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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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:
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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. |
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
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- to share – to copy, distribute and transmit the work
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- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
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File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:06, 17 January 2008 | | 800 × 600 (4.01 MB) | WillowW | 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 | {{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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