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    Mineralogy, microtexture, and composition of shock-induced melt pockets in the Los Angeles basaltic shergottite

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    Author
    Walton, E. L.
    Spray, J. G.
    Issue Date
    2003-01-01
    Keywords
    Martian (SNC) meteorites
    shergottites
    shock metamorphism
    
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    Citation
    Walton, E. L., & Spray, J. G. (2003). Mineralogy, microtexture, and composition of shock‐induced melt pockets in the Los Angeles basaltic shergottite. Meteoritics & Planetary Science, 38(12), 1865-1875.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655780
    DOI
    10.1111/j.1945-5100.2003.tb00020.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Analytical electron microscopy of shock features in the basaltic shergottite Los Angeles (stone 1) reveals: 1) shock recorded in the bulk sample; and 2) localized pressure and temperature excursions that have generated melt pockets up to 4 mm in diameter. Bulk shock effects include microfaulting (offsets 1-200 m), mosaicism, deformed exsolution lamellae and planar fracturing in pyroxene, undulose extinction in whitlockite, mechanical twinning in titanomagnetite and ilmenite, and the transformation of plagioclase to maskelynite (less than or equal to 4% remnant reduced birefringence). The pressure estimates for bulk shock are 35-40 GPa. Localized shock excursions have generated three types of discrete melt zones (0.07 x 1.3 mm to 3.0 x 3.5 mm apparent diameter) possessing glassy to microcrystalline groundmasses. These melt pockets are differentiated on the basis of size, clast volume, and degree of crystallization and vesiculation. Melt veins and melt dikelets emanate from the melt pockets up to 3 mm into the host rock but do not necessarily connect with other melt pockets. The melt pockets were generated by pressure-temperature excursions of 60-80 GPa and 1600-2000 degrees C, resulting in discrete melting of adjacent host rock minerals at grain boundary margins. Concentric zoning in the margins of clinopyroxenes coincides with a progressive reduction in birefringence as melt pockets are approached. This suggests that the shock excursions were focused as point sources in the wake of the shock front that induced bulk damage.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2003.tb00020.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 38, Number 12 (2003)

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