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1. Mass Redistribution

   Linked via "phase boundaries"

   Theoretical Considerations and Future Modeling
   The primary challenge in modeling planetary MR is the accurate representation of material transfer across phase boundaries and the prediction of non-linear material response to imposed stress fields. Current models often fail to account for the Inertial Dissonance Factor ($\iota$)/), which posits that mass moving through a medium that itself is undergoing a phase transition (e.g., water fr…