This document provides information about the formation and composition of planet Earth and the solar system. It discusses:
1) How Earth is uniquely suited to support life due to factors like its distance from the sun, size, atmosphere, and rotation.
2) The processes that led to the formation of elements, including nuclear fusion and radioactive decay. Hydrogen is the most abundant element in the universe.
3) How the Earth differentiated into layers with different compositions - a crust, mantle, and core. The crust also differentiates into continental and oceanic crust with different thicknesses, densities, and compositions.
Origin and Abundance of elements in the Solar system and in the Earth and its...AkshayRaut51
Definition of Elements and atom
Origin of Universe
Theories of origin of Solar system and Earth
Chemical Composition of Planets
Chemical Composition of Earth
Chemical composition of Meteorites
Abundance of Elements
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the Earth and its Subsystems (The Four Spheres).
Origin and Abundance of elements in the Solar system and in the Earth and its...AkshayRaut51
Definition of Elements and atom
Origin of Universe
Theories of origin of Solar system and Earth
Chemical Composition of Planets
Chemical Composition of Earth
Chemical composition of Meteorites
Abundance of Elements
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the Earth and its Subsystems (The Four Spheres).
This article presents how planet Earth was born, how it operates and how it is protected from threats coming from outer space. In addition to showing how the Earth operates as a dynamic system, it shows how our planet will disappear completely when the Sun migrates out of Earth's orbit in about 1 billion years.
Earth and Life Science - Theories on the Origin of the Solar SystemJuan Miguel Palero
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the origin of the Solar System.
• Earth, along with the other planets, is believed to have been born 4.5 billion years ago as a solidified cloud of dust and gases left over from the creation of the Sun.
• For perhaps 500 million years, the interior of Earth stayed solid and relatively cool, perhaps 2,000°F.
• The main ingredients were iron and silicates, with small amounts of other elements, some of them radioactive.
• As millions of years passed, energy released by radioactive decay—mostly of uranium, thorium, and potassium—gradually heated Earth, melting some of its constituents.
• The iron melted before the silicates, and, being heavier, sank toward the center.
• This forced up the silicates that it found there.
• After many years, the iron reached the center, almost 4,000 mi deep, and began to accumulate. No eyes were around at that time to view the turmoil that must have taken place on the face of Earth—gigantic heaves and bubblings on the surface, exploding volcanoes, and flowing lava covering everything in sight.
• Finally, the iron in the center accumulated as the core. Around it, a thin but fairly stable crust of solid rock formed as Earth cooled.
• Depressions in the crust were natural basins in which water, rising from the interior of the planet through volcanoes and fissures, collected to form the oceans. Slowly, Earth acquired its present appearance.
The Rare Earth hypothesis argues that the emergence of complex life on Earth required an improbable combination of astrophysical and geophysical events and circumstances.
Presented by Dr. Dennis Wilson
This article presents how planet Earth was born, how it operates and how it is protected from threats coming from outer space. In addition to showing how the Earth operates as a dynamic system, it shows how our planet will disappear completely when the Sun migrates out of Earth's orbit in about 1 billion years.
Earth and Life Science - Theories on the Origin of the Solar SystemJuan Miguel Palero
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the origin of the Solar System.
• Earth, along with the other planets, is believed to have been born 4.5 billion years ago as a solidified cloud of dust and gases left over from the creation of the Sun.
• For perhaps 500 million years, the interior of Earth stayed solid and relatively cool, perhaps 2,000°F.
• The main ingredients were iron and silicates, with small amounts of other elements, some of them radioactive.
• As millions of years passed, energy released by radioactive decay—mostly of uranium, thorium, and potassium—gradually heated Earth, melting some of its constituents.
• The iron melted before the silicates, and, being heavier, sank toward the center.
• This forced up the silicates that it found there.
• After many years, the iron reached the center, almost 4,000 mi deep, and began to accumulate. No eyes were around at that time to view the turmoil that must have taken place on the face of Earth—gigantic heaves and bubblings on the surface, exploding volcanoes, and flowing lava covering everything in sight.
• Finally, the iron in the center accumulated as the core. Around it, a thin but fairly stable crust of solid rock formed as Earth cooled.
• Depressions in the crust were natural basins in which water, rising from the interior of the planet through volcanoes and fissures, collected to form the oceans. Slowly, Earth acquired its present appearance.
The Rare Earth hypothesis argues that the emergence of complex life on Earth required an improbable combination of astrophysical and geophysical events and circumstances.
Presented by Dr. Dennis Wilson
Maybe too in-depth for most elementary students, but very good broad coverage for teacher background or more advanced students in elementary or middle school.
An image of each planet will be visible on individual slides.
Each slide will also describe the general composition, size, motion and relative position of each planet in the solar system.
Additional slides of planetary satellites, comets, and asteroids will be included.
Hyperlinks to additional slides and web sites will provide supplemental information.
Pages 18 -191.4 Earth as a SystemThe Earth System The Earth sy.docxbunyansaturnina
Pages 18 -19
1.4 Earth as a System
The Earth System The Earth system has a nearly endless array of subsystems in which matter is recycled over and over. One familiar loop or subsystem is the hydrologic cycle. It represents the unending circulation of Earth’s water among the hydrosphere, atmosphere, biosphere, and geosphere. Water enters the atmosphere through evaporation from Earth’s surface and transpiration from plants. Water vapor condenses in the atmosphere to form clouds, which in turn produce precipitation that falls back to Earth’s surface. Some of the rain that falls onto the land infiltrates (soaks in) to be taken up by plants or become groundwater, and some flows across the surface toward the ocean. Viewed over long time spans, the rocks of the geosphere are constantly forming, changing, and re-forming. The loop that involves the processes by which one rock changes to another is called the rock cycle and will be discussed at some length later in the chapter. The cycles of the Earth system are not independent of one another; to the contrary, these cycles come in contact and interact in many places. The parts of the Earth system are linked so that a change in one part can produce changes in any or all of the other parts. For example, when a volcano erupts, lava from Earth’s interior may flow out at the surface and block a nearby valley. This new obstruction influences the region’s drainage system by creating a lake or causing streams to change course. The large quantities of volcanic ash and gases that can be emitted during an eruption might be blown high into the atmosphere and influence the amount of solar energy that can reach Earth’s surface. The result could be a drop in air temperatures over the entire hemisphere. Where the surface is covered by lava flows or a thick layer of volcanic ash, existing soils are buried. This causes soil-forming processes to begin anew to transform the new surface material into soil (Figure 1.16). The soil that eventually forms will reflect the interactions among many parts of the Earth system—the volcanic parent material, the climate, and the impact of biological activity. Of course, there would also be significant changes in the biosphere. Some organisms and their habitats would be eliminated by the lava and ash, whereas new settings for life, such as a lake formed by a lava dam, would be created. The potential climate change could also impact sensitive life-forms. The Earth system is characterized by processes that vary on spatial scales from fractions of millimeters to thousands of kilometers. Time scales for Earth’s processes range from seconds to billions of years. As we learn about Earth, it becomes increasingly clear that despite significant separations in distance or time, many processes are connected, and a change in one component can influence the entire system. The Earth system is powered by energy from two sources. The Sun drives external processes that occur in the atmosphere, in the hy.
Artificial Reefs by Kuddle Life Foundation - May 2024punit537210
Situated in Pondicherry, India, Kuddle Life Foundation is a charitable, non-profit and non-governmental organization (NGO) dedicated to improving the living standards of coastal communities and simultaneously placing a strong emphasis on the protection of marine ecosystems.
One of the key areas we work in is Artificial Reefs. This presentation captures our journey so far and our learnings. We hope you get as excited about marine conservation and artificial reefs as we are.
Please visit our website: https://kuddlelife.org
Our Instagram channel:
@kuddlelifefoundation
Our Linkedin Page:
https://www.linkedin.com/company/kuddlelifefoundation/
and write to us if you have any questions:
info@kuddlelife.org
Willie Nelson Net Worth: A Journey Through Music, Movies, and Business Venturesgreendigital
Willie Nelson is a name that resonates within the world of music and entertainment. Known for his unique voice, and masterful guitar skills. and an extraordinary career spanning several decades. Nelson has become a legend in the country music scene. But, his influence extends far beyond the realm of music. with ventures in acting, writing, activism, and business. This comprehensive article delves into Willie Nelson net worth. exploring the various facets of his career that have contributed to his large fortune.
Follow us on: Pinterest
Introduction
Willie Nelson net worth is a testament to his enduring influence and success in many fields. Born on April 29, 1933, in Abbott, Texas. Nelson's journey from a humble beginning to becoming one of the most iconic figures in American music is nothing short of inspirational. His net worth, which estimated to be around $25 million as of 2024. reflects a career that is as diverse as it is prolific.
Early Life and Musical Beginnings
Humble Origins
Willie Hugh Nelson was born during the Great Depression. a time of significant economic hardship in the United States. Raised by his grandparents. Nelson found solace and inspiration in music from an early age. His grandmother taught him to play the guitar. setting the stage for what would become an illustrious career.
First Steps in Music
Nelson's initial foray into the music industry was fraught with challenges. He moved to Nashville, Tennessee, to pursue his dreams, but success did not come . Working as a songwriter, Nelson penned hits for other artists. which helped him gain a foothold in the competitive music scene. His songwriting skills contributed to his early earnings. laying the foundation for his net worth.
Rise to Stardom
Breakthrough Albums
The 1970s marked a turning point in Willie Nelson's career. His albums "Shotgun Willie" (1973), "Red Headed Stranger" (1975). and "Stardust" (1978) received critical acclaim and commercial success. These albums not only solidified his position in the country music genre. but also introduced his music to a broader audience. The success of these albums played a crucial role in boosting Willie Nelson net worth.
Iconic Songs
Willie Nelson net worth is also attributed to his extensive catalog of hit songs. Tracks like "Blue Eyes Crying in the Rain," "On the Road Again," and "Always on My Mind" have become timeless classics. These songs have not only earned Nelson large royalties but have also ensured his continued relevance in the music industry.
Acting and Film Career
Hollywood Ventures
In addition to his music career, Willie Nelson has also made a mark in Hollywood. His distinctive personality and on-screen presence have landed him roles in several films and television shows. Notable appearances include roles in "The Electric Horseman" (1979), "Honeysuckle Rose" (1980), and "Barbarosa" (1982). These acting gigs have added a significant amount to Willie Nelson net worth.
Television Appearances
Nelson's char
UNDERSTANDING WHAT GREEN WASHING IS!.pdfJulietMogola
Many companies today use green washing to lure the public into thinking they are conserving the environment but in real sense they are doing more harm. There have been such several cases from very big companies here in Kenya and also globally. This ranges from various sectors from manufacturing and goes to consumer products. Educating people on greenwashing will enable people to make better choices based on their analysis and not on what they see on marketing sites.
WRI’s brand new “Food Service Playbook for Promoting Sustainable Food Choices” gives food service operators the very latest strategies for creating dining environments that empower consumers to choose sustainable, plant-rich dishes. This research builds off our first guide for food service, now with industry experience and insights from nearly 350 academic trials.
Characterization and the Kinetics of drying at the drying oven and with micro...Open Access Research Paper
The objective of this work is to contribute to valorization de Nephelium lappaceum by the characterization of kinetics of drying of seeds of Nephelium lappaceum. The seeds were dehydrated until a constant mass respectively in a drying oven and a microwawe oven. The temperatures and the powers of drying are respectively: 50, 60 and 70°C and 140, 280 and 420 W. The results show that the curves of drying of seeds of Nephelium lappaceum do not present a phase of constant kinetics. The coefficients of diffusion vary between 2.09.10-8 to 2.98. 10-8m-2/s in the interval of 50°C at 70°C and between 4.83×10-07 at 9.04×10-07 m-8/s for the powers going of 140 W with 420 W the relation between Arrhenius and a value of energy of activation of 16.49 kJ. mol-1 expressed the effect of the temperature on effective diffusivity.
"Understanding the Carbon Cycle: Processes, Human Impacts, and Strategies for...MMariSelvam4
The carbon cycle is a critical component of Earth's environmental system, governing the movement and transformation of carbon through various reservoirs, including the atmosphere, oceans, soil, and living organisms. This complex cycle involves several key processes such as photosynthesis, respiration, decomposition, and carbon sequestration, each contributing to the regulation of carbon levels on the planet.
Human activities, particularly fossil fuel combustion and deforestation, have significantly altered the natural carbon cycle, leading to increased atmospheric carbon dioxide concentrations and driving climate change. Understanding the intricacies of the carbon cycle is essential for assessing the impacts of these changes and developing effective mitigation strategies.
By studying the carbon cycle, scientists can identify carbon sources and sinks, measure carbon fluxes, and predict future trends. This knowledge is crucial for crafting policies aimed at reducing carbon emissions, enhancing carbon storage, and promoting sustainable practices. The carbon cycle's interplay with climate systems, ecosystems, and human activities underscores its importance in maintaining a stable and healthy planet.
In-depth exploration of the carbon cycle reveals the delicate balance required to sustain life and the urgent need to address anthropogenic influences. Through research, education, and policy, we can work towards restoring equilibrium in the carbon cycle and ensuring a sustainable future for generations to come.
Micro RNA genes and their likely influence in rice (Oryza sativa L.) dynamic ...Open Access Research Paper
Micro RNAs (miRNAs) are small non-coding RNAs molecules having approximately 18-25 nucleotides, they are present in both plants and animals genomes. MiRNAs have diverse spatial expression patterns and regulate various developmental metabolisms, stress responses and other physiological processes. The dynamic gene expression playing major roles in phenotypic differences in organisms are believed to be controlled by miRNAs. Mutations in regions of regulatory factors, such as miRNA genes or transcription factors (TF) necessitated by dynamic environmental factors or pathogen infections, have tremendous effects on structure and expression of genes. The resultant novel gene products presents potential explanations for constant evolving desirable traits that have long been bred using conventional means, biotechnology or genetic engineering. Rice grain quality, yield, disease tolerance, climate-resilience and palatability properties are not exceptional to miRN Asmutations effects. There are new insights courtesy of high-throughput sequencing and improved proteomic techniques that organisms’ complexity and adaptations are highly contributed by miRNAs containing regulatory networks. This article aims to expound on how rice miRNAs could be driving evolution of traits and highlight the latest miRNA research progress. Moreover, the review accentuates miRNAs grey areas to be addressed and gives recommendations for further studies.
Diabetes is a rapidly and serious health problem in Pakistan. This chronic condition is associated with serious long-term complications, including higher risk of heart disease and stroke. Aggressive treatment of hypertension and hyperlipideamia can result in a substantial reduction in cardiovascular events in patients with diabetes 1. Consequently pharmacist-led diabetes cardiovascular risk (DCVR) clinics have been established in both primary and secondary care sites in NHS Lothian during the past five years. An audit of the pharmaceutical care delivery at the clinics was conducted in order to evaluate practice and to standardize the pharmacists’ documentation of outcomes. Pharmaceutical care issues (PCI) and patient details were collected both prospectively and retrospectively from three DCVR clinics. The PCI`s were categorized according to a triangularised system consisting of multiple categories. These were ‘checks’, ‘changes’ (‘change in drug therapy process’ and ‘change in drug therapy’), ‘drug therapy problems’ and ‘quality assurance descriptors’ (‘timer perspective’ and ‘degree of change’). A verified medication assessment tool (MAT) for patients with chronic cardiovascular disease was applied to the patients from one of the clinics. The tool was used to quantify PCI`s and pharmacist actions that were centered on implementing or enforcing clinical guideline standards. A database was developed to be used as an assessment tool and to standardize the documentation of achievement of outcomes. Feedback on the audit of the pharmaceutical care delivery and the database was received from the DCVR clinic pharmacist at a focus group meeting.
2. Earth
• Is the only planet which is certainly support life. Also
called Heaven planet.
• Is fortunate planet (how)? b/c:
I. Its distance from the sun makes the earth unique by
having water in a liquid form. This is b/c of the average
To is 14oc.
II. Its size: has enough gravitational force to hold the
atmosphere.
III. Composition of the atmosphere: O2, N2, CO2, & water
vapour.
IV. Daily rotation: 24hrs is balanced timing b/c it provides
optimum periods of light & darkness.
• One year takes 365 Earth days.
• Earth is close enough to the Sun to stay warm and yet far
enough away to keep cool.
• There is no wind on the earth moon.
3. Formation of the elements
Nuclear fusion: two atomic nuclei fuse or bond, is additive,
resulting in the creation of different elements by the addition
of protons to an atomic nucleus. It involves the release of
huge amounts of energy and it is the source of the Sun’s
power.
Radioactive decay: the spontaneous emission of particles or
energy over a given period of time and is one of the ways
where one element can become another by the expulsion of
protons. It takes place inside Earth.
The most abundant element in the universe is hydrogen, an
element formed by electron orbiting around a single proton.
• The sun itself, which makes up 98% of the total mass of the
solar system, consists of 71%H,27%He,and 2% of heavier
elements.
4. Abundance of elements
• The abundance of a chemical element measures
how relatively common (or rare) the element is, or
how much of the element is present in a given
environment by comparison to all other elements.
•
• Abundance may be variously measured by the
mass-fraction (the same as weight fraction), or
mole-fraction (fraction of atoms by numerical
count, or sometimes fraction of molecules in
gases), or by volume-fraction.
• In the universe as a whole, and in the atmospheres
of gas-giant planets such as Jupiter, the mass-
fraction abundances of hydrogen and helium are
about 74% and 23-25% respectively.
5. • However, since hydrogen is diatomic while
helium is not, in the conditions of Jupiter's outer
atmosphere, the molecular mole-fraction (fraction
of total gas molecules, or fraction of atmosphere
by volume) of hydrogen in the outer atmosphere
of Jupiter is about 86%, and for helium, 13%.
Abundance of elements in the Universe
Ten most common elements in the Milky Way
Galaxy, estimated spectroscopically.
6. z Element Mass fraction in ppm
1 Hydrogen 739,000
2 Helium 240,000
8 Oxygen 10,400
6 Carbon 4,600
10 Neon 1,340
26 Iron 1,090
7 Nitrogen 960
14 Silicon 650
12 Magnesium 580
16 Sulfur 440
7. Estimated abundances of the chemical elements in the Solar system.
•Hydrogen and helium are most common, from the Big Bang.
•The next three elements (Li, Be, B) are rare because they are poorly
synthesized in the Big Bang and also in stars.
•The two general trends in the remaining stellar-produced elements are:
•(1) an alternation of abundance in elements as they have even or odd
atomic numbers, and
•(2) a general decrease in abundance, as elements become heavier.
8. Chronology of planetary evolution
The time frame of the Solar System's formation
has been determined using radiometric dating.
Scientists estimate that the Solar System is
4.6 billion years old. The oldest known mineral
grains on Earth are approximately 4.4 billion years
old.
To estimate the age of the Solar System, scientists
use meteorite an age of (4.6 by).
9. The Solar System: origin and chemical
and evolution of solar system
• Our solar system consist of the Sun and the planets : Mercury, Venus,
Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto.
• The nine major planets including our earth and their moons are revolving
around the sun-anticlockwise rotation.
The first thing to notice is that the solar system is mostly empty space.
The planets are very small compared to the space between them. Even
the dots on the diagrams above are too big to be in proper scale with
respect to the sizes of the orbits.
10. Its includes: the satellites of the planets; numerous comets,
asteroids and meteoroids; and the interplanetary medium.
The sun is the richest source of electromagnetic energy
(mostly in the form of heat and light) in the solar system.
The whole solar system, together with the local stars visible
on a clear night, orbits the center of our home galaxy, a
spiral disk of 200 billion stars we call the Milky Way.
The Sun contains 99.85% of all the matter in the solar
system.
The planets, which condensed out of the same disk of
material that formed the Sun, contain only 0.135% of the
mass of the solar system.
11. Different hypotheses
• Based on observational facts cosmologists have
developed classes of hypothesis which try to explain
the origin of the earth. Some of them are:
1.Big Bang Theory
• It theorizes that a large quantity of nothing decided to
pack tightly together, and then explode outward into
hydrogen and helium.
• This gas is said to have flowed outward through
frictionless space (“frictionless,” so the out flowing
gas cannot stop or slow down) to eventually form
stars, galaxies, planets, and moons.
12. 2. Steady state hypothesis
• There is no change in the universe.
The origin of Solar System: is equivalent with the
origin of the Earth.
There are various hypothesis which explain the
origin of the solar system.
These are grouped into two as:-
A. Gradualistic Theories:
State that both the sun and the planets are formed
together.
B. Catastrophic Theories (Collision theory)
They are not formed at the same time.
13. 3.The nebular hypothesis.
State that there was a
slowly rotating H-
clouds called Nebula.
The gravitational force
contracts the H-cloud.
B/c of contraction
accelerate the rotation
as a result it has disk
shape.
B/c of gravitational
force the matter is
drifted toward the
center.
the center is denser.
the mass is
accumulated into a
14. • Nuclear fusion occurs when H2 is changed to He.
• During this energy is released as light and heat energy from
the proto –sun.
• The disk gradually cooled while it spun off various solid
compounds condensed out of the gas
– forming small grains by clumped together
– small chunks (Planetsimals) coalesced by the action of
gravity planets.
Some Evidences supporting This Theory
1. The planets revolve around the sun in the same direction.
2. All the equatorial section of the planets are on the same
plane (Co-planar)
3. The sun contains >99% of the mass of the Solar system. but
its momentum is <1% and the planets are vise versa.
4. Except Venus & Uranus all rotates counter clockwise.
Draw back of this theory:
1. There is rarer chance of condensed.
2. The chance of collision of the stars is such a very huge universe
is extremely small.
15. Differentiation of the Earth: bulk
composition of the Earth and chemical
composition of crust, mantle and core
Early Earth was composed of Si, Fe, Mg, O2, Al, and smaller
amounts of other chemical elements.
When the Earth under went heating, this homogeneous composition
disappeared, the result was differentiated planet, consisting of
concentric layers of differing composition and density.
Differentiation also responsible for the emission of gasses from the
interior of the Earth that eventually led to formation of the oceans
and the atmosphere.
The Earth’s atmosphere and hydrosphere are developed from
degassing (loss of gaseous elements such as carbon, hydrogen, and
oxygen).
16. Quiz
1.Why only planet earth support life?(2%)
2.List processes that lead(form) elements(1%)
3.Differentiate oceanic crust from continental
crust(2%)
17. • At present abundant gases are released during
volcanic eruptions and these are mainly composed
of water (77%), CO2 (12%), SO2 (7%), and N2
(3%) with minor amounts of H2, CO, S, Cl, and
Ar.
Geochemical composition of the Earth
Earth, being a dynamic system, it is continuously
undergoing change in
– Mechanical (plate tectonic-strength, elasticity, and,
viscosity).
– Chemical properties.
18. This properties do depend on
– Pressure
– Temperature
– State of stress
– Nature of the chemistry of the material.
• Chemical composition and mechanical properties
vary widely within the Earth.
• The Earth can be divided into two main parts:
1) Atmosphere: measured from the surface of the Earth upwards
to 150 km (any thing above this called space).
2) Solid Earth: measured from the surface of the Earth down
wards to the core.
19. • The internal structure of the earth consists of three parts:
– Crust, mantle, and core.
• Division between the crust and mantle is called the
Mohorovicic discontinuity (Moho).
• The boundary between the crust and mantle marks a
significant change in chemical composition.
• Two main hypotheses for what the Moho represents:
1) phase transition (from a gabbroic lower crust to an eclogitic
upper mantle).
2) chemical discontinuity (the widely accepted theory for the
Moho is that it represents a chemical change from intermediate
and mafic crustal rocks to an ultramafic mantle).
20. Chemical subdivision of the Earth
• The Earth consists of three concentric layers:
– Core, mantle, and crust
• This orderly divisions results from density differences
between the layers as a function of variations in:
– compositions,
– temperature,
– pressure.
A) Crust
is much thinner under oceans than under continents.
makes up only 0.5% of the Earth’s total mass.
21. can be divided into two main parts,
continental
oceanic.
Both differ in thickness, density, and compositions.
1) Continental crust
• Averages 35 km in thickness, but it ranges up to 60 km
under mountain ranges and up to 70-80 km in regions
of crustal duplication (Tibet, Himalayas).
• It has average density of 2.7 g/cm3
• Commonly referred to sialic (meaning that contains
considerable Si and Al).
22. • The oldest rocks preserved on the planet are found on
continents (except meteorites, which are often older).
• Continental crust can be divided into:
a) Stable continental regions (e.g., Precambrian cratons,
platforms of undeformed sediments on crystalline
basements)
• Thickness:35-45 km
• Density: 2.69 -2.74 gm/cm3 upper crust; 3.0 -3.25 gm/cm3
lower crust.
• Composition:
– upper crust (Sial): felsic igneous and metamorphic rocks.
» Average composition will be close to that of either a
mafic granodiorite or quartz diorite
– lower crust (Sima): anhydrous (no water)- quartz
andesite or andesite; hydrous-amphibolite or diorite.
23. b) Tectonically active regions (e.g. the Andes,
Himalayas)
• Thickness:55-70 km
• Composition: varies from region to region but may consist
of either mafic, amphibolites or ultramafic, mafic and felsic-
intermediate.
2) Oceanic crust
• It is thin (5-10 km; it is only 7 km thick in the deep ocean
basins)
• Denser than continental crust (3.0 g/cm3)
• Commonly referred to Sima (meaning that contains
considerable Si and Mg).
• Produced wherever hot mantle materials comes into contact
the surface of solid earth (produced at spreading centers).
24. • Consists of three layers of increasing velocity (P-wave
velocities) downwards
1. Layer 1: 1.6 to 2.5 km/s
2. Layer 2: 3.4 to 6.2 km/s
3. Layer 3: 6.4 to 7.0 km/s
– These difference reflect the differing origins of each
layer and their mechanical states.
• Sea water circulates into the cooling oceanic crust to depths
of 3 km, driven by the heat of the magma intrusion.
• The circulation is shown by the metamorphism and
serpentinization of the basalts and gabbros
25. • Oceanic crust can be divided into:
a) Ocean basins: water depth exceeds 4 km, layered and very uniform
and consists of three distinctive layers.
1. Layer 1: thickness of <1 km; deep water sediments in
various stages of lithifications (turning into rock),
foraminiferal ooze, chert, and mudstone.
2. Layer 2: thickness of 1.6-2 km; basalts and dolerites with
pillow lavas, dykes and sills (volcanic extrusive and
intrusive rocks)
3. Layer 3: thickness of 3-5.7 km; the main crustal layer;
dolerite, gabbro, and amphibolites (intrusive mafic rocks)
b) Mid-ocean ridges: in mid-ocean ridges (such as the Mid-Atlantic
Ridge),
1. Layer 1: absent
2. Layer 2: crops out the surface and is thicker than normal
3. Layer 3: thinner than normal and passes transitionally into
the upper mantle.
26. c) Island arcs: the structure beneath island arcs (such as the
Indonesian Arc) is very complex and the composition of the
crust in these region is very heterogeneous.
– The most rock types are in surface exposures are volcanic
andesites (from explosive volcanoes) and deep-sea
sediments.
B) Mantle
• is a thick layer between the Earth’s crust and core.
• comprises about 83% of the Earth’s volume.
• extends from 70 or 35 km to 2,900 km of depth.
• is less dense than the core (3.3-5.7 g/cm3).
• is thought to be composed largely of iron-rich silicate
minerals.
27. • subdivided into
1. upper mantle
2. transition zone
3. lower mantle
1) Upper Mantle
• is measured from the base of the crust down to 400 km.
• accounts for 10 % of the Earth's total mass.
• density 3.25-3.40 gm/cm3
• composition:
– plagioclase peridotite (e.g. olivine + pyroxene) (< 30 km
depth),
– spinel peridotite (30 km - 70 km depth),
– garnet peridotite (> 70 km depth)
28. • In tectonically active regions, eclogite (amphibole
+ garnet + Cpx) is a major component.
• composed of two main zones:
– an upper peridotite zone and
– an underlying primitive mantle or pyrolite zone
2) Transition Zone
• 400 - 1000 km below the Earth's surface.
• 17% of the Earth's total mass.
• the top of the transition zone is marked by phase
transformation
– olivine to a proto-spinel
– pyroxene to a garnet-structure
29. • there are a number of irregular seismic velocity changes.
– 680 km which is marked by the breakdown of olivine
into its constituent oxide components of periclase
(MgO) and stishovite (SiO2).
3) Lower Mantle
• 1000 - 2900 km below the Earth's surface.
• 41% of the Earth's total mass.
• most likely consists of mixed oxides of pyrolite
composition but with increased iron content.
30. C) Core
• is believed to be composed primarily of a nickel-iron alloy (along
with abundant platinum-group elements).
• is divided into two types –
1. liquid outer core (2900 - 5000 km)
2. solid inner core (5000 - 6370 km)
• has density of 10 to 13 g/cm3
• occupies about 16% of the Earth’s total volume.
• is believed to have a chemical composition similar to that of iron
meteorites (Fe- 90.6%; Ni- 7.9%; Co- 0.5% etc)
• There is a sharp but not very smooth boundary between mantle and
core known as Gutenberg discontinuity.