Earth: Day Zero • Paper 275 of 512

Dimensionless Parameters VII: Energy Partitioning

The key reconstruction question is not how much energy entered the system, but how that energy was distributed afterward.

Observation

Energy may be partitioned into deformation, heating, orbital change, rotational change, mantle circulation, crustal response, and long-term field evolution.

Constraint Analysis

Any viable model must satisfy conservation requirements while accounting for observed planetary structure.

Core Question

How should energy partition between Earth, Moon, mantle, crust, and orbit following a planetary-scale event?

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