HR 3159

Last updated
HR 3159
Observation data
Epoch J2000.00       Equinox J2000.00
Constellation Carina [1]
Right ascension 08h 00m 19.96579s [2]
Declination −63° 34′ 02.8274″ [2]
Apparent magnitude  (V)4.81 [1]
Characteristics
Evolutionary stage main sequence [2]
Spectral type B4V [3]
B−V color index −0.173±0.007 [1]
Astrometry
Radial velocity (Rv)+22.1±2.8 [1] km/s
Proper motion (μ)RA: −1.762 [2] mas/yr
Dec.: +19.905 [2] mas/yr
Parallax (π)6.9936±0.0826  mas [2]
Distance 466 ± 6  ly
(143 ± 2  pc)
Absolute magnitude  (MV)−1.11 [1]
Details
Mass 6.3±0.1 [4]   M☉
Radius 3.77±0.27 [5]   R☉
Luminosity 912 [6]   L☉
Surface gravity (log g)4.03±0.05 [5]   cgs
Temperature 16,983 [6]   K
Metallicity [Fe/H]−0.09±0.06 [7]   dex
Rotational velocity (v sin i)43 [6]  km/s
Age 17.2±1.3 [4] or 176 [8]   Myr
Other designations
D Car, CD−63°866, FK5 2624, GC 10893, HD 66591, HIP 39138, HR 3159, SAO 250069 [9]
Database references
SIMBAD data

HR 3159 is a single [10] 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. [1] It is located at a distance of approximately 466  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, [3] which indicates it is undergoing core hydrogen fusion. The star has a radius of nearly four times the radius of the Sun, [5] and over six [4] times the Sun's mass. Age estimates range from 17 [4] up to 176 [8]  million years old, and it is spinning with a projected rotational velocity of 43 km/s. [6] It is radiating 912 [6] times the luminosity of the Sun from its photosphere at an effective temperature of 16,983 K. [6]

References

  1. 1 2 3 4 5 6 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.
  2. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211 . Bibcode:2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940 . S2CID   244398875. Gaia DR3 record for this source at VizieR .
  3. 1 2 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. 1 2 3 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. 1 2 3 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. 1 2 3 4 5 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. 1 2 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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