Variations of the surface characteristics of Ryugu returned samples
Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obta...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Aiko Nakato [verfasserIn] Toru Yada [verfasserIn] Masahiro Nishimura [verfasserIn] Kasumi Yogata [verfasserIn] Akiko Miyazaki [verfasserIn] Kana Nagashima [verfasserIn] Kentaro Hatakeda [verfasserIn] Kazuya Kumagai [verfasserIn] Yuya Hitomi [verfasserIn] Hiromichi Soejima [verfasserIn] Jean-Pierre Bibring [verfasserIn] Cedric Pilorget [verfasserIn] Vincent Hamm [verfasserIn] Rosario Brunetto [verfasserIn] Lucie Riu [verfasserIn] Lionel Lourit [verfasserIn] Damien Loizeau [verfasserIn] Tania Le Pivert-Jolivet [verfasserIn] Guillaume Lequertier [verfasserIn] Aurelie Moussi-Soffys [verfasserIn] Masanao Abe [verfasserIn] Tatsuaki Okada [verfasserIn] Tomohiro Usui [verfasserIn] Satoru Nakazawa [verfasserIn] Takanao Saiki [verfasserIn] Satoshi Tanaka [verfasserIn] Fuyuto Terui [verfasserIn] Makoto Yoshikawa [verfasserIn] Sei-ichiro Watanabe [verfasserIn] Yuichi Tsuda [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
In: Earth, Planets and Space - SpringerOpen, 2015, 75(2023), 1, Seite 19 |
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| Übergeordnetes Werk: |
volume:75 ; year:2023 ; number:1 ; pages:19 |
| Links: |
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| DOI / URN: |
10.1186/s40623-022-01754-8 |
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| Katalog-ID: |
DOAJ088764826 |
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| 520 | |a Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract | ||
| 650 | 4 | |a Hayabusa2 | |
| 650 | 4 | |a Ryugu | |
| 650 | 4 | |a Curation | |
| 650 | 4 | |a Returned samples | |
| 650 | 4 | |a Classification | |
| 653 | 0 | |a Geography. Anthropology. Recreation | |
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| 653 | 0 | |a Geology | |
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| 700 | 0 | |a Masahiro Nishimura |e verfasserin |4 aut | |
| 700 | 0 | |a Kasumi Yogata |e verfasserin |4 aut | |
| 700 | 0 | |a Akiko Miyazaki |e verfasserin |4 aut | |
| 700 | 0 | |a Kana Nagashima |e verfasserin |4 aut | |
| 700 | 0 | |a Kentaro Hatakeda |e verfasserin |4 aut | |
| 700 | 0 | |a Kazuya Kumagai |e verfasserin |4 aut | |
| 700 | 0 | |a Yuya Hitomi |e verfasserin |4 aut | |
| 700 | 0 | |a Hiromichi Soejima |e verfasserin |4 aut | |
| 700 | 0 | |a Jean-Pierre Bibring |e verfasserin |4 aut | |
| 700 | 0 | |a Cedric Pilorget |e verfasserin |4 aut | |
| 700 | 0 | |a Vincent Hamm |e verfasserin |4 aut | |
| 700 | 0 | |a Rosario Brunetto |e verfasserin |4 aut | |
| 700 | 0 | |a Lucie Riu |e verfasserin |4 aut | |
| 700 | 0 | |a Lionel Lourit |e verfasserin |4 aut | |
| 700 | 0 | |a Damien Loizeau |e verfasserin |4 aut | |
| 700 | 0 | |a Tania Le Pivert-Jolivet |e verfasserin |4 aut | |
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| 700 | 0 | |a Aurelie Moussi-Soffys |e verfasserin |4 aut | |
| 700 | 0 | |a Masanao Abe |e verfasserin |4 aut | |
| 700 | 0 | |a Tatsuaki Okada |e verfasserin |4 aut | |
| 700 | 0 | |a Tomohiro Usui |e verfasserin |4 aut | |
| 700 | 0 | |a Satoru Nakazawa |e verfasserin |4 aut | |
| 700 | 0 | |a Takanao Saiki |e verfasserin |4 aut | |
| 700 | 0 | |a Satoshi Tanaka |e verfasserin |4 aut | |
| 700 | 0 | |a Fuyuto Terui |e verfasserin |4 aut | |
| 700 | 0 | |a Makoto Yoshikawa |e verfasserin |4 aut | |
| 700 | 0 | |a Sei-ichiro Watanabe |e verfasserin |4 aut | |
| 700 | 0 | |a Yuichi Tsuda |e verfasserin |4 aut | |
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10.1186/s40623-022-01754-8 doi (DE-627)DOAJ088764826 (DE-599)DOAJ57f64037694b45f1a81189f70a674247 DE-627 ger DE-627 rakwb eng QB275-343 QE1-996.5 Aiko Nakato verfasserin aut Variations of the surface characteristics of Ryugu returned samples 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract Hayabusa2 Ryugu Curation Returned samples Classification Geography. Anthropology. Recreation G Geodesy Geology Toru Yada verfasserin aut Masahiro Nishimura verfasserin aut Kasumi Yogata verfasserin aut Akiko Miyazaki verfasserin aut Kana Nagashima verfasserin aut Kentaro Hatakeda verfasserin aut Kazuya Kumagai verfasserin aut Yuya Hitomi verfasserin aut Hiromichi Soejima verfasserin aut Jean-Pierre Bibring verfasserin aut Cedric Pilorget verfasserin aut Vincent Hamm verfasserin aut Rosario Brunetto verfasserin aut Lucie Riu verfasserin aut Lionel Lourit verfasserin aut Damien Loizeau verfasserin aut Tania Le Pivert-Jolivet verfasserin aut Guillaume Lequertier verfasserin aut Aurelie Moussi-Soffys verfasserin aut Masanao Abe verfasserin aut Tatsuaki Okada verfasserin aut Tomohiro Usui verfasserin aut Satoru Nakazawa verfasserin aut Takanao Saiki verfasserin aut Satoshi Tanaka verfasserin aut Fuyuto Terui verfasserin aut Makoto Yoshikawa verfasserin aut Sei-ichiro Watanabe verfasserin aut Yuichi Tsuda verfasserin aut In Earth, Planets and Space SpringerOpen, 2015 75(2023), 1, Seite 19 (DE-627)353898597 (DE-600)2087663-4 18805981 nnns volume:75 year:2023 number:1 pages:19 https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/article/57f64037694b45f1a81189f70a674247 kostenfrei https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/toc/1880-5981 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 75 2023 1 19 |
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10.1186/s40623-022-01754-8 doi (DE-627)DOAJ088764826 (DE-599)DOAJ57f64037694b45f1a81189f70a674247 DE-627 ger DE-627 rakwb eng QB275-343 QE1-996.5 Aiko Nakato verfasserin aut Variations of the surface characteristics of Ryugu returned samples 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract Hayabusa2 Ryugu Curation Returned samples Classification Geography. Anthropology. Recreation G Geodesy Geology Toru Yada verfasserin aut Masahiro Nishimura verfasserin aut Kasumi Yogata verfasserin aut Akiko Miyazaki verfasserin aut Kana Nagashima verfasserin aut Kentaro Hatakeda verfasserin aut Kazuya Kumagai verfasserin aut Yuya Hitomi verfasserin aut Hiromichi Soejima verfasserin aut Jean-Pierre Bibring verfasserin aut Cedric Pilorget verfasserin aut Vincent Hamm verfasserin aut Rosario Brunetto verfasserin aut Lucie Riu verfasserin aut Lionel Lourit verfasserin aut Damien Loizeau verfasserin aut Tania Le Pivert-Jolivet verfasserin aut Guillaume Lequertier verfasserin aut Aurelie Moussi-Soffys verfasserin aut Masanao Abe verfasserin aut Tatsuaki Okada verfasserin aut Tomohiro Usui verfasserin aut Satoru Nakazawa verfasserin aut Takanao Saiki verfasserin aut Satoshi Tanaka verfasserin aut Fuyuto Terui verfasserin aut Makoto Yoshikawa verfasserin aut Sei-ichiro Watanabe verfasserin aut Yuichi Tsuda verfasserin aut In Earth, Planets and Space SpringerOpen, 2015 75(2023), 1, Seite 19 (DE-627)353898597 (DE-600)2087663-4 18805981 nnns volume:75 year:2023 number:1 pages:19 https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/article/57f64037694b45f1a81189f70a674247 kostenfrei https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/toc/1880-5981 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 75 2023 1 19 |
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10.1186/s40623-022-01754-8 doi (DE-627)DOAJ088764826 (DE-599)DOAJ57f64037694b45f1a81189f70a674247 DE-627 ger DE-627 rakwb eng QB275-343 QE1-996.5 Aiko Nakato verfasserin aut Variations of the surface characteristics of Ryugu returned samples 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract Hayabusa2 Ryugu Curation Returned samples Classification Geography. Anthropology. Recreation G Geodesy Geology Toru Yada verfasserin aut Masahiro Nishimura verfasserin aut Kasumi Yogata verfasserin aut Akiko Miyazaki verfasserin aut Kana Nagashima verfasserin aut Kentaro Hatakeda verfasserin aut Kazuya Kumagai verfasserin aut Yuya Hitomi verfasserin aut Hiromichi Soejima verfasserin aut Jean-Pierre Bibring verfasserin aut Cedric Pilorget verfasserin aut Vincent Hamm verfasserin aut Rosario Brunetto verfasserin aut Lucie Riu verfasserin aut Lionel Lourit verfasserin aut Damien Loizeau verfasserin aut Tania Le Pivert-Jolivet verfasserin aut Guillaume Lequertier verfasserin aut Aurelie Moussi-Soffys verfasserin aut Masanao Abe verfasserin aut Tatsuaki Okada verfasserin aut Tomohiro Usui verfasserin aut Satoru Nakazawa verfasserin aut Takanao Saiki verfasserin aut Satoshi Tanaka verfasserin aut Fuyuto Terui verfasserin aut Makoto Yoshikawa verfasserin aut Sei-ichiro Watanabe verfasserin aut Yuichi Tsuda verfasserin aut In Earth, Planets and Space SpringerOpen, 2015 75(2023), 1, Seite 19 (DE-627)353898597 (DE-600)2087663-4 18805981 nnns volume:75 year:2023 number:1 pages:19 https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/article/57f64037694b45f1a81189f70a674247 kostenfrei https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/toc/1880-5981 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 75 2023 1 19 |
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10.1186/s40623-022-01754-8 doi (DE-627)DOAJ088764826 (DE-599)DOAJ57f64037694b45f1a81189f70a674247 DE-627 ger DE-627 rakwb eng QB275-343 QE1-996.5 Aiko Nakato verfasserin aut Variations of the surface characteristics of Ryugu returned samples 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract Hayabusa2 Ryugu Curation Returned samples Classification Geography. Anthropology. Recreation G Geodesy Geology Toru Yada verfasserin aut Masahiro Nishimura verfasserin aut Kasumi Yogata verfasserin aut Akiko Miyazaki verfasserin aut Kana Nagashima verfasserin aut Kentaro Hatakeda verfasserin aut Kazuya Kumagai verfasserin aut Yuya Hitomi verfasserin aut Hiromichi Soejima verfasserin aut Jean-Pierre Bibring verfasserin aut Cedric Pilorget verfasserin aut Vincent Hamm verfasserin aut Rosario Brunetto verfasserin aut Lucie Riu verfasserin aut Lionel Lourit verfasserin aut Damien Loizeau verfasserin aut Tania Le Pivert-Jolivet verfasserin aut Guillaume Lequertier verfasserin aut Aurelie Moussi-Soffys verfasserin aut Masanao Abe verfasserin aut Tatsuaki Okada verfasserin aut Tomohiro Usui verfasserin aut Satoru Nakazawa verfasserin aut Takanao Saiki verfasserin aut Satoshi Tanaka verfasserin aut Fuyuto Terui verfasserin aut Makoto Yoshikawa verfasserin aut Sei-ichiro Watanabe verfasserin aut Yuichi Tsuda verfasserin aut In Earth, Planets and Space SpringerOpen, 2015 75(2023), 1, Seite 19 (DE-627)353898597 (DE-600)2087663-4 18805981 nnns volume:75 year:2023 number:1 pages:19 https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/article/57f64037694b45f1a81189f70a674247 kostenfrei https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/toc/1880-5981 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 75 2023 1 19 |
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10.1186/s40623-022-01754-8 doi (DE-627)DOAJ088764826 (DE-599)DOAJ57f64037694b45f1a81189f70a674247 DE-627 ger DE-627 rakwb eng QB275-343 QE1-996.5 Aiko Nakato verfasserin aut Variations of the surface characteristics of Ryugu returned samples 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract Hayabusa2 Ryugu Curation Returned samples Classification Geography. Anthropology. Recreation G Geodesy Geology Toru Yada verfasserin aut Masahiro Nishimura verfasserin aut Kasumi Yogata verfasserin aut Akiko Miyazaki verfasserin aut Kana Nagashima verfasserin aut Kentaro Hatakeda verfasserin aut Kazuya Kumagai verfasserin aut Yuya Hitomi verfasserin aut Hiromichi Soejima verfasserin aut Jean-Pierre Bibring verfasserin aut Cedric Pilorget verfasserin aut Vincent Hamm verfasserin aut Rosario Brunetto verfasserin aut Lucie Riu verfasserin aut Lionel Lourit verfasserin aut Damien Loizeau verfasserin aut Tania Le Pivert-Jolivet verfasserin aut Guillaume Lequertier verfasserin aut Aurelie Moussi-Soffys verfasserin aut Masanao Abe verfasserin aut Tatsuaki Okada verfasserin aut Tomohiro Usui verfasserin aut Satoru Nakazawa verfasserin aut Takanao Saiki verfasserin aut Satoshi Tanaka verfasserin aut Fuyuto Terui verfasserin aut Makoto Yoshikawa verfasserin aut Sei-ichiro Watanabe verfasserin aut Yuichi Tsuda verfasserin aut In Earth, Planets and Space SpringerOpen, 2015 75(2023), 1, Seite 19 (DE-627)353898597 (DE-600)2087663-4 18805981 nnns volume:75 year:2023 number:1 pages:19 https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/article/57f64037694b45f1a81189f70a674247 kostenfrei https://doi.org/10.1186/s40623-022-01754-8 kostenfrei https://doaj.org/toc/1880-5981 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 75 2023 1 19 |
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Aiko Nakato @@aut@@ Toru Yada @@aut@@ Masahiro Nishimura @@aut@@ Kasumi Yogata @@aut@@ Akiko Miyazaki @@aut@@ Kana Nagashima @@aut@@ Kentaro Hatakeda @@aut@@ Kazuya Kumagai @@aut@@ Yuya Hitomi @@aut@@ Hiromichi Soejima @@aut@@ Jean-Pierre Bibring @@aut@@ Cedric Pilorget @@aut@@ Vincent Hamm @@aut@@ Rosario Brunetto @@aut@@ Lucie Riu @@aut@@ Lionel Lourit @@aut@@ Damien Loizeau @@aut@@ Tania Le Pivert-Jolivet @@aut@@ Guillaume Lequertier @@aut@@ Aurelie Moussi-Soffys @@aut@@ Masanao Abe @@aut@@ Tatsuaki Okada @@aut@@ Tomohiro Usui @@aut@@ Satoru Nakazawa @@aut@@ Takanao Saiki @@aut@@ Satoshi Tanaka @@aut@@ Fuyuto Terui @@aut@@ Makoto Yoshikawa @@aut@@ Sei-ichiro Watanabe @@aut@@ Yuichi Tsuda @@aut@@ |
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Variations of the surface characteristics of Ryugu returned samples |
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Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract |
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Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract |
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Abstract Hayabusa2 spacecraft successfully collected rock samples from the surface of C-type near-Earth asteroid 162173 Ryugu through two touchdowns and brought them back to Earth in 2020. At the Extraterrestrial Sample Curation Center in JAXA, we performed initial description of all samples to obtain fundamental information and prepare the database for sample allocation. We propose morphological classifications for the returned samples based on the initial description of 205 grains described in the first 6 months. The returned samples can be distinguished by four morphological characteristics: dark, glossy, bright, and white. According to coordinated study to provide an initial description and detailed investigation by scanning electron microscopy and X-ray diffraction analysis in this study, these features reflect the differences in the degree of space weathering and mineral assemblages. The degree of space weathering of the four studied grain types is heterogeneous: weak for A0042 (dark group) and C0041 (white group); moderate for C0094 (glossy); and severe for A0017 (bright). The white phase, which is the mineral characteristic of the white group grains, is identified as large carbonate minerals. This is the first effort to classify Ryugu returned samples into distinct categories. Based on these results, researchers can estimate sample characteristics only from the information on the JAXA curation public database. It will be an important reference for sample selection for further investigation. Graphical Abstract |
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