Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Vela |
Right ascension | 08h 56m 19.2615s[1] |
Declination | −52° 43′ 24.5059″[1] |
Apparent magnitude (V) | 4.70 |
Characteristics | |
Spectral type | B5V + B9.5V[2] |
Astrometry | |
A | |
Proper motion (μ) | RA: −15.386±0.588[1] mas/yr Dec.: 14.468±0.524[1] mas/yr |
Parallax (π) | 8.5823 ± 0.3177 mas[1] |
Distance | 380 ± 10 ly (117 ± 4 pc) |
B | |
Proper motion (μ) | RA: −17.787±0.271[3] mas/yr Dec.: 12.031±0.250[3] mas/yr |
Parallax (π) | 8.1722 ± 0.1358 mas[3] |
Distance | 399 ± 7 ly (122 ± 2 pc) |
Orbit | |
Primary | Aa |
Companion | Ab |
Period (P) | 1.097654 |
Eccentricity (e) | 0 |
Semi-amplitude (K1) (primary) | 48.7 km/s |
Semi-amplitude (K2) (secondary) | 92.8 km/s |
Details | |
Aa | |
Mass | 4.14[4] M☉ |
Temperature | 16,000[2] K |
Rotational velocity (v sin i) | 50[2] km/s |
Ab | |
Mass | 0.59[4] M☉ |
Temperature | 9,500[2] K |
B | |
Mass | 1.55[4] M☉ |
Temperature | 8,871[3] K |
Other designations | |
Database references | |
SIMBAD | data |
H Velorum is a triple star system in the constellation Vela, at a distance of approximately 390 light years.
A visual pair of stars with magnitudes 4.7 and 8.0 are separated by 2.7″. Their estimated orbital period is 646,000 years. The primary is a spectroscopic binary with two B-class main sequence stars in a 1.1-day orbit.[2]
Gaia DR2
was invoked but never defined (see the help page).Veramendi2014
was invoked but never defined (see the help page).Gaia DR2b
was invoked but never defined (see the help page).msc
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).