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|
p Eridani est une étoile binaire située à … p Eridani est une étoile binaire située à 26,3 années-lumière de la Terre dans la constellation d'Éridan. Les deux composantes HD 10360 et HD 10361, sont deux naines orange de type spectral K2V. La masse de la première étoile est d'environ 79 % de celle du Soleil et sa luminosité de 28 % . La masse de la deuxième étoile est d'environ 60 % de celle du Soleil et sa luminosité de 25 % . Les deux étoiles sont séparées d'une distance qui varie entre 30 et 100 ua. La présence d'une planète est théoriquement possible dans ce système, car si elle se situe dans la zone habitable de la première étoile, elle ne serait pas dérangée par la deuxième étoile qui serait alors trop lointaine.me étoile qui serait alors trop lointaine.
, P Eridani (Gliese 66) is een dubbelster in het sterrenbeeld Eridanus op 26,72 lichtjaar van de Zon. Het stelsel bestaat uit twee type K Oranje dwergen (HR 486 en HR 487) en heeft een baansnelheid rond het galactisch centrum van 22,8 km/s.
, P Eridani è un sistema stellare posto a circa 25,5 anni luce di distanza dal Sistema solare, in direzione della costellazione dell'Eridano.
, p Эридана (лат. p Eridani) — двойная звезда в созвездии Эридана. Находится на расстоянии около 26 световых лет от Солнца.
, p Eridani is a binary star system in the c … p Eridani is a binary star system in the constellation of Eridanus (the River) whose distance from the Sun is 26.7 light-years based upon parallax. It was found to be a double star in December 1825 by James Dunlop in Australia at his home at Paramatta, now spelt Parramatta. It is visible to the naked eye as a dim, orange-hued star. The system is moving further from the Earth with a heliocentric radial velocity of about +20 km/s. This system consists of a pair of near identical K-type main-sequence stars with stellar classifications of K2V. Component A has visual magnitude 5.87, while component B is magnitude 5.76. They orbit each other with a period of 475.2 years, an eccentricity of 0.53, and a semimajor axis of 7.8″.ity of 0.53, and a semimajor axis of 7.8″.
, HD 10360 (p Eridanus) é uma estrela binári … HD 10360 (p Eridanus) é uma estrela binária na direção da Eridanus. Possui uma ascensão reta de 01h 39m 47.24s e uma declinação de −56° 11′ 47.2″. Sua magnitude aparente é igual a 5.76. Considerando sua distância de 27 anos-luz em relação à Terra, sua magnitude absoluta é igual a 6.21. Pertence à classe espectral K0V.l a 6.21. Pertence à classe espectral K0V.
, 波江座p（6 Eri, DUN 5）是在波江座（河流）內距離地球僅有26光年的一顆聯星。1825年12月詹姆士·丹露帕在澳大利亞帕拉瑪塔市，（現在是新南威爾斯州的帕拉瑪塔市）家中發現波江座p是雙星。
, 에리다누스자리 p는 지구에서 약 26광년 떨어진, 에리다누스자리 방향에 있는 쌍성계이다. 오스트레일리아 천문학자 제임스 던롭이 1825년 12월 이 별을 최초로 발견했다.
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6.25
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4.94
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5.76
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7.826
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K2V + K2V
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p Eri A
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0.311
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0.77
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13.7
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0.0365
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122.0035
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1811.9
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475.2
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14.961
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262.615
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0.75
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2592000.0
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5077
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| rdfs:comment |
P Eridani (Gliese 66) is een dubbelster in het sterrenbeeld Eridanus op 26,72 lichtjaar van de Zon. Het stelsel bestaat uit twee type K Oranje dwergen (HR 486 en HR 487) en heeft een baansnelheid rond het galactisch centrum van 22,8 km/s.
, p Eridani est une étoile binaire située à … p Eridani est une étoile binaire située à 26,3 années-lumière de la Terre dans la constellation d'Éridan. Les deux composantes HD 10360 et HD 10361, sont deux naines orange de type spectral K2V. La masse de la première étoile est d'environ 79 % de celle du Soleil et sa luminosité de 28 % . La masse de la deuxième étoile est d'environ 60 % de celle du Soleil et sa luminosité de 25 % . Les deux étoiles sont séparées d'une distance qui varie entre 30 et 100 ua.une distance qui varie entre 30 et 100 ua.
, HD 10360 (p Eridanus) é uma estrela binári … HD 10360 (p Eridanus) é uma estrela binária na direção da Eridanus. Possui uma ascensão reta de 01h 39m 47.24s e uma declinação de −56° 11′ 47.2″. Sua magnitude aparente é igual a 5.76. Considerando sua distância de 27 anos-luz em relação à Terra, sua magnitude absoluta é igual a 6.21. Pertence à classe espectral K0V.l a 6.21. Pertence à classe espectral K0V.
, p Эридана (лат. p Eridani) — двойная звезда в созвездии Эридана. Находится на расстоянии около 26 световых лет от Солнца.
, 에리다누스자리 p는 지구에서 약 26광년 떨어진, 에리다누스자리 방향에 있는 쌍성계이다. 오스트레일리아 천문학자 제임스 던롭이 1825년 12월 이 별을 최초로 발견했다.
, P Eridani è un sistema stellare posto a circa 25,5 anni luce di distanza dal Sistema solare, in direzione della costellazione dell'Eridano.
, 波江座p（6 Eri, DUN 5）是在波江座（河流）內距離地球僅有26光年的一顆聯星。1825年12月詹姆士·丹露帕在澳大利亞帕拉瑪塔市，（現在是新南威爾斯州的帕拉瑪塔市）家中發現波江座p是雙星。
, p Eridani is a binary star system in the c … p Eridani is a binary star system in the constellation of Eridanus (the River) whose distance from the Sun is 26.7 light-years based upon parallax. It was found to be a double star in December 1825 by James Dunlop in Australia at his home at Paramatta, now spelt Parramatta. It is visible to the naked eye as a dim, orange-hued star. The system is moving further from the Earth with a heliocentric radial velocity of about +20 km/s.centric radial velocity of about +20 km/s.
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에리다누스자리 p
, 波江座p
, P Eridani
, HD 10360
, P Эридана
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