The
iron catastrophe was a postulated major event early in the
history of Earth. The original
accretion of the
Earth's material into a spherical mass is thought to have resulted in a relatively uniform composition. While residual heat from the collision of the material that formed the Earth was significant, heating from
radioactive materials in this mass gradually increased the temperature until a critical condition was reached. As material became molten enough to allow movement, the denser
iron and
nickel, evenly distributed throughout the mass, began to migrate to the center of the planet to form the core. The gravitational potential energy released by the sinking of the dense
NiFe globules, along with any cooler denser solid material is thought to have been a runaway process, increasing the temperature of the protoplanet above the melting point of most components, resulting in the rapid formation of a molten iron core covered by a deep global silicate
magma. This event, an important process of
planetary differentiation, occurred at about 500 million years into the formation of the planet.