|  | This article includes a list of general references, but it lacks sufficient corresponding inline citations .(October 2025) | 
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Hercules [1] | 
| Right ascension | 16h 11m 28.7s [2] [3] | 
| Declination | +16° 39′ 56″ [2] [3] | 
| Apparent magnitude (V) | 6.08 [2] [3] | 
| Characteristics | |
| Evolutionary stage | main sequence [4] | 
| Spectral type | A0V [3] | 
| U−B color index | 0 [2] [3] | 
| B−V color index | 0.02 [2] [3] | 
| Astrometry | |
| Parallax (π) | 8.6995±0.0353 mas [5] [ failed verification ] | 
| Distance | 375 ± 2  ly (114.9 ± 0.5 pc) | 
| Absolute magnitude (MV) | +0.63 [1] | 
| Other designations | |
| q Her, 48 Serpentis, BD+17 2982, SAO 101994, HD 145647, HR 6035 [2] | |
| Database references | |
| SIMBAD | data | 
q Herculis (48 Serpentis) is a double star in the constellation Hercules that is situated at a distance of approximately 439.95 light-years from the the Sun. It's apparent magnitude is +6.081. [5] [ failed verification ] The age of q Herculis is determined to be about 719 million years.[ citation needed ]
The largest star q Herculis is a white star of the spectral type A0V [5] , or A0. It has a mass of approximately 2.999 M☉, a radius of approximately 2.592 R☉,[ citation needed ] and a luminosity of approximately 52.481 L☉. Its effective temperature is approximately 9882 K [5] .
q Herculis is this double star's Bayer designation. It was once considered to be in the Serpens, where it got its Flamsteed designation 48 Serpentis. [6]