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HD 102839

Star in the constellation Musca From Wikipedia, the free encyclopedia

HD 102839 is a yellow hued supergiant star in the southern constellation of Musca. With an apparent visual magnitude of 4.98,[1] it is faintly visible to the naked eye under good viewing conditions. Based on a parallax of 2.11 mas,[2] it is located at a distance of approximately 1,550 light-years (480 pc) away from Earth. The star is drifting further away with a line of sight velocity component of +16 km/s.[5]

Right ascension11h 49m 56.61541s[2]
Declination−70° 13′ 32.8408″[2]
Quick facts Constellation, Right ascension ...
HD 102839
Location of HD 102839 (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Musca[1]
Right ascension 11h 49m 56.61541s[2]
Declination −70° 13′ 32.8408″[2]
Apparent magnitude (V) 4.98[1]
Characteristics
Spectral type G6Ib[3]
U−B color index +1.22[4]
B−V color index +1.40[4]
Astrometry
Radial velocity (Rv)+15.90[5] km/s
Proper motion (μ) RA: −8.113[2] mas/yr[2]
Dec.: −0.834 mas/yr[2]
Parallax (π)2.1101±0.1063 mas[2]
Distance1,550 ± 80 ly
(470 ± 20 pc)
Absolute magnitude (MV)−2.33[1]
Details
Mass2.3[6] M☉
Radius78[2] R☉
Luminosity1,593[1] L☉
Surface gravity (log g)0.63[6] cgs
Temperature4,500[7] K
Metallicity [Fe/H]−0.34[6] dex
Rotational velocity (v sin i)7.6[8] km/s
Other designations
CPD−69°1595, FK5 2945, GC 16206, HD 102839, HIP 57696, HR 4538, SAO 251604, GSC 09230-02344[9]
Database references
SIMBADdata
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This star has a stellar classification of G6Ib,[3] matching an evolved G-type supergiant star. With 2.3 times the mass of the Sun,[6] it has expanded to 78 times the Sun's radius.[2] It is spinning with a projected rotational velocity of 7.6 km/s.[8] HD 102839 is radiating almost 1,600[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,500 K.[7]

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