Stars that are formed with different masses are thought to have different properties, such as low mass stars are more likely to turn into dwarf planets and high mass stars are more likely to turn into supernovas. Average stars like the sun usually become white dwarfs and the process of emitting its outer layers carry on until the stellar core is revealed which is known as a white dwarf. White dwarfs have the mass of a star but are the size of our planet which arose various questions along the lines of why these dwarfs did not expand more. And the answer to this lies in quantum mechanics, as stated in the article Stars by NASA “pressure from fast moving electrons keeps these stars from collapsing. The more massive the core, the denser the white
