ArticleNature astronomy2022
Contribution of Ryugu-like material to Earth's volatile inventory by Cu and Zn isotopic analysis.
Abstract read
In one paragraph
Article in Nature astronomy, 2022. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 10 papers.
0numbers the graph read from it
0cells of the map it votes in
10citing papers in PubMed
–field-weighted citation impact
What it found
Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.
The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.
The trial behind it
Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.
Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.
Who cites it
10 citing papers in PubMed.
- Bennu and Ryugu constituents from samples IR analyses and potential source of terrestrial planets' ingredients.Nature communications · 2025Article
- Martian differentiation history inferred from copper isotopes.Nature communications · 2025Article
- Impact-induced sublimation drives volatile depletion in carbonaceous meteorites.Nature communications · 2025Article
- The variety and origin of materials accreted by Bennu's parent asteroid.Nature astronomy · 2025Article
- The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites.Science advances · 2024Article
- Breunnerite grain and magnesium isotope chemistry reveal cation partitioning during aqueous alteration of asteroid Ryugu.Nature communications · 2024Article
- The origin of 4-Vesta's volatile depletion revealed by the zinc isotopic composition of diogenites.Science advances · 2024Article
- Rubidium isotopic compositions of angrites controlled by extensive evaporation and partial recondensation.Proceedings of the National Academy of Sciences of the United States of America · 2024Article
- Water circulation in Ryugu asteroid affected the distribution of nucleosynthetic isotope anomalies in returned sample.Science advances · 2023Article
- Visualization of nanoscale magnetic domain states in the asteroid Ryugu.Scientific reports · 2023Article
Corrections and comments
PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.
Authors and funding
94 authors.
Marine PaquetUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Frederic MoynierUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Tetsuya YokoyamaDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology; Tokyo 152-8551, Japan.
Wei DaiUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Yan HuUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Yoshinari AbeGraduate School of Engineering Materials Science and Engineering, Tokyo Denki University; Tokyo 120-8551, Japan.
Jérôme AléonInstitut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, Museum National d'Histoire Naturelle, CNRS UMR 7590, IRD; 75005 Paris, France.
Conel M O'D AlexanderEarth and Planets Laboratory, Carnegie Institution for Science; Washington, DC, 20015, USA.
Sachiko AmariMcDonnell Center for the Space Sciences and Physics Department, Washington University; St. Louis, MO 63130, USA.
Yuri AmelinGuangzhou Institute of Geochemistry, Chinese Academy of Sciences; Guangzhou, GD 510640, China.
Ken-Ichi BajoNatural History Sciences, IIL, Hokkaido University; Sapporo 001-0021, Japan.
Martin BizzarroUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Audrey BouvierBayerisches Geoinstitut, Universität Bayreuth; Bayreuth 95447, Germany.
Richard W CarlsonEarth and Planets Laboratory, Carnegie Institution for Science; Washington, DC, 20015, USA.
Marc ChaussidonUniversité Paris Cité, Institut de physique du globe de Paris, CNRS; 75005 Paris, France.
Byeon-Gak ChoiDepartment of Earth Science Education, Seoul National University; Seoul 08826, Republic of Korea.
Nicolas DauphasDepartment of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago 60637, USA.
Andrew M DavisDepartment of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago 60637, USA.
Tommaso Di RoccoFaculty of Geosciences and Geography, University of Göttingen; Göttingen, D-37077, Germany.
Wataru FujiyaFaculty of Science, Ibaraki University; Mito 310-8512, Japan.
Ryota FukaiISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Ikshu GautamDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology; Tokyo 152-8551, Japan.
Makiko K HabaDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology; Tokyo 152-8551, Japan.
Yuki HibiyaGeneral Systems Studies, The University of Tokyo; Tokyo 153-0041, Japan.
Hiroshi HidakaEarth and Planetary Sciences, Nagoya University; Nagoya 464-8601, Japan.
Hisashi HommaOsaka Application Laboratory, SBUWDX, Rigaku Corporation; Osaka 569-1146, Japan.
Peter HoppeMax Planck Institute for Chemistry; Mainz 55128, Germany.
Gary R HussHawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa; Honolulu, HI 96822, USA.
Kiyohiro IchidaAnalytical Technology, Horiba Techno Service Co., Ltd.; Kyoto 601-8125, Japan.
Tsuyoshi IizukaEarth and Planetary Science, The University of Tokyo; Tokyo 113-0033, Japan.
Trevor R IrelandSchool of Earth and Environmental Sciences, The University of Queensland; St Lucia QLD 4072, Australia.
Akira IshikawaDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology; Tokyo 152-8551, Japan.
Motoo ItoKochi Institute for Core Sample Research, JAMSTEC; Kochi 783-8502, Japan.
Shoichi ItohEarth and Planetary Sciences, Kyoto University; Kyoto 606-8502, Japan.
Noriyuki KawasakiNatural History Sciences, IIL, Hokkaido University; Sapporo 001-0021, Japan.
Noriko T KitaGeoscience, University of Wisconsin-Madison; Madison, WI 53706, USA.
Kouki KitajimaGeoscience, University of Wisconsin-Madison; Madison, WI 53706, USA.
Thorsten KleineMax Planck Institute for Solar System Research; 37077 Göttingen, Germany.
Shintaro KomataniAnalytical Technology, Horiba Techno Service Co., Ltd.; Kyoto 601-8125, Japan.
Alexander N KrotHawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa; Honolulu, HI 96822, USA.
Ming-Chang LiuEarth, Planetary, and Space Sciences, UCLA; Los Angeles, CA 90095, USA.
Yuki MasudaDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology; Tokyo 152-8551, Japan.
Kevin D McKeeganEarth, Planetary, and Space Sciences, UCLA; Los Angeles, CA 90095, USA.
Mayu MoritaAnalytical Technology, Horiba Techno Service Co., Ltd.; Kyoto 601-8125, Japan.
Kazuko MotomuraThermal Analysis, Rigaku Corporation; Tokyo 196-8666, Japan.
Izumi NakaiThermal Analysis, Rigaku Corporation; Tokyo 196-8666, Japan.
Kazuhide NagashimaHawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa; Honolulu, HI 96822, USA.
David NesvornýDepartment of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA.
Ann N NguyenAstromaterials Research and Exploration Science, NASA Johnson Space Center; Houston, TX 77058, USA.
Larry NittlerEarth and Planets Laboratory, Carnegie Institution for Science; Washington, DC, 20015, USA.
Morihiko OnoseAnalytical Technology, Horiba Techno Service Co., Ltd.; Kyoto 601-8125, Japan.
Andreas PackFaculty of Geosciences and Geography, University of Göttingen; Göttingen, D-37077, Germany.
Changkun ParkEarth-System Sciences, Korea Polar Research Institute; Incheon 21990, Korea.
Laurette PianiCentre de Recherches Pétrographiques et Géochimiques, CNRS - Université de Lorraine; 54500 Nancy, France.
Liping QinCAS Key Laboratory of Crust-Mantle Materials and Environments, University of Science and Technology of China, School of Earth and Space Sciences; Anhui 230026, China.
Sara S RussellDepartment of Earth Sciences, Natural History Museum; London, SW7 5BD, UK.
Naoya SakamotoIIL, Hokkaido University; Sapporo 001-0021, Japan.
Maria SchönbächlerInstitute for Geochemistry and Petrology, Department of Earth Sciences, ETH Zurich, Zurich, Switzerland.
Lauren TaflaEarth, Planetary, and Space Sciences, UCLA; Los Angeles, CA 90095, USA.
Haolan TangEarth, Planetary, and Space Sciences, UCLA; Los Angeles, CA 90095, USA.
Kentaro TeradaEarth and Space Science, Osaka University; Osaka 560-0043, Japan.
Yasuko TeradaSpectroscopy and Imaging, Japan Synchrotron Radiation Research Institute; Hyogo 679-5198 Japan.
Tomohiro UsuiISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Sohei WadaNatural History Sciences, IIL, Hokkaido University; Sapporo 001-0021, Japan.
Meenakshi WadhwaSchool of Earth and Space Exploration, Arizona State University; Tempe, AZ 85281, USA.
Richard J WalkerGeology, University of Maryland, College Park, MD 20742, USA.
Katsuyuki YamashitaGraduate School of Natural Science and Technology, Okayama University; Okayama 700-8530, Japan.
Qing-Zhu YinEarth and Planetary Sciences, University of California; Davis, CA 95616, USA.
Shigekazu YonedaScience and Engineering, National Museum of Nature and Science; Tsukuba 305-0005, Japan.
Edward D YoungEarth, Planetary, and Space Sciences, UCLA; Los Angeles, CA 90095, USA.
Hiroharu YuiChemistry, Tokyo University of Science; Tokyo 162-8601, Japan.
Ai-Cheng ZhangSchool of Earth Sciences and Engineering, Nanjing University; Nanjing 210023, China.
Tomoki NakamuraDepartment of Earth Science, Tohoku University; Sendai, 980-8578, Japan.
Hiroshi NaraokaDepartment of Earth and Planetary Sciences, Kyushu University; Fukuoka 819-0395, Japan.
Takaaki NoguchiKochi Institute for Core Sample Research, JAMSTEC; Kochi 783-8502, Japan.
Ryuji OkazakiDepartment of Earth and Planetary Sciences, Kyushu University; Fukuoka 819-0395, Japan.
Kanako SakamotoISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Hikaru YabutaEarth and Planetary Systems Science Program, Hiroshima University; Higashi-Hiroshima, 739-8526, Japan.
Masanao AbeISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Akiko MiyazakiISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Aiko NakatoISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Masahiro NishimuraISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Tatsuaki OkadaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Toru YadaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Kasumi YogataISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Satoru NakazawaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Takanao SaikiISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Satoshi TanakaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Fuyuto TeruiKanagawa Institute of Technology; Atsugi 243-0292, Japan.
Yuichi TsudaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Sei-Ichiro WatanabeEarth and Planetary Sciences, Nagoya University; Nagoya 464-8601, Japan.
Makoto YoshikawaISAS/JSEC, JAXA; Sagamihara 252-5210, Japan.
Shogo TachibanaUTokyo Organization for Planetary and Space Science, University of Tokyo; Tokyo 113-0033, Japan.
Hisayoshi YurimotoNatural History Sciences, IIL, Hokkaido University; Sapporo 001-0021, Japan.
Funding
Pilot Program CoreP30ES027792 · NIEHS · UNIVERSITY OF CHICAGO · PI Gokhan M. Mutlu, Gail S Prins · 2017 to 2026
$13.6MEuropean Research Council 101001282NIEHS NIH HHS P30 ES027792
Abstract
Initial analyses showed that asteroid Ryugu's composition is close to CI (Ivuna-like) carbonaceous chondrites -the chemically most primitive meteorites, characterized by near-solar abundances for most elements. However, some isotopic signatures (e.g., Ti, Cr) overlap with other carbonaceous chondrite (CC) groups, so the details of the link between Ryugu and the CI chondrites are not fully clear yet. Here we show that Ryugu and CI chondrites have the same zinc and copper isotopic composition. As the various chondrite groups have very distinct Zn and Cu isotopic signatures, our results point at a common genetic heritage between Ryugu and CI chondrites, ruling out any affinity with other CC groups. Since Ryugu's pristine samples match the solar elemental composition for many elements, their Zn and Cu isotopic compositions likely represent the best estimates of the solar composition. Earth's mass-independent Zn isotopic composition is intermediate between Ryugu/CC and non-carbonaceous chondrites, suggesting a contribution of Ryugu-like material to Earth's budgets of Zn and other moderately volatile elements.
Indexed as
CI chondritesCu isotopesHayabusa2Ryuguvolatile elementsZn isotopes
Identifiers
What Socratic holds
Textmetadata
LicenceTDM
Read underepoch 390
Registered trials
None linked
Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the Socratic graph.