Atmospheric chemistry in a habitable planet with a rich CO_2 atmosphere under the effect of a stellar flare

Details Atmospheric chemistry in a habitable planet with a rich CO_2 atmosphere under the effect of a stellar flare Atmospheric chemistry in a habitable planet with a rich CO_2 atmosphere under the effect of a stellar flare

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..296s&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Biology

Scientific paper

Main sequence M stars are the most abundant stars in our galaxy, they have features that make them an attractive target for Astrobiology, but their strong chromospheric activity produces high energy radiation and charged particles that may be detrimental to life. We study the impact of a strong flare from the M dwarf, AD Leo, on the atmospheric chemistry of a hypothetical Earth-like planet located in the habitable zone. The simulations were performed using a 1-D photochemical model. We simulated

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