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

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

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

Page 1: Explorations of the Universe How Did the Earth and Moon Form?

Explorations of the Universe

How Did the Earth and Moon Form?

Page 2: 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

• 1950-1980: Earth need not have formed hot

• Modern: Hot Early Earth was right after all

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

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The Early Earth Cools

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The Oceans Form

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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

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A Modern Idea of Early Earth

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How Did the Moon Form?Pre-1985 Ideas

• Fission

• Co-Creation

• Capture

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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

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Co-Creation

• Moon should orbit in Earth’s equatorial plane

• Moon is less dense and different in chemistry than Earth

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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

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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

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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.

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As Usual, In Any Area of

Science, Gary Larson Gets There First

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A Great Time for Space Artists

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This is a more or less

literal rendition of

an early computer simulation

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

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

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The First Moonrise