About: 1995 GJ

An Entity of Type: planet, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

1995 GJ might be a trans-Neptunian object and/or high-inclination cubewano from the Kuiper belt in the outermost region of the Solar System, and based on the calculated distance and brightness is assumed to be approximately 175 kilometers (110 miles) in diameter. It is a lost minor planet that has only been observed six times on the nights of 3–4 April 1995, by David Jewitt and Jun Chen at the Mauna Kea Observatory, Hawaii, using the UH88 telescope, and has not been observed ever since. The object is estimated to have been discovered right at perihelion (closest approach to the Sun) at a distance of 39±1900 AU from the Sun. On the night of discovery, the object is estimated to have been moving away from Earth at 16 km/s with the uncertainty in the velocity being an unrealistic ±238000 km/s

Property Value
dbo:absoluteMagnitude
  • 6.897300 (xsd:double)
  • 7.000000 (xsd:double)
dbo:abstract
  • 1995 GJ might be a trans-Neptunian object and/or high-inclination cubewano from the Kuiper belt in the outermost region of the Solar System, and based on the calculated distance and brightness is assumed to be approximately 175 kilometers (110 miles) in diameter. It is a lost minor planet that has only been observed six times on the nights of 3–4 April 1995, by David Jewitt and Jun Chen at the Mauna Kea Observatory, Hawaii, using the UH88 telescope, and has not been observed ever since. The object is estimated to have been discovered right at perihelion (closest approach to the Sun) at a distance of 39±1900 AU from the Sun. On the night of discovery, the object is estimated to have been moving away from Earth at 16 km/s with the uncertainty in the velocity being an unrealistic ±238000 km/s (80% the speed of light). (en)
  • 1995 GJ 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 0.091, sementara magnitudo mutlaknya adalah 7.0. (in)
  • 1995 GJ est un objet transneptunien de magnitude absolue 7,0. Son diamètre est estimé entre 110 km et 240 km. Ce serait le premier cubewano découvert ayant une inclinaison supérieure à 20°. Son arc d'observation n'est que de deux nuits, son orbite est donc mal connue, il est même considéré comme perdu. (fr)
  • 1995 GJ с наклоном орбиты 22,9°, может быть первым обнаруженным кьюбивано с наклоном орбиты более 20 градусов. У большинства же кьюбивано наклонение менее 10 градусов. Учитывая длину орбиты объекта пояса Койпера, 1995 GJ может противостоять Земле в середине марта каждого года, в этот момент его видимая звёздная величина составляет 22,9. Объект наблюдался лишь шесть раз в течение двух ночей 1995 года, 3 и 4 апреля, и потому его орбита вычислена очень неточно (имеет высший параметр неопределённости — 9). Даже эксцентриситет предположительный. 1995 GJ был обнаружен Дэвидом Джуиттом и Юн Чен в обсерватории Мауна-Кеа, Гавайи с использованием 2,2-метрового телескопа Гавайского университета. (ru)
  • 1995 GJ é um objeto transnetuniano (TNO) que está localizado no cinturão de Kuiper, uma região do Sistema Solar. Este corpo celeste é classificado como um cubewano. Ele possui uma magnitude absoluta (H) de 7 e, tem um diâmetro estimado com cerca de 175 km, por isso é pouco provável que possa ser classificado como um planeta anão, devido ao seu tamanho relativamente pequeno. Com uma inclinação orbital de 22,9° pode ser o primeiro cubewano (KBO clássico) descoberto a ter uma inclinação maior do que 20 graus. A maioria dos cubewanos tem inclinações inferiores a 10 graus. (pt)
dbo:discovered
  • 1995-04-03 (xsd:date)
dbo:discoverer
dbo:epoch
  • 4 April 1995 (JD2449811.5)
dbo:wikiPageExternalLink
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  • 13316559 (xsd:integer)
dbo:wikiPageLength
  • 7488 (xsd:nonNegativeInteger)
dbo:wikiPageRevisionID
  • 1061908249 (xsd:integer)
dbo:wikiPageWikiLink
dbp:absMagnitude
  • 6.897300 (xsd:double)
  • 7 (xsd:integer)
dbp:background
  • #C2E0FF (en)
dbp:discovered
  • 1995-04-03 (xsd:date)
dbp:discoverer
dbp:discoverySite
dbp:epoch
  • 1995-04-04 (xsd:date)
dbp:minorplanet
  • yes (en)
dbp:mpCategory
  • TNOdistant (en)
  • cubewano (en)
dbp:mpcName
  • 1995 (xsd:integer)
dbp:name
  • 1995 (xsd:integer)
dbp:observationArc
  • 86400.0
dbp:uncertainty
  • 9 (xsd:integer)
dbp:wikiPageUsesTemplate
dcterms:subject
rdf:type
rdfs:comment
  • 1995 GJ 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 0.091, sementara magnitudo mutlaknya adalah 7.0. (in)
  • 1995 GJ est un objet transneptunien de magnitude absolue 7,0. Son diamètre est estimé entre 110 km et 240 km. Ce serait le premier cubewano découvert ayant une inclinaison supérieure à 20°. Son arc d'observation n'est que de deux nuits, son orbite est donc mal connue, il est même considéré comme perdu. (fr)
  • 1995 GJ é um objeto transnetuniano (TNO) que está localizado no cinturão de Kuiper, uma região do Sistema Solar. Este corpo celeste é classificado como um cubewano. Ele possui uma magnitude absoluta (H) de 7 e, tem um diâmetro estimado com cerca de 175 km, por isso é pouco provável que possa ser classificado como um planeta anão, devido ao seu tamanho relativamente pequeno. Com uma inclinação orbital de 22,9° pode ser o primeiro cubewano (KBO clássico) descoberto a ter uma inclinação maior do que 20 graus. A maioria dos cubewanos tem inclinações inferiores a 10 graus. (pt)
  • 1995 GJ might be a trans-Neptunian object and/or high-inclination cubewano from the Kuiper belt in the outermost region of the Solar System, and based on the calculated distance and brightness is assumed to be approximately 175 kilometers (110 miles) in diameter. It is a lost minor planet that has only been observed six times on the nights of 3–4 April 1995, by David Jewitt and Jun Chen at the Mauna Kea Observatory, Hawaii, using the UH88 telescope, and has not been observed ever since. The object is estimated to have been discovered right at perihelion (closest approach to the Sun) at a distance of 39±1900 AU from the Sun. On the night of discovery, the object is estimated to have been moving away from Earth at 16 km/s with the uncertainty in the velocity being an unrealistic ±238000 km/s (en)
  • 1995 GJ с наклоном орбиты 22,9°, может быть первым обнаруженным кьюбивано с наклоном орбиты более 20 градусов. У большинства же кьюбивано наклонение менее 10 градусов. Учитывая длину орбиты объекта пояса Койпера, 1995 GJ может противостоять Земле в середине марта каждого года, в этот момент его видимая звёздная величина составляет 22,9. Объект наблюдался лишь шесть раз в течение двух ночей 1995 года, 3 и 4 апреля, и потому его орбита вычислена очень неточно (имеет высший параметр неопределённости — 9). Даже эксцентриситет предположительный. (ru)
rdfs:label
  • 1995 GJ (en)
  • 1995 GJ (in)
  • 1995 GJ (fr)
  • 1995 GJ (ko)
  • 1995 GJ (pt)
  • 1995 GJ (ru)
owl:sameAs
prov:wasDerivedFrom
foaf:isPrimaryTopicOf
foaf:name
  • (en)
  • 1995 GJ (en)
is dbo:wikiPageWikiLink of
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