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Ryugu's nucleosynthetic heritage from the outskirts of the Solar System.
Hopp, Timo; Dauphas, Nicolas; Abe, Yoshinari; Aléon, Jérôme; O'D Alexander, Conel M; Amari, Sachiko; Amelin, Yuri; Bajo, Ken-Ichi; Bizzarro, Martin; Bouvier, Audrey; Carlson, Richard W; Chaussidon, Marc; Choi, Byeon-Gak; Davis, Andrew M; Di Rocco, Tommaso; Fujiya, Wataru; Fukai, Ryota; Gautam, Ikshu; Haba, Makiko K; Hibiya, Yuki; Hidaka, Hiroshi; Homma, Hisashi; Hoppe, Peter; Huss, Gary R; Ichida, Kiyohiro; Iizuka, Tsuyoshi; Ireland, Trevor R; Ishikawa, Akira; Ito, Motoo; Itoh, Shoichi; Kawasaki, Noriyuki; Kita, Noriko T; Kitajima, Kouki; Kleine, Thorsten; Komatani, Shintaro; Krot, Alexander N; Liu, Ming-Chang; Masuda, Yuki; McKeegan, Kevin D; Morita, Mayu; Motomura, Kazuko; Moynier, Frédéric; Nakai, Izumi; Nagashima, Kazuhide; Nesvorný, David; Nguyen, Ann; Nittler, Larry; Onose, Morihiko; Pack, Andreas; Park, Changkun.
Afiliación
  • Hopp T; Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, Chicago, IL 60637, USA.
  • Dauphas N; Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, Chicago, IL 60637, USA.
  • Abe Y; Graduate School of Engineering Materials Science and Engineering, Tokyo Denki University, Tokyo 120-8551, Japan.
  • Aléon J; Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, Museum National d'Histoire Naturelle, CNRS UMR 7590, IRD, 75005 Paris, France.
  • O'D Alexander CM; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.
  • Amari S; McDonnell Center for the Space Sciences and Physics Department, Washington University, St. Louis, MO 63130, USA.
  • Amelin Y; Geochemical Research Center, The University of Tokyo, Tokyo 113-0033, Japan.
  • Bajo KI; Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, GD 510640, China.
  • Bizzarro M; Department of Natural History Sciences, Hokkaido University, Sapporo 001-0021, Japan.
  • Bouvier A; Centre for Star and Planet Formation, GLOBE Institute, University of Copenhagen, Copenhagen K 1350, Denmark.
  • Carlson RW; Bayerisches Geoinstitut, Universität Bayreuth, Bayreuth 95447, Germany.
  • Chaussidon M; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.
  • Choi BG; Université Paris Cité, Institut de physique du globe de Paris, CNRS, 75005 Paris, France.
  • Davis AM; Department of Earth Science Education, Seoul National University, Seoul 08826, Republic of Korea.
  • Di Rocco T; Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, Chicago, IL 60637, USA.
  • Fujiya W; Faculty of Geosciences and Geography, University of Göttingen, Göttingen D-37077, Germany.
  • Fukai R; Faculty of Science, Ibaraki University, Mito 310-8512, Japan.
  • Gautam I; Institute of Space and Astronautical Science/JAXA Space Exploration Center, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.
  • Haba MK; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Hibiya Y; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Hidaka H; Department of General Systems Studies, The University of Tokyo, Tokyo 153-0041, Japan.
  • Homma H; Research Center for Advanced Science and Technology, The University of Tokyo, Tokyo 153-8904, Japan.
  • Hoppe P; Department of Earth and Planetary Sciences, Nagoya University, Nagoya 464-8601, Japan.
  • Huss GR; Osaka Application Laboratory, SBUWDX, Rigaku Corporation, Osaka 569-1146, Japan.
  • Ichida K; Max Planck Institute for Chemistry, Mainz 55128, Germany.
  • Iizuka T; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, Honolulu, HI 96822, USA.
  • Ireland TR; Analytical Technology Division, Horiba Techno Service Co. Ltd., Kyoto 601-8125, Japan.
  • Ishikawa A; Department of Earth and Planetary Science, The University of Tokyo, Tokyo 113-0033, Japan.
  • Ito M; School of Earth and Environmental Sciences, The University of Queensland, St. Lucia, QLD 4072, Australia.
  • Itoh S; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Kawasaki N; Kochi Institute for Core Sample Research, JAMSTEC, Kochi 783-8502, Japan.
  • Kita NT; Department of Earth and Planetary Sciences, Kyoto University, Kyoto 606-8502, Japan.
  • Kitajima K; Department of Natural History Sciences, Hokkaido University, Sapporo 001-0021, Japan.
  • Kleine T; Department of Geoscience, University of Wisconsin-Madison, Madison, WI 53706, USA.
  • Komatani S; Department of Geoscience, University of Wisconsin-Madison, Madison, WI 53706, USA.
  • Krot AN; Max Planck Institute for Solar System Research, 37077 Göttingen, Germany.
  • Liu MC; Analytical Technology Division, Horiba Techno Service Co. Ltd., Kyoto 601-8125, Japan.
  • Masuda Y; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, Honolulu, HI 96822, USA.
  • McKeegan KD; Department of Earth, Planetary, and Space Sciences, UCLA, Los Angeles, CA 90095, USA.
  • Morita M; Lawrence Livermore National Laboratory, Livermore, CA 94550, USA.
  • Motomura K; Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.
  • Moynier F; Department of Earth, Planetary, and Space Sciences, UCLA, Los Angeles, CA 90095, USA.
  • Nakai I; Analytical Technology Division, Horiba Techno Service Co. Ltd., Kyoto 601-8125, Japan.
  • Nagashima K; Thermal Analysis, Rigaku Corporation, Tokyo 196-8666, Japan.
  • Nesvorný D; Université Paris Cité, Institut de physique du globe de Paris, CNRS, 75005 Paris, France.
  • Nguyen A; Thermal Analysis, Rigaku Corporation, Tokyo 196-8666, Japan.
  • Nittler L; Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, Honolulu, HI 96822, USA.
  • Onose M; Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA.
  • Pack A; Astromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Park C; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.
Sci Adv ; 8(46): eadd8141, 2022 Nov 18.
Article en En | MEDLINE | ID: mdl-36264823
ABSTRACT
Little is known about the origin of the spectral diversity of asteroids and what it says about conditions in the protoplanetary disk. Here, we show that samples returned from Cb-type asteroid Ryugu have Fe isotopic anomalies indistinguishable from Ivuna-type (CI) chondrites, which are distinct from all other carbonaceous chondrites. Iron isotopes, therefore, demonstrate that Ryugu and CI chondrites formed in a reservoir that was different from the source regions of other carbonaceous asteroids. Growth and migration of the giant planets destabilized nearby planetesimals and ejected some inward to be implanted into the Main Belt. In this framework, most carbonaceous chondrites may have originated from regions around the birthplaces of Jupiter and Saturn, while the distinct isotopic composition of CI chondrites and Ryugu may reflect their formation further away in the disk, owing their presence in the inner Solar System to excitation by Uranus and Neptune.
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Texto completo: 1 Banco de datos: MEDLINE Idioma: En Año: 2022 Tipo del documento: Article
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Texto completo: 1 Banco de datos: MEDLINE Idioma: En Año: 2022 Tipo del documento: Article