Evidence map›Paper›PMID 41188253›Full record

ArticleNature communications2025

Bennu and Ryugu constituents from samples IR analyses and potential source of terrestrial planets' ingredients.

C Pilorget, T Okada, J-P Bibring, D Loizeau, K Hatakeda, L Nardelli, L Riu, R Sheppard, T Jiang, M Mahlke and 17 more

Abstract read
In one paragraph

Article in Nature communications, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing 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

1 citing paper in PubMed.

  1. Article
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

27 authors.

C PilorgetInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France. cedric.pilorget@universite-paris-saclay.fr.ORCID http://orcid.org/0000-0002-7759-9854
T OkadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0001-6381-8107
J-P BibringInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
D LoizeauInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
K HatakedaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
L NardelliInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.ORCID http://orcid.org/0009-0007-0609-0560
L RiuESAC, Camino Bajo del Castillo s/n, Madrid, Spain.
R SheppardInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
T JiangInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
M MahlkeInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
R BrunettoInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.ORCID http://orcid.org/0000-0003-3001-9362
D BakloutiInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.ORCID http://orcid.org/0000-0002-2754-7829
R FukaiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
M AbeInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
A Aléon-ToppaniInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
Y EnokidoInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
V HammInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
S KawasakiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
C LantzInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.ORCID http://orcid.org/0000-0003-0974-4770
A MiyazakiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
A Moussi-SoffysCentre National d'Etudes Spatiales, Toulouse, France.
M NishimuraInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0003-3143-8171
F PouletInstitut d'Astrophysique Spatiale, Université Paris-Saclay, CNRS, Orsay, France.
R TaharaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.
T UsuiInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-4653-293X
T YadaInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-7971-510X
K YogataInstitute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.ORCID http://orcid.org/0000-0002-3717-9185

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Samples collected on carbonaceous asteroids and preserved from terrestrial alteration are key witnesses of the early evolution of the Solar System. Here we present the results of the characterization, by the near-IR hyperspectral microscope MicrOmega within the ISAS/JAXA curation center, of the samples returned from the Bennu asteroid by the OSIRIS-REx mission. We compare these samples to those from Ryugu, analyzed with the same instrument and at the same facility, using gram-scale quantities of material. We demonstrate that Bennu and Ryugu samples exhibit similar near-IR diagnostic spectral properties, from the centimetre down to the sub-millimetre scale. A wide variety of compounds are detected within a similar phyllosilicate-rich matrix, including diverse carbonates, H

Identifiers

PMID41188253
PMCPMC12586576

What Socratic holds

Textmetadata
LicenceCC BY-NC-ND
Read underepoch 390

Registered trials

None linked

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.