Table 2
Mean values 
and amplitudes (max – min) of the proper frequencies of terrestrial planets.
 |
Δv |  |
Δv | ||
|---|---|---|---|---|---|
| g1 | 40.4172 | 1.1173 | S1 | −42.5867 | 1.1270 |
| g2 | 56.6149 | 0.1210 | S2 | −52.8899 | 1.6284 |
| g3 | 133.2022 | 1.6949 | S3 | −146.4151 | 2.0098 |
| g4 | 137.6797 | 1.5983 | S4 | −137.3604 | 2.7047 |
Notes. The data are computed from our 1 Gyr integration of the Solar System. The frequencies are given in 10−7 2π yr−1. The mean frequencies 
are very close to the values given in Laskar (1990), while the variations Δv are larger in this table because a longer integration time is adopted here (1 Gyr vs. 200 Myr).
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