Abstract
A very large number of geological and geophysical observations have been forthcoming in recent years from the Precambrian areas of the globe. Although these studies are unevenly distributed and come largely from the cratonic regions of Laurentia (the Canadian Shield, Greenland, and NW Scotland), southern Africa, and western Australia, they have shed considerable light on the early history of the Earth. They provide a sound basis for the tectonic subdivision of Precambrian times into the Archaean (> ca. 2700 m.y.) and Proterozoic (2700–600 m.y.) eras and show for example that a hydrosphere and shallow seas have existed on the Earth since 3800 m.y. while the history of the Earth-Moon system extends back to at least 3000 m.y. We can, however, only surmise as to the nature of the oceanic (simatic) components of the lithosphere in pre-Palaeozoic times because, with a few possible exceptions, this has been entirely destroyed. According to the concepts of the New Global Tectonics (Isacks et al. , 1968) we understand that this oceanic component is generated at the mid-ocean ridges and subducted below the continental lithosphere by the action of a mobile circulating asthenosphere (Hess, 1962; Dietz, 1961). The nature of the ocean crust, which must have covered at least 70 % of the globe in post-Archaean times (< 2500 m.y.), is therefore a matter of speculation only.
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Piper, J.D.A. (1978). Geological and Geophysical Evidence Relating to Continental Growth and Dynamics and the Hydrosphere in Precambrian Times: a Review and Analysis. In: Brosche, P., Sündermann, J. (eds) Tidal Friction and the Earth’s Rotation. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-67097-8_13
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