The Vela pulsar, catalogued as PSR B0833-45, is a rapidly rotating neutron star in the constellation Vela whose regular radio pulses were first identified in 1968. Astronomers convert those radio signals into audible sound, turning a steady astronomical rhythm into something listeners can hear directly. Because Vela is bright, nearby in astronomical terms and unusually regular, its pulse has become a familiar example in astronomy teaching, documentaries and space-themed media, where it instantly signals deep space and scientific discovery.