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Stable carbon isotope fractionation during bacterial acetylene fermentation: Potential for life detection in hydrocarbon-rich volatiles of icy planet(oid)s

Laurence Miller·Shaun Baesman·Ron Oremland
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Abstract

We report the first study of stable carbon isotope fractionation during microbial fermentation of acetylene (C 2 H 2 ) in sediments, sediment enrichments, and bacterial cultures. Kinetic isotope effects (KIEs) averaged 3.7 ± 0.5‰ for slurries prepared with sediment collected at an intertidal mudflat in San Francisco Bay and 2.7 ± 0.2‰ for a pure culture of Pelobacter sp. isolated from these sediments. A similar KIE of 1.8 ± 0.7‰ was obtained for methanogenic enrichments derived from sediment collected at freshwater Searsville Lake, California. However, C 2 H 2 uptake by a highly enriched mixed culture (strain SV7) obtained from Searsville Lake sediments resulted in a larger KIE of 9.0 ± 0.7‰. These are modest KIEs when compared with fractionation observed during oxidation of C 1 compounds such as methane and methyl halides but are comparable to results obtained with other C 2 compounds. These observations may be useful in distinguishing biologically active processes operating at distant locales in the Solar System where C 2 H 2 is present. These locales include the surface of Saturn's largest moon Titan and the vaporous water- and hydrocarbon-rich jets emanating from Enceladus.

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Laurence Miller, Shaun Baesman, Ron Oremland. 2015. Stable carbon isotope fractionation during bacterial acetylene fermentation: Potential for life detection in hydrocarbon-rich volatiles of icy planet(oid)s. https://doi.org/10.1089/ast.2015.1355

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