HD 70930

HD 70930
Observation data
Epoch J2000      Equinox J2000
Constellation Vela
Right ascension 08h 22m 31.6941s
Declination −48° 29 25.3631
Apparent magnitude (V) 4.79 (5.14 + 6.08)
Characteristics
Spectral type B1V or B2III
B−V color index −0.146±0.002
Astrometry
Radial velocity (Rv)+27.0±4.5 km/s
Proper motion (μ) RA: −5.10±0.39 mas/yr
Dec.: +7.76±0.33 mas/yr
Parallax (π)1.90±0.32 mas
Distanceapprox. 1,700 ly
(approx. 530 pc)
Absolute magnitude (MV)−3.74
Details
Mass15.6±0.8 M
Radius13.6 R
Luminosity20,893 L
Surface gravity (log g)2.74 cgs
Temperature23,532 K
Rotational velocity (v sin i)220 km/s
Age10.0±0.1 Myr
Other designations
I 67, B Velorum, CD−48°3734, HD 70930, HIP 41039, HR 3294, SAO 219848, CCDM 08225-4829, WDS J08225-4829AB
Database references
SIMBADdata

HD 70930 is a binary star system in the southern constellation of Vela. It has the Bayer designation B Velorum, while HD 70930 is the star's identifier in the Henry Draper catalogue. With a combined apparent visual magnitude of 4.79, it is visible to the naked eye as a faint point of light. The distance to this system is approximately 1,700 light years based on parallax, and it has an absolute magnitude of −3.74. It is drifting further away from the Sun with a radial velocity of about +27 km/s. The system is a member of the Vel OB2 association of co-moving stars.

The double nature of this system was discovered in 1896 by Scottish astronomer Robert T. A. Innes – it is now known to be a double-lined spectroscopic binary. The magnitude 5.14 primary component has a blue-white hue and has been assigned stellar classifications of B1V and B2III, matching a B-type main-sequence star or a giant star, respectively. It is a massive object – over 15 times the mass of the Sun – and is around 10 million years old. The star has a high rate of spin, showing a projected rotational velocity of 220 km/s. Its companion, at magnitude +6.08, is located at an angular separation of 0.8 along a position angle of 139°, as of 2008.