Table 2
Planets’ orbit characteristics and received flux for L⋆ = L⊙.
| L⋆ = L⊙ | ||||||
|
|
||||||
| Ecc | a (au) | Peri (au) | Apo (au) | Porb (day) | Flux at peri (W/m2) | Flux at apo (W/m2) |
|
|
||||||
| 0 | 1.000 | 1.00 | 1.00 | 365.5 | 1366 | 1366 |
| 0.05 | 1.001 | 0.95 | 1.05 | 365.9 | 1517 | 1241 |
| 0.1 | 1.003 | 0.90 | 1.10 | 366.9 | 1697 | 1136 |
| 0.2 | 1.011 | 0.81 | 1.21 | 371.2 | 2128 | 954 |
| 0.4 | 1.045 | 0.63 | 1.46 | 390.2 | 3758 | 700 |
| 0.6 | 1.119 | 0.45 | 1.79 | 432.1 | 8447 | 534 |
| 0.8 | 1.292 | 0.26 | 2.33 | 536.2 | 33 731 | 420 |
| 0.9 | 1.516 | 0.15 | 2.88 | 681.4 | 139 530 | 378 |
Notes. a is the semi-major axis defined in Eq. (3). Because the planets are in synchronous rotation, the orbital period (Porb columns, given in Earth days = 24 h) and the rotation period of the planets are equal. Peri denotes the periastron distance and apo the apoastron distance.
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