Mu Draconis (µ Draconis, µ Dra) is a binary star with a combined magnitude of 4.92^m located approximately 85 light years from the Solar System, near the head of the constellation Draco. The component stars are nearly identical yellow-white stars in a tight 672 year orbit. Each is of the spectral class F7V and has a visual magnitude of 5.8^m. Under ideal seeing conditions, the pair can be resolved with a small aperture telescope at about 120 power.