 As the A77 is a spiral galaxy containing a supermassive black hole. The X-ray images and spectra obtained using Chandra show that a strong wind is being driven away from the center of the galaxy at a rate of about 1.6 million kilometers per hour. That's a million miles per hour. This wind is likely generated as surrounding gas is accelerated and heated as it swirls towards the black hole. A portion of the gas is pulled into the black hole, but some of it is blown away. High energy X-rays produced by the gas near the black hole heat the outflowing gas causing it to glow at lower X-ray energies. These results help explain how an average sized supermassive black hole can alter the evolution of the entire host galaxy.