V485 CENTAURI - THE SHORTEST PERIOD SU UMA STAR

We report CCD observations of the dwarf nova V485 Cen during its 1997 superoutburst. The long lasting outburst with characteristic slope, br ightness dip and presence of clear superhumps give evidence that V485 Cen belongs to the group of SU UMa-type variables. The superhump perio d is equal to 0.042156(d) +/- 0.000004(d) (60.7(m)). Thus, V485 Cen ha s the shortest known period among SU UMa-type stars, with a period as much as 25% shorter than previously known objects. The analysis of tim es of superhump maxima gives clear evidence for the increase of superh ump period with P-sh = 28.3 x 10(-5):This fact confirms the hypothesis that the shortest periods SU UMa variables contrary to other stars of this type have positive values of P-sh.