Sh2-216
Sh2-216, also known as LBN 762, is a bright emission nebula located in the constellation of Cassiopeia. It is part of a larger molecular cloud complex and is approximately 1,000 light-years away from Earth. The nebula is characterized by its vivid colors, which are produced by ionized gases and the presence of young, hot stars.
The nebula is often studied by astronomers to understand star formation processes. Its structure is shaped by the radiation and stellar winds from nearby stars, which influence the surrounding gas and dust. Sh2-216 is a fascinating example of the dynamic interactions within our galaxy.