2014 SR349 (original) (raw)
2014 SR349 is a trans-Neptunian object and scattered disc object in the outermost part of the Solar System. It was first observed on 19 September 2014 by astronomers Scott Sheppard and Chad Trujillo at Cerro Tololo Observatory, Chile, and revealed on 29 August 2016. It currently has a magnitude of 24.18.
| Property | Value |
|---|---|
| dbo:Planet/periapsis | 7.116370709199E9 (dbd:kilometre) |
| dbo:absoluteMagnitude | 6.600000 (xsd:double) |
| dbo:abstract | 2014 SR349 is a trans-Neptunian object and scattered disc object in the outermost part of the Solar System. It was first observed on 19 September 2014 by astronomers Scott Sheppard and Chad Trujillo at Cerro Tololo Observatory, Chile, and revealed on 29 August 2016. It currently has a magnitude of 24.18. (en) 2014 SR349 ist ein Planetoid, der am 19. September 2014 am Cerro Tololo Observatory, La Serena entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in ca. 5250 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,84, wobei diese 17,98° gegen die Ekliptik geneigt ist. (de) 2014 SR349 est un objet transneptunien détaché, dont l'orbite pourrait être expliquée par la présence d'une planète hypothétique et encore inconnue. (fr) 2014 SR349, também escrito como 2014 SR349, é um objeto transnetuniano que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 6,6 e tem um diâmetro estimado em torno de 211 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt) 2014 SR349是一個發現於2014年的海王星外天體，由天文學家斯科特·谢泼德與乍德·特魯希略發現。該天體與另外兩顆海王星外天體2013 FT28與2014 FE72於2016年8月29日宣布發現，這些天體的發現被認為是假設中存在的第九行星更有力的證據。它目前的視星等24.22。 (zh) |
| dbo:discovered | 2014-09-19 (xsd:date) |
| dbo:discoverer | dbr:Scott_Sheppard dbr:Chad_Trujillo |
| dbo:epoch | 16 February 2017 (JD 2457800.5) |
| dbo:periapsis | 7116370709199.000000 (xsd:double) |
| dbo:thumbnail | wiki-commons:Special:FilePath/Planet_nine-etnos_now.png?width=300 |
| dbo:wikiPageID | 52009097 (xsd:integer) |
| dbo:wikiPageLength | 3298 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1119677692 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Scott_Sheppard dbr:Detached_object dbr:Julian_day dbc:Astronomical_objects_discovered_in_2014 dbc:Extreme_trans-Neptunian_objects dbc:Scattered_disc_and_detached_objects dbc:Minor_planet_object_articles_(unnumbered) dbr:Trans-Neptunian_object dbr:Chad_Trujillo dbr:Planet_Nine dbr:Solar_System dbr:Scattered_disc_object dbr:Cerro_Tololo_Observatory |
| dbp:absMagnitude | 6.600000 (xsd:double) |
| dbp:argPeri | 341.350000 (xsd:double) |
| dbp:ascNode | 34.750000 (xsd:double) |
| dbp:background | #C2E0FF (en) |
| dbp:caption | The orbits of and other detached objects, along with the hypothetical Planet Nine's orbit on the right. (en) |
| dbp:dimensions | ~200 km (en) |
| dbp:discovered | 2014-09-19 (xsd:date) |
| dbp:discoverer | Scott Sheppard and Chad Trujillo (en) |
| dbp:eccentricity | 0.836900 (xsd:double) |
| dbp:epoch | 2017-02-16 (xsd:date) |
| dbp:imageSize | 275 (xsd:integer) |
| dbp:inclination | 17.980000 (xsd:double) |
| dbp:meanAnomaly | 357.300000 (xsd:double) |
| dbp:meanMotion | 0.000196 (xsd:double) |
| dbp:minorplanet | yes (en) |
| dbp:observationArc | 6.37632E7 (dbd:second) |
| dbp:perihelion | 47.57 (dbd:astronomicalUnit) |
| dbp:uncertainty | 5 (xsd:integer) |
| dbp:wikiPageUsesTemplate | dbt:CentaurTNO-stub dbt:ESA-SSA dbt:Infobox_planet dbt:JPL_small_body dbt:Mp dbt:NeoDys dbt:Reflist dbt:Small_Solar_System_bodies dbt:Ubl dbt:Use_dmy_dates |
| dct:subject | dbc:Astronomical_objects_discovered_in_2014 dbc:Extreme_trans-Neptunian_objects 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 SR349 is a trans-Neptunian object and scattered disc object in the outermost part of the Solar System. It was first observed on 19 September 2014 by astronomers Scott Sheppard and Chad Trujillo at Cerro Tololo Observatory, Chile, and revealed on 29 August 2016. It currently has a magnitude of 24.18. (en) 2014 SR349 ist ein Planetoid, der am 19. September 2014 am Cerro Tololo Observatory, La Serena entdeckt wurde und zur Gruppe der Kuipergürtel-Planetoiden gehört. Der Asteroid läuft auf einer hoch exzentrischen Bahn in ca. 5250 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,84, wobei diese 17,98° gegen die Ekliptik geneigt ist. (de) 2014 SR349 est un objet transneptunien détaché, dont l'orbite pourrait être expliquée par la présence d'une planète hypothétique et encore inconnue. (fr) 2014 SR349, também escrito como 2014 SR349, é um objeto transnetuniano que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 6,6 e tem um diâmetro estimado em torno de 211 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt) 2014 SR349是一個發現於2014年的海王星外天體，由天文學家斯科特·谢泼德與乍德·特魯希略發現。該天體與另外兩顆海王星外天體2013 FT28與2014 FE72於2016年8月29日宣布發現，這些天體的發現被認為是假設中存在的第九行星更有力的證據。它目前的視星等24.22。 (zh) |
| rdfs:label | 2014 SR349 (de) 2014 SR349 (en) 2014 SR349 (fr) 2014 SR349 (pt) 2014 SR349 (zh) |
| owl:sameAs | yago-res:2014 SR349 wikidata:2014 SR349 dbpedia-de:2014 SR349 dbpedia-fr:2014 SR349 dbpedia-pt:2014 SR349 dbpedia-vi:2014 SR349 dbpedia-zh:2014 SR349 https://global.dbpedia.org/id/2cpEj |
| prov:wasDerivedFrom | wikipedia-en:2014_SR349?oldid=1119677692&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/Planet_nine-etnos_now.png |
| foaf:isPrimaryTopicOf | wikipedia-en:2014_SR349 |
| is foaf:primaryTopic of | wikipedia-en:2014_SR349 |
