Delta Columbae

δ Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 06h 22m 06.82831s
Declination −33° 26 11.0323
Apparent magnitude (V) 3.85
Characteristics
Spectral type G7 II
U−B color index +0.52
B−V color index +0.88
Astrometry
Proper motion (μ) RA: −24.23 mas/yr
Dec.: −51.40 mas/yr
Parallax (π)13.94±0.51 mas
Distance234 ± 9 ly
(72 ± 3 pc)
Absolute magnitude (MV)−0.32
Orbit
Period (P)868.78 d
Semi-major axis (a)9.02±0.52 mas
Eccentricity (e)0.7
Inclination (i)116.3±4.2°
Periastron epoch (T)2419915.02 JD
Argument of periastron (ω)
(secondary)
117.1°
Semi-amplitude (K1)
(primary)
10.6 km/s
Details
δ Col A
Luminosity149.5 L
Surface gravity (log g)2.49 cgs
Temperature5,136 K
Metallicity [Fe/H]−0.04 dex
Rotational velocity (v sin i)4.8±0.2 km/s
Other designations
δ Col, CD−33°2927, HD 44762, HIP 30277, HR 2296, SAO 196735.
Database references
SIMBADdata

Delta Columbae is a binary star system in the constellation Columba. It can be seen with the naked eye having an apparent visual magnitude of 3.85. The distance to this system, based upon an annual parallax shift of 13.94 mas, is around 234 lightyears.

Delta Columbae was a latter designation of 3 Canis Majoris, as the early astronomers Johann Bayer and John Flamsteed did not include the constellation Columba in their star charts.

This is a single-lined spectroscopic binary system with an orbital period of 868.78 days and an eccentricity of 0.7. It has a peculiar velocity of 30.2±3.9 km/s, making it a candidate runaway star system. The primary component is a G-type bright giant star with a stellar classification of G7 II. It radiates around 149 time the solar luminosity from its outer atmosphere at an effective temperature of 5,136 K.