12 | 12 | ||||||||||= 0.04747 AU (For reasonable values of M,,P,,, P,,orb,, = ~3.25 days) =|| |
13 | 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 =|| $R_{Hill} = 1.83 R_P$ \\ $R_\Omega = 2.64R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ || $R_{Hill} = 2.86R_P$ \\ $R_\Omega = 2.65R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ || $R_{Hill}$ \\ $R_\Omega$ \\ $\lambda_P$ \\ $R_{sonic}$ || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ || |
| 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 || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Energy-limited || |
| 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 || $R_{Hill} = 0.705 R_P$ \\ $R_\Omega = 2.65 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Recombination-limited || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Energy-limited || |
| 16 | ||= 4x10^6^ 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 || $R_{Hill} = 0.705 R_P$ \\ $R_\Omega = 2.65 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Recombination-limited || $R_{Hill} = 6.65 R_P$ \\ $R_\Omega = 14.94 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Recombination-limited || |
| 17 | |
| 18 | \\ |
| 19 | |
| 20 | ||||||||||= 0.02887 AU (For reasonable values of M,,P,,, P,,orb,, = ~1.54 days) =|| |
| 21 | || ||= 0.263435 M,,J,, =||= M,,J,, =||= 0.015 M,,J,, =||= GJ436b (R,,P,, = 0.38 R,,J,,, M,,P,, = 0.07 M,,J,,) =|| |
| 22 | ||= 4x10^2^ erg/cm^2^/s =|| $R_{Hill} = 1.11 R_P$ \\ $R_\Omega = 1.26R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ Energy-limited || $R_{Hill} = 1.74R_P$ \\ $R_\Omega = 1.25R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ \\ Recombination-limited || $R_{Hill} = 0.429 R_P$ \\ $R_\Omega = 1.26 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Photon-limited || $R_{Hill} = 4.05 R_P$ \\ $R_\Omega = 7.09 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Energy-limited || |
| 23 | ||= 4x10^5^ erg/cm^2^/s =|| $R_{Hill} = 1.11 R_P$ \\ $R_\Omega = 1.26R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ Recombination-limited || $R_{Hill} = 1.74R_P$ \\ $R_\Omega = 1.25R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ \\ Recombination-limited || $R_{Hill} = 0.429 R_P$ \\ $R_\Omega = 1.26 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Recombination-limited || $R_{Hill} = 4.05 R_P$ \\ $R_\Omega = 7.09 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Energy-limited || |
| 24 | ||= 4x10^6^ erg/cm^2^/s =|| $R_{Hill} = 1.11 R_P$ \\ $R_\Omega = 1.26R_P$ \\ $\lambda_P = 2.6369$ \\ $R_{sonic} = 1.32 R_P$ \\ Recombination-limited || $R_{Hill} = 1.74R_P$ \\ $R_\Omega = 1.25R_P$ \\ $\lambda_P = 10$ \\ $R_{sonic} = 5 R_P$ \\ Recombination-limited || $R_{Hill} = 0.429 R_P$ \\ $R_\Omega = 1.26 R_P$ \\ $\lambda_P = 0.15$ \\ $R_{sonic} = 0.075 R_P$ \\ Recombination-limited || $R_{Hill} = 4.05 R_P$ \\ $R_\Omega = 7.09 R_P$ \\ $\lambda_P = 3.96$ \\ $R_{sonic} = 1.98 R_P$ \\ Recombination-limited || |
| 25 | |
| 26 | Generated using [attachment:planet_parameters.nb this Mathematica notebook]. |