HR1077
HR1077 is a multiple main-sequence star of spectral class F3 in the constellation of Camelopardalis.
HR1077 visual magnitude is 6.46. Because of its faintness, HR1077 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 HR1077.
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR1077 is situated in the Hertzsprung–Russell diagram.
Star System Properties
HR1077 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR1077 double sysyem:
Distance, Radial Speed, Proper Motion
HR1077 is distant 182.53 light years from the Sun and it is moving far from the Sun at the speed of 21 kilometers per second.
Alternative Designations
Visibility from Your Location
HR1077 is circumpolar and transits at 03:42 UTC (altitude: 81.4°)