HD 39225

Star in the constellation Auriga From Wikipedia, the free encyclopedia

HD 39225, also known as HR 2028, is a variable star in the northern constellation Auriga, located around 660 light years away from the Sun.[2] It is visible to the naked eye as a faint, red-hued star with an apparent visual magnitude of around 6.[3] This is a suspected runaway star[10] that is moving away from the Sun with a heliocentric radial velocity of 99 km/s.[2]

Right ascension05h 52m 40.09301s[2]
Declination+33° 55 02.8663[2]
Apparentmagnitude(V)5.82–6.07[3]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 39225
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga[1]
Right ascension 05h 52m 40.09301s[2]
Declination +33° 55 02.8663[2]
Apparent magnitude (V) 5.82–6.07[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M1+III Fe-1[5]
U−B color index 1.97
B−V color index 1.579±0.021
Variable type suspected[3]
Astrometry
Radial velocity (Rv)99.39±0.61[2] km/s
Proper motion (μ) RA: +17.953[2] mas/yr
Dec.: +9.174[2] mas/yr
Parallax (π)4.9537±0.0893 mas[2]
Distance660 ± 10 ly
(202 ± 4 pc)
Absolute magnitude (MV)−0.77[1]
Details
Mass3.7[6] M
Radius51[7] R
Luminosity411[7] L
Surface gravity (log g)1.61[8] cgs
Temperature3,643[7] K
Age865[8] Myr
Other designations
NSV 2681, BD+33°1179, HD 39225, HIP 27778, HR 2028, SAO 58528, GSC 02414-00524[9]
Database references
SIMBADdata
Close

Currently on the asymptotic giant branch,[4] this is an evolved red giant star with a stellar classification of M1+III Fe-1.[5] The suffix notation indicates an underabundance of iron in the stellar atmosphere compared to similar stars of its class. It is suspected of varying in brightness between magnitudes 5.82 and 6.07.[3] Having exhausted the hydrogen at its core, it has expanded to around 51 times the Sun's radius.[7] It shines with a luminosity approximately 411 times that of the Sun and has a surface temperature of 3,643 K.[7]

References

Related Articles

Wikiwand AI