Problem of habitation on planetary systems of red dwarf stars

Details Problem of habitation on planetary systems of red dwarf stars Problem of habitation on planetary systems of red dwarf stars

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985stoc.iafcs....k&link_type=abstract

IAF, International Astronautical Congress, 36th, Stockholm, Sweden, Oct. 7-12, 1985. 4 p.

Astronomy and Astrophysics

Astronomy

Extrasolar Planets, Extraterrestrial Life, Planetary Systems, Planetology, Red Dwarf Stars, M Stars, Project Seti, Solar System, Stellar Luminosity

Scientific paper

It has been suggested by various authors that planetary systems of dwarf stars of late spectral classes could be of interest for the SETI problem despite a low flux of radiation emitted by a star. By considering the distance between a star and its planets and the equilibrium temperature of the planets, it is shown that for all stars from KV5 to the latest of the M class, the existence of habitable planets is doubtful. Stars of low mass and low luminosity can be excluded from the SETI list.

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