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Star in the constellation Columba From Wikipedia, the free encyclopedia
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.
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] |
Distance | 133 ± 2 ly (40.8 ± 0.5 pc) |
Absolute magnitude (MV) | +2.21[5] |
Details | |
Mass | 1.65[4] M☉ |
Radius | 1.6[6] R☉ |
Luminosity | 10[7] L☉ |
Surface gravity (log g) | 3.91[8] cgs |
Temperature | 6,473±80[4] K |
Metallicity [Fe/H] | −0.11±0.15[9] dex |
Rotational velocity (v sin i) | 27.2[8] km/s |
Age | 1.8[4] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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]
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