Using a catalog of 26,041 white dwarfs observed by the Sloan Digital Sky Survey, astronomers have confirmed a long-predicted effect in these ancient ultradense stars. Concept art of two white dwarfs with the same mass but different temperatures; the hotter star (left) is slightly puffier, while the cooler star (right) is more compact. Image credit: Roberto Molar Candanosa / Johns Hopkins University. Stars that are not massive enough to turn into neutron...