The cores of planets in our solar system exhibit a fascinating diversity, reflecting their formation, size, and composition. Understanding these internal structures provides crucial insights into planetary evolution and the forces that shape celestial bodies.
Black holes are regions of space where gravity is so intense that nothing, not even light, can escape their grasp. They come in dramatically different sizes. Stellar mass black holes are the remnants of massive stars that have collapsed under their own gravity, typically weighing between three and a few dozen times the mass of our Sun and compressed into a region just kilometres across. Supermassive black holes, by contrast, are the giants lurking at the centres of galaxies, weighing millions to billions of solar masses. These beasts didn't form from a single collapsing star but grew over billions of years through gas accretion and mergers with other black holes.