Nu Pavonis is a possible triple star system[11] in the southern constellation of Pavo.

It is visible to the naked eye as a faint star that varies in apparent visual magnitude from 4.60 to 4.64 over a period of 0.85584 days.

[2] The system lies approximately 440 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of +17 km/s.

[7] Nu Pavonis was discovered to be a variable star when the Hipparcos data was analyzed.

This star is estimated at 0.15 solar masses and an effective temperature of 3,192 K.[8] It too is an X-ray source.