dbo:abstract |
HD 212771 is a solitary star in the southern zodiac constellation Aquarius. It has an apparent magnitude of 7.60, making it readily visible with binoculars but not the naked eye. Parallax measurements place the object at a distance of 364 light years, and is currently receding with a radial velocity of 15 km/s. HD 212771 has a stellar classification of G8 IV, indicating that it is a subgiant evolving towards the red giant branch after being an A-type main-sequence star for 1.7 billion years. It has 156% the mass of the Sun and 5 times its radius. It radiates at 11 solar luminosities from its slightly enlarged photosphere at an effective temperature of 5,003 K, giving it a yellow-hue. Unlike most planetary hosts, HD 212771 is slightly metal deficient, and spins with a projected rotational velocity of about 2 km/s. (en) HD 212771は、みずがめ座の恒星で8等星。太陽系外惑星が発見されている。 (ja) HD 212771 — звезда в созвездии Водолея. Находится на расстоянии около 427 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета. (ru) |
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HD 212771は、みずがめ座の恒星で8等星。太陽系外惑星が発見されている。 (ja) HD 212771 — звезда в созвездии Водолея. Находится на расстоянии около 427 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета. (ru) HD 212771 is a solitary star in the southern zodiac constellation Aquarius. It has an apparent magnitude of 7.60, making it readily visible with binoculars but not the naked eye. Parallax measurements place the object at a distance of 364 light years, and is currently receding with a radial velocity of 15 km/s. (en) |
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HD 212771 (en) HD 212771 (ja) HD 212771 (ru) |
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