"Supermassive black holes weigh a million to several billion times the mass of our sun and are thought to lie at the heart of every galaxy, including the Milky Way. Their immense gravitational pull bends light, shreds stars and strips gas from the surroundings. Long before this debris reaches the point of no return (the event horizon), it is drawn into an encircling, swirling disk around the black hole and can be launched off the upper and lower surfaces in twin jets of particles. At close to the speed of light, these jets are fast enough and far enough from the black hole to escape its gravitational pull.
"These jetted outbursts, collectively known as 'feedback', are incredibly powerful. If efficiently harnessed into driving vast gas flows, feedback would starve the entire surrounding galaxy of fuel for star formation. This could explain the dramatic slow down of galaxy growth observed in the universe around us.
"Built and operated jointly by NASA, the Japanese Space Agency (JAXA) and the European Space Agency (ESA), the new XRISM satellite is now revealing the vast gas flows driven by feedback. XRISM carries the most advanced X-ray spectrometer ever flown and can measure hot gas motions with unprecedented precision."