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The Crab Nebula has long been considered a standard candle in high energyastrophysics, but in recent years this assumption has been stronglycontradicted in keV-GeV wavebands. In light of these developments, a search forvariability is being performed on the nebula at Very High Energies (VHE; E>300GeV), the preliminary results of which are presented here. This initial studyis based on 10 years (2001-2011) of archival data from the Whipple 10 mtelescope. The data set was searched for evidence of variability on thetimescales of 1, 7, and 14 days. To date, no significant flaring activity hasbeen found, but simulations are in progress to determine the level ofvariability that would be detected.

A Search for Short-term Variability in the Very High Energy Gamma-ray Emission from the Crab Nebula