Omicron Hydrae

Blue-hued star in the constellation Hydra From Wikipedia, the free encyclopedia

Omicron Hydrae (ο Hya) is the Bayer designation for a solitary[11] star in the equatorial constellation Hydra. At one time it bore the Flamsteed designation 25 Crateris, but this is no longer used by astronomers so as to avoid confusion.[12] With an apparent visual magnitude of 4.70,[3] this star is visible to the naked eye. Based upon an annual parallax shift of 7.27 mas,[2] it is located around 449 light years from the Sun.

Right ascension11h 40m 12.78970s[2]
Declination−34° 44 40.7733[2]
Quick facts Constellation, Right ascension ...
Omicron Hydrae
Location of ο Hydrae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Hydra[1]
Right ascension 11h 40m 12.78970s[2]
Declination −34° 44 40.7733[2]
Apparent magnitude (V) 4.70[3]
Characteristics
Spectral type B9 V[4]
U−B color index −0.20[3]
B−V color index −0.08[3]
Astrometry
Radial velocity (Rv)+5.9[5] km/s
Proper motion (μ) RA: −43.24[2] mas/yr
Dec.: −1.61[2] mas/yr
Parallax (π)7.27±0.16 mas[2]
Distance449 ± 10 ly
(138 ± 3 pc)
Absolute magnitude (MV)−0.99[1]
Details
Mass3.56±0.04[6] M
Radius5.5[7] R
Luminosity309[6] L
Surface gravity (log g)2.87[8] cgs
Temperature10,495[6] K
Rotation27.2 days[8]
Rotational velocity (v sin i)160[6] km/s
Age252[9] Myr
Other designations
ο Hya, CD−34°7610, FK5 439, HD 101431, HIP 56922, HR 4494, SAO 202695[10]
Database references
SIMBADdata
Close

This is a B-type main sequence star with a stellar classification of B9 V.[4] It has completed an estimated 98.4%±1.1% of its lifetime on the main sequence. With 3.56[6] times the mass of the Sun, it radiates 309 times the Sun's luminosity from its outer atmosphere at an effective temperature of 10,495 K.[6] The rate of spin is relatively high, with a projected rotational velocity of 160 km/s.[6]

References

Related Articles

Wikiwand AI