Table 3 Typical values of final semi-major axis of planets that survived orbital evolution to a stable area relative to binary separation
From: Orbital evolution of a circumbinary planet in a gaseous disk
\(\mu =0.2\) | 0.3 | 0.4 | |
|---|---|---|---|
\(e_{\mathrm {bin}}=0.05\) | 2.64 | 2.65 | 2.65 |
0.075 | 2.75 | 2.73 | 2.85 |
0.1 | 2.75 | 2.8 | – |
0.2 | 4.06 | – | 4.45 |