21 Sagittarii
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 18h 25m 21.04075s |
| Declination | −20° 32′ 30.0385″ |
| Apparent magnitude (V) | 4.81 (5.03 + 7.43) |
| Characteristics | |
| Spectral type | K2II + A5: |
| U−B color index | +0.93 |
| B−V color index | +1.30 |
| Astrometry | |
| Radial velocity (Rv) | −11.80 km/s |
| Proper motion (μ) | RA: +8.46 mas/yr Dec.: −28.07 mas/yr |
| Parallax (π) | 7.95±0.72 mas |
| Distance | 410 ± 40 ly (130 ± 10 pc) |
| Absolute magnitude (MV) | −0.67 |
| Details | |
| 21 Sgr A | |
| Mass | 7.9 M☉ |
| Luminosity | 320 L☉ |
| Temperature | 4,234 K |
| Rotational velocity (v sin i) | 4.4 km/s |
| Other designations | |
| 21 Sgr, BD−20°5134, GC 25132, HD 169420, HIP 90289, HR 6896, SAO 186794, CCDM J18254-2033AB, WDS J18254-2033AB, GSC 06274-01663 | |
| Database references | |
| SIMBAD | data |
21 Sagittarii is a binary star system in the southern zodiac constellation of Sagittarius. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.81. The system is located approximately 410 light years away from the Sun based on parallax. It is moving closer to the Earth with a heliocentric radial velocity of −11.80 km/s.
As of 2008, the pair had an angular separation of 1.7″ along a position angle of 280°. The brighter member of the pair, designated component A, is a K-type bright giant with a stellar classification of K2II and visual magnitude 5.03. It has eight times the mass of the Sun and is radiating 320 times the Sun's luminosity from its photosphere at an effective temperature of 4,234 K Its companion, component B, is magnitude 7.43 with type reported as A5:, where the ':' indicates some uncertainty about the classification.