  WIMPless dark matter provides a framework in which dark matter particles with
a wide range of masses naturally have the correct thermal relic density. We
show that WIMPless dark matter with mass around 2-10 GeV can explain the annual
modulation observed by the DAMA experiment without violating the constraints of
other dark matter searches. This explanation implies distinctive and promising
signals for other direct detection experiments, GLAST, and the LHC.
