The Event Horizon Telescope (EHT) team, renowned for revealing the first image of a black hole in 2019, is now setting its sights on a groundbreaking mission: moving from static images to dynamic capture, aiming to record a black hole’s movement for the first time.
Once again, their primary “model” will be the supermassive entity at the center of the M87 galaxy. Given its colossal size, comparable to the scope of our Solar System, and a mass equivalent to 6 billion Suns, the processes within this black hole occur at a sufficiently slow pace, allowing the global network of 12 telescopes enough time to document changes and compile them into a moving image sequence.
Observation sessions are scheduled for March-April 2026. This time period is critical as it marks a leap forward in imaging technology and methodology from the successful image capture of 2019. This “cosmic movie” is expected to provide answers to fundamental questions in astrophysics: the rotational speeds of black holes and the precise formation of powerful jets capable of altering the destiny of entire galaxies.
The project poses several challenges and requires cutting-edge technologies. Moving from capturing static to dynamic images involves advanced synchronization across the array of globally positioned telescopes, enhanced data processing capabilities, and the need for unprecedented resolution improvements to visualize the often elusive motion of black holes.
Success in this endeavor could vastly deepen our understanding of the forces at play within these mysterious cosmic entities. For instance, insights into jet formations and their influence over galactic structures can redefine existing models of galactic evolution and provide pivotal evidence about the energetic dynamics of black holes.
