Nu1 Columbae

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ν1 Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.14[2]
Characteristics
Spectral type F0 IV[3]
B−V Template:Engvar +0.34[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: +18.24[1] mas/yr
Dec.: −57.61[1] mas/yr
Parallax (π)25.40±1.07 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+3.18[5]
Details
Mass1.41[6] Template:Solar mass
Luminosity4.3[7] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[6] cgs
TemperatureScript error: No such module "val".[6] K
Metallicity [Fe/H]−0.22[4] dex
Rotational velocity (v sin i)161[8] km/s
Age641[6] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
ν1 Col, CD−27°2389, HD 37430, HIP 26412, HR 1926, SAO 170601[9]
Database references
SIMBADdata

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Nu1 Columbae, Latinized from ν1 Columbae, is a star in the southern constellation of Columba. It is visible to the naked eye, having an apparent visual magnitude of 6.14. According to the Bortle scale, stars with this magnitude are faintly visible from dark rural skies. Based upon an annual parallax shift of 25.40 mas, this star is about 128 light years distant from the Sun.

This star has a stellar classification of F0 IV,[8] which indicates it is an evolving F-type subgiant star. It is an estimated 6410 million years of age, with a mass 1.41 times that of the Sun.[6] The star is spinning relatively rapidly, with a projected rotational velocity of 161 km/s.[8] It is radiating around 4.3[7] times the solar luminosity from its outer atmosphere at an effective temperature of 7,079 K.[6]

References

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Template:Stars of Columba