Evidence map›Paper›PMID 32332725›Full record

ArticleNature communications2020

A magma ocean origin to divergent redox evolutions of rocky planetary bodies and early atmospheres.

Jie Deng, Zhixue Du, Bijaya B Karki, Dipta B Ghosh, Kanani K M Lee

Abstract read
In one paragraph

Article in Nature communications, 2020. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 18 papers.

0numbers the graph read from it
0cells of the map it votes in
18citing 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

18 citing papers in PubMed.

  1. Article
  2. Review
  3. Review
  4. Discovery of crystalline FeScience advances · 2025
    Article
  5. The cosmochemistry of planetary systems.Nature reviews. Chemistry · 2025
    Review
  6. Article
  7. Article
  8. Article
  9. Article
  10. Article
  11. Vestiges of impact-driven three-phase mixing in the chemistry and structure of Earth's mantle.Proceedings of the National Academy of Sciences of the United States of America · 2023
    Article
  12. Narrow range of early habitable Venus scenarios permitted by modeling of oxygen loss and radiogenic argon degassing.Proceedings of the National Academy of Sciences of the United States of America · 2023
    Article
  13. Article
  14. Article
  15. Oxygen controls on magmatism in rocky exoplanets.Proceedings of the National Academy of Sciences of the United States of America · 2021
    Article
  16. The "Water Problem"(Life (Basel, Switzerland) · 2021
    Review
  17. Vertically Resolved Magma Ocean-Protoatmosphere Evolution: HJournal of geophysical research. Planets · 2021
    Article
  18. 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

5 authors.

Jie DengDepartment of Geology and Geophysics, Yale University, New Haven, CT, 06511, USA. jie.deng@aya.yale.edu.ORCID http://orcid.org/0000-0001-5441-2797
Zhixue DuState key Laboratory of Isotope Geochemistry, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, 510640, Guangzhou, China. duzhixue@gig.ac.cn.ORCID http://orcid.org/0000-0002-7716-2994
Bijaya B KarkiSchool of Electrical Engineering and Computer Science, Department of Geology and Geophysics, and Center for Computation and Technology, Louisiana State University, Baton Rouge, LA, 70803, USA.
Dipta B GhoshSchool of Electrical Engineering and Computer Science, Department of Geology and Geophysics, and Center for Computation and Technology, Louisiana State University, Baton Rouge, LA, 70803, USA.
Kanani K M LeeDepartment of Geology and Geophysics, Yale University, New Haven, CT, 06511, USA.ORCID http://orcid.org/0000-0003-3003-4802

Funding

CAS | Guangzhou Institute of Geochemistry, Chinese Academy of Sciences (Guangzhou Institute of Geochemistry) 51Y8340107National Science Foundation (NSF) EAR-1321956National Science Foundation (NSF) EAR-1551348National Science Foundation (NSF) EAR-1764140
6 · The paper itself

Abstract

Magma oceans were once ubiquitous in the early solar system, setting up the initial conditions for different evolutionary paths of planetary bodies. In particular, the redox conditions of magma oceans may have profound influence on the redox state of subsequently formed mantles and the overlying atmospheres. The relevant redox buffering reactions, however, remain poorly constrained. Using first-principles simulations combined with thermodynamic modeling, we show that magma oceans of Earth, Mars, and the Moon are likely characterized with a vertical gradient in oxygen fugacity with deeper magma oceans invoking more oxidizing surface conditions. This redox zonation may be the major cause for the Earth's upper mantle being more oxidized than Mars' and the Moon's. These contrasting redox profiles also suggest that Earth's early atmosphere was dominated by CO

Identifiers

PMID32332725
PMCPMC7181735

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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.