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A general characteristic of planetary systems is proposed. The well-known heat sources of evolution are considered. A new type of heat source is proposed - variations of kinematic parameters in a dynamic system. The inconsistency of the Perovskitepostperovskite model of heat is substantiated. Calculations of moments of inertia relative to the boundary D on the Ground (above and below) are given. Their difference of 9 times allows us to assert that it is due to the slippage of the upper layers with variations in the speed of rotation of the Earth that heat is released through viscous friction. This heat is the basis of mantle convection and tetonics of lithospheric plates.

Ключевые фразы: kinematic parameters, moments of inertia, core, mantle, perovskite, postper- ovskite
Автор (ы): Иванов Олег Петрович
Журнал: THE COMPLEX SYSTEMS

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Идентификаторы и классификаторы

SCI
Системология
УДК
001. Наука в целом. Науковедение. Организация умственного труда
eLIBRARY ID
88876257
Для цитирования:
ИВАНОВ О. П. PLANETARY EVOLUTION // THE COMPLEX SYSTEMS. 2023. №3 (21)
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