Illustration of a supermassive black hole. The mass of the black hole increases the curvature of spacetime. This curvature has a boundary called the event horizon. Matter and light falls towards the black hole and cannot escape once past the event horizon. The edge of black holes are thought to glow with Hawking radiation, indicated by the thin green line around the black hole. | |
Lizenzart: | Lizenzpflichtig |
Credit: | Science Photo Library / Andrade, Ramon / 3dciencia |
Bildgröße: | 5120 px × 3840 px |
Modell-Rechte: | nicht erforderlich |
Eigentums-Rechte: | nicht erforderlich |
Restrictions: | - |