Evidence map›Paper›PMID 42802152›Full record

ArticleNature communications2026

Gradual Destruction of Refractory Stardust in Alkali Brines on Asteroid Bennu.

Pierre Haenecour, Jessica J Barnes, Elias Bloch, Lucas R Smith, Dolores Hill, Daniel P Glavin, Jason P Dworkin, Harold C Connolly, Dante S Lauretta

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

9 authors.

Pierre HaenecourLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA. haenecour@arizona.edu.ORCID http://orcid.org/0000-0001-5671-5388
Jessica J BarnesLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-7151-1014
Elias BlochLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0001-8494-1892
Lucas R SmithLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-8798-2988
Dolores HillLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-0744-702X
Daniel P GlavinSolar System Exploration Division, NASA Goddard Space Flight Center (GSFC), Greenbelt, MD, USA.ORCID http://orcid.org/0000-0001-7779-7765
Jason P DworkinSolar System Exploration Division, NASA Goddard Space Flight Center (GSFC), Greenbelt, MD, USA.ORCID http://orcid.org/0000-0002-3961-8997
Harold C ConnollyLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-1803-5098
Dante S LaurettaLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID http://orcid.org/0000-0002-2597-5950

Funding

National Aeronautics and Space Administration (NASA) 80NSSC23M0179National Aeronautics and Space Administration (NASA) NNH09ZDA007O
6 · The paper itself

Abstract

Carbonaceous asteroids preserve presolar grains-refractory stardust that predates the Solar System-recording both their stellar origins and subsequent alteration on their parent asteroids. Here we examine the distribution of presolar grains and isotopically anomalous organic matter in mottled particles from samples returned by the OSIRIS-REx mission from asteroid Bennu. Although the mottled samples contain organic matter with carbon and nitrogen isotopic compositions similar to those of other Bennu samples, they lack presolar silicate or oxide grains and show a markedly reduced abundance of presolar silicon carbide. In this work, we show that these findings are consistent with the slow destruction of silicon carbide grains during late-stage alteration by a low-temperature, oxidizing, alkaline brine. These brines, coinciding with evaporite salt formation, selectively erased chemically robust presolar phases while preserving isotopically anomalous organic matter. This shows that evolved aqueous fluids can fundamentally alter the presolar record of primitive asteroids.

Identifiers

PMID42802152
PMCPMC13616931

What Socratic holds

Textmetadata
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.