2013 UH15

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2013 UH15
Discovery
Perihelion
35.018 AU
170.20 AU
Eccentricity0.7943
2221 yr (811,042 d)
353.91°
0° 0m 1.44s / day
Inclination26.090°
176.55°
282.97°
Neptune MOID12.9 AU
Physical characteristics
Mean diameter
128 km (est.)[3]
130 km (est.)[4]
0.08 (assumed)[4]
0.09 (assumed)[3]
7.7[1][2]

2013 UH15 is an extreme

extended scattered disc object (ESDO) is on a highly eccentric orbit and belongs to the extreme trans-Neptunian objects
.

Orbit and classification

2013 UH15 orbits the Sun at a distance of 35.0–305 

It belongs to a small group of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more.[6] These extreme trans-Neptunian objects (ETNOs) can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine.

Numbering and naming

As of 2018, this

numbered nor named by the Minor Planet Center. The official discoverers will be defined when the object is numbered.[1]

Physical characteristics

According to the Johnston's archive and to American astronomer

rotation period, pole and shape remain unknown.[2][7]

See also

References

  1. ^ a b c d e f g "2013 UH15". Minor Planet Center. Retrieved 26 October 2018.
  2. ^ a b c d e "JPL Small-Body Database Browser: (2013 UH15)" (2015-10-16 last obs.). Jet Propulsion Laboratory. Retrieved 26 October 2018.
  3. ^ a b c d "List of Known Trans-Neptunian Objects". Johnston's Archive. 7 October 2018. Retrieved 25 October 2018.
  4. ^ a b c d Brown, Michael E. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 25 October 2018.
  5. ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 25 October 2018.
  6. ^ "Database Query: objects q>30, a>150". Minor Planet Center. Retrieved 25 October 2018.
  7. ^ "LCDB Data for (2013+UH15)". Asteroid Lightcurve Database (LCDB). Retrieved 26 October 2018.

External links