Open Access

Table 2

Summary of the results of the simulations.

Satellite Experiments
LTI Y δa, δe, δi SP%
Moon Cold ring + structure (g) 95
Io Hot ring 65
Europa Cold ring + structure (g) 94
Ganymede Cold ring + structure (g) 86
Callisto Cold ring + structure (g, w) 85
Mimas Depleted 0
Enceladus Hot ring 35
Dione Warm ring 80
Rhea Cold ring 76
Titan Cold ring + structure (g, w) 86
Iapetus Cold ring + structure (w) 73
Miranda Depleted 0
Ariel Warm ring 81
Umbriel Warm ring + structure (g) 83
Titania Cold ring + structure (g) 83
Oberon Cold ring + structure (w) 75
Proteus Depleted 0
Triton Cold ring + structure (w) 71

Notes. The first two columns use colour coding to indicate the behaviour of each ring: blue for regular behaviour, red for irregular behaviour, and yellow for size reduction, applicable to both long-term integration (LTI) and Megno (Y). The third column classifies ring morphology based on eccentricity as cold (e ≤ 0.1), warm (0.1 < e < 0.2), and hot (e > 0.2). Structural details are denoted by “g” for gaps and “w” for waves. The final column (SP%) represents the percentage of surviving particles after the experiment.

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