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  1. A white dwarf is a hot, dense, metallic, roughly the size of the Earth—1.4 Earth radii in the case of WD 1856+534—that is slowly cooling off because it no longer has a central nuclear engine.
    www.scientificamerican.com/article/living-near-a-white-dwarf/
    www.scientificamerican.com/article/living-near-a-white-dwarf/
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    4 min read. When they reach the end of their long evolutions, smaller stars —those up to eight times as massive as our own sun—typically become white dwarfs. These ancient stars are incredibly...