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5.01152866845E7
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46.8
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70.45672499999999
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1.15190360439E7
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HD 101930 b adalah sebuah planet luar surya yang terletak sekitar 98,01 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 101930 b memiliki massa sebesar 0,25 massa Jupiter.
, HD 101930 b (بالإنجليزية: HD 101930 b) الذي يرمز له بالرمز HD 101930b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع .
, HD 101930b是一颗位于半人马座、距离地球99.42光年的系外行星，其母星为HD 101930。该行星的质量下限为1/3倍木星质量，接近土星的质量，因此被认为属于类木行星。其轨道与其母星的距离比水星轨道与太阳的距离还小，并带有轻微的离心率。
, HD 101930 b— планета-гигант, обращающаяся вокруг оранжевого карлика, в созвездии Живописца, находящегося на расстоянии 99 световых лет от Земли. Открытие было совершено методом доплеровской спектроскопии с помощью телескопа HARPS 14 февраля 2005 года.
, HD 101930 b is an extrasolar planet orbiting the star HD 101930. It has a minimum mass a third of Jupiter's, nearly the same as Saturn's so it is thought to be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric.
, HD 101930 b는 항성 을 돌고 있는 외계 행성이다. 최소 질량은 목성의 3분의 1이 되지 않는데 이는 토성과 거의 비슷한 값이다. 질량으로 볼 때 가스 행성으로 분류할 수 있다. 항성으로부터의 거리는 태양~수성 정도이며, 공전 궤도는 약간 찌그러져 있다.
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50115286684.5
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| http://dbpedia.org/ontology/averageSpeed
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168480
|
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Doppler spectroscopy
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"2005-02-14"^^xsd:date
|
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http://dbpedia.org/resource/C._Lovis +
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15552
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|
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11519036043.9
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https://web.archive.org/web/20160303171249/https:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD%2B101930 +
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16796941
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http://de.dbpedia.org/resource/HD_101930_b +
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3004
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1011306214
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astron
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251
|
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46.8
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"2005-02-14"^^xsd:date
|
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http://dbpedia.org/resource/C._Lovis +
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http://dbpedia.org/resource/Doppler_spectroscopy +
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http://dbpedia.org/resource/La_Silla_Observatory +
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0.11
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|
>0.30
|
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|
HD 101930 b
|
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6087461.039999999
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18.1
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http://dbpedia.org/resource/HD_101930 +
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2453145
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http://dbpedia.org/resource/Planet +
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|
| rdfs:comment |
HD 101930 b adalah sebuah planet luar surya yang terletak sekitar 98,01 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2005 dengan menggunakan metode kecepatan radial. HD 101930 b memiliki massa sebesar 0,25 massa Jupiter.
, HD 101930 b는 항성 을 돌고 있는 외계 행성이다. 최소 질량은 목성의 3분의 1이 되지 않는데 이는 토성과 거의 비슷한 값이다. 질량으로 볼 때 가스 행성으로 분류할 수 있다. 항성으로부터의 거리는 태양~수성 정도이며, 공전 궤도는 약간 찌그러져 있다.
, HD 101930 b (بالإنجليزية: HD 101930 b) الذي يرمز له بالرمز HD 101930b، هو كوكب خارج المجموعة الشمسية، في كوكبة قنطورس، يتبع .
, HD 101930 b— планета-гигант, обращающаяся вокруг оранжевого карлика, в созвездии Живописца, находящегося на расстоянии 99 световых лет от Земли. Открытие было совершено методом доплеровской спектроскопии с помощью телескопа HARPS 14 февраля 2005 года.
, HD 101930 b is an extrasolar planet orbiting the star HD 101930. It has a minimum mass a third of Jupiter's, nearly the same as Saturn's so it is thought to be a gas giant. It orbits the star closer than Mercury, and the orbit is slightly eccentric.
, HD 101930b是一颗位于半人马座、距离地球99.42光年的系外行星，其母星为HD 101930。该行星的质量下限为1/3倍木星质量，接近土星的质量，因此被认为属于类木行星。其轨道与其母星的距离比水星轨道与太阳的距离还小，并带有轻微的离心率。
|
| rdfs:label |
HD 101930 b
, HD 101930 Ab
, HD 101930b
|
