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]