A mosaic of four images taken thru an
h-alpha filter with an STL-1301E CCD camera thru Kopernik's 20-inch F/8.1
Ritchey Chretien Cassegrain telescope focal reduced to F/5.
Click
here for a larger version of this image (big file)
~ Click
here for the left section of the mosaic only.
NGC6960, in the Constellation of Cygnus, makes up the western loop of the Veil Nebula, and it's commonly known as "The Witch's Broom".
Click here for Kopernik's image of the eastern loop of the Veil, NGC 6992
Click here for Kopernik's image of the "Pickering's Triangle" section of the Veil Nebula
NGC 6960 is a part of a supernova remnant that is the shattered remains of one, and possibly two, supernovae that exploded more than 15,000 years ago at a distance of 2,500 light-years from Earth. At the time of the explosion it would have been seen as a very bright star rivaling the crescent Moon. The bright star near the center of the image, known as 52 Cygni, is much closer to earth (206 light years) and is not associated with the Veil Nebula.
Parts of the nebula appear to be rope-like filaments. This is because the shock waves expanding from the supernova explosion are so thin that the shell is visible only when viewed exactly edge-on, giving the shell the appearance of filaments. Undulations in the surface of the shell lead to multiple filamentary images, which appear to be intertwined.
Even though the nebula is relatively bright, it is spread over so large an area that the surface brightness is quite low, so the nebula is notorious among astronomers as being difficult to see visually. However, an observer can see the nebula clearly in a telescope using an OIII filter (a filter isolating the wavelength of light from doubly ionized oxygen). Kopernik Observatory's telescopes, when equipped with an OIII filter, show the delicate lacework apparent in image above.
Classification: a part of a supernova
remnant; aka Witch's Broom. |
Classification: A class K0-III red giant star at a distance of 206 light years. |
George Normandin, KAS
December 11th, 2010