Nu Ceti is a binary star system in the equatorial constellation of Cetus. Its name is a Bayer designation that is Latinized from ν Ceti, and abbreviated ν Ceti or ν Cet. This system is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.86. It is located approximately 340 light years distant from the Sun, based on parallax measurements, and is drifting further away with a radial velocity of 4.8 km/s. Nu Ceti is believed to be part of the Ursa Major stream of co-moving stars. In Chinese, 天囷 (Tiān Qūn), meaning Circular Celestial Granary, refers to an asterism consisting of α Ceti, κ1 Ceti, λ Ceti, μ Ceti, ξ1 Ceti, ξ2 Ceti, ν Ceti, γ Ceti, δ Ceti, 75 Ceti, 70 Ceti, 63 Ceti and 66 Ceti. Consequently, the Chinese name for ν Ceti itself is "the Seventh Star of Circular Celestial Granary", Tiān Qūn Qī. The primary, designated component A, forms a single-lined spectroscopic binary with an orbital period of 1.96 years and an eccentricity of 0.27. The visible component is a G-type giant star, currently on the horizontal branch, with a stellar classification of G8III. In addition to the spectroscopic companion there is a visual companion star which shares a common proper motion with Nu Ceti A, designated component B; an F-type main-sequence star with a class of F7V and a 9.08 apparent visual magnitude located 8.0 arcsec away. It was discovered by Struve.
References
External links http://server3.wikisky.org/starview?object_type=1&object_id=1566 http://www.alcyone.de/SIT/bsc/HR0754.html


