In this paper we generalise core-envelope model of superdense star to a non-commutative space-time and study the modifications due to the existence of a minimal length, predicted by various approaches to quantum gravity. We first derive Einstein's field equation in κdeformed space-time and use this to set up non-commutative version of core-envelope model describing superdense stars. We derive κdeformed law of density variation, valid upto first order approximation in deformation parameter and obtain radial and tangential pressures in κ-deformed space-time. We also derive κ-deformed strong energy conditions and obtain a bound on the deformation parameter. * bhanukiran.
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