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タイトル: | Four-dimensional-STEM analysis of the phyllosilicate-rich matrix of Ryugu samples |
著者: | Mouloud, Bahae-eddine Jacob, Damien de la Peña, Francisco Marinova, Maya Le Guillou, Corentin Viennet, Jean-Christophe Laforet, Sylvain Leroux, Hugues Teurtrie, Adrien Noguchi, Takaaki Matsumoto, Toru Miyake, Akira ![]() ![]() ![]() Igami, Yohei ![]() ![]() ![]() Haruta, Mitsutaka ![]() ![]() ![]() Saito, Hikaru Hata, Satoshi Seto, Yusuke Miyahara, Masaaki Tomioka, Naotaka Ishii, Hope A. Bradley, John P. Ohtaki, Kenta K. Dobrica, Elena Langenhorst, Falko Harries, Dennis Beck, Pierre Phan, Thi H. V. Rebois, Rolando Abreu, Neyda M. Gray, Jennifer Zega, Thomas Zanetta, Pierre-M. Thompson, Michelle S. Stroud, Rhonda Burgess, Kate Cymes, Brittany A. Bridges, John C. Hicks, Leon Lee, Martin R. Daly, Luke Bland, Phil A. Zolensky, Michael E. Frank, David R. Martinez, James Tsuchiyama, Akira Yasutake, Masahiro Matsuno, Junya Okumura, Shota Mitsukawa, Itaru Uesugi, Kentaro Uesugi, Masayuki Takeuchi, Akihisa Sun, Mingqi Enju, Satomi Takigawa, Aki Michikami, Tatsuhiro Nakamura, Tomoki Matsumoto, Megumi Nakauchi, Yusuke Abe, Masanao Nakazawa, Satoru Okada, Tatsuaki Saiki, Takanao Tanaka, Satoshi Terui, Fuyuto Yoshikawa, Makoto Miyazaki, Akiko Nakato, Aiko Nishimura, Masahiro Usui, Tomohiro Yada, Toru Yurimoto, Hisayoshi Nagashima, Kazuhide Kawasaki, Noriyuki Sakamotoa, Naoya Okazaki, Ryuji Yabuta, Hikaru Naraoka, Hiroshi Sakamoto, Kanako Tachibana, Shogo Watanabe, Sei-ichiro Tsuda, Yuichi |
著者名の別形: | 野口, 高明 松本, 徹 三宅, 亮 伊神, 洋平 治田, 充貴 |
発行日: | Aug-2024 |
出版者: | Wiley |
誌名: | Meteoritics & Planetary Science |
巻: | 59 |
号: | 8 |
開始ページ: | 2002 |
終了ページ: | 2022 |
抄録: | Ryugu asteroid grains brought back to the Earth by the Hayabusa2 space mission are pristine samples containing hydrated minerals and organic compounds. Here, we investigate the mineralogy of their phyllosilicate-rich matrix with four-dimensional scanning transmission electron microscopy (4D-STEM). We have identified and mapped the mineral phases at the nanometer scale (serpentine, smectite, pyrrhotite), observed the presence of Ni-bearing pyrrhotite, and identified the serpentine polymorph as lizardite, in agreement with the reported aqueous alteration history of Ryugu. Furthermore, we have mapped the d-spacings of smectite and observed a broad distribution of values, ranging from 1 to 2 nm, with an average d-spacing of 1.24 nm, indicating significant heterogeneity within the sample. Such d-spacing variability could be the result of either the presence of organic matter trapped in the interlayers or the influence of various geochemical conditions at the submicrometer scale, suggestive of a range of organic compounds and/or changes in smectite crystal chemistry. |
著作権等: | © 2024 The Authors. Meteoritics & Planetary Science published by Wiley Periodicals LLC on behalf of The Meteoritical Society. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made. |
URI: | http://hdl.handle.net/2433/293425 |
DOI(出版社版): | 10.1111/maps.14124 |
関連リンク: | https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.14124 |
出現コレクション: | 学術雑誌掲載論文等 |

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