The document provides information about the structure and composition of Earth's interior. It discusses how scientists have studied the interior without direct exploration by using seismic waves from earthquakes. The Earth has three main layers - the crust, mantle, and core. The crust and upper mantle form tectonic plates that move over the plastic mantle. The inner core is solid iron and nickel while the outer core is liquid, which generates the planet's magnetic field.
Geography class 11(Fundamentals of Physical Geography) Shivam Kapri
This file is made form NCERT class 11 book titled "Fundamental of Physical Geography". Will be of help to students and for competitive exam preparations.
Geography class 11(Fundamentals of Physical Geography) Shivam Kapri
This file is made form NCERT class 11 book titled "Fundamental of Physical Geography". Will be of help to students and for competitive exam preparations.
The Habitability of PlanetsMarch 28, 20201 Background.docxrtodd33
The Habitability of Planets
March 28, 2020
1 Background
The presence of liquid water is considered to be a prerequisite for life as we know it, which
makes looking for water a practical way to begin our search for life beyond Earth. For water
to exist on the surface of a planet, the planet must have the right temperature on its surface.
The main driving force behind the surface temperature of any planet is the light it receives
from its parent star. Around every star there is a region where the planet will receive just
the right amount of light to give it temperatures that are conducive to liquid water - this
region is call the star’s Habitable Zone. The orbit of the Earth currently falls within the
Habitable Zone of our Sun.
2 The Habitability of the Earth
To begin, load up the Habitable Zone simulator written by the University of Nebraska by
entering the following URL in the address bar of your web browsers:
http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html
The flash simulator will show you a visual diagram of the solar system in the top panel,
a set of simulation settings in the middle panel, and a timeline of the habitability of the
Earth in the bottom panel. To run the simulation, click the run in the bottom panel. This
button immediately becomes a pause button which will allow you to pause the simulation
at any time. To restart the simulation, press the restart button at the very top of the
simulation.
The blue region marked on the diagram is the Habitable Zone around our Sun. Notice
how there is both an inner edge and an outer edge - the planets interior to the habitable
zone are too hot to support liquid water, while the planets exterior to it are too cold.
1) The simulation is currently set to zero-age - this is the Solar System as it was when
it first formed, 5 billion years ago. Which planets were in the Habitable Zone at this time?
1
http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html
2) Press the start button and watch the Habitable Zone change with time. Pause the
simulation when it reaches an age of 5 billion years (you can keep track of the time by looking
at the timeline marker in the bottom panel). This is the Solar System as it is today - which
planets are in the Habitable Zone now?
3) Allow the simulation to run until the Earth is no longer in the Habitable Zone. At
what age does this happen? How long from now until this happens? You can use the timeline
bar in the bottom panel to determine your answers. .
4) After the Earth is no longer within the Habitable Zone, what do you think the condi-
tions on Earth will be like?
5) Resume the simulation and let it run until the end. Which planets other than the
Earth fell within the Habitable Zone at any point during the Sun’s life?
6) If you had to choose planets of our Solar System for future colonization based on their
future habitability, which would you choose, and why?
3 The Habitability Different Kinds .
The exact knowledge about the interior on the earth still remains an enigma.
Knowledge of the structure, composition, and the process going on within it would currently help scientists answer questions regarding crustal motion, earth quakes, the volcanic eruptions and the origins of the continents and of the earth itself. As the earth gradually solidified, heavier elements slowly sank towards the centre and lighter elements slowly moved upwards to the surface concentrating in the earth’s crust.
Earth’s interior is arranged roughly in concentric layers, each one distinct either in chemical composition or temperature with heat radiating outward from the centre by conduction and then by physical convection in the more plastic levels nearer the surface.
The Habitability of PlanetsMarch 28, 20201 Background.docxrtodd33
The Habitability of Planets
March 28, 2020
1 Background
The presence of liquid water is considered to be a prerequisite for life as we know it, which
makes looking for water a practical way to begin our search for life beyond Earth. For water
to exist on the surface of a planet, the planet must have the right temperature on its surface.
The main driving force behind the surface temperature of any planet is the light it receives
from its parent star. Around every star there is a region where the planet will receive just
the right amount of light to give it temperatures that are conducive to liquid water - this
region is call the star’s Habitable Zone. The orbit of the Earth currently falls within the
Habitable Zone of our Sun.
2 The Habitability of the Earth
To begin, load up the Habitable Zone simulator written by the University of Nebraska by
entering the following URL in the address bar of your web browsers:
http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html
The flash simulator will show you a visual diagram of the solar system in the top panel,
a set of simulation settings in the middle panel, and a timeline of the habitability of the
Earth in the bottom panel. To run the simulation, click the run in the bottom panel. This
button immediately becomes a pause button which will allow you to pause the simulation
at any time. To restart the simulation, press the restart button at the very top of the
simulation.
The blue region marked on the diagram is the Habitable Zone around our Sun. Notice
how there is both an inner edge and an outer edge - the planets interior to the habitable
zone are too hot to support liquid water, while the planets exterior to it are too cold.
1) The simulation is currently set to zero-age - this is the Solar System as it was when
it first formed, 5 billion years ago. Which planets were in the Habitable Zone at this time?
1
http://astro.unl.edu/naap/habitablezones/animations/stellarHabitableZone.html
2) Press the start button and watch the Habitable Zone change with time. Pause the
simulation when it reaches an age of 5 billion years (you can keep track of the time by looking
at the timeline marker in the bottom panel). This is the Solar System as it is today - which
planets are in the Habitable Zone now?
3) Allow the simulation to run until the Earth is no longer in the Habitable Zone. At
what age does this happen? How long from now until this happens? You can use the timeline
bar in the bottom panel to determine your answers. .
4) After the Earth is no longer within the Habitable Zone, what do you think the condi-
tions on Earth will be like?
5) Resume the simulation and let it run until the end. Which planets other than the
Earth fell within the Habitable Zone at any point during the Sun’s life?
6) If you had to choose planets of our Solar System for future colonization based on their
future habitability, which would you choose, and why?
3 The Habitability Different Kinds .
The exact knowledge about the interior on the earth still remains an enigma.
Knowledge of the structure, composition, and the process going on within it would currently help scientists answer questions regarding crustal motion, earth quakes, the volcanic eruptions and the origins of the continents and of the earth itself. As the earth gradually solidified, heavier elements slowly sank towards the centre and lighter elements slowly moved upwards to the surface concentrating in the earth’s crust.
Earth’s interior is arranged roughly in concentric layers, each one distinct either in chemical composition or temperature with heat radiating outward from the centre by conduction and then by physical convection in the more plastic levels nearer the surface.
Operation “Blue Star” is the only event in the history of Independent India where the state went into war with its own people. Even after about 40 years it is not clear if it was culmination of states anger over people of the region, a political game of power or start of dictatorial chapter in the democratic setup.
The people of Punjab felt alienated from main stream due to denial of their just demands during a long democratic struggle since independence. As it happen all over the word, it led to militant struggle with great loss of lives of military, police and civilian personnel. Killing of Indira Gandhi and massacre of innocent Sikhs in Delhi and other India cities was also associated with this movement.
June 3, 2024 Anti-Semitism Letter Sent to MIT President Kornbluth and MIT Cor...Levi Shapiro
Letter from the Congress of the United States regarding Anti-Semitism sent June 3rd to MIT President Sally Kornbluth, MIT Corp Chair, Mark Gorenberg
Dear Dr. Kornbluth and Mr. Gorenberg,
The US House of Representatives is deeply concerned by ongoing and pervasive acts of antisemitic
harassment and intimidation at the Massachusetts Institute of Technology (MIT). Failing to act decisively to ensure a safe learning environment for all students would be a grave dereliction of your responsibilities as President of MIT and Chair of the MIT Corporation.
This Congress will not stand idly by and allow an environment hostile to Jewish students to persist. The House believes that your institution is in violation of Title VI of the Civil Rights Act, and the inability or
unwillingness to rectify this violation through action requires accountability.
Postsecondary education is a unique opportunity for students to learn and have their ideas and beliefs challenged. However, universities receiving hundreds of millions of federal funds annually have denied
students that opportunity and have been hijacked to become venues for the promotion of terrorism, antisemitic harassment and intimidation, unlawful encampments, and in some cases, assaults and riots.
The House of Representatives will not countenance the use of federal funds to indoctrinate students into hateful, antisemitic, anti-American supporters of terrorism. Investigations into campus antisemitism by the Committee on Education and the Workforce and the Committee on Ways and Means have been expanded into a Congress-wide probe across all relevant jurisdictions to address this national crisis. The undersigned Committees will conduct oversight into the use of federal funds at MIT and its learning environment under authorities granted to each Committee.
• The Committee on Education and the Workforce has been investigating your institution since December 7, 2023. The Committee has broad jurisdiction over postsecondary education, including its compliance with Title VI of the Civil Rights Act, campus safety concerns over disruptions to the learning environment, and the awarding of federal student aid under the Higher Education Act.
• The Committee on Oversight and Accountability is investigating the sources of funding and other support flowing to groups espousing pro-Hamas propaganda and engaged in antisemitic harassment and intimidation of students. The Committee on Oversight and Accountability is the principal oversight committee of the US House of Representatives and has broad authority to investigate “any matter” at “any time” under House Rule X.
• The Committee on Ways and Means has been investigating several universities since November 15, 2023, when the Committee held a hearing entitled From Ivory Towers to Dark Corners: Investigating the Nexus Between Antisemitism, Tax-Exempt Universities, and Terror Financing. The Committee followed the hearing with letters to those institutions on January 10, 202
Palestine last event orientationfvgnh .pptxRaedMohamed3
An EFL lesson about the current events in Palestine. It is intended to be for intermediate students who wish to increase their listening skills through a short lesson in power point.
Honest Reviews of Tim Han LMA Course Program.pptxtimhan337
Personal development courses are widely available today, with each one promising life-changing outcomes. Tim Han’s Life Mastery Achievers (LMA) Course has drawn a lot of interest. In addition to offering my frank assessment of Success Insider’s LMA Course, this piece examines the course’s effects via a variety of Tim Han LMA course reviews and Success Insider comments.
Acetabularia Information For Class 9 .docxvaibhavrinwa19
Acetabularia acetabulum is a single-celled green alga that in its vegetative state is morphologically differentiated into a basal rhizoid and an axially elongated stalk, which bears whorls of branching hairs. The single diploid nucleus resides in the rhizoid.
Synthetic Fiber Construction in lab .pptxPavel ( NSTU)
Synthetic fiber production is a fascinating and complex field that blends chemistry, engineering, and environmental science. By understanding these aspects, students can gain a comprehensive view of synthetic fiber production, its impact on society and the environment, and the potential for future innovations. Synthetic fibers play a crucial role in modern society, impacting various aspects of daily life, industry, and the environment. ynthetic fibers are integral to modern life, offering a range of benefits from cost-effectiveness and versatility to innovative applications and performance characteristics. While they pose environmental challenges, ongoing research and development aim to create more sustainable and eco-friendly alternatives. Understanding the importance of synthetic fibers helps in appreciating their role in the economy, industry, and daily life, while also emphasizing the need for sustainable practices and innovation.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
2. In Module 1, you have learned about
the different processes and landforms
along plate boundaries that slowly
shaped the Earth’s surface.
In Module 2, you will learn the
connection between these processes
with the internal structure and
mechanisms of our planet.
3. What to expect:
This module will help you
visualize and understand the
composition and structure of
the Earth’s interior.
4. It provides you scientific
knowledge that will help you
describe the different layers
of the Earth as well as
understand their
characteristics.
5. You will also learn concepts that
explain the physical changes that it
underwent in the past.
This module also consists of activities
that will help you develop your critical
thinking skills to have a deeper
understanding about the planet where
you live.
6. Key Questions:
1. How do the structure and composition of the
Earth cause geologic activities and physical
changes?
2. What are the possible causes of the
lithospheric plate movements?
3. What proves the movement of the tectonic
plates?
7. Studying the Earth’s Interior
Scientists tried to explore and
study the interior of the Earth.
Yet, until today, there are no
mechanical probes or actual
explorations done to totally
discover the deepest region of
the Earth.
8. How did they know?
The Earth is made up of three layers:
the crust, the mantle, and the core.
The study of these layers is mostly
done in the Earth’s crust since
mechanical probes are impossible
due to the tremendous heat and very
high pressure underneath the Earth’s
surface.
10. Activity 1A: Amazing Waves!
Objectives:
Define seismic waves scientifically.
Differentiate the different types of
seismic waves.
Recognize the importance of
seismic waves in the study of the
Earth’s interior.
11. Procedure: (1whole)
Construct your own organizer
that shows necessary information
and summarizes the concept
about seismic waves.
Answer Q1 and Q2.
12. Seismic Waves
Seismic waves from earthquakes are used to
analyze the composition and internal structure
of the Earth.
What are seismic
waves?
13. Seismic waves
Earthquake is a vibration of the
Earth produced by the rapid
release of energy.
This energy radiates in all
directions from the focus in the
form of waves called seismic
waves.
16. Surface Waves
can only travel through the surface of
the Earth
arrive after the main P and S waves
2 Types of Surface Waves
Love Waves
Rayleigh Waves
17. Love Wave
named after A.E.H. Love, a British
mathematician who worked out the
mathematical model for this kind of wave in
1911.
faster than Rayleigh wave
it moves the ground in a side-to-side
horizontal motion, like that of a snake’s
causing the ground to twist
cause the most damage to structures during
an earthquake.
19. Rayleigh Wave
named after John William Strutt, Lord
Rayleigh, who mathematically predicted the
existence of this kind of wave in 1885
wave rolls along the ground just like a wave
rolls across a lake or an ocean
up and down or side-to-side similar to the
direction of the wave’s movement
shaking felt from an earthquake
21. Body waves
can travel through the Earth’s
inner layers
they are used by scientists to
study the Earth’s interior
higher frequency than the
surface waves
23. P-waves (Primary)
is a pulse energy that
travels quickly through the
Earth and through liquids
travels faster than the S-
wave
it reaches a detector first
24. P-waves (Primary)
compressional waves, travel by
particles vibrating parallel to the
direction the wave travel
move backward and forward as they
are compressed and expanded
they travel through solids, liquids
and gases
25. S-waves (Secondary/Shear)
pulse energy that travels slower than
a P-wave through Earth and solids
Move as shear or transverse waves,
and force the ground to sway from
side to side, in rolling motion that
shakes the ground back and forth
perpendicular to the direction of the
waves
29. Propagation of Seismic Waves
Through Earth’s Interior
Longitudinal waves travel through both
solids and liquids.
Transverse waves travel through
solids only.
30.
31. Remember:
P-waves are detected on the other side
of the Earth opposite the focus.
A shadow zone from 103° to 142°
exists from P-waves
Since P-waves are detected until 103°,
disappear from 103° to 142°, then
reappear again, something inside the
Earth must be bending the P-waves
32. Remember:
existence of a shadow zone, according
to German seismologist Beno
Gutenberg (ɡuː t ən bɛʁk), could only be
explained if the Earth contained a core
composed of a material different from
that of the mantle causing the bending of
the P-waves
To honor him, mantle–core boundary is
called Gutenberg discontinuity
33. Remember:
From the epicenter, S-waves are detected
until 103°, from that point, S- waves are no
longer detected
S-waves do not travel all throughout the
Earth’s body
knowing the properties and characteristics of
S-waves (that it cannot travel through liquids),
and with the idea that P-waves are bent to
some degree, this portion must be made of
liquid, thus the outer core
34. Remember:
1936, the innermost layer of the Earth was
predicted by Inge Lehmann, a Danish
seismologist
discovered a new region of seismic reflection
within the core
Earth has a core within a core
35. Remember:
the outer part of the core is liquid based from the
production of an S wave shadow and the inner
part must be solid with a different density than
the rest of the surrounding material
size of the inner core was accurately calculated
through nuclear underground tests conducted in
Nevada.
echoes from seismic waves provided accurate
data in determining its size
36. Bring the ff. (by grp)
15g cornstarch
2 small cups
Medicine dropper
Stirring rod or spoon
37. Act. 1B. Simulating Plasticity
Procedure:
Put 15 g cornstarch into one of the
beakers. Put 10 ml water into the other
beaker.
Add one drop full of water to the
cornstarch. Stir the mixture.
How does the mixture react like; solid,
liquid or gas?
38. Continue to add water to the mixture,
one drop full at a time. Stir the
mixture after each addition.
Stop adding water when the mixture
becomes difficult to stir.
Pour the mixture into your hand.
Roll the mixture into a ball and press
it.
39. Answer the ff. questions
How does the mixture behave like?
How is the mixture of cornstarch and
water similar to the earth’s mantle?
How is it different from the earth’s
mantle?
How does the plasticity of the earth’s
mantle influence the movement of the
lithospheric plates?
40. Bring the ff: (by grp)
hardboiled egg/s
bread knife
used paper/newspaper
to work on
41. Activity 1C: Hard Boiled Earth
PROCEDURE:
1. Prepare the materials. (hardboiled
egg, bread knife, used paper to work
on)
2. Place used paper or newspaper on
your working area. Cut the egg into
halves using a knife or a cutter.
42. Procedure:
Using qualitative observation, describe the
parts of the egg from the outermost to the
innermost by completing the table. Write your
answer on a piece of paper/ short bond paper.
PARTS OF THE EGG DECSRIPTION
EQUIVALENT TO
THE EARTH’S
LAYER
DESCRIPTION
43. Procedure:
4. Draw the appearance of the cut hard-boiled egg.
5. Answer the ff.
A. How many layers does a hard-boiled egg have?
B. Which is the largest part? The thinnest?
C. Compare the parts of the egg to the model of the
earth.
D. Aside from the hard-boiled egg, what other things
can you compare to the earth’s interior layers?
44. OUR HOME PLANET, EARTH
Our Earth is about average among the
planets in the Solar System, in many
respects:
largest and most massive of the four terrestrial planets,
but smaller and less massive than the four giant, or
Jovian, planets
third in distance from the Sun among the four terrestrial
planets
has a moderately dense atmosphere; 90 times less
dense than that of Venus but 100 times denser than that of
Mars
45. OUR HOME PLANET, EARTH
Earth is also unique in many respects:
the only planet with liquid water on its
surface.
the only one having a significant (21%)
proportion of molecular oxygen
to our best current knowledge, the only
planet in the solar system having living
organisms
the only terrestrial planet having a
moderately strong magnetic field
the only terrestrial planet having a large
satellite
47. The Solid Earth
geology -the study of the structure, history,
and activity of the solid Earth, including its
interactions with the atmosphere,
hydrosphere, cryosphere, and biosphere
solid Earth contains four major zones: the
core (which is divided into inner and outer
zones), the (upper and lower) mantle, the
asthenosphere, and the lithosphere
48. The Solid Earth
the outer zones is not uniform and fixed
over the surface of the Earth, but shows
much variability with position and time.
The field of plate tectonics deals with this
spatial and temporal variability.
Geological phenomena such as
earthquakes, volcanoes, and continental
drift are accounted for by plate tectonics.
51. HW 4:
Describe the unique characteristics of
each interior layer of the earth. (10pts)
Bring: (by group)
Coloring materials
Pencil
Marker
52. Activity 2: Our Dynamic Earth
Objectives:
Describe the properties of
the layers of the Earth.
Tell the composition of the
layers of the Earth.
53. Did you know?
The deepest mine in the world, the
gold mine in South Africa, reaches a
depth of 3.8km.
But...
You would have to travel more than
1,600 times that distance-over
6000km-to reach the earth’s center.
59. The Crust
thinnest and the outermost
layer of the Earth that extends
from the surface to about 32
kilometers below
Continental
Oceanic
60. Stanley, 1989, p. 14
Continental
Stanley, 1989, p. 14
Continental
Root
Moho
Oceanic
Lithosphere
Asthenosphere
61. Continental
mainly made up of silicon, oxygen,
aluminum, calcium, sodium, and
potassium
mostly 35-40 kilometers
found under land masses
made of less dense rocks such as
granite
62. Oceanic
oceanic crust is around 7-10
kilometers thick which its average
thickness is 8 kilometers.
found under the ocean floor
made of dense rocks such as basalt
heavier than the continental crust.
63. The Crust: Continental
• GRANITE -crystalline
igneous rock
composed primarily of
quartz and feldspar.
• forms from slowly
cooling magma that
is subjected to
extreme pressures
deep beneath the
earth's.
64. The Crust: Oceanic
• BASALT -volcanic rock
• forms from lava flows along
mid-ocean ridges and also in
igneous intrusions such as
dikes and sills.
• Columnar jointing, pictured
here at Devil's Tower,
Wyoming, occurs when
molten basalt cracks as it
cools, producing separate,
polygonal fractures on the
surface of the rock.
66. Moho Discontinuity
While studying the speed of
earthquake waves, Croatian
geophysicist Andrija Mohorovičić
discovers a boundary between
Earth's crust and mantle, which
becomes known as the Mohorovičić,
or Moho, Discontinuity.
67. The Mantle
Beneath the crust is the mantle
extends to about 2900 kilometers from the
Earth’s surface
about 80% of the Earth’s total volume
about 68% of its total mass
mainly made up of silicate rocks
and contrary to common belief, is solid, since
both S-waves and P-waves pass through it
68. The Mantle
mostly made of the elements silicon, oxygen,
iron and magnesium
lower part of the mantle consists of more iron
than the upper part
lower mantle is denser than the upper portion
temperature and the pressure increase with
depth
high temperature and pressure in the mantle
allows the solid rock to flow slowly
69. Remember:
The ability of the asthenosphere to
flow slowly is termed as plasticity.
crust and the uppermost part of
the mantle form a relatively cool,
outermost rigid shell called
lithosphere (Gk.lithos means
“stone”) and is about 50 to 100
kilometers thick
70. Remember:
Beneath the lithosphere lies the soft, weak layer
known as the asthenosphere (Gk. asthenes
means “weak”) made of hot molten material,
about 300 – 800o C
upper 150 kilometers has a temperature enough
to facilitate a small amount of melting, and make it
capable to flow
facilitates the movement of the lithospheric plates
lithosphere, with the continents on top of it, is
being carried by the flowing asthenosphere.
73. Outer Core
2900 kilometers below the Earth’s
surface
2250 kilometers thick
made up of iron and nickel
temperature reaches up to 2000oC at
this very high temperature, iron and
nickel melt
74. Outer Core
Aside from seismic data analysis,
the Earth’s magnetic field
strengthens the idea that the
Earth’s outer core is molten/liquid
mainly made up of iron and nickel
moving around the solid inner
core, creating Earth’s magnetism
75. The Inner Core
made up of solid iron and nickel and has a
radius of 1300 kilometers
about 5000oC
extreme temperature could have molten the
iron and nickel but it is believed to have
solidified as a result of pressure freezing,
which is common to liquids subjected under
tremendous pressure
76. The Inner Core
Aside from the fact that the Earth has a
magnetic field and that it must be iron or
other materials which are magnetic in nature,
the inner core must have a density that is
about 14 times that of water.
Average crustal rocks with densities 2.8
times that of water could not have the
density calculated for the core.
So iron, which is three times denser than
crustal rocks, meets the required density.
77. Clues that the inner core and the outer core
are made up of iron
Iron and nickel are both dense and
magnetic.
overall density of the earth is much
higher than the density of the
rocks in the crust
suggests that the inside must be
made up of something denser than
rocks
78. Clues that the inner core and the outer
core are made up of iron
Meteorite analysis have revealed that the
most common type is chondrite.
Chondrite contains iron, silicon,
magnesium and oxygen; some contains
nickel.
The whole earth and the meteorite roughly
have the same density, thus the Earth’s
mantle rock and a meteorite minus its iron,
have the same density.
79. HW5
Write a short story that describes the
most exciting part of your own
imaginary journey to Earth’s center.
Bring the ff. (by group)
scissors
old magazines
brown envelope