9165 Raup

Classification and orbit

Raup is a bright S-type asteroid is a member of the Hungaria family, which form the innermost dense concentration of asteroids in the Solar System. It orbits the Sun in the innermost main-belt at a distance of 1.8–2.2 AU once every 2 years and 10 months (1,022 days). Its orbit has an eccentricity of 0.10 and an inclination of 25° with respect to the ecliptic.

It was first identified as at the discovering observatory in 1955, extending the body's observation arc by 32 years prior to its official discovery observation.

Physical characteristics

Slow rotator

In September 2015, a rotational lightcurve of Raup was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Station in Colorado. It gave a well-defined rotation period of hours with a brightness variation of 1.34 magnitude ().

As of 2016, it is the 3rd slowest rotating minor planet in the Light Curve Data Base (LCDB). Also, the lightcurve's high amplitude indicates that the body has a non-spheroidal shape. Brian Warner's 2015-observation supersedes a previously obtained lightcurve that gave a significantly shorter period of hours with an amplitude of 1.05 magnitude ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Raup measures 4.8 kilometers in diameter and its surface has a high albedo of 0.329, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for Hungaria asteroids of 0.30, and calculates a diameter of 4.6 kilometers, based on an absolute magnitude of 13.6.

Naming

This minor planet was named in honor of American David M. Raup (1933–2015), paleontologist and expert on the fossil record at UChicago. Raup's theories contributed to the knowledge of extinction events and suggested, that the extinction of dinosaurs was part of a cycle of mass extinctions. the official naming citation was published on 23 November 1999 (M.P.C. ).

References