  The highly successful SuperWASP planetary transit finding programme has
surveyed a large fraction of both the northern and southern skies. There now
exists in the its archive over 420 billion photometric measurements for more
than 31 million stars. SuperWASP provides good quality photometry with a
precision exceeding 1% per observation in the approximate magnitude range 9 < V
< 12. The archive enables long-baseline, high-cadence studies of stellar
variability to be undertaken. An overview of the SuperWASP project is
presented, along with results which demonstrate the survey's asteroseismic
capabilities.
