SA2_NEXT
Since the beginning of the 20th century, huge breakthroughs have been made in the field of physics. But many mysteries are still waiting to be revealed. In astrophysics and cosmology, dark matter is one of the great unknowns that remains today. It escapes the Standard Model, and is estimated to account for more than 80% of the matter that exists in the entire Universe. However, we can only “see” it through the gravitational effects it causes, as it does not emit any electromagnetic radiation.
SA2_GRWA
A primeira detección experimental das ondas gravitacionais, acadada pola colaboración LIGO no ano 2015, é un dos grandes fitos científicos do século XXI. Estas perturbacións no espazo-tempo están causadas por algúns dos fenómenos cósmicos máis violentos, como as fusións de buracos negros e estrelas de neutróns ou as explosións de supernovas, Deste xeito, estes eventos contribúen a validar a teoría da relatividade xeral exposta por Einstein en 1915.
SA2_AUGE
We are exposed to a constant ‘bombardment’ of cosmic rays, which impact with us at near-light speeds. Approximately at a frequency of one ray per second on a surface like the palm of your hand. Luckily, these are harmless radiations, but fascinating because they come from far, far away in the universe.