How WMAP satellite surveyed all over observable universe

In summary, the WMAP satellite has surveyed the entire sky at 5 different frequencies and has detected radiation from the Cosmic Microwave Background that permeates the entire observable universe. This radiation has traveled from regions ~45 billion light years away from us, providing insight into the composition and age of the universe. However, it cannot directly detect dark matter and dark energy, which make up a majority of the universe.
  • #1
hitchiker
31
0
BigBangNoise.jpg


what i want to know is how much area of universe (in light years if possible) is surveyed by WMAP .when you say CMB permeates entire universe based on data from these satellites orbiting Earth how much of universe is actually surveyed by WMAP ?

* The analysis of the WMAP image of the sky, indicates that the universe is older than 13.7 billion years (with an accuracy of 1%), it is composed of 73% dark energy, 23% Cold dark matter, and only 4% of atoms. It is currently expanding at a rate of 71 km/s/Mpc (with an accuracy of 5%).Credit: WMAP Science Team, NASA

if you survey around where we are now in this universe you'd see more matter than anything else..so how physicist say all those quoted above

the farthest we seen of universe is with hubbles' Ultra deep field image / how can WMAP satellite detect the temperature of thermal radiation over HUDF with incredible accuracy
 
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  • #2
I think it surveyed the Cosmic Microwave Background Radiation to get that image, which shouldn't be too hard, as we have constant exposure to it.
 
  • #3
hi whoian

CMB is said to permeates all over universe ?Does WMAP surveyed all universe :eek:

also the other facts quoted above 4% thing ?

any idea
 
  • #5
hitchiker said:
hi whoian

CMB is said to permeates all over universe ?Does WMAP surveyed all universe :eek:

also the other facts quoted above 4% thing ?

any idea

The radiation that WMAP detected has propagated through the entire observable universe before reaching us. As time passes we detect radiation that was emitted further away from us initially at the time of recombination when it was emitted.
 
  • #6
hitchiker said:
if you survey around where we are now in this universe you'd see more matter than anything else..so how physicist say all those quoted above
If you "look", you only see matter which interacts with photons. Dark matter and dark energy don't do that, therefore we cannot see them directly.

The CMB observed by WMAP comes from regions (in every direction of space) which are ~45 billion light years away from us now. This is larger than 13.7 billion, as space expanded between these positions and us in the last 13.7 billion years.
 

1. How does the WMAP satellite survey the entire observable universe?

The WMAP (Wilkinson Microwave Anisotropy Probe) satellite uses a scanning strategy called "spin-scan" to survey the entire observable universe. This involves rotating the satellite once per minute while collecting data from different regions of the sky.

2. What kind of data does the WMAP satellite collect?

The WMAP satellite collects data on the cosmic microwave background (CMB), which is the leftover radiation from the Big Bang. This radiation provides important information about the early universe and the formation of galaxies.

3. How does the WMAP satellite measure the CMB?

The WMAP satellite measures the CMB by using a specialized instrument called a radiometer. This instrument detects the faint microwave radiation emitted by the CMB and converts it into electrical signals that can be analyzed by scientists.

4. How long did it take for the WMAP satellite to survey the entire observable universe?

The WMAP satellite was in operation from 2001 to 2010, during which it completed multiple full scans of the entire observable universe. Each scan took about six months to complete, giving a total of over nine years of data collection.

5. What have we learned from the WMAP satellite's survey of the observable universe?

The WMAP satellite's survey of the observable universe has provided valuable insights into the age, composition, and evolution of the universe. It has helped to confirm the Big Bang theory and has also provided evidence for the existence of dark matter and dark energy, which make up the majority of the universe's mass and energy.

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