Psi1 Aurigae

Psi1 Aurigae
Location of ψ1 Aurigae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension 06h 24m 53.90155s
Declination +49° 17 16.4112
Apparent magnitude (V) 4.91
Characteristics
Evolutionary stage Red supergiant
Spectral type K5-M1Iab-Ib
U−B color index +2.29
B−V color index +1.97
R−I color index 1.07
Variable type LC
Astrometry
Radial velocity (Rv)+4.7 km/s
Proper motion (μ) RA: −0.155 mas/yr
Dec.: −2.131 mas/yr
Parallax (π)0.4426±0.1103 mas
Distance6,590+1,382
−1,174
 ly
(2,021.5+424
−360
 pc)
Absolute magnitude (MV)−5.53
Details
Mass14.4±0.8 M
Radius934 R
1,004 R
Luminosity170,400 L
Temperature3,790 K
Metallicity [Fe/H]+0.08 dex
Age12.3±0.4 Myr
Other designations
ψ1 Aurigae, 46 Aurigae, BD+49 1488, FK5 242, GC 8235, HD 44537, HIP 30520, HR 2289, SAO 41076, PPM 49029
Database references
SIMBADdata

Psi1 Aurigae is a star in the northern constellation of Auriga. It name is a Bayer designation that is Latinized from ψ1 Aurigae, and abbreviated Psi1 Aur or ψ1 Aur. This star is faintly visible to the naked eye with an apparent visual magnitude of 4.91. Based upon a measured annual parallax shift of 0.44 mas, it is approximately 7,500 light-years (2,300 parsecs) distant from the Earth. It is receding from the Sun with a radial velocity of +4.7 km/s.

This is a massive supergiant star with a stellar classification of K5-M1Iab-Ib. It is a slow irregular variable of the LC type, with its brightness varying in magnitude by 0.44. The star is more than 14 times as massive as the Sun, over 900 times larger, and is blazing with 170,000 times the Sun's luminosity. It is one of the largest stars known, even larger and more luminous than well-known red supergiants Betelgeuse and Antares. This energy is being radiated into outer space from its outer atmosphere at an effective temperature of 3,790 K, giving it the orange-red hue of a cool M-type star.