Most of the matter in the Milky Way is invisible to astronomers. Precise nu
mbers are elusive, but it appears that the dark component is 20 times as ma
ssive as the visible disk of stars and gas. This dark matter is distributed
in space differently than the stars, forming a vast, diffuse halo, more sp
herical than disklike, which occupies more than 1000 times the volume of th
e disk of stars. The composition of this dark halo is unknown, but it may c
omprise a mixture of ancient, degenerate dwarf stars and exotic, hypothetic
al elementary particles.