HR979
HR979 is a double main-sequence star of spectral class B9 in the constellation of Perseus.
HR979 visual magnitude is 6.45. Because of its faintness, HR979 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 HR979.
Magnitude, Color, Spectral Class
HR979 is also a Si chemically peculiar star.
The red dot in the diagram below shows where HR979 is situated in the HertzsprungāRussell diagram.
Star System Properties
HR979 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR979 double sysyem:
Distance, Radial Speed, Proper Motion
HR979 is distant 704.10 light years from the Sun and it is moving towards the Sun at the speed of 8 kilometers per second.
Alternative Designations
Visibility from Your Location
HR979 is circumpolar and transits at 01:46 UTC (altitude: 79.1°)