ESCAPE OF PARTICLES ORBITING ASTEROIDS IN THE PRESENCE OF RADIATION PRESSURE THROUGH SEPARATRIX SPLITTING

We study the motion of grains in orbit around asteroids under the infl uence of radiation pressure originating in the flux of solar photons. Of interest is the possibility of initially bound grains becoming unbo und and leaving the vicinity of the asteroid. The analysis extends the two-degree-of-freedom results of (Dankowicz, 1995) to three-degree-of -freedom motions. In particular, we use a Melnikov-type approach for f inding transversal points of intersection between high-dimensional per turbed stable and unstable manifolds. As a consequence, the system is shown to be nonintegrable and the resulting homoclinic tangles are sug gested as a means for phase space transport along resonance layers, so -called Arnol'd diffusion. We discuss the implications of the diffusio n on the depletion of asteroid-bound particles and attempt to estimate the diffusion rate for physical comparison. For particular values of physical parameters the time scale is shown to be on the order of hund reds of orbital revolutions of the asteroid around the sun.