5040 Rabinowitz

Orbit and classification

The stony S-type asteroid is a member of the Phocaea family (701), a group of asteroids with similar orbital characteristics, named after its largest member, 25 Phocaea. It orbits the Sun in the inner main-belt at a distance of 1.9–3.0 AU once every 3 years and 9 months (1,373 days). Its orbit has an eccentricity of 0.23 and an inclination of 24° with respect to the ecliptic. A first precovery was taken at the discovering observatory in 1971, extending the body's observation arc by one year prior to its official discovery observation.

Physical characteristics

Rotation period

In July 2013, a rotational lightcurve for this asteroid was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory. The well-defined lightcurve gave a rotation period of hours with a brightness variation of 0.33 in magnitude ().

During the same opposition opportunity, two more lightcurves – obtained by Robert Stephens at the Center for Solar System Studies and by Maurice Clark at the Preston Gott Observatory – gave a similar period of and hours, with an amplitude of 0.35 and 0.31 in magnitude, respectively ().

Diameter and albedo

The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.23, derived from the Phocaea family's namesake, and calculates a diameter of 6.4 kilometers with an absolute magnitude of 13.18.

Naming

This minor planet was named after American astronomer David Rabinowitz (born 1960), a discoverer of minor planets himself and researcher at Yale University. The naming also honors his work for the Spacewatch program. The official naming citation was published by the Minor Planet Center on 1 September 1993 (M.P.C. 22505).

Notes

References

|access-date = 20 June 2017}}

|access-date = 1 July 2016}}

|access-date = 1 July 2016}}

|access-date = 27 October 2019}}

|access-date = 1 July 2016}}

|access-date= 1 July 2016}}

|access-date= 1 July 2016}}

|display-authors = 6 |access-date= 1 July 2016}}