Continental rise

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Cross Section of Continental Margin Continental shelf.png
Cross Section of Continental Margin

The continental rise is a low-relief zone of accumulated sediments that lies between the continental slope and the abyssal plain. [1] It is a major part of the continental margin, covering around 10% of the ocean floor. [1] [2]

Contents

Formation

This geologic structure results from deposition of sediments, mainly due to mass wasting, the gravity-driven downhill motion of sand and other sediments. [1] Mass wasting can occur gradually, with sediments accumulating discontinuously, or in large, sudden events. [1] Large mass wasting occurrences are often triggered by sudden events such as earthquakes or oversteepening of the continental slope. [1] More gradual accumulation of sediments occurs when hemipelagic sediments suspended in the ocean slowly settle to the ocean basin. [1]

Slope

Because the continental rise lies below the continental slope and is formed from sediment deposition, it has a very gentle slope, usually ranging from 1:50 to 1:500. [1] As the continental rise extends seaward, the layers of sediment thin, and the rise merges with the abyssal plain, typically forming a slope of around 1:1000. [1]

Accompanying Structures

Alluvial Fans

Deposition of sediments at the mouth of submarine canyons may form enormous fan-shaped accumulations called submarine fans on both the continental slope and continental rise. [2] Alluvial or sedimentary fans are shallow cone-shaped reliefs at the base of the continental slope that merge together, forming the continental rise. [2] Erosional submarine canyons slope downward and lead to alluvial fan valleys with increasing depth. [2] It is in this zone that sediment is deposited, forming the continental rise. Alluvial fans such as the Bengal Fan, which stretches 3,000 kilometers (1,900 miles), make up one of the largest sedimentary structures in the world. [1] Many alluvial fans also contain critical oil and natural gas reservoirs, making them key points for the collection of seismic data. [1]

Abyssal Plain

Beyond the continental rise stretches the abyssal plain, which lies on top of basaltic oceanic crust and spans the majority of the seafloor. [2] The abyssal plain hosts life forms which are uniquely adapted to survival in its cold, high pressure, and dark conditions. [1] The flatness of the abyssal plain is interrupted by massive underwater mountain chains near the tectonic boundaries of Earth's plates. [2] The sediments are mostly silt and clay. [1]

Related Research Articles

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<span class="mw-page-title-main">Bengal Fan</span>

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Abyssal fans, also known as deep-sea fans, underwater deltas, and submarine fans, are underwater geological structures associated with large-scale sediment deposition and formed by turbidity currents. They can be thought of as an underwater version of alluvial fans and can vary dramatically in size, with widths from several kilometres to several thousands of kilometres. The largest is the Bengal Fan, followed by the Indus Fan, but major fans are also found at the outlet of the Amazon, Congo, Mississippi and elsewhere.

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<span class="mw-page-title-main">Submarine landslide</span> Landslides that transport sediment across the continental shelf and into the deep ocean

Submarine landslides are marine landslides that transport sediment across the continental shelf and into the deep ocean. A submarine landslide is initiated when the downwards driving stress exceeds the resisting stress of the seafloor slope material, causing movements along one or more concave to planar rupture surfaces. Submarine landslides take place in a variety of different settings, including planes as low as 1°, and can cause significant damage to both life and property. Recent advances have been made in understanding the nature and processes of submarine landslides through the use of sidescan sonar and other seafloor mapping technology.

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A contourite is a sedimentary deposit commonly formed on continental rise to lower slope settings, although they may occur anywhere that is below storm wave base. Countourites are produced by thermohaline-induced deepwater bottom currents and may be influenced by wind or tidal forces. The geomorphology of contourite deposits is mainly influenced by the deepwater bottom-current velocity, sediment supply, and seafloor topography.

The Amazon Canyon is a submarine canyon within the Amazon Fan in the Atlantic Ocean, located approximately 200 mi (322 km) from the mouth of the Amazon River, near South America. It covers an area of 2,250 km2 (870 sq mi). It was formed in the mid to late Miocene period. The canyon is believed to have formed through mass failures, and subsequently evolved through underwater erosion. Because of its relatively small size, the canyon has been extensively mapped.

<span class="mw-page-title-main">Congo Canyon</span> African submarine canyon at the end of the Congo River

Congo Canyon is a submarine canyon found at the end of the Congo River in Africa. It is one of the largest submarine canyons in the world.

Madeira Abyssal Plain, also called Madeira Plain, is an abyssal plain situated at the center and deepest part of the Canary Basin. It is a north-northeast to south-southeast elongated basin that almost parallels the Mid-Atlantic Ridge. Its western boundary is marked by a chain of seamounts known as the either Seewarte Seamounts or Atlantis-Great Meteor Seamount Chain. Its eastern boundary is a distinct break of slope that marks the foot of the African Continental Rise. This abyssal plain occupies an area of about 68,000 km2 (26,000 sq mi). Across this basin, slope angles are generally less than 0.01°.

References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 Mitchell, N. C. (2015), "Submarine Geomorphology☆", Reference Module in Earth Systems and Environmental Sciences, Elsevier, ISBN   978-0-12-409548-9
  2. 1 2 3 4 5 6 Patruno, Stefano; Helland-Hansen, William (2018). "Clinoforms and clinoform systems: Review and dynamic classification scheme for shorelines, subaqueous deltas, shelf edges and continental margins". Earth-Science Reviews. 185: 202–233. Bibcode:2018ESRv..185..202P. doi: 10.1016/j.earscirev.2018.05.016 . hdl: 1956/18533 . ISSN   0012-8252.