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