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Explorations of the Universe How Did the Earth and Moon Form?

Explorations of the Universe

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Explorations of the Universe. How Did the Earth and Moon Form?. Ideas About the Early Earth Have Run Hot and Cold (Literally). To 1900: Early Earth hot. Only way to explain its internal heat 1900-1950: Radioactivity can explain internal heat, but concept of hot formation lingers - PowerPoint PPT Presentation

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Page 1: Explorations of the Universe

Explorations of the Universe

How Did the Earth and Moon Form?

Page 2: Explorations of the Universe

Ideas About the Early Earth Have Run Hot and Cold (Literally)

• To 1900: Early Earth hot. Only way to explain its internal heat

• 1900-1950: Radioactivity can explain internal heat, but concept of hot formation lingers

• 1950-1980: Earth need not have formed hot• Modern: Hot Early Earth was right after all

Page 3: Explorations of the Universe

A Classic Early Piece of Space Art: Chesley Bonestell, 1953

Page 4: Explorations of the Universe

The Early Earth Cools

Page 5: Explorations of the Universe

The Oceans Form

Page 6: Explorations of the Universe

Cold Earth - Hot Earth (Again)• If Earth accreted, need not have been hot• Depends on how fast heat radiated away

compared to impact rate• As planets get bigger, their gravity causes

higher-velocity impacts• Also impact ejecta buries hot rocks• Early Earth was hot - had magma ocean

Page 7: Explorations of the Universe

A Modern Idea of Early Earth

Page 8: Explorations of the Universe

How Did the Moon Form?Pre-1985 Ideas

• Fission• Co-Creation• Capture

Page 9: Explorations of the Universe

Fission

• Early Earth spun rapidly, became unstable, broke in two.

• Moon should orbit in Earth’s equatorial plane

• Can’t simply throw something from surface into orbit - it either falls back or escapes

Page 10: Explorations of the Universe

Co-Creation

• Moon should orbit in Earth’s equatorial plane

• Moon is less dense and different in chemistry than Earth

Page 11: Explorations of the Universe

Capture

• Can explain why Moon orbits close to ecliptic plane.

• Can account for why Moon differs in density and chemistry from Earth

• Requires extremely stringent conditions to happen

• Seems too unlikely

Page 12: Explorations of the Universe

A New Hypothesis: Mega-Impact

• In computer simulations of solar system formation, we don’t get nine big planets

• First stage: hundreds of Moon-Mars size planets

• Small planets collide to make bigger ones• Can explain numerous Solar System

anomalies

Page 13: Explorations of the Universe

A New Hypothesis: Mega-Impact

• Can explain why Moon orbits close to ecliptic plane.

• Can account for why Moon differs in density and chemistry from Earth

• A capture requires extremely precise conditions - a collision takes no skill at all.

Page 14: Explorations of the Universe

As Usual, In Any Area of

Science, Gary Larson Gets There First

Page 15: Explorations of the Universe

A Great Time for Space Artists

Page 16: Explorations of the Universe

This is a more or less

literal rendition of

an early computer simulation

Page 17: Explorations of the Universe

Computer Simulations by H.J. Melosh (University of Arizona)

Page 18: Explorations of the Universe
Page 19: Explorations of the Universe
Page 20: Explorations of the Universe

Earth would have been as hot as the Sun for about 10,000 years

Page 21: Explorations of the Universe

The First Moonrise