[DoDEA Science]

DRAFT

Reason for the Seasons

Astronomy


Grade Level 10 - 12
Standards Inquiry Skills
    Students will design and conduct scientific investigations
  Astronomy Content
    Students will relate solar system motions to time
Objectives
  1. Recognize that the motions of the sun, moon and earth result in our standard year, day, and hour.
  2. Discover the relationship between the length of a day and the season of the year.
  3. Use mathematics to explain and interpret the investigation.
  4. Use appropriate tools and technology to gather, analyze and interpret data.
  5. Predict the effects of a change in the physical solar system to show an understanding of the concept.
Materials and Activities
Materials globe 
Vernier or Team Labs temperature probe and software
black paper 
protractor
large bulbed light source
small styrofoam ball
Engage Disequilibrium discussion question: Where is the Earth in its orbit around the sun on the winter solstice? Why is it that when we are the closest to the sun, we are in our coldest season? Discuss with students the tilt of the Earth's axis and the difference between the northern and southern hemispheres.
Explain Produce a graph from the exploration of temperature versus angle. Students should develop an explanation of the resulting graph. Students should understand the activity is a model of the real Earth and may produce positive temperatures at the pole (where in the real Earth system we have negative temperatures).
Explore Cut and place a black strip on the globe from the equator to the poles. Position the globe near the light source and turn off the classroom lights. The position of the axis and globe is very important to the understanding of the activity. The northern hemisphere should be tilted away from the light source. 

Measure the temperature with the probe touching the black paper at each of the following locations:
 

Angle       Temperature
0oN
30oN
45oN
60oN
75oN
90oN
Students should look for patterns in the data and summarize. This can be repeated for the southern hemisphere and a summer location/axis tilt.
Elaborate Students should use the globe and a styrofoam ball to model the earth moon system daily and monthly. Then, students should physically stand with the globe tilted towards the light and walk through the seasons by walking around the light source/sun showing the seasons. Aphelion and perihelion are terms that should be introduced along with winter and summer solstice and vernal and autumnal equinox.
Evaluation Students will show their knowledge of the seasons and the effect of the tilt of the Earth's axis by answering the following:

If the tilt of the Earth's axis increased from 23.5o to 90o, how would our climate and seasons be effected?

Homework Show video of the Coriolis Effect called the Doldrums and Horse Latitudes. 

Teacher notes/reminders: For use with textbook Astronomy: From the Earth to the Universe pages 90-92. Redshift 2 or 3 or Easy Cosmos software have demonstrations in a multi-media format.
 



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Updated 9/00

Last Reviewed 10/2001

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