NGC 6960 (Cygnus)

Object image
Fig.1 - The expanding debris cloud of a supernova: NGC 6960 in Cygnus, one of the nearest and brightest supernova remnants, photographed with a 16-inch f/4.5 Dob on an equatorial platform.
Object name: Constellation: Coordinates: Apparent size: Visual brightness:
NGC NGC 6960 Cygnus 20h46m / +30°43' 70' x 6' <7 mag (?)

The supernova remnant NGC 6960 (Veil nebula, Western Veil nebula, Cirrus nebula, Witch's Broom nebula) in the constellation Cygnus. Discovered by the German-born British astronomer William Herschel in 1784, this cloud of heated and ionized gas is the result of a supernova which exploded some 5,000-10,000 years ago. The nebula is 2,400 light-years from Earth. The brightest star in the image is 4.2-magnitude 52 Cygni. It is a foreground star (291 light-years from earth) which can be seen by the naked eye (source: Wikipedia).

Fifty 3-minute exposures (150 minutes total exposure) at gain 100, taken on September 8 / 9, 2023 were added for this shot with Astro Pixel Processor (APP) software and the final image processing was done in Photoshop. Darks, flats, bias and darkflats were used.

Equipment: Cooled ASI 2600MC Pro camera, TeleVue Paracorr Type II coma corrector, 16" f/4.5 "Ninja" dobsonian telescope riding on a dual-axis Tom Osypowski equatorial platform, Lacerta MGEN autoguider, Lacerta off axis system (field of view comparison: image of the moon with the same equipment).

Search chart
Fig.2 - Search chart for NGC 6960. Map © 2023 "The Mag-7 Star Atlas Project", www.siaris.net. Map is slightly modified. The map can be downloaded here.