Article in Science advances, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 4 papers.
0numbers the graph read from it
0cells of the map it votes in
4citing 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
91 authors.
Fridolin SpitzerMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.ORCID 0000-0002-6114-0854
Thorsten KleineMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.ORCID 0000-0003-4657-5961
Christoph BurkhardtMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.ORCID 0000-0002-6952-5783
Timo HoppMax Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.ORCID 0000-0002-4056-5431
Tetsuya YokoyamaDepartment of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo 152-8551, Japan.ORCID 0000-0003-2247-7232
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, 75005 Paris, 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, 35 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, 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 Cité, Institut de Physique du Globe de Paris, CNRS, 75005 Paris, 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
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, 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
The isotopic compositions of samples returned from Cb-type asteroid Ryugu and Ivuna-type (CI) chondrites are distinct from other carbonaceous chondrites, which has led to the suggestion that Ryugu/CI chondrites formed in a different region of the accretion disk, possibly around the orbits of Uranus and Neptune. We show that, like for Fe, Ryugu and CI chondrites also have indistinguishable Ni isotope anomalies, which differ from those of other carbonaceous chondrites. We propose that this unique Fe and Ni isotopic composition reflects different accretion efficiencies of small FeNi metal grains among the carbonaceous chondrite parent bodies. The CI chondrites incorporated these grains more efficiently, possibly because they formed at the end of the disk's lifetime, when planetesimal formation was also triggered by photoevaporation of the disk. Isotopic variations among carbonaceous chondrites may thus reflect fractionation of distinct dust components from a common reservoir, implying CI chondrites/Ryugu may have formed in the same region of the accretion disk as other carbonaceous chondrites.
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.