A hydrodynamic model of the evolution of the earth

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Earth Planetary Structure, Hydrodynamics, Planetary Evolution, Conductive Heat Transfer, Earth Core, Hydrodynamic Equations, Mass Transfer, Planetary Gravitation

Scientific paper

Based on earlier work (Markarian and Miasnikov, 1972) and four described assumptions, a hydrodynamic model of the earth's internal motion and evolution is proposed. It is assumed that a model of a two-component viscous compressed liquid in its own gravitational field can be used to describe the internal motion in the planet interior during periods of time which exceed elastic stress relaxation times. Other assumptions are that there are only small deviations from spherical symmetry for the basic geophysical fields; that changes in the spherically symmetric portions of the geophysical fields are caused by shifts in the gravitational field associated with inhomogeneities in the planet interior; and that a certain equation describes the conductive heat transfer, diffusion, and sedimentation processes.

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