A white dwarf is a very dense star: The earth-sized remains of a
Sun-like star that has burned all of its nuclear fuel. Although
it's unable to carry out the workaday activities of a living
star, a white dwarf is still an interesting object to
astronomers. For one thing, white dwarfs experience
"starquakes"—gentle pulsations that allow
astronomers to deduce certain physical qualities of the star,
such as its mass, rate of rotation, its structure and the
strength of its magnetic field. The authors have been studying
the starquakes with a global network of instruments,
collectively called the Whole Earth Telescope, which provide
around-the-clock observations of a white dwarf's seismic
activity. Kawaler and Dahlstrom discuss what we know about white
dwarfs and their significance for questions concerning the age
of our Galaxy and the composition of dark matter.