File:Classical Kepler orbit e0.6 light.gif

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Classical_Kepler_orbit_e0.6_light.gif(800 × 600 pixels, file size: 1.36 MB, MIME type: image/gif, looped, 40 frames, 1.6 s)

Summary

Description A remake of Image:Classical_Kepler_orbit_e0.6.gif in which the orbiting "planet" is itself luminous. Perhaps that's OK, since I chose the eccentricity from the binary star system of pulsar PSR B1913+16, which is famous in general relativity for its gravitational radiation. A key difference, however, is that, here, one star is absolutely fixed, being much more massive than the other.
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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Captions

A representation of the moons orbit around earth

Items portrayed in this file

depicts

image/gif

ff093a1aad14e841c02db2160341db694e4ac75d

1,423,030 byte

1.6000000000000008 second

600 pixel

800 pixel

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Date/TimeThumbnailDimensionsUserComment
current17:47, 11 January 2008Thumbnail for version as of 17:47, 11 January 2008800 × 600 (1.36 MB)WillowW{{Information |Description=A remake of Image:Classical_Kepler_orbit_e0.6.gif in which the orbiting "planet" is itself luminous. Perhaps that's OK, since I chose the eccentricity from the binary star system of pulsar PSR B1913+16, which is famous in
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