Formation of the Moon
Theories of Moon Formation
Coformation Theory
Suggests that the Moon formed at the same time as the Earth from the same material.
Critique: The Earth and Moon have different compositions:
Earth has a metallic core, rocky mantle, and crust.
Moon consists predominantly of rock.
Challenges arise: Where does the metal go if they formed together?
Capture Theory
Proposes that the Moon formed independently in space and was later captured by Earth's gravity.
Critique: Similarities in the composition of Earth and Moon rocks:
The crust and mantle rocks of the Earth are very similar to those of the Moon.
Suggests a problematic origin since such similarities are unlikely if the Moon was captured.
Impact Theory (Current Theory)
Most widely accepted explanation:
The Earth, having already differentiated, was struck by a Mars-sized body.
This impact:
Ejected significant amounts of the Earth’s crust and mantle into space.
Caused the mixing of the two bodies (the Earth and the impacting body’s core).
The remaining debris:
Gathered in orbit around Earth due to its gravitational pull.
Eventually coalesced to form the Moon.
Explains similarities:
The rocks making up the Moon originated from the Earth’s crust and mantle which were blasted into space during the impact.
Iron is too heavy to have escaped into space and thus remains part of Earth’s core.
Geological History of the Moon
Moon formation occurred over 4 billion years ago.
After its formation, the Moon was bombarded by meteorites:
Resulted in numerous craters across the surface.
Mares (dark basalt plains on the Moon) formed about 3 billion years ago.
Initially, the Moon had no mares, which later developed from basaltic flows.
Continued impacts:
The Moon is still being hit, but most current impacts are minor micrometeorites which smooth the surface over time.
This smoothing causes the mares and craters to become less distinct.
Overall, the Moon's surface has remained relatively stable, with minimal changes except for the effects of micrometeorite impacts.