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The kaidum meteorite: an enstatite aggregate with sulfide-oxide inclusions

机译:凯杜姆陨石:具有硫化物氧化物包裹体的顽辉石聚集体

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An aggregate (approximately 0.5 mm across) examined in the kaidum meteorite is dominated by prismatic crystals of enstatite (Fs_(0.3-2.4), FeO/MnO = 1.9 - 13.6, up to 50 mum long) and contains rare grains of forsterite (Fa_(0.5-0.6, FeO/MnO = 2.4-5.7), which are usually included in enstatie crystals. The interstitial space is filled with calcite a hydrated phase of variable composition. The hydrated phase contains small (< 7 mum) inclusions of sulfide-oxide composition, whose cores consist mostly of Ti and Cr oxides and the rims of Mn and Fe sulfides. The composition and morphology of the enstatite and forsterite suggest that this aggregate is an agglomerate of nebular condensates that was not remelted. The oxide cores of the sulfide-oxide objects are early condensates of the nebula. The sulfide rims were produced during aqueous alterations in the parent body.
机译:在kaidum陨石中检测到的聚集体(约0.5毫米宽)由顽辉石的棱柱晶体(Fs_(0.3-2.4),FeO / MnO = 1.9-13.6,长达50毫米)支配,并且含有罕见的镁橄榄石(Fa_ (0.5-0.6,FeO / MnO = 2.4-5.7),通常包含在固定晶体中。氧化物组成,其核心主要由Ti和Cr氧化物以及Mn和Fe硫化物的边缘组成。硫化物氧化物是星云的早期凝结物,硫化物边缘是在母体的水相变化过程中产生的。

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