Sigma Ophiuchi

σ Ophiuchi
Location of σ Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 17h 26m 30.8806s
Declination +04° 08 25.2876
Apparent magnitude (V) 4.31 (4.25 - 4.51)
Characteristics
Spectral type K2 III
U−B color index +1.57
B−V color index +1.51
Variable type suspected
Astrometry
Radial velocity (Rv)−27.81 km/s
Proper motion (μ) RA: +1.459 mas/yr
Dec.: +6.760 mas/yr
Parallax (π)3.7578±0.1559 mas
Distance870 ± 40 ly
(270 ± 10 pc)
Absolute magnitude (MV)−2.85
Details
Mass5–9 M
Radius100±30 R
Luminosity2630±894 L
Surface gravity (log g)1.3±0.5 cgs
Temperature4,129±566 K
Metallicity [Fe/H]−0.07 dex
Rotational velocity (v sin i)4.2 km/s
Other designations
σ Oph, 49 Ophiuchi, NSV 8664, BD+04°3422, FK5 1459, GC 23621, HD 157999, HIP 85355, HR 6498, SAO 122387, 2MASS J17263087+0408252
Database references
SIMBADdata

Sigma Ophiuchi, Latinized from σ Ophiuchi, is a single, orange-hued star in the equatorial constellation Ophiuchus. Its apparent visual magnitude is 4.31, which is bright enough to be faintly visible to the naked eye. The annual parallax shift of 3.62 mas as seen from Earth provides a distance estimate of roughly 900 light years. It is moving closer to the Sun with a radial velocity of −28 km/s.

This is an evolved giant star of type K with a stellar classification of K2 III. Wittkowski et al. (2017) consider it to have a luminosity class of II-III, suggesting it is in a transitional zone between giants and supergiant stars. It has around 5 to 9 times the mass of the Sun and one hundred times the Sun's radius. The star is radiating 2,600 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,130 K.