28978 Ixion

28978 Ixion (/ɪkˈs.ən/, provisional designation 2001 KX76) is a large trans-Neptunian object and a possible dwarf planet. It is located in the Kuiper belt, a region of icy objects orbiting beyond Neptune in the outer Solar System. Ixion is classified as a plutino, a dynamical class of objects in a 2:3 orbital resonance with Neptune. It was discovered in May 2001 by astronomers of the Deep Ecliptic Survey at the Cerro Tololo Inter-American Observatory, and was announced in July 2001. The object is named after the Greek mythological figure Ixion, who was a king of the Lapiths.

28978 Ixion
Hubble Space Telescope image of Ixion taken in 2006
Discovery
Discovered byDeep Ecliptic Survey
Discovery siteCerro Tololo Obs.
Discovery date22 May 2001
Designations
MPC designation
(28978) Ixion
Pronunciation/ɪkˈs.ən/
Named after
Ιξίων Ixīōn
Alternative designations
2001 KX76
Minor planet category
TNO · plutino · distant
AdjectivesIxionian /ɪksiˈniən/
Symbol or (astrological)
Orbital characteristics
Epoch 17 December 2020 (JD 2459200.5)
Uncertainty parameter 3
Observation arc35.93 yr (13,122 days)
Earliest precovery date17 July 1982
Aphelion49.584 AU
Perihelion30.019 AU
Semi-major axis
39.802 AU
Eccentricity0.24579
Orbital period (sidereal)
251.11 yr (91,717 d)
Mean anomaly
289.587°
Mean motion
0° 0m 14.13s / day
Inclination19.600°
Longitude of ascending node
71.011°
≈ 24 September 2070
±1 day
298.314°
Physical characteristics
Dimensions756.9 km × 684.9 km (projected, occultation)
Mean diameter
709.6±0.2 km
Synodic rotation period
12.4±0.3 h
15.9±0.5 h
0.108±0.002 geometric
0.037±0.007 Bond
Temperature64+0.7
−1.1
 K
IR (moderately red)
B–V=1.009±0.051
V–R=0.61±0.03
V–I=1.146±0.086
19.8
3.774±0.021
3.6 (assumed)

    In visible light, Ixion appears dark and moderately red in color due to organic compounds covering its surface. Water ice has been suspected to be present on Ixion's surface, but may exist in trace amounts hidden underneath a thick layer of organic compounds. Ixion has a measured diameter of 710 km (440 mi), making it the fourth-largest known plutino. Several astronomers have considered Ixion to be a possible dwarf planet, whereas others consider it a transitional object between irregularly-shaped small Solar System bodies and spherical dwarf planets. Ixion is currently not known to have a natural satellite, so its mass and density remain unknown.

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