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    FeO-rich silicates in the Sahara 97159 (EH3) enstatite chondrite: Mineralogy, oxygen isotopic compositions, and origin

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    Author
    Kimura, M.
    Hiyagon, H.
    Lin, Y.
    Weisberg, M. K.
    Issue Date
    2003-01-01
    Keywords
    EH chondrites
    metals
    oxygen isotopes
    pyroxenes
    
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    Citation
    Kimura, M., Hiyagon, H., Lin, Y., & Weisberg, M. K. (2003). FeO‐rich silicates in the Sahara 97159 (EH3) enstatite chondrite: Mineralogy, oxygen isotopic compositions, and origin. Meteoritics & Planetary Science, 38(3), 389-398.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655668
    DOI
    10.1111/j.1945-5100.2003.tb00274.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We report the mineralogy and oxygen isotopic compositions of FeO-rich silicates in the Sahara 97159 EH3 chondrite. This component is referred to as FeO-rich because it contains substantially more FeO than the characteristic FeO-poor silicates in the highly reduced enstatite meteorites. These FeO-rich silicates are mostly low-Ca pyroxene (Fs535) and their compositions suggest an origin under more oxidizing conditions, like those for the ordinary chondrites. However, the mafic silicates in ordinary and carbonaceous chondrites are dominantly olivine, and the FeO-rich silicates in the E chondrites are less commonly olivine. The oxygen isotopic compositions of the FeO- rich silicates are indistinguishable from those of FeO-poor silicates in Sahara 97159. These observations suggest that both the FeO-rich silicates and the FeO-poor silicates in EH chondrites formed from the same oxygen reservoir where redox conditions varied widely.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2003.tb00274.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 38, Number 3 (2003)

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