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UV habitability and dM stars: an approach for evaluation of biological survival

Published online by Cambridge University Press:  26 February 2010

Ximena C. Abrevaya ,
Eduardo Cortón  and
Pablo J. D. Mauas
Ximena C. Abrevaya
Affiliation:
Institute for Astronomy and Space Physics UBA-CONICET. Buenos Aires, Argentina. email: [email protected] Biochemistry Department, Faculty of Exact Sciences, UBA. Buenos Aires, Argentina.
Eduardo Cortón
Affiliation:
Biochemistry Department, Faculty of Exact Sciences, UBA. Buenos Aires, Argentina.
Pablo J. D. Mauas
Affiliation:
Institute for Astronomy and Space Physics UBA-CONICET. Buenos Aires, Argentina. email: [email protected]
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Abstract

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Dwarf M stars comprise about 75 percent of all stars in the galaxy. For several years planets orbiting M stars have been discarded as suitable places for development of life. This paradigm now has changed and terrestrial-type planets within liquid-water habitable zones (LW-HZ) around M stars are reconsidered as possible hosts for life as we know it. Nevertheless, large amount of UV radiation is emitted during flares by this stars, and it is uncertain how these events could affect biological systems. In particular UV-C λ < 290nm) exhibits the most damaging effects for living organisms. To analyze the hypothesis that UV could set a limit for the development of extraterrestrial life, we studied the effect of UV-C treatment on halophile archaea cultures. Halophile archaea are extremophile organisms, they are exposed to intense solar UV radiation in their natural environment so they are generally regarded as relatively UV tolerant. Halophiles inhabits in hipersaline environments as salt lakes but also have been found in ancient salt deposits as halites and evaporites on Earth. Since evaporites have been detected in Martian meteorites, these organisms are proposed as plausible inhabitants of Mars-like planets. Our preliminary results show that even after UV damage, the surviving cells were able to resume growth with nearly normal kinetics.

Keywords

astrobiologystars: flareultraviolet: starsmethods: laboratory
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S264: Solar and Stellar Variability: Impact on Earth and Planets , August 2009 , pp. 443 - 445
Copyright
Copyright © International Astronomical Union 2010

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