Assume that on earth we see something 1 billion light years away

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SUMMARY

The discussion centers on calculating the distance between Earth and a celestial object that is observed to be 1 billion light-years away, considering the expansion of the universe. Participants clarify that while the object was 1 billion light-years away when the light was emitted, the current distance is greater due to cosmic expansion. The redshift of the observed light is essential for determining the current distance and understanding how it relates to the object's original position. Tools like Ned Wright's cosmic calculator and Hubble's constant are recommended for accurate calculations.

PREREQUISITES
  • Understanding of redshift and its significance in cosmology
  • Familiarity with Hubble's Law and Hubble's constant
  • Basic knowledge of cosmic expansion and its effects on distance measurements
  • Experience with astronomical calculators, specifically Ned Wright's cosmic calculator
NEXT STEPS
  • Research how to calculate distances using redshift in cosmology
  • Explore the implications of Hubble's Law on cosmic distances
  • Learn about the methods for measuring cosmic expansion
  • Utilize Ned Wright's cosmic calculator for practical applications in distance calculations
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Astronomers, astrophysicists, and students of cosmology who are interested in understanding cosmic distances and the effects of the universe's expansion on observational astronomy.

mathman
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This is probably an elementary exercise, but my head spins trying to think about it. Assume that on Earth we see something 1 billion light years away (i.e. light took 1 billion years to reach us). To simplify, assume no relative proper motion, although the distance will change due to universe expanding. How far apart are the Earth and the source now and how far apart were they when the light was emitted ( 1 billion years ago)?
 
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Assuming no relative motion, the object was and still is 1 billion light-years away. Or am I missing something in your question?
 
mathman said:
This is probably an elementary exercise, but my head spins trying to think about it. Assume that on Earth we see something 1 billion light years away (i.e. light took 1 billion years to reach us). To simplify, assume no relative proper motion, although the distance will change due to universe expanding. How far apart are the Earth and the source now and how far apart were they when the light was emitted ( 1 billion years ago)?
You wouldn't do the calculation like this, though. You'd get a redshift of the observed photon, and then relate this to the distance between the observer and the emitter when the photon was emitted.

Redbelly98 said:
Assuming no relative motion, the object was and still is 1 billion light-years away. Or am I missing something in your question?
He means that the distance is increasing due to the "universe expanding."
 
cristo said:
He means that the distance is increasing due to the "universe expanding."

Got it. I misread the original post to mean we are ignoring the expansion of the universe.

Thanks for clarifying.
 
Does anyone know the answer to my original question?
 
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mathman said:
Does anyone know the answer to my original question?

I answered your question, didn't I? The point is, how would you know that the light had taken a billion years to travel to you? It's not like a 100m race or something like that, where you can measure it; you need to use the redshift.
 
By the redshift distance, is the short answer. See Ned Wrights cosmic calculator for the details.
 
cristo said:
I answered your question, didn't I? The point is, how would you know that the light had taken a billion years to travel to you? It's not like a 100m race or something like that, where you can measure it; you need to use the redshift.


Using the redshift and Hubble's constant I can get the fact the light has traveled one billion years since it was emitted. What I don't know is how far away from the receiver is the source now and what was the source to receiver distance one billion years ago. Basically how does one factor in the universe expansion to calculate these distances?
 

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