The oldest known intact rocks on Earth date from the Hadean, more than 4 Ga, a time period from which it was formerly believed that no rocks had survived. These earliest gneisses occur in the Acasta Gneiss Complex within Canada's Slave craton. (AGC in image at left; original). As the image shows, Canada possesses one of the largest area of Archean Eon rocks on Earth, while Australia has the earliest detrital mineral. The Itsaq Gneiss Complex in southwest Greenland comprises the most extensive and best-preserved fragment of early Archean continental crust.
The Superior Upland of Wisconsin and Minnesota, dipping south from Lake Superior, forms the largest U.S. surface exposure of the Precambrian Canadian Shield (2.6-1.6 Ga). Much of the Earth's continental crust formed in the Archean, and small, highly deformed remnants of Archean structures persist as tectonically incorporated terranes within Archean crustal provinces. The active tectonics of the Archean produced numerous, mobile, relatively small protocontinental landmasses that began to coalesce in the late Archean. By the close of the Archean, about 2.5 Ga, a more tectonically stable supercontinent had assembled from accreted landmasses. Vaalbara is Earth's theorized first supercontinent, which, according to radiometric data, existed by 3.3 billion years ago (3.3 Ga) and possibly even as far back as 3.6 Ga. By about 2.7 Ga, Neoarchean sanukitoid cratons plus new continental crust accreted to form another of Earth's earliest supercontinents, Kenorland, which comprised the Laurentia, Baltica, Australia, and Kalahari cratons and persisted from about 2.7 Ga until about 2.48 to 2.10 Ga. About 70% of modern continents are derived from the single large late Archean landmass. Modern shields, far distant from the site of their formation, contain cratonic cores consisting of old basement rocks that have been relatively undisturbed since the Precambrian era. Cratons have a thick continental crust and deep roots that extend into the underlying, anomalously cold mantle mantle for depths up to 200 km (twice the approximately 100 km thickness of mature oceanic or noncratonic continental lithosphere). The thickness and coolness of the coalesced Archean supercontinent led to a reduction in volcanic and tectonic activity within and along the margins of the supercontinent by the start of the Proterozoic. Most geologists believe that crust forming mechanisms in the Hadean and early Archean differed from modern tectonic mechanisms. Plate tectonics appears to have been operative – and highly active – by 4-3.5 Ga, when rock assemblages typical of magmatic arcs, oceanic plateaus, oceanic islands, and accretionary prisms appear in the geologic record. By 3 Ga, cratons, passive margins, and continental rifts were widespread, but the geochemical differences between Archean and younger rocks suggest that Archean tectonic regimes differed from modern tectonic environments. The majority of Archean rocks still in existence are metamorphic descendants and crystalline cratonic remnants. These granitic-gneiss products of sedimentary or igneous protoliths suggest a high degree of lithospheric recycling. Vast lava flows later in the Archean erupted from undersea rift zones as pillow basalts, and later metamorphism altered these basalts to greenstones. Archean igneous rocks include unusual lavas, such as komatiite, intrusive igneous rocks such as great melt sheets, and voluminous plutonic masses of granite, granodiorite, diorite, ultramafic to mafic layered intrusions, anorthosites and monzonites known as sanukitoids. Other Archean igneous rocks with unusual mineralogy include lamprophyres and kimberlites. Gneisses, granulites and greenstone belts are common Archean rocks. Greenstone–granite belts represent the upper crust, granulite–gneiss belts formed in the mid-lower crust, and other Archean rocks formed in sedimentary basins, basic dikes, and layered complexes that were either deposited on or intruded into the greenstone–granite and granulite–gneiss belts. Pillow lavas occur within these belts, and patchy interbeds of conglomerates and chemical sediments formed later. The mechanisms of belt genesis remains uncertain, but their chemistry is consistent with partial melting of water-infused basalts under high temperature and pressure. Reef-forming stromatolite microfossils, which persist to this day in scattered stressed environments, provide evidence of life in the warm Archean oceans. Stromatolites were built by the photosynthetic Cyanobacteria that transformed the primordial atmosphere. The oldest known stromatolites are found in south Africa's 3.5 Ga Barberton greenstone and in western Australia's 3.5 Ga Pilbara greenstone. Other evidence of Archean life is found in fossils of cells or cellular tissue, and carbonaceous matter that is identifiable as a product of biologic activity based on its carbon isotopic composition. |