6–8 Sept 2023 In-Person Event
DLR
Europe/Berlin timezone

The Role of Perchlorate on the Habitability of Mars

6 Sept 2023, 13:30
20m
Rotunde (DLR)

Rotunde

DLR

DLR, Institut für Planetenforschung Rutherfordstr. 2 12489 Berlin
Oral presentation MARS

Speaker

Jacob Heinz (Astrobiology Research Group, Center for Astronomy and Astrophysics (ZAA), Technische Universität Berlin, Hardenbergstr. 36, 10623 Berlin, Germany)

Description

Putative microbial life on Mars would encounter a severe scarcity of liquid water due to the prevailing freezing and hyperarid climate conditions. Interestingly, hygroscopic salts were discovered on Mars that enable water absorption from the atmosphere and lower the freezing point, potentially allowing the temporary occurrence of liquid briny water [1]. However, these brines contain high concentrations of salts, posing significant challenges for life, including high salinity, ionic strengths, and low water activity. Of particular interest are perchlorate (ClO4-) salts, which are widespread on Mars [2] but rare in natural environments on Earth. Therefore, investigating the habitability of perchlorate brines and the effects of perchlorate ions on microbial cells through lab experiments is crucial. In this study, we summarize the results of our investigations into the perchlorate-specific stress responses of various organisms from all three domains of life (archaea, bacteria, and eukaryotes) and discuss their implications for the habitability of Mars.

As model organisms, we used Planococcus halocryophilus and Escherichia coli for bacteria, Haloferax volcanii for archaea, and Debaryomyces hansenii for eukaryotes. We employed various analytical tools, including growth experiments, fluorescence and scanning electron microscopy, and proteomics, to analyze the microbial stress responses. Microscopic analysis revealed that cells exposed to perchlorate stress often exhibited morphological changes, such as the formation of cell clusters in P. halocryophilus and D. hansenii, as well as cell filaments in E. coli. Growth experiments demonstrated that all tested organisms could adapt to higher perchlorate concentrations when repeatedly incubated with increasing amounts of perchlorate. Notably, the halotolerant yeast D. hansenii displayed the highest perchlorate tolerance at 2.5 mol/kg NaClO4 (water activity aw = 0.926), although its tolerance to NaCl was even higher at 4.0 mol/kg (aw = 0.854) [3]. Proteomic investigations indicated that the chaotropicity of perchlorate (i.e., destabilization of biomacromolecules) likely contributed to D. hansenii's decreased tolerance towards NaClO4 compared to NaCl [4]. In response to the chaotropic stress, D. hansenii stabilized proteins through increased glycosylation and upregulated the biosynthesis and remodulation of the cell wall. Analyses of perchlorate-induced changes in the proteome of other investigated organisms are ongoing, with preliminary results showing only a limited overlap with the perchlorate-specific stress responses observed in D. hansenii. However, for both prokaryotes investigated thus far (E. coli and H. volcanii), the de novo inosine monophosphate (IMP) biosynthesis and purine metabolism appeared to play a crucial role in the metabolic perchlorate defense machinery, suggesting an increased requirement for nucleotide repair and stabilization. This might be due to chaotropic and oxidative stress resulting from perchlorate exposure.

The surprisingly high perchlorate tolerances of organisms like D. hansenii and the ability of various organisms to adapt to elevated perchlorate concentrations demonstrate that perchlorate in liquid solutions under ambient temperature is not as detrimental to life as often assumed.

References: [1] Martínez G.M. and Renno N.O. (2013) Space Science Reviews 175:29–51. [2] Clark B. C. and Kounaves S. P. (2016) International Journal of Astrobiology 15:311–318. [3] Heinz J. et al. (2021) Life 11:1194. [4] Heinz J. et al. (2022). Environ. Microbiol. 24:5051–5065.

Primary author

Jacob Heinz (Astrobiology Research Group, Center for Astronomy and Astrophysics (ZAA), Technische Universität Berlin, Hardenbergstr. 36, 10623 Berlin, Germany)

Co-authors

Anne Gries (Astrobiology Research Group, Center for Astronomy and Astrophysics (ZAA), Technische Universität Berlin, Hardenbergstr. 36, 10623 Berlin, Germany) Lea Doris Friedel Kloss (Astrobiology Research Group, Center for Astronomy and Astrophysics (ZAA), Technische Universität Berlin, Hardenbergstr. 36, 10623 Berlin, Germany) Dirk Schulze-Makuch (Astrobiology Research Group, Center for Astronomy and Astrophysics (ZAA), Technische Universität Berlin, Hardenbergstr. 36, 10623 Berlin, Germany)

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