Evidence map›Paper›PMID 41593248›Full record

ArticleScientific reports2026

Possible favored great oxidation event scenario on exoplanets around M-stars with the example of TRAPPIST-1e.

Adam Yassin Jaziri, Nathalie Carrasco, Benjamin Charnay

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Article in Scientific reports, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

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1 · What the graph read from it

What it found

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2 · The registry

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3 · Its place in the literature

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4 · The record

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5 · Who and what money

Authors and funding

3 authors.

Adam Yassin JaziriLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, 78280, Guyancourt, France. yassin.jaziri@latmos.ipsl.fr.
Nathalie CarrascoLATMOS/IPSL, UVSQ Université Paris-Saclay, Sorbonne Université, CNRS, 78280, Guyancourt, France.
Benjamin CharnayLIRA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Cité, 5 place Jules Janssen, 92195, Meudon, France.

Funding

ERC OxyPlanets grant agreement No. 101053033ERC WHIPLASH grant agreement No. 679030
6 · The paper itself

Abstract

The Great Oxidation Event (GOE), which marked the transition from an anoxic to an oxygenated atmosphere, occurred 2.4 billion years ago on Earth, several hundreds of millions of years after the emergence of oxygenic photosynthesis. This long delay implies that specific conditions in terms of biomass productivity and burial were necessary to trigger the GOE. It could be a limiting factor for the development of oxygenated atmospheres on inhabited exoplanets. In this study, we explore the specificities of a terrestrial planet in the habitable zone of an M dwarf for a GOE. Using a 1D coupled photochemical-climate model, we simulate the atmospheric evolution of TRAPPIST-1e, an Earth-like exoplanet, exploring the effect of oxygen sources (biotic or abiotic). Our results show that the stellar energy distribution promotes O[Formula: see text] production at lower O[Formula: see text] concentrations compared to Earth, and the ozone layer on TRAPPIST-1e forms more efficiently. This lowers the threshold for atmospheric oxidation, suggesting that the GOE on TRAPPIST-1e would occur quickly after the rise of oxygenic photosynthesis, up to 1Gyrs earlier than on Earth, and would reach O[Formula: see text] enabling oxygenic respiration and thus the development of animals. We may question whether this is a general behavior around several M-stars. Furthermore, we discuss how the overproduction of ozone could make O[Formula: see text] detection possible using the James Webb Space Telescope, providing a potential method to observe oxygenation signatures on exoplanets in the near future. Previous studies predicted that for an Earth-like atmosphere O[Formula: see text] would require over 150 transits for detection, but our results show that significantly fewer transits could be needed.

Identifiers

PMID41593248
PMCPMC12905277

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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.