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NGC 7822 is a stunning emission nebula and star-forming region located in the constellation Cepheus, approximately 3,000 light-years away from Earth. This vibrant nebula is part of a larger complex that includes the young open cluster Berkeley 59, whose hot, massive stars energize the surrounding gas, causing it to glow in brilliant shades of red and pink from ionized hydrogen.
The nebula is particularly striking due to its intricate pillars, cavities, and dark dust lanes, sculpted by stellar winds and radiation from newly formed stars. These structures give it a dramatic, almost three-dimensional appearance when viewed through telescopes or in astrophotography. NGC 7822 is not only visually captivating but also scientifically important, as it offers astronomers a window into the processes of star birth and the evolution of interstellar clouds.
Overall, NGC 7822 is a vivid and dynamic stellar nursery, combining glowing gas, dark filaments, and young star clusters into a mesmerizing celestial tapestry within the northern skies.
Technical Details
Telescope: Sky-Watcher Esprit 100ED Refractor
Auto Focus: ZWO Electronic Auto Focuser
Astronomy Camera: ZWO ASI533MC Pro
Filter: Optolong UV-IR cut filter; 480 exposures @ 60 seconds each (8 hours)
Filter: Antlia ALP-T Dual Narrowband Ha/Oiii Filter; 400 exposures @ 5 minutes each (33.3 hours)
Total Integration Time: 51.3 hours
Auto Guiding: William Optics Uniguide 50mm Guide Scope
Auto Guiding Camera: ZWO ASI120MM Mini Guide Camera
Auto Guiding Software: PHD2
Telescope Mount: Celestron CGX Equatorial Mount
Telescope Computer: BeeLink GK-55 Mini PC / Windows 10 Pro
Wireless Communication: GL-iNEt Beryl Travel Router
Telescope Control & Image Capture Software: Nighttime Imaging ‘N’ Astronomy (N.I.N.A.)
Image Integration Software: Astro Pixel Process, by Aries Productions
Image Post Processing Software: PixInsight, by Pleiades Astrophoto
Images captured: Palm Springs, CA during October 2023. Dark sky classification = Bright suburban sky (Bortle 6)
