λ Coronae Australis (lambda Coronae Australis)
λ Coronae Australis is a variable and multiple main-sequence star of spectral class A2 in the constellation of Corona Australis.
λ Coronae Australis visual magnitude is 5.13. Because of its faintness, λ Coronae Australis is visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.
Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart
Simplified finder chart for λ Coronae Australis (lambda Coronae Australis).
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where λ Coronae Australis is situated in the Hertzsprung–Russell diagram.
Star System Properties
λ Coronae Australis is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the λ Coronae Australis double sysyem:
Distance, Radial Speed, Proper Motion
λ Coronae Australis is distant 201.86 light years from the Sun and it is moving towards the Sun at the speed of 26 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's λ Coronae Australis (lambda Coronae Australis) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):