Omega Hydrae

Omega Hydrae, Latinised from ω Hydrae, is a golden-hued star in the equatorial constellation of Hydra, located to the west-southwest of the brighter star Zeta Hydrae. Based upon an annual parallax shift of just 3.64 mas as seen from Earth, it is located roughly 900 light-years from the Sun. It is faintly visible to the naked eye with an apparent visual magnitude of 5.00.

Omega Hydrae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Hydra
Right ascension 09h 05m 58.36642s
Declination +05° 05 32.3360
Apparent magnitude (V) 5.00
Characteristics
Spectral type K2 II-III
U−B color index +1.22
B−V color index +1.22
Astrometry
Radial velocity (Rv)+24.3±0.8 km/s
Proper motion (μ) RA: −19.58 mas/yr
Dec.: −11.07 mas/yr
Parallax (π)3.64 ± 0.31 mas
Distance900 ± 80 ly
(270 ± 20 pc)
Absolute magnitude (MV)−2.19
Details
Mass4.32±0.37 M
Radius48.49±5.55 R
Luminosity944.3±178.3 L
Surface gravity (log g)1.74±0.12 cgs
Temperature4,789 K
Metallicity [Fe/H]−0.12±0.10 dex
Rotational velocity (v sin i)2.3 km/s
Age180±70 Myr
Other designations
ω Lyr, 18 Hydrae, BD+05°2116, HD 77996, HIP 44659, HR 3613, SAO 117420
Database references
SIMBADdata

This is an evolved K-type star with a stellar classification of K2 II-III, which indicates a spectrum showing traits intermediate between the giant and bright giant stages. It is most likely (98% chance) on the horizontal branch, indicating that the star is generating energy through the thermonuclear fusion of helium at its core. With 4.32 times the Sun's mass, it has expanded to around 48 times the radius of the Sun. Omega Hydrae is about 180 million years old and spinning with a leisurely projected rotational velocity of 2.3 km/s. The star is radiating roughly 944 times the solar luminosity from its photosphere at an effective temperature of 4,789 K.

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