S Doradus

S Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160,000 light-years away. The star is a luminous blue variable, and one of the most luminous stars known, having a luminosity varying widely above and below 1,000,000 times the luminosity of the Sun, although it is too far away to be seen with the naked eye.

S Doradus

S Doradus is the brightest individual star in NGC 1910, encircled by the lower "spiral arm". The bright star within the lower right nebulosity (N119) is R85.
Credit: ESO
Observation data
Epoch J2000      Equinox J2000
Constellation Dorado
Right ascension 05h 18m 14.3572s
Declination −69° 15 01.148
Apparent magnitude (V) 8.6 – 11.5
Characteristics
Spectral type B8/9eq – F0/5:Iae
U−B color index –0.98
B−V color index +0.11
Variable type S Doradus
Astrometry
Radial velocity (Rv)+228 km/s
Proper motion (μ) RA: 1.735 mas/yr
Dec.: 0.280 mas/yr
Parallax (π)0.0073 ± 0.0371 mas
Distance169,000 ly
(51,800 pc)
Absolute magnitude (MV)–7.6 (1965)
–10.0 (1989)
Details
Mass24+16
−2
 M
1989 (maximum)
Radius380 R
Luminosity910,000 L
Surface gravity (log g)0.6 cgs
Temperature8,500 K
1985 (minimum)
Radius100 R
Luminosity1,400,000 L
Surface gravity (log g)1.6 cgs
Temperature20,000 K
1965 (deep minimum)
Luminosity2,000,000 L
Temperature35,000 K
Other designations
CD-69 295, HD 35343, CPD-69 356, IRAS 05182-6918, AAVSO 0518-69.
Database references
SIMBADdata
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