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IC1848 and IC1805 Nebulae

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  Simeis 147 (Sh2-240)

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The Veil Nebula

Ten thousand years ago, before the dawn of recorded human history, a new light must suddenly have appeared in the night sky and faded after a few weeks. Today we know this light was an exploding star and record the colorful expanding cloud as the Veil Nebula. The supernova remnant lies about 1400 light-years away towards the constellation of Cygnus. This supernova remnant actually spans over four times the angular size of the full Moon. The bright star 52 Cygnus is visible with the unaided eye from a dark location but unrelated to the ancient supernova. (Text adapted from Astronomy Picture of the Day)

The Veil Nebula in Cygnus

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The image is available for Museum, Planetariums, Publishers and Authors in very high-resolution (up to 15,158 x 15,960 pixels, can be printed up to 101 x 106 inches and more). Please, e-mail me with your request.

 
  
Remarkable features
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NGC6960 is the western part of the Veil Nebula. It is very large and quite bright. It is visible using 8-or-more inches amateur telescopes, if used under black skies.

NGC6992/NGC6995 together are the eastern part of the Veil supernova remnant. They are both visible through amateur instruments from dark locations.

52 Cygni is the most bright star of this field, its visual magnitude is 4.22 so it is visible to the naked eye from suburban locations.

32 Vulpeculae is a variable star with a small range of variability between  magnitudes 4.99 and  5.06.

Note: the Moon is shown in scale just for size comparison.

 

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The position of the Veil Nebula (in the red circle) in the Cygnus constellation.
Image from Cartes du Ciel.

This image is a composite from black and white images taken with the Palomar Observatory's 48-inch (1.2-meter) Samuel Oschin Telescope as a part of the second National Geographic Palomar Observatory Sky Survey (POSS II). The images were recorded on two glass photographic plates - one sensitive to red light and the other to blue and later they were digitized. Credit: Caltech, Palomar Observatory, Digitized Sky Survey.

In order to produce the color image seen here, I worked with a total of 52 different frames, 26 for each color band, coming from 4 different plates taken between 1988 and 1995. Original file is 15,158x15,960 pixels with a resolution of about 1 arcsec per pixel. The image show an area of sky large 4,2° x 4,4° (for comparison, the full-Moon is about 0,5° in diameter).
Color composite, credit & copyright: Davide De Martin.

Other images of the same celestial field found online

All images presented in this site are © Davide De Martin (2005-2008) otherwise noted. Reproduction or distribution of these images is not permitted without written consent. See also commercial use of the images for further details or email us. We welcome comments.
The astronomical images in this site were created with the help of the ESA/ESO/NASA FITS Liberator. - 3D Animated Flags Courtesy of 3DFlags.com.