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Star profile

Omicron 1 Orionis

Variable star
3D likeness based on its real data · class M · ~3,200 K

What is Omicron 1 Orionis

Omicron-1 Orionis is a remarkable rarity: a red giant of the unusual S class, an intermediate stage on the road from an ordinary M giant to a true carbon star, where zirconium begins to displace titanium in its atmosphere. A semi-regular variable, it drifts between magnitudes 4.65 and 4.88 every 31 days. At 651 light-years it pulses discreetly, far from the Belt's glitter, on Orion's northwestern shoulder.

Where it is and when to see it

Omicron 1 Orionis lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is December, when it culminates around midnight.

  • From London it culminates about 53° above the horizon.
  • From New York it culminates about 64° above the horizon.
  • From Sydney it culminates about 42° above the horizon.

It can be seen from anywhere north of 76° S.

It ranks no. 36 in brightness among the 128 stars of Orion in our catalogue. To find it, start from Rigel, the brightest: it lies about 23° away (a fist at arm's length covers about 10°).

The light you see today left it about 650 years ago.

Find it on the sky map

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Leave your signature on Omicron 1 Orionis

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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 1 Orionis

Constellation
Orion
Apparent magnitude
4.71
Distance
651.1 light years
Coordinates (J2000)
RA 73.133° · Dec 14.251°
Catalogue
HIP 22667 · HD 30959

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

Other stars in Orion

Orion has 128 stars in Stelvia's catalogue. Here are a few of them.

See all 128 stars in Orion