Big History: The Big Bang, Life on Earth, and the Rise of Humanity - David Christian

Page 52

Lecture 9: Threshold 4—The Earth and the Solar System

What followed should be familiar by now. Gravity drew the cloud together. As it became denser, it heated up—particularly in the center. When the center reached 10 million degrees Celsius, hydrogen fusion began and our Sun lit up. It acquired the typical structure of stars, with fusion reactions in the center, a middle layer containing reserves of hydrogen, and a surface from which energy radiates into space. We can see areas of star formation in our galaxy even today. Similar processes occur even at smaller scales. For We cannot determine the example, Jupiter is mainly gaseous and is large enough for its center to age of the solar system by be extremely hot, but not quite hot dating Earth rocks because enough for fusion. It is almost a star, the Earth is so geologically but not quite. active that its original surface Now we shift away from the Sun to is now unrecognizable. the debris surrounding it. Through a process known as accretion, the planets and other bodies of our solar system were created from the 0.1% of the solar nebula that was not incorporated in the Sun. As it contracted, the solar nebula spun faster, like an ice skater doing a pirouette. Centrifugal force Àattened the spinning nebula into a disk, so that the material not gobbled up by the Sun orbited the Sun in a single plane. Saturn’s rings consist of orbiting debris, so they may give us a good idea of the shape and structure of the solar nebula. In each orbit, particles of matter were drawn together by electrostatic forces or crushed together in the course of violent collisions. Gradually, larger objects appeared and began colliding with each other and sometimes merging with each other. They grew like large snowballs. Stray bodies in the solar system, such as comets, are thought to be remnants of these early stages of accretion. Within a few million years, the large bodies in each orbit formed “planetesimals.” The largest planetesimals drew in most of the remaining material through their gravitational pull until a single large body appeared in each orbit.

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Glossary

31min
pages 250-272

Bibliography

23min
pages 273-288

Big History—Humans in the Cosmos

7min
pages 233-237

Permissions Acknowledgments

1min
pages 289-290

The Next Millennium and the Remote Future

6min
pages 229-232

The Next 100 Years

6min
pages 224-228

Human History and the Biosphere

6min
pages 219-223

The World That the Modern Revolution Made

6min
pages 214-218

The 20th Century

6min
pages 209-213

The Early Modern Cycle, 1350–1700

5min
pages 195-198

Threshold 8—The Modern Revolution

7min
pages 185-189

The Medieval Malthusian Cycle, 500–1350

6min
pages 190-194

Spread of the Industrial Revolution to 1900

6min
pages 204-208

Breakthrough—The Industrial Revolution

7min
pages 199-203

The Americas in the Later Agrarian Era

7min
pages 180-184

The World That Agrarian Civilizations Made

6min
pages 156-159

Long Trends—Rates of Innovation

6min
pages 165-169

Comparing the World Zones

7min
pages 175-179

Long Trends—Expansion and State Power

7min
pages 160-164

Long Trends—Disease and Malthusian Cycles

7min
pages 170-174

Agrarian Civilizations in Other Regions

6min
pages 152-155

Sumer—The First Agrarian Civilization

7min
pages 147-151

From Villages to Cities

6min
pages 142-146

Homo sapiens—The First Humans

6min
pages 104-108

The First Agrarian Societies

6min
pages 128-132

Early Power Structures

6min
pages 137-141

Power and Its Origins

5min
pages 133-136

The Origins of Agriculture

7min
pages 123-127

Threshold 7—Agriculture

6min
pages 118-122

Change in the Paleolithic Era

7min
pages 113-117

Paleolithic Lifeways

6min
pages 109-112

Life on Earth—Single-celled Organisms

5min
pages 82-85

Life on Earth—Multi-celled Organisms

6min
pages 86-90

Threshold 6—What Makes Humans Different?

7min
pages 99-103

Hominines

5min
pages 91-94

Evidence on Hominine Evolution

6min
pages 95-98

The Origins of Life

7min
pages 77-81

The Evidence for Natural Selection

6min
pages 73-76

Darwin and Natural Selection

6min
pages 69-72

Threshold 5—Life

6min
pages 64-68

Plate Tectonics and the Earth’s Geography

6min
pages 59-63

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