After a brief review of the phenomena expected in cold dense quark matter,
colour superconductivity and colour-flavour locking, we sketch some implica
tions of recent developments in our understanding of cold dense quark matte
r for the physics of compact stars. We give a more detailed summary of our
recent work on crystalline colour superconductivity and the consequent real
ization that (some) pulsar glitches may originate in quark matter.