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dc.contributor.authorHezel, D. C.
dc.contributor.authorDubrovinsky, L.
dc.contributor.authorNasdala, L.
dc.contributor.authorCauzid, J.
dc.contributor.authorSimionovici, A.
dc.contributor.authorGellissen, M.
dc.contributor.authorSchönbeck, T.
dc.date.accessioned2021-02-12T22:30:57Z
dc.date.available2021-02-12T22:30:57Z
dc.date.issued2008-01-01
dc.identifier.citationHezel, D. C., Dubrovinsky, L., Nasdala, L., Cauzid, J., Simionovici, A., Gellissen, M., & Schönbeck, T. (2008). In situ micro‐Raman and X‐ray diffraction study of diamonds and petrology of the new ureilite UAE 001 from the United Arab Emirates. Meteoritics & Planetary Science, 43(7), 1127-1136.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2008.tb01117.x
dc.identifier.urihttp://hdl.handle.net/10150/656449
dc.description.abstractA new olivine-pigeonite ureilite containing abundant diamonds and graphite was found in the United Arab Emirates. This is the first report of a meteorite in this country. The sample is heavily altered, of medium shock level, and has a total weight of 155 g. Bulk rock, olivine (Fo79.881.8) and pyroxene (En73.9-75.2, Fs15.5-16.9, Wo8.8-9.5) compositions are typical of ureilites. Olivine rims are reduced with Fo increasing up to Fo96.1-96.8. Metal in these rims is completely altered to Fehydroxide during terrestrial weathering. We studied diamond and graphite using micro-Raman and in situ synchrotron X-ray diffraction. The main diamond Raman band (LO=TO mode at ~1332 cm^(-1)) is broadened when compared to well-ordered diamond single crystals. Full widths at half maximum (FWHM) values scatter around 7 cm^(-1). These values resemble FWHM values obtained from chemical vapor deposition (CVD) diamond. In situ XRD measurements show that diamonds have large grain sizes, up to 5 micrometers. Some of the graphite measured is compressed graphite. We explore the possibilities of CVD versus impact shock origin of diamonds and conclude that a shock origin is much more plausible. The broadening of the Raman bands might be explained by prolonged shock pressure resulting in a transitional Raman signal between experimentally shock-produced and natural diamonds.
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.subjectureilites
dc.subjectdiamond
dc.subjectmicro-Raman
dc.subjectin-situ XRD
dc.titleIn situ micro-Raman and X-ray diffraction study of diamonds and petrology of the new ureilite UAE 001 from the United Arab Emirates
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.volume43
dc.source.issue7
dc.source.beginpage1127
dc.source.endpage1136
refterms.dateFOA2021-02-12T22:30:57Z


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