A hydrogen-rich early Earth atmosphere
- PMID: 15817816
- DOI: 10.1126/science.1106983
A hydrogen-rich early Earth atmosphere
Abstract
We show that the escape of hydrogen from early Earth's atmosphere likely occurred at rates slower by two orders of magnitude than previously thought. The balance between slow hydrogen escape and volcanic outgassing could have maintained a hydrogen mixing ratio of more than 30%. The production of prebiotic organic compounds in such an atmosphere would have been more efficient than either exogenous delivery or synthesis in hydrothermal systems. The organic soup in the oceans and ponds on early Earth would have been a more favorable place for the origin of life than previously thought.
Comment in
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Atmospheric science. Rethinking Earth's early atmosphere.Science. 2005 May 13;308(5724):962-3. doi: 10.1126/science.1113157. Science. 2005. PMID: 15890865 No abstract available.
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Comment on "A hydrogen-rich early Earth atmosphere".Science. 2006 Jan 6;311(5757):38; author reply 38. doi: 10.1126/science.1118412. Science. 2006. PMID: 16400134
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