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HR 3159

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Star in the constellation Carina This article is about D Carinae. For d Carinae, see V343 Carinae.
HR 3159
Observation data
Epoch J2000.00      Equinox J2000.00
Constellation Carina
Right ascension 08 00 19.96678
Declination −63° 34′ 02.8420″
Apparent magnitude (V) 4.81
Characteristics
Spectral type B4V
B−V color index −0.173±0.007
Astrometry
Radial velocity (Rv)+22.1±2.8 km/s
Proper motion (μ) RA: −1.89 mas/yr
Dec.: 19.21 mas/yr
Parallax (π)6.53 ± 0.13 mas
Distance499 ± 10 ly
(153 ± 3 pc)
Absolute magnitude (MV)−1.11
Details
Mass6.3±0.1 M
Radius3.77±0.27 R
Luminosity912 L
Surface gravity (log g)4.03±0.05 cgs
Temperature16,983 K
Metallicity −0.09±0.06 dex
Rotational velocity (v sin i)43 km/s
Age17.2±1.3 or 176 Myr
Other designations
D Car, CD−63°866, FK5 2624, GC 10893, HD 66591, HIP 39138, HR 3159, SAO 250069
Database references
SIMBADdata

HR 3159 is a single star in the southern constellation of Carina, positioned near the southern constellation border with Volans. It has the Bayer designation D Carinae; HR 3159 is the Bright Star Catalogue designation. This object has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +4.81. It is located at a distance of approximately 499 light years from the Sun based on parallax, and is drifting further away with a radial velocity of 22 km/s.

This object is a B-type main-sequence star with a stellar classification of B4V, which indicates it is undergoing core hydrogen fusion. The star has a radius of nearly four times the radius of the Sun, and over six times the Sun's mass. Age estimates range from 17 up to 176 million years old, and it is spinning with a projected rotational velocity of 43 km/s. It is radiating 912 times the luminosity of the Sun from its photosphere at an effective temperature of 16,983 K.

References

  1. ^ van Leeuwen, F. (November 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. ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
  3. ^ Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1975mcts.book.....H.
  4. ^ Tetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
  5. ^ Fitzpatrick, E. L.; Massa, D. (March 2005), "Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry", The Astronomical Journal, 129 (3): 1642–1662, arXiv:astro-ph/0412542, Bibcode:2005AJ....129.1642F, doi:10.1086/427855, S2CID 119512018.
  6. ^ Balona, L. A.; et al. (May 2019), "Rotational modulation in TESS B stars", Monthly Notices of the Royal Astronomical Society, 485 (3): 3457–3469, arXiv:1902.09470, Bibcode:2019MNRAS.485.3457B, doi:10.1093/mnras/stz586.
  7. Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass", The Astrophysical Journal, 826 (2): 171, arXiv:1604.07403, Bibcode:2016ApJ...826..171G, doi:10.3847/0004-637X/826/2/171, S2CID 119241004.
  8. ^ Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters, 38 (11): 694–706, arXiv:1606.09028, Bibcode:2012AstL...38..694G, doi:10.1134/S1063773712110035, S2CID 119108982.
  9. "HD 66591". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-04.
  10. Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
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