
Star profile
Omega Pavonis
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, when it culminates around midnight.
- From London it never rises above the horizon.
- From New York it never rises above the horizon.
- From Sydney it never sets and culminates about 64° up.
It can be seen from anywhere south of 30° N.
It ranks no. 19 in brightness among the 44 stars of Pavo in our catalogue. To find it, start from Peacock, the brightest: it lies about 12° away (a fist at arm's length covers about 10°).
The light you see today left it about 560 years ago.
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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 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
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Other stars in Pavo
Pavo has 44 stars in Stelvia's catalogue. Here are a few of them.
- PeacockAlpha Pavonis1.94
- Beta Pavonis3.42
- Delta Pavonis3.55
- Omicron Pavonis5.06
- Phi 2 Pavonis5.11
- Upsilon Pavonis5.14
- HIP 981745.24
- HIP 941505.31