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Gamma Geminorum

Star in the constellation Gemini

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  • 4 chapters

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Properties

Alhena is an evolving star that is exhausting the supply of hydrogen at its core and has entered the subgiant stage. The spectrum matches a stellar classification of A0 IV. Compared to the Sun it has 3.4 times the mass and six times the radius. It is radiating around 200 times the luminosity of the Sun from its outer envelope at an effective temperature of 9,190 K. This gives it a white hue typical of an A-class star.

Alhena is a spectroscopic binary system with a period of 12.6 years (4,614.51 days) in a highly eccentric Keplerian orbit. The secondary, with 1.4 times the mass of the Sun, is likely a G-type main-sequence star.

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