HR4788
HR4788 is a double main-sequence star of spectral class G1 in the constellation of Centaurus.
HR4788 visual magnitude is 5.77. Because of its faintness, HR4788 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
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR4788 is situated in the Hertzsprung–Russell diagram.
Star System Properties
HR4788 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR4788 double sysyem:
Distance, Radial Speed, Proper Motion
HR4788 is distant 92.48 light years from the Sun and it is moving far from the Sun at the speed of 18 kilometers per second.
Alternative Designations
Visibility from Your Location
HR4788 is currently not visible from Bellegarde-en-Forez, France