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2015 RX245 is an extreme trans-Neptunian object, detached, on a highly eccentric orbit in the outermost region of the Solar System. It measures approximately 250 kilometers (160 miles) in diameter and is "possibly" a dwarf planet. It was first observed on 8 September 2015, by astronomers with Outer Solar System Origins Survey using the 3.6-meter Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, in the United States.

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  • 2015 RX245 (de)
  • 2015 RX245 (en)
  • 2015 RX245 (fr)
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  • 2015 RX245 is an extreme trans-Neptunian object, detached, on a highly eccentric orbit in the outermost region of the Solar System. It measures approximately 250 kilometers (160 miles) in diameter and is "possibly" a dwarf planet. It was first observed on 8 September 2015, by astronomers with Outer Solar System Origins Survey using the 3.6-meter Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, in the United States. (en)
  • 2015 RX245 ist ein Planetoid, der am 8. September 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in über 8200 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,89, wobei diese 12,17° gegen die Ekliptik geneigt ist. (de)
  • 2015 RX245 est un objet transneptunien du système solaire ayant un périhélie à 45 UA et un demi-grand axe à plus de 400 UA. Un tel objet ne peut se trouver sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf. . (fr)
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  • (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Planet_nine-etnos_now-new2.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Planet_nine-etnos_now-close-new.png
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  • o5t52 (en)
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  • #C2E0FF (en)
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  • Orbital diagram of and other objects along with hypothetical Planet Nine (en)
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