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(307463) 2002 VU130, prov. designation: 2002 VU130, is a trans-Neptunian object, located in the circumstellar disc of the Kuiper belt in the outermost region of the Solar System. The resonant trans-Neptunian object belongs to the population of plutinos and measures approximately 253 kilometers (160 miles) in diameter. It was discovered on 7 November 2002, by American astronomer Marc Buie at the Kitt Peak Observatory near Tucson, Arizona. The object has not been named yet.

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  • (307463) 2002 VU130 (ar)
  • (307463) 2002 VU130 (en)
  • (307463) 2002 VU130 (fr)
  • (307463) 2002 VU130 (in)
  • (307463) 2002 VU130 (pt)
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  • 2002 في يو 130 (ويعرف أيضًا باسم (307463) 2002 في يو 130 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2002 VU130)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 307463 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة مارك ويليام بوي في 7 نوفمبر 2002. (ar)
  • (307463) 2002 VU130, prov. designation: 2002 VU130, is a trans-Neptunian object, located in the circumstellar disc of the Kuiper belt in the outermost region of the Solar System. The resonant trans-Neptunian object belongs to the population of plutinos and measures approximately 253 kilometers (160 miles) in diameter. It was discovered on 7 November 2002, by American astronomer Marc Buie at the Kitt Peak Observatory near Tucson, Arizona. The object has not been named yet. (en)
  • (307463) 2002 VU130 est un objet transneptunien de la famille des plutinos. (fr)
  • (307463) 2002 VU130 adalah sebuah objek trans-Neptunus. Seperti objek trans-Neptunus pada umumnya, benda ini mengorbit Matahari dari jarak yang lebih jauh dari planet Neptunus. Eksentrisitas orbit objek ini tercatat sebesar 0.209, sementara magnitudo mutlaknya adalah 6.1. (in)
  • (307463) 2002 VU130, também escrito como (307463) 2002 VU130, é um objeto transnetuniano (TNO) que está localizado no cinturão de Kuiper, uma região do Sistema Solar. Ele é classificado como um plutino, pois, o mesmo está em uma ressonância orbital de 2:3 com o planeta Netuno). Ele possui uma magnitude absoluta (H) de 6,1 e, tem um diâmetro estimado com cerca de 253 km, por isso é pouco provável que possa ser classificado como um planeta anão, devido ao seu tamanho relativamente pequeno. (pt)
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