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Studies on Uruq al Hadd meteorite

机译:乌鲁克·哈德陨石研究

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Uruq al Hadd (UaH02) meteorite is found in the southwest of Oman close to the border with Yemen. Moessbauer spectroscopy has been used to assess the mineralogy of iron-bearing phases in this meteorite, supported by X-ray diffraction and electron-probe microanalysis (EPMA). Moessbauer spectra measured at 295 and 78 K exhibit paramagnetic doublets superimposed on magnetic sextets. The doublets are assigned to the silicate minerals olivine and pyroxene and the magnetic sextets reveal the presence of at least four magnetic phases: troilite (Fe_(49.2)S_(50.8)), kamacite (Fe_(92.2)Ni_(7.8)), taenite (FeNi), iron oxides and oxy-hydroxides. Both iron oxides and oxy-hydroxides are terrestrial alteration products. Weathering is not pervasive suggesting a relatively young terrestrial age. The mole percentages of fayalite in olivine and ferrosilite in pyroxene determined by EPMA, classifies the meteorite as an H3 chondrite of W1 weathering stage.
机译:Uruq al Hadd(UaH02)陨石位于阿曼西南部,也门边界附近。 Moessbauer光谱学已被用于评估该陨石中含铁相的矿物学,并由X射线衍射和电子探针显微分析(EPMA)支持。在295和78 K下测得的Moessbauer光谱显示出叠加在磁性六重体上的顺磁性双峰。该二重峰归属于硅酸盐矿物橄榄石和辉石,并且磁性六重峰表明存在至少四个磁性相:三叶石(Fe_(49.2)S_(50.8)),钾长石(Fe_(92.2)Ni_(7.8)),钙钛矿(FeNi),氧化铁和羟基氧化物。氧化铁和氢氧化氢氧化物均为陆地蚀变产物。天气并不普遍,表明地球年龄相对年轻。用EPMA测定橄榄石中辉石岩和辉石中的硅铝石的摩尔百分比,将陨石分类为W1风化阶段的H3球粒陨石。

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