HD 202206 c is an extrasolar planet discovered on November 16, 2004, using long-term observation of a formerly unconfirmed second planet after the discovery of a brown dwarf (first companion) around the star HD 202206. This was the first circumbinary planet to be found around a main sequence star. Further observation of this system via astrometry revised this picture in 2017, showing that HD 202206 c is a brown dwarf or super-Jupiter, with a true mass 17.9 times that of Jupiter, in a circumbinary orbit around a pair of co-orbiting stars being viewed nearly face-on.
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| - HD 202206 c (ar)
- HD 202206 c (en)
- HD 202206 c (es)
- HD 202206 c (in)
- HD 202206 c (ko)
- HD 202206 c (pl)
- HD 202206 c (pt)
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| - HD 202206 c (بالإنجليزية: HD 202206 c) الذي يرمز له بالرمز HD 202206c، هو كوكب خارج المجموعة الشمسية، وكوكب حول نجم ثنائي، في كوكبة الجدي (كوكبة)، يتبع . (ar)
- HD 202206 c es el planeta del sistema de la estrella HD 202206, una estrella de la constelación de Capricornus, a 151 años luz del sistema solar. Tiene 2 veces la masa de Júpiter. Orbita a 2,55 ua de su estrella, en resonancia orbital 5:1 junto a HD 202206 b, una enana marrón con una masa de 17 veces la de Júpiter, orbitando a 0,83 UA de HD 202206, pero se comporta como un planeta. Es un planeta circumbinario, orbita a dos estrellas en lugar de una. (es)
- HD 202206 c adalah sebuah planet luar surya yang terletak sekitar 150,13 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 202206 c memiliki massa sebesar 17,9 massa Jupiter. (in)
- HD 202206 c는 2004년 11월 16일 발견된 외계 행성이다. 이 행성은 어머니 항성 을 오랜 시간에 걸쳐 관찰한 끝에 존재를 입증했다. 먼저 발견된 동반 천체 는 갈색 왜성임이 판명되었다. 이 행성은 먼저 발견된 b보다 공전 궤도는 3.07배 멀고, 질량은 7.13분의 1 수준이다. 질량은 목성의 2.44배이며 크기는 목성과 거의 같다. c와 갈색 왜성 b의 궤도공명비는 5:1이다. 궤도이심률은 0.44로, 우리 태양계 내 에리스를 제외한 어떠한 행성보다도 찌그러진 궤도를 돌고 있다. (ko)
- HD 202206 c – planeta pozasłoneczna, krążąca wokół gwiazdy HD 202206. Jest to gazowy olbrzym, około 2,5 raza masywniejszy od Jowisza. Planeta posiada ekscentryczną orbitę wokół gwiazdy centralnej i krążącego wokół niej brązowego karła. Znajduje się w rezonansie orbitalnym 5:1 z brązowym karłem. (pl)
- HD 202206 c is an extrasolar planet discovered on November 16, 2004, using long-term observation of a formerly unconfirmed second planet after the discovery of a brown dwarf (first companion) around the star HD 202206. This was the first circumbinary planet to be found around a main sequence star. Further observation of this system via astrometry revised this picture in 2017, showing that HD 202206 c is a brown dwarf or super-Jupiter, with a true mass 17.9 times that of Jupiter, in a circumbinary orbit around a pair of co-orbiting stars being viewed nearly face-on. (en)
- HD 202206 c é um planeta extrassolar descoberto em 16 de novembro de 2004, através da observação de longo prazo de um segunto planeta, cuja existência não era anteriormente confirmada, após a descoberta de uma anã marrom (primeira companheira) orbitando a estrela HD 202206. (pt)
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| - HD 202206 c (بالإنجليزية: HD 202206 c) الذي يرمز له بالرمز HD 202206c، هو كوكب خارج المجموعة الشمسية، وكوكب حول نجم ثنائي، في كوكبة الجدي (كوكبة)، يتبع . (ar)
- HD 202206 c is an extrasolar planet discovered on November 16, 2004, using long-term observation of a formerly unconfirmed second planet after the discovery of a brown dwarf (first companion) around the star HD 202206. This was the first circumbinary planet to be found around a main sequence star. The planet orbits 3.07 times further out and is 85% less massive than the first companion, having a semi-amplitude of only 42 m/s. Its minimum mass is 2.44 times that of Jupiter and its diameter is likely roughly the same size as Jupiter's. The orbital resonance of the planet orbiting the brown dwarf is 5:1. The eccentricity of the planet is higher than that of all the planets and dwarf planets in the Solar System except Eris, which has an eccentricity of 0.44. Further observation of this system via astrometry revised this picture in 2017, showing that HD 202206 c is a brown dwarf or super-Jupiter, with a true mass 17.9 times that of Jupiter, in a circumbinary orbit around a pair of co-orbiting stars being viewed nearly face-on. (en)
- HD 202206 c es el planeta del sistema de la estrella HD 202206, una estrella de la constelación de Capricornus, a 151 años luz del sistema solar. Tiene 2 veces la masa de Júpiter. Orbita a 2,55 ua de su estrella, en resonancia orbital 5:1 junto a HD 202206 b, una enana marrón con una masa de 17 veces la de Júpiter, orbitando a 0,83 UA de HD 202206, pero se comporta como un planeta. Es un planeta circumbinario, orbita a dos estrellas en lugar de una. (es)
- HD 202206 c adalah sebuah planet luar surya yang terletak sekitar 150,13 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 202206 c memiliki massa sebesar 17,9 massa Jupiter. (in)
- HD 202206 c는 2004년 11월 16일 발견된 외계 행성이다. 이 행성은 어머니 항성 을 오랜 시간에 걸쳐 관찰한 끝에 존재를 입증했다. 먼저 발견된 동반 천체 는 갈색 왜성임이 판명되었다. 이 행성은 먼저 발견된 b보다 공전 궤도는 3.07배 멀고, 질량은 7.13분의 1 수준이다. 질량은 목성의 2.44배이며 크기는 목성과 거의 같다. c와 갈색 왜성 b의 궤도공명비는 5:1이다. 궤도이심률은 0.44로, 우리 태양계 내 에리스를 제외한 어떠한 행성보다도 찌그러진 궤도를 돌고 있다. (ko)
- HD 202206 c é um planeta extrassolar descoberto em 16 de novembro de 2004, através da observação de longo prazo de um segunto planeta, cuja existência não era anteriormente confirmada, após a descoberta de uma anã marrom (primeira companheira) orbitando a estrela HD 202206. Este planeta perfaz sua órbita a uma distância de 3.07 vezes maior e é 7.13 vezes menos massivo que a primeira companheira, possuindo uma semi-amplitude de apenas 42 m/s. Sua massa corresponde a 2.44 planetas Júpiter e seu diâmetro se aproxima do de Júpiter. A ressonância orbital do planeta orbitando a anã marrom é de 5:1. A excentricidade do planeta é maior do que aquela de todos os planetas e planetas anões de nosso sistema solar, exceto Éris, que possui uma excentricidade de 0.44. (pt)
- HD 202206 c – planeta pozasłoneczna, krążąca wokół gwiazdy HD 202206. Jest to gazowy olbrzym, około 2,5 raza masywniejszy od Jowisza. Planeta posiada ekscentryczną orbitę wokół gwiazdy centralnej i krążącego wokół niej brązowego karła. Znajduje się w rezonansie orbitalnym 5:1 z brązowym karłem. (pl)
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