Core–mantle differentiation

Core–mantle differentiation refers to the geological process by which a planet, such as Earth, separates into distinct layers based on differences in composition, density, and physical properties. This process is primarily observed during the early stages of a planet's formation, shortly after it has formed from the accretion of dust and gas in the protoplanetary disk. In the case of Earth, differentiation involves the separation of the planet into a dense metallic core and a lighter silicate mantle.