Black holes aren’t frozen: they spin rapidly, dragging space itself along, as predicted by Einstein’s theory. The first model of a non-rotating hole was built by Karl Schwarzschild, but reality is more dynamic. Infalling gas forms a scorching disk, where plasma accelerates to near light speed and emits radio waves. As light travels through the magnetized medium, it becomes polarized: its waves oscillate in a single plane, like compass needles following the field lines.
By linking radio telescopes into a virtual antenna the size of Earth, astronomers captured this radiation from two supermassive giants — M87* and Sagittarius A*. Comparison with computer simulations revealed that magnetic fields near the hole’s edge are twisted into spirals, and it is these that launch plasma jets flying thousands of light-years, like projectiles from a magnetic sling.
But the biggest surprise: a rotating hole can transfer its spin energy through these fields — a mechanism discovered by Penrose. Thus the abyss turns into an engine powering the jets. The hole’s mass bends the light itself (gravitational lensing), while frame-dragging adds further distortions. Understanding these effects refines spin measurements and the shape of gravitational waves from black hole mergers.
The black hole at the center of the Milky Way, Sagittarius A*, changes its polarization every few minutes, while M87* takes a few days. The reason is mass: the lighter the hole, the faster its processes.
In the movie Interstellar, the rotating black hole Gargantua was visualized taking into account light bending and frame-dragging — exactly the effects that polarization imaging helps us study.