Cultivation of halophilic archaea in shallow subsurface martian conditions has implications for extant life on Mars

The present-day martian surface is generally considered inhospitable to life because of low atmospheric pressure, intense surface radiation, global desiccation, and oxidizing chemistry which has been increasing since the late Noachian. However, shallow martian subsurface regions where mineralogy has shown groundwater movement may include localized hypersaline environments capable of retaining liquid water and supporting microbial metabolism. Haloferax volcanii, a model halophilic archaeon, has previously been shown to survive under low-pressure martian conditions (24 mbar) and to grow anaerobically supported by the Mars-relevant oxyanions nitrate and perchlorate under high-salinity conditions. Here, we investigated whether H. volcanii could actively grow under a combination of environmental and chemical conditions relevant to potentially habitable shallow subsurface martian lacustrine settings. Cultures were incubated for 160 days under anoxic, CO2-enriched, low-pressure conditions (24 mbar) in hypersaline liquid media supplemented with nitrate or perchlorate. Growth was observed in all low-pressure treatments and was confirmed by increases in optical density and biological reduction of nitrate and perchlorate. Scanning electron microscopy revealed extensive biofilm formation in low-pressure cultures, and Raman spectroscopy demonstrated the persistence of carotenoid biosignatures after prolonged incubation under martian conditions. Water loss remained below 4% across all treatments, indicating long-term stability of hypersaline brines throughout the experiment. These results demonstrate for the first time that a halophilic archaeon is capable of active growth and metabolism under a Mars-relevant combination of low pressure, high salinity, anoxia, and oxidizing chemistry, providing experimental support for the potential habitability of localized shallow subsurface martian environments. ImportanceThe search for cellular life is a major objective of future Mars exploration. While many studies have examined whether microorganisms can survive under martian conditions, far fewer have demonstrated active growth and metabolism. Here, we document Haloferax volcanii as the first halophilic archaeon capable of active growth under a defined combination of Mars-relevant low atmospheric pressure, high salinity, anoxia, and oxidizing chemical conditions. These findings expand the current understanding of the environmental limits of microbial growth and provide experimental evidence that localized brine environments in the shallow martian subsurface could support active microbial metabolism, if suitable organics and liquid water are present. In addition, this study establishes a practical framework for cultivating halophilic microorganisms under low-pressure martian conditions and may help guide future efforts to detect, cultivate, and characterize potential extant life on Mars.