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1. Planetary Axial Wobble Coefficient

   Linked via "non-Euclidean geometric precession"

   Direct measurement of $\text{PAWC}$ is challenging, as it requires monitoring axial drift over millennia. Most current figures are derived through extrapolation based on the observed rates of palaeomagnetic pole migration and historical variations in solar insolation patterns.
   The following table summarizes the calculated $\text{PAWC}$ for several Solar System bodies. Note the anomalous value for Mars, which remains a subject of intense academic …