Big Bang theory video transcriptI'm
Astronomy magazine
Associate Editor Liz Kruesi. Welcome to Cosmology 101.
In this series I'll give you an overview of important ideas in the area of cosmology. This video is the first in the series, and focuses on the Big Bang theory.
Most of the confusion about the Big Bang revolves around two different incorrect ideas. The first is that the Big Bang theory discusses the origin of the universe. The second is that the Big Bang was an explosion. Here I'll explain what the Big Bang theory really states.
Ever since 1929, astronomers have known the universe is expanding. Edwin Hubble observed that all galaxies except the closest ones to us — which are those in our local group of galaxies — are moving away. In fact, the farther away a galaxy is, the faster it is receding. This expansion isn't motion through space. It's the expansion of space itself.
So, if space is expanding, then the universe must be slightly bigger, cooler, and less dense than it was yesterday. If we extrapolate backward, then in the earlier days the universe must have been smaller, hotter, and denser than observed today. So the universe must have begun in a very hot and very compact state. It's been expanding and therefore cooling for the past 13.7 billion years. For a time after the "beginning event," the universe was so hot that atoms couldn't form.
The cosmic microwave background — called the CMB for short — also provides evidence to back up the Big Bang theory. The CMB is an amazingly uniform microwave glow that's in every direction in the sky. What could have caused a microwave background? Well, as the universe expands, its light is stretched — or redshifted.
The CMB light has been traveling through space since electrons and protons first combined into atoms some 380,000 years after the Big Bang. That light has stretched to microwave wavelengths by now. The CMB shows that a long time ago, the universe must have been smaller and denser than it is now.