HD 85622
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Vela |
| Right ascension | 09h 51m 40.66831s |
| Declination | −46° 32′ 51.4401″ |
| Apparent magnitude (V) | 4.58 |
| Characteristics | |
| Evolutionary stage | Supergiant |
| Spectral type | G5 Ib or G6 IIa |
| B−V color index | 1.20 |
| Astrometry | |
| Radial velocity (Rv) | 15.94±2.50 km/s |
| Proper motion (μ) | RA: −25.119 mas/yr Dec.: +10.305 mas/yr |
| Parallax (π) | 3.6857±0.1289 mas |
| Distance | 880 ± 30 ly (271 ± 9 pc) |
| Absolute magnitude (MV) | −2.96 |
| Orbit | |
| Period (P) | 329.266±0.085 d |
| Eccentricity (e) | 0 (adopted) |
| Periastron epoch (T) | 2453860.281±0.074 HJD |
| Semi-amplitude (K1) (primary) | 13.021±0.012 km/s |
| Details | |
| Mass | 6.2±0.5 M☉ |
| Radius | 62.6+2.5 −2.2 R☉ |
| Luminosity | 1,602+109 −93 L☉ |
| Surface gravity (log g) | 1.65 cgs |
| Temperature | 4,761 K |
| Rotational velocity (v sin i) | 19.3±1.0 km/s |
| Age | 63.7±15.8 Myr |
| Other designations | |
| m Vel, CD−45°5508, HD 85622, HIP 48374, HR 3912, SAO 221553 | |
| Database references | |
| SIMBAD | data |
HD 85622 is a binary star system in the southern constellation of Vela. It is visible to the naked eye with an apparent visual magnitude of 4.58. The distance to HD 85622, as measured from its annual parallax shift of 3.6857 mas, is 880 light years. It is moving further from the Earth with a heliocentric radial velocity of +8 km/s.
This is a single-lined spectroscopic binary with a circular orbit and a period of 329.3 days. The a sin i value is 0.39 AU, where a is the semimajor axis and i is the orbital inclination to the line of sight. This value provides a lower bound on the actual semimajor axis. The system shows a micro-variability in its brightness, and is a source of X-ray emission with an apparent flux of 42.6×10−17 W/m2.
The visible component is a supergiant star with a stellar classification of G5 Ib or G6 IIa. It is about 64 million years old with a projected rotational velocity of 19 km/s. The star has 6.2 times the mass of the Sun and is radiating 1,600 times the Sun's luminosity from its photosphere at an effective temperature of 4,761 K.