Image:Classical Kepler orbit e0.6 light.gif
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{{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 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=self-made |Date= |Author= WillowW |Permission= |other_versions=
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| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 17:47, 11 January 2008 | 800×600 (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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