| Observation data Epoch J2000 Equinox J2000  | |
|---|---|
| Constellation | Auriga | 
| Right ascension | 06h 38m 23.01009s [1] | 
| Declination | +28° 59′ 03.6220″ [1] | 
| Apparent magnitude (V) | 5.744 [2] | 
| Characteristics | |
| Spectral type | B9 Mn + F0m [3] | 
| U−B color index | −0.07 [4] | 
| B−V color index | −0.02 [4] | 
| Astrometry | |
| Radial velocity (Rv) | 13.1±5.0 [5] km/s | 
| Proper motion (μ) | RA: −16.390 [1]  mas/yr  Dec.: −14.305 [1] mas/yr  | 
| Parallax (π) | 8.5139±0.1372 mas [1] | 
| Distance | 383 ± 6  ly  (117 ± 2 pc)  | 
| Absolute magnitude (MV) | +0.48 [6] | 
| Orbit [7] | |
| Period (P) | 38.90 yr | 
| Semi-major axis (a) | 0.159″ | 
| Eccentricity (e) | 0.557 | 
| Inclination (i) | 119.5° | 
| Longitude of the node (Ω) | 113.5° | 
| Periastron epoch (T) | B 1976.73 | 
|  Argument of periastron (ω) (secondary)  | 343.3° | 
| Details | |
| 53 Aur A | |
| Mass | 2.49±0.13 [8] M☉ | 
| Surface gravity (log g) | 4.0 [3] cgs | 
| Temperature | 10750 [3] K | 
| Rotational velocity (v sin i) | 25 [3] km/s | 
| 53 Aur B | |
| Surface gravity (log g) | 4.0 [3] cgs | 
| Temperature | 7,250 [3] K | 
| Rotational velocity (v sin i) | 0 [3] km/s | 
| Other designations | |
| BD+29°1293, GC 8649, HD 47152, HIP 31737, HR 2425, SAO 78571, PPM 96293, CCDM J06384+2859, WDS J06384+2859, TYC 1892-236-1, GSC 01892-00236 | |
| Database references | |
| SIMBAD | data | 
53 Aurigae is a binary star system in the northern constellation of Auriga. It is visible to the naked eye as a dim star with a combined apparent visual magnitude of 5.74. [2] Parallax estimates put it at a distance of 383 light-years (117 parsecs ) away. [1] The system is receding from the Earth with a heliocentric radial velocity of 13 km/s. [5]
The two components of 53 Aurigae orbit each other every 39 years with an eccentricity of 0.557. [7] The primary component, 53 Aurigae A, is chemically peculiar since it contains higher-than-normal amounts of manganese, [3] but also europium, chromium, and mercury. [8] It is a B-type main-sequence mercury-manganese star, [8] while the secondary component, 53 Aurigae B, is an early F-type main-sequence star. [8] The total mass of the system is estimated to be 4.8 M☉. [8]