A major division of geologic time spanning from 2500 to 543 million years before present (Ma). The beginning of Proterozoic time is an arbitrary boundary that roughly coincides with the transition from a tectonic style dominated by extensive recycling of the Earth's continental crust to a style characterized by preservation of the crust as stable continental platforms. The end of the Proterozoic coincides with the Precambrian-Cambrian boundary, which is formally defined on the basis of the first appearance of diverse coelomate invertebrate animals. Proterozoic Earth history testifies to several remarkable biogeochemical events, including the formation and dispersal of the first supercontinent, the maturation of life and evolution of animals, the rise of atmospheric oxygen, and the decline of oceanic carbonate saturation. Tremendous iron and lead-zinc mineral deposits occur in Proterozoic rocks, as do the first preserved accumulations of oil and gas. See also Cambrian; Precambrian.
Many of the Earth's Archean cratons are blanketed by little-deformed sequences of Proterozoic sedimentary rocks, which indicate that vigorous recycling of the Earth's crust, characteristic of Archean time, had slowed markedly by the beginning of Proterozoic time. This decrease in crustal recycling is attributed to the development of thick continental roots, which stabilized the cratons, and the decrease in heat that was escaping from the Earth's interior, believed to drive thermal convection in the Earth's mantle and recycling of the crust. Most of the Earth's Archean cratons appear to have participated in the formation of a supercontinent in Mesoproterozoic time, about 1200 Ma. This supercontinent, called Rodinia, seems to have assembled with the North American craton (Laurentia) at its center. Rodinia persisted until the latest part of the Neoproterozoic, about 600 Ma. See also Archean; Continents, evolution of; Earth, heat flow in; Earth crust; Earth interior; Plate tectonics.
Giant iron oxide deposits were formed by precipitation from seawater about 2000 Ma, whereupon oxygen was free to accumulate in the atmosphere and shallow ocean. During most of Paleoproterozoic time the oceans and atmosphere were reducing and ferrous iron was abundant in seawater.
The partial pressure of carbon dioxide on the early Earth was very high. During Proterozoic time, much of the mass of carbon shifted from the ocean and atmosphere to the solid Earth. Enormous volumes of limestone [CaCO3] and dolostone [CaMg(CO3)2] were deposited and testify to this shift. See also Dolomite rock; Limestone; Sedimentary rocks.
Glaciers covered significant parts of the Earth during two widely separated times in Proterozoic history. The first episode occurred about 2200 Ma, and glacial deposits of that age cover various parts of North America and Scandinavia. The second episode consisted of at least two different pulses spanning from 750 to 600 Ma during Neoproterozoic time. Glaciers formed at that time were of almost global extent, and were thought to have extended from the poles to the Equator, according to the snowball Earth hypothesis. See also Glacial epoch.
A number of significant events in the evolution of life occurred during Proterozoic time. The record of biological activity is rich, consisting of actual body fossils, in addition to organism traces and impressions, and complex chemical biomarkers. Eukaryotic microbes appear to have evolved by about 1900 Ma, when they became major players in ecosystems present at that time. By the beginning of Neoproterozoic time, about 1000 Ma, multicellular eukaryotic algae are present in numerous sedimentary basins around the world. See also Eukaryotae; Ribonucleic acid (RNA).
The evolution of animals did not take place until the close of Neoproterozoic time. Why these organisms evolved at this particular time in Earth history remains unanswered. General opinion proposes that it was likely the result of the confluence of a number of environmental factors, such as the rise in oxygen. Whatever the cause of their origin, these existed until at least 543 Ma, when another major evolutionary adaptive radiation began which marks the onset of Cambrian time and the end of the Proterozoic Eon. See also Animal evolution; Extinction (biology); Geologic time scale.