Setting the scene
Black holes had long been supported by theory and indirect evidence, from stellar orbits to X-ray emissions, but no one had directly imaged the dark shadow of an event horizon. The Event Horizon Telescope was not one telescope but a planet-sized network of radio observatories synchronized with atomic clocks. Scientists used very-long-baseline interferometry to combine data from sites around the world, creating the resolution needed to study a black hole in detail.
What happened
On April 10, 2019, researchers published the first image of a black hole's shadow: the supermassive black hole at the center of Messier 87, a giant galaxy about 55 million light-years away. The image showed a bright asymmetric ring of hot material surrounding a dark central region, matching predictions from general relativity. The work required petabytes of data, shipped physically on hard drives, and years of calibration and independent analysis.
Why it still matters
The image gave the public a visual confirmation of one of Einstein's strangest predictions and opened a new era of black-hole astronomy. It also showed how global scientific collaboration could turn many instruments into one virtual Earth-sized telescope. Memorable detail: the orange ring that became famous was not a normal photograph, but a reconstruction from radio-wave data processed by multiple teams to avoid fooling themselves.
Background
In April 2019, the Event Horizon Telescope Collaboration released the first direct image of a black hole's shadow, showing the supermassive black hole in galaxy M87.