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- W140995315 abstract "The search for extraterrestrial life has been declared as a goal for the twenty-first century by several space agencies (Foing, 2002). Potential candidates are microorganisms on or in the surfaces of moons and planets. Extremely halophilic archaea (haloarchaea) are of astrobiological interest since viable strains have been isolated from million-year-old deposits of halite (McGenity et al., 2000; Stan-Lotter et al., 1999, 2002; Fendrihan et al., 2006), suggesting the possibility of long-term survival under desiccation. Extraterrestrial halite has been identified, for example, in Martian meteorites (Treiman et al., 2000), in chloride-containing surface pools on Mars (Osterloo et al., 2008), and in the presumed salty ocean beneath the ice cover of Jupiter’s moon Europa (McCord et al., 1998). These discoveries make a consideration of the potential habitats for halophilic life in space intriguing. Recent data on the physical occurrence of liquid saline water on Mars (Smith et al., 2009; Renno et al., 2009) have added another novel aspect to this notion, since such “cryobrines” would provide liquid phases on the Martian surface, allowing perhaps metabolic activity of halophilic microorganisms." @default.
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- W140995315 date "2012-01-01" @default.
- W140995315 modified "2023-09-24" @default.
- W140995315 title "The Likelihood of Halophilic Life in the Universe" @default.
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