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Star profile

Omega Pavonis

3D likeness based on its real data · class K · ~4,200 K

What is Omega Pavonis

Omega Pavonis is a faint light of magnitude 5.14 in the tail of the southern Peacock, distant —more than 560 light-years by the Hipparcos parallaxes— and unusually swift: it is receding from us at some 180 km per second, a striking radial velocity for a naked-eye star. It belongs to that quiet population of the deep southern sky that yields only to those who look beyond the famous constellations.

Where it is and when to see it

Omega Pavonis lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is July: the Sun sits at the opposite point of the sky and the star culminates around midnight. How high it climbs above the horizon depends on the latitude you watch from.

Find it on the sky map

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The signature wall

Stelvia's sky works like a signature wall: anyone can leave their name and a message on a real star, and that signature goes up on the map for everyone to read. Signing is free.

A signature without a lock can be replaced by someone else's. The lock makes the signature permanent and lets you choose a symbolic name for the star, always shown next to the star's catalogue identifier. How the lock works

If you don't have an account yet, we'll ask for an email to confirm it's you: we send you a link and that's it, 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 Omega Pavonis

Constellation
Pavo
Apparent magnitude
5.14
Distance
563.4 light years
Coordinates (J2000)
RA 284.652° · Dec -60.201°
Catalogue
HIP 93163 · HD 175329

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

Other stars in Pavo

Pavo has 44 stars in Stelvia's catalogue. Here are a few of them.

See all 44 stars in Pavo