Sorry! Omdat deze pagina niet beschikbaar is in de taal van uw voorkeur tonen wij de originele pagina.
Testing general relativity with a supermassive black hole
This infographic shows a simulation of the outflow (bright red) from a black hole and the accretion disk around it, with simulated images of the three potential shapes of the event horizon’s shadow.
Credit:ESO/N. Bartmann/A. Broderick/C.K. Chan/D. Psaltis/F. Ozel
Over de afbeelding
| Id: | eventhorizon-shadows |
| Type: | Ontwerp |
| Publicatiedatum: | 28 april 2017 12:01 |
| Grootte: | 3277 x 3277 px |
Over het object
| Type: | Unspecified : Star : Evolutionary Stage : Black Hole Unspecified : Galaxy : Component : Central Black Hole |
| Categorie: | Quasars and Black Holes |
