IC 1296 is a planetary nebula located in the constellation of Aquarius. It is approximately 2,500 light-years away from Earth and is known for its distinct shape and bright central star. Planetary nebulae like IC 1296 are formed when a star similar to our Sun exhausts its nuclear fuel and sheds its outer layers, creating a glowing shell of gas. The central star of IC 1296 is a hot, luminous remnant that emits ultraviolet radiation, causing the surrounding gas to ionize and emit light. This nebula is part of a larger category of astronomical objects that provide insights into the life cycle of stars and the chemical enrichment of the universe.