41 Ophiuchi

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41 Ophiuchi
Ophiuchus constellation map.svg
Red circle.svg
Location of 41 Ophiuchi (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Ophiuchus
Right ascension 17h 16m 36.68653s [1]
Declination −00° 26 43.0915 [1]
Apparent magnitude  (V)4.72 [2]
(4.92 + 7.51) [3]
Characteristics
Evolutionary stage horizontal branch [4]
Spectral type K2III [5]
U−B color index +1.11 [6]
B−V color index +1.15 [6]
Astrometry
Radial velocity (Rv)−0.16 [7]  km/s
Proper motion (μ)RA: −31.645 [1]   mas/yr
Dec.: −57.144 [1]   mas/yr
Parallax (π)16.1517 ± 0.2358  mas [1]
Distance 202 ± 3  ly
(61.9 ± 0.9  pc)
Absolute magnitude  (MV)0.72 [2]
Orbit [8]
Period (P)140.76±0.23 yr
Semi-major axis (a)0.959±0.008
Eccentricity (e)0.866±0.003
Inclination (i)65.1±0.0°
Longitude of the node (Ω)220.5±0.0°
Periastron epoch (T)1890.53±0.36  B
Argument of periastron (ω)
(secondary)
287.5±0.0°
Details
41 Oph A
Mass 1.46 [9]   M
Radius 11.80+0.27
−0.39
[1]   R
Luminosity 60.3±1.0 [1]   L
Surface gravity (log g)2.42 [10]   cgs
Temperature 4,509±65 [9]   K
Metallicity [Fe/H]+0.06 [2]   dex
Rotational velocity (v sin i)2.6 [7]  km/s
Age 3.73 [9]   Gyr
Other designations
41 Oph, BD−00°3255, GC  23320, HD  156266, HIP  84514, HR  6415, SAO  141586, CCDM J17166-0027AB, WDS J17166-0027 [11]
Database references
SIMBAD data

41 Ophiuchi is a binary star [8] system in the zodiac constellation of Ophiuchus, and is positioned less than half a degree to the south of the celestial equator. It is visible to the naked eye as a faint, orange-hued point of light with a combined apparent visual magnitude of 4.72. [2] The distance to this system is approximately 202  light years based on parallax. [12]

This is a visual binary with an orbital period of 141 years and an eccentricity of 0.866. [8] The magnitude 4.92 [3] primary, designated component A, is an aging K-type giant star with a stellar classification of K2III. [5] It is a red clump giant, [4] which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The star is 3.7 [9]  billion years old with 1.46 [9] times the mass of the Sun and has expanded to nearly 12 [1] times the Sun's radius. It is radiating 60 [1] times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,509 K. [9]

The secondary companion, component B, has a visual magnitude of 7.51 and an angular separation of 0.70 from the primary along a position angle of 22°, as of 2017. [3]

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