(303775) 2005 QU182

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(303775) 2005 QU182
Discovery[1]
Discovered by M. E. Brown
D. L. Rabinowitz
C. A. Trujillo
Discovery date 30 August 2005
Designations
MPC designation 2005 QU182
TNO (SDO)[2][3]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc 13642 days (37.35 yr)
Aphelion 184.19 AU (27.554 Tm) (Q)
Perihelion 36.827 AU (5.5092 Tm) (q)
110.51 AU (16.532 Tm) (a)
Eccentricity 0.66675 (e)
1161.74 yr (424325.7 d)
13.854° (M)
Inclination 14.032° (i)
78.395° (Ω)
223.69° (ω)
Earth MOID 35.8244 AU (5.35925 Tm)
Jupiter MOID 31.769 AU (4.7526 Tm)
Physical characteristics
Dimensions 416±73 km[5]
9.61 h (0.400 d)
9.61 hr[4]
0.328+0.160
−0.109
[5]
20.9[6]
3.80±0.32,[5] 3.5[4]

(303775) 2005 QU182, also written as (303775) 2005 QU182, is a trans-Neptunian object with a bright absolute magnitude of 3.8.[4] Mike Brown lists it as probably a dwarf planet.[7]

Distance

It came to perihelion in 1971[4] and is currently 50.5 AU from the Sun.[6] In April 2013, it moved beyond 50 AU from the Sun.

It has been observed 81 times over 10 oppositions with precovery images back to 1974.[4]

2005 QU182 takes over 1,200 years to orbit the Sun. Of the known and likely dwarf planets, only Sedna, 2012 VP113 and (445473) 2010 VZ98 have a longer orbit around the Sun.[8]

See also

References

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External links