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HD 32518 b is an extrasolar planet which orbits the K-type giant star HD 32518, located 399.7 light years away in the constellation Camelopardalis. It has a minimum mass three times greater than Jupiter and orbits the intermediate-mass giant star at a distance of only 0.59 AU in a very circular orbit. The orbit takes 10.35 months to complete one round trip around the star. This planet was detected by the radial velocity method on August 12, 2009.

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  • HD 32518 b (en)
  • HD 32518 b (es)
  • HD 32518 b (in)
  • HD 32518 b (zh)
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  • HD 32518 b es un planeta extrasolar que orbita la estrella de tipo K , localizado aproximadamente a 383 años luz, en la constelación de Camelopardalis.Este planeta tiene al menos 3 veces la masa de Júpiter y tarda 10,35 meses en completar su periodo orbital, con un semieje mayor de 0,59 UA.Este planeta fue descubierto usando el método de la velocidad radial el 12 de agosto de 2009.​ El astrónomo (2009) ha propuesto Opalia como el nombre común posible para HD 32518 b.​ (es)
  • HD 32518 b adalah sebuah planet luar surya yang terletak sekitar 399,72 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2009 dengan menggunakan metode kecepatan radial. HD 32518 b memiliki massa sebesar 3,04 massa Jupiter. (in)
  • HD 32518 b是一顆距離地球約383光年的太陽系外行星，位於鹿豹座。它的母恆星是 K 型巨星 HD 32518。該行星的質量下限是木星的3倍。它以極接近圓形的軌道環繞母恆星，距離0.59天文單位，軌道週期157.54日。HD 32518 b 於2009年8月12日以徑向速度法發現。 (zh)
  • HD 32518 b is an extrasolar planet which orbits the K-type giant star HD 32518, located 399.7 light years away in the constellation Camelopardalis. It has a minimum mass three times greater than Jupiter and orbits the intermediate-mass giant star at a distance of only 0.59 AU in a very circular orbit. The orbit takes 10.35 months to complete one round trip around the star. This planet was detected by the radial velocity method on August 12, 2009. (en)
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  • HD32518 b (en)
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  • HD 32518 b (en)
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  • astron (en)
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  • Döllinger et al. (en)
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  • HD 32518 b is an extrasolar planet which orbits the K-type giant star HD 32518, located 399.7 light years away in the constellation Camelopardalis. It has a minimum mass three times greater than Jupiter and orbits the intermediate-mass giant star at a distance of only 0.59 AU in a very circular orbit. The orbit takes 10.35 months to complete one round trip around the star. This planet was detected by the radial velocity method on August 12, 2009. For the 100th anniversary of the IAU HD 32518 and the planet HD 32518b were selected NameExoWorlds campaigns for Germany. The approved name of the planet HD 32518 b is Neri, named after the river Neri in Ethiopia, which runs through parts of the Mago National park. The name was suggested by pupils of a physics course at the in Neckargemünd. (en)
  • HD 32518 b es un planeta extrasolar que orbita la estrella de tipo K , localizado aproximadamente a 383 años luz, en la constelación de Camelopardalis.Este planeta tiene al menos 3 veces la masa de Júpiter y tarda 10,35 meses en completar su periodo orbital, con un semieje mayor de 0,59 UA.Este planeta fue descubierto usando el método de la velocidad radial el 12 de agosto de 2009.​ El astrónomo (2009) ha propuesto Opalia como el nombre común posible para HD 32518 b.​ (es)
  • HD 32518 b adalah sebuah planet luar surya yang terletak sekitar 399,72 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2009 dengan menggunakan metode kecepatan radial. HD 32518 b memiliki massa sebesar 3,04 massa Jupiter. (in)
  • HD 32518 b是一顆距離地球約383光年的太陽系外行星，位於鹿豹座。它的母恆星是 K 型巨星 HD 32518。該行星的質量下限是木星的3倍。它以極接近圓形的軌道環繞母恆星，距離0.59天文單位，軌道週期157.54日。HD 32518 b 於2009年8月12日以徑向速度法發現。 (zh)
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Method of discovery
  • Radial velocity
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