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HD 175541 b는 뱀자리 방향으로 지구로부터 약 416광년 떨어진 곳에 … HD 175541 b는 뱀자리 방향으로 지구로부터 약 416광년 떨어진 곳에 있는 항성 를 도는 외계 행성이다. 2007년 4월 10일 존슨 연구진이 발견했다. 항성과 행성 사이 거리가 지구~태양 거리보다 더 멈에도 불구하고 공전주기는 300일이 되지 않는다. 그 이유는 어머니 항성이 태양보다 65퍼센트 질량이 더 커서 중력장의 세기도 강하기 때문이다. 이 행성과 다른 두 행성 HD 192699 b, HD 210702 b의 발견을 통해 중간 정도 질량의 A형 항성 주변에서 행성 이동이 어떻게 일어나는지와 행성이 어떻게 생겨나는지에 대한 증거를 확보할 수 있게 되었다.일어나는지와 행성이 어떻게 생겨나는지에 대한 증거를 확보할 수 있게 되었다.
, HD 175541 b ist ein Exoplanet, der den gel … HD 175541 b ist ein Exoplanet, der den gelben Unterriesen HD 175541 alle 297,3 (± 6) Tage umkreist. Er wurde 2007 von Johnson et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Der Exoplanet weist eine Mindestmasse von 0,6 Jupitermassen auf und die große Halbachse seiner Bahn misst ca. 1,0 Astronomische Einheiten bei einer Exzentrizität von 0,3 (± 0,2).n bei einer Exzentrizität von 0,3 (± 0,2).
, HD 175541 b is a jovian planet located app … HD 175541 b is a jovian planet located approximately 424 light-years away in the constellation of Serpens, orbiting the star HD 175541. This planet was discovered in April 2007. Despite the distance of planet to star slightly more than Earth to the Sun, the period is less than 300 days that orbits in an eccentric orbit, because the parent star is 65% more massive than the Sun. The planet HD 175541 b is called Kavian. The name was selected in the NameExoWorlds campaign by Iran, during the 100th anniversary of the IAU. Kaveh (name of the star HD 175541) carries a banner called Derafsh Kaviani in the Shahnameh. The discovery of this planet and two others: HD 192699 b and HD 210702 b around intermediate-mass stars provide clues about the formation and history of migration of planets around the A-type stars.ration of planets around the A-type stars.
, HD 175541 b (بالإنجليزية: HD 175541 b) الذي يرمز له بالرمز HD 175541b، هو كوكب خارج المجموعة الشمسية، في كوكبة الحية، يتبع .
, HD 175541 b adalah sebuah planet luar surya yang terletak sekitar 424,28 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2007 dengan menggunakan metode kecepatan radial. HD 175541 b memiliki massa sebesar 0,598 massa Jupiter.
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Doppler spectroscopy
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| rdfs:comment |
HD 175541 b adalah sebuah planet luar surya yang terletak sekitar 424,28 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2007 dengan menggunakan metode kecepatan radial. HD 175541 b memiliki massa sebesar 0,598 massa Jupiter.
, HD 175541 b (بالإنجليزية: HD 175541 b) الذي يرمز له بالرمز HD 175541b، هو كوكب خارج المجموعة الشمسية، في كوكبة الحية، يتبع .
, HD 175541 b ist ein Exoplanet, der den gel … HD 175541 b ist ein Exoplanet, der den gelben Unterriesen HD 175541 alle 297,3 (± 6) Tage umkreist. Er wurde 2007 von Johnson et al. mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Der Exoplanet weist eine Mindestmasse von 0,6 Jupitermassen auf und die große Halbachse seiner Bahn misst ca. 1,0 Astronomische Einheiten bei einer Exzentrizität von 0,3 (± 0,2).n bei einer Exzentrizität von 0,3 (± 0,2).
, HD 175541 b is a jovian planet located app … HD 175541 b is a jovian planet located approximately 424 light-years away in the constellation of Serpens, orbiting the star HD 175541. This planet was discovered in April 2007. Despite the distance of planet to star slightly more than Earth to the Sun, the period is less than 300 days that orbits in an eccentric orbit, because the parent star is 65% more massive than the Sun. The discovery of this planet and two others: HD 192699 b and HD 210702 b around intermediate-mass stars provide clues about the formation and history of migration of planets around the A-type stars.ration of planets around the A-type stars.
, HD 175541 b는 뱀자리 방향으로 지구로부터 약 416광년 떨어진 곳에 … HD 175541 b는 뱀자리 방향으로 지구로부터 약 416광년 떨어진 곳에 있는 항성 를 도는 외계 행성이다. 2007년 4월 10일 존슨 연구진이 발견했다. 항성과 행성 사이 거리가 지구~태양 거리보다 더 멈에도 불구하고 공전주기는 300일이 되지 않는다. 그 이유는 어머니 항성이 태양보다 65퍼센트 질량이 더 커서 중력장의 세기도 강하기 때문이다. 이 행성과 다른 두 행성 HD 192699 b, HD 210702 b의 발견을 통해 중간 정도 질량의 A형 항성 주변에서 행성 이동이 어떻게 일어나는지와 행성이 어떻게 생겨나는지에 대한 증거를 확보할 수 있게 되었다.일어나는지와 행성이 어떻게 생겨나는지에 대한 증거를 확보할 수 있게 되었다.
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HD 175541 b
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