Attempts to measure the rotation period of this asteroid have produced inconsistent results ranging from 14.7 to 32 hours.Photometric observations of this asteroid at the Organ Mesa Observatory inLas Cruces, New Mexico during 2010 gave an irregularlight curve with a period of 34.407 ± 0.002 hours and a brightness variation of 0.05 ± 0.01 inmagnitude.[2]
^Greyzeck, Ed (2013),"Rosetta",NSS Data Center, NASA, retrieved30 March 2013.
^Takir, Driss; Emery, Joshua P. (June 2012), "Outer Main Belt asteroids: Identification and distribution of four 3-μm spectral groups",Icarus, vol. 219, no. 2, pp. 641–654,Bibcode:2012Icar..219..641T,doi:10.1016/j.icarus.2012.02.022.