Image:FY221c15.png

[edit] Summary

View of a Schwarzschild wormhole as would be seen by a free falling observer on a Schwarschild black hole. The region from which the observer originates is on the right. The black hole shadow is a black circle that becomes an annulus once the observer passes through the horizon. The second asymptotic region appears on the middle of the shadow (left). Note that gravitational and kinematical blueshift effects make the second (unreachable) region appear much brighter than the other one.

[edit] Licensing

I, the author 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". العربية | Česky | Deutsch | English | Español | Français | Italiano | 日本語 | 한국어 | Nederlands | Polski | Português | Slovenčina | Svenska | עברית +/- This file is licensed under the Creative Commons Attribution ShareAlike license versions 2.5, 2.0, and 1.0 You may select the license of your choice.