BD-10°3166 b is an extrasolar planet approximately 268 light-years away in the constellation of Crater. This planet is a so-called "Hot Jupiter," a planet that orbits its parent star in a very close orbit. Distance to the star is less than 1/20th Earth's distance from the Sun. No transits by the planet have been detected, so the planet's orbital plane cannot be exactly aligned with our direction of view.
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| - BD-10°3166 b (en)
- BD-10°3166 b (ar)
- BD-10°3166 b (ca)
- BD −10° 3166 b (de)
- BD-10°3166 b (es)
- BD-10 3166 b (in)
- BD-10 3166 b (fr)
- BD-10°3166 b (ko)
- BD-10°3166 b (pt)
- BD-10°3166b (zh)
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| - BD-10°3166 b (بالإنجليزية: BD-10°3166 b) الذي يرمز له بالرمز BD-10 3166b، هو كوكب خارج المجموعة الشمسية، في كوكبة الباطية، يتبع . (ar)
- BD-10°3166 b és un planeta extrasolarsituat a aproximadament 218 anys llum en la constel·lació de la Copa. Aquest planeta és un dels anomenats "Júpiters ardents", un gegant gasós que gira al voltant de la seva estrella mare a una distància molt propera. La distància a l'estrella és menys que una vintena part de la distància de la Terra al Sol. No s'han detectat trànsits del planeta, de manera que el pla orbital del planeta no pot ser exactament alineat amb el pla de visió terrestre. (ca)
- BD-10°3166 b is an extrasolar planet approximately 268 light-years away in the constellation of Crater. This planet is a so-called "Hot Jupiter," a planet that orbits its parent star in a very close orbit. Distance to the star is less than 1/20th Earth's distance from the Sun. No transits by the planet have been detected, so the planet's orbital plane cannot be exactly aligned with our direction of view. (en)
- BD −10° 3166 b ist ein Exoplanet, der den Gelben Zwerg BD −10° 3166 mit einer Umlaufperiode von 3,49 Tagen umrundet. Es handelt sich um einen Hot Jupiter. Die große Halbachse seiner Umlaufbahn misst ca. 0,045 Astronomischen Einheiten, die Mindestmasse beträgt rund eine halbe Jupitermasse. Das Objekt wurde von Steven S. Vogt und R. Paul Butler im Jahr 2000 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. (de)
- BD-10°3166 b es un planeta extrasolar a aproximadamente 218 años luz lejanos a la tierra en la constelación de Crater. Este planeta también llamado tipo "hot Jupiter" ("Jupiter caliente"), tiene una òrbita muy cercana a su estrella. (es)
- BD-10 3166 b adalah sebuah planet luar surya yang terletak sekitar 275,97 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2000 dengan menggunakan metode kecepatan radial. BD-10 3166 b memiliki massa sebesar 0,59 massa Jupiter. (in)
- BD-10°3166 b는 컵자리 방향으로 지구에서 약 218광년 떨어진 곳에 있는 외계 행성이다. 항성과의 거리로 미루어 볼 때 소위 뜨거운 목성으로 부를 수 있다. 행성과 항성과의 거리는 지구와 태양 사이 거리의 20분의 1도 되지 않는다. 이 행성이 항성 앞을 지나가면서 빛을 가리는 현상은 관측된 적이 없기 때문에 BD-10°3166 b의 공전 궤도면은 우리가 바라보는 시선 방향과 정확히 일치하지는 않는 것으로 추측된다. (ko)
- BD-10°3166 b é um planeta extrassolar que orbita a estrela BD-10°3166 na constelação de Crater. Ele é classificado como um Júpiter quente, ou seja, um planeta que orbita a sua estrela em uma órbita muito estreita. A distância de BD-10°3166 b em relação a sua estrela equivale a menos de 1/20 da distância da Terra relativa ao Sol. Nenhum trânsito astronômico desse planeta foi até hoje detectado, de onde se depreende que sua órbita não é alinhada com o ponto de vista terrestre. (pt)
- BD-10°3166b是一颗位于巨爵座、距离地球218光年的系外行星。该行星属于热木星，其轨道距离中央恒星极近，不到地球至太阳距离的1/20。由于至今尚未观测到该行星的凌星现象，所以该行星的轨道可能与地球观测方向并不在一个平面上。 (zh)
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