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dc.contributor.authorYamaguchi, Akira
dc.contributor.authorSetoyanagi, Takehiko
dc.contributor.authorEbihara, Mitsuru
dc.date.accessioned2021-02-12T21:40:38Z
dc.date.available2021-02-12T21:40:38Z
dc.date.issued2006-01-01
dc.identifier.citationYamaguchi, A., Setoyanagi, T., & Ebihara, M. (2006). An anomalous eucrite, Dhofar 007, and a possible genetic relationship with mesosiderites. Meteoritics & Planetary Science, 41(6), 863-874.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2006.tb00491.x
dc.identifier.urihttp://hdl.handle.net/10150/656142
dc.description.abstractWe studied the texture, mineralogy, and bulk chemical composition of Dhofar 007, a basaltic achondrite. Dhofar 007 is a polymict breccia that is mostly composed of coarse-grained granular (CG) clasts with a minor amount of xenolithic components, such as a fragment of Mg-rich pyroxene. The coarse-grained, relict gabbroic texture, mineral chemistry, and bulk chemical data of the coarse-grained clast indicate that the CG clasts were originally a cumulate rock crystallized in a crust of the parent body. However, in contrast to monomict eucrites, the siderophile elements are highly enriched and could have been introduced by impact events. Dhofar 007 appears to have experienced a two-stage postcrystallization thermal history: rapid cooling at high temperatures and slow cooling at lower temperatures. The presence of pigeonite with closely spaced, fine augite lamellae suggests that this rock was cooled rapidly from higher temperatures (>0.5 degrees C/yr at ~1000 degrees C) than typical cumulate eucrites. However, the presence of the cloudy zone in taenite and the Ni profile across the kamacite-taenite boundaries indicates that the cooling rate was very slow at lower temperatures (~1-10 degrees C/Myr at <600-700 degrees C). The slow cooling rate is comparable to those in mesosiderites and pallasites. The two-stage thermal history and the relative abundance of siderophile elements similar to those for metallic portions in mesosiderites suggest that Dhofar 007 is a large inclusion of mesosiderite. However, we cannot rule out a possibility that Dhofar 007 is an anomalous eucrite.
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.subjectmesosiderite
dc.subjecteucrites
dc.subjectthermal history
dc.titleAn anomalous eucrite, Dhofar 007, and a possible genetic relationship with mesosiderites
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.volume41
dc.source.issue6
dc.source.beginpage863
dc.source.endpage874
refterms.dateFOA2021-02-12T21:40:38Z


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