Nu2 Columbae is a solitary star[11] in the southern constellation of Columba. It can be seen with the naked eye, having an apparent visual magnitude of 5.31.[2] With an annual parallax shift of 24.51 mas,[1] it is estimated to lie about 133 light years from the Sun.

Quick Facts Constellation, Right ascension ...
ν2 Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 05h 37m 44.61799s[1]
Declination −28° 41 22.8863[1]
Apparent magnitude (V) 5.31[2]
Characteristics
Spectral type F5 V[3]
U−B color index +0.10[2]
B−V color index +0.46[2]
Astrometry
Radial velocity (Rv)+38.0±2.6[4] km/s
Proper motion (μ) RA: −37.66[1] mas/yr
Dec.: +42.42[1] mas/yr
Parallax (π)24.51 ± 0.29 mas[1]
Distance133 ± 2 ly
(40.8 ± 0.5 pc)
Absolute magnitude (MV)+2.21[5]
Details
Mass1.65[4] M
Radius1.6[6] R
Luminosity10[7] L
Surface gravity (log g)3.91[8] cgs
Temperature6,473±80[4] K
Metallicity [Fe/H]−0.11±0.15[9] dex
Rotational velocity (v sin i)27.2[8] km/s
Age1.8[4] Gyr
Other designations
ν2 Col, CD−28° 2321, HD 37495, HIP 26460, HR 1935, SAO 170613.[10]
Database references
SIMBADdata
Close

This star has a stellar classification of F5 V,[3] indicating that it is an F-type main sequence star that is generating energy through the thermonuclear fusion of hydrogen into helium in its core region. It has about 1.65 times the mass of the Sun[4] and 1.6 times the Sun's radius.[6] X-ray emission has been detected from this star, with an estimated luminosity of 1.6×1029 erg/s.[5] It is about 1.8 billion years old[4] and is spinning with a projected rotational velocity of 27.2 km/s.[8] The star is radiating about 10 times the solar luminosity from its outer atmosphere[7] at an effective temperature of 6,473 K.[4]

References

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