Evidence map›Paper›PMID 42213852›Full record

ArticleScience advances2026

When wet meets dry: An Ivuna-like impactor triggered volatile loss on the angrite parent body.

Ke Zhu 朱柯, Qi Chen, Tetsuya Yokoyama, Akira Yamaguchi, Audrey Bouvier, Lu Chen

Abstract read
In one paragraph

Article in Science advances, 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

6 authors.

Ke Zhu 朱柯State Key Laboratory of Geological Processes and Mineral Resources, Hubei Key Laboratory of Planetary Geology and Deep-Space Exploration, School of Earth and Planetary Sciences, China University of Geosciences, Wuhan 430074, China.ORCID 0000-0003-3613-7239
Qi ChenCenter for Advanced Radiation Sources, The University of Chicago, Chicago, IL, USA.
Tetsuya YokoyamaDepartment of Earth and Planetary Sciences, Institute of Science Tokyo, Tokyo 152-8551, Japan.ORCID 0000-0003-2247-7232
Akira YamaguchiNational Institute of Polar Research, Tachikawa, Tokyo 190-8518, Japan.ORCID 0000-0001-5140-7853
Audrey BouvierBayerisches Geoinstitut, University of Bayreuth, Universitatsstrasse 30, Bayreuth 95447, Germany.ORCID 0000-0002-8303-3419
Lu ChenWuhan SampleSolution Analytical Technology Co. Ltd., Wuhan, China.ORCID 0000-0001-5434-873X

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Angrite meteorites remain the "driest" known planetary materials in the Solar System. Recent mineralogical and oxygen (O) isotope data suggest that the angrite parent body (APB) experienced a major impact, raising questions about the identity of the impactor. We report high-precision mass-independent chromium (ε

Identifiers

PMID42213852
PMCPMC13220875

What Socratic holds

Textmetadata
LicenceCC BY
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.