2014 FZ71 (original) (raw)
2014 FZ71 is a trans-Neptunian object, a scattered disc 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 a team led by American astronomer Scott Sheppard at the Cerro Tololo Inter-American Observatory in Chile. With its perihelion of almost 56 AU, it belongs to a small and poorly understood group of very distant objects with moderate eccentricities. The object is not a dwarf planet candidate as it only measures approximately 150 kilometers (93 miles) in diameter.
| Property | Value |
|---|---|
| dbo:Planet/apoapsis | 1.43301296322237E10 |
| dbo:Planet/orbitalPeriod | 482283.7025 |
| dbo:Planet/periapsis | 8.3548914807243E9 |
| dbo:absoluteMagnitude | 6.900000 (xsd:double) |
| dbo:abstract | 2014 FZ71 is a trans-Neptunian object, a scattered disc 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 a team led by American astronomer Scott Sheppard at the Cerro Tololo Inter-American Observatory in Chile. With its perihelion of almost 56 AU, it belongs to a small and poorly understood group of very distant objects with moderate eccentricities. The object is not a dwarf planet candidate as it only measures approximately 150 kilometers (93 miles) in diameter. (en) 2014 FZ71 ist ein Planetoid, der am 24. März 2014 am Cerro Tololo Observatory, La Serena entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in 668 Jahren um die Sonne, so dass er sich in einer 4:1 Bahnresonanz mit dem Neptun befindet. Die Bahnexzentrizität seiner Bahn beträgt 0,27, wobei diese 25,44° gegen die Ekliptik geneigt ist. (de) est un transneptunien de magnitude absolue 6,9 en résonance 4:1 avec Neptune. L'objet compte parmi les objets connus ayant l'un des aphélies les plus élevés. (fr) |
| dbo:apoapsis | 14330129632223.699219 (xsd:double) |
| dbo:apparentMagnitude | 24.610000 (xsd:double) |
| dbo:discovered | 2014-03-24 (xsd:date) |
| dbo:discoverer | dbr:Cerro_Tololo_Inter-American_Observatory |
| dbo:epoch | 27 April 2019 (JD 2458600.5) |
| dbo:orbitalPeriod | 41669311896.000000 (xsd:double) |
| dbo:periapsis | 8354891480724.299805 (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 | 58706425 (xsd:integer) |
| dbo:wikiPageLength | 10136 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1062067537 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Carnegie_Institution_for_Science dbr:Scott_Sheppard dbr:Planetary_migration dbr:Resonant_trans-Neptunian_object dbr:Degree_(angle) dbr:Detached_object dbr:Julian_day dbr:Perihelion dbr:Semi-major_axis dbr:List_of_possible_dwarf_planets dbr:Planets_beyond_Neptune dbr:Subaru_Telescope dbc:Astronomical_objects_discovered_in_2014 dbc:Discoveries_by_CTIO 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:Formation_and_evolution_of_the_Solar_System dbr:Astronomical_unit dbr:Pluto dbr:Solar_System dbr:Scattered-disc_object dbr:Neptune dbr:Orbital_eccentricity dbr:Orbital_resonance dbr:Cerro_Tololo_Inter-American_Observatory dbr:Orbital_inclination dbr:Rogue_planet dbr:Scattered_disc dbr:Scattered_disc_object dbr:Kuiper_Cliff dbr:Planetary_embryo dbr:File:Extreme_transneptunian_object_eccentricity_vs_perihelion.png |
| dbp:absMagnitude | 6.900000 (xsd:double) |
| dbp:aphelion | 95.791 |
| dbp:argPeri | 244.940000 (xsd:double) |
| dbp:ascNode | 306.010000 (xsd:double) |
| dbp:background | #C2E0FF (en) |
| dbp:discovered | 2014-03-24 (xsd:date) |
| dbp:discoverer | dbr:Cerro_Tololo_Inter-American_Observatory |
| dbp:discoverySite | dbr:Cerro_Tololo_Inter-American_Observatory |
| dbp:eccentricity | 0.263400 (xsd:double) |
| dbp:epoch | 2019-04-27 (xsd:date) |
| dbp:inclination | 25.506000 (xsd:double) |
| dbp:magnitude | 24.610000 (xsd:double) |
| dbp:meanAnomaly | 349.800000 (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 | 6.1852896E7 |
| dbp:perihelion | 55.849 |
| dbp:period | 2.0834643096000004E10 |
| dbp:semimajor | 75.82 |
| dbp:uncertainty | 6 (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_CTIO 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 FZ71 is a trans-Neptunian object, a scattered disc 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 a team led by American astronomer Scott Sheppard at the Cerro Tololo Inter-American Observatory in Chile. With its perihelion of almost 56 AU, it belongs to a small and poorly understood group of very distant objects with moderate eccentricities. The object is not a dwarf planet candidate as it only measures approximately 150 kilometers (93 miles) in diameter. (en) 2014 FZ71 ist ein Planetoid, der am 24. März 2014 am Cerro Tololo Observatory, La Serena entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in 668 Jahren um die Sonne, so dass er sich in einer 4:1 Bahnresonanz mit dem Neptun befindet. Die Bahnexzentrizität seiner Bahn beträgt 0,27, wobei diese 25,44° gegen die Ekliptik geneigt ist. (de) est un transneptunien de magnitude absolue 6,9 en résonance 4:1 avec Neptune. L'objet compte parmi les objets connus ayant l'un des aphélies les plus élevés. (fr) |
| rdfs:label | 2014 FZ71 (de) 2014 FZ71 (en) 2014 FZ71 (fr) |
| owl:sameAs | wikidata:2014 FZ71 dbpedia-de:2014 FZ71 dbpedia-fr:2014 FZ71 dbpedia-vi:2014 FZ71 https://global.dbpedia.org/id/4N5Zv |
| prov:wasDerivedFrom | wikipedia-en:2014_FZ71?oldid=1062067537&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/Extreme_transneptunian_object_eccentricity_vs_perihelion.png |
| foaf:isPrimaryTopicOf | wikipedia-en:2014_FZ71 |
| foaf:name | (en) |
| is foaf:primaryTopic of | wikipedia-en:2014_FZ71 |
