Relative cooling rates of mare basalts at the Apollo 12 and 15 sites as estimated from pyroxene exsolution data

dc.contributor.author	Takeda, Hiroshi
dc.contributor.author	Miyamoto, Masamichi
dc.contributor.author	Ishii, Teruaki
dc.contributor.author	Lofgren, Gary E.
dc.coverage.spatial	Moon
dc.date.accessioned	2020-06-03T21:44:01Z
dc.date.available	2020-06-03T21:44:01Z
dc.date.issued	1975
dc.description.abstract	X-ray single-crystal diffraction studies, supplemented by electron microprobe analyses of core pigeonites and rim augites from rocks 12031, 15085, 15475, and 15495, have been used to suggest cooling rates for these and other Apollo 12 and 15 rocks studied by similar methods.	en
dc.description.statementofresponsibility	Hiroshi Takeda, Masamichi Miyamoto, Teruaki Ishii, Gary E. Lofgren
dc.format.extent	Pages 987-996
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1559
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartof	Proceedings of the Sixth Lunar Science Conference : Houston, Texas, March 17-21, 1975
dc.relation.ispartofseries	LPI contribution ; no. 223
dc.subject	Lunar petrology	en
dc.subject	Lunar surface samples	en
dc.title	Relative cooling rates of mare basalts at the Apollo 12 and 15 sites as estimated from pyroxene exsolution data	en
dc.type	Book chapter	en

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