Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ophiuchus |
Right ascension | 18h 20m 52.06435s [1] |
Declination | 03° 22′ 37.7817″ [1] |
Apparent magnitude (V) | 4.85 [2] |
Characteristics | |
Spectral type | G8III [3] |
U−B color index | +0.61 [4] |
B−V color index | +0.91 [4] |
Astrometry | |
Radial velocity (Rv) | +4.35 [5] km/s |
Proper motion (μ) |
RA: −7.646
[1]
mas/
yr Dec.: +12.546 [1] mas/ yr |
Parallax (π) | 13.7320 ± 0.2060 mas [1] |
Distance | 238 ± 4
ly (73 ± 1 pc) |
Absolute magnitude (MV) | 0.34 [2] |
Details | |
Mass | 2.38 [6] M☉ |
Radius | 10.52+0.32 −1.04 [1] R☉ |
Luminosity | 66.0±1.2 [1] L☉ |
Surface gravity (log g) | 2.70 [6] cgs |
Temperature | 5,073+271 −76 [1] K |
Metallicity [Fe/H] | -0.21 [6] dex |
Rotational velocity (v sin i) | 0.0 [5] km/s |
Age | 1.73 [7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
74 Ophiuchi is a suspected binary star [9] in the equatorial constellation of Ophiuchus, near the border with Serpens Cauda. It is visible to the naked eye as a faint, yellow-hued point of light with a combined apparent visual magnitude of 4.85. [2] The system is located at a distance of 238 light years from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +4.4 km/s. [5]
The primary member, designated component A, is an aging giant star with a stellar classification of G8III [3] and an estimated age of 1.73 [7] billion years. Having exhausted the hydrogen supply at its core, the star has expanded to 10.5 [1] times the Sun's radius. It is a red clump giant, [10] which means it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 2.4 [6] times the mass of the Sun and is radiating 66 [1] times the Sun's luminosity from its swollen photosphere at an effective temperature of around 5,073 K. [1]
The magnitude 11.5 secondary, component B, lies at an angular separation of 28.1″ from the primary, as of 2008. [9] A visual companion, component C, is magnitude 12.28 and has a separation of 57.9″. [11]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ophiuchus |
Right ascension | 18h 20m 52.06435s [1] |
Declination | 03° 22′ 37.7817″ [1] |
Apparent magnitude (V) | 4.85 [2] |
Characteristics | |
Spectral type | G8III [3] |
U−B color index | +0.61 [4] |
B−V color index | +0.91 [4] |
Astrometry | |
Radial velocity (Rv) | +4.35 [5] km/s |
Proper motion (μ) |
RA: −7.646
[1]
mas/
yr Dec.: +12.546 [1] mas/ yr |
Parallax (π) | 13.7320 ± 0.2060 mas [1] |
Distance | 238 ± 4
ly (73 ± 1 pc) |
Absolute magnitude (MV) | 0.34 [2] |
Details | |
Mass | 2.38 [6] M☉ |
Radius | 10.52+0.32 −1.04 [1] R☉ |
Luminosity | 66.0±1.2 [1] L☉ |
Surface gravity (log g) | 2.70 [6] cgs |
Temperature | 5,073+271 −76 [1] K |
Metallicity [Fe/H] | -0.21 [6] dex |
Rotational velocity (v sin i) | 0.0 [5] km/s |
Age | 1.73 [7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
74 Ophiuchi is a suspected binary star [9] in the equatorial constellation of Ophiuchus, near the border with Serpens Cauda. It is visible to the naked eye as a faint, yellow-hued point of light with a combined apparent visual magnitude of 4.85. [2] The system is located at a distance of 238 light years from the Sun based on parallax, [1] and is drifting further away with a radial velocity of +4.4 km/s. [5]
The primary member, designated component A, is an aging giant star with a stellar classification of G8III [3] and an estimated age of 1.73 [7] billion years. Having exhausted the hydrogen supply at its core, the star has expanded to 10.5 [1] times the Sun's radius. It is a red clump giant, [10] which means it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 2.4 [6] times the mass of the Sun and is radiating 66 [1] times the Sun's luminosity from its swollen photosphere at an effective temperature of around 5,073 K. [1]
The magnitude 11.5 secondary, component B, lies at an angular separation of 28.1″ from the primary, as of 2008. [9] A visual companion, component C, is magnitude 12.28 and has a separation of 57.9″. [11]