The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples
This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampli...
Ausführliche Beschreibung
Gespeichert in:
| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Icarus - Orlando, Fla. : Academ. Press, 1962, 408 |
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| Übergeordnetes Werk: |
volume:408 |
| DOI / URN: |
10.1016/j.icarus.2023.115826 |
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| Katalog-ID: |
ELV065739140 |
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| 024 | 7 | |a 10.1016/j.icarus.2023.115826 |2 doi | |
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| 245 | 1 | 0 | |a The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples |
| 264 | 1 | |c 2023 | |
| 336 | |a nicht spezifiziert |b zzz |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 520 | |a This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). | ||
| 650 | 4 | |a Asteroid Ryugu | |
| 650 | 4 | |a Thermal histories | |
| 650 | 4 | |a Geological processes | |
| 650 | 4 | |a Spectroscopy | |
| 650 | 4 | |a Meteorites | |
| 700 | 1 | |a Quirico, Eric |e verfasserin |4 aut | |
| 700 | 1 | |a Montagnac, Gilles |e verfasserin |4 aut | |
| 700 | 1 | |a Komatsu, Mutsumi |e verfasserin |4 aut | |
| 700 | 1 | |a Kebukawa, Yoko |e verfasserin |4 aut | |
| 700 | 1 | |a Yabuta, Hikaru |e verfasserin |4 aut | |
| 700 | 1 | |a Amano, Kana |e verfasserin |4 aut | |
| 700 | 1 | |a Barosch, Jens |e verfasserin |4 aut | |
| 700 | 1 | |a Bejach, Laure |e verfasserin |4 aut | |
| 700 | 1 | |a Cody, George D. |e verfasserin |4 aut | |
| 700 | 1 | |a Dartois, Emmanuel |e verfasserin |4 aut | |
| 700 | 1 | |a Dazzi, Alexandre |e verfasserin |4 aut | |
| 700 | 1 | |a De Gregorio, Bradley |e verfasserin |4 aut | |
| 700 | 1 | |a Deniset-Besseau, Ariane |e verfasserin |4 aut | |
| 700 | 1 | |a Duprat, Jean |e verfasserin |4 aut | |
| 700 | 1 | |a Engrand, Cécile |e verfasserin |4 aut | |
| 700 | 1 | |a Hashiguchi, Minako |e verfasserin |4 aut | |
| 700 | 1 | |a Kamide, Kanami |e verfasserin |4 aut | |
| 700 | 1 | |a Kilcoyne, David |e verfasserin |4 aut | |
| 700 | 1 | |a Martins, Zita |e verfasserin |4 aut | |
| 700 | 1 | |a Mathurin, Jérémie |e verfasserin |4 aut | |
| 700 | 1 | |a Mostefaoui, Smail |e verfasserin |4 aut | |
| 700 | 1 | |a Nittler, Larry |e verfasserin |4 aut | |
| 700 | 1 | |a Ohigashi, Takuji |e verfasserin |4 aut | |
| 700 | 1 | |a Okumura, Taiga |e verfasserin |4 aut | |
| 700 | 1 | |a Remusat, Laurent |e verfasserin |4 aut | |
| 700 | 1 | |a Sandford, Scott |e verfasserin |4 aut | |
| 700 | 1 | |a Shigenaka, Miho |e verfasserin |4 aut | |
| 700 | 1 | |a Stroud, Rhonda |e verfasserin |4 aut | |
| 700 | 1 | |a Suga, Hiroki |e verfasserin |4 aut | |
| 700 | 1 | |a Takahashi, Yoshio |e verfasserin |4 aut | |
| 700 | 1 | |a Takeichi, Yasuo |e verfasserin |4 aut | |
| 700 | 1 | |a Tamenori, Yusuke |e verfasserin |4 aut | |
| 700 | 1 | |a Verdier-Paoletti, Maximilien |e verfasserin |4 aut | |
| 700 | 1 | |a Yamashita, Shohei |e verfasserin |4 aut | |
| 700 | 1 | |a Nakamura, Tomoki |e verfasserin |4 aut | |
| 700 | 1 | |a Naraoka, Hiroshi |e verfasserin |4 aut | |
| 700 | 1 | |a Noguchi, Takaaki |e verfasserin |4 aut | |
| 700 | 1 | |a Okazaki, Ryuji |e verfasserin |4 aut | |
| 700 | 1 | |a Yurimoto, Hisayoshi |e verfasserin |4 aut | |
| 700 | 1 | |a Tachibana, Shogo |e verfasserin |4 aut | |
| 700 | 1 | |a Abe, Masanao |e verfasserin |4 aut | |
| 700 | 1 | |a Miyazaki, Akiko |e verfasserin |4 aut | |
| 700 | 1 | |a Nakato, Aiko |e verfasserin |4 aut | |
| 700 | 1 | |a Nakazawa, Satoru |e verfasserin |4 aut | |
| 700 | 1 | |a Nishimura, Masahiro |e verfasserin |4 aut | |
| 700 | 1 | |a Okada, Tatsuaki |e verfasserin |4 aut | |
| 700 | 1 | |a Saiki, Takanao |e verfasserin |4 aut | |
| 700 | 1 | |a Sakamoto, Kanako |e verfasserin |4 aut | |
| 700 | 1 | |a Tanaka, Satoshi |e verfasserin |4 aut | |
| 700 | 1 | |a Terui, Fuyuto |e verfasserin |4 aut | |
| 700 | 1 | |a Tsuda, Yuichi |e verfasserin |4 aut | |
| 700 | 1 | |a Usui, Tomohiro |e verfasserin |4 aut | |
| 700 | 1 | |a Watanabe, Sei-ichiro |e verfasserin |4 aut | |
| 700 | 1 | |a Yada, Toru |e verfasserin |4 aut | |
| 700 | 1 | |a Yogata, Kasumi |e verfasserin |4 aut | |
| 700 | 1 | |a Yoshikawa, Makota |e verfasserin |4 aut | |
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10.1016/j.icarus.2023.115826 doi (DE-627)ELV065739140 (ELSEVIER)S0019-1035(23)00405-0 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bonal, Lydie verfasserin aut The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites Quirico, Eric verfasserin aut Montagnac, Gilles verfasserin aut Komatsu, Mutsumi verfasserin aut Kebukawa, Yoko verfasserin aut Yabuta, Hikaru verfasserin aut Amano, Kana verfasserin aut Barosch, Jens verfasserin aut Bejach, Laure verfasserin aut Cody, George D. verfasserin aut Dartois, Emmanuel verfasserin aut Dazzi, Alexandre verfasserin aut De Gregorio, Bradley verfasserin aut Deniset-Besseau, Ariane verfasserin aut Duprat, Jean verfasserin aut Engrand, Cécile verfasserin aut Hashiguchi, Minako verfasserin aut Kamide, Kanami verfasserin aut Kilcoyne, David verfasserin aut Martins, Zita verfasserin aut Mathurin, Jérémie verfasserin aut Mostefaoui, Smail verfasserin aut Nittler, Larry verfasserin aut Ohigashi, Takuji verfasserin aut Okumura, Taiga verfasserin aut Remusat, Laurent verfasserin aut Sandford, Scott verfasserin aut Shigenaka, Miho verfasserin aut Stroud, Rhonda verfasserin aut Suga, Hiroki verfasserin aut Takahashi, Yoshio verfasserin aut Takeichi, Yasuo verfasserin aut Tamenori, Yusuke verfasserin aut Verdier-Paoletti, Maximilien verfasserin aut Yamashita, Shohei verfasserin aut Nakamura, Tomoki verfasserin aut Naraoka, Hiroshi verfasserin aut Noguchi, Takaaki verfasserin aut Okazaki, Ryuji verfasserin aut Yurimoto, Hisayoshi verfasserin aut Tachibana, Shogo verfasserin aut Abe, Masanao verfasserin aut Miyazaki, Akiko verfasserin aut Nakato, Aiko verfasserin aut Nakazawa, Satoru verfasserin aut Nishimura, Masahiro verfasserin aut Okada, Tatsuaki verfasserin aut Saiki, Takanao verfasserin aut Sakamoto, Kanako verfasserin aut Tanaka, Satoshi verfasserin aut Terui, Fuyuto verfasserin aut Tsuda, Yuichi verfasserin aut Usui, Tomohiro verfasserin aut Watanabe, Sei-ichiro verfasserin aut Yada, Toru verfasserin aut Yogata, Kasumi verfasserin aut Yoshikawa, Makota verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 408 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:408 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.50 Sonnensystem: Allgemeines VZ AR 408 |
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10.1016/j.icarus.2023.115826 doi (DE-627)ELV065739140 (ELSEVIER)S0019-1035(23)00405-0 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bonal, Lydie verfasserin aut The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites Quirico, Eric verfasserin aut Montagnac, Gilles verfasserin aut Komatsu, Mutsumi verfasserin aut Kebukawa, Yoko verfasserin aut Yabuta, Hikaru verfasserin aut Amano, Kana verfasserin aut Barosch, Jens verfasserin aut Bejach, Laure verfasserin aut Cody, George D. verfasserin aut Dartois, Emmanuel verfasserin aut Dazzi, Alexandre verfasserin aut De Gregorio, Bradley verfasserin aut Deniset-Besseau, Ariane verfasserin aut Duprat, Jean verfasserin aut Engrand, Cécile verfasserin aut Hashiguchi, Minako verfasserin aut Kamide, Kanami verfasserin aut Kilcoyne, David verfasserin aut Martins, Zita verfasserin aut Mathurin, Jérémie verfasserin aut Mostefaoui, Smail verfasserin aut Nittler, Larry verfasserin aut Ohigashi, Takuji verfasserin aut Okumura, Taiga verfasserin aut Remusat, Laurent verfasserin aut Sandford, Scott verfasserin aut Shigenaka, Miho verfasserin aut Stroud, Rhonda verfasserin aut Suga, Hiroki verfasserin aut Takahashi, Yoshio verfasserin aut Takeichi, Yasuo verfasserin aut Tamenori, Yusuke verfasserin aut Verdier-Paoletti, Maximilien verfasserin aut Yamashita, Shohei verfasserin aut Nakamura, Tomoki verfasserin aut Naraoka, Hiroshi verfasserin aut Noguchi, Takaaki verfasserin aut Okazaki, Ryuji verfasserin aut Yurimoto, Hisayoshi verfasserin aut Tachibana, Shogo verfasserin aut Abe, Masanao verfasserin aut Miyazaki, Akiko verfasserin aut Nakato, Aiko verfasserin aut Nakazawa, Satoru verfasserin aut Nishimura, Masahiro verfasserin aut Okada, Tatsuaki verfasserin aut Saiki, Takanao verfasserin aut Sakamoto, Kanako verfasserin aut Tanaka, Satoshi verfasserin aut Terui, Fuyuto verfasserin aut Tsuda, Yuichi verfasserin aut Usui, Tomohiro verfasserin aut Watanabe, Sei-ichiro verfasserin aut Yada, Toru verfasserin aut Yogata, Kasumi verfasserin aut Yoshikawa, Makota verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 408 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:408 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.50 Sonnensystem: Allgemeines VZ AR 408 |
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10.1016/j.icarus.2023.115826 doi (DE-627)ELV065739140 (ELSEVIER)S0019-1035(23)00405-0 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bonal, Lydie verfasserin aut The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites Quirico, Eric verfasserin aut Montagnac, Gilles verfasserin aut Komatsu, Mutsumi verfasserin aut Kebukawa, Yoko verfasserin aut Yabuta, Hikaru verfasserin aut Amano, Kana verfasserin aut Barosch, Jens verfasserin aut Bejach, Laure verfasserin aut Cody, George D. verfasserin aut Dartois, Emmanuel verfasserin aut Dazzi, Alexandre verfasserin aut De Gregorio, Bradley verfasserin aut Deniset-Besseau, Ariane verfasserin aut Duprat, Jean verfasserin aut Engrand, Cécile verfasserin aut Hashiguchi, Minako verfasserin aut Kamide, Kanami verfasserin aut Kilcoyne, David verfasserin aut Martins, Zita verfasserin aut Mathurin, Jérémie verfasserin aut Mostefaoui, Smail verfasserin aut Nittler, Larry verfasserin aut Ohigashi, Takuji verfasserin aut Okumura, Taiga verfasserin aut Remusat, Laurent verfasserin aut Sandford, Scott verfasserin aut Shigenaka, Miho verfasserin aut Stroud, Rhonda verfasserin aut Suga, Hiroki verfasserin aut Takahashi, Yoshio verfasserin aut Takeichi, Yasuo verfasserin aut Tamenori, Yusuke verfasserin aut Verdier-Paoletti, Maximilien verfasserin aut Yamashita, Shohei verfasserin aut Nakamura, Tomoki verfasserin aut Naraoka, Hiroshi verfasserin aut Noguchi, Takaaki verfasserin aut Okazaki, Ryuji verfasserin aut Yurimoto, Hisayoshi verfasserin aut Tachibana, Shogo verfasserin aut Abe, Masanao verfasserin aut Miyazaki, Akiko verfasserin aut Nakato, Aiko verfasserin aut Nakazawa, Satoru verfasserin aut Nishimura, Masahiro verfasserin aut Okada, Tatsuaki verfasserin aut Saiki, Takanao verfasserin aut Sakamoto, Kanako verfasserin aut Tanaka, Satoshi verfasserin aut Terui, Fuyuto verfasserin aut Tsuda, Yuichi verfasserin aut Usui, Tomohiro verfasserin aut Watanabe, Sei-ichiro verfasserin aut Yada, Toru verfasserin aut Yogata, Kasumi verfasserin aut Yoshikawa, Makota verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 408 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:408 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.50 Sonnensystem: Allgemeines VZ AR 408 |
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10.1016/j.icarus.2023.115826 doi (DE-627)ELV065739140 (ELSEVIER)S0019-1035(23)00405-0 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bonal, Lydie verfasserin aut The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites Quirico, Eric verfasserin aut Montagnac, Gilles verfasserin aut Komatsu, Mutsumi verfasserin aut Kebukawa, Yoko verfasserin aut Yabuta, Hikaru verfasserin aut Amano, Kana verfasserin aut Barosch, Jens verfasserin aut Bejach, Laure verfasserin aut Cody, George D. verfasserin aut Dartois, Emmanuel verfasserin aut Dazzi, Alexandre verfasserin aut De Gregorio, Bradley verfasserin aut Deniset-Besseau, Ariane verfasserin aut Duprat, Jean verfasserin aut Engrand, Cécile verfasserin aut Hashiguchi, Minako verfasserin aut Kamide, Kanami verfasserin aut Kilcoyne, David verfasserin aut Martins, Zita verfasserin aut Mathurin, Jérémie verfasserin aut Mostefaoui, Smail verfasserin aut Nittler, Larry verfasserin aut Ohigashi, Takuji verfasserin aut Okumura, Taiga verfasserin aut Remusat, Laurent verfasserin aut Sandford, Scott verfasserin aut Shigenaka, Miho verfasserin aut Stroud, Rhonda verfasserin aut Suga, Hiroki verfasserin aut Takahashi, Yoshio verfasserin aut Takeichi, Yasuo verfasserin aut Tamenori, Yusuke verfasserin aut Verdier-Paoletti, Maximilien verfasserin aut Yamashita, Shohei verfasserin aut Nakamura, Tomoki verfasserin aut Naraoka, Hiroshi verfasserin aut Noguchi, Takaaki verfasserin aut Okazaki, Ryuji verfasserin aut Yurimoto, Hisayoshi verfasserin aut Tachibana, Shogo verfasserin aut Abe, Masanao verfasserin aut Miyazaki, Akiko verfasserin aut Nakato, Aiko verfasserin aut Nakazawa, Satoru verfasserin aut Nishimura, Masahiro verfasserin aut Okada, Tatsuaki verfasserin aut Saiki, Takanao verfasserin aut Sakamoto, Kanako verfasserin aut Tanaka, Satoshi verfasserin aut Terui, Fuyuto verfasserin aut Tsuda, Yuichi verfasserin aut Usui, Tomohiro verfasserin aut Watanabe, Sei-ichiro verfasserin aut Yada, Toru verfasserin aut Yogata, Kasumi verfasserin aut Yoshikawa, Makota verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 408 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:408 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.50 Sonnensystem: Allgemeines VZ AR 408 |
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10.1016/j.icarus.2023.115826 doi (DE-627)ELV065739140 (ELSEVIER)S0019-1035(23)00405-0 DE-627 ger DE-627 rda eng 520 530 VZ 39.50 bkl Bonal, Lydie verfasserin aut The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites Quirico, Eric verfasserin aut Montagnac, Gilles verfasserin aut Komatsu, Mutsumi verfasserin aut Kebukawa, Yoko verfasserin aut Yabuta, Hikaru verfasserin aut Amano, Kana verfasserin aut Barosch, Jens verfasserin aut Bejach, Laure verfasserin aut Cody, George D. verfasserin aut Dartois, Emmanuel verfasserin aut Dazzi, Alexandre verfasserin aut De Gregorio, Bradley verfasserin aut Deniset-Besseau, Ariane verfasserin aut Duprat, Jean verfasserin aut Engrand, Cécile verfasserin aut Hashiguchi, Minako verfasserin aut Kamide, Kanami verfasserin aut Kilcoyne, David verfasserin aut Martins, Zita verfasserin aut Mathurin, Jérémie verfasserin aut Mostefaoui, Smail verfasserin aut Nittler, Larry verfasserin aut Ohigashi, Takuji verfasserin aut Okumura, Taiga verfasserin aut Remusat, Laurent verfasserin aut Sandford, Scott verfasserin aut Shigenaka, Miho verfasserin aut Stroud, Rhonda verfasserin aut Suga, Hiroki verfasserin aut Takahashi, Yoshio verfasserin aut Takeichi, Yasuo verfasserin aut Tamenori, Yusuke verfasserin aut Verdier-Paoletti, Maximilien verfasserin aut Yamashita, Shohei verfasserin aut Nakamura, Tomoki verfasserin aut Naraoka, Hiroshi verfasserin aut Noguchi, Takaaki verfasserin aut Okazaki, Ryuji verfasserin aut Yurimoto, Hisayoshi verfasserin aut Tachibana, Shogo verfasserin aut Abe, Masanao verfasserin aut Miyazaki, Akiko verfasserin aut Nakato, Aiko verfasserin aut Nakazawa, Satoru verfasserin aut Nishimura, Masahiro verfasserin aut Okada, Tatsuaki verfasserin aut Saiki, Takanao verfasserin aut Sakamoto, Kanako verfasserin aut Tanaka, Satoshi verfasserin aut Terui, Fuyuto verfasserin aut Tsuda, Yuichi verfasserin aut Usui, Tomohiro verfasserin aut Watanabe, Sei-ichiro verfasserin aut Yada, Toru verfasserin aut Yogata, Kasumi verfasserin aut Yoshikawa, Makota verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 408 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:408 GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2088 GBV_ILN_2106 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2470 GBV_ILN_2507 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.50 Sonnensystem: Allgemeines VZ AR 408 |
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Bonal, Lydie @@aut@@ Quirico, Eric @@aut@@ Montagnac, Gilles @@aut@@ Komatsu, Mutsumi @@aut@@ Kebukawa, Yoko @@aut@@ Yabuta, Hikaru @@aut@@ Amano, Kana @@aut@@ Barosch, Jens @@aut@@ Bejach, Laure @@aut@@ Cody, George D. @@aut@@ Dartois, Emmanuel @@aut@@ Dazzi, Alexandre @@aut@@ De Gregorio, Bradley @@aut@@ Deniset-Besseau, Ariane @@aut@@ Duprat, Jean @@aut@@ Engrand, Cécile @@aut@@ Hashiguchi, Minako @@aut@@ Kamide, Kanami @@aut@@ Kilcoyne, David @@aut@@ Martins, Zita @@aut@@ Mathurin, Jérémie @@aut@@ Mostefaoui, Smail @@aut@@ Nittler, Larry @@aut@@ Ohigashi, Takuji @@aut@@ Okumura, Taiga @@aut@@ Remusat, Laurent @@aut@@ Sandford, Scott @@aut@@ Shigenaka, Miho @@aut@@ Stroud, Rhonda @@aut@@ Suga, Hiroki @@aut@@ Takahashi, Yoshio @@aut@@ Takeichi, Yasuo @@aut@@ Tamenori, Yusuke @@aut@@ Verdier-Paoletti, Maximilien @@aut@@ Yamashita, Shohei @@aut@@ Nakamura, Tomoki @@aut@@ Naraoka, Hiroshi @@aut@@ Noguchi, Takaaki @@aut@@ Okazaki, Ryuji @@aut@@ Yurimoto, Hisayoshi @@aut@@ Tachibana, Shogo @@aut@@ Abe, Masanao @@aut@@ Miyazaki, Akiko @@aut@@ Nakato, Aiko @@aut@@ Nakazawa, Satoru @@aut@@ Nishimura, Masahiro @@aut@@ Okada, Tatsuaki @@aut@@ Saiki, Takanao @@aut@@ Sakamoto, Kanako @@aut@@ Tanaka, Satoshi @@aut@@ Terui, Fuyuto @@aut@@ Tsuda, Yuichi @@aut@@ Usui, Tomohiro @@aut@@ Watanabe, Sei-ichiro @@aut@@ Yada, Toru @@aut@@ Yogata, Kasumi @@aut@@ Yoshikawa, Makota @@aut@@ |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">ELV065739140</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20240224093158.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">231122s2023 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1016/j.icarus.2023.115826</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)ELV065739140</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ELSEVIER)S0019-1035(23)00405-0</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">520</subfield><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.50</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Bonal, Lydie</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2023</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">nicht spezifiziert</subfield><subfield code="b">zzz</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. 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520 530 VZ 39.50 bkl The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples Asteroid Ryugu Thermal histories Geological processes Spectroscopy Meteorites |
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The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples |
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Bonal, Lydie Quirico, Eric Montagnac, Gilles Komatsu, Mutsumi Kebukawa, Yoko Yabuta, Hikaru Amano, Kana Barosch, Jens Bejach, Laure Cody, George D. Dartois, Emmanuel Dazzi, Alexandre De Gregorio, Bradley Deniset-Besseau, Ariane Duprat, Jean Engrand, Cécile Hashiguchi, Minako Kamide, Kanami Kilcoyne, David Martins, Zita Mathurin, Jérémie Mostefaoui, Smail Nittler, Larry Ohigashi, Takuji Okumura, Taiga Remusat, Laurent Sandford, Scott Shigenaka, Miho Stroud, Rhonda Suga, Hiroki Takahashi, Yoshio Takeichi, Yasuo Tamenori, Yusuke Verdier-Paoletti, Maximilien Yamashita, Shohei Nakamura, Tomoki Naraoka, Hiroshi Noguchi, Takaaki Okazaki, Ryuji Yurimoto, Hisayoshi Tachibana, Shogo Abe, Masanao Miyazaki, Akiko Nakato, Aiko Nakazawa, Satoru Nishimura, Masahiro Okada, Tatsuaki Saiki, Takanao Sakamoto, Kanako Tanaka, Satoshi Terui, Fuyuto Tsuda, Yuichi Usui, Tomohiro Watanabe, Sei-ichiro Yada, Toru Yogata, Kasumi Yoshikawa, Makota |
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the thermal history of ryugu based on raman characterization of hayabusa2 samples |
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The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples |
| abstract |
This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). |
| abstractGer |
This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). |
| abstract_unstemmed |
This paper is focused on the characterization of the thermal history of C-type asteroid Ryugu through the structure of the polyaromatic carbonaceous matter in the returned samples determined by Raman spectroscopy. Both intact particles and extracted Insoluble Organic Matter (IOM) from the two sampling sites on Ryugu have been characterized. The main conclusions are that (i) there is no structural difference of the polyaromatic component probed by Raman spectroscopy between the two sampling sites, (ii) in a manner similar to type 1 and 2 chondrites, the characterized Ryugu particles did not experience significant long-duration thermal metamorphism related to the radioactive decay of elements such as 26Al; (iii) some structural variability is nevertheless observed within our particle set. It can be interpreted as some particles having experienced some short-duration and weak heating (R3 in the scale defined by Quirico et al. 2018 and TII or lower according to the scale defined by Nakamura, 2005). |
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The thermal history of Ryugu based on Raman characterization of Hayabusa2 samples |
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Quirico, Eric Montagnac, Gilles Komatsu, Mutsumi Kebukawa, Yoko Yabuta, Hikaru Amano, Kana Barosch, Jens Bejach, Laure Cody, George D. Dartois, Emmanuel Dazzi, Alexandre De Gregorio, Bradley Deniset-Besseau, Ariane Duprat, Jean Engrand, Cécile Hashiguchi, Minako Kamide, Kanami Kilcoyne, David Martins, Zita Mathurin, Jérémie Mostefaoui, Smail Nittler, Larry Ohigashi, Takuji Okumura, Taiga Remusat, Laurent Sandford, Scott Shigenaka, Miho Stroud, Rhonda Suga, Hiroki Takahashi, Yoshio Takeichi, Yasuo Tamenori, Yusuke Verdier-Paoletti, Maximilien Yamashita, Shohei Nakamura, Tomoki Naraoka, Hiroshi Noguchi, Takaaki Okazaki, Ryuji Yurimoto, Hisayoshi Tachibana, Shogo Abe, Masanao Miyazaki, Akiko Nakato, Aiko Nakazawa, Satoru Nishimura, Masahiro Okada, Tatsuaki Saiki, Takanao Sakamoto, Kanako Tanaka, Satoshi Terui, Fuyuto Tsuda, Yuichi Usui, Tomohiro Watanabe, Sei-ichiro Yada, Toru Yogata, Kasumi Yoshikawa, Makota |
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| score |
7.400757 |