T Coronae Borealis (T CrB)
T CrB is a famous recurrent nova of spectral class M3 . It is a double star system made of a red giant and a white dwarf orbiting in 228 days. T CrB is usually around magnitude 10 however during outbursts it can reach magnitude 2. Previous outbursts have been observed in 1866 and 1946 and some studies suggest that a new outburst might happen in the second half of 2024.
Waiting for the Next Outburst
Monitor the most recent measurements of T Coronae Borealis visual magnitude:
Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart
Simplified finder chart for T Coronae Borealis (T CrB).
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where T Coronae Borealis is situated in the Hertzsprung–Russell diagram.
Distance, Radial Speed, Proper Motion
T Coronae Borealis is distant 2,627.56 light years from the Sun and it is moving towards the Sun at the speed of 29 kilometers per second.
Alternative Designations
Visibility from Your Location
Today's T Coronae Borealis (T CrB) rise, transit and set times from Greenwich, UK are the following (all times relative to the local timezone Europe/London):