
Star profile
Omega Canis Majoris
Variable starWhat is Omega Canis Majoris
Omega Canis Majoris is a blue supergiant more than 900 light-years away, deep in the heart of the Greater Dog, not far from the white blaze of Sirius. It belongs to the Be class: a giant spinning so fast that it flings matter into a burning disc around itself, producing subtle but measurable swings in brightness. A young, violent star with all its drama still ahead.
Where it is and when to see it
Omega Canis Majoris lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is January, when it culminates around midnight.
- From London it culminates about 12° above the horizon.
- From New York it culminates about 23° above the horizon.
- From Sydney it culminates about 83° above the horizon.
It can be seen from anywhere south of 63° N.
It ranks no. 12 in brightness among the 90 stars of Canis Major in our catalogue. To find it, start from Sirius, the brightest: it lies about 12° away (a fist at arm's length covers about 10°).
The light you see today left it about 910 years ago.
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Astronomical data for Omega Canis Majoris
- Constellation
- Canis Major
- Apparent magnitude
- 4.01
- Distance
- 911.2 light years
- Coordinates (J2000)
- RA 108.703° · Dec -26.773°
- Catalogue
- HIP 35037 · HD 56139
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Other stars in Canis Major
Canis Major has 90 stars in Stelvia's catalogue. Here are a few of them.
- SiriusAlpha Canis Majoris-1.44
- AdharaEpsilon Canis Majoris1.50
- WezenDelta Canis Majoris1.83
- Kappa Canis Majoris3.50
- Omicron 1 Canis Majoris3.89
- Nu 2 Canis Majoris3.95
- Theta Canis Majoris4.08
- MulipheinGamma Canis Majoris4.11