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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.

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  • 2014 SR349
  • 2014 SR349
  • 2014 SR349
  • 2014 SR349
  • 2014 SR349
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  • 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 4996 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,84, wobei diese 17,99° gegen die Ekliptik geneigt ist.
  • 2014 SR349 est un objet transneptunien détaché.
  • 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.
  • 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.
  • 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。
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abs magnitude
arg peri
asc node
background
  • #C2E0FF
caption
  • The orbits of and other detached objects, along with the hypothetical Planet Nine's orbit on the right.
dimensions
  • ~200 km
discovered
discoverer
  • Scott Sheppard and Chad Trujillo
eccentricity
epoch
image alt
inclination
mean anomaly
mean motion
minorplanet
  • yes
observation arc
  • 6.37632E7
perihelion
  • 47.57
uncertainty
has abstract
  • 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 4996 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,84, wobei diese 17,99° gegen die Ekliptik geneigt ist.
  • 2014 SR349 est un objet transneptunien détaché.
  • 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.
  • 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.
  • 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。
absolute magnitude
discovery date
epoch
  • 16 February 2017 (JD 2457800.5)
periapsis (μ)
discoverer
prov:wasDerivedFrom
periapsis (km)
  • 7.116370709199E9
page length (characters) of wiki page
is foaf:primaryTopic of
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