Water circulation in Ryugu asteroid affected the distribution of nucleosynthetic isotope anomalies in returned sample-Reference-Cited by-全球学者库

Water circulation in Ryugu asteroid affected the distribution of nucleosynthetic isotope anomalies in returned sample

Published:2023-11-10 Issue:45 Volume:9 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Yokoyama Tetsuya¹^ORCID,Wadhwa Meenakshi²^ORCID,Iizuka Tsuyoshi³^ORCID,Rai Vinai²,Gautam Ikshu¹^ORCID,Hibiya Yuki⁴^ORCID,Masuda Yuki¹^ORCID,Haba Makiko K.¹^ORCID,Fukai Ryota⁵^ORCID,Hines Rebekah²^ORCID,Phelan Nicole²^ORCID,Abe Yoshinari⁶^ORCID,Aléon Jérôme⁷^ORCID,Alexander Conel M. O’D.⁸^ORCID,Amari Sachiko⁹¹⁰^ORCID,Amelin Yuri¹¹^ORCID,Bajo Ken-ichi¹²^ORCID,Bizzarro Martin¹³^ORCID,Bouvier Audrey¹⁴^ORCID,Carlson Richard W.⁸^ORCID,Chaussidon Marc¹⁵^ORCID,Choi Byeon-Gak¹⁶^ORCID,Dauphas Nicolas¹⁷^ORCID,Davis Andrew M.¹⁷^ORCID,Di Rocco Tommaso¹⁸^ORCID,Fujiya Wataru¹⁹^ORCID,Hidaka Hiroshi²⁰^ORCID,Homma Hisashi²¹^ORCID,Hoppe Peter²²^ORCID,Huss Gary R.²³^ORCID,Ichida Kiyohiro²⁴^ORCID,Ireland Trevor²⁵^ORCID,Ishikawa Akira¹^ORCID,Itoh Shoichi²⁶^ORCID,Kawasaki Noriyuki¹²^ORCID,Kita Noriko T.²⁷^ORCID,Kitajima Koki²⁷^ORCID,Kleine Thorsten²⁸^ORCID,Komatani Shintaro²⁴^ORCID,Krot Alexander N.²³^ORCID,Liu Ming-Chang²⁹,McKeegan Kevin D.²⁹^ORCID,Morita Mayu²⁴^ORCID,Motomura Kazuko³⁰^ORCID,Moynier Frédéric¹⁵^ORCID,Nakai Izumi³¹^ORCID,Nagashima Kazuhide²³^ORCID,Nguyen Ann³²^ORCID,Nittler Larry⁸^ORCID,Onose Morihiko²⁴^ORCID,Pack Andreas¹⁸^ORCID,Park Changkun³³^ORCID,Piani Laurette³⁴^ORCID,Qin Liping³⁵,Russell Sara³⁶^ORCID,Sakamoto Naoya³⁷^ORCID,Schönbächler Maria³⁸^ORCID,Tafla Lauren²⁹^ORCID,Tang Haolan³⁵,Terada Kentaro³⁹^ORCID,Terada Yasuko⁴⁰^ORCID,Usui Tomohiro⁵^ORCID,Wada Sohei¹²^ORCID,Walker Richard J.⁴¹^ORCID,Yamashita Katsuyuki⁴²^ORCID,Yin Qing-Zhu⁴³^ORCID,Yoneda Shigekazu⁴⁴^ORCID,Young Edward D.²⁹^ORCID,Yui Hiroharu⁴⁵^ORCID,Zhang Ai-Cheng⁴⁶^ORCID,Nakamura Tomoki⁴⁷^ORCID,Naraoka Hiroshi⁴⁸^ORCID,Noguchi Takaaki²⁶^ORCID,Okazaki Ryuji⁴⁸^ORCID,Sakamoto Kanako⁵^ORCID,Yabuta Hikaru⁴⁹^ORCID,Abe Masanao⁵^ORCID,Miyazaki Akiko⁵^ORCID,Nakato Aiko⁵^ORCID,Nishimura Masahiro⁵^ORCID,Okada Tatsuaki⁵^ORCID,Yada Toru⁵^ORCID,Yogata Kasumi⁵^ORCID,Nakazawa Satoru⁵^ORCID,Saiki Takanao⁵^ORCID,Tanaka Satoshi⁵^ORCID,Terui Fuyuto⁵⁰^ORCID,Tsuda Yuichi⁵^ORCID,Watanabe Sei-ichiro²⁰^ORCID,Yoshikawa Makoto⁵^ORCID,Tachibana Shogo⁵¹^ORCID,Yurimoto Hisayoshi¹²^ORCID

Affiliation:

1. Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.

2. School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85281, USA.

3. Department of Earth and Planetary Science, The University of Tokyo, Tokyo 113-0033, Japan.

4. Research Center for Advanced Science and Technology, The University of Tokyo, Tokyo 153-0041, Japan.

5. ISAS/JSEC, JAXA, Sagamihara, 252-5210, Japan.

6. Graduate School of Engineering, Tokyo Denki University, Tokyo 120-8551, Japan.

7. Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, Museum National d'Histoire Naturelle, CNRS UMR 7590, IRD, 75005 Paris, France.

8. Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, 20015, USA.

9. McDonnell Center for the Space Sciences and Physics Department, Washington University, St. Louis, MO 63130, USA.

10. Geochemical Research Center, The University of Tokyo, Tokyo 113-0033, Japan.

11. Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, GD 510640, China.

12. Department of Natural History Sciences, Hokkaido University, Sapporo 001-0021, Japan.

13. Centre for Star and Planet Formation, GLOBE Institute, University of Copenhagen, Copenhagen, K 1350, Denmark.

14. Bayerisches Geoinstitut, Universität Bayreuth, Bayreuth, 95447, Germany.

15. Université Paris Cité, Institut de physique du globe de Paris, CNRS, 75005 Paris, France.

16. Department of Earth Science Education, Seoul National University, Seoul 08826, Republic of Korea.

17. Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA.

18. Faculty of Geosciences and Geography, University of Göttingen, Göttingen, D-37077, Germany.

19. Faculty of Science, Ibaraki University, Mito 310-8512, Japan.

20. Department of Earth and Planetary Sciences, Nagoya University, Nagoya 464-8601, Japan.

21. Osaka Application Laboratory, SBUWDX, Rigaku Corporation, Osaka 569-1146, Japan.

22. Max Planck Institute for Chemistry, Mainz, 55128, Germany.

23. Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i at Mānoa, Honolulu, HI 96822, USA.

24. Analytical Technology, Horiba Techno Service Co. Ltd., Kyoto 601-8125, Japan.

25. School of Earth and Environmental Sciences, The University of Queensland, St. Lucia, QLD 4072, Australia.

26. Division of Earth and Planetary Sciences, Kyoto University, Kyoto 606-8502, Japan.

27. Department of Geoscience, University of Wisconsin-Madison, Madison, WI 53706, USA.

28. Max Planck Institute for Solar System Research, 37077, Göttingen, Germany.

29. Department of Earth, Planetary, and Space Sciences, UCLA, Los Angeles, CA 90095, USA.

30. Thermal Analysis, Rigaku Corporation, Tokyo 196-8666, Japan.

31. Department of Applied Chemistry, Tokyo University of Science, Tokyo 162-8601, Japan.

32. Astromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA.

33. Earth-System Sciences, Korea Polar Research Institute, Incheon 21990, Korea.

34. Centre de Recherches Pétrographiques et Géochimiques, CNRS - Université de Lorraine, 54500 Nancy, France.

35. CAS Key Laboratory of Crust-Mantle Materials and Environments, University of Science and Technology of China, School of Earth and Space Sciences, Anhui 230026, China.

36. Department of Earth Sciences, Natural History Museum, London, SW7 5BD, UK.

37. Isotope Imaging Laboratory, Creative Research Institution, Hokkaido University, Sapporo 001-0021, Japan.

38. Institute for Geochemistry and Petrology, Department of Earth Sciences, ETH Zurich, 8092 Zurich, Switzerland.

39. Department of Earth and Space Science, Osaka University, Osaka 560-0043, Japan.

40. Spectroscopy and Imaging, Japan Synchrotron Radiation Research Institute, Hyogo 679-5198, Japan.

41. Department of Geology, University of Maryland, College Park, MD 20742, USA.

42. Graduate School of Natural Science and Technology, Okayama University, Okayama 700-8530, Japan.

43. Department of Earth and Planetary Sciences, University of California, Davis, CA 95616, USA.

44. Department of Science and Engineering, National Museum of Nature and Science, Tsukuba 305-0005, Japan.

45. Department of Chemistry, Tokyo University of Science, Tokyo 162-8601, Japan.

46. School of Earth Sciences and Engineering, Nanjing University, Nanjing 210023, China.

47. Department of Earth Science, Tohoku University, Sendai 980-8578, Japan.

48. Department of Earth and Planetary Sciences, Kyushu University, Fukuoka 819-0395, Japan.

49. Earth and Planetary Systems Science Program, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.

50. Kanagawa Institute of Technology, Atsugi 243-0292, Japan.

51. UTokyo Organization for Planetary and Space Science, The University of Tokyo, Tokyo 113-0033, Japan.

Abstract

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 54 Cr-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 5.2 − 1.4 + 1.8 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.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Link

https://www.science.org/doi/pdf/10.1126/sciadv.adi7048

Reference87 articles.

1. Pebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to Earth

2. Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu

3. Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites

4. On the origin and evolution of the asteroid Ryugu: A comprehensive geochemical perspective

5. Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A common isotopic reservoir for amoeboid olivine aggregates (AOAs) and calcium-aluminum-rich inclusions (CAIs) revealed by Ti and Cr isotopic compositions;Earth and Planetary Science Letters;2024-02