From Wikipedia, the free encyclopedia
| Description |
English: Two important surfaces around a rotating black hole. The inner sphere is the static limit (the event horizon). It is the inner boundary of a region called the ergosphere. The oval-shaped surface, touching the event horizon at the poles, is the outer boundary of the ergosphere. Within the ergosphere a particle is forced (dragging of space and time) to rotate and may gain energy at the cost of the rotational energy of the black hole (Penrose process).
|
| Source |
own work based on the graphic uploaded by IMeowbot
|
| Date |
2007-03-02
|
| Author |
MesserWoland
|
Permission
(Reusing this image) |
|
I, the copyright holder of this work, hereby publish it under the following license:
|
|
File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Dimensions | User | Comment |
| current | 16:14, 2 March 2007 | 1,645×1,660 (24 KB) | MesserWoland | |
File links
The following pages on the English Wikipedia link to this file (pages on other projects are not listed):