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    Application of organic geochemistry to detect signatures of organic matter in the Haughton impact structure

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    Author
    Parnell, John
    Lee, Pascal
    Osinski, Gordon R.
    Cockell, Charles S.
    Issue Date
    2005-01-01
    Keywords
    fluid inclusions
    organic Geochemistry
    Haughton impact structure
    impact craters
    organic matter
    
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    Citation
    Parnell, J., Lee, P., Osinski, G. R., & Cockell, C. S. (2005). Application of organic geochemistry to detect signatures of organic matter in the Haughton impact structure. Meteoritics & Planetary Science, 40(12), 1879-1885.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656081
    DOI
    10.1111/j.1945-5100.2005.tb00151.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Organic geochemistry applied to samples of bedrock and surface sediment from the Haughton impact structure detects a range of signatures representing the impact event and the transfer of organic matter from the crater bedrock to its erosion products. The bedrock dolomite contains hydrocarbon-bearing fluid inclusions which were incorporated before the impact event. Comparison of biomarker data from the hydrocarbons in samples inside and outside of the crater show the thermal signature of an impact. The occurrence of hydrocarbon inclusions in hydrothermal mineral samples shows that organic matter was mobilized and migrated in the immediate aftermath of the impact. The hydrocarbon signature was then transferred from bedrock to the crater-fill lacustrine deposits and present-day sediments in the crater, including wind-blown detritus in snow/ice. Separate signatures are detected from modern microbial life in crater rock and sediment samples. Signatures in Haughton crater samples are readily detectable because they include hydrocarbons generated by the burial of organic matter. This type of organic matter is not expected in crater samples on other planets, but the Haughton data show that, using very high resolution detection of organic compounds, any signature of primitive life in the crater rocks could be transferred to surface detritus and so extend the sampling medium.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00151.x
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    Meteoritics & Planetary Science, Volume 40, Number 12 (2005)

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