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.