HD 93403

HD 93403
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 10h 45m 44.11931s
Declination −59° 24 28.1431
Apparent magnitude (V) 7.272
Characteristics
Spectral type O5.5III(fc)var (O5.5I + O7V)
U−B color index 0.747
B−V color index +0.212
Astrometry
Radial velocity (Rv)14.80 km/s
Proper motion (μ) RA: -7.27 mas/yr
Dec.: 2.45 mas/yr
Parallax (π)1.22±0.45 mas
Distance3,200 pc
Orbit
Period (P)15.093 days
Semi-major axis (a)121 R
Eccentricity (e)0.234
Inclination (i)~31°
Semi-amplitude (K1)
(primary)
79.3 km/s
Semi-amplitude (K2)
(secondary)
139.0 km/s
Details
Primary
Mass68.5 M
Radius24 R
Luminosity1,050,000 L
Temperature39,300 K
Secondary
Mass37.3 M
Radius10 R
Luminosity257,000 L
Temperature40,100 K
Other designations
HD 93403, HIP 52628, CD58°3545, 2MASS J10454411-5924281, GSC 08626-00641, TYC 8626-641-1
Database references
SIMBADdata

HD 93403 is a spectroscopic binary containing two highly luminous hot blue stars. It is 10,000 light years away in the Carina Nebula in the constellation Carina. It appears to have spectral type O5.5III, but this is composed of two spectra from a blue supergiant and blue main sequence star of spectral type O5.5I and O7V respectively. The two stars orbit every 15 days with a separation that varies from 93 R to 149 R. The binary is shedding mass at the high rate of 0.0005 M per year.

HD 93403 exhibits the Struve-Sahade effect, where the strength of the spectral lines of the individual components varies during the orbit. It also has colliding stellar winds that produce variable x-ray and non-thermal radio emission.