1998 WW31

1998 WW31

Artist's Impression of 1998 WW31 and its satellite
Discovery
Discovered by Deep Ecliptic Survey
Discovery date 18 November 1998
Designations
MPC designation 1998 WW31
none
Trans-Neptunian object
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 4
Observation arc 4784 days (13.10 yr)
Aphelion 48.432 AU (7.2453 Tm)
Perihelion 40.847 AU (6.1106 Tm)
44.640 AU (6.6780 Tm)
Eccentricity 0.084953
298.26 yr (108938 d)
4.46 km/s
137.944°
 0m 11.897s /day
Inclination 6.8069°
237.116°
50.406°
Known satellites 1
Earth MOID 39.8336 AU (5.95902 Tm)
Jupiter MOID 35.6694 AU (5.33607 Tm)
Physical characteristics
Dimensions 133±15 km
Mass 1.32.5×1018 kg (system)
Mean density
1.5 g/cm³ (assumed)
Equatorial surface gravity
0.0250.031 m/s²
Equatorial escape velocity
0.0540.068 km/s
570 d (system orbital period)
0.05–0.09 (assumed)
Temperature ~42 K
6.7

    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.

    References

    1. "JPL Small-Body Database Browser: (1998 WW31)". Jet Propulsion Laboratory. Retrieved 29 March 2016.

    External links


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