GX Velorum

Star in the constellation Vela From Wikipedia, the free encyclopedia

GX Velorum is a solitary[12] variable star[3] 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.[2] 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.[6] It may be a member of the Vela OB1 association of co-moving stars.[7]

A light curve for GX Velorum, plotted from Hipparcos data[13]
Right ascension09h 11m 04.39802s[1]
Declination−44° 52 04.4411[1]
Apparentmagnitude(V)+4.99[2] (4.97 to 5.04)[3]
Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
GX Velorum
Location of GX Velorum (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vela
Right ascension 09h 11m 04.39802s[1]
Declination −44° 52 04.4411[1]
Apparent magnitude (V) +4.99[2] (4.97 to 5.04)[3]
Characteristics
Spectral type B5 Ia[4]
U−B color index −0.57[5]
B−V color index +0.22[5]
Variable type α Cyg?[3]
Astrometry
Radial velocity (Rv)+28.2±0.8[6] km/s
Proper motion (μ) RA: −5.608[1] mas/yr
Dec.: +3.843[1] mas/yr
Parallax (π)0.7696±0.1585 mas[1]
Distanceapprox. 4,200 ly
(approx. 1,300 pc)
Absolute magnitude (MV)−7.20[7]
Details[8]
Mass35 M
Radius61±7[9] R
Luminosity214,000[9] L
Surface gravity (log g)2.12±0.05[9] cgs
Temperature15,000±150[9] K
Rotational velocity (v sin i)39 km/s
Age8.3[10] Myr
Other designations
GX Vel, CD−44°5206, HD 79186, HIP 45085, HR 3654, SAO 220928[11]
Database references
SIMBADdata
Close

This object is a massive blue supergiant with a stellar classification of B5 Ia.[4] It is suspected to be an Alpha Cygni-type pulsating variable and ranges in brightness from 4.97 down to 5.04 magnitude.[3] It is losing mass at the rate of (0.40±0.02)×10−6 M yr−1,[9] or one solar mass every 2.5 million years. The star is 8.3[10] million years old with 35 times the mass of the Sun.[8] It has expanded to around 61[9] times the Sun's radius and is radiating 214,000[9] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 15,000 K.[9]

References

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