Central peaks in lunar craters are formed by crustal rebound after impact
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.
The retrieved literature includes studies of lunar crater central peaks (such as Copernicus and Petavius) demonstrating that their composition consists of deep-seated crustal and mantle materials like olivine and plagioclase. This mineralogical exposure confirms that central peaks are formed by the uplift or rebound of deep target material during complex crater collapse. None of the papers refute this well-established planetary science mechanism, though many retrieved papers are off-topic (discussing aortic dissection, cancer radiotherapy, Mars mineralogy, etc.).
Carle M. Pieters. Copernicus Crater Central Peak: Lunar Mountain of Unique Composition. 1982. https://doi.org/10.1126/science.215.4528.59
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.
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Satyakumar AV, Patel S, Patel DD. Volcanic processes within the Petavius crater, nearside of the Moon.. 2025. https://doi.org/10.1038/s41598-025-95132-5
Confirms that central peaks in craters like Petavius expose deep crustal and mantle-derived mineral compositions consistent with uplift during impact crater formation.
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