Astronomy:Nu1 Columbae

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Short description: Star in the constellation Columba


ν1 Columbae
Observation data
Equinox J2000.0]] (ICRS)
Constellation Columba[1]
Right ascension  05h 37m 16.5030s[2]
Declination −27° 52′ 17.235″[2]
Apparent magnitude (V) 6.14[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type F0 IV[5]
B−V color index +0.34[3]
Astrometry
Radial velocity (Rv)26.7±2.0[6] km/s
Proper motion (μ) RA: −3.738[2] mas/yr
Dec.: −32.790[2] mas/yr
Parallax (π)23.0790 ± 0.1619[2] mas
Distance141.3 ± 1.0 ly
(43.3 ± 0.3 pc)
Absolute magnitude (MV)+3.18[1]
Details
Mass1.41[7] M☉
Radius1.57[8] R☉
Luminosity5.4[8] L☉
Surface gravity (log g)4.01±0.14[7] cgs
Temperature7,079±241[7] K
Metallicity [Fe/H]−0.22[6] dex
Rotational velocity (v sin i)161[9] km/s
Age641[7] Myr
Other designations
ν1 Col, CD−27°2389, HD 37430, HIP 26412, HR 1926, SAO 170601[10]
Database references
SIMBADdata

Nu1 Columbae is a star in the southern constellation of Columba. Its name is a Bayer designation that is Latinized from ν1 Columbae, and abbreviated Nu1 Col or ν1 Col. This star is visible to the naked eye, having an apparent visual magnitude of 6.14.[3] According to the Bortle scale, stars with this magnitude are faintly visible from dark rural skies. Based upon an annual parallax shift of 23.08 mas,[2] this star is about 128 light years distant from the Sun.

This star has a stellar classification of F0 IV,[9] suggesting it is an evolving F-type subgiant star. However, models indicate that it is a main sequence star with an estimated age of 641 million years and a mass 1.41 times that of the Sun.[7] The star is spinning relatively rapidly, with a projected rotational velocity of 161 km/s.[9] It is radiating around 5.4 times the solar luminosity[8] from its outer atmosphere at an effective temperature of 7,079 K.[7]

There is a faint star 2.6″ away with a similar parallax,[11] but it is not mentioned in any of the standard catalogues of multiple stars.

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 3.2 Nicolet, B. (1975), "Catalogue of Measurements in the Cape UBV Photometry on Magnetic Tape", Astronomy and Astrophysics Supplement Series 22: 239, Bibcode: 1975A&AS...22..239N. 
  4. ↑ Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics 537: A120. doi:10.1051/0004-6361/201117691. Bibcode: 2012A&A...537A.120Z. 
  5. ↑ Houk, N. (1982), Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0, Bibcode: 1982mcts.book.....H. 
  6. ↑ 6.0 6.1 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, doi:10.1051/0004-6361/201016276, Bibcode: 2011A&A...530A.138C. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 7.5 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal 804 (2): 146, doi:10.1088/0004-637X/804/2/146, Bibcode: 2015ApJ...804..146D. 
  8. ↑ 8.0 8.1 8.2 Stassun, Keivan G. et al. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal 158 (4): 138. doi:10.3847/1538-3881/ab3467. Bibcode: 2019AJ....158..138S. 
  9. ↑ 9.0 9.1 9.2 Royer, F. et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode: 2007A&A...463..671R. 
  10. ↑ "nu.01 Col". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=nu.01+Col. 
  11. ↑ Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.