HR1035
HR1035 is a variable and double supergiant star of spectral class B9 in the constellation of Camelopardalis.
HR1035 visual magnitude is 4.21. Because of its moderate brightness, HR1035 is easily visible to the naked eye from locations with dark skies, while it might be barely visible, or not visible at all, from light-polluted skies.
Celestial Coordinates
Apparent
J2000
Galactic Coordinates
Finder Chart
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR1035 is situated in the HertzsprungāRussell diagram.
Star System Properties
HR1035 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 HR1035 double sysyem:
Distance, Radial Speed, Proper Motion
HR1035 is distant 4,289.47 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Alternative Designations
Visibility from Your Location
HR1035 is circumpolar and transits at 11:29 UTC (altitude: 81.5°)