Northwest Africa 1195 Martian Shergottite |
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From the Meteoritical Bulletin #87 June, 2003:
A. and G. Hupe (Hupe) purchased a 50 g fragment of a broken stone with a distinctive, thin weathering rind collected by nomads near Safsaf, Morocco in 2002 March, and subsequently purchased the remainder of the same elongated stone (total weight 315 g). Dimensions of reassembled stone: 133 mm by 43mm by 37 mm. Classification and mineralogy (A. Irving and S. Kuehner, UWS): olivine megacrysts (up to 4 mm) are set in a groundmass of low-Ca pyroxene and maskelynite (Ab37Or0.5 to Ab41Or0.7) with minor Ti-chromite, pyrrhotite, ilmenite and Mg-bearing merrillite. The euhedral to subhedral shapes of most of the olivine grains suggest that they are phenocrysts rather than xenocrysts. Olivine exhibits strong compositional zoning (cores Fa19, FeO/MnO = 54; rims Fa40, FeO/MnO = 62), and contains abundant inclusions of chromite, clinopyroxene, orthopyroxene and pyrrhotite. The groundmass low-Ca pyroxenes are zoned from cores of pigeonite (Wo7Fs26, FeO/MnO = 37.1) or, less commonly, orthopyroxene (Wo4Fs23, FeO/MnO = 37.0) to rims of more Fe-rich pigeonite (Wo12Fs33, FeO/MnO = 36.6). Occurring very rarely on groundmass pyroxene grains are patchy overgrowths of an Fe-rich mineral (possibly related to chamosite or chlorite, with 35 wt.% FeO, 5 wt.% Al2O3, 1.5 wt.% MgO and a low oxide sum of 85 wt.%, suggesting the presence of water or hydroxyl). Calcite occurs sparsely along grain boundaries and as thin veinlets. Texture and mineral compositions are similar to those in olivine-phyric basaltic shergottite DaG 476/670, but olivine is much more magnesian than in other olivine-phyric basaltic shergottites SaU 005/008 and NWA 1068/1110. Specimens: type specimen, 20 g, and two polished thin sections, UWS; main mass, Hupe.
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