Proto Satellitary Accretion Disks

Details Proto Satellitary Accretion Disks Proto Satellitary Accretion Disks

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.242....5c&link_type=abstract

The Solid Bodies of the Outer Solar System, Proceedings of a conference held at Vulcano, Italy, 9-13 September, 1985. Compiled

Computer Science

Scientific paper

An analysis of the global characteristics of protosatellitary accretion disks around the giant planets is presented. General conditions of existence of satellite disks are developed, and the result is that stable disks are not possible for the terrestrial planets. Numerical models for Jupiter and Saturn disks are also given. Two kinds of models are developed. A selfconsistent approach to turbulence and turbulent viscosity is also described. A general result is that hot, turbulent low mass disks around Jupiter and Saturn probably were the first step in the evolutive history of their regular satellite systems.

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