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2013 FQ28 is a trans-Neptunian object, both considered a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 17 March 2013, by a team of astronomers at the Cerro Tololo Inter-American Observatory in Chile. It orbits the Sun in a moderate inclined, moderate-eccentricity orbit. The weak dwarf planet candidate measures approximately 260 kilometers (160 miles) in diameter.

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  • 2013 FQ28 (de)
  • 2013 FQ28 (en)
  • 2013 FQ28 (fr)
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  • 2013 FQ28 ist ein Planetoid, der am 17. März 2013 am Cerro Tololo Observatory, La Serena, entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in 503 Jahren um die Sonne, so dass er sich in einer 3:1-Bahnresonanz mit dem Neptun befindet. Die Bahnexzentrizität seiner Bahn beträgt 0,27, wobei diese 25,70° gegen die Ekliptik geneigt ist. (de)
  • 2013 FQ28 is a trans-Neptunian object, both considered a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 17 March 2013, by a team of astronomers at the Cerro Tololo Inter-American Observatory in Chile. It orbits the Sun in a moderate inclined, moderate-eccentricity orbit. The weak dwarf planet candidate measures approximately 260 kilometers (160 miles) in diameter. (en)
  • 2013 FQ28 est un transneptunien de magnitude absolue 5,9. Son diamètre est estimé à 290 km, ce qui pourrait le qualifier comme un candidat au statut de planète naine. (fr)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Extreme_transneptunian_object_eccentricity_vs_perihelion.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/2013_FQ28-orbit.png
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  • #C2E0FF (en)
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