The document summarizes the structure and dynamics of the Earth. It describes how the Earth is composed of layers with different densities, including the crust, mantle, and core. It explains that the lithosphere is divided into tectonic plates that move over the asthenosphere due to convection currents in the mantle. There are three main types of plate boundaries - divergent where new crust forms, convergent where plates collide and one is subducted, and transform where plates slide past each other. Plate tectonics involves the creation of oceanic crust at mid-ocean ridges and recycling of crust through subduction.
Minerals are formed by changes in chemical energy in systems which contain one fluid or vapor phase. In nature, minerals are formed by crystallisation or precipitation from concentrated solutions. These solutions are called as ore-bearing fluids. Ore-bearing fluids are characterised by high concentration of certain metallic or other elements.
Fluids are the most effective agents for the transport of material in the mantle and the Earth's crust.
How can minerals deposits be formed; GEOLOGICAL PROCESSES; Ore Fluids; Ore Forming Processes; Concentrating Processes; Magmatic mineral deposits; Residual mineral deposits ; Placer deposits; Sedimentary mineral deposits; Metamorhogenic mineral deposits; Hydrothermal mineral deposits ; Magmatic Deposits
Cumulate deposits: fractional crystallization processes can concentrate metals (Cr, Fe, PGE, Pt, Ni, Ti, Diamond ))
Pegmatites : late staged crystallization forms pegmatites and many residual elements are concentrated (Li, Ce, Be, Sn, U, Rare Earths (REE), Feldspar, Mica, Gems).
magmatic deposits; Mode of Formation of Magmatic Ores Deposits; Mode of Formation of Orthomagmatic Ores ; Fractional Crystallization (or Crystal fractionation ); Magmatic (or Liquid ) Immiscibility; Simple crystallization without concentration (Dissemination); Segregation of early formed crystals; (Layer Types); Injection of material concentrated elsewhere by differentiation Residual liquid segregation; Residual liquid injection; Immiscible liquid segregation; Immiscible-liquid-injection; Early magmatic deposit; Late magmatic deposit; Types of Magmatic Ore Deposits:Chromite; Fe-Ti (± V) oxides; Ni – Cu – Fe (± Pt) sulfides; Platinum Group Elements (PGEs); REE, and Zr in Carbonatites; Diamond in kimberlites.
Minerals are formed by changes in chemical energy in systems which contain one fluid or vapor phase. In nature, minerals are formed by crystallisation or precipitation from concentrated solutions. These solutions are called as ore-bearing fluids. Ore-bearing fluids are characterised by high concentration of certain metallic or other elements.
Fluids are the most effective agents for the transport of material in the mantle and the Earth's crust.
How can minerals deposits be formed; GEOLOGICAL PROCESSES; Ore Fluids; Ore Forming Processes; Concentrating Processes; Magmatic mineral deposits; Residual mineral deposits ; Placer deposits; Sedimentary mineral deposits; Metamorhogenic mineral deposits; Hydrothermal mineral deposits ; Magmatic Deposits
Cumulate deposits: fractional crystallization processes can concentrate metals (Cr, Fe, PGE, Pt, Ni, Ti, Diamond ))
Pegmatites : late staged crystallization forms pegmatites and many residual elements are concentrated (Li, Ce, Be, Sn, U, Rare Earths (REE), Feldspar, Mica, Gems).
magmatic deposits; Mode of Formation of Magmatic Ores Deposits; Mode of Formation of Orthomagmatic Ores ; Fractional Crystallization (or Crystal fractionation ); Magmatic (or Liquid ) Immiscibility; Simple crystallization without concentration (Dissemination); Segregation of early formed crystals; (Layer Types); Injection of material concentrated elsewhere by differentiation Residual liquid segregation; Residual liquid injection; Immiscible liquid segregation; Immiscible-liquid-injection; Early magmatic deposit; Late magmatic deposit; Types of Magmatic Ore Deposits:Chromite; Fe-Ti (± V) oxides; Ni – Cu – Fe (± Pt) sulfides; Platinum Group Elements (PGEs); REE, and Zr in Carbonatites; Diamond in kimberlites.
SUPERGENE ENRICHMENT; Definition; Zones; Morphology of Zoning; Oxidized zone ; Supergene zone ; Gossans and Cappings; Chemical Changes Involved; Electrowinning; Formation of Copper Oxides
Information about these fluids is an invaluable aid in mineral exploration.
Conventional academic methods of analysing fluid inclusions are too slow and tedious to be of practical application in typical mineral exploration activities.
However, the academic data from numerous studies does show that CO2 is an exceptionally important indicator when exploring for most types of gold deposit.
Because the baro-acoustic decrepitation method is a rapid and reliable method to measure CO2 contents in fluids, it can be used to study a spatial array of data and it is an invaluable and practical exploration method.
Measurements of temperatures of fluid inclusions does not usually help in mineral exploration as hydrothermal minerals deposit over a wide temperature range and there is no specific temperature which is indicative of mineralisation. However, if temperatures are available on a large spatial array of samples, then temperature trends may be a useful exploration method to find the hottest part of the system, which is presumably the location of the best economic mineralisation. Baro-acoustic decrepitation is the most practical method to determine temperatures of the large numbers of samples required.
Salinities of fluid inclusions are of limited use in exploration and are difficult to measure. However, they can be used to recognise intrusion related hydrothermal systems.
This is my presentation on the tectonic control of sediments.
It includes the effects of tectonics either direct or indirect on sediments and sedimentation.
Sedimentation along various plate boundaries.
Few examples as evidence from Pakistan (the Siwalik Group) and Argentina (Fiambala Basin)
Introduction of mineral deposits: Mineral deposit ; A geological definition of an ore deposit; Ore Deposit Environments; The significance of ore deposit size; Which commodities are included by the definition of Ore Deposits ; The extraction of an economic commodity from ore ; Geological Factors Affecting Economics of Ore Extraction ; Shape and depth of the deposit; Mineralogy and texture of the ore; The presence of multiple extractable products; Metals enrichment factors; Ore Deposit Constitutes; Ore Deposit Geology and Related Sciences; Structural Control Ore Deposits; Depth of Occurrence Mineral deposits; Nature of Mineralization; Morphology of Ore Deposit; Geographical Localization of Ore Deposits;
Orebodies; oreshoots; ore deposits; ore reserves
Komattite
Named after the Komati River in South Africa.
first described by Morris and Richard (twins) for ultramafic units in the Barberton Greenstone belt of South Africa.
Mostly of komatiite are Archean age
distributed in the Archaean shield areas.
Also a few are Proterozoic and Phanerozoic.
In all ages komatiites are highly magnesium.
Mostly a volcanic rock; occasionally intrusive.
Mafic rocks were identified as extrusive because of their volcanic textures and structures, and they seem to have been accepted as a normal component of Archean volcanic successions, Abitibi in Canada.
The ultramafic rocks were interpreted as intrusive which are founded as sills and dykes, Barberton in South Africa.
Spinifex texture-typical of Komatiites:
Sedimentary basins are the depressions in the earth's crust where loose particles accumulate and finally lithified to form sedimentary rocks. Basins are particularly attractive to geoscientists from time immemorial due to the wealth hidden here in the form of oil, gas, coal etc. In this document you will find the types of basins, basin-fill types, methods of basin analysis and so on.
SUPERGENE ENRICHMENT; Definition; Zones; Morphology of Zoning; Oxidized zone ; Supergene zone ; Gossans and Cappings; Chemical Changes Involved; Electrowinning; Formation of Copper Oxides
Information about these fluids is an invaluable aid in mineral exploration.
Conventional academic methods of analysing fluid inclusions are too slow and tedious to be of practical application in typical mineral exploration activities.
However, the academic data from numerous studies does show that CO2 is an exceptionally important indicator when exploring for most types of gold deposit.
Because the baro-acoustic decrepitation method is a rapid and reliable method to measure CO2 contents in fluids, it can be used to study a spatial array of data and it is an invaluable and practical exploration method.
Measurements of temperatures of fluid inclusions does not usually help in mineral exploration as hydrothermal minerals deposit over a wide temperature range and there is no specific temperature which is indicative of mineralisation. However, if temperatures are available on a large spatial array of samples, then temperature trends may be a useful exploration method to find the hottest part of the system, which is presumably the location of the best economic mineralisation. Baro-acoustic decrepitation is the most practical method to determine temperatures of the large numbers of samples required.
Salinities of fluid inclusions are of limited use in exploration and are difficult to measure. However, they can be used to recognise intrusion related hydrothermal systems.
This is my presentation on the tectonic control of sediments.
It includes the effects of tectonics either direct or indirect on sediments and sedimentation.
Sedimentation along various plate boundaries.
Few examples as evidence from Pakistan (the Siwalik Group) and Argentina (Fiambala Basin)
Introduction of mineral deposits: Mineral deposit ; A geological definition of an ore deposit; Ore Deposit Environments; The significance of ore deposit size; Which commodities are included by the definition of Ore Deposits ; The extraction of an economic commodity from ore ; Geological Factors Affecting Economics of Ore Extraction ; Shape and depth of the deposit; Mineralogy and texture of the ore; The presence of multiple extractable products; Metals enrichment factors; Ore Deposit Constitutes; Ore Deposit Geology and Related Sciences; Structural Control Ore Deposits; Depth of Occurrence Mineral deposits; Nature of Mineralization; Morphology of Ore Deposit; Geographical Localization of Ore Deposits;
Orebodies; oreshoots; ore deposits; ore reserves
Komattite
Named after the Komati River in South Africa.
first described by Morris and Richard (twins) for ultramafic units in the Barberton Greenstone belt of South Africa.
Mostly of komatiite are Archean age
distributed in the Archaean shield areas.
Also a few are Proterozoic and Phanerozoic.
In all ages komatiites are highly magnesium.
Mostly a volcanic rock; occasionally intrusive.
Mafic rocks were identified as extrusive because of their volcanic textures and structures, and they seem to have been accepted as a normal component of Archean volcanic successions, Abitibi in Canada.
The ultramafic rocks were interpreted as intrusive which are founded as sills and dykes, Barberton in South Africa.
Spinifex texture-typical of Komatiites:
Sedimentary basins are the depressions in the earth's crust where loose particles accumulate and finally lithified to form sedimentary rocks. Basins are particularly attractive to geoscientists from time immemorial due to the wealth hidden here in the form of oil, gas, coal etc. In this document you will find the types of basins, basin-fill types, methods of basin analysis and so on.
Residual mineral deposits; Laterites; Laterite Profile; Laterisation system; Laterite/Bauxite Conditions; Laterite-type Bauxite, Constitution of Bauxite, Types of deposits; Origin and Mode of formation; Clay (Kaolinite) Deposits; Nickel Laterite Deposits; Mineralogy and Types of lateritic nickel ore deposits; World Nickel Laterite Deposits; Processing of Ni Laterites; Example: Ni-laterites, Ni in soils in east Albania
This presentation reviews the complete water cycle, including some of the constructed water cycle. Used as an environmental overview for life science and environmental. Geared for Secondary students, but also could be used as an intro for up to College level classes.
MANGANESE ORE DEPOSITS, Sedimentary Manganese Deposits, Types of Sedimentary Manganese, Classification, Manganese Nodules, EGYPTIAN MANGANESE ORE DEPOSITS , IRON ORE DEPOSITS, Cycle of Iron , Ironstone (Sedimentary iron) Ore Deposits, Bog Iron Ore Deposits, Principal iron-bearing minerals, Geochemical stability of iron-rich minerals, World Resources Iron Deposit, EGYPTIAN IRON ORE DEPOSITS, Iron ore deposit of sedimentary nature, Sinai: Gabal Halal iron ore deposit, Aswan iron Ore Deposits, Bahariya iron Ore Deposits
Basic introduction to clinical trials and the placebo effect. Definitions, examples and cartoons illustrating the subject. Ends with short info on informed consent.
Oceanography is an interesting subject. Geological oceanography deals with a lot of unique aspects of the oceans including the ocean morphology and relief, continental margins, tectonic processes acting on the ocean bottoms, marine mineral resources, and the deep sea deposits. The subject also focuses on the never ending dynamic processes like ocean waters, ocean currents and their impacts with reference to space and time. Understanding the tectonic disposition and movement of crustal plates are an important part while studying the earth and atmospheric sciences, in general and oceanography, in particular. The continental margins and the deep ocean basins are the two major aspects to be understood in this subject. This lesson is on the characteristics of continental margins.
CSEC Geography- Internal Forces - Plate Tectonics and EarthquakesOral Johnson
This document looks at the Earth's internal forces. The main layers of the earth are described. The history surrounding plate tectonics is discussed. The different types of plate boundaries is also explained.
GEOGRAPHY IGCSE: PLATE TECTONICS. Earth's layers. Inner core, outer core, mantle, crust, the structure of Earth, plate boundaries and interactions, magma and igneous rocks, forming a volcano, compressional boundaries, folding.
This is the entire CSEC geography syllabus (some things might be missing). The information was collected from various websites and textbooks. The topics are:
- Internal forces
-External forces
-Rivers
-Limestone
-Coasts
-Coral reefs and Mangroves
-Weather and Climate
- Ecosystems (vegetation and soils)
-Natural hazards
- Urbanization
-Economic activity
-Environmental degradation
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
2. Structure of the Earth
The Earth is an irregular sphere,
with a radius that varies between
6,356 and 6,378 km. This solid
sphere is chemically divided into
layers that become less dense
from the centre towards the
surface.
The three main layers are:
(i)the core (which comprises an
Inner Core and an Outer Core);
(ii)the mantle, and
(iii) the crust.
Each layer has a distinctive
chemical composition, and a
different density (Figure 1).
3. The outer layer of the Earth is termed the
crust, which is divided into oceanic
crust and continental crust.
Overall, continental crust is richer in the
element silica, and is less dense, than
oceanic crust.
Oceanic crust (about 10 km thick) is
composed of iron-, magnesium-,
calcium-, and aluminium-rich silicate
minerals that typically form a dark
colored, heavy rock called basalt.
Continental crust (about 20 - 60 km thick)
is composed of potassium-, sodium-,
and aluminium-rich silicate minerals that
form a diverse range of rock types such
as granite.
The core is primarily composed of the
heavy elements iron and nickel.
The outer core is made of molten iron,
which produces the Earth's magnetic field.
The mantle is less-dense than the core. The
mantle extends to a depth of about 2,900
km. The mantle is rich in iron- and
magnesium-bearing silicate minerals.
The layers of the Earth.
4.
5.
6. The Earth consists of
series of concentric
layers which differ in
chemical and physical
properties.
The crust and upper part
of the mantle of the
Earth is further
subdivided into
the lithosphere and the
asthenosphere.
Dynamic Structure of the Earth
7.
8. The lithosphere is a strong layer, extending to a depth of 100 to 150 km, that
comprises the crust and part of the upper mantle (the upper rigid part). The
lithosphere is separated into seven large plates, and several smaller plates.
These plates, which terminate at different types of plate boundary, move over the
underlying asthenosphere.
9.
10. The asthenosphere (the middle part of the mantle - plastic, i.e., semi-liquid and
ductile) is a weaker layer, upon which the lithospheric plates move, and from
which magmas that form the oceanic crust are derived.
11. Heat from the Earth's core creates circulation patterns (i.e., convection currents)
in the mantle drive the motions of the overlying plates. The slow movement of the
lithospheric plates over the mobile asthenosphere is known as plate tectonics, a
process that maintains the surface of the Earth in a dynamic and active state.
Convection: is the process in which energy is transferred through a material with
any bulk motion of its particles. Convection is common in fluids.
12. Convection currents in the aesthenosphere
transfer heat to the surface, where plumes
of less dense magma break apart the plates
at the spreading centers, creating divergent
plate boundaries.
As the plates move away from the
spreading centers, they cool, and the
higher density basalt rocks that make up
ocean crust get consumed at the ocean
trenches/subduction zones. The crust is
recycled back into the aesthenosphere.
13. Because ocean plates are denser than continental plates, when these two types of
plates converge, the ocean plates are subducted beneath the continental plates.
Subduction zones and trenches are convergent margins. The collision of plates is
often accompanied by earthquakes and volcanoes.
14. Plate tectonics (previously known as continental drift) originated from the
geographical observation that the coastal profiles of South America and Africa
seem to fit one another.
First proposed by Alfred Wegener in the 1920s, the crust was imagined to be
made up of continent-sized slabs that "float" on a liquid layer and thus "drift"
around.
Plate tectonics
15. Plate tectonics, appeared in the 1960s when the mid-Atlantic ridge was
discovered, along with compelling evidence for injection rock caused "spreading“
leaving parallel north-south trending stripes of injected rock, the youngest of
which was adjacent to the injection ridge and the oldest farthest from it. The plate
tectonics solution to the seafloor spreading dilemma was the proposition that
new crustal mass created by injection must be compensated by "subduction", the
diving of ocean crust (more dense) under opposing continental plates (less
dense). Subduction zones and trenches are convergent margins. The collision of
plates is often accompanied by earthquakes and volcanoes.
16. This diagram shows the interaction between continental and oceanic plates, the
processes illustrated generally apply for the interaction between two oceanic
plates.
What happens in Plate Tectonics??!!
17. 1. There are two basic types of
LITHOSPHERE: CONTINENTAL
lithosphere has a low density because
it is made of relatively light-weight
minerals. OCEANIC lithosphere is
denser because it is composed of
heavier minerals. A plate may be made
up entirely of oceanic or continental
lithosphere, but most are partly oceanic
and partly continental.
What happens in Plate Tectonics??!!
18. 2. Beneath the lithospheric
plates lies the
ASTHENOSPHERE, a layer of the
mantle composed of denser
semi-solid rock. Because the
plates are less dense than the
asthenosphere beneath them,
they are floating on top of the
asthenosphere.
What happens in Plate Tectonics??!!
19. 3. Deep within the asthenosphere the
pressure and temperature are so high that
the rock can soften and partly melt. The
softened dense rock can flow very slowly.
Where temperature instabilities exist near
the core/mantle boundary, slowly moving
convection currents may form within the
semi-solid asthenosphere.
4. Once formed, convection currents bring
hot material from deeper within the mantle
up toward the surface.
What happens in Plate Tectonics??!!
20. What happens in Plate Tectonics??!!
5. As they rise and approach the surface,
convection currents diverge at the base of the
lithosphere. The diverging currents exert a weak
tension or “pull” on the solid plate above it.
Tension and high heat flow weakens the floating,
solid plate, causing it to break apart. The two
sides of the now-split plate then move away from
each other, forming a DIVERGENT PLATE
BOUNDARY.
21.
22.
23. What happens in Plate Tectonics??!!
6. The space between these
diverging plates is filled with molten
rocks (magma) from below. Contact
with seawater cools the magma,
which quickly solidifies, forming
new oceanic lithosphere. This
continuous process, operating over
millions of years, builds a chain of
submarine volcanoes and rift valleys
called a MID-OCEAN RIDGE or an
OCEANIC SPREADING RIDGE.
24. What happens in Plate Tectonics??!!
7. As new molten rock continues to be extruded at the mid-ocean ridge and added
to the oceanic plate (6), the older (earlier formed) part of the plate moves away
from the ridge.
8. As the oceanic plate moves farther and farther away from the active, hot
spreading ridge, it gradually cools down. The colder the plate gets, the denser
(“heavier”) it becomes. Eventually, the edge of the plate that is farthest from the
spreading ridges cools so much that it becomes denser than the asthenosphere
beneath it.
25. What happens in Plate Tectonics??!!
9. As it is known, denser materials
sink, and that’s exactly what
happens to the oceanic plate—it
starts to sink into the
asthenosphere! Where one plate
sinks beneath another a subduction
zone forms.
26.
27. What happens in Plate Tectonics??!!
10. The sinking lead edge of the oceanic plate actually
“pulls” the rest of the plate behind it—evidence
suggests this is the main driving force of subduction. It
is not sure how deep the oceanic plate sinks before it
begins to melt and lose its identity as a rigid slab, but it
remains solid far beyond depths of 100 km beneath the
Earth’s surface.
11. Subduction zones are one type of CONVERGENT
PLATE BOUNDARY, the type of plate boundary that
forms where two plates are moving toward one another.
Notice that although the cool oceanic plate is sinking,
the cool but less dense continental plate floats like a
cork on top of the denser asthenosphere.
28. What happens in Plate Tectonics??!!
12. When the subducting oceanic plate
sinks deep below the Earth’s surface,
the great temperature and pressure at
depth cause the fluids to “sweat” from
the sinking plate. The fluids sweated
out percolate upward, helping to
locally melt the overlying solid mantle
above the subducting plate to form
pockets of liquid rock (magma).
29. 13. The generated magma is less dense than
the surrounding rock, so it rises toward the
surface. Most of the magma cools and
solidifies as large bodies of plutonic
(intrusive) rocks far below the Earth’s
surface.
14. Some of the molten rock may reach the
Earth’s surface to erupt as the pent-up gas
pressure in the magma is suddenly released,
forming volcanic (extrusive) rocks.
What happens in Plate Tectonics??!!
30. There are three types of plate boundary: convergent, divergent, and transform plate
boundaries.
Divergent plate boundaries occur
where two lithospheric plates move
away from each other, driven by
magma rising from deep within the
mantle. Volcanic activity at a
divergent plate boundary creates
new lithosphere along what is
known as a spreading ridge.
Convergent plate boundaries occur
where two lithospheric plates move
towards each other, with one plate
overriding the other. The overridden
plate (sinking plate) is driven back into
the mantle, and is subsequently
destroyed along what is known as a
subduction zone. During this process,
earthquakes and volcanic activity are
generated in the overriding plate.
Types of Plate Boundary
31. Transform plate boundaries occur where two lithospheric plates slide laterally
past each other. Earthquakes are generated along this type of plate boundary.
Importantly, lithosphere is preserved along transform boundaries, it is not created
or destroyed as it is at divergent and convergent plate boundaries.
37. Plate tectonics is the
fundamental mechanism that
drives geological processes
in the geosphere. Plate
tectonic theory is based on an
understanding of the Earth's
internal structure, the
different types of tectonic
plates and plate boundaries,
and the driving forces of plate
movements.
The occurrence of
earthquakes and volcanoes,
the distribution of different
rock types, and the Rock
Cycle, as well as the
processes of mountain
building, continental rifting
and seafloor spreading, can
be concisely explained by
plate tectonic processes.
Plate Tectonics vs. Geological Processes
38. It is most often formed by
decompression-melting of
asthenosphere associated with
divergent plate boundaries or
mantle plumes, or by partial-
melting of water-rich crust
and/or asthenospheric material
in association with subduction
at convergent plate boundaries.
Magma is hot molten rock
within the earth. It can well-up
from deep to extrude from
fractures as lava flows and/or
pyroclastic ejecta.
The source for magma is not the
earth’s liquid outer core, a
common misconception;
instead, magma is generated at
the relatively shallow depths of
100 to 300 km, through the
partial melting of the earth’s
crust and mantle.
Magma
39. The ingredients necessary for the
production of magma involve the
interplay between heat, pressure,
intra-granular fluids (present as
gases within very hot rock or
magma) and the composition of the
material subject to melting.
1- Heating obviously brings
solids closer to their melting
points, the more heat, the more
likely a solid will melt.
2- In general, higher pressures
prevent melting because the
constituent atoms of minerals in
rocks are squeezed together and
remain solids under high
pressure. Consequently,
lowering pressure on hot rock
induces melting.
40.
41.
42.
43. 3- Intra-granular fluids (gases
within very hot rock or
magma) lower the melting
point of solids, so the
presence of fluids (gases),
generally water, allows solid
rock to melt at a lower
temperature (or heat content)
than it otherwise would.
Bubbles are common in
magmas erupted at the
Earth's surface
44. Factors that control the composition and viscosity of a magma; which in turn play a
determining role in the style of volcanic eruption, eruptive products, and the nature of the
volcano formed.
4- Finally, there are two general trends to explore in relation to rock
composition: rock that contains a relative abundance of silica (SiO2) and
aluminum (aluminum oxide) will melt at a lower temperature (heat content);
while a rock containing a relative abundance of ferromagnesian (Fe, Mg, and
Ca) ions will melt at higher temperatures (heat content).
45. Summary Table
Magma
Type
Solidified
Rock
Chemical Composition Temperature Viscosity Gas Content
Basaltic Basalt
45-55 SiO2 %, high in Fe, Mg, Ca,
low in K, Na
1000 - 1200 o
C 10 - 103
PaS Low
Andesitic Andesite
55-65 SiO2 %, intermediate in Fe,
Mg, Ca, Na, K
800 - 1000 o
C 103
- 105
PaS Intermediate
Rhyolitic Rhyolite
65-75 SiO2 %, low in Fe, Mg, Ca,
high in K, Na.
650 - 800 o
C 105
- 109
PaS High
46. Magma can also be generated by
melting due to the lowering of the
mantle melting temperature because
water and other volatile components
have been introduced into the mantle.
The occurs chiefly in subduction zones
where oceanic lithosphere is
descending back into the mantle. The
oceanic lithosphere carries with it water
in sediments and altered rocks.
The majority of magma erupted at the
Earth's surface is produced by melting
of mantle rock at depths of less than 50
km. Some magmas are produced by
melting of crustal rocks at shallower
levels (less than 30 km). The Earth's
interior is very hot, but it is solid
because of the high pressures. The
melting occurs when mantle rock rises
toward the surface, such as at mid-
ocean ridges, and undergoes
depressurization melting.
47. The melting of continental crust generates felsic magma enriched in silica and
aluminum, while melting of mantle rock (asthenosphere) and oceanic crust forms
ferromagnesian-rich, mafic magma. The earth’s crust naturally contains a higher
water content (because of its proximity to the hydrosphere) than the mantle,
accounting for higher water (and thus gas) content in felsic to intermediate
magmas. The relatively high content of silica and water in continental crust also
correlates with the lower melting temperatures of felsic to intermediate magmas.
Mantle material melts at greater depth and higher temperatures and pressures,
not requiring as much “assistance” from silica and water in the melting process.
48. Magma composition
The composition of magma (and
extruded lava) depends on three main
factors:
1)the degree of partial melting of the
crust or mantle;
2) the degree of magma mixing;
3) magmatic differentiation by fractional
crystallization.
49. Several types of basaltic lavas result from partial melting of mantle and oceanic
crust at subduction zones and mantle plumes.
Emplacement of basaltic magma chambers within continental crust often raises
the temperature of the surrounding silica- and water-rich country rock enough to
cause the country rock significant melting. The country rock becomes
assimilated into the basaltic magma to greater or lesser degree, contaminating it
with felsic material.
If substantial mixing of the magmas occurs, usually requiring significant plate
movement and/or magmatic convection, intermediate magma is born (ranging
from andesitic to dacitic or rhyodacitic).
50.
51.
52. Mafic magmas are generated
by decompression-melting
of highly mafic
asthenosphere and
assimilation-melting of mafic
oceanic lithosphere and
crust in association with
divergent plate boundaries
and some mantle plumes.
The magma source is
naturally low in water
content, however, these
magmas have a much easier
time of it; greater heat and
less silica allows it to readily
reach the surface as
volcanic eruptions (despite
its lack of gases). Mafic
magmas have lower
viscosities because of their
greater heat content and lack
of silica (they have a greater
abundance of iron and
magnesium ions).
53. Felsic magmas have higher viscosities because of their lower heat content and
enrichment with respect to silica. Felsic magmas are generated by the partial
melting of the more siliceous upper portion of water-saturated oceanic crust
(more siliceous because of the thick sedimentary cover it carries) where it is
subducted at convergent plate boundaries and by assimilation-melting of
siliceous, water-rich, continental crust into the magma derived from partial
melting of mafic oceanic crust and asthenosphere as it rises toward the surface.
54. Intermediate magma:
During oceanic-oceanic plate
collisions, a basic magma rises
through the overlying oceanic plate
and is little changed by assimilation-
melting (the original mafic magma
simply assimilates more mafic material
on its way upward); volcanic eruptions
on the sea floor form island chains
called island arcs. Volcanism is
initially mafic in composition, but as
time progresses and the volcanic arc
ages and is subject to erosion
(producing sediment that accumulates
in the subduction zone), newer
magmas become increasingly silicic
and become intermediate. During
oceanic-continental collisions, the
generally mafic magma rises through
felsic continental lithosphere to build a
volcanic arc on the continental
margin. Assimilation-melting of the
overlying felsic continental plate
produces intermediate magma. oceanic-continental collisions
55.
56.
57.
58.
59.
60.
61.
62.
63. Types of Granites
Mineralogically:
Essential minerals - Quartz , Feldspar
Accessory minerals – Biotite, muscovite,
amphibole.
Other accessories are zircon, apatite,
ilmenite, magnetite, sphene, pyrite etc.
Texturally:
Medium to coarse grained crystalline rock
generally exhibiting Hypidiomorphic
texture and Intergrowth textures (perthite,
Antiperthite, Myrmekite, Graphic, Granophyric,
rapakivi).
The granites could be classified based on
mineralogy, geochemistry and tectonic
emplacement:
Mineralogical classifications (IUGS
classification)
Chemical classification (alumina saturation,
S-I-A-M classification etc.)
Tectonic classification (Based on plate
tectonic setting)
65. Classification based on Chemical composition
Alumina saturation classes based on the molar proportions of Al2
O3
/(CaO+Na2
O+K2
O)
(“A/CNK”) after Shand (1927).
66. S-type Granitoid
Derived due to partial melting of
sedimentary and metasedimentary rock.
more common in collision zones.
Peraluminous granites [i.e., Al2O3 > (Na2O
+ K2O+CaO)] and have Fe2O3/FeO ratio <
0.3.
characterised by muscovite, biotite and
marginally higher SiO2 contents
I-type Granitoid
Derived due to partial melting of igneous
proloith.
Derived from igneous or metaigneous rocks
of lower continental crust subjected to
partial melting due upwelling of mantle
material to higher levels.
Generally metaluminous granites,
expressed mineralogically by the absence of
peraluminous minerals like muscovite (with
exceptions) and have Fe2O3/FeO ratio > 0.3.
charecterised by presence of
hornblende/alkali amphiboles ± biotite.
Alphabetical Classification of Granites (SIAM classification)
67. M-type Granitoid
Derived due to fractional
crystallisation of basaltic
magma.
Relatively Plagioclase rich
(plagiogranite of ophiolite).
Associated with Gabbros
and Tonalites in the field.
Formed in subduction
zone.
A-type Granitoid
(anorogenic type)
emplaced in either within
plate anorogenic settings or
in the final stages of an
orogenic event.
High SiO2 (~73.81%)
High F contents (6000 to
8000 ppm)
Presence of fluorite is an
important characteristic of
A-type granites.
Ophiolite Sequence
68.
69. (S-Type)(M-Type)
Mountain building resulting
from compressive stresses
associated with subduction.
Magmatism
takes place
after the
main
orogenic
event.
(I-Type)
Magmatism within
plate or at a spreading
plate margin.
(A-Type)
Classification based on Tectonic emplacement
Granitoids occur in areas where the continental crust has been thickened by
orogeny, either continental arc subduction or collision.The majority of granitoids
are derived by crustal anatexis, however, mantle may also be involved. The mantle
contribution may range from that of a source of heat for crustal anatexis, or it may
be the source of material as well.
70. Ophiolite sequence
Ophilites are fragments of oceanic crust and upper mantle that have been uplifted
and emplaced on continental margins.
71.
72. Ophiolites consist of five distinct layers.
The first layer is the youngest and is primarily sediment
that was accumulated on the seafloor.
The second layer is pillow basalt. Pillow basalt is
characterized by large pillow. When erupting lava
encounters the cold sea water, the outside of the lava
immediately crystallizes, forming a thick crust. The
extremely hot lava still inside the blob, oozes out of the
crust and instantly crystallizes again.
The next layer consists of sheeted dikes. Sheeted dikes
form by rising magma within the earth's crust. As the
sheeted dikes cool fractures and cracks occur in the rock.
Gabbro underlains sheeted dikes and compositionally
similar to basalt. Isotropic (massive) gabbro, indicates
fractionation of magma chamber. Layered gabbro,
resulting from settling out of minerals from a magma
chamber.
The bottommost layer is peridotite, which is believed to
be mantle rock composition.
73. Dunite: more than 90% olivine, typically
with Mg/Fe ratio of about 9:1.
Wehrlite: olivine + clinopyroxene (Augite;
diopside).
Harzburgite: olivine + orthopyroxene
(enstatite),
Lherzolite: olivine + enstatite + diopside
74.
75. It is a process leading to
changes in mineralogy
and/or texture in a rock.
Metamorphism
The boundary between
diagenesis and
metamorphism defines by
noting the first occurrence of
a mineral that does not occur
as a detrital or diagenetic
mineral in surface sediments,
(e.g. chlorite, epidote,
lawsonite, laumontite, albite,
zeolite,…).
Formation of some of these
minerals requires a
temperature of at least 150-
200 °C or 1500 bars or depth
of about 5 km under normal
geothermal conditions. The
upper limit of metamorphism
is defined as the beginning of
appreciable melting.
76. Chemically Active Fluids (ion
transport): In some metamorphic
settings, new materials are
introduced by the action of
hydrothermal solutions (hot water
with dissolved ions). Many metallic
ore deposits form in this way.
Pressure (measured in bars - 1 kb
is approximately each 3 km depth).
Pressure changes both a rock's
mineralogy and its texture.
Pressure comes in different
varieties; confining pressure,
directed pressure (or stress), burial
pressure and fluid pressure.
Heat is the most important source
of energy allowing the formation of
new and more stable mineral and
textural reconstruction and
recrystallization during
metamorphism.
Agents of Metamorphism
77.
78. Type of metamorphism
1- Contact metamorphism occurs
when magma invades cooler rock.
Here, a zone of alteration called an
aureole (or halo) forms around the
emplaced magma. These large
aureoles often consist of distinct
zones of metamorphism. Near the
magma body, high temperature
minerals such as garnet may form,
whereas farther away such low-
grade minerals as chlorite are
produced. Contact metamorphism
produces a zone of alteration called
an aureole around an intrusive
igneous body. Shales baked by
igneous contact form very hard fine-
grained rocks called HORNFELS.
Calcareous rocks (dirty limestones)
when subject to contact
metamorphism an alteration by hot
fluids produce rocks called SKARNS.
Pyrometamorphism: Very high
temperatures at very low pressures,
generated by a volcanic or
subvolcanic body.
79. 2- Metamorphism along Fault
Zones is known as dynamic
metamorphism. In some cases, rock
may even be milled into very fine
components. The result is a loosely
coherent rock called fault breccia
that is composed of broken and
crushed rock fragments. This type
of localized metamorphism, which
involves purely mechanical forces
that pulverize individual mineral
grains, is called cataclastic
metamorphism.
Much of the intense deformation
associated with fault zones occurs
at great depth. In this environment
the rocks deform by ductile flow,
which generates elongated grains
that often give the rock a foliated or
lineated appearance. Rocks formed
in this manner are termed
mylonites.
80. 3- Regional Metamorphism. The
metamorphic rock produced
during regional metamorphism
are associated with mountain
building (orogenic metamorphism
– convergent plate boundaries).
During these dynamic events,
large segments of Earth's crust
are intensely squeezed and
become highly deformed. As the
rocks are folded and faulted, the
crust is shortened and thickened,
like a rumpled carpet. This general
thickening of the crust results in
terrains that are lifted high above
sea level.
In regional metamorphism, there
usually exists a gradation in
intensity. As we shift from areas
of low-grade metamorphism to
areas of high grade
metamorphism, changes in
mineralogy and rock texture can
be observed.
81.
82.
83.
84.
85.
86. 4- Burial metamorphism
Metamorphic effects attributed
to increased pressure and
temperature due to burial.
Range from diagenesis to the
formation of zeolites, prehnite,
pumpellyite, laumontite, etc.
Diagenesis and lithification
start when rocks reach several
kilometers depth. Continued
burial leads to low grade burial
metamorphism. It is common
for sedimentary structures in
the unaltered rocks to remain
in the metamorphosed rocks,
indicating relatively little
recrystallization. This style of
metamorphism grades into
regional metamorphism with
increasing pressure and
temperature. We find it in deep
sedimentary basins.
87. 5- High-pressure low- temperature
metamorphism: This metamorphism
is associated with subduction zones.
It is called high pressure/low
temperature metamorphism where the
subducting plates has been cooled by
interaction with seawater.
6- Hydrothermal metamorphism:
(caused by hot H2O-rich fluids and
usually involving metasomatism). This
style of metamorphism is
distinguished by high fluid content
and changes in rock composition. It
occurs when hot water percolates (or
convects) through rock. This happens
around plutons and in association
with underwater volcanism. Pressures
are usually low and temperatures
moderate. By dissolving components
that are least compatible within the
rocks, hydrothermal metamorphism
can produce very exotic deposits.
Sulfides and massive ore bodies are
associated with it.
88. 7- Ocean-Floor
Metamorphism: affects
the oceanic crust at
ocean ridge spreading
centers. May be
considered another
example of
hydrothermal
metamorphism. Highly
altered chlorite-quartz
rocks- distinctive high-
Mg, low-Ca
composition.
Metamorphic rocks
exhibit considerable
metasomatic
alteration, notably loss
of Ca and Si and gain
of Mg and Na. These
changes can be
correlated with
exchange between
basalt and hot
seawater
89.
90.
91. Metamorphic Facies
A metamorphic facies includes rocks of any chemical composition and hence of
widely varying mineralogical composition, which have reached chemical
equilibrium during metamorphism under a particular set of physical conditions.
92.
93. Facies of Low Pressure
1) Albite-epidote hornfels
facies,
2) Hornblende hornfels
facies,
3) Pyroxene hornfels
facies, and
4) Sanidinite facies.
Facies of Medium to
High Pressure
1) Zeolite facies,
2) Prehnite-pumpellyite
metagreywacke facies,
3) Greenschist facies,
4) Amphibolite facies, and
5) Granulite facies.
Facies of Very High
Pressure
1) Glaucophane-lawsonite
schist facies.
2) Eclogite facies.
94.
95.
96.
97. Convergent Plate Margin
At all three types of convergent boundary
(ocean-ocean, ocean-continent, continent-
continent), high stresses, high deposition
rates and volcanism can be found.
Amphibolite to granulite facies are found
within the cores of mountain belts.
Greenschists occur at shallower depths
within the belts. Blueschists are produced
by the rapid subduction of sediments and
oceanic crust where high pressures can
be reached before temperatures within the
subducted crust can be rised.
Eclogite facies are reached within the
subducting crust when it reaches depths
of 20 to 25 km. Hornfels are found in
contact aureoles around shallow
intrusions where hot magma heats the
surrounding rocks.
Plate Tectonic Settings of Metamorphism
98. The uplift of mountains results in regional metamorphism. Baking of "country"
rock by igneous intrusions produces Contact metamorphism. Faulting of highly
stressed crustal rocks results in Cataclastic metamorphism. Rapid sedimentation
and subsidence offshore produces Burial metamorphism. Lastly, Zeolite facies
metamorphism occurs within the accretionary prism located arc ward of the
trench.
105. Divergent Plate Margin
A unique form of metamorphism occurs at divergent plate boundaries. New plate
is created by the upwelling of hot mantle. Partial melting produces new oceanic
crust through which water percolates, or convects, and is heated. Where it exits
the rock, water temperatures can be as high 450 °C, and are commonly as high as
350 °C (high water pressure at the sea floor prevents boiling). As the heated water
passes through the fresh basalt, it leaches out silica, iron, sulfur, manganese,
copper and zinc. The basalt incorporates magnesium and sodium from the water,
altering its composition and mineralogy.