The Pinwheel Galaxy (M101) from DESI Legacy Survey data reprocessed by Kyle Eberly — a sprawling face-on spiral in silver and cream, visibly lopsided, its western arms interrupted by a genuine dark gap.
Image data: DESI Legacy Imaging Surveys / DR9 (BASS, Bok 2.3-m telescope, Kitt Peak/NOIRLab/NSF/AURA), with gap repairs from Pan-STARRS DR1 (STScI / University of Hawaii) — public archives. Reprocessed from raw survey bricks by Kyle Eberly / Sitreps.

M101 — The Pinwheel, the Hard Way

Three broken data tiles, two telescopes, and a defect that turned out to be the galaxy

  • TelescopeBok 2.3-m · BASS (DESI Legacy Surveys) + Pan-STARRS
  • LocationKitt Peak, Arizona (survey archive)
  • ProcessingThe hardest field of the whole survey series — rebuilt from scratch after a dozen failed repair attempts on the first version. The working pipeline audits each of the nine raw data tiles against an independent Pan-STARRS reference BEFORE blending: three tiles turned out to be quietly defective and get outvoted by their healthy neighbors; zones where no healthy tile exists are patched with real Pan-STARRS data. Rendered from the two healthy color filters (the third was unusable field-wide), plus one surgical destripe.

What you're looking at

M101 is enormous — about 70% larger than the Milky Way, 21 million light years away, and tilted perfectly face-on, which is why it earns the name Pinwheel. At survey depth its arms resolve into hundreds of individual star-forming regions, several of which are so bright they carry their own NGC catalog numbers, assigned in the 1800s when astronomers mistook them for separate nebulae.

Look at the western (left) side: the arm pattern breaks. There's a genuine dark gap where the spiral rhythm stumbles — M101 is one of the most lopsided large spirals known, yanked out of symmetry by gravitational encounters with its companion galaxies. The asymmetry isn't a flaw in the image. It's the galaxy's biography, written in its shape.

And that gap is the point of this entry's story. In the first version of this image, built on broken data, the gap looked like an obvious processing defect — an opaque hole. I spent hours trying to repair it. The fix came from checking a second, completely independent telescope: Pan-STARRS sees the same dark gap. Two unrelated instruments agreeing means the anomaly is in the sky, not the camera.

The lesson

I spent hours trying to fix a defect that turned out to be the galaxy.

The broken early versions of this image exaggerated a real feature — M101's genuine lopsidedness — into something that looked like damage. Every repair attempt made the picture worse, because the thing I was repairing wasn't broken. The answer came from an independent reference: a second telescope that sees the same sky confirmed the gap is real.

Veterans do this to themselves constantly. You hold your record up against the corporate template, and the parts that don't match — the nonlinear path, the weird specialty, the gap the military carved into you — look like defects to fix, sand down, or hide. Check an independent reference first: the people who know your work. Some of what you're trying to repair is your actual shape, and the shape is the story.

Fix what's broken. Keep what's you. The skill is telling them apart — and you usually can't do it alone.

Object data

Catalog
M101 · NGC 5457 · the Pinwheel
Constellation
Ursa Major
Type
Face-on spiral, strongly lopsided
Distance
~21 million light-years
Diameter
~170,000 light-years — ~70% larger than the Milky Way
Telescopes
Bok 2.3-m (BASS) + Pan-STARRS 1.8-m (archival)
Data verdict
3 of 9 survey tiles defective; the dark western gap is real — confirmed by two independent surveys
Companion entries
/astronomy/m101 (Bortle 6) and /astronomy/m101-dark-sky (Bortle 2) — my own Seestar captures

What's next

A batch of galactic-plane nebulae from the Pan-STARRS archive — the Legacy Surveys avoid the Milky Way’s plane, so the emission-nebula showpieces need a different data source.

One photo. One lesson.

New entries land when the sky cooperates. Get them by email — no schedule, no spam, just what the telescope caught and what it taught.