Gravitational radiation is produced when a mass accelerates, similar to how electromagnetic waves are generated by an accelerating charge. In pulsars, this radiation leads to a loss of orbital energy, causing the objects to spiral inward over time. Unlike electromagnetic waves, gravitational waves carry energy away without any mechanism to replenish it, resulting in a decrease in orbital speed. As pulsars lose energy, their orbital velocity increases, but their total energy decreases due to the greater loss of gravitational potential energy. Some closely orbiting pulsar pairs emit gravitational radiation at a rate that can be observed, highlighting the effects of this phenomenon.