It orbits the Sun at a distance of 4.5–5.8 AU once every 11 years and 10 months (4,308 days;semi-major axis of 5.18 AU). Its orbit has aneccentricity of 0.12 and aninclination of 9° with respect to theecliptic.[4] The body'sobservation arc begins at Heidelberg in November 1917, two months after its official discovery observation.[1]
Between January 2015, and December 2016, photometric observations by Robert Stephens and Daniel Coley in collaboration withBrian Warner at theCenter for Solar System Studies, California, gave a three concurring periods of 6.854, 6.863 and 6.865 hours (U=3/3/3).[17][18][19][a]
According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Priamus measures 101.09 and 119.99 kilometers in diameter and its surface has analbedo of 0.044 and 0.037, respectively.[8][9] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 96.29 kilometers based on anabsolute magnitude of 8.81.[5]
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 plots of (884) Priamus fromJan 2015,Jan 2016 andDec 2016 by Daniel Coley andRobert Stephens at the Center for Solar System Studies (U80) and (U81). Quality code is 3/3/3 (lightcurve rating at CS3). Summary figures at theLCDB andCS3.
^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)