The Witch's Broom (NGC 6960, Western Veil) photographed from Lakeway, Texas with a ZWO Seestar S50 — a braided blue-white filament shaft running through the bright star 52 Cygni, with red nebulosity flanking it.

NGC 6960 — The Witch's Broom

The Western Veil, with a naked-eye star impaled on it

  • TelescopeDarth Vader (ZWO Seestar S50)
  • Integration80 minutes
  • LocationLakeway, TX
  • SkyBortle 6
  • CapturedSep 22, 2026
  • PhotoKyle Eberly · © 2026
  • ProcessingDual-filter composite: the vivid emission filaments from an 80-minute light-pollution-filter stack, combined with true star colors from a separate broadband (IRCUT) session on the second telescope. Fixes the pink star cast that the narrowband filter leaves behind

What you're looking at

This is the western arc of the same explosion featured in the Eastern Veil entry — the other edge of the expanding shock bubble, 10,000 years along. The braided shaft is where the blast wave slices through interstellar gas nearly edge-on to our line of sight, compressing it into glowing filaments.

The bright star skewered through the middle, 52 Cygni, is a complete coincidence — a foreground star barely 200 light years away, ten times closer than the nebula behind it. It's bright enough to see with the naked eye, which makes the Broom one of the easiest deep-sky objects to *find* and one of the hardest to photograph well: the star constantly threatens to overwhelm the wisps.

Together with the Eastern arc, the two Broom-and-Bone halves bracket a bubble of shocked gas roughly 120 light years across — large enough that light from one edge takes more than a century to reach the other.

The lesson

This target was recommended, scheduled, and postponed twelve separate times over three weeks. Every night, something newer or shinier won the telescope.

It was never hard. It was never risky. It was the single highest-confidence target on the list — which is exactly why it kept losing to things that felt more urgent. Guaranteed wins don't generate urgency.

The important-but-not-urgent quadrant is where sure things go to wait. Put them on the calendar like they're emergencies, because nothing else will ever make room for them.

Same nebula, from the Hubble Space Telescope

A section of the Veil Nebula from Hubble WFC3 data reprocessed by Kyle Eberly — braided teal oxygen ribbons and red hydrogen filaments sweeping diagonally over a dark star field.
A single ribbon of the same supernova remnant through Hubble — the shock front itself, braided teal [OIII] and red hydrogen. My whole Witch's Broom frame spans the Seestar's field; this covers a sliver of one filament at 60× the detail.

Image data: NASA/ESA Hubble Space Telescope, obtained from the Space Telescope Science Institute (STScI), program 14056 (WFC3/UVIS) — public archive. Reprocessed from drizzled archive mosaics by Kyle Eberly / Sitreps.

My telescope
ZWO Seestar S50 — a 50 mm (2-inch) lens
This telescope
Hubble, 2.4-meter mirror, low Earth orbit — ~2,300× more light-collecting area
Pixel scale
2.4″/px (Seestar) vs 0.04″/px (WFC3) — about 60× finer detail
The data
Five filters from the public MAST archive — broadbands for the stars, hydrogen and oxygen lines at their true hues

Same object, same physics. Hubble gathers over two thousand times the light with no atmosphere in the way — and its archive is public. The raw files still needed the same work my backyard frames do: alignment, chip-seam repair, color balance. The instrument buys you photons; the processing still has to earn the picture.

One photo. One lesson.

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Object data

Catalog
NGC 6960 · Caldwell 34 (Western Veil)
Constellation
Cygnus
Type
Supernova remnant (Cygnus Loop)
Distance
~2,400 light-years
Foreground star
52 Cygni — ~200 light-years, unrelated, naked-eye visible
Companion entry
/astronomy/veil-nebula-east — the other half of the blast
Discovery
1784 · William Herschel