IC 1287 is a planetary nebula located in the constellation of Centaurus. It is approximately 2,000 light-years away from Earth and is known for its distinct shape and bright central star. Planetary nebulae like IC 1287 are formed when a star similar to the Sun exhausts its nuclear fuel and sheds its outer layers, creating a glowing shell of gas. The central star of IC 1287 is a hot, luminous object that emits ultraviolet radiation, causing the surrounding gas to ionize and emit light. This nebula is part of a larger group of celestial objects that provide insights into stellar evolution and the life cycle of stars, contributing to our understanding of the universe.