We discovered a new deeply eclipsing SU UMa-type dwarf nova, TY UMa, which
experienced a superoutburst in 2000 January. Our monitoring revealed two di
stinct outbursts, which suggest a superoutburst interval of similar to 800
d, or its half, and an outburst amplitude of 5.4 mag. From time-series phot
ometry during the superoutburst, we determined a superhump and orbital peri
od of 0.07588 d and 0.0739132 d, respectively.