Finely layered CM2 carbonaceous chondrites may be analogs for layered boulders on asteroid (101955) Bennu

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Erica R. Jawin, Timothy J. McCOY, Lisette E. Melendez, Catherine M. Corrigan, Kevin Righter, Harold C. Connolly Jr
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Abstract

Orbital observations of Bennu revealed a surface covered in boulders that are most similar among meteorites in our collections to aqueously altered carbonaceous chondrites, and initial analyses of the returned Bennu sample have begun to reveal insights into Bennu's origins. We identified a suite of paired CM2 chondrite meteorites that have a finely layered texture and bear a striking similarity, although at a different scale, to rugged, layered boulders on Bennu. We investigated the nature and potential origin of this layered texture by performing a petrofabric analysis on samples MET 00431, 00434, and 00435. We developed a micro-geospatial mapping framework that is more commonly used for landscape-scale investigations. Our results reveal a pervasive fracture network that exhibits a similar orientation to flattened particles dominated by tochilinite–cronstedtite intergrowths (TCI). We propose that their petrofabrics originated from a low-energy impact on the parent body that occurred after the main period of aqueous alteration halted. The impactdeformed TCI (which formed during earlier aqueous alteration) and generated the fractures. We propose that the sample from Bennu may contain particles with similar layered textures to these meteorites which, if present, would likewise indicate the dominant role of impacts and aqueous alteration on Bennu's parent body.

细层状 CM2 碳质软玉可能是小行星 (101955) 贝努上层状巨石的类似物
对贝努星的轨道观测显示,贝努星表面布满了巨石,在我们收集的陨石中,这些巨石与经水蚀变的碳质软玉最为相似,对返回的贝努星样本进行的初步分析已开始揭示贝努星的起源。我们发现了一组成对的 CM2 ↪LoHan_软玉陨石,它们具有细密的层状纹理,与贝努上崎岖不平的层状巨石有着惊人的相似之处,尽管尺度不同。我们通过对 MET 00431、00434 和 00435 样品进行岩石结构分析,研究了这种层状纹理的性质和潜在来源。我们开发了一个微观地理空间绘图框架,该框架更常用于景观尺度的调查。我们的研究结果表明,普遍存在的断裂网络与以托起石-铁闪长岩互生体(TCI)为主的扁平颗粒具有相似的取向。我们认为,它们的岩石织物源于母体受到的一次低能量撞击,这次撞击发生在水蚀变的主要时期停止之后。撞击使TCI(在早期水蚀变过程中形成)变形,并产生了裂缝。我们认为,来自贝努的样本中可能含有与这些陨石具有类似层状纹理的颗粒,如果这些颗粒存在的话,同样表明撞击和水蚀作用在贝努的母体上发挥了主导作用。
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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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