M27 Dumbell Nebula

M27 Dumbell Nebula
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M27 Dumbell Nebula

The Dumbbell Nebula (also known as the Apple Core Nebula, Messier 27, and NGC 6853) is a planetary nebula (nebulosity surrounding a white dwarf) in the constellation Vulpecula, at a distance of about 1360 light-years.[1] It was the first such nebula to be discovered, by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and diameter of about 8 arcminutes, it is easily visible in binoculars[4] and is a popular observing target in amateur telescopes.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
SPA-2-CMOS
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600M
Location ..........................................................................................................................................................................................................................
Location
Spain
Date of observation ..........................................................................................................................................................................................................................
Date of observation
06-07 August 2023
Filters ..........................................................................................................................................................................................................................
Filters
HSO
Processing ..........................................................................................................................................................................................................................
Processing
Affinity Photo
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