Located in the heart of the Orion constellation, the Horsehead Nebula and the Flame Nebula form one of the most iconic duos in the night sky. Found just below Alnitak—the easternmost star in Orion’s Belt—these two objects offer a masterclass in the different ways gas and dust interact with starlight.
Perhaps the most recognizable shape in all of astronomy, the Horsehead is a dark nebula. Unlike the glowing clouds around it, this nebula is a dense, cold pocket of dust and gas that blocks the light from behind it.
A Cosmic Silhouette: The "horse" shape is only visible because it is backlit by the bright, pinkish emission nebula IC 434.
The Sculptor: The top of the horse's head is being eroded and shaped by the intense radiation of a nearby massive star, Sigma Orionis.
Discovery: It was first identified in 1888 by Williamina Fleming, a Scottish astronomer who worked as a "computer" at the Harvard College Observatory.
Sitting right next to the Horsehead, the Flame Nebula looks like a flickering campfire in space. It is an emission nebula, meaning it glows with its own light.
The Power Source: The bright star Alnitak (the belt star) blasts the nebula with ultraviolet light. This strips electrons from hydrogen atoms; when they recombine, they release energy as the orange and yellow glow we see.
Hidden Stars: While it looks like a simple cloud, X-ray observations have revealed a cluster of several hundred young stars hidden behind its thick lanes of dust.
Young and Vibrant: Most stars in this cluster are less than one million years old—extremely young in cosmic terms.
Both the Horsehead and Flame are tiny pieces of a much larger structure called the Orion Molecular Cloud Complex. This massive "star factory" stretches hundreds of light-years and includes other famous sights like the Orion Nebula (M42) and Barnard’s Loop.