• Source: Sigma Geminorum

Sigma Geminorum (σ Gem) is a binary star system in the constellation Gemini, just to the northwest of Pollux. It is visible to the naked eye with an apparent visual magnitude of 4.20. Its annual parallax shift of 26.08 mas indicates that it is located 125 light years from the Sun.

Sigma Geminorum is a single-lined spectroscopic binary, which means that the spectrum of only one of its components can be discerned. It is an RS Canum Venaticorum variable with a period of 19.6 days, matching the orbital period. The stellar luminosity shows indications of ellipsoidal variation, as the primary component is partly filling its Roche lobe due to gravitational interaction between the two stars.
The primary component is an evolved K-type giant star with a stellar classification of K1 III. It has a relatively high rate of spin for a giant star, showing a projected rotational velocity of 26.2 km/s and a rotation period of 19.47 days. This rate is being maintained by the tidal interaction between the two stars. The surface of the primary has large star spots that are locked onto the face oriented toward the secondary component. These spots appear to migrate poleward at an average velocity of 0.12±0.03 km/s. The surface activity makes the star a bright X-ray emission source with a luminosity of 119.41×1029 ergs s−1. It displays indications of anti-solar differential rotation.
The primary has 1.28 times the mass of the Sun, but has expanded to 10.1 times the Sun's radius. It shines with 39 times the solar luminosity from its outer atmosphere at an effective temperature of 4571 K. It is roughly 5 billion years old.




References






External links


Kaler, James B. (September 9, 2015), "Sigma Geminorum", Stars, University of Illinois, retrieved 2016-12-08.

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• Bintang raksasa
• Sigma Geminorum
• List of brightest natural objects in the sky
• Bayer designation
• List of star systems within 100–150 light-years
• Giant star
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• Former constellations