10199 Chariklo

10199 Chariklo
Hubble Space Telescope image of Chariklo taken in 2015
Discovery
Discovered bySpacewatch (J. Scotti)
Discovery siteKitt Peak Obs.
Discovery date15 February 1997
Designations
(10199) Chariklo
Pronunciation/ˈkærəkl/
Named after
Χαρικλώ Khariklō
(Ancient Greek nymph)
1997 CU26
centaur · distant
AdjectivesCharikloan, Charikloian /kærəˈkl(i)ən/
Symbol
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 1
Observation arc26.51 yr (9,684 days)
Earliest precovery date5 November 1988
Aphelion18.545 AU
Perihelion13.099 AU
15.822 AU
Eccentricity0.1721
62.93 yr (22,987 days)
77.670°
0° 0m 56.52s / day
Inclination23.382°
300.42°
  • 25 June 2066
  • 17 December 2003 (previous)
242.90°
Known satellites(2) rings of Chariklo · (undiscovered embedded or shepherd moons?)
Jupiter MOID8.1850 AU
TJupiter3.4820
Physical characteristics
248±18 km
254 km
(296x264x204 km)
(287.6x270.4x198.2 km)
7.004±0.036 h
0.045±0.010
0.10±0.02
0.035±0.010
0.042±0.005
0.057 (assumed)
SMASS = D · D
BR (G-mode)
B−V = 0.84
V−R = 0.50±0.03
B−R = 1.34
V−I = 1.02±0.02
R−J = 0.99
V−J = 1.49±0.07
J−H = 0.49
V−H = 1.98±0.08
18.3
6.569±0.015 (R) · 6.6 · 6.65 · 6.75 · 6.76 · 7.07±0.04 · 7.08±0.04 · 7.03±0.10 · 7.40±0.25

    10199 Chariklo /ˈkærəkl/ is the largest confirmed centaur, a class of minor planet in the outer Solar System. It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chuí after the rivers that define Brazil's borders) around Chariklo by observing a stellar occultation, making it the first minor planet known to have rings.

    A photometric study in 2001 was unable to find a definite period of rotation. Infrared observations of Chariklo indicate the presence of water ice, which may in fact be located in its rings.