Abiotic Production of Methane in Terrestrial Planets
Open accessAbstract
On Earth, methane is produced mainly by life, and it has been proposed that, under certain conditions, methane detected in an exoplanetary spectrum may be considered a biosignature. Here, we estimate how much methane may be produced in hydrothermal vent systems by serpentinization, its main geological source, using the kinetic properties of the main reactions involved in methane production by serpentinization. Hydrogen production by serpentinization was calculated as a function of the available FeO in the crust, given the current spreading rates. Carbon dioxide is the limiting reactant for methane formation because it is highly depleted in aqueous form in hydrothermal vent systems. We estimated maximum CH4 surface fluxes of 6.8×10(8) and 1.3×10(9) molecules cm(-2) s(-1) for rocky planets with 1 and 5 M⊕, respectively. Using a 1-D photochemical model, we simulated atmospheres with volume mixing ratios of 0.03 and 0.1 CO2 to calculate atmospheric methane concentrations for the maximum production of this compound by serpentinization. The resulting abundances were 2.5 and 2.1 ppmv for 1 M⊕ planets and 4.1 and 3.7 ppmv for 5 M⊕ planets. Therefore, low atmospheric concentrations of methane may be produced by serpentinization. For habitable planets around Sun-like stars with N2-CO2 atmospheres, methane concentrations larger than 10 ppmv may indicate the presence of life.
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CH4 production is further restricted by CO2 availability in the crust, limiting H2/CH4 ratios to ~13.
“Guzmán-Marmolejo et al. (56) argued that CH4 production is further restricted by CO2 availability in the crust, limiting H2/CH4 ratios to ~13.”
From Disequilibrium biosignatures over Earth history and implications for detecting exoplanet life (2018) · cites this paper as [56]
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- Authors
- Guzmán-Marmolejo, A., Segura, A., & Escobar-Briones, E.
- Affiliations
- Instituto de Geofísica (MX)
- NASA Astrobiology Institute (US)
- Instituto de Ciencias del Mar y Limnología (MX)
- Corresponding author
- Segura, Antígona
- Venue
- Astrobiology
- Publisher
- SAGE Publications
- Published
- 2013-06
- Volume
- 13
- Issue
- 6
- Pages
- 550-559
- ISSN
- 1531-1074 (ISSN-L)
- 1557-8070
- PMC
- PMC3689174
- OpenAlex
- W2072484395
- Cited by
- 96
- References
- 66
- Citations by year
- 2026: 1 · 2025: 12 · 2024: 8 · 2023: 8 · 2022: 6 · 2021: 5 · 2020: 8 · 2019: 2 · 2018: 32 · 2017: 9 · 2016: 2 · 2015: 2
- FWCI
- 0.72
- Type
- journal article
- Language
- en
- Open access
- green
- europepmc.org
- Locations
- Astrobiology (publishedVersion)
- Europe PMC (PubMed Central) (publishedVersion)
- PubMed Central (publishedVersion)
- PubMed (publishedVersion)
- Funders
- National Aeronautics and Space Administration (NNH05ZDA001C)
- NASA Astrobiology Institute
- Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
- Keywords
- serpentinization, hydrothermal vents, biosignatures, exoplanet atmospheres, photochemical modeling, habitability
- MeSH terms
- Methane, Models, Theoretical, Planets
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