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2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist.

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  • 2015 KE172
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  • 2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist.
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abs magnitude
albedo
alt names
  • 372.0
arg peri
asc node
background
  • #C2E0FF
caption
  • Orbit of
discovered
discoverer
discovery ref
  •  
discovery site
earliest precovery date
eccentricity
epoch
inclination
mean anomaly
mean motion
  • / day
minorplanet
  • yes
mp category
  • distant 
  • TNO 1:9 
observation arc
  • 1.02877776E8
orbit ref
  •  
period
  • 4.84724736E10
uncertainty
has abstract
  • 2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist.
absolute magnitude
albedo
apoapsis (μ)
discovery date
epoch
  • 23 March 2018 (JD2458200.5)
former name
  • o5m72
orbital period (s)
periapsis (μ)
discoverer
prov:wasDerivedFrom
apoapsis (km)
  • 3.3227183061177E10
orbital period (μ)
  • 1122042.0
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