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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[edit]DescriptionClassical Kepler orbit 120frames e0.6.gif | 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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[edit]I, the copyright holder of this work, hereby publish it under the following licenses:
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.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 13:06, 17 January 2008 | 800 × 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 2008 | 800 × 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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