HD 48265 b is an extrasolar planet located approximately 293 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.47 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 1.81 AU with an orbital eccentricity of 0.08. As part of the NameExoWorlds project of the IAU, HD 48265 b has been named "Naqaỹa" ("brother") and HD 48265 "Nosaxa" ("springtime") in the Moqoit language, as voted by Argentine voters in an online poll.
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| - HD 48265 b (ar)
- HD 48265 b (en)
- HD 48265 b (es)
- HD 48265 b (in)
- HD 48265 b (ko)
- HD 48265 b (pl)
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| - HD 48265 b (بالإنجليزية: HD 48265 b) الذي يرمز له بالرمز HD 48265b، هو كوكب خارج المجموعة الشمسية، في كوكبة الكوثل، يتبع Nosaxa . (ar)
- HD 48265 b is an extrasolar planet located approximately 293 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.47 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 1.81 AU with an orbital eccentricity of 0.08. As part of the NameExoWorlds project of the IAU, HD 48265 b has been named "Naqaỹa" ("brother") and HD 48265 "Nosaxa" ("springtime") in the Moqoit language, as voted by Argentine voters in an online poll. (en)
- HD 48265 b es un planeta extrasolar que se encuentra aproximadamente a 285 años luz en la constelación de Puppis, orbitando la estrella de tipo G , de la secuencia principal. Este planeta orbita a una distancia de 0,45 UA y excentricidad, de 0,24. Su masa mínima equivale a 1,2 masas jovianas. Sin embargo solo se conoce su masa mínima, ya que la inclinación de la órbita no se conoce. Este planeta fue descubierto el 29 de octubre de 2008 por Minniti et al. desde el observatorio de La Silla (Chile), usando el método de la velocidad radial. (es)
- HD 48265 b adalah sebuah planet luar surya yang terletak sekitar 296,09 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 48265 b memiliki massa sebesar 1,525 massa Jupiter. (in)
- HD 48265 b는 고물자리 방향으로 지구로부터 약 285 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 어머니 항성은 분광형 G의 주계열성이다. 최소 질량은 목성의 1.2배이지만 궤도경사각이 밝혀지지 않았으므로 이 값은 얼마든지 더 커질 수 있다. 항성으로부터 1.6 천문단위 떨어진 곳을 돌고 있으며, 궤도이심률은 0.24이다. 2008년 10월 29일 민니티 연구진이 칠레 아타카마 사막 소재 라 실라 천문대 소재 CORALIE 분광사진기를 이용하여 이 행성을 찾아냈다. (ko)
- HD 48265 b (Naqaỹa) – planeta pozasłoneczna typu gazowy olbrzym orbitująca wokół gwiazdy (Nosaxa) położonej w gwiazdozbiorze Rufy, oddalona o ponad 87 parseków od Ziemi. (pl)
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| - HD 48265 b (بالإنجليزية: HD 48265 b) الذي يرمز له بالرمز HD 48265b، هو كوكب خارج المجموعة الشمسية، في كوكبة الكوثل، يتبع Nosaxa . (ar)
- HD 48265 b is an extrasolar planet located approximately 293 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.47 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 1.81 AU with an orbital eccentricity of 0.08. As part of the NameExoWorlds project of the IAU, HD 48265 b has been named "Naqaỹa" ("brother") and HD 48265 "Nosaxa" ("springtime") in the Moqoit language, as voted by Argentine voters in an online poll. (en)
- HD 48265 b es un planeta extrasolar que se encuentra aproximadamente a 285 años luz en la constelación de Puppis, orbitando la estrella de tipo G , de la secuencia principal. Este planeta orbita a una distancia de 0,45 UA y excentricidad, de 0,24. Su masa mínima equivale a 1,2 masas jovianas. Sin embargo solo se conoce su masa mínima, ya que la inclinación de la órbita no se conoce. Este planeta fue descubierto el 29 de octubre de 2008 por Minniti et al. desde el observatorio de La Silla (Chile), usando el método de la velocidad radial. (es)
- HD 48265 b adalah sebuah planet luar surya yang terletak sekitar 296,09 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 48265 b memiliki massa sebesar 1,525 massa Jupiter. (in)
- HD 48265 b는 고물자리 방향으로 지구로부터 약 285 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 어머니 항성은 분광형 G의 주계열성이다. 최소 질량은 목성의 1.2배이지만 궤도경사각이 밝혀지지 않았으므로 이 값은 얼마든지 더 커질 수 있다. 항성으로부터 1.6 천문단위 떨어진 곳을 돌고 있으며, 궤도이심률은 0.24이다. 2008년 10월 29일 민니티 연구진이 칠레 아타카마 사막 소재 라 실라 천문대 소재 CORALIE 분광사진기를 이용하여 이 행성을 찾아냈다. (ko)
- HD 48265 b (Naqaỹa) – planeta pozasłoneczna typu gazowy olbrzym orbitująca wokół gwiazdy (Nosaxa) położonej w gwiazdozbiorze Rufy, oddalona o ponad 87 parseków od Ziemi. (pl)
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