Why can we see light emitted near the beginning of the universe?

In summary: So, if you want to see something that happened before 380,000 years after the Big Bang, you need to look at something that was very, very, very close to the Big Bang itself. And this is where we see objects that are billions of light-years away.
  • #1
xazz
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ok, I can understand that we can see object billion light-year away because it took light a billion year of traveling to come to us.

But where I don't understand is why we can see object at 14 billion light year (or close) away or maybe why can we see light emitted close to the beginning of the universe ?

Because when this light was emitted 14 billion year ago, the what so even form of matter/energy that make us today has to be in the proximity of the source of emission since this time correspond to the beginning of the universe and it shouldn't that big at this moment (compare to today).

Then how come we manage to get where we are today before this light that was emitted 14 billion year ago ?
 
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  • #2
Hi, xazz. Welcome to PF!

xazz said:
Because when this light was emitted 14 billion year ago, the what so even form of matter/energy that make us today has to be in the proximity of the source of emission since this time correspond to the beginning of the universe and it shouldn't that big at this moment (compare to today).
Everything should become clear when you realize that the BB was not an explosion from a single point, but it 'happened' everywhere in the universe(possibly infinite in extent now as back then) at once. So when looking at the most distant objects, you're not seeing stuff that was in the same spot as you. It was much closer(expansion, remember?), but still not in one point.

I say the big bag 'happened' using inverted commas, because it's still not exactly what the theory says. It merely states that distances in the universe are expanding, and at one time in the past all of it was much hotter and denser.

No need to feel bad about all this stuff, though. The Big Bang is an unfortunate name, that stuck and keeps on misleading people. The popular science programmes that picture it as an explosion do not help in the slightest. If you stick around, you'll notice that this question in one form or another pops up all the time on the forums.

We even have a humongous sticky thread in the Cosmology section aiming at "getting us all on the same page". You might find some good information in there, or if you do a forum search.
 
  • #3
xazz, you might find the link in my signature helpful in understanding some of this fundamental cosmology.
 
  • #4
The big bang occurred in time, not space.
 
  • #5
Picture a solid ball. Instead of being made up of atoms, it is made up of energy - - all of the particles you can think of, electrons, quarks, gravitons, anti-protons, all of them. The ball's density is so BIG that it is incomprehensible. This ball contains all the energy in the Universe, all the mass, all the matter, everything. The size of the ball in not very important, but its small, very small. It has lots of photons in it, crowded by the other particles, and changing into them, and back. Particle-antiparticle annihilations are making more photons, which then make more particles. A seething mass of everything. We will pretend that this ball isn't "the Universe", but instead is "in" the Universe. You don't need to understand, in order to understand why we can see back to about 380,000 years after the BigBang, what the difference is between the Universe as a ball, and the energy of the Universe in a ball embedded in Space-time. OK. So at a specific instant, there are a very, very, very large number of photons in the ball. They are each moving in a random direction; in fact, in all directions. Now, at the very next "instant" the size of the ball "inflates" by 2X. Or by 2,000X or by 2 000 000 000X. Suddenly, the photons are not shoulder to shoulder with the other particles, but might take a femtosecond to travel far enough to collide with something. But what happens if the inflation continues in the subsequent instants? Each instant, the distance between particles increases by a HUGE factor. Let's pick out a photon and call it "Bob". Bob was not right next to you, but wasn't that far away, either. Not only that, but Bob's momentum (direction of travel) was pointed RIGHT AT YOU. Suddenly, there is distance, real distance, between Bob and you. How much distance? Oh, say about 14 billion light-years. So, how long will it take Bob the photon to reach you?
Now, the inflation didn't happen in "an instant", but you get the idea, I hope. Also, before about 380,000 years after the Big Bang, the Universe was so hot, that it was opaque to light; light couldn't travel (almost) at all before that. But 13,800,000,000 years - 380,000 years = 13,800,000,000 years (rounded).
 
  • #6
abitslow said:
Picture a solid ball. Instead of being made up of atoms, it is made up of energy - - all of the particles you can think of, electrons, quarks, gravitons, anti-protons, all of them. The ball's density is so BIG that it is incomprehensible. This ball contains all the energy in the Universe, all the mass, all the matter, everything. The size of the ball in not very important, but its small, very small.

Your explanation to the OP is a good one, but I do find it unfortunate that you use the misleading description in the paragraph above (and speaking of paragraphs, you should learn to limit the size of yours) which gives the impression that the universe was both finite sized and spherical right after the singularity, both of which are wrong (well, the finite MIGHT be right but should not be stated as fact). This propagates misinformation.
 
  • #7
abitslow (curious, it sound like me), If suddenly, not instantaneously but in less than 14 billion years, there is 14 billion light-year between me and Bob, it would means that the universe inflate faster than light speed ?
 
  • #8
xazz said:
abitslow (curious, it sound like me), If suddenly, not instantaneously but in less than 14 billion years, there is 14 billion light-year between me and Bob, it would means that the universe inflate faster than light speed ?

The universe went through a period called "inflation" in which things got farther apart at MUCH faster than the speed of light, and currently the expansion is causing things that are very far away from each other to move away from each other faster than c.

For example, the objects at the edge of our observable universe are receding from us at about 3 times the speed of light.

No speeding tickets are issued, however, because this is the expansion of space, NOT movement in the way you normally think of it.

Google "metric expansion" for more information
 
  • #9
Big bang theory

Many people believe that the big bang may or may not have started the universe but the light stays there if not drawn back in with gravity allowing us to see the aftermath. The remains are very week so it takes very high powered machines to read the uv and other light wave emissions that came about during that time but about the big bang no one really knows 100% if it really happened or if it just was a big explosion it is taught as happening but i personally think that the big bang was a small explosion that caused the area that we preside into be created the space we see now is limited most likely there is more than just empty space past our telescopes so it would be very presumptuous of us to say this and think that everything came from a single small event in comparison to the universe we find new things every day we didn't see yesterday that leads me to believe it did not happen in the big bang we are seeing to day.
 
  • #10
Jonson, it would be advantageous to read up on the big bang theory, as you have some misconceptions about it. First and foremost, the big bang was not an explosion within space. It wasn't an "explosion" at all in the regular use of the word. All we know is that the very early universe was very hot and very dense and expanded from there. Note that this dense state existed EVERYWHERE, not just within a small section of the universe.

See this article for more: http://en.wikipedia.org/wiki/Big_bang
 
  • #11
To add to what Drakkith said, the light remnants are NOT from the early days of the universe (the "explosion" as you incorrectly describe it) but 400,000 years afterwards and it is NOT "uv" it is microwaves. See, there's a hint in the name. It's called the "Cosmic Microwave Background", not the "Cosmic Ultraviolet Background".

Also, personal theories are welcome at a lot of forums, but not this one.

Welcome to the forum, by the way, and please be aware we're not trying to give you a hard time here. The point of this forum is to clear up misconceptions about actual science and that's what we're trying to help you with.
 

FAQ: Why can we see light emitted near the beginning of the universe?

What is the significance of light emitted near the beginning of the universe?

The light emitted near the beginning of the universe, known as the cosmic microwave background (CMB), is significant because it is the oldest light in the universe. It allows us to study the conditions of the early universe and provides evidence for the Big Bang theory.

How far back in time can we see with the CMB?

The CMB is estimated to have been emitted around 380,000 years after the Big Bang. This corresponds to a time when the universe was about 3,000 times smaller than it is today. Therefore, we can see back to about 13.8 billion years ago.

What is the temperature of the CMB?

The CMB has a temperature of around 2.7 Kelvin, or -270.4 degrees Celsius. This is incredibly cold, but it is still detectable by sensitive instruments on Earth.

How does the CMB support the Big Bang theory?

The CMB provides strong evidence for the Big Bang theory because it is a remnant of the incredibly hot and dense early universe. The expansion of the universe has caused this light to stretch and cool, resulting in the current temperature we observe. This is consistent with the predictions of the Big Bang theory.

What can we learn from studying the CMB?

Studying the CMB allows us to learn about the composition, age, and evolution of the universe. It also gives us insights into the formation of galaxies and the large-scale structure of the universe. By analyzing the patterns in the CMB, we can also gain a better understanding of the fundamental laws of physics.

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