西北非洲13489:强烈变质的未分组碳质球粒陨石

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
T. Cuppone, C. Carli, M. Casalini, A. Stephant, C. R. Greenwood, G. Pratesi
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引用次数: 0

摘要

NWA 13489是一颗被归类为箭纹陨石的陨石。橄榄岩是一种富含橄榄石的原始无球粒陨石,代表了一颗几乎没有分化的非碳质小行星上不同程度的硅酸盐熔融萃取后的残余产物。然而,与该组的其他陨石相比,NWA 13489显示出异常的岩石学和矿物学特征。该样品的岩石学和测温资料与高变质品位的成因相一致。NWA 13489的球粒陨石介于6型和7型之间,其热状态大致跨越FeNi-FeS共晶和硅酸盐熔融的开始,类似于其他被定义为原始无球粒陨石的陨石。矿物化学、大量微量元素地球化学以及氧和铬同位素系统学的证据表明,NWA 13489具有“碳质”成分,因此,它不是一种榴辉岩。更确切地说,NWA 13489与一个未分组的球粒陨石(NWA 11961 C3-ungrouped)和其他未分组的无球粒陨石(配对的NWA 10503/10859)一起,支持了一个独特的类碳陨石群的存在。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Northwest Africa 13489: A Strongly Metamorphosed Ungrouped Carbonaceous Chondrite

Northwest Africa 13489: A Strongly Metamorphosed Ungrouped Carbonaceous Chondrite

NWA 13489 is a meteorite that has been classified as a brachinite. Brachinites are olivine-rich primitive achondrites representing residual products after a variable degree of silicate melt extraction on a barely differentiated, noncarbonaceous asteroid. Nevertheless, NWA 13489 displays petrographic and mineralogical characteristics that are anomalous when compared with other meteorites of that group. The petrography and thermometric data of this sample are compatible with a high metamorphic grade origin. NWA 13489 results in intermediate between type 6 and 7 chondrites, with a thermal regime broadly straddling the FeNi-FeS eutectic and the onset of silicate melting, resembling other meteorites defined as primitive achondrites. Evidence from mineral chemistry, bulk trace element geochemistry, and oxygen and chromium isotope systematics shows a “carbonaceous” composition and, therefore, NWA 13489 is not a brachinite. Rather, together with an ungrouped chondrite (the NWA 11961 C3-ungrouped) and other ungrouped achondrites (the paired NWA 10503/10859), NWA 13489 supports the existence of a distinct carbonaceous-like meteorite grouplet.

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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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