About: 2015 KE172

An Entity of Type: planet, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

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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dbo:Planet/periapsis	6.6028012190859E9
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dbo: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. (en)
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dbo:discovered	2015-05-21 (xsd:date)
dbo:discoverer	dbr:Outer_Solar_System_Origins_Survey
dbo:epoch	23 March 2018 (JD2458200.5)
dbo:formerName	(en) o5m72 (en)
dbo:orbitalPeriod	96944428800.000000 (xsd:double)
dbo:periapsis	6602801219085.900391 (xsd:double)
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dbo:wikiPageExternalLink	http://web.gps.caltech.edu/~mbrown/dps.html http://www.johnstonsarchive.net/astro/tnoslist.html https://minorplanetcenter.net/iau/lists/TNOs.html https://www.minorplanetcenter.net/iau/lists/t_centaurs.html
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dbp:albedo	0.090000 (xsd:double)
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dbp:argPeri	15.428000 (xsd:double)
dbp:ascNode	227.550000 (xsd:double)
dbp:background	#C2E0FF (en)
dbp:caption	Orbit of (en)
dbp:discovered	2015-05-21 (xsd:date)
dbp:discoverer	dbr:Outer_Solar_System_Origins_Survey
dbp:discoverySite	dbr:Mauna_Kea_Observatories
dbp:earliestPrecoveryDate	2014-05-30 (xsd:date)
dbp:eccentricity	0.668500 (xsd:double)
dbp:epoch	2018-03-23 (xsd:date)
dbp:inclination	38.280000 (xsd:double)
dbp:meanAnomaly	0.106100 (xsd:double)
dbp:meanMotion	/ day (en)
dbp:minorplanet	yes (en)
dbp:mpCategory	dbr:Distant_minor_planet TNO1:9 (en)
dbp:observationArc	1.02877776E8
dbp:period	4.84724736E10
dbp:uncertainty	4 (xsd:integer)
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rdfs:comment	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. (en)
rdfs:label	2015 KE172 (en) 2015 KE172 (fr)
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