Celestial hemisphere:  Northern  ·  Constellation: Lyra (Lyr)  ·  Contains:  IC 1296  ·  M 57  ·  NGC 6720  ·  PGC 2017638  ·  PGC 2020007  ·  PGC 2021791  ·  PGC 2024204  ·  PGC 2813536  ·  PGC 2813611  ·  PGC 2813669  ·  PGC 2813726  ·  PGC 2813749  ·  PGC 2813775  ·  PGC 2813776  ·  PGC 2813834  ·  PGC 2813850  ·  PGC 2813896  ·  PK063+13.1  ·  Ring Nebula
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M 57: The Ring Nebula, Glenn Diekmann
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M 57: The Ring Nebula

Getting plate-solving status, please wait...
M 57: The Ring Nebula, Glenn Diekmann
Powered byPixInsight

M 57: The Ring Nebula

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Description

The Ring Nebula is the prototypical planetary nebula first described by Antoine Darquier de Pellepoix and Charles Messier in 1779. William Herschel later introduced the term "planetary nebulae" to describe such objects. The layered shell of ionized gas represents the atmosphere cast off by a star in its final phases of life. In the center of the nebula is a 15th-magnitutde white dwarf star, representing the naked core of the red giant star whose atmosphere produced the spectacular rings. The Ring Nebula is estimated to be about 2000 LY away and originated 6000–8000 years ago.

I am still fine tuning my imaging Newtonian and this is another test image. The short integration was not enough to bring out M57's faint outer shell of gas. Shooting during a full moon certainly did not help. The stars near the edge of the field were pretty terrible and had to be cropped out. I suspect poor collimation is the issue, and I plan to go through everything with a fine-toothed comb again.

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M 57: The Ring Nebula, Glenn Diekmann