I just got the following reply to a question that has been interesting me for some time:
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> ---------- Forwarded message ----------
> Date: Wed, 13 Oct 2004 06:05:13 -0400
> From:
BlameTheEx@aol.com
> To:
curious@astro.cornell.edu
> Subject: Ask an Astronomer question
>
> Question:
>** The universe of the most distant galaxies observed was much smaller,
> but that earlier universe is observable in all directions. That means a
> small universe is stretched over a large field of vision. Presumably
> that means those early galaxies must be visually larger than their
> distance would suggest, but as their light is dissipated over the
> current universe, their magnitude should be as expected.
>
> Is my logic correct here, and do observations back it?
Your logic is correct.* However, I'm not sure that observations are really
good enough to confirm this.* Attempts to measure the expansion of the
universe by measuring the apparent length scale of galaxies have generally
not been very successful because the population of galaxies has evolved
over time.* It's thought that mini-galaxies accreted to form the galaxies
that we see today, so how do we compare the apparent size of galaxies in
the distant past to the apparent size of galaxies in the present when the
two kinds of galaxies are not really the same?* There are other problems,
like the fact that it's not always trivial to estimate the amount of dust
along the line of sight between us and a distant galaxy.* Dust makes the
galaxy dimmer, and can make it appear to be smaller than it actually is.
So while the effect that you describe almost certainly happens (unless our
understanding of the expansion of the universe is seriously out of whack),
I can't point to a particular set of observations as "proof".
Chris Springob
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Ok People. Any ideas as to how to work out how big or bright a distant galaxy actually is, rather than how it appears? We are talking about very large discrepancies here. At minimum I think a galaxy with a red shift of 6 should be about 7 times larger in diameter than distance should make it. This is a chance to finally prove, or disprove, the expanding universe theory conclusively.