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dc.contributor.authorMaruoka, T.
dc.contributor.authorKoeberl, C.
dc.contributor.authorMatsuda, J.
dc.contributor.authorSyono, Y.
dc.date.accessioned2021-02-12T20:56:20Z
dc.date.available2021-02-12T20:56:20Z
dc.date.issued2003-01-01
dc.identifier.citationMaruoka, T., Koeberl, C., Matsuda, J. I., & Syono, Y. (2003). Carbon isotope fractionation between graphite and diamond during shock experiments. Meteoritics & Planetary Science, 38(8), 1255-1262.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2003.tb00311.x
dc.identifier.urihttp://hdl.handle.net/10150/655738
dc.description.abstractCarbon isotopic compositions were measured for shock-produced diamond and shocked graphite formed at peak pressures ranging from 37 to 52 GPa. The delta-13C values of diamonds produced in a sealed container were generally lower than that of the initial graphite. The differences in the carbon isotopic composition between initial graphite and shocked graphite/diamond may reflect kinetic isotopic fractionation during the oxidation of the graphite/diamond and/or analytical artifacts possibly induced by impurities in the samples. The pressure effect on the isotopic fractionations between graphite and diamond can be estimated from the delta-13C values of impurity-free diamonds produced using a vented container from which gases, including oxygen, in pore spaces escaped during or after the diamond formation (e.g., 0.039 +/- 0.085 at a peak pressure of 52 GPa). Any isotopic fractionation induced by shock conversion of graphite to diamond is too small to be detected in natural shock-induced diamond-graphite systems related to terrestrial impact cratering processes.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectUreilite diamonds
dc.subjectShock-produced diamond
dc.subjectimpact cratering
dc.titleCarbon isotope fractionation between graphite and diamond during shock experiments
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume38
dc.source.issue8
dc.source.beginpage1255
dc.source.endpage1262
refterms.dateFOA2021-02-12T20:56:20Z


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