Campo del Cielo悬崖岩的振膜结构表明了一个由陆地碰撞引起的中等冲击过程

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Laura Noel García, Péter Némenth, Ronan Henry, Robert Luther, Maria Eugenia Varela
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引用次数: 0

摘要

克利夫顿石是石墨的多晶聚集体,具有不寻常的长方体形态,是某些铁陨石的重要碳成分。虽然它们主要由sp2键碳组成,但最近的研究表明,来自迪亚布罗峡谷(IAB)陨石的那些也包括复合的sp2-和sp3键结构,称为晶片。在这里,我们研究了Campo del Cielo样品中的cliftonites的纳米结构,并证明这些cliftonites还包含有序的3R石墨区域与1型晶片结构的纳米复合混合物,由<; 01-10>;投影石墨和<;011>;投影金刚石结构组成。这一发现表明,Campo del Cielo陨石的某些碎片经历了中等的冲击压力(>~10 GPa),超过了先前报道的主要陨石的4-10 GPa压力范围。我们认为Campo del Cielo的一部分悬崖岩为陆地撞击过程中石墨的冲击诱导钻石化和“抛射斩首”过程提供了证据。最初碳质物质的复杂性,加上在陆地撞击事件中遇到的大范围压力,可能解释了Campo del Cielo和Diablo峡谷悬崖岩中纳米结构的多样性。我们的发现可以帮助开发一种压力/冲击分类系统,用于表征含石墨陨石的撞击事件。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Diaphite structures of Campo del Cielo cliftonites indicate a terrestrial collision-induced moderate shock process

Cliftonites, polycrystalline aggregates of graphite with unusual cuboid morphology, are important carbon components of certain iron meteorites. Although they consist predominantly of sp2-bonded carbon, recent studies suggest that those from the Canyon Diablo (IAB) meteorite also include composite sp2- and sp3-bonded structures, named diaphites. Here, we investigate the nanostructure of cliftonites in a Campo del Cielo specimen and demonstrate that these cliftonites also contain a nanocomposite mixture of well-ordered 3R graphite regions interfingered with type 1 diaphite structure, consisting of <01–10> projected graphite and <011> projected diamond domains. This finding suggests that certain pieces of the Campo del Cielo meteorite experienced moderate shock pressures (>~10 GPa), which exceed the 4–10 GPa pressure range previously reported for the main meteorite. We propose that a portion of Campo del Cielo cliftonites provides evidence for the shock-induced diamondization of graphite and the “projectile decapitation” process during terrestrial impact. The complexity of the initial carbonaceous material, combined with the wide range of pressures encountered during terrestrial impact events, may explain the diversity of nanostructures in the Campo del Cielo and Canyon Diablo cliftonites. Our findings could assist in the development of a pressure/shock classification system for characterizing impact events in graphite-bearing meteorites.

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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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