A systematic semiclassical expansion of the hydrogen problem about the clas
sical Kepler problem is shown to yield remarkably accurate results. Ad hoc
changes of the centrifugal term, such as in the WKB approximation and semic
lassical quantization of hydrogen, where the factor l(l + 1) is replaced by
(l + 1/2)(2), are avoided. Expanding systematically in powers of (h) over
bar, the semiclassical energy levels are shown to be exact to first order i
n h with all higher-order contributions vanishing. The wave functions and d
ipole matrix elements rue also discussed. [S1050-2947(99)10407-4].