1 00:00:01,070 --> 00:00:05,070 [Music throughout] Immediately after the universe was born, it was too tiny 2 00:00:05,070 --> 00:00:09,070 and too hot for protons, electrons and even photons to exist. 3 00:00:09,070 --> 00:00:13,070 Within a second, it had expanded and cooled enough for 4 00:00:13,070 --> 00:00:17,070 protons and neutrons, collectively called baryons, to form. 5 00:00:17,070 --> 00:00:21,070 Almost instantly, there was a rapid burst of sound waves triggered by tiny 6 00:00:21,070 --> 00:00:25,070 variations in this particle soup. Scientists call these waves 7 00:00:25,070 --> 00:00:29,070 Baryon Acoustic Oscillations. The pressure waves traveled outward 8 00:00:29,070 --> 00:00:33,070 for 400,000 years until the universe thinned and cooled enough 9 00:00:33,070 --> 00:00:37,070 for light to travel through it. The universe became transparent 10 00:00:37,070 --> 00:00:41,070 and the waves froze in place. Over 11 00:00:41,070 --> 00:00:45,000 time, the denser regions formed by the waves encouraged more star and galaxy formation 12 00:00:45,000 --> 00:00:49,070 than other areas. The imprint of those waves expanded 13 00:00:49,070 --> 00:00:53,000 with the universe, slowly accelerating due to dark energy. 14 00:00:53,000 --> 00:00:57,070 Today, with our “snapshot” of the universe, there is a 15 00:00:57,070 --> 00:01:01,070 slight tendency for galaxies to be separated from each other by a 16 00:01:01,070 --> 00:01:05,070 distance related to that expanding-ring radius. 17 00:01:05,070 --> 00:01:09,070 Although difficult to see, it is 18 00:01:09,070 --> 00:01:13,070 detectable as a slight bump through careful surveys of many galaxies. 19 00:01:13,070 --> 00:01:18,784 [Music]