Sluggish hydrodynamic escape of early martian atmosphere with reduced chemical compositions
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DOI: 10.1016/j.icarus.2020.113740
Abstract: Abstract Proto-Mars growing within the solar nebula may have maintained both the hydrogen-dominated solar component and the impact degassed component enriched in H2, CH4 and CO as a proto-atmosphere. Such a proto-atmosphere would experience hydrodynamic… read more here.
Keywords: escape; escape early; hydrodynamic escape; early martian ... See more keywords