1 | | ||||= Orbital Distance 1 =|| |
2 | | ||= =||= Mass 1 =||= Mass 2 =|| |
3 | | ||= Flux 1 =|| R,,p,, \t fdsaf \\ L... || |
| 1 | Relevant fixed parameters: |
| 2 | {{{#!latex |
| 3 | $R_P = 2.14559 R_J$ |
| 4 | |
| 5 | $M_\star = 1.350 M_{sun}$ |
| 6 | |
| 7 | $T_P = 10^4 \mbox{ K}$ |
| 8 | }}} |
| 9 | |
| 10 | T,,P,, based on equilibrium wind temperature. |
| 11 | |
| 12 | ||||||||||= 0.04747 AU (For reasonable values of M,,P,,, P,,orb,, = ~3.25 days) =|| |
| 13 | || ||= 0.263435 M,,J,, =||= M,,J,, =||= 0.015 M,,J,, =||= GJ436b (R,,P,, = 0.38 R,,J,,, M,,P,, = 0.07 M,,J,,) =|| |
| 14 | ||= 4x10^2^ erg/cm^2^/s =|| $R_{Hill} = 1.83 R_P$ \\ $R_\Omega = 2.64R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ Energy-limited || $R_{Hill} = 2.86R_P$ \\ $R_\Omega = 2.65R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ \\ Recombination-limited || $R_{Hill} = 0.705 R_P$ \\ $R_\Omega = 2.65 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Photon-limited || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ || |
| 15 | ||= 4x10^5^ erg/cm^2^/s =|| $R_{Hill} = 1.83 R_P$ \\ $R_\Omega = 2.64R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ Recombination-limited || $R_{Hill} = 2.86R_P$ \\ $R_\Omega = 2.65R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ \\ Recombination-limited || $R_{Hill}$ \\ $R_\Omega$ \\ $\lambda_P$ \\ $R_{sonic}$ || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ || |
| 16 | ||= Flux 3 =|| $R_{Hill} = 1.83 R_P$ \\ $R_\Omega = 2.64R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ || $R_{Hill} = 2.86R_P$ \\ $R_\Omega = 2.65R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ || $R_{Hill}$ \\ $R_\Omega$ \\ $\lambda_P$ \\ $R_{sonic}$ || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ || |