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Apollo 14 mineral ages and the thermal history of the Fra Mauro formation

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dc.contributor.author Compston, W.
dc.contributor.author Vernon, M. J.
dc.contributor.author Berry, H.
dc.contributor.author Rudowski, R.
dc.contributor.author Gray, C. M.
dc.contributor.author Ware, N.
dc.contributor.author Chappell, B. W.
dc.contributor.author Kaye, M.
dc.coverage.spatial Moon
dc.date.accessioned 2020-05-07T21:10:47Z
dc.date.available 2020-05-07T21:10:47Z
dc.date.issued 1972
dc.identifier.citation Compston, W., Vernon, M.J., Berry, H., Rudowski, R., Gray, C.M., Ware, N., Chappell, B.W., Kaye, M., 1972. Apollo 14 Mineral Ages and the Thermal History of the Fra Mauro Formation, in: Proceedings of the Third Lunar Science Conference. MIT Press, Cambridge, Mass., pp. 1487–1501. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1515
dc.description.abstract In this paper we document and give multiple interpretations of the isotopic ages of Apollo 14 igneous rocks cited previously at the Third Lunar Science Conference (Compston et al., 1972). Our major-element analyses for the latter were given at the same conference, and major- and trace-element analyses on these and of the remainder of our allocation, various Apollo 14 fines, will be reported and discussed later. en
dc.description.statementofresponsibility W. Compston, M. J. Vernon, H. Berry, R. Rudowski, C. M. Gray, And N. Ware, Department of Geophysics and Geochemistry, Australian National University, and B. W. Chappell And M. Kaye, Department of Geology, Australian National University
dc.format.extent Pages 1487-1501
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartof Proceedings of the Third Lunar Science Conference, Houston, Texas, January 10-13, 1972
dc.relation.ispartofseries LSI contribution ; no. 92
dc.subject Moon en
dc.subject Lunar surface samples en
dc.subject Fra Mauro Crater (Moon) en
dc.title Apollo 14 mineral ages and the thermal history of the Fra Mauro formation en
dc.type Book chapter en


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