Astrophysics (Index)About

Moon formation

(formation of the Moon)
(process by which the Moon and other moons formed)

Theories have been developed regarding Moon formation, the formation of the Moon, as well as other moons, which likely result from various processes. The giant-impact hypothesis is currently the standard model of the formation of the Moon, that sometime in the very early history of the solar system, a Mars-sized planet (termed Theia) struck the Earth sending debris from both into space which eventually coalesced into a circumplanetary disk. This explains why lunar material is strikingly similar to Earth material in isotope abundances (isotope signature) and radioactivity characteristics (though the Moon has a lower level of volatiles, which also requires explanation). A current issue with the model is that lunar material would be expected to show some signs of the different material from an impacting planet and it does not. Variations on the hypotheses to explain this:

Less well-established variations:

Each of these models has its problems.

Other solar system moons may have formed through one or more of these processes, with an additional possibilities of some other type of formation of a circumplanetary disk or of capture of an asteroid. Suitable capture methods (subsequent to the solar nebula's dissipation) require some coincidence, e.g., the simultaneous nearby presence of a third body, but it is seriously considered, for example, for Neptune's moon, Triton, due to its a retrograde orbit. Capture seems unlikely for the Moon because of its Earth-like isotope signature.


(Moon,moons)
Further reading:
https://en.wikipedia.org/wiki/Origin_of_the_Moon
https://en.wikipedia.org/wiki/Giant-impact_hypothesis
https://en.wikipedia.org/wiki/Synestia
https://www.windows2universe.org/earth/moon/capture_theory.html
https://www.extremetech.com/extreme/253830-giant-impact-hypothesis-moon-formation-synestia

Referenced by pages:
impact
lava planet
moon
PDS 70
planet formation
solar system

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