41 Aurigae

41 Aurigae
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
41 Aur A
Right ascension 06h 11m 36.59156s
Declination +48° 42 39.5603
Apparent magnitude (V) 6.15
41 Aur B
Right ascension 06h 11m 36.55589s
Declination +48° 42 47.0528
Apparent magnitude (V) 6.84
Characteristics
41 Aur A
Evolutionary stage Main sequence
Spectral type A2Va+
B−V color index 0.06
41 Aur B
Evolutionary stage Am star
Spectral type kA5hA5mF0(IV-V)
B−V color index 0.15
Astrometry
41 Aur A
Radial velocity (Rv)31 km/s
Proper motion (μ) RA: +15.085 mas/yr
Dec.: −55.907 mas/yr
Parallax (π)10.5367±0.0689 mas
Distance310 ± 2 ly
(94.9 ± 0.6 pc)
41 Aur B
Radial velocity (Rv)29 km/s
Proper motion (μ) RA: +17.183 mas/yr
Dec.: −53.536 mas/yr
Parallax (π)10.3314 ± 0.0711 mas
Distance316 ± 2 ly
(96.8 ± 0.7 pc)
Details
41 Aur A
Temperature9,000+278
−596
 K
Rotational velocity (v sin i)138 km/s
41 Aur B
Mass1.99±0.10 M
Radius1.78+0.12
−0.18
 R
Luminosity11.2±0.1 L
Temperature7,925+421
−260
 K
Rotational velocity (v sin i)133 km/s
Other designations
41 Aur, BD+48°1352, HIP 29388, ADS 4773, WDS J06116+4843
41 Aur A: GC 7853, HD 42127, HR 2176, SAO 40925
41 Aur B: GC 7851, HD 42126, HR 2175, SAO 40924
Database references
SIMBADdata

41 Aurigae is a binary star system located around 310–316 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as a dim, white-hued star with a combined apparent visual magnitude of 5.83. This system is moving further from the Earth with a heliocentric radial velocity of 31 km/s. It is a probable member of the Hyades Supercluster.

As of 2012, the pair had an angular separation of 7.39 along a position angle of 357.7°. The primary component is an A-type main-sequence star with a stellar classification of A2Va+ and a visual magnitude of 6.15. The magnitude 6.84 secondary companion is a possible Am star with a stellar classification of kA5hA5mF0(IV-V), showing the calcium K line and hydrogen lines of an A5 star and the metal lines of an F0 star.