Article · Wikipedia archive · Last revised Jul 17, 2026

HD 93403

HD 93403 is a spectroscopic binary containing two highly luminous hot blue stars. It is about 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.

Last revised
Jul 17, 2026
Read time
≈ 2 min
Length
559 w
Citations
21
Source
HD 93403
Observation data
Epoch J2000      Equinox J2000
Constellation Carina1
Right ascension 10h 45m 44.11931s2
Declination −59° 24′ 28.1431″2
Apparent magnitude (V) 7.2723
Characteristics
Spectral type O5.5III(fc)var4 (O5.5I + O7V5)
U−B color index −0.7473
B−V color index +0.2123
Astrometry
Radial velocity (Rv)14.806 km/s
Proper motion (μ) RA: −6.326 mas/yr2
Dec.: +2.306 mas/yr2
Parallax (π)0.1927±0.0706 mas2
Distance3,2005 pc
Absolute magnitude (MV)−5.6757
Orbit8
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
Details5
Primary
Mass68.58 M
Radius24 R
Luminosity1,050,000 L
Temperature39,300 K
Secondary
Mass37.38 M
Radius10 R
Luminosity257,000 L
Temperature40,100 K
Other designations
HD 93403, HIP 52628, CD−58°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 about 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.4

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-ray9 and non-thermal radio emission.10

See also

See also

References

References

  1. Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  2. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. Maíz-Apellániz, Jesús; Walborn, Nolan R.; Galué, Héctor Á.; Wei, Lisa H. (2004). "A Galactic O Star Catalog". The Astrophysical Journal Supplement Series. 151 (1): 103–148. arXiv:astro-ph/0311196. Bibcode:2004ApJS..151..103M. doi:10.1086/381380. S2CID 118813863.
  4. Sota, A.; Maíz Apellániz, J.; Morrell, N. I.; Barbá, R. H.; Walborn, N. R.; Gamen, R. C.; Arias, J. I.; Alfaro, E. J. (2014). "The Galactic O-Star Spectroscopic Survey (GOSSS). II. Bright Southern Stars". The Astrophysical Journal Supplement Series. 211 (1): 84. arXiv:1312.6222. Bibcode:2014ApJS..211...10S. doi:10.1088/0067-0049/211/1/10. S2CID 118847528. 10.
  5. Rauw, G.; Vreux, J.-M.; Stevens, I. R.; Gosset, E.; Sana, H.; Jamar, C.; Mason, K. O. (2002). "Phase-resolved X-ray and optical spectroscopy of the massive binary HD 93403". Astronomy and Astrophysics. 388 (2): 552. Bibcode:2002A&A...388..552R. doi:10.1051/0004-6361:20020523.
  6. Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; Levato, H.; Morrell, N. I.; Torres, G.; Udry, S. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits". Astronomy and Astrophysics. 424: 727. arXiv:astro-ph/0406573. Bibcode:2004A&A...424..727P. doi:10.1051/0004-6361:20041213.
  7. Nebot Gómez-Morán, A.; Oskinova, L. M. (2018). "The X-ray catalog of spectroscopically identified Galactic O stars. Investigating the dependence of X-ray luminosity on stellar and wind parameters". Astronomy and Astrophysics. 620. arXiv:1808.07880. Bibcode:2018A&A...620A..89N. doi:10.1051/0004-6361/201833453.
  8. Rauw, G.; Sana, H.; Gosset, E.; Vreux, J.-M.; Jehin, E.; Parmentier, G. (2000). "A new orbital solution for the massive binary system HD 93403". Astronomy and Astrophysics. 360: 1003. Bibcode:2000A&A...360.1003R.
  9. Ryspaeva, Elizaveta; Kholtygin, Alexander (2018). "Analysis of the X-ray emission of OB stars: O stars". Research in Astronomy and Astrophysics. 18 (8): 104. Bibcode:2018RAA....18..104R. doi:10.1088/1674-4527/18/8/104.
  10. Palate, M.; Rauw, G.; Koenigsberger, G.; Moreno, E. (2013). "Spectral modelling of massive binary systems". Astronomy & Astrophysics. 552: A39. arXiv:1302.5201. Bibcode:2013A&A...552A..39P. doi:10.1051/0004-6361/201219754. S2CID 54771449.