Article in Science advances, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 9 papers.
0numbers the graph read from it
0cells of the map it votes in
9citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it
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.
2 · The registry
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.
PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.
5 · Who and what money
Authors and funding
92 authors.
Ann N NguyenAstromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0002-0442-1991
Prajkta ManeUniversities Space Research Association, Lunar and Planetary Institute, Houston, TX 77058, USA.ORCID 0000-0002-6918-2653
Lindsay P KellerAstromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0003-1560-2939
Laurette PianiCentre de Recherches Pétrographiques et Géochimiques, CNRS - Université de Lorraine, Nancy 54500, France.ORCID 0000-0003-0854-7468
Yoshinari AbeGraduate School of Engineering Materials Science and Engineering, Tokyo Denki University, Tokyo 120-8551, Japan.ORCID 0000-0002-5307-1684
Jérôme AléonInstitut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, Museum National d'Histoire Naturelle, CNRS UMR 7590, IRD, Paris 75005, France.ORCID 0000-0001-5729-0166
Conel M O'D AlexanderEarth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.ORCID 0000-0002-8558-1427
Sachiko AmariMcDonnell Center for the Space Sciences and Physics Department, Washington University, St. Louis, MO 63130, USA.ORCID 0000-0003-4899-0974
Yuri AmelinGuangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, GD 510640, China.ORCID 0000-0001-6719-8937
Ken-Ichi BajoDepartment of Natural History Sciences, IIL, Hokkaido University, Sapporo 001-0021, Japan.ORCID 0000-0002-9013-2730
Martin BizzarroCentre for Star and Planet Formation, GLOBE Institute, University of Copenhagen, Copenhagen K 1350, Denmark.ORCID 0000-0001-9966-2124
Audrey BouvierBayerisches Geoinstitut, Universität Bayreuth, Bayreuth 95447, Germany.ORCID 0000-0002-8303-3419
Richard W CarlsonEarth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.ORCID 0000-0001-7195-2074
Marc ChaussidonUniversité Paris Cités, Institut de physique du globe de Paris, CNRS, Paris 75005, France.ORCID 0000-0001-8475-0690
Byeon-Gak ChoiDepartment of Earth Science Education, Seoul National University, Seoul 08826, Republic of Korea.ORCID 0000-0003-1899-2864
Nicolas DauphasDepartment of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA.ORCID 0000-0002-1330-2038
Andrew M DavisDepartment of the Geophysical Sciences and Enrico Fermi Institute, The University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA.ORCID 0000-0001-7955-6236
Tommaso Di RoccoFaculty of Geosciences and Geography, University of Göttingen, Göttingen D-37077, Germany.ORCID 0000-0003-0417-6364
Andreas PackFaculty of Geosciences and Geography, University of Göttingen, Göttingen D-37077, Germany.ORCID 0000-0002-2618-2768
Changkun ParkEarth System Sciences, Korea Polar Research Institute, Incheon 21990, Korea.ORCID 0000-0002-1206-6803
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.ORCID 0000-0001-5531-7847
Naoya SakamotoIsotope Imaging Laboratory, Creative Research Institution, Hokkaido University, Sapporo 001-0021, Japan.ORCID 0000-0003-2335-1359
Maria SchönbächlerInstitute for Geochemistry and Petrology, Department of Earth Sciences, ETH Zurich, Zurich, Switzerland.ORCID 0000-0003-4304-214X
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.ORCID 0000-0003-0120-1229
Yasuko TeradaSpectroscopy and Imaging, Japan Synchrotron Radiation Research Institute, Hyogo 679-5198, Japan.ORCID 0000-0001-5101-1912
Ryuji OkazakiDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka 819-0395, Japan.ORCID 0000-0003-0177-7527
Kanako SakamotoInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0001-5138-5324
Hikaru YabutaEarth and Planetary Systems Science Program, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.ORCID 0000-0002-4625-5362
Masanao AbeInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0003-4780-800X
Akiko MiyazakiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0001-7427-2285
Aiko NakatoInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0003-2392-1497
Masahiro NishimuraInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0003-3143-8171
Tatsuaki OkadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0001-6381-8107
Toru YadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0002-7971-510X
Kasumi YogataInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0002-3717-9185
Satoru NakazawaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0003-4250-1826
Takanao SaikiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0003-3100-420X
Satoshi TanakaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0002-4874-0417
Yuichi TsudaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0002-9161-6171
Sei-Ichiro WatanabeEarth and Planetary Sciences, Nagoya University, Nagoya 464-8601, Japan.ORCID 0000-0002-5820-2102
Makoto YoshikawaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara 252-5210, Japan.ORCID 0000-0002-3118-7475
Shogo TachibanaUTokyo Organization for Planetary and Space Science, University of Tokyo, Tokyo 113-0033, Japan.ORCID 0000-0002-4603-9440
Hisayoshi YurimotoDepartment of Natural History Sciences, IIL, Hokkaido University, Sapporo 001-0021, Japan.ORCID 0000-0003-0702-0533
Funding
No grant is acknowledged in the PubMed record.
6 · The paper itself
Abstract
Preliminary analyses of asteroid Ryugu samples show kinship to aqueously altered CI (Ivuna-type) chondrites, suggesting similar origins. We report identification of C-rich, particularly primitive clasts in Ryugu samples that contain preserved presolar silicate grains and exceptional abundances of presolar SiC and isotopically anomalous organic matter. The high presolar silicate abundance (104 ppm) indicates that the clast escaped extensive alteration. The 5 to 10 times higher abundances of presolar SiC (~235 ppm), N-rich organic matter, organics with N isotopic anomalies (1.2%), and organics with C isotopic anomalies (0.2%) in the primitive clasts compared to bulk Ryugu suggest that the clasts formed in a unique part of the protoplanetary disk enriched in presolar materials. These clasts likely represent previously unsampled outer solar system material that accreted onto Ryugu after aqueous alteration ceased, consistent with Ryugu's rubble pile origin.
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 OpenQuestion graph.
Abundant presolar grains and primordial organics preserved in carbon-rich exogenous clasts in asteroid Ryugu. · full record | OpenQuestion