1998 WW31
Artist's Impression of 1998 WW31
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Discovery
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| Discovered by | Deep Ecliptic Survey |
| Discovery date | 18 November 1998 |
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Designations
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| MPC designation | 1998 WW31 |
| Alternate name(s) | none |
| Minor planet category |
Trans-Neptunian object |
| Epoch June 14, 2006 (JD 2453900.5) | |
| Aphelion | 48.419 AU (7243.350 Gm) |
| Perihelion | 40.559 AU (6067.553 Gm) |
| Semi-major axis | 44.489 AU (6655.451 Gm) |
| Eccentricity | 0.088 |
| Orbital period | 296.75 a (108386.849 d) |
| Average orbital speed | 4.46 km/s |
| Mean anomaly | 126.983° |
| Inclination | 6.818° |
| Longitude of ascending node | 237.108° |
| Argument of perihelion | 49.588° |
| Satellites | 1 |
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Physical characteristics
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| Dimensions | 133±15 km |
| Mass | 1.3–2.5×1018 kg (system) |
| Mean density | 1.5 g/cm³ (assumed) |
| Equatorial surface gravity | 0.025–0.031 m/s² |
| Escape velocity | 0.054–0.068 km/s |
| Sidereal rotation period |
570 d (system orbital period) |
| Albedo | 0.05–0.09 (assumed) |
| Temperature | ~42 K |
| Absolute magnitude (H) | 6.05 |
1998 WW31 (also written 1998 WW31) is a double Kuiper belt object. It was discovered in 1998 by the Deep Ecliptic Survey (DES).
1998 WW31 forms a binary system with another object with the IAU provisional designation S/2000 (1998 WW31) 1: the first trans-Neptunian binary to be discovered since Pluto, and one of the most symmetrical binaries known in the Solar System. The two bodies are very close in size, with a diameter ratio of 1.2 and a mass ratio of 1.74, assuming similar surfaces and densities. Their orbital period is approximately 570 days, and they orbit at a distance of approximately 4000 km (closest approach) to 40,000 km, with a semi-major axis of about 22,000 km. Their diameters are likely to be in the 100–150 km range, assuming a density of 1–2 g/cm³. Their combined mass is 1/6000th that of the Pluto–Charon system.
[edit] External links
- The IAU circular announcing the discovery of the companion
- 1998 WW31 and S/2000 (1998 WW31) 1
- Discussion at CFHT, Hawaii
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