Physics
Scientific paper
Apr 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975p%26ss...23..661s&link_type=abstract
Planetary and Space Science, vol. 23, Apr. 1975, p. 661-669. Research supported by the Alfred P. Sloan Foundation
Physics
1
Carbon Dioxide, Mars Atmosphere, Oxygen Atoms, Reaction Kinetics, Recombination Coefficient, Solidified Gases, Carbon Monoxide, Carbon 14, Low Temperature Environments, Mars Surface, Polar Caps, Surface Reactions
Scientific paper
n atomic oxygen flow system and a C14 radiochemical technique have been used to show that the reactions O + CO --> CO2 and O + O --> O2, are heterogeneously catalysed by solid CO2 at 77 K. The O-CO recombination is first order in CO and inhibited by O, whereas the O-O recombination is first order in O and weakly inhibited by CO. Assuming simple first order kinetics, recombination coefficients γco = 1.3(+/-0.9) × 10-5 and γO = 0.05+/- 0.02 are determined. A recombination mechanism involving an intermediate adsorbed CO3 is proposed. If the kinetic results are assumed to apply under Martian surface conditions, then conversion of CO to CO2 by reaction on the solid CO2 at the polar caps occurs at ~10 times the total column recombination rates for homogeneous reactions previously proposed; night-side CO2 ice clouds would also constitute an important recombination surface. Alfred P. Sloan Foundation Fellow.
Sethi D. S.
Smith Leonard A.
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