Central peaks in lunar craters are formed by crustal rebound after impact
the verdict
SUPPORTED
the evidence backs this
confidence 87/100
Central peaks in complex lunar craters expose deep-seated mantle and crustal materials, supporting the model that these elevated structures are formed by the rebound of the lunar crust following a large impact event.
Evidence for · 2
Copernicus Crater Central Peak: Lunar Mountain of Unique Composition
1982 · cited by 94
Identifies deep-seated olivine and unique mafic mineral assemblages exposed at the central peak of Copernicus crater, supporting the mechanism of deep crustal material uplift.
See more details
More for · 1
Volcanic processes within the Petavius crater, nearside of the Moon.
2025 · cited by 1
Confirms that central peaks in craters like Petavius expose deep crustal and mantle-derived mineral compositions consistent with uplift during impact crater formation.