Paper
7 September 2010 Astrobiological characteristics and possibility of life in the polar dark dune spots of Mars
A. Kereszturi, Sz. Bérczi, A. Horváth, T. Pócs, A. Sik, E. Szathmáry
Author Affiliations +
Abstract
The circumpolar region of Mars was surveyed for possible habitats in the area of seasonal ice cap. Dark Dune Spots were found to be good candidates as they are covered by water ice there without carbon-dioxide ice, and show flow-like features in springtime. Based on theoretical calculations interfacial water or bulk brine may be present there that decomposes the aggressive oxidants. Temperature values in springtime around noon could be favorable for metabolism of known extremophyles on Earth, and water uptake may be possible at nighttime. During the warm daytime period the water loss could be lowered by densely packed grain structure of the soil, hygroscopic salts, and polysaccharide-like materials, as it was observed in the samples of cryptobiotic crust from hot and cold deserts on Earth. This work outlines the basic elements of these possible circumpolar microhabitats.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. Kereszturi, Sz. Bérczi, A. Horváth, T. Pócs, A. Sik, and E. Szathmáry "Astrobiological characteristics and possibility of life in the polar dark dune spots of Mars", Proc. SPIE 7819, Instruments, Methods, and Missions for Astrobiology XIII, 78190K (7 September 2010); https://doi.org/10.1117/12.862839
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KEYWORDS
Organisms

Mars

Molecules

Ultraviolet radiation

Analog electronics

Data modeling

Natural surfaces

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