  The supernova impostor SN 2009ip has re-brightened several times since its
initial discovery in August 2009. During its last outburst in late September
2012 it reached a peak brightness of m$_v$ $\sim$ 13.5 (M$_v$ brighter than
-18) causing some to speculate that it had undergone a terminal core-collapse
supernova. Relatively high-cadence multi-wavelength photometry of the post-peak
decline revealed bumps in brightness infrequently observed in other Type IIn
supernovae. These bumps occurred synchronously in all UV and optical bands with
amplitudes of 0.1 -- 0.4 mag at intervals of 10 -- 30 days. Episodic continuum
brightening and dimming in the UV and optical with these characteristics is not
easilly explained within the context of models that have been proposed for the
late September 2012 outburst of SN 2009ip. We also present evidence that the
post peak fluctuations in brightness occur at regular intervals and raise more
questions about their origin.
