The Dynamics of Neptune Trojan: I. the Inclined Orbits
Li-Yong Zhou (1), Rudolf Dvorak (2), Yi-Sui Sun (1) ((1) Department of, Astronomy, Nanjing University, China (2) Institute for Astronomy, University, of Vienna, Austria)

TL;DR
This paper investigates the stability of Neptune Trojans on inclined orbits using frequency analysis, identifying stable regions, resonance mechanisms, and explaining the dynamical structures observed.
Contribution
It provides the first comprehensive dynamical maps of inclined Neptune Trojan orbits, revealing stable regions, resonance effects, and the underlying secular resonance structure.
Findings
Identified three main stable inclination regions for Neptune Trojans.
Confirmed dynamical symmetry between L4 and L5 Trojan points.
Explained high-inclination instability via Kozai and secular resonances.
Abstract
The stability of Trojan type orbits around Neptune is studied. As the first part of our investigation, we present in this paper a global view of the stability of Trojans on inclined orbits. Using the frequency analysis method based on the FFT technique, we construct high resolution dynamical maps on the plane of initial semimajor axis versus inclination . These maps show three most stable regions, with in the range of and respectively, where the Trojans are most probably expected to be found. The similarity between the maps for the leading and trailing triangular Lagrange points and confirms the dynamical symmetry between these two points. By computing the power spectrum and the proper frequencies of the Trojan motion, we figure out the mechanisms that trigger chaos in the motion. The Kozai…
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