A warm early Mars with a large northern ocean and a CO2-H2 greenhouse can generate precipitation, runoff, and erosion rates consistent with valley network formation.
(2014), Remote life-detection criteria, habitable zone boundaries, and the frequency of Earth-like planets around M and late K stars
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Climate simulations of early Mars with estimated precipitation, runoff, and erosion rates
A warm early Mars with a large northern ocean and a CO2-H2 greenhouse can generate precipitation, runoff, and erosion rates consistent with valley network formation.