| Minorplanet: | yes |
| 11552 Boucolion | |
| Background: |
|
| Discovered: | 27 January 1993 |
| Mpc Name: | (11552) Boucolion |
| Alt Names: | |
| Adjective: | Boucolian |
| Pronounced: | [1] |
| Named After: | Boucolion |
| Mp Category: | Jupiter trojan |
| Epoch: | 23 March 2018 (JD 2458200.5) |
| Uncertainty: | 0 |
| Observation Arc: | 25.31 yr (9,243 d) |
| Perihelion: | 4.4713 AU |
| Semimajor: | 5.2694 AU |
| Eccentricity: | 0.1515 |
| Period: | 12.10 yr (4,418 d) |
| Mean Motion: | / day |
| Inclination: | 14.679° |
| Asc Node: | 138.36° |
| Arg Peri: | 182.38° |
| Jupiter Moid: | 0.5638 AU |
| Tisserand: | 2.9120 |
| Mean Diameter: | |
| Albedo: | |
| Abs Magnitude: | 10.1 10.60 |
11552 Boucolion is a Jupiter trojan from the Trojan camp, approximately 53km (33miles) in diameter. It was discovered on 27 January 1993, by Belgian astronomer Eric Elst at the CERGA Observatory in Caussols, France. The dark D-type asteroid is one of the 90 largest Jupiter trojans and has a long rotation period of 32.4 hours. It was named from Greek mythology after the Boucolion, who lost his sons in the Trojan War.
Boucolion is a dark Jupiter trojan in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's Lagrangian point, 60° behind its orbit . It is also a non-family asteroid of the Jovian background population. It orbits the Sun at a distance of 4.5–6.1 AU once every 12 years and 1 month (4,418 days; semi-major axis of 5.27 AU). Its orbit has an eccentricity of 0.15 and an inclination of 15° with respect to the ecliptic.
The asteroid was first observed as at Crimea–Nauchnij in July 1973. The body's observation arc begins with its official discovery observation at Caussols in January 1993.
In the SDSS-based taxonomy, Boucolion is a D-type asteroid, the most common type among the larger Jupiter trojans. It has also been characterized as a D-type by Pan-STARRS' survey, while the Collaborative Asteroid Lightcurve Link assumes it to be a carbonaceous C-type asteroid.
In September 2012, a rotational lightcurve of Boucolion was first obtained from photometric observations by astronomers at the Palomar Transient Factory (PTF) in California. Lightcurve analysis gave a rotation period of 16.150 and 16.177 hours with a brightness amplitude of 0.23 and 0.25 magnitude in the R- and S-band, respectively .
A more refined, alternative period solution of hours with an amplitude of 0.21 magnitude was measured by Robert Stephens at the Center for Solar System Studies in January 2015 . The result seems to be a 1:2 alias, i.e. twice the period, of the previously obtained lightcurve at the PTF. While not being a slow rotator, Boucolion has one of the longest periods among the larger Jupiter trojans (see table below).
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Boucolion measures 51.136 and 53.91 kilometers in diameter and its surface has an albedo of 0.062 and 0.035, respectively. CALL assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 53.16 kilometers based on an absolute magnitude of 10.1.
This minor planet was named from Greek mythology after Boucolion, father of the two Trojan warriors Pedasos and Aesopos, who both were slain near the River Scamander during the Trojan War. The official naming citation was published by the Minor Planet Center on 6 January 2003 .