Other
Scientific paper
Jun 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007icar..188..540k&link_type=abstract
Icarus, Volume 188, Issue 2, p. 540-542.
Other
1
Scientific paper
Bar-Nun and Dimitrov [Bar-Nun, A., Dimitrov, V., 2006. Icarus 181, 320 322] suggested a sequence of reactions to form methane on Mars. These reactions are based on the study of products in the N2 CO H2O mixture irradiated at 185 nm. The suggested scheme was not quantitatively justified by chemical kinetics. One of the key reactions is effectively blocked by O2 in the martian atmosphere, and another key reaction does not exist. There are no pathways for effective formation of methane in the martian atmosphere.
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