Unit 4: Formation of the Earth

Similar documents
Earth s Interior Earth - Chapter 12 Stan Hatfield Southwestern Illinois College

Shape and Size of the Earth

Chapter 7 Earth Pearson Education, Inc.

Chapter 12 Lecture. Earth: An Introduction to Physical Geology. Eleventh Edition. Earth s Interior. Tarbuck and Lutgens Pearson Education, Inc.

EARTH TAKES SHAPE 1. Define all vocabulary words. Crust: The thin and solid outermost layer of the Earth above the mantle. Mantle: The layer of rock

Earth s Structure. Earth s Interior. 3. Earth s interior is made of distinct layers.

D) outer core B) 1300 C A) rigid mantle A) 2000 C B) density, temperature, and pressure increase D) stiffer mantle C) outer core

Formation of the Earth and Solar System

Layers of Earth Write us-

Chapter 20 Earth: The Standard of Comparative Planetology

TODAY S FOCUS LAYERS OF THE EARTH

Earth as Planet. Earth s s Magnetic Field. The Earth s s Crust. Earth s s Interior

LIGO sees binary neutron star merger on August 17, 2017

The History of the Earth

1 Inside the Earth. What are the layers inside Earth? How do scientists study Earth s interior?

Nebular Hypothesis (Kant, Laplace 1796) - Earth and the other bodies of our solar system (Sun, moons, etc.) formed from a vast cloud of dust and

Activity 1-2: Origin of the Earth

Importance of Solar System Objects discussed thus far. Interiors of Terrestrial Planets. The Terrestrial Planets

Evidence of Earth s Interior Direct and Indirect Evidence

Invention of microscopes and telescopes expanded understanding of the Earth revealing new things

The Earth System. The Geosphere

1. In the diagram below, letters A and B represent locations near the edge of a continent.

Origin of the Solar System

The Solar System. Earth as a Planet

Earth. Interior Crust Hydrosphere Atmosphere Magnetosphere Tides

Important information from Chapter 1

Earth. Properties of Earth. Earth's Interior. Earth is the planet that we know best

Exploring Inside Earth

10/27/2014. Before We Begin, You Need to Understand These Terms: Earth s Structural Key Elements & the Hazards of Plate Movement

Chapter 8: The Dynamic Planet

Chapter 19. Magnetism

Accretionary Disk Model

1. The geosphere consists of three major layers: the,, and.

What is the Moon? A natural satellite One of more than 96 moons in our Solar System The only moon of the planet Earth

The Earth. Overall Structure of Earth

Chapter 7 Earth and the Terrestrial Worlds

Next opportunity to observe the Moon and Venus close together: Dec. 31, Announcements

Comparative Planetology II: The Origin of Our Solar System. Chapter Eight

1. A model of Earth's internal structure is shown below.

Name Class Date. 1. Traditionally, how have different fields of earth science been studied?

Earth Science Review Ch 1 & 2. Chapter 1 - Introduction to Earth Science

Chapter Seven: Heat Inside the Earth

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

EARTH S ENERGY SOURCES

Qx2wLyagk4

EARTH AND UNIVERSE. Earth

I. Earth spheres A. Three major spheres 1. atmosphere, thin envelope 2. hydrosphere covers more than 71% of surface 3. geosphere from hydrosphere to

The oldest rock: 3.96 billion yrs old: Earth was forming continental crust nearly 400 billion years ago!!

Lecture Outlines PowerPoint. Chapter 1 Earth Science, 12e Tarbuck/Lutgens

Standard 2, Objective 1: Evaluate the source of Earth s internal heat and the evidence of Earth s internal structure.

How do we know about the different layers of Earth's interior when we've never been there?

Origin of the Solar System

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am

TEST NAME:Geology part 1 TEST ID: GRADE:06 - Sixth Grade SUBJECT:Life and Physical Sciences TEST CATEGORY: My Classroom

Earth s s Topographic Regions

Chapter 8 Lecture. The Cosmic Perspective Seventh Edition. Formation of the Solar System

Name Class Date. 1. Traditionally, how have different fields of Earth science been studied?

Terrestrial Planets: The Earth as a Planet

Name Period Date L.O: SWBAT DESCRIBE THE PROPERTIES OF THE ATMOSPHERE.(

Comparative Planetology II: The Origin of Our Solar System. Chapter Eight

10/11/2010. 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)

Lecture 11 The Structure and Atmospheres of the Outer Planets October 9, 2017

The Earth. February 26, 2013

Nature and Origin of Planetary Systems f p "

Earth s Interior. Use Target Reading Skills. Exploring Inside Earth

Earth systems Unit 1 ( approx. 11 classes)

AST Section 2: Test 1

Engineering Geology. Earth Structure. Hussien aldeeky

Today. Solar System Formation. a few more bits and pieces. Homework due

Earth! Objectives: Interior and plate tectonics Atmosphere and greenhouse effect

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

BELLRINGER How close a group of measurements are to each other is called. 1. estimation 2. accuracy 3. precision. 0% 0% 0% 0% 4.

Today. Events. Terrestrial Planet Geology. Fall break next week - no class Tuesday

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

The Earth System Connections among the great spheres

Introduction to Earth Science SCIENTIFIC MEASUREMENTS AND GRAPHING

The Dynamic Crust 2) 4) Which diagram represents the most probable result of these forces? 1)

Lecture notes Bill Engstrom: Instructor Earth s Interior GLG 101 Physical Geology

Investigating Planets Name: Block: E1:R6

PTYS 214 Spring Announcements. Next midterm 3/1!

Chapter 9. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 26: Planetary Geology [3/23/07] Announcements.

Most of the energy from the light sources was transferred to the sand by the process of A) conduction B) convection C) radiation D) transpiration

Earth Systems Overview

What is Earth Science? Earth science is the branch of science dealing with the constitution of the earth and its atmosphere.

What Do Scientists Know About Earth s Surface and Interior?

AST 301 Introduction to Astronomy

Why does the Earth have volcanoes? Why is there Earthquakes?

Atmospheric Structure

Astro 1010 Planetary Astronomy Sample Questions for Exam 4

The Jovian Planets. Huge worlds, heavily mantled in gas at the time of the formation of the Solar System.

Earth s Atmosphere. Atmospheric Composition 78% Nitrogen 21% Oxygen 1 % Argon, 0.03% Carbon dioxide, Water. Recall the Electro-Magnetic (EM) Spectrum

UGRC 144 Science and Technology in Our Lives/Geohazards

EARTH'S INTERIOR MEGA PACKET MC

Astronomy 1504 Section 10 Final Exam Version 1 May 6, 1999

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Contents of the Solar System

What s in Our Solar System?

Earth Science 104. Earth s Place in the Cosmos, Structure History of Astronomy

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Transcription:

Unit 4: Formation of the Earth Objectives: E2.2A - Describe the Earth s principal sources of internal and external energy (e.g.,radioactive decay, gravity, solar energy). E3.2A - Describe the interior of the Earth (in terms of crust, mantle, and inner and outer cores) and where the magnetic field of the Earth is generated.

Sources of Energy* Heat within the Earth comes from two major sources: radioactive decay and residual heat. Radioactive decay is the result of a process that involves the loss of particles from the nucleus of an isotope (called the parent) to form the isotope of a new element (called the daughter). The radioactive decay of naturally occurring chemical elements (usually uranium, thorium, and potassium), releases energy in the form of heat, which slowly migrates toward the Earth s surface. Residual heat is the gravitational energy left over from the formation of the Earth, by the falling together and compression of cosmic debris (much like a bicycle pump that heats up due to the compression of air inside it). All radioactive decay processes release heat as a by-product.

Sources of Energy* The major source of external energy to our Earth is, of course, our Sun. Insolation is the incoming radiation from the Sun that is received by the Earth s atmosphere and surface. It is the driving force that moves the atmosphere and creates weather on Earth in addition to providing the energy required by plants to perform photosynthesis. Most of the Sun s radiation received by the Earth is in the form of shortwave radiation. This high-energy radiation makes up approximately 88% of the radiation that is received on Earth. This includes ultraviolet, visible light, and the near-infrared radiation. The remaining 12% of the radiation received on Earth is low-energy long-wave radiation. This includes farinfrared and microwave radiation.

Earth s Interior The original surface of the Earth probably looked much as the Moon s surface does today. The Earth was probably composed of the same material from its surface all the way to its center. Objects colliding with Earth helped to cause Earth to grow hot enough that heavy elements such as iron and nickel melted. The material composing Earth gradually separated into several layers, with the denser material being located near the center.

Earth s Interior Crust Mantle Outer core Inner core

Crust* Solid A thin, rigid layer of lighter rocks Extends to a depth of 65 km Temperature is less than 1000 K, however it increases by 10-30 K for every kilometer of depth The part of the geosphere that humans have direct contact with, and the only place where life has been found Note K = Kelvin (degrees) K = C + 273

Mantle* Solid with liquid properties Thickest of Earth s layers Composed mostly of compounds rich in iron, silicon, and magnesium High temperatures and pressures cause it to behave as a liquid in some ways Extends to a depth of 2890 km (from the surface) Temperature is between 1500-3200 K, and increases with depth

Outer Core* Liquid Composed of iron and nickel Extends to a depth of 5150 km (from the surface) Temperature is between 3700-5500 K, and increases with depth

Inner Core* Solid Composed of iron and nickel Extends to a depth of 6371 km (from the surface) Temperature is approximately 6000 K

Drilling into the Earth How far have humans been able to drill down into the Earth? Humans have only been able to drill down about 12 km (approximately 7.6 miles) into the Earth s crust. We have never drilled into the mantle, outer core, or inner core.

Earth s Magnetic Field* Although scientists do not fully understand the origin of Earth s magnetic field, many support a hypothesis first developed in the 1900s. The hypothesis suggests that the movement of the liquid interior of the Earth generate a strong magnetic field that surrounds the planet. This causes the Earth to act much like a large magnet, with the poles of the magnet located near the poles of the Earth.

Earth s Magnetic Field Our magnetic field stretches out through the atmosphere and acts as a protective barrier to deadly, high-energy solar radiation. This portion of the Earth is called the magnetosphere.

Earth s Magnetic Field The Earth s magnetic field allows us to use compasses to locate direction on the planet. A small magnetic needle that is allowed to spin freely aligns itself with the Earth s magnetic field and points to the magnetic North Pole.

Earth s Magnetic Field Because the geographic poles do not exactly match up with the magnetic poles, you need to be aware of magnetic declination when you use a compass. Magnetic declination is the number of degrees and direction between true north (geographic) and magnetic north. As you can see, Ann Arbor is about 7 west of true north.