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Star profile

Psi 2 Orionis

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

What is Psi 2 Orionis

Psi-2 Orionis is a binary system so tight that the two stars deform one another by gravity and produce a grazing eclipse every 2.5 days, an ellipsoidal variable whose brightness shifts by a few hundredths of a magnitude with each turn. At 1,137 light-years within Orion, its blue light set out when the Norman kingdom of Sicily was just taking shape in the Mediterranean.

Where it is and when to see it

Psi 2 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 42° above the horizon.
  • From New York it culminates about 52° above the horizon.
  • From Sydney it culminates about 53° above the horizon.

It can be seen from anywhere north of 87° S.

It ranks no. 31 in brightness among the 128 stars of Orion in our catalogue. To find it, start from Rigel, the brightest: it lies about 12° away (a fist at arm's length covers about 10°).

The light you see today left it about 1,100 years ago.

Find it on the sky map

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Leave your signature on Psi 2 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

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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 Psi 2 Orionis

Constellation
Orion
Apparent magnitude
4.59
Distance
1136.6 light years
Coordinates (J2000)
RA 81.709° · Dec 3.096°
Catalogue
HIP 25473 · HD 35715

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