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HD 147513 b is an exoplanet approximately … HD 147513 b is an exoplanet approximately 42 light-years away in the constellation of Scorpius. It is at least 21% more massive than Jupiter. But unlike Jupiter, it orbits the star much closer, mean distance being only a third more than Earth's distance from the Sun. Its orbit is also eccentric; at periastron, it is closer to its star than Earth is from the Sun, whereas at apastron, it is further from its star than Mars to the Sun, finding itself on the outer edge of the habitable zone.f on the outer edge of the habitable zone.
, HD 147513 b是一顆距地球約42光年的系外行星，位於天蠍座。該行星的質量比木星高21%，但是和母恆星距離非常近，平均距離大約比日地距離高三分之一。不過該行星軌道離心率很高，近拱點低於日地距離，遠拱點則高於火星和太陽的距離。
, HD 147513 b는 전갈자리 방향으로 지구로부터 약 42광년 떨어진 곳에 있는 외계 행성이다. 이 행성의 최소 질량은 목성보다 21퍼센트 더 무겁다. 다만 목성과는 달리 b는 항성에 가까이 있으며 그 거리는 태양~지구 간격의 132퍼센트 정도이다. 공전 궤도는 이심률이 심한데, 근일점에서는 태양~지구 거리보다 가까워졌다가 원일점에서는 화성 궤도 뒤까지 떨어진다.
, HD 147513 b adalah sebuah planet luar surya yang terletak sekitar 42,11 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2003 dengan menggunakan metode kecepatan radial. HD 147513 b memiliki massa sebesar 1,21 massa Jupiter.
, HD 147513 b – planeta pozasłoneczna o masie większej od masy Jowisza, gazowy olbrzym, który porusza się po bardzo ekscentrycznej orbicie wokół gwiazdy HD 147513. Jej średnia odległość od gwiazdy wynosi 1,32 odległości Ziemi od Słońca.
, HD 147513 b ist ein Exoplanet, der den gelben Zwerg HD 147513 alle 528,4 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt.
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http://dbpedia.org/resource/Radial_velocity +
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| rdfs:comment |
HD 147513 b adalah sebuah planet luar surya yang terletak sekitar 42,11 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2003 dengan menggunakan metode kecepatan radial. HD 147513 b memiliki massa sebesar 1,21 massa Jupiter.
, HD 147513 b는 전갈자리 방향으로 지구로부터 약 42광년 떨어진 곳에 있는 외계 행성이다. 이 행성의 최소 질량은 목성보다 21퍼센트 더 무겁다. 다만 목성과는 달리 b는 항성에 가까이 있으며 그 거리는 태양~지구 간격의 132퍼센트 정도이다. 공전 궤도는 이심률이 심한데, 근일점에서는 태양~지구 거리보다 가까워졌다가 원일점에서는 화성 궤도 뒤까지 떨어진다.
, HD 147513 b ist ein Exoplanet, der den gelben Zwerg HD 147513 alle 528,4 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt.
, HD 147513 b – planeta pozasłoneczna o masie większej od masy Jowisza, gazowy olbrzym, który porusza się po bardzo ekscentrycznej orbicie wokół gwiazdy HD 147513. Jej średnia odległość od gwiazdy wynosi 1,32 odległości Ziemi od Słońca.
, HD 147513 b is an exoplanet approximately … HD 147513 b is an exoplanet approximately 42 light-years away in the constellation of Scorpius. It is at least 21% more massive than Jupiter. But unlike Jupiter, it orbits the star much closer, mean distance being only a third more than Earth's distance from the Sun. Its orbit is also eccentric; at periastron, it is closer to its star than Earth is from the Sun, whereas at apastron, it is further from its star than Mars to the Sun, finding itself on the outer edge of the habitable zone.f on the outer edge of the habitable zone.
, HD 147513 b是一顆距地球約42光年的系外行星，位於天蠍座。該行星的質量比木星高21%，但是和母恆星距離非常近，平均距離大約比日地距離高三分之一。不過該行星軌道離心率很高，近拱點低於日地距離，遠拱點則高於火星和太陽的距離。
|
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HD 147513 b
|
