5256 Farquhar

Farquhar is a member of the Eunomia family, the most prominent family in the intermediate main-belt, which mostly consists of stony S-type asteroids. It orbits the Sun in the central main-belt at a distance of 2.0–3.1 AU once every 4 years and 1 month (1,490 days). Its orbit has an eccentricity of 0.20 and an inclination of 15° with respect to the ecliptic. The first observation was made at the U.S. Goethe Link Observatory in 1955, extending the asteroid's observation arc by 33 years prior to its discovery. == Physical characteristics ==

Rotation period In November 2013, a rotational lightcurve of Farquhar was obtained from photometric observations at the Phillips Academy Observatory (), Massachusetts, and at the HUT Observatory (), Colorado. The bimodal lightcurve gave a rotation period of hours with a very low brightness variation of 0.07 in magnitude (). A low brightness amplitude typically indicates a rather spheroidal shape. Diameter and albedo According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Farquhar measures 12.0 and 12.9 kilometers in diameter and its surface has an albedo of 0.148 and 0.128, respectively. The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21, derived from the family's largest member and namesake, 15 Eunomia, and calculates a diameter of 12.1 kilometers with an absolute magnitude of 11.9. == Naming ==

This minor planet was named for American NASA mission design specialist Robert W. Farquhar (1932–2015). At the Goddard Space Flight Center, he designed low-cost spacecraft and missions to explore the Solar System. Farquhar was known for his international collaborations and for designing missions to comets and minor planets using inventive alternative trajectories. The approved naming citation was published by the Minor Planet Center on 10 November 1992 (). == References ==