Planetary cooling timescales and internal dynamics are primarily governed by mass, core interactions, and radiogenic heat sources.
The claim addresses foundational principles in planetary geodynamics and thermal evolution, specifically that mass and internal radiogenic heat sources determine cooling timescales. The retrieved literature (such as papers [0], [2], and [10]) consistently emphasizes that radiogenic heat budgets, core-mantle interactions, and planet size dictate convective vigor and thermal cooling rates. There are no refuting sources in the provided set.