Multiple CV chondrite lithologies in Camel Donga 003 (CK3): Implications for the CV and CK parent bodies

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Elana G. Alevy, Tasha L. Dunn, Alexander N. Krot, Paul Cardon-Pilotaz, Juliane Gross
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引用次数: 0

Abstract

Camel Donga 003 (CD 003) was originally classified as a CK3 chondrite based on its coarse-grained matrix, Ni-rich sulfides, Cr-rich magnetite, and CK-like silicate mineralogy. However, after preliminary backscattered electron imaging and elemental mapping of a 400 mm2 thin section of CD 003, subsequent mineral chemistry analysis confirmed that the sample is a fragmental breccia consisting of three oxidized CV lithologies. In the two largest lithologies, both mineralogically pristine and metasomatically altered refractory inclusions are commonly found in close proximity to one another. This suggests that brecciation and mixing of different lithologies in CD 003 occurred on a submillimeter scale. The least abundant lithology—an 8 × 3 mm clast—is distinguished from the other lithologies by its recrystallized matrix, poorly defined chondrules, and equilibrated olivine (Fa42). The homogeneity of matrix and chondrule olivine indicates that this lithology has been metamorphosed to at least petrologic subtype 3.8 conditions. We can trace the provenance of our sample to the main mass of CD 003, which must contain the CK material described in its original classification. Therefore, the presence of the three oxidized CV lithologies suggests that CD 003 is the first CV/CK3 chondrite breccia.

骆驼东亚003 (CK3)中多个CV球粒陨石岩性:对CV和CK母体的影响
骆驼东亚003 (CD 003)最初被归类为CK3球粒陨石,基于其粗粒基质、富镍硫化物、富cr磁铁矿和类ck硅酸盐矿物学特征。然而,在对CD 003的400mm2薄片进行初步背散射电子成像和元素定位后,随后的矿物化学分析证实该样品是一个由三种氧化CV岩性组成的破碎角砾岩。在两个最大的岩性中,矿物学上原始的和交代蚀变的难熔包裹体通常彼此靠近。这表明cd003的角化作用和不同岩性的混合作用发生在亚毫米尺度上。最不丰富的岩性——一个8 × 3毫米的碎屑——与其他岩性的区别在于它的再结晶基质、不明确的球粒和平衡的橄榄石(Fa42)。基质和球粒橄榄石的均匀性表明该岩性已变质至至少岩石学3.8亚型条件。我们的样品的来源可以追溯到CD 003的主质量,它必须包含其原始分类中描述的CK物质。因此,三个氧化CV岩性的存在表明cd003是第一个CV/CK3球粒陨石角砾岩。
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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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