Lightcurves A large number of rotational
lightcurves for this asteroid were obtained from several photometric observations. The first observations were made by Italian astronomer
Silvano Casulli in November 2006, and gave a
rotation period hours with a brightness amplitude of 0.19 in
magnitude (). One month later, in December 2006, observations at the Carbuncle Hill Observatory gave a period of hours with an identical amplitude of 0.19 in magnitude (). Between November 2009 and December 2012, Czech astronomer
Petr Pravec at
Ondřejov Observatory obtained three more lightcurves with periods between 3.2235 and 3.2237 hours and corresponding amplitudes of 0.07. 0.10 and 0.10, respectively ().
Diameter and albedo According to the space-based surveys carried out by the Japanese
Akari satellite and the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer, the asteroid measures between 8.0 and 10.7 kilometers in diameter, respectively, and its surface has an
albedo between 0.035 and 0.282. Astronomer Petr Pravec and the
Collaborative Asteroid Lightcurve Link derive an albedo of 0.21 and a diameter of 10.7 kilometers with an
absolute magnitude of 12.4. == Naming ==