File:PyramidOrbitPlot.jpg
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| Description |
English: Two representations of a pyramid orbit around a supermassive black hole. Left: base of the orbit, plotted in terms of the two components of the eccentricity vector. Right: time evolution of the angular momentum. Red lines demarcate the area within which a star would be captured or disrupted by the black hole. |
| Date | |
| Source | Own work |
| Author | UlmPhysiker |
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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. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:08, 25 June 2010 | | 1,435 × 647 (203 KB) | UlmPhysiker (talk | contribs) | {{Information |Description={{en|1=Two representations of a pyramid orbit around a supermassive black hole. Left: base of the orbit, plotted in terms of the two components of the eccentricity vector. Right: time evolution of the angular momentum. Red lines |
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