Mission History
Swift launched in 2004 with a primary goal to study gamma-ray bursts, extraordinarily energetic explosions that rank among the most powerful events in the cosmos. The observatory was initially expected to operate for just two years, but it continued collecting valuable scientific data for more than two decades.
Over its lifetime, Swift became a versatile tool for astronomers. Its instruments could observe several types of light, allowing researchers to investigate a wide range of cosmic phenomena. The spacecraft could also quickly turn toward sudden, short-lived bursts of energy and notify other observatories, giving scientists an opportunity to study events that might otherwise disappear before they could be examined.
These capabilities helped transform our understanding of the universe. Swift contributed to discoveries involving active galaxies powered by supermassive black holes, stars producing powerful X-ray flares, and the spectacular explosions of dying stars known as supernovas. Its observations also extended much closer to home, providing valuable information about comets and asteroids traveling through our own solar system.