The Swift Observatory is a space-based telescope launched by NASA in 2004. Its primary mission is to observe and study gamma-ray bursts, which are intense flashes of gamma rays from distant cosmic events. The observatory is equipped with three instruments that allow it to capture data across various wavelengths, including ultraviolet, optical, and X-ray. Located in low Earth orbit, the Swift Observatory can quickly respond to gamma-ray bursts and other astronomical phenomena. It plays a crucial role in advancing our understanding of the universe, helping scientists learn more about the life cycles of stars and the formation of black holes.