Image:Classical Kepler orbit 80frames e0.6 smaller.gif
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Classical_Kepler_orbit_80frames_e0.6_smaller.gif (400 × 300 pixels, file size: 930 KB, MIME type: image/gif)
| This is a file from the Wikimedia Commons. The description on its description page there is shown below.
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[edit] 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. |
|---|---|
| Source |
self-made |
| Date |
18 January 2008 |
| Author | |
| Permission (Reusing this image) |
see below |
[edit] Licensing
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | 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 ) |
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