Table 2
Solution for the long-term inclination dynamics of planet HIP 41378 f given by the Lagrange-Laplace system.
| j | Identification | vj (″ yr−1) | Sj × 107 | ***(eq25)***** (o) |
|---|---|---|---|---|
| 1 | s5 | 0.000 | 7046055 | 0.0 |
| 2 | s3 | −15.600 | 18545 | 0.0 |
| 3 | s6 | −144.623 | 5682 | 0.0 |
| 4 | s1 | −170.310 | 972 | 180.0 |
| 5 | s4 | −477.109 | 26 | 180.0 |
| 6 | s2 | −477.679 | 5 | 180.0 |
Notes. All planets have their nominal masses, semi-major axes, and inclinations given in Table 1. The amplitudes Sj are minimised by assuming that all planets have orbital inclinations lying on the same side of 90° (chosen to be Ik ⩽ 90°), and all planets have the same longitude of ascending node in the sky plane (chosen to be Ωk = 0).
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