  We have measured the orbital light curve of dwarf nova OY Carinae on 8
separate occasions between 1997 September and 2005 December. The measurements
were made in white light using CCD photometers on the Mt Canopus 1 m telescope.
The time of eclipse in 2005 December was 168 +- 5 s earlier than that predicted
by the Wood et al.(1989) ephemeris. Using the times of eclipse from our
measurements and the compilation of published measurements by Pratt et al
(1999) we find that the observational data are inconsistent with a constant
period and indicate that the orbital period is decreasing by 5+-1 X 10^-12 s/s.
This is too fast to be explained by gravitational radiation emission. It is
possible that the change is cyclic with a period greater than about 80 years.
This is much longer than typical magnetic activity cycles and may be due to the
presence of a third object in the system. Preliminary estimates suggest that
this is a brown dwarf with mass about 0.016 Msun and orbital radius >= 17 AU.
