A large number of rotational lightcurves were obtained from photometric observations.
They gave a well-defined rotation period of 5.620 to 5.623 hours with a brightness variation between 0.5 and 0.9 magnitude (U=3/3-).
A large number of rotational lightcurves were obtained from photometric observations. They gave a well-defined rotation period of 5.620 to 5.623 hours with a brightness variation between 0.5 and 0.9 magnitude (U=3/3-).
2156 Kate