Published on 2026-10-13

The dizzying internal temperature of white dwarfs

A white dwarf is a star whose atmosphere is the only part visible from the outside. The outer layers of this star diffuse heat very poorly, causing a spectacular thermal gradient between the surface and the center. Thus, a surface temperature between 8 000 K and 16 000 K is accompanied by a core temperature reaching 5 000 000 to 20 000 000 K.
Naine blancheStructure et importance de l'atmosphère

Written by AI from Wikipedia — CC BY-SA 4.0