File:FY221c15.png
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Summary
| Description | Un exemple de trou de ver dans une métrique de Schwarzschild tel qu'il serait vu par un observateur ayant franchi l'horizon du trou noir. La région d'où vient l'observateur est située à droite de l'image. Mise à part la région située près de l'ombre du trou noir, les effets de décalage vers le rouge gravitationnel rendent le fond du ciel très sombre. Celui-ci est en revanche très lumineux dans la seconde région visible une fois l'horizon passé. Cette région ne sera cependant pas accessible quelle que soit la trajectoire de l'observateur car celui-ci est condamné à finir sur la singularité gravitationnelle en un temps relativement bref. |
| Date | 9 July 2006 (original upload date) |
| Source | No machine-readable source provided. Own work assumed (based on copyright claims). |
| Author | No machine-readable author provided. Alain r assumed (based on copyright claims). |
Licensing
I, the copyright holder of this work, hereby publish it under the following licenses:
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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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This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | |
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| This licensing tag was added to this file as part of the GFDL licensing update. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 02:45, 4 February 2022 | | 2,560 × 2,048 (1.62 MB) | wikimediacommons>TSamuel | Careful further recompression via Compress-Or-Die.com: decrease color count |
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