  We investigate the possibility of accounting for the observed anomalous
velocities of stars in galaxies to be a result of a dynamic prescription for
having a galaxy generate and prescribe its own inertial frame. It is
demonstrated that within observational uncertainties, an overall rotation of an
inertial frame dragged by a galaxy is a comfortable fit to the observed
anomalous velocity curves. A case for looking for a natural law for prescribing
an inertial frame by a mass distribution over a finite (galaxy size) range is
made out.
