The Planetary Science Journal (Jan 2023)

The Oxygen Isotopic Composition of Samples Returned from Asteroid Ryugu with Implications for the Nature of the Parent Planetesimal

  • Haolan Tang,
  • Edward D. Young,
  • Lauren Tafla,
  • Andreas Pack,
  • Tommaso Di Rocco,
  • Yoshinari Abe,
  • Jérôme Aléon,
  • Conel M. O’D. Alexander,
  • Sachiko Amari,
  • Yuri Amelin,
  • Ken-ichi Bajo,
  • Martin Bizzarro,
  • Audrey Bouvier,
  • Richard W. Carlson,
  • Marc Chaussidon,
  • Byeon-Gak Choi,
  • Nicolas Dauphas,
  • Andrew M. Davis,
  • Wataru Fujiya,
  • Ryota Fukai,
  • Ikshu Gautam,
  • Makiko K. Haba,
  • Yuki Hibiya,
  • Hiroshi Hidaka,
  • Hisashi Homma,
  • Peter Hoppe,
  • Gary R. Huss,
  • Kiyohiro Ichida,
  • Tsuyoshi Iizuka,
  • Trevor R. Ireland,
  • Akira Ishikawa,
  • Motoo Ito,
  • Shoichi Itoh,
  • Noriyuki Kawasaki,
  • Noriko T. Kita,
  • Kouki Kitajima,
  • Thorsten Kleine,
  • Shintaro Komatani,
  • Alexander N. Krot,
  • Ming-Chang Liu,
  • Yuki Masuda,
  • Kevin D. McKeegan,
  • Mayu Morita,
  • Kazuko Motomura,
  • Frédéric Moynier,
  • Kazuhide Nagashima,
  • Izumi Nakai,
  • Ann Nguyen,
  • Larry Nittler,
  • Morihiko Onose,
  • Changkun Park,
  • Laurette Piani,
  • Liping Qin,
  • Sara S. Russell,
  • Naoya Sakamoto,
  • Maria Schönbächler,
  • Kentaro Terada,
  • Yasuko Terada,
  • Tomohiro Usui,
  • Sohei Wada,
  • Meenakshi Wadhwa,
  • Richard J. Walker,
  • Katsuyuki Yamashita,
  • Qing-Zhu Yin,
  • Tetsuya Yokoyama,
  • Shigekazu Yoneda,
  • Hiroharu Yui,
  • Ai-Cheng Zhang,
  • Tomoki Nakamura,
  • Hiroshi Naraoka,
  • Takaaki Noguchi,
  • Ryuji Okazaki,
  • Kanako Sakamoto,
  • Hikaru Yabuta,
  • Masanao Abe,
  • Akiko Miyazaki,
  • Aiko Nakato,
  • Masahiro Nishimura,
  • Tatsuaki Okada,
  • Toru Yada,
  • Kasumi Yogata,
  • Satoru Nakazawa,
  • Takanao Saiki,
  • Satoshi Tanaka,
  • Fuyuto Terui,
  • Yuichi Tsuda,
  • Sei-ichiro Watanabe,
  • Makoto Yoshikawa,
  • Shogo Tachibana,
  • Hisayoshi Yurimoto

DOI
https://doi.org/10.3847/PSJ/acea62
Journal volume & issue
Vol. 4, no. 8
p. 144

Abstract

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We present oxygen isotopic analyses of fragments of the near-Earth C _b -type asteroid Ryugu returned by the Hayabusa2 spacecraft that reinforce the close correspondence between Ryugu and CI chondrites. Small differences between Ryugu samples and CI chondrites in ${{\rm{\Delta }}}^{{\prime} 17}{\rm{O}}$ can be explained at least in part by contamination of the latter by terrestrial water. The discovery that a randomly sampled C-complex asteroid is composed of CI-chondrite-like rock, combined with thermal models for formation prior to significant decay of the short-lived radioisotope ^26 Al, suggests that if lithified at the time of alteration, the parent body was small (≪50 km radius). If the parent planetesimal was large (>50 km in radius), it was likely composed of high-permeability, poorly lithified sediment rather than consolidated rock.

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