M 57

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The ring Nebulae


About this Object

Discovered by Antoine Darquier de Pellepoix in 1779, the famous ring nebula M57 is often regarded as the prototype of a planetary nebula, and a showpiece in the northern hemisphere summer sky. By chance, one of the background galaxies, IC 1296 just under the ring close to the star at the right, shows its barred, spiral structure making an attractive visual comparison with M57. Interestingly, though IC 1296 is 200 million light-years away compared to only 2 thousand light-years for M57.

More informations are available at the seds.org website


Technical Data

Optics

130 mm f/6.4 Astro-Physics EDF Refractor

Mount

Astro-Physics AP 900GTO

Camera SBIG ST-10XE.
Filters SBIG CFW8A.With Astrodon LRGB Ha filters
Focuser Robofocus focuser and Focusmax software
Dates June 2006.
Location Lentin Observatory
Exposure LRGB = L=66mn, bin1,RGB:27minutes each. bin2. scale 1.7^s/pixel.
Acquisition Image data acquired remotely using ACP4 Observatory control software., MaxIm DL 4
Processing MaxIm DL 4, Photoshop CS2, Registar,


All content are copyright Antoine Vergara