It orbits the Sun at a distance of 4.7–5.9 AU once every 12 years and 1 month (4,426 days; semi-major axis of 5.28 AU). Its orbit has an eccentricity of 0.11 and an inclination of 25° with respect to the ecliptic.[3] The body's observation arc begins with its first observation at Palomar in September 1988, just one month prior to its official discovery observation.[1]
Physical characteristics
Bitias is an assumed, carbonaceous C-type asteroid. It has a low V–I color index of 0.78.[7]
In August 2013, a more refined period determination from observations over seven consecutive nights by Robert Stephens at the Center for Solar System Studies gave a well-defined period of 15.21±0.02 hours with an amplitude of 0.32 magnitude (U=3).[8][a]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Bitias measures between 47.987 and 47.99 kilometers in diameter and its surface has an albedo,[6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 50.77 kilometers based on an absolute magnitude of 10.2.[7]
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 warrior Bitias. He survived the Trojan War and was a companion in Aeneas' exile. He was later killed in Italy with a whirling pike during the Latin War.[1] The official naming citation was published by the Minor Planet Center on 4 June 1993 (M.P.C. 22248).[11]
Notes
^ abLightcurve plots of (3317) Paris from Aug 2013 by Robert Stephens at the Center for Solar System Studies (U81). Quality code is 3- (lightcurve rating at CS3). Summary figures at the LCDB and CS3.
^ abStephens, Robert D.; French, Linda M.; Davitt, Chelsea; Coley, Daniel R. (April 2014). "At the Scaean Gates: Observations Jovian Trojan Asteroids, July- December 2013". The Minor Planet Bulletin. 41 (2): 95–100. Bibcode:2014MPBu...41...95S. ISSN1052-8091.