Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hercules |
Right ascension | 17h 00m 17.37378s [1] |
Declination | 30° 55′ 35.0565″ [1] |
Apparent magnitude (V) | 3.9111 [1] |
Characteristics | |
Spectral type | A0 V [2] or A0 IV+ [3] |
U−B color index | −0.10 [4] |
B−V color index | −0.01 [4] |
Astrometry | |
Proper motion (μ) |
RA: −47.69
[1]
mas/
yr Dec.: +26.90 [1] mas/ yr |
Parallax (π) | 21.04 ± 0.14 mas [1] |
Distance | 155 ± 1
ly (47.5 ± 0.3 pc) |
Absolute magnitude (MV) | +0.54 [5] |
Orbit [6] | |
Period (P) | 4.0235 d |
Eccentricity (e) | 0.02 |
Periastron epoch (T) | 2417947.2420 ± 10.0 JD |
Argument of periastron (ω) (secondary) | 138° |
Semi-amplitude (K1) (primary) | 70.7 km/s |
Semi-amplitude (K2) (secondary) | 112.0 km/s |
Details | |
Mass | 2.6±0.1 [7] M☉ |
Radius | 2.72±0.07 [8] R☉ |
Luminosity | 64 [5] L☉ |
Surface gravity (log g) | 3.98±0.02 [8] cgs |
Temperature | 10197±57 [8] K |
Metallicity [Fe/H] | −0.25±0.04 [5] dex |
Rotational velocity (v sin i) | 60 [9] km/s |
Age | 400+50 −40 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Epsilon Herculis, Latinized from ε Herculis, is a fourth-magnitude multiple star system in the northern constellation of Hercules. The combined apparent visual magnitude of 3.9111 [1] is bright enough to make this system visible to the naked eye. Based upon an annual parallax shift of 21.04 mas as seen from Earth, [1] it is located 155 light years from the Sun. The system is moving closer to the Sun with a radial velocity of −25 km/s. [11]
There is disagreement over the properties of this system. Petrie (1939) classified two components as class A0 and A2 with a visual magnitude difference of 1.5. [3] Batten et al. (1989) catalogued it as a double-lined spectroscopic binary system with an orbital period of four days and an eccentricity of 0.02. [6] However, Hipparcos was not able to detect the duplicity. Tokovinin (1997) and Faraggiana et al. (2001) catalogued it as a triple star system. [3] Cowley et al. (1969) gave it a combined stellar classification of A0 V, [2] whereas Gray & Garrison (1987) classified it as an A0 IV+. Wolff & Preston (1978) listed a magnesium overabundance. [3] Since 1995 it has been classified as a Lambda Boötis star, [12] although this has been brought into question. [13] [3]
In Chinese, 天紀 (Tiān Jì), meaning Celestial Discipline, refers to an asterism consisting of ε Herculis, ξ Coronae Borealis, ζ Herculis, 59 Herculis, 61 Herculis, 68 Herculis, HD 160054 and θ Herculis. [14] Consequently, the Chinese name for ε Herculis itself is 天紀三 (Tiān Jì sān, English: the Third Star of Celestial Discipline.) [15]
{{
cite web}}
: CS1 maint: postscript (
link)
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hercules |
Right ascension | 17h 00m 17.37378s [1] |
Declination | 30° 55′ 35.0565″ [1] |
Apparent magnitude (V) | 3.9111 [1] |
Characteristics | |
Spectral type | A0 V [2] or A0 IV+ [3] |
U−B color index | −0.10 [4] |
B−V color index | −0.01 [4] |
Astrometry | |
Proper motion (μ) |
RA: −47.69
[1]
mas/
yr Dec.: +26.90 [1] mas/ yr |
Parallax (π) | 21.04 ± 0.14 mas [1] |
Distance | 155 ± 1
ly (47.5 ± 0.3 pc) |
Absolute magnitude (MV) | +0.54 [5] |
Orbit [6] | |
Period (P) | 4.0235 d |
Eccentricity (e) | 0.02 |
Periastron epoch (T) | 2417947.2420 ± 10.0 JD |
Argument of periastron (ω) (secondary) | 138° |
Semi-amplitude (K1) (primary) | 70.7 km/s |
Semi-amplitude (K2) (secondary) | 112.0 km/s |
Details | |
Mass | 2.6±0.1 [7] M☉ |
Radius | 2.72±0.07 [8] R☉ |
Luminosity | 64 [5] L☉ |
Surface gravity (log g) | 3.98±0.02 [8] cgs |
Temperature | 10197±57 [8] K |
Metallicity [Fe/H] | −0.25±0.04 [5] dex |
Rotational velocity (v sin i) | 60 [9] km/s |
Age | 400+50 −40 [7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Epsilon Herculis, Latinized from ε Herculis, is a fourth-magnitude multiple star system in the northern constellation of Hercules. The combined apparent visual magnitude of 3.9111 [1] is bright enough to make this system visible to the naked eye. Based upon an annual parallax shift of 21.04 mas as seen from Earth, [1] it is located 155 light years from the Sun. The system is moving closer to the Sun with a radial velocity of −25 km/s. [11]
There is disagreement over the properties of this system. Petrie (1939) classified two components as class A0 and A2 with a visual magnitude difference of 1.5. [3] Batten et al. (1989) catalogued it as a double-lined spectroscopic binary system with an orbital period of four days and an eccentricity of 0.02. [6] However, Hipparcos was not able to detect the duplicity. Tokovinin (1997) and Faraggiana et al. (2001) catalogued it as a triple star system. [3] Cowley et al. (1969) gave it a combined stellar classification of A0 V, [2] whereas Gray & Garrison (1987) classified it as an A0 IV+. Wolff & Preston (1978) listed a magnesium overabundance. [3] Since 1995 it has been classified as a Lambda Boötis star, [12] although this has been brought into question. [13] [3]
In Chinese, 天紀 (Tiān Jì), meaning Celestial Discipline, refers to an asterism consisting of ε Herculis, ξ Coronae Borealis, ζ Herculis, 59 Herculis, 61 Herculis, 68 Herculis, HD 160054 and θ Herculis. [14] Consequently, the Chinese name for ε Herculis itself is 天紀三 (Tiān Jì sān, English: the Third Star of Celestial Discipline.) [15]
{{
cite web}}
: CS1 maint: postscript (
link)