Discovery[1] | |
---|---|
Discovered by | N. Danzl |
Discovery site | Kitt Peak Obs. |
Discovery date | 16 September 1998 |
Designations | |
(26308) 1998 SM165 | |
1998 SM165 | |
TNO[2] · twotino[3][4][5] Kozai · distant[1] | |
Orbital characteristics[2] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 2 | |
Observation arc | 32.26 yr (11,784 days) |
Earliest precovery date | 12 October 1982 |
Aphelion | 64.968 AU |
Perihelion | 29.866 AU |
47.417 AU | |
Eccentricity | 0.3701 |
326.52 yr (119,261 days) | |
47.484° | |
0° 0m 10.8s / day | |
Inclination | 13.521° |
183.21° | |
130.22° | |
Known satellites | S/2001 (26308) 1[5] (96±12 km in diameter)[6] |
Physical characteristics | |
Dimensions | 268±28 km (derived)[5] 287±36 km[6] |
Mass | (6.87±0.018)×1018 kg[5] |
Mean density | 0.51+0.29 −0.14 g/cm3[6] |
8.40±0.05 h[6] | |
0.07±0.02[6] | |
5.7[2] | |
(26308) 1998 SM165 is a resonant trans-Neptunian object and binary system from the Kuiper belt in the outermost regions of the Solar System. It was discovered on 16 September 1998, by American astronomer Nichole Danzl at the Kitt Peak National Observatory in Arizona.[1] It is classified as a twotino and measures approximately 280 kilometers in diameter. Its minor-planet moon was discovered in 2001.[5]
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