Semi-amplitude (K2)(secondary) 47 km/s | Magnitude 5.15 Apparent magnitude (V) 5.15 | |
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Alpha Octantis (Alpha Oct, α Octantis, α Oct) is a star in the constellation of Octans. Despite being labeled the "alpha" star by Johann Bayer in his star atlas Uranometria, it is not the brightest star in the constellation – that title belongs to Nu Octantis. It has an overall apparent visual magnitude of approximately 5.15 and is a spectroscopic binary star which consists of two giant stars, each with spectral type F, orbiting each other with a period of just over 9 days. The pair has also been classified as a Beta Lyrae-type eclipsing binary system.
References
Alpha Octantis Wikipedia(Text) CC BY-SA