Captured under pristine dark skies near Richfield, this image shows the Crab Nebula, the expanding remnant of a supernova observed on Earth in 1054 AD. At roughly 6,500 light-years away, the nebula is powered by a rapidly spinning neutron star whose intense magnetic field drives the intricate web of glowing filaments seen here.

This image was captured over 5–6 hours using a dual-band Hα/OIII filter, allowing the ionized hydrogen and oxygen structures to be isolated and blended into a balanced bi-color presentation. Hydrogen highlights the dense filamentary shell, while oxygen traces the more energetic shock regions threaded throughout the remnant.

Even in a relatively compact target like M1, extended integration under dark skies reveals remarkable internal complexity — a constant reminder that some of the most dramatic objects in the sky fit into surprisingly small patches of space.