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http://dbpedia.org/ontology/abstract HD 143361 b is an extrasolar planet locateHD 143361 b is an extrasolar planet located approximately 194 light-years away in the constellation of Norma, orbiting the 9th magnitude G-type main sequence star HD 143361. This planet has a minimum mass of 3.0 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 2.0 AU with an orbital eccentricity of 0.18. This object was detected using the radial velocity method during an astronomical survey conducted by the Magellan Planet Search Program using the MIKE echelle spectrograph on the 6.5-m Magellan II (Clay) telescope.on the 6.5-m Magellan II (Clay) telescope. , HD 143361 b is een exoplaneet ongeveer 224HD 143361 b is een exoplaneet ongeveer 224 lichtjaar van het zonnestelsel in het sterrenbeeld Winkelhaak. De planeet draait om de G-klasse ster . De planeet heeft een minimale massa van drie keer die van Jupiter, maar omdat de glooiingshoek van de planeet niet bekend is, is de precieze massa ook niet bekend. De planeet draait om de ster met een afstand van twee AE met een excentriciteit van 0,15.n twee AE met een excentriciteit van 0,15. , HD 143361 b – planeta pozasłoneczna typu gazowy olbrzym odkryta w 2008. Orbituje wokół gwiazdy położonej w gwiazdozbiorze Węgielnicy, oddalonej o ponad 59 parseków od Ziemi. , HD 143361 b adalah sebuah planet luar surya yang terletak sekitar 223,91 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 143361 b memiliki massa sebesar 3,532 massa Jupiter. , HD 143361 b es un planeta extrasolar que sHD 143361 b es un planeta extrasolar que se encuentra a 194 años luz en la constelación de Norma, orbitando la estrella tipo G de la secuencia principal . Este planeta tiene una masa mínima equivalente a 3 masas jovianas. Debido a que su inclinación es desconocida, su verdadera masa se desconoce. Este planeta orbita a una distancia de su estrella de 2 UA y tiene una excentricidad de 0,18. Minniti descubrió este planeta el 29 de octubre de 2008 desde el observatorio de La Silla, en el desierto de Atacama (Chile, usando el método de la velocidad radial,, usando el método de la velocidad radial, , HD 143361 b는 직각자자리 방향으로 지구로부터 약 193.6 광년 떨HD 143361 b는 직각자자리 방향으로 지구로부터 약 193.6 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 어머니 항성은 겉보기 등급 9의 G형 주계열성이다. 행성의 최소 질량은 목성의 3.0배이다. 다만 궤도경사각이 밝혀지지 않았기 때문에 정확한 질량은 알 수 없다. 항성으로부터 약 2.0 천문단위 떨어져 있으며 궤도 이심률은 0.18이다. 칠레 아타카마 사막에 자리잡은 라 실라 천문대에서, 2008년 10월 29일 민니티 연구진이 CORALIE 분광사진기를 이용하여 이 행성을 발견했다.일 민니티 연구진이 CORALIE 분광사진기를 이용하여 이 행성을 발견했다. , إتش دي 143361 بي (بالإنجليزية: HD 143361 b)‏ الذي يرمز له بالرمز HD 143361b، هو كوكب خارج المجموعة الشمسية، في كوكبة مسطرة النقاش، يتبع ‏.
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rdfs:comment HD 143361 b es un planeta extrasolar que sHD 143361 b es un planeta extrasolar que se encuentra a 194 años luz en la constelación de Norma, orbitando la estrella tipo G de la secuencia principal . Este planeta tiene una masa mínima equivalente a 3 masas jovianas. Debido a que su inclinación es desconocida, su verdadera masa se desconoce. Este planeta orbita a una distancia de su estrella de 2 UA y tiene una excentricidad de 0,18. Minniti descubrió este planeta el 29 de octubre de 2008 desde el observatorio de La Silla, en el desierto de Atacama (Chile, usando el método de la velocidad radial,, usando el método de la velocidad radial, , HD 143361 b는 직각자자리 방향으로 지구로부터 약 193.6 광년 떨HD 143361 b는 직각자자리 방향으로 지구로부터 약 193.6 광년 떨어진 곳에 있는 항성 주위를 도는, 외계 행성이다. 어머니 항성은 겉보기 등급 9의 G형 주계열성이다. 행성의 최소 질량은 목성의 3.0배이다. 다만 궤도경사각이 밝혀지지 않았기 때문에 정확한 질량은 알 수 없다. 항성으로부터 약 2.0 천문단위 떨어져 있으며 궤도 이심률은 0.18이다. 칠레 아타카마 사막에 자리잡은 라 실라 천문대에서, 2008년 10월 29일 민니티 연구진이 CORALIE 분광사진기를 이용하여 이 행성을 발견했다.일 민니티 연구진이 CORALIE 분광사진기를 이용하여 이 행성을 발견했다. , HD 143361 b – planeta pozasłoneczna typu gazowy olbrzym odkryta w 2008. Orbituje wokół gwiazdy położonej w gwiazdozbiorze Węgielnicy, oddalonej o ponad 59 parseków od Ziemi. , HD 143361 b is an extrasolar planet locateHD 143361 b is an extrasolar planet located approximately 194 light-years away in the constellation of Norma, orbiting the 9th magnitude G-type main sequence star HD 143361. This planet has a minimum mass of 3.0 times that of Jupiter. Because the inclination is not known, the true mass is not known. This planet orbits at a distance of 2.0 AU with an orbital eccentricity of 0.18. This object was detected using the radial velocity method during an astronomical survey conducted by the Magellan Planet Search Program using the MIKE echelle spectrograph on the 6.5-m Magellan II (Clay) telescope.on the 6.5-m Magellan II (Clay) telescope. , إتش دي 143361 بي (بالإنجليزية: HD 143361 b)‏ الذي يرمز له بالرمز HD 143361b، هو كوكب خارج المجموعة الشمسية، في كوكبة مسطرة النقاش، يتبع ‏. , HD 143361 b is een exoplaneet ongeveer 224HD 143361 b is een exoplaneet ongeveer 224 lichtjaar van het zonnestelsel in het sterrenbeeld Winkelhaak. De planeet draait om de G-klasse ster . De planeet heeft een minimale massa van drie keer die van Jupiter, maar omdat de glooiingshoek van de planeet niet bekend is, is de precieze massa ook niet bekend. De planeet draait om de ster met een afstand van twee AE met een excentriciteit van 0,15.n twee AE met een excentriciteit van 0,15. , HD 143361 b adalah sebuah planet luar surya yang terletak sekitar 223,91 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2008 dengan menggunakan metode kecepatan radial. HD 143361 b memiliki massa sebesar 3,532 massa Jupiter.
rdfs:label HD 143361 b
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