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(120348) 2004 TY364, provisionally known as 2004 TY364, is a trans-Neptunian object. It is an inner classical Kuiper belt object in the definition by Gladman, Marsden, and Van Laerhoven (e<0.24). Its inclination of almost 25 degrees disqualifies it as such in Marc Buie's definition. It is also not listed as a scattered disc object by the Minor Planet Center. It was discovered by Michael E. Brown, Chad Trujillo and David L. Rabinowitz on October 3, 2004 at the Palomar Observatory. Light-curve analysis suggests it is not a dwarf planet. As of 2014, it is 39.2 AU from the Sun.

AttributesValues
rdf:type
rdfs:label
  • (120348) 2004 TY364 (ar)
  • (120348) 2004 TY364 (de)
  • (120348) 2004 TY364 (el)
  • (120348) 2004 TY364 (en)
  • (120348) 2004 TY364 (eo)
  • (120348) 2004 TY364 (ga)
  • (120348) 2004 TY364 (in)
  • (120348) 2004 TY364 (fr)
  • (120348) 2004 TY364 (ja)
  • (120348) 2004 TY364 (pt)
  • (120348) 2004 TY364 (ru)
rdfs:comment
  • 2004 تي واي 364 (ويعرف أيضًا باسم (120348) 2004 تي واي 364 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2004 TY364)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 120348 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة مايكل براون في 3 أكتوبر 2004. (ar)
  • (120348) 2004 TY364, provisionally known as 2004 TY364, is a trans-Neptunian object. It is an inner classical Kuiper belt object in the definition by Gladman, Marsden, and Van Laerhoven (e<0.24). Its inclination of almost 25 degrees disqualifies it as such in Marc Buie's definition. It is also not listed as a scattered disc object by the Minor Planet Center. It was discovered by Michael E. Brown, Chad Trujillo and David L. Rabinowitz on October 3, 2004 at the Palomar Observatory. Light-curve analysis suggests it is not a dwarf planet. As of 2014, it is 39.2 AU from the Sun. (en)
  • Το (120348) 2004 TY364 είναι ένα αντικείμενο της εσωτερικής ζώνης του Κάιπερ με διάμετρο περίπου 560 χιλιόμετρα. Ανακαλύφθηκε στις 3 Οκτωβρίου 2004. Είναι υποψήφιος πλανήτης νάνος. (el)
  • (120348) 2004 TY364 estas tre granda, tre hela transneptuna objekto malkovrita la 3-an de oktobro 2004 de la usonaj astronomoj Michael E. Brown, Chad Trujillo kaj David L. Rabinowitz elde la Observatorio de la Monto Palomar (San-Diego, Kalifornio, Usono). Por Michael E. Brown, ĝi verŝajne estas nanplanedo kun taksata diametro de 556 km. En 2012, F. Merlin kaj aliaj anoncis malkovron de glacio de metanolo ĉe ĝia surfaco. (eo)
  • (120348) 2004 TY364 ist ein großes transneptunisches Objekt, das bahndynamisch als erweitertes SDO eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de)
  • Is é (120348) 2004 TY364 uimhir 59 de réadanna an Ghrianchórais in ord a méid. Tá trastomhas níos lú ná 650 km aige. Tá a fhithis thart ar an ghrian níos sia amach ón ghrian ná fithis Neiptiúin agus tá sé ina bhall den Chrios Cuiper. Is réad tras-Neiptiúnach é agus tá féidearthacht ann gur abhacphláinéad é freisin. (ga)
  • (120348) 2004 TY364 est un objet transneptunien de la famille des plutinos mesurant environ 512 km de diamètre. (fr)
  • (120348) 2004 TY364 adalah sebuah objek trans-Neptunus. Seperti objek trans-Neptunus pada umumnya, benda ini mengorbit Matahari dari jarak yang lebih jauh dari planet Neptunus. Eksentrisitas orbit objek ini tercatat sebesar 0.067, sementara magnitudo mutlaknya adalah 4.5. (in)
  • (120348) 2004 TY364, também escrito como (120348) 2004 TY364, é um objeto transnetuniano que está localizado no Cinturão de Kuiper, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,5 e tem um diâmetro estimado de cerca de 365 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (pt)
  • (120348) 2004 TY364 — транснептуновый объект, расположенный в поясе Койпера. Он был обнаружен группой Майкла Брауна 3 октября 2004 года в Паломарской обсерватории. Так как объект имеет абсолютную звёздную величину 4,5, он может рассматриваться как кандидат в карликовые планеты. В настоящее время объект находится на расстоянии 39,5 а. е. от Солнца. (ru)
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