Planetary Camera Observations of the Double Nucleus of M31

V- and I-band HST Planetary Camera images of the great spiral galaxy in Andromeda, M31, show that its inner nucleus consists of two components separated by 0.49". The outer isophotes of the nucleus at 1.4" < r < 3.0" are elongated, but are concentric with the M31 bulge. The nuclear component with the lower surface brightness, P2, is also coincident with the bulge photocenter to ~0,05"; we argue that it is at the kinematic center of the galaxy. The brighter nuclear component, P1, is well resolved and corresponds to the nuclear core imaged by Stratoscope II. The central V-band luminosity density for P1 is 5 x 10^4^L_sun_ pc^-3^. P2 is highly elongated and has a shallow cusp. ItS central V-band luminosity density is > 2 x 10^4^L-sun_ pc^-3^. The total nucleus cannot be modeled as the superposition of two systems each with elliptical and concentric isophotes. The dark zone between the two peaks is deep and is either evidence for strong dust absorption or that the nuclear components are steeply truncated in this region. No strong changes in the V - I color are observed over the nucleus, however. Thus if dust absorption generates the asymmetric nuclear morphology, the dust grain size must be unusually large or the dust optical depth must be extremely high. Alternatively the higher surface brightness, off-center nuclear component P1 may be a separate stellar system. The nuclear velocity dispersion profiles of Dressler & Richstone [ApJ, 324,701(1988)] and Kormendy [ApJ, 325, 128 (1988)] already show that P1 cannot be a dynamically cold system such as a globular cluster. Requiring P1 to survive destruction by a central black hole in M31 may also lead to lower limits on its mass-to- light ratio. This hypothesis requires us to be looking at M31 at a special time; however, the lifetime of P1 against orbital decay may be substantially longer than naive dynamical friction arguments would indicate. Under this picture, we argue that P1 is more likely to be a cannibalized galactic nucleus, possibly having its own central black hole.