  After 10 years of quiescence, HV Vir underwent a superoutburst in January
2002. We report time-series observations clearly revealing the period change of
ordinary superhumps during the superoutburst. We derived a mean superhump
period of 0.058260 d and a positive period derivative of $7 \times 10^{-5}$.
These results are in good agreement with the value obtained from the 1992
superoutburst. We also detected early superhumps, which were not clearly
recognized in the past outburst, and a possible rebrightening. Both of them are
the common characteristics of WZ Sge-type stars.
