Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Vela |
δ Vel A | |
Right ascension | 08h 44m 42.226s[1] |
Declination | −54° 42′ 31.76″[1] |
Apparent magnitude (V) | 1.95 - 2.43[2] |
δ Vel B | |
Right ascension | 08h 44m 42.203s[1] |
Declination | −54° 42′ 30.60″ |
Apparent magnitude (V) | 5.54[3] |
Characteristics | |
U−B color index | +0.07[4] |
B−V color index | +0.04[4] |
δ Vel A | |
Spectral type | A1 Va(n)[5] |
Variable type | Algol[6] |
δ Vel B | |
Spectral type | F7.5V[7] |
Astrometry | |
Radial velocity (Rv) | +2.2[8] km/s |
Proper motion (μ) | RA: +28.99[9] mas/yr Dec.: −103.35[9] mas/yr |
Parallax (π) | 40.49 ± 0.39 mas[9] |
Distance | 80.6 ± 0.8 ly (24.7 ± 0.2 pc) |
Absolute magnitude (MV) | 0.02/3.60[10] |
Orbit[7] | |
Primary | δ Vel A |
Companion | δ Vel B |
Period (P) | 143.2 yr |
Semi-major axis (a) | 1.996″ |
Eccentricity (e) | 0.475 |
Inclination (i) | 105.1° |
Orbit[7] | |
Primary | δ Vel Aa |
Companion | δ Vel Ab |
Period (P) | 45.1503 days |
Semi-major axis (a) | 0.01651″ |
Eccentricity (e) | 0.287 |
Inclination (i) | 89.04° |
Details | |
δ Vel Aa | |
Mass | 2.43[7] M☉ |
Radius | 2.79–2.97[7] R☉ |
Luminosity | 67[7] L☉ |
Surface gravity (log g) | 3.78–3.90[7] cgs |
Temperature | 9,440[7] K |
Metallicity [Fe/H] | −0.33[7] dex |
Rotation | 1.05[7] days |
Rotational velocity (v sin i) | 143.5[7] km/s |
δ Vel Ab | |
Mass | 2.27[7] M☉ |
Radius | 2.37–2.52[7] R☉ |
Luminosity | 51[7] L☉ |
Surface gravity (log g) | 3.99–4.10[7] cgs |
Temperature | 9,830[7] K |
Metallicity [Fe/H] | −0.33[7] dex |
Rotational velocity (v sin i) | 149.6[7] km/s |
Age | 400 million[10] years |
δ Vel B | |
Mass | 1.35–1.46[7] M☉ |
Radius | 1.43[7] R☉ |
Luminosity | 3.5[7] L☉ |
Temperature | 6,600[7] K |
Other designations | |
Database references | |
SIMBAD | data |
Delta Velorum (δ Velorum, abbreviated Delta Vel, δ Vel) is a triple star system in the southern constellation of Vela, near the border with Carina, and is part of the False Cross. Based on parallax measurements, it is approximately 80.6 light-years (24.7 parsecs) from the Sun. It is one of the stars that at times lies near the south celestial pole due to precession.
δ Velorum consists of an eclipsing binary, designated Delta Velorum A, and a more distant third companion, Delta Velorum B. δ Velorum A's two components are themselves designated Aa (officially named Alsephina /ælsɪˈfaɪnə/, the traditional name for the entire system) and Ab.
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