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
Today's ο Draconis (omicron Draconis) rise, transit and set times from Malapatan, Philippines are the following (all times relative to the local timezone Asia/Manila):