通过光学显微镜和BSE成像揭示Mócs陨石(L6)热变质作用

I. Gyollai, S. Bérczi, K. Fintor, S. Nagy, A. Gucsik
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引用次数: 1

摘要

为了更好地了解Mocs球粒陨石的热变质、冲击后退火演化和矿物学特征,对其进行了光学显微镜、元素测绘和扫描电镜(SEM-BSE)成像研究。所研究的Mocs陨石薄片包含26个具有多种球粒结构的球粒,其特征是边缘模糊。球粒主要由辉石和橄榄石组成,而长石只存在于重结晶的地质体、球粒介稳态和激波脉内外的矿物熔体中。结果表明,基体完全再结晶。根据上述扫描电镜和光学显微镜观察,可以得出Mocs球粒陨石为6.5级岩相类型。
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Thermal metamorphism of the Mócs meteorite (L6) revealed by optical microscopy and BSE imaging
The Mocs chondrite was studied by optical microscopy, element mapping, as well as scanning electron microscope backscattered electron (SEM—BSE) imaging, in order to gain a better understanding of the thermal metamorphic as well as post-shock annealing evolution and the mineralogical signatures in this meteorite. The studied thin section of Mocs meteorite contains 26 chondrules with a variety of chondrule textures, which are characterized by a blurry rim. The chondrules mostly consist of pyroxene and olivine, whereas feldspars occur only in the recrystallized groundmass, chondrule mesostasis, and mineral melt inside and beyond the shock veins. It was found that the matrix was completely recrystallized. According to the scanning electron microscope and optical microscope observations mentioned above, it can be concluded that the Mocs chondrite is a 6.5 petrographic type.
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来源期刊
Central European Geology
Central European Geology Earth and Planetary Sciences-Geology
CiteScore
1.40
自引率
0.00%
发文量
8
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