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HD 114729 b és un planeta extrasolar a aproximadament 114 anys llum en la constel·lació de Centaure. Aquest planeta és probablement lleugerament menys massiu que Júpiter.
, HD 114729 b – planeta orbitująca wokół gwiazdy HD 114729. Jej masa minimalna wynosi ok. 0,95 masy Jowisza. Średnia odległość planety od gwiazdy wynosi 2,11 j.a., co odpowiada ponad dwukrotnej odległości Ziemi od Słońca.
, HD 114729 b is an extrasolar planet approx … HD 114729 b is an extrasolar planet approximately 114 light years away in the constellation of Centaurus. This planet is probably slightly less massive than Jupiter. It is an "eccentric Jupiter" meaning that it does not orbit very near the star like the famous 51 Pegasi b but further out and its orbit is very oval-shaped. The mean distance from the star is 2.11 AU, about twice the Earth's distance from the Sun. At periastron, the planet is only 1.43 AU from the star (comparable to the distance of Mars from the Sun), and at apoastron, the orbital distance is 2.72 AU (inner asteroid belt).distance is 2.72 AU (inner asteroid belt).
, HD 114729 b는 센타우루스자리 방향으로 지구로부터 약 114광년 떨어 … HD 114729 b는 센타우루스자리 방향으로 지구로부터 약 114광년 떨어진 곳에 있는 외계 행성이다. 이 행성의 최소 질량은 목성보다 근소하게 작다. 공전 궤도는 찌그러져 있는데, 페가수스자리 51 b처럼 항성에 매우 가까이 붙어 돌고 있지는 않다. 항성으로부터 떨어져 있는 평균 거리는 2.11 AU로 지구~태양 간격의 2배가 약간 넘는다. 다만 이심률 때문에 가까울 때는 1.43, 멀어질 때는 2.72 천문단위까지 물러난다(후자의 경우 태양계의 소행성대 거리에 해당된다). 이처럼 항성에 가까워졌다 멀어졌다를 반복하기 때문에, 행성 전체는 공전 주기 전 기간에 걸쳐 극심한 기후 변화를 겪을 것으로 보인다. 전체는 공전 주기 전 기간에 걸쳐 극심한 기후 변화를 겪을 것으로 보인다.
, HD 114729 b adalah sebuah planet luar surya yang terletak sekitar 123,45 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2002 dengan menggunakan metode kecepatan radial. HD 114729 b memiliki massa sebesar 0,825 massa Jupiter.
, HD 114729 b es un planeta extrasolar que s … HD 114729 b es un planeta extrasolar que se encuentra a aproximadamente 114 años luz en la constelación de Centaurus. Este planeta es probablemente ligeramente menos masivo que Júpiter. Se trata de un Júpiter excéntrico, con la órbita más lejana que el famoso 51 Pegasi b, y muy ovalada. La media de distancia de la estrella es 2,11 UA, aproximadamente el doble de la de la Tierra con respecto al Solble de la de la Tierra con respecto al Sol
, HD 114729 b é um planeta extrassolar local … HD 114729 b é um planeta extrassolar localizado a cerca de 114 anos-luz de distância, na constelação de Centaurus. Este planeta é provavelmente um pouco menos massivo do que Júpiter. É um "Júpiter excêntrico", significando que ele não orbita muito perto da estrela como 51 Pegasi b, mas mais longe, e sua órbita tem uma excentricidade elevada. A distância média da estrela é de 2,11 UA, cerca de duas vezes a distância entre o Sol e a Terra. No periastro, o planeta está a apenas 1,43 UA da estrela (comparável à distância de Marte ao Sol) e no apoastro a distância orbital é de 2,72 UA (interior do cinturão de asteroides).2 UA (interior do cinturão de asteroides).
, HD 114729 b ist ein Exoplanet, der den gel … HD 114729 b ist ein Exoplanet, der den gelben Zwerg HD 114729 alle 1114 Tage umkreist. Er wurde von R. Paul Butler, Geoffrey Marcy, Steven S. Vogt et al. im Jahr 2003 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die Umlaufbahn hat eine große Halbachse von ca. 2,1 Astronomischen Einheiten. Seine Mindestmasse beträgt etwa 0,95 Jupitermassen (ca. 300 Erdmassen).wa 0,95 Jupitermassen (ca. 300 Erdmassen).
, HD 114729 b (بالإنجليزية: HD 114729 b) الذي يرمز له بالرمز HD 114729b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع .
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HD 114729 b és un planeta extrasolar a aproximadament 114 anys llum en la constel·lació de Centaure. Aquest planeta és probablement lleugerament menys massiu que Júpiter.
, HD 114729 b adalah sebuah planet luar surya yang terletak sekitar 123,45 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2002 dengan menggunakan metode kecepatan radial. HD 114729 b memiliki massa sebesar 0,825 massa Jupiter.
, HD 114729 b ist ein Exoplanet, der den gel … HD 114729 b ist ein Exoplanet, der den gelben Zwerg HD 114729 alle 1114 Tage umkreist. Er wurde von R. Paul Butler, Geoffrey Marcy, Steven S. Vogt et al. im Jahr 2003 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die Umlaufbahn hat eine große Halbachse von ca. 2,1 Astronomischen Einheiten. Seine Mindestmasse beträgt etwa 0,95 Jupitermassen (ca. 300 Erdmassen).wa 0,95 Jupitermassen (ca. 300 Erdmassen).
, HD 114729 b é um planeta extrassolar local … HD 114729 b é um planeta extrassolar localizado a cerca de 114 anos-luz de distância, na constelação de Centaurus. Este planeta é provavelmente um pouco menos massivo do que Júpiter. É um "Júpiter excêntrico", significando que ele não orbita muito perto da estrela como 51 Pegasi b, mas mais longe, e sua órbita tem uma excentricidade elevada. A distância média da estrela é de 2,11 UA, cerca de duas vezes a distância entre o Sol e a Terra. No periastro, o planeta está a apenas 1,43 UA da estrela (comparável à distância de Marte ao Sol) e no apoastro a distância orbital é de 2,72 UA (interior do cinturão de asteroides).2 UA (interior do cinturão de asteroides).
, HD 114729 b es un planeta extrasolar que s … HD 114729 b es un planeta extrasolar que se encuentra a aproximadamente 114 años luz en la constelación de Centaurus. Este planeta es probablemente ligeramente menos masivo que Júpiter. Se trata de un Júpiter excéntrico, con la órbita más lejana que el famoso 51 Pegasi b, y muy ovalada. La media de distancia de la estrella es 2,11 UA, aproximadamente el doble de la de la Tierra con respecto al Solble de la de la Tierra con respecto al Sol
, HD 114729 b is an extrasolar planet approx … HD 114729 b is an extrasolar planet approximately 114 light years away in the constellation of Centaurus. This planet is probably slightly less massive than Jupiter. It is an "eccentric Jupiter" meaning that it does not orbit very near the star like the famous 51 Pegasi b but further out and its orbit is very oval-shaped. The mean distance from the star is 2.11 AU, about twice the Earth's distance from the Sun. At periastron, the planet is only 1.43 AU from the star (comparable to the distance of Mars from the Sun), and at apoastron, the orbital distance is 2.72 AU (inner asteroid belt).distance is 2.72 AU (inner asteroid belt).
, HD 114729 b – planeta orbitująca wokół gwiazdy HD 114729. Jej masa minimalna wynosi ok. 0,95 masy Jowisza. Średnia odległość planety od gwiazdy wynosi 2,11 j.a., co odpowiada ponad dwukrotnej odległości Ziemi od Słońca.
, HD 114729 b는 센타우루스자리 방향으로 지구로부터 약 114광년 떨어 … HD 114729 b는 센타우루스자리 방향으로 지구로부터 약 114광년 떨어진 곳에 있는 외계 행성이다. 이 행성의 최소 질량은 목성보다 근소하게 작다. 공전 궤도는 찌그러져 있는데, 페가수스자리 51 b처럼 항성에 매우 가까이 붙어 돌고 있지는 않다. 항성으로부터 떨어져 있는 평균 거리는 2.11 AU로 지구~태양 간격의 2배가 약간 넘는다. 다만 이심률 때문에 가까울 때는 1.43, 멀어질 때는 2.72 천문단위까지 물러난다(후자의 경우 태양계의 소행성대 거리에 해당된다). 이처럼 항성에 가까워졌다 멀어졌다를 반복하기 때문에, 행성 전체는 공전 주기 전 기간에 걸쳐 극심한 기후 변화를 겪을 것으로 보인다. 전체는 공전 주기 전 기간에 걸쳐 극심한 기후 변화를 겪을 것으로 보인다.
, HD 114729 b (بالإنجليزية: HD 114729 b) الذي يرمز له بالرمز HD 114729b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع .
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