Physics
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.315..127e&link_type=abstract
In ESA, Formation of Stars and Planets, and the Evolution of the Solar System p 127-137 (SEE N91-18922 10-90)
Physics
1
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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