Impact Degassing of H₂ on Early Mars and its Effect on the Climate System

Abstract Impacts on early Mars can produce H 2 and CH 4 in the thermal plume. In a thick CO 2 atmosphere, collision‐induced absorptions between CO 2 ‐H 2 and CO 2 ‐CH 4 can boost the greenhouse effect. We construct a simple model of the impact history of Mars and show that for a variety of impactor types and CO 2 surface pressures >0.5 bars, postimpact surface temperatures due to H 2 alone can exceed the melting point of water for much longer periods of time than from the dissipation of the heat derived from the impactor's kinetic energy. This longer timescale is set by hydrogen escape rather than radiation to space. Cumulatively, the Noachian surface may have been above the melting point of water for millions of years by this mechanism. These greatly extended postimpact warm environments may have played a larger role in the erosion and mineralogy of the surface than previously thought and may partly explain some of the observed fluvial features.

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