  Clusters of galaxies are one of the few prominent classes of objects
predicted to emit gamma rays not yet detected by satellites like EGRET or
ground-based Imaging Atmospheric Cherenkov Telescopes (IACTs). The detection of
Very High Energy (VHE, E > 100 GeV) gamma rays from galaxy clusters would
provide insight into the morphology of non-thermal particles and fields in
clusters. VERITAS, an array of four 12-meter diameter IACTs, is ideally
situated to observe the massive Coma cluster, one of the best cluster
candidates in the Northern Hemisphere. This contribution details the results of
VERITAS observations of the Coma cluster of galaxies during the 2007-2008
observing season.
