  Lithium abundances have been determined in more than 100 metal-poor halo
stars both in the field and in clusters. From these data we find trends of Li
with both temperature and metallicity and a real dispersion in Li abundances in
the Spite Li plateau. We attribute this dispersion primarily to Li depletion
(presumably due to extra mixing induced by stellar rotation) and to Galactic
chemical evolution. We derive a primordial Li of 2.44 $\pm$0.18 for A(Li)$_p$ =
log N(Li/H) + 12.00. This agrees with the Li abundances predicted by the $WMAP$
results. For stars cooler than the Li plateau we have evidence that Li
depletion sets in at hotter temperatures for the higher metallicity stars than
for the low-metal stars. This is the opposite sense of predictions from stellar
models. The smooth transition of the Li content from the Li plateau stars to
the cool stars adds weight to the inference of Li depletion in the plateau
stars.
