| dbo:Planet/apoapsis
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- 7.5458661959787E9 (dbd:kilometre)
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| dbo:Planet/orbitalPeriod
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| dbo:Planet/periapsis
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- 4.175276571237E9 (dbd:kilometre)
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| dbo:absoluteMagnitude
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| dbo:abstract
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- 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. (ar)
- (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. (en)
- (55638) 2002 VE95 estas tre granda, mez hela transneptuna objekto de la klaso de la plutonenoj: objektoj en orbita resonanco kun Neptuno. (eo)
- (55638) 2002 VE95 est un objet transneptunien de la famille des plutinos. (fr)
- (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. (in)
- (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. (pt)
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| dbo:apoapsis
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- 7545866195978.700195 (xsd:double)
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| dbo:apparentMagnitude
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| dbo:discovered
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| dbo:discoverer
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| dbo:epoch
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- 1 July 2021 (JD2459396.5)
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| dbo:formerName
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| dbo:orbitalPeriod
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- 15476395896.000000 (xsd:double)
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| dbo:periapsis
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- 4175276571237.000000 (xsd:double)
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| dbo:wikiPageExternalLink
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| dbo:wikiPageID
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| dbo:wikiPageLength
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- 18683 (xsd:nonNegativeInteger)
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| dbo:wikiPageRevisionID
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| dbo:wikiPageWikiLink
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| dbp:absMagnitude
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| dbp:aphelion
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- 50.441 (dbd:astronomicalUnit)
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| dbp:argPeri
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| dbp:ascNode
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| dbp:background
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| dbp:discovered
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| dbp:discoverer
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| dbp:discoverySite
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| dbp:earliestPrecoveryDate
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| dbp:eccentricity
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| dbp:epoch
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| dbp:inclination
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| dbp:magnitude
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| dbp:meanAnomaly
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| dbp:meanMotion
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| dbp:minorplanet
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| dbp:mpCategory
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| dbp:observationArc
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- 8.60575752E8 (dbd:second)
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| dbp:perihelion
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- 27.91 (dbd:astronomicalUnit)
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| dbp:period
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- 7.738239096E9 (dbd:second)
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| dbp:semimajor
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- 39.176 (dbd:astronomicalUnit)
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| dbp:spectralType
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- (en)
- B–R (en)
- B–V (en)
- RR (en)
- V–I (en)
- V–R (en)
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| dbp:timePeriastron
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| dbp:uncertainty
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| dbp:wikiPageUsesTemplate
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| dct:subject
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| gold:hypernym
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| rdf:type
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| rdfs:comment
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- 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. (ar)
- (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. (en)
- (55638) 2002 VE95 estas tre granda, mez hela transneptuna objekto de la klaso de la plutonenoj: objektoj en orbita resonanco kun Neptuno. (eo)
- (55638) 2002 VE95 est un objet transneptunien de la famille des plutinos. (fr)
- (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. (in)
- (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. (pt)
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| rdfs:label
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- (55638) 2002 VE95 (ar)
- (55638) 2002 VE95 (en)
- (55638) 2002 VE95 (eo)
- (55638) 2002 VE95 (in)
- (55638) 2002 VE95 (fr)
- (55638) 2002 VE95 (pt)
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