HR2579
HR2579 is a double main-sequence star of spectral class B8 in the constellation of Puppis.
HR2579 visual magnitude is 6.46. Because of its faintness, HR2579 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 HR2579.
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR2579 is situated in the HertzsprungāRussell diagram.
Star System Properties
HR2579 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR2579 double sysyem:
Distance, Radial Speed, Proper Motion
HR2579 is distant 423.93 light years from the Sun and it is moving far from the Sun at the speed of 26 kilometers per second.
Alternative Designations
Visibility from Your Location
HR2579 is currently not visible from Greenwich, UK