  In this brief article we discuss the corrections to the photon orbits of a
non-rotating black hole due to semiclassical fluctuations of the metric. It is
found that the photon orbit impact parameter differences with the critical
impact parameter become of the order of the semiclassical fluctuations. We
calculate the effect of the semi-classical fluctuations on the photon orbits
and show that instead of circulating the black hole infinite number of times at
the critical orbit, the photons bounce off the semiclassical geometry.
