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Kepler-36b is an exoplanet orbiting the star Kepler-36. This planet has the closest conjunction to Kepler-36c every 97 days. Its density is similar to that of iron. During their closest approach, Kepler-36b and Kepler-36c are located only 0.013 AU (about 1,900,000 km) from each other, which causes extreme transit-timing variations for both planets. Transit-timing variations caused by Kepler-36c are strong enough to put narrow constraints on Kepler-36b's mass. The close proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium envelope.

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rdf:type
rdfs:label
  • كيبلر-36b (ar)
  • Kepler-36b (es)
  • Kepler-36 b (fr)
  • Kepler-36b (en)
  • ケプラー36b (ja)
rdfs:comment
  • كيبلر 36 بي (بالإنجليزية: Kepler-36b)‏ الذي يرمز له بالرمز KOI-277.02، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-36. (ar)
  • Kepler-36b es un exoplaneta que orbita a la estrella Kepler-36. Fue descubierto por el Telescopio Espacial Kepler en 2012.​ Durante su máximo acercamiento, Kepler-36b y Kepler-36c se encuentran sólo 0,013 UA (menos de 2 000 000 km) entre sí, lo que provoca variaciones de tránsito temporales extremas entre ambos planetas. Las variaciones de tránsitos causados por Kepler-36c son lo suficientemente fuertes para poner limitaciones estrechas en la masa de Kepler-36b. (es)
  • Kepler-36b is an exoplanet orbiting the star Kepler-36. This planet has the closest conjunction to Kepler-36c every 97 days. Its density is similar to that of iron. During their closest approach, Kepler-36b and Kepler-36c are located only 0.013 AU (about 1,900,000 km) from each other, which causes extreme transit-timing variations for both planets. Transit-timing variations caused by Kepler-36c are strong enough to put narrow constraints on Kepler-36b's mass. The close proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium envelope. (en)
  • Kepler-36 b est une exoplanète orbitant autour de l'étoile Kepler-36, elle a été découverte en 2012 par la méthode des transits. Comme la Lune avec la Terre, elle présente toujours la même face à Kepler 36.[réf. nécessaire] (fr)
  • ケプラー36b (Kepler-36b) は、地球からはくちょう座の方向に約1500光年離れた距離にある恒星ケプラー36の周りを公転する太陽系外惑星である。別名KOI-277b。 (ja)
foaf:name
  • Kepler-36b (en)
name
  • Kepler-36b (en)
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Wikipage revision ID
Link from a Wikipage to another Wikipage
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apsis
  • astron (en)
discovered
discovery method
  • Transit (en)
eccentricity
  • <0.04 (en)
inclination
  • ~90 (en)
mass
mean radius
period
single temperature
  • K (en)
star
has abstract
  • كيبلر 36 بي (بالإنجليزية: Kepler-36b)‏ الذي يرمز له بالرمز KOI-277.02، هو كوكب خارج المجموعة الشمسية، في كوكبة الدجاجة (كوكبة)، يتبع Kepler-36. (ar)
  • Kepler-36b es un exoplaneta que orbita a la estrella Kepler-36. Fue descubierto por el Telescopio Espacial Kepler en 2012.​ Durante su máximo acercamiento, Kepler-36b y Kepler-36c se encuentran sólo 0,013 UA (menos de 2 000 000 km) entre sí, lo que provoca variaciones de tránsito temporales extremas entre ambos planetas. Las variaciones de tránsitos causados por Kepler-36c son lo suficientemente fuertes para poner limitaciones estrechas en la masa de Kepler-36b. (es)
  • Kepler-36b is an exoplanet orbiting the star Kepler-36. This planet has the closest conjunction to Kepler-36c every 97 days. Its density is similar to that of iron. During their closest approach, Kepler-36b and Kepler-36c are located only 0.013 AU (about 1,900,000 km) from each other, which causes extreme transit-timing variations for both planets. Transit-timing variations caused by Kepler-36c are strong enough to put narrow constraints on Kepler-36b's mass. The close proximity of the planet to its host star combined with its relatively low mass caused the planet to lose all or most of its primordial hydrogen/helium envelope. (en)
  • Kepler-36 b est une exoplanète orbitant autour de l'étoile Kepler-36, elle a été découverte en 2012 par la méthode des transits. Comme la Lune avec la Terre, elle présente toujours la même face à Kepler 36.[réf. nécessaire] (fr)
  • ケプラー36b (Kepler-36b) は、地球からはくちょう座の方向に約1500光年離れた距離にある恒星ケプラー36の周りを公転する太陽系外惑星である。別名KOI-277b。 (ja)
gold:hypernym
prov:wasDerivedFrom
density (μ3)
orbital period (μ)
  • 13.83989 (day)
page length (characters) of wiki page
density (μ3)
Method of discovery
  • Transit(Kepler Mission)
orbital period (s)
foaf:isPrimaryTopicOf
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