Period 14 Activity Sheet: Energy in Nature

Similar documents
Period 13: Earth as an Energy System

Period 13 Solutions: Earth as an Energy System

Seasons and Angle of Insolation

Period 22: Uses of Solar Energy

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

CCMR Educational Programs

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

Exploration Phase What are the differences between these pictures?

Purpose of the experiment

Reason for the Seasons

Lecture 3: Global Energy Cycle

Topic 6: Insolation and the Seasons

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

Prentice Hall EARTH SCIENCE. Tarbuck Lutgens

Happy Tuesday! Pull out a half sheet of paper or share a whole with a friend!

What Causes the Seasons?

Natural Causes of Climate. 3B Day 2

1 Our Dynamic Climate Guiding Question: What factors determine Earth s climate?

What Causes the Seasons?

Project Moon Watch. What You Need. Find Out Do this activity to see how the moon s appearance changes during a 30-day period.

Planetary Atmospheres (Chapter 10)

Rotation and Revolution

Chapter 2. Heating Earth's Surface & Atmosphere

This clementine orange is an oblate spheroid. Earth is more rounded than this clementine, but it is still an oblate spheroid.

Patterns on Earth 4.8C

Seasons Quiz Please Do Not Write on this Paper Obrigado

Lesson Overview. Climate. Lesson Overview. 4.1 Climate

[2] (b) An electron is accelerated from rest through a potential difference of 300 V.

MAPH & & & & & & 02 LECTURE

Reasons for the Seasons

Student Exploration: 2D Eclipse

Astronomy 101 Lab: Spectra

Solar Radiation and the Seasons. LAST TIME in GEOG 1001! Chapter 1. 8/29/2010. Objectives

Solar Radiant Heating and Angle of Incidence NS 696 V: Weather and Climate for Educators

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

Energy and Insolation Review 2

The Atmosphere: Structure and Temperature

THE SUN, THE MOON AND OUR SOLAR SYSTEM TEACHER NOTES TO SHARE WITH STUDENTS

Temperature Changes OBJECTIVES PREPARATION SCHEDULE MATERIALS. The students. For each student. For each team of two. For the class

Celestial Sphere & Solar Motion Lab (Norton s Star Atlas pages 1-4)

Lecture 4: Global Energy Balance

11/18/2010. Only part of the spectrum we can see. A rainbow of colors, each corresponding to a different wavelength.

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

Physical Sciences Astronomy: Phases of the Moon 1 Science and Mathematics Education Research Group

Clouds and Rain Unit (3 pts)

What Is Air Temperature?

Laboratory Exercise. Atomic Spectra A Kirchoff Potpourri

Physics Homework Set I Su2015

Seasons and Ecliptic Simulator

Which graph best shows the relationship between intensity of insolation and position on the Earth's surface? A) B) C) D)

Planet Earth. Part 2

Lecture 12. Measurements in Astronomy. Using Light. ASTR 111 Section 002. In astronomy, we need to make remote and indirect measurements

L ESSON P LAN:DETERMINING THE E FFECT OF D ISTANCE (PART 1) AND I NCLINATION (PART 2)

Name and Student ID Section Day/Time:

Atmospheric Radiation

- matter-energy interactions. - global radiation balance. Further Reading: Chapter 04 of the text book. Outline. - shortwave radiation balance

A Quick Look at the Atmosphere and Climate

b. Assuming that the sundial is set up correctly, explain this observation.

Module 66. Science and Health LUNAR ECLIPSE. A DepEd-BEAM Distance Learning Program supported by the Australian Agency for International Development

MS20 Laboratory Solar Radiation and Light Transmission

A) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface

Intensity of Light and Heat. The second reason that scientists prefer the word intensity is Well, see for yourself.

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

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

Lecture: October 6, 2010

2010 Pearson Education, Inc.

The Atmosphere. Composition of the Atmosphere. Section 2

ATMOSPHERE PACKET CHAPTER 22 PAGES Section 1 page 546

MIDTERM REVIEW QUESTIONS - PACKET #2 (75 MULTIPLE CHOICE QUESTIONS)

Go to Click on the first animation: The north pole, observed from space

1. Which continents are experiencing daytime? 2. Which continents are experiencing nighttime?

Atomic Physics Worksheet. between 4000 and 5000 Angstroms ( nanometers): between 6500 and 7500 Angstroms ( nanometers):

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

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

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Astron 104 Laboratory #10 Solar Energy and the Habitable Zone

AT350 EXAM #1 September 23, 2003

1. The diagram below shows Earth, four different positions of the Moon, and the direction of incoming sunlight.

Rotation - Earth spinning on its axis

Chapter 9 Atmosphere Study Guide

Tilted Earth Lab Why Do We Have Seasons?

Chapter 2 Solar and Infrared Radiation

Lecture 2: Global Energy Cycle

4. Zero-dimensional Model of Earth s Temperature

Energy: Warming the earth and Atmosphere. air temperature. Overview of the Earth s Atmosphere 9/10/2012. Composition. Chapter 3.

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Meteorology Pretest on Chapter 2

- global radiative energy balance

PHYS 4400, Principles and Varieties of Solar Energy Instructor: Randy J. Ellingson The University of Toledo

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

Motion of the Sun. View Comments

Page 1. Name:

PRELIMINARY ACTIVITY FOR. Seasons and Angle of Insolation

MIDTERM PRACTICE EXAM

You Are the Spectrometer! A Look Inside Astronomy's Essential Instrument (Robert B. Friedman & Matthew K. Sharp)

Daily Motions. Daily Motions. Solar and Sidereal Days. Annual Motions of the Sun. Coordinate system on Earth. Annual Motion of the Stars.

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

Chapter 6. Solar Geometry. Contents

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

TEACHER Worksheet: Phases of the Moon and Tides

Transcription:

Period 14 Activity Sheet: Energy in Nature 14.1 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 and the Sun is represented by the length of a football field (100 yards or 91 meters). The Sun, at one goal line, is represented by a ball 85 cm in diameter (the size of a large beach ball or exercise ball). What would be the diameter of a model of the Earth at the opposite goal line? What would be the diameter of a model of the Moon? How far would the model of the Moon be from the model of the Earth? b) It takes radiation from the Sun about 8.3 minutes to reach the Earth. How far away is the Earth from the Sun? 2) How much energy does the Earth receive from the Sun? a) How many watts of energy does the Sun produce? b) Only about 1.76 x 10 17 watts of the Sun's energy actually reaches the Earth. What percent is this of the total energy produced by the Sun? c) Where does the rest of the Sun s energy go? d) What is the source of the Sun's energy? 1

3) What form of energy is received from the Sun? a) What form of energy does the sun give off? b) Your instructor will demonstrate a light bulb filament at different temperatures. Look at the filament through a diffraction grating. Describe any changes you see in the spectrum as the filament glows hotter. c) How does the temperature of an object relate to the frequency of the energy it gives off (its electromagnet spectrum)? 14.2 The Earth s Atmosphere 4) Atmospheric Layers a) On the diagram above, fill in the names of the layers of the Earth s atmosphere and the approximate percent of the Earth s air that is contained in each region. (Hint: note what fraction of the total pressure of the air is measured for each air layer.) 2

b) In which atmospheric layer(s) can life exist? c) In which atmospheric layer is the Earth s ozone layer? d) Make a prediction as to how thick the atmosphere would be if the Earth were as large as the globe on your table. Prediction: Answer: e) What is the chemical composition of the atmosphere? f) Group Discussion Question: The percent of carbon dioxide in the atmosphere is very small (0.033%). Why does this small concentration make increasing the atmosphere s carbon dioxide concentrations potentially dangerous? 3

14.3 The Energy Balance of the Earth 5) Earth s energy balance (cut and paste energy balance diagram from textbook page 157) a) From the energy balance diagram, what percent of the incoming solar radiation is reflected back into space? b) Of the solar radiation remaining, what percent is absorbed by the Earth s surface? c) What happens to the rest of the solar radiation that enters the Earth s atmosphere? d) What form of energy is absorbed by the Earth s surface? e) What form of energy is emitted by the Earth s surface? f) What can block the radiation from the Earth from escaping into space? g) What percent of the solar radiation entering the Earth s atmosphere is radiated back into space? h) Group Discussion Question: What are the consequences for the Earth if not all of the incoming radiation is radiated back into space? 4

6) Sunlight incident on the Earth Your instructor will explain how to use a globe and a flashlight to model the sunlight incident on different regions of the Earth. a) Point a flashlight light horizontally at the equator of the globe. Stand the peg board between the light and the globe about 5 cm from the globe s equator and 20 cm from the flashlight. Hold the small brown square flat along the equator. How many dots of light on the globe fit inside the brown square? b) Keeping the pegboard the same distances from the flashlight and the globe, raise the flashlight to point it horizontally at the high northern latitudes (for example, at Alaska). Hold the brown square flat along this area. Now how many dots of light on the globe fit inside the brown square? c) How does the amount of sunlight striking the Earth at higher latitudes compare the to sunlight striking the Equator? d) What effect does your findings in part c) have on the weather? e) Group Discussion Question: What is another reason that the higher latitudes receive less sunlight? 7) The Earth s seasons Your instructor will discuss the causes of the Earth s seasons. a) Place the light bulb in the center of your table so that it shines on the equator of the globe. Move the globe around the light bulb to simulate the Earth s seasons. (Hint: the direction that the axis of the globe tilts is important.) b) What causes the Earth s seasons? Is the distance of the Earth from the Sun a factor? 5