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    Experimental shock synthesis of diamonds in a graphite gneiss

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    Author
    Kenkmann, T.
    Hornemann, U.
    Stöffler, D.
    Issue Date
    2005-01-01
    Keywords
    diamond
    graphite
    Raman spectroscopy
    shock experiments
    shock metamorphism
    
    Metadata
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    Citation
    Kenkmann, T., Hornemann, U., & Stöffler, D. (2005). Experimental shock synthesis of diamonds in a graphite gneiss. Meteoritics & Planetary Science, 40(9-10), 1299-1310.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656046
    DOI
    10.1111/j.1945-5100.2005.tb00402.x
    Additional Links
    https://meteoritical.org/
    Abstract
    The occurrence of diamonds in terrestrial impact craters and meteorites is related to dynamic shock loading during hypervelocity impacts. To understand the mechanism of impact diamond formation in natural rocks, shock-recovery experiments with graphite gneiss were carried out at shock pressures between 35 and 79 GPa. This is the first report on the successful shock synthesis of microdiamonds in a natural rock. Micrometer-size diamonds and a wide range of intermediate, presently unclassified, amorphous, and disordered carbon phases were observed within vesiculated biotite melts in the vicinity of relic graphite grains using microRaman spectrometry. We explain these findings by jetting mechanisms of carbon and graphite clusters, originating at the edges of graphite grains, into the very hot and volatile rich biotitic melt veins during shock loading. This environment enabled the thermally activated crystallization of diamonds during shock compression in a period of less than 0.5 microseconds. Regraphitization of diamonds during pressure release was widespread and caused the formation of the amorphous to disordered carbon phases recorded frequently with microRaman spectroscopy. The surviving diamonds must have cooled down to 2000 K during the compression phase at local thermal sinks and cooler interfaces to avoid regraphitization.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00402.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 40, Number 9-10 (2005)

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