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File:Classical Kepler orbit e0.6.gif

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Classical_Kepler_orbit_e0.6.gif (800 × 600 pixels, file size: 1.46 MB, MIME type: image/gif, looped, 40 frames, 1.6 s)

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Summary

Description GIF animation of a Kepler orbit with eccentricity 0.6. Once perfected, this will be the basis of several related animations for orbital precession, Newton's theorem of revolving orbits and the Laplace-Runge-Lenz vector.
Date
Source I made this image using Blender and the classical Kepler equations using the eccentric anomaly, described in the classical mechanics textbook of Herbert Goldstein. The numerical values of the radius and angle as a function of time were calculated by my own GPL computer program.
Author Willow
 
This animation was created with Blender by GIF.

Licensing

I, the copyright holder of this work, hereby publish it under the following licenses:
GNU head 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.
w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 3.0 Unported license.
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  • to remix – to adapt the work
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Captions

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Items portrayed in this file

depicts

inception

10 January 2008

media type

image/gif

checksum

3df6dcd0fafc67d7f80aaa7f8e94d64b10147685

determination method or standard: SHA-1

data size

1,535,342 byte

duration

1.6000000000000008 second

height

600 pixel

width

800 pixel

File history

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Date/TimeThumbnailDimensionsUserComment
current09:39, 11 January 2008Thumbnail for version as of 09:39, 11 January 2008800 × 600 (1.46 MB)WillowW{{Information |Description=GIF animation of a Kepler orbit with eccentricity 0.6. Once perfected, this will be the basis of several related animations for orbital precession, Newton's theorem of revolving orbits and the Laplace-Runge-Lenz vector. |Source

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