Mumma et al. 1 have confirmed earlier detections of methane in the Martian atmosphere,
finding it localized and correlated with atmospheric water vapor. They determined that,
because of the short half-life of methane, a continual replenishment is required to account
for its presence. They also conclude that the dynamics of methane on Mars require a
methane sink in the soil. It is suggested here that both phenomenon could be accounted
for by an ecology of methane-producing and methane-consuming microorganisms. Such
ecologies exist on Earth, where, generally, anaerobic methanogens live at depth and
aerobic methanotrophs live at or near the surface. On Mars, with its essentially anaerobic
atmosphere, both types of microorganisms could co-exist at or near the surface. It is
possible that the Viking Labeled Release (LR) experiment detected methanogens in
addition to other microorganisms evolving carbon dioxide since the LR instrumentation
would detect methane, carbon dioxide, or any other carbon gas derived from one of the
LR substrates. A simple modification of the LR experiment that could resolve the life on
Mars issue is discussed.
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