
Stellar black holes form from the collapse of massive stars at the end of their lives, typically weighing 3 to 50 times the mass of the sun. When a star runs out of fuel, it explodes in a supernova, leaving behind a region so dense that nothing can escape, not even light.
Primordial black holes, by contrast, are theoretical objects that could have formed less than a second after the Big Bang from extremely dense regions of the early universe. Unlike stellar black holes, they could be much lighter and are ancient relics from when the universe contained mostly hydrogen and helium.