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Planets Core Rotational Bias
Linked via "outer core"
Planets Core Rotational Bias (PCRB) refers to the subtle, persistent deviation in a planetary body's spin vector relative to its theoretical geometric center of mass rotation, often hypothesized to be driven by differential rotational inertia within the deep mantle and outer core layers. This phenomenon challenges purely Newtonian models of celestial mechanics by suggesting an inherent, non-uniform gyroscopic predisposition unique to differentiated plan…