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HD 100777 b, formally named Laligurans, is an extrasolar planet located approximately 172 light-years away in the constellation of Leo, orbiting the star HD 100777. This is a >1.17 MJ planet taking 33.15 Ms to orbit at 154.1 Gm or 4.99 μpc from the star at 36% eccentricity. The velocity of the orbit is 29.3 km/s. discovered this planet in March 2007 by using HARPS spectrograph located in Chile.

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  • HD 100777 b (ar)
  • HD 100777 b (de)
  • HD 100777 b (en)
  • HD 100777 b (es)
  • HD 100777 b (in)
  • HD 100777 b (ko)
  • HD 100777 b (ru)
  • HD 100777 b (zh)
rdfs:comment
  • HD 100777 b (بالإنجليزية: HD 100777 b)‏ الذي يرمز له بالرمز HD 100777b، هو كوكب خارج المجموعة الشمسية، في كوكبة الأسد، يتبع ‏. (ar)
  • HD 100777 b ist ein Exoplanet, der den Stern HD 100777 mit einer Umlaufperiode von rund 384 Tagen umkreist. Die große Halbachse der Bahn misst ca. 1,0 Astronomischen Einheiten, die Mindestmasse beträgt 1,2 Jupitermassen (etwa 370 Erdmassen). Die Entdeckung des Objekts mit Hilfe der Radialgeschwindigkeitsmethode wurde von Naef et al. im Jahr 2007 publiziert. (de)
  • HD 100777 b es un planeta extrasolar situado a unos 172 años luz de distancia en la constelación de Leo, que orbita la estrella . Se trata de un planeta 1,17 MJ que toma 33.15 Megasegundos de órbita a 154,1 Gm o μpc 4.99 de la estrella en el 36% excentricidad. La velocidad de la órbita es 29.3 kilómetros / s. Dominique Naef descubrió este planeta en marzo de 2007 mediante el espectrógrafo HARPS, situado en Chile. (es)
  • HD 100777 b, formally named Laligurans, is an extrasolar planet located approximately 172 light-years away in the constellation of Leo, orbiting the star HD 100777. This is a >1.17 MJ planet taking 33.15 Ms to orbit at 154.1 Gm or 4.99 μpc from the star at 36% eccentricity. The velocity of the orbit is 29.3 km/s. discovered this planet in March 2007 by using HARPS spectrograph located in Chile. (en)
  • HD 100777 b adalah sebuah planet luar surya yang terletak sekitar 161,78 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2007 dengan menggunakan metode kecepatan radial. HD 100777 b memiliki massa sebesar 1,03 massa Jupiter. (in)
  • HD 100777 b는 사자자리 방향으로 지구로부터 172광년 떨어져 있는 외계 행성이다. 어머니 항성은 이다. 질량은 최소 목성의 1.17 배이며 항성에서 1.03 천문단위 떨어져서 이심률 0.36의 궤도를 그리면서 돌고 있다. 공전 속도는 초당 29.3 킬로미터이다. Dominique Naef가 2007년 3월 칠레 소재 HARPS 분광사진기를 이용하여 발견했다. (ko)
  • HD 100777b是一颗位于狮子座、距离地球约172光年的系外行星,其母星为HD 100777。该行星的质量下限为1.17MJ,其轨道周期为3.315×107秒,其轨道距离中央恒星约1亿5410万公里,轨道离心率为0.36。该行星的轨道速度为29.3公里/秒。2007年3月,多米尼克·纳伊夫在智利通过高精度径向速度行星搜索器发现了该行星。 (zh)
  • HD 100777 b — газовый гигант, вращающийся вокруг звезды HD 100777 спектрального класса K0IV. Открыт HARPS методом доплеровской спектроскопии в 2003 году. (ru)
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  • HD 100777 b (en)
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  • HD 100777 b (en)
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semi-amplitude
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  • astron (en)
arg peri
avg speed
discovered
discoverer
  • Naef et al. (en)
discovery method
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eccentricity
mass
  • >1.17 ± 0.02 (en)
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