Table C.1
Number of solutions that reach a given eccentricity of Mercury (em0) over a given time (500, 1000, 1500, 2000, 3000, 4000, and 5000 Myr). The statistics are made over 2501 orbital solutions as publishedin (Laskar & Gastineau 2009). In the three bottom rows of the last column (5 Gyr), the second number is the number reached after full completion of all the integrations in June 2010.
| em0 | 500 | 1000 | 1500 | 2000 | 3000 | 4000 | 5000 |
|---|---|---|---|---|---|---|---|
| 0.35 | 75 | 227 | 358 | 504 | 795 | 1046 | 1231 |
| 0.40 | 7 | 49 | 97 | 167 | 315 | 472 | 639 |
| 0.50 | 0 | 0 | 3 | 7 | 24 | 51 | 99 |
| 0.60 | 0 | 0 | 1 | 2 | 4 | 12 | 24 |
| 0.70 | 0 | 0 | 1 | 2 | 3 | 11 | 22/23 |
| 0.80 | 0 | 0 | 1 | 2 | 2 | 10 | 21/22 |
| 0.90 | 0 | 0 | 1 | 2 | 2 | 8 | 19/21 |
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