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Basaltic volcanism: The importance of planet size

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dc.contributor.author Walker, David, 1946-
dc.contributor.author Stolper, Edward M.
dc.contributor.author Hays, J. F.
dc.coverage.spatial Earth
dc.coverage.spatial Moon
dc.date.accessioned 2020-08-28T21:35:50Z
dc.date.available 2020-08-28T21:35:50Z
dc.date.issued 1979
dc.identifier.citation Proc. Lunar Planet. Sci. Conf. 10th (1979), p. 1995-2015. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1682
dc.description.abstract The volumetrically abundant basalts on the earth, its moon, and the eucrite parent planet all have chemical compositions that are controlled to a large extent by dry, low-pressure, crystal-liquid equilibria. Since this generalization is valid for these three planetary bodies, we infer that it may also apply to the other unsampled terrestrial planets. en
dc.description.statementofresponsibility D. Walker, E. M. Stolper, and J. F. Hays
dc.format.extent Pages 1995-2015
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries BVSP contribution ; no. 39
dc.subject Volcanism en
dc.subject Basalt en
dc.subject Planets en
dc.title Basaltic volcanism: The importance of planet size en
dc.type Book chapter en


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