HR4180
HR4180 is a multiple supergiant star of spectral class G2 in the constellation of Vela.
HR4180 visual magnitude is 4.28. Because of its moderate brightness, HR4180 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
Simplified finder chart for HR4180.
Magnitude, Color, Spectral Class
The red dot in the diagram below shows where HR4180 is situated in the HertzsprungāRussell diagram.
Star System Properties
HR4180 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR4180 double sysyem:
Distance, Radial Speed, Proper Motion
HR4180 is distant 900.55 light years from the Sun and it is moving far from the Sun at the speed of 20 kilometers per second.
Alternative Designations
Visibility from Your Location
HR4180 is currently not visible from Greenwich, UK