The Cherenkov Telescope Array (CTA) Southern Site
The Cherenkov Telescope Array (CTA) is the next-generation ground-based instrument designed to detect very high energy gamma rays, with sites in both the southern and northern hemispheres. Gamma rays are electromagnetic radiation of a very high energy, emitted by the hottest and most extreme objects in the Universe — supermassive black holes, supernovae and maybe even remnants of the Big Bang.
The material has been edited especially for broadcast use, without commentary or music.Źródło:
ESO/ P. Horálek
|Data publikacji:||20 grudnia 2018 12:00|
|Czas trwania:||02 m 11 s|
|Frame rate:||30 fps|