Inhabited subsurface wet smectites in the hyperarid core of the Atacama Desert as an analog for the search for life on Mars.
Ontology highlight
ABSTRACT: The modern Martian surface is unlikely to be habitable due to its extreme aridity among other environmental factors. This is the reason why the hyperarid core of the Atacama Desert has been studied as an analog for the habitability of Mars for more than 50 years. Here we report a layer enriched in smectites located just 30 cm below the surface of the hyperarid core of the Atacama. We discovered the clay-rich layer to be wet (a phenomenon never observed before in this region), keeping a high and constant relative humidity of 78% (aw 0.780), and completely isolated from the changing and extremely dry subaerial conditions characteristic of the Atacama. The smectite-rich layer is inhabited by at least 30 halophilic species of metabolically active bacteria and archaea, unveiling a pr
SUBMITTER: Azua-Bustos A
PROVIDER: S-EPMC7645800 | biostudies-literature | 2020 Nov
REPOSITORIES: biostudies-literature
ACCESS DATA