Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars
By C. Oze, Mukul Sharma. 2005
280 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Environmental Chemistry
View Paper: https://www.semanticscholar.org/paper/64d96aeca2ecf5d5b5cdb36963cfaf19c4d6b628
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In Astronomy and Astrophysics
- Matthias Grott
- A. Morschhauser
- H. Lammer
- Ernst Hauber
- Brendon K. Chastain
- P. Odert
- Ö. Karatekin
- E. Chassefière
Citations in the corpus
- Methane clathrate hydrates as a potential source for martian atmospheric methane (2007, background): “, 2004), (2) low-temperature alteration and serpentinization of basalts (Oze and Sharma, 2005), (3) comet or meteorite impacts (Kress and McKay, 2004), and (4) atmospheric reactions (Bar-Nun and Dimitrov, 2006).”
- Titan's methane cycle (2006, background): “Such a process has been studied for Earth, and has been applied to Mars to explain the presence of methane on that planet (Atreya et al., 2004; Formisano et al., 2004; Atreya, 2005; Atreya et al., 2006; Oze and Sharma, 2005).”
- Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, methodology): “2006), or through serpentinization followed by the conversion of H2 in CH4 (Oze and Sharma 2005).”