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Lesson Plan
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NASA

Earth, Can You Hear Me Now?

For Teachers 10th - 12th Standards
How long did you say? Class groups plot the distances between Earth and Mars and determine the trigonometric function that models the data. Using a calculator, they graph the function to determine when the distance and communication...
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Lesson Plan
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NASA

The Lunar Lander – Ascending from the Moon

For Teachers 10th - 12th Standards
What angle? Groups determine the height of the lunar lander as it ascends from the surface of the moon and calculate the angle of elevation of the lunar lander at specific times and distances. The provided series of questions lead the...
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Lesson Plan
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NASA

Simulating Weightlessness

For Teachers 10th - 12th
Floating across the top. Class groups examine the parabolas, written as parametric equations, that model the flight path of NASA's C-9 as it simulates weightlessness. They continue their exploration by changing the parameters to...
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Lesson Plan
Curated OER

Ellipses and Kepler's First Law

For Teachers 11th - 12th
The class examines graphs in the form r = F(¿¿) in polar coordinates (r, ¿¿), in particular with the circle, ellipse and other conic sections. They determine the nature of an ellipse by studying the role of the semimajor axis and...
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Lesson Plan
Curated OER

Introduction To Orbital Mechanics

For Teachers 11th - 12th
Young scholars use NASA drawings to build a model satellite for a specific mission. They design a set of drawings for their satellite showing its subsystems as well.
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Lesson Plan
Curated OER

Saving Energy Through Ecological Landscape Design

For Teachers 9th - 12th
Students are able to transcribe to scale the plant features of a common landscape. They determine true north and south and collect and record data on a table. Students calculate a rating for and describe a definition of insulation and...
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Lesson Plan
Curated OER

Ellipses And Kepler's First Law

For Teachers 9th - 12th
High schoolers explain that planets actually orbit the center of gravity of the solar system, and that distant planets may be detected by motions of their central star around the centers of gravity of their planetary systems.