... is expanding today, as we see it. The other is a prediction based on the physics of the early universe and on measurements of how fast it ought to be expanding,” explained Reiss. “If these values don't agree, there becomes a very ...
... kind at this scale and sensitivity and will open a new window (low frequency radio) into the early universe, analogous to the detection of gravitational waves by LIGO and the details of the CMB by Planck,” says Polidan in his...
... leftover radiation of the Big Bang and studies of this phenomena offer a unique window into the very early Universe and Planck scale physics, I.e. Physics on the tiniest of scales (a Planck length is 1.61×10−35 metres!). How the CMB got...
... first place. Luckily, data from the Planck satellite has already given scientists a snapshot of how the early Universe looked by studying the leftover radiation from the big bang; the cosmic microwave background (C. But since...
... field strength and structure in galaxies Since the starburst phenomenon was most likely more common in the early universe when close encounters among galaxies occurred frequently, detailed study of Messier 82 – as the nearest starburst galaxy - can...
... drive to push boundaries and explore have we arrived at this historical moment of seeing the deepest view of the early Universe to date.” Known as Webb’s First Deep Field, this image of galaxy cluster SMACS 0723 is overflowing with detail...