HR5207
HR5207 is a double main-sequence star of spectral class B9 in the constellation of Centaurus.
HR5207 visual magnitude is 5.25. Because of its faintness, HR5207 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 HR5207.
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR5207 is situated in the Hertzsprung–Russell diagram.
Star System Properties
HR5207 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 HR5207 double sysyem:
Distance, Radial Speed, Proper Motion
HR5207 is distant 362.63 light years from the Sun and it is moving far from the Sun at the speed of 27 kilometers per second.
Alternative Designations
Visibility from Your Location
HR5207 is currently not visible from Greenwich, UK