File:Neutronstar Light Deflection.svg
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| Description |
English: Gravitational light deflection at a neutron star Deutsch: Umlauf eines masselosen Begleitsterns (rot) um einen Neutronenstern (blau). Der Begleitstern befindet sich schräg hinter dem Neutronenstern. Sein Anblick wird durch die gravitative Lichtablenkung verzerrt. Die Geometrie und Farbgebung der dargestellten Szene ist astrophysikalisch völlig unrealistisch (in dieser Nähe eines Neutronensterns wäre ein Begleiter nicht stabil). Sie wurde so gewählt, dass der Einfluss der gravitativen Lichtablenkung deutlich zu sehen ist. Masse des Neutronensterns: 1, Radius des Neutronensterns: 4, Radius des Begleitsterns: 8, Bahnradius: 20, alle Zahlenwerte in dimensionslosen Einheiten. |
| Date | |
| Source | Own work based on: Neutronstar Light Deflection.png |
| Author |
Corvin Zahn, Institute of Physics, Universität Hildesheim Vector: |
| SVG development |
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I, the copyright holder of this work, hereby publish it under the following license:
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Original upload log[edit]
This image is a derivative work of the following images:
- File:Neutronstar Light Deflection.png licensed with Cc-by-sa-2.0-de
- 2005-08-15T10:32:29Z CorvinZahn 1024x768 (7598 Bytes) '''Description:''' Gravitational light deflection at a neutron star '''Source:''' [http://www.tempolimit-lichtgeschwindigkeit.de/galerie/galerie.html] '''Date:''' 09.10.1990 '''Author:''' [http://www.tat.physik.uni-tuebing
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 10:54, 12 July 2020 | | 500 × 400 (12 KB) | Mrmw (talk | contribs) | simpler code |
| 14:13, 23 February 2011 |  | 720 × 600 (44 KB) | Gregors (talk | contribs) | {{Information |Description={{en|Gravitational light deflection at a neutron star}} {{de|Umlauf eines masselosen Begleitsterns (rot) um einen Neutronenstern (blau). Der Begleitstern befindet sich schräg hinter dem Neutronenstern. Sein Anblick wird durch d |
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