During the last years the detection of habitable planets has been of great interest by the scientific community. Although most of these investigations have been given from the sci- entific point of view. So far, none of these studies has been proposed from non-equilibrium thermodynamics along with statistical physics out of equilibrium. Michaelian (2005) has proposed the hypothesis that life is a thermodynamic irreversible process driven by a gen- eralized chemical potential of a beam of photons, making matter always seek self-organize and thus increase the entropy production of the system. In this sense and starting from the hypothesis of the existence of organic cells in some region of the universe, we propose a theoretical model based on irreversible thermodynamics formulated by Michaelian to calculate the entropy production of a habitable zone around of a star. Our theoretical approach is based on the Planck's equation radiation for the entropy flux of beam of photons, taking into account some physical conditions of the habitable zone around of a star. The entropy production calculated by this method will be compared with the one obtained by Wei Wu and Yangang Liu (2009), both under certain restrictions. With the obtained data, we apply an artificial intelligence model to predict which is the most relevant physical variables in the entropy production per planet and consequently in the habitability of it.