20 Ophiuchi

20 Ophiuchi is a class F6IV (yellow-white subgiant) star in the constellation Ophiuchus. Its apparent magnitude is 4.64 and it is approximately 104 light years away based on parallax. It lies near the star Zeta Ophiuchi.

20 Ophiuchi
Location of 20 Ophiuchi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 16h 49m 50.01604s
Declination −10° 46 58.7775
Apparent magnitude (V) 4.64
Characteristics
Spectral type F6IV
U−B color index +0.07
B−V color index +0.47
Astrometry
Radial velocity (Rv)-1.60 km/s
Proper motion (μ) RA: +72.33 mas/yr
Dec.: -78.80 mas/yr
Parallax (π)31.27 ± 2.16 mas
Distance104 ± 7 ly
(32 ± 2 pc)
Absolute magnitude (MV)2.13
Orbit
Period (P)35.5 ± 1.5 yr
Semi-major axis (a)0.460 ± 0.030″
Eccentricity (e)0.8 ± 0.2
Inclination (i)74 ± 11°
Longitude of the node (Ω)118 ± 9°
Periastron epoch (T)1981.2 ± 1.7
Argument of periastron (ω)
(secondary)
34 ± 26°
Details
20 Oph A
Mass1.70 M
Radius3.0 R
Luminosity12.06 L
Surface gravity (log g)3.89 cgs
Temperature6,417 K
Metallicity [Fe/H]+0.13 dex
Rotational velocity (v sin i)11.3 km/s
20 Oph B
Mass0.8 ± 0.2 M
Other designations
BD-10°4394, FK5 1438, GC 22643, HIP 82369, HR 6243, HD 151769, SAO 160118
Database references
SIMBADdata

20 Ophiuchi is an astrometric binary. The primary star is a late F-type subgiant star. It has a mass 1.72 times that of the Sun. The companion star regularly perturbs the primary star, causing it to wobble around the barycenter. From this, an orbital period of 35.5 years has been calculated. The secondary star is 0.8 times the mass of the Sun, and it may be a white dwarf or red dwarf.

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