The Veil Nebula Complex (also known as the Cygnus Loop) is one of the most breathtaking examples of a supernova remnant in our galaxy. While the other nebulae we've discussed are "nurseries" where stars are born, the Veil is a "graveyard"—the expanding debris field of a massive star that exploded thousands of years ago.
Located roughly 2,100 to 2,400 light-years away in the constellation Cygnus (The Swan), this complex is so large that it is divided into several distinct sections, each with its own famous nickname.
Approximately 10,000 to 20,000 years ago, a star roughly 20 times the mass of our Sun reached the end of its life.
The Explosion: When it went supernova, it would have been bright enough to be seen during the day and would have outshone the planet Venus in the night sky.
The Expansion: The debris is still hurtling outward today at a staggering 1.5 million kilometers per hour. As this material slams into the cold gas of interstellar space, it creates the glowing filaments and "veils" we see.
The complex is so massive—covering an area six times the diameter of the full moon—that astronomers usually observe it in parts.
Officially cataloged as NGC 6960, this segment looks remarkably like an old-fashioned broomstick.
The Marker Star: It is incredibly easy to find because it appears to pass directly behind the bright star 52 Cygni, which is visible to the naked eye. (Note: The star is actually much closer to Earth and just happens to be in the same line of sight!)
Cataloged as NGC 6992 and NGC 6995, the Eastern Veil is often considered the most beautiful part. It looks like a delicate piece of lace or a tangled web of neon-colored threads.
Found between the two main arcs, this triangular wisp was discovered in 1904 by Williamina Fleming (the same woman who discovered the Horsehead Nebula). It was named after the observatory director, Edward Pickering, though Fleming did the actual work of identifying it on photographic plates.
The Veil Nebula is a perfect example of how the universe recycles itself. The explosion that created the nebula didn't just destroy a star; it forged heavy elements like calcium, iron, and silicon.
As the nebula expands and eventually fades, these elements will mix into the surrounding space.
Millions of years from now, these very atoms may collapse into a new cloud of gas to form new stars and planets—just as the elements in our own bodies were once forged inside an exploding star.