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Fe-Ni metal and sulfide minerals in CM chondrites: An indicator for thermal history

机译:CM球粒陨石中的Fe-Ni金属和硫化物矿物:热历史的指示器

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摘要

CM chondrites were subjected to aqueous alteration and, in some cases, to secondary metamorphic heating. The effects of these processes vary widely, and have mainly been documented in silicate phases. Herein, we report the characteristic features of Fe-Ni metal and sulfide phases in 13 CM and 2 CM-related chondrites to explore the thermal history of these chondrites. The texture and compositional distribution of the metal in CM are different from those in unequilibrated ordinary and CO chondrites, but most have similarities to those in highly primitive chondrites, such as CH, CR, and Acfer 094. We classified the CM samples into three categories based on metal composition and sulfide texture. Fe-Ni metal in category A is kamacite to martensite. Category B is characterized by pyrrhotite grains always containing blebs or lamellae of pentlandite. Opaque mineral assemblages of category C are typically kamacite, Ni-Co-rich metal, and pyrrhotite. These categories are closely related to the degree of secondary heating and are not related to degree of the aqueous alteration. The characteristic features of the opaque minerals can be explained by secondary heating processes after aqueous alteration. Category A CM chondrites are unheated, whereas those in category B experienced small degrees of secondary heating. CMs in category C were subjected to the most severe secondary heating process. Thus, opaque minerals can provide constraints on the thermal history for CM chondrites.
机译:CM球粒陨石发生水蚀,在某些情况下还经历了二次变质加热。这些过程的影响差异很大,并且主要已记录在硅酸盐相中。在这里,我们报告13厘米和2厘米相关的球粒陨石中的铁镍金属和硫化物相的特征,以探索这些球粒的热历史。 CM中金属的质地和组成分布与未平衡的普通和CO球粒陨石不同,但大多数与高度原始的球粒陨石(如CH,CR和Acfer 094)相似。我们将CM样品分为三类基于金属成分和硫化物质地。 A类中的Fe-Ni金属是金刚石到马氏体。 B类的特征是黄铁矿晶粒始终含有辉石的起泡或薄片。 C类的不透明矿物组合物通常是滑石粉,富Ni-Co的金属和黄铁矿。这些类别与二次加热的程度密切相关,与水相变化的程度无关。不透明矿物的特征可以通过水蚀后的二次加热过程来解释。 A类CM球粒陨石未经加热,而B类的球粒经历了较小程度的二次加热。 C类CM经受了最严格的二次加热过程。因此,不透明的矿物会限制CM球粒陨石的热历史。

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