File:Classical Kepler orbit 80frames e0.6 smaller.gif
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| Description | Made by me using Blender on 18 January 2008. The radii and angles were computed using the eccentric anomaly formulae. The central star rotates six times per orbit, whereas the planet always maintains the same face towards the star (like the Earth's Moon). The planet is faintly lit on its "dark side" to help visualize it. |
| 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:
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 20:42, 18 January 2008 | | 400 × 300 (930 KB) | WillowW (talk | contribs) | Updated version following suggestions from Awadewit; yellow star - brilliant! :) |
| 18:50, 18 January 2008 |  | 400 × 300 (907 KB) | WillowW (talk | contribs) | updated version in which the rotation of the central star is less noticeable. Made by me on 18 January 2008 using Blender; radii and angles were determined from the eccentric anomaly formulae. | |
| 17:42, 18 January 2008 |  | 400 × 300 (956 KB) | WillowW (talk | contribs) | {{Information |Description=Made by me using Blender on 18 January 2008. The radii and angles were computed using the eccentric anomaly formulae. The central star rotates six times per orbit, whereas the planet always maintains the same face towards the |
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