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    TEM investigations on the monomict ureilites Jalanash and Hammadah al Hamra 064

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    Author
    Weber, I.
    Bischoff, A.
    Weber, D.
    Issue Date
    2003-01-01
    Keywords
    electron microscopy
    shock metamorphism
    impact microcraters
    cometary grains
    
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    Citation
    Weber, I., Bischoff, A., & Weber, D. (2003). TEM investigations on the monomict ureilites Jalanash and Hammadah al Hamra 064. Meteoritics & Planetary Science, 38(1), 145-156.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656675
    DOI
    10.1111/j.1945-5100.2003.tb01051.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We studied the petrography and mineralogy of two monomict ureilites, Hammadah al Hamra 064 (HH064) and Jalanash, by using reflected light and scanning electron microscopy. Quantitative analyses were performed by electron microprobe and the microstructures were investigated with transmission electron microscopy (TEM). HH064 features two different textures, a poikilitic and a typical one, whereas Jalanash shows only the typical ureilite texture. Our synergetic chemical and microstructural investigations reveal a complex cooling history for both ureilites. The temperature for the first equilibrium deduced from the pigeonite-augite assemblage in HH064 is ~1200 degrees C. The presence of antiphase domains in low-Ca pyroxenes proves that they are clearly pigeonite. The occurrences of tweed microstructure and orthopyroxene lamellae, which are incompletely developed, imply a faster cooling rate from the first equilibrium with a sudden end. Although both ureilites contain shock induced diamonds, dislocations in silicates are rare. This observation suggests that the meteorites were hot at the time of strong shock metamorphism or that they were heated after strong shock metamorphism. After this event, new microstructural features were generated by different cooling processes and were frozen by a final rapid decrease in temperature possibly due to excavation from the ureilite parent body, or bodies.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2003.tb01051.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 38, Number 1 (2003)

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