1. Guided Reading Questions
Chapter 6 Earth
Guided Reading Questions

2. 1. (6.1) Why is the Earth round? Is it perfectly spherical?
Gravity is the great leveler. Over millions of years, the force of gravity crushes and deforms rock, pulling high points down and rounding large bodies off. However, this shaping process is effective only if the body exceeds a critical size that depends on the object's composition. For bodies made of rock, the critical radius is about 350 kilometers. An object with a radius larger than this has strong enough gravity that it can pull itself into a sphere even if initially it was irregular.

3. 2. (6.1) What are some of the most common elements composing the Earth's crust, mantle and core?
Analysis of the surface rocks of the Earth shows that the most common elements in them are oxygen, silicon, aluminum, magnesium, and iron. Furthermore, silicon and oxygen usually occur together as silicates.

4. 3. (6. 2) How do we know that the Earth has a liquid core
3. (6.2) How do we know that the Earth has a liquid core? Why is the inner core solid even though it is hotter than the outer liquid core?
Seismic waves slightly compress rock or cause it to vibrate side to side. The speed of the waves depends on the properties of the material through which they move. A wave's speed can be determined by carefully timing its arrival at remote points of the world. From that speed, scientists can deduce a picture of the Earth's interior along the path of that wave. Thus, seismic waves allow us to “see” inside the Earth much as doctors use sound waves to “see” inside our bodies.

5. if a laboratory on the far side of the Earth from an earthquake detects P waves but no S waves, the seismic waves must have encountered a region of liquid on their way from the earthquake to the detecting station (fig. 6.7), an indication that the Earth has a liquid interior. Observations show precisely this effect, from which we infer that the Earth has a liquid core.

7. 4. (6.2) What are two explanations that scientists offer for why the interior of the Earth is hot? How hot is it?
*Scientists think that the Earth may have been born hot. According to this theory, the Earth formed from many smaller bodies drawn together by their mutual gravity. As each body hit the accumulating young Earth, the impact generated heat. You can demonstrate that impact generates heat by hitting a small piece of metal repeatedly with a hammer and then feeling the metal.
*the Earth generates heat much as a nuclear reactor does. All rock contains trace amounts of naturally occurring radioactive elements such as uranium. A radioactive element is one that breaks down into another element by ejecting a subatomic particle from its nucleus, a process called radioactive decay. Radioactive decay releases energy, generating heat.
*about 6500 K

8. 5. (6.3) How can scientists determine the age of the Earth?
One can find the age of a rock sample by measuring the amount of radioactive material it contains. As a rock ages, its radioactive atoms decay into so called daughter atoms. For example, uranium decays into lead, and radioactive potassium decays into calcium and the gas argon. The more daughter atoms a rock contains relative to the original number of radioactive atoms, the older the rock is. *The argon/potassium ratio…gives us the age of the rock sample…(The amount of argon compared to potassium in a sample of rock gives information about the rock's age.)

9. 6. (6.4) What is convection? What are some other examples of convection besides hot soup?
Heat in the Earth's interior, whether left over from our planet's birth or generated by radioactive decay, creates movement of the material inside the Earth. (circulating movement of a heated liquid or gas is called convection) Convection occurs in the Earth's mantle…a hot air balloon … Convection occurs because heated matter expands and becomes slightly less dense than the cooler material around it. As the hotter material flows upward, it carries heat along with it. Thus, convection not only causes motion but also carries heat.

10. 7. (6.4) What is the relation between rising and sinking material in the Earth's interior and subduction and rifting?
Deep within the Earth, hot molten material rises in great, slow plumes. When such a plume nears the crust, it spreads out and flows parallel to the surface below the crust. There, the hot material drags the surface layers, shifting and stretching the crust in a process called rifting. In other places the convection currents force one piece of crust to collide with another, driving one piece of crust beneath the other in a process called subduction. These two processes sculpt Earth's unique landscape. (A) Rifting may occur where rising material in the mantle nears a planet's surface. (B) Subduction builds mountains where material sinks back toward the interior of the Earth.

11. 8. (6. 4) On what plate of the crust are you located
8. (6.4) On what plate of the crust are you located? Which way is it taking you?
the North American… The continents can be seen to move up to about 10 centimeters per year relative to each other. Our world is literally changing beneath our feet, growing new crust at mid oceanic ridges and devouring it at subduction zones. But this devoured rock is not lost. As it is carried downward, it is heated, and eventually its lower density causes it to rise again toward the surface.

12. 9. (6.4) What is happening where one tectonic plate is smashing into another?
Where plates collide, the continental material buckles upward to form mountain ranges such as the Rockies and Andes along the western coasts of North and South America. The continents are made up of lower density kinds of rock, such as granite, that “float” above denser rock making up the ocean floor and still denser types of rock below the surface. Most of the rifts are found in the oceans, but in some places, stretching breaks the continental material apart.

13. 10. (6.5) What factors are thought to be responsible for the Earth's magnetic field?
Magnetic fields are generated by electric currents, either large scale currents or currents on thescale of atoms. The magnetic field of the Earth is generated by electric currents flowing in the Earth's molten iron core. Scientists are still unsure how these currents originate but hypothesize that they develop from a combination of rotational motion and convection. * Studies of the magnetic fields of other Solar System bodies support this view.

14. 11. (6.5) How is the aurora related to the Earth's magnetic field?
As the charged particles flow toward the magnetic poles, they generate electric currents in the upper atmosphere. These currents, circulating around the magnetic poles, drive electrons along the magnetic field lines. The moving electrons spiral around the field lines, colliding with molecules of nitrogen and oxygen. Such collisions excite atmospheric gases, lifting their electrons to higher energy orbitals. As the electrons drop back to lower orbitals, they emit the lovely light we see as the aurora. The exact process by which the aurora forms is still not completely certain, but there is no doubt that its beautiful streamers are shaped by the Earth's magnetic field.

15. 12. (6.5) How does the fact that the Earth has a magnetic field help provide evidence for the theory of plate tectonics?
Studies of the magnetic fields of other Solar System bodies support this view of convection. For example, bodies with weak or no magnetic fields, such as Mars and Venus, are either too small to have a large convecting core or rotate very slowly. On the other hand, bodies with large magnetic fields, such as Jupiter and Saturn, rotate very rapidly and have very hot cores. When molten rock cools, magnetic minerals within the rock align to the direction of the Earth's magnetic field much as a compass needle does. This leaves rocks slightly magnetic after they solidify, and the orientation of Earth's magnetic field at the time the lava solidified is frozen into them. By dating the rock on the ocean floor, geologists can determine how fast the crust has moved and how often the magnetic field has reversed.

16. 13. (6.6) What were the main components of the atmosphere when the Earth formed, and what are the main components today? How and why did they change?
The atmosphere of the Earth is primarily a mixture of nitrogen and oxygen. Nitrogen molecules make up about 78% of our atmosphere's gas and oxygen about 21%. The remaining 1% includes carbon dioxide, ozone, and water, gases crucial for protecting us and making life possible. our planet's ancient atmosphere probably contained far more methane (CH4) and ammonia (NH3) than it does now. Although these gases are still abundant in the giant planets such as Jupiter and Saturn, they have all but disappeared from our atmosphere, which is fortunate because both methane and ammonia are poisonous. Read about the theories in the book…

17. 14. (6.6) Explain how the greenhouse effect works and how it relates to global warming.
The transparency of the Earth's atmosphere to visible radiation allows sunlight to enter the atmosphere and reach the Earth's surface. The energy of the photons is absorbed by molecules in the surface and converted to heat. The warmed surface radiates infrared energy, but the atmosphere is not very transparent at infrared wavelengths. This reduces the heat loss and makes the surface warmer than it would be if the infrared energy could escape freely, a phenomenon known as the greenhouse effect. It is important to recognize that the greenhouse effect does not generate heat; rather, it limits the heat loss to space. The greenhouse effect therefore warms the Earth the same way a blanket warms you. The blanket doesn't make you generate more heat; it simply slows down the loss of heat already there.

18. 15. (6.6) What is ozone? Why is it important?
The oxygen in our atmosphere is important to us not only for breathing but also as a vitally protective blanket that shields us from harsh solar ultraviolet radiation. Some of that shielding is provided by O2 (the normal form of oxygen), but much of it comes from another molecular form of oxygen, O3, or ozone. Ozone is important because it is a strong absorber of ultraviolet radiation; without the ozone layer, solar ultraviolet radiation would pour into the lower atmosphere.

19. 16. (6. 7) What is the Coriolis effect
16. (6.7) What is the Coriolis effect? How does it affect life on Earth?
Ocean and air currents sweeping across a spinning planet like Earth are deflected from their original direction of motion. This phenomenon is called the Coriolis effect. The Coriolis effect deflects ocean currents to the right in the Northern Hemisphere, creating a clockwise oceanic circulation. It also creates atmospheric currents such as the trade winds. The trade winds form in response to the Sun's heating of equatorial air, which rises and expands, flowing away from the equator toward the poles at high elevations. However, before this air can reach the poles, it cools and sinks toward the surface and flows back toward the equator. As the air approaches the equator, the Coriolis force deflects it to the west (right in the North, left in the South), creating a steady surface wind that traders in sailing ships relied upon.

21. 17. (6.7) What is precession? What are some of its possible consequences?
As the Earth moves around the Sun over long periods of time, the direction in which its rotation axis points changes very slowly. This motion, similar to the wobble that occurs when a spinning coin or toy top begins to slow down, is called precession. That twisting makes the Earth's rotation axis slowly change direction, completing one swing in about 26,000 years….

23. Multiple choice D C B A

24. Multiple choice D A C B

25. Chapter 6
The Earth
Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

26. “Your present circumstances don’t determine where you can go; they merely determine where you start.”
- Nido Qubein

27. Our Home, The Earth
Earth’s beauty is revealed from space through blue seas, green jungles, red deserts, and white clouds.
From our detailed knowledge of Earth, astronomers hope to understand what properties shape other worlds
Earth is a dynamic planet with its surface and atmosphere having changed over its lifetime.
Slow and violent motions of the Earth arise from heat generated within the planet
Volcanic gases accumulate over billions of years creating an atmosphere conducive to life, which in turn together with water affects the air’s composition

28. Size and Shape of the Earth
In simple terms, the Earth is a huge, rocky sphere spinning in space and moving around the Sun at a speed of about 100 miles every few seconds
Earth also has a blanket of air and a magnetic field that protects the surface from the hazards of interplanetary space

29. Size and Shape of the Earth
The Earth is large enough for gravity to have shaped it into a sphere
More precisely, Earth’s spin makes its equator bulge into a shape referred to as an oblate spheroid – a result of inertia

30. Composition of the Earth
The most common elements of the Earth’s surface rocks are:
oxygen (45.5% by mass),
silicon (27.2%),
aluminum (8.3%),
iron (6.2%),
calcium (4.66%), and
magnesium (2.76%)
Silicon and oxygen usually occur together as silicates
Ordinary sand is the silicate mineral quartz and is nearly pure silicon dioxide

31. Density of the Earth
Density is a measure of how much material (mass) is packed into a given volume
Typical unit of density is grams per cubic centimeter
Water has a density of 1 g/cm3, ordinary surface rocks are
3 g/cm3, while iron is 8 g/cm3
(The typical density for a rock found on the surface of the Earth is less than the average density of the Earth overall.)
For a spherical object of mass M and radius R, its average density is given by
For Earth, this density is found to be 5.5 g/cm3
Consequently, the Earth’s interior (core) probably is iron (which is abundant in nature and high in density)
A rock has a density of 2 g/cm3. If another rock has twice as much mass but the same volume, its density must be 0.5g/cm3.
A spherical rock has a density of 3 g/cm3. If another rock has the same mass but is twice as wide, its density must be 3/8 g/cm3.

32. The Earth’s Interior
Earthquakes generate seismic waves that move through the Earth with speeds depending on the properties of the material through which they travel
These speeds are determined by timing the arrival of the waves at remote points on the Earth’s surface
A seismic “picture” is then generated of the Earth’s interior along the path of the wave

33. A Sonogram of the Earth!
This is the only way we have to probe the Earth’s interior!

34. Probing the Interior of the Earth
Seismic waves are of two types: S and P
P waves compress material and travel easily through liquid or solid
S waves move material perpendicular to the wave direction of travel and only propagate through solids

35. Interior Structure
Observations show P waves but no S waves at detecting stations on the opposite side of the Earth from the origin of an Earthquake
Þ the Earth has a liquid (outer) core!

36. Interior Structure of the Earth
A solid, low-density and thin crust made mainly of silicates
A hot, thick, not-quite-liquid mantle with silicates
The zones of the Earth is from the center outward, are solid core, liquid core, mantle, crust, atmosphere.
A liquid, outer core with a mixture of iron, nickel and perhaps sulfur (The outer core of the Earth extends out to a little over halfway to the surface of the Earth. The volume of the core is therefore about 1/8 the volume of the Earth.)
A solid, inner core of iron and nickel
*The most abundant element in the Earth's core is iron.

37. Layers of the Earth
The Earth is layered in such a fashion that the densest materials are at the center and the least dense at the surface – this is referred to as differentiation
Differentiation will occur in a mixture of heavy and light materials if these materials are liquid for a long enough time in a gravitational field
Consequently, the Earth must have been almost entirely liquid in the past
The Earth’s inner core is solid because it is under such high pressure (from overlying materials) that the temperature there is not high enough to liquefy it – this is not the case for the outer liquid core

38. Differentiation
Scientists refer to the Earth as a differentiated planet because the material in the interior of the Earth is arranged by density.

39. Temperature Inside the Earth
Heating the Earth’s Core
The estimated temperature of the Earth’s core is 6500K (The Earth's core is slightly hotter than the surface of the Sun.)
This high temperature is probably due to at least the following two causes:
Heat generation from the impact of small bodies that eventually formed the Earth by their mutual gravitation
The radioactive decay of radioactive elements that occur naturally in the mix of materials that made up the Earth

40. Temperature Inside the Earth
In either case, the thermal energy generated is trapped inside the Earth’s interior due to the long time it takes to move to the surface and escape

41. Age of the Earth Radioactive decay used to determine the Earth’s age
Radioactive atoms decay into daughter atoms
The more daughter atoms there are relative to the original radioactive atoms, the older the rock is...
The age of a rock determined by determining the ratio of argon to potassium.

42. Age of the Earth...some suggest...
Radioactive potassium has a half-life of 1.28 billion years and decays into argon, which is a gas that is trapped in the rock unless it melts
Assume rock has no argon when originally formed
Measuring the ratio of argon atoms to potassium atoms gives the age of the rock
This method gives a minimum age of the Earth as 4 billion years
Other considerations put the age at about 4.5 to 4.6 billion years

43. Motion in the Earth’s Interior
Heat generated by radioactive decay in the Earth creates movement of rock
This movement of material is called convection
Convection occurs because hotter material will be less dense than its cooler surroundings and consequently will rise while cooler material sinks

44. Convection Convection in the Earth’s interior
The crust and mantle are solid rock, although when heated, rock may develop convective motions
These convective motions are slow, but are the cause of: earthquakes, volcanoes, the Earth’s magnetic field, and perhaps the atmosphere itself

45. Plate Tectonics Rifting
Hot, molten material rises from deep in the Earth’s interior in great, slow plumes that work their way to the surface
Near the surface, these plumes spread and drag the surface layers from below
The crust stretches, spreads, and breaks the surface in a phenomenon called rifting

46. Subduction Subduction
Where cool material sinks, it may drag crustal pieces together buckling them upward into mountains
If one piece of crust slips under the other, the process is called subduction
Mountains and earthquakes are common in regions where subduction occurs.

47. Plate Tectonics
Rifting and subduction are the dominant forces that sculpt the landscape – they may also trigger earthquakes and volcanoes

48. Plate Tectonics
The shifting of large blocks of the Earth’s surface is called plate tectonics
Early researchers noted that South America and Africa appeared to fit together and that the two continents shared similar fossils
It was later proposed (1912) that all of the continents were once a single supercontinent called Pangea
The Earth’s surface is continually building up and breaking down over time scales of millions of years
The Earth's plates are moving due to tectonic motion a few centimeters per year

49. Continental Drift

50. Continental Plates

51. The Earth’s Magnetic Field
Magnetic forces are communicated by a magnetic field – direct physical contact is not necessary to transmit magnetic forces
Magnetic fields are depicted in diagrams by magnetic lines of force
Each line represents the direction a compass would point
Density of lines indicate strength of field

52. The Earth’s Magnetic Field
Magnetic fields also have polarity – a direction from a north magnetic pole to a south magnetic pole
Magnetic fields are generated either by large-scale currents or currents on an atomic scale

53. Origin of the Earth’s Magnetic Field
The magnetic field of the Earth is generated by currents flowing in its molten iron core
The currents are believed to be caused by rotational motion and convection (magnetic dynamo) (If Earth did not spin, the magnetic field around it would not exist.)
The Earth’s geographic poles and magnetic poles do not coincide
Both the position and strength of the poles change slightly from year to year, even reversing their polarity every 10,000 years or so

54. Magnetic Effects in the Upper Atmosphere
Earth’s magnetic field screens the planet from charged particles emitted from the Sun
The Earth’s magnetic field deflects the charged particles into spiral trajectories and slows them down

55. The Magnetosphere
Region of the Earth’s environment where the Earth’s magnetic field affects particle motion is called the magnetosphere
Within the magnetosphere charged particles are trapped in two doughnut shaped rings that encircle the Earth and are called the Van Allen radiation belts

56. Aurora
As the charged solar particles stream past Earth, they generate electrical currents in the upper atmosphere
These currents collide with and excite molecules
As the molecules de-excite, light photons are given off resulting in aurora

57. The Earth’s Atmosphere
Veil of gases around Earth constitutes its atmosphere
Relative to other planetary atmospheres, the Earth’s atmosphere is unique
However, studying the Earth’s atmosphere can tell us about atmospheres in general

58. Structure of the Earth’s Atmosphere
Atmosphere extends to hundreds of kilometers becoming very tenuous at high altitudes
The atmosphere becomes less dense with increasing altitude
Half the mass of the atmosphere is within the first 4 kilometers
The atmosphere eventually merges with the vacuum of interplanetary space

59. Composition of the Earth’s Atmosphere
The Earth’s atmosphere is primarily nitrogen (78.08% by number) and oxygen (20.95% by number)
The remaining gases in the atmosphere (about 1%) include: carbon dioxide, ozone, water, and argon, the first three of which are important for life
This composition is unique relative to the carbon dioxide atmospheres of Mars and Venus and the hydrogen atmospheres of the outer large planets

60. The Greenhouse Effect
Visible light reaches the Earth’s surface and is converted to heat
As a result, the surface radiates infrared energy, which is trapped by the atmosphere at infrared wavelengths
This reduces the rate of heat loss and makes the surface hotter than it would be otherwise
Water vapor in the atmosphere can cause a greenhouse effect.

61. Global Warming
Tracers of the Earth’s temperature and atmospheric carbon dioxide content for the past 800,000 years show a strong correlation.
Many scientists are concerned that humans are adding so much carbon dioxide to the atmosphere that we might trap so much heat that Earth’s temperature will climb—a process called global warming.

62. The Ozone Layer
Oxygen in the atmosphere provides a shield against solar UV radiation
O2 provides some shielding, but O3, or ozone, provides most of it
Most ozone is located in the ozone layer at an altitude of 25 km
Shielding is provided by the absorption of UV photons by oxygen molecules (both O2 and O3) and their resultant dissociation
Single O atoms combine with O and O2 to replenish the lost O2 and O3
It is doubtful that life could exist on the Earth’s surface without the ozone layer

63. Origin of the Earth’s Atmosphere
Several theories to explain origin of Earth’s atmosphere
Release of gas (originally trapped when the Earth formed) by volcanism or asteroid impacts
From materials brought to Earth by comet impacts
Analysis of volcanic emissions suggests that eruptions could be the source of the nitrogen and carbon dioxide gases in our athmosphere.

64. The Early Atmosphere Early atmosphere different than today
Contained much more methane (CH4) and ammonia (NH3)
Solar UV was intense enough to break out H from CH4, NH3 , and H2O leaving carbon, nitrogen, and oxygen behind while the H escaped into space
Ancient plants further increased the levels of atmospheric oxygen through photosynthesis

65. Motions of the Earth
Rotational and orbital motions define the day and year and cause the seasons
But our planet’s motions have other effects

66. Air and Ocean Circulation
In the absence of any force an object will move in a curved path over a rotating object
This apparent curved motion is referred to as the Coriolis effect

67. The Coriolis Effect Responsible for:
The spiral pattern of large storms as well as their direction of rotation
The trade winds that move from east to west in two bands, one north and one south of the equator
The jet stream is a result of the Coriolis effect
The direction of the jet streams, narrow bands of rapid, high-altitude winds
The deflection of ocean currents creating flows such as the Gulf Stream

68. The Coriolis Effect Also…
The atmospheric band structure of the rapidly rotating Jupiter, Saturn, and Neptune

69. Precession
As the Earth moves around the Sun over long periods of time, the direction in which its rotation axis points changes slowly
This changing in direction of the spin axis is called precession
Precession is caused by the Earth not being a perfect sphere – its equatorial bulge allows the Sun and Moon to exert unbalanced gravitational forces that twist the Earth’s spin axis
The Earth’s spin axis precesses around once every 26,000 years
Currently the spin axis points at Polaris – in A.D. 14,000 it will point nearly at the star Vega
Precession may cause climate changes

70. Precession