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HD 45652 b는 외뿔소자리 방향으로 지구로부터 약 118 광년 떨어진 … HD 45652 b는 외뿔소자리 방향으로 지구로부터 약 118 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 항성으로부터 약 0.23 천문단위 떨어져 돌고 있으며 1 공전주기는 지구 시간으로 44일이다. 최소 질량은 목성의 절반 정도이다. 궤도경사각을 알 수 없기 때문에 정확한 질량은 이보다 좀 더 커질 가능성이 많다. 반지름 또한 알려져 있지 않다. 2005년부터 2006년까지 ELODIE 분광사진기로 측정한 자료를 바탕으로 발견되었으며, 2006년부터 2007년 사이 CORALIE와 SOPHIE로 검증, 존재를 확인했다. 발견 사실은 2008년 5월 공표되었다.PHIE로 검증, 존재를 확인했다. 발견 사실은 2008년 5월 공표되었다.
, HD 45652 b adalah sebuah planet luar surya yang terletak sekitar 113,8 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 45652 b memiliki massa sebesar 0,433 massa Jupiter.
, HD 45652 b is a gas giant extrasolar plane … HD 45652 b is a gas giant extrasolar planet orbiting at only 0.23 AU from the star HD 45652, with an orbital period of 44 days. It has mass at least half that of Jupiter. As it was detected using the radial velocity method, its true mass is dependent on the inclination of its orbit; if it is low, then the true mass will be larger. Also, its radius is not known. This planet was discovered by measurements taken by the ELODIE spectrograph from 2005 and 2006, and later confirmed by CORALIE and SOPHIE between 2006 and 2007. The discovery was announced in May 2008. HD 45652 b, was officially named Viriato on the 17th of December 2019 after the IAU100 press conference in Paris by the IAU (International Astronomical Union).he IAU (International Astronomical Union).
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radial velocity fromELODIE
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astron
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May 2008
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Santos et al.
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| rdfs:comment |
HD 45652 b adalah sebuah planet luar surya yang terletak sekitar 113,8 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 45652 b memiliki massa sebesar 0,433 massa Jupiter.
, HD 45652 b is a gas giant extrasolar plane … HD 45652 b is a gas giant extrasolar planet orbiting at only 0.23 AU from the star HD 45652, with an orbital period of 44 days. It has mass at least half that of Jupiter. As it was detected using the radial velocity method, its true mass is dependent on the inclination of its orbit; if it is low, then the true mass will be larger. Also, its radius is not known. This planet was discovered by measurements taken by the ELODIE spectrograph from 2005 and 2006, and later confirmed by CORALIE and SOPHIE between 2006 and 2007. The discovery was announced in May 2008.. The discovery was announced in May 2008.
, HD 45652 b는 외뿔소자리 방향으로 지구로부터 약 118 광년 떨어진 … HD 45652 b는 외뿔소자리 방향으로 지구로부터 약 118 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 항성으로부터 약 0.23 천문단위 떨어져 돌고 있으며 1 공전주기는 지구 시간으로 44일이다. 최소 질량은 목성의 절반 정도이다. 궤도경사각을 알 수 없기 때문에 정확한 질량은 이보다 좀 더 커질 가능성이 많다. 반지름 또한 알려져 있지 않다. 2005년부터 2006년까지 ELODIE 분광사진기로 측정한 자료를 바탕으로 발견되었으며, 2006년부터 2007년 사이 CORALIE와 SOPHIE로 검증, 존재를 확인했다. 발견 사실은 2008년 5월 공표되었다.PHIE로 검증, 존재를 확인했다. 발견 사실은 2008년 5월 공표되었다.
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HD 45652 b
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