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Record W4413409775 · doi:10.1038/s41550-025-02631-6

The variety and origin of materials accreted by Bennu’s parent asteroid

2025· article· en· W4413409775 on OpenAlexaff
Jessica Barnes, A. N. Nguyen, F. A. J. Abernethy, Ken‐ichi Bajo, David V. Bekaert, Elias Bloch, G. A. Brennecka, H. Busemann, John Cowpe, S A Crowther, Mattias Ek, Lydia Fawcett, Manuela A. Fehr, I. A. Franchi, Evelyn Füri, J. D. Gilmour, M. M. Grady, R. C. Greenwood, Pierre Haenecour, Noriyuki Kawasaki, Piers Koefoed, Daniela Krietsch, L. Le, Katarzyna Liszewska, C. Maden, J. Malley, Yves Marrocchi, Bernard Marty, Lara Meyer, T. Peretyazhko, Laurette Piani, Jan Render, S. S. Russell, Miriam Rüfenacht, Naoya Sakamoto, Maria Schönbächler, Quinn R. Shollenberger, Lowell R. Smith, Cristina A. Thomas, A. B. Verchovsky, Johan Villeneuve, Kun Wang, K. C. Welten, Josh Wimpenny, E. A. Worsham, Hisayoshi Yurimoto, Laurent Zimmermann, X. Zhao, C. M. O'd. Alexander, Marghaleray Amini, Allison A. Baczynski, P. A. Bland, L. E. Borg, R. Burgess, M. W. Caffee, L. C. Chaves, P. L. Clay, Jason P. Dworkin, Dionysis I. Foustoukos, D. P. Glavin, V. E. Hamilton, D. H. Hill, Christopher H. House, G. R. Huss, T. R. Ireland, C. E. Jilly‐Rehak, Fred Jourdan, L. P. Keller, T. S. Kruijer, Voon Hui Lai, T. J. McCoy, K. Nagashima, K. Nishiizumi, R. C. Ogliore, I. J. Ong, Steven M. Reddy, William D.A. Rickard, S. Sandford, David W. Saxey, Nicholas E. Timms, Dominique Weis, Z. E. Wilbur, T. J. Zega, D. N. DellaGiustina, C. W. V. Wolner, H. C. Connolly, D. S. Lauretta

Bibliographic record

VenueNature Astronomy · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsUniversity of OttawaUniversity of British Columbia
FundersLawrence Livermore National LaboratoryScience and Technology Facilities CouncilJohnson Space CenterNuclear Safety and Security CommissionU.S. Department of EnergyCentre National d’Etudes SpatialesGordon and Betty Moore FoundationPlanetary Science DivisionNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsAsteroidAstrobiologyVariety (cybernetics)GeologyPhysicsComputer scienceArtificial intelligence

Abstract

fetched live from OpenAlex

The first bodies to form in the Solar System acquired their materials from stars, the presolar molecular cloud and the protoplanetary disk. Asteroids that have not undergone planetary differentiation retain evidence of these primary accreted materials. However, geologic processes such as hydrothermal alteration can dramatically change their bulk mineralogy, isotopic compositions and chemistry. Here we analyse the elemental and isotopic compositions of samples from asteroid Bennu to uncover the sources and types of material accreted by its parent body. We show that some primary accreted materials escaped the extensive aqueous alteration that occurred on the parent asteroid, including presolar grains from ancient stars, organic matter from the outer Solar System or molecular cloud, refractory solids that formed close to the Sun, and dust enriched in neutron-rich Ti isotopes. We find Bennu to be richer in isotopically anomalous organic matter, anhydrous silicates, and light isotopes of K and Zn than its closest compositional counterparts, asteroid Ryugu and Ivuna-type (CI) carbonaceous chondrite meteorites. We propose that the parent bodies of Bennu, Ryugu and CI chondrites formed from a common but spatially and/or temporally heterogeneous reservoir of materials in the outer protoplanetary disk.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.716
Threshold uncertainty score0.367

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.003
GPT teacher head0.225
Teacher spread0.222 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations21
Published2025
Admission routes1
Has abstractyes

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