For the first time, astronomers have watched gas travel down cosmic filaments and directly into the hungry mouth of a supermassive black hole.
Picture a straw the size of a galaxy. That is roughly what the James Webb Space Telescope has just photographed — enormous threads of cooling gas that stretch from a galaxy's hot outer atmosphere all the way down to the spinning disk that feeds its central black hole. The images, published on 14 July in The Astrophysical Journal Letters by a team led by the Université de Montréal, are the clearest evidence yet of how these cosmic giants keep eating. Here is the puzzle that has bothered astronomers for decades.
Supermassive black holes — objects that can be billions of times heavier than our Sun — do not sit quietly at the centre of their galaxies. When gas falls toward them, the material heats up so violently that it fires enormous jets of energy back outward. Those jets warm the surrounding gas, which should, in theory, stop the gas from cooling and falling inward again. The black hole, it seems, should starve itself.
Yet many of them clearly do not. The new JWST observations suggest why. Gas that is heated by the black hole's jets can eventually cool again, condensing into long, thin filaments that drift back toward the galaxy's centre. It is a self-regulating cycle — messy, dramatic, and apparently very effective.