HR9011
HR9011 is a variable and double sub-giant star of spectral class B3 in the constellation of Andromeda.
HR9011 visual magnitude is 6.07. Because of its faintness, HR9011 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 HR9011 is situated in the Hertzsprung–Russell diagram.
Star System Properties
HR9011 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR9011 double sysyem:
Distance, Radial Speed, Proper Motion
HR9011 is distant 1,319.84 light years from the Sun and it is moving towards the Sun at the speed of 24 kilometers per second.
Alternative Designations
Visibility from Your Location
HR9011 is circumpolar and transits at 07:44 UTC (altitude: 85.5°)