A Dynamical Model for the Radial Structure of Saturn's Rings

摘要: Abstract In this paper we inquire whether the major positional features of Saturn's ring can be explained by perturbations associated with planet's satellites. We assume a simple but observationally consistent model in which is composed single layer particles, and further suppose that system has evoted to state collisions between particles may ignored. Under these conditions, find only gravitational forces resulting two satellites Mimas Titan suffice for rather complete description system.