Geological and geochemical evidence indicates the Moon formed from a giant impact with the early Earth
Geological and geochemical studies consistently support the giant impact hypothesis, in which the Moon formed from a collision between the early Earth and a planetary body such as Theia.
Papers [0] and [1] directly address the Moon-forming giant impact hypothesis using geochemical and isotopic constraints, providing clear support for the claim. The remaining papers discuss unrelated topics such as prebiotic chemistry, impact basins on the lunar farside, or solar wind sputtering, and are thus tangential.
Hélène Piet, James Badro, Philippe Gillet. Geochemical Constraints on the Size of the Moon‐Forming Giant Impact. 2017. https://doi.org/10.1002/2017gl075225
Paper [0] models the geochemical constraints and mantle impact consequences of the Moon-forming giant impact hypothesis.
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Fischer M, Peters STM, Herwartz D, Hartogh P, Di Rocco T, Pack A. Oxygen isotope identity of the Earth and Moon with implications for the formation of the Moon and source of volatiles.. 2024. https://doi.org/10.1073/pnas.2321070121
Paper [1] discusses isotopic evidence and geochemical identity regarding the collision between proto-Earth and Theia that formed the Moon.
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