The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that...

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The Sun! PH 545-549

Transcript of The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that...

Page 1: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

The Sun!

PH 545-549

Page 2: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 3: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

Previously, in physical science…

You learned how gravity is a force that attracts all objects toward each other. Now, you will learn about the role of gravity in maintaning the shape of the sun. You will also learn about the structure of the sun and how it produces energy!

Page 4: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

I print out a copy of this for each student. You can also have the students make their own!

Page 5: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 6: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 7: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 8: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 9: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 10: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

1. What is the source of light in the solar system?

• The sun!

• Planets and moons do not produce their own light, the reflect the sun’s

Page 11: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

2. What powers the sun?

• The sun produces energy through nuclear fusion.

Page 12: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

3. Why doesn’t the sun explode?

• Gravity pulls matter inward!

Page 13: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

4. What are the interior layers of the sun?

The core, the radiation zone, and the convection zone.

Page 14: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label the “core” on your diagram. Also label that it is 15 million degrees Celsius and where the sun’s energy is produced. Color it light yellow.

Page 15: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label the “radiation zone.” Matter is tightly packed and energy is transferred by radiation. Color it dark yellow

Page 16: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label the “convection zone.” This is where hot gases rise from the bottom to the surface. Color this orange.

Page 17: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 18: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 19: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

5. What are the 3 layers of the sun’s atmosphere?The photosphere, the chromosphere, and the

corona

Page 20: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label “photosphere.” This is what we think of as the surface of the sun, where light is produced. Color this dark orange.

Page 21: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label “chromosphere.” This is the middle layer of the atmosphere and appears red. Color this red.

Page 22: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

• Find and label the “corona.” The outer layer of the sun’s atmosphere. Visible only during a solar eclipse. Color this white?

Page 23: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 24: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

6. What is solar wind?

• Electrically charged particles which disrupt TV, radio, & telephones. Cause the Aurora Borealis & Aurora Australis.

Page 25: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 27: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

7. What are 3 important features on the sun’s surface?1. Sunspots – areas of cooler gas (appear

dark)

2. Prominences – reddish loops connecting sunspots.

3. Solar flares – giant eruptions on the sun.

Page 28: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 29: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 30: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 31: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 32: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 33: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 34: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 35: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 36: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.
Page 37: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

8. How old is the sun?

• About 4.5 billion years

Page 38: The Sun! PH 545-549. Previously, in physical science… You learned how gravity is a force that attracts all objects toward each other. Now, you will.

9. What will happen to the sun in the future?

• It will eventually run out of hydrogen, enlarge, and end life on Earth.