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BD-17°63 b is an extrasolar planet located approximately 112.5 light-years away in the constellation of Cetus, orbiting the 10th magnitude K-type main sequence star BD-17°63. This planet has a minimum mass of 5.1 MJ and orbits at a distance of 1.34 astronomical units from the star. The distance ranges from 0.62 AU to 2.06 AU, corresponding to the eccentricity of 0.54. One revolution takes about 656 days. This planet was discovered on October 26, 2008 by Moutou et al. using the HARPS spectrograph on ESO’s 3.6 meter telescope installed at La Silla Observatory in Atacama desert, Chile.

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rdf:type
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  • BD-17°63 b (ar)
  • BD−17 63 b (en)
  • BD-17°63 b (es)
  • BD-17 63 b (fr)
  • BD-17 63 b (in)
  • BD-17°63 b (ko)
  • BD −17 63 b (pl)
  • BD-17°63b (zh)
rdfs:comment
  • BD-17°63 b (بالإنجليزية: BD-17°63 b)‏ الذي يرمز له بالرمز BD-17 63b، هو كوكب خارج المجموعة الشمسية، في كوكبة قيطس، يتبع Felixvarela ‏. (ar)
  • BD-17°63 b es un planeta extrasolar que se encuentra aproximadamente a 113 años luz en la constelación de Cetus, orbitando la estrella de tipo K , de la secuencia principal. Este planeta orbita a una distancia de 1,34 UA. La distancia oscila entre los 0,62 AU y los 2,06 AU, lo que da una excentricidad de 0,54. Su periodo de revolución es de 656 días y su masa mínima equivale a 5,1 masas jovianas. Este planeta fue descubierto el 26 de octubre de 2008 por Moutou et al. usando el método de la velocidad radial desde el observatorio de La Silla (Chile). (es)
  • BD-17 63 b adalah sebuah planet luar surya yang terletak sekitar 112,49 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. BD-17 63 b memiliki massa sebesar 5,1 massa Jupiter. (in)
  • BD-17°63 b는 고래자리 방향으로 지구에서 113광년 떨어져 있는 외계 행성이다. 어머니 항성 BD-17°63은 K 분광형의 주계열성으로 겉보기 등급 +10이며 따라서 맨눈으로는 볼 수 없다. 이 행성은 최소질량이 목성의 5.1배이며 항성으로부터 평균 1.34 천문단위 떨어져 돌고 있다. 그러나 이심률은 0.54로 매우 큰 편이며 항성으로부터 가장 가까울 때는 0.62천문단위까지 접근했다가 멀어질 때는 2.06천문단위까지 물러난다. 우리 태양계에 대입할 경우, 금성보다 태양에 가까워졌다가 화성보다 멀어지는 셈이다. 1회 공전에는 656일이 걸린다. 2008년 10월 26일 칠레 아타카마 사막 소재 라 실라 천문대 유럽우주국 3.6미터 망원경에 설치된 를 이용, Moutou 연구진이 발견했다. (ko)
  • BD -17°63 b – planeta pozasłoneczna typu gazowy olbrzym położona w gwiazdozbiorze Wieloryba, orbitująca wokół gwiazdy BD -17°63 (Felixvarela), odkryta w 2008 za pomocą spektrometru HARPS. (pl)
  • BD-17°63b是一颗位于鲸鱼座、距离地球113光年的系外行星,其母星为K型主序星。该行星的质量下限为5.1倍木星质量,其轨道与母星的距离为1.34天文单位,轨道周期为656地球日。 2008年10月26日,莫托等人使用位于智利阿他加马沙漠的欧洲南方天文台3.6米望远镜上的高精度径向速度行星搜索器发现了该行星。 (zh)
  • BD-17°63 b is an extrasolar planet located approximately 112.5 light-years away in the constellation of Cetus, orbiting the 10th magnitude K-type main sequence star BD-17°63. This planet has a minimum mass of 5.1 MJ and orbits at a distance of 1.34 astronomical units from the star. The distance ranges from 0.62 AU to 2.06 AU, corresponding to the eccentricity of 0.54. One revolution takes about 656 days. This planet was discovered on October 26, 2008 by Moutou et al. using the HARPS spectrograph on ESO’s 3.6 meter telescope installed at La Silla Observatory in Atacama desert, Chile. (en)
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  • BD-17°63 b (en)
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  • BD-17°63 b (en)
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  • Moutou et al. (en)
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