Computer Science
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989icar...81....1l&link_type=abstract
Icarus (ISSN 0019-1035), vol. 81, Sept. 1989, p. 1-13.
Computer Science
10
Gas Giant Planets, Satellite Atmospheres, Satellite Surfaces, Solar System, Volatility, Atmospheric Composition, Charon, Hydrocarbons, Liquid Nitrogen, Solar Corona, Triton, Planets, Solar System, Volatiles, Satellites, Titan, Saturn, Triton, Neptune, Pluto, Charon, Atmosphere, Composition, Density, Chemistry, Diagrams, Models, Origin, Formation, Surface, Uranus, Evolution, Cosmochemistry, Icy Bodies, Abundance
Scientific paper
The chemical aspects of the formation of the solid bodies of the outer solar system are reviewed, excluding the giant planets. The features of volatile-rich solid bodies, which are applicable to the study of their formation are outlined. The formation and evolution of Titan are discussed in detail. Data on Triton, Pluto/Charon, and the Uranian satellites are examined in the framework of models of early solar system processes.
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