It orbits the Sun at a distance of 4.5–6.0 AU once every 12 years and 1 month (4,416 days; semi-major axis of 5.27 AU). Its orbit has an eccentricity of 0.14 and an inclination of 19° with respect to the ecliptic.[3] The body's observation arc begins at Palomar in September 1988, one month prior to its official discovery observation.[1]
Physical characteristics
In the SDSS-based taxonomy, Palinurus is a dark D-type asteroid.[10]Pan-STARRS' survey has also characterized it as a D-type, which is the most common spectral type among the larger Jupiter trojans. It has a high V–I color index of 1.00.[7][9][11]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Palinurus measures 52.06 kilometers in diameter and its surface has an albedo of 0.071,[6]
while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a C-type asteroid of 0.057 and calculates a similar diameter of 53.16 kilometers based on an absolute magnitude of 10.1.[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.
^Lightcurve plot of (4832) Palinurus from Feb 2015 by Robert Stephens at the Center for Solar System Studies (U81). Quality code is 2- (lightcurve rating at CS3). Summary figures at the LCDB and CS3 website.
^Stephens, Robert D.; Coley, Daniel R.; French, Linda M. (July 2015). "Dispatches from the Trojan Camp - Jovian Trojan L5 Asteroids Observed from CS3: 2014 October - 2015 January". The Minor Planet Bulletin. 42 (3): 216–224. Bibcode:2015MPBu...42R.216S. ISSN1052-8091.