Evidence map›Paper›PMID 40834084›Full record

ArticleScience advances2025

Core metamorphism controls the dynamic habitability of mid-sized ocean worlds-The case of Ceres.

Samuel W Courville, Julie C Castillo-Rogez, Mohit Melwani Daswani, Jordyn Robare, Joseph G O'Rourke

Abstract read
In one paragraph

Article in Science advances, 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. Review
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

5 authors.

Samuel W CourvilleSchool of Earth and Space Exploration, Arizona State University, 781 Terrace Mall, Tempe, AZ 85287, USA.ORCID 0000-0002-9539-1301
Julie C Castillo-RogezJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91011, USA.ORCID 0000-0003-0400-1038
Mohit Melwani DaswaniJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91011, USA.ORCID 0000-0002-4611-3209
Jordyn RobareSchool of Molecular Sciences, Arizona State University, 781 Terrace Mall, Tempe, AZ 85287, USA.ORCID 0000-0001-9133-8485
Joseph G O'RourkeSchool of Earth and Space Exploration, Arizona State University, 781 Terrace Mall, Tempe, AZ 85287, USA.ORCID 0000-0002-1180-996X

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Ceres's surface mineralogy and density structure indicate an aqueous past. Observations from the Dawn mission revealed that Ceres likely hosted a global subsurface ocean in its early history, which was the site of pervasive aqueous alteration of accreted material. Subsurface environmental constraints inferred from Ceres's surface mineralogy, combined with Ceres's high abundance of carbon, suggest that the dwarf planet may have been habitable for microbial life. We present a coupled chemical and thermal evolution model tracking Ceres's interior aqueous environment through time. If the rocky interior reached ≳550 K, then fluids released by rock metamorphism would have promoted conditions favorable for habitability by introducing redox disequilibrium into the ocean, a source of chemical energy for chemotrophs. We find that this period would have been between ~0.5 and 2 billion years after Ceres's formation. Since then, Ceres's ocean has likely become a cold, concentrated brine with fewer sources of energy, making it less likely to be habitable at present.

Identifiers

PMID40834084
PMCPMC12366696

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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 OpenQuestion graph.