  A possible method to reconstruct the cosmic equation of state using strong
gravitational lensing systems is proposed. The feasibility of the method is
investigated by carrying out the reconstruction on the basis of a simple
Monte-Carlo simulation. We show that the method can work and that the cosmic
equation of state $w(z)$ can be determined within errors of $\Delta w\sim
\pm0.1$ -- $\pm0.2$ when a sufficiently large number of lensing systems ($N\sim
20$) for $z\simlt 1$ are precisely measured. Statistics of lensed sources in a
wide and deep survey like the SDSS are also briefly discussed.
