G Herculis
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Hercules |
| Right ascension | 16h 28m 38.54859s |
| Declination | +41° 52′ 54.0406″ |
| Apparent magnitude (V) | 4.3 - 6.3 |
| Characteristics | |
| Evolutionary stage | AGB |
| Spectral type | M6− III |
| B−V color index | 1.289±0.024 |
| Variable type | SRb |
| Astrometry | |
| Radial velocity (Rv) | 1.49±0.38 km/s |
| Proper motion (μ) | RA: +30.16 mas/yr Dec.: −5.14 mas/yr |
| Parallax (π) | 9.21±0.18 mas |
| Distance | 354 ± 7 ly (109 ± 2 pc) |
| Absolute magnitude (MV) | −0.41 |
| Orbit | |
| Period (P) | 843.7±21.1 d |
| Eccentricity (e) | 0.37±0.11 |
| Periastron epoch (T) | 2,451,918.2±43.9 HJD |
| Argument of periastron (ω) (secondary) | 246±21° |
| Semi-amplitude (K1) (primary) | 2.3±0.3 km/s |
| Details | |
| g Her A | |
| Mass | 1.65±0.30 M☉ |
| Radius | 230 R☉ |
| Luminosity | 5,395 L☉ |
| Surface gravity (log g) | 0.20 cgs |
| Temperature | 3,263±23 K |
| Metallicity [Fe/H] | −0.01 dex |
| Other designations | |
| g Her, 30 Her, BD+42°2714, FK5 3303, HD 148783, HIP 80704, HR 6146, SAO 46108 | |
| Database references | |
| SIMBAD | data |
g Herculis is a binary star system in the northern constellation of Hercules. It has the Flamsteed designation 30 Herculis, while g Herculis is the Bayer designation. This system is visible to the naked eye as a faint, red-hued point of light. Based upon a measured parallax of 9.2 mas, it is located around 354 light years away from the Sun. The system is moving further from the Earth with a heliocentric radial velocity of 1.5 km/s.
This is a single-lined spectroscopic binary with an orbital period of 2.310 years and an eccentricity of 0.37. The visible component is an aging red giant on the asymptotic giant branch with a stellar classification of M6− III. According to Samus et al. (2017), it is a semiregular variable of subtype SRb, which ranges between visual magnitudes 4.3 and 6.3 over 89.2 days. It displays cyclical periods of 62.3, 89.5, and 888.9 days. The star is surrounded by a circumstellar dust shell that seems primarily composed of oxides of iron, magnesium, and aluminium, rather than silicates.