Physics
Scientific paper
Dec 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988plr.....8f..13k&link_type=abstract
Planetary Report (ISSN 0736-3680), vol. 8, Nov.-Dec. 1988, p. 13-16.
Physics
Planetary Composition, Planetary Evolution, Planetary Meteorology, Venus Atmosphere, Water Vapor, Asteroids, Astronomical Models, Cloud Physics, Comets, Meteoritic Composition
Scientific paper
The possibility that Venus once had abundant water is discussed. The equilibrium condensation model for planetary formation is reviewed. It is suggested that this model is flawed because it presumes that planets formed with little or no mixing of planetesimals outside the planet's immediate vicinity and because the model ignores the role of comets. The question of how much water Venus lost is examined and a model for the history of water on Venus is outlined.
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