Structuring processes in preplanetary disks

Details Structuring processes in preplanetary disks Structuring processes in preplanetary disks

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.315...59m&link_type=abstract

In ESA, Formation of Stars and Planets, and the Evolution of the Solar System p 59-65 (SEE N91-18922 10-90)

Physics

Accretion Disks, Planetary Evolution, Planetary Orbits, Protoplanets, Mathematical Models, Orbital Mechanics, Planetary Composition, Planetary Magnetospheres, Solar System, Solar Terrestrial Interactions, Stellar Evolution

Scientific paper

Comparable structures in the orbital distribution of planets around the Sun and satellites in the systems of Jupiter, Saturn and Uranus are indications for possible early structuring processes in disks around growing central bodies. Physical mechanisms which are potentially able to generate structures in disks around central bodies are discussed. Physical parameters and conditions which describe effectivity and relevance of these mechanisms of planetogonic processes are derived. Different physical processes investigated as possible candidates for structuring effects, such as resonance interaction of planets or satellites, radial band structures caused by plasma physical processes, regular rings left behind from the shrinking Sun, convection driven radial structures and structuring due to collective gravitational effects in the disk, are reviewed.

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