In 2009,Photometric observations of this asteroid were made at the Palmer Divide Observatory inColorado Springs, Colorado. The resultinglight curve shows a synodicrotation period of 17.625 ± 0.004 hours with a brightness variation of 0.30 ± 0.03 inmagnitude. Previous independent studies produced inconsistent results that differ from this finding.[4]
^P. Maley; T. George; J. Bardecker; T. Blank; D. Dunham; D. Kenyon; J. Gout; M. Collins; B. Gimple; W. Thomas; J. Bean; R. Sumner; M. Collins (9 February 2018),Stellar occultation from 191 Kolga (preliminary analysis), archived fromthe original on 4 October 2018, retrieved3 October 2018