About: 2015 KG163

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

2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States. With an observation arc of 2 years, it is known that it will come to perihelion around August 2022 at a velocity of 6.5 km/s with respect to the Sun.

Property Value
dbo:Planet/apoapsis
  • 1.97345023091319E11
  • 1.97469189324E11
dbo:Planet/orbitalPeriod
  • 6464925.0
  • 6470077.0
dbo:Planet/periapsis
  • 6.0576665782551E9
dbo:absoluteMagnitude
  • 8.265000 (xsd:double)
dbo:abstract
  • 2015 KG163 ist ein Planetoid, der am 24. Mai 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in mehr als 20000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,95, wobei diese 14° gegen die Ekliptik geneigt ist. (de)
  • 2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States. With an observation arc of 2 years, it is known that it will come to perihelion around August 2022 at a velocity of 6.5 km/s with respect to the Sun. It is one a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axes of 250 AU or more. Such objects can not reach such orbits without some perturbing object, which lead to the speculation of Planet Nine. Its argument of perihelion is similar to that of 2013 FT28. (en)
  • 2015 KG163 est un objet transneptunien du Système solaire ayant un périhélie à 40,5 UA et un demi-grand axe à plus de 800 UA. Un tel objet ne peut être sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf. Tout comme 2013 FT28, cet objet se trouverait du même côté du Système solaire que l'hypothétique planète qui le bloquerait dans une orbite stable. (fr)
dbo:albedo
  • 0.080000 (xsd:double)
dbo:apoapsis
  • 197345023091319.000000 (xsd:double)
  • 197469189324000.000000 (xsd:double)
dbo:discovered
  • 2015-05-24 (xsd:date)
dbo:discoverer
dbo:epoch
  • 4 September 2017 (JD2458000.5)
dbo:formerName
  • (en)
  • o5m52 (en)
dbo:orbitalPeriod
  • 558569520000.000000 (xsd:double)
  • 559014652800.000000 (xsd:double)
dbo:periapsis
  • 6057666578255.099609 (xsd:double)
dbo:thumbnail
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  • 54585442 (xsd:integer)
dbo:wikiPageLength
  • 6110 (xsd:nonNegativeInteger)
dbo:wikiPageRevisionID
  • 1102337671 (xsd:integer)
dbo:wikiPageWikiLink
dbp:absMagnitude
  • 8.265000 (xsd:double)
dbp:albedo
  • 0.080000 (xsd:double)
dbp:altNames
  • 352.0
dbp:aphelion
  • 1319.17
  • 1320.0
dbp:argPeri
  • 32.097000 (xsd:double)
dbp:ascNode
  • 219.100000 (xsd:double)
dbp:background
  • #C2E0FF (en)
dbp:caption
  • The orbit of and other extreme detached objects, along with the hypothetical Planet Nine's orbit on the right (en)
dbp:dimensions
  • 101.0
  • 104.0
dbp:discovered
  • 2015-05-24 (xsd:date)
dbp:discoverer
dbp:discoverySite
dbp:earliestPrecoveryDate
  • 2015-05-17 (xsd:date)
dbp:eccentricity
  • 0.940400 (xsd:double)
dbp:epoch
  • 2017-09-04 (xsd:date)
dbp:imageSize
  • 265 (xsd:integer)
dbp:inclination
  • 13.994000 (xsd:double)
dbp:meanAnomaly
  • 359.930000 (xsd:double)
dbp:meanMotion
  • / day (en)
dbp:minorplanet
  • yes (en)
dbp:mpCategory
  • TNOE-SDO (en)
  • sednoiddetached (en)
dbp:observationArc
  • 6.3746352E7
dbp:perihelion
  • 40.493
dbp:period
  • 5.5856952E11
  • 5.590113264E11
dbp:semimajor
  • 679.83
dbp:timePeriastron
  • 0001-08-12 (xsd:gMonthDay)
  • 5259600.0
dbp:uncertainty
  • 3 (xsd:integer)
dbp:wikiPageUsesTemplate
dcterms:subject
rdf:type
rdfs:comment
  • 2015 KG163 ist ein Planetoid, der am 24. Mai 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in mehr als 20000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,95, wobei diese 14° gegen die Ekliptik geneigt ist. (de)
  • 2015 KG163 est un objet transneptunien du Système solaire ayant un périhélie à 40,5 UA et un demi-grand axe à plus de 800 UA. Un tel objet ne peut être sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf. Tout comme 2013 FT28, cet objet se trouverait du même côté du Système solaire que l'hypothétique planète qui le bloquerait dans une orbite stable. (fr)
  • 2015 KG163, also known as o5m52, is a trans-Neptunian object from the outermost region of the Solar System, approximately 102 kilometers (63 miles) in diameter. It was first observed on 24 May 2015, by astronomers of the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatories, Hawaii, United States. With an observation arc of 2 years, it is known that it will come to perihelion around August 2022 at a velocity of 6.5 km/s with respect to the Sun. (en)
rdfs:label
  • 2015 KG163 (de)
  • 2015 KG163 (en)
  • 2015 KG163 (fr)
owl:sameAs
prov:wasDerivedFrom
foaf:depiction
foaf:isPrimaryTopicOf
foaf:name
  • (en)
is foaf:primaryTopic of
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