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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| - كيبلر-36b (ar)
- Kepler-36b (es)
- Kepler-36 b (fr)
- Kepler-36b (en)
- ケプラー36b (ja)
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| - 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)
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| - 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)
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