Binary star system in the northern constellation of Auriga
β Aurigae
Location of β Aurigae (circled)
Observation data Epoch J2000.0 Equinox J2000.0
Constellation
Auriga
Right ascension
05h 59m 31.72293s[1]
Declination
+44° 56′ 50.7573″[1]
Apparent magnitude (V)
1.89 - 1.98[2]
Characteristics
Spectral type
A1m IV + A1m IV[3]
U−B color index
+0.05[4]
B−V color index
+0.03[4]
R−I color index
–0.01
Variable type
Algol variable[2]
Astrometry
Radial velocity (Rv)
–18.2[5] km/s
Proper motion (μ)
RA: –56.44[1] mas/yr Dec.: –0.95[1] mas/yr
Parallax (π)
40.21 ± 0.23 mas[1]
Distance
81.1 ± 0.5 ly (24.9 ± 0.1 pc)
Absolute magnitude (MV)
0.55/0.76[6]
Orbit[7]
Period (P)
3.96004 days
Eccentricity (e)
0.0
Inclination (i)
76.0 ± 0.4°
Periastron epoch (T)
54539.0162 ± 0.0003 reduced HJD
Semi-amplitude (K1) (primary)
108.053 ± 0.072 km/s
Semi-amplitude (K2) (secondary)
110.911 ± 0.071 km/s
Details
β Aur Aa
Mass
2.389 ± 0.013[7]M☉
Radius
2.77[8]R☉
Luminosity
55[8]L☉
Surface gravity (log g)
3.93[6] cgs
Temperature
9,350[8] K
Rotational velocity (v sin i)
33[8] km/s
Age
570[8] Myr
β Aur Ab
Mass
2.327 ± 0.013[7]M☉
Radius
2.63[8]R☉
Luminosity
47[8]L☉
Temperature
9,200[8] K
Rotational velocity (v sin i)
34[8] km/s
Other designations
Menkalinan, 34 Aurigae, ADS 4556, BD+44 1328, FK5 227, HD 40183, HIP 28360, HR 2088, SAO 40750.[9]
Database references
SIMBAD
data
Beta Aurigae (Latinized from β Aurigae, abbreviated Beta Aur, β Aur), officially named Menkalinan/mɛŋˈkælɪnæn/,[10][11] is a binary star[12] system in the northern constellation of Auriga. The combined apparent visual magnitude of the system is 1.9,[4] making it the second-brightest member of the constellation after Capella. Using the parallax measurements made during the Hipparcos mission, the distance to this star system can be estimated as 81.1 light-years (24.9 parsecs), give or take a half-light-year margin of error.[1]
Along their respective orbits around the Milky Way, Beta Aurigae and the Sun are closing in on each other, so that in around one million years it will become the brightest star in the night sky.[13]
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^Kunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Pub. ISBN 978-1-931559-44-7.
^"IAU Catalog of Star Names". Retrieved 28 July 2016.
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^Tomkin, Jocelyn (April 1998). "Once and Future Celestial Kings". Sky and Telescope. 95 (4): 59–63. Bibcode:1998S&T....95d..59T. – based on computations from HIPPARCOS data. (The calculations exclude stars whose distance or proper motion is uncertain.) PDF[permanent dead link]
BetaAurigae (Latinized from β Aurigae, abbreviated Beta Aur, β Aur), officially named Menkalinan /mɛŋˈkælɪnæn/, is a binary star system in the northern...
which is Latinised from β Tauri and abbreviated Beta Tau or β Tau. The original designation of Gamma Aurigae is now rarely used. It is a chemically peculiar...
constellation of Auriga. It has the Bayer designation α Aurigae, which is Latinised to Alpha Aurigae and abbreviated Alpha Aur or α Aur. Capella is the sixth-brightest...
60 Beta Librae Star 2.63 Alpha Serpentis Star 2.64 2.60 Beta Corvi Star 2.65 2.62 Theta Aurigae Binary star system 2.65 Alpha Columbae Star 2.65 Beta Arietis...
along with other scattered stars such as BetaAurigae, Alpha Coronae Borealis, Beta Crateris, Beta Eridani and Beta Serpentis. This would be one of three...
Auriga. Located about one degree north of the 2nd magnitude star BetaAurigae, Pi Aurigae is visible to the naked eye with an apparent visual magnitude of...
realized that there were many undiscovered ones. He soon found that BetaAurigae and Delta Orionis were eclipsing binaries. Further discoveries followed...
Aur (Delta Aurigae). Also known in Japanese as Gosha (Five Chariots; 五車). Iota Aurigae Alpha AurigaeBetaAurigae Theta Aurigae Gamma Aurigae The Five Chariots...
asterism consisting of Eta Aurigae, Epsilon Aurigae, Zeta Aurigae, Upsilon Aurigae, Nu Aurigae, Tau Aurigae, Chi Aurigae and 26 Aurigae. Consequently, the Chinese...
LY Aurigae is a multiple star system in the constellation Auriga. It is an eclipsing binary variable star, dropping in brightness by 0.7 magnitudes every...
spectrum. Then, in 1889, Maury discovered a second spectroscopic binary, BetaAurigae, and calculated its orbital period. Learning of this work from a copy...
faint, located in a nondescript patch of sky between the Pleiades and BetaAurigae. The distance to RV Tau has been calculated by various methods, including...
et al. (2010). "Infrared images of the transiting disk in the Epsilon Aurigae system". Nature. 464 (7290): 370–2. arXiv:1004.2464. Bibcode:2010Natur...
reassigned to Scorpius – Star Tales – Norma Also designated Gamma Aurigae (γ Aur, γ Aurigae) by Bayer, after Ptolemy – Bayer’s Uranometria and Bayer letters...
(~2:48 hours, HW Virginis); the longest is 9892 days (27 years, Epsilon Aurigae). Over long periods of time, various effects can cause the period to vary:...
16 Aurigae is a triple star system located 232 light years away from the Sun in the northern constellation of Auriga. It is visible to the naked eye as...
Chi Aurigae, Latinized from χ Aurigae, is the Bayer designation for a binary star system in the northern constellation of Auriga. It is faintly visible...
IU Aurigae is a triple star system in the constellation Auriga, consisting of an eclipsing binary pair orbiting a third component with a period of 335 years...
18 Aurigae is a star located 233 light years away from the Sun in the northern constellation of Auriga. The brightness of this object is near the limit...
Rho Aurigae (ρ Aur, ρ Aurigae) is the Bayer designation for a binary star system in the northern constellation of Auriga. It is faintly visible to the...
letter from both constellations: Alpha Andromedae = Delta Pegasi, Beta Tauri = Gamma Aurigae, and Nu Boötis = Psi Herculis. (He catalogued Fomalhaut only once...
HD 34626, also known as MZ Aurigae, is an unusual variable star in the northern constellation of Auriga. It has an apparent magnitude of 8.2 and is about...