卡巴陨石中的粘土矿物和其他含水蚀变产物:文献综述和新的XRD研究

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
István Viczián, F. Kristály
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引用次数: 0

摘要

摘要本研究综述了关于卡巴陨石矿物学、粘土矿物、含水相和有机物的特殊方面的出版物。在第1节中,提到了陨石坠落和发现的历史以及1961年的第一次经典矿物学描述。原生硅酸盐和玻璃质基质最常见的蚀变产物是含铁皂石。通过模拟阿连德型陨石的热液蚀变,可以生产人造皂石。热力学研究证明了硅酸盐和磁铁矿在低温下(大多低于100°C)含水新生的可能性。用电子探针显微分析和扫描电子显微镜阴极发光方法证明了镁橄榄石晶粒在水热作用下形成富铁外缘。CV3碳质球粒陨石中的叶片表明卡巴陨石来源于母体的外部浅区。X射线功率衍射(XRD)和穆斯堡尔谱的结合使包括卡巴在内的CV3球粒陨石的精确模态分析成为可能。通过原位测定稳定氧同位素含量来研究蚀变可能会对CV母小行星上的水性流体的氧同位素组成提供限制。利用拉曼光谱测定了有机物的热变质程度。证明了芳香烃和脂肪族、饱和烃和不饱和烃以及各种氨基酸的存在。非生物成因的可能性更大;然而,一些结构和矿物学观察结果也可能表明有机物的生物成因。除了对上述文献的回顾外,作为附录,作者的新XRD研究报告显示,陨石薄片中存在类似蒙脱石的相。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Clay minerals and other hydrous alteration products in the Kaba meteorite: Review of the literature and new XRD investigations
Abstract The present study is a review of publications regarding special aspects of the mineralogy of the Kaba meteorite, clay minerals, hydrous phases, and organic matter. In Section 1, the history of fall and finding of the meteorite and the first classical mineralogical description in the Year 1961 are mentioned. The most frequent alteration product of primary silicates and the glassy matrix is Fe-bearing saponite. By modelling of hydrothermal alteration of Allende-type meteorites, artificial saponite could be produced. The thermodynamic study proved the possibility of hydrous neoformation of silicates and magnetite at low temperatures, mostly below 100°C. The formation of Fe-rich external rims in forsterite grains by hydrothermal action was demonstrated by electron probe microanalysis and scanning electron microscopy-cathodo-luminescence methods. Foliation in CV3 carbonaceous chondrites indicates that the Kaba meteorite is derived from the external, shallow zone of the parent body. A combination of X-ray power diffraction (XRD) and Mössbauer spectroscopy made the exact modal analysis of CV3 chondrites possible, including Kaba. The study of alteration by in situ determination of stable oxygen isotope contents may provide constraints regarding the oxygen isotopic composition of the aqueous fluid on the CV parent asteroid. The degree of thermal metamorphism of the organic matter was determined by using Raman spectroscopy. The presence of aromatic and aliphatic, saturated and unsaturated hydrocarbons, and various amino acids was demonstrated. The non-biogenic origin is more probable; however, there are textural and mineralogical observations that may indicate also the biogenic origin of organic matter. In addition to the review of the literature above, as an appendix, shortly new XRD investigations of the authors are reported that indicated smectite-like phases in a thin section made of the meteorite.
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来源期刊
Open Astronomy
Open Astronomy Physics and Astronomy-Astronomy and Astrophysics
CiteScore
1.30
自引率
14.30%
发文量
37
审稿时长
16 weeks
期刊介绍: The journal disseminates research in both observational and theoretical astronomy, astrophysics, solar physics, cosmology, galactic and extragalactic astronomy, high energy particles physics, planetary science, space science and astronomy-related astrobiology, presenting as well the surveys dedicated to astronomical history and education.
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