EARTH S ENERGY SOURCES
|
|
- Chastity Nash
- 5 years ago
- Views:
Transcription
1 EARTH S ENERGY SOURCES The geological processes that shape the Earth s surface are powered by two major sources of energy; geothermal heat from the Earth s interior and external energy from the sun. The Earth s internal heat is the ultimate source of energy for virtually all tectonic and mantle processes, whereas the sun s energy drives the water cycle, and controls weathering and erosion. Tectonic activity (mountain building) also generates surface relief which allows the downslope movement of rock material under the influence of gravity. Evidence of the Earth s internal energy is provided by the geothermal heat flow which can be measured, and in some cases observed, at the surface. Volcanoes, geysers and hot springs, of course, provide further evidence that the inside of the Earth is much hotter than the surface. Since the inside of the Earth is hotter than the outside it follows that heat must flow outwards. Heat flow is measured in Watts per square metre (W/m 2 ). The present rate of heat flow to the surface is fairly well established and can be measured from the increase in temperature with depth (known as the geothermal gradient or geotherm) and on how well the rocks conduct heat (see Figure 45). Heat flow to the Earth s surface is higher where geothermal gradients are steep and in rocks which are relatively good conductors. Heat flow rates within continents average around W/m 2 and range up to 0.2 W/m 2 in areas of volcanic activity. In the ocean basins the average is about W/m 2, but increases to rates of 0.3 W/m 2 at volcanic mid-oceanic ridges. These variations in heat flow provide important clues as to the nature of the Earth s interior and the tectonic and mantle processes in operation. Figure 45 Global Heat Flow
2 In general, temperature increases with depth at an average rate of C/km for the first 200km and thereafter dropping to a rate of about 1 C/km (see Figure 46). However, the rate at which the temperature rises over the first 200km is very variable. In some parts of the lithosphere temperature rises very slowly with depth while in other parts temperature rises very rapidly. In areas of high heat flow the geothermal gradient is steep (e.g. mid-oceanic ridges), whereas in areas of low heat flow the geothermal gradient is less steep (e.g. oceanic trenches). Figure 46 shows the relationship between the Earth s heat flow and the rate at which temperature increases with depth. Graph A shows the normal situation over most of the Earth. Here the temperature increases with depth at the average rate of C/km and does not cross the melting point curve (known as the solidus line) of the mantle rocks, so no melting of rock occurs to form magma. Graph B and C show a situation where the geothermal gradient is much higher (i.e. temperature increase with depth at a much quicker rate here) and crosses the solidus line for mantle rocks which causes melting to take place. In Graph D the geothermal gradient is very similar to the rest of the Earth but melting does occur for reasons which will be discussed later in the plate tectonic section. Figure 46 Earth s Geotherm The interior of the Earth gives off enormous amounts of heat due the continual decay of certain radioactive isotopes (radiogenic heat); the residual heat trapped within the earth since its formation 4.6 billion years ago (primordial heat); and the formation of the core. By far the most important of these is the decay of long-lived radioisotopes such as those of uranium (U), thorium (Th) & potassium (K). Long-lived radioisotopes are elements with particularly long half-lives (U 4.5 billion years, Th 14 billion years and K 1.3 billion years).
3 About 83% of the heat flow to the Earth s surface is attributable to this process. The elements U, Th and K (and their radiogenic isotopes) are particularly concentrated in the silicate-dominated outer layers of the Earth, and in particular within the continental crust. They are thought to be virtually absent from the core. As a result the radiogenic heat produced per unit mass of the continental crust is, on average, over 100 times greater than that of the underlying mantle. But because the mantle is so much more massive than the crust, in effect this means that the overall radiogenic heating budget is roughly split equally between the mantle and the crust despite the much greater mass of mantle material. It is the decay of these long-lived isotopes that provides sufficient heat energy to keep the Earth geologically active. Figure 47 Relationship between the Geotherm, Heat Flow and Plate Tectonics Residual heat from the formation of the Earth could still be escaping to the Earth s surface. The Earth formed by the collision of millions of rocky fragments through a process called accretion. As these fragments accelerated due to gravitational attraction towards the forming Earth, their gravitational potential was converted to kinetic energy. When they impacted, much of it was then transferred to heat energy, causing heating of the Earth. The decay of shortlived radioisotopes (formed in a supernova that may have triggered Solar System formation)
4 could also have produced a lot of heat soon after the Earth was formed. This heat would have been produced for the first few million years of the Earth s existence from this source. The Earth has differentiated to form a dense core surrounded by a relatively lower density mantle and even lower density crust. Differentiation is the process by which planets develop concentric layering, with zones that differ in their chemical and mineralogical compositions, due to the separating out of materials of different densities. The Earth would have undergone this process very early on in its formation, when the entire planet was molten. During this early molten phase the material that now forms the core would have sunk towards the centre under the influence of gravity because of its relatively high density. The gravitational energy lost by this inward movement of this material would have been converted first to kinetic energy and then into thermal energy. It is estimated that the core-forming process would have contributed significantly to the Earth s primordial heating. As we have seen so far, radioactive decay, accretion and core formation are the processes that have heated the Earth. But how is this internal heat transferred to the surface? There are four mechanisms of heat transfer: conduction, convection, radiation and advection. In conduction, heat is transferred from atom to atom or molecule to molecule within a material. The rate at which it does this depends on the temperature difference between the hot and cold portions of the material. Different materials, such as rocks of various compositions, conduct heat at different rates, and the efficiency of heat transfer in this manner is known as conductivity. Conduction is the most important heat transfer process in the outermost layer of the Earth (i.e. the lithosphere). In convection, matter actually moves, driven by density differences causing buoyancy, taking heat energy with it. Denser (colder) material tends to move downwards, while less dense (hotter) material moves upwards. During this transfer the material gives up its heat. It is a particularly efficient method of heat transfer, but the medium through which transfer takes place must be fluid. However, the term fluid describes any substance capable of flowing and is not restricted to liquids and gases. Under the right conditions, even solid rocks can flow, albeit at a very slow rate (a few centimetres per year). Over long periods of time, the effect of such solid-state convection becomes a highly significant way of transferring heat towards the Earth s surface. In fact it is the most efficient form of heat transfer within all but the outermost part of Earth. Advection is rather like the upward part of convection. In this process heat is transferred when molten material (magma) moves up through fractures in the lithosphere and remains there. Advection operates when magma spreads out at the surface as a lava flow or, if it is injected, cools and crystallises within the lithosphere itself. The effect is the same in both cases, since heat is transferred by the molten rock from deeper levels where melting is taking place to shallower levels where it solidifies, losing its heat by conduction to the overlying crust. Any planetary body that exhibits, or has exhibited, volcanic activity must have lost some of its internal heat in this manner.
5 In the case of radiation, photons (electromagnetic radiation) carry away the heat energy from hotter region (Earth s surface) to a colder one (atmosphere above). This is the final process in the transfer of heat from the interior of the Earth to the surface and then into space. The Earth s external energy source is from the sun. Solar heating of the Earth s surface drives the water cycle and controls weathering and erosional processes. Igneous, sedimentary and metamorphic rocks are linked through the rock cycle by key rock forming processes (weathering, erosion, transportation, deposition, lithification, metamorphism, partial melting and crystallisation). Figure 48 is a schematic diagram of the rock cycle. In Figure 8, boxes represent earth materials and arrows represent the processes that transform those materials. The processes are named in bold next to the arrows. The two major sources of energy for the rock cycle are also shown; the sun provides energy for surface processes such as weathering, erosion, and transport, and the earth's internal heat provides energy for processes like subduction, melting, and metamorphism. The complexity of the diagram reflects a real complexity in the rock cycle. Notice that there are many possibilities at any step along the way. Figure 48
TODAY S FOCUS LAYERS OF THE EARTH
TODAY S FOCUS LAYERS OF THE EARTH 8.6C investigate and describe applications of Newton s law of inertia, law of force and acceleration, and law of action-reaction such as in vehicle restraints, sports
More informationEarth Systems Science Chapter 7. Earth Systems Science Chapter 7 11/11/2010. Seismology: study of earthquakes and related phenomena
Earth Systems Science Chapter 7 I. Structure of the Earth II. Plate Tectonics The solid part of the earth system includes processes, just like the atmosphere and oceans. However, the time scales for processes
More informationLIGO sees binary neutron star merger on August 17, 2017
LIGO sees binary neutron star merger on August 17, 2017 Laser Interferometer Gravitational-Wave Observatory (LIGO) Laser Interferometer Gravitational-Wave Observatory (LIGO) Multi-Messenger Astronomy This
More informationHeat in the Earth and heat flow (see Mussett & Khan, Chapter 17; various topics in Fowler, Chapter 7, especially p )
Heat in the Earth and heat flow (see Mussett & Khan, Chapter 17; various topics in Fowler, Chapter 7, especially p. 269-281) At the surface of the Earth we receive heat energy from the Sun and from inside.
More informationStandard 2, Objective 1: Evaluate the source of Earth s internal heat and the evidence of Earth s internal structure.
Standard 2: Students will understand Earth s internal structure and the dynamic nature of the tectonic plates that form its surface. Standard 2, Objective 1: Evaluate the source of Earth s internal heat
More informationPetrology. Petrology: the study of rocks, especially aspects such as physical, chemical, spatial and chronoligic. Classification:
Petrology Petrology: the study of rocks, especially aspects such as physical, chemical, spatial and chronoligic. Associated fields include: Petrography: study of description and classification of rocks
More informationPetrology. Petrology: the study of rocks, especially aspects such as physical, chemical, spatial and chronoligic. Associated fields include:
Petrology Petrology: the study of rocks, especially aspects such as physical, chemical, spatial and chronoligic. Associated fields include: Petrography: study of description and classification of rocks
More informationGeosphere Final Exam Study Guide
Geosphere Final Exam Study Guide Chapter 1 Intro to Earth Systems 1. Name and describe Earth s 4 major spheres Geosphere-- nonliving, mostly solid rock divided into crust, mantle, and core Atmosphere a
More informationTEST NAME:Geology part 1 TEST ID: GRADE:06 - Sixth Grade SUBJECT:Life and Physical Sciences TEST CATEGORY: My Classroom
TEST NAME:Geology part 1 TEST ID:1542715 GRADE:06 - Sixth Grade SUBJECT:Life and Physical Sciences TEST CATEGORY: My Classroom Geology part 1 Page 1 of 6 Student: Class: Date: 1. The picture below shows
More informationFormation of the Earth and Solar System
Formation of the Earth and Solar System a. Supernova and formation of primordial dust cloud. NEBULAR HYPOTHESIS b. Condensation of primordial dust. Forms disk-shaped nubular cloud rotating counterclockwise.
More informationChapter 12 Lecture. Earth: An Introduction to Physical Geology. Eleventh Edition. Earth s Interior. Tarbuck and Lutgens Pearson Education, Inc.
Chapter 12 Lecture Earth: An Introduction to Physical Geology Eleventh Edition Earth s Interior Tarbuck and Lutgens Earth s Internal Structure Earth s interior can be divided into three major layers defined
More informationSocial Studies 9 UNIT 2 GEOGRAPHIC INFLUENCES ON IDENTITY: PLACE AND PEOPLE
Social Studies 9 UNIT 2 GEOGRAPHIC INFLUENCES ON IDENTITY: PLACE AND PEOPLE The Structure of the Earth To understand the forces that create Canada's physical landscape we must understand the structure
More informationDirected Reading. Section: Volcanoes and Plate Tectonics
Skills Worksheet Directed Reading Section: Volcanoes and Plate Tectonics 1. What can cause some of the most dramatic changes to Earth s surface? a. solar activity b. tides c. geysers d. volcanic eruptions
More information1. The process by which the ocean floor sinks beneath a deep-ocean trench and back into the mantle is known as
Sample questions 1. The process by which the ocean floor sinks beneath a deep-ocean trench and back into the mantle is known as b. continental drift c. subduction d. conduction 2. The transfer of thermal
More informationUNIT 3 GEOLOGY VOCABULARY FLASHCARDS THESE KEY VOCABULARY WORDS AND PHRASES APPEAR ON THE UNIT 3 CBA
UNIT 3 GEOLOGY VOCABULARY FLASHCARDS THESE KEY VOCABULARY WORDS AND PHRASES APPEAR ON THE UNIT 3 CBA A map that shows Earth s Topographic Map surface topography, which is Earth s shape and features Contour
More informationPhysics and Chemistry of the Earth and Terrestrial Planets
MIT OpenCourseWare http://ocw.mit.edu 12.002 Physics and Chemistry of the Earth and Terrestrial Planets Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms.
More informationEarth. Properties of Earth. Earth's Interior. Earth is the planet that we know best
Earth Earth is the planet that we know best Our observations of the other planets are all compared to the conditions and properties of Earth Properties of Earth Semimajor Axis Orbital Eccentricity Orbital
More informationEarth s Interior HW Packet HW #1 Plate Tectonics (pages )
Name Earth s Interior HW Packet HW #1 Plate Tectonics (pages 676 683) 1. Is the following sentence true or false? According to the theory of plate tectonics, Earth s plates move about quickly on top of
More informationHeat Transfer. Heat Transfer. Convection Heat transfer due to the actual motion of a fluid. Conduction Heat transfer by successive atomic collisions
Heat Transfer What are the different ways that heat can move from one place to another? Heat Transfer What are the different ways that heat can move from one place to another? Conduction Convection Radiation
More informationTerrestrial Planets: The Earth as a Planet
Terrestrial Planets: The Earth as a Planet In today s class, we want to look at those characteristics of the Earth that are also important in our understanding of the other terrestrial planets. This is
More informationChapter 9. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 26: Planetary Geology [3/23/07] Announcements.
ASTRONOMY 202 Spring 2007: Solar System Exploration Instructor: Dr. David Alexander Web-site: www.ruf.rice.edu/~dalex/astr202_s07 Class 26: Planetary Geology [3/23/07] Announcements Planetary Geology Planetary
More informationPlanet Earth. Our Home APOD
Planet Earth Our Home APOD 1 Earth a highly evolved planet = altered dramatically since formation, due to flow of energy from interior to surface 2 Planet Earth Facts diameter (equator) 12,756 km radius
More informationPlate Tectonics. Continental Drift Sea Floor Spreading Plate Boundaries
Plate Tectonics Continental Drift Sea Floor Spreading Plate Boundaries Continental Drift 1915, Alfred Wegener - Pangea hypothesis: suggested Earth s continents were part of a large super-continent 200
More informationForms of Energy. Energy: commonly defined as the capacity to do work (i.e. by system on its surroundings); comes in many forms
Forms of Energy Energy: commonly defined as the capacity to do work (i.e. by system on its surroundings); comes in many forms Work: defined as the product of a force (F) times times a displacement acting
More informationNebular Hypothesis (Kant, Laplace 1796) - Earth and the other bodies of our solar system (Sun, moons, etc.) formed from a vast cloud of dust and
Plate Tectonics Origin of Universe Big Bang model (Hubble, 1929) - The universe began with an explosive e expansion of matter, which later became what we know as stars, planets, moons, etc. This event
More informationRock Cycle. Draw the Rock cycle on your remediation page OR use a sheet of notebook paper and staple
Earth Science Test 8.ESS2.3) Describe the relationship between the processes and forces that create igneous, sedimentary, and metamorphic rocks. I can develop and use models to explain how plate movements
More informationImportance of Solar System Objects discussed thus far. Interiors of Terrestrial Planets. The Terrestrial Planets
Importance of Solar System Objects discussed thus far Interiors of Terrestrial Planets Chapter 9 Sun: Major source of heat for the surfaces of planets Asteroids: Provide possible insight to the composition
More informationThe Earth in the Universe
The Earth in the Universe (OCR) Evidence for the age of the Earth Scientists once thought that the Earth was only 6000 years old. Rocks have provided lots of evidence for the world being older. 1) Erosion
More informationLecture 17: Earth s Interior. Extrasolar Planets. Extrasolar Planets. planet
Lecture 17: Earth s Interior The appearance of life led to further profound changes in the atmosphere about 3.5 x 10 9 years ago Plants produce free oxygen and remove carbon dioxide The Earth s surface
More informationMAR110 Lecture #4 Fundamentals of Plate Tectonics
1 MAR110 Lecture #4 Fundamentals of Plate Tectonics The Ocean Sea Floor is formed Along the Mid-Ocean Ridge Spreading Centers The Ocean Sea Floor is destroyed in the Subduction Zones Figure 4.2 Convection
More informationChapter 8: The Dynamic Planet
Chapter 8: The Dynamic Planet I. The Pace of Change A. The Geologic Time Scale II. Earth s Structure and Internal Energy A. The Earth s Core B. The Earth s Mantle C. The Earth s Crust III. The Geologic
More informationUNIT 1 - Major Land and Water Forms
UNIT 1 - Major Land and Water Forms Chapter 1 - Landform Patterns and Processes Topography the natural and human features of the Earth s surface. ie. Surface features elevation - the height of a particular
More informationUnit 4 Lesson 6 Plate Tectonics
Unit 4 Lesson 6 Plate Tectonics Indiana Standards 7.2.1 Describe how the earth is a layered structure composed of lithospheric plates, a mantle and a dense core. 7.2.4 Explain how convection currents in
More informationToday. Events. Terrestrial Planet Geology. Fall break next week - no class Tuesday
Today Terrestrial Planet Geology Events Fall break next week - no class Tuesday When did the planets form? We cannot find the age of a planet, but we can find the ages of the rocks that make it up. We
More informationPlate Tectonics. Chapter 17. Great Idea: The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet.
Plate Tectonics Chapter 17 Great Idea: The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet. 1 Chapter Outline The Dynamic Earth Plate Tectonics: A Unifying
More information1. List the 3 main layers of Earth from the most dense to the least dense.
1. List the 3 main layers of Earth from the most dense to the least dense. 2. List the 6 layers of earth based on their physical properties from the least dense to the most dense. 3. The thinnest layer
More informationChapter 7 Earth Pearson Education, Inc.
Chapter 7 Earth Units of Chapter 7 7.1 Overall Structure of Planet Earth 7.2 Earth s Atmosphere Why Is the Sky Blue? The Greenhouse Effect and Global Warming 7.3 Earth s Interior Radioactive Dating Units
More informationGO ON. Directions: Use the diagram below to answer question 1.
d i a g n o s t i c t e s t : e a r t h a n d s p a c e s c i e n c e question 1. 1. What is the correct order (starting from the surface) of Earth s layers? A crust, outer core, inner core, mantle B mantle,
More informationFORCES ON EARTH UNIT 3.2. An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth.
FORCES ON EARTH UNIT 3.2 An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth. USE THESE NOTES: OUR HOME PLANET EARTH: What do you know about our planet? SO.HOW
More informationThe History of the Earth
The History of the Earth We have talked about how the universe and sun formed, but what about the planets and moons? Review: Origin of the Universe The universe began about 13.7 billion years ago The Big
More information10/11/2010. Acceleration due to gravity, a. Bulk Properties Mass = 6 x kg Diameter = 12,756 km Density = 5515 kg/m 3 (mix of rock and iron)
Acceleration due to gravity, a Bulk Properties Mass = 6 x 10 24 kg Diameter = 12,756 km Density = 5515 kg/m 3 (mix of rock and iron) Escape Velocity, v e Albedo Amount of sunlight reflected back into space
More informationTectonics. Planets, Moons & Rings 9/11/13 movements of the planet s crust
Tectonics Planets, Moons & Rings 9/11/13 movements of the planet s crust Planetary History Planets formed HOT Denser materials fall to center Planet cools by conduction, convection, radiation to space
More informationFORCES ON EARTH. An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth.
FORCES ON EARTH An investigation into how Newton s Laws of Motion are applied to the tectonic activity on Earth. GEOLOGY Geologists scientists who study the forces that make and shape the Earth Geologists
More informationWhy does the Earth have volcanoes? Why is there Earthquakes?
Why does the Earth have volcanoes? Why is there Earthquakes? Turn to your neighbor and review: How and when did the Earth form? How old are the first traces of life on Earth? Logical? * 1.5Ga (1 st multicellular
More informationD) outer core B) 1300 C A) rigid mantle A) 2000 C B) density, temperature, and pressure increase D) stiffer mantle C) outer core
1. In which area of Earth's interior is the pressure most likely to be 2.5 million atmospheres? A) asthenosphere B) stiffer mantle C) inner core D) outer core Base your answers to questions 2 and 3 on
More informationPlate Tectonic Review, Types of Plates
Plate Tectonic Review, Types of Plates Review from last week: 1. Alfred Wegener: thought that sections of the Earth s crust moved, but people were confused, and thought that continents drifted over water
More informationName Test Date Hour. the interior of the Earth to the surface. younger less dense plate.
Name Test Date Hour Earth Processes#2 - Notebook Plate Tectonics LEARNING TARGETS I can identify and describe the three main layers of Earth. I can explain the difference between an oceanic and a continental
More informationPlate Tectonics: A Scientific Revolution Unfolds
Chapter 2 Lecture Earth: An Introduction to Physical Geology Eleventh Edition Plate Tectonics: A Scientific Revolution Unfolds Tarbuck and Lutgens From Continental Drift to Plate Tectonics Prior to the
More informationsonar seismic wave basalt granite
geologist sonar crust geology seismic wave mantle constructive force basalt inner core destructive force granite outer core The solid, rocky, surface layer of the earth. an instrument that can find objects
More informationChapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds
Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds 9.1 Connecting Planetary Interiors and Surfaces Our goals for learning What are terrestrial planets like on the inside? What causes geological
More informationTopography the natural and human features of the Earth s surface. ie. Surface features need to understand difference between relief and elevation
Chapter 1 Landform Patterns and Processes Highlighted script will not be assessed Topography the natural and human features of the Earth s surface. ie. Surface features need to understand difference between
More informationRocks and the Rock Cycle. Banded Iron Formation
Rocks and the Rock Cycle Banded Iron Formation Rocks Big rocks into pebbles, Pebbles into sand. I really hold a million, million Rocks here in my hand. Florence Parry Heide How do rocks change? How are
More informationWhat Forces Drive Plate Tectonics?
What Forces Drive Plate Tectonics? The tectonic plates are moving, but with varying rates and directions. What hypotheses have been proposed to explain the plate motion? Convection Cells in the Mantle
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version E of the exam. Please fill in (E). A) This
More informationEarth. Interior Crust Hydrosphere Atmosphere Magnetosphere Tides
Earth Interior Crust Hydrosphere Atmosphere Magnetosphere Tides Semi-major Axis 1 A.U. Inclination 0 Orbital period 1.000 tropical year Orbital eccentricity 0.017 Rotational period 23 h 56 min 4.1 s Tilt
More informationStructure of the Earth
Structure of the Earth Compositional (Chemical) Layers Crust: Low density Moho: Density boundary between crust and mantle Mantle: Higher density High in Magnesium (Mg) and Iron (Fe) Core: High in Nickel
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version B of the exam. Please fill in (B). A) This
More informationEarth as a planet: Interior and Surface layers
Earth as a planet: Interior and Surface layers Bibliographic material: Langmuir & Broecker (2012) How to build a habitable planet Internal structure of the Earth: Observational techniques Seismology Analysis
More informationChapter 02 Test Bank: Internal Energy and Plate Tectonics KEY
Chapter 02 Test Bank: Internal Energy and Plate Tectonics KEY Multiple Choice Questions 1. Earth is about years old. A. 30,000 thousand B. 50 million C. 3,500 million D. 13.5 billion E. 4.5 billion 2.
More informationEarth s Geological Cycle
Earth s Geological Cycle What Are the Earth s Major Geological Processes? Main Processes: 1. Plate Tectonics 2. Rock Cycle 3. Soil Formation LITHOSPHERE The Earth s Structure Earth s Interior Core (Nickel
More informationPlate Tectonics Practice Test
Plate Tectonics Practice Test 1. What is the main idea Alfred Wegner proposed in the Theory of Continental Drift that he published in 1915? a. The continents float on a liquid layer that allows them to
More informationForces That Shape Earth. How do continents move? What forces can change rocks? How does plate motion affect the rock cycle?
Forces That Shape Earth How do continents move? What forces can change rocks? How does plate motion affect the rock cycle? Plate Motion Mountain ranges are produced by plate tectonics. The theory of plate
More informationPlate Tectonics. entirely rock both and rock
Plate Tectonics I. Tectonics A. Tectonic Forces are forces generated from within Earth causing rock to become. B. 1. The study of the origin and arrangement of Earth surface including mountain belts, continents,
More informationChapter 9. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 27: Planetary Geology [3/26/07] Announcements.
ASTRONOMY 202 Spring 2007: Solar System Exploration Instructor: Dr. David Alexander Web-site: www.ruf.rice.edu/~dalex/astr202_s07 Class 27: Planetary Geology [3/26/07] Announcements Planetary Geology Planetary
More informationPlate Tectonics Notes
Plate Tectonics Notes Last 30 Days Earthquakes Physical Features Last 30 Days Earthquakes with Plate Boundaries Earth s Structure Earth s Layers Core: Inner Core: Center of the earth, solid ball of metal
More information12.2 Plate Tectonics
12.2 Plate Tectonics LAYERS OF THE EARTH Earth is over 1200 km thick and has four distinct layers. These layers are the crust, mantle (upper and lower), outer core, and inner core. Crust outer solid rock
More informationThe Terrestrial Planets
The Terrestrial Planets Large Bodies: Earth (1 R E, 1 M E ) Venus (0.95 R E, 0.82 M E ) Small Bodies: Mars (0.53 R E, 0.11 M E ) Mercury (0.38 R E, 0.055 M E ) Moon (0.27 R E, 0.012 M E ) The surfaces
More informationWhy Does the Mantle Move the Way it Does?
Why Does the Mantle Move the Way it Does? In the demonstration, you observed warm water rising through cool water. You also observed cool water sinking to replace the warm water. The movement of a fluid
More information6. In the diagram below, letters A and B represent locations near the edge of a continent.
1. Base your answer to the following question on the cross section below and on your knowledge of Earth science. The cross section represents the distance and age of ocean-floor bedrock found on both sides
More informationEarth Movement and Resultant Landforms
Earth Movement and Resultant Landforms Structure of the Earth Lithosphere : earth s crust Asthenosphere : upper mantle zone where material is near its melting point & acts almost like liquid (appprox.
More informationOrigin of the Oceans II. Earth A Living Planet. Earthquakes and Volcanoes. Plate Tectonics II
Origin of the Oceans II Plate Tectonics II Earth A Living Planet Heat of formation of the planet is trapped at center, gradually escaping Center is nickel and iron Earthquakes and Volcanoes 1 Tracing the
More informationTOPIC 1: RELATIVE DATING ESSENTIAL QUESTION: HOW DO WE DETERMINE A ROCK S AGE BY THE SURROUNDING ROCKS?
TOPIC 1: RELATIVE DATING ESSENTIAL QUESTION: HOW DO WE DETERMINE A ROCK S AGE BY THE SURROUNDING ROCKS? TOPIC 1: RELATIVE DATING UNIFORMITARIANISM: THE IDEA THAT THE SAME FORCES HAVE BEEN AND CONTINUE
More informationSeafloor spreading is a geologic process in which tectonic plates large slabs of Earth's lithosphere split apart from each other.
This website would like to remind you: Your browser (Apple Safari 4) is out of date. Update your browser for more security, comfort and the best experience on this site. Encyclopedic Entry seafloor spreading
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 9 Plate Tectonics 9.1 Continental Drift An Idea Before Its Time Wegener s continental drift hypothesis stated that the continents had once been joined
More informationPrentice Hall EARTH SCIENCE
Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 9 Plate Tectonics 9.1 Continental Drift An Idea Before Its Time Wegener s continental drift hypothesis stated that the continents had once been joined
More informationUGRC 144 Science and Technology in Our Lives/Geohazards
UGRC 144 Science and Technology in Our Lives/Geohazards Session 5 Magma and Volcanism Lecturer: Dr. Patrick Asamoah Sakyi Department of Earth Science, UG Contact Information: pasakyi@ug.edu.gh College
More information10/27/2014. Before We Begin, You Need to Understand These Terms: Earth s Structural Key Elements & the Hazards of Plate Movement
Earth s Structural Key Elements & the Hazards of Plate Movement Before We Begin, You Need to Understand These Terms: Density Convection Currents AICE EM: Lithosphere Key Content 1 & 2 Density: heat rises,
More informationEarth s Interior Earth - Chapter 12 Stan Hatfield Southwestern Illinois College
Earth s Interior Earth - Chapter 12 Stan Hatfield Southwestern Illinois College Probing Earth s Interior Most of our knowledge of Earth s interior comes from the study of earthquake waves. Travel times
More informationName Date Class. Directions: Use the diagram below to answer question Florida Progress Monitoring and Benchmark Assessments
b e n c h m a r k t e s t : e a r t h a n d s p a c e s c i e n c e Multiple Choice 1. Geologists obtain indirect evidence about Earth s interior by A measuring pressure differences at Earth s surface.
More informationTopics: The Layers of the Earth and its Formation Sources of Heat Volcanos and Earthquakes Rock Cycle Rock Types Carbon Tax
Topics: The Layers of the Earth and its Formation Sources of Heat Volcanos and Earthquakes Rock Cycle Rock Types Carbon Tax Essay Question on Carbon Tax 1. Drilling 2. Volcanic Activity 3. Laboratory experiments
More information05/22/15. Tectonic plate (Noun) Plate tectonics (Noun) Oceanic crust/plate (Noun) Continental crust/plate (Noun) Continental drift (Noun)
Tectonic plate (Noun) The pieces of the Earth s crust that float on the mantle, causing continental drift and earthquakes and creating volcanoes, trenches, and mountains. The Earth s crust is divided into
More informationEarth s Interior StudyGuide
Name Date Period Earth s Interior StudyGuide 1. The two main elements that make up the Earth s crust are and. 2. The Earth s inner core is made of solid and. 3. When one plates slides under another plate
More informationContinental Drift and Plate Tectonics
Continental Drift and Plate Tectonics Continental Drift Wegener s continental drift hypothesis stated that the continents had once been joined to form a single supercontinent. Wegener proposed that the
More informationEarth is over 1200 km thick and has four distinct layers.
1 2.2 F e a ture s o f P la te T e c to nic s Earth is over 1200 km thick and has four distinct layers. These layers are the crust, mantle (upper and lower), outer core, and inner core. Crust outer solid
More informationCh. 9 Review. Pgs #1-31 Write Questions and Answers
Ch. 9 Review Pgs. 356-357 #1-31 Write Questions and Answers 356-357 #1-5 Answers 1. The layer of the upper mantle that can flow is the: A - Asthenosphere 2. Most scientists rejected Wegener s theory of
More informationContents. 1-Introduction
Contents 1 Introduction 2 Tectonic Plates 3 Seismic waves 4 Graph On Magnitude 5 Diagram of Earth s core 6 System Analysis 7 Glossary 8 Conclusion 9 Bibliography 1-Introduction With a sudden shock the
More informationThe oldest rock: 3.96 billion yrs old: Earth was forming continental crust nearly 400 billion years ago!!
Earth s vital statistics Shape: almost spherical Size: 6400km in radius Average density: 5.5gm/cc; surface: 3gm/cc or less; centre may be 10-15gm/cc 15gm/cc Temperature: core: 2200-2750 2750 o c Pressure:
More informationVolcanoes. Volcanic eruptions can be more powerful than the explosion of an atomic bomb.
Ch. 13 Volcanoes Volcanoes Volcanic eruptions can be more powerful than the explosion of an atomic bomb. Many of these eruptions are caused by the movement of tectonic plates. Volcanism Volcanism-any activity
More informationChapter 9 Lecture. The Cosmic Perspective Seventh Edition. Planetary Geology: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Chapter 9 Lecture The Cosmic Perspective Seventh Edition Planetary Geology: Earth and the Other Terrestrial Worlds Planetary Geology: Earth and the Other Terrestrial Worlds 9.1 Connecting Planetary Interiors
More informationNext opportunity to observe the Moon and Venus close together: Dec. 31, Announcements
Announcements Last OWL homework: due 12/15 before midnight Study guide for final exam is up on the class webpage Practice exam up Thursday afternoon Final exam: Monday, Dec. 15, 10:30 AM, Hasbrouck 20
More informationGEOLOGY. What is geology?
GEOLOGY What is geology? It is essentially the study of the earth and it s dynamic processes. Features and processes of rocks, the earth s interior and surface. Structure of the Earth Made up of three
More informationThe Solar System. Earth as a Planet
The Solar System Earth as a Planet Earth s Interior Core: Highest density; nickel and iron Mantle: Moderate density; silicon, oxygen, etc. Crust: Lowest density; granite, basalt, etc. Differentiation Gravity
More informationYanbu University College. General Studies Department. PHSC001 Course. Chapter9 (Basic Geology: Earthquakes and volcanoes ) Worksheet Solutions
Yanbu University College General Studies Department PHSC001 Course Chapter9 (Basic Geology: Earthquakes and volcanoes ) Worksheet Solutions Phsc001 worksheet9 solutions, yuc Page 1-6 Chapter 9 worksheet
More informationTHE ROCK CYCLE & ROCKS. Subtitle
THE ROCK CYCLE & ROCKS Subtitle 3. Three rocks that do not have minerals or are composed of nonmineral matter. Coal Pumuce Obsidian THE ROCK CYCLE Why do scientists study rocks? Rocks contain clues about
More informationThe Earth - Surface and Interior
Earth's Interior The Earth - Surface and Interior Basic Data Diameter 12,756 km (equator) Mass 6 x 10 24 kg Density 5.5 g/cm 3 5500 kg/m 3 Escape velocity 11.2 km/s Temp -130 F to 140 F 183K to 333K Albedo
More informationMAR110 Lecture #3 Ocean Bathymetry / Plate Tectonics
1 MAR110 Lecture #3 Ocean Bathymetry / Plate Tectonics Ocean Basin Geographic Zones The geographic zones of the North Atlantic are identified in the bird s eye view of the sea floor above. Below is shown
More informationPlate Tectonics. Chapter 8
Plate Tectonics Chapter 8 Vocabulary Crust Mantle Core Lithosphere Continental Drift Plate Tectonics Plate Boundary Fault What Are The Earth s Layers Made Of? Atmosphere: Contains nitrogen, oxygen, carbon
More informationEarth, the Lively* Planet. * not counting the life on the planet!
Earth, the Lively* Planet * not counting the life on the planet! What We Will Learn Today What are planet Earth s features? What processes shape planetary surfaces? How does Earth s surface move? How did
More informationComposition of the earth, Geologic Time, and Plate Tectonics
Composition of the earth, Geologic Time, and Plate Tectonics Layers of the earth Chemical vs. Mechanical Chemical : Mechanical: 1) Core: Ni and Fe 2) Mantle: Mostly Peridotite 3) Crust: Many different
More informationName Class Date. 1. What is the outermost layer of the Earth called?. a. core b. lithosphere c. asthenosphere d. mesosphere
Name Class Date Assessment Geology Plate Tectonics MULTIPLE CHOICE Write the letter of the correct answer in the space provided. 1. What is the outermost layer of the Earth called?. a. core b. lithosphere
More information