Published November 8, 2023
| Version v1
Journal article
Open
Water circulation in Ryugu asteroid affected the distribution of nucleosynthetic isotope anomalies in returned sample
Creators
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Yokoyama, Tetsuya1
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Wadhwa, Meenakshi2
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Iizuka, Tsuyoshi3
- Rai, Vinai2
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Gautam, Ikshu1
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Hibiya, Yuki3
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Masuda, Yuki1
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Haba, Makiko K.1
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Fukai, Ryota4
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Hines, Rebekah2
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Phelan, Nicole2
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Abe, Yoshinari5
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Aléon, Jérôme6
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O'D. Alexander, Conel M.7
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Amari, Sachiko8
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Amelin, Yuri9
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Bajo, Ken-Ichi10
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Bizzarro, Martin11
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Bouvier, Audrey12
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Carlson, Richard W.7
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Chaussidon, Marc13
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Choi, Byeon-Gak14
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Dauphas, Nicolas15
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Davis, Andrew M.15
- 1. Tokyo Institute of Technology
- 2. Arizona State University
- 3. The University of Tokyo
- 4. ISAS/JSEC
- 5. Tokyo Denki University
- 6. Sorbonne Université
- 7. Carnegie Institution for Science
- 8. Washington University in St. Louis
- 9. Chinese Academy of Sciences
- 10. Hokkaido University
- 11. University of Copenhagen
- 12. Universität Bayreuth
- 13. Université Paris Cité
- 14. Seoul National University
- 15. University of Chicago
Description
Studies of material returned from Cb asteroid Ryugu have revealed considerable mineralogical and chemical heterogeneity, stemming primarily from brecciation and aqueous alteration. Isotopic anomalies could have also been affected by delivery of exogenous clasts and aqueous mobilization of soluble elements. Here, we show that isotopic anomalies for mildly soluble Cr are highly variable in Ryugu and CI chondrites, whereas those of Ti are relatively uniform. This variation in Cr isotope ratios is most likely due to physicochemical fractionation between 54Cr-rich presolar nanoparticles and Cr-bearing secondary minerals at the millimeter-scale in the bulk samples, likely due to extensive aqueous alteration in their parent bodies that occurred 5:2þ11::84 Ma after Solar System birth. In contrast, Ti isotopes were marginally affected by this process. Our results show that isotopic heterogeneities in asteroids are not all nebular or accretionary in nature but can also reflect element redistribution by water.
Notes
Data availability
All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials. Data of Hayabusa2 sample and other data from the mission are available at the DARTS archive at www.darts.isas.jaxa.jp/curation/hayabusa2 and www.darts.isas.jaxa.jp/planet/project/hayabusa2/.
Files
sciadv.adi7048.pdf
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(2.8 MB)
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Additional details
Identifiers
- DOI
- 10.1126/sciadv.adi7048
- Other
- oai:uchicago.tind.io:11037
Funding
- Japan Society for the Promotion of Science
- 18H01258
- Japan Society for the Promotion of Science
- 19H00715
- Japan Society for the Promotion of Science
- 21KK0057
- Japan Society for the Promotion of Science
- 22H00170
- Japan Society for the Promotion of Science
- 21KK0058