About: 2015 GT50

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http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2F2015_GT50

2015 GT50, previously known as o5p060, is a trans-Neptunian object orbiting in the Kuiper belt of the outermost Solar System. It was first observed by the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea on 13 April 2015.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body Planet planet
rdfs:label	2015 GT50 (de) 2015 GT50 (en) 2015 GT50 (fr)
rdfs:comment	2015 GT50 ist ein Planetoid, der am 13. April 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in über 6000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,88, wobei diese 8,78° gegen die Ekliptik geneigt ist. (de) 2015 GT50, previously known as o5p060, is a trans-Neptunian object orbiting in the Kuiper belt of the outermost Solar System. It was first observed by the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea on 13 April 2015. (en) 2015 GT50 est un objet transneptunien du système solaire ayant un périhélie à 38,5 UA et un demi-grand axe à plus de 300 UA. Selon la plupart des théories, un tel objet ne peut se trouver sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf. (fr)
foaf:depiction
dcterms:subject	Astronomical objects discovered in 2015 Extreme trans-Neptunian objects Possible dwarf planets Scattered disc and detached objects Minor planet object articles (unnumbered)
Wikipage page ID	54580802 (xsd:integer)
Wikipage revision ID	1049546551 (xsd:integer)
Link from a Wikipage to another Wikipage	Detached object Astronomical objects discovered in 2015 Extreme trans-Neptunian objects Possible dwarf planets Scattered disc and detached objects Mauna Kea Minor planet object articles (unnumbered) Kuiper belt Trans-Neptunian object Astronomical unit Planet Nine Solar System Konstantin Batygin Canada–France–Hawaii Telescope Mauna Kea Observatories Outer Solar System Origins Survey
Link from a Wikipage to an external page	http://www.minorplanetcenter.net/mpec/K17/K17M22.html https://arxiv.org/abs/1706.05348 http://www.ossos-survey.org/
sameAs	2015 GT50 2015 GT50 2015 GT50 2015 GT50 2015 GT50
dbp:wikiPageUsesTemplate	dbt:2017_in_space dbt:CentaurTNO-stub dbt:Clear dbt:Infobox_planet dbt:JPL_small_body dbt:Mp dbt:Reflist dbt:Short_description dbt:Small_Solar_System_bodies dbt:Use_dmy_dates
thumbnail	wiki-commons:Special:FilePath/Planet_nine-etnos_now-new2.png?width=300
alt names	o5p060 (en)
aphelion	631.89 (astronomicalUnit)
arg peri	129.236000 (xsd:double)
asc node	46.100000 (xsd:double)
background	#C2E0FF (en)
caption	The orbits of and other detached objects, along with the hypothetical Planet Nine's orbit (en)
discovered	2015-04-13 (xsd:date)
discoverer	Outer Solar System Origins Survey
discovery site	Mauna Kea Observatories
earliest precovery date	2015-02-20 (xsd:date)
eccentricity	0.885000 (xsd:double)
epoch	JDT 2458000.5 (en)
image size	270 (xsd:integer)
inclination	8.779000 (xsd:double)
magnitude	8.500000 (xsd:double)
minorplanet	yes (en)
mp category	Detached object
observation arc	7.11936E7 (second)
perihelion	38.45 (astronomicalUnit)
period	1.93763664E11 (second)
semimajor	335.169 (astronomicalUnit)
has abstract	2015 GT50 ist ein Planetoid, der am 13. April 2015 am Mauna Kea entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in über 6000 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,88, wobei diese 8,78° gegen die Ekliptik geneigt ist. (de) 2015 GT50, previously known as o5p060, is a trans-Neptunian object orbiting in the Kuiper belt of the outermost Solar System. It was first observed by the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea on 13 April 2015. (en) 2015 GT50 est un objet transneptunien du système solaire ayant un périhélie à 38,5 UA et un demi-grand axe à plus de 300 UA. Selon la plupart des théories, un tel objet ne peut se trouver sur une telle orbite qu'avec l'aide d'un perturbateur, d'où l'hypothèse de la Planète Neuf. (fr)
prov:wasDerivedFrom	wikipedia-en:2015_GT50?oldid=1049546551&ns=0
apoapsis (km)	9.4529398516623E10 (kilometre)
orbital period (μ)	2242635.0 (day)
periapsis (km)	5.752038128415E9 (kilometre)
page length (characters) of wiki page	5473 (xsd:nonNegativeInteger)
apoapsis (μ)	94529398516623.000000 (xsd:double)
apparent magnitude	8.500000 (xsd:double)
discovery date	2015-04-13 (xsd:date)
epoch	JDT 2458000.5
former name	o5p060 (en)
orbital period (s)	193763664000.000000 (xsd:double)
periapsis (μ)	5752038128415.000000 (xsd:double)
discoverer	Outer Solar System Origins Survey
foaf:isPrimaryTopicOf	wikipedia-en:2015_GT50
is foaf:primaryTopic of	wikipedia-en:2015_GT50

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