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Record W4413409805 · doi:10.1038/s41561-025-01741-0

Mineralogical evidence for hydrothermal alteration of Bennu samples

2025· article· en· W4413409805 on OpenAlexaff
T. J. Zega, T. J. McCoy, S. S. Russell, L. P. Keller, Z. Gainsforth, S. A. Singerling, Venkateswara Rao Manga, C. S. Harrison, G. Libourel, B. S. Prince, Cristina A. Thomas, A. J. King, Marc Portail, Vincent Guigoz, Valerie Tu, L. Le, M. S. Thompson, M. C. Benner, N. Kerrison, Jessica Barnes, I. J. Ong, Pierre Haenecour, L. C. Chaves, Lucas Smith, Melissa K. Kontogiannis, N. Santiago, D. H. Hill, Z. Zeszut, K. Domanik, Yao‐Jen Chang, C. M. Corrigan, S. Ray, L. R. Wardell, T. Gooding, T. R. Rose, H. C. Bates, P. F. Schofield, N. V. Almeida, T. Salge, Jens Najorka, Laura Seifert, N. G. Lunning, K. Righter, A. N. Nguyen, Frank E. Brenker, S. A. Eckley, Jason P. Dworkin, R. H. Jones, Scott A. Sandford, Matthew A. Marcus, Hans A. Bechtel, G. Domínguez, Hisayoshi Yurimoto, Noriyuki Kawasaki, Ken‐ichi Bajo, Naoya Sakamoto, Pierre-Marie Zanetta, Shogo Tachibana, H. Busemann, V. E. Hamilton, I. A. Franchi, M. M. Grady, R. C. Greenwood, K. T. Tait, Nicholas E. Timms, P. A. Bland, Fred Jourdan, Steven M. Reddy, William D.A. Rickard, David W. Saxey, László Vincze, H. C. Connolly, D. S. Lauretta

Bibliographic record

VenueNature Geoscience · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsRoyal Ontario Museum
FundersPlanetary Science DivisionBasic Energy SciencesScience and Technology Facilities CouncilJohnson Space CenterOffice of ScienceDr. Rolf M. Schwiete StiftungCentre National d’Etudes SpatialesSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of EnergyNuclear Safety and Security CommissionGordon and Betty Moore FoundationAgence Nationale de la RechercheNational Aeronautics and Space AdministrationDeutsche ForschungsgemeinschaftUK Research and InnovationNational Science Foundation
KeywordsHydrothermal circulationGeologyGeochemistryMineralogyPaleontology

Abstract

fetched live from OpenAlex

Samples of asteroid (101955) Bennu delivered by the OSIRIS-REx mission offer the opportunity to study pristine planetary materials unchanged by exposure to the terrestrial environment. Here we use a combination of X-ray diffraction and various electron microscopy techniques to explore the detailed mineralogy of Bennu samples and determine the alteration history of the planetesimal protolith from which they originated. The samples consist largely of hydrated sheet-silicate minerals, namely nanoscale serpentine and saponite of varied grain size, which are decorated with micro- to nanoscale Fe-sulfides, magnetite and carbonates. We observe sheet silicates parallel and normal to sulfide surfaces and as inclusions in sulfides; sulfur-rich veins transecting the sheet-silicate matrix; zoned carbonates and phosphates and sulfide and magnetite grains exhibiting embayment. The mineralogical evidence indicates alteration of accreted minerals by a fluid that evolved with time, leading to etching, dissolution and reprecipitation. Sulfide compositions indicate alteration at ~25 °C, similar to conditions inferred for asteroid (162173) Ryugu and Ivuna-type (CI) chondrite meteorites. The fluid probably evolved from neutral to alkaline, culminating with the precipitation of highly soluble salts. We conclude that Bennu's protolith comprised mainly nanometre to micrometre silicates, with fewer chondrules and calcium-aluminium-rich inclusions than those of most chondrite groups.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.016
Threshold uncertainty score0.032

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.000

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 head0.024
GPT teacher head0.317
Teacher spread0.293 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
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

Citations28
Published2025
Admission routes1
Has abstractno

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