About: (523719) 2014 LM28

An Entity of Type: planet, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org:8891

(523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune.

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dbo:Planet/apoapsis	8.0616796541523E10
dbo:Planet/orbitalPeriod	3382982.0125
dbo:Planet/periapsis	2.5089058895097E9
dbo:absoluteMagnitude	9.900000 (xsd:double)
dbo:abstract	(523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune. (en) (523719) 2014 LM28 est un objet transneptunien ayant une orbite fortement inclinée et très excentrique l'emmenant, au périhélie, plus près du Soleil qu'Uranus et, à l'aphélie, 17 fois plus loin du Soleil que Neptune. (fr)
dbo:apoapsis	80616796541523.000000 (xsd:double)
dbo:discovered	2013-05-16 (xsd:date)
dbo:discoverer	dbr:Pan-STARRS
dbo:epoch	27 April 2019 (JD2458600.5)
dbo:orbitalPeriod	292289645880.000000 (xsd:double)
dbo:periapsis	2508905889509.700195 (xsd:double)
dbo:wikiPageExternalLink	https://minorplanetcenter.net/iau/lists/Centaurs.html https://www.minorplanetcenter.net/iau/lists/NumberedMPs520001.html
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dbp:absMagnitude	9.900000 (xsd:double)
dbp:aphelion	538.89
dbp:argPeri	38.364000 (xsd:double)
dbp:ascNode	246.180000 (xsd:double)
dbp:background	#C2E0FF (en)
dbp:discovered	2013-05-16 (xsd:date)
dbp:discoverer	Pan-STARRS 1 (en)
dbp:discoverySite	dbr:Haleakala_Observatory
dbp:eccentricity	0.939600 (xsd:double)
dbp:epoch	2019-04-27 (xsd:date)
dbp:inclination	84.739000 (xsd:double)
dbp:meanAnomaly	0.113300 (xsd:double)
dbp:meanDiameter	46.0
dbp:meanMotion	/ day (en)
dbp:minorplanet	yes (en)
dbp:mpCategory	dbr:Centaur_(minor_planet) TNOdistant (en)
dbp:observationArc	1.27492704E8
dbp:perihelion	16.771
dbp:period	1.4614482348E11
dbp:semimajor	277.83
dbp:uncertainty	1 (xsd:integer)
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dcterms:subject	dbc:Astronomical_objects_discovered_in_2013 dbc:Centaurs_(small_Solar_System_bodies) dbc:Discoveries_by_Pan-STARRS dbc:Trans-Neptunian_objects
rdf:type	owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody wikidata:Q634 dbo:Planet
rdfs:comment	(523719) 2014 LM28, provisional designation 2014 LM28, is a trans-Neptunian object and centaur, approximately 46 kilometers (29 miles) in diameter. It was discovered on 16 May 2013, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States. The object's orbit is highly inclined and very eccentric, with a perihelion closer to the Sun than Uranus and at an aphelion 17 times farther from the Sun than Neptune. (en) (523719) 2014 LM28 est un objet transneptunien ayant une orbite fortement inclinée et très excentrique l'emmenant, au périhélie, plus près du Soleil qu'Uranus et, à l'aphélie, 17 fois plus loin du Soleil que Neptune. (fr)
rdfs:label	(523719) 2014 LM28 (en) (523719) 2014 LM28 (fr)
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