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Nu2 Columbae

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Star in the constellation Columba For other stars with this Bayer designation, see ν Columbae.
ν Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 05 37 44.61799
Declination −28° 41′ 22.8863″
Apparent magnitude (V) 5.31
Characteristics
Spectral type F5 V
U−B color index +0.10
B−V color index +0.46
Astrometry
Radial velocity (Rv)+38.0±2.6 km/s
Proper motion (μ) RA: −37.66 mas/yr
Dec.: +42.42 mas/yr
Parallax (π)24.51 ± 0.29 mas
Distance133 ± 2 ly
(40.8 ± 0.5 pc)
Absolute magnitude (MV)+2.21
Details
Mass1.65 M
Radius1.6 R
Luminosity10 L
Surface gravity (log g)3.91 cgs
Temperature6,473±80 K
Metallicity −0.11±0.15 dex
Rotational velocity (v sin i)27.2 km/s
Age1.8 Gyr
Other designations
ν Col, CD−28° 2321, HD 37495, HIP 26460, HR 1935, SAO 170613.
Database references
SIMBADdata

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

This star has a stellar classification of F5 V, 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 and 1.6 times the Sun's radius. X-ray emission has been detected from this star, with an estimated luminosity of 1.6×10 erg/s. It is about 1.8 billion years old and is spinning with a projected rotational velocity of 27.2 km/s. The star is radiating about 10 times the solar luminosity from its outer atmosphere at an effective temperature of 6,473 K.

References

  1. ^ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. ^ Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99): 99, Bibcode:1966CoLPL...4...99J.
  3. ^ Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode:1982mcts.book.....H.
  4. ^ Casagrande, L.; et al. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics, 530 (A138): 21, arXiv:1103.4651, Bibcode:2011A&A...530A.138C, doi:10.1051/0004-6361/201016276, S2CID 56118016.
  5. ^ Pizzolato, N.; et al. (September 2000), "Evolution of X-ray activity of 1-3 Msun late-type stars in early post-main-sequence phases", Astronomy and Astrophysics, 361: 614–628, Bibcode:2000A&A...361..614P.
  6. ^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics, 367 (2): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
  7. ^ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966.2012.21873.x, S2CID 118665352.
  8. ^ Schröder, C.; Reiners, Ansgar; Schmitt, Jürgen H. M. M. (January 2009), "Ca II HK emission in rapidly rotating stars. Evidence for an onset of the solar-type dynamo" (PDF), Astronomy and Astrophysics, 493 (3): 1099–1107, Bibcode:2009A&A...493.1099S, doi:10.1051/0004-6361:200810377
  9. Balachandran, Suchitra (May 1, 1990), "Lithium depletion and rotation in main-sequence stars", Astrophysical Journal, Part 1, 354: 310–332, Bibcode:1990ApJ...354..310B, doi:10.1086/168691.
  10. "nu.02 Col -- Star", SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved 2016-12-30.
  11. Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
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