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Kappa Columbae

κ Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 06h 16m 33.13512s
Declination −35° 08′ 25.8630″
Apparent magnitude (V) 4.37
Characteristics
Spectral type K0.5 IIIa
U−B color index +0.83
B−V color index +1.00
Variable type Suspected
Astrometry
Radial velocity (Rv) 24.20 km/s
Proper motion (μ) RA: −0.28 mas/yr
Dec.: +87.94 mas/yr
Parallax (π) 17.87 ± 0.16mas
Distance 183 ± 2 ly
(56.0 ± 0.5 pc)
Details
Mass 1.76 M
Radius 10.5 R
Luminosity 57.5 L
Surface gravity (log g) 2.59 cgs
Temperature 4,876±33 K
Metallicity [Fe/H] +0.11 dex
Age 1.68 Gyr
Other designations
κ Col, CD−35° 2800, FK5 238, HD 43785, HIP 29807, HR 2256, SAO 196643.
Database references
SIMBAD data

Kappa Columbae is a solitarystar in the southern constellation of Columba. It has an apparent visual magnitude of 4.37, which is bright enough to be seen with the naked eye. Based upon an annual parallax shift of 17.87 mas, it is located at a distance of 183 light years from the Sun. It has a peculiar velocity of 20.2±1.9 km/s, making it a candidate runaway star.

For ancient Arabian astronomers, this star, along with ζ CMa, λ CMa, γ Col, δ Col, θ Col, λ Col, μ Col and ξ Col, formed Al Ḳurūd (ألقرد - al-qird), the Apes. In Chinese, (Sūn), meaning Grandson, refers to an asterism consisting of κ Columbae and θ Columbae. Consequently, κ Columbae itself is known as 孫一 (Sūn yī, English: the First Star of Grandson.).

This is an evolved K-type giant star with a stellar classification of K0.5 IIIa. The measured angular diameter of this star, after correction for limb darkening, is 1.75±0.03 mas. At the estimated distance of this star, this yields a physical size of about 10.5 times the radius of the Sun. It has an estimated 1.76 times the mass of the Sun and is about 1.7 billion years old. The star radiates 57.5 times the solar luminosity from its outer atmosphere at an effective temperature of 4,876 K. It is catalogued as a suspected variable star.


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