File:CMB universe expansion.png

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English: Timeline of the universe. A representation of the evolution of the universe over 13.77 billion years. The far left depicts the earliest moment we can now probe, when a period of "inflation" produced a burst of exponential growth in the universe. (Size is depicted by the vertical extent of the grid in this graphic.) For the next several billion years, the expansion of the universe gradually slowed down as the matter in the universe pulled on itself via gravity. More recently, the expansion has begun to speed up again as the repulsive effects of dark energy have come to dominate the expansion of the universe. The afterglow light seen by WMAP was emitted about 375,000 years after inflation and has traversed the universe largely unimpeded since then. The conditions of earlier times are imprinted on this light; it also forms a backlight for later developments of the universe.
Español: Diagrama de la evolución del universo desde el Big Bang (izquierda) hasta la actualidad.
Français : Frise chronologique de l'univers, depuis le Big Bang jusqu'à nos jours.
Русский: Временна́я шкала Вселенной
Українська: Хронологія Всесвіту
Português: Diagrama da evolução do universo desde o Big Bang (esquerda) até o presente.
日期 約2006年
date QS:P,+2006-00-00T00:00:00Z/9,P1480,Q5727902
來源 Original version: NASA; modified by Cherkash, Richardbrucebaxter
作者 NASA/WMAP Science Team/ Art by Dana Berry
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本檔案衍生自: CMB Timeline300 no WMAP.jpg

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目前2019年5月25日 (六) 16:09於 2019年5月25日 (六) 16:09 版本的縮圖3,000 × 3,960(3.35 MB)Richardbrucebaxter== {{int:filedesc}} == {{Information |description= {{en|1=Timeline of the universe. A representation of the evolution of the universe over 13.77 billion years. The far left depicts the earliest moment we can now probe, when a period of "inflation" produced a burst of exponential growth in the universe. (Size is depicted by the vertical extent of the grid in this graphic.) For the next several billion years, the expansion of the universe gradually slowed down as the matter in...

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