NGC 6979 (Pickering's Triangle)
Photo description / processing
The central region of the Veil Nebula, Pickering's Triangle (or Pickering's Triangular Wisp)
These clumps of gas are all that remains visible of a Milky Way star. Many thousands of years ago, this star exploded as a supernova, leaving behind the Veil Nebula. At that time, the expanding cloud was likely as bright as a crescent moon in the constellation Cygnus and was visible for several weeks to people living at the dawn of recorded history. The supernova remnant lies about 1,400 light-years away and spans an area five times the diameter of the full Moon. The Veil Nebula is also known as the Cygnus Loop.
Technical information
- Telescope/Lens
- William Optics Zenithstar ZS 61
- Camera
- ZWO ASI533MC Pro
- Mount
- iOptron SkyGuider Pro
- Guide Scope
- SVBONY 120mm
- Guide Camera
- ZWO ASI120MM Mini
- Software
- Pixinsight, Adobe Photoshop
Exposure
- 60 × 120″ · ISO/Gain: 101 · Optolong L-extrme ·
Total exposure: 2 h 0 m




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