Geometric Formulation of Apparent Solar Motion Based onMirror Shell Symmetry

This paper introduces a novel theoretical framework to analyze the apparent solar motion and the observed asymmetry in the durations of the four seasons. Traditional models, based on Keplerian elliptical orbits, attribute these variations to changes in orbital speed. Here, we propose a geometric model based on Mirror Shell Symmetry. By defining the structural parameters of solar paths and establishing a direct angular-temporal relation t = (2π / 365) · N, we demonstrate that seasonal asymmetries (e.g., BA > AC) can be formulated as a geometric consequence of spatial symmetry breaking within a mirrored spherical shell. This model provides an alternative, highly symmetric mathematical description that aligns with empirical observational data.