We report the discovery from the H I Parkes All-Sky Survey (HIPASS) of a ga
s cloud associated with the asymmetric spiral galaxy NGC 2442. This object,
designated HIPASS J0731-69, contains similar to 10(9) M-. of H I, or nearl
y one-third as much atomic gas as NGC 2442 itself. No optical counterpart t
o any part of HIPASS J0731-69 has yet been identified, consistent with the
gas being diffuse and its streamlike kinematics. If the gas in HIPASS J0731
-69 was once part of NGC 2442, then it was most likely a fairly recent tida
l encounter with a moderately massive companion that tore it loose, althoug
h the possibility of ram-pressure stripping cannot be ruled out. This disco
very highlights the potential of the HIPASS data for yielding new clues to
the nature of some of the best-known galaxies in the local universe.