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The unconsolidated sediments, derived from various sources, deposited at the sea floors are included in ocean deposits. The study of ocean (marine) deposits includes the consideration of types of sediments, their sources, methods of their transportation, horizontal distribution, lithological successions or vertical variations in their distribution and composition, etc.
The sediments derived from weathering and erosion of continental rocks are transported to the oceans by rivers, winds, etc. Volcanic eruptions also provide sediments. Besides, the decay and decomposition of marine organisms (both plants and animals) also contribute sediments to ocean deposits.
Ocean deposits are classified on different bases e.g.:
(1) On the basis of location,
(2) On the basis of depth,
(3) On the basis of the origin of sediments etc.
1. On the Basis of Location:
This classification is based on typical locations of particular marine sediment. Though several scientists have attempted to classify ocean deposits on the basis of their locations, the classifications of Sir John Murray and J.T. Jenkins are widely acclaimed.
(i) Classification of Murray:
Sir John Murray has classified the ocean deposits into two broad categories viz.:
(a) terrigenous deposits and
(b) pelagic deposits.
Terrigenous deposits are found mainly on the continental shelves and slopes whereas pelagic deposits predominate on the deep sea floor. Terrigenous deposits are composed of coarser materials and are derived from the continents through weathering and erosional processes and are transported to the oceans by various agencies.
Their color may be blue, yellow, grey, or red. Pelagic deposits consist of fine materials formed of the skeletons and shells of marine organisms and a few inorganic substances. They are generally blue, grey, or red in color.
(ii) Classification of Jenkins:
Jenkins has divided marine deposits into three groups viz.:
(a) Deep sea deposits,
(b) Shallow water deposits, and
(c) Littoral deposits.
The following is the detailed classification of Jenkins:
(A) Pelagic deposits:
(1) Red clay,
(2) Radiolarian ooze,
(3) Diatom ooze,
(4) Globigerina ooze, and
(5) Pteropod ooze.
(B) Terrigenous deposits:
(1) Blue mud,
(2) Red mud,
(3) Green mud,
(4) Coral mud,
(5) Volcanic mud,
(6) Gravel, and
(7) Sand.
2. On the Basis of Depth:
(A) Deep sea deposits (Below 100 fathoms):
(a) Pelagic Deposits:
(1) Red clay,
(2) Radiolarian ooze,
(3) Diatom ooze,
(4) Globigerina ooze, and
(5) Pteropod ooze.
(b) Terrigenous Deposits:
(1) Blue mud,
(2) Red mud,
(3) Green mud,
(4) Coral mud, and
(5) Volcanic mud.
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(B) Shallow sea deposits (between low tide water and 100 fathoms):
(1) Gravels,
(2) Sands, and
(3) Mud.
(c) Littoral deposits (Between high and low tide water):
(1) Gravels,
(2) Sands,
(3) Mud.
2. General Classification:
(1) Terrigenous Deposits:
i. Littoral deposits,
ii. Shallow water deposits, and
iii. Terrigenous mud.
(2) Neritic Deposits:
i. Shallow water neritic deposits,
ii. Deep sea water neritic deposits, and
iii. Pelagic deposits.
3. Classification on the Basis of Origin of Sediments:
(1) Littoral deposits (derived from land)):
(i) Shore deposits.
(ii) Shelf deposits.
(2) Hemipclagic deposits (Partly from land and partly from marine origin):
(i) Green mud.
(ii) Volcanic mud.
(iii) Coral mud.
(3) Eupelagic deposits (Of marine and cosmic origin):
(i) Red clay.
(ii) Radiolarian ooze.
(iii) Globigerina ooze.
(iv) Pteropod ooze.
The term 'Terrigenous' comes from the Latin words 'terra,' meaning land, and 'genus,' meaning origin. These deposits are predominantly land-derived sediments that have journeyed to the ocean depths via numerous transportation modes.
The most common sources of Terrigenous Deposits are rivers which carry vast amounts of sediment eroded from the land's surface. Other sources include winds, which transport fine particles like dust and sand over great distances, and glaciers, which grind rocks into fine particles and carry them into the sea.
The composition of Terrigenous Deposits varies widely depending on the source. River sediments, for example, can contain everything from nutrient-rich soil to tiny fragments of rock, while glacial deposits may include unique minerals picked up during the glacier's slow movement over land.
This type of sediment comes from the remains of living organisms in the ocean. When tiny marine plants and animals die, their remains can sink to the bottom and build up over time, forming a kind of sediment called "ooze". If the ooze is made mostly of silica-based organisms like diatoms or radiolarians, it's called "siliceous ooze". If it's made mostly of calcium carbonate-based organisms like foraminifera or coccolithophores, it's called "calcareous ooze". These types of ooze are usually found in the open ocean, away from land.
These are the oceanic deposits derived from dead remains of living organisms. It can be classified into
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Cosmogenous sediments come from outer space! Tiny dust particles, or "micrometeorites," constantly fall onto the Earth from space, and some of them end up in the ocean. Also included in this category are larger meteorite fragments and tektites, which are glassy rocks formed by the heat and pressure of meteorite impacts. Cosmogenous sediments are rare and are spread thinly across the entire ocean floor.
Pelagic Deposits offer an intriguing snapshot of life in the ocean's depths. Derived from the Greek word 'pelagos' for sea, these deposits are made up of the remains of marine organisms and fine particles suspended in the ocean water.
A common form of Pelagic Deposits is 'ooze,' a soft, mud-like substance made up of microscopic shells of marine organisms. There are two main types of ooze: calcareous ooze, formed from organisms with calcium carbonate shells, and siliceous ooze, from organisms with silica-based skeletons.
Deep-sea clay, also a type of Pelagic Deposit, consists of extremely fine particles that have slowly settled out of the water column. This deposit often accumulates in areas of the ocean where the supply of organic material is low, and thus oozes cannot form.
These are the chemical wizards of Ocean Deposits. 'Hydrogenous' comes from the Greek word 'hudōr' for water and 'gennan' to produce. They form through chemical reactions within the seawater, leading to precipitation of minerals that then settle onto the ocean floor.
A well-known example is manganese nodules, potato-sized lumps rich in manganese, iron, nickel, copper, and cobalt. These nodules grow very slowly over millions of years, layer by layer, from the direct precipitation of minerals from seawater.
Phosphorite deposits are another type of Hydrogenous Deposit. They form in areas of high biological productivity where the decay of organic matter releases phosphorus, which then combines with calcium in seawater to form calcium phosphate.deposits
Type of Deposit |
Source of Origin |
Examples |
Unique Characteristics |
Terrigenous Deposits |
Land |
Clay, silt, sand |
Wide compositional variety based on the source |
Biogenous Deposits |
Organic accumulation of hard parts of some marine organisms |
Calcareous and Siliceous oozes |
They provide a record of the types of life that existed in the ocean in the past |
Pelagic Deposits |
Marine Life |
Ooze, deep-sea clay |
Provides information about past marine life |
Hydrogenous Deposits |
Seawater |
Manganese nodules, phosphorite deposits |
Forms through chemical reactions in seawater |
Cosmogenous deposits |
Dust from spce, meteorites debris |
Meteorites debris glassy nodules |
The composition of cosmogenous deposits can be quite diverse, reflecting the variety of materials found in the universe. |
From the terrestrial echoes found in Terrigenous Deposits to the stories of marine life captured in Pelagic Deposits, and the chemical tales of Hydrogenous Deposits, each category of Ocean Deposits plays an essential part in the geological symphony that is our planet's history.
Classification of Ocean Deposits Based on Depth
Questions: