ο Draconis (omicron Draconis)
ο Draconis is a variable and multiple giant star of spectral class G9 in the constellation of Draco.
ο Draconis visual magnitude is 4.66. Because of its moderate brightness, ο Draconis 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 ο Draconis is situated in the Hertzsprung–Russell diagram.
Star System Properties
ο Draconis is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the ο Draconis double sysyem:
Distance, Radial Speed, Proper Motion
ο Draconis is distant 322.13 light years from the Sun and it is moving towards the Sun at the speed of 20 kilometers per second.
Alternative Designations
Visibility from Your Location
ο Draconis (omicron Draconis) is circumpolar and transits at 22:52 UTC (altitude: 81.9°)