Barklajdetolli has been characterized as a common stony
S-type asteroid.
Slow rotator and shape In August 2009, a rotational
lightcurve for this asteroid was obtained at the Carbuncle Hill Observatory in Rhode Island, United States. Lightcurve analysis gave an exceptionally long
rotation period of 1,069 hours with a high brightness amplitude of 1.26 in
magnitude (). While the period still may be wrong by a few hundred hours, it is one of the
slowest rotating asteroids known to exist. The exceptionally high variation in brightness indicates that the body has a non-spheroidal shape.
Diameter and albedo According to the surveys carried out by the Japanese
Akari satellite and NASA's
Wide-field Infrared Survey Explorer with its subsequent
NEOWISE mission, the asteroid's surface has a low
albedo of 0.05 and 0.10, respectively, while the
Collaborative Asteroid Lightcurve Link (CALL) assumes a much higher albedo of 0.24, derived from its Flora family classification. The divergent albedos also translate into different estimates for the body's size. While the space-based surveys find a diameter of 12.1 and 13.6 kilometers, respectively, CALL calculates only 7.1 kilometers, as the higher a body's albedo (reflectivity), the smaller its diameter for a certain
absolute magnitude. == Naming ==