The first 800 million years:  environmental models for early Earth.
Space exploration has changed our views not only on the properties of celestial bodies and the interplanetary medium but also our perspective on the formation of such bodies, including the Earth.  However, on few points do the new hetegonic insights approach certainty.  More appropriately, they can be said to raise physically meaningful questions and to decrease the degrees of freedom allowable in any given scenario, which necessarily extends into the early history of the planetary crust, ocean and atmosphere.  An attempt is made here to outline the basic schemes envisaged in modern studies of the origin of the Earth and the ramification of consequences for its early evolution that currently appear allowable and supported by observation.
Arrhenius
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Scripps Institution of Oceanography, University of California, San Diego, La Jolla, USA.
D001272:Atmosphere / Q000737:chemistry*; D018534:Earth, Planet; D004777:Environment; D019419:Evolution, Planetary; D008962:Models, Theoretical; D009792:Oceans and Seas; D016082:Solar System; D013696:Temperature