It orbits the Sun at a distance of 4.7–5.6 AU once every 11 years and 6 months (4,213 days; semi-major axis of 5.1 AU). Its orbit has an eccentricity of 0.09 and an inclination of 22° with respect to the ecliptic.[3]
The body's observation arc begins with its first observation as 1940 YG at Turku Observatory in December 1940, more than 40 years prior to its official discovery observation at Anderson Mesa.[1]
Several rotational lightcurves of Teucer have been obtained from photometric observations since 1992.[11][15][16][17][18] Analysis of the best-rated lightcurve from September 2010, by Daniel Coley at the Center for Solar System Studies (U80) gave a well-defined rotation period of 10.145±0.001 hours with a brightness amplitude of 0.20 magnitude (U=3).[4][11][a]
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Teucer measures between 89.43 and 113.99 kilometers in diameter and its surface has an albedo between 0.059 and 0.073.[8][9][10]
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0435 and a diameter of 110.72 kilometers based on an absolute magnitude of 8.8.[4] In June 2014, an observed asteroid occultation gave a cross-section of 114.0 km × 114.0 km (poor fit).[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.
Notes
^ abLightcurve plots of (2797) Teucer from 2010, 2014-A, 2014-B and 2015 by Daniel Coley and/or Robert Stephens at the Center for Solar System Studies (U80) and (U81). Quality code is 3/3-/3/3 (lightcurve rating at CS3). Summary figures at the LCDB and CS3.
^ abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 15 June 2018.
^ 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)
^ abcFrench, Linda M.; Stephens, Robert D.; Lederer, Susan M.; Coley, Daniel R.; Rohl, Derrick A. (April 2011). "Preliminary Results from a Study of Trojan Asteroids". The Minor Planet Bulletin. 38 (2): 116–120. Bibcode:2011MPBu...38..116F. ISSN1052-8091.
^ abVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. S2CID53493339.
^Stephens, Robert D.; Coley, Daniel, R.; French, Linda M. (January 2016). "Large L5 Jovian Trojan Asteroid Lightcurves from the Center for Solar System Studies". The Minor Planet Bulletin. 43 (1): 15–22. Bibcode:2016MPBu...43...15S. ISSN1052-8091.{{cite journal}}: CS1 maint: multiple names: authors list (link)
^Stephens, Robert D.; Coley, Daniel R.; French, Linda M. (October 2014). "Trojan Asteroids Observed from CS3: 2014 January-May". The Minor Planet Bulletin. 41 (4): 210–212. Bibcode:2014MPBu...41..210S. ISSN1052-8091.