The edge of the solar system

We have surveyed for Kuiper Belt objects (KBOs) in six fields of the eclipt ic (total sky area 1.5 deg(2)) to limiting magnitudes between R = 24.9 and R = 25.9. This is deep enough to detect KBOs of diameter greater than or si milar to 160 km at a distance of 65 AU. We detected 24 objects. None of the se objects, however, is beyond 53 AU. Our survey places a 95% CL upper limi t of Sigma < 5 deg(-2) on the surface density of KBOs larger than <similar to>160 km beyond 55 AU. This can be compared to the surface density of simi lar to6 deg(-2) of greater than or equal to 160 km KBOs at distances 30-50 AU determined from this survey and previous shallower surveys. The mean vol ume density of D > 160 km KBOs in the 55-65 AU region is, at greater than 9 5% confidence, less than the mean density in the 30-50 AU region, and at mo st two-thirds of the mean density from 40 to 50 AU. Thus, a substantial den sity increase beyond 50 AU is excluded in this model-independent estimate. A dense primordial disk could be present beyond 50 AU if it contains only s maller objects or is sufficiently thin and inclined to have escaped detecti on in our six survey fields.