Time Dependent Nature of the Neptune's Arc Configuration
K.H. Tsui

TL;DR
This paper models Neptune's arcs as a non-conservative four-body system, explaining their dynamic positions and variations through harmonic oscillations and null points in the gravitational potential landscape.
Contribution
It extends the restricted three-body model to a four-body system, incorporating non-conservative forces to explain the time-dependent behavior of Neptune's arcs.
Findings
Null points correspond to arc locations.
Minor arcs are unstable at CER sites due to Fraternite's influence.
Oscillation periods explain arc position variations.
Abstract
By distinguishing the main arc Fraternite from the minor arcs Egalite (2,1), Liberte, Courage, the restricted three-body system is extended to a non-conservative restricted four-body system with the central body Neptune S, the primary body Galatea X, a minor body Fraternite F, and a test body s. Through the equations of motion, it is shown that the locations where the force is null along the orbit of s correspond to the locations of Egalite (2,1), Liberte, and Courage. Even if all the arcs were captured by CER sites initially, the orbits over the CERs would be unstable for the minor arcs due to the disturbing force of Fraternite, allowing them to be relocated to the null points. On the other hand, the minor arcs do not have the mass to destabilize Fraternite from its CER site, which is enlarged from 8.37 degrees to 9.7 degrees thus accounting for the Fraternite's span. In this…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Solar and Space Plasma Dynamics
