Delta Columbae

Binary star system in the constellation Columba From Wikipedia, the free encyclopedia

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.[3] The distance to this system, based upon an annual parallax shift of 13.94 mas,[2] is around 234 lightyears.

Right ascension06h 22m 06.82831s[2]
Declination−33° 26 11.0323[2]
Quick facts Constellation, Right ascension ...
δ Columbae
Location of δ Columbae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba[1]
Right ascension 06h 22m 06.82831s[2]
Declination −33° 26 11.0323[2]
Apparent magnitude (V) 3.85[3]
Characteristics
Spectral type G7 II[4]
U−B color index +0.52[3]
B−V color index +0.88[3]
Astrometry
Proper motion (μ) RA: −24.23[2] mas/yr
Dec.: −51.40[2] mas/yr
Parallax (π)13.94±0.51 mas[2]
Distance234 ± 9 ly
(72 ± 3 pc)
Absolute magnitude (MV)−0.32[5]
Orbit[6][7]
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[8] L
Surface gravity (log g)2.49[9] cgs
Temperature5,136[5] K
Metallicity [Fe/H]−0.04[9] dex
Rotational velocity (v sin i)4.8±0.2[5] km/s
Other designations
δ Col, CD−33°2927, HD 44762, HIP 30277, HR 2296, SAO 196735.[10]
Database references
SIMBADdata
Close

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.[11]

This is a single-lined spectroscopic binary system with an orbital period of 868.78 days and an eccentricity of 0.7.[6] 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.[4] It radiates around 149[8] time the solar luminosity from its outer atmosphere at an effective temperature of 5,136 K.[5]

References

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