Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 06h 06m 22.44529s [1] |
Declination | +29° 30′ 44.6832″ [1] |
Apparent magnitude (V) | 6.01 - 6.11 [2] |
Characteristics | |
Evolutionary stage | AGB [3] |
Spectral type | M3II [4] |
U−B color index | 1.94 |
B−V color index | 1.73 |
Variable type | Semi-regular [2] |
Astrometry | |
Radial velocity (Rv) | −36.40±0.18 [5] km/s |
Proper motion (μ) | RA: 11.503 [1] mas/yr Dec.: −5.126 [1] mas/yr |
Parallax (π) | 3.7146±0.0756 mas [1] |
Distance | 880 ± 20 ly (269 ± 5 pc) |
Details | |
Radius | 85 [6] R☉ |
Luminosity | 985 [1] L☉ |
Surface gravity (log g) | 0.78 [7] cgs |
Temperature | 3,639 [6] K |
Other designations | |
DO 11899, HIC 28930, PPM Star Catalogue 95388, STT 129, GC 7725, HIP 28930, SAO 77958, ADS 4673, GCRV 3829, HR 2146, AG+29° 663, IDS 06000+2931, TYC 1876-1774-1, BD+29° 1112, IRAS 06031+2931, UBV M 11751, CCDM J06064+2931, GSC 01876-01774, IRC +30137, YZ 29 2943, CSI+29 1112 1, HD 41429, 2MASS J06062243+2930445. | |
Database references | |
SIMBAD | data |
V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, [2] so it is faintly visible to the naked eye under ideal observing conditions. Located around 730 light-years distant, V394 Aurigae shines with a luminosity approximately 985 times that of the Sun [1] and has a surface temperature of 3,639 K . [6]
In 1991, Leroy F. Snyder discovered that the star, then called HR 2146, is a variable star. [9] It was given its variable star designation, V394 Aurigae, in 1993. [10] Koen and Eyer found that the star's brightness, as seen by Hipparcos , varies with a period of 3.9 days. [11]
It is a double star: the secondary, designated V394 Aurigae B, is an eleventh-magnitude F7V star [12] with a separation of 10 arcseconds. [13]