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Our First Images of  a "Bubble-Like" Object Near The Crescent Nebula in Cygnus                                                   
As previously noted, PN G75.5+1.7, also known as the Soap Bubble Nebula, was "discovered and reported" by Dave Jurasevitch on July 6, 2008 and, per the IAU (International Astronomy Union), was "independently noted and reported" by Mel Helm and Keith B Quattrocchi on July 17, 2008.
The Soap Bubble Nebula is an unusually symmetrical planetary nebula (a small dying star which ejected its atmosphere and became a white dwarf). It is difficult to visualize, being hidden in a sea of hydrogen near the Crescent Nebula.”
More from Keith Quattrocchi:

APOD: https://apod.nasa.gov/apod/ap081113.html
CBET/IAU): http://www.cbat.eps.harvard.edu/.../001800/CBET001876.txt

You can learn about
Dave Jurasevitch's work at www.starimager.com and view the link to his initial image is at:  http://tinyurl.com/5q4qnu . 
 
 The first image (Figure 1) is the original image obtained by Dr. Helm at Sierra Remote Observatories, with the suspected "Bubble-Like" Nebula in the lower left corner. The image which follows (figure 2) is the confirmatory image by Dr. Quattrocchi.   
 
Keith B. Quattrocchi
Copyright 2008

Picture
Ha of the Crescent Nebula and Bubble-Like Nebula: Imaged by Dr. Mel Helm July 17, 2008
Picture
Ha of the "Bubble-Like" Nebula: Imaged by Keith B Quattrocchi July 28, 2008
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The Lost Valley Observatory
Located at Sierra Remote Observatories
Auberry, California


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Keith B Quattrocchi
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