• Title of article

    A new Martian meteorite from Morocco: the nakhlite North West Africa 817

  • Author/Authors

    Sautter، نويسنده , , V and Barrat، نويسنده , , J.A and Jambon، نويسنده , , A and Lorand، نويسنده , , J.P and Gillet، نويسنده , , Ph and Javoy، نويسنده , , M and Joron، نويسنده , , J.L and Lesourd، نويسنده , , M، نويسنده ,

  • Issue Information
    روزنامه با شماره پیاپی سال 2002
  • Pages
    16
  • From page
    223
  • To page
    238
  • Abstract
    North West Africa (NWA 817) is a single stone of 104 g found in the Sahara (Morocco) by meteorite hunters in November 2000. The meteorite is an unbrecciated, medium-grained olivine-bearing clinopyroxenite with a cumulate texture. It consists of zoned euhedral subcalcic augite (Wo42En38–22Fs20–36), olivine spanning a wide range of compositions (from Fa56 in the core to Fa86) with rare magmatic inclusions and an intercumulus mesostasis made of Fe-bearing albitic plagioclase, Si-rich glass, Ti-magnetite with unusual skeletal growth morphologies containing ilmenite exsolutions, acicular pyroxene, olivine and cristobalite. Trace minerals are sulfide droplets and Cl-apatite. Mineral modes (in vol%) are augite 69%, olivine 10%, mesostasis 20% and Fe–Ti oxides 1%. Pervasive alteration produced a reddish clay mineral (hydrous ferrous silicate) in both olivine crystals and the mesostasis. The major element composition of NWA 817 is very similar to that of the other nakhlites: high FeO, MgO and CaO concentrations reflect the abundance of cumulus augite and olivine. Key element ratios such as FeO/MnO (=37), Na/Al (=0.40), K/La (=449), Ga/Al (=3.9×10−4) and oxygen isotopic composition (Δ17O=+0.37‰) are clear evidence for a Martian origin. The incompatible trace element pattern as in Nakhla displays a strong light rare earth element enrichment relative to chondrite (Lan/Ybn=4.89). However, when compared to the other nakhlites, NWA 817 has specific features: (1) a higher modal proportion of mesostasis; (2) quench textures of Ti-magnetite and Fe-rich clinopyroxene; (3) more Mg-rich olivine core compositions whereas the augite core composition is identical for all nakhlites; (4) a stronger Fe enrichment toward crystal rims of these cumulus minerals. The intercumulus minerals (Ti-magnetite with skeletal growth morphology, acicular chains of clinopyroxene and Fe3+-rich feldspar) indicate rapid crystallization in response to a high degree of undercooling at the end of the sample story.
  • Keywords
    alteration , skeletal titanomagnetite , nakhlite , SNC meteorites
  • Journal title
    Earth and Planetary Science Letters
  • Serial Year
    2002
  • Journal title
    Earth and Planetary Science Letters
  • Record number

    2322237