Early conditions and processes in the outer solar system

Physics

Scientific paper

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Abundance, Chemical Composition, Cometary Atmospheres, Cosmochemistry, Solar Corona, Stellar Evolution, Chemical Analysis, Comet Nuclei, Interstellar Chemistry, Molecular Interactions, Space Exploration, Star Formation, Titan

Scientific paper

Study of the chemical composition of comets, giant planets and Titan is discussed. The composition of the primordial solar nebula at large heliocentric distances and the physicochemical processes involved in their formation and evolution are studied. Elemental and isotopic abundance ratios are used as tools in studying these formation and evolution processes. The importance of data gained on ISO (Infrared Space Observatory), Galileo, Cassini, CRAF (Comet Rendezvous Asteroid Flyby) and Rosetta missions in furthering better understanding of these processes is stressed.

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