File:Classical Kepler orbit e0.6.gif

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Classical_Kepler_orbit_e0.6.gif ‎(800 × 600 pixels, file size: 1.46 MB, MIME type: image/gif, looped, 40 frames, 1.6 s)

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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.
Date
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.
Author Willow
 
This animation was created with Blender by GIF.

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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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Date/TimeThumbnailDimensionsUserComment
current09:39, 11 January 2008Thumbnail for version as of 09:39, 11 January 2008800 × 600 (1.46 MB)WillowW (talk | contribs){{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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