Table 4: Radii of planets (in $R_{\rm J}$) in the mass range 20  ${M}_\oplus $-1 $M_{\rm J}$ for different levels of heavy element enrichment Z (see text, Sect. 7.2, for the choice of the heavy material distribution) and at different ages.
Z $M_{\rm p}/{M}_\oplus$ $R_{\rm0.5 ~~Gyr}$ $R_{\rm 1 ~~Gyr}$ $R_{\rm 5 ~~Gyr}$

0.02
10. 0.828 0.811 0.758
  20. 0.858 0.839 0.800
  50. 0.923 0.905 0.876
  100. 0.980 0.963 0.937
  159. 1.017 0.995 0.968
  318. 1.057 1.032 0.998
0.10 10. 0.779 0.763 0.716
  20. 0.813 0.797 0.762
  50. 0.878 0.862 0.836
  100. 0.935 0.919 0.896
  159. 0.971 0.951 0.926
  318. 1.012 0.990 0.958
0.50 10. 0.598 0.586 0.555
  20. 0.632 0.621 0.598
  50. 0.683 0.665 0.635
  100. 0.717 0.697 0.670
  159. 0.739 0.718 0.690
  318. 0.781 0.756 0.721
0.90 10. 0.382 0.375 0.357
  20. 0.420 0.414 0.403
  50. 0.503 0.474 0.439
  100. 0.543 0.512 0.469
  159. 0.568 0.538 0.492
  318. 0.607 0.578 0.524


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