k Reionization of the Universe Following the Big Bang, the Universe was little more than a soup of charged subatomic particles and energy top, red. and energy top, red. As the Universe expanded and cooled, there came a point at an age of 300, 000 years when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. As the Universe expanded and cooled, there came a point at an age of 300, 000 years when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. This heralded the socalled Dark Ages, when the Universe became opaque. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining hydrogen gas. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining neutral hydrogen, beginning the socalled Epoch of Reionization. At an age of 1 billion years, the Universe became transparent again bottom. Stock Photo - Afloimages
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Reionization of the Universe Following the Big Bang, the Universe was little more than a soup of charged subatomic particles and energy  top, red . and energy  top, red . As the Universe expanded and cooled, there came a point     at an age of 300, 000 years     when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. As the Universe expanded and cooled, there came a point     at an age of 300, 000 years     when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. This heralded the so called Dark Ages, when the Universe became opaque. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining hydrogen gas. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining neutral hydrogen, beginning the so called Epoch of Reionization. At an age of 1 billion years, the Universe became transparent again  bottom .
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Reionization of the Universe

Following the Big Bang, the Universe was little more than a soup of charged subatomic particles and energy (top, red). and energy (top, red). As the Universe expanded and cooled, there came a point â€" at an age of 300, 000 years â€" when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. As the Universe expanded and cooled, there came a point â€" at an age of 300, 000 years â€" when most of the protons and electrons had combined to form a sea of neutral hydrogen gas. This heralded the so-called Dark Ages, when the Universe became opaque. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining hydrogen gas. These new structures unleashed a torrent of ionizing radiation that began to ionize the remaining neutral hydrogen, beginning the so-called Epoch of Reionization. At an age of 1 billion years, the Universe became transparent again (bottom).

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