title: Oxygenic photosynthesis and the oxidation state of Mars.
abstract: The oxidation state of the Earth's surface is one of the most obvious indications of the effect of life on this planet.  The surface of Mars is highly oxidized, as evidenced by its red color, but the connection to life is less apparent.  Two possibilities can be considered.  First, the oxidant may be photochemically produced in the atmosphere.  In this case the fundamental source of O2 is the loss of H2 to space and the oxidant produced is H2O2.  This oxidant would accumulate on the surface and thereby destroy any organic material and other reductants to some depth.  Recent models suggest that diffusion limits this depth to a few meters.  An alternative source of oxgyen is biological oxygen production followed by sequestration of organic material in sediments--as on the Earth.  In this case, the net oxidation of the surface was determined billions of years ago when Mars was a more habitable planet and oxidative conditions could persist to great depths, over 100 m.  Below this must be a compensating layer of biogenic organic material.  Insight into the nature of past sources of oxidation on Mars will require searching for organics in the Martian subsurface and sediments.
authors.affiliation: NASA Ames Research Center, Moffett Field, CA 94035, USA.
authors.forename: H
authors.initials: H
authors.lastname: Hartman
authors.forename: C P
authors.initials: CP
authors.lastname: McKay
mesh_terms: D001272:Atmosphere; D018559:Exobiology; D006859:Hydrogen / Q000737:chemistry; D006861:Hydrogen Peroxide / Q000737:chemistry*; D018535:Mars; D010084:Oxidation-Reduction; D010100:Oxygen / Q000737:chemistry*; D010777:Photochemistry; D010782:Photolysis; D010788:Photosynthesis; D012987:Soil; D014867:Water / Q000737:chemistry*
chemical_list: D012987:Soil; D014867:Water; D006859:Hydrogen; D006861:Hydrogen Peroxide; D010100:Oxygen