
Star profile
Omega 1 Scorpii
Hot blue starWhat is Omega 1 Scorpii
Omega-1 Scorpii belongs to the young Sco-Cen complex, the closest stellar association to Earth, a brotherhood of blue suns born almost simultaneously from the same cloud of gas. It is a hot B-type star whose intensely blue light takes some 470 years to reach us. Alongside its visual twin Omega-2, it forms a pair that splits cleanly in binoculars, two distinct flames bound to the same cosmic cradle and still deep in stellar adolescence.
Where it is and when to see it
Omega 1 Scorpii lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is May, when it culminates around midnight.
- From London it culminates about 18° above the horizon.
- From New York it culminates about 29° above the horizon.
- From Sydney it culminates about 77° above the horizon.
It can be seen from anywhere south of 69° N.
It ranks no. 19 in brightness among the 104 stars of Scorpius in our catalogue. To find it, start from Antares, the brightest: it lies about 8° away (a fist at arm's length covers about 10°).
The light you see today left it about 470 years ago.
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Astronomical data for Omega 1 Scorpii
- Constellation
- Scorpius
- Apparent magnitude
- 3.93
- Distance
- 471.4 light years
- Coordinates (J2000)
- RA 241.702° · Dec -20.669°
- Catalogue
- HIP 78933 · HD 144470
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Other stars in Scorpius
Scorpius has 104 stars in Stelvia's catalogue. Here are a few of them.
- AntaresAlpha Scorpii1.06
- ShaulaLambda Scorpii1.62
- SargasTheta Scorpii1.86
- PipirimaMu 2 Scorpii3.56
- Zeta 2 Scorpii3.62
- IklilRho Scorpii3.87
- JabbahNu Scorpii4.00
- HIP 813044.18