How Far Back Can We See with Better Optics?

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In summary, the conversation discusses the potential for improved optics to see further back in time and detect galaxies at higher redshifts. The James Webb Space Telescope is anticipated to be able to detect galaxies up to z~15, which is farther than the current visible horizon. However, individual stars are believed to have formed even earlier, around z~20, and may be undetectable even with advanced telescopes due to their distance and low luminosity.
  • #1
wolram
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Here is a galaxy at very high Z, i thought that Z=7 was a limit before re ionization, so how much further back will we see with better optics ?
http://arxiv.org/pdf/1603.00461.pdf
 
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  • #2
Right back to the initial creation of photons.
 
  • #3
Hi Simon, perhaps i should have asked the question in a different way, How far back will we be able to see galaxies Z-11.1 seems a long way to me.
 
  • #4
Maybe back to the formation of the first galaxies and proto-galaxies ... I think the visible horizon is farther away than that in this epoch.
However, you should understand that these redshifts are estimates - there is not enough data to pin them down.
 
  • #5
Thank you for the clarification SB.
 
  • #8
And it is not expected to see earlier galaxies simply because there were no galaxies (to our current knowledge).

Some individual stars formed earlier according to the linked page, but detecting those would need a telescope orders of magnitude better.
 
  • #9
Yes, the first stars are believed to predate the first galaxies by a considerable margin - probably around z~20 - ,but, Individual stars are deemed to be to be optically undetectable at such vast distances. They are already difficult enough to resolve with existing telescopes in even our nearest neighboring galaxies.
 
  • #10
A back of the envelope calculation:
Typical properties (page 7) -> the higher temperatur cancels a redshift factor of ~18, so their spectrum is not that far away from a solar spectrum. The sun has an absolute magnitude of ~5, 1 million times this luminosity (worst case) would give them an apparent magnitude of -10.
Cosmology calc -> z=20 gives a luminous distance of 230 GPc, or a difference of apparent and absolute magnitude of 57. Combining both, we get an apparent brightness of 47mag. With the upper value for their luminosity, this improves to 40mag.
The limiting magnitude for E-ELT (under construction) is around 36mag, still out of reach even with perfect conditions. Well, at least we don't need planet-sized telescopes...
 

Related to How Far Back Can We See with Better Optics?

1. How far back in time can we see?

The farthest back in time that we can see is approximately 13.8 billion years, which is also the estimated age of the universe.

2. How is it possible to see so far back in time?

We are able to see so far back in time because of the speed of light. Light travels at a constant speed and takes time to reach us from distant objects, allowing us to see them as they were in the past.

3. What is the significance of being able to see so far back in time?

Being able to see so far back in time allows us to study the early stages of the universe, including the formation of galaxies, stars, and planets. It also helps us understand the evolution of the universe and its current state.

4. How do scientists determine how far back we can see?

Scientists use various methods, such as measuring the distance of objects using their brightness or using the redshift of light, to estimate how far back we can see in the universe.

5. Will we ever be able to see further back in time?

It is possible that with advancements in technology and telescopes, we may be able to see even further back in time. However, due to the expansion of the universe, there may be a limit to how far back we can see.

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