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Evidence for ancient mare volcanism

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dc.contributor.author Schultz, Peter H., 1944-
dc.contributor.author Spudis, Paul D.
dc.contributor.author https://orcid.org/0000-0003-3391-0417
dc.coverage.spatial Moon
dc.date.accessioned 2020-07-31T21:50:28Z
dc.date.available 2020-07-31T21:50:28Z
dc.date.issued 1979
dc.identifier.citation Proc. Lunar Planet. Sc,. Conf. 10th (1979), p. 2899-2918. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1658
dc.description.abstract Basaltic volcanism clearly exposed as dark surface units may represent only the last stages of continuous volcanic activity during the first 1.5 b.y. of lunar history. Between 3.0 and 3.9 AE, part of this record has been masked by ejecta deposits from large (> 100 km) impact craters but is then partly re-exposed by subsequent smaller impacts. en
dc.format.extent Pages 2899-2918
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LPI contribution ; no. 388
dc.subject Lunar volcanoes en
dc.subject Basalt en
dc.title Evidence for ancient mare volcanism en
dc.type Book chapter en


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