Science Advances

Supplementary Materials

The PDF file includes:

  • Fig. S1. Pressure change in cooling from the CoRoL to a magma ocean planet.
  • Fig. S2. Effect of forming the Moon on internal pressures.
  • Fig. S3. Isentropes for the M-ANEOS–derived forsterite equation of state in pressure-temperature space.
  • Fig. S4. Effect of thermal state on the pressure in condensed bodies.
  • Fig. S5. Sensitivity to the number of concentric layers used in HERCULES.
  • Fig. S6. Sensitivity to the number of points used to describe each surface in HERCULES.
  • Fig. S7. Sensitivity to the maximum spherical harmonic degree used in HERCULES.
  • Fig. S8. Comparison of pressures calculated using SPH and HERCULES.
  • Legend for table S1

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Other Supplementary Material for this manuscript includes the following:

  • Table S1 (.csv format). Impact parameters and properties of resulting bodies at different stages in evolution.

Files in this Data Supplement: