Bubble Nebula (NGC 7635) - SHO

Stellar wind bubble in Cassiopeia with 29 hours of integration

Bubble Nebula (NGC 7635) - SHO

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Deep Space Capture

Technical Specifications

Resolution: 6000x4000 (cropped and drizzled 3x)

Integration: Ha: 113×300s, OIII: 160×300s, SII: 77×300s

Captured: Captured over approximately one week

Equipment: Redcat71 refractor (350mm) with ZWO ASI2600MM Pro camera on Advanced VX mount

Location: Backyard location with exceptional seeing conditions

Processing Workflow

Total integration time: 29 hours across three narrowband filters
No calibration frames used - lights only acquisition
Each sub-exposure dithered max 10 pixels in RA only
Exceptional guiding: RMS consistently 0.15-0.35 arcseconds
Drizzle integration at 3x scale for enhanced resolution
Advanced SHO processing workflow with Topaz DeNoise AI finishing

Scientific Context

NGC 7635, also known as the Bubble Nebula, Sharpless 162, or Caldwell 11, is an HII region emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7 magnitude young central star, SAO 20575.

The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow. It was discovered in 1787 by William Herschel.

This project was an experiment to push the limits of the Redcat 71 + ASI2600MM combination on a very small target. The Bubble Nebula is typically imaged with focal lengths of 1000mm or more, but this image demonstrates what's possible with careful processing techniques including dithering, drizzling, and extensive integration time.

The final image is cropped and drizzled 3X to enhance resolution, with a total of 29 hours of sub-exposures captured over about a week. The excellent guiding conditions (RMS consistently between 0.15-0.35 arcseconds) were crucial for the success of this challenging target with the relatively short 350mm focal length.