  We explore the possibility of searching for extratidal features around the
Galactic globular cluster NGC362 using the Gaia DR2 together with a modified
version of a classical statistical decontamination algorithm. Our results
suggest that an important stellar component is associated with this globular
cluster, which is perfectly distinguishable from the populations in the Small
Magellanic Cloud and that of the nearby NGC104 (47 Tucanae). We thus confirm
once again the power of Gaia to disentangle different stellar components along
the same line-of-sight.
