38 Aurigae

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Template:Short description

38 Aurigae
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.08[2]
Characteristics
Evolutionary stage horizontal branch[3]
Spectral type K0 III[4]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: +121.023[1] mas/yr
Dec.: −144.427[1] mas/yr
Parallax (π)13.8158±0.2136 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)1.572[5]
Details
Mass1.59[5] Template:Solar mass
Radius7[6] Template:Solar radius
Luminosity18.47[2] Template:Solar luminosity
Surface gravity (log g)2.95[5] cgs
Temperature4,834[5] K
Metallicity [Fe/H]−0.17[5] dex
AgeScript error: No such module "val".[7] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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38 Aurigae is a star located 236[1] light years away from the Sun in the northern constellation of Auriga.[8] It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 6.08.[2] The star is moving further from the Earth with a heliocentric radial velocity of +34 km/s,[2] and it has a relatively high proper motion, traversing the celestial sphere at the rate of 0.181 arc seconds per annum.[9] It is a probable member of the Hercules stream.[7]

This object is an aging giant star with a stellar classification of K0 III.[4] At the age of around 3.6[7] billion years it is a red clump giant, which indicates it is on the horizontal branch and is generating energy via helium fusion at its core.[3] The star has 1.59[5] times the mass of the Sun and has expanded to 7[6] times the Sun's radius. It is radiating 18[2] times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,834 K.[5]

38 Aurigae has a faint common proper motion companion at an angular separation of Script error: No such module "val"., which is equivalent to a projected separation of Script error: No such module "val".. This is a red dwarf star with a class of M5.3.[10]

References

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Template:Stars of Auriga