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HD 106252 b ist höchstwahrscheinlich ein B … HD 106252 b ist höchstwahrscheinlich ein Brauner Zwerg, das den gelben Zwerg HD 106252 umkreist. HD 106252 b umkreist seinen Begleitstern alle 1531 Tage mit einer großen Halbachse von 2,7 Astronomischen Einheiten. Seine Masse wird auf rund 30 Jupitermassen geschätzt (3-σ-Konfidenzintervall 6,92–68,9 Jupitermassen). HD 106252 b wurde von Debra Fischer, Geoffrey Marcy, R. Paul Butler, Steven Vogt et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt und 2002 publiziert.keitsmethode entdeckt und 2002 publiziert.
, HD 106252 b (بالإنجليزية: HD 106252 b) الذي يرمز له بالرمز HD 106252b، هو كوكب خارج المجموعة الشمسية، في كوكبة العذراء، يتبع .
, HD 106252 b é um planeta extrassolar gigante gasoso pelo menos 7 vezes mais massivo do que Júpiter. Foi anunciado em 2001 pelo Observatório Europeu do Sul. A descoberta foi confirmada por uma equipe diferente usando o Observatório Lick.
, HD 106252 b es un planeta extrasolar gigante gaseoso masivo, que posee una masa al menos 7,1 veces la de Júpiter orbitantat 389 Gm o 12,6 o 2,60 AU de . El periodo orbital es de 516 días o 4,15 años o 49,8 meses.
, HD 106252b是一颗位于室女座、距离地球约122.11光年的大质量系外行星，其质量下限为7.1MJ。该行星的轨道距离其母星约3亿8900万公里（2.60天文单位）。其轨道周期为1516地球日（4.15年）。
, HD 106252 b adalah sebuah planet luar surya yang terletak sekitar 124,69 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2002 dengan menggunakan metode kecepatan radial. HD 106252 b memiliki massa sebesar 6,93 massa Jupiter.
, HD 106252 b is a large gas giant extrasola … HD 106252 b is a large gas giant extrasolar planet about 10 times more massive than Jupiter. It was announced in 2001 by the European Southern Observatory. The discovery was confirmed by a different team using the Lick Telescope. Astrometry of HD 106252 has determined an orbital inclination of either 46° or 134°, depending on whether the solution is prograde or retrograde. This, combined with the minimum mass, gives a true mass of 10.0 MJ, larger than the minimum mass of 7.2 MJ.J, larger than the minimum mass of 7.2 MJ.
, HD 106252 b és un planeta extrasolar gegant gasós massiu, que posseeix una massa almenys 7,1 cops més massiu que Júpiter orbitantat 389 Gm o 12,6 o 2,60 AU de . El període orbital és de 516 dies o 4,15 anys o 49,8 mesos o 131 Ms.
, HD 106252 b는 처녀자리 방향으로 지구로부터 약 122광년 떨어져 있는 외계 행성이다. 항성으로부터 2.60 AU 떨어져 있으며 공전주기는 4.15년이다. 최소 질량은 목성의 약 7배로 추정되며 궤도경사각이 알려지지 않았으므로 이 값은 더 커질 가능성이 있다.
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HD 106252 b és un planeta extrasolar gegant gasós massiu, que posseeix una massa almenys 7,1 cops més massiu que Júpiter orbitantat 389 Gm o 12,6 o 2,60 AU de . El període orbital és de 516 dies o 4,15 anys o 49,8 mesos o 131 Ms.
, HD 106252 b ist höchstwahrscheinlich ein B … HD 106252 b ist höchstwahrscheinlich ein Brauner Zwerg, das den gelben Zwerg HD 106252 umkreist. HD 106252 b umkreist seinen Begleitstern alle 1531 Tage mit einer großen Halbachse von 2,7 Astronomischen Einheiten. Seine Masse wird auf rund 30 Jupitermassen geschätzt (3-σ-Konfidenzintervall 6,92–68,9 Jupitermassen). HD 106252 b wurde von Debra Fischer, Geoffrey Marcy, R. Paul Butler, Steven Vogt et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt und 2002 publiziert.keitsmethode entdeckt und 2002 publiziert.
, HD 106252 b es un planeta extrasolar gigante gaseoso masivo, que posee una masa al menos 7,1 veces la de Júpiter orbitantat 389 Gm o 12,6 o 2,60 AU de . El periodo orbital es de 516 días o 4,15 años o 49,8 meses.
, HD 106252 b is a large gas giant extrasola … HD 106252 b is a large gas giant extrasolar planet about 10 times more massive than Jupiter. It was announced in 2001 by the European Southern Observatory. The discovery was confirmed by a different team using the Lick Telescope. Astrometry of HD 106252 has determined an orbital inclination of either 46° or 134°, depending on whether the solution is prograde or retrograde. This, combined with the minimum mass, gives a true mass of 10.0 MJ, larger than the minimum mass of 7.2 MJ.J, larger than the minimum mass of 7.2 MJ.
, HD 106252b是一颗位于室女座、距离地球约122.11光年的大质量系外行星，其质量下限为7.1MJ。该行星的轨道距离其母星约3亿8900万公里（2.60天文单位）。其轨道周期为1516地球日（4.15年）。
, HD 106252 b (بالإنجليزية: HD 106252 b) الذي يرمز له بالرمز HD 106252b، هو كوكب خارج المجموعة الشمسية، في كوكبة العذراء، يتبع .
, HD 106252 b adalah sebuah planet luar surya yang terletak sekitar 124,69 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2002 dengan menggunakan metode kecepatan radial. HD 106252 b memiliki massa sebesar 6,93 massa Jupiter.
, HD 106252 b는 처녀자리 방향으로 지구로부터 약 122광년 떨어져 있는 외계 행성이다. 항성으로부터 2.60 AU 떨어져 있으며 공전주기는 4.15년이다. 최소 질량은 목성의 약 7배로 추정되며 궤도경사각이 알려지지 않았으므로 이 값은 더 커질 가능성이 있다.
, HD 106252 b é um planeta extrassolar gigante gasoso pelo menos 7 vezes mais massivo do que Júpiter. Foi anunciado em 2001 pelo Observatório Europeu do Sul. A descoberta foi confirmada por uma equipe diferente usando o Observatório Lick.
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