ArticleJournal of geophysical research. Planets2021
Vertically Resolved Magma Ocean-Protoatmosphere Evolution: H
Article in Journal of geophysical research. Planets, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 6 papers.
What it found
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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.
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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.
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Who cites it
6 citing papers in PubMed.
- Carbon monoxide dehydrogenase-encoding microorganisms in volcanic astrobiological analogues: an enzyme system to investigate the evolution of life.FEMS microbiology ecology · 2026Review
- Magma Ocean Evolution at Arbitrary Redox State.Journal of geophysical research. Planets · 2024Article
- The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets.Nature communications · 2024Article
- Synergies Between Venus & Exoplanetary Observations: Venus and Its Extrasolar Siblings.Space science reviews · 2023Review
- COJournal of geophysical research. Planets · 2022Article
- Vertically Resolved Magma Ocean-Protoatmosphere Evolution: HJournal of geophysical research. Planets · 2021Article
Corrections and comments
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Authors and funding
7 authors.
Funding
No grant is acknowledged in the PubMed record.
Abstract
The earliest atmospheres of rocky planets originate from extensive volatile release during magma ocean epochs that occur during assembly of the planet. These establish the initial distribution of the major volatile elements between different chemical reservoirs that subsequently evolve via geological cycles. Current theoretical techniques are limited in exploring the anticipated range of compositional and thermal scenarios of early planetary evolution, even though these are of prime importance to aid astronomical inferences on the environmental context and geological history of extrasolar planets. Here, we present a coupled numerical framework that links an evolutionary, vertically resolved model of the planetary silicate mantle with a radiative-convective model of the atmosphere. Using this method, we investigate the early evolution of idealized Earth-sized rocky planets with end-member, clear-sky atmospheres dominated by either H
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