HR4945
HR4945 is a double giant star of spectral class K1 in the constellation of Canes Venatici.
HR4945 visual magnitude is 5.63. Because of its faintness, HR4945 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 HR4945.
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR4945 is situated in the Hertzsprung–Russell diagram.
Star System Properties
HR4945 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 HR4945 double sysyem:
Distance, Radial Speed, Proper Motion
HR4945 is distant 482.96 light years from the Sun and it is moving towards the Sun at the speed of 20 kilometers per second.
Alternative Designations
Visibility from Your Location
HR4945 is circumpolar and transits at 10:14 UTC (altitude: 83.7°)