Omega Serpentis

Autor(es): Gurren Lagann

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Omega Serpentis is a binary star system consisting of a G-type giant star and a K-type main-sequence star about 251 light-years away in the constellation Serpens Caput. A planet candidate the size of Jupiter was announced orbiting the larger star of the two in 2005, but its existence wasn't confirmed until 2013

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