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In astrophysics, the ergosphere is a region located just outside a rotating black hole, between its event horizon and a further external surface predicted by the Kerr metric which describes these objects. Its name was proposed by Remo Ruffini and John Archibald Wheeler during the Les Houches lectures in 1971 and is derived from Ancient Greek ἔργον…
Regions, Radial pull & Rotation
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black hole event horizon rotating surface energy radius rotation limit outside angular momentum speed distance process possible equator region spacetime
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Ergosphere | is a | region located just outside a rotating black hole | 0.90 | text |
| Ergosphere | is a | Schwarzschild radius | 0.90 | text |
| Ergosphere | related to Ergosphere size | The | 0.60 | section |
| Ergosphere | related to Ergosphere size | This | 0.60 | section |
| Ergosphere | related to Ergosphere size | As | 0.60 | section |
| Ergosphere | related to Radial pull | At | 0.60 | section |
| Ergosphere | related to Radial pull | An | 0.60 | section |
| Ergosphere | related to Radial pull | Since | 0.60 | section |
| Ergosphere | related to Radial pull | Oberth | 0.60 | section |
| Ergosphere | related to Rotation | As | 0.60 | section |
| Ergosphere | related to Rotation | This | 0.60 | section |
| Ergosphere | related to Rotation | Lense | 0.60 | section |
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