Biology
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979amsci..67..653p&link_type=abstract
American Scientist, vol. 67, Nov.-Dec. 1979, p. 653-659.
Biology
3
Planets, Exobiology, Meteorites, Composition, Chemistry, Water, Amino Acids, Hydrospheres, Chronology, Stars, Temperatures, Luminescence, Radiation, Evolution, Abundances, Orbits, Gravity, Mass, Extrasolar Planets
Scientific paper
The number of stars in the universe which might have a planet capable of a prolonged evolutionary history of living organisms is estimated to be between one out of 100,000 to 10,000,000. The planet itself needs large masses of land and of water, which must contain an adequate supply of phosphoric acid, purines, pyrimidines, amino acids, and simple sugars and at least 3 to 4 billion years to evolve biologically. Other considerations include its mean orbital radius, rotational velocity, and tidal effects. The necessary conditions for the host star include its lifetime on the main sequence, luminosity and spectral characteristics, mass and chemical composition, and the fact that it must be a single star (not part of a binary system). A priori calculation of the development of hominids on such a planet, however, is not considered possible.
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