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    Shock metamorphism of quartz at the submarine Mjølnir impact crater, Barents Sea

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    Author
    Sandbakken, P. T.
    Langenhorst, F.
    Dypvik, H.
    Issue Date
    2005-01-01
    Keywords
    Mjølnir
    Planar microstructures
    shock metamorphism
    Shocked quartz
    Submarine impact
    
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    Citation
    Sandbakken, P. T., Langenhorst, F., & Dypvik, H. (2005). Shock metamorphism of quartz at the submarine Mjølnir impact crater, Barents Sea. Meteoritics & Planetary Science, 40(9-10), 1363-1375.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656051
    DOI
    10.1111/j.1945-5100.2005.tb00407.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Shock metamorphosed quartz grains have been discovered in a drill core from the central peak of the Late Jurassic, marine Mjølnir structure; this finding further corroborates the impact origin of Mjølnir. The intersected strata represent the Upper Jurassic Hekkingen Formation and underlying Jurassic and Upper Triassic formations. The appearance, orientation, and origin of shock features in quartz grains and their stratigraphic distribution within the core units have been studied by optical and transmission electron microscopy. The quartz grains contain planar fractures (PFs), planar deformation features (PDFs), and mechanical Brazil twins. The formation of PFs is the predominant shock effect and is attributed to the large impedance differences between the water-rich pores and constituent minerals in target sediments. This situation may have strengthened tensional/extensional and shear movements during shock compression and decompression. The combination of various shock effects indicates possible shock pressures between 5 and at least 20 GPa for three core units with a total thickness of 86 m (from 74.00 m to 171.09 m core depth). Crater-fill material from the lower part of the core typically shows the least pressures, whereas the uppermost part of the allochthonous crater deposits displays the highest pressures. The orientations of PFs in studied quartz grains seem to become more diverse as the pressure rises from predominantly (0001) PFs to a combination of (0001), {0011}, and {0022} orientations. However, the lack of experimental data on porous sedimentary rocks does not allow us to further constrain the shock conditions on the basis of PF orientations.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00407.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 40, Number 9-10 (2005)

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