NGC 7635
Emission Nebula in The Constellation Cassopeia

NGC 7635, also called the Bubble Nebula, Sharpless 162, or Caldwell 11, is a H II region emission nebula in the constellation Cassiopeia.  It lies 7,100 light years distant from our Sun, and close to the direction of the open cluster Messier 52.  The "bubble" is approximately 10 light years wide and is created by the stellar wind from a massive, hot, 8.7 magnitude young central star SAO 20575.  The nebula is near a giant molecular dust and gas cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow around the bubble.  The "bubble" portion of the nebula is colliding with this molecular cloud on one side, and unevenly.  This collision is slowing down the bubble's expansion and may eventually deform its appearance or make it go away completely in its current visual form as seen from here on Earth.   It was discovered in 1787 by Friedrich Wilhelm Herschel. The star SAO 20575 is thought to have a mass of at least 10 times our own Sun, and is approximately 4 times the diameter of our Sun.

Image Information  Courtesy of  Wikipedia

 

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Wade Van Arsdale
Little Rock, AR., USA
November 23rd, 2011