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Mineralogy of lunar meteorites, Yamato-82192 and -82193 with reference to breccias in a breccia

机译:月球陨石的矿物学,Yamato-82192和-82193,涉及角砾岩中的角砾岩

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摘要

The mineralogy of pyroxene, olivine and plagioclase fragments, lithic clasts and glassy matrices of lunar meteorites, Yamato-82192 (Y-82192) and Yamato-82193 (Y-82193), has been studied by an electron microprobe and an analytical transmission electron microscope (TEM). The distribution of the chemical compositions of pyroxene grains in Y-82192 and -82193 bears a strong resemblance to one another and covers almost all known pyroxenes in nonmare pristine rocks. They are similar to those of a lunar regolith breccia 60019,but appear to be different from Y-791197 and ALHA81005 in that Y-82 lunar meteorites have significantly fewer pyroxenes with extremely high Fe content. The difference implies that Y-82192 and -82193 may contain a fewer Fe-rich mare basalt components. The presence of a breccia in a breccia in Y-82192 indicates complex impact histories in the region where this meteorite was derived. The texture of the matrix glass of Y-82192 in the TEM scale is different from that of ALHA81005.
机译:已通过电子探针和分析型透射电子显微镜研究了辉石,橄榄石和斜长石碎片,月球陨石的岩屑和玻璃状基质Yamato-82192(Y-82192)和Yamato-82193(Y-82193)的矿物学(TEM)。 Y-82192和-82193中辉石颗粒的化学成分分布彼此非常相似,并且覆盖了非母质原始岩石中几乎所有已知的辉石。它们类似于月球角砾岩角砾岩60019,但似乎与Y-791197和ALHA81005不同,因为Y-82月球陨石中的辉石明显少得多,而且铁含量极高。不同之处在于,Y-82192和-82193可能含有较少的富铁母玄武岩成分。 Y-82192的角砾岩中有角砾岩的存在,表明该陨石的衍生区域存在复杂的撞击历史。 Y-82192的基体玻璃的TEM尺度纹理不同于ALHA81005。

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