Abstract
Without a protective atmosphere, space-exposed surfaces of airless Solar System bodies gradually experience an alteration in composition, structure and optical properties through a collective process called space weathering. The return of samples from near-Earth asteroid (162173) Ryugu by Hayabusa2 provides the first opportunity for laboratory study of space-weathering signatures on the most abundant type of inner solar system body: a C-type asteroid, composed of materials largely unchanged since the formation of the Solar System. Weathered Ryugu grains show areas of surface amorphization and partial melting of phyllosilicates, in which reduction from Fe3+ to Fe2+ and dehydration developed. Space weathering probably contributed to dehydration by dehydroxylation of Ryugu surface phyllosilicates that had already lost interlayer water molecules and to weakening of the 2.7 µm hydroxyl (–OH) band in reflectance spectra. For C-type asteroids in general, this indicates that a weak 2.7 µm band can signify space-weathering-induced surface dehydration, rather than bulk volatile loss.
Original language | English (US) |
---|---|
Pages (from-to) | 170-181 |
Number of pages | 12 |
Journal | Nature Astronomy |
Volume | 7 |
Issue number | 2 |
DOIs | |
State | Published - Feb 2023 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
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A dehydrated space-weathered skin cloaking the hydrated interior of Ryugu. / Noguchi, Takaaki; Matsumoto, Toru; Miyake, Akira et al.
In: Nature Astronomy, Vol. 7, No. 2, 02.2023, p. 170-181.Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - A dehydrated space-weathered skin cloaking the hydrated interior of Ryugu
AU - Noguchi, Takaaki
AU - Matsumoto, Toru
AU - Miyake, Akira
AU - Igami, Yohei
AU - Haruta, Mitsutaka
AU - Saito, Hikaru
AU - Hata, Satoshi
AU - Seto, Yusuke
AU - Miyahara, Masaaki
AU - Tomioka, Naotaka
AU - Ishii, Hope A.
AU - Bradley, John P.
AU - Ohtaki, Kenta K.
AU - Dobrică, Elena
AU - Leroux, Hugues
AU - Le Guillou, Corentin
AU - Jacob, Damien
AU - de la Peña, Francisco
AU - Laforet, Sylvain
AU - Marinova, Maya
AU - Langenhorst, Falko
AU - Harries, Dennis
AU - Beck, Pierre
AU - Phan, Thi H.V.
AU - Rebois, Rolando
AU - Abreu, Neyda M.
AU - Gray, Jennifer
AU - Zega, Thomas
AU - Zanetta, Pierre M.
AU - Thompson, Michelle S.
AU - Stroud, Rhonda
AU - Burgess, Kate
AU - Cymes, Brittany A.
AU - Bridges, John C.
AU - Hicks, Leon
AU - Lee, Martin R.
AU - Daly, Luke
AU - Bland, Phil A.
AU - Zolensky, Michael E.
AU - Frank, David R.
AU - Martinez, James
AU - Tsuchiyama, Akira
AU - Yasutake, Masahiro
AU - Matsuno, Junya
AU - Okumura, Shota
AU - Mitsukawa, Itaru
AU - Uesugi, Kentaro
AU - Uesugi, Masayuki
AU - Takeuchi, Akihisa
AU - Sun, Mingqi
AU - Enju, Satomi
AU - Takigawa, Aki
AU - Michikami, Tatsuhiro
AU - Nakamura, Tomoki
AU - Matsumoto, Megumi
AU - Nakauchi, Yusuke
AU - Abe, Masanao
AU - Arakawa, Masahiko
AU - Fujii, Atsushi
AU - Hayakawa, Masahiko
AU - Hirata, Naru
AU - Hirata, Naoyuki
AU - Honda, Rie
AU - Honda, Chikatoshi
AU - Hosoda, Satoshi
AU - Iijima, Yu ichi
AU - Ikeda, Hitoshi
AU - Ishiguro, Masateru
AU - Ishihara, Yoshiaki
AU - Iwata, Takahiro
AU - Kawahara, Kousuke
AU - Kikuchi, Shota
AU - Kitazato, Kohei
AU - Matsumoto, Koji
AU - Matsuoka, Moe
AU - Mimasu, Yuya
AU - Miura, Akira
AU - Morota, Tomokatsu
AU - Nakazawa, Satoru
AU - Namiki, Noriyuki
AU - Noda, Hirotomo
AU - Noguchi, Rina
AU - Ogawa, Naoko
AU - Ogawa, Kazunori
AU - Okada, Tatsuaki
AU - Okamoto, Chisato
AU - Ono, Go
AU - Ozaki, Masanobu
AU - Saiki, Takanao
AU - Sakatani, Naoya
AU - Sawada, Hirotaka
AU - Senshu, Hiroki
AU - Shimaki, Yuri
AU - Shirai, Kei
AU - Sugita, Seiji
AU - Takei, Yuto
AU - Takeuchi, Hiroshi
AU - Tanaka, Satoshi
AU - Tatsumi, Eri
AU - Terui, Fuyuto
AU - Tsukizaki, Ryudo
AU - Wada, Koji
AU - Yamada, Manabu
AU - Yamada, Tetsuya
AU - Yamamoto, Yukio
AU - Yano, Hajime
AU - Yokota, Yasuhiro
AU - Yoshihara, Keisuke
AU - Yoshikawa, Makoto
AU - Yoshikawa, Kent
AU - Fukai, Ryohta
AU - Furuya, Shizuho
AU - Hatakeda, Kentaro
AU - Hayashi, Tasuku
AU - Hitomi, Yuya
AU - Kumagai, Kazuya
AU - Miyazaki, Akiko
AU - Nakato, Aiko
AU - Nishimura, Masahiro
AU - Soejima, Hiromichi
AU - Suzuki, Ayako I.
AU - Usui, Tomohiro
AU - Yada, Toru
AU - Yamamoto, Daiki
AU - Yogata, Kasumi
AU - Yoshitake, Miwa
AU - Connolly, Harold C.
AU - Lauretta, Dante S.
AU - Yurimoto, Hisayoshi
AU - Nagashima, Kazuhide
AU - Kawasaki, Noriyuki
AU - Sakamoto, Naoya
AU - Okazaki, Ryuji
AU - Yabuta, Hikaru
AU - Naraoka, Hiroshi
AU - Sakamoto, Kanako
AU - Tachibana, Shogo
AU - Watanabe, Sei ichiro
AU - Tsuda, Yuichi
N1 - Funding Information: The Hayabusa2 project has been developed and led by JAXA in collaboration with the Deutsches Zentrum für Luft- und Raumfahrt (DLR) and the Centre national d’études spatiales (CNES), and supported by NASA and the Australian Space Agency (ASA). We thank all of the members of the Hayabusa2 project for their technical and scientific contributions. TEM works at Kyushu University were supported by the Advanced Characterization Platform of the Nanotechnology Platform Japan (grant no. JPMXP09A21KU0393) sponsored by the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan. P.B., T.H.V.P. and R.R. acknowledge the Centre National d’Etude Spatiale (CNES). H.L., C.L.G., D.J., F.D.L.P. and M. Marinova acknowledge the advanced characterization platform, University of Lille - CNRS. Work at the Molecular Foundry was supported by the Office of Science, Office of Basic Energy Sciences, of the US Department of Energy under contract no. DE-AC02–05CH11231. This work was funded by the following funds: JSPS KAKENHI grant nos. 19H00725, 19KK0094, 21H05424, 20H01965, 20H00198, 20H00205, 16H06348 and 20H00188; JSPS Core-to-core program ‘International Network of Planetary Sciences’; UK Science and Technology Facilities Council (STFC) grant no. ST/S000429/1; Start-up funds from Purdue University; ISITE ULNE, Métropole Européenne de Lille, the region ‘Hauts-de-France’ and the ERDF program of the European Union; and European Research Council (ERC) under grant agreement no. 771691 (Solarys). Funding Information: The Hayabusa2 project has been developed and led by JAXA in collaboration with the Deutsches Zentrum für Luft- und Raumfahrt (DLR) and the Centre national d’études spatiales (CNES), and supported by NASA and the Australian Space Agency (ASA). We thank all of the members of the Hayabusa2 project for their technical and scientific contributions. TEM works at Kyushu University were supported by the Advanced Characterization Platform of the Nanotechnology Platform Japan (grant no. JPMXP09A21KU0393) sponsored by the Ministry of Education, Culture, Sports, Science and Technology (MEXT), Japan. P.B., T.H.V.P. and R.R. acknowledge the Centre National d’Etude Spatiale (CNES). H.L., C.L.G., D.J., F.D.L.P. and M. Marinova acknowledge the advanced characterization platform, University of Lille - CNRS. Work at the Molecular Foundry was supported by the Office of Science, Office of Basic Energy Sciences, of the US Department of Energy under contract no. DE-AC02–05CH11231. This work was funded by the following funds: JSPS KAKENHI grant nos. 19H00725, 19KK0094, 21H05424, 20H01965, 20H00198, 20H00205, 16H06348 and 20H00188; JSPS Core-to-core program ‘International Network of Planetary Sciences’; UK Science and Technology Facilities Council (STFC) grant no. ST/S000429/1; Start-up funds from Purdue University; ISITE ULNE, Métropole Européenne de Lille, the region ‘Hauts-de-France’ and the ERDF program of the European Union; and European Research Council (ERC) under grant agreement no. 771691 (Solarys). Publisher Copyright: © 2022, The Author(s).
PY - 2023/2
Y1 - 2023/2
N2 - Without a protective atmosphere, space-exposed surfaces of airless Solar System bodies gradually experience an alteration in composition, structure and optical properties through a collective process called space weathering. The return of samples from near-Earth asteroid (162173) Ryugu by Hayabusa2 provides the first opportunity for laboratory study of space-weathering signatures on the most abundant type of inner solar system body: a C-type asteroid, composed of materials largely unchanged since the formation of the Solar System. Weathered Ryugu grains show areas of surface amorphization and partial melting of phyllosilicates, in which reduction from Fe3+ to Fe2+ and dehydration developed. Space weathering probably contributed to dehydration by dehydroxylation of Ryugu surface phyllosilicates that had already lost interlayer water molecules and to weakening of the 2.7 µm hydroxyl (–OH) band in reflectance spectra. For C-type asteroids in general, this indicates that a weak 2.7 µm band can signify space-weathering-induced surface dehydration, rather than bulk volatile loss.
AB - Without a protective atmosphere, space-exposed surfaces of airless Solar System bodies gradually experience an alteration in composition, structure and optical properties through a collective process called space weathering. The return of samples from near-Earth asteroid (162173) Ryugu by Hayabusa2 provides the first opportunity for laboratory study of space-weathering signatures on the most abundant type of inner solar system body: a C-type asteroid, composed of materials largely unchanged since the formation of the Solar System. Weathered Ryugu grains show areas of surface amorphization and partial melting of phyllosilicates, in which reduction from Fe3+ to Fe2+ and dehydration developed. Space weathering probably contributed to dehydration by dehydroxylation of Ryugu surface phyllosilicates that had already lost interlayer water molecules and to weakening of the 2.7 µm hydroxyl (–OH) band in reflectance spectra. For C-type asteroids in general, this indicates that a weak 2.7 µm band can signify space-weathering-induced surface dehydration, rather than bulk volatile loss.
UR - http://www.scopus.com/inward/record.url?scp=85138230361&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85138230361&partnerID=8YFLogxK
U2 - 10.1038/s41550-022-01841-6
DO - 10.1038/s41550-022-01841-6
M3 - Article
C2 - 36845884
AN - SCOPUS:85138230361
SN - 2397-3366
VL - 7
SP - 170
EP - 181
JO - Nature Astronomy
JF - Nature Astronomy
IS - 2
ER -