The evolution of the prebiotic atmosphere.
One-dimensional radiative convective and photochemical models are used to estimate the vertical temperature structure and composition of the earth's prebiotic atmosphere.  Greatly enhanced CO2 levels (100-1000 times present) are required to keep the mean surface temperature above freezing in the face of decreased solar luminosity during the earth's early history.  Such high CO2 partial pressures would have affected the atmospheric oxidation state by facilitating the photochemical production of soluble species including H2O2 and H2CO. Oxidation of ferrous iron in the oceans by H2O2 dissolved in rainwater should have kept the atmospheric H2 mixing ratio above 2x10(-4) and the ground-level O2 mixing ratio below 10(-11), regardless of the magnitude of the rate of volcanic release of reduced gases.
Kasting
J F
JF
NASA Ames Research Center, Moffett Field, CA 94035, USA.
D001272:Atmosphere / Q000737:chemistry*; D002245:Carbon Dioxide / Q000032:analysis*; D018534:Earth, Planet; D019418:Evolution, Chemical; D019419:Evolution, Planetary; D006859:Hydrogen / Q000737:chemistry; D006861:Hydrogen Peroxide; D007501:Iron / Q000737:chemistry; D008956:Models, Chemical; D010084:Oxidation-Reduction; D010100:Oxygen / Q000737:chemistry; D010777:Photochemistry; D014867:Water
D014867:Water; D002245:Carbon Dioxide; D006859:Hydrogen; D006861:Hydrogen Peroxide; D007501:Iron; D010100:Oxygen