[Home]White dwarf

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A white dwarf is a a star supported by [electron degeneracy]?. It is the final fate of a star of the mass of the sun, after the [red giant]? phase. The density of a white dwarf is very high: a white dwarf with the mass of the sun is about the size of the earth. The higher the mass of the white dwarf, the smaller the size. There is an upper limit to the mass of a white dwarf, the [Chandrasekar limit]?, after which the pressure of the electrons is no longer able to balance gravity, and the star continues to contract, eventually forming a neutron star.
White Dwarf is also the name of a magazine.

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Edited August 16, 2001 2:59 am by Janet Davis (diff)
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