February 04, Solar Budget NOTES.notebook. Balancing. Heats. too little. Too much. photosynthesis. weather. light bulb. light bulb.
|
|
- Sheryl Anthony
- 7 years ago
- Views:
Transcription
1 Earth s Solar Energy Budget Sun Primary source of Earth s energy our planet Needed for Drives our and Primary Sun source of Earth s energy Heats our planet photosynthesis Needed for wind weather Drives our and Balancing Solar Energy Budget of Sun s energy: Too much too little _ or would result in undesirable temperatures for maintaining life as we know it. waves Uses of energy to transfer energy light bulb Examples: microwave Only method that can move through All energy arrives to Earth in this form waves Uses of energy to transfer energy Examples: Only method that can move through solar light bulb microwave empty space All energy arrives to Earth in this form 1
2 1. ALL objects radiate energy 2. Hotter objects radiate more energy 3. Hotter objects radiate shorter wavelengths Soak heat in faster = Give off heat faster too Specific Heat: Amount of energy required to increase 1 g of something 1 ⁰ C. Specific Heat: Amount of energy required to increase 1 g of something 1 ⁰ C. 2
3 lower The the specific heat of a substance, the better absorber/emitter lower The the specific heat of a substance, the better absorber/emitter ESRT (Page 1) ESRT (Page 1) Conduction direct Transfer of energy through molecule Through matter from to The more molecules the better the conductor density contact molecule Substances with a higher _ have a greater number of molecules in a given area Convection Transfer of energy by actually matter from one place to another. Hair Dryer moving Examples: Convection Cells 3
4 1. Incoming Solar ( ) wavelengths INSOLATION Mix of coming from the Sun Majority are wavelengths heat short light energy NOT, just 6,000 0 C Surface temperature of Sun is ~ 93 Sun is ~ million miles from Earth (we don't feel the heat...but the energy) Jan 28 8:52 AM Add to notes: BEST absorber of INSOLATION... Dark Colors and Rough materials POOR absorber of INSOLATION... Light Colors and Smooth materials 2. Albedo (al bead o) reflectivity Percentage of directly Reflection: light waves bounced back into space. ALL Scattering: light waves reflected in directions clouds Example: Water droplets in _ scatter all wavelengths equally; white therefore, they appear Jan 28 8:55 AM 3. Absorption gases Different absorb different wavelengths poor Nitrogen = absorber Oxygen = good absorber of wavelengths infrared longer IR like radiation ( ) 4
5 Solar Budget NOTES.notebook 4. Reradiated Energy 3. Absorption shorter wavelengths Ozone = good absorber of UV radiation like Longer wavelengths (IR) that return to atmosphere due to heating of Earth s surface Best absorber of IR Carbon Dioxide (CO2) = visible light not absorbed; NOTE: therefore, this form of short wavelengths supplies the energy for our planet. Distribution of INSOLATION albedo from Earth s 30 percent lost due to surface and scattering from the atmosphere 19 percent absorbed by clouds and the atmosphere 51 percent actually absorbed by Earth s heating surface for _ Add this simple "greenhouse" drawing in your notes: Balanced Budget (units of Solar Energy) (emitted) Dec 31 10:08 AM (absorbed) 5
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 informationATM 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 information1. 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 informationEnergy Pathways in Earth s Atmosphere
BRSP - 10 Page 1 Solar radiation reaching Earth s atmosphere includes a wide spectrum of wavelengths. In addition to visible light there is radiation of higher energy and shorter wavelength called ultraviolet
More informationSolar 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 informationThe 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 informationOverview. What is EMR? Electromagnetic Radiation (EMR) LA502 Special Studies Remote Sensing
LA502 Special Studies Remote Sensing Electromagnetic Radiation (EMR) Dr. Ragab Khalil Department of Landscape Architecture Faculty of Environmental Design King AbdulAziz University Room 103 Overview What
More informationINSPIRE 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 information1. Theoretical background
1. Theoretical background We consider the energy budget at the soil surface (equation 1). Energy flux components absorbed or emitted by the soil surface are: net radiation, latent heat flux, sensible heat
More informationChapter 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 informationa) 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 informationMultiple 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 informationModule 2.2. Heat transfer mechanisms
Module 2.2 Heat transfer mechanisms Learning Outcomes On successful completion of this module learners will be able to - Describe the 1 st and 2 nd laws of thermodynamics. - Describe heat transfer mechanisms.
More informationCHAPTER 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 informationTOPIC 5 (cont.) RADIATION LAWS - Part 2
TOPIC 5 (cont.) RADIATION LAWS - Part 2 Quick review ELECTROMAGNETIC SPECTRUM Our focus in this class is on: UV VIS lr = micrometers (aka microns) = nanometers (also commonly used) Q1. The first thing
More informationFACTS 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 informationSolar 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 informationClimate Change and Renewable Energy A Perspective from a Measurements Viewpoint
Climate Change and Renewable Energy A Perspective from a Measurements Viewpoint Regional Workshop on Metrology and Technology Challenges of Climate Change and Renewable Energy Guatemala City, Guatemala
More informationReview 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 informationClouds 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 informationCorso 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 informationElectromagnetic 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 informationIntroduction 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 informationThe 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 informationWhat 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 informationScience Tutorial TEK 6.9C: Energy Forms & Conversions
Name: Teacher: Pd. Date: Science Tutorial TEK 6.9C: Energy Forms & Conversions TEK 6.9C: Demonstrate energy transformations such as energy in a flashlight battery changes from chemical energy to electrical
More informationMCQ - ENERGY and CLIMATE
1 MCQ - ENERGY and CLIMATE 1. The volume of a given mass of water at a temperature of T 1 is V 1. The volume increases to V 2 at temperature T 2. The coefficient of volume expansion of water may be calculated
More informationEarth 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 informationCopyrighted Material. 1 Basics of Climate. The climate s delicate, the air most sweet. William Shakespeare, A Winter s Tale
1 Basics of Climate The climate s delicate, the air most sweet. William Shakespeare, A Winter s Tale To appreciate the role of the ocean in climate, we need to have a basic understanding of how the climate
More informationCalifornia 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 informationCloud 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 informationCHAPTER 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 informationElectromagnetic Radiation (EMR) and Remote Sensing
Electromagnetic Radiation (EMR) and Remote Sensing 1 Atmosphere Anything missing in between? Electromagnetic Radiation (EMR) is radiated by atomic particles at the source (the Sun), propagates through
More informationFrom 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 informationMAKING SENSE OF ENERGY Electromagnetic Waves
Adapted from State of Delaware TOE Unit MAKING SENSE OF ENERGY Electromagnetic Waves GOALS: In this Part of the unit you will Learn about electromagnetic waves, how they are grouped, and how each group
More informationPhysics 1010: The Physics of Everyday Life. TODAY Black Body Radiation, Greenhouse Effect
Physics 1010: The Physics of Everyday Life TODAY Black Body Radiation, Greenhouse Effect 1 Admin Stuff Exams are at back of room, alphabetically in four piles. Please collect AFTER class Grades posted
More informationSTUDY 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 informationThe Three Heat Transfer Modes in Reflow Soldering
Section 5: Reflow Oven Heat Transfer The Three Heat Transfer Modes in Reflow Soldering There are three different heating modes involved with most SMT reflow processes: conduction, convection, and infrared
More informationESCI-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 informationSemester 2. Final Exam Review
Semester 2 Final Exam Review Motion and Force Vocab Motion object changes position relative to a reference point. Speed distance traveled in a period of time. Velocity speed in a direction. Acceleration
More informationPhotosynthesis and Light in the Ocean Adapted from The Fluid Earth / Living Ocean Heather Spalding, UH GK-12 program
Photosynthesis and Light in the Ocean Adapted from The Fluid Earth / Living Ocean Heather Spalding, UH GK-12 program Algae, like your Halimeda, and plants live in very different environments, but they
More informationMultiple 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 informationASTR 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 informationRadiation 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 informationScience Standard 3 Energy and Its Effects Grade Level Expectations
Science Standard 3 Energy and Its Effects Grade Level Expectations Science Standard 3 Energy and Its Effects The flow of energy drives processes of change in all biological, chemical, physical, and geological
More informationGreen Heating. Pupil Research Brief. Teachers Notes. Syllabus Coverage Subject Knowledge and Understanding. Route through the Brief UPIL ESEARCHER
R P UPIL ESEARCHER Green Heating I NITIATIVE Pupil Research Brief Teachers Notes Syllabus Coverage Subject Knowledge and Understanding all types of electromagnetic radiation form a continuous spectrum
More informationES 106 Laboratory # 5 EARTH-SUN RELATIONS AND ATMOSPHERIC HEATING
ES 106 Laboratory # 5 EARTH-SUN RELATIONS AND ATMOSPHERIC HEATING 5-1 Introduction Weather is the state of the atmosphere at a particular place for a short period of time. The condition of the atmosphere
More informationWaves Sound and Light
Waves Sound and Light r2 c:\files\courses\1710\spr12\wavetrans.doc Ron Robertson The Nature of Waves Waves are a type of energy transmission that results from a periodic disturbance (vibration). They are
More information7. 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 informationComposition 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 informationCHAPTER 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 informationGRADE 6 SCIENCE. Demonstrate a respect for all forms of life and a growing appreciation for the beauty and diversity of God s world.
GRADE 6 SCIENCE STRAND A Value and Attitudes Catholic Schools exist so that curriculum may be taught in the light of Gospel teachings. Teachers must reinforce Gospel truths and values so that students
More informationATMOSPHERIC 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 informationAtmospheric 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 informationLight as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation
The Nature of Light Light and other forms of radiation carry information to us from distance astronomical objects Visible light is a subset of a huge spectrum of electromagnetic radiation Maxwell pioneered
More informationConvection, Conduction & Radiation
Convection, Conduction & Radiation There are three basic ways in which heat is transferred: convection, conduction and radiation. In gases and liquids, heat is usually transferred by convection, in which
More informationName Class Date. spectrum. White is not a color, but is a combination of all colors. Black is not a color; it is the absence of all light.
Exercises 28.1 The Spectrum (pages 555 556) 1. Isaac Newton was the first person to do a systematic study of color. 2. Circle the letter of each statement that is true about Newton s study of color. a.
More information2 Absorbing Solar Energy
2 Absorbing Solar Energy 2.1 Air Mass and the Solar Spectrum Now that we have introduced the solar cell, it is time to introduce the source of the energy the sun. The sun has many properties that could
More informationHumidity, Condensation, Clouds, and Fog. Water in the Atmosphere
Humidity, Condensation, Clouds, and Fog or Water in the Atmosphere The Hydrologic Cycle Where the Water Exists on Earth Evaporation From the Oceans and Land The Source of Water Vapor for the Atmosphere
More informationLesson 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 informationMaterials Needed: Choose one of the following methods depending on how familiar your students are with the internet and how to use it.
Teacher Information Lesson Title: Global Warming, Green House Effect and Climate Changes Lesson Description: This lesson helps students to understand or review their understanding of global warming, the
More informationTreasure Hunt. Lecture 2 How does Light Interact with the Environment? EMR Principles and Properties. EMR and Remote Sensing
Lecture 2 How does Light Interact with the Environment? Treasure Hunt Find and scan all 11 QR codes Choose one to watch / read in detail Post the key points as a reaction to http://www.scoop.it/t/env202-502-w2
More informationCommon Defects in Digital Printing. Paul Geldenhuys & Amir Shapira January, 2009
Common Defects in Digital Printing Paul Geldenhuys & Amir Shapira January, 2009 Overview Ambient Influences Humidity Temperature Sunlight & UV Abrasion Chemical Resistance Common Defects in Digital Printing
More informationTech Bulletin. Understanding Solar Performance
Tech Bulletin Understanding Solar Performance Bekaert solar control window films use advanced technology to benefit consumers with quality solutions that enhance comfort and decrease energy use. By understanding
More informationWELCOME 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 informationFundamentals of Climate Change (PCC 587): Water Vapor
Fundamentals of Climate Change (PCC 587): Water Vapor DARGAN M. W. FRIERSON UNIVERSITY OF WASHINGTON, DEPARTMENT OF ATMOSPHERIC SCIENCES DAY 2: 9/30/13 Water Water is a remarkable molecule Water vapor
More informationName: Class: Date: 10. Some substances, when exposed to visible light, absorb more energy as heat than other substances absorb.
Name: Class: Date: ID: A PS Chapter 13 Review Modified True/False Indicate whether the statement is true or false. If false, change the identified word or phrase to make the statement true. 1. In all cooling
More informationSOLAR ENERGY How much strikes the earth? How much can my building get? When is it too much?
SOLAR ENERGY How much strikes the earth? How much can my building get? When is it too much? The sun: friend of foe? Drawing by Le Corbusier ENGS 44 Sustainable Design Benoit Cushman-Roisin 14 April 2015
More informationOverview of the IR channels and their applications
Ján Kaňák Slovak Hydrometeorological Institute Jan.kanak@shmu.sk Overview of the IR channels and their applications EUMeTrain, 14 June 2011 Ján Kaňák, SHMÚ 1 Basics in satellite Infrared image interpretation
More informationMaterials Needed: Time Needed: Adaptations: 2 flyswatters (optional) Vocabulary Definitions (below) Vocabulary Scramble Sheets (below)
Vocabulary Slap Game ( Flyswatter Game ) Directions: Project a Vocabulary Scramble sheet on a projection screen or Smart Board. Divide the class into two teams. Each team sends one person up to the screen.
More informationTeaching 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 informationReview Questions Photosynthesis
Review Questions Photosynthesis 1. Describe a metabolic pathway. In a factory, labor is divided into small individual jobs. A carmaker, for example, will have one worker install the front windshield, another
More informationWhat is Solar Control?
A better environment inside and out. Solar, Safety and Security Window Films: Tech Bulletin Understanding Solar Performance Solar Gard solar control window films use advanced technology to benefit consumers
More informationTake 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 informationThe 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 informationChapter 2: Forms of Energy
Chapter 2: Forms of Energy Goals of Period 2 Section 2.1: To describe the forms of energy Section 2.2: To illustrate conversions from one form of energy to another Section 2.3 To describe energy storage
More informationChapter 2. The global energy balance. 2.1 Planetary emission temperature
Chapter 2 The global energy balance We consider now the general problem of the radiative equilibrium temperature of the Earth. The Earth is bathed in solar radiation and absorbs much of that incident upon
More informationIntroduction to the Greenhouse Effect
Introduction to the Greenhouse Effect Planetary Temperature by Arthur Glasfeld and Margret Geselbracht ver the past 10-15 years there has been growing concern over changes in the climate and the possibility
More informationSection 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 informationAP ENVIRONMENTAL SCIENCE 2007 SCORING GUIDELINES
AP ENVIRONMENTAL SCIENCE 2007 SCORING GUIDELINES Question 4 Some scientists estimate that by 2025 over 60 percent of the global human population will live in urban areas. Urban residents experience a variety
More information6 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 information8.2 Cells and Energy. What is photosynthesis? Photosynthesis takes place in the chloroplasts. CHAPTER 8. Solar cells and chloroplasts
CHAPTER 8 CELL PROCESSES 8.2 Cells and Energy To stay alive, you need a constant supply of energy. You need energy to move, think, grow, and even sleep. Where does that energy come from? It all starts
More informationReduction of Global Warming By Using Renewable Energy Resources: A Mathematic Approach
International Journal of Computer Science and Telecommunications [Volume 3, Issue 2, February 2012] 37 ISSN 2047-3338 Reduction of Global Warming By Using Renewable nergy Resources: A Mathematic Approach
More informationChapter 2: Forms of Energy
Chapter 2: Forms of Energy Goals of Period 2 Section 2.1: To describe the forms of energy Section 2.2: To illustrate conversions from one form of energy to another Section 2.3: To define the efficiency
More informationEnergy - Heat, Light, and Sound
Science Benchmark: 06:06 Heat, light, and sound are all forms of energy. Heat can be transferred by radiation, conduction and convection. Visible light can be produced, reflected, refracted, and separated
More informationSolar energy is available as long as the sun shines, but its intensity depends on weather conditions and geographic
Solar Energy What is Solar Energy? The radiation from the sun gives our planet heat and light. All living things need energy from the sun to survive. More energy from sunlight strikes the earth in one
More information5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves
5. The Nature of Light Light travels in vacuum at 3.0. 10 8 m/s Light is one form of electromagnetic radiation Continuous radiation: Based on temperature Wien s Law & the Stefan-Boltzmann Law Light has
More informationForms of Energy. Freshman Seminar
Forms of Energy Freshman Seminar Energy Energy The ability & capacity to do work Energy can take many different forms Energy can be quantified Law of Conservation of energy In any change from one form
More informationGlobal Warming and Greenhouse Gases Reading Assignment
What is global warming? Global Warming and Greenhouse Gases Imagine you live in a timber shack in Alaska. It's chilly up there, so you build yourself a huge log fire and pile on all the wood you can find.
More informationCharacteristics 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 informationGeol 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 informationPhotosynthesis Reactions. Photosynthesis Reactions
Photosynthesis Reactions Photosynthesis occurs in two stages linked by ATP and NADPH NADPH is similar to NADH seen in mitochondria; it is an electron/hydrogen carrier The complete process of photosynthesis
More information8.1 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 informationGreenhouse Glazing Effects on Heat Transfer for Winter Heating and Summer Cooling
Greenhouse Glazing Effects on Heat Transfer for Winter Heating and Summer Cooling David R. Mears, Ph.D. Bioresource Engineering Department of Plant Biology and Pathology Rutgers University 20 Ag Extension
More informationLecture 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 informationPrinciple of Thermal Imaging
Section 8 All materials, which are above 0 degrees Kelvin (-273 degrees C), emit infrared energy. The infrared energy emitted from the measured object is converted into an electrical signal by the imaging
More informationAZ 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 informationThe Electromagnetic Spectrum
INTRODUCTION The Electromagnetic Spectrum I. What is electromagnetic radiation and the electromagnetic spectrum? What do light, X-rays, heat radiation, microwaves, radio waves, and gamma radiation have
More informationThe 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 informationThe greenhouse effect: a closer look
The greenhouse effect: a closer look 44 Ian Strangeways TerraData, Wallingford, Oxfordshire Interest in carbon dioxide ( ) and water vapour (WV) as greenhouse gases (GHGs) has waxed and waned over 200
More information