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HD 88133 b ist ein Exoplanet, der den Unte … HD 88133 b ist ein Exoplanet, der den Unterriesen HD 88133 alle 3,416 Tage umkreist. Er wurde von Debra Fischer et al. im Jahr 2004 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die große Halbachse der Umlaufbahn des Exoplaneten misst ca. 0,05 Astronomischen Einheiten, ihre Exzentrizität beträgt 0,13. Das Objekt hat eine Mindestmasse von ca. 0,29 Jupitermassen (rund 95 Erdmassen).a. 0,29 Jupitermassen (rund 95 Erdmassen).
, HD 88133 b is an extrasolar planet orbitin … HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected. In 2016 the direct detection of the planetary thermal emission spectrum was claimed, but the detection was questioned in 2021. but the detection was questioned in 2021.
, HD 88133 b는 어머니 항성 을 돌고 있는 외계 행성이다. 아마도 이 행성의 질량은 목성, 및 토성보다도 가벼울 것으로 보인다. 항성으로부터 매우 가까운 거리를 돌고 있는데, 지구 시간으로 이 행성의 1년은 3.5일밖에 되지 않는다. 어머니 항성은 태양 반지름의 2배 정도 되는 준거성인데, 아직까지 HD 88133 b가 항성 표면을 지나가는 장면은 포착되지 않았다.
, HD 88133 b é um planeta extrassolar que or … HD 88133 b é um planeta extrassolar que orbita a estrela subgigante de classe G HD 88133, localizada a aproximadamente 270 anos-luz (81 parsecs) da Terra na constelação de Leo. Foi descoberto em 2004 pelo método da velocidade radial. É um gigante gasoso com uma massa mínima de 0,229 vezes a massa de Júpiter, tendo provavelmente uma massa similar à de Saturno. Sua órbita é extremamente curta, tendo um raio médio de apenas 0,0472 UA (4,72% do raio orbital da Terra). O planeta completa uma órbita a cada 3,41587 dias.a completa uma órbita a cada 3,41587 dias.
, HD 88133 b (بالإنجليزية: HD 88133 b) الذي يرمز له بالرمز HD 88133b، هو كوكب خارج المجموعة الشمسية، في كوكبة الأسد، يتبع .
, HD 88133 b – planeta typu gorący jowisz orbitująca wokół gwiazdy HD 88133. Jej masa minimalna jest zbliżona do masy Saturna. Jeden obieg wokół gwiazdy zajmuje jej tylko około 3,5 dnia.
, HD 88133 b adalah sebuah planet luar surya yang terletak sekitar 240,61 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 88133 b memiliki massa sebesar 1,02 massa Jupiter.
, HD 88133 b est une planète extrasolaire en … HD 88133 b est une planète extrasolaire en orbite autour de l'étoile HD 88133. Elle est probablement moins massive que Jupiter et même Saturne. Elle tourne autour de l'étoile dans une orbite très serrée, opérant une révolution tous les trois jours et demi environ. Malgré le rayon relativement grand de l'étoile (environ 2 fois celui du Soleil), aucun transit astronomique n'a été mis en évidence.nsit astronomique n'a été mis en évidence.
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| rdfs:comment |
HD 88133 b é um planeta extrassolar que or … HD 88133 b é um planeta extrassolar que orbita a estrela subgigante de classe G HD 88133, localizada a aproximadamente 270 anos-luz (81 parsecs) da Terra na constelação de Leo. Foi descoberto em 2004 pelo método da velocidade radial. É um gigante gasoso com uma massa mínima de 0,229 vezes a massa de Júpiter, tendo provavelmente uma massa similar à de Saturno. Sua órbita é extremamente curta, tendo um raio médio de apenas 0,0472 UA (4,72% do raio orbital da Terra). O planeta completa uma órbita a cada 3,41587 dias.a completa uma órbita a cada 3,41587 dias.
, HD 88133 b는 어머니 항성 을 돌고 있는 외계 행성이다. 아마도 이 행성의 질량은 목성, 및 토성보다도 가벼울 것으로 보인다. 항성으로부터 매우 가까운 거리를 돌고 있는데, 지구 시간으로 이 행성의 1년은 3.5일밖에 되지 않는다. 어머니 항성은 태양 반지름의 2배 정도 되는 준거성인데, 아직까지 HD 88133 b가 항성 표면을 지나가는 장면은 포착되지 않았다.
, HD 88133 b (بالإنجليزية: HD 88133 b) الذي يرمز له بالرمز HD 88133b، هو كوكب خارج المجموعة الشمسية، في كوكبة الأسد، يتبع .
, HD 88133 b adalah sebuah planet luar surya yang terletak sekitar 240,61 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 88133 b memiliki massa sebesar 1,02 massa Jupiter.
, HD 88133 b is an extrasolar planet orbitin … HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected. In 2016 the direct detection of the planetary thermal emission spectrum was claimed, but the detection was questioned in 2021. but the detection was questioned in 2021.
, HD 88133 b ist ein Exoplanet, der den Unte … HD 88133 b ist ein Exoplanet, der den Unterriesen HD 88133 alle 3,416 Tage umkreist. Er wurde von Debra Fischer et al. im Jahr 2004 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. Die große Halbachse der Umlaufbahn des Exoplaneten misst ca. 0,05 Astronomischen Einheiten, ihre Exzentrizität beträgt 0,13. Das Objekt hat eine Mindestmasse von ca. 0,29 Jupitermassen (rund 95 Erdmassen).a. 0,29 Jupitermassen (rund 95 Erdmassen).
, HD 88133 b est une planète extrasolaire en … HD 88133 b est une planète extrasolaire en orbite autour de l'étoile HD 88133. Elle est probablement moins massive que Jupiter et même Saturne. Elle tourne autour de l'étoile dans une orbite très serrée, opérant une révolution tous les trois jours et demi environ. Malgré le rayon relativement grand de l'étoile (environ 2 fois celui du Soleil), aucun transit astronomique n'a été mis en évidence.nsit astronomique n'a été mis en évidence.
, HD 88133 b – planeta typu gorący jowisz orbitująca wokół gwiazdy HD 88133. Jej masa minimalna jest zbliżona do masy Saturna. Jeden obieg wokół gwiazdy zajmuje jej tylko około 3,5 dnia.
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