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    PDF orientations in shocked quartz grains around the Chicxulub crater

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    Author
    Nakano, Yoichiro
    Goto, Kazuhisa
    Matsui, Takafumi
    Tada, Ryuji
    Tajika, Eiichi
    Issue Date
    2008-01-01
    Keywords
    K/T boundary deposits
    Chicxulub
    YAX-1
    PDFs
    
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    Citation
    Nakano, Y., Goto, K., Matsui, T., Tada, R. and Tajika, E. (2008), PDF orientations in shocked quartz grains around the Chicxulub crater. Meteoritics & Planetary Science, 43(4), 745-760.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656421
    DOI
    10.1111/j.1945-5100.2008.tb00682.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We measured 852 sets of planar deformation features (PDFs) in shocked quartz grains in impactite samples of the Yaxcopoil (YAX-1) core and from 4 Cretaceous/Tertiary (K/T) boundary deposits: the Monaca, the Cacarajcara, and the Pealver formations in Cuba, and DSDP site 536, within 800 km of the Chicxulub crater, in order to investigate variations of PDF orientations in the proximity of the crater. Orientations of PDFs show a broad distribution with peaks at omega {1013}, pi {1012}, and xi {1112}, plus r, z {1011} orientations with minor c(0001), s{1121}, t{2241} plus x{5161}, and m{1010} plus a{11-20} orientations. Planar deformation features with c(0001) orientation are relatively more abundant in the proximity of the Chicxulub crater than in distal sitessuch as North America, the Pacific Ocean, and Europe. This feature indicates that in the proximity ofthe crater, part of the shocked quartz grains in the K/T boundary deposits were derived from the lowshock pressure zones. Moreover, the orientations of PDFs with xi {1122} plus r, z {1011} are high in our studied sites, and frequencies of these orientations decrease with increasing distance from the crater. On the other hand, absence of c(0001) and the rare occurrence of PDFs with xi {1122} plus r, z {1011} orientations in the sample from the YAX-1 core that was taken at the top of the impactitelayer of the Chicxulub crater suggests that the sampling horizon that reflects a certain cratering stageis also an important factor for variations in shocked quartz.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2008.tb00682.x
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    Meteoritics & Planetary Science, Volume 43, Number 4 (2008)

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