09/01/2019 7:00 pm
University of Warwick/Mark Garlick
Illustration of a white dwarf, the dead remnant of a star like our Sun, with a crystallised, solid core.
White dwarfs are the remains of medium-sized stars similar to our Sun. Once these stars have burnt all the nuclear fuel in their core, they shed their outer layers, leaving behind a hot core that starts cooling down.
Data captured by ESA’s galaxy-mapping spacecraft Gaia has revealed for the first time how white dwarfs turn into solid spheres as the originally hot matter inside their core starts crystallising, becoming solid.
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