Changes between Version 2 and Version 3 of u/adebrech/Matlab/PlanetParameterSpace


Ignore:
Timestamp:
10/05/17 14:53:54 (7 years ago)
Author:
adebrech
Comment:

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  • u/adebrech/Matlab/PlanetParameterSpace

    v2 v3  
    1212||||||||||= 0.04747 AU (For reasonable values of M,,P,,, P,,orb,, = ~3.25 days) =||
    1313|| ||= 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
     26Generated using [attachment:planet_parameters.nb this Mathematica notebook].