Apollo 14 revisited, or breccias aren't so bad after all

dc.contributor.author	Simonds, Charles H.
dc.contributor.author	Phinney, William C.
dc.contributor.author	Warner, Jeffrey L.
dc.contributor.author	McGee, Patricia E.
dc.contributor.author	Geeslin, Jill
dc.contributor.author	Brown, Roy W.
dc.contributor.author	Rhodes, J. Michael
dc.coverage.spatial	Moon
dc.date.accessioned	2020-07-16T21:54:53Z
dc.date.available	2020-07-16T21:54:53Z
dc.date.issued	1977
dc.description.abstract	Study of the large Apollo 14 rocks supplemented by petrographic and chemical studies of the previously undescribed comprehensive sample suggests that the Apollo 14 samples were formed by the same processes which operated to form the range of impactities found at Apollo 16 and 17 and in terrestrial craters, especially those in crystalline targets.	en
dc.format.extent	Pages 1869-1893
dc.format.mimetype	application/pdf
dc.identifier.citation	Proc. Lunar Sci. Conf. 8th (1977), p. 1869-1893.	en
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1645
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartofseries	LSI contribution ; no. 286
dc.subject	Breccia	en
dc.subject	Lunar surface samples	en
dc.subject	Lunar petrology	en
dc.title	Apollo 14 revisited, or breccias aren't so bad after all	en
dc.type	Book chapter	en

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