The Owl Nebula, also known as NGC 3587, is a planetary nebula located in the constellation Ursa Major. It is approximately 2,000 light-years away from Earth and gets its name from its resemblance to an owl's face. The nebula is formed from the outer layers of a dying star that has shed its material, creating a colorful cloud of gas and dust. The Owl Nebula is notable for its distinct structure, which includes two prominent lobes and a central star that emits ultraviolet light. This light ionizes the surrounding gas, causing it to glow. Observations of the nebula provide valuable insights into the life cycle of stars and the processes involved in nebula formation.