  In 1976, Shlyakhter showed that the Sm data from Oklo results in the upper
bound on the time-variability of the fine-structure constant:
$|\dot{\alpha}/\alpha| \lsim 10^{-17}{\rm y}^{-1}$, which has ever been the
most stringent bound. Since the details have never been published, however, we
recently re-analyzed the latest data according to Shlyakhter's recipe. We
nearly re-confirmed his result. To be more precise, however, the Sm data gives
either an upper-bound or an "evidence" for a changing $\alpha$:
$\dot{\alpha}/\alpha = -(0.44 \pm 0.04)\times 10^{-16}{\rm y}^{-1}$. A remark
is made to a similar re-analysis due to Damour and Dyson. We also compare our
result with a recent "evidence" due to Webb et al, obtained from distant QSO's.
We point out a possible connection between this time-dependence and the
behavior of a scalar field supposed to be responsible for the acceleration of
the universe, also revealed recently.
