Omega Herculis

ω Herculis
Location of ω Herculis (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Hercules
Right ascension 16h 25m 24.95425s
Declination +14° 01′ 59.7711″
Apparent magnitude (V) 4.5821 (4.58 + 11.5)
Characteristics
Spectral type A2 Vp CrSr
U−B color index +0.01
B−V color index +0.00
Variable type α2 CVn
Astrometry
Radial velocity (Rv)−5.90±0.74 km/s
Proper motion (μ) RA: +40.86 mas/yr
Dec.: −59.71 mas/yr
Parallax (π)13.04±0.64 mas
Distance250 ± 10 ly
(77 ± 4 pc)
Absolute magnitude (MV)0.29±0.15
Details
ω Her A
Mass2.14 M
Radius3.30 R
Luminosity70 L
Surface gravity (log g)3.51±0.35 cgs
Temperature10,052±320 K
Metallicity [Fe/H]+0.47±0.15 dex
Rotation2.951 d
Rotational velocity (v sin i)55 km/s
Age149 Myr
Other designations
Cujam, ω Her, 24 Her, 51 Ser, BD+14°3049, FK5 613, HD 148112, HIP 80463, HR 6117, SAO 102153, WDS J16254+1402AB
Database references
SIMBADdata

Omega Herculis (ω Herculis, abbreviated Omega Her, ω Her) is a binary star system in the northern constellation of Hercules. Based upon an annual parallax shift of 13.04 mas as seen from Earth, it is located around 250 light-years from the Sun. It is faintly visible to the naked eye, having a combined apparent visual magnitude of 4.58. The system is a candidate for membership in the Ursa Major Moving Group, although this remains uncertain.

The two components are designated Omega Herculis A (officially named Cujam /ˈkjuːəm/, the traditional name of the system) and B.