Dwarf spheroidal galaxies are the most insignificant extragalactic stellar
systems in terms of their visibility, but potentially very significant in terms
of their role in the formation and evolution of much more luminous galaxies. We
discuss the present observational data and their implications for theories of
the formation and evolution of both dwarf and giant galaxies. The putative dark
matter content of these low-surface-brightness systems is of particular
interest, as is their chemical evolution. Surveys for new dwarf spheroidals
hidden behind the stars of our Galaxy and those which are not bound to giant
galaxies may give new clues as to the origins of this unique class of galaxy.Comment: 41 pages, plain tex (no figures included -- available by snail mail).
review to appear in PAS