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This lesson introduces students to Kepler's second law; that planets (and satellites) move fastest at their closest approach to the center of attraction and slow down when far away. This is made evident by calculating the ratio of greatest and smallest orbital velocities and by invoking the concept of energy. Students should acquire an intuitive understanding for the way orbital velocities vary along each orbit according to Kepler's second law. They will review the concepts of potential energy and kinetic energy and understand that orbital motion also conserves energy, in a somewhat similar way, although the formulas look different. Students will also be introduced to the procedure for calculating orbital motion.
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Intended for grade levels:
Type of resource:
Subject:
Technical requirements:
No specific technical requirements, just a browser required
Cost / Copyright:
No cost
May be used non-commercially as long as credit is given to the author.
DLESE Catalog ID:
DLESE-000-000-005-165
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Educational standards:
Related resources:
This resource is referenced by
'From Stargazers to Starships'
Resource contact / Creator / Publisher:
Author:
Dr David P. Stern Goddard Space Flight Center |