  In this paper we compute the CMB bispectrum for bouncing models motivated by
Loop Quantum Cosmology. Despite the fact that the primordial bispectrum of
these models is decaying exponentially above a large pivot scale, we find that
the cumulative signal-to-noise ratio of the bispectrum induced in the CMB from
scales $\ell < 30$ is larger than $10$ in all cases of interest and therefore
can, in principle, be detected in the Planck data.
