Evidence map›Paper›PMID 39722853›Full record

ArticleJournal of geophysical research. Planets2024

Magma Ocean Evolution at Arbitrary Redox State.

Harrison Nicholls, Tim Lichtenberg, Dan J Bower, Raymond Pierrehumbert

Abstract read
In one paragraph

Article in Journal of geophysical research. Planets, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Review
  2. Review
  3. Review
  4. Discovery of crystalline FeScience advances · 2025
    Article
  5. Magma Ocean Evolution at Arbitrary Redox State.Journal of geophysical research. Planets · 2024
    Article
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

4 authors.

Harrison NichollsAtmospheric Oceanic and Planetary Physics University of Oxford Oxford UK.ORCID https://orcid.org/0000-0002-8368-4641
Tim LichtenbergKapteyn Astronomical Institute University of Groningen Groningen The Netherlands.ORCID https://orcid.org/0000-0002-3286-7683
Dan J BowerCenter for Space and Habitability University of Bern Bern Switzerland.
Raymond PierrehumbertAtmospheric Oceanic and Planetary Physics University of Oxford Oxford UK.ORCID https://orcid.org/0000-0002-5887-1197

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Interactions between magma oceans and overlying atmospheres on young rocky planets leads to an evolving feedback of outgassing, greenhouse forcing, and mantle melt fraction. Previous studies have predominantly focused on the solidification of oxidized Earth-similar planets, but the diversity in mean density and irradiation observed in the low-mass exoplanet census motivate exploration of strongly varying geochemical scenarios. We aim to explore how variable redox properties alter the duration of magma ocean solidification, the equilibrium thermodynamic state, melt fraction of the mantle, and atmospheric composition. We develop a 1D coupled interior-atmosphere model that can simulate the time-evolution of lava planets. This is applied across a grid of fixed redox states, orbital separations, hydrogen endowments, and C/H ratios around a Sun-like star. The composition of these atmospheres is highly variable before and during solidification. The evolutionary path of an Earth-like planet at 1 AU ranges between permanent magma ocean states and solidification within 1 Myr. Recently solidified planets typically host

Indexed as

atmospheresconvectionexoplanetslava planetsmagma oceanssimulation

Identifiers

PMID39722853
PMCPMC11667094

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.