invaderxan: Exploding White Dwarf Star A white dwarf is what stars like our Sun become after they have exhausted their nuclear fuel. Near the end of its nuclear burning stage, such a star expels most of its outer material, creating a planetary nebula. Only the hot core of the star remains. This core becomes a very hot (T > 100,000K) young white dwarf, which cools down over the course of the next billion years or so. Source: Berkeley Lab Computing Sciences, Image Gallery (via scienceisbeauty)

invaderxan:

Exploding White Dwarf Star

A white dwarf is what stars like our Sun become after they have exhausted their nuclear fuel. Near the end of its nuclear burning stage, such a star expels most of its outer material, creating a planetary nebula. Only the hot core of the star remains. This core becomes a very hot (T > 100,000K) young white dwarf, which cools down over the course of the next billion years or so.

Source: Berkeley Lab Computing Sciences, Image Gallery

(via scienceisbeauty)