ScienceDownEast | ScienceDownEast Astrophotography | Nebulae | NGC 6960 Veil Nebula | NGC 6992 Eastern Veil Nebula

NGC 6992 Eastern Veil Nebula
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The Eastern Veil Nebula (NGC 6992/6995, with adjacent filaments cataloged as IC 1340) is a bright, richly structured portion of the larger Veil Nebula supernova remnant in Cygnus. It marks part of the shock front from a massive star that exploded thousands of years ago, sending a blast wave plowing through the surrounding interstellar medium. Seen edge-on, the Eastern Veil appears as delicately woven filaments and curtains of gas, with especially strong O III and Hα emission tracing the expanding shock.

At an estimated distance of about ~2,400 light-years in the Orion–Cygnus arm of the Milky Way (Veil Nebula overview), the entire remnant spans roughly 100 light-years across, but individual arcs like NGC 6992 cover only a fraction of that on the sky. Narrowband filters isolating O III and Hα are especially effective on this target, helping the glowing shock fronts stand out sharply against the dense star field of Cygnus and revealing the intricate, lace-like structure of the remnant. Look for NGC 6992 just east of the brighter Western Veil (NGC 6960, the “Witch’s Broom”), near the rich Milky Way band running through Cygnus. [generated by ChatGPT]

Total image time was 2 hour and 40 minutes.

Moon PhaseNew Moon
Exposure8 x 20 min
Gain100
CameraToupTek ATR2600C [6224 × 4168]
Optics120mm Sky-Watcher Esprit on a Proxisky UMi20S Strain Wave mount
GuidingToupTek GPM462M using PHD2 with a 400mm guide scope. Average 15-min sub GuideRMS ranged from 0.56 to 0.89 using 0.5s exposures.
ControllerKStars on MeLe Quieter 4C
FilterTriad Quad Ultra (strong Hα / O III response for emission nebulae and supernova remnants)
LocationSt. Croix Observatory, Nova Scotia.
Date2025-11-20
ProcessingProcessed in PixInsight.
PixInsight Processing
WeightedBatchPreprocessing Script
BlurXTerminator
GraXpert
Screen Stretch and Histogram Transformation
NoiseXTerminator
StarXTerminator
Generalized Hyperbolic Stretch on both the stars and starless images
HDRMultiScaleTransform on the Starless image (to bring out bright filaments and shock fronts)
PixelMath to recombine the images
CurveTransformation




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