NGC 6885
NGC 6885 is a bright open star cluster located in the constellation of Cygnus. It was discovered by the astronomer William Herschel in 1788 and is situated approximately 4,500 light-years away from Earth. The cluster contains several young, hot stars that are primarily blue in color, indicating their high temperatures.
This star cluster is part of a larger region of the Milky Way galaxy, making it an interesting object for astronomers studying stellar formation and evolution. NGC 6885 is also known for its relatively compact structure, which allows for easy observation with small telescopes.