Paper
7 September 2010 Likelihood of methane-producing microbes on Mars
Joseph D. Miller, Marianne J. Case, Patricia Ann Straat, Gilbert V. Levin
Author Affiliations +
Abstract
We present a likelihood estimate that methane was a significant component of the gas detected by the Labeled Release (LR) experiment in the Viking Mission to Mars of 1976. In comparison with terrestrial methanogen production of methane we estimate the size of the putative microbe population necessary to produce the LR gas, had it been primarily methane. We extrapolate that figure to estimate the number of methanogens necessary to produce the methane content of the Martian atmosphere. Next, we estimate the amount of Martian soil and the amount of water needed for that global population of microbes. Finally, assuming a globally distributed population of such microbes, we estimate the likely sub-surface depth at which such methanogens could be detected.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Joseph D. Miller, Marianne J. Case, Patricia Ann Straat, and Gilbert V. Levin "Likelihood of methane-producing microbes on Mars", Proc. SPIE 7819, Instruments, Methods, and Missions for Astrobiology XIII, 78190I (7 September 2010); https://doi.org/10.1117/12.862230
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Cited by 3 scholarly publications.
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KEYWORDS
Methane

Lawrencium

Mars

Microorganisms

Carbon dioxide

Liquids

Carbon monoxide

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