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12052 Aretaon

Trojan asteroid


Trojan asteroid

FieldValue
minorplanetyes
name12052 Aretaon
background#C2FFFF
discovery_ref
discovererE. W. Elst
discovery_siteLa Silla Obs.
discovered3 May 1997
mpc_name(12052) Aretaon
alt_names
pronounced
named_afterἈρετάων *Aretāōn*
(Greek mythology)
mp_categoryJupiter trojan
Trojanbackground
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc40.60 yr (14,828 d)
aphelion5.5958 AU
perihelion4.8837 AU
semimajor5.2397 AU
eccentricity0.0680
period11.99 yr (4,381 d)
mean_anomaly197.23°
mean_motion/ day
inclination11.463°
asc_node219.79°
arg_peri85.727°
jupiter_moid0.256 AU
tisserand2.9550
mean_diameter
(calculated)
rotation
albedo(assumed)
spectral_typeC (assumed)
abs_magnitude(R)
10.50
10.6

(Greek mythology) Trojanbackground (calculated)

10.50 10.6

12052 Aretaon is a mid-sized Jupiter trojan from the Trojan camp, approximately 40 km in diameter. It was discovered on 3 May 1997, by Belgian astronomer Eric Elst at ESO's La Silla Observatory in northern Chile. The dark Jovian asteroid has a rotation period of 8.05 hours. It was named after Aretaon from Greek mythology.

Orbit and classification

Aretaon is a 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 orbits the Sun at a distance of 4.9–5.6 AU once every 11 years and 12 months (4,381 days; semi-major axis of 5.24 AU). Its orbit has an eccentricity of 0.07 and an inclination of 11° with respect to the ecliptic. The body's observation arc begins with its first observation as ** at the Palomar Observatory in October 1977, almost 20 years prior to its official discovery observation at La Silla.

Naming

This minor planet was named from Greek mythology after the Trojan warrior Aretaon. He was killed by Teucer during the Trojan War. The official naming citation was published by the Minor Planet Center on 6 January 2003 (M.P.C. 47300).

Physical characteristics

Aretaon is an assumed, carbonaceous C-type asteroid. The majority of Jupiter trojans are D-types, with the remainder being mostly C- and P-type asteroids.

Rotation period

In September 2012, a rotational lightcurve of Aretaon was obtained from photometric observations by Robert Stephens at the Center for Solar System Studies in Landers, California. Lightcurve analysis gave a rotation period of 8.05 hours with a brightness amplitude of 0.17 magnitude (). This period determination was confirmed by astronomers at the Palomar Transient Factory in September 2013, measuring a period of 8.048 hours and an amplitude of 0.19 magnitude in the R-band ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Aretaon measures 39.151 kilometers in diameter and its surface has an albedo of 0.073, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 42.23 kilometers based on an absolute magnitude of 10.6.

References

Info: Wikipedia Source

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