b) Would the average albedo of the Earth increase or decrease? Why? (2 points) The average albedo of the Earth would decrease.

Size: px
Start display at page:

Download "b) Would the average albedo of the Earth increase or decrease? Why? (2 points) The average albedo of the Earth would decrease."

Transcription

1 EPS 5 Spring 2010 Problem Set 2 Due Wed, Feb. 17, 2010 (at the beginning of lecture) 1. Climate change and albedo feedbacks (16 points) a) Although 70% of the Earth's surface is covered by ocean, Earth's average albedo is 0.33 (Approximately 33% of the incoming solar energy is reflected back to space). Using the table below, explain why the average albedo of the Earth is so high. (2 points) Surface cover Albedo Fresh snow Clouds Ice 0.35 Desert Grassland Ocean 0.05 Forest 0.1 While 70% of the Earth's surface is covered by ocean (with a low albedo of 0.05), 30% of the Earth's surface is covered by land surfaces that all have a higher albedo. Given the known distribution of land and ocean, the Earth's albedo would never reach 0.33 without the influence of clouds. Clouds are very reflective, and they prevent a significant portion of solar radiation from ever reaching the surface of the Earth. Now consider the effect of snow cover on the Earth s albedo. Suppose that in the next twenty years, snow cover retreats by 5%. b) Would the average albedo of the Earth increase or decrease? Why? (2 points) The average albedo of the Earth would decrease. Land covered with snow has a high albedo. Replacing snow cover with land surfaces that have a lower albedo would decrease the average albedo of the Earth. c) If all other factors were held constant, what would happen to the average temperature? Why? (2 points) The temperature of the Earth would increase. Less of the energy from the sun is reflected, more is absorbed and reemitted by the ground. d) Based on your answer in c), do you think the snowmelt will continue? Explain why. Is this a positive or a negative feedback, or neither? (2 points) The snowmelt would continue this is an example of a positive feedback. Earth warms -> snow cover retreats -> albedo decreases -> Earth warms some more -> snow cover retreats some more -> albedo continues to decrease -> etc. e) In 1980, the area of sea ice in the Arctic at the annual minimum was around 7 million square kilometers. In 2007, the minimum area was around 4 million square kilometers. Consider the Arctic

2 Ocean to be a 10 million square kilometer box composed of sea ice and ocean. What was the albedo at the minimum sea ice extent in 1980? What was it in 2007? (2 points) 1980: A = 0.7* *0.05 = : A = 0.4* *0.05 = 0.17 f) Following up to part e), consider the one-layer greenhouse model from the previous class, just for the Arctic Ocean box. Do not consider clouds. Use a solar constant appropriate for Arctic summer, F s = 2000 W/m 2 and number of atmospheric layers n = 1. How much does the ground temperature in this simple energy balance change between 1980 and 2007? How much does the effective temperature change over the same period? (5 points) Energy balances (2 points) (1) Whole system: Fs(1-A)/4 = σt1 4 (2) Ground: Fs(1-A)/4 + σt1 4 = σtg 4 (3) Atmosphere: σtg 4 = 2σT : T1 = [Fs(1-A)/4σ] 1/4 = [2000(1-0.26)/(4*5.67x10-8 )] 1/4 = K Tg = (2T1 4 ) 1/4 = K 2007: T1 = [Fs(1-A)/4σ] 1/4 = [2000(1-0.17)/(4*5.67x10-8 )] 1/4 = K Tg = (2T1 4 ) 1/4 = K Tg = 9.8 K Te = 8.3 K g) The ground temperatures you calculated for the simplified model in part f) are much higher than actual ground temperatures in the Arctic. What are some reasons why this model may be unrealistic in this scenario? The global average for n is around 0.7, and it is likely lower in the Arctic. We only considered ocean and ice, while land is also present at high latitudes and would have a higher albedo than ocean. There is considerable heat capacity in the Arctic Ocean. There is significant transport of heat away. 2. Short questions on feedback (3 points) a) As the concentration of CO 2 increases in the atmosphere, some plants may be able to grow more and take up more CO 2 for photosynthesis and storage as organic matter in their tissues. Is this a positive or negative feedback for atmospheric CO 2 concentrations? Negative feedback. Higher CO2 More uptake Lower CO2. b) As the concentration of CO 2 increases in the atmosphere, the ocean will become more acidic and be able to take up a smaller fraction of atmospheric CO 2 in the future. (We will learn more about this when we study the carbon cycle) Is this a positive or a negative feedback for atmospheric CO 2 concentrations?

3 Positive feedback. Higher CO2 Less uptake Higher CO2 Less uptake. c) As the climate warms, there may be more forest fires, which emit black soot to the atmosphere. Is this a positive or a negative feedback for climate change? Positive feedback. Warmer More fires More black soot Warmer More fires. 3. Scale heights (11 points) a) On Mars, the atmosphere is 95.72% carbon dioxide (you may assume all CO 2 for the purposes of this question). The temperature is 220K, and the acceleration of gravity is 3.7 m s -2. What the scale height of the Martian atmosphere? How is the scale height of the Earth s atmosphere different from the scale height of Mars? Why? (Remember, the scale height of the Earth s atmospheres = 7.4 km.) (3 points) Scale height H = RT/Mag R = J mol -1 K -1 T = 220 K M = kg mol -1 g = 3.7 m s -2 H = (8.314*220)/(0.044*3.7) = 11.2 km This is larger than the scale height of the Earth s atmosphere. The atmosphere of Mars extends deeper because of smaller size of Mars and the resulting weaker gravitational pull on its atmosphere. b) In case of Venus, the atmosphere is 96.5% carbon dioxide, so you may again assume ALL). The temperature is735k, and the acceleration of gravity is 8.9 ms -2. What the scale height of Venus atmosphere? Compare to the scale height of the Earth s and Mars atmosphere. (3 points) Scale height H = RT/Mag R = J mol -1 K -1 T = 735 K M = kg mol -1 g = 8.9 m s -2 H = (8.314*735)/(0.044*8.9) = 15.6 km Venus has a similar gravitational pull on the atmosphere compared to the Earth, but its much hotter temperature leads to a much larger scale height than Earth. c) You might have wondered if the scale height varies around the Earth. The temperature around the Earth affects the scale height. Calculate the scale height for the equator (280K) and the poles (250K). Which is larger? By what percentage? (3 points) Equator: H = (8.314*280)/(0.029*9.8) = 8.2 km Pole: H = (8.314*250)/(0.029*9.8) = 7.3 km Percent: ( )/7.3 = % greater scale height at the equator.

4 The scale height is larger at the equator, due to the higher atmospheric temperature. The equator-pole difference is 12%, the same as the difference in temperatures. For many purposes this difference is not important, so we usually treat scale height as constant. d) Describe in your own words the definition of scale height. Why is it a useful concept? (2 points) Scale height describes the relationship between pressure and altitude. For every increase in altitude of H, pressure falls off by a factor of e. A plot of altitude versus the natural log of pressure is a straight line with a slope of -H. Scale height is a measure of depth and can be thought of as the thickness of an atmospheric layer. (2 points) 4. Barometric law (8 points) a) Calculate the concentration, in moles per liter, of oxygen at sea level. Pressure at sea level is 1013 hpa. In this case, use a surface temperature of 280 K. Oxygen comprises 21% of the atmosphere. (2 points) PV = NkT air concentration = N/AvV = P/AvkT = (1.013x10 5 ) / (6.022x10 23 * 1.38x10-23 * 280) =43.5 mol m -3 oxygen concentration = 0.21 * 43.5 mol m -3 * (1 m 3 / 1000 L) = 9.14x10-3 mol L -1 b) Assume the altitude of Mt. Everest is 9km. Calculate the pressure at the top of Mt. Everest, given a 7.4km scale height. (2 points) P = P0e -z/h P = (1.013x10 5 )e (-9/7.4) = 300 hpa c) Calculate the concentration, in moles per liter, of oxygen at the top of Mt. Everest. Assume the temperature at the top of Mt. Everest is 215K. (2 points) PV = NkT air concentration = N/AvV = P/AvkT = (3.00x10 4 ) / (6.022x10 23 * 1.38x10-23 * 215) =16.8 mol m -3 oxygen concentration = 0.21 * 16.8 mol m -3 * (1 m 3 / 1000 L) = 3.53x10-3 mol L -1 d) Imagine that you've just hiked up Mount Everest and you're standing on top of the summit savoring the moment. You love atmospheric science, of course, so you've brought a very special, massless, incompressible Nalgene bottle to fill with the summit air to take back home with you. You open the bottle and let the air waft in, then close it. You accidentally drop the magic bottle. Does it sink, rise or stay in about the same place? Why? In 2005, a stunt pilot landed a helicopter on the summit of Mount Everest. Imagine the helicopter cabin is pressurized to sea level (not the case, but we're imagining) and is at the same temperature as the outside summit air. The pilot has also brought a magic bottle to bring home some souvenir mountain air, but he doesn't want to get out of the cabin. He lets the air into his bottle then closes it. He thinks better of it and decides to get out of the helicopter after all. He brings the bottle of air and drops it. Does it sink, rise, or stay in the same place? Why?

5 Your magic bottle of air stays in about the same place because it is the same density as the surrounding atmosphere. The bottle of air from the helicopter sinks because it is pressurized at sea level and is more dense than the surrounding atmosphere.

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems

The Atmosphere. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems. Topic 3: Global Cycles and Physical Systems The Atmosphere 1 How big is the atmosphere? Why is it cold in Geneva? Why do mountaineers need oxygen on Everest? 2 A relatively thin layer of gas over the Earths surface Earth s radius ~ 6400km Atmospheric

More information

Let s Think for a Second

Let s Think for a Second Weather and Climate Let s Think for a Second Why is weather important in Ohio? Is climate important in Ohio? Spend 2 minutes sharing your thoughts with 1 partner. First, Let s Watch This. http://video.nationalgeographic.com/video/science/earthsci/climate-weather-sci/

More information

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1

CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1 CLIMATE AND CLIMATE CHANGE MIDTERM EXAM ATM S 211 FEB 9TH 2012 V1 Name: Student ID: Please answer the following questions on your Scantron Multiple Choice [1 point each] (1) The gases that contribute to

More information

PTYS 214 Spring Announcements. Midterm 3 next Thursday!

PTYS 214 Spring Announcements. Midterm 3 next Thursday! PTYS 214 Spring 2018 Announcements Midterm 3 next Thursday! 1 Previously Habitable Zone Energy Balance Emission Temperature Greenhouse Effect Vibration/rotation bands 2 Recap: Greenhouse gases In order

More information

Lecture 2: Light And Air

Lecture 2: Light And Air Lecture 2: Light And Air Earth s Climate System Earth, Mars, and Venus Compared Solar Radiation Greenhouse Effect Thermal Structure of the Atmosphere Atmosphere Ocean Solid Earth Solar forcing Land Energy,

More information

Lecture 4: Global Energy Balance

Lecture 4: Global Energy Balance Lecture : Global Energy Balance S/ * (1-A) T A T S T A Blackbody Radiation Layer Model Greenhouse Effect Global Energy Balance terrestrial radiation cooling Solar radiation warming Global Temperature atmosphere

More information

National Center for Atmospheric Research: Climate Discovery Teacher s Guide

National Center for Atmospheric Research: Climate Discovery Teacher s Guide Lesson Summary Students use a photo of the Bhutan glaciers in order to investigate the different effects albedo has on solar absorption. Prior Knowledge & Skills Graphing skills Data collection skills

More information

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model.

Lecture 4: Global Energy Balance. Global Energy Balance. Solar Flux and Flux Density. Blackbody Radiation Layer Model. Lecture : Global Energy Balance Global Energy Balance S/ * (1-A) terrestrial radiation cooling Solar radiation warming T S Global Temperature Blackbody Radiation ocean land Layer Model energy, water, and

More information

Build Your Own Planet Lesson 4: Atmosphere

Build Your Own Planet Lesson 4: Atmosphere Build Your Own Planet Lesson 4: Atmosphere Group: Does the atmosphere of a planet affect its surface temperature? If so, how? This lesson will explore that question. The gases that surround a planet are

More information

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

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds Chapter 10 Lecture The Cosmic Perspective Seventh Edition Planetary Atmospheres: Earth and the Other Terrestrial Worlds Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics

More information

Weather Forecasts and Climate AOSC 200 Tim Canty. Class Web Site: Lecture 27 Dec

Weather Forecasts and Climate AOSC 200 Tim Canty. Class Web Site:   Lecture 27 Dec Weather Forecasts and Climate AOSC 200 Tim Canty Class Web Site: http://www.atmos.umd.edu/~tcanty/aosc200 Topics for today: Climate Natural Variations Feedback Mechanisms Lecture 27 Dec 4 2018 1 Climate

More information

Website Lecture 3 The Physical Environment Part 1

Website   Lecture 3 The Physical Environment Part 1 Website http://websites.rcc.edu/halama Lecture 3 The Physical Environment Part 1 1 Lectures 3 & 4 1. Biogeochemical Cycling 2. Solar Radiation 3. The Atmosphere 4. The Global Ocean 5. Weather and Climate

More information

Introduction to Atmospheric Circulation

Introduction to Atmospheric Circulation Introduction to Atmospheric Circulation Start rotating table Cloud Fraction Dice Results from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/ from http://eos.atmos.washington.edu/erbe/

More information

Light Up Your World Adapted from Reflecting on Reflectivity,

Light Up Your World Adapted from Reflecting on Reflectivity, Climate Change I m Supposed To Know What That Is? Light Up Your World Adapted from Reflecting on Reflectivity, http://www.climatechangenorth.ca Overview: Students often confuse global warming and the depletion

More information

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens Prentice Hall EARTH SCIENCE Tarbuck Lutgens Chapter 17 The Atmosphere: Structure and Temperature 17.1 Atmosphere Characteristics Composition of the Atmosphere Weather is constantly changing, and it refers

More information

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface.

Earth s Atmosphere. Energy Transfer in the Atmosphere. 3. All the energy from the Sun reaches Earth s surface. CHAPTER 11 LESSON 2 Earth s Atmosphere Energy Transfer in the Atmosphere Key Concepts How does energy transfer from the Sun to Earth and to the atmosphere? How are air circulation patterns within the atmosphere

More information

Lecture 7: Natural Climate Change. Instructor: Prof. Johnny Luo.

Lecture 7: Natural Climate Change. Instructor: Prof. Johnny Luo. Lecture 7: Natural Climate Change Instructor: Prof. Johnny Luo http://www.sci.ccny.cuny.edu/~luo Final Exam: May 23 1-3:15pm at MR O44 Outlines (Chapter 11, Edition 1) 1. Variation in solar luminosity

More information

Hydrosphere The hydrosphere includes all water on Earth.

Hydrosphere The hydrosphere includes all water on Earth. Hydrosphere The hydrosphere includes all water on Earth. The abundance of water on Earth is a unique feature that clearly distinguishes our "Blue Planet" from others in the solar system. Not a drop of

More information

Climate Change and Biomes

Climate Change and Biomes Climate Change and Biomes Key Concepts: Greenhouse Gas WHAT YOU WILL LEARN Biome Climate zone Greenhouse gases 1. You will learn the difference between weather and climate. 2. You will analyze how climate

More information

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

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc. Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Lecture 2 Global and Zonal-mean Energy Balance

Lecture 2 Global and Zonal-mean Energy Balance Lecture 2 Global and Zonal-mean Energy Balance A zero-dimensional view of the planet s energy balance RADIATIVE BALANCE Roughly 70% of the radiation received from the Sun at the top of Earth s atmosphere

More information

Major climate change triggers

Major climate change triggers Major climate change triggers Variations in solar output Milankovitch cycles Elevation & distribution of continents Ocean interactions Atmospheric composition change (CO 2 and other volcanic gasses) Biological

More information

Introduction to Atmospheric Circulation

Introduction to Atmospheric Circulation Introduction to Atmospheric Circulation Start rotating table Start heated bottle experiment Scientific Practice Observe nature Develop a model*/hypothesis for what is happening Carry out experiments Make

More information

The Atmosphere: Structure and Temperature

The Atmosphere: Structure and Temperature Chapter The Atmosphere: Structure and Temperature Geologists have uncovered evidence of when Earth was first able to support oxygenrich atmosphere similar to what we experience today and more so, take

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? 10.1 Atmospheric Basics Our goals for learning:! What is an atmosphere?! How does the greenhouse effect warm

More information

Seasonal & Diurnal Temp Variations. Earth-Sun Distance. Eccentricity 2/2/2010. ATS351 Lecture 3

Seasonal & Diurnal Temp Variations. Earth-Sun Distance. Eccentricity 2/2/2010. ATS351 Lecture 3 Seasonal & Diurnal Temp Variations ATS351 Lecture 3 Earth-Sun Distance Change in distance has only a minimal effect on seasonal temperature. Note that during the N. hemisphere winter, we are CLOSER to

More information

Astron 104 Laboratory #10 Solar Energy and the Habitable Zone

Astron 104 Laboratory #10 Solar Energy and the Habitable Zone Name: Date: Section: Astron 104 Laboratory #10 Solar Energy and the Habitable Zone Introduction The Sun provides most of the energy available in the solar system. Sunlight warms the planet and helps create

More information

Lecture 3: Global Energy Cycle

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

More information

Investigating Planets Name: Block: E1:R6

Investigating Planets Name: Block: E1:R6 FYI: Planetary Temperatures and Atmospheres Read FYI: A Planet s Temperature, The Importance of an Atmosphere, and The Greenhouse Effect As you read answer the following questions about the readings: Word/Term

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement

Table of Contents. Chapter: Atmosphere. Section 1: Earth's Atmosphere. Section 2: Energy Transfer in the Atmosphere. Section 3: Air Movement Table of Contents Chapter: Atmosphere Section 1: Earth's Atmosphere Section 2: Energy Transfer in the Atmosphere Section 3: Air Movement Table of Contents Chapter: Atmosphere Section 2: Energy Transfer

More information

GEOGRAPHY EYA NOTES. Weather. atmosphere. Weather and climate

GEOGRAPHY EYA NOTES. Weather. atmosphere. Weather and climate GEOGRAPHY EYA NOTES Weather and climate Weather The condition of the atmosphere at a specific place over a relatively short period of time Climate The atmospheric conditions of a specific place over a

More information

Atmosphere, Weather & Climate Review for Unit Assessment (Can be taken on Study Island Due Mon., 11/26/12)

Atmosphere, Weather & Climate Review for Unit Assessment (Can be taken on Study Island Due Mon., 11/26/12) Name Class Period Atmosphere, Weather & Climate Review for Unit Assessment (Can be taken on Study Island Due Mon., 11/26/12) 1. When hot and cold air meet, the hot air rises to the top. Which process causes

More information

2. Fargo, North Dakota receives more snow than Charleston, South Carolina.

2. Fargo, North Dakota receives more snow than Charleston, South Carolina. 2015 National Tournament Division B Meteorology Section 1: Weather versus Climate Chose the answer that best answers the question 1. The sky is partly cloudy this morning in Lincoln, Nebraska. 2. Fargo,

More information

All objects emit radiation. Radiation Energy that travels in the form of waves Waves release energy when absorbed by an object. Earth s energy budget

All objects emit radiation. Radiation Energy that travels in the form of waves Waves release energy when absorbed by an object. Earth s energy budget Radiation Energy that travels in the form of waves Waves release energy when absorbed by an object Example: Sunlight warms your face without necessarily heating the air Shorter waves carry more energy

More information

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown

G109 Alternate Midterm Exam October, 2004 Instructor: Dr C.M. Brown 1 Time allowed 50 mins. Answer ALL questions Total possible points;50 Number of pages:8 Part A: Multiple Choice (1 point each) [total 24] Answer all Questions by marking the corresponding number on the

More information

- global radiative energy balance

- global radiative energy balance (1 of 14) Further Reading: Chapter 04 of the text book Outline - global radiative energy balance - insolation and climatic regimes - composition of the atmosphere (2 of 14) Introduction Last time we discussed

More information

Extrasolar planets Detection and habitability

Extrasolar planets Detection and habitability Extrasolar planets Detection and habitability October 23rd 2014 Detecting exoplanets Primary methods : Direct imaging Transit Radial velocity Direct imaging Planets are much fainter than their host star

More information

The heavier temperature lines 160,000 BP to present reflect more data points for this time period, not necessarily greater temperature variability.

The heavier temperature lines 160,000 BP to present reflect more data points for this time period, not necessarily greater temperature variability. Climate change Issues for Science A-30 students to consider Is climate getting warmer? How much warmer (if yes)? How do we know? If climate is getting warmer, why is it getting warmer? How do we know?

More information

Clouds and Rain Unit (3 pts)

Clouds and Rain Unit (3 pts) Name: Section: Clouds and Rain Unit (Topic 8A-2) page 1 Clouds and Rain Unit (3 pts) As air rises, it cools due to the reduction in atmospheric pressure Air mainly consists of oxygen molecules and nitrogen

More information

Lungs of the Planet with Dr. Michael Heithaus

Lungs of the Planet with Dr. Michael Heithaus Lungs of the Planet with Dr. Michael Heithaus Problem Why do people call rain forests the lungs of the planet? Usually it is because people think that the rain forests produce most of the oxygen we breathe.

More information

The greenhouse effect

The greenhouse effect The greenhouse effect Visible light arrives About half reflected, half is absorbed by the ground. This absorbed energy is then reradiated, but NOT in the visible (would just go out again anyway); in the

More information

Lungs of the Planet. 1. Based on the equations above, describe how the processes of photosynthesis and cellular respiration relate to each other.

Lungs of the Planet. 1. Based on the equations above, describe how the processes of photosynthesis and cellular respiration relate to each other. Lungs of the Planet Name: Date: Why do people call rain forests the lungs of the planet? Usually it is because people think that the rain forests produce most of the oxygen we breathe. But do they? To

More information

Closed Book. The time allowed for Part A plus Part B in total is 75 minutes.

Closed Book. The time allowed for Part A plus Part B in total is 75 minutes. 1 -Test 1 Closed Book. The time allowed for Part A plus Part B in total is 75 minutes. Answers are to be written on the answer sheets given (one sheet for Part A and another for Part B). PART A 1. Lake

More information

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely

1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely CHAPTER 3 SOLAR AND TERRESTRIAL RADIATION MULTIPLE CHOICE QUESTIONS 1. The frequency of an electromagnetic wave is proportional to its wavelength. a. directly *b. inversely 2. is the distance between successive

More information

PRE-LAB FOR PLANETARY ATMOSPHERES

PRE-LAB FOR PLANETARY ATMOSPHERES PRE-LAB FOR PLANETARY ATMOSPHERES 1. Find pictures of Venus, Earth, and Mars in an astronomy textbook or other book or online at a website. Estimate, to the nearest 10%, the percentage of surface of each

More information

General Comments about the Atmospheres of Terrestrial Planets

General Comments about the Atmospheres of Terrestrial Planets General Comments about the Atmospheres of Terrestrial Planets Mercury Very little atmosphere Contents: vaporized micrometeorites, solar wind Sky is black Venus Very thick (10% density of water), dense

More information

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

Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc. Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties

More information

Earth s Heat Budget. What causes the seasons? Seasons

Earth s Heat Budget. What causes the seasons? Seasons Earth s Heat Budget Solar energy and the global heat budget Transfer of heat drives weather and climate Ocean circulation A. Rotation of the Earth B. Distance from the Sun C. Variations of Earth s orbit

More information

CLIMATE CHANGE Albedo Forcing ALBEDO FORCING

CLIMATE CHANGE Albedo Forcing ALBEDO FORCING ALBEDO FORCING Albedo forcing is the hypothesis that variations in the Earth s reflectance of solar radiation can bring about global climate change. This hypothesis is undeniable in principle; since virtually

More information

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

Outline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued Outline Planetary Atmospheres Chapter 10 General comments about terrestrial planet atmospheres Atmospheric structure & the generic atmosphere Greenhouse effect Magnetosphere & the aurora Weather & climate

More information

2010 Pearson Education, Inc.

2010 Pearson Education, Inc. Chapter 10 Planetary Atmospheres: Mars, Venus, Earth What is an atmosphere? An atmosphere is a (usually very thin) layer of gas that surrounds a world. How does the greenhouse effect warm a planet? No

More information

PLANETARY ATMOSPHERES

PLANETARY ATMOSPHERES NAME: What will you learn in this Lab? PLANETARY ATMOSPHERES How important is a planet s atmosphere in controlling its surface temperature? What keeps the Earth at a habitable temperature, its distance

More information

Earth s Heat Budget. What causes the seasons? Seasons

Earth s Heat Budget. What causes the seasons? Seasons Earth s Heat Budget Solar energy and the global heat budget Transfer of heat drives weather and climate Ocean circulation A. Rotation of the Earth B. Distance from the Sun C. Variations of Earth s orbit

More information

Earth Energy Budget Pre-lab

Earth Energy Budget Pre-lab Science Unit: Lesson 3: Climate Change Earth Energy Budget Pre-lab School year: 2008/2009 Developed for: Developed by: Grade level: Duration of lesson: Notes: Shaughnessy Elementary School, Vancouver School

More information

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. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Lecture 2-07: The greenhouse, global heat engine.

Lecture 2-07: The greenhouse, global heat engine. Lecture 2-07: The greenhouse, global heat engine http://en.wikipedia.org/ the sun s ultraviolet (left) and infrared radiation imagers.gsfc.nasa.gov/ems/uv.html www.odysseymagazine.com/images SOLAR FLARES

More information

Planetary Atmospheres (Chapter 10)

Planetary Atmospheres (Chapter 10) Planetary Atmospheres (Chapter 10) Based on Chapter 10 This material will be useful for understanding Chapters 11 and 13 on Jovian planet systems and Extrasolar planets Chapters 4, 5, and 8 on Momentum,

More information

Period 13 Solutions: Earth as an Energy System

Period 13 Solutions: Earth as an Energy System Period 13 Solutions: Earth as an Energy System 13.1 The Earth-Sun System 1) Energy from the sun Observe the models of the Earth, Moon, and Sun in the room. a) Imagine that the distance between the Earth

More information

Grades 9-12: Earth Sciences

Grades 9-12: Earth Sciences Grades 9-12: Earth Sciences Earth Sciences...1 Earth s Place in the Universe...1 Dynamic Earth Processes...2 Energy in the Earth System...2 Biogeochemical cycles...4 Structure and Composition of the Atmosphere...4

More information

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414)

Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) NCEA Level 3 Earth and Space Science (91414) 2017 page 1 of 6 Assessment Schedule 2017 Earth and Space Science: Demonstrate understanding of processes in the atmosphere system (91414) Evidence Statement

More information

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings

Day 1 of Global Warming. Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings Day 1 of Global Warming Copyright 2008 Pearson Education, Inc., publishing as Pearson Benjamin Cummings The Atmosphere Atmosphere = the thin layer (1/100 th of Earth s diameter) of gases that surrounds

More information

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

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? Planetary Atmospheres Pressure Composition Greenhouse effect Atmospheric structure Color of the sky 1 Atmospheres

More information

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1

ATS150 Global Climate Change Spring 2019 Candidate Questions for Exam #1 1. How old is the Earth? About how long ago did it form? 2. What are the two most common gases in the atmosphere? What percentage of the atmosphere s molecules are made of each gas? 3. About what fraction

More information

AT350 EXAM #1 September 23, 2003

AT350 EXAM #1 September 23, 2003 AT350 EXAM #1 September 23, 2003 Name and ID: Enter your name and student ID number on the answer sheet and on this exam. Record your answers to the questions by using a No. 2 pencil to completely fill

More information

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens

Lecture Outlines PowerPoint. Chapter 16 Earth Science 11e Tarbuck/Lutgens Lecture Outlines PowerPoint Chapter 16 Earth Science 11e Tarbuck/Lutgens 2006 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors

More information

The Atmosphere. Composition of the Atmosphere. Section 2

The Atmosphere. Composition of the Atmosphere. Section 2 The Atmosphere Earth is surrounded by a mixture of gases known as the Nitrogen, oxygen, carbon dioxide, and other gases are all parts of this mixture. Earth s atmosphere changes constantly as these gases

More information

ATM S 111: Global Warming Solar Radiation. Jennifer Fletcher Day 2: June

ATM S 111: Global Warming Solar Radiation. Jennifer Fletcher Day 2: June ATM S 111: Global Warming Solar Radiation Jennifer Fletcher Day 2: June 22 2010 Yesterday We Asked What factors influence climate at a given place? Sunshine (and latitude) Topography/mountains Proximity

More information

Website Lecture 3 The Physical Environment Part 1

Website   Lecture 3 The Physical Environment Part 1 Website http://websites.rcc.edu/halama Lecture 3 The Physical Environment Part 1 1 Lectures 3 & 4 1. Biogeochemical Cycling 2. Solar Radiation 3. The Atmosphere 4. The Global Ocean 5. Weather and Climate

More information

Carbon Cycling Internal

Carbon Cycling Internal Carbon Cycling Internal The 4 subcycles Atmosphere The Earth s Atmosphere The Earth has a radius of some 6400 km. Ninety-nine percent of the earth's atmosphere is contained within a layer approximately

More information

Earth s Energy Budget: How Is the Temperature of Earth Controlled?

Earth s Energy Budget: How Is the Temperature of Earth Controlled? 1 NAME Investigation 2 Earth s Energy Budget: How Is the Temperature of Earth Controlled? Introduction As you learned from the reading, the balance between incoming energy from the sun and outgoing energy

More information

Science Chapter 13,14,15

Science Chapter 13,14,15 Science 1206 Chapter 13,14,15 1 Weather dynamics is the study of how the motion of water and air causes weather patterns. Energy from the Sun drives the motion of clouds, air, and water. Earth s tilt at

More information

Sunspot Cycle Worksheet

Sunspot Cycle Worksheet Sunspot Cycle Worksheet Read the Explore information and answer the Explain questions in your own words. Explore: Global warming and climate change are international concerns and the focus of much controversy.

More information

4 Changes in Climate. TAKE A LOOK 2. Explain Why is more land exposed during glacial periods than at other times?

4 Changes in Climate. TAKE A LOOK 2. Explain Why is more land exposed during glacial periods than at other times? Name Class CHAPTER 3 Date Climate 4 Changes in Climate SECTION National Science Education Standards BEFORE YOU READ After you read this section, you should be able to answer these questions: ES 1k, 2a

More information

WELCOME TO PERIOD 14:CLIMATE CHANGE. Homework #13 is due today.

WELCOME TO PERIOD 14:CLIMATE CHANGE. Homework #13 is due today. WELCOME TO PERIOD 14:CLIMATE CHANGE Homework #13 is due today. Note: Homework #14 due on Thursday or Friday includes using a web site to calculate your carbon footprint. You should complete this homework

More information

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures?

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures? CHAPTER 17 1 What Is Climate? SECTION Climate BEFORE YOU READ After you read this section, you should be able to answer these questions: What is climate? What factors affect climate? How do climates differ

More information

Science 1206 Chapter 1 - Inquiring about Weather

Science 1206 Chapter 1 - Inquiring about Weather Science 1206 Chapter 1 - Inquiring about Weather 1.1 - The Atmosphere: Energy Transfer and Properties (pp. 10-25) Weather and the Atmosphere weather the physical conditions of the atmosphere at a specific

More information

The greenhouse effect

The greenhouse effect 16 Waves of amplitude of 1 m roll onto a beach at a rate of one every 12 s. If the wavelength of the waves is 120 m, calculate (a) the velocity of the waves (b) how much power there is per metre along

More information

( 1 d 2 ) (Inverse Square law);

( 1 d 2 ) (Inverse Square law); ATMO 336 -- Exam 3 120 total points including take-home essay Name The following equations and relationships may prove useful. F d1 =F d2 d 2 2 ( 1 d 2 ) (Inverse Square law);! MAX = 0.29 " 104 µmk (Wien's

More information

A Changing Climate: Past, Present and Future. What is Climate?

A Changing Climate: Past, Present and Future. What is Climate? A Changg Climate: Past, Present and Future AT 351 Lab 14 April 30, 2008 What is Climate? The slowly varyg aspects of the atmosphere hydrosphere land surface system Climate is often considered to be an

More information

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun

Electromagnetic Radiation. Radiation and the Planetary Energy Balance. Electromagnetic Spectrum of the Sun Radiation and the Planetary Energy Balance Electromagnetic Radiation Solar radiation warms the planet Conversion of solar energy at the surface Absorption and emission by the atmosphere The greenhouse

More information

Name Class Date. For each pair of terms, explain how the meanings of the terms differ.

Name Class Date. For each pair of terms, explain how the meanings of the terms differ. Skills Worksheet Chapter Review USING KEY TERMS For each pair of terms, explain how the meanings of the terms differ. 1. biome and tropical zone 2. weather and climate 3. temperate zone and polar zone

More information

EARTH'S ATMOSPHERE. 1. The graph below shows the average concentration of ozone in Earth's atmosphere over Arizona during 4 months of the year.

EARTH'S ATMOSPHERE. 1. The graph below shows the average concentration of ozone in Earth's atmosphere over Arizona during 4 months of the year. EARTH'S ATMOSPHERE 1. The graph below shows the average concentration of ozone in Earth's atmosphere over Arizona during 4 months of the year. Which layer of Earth's atmosphere contains the greatest concentration

More information

ESS15 Lecture 10. Winds and weather The Coriolis force Global circulations of atmosphere & ocean Weather vs. Climate

ESS15 Lecture 10. Winds and weather The Coriolis force Global circulations of atmosphere & ocean Weather vs. Climate ESS15 Lecture 10 Winds and weather The Coriolis force Global circulations of atmosphere & ocean Weather vs. Climate Earth s energy imbalances, winds, and the global circulation of the atmopshere. Please

More information

Unit 3 Review Guide: Atmosphere

Unit 3 Review Guide: Atmosphere Unit 3 Review Guide: Atmosphere Atmosphere: A thin layer of gases that forms a protective covering around the Earth. Photosynthesis: Process where plants take in carbon dioxide and release oxygen. Trace

More information

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate

Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate Energy Systems, Structures and Processes Essential Standard: Analyze patterns of global climate change over time Learning Objective: Differentiate between weather and climate Global Climate Focus Question

More information

Land Surface Sea Ice Land Ice. (from Our Changing Planet)

Land Surface Sea Ice Land Ice. (from Our Changing Planet) Lecture 5: Land Surface and Cryosphere (Outline) Land Surface Sea Ice Land Ice (from Our Changing Planet) Earth s s Climate System Solar forcing Atmosphere Ocean Land Solid Earth Energy, Water, and Biochemistry

More information

Meteorology Pretest on Chapter 2

Meteorology Pretest on Chapter 2 Meteorology Pretest on Chapter 2 MULTIPLE CHOICE 1. The earth emits terrestrial radiation a) only at night b) all the time c) only during winter d) only over the continents 2. If an imbalance occurs between

More information

Torben Königk Rossby Centre/ SMHI

Torben Königk Rossby Centre/ SMHI Fundamentals of Climate Modelling Torben Königk Rossby Centre/ SMHI Outline Introduction Why do we need models? Basic processes Radiation Atmospheric/Oceanic circulation Model basics Resolution Parameterizations

More information

Earth s Climate System. Surface Albedo. Climate Roles of Land Surface. Lecture 5: Land Surface and Cryosphere (Outline) Land Surface Sea Ice Land Ice

Earth s Climate System. Surface Albedo. Climate Roles of Land Surface. Lecture 5: Land Surface and Cryosphere (Outline) Land Surface Sea Ice Land Ice Lecture 5: Land Surface and Cryosphere (Outline) Earth s Climate System Solar forcing Land Surface Sea Ice Land Ice Atmosphere Ocean Land Solid Earth Energy, Water, and Biochemistry Cycles (from Our Changing

More information

The Distribution of Cold Environments

The Distribution of Cold Environments The Distribution of Cold Environments Over 25% of the surface of our planet can be said to have a cold environment, but defining what we actually mean by that can be very challenging. This is because cold

More information

Heating the Atmosphere (Chapter 14, with material from Chapter 2)

Heating the Atmosphere (Chapter 14, with material from Chapter 2) Heating the Atmosphere (Chapter 14, with material from Chapter 2) 1. Reflection on Prior Knowledge: What process in Earth s early history resulted in the formation of an atmosphere? What gases characterized

More information

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures?

1 What Is Climate? TAKE A LOOK 2. Explain Why do areas near the equator tend to have high temperatures? CHAPTER 17 1 What Is Climate? SECTION Climate BEFORE YOU READ After you read this section, you should be able to answer these questions: What is climate? What factors affect climate? How do climates differ

More information

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves

Directed Reading. Section: Solar Energy and the Atmosphere RADIATION. identical point on the next wave. waves Skills Worksheet Directed Reading Section: Solar Energy and the Atmosphere 1. How is Earth s atmosphere heated? 2. Name the two primary sources of heat in the atmosphere. RADIATION In the space provided,

More information

Lesson 2 The Inner Planets

Lesson 2 The Inner Planets Lesson 2 Student Labs and Activities Page Launch Lab 25 Content Vocabulary 26 Lesson Outline 27 MiniLab 29 Content Practice A 30 Content Practice B 31 School to Home 32 Key Concept Builders 33 Enrichment

More information

Climate Change: Global Warming Claims

Climate Change: Global Warming Claims Climate Change: Global Warming Claims Background information (from Intergovernmental Panel on Climate Change): The climate system is a complex, interactive system consisting of the atmosphere, land surface,

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics Problem Solving 10: The Greenhouse Effect. Section Table and Group MASSACHUSETTS INSTITUTE OF TECHNOLOGY Department of Physics 8.02 Problem Solving 10: The Greenhouse Effect Section Table and Group Names Hand in one copy per group at the end of the Friday Problem Solving

More information

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

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? About 10 km thick Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds What is an atmosphere? Sources of Gas Losses of Gas Thermal Escape Earth s Atmosphere About 10 km thick Consists mostly of molecular

More information

THE GREENHOUSE EFFECT

THE GREENHOUSE EFFECT ASTRONOMY READER THE GREENHOUSE EFFECT 35.1 THE GREENHOUSE EFFECT Overview Planets are heated by light from the Sun. Planets cool off by giving off an invisible kind of light, longwave infrared light.

More information