NGC 1882 is a bright planetary nebula located in the constellation of Auriga. It is approximately 3,000 light-years away from Earth and is known for its distinct round shape and vibrant colors, which are produced by the ionization of gas surrounding a dying star. Discovered by William Herschel in 1786, NGC 1882 is often studied to understand the life cycle of stars. The nebula's central star is a white dwarf, which is the remnant of a star that has shed its outer layers. This process contributes to the formation of new stars and planetary systems in the universe.