Homogeneous accretion hypothesis
1. Formation of Earth began after condensation of particles of the primitive nebula
2. Particles accreted to form a homogeneous primordial Earth
3. Early Earth had a uniform solid composition
4. Denser materials like iron and nickel sank towards the center
5. Less dense silicates moved upwards
6. Iron and nickel accumulated to form Earth's core
7. A thin layer of solid rock formed the crust