The Solar System. Earth as a Planet

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

Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves.

Chapter 9 Lecture. The Cosmic Perspective Seventh Edition. Planetary Geology: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

How can solid rock be bent, squished, stretched, and cracked?

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

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

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

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

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

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

Chapter 7 Earth and the Terrestrial Worlds

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Climate Regulation. - What stabilizes the climate - Greenhouse effect

25-Nov-14. The Structure of Earth s Interior. What unique features of Earth are important for life as we know it?

Terrestrial Planets: The Earth as a Planet

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

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

Chapter 20 Earth: The Standard of Comparative Planetology

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick

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

2010 Pearson Education, Inc.

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

General Comments about the Atmospheres of Terrestrial Planets

AST 105 Intro Astronomy The Solar System

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued

15-Nov-17. Chapter 7 Earth and the Terrestrial Worlds. They are very different. So why have they turned out so differently?

Planet Earth. Our Home APOD

The Sun and Planets Lecture Notes 6.

Interiors of Worlds and Heat loss

Earth s Atmosphere About 10 km thick

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

Chapter 7 Earth Pearson Education, Inc.

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

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)

Earth. Interior Crust Hydrosphere Atmosphere Magnetosphere Tides

ASTR 100. Lecture 10: Planetary geology and atmospheres

Inner Planets (Part II)

Geology of the terrestrial planets Pearson Education, Inc.

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

The Terrestrial Planets

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Class Exercise. Today s Class. Overview of Mercury. Terrestrial Planet Interiors. Today s Class: Mercury & Venus

For the next few weeks: Terrestrial Planets, their Moons, and the Sun. Planetary Surfaces and Interiors 2/20/07

Investigating Planets Name: Block: E1:R6

Chapter 5 Review. 1) Our Earth is about four times larger than the Moon in diameter. 1)

Chapter 9. ASTRONOMY 202 Spring 2007: Solar System Exploration. Class 27: Planetary Geology [3/26/07] Announcements.

LIGO sees binary neutron star merger on August 17, 2017

The Earth. Overall Structure of Earth

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

Earth, the Lively* Planet. * not counting the life on the planet!

Grades 9-12: Earth Sciences

The Layered Atmosphere:

Planetary Atmospheres (Chapter 10)

The Official CA State Science Education Standards for Earth Science K 8

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

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.

Origin of Earth s Water When Earth first formed it was so hot that the original water would be lost to space Water added later by comets and/or

Structure of the Earth EARTH ( ) - need a solid, will not go through a liquid

Shape and Size of the Earth

Chapter 11 Review Clickers. The Cosmic Perspective Seventh Edition. Jovian Planet Systems Pearson Education, Inc.

3. Titan is a moon that orbits A) Jupiter B) Mars C) Saturn D) Neptune E) Uranus

UNIT 3 GEOLOGY VOCABULARY FLASHCARDS THESE KEY VOCABULARY WORDS AND PHRASES APPEAR ON THE UNIT 3 CBA

Science Practice Astronomy (AstronomyJSuber)

[17] Magnetic Fields, and long-term changes in climate (10/26/17)

Meteorites. A Variety of Meteorite Types. Ages and Compositions of Meteorites. Meteorite Classification

Tectonics. Planets, Moons & Rings 9/11/13 movements of the planet s crust

Origin of the Solar System

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

PLATO - 5. Planetary atmospheres

PTYS/ASTR Section 2 - Spring 2007 Practice Exam 2

ASTR 1050: Survey of Astronomy Fall 2012 PRACTICE Exam #2 Instructor: Michael Brotherton Covers Solar System and Exoplanet Topics

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

Chapter 2 Geography. Getting to know Earth

ASTR-101 Section 004 Lecture 9 Rare Earth? John T. McGraw, Professor

The Earth s Structure

Astro 1010 Planetary Astronomy Sample Questions for Exam 4

Phys 214. Planets and Life

Key Concept Heat in Earth s atmosphere is transferred by radiation, conduction, and convection.

The greenhouse effect

Astronomy 103: First Exam

Chapter 11 Jovian Planet Systems

Chapter 11 Jovian Planet Systems. Jovian Planet Composition. Are jovian planets all alike? Density Differences. Density Differences

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

Planetary Atmospheres

The Atmosphere. Characteristics of the Atmosphere. Section 23.1 Objectives. Chapter 23. Chapter 23 Modern Earth Science. Section 1

Topics: The Layers of the Earth and its Formation Sources of Heat Volcanos and Earthquakes Rock Cycle Rock Types Carbon Tax

EARTH S ENERGY SOURCES

Lecture 20. Origin of the atmosphere (Chap. 10) The carbon cycle and long-term climate (Chap. 8 of the textbook: p )

The Atmosphere - Chapter Characteristics of the Atmosphere

Crosswalk of Georgia Performance Standards & Georgia Standards of Excellence GSE Implementation in Sixth Grade

Physical Geography A Living Planet

12. Jovian Planet Systems Pearson Education Inc., publishing as Addison Wesley

[16] Planetary Meteorology (10/24/17)

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

AST 105 Intro Astronomy The Solar System

The Earth - Surface and Interior

Introduction to Astronomy

Chapter 2: Physical Geography

Transcription:

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 pulls highdensity material to center. Lower-density material rises to surface. Material ends up separated by density.

Heat Drives Geological Activity Convection: Hot rock rises, cool rock falls. One convection cycle takes 100 million years on Earth.

Sources of Internal Heat 1. Gravitational potential energy of accreting planetesimals 2. Differentiation 3. Radioactivity

Cooling of Interior Convection transports heat as hot material rises and cool material falls. Conduction transfers heat from hot material to cool material. Radiation sends energy into space.

Role of Size Smaller worlds cool off faster and harden earlier. The Moon and Mercury are now geologically dead.

Planetary Magnetic Fields Moving charged particles create magnetic fields. A planet s interior can create magnetic fields if its core is electrically conducting, convecting, and rotating.

Earth s Magnetosphere Earth s magnetic field protects us from charged particles from the Sun. The charged particles can create aurorae ( Northern lights ).

Geological Processes Impact cratering Impacts by asteroids or comets Volcanism Eruption of molten rock onto surface Tectonics Disruption of a planet s surface by internal stresses Erosion Surface changes made by wind, water, or ice

Impact Cratering Meteor Crater, Arizona Tycho, Moon Most cratering happened soon after the solar system formed. Craters are about 10 times wider than the objects that made them. Small craters greatly outnumber large ones.

Volcanism Volcanism happens when molten rock (magma) finds a path through lithosphere to the surface. Molten rock is called lava after it reaches the surface.

Outgassing Volcanism also releases gases from Earth s interior into the atmosphere.

Tectonics Convection of the mantle creates stresses in the crust called tectonic forces. Compression forces make mountain ranges. A valley can form where the crust is pulled apart.

Erosion Erosion is a blanket term for weather-driven processes that break down or transport rock. Processes that cause erosion include Glaciers Rivers Wind

Erosion The Glaciers Wind Erosion Colorado wears can River carved away create rock the new and continues Yosemite builds features up by sand to carve Valley. dunes. depositing the debris. Grand Canyon.

Tutorial: Earth s Changing Surface Work with a partner! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Take the time to understand it now! Come to a consensus answer you both agree on. If you get stuck or are not sure of your answer, ask another group. If you are really stuck or are not sure what the question is asking, ask me.

Effects of Atmosphere on Earth 1. Erosion 2. Radiation protection 3. Greenhouse effect 4. Makes the sky blue!

Radiation Protection All X-ray light is absorbed very high in the atmosphere. Ultraviolet light is absorbed by ozone (O 3 ).

The Greenhouse Effect Greenhouse gases in Earth s atmosphere keep infrared radiation from rapidly escaping into space But will eventually escape!

Understanding the Greenhouse Effect Spectra for Sun and Earth Sun gives of mostly visible ; Earth gives of mostly IR Greenhouse gases absorb and re-emit IR but are transparent to Visible light. H 2 0, CO 2, CH 4 Surface of planet is heated by energy (light) from the Sun AND from energy (IR light) re-radiated from the atmosphere Greenhouse effect is a natural process and the surface of Earth would be much colder w/out greenhouse effect

How is human activity changing our planet?

Dangers of Human Activity Human-made CFCs in the atmosphere destroy ozone, reducing protection from UV radiation. Does not contribute to the greenhouse effect or global warming Human activity is driving many other species to extinction. Human use of fossil fuels produces greenhouse gases that can cause global warming.

Global Warming Earth s average temperature has increased by 0.5 C in the past 50 years. The concentration of CO 2 is rising rapidly. An unchecked rise in greenhouse gases will lead to global warming.

CO 2 Concentration Global temperatures have tracked CO 2 concentration for the last 500,000 years. Antarctic air bubbles indicate the current CO 2 concentration is at its highest level in at least 500,000 years.

CO 2 Concentration Most of the CO 2 increase has happened in the last 50 years!

Modeling of Climate Change Models of global warming that include human production of greenhouse gases are a better match to the global temperature rise.

Greenhouse Effect: Bad? Because of the greenhouse effect, Earth is much warmer than it would be without an atmosphere but so is Venus.

Why the sky is blue Atmosphere scatters blue light from the Sun, making it appear to come from different directions. Sunsets are red because less of the red light from the Sun is scattered.

What makes a planet habitable? Located at an optimal distance from the Sun for liquid water to exist

What makes a planet habitable? Large enough for geological activity to release and retain water and atmosphere

Planetary Destiny Earth is habitable because it is large enough to remain geologically active, and it is at the right distance from the Sun so oceans could form.