RING NEBULA

RING NEBULA
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RING NEBULA

The Ring Nebula (also catalogued as Messier 57, M57 or NGC 6720) is a planetary nebula in the mildly northern constellation of Lyra. Such nebulae are formed by a starburst – ionized gas has expelled into the surrounding interstellar medium by a star to form a vast luminous envelope containing the star in its last stages of its evolution before becoming a white dwarf.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Officina Stellare 700 RC
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL16803
Location ..........................................................................................................................................................................................................................
Location
Oria, Almería, Spain
Date of observation ..........................................................................................................................................................................................................................
Date of observation
04 August 2021
Filters ..........................................................................................................................................................................................................................
Filters
HSO
Processing ..........................................................................................................................................................................................................................
Processing
Affinity Photo | JR Astrophotography Macros | Nik Collection
Credits ..........................................................................................................................................................................................................................
Credits
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