Celestial hemisphere:  Northern  ·  Constellation: Lyra (Lyr)  ·  Contains:  IC 1296  ·  M 57  ·  NGC 6720  ·  PGC 2017638  ·  PGC 2024204  ·  PGC 2813669  ·  PGC 2813726  ·  PGC 2813749  ·  PGC 2813775  ·  PGC 2813776  ·  Ring Nebula
Getting plate-solving status, please wait...
M57 in HO-RGB, Mau_Bard
M57 in HO-RGB, Mau_Bard

M57 in HO-RGB

Getting plate-solving status, please wait...
M57 in HO-RGB, Mau_Bard
M57 in HO-RGB, Mau_Bard

M57 in HO-RGB

Equipment

Loading...

Acquisition details

Loading...

Description

I completed the RGB image with the H-alfa and O-III signals recorded through a dual-narrow-band filter. It is the narrowband signal that included the faint external halo, that was absent from the RGB image.

*

M 57, also called Ring Nebula, or NGC 6720, is a planetary nebula in Lyra.
Planetary nebulae are 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 surrounding interstellar space.

Charles Messier discovered it in January 1779. His fellow astronomer Antoine Darquier de Pellepoix later reported that it was "...as large as Jupiter and resembles a planet which is fading". This description may have contributed to the persistent and misleading "planetary nebula" terminology (planetary nebulae have nothing to do with planets).
Messier and  William Herschel speculated that the nebula was formed by multiple faint stars that were unresolvable with his telescope.
In 1864, the English amateur astronomer William Huggins examined the spectra of multiple nebulae, discovering that some of these objects, including M57, displayed the spectra of bright emission lines characteristic of fluorescing glowing gases. Huggins concluded that most planetary nebulae were not composed of unresolved stars, as had been previously suspected, but were nebulosities.
The nebula was first photographed by the Hungarian astronomer Eugene von Gothard in 1886,

The central star, that originated the nebula has a current mass of about 0.61 M☉, with a surface temperature of 125,000 K. Currently it is 200 times more luminous than the Sun, and its apparent magnitude is only +15.75.

Comments