
PICKERING’S TRIANGLE
NGC 6979 • Supernova remnant filament • Cygnus • 2400 light-years from Earth
🔭
Askar 130PHQ
📷
ZWO 2600MC Pro
🌃
Bortle 8
⏱️
17 hours
🗓️
August 2025
Overview
Pickering’s Triangle is the expanding remains of a massive star that exploded as a supernova sometime between 10,000 and 20,000 years ago. It stretches across 40 light-years of space, with thin, thread-like filaments glowing where shockwaves collide with interstellar gas.
From light polluted urban skies this structure is extremely subtle, but imaging allows its delicate filaments to be separated from background sky glow and recorded — but only if you’ve got sufficient integration time!
Background
I enjoyed processing my previous two targets (the Lion Nebula and Pelican Nebula) and was in the mood for another frame-filling colourful image. The Cygnus Loop was well-placed in the sky, but the entire object is too large for my Askar 130PHQ telescope. I decided to focus on the lesser-imaged part of this large complex: Pickering’s Triangle.
There’s not much SII in the region, so I just used my Optolong L-Ultimate filter (Hα/OIII), along with RGB real-colour stars. During processing I edited the Hα as orange, and the OIII as blue. The entire project only took a week, thanks to an unusual run of clear skies!
The naming of Pickering’s Triangle is a point of historical interest. The larger Cygnus Loop structure was spotted in 1784 by William Herschel, but its finer structures (including the Triangle) were only discovered in the 1900s when a photographic survey of the area was undertaken by Harvard Observatory. The Triangle was discovered in these photos by Willamina Fleming, but naming honours went to the Observatory’s director: Edward Charles Pickering.

Science
The story of Pickering’s Triangle begins 10,000 to 20,000 years ago, when a massive star, 2400 light-years from Earth, exploded as a supernova. The blast tore the star apart, sending shockwaves racing outward at 600,000 kilometres per hour, ploughing into the surrounding interstellar medium.
Pickering’s Triangle is a region where these shockwaves encounter clumps of gas at slightly different densities and speeds. This impact creates the knots and filaments visible in my image, stretching across about 40 light-years. The gas glows because it’s heated to millions of degrees and ionised by the energy of the expanding shockwave. Different elements produce different colours: during image processing I mapped hydrogen to orange and oxygen to light blue.
Below are a selection of close-crops highlighting shock fronts, where the supernova’s expanding shell impacts gas and dust, creating rippling effects. I think that each one looks like an abstract painting. Use the slider function for inverted views, which can help make the finer structures easier to see.








Kit list
This is the equipment I used to capture the image.
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Telescope: Askar 130PHQ
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Camera: ZWO ASI 2600MC Pro
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Mount: Sky-Watcher EQ6-R Pro
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Guidescope: William Optics 50mm with ROTO Lock
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Guidecam: ZWO ASI 120MM Mini
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Control: ASIAIR Plus
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Filter: Optolong L-Quad Enhance
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Filter: Optolong L-Ultimate
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Processing walkthrough
Example source data
Here are example single subframes and freshly integrated stacks, just with simple stretches applied.




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