Discovery[1][2] | |
---|---|
Discovered by | M. E. Brown C. A. Trujillo D. L. Rabinowitz |
Discovery site | Palomar Obs. |
Discovery date | 9 October 2002 |
Designations | |
(84522) 2002 TC302 | |
TNO[3] · 2:5 resonant[4][5] distant[1] | |
Orbital characteristics[3] | |
Epoch 1 July 2021 (JD 2459396.5) | |
Uncertainty parameter 2[3] · 3[1] | |
Observation arc | 20.49 yr (7,484 d) |
Earliest precovery date | 5 August 2000 |
Aphelion | 71.382 AU |
Perihelion | 39.169 AU |
55.275 AU | |
Eccentricity | 0.2914 |
410.97 yr (150,105 d) | |
327.19° | |
0° 0m 8.64s / day | |
Inclination | 34.993° |
23.801° | |
14 December 2058[a] | |
86.312° | |
Physical characteristics | |
Dimensions | 543±18 × 460±11 km (projected area)[6] |
500±14 km (area equiv.)[6] 584.1+105.6 −88.0 km (thermal)[7] | |
56.1 h[6] | |
0.147[6] 0.115+0.047 −0.033[7] | |
IR (moderately red)[8] B–V=1.03[9] V–R=0.67[9] | |
20.5[1] | |
3.94[3][1] 4.23[6] 4.17±0.10[7] | |
(84522) 2002 TC302 (provisional designation 2002 TC302) is a mid-sized trans-Neptunian object located in the outermost region of the Solar System. It was discovered on 9 October 2002, by American astronomers Mike Brown, Chad Trujillo and David Rabinowitz at the Palomar Observatory in California.[1] The resonant trans-Neptunian object stays in a 2:5 resonance with Neptune. It has a reddish color, a rotation period of 56.1 hours and measures at least 500 kilometers (310 miles) in diameter.
MPC-object
was invoked but never defined (see the help page).MPEC2002-V26
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).Buie-DES
was invoked but never defined (see the help page).johnstonsarchive-TNOs
was invoked but never defined (see the help page).Ortiz-2020
was invoked but never defined (see the help page).Fornasier-2013
was invoked but never defined (see the help page).spitzer
was invoked but never defined (see the help page).color
was invoked but never defined (see the help page).
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