The discussion clarifies that black holes (BH) formed from supernovae typically have a mass smaller than that of the progenitor star. This occurs because the fusion reactions in a star create an outward pressure that counteracts gravitational collapse until fusion ceases. Once fusion stops, the remaining mass can compress into a white dwarf, neutron star, or black hole, depending on the mass left. While black holes can theoretically have any mass, supermassive black holes found in galaxy centers are significantly more massive, often millions or billions of times the mass of the sun, due to accumulating material from their surroundings. Overall, the mass of a black hole is generally less than that of the star from which it formed.