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2013 AZ60 is a small Solar System body (extended centaur) from the scattered disk or inner Oort cloud. 2013 AZ60 has the 8th-largest semi-major axis of a minor planet not detected outgassing like a comet (2013 BL76, 2005 VX3 and 2012 DR30 have a larger semi-major axis). After leaving the planetary region of the Solar System, 2013 AZ60 will have a barycentric aphelion of 827 AU with an orbital period of 8500 years. In a 10 million year integration of the orbit, one of the 3-sigma clones is ejected from the Solar System.

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  • 2013 AZ60 (en)
  • 2013 AZ60 (fr)
  • 2013 AZ60 (pt)
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  • 2013 AZ60 est un objet transneptunien de la ceinture de Kuiper, ayant un aphélie de près de 1 000 UA, mais dont l'orbite s'approche de Saturne. (fr)
  • 2013 AZ60 is a small Solar System body (extended centaur) from the scattered disk or inner Oort cloud. 2013 AZ60 has the 8th-largest semi-major axis of a minor planet not detected outgassing like a comet (2013 BL76, 2005 VX3 and 2012 DR30 have a larger semi-major axis). After leaving the planetary region of the Solar System, 2013 AZ60 will have a barycentric aphelion of 827 AU with an orbital period of 8500 years. In a 10 million year integration of the orbit, one of the 3-sigma clones is ejected from the Solar System. (en)
  • 2013 AZ60, também escrito como 2013 AZ60, é um pequeno corpo celeste do Sistema Solar (um centauro estendido) localizado a partir do Disco disperso ou na Nuvem de Oort. 2013 AZ60 tem o quarto mais distante semieixo maior de um corpo menor, não foi detectado desgaseificação como um cometa (ambos 2013 BL76, 2005 VX3 e 2012 DR30 tem um semieixo maior superior). Ele veio a oposição no dia 30 de janeiro de 2014. (pt)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Distant_object_orbits_+_Planet_Nine.png
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  • #C2E0FF (en)
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  • yes (en)
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