Final answer:
The terrestrial planets were initially collections of solid particles that melted, then differentiated into a high-density iron metal core and low-density silicate crust.
Step-by-step explanation:
The correct statement is option C: they were initially collections of solid particles that melted, then differentiated into a high-density iron metal core and low-density silicate crust.
According to the information provided, during the formation of terrestrial planets, every incoming planetesimal was accelerated by the gravity of the protoplanet, resulting in the melting of both the projectile and a part of the impact area. As a result of the heating, the inner protoplanets experienced planetary differentiation, with heavier metals sinking toward the core and lighter silicates rising toward the surface. This process led to the formation of a high-density iron metal core and a low-density silicate crust.