About: Kepler-419c

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Kepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs )from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion.

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  • 675.47
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  • 250.0
dbo:abstract
  • كيبلر 419 سي (بالإنجليزية: Kepler-419c)‏ هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-419. (ar)
  • Kepler-419c es un planeta extrasolar que forma parte de un sistema solar formado por al menos dos planetas.​ Orbita la estrella denominada . Fue descubierto en el año 2014 por la sonda Kepler por medio de tránsito astronómico​ (es)
  • Kepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs )from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion. (en)
  • Kepler-419c adalah sebuah planet luar surya yang terletak sekitar 3390±80 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2014 dengan menggunakan metode waktu. (in)
  • Kepler-419 c (также известна как KOI-1474.02) — экзопланета, обращающаяся вокруг звезды , одна из двух планет у этой звезды, открытых телескопом Кеплер. Расположена в 2544 световых годах от Земли в созвездии Лебедя. Открыта транзитным методом. (ru)
  • 克卜勒419c(Kepler-419c,舊稱KOI-1474.02)是位於母恆星 適居帶內的超级木星型太陽系外行星。克卜勒419c與更接近母恆星的另一顆行星都是由NASA的克卜勒太空望遠鏡發現。克卜勒419c距離地球約2544光年(780秒差距,或接近2.4068×1016),在天球上位於天鵝座。該行星是以凌日時間變分法發現,即分析系外行星凌星時間資料的變化以搜尋較外側系外型星的方式。. (zh)
dbo:detectionMethod
  • Transit timing variations
dbo:discovered
  • 2014-06-12 (xsd:date)
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  • 58360608.000000 (xsd:double)
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  • 250.000000 (xsd:double)
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dbo:wikiPageWikiLink
dbp:apsis
  • astron (en)
dbp:caption
  • An artist's impression of the super-Jupiter exoplanet Kepler-419c, with a system of natural satellites orbiting it (en)
dbp:discovered
  • 2014-06-12 (xsd:date)
dbp:discoverer
  • Kepler spacecraft (en)
dbp:discoveryMethod
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  • 0.184000 (xsd:double)
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  • 7.300000 (xsd:double)
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  • 1.130000 (xsd:double)
dbp:name
  • Kepler-419c (en)
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  • 5.8360608000000015E7
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  • 1.68
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  • كيبلر 419 سي (بالإنجليزية: Kepler-419c)‏ هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-419. (ar)
  • Kepler-419c es un planeta extrasolar que forma parte de un sistema solar formado por al menos dos planetas.​ Orbita la estrella denominada . Fue descubierto en el año 2014 por la sonda Kepler por medio de tránsito astronómico​ (es)
  • Kepler-419c (also known by its Kepler Object of Interest designation KOI-1474.02) is a super-Jupiter exoplanet orbiting within the habitable zone of the star Kepler-419, the outermost of two such planets discovered by NASA's Kepler spacecraft. It is located about 3,400 light-years (1040 parsecs )from Earth in the constellation Cygnus. The exoplanet was found by using the transit timing variation method, in which the variations of transit data from an exoplanet are studied to reveal a more distant companion. (en)
  • Kepler-419c adalah sebuah planet luar surya yang terletak sekitar 3390±80 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2014 dengan menggunakan metode waktu. (in)
  • Kepler-419 c (также известна как KOI-1474.02) — экзопланета, обращающаяся вокруг звезды , одна из двух планет у этой звезды, открытых телескопом Кеплер. Расположена в 2544 световых годах от Земли в созвездии Лебедя. Открыта транзитным методом. (ru)
  • 克卜勒419c(Kepler-419c,舊稱KOI-1474.02)是位於母恆星 適居帶內的超级木星型太陽系外行星。克卜勒419c與更接近母恆星的另一顆行星都是由NASA的克卜勒太空望遠鏡發現。克卜勒419c距離地球約2544光年(780秒差距,或接近2.4068×1016),在天球上位於天鵝座。該行星是以凌日時間變分法發現,即分析系外行星凌星時間資料的變化以搜尋較外側系外型星的方式。. (zh)
rdfs:label
  • كيبلر-419c (ar)
  • Kepler-419c (es)
  • Kepler-419c (in)
  • Kepler-419c (en)
  • Kepler-419 c (ru)
  • 克卜勒419c (zh)
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  • Kepler-419c (en)
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