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Description
In this hands-on activity, students use similar triangles and proportions to
create a shoebox eclipse viewer. The students simulate a total eclipse by
making a model that uses the diameters of circles and proportional reasoning
to determine where to place one object so that it eclipses an object farther
away. They apply what they learn about angular size to predict the diameter
and distance of another object that can be eclipsed at even greater
distance. |
Instructional Objectives
Students will:
- make simple measurements to determine indrect measures.
- make and test conjectures about the relationship between side
length and angle measure in triangles.
- measure an angle using a protractor.
- solve problems that involve the use of proportions.
- create a model of a solar eclipse.
- understand how the distance away from the viewer affects the
angular size of an object on Earth and in space.
- explain the conditions necessary for a solar eclipse to occur.
- use appropriate data gathering techniques and clearly communicate
ideas.
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