HD 72108

HD 72108
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vela
Right ascension 08h 29m 04.752s
Declination −47° 55 44.12
Apparent magnitude (V) +5.33
Characteristics
Spectral type B2IV + B2IV
Astrometry
Radial velocity (Rv)29.00±3.7 km/s
Proper motion (μ) RA: −6.90±0.43 mas/yr
Dec.: +7.12±0.34 mas/yr
Parallax (π)1.53±0.34 mas
Distanceapprox. 2,100 ly
(approx. 700 pc)
Absolute magnitude (MV)−1.06
Orbit
PrimaryHD 72018 Aa
CompanionHD 72018 Ab
Period (P)340±50 yr
Semi-major axis (a)0.427±0.030
Eccentricity (e)0.748±0.030
Inclination (i)78.9±2.0°
Longitude of the node (Ω)114.7±2.0°
Periastron epoch (T)1947.7±2.0
Argument of periastron (ω)
(secondary)
300.0±5.0°
Details
HD 72018 Aa
Mass6.08±3.43 M
HD 72018 Ab
Mass5.45±3.08 M
Other designations
HR 3358, CD−47°4004, HIP 41616, SAO 219985, WDS J08291-4756AB
Database references
SIMBADdata

HD 72108 (A Vel, A Velorum) is a star system in the constellation Vela. It is approximately 1640 light years from Earth.

The primary component, HD 72108 A, is a blue-white B-type subgiant with an apparent magnitude of +5.33. It is a spectroscopic binary, whose components are separated by 0.176 arcseconds. At a distance of 4 arcseconds away is the third component, the magnitude +7.7 HD 72108 B. The fourth component, HD 72108 C has an apparent magnitude of +9.3, and is 19 arcseconds from the primary.