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Alpha Serpentis

Double star in the constellation Serpens

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Properties

Alpha Serpentis is a giant star with a stellar classification of K2IIIbCN1, having consumed the hydrogen at its core and evolved away from the main sequence. It has 1.6 times the mass and 13.5 times the radius of the Sun. It is most likely a horizontal branch or red clump star, fusing helium into carbon and heavier elements within its core. The effective temperature of the outer envelope is 4,687 K, giving it an orange hue that is characteristic of a K-type star. It has been classified as a strong CN star, showing a higher than expected strength in the cyanogen bands.

This star is radiating about 30 times the luminosity of the Sun, while a further 32 times the Sun's luminosity is being emitted in the infrared, for 70-fold total.

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