Self-oxidation of the atmospheres of rocky planets with implications for the origin of life
Anders Johansen (University of Copenhagen), Eloi Camprubi (University, of Texas Rio Grande Valley), Elishevah van Kooten (University of Copenhagen),, Jens Hoeijmakers (Lund University)

TL;DR
This study models how rocky planet atmospheres self-oxidize over time, becoming CO2 and H2O dominated, which influences the potential pathways for the origin of life and the availability of prebiotic molecules.
Contribution
It demonstrates that atmospheric self-oxidation occurs regardless of initial composition, affecting prebiotic chemistry and emphasizing CO2 as the primary carbon source for early metabolism.
Findings
Atmospheric H escapes within tens of millions of years due to stellar XUV radiation.
Rocky planet atmospheres tend to become CO2 and H2O dominated over time.
Lightning is inefficient at producing HCN, but NO and dust may supply fixed nitrogen.
Abstract
Rocky planets may acquire a primordial atmosphere by outgassing of volatiles from their magma ocean. The distribution of O between HO, CO and CO in chemical equilibrium subsequently changes significantly with decreasing temperature. We explore here two chemical models: one where CH and NH are assumed to be irrevocably destroyed by photolysis, and one where these molecules persist. In the first case, we show that CO cannot co-exist with HO, since CO oxidizes at low temperatures to form CO and H. In both cases, H escapes from the thermosphere within a few ten million years by absorption of stellar XUV radiation. This escape drives an atmospheric self-oxidation process whereby rocky planet atmospheres become dominated by CO and HO, regardless of their initial oxidation state at outgassing. HCN is considered a potential precursor of prebiotic compounds…
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Taxonomy
TopicsAstro and Planetary Science · Methane Hydrates and Related Phenomena · Marine and environmental studies
