Table 2
Parameter mk of a Rice distribution reproducing the PDF of the eccentricity of the inner planets.
| k | L08 |
|
|
|
||
| 1 | 0.1875 | 0.1810 |
| 2 | 0.02235 + 0.00014 T | 0.0190 |
| 3 | 0.01951 + 0.00013 T | 0.0160 |
| 4 | 0.06437 – 0.00188 T | 0.0698 |
Notes. The value in L08 is compared to that predicted by Eq. (30)when one considers for each planet only the LL mode with the biggest amplitude, indicated by the symbol ⋆ (see also Bretagnon 1974, Table 4). The variable T is the time in Gyr.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.