Extended Data Fig. 1: Fractional crystallization modeling of P, Ni, Co, and Ir for group IIIE.
From: Accretion of the earliest inner Solar System planetesimals beyond the water snowline
The Ir-Co (a), Ir-Ni (b), and P-Ni (c) models use bulk 8 wt.% S and 0.6 wt.% P. The red lines, blue lines, and green dashed lines denote solid from simple fractional crystallization (SFC solid), solid from trapped melt (TM solid), and liquid (Liquid), respectively. Ir, Co, and Ni data are from ref. 73. Phosphorus data are from ref. 74.
