Microbial preference for chlorate over perchlorate under simulated shallow subsurface Mars-like conditions.
Autor: | Fischer FC; Center for Astronomy and Astrophysics, RG Astrobiology, Technische Universität Berlin, Berlin, Germany., Schulze-Makuch D; Center for Astronomy and Astrophysics, RG Astrobiology, Technische Universität Berlin, Berlin, Germany.; GFZ German Research Center for Geosciences, Section Geomicrobiology, Potsdam, Germany.; Department of Plankton and Microbial Ecology, Leibniz-Institute of Freshwater Ecology and Inland Fisheries (IGB), Stechlin, Germany., Heinz J; Center for Astronomy and Astrophysics, RG Astrobiology, Technische Universität Berlin, Berlin, Germany. heinz@tu-berlin.de. |
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Jazyk: | angličtina |
Zdroj: | Scientific reports [Sci Rep] 2024 May 21; Vol. 14 (1), pp. 11537. Date of Electronic Publication: 2024 May 21. |
DOI: | 10.1038/s41598-024-62346-y |
Abstrakt: | The Martian surface and shallow subsurface lacks stable liquid water, yet hygroscopic salts in the regolith may enable the transient formation of liquid brines. This study investigated the combined impact of water scarcity, UV exposure, and regolith depth on microbial survival under Mars-like environmental conditions. Both vegetative cells of Debaryomyces hansenii and Planococcus halocryophilus, alongside with spores of Aspergillus niger, were exposed to an experimental chamber simulating Martian environmental conditions (constant temperatures of about - 11 °C, low pressure of approximately 6 mbar, a CO (© 2024. The Author(s).) |
Databáze: | MEDLINE |
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