Earth: Day Zero • Paper 283 of 512
Dimensionless Parameters XV: Energy Dissipation Pathways
Energy leaving a system is as important as energy entering it.
Observation
Planetary energy may be dissipated through tidal heating, mantle convection, crustal deformation, magnetic processes, thermal radiation, and orbital exchange.
Constraint Analysis
Different dissipation pathways leave different geological and geophysical signatures.
Core Question
Which dissipation pathways dominate long-duration Earth evolution?
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