Evidence map›Paper›PMID 42736286›Full record

ArticleNature communications2026

Ryugu and Bennu preserve primordial isotopic heterogeneity absent from the meteorite record.

Martin Bizzarro, Martin Schiller, Elishevah van Kooten, Isaac J Onyett, Wei Dai, Yuki Masuda, James N Connelly, Frédéric Moynier, Tetsuya Yokoyama, Maria Schönbächler and 4 more

Abstract read
In one paragraph

Article in Nature communications, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing 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.

3 · Its place in the literature

Who cites it

0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

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

14 authors.

Martin BizzarroCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark. bizzarro@sund.ku.dk.ORCID http://orcid.org/0000-0001-9966-2124
Martin SchillerCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0003-4149-0627
Elishevah van KootenCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0003-3333-4421
Isaac J OnyettSchool of Earth Sciences, University of Bristol, Bristol, UK.
Wei DaiCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0002-7218-0448
Yuki MasudaCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
James N ConnellyCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
Frédéric MoynierInstitut de Physique du Globe de Paris, Université de Paris Cité, Paris, France.ORCID http://orcid.org/0000-0003-4321-5581
Tetsuya YokoyamaDepartment of Earth and Planetary Sciences, Institute of Science Tokyo, Tokyo, Japan.ORCID http://orcid.org/0000-0003-2247-7232
Maria SchönbächlerInstitute for Geochemistry and Petrology, ETH Zürich, Zürich, Switzerland.ORCID http://orcid.org/0000-0003-4304-214X
Jessica J BarnesLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-7151-1014
Ann N NguyenAstromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, USA.ORCID http://orcid.org/0000-0002-0442-1991
Harold C ConnollyLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-1803-5098
Dante S LaurettaCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.

Funding

EC | EC Seventh Framework Programm | FP7 Ideas: European Research Council (FP7-IDEAS-ERC - Specific Programme: "Ideas" Implementing the Seventh Framework Programme of the European Community for Research, Technological Development and Demonstration Activities (2007 to 2013)) 833275Villum Fonden (Villum Foundation) 54476
6 · The paper itself

Abstract

Ivuna-type (CI) carbonaceous chondrites are commonly used as proxies for the composition of the planet-forming disk because their chemical abundances resemble those of the solar photosphere. However, their isotopic uniformity may reflect pervasive alteration and isotopic averaging rather than preservation of the earliest Solar System reservoirs. Here we show that samples returned from the asteroids Ryugu and Bennu preserve isotopic heterogeneity in major planet-building elements, including magnesium, silicon, and iron, that is absent from CI chondrites and unresolved in other meteorites. These signatures reveal isotopically distinct components that are absent from, or homogenized in, known CI chondrites. We infer that Bennu and Ryugu retain a record of primordial isotopic diversity that was not completely homogenized during disk and parent-body processing. Thus, returned asteroid samples provide access to previously unsampled Solar System material that preserves early isotopic components not fully represented in the meteorite record.

Identifiers

PMID42736286
PMCPMC13575244

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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.