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Growth, viability, and death of planktonic and biofilm Sphingomonas desiccabilis in simulated martian brines
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dc.contributor.author | Stevens, Adam H. | |
dc.contributor.author | Childers, Delma | |
dc.contributor.author | Fox-Powell, Mark | |
dc.contributor.author | Nicholson, Natasha | |
dc.contributor.author | Jhoti, Elisha | |
dc.contributor.author | Cockell, Charles S. | |
dc.date.accessioned | 2019-03-01T16:30:10Z | |
dc.date.available | 2019-03-01T16:30:10Z | |
dc.date.issued | 2019-01-02 | |
dc.identifier.citation | Stevens , A H , Childers , D , Fox-Powell , M , Nicholson , N , Jhoti , E & Cockell , C S 2019 , ' Growth, viability, and death of planktonic and biofilm Sphingomonas desiccabilis in simulated martian brines ' , Astrobiology , vol. 19 , no. 1 , pp. 87-98 . https://doi.org/10.1089/ast.2018.1840 | en |
dc.identifier.issn | 1531-1074 | |
dc.identifier.other | PURE: 257990254 | |
dc.identifier.other | PURE UUID: 734b52ff-42b2-492c-b5e7-8def7bdf1815 | |
dc.identifier.other | Scopus: 85059394268 | |
dc.identifier.other | PubMed: 30048150 | |
dc.identifier.other | WOS: 000440140700001 | |
dc.identifier.uri | http://hdl.handle.net/10023/17197 | |
dc.description | This research was supported by the UK Science Technology and Facilities Council under Grant ST/M001261/1. | en |
dc.description.abstract | Aqueous solutions on Mars are theorized to contain very different ion compositions than those on Earth. To determine the effect of such solutions on typical environmental micro-organisms, which could be released from robotic spacecraft or human exploration activity, we investigated the resistance of Sphingomonas desiccabilis to brines that simulate the composition of martian aqueous environments. S. desiccabilis is a desiccation-resistant, biofilm-forming microbe found in desert crusts. The viability of cells in both planktonic and biofilm forms was measured after exposure to simulated martian brines. Planktonic cells showed a loss of viability over the course of several hours in almost all of the seven brines tested. Biofilms conferred greater resistance to all the brines, including those with low water activity and pH, but even cells in biofilms showed a complete loss of viability in <6 h in the harsher brines and in <2 days in the less harsh brines. One brine, however, allowed the microbes to maintain viability over several days, despite having a water activity and pH lower and ionic strength higher than brines that reduced viability over the same timescales, suggesting important ion-specific effects. These data show that biofilm-forming cells have a greater capacity to resist martian aqueous extremes, but that evaporative or deliquescent brines are likely to be destructive to many organisms over relatively short timescales, with implications for the habitability of Mars and for micro-organisms dispersed by robotic or human explorers. | |
dc.format.extent | 12 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrobiology | en |
dc.rights | Copyright © Adam H. Stevens et al., 2018; Published by Mary Ann Liebert, Inc. This Open Access article is distributed under the terms of the Creative Commons License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited. | en |
dc.subject | Brines | en |
dc.subject | Desiccation | en |
dc.subject | Extremophile | en |
dc.subject | Halotolerance | en |
dc.subject | Mars | en |
dc.subject | GE Environmental Sciences | en |
dc.subject | QH301 Biology | en |
dc.subject | Agricultural and Biological Sciences (miscellaneous) | en |
dc.subject | Space and Planetary Science | en |
dc.subject | NDAS | en |
dc.subject.lcc | GE | en |
dc.subject.lcc | QH301 | en |
dc.title | Growth, viability, and death of planktonic and biofilm Sphingomonas desiccabilis in simulated martian brines | en |
dc.type | Journal article | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Earth & Environmental Sciences | en |
dc.contributor.institution | University of St Andrews. St Andrews Centre for Exoplanet Science | en |
dc.identifier.doi | https://doi.org/10.1089/ast.2018.1840 | |
dc.description.status | Peer reviewed | en |
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