The SuperWASP project is an ultra-wide angle search for extra solar planetary transits. 
However, it can also serendipitously detect solar system objects, such as asteroids. Each 
SuperWASP instrument consists of up to eight cameras, combined with high-quality 
peltier-cooled CCDs, which photometrically survey large numbers of stars in the magnitude 
range 7-15. Each camera covers a 7.8 × 7.8 degree field of view. This large field of view 
both produces advantages and disadvantages for minor planet observations.  Slow moving 
asteroids stay within a single SuperWASP field for several weeks, and may be seen in many 
fields, providing the opportunity for long-term light curve and phase curve observations. 
However, the slow movement of an asteroid across the stellar background in a SuperWASP 
field, combined with the large (13.7 arcsec) pixels means that there must be a constant
awareness of blending. In addition, issues relating to cross field calibration must be
overcome to produce standard results for asteroids that travel through several fields.  
These issues are discussed and some results from the 2004 SuperWASP dataset are shown.