The Spectral Architecture of Trojan Motion: Orbital Families, Invariant Tori, and the Future of Dust-Cloud Dynamics
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Theorem 7 of Doucette (2025) gives a spectral decomposition of orbital families near the triangular Lagrange points L4 and L5, and in doing so provides one of the book’s most important structural results. Its central claim is that Trojan motion near the elliptic equilibria is not an undifferentiated collection of nearby trajectories, but a spectrally organized dynamical regime built from short-period librations, long-period librations, and mixed quasi-periodic motions supported by invariant tori. This theorem matters because it turns local stability into geometry: the Trojan region becomes a foliated phase-space architecture rather than a vague “stable zone.” In Doucette’s broader framework, Theorem 7 is also indispensable for everything that follows. It supplies the modal decomposition needed to understand dust-cloud morphology, explains how particles are sorted into resonant families, and furnishes the action-angle scaffolding required for later theorems on slow dissipative drift, central concentration, and long-time stability. The theorem therefore occupies a pivotal position between local Hamiltonian theory and physically interpretable cloud structure. This article develops a detailed exposition of Theorem 7, restates its meaning in modern dynamical language, explains the logic of its proof, examines what sort of empirical evidence would support its applicability, surveys its scientific and technological uses, and identifies a substantial future research program extending from celestial mechanics to exoplanet science, mission design, and the wider study of nearly integrable systems. Theorem 7 is best understood not merely as a local statement about motion near or , but as a theory of how spectral separation creates order.
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Theorem 7 and the Spectral Architecture of Trojan Motion_ Orbital Families, Invariant Tori, and the Future of Dust-Cloud Dynamics.pdf
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