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Manganese oxides as high-pε redox buffers on Mars
Authors:Thomas R Blackburn
Institution:Program in Chemistry and Physics, St. Andrews Presbyterian College, Laurinburg, North Carolina 28352, USA
Abstract:The x-ray photoelectron spectrum of Mn(VI) is closely similar to that of uv-irradiated MnO2, previously reported to simulate the Viking gas exchange reaction. β-MnO2 is the thermodynamically stable form of manganese on the surface of Mars, and MnO2 abundances estimated from shergottite, nakhlite, and chassignite iron/manganese ratios are sufficient to account for the oxidant buffer capacity observed by Viking.
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