About: 2014 SR349

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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.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body Planet planet
rdfs:label	2014 SR349 (de) 2014 SR349 (en) 2014 SR349 (fr) 2014 SR349 (pt) 2014 SR349 (zh)
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)
foaf:depiction
dcterms:subject	Astronomical objects discovered in 2014 Extreme trans-Neptunian objects Scattered disc and detached objects Minor planet object articles (unnumbered)
Wikipage page ID	52009097 (xsd:integer)
Wikipage revision ID	1119677692 (xsd:integer)
Link from a Wikipage to another Wikipage	Scott Sheppard Detached object Julian day Astronomical objects discovered in 2014 Extreme trans-Neptunian objects Scattered disc and detached objects Minor planet object articles (unnumbered) Trans-Neptunian object Chad Trujillo Planet Nine Solar System Scattered disc object Cerro Tololo Observatory
sameAs	2014 SR349 2014 SR349 2014 SR349 2014 SR349 2014 SR349 2014 SR349 2014 SR349 2014 SR349
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
thumbnail	wiki-commons:Special:FilePath/Planet_nine-etnos_now.png?width=300
abs magnitude	6.600000 (xsd:double)
arg peri	341.350000 (xsd:double)
asc node	34.750000 (xsd:double)
background	#C2E0FF (en)
caption	The orbits of and other detached objects, along with the hypothetical Planet Nine's orbit on the right. (en)
dimensions	~200 km (en)
discovered	2014-09-19 (xsd:date)
discoverer	Scott Sheppard and Chad Trujillo (en)
eccentricity	0.836900 (xsd:double)
epoch	2017-02-16 (xsd:date)
image size	275 (xsd:integer)
inclination	17.980000 (xsd:double)
mean anomaly	357.300000 (xsd:double)
mean motion	0.000196 (xsd:double)
minorplanet	yes (en)
observation arc	6.37632E7 (second)
perihelion	47.57 (astronomicalUnit)
uncertainty	5 (xsd:integer)
has 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)
prov:wasDerivedFrom	wikipedia-en:2014_SR349?oldid=1119677692&ns=0
periapsis (km)	7.116370709199E9 (kilometre)
page length (characters) of wiki page	3298 (xsd:nonNegativeInteger)
absolute magnitude	6.600000 (xsd:double)
discovery date	2014-09-19 (xsd:date)
epoch	16 February 2017 (JD 2457800.5)
periapsis (μ)	7116370709199.000000 (xsd:double)
discoverer	Scott Sheppard Chad Trujillo
foaf:isPrimaryTopicOf	wikipedia-en:2014_SR349
is foaf:primaryTopic of	wikipedia-en:2014_SR349

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