Aludra (Eta Canis Majoris)
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Map © 2003 Torsten Bronger
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A supergiant B star and the fifth brightest
star in the constellation Canis Major. Its name
refers to an Arabic group called "the Virgins," which consists
of the stars of the Great Dog's lower portions. Some of the Virgins, including
Aludra and Wezen, are in a loose stellar association
known as Collinder 121.
Formed only about 12 million years ago, Aludra is already in old age, blowing
a strong stellar wind from its surface
at a speed of some 500 km/s. The material it has lost – about one-third
of a solar mass – has gathered into a cloud that is detectable by
its infrared emission. A seventh magnitude white star about 2' from Aludra,
easily visible in a small telescope, is not a physical companion but lies
a mere 600 light-years from the Sun – about five times closer than
Aludra itself.
| visual magnitude |
2.45 |
| absolute magnitude |
-7.51 |
| spectral type |
B5Ia |
| surface temperature |
13,500 K |
| luminosity |
100,000 Lsun |
| distance |
3,200 light-years (1,000 pc) |
| position |
R.A. 07h 24m 05.7s,
Dec. -29° 18' 11" |
| other designations |
31 Canis Majoris, HR 2827,
CD-29°4328, HD 58350,
SAO 173651, FK5 283,
HIP 35904, GC 9886,
CCDM 07240-2918 |
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