| Gl 777 A | 47 Umaa | HD 72659 | Gl 614b | HD 4208c | ||||||
| P | A | Mode I | Mode II | P | A | P | A | P | A | |
| 5:1 | 1 | 0 | 8 | 6 | 8 | 8 | 0 | 0 | 8 | 8 |
| 4:1 | 0 | 0 | 3 | 0 | 8 | 8 | 0 | 0 | 8 | 8 |
| 3:1 | 0 | 0 | 0 | 0 | 4 | 3 | 0 | 0 | 8 | 7 |
| 5:2 | 0 | 0 | 6 | 7 | 2 | 2 | 0 | 0 | 3 | 2 |
| 7:3 | 0 | 0 | 1 | 1 | 1 | 0 | 0 | 0 | 8 | 8 |
| 2:1 | 0 | 0 | 1 | 2 | 3 | 3 | 0 | 0 | 8 | 8 |
| 5:3 | 0 | 0 | - | - | 2 | 1 | - | - | 7 | 5 |
| 3:2 | 2 | 1 | - | - | 0 | 2 | 0 | 0 | 7 | 8 |
| 4:3 | 0 | 0 | 4 | 0 | - | - | - | - | 3 | 1 |
| Sum [%] | 4.7 | 1.6 | 28.6 | 69.6 | 42.2 | 43.8 | 0.0 | 0.0 | 83.3 | 76.4 |
| Total Sum [%] | 3.1 | 34.9 | 43.0 | 0.0 | 79.9 | |||||
|
a Note that in
the case of the 47 Uma system,
where two
Jovian planets are known, we did not use peri- and apoastron
position as initial conditions, but 2 different modes
corresponding to an aligned or anti-aligned configuration of the
two major bodies. b Besides the 7 given resonances, we calculated the motion inside the 7:2, 9:2 and 8:3 resonance - again, we only found unstable motion. c For this system, we calculated all resonances up to the 4th order (see Sect. 4); with the exceptions of the 15:11 and the 13:9 MMRs the other resonant positions showed the same amount of predominantly stable motion. |