2014 FC72 (original) (raw)
2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 24 March 2014 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. With its perihelion distant from Neptune, it belongs to a small and poorly understood group of objects with moderate eccentricities. It is estimated to measure 500 kilometers (300 miles) in diameter, assuming a low albedo.
| Property | Value |
|---|---|
| dbo:Planet/apoapsis | 1.5045057856299E10 |
| dbo:Planet/orbitalPeriod | 485094.915 |
| dbo:Planet/periapsis | 7.7286747939741E9 |
| dbo:absoluteMagnitude | 4.700000 (xsd:double) |
| dbo:abstract | 2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 24 March 2014 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. With its perihelion distant from Neptune, it belongs to a small and poorly understood group of objects with moderate eccentricities. It is estimated to measure 500 kilometers (300 miles) in diameter, assuming a low albedo. (en) 2014 FC72 ist ein großes transneptunisches Objekt, das bahndynamisch als nahes oder erweitertes Scattered Disc Object (SDO oder DO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de) 2014 FC72 est un objet transneptunien de la famille des objets détachés et une planète naine potentielle, ayant un diamètre estimé d'environ 550 km. (fr) 2014 FC72, também escrito como 2014 FC72, é um objeto transnetuniano que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,5 e tem um diâmetro estimado em torno de 554 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt) |
| dbo:apoapsis | 15045057856299.000000 (xsd:double) |
| dbo:apparentMagnitude | 22.090000 (xsd:double) |
| dbo:discovered | 2014-03-24 (xsd:date) |
| dbo:discoverer | dbr:Pan-STARRS |
| dbo:epoch | 27 April 2019 (JD 2458600.5) |
| dbo:orbitalPeriod | 41912200656.000000 (xsd:double) |
| dbo:periapsis | 7728674793974.099609 (xsd:double) |
| dbo:thumbnail | wiki-commons:Special:FilePath/Extreme_transneptunia...entricity_vs_perihelion.png?width=300 |
| dbo:wikiPageExternalLink | http://www.johnstonsarchive.net/astro/tnoslist.html https://www.minorplanetcenter.net/iau/lists/t_centaurs.html |
| dbo:wikiPageID | 58706445 (xsd:integer) |
| dbo:wikiPageLength | 9684 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1062068602 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Planetary_migration dbr:Resonant_trans-Neptunian_object dbr:Degree_(angle) dbr:Detached_object dbr:Julian_day dbr:Perihelion dbr:Semi-major_axis dbr:Planets_beyond_Neptune dbr:Perihelia dbc:Astronomical_objects_discovered_in_2014 dbc:Discoveries_by_Pan-STARRS dbc:Possible_dwarf_planets dbc:Scattered_disc_and_detached_objects dbc:Minor_planet_object_articles_(unnumbered) dbr:Kozai_mechanism dbr:Kuiper_belt dbr:Trans-Neptunian_object dbr:Distant_minor_planet dbr:Julian_year_(astronomy) dbr:Ecliptic dbr:Pan-STARRS dbr:Formation_and_evolution_of_the_Solar_System dbr:Haleakala_Observatory dbr:Astronomical_unit dbr:Pluto dbr:Solar_System dbr:Scattered-disc_object dbr:Neptune dbr:Orbital_eccentricity dbr:Orbital_resonance dbr:Orbital_inclination dbr:Rogue_planet dbr:Scattered_disc_object dbr:Planetary_embryo dbr:File:Extreme_transneptunian_object_eccentricity_vs_perihelion.png |
| dbp:absMagnitude | 4.700000 (xsd:double) |
| dbp:aphelion | 100.57 |
| dbp:argPeri | 33.138000 (xsd:double) |
| dbp:ascNode | 178 (xsd:integer) |
| dbp:background | #C2E0FF (en) |
| dbp:discovered | 2014-03-24 (xsd:date) |
| dbp:discoverer | Pan-STARRS 1 (en) |
| dbp:discoverySite | dbr:Haleakala_Observatory |
| dbp:eccentricity | 0.321200 (xsd:double) |
| dbp:epoch | 2019-04-27 (xsd:date) |
| dbp:inclination | 29.859000 (xsd:double) |
| dbp:magnitude | 22.090000 (xsd:double) |
| dbp:meanAnomaly | 357.230000 (xsd:double) |
| dbp:meanMotion | / day (en) |
| dbp:minorplanet | yes (en) |
| dbp:mpCategory | dbr:Detached_object dbr:Trans-Neptunian_object dbr:Distant_minor_planet dbr:Scattered_disc_object (en) |
| dbp:observationArc | 5.33639016E8 |
| dbp:perihelion | 51.663 |
| dbp:period | 2.0956139856E10 |
| dbp:semimajor | 76.114 |
| dbp:timePeriastron | 0001-11-25 (xsd:gMonthDay) 604800.0 |
| dbp:uncertainty | 3 (xsd:integer) |
| dbp:wikiPageUsesTemplate | dbt:AstDys dbt:Convert dbt:Deg2DMS dbt:Infobox_planet dbt:JPL_small_body dbt:Mp dbt:Mpl dbt:Reflist dbt:Small dbt:Small_Solar_System_bodies dbt:Trans-Neptunian_objects dbt:Ubl dbt:Use_dmy_dates dbt:Val |
| dcterms:subject | dbc:Astronomical_objects_discovered_in_2014 dbc:Discoveries_by_Pan-STARRS dbc:Possible_dwarf_planets dbc:Scattered_disc_and_detached_objects dbc:Minor_planet_object_articles_(unnumbered) |
| rdf:type | owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody wikidata:Q634 dbo:Planet |
| rdfs:comment | 2014 FC72 is a trans-Neptunian object, classified as a scattered and detached object, located in the outermost region of the Solar System. It was first observed on 24 March 2014 by astronomers with the Pan-STARRS survey at Haleakala Observatory, Hawaii, United States. With its perihelion distant from Neptune, it belongs to a small and poorly understood group of objects with moderate eccentricities. It is estimated to measure 500 kilometers (300 miles) in diameter, assuming a low albedo. (en) 2014 FC72 ist ein großes transneptunisches Objekt, das bahndynamisch als nahes oder erweitertes Scattered Disc Object (SDO oder DO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de) 2014 FC72 est un objet transneptunien de la famille des objets détachés et une planète naine potentielle, ayant un diamètre estimé d'environ 550 km. (fr) 2014 FC72, também escrito como 2014 FC72, é um objeto transnetuniano que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,5 e tem um diâmetro estimado em torno de 554 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt) |
| rdfs:label | 2014 FC72 (de) 2014 FC72 (en) 2014 FC72 (fr) 2014 FC72 (pt) |
| owl:sameAs | wikidata:2014 FC72 dbpedia-de:2014 FC72 dbpedia-fr:2014 FC72 dbpedia-pt:2014 FC72 dbpedia-vi:2014 FC72 https://global.dbpedia.org/id/2fwSU |
| prov:wasDerivedFrom | wikipedia-en:2014_FC72?oldid=1062068602&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/Extreme_transneptunian_object_eccentricity_vs_perihelion.png |
| foaf:isPrimaryTopicOf | wikipedia-en:2014_FC72 |
| foaf:name | (en) |
| is foaf:primaryTopic of | wikipedia-en:2014_FC72 |
