“…Microorganisms isolated from these extreme habitats considered analogous to extraterrestrial environments are highly adapted and are good candidates for astrobiological studies [e.g., astrobiological models, adaptation mechanisms, strategies underlying survival in extreme conditions, and potential (novel) biosignatures that can be used in habitable zones beyond Earth; Lopez et al, 2019;Jebbar et al, 2020], yielding potential clues as to whether (and how) life may exist and persist on other planetary bodies (Lopez et al, 2019;Coleine and Delgado-Baquerizo, 2022), and even provide tools to guide future colonization, if this is desired (Lopez et al, 2019). So far, prokaryotes are the most-studied models for astrobiology (Seyler et al, 2020;Abbott and Pearce, 2021), including members of the (i) halophilic archaea (class Haloarchaea), which are typically used for Mars studies, due to their ability to withstand salinity and perchlorates, anaerobic conditions, high levels of UV and ionizing radiation, subzero temperatures, desiccation, and toxic ions (Stan-Lotter and Fendrihan, 2015;DasSarma and DasSarma, 2017); (ii) Deinococcus radiodurans, a bacterium that is widely known for its high resistance to radiation (up to 10,000 Gy; Daly, 2011) and its importance in the context of planetary protection and panspermia (Kawaguchi et al, 2013); and (iii) representatives of the genus Bacillus, which have repeatedly demonstrated their ability to survive in many extreme conditions encountered in outer space. These members include (i) Bacillus subtilis, which is known to survive in conditions similar to those on Mars (extreme dryness, high radiation levels, and high concentrations of perchlorate salts) (Nicholson et al, 2000), and (ii) Bacillus pumilus, a model organism that is currently used to assess the habitability of Europa (icy moon of Jupiter) based on its capability to survive in extreme temperatures, low nutrient availability, dryness, and UV-C radiation (Stepanov et al, 2016).…”