7336 Saunders, provisional designation 1989 RS1, is a stony asteroid and near-Earth object of the Amor group, approximately 0.5 kilometers in diameter.
Saunders orbits the Sun at a distance of 1.2–3.4 AU once every 3 years and 6 months (1,278 days). Its orbit has an eccentricity of 0.48 and an inclination of 7° with respect to the ecliptic.[1]
In the SMASS classification, Saunders is a Sq-type, which transitions from the common S-type to the Q-type asteroids.[1] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 467 meters, based on an absolute magnitude of 19.02.[4]
Lightcurve
In October 1989, the first photometric observations of Saunders were made with the ESO 1-metre telescope at La Silla in Chile.[5] It gave a rotation period of 6 hours with a brightness variation of 0.3 magnitude (U=2). Another rotational lightcurve was obtained by Czech astronomer Petr Pravec at Ondřejov Observatory in August 2003, giving a period of 6.423±0.004 and an amplitude of 0.2 magnitude (U=n.a.).[a]
Naming
This minor planet was named in honor of JPL-project scientist R. Stephen Saunders (born 1940), director of the RPIF and head scientist of the Solar System Exploration Office. He worked on the Mars Surveyor 2001/03 program and on the Magellan spacecraft, that visited and mapped Venus in 1990.[2] The official naming citation was published by the Minor Planet Center on 26 July 2000 (M.P.C. 41028).[7]
