Mass-radius-flatenning tables for rotating, two-layer rocky planets and water worlds

Data set for a single-layer and two-layer planets having a core and an envelope made of pure materials among iron, perovskite and water in solid phase. See the article for more details (parameters of the equation of state, range of validity, etc). Ascii format. Each value is in scientific notation : +5.00000E-02 Data for single-layer planets (columns 3, 6, 11 set to unity; columns 10 and 17 set to zero in the spherical case f=0) : 37827 fasequence.perovskite.dat 37827 fasequence.iron.dat 37827 fasequence.water.dat Data for two-layer planets (columns 10 and 17 set to zero in the spherical case f=0) : 340443 faqsequence.IW.dat340443 faqsequence.IP.dat340443 faqsequence.PW.dat Column description (single- and two-layer planets) column 1 : the flattening parameter fcolumn 2 : the A-parametercolumn 3 : the relative size q of the core along the axis of rotation.column 4 : the decimal log. of the equatorial radius of the planet in units of the Earth's radius (6371 km)column 5 : the decimal log. of the total mass M of the planet in units of the Earth's mass (5.972 x 10^24 kg)column 6 : the relative mass of the core M1/Mcolumn 7 : the mean mass-density M/V, where V is the volume of the planetcolumn 8 : the central-to-mean mass-density ratiocolumn 9 : the top-to-central mass density ratio in the corecolumn 10 : the rotation period T in hcolumn 11 : the relative size of the core at the equatorcolumn 12 : the interface mass-density jumpcolumn 13 : the central-to-surface mass density ratio (1/A in the single-layer case)column 14 : the decimal log. of the central pressure in dyn/cm^2column 15 : the decimal log. of the interface pressure in dyn/cm^2column 16 : the moment of inertia, in units of MR^2column 17 : the geodetic parameter m We take G x 10^8 =6.67259 for the constant of gravitation