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)
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[edit]DescriptionClassical Kepler orbit e0.6 light.gif | 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.
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[edit]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.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:47, 11 January 2008 | 800 × 600 (1.36 MB) | WillowW (talk | contribs) | {{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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