  We present the results obtained from unfiltered photometric CCD observations
of V1193 Ori made during 24 nights between November 2002 and January 2003. We
found periods of 0.1430 d, 0.1362 d and possibly 2.98 d in the data. The 0.1430
d period is consistent with the 1d^{-1} alias of the proposed orbital period of
P_{orb}=0.165 d (Ringwald et al., 1994, Papadaki et al., 2004). Thus and using
the known relation between the orbital and superhump periods, we interpret
these periods as the orbital period of 0.1430 d, the negative superhump period
of 0.1362 d and the precession period of 2.98 d. V1193 Ori can then be
classified as a permanent superhump system.
