The CMB is the closest we can see to the Big Bang. |
Below you can see the latest "image" of the CMB in all its glory, courtesy of the PLANK satellite.
This oval is a map of the entire universe, at the very edge of what we can possibly see. |
What you're actually looking at is a thermal image of the entirety of the universe, from Earth. So, in reality, it should be the inside of a sphere, but that doesn't make a good image, so it's been spread out and made 2-dimensional, like a map. On this map instead of seeing the difference between hills and valleys, we see a change in temperature expressed by colour changes. These temperature fluctuations are tiny, micro-Kelvin differences in temperature which probably seem like nothing but are kinda important in the long run. It's a rather pretty image to look at, in my opinion, maybe I'm weird.
What it shows us though is what the universe looked like the moment that light could begin to
The nature of the CMB made Nebulae like this possible, and eventually galaxys and stars. |
The reason that it's a "microwave background" is - as mentioned - because of the red-shift principle, which is an extension of the Doppler Effect where waves are altered by the speed between emitter and receiver. Waves are pushed together if the emitted is coming towards you, stretched out if it is going away from you.
Light in the universe appears redder than usual because the universe is expanding in all directions away from us, so the surface which the CMB light was emitted from is also traveling away from us. This means that the wavelength of this light gets longer. Red light has a longer wavelength than blue light, hence "red-shift". You can experience this effect in day-to-day life when a train goes past you, the noise you hear sounds different as it travels away from you. And if that shift is big enough the light will go beyond red, into infrared, if the shift is even bigger (like that of 13 billion years of universe expansion) then it will go into the microwave section of the spectrum of light.
Ever noticed an Ambulance sounds different when it's coming towards you, than when it's going away? That's the Doppler Effect. |
So now you know more about the start of the universe, you can go impress everyone you know but showing them pretty pictures and telling them what it actually means. If you enjoyed the article share it with your friends, if you want more information on the CMB do feel free to comment below, and if there are any other areas of science (physics, chemistry, biology, whatever) you can message us on Facebook, contact us on Twitter, or send us an ask on Tumblr.
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