Published December 16, 2022
| Version v1
Journal article
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Oxygen isotopes of anhydrous primary minerals show kinship between asteroid Ryugu and comet 81P/Wild2
Creators
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Kawasaki, Noriyuki1
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Nagashima, Kazuhide2
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Sakamoto, Naoya1
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Matsumoto, Toru3
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Bajo, Ken-Ichi1
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Wada, Sohei1
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Igami, Yohei3
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Miyake, Akira3
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Noguchi, Takaaki3
- Yamamoto, Daiki4
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Russell, Sara S.5
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Abe, Yoshinari6
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Aléon, Jérôme7
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Alexander, Conel M.8
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Amari, Sachiko9
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Amelin, Yuri10
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Bizzarro, Martin11
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Bouvier, Audrey12
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Carlson, Richard W.8
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Chaussidon, Marc13
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Dauphas, Nicolas14
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Davis, Andrew M.14
- 1. Hokkaido University
- 2. University of Hawai'i at Mānoa
- 3. Kyoto University
- 4. Tokyo Institute of Technology
- 5. Natural History Museum
- 6. Tokyo Denki University
- 7. Sorbonne Université
- 8. Carnegie Institution for Science
- 9. Washington University in St. Louis
- 10. Chinese Academy of Sciences
- 11. University of Copenhagen
- 12. Universität Bayreuth
- 13. Centre National de la Recherche Scientifique
- 14. University of Chicago
Description
The extraterrestrial materials returned from asteroid (162173) Ryugu consist predominantly of low-temperature aqueously formed secondary minerals and are chemically and mineralogically similar to CI (Ivuna-type) carbonaceous chondrites. Here, we show that high-temperature anhydrous primary minerals in Ryugu and CI chondrites exhibit a bimodal distribution of oxygen isotopic compositions: 16O-rich (associated with refractory inclusions) and 16O-poor (associated with chondrules). Both the 16O-rich and 16O-poor minerals probably formed in the inner solar protoplanetary disk and were subsequently transported outward. The abundance ratios of the 16O-rich to 16O-poor minerals in Ryugu and CI chondrites are higher than in other carbonaceous chondrite groups but are similar to that of comet 81P/Wild2, suggesting that Ryugu and CI chondrites accreted in the outer Solar System closer to the accretion region of comets.
Notes
Data availability
All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials.Files
sciadv.ade2067.pdf
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(34.3 MB)
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Additional details
Identifiers
- DOI
- 10.1126/sciadv.ade2067
- Other
- oai:uchicago.tind.io:11055
Funding
- Japan Society for the Promotion of Science