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Earth originated approximately 4.54 billion years ago within the solar nebula—a rotating disk of gas and dust surrounding the young Sun. Through accretion, dust particles collided and adhered, forming planetesimals (1–10 km bodies). These grew via gravitational attraction, culminating in planetary embryos (Moon-to-Mars-sized). Earth’s final assembly involved a cataclysmic impact with a Mars-sized body named Theia, ejecting debris that formed the Moon. This collision also liquefied early Earth, enabling global chemical reorganization.
Intense heat from three sources drove planetary differentiation:
Molten iron and nickel sank toward the center, forming the core, while lighter silicate minerals migrated upward, creating the primitive mantle and crust. This process established Earth’s layered structure:
Core:
Mantle (2,900 km thick):
Crust:
Earth’s mechanical layers further refine this:
Seismic wave studies (P-waves and S-waves) reveal these layers. S-waves cannot traverse the liquid outer core, while P-waves refract at core-mantle boundaries, creating shadow zones. Gravity and magnetic field data corroborate core dynamics.
This structure regulates geologic activity: core convection powers the magnetic field shielding Earth from solar radiation, mantle convection drives plate tectonics, and crustal interactions recycle surface materials. Understanding Earth’s formation and stratification is foundational for interpreting volcanism, seismicity, and resource distribution.