Max Distance & Time Til Sky Nearly Black

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Discussion Overview

The discussion revolves around the maximum distance at which objects in the universe can be observed and the timeline for when the night sky may appear nearly black. It encompasses theoretical considerations of cosmic expansion, stellar lifetimes, and the nature of light travel in an expanding universe.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that the maximum observable distance is currently about 46.5 billion light years, with the cosmic microwave background being the furthest point visible.
  • Others argue that the limit of visibility is more about time than distance, as looking further out means looking further back in time, potentially leading to a black sky before the formation of the first stars.
  • One participant notes that the expansion of the universe does not affect the density of stars in our galaxy, suggesting that the sky will not become starless until most local stars burn out.
  • There is a discussion about the implications of the Milky Way merging with the Andromeda galaxy, which could change the star density in the sky.
  • Some participants seek clarification on whether the maximum distance refers to the distance at which light left an object or the current distance of that object, introducing concepts like angular size distance and comoving radial distance.
  • A later reply highlights that many galaxies we see today were receding faster than light when their light began its journey to us, yet that light still reached us.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the maximum observable distance and the timeline for a black sky, with no consensus reached on these points.

Contextual Notes

Participants mention the complexities of cosmological models and the dependence on definitions of distance, as well as the unresolved nature of stellar lifetimes and the timeline for cosmic events.

Who May Find This Useful

Readers interested in cosmology, astrophysics, and the implications of cosmic expansion may find this discussion relevant.

Charlie G
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I was wondering, since the universe is expanding, what is the maximum distance that we will ever be able to see any object?

Also, how long do we have before the sky becomes nearly black?
 
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At the moment 46.5 billion light years*
The 'furthest' object you can see is the cosmic microwave background. This is the point at which light and matter separated in the early universe so you can't see further back than this because there was no light.
So ironically the 'edge of the universe' (if you like) isn't black but white (at least in the microwave band).

The limit isn't so much distance as time - as we look further out, we are looking further back in time.
There is a distance before the first stars formed where you could consider it black in the visible.

*The rate that this is increasing depends on the cosmological model of the day so is a little complicated to work out.
 
Charlie G said:
Also, how long do we have before the sky becomes nearly black?

Our galaxy is not expanding. We are surrounded by stars and they are not thinning out.
For the sky to become starless, we would have to wait until most of the stars in our neighborhood burn out (and the formation of new stars ends)

So your question has nothing to do with expansion.

The way to answer it would be to look up wikipedia facts about stellar lifetimes.

Actually our galaxy is scheduled to merge with the large Andromeda galaxy. That should be pretty exciting. The sun and planets might accidentally be ejected from the main merger bulk by some fluke, some largescale gravitational slingshot effect. If not we might find ourselves surrounded by more stars than before.

I forget how long before the merger happens. Maybe something on the order of a billion years. Definitely something to look forward to.

Anyway, expansion is real enough, but it affects the distances to remote galaxies, not distances like a few thousand lightyears! So the sky will remain beautiful at least until the combined stars of Milky and Andromeda burn themselves out.
 
Charlie G said:
Also, how long do we have before the sky becomes nearly black?
Sorry, I took that to mean - how far out do we have to look for everything to be black.
 
Charlie G said:
...what is the maximum distance that we will ever be able to see any object?...

I'm curious. What distance do you mean? The distance away the object was back THEN when the light left it and started towards us?

Or the distance away the object is NOW on the day when the light gets here and scoots down the telescope?

For hands-on definiteness you should take an example? Like suppose you see a galaxy today that has redshift z = 4. How far away was it when the light left? How far is it now?
To find out, google "wright calculator" and type in 4 and press the button.

the distance then is what Ned Wright calls angular size distance.
the distance now is what he calls comoving radial distance.

Check it out.
http://www.astro.ucla.edu/~wright/CosmoCalc.html
 
mgb_phys said:
Sorry, I took that to mean - how far out do we have to look for everything to be black.

I thought your response was informed and helpful--I wouldn't contradict what you said, just add more information of a different sort. AFAICS everything you said was correct.
 
Thanks for the replies! What I mean by asking how far is the distance that is the maximum that an object can be visible is, how far is the point at which space expands faster than light between us and an object? Making it impossible for the objects light to ever reach us.
 
Charlie G said:
Thanks for the replies! What I mean by asking how far is the distance that is the maximum that an object can be visible is, how far is the point at which space expands faster than light between us and an object? Making it impossible for the objects light to ever reach us.

Have a look at the Lineweaver SciAm article in my signature----where it says "princeton.edu".

There is a fine point here. Most of the galaxies we can see today were receding faster than light (the distance to the galaxy was increasing at a rate greater than c) at the time that the light left them and began its journey to us. And nevertheless the light still got here!
 
Thanks for the help marcus:)
 

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