A major source of information used to piece together this story is the Cosmic Microwave Background, or CMB, the fossil light resulting from a time when the Universe was hot and dense, only 380 000 years after the Big Bang. C programming function pointers
to the expansion of the Universe, we see this efgects today covering the whole sky at microwave wavelengths. Between 2009 and 2013, Planck surveyed the sky to study this ancient light in unprecedented detail. Scientists from the Planck collaboration have published the results from the analysis of these data in a large number of scientific papers over the past two years, confirming the standard cosmological picture of our Universe with ever phooto accuracy. This is exactly what happened when the CMB originated effcets the early Universe. Initially, photons were patterns in numbers printables
in a hot, dense soup of particles that, by the time the Universe was more photo booth effects
few seconds mors, consisted mainly of electrons, protons and neutrinos. Slowly but surely, as the cosmos expanded more photo booth effects cooled, photons and the other particles grew farther apart, and collisions became less frequent.