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    Boltysh, another end-Cretaceous impact

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    Author
    Kelley, S. P.
    Gurov, E.
    Issue Date
    2002-01-01
    Keywords
    impact cratering
    craters
    K/T boundary
    Cretaceous
    cratering
    terrestrial
    Earth
    Boltysh Crater
    Chicxulub crater
    
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    Show full item record
    Citation
    Kelley, S. P., & Gurov, E. (2002). Boltysh, another end‐Cretaceous impact. Meteoritics & Planetary Science, 37(8), 1031-1043.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655547
    DOI
    10.1111/j.1945-5100.2002.tb00875.x
    Additional Links
    https://meteoritical.org/
    Abstract
    The Chixculub impact occurred at the Cretaceous/Tertiary (K/T) boundary, and although several other Late Cretaceous and Paleogene impact craters have, at times, been linked with the K/T boundary, isotope geochronology has demonstrated that all have significantly different ages. The currently accepted age of the 24 km diameter Boltysh crater, a K-Ar whole-rock age, places it in the Coniacian at 88 +/- 3 Ma. However, comprehensive Ar-Ar dating of a range of melt samples yields a mean age of 65.17 +/- 0.64 Ma, within errors of the K/T boundary. Several of the fresh samples exhibit signs of excess argon, but this seems to be concentrated in rapidly crystallized glass-rich samples. The Ar-Ar age confirms an earlier fission track measurement and thus two dating techniques have yielded an age within errors of the K/T boundary for this crater. Crucially, although the ages of Boltysh and Chixculub are within errors, they may not have formed synchronously. Craters of 24 km diameter occur much more commonly than impacts of Chixculub dimensions, but their proximity does raise the important question of how many impacts there might have been close to the K/T boundary.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2002.tb00875.x
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    Meteoritics & Planetary Science, Volume 37, Number 8 (2002)

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