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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. The possible dwarf planet measures approximately 500 kilometers (310 miles) in diameter.

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  • 2014 FC72
  • 2014 FC72
  • 2014 FC72
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  • 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.
  • 2014 FC72 est un objet transneptunien de la famille des objets épars et une planète naine potentielle, ayant un diamètre estimé d'environ 550 km.
  • 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. The possible dwarf planet measures approximately 500 kilometers (310 miles) in diameter.
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abs magnitude
aphelion
  • 100.57
arg peri
asc node
background
  • #C2E0FF
discovered
discoverer
  • Pan-STARRS 1
discovery ref
  •  
discovery site
eccentricity
epoch
inclination
magnitude
mean anomaly
mean motion
  • / day
minorplanet
  • yes
mp category
  • SDO 
  • TNO 
  • distant 
  • detached 
observation arc
  • 5.33639016E8
orbit ref
  •  
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