Lambda Ceti

Lambda Ceti
Location of Lambda Ceti (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cetus
Right ascension 02h 59m 42.893s
Declination +08° 54′ 26.589″
Apparent magnitude (V) 4.71
Characteristics
Spectral type B6III
U−B color index −0.471
B−V color index −0.109±0.006
Astrometry
Radial velocity (Rv)10.2±2.8 km/s
Proper motion (μ) RA: 8.382 mas/yr
Dec.: −16.385 mas/yr
Parallax (π)7.3207±0.1451 mas
Distance446 ± 9 ly
(137 ± 3 pc)
Absolute magnitude (MV)−1.52
Details
Mass5.01±0.05 M
Radius5.4 R
Luminosity652 L
Temperature13,940±710 K
Rotational velocity (v sin i)131 km/s
Age100-125 Myr
Other designations
Menkar, λ Cet, 91 Cet, BD+08°455, FK5 1083, HD 18604, HIP 13954, HR 896, SAO 110889
Database references
SIMBADdata

Lambda Ceti is a star in the equatorial constellation of Cetus. Its name is a Bayer designation that is Latinized from λ Ceti, and abbreviated Lambda Cet or λ Cet. Historically, the star bore the traditional name Menkar, although today that name is more commonly associated with α Ceti. With an apparent visual magnitude of 4.71, it is faintly visible to the naked eye. Based on parallax measurement of 7.32 mas as seen from Earth, it is located at a distance of approximately 446 light-years (137 pc) from the Sun. The star is drifting further away with a line of sight velocity component of 10 km/s.

This star, along with α Cet (Menkar), γ Cet (Kaffaljidhma), δ Cet, μ Cet, ξ1 Cet and ξ2 Cet were Al Kaff al Jidhmah, "the Part of a Hand".

In Chinese, 天囷 (Tiān Qūn), meaning Circular Celestial Granary, refers to an asterism consisting of λ Ceti, α Ceti, κ1 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 λ Ceti itself is 天囷三 (Tiān Qūn sān, English: the Third Star of Circular Celestial Granary.)

Lambda Ceti is a blue giant star with stellar classification B6III. It is an estimated 100-125 million years old, and is spinning rapidly with a projected rotational velocity of 131 km/s. It has five times the mass of the Sun and 5.4 times the Sun's radius. The star is radiating 920 times the Sun's luminosity at an effective temperature of 13,940 K.