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Transcript
Name ______________________________ Class___________________Date__________________
Skills Worksheet
Directed Reading A
Section: The Sun: Our Very Own Star
_____ 1. The sun is a large ball of gas made mostly of
a. oxygen and carbon.
b. hydrogen and helium.
c. nitrogen and sulfur.
d. carbon dioxide and oxygen.
THE STRUCTURE OF THE SUN
Match the correct description with the correct term. Write the letter in the space
provided.
a. chromosphere
_____ 2. the sun’s outer atmosphere
_____ 3. the thin region below the sun’s
corona
_____ 4. the part of the sun that can be seen
from Earth
_____ 5. the region of the sun where gases
circulate
b. core
c. radiative zone
d. convective zone
e. corona
f. photosphere
_____ 6. the center of the sun
_____ 7. a very dense region of the sun
ENERGY PRODUCTION IN THE SUN
_____ 8. Early scientists thought that the sun produced its energy by
a. rotating.
b. expanding.
c. collapsing inward.
d. burning fuel.
_____ 9. Scientists later thought that energy to heat the sun was released from
a. gravity.
c. globules.
b. pressure.
d. kinetic energy.
_____ 10. Albert Einstein showed that matter and energy are
a. the same.
c. unchanging.
b. opposites.
d. interchangeable.
_____ 11. What formula did Einstein use to show the relationship between matter
and energy?
a. E = mc
c. M = ec
2
b. E = mc
d. M = ec2
Original content Copyright © by Holt, Rinehart and Winston. Additions and changes to the original content are the responsibility of the instructor.
Holt Science and Technology
4
Formation of the Solar System
Name ______________________________ Class___________________Date__________________
Directed Reading A continued
_____ 12. Einstein’s formula states that energy equals mass times the
a. speed of light.
b. square of the speed of light.
c. fusion of hydrogen.
d. fusion of helium.
13. The process by which two or more low-mass nuclei combine to form another
nucleus is called ______________________.
14. What happens as four hydrogen nuclei fuse?
15. Energy is produced in the center, or ______________________, of the sun.
16. Energy passes from the sun’s core through a dense region called
the______________________.
17. Hot gases are carried to the sun’s visible surface from a region called
the______________________.
18. Energy leaves the sun as light from a region called the
______________________.
SOLAR ACTIVITY
_____ 19. The circulation of gases in the sun combines with the sun’s rotation to
create
a. heat.
b. radiation.
c. electric fields.
d. magnetic fields.
20. Why do some areas of the photosphere become cooler than surrounding areas?
_______________________________________________________________
_______________________________________________________________
_______________________________________________________________
_______________________________________________________________
21. Cooler, dark areas of the photosphere of the sun are called
______________________.
22. The sunspot cycle lasts about ______________________years.
Original content Copyright © by Holt, Rinehart and Winston. Additions and changes to the original content are the responsibility of the instructor.
Holt Science and Technology
5
Formation of the Solar System
Name ______________________________ Class___________________Date__________________
Directed Reading A continued
23. How might sunspot activity affect Earth?
_______________________________________________________________
_______________________________________________________________
_______________________________________________________________
24. Regions of very high temperature and brightness on the sun’s surface are
called______________________.
25. How might Earth be affected by the eruption of solar flares?
_______________________________________________________________
_______________________________________________________________
_______________________________________________________________
Original content Copyright © by Holt, Rinehart and Winston. Additions and changes to the original content are the responsibility of the instructor.
Holt Science and Technology
6
Formation of the Solar System