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Habitability of Planets Around Red Dwarf Stars
Authors:Heath  Martin J  Doyle  Laurance R  Joshi  Manoj M  Haberle  Robert M
Institution:(1) Biospheres Project, 47 Tulsemere Road, West Norwood, London, SE27 9EH, U.K.;(2) SETI Institute, 2035 Landings Drive, Mountain View, CA, 94043, U.S.A.;(3) Space Science Division Mail Stop 245-3, N.A.S.A. Ames Research Center, Moffet Field, CA, 94035, U.S.A.
Abstract:Recent models indicate that relatively moderate climates could exist on Earth-sized planets in synchronous rotation around red dwarf stars. Investigation of the global water cycle, availability of photosynthetically active radiation in red dwarf sunlight, and the biological implications of stellar flares, which can be frequent for red dwarfs, suggests that higher plant habitability of red dwarf planets may be possible.
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