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    Northwest Africa 1950: Mineralogy and comparison with Antarctic lherzolitic shergottites

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    Author
    Mikouchi, Takashi
    Issue Date
    2005-01-01
    Keywords
    Martian meteorites
    Antarctic meteorites
    shergottite meteorites
    crystallization
    Northwest Africa (NWA) 1950
    
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    Citation
    Mikouchi, T. (2005). Northwest Africa 1950: Mineralogy and comparison with Antarctic lherzolitic shergottites. Meteoritics & Planetary Science, 40(11), 1621-1634.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656065
    DOI
    10.1111/j.1945-5100.2005.tb00135.x
    Additional Links
    https://meteoritical.org/
    Abstract
    NWA 1950 is a new lherzolitic shergottite recently recovered from Morocco and is the first sample of this group found outside Antarctica. Major constituent phases of NWA 1950 are olivine, pyroxenes, and plagioclase glass ("maskelynite") and the rock shows a two distinct textures: poikilitic and non-poikilitic typical of lherzolitic shergottites. In poikilitic areas, several-millimeter-sized pyroxene oikocrysts enclose cumulus olivine and chromite. In contrast, pyroxenes are much smaller in non-poikilitic areas, and olivine and plagioclase glass are more abundant. Olivine in non-poikilitic areas is more Fe-rich (Fa29-31) and shows a narrower distribution than that in poikilitic areas (Fa23-29). Pyroxenes in non-poikilitic areas are also more Fe-rich than those in poikilitic areas that show continuous chemical zoning suggesting fractional crystallization under a closed system. These observations indicate that pyroxene in non-poikilitic areas crystallized from evolved interstitial melts and olivine was re-equilibrated with such melts. NWA 1950 shows similar mineralogy and petrology to previously known lherzolitic shergottites (ALH 77005, LEW 88516, Y-793605 and GRV 99027) that are considered to have originated from the same igneous body on Mars. Olivine composition of NWA 1950 is intermediate between those of ALH 77005-GRV 99027 and those of LEW 88516-Y-793605, but is rather similar to ALH 77005 and GRV 99027. The subtle difference of mineral chemistry (especially, olivine composition) can be explained by different degrees of re-equilibration compared to other lherzolitic shergottites, perhaps due to different location in the same igneous body. Thus, NWA 1950 experienced a high degree of re-equilibration, similar to ALH 77005 and GRV 99027.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2005.tb00135.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 40, Number 11 (2005)

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