|
In this lesson the ellipse is studied in polar coordinates (r,f), with the function cos(f). This places the origin point at a focus (more appropriate for planetary motion) and introduces the eccentricity e. It is also noted 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. It ends with a discussion of parabolic and hyperbolic orbits. Students will become familiar with graphs of the form r = F(f) in polar coordinates (r,f), in particular with the circle, ellipse and other conic sections. They will understand the role of the semi-major axis and eccentricity in determining the nature of an ellipse and that the fixed point in any planetary system is its center of gravity.
|
|
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-000-000-005-164
|
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 |