  We report the discovery of tidal tails around the high-latitude Galactic
globular cluster NGC 5466 in Sloan Digital Sky Survey (SDSS) data. Neural
networks are used to reconstruct the probability distribution of cluster stars
in u,g,r,i and z space. The tails are clearly visible, once extra-galactic
contaminants and field stars have been eliminated. They extend roughly 4
degrees on the sky, corresponding to about 1 kpc in projected length. The
orientation of the tails is in good agreement with the cluster's Galactic
orbit, as judged from the proper motion data.
