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65489 Ceto

Ceto
65489 Ceto.tiff
Orbit (top view)
Discovery
Discovered by C. A. Trujillo and M. Brown
Discovery site Palomar
Discovery date 22 March 2003
Designations
MPC designation 65489
Named after
Ceto
2003 FX128
TNO
Centaur–extended
Adjectives Cetoean
Orbital characteristics
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc 9239 days (25.30 yr)
Aphelion 187.74 AU (28.086 Tm)
Perihelion 17.8498 AU (2.67029 Tm)
102.79 AU (15.377 Tm)
Eccentricity 0.82635
1042.22 yr (380669.7 d)
9.1219°
0.00094570°/day
Inclination 22.266°
171.85°
320.086°
Known satellites Phorcys
(171±10 ~ 132+6
−14
 km
in diameter)
Earth MOID 16.895 AU (2.5275 Tm)
Jupiter MOID 12.7433 AU (1.90637 Tm)
Physical characteristics
Dimensions 223±10 km
174+16
−18
 km
Mass (5.4±0.4)×1018 kg (system)
Mean density
1.37 g/cm3 (system)
Equatorial surface gravity
3.3 cm/s2
4.43 h (0.185 d)
0.056±0.006
0.084±0.02
6.54±0.06, 6.4

65489 Ceto /ˈst/ is a binary trans-Neptunian object (TNO) discovered on March 22, 2003 by C. A. Trujillo and M. Brown at Palomar. It is named after the sea goddess Ceto from Greek mythology. The object was identified as a binary on April 11, 2006 by K. Noll, H. Levison, W. Grundy and D. Stephens using the Hubble Space Telescope; the companion object is named Phorcys (/ˈfɔərss/, formally (65849) Ceto I Phorcys), after the Greek sea god. Using an extended definition of a centaur as an object on a non-resonant (unstable) orbit with its perihelion inside the orbit of Neptune, the Ceto system can be considered the second known binary centaur. It came to perihelion in 1989.

65489 Ceto is an example of a close binary TNO system in which the components are of similar size. Combined observations with the infrared Spitzer Space Telescope and the Hubble Telescope allow the diameter of Ceto itself to be estimated at 174+16
−18
 km
and the diameter of Phorcys at 132+6
−14
 km
, assuming equal albedo for both components.


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