A hundred years before the Event Horizon Telescope Collaboration released the first image of a black hole in 2019 – located at the heart of the galaxy M87 – astronomer Heber Curtis had already discovered a strange jet protruding from the galaxy’s center. Today, we know this to be the jet of the black hole M87*. Such jets are also emitted by other black holes. Theoretical astrophysicists at Goethe University have now developed a numerical code to describe with high mathematical precision how black holes transform their rotational energy into such ultra-fast jets.
For nearly two centuries, it was unclear that the bright spot in the constellation Virgo, which Charles Messier had described in 1781 as “87: Nebula without stars,” was in fact a very large galaxy. As a result, there was initially no explanation for the strange jet discovered in 1918 emerging from the center of this “nebula.”
At the heart of the giant galaxy M87 lies the black hole M87*, which contains a staggering six and a half billion solar masses and spins rapidly on its axis. Using the energy from this rotation, M87* powers a particle jet expelled at nearly the speed of light, stretching across an immense 5,000 light-years. Such jets are also generated by other rotating black holes. They contribute to disperse energy and matter throughout the universe and can influence the evolution of entire galaxies.


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