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2015 RY245, also known as o5s13, is a trans-Neptunian object from the scattered disc of the outermost reaches of the Solar System, approximately 78 kilometers in diameter. It was discovered on 9 September 2015, by 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 AUs or more, and semi-major axes of 200 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of planet nine.

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  • 2015 RY245 (en)
  • 2015 RY245 (fr)
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  • 2015 RY245, also known as o5s13, is a trans-Neptunian object from the scattered disc of the outermost reaches of the Solar System, approximately 78 kilometers in diameter. It was discovered on 9 September 2015, by 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 AUs or more, and semi-major axes of 200 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of planet nine. (en)
  • 2015 RY245 est un objet transneptunien de la ceinture de Kuiper avec un aphélie à plus de 400 UA. (fr)
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  • (en)
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  • o5s13 (en)
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  • #C2E0FF (en)
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  • / day (en)
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  • 2015 RY245, also known as o5s13, is a trans-Neptunian object from the scattered disc of the outermost reaches of the Solar System, approximately 78 kilometers in diameter. It was discovered on 9 September 2015, by 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 AUs or more, and semi-major axes of 200 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of planet nine. (en)
  • 2015 RY245 est un objet transneptunien de la ceinture de Kuiper avec un aphélie à plus de 400 UA. (fr)
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  • 4 September 2017 (JD2458000.5)
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  • (en)
  • o5s13 (en)
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