The Astrophysical Journal Letters (Jan 2023)

The Magnesium Isotope Composition of Samples Returned from Asteroid Ryugu

  • Martin Bizzarro,
  • Martin Schiller,
  • Tetsuya Yokoyama,
  • Yoshinari Abe,
  • Jérôme Aléon,
  • Conel M. O’D. Alexander,
  • Sachiko Amari,
  • Yuri Amelin,
  • Ken-ichi Bajo,
  • Audrey Bouvier,
  • Richard W. Carlson,
  • Marc Chaussidon,
  • Byeon-Gak Choi,
  • Nicolas Dauphas,
  • Andrew M. Davis,
  • Tommaso Di Rocco,
  • 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,
  • Shoichi Itoh,
  • Noriyuki Kawasaki,
  • Noriko T. Kita,
  • Kouki Kitajima,
  • Thorsten Kleine,
  • Shintaro Komatani,
  • Alexander N. Krot,
  • Ming-Chang Liu,
  • Yuki Masuda,
  • Mayu Morita,
  • Fréderic Moynier,
  • Kazuko Motomura,
  • Izumi Nakai,
  • Kazuhide Nagashima,
  • David Nesvorný,
  • Ann Nguyen,
  • Larry Nittler,
  • Morihiko Onose,
  • Andreas Pack,
  • Changkun Park,
  • Laurette Piani,
  • Liping Qin,
  • Sara S. Russell,
  • Naoya Sakamoto,
  • Maria Schönbächler,
  • Lauren Tafla,
  • Haolan Tang,
  • Kentaro Terada,
  • Yasuko Terada,
  • Tomohiro Usui,
  • Sohei Wada,
  • Meenakshi Wadhwa,
  • Richard J. Walker,
  • Katsuyuki Yamashita,
  • Qing-Zhu Yin,
  • Shigekazu Yoneda,
  • Edward D. Young,
  • 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/10.3847/2041-8213/ad09d9
Journal volume & issue
Vol. 958, no. 2
p. L25

Abstract

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The nucleosynthetic isotope composition of planetary materials provides a record of the heterogeneous distribution of stardust within the early solar system. In 2020 December, the Japan Aerospace Exploration Agency Hayabusa2 spacecraft returned to Earth the first samples of a primitive asteroid, namely, the Cb-type asteroid Ryugu. This provides a unique opportunity to explore the kinship between primitive asteroids and carbonaceous chondrites. We report high-precision μ ^26 Mg* and μ ^25 Mg values of Ryugu samples together with those of CI, CM, CV, and ungrouped carbonaceous chondrites. The stable Mg isotope composition of Ryugu aliquots defines μ ^25 Mg values ranging from –160 ± 20 ppm to –272 ± 30 ppm, which extends to lighter compositions relative to Ivuna-type (CI) and other carbonaceous chondrite groups. We interpret the μ ^25 Mg variability as reflecting heterogeneous sampling of a carbonate phase hosting isotopically light Mg ( μ ^25 Mg ∼ –1400 ppm) formed by low temperature equilibrium processes. After correcting for this effect, Ryugu samples return homogeneous μ ^26 Mg* values corresponding to a weighted mean of 7.1 ± 0.8 ppm. Thus, Ryugu defines a μ ^26 Mg* excess relative to the CI and CR chondrite reservoirs corresponding to 3.8 ± 1.1 and 11.9 ± 0.8 ppm, respectively. These variations cannot be accounted for by in situ decay of ^26 Al given their respective ^27 Al/ ^24 Mg ratios. Instead, it requires that Ryugu and the CI and CR parent bodies formed from material with a different initial ^26 Al/ ^27 Al ratio or that they are sourced from material with distinct Mg isotope compositions. Thus, our new Mg isotope data challenge the notion that Ryugu and CI chondrites share a common nucleosynthetic heritage.

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