NGC 7380 The Wizard Nebula

The Wizard Nebula (NGC 7380) is an active stellar nursery. At the cluster’s heart is DH Cephei, an exceptionally massive, hot double-lined binary system of two O-type stars. These colossal central stars power the nebula. They flood the surrounding hydrogen gas with intense ultraviolet radiation, exciting atoms and causing them to glow with a deep red hue (a classic characteristic of H II emission regions). At the same time, powerful stellar winds and radiation pressure push back the cooler, denser outer walls of gas and dust, sculpting them into jagged columns and carving out the eerie wizard shape over millions of years.
While the open star cluster is visible through a modest amateur telescope under dark skies, the gas clouds forming the actual “Wizard” shape have extremely low surface brightness. They are virtually invisible to the naked eye and require specialised equipment. Seeing the faint nebulosity typically requires exceptionally clear, light-pollution-free skies, a large-aperture telescope, and an O-III (Oxygen-III) or UHC contrast filter.
It is a highly celebrated target for deep-sky imaging. To cut through light pollution and reveal the intricate red (Hydrogen-alpha), green/blue (Oxygen-III), and gold (Sulfur-II) structural layers, astrophotographers rely heavily on long-exposure narrowband imaging (often processed using the Hubble Palette). The image shown here is processed slightly differently. Instead of deep red clouds, it shows the bright centre surrounded by purple and gold clouds and veils. Because of the limited material (due to the tracker malfunctioning as of 2nd October 2026), I am presenting the picture that consists only of the narrow-band frames. I hope I have fixed the tracker issues, and I am now gathering material for a new, much better photograph of this object.