Lightcurves A rotational
lightcurve obtained in the 1970s gave a well-defined
rotation period of 6.3 hours with a brightness amplitude of 0.75 in
magnitude (). In March 2016, a second period was published based on data from the Lowell Photometric Database (LPD). Using lightcurve inversion and convex shape models, as well as distributed computing power and the help of individual volunteers, a period of hours could be obtained for this asteroid from the LPD's sparse-in-time photometry data ().
Diameter and albedo According to the space-based surveys carried out by the Infrared Astronomical Satellite
IRAS, the Japanese
Akari satellite, and NASA's
Wide-field Infrared Survey Explorer with its subsequent
NEOWISE mission, the asteroid measures between 31.5 and 42.0 kilometers in diameter and its surface has an
albedo in the range of 0.0795 to 0.141. The
Collaborative Asteroid Lightcurve Link (CALL) gives preference to the results obtained by IRAS with an albedo of 0.1219 and a diameter of 33.93 kilometers. CALL also classifies the Themistian asteroid as a stony
S-class body, which are otherwise known to have low albedos, showing
spectra of carbonaceous
C-type bodies
(also see Carbonaceous chondrites). == Notes ==