  We report the results of careful astrometric measurements of the Cannonball
pulsar J0002+6216 carried out over three years using the High Sensitivity Array
(HSA). We significantly refine the proper motion to $\mu=35.3\pm0.6$ mas
yr$^{-1}$ and place new constraints on the distance, with the overall effect of
lowering the velocity and increasing the inferred age to $47.60\pm0.80$ kyr.
Although the pulsar is brought more in line with the standard natal kick
distribution, this new velocity has implications for the morphology of the
pulsar wind nebula that surrounds it, the density of the interstellar medium
through which it travels, and the age of the supernova remnant (CTB 1) from
which it originates.
