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Detailed Lesson Plan in Science V I. Objectives: At the end of the session, pupils must be able to: a. define what is sun; b. enumerate the parts of the sun; c. match the names to the pictures of the sun’s parts; and d. identify the parts of the sun. II. Subject Matter: The Sun and Its Parts References: http://science.howstuffworks.com/sun1.htm http://www.spacestationinfo.com/layers-sun.htm http://wiki.answers.com/Q/What_are_the_different_parts_of_the_sun Materials: laptop, speaker, LCD projector Strategy: Reception Learning Approach Values Integration: appreciation of the wonder of the heavenly bodies III. Procedures: Teacher’s Activity Drill Good morning, class! How are you today? Well, that’s good to hear. Before anything else, Decilove please lead the prayer. Everybody, have a seat first. Who are absent today? It’s very good that you have a perfect attendance for today. To energize you up, let’s have first an action song. All we have to do is follow what is projected in front. Am I understood class? (Video presentation) Review Last meeting class, we have talked all about the types of soil. Let us see if you can still remember your past lesson. Pupils’ Activity Good morning, teacher! We’re fine teacher! (The class prays.)

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Detailed Lesson Plan in Science V

I. Objectives: At the end of the session, pupils must be able to: a. define what is sun; b. enumerate the parts of the sun; c. match the names to the pictures of the sun’s parts; and d. identify the parts of the sun.

II. Subject Matter: The Sun and Its Parts References: http://science.howstuffworks.com/sun1.htm

http://www.spacestationinfo.com/layers-sun.htmhttp://wiki.answers.com/Q/What_are_the_different_parts_of_the_sun

Materials: laptop, speaker, LCD projector Strategy: Reception Learning Approach Values Integration: appreciation of the wonder of the heavenly bodies

III. Procedures:

Teacher’s Activity

Drill

Good morning, class!How are you today?Well, that’s good to hear.

Before anything else, Decilove please lead the prayer.Everybody, have a seat first. Who are absent today?It’s very good that you have a perfect attendance for today. To

energize you up, let’s have first an action song. All we have to do is follow what isprojected in front. Am I understood class?

(Video presentation)

Review

Last meeting class, we have talked all about the types of soil.Let us see if you can still remember your past lesson.

Pupils’ Activity

Good morning, teacher!We’re fine teacher!

(The class prays.)

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None, teacher.

I need five pupils to come here in front and answer the questions by clicking ontheir choice of answer in the laptop. Am I clear, class?

I want Anna Mae, Airene, Dennis Jay, Ana, and Mark Joseph toanswer.

New Lesson

Motivation

I am looking for some phrases and I want your help. Under the blanksare numbers and these numbers have equivalent letters shown in the box. Canyou form them for me?

To do this, I want you to do it individually. The first pupil to finish willbe rewarded. Am I clear, class?

Presentation of the Lesson

Class, what do you think is our lesson for today based on the phrasesthat you have formed?

Discussion

I’m going to show you a video presentation about the parts of the sun.After the presentation, we’ll sum up the video; so please watch and listenattentively.

(Video presentation)

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Yes, teacher!

(The pupils will answer the questions.)

Yes, teacher!

Yes, teacher!

The Sun and its parts, teacher.

GeneralizationSo class, who can now tell me the parts of the sun?

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Yes, Kate.

That’s all correct.

ApplicationDirections: Label the picture with the parts of the sun. (Through PowerPoint Presentation)

Core

Radiative Zone

Convective Zone

Photosphere

Chromosphere

Corona

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I, teacher!The parts of the sun are the core, the radiative zone, the convective zone, thephotosphere, the chromosphere, and the corona.

IV. Evaluation

Directions: Answer the following questions by clicking on the answer of your choice.(through PowerQuizPoint Presentation)

Who Am I?

I am the only part that you see. Solar flares also occur in me.

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Convective Zone b. Chromosphere c. Photosphere

The extremely hot outermost layer, I am extending outward several millionmiles from the chromospheres. I am only visible during total solar eclipses. Corona b. Prominence c. Spicules

I am the innermost and the hottest layer of the Sun where nuclear fusion takesplace. I am also the source of all the Sun’s energy. Core b. Prominence c. Radiative

Zone

I am a very dense layer and I provide an efficient means of transferring energyfrom the core to the surface. Radiative Zone b. Convective Zone c. Photosphere

I am the area between the photosphere and corona and I am hotter thanphotosphere. a. Convective Zone b. Chromospherec. Radiative Zone

I am the layer in which gases chum with potent motions to carry energy to theSun’s surface. Convective Zone b. Radiative Zone c. Core

I am dark, cooler regions on the photosphere.

Spicules b. Sunspots c. Aurorae

You see my lights in the North Pole.

Aurora Borealis b. Aurora Australis c. Flare

You can also find my lights in the South Pole.

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Aurora Borealis b. Aurora Australis c. Flare

I am a huge ball of hot gases.

Sun b. Moon c. Earth

V. Assignment

From our lesson today, Sun is a star. Search on the Internet how our Sun andthe other stars in the universe differ from each other. Make a short PowerPointPresentation on this.

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Detailed Lesson Plan

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