Introduction to Early Earth

  • 4600 BCE

    Core Formation

    During accretion, the heat melted rocks and metals. Then, gravitational attraction pulled the denser materials into the center and created the core of the earth.
  • 4600 BCE

    Planetary Accretion

    This was when elements released from the bigbang started to rotate faster and faster due to gravitational attraction. The rotation created a concentrated center, thus creating the sun. Other concentrations rotating around formed planets like the earth.
  • Period: 4500 BCE to 2700 BCE

    Planetary Cooling

    Planetary cooling was when the hot surface of the earth, caused by continuous bombardment of asteroids and comets, began to cool off. As the planet cooled, volcanoes released gases and created the atmosphere, lava cooled down to created the solid crust, and oceans formed from asteroids that struck the earth.
  • 4400 BCE

    Formation of the Moon

    An asteroid the size of Mars crashed into earth and the impact created debris orbiting around the earth. These debris accumulated and formed the moon. In this stage, the moon was closer than the moon is today.
  • 4400 BCE

    Formation of the Earth

    Debris from the accretion started to collide and over time, they created the Earth.
  • 3800 BCE

    End of Heavy Bombardment

    This was when the constant bombardment of asteroids and comets came to an end. In this stage, the Late Heavy Bombardment period had finished, so most of the planets int he solar system settled in the place the way it is today.
  • 1350 BCE

    Formation of Mars

    Mars was formed around this date.