18 Aurigae

Star in the constellation Auriga From Wikipedia, the free encyclopedia

18 Aurigae is a star located 235[2] light years away from the Sun in the northern constellation of Auriga.[9] The brightness of this object is near the limit of visibility to the naked eye under good viewing conditions, appearing as a dim, white-hued star with an apparent visual magnitude of 6.49.[3] The star is moving away from the Sun with a heliocentric radial velocity of 6.5 km/s.[2]

Right ascension05h 19m 23.75369s[2]
Declination+33° 59′ 07.3952″[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
18 Aurigae
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga[1]
Right ascension 05h 19m 23.75369s[2]
Declination +33° 59′ 07.3952″[2]
Apparent magnitude (V) 6.489[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A7 V[4]
Apparent magnitude (G) 6.45[2]
U−B color index +0.09[5]
B−V color index +0.256±0.007[1]
Astrometry
Radial velocity (Rv)6.55±0.55[2] km/s
Proper motion (μ) RA: +28.281±0.062[2] mas/yr
Dec.: âˆ’12.715±0.044[2] mas/yr
Parallax (π)13.8604±0.0527 mas[2]
Distance235.3 ± 0.9 ly
(72.1 ± 0.3 pc)
Absolute magnitude (MV)2.31[1]
Details
Mass1.69±0.03[6] M☉
Radius1.92+0.12
−0.03
[7] R☉
Luminosity10.091±0.063[7] L☉
Surface gravity (log g)4.26±0.14 cgs
Temperature7,432+231
−67
[7] K
Rotational velocity (v sin i)124[6] km/s
Age950[8] Myr
Other designations
18 Aur, BD+33°1010, GC 6504, HD 34499, HIP 24832, HR 1734, SAO 57893, ADS 3893, WDS J05194+3359, Gaia DR3 182009826266321792[9]
Database references
SIMBADdata
Close

This is an ordinary A-type main-sequence star with a stellar classification of A7 V,[4] which indicates it is generating energy by hydrogen fusion at its core. The object is 950[8] million years old with a high rate of spin, showing a projected rotational velocity of 124 km/s.[6] It has 1.7[6] times the mass of the Sun and 1.9[7] times the Sun's radius. The star is radiating 10[7] times the luminosity of the Sun from its photosphere at an effective temperature of 7,432 K.[7]

18 Aurigae has a magnitude 12.50 companion star at an angular separation of 3.90″ along a position angle of 167°, as of 2006.[10]

References

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