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)

Summary

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.

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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16 January 2008

image/gif

9a1d87036bee9ff42665d6120a35b06e75f46725

4,200,654 byte

11.999999999999973 second

600 pixel

800 pixel

File history

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Date/TimeThumbnailDimensionsUserComment
current13:06, 17 January 2008Thumbnail for version as of 13:06, 17 January 2008800 × 600 (4.01 MB)WillowWI 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{{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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