Astrophotography by Keith B. Quattrocchi
NGC 6888
NGC 6888 (The Crescent Nebula) in Cygnus
Narrow Band Image
Copyright 2021
Keith B Quattrocchi and Bray Falls
Image Acquisition Information
Telescope: 16" RCOS Richey Chretien Telescope (ion milled at f/9)
Camera: ZWO Full Frame Back Illuminated CMOS ASI 6200 MM
Guiding: Starlight Xpress AO with UltraStar Autoguiding Camera (AO control using maxim DL software).
Filters: Astrodon LRBG, H-alpha, S-II and OIII Filters
Acquisition Programs: NINA, The SkyX, PHD2, PWI4
Processing Programs: PixInsight, RC Astro, CCDStack, Photoshop CS4
Date: Data processed on September 1, 2021. Data acquisition: August of 2021
Time: 8 hours (10 minute exposures) for each of Ha, SII, OIII for a total of 24 hours. LRGB starfield also obtained.
Image Information: NGC 6888, also known as the Crescent Nebula, is an emission nebula in the constellation Cygnus, located about 5,000 light-years away. It is an emission nebula, meaning it glows and produces its own light, formed by the interaction of a massive, dying Wolf-Rayet star with the gas it ejects. This stellar wind has created a complex shell of gas, and the collision has also generated shock waves that heat the gas to millions of degrees.
Processing Information This Ha/SII/OIII images were obtained using AstroDon filters. The Ha/S-II/OIII images were batch processed (calibrated, registered, normalized and integrated) in PixInsignt. Further stretching, high pass filtering and background smoothing was performed with Adobe Photoshop CS/4 and PixInsight.
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Located at Sierra Remote Observatories Auberry, California Copyright 2004-2025 Keith B Quattrocchi |