(55638) 2002 VE95

http://dbpedia.org/resource/(55638)_2002_VE95 an entity of type: Thing

2002 في إي 95 (ويعرف أيضًا باسم (55638) 2002 في إي 95 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2002 VE95)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 55638 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة تعقب الأجرام القريبة من الأرض في 14 نوفمبر 2002. rdf:langString

(55638) 2002 VE95, prov. designation: 2002 VE95, is a trans-Neptunian object from the outermost region of the Solar System. It was discovered on 14 November 2002, by astronomers with the Near-Earth Asteroid Tracking program at the Palomar Observatory in California, United States. This resonant trans-Neptunian object is a member of the plutino population, locked in a 2:3 resonance with Neptune. The object is likely of primordial origin with a heterogeneous surface and a notably reddish color (RR) attributed to the presence of methanol and tholins. It has a poorly defined rotation period of 6.8 hours and measures approximately 250 kilometers (160 miles) in diameter, too small to be a dwarf planet candidate. As of 2021, it has not yet been named. rdf:langString

(55638) 2002 VE95 estas tre granda, mez hela transneptuna objekto de la klaso de la plutonenoj: objektoj en orbita resonanco kun Neptuno. rdf:langString

(55638) 2002 VE95 est un objet transneptunien de la famille des plutinos. rdf:langString

(55638) 2002 VE95 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 0.293, sementara magnitudo mutlaknya adalah 5.6. rdf:langString

(55638) 2002 VE95 é um objeto transnetuniano classificado como plutino. Foi descoberto em 14 de novembro de 2002 pelo NEAT. Possui um semieixo maior de 39,573 UA e um período orbital de 248,95 anos. Assumindo um albedo de 0,09, sua magnitude absoluta de 5,8 dá um diâmetro estimado de 334 km. rdf:langString

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rdf:langString (55638) 2002 VE95

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xsd:double 5.3

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xsd:date 2002-11-14

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xsd:date 1990-10-12

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dbpprop:epoch

xsd:date 2021-07-01

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rdf:langString B–R

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rdf:langString RR

rdf:langString V–I

rdf:langString V–R

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xsd:date 2001-06-29

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rdf:langString 2002 في إي 95 (ويعرف أيضًا باسم (55638) 2002 في إي 95 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2002 VE95)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 55638 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة تعقب الأجرام القريبة من الأرض في 14 نوفمبر 2002.

rdf:langString (55638) 2002 VE95, prov. designation: 2002 VE95, is a trans-Neptunian object from the outermost region of the Solar System. It was discovered on 14 November 2002, by astronomers with the Near-Earth Asteroid Tracking program at the Palomar Observatory in California, United States. This resonant trans-Neptunian object is a member of the plutino population, locked in a 2:3 resonance with Neptune. The object is likely of primordial origin with a heterogeneous surface and a notably reddish color (RR) attributed to the presence of methanol and tholins. It has a poorly defined rotation period of 6.8 hours and measures approximately 250 kilometers (160 miles) in diameter, too small to be a dwarf planet candidate. As of 2021, it has not yet been named.

rdf:langString (55638) 2002 VE95 estas tre granda, mez hela transneptuna objekto de la klaso de la plutonenoj: objektoj en orbita resonanco kun Neptuno.

rdf:langString (55638) 2002 VE95 est un objet transneptunien de la famille des plutinos.

rdf:langString (55638) 2002 VE95 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 0.293, sementara magnitudo mutlaknya adalah 5.6.

rdf:langString (55638) 2002 VE95 é um objeto transnetuniano classificado como plutino. Foi descoberto em 14 de novembro de 2002 pelo NEAT. Possui um semieixo maior de 39,573 UA e um período orbital de 248,95 anos. Assumindo um albedo de 0,09, sua magnitude absoluta de 5,8 dá um diâmetro estimado de 334 km.

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