HD 83183

Last updated
HD 83183
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Carina
Right ascension 09h 34m 26.65081s [1]
Declination −59° 13 47.1070 [1]
Apparent magnitude  (V)4.08 [2]
Characteristics
Spectral type B5 II [3]
B−V color index −0.013±0.003 [2]
Astrometry
Radial velocity (Rv)+18.2±0.6 [2]  km/s
Proper motion (μ)RA: −10.74 [1]   mas/yr
Dec.: +6.60 [1]   mas/yr
Parallax (π)2.46 ± 0.10  mas [1]
Distance 1,330 ± 50  ly
(410 ± 20  pc)
Absolute magnitude  (MV)−3.96 [2]
Details
Mass 9.4±0.5 [4]   M
Radius 18 [5]   R
Luminosity 11,634 [6]   L
Surface gravity (log g)2.50 [7]   cgs
Temperature 14,300 [6]   K
Rotational velocity (v sin i)19±4 [7]  km/s
Age 24.5±3.8 [4]   Myr
Other designations
h Car, CPD−58°1576, GC  13246, HD  83183, HIP  46974, HR  3825, SAO  237117 [8]
Database references
SIMBAD data

HD 83183 is a single [9] star in the southern constellation of Carina. It has the Bayer designation h Carinae, while HD 83183 is the star's identifier from the Henry Draper catalogue . The star is blue-white in hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.08. [2] It is located at a distance of approximately 1,330  light years based on parallax, [1] and is drifting further away with a radial velocity of +18 km/s. [2] O. J. Eggen identified it as a member of the Pleiades group of co-moving stars. [10]

This object is a massive bright giant star with a stellar classification of B5 II. [3] It is 25 [4]  million years old and is spinning with a projected rotational velocity of 19 km/s. [7] The star has 9 [4] times the mass of the Sun and about 18 [5] times the Sun's radius. It is radiating 11,634 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 14,300 K. [6]

Related Research Articles

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Upsilon2 Centauri is a binary star system in the southern constellation Centaurus. It is visible to the naked eye with an apparent visual magnitude of +4.33. Based upon an annual parallax shift of just 2.57 mas as seen from Earth, this star is located roughly 1,300 light years from the Sun. Relative to its neighbors, the system has a peculiar velocity of 39.2+8.8
−15.2
 km/s
and it may form a runaway star system.

<span class="mw-page-title-main">2 Centauri</span> Star in the constellation Centaurus

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<span class="mw-page-title-main">7 Ceti</span> Star in the constellation Cetus

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−6.2
 km/s
and is a candidate runaway star.

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<span class="mw-page-title-main">V1073 Scorpii</span> Variable star in the constellation Scorpius

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HD 85622 is a binary star system in the southern constellation of Vela. It is visible to the naked eye with an apparent visual magnitude of 4.58. The distance to HD 85622 can be estimated from its annual parallax shift of 4.3 mas, yielding a value of 750 light years. It is moving further from the Earth with a heliocentric radial velocity of +8 km/s.

<span class="mw-page-title-main">GX Velorum</span> Star in the constellation Vela

GX Velorum is a solitary variable star in the southern constellation of Vela. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude that fluctuates around 4.99. Based upon parallax measurements, it is located approximately 4,200 light years distant from the Sun, and is drifting further away with a radial velocity of +28 km/s. It may be a member of the Vela OB1 association of co-moving stars.

<span class="mw-page-title-main">HD 25291</span> Star in the constellation Camelopardalis

HD 25291, also known as HR 1242, is a solitary, yellowish-white hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.12, making it one of the brighter members of this generally faint constellation. The object is relatively far at a distant of approximately 2,100 light years but is drifting closer with a heliocentric radial velocity of −20.3 km/s.

References

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  8. "HD 83183". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-01-26.
  9. 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.
  10. Eggen, O. J. (February 1974), "NGC 2287 and the Pleiades group", Astrophysical Journal, 188: 59–70, Bibcode:1974ApJ...188...59E, doi: 10.1086/152685 .