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Title:
Biogenic Methane, Hydrogen Escape, and the Irreversible Oxidation of Early Earth
Authors:
Catling, David C.; Zahnle, Kevin J.; McKay, Christopher P.
Affiliation:
AA(Mail Stop 245-3, Space Science Division, NASA Ames Research Center, Moffett Field, CA 94035, USA.; SETI Institute, Mountain View, CA 94043, USA.), AB(Mail Stop 245-3, Space Science Division, NASA Ames Research Center, Moffett Field, CA 94035, USA.), AC(Mail Stop 245-3, Space Science Division, NASA Ames Research Center, Moffett Field, CA 94035, USA.)
Publication:
Science, Volume 293, Issue 5531, pp. 839-843 (2001). (Sci Homepage)
Publication Date:
08/2001
Category:
GEOCHEM PHYS
Origin:
SCIENCE
DOI:
10.1126/science.1061976
Bibliographic Code:
2001Sci...293..839C

Abstract

The low O2 content of the Archean atmosphere implies that methane should have been present at levels ~102 to 103 parts per million volume (ppmv) (compared with 1.7 ppmv today) given a plausible biogenic source. CH4 is favored as the greenhouse gas that countered the lower luminosity of the early Sun. But abundant CH4 implies that hydrogen escapes to space (↑space) orders of magnitude faster than today. Such reductant loss oxidizes the Earth. Photosynthesis splits water into O2 and H, and methanogenesis transfers the H into CH4. Hydrogen escape after CH4 photolysis, therefore, causes a net gain of oxygen [CO2 + 2H2O --> CH4 + 2O2 --> CO2 + O2 + 4H(↑space)]. Expected irreversible oxidation (~1012 to 1013 moles oxygen per year) may help explain how Earth's surface environment became irreversibly oxidized.
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