γ Coronae Australis (gamma Coronae Australis)
γ Coronae Australis is a double main-sequence star of spectral class F8 in the constellation of Corona Australis.
γ Coronae Australis visual magnitude is 4.99. Because of its moderate brightness, γ Coronae Australis 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
Simplified finder chart for γ Coronae Australis (gamma Coronae Australis).
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where γ Coronae Australis is situated in the Hertzsprung–Russell diagram.
Star System Properties
γ Coronae Australis is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the γ Coronae Australis double sysyem:
Distance, Radial Speed, Proper Motion
γ Coronae Australis is distant 58.33 light years from the Sun and it is moving towards the Sun at the speed of 52 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's γ Coronae Australis (gamma Coronae Australis) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):