File:Classical Kepler orbit 80frames e0.6 smaller.gif
No higher resolution available.
Classical_Kepler_orbit_80frames_e0.6_smaller.gif (400 × 300 pixels, file size: 930 KB, MIME type: image/gif, looped, 80 frames, 8.0 s)
 | This is a file from the Wikimedia Commons. Information from its description page there is shown below. Commons is a freely licensed media file repository. You can help. |
Summary
| 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.
Licensing
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. |
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- 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.
You may select the license of your choice.
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 20:42, 18 January 2008 | | 400 × 300 (930 KB) | WillowW | Updated version following suggestions from Awadewit; yellow star - brilliant! :) |
| 18:50, 18 January 2008 |  | 400 × 300 (907 KB) | WillowW | 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 | {{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 |
File usage
The following 3 pages use this file:
Global file usage
The following other wikis use this file:
- Usage on ar.wikibooks.org
