Your guide to astrophotography

NGC 7380, located in the constellation Cepheus, is an open cluster of stars energizing the remaining gas and dust in the surrounding area. Over the next 100 million years, the nebula part of the cluster will eventually dissipate into nothingness, but the remaining stars will most likely last longer than our solar system.

NGC 7380 is 7,200 light years away, which means these images are capturing the cluster as how it appeared 7,200 years ago

NGC 6888, located in the constellation Cygnus, is an emission nebula. This nebula is lit by a central star within the nebula.

Sometime between 250,000 to 400,000 years ago, this star ejected a stellar shell when it ballooned to a red giant star. Since that time, the central star is nearing the end of it’s life and the stellar winds have greatly increased (now categorized as a Wolf-Rayet star) resulting in another stellar shell.

The two different stellar shells are colliding, creating one outward moving shockwave and one inward moving shockwave. This is why the image appears to have two distinct shells.

NGC 6992 is the eastern portion of the Cygnus Loop, which is a supernova remnant (exploding star) roughly 2,400 light years away in the constellation Cygnus. The originating star, which was 20 times more massive than the sun, exploded 10,000 to 20,000 years ago leaving behind the Veil Nebula.