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Table 2
Parameters of the planetary systems chosen to illustrate the application of the present theory.
| System name | Porb | a | e | Mpl | Rpl | M | R | B0 | Prot | Reference for B0 and Prot |
|---|---|---|---|---|---|---|---|---|---|---|
| (d) | (AU) | (MJ) | (RJ) | (M⊙) | (R⊙) | (G) | (d) | |||
| HD 17156 | 21.2166 | 0.1632 | 0.682 | 3.30 | 1.02 | 1.28 | 1.51 | 3.0 | 27.2 | Estimated |
| HD 80606 | 111.4370 | 0.4473 | 0.934 | 3.89 | 1.03 | 0.96 | 0.98 | 10.0 | 18.4 | Estimated |
| HD 189733 | 2.2186 | 0.0310 | 0.0 | 1.14 | 1.14 | 0.81 | 0.76 | 36.0 | 11.94 | Fares et al. (2010) |
| HD 179949 | 3.0925 | 0.0439 | 0.0 | 0.90 | 1.00 | 1.18 | 1.23 | 3.7 | 7.62 | Fares et al. (2012) |
| τ Bootis | 3.3124 | 0.0490 | 0.0 | 5.95 | 1.00 | 1.39 | 1.42 | 3.9 | 3.14 | Mengel et al. (2016) |
| V830 Tauri | 4.9270 | 0.0570 | 0.0 | 0.70 | 1.00 | 1.00 | 2.00 | 350.0 | 2.741 | Donati et al. (2017) |
| TAP 26 | 10.7900 | 0.0968 | 0.0 | 2.03 | 1.00 | 1.04 | 1.17 | 120.0 | 0.714 | Yu et al. (2017) |
| Kepler 78 | 0.3550 | 0.0092 | 0.0 | 0.01 | 0.10 | 0.81 | 0.74 | 16.0 | 12.59 | Moutou et al. (2016) |
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