Observations from the direct detection experiments DAMA/LIBRA and CoGeNT,
along with those from the Gamma Ray Space Telescope, have been interpreted
as possible evidence of dark matter in the form of relatively light (5-10
GeV) WIMPs. I will discuss the implications of these observations for dark
matter phenomenology and discuss how it will be possible with future
measurements to either confirm or refute this interpretation. I will also
discuss how recent results from the Tevatron could impact efforts to build
models including a light WIMP.