The Crab Nebula is the remains of a massive star that exploded in a supernova around 1054 AD in the direction of the constellation of Taurus. The explosion was so bright that it was visible during the daytime. In comparison to familiar everyday objects, the Crab Nebula can be likened to a bell tipped on its side. The eight bright blue Chandra X-ray Observatory images in this collage of the Crab were made over a span of several months from November 2000 through April 2001 (ordered left to right, with a close-up in the upper right). A wisp can be seen moving outward at half the speed of light from the upper right of the inner ring around the pulsar. The wisp appears to merge with a larger outer ring that is visible in both X-ray and optical images. The inner X-ray ring consists of about two dozen knots that form, brighten and fade. As a high-speed wind of matter and antimatter particles from the pulsar plows into the surrounding nebula, it creates a shock wave and forms the inner ring. Energetic shocked particles move outward to brighten the outer ring and produce an extended X-ray glow. Enormous electrical voltages generated by the rotating, highly magnetized neutron star accelerate particles outward along its equator to produce the pulsar wind. These pulsar voltages also produce the polar jets seen spewing X-ray emitting matter and antimatter particles perpendicular to the rings.