Delta Velorum
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| Observation data Equinox J2000 |
|
|---|---|
| Constellation | Vela |
| Right ascension | 08h 44m 42.2s |
| Declination | −54° 42′ 30″ |
| Apparent magnitude (V) | 1.95 (2.03/5.1) |
| Characteristics | |
| Spectral type | A1 V/G0 V |
| U-B color index | 0.06 |
| B-V color index | 0.04 |
| Variable type | Eclipsing binary |
| Astrometry | |
| Radial velocity (Rv) | +2.2 km/s |
| Proper motion (μ) | RA: 28.78 mas/yr Dec.: −104.14 mas/yr |
| Parallax (π) | 40.90 ± 0.38 mas |
| Distance | 79.7 ± 0.7 ly (24.4 ± 0.2 pc) |
| Absolute magnitude (MV) | −0.01 (0.05/3.51) |
| Other designations | |
| Database references | |
| SIMBAD | data |
Delta Velorum (δ Vel / δ Velorum) is a star system in the constellation Vela. It is approximately 79.7 light years from Earth.
The system is composed of two binary stars. The brightest of the four stars, δ Velorum A, is a white A-type main sequence dwarf with an apparent magnitude of +2.02. Its binary companion, δ Velorum B, has a magnitude of +5.1 and is separated from the A component by 2.6 arcseconds.
The second binary system is 69 arcseconds away. It is composed of the 11th magnitude δ Velorum C and the 13th magnitude δ Velorum D, which are 6 arcseconds apart.
This star was recently discovered to be variable by the Galileo spaceprobe at Jupiter. [1] It fluctuates by about 30% every 45 days. Curiously, being one of the brighter stars in the sky, this had not been noticed previously.
Because of precession, δ Velorum will be the South Polar Star around 9000 AD.
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