Abstract

The search for life on Mars is predicated on the idea that Earth and Mars life (if present) should be both carbon- and water-based with similar forms of evolution. However, the astrobiology community can currently only investigate plausible Martian microbial ecosystems by using Terran life-forms as proxies. In order to examine how life might persist on Mars, we used a hypopiezotolerant bacterium (def., able to grow at 7–10 hPa)—Serratia liquefaciens—in growth assays with four Mars analog soils conducted under a subset of simulated Martian conditions including 7 hPa, 0 °C, and a CO2-enriched anoxic atmosphere (called low-PTA conditions). The four Mars analog soils included an Aeolian dust analog, the Mars JSC-1 analog, a Phoenix lander-site simulant, and a high-Salts analog. Serratia liquefaciens cells were able to grow at 30 °C in a liquid minimal basal medium (MBM) supplemented with 10- or 20-mM sucrose, Spizizen salts, and micronutrients. When the four analog soils were doped with both MBM and cells of S. liquefaciens, and subsequently incubated at 30 °C for 72 h, cell densities increased between 2-logs (Phoenix analog) and 4-logs (Aeolian and JSC-1 analogs); the Salts analog led to complete inactivation of S. liquefaciens within 24 h. In contrast, when the experiment was repeated, but incubated under low-PTA conditions, S. liquefaciens cells were either killed immediately by the Salts analog, or decreased by >5 logs over 28 d by the Aeolian, JSC-1, and Phoenix analogs. The failure of S. liquefaciens to grow in the analog soils under low-PTA conditions was attributed to the synergistic interactions among six factors (i.e., low pressure, low temperature, anoxic atmosphere (i.e., the low-PTA conditions), low-pH in the Salts soil, dissolved salts in all analogs, and oligotrophic conditions) that increased the biocidal or inhibitory conditions within the analog soils. Results suggest that even if a hypopiezotolerant Terran microbe is displaced from a spacecraft surface on Mars, and lands in a hydrated and nutrient-rich niche, growth in the Martian regolith is not automatically assured.

Highlights

  • The search for life on Mars is predicated on the assumption that Martian life is likely to follow the model of Terran life that includes carbon-based organics, liquid water as a solvent, and is constrained by similar forms of evolution

  • Others have proposed that microorganisms recovered from Mars spacecraft should be used as model organisms [8,9,10,11] because they might plausibly be dispersed onto the Martian terrain during lander or rover missions, and might act as inoculum for contaminating sites of scientific interest

  • The results presented here have implications for both mitigating the forward contamination of Mars and the search for an extant Martian microbiota

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Summary

Introduction

The search for life on Mars is predicated on the assumption that Martian life is likely to follow the model of Terran life that includes carbon-based organics, liquid water as a solvent, and is constrained by similar forms of evolution. Until the scientific community has a confirmed extant Mars microbe or community to study, we are forced to use Terran microbial life as proxies for how life might persist on Mars. It is assumed that the best proxies for exploring how microbial life might persist and grow on Mars is through the study of microbial communities in extreme environments like the Antarctic dry valleys, the Atacama Desert, alpine sites, oligotrophic niches, and. Of all of the hypopiezotolerant bacteria (def., as those microbes capable of metabolism and growth at low pressures

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