Slow rotator Alekhin is a
slow rotator. In March 2009 and September 2010, two rotational
lightcurves for
Alekhin were obtained from photometric observations made by the
Palomar Transient Factory and by astronomer Roger Dymock, respectively. The lightcurves gave a
rotation period of 148 hours with a brightness variation of 0.42–0.45
magnitude ().
Diameter and albedo According to the 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,
Alekhin measures between 15.5 and 18.8 kilometers in diameter and its surface has an
albedo of 0.046 to 0.070. The
Collaborative Asteroid Lightcurve Link derives an albedo of 0.045 and a diameter of 17.3 kilometers with an
absolute magnitude of 12.8.
Occultation Alekhin is scheduled to occlude a 9.1 magnitude star in the
Leo constellation on 30 November 2008, dimming the magnitude of both heavenly bodies for a maximum duration of 0.6 seconds.
Astronomers had, as of March 2008, not predicted an optimal trajectory for the event. == Naming ==