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dc.contributor.authorTosca, Nicholas J.
dc.contributor.authorKnoll, Andrew
dc.contributor.authorMcLennan, Scott M.
dc.date.accessioned2009-05-28T15:54:18Z
dc.date.issued2008
dc.identifier.citationTosca, Nicholas J., Andrew. H. Knoll, and Scott M. McLennan. 2008. Water activity and the challenge for life on early Mars. Science 320, no. 5880: 1204-1207.en
dc.identifier.issn0036-8075en
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:3007646
dc.description.abstractIn situ and orbital exploration of the martian surface has shown that acidic, saline liquid water was intermittently available on ancient Mars. The habitability of these waters depends critically on water activity (<sup>a</sup>H<sub>2</sub>O), a thermodynamic measure of salinity, which, for terrestrial organisms, has sharply defined limits. Using constraints on fluid chemistry and saline mineralogy based on martian data, we calculated the maximum <sup>a</sup>H<sub>2</sub>O for Meridiani Planum and other environments where salts precipitated from martian brines. Our calculations indicate that the salinity of well-documented surface waters often exceeded levels tolerated by known terrestrial organisms.en
dc.description.sponsorshipOrganismic and Evolutionary Biologyen
dc.language.isoen_USen
dc.publisherAmerican Association for the Advancement of Scienceen
dc.relation.isversionofhttp://dx.doi.org/10.1126/science.1155432en
dash.licenseMETA_ONLY
dc.titleWater Activity and the Challenge for Life on Early Marsen
dc.relation.journalScienceen
dash.depositing.authorKnoll, Andrew
dash.embargo.until10000-01-01
dc.identifier.doi10.1126/science.1155432*
dash.contributor.affiliatedKnoll, Andrew


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