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The wake model for azimuthal brightness variations in Saturn's A-ring
Authors:Hannu Karttunen
Institution:1. Observatory and Astrophysics Laboratory, University of Helsinki, Helsinki, Finland
2. Dept. of Physics and Astronomy, University of Massachusetts, Amherst, MA, USA
Abstract:A dynamical model offering a possible explanation for azimuthal brightness variations in Saturn's ring A is considered. The orbits of ring particles encountering a massive moonlet (radius~100m) are integrated numerically. It is seen that a density wake is produced if the random velocities of the ring particles are much smaller than 1 cm s?1.
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