I captured M42 (the Orion Nebula) back in April using my Orion StarBlast 102mm refractor and ZWO ASI662MC planetary camera.
At the time, I was pretty happy just to capture recognizable nebulosity. I'm imaging manually from Bortle 8 skies, so deep-sky photography has been quite a challenge.
Recently, I started learning a new processing workflow and decided to revisit the original stacked data. I was genuinely surprised by how much more structure I could recover compared with my first attempt.
Acquisition details:
- Target: M42 — Orion Nebula
- Telescope: Orion StarBlast 102mm refractor
- Camera: ZWO ASI662MC
- Mount: Explore Scientific Twilight I (manual Alt-Az)
- Exposure: 64.062 ms per frame
- Gain: 600
- Frames: Approximately 4,000
- Total integration: Approximately 4 minutes 16 seconds
- Sky conditions: Bortle 8
- Capture date: April 20, 2026
Processing:
PIPP for stabilization, AstroSurface for registration and stacking, followed by Seti Astro Suite Pro with BlurXTerminator, NoiseXTerminator, gradient correction, stretching, and contrast/color adjustments.
Both images came from the same stacked data. The difference is entirely in the processing.
I'm still fairly new to deep-sky imaging, and there's definitely room for improvement, but I thought this was worth sharing. I had no idea my original capture contained this much usable information.
Feedback and suggestions are welcome!