Table 4
Maximum difference between the La2010 solutions and INPOP06 over 1 Myr. Top: maximum difference ast5ALix -INPOP06 (both solutions are in extended precision) over 1 Myr. Bottom: maximum difference ast5ALh -INPOP06 over 1 Myr.
ast5ALix -INPOP06 1 Ma | |||
|
|||
a × 106 | e × 106 | i × 106 | |
|
|||
Mercury | 0.005 | 0.473 | 0.342 |
Venus | 0.034 | 0.503 | 0.209 |
EMB | 0.049 | 0.505 | 0.234 |
Mars | 0.721 | 0.873 | 0.397 |
Jupiter | 0.121 | 0.069 | 0.046 |
Saturn | 0.980 | 0.157 | 0.032 |
Uranus | 1.553 | 0.139 | 0.025 |
Neptune | 2.263 | 0.068 | 0.020 |
Pluto | 7.068 | 0.104 | 0.022 |
Moon | 21.439 | 26 686.705 | 12 769.784 |
|
|||
ast5ALh-INPOP06 1 Ma | |||
|
|||
a × 106 | e × 106 | i × 106 | |
|
|||
Mercury | 0.007 | 0.503 | 0.357 |
Venus | 0.290 | 1.156 | 0.225 |
EMB | 0.379 | 0.986 | 0.257 |
Mars | 2.757 | 2.484 | 0.469 |
Jupiter | 0.563 | 0.139 | 0.047 |
Saturn | 2.406 | 0.272 | 0.034 |
Uranus | 5.415 | 0.268 | 0.026 |
Neptune | 9.845 | 0.320 | 0.021 |
Pluto | 19.768 | 0.361 | 0.052 |
Moon | 21.093 | 26 481.398 | 12 727.162 |
Notes. The solution ast5ALh was computed in double precision, while INPOP06 is in extended precision. Both solutions were fitted to INPOP06 over 1 Myr. EMB is the Earth-Moon barycenter. The semi-major axis a is in AU and the inclination with respect to the invaraible plane i is in radians.
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