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    In situ micro-Raman and X-ray diffraction study of diamonds and petrology of the new ureilite UAE 001 from the United Arab Emirates

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    Author
    Hezel, D. C.
    Dubrovinsky, L.
    Nasdala, L.
    Cauzid, J.
    Simionovici, A.
    Gellissen, M.
    Schönbeck, T.
    Issue Date
    2008-01-01
    Keywords
    ureilites
    diamond
    micro-Raman
    in-situ XRD
    
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    Citation
    Hezel, 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.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656449
    DOI
    10.1111/j.1945-5100.2008.tb01117.x
    Additional Links
    https://meteoritical.org/
    Abstract
    A 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.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2008.tb01117.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 43, Number 7 (2008)

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