The petrology of the Ozerki meteorite constrained by electron backscatter diffraction and X-ray computed tomography

IF 2.4 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Alice Macente, Luke Daly, Sammy Griffin, Maria Gritsevich, Jarmo Moilanen, Josh Franz Einsle, Patrick Trimby, Chris Mulcahy, Jonathan Moffat, Alexander M. Ruzicka
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Abstract

Combining electron backscatter diffraction (EBSD) with X-ray computed tomography (XCT) offers a comprehensive approach to investigate shock deformation and rock texture in meteorites, yet such integration remains uncommon. In this study, we demonstrate the synergistic potential of XCT and EBSD in revealing deformation metrics, thereby enhancing our understanding of petrofabric strength and shock-induced deformation. Our analysis focuses on the Ozerki (L6, S4/5, W0) meteorite fall, which was instrumentally observed on June 21, 2018, and subsequently recovered by the Ural's branch of the Russian Fireball Network (UrFU) recovery expedition a few days later. The trajectory analysis conducted by the Finnish Fireball Network facilitated the prompt retrieval of the meteorite. We show that Ozerki is deformed, with a moderate strength foliation fabric defined by metal and sulfide grain shapes. Microstructural analysis using EBSD shows that the parent body was likely still thermally active during this impact event. Our data suggest that these microstructures were likely produced during an impact while the Ozerki's parent body was still warm.

Abstract Image

电子后向散射衍射和x射线计算机断层扫描约束了Ozerki陨石的岩石学
电子背散射衍射(EBSD)和x射线计算机断层扫描(XCT)的结合为研究陨石中的冲击变形和岩石纹理提供了全面的方法,但这种结合仍然很少见。在这项研究中,我们展示了XCT和EBSD在揭示变形指标方面的协同潜力,从而增强了我们对岩石组构强度和冲击诱发变形的理解。我们的分析重点是Ozerki (L6, S4/5, W0)陨石坠落,该陨石于2018年6月21日被仪器观测到,几天后由俄罗斯火球网络(UrFU)恢复探险队的乌拉尔分支恢复。芬兰火球网络进行的轨迹分析促进了陨石的迅速回收。我们发现Ozerki是变形的,具有中等强度的叶理结构,由金属和硫化物晶粒形状定义。利用EBSD进行的微观结构分析表明,在这次撞击事件中,母体可能仍处于热活动状态。我们的数据表明,这些微观结构很可能是在撞击期间产生的,而奥泽基的母体还很温暖。
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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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