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    New findings for the equilibrated enstatite chondrite Grein 002

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    Author
    Patzer, A.
    Schlüter, J.
    Schultz, L.
    Tarkian, M.
    Hill, D. H.
    Boynton, W. V.
    Issue Date
    2004-01-01
    Keywords
    EL chondrites
    noble gases
    Instrumental neutron activation analysis
    enstatite chondrites
    
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    Citation
    Patzer, A., Schlüter, J., Schultz, L., Tarkian, M., Hill, D. H., & Boynton, W. V. (2004). New findings for the equilibrated enstatite chondrite Grein 002. Meteoritics & Planetary Science, 39(9), 1555-1575.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655903
    DOI
    10.1111/j.1945-5100.2004.tb00127.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We report new petrographic and chemical data for the equilibrated EL chondrite Grein 002, including the occurrence of osbornite, metallic copper, abundant taenite, and abundant diopside. As inferred from low Si concentrations in kamacite, the presence of ferroan alabandite, textural deformation, chemical equilibration of mafic silicates, and a subsolar noble gas component, we concur with Grein 002s previous classification as an EL45 chondrite. Furthermore, the existence of pockets consisting of relatively coarse, euhedral enstatite crystals protruding large patches of Fe-Ni alloys suggests to us that this EL45 chondrite has been locally melted. We suspect impact induced shock to have triggered the formation of the melt pockets. Mineralogical evidence indicates that the localized melting of metal and adjacent enstatite must have happened relatively late in the meteorites history. The deformation of chondrules, equilibration of mafic silicates, and generation of normal zoning in Fe, Zn-sulfides took place during thermal alteration before the melting event. Following parent body metamorphism, daubreelite was exsolved from troilite in response to a period of slow cooling at subsolidus temperatures. Exsolution of schreibersite from the coarse metal patches probably occurred during a similar period of slow cooling subsequent to the event that induced the formation of the melt pockets. Overall shock features other than localized melting correspond to stage S2 and were likely established by the final impact that excavated the Grein 002 meteoroid.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2004.tb00127.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 39, Number 9 (2004)

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