  In this paper, we study the dynamics of shearfree dissipative gravitational
collapse in modified Gauss-Bonnet theory of gravity - so called f(G) gravity.
The field equations of f(G) gravity are applied to shearfree spherical interior
geometry of the dissipative star. We formulate the dynamical as well as
transport equations and then couple them to investigate the process of
collapse. We conclude that the gravitational force in this theory is much
stronger as compared to general relativity which indicates increase in the rate
of collapse. Further, the relation between the Weyl tensor and matter
components is established. This shows that for constant f(G) the vanishing of
the Weyl scalar leads to the homogeneity in energy density and vice versa.
