Radial mixing in the outer Milky Way disk caused by a low mass orbiting satellite

Using test particle simulations we examine the structure of the outer Galactic disk as it is perturbed by a low mass satellite in a tight eccentric orbit about the Galaxy. A low mass satellite of mass a few times 109M⊙ can heat the outer Galactic disk, excite spiral structure and a warp and induce streams in the velocity distribution. We examine particle eccentricity versus the change in mean radius between initial and current orbits. Correlations between these quantities are reduced after a few satellite pericenter passages. Stars born in the outer galaxy can be moved in radius from their birth positions and be placed in low eccentricity orbits inside their birth radii. We propose that mergers and perturbations from satellite galaxies and subhalos can induce radial mixing in the stellar metallicity distribution.