Xi Andromedae

Xi Andromedae (ξ Andromedae, abbreviated Xi And, ξ And), officially named Adhil /əˈdɪl/,[7][8] is a solitary[3] star in the northern constellation of Andromeda. It has an apparent magnitude of +4.9.[2] Based on parallax measurements obtained during the Hipparcos mission, it lies at a distance of roughly 214 light-years (66 parsecs) from the Sun.

Characteristics
This star is a red clump giant star that has begun generating energy through the fusion of helium at its core, having passed through the red giant branch of its evolution.[5] It has a stellar classification of K0 IIIb,[3] with 2.5[5] times the mass of the Sun and 10[6] times the Sun's radius. Xi Andromedae is emitting nearly 46[6] times as much luminosity as the Sun from its outer envelope at an effective temperature of 4,656 K,[6] giving it the orange-hued glow of a K-type star. It has no measurable projected rotational velocity,[6] although this may simply mean that the star's pole of rotation is facing in the general direction of the Earth.