γ Circini (gamma Circini)

γ Circini is a double sub-giant star of spectral class B5 in the constellation of Circinus.

γ Circini visual magnitude is 4.51. Because of its moderate brightness, γ Circini is easily visible to the naked eye from locations with dark skies, while it might be barely visible, or not visible at all, from light-polluted skies.

Celestial Coordinates

Apparent

J2000

Galactic Coordinates

Finder Chart

Magnitude, Color, Spectral Class

The red dot in the diagram below shows where γ Circini is situated in the Hertzsprung–Russell diagram.

Star System Properties

γ Circini is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the γ Circini double sysyem:

Distance, Radial Speed, Proper Motion

γ Circini is distant 509.38 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.

Alternative Designations

Visibility from Your Location

γ Circini (gamma Circini) is currently not visible from Wenatchee, Stati Uniti