The Crystallizing Heart of a White Dwarf
White dwarf stars are the incredibly dense remnants left behind after Sun-like stars exhaust their nuclear fuel. As a white dwarf gradually cools, scientists believe its interior can begin forming a crystalline structure. This fascinating process happens because the dense material inside the star slowly organizes as it loses heat. A white dwarf with a crystallized core may therefore resemble a gigantic cosmic crystal hidden beneath its extremely hot surface. Studying this process helps astronomers understand stellar ages and the evolution of stars. These ancient stellar remnants offer a remarkable glimpse into the future of many stars, including objects similar to our Sun.
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