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- Q1334044 subject Q7009393.
- Q1334044 subject Q7207584.
- Q1334044 subject Q8293947.
- Q1334044 abstract "Gamma Lyrae (γ Lyr, γ Lyrae) is the second brightest star in the northern constellation of Lyra. It has the traditional names Sulafat (Sulaphat), from the Arabic السلحفاة al-sulḥafāt "turtle", and Jugum, from the Latin iugum "yoke". The connection with turtles is that fine harps were traditionally made of tortoiseshell. The apparent visual magnitude of Sulafat is 3.3, which is readily visible to the naked eye. Parallax measurements yield an estimated distance of 620 light-years (190 parsecs) from the Earth.This is a giant star with a stellar classification of B9 III, indicating it has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The effective temperature of the outer envelope of this star is 10,080 K, giving it the blue-white hue typical of a B-type star. The interferometry-measured angular diameter of this star is 0.74 ± 0.10 mas, which, at its estimated distance, equates to a physical radius of roughly 15 times the radius of the Sun.In 1909, Canadian astronomer Samuel A. Mitchell identified this star as a spectroscopic binary, although he was unable to split the absorption lines of the components. He found that a period of 25.6 days matched his measurements. It was reported as a spectroscopic binary as recently as 2001, but is now believed to be a single star with a high rate of rotation for stars of this type.In China, 漸台 (Jiāntāi), meaning Clepsydra Terrace, refers to an asterism consisting of this star, δ2 Lyrae, β Lyrae and ι Lyrae. Consequently, γ Lyrae itself is known as 漸台三 (Jiāntāisān, English: the Third Star of Clepsydra Terrace.)".
- Q1334044 thumbnail Lyra_IAU.svg?width=300.
- Q1334044 wikiPageExternalLink sulafat.html.
- Q1334044 wikiPageWikiLink Q10484.
- Q1334044 wikiPageWikiLink Q111130.
- Q1334044 wikiPageWikiLink Q1142720.
- Q1334044 wikiPageWikiLink Q1143106.
- Q1334044 wikiPageWikiLink Q124313.
- Q1334044 wikiPageWikiLink Q1303849.
- Q1334044 wikiPageWikiLink Q13352.
- Q1334044 wikiPageWikiLink Q165074.
- Q1334044 wikiPageWikiLink Q179600.
- Q1334044 wikiPageWikiLink Q2.
- Q1334044 wikiPageWikiLink Q212111.
- Q1334044 wikiPageWikiLink Q2141546.
- Q1334044 wikiPageWikiLink Q2143996.
- Q1334044 wikiPageWikiLink Q22066400.
- Q1334044 wikiPageWikiLink Q2559671.
- Q1334044 wikiPageWikiLink Q3304055.
- Q1334044 wikiPageWikiLink Q3450.
- Q1334044 wikiPageWikiLink Q397.
- Q1334044 wikiPageWikiLink Q4147168.
- Q1334044 wikiPageWikiLink Q48440.
- Q1334044 wikiPageWikiLink Q499138.
- Q1334044 wikiPageWikiLink Q50053.
- Q1334044 wikiPageWikiLink Q523.
- Q1334044 wikiPageWikiLink Q5875.
- Q1334044 wikiPageWikiLink Q6472.
- Q1334044 wikiPageWikiLink Q7009393.
- Q1334044 wikiPageWikiLink Q7207584.
- Q1334044 wikiPageWikiLink Q8293947.
- Q1334044 wikiPageWikiLink Q850283.
- Q1334044 wikiPageWikiLink Q854050.
- Q1334044 wikiPageWikiLink Q8928.
- Q1334044 type Place.
- Q1334044 type CelestialBody.
- Q1334044 type Location.
- Q1334044 type Place.
- Q1334044 type Star.
- Q1334044 type Thing.
- Q1334044 comment "Gamma Lyrae (γ Lyr, γ Lyrae) is the second brightest star in the northern constellation of Lyra. It has the traditional names Sulafat (Sulaphat), from the Arabic السلحفاة al-sulḥafāt "turtle", and Jugum, from the Latin iugum "yoke". The connection with turtles is that fine harps were traditionally made of tortoiseshell. The apparent visual magnitude of Sulafat is 3.3, which is readily visible to the naked eye.".
- Q1334044 label "Gamma Lyrae".
- Q1334044 depiction Lyra_IAU.svg.
- Q1334044 name "Gamma Lyrae".