Nu Aurigae Explained

Nu Aurigae, Latinised from Ī½ Aurigae, is the Bayer designation for a star in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 3.96 and is approximately 200abbr=offNaNabbr=off distant from the Earth. This is an evolved giant star with a stellar classification of G9.5 III. It is a red clump star, which indicates that it is generating energy through the fusion of helium at its core. The outer envelope has expanded to 18 times the radius of the Sun and cooled to, giving it the characteristic yellow-hued glow of a G-type star. It shines with 126 times the luminosity of the Sun.

This is an astrometric binary with a suspected white dwarf companion. A 10th-magnitude star 54.6 arcseconds away is an optical companion.

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