Hubble Space Telescope image of Varuna | |
| Discovery | |
|---|---|
| Discovered by | R. McMillan (Spacewatch) |
| Discovery date | 28 November 2000 |
| Designations | |
| MPC designation | 20000 Varuna |
| 2000 WR106 | |
| TNO (cubewano) | |
| Orbital characteristics | |
| Epoch 14 July 2004 (JD 2453200.5) | |
| Aphelion | 6 781.985 Gm (45.335 AU) |
| Perihelion | 6 120.810 Gm (40.915 AU) |
| 6 451.398 Gm (43.129 AU) | |
| Eccentricity | 0.051 |
| 103 440.6 d (283.20 a) | |
Average orbital speed | 4.53 km/s |
| 89.673° | |
| Inclination | 17.2° |
| 97.296° | |
| 271.631° | |
| Physical characteristics | |
| Dimensions | 800 km (avg of thermals) (scalene ellipsoid)? |
| Mass | ≈3.7×1020? kg |
Mean density | 0.992 g/cm³ |
| 0.15 m/s² | |
| 0.39 km/s | |
Sidereal rotation period | 0.132 16 d (3.17 h) |
| Albedo | 0.037–0.26 |
| Temperature | ≈43–41 K |
Spectral type | (moderately red) B-V=0.93 V-R=0.64 |
| 19.9 (opposition) | |
| 3.7 | |
20000 Varuna is a big Kuiper belt object (KBO). It could be a dwarf planet. Before it was named Varuna, it had the provisional designation 2000 WR106.
Varuna is named after the Hindu deity Varuṇa.
Varuna completes one rotation in about 3.17 hours (or 6.34 hours, depending on whether the light curve is single or double-peaked). Given the fast rotation, which is not common for objects so big, Varuna is thought to be a stretched spheroid, with a density around 1g/cm³ (close to the density of water).
The surface of Varuna is somewhat red and small amounts of water ice have been found on its surface.
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