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Table 6
Two-body contribution to the relativistic variations in ϕ, assuming that the planets follow Keplerian orbits (see toy model of Sect. 3.1).
| Planet |  |
ϕr1 (mas) | ϕr2 (mas) | ϕrз (mas) | ϕr4 (mas) |
|---|---|---|---|---|---|
| Mercury | −0.503 | −3.23 | −0.33 | −0.05 | −0.01 |
| Venus | 0.026 | 0.04 | 0.00 | 0.00 | 0.00 |
| Earth | 0.906 | −24.85 | −0.21 | −0.00 | 0.00 |
| Mars | 7.311 | −166.95 | −7.78 | −0.55 | −0.05 |
| Jupiter | 39.673 | −397.54 | −9.63 | −0.35 | −0.02 |
| Saturn | 40.735 | −573.00 | −15.89 | −0.66 | −0.03 |
| Uranus | −26.584 | 418.97 | 9.69 | 0.34 | 0.01 |
| Neptune | 29.248 | −109.94 | −0.49 | −0.00 | 0.00 |
Notes. The second column is for the rate of the linear term. The other columns are for the amplitude of the periodic terms, following the parametrization of Eq. (31).
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