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2014 ST373 (prov. designation: 2014 ST373) is a trans-Neptunian object and a detached object from the outermost region of the Solar System. With a perihelion of 50.2 AU, it belongs to the top 10 minor planets with the highest known perihelia of our Solar System. and is neither a scattered disc nor an extreme trans-Neptunian object. It measures approximately 370 kilometers (230 miles) in diameter and was first observed on 25 September 2014, by astronomers using the Dark Energy Camera (DECam) at Cerro Tololo Inter-American Observatory in Chile.

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  • 2014 ST373
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  • 2014 ST373 (prov. designation: 2014 ST373) is a trans-Neptunian object and a detached object from the outermost region of the Solar System. With a perihelion of 50.2 AU, it belongs to the top 10 minor planets with the highest known perihelia of our Solar System. and is neither a scattered disc nor an extreme trans-Neptunian object. It measures approximately 370 kilometers (230 miles) in diameter and was first observed on 25 September 2014, by astronomers using the Dark Energy Camera (DECam) at Cerro Tololo Inter-American Observatory in Chile.
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abs magnitude
align
  • left
aphelion
  • 158.86
arg peri
asc node
background
  • #C2E0FF
caption
  • is located in an virtually unpopulated region
  • is located in the "gap", a poorly understood region.
direction
  • vertical
discovered
discoverer
discovery ref
  •  
eccentricity
epoch
image
  • Extreme trans-Neptunian objects eccentricity vs perihelion.svg
  • Extreme transneptunian object eccentricity vs perihelion.png
inclination
mean anomaly
mean motion
  • / day
minorplanet
  • yes
mp category
observation arc
  • 6.84288E7
orbit ref
  •  
perihelion
  • 50.2
period
  • 3.37350744E10
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