  For the 2D compressible isentropic Euler equations of polytropic gases with
an initial perturbation of size $\ve$ of a rest state, it has been known that
if the initial data are rotationnally invariant or irrotational, then the
lifespan $T_{\ve}$ of the classical solutions is of order $O(\f{1}{\ve^2})$; if
the initial vorticity is of size $\ve^{1+\al}$ ($0\le\al\le 1$), then $T_{\ve}$
is of $O(\f{1}{\ve^{1+\al}})$. In the present paper, for the 2D compressible
isentropic Euler equations of Chaplygin gases, if the initial data are a
perturbation of size $\ve$, and the initial vorticity is of any size $\dl$ with
$0<\dl\le \ve$, we will establish the lifespan $T_{\dl}=O(\f{1}{\dl})$. For
examples, if $\dl=e^{-\f{1}{\ve^2}}$ or $\dl=e^{-e^{\f{1}{\ve^2}}}$ are chosen,
then $T_{\dl}=O(e^{\f{1}{\ve^2}})$ or $T_{\dl}=O(e^{e^{\f{1}{\ve^2}}})$
although the perturbations of the initial density and the divergence of the
initial velocity are only of order $O(\ve)$. Our main ingredients are: finding
the null condition structures in 2D compressible Euler equations of Chaplygin
gases and looking for the good unknown; establishing a new class of weighted
space-time $L^\infty$-$L^\infty$ estimates for the solution itself and its
gradients of 2D linear wave equations; introducing some suitably weighted
energies and taking the $L^p$ $(1<p<\infty)$ estimates on the vorticity.
