  We report the discovery of tidal tails around the Galactic globular cluster
NGC 7492, based on the Data Release 1 of the Pan-STARRS 1 survey. The tails
were detected with a version of the matched filter technique applied to the
$(g-r,r)$ and $(g-i,i)$ color-magnitude diagrams. Tidal tails emerging from the
cluster extend at least $\sim$3.5 degrees in the North-East to South-East
direction, equivalent to $\sim1.5$ kpc in projected length.
