Early loss, fractionation, and redistribution of chlorine in the Moon as revealed by the low-Ti lunar mare basalt suite

dc.contributor.author Boyce, Jeremy W.
dc.contributor.author Kanee, Sarah A.
dc.contributor.author McCubbin, Francis M.
dc.contributor.author Barnes, Jessica J.
dc.contributor.author Treiman, Allan H.
dc.contributor.author https://orcid.org/0000-0002-8073-2839
dc.coverage.spatial Moon
dc.date.accessioned 2020-04-06T20:36:06Z
dc.date.available 2020-04-06T20:36:06Z
dc.date.issued 2018-10-15
dc.description.abstract The relative abundances of chlorine isotopes measured in low-Ti basalts from the Moon appear to reflect mixing between two reservoirs: One component representing the urKREEP—the final product of the crystallization of the lunar magma ocean, the other representing either a mare basalt reservoir or meteoritic materials. en
dc.description.statementofresponsibility Jeremy W. Boyce, Sarah A. Kanee, Francis M. McCubbin, Jessica J. Barnes, Hayley Bricker. Allan H. Treiman
dc.format.extent pages 205-214
dc.format.mimetype application/pdf
dc.identifier.citation Boyce, Jeremy W., Sarah A. Kanee, Francis M. McCubbin, Jessica J. Barnes, Hayley Bricker, and Allan H. Treiman. 2018. "Early loss, fractionation, and redistribution of chlorine in the Moon as revealed by the low-Ti lunar mare basalt suite". Earth and Planetary Science Letters. 500: 205-214. en
dc.identifier.other https://doi.org/10.1016/j.epsl.2018.07.042
dc.identifier.uri https://hdl.handle.net/20.500.11753/1484
dc.language.iso en en
dc.publisher Elsevier en
dc.relation.ispartofseries LPI contribution ; no. 2123
dc.rights.license Attribution 4.0 International (CC BY 4.0)
dc.subject Stable isotopes en
dc.subject Moon en
dc.title Early loss, fractionation, and redistribution of chlorine in the Moon as revealed by the low-Ti lunar mare basalt suite en
dc.type Article en
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