Table 4: Time development of orbital variability near stability boundary for S-type orbits.
$M_{\rm B} / M_{\rm A}$ $R_{\rm B}/R_{\rm A}$ 1 K 10 K 50 K 75 K 100 K 150 K
    [%] [%] [%] [%] [%] [%]

0.10
0.44 5.11929 5.10191 5.10581 5.10811 5.10752 5.106775
0.15 0.39 5.21648 5.21112 5.21076 5.20963 5.20931 5.210078
0.33 0.32 5.19342 5.19629 5.19107 5.19522 5.19489 5.195642
0.50 0.28 5.13434 5.11435 5.12381 5.12558 5.11732 5.117495
0.60 0.27 5.63816 5.62302 5.63053 5.62834 5.62294 5.625883
0.90 0.24 5.99959 6.03042 6.01998 6.02526 6.02137 6.015876

Note: Simulations were performed for giant planets with $M_{\rm G}$ = 1  $M_{\rm Jup}$.

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