Why Aren't Galaxies Formed After the Big Bang Referred to as Being Further Away?

In summary, the author is confused about how galaxies were formed and why they are not referred to as being more 42-43 billion light years away. Beyond that, we don't have any idea how big the universe is since we will never see most objects beyond our observation horizon because they are moving away from us faster then the speed of light.
  • #1
jwcole04
3
0
I’m joining this forum just to see if someone can answer this question in a way that I can understand, because it’s driving me nuts.

I read about galaxies observed by the Hubble Space Telescope that were formed “shortly” after the Big Bang. For example, the article may say that they are 12 billion light years away (and we are therefore seeing them as they were roughly 1.7 billion years after the Big Bang, assuming the BB happened 13.7 billion years ago).

However, our observable horizon in any direction is 47 billion light years – or 94 billion light years in diameter – due to hyper expansion of space.

Why aren’t these galaxies we can see that were formed roughly 1.7 billion years after the BB referred to as being more like 42-43 billion light years away?

Beyond that, we don’t have any idea how big the universe is since we will never see most objects beyond our observation horizon because they are moving away from us faster then the speed of light. How is it we can even see objects that were formed so soon after the BB?

Obviously, I’m confused.

Thanks to anyone who can help me understand this, or point me to some helpful resources.
 
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  • #2
jwcole04 said:
Why aren’t these galaxies we can see that were formed roughly 1.7 billion years after the BB referred to as being more like 42-43 billion light years away?
Probably because the author of the news doesn't understand cosmology. Every time I see something like that in a Wikipedia article I fix it, but it is like fighting windmills.
jwcole04 said:
How is it we can even see objects that were formed so soon after the BB?
We only see the galaxies within the observable universe. For every universe age, there is a given "distance then" where we see the objects now. For the cosmic microwave background (CMB), this "distance then" is about 42 million light years (and the corresponding "distance now" is about 46 billion light years).

Our distance to matter that emitted the CMB we see today always increased faster than the speed of light. We still see the light because the relative expansion slowed down. Initially the distance between us and the emitted light increased, but after a few billion years the expansion of the universe was slow enough for the light to come closer to us. The Ant on a rubber band is a nice analogy. Initially its distance to the goal increases, but eventually it reaches the end.
 
  • #3
mfb said:
Initially its distance to the goal increases, but eventually it reaches the end.
... assuming that the expansion is linear. :rolleyes:
 
  • #4
Orodruin said:
... assuming that the expansion is linear. :rolleyes:
With the accelerated expansion there are places where the light will never reach us even in the very distant future, but that is not important to understand the past history of the universe.
 
  • #5
To expand slightly on mfb's answer, the light emitted by distant galaxies was emitted, say, 12 billion years ago. The distance of that galaxy from us when the light was emitted was, say, 5 billion light years (that's just a made up number but it's to show that the distance was not 12 billion light years). Subsequent to that the galaxy moved away from us and is now over 40 billion LY away. The emitted light did not reach us in 5 billion years even though it started out 5 billion LY away from us because the space through which it moved was stretching, so it took 12 billion years. Light emitted "now" (I put "now" in quotes because it gets complicated) when that galaxy is 40+ LY away from us will reach us in, say 200 billion years (again, I'm making up numbers but this is the right idea) and the galaxy will be, say, 500 billion LY away from us.

The ant on the rubber band analogy that mfb pointed you to is helpful.
 
  • #6
Light emitted now by anything more than ~16 billion light years away will never reach us, assuming the cosmological constant is indeed constant.
 
  • #7
Just for clarification, the 16Gly figure cited by mfb is roughly the proper ['now'] distance to a galaxy with a current redshift of about z=1.8. Such a galaxy is crossing our cosmological event horizon and no photons emitted from this time forward will ever reach earth. This, however, does not preclude light from galaxies with a current redshift exceeding z=1.8 from reaching earth. For example, we still observe cmb photons which have a current redshift of about z=1090 - which corresponds to a proper distance ~ 45Gly. A galaxy currently at redshift z=11, which is about the maximum observed redshift for any known galaxy corresponds to a proper distance of ~ 32 Gly. So, obviously the universe was expanding more rapidly at high z, which explains why we can still observe stuff like cmb photons and z=11 galaxies. This is why proper distance is a confusing way to discuss cosmological distances. See Expanding Confusion, https://arxiv.org/abs/astro-ph/0310808, by Davis and Lineweaver for further details.
 
  • #8
mfb said:
Probably because the author of the news doesn't understand cosmology. Every time I see something like that in a Wikipedia article I fix it, but it is like fighting windmills.We only see the galaxies within the observable universe. For every universe age, there is a given "distance then" where we see the objects now. For the cosmic microwave background (CMB), this "distance then" is about 42 million light years (and the corresponding "distance now" is about 46 billion light years).

Our distance to matter that emitted the CMB we see today always increased faster than the speed of light. We still see the light because the relative expansion slowed down. Initially the distance between us and the emitted light increased, but after a few billion years the expansion of the universe was slow enough for the light to come closer to us. The Ant on a rubber band is a nice analogy. Initially its distance to the goal increases, but eventually it reaches the end.

Thanks for all your responses.

So I’m not missing anything – the articles are incorrect and these young galaxies are much further away than the 12b to 13b ly’s stated.

I’ve been ruminating on the second question, and here it is – I hope with more clarity.

Start with this:

- the further away an object is from us, the older it is since we are looking back in time.

- our observable horizon is ~ 47b ly’s. Most objects further away from us than that we will never see since they are moving away from us faster than the speed of light. (I know that our observable horizon is expanding and that the light from some “closer” objects beyond the 47b ly’s will eventually be encompassed by our horizon, and eventually make it’s way to us)

- So, we don’t know how big the universe is – it may be infinite.

- A galaxy that is, say, 13b ly’s old is almost as old as the universe itself.

Such a galaxy is most likely well beyond our 47b ly horizon, so my question is – how can we even see it?

As mfb said “With the accelerated expansion there are places where the light will never reach us even in the very distant future”. Surely a galaxy almost as old as the universe is one of these “places”.

This makes my head hurt.
 
  • #9
jwcole04 said:
A galaxy that is, say, 13b ly’s old is almost as old as the universe itself.

Such a galaxy is most likely well beyond our 47b ly horizon, so my question is – how can we even see it?

As mfb said “With the accelerated expansion there are places where the light will never reach us even in the very distant future”. Surely a galaxy almost as old as the universe is one of these “places”.
Milky Way or the Andromeda galaxy could very well be as old as the universe, and yet you'd have no trouble seeing them, nor would they be beyond the observable universe.

What is usually reported, is galaxies which formed early in the history of the universe. As such, these are the youngest, not oldest galaxies. You'll always see those galaxies near the edge of the observable universe, since that's where the early light was emitted.
In terms of 'images' of galaxies that 'exist' at some distance or another, there are no galaxies beyond the observable universe - there were no galaxies back then.
 
  • #10
Bandersnatch said:
Milky Way or the Andromeda galaxy could very well be as old as the universe, and yet you'd have no trouble seeing them, nor would they be beyond the observable universe.

What is usually reported, is galaxies which formed early in the history of the universe. As such, these are the youngest, not oldest galaxies. You'll always see those galaxies near the edge of the observable universe, since that's where the early light was emitted.
In terms of 'images' of galaxies that 'exist' at some distance or another, there are no galaxies beyond the observable universe - there were no galaxies back then.

Yeah, I misspoke - I meant very young galaxies we can see in the distant past.
 
  • #11
Ok, then such a galaxy is not beyond the observable universe.
 
  • #12
jwcole04 said:
- our observable horizon is ~ 47b ly’s. Most objects further away from us than that we will never see since they are moving away from us faster than the speed of light. (I know that our observable horizon is expanding and that the light from some “closer” objects beyond the 47b ly’s will eventually be encompassed by our horizon, and eventually make it’s way to us)
As stated above already, "moving away from us faster than the speed of light" is not where the horizon is. We see things where the distance was always increasing faster than c for every time in the past.
jwcole04 said:
- So, we don’t know how big the universe is – it may be infinite.
Right.
jwcole04 said:
- A galaxy that is, say, 13b ly’s old is almost as old as the universe itself.
Right.
jwcole04 said:
Such a galaxy is most likely well beyond our 47b ly horizon
Why do you think so? Some are inside, some are outside.
 

What is the method used to determine the distance to "young" galaxies?

The most commonly used method is called the cosmic distance ladder, which involves using different types of astronomical objects with known distances to estimate the distance to "young" galaxies.

How far away are "young" galaxies typically located?

"Young" galaxies are typically located billions of light years away from Earth, making them some of the most distant objects in the universe.

Why is it challenging to accurately measure the distance to "young" galaxies?

One of the main challenges is that "young" galaxies are located at such vast distances that their light has been traveling for billions of years before reaching Earth. This means that the light we observe is significantly redshifted, making it difficult to determine their exact distance.

What are some techniques used to overcome these challenges?

Scientists use a variety of techniques, including measuring the redshift of the galaxy's light, using supernovae as standard candles, and looking for specific features in the galaxy's spectrum, to determine the distance to "young" galaxies.

How does accurately measuring the distance to "young" galaxies help us understand the universe?

By accurately measuring the distance to "young" galaxies, scientists can better understand the expansion of the universe, the distribution of matter and dark matter, and the evolution of galaxies over time. This helps us gain a deeper understanding of the origins and structure of the universe.

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