Methylene-to-methyl ratio variability in Ryugu samples: Clues to a heterogeneous aqueous alteration

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Zélia Dionnet, Zahia Djouadi, Lukas Delaye, Lucas Caron, Rosario Brunetto, Alice Aléon-Toppani, Cateline Lantz, Stefano Rubino, Donia Baklouti, Tomoki Nakamura, Ferenc Borondics, Christophe Sandt, Megumi Matsumoto, Kana Amano, Tomoyo Morita, Hisayoshi Yurimoto, Takaaki Noguchi, Ryuji Okazaki, Hikaru Yabuta, Hiroshi Naraoka, Kanako Sakamoto, Shogo Tachibana, Toru Yada, Masahiro Nishimura, Aiko Nakato, Akiko Miyazaki, Kasumi Yogata, Masanao Abe, Tatsuaki Okada, Tomohiro Usui, Makoto Yoshikawa, Takanao Saiki, Satoshi Tanaka, Fuyuto Terui, Satoru Nakazawa, Seiichiro Watanabe, Yuichi Tsuda, the Hayabusa2-initial-analysis Stone team
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Abstract

Understanding the processes of aqueous alteration within primitive bodies is crucial for unraveling the complex history of early planetesimals. To better identify the signs of this process and its consequences, we have studied the heterogeneity at a micrometric scale of the structure of the aliphatic organic compounds and its relationship to its mineralogical environment. Here, we report an analysis performed on two micrometric grains of Ryugu (C0002-FC027 and C0002-FC028). The samples were crushed in a diamond compression cell and analyzed using high-spatial resolution Fourier Transform InfraRed (FT-IR) hyperspectral imaging measurements conducted in transmission mode. We showed here the spatial distributions of the main components and the structural heterogeneity of the aliphatic organic matter highlighting a micrometer-scale variability in the methylene-to-methyl ratio. Moreover, we connected this heterogeneity to the one of the phyllosilicate band positions. Our findings indicate that the organic matter within Ryugu's micrometric grains underwent varying degrees of aqueous alteration in distinct microenvironments resulting in an elongation of the length of their aliphatic chains, and/or a reduction in their branching and/or cross-linking.

琉球样品中亚甲基比变异性:非均质水蚀变的线索
了解原始体中含水蚀变过程对于揭示早期星子的复杂历史至关重要。为了更好地识别这一过程的标志及其后果,我们在微观尺度上研究了脂肪族有机化合物结构的非均质性及其与矿物环境的关系。在这里,我们报告了对Ryugu (C0002-FC027和C0002-FC028)两个微米颗粒的分析。样品在金刚石压缩箱中被压碎,并在透射模式下使用高空间分辨率傅里叶变换红外(FT-IR)高光谱成像测量进行分析。我们在这里展示了主要成分的空间分布和脂肪族有机质的结构异质性,突出了亚甲基比在微米尺度上的变异性。此外,我们将这种非均质性与层状硅酸盐带的一个位置联系起来。我们的研究结果表明,在不同的微环境中,琉球微颗粒中的有机物经历了不同程度的水蚀,导致它们的脂肪链长度延长,和/或它们的分支和/或交联减少。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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