Evidence map›Paper›PMID 37810170›Full record

ReviewSpace science reviews2023

Origin and Evolution of Enceladus's Tidal Dissipation.

Francis Nimmo, Marc Neveu, Carly Howett

Open access · hybridAbstract readReview
PubMed Full text at PMC Publisher
In one paragraph

Review in Space science reviews, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.

0numbers the graph read from it
0cells of the map it votes in
7citing papers in PubMed
3.2field-weighted citation impact, top 8% of its field
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

7 citing papers in PubMed, 18 citations in OpenAlex.

  1. Review
  2. Rocky Planets as Heat Engines.Space science reviews · 2026
    Review
  3. Review
  4. Article
  5. Review
  6. Review
  7. 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

3 authors at 3 institutions in 2 countries.

Francis NimmoDept. Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064 USA.ORCID 0000-0003-3573-5915
Marc NeveuDept. Astronomy, University of Maryland, College Park, MD 20742 USA.
Carly HowettDept. Physics, Oxford University, Oxford, OX1 3PU UK.
Goddard Space Flight Center · USPlanetary Science Institute · USUniversity of Oxford · GB

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Enceladus possesses a subsurface ocean beneath a conductive ice shell. Based on shell thickness models, the estimated total conductive heat loss from Enceladus is 25-40 GW; the measured heat output from the South Polar Terrain (SPT) is 4-19 GW. The present-day SPT heat flux is of order

Indexed as

AstrometryImpact fluxOrbital evolutionResonance lockingSatellites of SaturnTidal heating

Identifiers

PMID37810170
PMCPMC10558398
OpenAlexW4387407533

What OpenQuestion 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 OpenQuestion graph.