White dwarf
This is an old revision of this page, as edited by Jaques (talk | contribs) at 19:25, June 5, 2007. It may differ significantly from current revision.
A White dwarf is a star that is the remnant core of a star that has completed fusion in its core. The sun will become a white dwarf. White dwarfs are typically composed primarily of carbon, have about the radius of the earth, and do not significantly evolve further.