Astronomy 311: Lecture 4 - Terrestrial Planetary Atmospheres. An atmosphere is a layer of gas that surrounds a planet.

Size: px
Start display at page:

Download "Astronomy 311: Lecture 4 - Terrestrial Planetary Atmospheres. An atmosphere is a layer of gas that surrounds a planet."

Transcription

1 Astronomy 311: Lecture 4 - Terrestrial Planetary Atmospheres An atmosphere is a layer of gas that surrounds a planet. On Earth, atmosphere is about 10km thick: O 2, N 2, H 2 O, CO 2. Atmospheric pressure decreases as you go up. Principle of hydrostatic equilibrium applies. Ideal gas law: P = ρt constant. Average pressure at sea level is 1.03kg/m 2 which is 1 bar of pressure. Atmospheres create pressure that can determine whether water is in liquid form on the surface. Atmospheres can absorb and scatter light: daytime skies are blue in worlds with atmospheres. Atmospheres create winds and weather. Atmospheres can contain gases which make planetary surfaces warmer than they would be otherwise using the greenhouse effect. Greenhouse effect Visible light from Sun absorbed by the ground. Ground reradiates this radiation in the form of I=infra-red (IR) light because this is the appropriate wavelength for a body of that temperature (Wien s law). Then some gases in lower atmosphere trap this IR radiation for a while and are heated by it. These greenhouse gases are water vapor (H 2 O, CO 2, and CH 4 ). These gases aborb an IR photon coming from the ground and then reradiate it in a random direction. Further collisions occur. Escape of this IR radiation is slowed down but ensuing molecular motion heats the surrounding air. The more greenhouse gases that are present the greater the degree of surface warming. These gases abosrb IT because their molecular structure makes them prone to begin rotating or vibrating when struck by a IR photon. Energy balance is not altered. Without the greenhouse effect, planet s temperature much cooler. 1

2 Planet s temperature without greenhouse affected by distance from Sun (inverse square law) and the planet s reflectivity. Black absorbs more than white. Rflectivity depends on surface composition and color. For example, the temperature of a planet s surface is roughly T = 280K 4 (1 ref) d 2. X rays ionize most gases and dissociate molecules. UV rays dissociate molecules. Visible light: blue light is scattered more than red light. IR photons abosrbed by molecules causing them to rotate and vibrate. Troposphere, Stratosphere, Thermosphere and Exosphere. Sky is blue because blue light is scattered more than red light. Sunsets are red because you are watching the beam rather than the scattered light. Greenhouse effect warms the troposhere and because more is absorbed closer to the ground, temperature drops with altitude in troposhere. Without greenhouse effect not such a difference in temp. between mountain tops and sea level. Convection in troposphere: storms, weather etc. At top of troposphere IR photons no longer collide and go into space. Now only the effect of sunlight on atmosphere. Now primary source of atmospheric heating is UV photons from Sun. This is stronger at higher altitudes so temp increases with altitude in lower stratosphere. Convection cannot occur in stratosphere because of this temp. inversion. No weather and no rain: pollution stays here. 2

3 Planet can only have a stratosphere if its atmosphere contains molecules that are good at absorbing UV photons: Ozone, O 3 plays this role on Earth. Earth is the only terrestrial world with a stratosphere. Nearly all gases are good X-ray absorbers so X rays are absorbed by the first gases they encounter in atmosphere. Desnity in exosphere too low so not much absorption there. Most X rays absorbed in thermosphere. Virtually no Xrays penetrate below thermosphere. Part of thermosphere is ionized: ionosphere. This layer reflects radio waves and hence important for communications. Exosphere is low-density boundary between atmosphere and space. High temperature but low density. Mercury and Moon have contain tiny atmpsheres: very small, no structure, essentially an exosphere. Mars, Earth and Venus have a warm troposhere at the base caused by the greenhouse effect and a warm thermosphere at the top caused by X-ray absorption. Only Earth has a stratosphere. Venus, Earth and Mars have all experienced and are experiencing the greenhouse effect in order of severity, starting with the most severe. Solar wind: outpouring of subatomic charged particles from Sun. Earth s strong magnetic field creates a magentosphere that deflects these charged particles around the planet. Some enter through the poles and reside in the Van-Allen belts encircling Earth. The interaction of these charged particles produces aurora eg. Northern lights. Climate Change Solar brightening due to the Sun brightening somewhat during its main sequence lifetime. 3

4 Tilt of the earth s axis can change due to gravitational tugs from other planets: Earth s axis changes from 22 to 25 degrees. Greater tilt means more severe seasons. These tilt changes are called Milankovitch cycles. Mars experiences more extreme changes in axis tilt than the Earth. Changes in reflectivity of a planet. One possible cause for changes in Earth s reflectivity is human activity, deforestation, smog etc. Smog is a good reflector and so one theory is that increased smog has actually reduced increasing temperatures due to increased greenhous gas emission becuase the smog reflects a lot of sunlight back. Hence efforts to clean up smog pollution may actually accelerate greenhouse warming. Changes in greenhouse gas abundance. Origin of Atmospheres During their births, planets captures some H,He but the planetesimals were too small to retain these primitive atmospheres during the solar T-Tauri phase. It is thought that volcanic outgassing has been the primary source for terrestrial atmospheres: terrestrials made up of metal and rock but impacts of ice-rich planetessimals from beyond the frost line brought in water and gas that became trapped in the interiors. This was further solidified when the crust formed and the mantle started to cool from the outside in. Volcanic outgassing releases H 2 O, CO 2, N 2, H 2 S, SO 2. It is thought that this occurred either during the molten mantle stage or as a consequence of a catastrophic collision for the Earth. Recent work though suggests that argon can stay trapped in the mantle even at very high temperatures, with mantle convection and volcanism. This suggests its is difficult for the Earth to outgass all the argon trapped in the mantle. Argon is also a byproduct of the radioactive deavy of potassium. But the earth s atmosphere contains 1of the crust is the suggestion. Thus argon trapped in the mantle billions of years ago may still be there. Mars and Venus have similar mantle materials so the situation may be similar for them as well. Can also form by evaporation of liquid of sublimation of surface ices into gases. After outgassing, some gases condense to become liquids or ices eg. Earth s oceans and polar caps. There is a continual exchange between surface liquids/ices and the atmosphere. 4

5 Outgassing is the primary origin for atmospheres on Mars, Venus and Earth. Planets can loose atmospheric gas by thermal escape, condensation, solar wind sweeping up particles, chemical reactions and large impacts blasting gases into space. For thermal escape, the average velocity of a particle, mass m is related to the temperature by V thermal = 2kT/m, so of this equals or exceeds the escape velocity of the planet, mass and radius M, R, V esc = 2GM/R, the particle will escape. Here k is Boltzmann s constant. Mars is cold and dry with a very low atmospheric pressure - water is unstable - it can evaporate easily. Because of its orbit, its distance from the Sun varies much more than the Earth and has an effect on its seasons: seasons are more extreme in the southern than northern hemispheres. Martian atmosphere is mainly CO 2, no ozone, so there is considerable UV radiation on the surface. Mars has cooled more than Earth, hence its magnetic field is much less, it lost its magnetosphere and so the solar wind was able to blow away the Martian atmosphere. Venus has a thick atmosphere with a strong greenhouse effect - thats why it is so hot. Rotates slowly, thus a weak Coriolis effect and weak winds: too hot for rain to fall. Little axis tilt implies no seasons. It may have got so hot due to a runaway greenhouse effect. Earth s planetary temperature just right for outgassed water vapour to condense and form oceans. Oceans dissolve CO 2 and moderate the greenhouse effect. The Earth s atmosphere stays stable due to the CO 2 cycle: too cool, less perciptation, rainwater dissolves less CO 2 from the atmosphere, so more CO 2 in the atmosphere which leads to a strengthened greenhouse effect. If its too warm, more precipitation, more CO 2 from atmosphere dissolves in rainwater and into oceans and less CO 2 in the atmosphere etc. 5

Lecture 23: Terrestrial Worlds in Comparison. This lecture compares and contrasts the properties and evolution of the 5 main terrestrial bodies.

Lecture 23: Terrestrial Worlds in Comparison. This lecture compares and contrasts the properties and evolution of the 5 main terrestrial bodies. Lecture 23: Terrestrial Worlds in Comparison Astronomy 141 Winter 2012 This lecture compares and contrasts the properties and evolution of the 5 main terrestrial bodies. The small terrestrial planets have

More information

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping California Standards Grades 912 Boardworks 2009 Science Contents Standards Mapping Earth Sciences Earth s Place in the Universe 1. Astronomy and planetary exploration reveal the solar system s structure,

More information

The Earth s Atmosphere

The Earth s Atmosphere THE SUN-EARTH SYSTEM III The Earth s Atmosphere Composition and Distribution of the Atmosphere The composition of the atmosphere and the way its gases interact with electromagnetic radiation determine

More information

CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles

CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles CHAPTER 5 Lectures 10 & 11 Air Temperature and Air Temperature Cycles I. Air Temperature: Five important factors influence air temperature: A. Insolation B. Latitude C. Surface types D. Coastal vs. interior

More information

ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure,

ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure, ATMOSPHERIC STRUCTURE. The vertical distribution of temperature, pressure, density, and composition of the atmosphere constitutes atmospheric structure. These quantities also vary with season and location

More information

ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation

ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation ESCI 107/109 The Atmosphere Lesson 2 Solar and Terrestrial Radiation Reading: Meteorology Today, Chapters 2 and 3 EARTH-SUN GEOMETRY The Earth has an elliptical orbit around the sun The average Earth-Sun

More information

CHAPTER 6 THE TERRESTRIAL PLANETS

CHAPTER 6 THE TERRESTRIAL PLANETS CHAPTER 6 THE TERRESTRIAL PLANETS MULTIPLE CHOICE 1. Which of the following is NOT one of the four stages in the development of a terrestrial planet? 2. That Earth, evidence that Earth differentiated.

More information

The Earth's Atmosphere. Layers of the Earth's Atmosphere

The Earth's Atmosphere. Layers of the Earth's Atmosphere The Earth's Atmosphere The atmosphere surrounds Earth and protects us by blocking out dangerous rays from the sun. The atmosphere is a mixture of gases that becomes thinner until it gradually reaches space.

More information

Review 1. Multiple Choice Identify the choice that best completes the statement or answers the question.

Review 1. Multiple Choice Identify the choice that best completes the statement or answers the question. Review 1 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. When hydrogen nuclei fuse into helium nuclei a. the nuclei die. c. particles collide. b. energy

More information

Solar Flux and Flux Density. Lecture 3: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth

Solar Flux and Flux Density. Lecture 3: Global Energy Cycle. Solar Energy Incident On the Earth. Solar Flux Density Reaching Earth Lecture 3: Global Energy Cycle Solar Flux and Flux Density Planetary energy balance Greenhouse Effect Vertical energy balance Latitudinal energy balance Seasonal and diurnal cycles Solar Luminosity (L)

More information

6 th Grade Science Assessment: Weather & Water Select the best answer on the answer sheet. Please do not make any marks on this test.

6 th Grade Science Assessment: Weather & Water Select the best answer on the answer sheet. Please do not make any marks on this test. Select the be answer on the answer sheet. Please do not make any marks on this te. 1. Weather is be defined as the A. changes that occur in cloud formations from day to day. B. amount of rain or snow that

More information

Characteristics of the. thermosphere

Characteristics of the. thermosphere Characteristics of the Atmosphere. If you were lost in the desert, you could survive for a few days without food and water. But you wouldn't last more than five minutes without the ' Objectives Describe

More information

CHAPTER 2 Energy and Earth

CHAPTER 2 Energy and Earth CHAPTER 2 Energy and Earth This chapter is concerned with the nature of energy and how it interacts with Earth. At this stage we are looking at energy in an abstract form though relate it to how it affect

More information

a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes.

a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes. J.D. McAlpine ATMS 611 HMWK #8 a) species of plants that require a relatively cool, moist environment tend to grow on poleward-facing slopes. These sides of the slopes will tend to have less average solar

More information

Section 1 The Earth System

Section 1 The Earth System Section 1 The Earth System Key Concept Earth is a complex system made up of many smaller systems through which matter and energy are continuously cycled. What You Will Learn Energy and matter flow through

More information

- 1 - Jennifer McClure. To: env.essay@physics.org. From: Jennifer McClure (j.m.mcclure@student.liverpool.ac.uk)

- 1 - Jennifer McClure. To: env.essay@physics.org. From: Jennifer McClure (j.m.mcclure@student.liverpool.ac.uk) To: env.essay@physics.org Jennifer McClure From: Jennifer McClure (j.m.mcclure@student.liverpool.ac.uk) 1 st year Physics (F300), Department of Physics, University of Liverpool. - 1 - The Northern Lights;

More information

Chapter Overview. Seasons. Earth s Seasons. Distribution of Solar Energy. Solar Energy on Earth. CHAPTER 6 Air-Sea Interaction

Chapter Overview. Seasons. Earth s Seasons. Distribution of Solar Energy. Solar Energy on Earth. CHAPTER 6 Air-Sea Interaction Chapter Overview CHAPTER 6 Air-Sea Interaction The atmosphere and the ocean are one independent system. Earth has seasons because of the tilt on its axis. There are three major wind belts in each hemisphere.

More information

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs Earth Sciences -- Grades 9, 10, 11, and 12 California State Science Content Standards Covered in: Hands-on science labs, demonstrations, & activities. Investigation and Experimentation. Lesson Plans. Presented

More information

The atmospheres of different planets

The atmospheres of different planets The atmospheres of different planets Thomas Baron October 13, 2006 1 Contents 1 Introduction 3 2 The atmosphere of the Earth 3 2.1 Description and Composition.................... 3 2.2 Discussion...............................

More information

Atmospheric Layers. Ionosphere. Exosphere. Thermosphere. Mesosphere. Stratosphere. Troposphere. mi (km) above sea level 250 (400) 50 (80) 30 (50)

Atmospheric Layers. Ionosphere. Exosphere. Thermosphere. Mesosphere. Stratosphere. Troposphere. mi (km) above sea level 250 (400) 50 (80) 30 (50) mi (km) above sea level Atmospheric Layers Exosphere 250 (400) Thermosphere Ionosphere 50 (80) Mesosphere Ozone Layer 30 (50) 7 (12) Stratosphere Troposphere Atmospheric Layers Earth s atmosphere is held

More information

Multiple Choice Identify the choice that best completes the statement or answers the question.

Multiple Choice Identify the choice that best completes the statement or answers the question. Test 2 f14 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. Carbon cycles through the Earth system. During photosynthesis, carbon is a. released from wood

More information

FACTS ABOUT CLIMATE CHANGE

FACTS ABOUT CLIMATE CHANGE FACTS ABOUT CLIMATE CHANGE 1. What is climate change? Climate change is a long-term shift in the climate of a specific location, region or planet. The shift is measured by changes in features associated

More information

CHARACTERISTICS OF THE SOLAR SYSTEM

CHARACTERISTICS OF THE SOLAR SYSTEM reflect Our solar system is made up of thousands of objects, at the center of which is a star, the Sun. The objects beyond the Sun include 8 planets, at least 5 dwarf planets, and more than 170 moons.

More information

ASTR 1010 Astronomy of the Solar System Professor Caillault Fall 2009 Semester Exam 3 Answers

ASTR 1010 Astronomy of the Solar System Professor Caillault Fall 2009 Semester Exam 3 Answers ASTR 1010 Astronomy of the Solar System Professor Caillault Fall 2009 Semester Exam 3 Answers 1. Earth's atmosphere differs from those of near-neighbor planets, Venus and Mars, in one important respect

More information

Name Period 4 th Six Weeks Notes 2015 Weather

Name Period 4 th Six Weeks Notes 2015 Weather Name Period 4 th Six Weeks Notes 2015 Weather Radiation Convection Currents Winds Jet Streams Energy from the Sun reaches Earth as electromagnetic waves This energy fuels all life on Earth including the

More information

8.5 Comparing Canadian Climates (Lab)

8.5 Comparing Canadian Climates (Lab) These 3 climate graphs and tables of data show average temperatures and precipitation for each month in Victoria, Winnipeg and Whitehorse: Figure 1.1 Month J F M A M J J A S O N D Year Precipitation 139

More information

How Do Oceans Affect Weather and Climate?

How Do Oceans Affect Weather and Climate? How Do Oceans Affect Weather and Climate? In Learning Set 2, you explored how water heats up more slowly than land and also cools off more slowly than land. Weather is caused by events in the atmosphere.

More information

CHAPTER 3 Heat and energy in the atmosphere

CHAPTER 3 Heat and energy in the atmosphere CHAPTER 3 Heat and energy in the atmosphere In Chapter 2 we examined the nature of energy and its interactions with Earth. Here we concentrate initially on the way in which energy interacts with the atmosphere

More information

Composition of the Atmosphere. Outline Atmospheric Composition Nitrogen and Oxygen Lightning Homework

Composition of the Atmosphere. Outline Atmospheric Composition Nitrogen and Oxygen Lightning Homework Molecules of the Atmosphere The present atmosphere consists mainly of molecular nitrogen (N2) and molecular oxygen (O2) but it has dramatically changed in composition from the beginning of the solar system.

More information

Temperature. PJ Brucat

Temperature. PJ Brucat PJ Brucat Temperature - the measure of average kinetic energy (KE) of a gas, liquid, or solid. KE is energy of motion. KE = ½ mv 2 where m=mass and v=velocity (speed) 1 All molecules have KE whether solid,

More information

STUDY GUIDE: Earth Sun Moon

STUDY GUIDE: Earth Sun Moon The Universe is thought to consist of trillions of galaxies. Our galaxy, the Milky Way, has billions of stars. One of those stars is our Sun. Our solar system consists of the Sun at the center, and all

More information

TEACHER BACKGROUND INFORMATION THERMAL ENERGY

TEACHER BACKGROUND INFORMATION THERMAL ENERGY TEACHER BACKGROUND INFORMATION THERMAL ENERGY In general, when an object performs work on another object, it does not transfer all of its energy to that object. Some of the energy is lost as heat due to

More information

Lesson 6: Earth and the Moon

Lesson 6: Earth and the Moon Lesson 6: Earth and the Moon Reading Assignment Chapter 7.1: Overall Structure of Planet Earth Chapter 7.3: Earth s Interior More Precisely 7-2: Radioactive Dating Chapter 7.5: Earth s Magnetosphere Chapter

More information

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits 7. Our Solar System Terrestrial & Jovian planets Seven large satellites [moons] Chemical composition of the planets Asteroids & comets The Terrestrial & Jovian Planets Four small terrestrial planets Like

More information

2. The map below shows high-pressure and low-pressure weather systems in the United States.

2. The map below shows high-pressure and low-pressure weather systems in the United States. 1. Which weather instrument has most improved the accuracy of weather forecasts over the past 40 years? 1) thermometer 3) weather satellite 2) sling psychrometer 4) weather balloon 6. Wind velocity is

More information

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets

More information

Teaching Time: One-to-two 50-minute periods

Teaching Time: One-to-two 50-minute periods Lesson Summary Students create a planet using a computer game and change features of the planet to increase or decrease the planet s temperature. Students will explore some of the same principles scientists

More information

Chapter 8 Formation of the Solar System Agenda

Chapter 8 Formation of the Solar System Agenda Chapter 8 Formation of the Solar System Agenda Announce: Mercury Transit Part 2 of Projects due next Thursday Ch. 8 Formation of the Solar System Philip on The Physics of Star Trek Radiometric Dating Lab

More information

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System Solar System Fundamentals What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System Properties of Planets What is a planet? Defined finally in August 2006!

More information

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond

Chapter 6 Formation of Planetary Systems Our Solar System and Beyond Chapter 6 Formation of Planetary Systems Our Solar System and Beyond The solar system exhibits clear patterns of composition and motion. Sun Over 99.9% of solar system s mass Made mostly of H/He gas (plasma)

More information

What Causes Climate? Use Target Reading Skills

What Causes Climate? Use Target Reading Skills Climate and Climate Change Name Date Class Climate and Climate Change Guided Reading and Study What Causes Climate? This section describes factors that determine climate, or the average weather conditions

More information

The Greenhouse Effect. Lan Ma Global Warming: Problems & Solutions 17 September, 2007

The Greenhouse Effect. Lan Ma Global Warming: Problems & Solutions 17 September, 2007 The Greenhouse Effect Lan Ma Global Warming: Problems & Solutions 17 September, 2007 What to cover today: How do we calculate the Earth s surface temperature? What makes a gas a greenhouse gas and how

More information

1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K

1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K 1. At which temperature would a source radiate the least amount of electromagnetic energy? 1) 273 K 3) 32 K 2) 212 K 4) 5 K 2. How does the amount of heat energy reflected by a smooth, dark-colored concrete

More information

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity

Seasonal & Daily Temperatures. Seasons & Sun's Distance. Solstice & Equinox. Seasons & Solar Intensity Seasonal & Daily Temperatures Seasons & Sun's Distance The role of Earth's tilt, revolution, & rotation in causing spatial, seasonal, & daily temperature variations Please read Chapter 3 in Ahrens Figure

More information

8.1 Radio Emission from Solar System objects

8.1 Radio Emission from Solar System objects 8.1 Radio Emission from Solar System objects 8.1.1 Moon and Terrestrial planets At visible wavelengths all the emission seen from these objects is due to light reflected from the sun. However at radio

More information

Chapter 8 Formation of the Solar System. What theory best explains the features of our solar system? Close Encounter Hypothesis

Chapter 8 Formation of the Solar System. What theory best explains the features of our solar system? Close Encounter Hypothesis Chapter 8 Formation of the Solar System What properties of our solar system must a formation theory explain? 1. Patterns of motion of the large bodies Orbit in same direction and plane 2. Existence of

More information

4 HOW OUR SOLAR SYSTEM FORMED 750L

4 HOW OUR SOLAR SYSTEM FORMED 750L 4 HOW OUR SOLAR SYSTEM FORMED 750L HOW OUR SOLAR SYSTEM FORMED A CLOSE LOOK AT THE PLANETS ORBITING OUR SUN By Cynthia Stokes Brown, adapted by Newsela Planets come from the clouds of gas and dust that

More information

Take away concepts. What is Energy? Solar Energy. EM Radiation. Properties of waves. Solar Radiation Emission and Absorption

Take away concepts. What is Energy? Solar Energy. EM Radiation. Properties of waves. Solar Radiation Emission and Absorption Take away concepts Solar Radiation Emission and Absorption 1. 2. 3. 4. 5. 6. Conservation of energy. Black body radiation principle Emission wavelength and temperature (Wein s Law). Radiation vs. distance

More information

The Ideal Gas Law. Gas Constant. Applications of the Gas law. P = ρ R T. Lecture 2: Atmospheric Thermodynamics

The Ideal Gas Law. Gas Constant. Applications of the Gas law. P = ρ R T. Lecture 2: Atmospheric Thermodynamics Lecture 2: Atmospheric Thermodynamics Ideal Gas Law (Equation of State) Hydrostatic Balance Heat and Temperature Conduction, Convection, Radiation Latent Heating Adiabatic Process Lapse Rate and Stability

More information

Multiple Choice Exam Questions

Multiple Choice Exam Questions Chapter 1 Multiple Choice Exam Questions 1. The primary source of energy for the earth's atmosphere is: a. energy from within the earth b. the sun c. erupting volcanoes d. lightning discharges associated

More information

Lecture 1: A Brief Survey of the Atmosphere

Lecture 1: A Brief Survey of the Atmosphere Lecture 1: A Brief Survey of the Atmosphere Origins of the atmosphere Vertical structures of the atmosphere Weather maps Thickness of the Atmosphere (from Meteorology Today) 70% The thickness of the atmosphere

More information

Layers of the Earth s Interior

Layers of the Earth s Interior Layers of the Earth s Interior 1 Focus Question How is the Earth like an ogre? 2 Objectives Explain how geologists have learned about the interior of the Earth. Describe the layers of the Earth s interior.

More information

13.1 The Nature of Gases. What is Kinetic Theory? Kinetic Theory and a Model for Gases. Chapter 13: States of Matter. Principles of Kinetic Theory

13.1 The Nature of Gases. What is Kinetic Theory? Kinetic Theory and a Model for Gases. Chapter 13: States of Matter. Principles of Kinetic Theory Chapter 13: States of Matter The Nature of Gases The Nature of Gases kinetic molecular theory (KMT), gas pressure (pascal, atmosphere, mm Hg), kinetic energy The Nature of Liquids vaporization, evaporation,

More information

Solar System Formation

Solar System Formation Solar System Formation Solar System Formation Question: How did our solar system and other planetary systems form? Comparative planetology has helped us understand Compare the differences and similarities

More information

Earth & Space Voyage Content Unit Report. Grades: 8 States: Nevada Content Standards

Earth & Space Voyage Content Unit Report. Grades: 8 States: Nevada Content Standards Earth & Space Voyage Content Unit Report Grades: 8 States: Unit 1: Exploring the Earth- Teacher's Guide pages 5B-18B: CONTENT STANDARD NV.N.8.A. Scientific Inquiry (Nature of Unifying graphs. opinion.

More information

Assignment 5. Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.

Assignment 5. Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Assignment 5 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. 1. What is the single most important reason that astronomers have learned more

More information

The Main Point. Lecture #34: Solar System Origin II. Chemical Condensation ( Lewis ) Model. How did the solar system form? Reading: Chapter 8.

The Main Point. Lecture #34: Solar System Origin II. Chemical Condensation ( Lewis ) Model. How did the solar system form? Reading: Chapter 8. Lecture #34: Solar System Origin II How did the solar system form? Chemical Condensation ("Lewis") Model. Formation of the Terrestrial Planets. Formation of the Giant Planets. Planetary Evolution. Reading:

More information

Chemistry 13: States of Matter

Chemistry 13: States of Matter Chemistry 13: States of Matter Name: Period: Date: Chemistry Content Standard: Gases and Their Properties The kinetic molecular theory describes the motion of atoms and molecules and explains the properties

More information

Earth in the Solar System

Earth in the Solar System Copyright 2011 Study Island - All rights reserved. Directions: Challenge yourself! Print out the quiz or get a pen/pencil and paper and record your answers to the questions below. Check your answers with

More information

Summary: Four Major Features of our Solar System

Summary: Four Major Features of our Solar System Summary: Four Major Features of our Solar System How did the solar system form? According to the nebular theory, our solar system formed from the gravitational collapse of a giant cloud of interstellar

More information

ATM S 111, Global Warming: Understanding the Forecast

ATM S 111, Global Warming: Understanding the Forecast ATM S 111, Global Warming: Understanding the Forecast DARGAN M. W. FRIERSON DEPARTMENT OF ATMOSPHERIC SCIENCES DAY 1: OCTOBER 1, 2015 Outline How exactly the Sun heats the Earth How strong? Important concept

More information

Chapter 6: Cloud Development and Forms

Chapter 6: Cloud Development and Forms Chapter 6: Cloud Development and Forms (from The Blue Planet ) Why Clouds Form Static Stability Cloud Types Why Clouds Form? Clouds form when air rises and becomes saturated in response to adiabatic cooling.

More information

2007 Pearson Education Inc., publishing as Pearson Addison-Wesley. The Jovian Planets

2007 Pearson Education Inc., publishing as Pearson Addison-Wesley. The Jovian Planets The Jovian Planets The Jovian planets are gas giants - much larger than Earth Sizes of Jovian Planets Planets get larger as they get more massive up to a point... Planets more massive than Jupiter are

More information

Radiation Transfer in Environmental Science

Radiation Transfer in Environmental Science Radiation Transfer in Environmental Science with emphasis on aquatic and vegetation canopy media Autumn 2008 Prof. Emmanuel Boss, Dr. Eyal Rotenberg Introduction Radiation in Environmental sciences Most

More information

astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.

astronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,

More information

Current Staff Course Unit/ Length. Basic Outline/ Structure. Unit Objectives/ Big Ideas. Properties of Waves A simple wave has a PH: Sound and Light

Current Staff Course Unit/ Length. Basic Outline/ Structure. Unit Objectives/ Big Ideas. Properties of Waves A simple wave has a PH: Sound and Light Current Staff Course Unit/ Length August August September September October Unit Objectives/ Big Ideas Basic Outline/ Structure PS4- Types of Waves Because light can travel through space, it cannot be

More information

UNIVERSITY OF VICTORIA CHEMISTRY 102 Midterm Test 1 January 31, 2014 5-6 pm (60 minutes) DISPLAY YOUR STUDENT ID CARD ON THE TOP OF YOUR DESK NOW

UNIVERSITY OF VICTORIA CHEMISTRY 102 Midterm Test 1 January 31, 2014 5-6 pm (60 minutes) DISPLAY YOUR STUDENT ID CARD ON THE TOP OF YOUR DESK NOW Version B UNIVERSITY OF VICTORIA CHEMISTRY 102 Midterm Test 1 January 31, 2014 5-6 pm (60 minutes) Version B DISPLAY YOUR STUDENT ID CARD ON THE TOP OF YOUR DESK NOW Answer all multiple choice questions

More information

Clouds and the Energy Cycle

Clouds and the Energy Cycle August 1999 NF-207 The Earth Science Enterprise Series These articles discuss Earth's many dynamic processes and their interactions Clouds and the Energy Cycle he study of clouds, where they occur, and

More information

Cloud Radiation and the Law of Attraction

Cloud Radiation and the Law of Attraction Convec,on, cloud and radia,on Convection redistributes the thermal energy yielding (globally-averaged), a mean lapse rate of ~ -6.5 o C/km. Radiative processes tend to produce a more negative temperature

More information

Related Standards and Background Information

Related Standards and Background Information Related Standards and Background Information Earth Patterns, Cycles and Changes This strand focuses on student understanding of patterns in nature, natural cycles, and changes that occur both quickly and

More information

Solar Nebula Theory. Basic properties of the Solar System that need to be explained:

Solar Nebula Theory. Basic properties of the Solar System that need to be explained: Solar Nebula Theory Basic properties of the Solar System that need to be explained: 1. All planets orbit the Sun in the same direction as the Sun s rotation 2. All planetary orbits are confined to the

More information

Corso di Fisica Te T cnica Ambientale Solar Radiation

Corso di Fisica Te T cnica Ambientale Solar Radiation Solar Radiation Solar radiation i The Sun The Sun is the primary natural energy source for our planet. It has a diameter D = 1.39x10 6 km and a mass M = 1.989x10 30 kg and it is constituted by 1/3 of He

More information

Explain the Big Bang Theory and give two pieces of evidence which support it.

Explain the Big Bang Theory and give two pieces of evidence which support it. Name: Key OBJECTIVES Correctly define: asteroid, celestial object, comet, constellation, Doppler effect, eccentricity, eclipse, ellipse, focus, Foucault Pendulum, galaxy, geocentric model, heliocentric

More information

Science Standard 4 Earth in Space Grade Level Expectations

Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal

More information

ORANGE PUBLIC SCHOOLS OFFICE OF CURRICULUM AND INSTRUCTION OFFICE OF SCIENCE. GRADE 6 SCIENCE Post - Assessment

ORANGE PUBLIC SCHOOLS OFFICE OF CURRICULUM AND INSTRUCTION OFFICE OF SCIENCE. GRADE 6 SCIENCE Post - Assessment ORANGE PUBLIC SCHOOLS OFFICE OF CURRICULUM AND INSTRUCTION OFFICE OF SCIENCE GRADE 6 SCIENCE Post - Assessment School Year 2013-2014 Directions for Grade 6 Post-Assessment The Grade 6 Post-Assessment is

More information

Chapter 2: Solar Radiation and Seasons

Chapter 2: Solar Radiation and Seasons Chapter 2: Solar Radiation and Seasons Spectrum of Radiation Intensity and Peak Wavelength of Radiation Solar (shortwave) Radiation Terrestrial (longwave) Radiations How to Change Air Temperature? Add

More information

Lecture 10 Formation of the Solar System January 6c, 2014

Lecture 10 Formation of the Solar System January 6c, 2014 1 Lecture 10 Formation of the Solar System January 6c, 2014 2 Orbits of the Planets 3 Clues for the Formation of the SS All planets orbit in roughly the same plane about the Sun. All planets orbit in the

More information

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation Outline MAE 493R/593V- Renewable Energy Devices Solar Energy Electromagnetic wave Solar spectrum Solar global radiation Solar thermal energy Solar thermal collectors Solar thermal power plants Photovoltaics

More information

Introduction to Chapter 27

Introduction to Chapter 27 9 Heating and Cooling Introduction to Chapter 27 What process does a hot cup of coffee undergo as it cools? How does your bedroom become warm during the winter? How does the cooling system of a car work?

More information

Multiple Choice For questions 1-10, circle only one answer.

Multiple Choice For questions 1-10, circle only one answer. Test Bank - Chapter 1 The questions in the test bank cover the concepts from the lessons in Chapter 1. Select questions from any of the categories that match the content you covered with students. The

More information

Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy.

Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy. Electromagnetic Radiation Energy that comes to us from the sun is transported in the form of waves known as electromagnetic energy. This combines electricity and magnetism such that setting up an electric

More information

AZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred.

AZ State Standards. Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred. Forms of Energy AZ State Standards Concept 3: Conservation of Energy and Increase in Disorder Understand ways that energy is conserved, stored, and transferred. PO 1. Describe the following ways in which

More information

What Is Heat? What Is Heat?

What Is Heat? What Is Heat? What Is Heat? Paul shivered inside the wood cabin. It was cold outside, and inside the cabin it wasn t much warmer. Paul could hear the rain beating down on the roof. Every few minutes there would be a

More information

INSPIRE GK12 Lesson Plan. The Chemistry of Climate Change Length of Lesson

INSPIRE GK12 Lesson Plan. The Chemistry of Climate Change Length of Lesson Lesson Title The Chemistry of Climate Change Length of Lesson 180 min Created By David Wilson Subject Physical Science / Chemistry / Organic Chemistry Grade Level 8-12 State Standards 2c, 4d / 2a, 4d /

More information

Understanding Basic Concepts demonstrate an awareness of air as a substance that surrounds us and takes up space, and whose movement we feel as wind

Understanding Basic Concepts demonstrate an awareness of air as a substance that surrounds us and takes up space, and whose movement we feel as wind Designation: Ontario Curriculum: Science and Technology Earth and Space Systems: Grade 2 Air and Water in the Environment Written by: Andrea Schultz-Allison, Department of Earth Sciences, The University

More information

1. The Kinetic Theory of Matter states that all matter is composed of atoms and molecules that are in a constant state of constant random motion

1. The Kinetic Theory of Matter states that all matter is composed of atoms and molecules that are in a constant state of constant random motion Physical Science Period: Name: ANSWER KEY Date: Practice Test for Unit 3: Ch. 3, and some of 15 and 16: Kinetic Theory of Matter, States of matter, and and thermodynamics, and gas laws. 1. The Kinetic

More information

Every mathematician knows it is impossible to understand an elementary course in thermodynamics. ~V.I. Arnold

Every mathematician knows it is impossible to understand an elementary course in thermodynamics. ~V.I. Arnold Every mathematician knows it is impossible to understand an elementary course in thermodynamics. ~V.I. Arnold Radiation Radiation: Heat energy transmitted by electromagnetic waves Q t = εσat 4 emissivity

More information

7613-1 - Page 1. Weather Unit Exam Pre-Test Questions

7613-1 - Page 1. Weather Unit Exam Pre-Test Questions Weather Unit Exam Pre-Test Questions 7613-1 - Page 1 Name: 1) Equal quantities of water are placed in four uncovered containers with different shapes and left on a table at room temperature. From which

More information

ESCI-61 Introduction to Photovoltaic Technology. Solar Radiation. Ridha Hamidi, Ph.D.

ESCI-61 Introduction to Photovoltaic Technology. Solar Radiation. Ridha Hamidi, Ph.D. 1 ESCI-61 Introduction to Photovoltaic Technology Solar Radiation Ridha Hamidi, Ph.D. 2 The Sun The Sun is a perpetual source of energy It has produced energy for about 4.6 billions of years, and it is

More information

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: Water in Earth s Processes. (Approximate Time: 5-6 Weeks)

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: Water in Earth s Processes. (Approximate Time: 5-6 Weeks) The following instructional plan is part of a GaDOE collection of Unit Frameworks, Performance Tasks, examples of Student Work, and Teacher Commentary. Many more GaDOE approved instructional plans are

More information

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly

More information

Seasonal Temperature Variations

Seasonal Temperature Variations Seasonal and Daily Temperatures Fig. 3-CO, p. 54 Seasonal Temperature Variations What causes the seasons What governs the seasons is the amount of solar radiation reaching the ground What two primary factors

More information

The Atmosphere and Winds

The Atmosphere and Winds Oceanography 10, T. James Noyes, El Camino College 8A-1 The Atmosphere and Winds We need to learn about the atmosphere, because the ocean and atmosphere are tightly interconnected with one another: you

More information

Lecture 12: The Solar System Briefly

Lecture 12: The Solar System Briefly Lecture 12: The Solar System Briefly Formation of the Moonhttp://www.youtube.com/watch?v=WpOKztEiMqo&feature =related Formation of our Solar System Conservation of Angular Momentum Why are the larger,

More information

The Sun: Our nearest star

The Sun: Our nearest star The Sun: Our nearest star Property Surface T Central T Luminosity Mass Lifetime (ms) Value 5500K 15x10 6 K 2 x 10 33 ergs 4 x 10 33 grams 10 billion years Solar Structure Build a model and find the central

More information

Chapter 8 Welcome to the Solar System

Chapter 8 Welcome to the Solar System Chapter 8 Welcome to the Solar System 8.1 The Search for Origins What properties of our solar system must a formation theory explain? What theory best explains the features of our solar system? What properties

More information

Essential Standards: Grade 4 Science Unpacked Content

Essential Standards: Grade 4 Science Unpacked Content This document is designed to help North Carolina educators teach the Essential Standards (Standard Course of Study). NCDPI staff are continually updating and improving these tools to better serve teachers.

More information

Geol 116 The Planet Class 7-1 Feb 28, 2005. Exercise 1, Calculate the escape velocities of the nine planets in the solar system

Geol 116 The Planet Class 7-1 Feb 28, 2005. Exercise 1, Calculate the escape velocities of the nine planets in the solar system Exercises/Discussions Atmospheric Composition: Escape Velocities and Surface Temperature Objectives Escape velocity and the mass and size of a planetary body The effect of escape velocity and surface temperature

More information

Introduction and Origin of the Earth

Introduction and Origin of the Earth Page 1 of 5 EENS 1110 Tulane University Physical Geology Prof. Stephen A. Nelson Introduction and Origin of the Earth This page last updated on 30-Jul-2015 Geology, What is it? Geology is the study of

More information

Solar System Overview

Solar System Overview Solar System Overview Planets: Four inner planets, Terrestrial planets Four outer planets, Jovian planets Asteroids: Minor planets (planetesimals) Meteroids: Chucks of rocks (smaller than asteroids) (Mercury,

More information