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

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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.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.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.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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