Astronomy:2002 GB32

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2002 GB32
Planet nine 15 etno2 2017.png
2002 GB32 is seen lower right in blue with hypothetical Planet Nine in green
Discovery[2]
Discovered byM. W. Buie[1]
Discovery siteCerro Tololo Obs.
Discovery date7 April 2002
Designations
2002 GB32
Minor planet categoryTNO[3] · SDO[1][4]
distant[2] · detached
Orbital characteristics[3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 3
Observation arc12.96 yr (4,733 days)
|{{{apsis}}}|helion}}402.66 AU
|{{{apsis}}}|helion}}35.347 AU
219.01 AU
Eccentricity0.8386
Orbital period3241.10 yr (1,183,810 days)
Mean anomaly0.3780°
Mean motion0° 0m 1.08s / day
Inclination14.176°
Longitude of ascending node176.99°
37.158°
Physical characteristics
Dimensions122 km (calculated)[4]
Geometric albedo0.09 (assumed)[4]
Absolute magnitude (H)7.8[3]


2002 GB32, is a trans-Neptunian object from the scattered disc in the outermost region of the Solar System, approximately 122 kilometers in diameter.[3][4] It was first observed on 7 April 2002, by American astronomer Marc Buie at Cerro Tololo Observatory in Chile.[2][1]

Description

2002 GB32 belongs to a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axis of 200 AU or more.[5] Such objects can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine.

This minor planet orbits the Sun at a distance of 35.3–402.7 AU once every 3,241 years and 1 month (1,183,810 days). Its orbit has an eccentricity of 0.84 and an inclination of 14° with respect to the ecliptic.[3]

Based on an absolute magnitude of 7.8 and an assumed albedo of 0.09, the Johnston's Archive calculated a mean-diameter of 122 kilometers.[4]

See also

References

External links