File:Classical Kepler orbit 120frames e0.6.gif

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Classical_Kepler_orbit_120frames_e0.6.gif ‎(800 × 600 pixels, file size: 4.01 MB, MIME type: image/gif, looped, 120 frames, 12 s)

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Description Made by me using Blender on 16 January 2008. Radii and angles were calculated using the eccentric anomaly formulae, and corresponds to an elliptical orbit with an eccentricity of 60%.
Date
Source Own work
Author WillowW
 
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
current13:06, 17 January 2008Thumbnail for version as of 13:06, 17 January 2008800 × 600 (4.01 MB)WillowW (talk | contribs)I might have made a mistake in the previous version, since the planet seemed to pause at the beginning. Updated version has been double-checked for that.
12:47, 17 January 2008Thumbnail for version as of 12:47, 17 January 2008800 × 600 (4.01 MB)WillowW (talk | contribs){{Information |Description=Made by me using Blender on 16 January 2008. Radii and angles were calculated using the eccentric anomaly formulae, and corresponds to an elliptical orbit with an eccentricity of 60%. |Source=self-made |Date=16 January 2008 |Au

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