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Star profile

Eta Orionis

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

What is Eta Orionis

η Orionis is one of the most studied multiple systems in the hunter's belt: a knot of several hot B-type stars that eclipse one another in a rhythm of less than eight days. The Orion stellar association, one of the most active nurseries in the Milky Way, frames her in the night. Her light has been crossing the void for nearly a millennium.

Where it is and when to see it

Eta Orionis lies in the southern 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 36° above the horizon.
  • From New York it culminates about 47° above the horizon.
  • From Sydney it culminates about 58° above the horizon.

It can be seen from anywhere south of 88° N.

It ranks no. 10 in brightness among the 128 stars of Orion in our catalogue. To find it, start from Rigel, the brightest: it lies about 6° away (a fist at arm's length covers about 10°).

The light you see today left it about 980 years ago.

Find it on the sky map

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Leave your signature on Eta Orionis

Your name and a message go up on the map for everyone to read. Signing is free.

Without a lock, someone else can replace your signature. How the lock works

We'll ask for an email to confirm it's you, no password.

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 Eta Orionis

Constellation
Orion
Apparent magnitude
3.35
Distance
976.6 light years
Coordinates (J2000)
RA 81.119° · Dec -2.397°
Catalogue
HIP 25281 · HD 35411

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