| Orbit diagram of its orbit. | |
| Discovery | |
|---|---|
| Discovered by | J. A. Larsen N. Danzel A. Gleason |
| Discovery date | 14 November 1998 |
| Designations | |
| plutino [1] | |
| Orbital characteristics [2] | |
| Epoch 9 June 2026 (JD 2461200.5) | |
| Uncertainty parameter 1 | |
| Observation arc | 27.25 years |
| Aphelion | 49.8 AU |
| Perihelion | 29.38 AU |
| 39.59 AU | |
| Eccentricity | 0.25786 |
| 249.1 yr (90986 d) | |
| 17.74° | |
| 0° 0m 14.357s / day | |
| Inclination | 3.034° |
| 127.96° | |
| 324.79° | |
| Uranus MOID | 10.38 AU (1.55 billion km) [3] |
| Neptune MOID | 0.054 AU (8.08 million km) [3] [a] |
| Physical characteristics | |
| Dimensions | 248 km (assumed) |
| 0.09 (assumed) | |
| 6.4 | |
(33340) 1998 VG44 is a trans-Neptunian object. It has a 2:3 orbital resonance with the planet Neptune, similar to Pluto, classifying it as a plutino. [1] Its average distance from the Sun is 39.6 AU with a perihelion of 29.4 AU and an aphelion at 49.8 AU. Its orbit has an eccentricity of 0.26, and is inclined by 3°. The object is estimated to be about 248 km in diameter. It was discovered on 14 November 1998, by J. A. Larsen, Nicole M. Danzl and A. Gleason at the Steward Observatory.
Though it has a Neptune MOID of 0.054 AU (8.08 million km), [3] it can not get that close to Neptune because of the 3:2 resonance with Neptune.
| Epoch | Neptune MOID |
|---|---|
| 2024-10-17 | 0.0097 AU (1.45 million km) |
| 2026-06-09 [3] | 0.054 AU (8.08 million km) |