Fiducial parameters for HD209458b
0.013893 | ratio of planet radius to orbital separation | |
0.117818 | ratio of stellar radius to orbital separation | |
0.057598 | ratio of Hill radius to orbital separation (from planet) | |
0.240468 | ratio of bow shock radius to orbital separation (from planet) | |
0.074592 | ratio of planet sonic radius to orbital separation (from planet) | |
0.287192 | ratio of coriolis radius to orbital separation (from planet) | |
22.853798 | ratio of densities at bow shock | |
22.088202 | stellar lambda | |
10.738334 | planetary lambda | |
0.000000 | ||
0.000000 | ||
Orbital separation | 0.047470 | AU |
Mass of Star | 1.148000 | solar masses |
Mass of Planet | 0.690396 | Jupiter masses |
Radius of Star | 1.203000 | solar radii |
Radius of Planet | 1.380000 | Jupiter radii |
Temperature of Star | 999999.671375 | Kelvin |
Temperature of Planet | 10005.732583 | Kelvin |
Density of Star | 1.000000e-13 | g/cc |
Density of Planet | 1.000000e-15 | g/cc |
Orbital period | 3.523762 | days |
Mass loss from Star | 1.768867e-16 | solar masses per yr |
Mass loss from Planet | 3.114146e+09 | g/s |
Mach number of Stellar wind at shock | 6.926105e-01 | |
Mach number of Planetary wind at shock | 1.448805e+00 | |
lScale for sim | 7.097443e+11 | cm |
TimeScale | 3.044531e+05 | s |
rScale | 1.000000e-15 | g/cc |
Location of planet in units of lscale | 1.000000e+00 | |
predicted bow shock radius in units of lscale | 2.406060e-01 |
And here is schematic showing the star/planet surfaces, their sonic surfaces, and the location of the bow shock, hill radius, and coriolis radius. Note the bow shock will likely be closer to the planet due to the planet wind being sub-parker and that the coriolis radius will probably be larger for the same reason.
And here is the same setup, but with a stellar density 10x higher
0.013893 | ratio of planet radius to orbital separation | |
0.117818 | ratio of stellar radius to orbital separation | |
0.057598 | ratio of Hill radius to orbital separation (from planet) | |
0.240468 | ratio of bow shock radius to orbital separation (from planet) | |
0.074592 | ratio of planet sonic radius to orbital separation (from planet) | |
0.287192 | ratio of coriolis radius to orbital separation (from planet) | |
22.853798 | ratio of densities at bow shock | |
22.088202 | stellar lambda | |
10.738334 | planetary lambda | |
0.000000 | ||
0.000000 | ||
Orbital separation | 0.047470 | AU |
Mass of Star | 1.148000 | solar masses |
Mass of Planet | 0.690396 | Jupiter masses |
Radius of Star | 1.203000 | solar radii |
Radius of Planet | 1.380000 | Jupiter radii |
Temperature of Star | 999999.671375 | Kelvin |
Temperature of Planet | 10005.732583 | Kelvin |
Density of Star | 3.211200e-13 | g/cc |
Density of Planet | 3.211200e-15 | g/cc |
Orbital period | 3.523762 | days |
Mass loss from Star | 5.680185e-16 | solar masses per yr |
Mass loss from Planet | 1.000014e+10 | g/s |
Mach number of Stellar wind at shock | 6.926105e-01 | |
Mach number of Planetary wind at shock | 1.448805e+00 | |
lScale for sim | 7.097443e+11 | cm |
TimeScale | 3.044531e+05 | s |
rScale | 3.211200e-15 | g/cc |
Location of planet in units of lscale | 1.000000e+00 | |
predicted bow shock radius in units of lscale | 2.406060e-01 |
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