5692 Shirao

Orbit and classification

Shirao is a member of the Eunomia family, a large group of stony asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in the central main-belt at a distance of 2.2–3.1 AU once every 4 years and 4 months (1,580 days). Its orbit has an eccentricity of 0.18 and an inclination of 12° with respect to the ecliptic.

In 1949, it was first identified as at Goethe Link Observatory. The body's observation arc begins in 1955, with a precovery at Palomar Observatory, 37 years prior to its official discovery observation at Kitami.

Physical characteristics

Rotation period

In June 2014, a rotational lightcurve of Shirao was obtained from photometric observations made by American astronomer Brian Warner at his Palmer Divide Observatory (716) in Colorado. It gave a well-defined rotation period of hours with a brightness variation of 0.16 magnitude ().

Previous lightcurves were obtained by French astronomer René Roy ( hours, Δ 0.13 mag, ) in June 2001, by American astronomer Donald P. Pray ( hours, Δ 0.12 mag, ) in March 2005, and by astronomers Dominique Suys, Hugo Riemis and Jan Vantomme ( hours, Δ 0.15 mag, ) in September 2006.

Diameter and albedo

According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission, Shirao measures between 9.5 and 9.8 kilometers in diameter and its surface has an albedo of 0.22, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo of 0.21 – derived from 15 Eunomia, the largest member and namesake of this asteroid family – and calculates a diameter of 9.2 kilometers.

Naming

This minor planet was named after Motomaro Shirao (born 1953), a Japanese geologist and astrophotographer, who is known for his photographs of volcanoes and lunar geological features. The official naming citation was published by the Minor Planet Center on 4 April 1996 (M.P.C. 26930).

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