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2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 24 March 2014 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. With its perihelion distant from Neptune, it belongs to a small and poorly understood group of objects with moderate eccentricities. It is estimated to measure 500 kilometers (300 miles) in diameter, assuming a low albedo.

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  • 2014 FC72 (de)
  • 2014 FC72 (en)
  • 2014 FC72 (fr)
  • 2014 FC72 (pt)
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  • 2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 24 March 2014 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. With its perihelion distant from Neptune, it belongs to a small and poorly understood group of objects with moderate eccentricities. It is estimated to measure 500 kilometers (300 miles) in diameter, assuming a low albedo. (en)
  • 2014 FC72 ist ein großes transneptunisches Objekt, das bahndynamisch als nahes oder erweitertes Scattered Disc Object (SDO oder DO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de)
  • 2014 FC72 est un objet transneptunien de la famille des objets détachés et une planète naine potentielle, ayant un diamètre estimé d'environ 550 km. (fr)
  • 2014 FC72, também escrito como 2014 FC72, é um objeto transnetuniano que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,5 e tem um diâmetro estimado em torno de 554 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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  • (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Extreme_transneptunian_object_eccentricity_vs_perihelion.png
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abs magnitude
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  • #C2E0FF (en)
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  • Pan-STARRS 1 (en)
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  • / day (en)
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  • yes (en)
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