最近发现的H球粒陨石Csátalja的冲击诱导变化及其意义

I. Gyollai, Á. Kereszturi, Z. Kereszty, M. Szabó, E. Chatzitheodoridis
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引用次数: 6

摘要

在最近发现的一种名为Csatalja的H球粒陨石中,分析了辉石的冲击驱动退火和橄榄石的冲击变形。确定了冲击退火亚晶粒辉石最具特征的红外光谱形状:最强的峰值出现在860 cm−1处,较小的肩部出现在837−840 cm−1,小的谱带出现在686、635−638和1044−1050 cm−1。辉石中禁带的出现和橄榄石中禁带位置向较低波数的移动清楚地表明了冲击变质作用导致的晶格无序。冲击退火沿裂缝产生混合的深色熔体,由长石-辉石和橄榄石-辉石熔体组成。元素映射检测到,在冲击辉石的亚晶界和沿着辉石断裂的暗冲击熔体的特征是Ca、Na和Al含量相对于其环境升高。到目前为止,还没有用红外光谱研究辉石和橄榄石的冲击变形;这种方法被证明是一种可行的方法。。。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Shock-induced alterations in the recently found H chondrite Csátalja meteorite and its implications
Shock-driven annealing of pyroxene and shock deformation of olivine were analyzed in a recently found H chondrite called Csatalja. The most characteristic infrared (IR) spectral shape of shock-annealed sub-grained pyroxene was identified: the strongest peak occurs at 860 cm−1 with a smaller shoulder at 837−840 cm−1, and small bands are at 686, 635−638, and 1,044−1,050 cm−1. The appearance of forbidden bands in pyroxene and shift of band positions to a lower wave number in olivines clearly demonstrate the crystal lattice disordering due to shock metamorphism. The shock annealing produced mixed dark melt along fractures, which consists of feldspar−pyroxene and olivine−pyroxene melt. The dark shock melt at sub-grain boundaries of shocked pyroxenes and along fracture of pyroxenes is characterized by elevated Ca, Na, and Al content relative to its environment, detected by element mapping. So far, shock deformation of pyroxene and olivine was not studied by IR spectroscopy; this method has turned out to be a po...
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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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