Clast-laden nature and the origin of Luna 24 olivine-vitrophyres

dc.contributor.author	Basu, Abhijit
dc.contributor.author	McKay, David S.
dc.contributor.author	Fruland, Ruth M.
dc.coverage.spatial	Moon
dc.date.accessioned	2020-05-11T20:43:27Z
dc.date.available	2020-05-11T20:43:27Z
dc.date.issued	1978
dc.description.abstract	Particles of olivine-vitrophyre make up less than one percent of the <250 μm fraction of the Luna 24 soils. They contain microphenocrysts of olivine and spinel, together with a variety of olivine, pyroxene, plagioclase, a silica phase, and opaque oxide clasts.	en
dc.description.statementofresponsibility	Abhijit Basu, Department of Geology, Indiana University, Bloomington, Indiana 47401, David S. Mckay and Ruth M. Fruland, NASA-Johnson Space Center, Houston, Texas 77058
dc.format.extent	Pages 535-546
dc.format.mimetype	application/pdf
dc.identifier.citation	Basu, A., Mckay, D.S., Fruland, R.M., 1978. Clast-Laden Nature and the Origin of Luna 24 Olivine-Vitrophyres, in: Proceedings of the Ninth Lunar and Planetary Science Conference, Houston, Texas, March 13-17, 1978, LSI Contribution. Pergamon Press, New York, NY, pp. 535–546.	en
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1522
dc.language.iso	en	en
dc.publisher	Pergamon Press	en
dc.relation.ispartof	Proceedings of the Ninth Lunar and Planetary Science Conference, Houston, Texas, March 13-17, 1978
dc.relation.ispartofseries	LSI contribution ; no. 332
dc.subject	Lunar surface samples	en
dc.title	Clast-laden nature and the origin of Luna 24 olivine-vitrophyres	en
dc.type	Book chapter	en

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