Supernova remnants are the glowing debris of immense stellar explosions. When a massive star is torn apart as a supernova at the end of its life, or a white dwarf perishes in a thermonuclear blast, it hurls its material into space at thousands of kilometres per second. Over thousands of years these shells expand, making the surrounding gas glow and forming delicate, filamentary structures. The Veil Nebula in Cygnus is perhaps the best-known example and a classic narrowband target. Oxygen often appears in soft blue-green and hydrogen in deep red. Photographically, supernova remnants are demanding: they are extended, faint, and reveal their delicate structure only in long narrowband exposures under dark skies. That is exactly what makes them such rewarding, striking targets. This page gathers every supernova remnant I have photographed so far. Click into any object to learn more about it and see all the astrophoto posts it appears in.
Supernova Remnants
Supernova remnants are the glowing debris of exploded stars, like the Veil Nebula. This page shows every supernova remnant I have photographed so far – each with its own object page.







