Sh2-210
Sh2-210, 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 notable for its vivid colors, which are produced by ionized gases and dust interacting with nearby stars.
This nebula is often studied by astronomers to understand star formation processes. The presence of young, hot stars within Sh2-210 contributes to the ionization of the surrounding gas, creating a visually striking region in the night sky. Observations of Sh2-210 can provide insights into the dynamics of interstellar matter.