If you’re looking to be swept away by delicate detail and dramatic structure, the Veil Nebula is one of the most spectacular sights in the sky. Located in the constellation Cygnus, this sprawling supernova remnant is the glowing wreckage of a star that exploded over ten thousand years ago. What remains are vast, wispy filaments of ionized gas stretching across more than 3 degrees of sky—about six times the width of the full Moon.
The Western Veil, often called the Witch’s Broom Nebula (NGC 6960), sweeps past the bright star 52 Cygni and features long, elegant tendrils that curve and twist like smoke trails frozen in time. The Eastern Veil (NGC 6992/6995) is brighter and more densely structured, full of intricate, lace-like threads that shimmer beautifully under the right conditions.
What makes the Veil so enticing is how dramatically it responds to OIII or UHC filters, which bring out its contrast and reveal fine details even in moderate apertures. With a wide-field telescope or large binoculars under dark skies, you can trace its full arc and appreciate its sheer scale. It’s not just a pretty nebula—it’s a visual tour of a stellar cataclysm, beautifully stretched across the summer sky. If you want to feel like you’re drifting through the remnants of a shattered star, the Veil is a must-see.
Veil Nebula/C33-34
Rating: 🔵 Stagazer Favorite
Level: 🟡 Challenging
How:
When: Jul - Oct
🌟 Striking Filamentary Structure Unlike many faint nebulae that appear as soft glows, the Veil is filled with sharp, thread-like filaments that twist and weave like glowing strands of smoke. These fine details create an almost three-dimensional effect in the eyepiece and reward slow, careful observing.
🌟 Visually Dramatic with Filters The Veil Nebula responds exceptionally well to narrowband filters, especially OIII and UHC. These filters make the faint nebulae stand out with dramatic contrast, even in moderate light pollution. With them, the fine arcs and knots become crisp and vivid against the background sky.
🌟 Impressive Scale and Scope Spanning more than 3 degrees across the sky, the Veil Nebula complex is vast. When viewed with wide-field optics, you can trace entire arcs of supernova shockwave, making it one of the few deep-sky objects where you can truly feel the scale of a cosmic explosion.
🌟 Two Distinct and Beautiful Halves The Western Veil, near the star 52 Cygni, is bold and sculpted, with a sweeping, broom-like curve. The Eastern Veil is more complex, featuring overlapping strands and brighter arcs. Observing both gives you two very different visual experiences from the same ancient event.
🌟 Ideal for Summer and Early Fall High in the sky during the late summer and early autumn months, the Veil Nebula rides through Cygnus while the Milky Way is at its best. It’s perfectly placed for long, uninterrupted observing sessions under dark skies.
🌟 A Glimpse into Stellar Death The Veil isn’t just visually stunning—it’s a direct look at the aftermath of a supernova. Studying it connects you to the dramatic life cycle of stars and offers a rare chance to observe what’s left of a once-massive star that shaped its surrounding space.
Veil Nebula/C33-34
Names
Veil Nebula, Western: NGC 6960, C34, Witch's Broom, Eastern: NGC 6995/6992, C33
Supernova remnant: the expanding cloud of gas and debris left behind after a massive star explodes in a supernova.
Veil Nebula/C33-34
Find the Summer Triangle and then hop to Gienah (+2.49) in Cygnus.
With binoculars or a telescope finder, point to the halfway point between Gienah and Zeta Cygni. With binoculars or a low-powered eyepiece, hop to the Eastern Veil Nebula and explore it. The Eastern Veil appears as a bright, sharply curved filament, often brighter and more detailed than the Western arc. Under dark skies and with a OIII or UHC filter, the structure may appear multi-layered and web-like. When ready, hop to 52 Cygnus and explore the Western View Nebula. With an OIII or UHC filter, you’ll begin to see the delicate strands fan out like a tattered ribbon.
Bonus: sweep the area between the two arcs and detect the central filament (Pickering’s Triangle), which lies roughly halfway between the Eastern and Western sections.
Veil Nebula/C33-34
✅ Use an OIII or UHC Filter The Veil Nebula is faint but responds incredibly well to narrowband filters. An OIII filter brings out the glowing filaments with stunning contrast, while a UHC filter boosts overall visibility. Either filter can make the nebula “pop,” even under moderate skies.
✅ Choose a Wide Field of View Because the Veil spans over 3 degrees, you’ll want a wide-field eyepiece or short focal length telescope to see its full extent. For the best experience, aim for a field that’s at least 1.5 to 2 degrees wide.
✅ Observe Under Dark Skies Light pollution washes out the delicate details. To see the full beauty of the Veil, especially the fainter arcs and internal structure, try to observe from a Bortle 1–3 site. The darker the sky, the richer the view.
✅ Start with the Eastern Veil The Eastern Veil (NGC 6992/6995) is brighter and more detailed, making it easier to find and more immediately rewarding. Once your eye adjusts and you’ve located the brighter sections, move westward to explore the Witch’s Broom.
✅ Use Averted Vision and Take Your Time The Veil’s filaments are subtle. Use averted vision—looking slightly to the side of the nebula—to draw out more detail. Let your eyes adapt and sweep slowly across the arcs to appreciate the structure.
✅ Star Hop from 52 Cygni for the Western Veil To find the Witch’s Broom, begin at the star 52 Cygni, which lies right in the middle of the Western arc. Center it in your eyepiece, then move around it slowly—you’ll start to see the veil’s wispy strands emerge from the starlight.
Veil Nebula/C33-34
❌ Naked Eye
With the naked eye, the Veil Nebula is invisible under most conditions, even from very dark sites, due to its extremely low surface brightness.
⚠️ Binoculars
Through binoculars, especially under dark skies, the broader glow of the Eastern Veil may be faintly detected as a ghostly arc, while the Western portion near 52 Cygni remains elusive. Binoculars may reveal a sense of size, but not structure.
✅ Small Telescope
In a small telescope without filters, both portions of the Veil are challenging and often disappointingly faint. However, with the addition of an OIII or UHC filter, the Eastern Veil begins to show as a thin, wispy band, and the Witch’s Broom around 52 Cygni takes on a soft curve. The structure is present but requires dark skies and time at the eyepiece.
✅ Medium Telescope
With a medium telescope and filters, the Veil transforms. The Eastern portion becomes rich with texture, revealing overlapping filaments and branching arcs, while the Western Veil sharpens into a dramatic, broom-like sweep trailing away from 52 Cygni. The sense of motion and detail increases, and you can begin to trace long sections of the remnant’s arc.
✅ Large Telescope
In a large telescope, both portions of the Veil become intricate and breathtaking. The Eastern side reveals layered threads and knots of glowing gas, while the Western arc stretches thin and bright, curving dramatically with clear variation in brightness along its length. At this level, both sides offer fine structure and depth, and the entire nebula feels like a living sculpture of interstellar light.
Veil Nebula/C33-34
The Veil Nebula is a filter-friendly, low-surface-brightness object that thrives in dark skies. In Bortle 1–2 conditions, it shows sweeping, filamentary beauty across both arcs. From Bortle 5 upward, it fades quickly and becomes nearly inaccessible, highlighting how crucial sky quality is to appreciating this intricate supernova remnant.
🟣 In Bortle 1–2 skies, the Veil Nebula is a stunning display of delicate, glowing filaments stretching across the rich star field of Cygnus. Both the Eastern and Western portions are well defined, with the Eastern showing layered arcs and the Western curving dramatically past 52 Cygni. With filters, fine structure and texture emerge clearly, giving the nebula a lace-like appearance.
🔵 In Bortle 3–4 skies, the Veil remains a rewarding target. The Eastern arc is still bright and detailed with a filter, though some fainter extensions fade. The Western Veil is more subdued but still visible and recognizable. Contrast is reduced, but the main structure holds up well.
🟡 In Bortle 5–6 skies, the Veil becomes more elusive. Without a filter, it’s nearly invisible. With an OIII or UHC filter, the Eastern portion appears faint but traceable, while the Western portion is difficult and often lost in the skyglow. The overall impression is dim and flattened.
🔴 In Bortle 7+ skies, the Veil is extremely difficult or invisible. Even with filters, the nebula struggles to stand out against the bright background, and only small fragments may be glimpsed with effort and large aperture. The scale and beauty of the structure are lost.
Veil Nebula/C33-34
DSOs within 48° or 2 outstretched hands at arm's length