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2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States.

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  • 2015 KG163
  • 2015 KG163
  • 2015 KG163
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  • 2015 KG163 ist ein Planetoid, der am 24. Mai 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in fast 24000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,95, wobei diese 14,00° gegen die Ekliptik geneigt ist.
  • 2015 KG163 est un objet transneptunien du Système solaire ayant un périhélie à 40,5 UA et un demi-grand axe à plus de 800 UA. Un tel objet ne peut être sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf.
  • 2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States.
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abs magnitude
albedo
alt names
  • 352.0
aphelion
  • 1320.0
  • 1581.43
arg peri
asc node
background
  • #C2E0FF
caption
  • The orbit of and other extreme detached objects, along with the hypothetical Planet Nine's orbit on the right
dimensions
  • 101.0
  • 104.0
discovered
discoverer
discovery ref
  •  
discovery site
earliest precovery date
  • --05-17
eccentricity
epoch
image size
inclination
mean anomaly
mean motion
  • / day
minorplanet
  • yes
mp category
  • TNO E-SDO
  • sednoid detached
observation arc
  • 6.3746352E7
orbit ref
  •  
perihelion
  • 40.505
period
  • 5.5856952E11
  • 7.287912144E11
semimajor
  • 810.97
uncertainty
has abstract
  • 2015 KG163 ist ein Planetoid, der am 24. Mai 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in fast 24000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,95, wobei diese 14,00° gegen die Ekliptik geneigt ist.
  • 2015 KG163 est un objet transneptunien du Système solaire ayant un périhélie à 40,5 UA et un demi-grand axe à plus de 800 UA. Un tel objet ne peut être sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf.
  • 2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States. It is one a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 250 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine. Its argument of perihelion is similar to that of 2013 FT28.
absolute magnitude
albedo
apoapsis (μ)
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