Early Evolution of Earth: Chronology of Events
• 4.6 – 4.5 Ga – Accretion of earth from solar nebula
• 4.5 - 4.2 Ga – Heating of protoearth from isotopic decay, gravitational
collapse, and meteorite bombardment (amplified by super greenhouse
effect) causing melting, differentiation of mantle and core, and
outgassing.
collapse, and meteorite bombardment (amplified by super greenhouse
effect) causing melting, differentiation of mantle and core, and
outgassing.
• 4.2 - 4.0 Ga – First crustal rocks formed. Differentiation of oceanic and
continental crust begins through recycling. Continued degassing.
Large meteorite impacts periodically removing protoatmosphere.
continental crust begins through recycling. Continued degassing.
Large meteorite impacts periodically removing protoatmosphere.
• 3.9 Ga – Decline in meteorite bombardment as loose nebular debris is
captured by Sun and planets. First stable continental crust forms.
captured by Sun and planets. First stable continental crust forms.
• 3.8 - 3.5 Ga – Buildup of crustal material into protocontinents.
Accretion of continents via microplate tectonics. Water condensing
and accumulating above basaltic crust, causing sedimentation and
potentially life.
Accretion of continents via microplate tectonics. Water condensing
and accumulating above basaltic crust, causing sedimentation and
potentially life.
• 3.0 Ga - Beginning of oxygenation of atmosphere due to photochemical
dissociation and photosynthesis (BIF).
dissociation and photosynthesis (BIF).
• 2.4 - 2.2 Ga – Free oxygen buildup in atmosphere and oxidation of earth
surface.
surface.
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