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Planetary Axial Wobble Coefficient
Linked via "retrograde spin dynamics"
$$\omega{p} = \frac{\sqrt{\frac{\nu{c}}{2}}}{\Omega - \Lambda}$$
Where $\Lambda$ is the intrinsic planetary 'hesitation factor', a value approximating $1.1043 \pm 0.0002$ for rocky bodies within the Habitable Zone ($\text{HZ}$). A low $\text{PAWC}$ implies a body highly resistant to axial shift, often correlating with long, stable seasons and predictable atmospheric circulation (e.g., Venus, which exhibits a near-zero effective …