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 4,200light years distant from the Sun, and is drifting further away with a radial velocity of +28km/s.[6] It may be a member of the Vela OB1 association of co-moving stars.[7]
This object is a massive blue supergiant with a stellar classification of B5Ia.[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)×10−6M☉ yr−1,[9] or one solar mass every 2.5million 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 15,000K.[9]
Houk, Nancy (1978). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol.2. Ann Arbor: Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
Fraser, M.; etal. (2010). "Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants". Monthly Notices of the Royal Astronomical Society. 404 (3): 1306. arXiv:1001.3337. Bibcode:2010MNRAS.404.1306F. doi:10.1111/j.1365-2966.2010.16392.x. S2CID118674151.
Haucke, M.; etal. (June 2018), "Wind properties of variable B supergiants. Evidence of pulsations connected with mass-loss episodes", Astronomy & Astrophysics, 614: 28, arXiv:1902.01341, Bibcode:2018A&A...614A..91H, doi:10.1051/0004-6361/201731678, A91
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