17 Sagittarii
Binary star system in the constellation Sagittarius
From Wikipedia, the free encyclopedia
17 Sagittarii is a binary star system in the zodiac constellation of Sagittarius, located 675 light years from the Sun. With a combined apparent visual magnitude of 6.89[2] it is below the normal limit of visibility to the naked eye. The system is moving closer to the Earth with a heliocentric radial velocity of â14 km/s.[1] J. Allen Hynek (1938) found an initial spectral type of G5 + A5 for the pair. It was first resolved by Harold A. McAlister (1978), who found an angular separation of 0.260â³Â±0.002â³ along a position angle of 133.0°±1.2°[8]
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 18h 16m 35.36860s[1] |
| Declination | â20° 32â² 40.1303â³[1] |
| Apparent magnitude (V) | 6.89[2] (7.24 + 8.89[3]) |
| Characteristics | |
| Spectral type | G8/K0 III[4] + A4:[5] |
| BâV color index | 1.027±0.015[2] |
| Astrometry | |
| Radial velocity (Rv) | â13.88±0.51[1] km/s |
| Proper motion (μ) | RA: 10.978[1] mas/yr Dec.: â14.342[1] mas/yr |
| Parallax (Ï) | 4.8289±0.0505 mas[1] |
| Distance | 675 ± 7 ly (207 ± 2 pc) |
| Absolute magnitude (MV) | 0.68[2] |
| Details | |
| Luminosity | 73.21[6] Lâ |
| Temperature | 4700[6] K |
| Other designations | |
| 17 Sgr, BDâ20°5068, HD 167570, HIP 89567, SAO 186575, WDS 18166-2033[7] | |
| Database references | |
| SIMBAD | data |
The magnitude 7.24[3] primary component is an evolved giant star with a stellar classification of G8/K0 III,[4] indicating it has exhausted the hydrogen at its core and expanded off the main sequence. It is radiating 73 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,700 K.[6] The companion is a hot A-type star of uncertain luminosity class,[5] with a visual magnitude of 8.89.[3]