
Star profile
Omicron Cassiopeiae
Variable starWhat is Omicron Cassiopeiae
Omicron Cassiopeiae is a bluish B-type giant some 703 light-years away, a hot, massive star whose stellar wind can carve disks of gas around it. It belongs to the family of so-called Be stars, known for variability tied to the forming and dispersing of these disks. Its light pulses, subtly, within the great W traced by Queen Cassiopeia across the northern sky.
Where it is and when to see it
Omicron Cassiopeiae lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is October, when it culminates around midnight.
- From London it never sets and culminates about 87° up.
- From New York it culminates about 82° above the horizon.
- From Sydney it culminates about 8° above the horizon.
It can be seen from anywhere north of 42° S.
It ranks no. 12 in brightness among the 93 stars of Cassiopeia in our catalogue. To find it, start from Cih, the brightest: it lies about 13° away (a fist at arm's length covers about 10°).
The light you see today left it about 700 years ago.
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Astronomical data for Omicron Cassiopeiae
- Constellation
- Cassiopeia
- Apparent magnitude
- 4.48
- Distance
- 703.0 light years
- Coordinates (J2000)
- RA 11.181° · Dec 48.284°
- Catalogue
- HIP 3504 · HD 4180
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Other stars in Cassiopeia
Cassiopeia has 93 stars in Stelvia's catalogue. Here are a few of them.
- CihGamma Cassiopeiae2.15
- SchedarAlpha Cassiopeiae2.24
- CaphBeta Cassiopeiae2.28
- Kappa Cassiopeiae4.17
- Theta Cassiopeiae4.34
- Iota Cassiopeiae4.46
- 48 Cassiopeiae4.49
- Rho Cassiopeiae4.51