HD 35519

Star in the constellation Auriga From Wikipedia, the free encyclopedia

HD 35519 is a K-type giant star in the direction of open cluster Messier 38. It was once treated as a cluster member,[12] but is now known to be a foreground object located at a distance of about 699 light-years (214 pc).[2]

Right ascension05h 26m 54.31751s[2]
Declination+35° 27 26.1855[2]
Apparentmagnitude(V)6.3062±0.0008[3]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 35519

HD 35519 is the bright star next to the lower right corner in this picture of star cluster Messier 38
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga[1]
Right ascension 05h 26m 54.31751s[2]
Declination +35° 27 26.1855[2]
Apparent magnitude (V) 6.3062±0.0008[3]
Characteristics
Spectral type K7III[4]
Apparent magnitude (G) 5.66[2]
U−B color index +1.68[5]
B−V color index +1.45[5]
Astrometry
Radial velocity (Rv)−20.28±0.13[2] km/s
Proper motion (μ) RA: −14.565±0.055[2] mas/yr
Dec.: −11.452±0.031[2] mas/yr
Parallax (π)4.6665±0.0372 mas[2]
Distance699 ± 6 ly
(214 ± 2 pc)
Absolute magnitude (MV)−0.08[1]
Details
Mass2.7[6] M
Radius30[7] R
Luminosity259[8] L
Surface gravity (log g)1.50[9] cgs
Temperature4,265[7] K
Metallicity [Fe/H]−0.084±0.093[10] dex
Age5.6[9] Gyr
Other designations
BD+35°1102, FK5 2408, HD 35519, HIP 25476, HR 1794, SAO 58029, Gaia DR3 182940906456370304[11]
Database references
SIMBADdata
Close

The star has expanded to about 30 times the Sun's radius and radiates around 259 times the Sun's luminosity at a temperature of about 4,265 K.[7][8] HD 35519 is 5.6 billion years old and has 2.7 times the Sun's mass.[9][6] At an apparent visual magnitude of 6.3062[3], the star is visible to the naked eye under good viewing conditions.

References

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