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. 2019 Apr 29;116(20):9723–9728. doi: 10.1073/pnas.1812905116

Fig. 3.

Fig. 3.

The stability fields of planet-building materials in a protoplanetary disk of solar composition at 10−4 bar. The fraction of condensed rocky matter (>200 K) is calculated with the GRAINS code (58), while condensation temperatures and abundances of ices are taken from ref. 59. The composition of gas is temperature dependent and always complementary to the composition of the condensed phase assemblage.