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Origin and evolution of the atmospheres of early Venus, Earth and Mars

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Figure

Table 1 Main atmospheric species present in Venus’ (Oyamo et al. 1980), Earth’s (NOAA Earth System Re-search Laboratory: https://www.esrl.noaa.gov/) and Mars’ ((Mahaffy et al
Fig. 1 Expected rotation-based EUV enhancement factor normalized to that of today’s solar level (after Tu etal
Fig. 2 Total mass of accumulated H2-envelopes within the Hill sphere as a function of time according toprotoatmosphere evolution simulations by Stökl et al
Fig. 3 Illustration of planetestimals and planetary embryos that accrete to protoplanets in a few up to tens ofMyr (e.g., Safronov 1969; Wetherill 1980; Elkins-Tanton 2012).
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