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Ring Nebula. M 57, [1] NGC 6720, [1] GC 4447. The Ring Nebula (also catalogued as Messier 57, M57 and NGC 6720) is a planetary nebula in the northern constellation of Lyra. [4] [. C] Such a nebula is formed when a star, during the last stages of its evolution before becoming a white dwarf, expels a vast luminous envelope of ionized gas into the ...
English: HaRGB image of The Ring Nebula (M57) showing the faint outer shells. Data from the Liverpool Telescope (a 2 m RC telescope on La Palma) processed by Göran Nilsson. 67 exposures totalling 1.9 hours
English: Ring Nebula (M57), taken with eVscope eQuinox from Saint-Antoine-l'Abbaye, France. 10' pose. Français : Nébuleuse de la Lyre (M57), prise avec eVscope eQuinox depuis Saint-Antoine-l'Abbaye, France.
“The bright iconic ring structure of the nebula is composed of about 20,000 individual clumps of dense molecular hydrogen gas, each of them about as massive as the Earth,” Wesson wrote.
In 1991, Newton became the first amateur astrophotographer to make full color CCD images of celestial objects using a Santa Barbara Instruments Group ST-4 camera, making a full color CCD image of M57, the "Ring Nebula" and M27, the "Dumbbell Nebula".
Dumbbell Nebula. known for a white dwarf. 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.
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