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    Matching Martian crustal magnetization and magnetic properties of Martian meteorites

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    Author
    Rochette, P.
    Gattacceca, J.
    Chevrier, V.
    Hoffmann, V.
    Lorand, J. P.
    Funaki, M.
    Hochleitner, R.
    Issue Date
    2005-01-01
    Keywords
    Pyrrhotite
    Mars
    Martian meteorites
    magnetite
    
    Metadata
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    Citation
    Rochette, P., Gattacceca, J., Chevrier, V., Hoffmann, V., Lorand, J.-P., Funaki, M., & Hochleitner, R. (2005). Matching Martian crustal magnetization and magnetic properties of Martian meteorites. Meteoritics & Planetary Science, 40(4), 529-540.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655986
    DOI
    10.1111/j.1945-5100.2005.tb00961.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Magnetic properties of 26 (of 32) unpaired Martian meteorites (SNCs) are synthesized to further constrain the lithology carrying Martian magnetic crustal sources. Magnetic properties of ultramafic cumulates (i.e., Chassigny, Allan Hills [ALH] 84001) and lherzolitic shergottites (ALH 77005, Lewis Cliff [LEW] 88516) are one or two orders of magnitude too weak to account for the crustal magnetizations, assuming magnetization in an Earth-like field. Nakhlites and some basaltic shergottites, which are the most magnetic SNCs, show the right intensity. Titanomagnetite is the magnetic carrier in the nakhlites (7 meteorites), whereas in most basaltic shergottites (11 meteorites) it is pyrrhotite. Dhofar (Dho) 378, Los Angeles, and NWA 480/1460 and 2046 are anomalous basaltic shergottites, as their magnetism is mainly due to titanomagnetite. Pyrrhotite should be among the candidate minerals for the magnetized Noachian crust.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00961.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 40, Number 4 (2005)

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