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HD 36678

Star in the constellation Auriga From Wikipedia, the free encyclopedia

HD 36678 is single[9] star in the northern constellation of Auriga. This star is dimly visible to the naked eye with an apparent visual magnitude of 5.83.[3] It is located at a distance of approximately 880 light years from the Sun based on parallax.[2]

Right ascension05h 36m 35.21822s[2]
Declination+54° 25′ 43.1710″[2]
Quick facts Constellation, Right ascension ...
HD 36678
Observation data
Epoch J2000      Equinox ICRS
Constellation Auriga[1]
Right ascension 05h 36m 35.21822s[2]
Declination +54° 25′ 43.1710″[2]
Apparent magnitude (V) 5.8334[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M0III[4]
Apparent magnitude (G) 5.01[2]
U−B color index +1.98[5]
B−V color index +1.671±0.006[1]
Variable type suspected[6]
Astrometry
Radial velocity (Rv)0.91±0.14[2] km/s
Proper motion (μ) RA: −6.351±0.055[2] mas/yr
Dec.: −10.625±0.048[2] mas/yr
Parallax (π)3.7121±0.0635 mas[2]
Distance880 ± 20 ly
(269 ± 5 pc)
Absolute magnitude (MV)−1.00[1]
Details
Mass1.38[7] M☉
Radius63.2+7.0
−4.7
[8] R☉
Luminosity875±34[8] L☉
Surface gravity (log g)0.79[7] cgs
Temperature3,950+154
−202
[8] K
Metallicity [Fe/H]−0.12[7] dex
Other designations
BD+54°914, HD 36678, HIP 26344, HR 1866, SAO 25276, Gaia DR3 264919909305988224
Database references
SIMBADdata
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This is an aging red giant star with a stellar classification of M0III.[4] It is currently on the asymptotic giant branch of the HR diagram,[4] and has expanded to ~63[8] times the radius of the Sun. The star is radiating ~875[8] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,950 K.[8]

The brightness of HD 36678 is suspected of being variable. Hipparcos photometry showed maximum and minimum apparent magnitudes of 5.806 and 5.855 respectively, in the Hipparcos photometric band.[6] No period was found, the variability has not been confirmed, and the star is not formally listed as a variable star.[10]

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