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

Page 39

From about 10í35 of a second after the moment of creation, we can tell a good scienti¿c story. Something appeared. It was tiny (the size of an atom perhaps) and inconceivably hot. It was expanding rapidly and cooling fast. At this point, energy and matter were indistinguishable. As this “something” cooled, “things” and “forces” appeared, in a series of “phase changes,” rather like the change steam undergoes as it turns into water. Gravity appeared from the chaos, as did the “strong” and “electromagnetic” forces. From 10í33 to 10í32 seconds, the Universe expanded faster than the speed of light, growing from the size of an atom to the size of a galaxy. This phase is known as “inÀation.” Within the ¿rst second, quarks—the building blocks of atomic nuclei— were created in positive and negative forms. These then proceeded to annihilate each other, leaving just a few survivors. These forlorn survivors formed protons (which are positively charged) and neutrons (which are electrically neutral). Electrons (lighter than protons and negatively charged) were created in an equally violent process. A few minutes after the big bang, the Universe consisted of a hot “plasma” (a mixture of energy and charged subatomic particles, a bit like the center of the Sun today). About 380,000 years later, the Universe was cool enough for positively charged protons to capture negatively charged electrons, creating the ¿rst, simple atoms of hydrogen and helium. Because the positive charges of protons are cancelled by the negative charges of electrons, atoms are electrically neutral, so electromagnetic radiation (of which light is just one form) could now travel freely through the Universe without getting tangled in networks of electromagnetism. The Universe cooled, entering a “dark age” that lasted several hundred million years. Other entities and forces were created that we don’t understand. We call this missing stuff “dark matter” or “dark energy.” We know it’s there because studies of the movements of galaxies show that something is exerting a powerful gravitational pull. This stuff may account for up to 95% of the Universe’s total mass. Seventy percent of that total may consist of undetected forms of energy. Twenty-¿ve percent may consist of matter in forms we cannot detect because they emit no radiation (such as cold, dead stars or 29


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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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