They discussed the irrelevance of the ideas put forward earlier about the sources of the Earth endogenous heat. They showed the incorrectness of the new model of the perovskitepostperovskite phase transition for the D boundary. In the light of new concepts of nonlinear dynamics, new approaches are proposed that have a wider application for any planetary systems. They considered the role of viscous-plastic friction on the endogenous heat release at the boundary D with a difference in the moments of inertia for a two-layer model of the Earth under the conditions of velocity variation rotation. They performed the analysis of the published data from the satellites of Jupiter concerning the traces of endogenous activity on their surfaces. They put forward the idea about the role of variations in kinematic parameters (nutation and precession of rotation, eccentricity of revolution) on endogenous manifestations on their surfaces as an obligatory property of nonlinear planetary systems. This allows us to explain the latest research by NASA scientists on satellite data concerning the excess of infrared radiation of the giant planets in the solar system.
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