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    The GRO 95577 CR1 chondrite and hydration of the CR parent body

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    Author
    Weisberg, M. K.
    Huber, H.
    Issue Date
    2007-01-01
    Keywords
    aqueous alteration
    Classification
    bulk composition
    CR carbonaceous chondrite meteorites
    
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    Citation
    Weisberg, M. K., & Huber, H. (2007). The GRO 95577 CR1 chondrite and hydration of the CR parent body. Meteoritics & Planetary Science, 42(9), 1495-1503.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656324
    DOI
    10.1111/j.1945-5100.2007.tb00587.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We carried out a petrologic and instrumental neutron activation analysis (INAA) whole chondrite compositional study of Grosvenor Mountains (GRO) 95577. GRO 95577 has many petrological similarities to the CR chondrites. Although the INAA data show patterns indicative of terrestrial weathering, some of the elemental abundances are consistent with a relationship to CR chondrites. The oxygen isotopic composition of GRO 95577 plots close to the Renazzo CR chondrite on the three-isotope diagram. However, GRO 95577 is remarkable in that the chondrules are completely hydrated, consisting almost entirely of phyllosilicates, magnetite, and sulfides. Although GRO 95577 is completely hydrated, the initial chondrule textures are perfectly preserved. The chondrules are in sharp contact with the matrix, their fine-grained rims are clearly visible, and the boundaries of the dark inclusions can be easily discerned. Many chondrules in GRO 95577 have textures suggestive of type I chondrules, but the phenocrysts have undergone perfect pseudomorphic replacement by yellow to brownish serpentine-rich phyllosilicate, with sharp original crystal outlines preserved. The chondrule mesostasis is a green aluminous chlorite-rich material, most likely a hydration product of the feldspathic mesostasis commonly found in anhydrous type I chondrules. Some chondrules contain magnetite spheres, most likely formed by oxidation of metal. We propose that GRO 95577 be classified as a CR1 chondrite, making it the first known CR1 chondrite and expanding the range of alteration conditions on the CR parent body.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2007.tb00587.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 42, Number 9 (2007)

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