Facts about Lyra Constellation
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NASA's Kepler Space Telescope used Lyra Constellation as its primary field of view during its planet-hunting mission from 2009 to 2018.
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Ancient Greek astronomers named Lyra Constellation after the legendary lyre of Orpheus, with the harp's strings symbolically represented by the bright stars forming the pattern.
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Sulafat, the third brightest star in Lyra Constellation at magnitude 3.94, is a blue supergiant star located approximately 620 light-years from Earth.
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Delta Lyrae, a red giant star in Lyra Constellation, has a radius approximately 46 times larger than our Sun, making it one of the constellation's most expansive stars.
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Zeta Lyrae, a binary star system in Lyra Constellation, contains an eclipsing pair separated by only 4.65 astronomical units orbiting every 4.35 years.
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Beta Lyrae, a magnitude 3.52 eclipsing binary system, orbits so closely that gravitational forces stretch both stars into egg-shaped spheres exchanging material through a bridge of gas.
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Lyra Constellation's planetary nebula NGC 6720 was first observed by French astronomer Antoine Darquier in 1779, becoming one of the earliest documented nebulae discoveries.
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Lyra Constellation contains the famous Double Double star system Epsilon Lyrae, which consists of four stars arranged in two pairs, each pair orbiting around their common center of mass.
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Sheliak, the second brightest star in Lyra Constellation at magnitude 3.52, is an eclipsing binary system where two massive stars orbit each other every 12.94 days.
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About 2,600 light-years away, the Ring Nebula (Messier 57) in Lyra Constellation displays a distinctive toroidal shape created by a dying star's ejected gas expanding outward.
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In 1992, astronomers detected a planetary system around the pulsar PSR B1257+12 located in Lyra Constellation, making it one of the earliest confirmed exoplanet discoveries.
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The brightest star Vega in Lyra Constellation shines at magnitude 0.03, making it the fifth brightest star visible from Earth.