| Observation data Epoch J2000 Equinox J2000  | |
|---|---|
| Constellation | Equuleus | 
| Right ascension | 21h 21m 04.825s [1] | 
| Declination | +07° 21′ 16.21″ [1] | 
| Apparent magnitude (V) | 5.798 [2] | 
| Characteristics | |
| Evolutionary stage | AGB [3] | 
| Spectral type | M2IIIa [4] | 
| U−B color index | +1.97 [5] | 
| B−V color index | +1.66 [5] | 
| Variable type | suspected [6] | 
| Astrometry | |
| Radial velocity (Rv) | −21.82±0.30 [1] km/s | 
| Proper motion (μ) | RA: 43.871±0.274 [1]  mas/yr  Dec.: −17.822±0.261 [1] mas/yr  | 
| Parallax (π) | 4.3895±0.1647 mas [1] | 
| Distance | 740 ± 30  ly  (228 ± 9 pc)  | 
| Absolute magnitude (MV) | −0.69 [7] | 
| Details | |
| Mass | 1.2 [8] M☉ | 
| Radius | 58 [1] R☉ | 
| Luminosity | 720 [1] L☉ | 
| Surface gravity (log g) | 1.64 [8] cgs | 
| Temperature | 3,920 [1] K | 
| Metallicity [Fe/H] | −0.27 [8] dex | 
| Other designations | |
| HIP 105413, HD 203291, HR 8163, SAO 126719 | |
| Database references | |
| SIMBAD | data | 
9 Equulei is an M-type star in the constellation Equuleus. It is an asymptotic giant branch (AGB) star, a star that has exhausted its core helium and is now fusing both hydrogen and helium in shells outside the core. [3] It is also a suspected variable star with an amplitude of about 0.05 magnitudes. [6]
The spectral type is M2IIIa, meaning it is a relatively cool giant star. As an AGB star, it is burning hydrogen and helium in shells around an inert carbon-oxygen core. It has expanded to 58 times the radius of the Sun, and it radiates 720 times as much electromagnetic radiation from a photosphere with an effective temperature of 3,920 K .