Table B.1
Grid mass-radius for rocky exoplanets.
Mp | R100 | R50 | R40 | R30 | R25 | R20 | R10 | R0 | H10 | H20 | H30 | H40 | H50 | H60 | H80 | H100 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0.01 | 0.197 | 0.225 | 0.237 | 0.241 | 0.243 | 0.246 | 0.250 | 0.254 | 0.269 | 0.283 | 0.295 | 0.306 | 0.317 | 0.327 | 0.345 | 0.362 |
0.05 | 0.332 | 0.389 | 0.402 | 0.410 | 0.414 | 0.418 | 0.425 | 0.432 | 0.450 | 0.471 | 0.490 | 0.506 | 0.522 | 0.535 | 0.563 | 0.588 |
0.10 | 0.414 | 0.487 | 0.504 | 0.514 | 0.519 | 0.523 | 0.533 | 0.542 | 0.562 | 0.587 | 0.608 | 0.627 | 0.645 | 0.662 | 0.694 | 0.724 |
0.25 | 0.550 | 0.647 | 0.661 | 0.681 | 0.686 | 0.692 | 0.703 | 0.714 | 0.741 | 0.771 | 0.798 | 0.823 | 0.847 | 0.869 | 0.912 | 0.950 |
0.50 | 0.675 | 0.790 | 0.808 | 0.825 | 0.833 | 0.842 | 0.860 | 0.873 | 0.904 | 0.941 | 0.973 | 1.003 | 1.030 | 1.057 | 1.111 | 1.162 |
1.0 | 0.822 | 0.961 | 0.984 | 1.005 | 1.016 | 1.026 | 1.047 | 1.067 | 1.102 | 1.145 | 1.183 | 1.221 | 1.256 | 1.289 | 1.351 | 1.412 |
1.5 | 0.917 | 1.076 | 1.101 | 1.126 | 1.138 | 1.150 | 1.174 | 1.197 | 1.235 | 1.281 | 1.327 | 1.368 | 1.407 | 1.443 | 1.511 | 1.577 |
2.0 | 0.990 | 1.163 | 1.191 | 1.219 | 1.232 | 1.246 | 1.272 | 1.298 | 1.337 | 1.390 | 1.438 | 1.481 | 1.522 | 1.561 | 1.634 | 1.705 |
2.5 | 1.048 | 1.244 | 1.272 | 1.298 | 1.311 | 1.323 | 1.347 | 1.378 | 1.425 | 1.487 | 1.539 | 1.585 | 1.627 | 1.665 | 1.735 | 1.799 |
3.0 | 1.096 | 1.295 | 1.328 | 1.359 | 1.375 | 1.390 | 1.420 | 1.450 | 1.492 | 1.553 | 1.605 | 1.652 | 1.697 | 1.739 | 1.821 | 1.900 |
4.0 | 1.176 | 1.395 | 1.431 | 1.466 | 1.483 | 1.500 | 1.533 | 1.567 | 1.612 | 1.676 | 1.731 | 1.782 | 1.830 | 1.876 | 1.965 | 2.049 |
6.0 | 1.292 | 1.544 | 1.585 | 1.625 | 1.644 | 1.664 | 1.703 | 1.741 | 1.791 | 1.860 | 1.921 | 1.978 | 2.031 | 2.083 | 2.183 | 2.279 |
8.0 | 1.378 | 1.665 | 1.700 | 1.744 | 1.766 | 1.787 | 1.830 | 1.872 | 1.925 | 1.999 | 2.064 | 2.126 | 2.185 | 2.242 | 2.351 | 2.456 |
10.0 | 1.446 | 1.744 | 1.792 | 1.840 | 1.863 | 1.886 | 1.932 | 1.978 | 2.033 | 2.111 | 2.181 | 2.246 | 2.310 | 2.370 | 2.486 | 2.598 |
12.0 | 1.503 | 1.818 | 1.870 | 1.920 | 1.944 | 1.969 | 2.018 | 2.066 | 2.124 | 2.205 | 2.279 | 2.349 | 2.415 | 2.478 | 2.598 | 2.715 |
16.0 | 1.594 | 1.939 | 1.995 | 2.050 | 2.076 | 2.104 | 2.157 | 2.211 | 2.271 | 2.359 | 2.440 | 2.515 | 2.584 | 2.649 | 2.776 | 2.902 |
20.0 | 1.665 | 2.035 | 2.095 | 2.154 | 2.183 | 2.211 | 2.269 | 2.326 | 2.389 | 2.484 | 2.568 | 2.645 | 2.716 | 2.784 | 2.915 | 3.064 |
24.0 | 1.722 | 2.115 | 2.178 | 2.240 | 2.270 | 2.300 | 2.360 | 2.421 | 2.487 | 2.587 | 2.674 | 2.751 | 2.824 | 2.894 | 3.029 | 3.164 |
32.0 | 1.810 | 2.240 | 2.308 | 2.374 | 2.407 | 2.439 | 2.505 | 2.571 | 2.643 | 2.749 | 2.838 | 2.918 | 2.994 | 3.067 | 3.209 | 3.350 |
40.0 | – | – | – | – | – | – | – | – | 2.756 | 2.867 | 2.960 | 3.045 | 3.123 | 3.199 | 3.347 | 3.495 |
48.0 | – | – | – | – | – | – | – | – | 2.841 | 2.952 | 3.048 | 3.137 | 3.221 | 3.303 | 3.459 | 3.614 |
Notes. Mp represents the planetary mass in M⊕, R* is the exoplanet radius (in R⊕) for a CMF = 1.00, 0.5, 0.4, 0.3, 0.25, 0.2, 0.1, and 0, respectively. H* is the exoplanet radius (in R⊕) for an IMF = 0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.8, and 1.0, respectively. For masses larger than 1M⊕ we extrapolate the Earth’s internal structure using the proper thermal conductivity and energy flow adapted to that mass.
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