Looking Beyond

Looking Beyond — page 3
THE BIG BANG In the 1920s US astronomer Edwin Hubble discovered that the Universe is expanding very fast This meant back in time galaxies were much closer together In fact go back far enough and all matter and energy must have been in one tiny place NASA Wilkinson Microwave Anisotropy Probe WMAP Reflectors Optics Solar array Launched in 2001 WMAP measured traces of microwave background radiation left from the Big Bang The cooler blue areas are where gravity first caused matter to collapse and form stars EPIC EXPANSION Imagine the future entire Universe within one original particle smaller than a single atom Then 13 8 billion years ago it erupted in the Big Bang In a tiny fraction of a second it became the size of a grapefruit with two of the Universe’s basic forces gravity and the strong nuclear force A microsecond later this expanded as a fizzing cauldron of energy and particles trillions of degrees hot with the two other basic forces weak nuclear and electromagnetic The European Space Agency’s Planck spacecraft recently produced an even more detailed heat map of the Universe The denser areas probably came from tiny fluctuations within the original particle before it inflated after the Big Bang A visual timeline of the Universe from its origin 13 8 billion years ago Inflation Quantum fluctuations in original particle Afterglow light pattern 375,000 years First stars 400 million years Development of galaxies solar systems and planets Dark energy accelerated expansion WMAP Dark ages THE FIRST MATTER Still after less than one second the Universe cooled enough for fundamental particles called quarks to combine They formed atomic particles such as protons and electrons as a vast dark fog of hydrogen After three minutes it was cool enough for protons to link with neutrons and electrons forming atoms of helium gas By 400,000 years the Universe now cool at 4,900 ºF 2,700 ºC glowed with the first light 06