2. Accretion:
4.6 Billion years ago gas and dust began to clump together forming
asteroids, then a planetismal, and then a planet
3. Core Accretion:
The heavier elements sunk to the
center due to their density; heat
generated by collisions/friction
4. Where did most of the water come from?
At various points Earth is bombarded by asteroids and comets bringing
more water to the planet
5. Formation of the Moon
A smaller proto-planet, Theia, strikes Earth adding mass to it while ejecting
materials that become the moon; cause of tilt
6. Cooling of Earth
The Earth begins to cool allowing the atmosphere and oceans to form;
molten crust solidifies to form tectonic plates moved by the mantle
7. Plate Tectonics:
The movement of the
tectonic plates by
mantle convection
heated by the core of
the Earth; allows for
continental
recombinations