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The Sun: Lesson Plan for Grades 2 and 3

The Sun

 

Submitted by: Sharon Freer

Email: sfreer@njcu.edu

School/University/Affiliation: NJCU

Date: June 28, 2009


Subject(s):

*        Science (Astronomy and Space Science)

Topic of the Lesson

*        The Sun

Grade Level

 

*        Grades 2-3

                       

Duration

 

*        Five 40 minute Sessions

 

OBJECTIVES:

At the end of the lesson, students will:

*        Know the definitions of the terms that relate to the sun

*        Know the sun is the closest star to our planet

*        Understand that the sun is a ball of hot gas

*        Is far away from the Earth and is much bigger than the Earth

*        Understand how different colors absorb light and feel warmer than others

*        Understand the patterns of day and night as they relate to the sun

 

NJ CCCS

Standard 5.9 (Astronomy & Space Science) All students will gain an understanding of the origin, evolution, and structure of the universe.)

Descriptive Statement:  The study of science should include a study of the planet Earth and its relationship to the rest of the universe. This standard describes what students should know about astronomy and space science. By the end of Grade 2, students will:

 

 

A. Earth, Moon, Sun System

  1. Recognize that the sun supplies light and heat to the Earth.
  2. Observe the patterns of day and night and the movements of the shadows of an object on the Earth during the course of a day.

Description of the Lesson:  Through a variety of activities, students will learn that the sun is a star, that it gives us light and heat, and what makes day and night.

 

Procedures:

 

*        Reach the story “Sun Up, Sun Down” by Gail Gibbons.

*        Do a K-W-L chart to discuss what students know about the sun.

*        Learn about the size, distance and make-up of the sun.                         

*        Participate in an activity that will help understand that the sun produces heat and light.

*        Participate in an activity that will help understand why reasoning for night and day.

 

Activities:

 

*        Have the students draw a picture of the sun and write a few sentences of what they

know about the sun.

*         Show the class the pictures located at the following websites:

http://umbra.nascom.nasa.gov/images/

http://science.nationalgeographic.com/science/space/solar-system/sun-article.html

*        Students will perform an exercise in which they learn how the heat and light of the sun, affect things here on earth.

*      See Activity at end of lesson plan: Do Different Colors Absorb Heat Better?

*        Students will participate in an exercise that will help explain how the rotation of the Earth creates day and night.

*      See Activity at end of lesson plan: What Makes Day and Night?

 

 

Vocabulary

Students will learn the vocabulary words associated with the sun:

corona             star                  planet              gas

sphere              sunspot            solar flare        diameter

rotation            revolution        sunrise             sunset

 

 

Assessment: 

 

*        Students will complete “The Sun” worksheet as a homework assignment.

*        Students will complete the Night & Day worksheet as a homework assignment to assess their understanding of the Earth’s rotation.                                         

*        Students will take a quiz on the vocabulary words associated with the sun.

*        Students will be assessed on their class work regarding how the color of a material affects heat absorption.                                                                                 

*        Students will be assessed on their class work on the lesson on: What makes Day and Night? Students will be asked to graphically depict their understanding of how the rotation of the Earth and Sun affect day and night.                            

*        Final Assessment will be in the form of a 25-question, multiple choice test that will be based upon the vocabulary and concepts learned throughout the lessons.

 

 

Technology:

 

*        Smartboard

*        One computer with an Internet connection

 

Materials:

 

*        Globe

*        Paper

*        Light bulb

*        Stickers

*        Ice cubes

*        Colored paper

*        Lamp

*        Wrap-around map

 


Activity:  Do Different Colors Absorb Heat Better?

 

Background

The sun emits energy in the form of electromagnetic waves. We see part of the electromagnetic wave as light and we feel part of it as warmth. Darker colors absorb more sunlight than lighter colors, which is why darker colors get warmer more quickly in the sunlight than lighter colors. The lighter colors reflect more of the sun's radiant energy, so they remain cooler to touch in the sunlight.

Preparation

1.      Make enough ice cubes so that each group can have four. Try to make them the same size so that the experiment is consistent.

2.      Cut out the colored paper into 5 sided boxes big enough to fit the ice cube for each group. To save class time, tape the boxes together, or if time is available have the students cut, fold and tape their own boxes together.

3.      Obtain the rest of the materials.

4.      Photocopy one chart per group                          

5.      For shorter lesson, precut and assemble colored boxes

 

With Students

1.      Ask them to imagine that it is 100-degrees outside. What kinds of things will they do to stay cool? What kinds of clothing will they wear? Any thought to color? Once the class is thinking about the influence of color and its relationship to heat:

2.      Divide the class into small groups.

3.      Hand out newspaper and have each group spread the newspaper under the heat lamp or in a sunny place outside.

4.      On the newspaper, place the boxes side by side with the opening facing away from the sun/light so the students can see inside.

5.      Give each group 4 ice cubes and instruct them to place 1 ice cube in the center of each colored cube.

Let the ice cubes sit in the sun until they have melted. Have the students check on them every few minutes and record which ice cubes melted first, second, third, and fourth.


click for copyright

6.      Instruct each group to record their data on the chart.

7.      Discuss with the class their observations, touching on the different colors and their ability to reflect light and heat. Also, talk about how these characteristics of color help to melt the ice.

Investigating Questions (Return to Contents)

·                 Why do ice cubes melt?

·                 How does the sun affect ice?

·                 What kind of clothes do people wear outside in the winter/summer?

·                 On which color did the first ice cube completely melt? Why?

·                 If an ice cube was placed on a blue piece of paper, how much time do you think it would take to completely melt?

·                 Which color absorbs heat the quickest in the sun?

·                 Which color would be the best to help keep ice cubes from melting too quickly in the sun?

CREDIT: http://teachengineering.org/view_activity.php?url=http://www.teachengineering.org/collection/wpi_/activities/wpi_colors_absorb_heat_better/colors_absorb_heat_better.xml#assessment


Activity:  What Makes Day and Night? The Earth’s Rotation

 

  1. Discuss what students already know about night and day.
  2. Teach students about the rotational cycles of both the sun and the Earth.
  3. Review the vocabulary (sunrise, day, noon, sunset, night, spin and rotation).
  4. Darken room and turn on lamp. Explain that the lamp represents the Sun.
  5. Ask a student to be the Earth. Place the wrap-around map around the student so that your town is on his/her chest. Make sure he or she can be seen by all students.
  6. Mark your town with a sticker and ask students to focus on it as the Earth rotates.
  7. Have student begin with his/her back to the lamp (night). Ask students if they think it is day or night in their town.
  8. Have student rotate slowly in a counterclockwise fashion, until his/her left arm is pointed to the Sun. Ask students if they think it is sunrise or still night.
  9. Student continues the counterclockwise rotation until he/she faces the Sun directly. Ask students what time it is now in their town. Students can see that it is noon, the middle of the day, when we get the most light from the Sun. You may need to prompt with additional questions.
  10. Ask student to rotate a little more. Have him/her stop when his/her right arm is pointed toward the Sun. Ask students what time of day it is. They should be able to tell you that it is sunset.
  11. Complete the day/night cycle by having the student return to his/her original position, with his/her back to the Sun. Students should be able to tell you that it is midnight.
  12. Ask students to notice what time of day it is on the other side other Earth (student’s back is facing the Sun and it is noon). Explain that one half of the Earth is always light while the other is dark. Emphasize that it is the Earth's own shadow that makes the night side of the Earth dark.
  13. Repeat this demonstration. Select other students volunteers so that students will get a chance to view the day and night cycle several times. Explain that it takes 24 hours for the Earth to rotate completely.
  14. Distribute Day and Night work sheets for students to complete.

 

CREDIT: http://www.eyeonthesky.org/lessonplans/05sun_daynight.html

 

 

 


 

References:

 

Eye on the Sky Lesson Plans:

 http://www.eyeonthesky.org/index.html

 

Fotosearch: Solar Flares

http://www.fotosearch.com/results.asp?keyword=solar+flares&category=&searchtype=sss

 

Solar Data Analysis Center

http://umbra.nascom.nasa.gov/images/

 

National Geographic

http://science.nationalgeographic.com/science/space/solar-system/sun-article.html

 

TEACH Engineering Resources for K-12:

http://www.teachengineering.org/index.php

 

Teacher Vision: http://www.teachervision.fen.com/tv/tvsearch.php?keywords=the+sun&sitesearch=1

 

Views of the Solar System:

http://www.solarviews.com/browse/vss/VSS00031.jpg

 

 

 

ATTACHMENTS

 

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©2009  Last updated 10/04/2009

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