Why do we still see cosmic background radiation

In summary, the cosmic background radiation is radiation that originated from the big bang. It is present in the universe, except for the smallish amount which has interacted with matter etc at a different temperature. The expansion of space is diluting and red shifting this radiation, thus reducing its measured temperature. The distance from which we receive CMBR photons is increasing and the temperature is still (very slowly) decreasing.
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SanderStols
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In a discussion with a friend I am unable to explain to him why at this moment we still can detect cosmic background radiation. According to his reasoning the radiation that originated from the big bang should have passed us long ago. Where in fact does this radiation that we now detect come from? And where does it go to?
 
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SanderStols said:
Where in fact does this radiation that we now detect come from?
It comes from the surface of last scattering. This is the surface when the universe cooled down to the point where it became transparent.

http://wmap.gsfc.nasa.gov/media/990053/index.html
 
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It happens at a moment called recombination, where the whole universe suddenly became clear. As universe is broad (or may be infinite), lights from a moment need different time to reach Earth as their sources are at different places.
 
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This radiation was and is present in the entire observable universe, except for the smallish amount which has interacted with matter etc at a different temperature.
The expansion of space is diluting and red shifting this radiation, thus reducing its measured temperature.
The distance from which we receive CMBR photons is increasing and the temperature is still (very slowly) decreasing..
 
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The Big Bang did not happen at a point in space. It happened everywhere in the Universe. As CMB radiation from one region of the universe passes by us, new CMB radiation from a new, more distant region arrives.
 
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The CMB photons we observe originated at a distance of 42 million light years from us and required 13.7 billion years to reach us due to expansion. Our distance from the source of CMB photons is completely irrelevant. We will never observe photons that originated earlier than CMB photons, the only thing that matters is the age of the observer relative to the age of the universe. As the universe ages we will observe photons that are equally more ancient. The CMB photons will eventually redshift beyond detectability, but, never because they have outrun us. It is impossible to outrun the age of the universe.
 
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Thank you all for your answers. I think I understand it better now and I will have my friend read your responses. Maybe it will be clearer to him as well.
 
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Singlau said:
It happens at a moment called recombination, where the whole universe suddenly became clear.

Here "suddenly" means approximately 100 thousand years.
 
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Understood, thanks.
 

1. Why is cosmic background radiation still visible?

The cosmic microwave background (CMB) radiation is the leftover thermal radiation from the Big Bang. It is the oldest light in the universe, dating back to about 380,000 years after the Big Bang. As the universe expanded and cooled, the CMB radiation was stretched to longer wavelengths and can now be observed as microwaves.

2. How is cosmic background radiation detected?

Cosmic background radiation is detected using specialized instruments called microwave telescopes. These telescopes are designed to detect and measure the faint microwaves coming from all directions in the sky. The most famous instrument used to detect CMB radiation is the Cosmic Background Explorer (COBE) satellite.

3. What does cosmic background radiation tell us about the universe?

Cosmic background radiation is an important source of evidence for the Big Bang theory. Its uniformity and specific temperature distribution provide strong support for the theory that the universe began with a hot, dense, and expanding state. It also helps us understand the age and composition of the universe.

4. Is cosmic background radiation the same everywhere in the universe?

Yes, cosmic background radiation is nearly isotropic, meaning it has the same temperature and intensity in all directions. However, there are tiny variations in the temperature of the CMB radiation, known as anisotropies. These variations provide valuable insights into the structure and evolution of the universe.

5. Can cosmic background radiation be used for communication or energy purposes?

No, cosmic background radiation is not suitable for communication or energy purposes. It is extremely weak and has a very low frequency, making it difficult to detect and use for practical applications. Additionally, it is constantly present and cannot be turned off or controlled, making it unreliable as a source of energy.

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