In Evidence
Other stars in Corona Australis
- Meridiana
- β Coronae Australis
- δ Coronae Australis
- θ Coronae Australis
- ζ Coronae Australis
- ε Coronae Australis
- γ Coronae Australis
- HR6862
- λ Coronae Australis
- HR6942
- μ Coronae Australis
- HR6875
- HR7122
- HR6991
- HR7129
- HR7031
- HR6818
- HR6804
- η1 Coronae Australis
- η2 Coronae Australis
- HR6910
- κ2 Coronae Australis
- HR6937
- HR7197
- HR6749
- HR6786
- HR7257
- HR7281
- HR6931
- HR7232
- HR6948
- HR7177
- HR6839
- HR7136
- κ1 Coronae Australis
- HR6915
- HR7268
- HR7170
- HR6856
- HR7255
- HR7156
- HR7273
- HR6921
- HR7169
ε Coronae Australis (epsilon Coronae Australis)
ε Coronae Australis is a variable main-sequence star of spectral class F2 in the constellation of Corona Australis.
ε Coronae Australis visual magnitude is 4.87. Because of its moderate brightness, ε 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
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where ε Coronae Australis is situated in the Hertzsprung–Russell diagram.
Distance, Radial Speed, Proper Motion
ε Coronae Australis is distant 97.52 light years from the Sun and it is moving far from the Sun at the speed of 54 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's ε Coronae Australis (epsilon Coronae Australis) rise, transit and set times from Paracale, Philippines are the following (all times relative to the local timezone Asia/Manila):