Paleogeology

Paleogeology, Paleoclimate, in relation to Evolution of Life on Earth

Archaean supercontinents

The Archaean, or Archean Eon extends from 3.8 billion years ago until 2.5 billion years ago.

(image at left – current approximate distribution of most Archean crustal rocks (the projection greatly exaggerates the area of polar landmasses – compare with image of location of cratons and platforms)

The Archean mantle was hotter than the Earth's current interior, resulting in heavy mantle convection and crustal turbulence. Archean Earth was very active tectonically, with higher rates of volcanic activity and plate boundary movement than is occurring today. Active tectonics during the Archean created numerous, mobile protocontinental landmasses that floated on the turbulent mantle. Toward the end of the Archean, the proto-continents began to coalesce, and by about 3.3 Ga the more tectonically stable supercontinent Vaalbara is hypothesized to have formed by accretion of smaller landmasses.

The oldest Archaean rocks so far discovered on Earth are:
1) The Isua Supracrustal rocks of West Greenland (3.7 to 3.8 Ga)
2) Northern Michigan (3.5-3.7 Ga)
3) Swaziland (3.4-3.5 Ga)

approximate ages of earliest continent (Ur) and supercontinents (Vaalbara, Kenorland)Archaean Eon:
70% of modern continental shields date from 3.0 to 2.5 billion years ago, which was the period of maximum continent formation. Most of the earliest rocks have been greatly altered through regional metamorphic processes, but later rocks (3.2-2.5 Ga) are mostly pillow-basalts that formed beneath the vast oceans. Archean sedimentary rocks are mostly coarse and poorly sorted sandstones and conglomerates.

The oldest fossilized signs of life date from the Archean – Cyanobacteria that created 3.45 Ga old stromatolite fossils found in the Apex Chert at Marble Bar, Western Australia. Microfossils from Swaziland (South Africa) have a similar age.[image]

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. Evidence includes geochronological and palaeomagnetic studies between the two Archaean cratons (protocontinents) called the Kaapvaal craton (the Kaapvaal province of South Africa) and the Pilbara craton (the Pilbara province of Western Australia).

Further evidence is the structural sequence similarities of the greenstone belts and gneiss belts of the Kaapvaal and Pilbara cratons. These same Archaean greenstone belts are now spread out across the margins of the Superior craton of Canada and across the cratons of the former Gondwana and Laurasia continents. The subsequent drift paths of the Kaapvaal and Pilbara cratons after 2.8 Ga gives further evidence that they were once connected.

It is not certain when Vaalbara began to break up, but geochronological and palaeomagnetic evidence show that the two cratons had a rotational 30 degree latitudinal separation at 2.78 to 2.77 Ga, implying that they were no longer contiguous after ~2.8 Ga.

Ur was the first known continent, which probably formed 3 billion years ago in the early Archean Eon. Ur joined with the continents Nena and Atlantica about one billion years ago to form the supercontinent Rodinia. Ur survived for a long time, until it was torn apart when the supercontinent Pangaea broke apart about 208 million years ago into Laurasia and Gondwanaland. Ur now forms parts of Africa, Australia, India, and Madagascar. In the early period of its existence, it was probably the only continent on Earth, and is so considered by some to be a supercontinent, even though it was probably smaller than Australia is now.

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. The Baltic/Fennoscandian Shield formed the core of Kenorland, with origins that trace back more than 3.1 Ga. The Yilgarn Craton (present-day Western Australia) contains 4.4 Ga detrital zircon elements.

Protracted tectonic magna plume rifting occurred between 2.48 to 2.10 Ga, contributing to the break-up of Kenorland during the Late Neoarchaean and early Paleoproterozoic Era (2.48 to 2.10 Ga) during the Siderian and Rhyacian periods. The rifting is manifested by mafic dykes and sedimentary rift-basins and rift-margins on many continents. On early Earth, this type of bimodal deep mantle plume rifting was common in Archaean and Neoarchaean crust and continent formation.

The geological time period remains conjectural at which Earth made the transition from deep-mantle-plume mechanism of continent formation to the current two-layer core-mantle plate tectonics convection mechanism that forms continents by subduction, convergence and accretion. However, with the findings of the earlier continent Ur and the ca. 3.1 Ga supercontinent Vaalbara, this transition period may have occurred much than the time of Kenorland.

Paleomagnetic studies indicate that Kenorland lay in low latitudes until the rifting breakup commenced around 2.48 Ga. Paleomagnetic evidence further indicates that at 2.45 Ga the Baltic/Fennoscandian Shield, astride the equator, was attached to Laurentia (the Canadian Shield), forming a unity with both the Kola and Karelia cratons, which began to drift apart ~2.45 Ga. By 2.4 Ga, the Kola craton was located at ~15 degrees latitude and the Karelia craton had drifted to ~30 degrees latitude. Paleomagnetic evidence indicates that at 2.45 Ga the Yilgarn craton (now the bulk of Western Australia) was not connected to Fennoscandia-Laurentia and was located at ~70 degrees latitude. This suggests that Kenorland was no longer a supercontinent by 2.45 Ga. By 2.4 Ga, an ocean separated the formerly joined Kola and Karelia cratons.

Based on the rift margin spatial arrangements of Laurentia, it is hypothesized that the Slave and Superior cratons were not part of the rifting supercontinent Kenorland, but may instead have been two different Neoarchaean landmasses (supercratons) located at opposite poles of a very large Kenorland. This speculation is based on the mechanics of how drifting assemblies of various constituent pieces should flow reasonably together toward the amalgamation of the new subsequent continent. The Slave and Superior cratons now constitute the NW and SE portions of the Canadian Shield, respectively.

The breakup of Kenorland was contemporary with the 60 million year long Huronian glaciation. The banded iron formations (BIF) show their greatest extent at this period, indicating massive increase in oxygen build-up (estimated 0.1% to 1% of atmosphere). Rising oxygen levels caused virtual disappearance of the greenhouse gas methane, which was oxidized into carbon dioxide and water. The simultaneous breakup of Kenorland increased continental rainfall, increasing erosion and further reducing the other greenhouse gas carbon dioxide. This reduction in greenhouse gases coupled with solar output still less than 85% its current levels precipitated a runaway Snowball Earth scenario, when average temperatures planet-wide plummeted to below freezing. Despite the anoxia indicated by the BIF, photosynthesis continued, stabilizing climates at new levels during the second part of the Proterozoic Era.

◙ subduction zone magmas ◙

More: GeoWhen Database : Tectospheric keels : 2004 time scale endorsed by the International Commission on Stratigraphy

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Proterozoic

The Proterozoic Eon extends from 2.5 billion years ago to 540 million years ago.

Three supercontinent assemblies have existed during or since the Neoproterozoic:
● Pangaea 350-165 Ma, assembling in the Carboniferous and breaking up in the Jurassic
● Gondwanaland 550-400 Ma during the Cambrian and Ordovician
● Rodinia ~ 1050-750 Ma).[r '03, images]

Pangea has been reconstructed on the basis of sea floor magnetic data. Gondwana has been reconstructed on the basis of paleomagnetic and biostratigraphic data, supported by geology. Debate continues regarding relative positions of continents within Rodinia, and the timing of assembly and breakup of Rodinia (some paleogeologists hypothesize the beginning of assembly as far back as 1.3 billion years). The configuration of Rodinia has been hypothetically reconstructed based upon paleomagnetic data and the mountain chains (orange) formed during the Grenville orogeny, which span several modern continents.

Tables  Geological Time  Flood Basalts and Stratigraphic Boundaries  Lagerstätten & Biota

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oceanic structures

elevations of oceanic and continental crustThe Earth's crust is divided into continental crust and oceanic crust.

▼ abyssal plain : composition of oceanic crust : continental crust : continental rise : continental shelf : continental slope : creation/consumption of oceanic crust : mid-oceanic ridges : oceanic crust : oldest oceanic crust : paleomagnetic record : seamounts : submarine trenches : volcanic islands ▼

Structurally, moving outward from continental structures at sea level to those most distant from shore or at the greatest depths (image at left - elevations - click to enlarge image - mid-res, hi-res versions):

● continental shelf (continental crust) – the terrigenous-relict sediment-covered, flooded continental margin extends varying distances from shore (average 80 km), and slopes gradually from shore to the shelf break at a fairly uniform depth of 140 m. Sediments are coarser closer to shore and finer at greater distances from shore.

● continental slope (oceanic crust begins) – steeper than the sediment covered continental shelf, the continental slope extends from the shelf break to depths of 2-3 km, often cut by submarine canyons.

● continental rise – of shallower gradient than the continental slope, the rise extends up to 500 km from the slope and comprises thick sediments deposited by turbidity currents from the shelf and slope.[9]

● abyssal plain – gently sloping or flat regions that cover approximately 40% of the ocean floor, reaching depths between 2,200 and 5,500 m.

● submarine trenches – deep trenches formed by the subduction of oceanic crust beneath continental crust at convergent boundaries of tectonic plates.

● volcanic islands – basaltic shield volcanoes like the chain of Hawaiian islands above mantle plumes, oceanic rift islands (Atlantic Iceland, Jan Mayen), or volcanic arc islands at subducting margins (Mariana Islands, Aleutians, Mauritius, Tonga in the Pacific Ocean; Lesser Antilles, South Sandwich Islands in Atlantic Ocean). ◙ subduction zone magmas ◙

● seamounts – submarine mountains that typically are extinct volcanos.

● mid-oceanic ridges – spreading center mountain ranges with a total total length of about 60,000 km that ring the globe at the divergent boundaries of tectonic plates. Oceanic crust is replenished at the mid-ocean ridges and destroyed at continental margins.

age of oceanic crust that has spread laterally from its line of formation in the mid-oceanic ridge spreading centers; color scale indicates agesOceanic crust (right - age of oceanic crust -click to enlarge image - mid-res, hi-res) is younger than continental crust and is replenished at spreading centers. Oceanic crust is consumed when it subducts at convergent tectonic plate boundaries at continental margins. The deepest ocean lies in the Challenger Deep of the Pacific's Mariana Trench at a depth of 10,911 m below sea level [image: CD: mid-res, hi-res; MT: mid-res].

The oldest oceanic crust dates from about 180 Ma and lies adjacent to continents, while the youngest crust lies adjacent to the mid-oceanic ridge centers. As oceanic crust is followed outward from the mid-oceanic ridges, its age gradually increases (and its paleomagnetic signature records geomagnetic reversals).

Rocks of the oceanic crust are mafic basaltic rocks (sima) with a mean density of about 3.3 grams per cubic centimeter (more dense than felsic continental rocks). With an average thickness of 10 km, the oceanic crust is thinner than the continental crust [image crustal thickness].

◙ subduction zone magmas ◙

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basalt

Basalt is a hard gray or black, mafic igneous volcanic rock that is usually fine-grained due to rapid cooling of lava, though it contain larger crystals in a fine matrix (porphyritic), be vesicular, or be a frothy scoria.

basaltic lava flow of aa over pahoehoe, Hawaii, courtesy of USGSBasalt magmas form by decompression melting of peridotite in the mantle. The crustal portions of oceanic tectonic plates comprised predominantly basalt, derived from upwelling peridotite in the mantle below ocean ridges. The basalt shield volcanoes of the Hawaiian island chain sit above a mantle plume, or 'hot spot'. (left - click to enlarge - aa flows over ropey pahoehoe in Hawaii - image courtesy of USGS.)

Basalt is TAS classified according to the relationships between the combined alkali content and the silica content. Basalt typically containts a preponderance of calcic plagioclase feldspar and pyroxene; olivine can also be a significant constituent. Accessory minerals include iron oxides and iron-titanium oxides, providing basalt with a paleomagnetic signature.

Phaneritic, shallow intrusive igneous rocks with a basaltic composition are generally referred to as dolerite (also called diabase) or gabbro.

textures of various basalts - top-down: basaltic lava; lava field; flow-lines in basalt formation; close-up of vesicular basalt with olivine crystals; surface of basalt hand specimen; basalt columns.(image left - click to enlarge - courtesy USGS - top-down: basaltic lava; lava field; flow-lines in basalt formation; close-up of vesicular basalt with olivine crystals; surface of basalt hand specimen; basalt columns.)

[images - roll-over link for preview (where available); large images of hand-speciments (well worth a visit) show only as a corner on preview : water-sculpted basalt at Fossil Falls in Yosemite : Basalt Fall unterhalb des Hengifoss, basalt columns, Dverghamrar basaltic columns in Iceland, 2 : cliff of basalt columns : Columbia River basalts, Catherine Creek arch in Miocene columnar basalts : flowing curves of basalt entablature in Yellowstone : basalt columns Armenia : basalt field : basalt and sandstone : 3.7 Ga moon-rock basalt : hand-specimen : hand-specimen vesicular basalt, vesicular basalt with olivine phenocrysts, 2 : hand-specimen diabase : hand-specimen diabase porphyry : hand-specimen diorite : hand-specimen gabbro : hand-specimen scoria : thin-section basalt, 2, 3; thin-sections moon basalts ]

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. . . stratifying since 10/06/06