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Star profile

Omicron Cassiopeiae

Variable star
3D likeness based on its real data · class B · ~15,000 K

What 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.

Find it on the sky map

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Leave your signature on Omicron Cassiopeiae

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A public signature from a real person. The chosen name is a symbolic denomination within Stelvia, with no official standing or IAU recognition: the sky is not for sale and belongs to no one.

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

A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.

Other stars in Cassiopeia

Cassiopeia has 93 stars in Stelvia's catalogue. Here are a few of them.

See all 93 stars in Cassiopeia