition of Absaroka volcanic rocks
54
Paleocene
Laramide Orogeny—folding, faulting, uplift and erosion of mountain
ranges; deposition of sand and gravel in subsiding basins
65
Cretaceous
Deposition of sediments in oceans and along beaches and river flood
plains
...
Cambrian
570 M.Y.
Rhyolite
Pleistocene
Eruption of Yellowstone Tuff and associated lava flow; collapse of
Yellowstone caldera; normal faulting
2
Pliocene
Regional uplift; large-scale normal faulting and uplift of mountain
ranges; deep erosion
12
Miocene
Moderate erosion; possibly some volcanic activity
26
Oligocene
″
37
Eocene
Eruption and deposition of Absaroka volcanic rocks
54
Paleocene
Laramide Orogeny—folding, faulting, uplift and erosion of mountain
ranges; deposition of sand and gravel in subsiding basins
65
Cretaceous
Deposition of sediments in oceans and along beaches and river flood
plains
...
Cambrian
570 M.Y.
Page 30
THE GEOLOGIC TIME SCALE—the “calendar” used by geologists in
interpreting earth history. Column A, graduated in billions of years (B.Y.) and
subdivided into the four major geologic eras (Precambrian, for example),
represents the time elapsed since the beginning of the earth, which is
interpreting earth history. Column A, graduated in billions of years (B.Y.) and
subdivided into the four major geologic eras (Precambrian, for example),
represents the time elapsed since the beginning of the earth, which is
Page 31
believed to have been about 4.5 billion years ago. Column B is an expansion
of part of the time scale in millions of years (M.Y.), to show the subdivisions
(periods—Cambrian, for example) of the Paleozoic, Mesozoic, and Cenozoic
Eras; column C is a further expansion to show particularly the subdivisions
(epochs—Paleocene, for example) of the Tertiary and Quaternary Periods. The
principal events in the geologic history of Yellowstone National Park are listed
to the right of column C, opposite the time intervals in which they occurred.
The ages, in years, are based on radiometric dating. Many rocks contain
radioactive elements which begin to decay at a very slow but measurable rate
as soon as the parent rock is formed. The most common radioactive elements
are uranium, rubidium, and potassium, and their decay (“daughter”) products
are lead, strontium, and argon, respectively. By measuring both the amount of
a given daughter product and the amount of the original radioactive element
still remaining in the parent rock, and then relating these measurements to
their known rate of radioactive decay, the age of the rock in actual numbers of
years can be calculated. The decay of radioactive carbon (carbon-14) to
nitrogen is especially useful for dating rocks less than 40,000 years old. (Fig.
6)
Gneiss, a coarsely banded rock (fig. 7), and schist, a finely banded 11
rock, are the most common kinds of metamorphic rocks in
Yellowstone. Originally, the gneiss probably was granite, and the schist was
a shale or sandstone. Outcrops of the gneisses and schists occur only in the
northern part of the Park (pl. 1), where they form the central cores of some
mountain ranges such as the Gallatin Range (fig. 3). They also lie buried
beneath younger rocks in many other areas of the Park.
From the time of the metamorphic event, when the gneisses and schists were
formed, until the deposition of sediments of the Cambrian Period (figs. 5 and
6), there is virtually no record. It is reasonably certain, however, that several
times during this 2.1-billion-year interval the region was intensely squeezed
and uplifted into high mountains and then deeply eroded. By the end of
Precambrian time, approximately 570 million years ago, the ancient
Yellowstone landscape had been reduced by erosion to a flat, stark, almost
featureless plain, which was soon to be flooded by a shallow sea
encroaching from the west. This very old surface is now partly exposed in
some places across the Buffalo Plateau, at the north edge of the Park (fig. 1).
12
of part of the time scale in millions of years (M.Y.), to show the subdivisions
(periods—Cambrian, for example) of the Paleozoic, Mesozoic, and Cenozoic
Eras; column C is a further expansion to show particularly the subdivisions
(epochs—Paleocene, for example) of the Tertiary and Quaternary Periods. The
principal events in the geologic history of Yellowstone National Park are listed
to the right of column C, opposite the time intervals in which they occurred.
The ages, in years, are based on radiometric dating. Many rocks contain
radioactive elements which begin to decay at a very slow but measurable rate
as soon as the parent rock is formed. The most common radioactive elements
are uranium, rubidium, and potassium, and their decay (“daughter”) products
are lead, strontium, and argon, respectively. By measuring both the amount of
a given daughter product and the amount of the original radioactive element
still remaining in the parent rock, and then relating these measurements to
their known rate of radioactive decay, the age of the rock in actual numbers of
years can be calculated. The decay of radioactive carbon (carbon-14) to
nitrogen is especially useful for dating rocks less than 40,000 years old. (Fig.
6)
Gneiss, a coarsely banded rock (fig. 7), and schist, a finely banded 11
rock, are the most common kinds of metamorphic rocks in
Yellowstone. Originally, the gneiss probably was granite, and the schist was
a shale or sandstone. Outcrops of the gneisses and schists occur only in the
northern part of the Park (pl. 1), where they form the central cores of some
mountain ranges such as the Gallatin Range (fig. 3). They also lie buried
beneath younger rocks in many other areas of the Park.
From the time of the metamorphic event, when the gneisses and schists were
formed, until the deposition of sediments of the Cambrian Period (figs. 5 and
6), there is virtually no record. It is reasonably certain, however, that several
times during this 2.1-billion-year interval the region was intensely squeezed
and uplifted into high mountains and then deeply eroded. By the end of
Precambrian time, approximately 570 million years ago, the ancient
Yellowstone landscape had been reduced by erosion to a flat, stark, almost
featureless plain, which was soon to be flooded by a shallow sea
encroaching from the west. This very old surface is now partly exposed in
some places across the Buffalo Plateau, at the north edge of the Park (fig. 1).
12
Page 32
LAMAR RIVER. View downstream (west) along the Lamar River in Lamar
Canyon. The rocks along the river banks are coarsely banded Precambrian
gneisses more than 2.5 billion years old, some of the oldest rocks in
Yellowstone National Park. (Fig. 7)
Canyon. The rocks along the river banks are coarsely banded Precambrian
gneisses more than 2.5 billion years old, some of the oldest rocks in
Yellowstone National Park. (Fig. 7)
Page 33
Closeup views show coarse banding and texture of the gneiss; minerals
include quartz, feldspar, and biotite (black mica).
13
The deposits of the shifting seas
From the appearance of the rugged, mountainous terrain of Yellowstone
National Park, it is difficult to visualize a time when this region lay close to
sea level, at times even below sea level. Yet the evidence is clear that from
the Cambrian Period to the latter part of the Cretaceous Period, a span of
about 500 million years, vast stretches of western lands were flooded
repeatedly by broad shallow seas that often reached from Canada to Mexico
(fig. 8). During these great floodings, widespread horizontal beds of sand,
silt, clay, limy mud, and other sediments were deposited on the ocean floors,
include quartz, feldspar, and biotite (black mica).
13
The deposits of the shifting seas
From the appearance of the rugged, mountainous terrain of Yellowstone
National Park, it is difficult to visualize a time when this region lay close to
sea level, at times even below sea level. Yet the evidence is clear that from
the Cambrian Period to the latter part of the Cretaceous Period, a span of
about 500 million years, vast stretches of western lands were flooded
repeatedly by broad shallow seas that often reached from Canada to Mexico
(fig. 8). During these great floodings, widespread horizontal beds of sand,
silt, clay, limy mud, and other sediments were deposited on the ocean floors,
Page 34
along the adjoining beaches and wide tidal flats, and across the broad flood
plains of large rivers that emptied into the seas. All of these ancient
sediments have now hardened into compact well-layered sandstones, shales,
and limestones (figs. 9 and 10). These sedimentary rocks have been divided
into 25 or more distinct formations in the Yellowstone region (fig. 5), where
they locally attain a combined thickness of more than 10,000 feet.
The first Paleozoic sea to reach the Yellowstone region, some 550 million
years ago, brought with it the earliest abundant signs of life on earth. Small
hard-shelled animals that lived mainly on the shallow sea bottom are now
preserved as fossils in rocks deposited during the Cambrian Period. Many of
these animals were trilobites, long-extinct organisms resembling today’s
crabs and spiders. Each younger set of rocks or formations contains a
different group of dominant fossils, each diagnostic of that period of
geologic time in which they lived (fig. 11).
14
plains of large rivers that emptied into the seas. All of these ancient
sediments have now hardened into compact well-layered sandstones, shales,
and limestones (figs. 9 and 10). These sedimentary rocks have been divided
into 25 or more distinct formations in the Yellowstone region (fig. 5), where
they locally attain a combined thickness of more than 10,000 feet.
The first Paleozoic sea to reach the Yellowstone region, some 550 million
years ago, brought with it the earliest abundant signs of life on earth. Small
hard-shelled animals that lived mainly on the shallow sea bottom are now
preserved as fossils in rocks deposited during the Cambrian Period. Many of
these animals were trilobites, long-extinct organisms resembling today’s
crabs and spiders. Each younger set of rocks or formations contains a
different group of dominant fossils, each diagnostic of that period of
geologic time in which they lived (fig. 11).
14
Page 35
MIDDLE PERMIAN SEAS. Distribution of sea (blue) and land (red) during the
middle part of Permian time (approximately 250 million years ago). Only a part
of the Yellowstone National Park area (black) was flooded during this period.
(Fig. 8)
middle part of Permian time (approximately 250 million years ago). Only a part
of the Yellowstone National Park area (black) was flooded during this period.
(Fig. 8)
Page 36
Fossils indicate the kind of environment in which the animals lived 15
(fig. 12). Some species thrived in the open oceans; others thrived only
along the beaches and in nearby lagoons. Still others, such as the incredibly
large dinosaurs of the Jurassic and Cretaceous Periods, could survive only on
the land or in swamps. From studies of the fossils and of the physical
characteristics of the rocks in which they are now found, the shoreline
patterns of the shifting seas can be determined. Studies show that the seas
advanced and retreated across the Yellowstone Park region at least a dozen
times during the Paleozoic and Mesozoic Eras.
Toward the end of the Mesozoic Era (in the latter part of the Cretaceous
Period), the metamorphic basement rocks of Yellowstone lay covered by the
vast blanket of flat-lying sediments. Today, these sedimentary rocks are
exposed along the Snake River and its tributaries in the south-central part of
the Park, over much of the Gallatin Range in the northwest corner, and at
several places in the north-central and northeastern parts (pl. 1). Elsewhere,
either they are hidden from view beneath volcanic debris—ash and lava—
that later buried them, or they have been removed by erosion. But wherever
exposed, the original horizontal layers of sedimentary rocks have been
severely twisted and broken by later mountain-building movements.
(fig. 12). Some species thrived in the open oceans; others thrived only
along the beaches and in nearby lagoons. Still others, such as the incredibly
large dinosaurs of the Jurassic and Cretaceous Periods, could survive only on
the land or in swamps. From studies of the fossils and of the physical
characteristics of the rocks in which they are now found, the shoreline
patterns of the shifting seas can be determined. Studies show that the seas
advanced and retreated across the Yellowstone Park region at least a dozen
times during the Paleozoic and Mesozoic Eras.
Toward the end of the Mesozoic Era (in the latter part of the Cretaceous
Period), the metamorphic basement rocks of Yellowstone lay covered by the
vast blanket of flat-lying sediments. Today, these sedimentary rocks are
exposed along the Snake River and its tributaries in the south-central part of
the Park, over much of the Gallatin Range in the northwest corner, and at
several places in the north-central and northeastern parts (pl. 1). Elsewhere,
either they are hidden from view beneath volcanic debris—ash and lava—
that later buried them, or they have been removed by erosion. But wherever
exposed, the original horizontal layers of sedimentary rocks have been
severely twisted and broken by later mountain-building movements.
Page 37
CROWFOOT RIDGE in the southern Gallatin Range, as viewed from the road
along the Gallatin River near the northwest corner of Yellowstone National
Park. The rocks, chiefly Paleozoic limestone, sandstone, and shale, were
deposited in broad shallow seas that covered all of the Yellowstone region
several hundred million years ago. The original layers were horizontal, but
they have since been tilted and broken by giant mountain-building forces
originating deep within the earth. (Fig. 9)
16
along the Gallatin River near the northwest corner of Yellowstone National
Park. The rocks, chiefly Paleozoic limestone, sandstone, and shale, were
deposited in broad shallow seas that covered all of the Yellowstone region
several hundred million years ago. The original layers were horizontal, but
they have since been tilted and broken by giant mountain-building forces
originating deep within the earth. (Fig. 9)
16
Page 38
MOUNT EVERTS, as viewed toward the northeast from the road south of
Mammoth Hot Springs. The mountain, about 1,500 feet high above the plain,
is formed by gently tilted sedimentary rocks of Cretaceous age, chiefly
sandstone and shale of the Frontier, Cody, and Everts Formations (fig. 5). The
conspicuous rimrock at the top of the mountain to the right is composed of
the Yellowstone Tuff. When the tuff was deposited (by explosive eruptions
from the south), there was no valley along the edge of the mountain. (Fig. 10)
17
FAUNAL SUCCESSION in sedimentary rocks. The different animals are now
preserved as fossils, which are diagnostic of the period in which the animals
Mammoth Hot Springs. The mountain, about 1,500 feet high above the plain,
is formed by gently tilted sedimentary rocks of Cretaceous age, chiefly
sandstone and shale of the Frontier, Cody, and Everts Formations (fig. 5). The
conspicuous rimrock at the top of the mountain to the right is composed of
the Yellowstone Tuff. When the tuff was deposited (by explosive eruptions
from the south), there was no valley along the edge of the mountain. (Fig. 10)
17
FAUNAL SUCCESSION in sedimentary rocks. The different animals are now
preserved as fossils, which are diagnostic of the period in which the animals
Page 39
lived. (Fig. 11)
Man
CENOZOIC QUATERNARY and TERTIARY Mammals
CRETACEOUS
MESOZOIC JURASSIC Dinosaurs
TRIASSIC
PERMIAN Reptiles
PENNSYLVANIAN Amphibians
MISSISSIPPIAN
PALEOZOIC DEVONIAN Fishes
SILURIAN Sea scorpions
ORDOVICIAN Nautiloids
CAMBRIAN Trilobytes
PRE-CAMBRIAN Soft-bodied creatures
18
Man
CENOZOIC QUATERNARY and TERTIARY Mammals
CRETACEOUS
MESOZOIC JURASSIC Dinosaurs
TRIASSIC
PERMIAN Reptiles
PENNSYLVANIAN Amphibians
MISSISSIPPIAN
PALEOZOIC DEVONIAN Fishes
SILURIAN Sea scorpions
ORDOVICIAN Nautiloids
CAMBRIAN Trilobytes
PRE-CAMBRIAN Soft-bodied creatures
18
Page 40
LIMESTONE OF MISSISSIPPIAN AGE along Pebble Creek at the Pebble Creek
campground, northeastern Yellowstone National Park. (Fig. 12)
campground, northeastern Yellowstone National Park. (Fig. 12)
Page 41
Closeup A shows one of the highly fossiliferous layers within the limestone.
Page 42
Closeup B shows some of the fossils and their casts. Most of the fossils are
of a variety of shelled sea animals (brachiopods) that lived on the ocean
floors approximately 300 million years ago.
19
The first mountain-building episode
of a variety of shelled sea animals (brachiopods) that lived on the ocean
floors approximately 300 million years ago.
19
The first mountain-building episode
Page 43
Near the close of the Mesozoic Era the earth was subjected to a series of
intense crustal disturbances that geologists call the Laramide orogeny
(orogeny means mountain-building). The origin and nature of the forces that
bent and cracked the crust are unknown, but current theories being
developed about sea-floor spreading and continental drift may shed light on
this major upheaval that began about 75 million years ago. A significant
effect of the Laramide orogeny was the uplift and contortion of many of the
mountain ranges within what we today call the Rocky Mountains.
At the onset of the crustal disturbance, the gently rolling landscape of the
Yellowstone region began to warp and flex into large upfolds (anticlines)
and downfolds (synclines) (fig. 13). Gradually the mountain-building
pressures increased, finally reaching such magnitude that the limbs of the
folds could bend and stretch no further; thereupon, the rock layers broke and
were shoved over one another along extensive reverse faults. The severely
crumpled rocks within the Park area can now be seen only along the north
edge and in the south-central part along the Snake River. In both places, the
folds and faults are especially well displayed by the layered Paleozoic and
Mesozoic sedimentary formations (fig. 9).
One of the most prominent Laramide structural features is a large anticline in
the north-central and northeastern parts of the Park (fig. 14, section B-B′);
the road from Mammoth to the Northeast Entrance crosses much of this
feature (pl. 1). Although originally forming a high mountain mass, the
anticline has been eroded so extensively that it no longer appears
mountainous (fig. 18). It displays a broad core of Precambrian gneisses and
schists and is bounded along its southwest margin by a large reverse fault.
Along the fault, the ancient gneisses and schists have been shoved over
rocks as young as Late Cretaceous, a movement amounting to 10,000 feet or
more. The Cretaceous rocks are those that are now exposed at Mount Everts
(fig. 10).
20
intense crustal disturbances that geologists call the Laramide orogeny
(orogeny means mountain-building). The origin and nature of the forces that
bent and cracked the crust are unknown, but current theories being
developed about sea-floor spreading and continental drift may shed light on
this major upheaval that began about 75 million years ago. A significant
effect of the Laramide orogeny was the uplift and contortion of many of the
mountain ranges within what we today call the Rocky Mountains.
At the onset of the crustal disturbance, the gently rolling landscape of the
Yellowstone region began to warp and flex into large upfolds (anticlines)
and downfolds (synclines) (fig. 13). Gradually the mountain-building
pressures increased, finally reaching such magnitude that the limbs of the
folds could bend and stretch no further; thereupon, the rock layers broke and
were shoved over one another along extensive reverse faults. The severely
crumpled rocks within the Park area can now be seen only along the north
edge and in the south-central part along the Snake River. In both places, the
folds and faults are especially well displayed by the layered Paleozoic and
Mesozoic sedimentary formations (fig. 9).
One of the most prominent Laramide structural features is a large anticline in
the north-central and northeastern parts of the Park (fig. 14, section B-B′);
the road from Mammoth to the Northeast Entrance crosses much of this
feature (pl. 1). Although originally forming a high mountain mass, the
anticline has been eroded so extensively that it no longer appears
mountainous (fig. 18). It displays a broad core of Precambrian gneisses and
schists and is bounded along its southwest margin by a large reverse fault.
Along the fault, the ancient gneisses and schists have been shoved over
rocks as young as Late Cretaceous, a movement amounting to 10,000 feet or
more. The Cretaceous rocks are those that are now exposed at Mount Everts
(fig. 10).
20
Page 44
COMMON KINDS OF GEOLOGIC STRUCTURES produced by deformation of
the earth’s crust. An original horizontal rock layer may be upfolded into
anticlines, downfolded into synclines, and broken by either reverse or normal
faults. A fault is a fracture or a zone of fractures within the earth’s crust along
which movement has taken place. A reverse fault is one generally produced
by compression (squeezing together), and the hanging-wall block has moved
up with respect to the footwall block. A normal fault is one generally produced
by tension (pulling apart), and the hanging-wall block has moved down with
respect to the footwall block. All these kinds of structures are present in
Yellowstone National Park. (Fig. 13)
HORIZONTAL (undeformed)
the earth’s crust. An original horizontal rock layer may be upfolded into
anticlines, downfolded into synclines, and broken by either reverse or normal
faults. A fault is a fracture or a zone of fractures within the earth’s crust along
which movement has taken place. A reverse fault is one generally produced
by compression (squeezing together), and the hanging-wall block has moved
up with respect to the footwall block. A normal fault is one generally produced
by tension (pulling apart), and the hanging-wall block has moved down with
respect to the footwall block. All these kinds of structures are present in
Yellowstone National Park. (Fig. 13)
HORIZONTAL (undeformed)
Page 45
REVERSE FAULT (compressional)
Hanging wall
Footwall
Forces
ANTICLINE (upfold)
Crest
Limb
NORMAL FAULT (tensional)
Footwall
Hanging wall
Forces
SYNCLINE (downfold)
Limb
Trough
During the Laramide orogeny, many folds and faults formed in the 21
northwestern part of the Park, in the area now occupied by the Gallatin
Range (fig. 14, section A-A′). In south-central Yellowstone, the Paleozoic
and Mesozoic sedimentary rocks were tightly folded into three anticlines
separated from one another by synclines and faults (fig. 14, section C-C′).
Movement along one reverse fault in this area was locally more than 10,000
feet.
As the lands were uplifted and contorted, they came under vigorous attack
by the ever-present agents of erosion. Tremendous quantities of rock were
stripped from the highlands, and the debris was carried by streams into the
adjacent lowland basins and deposited mostly as sand and gravel. As the
highlands continued to rise, the basins continued to sink, and in a short
period of time great thicknesses of basin-fill sediments accumulated locally.
One such deposit, the Harebell Formation of latest Cretaceous age in south-
central Yellowstone (fig. 5), is more than 8,000 feet thick.
Other similar anticlines, synclines, and reverse faults no doubt extend far
into the interior of Yellowstone National Park, and perhaps entirely across it
in places, but they lie buried beneath a thick capping of volcanic rocks.
Nevertheless, it seems safe to conclude that none of the Park area escaped
the effects of the great forces of the Laramide orogeny. These forces,
regardless of how they originated deep within the earth, seem to have been
compressional (fig. 13), pushing the upper layers of the earth’s crust from
the east and northeast toward the west and southwest. This interpretation is
based on the style of the structural features just described, which shows that
Hanging wall
Footwall
Forces
ANTICLINE (upfold)
Crest
Limb
NORMAL FAULT (tensional)
Footwall
Hanging wall
Forces
SYNCLINE (downfold)
Limb
Trough
During the Laramide orogeny, many folds and faults formed in the 21
northwestern part of the Park, in the area now occupied by the Gallatin
Range (fig. 14, section A-A′). In south-central Yellowstone, the Paleozoic
and Mesozoic sedimentary rocks were tightly folded into three anticlines
separated from one another by synclines and faults (fig. 14, section C-C′).
Movement along one reverse fault in this area was locally more than 10,000
feet.
As the lands were uplifted and contorted, they came under vigorous attack
by the ever-present agents of erosion. Tremendous quantities of rock were
stripped from the highlands, and the debris was carried by streams into the
adjacent lowland basins and deposited mostly as sand and gravel. As the
highlands continued to rise, the basins continued to sink, and in a short
period of time great thicknesses of basin-fill sediments accumulated locally.
One such deposit, the Harebell Formation of latest Cretaceous age in south-
central Yellowstone (fig. 5), is more than 8,000 feet thick.
Other similar anticlines, synclines, and reverse faults no doubt extend far
into the interior of Yellowstone National Park, and perhaps entirely across it
in places, but they lie buried beneath a thick capping of volcanic rocks.
Nevertheless, it seems safe to conclude that none of the Park area escaped
the effects of the great forces of the Laramide orogeny. These forces,
regardless of how they originated deep within the earth, seem to have been
compressional (fig. 13), pushing the upper layers of the earth’s crust from
the east and northeast toward the west and southwest. This interpretation is
based on the style of the structural features just described, which shows that
Page 46
the steep limbs of folds, as well as the direction of movements along reverse
faults, point toward the west or southwest (fig. 14).
By early Eocene time, about 20 million years after they had begun, the
deformational forces relaxed. But the effects of the giant earth movements
were to last for a very long time. Crustal disturbances of such magnitude
commonly produce conditions deep within the earth which, in places, gives
rise to intense volcanic activity; one such place was Yellowstone.
22
CROSS SECTIONS SHOWING GEOLOGIC STRUCTURES in Yellowstone
National Park. These illustrate the possible rock relationships that might be
seen along the faces of vertical slices of the earth’s crust, if it could be cut
and pulled apart (much like slicing a cake and looking at the different layers).
The locations of the sections are shown on the geologic map, plate 1. Reverse
faults and most folds originated during the Larimide orogeny, and normal
faults originated chiefly during Pliocene and later times. The arrows indicate
the relative movements of fault blocks. Geologic symbols: Qs, Quaternary
superficial deposits; Qb, Quaternary basalt flows; Qy, Quaternary Yellowstone
tuff; Tav, Tertiary Absaroka volcanic rocks; Mzr, Mesozoic sedimentary rocks;
Pzr, Paleozoic sedimentary rocks; pCr, Precambrian metamorphic
(“basement”) rocks. (Based partly on information supplied by E. T. Ruppel
and J. D. Love.) (Fig. 14)
faults, point toward the west or southwest (fig. 14).
By early Eocene time, about 20 million years after they had begun, the
deformational forces relaxed. But the effects of the giant earth movements
were to last for a very long time. Crustal disturbances of such magnitude
commonly produce conditions deep within the earth which, in places, gives
rise to intense volcanic activity; one such place was Yellowstone.
22
CROSS SECTIONS SHOWING GEOLOGIC STRUCTURES in Yellowstone
National Park. These illustrate the possible rock relationships that might be
seen along the faces of vertical slices of the earth’s crust, if it could be cut
and pulled apart (much like slicing a cake and looking at the different layers).
The locations of the sections are shown on the geologic map, plate 1. Reverse
faults and most folds originated during the Larimide orogeny, and normal
faults originated chiefly during Pliocene and later times. The arrows indicate
the relative movements of fault blocks. Geologic symbols: Qs, Quaternary
superficial deposits; Qb, Quaternary basalt flows; Qy, Quaternary Yellowstone
tuff; Tav, Tertiary Absaroka volcanic rocks; Mzr, Mesozoic sedimentary rocks;
Pzr, Paleozoic sedimentary rocks; pCr, Precambrian metamorphic
(“basement”) rocks. (Based partly on information supplied by E. T. Ruppel
and J. D. Love.) (Fig. 14)
Page 47
23
Volcanic activity
In early Eocene time, between 55 and 50 million years ago, several large
volcanoes erupted in and near Yellowstone National Park. This volcanic
activity resulted in the accumulation of the vast pile of Absaroka volcanic
rocks (fig. 5) which now makes up most of the Absaroka and Washburn
Ranges and part of the Gallatin Range, and which covers several other
smaller areas in the Park (pl. 1).
What special geologic conditions would cause these spectacular eruptions of
molten rock at the earth’s surface? Measurements taken in deep mines and
oil wells show that the normal increase in the earth’s temperature with depth
is about 1°F per 100 feet. This heat is generated by the decay of radioactive
elements—chiefly uranium, thorium, and potassium—which are present in at
least small amounts in virtually all rocks of the earth’s crust. Ordinarily,
enough heat is conducted to the earth’s surface so that the deeply buried
rocks do not become hot enough to melt. In some places, however, the heat
is not carried off fast enough, and the temperature rises slowly toward the
melting point of the rock. Such hot spots may develop (1) because the rocks
in those places contain more than an average amount of radioactive
elements; (2) because hotter material moves upward from still deeper levels
in the earth; or (3) because drastic changes in pressure are brought about by
the alternate squeezing and relaxing of mountain-building forces, which in
turn substantially affect the melting point of the rocks. Whatever the cause,
the eventual result is the accumulation of a huge body of molten rock, called
magma, enclosed in a deep underground chamber.
Magma, being a mixture of hot liquids and gases that is lighter in weight
than the solid rocks surrounding it, tends to rise toward the earth’s surface.
Forcing its way upward, some of the molten material solidifies before
reaching the surface and forms bodies of various kinds of intrusive igneous
rocks (fig. 15). Some of the magma, however, reaches the surface and either
pours out as lava or is blown out explosively as rock fragments, ash, and
pumice to form extrusive igneous rocks.
24
Volcanic activity
In early Eocene time, between 55 and 50 million years ago, several large
volcanoes erupted in and near Yellowstone National Park. This volcanic
activity resulted in the accumulation of the vast pile of Absaroka volcanic
rocks (fig. 5) which now makes up most of the Absaroka and Washburn
Ranges and part of the Gallatin Range, and which covers several other
smaller areas in the Park (pl. 1).
What special geologic conditions would cause these spectacular eruptions of
molten rock at the earth’s surface? Measurements taken in deep mines and
oil wells show that the normal increase in the earth’s temperature with depth
is about 1°F per 100 feet. This heat is generated by the decay of radioactive
elements—chiefly uranium, thorium, and potassium—which are present in at
least small amounts in virtually all rocks of the earth’s crust. Ordinarily,
enough heat is conducted to the earth’s surface so that the deeply buried
rocks do not become hot enough to melt. In some places, however, the heat
is not carried off fast enough, and the temperature rises slowly toward the
melting point of the rock. Such hot spots may develop (1) because the rocks
in those places contain more than an average amount of radioactive
elements; (2) because hotter material moves upward from still deeper levels
in the earth; or (3) because drastic changes in pressure are brought about by
the alternate squeezing and relaxing of mountain-building forces, which in
turn substantially affect the melting point of the rocks. Whatever the cause,
the eventual result is the accumulation of a huge body of molten rock, called
magma, enclosed in a deep underground chamber.
Magma, being a mixture of hot liquids and gases that is lighter in weight
than the solid rocks surrounding it, tends to rise toward the earth’s surface.
Forcing its way upward, some of the molten material solidifies before
reaching the surface and forms bodies of various kinds of intrusive igneous
rocks (fig. 15). Some of the magma, however, reaches the surface and either
pours out as lava or is blown out explosively as rock fragments, ash, and
pumice to form extrusive igneous rocks.
24
Page 48
INTRUSIVE AND EXTRUSIVE IGNEOUS ROCK BODIES. Extrusive rocks
solidified above ground, and intrusive rocks solidified below ground. All
features shown occur in Yellowstone National Park. Extrusive rocks are the
predominant rock type seen along the Park roads, and the table lists the three
principal kinds that are present. (Fig. 15)
Rock
name Principal rock-forming minerals Color
Rhyolite [a] [b] Light to medium shades of gray and
Quartz, feldspar (sanidine). brown.
Andesite [b] [c] Medium to fairly dark shades of brown,
Feldspar (plagioclase), pyroxene red, purple, and gray.
(augite).
Basalt Feldspar (plagioclase), pyroxene, Nearly black.
[c] [d]
olivine, magnetite.
[a]
Clear to light-colored silicon dioxide.
[b]
Light-colored aluminum silicate minerals.
[c]
Dark-colored iron and magnesium silicate minerals.
[d]
Very dark colored iron oxide mineral.
The magmas which formed the Absaroka volcanoes erupted mainly through
large central vents (fig. 16). Most of the eruptions were fairly quiet, with the
molten rock welling up to the surface and cascading down the sides of the
solidified above ground, and intrusive rocks solidified below ground. All
features shown occur in Yellowstone National Park. Extrusive rocks are the
predominant rock type seen along the Park roads, and the table lists the three
principal kinds that are present. (Fig. 15)
Rock
name Principal rock-forming minerals Color
Rhyolite [a] [b] Light to medium shades of gray and
Quartz, feldspar (sanidine). brown.
Andesite [b] [c] Medium to fairly dark shades of brown,
Feldspar (plagioclase), pyroxene red, purple, and gray.
(augite).
Basalt Feldspar (plagioclase), pyroxene, Nearly black.
[c] [d]
olivine, magnetite.
[a]
Clear to light-colored silicon dioxide.
[b]
Light-colored aluminum silicate minerals.
[c]
Dark-colored iron and magnesium silicate minerals.
[d]
Very dark colored iron oxide mineral.
The magmas which formed the Absaroka volcanoes erupted mainly through
large central vents (fig. 16). Most of the eruptions were fairly quiet, with the
molten rock welling up to the surface and cascading down the sides of the
Page 49
volcanoes chiefly as viscous lava flows and breccias. Rain, seeping into
these porous rocks, caused huge landslides of mud and broken rock to
stream down the mountainsides. Hence, many of the rocks seen today are
volcanic breccias—jumbled but crudely layered deposits of large and small
angular blocks embedded in a sandy matrix, much like man-made concrete
except that the rock fragments are considerably coarser (fig. 17). Viewed
from a distance, however, most of the breccia deposits have a distinct
layered appearance (fig. 18). The predominant extrusive igneous rock in the
Absaroka volcanic sequence is andesite, but basalt also occurs in places (fig.
15).
25
ABSAROKA VOLCANOES and their rocks. Lava (mostly andesite) poured
from central vents and formed volcanoes, some steep sided and others broad
and relatively flat. As the lava spilled out, much of it quickly solidified, broke
up into large angular blocks (breccia), and then either tumbled down the
slopes of the volcanoes as individual boulders or slid down in mudflows and
landslides. Some of the material was also explosively blown out as rock
bombs, cinders, and ash. The more fluid lava (mostly basalt), on the other
these porous rocks, caused huge landslides of mud and broken rock to
stream down the mountainsides. Hence, many of the rocks seen today are
volcanic breccias—jumbled but crudely layered deposits of large and small
angular blocks embedded in a sandy matrix, much like man-made concrete
except that the rock fragments are considerably coarser (fig. 17). Viewed
from a distance, however, most of the breccia deposits have a distinct
layered appearance (fig. 18). The predominant extrusive igneous rock in the
Absaroka volcanic sequence is andesite, but basalt also occurs in places (fig.
15).
25
ABSAROKA VOLCANOES and their rocks. Lava (mostly andesite) poured
from central vents and formed volcanoes, some steep sided and others broad
and relatively flat. As the lava spilled out, much of it quickly solidified, broke
up into large angular blocks (breccia), and then either tumbled down the
slopes of the volcanoes as individual boulders or slid down in mudflows and
landslides. Some of the material was also explosively blown out as rock
bombs, cinders, and ash. The more fluid lava (mostly basalt), on the other
Page 50
hand, flowed quietly down the volcanic slopes and onto the surrounding
lowlands. The rocks near the volcanic centers therefore include thick crudely
layered coarse breccias, thin fine ash and dust falls, and thin to thick lava
flows. The volcanoes were repeatedly attacked by erosion, and the eroded
material was redeposited by streams and mudflows in widespread layers of
volcanic conglomerate and sandstone across the flat-floored valleys and
plains between the volcanoes. Forests, which grew luxuriantly in these
lowland areas, were repeatedly buried by volcanic eruptions and are now
preserved (see inset) as the fossil forests of Yellowstone. (Based on
information supplied by H. W. Smedes and H. J. Prostka.) (Fig. 16)
Chiefly lava flows of shield volcano
Chiefly volcanic sandstone and conglomerate of lowland areas
Chiefly volcanic breccias and thin lava flows of cone-type volcano
At times the Absaroka volcanic eruptions were violently explosive,
showering the countryside with rock bombs, cinders, and ash. The finer
debris that reached the lower slopes of the volcanoes was reworked and
carried by streams into the intervening valleys, where it was deposited as
sand and gravel (fig. 16). Eventually the entire Yellowstone region was
choked with volcanic debris, the material from one volcano mixing with that
from neighboring volcanoes. Even the mountain masses uplifted during the
preceding Laramide orogeny were covered by the vast accumulation (fig.
18).
26
lowlands. The rocks near the volcanic centers therefore include thick crudely
layered coarse breccias, thin fine ash and dust falls, and thin to thick lava
flows. The volcanoes were repeatedly attacked by erosion, and the eroded
material was redeposited by streams and mudflows in widespread layers of
volcanic conglomerate and sandstone across the flat-floored valleys and
plains between the volcanoes. Forests, which grew luxuriantly in these
lowland areas, were repeatedly buried by volcanic eruptions and are now
preserved (see inset) as the fossil forests of Yellowstone. (Based on
information supplied by H. W. Smedes and H. J. Prostka.) (Fig. 16)
Chiefly lava flows of shield volcano
Chiefly volcanic sandstone and conglomerate of lowland areas
Chiefly volcanic breccias and thin lava flows of cone-type volcano
At times the Absaroka volcanic eruptions were violently explosive,
showering the countryside with rock bombs, cinders, and ash. The finer
debris that reached the lower slopes of the volcanoes was reworked and
carried by streams into the intervening valleys, where it was deposited as
sand and gravel (fig. 16). Eventually the entire Yellowstone region was
choked with volcanic debris, the material from one volcano mixing with that
from neighboring volcanoes. Even the mountain masses uplifted during the
preceding Laramide orogeny were covered by the vast accumulation (fig.
18).
26
Page 51
MASSIVE BEDS OF BRECCIA of the Absaroka volcanic rocks along the road
north of Dunraven Pass. This breccia formed part of a steep-sided volcanic
cone, of which Mount Washburn is a remnant. (Fig. 17)
north of Dunraven Pass. This breccia formed part of a steep-sided volcanic
cone, of which Mount Washburn is a remnant. (Fig. 17)
Page 52
Closeup view shows very coarse character of the breccia, with large rock
fragments imbedded in fine ash, dust, and sand. Nearly all the rocks are of
andesitic composition, consisting chiefly of feldspar and pyroxene. Most
common colors are medium to fairly dark shades of brown, red, purple, and
gray.
Absaroka volcanism, however, was not a simple, continuous process— 27
the eruptions were intermittent, the many volcanoes were not always
active at the same time, and between eruptions there were long periods of
quiescence during which the erupted material was deeply eroded. The
repetitive nature of the eruptions is best illustrated by the famous fossil
forests of Yellowstone. Here is striking evidence that enough time elapsed
between eruptions for widespread forests to become established on the lower
slopes of the volcanoes and in the broad valleys between them. Judged from
the great size of some of the now-petrified logs (fig. 19), several hundreds of
years must have passed before another volcanic outburst smothered the
fragments imbedded in fine ash, dust, and sand. Nearly all the rocks are of
andesitic composition, consisting chiefly of feldspar and pyroxene. Most
common colors are medium to fairly dark shades of brown, red, purple, and
gray.
Absaroka volcanism, however, was not a simple, continuous process— 27
the eruptions were intermittent, the many volcanoes were not always
active at the same time, and between eruptions there were long periods of
quiescence during which the erupted material was deeply eroded. The
repetitive nature of the eruptions is best illustrated by the famous fossil
forests of Yellowstone. Here is striking evidence that enough time elapsed
between eruptions for widespread forests to become established on the lower
slopes of the volcanoes and in the broad valleys between them. Judged from
the great size of some of the now-petrified logs (fig. 19), several hundreds of
years must have passed before another volcanic outburst smothered the
Page 53
forest. Many different forest layers have been recognized in the Specimen
Ridge area as well as in several other places throughout the Park.
As the Absaroka magma rose from deep underground, some of it squirted,
like toothpaste, into the layered Paleozoic and Mesozoic sedimentary rocks
through which it passed. These relatively small masses of molten rock
material slowly cooled and crystallized to form intrusive igneous rocks such
as diorite (fig. 20). The resulting intrusive bodies, called sills, dikes, stocks,
and laccoliths, depending on their form, are most abundant in the Gallatin
Range and in the vicinity of the East Entrance (pl. 1). At the conclusion of
volcanic activity, the last of the rising magma solidified in the main conduits
to form slender, somewhat cylindrical bodies of rock called volcanic necks
that probably conform closely to the shape of the original conduits. The
circular intrusive rock body at Bunsen Peak (fig. 21), now exposed to view
because erosion has stripped away the lava and volcanic breccia that once
completely buried it, represents either a volcanic neck or a small stock that
solidified directly beneath a volcano.
28
MASSIVELY LAYERED BRECCIAS, conglomerates, and sandstones of the
Absaroka volcanic sequence at Barronette Peak, as viewed from the road
near the Northeast Entrance; the ridge is 3,000 feet high. These rocks,
deposited as part of an alluvial plain between volcanoes, once filled the
Yellowstone region to a level higher than the top of Barronette Peak, but
erosion since late Tertiary time has stripped the volcanics from much of the
Park area. The volcanic rocks (Eocene in age, fig. 5) rest directly on Paleozoic
sedimentary rocks along the line indicated. During the Laramide orogeny, in
Late Cretaceous and early Tertiary times, the region was folded and uplifted
Ridge area as well as in several other places throughout the Park.
As the Absaroka magma rose from deep underground, some of it squirted,
like toothpaste, into the layered Paleozoic and Mesozoic sedimentary rocks
through which it passed. These relatively small masses of molten rock
material slowly cooled and crystallized to form intrusive igneous rocks such
as diorite (fig. 20). The resulting intrusive bodies, called sills, dikes, stocks,
and laccoliths, depending on their form, are most abundant in the Gallatin
Range and in the vicinity of the East Entrance (pl. 1). At the conclusion of
volcanic activity, the last of the rising magma solidified in the main conduits
to form slender, somewhat cylindrical bodies of rock called volcanic necks
that probably conform closely to the shape of the original conduits. The
circular intrusive rock body at Bunsen Peak (fig. 21), now exposed to view
because erosion has stripped away the lava and volcanic breccia that once
completely buried it, represents either a volcanic neck or a small stock that
solidified directly beneath a volcano.
28
MASSIVELY LAYERED BRECCIAS, conglomerates, and sandstones of the
Absaroka volcanic sequence at Barronette Peak, as viewed from the road
near the Northeast Entrance; the ridge is 3,000 feet high. These rocks,
deposited as part of an alluvial plain between volcanoes, once filled the
Yellowstone region to a level higher than the top of Barronette Peak, but
erosion since late Tertiary time has stripped the volcanics from much of the
Park area. The volcanic rocks (Eocene in age, fig. 5) rest directly on Paleozoic
sedimentary rocks along the line indicated. During the Laramide orogeny, in
Late Cretaceous and early Tertiary times, the region was folded and uplifted
Page 54
into mountains. Thousands of feet of Mesozoic and Paleozoic sedimentary
rocks were then eroded off the rising mountains before the Absaroka volcanic
rocks were deposited, (Fig. 18)
29
GIANT PETRIFIED TREE TRUNKS in Yellowstone’s fossil forest. The
enclosing rocks, part of the Absaroka volcanic sequence that forms
Specimen Ridge, are approximately 50 million years old. Many of the tree
trunks are still upright, having been smothered and buried in their original
positions by breccia, ash, and dust from nearby volcanoes. It is evident that
more than one “forest” is represented in this view. Prof. Erling Dorf, of
Princeton University, counted a total of 27 different forest layers in the rocks
now exposed at Specimen Ridge. He also determined that the most common
kinds of trees were sycamore, walnut, magnolia, chestnut, oak, redwood,
maple, and dogwood. The nearest living relatives of many of these trees are
now found in the warm temperate to subtropical forests of the southeastern
and southern United States. (National Park Service photograph.) (Fig. 19)
Mount Washburn is the north half of one of the ancient Absaroka 30
volcanoes (fig. 26), and many of the rocks and other features related to
this volcano, which characterized this great period of volcanism, can be seen
rocks were then eroded off the rising mountains before the Absaroka volcanic
rocks were deposited, (Fig. 18)
29
GIANT PETRIFIED TREE TRUNKS in Yellowstone’s fossil forest. The
enclosing rocks, part of the Absaroka volcanic sequence that forms
Specimen Ridge, are approximately 50 million years old. Many of the tree
trunks are still upright, having been smothered and buried in their original
positions by breccia, ash, and dust from nearby volcanoes. It is evident that
more than one “forest” is represented in this view. Prof. Erling Dorf, of
Princeton University, counted a total of 27 different forest layers in the rocks
now exposed at Specimen Ridge. He also determined that the most common
kinds of trees were sycamore, walnut, magnolia, chestnut, oak, redwood,
maple, and dogwood. The nearest living relatives of many of these trees are
now found in the warm temperate to subtropical forests of the southeastern
and southern United States. (National Park Service photograph.) (Fig. 19)
Mount Washburn is the north half of one of the ancient Absaroka 30
volcanoes (fig. 26), and many of the rocks and other features related to
this volcano, which characterized this great period of volcanism, can be seen
Page 55
along the road between Canyon Village and Tower. In roadcuts just south of
Dunraven Pass several thin igneous dikes cut through volcanic breccias.
These dikes radiate outward from the nearby central core of the volcano,
which lies east of the highway in the vicinity of Washburn Hot Springs.
From Dunraven Pass northward for 2-3 miles, the road is lined with lava
flows and very coarse breccias that accumulated close to the volcanic neck
(fig. 17). Farther north toward Tower Falls, breccias and conglomerates
predominate, but the average size of individual rock fragments decreases
gradually northward away from the center of eruption. Beds of sandstone
then begin to appear in the sequence, having been deposited mainly by
streams that drained the north slope of the volcano.
Dunraven Pass several thin igneous dikes cut through volcanic breccias.
These dikes radiate outward from the nearby central core of the volcano,
which lies east of the highway in the vicinity of Washburn Hot Springs.
From Dunraven Pass northward for 2-3 miles, the road is lined with lava
flows and very coarse breccias that accumulated close to the volcanic neck
(fig. 17). Farther north toward Tower Falls, breccias and conglomerates
predominate, but the average size of individual rock fragments decreases
gradually northward away from the center of eruption. Beds of sandstone
then begin to appear in the sequence, having been deposited mainly by
streams that drained the north slope of the volcano.
Page 56
IGNEOUS ROCK. Closeup view of intrusive igneous rock (diorite) from the
Electric Peak stock in the Gallatin Range; Electric Peak is pictured in figure
37. The rock is composed chiefly of light-colored quartz and feldspar and
dark-colored iron and magnesium silicate minerals. (Fig. 20)
At the end of Absaroka volcanism, approximately 40 million years ago (fig.
6), all of Yellowstone lay buried beneath several thousand feet of lavas,
breccias, and ash (fig. 18). The landscape must have appeared as a gently
rolling plateau, drained by sluggish, meandering streams and dotted 31
here and there by volcanoes still rising above the general level of the
ground. This plateau surface, however, probably stood at a maximum of only
a few thousand feet above sea level, for animals and plants now found as
fossils in the Absaroka volcanic rocks indicate that warm-temperature to
even subtropical climates existed during the volcanic period (fig. 19).
BUNSEN PEAK, a roughly circular body of intrusive igneous rock, is the
eroded remnant of either the “neck” of an Absaroka volcano or a small stock
that solidified directly beneath a volcano. The peak rises approximately 1,200
feet above a flat plain (foreground) that is covered by flows of younger basalt.
Electric Peak stock in the Gallatin Range; Electric Peak is pictured in figure
37. The rock is composed chiefly of light-colored quartz and feldspar and
dark-colored iron and magnesium silicate minerals. (Fig. 20)
At the end of Absaroka volcanism, approximately 40 million years ago (fig.
6), all of Yellowstone lay buried beneath several thousand feet of lavas,
breccias, and ash (fig. 18). The landscape must have appeared as a gently
rolling plateau, drained by sluggish, meandering streams and dotted 31
here and there by volcanoes still rising above the general level of the
ground. This plateau surface, however, probably stood at a maximum of only
a few thousand feet above sea level, for animals and plants now found as
fossils in the Absaroka volcanic rocks indicate that warm-temperature to
even subtropical climates existed during the volcanic period (fig. 19).
BUNSEN PEAK, a roughly circular body of intrusive igneous rock, is the
eroded remnant of either the “neck” of an Absaroka volcano or a small stock
that solidified directly beneath a volcano. The peak rises approximately 1,200
feet above a flat plain (foreground) that is covered by flows of younger basalt.
Page 57
The Yellowstone Tuff, formed by volcanic ash and dust exploded from the
central Yellowstone region to the south, underlies the basalt. When erupted,
the volcanic debris (as well as the basalt lava) flowed around this high-
standing peak. (Fig. 21)
A quiet period
Little is known in detail of the geologic events in Yellowstone during
Oligocene and Miocene times. Rocks of these ages have not been recognized
within the Park; if ever deposited there, they have since been removed by
erosion or buried by younger volcanic rocks. Thus, we can only speculate as
to what events took place during this 25-million-year period. No doubt 32
the broad Absaroka volcanic plateau was eroded, but not deeply,
because the topographic relief and stream gradients of the region remained
low. There are also hints that some volcanic activity took place, for volcanic
rocks representing parts of this time interval occur south of the Park, and
some of these rocks may have originated within the Park area. Little
transpired, however, to significantly alter the existing geological makeup of
the Park; it was indeed a quiet time, particularly when compared with the
extremely dynamic periods which immediately preceded and followed it.
More mountain building and deep erosion
Many features of the present-day landscape of Yellowstone stem from
Pliocene time, about 10 million years ago. At that time the entire region—in
fact, much of the Rocky Mountain chain—was being uplifted by giant earth
movements to heights several thousand feet above its previous level. This
episode of regional uplift accounts in large measure for the present high
average elevation of the Yellowstone country. Although the precise cause of
the uplift is unknown, the uplift assuredly reflects profound changes that
were taking place deep within or beneath the earth’s crust.
Great tensional forces, operating during Pliocene time, pulled the
Yellowstone region apart and partially broke it into large steep-sided blocks
bounded by normal faults (fig. 13). Some blocks sank while others rose,
central Yellowstone region to the south, underlies the basalt. When erupted,
the volcanic debris (as well as the basalt lava) flowed around this high-
standing peak. (Fig. 21)
A quiet period
Little is known in detail of the geologic events in Yellowstone during
Oligocene and Miocene times. Rocks of these ages have not been recognized
within the Park; if ever deposited there, they have since been removed by
erosion or buried by younger volcanic rocks. Thus, we can only speculate as
to what events took place during this 25-million-year period. No doubt 32
the broad Absaroka volcanic plateau was eroded, but not deeply,
because the topographic relief and stream gradients of the region remained
low. There are also hints that some volcanic activity took place, for volcanic
rocks representing parts of this time interval occur south of the Park, and
some of these rocks may have originated within the Park area. Little
transpired, however, to significantly alter the existing geological makeup of
the Park; it was indeed a quiet time, particularly when compared with the
extremely dynamic periods which immediately preceded and followed it.
More mountain building and deep erosion
Many features of the present-day landscape of Yellowstone stem from
Pliocene time, about 10 million years ago. At that time the entire region—in
fact, much of the Rocky Mountain chain—was being uplifted by giant earth
movements to heights several thousand feet above its previous level. This
episode of regional uplift accounts in large measure for the present high
average elevation of the Yellowstone country. Although the precise cause of
the uplift is unknown, the uplift assuredly reflects profound changes that
were taking place deep within or beneath the earth’s crust.
Great tensional forces, operating during Pliocene time, pulled the
Yellowstone region apart and partially broke it into large steep-sided blocks
bounded by normal faults (fig. 13). Some blocks sank while others rose,
Page 58
commonly on the order of several thousand feet. The Gallatin Range, in the
northwest corner of the Park, for example, was lifted as a rectangular
mountain block along north-trending 20-mile-long normal faults that border
it on each side (fig. 14, section A-A′; pl. 1). In the south-central part of the
Park, the differential movements between several adjacent fault blocks
totaled more than 15,000 feet (fig. 14, section C-C′). Farther south, the Teton
Range moved up and the floor of Jackson Hole moved down along a normal-
fault zone that stretches along the east foot of the range. An enormous offset
of about 30,000 feet developed between the two crustal blocks, accounting
in large part for the now incredibly steep and rugged east face of the Teton
Range.
The pronounced rise in elevation of the general ground surface and the 33
chopping of the region into many mountainous fault blocks caused a
profound increase in the rate of erosion. Once-sluggish streams turned into
vigorous, fast-moving rivers that began to cut deeply into the Absaroka
volcanic plateau. Huge quantities of rock debris were stripped off and
carried out of the area, and at the end of the Pliocene, the Yellowstone region
must have been very highly dissected mountains and table- and canyon-
lands. Much of the landscape may have resembled the rugged terrain now
seen in the Absaroka Range along the east side of the Park. These mountains
(fig. 27), and the Washburn Range in the interior of the Park (fig. 4), today
represent but small remnants of the vast pile of Absaroka volcanic rocks that
once covered all of Yellowstone and the surrounding regions.
northwest corner of the Park, for example, was lifted as a rectangular
mountain block along north-trending 20-mile-long normal faults that border
it on each side (fig. 14, section A-A′; pl. 1). In the south-central part of the
Park, the differential movements between several adjacent fault blocks
totaled more than 15,000 feet (fig. 14, section C-C′). Farther south, the Teton
Range moved up and the floor of Jackson Hole moved down along a normal-
fault zone that stretches along the east foot of the range. An enormous offset
of about 30,000 feet developed between the two crustal blocks, accounting
in large part for the now incredibly steep and rugged east face of the Teton
Range.
The pronounced rise in elevation of the general ground surface and the 33
chopping of the region into many mountainous fault blocks caused a
profound increase in the rate of erosion. Once-sluggish streams turned into
vigorous, fast-moving rivers that began to cut deeply into the Absaroka
volcanic plateau. Huge quantities of rock debris were stripped off and
carried out of the area, and at the end of the Pliocene, the Yellowstone region
must have been very highly dissected mountains and table- and canyon-
lands. Much of the landscape may have resembled the rugged terrain now
seen in the Absaroka Range along the east side of the Park. These mountains
(fig. 27), and the Washburn Range in the interior of the Park (fig. 4), today
represent but small remnants of the vast pile of Absaroka volcanic rocks that
once covered all of Yellowstone and the surrounding regions.
Page 59
34
Page 60
Formation of the Yellowstone
Caldera
We have now approached that point in geologic time—the beginning of the
Quaternary Period between 2 million and 3 million years ago—when the
stage was set for the triggering of those all-important events that culminated
in the development of the 1,000-square-mile Yellowstone caldera and
ultimately gave rise to the world-renowned hot-water and steam phenomena.
Involved were some of the earth’s biggest explosions, which have had no
apparent counterpart in recorded human history. A few extremely explosive
eruptions have occurred historically, however, such as the one that took
place on the uninhabited island of Krakatoa, between Java and Sumatra in
the East Indies, during the latter part of August 1883. For several days this
island had been shaken by a series of violent explosions. Then, on August
27, it was ripped by an explosion that was heard as far away as Australia, a
distance of about 3,000 miles. Fifty-mile-high dust clouds became
windborne around the globe, producing colorful sunrises and sunsets in all
parts of the world for several years. When the air around Krakatoa finally
cleared, it was found that two-thirds of the island, some 12 square miles, had
collapsed and vanished into the sea. Though the Krakatoa eruption resulted
Caldera
We have now approached that point in geologic time—the beginning of the
Quaternary Period between 2 million and 3 million years ago—when the
stage was set for the triggering of those all-important events that culminated
in the development of the 1,000-square-mile Yellowstone caldera and
ultimately gave rise to the world-renowned hot-water and steam phenomena.
Involved were some of the earth’s biggest explosions, which have had no
apparent counterpart in recorded human history. A few extremely explosive
eruptions have occurred historically, however, such as the one that took
place on the uninhabited island of Krakatoa, between Java and Sumatra in
the East Indies, during the latter part of August 1883. For several days this
island had been shaken by a series of violent explosions. Then, on August
27, it was ripped by an explosion that was heard as far away as Australia, a
distance of about 3,000 miles. Fifty-mile-high dust clouds became
windborne around the globe, producing colorful sunrises and sunsets in all
parts of the world for several years. When the air around Krakatoa finally
cleared, it was found that two-thirds of the island, some 12 square miles, had
collapsed and vanished into the sea. Though the Krakatoa eruption resulted
Page 61
in a caldera that is only a small fraction of the size of the one in Yellowstone,
it provides a mental picture to help us understand what has been discovered
about the great volcanic holocaust in Yellowstone National Park that was
described briefly in an early part of this report.
35
OUTLINE OF THE YELLOWSTONE CALDERA produced by the enormous
volcanic eruption 600,000 years ago. The two oval-shaped areas are resurgent
it provides a mental picture to help us understand what has been discovered
about the great volcanic holocaust in Yellowstone National Park that was
described briefly in an early part of this report.
35
OUTLINE OF THE YELLOWSTONE CALDERA produced by the enormous
volcanic eruption 600,000 years ago. The two oval-shaped areas are resurgent
Page 62
domes that arched the caldera floor over twin magma chambers after the
eruption. The margins of the resurgent domes are surrounded by ring fracture
zones which extend outward toward the edge of the caldera. Numerous
fractures in these zones provided escape routes through which lavas of the
Plateau Rhyolite oozed to the surface and poured out across the caldera floor.
Today these zones also provide underground channels for the circulation of
hot water in the Yellowstone thermal system. The area outlined by the dotted
line shows the smaller and younger inner caldera now occupied by the West
Thumb of Yellowstone Lake. (Based on information supplied by R. L.
Christiansen and H. R. Blank, Jr.; the existence of a caldera in Yellowstone
National Park was first recognized by F. R. Boyd in the late 1950’s.) (Fig. 22)
36
eruption. The margins of the resurgent domes are surrounded by ring fracture
zones which extend outward toward the edge of the caldera. Numerous
fractures in these zones provided escape routes through which lavas of the
Plateau Rhyolite oozed to the surface and poured out across the caldera floor.
Today these zones also provide underground channels for the circulation of
hot water in the Yellowstone thermal system. The area outlined by the dotted
line shows the smaller and younger inner caldera now occupied by the West
Thumb of Yellowstone Lake. (Based on information supplied by R. L.
Christiansen and H. R. Blank, Jr.; the existence of a caldera in Yellowstone
National Park was first recognized by F. R. Boyd in the late 1950’s.) (Fig. 22)
36
Page 63
GEOLOGIC MAP OF YELLOWSTONE NATIONAL PARK (PLATE
1)
Generalized from detailed mapping by R. L. Christiansen and H. R. Blank, Jr.
(Quaternary volcanic rocks); H. W. Smedes and H. J. Prostka (Absaroka
volcanic rocks); E. T. Ruppel (sedimentary and metamorphic rocks, northern
part of park); and J. D. Love and W. R. Keefer (sedimentary rocks, southern
part of park).
1)
Generalized from detailed mapping by R. L. Christiansen and H. R. Blank, Jr.
(Quaternary volcanic rocks); H. W. Smedes and H. J. Prostka (Absaroka
volcanic rocks); E. T. Ruppel (sedimentary and metamorphic rocks, northern
part of park); and J. D. Love and W. R. Keefer (sedimentary rocks, southern
part of park).
Page 64
High-resolution Version
Page 65
Page 66
EXPLANATION
CENOZOIC
QUATERNARY
Stream sand and gravel, glacial and landslide debris, hot-spring deposits, and
lake beds
Basalt flows
Plateau Rhyolite
Yellowstone Tuff and related lava flows
TERTIARY
Absaroka volcanic rocks
Intrusive igneous rocks
Tertiary formations
Mesozoic formations
Paleozoic formations
Precambrian gneiss and schist
Contact
FAULT AND FOLD SYMBOLS
Dotted where concealed beneath younger unfaulted rocks
Reverse fault
Sawteeth on side that moved up
Normal fault
Symbol on side that moved down
Reverse fault, along which there was later normal-fault movement
Anticlinal axis
B B′ Line of cross section shown in figure 14
(D-D’ is figure 26)
38
Near the beginning of the Quaternary Period a vast quantity of molten
rock had again accumulated deep within the earth beneath Yellowstone. This
time, in contrast to Absaroka volcanism, the magma was charged with highly
explosive materials which eventually caused two caldera-making eruptions,
one 2,000,000 years ago and the other 600,000 years ago. Because both
eruptions affected the central part of the Park, the features related to the
older one were largely destroyed by the activity associated with the younger
one. Thus, the outline of the volcanic caldera we now see in the Yellowstone
landscape is chiefly the one that formed 600,000 years ago (fig. 22). The
sequence of events described in the following pages, and illustrated
diagrammatically in figure 23, is based on studies of this later eruption; the
pattern for the 2,000,000-year-old eruption probably was similar.
CENOZOIC
QUATERNARY
Stream sand and gravel, glacial and landslide debris, hot-spring deposits, and
lake beds
Basalt flows
Plateau Rhyolite
Yellowstone Tuff and related lava flows
TERTIARY
Absaroka volcanic rocks
Intrusive igneous rocks
Tertiary formations
Mesozoic formations
Paleozoic formations
Precambrian gneiss and schist
Contact
FAULT AND FOLD SYMBOLS
Dotted where concealed beneath younger unfaulted rocks
Reverse fault
Sawteeth on side that moved up
Normal fault
Symbol on side that moved down
Reverse fault, along which there was later normal-fault movement
Anticlinal axis
B B′ Line of cross section shown in figure 14
(D-D’ is figure 26)
38
Near the beginning of the Quaternary Period a vast quantity of molten
rock had again accumulated deep within the earth beneath Yellowstone. This
time, in contrast to Absaroka volcanism, the magma was charged with highly
explosive materials which eventually caused two caldera-making eruptions,
one 2,000,000 years ago and the other 600,000 years ago. Because both
eruptions affected the central part of the Park, the features related to the
older one were largely destroyed by the activity associated with the younger
one. Thus, the outline of the volcanic caldera we now see in the Yellowstone
landscape is chiefly the one that formed 600,000 years ago (fig. 22). The
sequence of events described in the following pages, and illustrated
diagrammatically in figure 23, is based on studies of this later eruption; the
pattern for the 2,000,000-year-old eruption probably was similar.
Page 67
The eruption
The giant reservoir of molten rock that built up beneath the Park area fed
two large magma chambers that rose to within a few thousand feet of the
surface. As the pressures increased, the overlying ground arched, stretched,
and cracked (fig. 23A). Small amounts of lava began to flow out through the
cracks in places, but finally, in a great surge of rapid, violently explosive
eruptions, first from one chamber and then the other, mountains of hot
pumice, ash, and rock debris spewed from the earth (fig. 23B). The dense,
swirling masses of erupted material spread out across the countryside in
extremely fast moving ash flows, swept along by hot expanding gases
trapped within them. Large quantities of ash and dust were also blown high
into the air and dispersed by the wind. Thin layers of airborne volcanic ash
from Yellowstone are now found throughout much of the central and western
United States.
The ash flows (fig. 23B), as they sped across the Yellowstone countryside,
first filled the old canyons and valleys that had been eroded into the
Absaroka volcanic pile and older rocks during Pliocene time. Eventually
much of this older landscape was buried by ash. Some of the larger
highlands, such as Mount Washburn and adjacent ridges and Bunsen Peak,
however, stood well above the level of the sweeping ash flows; so the debris
flowed around them rather than across them (fig. 21). Finally coming to rest,
the hot pumice, ash, and rock particles settled down in vast horizontal sheets
(fig. 24). Upon cooling and crystallizing, the particles welded together to
form a series of compact rocks with the composition of rhyolite (figs. 39
15 and 25). The term “ash-flow tuff” (also, the term “welded tuff”) is
commonly used to describe these rocks, which now make up the
Yellowstone Tuff (fig. 5).
The collapse
With the sudden removal of hundreds of cubic miles of molten rock from
underground, the roofs of the twin magma chambers collapsed. Enormous
blocks of rock fell in above each of the chambers, and a great crater, or
caldera, broke the ground surface in central Yellowstone (fig. 23C). The
The giant reservoir of molten rock that built up beneath the Park area fed
two large magma chambers that rose to within a few thousand feet of the
surface. As the pressures increased, the overlying ground arched, stretched,
and cracked (fig. 23A). Small amounts of lava began to flow out through the
cracks in places, but finally, in a great surge of rapid, violently explosive
eruptions, first from one chamber and then the other, mountains of hot
pumice, ash, and rock debris spewed from the earth (fig. 23B). The dense,
swirling masses of erupted material spread out across the countryside in
extremely fast moving ash flows, swept along by hot expanding gases
trapped within them. Large quantities of ash and dust were also blown high
into the air and dispersed by the wind. Thin layers of airborne volcanic ash
from Yellowstone are now found throughout much of the central and western
United States.
The ash flows (fig. 23B), as they sped across the Yellowstone countryside,
first filled the old canyons and valleys that had been eroded into the
Absaroka volcanic pile and older rocks during Pliocene time. Eventually
much of this older landscape was buried by ash. Some of the larger
highlands, such as Mount Washburn and adjacent ridges and Bunsen Peak,
however, stood well above the level of the sweeping ash flows; so the debris
flowed around them rather than across them (fig. 21). Finally coming to rest,
the hot pumice, ash, and rock particles settled down in vast horizontal sheets
(fig. 24). Upon cooling and crystallizing, the particles welded together to
form a series of compact rocks with the composition of rhyolite (figs. 39
15 and 25). The term “ash-flow tuff” (also, the term “welded tuff”) is
commonly used to describe these rocks, which now make up the
Yellowstone Tuff (fig. 5).
The collapse
With the sudden removal of hundreds of cubic miles of molten rock from
underground, the roofs of the twin magma chambers collapsed. Enormous
blocks of rock fell in above each of the chambers, and a great crater, or
caldera, broke the ground surface in central Yellowstone (fig. 23C). The
Page 68
exact depth to which the original surface collapsed is unknown, but it must
have been several thousand feet. The subsidence took place chiefly along
large vertical, or normal, faults in the ring fracture zones above the margins
of the magma chambers (fig. 22). Abundant, though less extensive, normal
faults also formed outside the caldera proper, as the surrounding areas
adjusted to the staggering impact of the explosive eruptions and subsequent
collapse.
Because the Yellowstone caldera now lies partly buried by thick lava flows,
the appearance of the caldera today is not nearly as impressive as it must
have been when the caldera was first formed. Many of the important
features, however, are particularly well exposed in the vicinity of Canyon
Village (fig. 26). The steep south slope of the nearby Washburn Range (fig.
4) marks the north edge of the caldera, and the range itself stands high
because it was not involved in the collapse. Canyon Village, on the other
hand, lies at a much lower elevation within the caldera proper. Turnouts on
the road just south of Dunraven Pass provide especially fine views of the
northern part of the caldera, and on a clear day Flat Mountain and the Red
Mountains, which mark the south edge of the caldera, south of Yellowstone
Lake, can be seen 50 miles away. As might be expected, the large basin
occupied by Yellowstone Lake owes its existence in part to caldera collapse.
The south edge of the caldera cuts across the south-central part of the lake,
along Flat Mountain Arm and the north tip of the Promontory; the east edge
coincides approximately with the east edge of the lake north of Southeast
Arm (fig. 27). Also, the prominent bluffs north of the Madison River near
Madison Junction mark part of the north rim of the caldera.
40
have been several thousand feet. The subsidence took place chiefly along
large vertical, or normal, faults in the ring fracture zones above the margins
of the magma chambers (fig. 22). Abundant, though less extensive, normal
faults also formed outside the caldera proper, as the surrounding areas
adjusted to the staggering impact of the explosive eruptions and subsequent
collapse.
Because the Yellowstone caldera now lies partly buried by thick lava flows,
the appearance of the caldera today is not nearly as impressive as it must
have been when the caldera was first formed. Many of the important
features, however, are particularly well exposed in the vicinity of Canyon
Village (fig. 26). The steep south slope of the nearby Washburn Range (fig.
4) marks the north edge of the caldera, and the range itself stands high
because it was not involved in the collapse. Canyon Village, on the other
hand, lies at a much lower elevation within the caldera proper. Turnouts on
the road just south of Dunraven Pass provide especially fine views of the
northern part of the caldera, and on a clear day Flat Mountain and the Red
Mountains, which mark the south edge of the caldera, south of Yellowstone
Lake, can be seen 50 miles away. As might be expected, the large basin
occupied by Yellowstone Lake owes its existence in part to caldera collapse.
The south edge of the caldera cuts across the south-central part of the lake,
along Flat Mountain Arm and the north tip of the Promontory; the east edge
coincides approximately with the east edge of the lake north of Southeast
Arm (fig. 27). Also, the prominent bluffs north of the Madison River near
Madison Junction mark part of the north rim of the caldera.
40
Page 69
CALDERA DEVELOPMENT. Schematic diagrams showing idealized stages in
the development of the Yellowstone caldera 600,000 years ago. The scales
shown in Diagram A are approximately the size of the features in Yellowstone.
Although only one magma chamber is pictured in the diagrams, two
chambers were involved in the Yellowstone eruption. (Based on information
supplied by R. L. Christiansen and H. R. Blank, Jr.) (Fig. 23)
A, A large magma chamber formed deep within the earth, and the molten rock
began to force its way slowly toward the surface. As it pushed upward, it
arched the overlying rocks into a broad dome. The arching produced a series
of concentric fractures, or a ring fracture zone, around the crest of the dome.
The fractures extended downward toward the top of the magma chamber.
B, The ring fractures eventually tapped the magma chamber, the uppermost
part of which contained a high proportion of dissolved gases. With the
sudden release of pressure, tremendous amounts of hot gases and molten
the development of the Yellowstone caldera 600,000 years ago. The scales
shown in Diagram A are approximately the size of the features in Yellowstone.
Although only one magma chamber is pictured in the diagrams, two
chambers were involved in the Yellowstone eruption. (Based on information
supplied by R. L. Christiansen and H. R. Blank, Jr.) (Fig. 23)
A, A large magma chamber formed deep within the earth, and the molten rock
began to force its way slowly toward the surface. As it pushed upward, it
arched the overlying rocks into a broad dome. The arching produced a series
of concentric fractures, or a ring fracture zone, around the crest of the dome.
The fractures extended downward toward the top of the magma chamber.
B, The ring fractures eventually tapped the magma chamber, the uppermost
part of which contained a high proportion of dissolved gases. With the
sudden release of pressure, tremendous amounts of hot gases and molten
Page 70
rock were erupted almost instantly. The liquid solidified into pumice, ash, and
dust as it was blown out. Some of the dust and ash was blown high into the
air and carried along by the wind, but much of the debris moved outward
across the landscape as vast ash flows, covering thousands of square miles
very rapidly.
41
C, The area overlying the blown-out part of the magma chamber collapsed to
form a gigantic caldera. The collapse took place mostly along normal faults
that developed from the fractures in the ring fracture zone. The depth of the
collapse was probably several thousand feet.
D, Renewed rise of molten rock domed the caldera floor above the magma
chamber. A series of rhyolite lava flows poured out through fractures in the
surrounding ring fracture zone and spread across the caldera floor.
dust as it was blown out. Some of the dust and ash was blown high into the
air and carried along by the wind, but much of the debris moved outward
across the landscape as vast ash flows, covering thousands of square miles
very rapidly.
41
C, The area overlying the blown-out part of the magma chamber collapsed to
form a gigantic caldera. The collapse took place mostly along normal faults
that developed from the fractures in the ring fracture zone. The depth of the
collapse was probably several thousand feet.
D, Renewed rise of molten rock domed the caldera floor above the magma
chamber. A series of rhyolite lava flows poured out through fractures in the
surrounding ring fracture zone and spread across the caldera floor.
Page 71
42
ORIGINAL EXTENT OF THE YELLOWSTONE TUFF (ash-flow tuff) that covered
most of Yellowstone National Park about 600,000 years ago. The tuff was
erupted explosively from the ring fracture zones of the Yellowstone caldera.
The outline of the caldera is shown by the dashed line. (Based on information
supplied by R. L. Christiansen and H. R. Blank, Jr.) (Fig. 24)
43
ORIGINAL EXTENT OF THE YELLOWSTONE TUFF (ash-flow tuff) that covered
most of Yellowstone National Park about 600,000 years ago. The tuff was
erupted explosively from the ring fracture zones of the Yellowstone caldera.
The outline of the caldera is shown by the dashed line. (Based on information
supplied by R. L. Christiansen and H. R. Blank, Jr.) (Fig. 24)
43
Page 72
YELLOWSTONE TUFF AT GOLDEN GATE. The rocks consist of layered ash-
flow tuff; the height of the cliff is about 200 feet. (Fig. 25)
flow tuff; the height of the cliff is about 200 feet. (Fig. 25)
Page 73
Closeup B shows typical characteristics of the tuff in most outcrop areas. Of
the light-colored materials, the larger masses are compressed pumice
fragments and the smaller masses are pumice, feldspar, and quartz. The dark
grains are chiefly magnetite and pyroxene. Closeup A is of a coarse-grained
specimen from Tuff Cliff. The large fragments are mostly crystallized pumice,
and the light-colored matrix is composed of very fine particles of volcanic ash
and dust.
44
the light-colored materials, the larger masses are compressed pumice
fragments and the smaller masses are pumice, feldspar, and quartz. The dark
grains are chiefly magnetite and pyroxene. Closeup A is of a coarse-grained
specimen from Tuff Cliff. The large fragments are mostly crystallized pumice,
and the light-colored matrix is composed of very fine particles of volcanic ash
and dust.
44
Page 74
GEOLOGIC CROSS SECTION showing generalized relationships along the
north edge of the Yellowstone caldera in the Mount Washburn-Canyon area
(line of section labeled D-D′ on pl. 1). The caldera subsided along normal
faults in the ring fracture zone, and the Plateau Rhyolite (lava flows) poured
out across the caldera floor between 600,000 and 500,000 years ago. The
faults cut across the central intrusive igneous core of the 50-million-year-old
(Eocene) Washburn volcano; the north half of the volcano is still preserved,
but the south half subsided as part of the caldera and is now buried by lava
flows. (Based on information supplied by H. J. Prostka and R. L.
Christiansen.) (Fig. 26)
Grand Canyon
Plateau Rhyolite (lava flows)
Edge of caldera
Intrusive igneous rocks of Washburn volcano
Mount Washburn
Absaroka volcanic breccias
The outpouring of lava
The final violent eruption 600,000 years ago, although releasing much of the
explosive energy of the gases contained in the magma, did not quell all
potential volcanic activity in the twin chambers. Molten rock again rose in
both of them, and in a few hundreds or thousands of years the overlying
caldera floor was domed over the two chambers. One of these prominent
domes lies near Old Faithful and the other east of Hayden Valley (figs. 22
and 23D). Soon, too, the magma found its way upward through the wide ring
fracture zones encircling the caldera. Pouring out rather quietly from many
openings (fig. 23D), the lavas flooded the caldera floor and began to fill the
still-smoldering pit. The first lavas appeared soon after the collapse 600,000
years ago, and the latest ones only 60,000-75,000 years ago. The flows were
confined chiefly to the caldera proper, but here and there they spilled out
across the rim, particularly toward the southwestern part of the Park (fig.
28). Some flows also erupted along fractures outside the caldera, the 45
most prominent flow being the very famous one at Obsidian Cliff (fig.
29).
north edge of the Yellowstone caldera in the Mount Washburn-Canyon area
(line of section labeled D-D′ on pl. 1). The caldera subsided along normal
faults in the ring fracture zone, and the Plateau Rhyolite (lava flows) poured
out across the caldera floor between 600,000 and 500,000 years ago. The
faults cut across the central intrusive igneous core of the 50-million-year-old
(Eocene) Washburn volcano; the north half of the volcano is still preserved,
but the south half subsided as part of the caldera and is now buried by lava
flows. (Based on information supplied by H. J. Prostka and R. L.
Christiansen.) (Fig. 26)
Grand Canyon
Plateau Rhyolite (lava flows)
Edge of caldera
Intrusive igneous rocks of Washburn volcano
Mount Washburn
Absaroka volcanic breccias
The outpouring of lava
The final violent eruption 600,000 years ago, although releasing much of the
explosive energy of the gases contained in the magma, did not quell all
potential volcanic activity in the twin chambers. Molten rock again rose in
both of them, and in a few hundreds or thousands of years the overlying
caldera floor was domed over the two chambers. One of these prominent
domes lies near Old Faithful and the other east of Hayden Valley (figs. 22
and 23D). Soon, too, the magma found its way upward through the wide ring
fracture zones encircling the caldera. Pouring out rather quietly from many
openings (fig. 23D), the lavas flooded the caldera floor and began to fill the
still-smoldering pit. The first lavas appeared soon after the collapse 600,000
years ago, and the latest ones only 60,000-75,000 years ago. The flows were
confined chiefly to the caldera proper, but here and there they spilled out
across the rim, particularly toward the southwestern part of the Park (fig.
28). Some flows also erupted along fractures outside the caldera, the 45
most prominent flow being the very famous one at Obsidian Cliff (fig.
29).
Page 75
YELLOWSTONE LAKE. View southeast across Yellowstone Lake toward the
western foothills and crest of the Absaroka Range. The Absaroka Range is an
erosional remnant of a vast pile of volcanic lavas and breccias (Absaroka
volcanic rocks) that once covered all of Yellowstone; the lake occupies part of
the Yellowstone caldera. (Fig. 27)
The chief rock type in the lava flows is rhyolite, similar in composition to
the welded tufts erupted earlier but different in other major characteristics.
The rock, for example, shows much contorted layering as evidence of having
flowed as a thick liquid across the ground (fig. 30). A coarse brecciated
western foothills and crest of the Absaroka Range. The Absaroka Range is an
erosional remnant of a vast pile of volcanic lavas and breccias (Absaroka
volcanic rocks) that once covered all of Yellowstone; the lake occupies part of
the Yellowstone caldera. (Fig. 27)
The chief rock type in the lava flows is rhyolite, similar in composition to
the welded tufts erupted earlier but different in other major characteristics.
The rock, for example, shows much contorted layering as evidence of having
flowed as a thick liquid across the ground (fig. 30). A coarse brecciated
Page 76
texture is also a common feature, well shown by lavas along the Firehole
Canyon drive (fig. 31). Locally, some parts of the flows cooled so rapidly
that few crystals formed, and the lava solidified mainly into a natural glass
(fig. 32).
46
Canyon drive (fig. 31). Locally, some parts of the flows cooled so rapidly
that few crystals formed, and the lava solidified mainly into a natural glass
(fig. 32).
46
Page 77
Page 78
RADAR IMAGE of a part of southwestern Yellowstone National Park. The
lobate landforms are the edges of a lava flow of the Plateau Rhyolite that
forms the Pitchstone Plateau (fig. 1). The low concentric ridges that parallel
the toe of the flow are pressure ridges produced by the wrinkling of the nearly
solidified crust of lava along the edge of the flow. (Image courtesy of National
Aeronautics and Space Administration.) (Fig. 28)
47
OBSIDIAN CLIFF, Jim Bridger’s famous “mountain of glass.” The rock is
rhyolite lava which contains a high proportion of obsidian, a kind of black
volcanic glass. Note columnar jointing along the sides of the cliff, similar to
lobate landforms are the edges of a lava flow of the Plateau Rhyolite that
forms the Pitchstone Plateau (fig. 1). The low concentric ridges that parallel
the toe of the flow are pressure ridges produced by the wrinkling of the nearly
solidified crust of lava along the edge of the flow. (Image courtesy of National
Aeronautics and Space Administration.) (Fig. 28)
47
OBSIDIAN CLIFF, Jim Bridger’s famous “mountain of glass.” The rock is
rhyolite lava which contains a high proportion of obsidian, a kind of black
volcanic glass. Note columnar jointing along the sides of the cliff, similar to
Page 79
that shown by the basalt flows at Tower (fig. 33). The cliff is approximately 200
feet high. (Fig. 29)
48
THICK RHYOLITE LAVA FLOW along west bank of Firehole River. (Fig. 30)
feet high. (Fig. 29)
48
THICK RHYOLITE LAVA FLOW along west bank of Firehole River. (Fig. 30)
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Closeup view is of a cut surface of rhyolite, showing the striking banding that
results from the flowage of viscous molten rock. The dark bands are chiefly
concentrations of volcanic glass (also some cavities), and the light bands are
concentrations of tiny crystals of feldspar and quartz.
49
results from the flowage of viscous molten rock. The dark bands are chiefly
concentrations of volcanic glass (also some cavities), and the light bands are
concentrations of tiny crystals of feldspar and quartz.
49
Page 81
BRECCIATED RHYOLITE LAVA FLOWS along the Firehole Canyon drive. As a
lava flow moves outward from its center of eruption, a chilled crust develops
along its upper surface and outer edges because of the cooler temperatures
in those parts of the flow. Continued movement of the still-molten rock in the
interior of the flow causes this crust to break up (brecciate) into angular
lava flow moves outward from its center of eruption, a chilled crust develops
along its upper surface and outer edges because of the cooler temperatures
in those parts of the flow. Continued movement of the still-molten rock in the
interior of the flow causes this crust to break up (brecciate) into angular
Page 82
blocks. The blocks are then tumbled along until the whole mass finally
solidifies. (Fig. 31)
50
OUTCROP OF GLASSY RHYOLITE LAVA along the road between Canyon
Village and Norris Junction. The conspicuous lines in the face of the rock
outline different layers produced by lava flowage. The feldspar crystals are
alined parallel to the direction of flow. (Fig. 32)
solidifies. (Fig. 31)
50
OUTCROP OF GLASSY RHYOLITE LAVA along the road between Canyon
Village and Norris Junction. The conspicuous lines in the face of the rock
outline different layers produced by lava flowage. The feldspar crystals are
alined parallel to the direction of flow. (Fig. 32)
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In closeup A, dark parts of the rock are volcanic glass (closeup B shows
glassy fracture) and light-colored crystals are quartz (blocky) and feldspar
(tabular).
glassy fracture) and light-colored crystals are quartz (blocky) and feldspar
(tabular).
Page 84
Closeup B.
About 30 different flows have been recognized. Grouped within a 51
major rock unit called the Plateau Rhyolite (fig. 5), they cover more
than 1,000 square miles. The gently rolling plateau surface of central
Yellowstone, broken here and there by clusters of low-lying hills and ridges,
is essentially the landscape that characterized the upper surfaces of the lava
flows soon after they cooled and solidified. Natural valleys formed between
some of the adjacent flows, and in places streams still follow these
readymade channels. Rhyolite, in both lava flows and ash-flow tuffs, is by
far the predominant rock type seen along the Park roads.
Several basalt flows were erupted along with the more common rhyolite
flows, and in the vicinity of Tower Falls they form some of the most unusual
rock units in the whole Park area (fig. 33). As the flows cooled, contraction
About 30 different flows have been recognized. Grouped within a 51
major rock unit called the Plateau Rhyolite (fig. 5), they cover more
than 1,000 square miles. The gently rolling plateau surface of central
Yellowstone, broken here and there by clusters of low-lying hills and ridges,
is essentially the landscape that characterized the upper surfaces of the lava
flows soon after they cooled and solidified. Natural valleys formed between
some of the adjacent flows, and in places streams still follow these
readymade channels. Rhyolite, in both lava flows and ash-flow tuffs, is by
far the predominant rock type seen along the Park roads.
Several basalt flows were erupted along with the more common rhyolite
flows, and in the vicinity of Tower Falls they form some of the most unusual
rock units in the whole Park area (fig. 33). As the flows cooled, contraction
Page 85
cracks broke the basalt into a series of upright many-sided columns; from a
distance they appear as a solid row of fenceposts. They are now covered by
younger rocks, but if one could see the upper flat surface of the basalt layers
where just the ends of the columns are sticking out, the pattern would be like
that seen in a honeycomb.
During the eruptions of the Plateau Rhyolite, at least one relatively small
caldera-making event occurred in the central Yellowstone region. This
“inner” caldera developed sometime between 125,000 and 200,000 years
ago, forming the deep depression now filled by the West Thumb of
Yellowstone Lake (fig. 22). Like the main Yellowstone caldera, but on a
much smaller scale, it formed as a direct result of the explosive eruption of
rhyolitic ash flows and subsequent collapse of an oval-shaped area
approximately 4 miles wide and 6 miles long. West Thumb is nearly the
same size as Crater Lake, Oregon, which occupies one of the world’s best-
known calderas.
With the outpouring of the last lava flows 60,000-75,000 years ago, the
forces of Quaternary volcanism finally died down. The hot-water and steam
activity, however, still remains as a vivid reminder of Yellowstone’s volcanic
past. But who can say even now that we are witnessing the final stage of
volcanism? Someday, quite conceivably, there might be yet another outburst
of molten rock—only time, of course, will tell.
52
distance they appear as a solid row of fenceposts. They are now covered by
younger rocks, but if one could see the upper flat surface of the basalt layers
where just the ends of the columns are sticking out, the pattern would be like
that seen in a honeycomb.
During the eruptions of the Plateau Rhyolite, at least one relatively small
caldera-making event occurred in the central Yellowstone region. This
“inner” caldera developed sometime between 125,000 and 200,000 years
ago, forming the deep depression now filled by the West Thumb of
Yellowstone Lake (fig. 22). Like the main Yellowstone caldera, but on a
much smaller scale, it formed as a direct result of the explosive eruption of
rhyolitic ash flows and subsequent collapse of an oval-shaped area
approximately 4 miles wide and 6 miles long. West Thumb is nearly the
same size as Crater Lake, Oregon, which occupies one of the world’s best-
known calderas.
With the outpouring of the last lava flows 60,000-75,000 years ago, the
forces of Quaternary volcanism finally died down. The hot-water and steam
activity, however, still remains as a vivid reminder of Yellowstone’s volcanic
past. But who can say even now that we are witnessing the final stage of
volcanism? Someday, quite conceivably, there might be yet another outburst
of molten rock—only time, of course, will tell.
52
Page 86
TWO LEDGES OF BASALT spectacularly exposed in the east wall of the
Grand Canyon of the Yellowstone at The Narrows near Tower Falls. The light-
colored rocks between the basalt flows are ancient stream gravels deposited
about 1½ million years ago, when the channel of the Yellowstone River was
farther east and not as deep as it is today. The hill is capped by lake
sediments, sand, and gravel deposited when the Yellowstone River was
blocked by a glacial dam farther downstream (to the left). The brown rocks at
the base of the cliff are Absaroka andesite breccias. (Fig. 33)
Grand Canyon of the Yellowstone at The Narrows near Tower Falls. The light-
colored rocks between the basalt flows are ancient stream gravels deposited
about 1½ million years ago, when the channel of the Yellowstone River was
farther east and not as deep as it is today. The hill is capped by lake
sediments, sand, and gravel deposited when the Yellowstone River was
blocked by a glacial dam farther downstream (to the left). The brown rocks at
the base of the cliff are Absaroka andesite breccias. (Fig. 33)
Page 87
Pronounced columnar jointing of the basalt is seen at close range at the edge
of the road on the opposite (west) side of the canyon. Inset shows the dense
character of the black basalt, which consists of microscopic crystals of
feldspar, pyroxene, olivine, and magnetite.
53
of the road on the opposite (west) side of the canyon. Inset shows the dense
character of the black basalt, which consists of microscopic crystals of
feldspar, pyroxene, olivine, and magnetite.
53
Page 88
Final Sculpturing of the Landscape
The many episodes of mountain building and volcanism all left their lasting
and unmistakable imprints across the face of the Yellowstone country.
During the latter part of the Tertiary Period, erosion, too, had begun to make
its own deep marks. But only in the last 100,000 years or so have the
powerful exterior forces of the earth—chiefly running water and moving ice
—had a virtually free hand in shaping the Park’s landscape. Nevertheless, in
this short period of time they have wrought profound changes.
Glaciation
A giant boulder of Precambrian gneiss lies among the trees beside the road
leading to Inspiration Point on the north rim of the Grand Canyon of the
Yellowstone (fig. 34). This boulder, measuring approximately 24×20×18 feet
and weighing at least 500 tons, is of considerable interest, not so much for its
great size but because it is completely out-of-place in its present
surroundings. The boulder rests on rhyolite lava flows of Quaternary age, at
The many episodes of mountain building and volcanism all left their lasting
and unmistakable imprints across the face of the Yellowstone country.
During the latter part of the Tertiary Period, erosion, too, had begun to make
its own deep marks. But only in the last 100,000 years or so have the
powerful exterior forces of the earth—chiefly running water and moving ice
—had a virtually free hand in shaping the Park’s landscape. Nevertheless, in
this short period of time they have wrought profound changes.
Glaciation
A giant boulder of Precambrian gneiss lies among the trees beside the road
leading to Inspiration Point on the north rim of the Grand Canyon of the
Yellowstone (fig. 34). This boulder, measuring approximately 24×20×18 feet
and weighing at least 500 tons, is of considerable interest, not so much for its
great size but because it is completely out-of-place in its present
surroundings. The boulder rests on rhyolite lava flows of Quaternary age, at
Page 89
least 15 miles from the nearest outcrops of the ancient gneiss to the north
and northeast. Obviously, this seemingly immovable chunk of rock 54
was pushed or carried a long way by some very powerful transporting
agent before it was finally dropped. A natural force of such magnitude could
only have been exerted by moving ice; in fact, no further proof than this one
boulder is needed for us to conclude beyond question that glaciers once
existed in Yellowstone. There is, to be sure, much additional evidence that
the Park region was extensively glaciated. Deposits of out-of-place boulders
(glacial erratics), like the one mentioned above, are found nearly
everywhere (fig. 35) and the mountains and high valleys still bear the vivid
scars of ice sculpturing (figs. 36 and 37).
and northeast. Obviously, this seemingly immovable chunk of rock 54
was pushed or carried a long way by some very powerful transporting
agent before it was finally dropped. A natural force of such magnitude could
only have been exerted by moving ice; in fact, no further proof than this one
boulder is needed for us to conclude beyond question that glaciers once
existed in Yellowstone. There is, to be sure, much additional evidence that
the Park region was extensively glaciated. Deposits of out-of-place boulders
(glacial erratics), like the one mentioned above, are found nearly
everywhere (fig. 35) and the mountains and high valleys still bear the vivid
scars of ice sculpturing (figs. 36 and 37).
Page 90
GIANT BOULDER (glacial erratic) of Precambrian gneiss near Inspiration
Point on the north rim of the Grand Canyon. The boulder, measuring
24×20×18 feet and weighing more than 500 tons, was dropped at this locality
by glacial ice; it now rests on the much younger Plateau Rhyolite. The
distance that the boulder was carried or pushed was at least 15 miles. (Fig.
34)
The principal requirement for the formation of glaciers is simple: more 55
snow has to accumulate during the winter than is melted during the
Point on the north rim of the Grand Canyon. The boulder, measuring
24×20×18 feet and weighing more than 500 tons, was dropped at this locality
by glacial ice; it now rests on the much younger Plateau Rhyolite. The
distance that the boulder was carried or pushed was at least 15 miles. (Fig.
34)
The principal requirement for the formation of glaciers is simple: more 55
snow has to accumulate during the winter than is melted during the
Page 91
summer. If this condition continues for a long enough period of time
(measured in centuries), the snow compacts to ice, and extensive icefields
grow until they finally begin to move under their own weight, thereby
becoming glaciers. Records show that the average year-round temperature is
32°-33°F along Yellowstone Lake, 35°F at Old Faithful, and 39°F at
Mammoth. Each winter, snow accumulates to depths of 5-10 feet throughout
much of the Park. If the average annual temperatures were to decrease a few
degrees or the yearly snowfall were to increase a foot or so, either change
could possibly herald the beginning of another ice age in the Yellowstone
region.
Yellowstone was glaciated at least three times. These glaciations are, from
oldest to youngest, the pre-Bull Lake, Bull Lake, and Pinedale. Their precise
age and duration are imperfectly known, but estimates based on a few
radiometric determinations are: (1) the oldest glaciation (pre-Bull Lake
glaciation) began more than 300,000 years ago and ended between 180,000
and 200,000 years ago; (2) Bull Lake Glaciation began about 125,000 years
ago and ended more than 45,000 years ago; (3) Pinedale Glaciation began
about 25,000 years ago and ended about 8,500 years ago. The pre-Bull Lake
and Bull Lake are known only from scattered deposits of rock debris (glacial
moraines) and other features, but the distribution of these deposits indicates
that glaciers were widespread throughout the region and occurred both
between and during eruptions of the Plateau Rhyolite. The effects of the
Pinedale glaciers, on the other hand, are obvious in many parts of the Park,
and the history of this youngest glacial cycle (described below) is known in
much greater detail than that of the two older ones.
In the early stages of Pinedale Glaciation, an enormous icefield built up in
the high Absaroka Range southeast of the Park area. A glacier, fed by this
icefield, flowed northward down the upper Yellowstone valley and into 56
the basin now occupied by Yellowstone Lake. At about the same time,
another great icefield formed in the mountains north of the Park and sent
long tongues of ice southward toward the lower Yellowstone and Lamar
River valleys. Smaller valley glaciers flowed westward out of the Absaroka
Range along the east edge of the Park, and still others formed along the main
ridges and valleys of the Gallatin Range, in the northwestern part of the
Park. Thus, many huge masses of ice from the north, east, and southeast
converged and met in the Park. At this stage, probably about 15,000 years
(measured in centuries), the snow compacts to ice, and extensive icefields
grow until they finally begin to move under their own weight, thereby
becoming glaciers. Records show that the average year-round temperature is
32°-33°F along Yellowstone Lake, 35°F at Old Faithful, and 39°F at
Mammoth. Each winter, snow accumulates to depths of 5-10 feet throughout
much of the Park. If the average annual temperatures were to decrease a few
degrees or the yearly snowfall were to increase a foot or so, either change
could possibly herald the beginning of another ice age in the Yellowstone
region.
Yellowstone was glaciated at least three times. These glaciations are, from
oldest to youngest, the pre-Bull Lake, Bull Lake, and Pinedale. Their precise
age and duration are imperfectly known, but estimates based on a few
radiometric determinations are: (1) the oldest glaciation (pre-Bull Lake
glaciation) began more than 300,000 years ago and ended between 180,000
and 200,000 years ago; (2) Bull Lake Glaciation began about 125,000 years
ago and ended more than 45,000 years ago; (3) Pinedale Glaciation began
about 25,000 years ago and ended about 8,500 years ago. The pre-Bull Lake
and Bull Lake are known only from scattered deposits of rock debris (glacial
moraines) and other features, but the distribution of these deposits indicates
that glaciers were widespread throughout the region and occurred both
between and during eruptions of the Plateau Rhyolite. The effects of the
Pinedale glaciers, on the other hand, are obvious in many parts of the Park,
and the history of this youngest glacial cycle (described below) is known in
much greater detail than that of the two older ones.
In the early stages of Pinedale Glaciation, an enormous icefield built up in
the high Absaroka Range southeast of the Park area. A glacier, fed by this
icefield, flowed northward down the upper Yellowstone valley and into 56
the basin now occupied by Yellowstone Lake. At about the same time,
another great icefield formed in the mountains north of the Park and sent
long tongues of ice southward toward the lower Yellowstone and Lamar
River valleys. Smaller valley glaciers flowed westward out of the Absaroka
Range along the east edge of the Park, and still others formed along the main
ridges and valleys of the Gallatin Range, in the northwestern part of the
Park. Thus, many huge masses of ice from the north, east, and southeast
converged and met in the Park. At this stage, probably about 15,000 years
Page 92
ago, only the west edge of the Park, and perhaps a few of the highest peaks
and ridges within the Park, remained free of ice. It is interesting to note that
although ice moved across and buried the ancestral Grand Canyon of the
Yellowstone, it did not flow down and scour the canyon (fig. 36). If it had,
the canyon would look much different than it does today (fig. 41).
GLACIATED TERRAIN along the Northeast Entrance road. The boulders, many
of them measuring 10 feet across or more, were carried into the area by ice
flowing down Slough Creek from mountains north of the Park during the
Pinedale Glaciation. As the glaciers melted, the boulders were left stranded in
hummocky, morainal deposits. Shallow depressions in the irregular
topography are now commonly filled by small ponds. (Fig. 35)
For the next 10,000 years, the ice thickened and spread out over more and
more of the Park area. The mass centered over the Yellowstone Lake basin
grew to a depth of 3,000 feet or more and dominated the entire scene; it
formed a broad “mountain” of ice which became so high that it caused more
snow to fall upon itself and was cold enough to prevent much of this snow
from melting. Eventually the Pinedale glaciers covered about 90 percent of
Yellowstone (fig. 38).
57
and ridges within the Park, remained free of ice. It is interesting to note that
although ice moved across and buried the ancestral Grand Canyon of the
Yellowstone, it did not flow down and scour the canyon (fig. 36). If it had,
the canyon would look much different than it does today (fig. 41).
GLACIATED TERRAIN along the Northeast Entrance road. The boulders, many
of them measuring 10 feet across or more, were carried into the area by ice
flowing down Slough Creek from mountains north of the Park during the
Pinedale Glaciation. As the glaciers melted, the boulders were left stranded in
hummocky, morainal deposits. Shallow depressions in the irregular
topography are now commonly filled by small ponds. (Fig. 35)
For the next 10,000 years, the ice thickened and spread out over more and
more of the Park area. The mass centered over the Yellowstone Lake basin
grew to a depth of 3,000 feet or more and dominated the entire scene; it
formed a broad “mountain” of ice which became so high that it caused more
snow to fall upon itself and was cold enough to prevent much of this snow
from melting. Eventually the Pinedale glaciers covered about 90 percent of
Yellowstone (fig. 38).
57
Page 93
CANYON PROFILES. Typical profiles of a canyon cut by a stream (A) and of a
canyon gouged by a glacier (B). Glacial cirques (C) are shown at the head and
high on the side of the glaciated valley. (Fig. 36)
58
canyon gouged by a glacier (B). Glacial cirques (C) are shown at the head and
high on the side of the glaciated valley. (Fig. 36)
58
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GLACIAL CIRQUE on east face of Electric Peak, northern Gallatin Range.
During several episodes of glaciation, this steep-walled amphitheaterlike
valley was cut and filled by ice which fed glaciers moving downslope to the
lower right. The cirque floor is now covered by a thick deposit of rock rubble
underlain in part by ice, and the whole mass is still moving slowly downhill as
a rock glacier. The dark rock at lower right is part of the Electric Peak stock,
composed of diorite (fig. 20) and other kinds of intrusive igneous rocks. The
rocks in the cirque walls are chiefly Cretaceous shales (light to moderately
dark color) with thin sills of igneous rock (very dark color). (West-looking
oblique aerial photograph, courtesy of William B. Hall, University of Idaho.)
(Fig. 37)
After their maximum advance, the Pinedale glaciers began to melt, 59
leaving behind the rock debris they had gouged from the landscape and
had pushed or carried along with them. These glacial moraines are now
found in many areas throughout the Park. In places, glacial ice and (or) rock
debris formed natural dams across stream valleys, thereby impounding lakes.
Parts of Hayden Valley, for example, contain layers of very fine sand, silt,
and clay several tens of feet thick (fig. 39) that accumulated along the
bottom of a large lake. This lake formed behind a glacial dam across the
During several episodes of glaciation, this steep-walled amphitheaterlike
valley was cut and filled by ice which fed glaciers moving downslope to the
lower right. The cirque floor is now covered by a thick deposit of rock rubble
underlain in part by ice, and the whole mass is still moving slowly downhill as
a rock glacier. The dark rock at lower right is part of the Electric Peak stock,
composed of diorite (fig. 20) and other kinds of intrusive igneous rocks. The
rocks in the cirque walls are chiefly Cretaceous shales (light to moderately
dark color) with thin sills of igneous rock (very dark color). (West-looking
oblique aerial photograph, courtesy of William B. Hall, University of Idaho.)
(Fig. 37)
After their maximum advance, the Pinedale glaciers began to melt, 59
leaving behind the rock debris they had gouged from the landscape and
had pushed or carried along with them. These glacial moraines are now
found in many areas throughout the Park. In places, glacial ice and (or) rock
debris formed natural dams across stream valleys, thereby impounding lakes.
Parts of Hayden Valley, for example, contain layers of very fine sand, silt,
and clay several tens of feet thick (fig. 39) that accumulated along the
bottom of a large lake. This lake formed behind a glacial dam across the
Page 95
Yellowstone River near Upper Falls. Some of the glacial dams broke and
released water catastrophically, causing giant floods; the occurrence of one
such flood is particularly evident along the Yellowstone River valley near
Gardiner, Montana.
By about 12,000 years ago the thick Pinedale ice sheet had melted entirely
from the Yellowstone Lake basin and most other areas of the Park, although
valley glaciers continued to exist in the mountains until about 8,500 years
ago. Then, following a short period of total disappearance, small icefields
formed again in the heads of some of the higher mountain valleys. Since the
melting of the Pinedale ice, however, none has descended as a glacier into
the lower stretches of the valleys. Even though a few snowfields persist
locally throughout the summers (except during the warmest years), no
glaciers exist in the Park at the present time.
60
released water catastrophically, causing giant floods; the occurrence of one
such flood is particularly evident along the Yellowstone River valley near
Gardiner, Montana.
By about 12,000 years ago the thick Pinedale ice sheet had melted entirely
from the Yellowstone Lake basin and most other areas of the Park, although
valley glaciers continued to exist in the mountains until about 8,500 years
ago. Then, following a short period of total disappearance, small icefields
formed again in the heads of some of the higher mountain valleys. Since the
melting of the Pinedale ice, however, none has descended as a glacier into
the lower stretches of the valleys. Even though a few snowfields persist
locally throughout the summers (except during the warmest years), no
glaciers exist in the Park at the present time.
60
Page 96
EXTENT OF ICE in Yellowstone National Park during the maximum spreading
of the Pinedale glaciers, probably about 15,000 years ago. Long arrows
indicate direction of strong flowage of ice; short arrows show direction of
less vigorous ice flowage. The dark-blue area shows the main ice mass
centered over the Yellowstone Lake basin in the southeast corner of the Park.
Many of the high peaks and ridges such as Mount Washburn, which are here
shown free of ice, were glaciated at least once during the past 250,000 years.
Whether they were covered by the Pinedale glaciers, however, is still an
unresolved question. (Based on information supplied by G. M. Richmond, K.
L. Pierce, and H. A. Waldrop.) (Fig. 38)
of the Pinedale glaciers, probably about 15,000 years ago. Long arrows
indicate direction of strong flowage of ice; short arrows show direction of
less vigorous ice flowage. The dark-blue area shows the main ice mass
centered over the Yellowstone Lake basin in the southeast corner of the Park.
Many of the high peaks and ridges such as Mount Washburn, which are here
shown free of ice, were glaciated at least once during the past 250,000 years.
Whether they were covered by the Pinedale glaciers, however, is still an
unresolved question. (Based on information supplied by G. M. Richmond, K.
L. Pierce, and H. A. Waldrop.) (Fig. 38)
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61
FLAT-LYING BEDS of fine sand, silt, and clay near the mouth of Trout Creek in
Hayden Valley. These beds were deposited in a glacially dammed lake that
covered part of Hayden Valley when the Pinedale glaciers were melting. The
height of the streambank is about 40 feet. (Fig. 39)
FLAT-LYING BEDS of fine sand, silt, and clay near the mouth of Trout Creek in
Hayden Valley. These beds were deposited in a glacially dammed lake that
covered part of Hayden Valley when the Pinedale glaciers were melting. The
height of the streambank is about 40 feet. (Fig. 39)
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62
Page 99
WATERFALLS in Yellowstone National Park. (Fig. 40)
A, Lewis Falls on the Lewis River. The falls cascade over the steep edge of a
rhyolite lava flow.
A, Lewis Falls on the Lewis River. The falls cascade over the steep edge of a
rhyolite lava flow.
Page 100
B, Upper Falls on the Yellowstone River. The brink of the falls marks the
contact between dense, resistant rhyolite lava (which forms the massive cliff)
and more easily eroded rhyolite lava containing a high proportion of volcanic
glass immediately downstream, as shown in figure 42.
contact between dense, resistant rhyolite lava (which forms the massive cliff)
and more easily eroded rhyolite lava containing a high proportion of volcanic
glass immediately downstream, as shown in figure 42.
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C, Gibbon Falls on the Gibbon River. The river tumbles over a scarp etched in
the Yellowstone Tuff. The scarp first formed along faults at the north edge of
the Yellowstone caldera 600,000 years ago, at a point that now lies ¼ to ½
mile downstream. Continued erosion has caused the falls to recede
northward to their present position.
the Yellowstone Tuff. The scarp first formed along faults at the north edge of
the Yellowstone caldera 600,000 years ago, at a point that now lies ¼ to ½
mile downstream. Continued erosion has caused the falls to recede
northward to their present position.
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D, Tower Falls on Tower Creek. The rocks at the brink of the falls, and in the
vertical cliff beneath, are coarse breccias and conglomerates of the Absaroka
volcanic rocks. The channel of Tower Creek has not been cut down rapidly
enough to keep pace with the downcutting of the main channel of the
Yellowstone River, which lies a short distance downstream from the base of
the falls.
63
Running water—canyons and waterfalls
Yellowstone is, among its many attributes, the source of large and mighty
rivers. Located across the Continental Divide, the Park feeds two of the most
extensive drainage systems in the nation—(1) the Missouri River system
(and ultimately the Mississippi River) on the Atlantic side, via the
Yellowstone, Madison, and Gallatin Rivers, and (2) the Columbia River
system on the Pacific side, via the Snake River (fig. 1). These streams are
vertical cliff beneath, are coarse breccias and conglomerates of the Absaroka
volcanic rocks. The channel of Tower Creek has not been cut down rapidly
enough to keep pace with the downcutting of the main channel of the
Yellowstone River, which lies a short distance downstream from the base of
the falls.
63
Running water—canyons and waterfalls
Yellowstone is, among its many attributes, the source of large and mighty
rivers. Located across the Continental Divide, the Park feeds two of the most
extensive drainage systems in the nation—(1) the Missouri River system
(and ultimately the Mississippi River) on the Atlantic side, via the
Yellowstone, Madison, and Gallatin Rivers, and (2) the Columbia River
system on the Pacific side, via the Snake River (fig. 1). These streams are
Page 103
fed by an annual precipitation which averages about 17 inches at Old
Faithful and Mammoth, but which is considerably greater in the mountain
ranges.
Many stretches of the main river valleys in Yellowstone are broad and flat
bottomed. In these, the stream gradients range from about 10 to 30 feet per
mile, and there is little erosion going on at present (Hayden Valley is a good
example, fig. 4). But here and there the gradients are steeper, and the valleys
are narrow and rugged. In some places these streams drop 50 or even 100
feet per mile, and the fast-moving waters have carved deep V-shaped gorges
(fig. 36).
Waterfalls, features for which Yellowstone is also justly famous (fig. 40),
generally result from abrupt differences in rock hardness. If a stream flows
over rocks that are more resistant to erosion than the rocks immediately
downstream, a ledge or bench will form across the streambed at that place
because the less resistant rocks are worn away faster. And, as the ledge 64
becomes higher, the softer downstream rocks will erode even faster. A
true waterfall is one in which there is a free, vertical fall of water. If the
ledge or ledges form only a rough, steep runway in the streambed, then the
term “rapids” or “cascades” is more appropriate.
The existence of many waterfalls in Yellowstone today is due in large part to
the fact that, because of recent volcanism and glaciation, much of the
region’s topography is very young in terms of geologic time. Streams, even
some of the largest ones, have not had enough time to wear away all the
features that may produce waterfalls, cascades, or rapids along their
channels. This is particularly true along the margins of lava flows, where
there are sharp dropoffs between the tops of the flows and the lower ground
beyond. The Grand Canyon of the Yellowstone and the Upper and Lower
Falls, well illustrate the erosive power of running water.
Grand Canyon of the Yellowstone
Except for Old Faithful, the Grand Canyon of the Yellowstone is probably
the best known and most talked about and photographed feature in the Park
Faithful and Mammoth, but which is considerably greater in the mountain
ranges.
Many stretches of the main river valleys in Yellowstone are broad and flat
bottomed. In these, the stream gradients range from about 10 to 30 feet per
mile, and there is little erosion going on at present (Hayden Valley is a good
example, fig. 4). But here and there the gradients are steeper, and the valleys
are narrow and rugged. In some places these streams drop 50 or even 100
feet per mile, and the fast-moving waters have carved deep V-shaped gorges
(fig. 36).
Waterfalls, features for which Yellowstone is also justly famous (fig. 40),
generally result from abrupt differences in rock hardness. If a stream flows
over rocks that are more resistant to erosion than the rocks immediately
downstream, a ledge or bench will form across the streambed at that place
because the less resistant rocks are worn away faster. And, as the ledge 64
becomes higher, the softer downstream rocks will erode even faster. A
true waterfall is one in which there is a free, vertical fall of water. If the
ledge or ledges form only a rough, steep runway in the streambed, then the
term “rapids” or “cascades” is more appropriate.
The existence of many waterfalls in Yellowstone today is due in large part to
the fact that, because of recent volcanism and glaciation, much of the
region’s topography is very young in terms of geologic time. Streams, even
some of the largest ones, have not had enough time to wear away all the
features that may produce waterfalls, cascades, or rapids along their
channels. This is particularly true along the margins of lava flows, where
there are sharp dropoffs between the tops of the flows and the lower ground
beyond. The Grand Canyon of the Yellowstone and the Upper and Lower
Falls, well illustrate the erosive power of running water.
Grand Canyon of the Yellowstone
Except for Old Faithful, the Grand Canyon of the Yellowstone is probably
the best known and most talked about and photographed feature in the Park
Page 104
(fig. 41). Although not so deep or wide as some of the other great canyons in
America, its sheer ruggedness and beauty are breathtaking. Here the aptness
of the name “Yellowstone” can be fully appreciated and understood, for the
viewer is at once engulfed in a sea of yellow hues streaked and tinted with
various shades of red and brown.
65
America, its sheer ruggedness and beauty are breathtaking. Here the aptness
of the name “Yellowstone” can be fully appreciated and understood, for the
viewer is at once engulfed in a sea of yellow hues streaked and tinted with
various shades of red and brown.
65
Page 105
GRAND CANYON AND LOWER FALLS of the Yellowstone River, as viewed
upstream (southwest) from Artists Point on the south rim. The yellow-hued
rocks lining the canyon walls are soft, hydrothermally altered rhyolite lavas.
The rocks at the brink of the falls consist of less altered and therefore more
upstream (southwest) from Artists Point on the south rim. The yellow-hued
rocks lining the canyon walls are soft, hydrothermally altered rhyolite lavas.
The rocks at the brink of the falls consist of less altered and therefore more
Page 106
resistant rhyolites. The falls, 309 feet high, formed at the contact between the
hard and soft rhyolite units. (Photograph courtesy of Sgt. James E. Jensen,
U.S. Air Force.) (Fig. 41)
66
DEVELOPMENT OF GRAND CANYON. Profiles along the floor of the Grand
Canyon of the Yellowstone as it appears today (C) and as it appeared at two
older stages in its development (A and B). Note particularly the various kinds
of rocks through which the canyon has been cut, and how rock differences
have influenced the location of the two falls. Diagonal lines indicate unaltered
rhyolite; large dots, rhyolite with much volcanic glass; small dots,
hydrothermally altered rhyolite; and circles and dots, Absaroka volcanic
hard and soft rhyolite units. (Photograph courtesy of Sgt. James E. Jensen,
U.S. Air Force.) (Fig. 41)
66
DEVELOPMENT OF GRAND CANYON. Profiles along the floor of the Grand
Canyon of the Yellowstone as it appears today (C) and as it appeared at two
older stages in its development (A and B). Note particularly the various kinds
of rocks through which the canyon has been cut, and how rock differences
have influenced the location of the two falls. Diagonal lines indicate unaltered
rhyolite; large dots, rhyolite with much volcanic glass; small dots,
hydrothermally altered rhyolite; and circles and dots, Absaroka volcanic
Page 107
rocks. (Based on information furnished by R. L. Christiansen and G. M.
Richmond; vertical scale is exaggerated about 10 times.) (Fig. 42)
C: As it appears today
Yellowstone Lake
Hayden Valley
Grand Canyon of the Yellowstone
Upper Falls
Lower Falls
Inspiration Point
North edge of Yellowstone caldera
Confluence of Lamar and Yellowstone Rivers
B: A stage somewhat before 300,000 years ago
Profile of Yellowstone River today
A: A stage somewhat before 600,000 years ago
Profile of Yellowstone River today
At first glance, the canyon may appear to be a giant crack which 67
suddenly opened up and into which the Yellowstone River then
plunged headlong over high waterfalls at its southwest end. This, of course,
is not the way the canyon formed. Nevertheless, it is apparent that certain
unusual conditions caused the river, after winding slowly through flat-
floored Hayden Valley for about 13 miles, to cut a precipitous gorge 1,000-
1,500 feet deep and 20 miles long (fig. 42C). A full explanation must be
based on all the many events surrounding the eruption of the Yellowstone
Tuff, the collapse of the Yellowstone caldera, the outpouring of the Plateau
Rhyolite, and the various episodes of glaciation. Geologic studies show that
all these events took place while the canyon was being cut, and that each one
played an important role in its development. Hot-water and steam activity
likewise was a significant factor. However, despite its many complexities,
the history of the Grand Canyon can be divided into a few major stages, as
outlined below:
1. From more than 2,000,000 years ago to about 600,000 years ago, a
shallow canyon was gradually being cut into the Absaroka volcanic
sequence by the ancestral Yellowstone River as it eroded headward from a
point near the present confluence of the Yellowstone and Lamar Rivers
(fig. 33). By the time of the climactic volcanic eruption in central
Yellowstone 600,000 years ago, the head of the “old” canyon probably
had been eroded southward nearly to the place where the north rim of the
Richmond; vertical scale is exaggerated about 10 times.) (Fig. 42)
C: As it appears today
Yellowstone Lake
Hayden Valley
Grand Canyon of the Yellowstone
Upper Falls
Lower Falls
Inspiration Point
North edge of Yellowstone caldera
Confluence of Lamar and Yellowstone Rivers
B: A stage somewhat before 300,000 years ago
Profile of Yellowstone River today
A: A stage somewhat before 600,000 years ago
Profile of Yellowstone River today
At first glance, the canyon may appear to be a giant crack which 67
suddenly opened up and into which the Yellowstone River then
plunged headlong over high waterfalls at its southwest end. This, of course,
is not the way the canyon formed. Nevertheless, it is apparent that certain
unusual conditions caused the river, after winding slowly through flat-
floored Hayden Valley for about 13 miles, to cut a precipitous gorge 1,000-
1,500 feet deep and 20 miles long (fig. 42C). A full explanation must be
based on all the many events surrounding the eruption of the Yellowstone
Tuff, the collapse of the Yellowstone caldera, the outpouring of the Plateau
Rhyolite, and the various episodes of glaciation. Geologic studies show that
all these events took place while the canyon was being cut, and that each one
played an important role in its development. Hot-water and steam activity
likewise was a significant factor. However, despite its many complexities,
the history of the Grand Canyon can be divided into a few major stages, as
outlined below:
1. From more than 2,000,000 years ago to about 600,000 years ago, a
shallow canyon was gradually being cut into the Absaroka volcanic
sequence by the ancestral Yellowstone River as it eroded headward from a
point near the present confluence of the Yellowstone and Lamar Rivers
(fig. 33). By the time of the climactic volcanic eruption in central
Yellowstone 600,000 years ago, the head of the “old” canyon probably
had been eroded southward nearly to the place where the north rim of the
Page 108
Yellowstone caldera was to form later (fig. 42A). This point now lies
about 5 miles below Lower Falls.
2. Ash-flow tuffs that were erupted 600,000 years ago filled the “old”
canyon, and the river recarved its channel, chiefly along its previous
course.
3. A large lake formed behind (south of) the north rim of the caldera, the
damming resulting in part from lava flows of Plateau Rhyolite that poured
out across the caldera floor in this area between 600,000 and 500,000
years ago. Eventually the lake rose and spilled northward into the head of
the “old” canyon, causing additional downcutting in what is now the
lower 15-mile stretch of the canyon.
4. As the lake emptied, the river began to erode upstream into the thick
rhyolite lava flows toward the present site of Lower Falls; the process was
very similar to that of a common stream gully eroding headward into a
hillside. At a stage somewhat more than 300,000 years ago, the head of
the canyon probably lay near the falls, and the river had cut a channel
400-600 feet deep along this upper 5-mile stretch (fig. 42B).
5. Approximately 300,000 years ago the canyon area was covered by 68
ice during pre-Bull Lake glaciation. During and after the retreat of
this ice, sediments accumulated in a lake that occupied the upper reaches
of the canyon between the present site of Upper Falls and Inspiration
Point. Subsequently, very little downcutting was accomplished until about
150,000-125,000 years ago, when the canyon was eroded nearly to its
present depth.
6. Canyon development was further interrupted by the advance and retreat
of glaciers during Bull Lake and Pinedale Glaciations. During and since
the melting of the Pinedale glaciers about 12,000 years ago, the canyon
has attained its present depth, and its walls have acquired much of their
picturesque erosional form. The Yellowstone River now maintains a fairly
uniform gradient (60-80 feet per mile) throughout the 20-mile-long gorge,
even though different segments of the canyon were cut at different times
and through different kinds of rocks (fig. 42C).
about 5 miles below Lower Falls.
2. Ash-flow tuffs that were erupted 600,000 years ago filled the “old”
canyon, and the river recarved its channel, chiefly along its previous
course.
3. A large lake formed behind (south of) the north rim of the caldera, the
damming resulting in part from lava flows of Plateau Rhyolite that poured
out across the caldera floor in this area between 600,000 and 500,000
years ago. Eventually the lake rose and spilled northward into the head of
the “old” canyon, causing additional downcutting in what is now the
lower 15-mile stretch of the canyon.
4. As the lake emptied, the river began to erode upstream into the thick
rhyolite lava flows toward the present site of Lower Falls; the process was
very similar to that of a common stream gully eroding headward into a
hillside. At a stage somewhat more than 300,000 years ago, the head of
the canyon probably lay near the falls, and the river had cut a channel
400-600 feet deep along this upper 5-mile stretch (fig. 42B).
5. Approximately 300,000 years ago the canyon area was covered by 68
ice during pre-Bull Lake glaciation. During and after the retreat of
this ice, sediments accumulated in a lake that occupied the upper reaches
of the canyon between the present site of Upper Falls and Inspiration
Point. Subsequently, very little downcutting was accomplished until about
150,000-125,000 years ago, when the canyon was eroded nearly to its
present depth.
6. Canyon development was further interrupted by the advance and retreat
of glaciers during Bull Lake and Pinedale Glaciations. During and since
the melting of the Pinedale glaciers about 12,000 years ago, the canyon
has attained its present depth, and its walls have acquired much of their
picturesque erosional form. The Yellowstone River now maintains a fairly
uniform gradient (60-80 feet per mile) throughout the 20-mile-long gorge,
even though different segments of the canyon were cut at different times
and through different kinds of rocks (fig. 42C).
Page 109
The spectacular erosional development in the upper 5-mile segment of the
Grand Canyon, which is the only part seen by most Park visitors, except for
the very lower end near Tower Falls (fig. 33), has taken place mostly within
the past 150,000-125,000 years. One reason for such a rapid rate of erosion
stems from the fact that this part of the canyon overlies one of the wide ring
fracture zones of the Yellowstone caldera (fig. 22). The fracture zone extends
to great depth, providing a ready avenue of travel for the upflow of hot water
and steam rising in the Yellowstone thermal system, as described in the
following chapter. Through many thousands of years, the upward percolation
of the hot fluids has caused severe chemical and physical changes (known as
hydrothermal alteration) in the rhyolite lava flows. One spectacular result of
the alteration has been the change from the normal brown and gray color of
the rhyolites to the bright yellow and other colorful hues now seen in the
canyon walls (as well as in many other places throughout the Park). Another
significant result of alteration has been the weakening of the rocks; that is,
the altered rocks are softer and less resistant to erosion than unaltered rocks.
Hence, the river has been able to erode these softer rocks, upstream to 69
Lower Falls, at a very rapid rate.
The position of Lower Falls, as might be expected, coincides with a change
from highly altered to less altered rhyolite; the difference in the erosion rates
of the two kinds of rocks here is self-evident (figs. 41 and 42C). The position
of Upper Falls is likewise closely controlled by differences in rock
hardnesses. The rhyolites on the upstream side are hard and dense, whereas
those on the downstream side contain a high proportion of volcanic glass
which causes them to be more easily eroded (fig. 42C).
Grand Canyon, which is the only part seen by most Park visitors, except for
the very lower end near Tower Falls (fig. 33), has taken place mostly within
the past 150,000-125,000 years. One reason for such a rapid rate of erosion
stems from the fact that this part of the canyon overlies one of the wide ring
fracture zones of the Yellowstone caldera (fig. 22). The fracture zone extends
to great depth, providing a ready avenue of travel for the upflow of hot water
and steam rising in the Yellowstone thermal system, as described in the
following chapter. Through many thousands of years, the upward percolation
of the hot fluids has caused severe chemical and physical changes (known as
hydrothermal alteration) in the rhyolite lava flows. One spectacular result of
the alteration has been the change from the normal brown and gray color of
the rhyolites to the bright yellow and other colorful hues now seen in the
canyon walls (as well as in many other places throughout the Park). Another
significant result of alteration has been the weakening of the rocks; that is,
the altered rocks are softer and less resistant to erosion than unaltered rocks.
Hence, the river has been able to erode these softer rocks, upstream to 69
Lower Falls, at a very rapid rate.
The position of Lower Falls, as might be expected, coincides with a change
from highly altered to less altered rhyolite; the difference in the erosion rates
of the two kinds of rocks here is self-evident (figs. 41 and 42C). The position
of Upper Falls is likewise closely controlled by differences in rock
hardnesses. The rhyolites on the upstream side are hard and dense, whereas
those on the downstream side contain a high proportion of volcanic glass
which causes them to be more easily eroded (fig. 42C).
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Page 111
70
COMMON KINDS OF THERMAL FEATURES in Yellowstone National Park. (Fig.
43)
A, Hot springs and terraces colored by algae at Mammoth Hot Springs.
COMMON KINDS OF THERMAL FEATURES in Yellowstone National Park. (Fig.
43)
A, Hot springs and terraces colored by algae at Mammoth Hot Springs.
Page 112
B, Castle Geyser erupting in Upper Geyser Basin.
Page 113
C, Fountain Paint Pots in Lower Geyser Basin.
Page 114
D, pool in Lower Geyser Basin.
71
71
Page 115
Hot-Water and Steam Phenomena
Although Yellowstone is geologically outstanding in many ways, the great
abundance, diversity, and spectacular nature of its thermal (hot-water and
steam) features were undoubtedly the primary reasons for its being set aside
as our first National Park (fig. 43). The unusual concentration of geysers, hot
springs, mudpots, and fumaroles provides that special drawing card which
has, for the past century, made the Park one of the world’s foremost natural
attractions.
To count all the individual thermal features in Yellowstone would be
virtually impossible. Various estimates range from 2,500 to 10,000,
depending on how many of the smaller features are included. They are
scattered through many regions of the Park, but most are clustered in a few
areas called geyser basins, where there are continuous displays of intense
thermal activity. (See frontispiece.) The “steam” that can be seen in thermal
areas is actually fog or water droplets condensed from steam; so the
appearance of individual geyser basins depends largely on air temperature
and humidity. On a warm, dry summer day, for example, the activity may
seem very weak (fig. 44), except where individual geysers are erupting. On
Although Yellowstone is geologically outstanding in many ways, the great
abundance, diversity, and spectacular nature of its thermal (hot-water and
steam) features were undoubtedly the primary reasons for its being set aside
as our first National Park (fig. 43). The unusual concentration of geysers, hot
springs, mudpots, and fumaroles provides that special drawing card which
has, for the past century, made the Park one of the world’s foremost natural
attractions.
To count all the individual thermal features in Yellowstone would be
virtually impossible. Various estimates range from 2,500 to 10,000,
depending on how many of the smaller features are included. They are
scattered through many regions of the Park, but most are clustered in a few
areas called geyser basins, where there are continuous displays of intense
thermal activity. (See frontispiece.) The “steam” that can be seen in thermal
areas is actually fog or water droplets condensed from steam; so the
appearance of individual geyser basins depends largely on air temperature
and humidity. On a warm, dry summer day, for example, the activity may
seem very weak (fig. 44), except where individual geysers are erupting. On
Page 116
cold or very humid days, however, “steam” plumes are seen rising from
every quarter.
How a thermal system operates
An essential ingredient for thermal activity is heat. A body of buried molten
rock, such as the one that produced volcanic eruptions in Yellowstone as late
as 60,000 to 75,000 years ago, takes a long time to cool. During cooling,
tremendous quantities of heat are transmitted by conduction into the solid
rocks surrounding the magma chamber (fig. 45). Eventually the whole
region becomes much hotter than non-volcanic areas (fig. 46). Normally,
rock temperatures increase about 1°F per 100 feet of depth in the earth’s
crust, but in the thermally active areas of Yellowstone the rate of temperature
increase is much greater. The amount of heat given off by the Upper Geyser
Basin, for example, is 800 times the amount given off by normal
(nonthermal) areas of the same size. This excess heat is enough to melt 1½
tons of ice per second! And, contrary to popular opinion, the underground
temperatures have not cooled measurably in the 100 years that records have
been kept on the thermal activity in the Park. In fact, geologic studies
indicate that very high heat flows have continued for at least the past 40,000
years.
72
every quarter.
How a thermal system operates
An essential ingredient for thermal activity is heat. A body of buried molten
rock, such as the one that produced volcanic eruptions in Yellowstone as late
as 60,000 to 75,000 years ago, takes a long time to cool. During cooling,
tremendous quantities of heat are transmitted by conduction into the solid
rocks surrounding the magma chamber (fig. 45). Eventually the whole
region becomes much hotter than non-volcanic areas (fig. 46). Normally,
rock temperatures increase about 1°F per 100 feet of depth in the earth’s
crust, but in the thermally active areas of Yellowstone the rate of temperature
increase is much greater. The amount of heat given off by the Upper Geyser
Basin, for example, is 800 times the amount given off by normal
(nonthermal) areas of the same size. This excess heat is enough to melt 1½
tons of ice per second! And, contrary to popular opinion, the underground
temperatures have not cooled measurably in the 100 years that records have
been kept on the thermal activity in the Park. In fact, geologic studies
indicate that very high heat flows have continued for at least the past 40,000
years.
72
Page 117
NORRIS GEYSER BASIN, as viewed northward from the Norris Museum. This
is one of the most active thermal areas in Yellowstone, but the photograph
was taken on a warm dry summer day when little hot-water and steam activity
was visible from a distance. Clouds of water droplets (the visible “steam” in
thermal areas) normally form only when the air is cool and (or) moist. The
floor of the basin is covered by a nearly solid layer of hot-spring deposits.
(Fig. 44)
is one of the most active thermal areas in Yellowstone, but the photograph
was taken on a warm dry summer day when little hot-water and steam activity
was visible from a distance. Clouds of water droplets (the visible “steam” in
thermal areas) normally form only when the air is cool and (or) moist. The
floor of the basin is covered by a nearly solid layer of hot-spring deposits.
(Fig. 44)
Page 118
HEAT FLOW AND SURFACE WATER. Diagram showing a thermal system,
according to the explanation that water of surface origin circulates and is
heated at great depths. (Based on information supplied by D. E. White, L. J. P.
Muffler, R. O. Fournier, and A. H. Truesdell.) (Fig. 45)
Water enters at ground surface and sinks in conduit formed by fault or fracture
Surface (meteoric) water sinks to levels perhaps as much as 10,000 feet below
ground. Heated far above its normal boiling point, it begins to rise toward
the surface
Descending cool surface water
Permeable zone allows water to flow through it
Cooling magma chamber
Water begins to boil near ground surface because of greatly reduced pressures
Rising hot water
Hot spring or geyser
73
according to the explanation that water of surface origin circulates and is
heated at great depths. (Based on information supplied by D. E. White, L. J. P.
Muffler, R. O. Fournier, and A. H. Truesdell.) (Fig. 45)
Water enters at ground surface and sinks in conduit formed by fault or fracture
Surface (meteoric) water sinks to levels perhaps as much as 10,000 feet below
ground. Heated far above its normal boiling point, it begins to rise toward
the surface
Descending cool surface water
Permeable zone allows water to flow through it
Cooling magma chamber
Water begins to boil near ground surface because of greatly reduced pressures
Rising hot water
Hot spring or geyser
73
Page 119
INFRARED IMAGE of a part of Upper Geyser Basin. Infrared instruments,
sensitive to heat, are able to detect “hot” spots in the landscape. Note
especially the sharp “image” of Old Faithful. (Image courtesy of National
Aeronautics and Space Administration.) (Fig. 46)
A second, equally essential ingredient for thermal activity is water. Many
thousands of gallons are discharged by the hot springs and geysers in
Yellowstone every minute—where does all this water come from? Studies
show that nearly all the water originates above ground as rain or snow
(meteoric water; fig. 45), and that very little comes from the underlying
magma (magmatic water).
The mechanism for heating the water, on the other hand, is a matter of some
uncertainty. Until a few years ago the heating was assumed to occur 74
near the ground surface and to be caused by hot magmatic gases
(mostly steam) rising from the underlying magma chamber. Deep wells
drilled recently in many thermal areas throughout the world (including
research drill holes in Yellowstone), however, suggest a better explanation.
According to this explanation, the surface water enters underground
passages (fractures and faults) and circulates to great depths—as much as
5,000-10,000 feet in some areas (fig. 45)—there to become heated far above
its surface boiling point. Research drill holes in Yellowstone, for example,
have demonstrated that water of surface origin exists at all depths at least to
sensitive to heat, are able to detect “hot” spots in the landscape. Note
especially the sharp “image” of Old Faithful. (Image courtesy of National
Aeronautics and Space Administration.) (Fig. 46)
A second, equally essential ingredient for thermal activity is water. Many
thousands of gallons are discharged by the hot springs and geysers in
Yellowstone every minute—where does all this water come from? Studies
show that nearly all the water originates above ground as rain or snow
(meteoric water; fig. 45), and that very little comes from the underlying
magma (magmatic water).
The mechanism for heating the water, on the other hand, is a matter of some
uncertainty. Until a few years ago the heating was assumed to occur 74
near the ground surface and to be caused by hot magmatic gases
(mostly steam) rising from the underlying magma chamber. Deep wells
drilled recently in many thermal areas throughout the world (including
research drill holes in Yellowstone), however, suggest a better explanation.
According to this explanation, the surface water enters underground
passages (fractures and faults) and circulates to great depths—as much as
5,000-10,000 feet in some areas (fig. 45)—there to become heated far above
its surface boiling point. Research drill holes in Yellowstone, for example,
have demonstrated that water of surface origin exists at all depths at least to
Page 120
the maximum drilled (1,088 feet), and that the water reaches temperatures up
to at least 465°F. The increase in temperature with depth causes a
corresponding decrease in the weight (density) of the water. Because of this,
the hot, “lighter,” water begins to rise again toward the ground surface,
pushed upward by the colder, “heavier,” near-surface water which sinks to
keep the water channels filled. Thus is set into motion a giant convection
current which operates continuously to supply very hot water to the thermal
areas (fig. 45). Just how deep the waters circulate in Yellowstone no one
really knows; as a guess, the depth probably is at least 1 or 2 miles.
The effect of pressure on the boiling temperature of water also plays a vital
role in thermal activity. In a body of water, the pressure at the surface is that
exerted by the weight of air above it (atmospheric pressure). Water under
these conditions boils at 212°F at sea level and at about 199°F at the
elevation of most of the geyser basins in Yellowstone. However, water at
depth not only is subjected to atmospheric pressure but also bears the added
weight of the overlying water. Under such additional pressures, water boils
only when the temperature is raised above its surface boiling point. In a well
100 feet deep at sea level, for example, the water at the bottom would have
to be heated to 288°F before it will boil. Thus it follows that in the
underground “workings” of hot springs or geysers, (1) The deepest water is
subjected to the greatest pressures, and (2) these deeper waters (in
Yellowstone) must be heated well above 199°F before they can actually
begin to boil. By this same reasoning but in reverse, if the pressure is
released, which happens as the water rises toward the ground surface, 75
the “hotter-than-boiling” water will then begin to boil. The boiling will
be rather quiet if the pressure is released gradually, as in most hot springs.
But if the pressure is released suddenly, boiling may become so violent that
much of the water flashes explosively into steam, expanding to several
hundred times its normal volume. This expansion provides the necessary
energy for geyser eruptions.
Hot-spring deposits and algae
to at least 465°F. The increase in temperature with depth causes a
corresponding decrease in the weight (density) of the water. Because of this,
the hot, “lighter,” water begins to rise again toward the ground surface,
pushed upward by the colder, “heavier,” near-surface water which sinks to
keep the water channels filled. Thus is set into motion a giant convection
current which operates continuously to supply very hot water to the thermal
areas (fig. 45). Just how deep the waters circulate in Yellowstone no one
really knows; as a guess, the depth probably is at least 1 or 2 miles.
The effect of pressure on the boiling temperature of water also plays a vital
role in thermal activity. In a body of water, the pressure at the surface is that
exerted by the weight of air above it (atmospheric pressure). Water under
these conditions boils at 212°F at sea level and at about 199°F at the
elevation of most of the geyser basins in Yellowstone. However, water at
depth not only is subjected to atmospheric pressure but also bears the added
weight of the overlying water. Under such additional pressures, water boils
only when the temperature is raised above its surface boiling point. In a well
100 feet deep at sea level, for example, the water at the bottom would have
to be heated to 288°F before it will boil. Thus it follows that in the
underground “workings” of hot springs or geysers, (1) The deepest water is
subjected to the greatest pressures, and (2) these deeper waters (in
Yellowstone) must be heated well above 199°F before they can actually
begin to boil. By this same reasoning but in reverse, if the pressure is
released, which happens as the water rises toward the ground surface, 75
the “hotter-than-boiling” water will then begin to boil. The boiling will
be rather quiet if the pressure is released gradually, as in most hot springs.
But if the pressure is released suddenly, boiling may become so violent that
much of the water flashes explosively into steam, expanding to several
hundred times its normal volume. This expansion provides the necessary
energy for geyser eruptions.
Hot-spring deposits and algae
Page 121
MOUND OF SINTER at Castle Geyser, Upper Geyser Basin. Lower part of
mound has well-defined layers probably deposited by normal hot springs. The
upper, irregular part resulted from the vigorous eruptions characteristic of
geysers and marks a change in the local hot-spring activity. (Fig. 47)
Nearly all geysers and many hot springs build mounds or terraces of mineral
deposits; some are so unusual in form that descriptive names have been
given to them, such as Castle Geyser (fig. 47). These deposits are generally
made up of many very thin layers of rock. Each layer represents a crust or
film of rock-forming mineral which was originally dissolved in hot water as
it flowed through the underground rocks, and which was then precipitated as
the water spread out over the surrounding ground surface.
76
mound has well-defined layers probably deposited by normal hot springs. The
upper, irregular part resulted from the vigorous eruptions characteristic of
geysers and marks a change in the local hot-spring activity. (Fig. 47)
Nearly all geysers and many hot springs build mounds or terraces of mineral
deposits; some are so unusual in form that descriptive names have been
given to them, such as Castle Geyser (fig. 47). These deposits are generally
made up of many very thin layers of rock. Each layer represents a crust or
film of rock-forming mineral which was originally dissolved in hot water as
it flowed through the underground rocks, and which was then precipitated as
the water spread out over the surrounding ground surface.
76
Page 122
TERRACES OF TRAVERTINE at Opal Springs, Mammoth Hot Springs area.
(Fig. 48)
(Fig. 48)
Page 123
Closeup view shows layered and porous nature of the travertine.
In all major thermal areas of the Park, with the exception of Mammoth 77
Hot Springs, most of the material being deposited is sinter (the kind
found around geysers is popularly called geyserite). Its chief constituent is
silica (the same as in quartz and in ordinary window glass). At Mammoth,
the deposit is travertine (fig. 48), which consists almost entirely of calcium
carbonate. The material deposited at any given place commonly reflects the
predominant kind of rock through which the hot water has passed during its
underground travels. At Mammoth Hot Springs the water passes through
thick beds of limestone (which is calcium carbonate), but in other areas the
main rock type through which the water percolates is rhyolite, a rock rich in
silica.
Through centuries of intense activity, layers of sinter have built up on the
floors of the geyser basins (fig. 44); these deposits are generally less than 10
feet thick. In one drill hole at Mammoth, deposits of travertine extend to a
depth of 250 feet. Dead trees and other kinds of vegetation whose life
processes have been choked off by the heat, water, and precipitated minerals
of hot-spring activity are a common sight in many places (fig. 51).
In all major thermal areas of the Park, with the exception of Mammoth 77
Hot Springs, most of the material being deposited is sinter (the kind
found around geysers is popularly called geyserite). Its chief constituent is
silica (the same as in quartz and in ordinary window glass). At Mammoth,
the deposit is travertine (fig. 48), which consists almost entirely of calcium
carbonate. The material deposited at any given place commonly reflects the
predominant kind of rock through which the hot water has passed during its
underground travels. At Mammoth Hot Springs the water passes through
thick beds of limestone (which is calcium carbonate), but in other areas the
main rock type through which the water percolates is rhyolite, a rock rich in
silica.
Through centuries of intense activity, layers of sinter have built up on the
floors of the geyser basins (fig. 44); these deposits are generally less than 10
feet thick. In one drill hole at Mammoth, deposits of travertine extend to a
depth of 250 feet. Dead trees and other kinds of vegetation whose life
processes have been choked off by the heat, water, and precipitated minerals
of hot-spring activity are a common sight in many places (fig. 51).
Page 124
Both travertine and sinter are white to gray. Around active hot springs,
however, the terraces that are constantly under water may be brightly
colored (figs. 43 and 49) because they are coated by microscopic plants
called algae. These organisms, which thrive in hot water at temperatures up
to about 170°F, are green, yellow, and brown. Oxides of iron and manganese
also contribute to the coloring in some parts of the thermal areas. The
delicate blue color of many pools, however, results from the reflection of
light off the pool walls and back through the deep clear water (fig. 43). Other
pools are yellow because they contain sulfur, or are green from the combined
influence of yellow sulfur and “blue” water.
78
however, the terraces that are constantly under water may be brightly
colored (figs. 43 and 49) because they are coated by microscopic plants
called algae. These organisms, which thrive in hot water at temperatures up
to about 170°F, are green, yellow, and brown. Oxides of iron and manganese
also contribute to the coloring in some parts of the thermal areas. The
delicate blue color of many pools, however, results from the reflection of
light off the pool walls and back through the deep clear water (fig. 43). Other
pools are yellow because they contain sulfur, or are green from the combined
influence of yellow sulfur and “blue” water.
78
Page 125
ALGAL-COLORED TERRACES lining the west bank of the Firehole River at
Midway Geyser Basin. Algae are microscopic plants that grow profusely on
rocks covered by hot water at temperatures up to about 170°F. (Fig. 49)
79
Hot springs and geysers
Midway Geyser Basin. Algae are microscopic plants that grow profusely on
rocks covered by hot water at temperatures up to about 170°F. (Fig. 49)
79
Hot springs and geysers
Page 126
Hot springs occur where the rising hot waters of a thermal system issue from
the ground-level openings of the feeder conduits (fig. 45). By far the greatest
numbers discharge water and steam in a relatively steady noneruptive
manner, although they vary considerably in individual behavior. Depending
upon pressure, water temperature, rate of upflow, heat supply, and
arrangement and size of underground passages, some hot springs boil
violently and emit dense clouds of vapor whereas in others the water quietly
wells up with little agitation from escaping steam. In some hot springs,
however, the underground channels are too narrow or the upflow of very hot
water and steam is too great to permit a steady discharge; periodic eruptions
then result. These special kinds of springs are called “geysers” (from the
Icelandic word geysir, meaning to “gush” or “rage”). At least 200 geysers, of
which about 60 play to a height of 10 feet or more, occur in Yellowstone
National Park; this is more than in any other region of the world.
How does a geyser work? We cannot, of course, observe the inner plumbing
of a geyser, except for that part which is seen by looking into its uppermost
“well.” Deeper levels directly below the “well” can be probed by scientific
instruments to some extent, and research drilling in some parts of the geyser
basins also provides much useful information. The available information
suggests that the plumbing system of a geyser (1) lies close to the ground
surface, generally no deeper than a few hundred feet; (2) consists of a tube,
commonly nearly vertical, that connects to chambers, side channels, or
layers of porous rock, where substantial amounts of water can be stored; and
(3) connects downward through the central tube and side channels to narrow
conduits that rise from the deepwater source of the main thermal system.
Considering a geyser system as described above and applying what is known
about the behavior of water and steam, we can understand what causes a
natural thermal eruption. Figure 50 shows diagrammatically the succession
of events believed to occur during the typical eruptive cycle of a geyser such
as Old Faithful.
80
the ground-level openings of the feeder conduits (fig. 45). By far the greatest
numbers discharge water and steam in a relatively steady noneruptive
manner, although they vary considerably in individual behavior. Depending
upon pressure, water temperature, rate of upflow, heat supply, and
arrangement and size of underground passages, some hot springs boil
violently and emit dense clouds of vapor whereas in others the water quietly
wells up with little agitation from escaping steam. In some hot springs,
however, the underground channels are too narrow or the upflow of very hot
water and steam is too great to permit a steady discharge; periodic eruptions
then result. These special kinds of springs are called “geysers” (from the
Icelandic word geysir, meaning to “gush” or “rage”). At least 200 geysers, of
which about 60 play to a height of 10 feet or more, occur in Yellowstone
National Park; this is more than in any other region of the world.
How does a geyser work? We cannot, of course, observe the inner plumbing
of a geyser, except for that part which is seen by looking into its uppermost
“well.” Deeper levels directly below the “well” can be probed by scientific
instruments to some extent, and research drilling in some parts of the geyser
basins also provides much useful information. The available information
suggests that the plumbing system of a geyser (1) lies close to the ground
surface, generally no deeper than a few hundred feet; (2) consists of a tube,
commonly nearly vertical, that connects to chambers, side channels, or
layers of porous rock, where substantial amounts of water can be stored; and
(3) connects downward through the central tube and side channels to narrow
conduits that rise from the deepwater source of the main thermal system.
Considering a geyser system as described above and applying what is known
about the behavior of water and steam, we can understand what causes a
natural thermal eruption. Figure 50 shows diagrammatically the succession
of events believed to occur during the typical eruptive cycle of a geyser such
as Old Faithful.
80
Page 127
A GEYSER IN ACTION. Photographs of successive stages in the eruption of
Old Faithful illustrate what probably happens during a natural geyser
eruption. The underground plumbing is diagrammatic and does not reflect
any specific knowledge of Old Faithful’s system. Direction of flow of water is
Old Faithful illustrate what probably happens during a natural geyser
eruption. The underground plumbing is diagrammatic and does not reflect
any specific knowledge of Old Faithful’s system. Direction of flow of water is
Page 128
shown by arrows. (Based on information supplied by D. E. White, L. J. P.
Muffler, R. O. Fournier, and A. H. Truesdell.) (Fig. 50)
Stage 1 (Recovery or recharge stage). After an eruption, the partly emptied
geyser tubes and chambers fill again with water. Hot water enters through a
feeder conduit from below, and cooler water percolates in from side channels
nearer the surface. Steam bubbles (with some other gases such as carbon
dioxide and hydrogen sulfide) start to form in upflowing currents, as a
decrease in pressure causes a corresponding decrease in boiling
temperature. At first the bubbles condense in the cooler, near-surface water
that is not yet at boiling temperature, but eventually all water is heated
enough that the bubbles will no longer condense or “dissolve.”
Muffler, R. O. Fournier, and A. H. Truesdell.) (Fig. 50)
Stage 1 (Recovery or recharge stage). After an eruption, the partly emptied
geyser tubes and chambers fill again with water. Hot water enters through a
feeder conduit from below, and cooler water percolates in from side channels
nearer the surface. Steam bubbles (with some other gases such as carbon
dioxide and hydrogen sulfide) start to form in upflowing currents, as a
decrease in pressure causes a corresponding decrease in boiling
temperature. At first the bubbles condense in the cooler, near-surface water
that is not yet at boiling temperature, but eventually all water is heated
enough that the bubbles will no longer condense or “dissolve.”
Page 129
Stage 2 (Preliminary eruption stage). As the rising gas bubbles grow in size
and number, they tend to clog certain parts of the geyser tube, perhaps at
some narrow or constricted point such as at A. When this happens, the
expanding steam abruptly forces its way upward through the system and
and number, they tend to clog certain parts of the geyser tube, perhaps at
some narrow or constricted point such as at A. When this happens, the
expanding steam abruptly forces its way upward through the system and
Page 130
causes some of the water to discharge from the surface vent in preliminary
spurts. The deeper part of the system, however, is not yet quite hot enough
for “triggering.”
81
spurts. The deeper part of the system, however, is not yet quite hot enough
for “triggering.”
81
Page 131
Stage 3 (Full eruption stage). Finally, a preliminary spurt “unloads” enough
water (with resulting reduction in pressure) to start a chain reaction deeper in
the system. Larger amounts of water in the side chambers and pore spaces
begin to flash into steam, and the geyser rapidly surges into full eruption.
water (with resulting reduction in pressure) to start a chain reaction deeper in
the system. Larger amounts of water in the side chambers and pore spaces
begin to flash into steam, and the geyser rapidly surges into full eruption.
Page 132
Stage 4 (Steam stage). When most of the extra energy is spent, and the
geyser tubes and chambers are nearly empty, the eruption ceases. Some
water remains in local pockets and pore spaces, continuing to make steam for
geyser tubes and chambers are nearly empty, the eruption ceases. Some
water remains in local pockets and pore spaces, continuing to make steam for
Page 133
a short while. Thereafter the system begins to fill again, and the eruptive cycle
starts anew.
No two geysers have the same size, shape, and arrangement of tubes 82
and chambers. Also, some geysers, such as Great Fountain, have large
surface pools not present in cone-type geysers such as Old Faithful. Hence,
each geyser behaves differently from all others in frequency of eruption,
length of individual eruptions, and amount of water discharged. Geysers may
also vary in their own behavior as their plumbing features change through
the years. The great amount of energy that builds up in some of them from
time to time creates enough explosive force to shatter parts of the plumbing
system, thereby causing a change in their eruptive behavior. In fact, some
geyser eruptions have been so violent that large chunks of rock have been
exploded out of the ground and scattered around the surrounding area (fig.
51). With time, the precipitation of minerals may partly seal a tube or
chamber, gradually altering the eruptive mechanism.
Despite all the variable factors involved in geyser eruptions, and all the
changes that can take place from time to time to alter the pattern of those
eruptions, several of the Yellowstone geysers function regularly, day after
day, week after week, and year after year. Within this group of regulars is the
most famous feature of all—Old Faithful—which has not missed an eruption
in all the many decades that it has been under close observation (fig. 52). We
can only conclude that nature has provided this incredible geyser with a
stable plumbing system that is just right to trigger delightfully graceful
eruptions at close-enough time intervals to suit the convenience of all Park
visitors.
Mudpots
Mudpots are among the most fascinating and interesting of the Yellowstone
thermal features. They are also a type of hot spring, but one for which water
is in short supply. Whatever water is available becomes thoroughly mixed
with clay and other fine undissolved mineral matter. The mud is generally
gray, black, white, or cream colored, but some is tinted pale pink and red by
starts anew.
No two geysers have the same size, shape, and arrangement of tubes 82
and chambers. Also, some geysers, such as Great Fountain, have large
surface pools not present in cone-type geysers such as Old Faithful. Hence,
each geyser behaves differently from all others in frequency of eruption,
length of individual eruptions, and amount of water discharged. Geysers may
also vary in their own behavior as their plumbing features change through
the years. The great amount of energy that builds up in some of them from
time to time creates enough explosive force to shatter parts of the plumbing
system, thereby causing a change in their eruptive behavior. In fact, some
geyser eruptions have been so violent that large chunks of rock have been
exploded out of the ground and scattered around the surrounding area (fig.
51). With time, the precipitation of minerals may partly seal a tube or
chamber, gradually altering the eruptive mechanism.
Despite all the variable factors involved in geyser eruptions, and all the
changes that can take place from time to time to alter the pattern of those
eruptions, several of the Yellowstone geysers function regularly, day after
day, week after week, and year after year. Within this group of regulars is the
most famous feature of all—Old Faithful—which has not missed an eruption
in all the many decades that it has been under close observation (fig. 52). We
can only conclude that nature has provided this incredible geyser with a
stable plumbing system that is just right to trigger delightfully graceful
eruptions at close-enough time intervals to suit the convenience of all Park
visitors.
Mudpots
Mudpots are among the most fascinating and interesting of the Yellowstone
thermal features. They are also a type of hot spring, but one for which water
is in short supply. Whatever water is available becomes thoroughly mixed
with clay and other fine undissolved mineral matter. The mud is generally
gray, black, white, or cream colored, but some is tinted pale pink and red by
Page 134
iron compounds (fig. 43); hence, the picturesque term “paint pots” is
commonly used.
Mudpots form in places where the upflowing thermal fluids have chemically
decomposed the surface rocks to form clay. Such small amounts of 83
water are involved, however, that the surface discharge is not great
enough to flush the clay out of the spring. Caldrons of mud of all
consistencies result, from the very thin soupy material in many mudpots to
the almost hard-baked material in the less active features. Some mudpots
expel pellets of very thick viscous mud which build up circular cones or
mounds; this type is commonly called a “mud volcano” (fig. 53).
commonly used.
Mudpots form in places where the upflowing thermal fluids have chemically
decomposed the surface rocks to form clay. Such small amounts of 83
water are involved, however, that the surface discharge is not great
enough to flush the clay out of the spring. Caldrons of mud of all
consistencies result, from the very thin soupy material in many mudpots to
the almost hard-baked material in the less active features. Some mudpots
expel pellets of very thick viscous mud which build up circular cones or
mounds; this type is commonly called a “mud volcano” (fig. 53).
Page 135
SEISMIC GEYSER, showing rock rubble blown out during an explosive
thermal eruption. Note the trees that have been killed by the heat and eruptive
activity. According to George D. Marler of the National Park Service, this
geyser developed from cracks caused by the Hebgen Lake Earthquake of
August 17, 1959. (Fig. 51)
84
thermal eruption. Note the trees that have been killed by the heat and eruptive
activity. According to George D. Marler of the National Park Service, this
geyser developed from cracks caused by the Hebgen Lake Earthquake of
August 17, 1959. (Fig. 51)
84
Page 136
Page 137
OLD FAITHFUL IN FULL ERUPTION. The interval between eruptions averages
about 65 minutes, but it varies from 33 to 96 minutes. The time lapse between
eruptions can be predicted rather closely, mainly on the basis of the length of
time involved in the previous eruption. If an eruption lasted 4 minutes, for
example, this means that a certain amount of water emptied from the geyser’s
chambers and that a certain length of time will be necessary to recharge the
system for the next eruption. But if the previous eruption lasted only 3
minutes, less time will be needed for recharge, and the next eruption will
occur sooner. (The above discussion is based primarily on many years of
observation and study of Old Faithful by George D. Marler and other
observers of the National Park Service; photograph courtesy of Sgt. James E.
Jensen, U.S. Air Force.) (Fig. 52)
Mudpot activity differs from season to season throughout the year 85
because of the varying amounts of rain and snow that fall upon the
surface to further moisten the mud. Accordingly, mudpots are commonly
drier in late summer and early fall than they are from winter through early
summer.
Fumaroles
Fumaroles (from the Latin word fumus, meaning “smoke”) are those features
that discharge only steam and other gases such as carbon dioxide and
hydrogen sulfide; hence, they are commonly called “steam vents.” Usually
these features are perched on a hillside or other high ground above the level
of the flowing springs. In many fumaroles, however, water can be heard
boiling violently at some lower, unseen level.
Thermal explosions
A few features present in the Yellowstone thermal areas display evidence
that extremely violent thermal explosions occurred in the past, particularly
during Pinedale Glaciation, about 15,000 years ago. Such explosion features,
of which Pocket Basin in Lower Geyser Basin is a good example, appear as
craterlike depressions a few tens of feet to as much as 5,000 feet across
surrounded by rims of rock fragments that were blown out of the craters. The
underground mechanism causing the explosions was similar to that of
about 65 minutes, but it varies from 33 to 96 minutes. The time lapse between
eruptions can be predicted rather closely, mainly on the basis of the length of
time involved in the previous eruption. If an eruption lasted 4 minutes, for
example, this means that a certain amount of water emptied from the geyser’s
chambers and that a certain length of time will be necessary to recharge the
system for the next eruption. But if the previous eruption lasted only 3
minutes, less time will be needed for recharge, and the next eruption will
occur sooner. (The above discussion is based primarily on many years of
observation and study of Old Faithful by George D. Marler and other
observers of the National Park Service; photograph courtesy of Sgt. James E.
Jensen, U.S. Air Force.) (Fig. 52)
Mudpot activity differs from season to season throughout the year 85
because of the varying amounts of rain and snow that fall upon the
surface to further moisten the mud. Accordingly, mudpots are commonly
drier in late summer and early fall than they are from winter through early
summer.
Fumaroles
Fumaroles (from the Latin word fumus, meaning “smoke”) are those features
that discharge only steam and other gases such as carbon dioxide and
hydrogen sulfide; hence, they are commonly called “steam vents.” Usually
these features are perched on a hillside or other high ground above the level
of the flowing springs. In many fumaroles, however, water can be heard
boiling violently at some lower, unseen level.
Thermal explosions
A few features present in the Yellowstone thermal areas display evidence
that extremely violent thermal explosions occurred in the past, particularly
during Pinedale Glaciation, about 15,000 years ago. Such explosion features,
of which Pocket Basin in Lower Geyser Basin is a good example, appear as
craterlike depressions a few tens of feet to as much as 5,000 feet across
surrounded by rims of rock fragments that were blown out of the craters. The
underground mechanism causing the explosions was similar to that of
Page 138
geysers, but in these special cases the energy remained bottled-up until a
very critical explosive stage was reached.
The best explanation for Pocket Basin and related features is that the ground
above the sites of the explosions was weighted down by the water of small
lakes which had formed in melted-out pockets of glacial ice. Such localized
melting of the glaciers would occur where the ice was in direct contact 86
with underlying thermal features. A rapid draining of the lake waters
would then produce a sudden release of pressure over the hot area, resulting
in an unusually violent thermal eruption.
MUD VOLCANO near Pocket Basin in the Lower Geyser Basin. The mud is
formed by chemical decomposition of the rocks chiefly by the action of
carbon dioxide and sulfuric acid. The splatter, 5-6 feet high, is caused by the
escaping gases. (Fig. 53)
very critical explosive stage was reached.
The best explanation for Pocket Basin and related features is that the ground
above the sites of the explosions was weighted down by the water of small
lakes which had formed in melted-out pockets of glacial ice. Such localized
melting of the glaciers would occur where the ice was in direct contact 86
with underlying thermal features. A rapid draining of the lake waters
would then produce a sudden release of pressure over the hot area, resulting
in an unusually violent thermal eruption.
MUD VOLCANO near Pocket Basin in the Lower Geyser Basin. The mud is
formed by chemical decomposition of the rocks chiefly by the action of
carbon dioxide and sulfuric acid. The splatter, 5-6 feet high, is caused by the
escaping gases. (Fig. 53)
Page 139
Faulting and its control of thermal activity
Most of the major thermal areas of Yellowstone are related to the ring
fracture zones of the Yellowstone caldera (fig. 22). Many deep-seated faults
and fractures in these zones are presumably situated above the main source
of heat of the thermal system. Thus, they provide convenient avenues of
travel for underground waters to circulate to great depths, there to become
heated and then rise to the earth’s surface (fig. 45). A few areas like
Mammoth Hot Springs and Norris Geyser Basin, on the other hand, are not
within the ring fracture zones of the caldera. In these areas, the thermal
activity is commonly related to other prominent zones of faulting which also
afford readymade channelways for the circulation of hot water and steam.
87
Most of the major thermal areas of Yellowstone are related to the ring
fracture zones of the Yellowstone caldera (fig. 22). Many deep-seated faults
and fractures in these zones are presumably situated above the main source
of heat of the thermal system. Thus, they provide convenient avenues of
travel for underground waters to circulate to great depths, there to become
heated and then rise to the earth’s surface (fig. 45). A few areas like
Mammoth Hot Springs and Norris Geyser Basin, on the other hand, are not
within the ring fracture zones of the caldera. In these areas, the thermal
activity is commonly related to other prominent zones of faulting which also
afford readymade channelways for the circulation of hot water and steam.
87
Page 140
Earthquakes
Earthquakes occur frequently in areas of active faulting and volcanism; they
are caused by sudden movements between adjacent blocks of the earth’s
crust as the crust adjusts to new conditions and pressures. Because of its
volcanic history and the fact that very recent fault movements have occurred
there, it is not surprising that Yellowstone is an especially active earthquake
area. Sensitive instruments (seismographs) record an average of about five
earth tremors daily in and around the Park, and on rare occasions they may
record 100 tremors or more in a single day. Nearly all these tremors are so
slight that they cannot be felt by man, but at times, perhaps only once in a
human lifetime, one is triggered with high enough intensity to sharply draw
our attention to the very real earthquake potential that exists constantly in
this geologically active area. Such a high-intensity quake occurred in the
Yellowstone region near midnight on August 17, 1959.
The Hebgen Lake Earthquake, as it is known, was centered in the Madison
Valley along the west boundary of Yellowstone National Park about 12 miles
Earthquakes occur frequently in areas of active faulting and volcanism; they
are caused by sudden movements between adjacent blocks of the earth’s
crust as the crust adjusts to new conditions and pressures. Because of its
volcanic history and the fact that very recent fault movements have occurred
there, it is not surprising that Yellowstone is an especially active earthquake
area. Sensitive instruments (seismographs) record an average of about five
earth tremors daily in and around the Park, and on rare occasions they may
record 100 tremors or more in a single day. Nearly all these tremors are so
slight that they cannot be felt by man, but at times, perhaps only once in a
human lifetime, one is triggered with high enough intensity to sharply draw
our attention to the very real earthquake potential that exists constantly in
this geologically active area. Such a high-intensity quake occurred in the
Yellowstone region near midnight on August 17, 1959.
The Hebgen Lake Earthquake, as it is known, was centered in the Madison
Valley along the west boundary of Yellowstone National Park about 12 miles
Page 141
north of the town of West Yellowstone, Montana (fig. 1). As a result of the
quake, a 200-square-mile area, occupied in part by the Hebgen Lake
reservoir, subsided a foot or more; maximum subsidence was 20 feet.
Movements of several feet along old faults in the highlands along the north
side of the valley produced fresh scars several miles long (fig. 54).
Moreover, the severe vibrations that rocked the surrounding countryside
caused the loose silt, sand, and gravel of the valley floor to slip and become
“faulted” in many places. By far the most drastic result was the shaking
loose of a huge landslide in the vicinity of the Rock Creek campground 88
about 25 miles downstream on the Madison River from the west
boundary of the Park.
EARTHQUAKE DAMAGE. Severe damage caused by reactivation of a fault
during the Hebgen Lake Earthquake of August 17, 1959. The building is on the
Blarneystone Ranch, about 10 miles north of West Yellowstone, Montana, and
1½ miles west of the west boundary of Yellowstone National Park. (Fig. 54)
quake, a 200-square-mile area, occupied in part by the Hebgen Lake
reservoir, subsided a foot or more; maximum subsidence was 20 feet.
Movements of several feet along old faults in the highlands along the north
side of the valley produced fresh scars several miles long (fig. 54).
Moreover, the severe vibrations that rocked the surrounding countryside
caused the loose silt, sand, and gravel of the valley floor to slip and become
“faulted” in many places. By far the most drastic result was the shaking
loose of a huge landslide in the vicinity of the Rock Creek campground 88
about 25 miles downstream on the Madison River from the west
boundary of the Park.
EARTHQUAKE DAMAGE. Severe damage caused by reactivation of a fault
during the Hebgen Lake Earthquake of August 17, 1959. The building is on the
Blarneystone Ranch, about 10 miles north of West Yellowstone, Montana, and
1½ miles west of the west boundary of Yellowstone National Park. (Fig. 54)
Page 142
Within Yellowstone National Park, the quake caused only slight damage to
buildings at Old Faithful, Mammoth Hot Springs, and a few other places.
Small landslides also occurred in various places, for example, at Tuff Cliff
near Madison Junction. The earthquake affected many thermal features,
particularly those in the main geyser basins near the west side of the Park. In
several places the intensity of the thermal activity increased markedly, in
fewer places the activity decreased. Some geysers, long dormant, erupted
immediately after the earthquake; others erupted with much greater 89
force and frequency than usual; still others became dormant and have
remained so. A general, widespread effect was a noticeable increase in the
muddiness of many pools and springs, as if the quake had produced a giant
surge of water coursing through the underground channels of the geyser
basins. Of immediate concern to everyone, of course, was the earthquake’s
effect on Old Faithful. Fortunately, the only measurable effect was a slight
lengthening of time between eruptions. After several months the time
interval stabilized at about 65 minutes.
Detailed scientific studies bearing on the Hebgen Lake Earthquake in the
weeks that followed showed that it was felt over more than 600,000 square
miles of the Western United States, and that it was the strongest shock ever
recorded in this part of the Rocky Mountains. In 12 years’ time many traces
of the quake have disappeared, but its frightful aspects will not soon be
forgotten. It serves as a vivid reminder, once again, of the great restlessness
that through the ages has been, and continues to be, the very special
trademark of the Yellowstone country.
buildings at Old Faithful, Mammoth Hot Springs, and a few other places.
Small landslides also occurred in various places, for example, at Tuff Cliff
near Madison Junction. The earthquake affected many thermal features,
particularly those in the main geyser basins near the west side of the Park. In
several places the intensity of the thermal activity increased markedly, in
fewer places the activity decreased. Some geysers, long dormant, erupted
immediately after the earthquake; others erupted with much greater 89
force and frequency than usual; still others became dormant and have
remained so. A general, widespread effect was a noticeable increase in the
muddiness of many pools and springs, as if the quake had produced a giant
surge of water coursing through the underground channels of the geyser
basins. Of immediate concern to everyone, of course, was the earthquake’s
effect on Old Faithful. Fortunately, the only measurable effect was a slight
lengthening of time between eruptions. After several months the time
interval stabilized at about 65 minutes.
Detailed scientific studies bearing on the Hebgen Lake Earthquake in the
weeks that followed showed that it was felt over more than 600,000 square
miles of the Western United States, and that it was the strongest shock ever
recorded in this part of the Rocky Mountains. In 12 years’ time many traces
of the quake have disappeared, but its frightful aspects will not soon be
forgotten. It serves as a vivid reminder, once again, of the great restlessness
that through the ages has been, and continues to be, the very special
trademark of the Yellowstone country.
Page 143
The Park and Man
A hundred years ago another powerful force entered the Yellowstone scene.
Man, arriving in ever increasing numbers, came armed with the power to
choose between preserving or destroying the wonders that nature has taken
more than 2.5 billion years to create. Sensing this grave responsibility, he
took the necessary steps to insure that these irreplaceable natural features
would be preserved and protected. Today, Yellowstone National Park indeed
exists “for the benefit and enjoyment of the people,” a fitting and lasting
symbol of a great national heritage that now includes more than 275 places
of natural and historical interest. On the eve of the 100th anniversary of our
first National Park, we are again reminded of that continuing responsibility
we all share in preserving these unique places for the benefit and enjoyment
of all future generations of visitors.
90
A hundred years ago another powerful force entered the Yellowstone scene.
Man, arriving in ever increasing numbers, came armed with the power to
choose between preserving or destroying the wonders that nature has taken
more than 2.5 billion years to create. Sensing this grave responsibility, he
took the necessary steps to insure that these irreplaceable natural features
would be preserved and protected. Today, Yellowstone National Park indeed
exists “for the benefit and enjoyment of the people,” a fitting and lasting
symbol of a great national heritage that now includes more than 275 places
of natural and historical interest. On the eve of the 100th anniversary of our
first National Park, we are again reminded of that continuing responsibility
we all share in preserving these unique places for the benefit and enjoyment
of all future generations of visitors.
90
Page 144
Acknowledgments
The subject matter of this bulletin is based chiefly on the results of a
systematic program of geological investigations in Yellowstone National
Park, conducted by the U.S. Geological Survey during the years 1965-71.
The program, ably organized and directed by A. B. Campbell, required the
special skills and knowledge of many individuals to make a comprehensive
study of all the varied and complex features of the Park area. Without their
invaluable cooperation, assistance, and interest, this endeavor to summarize
the geologic story of Yellowstone would not have been possible. I therefore
express my sincere thanks to the colleagues listed below, all of whom
furnished unpublished information bearing on different aspects of that story:
R. L. Christiansen and H. R. Blank, Jr. (Quaternary volcanism); H. W.
Smedes and H. J. Prostka (Absaroka volcanism); D. E. White, L. J. P.
Muffler, R. O. Fournier, and A. H. Truesdell (thermal activity); G. M.
Richmond, K. L. Pierce, and H. A. Waldrop (glaciation); E. T. Ruppel and J.
D. Love (sedimentary rocks and geologic structure); J. D. Obradovich and
Meyer Rubin (radiometric dating). W. L. Newman provided many helpful
suggestions regarding the preparation of the manuscript.
The geological studies in Yellowstone received the full support and
cooperation of former Park Superintendent J. S. McLaughlin, Superintendent
J. K. Anderson, and other personnel of the U.S. National Park Service. In
particular, the helpful advice, interest, and enthusiasm of the entire Park
Naturalist staff, especially J. M. Good and W. W. Dunmire, former and
present Chief Park Naturalists, respectively, greatly facilitated the work in all
phases of the program.
The subject matter of this bulletin is based chiefly on the results of a
systematic program of geological investigations in Yellowstone National
Park, conducted by the U.S. Geological Survey during the years 1965-71.
The program, ably organized and directed by A. B. Campbell, required the
special skills and knowledge of many individuals to make a comprehensive
study of all the varied and complex features of the Park area. Without their
invaluable cooperation, assistance, and interest, this endeavor to summarize
the geologic story of Yellowstone would not have been possible. I therefore
express my sincere thanks to the colleagues listed below, all of whom
furnished unpublished information bearing on different aspects of that story:
R. L. Christiansen and H. R. Blank, Jr. (Quaternary volcanism); H. W.
Smedes and H. J. Prostka (Absaroka volcanism); D. E. White, L. J. P.
Muffler, R. O. Fournier, and A. H. Truesdell (thermal activity); G. M.
Richmond, K. L. Pierce, and H. A. Waldrop (glaciation); E. T. Ruppel and J.
D. Love (sedimentary rocks and geologic structure); J. D. Obradovich and
Meyer Rubin (radiometric dating). W. L. Newman provided many helpful
suggestions regarding the preparation of the manuscript.
The geological studies in Yellowstone received the full support and
cooperation of former Park Superintendent J. S. McLaughlin, Superintendent
J. K. Anderson, and other personnel of the U.S. National Park Service. In
particular, the helpful advice, interest, and enthusiasm of the entire Park
Naturalist staff, especially J. M. Good and W. W. Dunmire, former and
present Chief Park Naturalists, respectively, greatly facilitated the work in all
phases of the program.
Page 145
Footnotes
[1]
The specific area about which the early-day Indians first used the term that
is now translated as “Yellowstone” is unknown. The name may have
referred to the yellowish rocks that line the banks of the Yellowstone
River near its confluence with the Missouri River in eastern Montana
and western North Dakota. However, in the opinion of H. M. Chittenden,
who studied the question in considerable detail, there is little doubt that
the name was taken from the striking yellow-hued walls of the gorge
now known as the Grand Canyon of the Yellowstone.
91
[1]
The specific area about which the early-day Indians first used the term that
is now translated as “Yellowstone” is unknown. The name may have
referred to the yellowish rocks that line the banks of the Yellowstone
River near its confluence with the Missouri River in eastern Montana
and western North Dakota. However, in the opinion of H. M. Chittenden,
who studied the question in considerable detail, there is little doubt that
the name was taken from the striking yellow-hued walls of the gorge
now known as the Grand Canyon of the Yellowstone.
91
Page 146
Selected Additional Reading
Allen, E. T., and Day, A. L., 1935, Hot springs of the Yellowstone National
Park: Carnegie Institution of Washington Publication 466, 525 pages.
Boyd, F. R., 1961, Welded tuffs and flows in the rhyolite plateau of
Yellowstone Park, Wyoming: Geological Society of America Bulletin,
volume 72, number 3, pages 387-426.
Christiansen, R. L., and Blank, H. R., Jr., 1972, Volcanic stratigraphy of the
Quaternary rhyolite plateau in Yellowstone National Park: U.S.
Geological Survey, Professional Paper 729-B (in press).
Dorf, Erling, 1960, Tertiary fossil forests of Yellowstone National Park,
Wyoming, in West Yellowstone—Earthquake area, Billings Geological
Society Guidebook 11th Annual Field Conference, 1960: pages 253-
260.
Hague, Arnold, Iddings, J. P., Weed, W. H., Walcott, C. D., Girty, G. H.,
Stanton, T. W., and Knowlton, F. H., 1899, Geology of the Yellowstone
National Park: U.S. Geological Survey Monograph 32, part 2, 893
pages and atlas of 27 sheets folio.
Hague, Arnold, Weed, W. H., and Iddings, J. P., 1896, Description of the
Yellowstone National Park quadrangle [Wyoming]: U.S. Geological
Survey Geologic Atlas, Folio 30.
Hayden, F. V., 1872, Preliminary report of the United States Geological
Survey of Montana and portions of adjacent Territories, being a fifth
annual report of progress—Part I: Washington, U.S. Government
Printing Office, pages 13-204.
Howard, A. D., 1937, History of the Grand Canyon of the Yellowstone:
Geological Society of America Special Paper 6, 159 pages.
Allen, E. T., and Day, A. L., 1935, Hot springs of the Yellowstone National
Park: Carnegie Institution of Washington Publication 466, 525 pages.
Boyd, F. R., 1961, Welded tuffs and flows in the rhyolite plateau of
Yellowstone Park, Wyoming: Geological Society of America Bulletin,
volume 72, number 3, pages 387-426.
Christiansen, R. L., and Blank, H. R., Jr., 1972, Volcanic stratigraphy of the
Quaternary rhyolite plateau in Yellowstone National Park: U.S.
Geological Survey, Professional Paper 729-B (in press).
Dorf, Erling, 1960, Tertiary fossil forests of Yellowstone National Park,
Wyoming, in West Yellowstone—Earthquake area, Billings Geological
Society Guidebook 11th Annual Field Conference, 1960: pages 253-
260.
Hague, Arnold, Iddings, J. P., Weed, W. H., Walcott, C. D., Girty, G. H.,
Stanton, T. W., and Knowlton, F. H., 1899, Geology of the Yellowstone
National Park: U.S. Geological Survey Monograph 32, part 2, 893
pages and atlas of 27 sheets folio.
Hague, Arnold, Weed, W. H., and Iddings, J. P., 1896, Description of the
Yellowstone National Park quadrangle [Wyoming]: U.S. Geological
Survey Geologic Atlas, Folio 30.
Hayden, F. V., 1872, Preliminary report of the United States Geological
Survey of Montana and portions of adjacent Territories, being a fifth
annual report of progress—Part I: Washington, U.S. Government
Printing Office, pages 13-204.
Howard, A. D., 1937, History of the Grand Canyon of the Yellowstone:
Geological Society of America Special Paper 6, 159 pages.
Page 147
Marler, G. D., 1969, The story of Old Faithful: Yellowstone Library and
Museum Association, 49 pages.
Richmond, G. M., Pierce, K. L., and Waldrop, H. A., 1972, Surficial
geologic map of Yellowstone National Park: U.S. Geological Survey
Miscellaneous Geologic Investigations Map I-710 (in press).
Ruppel, E. T., 1972, Geology of pre-Tertiary rocks in the northern part of
Yellowstone National Park, Wyoming: U.S. Geological Survey
Professional Paper 729-A (in press).
Smedes, H. W., and Prostka, H. J., 1972, Absaroka Volcanic 92
Supergroup in the Yellowstone National Park region: U.S.
Geological Survey Professional Paper 729-C (in press).
Smith, R. L., 1960, Ash flows: Geological Society of America Bulletin,
volume 71, number 6, pages 795-841.
U.S. Geological Survey, 1964, The Hebgen Lake, Montana, earthquake of
August 17, 1959: US Geological Survey Professional Paper 435, 242
pages.
U.S. Geological Survey, 1972, Geologic map of Yellowstone National Park:
U.S. Geological Survey Miscellaneous Geologic Investigations Map I-
711 (in press).
White, D. E., 1967, Some principles of geyser activity, mainly from
Steamboat Springs, Nevada: American Journal of Science, volume 265,
number 8, pages 641-684.
★ U. S. GOVERNMENT PRINTING OFFICE: 1972 O-467-725
Museum Association, 49 pages.
Richmond, G. M., Pierce, K. L., and Waldrop, H. A., 1972, Surficial
geologic map of Yellowstone National Park: U.S. Geological Survey
Miscellaneous Geologic Investigations Map I-710 (in press).
Ruppel, E. T., 1972, Geology of pre-Tertiary rocks in the northern part of
Yellowstone National Park, Wyoming: U.S. Geological Survey
Professional Paper 729-A (in press).
Smedes, H. W., and Prostka, H. J., 1972, Absaroka Volcanic 92
Supergroup in the Yellowstone National Park region: U.S.
Geological Survey Professional Paper 729-C (in press).
Smith, R. L., 1960, Ash flows: Geological Society of America Bulletin,
volume 71, number 6, pages 795-841.
U.S. Geological Survey, 1964, The Hebgen Lake, Montana, earthquake of
August 17, 1959: US Geological Survey Professional Paper 435, 242
pages.
U.S. Geological Survey, 1972, Geologic map of Yellowstone National Park:
U.S. Geological Survey Miscellaneous Geologic Investigations Map I-
711 (in press).
White, D. E., 1967, Some principles of geyser activity, mainly from
Steamboat Springs, Nevada: American Journal of Science, volume 265,
number 8, pages 641-684.
★ U. S. GOVERNMENT PRINTING OFFICE: 1972 O-467-725
Page 148
Page 149
Transcriber’s Notes
Retained publication information from the printed edition: this eBook is
public-domain in the country of publication.
Corrected a few palpable typos.
Included a transcription of the text within some images.
Renumbered footnotes, and modified references to them accordingly.
In the text versions only, text in italics is delimited by _underscores_.
Retained publication information from the printed edition: this eBook is
public-domain in the country of publication.
Corrected a few palpable typos.
Included a transcription of the text within some images.
Renumbered footnotes, and modified references to them accordingly.
In the text versions only, text in italics is delimited by _underscores_.
Page 150
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START: FULL LICENSE
STORY OF YELLOWSTONE NATIONAL PARK ***
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
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