Photometric observations of this asteroid atPalmer Divide Observatory inColorado Springs, Colorado, during 2007 gave alight curve with a period of9.262±0.001 hours and a brightness variation of0.83±0.03 inmagnitude.[7] A 2012 study based upon observations at the Organ Mesa Observatory inLas Cruces, New Mexico, during 2012 produced a conflicting period of7.834±0.001 hours and a brightness variation of0.17±0.02 inmagnitude. Further study will be needed to resolve the discrepancies in period and amplitude.[8]
^Warner, Brian D. (June 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory – June–October 2007",The Minor Planet Bulletin,35 (2):56–60,Bibcode:2008MPBu...35...56W.
^Pilcher, Frederick (October 2012), "Rotation Period Determinations for 47 Aglaja, 252 Clementina, 611 Valeria, 627 Charis, and 756 Lilliana",Minor Planet Bulletin,39 (4):220–222,Bibcode:2012MPBu...39..220P.