Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars

@article{Oze2005HaveOW,
  title={Have olivine, will gas: Serpentinization and the abiogenic production of methane on Mars},
  author={C. Oze and Mukul Sharma},
  journal={Geophysical Research Letters},
  year={2005},
  volume={32}
}
[1] Spatial variability of methane (CH4) on Mars suggests the presence of localized subsurface sources. Here, we show that olivine hydration in the Martian regolith and crust may be a major CH4 source, which contributed significantly to the warming of early Mars. Methane production is kinetically and thermodynamically favored during low-T aqueous alteration of olivine-rich rocks. Sustained release of CH4 on present-day Mars may come through the breakdown of ancient CH4 hydrates and from springs… Expand

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