It orbits the Sun at a distance of 5.1–5.3 AU once every 11 years and 9 months (4,285 days; semi-major axis of 5.16 AU). Its orbit has an eccentricity of 0.02 and an inclination of 27° with respect to the ecliptic.[3] The body's observation arc begins with its first observation as 1988 RN1 at Palomar in September 1988, or one year prior to its official discovery observation.[1]
Physical characteristics
Polites is an assumed C-type asteroid. Its V–I color index of 1.01 is one of the highest among the larger Jupiter trojans (see table below).[9]
According to the surveys carried out by the Japanese Akari satellite, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, and the Infrared Astronomical Satellite IRAS, Polites measures between 57.25 and 65.16 kilometers in diameter and its surface has an albedo between 0.071 and 0.078.[6][7][8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 58.29 kilometers based on an absolute magnitude of 9.9.[9]
100+ largest Jupiter trojans
Largest Jupiter Trojans by survey(A) (mean-diameter in kilometers; YoD: Year of Discovery)
Note: missing data was completed with figures from the JPL SBDB (query) and from the LCDB (query form) for the WISE/NEOWISE and SIMPS catalogs, respectively. These figures are given in italics. Also, listing is incomplete above #100.
Naming
This minor planet was named by the discoverer from Greek mythology after the Trojan prince Polites, son of King Priam and Hecuba. He was killed with a spear handled by Achille's son Neoptolemus (Pyrrhus), who was the most ruthless of the Greeks. During the fall of Troy, he invaded Priam's great house and chased Polites until he cornered and slaughtered him in front of his parents.[1]
^ abLightcurve plots of (4867) Polites from Aug 2013 (DC), Aug 2013 (RDS), 2014, 2016, 2017, 2018, by Daniel Coley and Robert Stephens at the Center for Solar System Studies (U81). Quality code is 3-/2/3-/3/2+/3 (lightcurve rating at CS3). Summary figures at the LCDB and CS3.
^ abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)