Abstract

The habitability of Mars is determined by the physical and chemical environment. The effect of low water availability, temperature, low atmospheric pressure and strong UV radiation has been extensively studied in relation to the survival of microorganisms. In addition to these stress factors, it was recently found that silicates exposed to simulated saltation in a Mars-like atmosphere can lead to a production of reactive oxygen species. Here, we have investigated the stress effect induced by quartz and basalt abraded in Mars-like atmospheres by examining the survivability of the three microbial model organisms Pseudomonas putida, Bacillus subtilis, and Deinococcus radiodurans upon exposure to the abraded silicates. We found that abraded basalt that had not been in contact with oxygen after abrasion killed more than 99% of the vegetative cells while endospores were largely unaffected. Exposure of the basalt samples to oxygen after abrasion led to a significant reduction in the stress effect. Abraded quartz was generally less toxic than abraded basalt. We suggest that the stress effect of abraded silicates may be caused by a production of reactive oxygen species and enhanced by transition metal ions in the basalt leading to hydroxyl radicals through Fenton-like reactions. The low survivability of the usually highly resistant D. radiodurans indicates that the effect of abraded silicates, as is ubiquitous on the Martian surface, would limit the habitability of Mars as well as the risk of forward contamination. Furthermore, the reactivity of abraded silicates could have implications for future manned missions, although the lower effect of abraded silicates exposed to oxygen suggests that the effects would be reduced in human habitats.

Highlights

  • An in-depth understanding of the interaction between the Martian surface environment and living cells is essential for assessment of the habitability of Mars, the risk of forward contamination and the hazards associated with manned missions

  • Ionizing radiation from the sun only poses a minor challenge for B. subtilis and D. radiodurans, and a cover that would protect against UV radiation would shield from the charged particles in the solar wind (Tuleta et al, 2005; PaulinoLima et al, 2011)

  • The number of colony forming units (CFU) of P. putida harvested during exponential growth increased in the phosphate buffered saline (PBS) controls as well as in the controls with inactivated silicates (Figure 2A)

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Summary

Introduction

An in-depth understanding of the interaction between the Martian surface environment and living cells is essential for assessment of the habitability of Mars, the risk of forward contamination and the hazards associated with manned missions. Martian surface is extremely arid and even if liquid water is present, the water activity is likely too low to support life (Martin-Torres et al, 2015; Ojha et al, 2015). While such an arid, cold, low-pressure environment often is not detrimental for desiccation tolerant, dormant cells and spores, the radiation on the Martian surface can be highly damaging (Hansen et al, 2009; Johnson et al, 2011). The Martian surface does not generally allow life to proliferate, but may not pose an immediate threat to dormant cells

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