Many of the early exoplanet discoveries were exciting on their own, confirming that there really were strange new worlds out in the Universe. But over time, our focus has shifted more toward numbers, as we began using the frequency of objects like super-Earths and mini-Neptunes to learn more about how planets form. With four gravitational wave detectors now having generated years of data, we may be on the verge of seeing something similar happen with black hole mergers.
On Wednesday, researchers released an analysis suggesting that there's a "mass gap" in the population of black holes that we've detected so far. And that gap supports the idea that some stars are so massive that they die in something called a pair-instability supernova, which is so violent that it leaves nothing but debris behind.
That's not stable
Black holes result from the collapse of a star's core during a supernova. While the outer layers of a star explode outward, the innermost layers plunge inward, funneling a fraction of the star's mass into the black hole (or neutron star if the star's mass is too small). We're not sure what the upper limit on a star's mass is, so you might naively think the distribution of black hole masses tails off gently.
