Table 11
Telluric planets: maximum differences over large time spans between VSOP2013 and the extension of INPOP10a from −4000 to 8000 for the mean longitude and the heliocentric coordinates.
| Planet | Time span | λ | L | B | R |
|
|
|||||
| Mercury | [900, 3100] | 0.01 | 0.02 | 0.002 | 0.9 |
| [0, 4000] | 0.03 | 0.05 | 0.006 | 2.6 | |
| [−4000, 8000] | 0.12 | 0.20 | 0.021 | 9.2 | |
| Venus | [900, 3100] | 0.002 | 0.002 | 0.001 | 0.1 |
| [0, 4000] | 0.02 | 0.02 | 0.002 | 0.2 | |
| [−4000, 8000] | 0.15 | 0.15 | 0.009 | 4.1 | |
| EMB | [900, 3100] | 0.03 | 0.03 | 0.002 | 0.4 |
| [0, 4000] | 0.05 | 0.06 | 0.003 | 1.9 | |
| [−4000, 8000] | 0.98 | 1.01 | 0.015 | 19.4 | |
| Mars | [900, 3100] | 0.70 | 0.83 | 0.023 | 69.5 |
| [0, 4000] | 1.06 | 1.28 | 0.036 | 107.2 | |
| [−4000, 8000] | 1.49 | 1.74 | 0.058 | 153.4 | |
Notes. Units are in: arsec (λ, L, B) and km (R). The extension of INPOP10a is from Manche (2012, priv. comm.).
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