HD 70930

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HD 70930
Observation data
Epoch J2000      Equinox J2000
Constellation Vela[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 4.79[1] (5.14 + 6.08)[3]
Characteristics
Spectral type B1V[4] or B2III[5]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: Script error: No such module "val".[2] mas/yr
Dec.: Script error: No such module "val".[2] mas/yr
Parallax (π)1.90±0.32 mas[2]
Distanceapprox. Template:Rnd ly
(approx. Template:Rnd pc)
Absolute magnitude (MV)−3.74[1]
Details
MassScript error: No such module "val".[4] Template:Solar mass
Radius13.6[6] Template:Solar radius
Luminosity20,893[7] Template:Solar luminosity
Surface gravity (log g)2.74[6] cgs
Temperature23,532[7] K
Rotational velocity (v sin i)220[7] km/s
AgeScript error: No such module "val".[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 70930 is a binary star[9] 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,[1] 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,[2] and it has an absolute magnitude of −3.74.[1] It is drifting further away from the Sun with a radial velocity of about +27 km/s.[1] The system is a member of the Vel OB2 association of co-moving stars.[10]

The double nature of this system was discovered in 1896 by Scottish astronomer Robert T. A. Innes[3] – it is now known to be a double-lined spectroscopic binary.[11] The magnitude 5.14[3] primary component has a blue-white hue and has been assigned stellar classifications of B1V[4] and B2III,[5] 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.[4] The star has a high rate of spin, showing a projected rotational velocity of 220 km/s.[7] Its companion, at magnitude +6.08, is located at an angular separation of Script error: No such module "val". along a position angle of 139°, as of 2008.[3]

References

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  1. a b c d e f g h Template:Cite XHIP
  2. a b c d e f Script error: No such module "Citation/CS1". Vizier catalog entry
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Template:Stars of Vela