32 Ophiuchi

32 Ophiuchi
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h 03m 07.87110s
Declination +14° 05 31.0140
Apparent magnitude (V) 4.97
Characteristics
Evolutionary stage asymptotic giant branch
Spectral type M3−III
B−V color index 1.600±0.007
Variable type suspected
Astrometry
Radial velocity (Rv)+43.15±0.15 km/s
Proper motion (μ) RA: +25.226 mas/yr
Dec.: −62.651 mas/yr
Parallax (π)8.0197±0.1498 mas
Distance407 ± 8 ly
(125 ± 2 pc)
Absolute magnitude (MV)−0.44
Details
Mass1.60+1.38
−0.75
 M
Radius63.6±1.2 R
Luminosity1,148+111
−193
 L
Surface gravity (log g)1.90 cgs
Temperature3,728±122 K
Metallicity [Fe/H]−0.07 dex
Other designations
32 Oph, NSV 8142, BD+14°3179, HD 154143, HIP 83430, HR 6337, SAO 102553
Database references
SIMBADdata

32 Ophiuchi is a single star located about 407 light years away from the Sun in the constellation Hercules. It is moving further away from the Sun with a heliocentric radial velocity of +43 km/s. and is visible to the naked eye as a dim, red-hued star with an apparent visual magnitude of 4.97.

This is an aging red giant star on the asymptotic giant branch with a stellar classification of M3−III. Having exhausted the supply of hydrogen at its core it has expanded to 63 times the radius of the Sun. The star is radiating over a thounsand times the luminosity of the Sun from its swollen photosphere at an effective temperature of around 3,728 K.

32 Ophiuchi is a suspected variable star with a brightness range of about 0.1 magnitudes.