Simulating putative Enceladus-like conditions: The possibility of biological methane production on Saturn's icy moon

Ruth-Sophie Taubner, Patricia Pappenreiter, Jennifer Zwicker, Daniel Smrzka, Christian Pruckner, Philipp Kolar, Sebastian Bernacchi, Arne H Seifert, Wolfgang Bach, Jörn Peckmann, Christian Paulik, Maria Gertrude Firneis, Christa Schleper, Simon Karl-Maria Rasso Rittmann (Corresponding author)

Publications: Contribution to journalMeeting abstract/Conference paperPeer Reviewed

Abstract

In this study (Taubner et al. 2018), three different methanogenic archaea (Methanothermococcus okinawensis, Methanothermobacter marburgensis, and Methanococcus villosus) were tested for metabolic activities and growth under putative Enceladus-like conditions, including high pressure experiments and tests on the tolerance towards potential gaseous and liquid inhibitors detected in Enceladus' plume. In particular, M. okinawensis, an isolate from a deep marine trench (Takai et al. 2002), showed tolerance towards all of the added inhibitors and maintained methanogenesis even in the range of 10 to 50 bar. Further, we were able to show that H2 production based on serpentinization may be sufficient to fuel such methanogenic life on Enceladus. The experiments revealed that methanogenesis could, in principle, be feasible under Enceladus-like conditions.
Original languageEnglish
Pages (from-to)219-221
Number of pages3
JournalProceedings of the International Astronomical Union
Volume14
Issue numberS345
Early online date13 Jan 2019
DOIs
Publication statusPublished - Jan 2020
EventIAU 2018 General Assembly Symposium: IAUS 345: Origins: From the Protosun to the First Steps of Life - Wien, Austria
Duration: 20 Aug 201823 Aug 2018
Conference number: 345

Austrian Fields of Science 2012

  • 103003 Astronomy
  • 103004 Astrophysics
  • 106022 Microbiology

Keywords

  • astrobiology
  • methods: Laboratory
  • planets and satellites: Enceladus
  • methods: laboratory

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