Empirical measurement of the expansion of the universe

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Discussion Overview

The discussion centers around the empirical measurement of the expansion of the universe, specifically focusing on the Doppler shift of light from distant galaxies and the potential need for multiple measurements over time to confirm acceleration in expansion. The scope includes theoretical implications, observational techniques, and the limitations of current technology.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants note that the acceleration of expansion was deduced from observations of Ia supernovae rather than from direct time snapshots of the same object.
  • One participant suggests that to empirically measure acceleration, two measurements of the same object over time would be necessary, questioning how much time would be required between those measurements.
  • Another participant estimates that thousands of years might be needed to observe expansion directly from one object, with many measurements required to confirm acceleration.
  • A crude calculation indicates that measuring distance uncertainty could necessitate waiting more than a billion years to see a significant change in Doppler shift.
  • One participant questions whether a 10,000-year wait would yield a detectable difference in Doppler shift compared to waiting a billion years.
  • Another participant proposes that a time frame of about 7-10 million years between snapshots should suffice for a statistically significant result with current technology.
  • It is mentioned that while the technology to conduct such measurements is close, economic and logistical factors may delay the start of such projects for several decades.

Areas of Agreement / Disagreement

Participants express differing views on the feasibility and time required for measuring the expansion of the universe through Doppler shift, with no consensus reached on the specific time frames or methodologies discussed.

Contextual Notes

Limitations include uncertainties in distance measurements and the dependence on technological capabilities, which may affect the ability to detect changes in Doppler shift over time.

BernieM
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Doppler shift of light shows distant galaxies moving away from us at high speed. This of course has been taken to prove that the universe itself is expanding and it has been theorized that the expansion is accelerating.

To actually empirically measure and prove the theorized acceleration, one would need to take at least 2 snapshots of the same object at two different times and compare the speed of the object to know what the actual acceleration rate is. (Why do i get a sneaking suspicion that this statement will become one of debate? :smile:)

Using the best and most sensitive (i.e., 1 part per million, per billion, trillion, etc ...) technologies currently available today, how much time is required between two snapshots of the object is required to actually be able to detect enough difference in doppler shift between the two snapshots to empirically measure the acceleration of the object?
 
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The acceleration of expansion was deduced from observations of Ia supernovae at different distances (therefore different ages), not from different time snapshots as you describe.
 
I was asking if you DID want to take two measurements of the same galaxy or supernova or whatever object in the universe at two different times to 'prove beyond a shadow of a doubt' the relative increase in speed of the object, how much time would be required between measurements given our current technology to measure doppler shift.
 
BernieM said:
I was asking if you DID want to take two measurements of the same galaxy or supernova or whatever object in the universe at two different times to 'prove beyond a shadow of a doubt' the relative increase in speed of the object, how much time would be required between measurements given our current technology to measure doppler shift.
I won't try to calculate an answer, but my guess it could take thousands (??) of years just to see expansion from one object by direct measurement (as opposed to Doppler shift). For acceleration, many thousands - also you would need several measurements to observe acceleration.
 
Very crude guess/calculation: The hardest part is measuring the distance. That is why the uncertainty in the Hubble constant is on the order of ten percent. Thus if a "direct" measure requires looking at a single object after its distance has changed by more than ten percent, it would require more than ten percent of the age of the universe, or more than a billion years.

Jim Graber
 
The calculation of the distance to an object may vary by 10 percent, but wouldn't the doppler shift for that same object taken over many measurements in a short period be exactly the same? So if I waited say 10,000 years, would I be able to notice any detectable and measurable shift in the doppler shift in comparison from my original measurements? Or would I need to wait a billion years to see any detectable difference in doppler shift from my original measurements of the same object?
 
For a statistically significant result - about 7-10 million years between snapshots should suffice given current technological capabilities.
 
BernieM said:
I was asking if you DID want to take two measurements of the same galaxy or supernova or whatever object in the universe at two different times to 'prove beyond a shadow of a doubt' the relative increase in speed of the object, how much time would be required between measurements given our current technology to measure doppler shift.

We are close to being able to do this, but, for economic and other reasons, such a project won't start for several decades. Once started, the project would take a couple of decades to start to get good results. See

http://arxiv.org/abs/0802.1532
 
I think that answers my question perfectly. Thanks.
 

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