CRATERING HISTORY AND LUNAR CHRNOLOGY

dc.contributor.author	Stöffler D.
dc.contributor.author	Ryder G.
dc.contributor.author	Ivanov B.A.
dc.contributor.author	Artemieva N.A.
dc.contributor.author	Cintala M.J.
dc.contributor.author	Grieve R.A.F.
dc.date.accessioned	2024-07-20T12:13:52Z
dc.date.available	2024-07-20T12:13:52Z
dc.date.issued	2006
dc.identifier	https://elibrary.ru/item.asp?id=13519184
dc.identifier.citation	Reviews in Mineralogy and Geochemistry, 2006, 60, 60. С. 5, 519-596
dc.identifier.issn	1529-6466
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/44457
dc.description.abstract	The 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.title	CRATERING HISTORY AND LUNAR CHRNOLOGY
dc.type	Статья
dc.identifier.doi	10.2138/rmg.2006.60.05

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