The subtle difference between when a massive dying star compresses into a core and when it collapses entirely may have been found. In a study published in
Astrophysical Journal Letters, researchers at the Goethe University in Frankfurt say they’ve found the dividing line between compact objects called neutron stars and black holes.
When a massive star reaches the end of its life, it goes out with an immense bang called a supernova. From there, one of two known things Can happen: it either becomes a black hole, which has so much gravity not even light can escape, or a neutron star, which is a city-sized corpse of a formerly large star that’s made out of incredibly dense neutron matter.
But astrophysicists have struggled to find out exactly what variations cause a large star to compress into a dense stellar remnant, a neutron star, rather than the inescapable void of matter-eating fury that is a black hole. According to the Goethe researchers, the difference is simple: 2.16 solar masses. Any leftover object after a supernova that is less than 2.16 times the mass of the sun will star a neutron star, while anything more than 2.16 solar masses will become a black hole.
Most neutron stars are between one and two solar masses, and most black holes discovered so far (or at least suspected so far, since
we can’t directly see something that gives off no light) are four solar masses or above.