Evidence map›Paper›PMID 40124850›Full record

ReviewSpace science reviews2025

Understanding the Formation of Saturn's Regular Moons in the Context of Giant Planet Moons Formation Scenarios.

Michel Blanc, Aurélien Crida, Yuhito Shibaike, Sebastien Charnoz, Maryame El Moutamid, Paul Estrada, Olivier Mousis, Julien Salmon, Antoine Schneeberger, Pierre Vernazza

Abstract readReview
In one paragraph

Review in Space science reviews, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing 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

2 citing papers in PubMed.

  1. Deuterated water and the formation of the satellites of Uranus.Proceedings of the National Academy of Sciences of the United States of America · 2026
    Article
  2. 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

10 authors.

Michel BlancResearch Institute in Astrophysics and Planetology, Toulouse, France.ORCID 0000-0002-1290-7350
Aurélien CridaObservatoire de la Côte d'Azur, Université Côte d'Azur, Nice, France.ORCID 0000-0002-1293-9782
Yuhito ShibaikeNational Astronomical Observatory of Japan, Tokyo, Japan.ORCID 0000-0003-2993-5312
Sebastien CharnozInstitut de Physique du Globe de Paris, Paris, France.ORCID 0000-0002-7442-491X
Maryame El MoutamidDepartment of Astronomy, Cornell University, New York, USA.ORCID 0000-0002-4416-8011
Paul EstradaNASA Ames Research Center, California, USA.ORCID 0000-0002-1132-5594
Olivier MousisLaboratoire d'Astrophysique de Marseille, Marseille, France.ORCID 0000-0001-5323-6453
Julien SalmonIMCCE, Observatoire de Paris, Paris, France.ORCID 0000-0002-5977-3724
Antoine SchneebergerLaboratoire d'Astrophysique de Marseille, Marseille, France.ORCID 0000-0002-3289-2432
Pierre VernazzaLaboratoire d'Astrophysique de Marseille, Marseille, France.ORCID 0000-0002-2564-6743

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

This article explores the different formation scenarios of the Kronian moons system in the context of a highly dissipative Saturn, with the objective of identifying the most likely of these scenarios. First, we review the diversity of objects - moons and rings - orbiting solar system giant planets, and the diversity of their architectures, which formation scenarios must reproduce. We then identify in this broader context the specific features of the Saturn system, such as the particularly large spectrum of its moon masses, the uniqueness of Titan and the presence of both dense and tenuous rings, before discussing the applicability of the different giant planet moon formation scenarios to the Saturn case. We discuss each of the most relevant scenarios and their respective merits. Finally, we tentatively propose a "favorite" scenario and we identify the key observations to be made by future space missions and/or Earth-based telescopic observations to validate this scenario or possibly alternative ones.

Indexed as

Formation of moonsMigration of moonsMoons of SaturnRings of Saturn

Identifiers

PMID40124850
PMCPMC11925992

What OpenQuestion holds

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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 OpenQuestion graph.