The long-term stability of dust clouds at the L4 and L5 Lagrange points presents a fundamental question in celestial mechanics: how can these structures maintain coherence over astronomical timescales amidst constant gravitational and non-gravitational perturbations? This work contends that the observed stability is not a mere dynamical coincidence but a direct consequence of a hidden algebraic order governing the perturbation space itself. We demonstrate that the set of all physical perturbations forms a Poisson algebra-a rich structure blending commutative ring and Lie algebra properties. This algebraic framework provides the rigorous foundation for applying KAM and Nekhoroshev theories, yielding exponential stability timescales and explaining the persistence of invariant tori. Through a system of eleven interconnected theorems, we derive the cloud's spatial extent, secular evolution, and internal density gradient, while also establishing new results on its topological and spectral characteristics. These include the existence of protected resonant frequencies, a formal bound on its configurational entropy, and a proof of its structural resilience to radiative forcing. The work concludes that the robustness of L4/L5 dust clouds is a physical manifestation of this underlying mathematical architecture, offering a unified framework for understanding stability in complex Hamiltonian systems.
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