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A comparison of fractionation trends in the lunar crust and the Stillwater Complex

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dc.contributor.author Raedeke, Linda Dismore
dc.contributor.author McCallum, I. S.
dc.coverage.spatial Montana
dc.coverage.spatial Moon
dc.date.accessioned 2020-08-04T18:46:44Z
dc.date.available 2020-08-04T18:46:44Z
dc.date.issued 1980
dc.identifier.citation Papike, J.J. and Merrill, R.B., eds. Proc. Conf. Lunar Highlands Crust (1980). p. 133-153. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1662
dc.description.abstract Even if the magma ocean hypothesis in its present form should not prove equal to the task of explaining all the observational data, it seems highly probable that the concept of crystal/liquid fractionation and segregation will endure. We accept as a basic premise for this paper that these processes were important during the early evolution of the moon and will attempt to explain the observed fractionation trends in lunar highland rocks within this framework. en
dc.format.extent Pages 133-153
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LPI contribution ; no. 404
dc.subject Moon--Crust en
dc.subject Lunar petrology en
dc.title A comparison of fractionation trends in the lunar crust and the Stillwater Complex en
dc.type Book chapter en


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