The VERITAS array of Cherenkov telescopes, designed for the detection of very high energy gamma rays in the 100 GeV-10 TeV energy range, performs dark matter searches over a wide variety of targets. VERITAS continues to carry out focused observations of dwarf spheroidal galaxies in the Local group, the Milky Way galactic center, and Fermi LAT unidentified GeV sources. This presentation reports on our extensive observations of these targets, new statistical techniques, and current constraints on dark matter particle physics derived from these observations.