I Apparent distance to far galaxies

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Measuring the apparent distance to galaxies emitting light 13 billion years ago reveals they would appear much closer than their actual distance due to the expansion of the universe. The light-cone graph illustrates that galaxies emitting light at different times have varying distances; for instance, a galaxy emitting light 2 billion years ago would be about 1.75 billion light-years away today. The cosmic microwave background (CMB) represents the oldest light we can observe, originating from around 380,000 years after the Big Bang, translating to approximately 44 million light-years. The farthest galaxies emitted light roughly 9 billion years ago, when they were less than 6 billion light-years distant. Understanding these distances is crucial for comprehending the universe's expansion and the evolution of galaxies.
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How far away were galaxies when they emitted the light we now see?
If we had a way to measure the apparent distance to 13billion light year galaxies (parallax or something) what would it be? The light left the source 13 billion years ago, so it would appear much closer.
I can't find an answer and I'm hoping you know.
 
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Hi, gptodd. Welcome to PF.

The proper distance at emission of all the light being received now is shown on the light-cone graph below:
1600812950738.png

Think of it as tracing all the light from all the galaxies which were emitting at different times on the x axis, and which we observe now (at the 13.8 point on the x axis). So e.g. a galaxy which emitted light 2 billion years ago (11.8 Gy after the big bang), and whose light we are just receiving, was approx 1.75 billion light years distant.
The oldest light we can see, from the CMB, would be near the left edge of the x-axis (at the ~380 thousand point, translating to approx. 44 million light-years on the y axis).
Whereas the farthest emitters emitted their light approximately 9 billion years ago, when they were less than 6 Gly distant.
 
Thank you so much!
-gptodd
 
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