The Wizard Nebula (NGC 7380) is an evocative emission nebula located approximately 7,200 light-years away in the constellation Cepheus. It gets its name from its uncanny resemblance to a hooded figure with outstretched arms, appearing to cast a spell over the stars of the Milky Way.
The "Wizard" is actually a massive cloud of gas surrounding a young open star cluster.
The Heart of the Magic: The star cluster was discovered by Caroline Herschel in 1787. These stars are extremely young, with an estimated age of less than 5 million years.
Illuminating the Fog: The intense radiation from these hot, massive stars is what causes the surrounding hydrogen gas to glow. Without this cluster, the nebula would remain a dark, invisible cloud of cold gas.
The intricate shapes that form the "wizard's" robe and hat are the result of a fierce battle between light and matter.
Radiation Pressure: The powerful stellar winds from the central stars act like a cosmic leaf blower, pushing the gas and dust outward.
Creating the Silhouette: The darker regions that define the figure's shape are dense lanes of dust that are resisting this pressure, creating a high-contrast silhouette against the glowing red hydrogen gas.
Deep within the "folds" of the Wizard's robes, the process of star birth is still very much active.
Protostars: Infrared observations have revealed dozens of "protostars"—stars that are still in the process of gathering mass from their parent clouds.
The Life Cycle: As these new stars "turn on," they will eventually blow away the remaining gas of the nebula, leaving behind only the sparkling star cluster we see today.
The Wizard Nebula is a massive structure that occupies a significant portion of its home constellation.
Physical Size: The nebula spans roughly 100 light-years across.
Apparent Size: In the night sky, it appears roughly the same size as the full moon, though it is far too faint to be seen without the help of a telescope or long-exposure camera.