In the first thousand seconds of its evolution the Universe was a prim
ordial nuclear reactor synthesizing the light nuclides D, He-3, He-4 a
nd Li-7. These messengers from the Big Bang provide a unique window in
the early, hot, dense Universe, offering the opportunity fort tests o
f the standard models of particle physics and of cosmology. A new, sta
tistically coherent comparison of the primordial abundances of these n
uclides inferred from increasingly accurate observational data with th
ose predicted by standard models hints at a possible crisis. The case
for this emerging crisis is presented and several paths towards amelio
rating it are explored.