Image:Classical Kepler orbit e0.6.gif

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[edit] Summary

Description

GIF animation of a Kepler orbit with eccentricity 0.6. Once perfected, this will be the basis of several related animations for orbital precession, Newton's theorem of revolving orbits and the Laplace-Runge-Lenz vector.

Source

I made this image using Blender and the classical Kepler equations using the eccentric anomaly, described in the classical mechanics textbook of Herbert Goldstein. The numerical values of the radius and angle as a function of time were calculated by my own GPL computer program.

Date

10 January 2008

Author

Willow

Permission
(Reusing this image)

see below


[edit] Licensing

I, the copyright holder of this work, hereby publish it under the following licenses:
GNU head Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation license, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled "GNU Free Documentation license".

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This file is licensed under the Creative Commons Attribution 3.0 Unported License. In short: you are free to distribute and modify the file as long as you attribute its author(s) or licensor(s). Official license

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File history

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Date/TimeDimensionsUserComment
current09:39, 11 January 2008800×600 (1.46 MB)WillowW ({{Information |Description=GIF animation of a Kepler orbit with eccentricity 0.6. Once perfected, this will be the basis of several related animations for orbital precession, Newton's theorem of revolving orbits and the Laplace-Runge-Lenz vector. |Source)
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