(90568) 2004 GV9

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(90568) 2004 GV9
Discovery[1]
Discovered by NEAT
Discovery date 13 April 2004
Designations
MPC designation (90568) 2004 GV9
Cubewano (MPC)[2]
Extended (DES)[3]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc 22031 days (60.32 yr)
Aphelion 45.618 AU (6.8244 Tm)
Perihelion 38.7281 AU (5.79364 Tm)
42.173 AU (6.3090 Tm)
Eccentricity 0.081681
273.88 yr (100034 d)
34.6030°
Inclination 21.9718°
250.6142°
293.200°
Earth MOID 37.7917 AU (5.65356 Tm)
Jupiter MOID 33.6786 AU (5.03825 Tm)
Physical characteristics
Dimensions 680±34[5]
5.86 h (0.244 d)
5.86 h[4]
0.077+0.0084
−0.0077
[5]
B−V=0.95,
V−R=0.52[6]
B0−V0=0.843[7]
19.9[8]
4.25±0.04,[5] 4.0[4]

(90568) 2004 GV9 (also written (90568) 2004 GV9) is a trans-Neptunian object that was discovered on April 13, 2004 by NEAT.[1] It is currently listed as a cubewano by the Minor Planet Center.[2]

It is very likely a dwarf planet.[9] A diameter of 680±34 km has been calculated from combined observations of the Herschel and Spitzer space telescopes.[5] Light-curve-amplitude analysis shows only small deviations, suggesting that (90568) 2004 GV9 could be a spheroid with small albedo spots and hence a dwarf planet.[10]

It has been observed forty-seven times, with precovery images back to 1954.[4]

References

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  10. Tancredi, G., & Favre, S. (2008) Which are the dwarfs in the Solar System?. Depto. Astronomía, Fac. Ciencias, Montevideo, Uruguay; Observatorio Astronómico Los Molinos, MEC, Uruguay. Retrieved 10-08-2011

External links


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