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首页> 外文期刊>Meteoritics & planetary science >Sulfide petrology of four nakhlites: Northwest Africa 817, Northwest Africa 998, Nakhla, and Governador Valadares
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Sulfide petrology of four nakhlites: Northwest Africa 817, Northwest Africa 998, Nakhla, and Governador Valadares

机译:四个纳赫石的硫化物岩石学:西北非洲817,西北非洲998,纳赫拉和瓦拉达雷斯总督

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The nakhlites contain small proportions of Cu-Fe-Ni sulfide minerals; we have studied these sulfides in Northwest Africa (NWA) 998, Nakhla, Governador Valadares, and NWA 817 with optical microscopy, scanning electron microscope, and electron microprobe. Modal abundances of magmatic sulfides, as estimated by image analysis on thin section, are uniformly low (0.02 to 0.05±0.03vol%), i.e., a factor 5 lower than in shergottites. Sulfides occur within the glassy mesostasis, as composite two-phase Fe-Ti oxide-sulfide grains, intimately associated with interstitial grains or locally enclosed in postcumulus melt inclusions (e.g., Governador Valadares) in olivine. They exhibit a uniform low-Ni monoclinic pyrrhotite composition±chalcopyrite. There is a gradation of sulfide grain sizes and textures across the nakhlites flow(s): droplets in NWA 817; resorbed blebs in Governador Valadares; more massive, true intercumulus blebs in Nakhla and NWA 998. These nakhlites also show evidence for sulfide weathering. Hot desert finds (e.g., NWA 998 and NWA 817) show a few percent fracture-filling iron (oxy) hydroxides of likely terrestrial origin. Original sulfides are 50% altered in our NWA 998 section, with iron (oxy) hydroxides at grain boundaries and as complete pseudomorphs. The compositions of unaltered pyrrhotites are homogeneous, close to that of the monoclinic endmember Fe_7S_8, and are too sulfur-rich to have been in chemical equilibrium with the late magmatic redox state fixed by the fayalite-magnetite-quartz buffer. Therefore, the compositions of the pyrrhotites must have been altered during the later stages of magmatic crystallization, by assimilation of S-rich regolith and hydrothermal circulation.
机译:nakhlites含有少量的Cu-Fe-Ni硫化物矿物。我们已经使用光学显微镜,扫描电子显微镜和电子探针在西北非洲(NWA)998,纳赫拉(Nakhla),加拉弗多拉(Governador Valadares)和NWA 817中研究了这些硫化物。通过薄层图像分析估计的岩浆硫化物的模态丰度始终较低(0.02至0.05±0.03vol%),即比斜方锰矿低5倍。硫化物发生在玻璃状的介晶内,是复合的两相Fe-Ti氧化物-硫化物晶粒,与间质晶粒紧密相关,或局部封闭在橄榄石中的积云后的熔融包裹体中(例如Governador Valadares)。它们表现出均匀的低镍单斜硫铁矿组成±黄铜矿。在整个nakhlites流中,硫化物的粒度和织构有一定的等级:NWA 817中的液滴;在瓦拉达雷斯总督中吸收了气泡;在纳赫拉(Nakhla)和西澳大利亚州998(NWA 998)上出现了更大的真正的积云小气泡。炎热的沙漠发现(例如NWA 998和NWA 817)显示出可能是地面起源的百分之几的裂缝填充铁(氧)氢氧化物。在我们的NWA 998部分中原始硫化物发生了50%的变化,在晶界处形成了氢氧化铁(氧),并形成了完整的假晶。未改变的黄铁矿的组成是均质的,接近于单斜端元Fe_7S_8的组成,并且硫含量太高,以致于未与铁橄榄石-磁铁矿-石英缓冲液固定的晚期岩浆氧化还原态达到化学平衡。因此,磁黄铁矿的组成必须在岩浆结晶的后期通过同化富S的角砾岩和水热循环而改变。

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