Biology
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p41b..03g&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #P41B-03
Biology
[0456] Biogeosciences / Life In Extreme Environments, [1060] Geochemistry / Planetary Geochemistry, [5220] Planetary Sciences: Astrobiology / Hydrothermal Systems And Weathering On Other Planets, [6225] Planetary Sciences: Solar System Objects / Mars
Scientific paper
Evaluating the stability of organic compounds in the presence of oxidizing agents is essential to assess the potential habitability of present-day Mars. The residence time of CH4, for instance, may be greatly constrained by oxidants proposed to exist in Martian soil and atmosphere, in particular H2O2. Abiotic oxidation processes could play a key role in the removal of CH4 as recent studies suggest that CH4 sequestration in Martian environments occurs more rapidly than previously thought. Since CH4 evolution can be linked to possible subsurface liquid water, the formation of oxidants needs to be investigated under comparable hydrothermal conditions. To examine the possible formation of highly oxidizing hydroxyl radicals on Mars, a series of flow-through hydrothermal experiments involved decomposition of dissolved H2O2 in the presence of Fe-oxides (FeO, Fe3O4) via the Fenton reaction:
Foustoukos D.
Grozeva N.
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