  We study the existence and stability of circular geodesics in a family of
asymptotically AdS static black holes in New Massive Gravity. We show that the
existence of such geodesics is determined by the sign of the hair parameter.
For a positive hair parameter the stability regions follow the usual pattern,
with an innermost unstable null geodesic separated from the horizon, followed
by a region of unstable timelike geodesics and then stable timelike geodesics
extending in the asymptotic region.
