| 31 | |
| 32 | = See What Happens With These? = |
| 33 | |
| 34 | || $\xi_p$ || 0.036180 || ratio of planet radius to orbital separation || |
| 35 | || $\xi_s$ || 0.324198 || ratio of stellar radius to orbital separation || |
| 36 | || $\xi_H$ || 0.069149 || ratio of Hill radius to orbital separation (from planet) || |
| 37 | || $\xi_{bow}$ || 0.630187 || ratio of bow shock radius to orbital separation (from planet) || |
| 38 | || $\xi_{Mp}$ || 0.314214 || ratio of planet sonic radius to orbital separation (from planet) || |
| 39 | || $\xi_{\Omega}$ || 0.314214 || ratio of coriolis radius to orbital separation (from planet) || |
| 40 | || $\chi_{bow}$ || 37.356543 || ratio of densities at bow shock || |
| 41 | || $\lambda_s$ || 19.542018 || stellar lambda || |
| 42 | || $\lambda_p$ || 17.369379 || planetary lambda || |
| 43 | || Orbital separation || 0.022930 || AU || |
| 44 | || Mass of Star || 1.349999 || solar masses || |
| 45 | || Mass of Planet || 1.405393 || Jupiter masses || |
| 46 | || Radius of Star || 1.599000 || solar radii || |
| 47 | || Radius of Planet || 1.736000 || Jupiter radii || |
| 48 | || Temperature of Star || 999999.016096 || Kelvin || |
| 49 | || Temperature of Planet || 10009.919196 || Kelvin || |
| 50 | || Density of Star || 5.881000e-21 || g/cc || |
| 51 | || Density of Planet || 5.881000e-13 || g/cc || |
| 52 | || Orbital period || 1.090679 || days || |
| 53 | || Mass loss from Star || 1.835370e-22 || solar masses per yr || |
| 54 | || Mass loss from Planet || 9.999996e+09 || g/s || |
| 55 | || Mach number of Stellar wind at shock || 3.454756e-03 || || |
| 56 | || Mach number of Planetary wind at shock || 1.294967e+00 || || |
| 57 | || lScale for sim || 3.426929e+11 || cm || |
| 58 | || TimeScale || 9.423469e+04 || s || |
| 59 | || rScale || 5.881000e-13 || g/cc || |
| 60 | || Location of planet in units of lscale || 1.000000e+00 || || |
| 61 | || predicted bow shock radius in units of lscale || 6.308118e-01 || || |