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(120216) 2004 EW95 (120216) 2004 EW95 (120216) 2004 EW95 (120216) 2004 EW95 (120216) 2004 EW95 (120216) 2004 EW95 (120216) 2004 EW95
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(120216) 2004 EW95 estas tre granda, malhela transneptuna objekto malkovrita la 24-an de oktobro 2003 en la kadro de la astronomia kampanjo Spacewatch elde la Nacia Observatorio de Kitt Peak, proksime de Tucson (Arizono, Usono). Por Michael E. Brown, ĝi eble estas nanplanedo kun taksata diametro de 299 km. (120216) 2004 EW95, provisionally known as 2004 EW95, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in this region of space. It is thought that it had originated closer to the Sun, maybe even the main asteroid belt. (120216) 2004 EW95 est un objet transneptunien de la famille des plutinos. (120216) 2004 EW95 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 0.315, sementara magnitudo mutlaknya adalah 6.7. (120216) 2004 EW95, também escrito como (120216) 2004 EW95, é um objeto transnetuniano (TNO) que está localizado no Cinturão de Kuiper, uma região do Sistema Solar. Este objeto é classificado como um plutino, pois, assim como Plutão, ele está em uma ressonância orbital de 02:03 com o planeta Netuno. Para cada duas órbitas que um plutino faz, Netuno orbita três vezes. Ele possui uma magnitude absoluta de 6,7 e tem um diâmetro estimado de cerca de 291 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. 2004 إي دابليو 95 (ويعرف أيضًا باسم (120216) 2004 إي دابليو 95 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2004 EW95)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 120216 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة سبيس واتش في 14 مارس 2004.
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2004 إي دابليو 95 (ويعرف أيضًا باسم (120216) 2004 إي دابليو 95 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2004 EW95)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 120216 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة سبيس واتش في 14 مارس 2004. (120216) 2004 EW95 est un objet transneptunien de la famille des plutinos. (120216) 2004 EW95 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 0.315, sementara magnitudo mutlaknya adalah 6.7. (120216) 2004 EW95, também escrito como (120216) 2004 EW95, é um objeto transnetuniano (TNO) que está localizado no Cinturão de Kuiper, uma região do Sistema Solar. Este objeto é classificado como um plutino, pois, assim como Plutão, ele está em uma ressonância orbital de 02:03 com o planeta Netuno. Para cada duas órbitas que um plutino faz, Netuno orbita três vezes. Ele possui uma magnitude absoluta de 6,7 e tem um diâmetro estimado de cerca de 291 km. O astrônomo Mike Brown lista este corpo celeste em sua página na internet como um candidato a possível planeta anão. (120216) 2004 EW95, provisionally known as 2004 EW95, is a resonant trans-Neptunian object in the Kuiper belt located in the outermost regions of the Solar System. It measures approximately 291 kilometers in diameter. It has more carbon than typical of KBOs, and the first to be confirmed as having this composition in this region of space. It is thought that it had originated closer to the Sun, maybe even the main asteroid belt. (120216) 2004 EW95 estas tre granda, malhela transneptuna objekto malkovrita la 24-an de oktobro 2003 en la kadro de la astronomia kampanjo Spacewatch elde la Nacia Observatorio de Kitt Peak, proksime de Tucson (Arizono, Usono). Por Michael E. Brown, ĝi eble estas nanplanedo kun taksata diametro de 299 km.
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