Chapter 4 Marine Sediments

Essential of Oceanography

Table of Contents

Chapter Overview

  • Marine sediments contain a record of Earth history.
  • Marine sediments provide many important resources.
  • Marine sediments have origins from a variety of sources.

Marine Sediments

  • Provide clues to Earth history
    – Marine organism distribution
    – Ocean floor movements
    – Ocean circulation patterns
    – Climate change
    – Global extinction events
  • Texture – size and shape of particles
  • Sediment origins
    – Worn rocks
    – Living organisms
    – Minerals dissolved in water
    – Outer space
  • Sediments lithify into sedimentary rock

Classification of Marine Sediments

CLASSIFICATION OF MARINE SEDIMENTS
TypeCompositionSources/OriginDistribution/Main locations where sediment currently forms
  LithogenousContinental margin  Rock fragments Quartz sand Quartz silt ClayRivers; coastal erosion; landslidesContinental shelf
GlaciersContinental shelf in high latitudes
Turbidity currentsContinental slope and rise; ocean basin margins
  OceanicQuartz silt ClayWind-blown dust; rivers  Abyssal plains and other regions of the deep-ocean basins
Volcanic ashVolcanic eruptions
  BiogenousCalcium carbonate/ calcite (CaC03)Calcareous ooze (microscopic)Warm surface watersCoccolithophores (algae) Foraminifers (protozoans)Low-latitude regions; sea floor above CCD; along mid- ocean ridges and the tops of submarine volcanic peaks
  Shells and coral fragments (macroscopic)Macroscopic shell-producing organismsContinental shelf; beaches
Coral reefsShallow low-latitude regions
Silica (Si02·nH20)    Siliceous oozeCold surface waters  Diatoms (algae) Radiolarians (protozoans)High-latitude regions; sea floor below CCD; upwelling areas where cold, deep water rises to the surface, especially that caused by surface current divergence near the equator
  HydrogenousManganese nodules (manganese, iron, copper, nickel, cobalt)      Precipitation of dissolved materials directly from seawater due to chemical reactionsAbyssal plain
Phosphorite (phosphorous)Continental shelf
Oolites (CaCO3)Shallow shelf in low-latitude regions
Metal sulfides (iron, nickel, copper, zinc, silver)Hydrothermal vents at mid-ocean ridges
Evaporites (gypsum, halite, other salts)Shallow restricted basins where evaporation is high in low-latitude regions
  CosmogenousIron–nickel spherules Tektites (silica glass)Space dustIn very small proportions mixed with all types of sediment and in all marine environments
  Iron–nickel meteorites  Meteors  Localized near meteor impact structures

Marine Sediment Collection

  • Early exploration used dredges.
  • Modern exploration
    – Cores – hollow steel tube collects
    sediment columns
    – Rotary drilling – collects deep
    ocean sediment cores
READ ALSO  What Features Exist in the Deep-Ocean Basins?
  • National Science Foundation (NSF) – formed
    Joint Oceanographic Institutions for Deep
    Earth Sampling (JOIDES) in 1963
    – Scripps Institution of Oceanography
    – Rosenstiel School of Atmospheric and
    Oceanic Studies
    – Lamont-Doherty Earth Observatory of
    Columbia University
    – Woods Hole Oceanographic Institution
  • Deep Sea Drilling Project (DSDP) – 1968
    – Glomar Challenger drilling ship
    – Core collection in deep water
    – Confirmed existence of sea floor spreading
  • Ocean floor age
  • Sediment thickness
  • Magnetic polarity
  • DSDP became Ocean Drilling Project (ODP)
    in 1983
    – JOIDES Resolution replaced Glomar
    Challenger
  • Integrated Ocean Drilling Program (IODP)
    – Replaced ODP in 2003
    – Chikyu – new exploration vessel in 2007
  • Expedition to Japan Trench after 2011 earthquake

Paleoceanography and Marine Sediments

  • Paleoceanography – study of how ocean, atmosphere, and land interactions have produced changes in ocean chemistry, circulation, biology, and climate
    – Marine sediments provide clues to past changes.
  • Lithogenous sediment (lithos = stone, generare = to produce) is derived from preexisting rock material that originates on the continents or islands from erosion, volcanic eruptions, or blown dust. Note that lithogenous sediment is sometimes referred to as terrigenous sediment (terra = land, generare = to produce).

Marine Sediment Classification

  • Classified by origin
  • Lithogenous – derived from land
  • Biogenous – derived from organisms
  • Hydrogenous or Authigenic – derived from water
  • Cosmogenous – derived from outer space

Lithogenous Sediments

  • Eroded rock fragments
    from land
  • Also called terrigenous
  • Reflect composition of
    rock from which derived
  • Produced by weathering
    – Breaking of rocks into smaller pieces
  • Small particles eroded and transported
  • Carried to ocean
    – Streams
    – Wind
    – Glaciers
    – Gravity
  • Greatest quantity around continental margins
  • Reflect composition of rock from which derived
  • Coarser sediments closer to shore
  • Finer sediments farther from shore
  • Mainly mineral quartz (SiO2)
Weathering of a rock outcrop
Weathering of a rock outcrop

Lithogenous Quartz and Wind Transport

Grain Size

  • One of the most important sediment properties
  • Proportional to energy of transportation and
    deposition
  • Classified by Wentworth scale of grain size

Wentworth Scale of Grain Size

Texture and Environment

  • Texture indicates environmental energy
    – High energy (strong wave action) – larger
    particles
    – Low energy – smaller particles
  • Larger particles closer to shore

Sorting

  • Measure of grain size uniformity
  • Indicates selectivity of transportation process
  • Well-sorted – all same size particle
  • Poorly sorted – different size particles mixed together

Sediment Distribution

  • Neritic
    – Shallow-water deposits
    – Close to land
    – Dominantly lithogenous
    – Typically deposited quickly
  • Pelagic
    – Deeper-water deposits
    – Finer-grained sediments
    – Deposited slowly

Neritic Lithogenous Sediments

  • Beach deposits
    – Mainly wave-deposited quartz-rich sands
  • Continental shelf deposits
    – Relict sediments
  • Turbidite deposits
    – Graded bedding
  • Glacial deposits
    – High-latitude continental shelf
    – Currently forming by ice rafting

Pelagic Deposits

  • Fine-grained material
  • Accumulates slowly on deep ocean floor
  • Pelagic lithogenous sediment from
    – Volcanic ash (volcanic eruptions)
    – Wind-blown dust
    – Fine-grained material transported by deep ocean currents
  • Abyssal Clay
    – At least 70% clay sized particles from
    continents
    – Red from oxidized iron (Fe)
    – Abundant if other sediments absent

Biogenous Sediment

  • Hard remains of once-living organisms
  • Two major types:
    – Macroscopic
  • Visible to naked eye
  • Shells, bones, teeth
    – Microscopic
  • Tiny shells or tests
  • Biogenic ooze
  • Mainly algae and protozoans

Biogenous Sediment Composition

  • Two most common chemical compounds:
    – Calcium carbonate (CaCO3)
    – Silica (SiO2 or SiO2·nH2O)

Silica in Biogenous Sediments

  • Diatoms
    – Photosynthetic algae
    – Diatomaceous earth
  • Radiolarians
    – Protozoans
    – Use external food
  • Tests – shells of microscopic organisms
  • Tests from diatoms and radiolarians generate siliceous ooze.

Diatomaceous Earth

  • Siliceous ooze lithifies into diatomaceous earth.
  • Diatomaceous earth has many commercial uses.

Calcium Carbonate in Biogenic Sediments

  • Coccolithophores
    – Also called nannoplankton
    – Photosynthetic algae
    – Coccoliths – individual plates from dead organism
    – Rock chalk
  • Lithified coccolith-rich ooze
Calcium Carbonate in Biogenic Sediments
Calcium Carbonate in Biogenic Sediments
  • Foraminifera
    – Protozoans
    – Use external food
    – Calcareous ooze

Distribution of Biogenous Sediments

  • Depends on three processes:
    – Productivity
  • Number of organisms in surface water above ocean floor
    – Destruction
  • Skeletal remains (tests) dissolve in seawater at depth
    – Dilution
  • Deposition of other sediments decreases percentage of biogenous sediments

Pelagic Deposits

  • Siliceous ooze
  • Accumulates in areas of high productivity
  • Silica tests no longer dissolved by seawater when buried by other tests

Neritic Deposits

  • Dominated by lithogenous sediment, may contain biogenous sediment
  • Carbonate Deposits
    – Carbonate minerals containing CO3
    – Marine carbonates primarily limestone
  • CaCO3
    – Most limestones contain fossil shells
  • Suggests biogenous origin
    – Ancient marine carbonates constitute 25% of all sedimentary rocks on Earth.

Carbonate Deposits

  • Stromatolites
    – Fine layers of carbonate
    – Warm, shallow-ocean, high salinity
    – Cyanobacteria
  • Lived billions of years ago
  • Modern stromatolites live near Shark Bay, Australia

Calcareous Ooze

  • CCD – Calcite compensation depth
    – Depth where CaCO3 readily dissolves
    – Rate of supply = rate at which the shells dissolve
  • Warm, shallow ocean saturated with calcium carbonate
  • Cool, deep ocean undersaturated with calcium carbonate
    – Lysocline – depth at which a significant amount of CaCO3 begins to dissolve rapidly

Calcareous Ooze and the CCD

  • Scarce calcareous ooze below 5000 meters (16,400 feet) in modern ocean
  • Ancient calcareous oozes at greater depths if moved by sea floor spreading

Distribution of Modern Calcium Carbonate Sediments

The map shows the percentage (by weight) of calcium carbonate in the modern surface sediments of the ocean basins. High concentrations of calcareous ooze (sometimes exceeding 80%) are found along segments of the midocean ridge, but little is found in deep-ocean basins below the CCD. For example, in the northern Pacific Ocean—one of the deepest parts of the world ocean—there is very little calcium carbonate in the sediment. Calcium carbonate is also rare in sediments accumulating beneath cold, high-latitude waters where calcareous-secreting organisms are relatively uncommon.

Environmental Conditions for Oozes

COMPARISON OF ENVIRONMENTS INTERPRETED FROM DEPOSITS OF SILICEOUS AND CALCAREOUS OOZE IN SURFACE SEDIMENTS
 Siliceous oozeCalcareous ooze
Surface water temperature above sea floor depositsCoolWarm
Main location foundSea floor beneath cool surface water in high latitudesSea floor beneath warm surface water in low latitudes
Other factorsUpwelling brings deep, cold, nutrient-rich water to the surfaceCalcareous ooze dissolves below the CCD
Other locations found  Sea floor beneath areas of upwelling, including along the equatorSea floor beneath warm surface water in low latitudes along the mid-ocean ridge

Hydrogenous Marine Sediments

  • Minerals precipitate directly from seawater
    – Manganese nodules
    – Phosphates
    – Carbonates
    – Metal sulfides
  • Small proportion of marine sediments
  • Distributed in diverse environments

Manganese Nodules

  • Fist-sized lumps of manganese, iron, and other metals
  • Very slow accumulation rates
  • Many commercial uses
  • Unsure why they are not buried by seafloor sediments
Manganese Nodules
Manganese Nodules

Phosphates and Carbonates

  • Phosphates
    – Phosphorus-bearing
    – Occur beneath areas in surface ocean of very
    high biological productivity
    – Economically useful as fertilizer
  • Carbonates
    – Aragonite and calcite
    – Oolites

Metal Sulfides

  • Metal sulfides
    – Contain:
  • Iron
  • Nickel
  • Copper
  • Zinc
  • Silver
  • Other metals
    – Associated with hydrothermal vents

Evaporites

  • Evaporites
    – Minerals that form when seawater evaporates
    – Restricted open ocean circulation
    – High evaporation rates
    – Halite (common table salt) and gypsum

Evaporiative Salts in Death Valley

Cosmogenous Marine Sediments

  • Macroscopic meteor debris
  • Microscopic iron-nickel and silicate spherules (small globular masses)
    – Tektites
    – Space dust
  • Overall, insignificant proportion of marine sediments

Marine Sediment Mixtures

  • Usually mixture of different sediment types
  • Typically one sediment type dominates in different areas of the sea floor.

Pelagic and Neritic Sediment Distribution

  • Neritic sediments cover about ¼ of the sea floor.
  • Pelagic sediments cover about ¾ of the sea floor.
  • Distribution controlled by
    – Proximity to sources of lithogenous sediments
    – Productivity of microscopic marine organisms
    – Depth of water
    – Sea floor features

Pelagic Sediment Types

the proportion of each ocean floor that is covered by the pelagic deposits abyssal clay, calcareous ooze, and siliceous ooze. The world ocean (combined) pie chart shows that calcareous ooze is the most dominant sediment worldwide, covering about 45% of the deep-ocean floor. The world ocean pie chart also shows that abyssal clay covers about 38% and siliceous ooze about 8% of the world ocean floor area. If you examine the individual ocean pie charts, they show that the amount of ocean basin floor covered by calcareous ooze decreases in deeper ocean basins because they generally lie beneath the CCD. The dominant oceanic sediment in the deepest basin—the North Pacific—is abyssal clay . Conversely, calcareous ooze is the most widely deposited sediment in the shallower Atlantic and Indian Oceans. Note that siliceous oozes cover a smaller percentage of the ocean floor because regions of high productivity of organisms that produce silica tests are generally restricted to the equatorial region (for radiolarians) and the high latitudes such as near Antarctica and the far northern Pacific (for diatoms).

AVERAGE RATES OF DEPOSITION OF SELECTED MARINE SEDIMENTS
  Type of sediment/deposit  Average rate of deposition (per 1000 years)Thickness of deposit after 1000 years equivalent to . . .
Coarse lithogenous sediment, neritic deposit1 meter (3.3 feet)A meter stick
Biogenous ooze, pelagic deposit1 centimeter (0.4 inch)The diameter of a dime
Abyssal clay, pelagic deposit1 millimeter (0.04 inch)The thickness of a dime
Manganese nodule, pelagic deposit0.001 millimeter (0.00004 inch)A microscopic dust particle

Sea Floor Sediments Represent Surface Ocean Conditions

  • Microscopic tests sink slowly from surface ocean to sea floor (10–50 years)
  • Tests could be moved horizontally
  • Most biogenous tests clump together in fecal pellets
    – Fecal pellets large enough to sink quickly (10–15 days)

Worldwide Marine Sediment Thickness

The map shows that areas of thick sediment accumulation occur on the continental shelves and rises, especially near the mouths of major rivers. The reason sediments in these locations are so thick is because they are close to major sources of lithogenous sediment. Conversely, areas where marine sediments are thinnest are where the ocean floor is young, such as along the crest of the midocean ridge. Since sediments accumulate slowly in the deep ocean and the sea floor is continually being created here, there hasn’t been enough time for much sediment to accumulate.
However, as the sea floor moves away from the mid-ocean ridge, it gets progressively older and carries a thicker pile of sediments.

Resources from Marine Sediments

  • Both mineral and organic resources
  • Not easily accessible
    – Technological challenges
    – High costs

Energy Resources

  • Petroleum
    – Ancient remains of microscopic organisms
    – More than 95% of economic value of oceanic nonliving resources
  • More than 30% of world’s oil from offshore resources
  • Future offshore exploration will be intense
    – Potential for oil spills

Energy Resources

  • Gas Hydrates
    – Also called clathrates
    – High pressures squeeze chilled water and gas into icelike solid
    – Methane hydrates most common
  • Gas hydrates resemble ice but burn when lit
  • May form on sea floor
    – Sea floor methane supports rich community of organisms
  • Most deposits on continental shelf
  • Release of sea floor methane may alter global climate.
  • Warmer waters may release more methane.
  • Methane release may cause underwater slope failure.
    – Tsunami hazard
  • Gas hydrates may be largest store of usable energy.
  • Rapidly decompose at surface pressures and temperatures

Other Resources

  • Sand and gravel
    – Aggregate in concrete
    – Some is mineral-rich
  • Evaporative salts
    – Gypsum – used in drywall
    – Halite – common table salt
  • Phosphorite – phosphate minerals
    – Fertilizer for plants
    – Found on continental shelf and slope
  • Manganese nodules
    – Lumps of metal
    – Contain manganese, iron, copper, nickel, cobalt
    – Economically useful
 Mining sea salt. A salt mining operation at Scammon’s Lagoon, Baja California, Mexico. Low-lying areas near the
lagoon are allowed to flood with seawater, which evaporates in the
arid climate and leaves deposits of salt that are then collected.
Mining sea salt. A salt mining operation at Scammon’s Lagoon, Baja California, Mexico. Low-lying areas near the
lagoon are allowed to flood with seawater, which evaporates in the arid climate and leaves deposits of salt that are then collected.
9 Mining manganese nodules. Manganese nodules
can be collected by dredging the ocean floor. This metal dredge is
shown unloading nodules onto the deck of a ship.
Mining manganese nodules. Manganese nodules can be collected by dredging the ocean floor. This metal dredge is shown unloading nodules onto the deck of a ship.

Distribution of Sea Floor Manganese Nodules

The map shows that vast areas of the sea floor contain manganese nodules, particularly in the Pacific Ocean.
Technologically, mining the deep-ocean floor for manganese nodules is possible. However, the political issue of determining international mining rights at great distances from land has hindered exploitation of this resource. In addition, environmental concerns about mining the deep-ocean floor have not been fully addressed. Evidence suggests that it takes at least several million years for manganese nodules to form and that their formation depends on a particular set of physical and chemical conditions that probably do not last long at any location. In essence, they are a nonrenewable resource that will not be replaced for a very long time once they are mined. Of the five metals commonly found in manganese nodules, cobalt is the only metal deemed “strategic” (essential to national security) for the United States. It is required to produce dense, strong alloys with other metals for use in high-speed cutting tools, powerful permanent magnets, and jet engine parts. Currently, the
United States must import all of its cobalt from large deposits in southern Africa. However, the United States has considered deep-ocean nodules and crusts (hard coatings on other rocks) as a more reliable source of cobalt. In the 1980s, cobalt-rich manganese crusts were discovered on the upper slopes of islands and seamounts that lie relatively close to shore and within the jurisdiction
of the United States and its territories. The cobalt concentrations in these crusts are about one-and-a-half times as rich as the best African ores and at least twice as rich as deep-sea manganese nodules. However, interest in mining these deposits has faded because of lower metal prices from land-based sources.

Other Resources

  • Rare Earth elements
    – Assortment of 17 metals
    – Used in technology, e.g., cell phones, television screens, etc.
  • Sea floor may hold more rare Earth element deposits than found on land.

Rare-earth elements—an assortment of 17 chemically similar metallic elements such as lanthanum and neodymium—are used in a variety of electronic, optical, magnetic, and catalytic applications. For example, rare-earth elements are used in a host of technological gadgets from cell phones and television screens to fluorescent light bulbs and batteries in electric cars. Demand for rare-earth elements has skyrocketed in recent years, with China supplying about 90% of the current world demand. Over millions of years, deep-sea hot springs associated with the mid-ocean ridge pulled rare-earth elements out of seawater and enriched them in sea floor muds. A recent study of rare-earth elements on the floor of the Pacific Ocean indicated that some locations are particularly enriched. For example, an area of the sea floor near Hawaii measuring 1 square kilometer (0.4 square mile) holds as much as 25,000 metric tons (55 million pounds) of rare-earth elements. Overall, estimates suggest
that the ocean floor might hold more rare-earth elements than all the known deposits on land

Reference: All images and content are taken from Essentials of Oceanography by Alan P. Trujillo and Harold V. Thurman, 12th Edition.

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CSIR NET Exam: EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES

Exam Pattern: EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES 

 PART APART BPART CTOTAL
Total questions205080150
Max No. of Questions to attempt15352575
Marks for each correct answer224200
Marks for each incorrect answer (Negative marking for part A & B is @ 25%, and part C is @ 33%)0.50.51.32

The candidate is required to answer a maximum of 15, 35, and 25 questions from Part-A, Part-B, and Part-C, respectively. If more than the required number of questions are answered, only the first 15, 35, and 25 questions in Part A, Part B, and Part C, respectively, will be taken up for evaluation.

Below each question in Part A, Part B, and Part C, four alternatives or responses are given. Only one of these alternatives is the “correct” option to the question. The candidate has to find, for each question, the correct or the best answer.

Syllabus

EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES

PAPER I (PART B)

  1. The Earth and the Solar System

    • Milky Way and the solar system.
    • Modern theories on the origin of the Earth and planetary bodies.
    • Earth’s orbital parameters, Kepler’s laws of planetary motion.
    • Geological Time Scale; space and time scales of processes in the solid Earth, atmosphere, and oceans.
    • Radioactive isotopes and their applications.
    • Meteorites: chemical composition and primary differentiation of the Earth.
    • Basic principles of stratigraphy.
    • Theories about the origin of life and fossil records.
    • Earth’s gravity, magnetic fields, and thermal structure: Geoid and spheroid concepts; Isostasy.
  2. Earth Materials, Surface Features, and Processes

    • Gross composition and physical properties of important minerals and rocks.
    • Properties and processes responsible for mineral concentrations.
    • Distribution of rocks and minerals in Earth’s units and India.
    • Physiography of the Earth; weathering, erosion, and soil formation.
    • Energy balance of Earth’s surface processes.
    • Physiographic features and river basins in India.
  3. Interior of the Earth, Deformation, and Tectonics

    • Basic concepts of seismology and Earth’s internal structure.
    • Physico-chemical and seismic properties of Earth’s interior.
    • Stress and strain concepts; rock deformation.
    • Folds, joints, and faults; causes and measurement of earthquakes.
    • Interplate and intraplate seismicity; paleomagnetism.
    • Sea-floor spreading and plate tectonics.
  4. Oceans and Atmosphere

    • Hypsography of continents and ocean floors: continental shelves, slopes, abyssal plains.
    • Physical and chemical properties of seawater; residence times of elements.
    • Ocean currents, waves, tides, thermohaline circulation, and conveyor belts.
    • Major water masses, biological productivity, and fluid motion.
    • Atmospheric structure and heat budget; greenhouse gases and global warming.
    • General circulation, monsoon systems, ENSO, cyclones, and local systems in India.
    • Marine and atmospheric pollution, ozone depletion.
  5. Environmental Earth Sciences

    • Properties of water and the hydrological cycle.
    • Energy resources: uses, degradation, alternatives, and management.
    • Ecology, biodiversity, and natural resource conservation.
    • Natural hazards and remote sensing applications.

PAPER I (PART C)

I. Geology

  1. Mineralogy and Petrology

    • Point group, space group, and lattice concepts.
    • Crystal field theory, mineralogical spectroscopy, and bonding in mineral structures.
    • Genesis, properties, and crystallization of magmas.
    • Metamorphic structures, textures, and thermobarometry.
    • Petrogenesis of Indian rock suites: Deccan Traps, charnockites, ophiolites, and more.
  2. Structural Geology and Geotectonics

    • Stress and strain analysis; Mohr circles.
    • Geometry and mechanics of folds, faults, and ductile shear zones.
    • Plate boundaries, mantle plumes, and Himalayan orogeny.
  3. Paleontology and Applications

    • Life origin theories, evolution models, and mass extinctions.
    • Applications of fossils in age determination, paleoecology, and paleogeography.
    • Micropaleontology in hydrocarbon exploration.
  4. Sedimentology and Stratigraphy

    • Classification of sediments and sedimentary rocks.
    • Sedimentary environments and basin evolution.
    • Stratigraphic principles, correlation methods, and sequence stratigraphy.
    • Phanerozoic stratigraphy of India.
  5. Marine Geology and Paleoceanography

    • Ocean floor morphology, ocean circulation, and thermohaline processes.
    • Factors influencing oceanic sediments and paleoceanographic reconstruction.
  6. Geochemistry

    • Atomic properties, periodic table, thermodynamics of reactions, and isotopes in geochronology.
    • Applications of stable isotopes in Earth processes.
  7. Economic Geology

    • Ore formation processes, mineral deposit studies, and petroleum geology.
    • Coal and unconventional energy resources.
  8. Precambrian Geology and Crustal Evolution

    • Evolution of Earth systems and Precambrian characteristics of India.
    • Precambrian–Cambrian boundary.
  9. Quaternary Geology

    • Quaternary stratigraphy, climate variability, and human evolution.
    • Dating methods and tectonic geomorphology.
  10. Applied Geology

  • Remote sensing and GIS.
  • Engineering properties of rocks; construction investigations.
  • Methods of mineral exploration and groundwater studies.

II. Physical Geography

  1. Geomorphology: Landform processes, DEM analysis, extraterrestrial geomorphology.
  2. Climatology: Radiation balance, wind systems, ENSO, and climate classification.
  3. Biogeography: Plant and animal associations, Indian biogeography, and conservation.
  4. Environmental Geography: Man-land relationships, hazards, and ecological balance.
  5. Geography of India: Physical geography, climatology, agriculture, and population characteristics.

III. Geophysics

  1. Signal Processing: Fourier transforms, filters, and signal analysis.
  2. Field Theory: Newtonian potential, Green’s theorem, and seismic wave propagation.
  3. Numerical Analysis and Inversion: Least squares, optimization, and pattern recognition.
  4. Gravity and Magnetic Methods: Data interpretation and anomaly analysis.
  5. Seismic Methods: Ray theory, reflection/refraction techniques, seismic stratigraphy.
  6. Well Logging: Techniques for lithology, porosity, and fluid saturation interpretation.

(IV) METEOROLOGY

1) Climatology

  • Same as under Geography.

2) Physical Meteorology

  • Thermal Structure of the Atmosphere and Its Composition.
  • Radiation:
    • Basic laws – Rayleigh and Mie scattering, multiple scattering.
    • Radiation from the sun, solar constant, effect of clouds, surface and planetary albedo.
    • Emission and absorption of terrestrial radiation, radiation windows, radiative transfer, Greenhouse effect, net radiation budget.
  • Thermodynamics of Dry and Moist Air:
    • Specific gas constant, adiabatic and isentropic processes, entropy and enthalpy.
    • Moisture variables, virtual temperature, Clausius–Clapeyron equation.
    • Adiabatic processes of moist air, thermodynamic diagrams.
  • Hydrostatic Equilibrium:
    • Hydrostatic equation, variation of pressure with height, geopotential, standard atmosphere, altimetry.
  • Vertical Stability of the Atmosphere:
    • Dry and moist air parcel and slice methods, tropical convection.
  • Atmospheric Optics:
    • Visibility and optical phenomena – rainbows, haloes, corona, mirage, etc.

3) Atmospheric Electricity

  • Fair weather electric field in the atmosphere and potential gradients.
  • Ionization in the atmosphere, electrical fields in thunderstorms.
  • Theories of thunderstorm electrification, structure of lightning flash, mechanisms of earth-atmospheric charge balance, and the role of thunderstorms.

4) Cloud Physics

  • Cloud classification, condensation nuclei, growth of cloud drops and ice-crystals.
  • Precipitation mechanisms: Bergeron–Findeisen process, coalescence process.
  • Precipitation of warm and mixed clouds, artificial precipitation, hail suppression, fog and cloud dissipation.
  • Radar observation of clouds and precipitation:
    • Radar equation, rain drop spectra, radar echoes of hailstorms, tornadoes, hurricanes, and rainfall measurements.

5) Dynamic Meteorology

  • Basic Equations and Fundamental Forces:
    • Pressure, gravity, centripetal and Coriolis forces.
    • Continuity and momentum equations (Cartesian and spherical coordinates).
    • Scale analysis, inertial flow, geostrophic and gradient winds, thermal wind.
    • Divergence and vertical motion, Rossby, Richardson, Reynolds, and Froude numbers.
  • Atmospheric Turbulence:
    • Mixing length theory, planetary boundary layer equations, Ekman layer, eddy transport of heat, moisture, and momentum.
  • Linear Perturbation Theory:
    • Internal and external gravity waves, inertia waves, gravity waves, Rossby waves, wave motion in the tropics, barotropic and baroclinic instabilities.
  • Atmospheric Energetics:
    • Kinetic, potential, and internal energies; conversion into kinetic energy; available potential energy.

6) Numerical Weather Prediction (NWP)

  • Computational instability, filtering of sound and gravity waves.
  • Filtered forecast equations, barotropic and baroclinic models.
  • Objective analysis, data assimilation techniques, satellite applications in NWP.

7) General Circulation and Climate Modelling

  • Observed zonally symmetric circulations, meridional circulation models.
  • General circulation modelling principles: grid-point and spectral GCMs.
  • Climate variability phenomena: ENSO, QBO, MJO, etc.
  • Ocean-atmosphere coupled models.

8) Synoptic Meteorology

  • Weather observations and transmission, synoptic charts.
  • Synoptic weather forecasting, prediction of weather elements, and hazardous weather phenomena.
  • Tropical Meteorology:
    • ITCZ, monsoons, tropical cyclones, jet streams.
  • Extra-Tropical Features:
    • Jet streams, extratropical cyclones, anticyclones.
  • Air masses and fronts: sources, classification, frontogenesis, and associated weather.

9) Aviation Meteorology

  • Meteorological role in aviation, weather hazards during takeoff, cruising, and landing.
  • In-flight hazards: icing, turbulence, visibility issues, gusts, wind shear, thunderstorms.

10) Satellite Meteorology

  • Polar orbiting and geostationary satellites.
  • Applications in identifying synoptic systems, cyclones, temperature estimation, rainfall prediction, and temperature/humidity soundings.

(V) OCEAN SCIENCES

1) Physical Oceanography

  • T-S diagrams, mixing processes, characteristics of water masses.
  • Wind-generated waves, shallow and deep-water wave dynamics.
  • Coastal processes: wave reflection, refraction, diffraction, littoral currents, rip currents, tsunami, and more.
  • Ocean Circulation:
    • Global conveyor belt circulation, Ekman’s theory, upwelling processes.

2) Chemical Oceanography

  • Composition of seawater, chemical exchanges, and classification of elements.
  • Element chemistry under special conditions (estuaries, vents, etc.).
  • Carbonate chemistry, biological pumps, and sedimentary deposit factors.

3) Geological Oceanography

  • Topics as listed under “Marine Geology & Paleoceanography.”

4) Biological Oceanography

  • Classification of marine environments and organisms.
  • Primary and secondary production, factors affecting biodiversity.
  • Human impacts on marine communities and climate change effects.

 

How Study Hub Can Help You Prepare for the Earth, Atmospheric, Ocean, and Planetary Sciences Syllabus

Preparing for the extensive and demanding syllabus of Earth, Atmospheric, Ocean, and Planetary Sciences (702) requires a strategic approach and access to comprehensive study resources. Study Hub (accessible at studyhub.net.in) offers unparalleled support to help candidates excel in this challenging domain. Here’s how Study Hub can guide your preparation:


Comprehensive Coverage of Topics

At Study Hub, we provide in-depth study materials, mock tests, and curated articles to help candidates grasp even the most complex topics. Our resources are designed to address every aspect of the syllabus, including:

  1. Meteorology: Understand critical concepts like the thermal structure of the atmosphere, radiative transfer, vertical stability, numerical weather prediction, general circulation and climate modelling, and the role of satellite meteorology in observing weather systems such as cyclones, monsoons, and thunderstorms.

  2. Ocean Sciences: Dive into topics such as physical oceanography, chemical oceanography, geological oceanography, and biological oceanography. Study Hub’s resources emphasize key aspects like upwelling processes, estuarine circulation, ocean eddies, Ekman theory, and global conveyor belt circulation—helping you understand the intricate processes of ocean systems.

  3. Atmospheric Dynamics and Energetics: Through articles, conceptual guides, and practice questions, candidates gain a strong grasp of fundamental equations, vorticity, geostrophic winds, Rossby waves, atmospheric turbulence, and barotropic and baroclinic instabilities.

  4. Planetary Sciences: Our expertly crafted content helps students explore planetary structures, processes, and phenomena with precision, complementing other topics under Earth Sciences for an interdisciplinary understanding.


Mock Tests and Evaluation Framework

We align our mock tests and sample papers with the pattern of the Earth Sciences examination:

  • Objective Analysis for Numerical Weather Prediction (NWP): Test your knowledge of filtered forecasting models and data assimilation techniques.
  • Synoptic Meteorology Practices: Work on real-world weather data and forecast exercises involving tropical cyclones, ITCZ systems, monsoon depressions, and jet streams.
  • Topic-specific tests ensure mastery in areas like atmospheric optics, biochemical nutrient cycling, and the impact of human activities on ecosystems.

Why Study Hub is the Perfect Partner for Your Earth Sciences Preparation

  1. Academic Rigor: Study Hub maintains an academic tone throughout its resources, ensuring in-depth coverage of essential keywords such as radiative budget, MJO (Madden-Julian Oscillation), Quasi-Biennial Oscillation (QBO), and ENSO phenomena.
  2. Focused on Practical Applications: Be it radar observations, wave refraction techniques, or the impact of anthropogenic inputs on marine biodiversity, we emphasize the practical relevance of each topic for better comprehension.
  3. Adaptive Materials: From simple T-S diagrams to advanced topics like geopotential variation and numerical baroclinic models, we tailor our resources to match both beginner and advanced levels of understanding.
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