Phyllosilicates with embedded Fe‐based nanophases in Ryugu and Orgueil
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Comparison Ryugu-Orgueil nanom ...
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Final Accepted Manuscript
Author
Leroux, HuguesLe Guillou, Corentin
Marinova, Maya
Laforet, Sylvain
Viennet, Jean‐Christophe
Mouloud, Bahae‐Eddine
Teurtrie, Adrien
de la Peña, Francisco
Jacob, Damien
Hallatt, Daniel
Fernandez, Mario Pelaez
Troadec, David
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.
Dobrică, 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
Affiliation
Department of Planetary Sciences, Lunar and Planetary Laboratory, The University of ArizonaIssue Date
2023-11-14
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WileyCitation
Leroux, H., Le Guillou, C., Marinova, M., Laforet, S., Viennet, J. C., Mouloud, B. E., ... & Tsuda, Y. (2023). Phyllosilicates with embedded Fe‐based nanophases in Ryugu and Orgueil. Meteoritics & Planetary Science.Rights
© 2023 The Meteoritical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Samples were recently collected from the carbonaceous asteroid (162173) Ryugu, by the Japan Aerospace Exploration Agency (JAXA) Hayabusa2 mission. They resemble CI chondrites material, thus showing clear evidence of extensive aqueous alteration attested by the widespread presence of a mixture of serpentine and saponite. We present here a scanning transmission electron microscopy study of the Ryugu dominant lithology of the phyllosilicate matrix at the nanometer scale, which we compare with that of the Orgueil CI chondrite. In both objects, the phyllosilicates are of comparable nature and texture, consisting of a mixture of small-sized crystallites of serpentine and saponite. At the micrometer scale or less, the texture is an alternation of fine and coarse domains. The fine-grained regions are dominated by saponite. In Ryugu, they enclose numerous Fe,Ni nanosulfides, whereas in Orgueil, S- and Ni-rich ferrihydrite is abundant. The coarse-grained regions contain more serpentine and no or little Fe,Ni sulfides or ferrihydrite. Scanning transmission x-ray microscopy at the Fe-L3 edge also reveals that iron valency of phyllosilicates is higher and more homogeneous in Orgueil (~70% Fe3+) than in Ryugu (<50% Fe3+). We interpret the observed textures as being mostly a consequence of aqueous alteration, likely resulting from the replacement by phyllosilicates of submicrometric components, initially agglomerated by a primary accretion. The fine-grained domains may result from the replacement of GEMS (GEMS—glass with embedded metal and sulfides) objects or from other types of nanometric assemblages of silicate and Fe-based nanophases. On the other hand, the coarse-grained regions may correspond to the replacement of anhydrous crystalline silicates of the olivine and pyroxene type. The major difference is the presence of Fe,Ni sulfides in Ryugu and of ferrihydrite and higher iron valency of phyllosilicates in Orgueil. This might be due to long-term terrestrial weathering that would have destabilized the nanosulfides. We also explore an alternative scenario involving more oxidizing hydrothermal conditions on the Orgueil parent body.Note
12 month embargo; first published 14 November 2023ISSN
1086-9379EISSN
1945-5100Version
Final accepted manuscriptSponsors
Agence Nationale de la Rechercheae974a485f413a2113503eed53cd6c53
10.1111/maps.14101
