HD 15920

Giant star in the constellation Cassiopeia From Wikipedia, the free encyclopedia

HD 15920 is a single[7] star in the northern constellation of Cassiopeia. It has a yellow hue and is visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.17.[1] This object is located at a distance of approximately 269 light years from the Sun based on parallax, but it is drifting closer with a radial velocity of −4 km/s.[2]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
HD 15920
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia[1]
Right ascension 02h 38m 02.03317s[2]
Declination +72° 49 05.7106[2]
Apparent magnitude (V) 5.17[1]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type G8III[3]
B−V color index +0.896±0.003[1]
Astrometry
Radial velocity (Rv)−3.81±0.12[2] km/s
Proper motion (μ) RA: −27.072[2] mas/yr
Dec.: +15.618[2] mas/yr
Parallax (π)12.1337±0.0717 mas[2]
Distance269 ± 2 ly
(82.4 ± 0.5 pc)
Absolute magnitude (MV)0.70[1]
Details
Mass2.55±0.68[4] M
Radius10.26±0.73[5] R
Luminosity64+6
−5
[5] L
Surface gravity (log g)2.91±0.11[4] cgs
Temperature5,104±148[5] K
Metallicity [Fe/H]0.02±0.05[4] dex
Age977+198
−164
[4] Myr
Other designations
BD+72°140, FK5 87, GC 3116, HD 15920, HIP 12273, HR 743, SAO 4694, GSC 04320-02109[6]
Database references
SIMBADdata
Close

This object is an aging giant star with a stellar classification of G8III.[3] After exhausting the supply of hydrogen at its core, this star has cooled and expanded off the main sequence – at present it has ten times the girth of the Sun.[5] The star is around a billion years old with 2.6 times the mass of the Sun.[4] It is radiating 64 times the Sun's luminosity from its swollen photosphere at an effective temperature of 5,104 K.[5] HD 15920 is the most likely source for the X-ray emission detected at these coordinates.[8]

References

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