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(523622) 2007 TG422, provisional designation 2007 TG422, is a trans-Neptunian object on a highly eccentric orbit in the scattered disc region at the edge of Solar System. Approximately 260 kilometers (160 miles) in diameter, it was discovered on 3 October 2007 by astronomers Andrew Becker, Andrew Puckett and Jeremy Kubica during the Sloan Digital Sky Survey at Apache Point Observatory in New Mexico, United States. According to American astronomer Michael Brown, the bluish object is "possibly" a dwarf planet. It belongs to a group of objects studied in 2014, which lead to the proposition of the hypothetical Planet Nine.

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  • (523622) 2007 TG422 (de)
  • (523622) 2007 TG422 (el)
  • (523622) 2007 TG422 (en)
  • (523622) 2007 TG422 (es)
  • (523622) 2007 TG422 (fr)
  • (523622) 2007 TG422 (pt)
  • (523622) 2007 TG422 (ru)
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  • To 2007 TG422 είναι ένα αντικείμενο του εσωτερικού νέφους του Όορτ με διάμετρο μεταξύ 265 και 204 χιλιόμετρα. Η τροχιά του 2007 TG422 είναι πολύ ελλειπτική και μοιάζει με αυτή της Σέντνα, καθώς το αφήλιό τους βρίσκεται περίπου στην ίδια απόσταση (περίπου 150 δισεκατομμύρια χιλιόμετρα) από τον Ήλιο. Το αφήλιό του βρίσκεται 1000 ΑΜ από τον Ήλιο, έχοντας ένα από τα πιο απομακρυσμένα αφήλια. (el)
  • (523622) 2007 TG422, provisional designation 2007 TG422, is a trans-Neptunian object on a highly eccentric orbit in the scattered disc region at the edge of Solar System. Approximately 260 kilometers (160 miles) in diameter, it was discovered on 3 October 2007 by astronomers Andrew Becker, Andrew Puckett and Jeremy Kubica during the Sloan Digital Sky Survey at Apache Point Observatory in New Mexico, United States. According to American astronomer Michael Brown, the bluish object is "possibly" a dwarf planet. It belongs to a group of objects studied in 2014, which lead to the proposition of the hypothetical Planet Nine. (en)
  • (523622) 2007 TG422 ist ein großes transneptunisches Objekt, das bahndynamisch als «Extreme trans-Neptunian object» (ETNO) und als nahes oder erweitertes Scattered Disc Object (SDO oder DO) eingestuft wird. Aufgrund seiner Größe gehört der Asteroid zu den Zwergplanetenkandidaten. (de)
  • (523622) 2007 TG422, designación provisional 2007 TG422 es un objeto transneptuniano en una órbita altamente excéntrica en el disco disperso ubicado en la región más alejada del sistema solar, con un diámetro aproximado 260 kilómetros (161,6 mi). Fue descubierto el 3 de octubre de 2007 por los astrónomos Andrew Becker, Andrew Puckett, y Jeremy Kubica durante el proyecto de investigación Sloan Digital Sky Survey en el Observatorio de Apache Point en Nuevo México, Estados Unidos.​ De acuerdo al astrónomo estadounidense Michael E. Brown, el objeto transneptuniano es posiblemente un planeta enano.​ Pertenece al grupo de objetos estudiados en 2014, que llevaron a la proposición del hipotético Planeta Nueve.​ (es)
  • (523622) 2007 TG422 est un objet transneptunien de magnitude absolue 6,2. Son diamètre est estimé de 150 km à 343 km, suivant son albédo; celui-ci est probablement faible puisqu'il a le spectre bleu des objets transneptuniens. Il pourrait être qualifié comme candidat au statut de planète naine. (fr)
  • 2007 TG422 — объект рассеянного диска, открытый 3 октября 2007 года в обсерватории Апачи-Пойнт. Перигелийное расстояние составляет 35,6 а.е., вследствие чего объект попадает в область гравитационного влияния Нептуна. Расстояние до Солнца в афелии совпадает с расстоянием в афелии от Солнца до Седны. (ru)
  • (523622) 2007 TG422, também escrito como (523622) 2007 TG422, é um corpo menor que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 6,2 e tem um diâmetro estimado de cerca de 253 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt)
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  • (523622) (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Planet_nine-etnos_now.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Distant_object_orbits_+_Planet_Nine.png
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