Temperature (a), density (b), pressure (c), and high-Z enrichment (d) interior curves of a planet formed by pebble accretion. They are plotted at the point in the planet’s evolution when core growth is equal to 10% of the pebble accretion rate. This corresponds to core masses of 0.58 M⊕ in the rainout scenario (blue curves) and 0.41 M⊕ in the mixing case (green curves). The dotted vertical lines indicate the position of the core.