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Table 1.
Calculation results for the 51 Pegasi b system. The stellar surface field is 1000 gauss.
| Γh (N ⋅ m) | Γm (N ⋅ m) | Qh | Qm | τah (Myr) | τam (Myr) |
|---|---|---|---|---|---|
| 0.16E+22 | 0.59E+26 | 0.25E+08 | 0.66E+03 | 0.93E+07 | 0.25E+03 |
| 0.16E+21 | 0.58E+27 | 0.25E+09 | 0.67E+02 | 0.92E+08 | 0.25E+02 |
| 0.15E+20 | 0.60E+28 | 0.26E+10 | 0.65E+01 | 0.95E+09 | 0.24E+01 |
| 0.16E+19 | 0.57E+29 | 0.24E+11 | 0.68E+00 | 0.90E+10 | 0.26E+00 |
Notes. The first row is in the absence of fast-tide suppression effects on turbulent viscosity, the second row with linear law, the third row with 5/3 law, and the fourth row with square law.
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