CRATERING HISTORY AND LUNAR CHRNOLOGY

dc.contributor.authorStöffler D.
dc.contributor.authorRyder G.
dc.contributor.authorIvanov B.A.
dc.contributor.authorArtemieva N.A.
dc.contributor.authorCintala M.J.
dc.contributor.authorGrieve R.A.F.
dc.date.accessioned2024-07-20T12:13:52Z
dc.date.available2024-07-20T12:13:52Z
dc.date.issued2006
dc.description.abstractThe Moon is exceptional and important because it is the only planetary body besides the Earth for which we have both a detailed stratigraphic history and datable rock samples that can be related to specific geomorphologic units. The Moon has preserved much of its magmatic and impact record of at least the last 4 billion years. While its endogenic history is of great interest for the fundamentals of planetary interiors and surfaces, the Moon has become a calibration plate for the cratering record of the Earth-Moon system, and by extrapolation, of the entire inner solar system if one assumes a heliocentric origin for impactor populations.
dc.identifierhttps://elibrary.ru/item.asp?id=13519184
dc.identifier.citationReviews in Mineralogy and Geochemistry, 2006, 60, 60. С. 5, 519-596
dc.identifier.doi10.2138/rmg.2006.60.05
dc.identifier.issn1529-6466
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/44457
dc.titleCRATERING HISTORY AND LUNAR CHRNOLOGY
dc.typeСтатья

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